tag:blogger.com,1999:blog-41583727077109824642024-03-04T20:17:48.905-08:00Sobre a Constelação Eridanus, o Rio Eridano, o Rio dos Céus EstreladosJanine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comBlogger9125tag:blogger.com,1999:blog-4158372707710982464.post-71591624796962741022013-11-30T07:18:00.002-08:002015-04-08T10:05:32.020-07:00Eridanus, O Rio dos Céus Estrelados<div style="text-align: justify;">
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">Uma estrela pisca me chamando: é Achernar! </span><br />
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ei-la que surge majestosa, iluminando os céus bem ao sul, </span></span><span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">apontando para o Rio Eridano, </span></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">sinuosamente enredilhando-se pelas terras desde os pés do Gigante Caçador </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">até desaguar suas águas através esta maravilha que vem anunciando a chegada do mar!</span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma questão bastante fundamental </span></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">é o fato de que para bem podermos conhecer os céus estrelados mais ao sul, </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">é preciso que estejamos em lugares de céus escuros e transparentes </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">e, preferencialmente, em noites sem-Lua.</span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">No caso do Rio Eridanus, eu somente consigo delineá-lo nos céus estrelados </span></span><span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">quando a noite é escura, bem escura</span></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;"> - pois que as estrelas que compõem a sinuosidade maravilhosa </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">apresentada por esta constelação </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">são luzes não muito iluminadas - </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">com a fantástica exceção da estrela-alpha Eridanii, Achernar!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando Achernar entra em cena no horizonte sudeste, </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">o céu vem apresentando situações muitíssimo interessantes: </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Escorpião apronta-se para deitar-se no horizonte oeste </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e isto significa que o Gigante Órion </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">já tem toda a intenção de apresentar-se no horizonte leste! </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E sabemos que a estrela que marca </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">um dos pés do Gigante Caçador, Rigel, estrela-beta Orionis, </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">acontece exatamente no lugar onde o Rio Eridanus nasce</span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> e é marcado por sua estrela-bela Eridanii, Cursa.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">No entanto, antes mesmo de o Gigante surgir no horizonte leste </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e ainda contando com a presença de Escorpião rastejando pelos céus do oeste,</span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> o Rio Eridanus já se insinua através sua Foz enriquecida pela estrela-alpha Eridanii, Achernar!</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando eu olho o Rio dos Céus Estrelados, Eridanus, realizando seu enredilhado de estrelinhas tímidas através os céus mais ao sul..., eu tento não me esquecer que por detrás daquelas águas estelares existem outras tantas e tantas estrelas agrupadas em aglomerados e também formando um superaglomerado! E também não me esqueço que ainda mais além de luzes visíveis aos olhos nús bem como invisíveis e vistas somente através potentes telescópios..., existe algo que pode se supor como um super-nada, um supervoid, um super vazio, um super vácuo... talvez o maior que se conheça.... se é que existe.</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quer dizer, o Rio dos Céus Estrelados, Eridanus, corre por tempos e por espaços que a mente humana consegue sequer supor.</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">alguma informação sobre a constelação Eridanus,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">o Rio dos Céus Estrelados:</span></div>
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<a href="http://sobreeridanus.blogspot.com.br/2013/11/eridanus-o-rio-eridano-o-texto-completo.html" style="color: #7d171d; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 14px; line-height: 16.7999992370605px; text-align: left; text-decoration: none; text-indent: -15px;">Eridanus, O Rio dos Céus Estrelados</a></div>
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<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="font-size: 14px; line-height: 16.7999992370605px;">Com um abraço estrelado,</span></span></div>
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<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="font-size: 14px; line-height: 16.7999992370605px;">Janine Milward</span></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-4158372707710982464.post-64196159214136266662013-11-30T07:14:00.004-08:002015-04-08T09:21:11.966-07:00Meus (Janine) Comentários sobre o Rio Eridanus<div class="main-outer" style="min-height: 0px; position: relative;">
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<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="line-height: normal; text-align: left; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Da Terra ao Céu ....</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">.....<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="text-decoration: none;">e ao Infinito </a></span></h1>
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Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo<o:p></o:p></div>
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e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;<o:p></o:p></div>
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bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.<o:p></o:p></div>
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<span style="line-height: 14.25pt;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span></div>
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Com um abraço estrelado,</div>
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Janine Milward<o:p></o:p></div>
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<b>Eridanus</b><o:p></o:p></div>
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<a href="https://www.raremaps.com/gallery/detail/31524op/_Eridanus_Stars_Heightened_in_Gold/Bayer.html" style="text-decoration: none;">https://www.raremaps.com/gallery/detail/31524op/_Eridanus_Stars_Heightened_in_Gold/Bayer.html</a></div>
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<strong style="line-height: normal;">Map Maker: </strong><span style="line-height: normal;"></span><a href="https://www.raremaps.com/gallery/browse/creator_id/247" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; line-height: normal; text-decoration: none;">Johann Bayer</a></div>
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<a href="http://www.aradergalleries.com/detail.php?id=3658" style="text-decoration: none;">http://www.aradergalleries.com/detail.php?id=3658</a></div>
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<b style="line-height: 14.25pt;"><i>A selection of hand-colored engravings from Uranometria</i></b></div>
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<span style="line-height: 14.25pt;">Published: Ausburg 1603</span></div>
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<span style="line-height: 14.25pt;">Dimensions: Paper size app 15 1/2 x 12 inches</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">MEUS (Janine) COMENTÁRIOS SOBRE O RIO ERIDANUS</b></span></div>
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<a href="http://carlosnieto.com/empresas/lecturatarot/blog/constelacion-de-eridanus/" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://carlosnieto.com/empresas/lecturatarot/blog/constelacion-de-eridanus/</span></a></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O RIO ERIDANUS NASCE BEM AOS PÉS - estrela-beta Orionis, Rigel -</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> DO GIGANTE CAÇADOR ÓRION.</span></b></div>
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<b style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A estrela-beta Eridanii, Cursa, </span></b></div>
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<b style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">aponta para este lugar de nascimento do Rio dos Céus Estrelados.</span></b></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Houve um tempo quando o final do Rio Eridanus</span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> era marcado pela estrela-teta Eridanii, Acamar.</span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">No entanto, este Rio ganhou mais terras, foi alongado,</span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> até a representante de sua Foz, a estrela-alpha Eridanii, Achernar!</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEied1P3-QazafKyUbsWWeeZU7wjkkFdCfKd1nwI377dS5-yhk_BxToY645ACKJXVxxSBhcZTFBhxHp7h9V2TGrbdeZln95nQg3aLe_z5-ja_sYdX8r0jArMdTFKcXe283XWNW4nhNnSo94n/s1600/Amazonas+4.png" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEied1P3-QazafKyUbsWWeeZU7wjkkFdCfKd1nwI377dS5-yhk_BxToY645ACKJXVxxSBhcZTFBhxHp7h9V2TGrbdeZln95nQg3aLe_z5-ja_sYdX8r0jArMdTFKcXe283XWNW4nhNnSo94n/s1600/Amazonas+4.png</span></a></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Nosso Rio Eridanus brasileiro bem pode ser representado como o Rio Amazonas, </span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">não é mesmo?</span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O alongamento do Rio Eridanus faz muito sentido, </span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">a partir do ponto de vista de que a belíssima Achernar, a Foz do Rio dos Céus Estrelados,</span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> vem anunciar a chegada de Argo Navis, o Navio!</span></span></div>
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<a href="http://carlosnieto.com/empresas/lecturatarot/blog/constelacion-de-eridanus/" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://carlosnieto.com/empresas/lecturatarot/blog/constelacion-de-eridanus/</span></a></div>
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<span style="border: 0px; margin: 0px; padding: 0px; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Constelación Argo Navis, G. Mercator, año, 1.551</span></span></h3>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhxBYC8cRamzkfIBUxcdU0dfhqzIY7g_CdOfH_NMDRWpiDGOY-m7gLnFONjVVqavUyhSg3oDMgcpHzxfUlr8NHrD5pprN_hI_uJTbebcCOAp2rt_Xz9eMAzChxJOUcRuQx2FqDNhiqfkeBE/s1600/stellarium.JPG" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhxBYC8cRamzkfIBUxcdU0dfhqzIY7g_CdOfH_NMDRWpiDGOY-m7gLnFONjVVqavUyhSg3oDMgcpHzxfUlr8NHrD5pprN_hI_uJTbebcCOAp2rt_Xz9eMAzChxJOUcRuQx2FqDNhiqfkeBE/s640/stellarium.JPG" height="426" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Programa Stellarium</span></div>
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<span style="margin-left: 1em; margin-right: 1em;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhK4KKdbLAJBV6d_OyLa2AQ8wP9qH_rEaF-Ct8VOouoaCR1fdFiqal5537LBM-lLteQwWh46WdDJKV-GJEO9IUuDJojFSElNvI1ygIKWOXtCg7d2kf1btBBxAjgjkXc0ZYCT1NSGnss2tBJ/s1600/novo-2.jpgstellariu+2.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhK4KKdbLAJBV6d_OyLa2AQ8wP9qH_rEaF-Ct8VOouoaCR1fdFiqal5537LBM-lLteQwWh46WdDJKV-GJEO9IUuDJojFSElNvI1ygIKWOXtCg7d2kf1btBBxAjgjkXc0ZYCT1NSGnss2tBJ/s640/novo-2.jpgstellariu+2.jpg" height="360" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Programa Stellarium</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 18px;">QUANDO ACHERNAR APONTA NO HORIZONTE SUDESTE</b><span style="line-height: 18px;">, </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18px;">e</span><span style="line-height: 18px;">u gosto de estar jantando (ou tomando meu desjejum!) </span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; line-height: 18px;">- e minha sala-de-refeições é como uma varanda aberta para o Sítio das Estrelas</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; line-height: 18px;"> e para o céu estrelado.</span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela pisca me chamando: é Achernar! </span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ei-la que surge majestosa, iluminando os céus bem ao sul, </span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">apontando para o Rio Eridano, </span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">sinuosamente enredilhando-se pelas terras desde os pés do Gigante Caçador</span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> até desaguar suas águas através esta maravilha que vem anunciando a chegada do mar!</span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É realmente muito agradável termos uma bela visão dos céus bem mais ao sul </span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- apesar de que, confesso, a multidão de pequenas constelações ainda me confunde,</span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> ainda não sei bem delinear muitas delas, deixo-me envolver por um certo tom de caos...,</span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> talvez parecido com o inicial caos que teria advindo aos observadores dos céus, </span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">há alguns poucos séculos, </span></span></div>
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<span style="background-color: white; color: #073763;"><span style="line-height: 18px;"><span style="font-family: Arial, Helvetica, sans-serif;">quando aproveitaram as caravelas arrojadas </span></span><span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px;">e desbravadoras </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">de novos mares nunca dantes navegados</span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> (e também os navios a vapor) para conhecerem as estrelas buscando o sul... </span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Penso que o sul traz um tom de fantasia, de imaginação solta, de paraíso na Terra, algo assim</span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> - e também de desejo e de concretização de ideais e de situações agradáveis, confortantes ao coração. </span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quer dizer, as constelações bem mais ao sul que foram sendo figuradas,</span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> delineadas e nomeadas, </span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">expressam, de alguma forma, estas questões. </span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma questão bastante fundamental </span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">é o fato de que para bem podermos conhecer os céus estrelados mais ao sul, </span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">é preciso que estejamos em lugares de céus escuros e transparentes </span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e, preferencialmente, em noites sem-Lua.</span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(De uma maneira geral, as pessoas se mostram surpresas </span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">quando eu digo que o melhor momento para o observador de estrelas </span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">acontece quando Selene está ausente - nem que seja por algumas horas, </span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em tempos de Lua de Nova a Crescente ou de Lua Minguante a Nova!).</span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">No caso do Rio Eridanus, eu somente consigo delineá-lo nos céus estrelados</span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> quando a noite é escura, bem escura</span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> - pois que as estrelas que compõem a sinuosidade maravilhosa</span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> apresentada por esta constelação </span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">são luzes não muito iluminadas - </span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">com a fantástica exceção da estrela-alpha Eridanii, Achernar!</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando Achernar entra em cena no horizonte sudeste,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> o céu vem apresentando situações muitíssimo interessantes: </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Escorpião apronta-se para deitar-se no horizonte oeste</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> e isto significa que o Gigante Órion </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">já tem toda a intenção de apresentar-se no horizonte leste! </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E sabemos que a estrela que marca </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">um dos pés do Gigante Caçador, Rigel, estrela-beta Orionis, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">acontece exatamente no lugar onde o Rio Eridanus nasce</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> e é marcado por sua estrela-bela Eridanii, Cursa.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">No entanto, antes mesmo de o Gigante surgir no horizonte leste </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e ainda contando com a presença de Escorpião rastejando pelos céus do oeste,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> o Rio Eridanus já se insinua através sua Foz enriquecida pela estrela-alpha Eridanii, Achernar!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Este é um momento de céu estrelado apresentando-se de maneira radiosa! </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Existe a junção entre o Escorpião e o Sagitário</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> nos introduzindo aos caminhos que nos levam ao centro da Galáxia!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Capricórnio e Aquário também apresentam-se de maneira bem interessante </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">quando em noites de céus escuros e transparentes e sem Lua </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">porque sempre vejo uma "fraldinha" sendo delineada pelo Capricórnio </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e fico rindo e sorrindo diante das estrelinhas em zigue-zague </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">que podemos encontrar no Aguadeiro!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É certo que também o Grande Triângulo do Norte encanta nossa visão mais ao norte, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">não é verdade, com as presenças das constelações da Águia, da Lira e do Cisne </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e esta figura triangular acontecendo através suas estrelas-alpha,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> respectivamente Altair, Vega e Deneb.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Muito me encanta o fato de que o Grande Quadrado formado pelo Cavalo Alado Pegasus</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> me faz recordar que se eu olhar diretamente para o sul, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">irei encontrar as duas Nuvens de Magalhães sempre nos induzindo à dúvida:</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> serão nuvens reais passeando pelo céu e tão próximas de nós....</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> ou serão as Nuvens que, na verdade, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">são galáxias atuantes em nosso chamado Grupo Local? </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É uma dúvida muito emocionante, eu penso.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Programa Stellarium</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ainda existem outras questões bem importantes</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> que envolvem a entrada em cena nos céus estrelados do sul </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">da constelação do Rio Eridanus: </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Se você olhar atentamente a carta celeste,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> verá que a pequena constelação Fornax, a Fornalha,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> é quase que inteiramente envolvida </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">por uma das sinuosidades por onde o Rio Eridanus passa. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> E também, olhando um tantinho ao sul,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> você perceberá a presença da constelação Dorado, o Peixe Dourado.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esse lugar no céu - imenso espaço! -, revela Aglomerados e Voids</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> e são conhecidos como Fornax Cluster e Eridanus Cluster e Fornax e Eridanus Void. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> A bem da verdade,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> muitas das vezes o Leitor encontrará a menção da constelação Fornax</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> nomeando Aglomerado e Void </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- nem sempre o nome Eridanus estará sendo mencionado</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> (ou mesmo o nome Dorado, em alguns casos).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Porém, ainda mais importante, a meu ver, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">é o fato de que é possível que exista o maior Void já encontrado</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> exatamente na direção da constelação Eridanus.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tudo isso quer significar que </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">sempre que estivermos observando a constelação do Eridanus , </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em uma de suas curvas de Rio, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">saberemos que além, muito além de nossa visão apenas física, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">existe um mundo imenso, gigantesco, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">um mundo de galáxias aglomeradas e também um mundão de Vazio. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quer dizer, Luz e Vazio existem para ainda além do Rio.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763;">Programa Stellarium</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;"><br /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Achernar busca seu lugar mais alto no céu estrelado do sul </span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">
</span>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">enquanto Canopus, estrela-alpha Carinae, surge no horizonte sudeste</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> anunciando o Argo Navis, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">o Navio flutuando nas águas dos grandes rios ou dos mares </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">que acolhem as águas advindas do Eridanus através sua Foz, a bela Achernar. </span></div>
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Assim, o céu estrelado mais ao sul torna-se um lugar realmente encantador e bem iluminado</div>
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por estas estrelas tão chamativas!</div>
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O Escorpião já desapareceu no horizonte oeste </div>
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- o que significa que o Gigante Órion pode surgir no horizonte leste </div>
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e testemunhando o lugar onde o Rio Eridanus nasce: a seus pés,</div>
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através a bênção de sua belíssima estrela-beta Orionis, Rigel </div>
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(e o termo Rigel quer dizer pé - assim como vemos Regulus nomeando a pata do Leão; </div>
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assim como vemos Rigel Kent, Rigel Centauri, nomeando a estrela-alpha do Centauro </div>
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e sua importância como pertencente ao sistema estelar mais próximo a nós).</div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhPY5BzLQE9mUSQFDIrwyK-xeLebpzlCAtRhxZljrQFE4GKgW4BnyZoBIWbg5wylFOvv5mF8zHKrdvIPBvcDSGZIvXI5hdzXMPNF8L9gFbOVa21dQ94CRyPnVJco9sH-ed2lx5CFLheZ0u1/s1600/stellarium+-+Navio+chegando+sendo+anunciado+por+Canopus+-+Orion+chegando+e+Escorpi%C3%A3o+indo+embora.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhPY5BzLQE9mUSQFDIrwyK-xeLebpzlCAtRhxZljrQFE4GKgW4BnyZoBIWbg5wylFOvv5mF8zHKrdvIPBvcDSGZIvXI5hdzXMPNF8L9gFbOVa21dQ94CRyPnVJco9sH-ed2lx5CFLheZ0u1/s640/stellarium+-+Navio+chegando+sendo+anunciado+por+Canopus+-+Orion+chegando+e+Escorpi%C3%A3o+indo+embora.jpg" height="373" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Programa Stellarium</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18px;">Quando Achernar alcança seu lugar mais alto nos céus estrelados do sul, </span></span></div>
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acontece uma situação muitíssimo interessante: </div>
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visualmente, Canopus, estrela-alpha Carinae, e Achernar, estrela-alpha Eridanii, </div>
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apresentam-se num mesmo nível </div>
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e enfeitam imensamente o céu sulino e cativam nosso olhar.</div>
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<span style="line-height: 18px;"><br /></span></div>
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O Gigante Órion também alcança o zênite e suas três estrelas formadoras de seu Cinturão </div>
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<div style="text-align: justify;">
- Alnilan, Alnitak e Mintak -,</div>
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sorriem para nós como se fossem as Três Marias </div>
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(porque são assim nomeadas popularmente).</div>
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Existem momentos muito importantes no céu: </div>
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um desses momentos é representado pelo Mito de Andromeda e Perseus.</div>
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A bem da verdade, Cepheus e Cassiopeia já saíram de cena</div>
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(e principalmente para mim porque estão tão ao norte que não posso alcançá-los). </div>
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Pegasus também voa alhures, carregando consigo a Princesa Acorrentada. </div>
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No entanto, Perseus permanece e sempre mostrando a cabeça deceoada da Medusa</div>
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bem como os Peixes que nadam nos mares onde Cetus, o Monstro Marinho, a Baleia, nada</div>
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com seu corpanzil feito de estrelas bem delineadas.</div>
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Os mares do norte vão concluindo e dando lugar à terra firme onde o Carneiro, Aries,</div>
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e o Touro pastam. </div>
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<span style="line-height: 18px;"><br /></span></div>
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O outro momento fantástico</div>
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é revelado pela caudalosa fumacinha branca de estrelinhas de algodão</div>
<div style="text-align: justify;">
formando a Via Lactea e iluminando imensamente esta parte do céu,</div>
<div style="text-align: justify;">
desde o norte até o sul!</div>
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<span style="line-height: 18px;"><br /></span></div>
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E, sem dúvida alguma,</div>
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sempre a presença da estrela mais linda e mais cantada, Sirius,</div>
<div style="text-align: justify;">
estrela-alpha Canis Majoris,</div>
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nos faz vibrar o coração.</div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhmquTV2o3R2xOsbTMvmLsHfVTZLckuyfK1He48nQvT0damLpHuUVKdaxhmUh796_eqDbOH7si1k8lXVeaQtEJPUG5JNkSjxJeQK5GPbTWHaWbrR2j5pSc_GK7C3qvk7BTSHMxjOsQ7JeKk/s1600/stellarium+-+Eridanus+alto+e+mostrando+Orion+por+inteiro.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhmquTV2o3R2xOsbTMvmLsHfVTZLckuyfK1He48nQvT0damLpHuUVKdaxhmUh796_eqDbOH7si1k8lXVeaQtEJPUG5JNkSjxJeQK5GPbTWHaWbrR2j5pSc_GK7C3qvk7BTSHMxjOsQ7JeKk/s640/stellarium+-+Eridanus+alto+e+mostrando+Orion+por+inteiro.jpg" height="374" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Programa Stellarium</span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"></span><br /></span></span>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18px;">O tempo passa, a noite vai empurrando suas estrelas sempre do leste para o oeste...,</span></span></div>
<div style="text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18px;">e o Gigante Órion se esconde novamente da visão do animal rastejante, o Escorpião,</span></span></div>
<div style="text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18px;">que começa a surgir no leste.</span></span></div>
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<span style="line-height: 18px;"><br /></span></div>
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<span style="line-height: 18px;"><div style="text-align: justify;">
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O Rio Eridanus também desaparece, deixando as maravilhas dos céus estrelados do sul</div>
<div style="text-align: justify;">
acontecerem através o Navio que mostra por inteiro</div>
<div style="text-align: justify;">
e navegando placidamente, através o Centauro</div>
<div style="text-align: justify;">
sempre guardando consigo nosso Cruzeiro do Sul.</div>
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</span><div style="text-align: justify;">
<div style="text-align: justify;">
<span style="line-height: 18px;"><br /></span></div>
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<span style="line-height: 18px;"><div style="text-align: justify;">
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Os Gêmeos Castor e Pollux, sempre juntos e conversando entre si,</div>
<div style="text-align: justify;">
anseiam pelo momento de se apresentarem do outro lado do mundo...,</div>
<div style="text-align: justify;">
enquanto o Caranguejo ainda se insinua e nos embevece a visão de sua Colmeia de Abelhas,</div>
<div style="text-align: justify;">
berço de estrelinhas-bebês em seu ventre.</div>
<div style="text-align: justify;">
A Hydra é sempre um prazer de ser vista, enredilhando-se espaçosamente</div>
<div style="text-align: justify;">
desde o Caranguejo até quase a Balança</div>
<div style="text-align: justify;">
e carregando consigo o Sextante, a Taça e o belíssimo voo do Corvo.</div>
<div style="text-align: justify;">
O garboso Leão dos céus ruge, sempre sendo</div>
<div style="text-align: justify;">
seguido pela virginal Virgem que esconde mil e um segredos! </div>
</div>
</span><div style="text-align: justify;">
<div style="text-align: justify;">
<span style="line-height: 18px;"><br /></span></div>
</div>
<span style="line-height: 18px;"><div style="text-align: justify;">
<div style="text-align: justify;">
Sempre em tempos de céus escuros, bem escuros e transparentes,</div>
<div style="text-align: justify;">
a visão da Cabeleira de Berenice é algo absolutamente inesquecível!</div>
<div style="text-align: justify;">
E, certamente, Spica, estrela-alpha Virginis, e Arcturus, estrela-alpha Bootes, rivalizam em suas luzes e nos fazem felizes.</div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
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<div style="text-align: justify;">
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763;">Com um abraço estrelado,</span></span></div>
</div>
</div>
<div style="text-align: center;">
<div style="text-align: justify;">
<div style="line-height: 18px; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-4158372707710982464.post-22511705245150347232013-11-30T07:14:00.002-08:002015-04-08T09:24:04.471-07:00Richard H. Allen e seus Comentários sobre o Rio Eridanus<div style="text-align: justify;">
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<span style="background-color: white;"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/home.html" style="color: rgb(204, 0, 0) !important; text-decoration: none;" target="index"><b><span class="larger" style="font-size: 17.9200000762939px;">Star Names<br /><span class="small" style="font-size: 15.2319993972778px;">Their Lore and Meaning </span></span><br />by<br /><span class="larger" style="font-size: 17.9200000762939px;">Richard Hinckley Allen </span></b></a><br />as reprinted<br />in the Dover edition, 1963</span></div>
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<span style="background-color: white;">The text is in the public domain.</span></div>
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<span style="color: #000066; font-family: Palatino Linotype, Palatino, Gentium Plus, serif;"><span style="background-color: white; font-size: 12.8000001907349px;">http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Eridanus*.html</span></span></div>
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<span style="background-color: white;">. . . amnis, quod de coelo exoritur sub solio Jovis</span></div>
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<span style="background-color: white;">Plautus' <i>Trinummus</i> <a class="added_link" href="http://www.thelatinlibrary.com/plautus/trinummus.shtml" style="color: rgb(85, 85, 255) !important; font-size: 7.86080026626587px; font-style: italic; font-weight: bold; text-decoration: none;" target="offsite">[Act IV, Scene II, v. 940]</a>.</span></div>
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<span style="background-color: white;">. . . the starry Stream.</span></div>
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<span style="background-color: white;">For this a remnant of Eridanos,</span></div>
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<span style="background-color: white;">That stream of tears, 'neath the gods' feet is borne.</span></div>
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<span style="background-color: white;">Brown's <i>Aratos</i>.</span></div>
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<span style="background-color: white;">The River Eridanus,</span></h2>
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<span style="background-color: white;">the French <b><span class="French" style="color: rgb(0, 153, 51) !important;">Eridan</span></b>, the Italian <b><span class="source" style="color: rgb(0, 102, 0) !important;">Eridano</span></b>, and the German <b><span class="source" style="color: rgb(0, 102, 0) !important;">Fluss Eridanus</span></b>, is divided into the Northern and the Southern Stream; the former winding from the star Rigel of Orion to the paws of Cetus; the latter extending thence southwards, southeast, and finally southwest below the horizon of New York City, 2° beyond the <i>lucida</i> Achernar, near the junction of <a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Phoenix*.html" style="color: rgb(204, 0, 0) !important; text-decoration: none;">Phoenix</a>, <a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Tucana*.html" style="color: rgb(204, 0, 0) !important; text-decoration: none;">Tucana</a>, <a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Hydrus*.html" style="color: rgb(204, 0, 0) !important; text-decoration: none;">Hydrus</a>, and <a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Horologium*.html" style="color: rgb(204, 0, 0) !important; text-decoration: none;">Horologium</a>. Excepting Achernar, however, it has no star larger than a 3d‑magnitude, although it is the longest constellation in the sky, and Gould catalogues in it 293 naked-eye components.</span></div>
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<span style="background-color: white;">Although the ancients popularly regarded it as of indefinite extent, in classical astronomy the further termination was at the star <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">θ</span> in 40°47′ of south declination; but modern astronomers have carried it to about 60°.</span></div>
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<span style="background-color: white;">With the Greeks it usually was <b><span class="Greek" style="color: rgb(153, 102, 0) !important; font-family: Avdira, 'Titus Cyberbit Basic', serif !important;">ὁ̔ Ποταμός</span></b>, the River, adopted by the Latins as <b><span class="Latin" style="color: rgb(153, 0, 0) !important;">Amnis</span></b>, <b><span class="Latin" style="color: rgb(153, 0, 0) !important;">Flumen</span></b>, <b><span class="Latin" style="color: rgb(153, 0, 0) !important;">Fluvius</span></b>, and specially as <b><span class="Latin" style="color: rgb(153, 0, 0) !important;">Padus</span></b> and <b><span class="Latin" style="color: rgb(153, 0, 0) !important;">Eridanus</span></b>; this last, as <b><span class="Greek" style="color: rgb(153, 102, 0) !important; font-family: Avdira, 'Titus Cyberbit Basic', serif !important;">Ἐριδανός</span></b>, having appeared for it with Aratos and Eratosthenes. Geographically the word is first found in Hesiod's <i>Θεογονία</i> for the Phasis<a class="ref" href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Eridanus*.html#note1" id="ref1" style="color: rgb(255, 0, 0) !important; font-family: Verdana, sans-serif; font-size: 9.27999973297119px; font-weight: bold; padding: 0.2em; text-decoration: none; vertical-align: super;">1</a> in Asia, celebrated in classic history and mythology,</span></div>
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<span style="background-color: white;">That rises deep and stately rowls along</span></div>
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<span style="background-color: white;">into the Euxine Sea near the spot where the Argonauts secured the golden fleece.</span></div>
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<span style="background-color: white;">Other authors identified our Eridanus with the fabled stream flowing into the ocean from northwestern Europe, — a stream that always has been a matter of discussion and speculation (indeed, Strabo <a class="added_link" href="http://penelope.uchicago.edu/Thayer/E/Roman/Texts/Strabo/5A*.html#1.9" style="color: rgb(85, 85, 255) !important; font-size: 12.8000001907349px; font-style: italic; font-weight: bold; text-decoration: none;" target="Strabo_E">[V.1.9] </a>called it "the nowhere existing"), — or with Homer's Ocean Stream flowing around the earth, whence the early titles for these stars, <b><span class="Latin" style="color: rgb(153, 0, 0) !important;">Oceanus</span></b> and the <b>River of Ocean</b>. They also have been associated with the famous little brook under the Acropolis; with the Ligurian Bodencus — the Padus of ancient, and the Po <a href="https://www.blogger.com/null" id="p216"></a></span><span class="noindex pagenum" style="color: rgb(255, 51, 0) !important; font-size: x-small; position: absolute; right: 1.5em; text-align: right; top: auto; width: 70px;"><span style="background-color: white;">p216</span></span><span style="background-color: white;">of modern, Italy <a class="added_link" href="http://penelope.uchicago.edu/Thayer/E/Roman/Texts/Diodorus_Siculus/5B*.html#23.3" style="color: rgb(85, 85, 255) !important; font-size: 12.8000001907349px; font-style: italic; font-weight: bold; text-decoration: none;" target="Diodorus_E">[Diodorus, <span class="small" style="font-size: 10.8800001144409px;">V</span>.23.3]</a>, — famous in all classical times as the largest of that country's rivers, Vergil's <span class="Latin" style="color: rgb(153, 0, 0) !important;">Rex fluviorum</span> <a class="added_link" href="http://www.hs-augsburg.de/~harsch/Chronologia/Lsante01/Vergilius/ver_ge01.html" style="color: rgb(85, 85, 255) !important; font-size: 12.8000001907349px; font-style: italic; font-weight: bold; text-decoration: none;" target="offsite">[<i>Georg.</i> <span class="small" style="font-size: 10.8800001144409px;">I</span>.482]</a>; with the Ebro of Spain <a class="added_link" href="http://penelope.uchicago.edu/Thayer/L/Roman/Texts/Pliny_the_Elder/37*.html#31" style="color: rgb(85, 85, 255) !important; font-size: 12.8000001907349px; font-style: italic; font-weight: bold; text-decoration: none;" target="Pliny">[Pliny, <i>N.H.</i> <span class="small" style="font-size: 10.8800001144409px;">XXXVII</span>.31‑32]</a>; with the Granicus of Alexander the Great; with the Rhenus and the Rhodanus, — our Rhine and Rhone; and with the modern Radaune, flowing into the Vistula at Danzig.</span></div>
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<span style="background-color: white;">Some of these originals of our River, especially the Padus, were seats of the early amber trade, thus recalling the story of the Heliades, whose tears, shed at the death of their brother Phaëthon, turned into amber as they fell into "that stream of tears" on which that unfortunate was hurled by Jove after his disastrous attempt to drive the chariot of the sun. This was a favorite theme with poets, from Ovid, in the <i>Metamorphoses</i><a class="added_link" href="http://www.thelatinlibrary.com/ovid/ovid.met2.shtml" style="color: rgb(85, 85, 255) !important; font-size: 12.8000001907349px; font-style: italic; font-weight: bold; text-decoration: none;" target="offsite">[II.319 ff.]</a>, to Dean Milman, in <i>Samor</i>, and the foundation of the story that the river was transferred to the sky to console Apollo for the loss of his son.</span></div>
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<span style="background-color: white;">But none of these comparatively northern streams suit the stellar position of our Eridanus, for it is a southern constellation, and it would seem that its earthly counterpart ought to be found in a corresponding quarter. In harmony with this, we know that Eratosthenes and the scholiasts on Germanicus and Hyginus said that it represented the Nile, the only noteworthy river that flows from the south to the north, as this is said to do when rising above the horizon. Thus it is <b><span class="Latin" style="color: rgb(153, 0, 0) !important;">Nilus</span></b> in the <i>Alfonsine Tables</i>, the edition of 1521 saying, <span class="Latin" style="color: rgb(153, 0, 0) !important;">Stellatio fluvii id est Eridanus sive Gyon sive Nilus</span>; <b><span class="Latin" style="color: rgb(153, 0, 0) !important;">Gyon</span></b><a class="ref" href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Eridanus*.html#note2" id="ref2" style="color: rgb(255, 0, 0) !important; font-family: Verdana, sans-serif; font-size: 9.27999973297119px; font-weight: bold; padding: 0.2em; text-decoration: none; vertical-align: super;">2</a> coming from the statement in <i>Genesis</i> ii.13:</span></div>
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<span style="background-color: white;">the name of the second river is Gihon: the same is it that compasseth the whole land of Cush;</span></div>
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<span style="background-color: white;">this latter being misunderstood for the Nile country instead of the Asiatic Kush that was unquestionably intended by the sacred writer. La Lande cited <b>Mulda</b>, equivalent to another title for the stellar Eridanus, — <b><span class="Greek" style="color: rgb(153, 102, 0) !important; font-family: Avdira, 'Titus Cyberbit Basic', serif !important;">Μέλας</span></b>, Black, — and so again connected with Egypt, whose native name, Khem, has this same meaning, well describing the color of the fertile deposit that the Nile waters leave on the land. This became the Latin <b><span class="Latin" style="color: rgb(153, 0, 0) !important;">Melo</span></b>, an early name for the Nile <span class="added_link" style="color: rgb(102, 102, 102) !important; font-size: 12.8000001907349px; font-style: italic; font-weight: bold;">[Serv. ad Georg. IV.291]</span>, <a class="added_link" href="http://remacle.org/bloodwolf/erudits/Festus/m.htm" style="color: rgb(85, 85, 255) !important; font-size: 12.8000001907349px; font-style: italic; font-weight: bold; text-decoration: none;" target="offsite">[Paul. ap. Fest.]</a>, as it also was for the constellation.</span></div>
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<span style="background-color: white;">This allusion to the Nile recalls the ancient wide-spread brief that it and the Euphrates were but different portions of the same stream; and Brown, in his monograph <i>The Eridanus</i>, argues that we should identify the Euphrates with the sky figure. He finds his reasons in the fact that both are frequently alluded to, from very early days to the classical age, as The River, <a href="https://www.blogger.com/null" id="p217"></a></span><span class="noindex pagenum" style="color: rgb(255, 51, 0) !important; font-size: x-small; position: absolute; right: 1.5em; text-align: right; top: auto; width: 70px;"><span style="background-color: white;">p217</span></span><span style="background-color: white;">the Euphrates originally being <span class="archaic" style="color: rgb(102, 102, 0) !important;">Pura</span> or <span class="archaic" style="color: rgb(102, 102, 0) !important;">Purat</span>, the Water, as the Nile was, and even now is, <span class="archaic" style="color: rgb(102, 102, 0) !important;">Ioma</span> or <span class="archaic" style="color: rgb(102, 102, 0) !important;">Iauma</span>, the Sea; that they resemble each other as long and winding streams with two great branches; that each is connected with a Paradise — Eden and Heaven; that the adjoining constellations seems to be Euphratean in origin; and that each is in some way associated with the Nile, and each with the overthrow of the sun-god.</span></div>
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<span style="background-color: white;">There is much in the Euphratean records alluding to a stellar stream that may be our Eridanus, — possibly the Milky Way, another sky river; yet it is to the former that the passage translated by Fox Talbot possibly refers:</span></div>
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<span style="background-color: white;">Like the stars of heaven he shall shine; like the River of Night he shall flow;</span></div>
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<span style="background-color: white;">and its title has been derived from the Akkadian <span class="archaic" style="color: rgb(102, 102, 0) !important;">Aria-dan</span>, the Strong River. George Smith thinks that the heavenly Eridanus may have been the Euphratean <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Erib-me‑gali</span></b>.</span></div>
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<span style="background-color: white;">Its hither termination at the star Rigel gave it the title <b>River of Orion</b>, used by Hipparchos, Proclus, and others; and Landseer wrote:</span></div>
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<span style="background-color: white;">the stars now constellated as Erydanus were originally known in different countries by the names of <b>Nile</b>, <b>Nereus</b>, and <b>Ocean</b>, or <b>Neptune</b>.</span></div>
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<span style="background-color: white;">Riccioli cited for it <b>Vardi</b>, and a Moorish title, according to Bayer, was <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Guad</span></b>, — the 1720 edition of the <i>Uranometria</i> has <b>Guagi</b>, — all these from the Arabic <span class="archaic" style="color: rgb(102, 102, 0) !important;">wādī</span>, and reminding us of the <span class="archaic" style="color: rgb(102, 102, 0) !important;">Wādī al Kabīr</span>, the Great River, the Spaniards' <span class="source" style="color: rgb(0, 102, 0) !important;">Guadalquivir</span>; but the common designation among the Arabians was <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Al Nahr</span></b>, the River, transcribed <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Nar</span></b> and <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Nahar</span></b>, — Chilmead's <b>Alvahar</b>; this Semitic word, occasionally written <span class="archaic" style="color: rgb(102, 102, 0) !important;">Nahal</span>, also having been adduced as a derivation of the word <span class="source" style="color: rgb(0, 102, 0) !important;">Nile</span>.</span></div>
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<span style="background-color: white;">Assemani quoted <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Al Kaff Algeria</span></b> from the Borgian globe for stars in the bend of the stream; but Ideler claimed these for Al Kaff al Jidhmah of Cetus.</span></div>
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<span style="background-color: white;">Caesius thought our Eridanus the sky representative of the <b>Jordan</b>, or of the <b>Red Sea</b>, which the Israelites passed over as on dry land.</span></div>
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<span style="background-color: white;">Old illuminated manuscripts added a venerable river-god lying on the surface of the stream, with urn, aquatic plants, and rows of stars; for all of which the <i>Hyginus</i> of 1488 substitutes the figure of a nude woman, with stars lining the lower bank. Bayer's illustration is quite artistic, with reeds and sedge on the margins. The monster Cetus often is depicted with his fore paws, or flippers, in the River.</span></div>
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<span style="background-color: white;"><a href="https://www.blogger.com/null" id="Alpha"></a><span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 16.2719993591309px; font-style: italic;">α</span>, 0.4, white.</span></h3>
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<span style="background-color: white;"><b>Achernar</b> is from <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Al Āḣir al Nahr</span></b>, the End of the River, nearly its present position in the constellation, about 32° from the south pole; but the <a href="https://www.blogger.com/null" id="p218"></a></span><span class="noindex pagenum" style="color: rgb(255, 51, 0) !important; font-size: x-small; position: absolute; right: 1.5em; text-align: right; top: auto; width: 70px;"><span style="background-color: white;">p218</span></span><span style="background-color: white;">title was first given to the star now lettered <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">θ</span>, the farthest in the Stream known by Arabian astronomers. For <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">α</span> Bayer had <b>Acharnar</b> <i>pro</i> <b>Acharnahar</b><i>vel</i> <b>Acharnarim</b>, and <b>Enar</b>; Caesius, <b>Acarnar</b>; Riccioli, <b>Acarnaharim</b> and <b>Acharnaar</b>; Scaliger, <b>Acharnarin</b>; Schickard, <b>Achironnahri</b>; while<b>Achenar</b> and <b>Archarnar</b> are still occasionally used.</span></div>
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<span style="background-color: white;">This star is supposed to be one of Dante's <b><span class="source" style="color: rgb(0, 102, 0) !important;">Tre Fascelle</span></b>, notwithstanding its invisibility from Italy.<a class="ref" href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Eridanus*.html#note:Tre_Fascelle_in_Dante" id="ref:Tre_Fascelle_in_Dante" style="color: rgb(255, 0, 0) !important; font-family: Verdana, sans-serif; font-size: 9.27999973297119px; font-weight: bold; padding: 0.2em; text-decoration: none; vertical-align: super;">a</a></span></div>
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<span style="background-color: white;">Chinese astronomers knew it as <b><span class="Chinese" style="color: rgb(218, 83, 0) !important;">Shwuy Wei</span></b>.</span></div>
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<span style="background-color: white;">Ptolemy did not mention it, although he could have seen it from the latitude of Alexandria, 31°11′, — a fact, among others, which argues that his catalogue was not based upon original observations, but drawn from the now lost catalogue of Hipparchos, compiled at Rhodes, more than 5° further north, from which place Achernar was not visible.</span></div>
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<span style="background-color: white;">It culminates on the 4th of December, due south of Baten Kaitos.</span></div>
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<span style="background-color: white;"><a href="https://www.blogger.com/null" id="Beta"></a><span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 16.2719993591309px; font-style: italic;">β</span>, 2.9, topaz yellow.</span></h3>
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<span style="background-color: white;"><b>Cursa</b>, 3° to the northwest of Rigel in Orion, is the principal star in this constellation, seen from the latitude of New York City.</span></div>
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<span style="background-color: white;">The word is from <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Al Kursiyy al Jauzah</span></b>, the Chair, or Footstool, of the Central One, <i>i.e.</i> Orion, formed by <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">β</span>, <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">λ</span>, and <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">ψ</span> Eridani with <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">τ</span><a class="correction" href="https://www.blogger.com/null" style="color: rgb(255, 0, 0) !important; cursor: crosshair; font-family: Verdana, sans-serif; font-size: 8.47999954223633px; vertical-align: top;">º</a> Orionis, and regarded as the support of his left foot; but in the earlier astronomy of the nomads it was one of <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Al Udḥā al Naʽām</span></b>, the Ostrich's Nest, that some extended to <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">ο<span class="superscript" style="font-size: 8.64000034332275px; vertical-align: top;">1</span></span> and <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">ο<span class="superscript" style="font-size: 8.64000034332275px; vertical-align: top;">2</span></span>.</span></div>
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<span style="background-color: white;">The <i>Century Cyclopedia</i> gives <b>Dhalim</b> as an alternative title, undoubtedly from <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Al Ṭhalīm</span></b>, the Ostrich; but, although used for <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">β</span> by several writers, this better belongs to <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">θ</span>.</span></div>
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<span style="background-color: white;">The Chinese called <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">β</span> <b><span class="Chinese" style="color: rgb(218, 83, 0) !important;">Yuh Tsing</span></b>, the Golden Well.</span></div>
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<span style="background-color: white;"><a href="https://www.blogger.com/null" id="Gamma"></a><span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 16.2719993591309px; font-style: italic;">γ<span class="superscript" style="font-size: 9.76319980621338px; vertical-align: top;">1</span></span>, 3, yellow.</span></h3>
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<span style="background-color: white;"><b>Zaurac</b> and <b>Zaurak</b> are from the Arabic <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Al Nā᾽ir al Zauraḳ</span></b>, the Bright Star of the Boat; but Ideler applied this early designation to the star that now is <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">α</span> of our Phoenix.</span></div>
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<span style="background-color: white;">With <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">δ</span>, <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">ε</span>, <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">η</span>, and others near, it made up the Chinese <b><span class="Chinese" style="color: rgb(218, 83, 0) !important;">Tien Yuen</span></b>, the Heavenly Park.</span></div>
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<span style="background-color: white;"><a href="https://www.blogger.com/null" id="Eta"></a><span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 16.2719993591309px; font-style: italic;">η</span>, 3.7, pale yellow.</span></h3>
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<span style="background-color: white;"><b>Azha</b> is supposed to have been the <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Azḥā</span></b> of Al Sufi, and the equivalent <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Ashiyane</span></b> of the Persians, and was known by Kazwini as <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Al Udḥiyy</span></b>, being <a href="https://www.blogger.com/null" id="p219"></a></span><span class="noindex pagenum" style="color: rgb(255, 51, 0) !important; font-size: x-small; position: absolute; right: 1.5em; text-align: right; top: auto; width: 70px;"><span style="background-color: white;">p219</span></span><span style="background-color: white;">chief among the stars of the Ostrich's Nest, which the word signifies. The other components were <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">ζ</span>, <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">ρ</span>, and <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">σ</span>; but this last, the 17th of Ptolemy, is not now to be identified in the sky, although it may be one of the three stars <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">ρ</span> displaced by proper motion since Ptolemy's time.</span></div>
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<span style="background-color: white;">Near <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">η</span>, towards <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">τ</span>, are some other stars — <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">ε</span> and <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">π</span> Ceti among them — which in early days were included in the Nest, but later were set apart by Al Sufi as <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Al Sadr al Ḳetus</span></b>, the Breast of the Whale.</span></div>
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<span style="background-color: white;"><a href="https://www.blogger.com/null" id="Theta"></a><span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 16.2719993591309px; font-style: italic;">θ</span>, Double, 3 and 5.25.</span></h3>
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<span style="background-color: white;"><b>Achernar</b> was the early name for this at the then recognized end of the stream, Halley saying of it, <span class="Latin" style="color: rgb(153, 0, 0) !important;">ultima fluminis in veteri catalogo</span>, referring to Tycho's work, of which his own was a supplement. Various forms of its title are given <a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Eridanus*.html#Alpha" style="color: rgb(204, 0, 0) !important; text-decoration: none;">under <span class="star" style="color: rgb(51, 102, 255) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">α</span></a>, but <b>Acamar</b>, from the <i>Alfonsine Tables</i>, is peculiar to <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">θ</span>.</span></div>
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<span style="background-color: white;">Ulug Beg called it <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Al Ṭhalīm</span></b>, the Ostrich, but Hyde rendered this the <b>Dam</b>, as if blocking the flow of the stream to the south.</span></div>
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<span style="background-color: white;">Bullialdus, in his edition of Chrysococca's work, had it <b><span class="Greek" style="color: rgb(153, 102, 0) !important; font-family: Avdira, 'Titus Cyberbit Basic', serif !important;">Αὖλαξ</span></b>,<a class="correction" href="https://www.blogger.com/null" style="color: rgb(255, 0, 0) !important; cursor: crosshair; font-family: Verdana, sans-serif; font-size: 8.47999954223633px; vertical-align: top;">º</a> the Furrow, equivalent to the <span class="Latin" style="color: rgb(153, 0, 0) !important;">sulcus</span> used by Vergil to denote the track of a vessel, appropriate enough to a star situated in the Stream of Ocean; and Riccioli distinctly gave <b>Sulcus</b> for it in his <i>Astronomia Reformata</i>.</span></div>
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<span style="background-color: white;">It is the solitary star visible from the latitude of New York City in early winter evenings, low down in the south, on the meridian with Menkar of the Whale; but Baily said that its brilliancy has probably lessened since Ptolemy's time, for the latter designated it by <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">α</span> — <i>i.e.</i> of the 1st magnitude.</span></div>
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<span style="background-color: white;">Between it and Fomalhaut lie many small stars, not mentioned by Ptolemy, that Hyde said were <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Al Zibāl</span></b>; but Al Sufi had already called them<b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Al Ri᾽āl</span></b>, the Little Ostriches.</span></div>
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<span style="background-color: white;"><span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">ι</span>, <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">κ</span>, <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">φ</span>, and <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">χ</span>, of about the 4th magnitude, were another <b><span class="Chinese" style="color: rgb(218, 83, 0) !important;">Tien Yuen</span></b> of the Chinese, different from that marked by <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">γ</span>; <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">ι</span> and <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">κ</span> are the lowest in the constellation visible from the latitude of New York.</span></div>
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<span style="background-color: white;"><span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">μ</span> and <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">ω</span>, 4th‑magnitude stars lying westward of <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">β</span>, were <b><span class="Chinese" style="color: rgb(218, 83, 0) !important;">Kew Yew</span></b> in China; Reeves including under this title <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">b</span> and the stars of the Sceptre.</span></div>
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<span style="background-color: white;"><a href="https://www.blogger.com/null" id="Omicron1"></a><span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 16.2719993591309px; font-style: italic;">ο<span class="superscript" style="font-size: 9.76319980621338px; vertical-align: top;">1</span></span>, 4.1, clear white.</span></h3>
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<span style="background-color: white;">In early Arabia this was <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Al Baīḍ</span></b>, the Egg, from its peculiar white color, as well as from its position near the Ostrich's Nest. Modern lists generally write it <b>Beid</b>.</span></div>
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<span style="background-color: white;"><b>Situla</b>, the Urn, also has been used for it, although there is no apparent applicability here, and the title is universally recognized for <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">κ</span> Aquarii.</span></div>
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<span style="background-color: white;"><a href="https://www.blogger.com/null" id="p220"></a></span><span class="noindex pagenum" style="color: rgb(255, 51, 0) !important; font-size: x-small; position: absolute; right: 1.5em; text-align: right; top: auto; width: 70px;"><span style="background-color: white;">p220</span></span><span style="background-color: white;"><a href="https://www.blogger.com/null" id="Omicron2"></a><span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 16.2719993591309px; font-style: italic;">ο<span class="superscript" style="font-size: 9.76319980621338px; vertical-align: top;">2</span></span>, Triple, 4, 9.1, and 10.8, orange and sky blue,</span></h3>
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<span style="background-color: white;">is the <b>Keid</b> of modern lists, Burritt's <b>Kied</b>, from <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Al Ḳaid</span></b>, the Egg-shells, thrown out from the nest close by.</span></div>
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<span style="background-color: white;">The Abbé Hell used it in the construction of his constellation Psalterium.</span></div>
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<span style="background-color: white;">Its duplicity was discovered by Sir William Herschel in 1783, and in 1851 Otto Struve found the smaller star itself double and a binary of short period. The system is remarkable from its great proper motion of 4ʺ.1 annually. The two larger stars are 83ʺ apart, at a position angle of 108°, and the smaller 4ʺ apart, at an angle of 111°. The parallax by Elkin indicates a distance of twenty light years.</span></div>
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<span style="background-color: white;"><a href="https://www.blogger.com/null" id="Tau"></a><span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 16.2719993591309px; font-style: italic;">τ<span class="superscript" style="font-size: 9.76319980621338px; vertical-align: top;">2</span></span>, 4, yellow.</span></h3>
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<span style="background-color: white;"><b>Angetenar</b> of the <i>Alfonsine Tables</i>, now the common title, the <b>Argentenar</b> of Riccioli and <b>Anchenetenar</b> of Scaliger, is from <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Al Ḥināyat al Nahr</span></b>, the Bend in the River, near which it lies; Ideler transcribing this as <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Al Anchat al Nahar</span></b>. This is one of Bayer's nine stars of the same letter lying just above Fornax; he said of them, <span class="Latin" style="color: rgb(153, 0, 0) !important;">sibi mutuo succedentes novem</span>.</span></div>
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<span style="background-color: white;">See found, in 1897, a 14.9‑magnitude bluish star, about 52ʺ away, at a position angle of 128°.3.</span></div>
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<span style="background-color: white;"><a href="https://www.blogger.com/null" id="Upsilon"></a><span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 16.2719993591309px; font-style: italic;">υ<span class="superscript" style="font-size: 9.76319980621338px; vertical-align: top;">1</span></span>‑<span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 16.2719993591309px; font-style: italic;">υ<span class="superscript" style="font-size: 9.76319980621338px; vertical-align: top;">7</span></span></span></h3>
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<span style="background-color: white;">mark another series of seven stars called in Bayer's text <b>Beemim</b> and <b>Theemim</b>. This last, used by Bode and now in current use, is perhaps the Arabic <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Al Tau᾽amān</span></b> and the Jews' <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Tĕōmīm</span></b>, the Twins, from the pairs <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">υ<span class="superscript" style="font-size: 8.64000034332275px; vertical-align: top;">1</span></span>, <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">υ<span class="superscript" style="font-size: 8.64000034332275px; vertical-align: top;">2</span></span>, and <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">υ<span class="superscript" style="font-size: 8.64000034332275px; vertical-align: top;">3</span></span>, <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">υ<span class="superscript" style="font-size: 8.64000034332275px; vertical-align: top;">4</span></span>. Grotius thought it derived either from the foregoing or from an Arabic term for two medicinal roots; but Ideler's suggestion that it is from the Hebrew <span class="archaic" style="color: rgb(102, 102, 0) !important;">Bamma᾽yim</span>, <span class="source" style="color: rgb(0, 102, 0) !important;">In the Water</span>, would seem more reasonable, although we have but few star-names from Judaea, and he intimated that it might be a distorted form of <span class="archaic" style="color: rgb(102, 102, 0) !important;">Al Ṭhalīm</span>, the Ostrich. The<i>Almagest</i> of 1515 has <b>Beemun</b>; and the <i>Standard Dictionary</i>, <b>The.eʽ.nim</b>.</span></div>
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<span style="background-color: white;">The Author's Notes:</span></h2>
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<span style="background-color: white;"><a class="note" href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Eridanus*.html#ref1" id="note1" style="color: rgb(255, 0, 0) !important; font-family: Verdana, sans-serif; font-size: 9.27999973297119px; font-weight: bold; text-decoration: none; vertical-align: super;">1</a> This is the modern Rion, or Rioni, the Fasch of the Turks; this last title being a general appellation in early Oriental geography for all rivers, perhaps from the Sanskrit <span class="archaic" style="color: rgb(102, 102, 0) !important;">Phas</span>, Water, or <span class="archaic" style="color: rgb(102, 102, 0) !important;">Was</span>, still seen in the German <span class="source" style="color: rgb(0, 102, 0) !important;">Wasser</span>.</span></div>
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<span style="background-color: white;">★</span></div>
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<span style="background-color: white;"><a href="https://www.blogger.com/null" id="endnotes" style="font-size: medium; line-height: 24px; text-align: start;"></a><span style="font-size: small; line-height: 24px; text-align: start;"></span></span></div>
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<span style="background-color: white;"><a class="note" href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Eridanus*.html#ref2" id="note2" style="color: rgb(255, 0, 0) !important; font-family: Verdana, sans-serif; font-size: 9.27999973297119px; font-weight: bold; text-decoration: none; vertical-align: super;">2</a> The word <span class="archaic" style="color: rgb(102, 102, 0) !important;">Sihor</span> for the Nile, in our Authorized Version of <a href="http://www.newadvent.org/bible/jer002.htm#18" style="color: rgb(204, 0, 0) !important; text-decoration: none;" target="offsite"><i>Jeremiah</i> ii.18</a>, is <span class="Greek" style="color: rgb(153, 102, 0) !important; font-family: Avdira, 'Titus Cyberbit Basic', serif !important;">Γηων</span> in the <i>Septuagint</i>, Josephus also using it in his <i>Ἰουδαϊκή Ἀρχαιολογία</i>, or <i>Jewish Antiquities</i>, in referring to the Nile as one of the four great branches of the River of Paradise.</span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-4158372707710982464.post-58615923936662367422013-11-30T07:13:00.007-08:002015-04-08T09:41:22.446-07:00 Estrelas, Galáxias, Aglomerado, Void<span style="background-color: white; color: #073763;"><br /></span>
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<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="line-height: normal; text-align: left; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Da Terra ao Céu ....</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">.....<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="text-decoration: none;">e ao Infinito </a></span></h1>
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<a href="http://daterraaoceueaoinfinito.blogspot.com.br/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://daterraaoceueaoinfinito.blogspot.com.br/</span></a></div>
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Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo<o:p></o:p></div>
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e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;<o:p></o:p></div>
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bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.<o:p></o:p></div>
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<span style="line-height: 14.25pt;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span></div>
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Com um abraço estrelado,</div>
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Janine Milward<o:p></o:p></div>
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<b><span style="font-size: large;">Eridanus</span></b><o:p></o:p></div>
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<a href="http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_025.jpg">http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_025.jpg</a></div>
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<img src="https://www.raremaps.com/maps/medium/31524op.jpg" /></div>
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<a href="https://www.raremaps.com/gallery/detail/31524op/_Eridanus_Stars_Heightened_in_Gold/Bayer.html">https://www.raremaps.com/gallery/detail/31524op/_Eridanus_Stars_Heightened_in_Gold/Bayer.html</a><br />
<strong style="line-height: normal;">Map Maker: </strong><span style="line-height: normal;"></span><a href="https://www.raremaps.com/gallery/browse/creator_id/247" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; line-height: normal; text-decoration: none;">Johann Bayer</a><br />
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<a href="http://www.aradergalleries.com/detail.php?id=3658">http://www.aradergalleries.com/detail.php?id=3658</a></div>
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<b style="line-height: 14.25pt;"><i>A selection of hand-colored engravings from Uranometria</i></b></div>
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<span style="line-height: 14.25pt;">Published: Ausburg 1603</span></div>
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<span style="line-height: 14.25pt;">Dimensions: Paper size app 15 1/2 x 12 inches</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.brasilfront.xpg.com.br/wp-content/uploads/rio-amazonas-natureza.jpg" style="background-color: white;">http://www.brasilfront.xpg.com.br/wp-content/uploads/rio-amazonas-natureza.jpg</a></span></div>
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<b><span lang="PT" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Da Terra ao Céu<o:p></o:p></span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="PT"> e ao Infinito</span></b><o:p></o:p></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelações, Estrelas e Objetos Celestes<o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(sob o ponto de vista do Mundo Ocidental)<o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Suas histórias, seus mitos, seus significados e suas sintetizadas descrições<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">Reunião das Informações e Compilação,</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">Tradução para a língua portuguesa (em alguns momentos)</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">bem como Comentários Pessoais:</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><span lang="PT">Janine Milward</span></i><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado. Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(tais como Ascensão Reta e Declinação, em muitos dos casos)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">são época/equinócio 1980<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e devem requerer do Caminhante do Céu<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Mario Jaci Monteiro - Cartas Celestes, as 88 Constelações</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; line-height: 11px;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; line-height: 11px;"> - excerto apresentando ALFABETO GREGO, CONVENÇÕES E USO DA CARTA CELESTE</span><br />
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;"><span lang="EN-US"> </span>ERIDANUS, O RIO ERIDANO</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Posicionamento:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 1h22m / 5h9m Declinação +0<sup>o</sup>.1 / -58<sup>o</sup>.1<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Mito:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação representa o Rio Padus ou onde Phaeton caiu quando degolado por Júpiter por causa de ter botado fogo no mundo ao mal-guiar o carro de seu pai, Phoebus.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Erídano é supostamente uma representação de equivalência celestial de um rio; é o Nilo para os Egípcios, e o Eufrates para os Babilônios.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Acessando<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> <a href="http://www.constellationsofwords.com/Constellations/Eridanus.html">http://www.constellationsofwords.com/Constellations/Eridanus.html</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">você encontrará<span class="apple-converted-space"> </span>Informações bem interessantes<span class="apple-converted-space"> </span>sobre o significado da nomeação Eridanus, suas principais Estrelas e excertos do texto de Richard H. Allen contando a História desta Constelação.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Fronteiras:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Eridanus faz fronteira com Horologium, Caelum, Lepus, Orion, Taurus, Cetus, Fornax, Pheonix e Hydra</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://carlosnieto.com/empresas/lecturatarot/blog/constelacion-de-eridanus/" style="background-color: white;">http://carlosnieto.com/empresas/lecturatarot/blog/constelacion-de-eridanus/</a></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="background-color: white; color: #660000;">Algumas Estrelas </span></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="background-color: white; color: #660000;">e Alguns Objetos Interessantes, </span></b></span></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>em Rio Erídano:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Achernar</b><b>. Alpha Eridani. </b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 01h37,0 - Declinação -57<sup>o</sup> 20<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual 0,60 - Distância 118 anos-luz<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela branca situada na boca do Rio. De Al Ahir al Nahr, o Fim do Rio. A Foz do Rio Erídano.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta é uma estrela tão ao sul que não faz parte da visão dos habitantes em latitudes bem ao norte.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Cursa</b><b> - Beta Eridani</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual 2.8 Distância 80 anos-luz,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Cadeira, vocábulo oriundo da expressão árabew Al Kursiyy Al Jauzah. Esta estrela é o começo do Rio Erídano e encontra-se aos pés do Gigante Órion e sua estrela beta Rigel.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Acamar</b><b> - Teta Eridani - Estrela Dupla</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 02h57,5 - Declinação - 40<sup>o</sup> 23<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual 3,42 e 4,5 - Distância 65 anos-luz<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distância entre estrelas 8”,15<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A Lua. O Branco, nome de origem árabe que foi utilizado pela primeira vez nas Tabuas Alfonsinas. Esta estrela já representou a Foz do Rio antes de a constelação ser estendida até alcançar a verdadeira Foz, Achernar.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É um sistema triplo sendo que o membro mais brilhante é visível a olho nu como uma anã amarela, sendo que suas duas companheiras são muito pálidas, uma das quais é uma anã vermelha e a outra, uma anã branca.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Alnahar </b><b>- Delta Eridani</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Rio, nome de origem árabe.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Angetenar</b><b> - Tau Eridani</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Meandro do Rio, proveniente da expressão árabe Al Hinayat al Nahr.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Azha</b><b> - Eta Eridani</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ninho de Avestruz.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Beid ou Keid</b><b> - Omicron Eridani</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ovo, do árabe Al Bais, o ovo do ninho de avestruz. Nome árabe proveniente da expressão Al Kaid.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Theermin</b><b> - Epsilon Eridani</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os Gêmeos, nome oriundo do árabe Al Tauaman.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Zaurak</b><b> - Gamma Eridani</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Barco, oriundo do árabe Al Nair Al Zaurak, ou seja, a brilhante estrela do barco.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Hubble Observations Confirm that Planets Form from Disks Around Stars</span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;"><img src="http://imgsrc.hubblesite.org/hu/db/images/hs-2006-32-a-web_print.jpg" height="512" width="640" /></span></div>
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<a href="http://hubblesite.org/newscenter/archive/releases/2006/32/image/a/format/web_print/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/2006/32/image/a/format/web_print/</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold;">Credit:</span> <a href="http://www.nasa.gov/">NASA</a>, <a href="http://www.spacetelescope.org/">ESA</a>, and G. Bacon (<a href="http://www.stsci.edu/">STScI</a>)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">This is an artist's concept of a Jupiter-mass planet orbiting the nearby star Epsilon Eridani. Located 10.5 light-years away, it is the closest known exoplanet to our solar system. The planet is in an elliptical orbit that carries it as close to the star as Earth is from the Sun, and as far from the star as Jupiter is from the Sun.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Epsilon Eridandi is a young star, only 800 million years old. It is still surrounded by a disk of dust that extends 20 billion miles from the star. The disk appears as a linear sheet of reflecting dust in this view because it is seen edge-on from the planet's orbit, which is in the same plane as the dust disk.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">LEIA MAIS EM <a href="http://hubblesite.org/newscenter/archive/releases/2006/32/image/a/" style="text-align: justify;">http://hubblesite.org/newscenter/archive/releases/2006/32/image/a/</a></span></div>
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<a href="http://hubblesite.org/newscenter/archive/releases/2006/32/image/b/format/web_print/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/2006/32/image/b/format/web_print/</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Image Type:</strong> Illustration</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold;">Credit:</span> <a href="http://www.nasa.gov/">NASA</a>, <a href="http://www.spacetelescope.org/">ESA</a>, and A. Feild (<a href="http://www.stsci.edu/">STScI</a>)</span></div>
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<a href="http://hubblesite.org/newscenter/archive/releases/2006/32/image/b/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/2006/32/image/b/</span></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;"><a href="http://www.spitzer.caltech.edu/images/1966-ssc2008-19a-Epsilon-Eridani-Double-the-Rubble" style="background-color: white;">http://www.spitzer.caltech.edu/images/1966-ssc2008-19a-Epsilon-Eridani-Double-the-Rubble</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">This artist's conception shows the closest known planetary system to our own, called Epsilon Eridani. Observations from NASA's Spitzer Space Telescope show that the system hosts two asteroid belts, in addition to previously identified candidate planets and an outer comet ring.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Epsilon Eridani is located about 10 light-years away in the constellation Eridanus. It is visible in the night skies with the naked eye.</span></div>
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<span style="font-size: xx-small; font-weight: bold; line-height: 20px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Young Solar System in the Making</span></span></div>
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<a href="http://www.spitzer.caltech.edu/images/1962-ssc2008-19b-Young-Solar-System-in-the-Making"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spitzer.caltech.edu/images/1962-ssc2008-19b-Young-Solar-System-in-the-Making</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">This artist's diagram compares the Epsilon Eridani system to our own solar system. The two systems are structured similarly, and both host asteroids (brown), comets (blue) and planets (white dots).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Epsilon Eridani is our closest known planetary system, located about 10 light-years away in the constellation Eridanus. Its central star is a younger, fainter version of our sun, and is about 800 million years oldâabout the same age of our solar system when life first took root on Earth.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Observations from NASA's Spitzer Space Telescope show that the system hosts two asteroid belts, in addition to previously identified candidate planets and an outer comet ring.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Leia mais em <a href="http://www.spitzer.caltech.edu/images/1962-ssc2008-19b-Young-Solar-System-in-the-Making">http://www.spitzer.caltech.edu/images/1962-ssc2008-19b-Young-Solar-System-in-the-Making</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-weight: bold; text-align: -webkit-center;">Johann Bayer — Eridanus</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Eridanus" src="http://www.aradergalleries.com/maps/images/158_Bayer/br_eridanus.jpg" height="462" width="640" /></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiW72QdwaG_ohEmKpXvcN0KkM127kZM1I-7D6VZyv7NcOBGe4rgUnKwnO3xlQJCOIw6Fn_jkMau4wfZKTEUaKRAbIjPVaCFSkx1I_SUVEYSF3-ijWv0ObPimROUGQPJ6GcIZtvegSaTbEbu/s1600/eridanus,+fornax+e+dorado.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiW72QdwaG_ohEmKpXvcN0KkM127kZM1I-7D6VZyv7NcOBGe4rgUnKwnO3xlQJCOIw6Fn_jkMau4wfZKTEUaKRAbIjPVaCFSkx1I_SUVEYSF3-ijWv0ObPimROUGQPJ6GcIZtvegSaTbEbu/s1600/eridanus,+fornax+e+dorado.jpg" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Programa Stellarium</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">VEJA QUE A PEQUENA CONSTELAÇÃO FORNAX, A FORNALHA, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ACONTECE INSERIDA EM UMA DAS TANTAS CURVAS DO RIO ERIDANUS</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e veja que Achernar, estrela-alpha Eridanii, situa-se bem próxima ao Peixe DORADO.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Estas duas constelações vêm sendo sempre muito comentadas porquanto acolhem Aglomerados e Void, Vazio.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Na maioria das vezes, acontece a denominação Fornax Supercluster e Fornax Void porém a verdade é que na direção onde as constelações Eridanus e Fornax se encontram, Aglomerados e Vazios acontecem.</span></div>
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<a href="http://commons.wikimedia.org/wiki/File:2MASS_LSS_chart-NEW_Nasa.jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://commons.wikimedia.org/wiki/File:2MASS_LSS_chart-NEW_Nasa.jpg</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="external text" href="http://spider.ipac.caltech.edu/staff/jarrett/papers/LSS/" rel="nofollow">"Large Scale Structure in the Local Universe: The 2MASS Galaxy Catalog"</a><span style="line-height: 19.1875px;">, Jarrett, T.H. 2004, PASA, 21, 396</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 19.1875px;">Panoramic view of the entire near-infrared sky reveals the distribution of galaxies beyond the </span><a class="extiw" href="http://en.wikipedia.org/wiki/Milky_Way" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="w:Milky Way">Milky Way</a><span style="line-height: 19.1875px;">. The image is derived from the </span><a class="extiw" href="http://en.wikipedia.org/wiki/2MASS" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="w:2MASS">2MASS Extended Source Catalog (XSC)</a><span style="line-height: 19.1875px;">—more than 1.5 million galaxies, and the Point Source Catalog (PSC)--nearly 0.5 billion Milky Way stars</span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">The Fornax and Eridanus clusters are two verThe Fornax and Eridanus clusters are two very famous clusters in the southern hemisphere. Although they look near to each other, they are separated by about 20 million light years. The nearer Fornax cluster is about 65 million light years from us, and the Eridanus cluster is about 85 million light years from us. There are many other groups of galaxies scattered around these two clusters and collectively these groups are often called the <em>Fornax Supercluster</em> or <em>Southern Supercluster</em>.y famous clusters in the southern hemisphere. Although they look near to each other, they are separated by about 20 million light years. The nearer Fornax cluster is abo</span><span style="font-family: Arial, Helvetica, sans-serif;">ut 65 million light years from us, and the Eridanus cluster is about 85 million light years from us. </span></span></div>
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<span style="text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">This is a map of the Eridanus Cluster. This cluster is less spectacular than the Fornax cluster, partly because the galaxies are spread across a larger area and partly because the cluster is rather further and hence dimmer than the Fornax cluster. The Eridanus cluster is roughly split into two halves: a northern subgroup around NGC 1407 and a southern subgroup around NGC 1395.</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763;"><img alt="The Eridanus Cluster" src="http://www.atlasoftheuniverse.com/galgrps/eri.gif" style="text-align: center;" /></span></span></div>
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<tr><th colspan="2" style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Properties of the Eridanus Cluster</span></th></tr>
<tr><td style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Equatorial Coordinates</span></td><td class="center" style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">RA=03h35m Dec=-22°</span></td></tr>
<tr><td style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Galactic Coordinates</span></td><td class="center" style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">l=214° b=-53°</span></td></tr>
<tr><td style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Supergalactic Coordinates</span></td><td class="center" style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">L=281° B=-43°</span></td></tr>
<tr><td style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distance to the centre of the cluster</span></td><td class="center" style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">85 million light years</span></td></tr>
<tr><td style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Number of large galaxies in the cluster</span></td><td class="center" style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">73</span></td></tr>
<tr><td style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Alternative names for the cluster</span></td><td class="center" style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Fornax II cluster</span></td></tr>
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<a href="http://www.atlasoftheuniverse.com/galgrps/for.html" style="text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.atlasoftheuniverse.com/galgrps/for.htm</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;">The center of the </span><b style="line-height: 19.1875px; text-align: start;">Eridanus Cluster</b><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;"> is roughly 23 </span><a href="http://en.wikipedia.org/wiki/Parsec#Megaparsecs_and_gigaparsecs" style="background-image: none; color: #fff2cc; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Parsec">Mpc</a><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;"> (75 </span><a href="http://en.wikipedia.org/wiki/Light-year#Distances_in_light-years" style="background-image: none; color: #fff2cc; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Light-year">Mly</a><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;">) from </span><a href="http://en.wikipedia.org/wiki/Earth" style="background-image: none; color: #fff2cc; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Earth">Earth</a><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;">, and contains about 73 main </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Galaxies" style="background-image: none; color: #fff2cc; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Galaxies">galaxies</a><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;"> and about 200 total galaxies. About 30% have </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Hubble_classification" style="background-image: none; color: #fff2cc; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Hubble classification">Hubble classifications</a><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;"> of elliptical or S0 and the remaining 70% are spiral or irregular.</span><sup class="reference" id="cite_ref-JAA-Omar_2-3" style="color: #fff2cc; line-height: 1em; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-JAA-Omar-2" style="background-image: none; text-decoration: none; white-space: nowrap;">[2]</a></sup><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;"> These galaxies reside in smaller groups which are all loosely gravitationally bound to each other, suggesting that the system is still condensing from the </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Hubble_flow" style="background-image: none; color: #fff2cc; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Hubble flow">Hubble flow</a><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;"> and may eventually form a cluster of about 10</span><sup style="color: #fff2cc; line-height: 1em; text-align: start;">14</sup><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;"> </span><a href="http://en.wikipedia.org/wiki/Solar_mass" style="background-image: none; color: #fff2cc; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Solar mass">M<sub style="line-height: 1em;">☉</sub></a><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;">. A low velocity dispersion compared to that of, for example, the Coma cluster, supports this hypothesis.</span><sup class="reference" id="cite_ref-AJ-Willmer_3-2" style="color: #fff2cc; line-height: 1em; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-AJ-Willmer-3" style="background-image: none; text-decoration: none; white-space: nowrap;">[3]</a></sup><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;"> The Eridanus Cluster is located in the </span><a href="http://en.wikipedia.org/wiki/Constellation" style="background-image: none; color: #fff2cc; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Constellation">constellation</a><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;"> </span><a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)" style="background-image: none; color: #fff2cc; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Eridanus (constellation)">Eridanus</a><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;"> near the </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Fornax_cluster" style="background-image: none; color: #fff2cc; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Fornax cluster">Fornax cluster</a><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;">, and is sometimes called the "Fornax II Cluster".</span><sup class="reference" id="cite_ref-atlasoftheuniverse_4-1" style="color: #fff2cc; line-height: 1em; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-atlasoftheuniverse-4" style="background-image: none; text-decoration: none; white-space: nowrap;">[4]</a></sup></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster" style="background-color: white;">http://en.wikipedia.org/wiki/Eridanus_Cluster</a></span></div>
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<tr><th colspan="2" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Eridanus Cluster</span></th></tr>
<tr><th colspan="2" style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Observation data (<a href="http://en.wikipedia.org/wiki/Epoch_(astronomy)" style="background-image: none; text-decoration: none;" title="Epoch (astronomy)">Epoch</a> <a href="http://en.wikipedia.org/wiki/Epoch_(astronomy)#Julian_years_and_J2000" style="background-image: none; text-decoration: none;" title="Epoch (astronomy)">J2000</a>)</span></th></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Constellation" style="background-image: none; text-decoration: none;" title="Constellation"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constellation(s)</span></a></th><td style="vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)" style="background-image: none; text-decoration: none;" title="Eridanus (constellation)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Eridanus</span></a></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Right_ascension" style="background-image: none; text-decoration: none;" title="Right ascension"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Right ascension</span></a></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03<sup style="line-height: 1em;">h</sup> 28<sup style="line-height: 1em;">m</sup> 13.8<sup style="line-height: 1em;">s</sup><sup class="reference" id="cite_ref-NED-Eridanus_1-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-NED-Eridanus-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Declination" style="background-image: none; text-decoration: none;" title="Declination"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Declination</span></a></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">−20° 44′ 40″<sup class="reference" id="cite_ref-NED-Eridanus_1-1" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-NED-Eridanus-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Brightest member</span></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/NGC_1232" style="background-image: none; text-decoration: none;" title="NGC 1232">NGC 1232</a> (B)</span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Number of galaxies</span></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">~200<sup class="reference" id="cite_ref-JAA-Omar_2-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-JAA-Omar-2" style="background-image: none; text-decoration: none; white-space: nowrap;">[2]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Velocity_dispersion" style="background-image: none; text-decoration: none;" title="Velocity dispersion"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Velocity dispersion</span></a></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">261 km/s<sup class="reference" id="cite_ref-AJ-Willmer_3-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-AJ-Willmer-3" style="background-image: none; text-decoration: none; white-space: nowrap;">[3]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Redshift" style="background-image: none; text-decoration: none;" title="Redshift"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Redshift</span></a></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">0.005570<sup class="reference" id="cite_ref-NED-Eridanus_1-2" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-NED-Eridanus-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distance<br />(<a class="mw-redirect" href="http://en.wikipedia.org/wiki/Co-moving_distance" style="background-image: none; text-decoration: none;" title="Co-moving distance">co-moving</a>)</span></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">23 <a href="http://en.wikipedia.org/wiki/Parsec#Megaparsecs_and_gigaparsecs" style="background-image: none; text-decoration: none;" title="Parsec">Mpc</a> (75 <a href="http://en.wikipedia.org/wiki/Light-year#Distances_in_light-years" style="background-image: none; text-decoration: none;" title="Light-year">Mly</a>)<sup class="reference" id="cite_ref-NED-Eridanus_1-3" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-NED-Eridanus-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Intracluster_medium" style="background-image: none; text-decoration: none;" title="Intracluster medium"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ICM temperature</span></a></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">~10<sup style="line-height: 1em;">7</sup> <a href="http://en.wikipedia.org/wiki/Kelvin" style="background-image: none; text-decoration: none;" title="Kelvin">K</a> (~1 <a class="mw-redirect" href="http://en.wikipedia.org/wiki/KeV" style="background-image: none; text-decoration: none;" title="KeV">keV</a>)<sup class="reference" id="cite_ref-JAA-Omar_2-1" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-JAA-Omar-2" style="background-image: none; text-decoration: none; white-space: nowrap;">[2]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Binding_energy" style="background-image: none; text-decoration: none;" title="Binding energy"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Binding mass</span></a></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">~10<sup style="line-height: 1em;">14</sup> <a href="http://en.wikipedia.org/wiki/Solar_mass" style="background-image: none; text-decoration: none;" title="Solar mass">M<sub style="line-height: 1em;">☉</sub></a><sup class="reference" id="cite_ref-AJ-Willmer_3-1" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-AJ-Willmer-3" style="background-image: none; text-decoration: none; white-space: nowrap;">[3]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Flux" style="background-image: none; text-decoration: none;" title="Flux"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">X-ray flux</span></a></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">0.105 m<a href="http://en.wikipedia.org/wiki/Crab_(unit)" style="background-image: none; text-decoration: none;" title="Crab (unit)">Crab</a><sup class="reference" id="cite_ref-JAA-Omar_2-2" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-JAA-Omar-2" style="background-image: none; text-decoration: none; white-space: nowrap;">[2]</a></sup></span></td></tr>
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<tr><td colspan="2" style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Fornax II Cluster,<sup class="reference" id="cite_ref-atlasoftheuniverse_4-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-atlasoftheuniverse-4" style="background-image: none; text-decoration: none; white-space: nowrap;">[4]</a></sup> de Vaucouleurs Group 31<sup class="reference" id="cite_ref-Chincarini_1974_5-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-Chincarini_1974-5" style="background-image: none; text-decoration: none; white-space: nowrap;">[5</a></sup></span></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span class="mw-headline" id="Table_of_galaxies">Table of galaxies</span><span class="mw-editsection" style="-webkit-user-select: none; display: inline-block; line-height: 1em; margin-left: 1em; padding-right: 0.25em; unicode-bidi: -webkit-isolate; vertical-align: baseline; white-space: nowrap;"><span class="mw-editsection-bracket">[</span><a href="http://en.wikipedia.org/w/index.php?title=Eridanus_Cluster&action=edit&section=1" style="background-image: none; text-decoration: none;" title="Edit section: Table of galaxies">edit</a><span class="mw-editsection-bracket">]</span></span></span></h2>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif; line-height: 1.5em;">Column 1: Name of the</span><span style="font-family: Arial, Helvetica, sans-serif; line-height: 1.5em;"> </span><a href="http://en.wikipedia.org/wiki/Galaxy" style="background-image: none; font-family: Arial, Helvetica, sans-serif; line-height: 1.5em; text-decoration: none;" title="Galaxy">galaxy</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 1.5em;">Column 2:</span><span style="line-height: 1.5em;"> </span><a href="http://en.wikipedia.org/wiki/Right_ascension" style="background-image: none; line-height: 1.5em; text-decoration: none;" title="Right ascension">Right ascension</a><span style="line-height: 1.5em;"> </span><span style="line-height: 1.5em;">for</span><span style="line-height: 1.5em;"> </span><a href="http://en.wikipedia.org/wiki/Epoch_(astronomy)#Julian_years_and_J2000" style="background-image: none; line-height: 1.5em; text-decoration: none;" title="Epoch (astronomy)">epoch J2000</a></span></div>
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"></span><br /></span>
<br />
<div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 1.5em;">Column 3:</span><span style="line-height: 1.5em;"> </span><a href="http://en.wikipedia.org/wiki/Declination" style="background-image: none; line-height: 1.5em; text-decoration: none;" title="Declination">Declination</a><span style="line-height: 1.5em;"> </span><span style="line-height: 1.5em;">for epoch J2000</span></span></div>
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"></span><br /></span>
<br />
<div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 1.5em;">Column 4: Blue</span><span style="line-height: 1.5em;"> </span><a href="http://en.wikipedia.org/wiki/Apparent_magnitude" style="background-image: none; line-height: 1.5em; text-decoration: none;" title="Apparent magnitude">apparent magnitude</a><span style="line-height: 1.5em;"> </span><span style="line-height: 1.5em;">of the galaxy</span></span></div>
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"></span><br /></span>
<br />
<div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 1.5em;">Column 5:</span><span style="line-height: 1.5em;"> </span><a href="http://en.wikipedia.org/wiki/Hubble_sequence" style="background-image: none; line-height: 1.5em; text-decoration: none;" title="Hubble sequence">Galaxy type</a><span style="line-height: 1.5em;">: E=Elliptical; S0=Lenticular; Sa, Sb, Sc, Sd=Spiral; SBa, SBb, SBc, SBd=Barred Spiral; Sm, SBm, Irr=Irregular</span></span></div>
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">
</span>
</span><br />
<div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 1.5em;">Column 6: Angular diameter of the galaxy (</span><a href="http://en.wikipedia.org/wiki/Minute_of_arc" style="background-image: none; line-height: 1.5em; text-decoration: none;" title="Minute of arc">arcminutes</a><span style="line-height: 1.5em;">)</span></span></div>
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">
</span>
</span><br />
<div>
<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; line-height: 1.5em;">Column 7: Diameter of the galaxy (thousands of light years)</span></span></div>
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">
</span>
</span><br />
<div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 1.5em;">Column 8: Recessional velocity (km/s) of the galaxy relative to the</span><span style="line-height: 1.5em;"> </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Cosmic_microwave_background_radiation" style="background-image: none; line-height: 1.5em; text-decoration: none;" title="Cosmic microwave background radiation">cosmic microwave background</a></span></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">
</span>
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"></span><br /></span>
<br />
<div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"></span><br /></span>
<br />
<table class="wikitable sortable jquery-tablesorter" style="border-collapse: collapse; border: 1px solid rgb(170, 170, 170); margin: 1em 60px 1em 0px; text-align: center;"><thead style="line-height: 19.1875px;"></thead><tbody style="line-height: 19.1875px;">
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: left;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Name</span></b></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: left;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Right_Ascension" style="background-image: none; text-decoration: none;" title="Right Ascension">RA</a> <a href="http://en.wikipedia.org/wiki/Equatorial_coordinate_system" style="background-image: none; text-decoration: none;" title="Equatorial coordinate system">equatorial<br />coordinates</a></span></b></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: left;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Declination" style="background-image: none; text-decoration: none;" title="Declination">Dec</a> equatorial<br />coordinates</span></b></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: left;"><b><a href="http://en.wikipedia.org/wiki/Photographic_magnitude" style="background-image: none; text-decoration: none;" title="Photographic magnitude"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Blue<br />Mag</span></a></b></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: left;"><b><a href="http://en.wikipedia.org/wiki/Hubble_sequence" style="background-image: none; text-decoration: none;" title="Hubble sequence"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Type</span></a></b></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Size<br />(arcmin)</span></b></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Size<br />(kly)</span></b></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">RV<br />(km/s)</span></b></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_547-09&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 547-09 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 547-09</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 06.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 23</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">16.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Irr</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1509</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_547-12&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 547-12 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 547-12</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 09.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-17 50</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">16.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Scd</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1837</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://en.wikipedia.org/wiki/NGC_1232" style="background-image: none; text-decoration: none;" title="NGC 1232"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1232</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 09.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-20 35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">10.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">6.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">170</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1517</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=IC_1898&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="IC 1898 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">IC 1898</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 10.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-22 24</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">3.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">85</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1164</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_547-20&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 547-20 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 547-20</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 13.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-17 56</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">16.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBm</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1825</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1258&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1258 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1258</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 14.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 46</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1340</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1297&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1297 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1297</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 19.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 06</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">50</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1395</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://en.wikipedia.org/wiki/NGC_1300" style="background-image: none; text-decoration: none;" title="NGC 1300"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1300</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 19.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 25</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">11.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBbc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">6.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">150</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1421</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1315&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1315 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1315</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 23.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 23</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1534</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=PGC_12680&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="PGC 12680 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">PGC 12680</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 23.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 17</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> ?</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Irr</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1400</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-05&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-05 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-05</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 23.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 45</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBm</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1690</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1325&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1325 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1325</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 24.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 33</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">12.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBbc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">4.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">115</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1446</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1325A&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1325A (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1325A</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 24.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 20</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBcd</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">45</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1188</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-16&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-16 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-16</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 26.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 20</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Scd</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">40</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1977</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1332&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1332 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1332</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 26.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 20</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">11.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">4.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">105</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1383</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-21&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-21 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-21</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 27.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 14</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBd</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">50</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1541</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-25&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-25 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-25</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 29.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-22 09</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBa</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1542</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1345&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1345 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1345</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 29.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-17 47</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1385</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_481-30&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 481-30 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 481-30</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 29.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-23 21</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Scd</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1504</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1347&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1347 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1347</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 29.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-22 17</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1624</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-28&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-28 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-28</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 30.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-17 56</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1360</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-29&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-29 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-29</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 30.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 03</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBbc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1175</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1353&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1353 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1353</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 32.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-20 49</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">12.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBb</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">3.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">85</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1390</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-32&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-32 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-32</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 32.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-17 43</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBm</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">40</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1815</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-33&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-33 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-33</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 32.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18 57</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1552</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-34&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-34 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-34</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 33.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 05</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1610</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_482-05&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 482-05 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 482-05</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 33.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-24 08</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBcd</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">50</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1783</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=IC_1952&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="IC 1952 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">IC 1952</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 33.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-23 43</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBbc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">60</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1683</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=IC_1953&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="IC 1953 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">IC 1953</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 33.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 29</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">12.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">65</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1733</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1359&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1359 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1359</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 33.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 29</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBm</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">55</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1833</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1362&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1362 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1362</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 33.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-20 17</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1085</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-44&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-44 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-44</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 34.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 25</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1561</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-47&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-47 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-47</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 34.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 02</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">60</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1472</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1371&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1371 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1371</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 35.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-24 56</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">11.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBa</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">5.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">140</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1344</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1370&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1370 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1370</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 35.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-20 22</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">933</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=IC_1962&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="IC 1962 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">IC 1962</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 35.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 18</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBd</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">60</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1670</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_482-11&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 482-11 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 482-11</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 36.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-25 36</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sbc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1469</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1377&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1377 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1377</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 36.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-20 54</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">45</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1645</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1385&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1385 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1385</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 37.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-24 30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">11.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">3.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">90</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1373</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1383&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1383 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1383</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 37.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18 20</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">40</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1828</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_482-17&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 482-17 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 482-17</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 37.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-22 55</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sab</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1330</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1390&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1390 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1390</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 37.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 00</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBa</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1078</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1395&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1395 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1395</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 38.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-23 02</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">10.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">5.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">140</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1577</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1398&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1398 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1398</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 38.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-26 20</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">10.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBab</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">7.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">175</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1289</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1403&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1403 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1403</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 39.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-22 23</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1751</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1401&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1401 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1401</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 39.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-22 43</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">50</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1406</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1400&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1400 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1400</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 39.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18 41</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">12.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">60</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">415</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-63&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-63 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-63</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 39.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-20 01</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sbc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1846</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-65&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-65 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-65</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 40.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 22</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sa</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1102</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=IC_343&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="IC 343 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">IC 343</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 40.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18 27</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1730</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1407&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1407 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1407</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 40.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18 35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">10.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">5.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">125</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1650</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-68&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-68 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-68</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 40.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18 56</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1636</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1412&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1412 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1412</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 40.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-26 52</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1675</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-70&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-70 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-70</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 40.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-22 17</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBcd</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">40</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1615</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_482-32&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 482-32 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 482-32</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 40.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-26 47</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Irr</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1621</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1415&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1415 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1415</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 40.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-22 34</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">12.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sa</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">3.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">80</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1451</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1414&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1414 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1414</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 41.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 43</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBbc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">40</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1464</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_482-35&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 482-35 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 482-35</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 41.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-23 50</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBab</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">45</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1756</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1422&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1422 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1422</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 41.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 41</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBab</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">55</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1514</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=IC_346&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="IC 346 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">IC 346</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 41.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18 16</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">45</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1830</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-79&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-79 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-79</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 41.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18 54</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sa</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1914</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-82&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-82 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-82</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 42.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-17 30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sbc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1590</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1426&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1426 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1426</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 42.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-22 06</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">12.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">60</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1296</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_549-02&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 549-02 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 549-02</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 43.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 01</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBm</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">988</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_549-06&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 549-06 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 549-06</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 43.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 14</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Irr</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1490</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1439&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1439 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1439</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 44.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 55</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">12.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">65</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1577</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1440&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1440 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1440</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 45.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18 16</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">12.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">55</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1403</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1438&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1438 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1438</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 45.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-23 00</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBa</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">50</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1438</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1452&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1452 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1452</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 45.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18 38</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">12.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sa</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">60</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1619</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_549-18&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 549-18 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 549-18</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 48.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 28</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">60</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1473</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_482-46&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 482-46 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 482-46</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 49.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-27 00</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">3.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">90</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1422</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_482-49&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 482-49 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 482-49</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 52.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-23 03</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1377</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1482&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1482 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1482</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 54.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-20 30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">55</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1753</span></td></tr>
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<a href="http://en.wikipedia.org/wiki/Eridanus_Cluster"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://en.wikipedia.org/wiki/Eridanus_Cluster</span></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">http://www.whillyard.com. </b></span></div>
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<a href="http://www.whillyard.com/science-pages/clustering.html"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.whillyard.com/science-pages/clustering.html</span></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">Fornax Cluster & </b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">Eridanus Group</b></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><b>The Fornax Cluster</b></span><span style="font-family: Arial, Helvetica, sans-serif;"> is a small cluster of about 58 galaxies, much smaller than the Virgo Cluster, for example, located around 20 Mpc away. It contains two massive galaxies - NGC 1316, a lenticular, and NGC 1365, a barred spiral. Both are more than twice the diameter of the Milky Way. There is substantial evidence that one, or maybe two, sub-groups of galaxies have collided with the main group in the astronomically recent past. </span><span style="font-family: Arial, Helvetica, sans-serif;"><b> Associated with the Fornax Cluster, the Eridanus Group</b></span><span style="font-family: Arial, Helvetica, sans-serif;"> lies about 7 Mpc further away. It contains around 200 galaxies, is approximately 10 Mpc across, and about 23 Mpc away. </span><span style="font-family: Arial, Helvetica, sans-serif;">This grouping is in the early stages of formation, and with the Fornax cluster, the Dorado group and others, forms the <b>Eridanus-Fornax-Dorado Filament</b>.</span><span style="font-family: Arial, Helvetica, sans-serif;"> It is very interesting because although many of its constituent galaxies are quite old, the group itself is rather young and still forming. It also has a large number of lenticular (type S0) galaxies. These are believed to be part of the evolution of spiral galaxies again implying great age for many of the galaxies. </span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.whillyard.com/science-pages/clustering.html" style="background-color: white;">http://www.whillyard.com/science-pages/clustering.html</a></span></div>
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<a href="http://cseligman.com/text/atlas/ngc14.htm#1417"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://cseligman.com/text/atlas/ngc14.htm#1417</span></a></div>
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<a href="http://www.blogger.com/blogger.g?blogID=4158372707710982464" name="1417" style="font-family: Arial, Helvetica, sans-serif;"><big><b><span style="background-color: white; color: #073763;">NGC 1417 (= PGC 13584)</span></b></big></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.blogger.com/blogger.g?blogID=4158372707710982464" name="1417">Discovered (Oct 5, 1785) by </a><a href="http://cseligman.com/text/atlas/discoverers.htm#fwherschel">William Herschel</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763;">A 12th-magnitude spiral galaxy (type SAB(rs)b) in <a href="http://cseligman.com/text/atlas/eridanus.htm#1417">Eridanus</a> (RA 03 41 57.2, Dec -04 42 19)</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apparent size 2.3 by 1.2 arcmin.</span></div>
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<span style="background-color: white; color: #073763;"><img alt="DSS image of spiral galaxy NGC 1417" border="1" src="http://cseligman.com/text/atlas/ngc1417.jpg" height="750" style="font-family: Arial, Helvetica, sans-serif;" title="DSS image of spiral galaxy NGC 1417" width="750" /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Above, a 2.4 arcmin wide closeup of NGC 1417</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Below, a 12 arcmin wide region centered on the galaxy, also showing <a href="http://cseligman.com/text/atlas/ngc14.htm#1418">NGC 1418</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="DSS image of region near spiral galaxy NGC 1417, also showing spiral galaxy NGC 1418" border="1" src="http://cseligman.com/text/atlas/ngc1417wide.jpg" height="750" title="DSS image of region near spiral galaxy NGC 1417, also showing spiral galaxy NGC 1418" width="750" /></span></div>
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.blogger.com/blogger.g?blogID=4158372707710982464" name="1418"></a></span><br /></span>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.blogger.com/blogger.g?blogID=4158372707710982464" name="1418"></a><a href="http://cseligman.com/text/atlas/ngc14.htm#1417">http://cseligman.com/text/atlas/ngc14.htm#1417</a></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.blogger.com/blogger.g?blogID=4158372707710982464" name="1418" style="background-color: white;"><br /></a></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.blogger.com/blogger.g?blogID=4158372707710982464" name="1418" style="background-color: white;"><br /></a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">NGC 1232</b><span style="color: black; line-height: 19.1875px; text-align: start;"> </span><span style="line-height: 19.1875px; text-align: start;">é uma </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a><span style="line-height: 19.1875px; text-align: start;"> localizada a cerca de setenta e dois milhões de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="line-height: 19.1875px; text-align: start;"> (aproximadamente 22,07</span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Megaparsec" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Megaparsec">megaparsecs</a><span style="line-height: 19.1875px; text-align: start;">) de distância na direção da </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o_de_Er%C3%ADdano" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Constelação de Erídano">constelação de Erídano</a><span style="line-height: 19.1875px; text-align: start;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;"> de 9,8, uma declinação de -20º 34' 45" e uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="line-height: 19.1875px; text-align: start;"> de 03 </span><a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Hora">horas</a><span style="line-height: 19.1875px; text-align: start;">, 09 </span><a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Minuto">minutos</a><span style="line-height: 19.1875px; text-align: start;"> e 45,1 </span><a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Segundo">segundos</a><span style="line-height: 19.1875px; text-align: start;">.e tem cerca de 200 mil anos luzes de diâmetro</span></span></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_date" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 143.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Data</span></td><td><time class="dtstart" datetime="2010-10-27"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">27 de outubro de 2010</span></time></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 143.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Origem</span></td><td><a class="external free" href="http://www.eso.org/public/images/eso1042g/" rel="nofollow"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.eso.org/public/images/eso1042g/</span></a></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 143.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Autor</span></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO/P. Grosbøl</span></td></tr>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; font-weight: bold; line-height: normal; text-align: -webkit-left;">NGC 1232: Dwarf Galaxy Caught Ramming Into a Large Spiral</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 13px;">X-ray: NASA/CXC/Huntingdon Inst. for X-ray Astronomy/G.Garmire, Optical: ESO/VLT</span></div>
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<span class="side_menu" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">Tour of NGC 1232</span></div>
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<li style="text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Observations with Chandra have revealed a giant cloud of superheated gas in a galaxy about 60 million light years from Earth.</span></li>
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<li style="text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Because this gas is about 6 million degrees, it only glows in X-ray light.</span></li>
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<li style="text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A collision between a dwarf galaxy and a much larger galaxy called NGC 1232 is the likely cause of this gas cloud.</span></li>
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<li style="text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A new composite of X-rays (purple) from Chandra and optical data (blue and white) shows the scene of the collision.</span></li>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 16px; text-align: -webkit-left;">Observations with NASA's Chandra X-ray Observatory have revealed a massive cloud of multimillion-degree gas in a galaxy about 60 million light years from Earth. The hot gas cloud is likely caused by a collision between a dwarf galaxy and a much larger galaxy called NGC 1232. If confirmed, this discovery would mark the first time such a collision has been detected only in </span><a href="http://chandra.harvard.edu/resources/em_radiation.html" style="line-height: 16px; text-align: -webkit-left; text-decoration: none;">X-rays</a><span style="line-height: 16px; text-align: -webkit-left;">, and could have implications for understanding how galaxies grow through similar collisions.</span></span></div>
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<span style="line-height: 16px; text-align: -webkit-left;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">LEIA MAIS EM </span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://chandra.harvard.edu/photo/2013/ngc1232/index.html" style="background-color: white;">http://chandra.harvard.edu/photo/2013/ngc1232/index.html</a></span></div>
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<h1 class="pr_title" style="border-bottom-color: rgb(0, 91, 160); border-bottom-style: solid; border-bottom-width: 1px; margin: 0px 0px 0.5em; padding: 0.9em 0px 0px;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">A Blue Whirlpool in The River</span></h1>
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<span style="background-color: white; color: #073763;"><img src="http://www.eso.org/public/archives/images/screen/eso1231a.jpg" height="371" width="640" /></span><br />
<a href="http://www.eso.org/public/archives/images/screen/eso1231a.jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.eso.org/public/archives/images/screen/eso1231a.jpg</span></a><br />
<span style="line-height: 16.796875px; text-align: left;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A new image taken with ESO’s Very Large Telescope shows the galaxy NGC 1187. This impressive spiral lies about 60 million light-years away in the constellation of Eridanus (The River). NGC 1187 has hosted two supernova explosions during the last thirty years, the latest one in 2007. This picture of the galaxy is the most detailed ever taken.</span></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.eso.org/public/videos/eso1231a/" style="background-color: white; margin: 0px; padding: 0px; text-decoration: none;"><img alt="Zooming in on the spiral galaxy NGC 1187" src="http://www.eso.org/public/archives/videos/thumb/eso1231a.jpg" style="border: 0px; margin: 0px; padding: 10px;" width="122" /></a></span><br />
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<a href="http://www.eso.org/public/videos/eso1231a/" style="margin: 0px; padding: 0px; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">PR Video eso1231a</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Zooming in on the spiral galaxy NGC 1187</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.eso.org/public/videos/eso1231b/" style="background-color: white; margin: 0px; padding: 0px; text-decoration: none;"><img alt="Panning across a new VLT image of the spiral galaxy NGC 1187" src="http://www.eso.org/public/archives/videos/thumb/eso1231b.jpg" style="border: 0px; margin: 0px; padding: 10px;" width="122" /></a></span><br />
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<a href="http://www.eso.org/public/videos/eso1231b/" style="margin: 0px; padding: 0px; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">PR Video eso1231b</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Panning across a new VLT image of the spiral galaxy NGC 1187</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">LEIA MAIS EM</span></span><br />
<a href="http://www.eso.org/public/news/eso1231/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.eso.org/public/news/eso1231/</span></a><br />
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<a class="ga_static_tracking" href="http://www.eso.org/public/archives/images/screen/eso1231c.jpg" rel="shadowbox" style="margin: 0px; padding: 0px;" title="The spiral galaxy NGC 1187 in the constellation of Eridanus"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="The spiral galaxy NGC 1187 in the constellation of Eridanus" border="0" src="http://www.eso.org/public/archives/images/medium/eso1231c.jpg" height="640" style="border: 0px; margin: 0px; padding: 10px;" width="598" /> </span></a><br />
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<a class="ga_static_tracking" href="http://www.eso.org/public/archives/images/screen/eso1231c.jpg" rel="shadowbox" style="margin: 0px; padding: 0px;" title="The spiral galaxy NGC 1187 in the constellation of Eridanus"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">This chart shows the location of NGC 1187 in the constellation of Eridanus (The River). This map shows most of the stars visible to the unaided eye under good conditions, and NGC 1187 itself is highlighted with a red circle on the image. This galaxy appears as a faint smudge through medium-sized amateur telescopes under good conditions.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO, IAU and Sky & Telescope</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.eso.org/public/images/eso1231c/" style="background-color: white;">http://www.eso.org/public/images/eso1231c/</a></span></div>
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<a href="http://www.raremaps.com/gallery/detail/29167/Orion_and_Haase_Lepus_the_Rabbit/Bode.html"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/detail/29167/Orion_and_Haase_Lepus_the_Rabbit/Bode.html</span></a><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Title: </strong>Orion and Haase (Lepus the Rabbit)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1098" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">Johann Ehlert Bode</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>IC 2118</b> (also known as <b>Witch Head Nebula</b> due to its shape), is an extremely faint <a href="http://en.wikipedia.org/wiki/Reflection_nebula" style="background-image: none; text-decoration: none;" title="Reflection nebula">reflection nebula</a> believed to be an ancient supernova remnant or gas cloud illuminated by nearby <a href="http://en.wikipedia.org/wiki/Supergiant" style="background-image: none; text-decoration: none;" title="Supergiant">supergiant</a> star <a href="http://en.wikipedia.org/wiki/Rigel" style="background-image: none; text-decoration: none;" title="Rigel">Rigel</a> in <a href="http://en.wikipedia.org/wiki/Orion_(constellation)" style="background-image: none; text-decoration: none;" title="Orion (constellation)">Orion</a>. It lies in the <a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)" style="background-image: none; text-decoration: none;" title="Eridanus (constellation)">Eridanus</a>constellation, about 900 <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Light-years" style="background-image: none; text-decoration: none;" title="Light-years">light-years</a> from <a href="http://en.wikipedia.org/wiki/Earth" style="background-image: none; text-decoration: none;" title="Earth">Earth</a>. The nature of the dust particles, reflecting blue light better than red, is a factor in giving the Witch Head its blue color. Radio observations show substantial carbon monoxide emission throughout parts of IC 2118 an indicator of the presence of molecular clouds and star formation in the nebula. In fact candidates for pre-main sequence stars and some classic <a class="mw-redirect" href="http://en.wikipedia.org/wiki/T_Tauri_star" style="background-image: none; text-decoration: none;" title="T Tauri star">T-Tauri stars</a> have been found deep within the nebula.<sup class="reference" id="cite_ref-1" style="color: #fff2cc; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/IC_2118#cite_note-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The molecular clouds of IC 2118 are probably juxtaposed to the outer boundaries of the vast <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Orion-Eridanus_Superbubble" style="background-image: none; text-decoration: none;" title="Orion-Eridanus Superbubble">Orion-Eridanus bubble</a>, a giant supershell of molecular hydrogen blown by the high mass stars of the Orion OB1 association. As the supershell expands into the interstellar medium, favorable circumstances for star formation occur. IC 2118 is located in one such area.The wind blown appearance and cometary shape of the bright reflection nebula is highly suggestive of a strong association with the high mass luminous stars of Orion OB1. The fact that the heads of the cometary clouds of IC2118 point northeast towards the association is strong support of that relationship.</span></div>
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<a href="http://en.wikipedia.org/wiki/IC_2118"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://en.wikipedia.org/wiki/IC_2118</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: normal; text-align: -webkit-center;">The Witch Head Nebula </b><span style="line-height: normal; text-align: -webkit-center;"></span><br style="line-height: normal; text-align: -webkit-center;" /><b style="line-height: normal; text-align: -webkit-center;">Credit: </b><span style="line-height: normal; text-align: -webkit-center;"></span><a href="mailto:Gary.L.Stevens@jpl.nasa.gov" style="line-height: normal; text-align: -webkit-center;">Gary Stevens</a></span></div>
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<a href="http://apod.nasa.gov/apod/ap010227.html"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://apod.nasa.gov/apod/ap010227.html</span></a></div>
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<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Type</span></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Reflection</span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Right_ascension" style="background-image: none; text-decoration: none;" title="Right ascension"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Right ascension</span></a></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">05<sup style="line-height: 1em;">h</sup> 02<sup style="line-height: 1em;">m</sup> 00.00<sup style="line-height: 1em;">s</sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Declination" style="background-image: none; text-decoration: none;" title="Declination"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Declination</span></a></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-07° 54′ 00.0"</span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distance</span></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1,000 <a href="http://en.wikipedia.org/wiki/Light-year" style="background-image: none; text-decoration: none;" title="Light-year">ly</a></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Apparent_magnitude" style="background-image: none; text-decoration: none;" title="Apparent magnitude">Apparent magnitude</a><small>(V)</small></span></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13</span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Angular_diameter" style="background-image: none; text-decoration: none;" title="Angular diameter">Apparent dimensions</a> <small>(V)</small></span></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">3 × 1 <a href="http://en.wikipedia.org/wiki/Degree_(angle)" style="background-image: none; text-decoration: none;" title="Degree (angle)">°</a></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Constellation" style="background-image: none; text-decoration: none;" title="Constellation"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constellation</span></a></th><td style="vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)" style="background-image: none; text-decoration: none;" title="Eridanus (constellation)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Eridanus</span></a></td></tr>
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<span style="font-family: Arial, Helvetica, sans-serif; font-size: small;">Baby Stars Brewing in the Witch Head Nebula</span></span></h2>
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<a href="http://www.spitzer.caltech.edu/images/2288-sig06-013-Baby-Stars-Brewing-in-the-Witch-Head-Nebula"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spitzer.caltech.edu/images/2288-sig06-013-Baby-Stars-Brewing-in-the-Witch-Head-Nebula</span></a><br />
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<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Credit</span></dt>
<dd property="photoshop:Credit" style="margin: 0px; padding: 2px 0px 0px 5px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NASA/JPL-Caltech/L. Rebull (SSC/Caltech)</span></dd>
<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Observers</span></dt>
<dd style="margin: 0px; padding: 2px 0px 0px 5px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">L. Rebull (Spitzer Science Center), T. Spuck (Oil City Area Sr. High School), B. Sepulveda (Lincoln High School), T. Maranto (Phillips Exeter Academy), C. Weehler (Luther Burbank High School), T. Roelofsen (Bassick High School), B. Ehrhart (Oil City Area Sr. High School), D. Bowser II (Oil City Area Sr. High School), M. Greer (Phillips Exeter Academy), J. Preis (Phillips Exeter Academy), P. Weston (Phillips Exeter Academy), A. Hughes (Lincoln High School), N. Sharma (Lincoln High School), J. Herrera (Luther Burbank High School),</span></dd></dl>
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<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Name</span></dt>
<dd style="margin: 0px; padding: 2px 0px 0px 5px; text-align: center;"><span property="dc:subject"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Witch Head Nebula</span></span></dd>
<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Type</span></dt>
<dd property="avm:Subject.Category" style="margin: 0px; padding: 2px 0px 0px 5px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Nebula > Type > Star Formation</span></dd>
<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distance</span></dt>
<dd property="avm:Distance" style="margin: 0px; padding: 2px 0px 0px 5px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">800 Light Years</span></dd></dl>
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<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Position (J2000)</span></dt>
<dd property="avm:Spatial.ReferenceValue" style="margin: 0px; padding: 2px 0px 0px 5px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">RA = 5<sup>h</sup> 7<sup>m</sup> 50.3<sup>s</sup></span></dd><dd property="avm:Spatial.ReferenceValue" style="margin: 0px; padding: 2px 0px 0px 5px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dec = -6° 21' 31.5"</span></dd>
<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Field of View</span></dt>
<dd property="avm:Spatial.ReferenceDimension" style="margin: 0px; padding: 2px 0px 0px 5px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">18.4 x 15.2 arcminutes</span></dd>
<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Orientation</span></dt>
<dd property="avm:Spatial.Rotation" style="margin: 0px; padding: 2px 0px 0px 5px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">North is 1.1° left of vertical</span></dd>
<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constellation</span></dt>
<dd style="margin: 0px; padding: 2px 0px 0px 5px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Eridanus</span></dd></dl>
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<span style="background-color: #073763; line-height: 18px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Eight hundred light-years away in the Orion constellation, a gigantic murky cloud called the "Witch Head Nebula" is teeming with dust-obscured newborn stars waiting to be uncovered. In this image, the super sensitive infrared eyes of NASA's Spitzer Space Telescope reveal 12 new baby stars in a small portion of the cloud commonly referred to as the Witch Head's "pointy chin."</span></span><br />
<a href="http://www.spitzer.caltech.edu/images/2288-sig06-013-Baby-Stars-Brewing-in-the-Witch-Head-Nebula"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spitzer.caltech.edu/images/2288-sig06-013-Baby-Stars-Brewing-in-the-Witch-Head-Nebula</span></a><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1132</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; text-decoration: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_el%C3%ADptica" style="background-image: none; text-decoration: none;" title="Galáxia elíptica">elíptica</a> (E) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Eridanus" style="background-image: none; text-decoration: none;" title="Eridanus">Eridanus</a>. Possui uma declinação de -01° 16' 28" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-image: none;" title="Ascensão recta">ascensão recta</a> de 2 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; text-decoration: none;" title="Hora">horas</a>, 52 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; text-decoration: none;" title="Minuto">minutos</a> e 51,8 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; text-decoration: none;" title="Segundo">segundos</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A galáxia <b>NGC 1132</b> foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/23_de_Novembro" style="background-image: none; text-decoration: none;" title="23 de Novembro">23 de Novembro</a> de <a href="http://pt.wikipedia.org/wiki/1827" style="background-image: none; text-decoration: none;" title="1827">1827</a> por <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-image: none; text-decoration: none;" title="John Herschel">John Herschel</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/NGC_1132">http://pt.wikipedia.org/wiki/NGC_1132</a><span style="font-weight: bold;"></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-weight: bold;">NGC 1132: A Mysterious Elliptical Galaxy</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; font-weight: bold;"><img alt="NGC 1132" src="http://chandra.harvard.edu/photo/2008/ngc1132/ngc1132_w11.jpg" /></span></div>
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<a href="http://chandra.harvard.edu/photo/2008/ngc1132/index.html"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://chandra.harvard.edu/photo/2008/ngc1132/index.html</span></a></div>
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<tr><td style="padding-left: 23px;" valign="top" width="40%"><span class="bold"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Credit </span></span></td><td valign="top" width="60%"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">X-ray: NASA/CXC/Penn State/G. Garmire; Optical: NASA/ESA/STScI/M. West</span></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">This image of the elliptical galaxy NGC 1132 and its surrounding region combines data from NASA's Chandra X-ray Observatory and the Hubble Space Telescope. The blue/purple in the image is the X-ray glow from hot, diffuse gas detected by Chandra. Hubble's data reveal a giant foreground elliptical galaxy, plus numerous dwarf galaxies in its neighborhood, and many much more distant galaxies in the background.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Astronomers have dubbed NGC 1132 a "fossil group" because it contains an enormous amount of dark matter, comparable to the dark matter found in an entire group of galaxies. Also, the large amount of hot gas detected by Chandra is usually found for groups of galaxies, rather than a single galaxy.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Leia mais em <a href="http://chandra.harvard.edu/photo/2008/ngc1132/index.html">http://chandra.harvard.edu/photo/2008/ngc1132/index.html</a></span></div>
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<a href="http://chandra.harvard.edu/photo/2008/ngc1132/ngc1132_hst.jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://chandra.harvard.edu/photo/2008/ngc1132/ngc1132_hst.jpg</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; text-align: left;">Hubble Optical Image of NGC 1132 </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="text-align: left;">The elliptical galaxy NGC 1132 reveals the final result of what may have been a group of galaxies that merged together in the recent past. Another possibility is that the galaxy formed in isolation as a "lone wolf" in a universe ablaze with galaxy groups and clusters. This image of NGC 1132 was taken with Hubble's Advanced Camera for Surveys. Data obtained in 2005 and 2006 through green and near-infrared filters were used in the composite. NGC 1132 is located approximately 318 million light-years away in the constellation Eridanus, the River. </span><a href="http://hubblesite.org/newscenter/archive/releases/2008/07" style="text-align: left; text-decoration: none;" target="_blank">More information at Hubble</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span class="caption" style="background-color: white; color: #073763; line-height: 12px; text-align: left;">(Credit: Optical: NASA/ESA/STScI/M. West)</span></span></div>
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<span class="caption" style="font-weight: normal; line-height: 12px; text-align: left;"><a href="http://chandra.harvard.edu/photo/2008/ngc1132/ngc1132_xray.jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://chandra.harvard.edu/photo/2008/ngc1132/ngc1132_xray.jpg</span></a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; text-align: left;">Chandra X-ray Image of NGC 1132 </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; text-align: left;">This image of elliptical galaxy NGC 1132 and its surrounding region shows the X-ray glow from hot, diffuse gas detected by Chandra. Astronomers have dubbed NGC 1132 a "fossil group" because it contains an enormous amount of dark matter, comparable to the dark matter found in an entire group of galaxies. Also, the large amount of hot gas detected by Chandra is usually found for groups of galaxies, rather than a single galaxy. On the right, the white box represents the Hubble Space Telescope's field of view.</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span class="caption" style="background-color: white; color: #073763; line-height: 12px; text-align: left;">(Credit: X-ray:NASA/CXC/Penn State/G. Garmire)</span></span></div>
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<a href="http://chandra.harvard.edu/photo/2008/ngc1132/more.html"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://chandra.harvard.edu/photo/2008/ngc1132/more.html</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1700</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; text-decoration: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_el%C3%ADptica" style="background-image: none; text-decoration: none;" title="Galáxia elíptica">elíptica</a> (E4) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Eridanus" style="background-image: none; text-decoration: none;" title="Eridanus">Eridanus</a>. Possui uma declinação de -04° 51' 55" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-image: none; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 4 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; text-decoration: none;" title="Hora">horas</a>, 56 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; text-decoration: none;" title="Minuto">minutos</a> e 56,2 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; text-decoration: none;" title="Segundo">segundos</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A galáxia <b>NGC 1700</b> foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/5_de_Outubro" style="background-image: none; text-decoration: none;" title="5 de Outubro">5 de Outubro</a> de <a href="http://pt.wikipedia.org/wiki/1785" style="background-image: none; text-decoration: none;" title="1785">1785</a> por <a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-image: none; text-decoration: none;" title="William Herschel">William Herschel</a>.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/NGC_1700" style="background-color: white;">http://pt.wikipedia.org/wiki/NGC_1700</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span class="page_title" style="background-color: white; color: #073763; font-size: small; font-variant: small-caps; text-align: left;"><span class="page_title">Giant X-Ray Disk Sheds Light On Galactic Merger</span> </span></span></div>
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<a href="http://chandra.harvard.edu/photo/2002/n1700/n1700_xray.jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://chandra.harvard.edu/photo/2002/n1700/n1700_xray.jpg</span></a></div>
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<span class="caption" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 12px;">Credit: NASA/Ohio U./T.Statler et al.</span></div>
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<em><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The Chandra image of the elliptical galaxy NGC 1700 shows a flattened oval of multi-million degree gas, supporting the idea that it is the result of a merger of two smaller galaxies about 3 billion years ago.</span></em></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">.........</span><span style="font-family: Arial, Helvetica, sans-serif;">another version of the Chandra image shows only the low-energy X-rays and reveals a giant inner disk. This disk of 6-million degree gas appears light blue in the multicolor image above.</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">NGC 1309</b><span style="font-weight: normal; line-height: 19.1875px; text-align: start;"> é uma </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-image: none; font-weight: normal; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a><span style="font-weight: normal; line-height: 19.1875px; text-align: start;"> localizada a cerca de cem milhões de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; font-weight: normal; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="font-weight: normal; line-height: 19.1875px; text-align: start;"> de distância na direção da </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o_de_Er%C3%ADdano" style="background-image: none; font-weight: normal; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Constelação de Erídano">constelação de Erídano</a><span style="font-weight: normal; line-height: 19.1875px; text-align: start;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; font-weight: normal; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="font-weight: normal; line-height: 19.1875px; text-align: start;"> de 11,5, uma declinação de -15º 24' 02" e uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-image: none; font-weight: normal; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="font-weight: normal; line-height: 19.1875px; text-align: start;"> de 3 </span><a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; font-weight: normal; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Hora">horas</a><span style="font-weight: normal; line-height: 19.1875px; text-align: start;">, 22</span><a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; font-weight: normal; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Minuto">minutos</a><span style="font-weight: normal; line-height: 19.1875px; text-align: start;"> e 6,5 </span><a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; font-weight: normal; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Segundo">segundos</a><span style="font-weight: normal; line-height: 19.1875px; text-align: start;">.</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="line-height: 18px; text-align: start;">Credit:</span><span style="font-weight: normal; line-height: 18px; text-align: start;"> </span><a href="http://www.nasa.gov/" style="font-weight: normal; line-height: 18px; text-align: start;">NASA</a><span style="font-weight: normal; line-height: 18px; text-align: start;">, </span><a href="http://www.spacetelescope.org/" style="font-weight: normal; line-height: 18px; text-align: start;">ESA</a><span style="font-weight: normal; line-height: 18px; text-align: start;">, The </span><a href="http://heritage.stsci.edu/" style="font-weight: normal; line-height: 18px; text-align: start;">Hubble Heritage</a><span style="font-weight: normal; line-height: 18px; text-align: start;"> Team, (</span><a href="http://www.stsci.edu/" style="font-weight: normal; line-height: 18px; text-align: start;">STScI</a><span style="font-weight: normal; line-height: 18px; text-align: start;">/</span><a href="http://www.aura-astronomy.org/" style="font-weight: normal; line-height: 18px; text-align: start;">AURA</a><span style="font-weight: normal; line-height: 18px; text-align: start;">) and A. Riess (</span><a href="http://www.stsci.edu/" style="font-weight: normal; line-height: 18px; text-align: start;">STScI</a><span style="font-weight: normal; line-height: 18px; text-align: start;">)</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Looking like a child's pinwheel ready to be set a spinning by a gentle breeze, this dramatic spiral galaxy is one of the latest viewed by NASA's Hubble Space Telescope. Stunning details of the face-on spiral galaxy, cataloged as NGC 1309, are captured in this color image.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Recent observations of the galaxy taken in visible and infrared light come together in a colorful depiction of many of the galaxy's features. Bright blue areas of star formation pepper the spiral arms, while ruddy dust lanes follow the spiral structure into a yellowish central nucleus of older-population stars. The image is complemented by myriad far-off background galaxies.</span></div>
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<span style="font-weight: normal; line-height: 18px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SN2002fk as observed from Lick Observatory Kait 0.76 meter telescope in 2002. The location of the supernova is marked on the 2005 Hubble ACS image.</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold;">Credit for Lick Observatory Image:</span> W. Li and A. V. Filippenko (University of California, Berkeley)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold;">Credit for HST Image:</span> <a href="http://www.nasa.gov/">NASA</a>, <a href="http://www.spacetelescope.org/">ESA</a>, The <a href="http://heritage.stsci.edu/">Hubble Heritage</a> Team (<a href="http://www.stsci.edu/">STScI</a>/<a href="http://www.aura-astronomy.org/">AURA</a>), and A. Riess (<a href="http://www.stsci.edu/">STScI</a>)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1614</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; text-decoration: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral_barrada" style="background-image: none; text-decoration: none;" title="Galáxia espiral barrada">espiral barrada</a> (SBc/P) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Eridanus" style="background-image: none; text-decoration: none;" title="Eridanus">Eridanus</a>. Possui uma declinação de -08° 34' 45" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-image: none; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 4 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; text-decoration: none;" title="Hora">horas</a>, 33 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; text-decoration: none;" title="Minuto">minutos</a> e 59,8 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; text-decoration: none;" title="Segundo">segundos</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A galáxia <b>NGC 1614</b> foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/29_de_Dezembro" style="background-image: none; text-decoration: none;" title="29 de Dezembro">29 de Dezembro</a> de <a href="http://pt.wikipedia.org/wiki/1885" style="background-image: none; text-decoration: none;" title="1885">1885</a> por <a href="http://pt.wikipedia.org/wiki/Lewis_A._Swift" style="background-image: none; text-decoration: none;" title="Lewis A. Swift">Lewis A. Swift</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Hubble Interacting Galaxy NGC 1614</span></h2>
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<a href="http://hubblesite.org/newscenter/archive/releases/2008/16/image/bq/format/large_web/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/2008/16/image/bq/format/large_web/</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Object Names:</strong> NGC 1614, Arp 186, Mrk 0617, II Zw 015</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Image Type:</strong> Astronomical</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold;">Credit:</span> <a href="http://www.nasa.gov/">NASA</a>, <a href="http://www.spacetelescope.org/">ESA</a>, the <a href="http://heritage.stsci.edu/">Hubble Heritage</a> (<a href="http://www.stsci.edu/">STScI</a>/<a href="http://www.aura-astronomy.org/">AURA</a>)-<a href="http://www.spacetelescope.org/">ESA</a>/Hubble Collaboration, and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The galaxy system NGC 1614 has a bright optical center and two clear inner spiral arms that are fairly symmetrical. It also has a spectacular outer structure that consists principally of a large one-sided curved extension of one of these arms to the lower right, and a long, almost straight tail that emerges from the nucleus and crosses the extended arm to the upper right. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">LEIA MAIS EM</span></div>
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<a href="http://hubblesite.org/newscenter/archive/releases/2008/16/image/bq/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/2008/16/image/bq/</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1531</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; text-decoration: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_el%C3%ADptica" style="background-image: none; text-decoration: none;" title="Galáxia elíptica">elíptica</a> (E-S0) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Eridanus" style="background-image: none; text-decoration: none;" title="Eridanus">Eridanus</a>. Possui uma declinação de -32° 51' 03" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-image: none;" title="Ascensão recta">ascensão recta</a> de 4 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; text-decoration: none;" title="Hora">horas</a>, 11 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; text-decoration: none;" title="Minuto">minutos</a> e 59,1 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; text-decoration: none;" title="Segundo">segundos</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A galáxia <b>NGC 1531</b> foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/19_de_Outubro" style="background-image: none; text-decoration: none;" title="19 de Outubro">19 de Outubro</a> de <a href="http://pt.wikipedia.org/wiki/1835" style="background-image: none; text-decoration: none;" title="1835">1835</a> por <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-image: none; text-decoration: none;" title="John Herschel">John Herschel</a>.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-weight: bold;"><a href="http://pt.wikipedia.org/wiki/NGC_1531" style="background-color: white;">http://pt.wikipedia.org/wiki/NGC_1531</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1532</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; text-decoration: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral_barrada" style="background-image: none; text-decoration: none;" title="Galáxia espiral barrada">espiral barrada</a> (SBb) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Eridanus" style="background-image: none; text-decoration: none;" title="Eridanus">Eridanus</a>. Possui uma declinação de -32° 52' 23" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-image: none; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 4 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; text-decoration: none;" title="Hora">horas</a>, 12 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; text-decoration: none;" title="Minuto">minutos</a> e 03,8 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; text-decoration: none;" title="Segundo">segundos</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A galáxia <b>NGC 1532</b> foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/29_de_Outubro" style="background-image: none; text-decoration: none;" title="29 de Outubro">29 de Outubro</a> de <a href="http://pt.wikipedia.org/wiki/1826" style="background-image: none; text-decoration: none;" title="1826">1826</a> por <a href="http://pt.wikipedia.org/wiki/James_Dunlop" style="background-image: none; text-decoration: none;" title="James Dunlop">James Dunlop</a>.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/NGC_1532" style="background-color: white;">http://pt.wikipedia.org/wiki/NGC_1532</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Ballet of Interacting Galaxies</span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="font-weight: normal; line-height: 19.1875px;">This photograph was produced by </span><b style="line-height: 19.1875px;"><a class="extiw" href="http://en.wikipedia.org/wiki/European_Southern_Observatory" style="background-image: none; text-decoration: none;" title="en:European Southern Observatory">European Southern Observatory (ESO)</a></b><span style="font-weight: normal; line-height: 19.1875px;">.</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="external text" href="http://www.eso.org/" rel="nofollow">ESO</a><span style="font-weight: normal; line-height: 19.1875px;">/IDA/Danish 1.5 m/R.Gendler and J.-E. Ovaldsen</span></span></div>
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<a href="http://www.eso.org/public/images/ngc1532/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.eso.org/public/images/ngc1532/</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The pair of galaxies NGC 1531/2, engaged in a spirited waltz, is located about 70 million light-years away towards the southern constellation Eridanus (The River). The deformed foreground spiral galaxy laced with dust lanes NGC 1532 is so close to its companion — the background galaxy with a bright core just above the centre of NGC 1532 — that it gets distorted: one of its spiral arms is warped and plumes of dust and gas are visible above its disc. The cosmic dance leads to another dramatic effect: a whole new generation of massive stars were born in NGC 1532 because of the interaction. They are visible as the purple objects in the spiral arms.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">This exquisite image was made using the 1.5-metre Danish telescope at the ESO La Silla Observatory, Chile. It is based on data obtained through three different filters: B, V and R. The field of view is 12 x 12 arcmin.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1518</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; text-decoration: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral_barrada" style="background-image: none; text-decoration: none;" title="Galáxia espiral barrada">espiral barrada</a> (SBd) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Eridanus" style="background-image: none; text-decoration: none;" title="Eridanus">Eridanus</a>. Possui uma declinação de -21° 10' 46" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-image: none; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 4 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; text-decoration: none;" title="Hora">horas</a>, 06 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; text-decoration: none;" title="Minuto">minutos</a> e 49,0 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; text-decoration: none;" title="Segundo">segundos</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A galáxia <b>NGC 1518</b> foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/13_de_Novembro" style="background-image: none; text-decoration: none;" title="13 de Novembro">13 de Novembro</a> de <a href="http://pt.wikipedia.org/wiki/1835" style="background-image: none; text-decoration: none;" title="1835">1835</a> por <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-image: none; text-decoration: none;" title="John Herschel">John Herschel</a>.</span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_1518"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_1518</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://cseligman.com/text/atlas/ngc15.htm#1518"></a><a href="http://cseligman.com/text/atlas/ngc15.htm#1518">http://cseligman.com/text/atlas/ngc15.htm#1518</a></span></div>
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<a href="http://www.blogger.com/blogger.g?blogID=4158372707710982464" name="1518"><big><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1518 (= PGC 14475)</span></b></big></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.blogger.com/blogger.g?blogID=4158372707710982464" name="1518">Discovered (Nov 13, 1835) by </a><a href="http://cseligman.com/text/atlas/discoverers.htm#jfwherschel">John Herschel</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="font-weight: normal;">A 12th-magnitude spiral galaxy (type SB(s)dm) in </span><a href="http://cseligman.com/text/atlas/eridanus.htm#1518" style="font-weight: normal;">Eridanus</a><span style="font-weight: normal;"> (RA 04 06 49.0, Dec -21 10 46)</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The second IC notes (per Howe) "Minute of RA is 00, not 01". Based on a recessional velocity of 920 km/sec, NGC 1517 is about 40 million light years away, in reasonable agreement with redshift-independent distance estimates of 25 to 40 million light years. Given that and its apparent size of 2.9 by 1.4 arcmin, it is about 35 thousand light years across.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="DSS image of spiral galaxy NGC 1518" border="1" src="http://cseligman.com/text/atlas/ngc1518.jpg" height="750" style="font-weight: normal;" title="DSS image of spiral galaxy NGC 1518" width="750" /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-weight: normal;">Above, a 3.6 arcin wide closeup of NGC 1518</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="font-weight: normal;">Below, a detailed view of the northern half of the galaxy </span><small style="font-weight: normal;">(Image Credits: Hubble Legacy Archive)</small></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="More or less cleaned up 'raw' HST image of part of spiral galaxy NGC 1518" border="1" src="http://cseligman.com/text/atlas/ngc1518hst.jpg" height="1039" style="font-weight: normal;" title="More or less cleaned up 'raw' HST image of spiral galaxy NGC 1518" width="750" /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-weight: normal;">Below, a 12 arcmin wide region centered on the galaxy</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="DSS image of region near spiral galaxy NGC 1518" border="1" src="http://cseligman.com/text/atlas/ngc1518wide.jpg" height="750" style="font-weight: normal;" title="DSS image of region near spiral galaxy NGC 1518" width="750" /></span></div>
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<a href="http://cseligman.com/text/atlas/ngc15.htm#1518"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://cseligman.com/text/atlas/ngc15.htm#1518</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1535 - Eridanus - Nebulosa Nebulosa Planetária</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 04h13m Declinação -12<sup>o</sup>.48<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo Nebulosa Planetária NP Dimensão 0,5 Magnitude 17<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude da Estrela associada 12 <o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">NGC 1535</b><span style="line-height: 19.1875px; text-align: start;"> é uma </span><a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Nebulosa planetária">nebulosa planetária</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Eridanus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Eridanus">constelação de Eridanus</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="William Herschel">William Herschel</a><span style="line-height: 19.1875px; text-align: start;"> em 1785, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="line-height: 19.1875px; text-align: start;"> refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;">(+9,6), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="line-height: 19.1875px; text-align: start;"> amadores ou com equipamentos superiores.</span></span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_1535"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_1535</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1234</b> is <a href="http://en.wikipedia.org/wiki/Barred_spiral_galaxy" style="background-image: none; text-decoration: none;" title="Barred spiral galaxy">barred spiral galaxy</a> in the constellation <a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)" style="background-image: none; text-decoration: none;" title="Eridanus (constellation)">Eridanus</a>, discovered by <a class="new" href="http://en.wikipedia.org/w/index.php?title=Francis_Preserved_Leavenworth&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="Francis Preserved Leavenworth (page does not exist)">Francis Preserved Leavenworth</a> in 1886.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Its <a href="http://en.wikipedia.org/wiki/Apparent_magnitude" style="background-image: none; text-decoration: none;" title="Apparent magnitude">apparent magnitude</a> is 14.2</span></div>
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<a href="http://en.wikipedia.org/wiki/NGC_1234"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://en.wikipedia.org/wiki/NGC_1234</span></a></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 143.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Author</span></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background-image: none; text-decoration: none;" title="en:NASA">en:NASA</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-image: none; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span></td></tr>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; line-height: 19.1875px;"><b>NGC 1300</b> is a <a href="http://en.wikipedia.org/wiki/Barred_spiral_galaxy" style="background-image: none; text-decoration: none;" title="Barred spiral galaxy">barred spiral galaxy</a> about <a class="mw-redirect" href="http://en.wikipedia.org/wiki/1_E23_m" style="background-image: none; text-decoration: none;" title="1 E23 m">61 million</a> <a href="http://en.wikipedia.org/wiki/Light-year" style="background-image: none; text-decoration: none;" title="Light-year">light-years</a> away in the <a href="http://en.wikipedia.org/wiki/Constellation" style="background-image: none; text-decoration: none;" title="Constellation">constellation</a> <a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)" style="background-image: none; text-decoration: none;" title="Eridanus (constellation)">Eridanus</a>. The galaxy is about 110,000 light-years across; just slightly larger than our own galaxy, the <a href="http://en.wikipedia.org/wiki/Milky_Way" style="background-image: none; text-decoration: none;" title="Milky Way">Milky Way</a>. It is a member of the<a href="http://en.wikipedia.org/wiki/Eridanus_Cluster" style="background-image: none; text-decoration: none;" title="Eridanus Cluster">Eridanus Cluster</a>, a cluster of 200 galaxies.<sup class="reference" id="cite_ref-NGC1300_3-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/NGC_1300#cite_note-NGC1300-3" style="background-image: none; text-decoration: none; white-space: nowrap;">[3]</a></sup><sup class="reference" id="cite_ref-atlas_4-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/NGC_1300#cite_note-atlas-4" style="background-image: none; text-decoration: none; white-space: nowrap;">[4]</a></sup> It was discovered by <a class="mw-redirect" href="http://en.wikipedia.org/wiki/John_Frederick_William_Herschel" style="background-image: none; text-decoration: none;" title="John Frederick William Herschel">John Frederick William Herschel</a> in 1835.<sup class="Template-Fact" style="line-height: 1em; white-space: nowrap;">[<i><a href="http://en.wikipedia.org/wiki/Wikipedia:Citation_needed" style="background-image: none; text-decoration: none;" title="Wikipedia:Citation needed"><span title="This claim needs references to reliable sources. (March 2007)">citation needed</span></a></i>]</sup></span></span></div>
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<a href="http://en.wikipedia.org/wiki/File:Hubble2005-01-barred-spiral-galaxy-NGC1300.jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://en.wikipedia.org/wiki/File:Hubble2005-01-barred-spiral-galaxy-NGC1300.jpg</span></a></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 143.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Source</span></td><td><ul style="line-height: 1.5em;">
<li style="margin-bottom: 0.1em;"><a class="external free" href="http://hubblesite.org/newscenter/archive/releases/2005/01/image/a" rel="nofollow"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/2005/01/image/a</span></a></li>
<li style="margin-bottom: 0.1em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="external free" href="http://www.spacetelescope.org/images/html/opo0501a.html" rel="nofollow">http://www.spacetelescope.org/images/html/opo0501a.html</a> (<a class="external text" href="http://www.spacetelescope.org/images/large/opo0501a.jpg" rel="nofollow">direct link</a>)</span></li>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 143.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Author</span></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NASA, ESA, and The Hubble Heritage Team STScI/AURA)</span></td></tr>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; line-height: 18px;">At Hubble's resolution, a myriad of fine details, some of which have never before been seen, is seen throughout the galaxy's arms, disk, bulge, and nucleus. Blue and red supergiant stars, star clusters, and star-forming regions are well resolved across the spiral arms, and dust lanes trace out fine structures in the disk and bar. Numerous more distant galaxies are visible in the background, and are seen even through the densest regions of NGC 1300</span></span></div>
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<a href="http://hubblesite.org/newscenter/archive/releases/2005/01/image/a/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/2005/01/image/a/</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold;">Credit:</span> <a href="http://www.nasa.gov/">NASA</a>, <a href="http://www.spacetelescope.org/">ESA</a>, and The <a href="http://heritage.stsci.edu/">Hubble Heritage</a> Team (<a href="http://www.stsci.edu/">STScI</a>/<a href="http://www.aura-astronomy.org/">AURA</a>)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold;">Acknowledgment:</span> P. Knezek (WIYN)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Giant Radio Jet Coming from Wrong Kind of Galaxy</span></h1>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://hubblesite.org/newscenter/archive/releases/2003/04/image/b/format/web_print/" style="background-color: white;">http://hubblesite.org/newscenter/archive/releases/2003/04/image/b/format/web_print/</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold; line-height: 18px; text-align: start;">Credit:</span><span style="line-height: 18px; text-align: start;"> </span><a href="http://www.nasa.gov/" style="line-height: 18px; text-align: start;">NASA</a><span style="line-height: 18px; text-align: start;">, W. Keel (University of Alabama), M. Ledlow (Gemini Observatory), F. Owen (NRAO) and AUI/NSF</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://hubblesite.org/newscenter/archive/releases/2003/04/image/a/format/large_web/" style="background-color: white;">http://hubblesite.org/newscenter/archive/releases/2003/04/image/a/format/large_web/</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Jurassic Space: Ancient Galaxies Come Together After Billions of Years</span></h1>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://hubblesite.org/newscenter/archive/releases/2010/08/image/a/format/web_print/" style="background-color: white;">http://hubblesite.org/newscenter/archive/releases/2010/08/image/a/format/web_print/</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Object Name:</strong> HCG 31</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Image Type:</strong> Astronomical</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold;">Credit:</span> <a href="http://www.nasa.gov/">NASA</a>, <a href="http://www.spacetelescope.org/">ESA</a>, S. Gallagher (The University of Western Ontario), and J. English (University of Manitoba)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">These four dwarf galaxies waited billions of years to come together, setting off a fireworks show as thousands of new star clusters come to life. The distorted galaxies are quickly producing massive, hot, young stars that are pumping out ultraviolet radiation, heating up surrounding gas clouds, and causing them to glow.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Such encounters between dwarf galaxies are normally seen billions of light-years away and therefore occurred billions of years ago. But these galaxies, members of Hickson Compact Group 31, are relatively nearby, only 166 million light-years away.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">LEIA MAIS EM <a href="http://hubblesite.org/newscenter/archive/releases/2010/08/image/a/" style="line-height: 19.1875px; text-align: justify;">http://hubblesite.org/newscenter/archive/releases/2010/08/image/a/</a></span></div>
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<a href="http://hubble.hq.eso.org/images/potw1349a/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">A members-only galaxy club</span></a></h2>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://hubble.hq.eso.org/static/archives/images/screen/potw1349a.jpg" height="330" width="640" /></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">This new Hubble image shows a handful of galaxies in the constellation of Eridanus (The River).</span><span style="font-family: Arial, Helvetica, sans-serif;"> NGC 1190</span><span style="font-family: Arial, Helvetica, sans-serif;">, shown here on the right of the frame, stands apart from the rest; it belong to an exclusive club known as Hickson Compact Group 22 (HCG 22).</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">There are four other members of this group, all of which lie out of frame: NGC 1189, NGC 1191, NGC 1192, and NGC 1199. The other galaxies shown here are nearby galaxies 2MASS J03032308-1539079 (centre), and dCAZ94 HCG 22-21 (left), both of which are not part of HCG 22.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">LEIA MAIS EM</span></div>
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<a href="http://hubble.hq.eso.org/images/potw/?search=Eridanus"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubble.hq.eso.org/images/potw/?search=Eridanus</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1190</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; text-decoration: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_lenticular" style="background-image: none; text-decoration: none;" title="Galáxia lenticular">lenticular</a> (S0) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Eridanus" style="background-image: none; text-decoration: none;" title="Eridanus">Eridanus</a>. Possui uma declinação de -15° 39' 44" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-image: none; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 3 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; text-decoration: none;" title="Hora">horas</a>, 03 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; text-decoration: none;" title="Minuto">minutos</a> e 26,0 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; text-decoration: none;" title="Segundo">segundos</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A galáxia <b>NGC 1190</b> foi descoberta em <a href="http://pt.wikipedia.org/wiki/1886" style="background-image: none; text-decoration: none;" title="1886">1886</a> por <a href="http://pt.wikipedia.org/wiki/Frank_Leavenworth" style="background-image: none; text-decoration: none;" title="Frank Leavenworth">Frank Leavenworth</a>.</span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_1190"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_1190</span></a></div>
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<a href="http://hubble.hq.eso.org/images/potw1103a/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Islands of stars in the river</span></a></h2>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The spiral galaxy <b>NGC 1345</b> and its loose and ragged arms dominate this rich image from the NASA/ESA Hubble Space Telescope. It is a member of the Eridanus Galaxy Cluster — a group of about 70 galaxies that lies 85 million light-years away in the constellation of Eridanus (the River). This region of the night sky is well populated with bright galaxies, with the Fornax Cluster of galaxies also nearby on the celestial sphere, although the two clusters are actually separated by about 20 million light-years. Collectively, they are known as the Fornax Supercluster or the Southern Supercluster.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">John Herschel discovered NGC 1345 in 1835 from South Africa. He described it as small and very faint and it is still far from easy to see it even with quite a large amateur telescope, where it appears as a small, circular fuzz.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">LEIA MAIS EM <a href="http://hubble.hq.eso.org/images/potw/?search=Eridanus" style="line-height: normal;">http://hubble.hq.eso.org/images/potw/?search=Eridanus</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1345</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; text-decoration: none;" title="Galáxia">galáxia</a> {{{typ}}} localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Eridanus" style="background-image: none; text-decoration: none;" title="Eridanus">Eridanus</a>. Possui uma declinação de -17° 46' 45" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-image: none;" title="Ascensão recta">ascensão recta</a> de 3 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; text-decoration: none;" title="Hora">horas</a>, 29 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; text-decoration: none;" title="Minuto">minutos</a> e 31,5 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; text-decoration: none;" title="Segundo">segundos</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A galáxia <b>NGC 1345</b> foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/11_de_Dezembro" style="background-image: none; text-decoration: none;" title="11 de Dezembro">11 de Dezembro</a> de <a href="http://pt.wikipedia.org/wiki/1835" style="background-image: none; text-decoration: none;" title="1835">1835</a> por <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-image: none; text-decoration: none;" title="John Herschel">John Herschel</a>.</span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_1345"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_1345</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">NASA Telescopes Help Discover Surprisingly Young Galaxy</span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Object Name:</strong> Abell 383</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Image Type:</strong> Astronomical</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold;">Credit:</span> <a href="http://www.nasa.gov/">NASA</a>, <a href="http://www.spacetelescope.org/">ESA</a>, J. Richard (Center for Astronomical Research/Observatory of Lyon, France), and J.-P. Kneib (Astrophysical Laboratory of Marseille, France)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold;">Acknowledgment:</span> M. Postman (<a href="http://www.stsci.edu/">STScI</a>)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Astronomers have uncovered one of the youngest galaxies in the distant universe, with stars that formed 13.5 billion years ago, a mere 200 million years after the Big Bang. The finding addresses questions about when the first galaxies arose, and how the early universe evolved.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NASA's Hubble Space Telescope was the first to spot the newfound galaxy. Detailed observations from the W.M. Keck Observatory on Mauna Kea in Hawaii revealed the observed light dates to when the universe was only 950 million years old; the universe formed about 13.7 billion years ago.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">LEIA MAIS EM <a href="http://hubblesite.org/newscenter/archive/releases/2011/12/image/a/" style="line-height: 19.1875px; text-align: justify;">http://hubblesite.org/newscenter/archive/releases/2011/12/image/a/</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Lensing Galaxy Cluster Abell 383 (Annotated)</span></h2>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 19.1875px;"><span style="background-color: white; color: #073763; font-weight: bold; line-height: normal; text-align: -webkit-left;">Abell 383: Getting a Full Picture of an Elusive Subject</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Abell 383" src="http://chandra.harvard.edu/photo/2012/a383/a383_w33.jpg" /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://chandra.harvard.edu/photo/2012/a383/index.html" style="background-color: white;">http://chandra.harvard.edu/photo/2012/a383/index.html</a></span></div>
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<tr><td valign="top" width="60%"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">X-ray: NASA/CXC/Caltech/A.Newman et al/Tel Aviv/A.Morandi & M.Limousin; Optical: NASA/STScI, ESO/VLT, SDSS</span></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 16px; text-align: -webkit-left;">Two teams of astronomers have used data from NASA's Chandra X-ray Observatory and other telescopes to map the distribution of </span><a href="http://chandra.harvard.edu/xray_astro/dark_matter/" style="line-height: 16px; text-align: -webkit-left; text-decoration: none;">dark matter</a><span style="line-height: 16px; text-align: -webkit-left;"> in a galaxy cluster known as Abell 383, which is located about 2.3 billion light years from Earth.</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 16px;">LEIA MAIS EM </span><a href="http://chandra.harvard.edu/photo/2012/a383/index.html" style="text-align: justify;">http://chandra.harvard.edu/photo/2012/a383/index.html</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-weight: bold; text-align: -webkit-left;">Abell 521: A Galaxy Cluster Mash-up</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://chandra.harvard.edu/photo/2008/a521/index.html" style="background-color: white; line-height: 19.1875px;">http://chandra.harvard.edu/photo/2008/a521/index.html</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; line-height: 16px; text-align: -webkit-left;">This composite image shows the galaxy cluster Abell 521, located about 2.9 billion light years from Earth.</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 16px; text-align: -webkit-left;">LEIA MAIS EM </span><a href="http://chandra.harvard.edu/photo/2008/a521/index.html">http://chandra.harvard.edu/photo/2008/a521/index.html</a></span></div>
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<a href="http://upload.wikimedia.org/wikipedia/commons/thumb/0/0f/Earth%27s_Location_in_the_Universe_SMALLER_%28JPEG%29.jpg/1024px-Earth%27s_Location_in_the_Universe_SMALLER_%28JPEG%29.jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://upload.wikimedia.org/wikipedia/commons/thumb/0/0f/Earth%27s_Location_in_the_Universe_SMALLER_%28JPEG%29.jpg/1024px-Earth%27s_Location_in_the_Universe_SMALLER_%28JPEG%29.jpg</span></a><br />
<table cellpadding="4" class="toccolours vevent mw-content-ltr" style="border: 1px solid rgb(170, 170, 170); direction: ltr; line-height: 19.1875px; padding: 5px; text-align: center; width: 1024px;"><tbody>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 143.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Author</span></td><td><a href="http://commons.wikimedia.org/wiki/User:Azcolvin429" style="background-image: none;" title="User:Azcolvin429"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Andrew Z. Colvin</span></a></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>O TEXTO ABAIXO É DE UMA SIMPLICIDADE ÍMPAR, </b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>a meu ver, </b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NA EXPLICAÇÃO SOBRE AS ESTRUTURAS DO UNIVERSO.</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A síntese e a tradução livre e literal foi realizada por mim, Janine.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="font-weight: normal;">Direitos autorais </span><span style="font-weight: normal; line-height: 13.5pt; text-align: start;">© 2013 A AstroGnom.</span></span></h3>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://de.spacechris.com/2013/05/12/was-ist-ein-void-die-strukturen-des-universums/#comments">http://de.spacechris.com/2013/05/12/was-ist-ein-void-die-strukturen-des-universums/#comments</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://de.spacechris.com/2013/05/12/ein-dankeschon-an-chris-hadfield/"><span lang="EN-US">Ein ‘Dankeschön’ an Chris Hadfield</span></a> <span lang="EN-US">– Agradecimento a Chris Hadfield<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">von<span class="apple-converted-space"> </span></span><span class="fn"><a href="http://de.spacechris.com/author/admin/"><span style="text-align: start;"><span lang="EN-US">Spacechris</span></span></a></span><span class="fn"> <span lang="EN-US">– De </span></span><a href="http://de.spacechris.com/author/admin/"><span lang="EN-US">http://de.spacechris.com/author/admin/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="font-weight: normal;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Was ist ein “Void”? Die Strukturen des Universums<o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">What is a "Void"?</span><span lang="EN-US"> </span><span lang="EN-US">The </span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">structures of the universe<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Síntese e tradução livre e literal realizada a partir da versão inglesa por Janine Milward<o:p></o:p></span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O que é um “Void”? As Estruturas do Universo<o:p></o:p></span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É preciso que saibamos que nosso universo não é sem-estrutura. Mesmo em escalas imensas, uma estrutura pode ser encontrada. Para melhor compreendermos essa realidade, temos que fazer uma enorme viagem.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ao fazermos um ZOOM a partir da Terra e em direção à imensidão do universo, estaremos primeiramente encontrando 7 planetas que, juntamente com nossa Terra, se movimentam em torno de uma estrela, o Sol. Planetas e Sol formam o Sistema Solar. <o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando o zoom se amplia, descobrimos muitas estrelas, outros sistemas solares. Estes sistemas solares vivenciam em conjunto uma estrutura chamada Galáxia. Nossa Galáxia é conhecida por nós como Via Lactea. Quando nosso zoom se amplia ainda mais, encontramos uma vizinhança de nossa Galáxia, algumas outras galáxias – como, por exemplo, a galáxia Andromeda. Estas galáxias foram Grupos ou Aglomerados. A Via Lactea e Andromeda e outras galáxias menores em nossa vizinhança formam o chamado Grupo Local. O Grupo Local contém cerca de 500 galáxias e possui um diâmetro aproximado de 7 milhões de anos-luz.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ao aprofundarmos o zoom, encontraremos muitas dessas galáxias e que vão formando estruturas. Os Aglomerados de galáxias se encontram com outros Aglomerados e são formados aquilo que denominamos de Superaglomerados. Nosso Grupo Local pertence ao Superaglomerado Virgo. Esse Superaglomerado possui cerca de 200 Aglomerados de galáxias e possui um diâmetro de cerca de 200 milhões de anos-luz.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Porém, as dimensões continuam em suas amplitudes e quando usamos o zoom para ainda além os Superaglomerados, podemos notar que estes Superaglomerados também formam estruturas que são chamadas de Filamentos. Um famoso Filamento é referido como A Grande Muralha (The Great Wall). A Grande Muralha possui um comprimento aproximado de 500 milhões de anos-luz e possui altura de cerca de 300 milhões de anos-luz e 15 milhões de anos-luz de espessura.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ainda mais distante, estaremos encontrando a Grande Muralha Sloan (Sloan Great Wall) – também um Filamento porém de dimensão inteiramente diferente. A Grande Muralha Sloan possui um comprimento aproximado de 1.3 bilhões de anos-luz!<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">Agora que esclarecemos sobre as estruturas no espaço, podemos começar a conversar sobre o Void, o Vazio. Mencionamos as maiores estruturas do universo – os Filamentos todos ligados entre si como se fosse uma malha de favo de mel. Entre os Filamentos, existe o Void, o Nada, o Vazio. Não existe nada no Vazio, nem gás, nem poeira e certamente nem estrelas ou planetas. No entanto, acredita-se que a tão comentada Matéria Escura exista nos Voids – mesmo que não emita luz ou radiação quaisquer e que, portanto, não é visível.</span><span style="font-family: Arial, sans-serif; font-size: 9pt;"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">https://cienciasetecnologia.com/superaglomerados-galaxias-vacuos-rede-cosmica/</span></span><br />
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<a href="http://www.whillyard.com/science-pages/voids.html"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.whillyard.com/science-pages/voids.html</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Cosmic voids, and supervoids, are large volumes of space that are devoid of matter. This includes normal matter, in the form of galaxies, and dark matter. Initially, astronomers were not sure if the voids contained dark matter, even though there were no galaxies, but recent observations show that the halos of dark matter are not present. The filamentary structure of galactic superclusters surrounds the voids. While space is mostly empty, voids are large volumes, tens of megaparsecs across. The largest confirmed supervoids are about 100 Mpc (325 million light-years) or more across . The larger known voids include the Boötes Supervoid, and the Northern and Southern Local Supervoids. To explain the cold spot in the cosmic microwave background (CMB), some astronomers propose a huge supervoid, tentatively dubbed the Eridanus or Great supervoid. The Capricornus void is another disputed void, but would be around 230 Mpc across. This link has some of the latest information on<a href="http://www.universetoday.com/2008/08/17/dark-matter-is-missing-from-cosmic-voids/" target="_blank">cosmic voids</a>. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The Eridanus Supervoid, or Great Void, is conjectural, and has been suggested as a way to explain the "cold spot" in the cosmic microwave background radiation, or CMB. This would be an extraordinarily large region of the universe, at least 150 Mpc or 500 million light-years across, and possibly twice this figure. It is also very distant at between 1.8 Gpc and 3 Gpc (6 to 10 billion light-years). Many astronomers and cosmologists do not accept the supervoid theory for the aberration in the CMB, but many of the alternatives are even more astounding including cosmic textures and parallel universes. So the jury remains out on this one. </span></div>
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<a href="http://www.whillyard.com/science-pages/voids.html"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.whillyard.com/science-pages/voids.html</span></a></div>
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<a href="http://en.wikipedia.org/wiki/Void_(astronomy)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://en.wikipedia.org/wiki/Void_(astronomy)</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">In <a href="http://en.wikipedia.org/wiki/Astronomy" style="background-image: none; text-decoration: none;" title="Astronomy">astronomy</a>, <b>voids</b> are the vast empty spaces between <a href="http://en.wikipedia.org/wiki/Galaxy_filament" style="background-image: none; text-decoration: none;" title="Galaxy filament">filaments</a> (the largest-scale structures in the <a href="http://en.wikipedia.org/wiki/Universe" style="background-image: none; text-decoration: none;" title="Universe">Universe</a>), which contain <a href="http://en.wikipedia.org/wiki/Void_galaxy" style="background-image: none; text-decoration: none;" title="Void galaxy">very few</a>, or no, <a href="http://en.wikipedia.org/wiki/Galaxy" style="background-image: none; text-decoration: none;" title="Galaxy">galaxies</a>. They were first discovered in 1978 during a pioneering study by Stephen Gregory and <a href="http://en.wikipedia.org/wiki/Laird_A._Thompson" style="background-image: none; text-decoration: none;" title="Laird A. Thompson">Laird A. Thompson</a> at the <a href="http://en.wikipedia.org/wiki/Kitt_Peak_National_Observatory" style="background-image: none; text-decoration: none;" title="Kitt Peak National Observatory">Kitt Peak National Observatory</a>.<sup class="reference" id="cite_ref-1" style="color: #fff2cc; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Void_(astronomy)#cite_note-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup> Voids typically have a diameter of 11 to 150 <a href="http://en.wikipedia.org/wiki/Parsec#Megaparsecs_and_gigaparsecs" style="background-image: none; text-decoration: none;" title="Parsec">megaparsecs</a>; particularly large voids, defined by the absence of rich <a href="http://en.wikipedia.org/wiki/Supercluster" style="background-image: none; text-decoration: none;" title="Supercluster">superclusters</a>, are sometimes called "supervoids". Voids located in high-density environments are smaller than voids situated in low-density spaces of the universe.<sup class="reference" id="cite_ref-2" style="color: #fff2cc; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Void_(astronomy)#cite_note-2" style="background-image: none; text-decoration: none; white-space: nowrap;">[2]</a></sup> Voids are believed to have been formed by <a href="http://en.wikipedia.org/wiki/Baryon_acoustic_oscillations" style="background-image: none; text-decoration: none;" title="Baryon acoustic oscillations">baryon acoustic oscillations</a> in the <a href="http://en.wikipedia.org/wiki/Big_Bang" style="background-image: none; text-decoration: none;" title="Big Bang">Big Bang</a>—collapses of mass followed by implosions of the compressed <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Baryonic_matter" style="background-image: none; text-decoration: none;" title="Baryonic matter">baryonic matter</a>. Starting from initially small<a href="http://en.wikipedia.org/wiki/Anisotropy" style="background-image: none; text-decoration: none;" title="Anisotropy">anisotropies</a> due to <a href="http://en.wikipedia.org/wiki/Quantum_fluctuation" style="background-image: none; text-decoration: none;" title="Quantum fluctuation">quantum fluctuations</a> in the early Universe, the anisotropies grew larger in scale over time. Regions of higher density collapsed more rapidly under gravity, eventually resulting in the large-scale, foam-like structure or “cosmic web” of voids and galaxy filaments seen today.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Voids appear to correlate with the observed temperature of the <a href="http://en.wikipedia.org/wiki/Cosmic_microwave_background" style="background-image: none; text-decoration: none;" title="Cosmic microwave background">cosmic microwave background</a> (CMB), due to the <a href="http://en.wikipedia.org/wiki/Sachs%E2%80%93Wolfe_effect" style="background-image: none; text-decoration: none;" title="Sachs–Wolfe effect">Sachs–Wolfe effect</a>. Colder regions correlate with voids, whereas hotter regions correlate with filaments, because of <a href="http://en.wikipedia.org/wiki/Gravitational_redshift" style="background-image: none; text-decoration: none;" title="Gravitational redshift">gravitational redshifting</a>. As the Sachs–Wolfe effect is only significant if the Universe is dominated by <a href="http://en.wikipedia.org/wiki/Radiation" style="background-image: none; text-decoration: none;" title="Radiation">radiation</a> or <a href="http://en.wikipedia.org/wiki/Dark_energy" style="background-image: none; text-decoration: none;" title="Dark energy">dark energy</a>, the existence of voids is significant in providing physical evidence for dark energy. <sup class="reference" id="cite_ref-3" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Void_(astronomy)#cite_note-3" style="background-image: none; text-decoration: none; white-space: nowrap;">[3]</a></sup></span></div>
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<span style="line-height: 18px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The Virgo Cluster, however, is merely a minor </span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: #073763; color: #073763; line-height: 18px; text-align: start;">member of a much larger whole. The </span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763; line-height: 18px; text-align: start;">neighboring superclusters are massive, most </span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763; line-height: 18px; text-align: start;">of them three and four times larger than the </span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763; line-height: 18px; text-align: start;">Virgo Cluster and spanning a distance of some </span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763; line-height: 18px; text-align: start;">100 million light years. These leviathans in </span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763; line-height: 18px; text-align: start;">turn form massive chains and walls that </span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763; line-height: 18px; text-align: start;">weave throughout the cosmos. Between </span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763; line-height: 18px; text-align: start;">them exists, quite literally, nothing. These </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18px; text-align: start;">giant voids are hundreds of millions of light </span></span></div>
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years in diameter and most of them contain </div>
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absolutely nothing at all. No stars. No galaxy.</div>
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No matter.</div>
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<span style="line-height: 18px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">LEIA MAIS EM </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span style="line-height: 19.1875px;">The </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Eridanus_Supervoid" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Eridanus Supervoid">Eridanus Supervoid</a></b><span style="line-height: 19.1875px;"><b> </b>is the largest </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Supervoid" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Supervoid">supervoid</a><span style="line-height: 19.1875px;"> (an area of the </span><a href="http://en.wikipedia.org/wiki/Universe" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Universe">universe</a><span style="line-height: 19.1875px;"> devoid of</span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Galaxies" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Galaxies">galaxies</a><span style="line-height: 19.1875px;">) discovered as of 2007. At a diameter of about one billion </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Light_year" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Light year">light years</a><span style="line-height: 19.1875px;"> it is much larger than any other known void. It was discovered by linking a "cold spot" in the </span><a href="http://en.wikipedia.org/wiki/Cosmic_microwave_background" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Cosmic microwave background">cosmic microwave background</a><span style="line-height: 19.1875px;"> to an absence of </span><a href="http://en.wikipedia.org/wiki/Radio_galaxy" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Radio galaxy">radio galaxies</a><span style="line-height: 19.1875px;"> in data of the </span><a href="http://en.wikipedia.org/wiki/United_States" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="United States">United States</a><span style="line-height: 19.1875px;"> </span><a href="http://en.wikipedia.org/wiki/National_Radio_Astronomy_Observatory" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="National Radio Astronomy Observatory">National Radio Astronomy Observatory</a><span style="line-height: 19.1875px;">'s </span><a href="http://en.wikipedia.org/wiki/Very_Large_Array" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Very Large Array">Very Large Array</a><span style="line-height: 19.1875px;"> Sky Survey.</span><sup class="reference" id="cite_ref-2" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)#cite_note-2" style="background-image: none; text-decoration: none; white-space: nowrap;">[2]</a></sup><span style="line-height: 19.1875px;"> There is some speculation that the void may be due to </span><a href="http://en.wikipedia.org/wiki/Quantum_entanglement" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Quantum entanglement">quantum entanglement</a><span style="line-height: 19.1875px;"> between </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Our_universe" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Our universe">our universe</a><span style="line-height: 19.1875px;"> and </span><a href="http://en.wikipedia.org/wiki/Multiverse" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Multiverse">another</a><span style="line-height: 19.1875px;">.</span><sup class="reference" id="cite_ref-3" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)#cite_note-3" style="background-image: none; text-decoration: none; white-space: nowrap;">[3]</a></sup><sup class="reference" id="cite_ref-4" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)#cite_note-4" style="background-image: none; text-decoration: none; white-space: nowrap;">[4]</a></sup></span></div>
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<pre style="text-align: center;"><span style="white-space: normal;"><span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.atlasoftheuniverse.com/nearsc.html" style="text-align: left;"><span style="background-color: white; color: #073763;">http://www.atlasoftheuniverse.com/nearsc.html</span></a></span></span><div style="white-space: normal;">
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a href="http://news.softpedia.com/newsImage/Large-Cosmic-Void-May-Be-a-Black-Hole-2.jpg/" style="background-color: white;">http://news.softpedia.com/newsImage/Large-Cosmic-Void-May-Be-a-Black-Hole-2.jpg/</a></span></h3>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="text-align: start;">Image comment:</b><span style="text-align: start;"> Massive voids separate galaxy superclusters across the Universe</span> <b style="text-align: start;">Image credits:</b><span style="text-align: start;"> NASA / ESA</span></span></div>
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<strong style="line-height: 14px; text-align: justify;"><span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">In a new study, a team of astronomers proposes that a so-called Universe-in-mas black hole is responsible for the development of</span><span style="font-family: Arial, Helvetica, sans-serif;"> an incredibly-large void in the constellation Eridanus.</span></span></strong></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 14px; white-space: normal;"><b> </b></span><a href="http://news.softpedia.com/news/Large-Cosmic-Void-May-Be-a-Black-Hole-201721.shtml">http://news.softpedia.com/news/Large-Cosmic-Void-May-Be-a-Black-Hole-201721.shtml</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span class="mw-headline" id="Supervoid">Supervoid</span><span class="mw-editsection" style="-webkit-user-select: none; color: #fff2cc; display: inline-block; line-height: 1em; margin-left: 1em; padding-right: 0.25em; unicode-bidi: -webkit-isolate; vertical-align: baseline; white-space: nowrap;"><span class="mw-editsection-bracket">[</span><a href="http://en.wikipedia.org/w/index.php?title=Eridanus_(constellation)&action=edit&section=3" style="background-image: none; text-decoration: none;" title="Edit section: Supervoid">edit</a><span class="mw-editsection-bracket">]</span></span></span></h3>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>The <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Eridanus_Supervoid" style="background-image: none; text-decoration: none;" title="Eridanus Supervoid">Eridanus Supervoid</a></b> is the largest <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Supervoid" style="background-image: none; text-decoration: none;" title="Supervoid">supervoid</a> (an area of the <a href="http://en.wikipedia.org/wiki/Universe" style="background-image: none; text-decoration: none;" title="Universe">universe</a> devoid of<a class="mw-redirect" href="http://en.wikipedia.org/wiki/Galaxies" style="background-image: none; text-decoration: none;" title="Galaxies">galaxies</a>) discovered as of 2007. At a diameter of about one billion <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Light_year" style="background-image: none; text-decoration: none;" title="Light year">light years</a> it is much larger than any other known void. It was discovered by linking a "cold spot" in the <a href="http://en.wikipedia.org/wiki/Cosmic_microwave_background" style="background-image: none; text-decoration: none;" title="Cosmic microwave background">cosmic microwave background</a> to an absence of <a href="http://en.wikipedia.org/wiki/Radio_galaxy" style="background-image: none; text-decoration: none;" title="Radio galaxy">radio galaxies</a> in data of the <a href="http://en.wikipedia.org/wiki/United_States" style="background-image: none; text-decoration: none;" title="United States">United States</a> <a href="http://en.wikipedia.org/wiki/National_Radio_Astronomy_Observatory" style="background-image: none; text-decoration: none;" title="National Radio Astronomy Observatory">National Radio Astronomy Observatory</a>'s <a href="http://en.wikipedia.org/wiki/Very_Large_Array" style="background-image: none; text-decoration: none;" title="Very Large Array">Very Large Array</a> Sky Survey.<sup class="reference" id="cite_ref-2" style="color: #fff2cc; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)#cite_note-2" style="background-image: none; text-decoration: none; white-space: nowrap;">[2]</a></sup> There is some speculation that the void may be due to <a href="http://en.wikipedia.org/wiki/Quantum_entanglement" style="background-image: none; text-decoration: none;" title="Quantum entanglement">quantum entanglement</a> between <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Our_universe" style="background-image: none; text-decoration: none;" title="Our universe">our universe</a> and <a href="http://en.wikipedia.org/wiki/Multiverse" style="background-image: none; text-decoration: none;" title="Multiverse">another</a>.<sup class="reference" id="cite_ref-3" style="color: #fff2cc; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)#cite_note-3" style="background-image: none; text-decoration: none; white-space: nowrap;">[3]</a></sup><sup class="reference" id="cite_ref-4" style="color: #fff2cc; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)#cite_note-4" style="background-image: none; text-decoration: none; white-space: nowrap;">[4]</a></sup></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">See also: <a class="mw-redirect" href="http://en.wikipedia.org/wiki/WMAP_cold_spot" style="background-image: none; text-decoration: none;" title="WMAP cold spot">WMAP cold spot</a></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><b style="background-color: white;"> that measures nearly a billion light-years across.</b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">It is empty of both normal matter - such as galaxies and stars -</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"> and the mysterious "dark matter" that cannot be seen directly with telescopes.</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"> The "hole" is located in the direction of the Eridanus constellation</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"> and has been identified in data </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">from a survey of the sky made at radio wavelengths.</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; font-size: small;"> <a href="http://news.bbc.co.uk/2/hi/science/nature/6962185.stm">http://news.bbc.co.uk/2/hi/science/nature/6962185.stm</a></span></span></td></tr>
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<a href="http://www.dailygalaxy.com/my_weblog/2010/08/the-eridanus-void-does-a-megamassive-black-hole-onebillion-light-years-across-exist-a-galaxy-most-po.html" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">The Eridanus Void: Does a MegaMassive Black Hole One-Billion Light Years Across Exist? (A 'Galaxy' Most Popular)</span></a></h3>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">n the Constellation Eridanus appears to be improbable given current cosmological models. A radical and controversial theory proposes that it is a "universe-in-mass black hole" rather than hypothetical dark matter responsible for the phenomenon described as the expanding-accelerating universe. This radical theory of cosmology suggests that stars at the edge of the Hubble length universe are being consumed by a universe-in-mass black hole.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">In August of 2007, astronomers at the University of Minnesota located a gigantic hole in the universe. This empty space, stretching nearly a billion light-years across, is devoid of any matter such as galaxies, stars, and gas, and neither does it contain the strange and mysterious dark matter, which can be detected but not seen.</span></div>
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<a href="http://www.dailygalaxy.com/my_weblog/2010/08/the-eridanus-void-does-a-megamassive-black-hole-onebillion-light-years-across-exist-a-galaxy-most-po.html"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.dailygalaxy.com/my_weblog/2010/08/the-eridanus-void-does-a-megamassive-black-hole-onebillion-light-years-across-exist-a-galaxy-most-po.html</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">New cosmic map reveals colossal structures</span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: normal; text-align: left;">by </span><b style="border: 0px; line-height: normal; margin: 0px; padding: 0px; text-align: left;"><a href="http://www.newscientist.com/search?rbauthors=David+Shiga" style="border: 0px; margin: 0px; padding: 0px; text-decoration: none;">David Shiga</a></b></span></div>
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<a href="http://www.newscientist.com/data/images/ns/cms/dn16903/dn16903-1_500.jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.newscientist.com/data/images/ns/cms/dn16903/dn16903-1_500.jpg</span></a><br />
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<span style="background-color: #073763; line-height: normal; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The new survey mapped the positions of more than 100,000 galaxies. The black strips are areas the survey did not cover because matter in our own galaxy blocked the view (Illustration: Chris Fluke/Swinburne University of Technology)</span></span></div>
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<span style="background-color: #073763; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Enormous cosmic voids and giant concentrations of matter have been observed in a new galaxy survey, one of the biggest completed so far. One of the voids is so large that it is difficult to explain where it came from.</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The survey also found some enormous voids – regions of space that are relatively empty, including one that is about 3.5 billion light years across.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">"This is as big as I've ever seen," survey team member <a href="http://www.cfa.harvard.edu/~huchra/" style="border: 0px; margin: 0px; padding: 0px; text-decoration: none;" target="ns">John Huchra</a> of the Harvard-Smithsonian Center for Astrophysics told <b style="border: 0px; margin: 0px; padding: 0px;">New Scientist</b>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Another <a href="http://www.newscientist.com/article/dn12546-biggest-void-in-space-is-1-billion-light-years-across.html" style="border: 0px; margin: 0px; padding: 0px; text-decoration: none;">large void</a> about 1 billion light years across was discovered previously.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">In fact the newly found void is so large that it is difficult to fit into our present understanding of the universe on the largest scales. Computer simulations show that gravity causes galaxies and galaxy clusters to get closer together over time, with voids growing between the clusters.</span></div>
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<a href="http://www.newscientist.com/article/dn16903-new-cosmic-map-reveals-colossal-structures.html#.UqoNRtJDtx2"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.newscientist.com/article/dn16903-new-cosmic-map-reveals-colossal-structures.html#.UqoNRtJDtx2</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="font-weight: normal;"> by</span><span style="font-weight: normal;"> </span><span style="border: 0px; font-weight: normal; margin: 0px; padding: 0px;"><a href="http://www.newscientist.com/search?rbauthors=Anil+Ananthaswamy" style="border: 0px; margin: 0px; padding: 0px; text-decoration: none;">Anil Ananthaswamy</a></span></span></h1>
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<span style="background-color: #073763; line-height: normal; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The biggest known hole in the universe has left a cold-spot in the cosmic microwave radiation (Illustration: Bill Saxton, NRAO/AUI/NSF, NASA)</span></span></div>
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<span style="font-weight: normal; line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Radio astronomers have found the biggest hole ever seen in the universe. The void, which is nearly a billion light years across, is empty of both normal matter and dark matter. The finding challenges theories of large-scale structure formation in the universe.</span></span></h1>
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<span style="background-color: #073763; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The void, which is about 6 billion to 10 billion light years away, is considerably larger than any found before. Until now, optical surveys have found no voids larger than 80 megaparsecs wide - making the new hole 40 times larger in volume than the previous record holder.</span></span></div>
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<span style="background-color: #073763; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Computer simulations that recreate the formation of clusters and super-clusters have never seen voids of this size. That could be because modellers have not simulated large enough volumes to see such a void, says Rudnick. If they did, maybe a void would emerge. "It is an open question whether this will create problems for structure formation," he says.</span></span></div>
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<span style="background-color: #073763; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">LEIA MAIS EM </span></span></div>
<a href="http://www.newscientist.com/article/dn12546-biggest-void-in-space-is-1-billion-light-years-across.html#.UqoOntJDtx0"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.newscientist.com/article/dn12546-biggest-void-in-space-is-1-billion-light-years-across.html#.UqoOntJDtx0</span></a><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Acessando a Animação abaixo, você poderá saber melhor sobre </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">ERIDANUS SUPERVOID</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> (e também sobre Fornax Cluster):</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: normal;">The Scale of the Universe - Interactive </b><span style="line-height: normal;"></span><br style="line-height: normal;" /><b style="line-height: normal;">Flash Animation Credit & Copyright: </b><span style="line-height: normal;"></span><a href="http://htwins.net/" style="line-height: normal;">Cary & Michael Huang</a></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgv6olvprFB1aM0TZ4vWaLZ5oKEfeKMKqmjK7yP421gdWzAqwUR6WbukFrU4G7JJwoUSmkfoQfPBZZGD2TacGULsOUoyEh9w1QSKVG2QxMFmvyLw3W2OV0gAbCotXjKUS2krHNdkcpin-lo/s1600/eridanus+supervoid+-+largest+scales+of+the+universe.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgv6olvprFB1aM0TZ4vWaLZ5oKEfeKMKqmjK7yP421gdWzAqwUR6WbukFrU4G7JJwoUSmkfoQfPBZZGD2TacGULsOUoyEh9w1QSKVG2QxMFmvyLw3W2OV0gAbCotXjKUS2krHNdkcpin-lo/s640/eridanus+supervoid+-+largest+scales+of+the+universe.jpg" height="416" width="640" /></span></a></div>
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<a href="http://apod.nasa.gov/apod/ap120312.html"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://apod.nasa.gov/apod/ap120312.html</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Explanation: </b>What does the universe look like on small scales? On large scales? <a href="http://apod.nasa.gov/apod/ap100725.html">Humanity</a> is discovering that the universe is a very different place on every proportion that has been explored. For example, so far as we know, every tiny proton is <a href="http://en.wikipedia.org/wiki/Identical_particles">exactly the same</a>, but every <a href="http://apod.nasa.gov/apod/ap120107.html">huge galaxy</a> is different. On more familiar scales, a small glass table top to a human is a <a href="http://en.wikipedia.org/wiki/Fantastic_Voyage">vast plane</a> of strange smoothness to a <a href="http://www.youtube.com/watch?v=47CIdUld8eQ">dust mite</a> -- possibly <a href="http://www.wisegeek.com/where-does-dust-come-from.htm">speckled</a> with cell boulders. Not all scale lengths are <a href="http://www.youtube.com/watch?v=4PKjF7OumYo">well explored</a> -- what happens to the smallest mist droplets you sneeze, for example, is a topic of active research -- and possibly useful to know to help <a href="http://en.wikipedia.org/wiki/Airborne_disease">stop the spread</a> of disease. The <a href="http://htwins.net/scale2/">above interactive flash animation</a>, a modern version of the classic video <a href="http://apod.nasa.gov/apod/ap110201.html">Powers of Ten</a>, is a new window to many of the <a href="http://apod.nasa.gov/apod/ap100120.html">known scales</a> of our universe. By moving the scroll bar across the bottom, you can explore a <a href="http://www.kruger-2-kalahari.com/images/the-long-the-tall-and-the-short-21373953.jpg">diversity of sizes</a>, while clicking on different items will bring up descriptive information.</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Authors & editors: </b><a href="http://www.phy.mtu.edu/faculty/Nemiroff.html">Robert Nemiroff</a> (<a href="http://www.phy.mtu.edu/">MTU</a>) & <a href="http://antwrp.gsfc.nasa.gov/htmltest/jbonnell/www/bonnell.html">Jerry Bonnell</a> (<a href="http://www.astro.umd.edu/">UMCP</a>)<br /><b>NASA Official: </b>Phillip Newman <a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply">Specific rights apply</a>.<br /><a href="http://www.nasa.gov/about/highlights/HP_Privacy.html">NASA Web Privacy Policy and Important Notices</a><br /><b>A service of:</b> <a href="http://astrophysics.gsfc.nasa.gov/">ASD</a> at <a href="http://www.nasa.gov/">NASA</a> / <a href="http://www.nasa.gov/centers/goddard/">GSFC</a><br /><b>&</b> <a href="http://www.mtu.edu/">Michigan Tech. U.</a></span></center>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NA CONSTELAÇÃO DE ERIDANUS, O RIO ERIDANO:</b><o:p></o:p></span></div>
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<span style="line-height: 21.59375px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Searching for all objects in Eridanus.</span></span></div>
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<tr><td colspan="5" height="36" valign="bottom"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Eridanus: Visible in July before dawn, to March after dusk, best in November.</span></td></tr>
<tr><td class="starName" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=2.971&declination=-40.304&viewAngle=25"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Acamar</span></a></td><td class="starGreek" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">θ2</span></td><td class="starGreek" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Theta 2</span></td><td class="description" style="padding-left: 5px; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">´end of the river´ (before Achernar was added)</span></td><td class="starName" style="padding-left: 5px; padding-right: 5px;"><a href="http://www.astro.uiuc.edu/~jkaler/sow/acamar.html" target="starnotes" title="Jim Kaler´s star notes for Acamar"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Jim Kaler Notes</span></a></td></tr>
<tr><td class="starName" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=1.629&declination=-57.237&viewAngle=25"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Achernar</span></a></td><td class="starGreek" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">α</span></td><td class="starGreek" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Alpha</span></td><td class="description" style="padding-left: 5px; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">´end of the river´</span></td><td class="starName" style="padding-left: 5px; padding-right: 5px;"><a href="http://www.astro.uiuc.edu/~jkaler/sow/achernar.html" target="starnotes" title="Jim Kaler´s star notes for Achernar"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Jim Kaler Notes</span></a></td></tr>
<tr><td class="starName" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=2.940&declination=-8.898&viewAngle=25"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Azha</span></a></td><td class="starGreek" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">η</span></td><td class="starGreek" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Eta</span></td><td class="description" style="padding-left: 5px; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">´hatching place´</span></td><td class="starName" style="padding-left: 5px; padding-right: 5px;"><a href="http://www.astro.uiuc.edu/~jkaler/sow/azha.html" target="starnotes" title="Jim Kaler´s star notes for Azha"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Jim Kaler Notes</span></a></td></tr>
<tr><td class="starName" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=5.131&declination=-5.086&viewAngle=25"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Cursa</span></a></td><td class="starGreek" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">β</span></td><td class="starGreek" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Beta</span></td><td class="description" style="padding-left: 5px; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">´chair/footstool of Orion´</span></td><td class="starName" style="padding-left: 5px; padding-right: 5px;"><a href="http://www.astro.uiuc.edu/~jkaler/sow/cursa.html" target="starnotes" title="Jim Kaler´s star notes for Cursa"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Jim Kaler Notes</span></a></td></tr>
<tr><td class="starName" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=3.721&declination=-9.763&viewAngle=25"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Rana</span></a></td><td class="starGreek" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">δ</span></td><td class="starGreek" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Delta</span></td><td class="description" style="padding-left: 5px; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">´frog´</span></td><td class="starName" style="padding-left: 5px; padding-right: 5px;"><a href="http://www.astro.uiuc.edu/~jkaler/sow/rana.html" target="starnotes" title="Jim Kaler´s star notes for Rana"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Jim Kaler Notes</span></a></td></tr>
<tr><td class="starName" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=3.967&declination=-13.509&viewAngle=25"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Zaurak</span></a></td><td class="starGreek" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">γ</span></td><td class="starGreek" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Gamma</span></td><td class="description" style="padding-left: 5px; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">´boat´</span></td></tr>
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<tr><td colspan="5" height="36" valign="bottom"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Eridanus: Visible in August before dawn, to April after dusk, best in December.</span></td></tr>
<tr><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; vertical-align: top;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=4.2383&declination=-12.7383&viewAngle=20.0"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Cleopatra´s Eye</span></a></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="150"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">NGC1535</span></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">04h 14.3m</span></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">-12° 44.3´</span></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="300"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">(Alicia Tristan)</span></td></tr>
<tr><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; vertical-align: top;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=4.4133&declination=-21.1833&viewAngle=20.0"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Eridanus Globular Cluster</span></a></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="150"></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">04h 24.8m</span></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">-21° 11.0´</span></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="300"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">(Sky Catalogue 2000.0)</span></td></tr>
<tr><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; vertical-align: top;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=3.4067&declination=-21.5433&viewAngle=20.0"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Holmberg VI</span></a></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="150"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">NGC1325A</span></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">03h 24.4m</span></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">-21° 32.6´</span></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="300"></td></tr>
<tr><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; vertical-align: top;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=3.9867&declination=-21.3333&viewAngle=20.0"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Horologium Dwarf</span></a></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="150"></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">03h 59.2m</span></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">-21° 20.0´</span></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="300"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">also Schuster´s Spiral</span></td></tr>
<tr><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; vertical-align: top;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=3.9867&declination=-21.3333&viewAngle=20.0"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Schuster´s Spiral</span></a></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="150"></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">03h 59.2m</span></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">-21° 20.0´</span></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="300"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">also Horologium Dwarf</span></td></tr>
<tr><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; vertical-align: top;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=5.115&declination=-7.2167&viewAngle=20.0"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Witch Head Nebula</span></a></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="150"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">IC2118</span></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">05h 06.9m</span></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">-07° 13.0´<br /><br /><a href="http://www.nightskyatlas.com/dsoNames.jsp">http://www.nightskyatlas.com/dsoNames.jsp</a></span><br />
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<b><span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Principal Stars of Eridanus - The Night Sky Atlas<o:p></o:p></span></span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a href="http://www.nightskyatlas.com/stardata.jsp?id=ERI"><span lang="EN-US">http://www.nightskyatlas.com/stardata.jsp?id=ERI</span></a><o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Multiple Stars of Eridanus - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">NGC Objects in Eridanus - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">IC Objects in Eridanus - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Abell Galaxy Clusters - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a href="http://www.nightskyatlas.com/catAbell.jsp"><span lang="EN-US">http://www.nightskyatlas.com/catAbell.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="https://www.raremaps.com/gallery/detail/31524op/_Eridanus_Stars_Heightened_in_Gold/Bayer.html">https://www.raremaps.com/gallery/detail/31524op/_Eridanus_Stars_Heightened_in_Gold/</a><a href="https://www.raremaps.com/gallery/detail/31524op/_Eridanus_Stars_Heightened_in_Gold/Bayer.html">Bayer.html</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong style="color: #fff2cc; text-align: start;">Map Maker: </strong><span style="color: #fff2cc; text-align: start;"></span><a href="https://www.raremaps.com/gallery/browse/creator_id/247" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-align: start; text-decoration: none;">Johann Bayer</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas – As Constelações - são como janelas que se abrem para a infinitude do universo e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e sendo por nossa mente conscientizado. Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">COM UM ABRAÇO ESTRELADO,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>REFERÊNCIAS BIBLIOGRÁFICAS impressas:</b><o:p></o:p></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">COMPILAÇÃO E TRADUÇÃO literal (quando necessária) de Janine Milward:<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As Cartas Celestes foram realizadas por Mario Jaci Monteiro e escaneadas por Janine<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- </span><b>Mario Jaci Monteiro</b> , <b>As Constelações, Cartas Celestes</b> -<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- <b>Wil Tirion - Atlas of the Night Sky</b> - The Hamlyn Publishing Group Limited, London, England</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- <b>Antonin Rükl - The Hamlyn Encyclopedia of Stars & Planets</b> - The Hamlyn Publishng Group Limited, London, England</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- <b>Richard Hinckley Allen, Star Names, Their Lore and Meaning</b>, Dover Publications, Inc, New York, USA</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- <b>Bernard Pellequer - Pequeno Guia do Céu</b> - Editora Martins Fontes, São Paulo, Brasil</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- <b>Identificação do Céu</b> (Livro que foi sendo revisado e reeditado algumas vezes) de autoria de <b>Fernando Vieira</b>,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Secretaria Municipal de Cultura, Fundação Planetário da Cidade do Rio de Janeiro<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(com dedicatória do próprio autor para mim em Curso de Identificação do Céu,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em 30/07/1999))<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do <b>Atlas Celeste</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">de autoria de <b>Ronaldo Rogério de Freitas Mourão</b>,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(com dedicatória do próprio autor para mim<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em evento realizado no Museu de Astronomia do Rio de Janeiro,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em 16/06/1989)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As Cartas Celestes foram realizadas por Mario Jaci Monteiro e escaneadas por Janine<span lang="PT"><br /></span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- </span><b>Mario Jaci Monteiro</b> , <b>As Constelações, Cartas Celestes</b> -<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC - com dedicatória do autor para mim, em março de 2004 (quando Mário Jaci generosamente me presenteou com um instrumento de observação (kepleriano) artesanalmente construído por ele).<o:p></o:p></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-4158372707710982464.post-65793518569821705852013-11-30T07:13:00.005-08:002015-04-08T09:45:20.223-07:00Eridanus - o texto completo<br />
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<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="line-height: normal; text-align: left; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Da Terra ao Céu ....</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">.....<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="text-decoration: none;">e ao Infinito </a></span></h1>
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<a href="http://daterraaoceueaoinfinito.blogspot.com.br/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://daterraaoceueaoinfinito.blogspot.com.br/</span></a></div>
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Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo<o:p></o:p></div>
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e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;<o:p></o:p></div>
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bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.<o:p></o:p></div>
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<span style="line-height: 14.25pt;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span></div>
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Com um abraço estrelado,</div>
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Janine Milward<o:p></o:p></div>
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<b><span style="font-size: large;">Eridanus</span></b><o:p></o:p></div>
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<a href="http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_025.jpg">http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_025.jpg</a></div>
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<a href="https://www.raremaps.com/gallery/detail/31524op/_Eridanus_Stars_Heightened_in_Gold/Bayer.html">https://www.raremaps.com/gallery/detail/31524op/_Eridanus_Stars_Heightened_in_Gold/Bayer.html</a><br />
<strong style="line-height: normal;">Map Maker: </strong><span style="line-height: normal;"></span><a href="https://www.raremaps.com/gallery/browse/creator_id/247" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; line-height: normal; text-decoration: none;">Johann Bayer</a><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhYRsE8Wb9pPbf_yvTFKzhWJfDJfzClJcaMKd9myi1C_XiDTeCONnqhUxI6n8WPm58PNF3tKNunmCzamBFQKedeol_b1jCpJFfJtmcWnblbjGQB2JAuYogmYGObHg7q8OchGDHNiV_VWXm0/s1600/johan+bayer+colorido.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhYRsE8Wb9pPbf_yvTFKzhWJfDJfzClJcaMKd9myi1C_XiDTeCONnqhUxI6n8WPm58PNF3tKNunmCzamBFQKedeol_b1jCpJFfJtmcWnblbjGQB2JAuYogmYGObHg7q8OchGDHNiV_VWXm0/s640/johan+bayer+colorido.jpg" height="462" width="640" /></a></div>
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<a href="http://www.aradergalleries.com/detail.php?id=3658">http://www.aradergalleries.com/detail.php?id=3658</a></div>
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<b style="line-height: 14.25pt;"><i>A selection of hand-colored engravings from Uranometria</i></b></div>
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<span style="line-height: 14.25pt;">Published: Ausburg 1603</span></div>
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<b><span lang="PT" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Da Terra ao Céu<o:p></o:p></span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="PT"> e ao Infinito</span></b><o:p></o:p></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelações, Estrelas e Objetos Celestes<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><span lang="PT">Janine Milward</span></i><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado. Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(tais como Ascensão Reta e Declinação, em muitos dos casos)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Mario Jaci Monteiro - Cartas Celestes, as 88 Constelações</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; line-height: 11px;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; line-height: 11px;"> - excerto apresentando ALFABETO GREGO, CONVENÇÕES E USO DA CARTA CELESTE</span><br />
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><a href="http://www.raremaps.com/gallery/detail/29167/Orion_and_Haase_Lepus_the_Rabbit/Bode.html"><span style="font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/detail/29167/Orion_and_Haase_Lepus_the_Rabbit/Bode.html</span></a></span></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Title: </strong>Orion and Haase (Lepus the Rabbit)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1098" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">Johann Ehlert Bode</a></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;"><span lang="EN-US"> </span>ERIDANUS, O RIO ERIDANO</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Posicionamento:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 1h22m / 5h9m Declinação +0<sup>o</sup>.1 / -58<sup>o</sup>.1<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Mito:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação representa o Rio Padus ou onde Phaeton caiu quando degolado por Júpiter por causa de ter botado fogo no mundo ao mal-guiar o carro de seu pai, Phoebus.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Erídano é supostamente uma representação de equivalência celestial de um rio; é o Nilo para os Egípcios, e o Eufrates para os Babilônios.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Acessando<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> <a href="http://www.constellationsofwords.com/Constellations/Eridanus.html">http://www.constellationsofwords.com/Constellations/Eridanus.html</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">você encontrará<span class="apple-converted-space"> </span>Informações bem interessantes<span class="apple-converted-space"> </span>sobre o significado da nomeação Eridanus, suas principais Estrelas e excertos do texto de Richard H. Allen contando a História desta Constelação.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Fronteiras:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Eridanus faz fronteira com Horologium, Caelum, Lepus, Orion, Taurus, Cetus, Fornax, Pheonix e Hydra</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">MEUS (Janine) COMENTÁRIOS SOBRE O RIO ERIDANUS</b></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Eridanus" src="http://www.lindahall.org/services/digital/ebooks/bayer/bigpix/040036bc.jpg" height="486" width="640" /></span></div>
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<a href="http://www.lindahall.org/services/digital/ebooks/bayer/bayer84.shtml"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.lindahall.org/services/digital/ebooks/bayer/bayer84.shtml</span></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://carlosnieto.com/empresas/lecturatarot/blog/constelacion-de-eridanus/" style="background-color: white;">http://carlosnieto.com/empresas/lecturatarot/blog/constelacion-de-eridanus/</a></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">O RIO ERIDANUS NASCE BEM AOS PÉS - estrela-beta Orionis, Rigel - DO GIGANTE CAÇADOR ÓRION.</b></span></div>
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<b style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A estrela-beta Eridanii, Cursa, aponta para este lugar de nascimento do Rio dos Céus Estrelados.</span></b></div>
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<a href="http://www.lindahall.org/services/digital/ebooks/reissig/reissig81.shtml"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.lindahall.org/services/digital/ebooks/reissig/reissig81.shtml</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">Houve um tempo quando o final do Rio Eridanus era marcado pela estrela-teta Eridanii, Acamar.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">No entanto, este Rio ganhou mais terras, foi alongado, até a representante de sua Foz, a estrela-alpha Eridanii, Achernar!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">Nosso Rio Eridanus brasileiro bem pode ser representado como o Rio Amazonas, não é mesmo?</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">O alongamento do Rio Eridanus faz muito sentido, a partir do ponto de vista de que a belíssima Achernar, a Foz do Rio dos Céus Estrelados, vem anunciar a chegada de Argo Navis, o Navio!</span></div>
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<a href="http://carlosnieto.com/empresas/lecturatarot/blog/constelacion-de-eridanus/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://carlosnieto.com/empresas/lecturatarot/blog/constelacion-de-eridanus/</span></a></div>
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<span style="border: 0px; margin: 0px; padding: 0px; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Constelación Argo Navis, G. Mercator, año, 1.551</span></span></h3>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhxBYC8cRamzkfIBUxcdU0dfhqzIY7g_CdOfH_NMDRWpiDGOY-m7gLnFONjVVqavUyhSg3oDMgcpHzxfUlr8NHrD5pprN_hI_uJTbebcCOAp2rt_Xz9eMAzChxJOUcRuQx2FqDNhiqfkeBE/s1600/stellarium.JPG" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhxBYC8cRamzkfIBUxcdU0dfhqzIY7g_CdOfH_NMDRWpiDGOY-m7gLnFONjVVqavUyhSg3oDMgcpHzxfUlr8NHrD5pprN_hI_uJTbebcCOAp2rt_Xz9eMAzChxJOUcRuQx2FqDNhiqfkeBE/s640/stellarium.JPG" height="426" width="640" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Programa Stellarium</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; margin-left: 1em; margin-right: 1em;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhK4KKdbLAJBV6d_OyLa2AQ8wP9qH_rEaF-Ct8VOouoaCR1fdFiqal5537LBM-lLteQwWh46WdDJKV-GJEO9IUuDJojFSElNvI1ygIKWOXtCg7d2kf1btBBxAjgjkXc0ZYCT1NSGnss2tBJ/s1600/novo-2.jpgstellariu+2.jpg" imageanchor="1" style="background-color: white; margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhK4KKdbLAJBV6d_OyLa2AQ8wP9qH_rEaF-Ct8VOouoaCR1fdFiqal5537LBM-lLteQwWh46WdDJKV-GJEO9IUuDJojFSElNvI1ygIKWOXtCg7d2kf1btBBxAjgjkXc0ZYCT1NSGnss2tBJ/s640/novo-2.jpgstellariu+2.jpg" height="360" width="640" /></a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Programa Stellarium</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 18px;">QUANDO ACHERNAR APONTA NO HORIZONTE SUDESTE</b><span style="line-height: 18px;">, e</span><span style="line-height: 18px;">u gosto de estar jantando (ou tomando meu desjejum!) - e minha sala-de-refeições é como uma varanda aberta para o Sítio das Estrelas e para o céu estrelado.</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">Uma estrela pisca me chamando: é Achernar! Ei-la que surge majestosa, iluminando os céus bem ao sul, apontando para o Rio Eridano, sinuosamente enredilhando-se pelas terras desde os pés do Gigante Caçador até desaguar suas águas através esta maravilha que vem anunciando a chegada do mar!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">É realmente muito agradável termos uma bela visão dos céus bem mais ao sul - apesar de que, confesso, a multidão de pequenas constelações ainda me confunde, ainda não sei bem delinear muitas delas, deixo-me envolver por um certo tom de caos..., talvez parecido com o inicial caos que teria advindo aos observadores dos céus, há alguns poucos séculos, quando aproveitaram as caravelas arrojadas e desbravadoras de novos mares nunca dantes navegados (e também os navios a vapor) para conhecerem as estrelas buscando o sul... </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px;"><span style="background-color: white; color: #073763;">Penso que o sul traz um tom de fantasia, de imaginação solta, de paraíso na Terra, algo assim - e também de desejo e de concretização de ideais e de situações agradáveis, confortantes ao coração. Quer dizer, as constelações bem mais ao sul que foram sendo figuradas, delineadas e nomeadas, expressam, de alguma forma, estas questões. </span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px;"><span style="background-color: white; color: #073763;">Uma questão bastante fundamental é o fato de que para bem podermos conhecer os céus estrelados mais ao sul, é preciso que estejamos em lugares de céus escuros e transparentes e, preferencialmente, em noites sem-Lua.</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px;"><span style="background-color: white; color: #073763;">(De uma maneira geral, as pessoas se mostram surpresas quando eu digo que o melhor momento para o observador de estrelas acontece quando Selene está ausente - nem que seja por algumas horas, em tempos de Lua de Nova a Crescente ou de Lua Minguante a Nova!).</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px;"><span style="background-color: white; color: #073763;">No caso do Rio Eridanus, eu somente consigo delineá-lo nos céus estrelados quando a noite é escura, bem escura - pois que as estrelas que compõem a sinuosidade maravilhosa apresentada por esta constelação são luzes não muito iluminadas - com a fantástica exceção da estrela-alpha Eridanii, Achernar!</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando Achernar entra em cena no horizonte sudeste, o céu vem apresentando situações muitíssimo interessantes: </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Escorpião apronta-se para deitar-se no horizonte oeste e isto significa que o Gigante Órion já tem toda a intenção de apresentar-se no horizonte leste! E sabemos que a estrela que marca um dos pés do Gigante Caçador, Rigel, estrela-beta Orionis, acontece exatamente no lugar onde o Rio Eridanus nasce e é marcado por sua estrela-bela Eridanii, Cursa.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">No entanto, antes mesmo de o Gigante surgir no horizonte leste e ainda contando com a presença de Escorpião rastejando pelos céus do oeste, o Rio Eridanus já se insinua através sua Foz enriquecida pela estrela-alpha Eridanii, Achernar!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Este é um momento de céu estrelado apresentando-se de maneira radiosa! </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Existe a junção entre o Escorpião e o Sagitário nos introduzindo aos caminhos que nos levam ao centro da Galáxia!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Capricórnio e Aquário também apresentam-se de maneira bem interessante quando em noites de céus escuros e transparentes e sem Lua porque sempre vejo uma "fraldinha" sendo delineada pelo Capricórnio e fico rindo e sorrindo diante das estrelinhas em zigue-zague que podemos encontrar no Aguadeiro!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É certo que também o Grande Triângulo do Norte encanta nossa visão mais ao norte, não é verdade, com as presenças das constelações da Águia, da Lira e do Cisne e esta figura triangular acontecendo através suas estrelas-alpha, respectivamente Altair, Vega e Deneb.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Muito me encanta o fato de que o Grande Quadrado formado pelo Cavalo Alado Pegasus me faz recordar que se eu olhar diretamente para o sul, irei encontrar as duas Nuvens de Magalhães sempre nos induzindo à dúvida: serão nuvens reais passeando pelo céu e tão próximas de nós.... ou serão as Nuvens que, na verdade, são galáxias atuantes em nosso chamado Grupo Local? É uma dúvida muito emocionante, eu penso.</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Programa Stellarium</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ainda existem outras questões bem importantes</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> que envolvem a entrada em cena nos céus estrelados do sul </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">da constelação do Rio Eridanus: </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Se você olhar atentamente a carta celeste,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> verá que a pequena constelação Fornax, a Fornalha,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> é quase que inteiramente envolvida </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">por uma das sinuosidades por onde o Rio Eridanus passa. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> E também, olhando um tantinho ao sul,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> você perceberá a presença da constelação Dorado, o Peixe Dourado.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esse lugar no céu - imenso espaço! -, revela Aglomerados e Voids</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> e são conhecidos como Fornax Cluster e Eridanus Cluster e Fornax e Eridanus Void. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> A bem da verdade,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> muitas das vezes o Leitor encontrará a menção da constelação Fornax</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> nomeando Aglomerado e Void </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- nem sempre o nome Eridanus estará sendo mencionado</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> (ou mesmo o nome Dorado, em alguns casos).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Porém, ainda mais importante, a meu ver, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">é o fato de que é possível que exista o maior Void já encontrado</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> exatamente na direção da constelação Eridanus.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tudo isso quer significar que </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">sempre que estivermos observando a constelação do Eridanus , </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em uma de suas curvas de Rio, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">saberemos que além, muito além de nossa visão apenas física, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">existe um mundo imenso, gigantesco, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">um mundo de galáxias aglomeradas e também um mundão de Vazio. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quer dizer, Luz e Vazio existem para ainda além do Rio.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br />Achernar busca seu lugar mais alto no céu estrelado do sul enquanto Canopus, estrela-alpha Carinae, surge no horizonte sudeste anunciando o Argo Navis, o Navio flutuando nas águas dos grandes rios ou dos mares que acolhem as águas advindas do Eridanus através sua Foz, a bela Achernar. Assim, o céu estrelado mais ao sul torna-se um lugar realmente encantador e bem iluminado por estas estrelas tão chamativas!</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br />O Escorpião já desapareceu no horizonte oeste - o que significa que o Gigante Órion pode surgir no horizonte leste e testemunhando o lugar onde o Rio Eridanus nasce: a seus pés, através a bênção de sua belíssima estrela-beta Orionis, Rigel (e o termo Rigel quer dizer pé - assim como vemos Regulus nomeando a pata do Leão; assim como vemos Rigel Kent, Rigel Centauri, nomeando a estrela-alpha do Centauro e sua importância como pertencente ao sistema estelar mais próximo a nós).</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhPY5BzLQE9mUSQFDIrwyK-xeLebpzlCAtRhxZljrQFE4GKgW4BnyZoBIWbg5wylFOvv5mF8zHKrdvIPBvcDSGZIvXI5hdzXMPNF8L9gFbOVa21dQ94CRyPnVJco9sH-ed2lx5CFLheZ0u1/s1600/stellarium+-+Navio+chegando+sendo+anunciado+por+Canopus+-+Orion+chegando+e+Escorpi%C3%A3o+indo+embora.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhPY5BzLQE9mUSQFDIrwyK-xeLebpzlCAtRhxZljrQFE4GKgW4BnyZoBIWbg5wylFOvv5mF8zHKrdvIPBvcDSGZIvXI5hdzXMPNF8L9gFbOVa21dQ94CRyPnVJco9sH-ed2lx5CFLheZ0u1/s640/stellarium+-+Navio+chegando+sendo+anunciado+por+Canopus+-+Orion+chegando+e+Escorpi%C3%A3o+indo+embora.jpg" height="372" width="640" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><br /><br />Quando Achernar alcança seu lugar mais alto nos céus estrelados do sul, acontece uma situação muitíssimo interessante: visualmente, Canopus, estrela-alpha Carinae, e Achernar, estrela-alpha Eridanii, apresentam-se num mesmo nível e enfeitam imensamente o céu sulino e cativam nosso olhar.</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br />O Gigante Órion também alcança o zênite e suas três estrelas formadoras de seu Cinturão - Alnilan, Alnitak e Mintak -, sorriem para nós como se fossem as Três Marias (porque são assim nomeadas popularmente).</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br />Existem momentos muito importantes no céu: um desses momentos é representado pelo Mito de Andromeda e Perseus. A bem da verdade, Cepheus e Cassiopeia já saíram de cena (e principalmente para mim porque estão tão ao norte que não posso alcançá-los). Pegasus também voa alhures, carregando consigo a Princesa Acorrentada. No entanto, Perseus permanece e sempre mostrando a cabeça deceoada da Medusa bem como os Peixes que nadam nos mares onde Cetus, o Monstro Marinho, a Baleia, nada com seu corpanzil feito de estrelas bem delineadas.</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br />Os mares do norte vão concluindo e dando lugar à terra firme onde o Carneiro, Aries, e o Touro pastam. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br />O outro momento fantástico é revelado pela caudalosa fumacinha branca de estrelinhas de algodão formando a Via Lactea e iluminando imensamente esta parte do céu, desde o norte até o sul!</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br />E, sem dúvida alguma, sempre a presença da estrela mais linda e mais cantada, Sirius, estrela-alpha Canis Majoris, nos faz vibrar o coração.</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><br /><br />O tempo passa, a noite vai empurrando suas estrelas sempre do leste para o oeste..., e o Gigante Órion se esconde novamente da visão do animal rastejante, o Escorpião, que começa a surgir no leste.</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br />O Rio Eridanus também desaparece, deixando as maravilhas dos céus estrelados do sul acontecerem através o Navio que mostra por inteiro e navegando placidamente, através o Centauro sempre guardando consigo nosso Cruzeiro do Sul.</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br />Os Gêmeos Castor e Pollux, sempre juntos e conversando entre si, anseiam pelo momento de se apresentarem do outro lado do mundo..., enquanto o Caranguejo ainda se insinua e nos embevece a visão de sua Colmeia de Abelhas, berço de estrelinhas-bebês em seu ventre. A Hydra é sempre um prazer de ser vista, enredilhando-se espaçosamente desde o Caranguejo até quase a Balança e carregando consigo o Sextante, a Taça e o belíssimo voo do Corvo. O garboso Leão dos céus ruge, sempre sendo seguido pela virginal Virgem que esconde mil e um segredos! </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br />Sempre em tempos de céus escuros, bem escuros e transparentes, a visão da Cabeleira de Berenice é algo absolutamente inesquecível! E, certamente, Spica, estrela-alpha Virginis, e Arcturus, estrela-alpha Bootes, rivalizam em suas luzes e nos fazem felizes.</span><br />
<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="background-color: white; color: #073763;">Algumas Estrelas </span></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="background-color: white; color: #073763;">e Alguns Objetos Interessantes, </span></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>em Rio Erídano:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Achernar</b><b>. Alpha Eridani. </b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 01h37,0 - Declinação -57<sup>o</sup> 20<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual 0,60 - Distância 118 anos-luz<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela branca situada na boca do Rio. De Al Ahir al Nahr, o Fim do Rio. A Foz do Rio Erídano.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta é uma estrela tão ao sul que não faz parte da visão dos habitantes em latitudes bem ao norte.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Cursa</b><b> - Beta Eridani</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual 2.8 Distância 80 anos-luz,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Cadeira, vocábulo oriundo da expressão árabew Al Kursiyy Al Jauzah. Esta estrela é o começo do Rio Erídano e encontra-se aos pés do Gigante Órion e sua estrela beta Rigel.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Acamar</b><b> - Teta Eridani - Estrela Dupla</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 02h57,5 - Declinação - 40<sup>o</sup> 23<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual 3,42 e 4,5 - Distância 65 anos-luz<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distância entre estrelas 8”,15<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A Lua. O Branco, nome de origem árabe que foi utilizado pela primeira vez nas Tabuas Alfonsinas. Esta estrela já representou a Foz do Rio antes de a constelação ser estendida até alcançar a verdadeira Foz, Achernar.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É um sistema triplo sendo que o membro mais brilhante é visível a olho nu como uma anã amarela, sendo que suas duas companheiras são muito pálidas, uma das quais é uma anã vermelha e a outra, uma anã branca.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Alnahar </b><b>- Delta Eridani</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Rio, nome de origem árabe.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Angetenar</b><b> - Tau Eridani</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Meandro do Rio, proveniente da expressão árabe Al Hinayat al Nahr.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Azha</b><b> - Eta Eridani</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ninho de Avestruz.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Beid ou Keid</b><b> - Omicron Eridani</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ovo, do árabe Al Bais, o ovo do ninho de avestruz. Nome árabe proveniente da expressão Al Kaid.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Theermin</b><b> - Epsilon Eridani</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os Gêmeos, nome oriundo do árabe Al Tauaman.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Zaurak</b><b> - Gamma Eridani</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Barco, oriundo do árabe Al Nair Al Zaurak, ou seja, a brilhante estrela do barco.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Hubble Observations Confirm that Planets Form from Disks Around Stars</span></h1>
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<a href="http://hubblesite.org/newscenter/archive/releases/2006/32/image/a/format/web_print/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/2006/32/image/a/format/web_print/</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold;">Credit:</span> <a href="http://www.nasa.gov/">NASA</a>, <a href="http://www.spacetelescope.org/">ESA</a>, and G. Bacon (<a href="http://www.stsci.edu/">STScI</a>)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">This is an artist's concept of a Jupiter-mass planet orbiting the nearby star Epsilon Eridani. Located 10.5 light-years away, it is the closest known exoplanet to our solar system. The planet is in an elliptical orbit that carries it as close to the star as Earth is from the Sun, and as far from the star as Jupiter is from the Sun.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Epsilon Eridandi is a young star, only 800 million years old. It is still surrounded by a disk of dust that extends 20 billion miles from the star. The disk appears as a linear sheet of reflecting dust in this view because it is seen edge-on from the planet's orbit, which is in the same plane as the dust disk.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">LEIA MAIS EM <a href="http://hubblesite.org/newscenter/archive/releases/2006/32/image/a/">http://hubblesite.org/newscenter/archive/releases/2006/32/image/a/</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold;">Credit:</span> <a href="http://www.nasa.gov/">NASA</a>, <a href="http://www.spacetelescope.org/">ESA</a>, and A. Feild (<a href="http://www.stsci.edu/">STScI</a>)</span></div>
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<a href="http://hubblesite.org/newscenter/archive/releases/2006/32/image/b/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/2006/32/image/b/</span></a></div>
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<span style="line-height: 18px;">Epsilon Eridani: Double the Rubble</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">This artist's conception shows the closest known planetary system to our own, called Epsilon Eridani. Observations from NASA's Spitzer Space Telescope show that the system hosts two asteroid belts, in addition to previously identified candidate planets and an outer comet ring.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Epsilon Eridani is located about 10 light-years away in the constellation Eridanus. It is visible in the night skies with the naked eye.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Leia mais em </span></div>
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<a href="http://www.spitzer.caltech.edu/images/1966-ssc2008-19a-Epsilon-Eridani-Double-the-Rubble"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spitzer.caltech.edu/images/1966-ssc2008-19a-Epsilon-Eridani-Double-the-Rubble</span></a></div>
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<a href="http://www.spitzer.caltech.edu/images/1962-ssc2008-19b-Young-Solar-System-in-the-Making"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spitzer.caltech.edu/images/1962-ssc2008-19b-Young-Solar-System-in-the-Making</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">This artist's diagram compares the Epsilon Eridani system to our own solar system. The two systems are structured similarly, and both host asteroids (brown), comets (blue) and planets (white dots).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Epsilon Eridani is our closest known planetary system, located about 10 light-years away in the constellation Eridanus. Its central star is a younger, fainter version of our sun, and is about 800 million years oldâabout the same age of our solar system when life first took root on Earth.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Observations from NASA's Spitzer Space Telescope show that the system hosts two asteroid belts, in addition to previously identified candidate planets and an outer comet ring.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Leia mais em <a href="http://www.spitzer.caltech.edu/images/1962-ssc2008-19b-Young-Solar-System-in-the-Making">http://www.spitzer.caltech.edu/images/1962-ssc2008-19b-Young-Solar-System-in-the-Making</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-weight: bold; text-align: -webkit-center;">Johann Bayer — Eridanus</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Eridanus" src="http://www.aradergalleries.com/maps/images/158_Bayer/br_eridanus.jpg" height="462" width="640" /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.aradergalleries.com/detail.php?id=3658" style="background-color: white;">http://www.aradergalleries.com/detail.php?id=3658</a></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiW72QdwaG_ohEmKpXvcN0KkM127kZM1I-7D6VZyv7NcOBGe4rgUnKwnO3xlQJCOIw6Fn_jkMau4wfZKTEUaKRAbIjPVaCFSkx1I_SUVEYSF3-ijWv0ObPimROUGQPJ6GcIZtvegSaTbEbu/s1600/eridanus,+fornax+e+dorado.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiW72QdwaG_ohEmKpXvcN0KkM127kZM1I-7D6VZyv7NcOBGe4rgUnKwnO3xlQJCOIw6Fn_jkMau4wfZKTEUaKRAbIjPVaCFSkx1I_SUVEYSF3-ijWv0ObPimROUGQPJ6GcIZtvegSaTbEbu/s1600/eridanus,+fornax+e+dorado.jpg" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Programa Stellarium</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">VEJA QUE A PEQUENA CONSTELAÇÃO FORNAX, A FORNALHA, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ACONTECE INSERIDA EM UMA DAS TANTAS CURVAS DO RIO ERIDANUS</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e veja que Achernar, estrela-alpha Eridanii, situa-se bem próxima ao Peixe DORADO.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Estas duas constelações vêm sendo sempre muito comentadas porquanto acolhem Aglomerados e Void, Vazio.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Na maioria das vezes, acontece a denominação Fornax Supercluster e Fornax Void porém a verdade é que na direção onde as constelações Eridanus e Fornax se encontram, Aglomerados e Vazios acontecem.</span><br />
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<a href="http://commons.wikimedia.org/wiki/File:2MASS_LSS_chart-NEW_Nasa.jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://commons.wikimedia.org/wiki/File:2MASS_LSS_chart-NEW_Nasa.jpg</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="external text" href="http://spider.ipac.caltech.edu/staff/jarrett/papers/LSS/" rel="nofollow">"Large Scale Structure in the Local Universe: The 2MASS Galaxy Catalog"</a><span style="line-height: 19.1875px;">, Jarrett, T.H. 2004, PASA, 21, 396</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 19.1875px;">Panoramic view of the entire near-infrared sky reveals the distribution of galaxies beyond the </span><a class="extiw" href="http://en.wikipedia.org/wiki/Milky_Way" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="w:Milky Way">Milky Way</a><span style="line-height: 19.1875px;">. The image is derived from the </span><a class="extiw" href="http://en.wikipedia.org/wiki/2MASS" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="w:2MASS">2MASS Extended Source Catalog (XSC)</a><span style="line-height: 19.1875px;">—more than 1.5 million galaxies, and the Point Source Catalog (PSC)--nearly 0.5 billion Milky Way stars</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">The Fornax and Eridanus Clusters</span></h1>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">The Fornax and Eridanus clusters are two verThe Fornax and Eridanus clusters are two very famous clusters in the southern hemisphere. Although they look near to each other, they are separated by about 20 million light years. The nearer Fornax cluster is about 65 million light years from us, and the Eridanus cluster is about 85 million light years from us. There are many other groups of galaxies scattered around these two clusters and collectively these groups are often called the <em>Fornax Supercluster</em> or <em>Southern Supercluster</em>.y famous clusters in the southern hemisphere. Although they look near to each other, they are separated by about 20 million light years. The nearer Fornax cluster is abo</span><span style="font-family: Arial, Helvetica, sans-serif;">ut 65 million light years from us, and the Eridanus cluster is about 85 million light years from us. </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">The Eridanus Cluster</span></h2>
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<span style="text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">This is a map of the Eridanus Cluster. This cluster is less spectacular than the Fornax cluster, partly because the galaxies are spread across a larger area and partly because the cluster is rather further and hence dimmer than the Fornax cluster. The Eridanus cluster is roughly split into two halves: a northern subgroup around NGC 1407 and a southern subgroup around NGC 1395.</span></span></div>
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<tr><th colspan="2" style="border: 1px solid rgb(0, 102, 204); text-align: center; vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Properties of the Eridanus Cluster</span></th></tr>
<tr><td style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Equatorial Coordinates</span></td><td class="center" style="border: 1px solid rgb(0, 102, 204); text-align: center; vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">RA=03h35m Dec=-22°</span></td></tr>
<tr><td style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Galactic Coordinates</span></td><td class="center" style="border: 1px solid rgb(0, 102, 204); text-align: center; vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">l=214° b=-53°</span></td></tr>
<tr><td style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Supergalactic Coordinates</span></td><td class="center" style="border: 1px solid rgb(0, 102, 204); text-align: center; vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">L=281° B=-43°</span></td></tr>
<tr><td style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distance to the centre of the cluster</span></td><td class="center" style="border: 1px solid rgb(0, 102, 204); text-align: center; vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">85 million light years</span></td></tr>
<tr><td style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Number of large galaxies in the cluster</span></td><td class="center" style="border: 1px solid rgb(0, 102, 204); text-align: center; vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">73</span></td></tr>
<tr><td style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Alternative names for the cluster</span></td><td class="center" style="border: 1px solid rgb(0, 102, 204); text-align: center; vertical-align: middle;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Fornax II cluster</span></td></tr>
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<a href="http://www.atlasoftheuniverse.com/galgrps/for.html" style="text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.atlasoftheuniverse.com/galgrps/for.htm</span></a></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="-webkit-text-stroke-width: 0px; font-family: Arial, Helvetica, sans-serif; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; text-transform: none; white-space: normal; word-spacing: 0px;"></span><br /></span></span>
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<span style="-webkit-text-stroke-width: 0px; background-color: #073763; color: #073763; font-family: Arial, Helvetica, sans-serif; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; text-transform: none; white-space: normal; word-spacing: 0px;"><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;">The center of the </span><b style="line-height: 19.1875px; text-align: start;">Eridanus Cluster</b><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;"> is roughly 23 </span><a href="http://en.wikipedia.org/wiki/Parsec#Megaparsecs_and_gigaparsecs" style="background-image: none; color: #fff2cc; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Parsec">Mpc</a><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;"> (75 </span><a href="http://en.wikipedia.org/wiki/Light-year#Distances_in_light-years" style="background-image: none; color: #fff2cc; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Light-year">Mly</a><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;">) from </span><a href="http://en.wikipedia.org/wiki/Earth" style="background-image: none; color: #fff2cc; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Earth">Earth</a><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;">, and contains about 73 main </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Galaxies" style="background-image: none; color: #fff2cc; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Galaxies">galaxies</a><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;"> and about 200 total galaxies. About 30% have </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Hubble_classification" style="background-image: none; color: #fff2cc; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Hubble classification">Hubble classifications</a><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;"> of elliptical or S0 and the remaining 70% are spiral or irregular.</span><sup class="reference" id="cite_ref-JAA-Omar_2-3" style="color: #fff2cc; line-height: 1em; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-JAA-Omar-2" style="background-image: none; text-decoration: none; white-space: nowrap;">[2]</a></sup><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;"> These galaxies reside in smaller groups which are all loosely gravitationally bound to each other, suggesting that the system is still condensing from the </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Hubble_flow" style="background-image: none; color: #fff2cc; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Hubble flow">Hubble flow</a><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;"> and may eventually form a cluster of about 10</span><sup style="color: #fff2cc; line-height: 1em; text-align: start;">14</sup><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;"> </span><a href="http://en.wikipedia.org/wiki/Solar_mass" style="background-image: none; color: #fff2cc; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Solar mass">M<sub style="line-height: 1em;">☉</sub></a><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;">. A low velocity dispersion compared to that of, for example, the Coma cluster, supports this hypothesis.</span><sup class="reference" id="cite_ref-AJ-Willmer_3-2" style="color: #fff2cc; line-height: 1em; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-AJ-Willmer-3" style="background-image: none; text-decoration: none; white-space: nowrap;">[3]</a></sup><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;"> The Eridanus Cluster is located in the </span><a href="http://en.wikipedia.org/wiki/Constellation" style="background-image: none; color: #fff2cc; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Constellation">constellation</a><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;"> </span><a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)" style="background-image: none; color: #fff2cc; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Eridanus (constellation)">Eridanus</a><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;"> near the </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Fornax_cluster" style="background-image: none; color: #fff2cc; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Fornax cluster">Fornax cluster</a><span style="color: #fff2cc; line-height: 19.1875px; text-align: start;">, and is sometimes called the "Fornax II Cluster".</span><sup class="reference" id="cite_ref-atlasoftheuniverse_4-1" style="color: #fff2cc; line-height: 1em; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-atlasoftheuniverse-4" style="background-image: none; text-decoration: none; white-space: nowrap;">[4]</a></sup></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster" style="background-color: white;">http://en.wikipedia.org/wiki/Eridanus_Cluster</a></span></div>
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<tr><th colspan="2" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; text-align: center; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Eridanus Cluster</span></th></tr>
<tr><th colspan="2" style="text-align: center; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Observation data (<a href="http://en.wikipedia.org/wiki/Epoch_(astronomy)" style="background-image: none; text-decoration: none;" title="Epoch (astronomy)">Epoch</a> <a href="http://en.wikipedia.org/wiki/Epoch_(astronomy)#Julian_years_and_J2000" style="background-image: none; text-decoration: none;" title="Epoch (astronomy)">J2000</a>)</span></th></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Constellation" style="background-image: none; text-decoration: none;" title="Constellation"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constellation(s)</span></a></th><td style="vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)" style="background-image: none; text-decoration: none;" title="Eridanus (constellation)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Eridanus</span></a></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Right_ascension" style="background-image: none; text-decoration: none;" title="Right ascension"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Right ascension</span></a></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03<sup style="line-height: 1em;">h</sup> 28<sup style="line-height: 1em;">m</sup> 13.8<sup style="line-height: 1em;">s</sup><sup class="reference" id="cite_ref-NED-Eridanus_1-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-NED-Eridanus-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Declination" style="background-image: none; text-decoration: none;" title="Declination"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Declination</span></a></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">−20° 44′ 40″<sup class="reference" id="cite_ref-NED-Eridanus_1-1" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-NED-Eridanus-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Brightest member</span></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/NGC_1232" style="background-image: none; text-decoration: none;" title="NGC 1232">NGC 1232</a> (B)</span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Number of galaxies</span></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">~200<sup class="reference" id="cite_ref-JAA-Omar_2-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-JAA-Omar-2" style="background-image: none; text-decoration: none; white-space: nowrap;">[2]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Velocity_dispersion" style="background-image: none; text-decoration: none;" title="Velocity dispersion"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Velocity dispersion</span></a></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">261 km/s<sup class="reference" id="cite_ref-AJ-Willmer_3-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-AJ-Willmer-3" style="background-image: none; text-decoration: none; white-space: nowrap;">[3]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Redshift" style="background-image: none; text-decoration: none;" title="Redshift"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Redshift</span></a></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">0.005570<sup class="reference" id="cite_ref-NED-Eridanus_1-2" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-NED-Eridanus-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distance<br />(<a class="mw-redirect" href="http://en.wikipedia.org/wiki/Co-moving_distance" style="background-image: none; text-decoration: none;" title="Co-moving distance">co-moving</a>)</span></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">23 <a href="http://en.wikipedia.org/wiki/Parsec#Megaparsecs_and_gigaparsecs" style="background-image: none; text-decoration: none;" title="Parsec">Mpc</a> (75 <a href="http://en.wikipedia.org/wiki/Light-year#Distances_in_light-years" style="background-image: none; text-decoration: none;" title="Light-year">Mly</a>)<sup class="reference" id="cite_ref-NED-Eridanus_1-3" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-NED-Eridanus-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Intracluster_medium" style="background-image: none; text-decoration: none;" title="Intracluster medium"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ICM temperature</span></a></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">~10<sup style="line-height: 1em;">7</sup> <a href="http://en.wikipedia.org/wiki/Kelvin" style="background-image: none; text-decoration: none;" title="Kelvin">K</a> (~1 <a class="mw-redirect" href="http://en.wikipedia.org/wiki/KeV" style="background-image: none; text-decoration: none;" title="KeV">keV</a>)<sup class="reference" id="cite_ref-JAA-Omar_2-1" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-JAA-Omar-2" style="background-image: none; text-decoration: none; white-space: nowrap;">[2]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Binding_energy" style="background-image: none; text-decoration: none;" title="Binding energy"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Binding mass</span></a></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">~10<sup style="line-height: 1em;">14</sup> <a href="http://en.wikipedia.org/wiki/Solar_mass" style="background-image: none; text-decoration: none;" title="Solar mass">M<sub style="line-height: 1em;">☉</sub></a><sup class="reference" id="cite_ref-AJ-Willmer_3-1" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-AJ-Willmer-3" style="background-image: none; text-decoration: none; white-space: nowrap;">[3]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Flux" style="background-image: none; text-decoration: none;" title="Flux"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">X-ray flux</span></a></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">0.105 m<a href="http://en.wikipedia.org/wiki/Crab_(unit)" style="background-image: none; text-decoration: none;" title="Crab (unit)">Crab</a><sup class="reference" id="cite_ref-JAA-Omar_2-2" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-JAA-Omar-2" style="background-image: none; text-decoration: none; white-space: nowrap;">[2]</a></sup></span></td></tr>
<tr><th colspan="2" style="text-align: center; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Other designations</span></th></tr>
<tr><td colspan="2" style="text-align: center; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Fornax II Cluster,<sup class="reference" id="cite_ref-atlasoftheuniverse_4-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-atlasoftheuniverse-4" style="background-image: none; text-decoration: none; white-space: nowrap;">[4]</a></sup> de Vaucouleurs Group 31<sup class="reference" id="cite_ref-Chincarini_1974_5-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_Cluster#cite_note-Chincarini_1974-5" style="background-image: none; text-decoration: none; white-space: nowrap;">[5</a></sup></span></td></tr>
</tbody></table>
<h2 style="-webkit-text-stroke-width: 0px; background-image: none; border-bottom-color: rgb(170, 170, 170); border-bottom-style: solid; border-bottom-width: 1px; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; margin: 0px 0px 0.6em; overflow: hidden; padding-bottom: 0.17em; padding-top: 0.5em; text-align: center; text-transform: none; white-space: normal; word-spacing: 0px;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span class="mw-headline" id="Table_of_galaxies">Table of galaxies</span><span class="mw-editsection" style="-webkit-user-select: none; display: inline-block; line-height: 1em; margin-left: 1em; padding-right: 0.25em; unicode-bidi: -webkit-isolate; vertical-align: baseline; white-space: nowrap;"><span class="mw-editsection-bracket">[</span><a href="http://en.wikipedia.org/w/index.php?title=Eridanus_Cluster&action=edit&section=1" style="background-image: none; text-decoration: none;" title="Edit section: Table of galaxies">edit</a><span class="mw-editsection-bracket">]</span></span></span></h2>
<div style="-webkit-text-stroke-width: 0px; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: 1.5em; margin-bottom: 0.5em; margin-top: 0.4em; text-transform: none; white-space: normal; word-spacing: 0px;">
</div>
<div style="text-align: center;">
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif; line-height: 1.5em;">Column 1: Name of the</span><span style="font-family: Arial, Helvetica, sans-serif; line-height: 1.5em;"> </span><a href="http://en.wikipedia.org/wiki/Galaxy" style="background-image: none; font-family: Arial, Helvetica, sans-serif; line-height: 1.5em; text-decoration: none;" title="Galaxy">galaxy</a></span></div>
<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"></span><br /></span></span>
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 1.5em;">Column 2:</span><span style="line-height: 1.5em;"> </span><a href="http://en.wikipedia.org/wiki/Right_ascension" style="background-image: none; line-height: 1.5em; text-decoration: none;" title="Right ascension">Right ascension</a><span style="line-height: 1.5em;"> </span><span style="line-height: 1.5em;">for</span><span style="line-height: 1.5em;"> </span><a href="http://en.wikipedia.org/wiki/Epoch_(astronomy)#Julian_years_and_J2000" style="background-image: none; line-height: 1.5em; text-decoration: none;" title="Epoch (astronomy)">epoch J2000</a></span></div>
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"></span></span><br />
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 1.5em;">Column 3:</span><span style="line-height: 1.5em;"> </span><a href="http://en.wikipedia.org/wiki/Declination" style="background-image: none; line-height: 1.5em; text-decoration: none;" title="Declination">Declination</a><span style="line-height: 1.5em;"> </span><span style="line-height: 1.5em;">for epoch J2000</span></span></div>
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"></span></span><br />
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 1.5em;">Column 4: Blue</span><span style="line-height: 1.5em;"> </span><a href="http://en.wikipedia.org/wiki/Apparent_magnitude" style="background-image: none; line-height: 1.5em; text-decoration: none;" title="Apparent magnitude">apparent magnitude</a><span style="line-height: 1.5em;"> </span><span style="line-height: 1.5em;">of the galaxy</span></span></div>
<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"></span></span></span><br />
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 1.5em;">Column 5:</span><span style="line-height: 1.5em;"> </span><a href="http://en.wikipedia.org/wiki/Hubble_sequence" style="background-image: none; line-height: 1.5em; text-decoration: none;" title="Hubble sequence">Galaxy type</a><span style="line-height: 1.5em;">: E=Elliptical; S0=Lenticular; Sa, Sb, Sc, Sd=Spiral; SBa, SBb, SBc, SBd=Barred Spiral; Sm, SBm, Irr=Irregular</span></span></div>
<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"></span></span></span><br />
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 1.5em;">Column 6: Angular diameter of the galaxy (</span><a href="http://en.wikipedia.org/wiki/Minute_of_arc" style="background-image: none; line-height: 1.5em; text-decoration: none;" title="Minute of arc">arcminutes</a><span style="line-height: 1.5em;">)</span></span></div>
<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"></span></span></span><br />
<div style="text-align: center;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; line-height: 1.5em;">Column 7: Diameter of the galaxy (thousands of light years)</span></span></div>
<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"></span></span></span><br />
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 1.5em;">Column 8: Recessional velocity (km/s) of the galaxy relative to the</span><span style="line-height: 1.5em;"> </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Cosmic_microwave_background_radiation" style="background-image: none; line-height: 1.5em; text-decoration: none;" title="Cosmic microwave background radiation">cosmic microwave background</a></span></div>
<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"></span><span style="font-family: Arial, Helvetica, sans-serif;"></span><br /></span></span>
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"></span></span><br />
<table class="wikitable sortable jquery-tablesorter" style="-webkit-text-stroke-width: 0px; border-collapse: collapse; border: 1px solid rgb(170, 170, 170); font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; margin: 1em 60px 1em 0px; text-align: center; text-transform: none; white-space: normal; word-spacing: 0px;"><thead style="line-height: 19.1875px;"></thead><tbody style="line-height: 19.1875px;">
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: left;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Name</span></b></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: left;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Right_Ascension" style="background-image: none; text-decoration: none;" title="Right Ascension">RA</a> <a href="http://en.wikipedia.org/wiki/Equatorial_coordinate_system" style="background-image: none; text-decoration: none;" title="Equatorial coordinate system">equatorial<br />coordinates</a></span></b></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: left;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Declination" style="background-image: none; text-decoration: none;" title="Declination">Dec</a> equatorial<br />coordinates</span></b></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: left;"><b><a href="http://en.wikipedia.org/wiki/Photographic_magnitude" style="background-image: none; text-decoration: none;" title="Photographic magnitude"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Blue<br />Mag</span></a></b></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: left;"><b><a href="http://en.wikipedia.org/wiki/Hubble_sequence" style="background-image: none; text-decoration: none;" title="Hubble sequence"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Type</span></a></b></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Size<br />(arcmin)</span></b></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Size<br />(kly)</span></b></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">RV<br />(km/s)</span></b></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_547-09&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 547-09 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 547-09</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 06.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 23</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">16.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Irr</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1509</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_547-12&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 547-12 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 547-12</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 09.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-17 50</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">16.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Scd</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1837</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://en.wikipedia.org/wiki/NGC_1232" style="background-image: none; text-decoration: none;" title="NGC 1232"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1232</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 09.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-20 35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">10.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">6.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">170</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1517</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=IC_1898&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="IC 1898 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">IC 1898</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 10.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-22 24</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">3.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">85</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1164</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_547-20&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 547-20 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 547-20</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 13.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-17 56</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">16.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBm</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1825</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1258&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1258 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1258</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 14.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 46</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1340</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1297&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1297 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1297</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 19.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 06</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">50</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1395</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://en.wikipedia.org/wiki/NGC_1300" style="background-image: none; text-decoration: none;" title="NGC 1300"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1300</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 19.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 25</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">11.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBbc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">6.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">150</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1421</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1315&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1315 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1315</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 23.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 23</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1534</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=PGC_12680&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="PGC 12680 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">PGC 12680</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 23.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 17</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> ?</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Irr</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1400</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-05&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-05 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-05</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 23.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 45</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBm</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1690</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1325&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1325 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1325</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 24.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 33</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">12.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBbc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">4.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">115</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1446</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1325A&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1325A (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1325A</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 24.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 20</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBcd</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">45</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1188</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-16&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-16 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-16</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 26.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 20</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Scd</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">40</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1977</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1332&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1332 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1332</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 26.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 20</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">11.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">4.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">105</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1383</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-21&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-21 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-21</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 27.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 14</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBd</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">50</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1541</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-25&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-25 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-25</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 29.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-22 09</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBa</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1542</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1345&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1345 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1345</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 29.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-17 47</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1385</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_481-30&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 481-30 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 481-30</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 29.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-23 21</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Scd</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1504</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1347&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1347 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1347</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 29.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-22 17</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1624</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-28&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-28 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-28</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 30.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-17 56</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1360</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-29&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-29 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-29</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 30.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 03</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBbc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1175</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1353&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1353 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1353</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 32.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-20 49</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">12.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBb</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">3.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">85</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1390</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-32&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-32 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-32</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 32.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-17 43</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBm</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">40</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1815</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-33&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-33 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-33</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 32.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18 57</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1552</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-34&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-34 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-34</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 33.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 05</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1610</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_482-05&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 482-05 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 482-05</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 33.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-24 08</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBcd</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">50</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1783</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=IC_1952&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="IC 1952 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">IC 1952</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 33.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-23 43</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBbc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">60</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1683</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=IC_1953&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="IC 1953 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">IC 1953</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 33.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 29</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">12.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">65</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1733</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1359&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1359 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1359</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 33.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 29</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBm</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">55</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1833</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1362&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1362 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1362</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 33.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-20 17</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1085</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-44&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-44 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-44</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 34.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 25</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1561</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-47&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-47 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-47</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 34.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 02</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">60</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1472</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1371&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1371 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1371</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 35.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-24 56</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">11.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBa</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">5.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">140</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1344</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1370&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1370 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1370</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 35.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-20 22</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">933</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=IC_1962&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="IC 1962 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">IC 1962</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 35.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 18</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBd</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">60</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1670</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_482-11&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 482-11 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 482-11</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 36.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-25 36</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sbc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1469</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1377&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1377 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1377</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 36.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-20 54</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">45</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1645</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1385&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1385 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1385</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 37.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-24 30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">11.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">3.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">90</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1373</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1383&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1383 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1383</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 37.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18 20</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">40</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1828</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_482-17&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 482-17 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 482-17</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 37.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-22 55</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sab</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1330</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1390&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1390 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1390</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 37.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 00</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBa</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1078</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1395&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1395 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1395</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 38.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-23 02</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">10.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">5.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">140</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1577</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1398&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1398 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1398</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 38.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-26 20</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">10.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBab</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">7.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">175</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1289</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1403&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1403 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1403</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 39.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-22 23</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1751</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1401&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1401 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1401</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 39.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-22 43</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">50</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1406</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1400&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1400 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1400</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 39.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18 41</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">12.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">60</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">415</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-63&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-63 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-63</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 39.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-20 01</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sbc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1846</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-65&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-65 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-65</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 40.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 22</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sa</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1102</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=IC_343&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="IC 343 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">IC 343</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 40.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18 27</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1730</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1407&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1407 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1407</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 40.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18 35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">10.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">5.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">125</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1650</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-68&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-68 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-68</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 40.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18 56</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1636</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1412&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1412 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1412</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 40.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-26 52</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">35</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1675</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-70&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-70 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-70</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 40.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-22 17</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBcd</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">40</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1615</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_482-32&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 482-32 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 482-32</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 40.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-26 47</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Irr</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1621</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1415&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1415 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1415</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 40.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-22 34</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">12.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sa</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">3.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">80</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1451</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1414&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1414 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1414</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 41.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 43</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBbc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">40</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1464</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_482-35&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 482-35 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 482-35</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 41.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-23 50</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBab</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">45</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1756</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1422&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1422 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1422</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 41.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 41</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBab</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">55</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1514</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=IC_346&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="IC 346 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">IC 346</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 41.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18 16</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">45</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1830</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-79&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-79 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-79</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 41.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18 54</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sa</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1914</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_548-82&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 548-82 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 548-82</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 42.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-17 30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sbc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1590</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1426&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1426 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1426</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 42.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-22 06</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">12.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">60</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1296</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_549-02&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 549-02 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 549-02</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 43.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-19 01</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBm</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">988</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_549-06&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 549-06 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 549-06</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 43.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 14</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Irr</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1490</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1439&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1439 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1439</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 44.8</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 55</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">12.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">65</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1577</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1440&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1440 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1440</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 45.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18 16</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">12.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">55</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1403</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1438&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1438 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1438</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 45.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-23 00</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBa</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">50</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1438</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1452&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1452 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1452</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 45.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18 38</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">12.9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sa</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">60</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1619</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_549-18&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 549-18 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 549-18</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 48.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21 28</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SBc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">60</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1473</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_482-46&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 482-46 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 482-46</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 49.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-27 00</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.7</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">3.5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">90</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1422</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=ESO_482-49&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="ESO 482-49 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO 482-49</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 52.4</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-23 03</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1.1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1377</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_1482&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="NGC 1482 (page does not exist)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1482</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">03 54.6</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-20 30</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13.3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2.2</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">55</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1753</span></td></tr>
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<a href="http://en.wikipedia.org/wiki/Eridanus_Cluster"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://en.wikipedia.org/wiki/Eridanus_Cluster</span></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">http://www.whillyard.com. </b></span></div>
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<a href="http://www.whillyard.com/science-pages/clustering.html"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.whillyard.com/science-pages/clustering.html</span></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">Fornax Cluster & </b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">Eridanus Group</b></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><b>The Fornax Cluster</b></span><span style="font-family: Arial, Helvetica, sans-serif;"> is a small cluster of about 58 galaxies, much smaller than the Virgo Cluster, for example, located around 20 Mpc away. It contains two massive galaxies - NGC 1316, a lenticular, and NGC 1365, a barred spiral. Both are more than twice the diameter of the Milky Way. There is substantial evidence that one, or maybe two, sub-groups of galaxies have collided with the main group in the astronomically recent past. </span><span style="font-family: Arial, Helvetica, sans-serif;"><b> Associated with the Fornax Cluster, the Eridanus Group</b></span><span style="font-family: Arial, Helvetica, sans-serif;"> lies about 7 Mpc further away. It contains around 200 galaxies, is approximately 10 Mpc across, and about 23 Mpc away. </span><span style="font-family: Arial, Helvetica, sans-serif;">This grouping is in the early stages of formation, and with the Fornax cluster, the Dorado group and others, forms the <b>Eridanus-Fornax-Dorado Filament</b>.</span><span style="font-family: Arial, Helvetica, sans-serif;"> It is very interesting because although many of its constituent galaxies are quite old, the group itself is rather young and still forming. It also has a large number of lenticular (type S0) galaxies. These are believed to be part of the evolution of spiral galaxies again implying great age for many of the galaxies. </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">LEIA MAIS EM</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.whillyard.com/science-pages/clustering.html" style="background-color: white;">http://www.whillyard.com/science-pages/clustering.html</a></span></div>
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<a href="http://cseligman.com/text/atlas/ngc14.htm#1417"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://cseligman.com/text/atlas/ngc14.htm#1417</span></a></div>
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<a href="http://www.blogger.com/blogger.g?blogID=4158372707710982464" name="1417" style="font-family: Arial, Helvetica, sans-serif;"><big><b><span style="background-color: white; color: #073763;">NGC 1417 (= PGC 13584)</span></b></big></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.blogger.com/blogger.g?blogID=4158372707710982464" name="1417">Discovered (Oct 5, 1785) by </a><a href="http://cseligman.com/text/atlas/discoverers.htm#fwherschel">William Herschel</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763;">A 12th-magnitude spiral galaxy (type SAB(rs)b) in <a href="http://cseligman.com/text/atlas/eridanus.htm#1417">Eridanus</a> (RA 03 41 57.2, Dec -04 42 19)</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apparent size 2.3 by 1.2 arcmin.</span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjPucQMzTL9wMAKJQVtcetW2YSc4uy7y3o_bVjR_bgITujIaIeAlUGWjB0pE1Ekh2F-EQBPFklnLhHw0Hnycu6RCV8VVn4ogl7IjW8MyO01U4Ckp7LhdWAA0czqjsOt8btyTmf7R527PYnJ/s1600/ngc1417.jpg" imageanchor="1" style="background-color: white; margin-left: 1em; margin-right: 1em;"><span style="color: #073763;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjPucQMzTL9wMAKJQVtcetW2YSc4uy7y3o_bVjR_bgITujIaIeAlUGWjB0pE1Ekh2F-EQBPFklnLhHw0Hnycu6RCV8VVn4ogl7IjW8MyO01U4Ckp7LhdWAA0czqjsOt8btyTmf7R527PYnJ/s1600/ngc1417.jpg" height="400" width="400" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Above, a 2.4 arcmin wide closeup of NGC 1417</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Below, a 12 arcmin wide region centered on the galaxy, also showing <a href="http://cseligman.com/text/atlas/ngc14.htm#1418">NGC 1418</a></span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg8FVcW9C4DUlgUld6GuebqIwzzsUyZO584ldeRM-d_KzOV6_rMC1WEQ604DxvRwcBQgX_qP9P1NDwJDyAzFuCoimpy9x3zPnP-r2N7TJmMdaBkhtHdySqxifHzVpdrwDuZgrd0aP6aUWCn/s1600/ngc1417wide.jpg" imageanchor="1" style="background-color: white; margin-left: 1em; margin-right: 1em;"><span style="color: #073763;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg8FVcW9C4DUlgUld6GuebqIwzzsUyZO584ldeRM-d_KzOV6_rMC1WEQ604DxvRwcBQgX_qP9P1NDwJDyAzFuCoimpy9x3zPnP-r2N7TJmMdaBkhtHdySqxifHzVpdrwDuZgrd0aP6aUWCn/s1600/ngc1417wide.jpg" height="400" width="400" /></span></a></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.blogger.com/blogger.g?blogID=4158372707710982464" name="1418"></a></span></span></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.blogger.com/blogger.g?blogID=4158372707710982464" name="1418"></a><a href="http://cseligman.com/text/atlas/ngc14.htm#1417">http://cseligman.com/text/atlas/ngc14.htm#1417</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">NGC 1232</b><span style="color: black; line-height: 19.1875px; text-align: start;"> </span><span style="line-height: 19.1875px; text-align: start;">é uma </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a><span style="line-height: 19.1875px; text-align: start;"> localizada a cerca de setenta e dois milhões de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="line-height: 19.1875px; text-align: start;"> (aproximadamente 22,07</span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Megaparsec" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Megaparsec">megaparsecs</a><span style="line-height: 19.1875px; text-align: start;">) de distância na direção da </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o_de_Er%C3%ADdano" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Constelação de Erídano">constelação de Erídano</a><span style="line-height: 19.1875px; text-align: start;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;"> de 9,8, uma declinação de -20º 34' 45" e uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="line-height: 19.1875px; text-align: start;"> de 03 </span><a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Hora">horas</a><span style="line-height: 19.1875px; text-align: start;">, 09 </span><a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Minuto">minutos</a><span style="line-height: 19.1875px; text-align: start;"> e 45,1 </span><a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Segundo">segundos</a><span style="line-height: 19.1875px; text-align: start;">.e tem cerca de 200 mil anos luzes de diâmetro</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/NGC_1232" style="background-color: white;">http://pt.wikipedia.org/wiki/NGC_1232</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Ficheiro:HAWK-I NGC 1232.jpg" src="http://upload.wikimedia.org/wikipedia/commons/thumb/a/ad/HAWK-I_NGC_1232.jpg/600px-HAWK-I_NGC_1232.jpg" /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/Ficheiro:HAWK-I_NGC_1232.jpg" style="background-color: white;">http://pt.wikipedia.org/wiki/Ficheiro:HAWK-I_NGC_1232.jpg</a></span></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_date" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 143.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Data</span></td><td><time class="dtstart" datetime="2010-10-27"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">27 de outubro de 2010</span></time></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 143.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Origem</span></td><td><a class="external free" href="http://www.eso.org/public/images/eso1042g/" rel="nofollow"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.eso.org/public/images/eso1042g/</span></a></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 143.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Autor</span></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO/P. Grosbøl</span></td></tr>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; font-weight: bold; text-align: -webkit-left;">NGC 1232: Dwarf Galaxy Caught Ramming Into a Large Spiral</span></span></div>
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<a href="http://chandra.harvard.edu/photo/2013/ngc1232/ngc1232_lg.jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://chandra.harvard.edu/photo/2013/ngc1232/ngc1232_lg.jpg</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 13px;">X-ray: NASA/CXC/Huntingdon Inst. for X-ray Astronomy/G.Garmire, Optical: ESO/VLT</span></div>
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<li style="text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Observations with Chandra have revealed a giant cloud of superheated gas in a galaxy about 60 million light years from Earth.</span></li>
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<li style="text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Because this gas is about 6 million degrees, it only glows in X-ray light.</span></li>
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<li style="text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A collision between a dwarf galaxy and a much larger galaxy called NGC 1232 is the likely cause of this gas cloud.</span></li>
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<li style="text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A new composite of X-rays (purple) from Chandra and optical data (blue and white) shows the scene of the collision.</span></li>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 16px; text-align: -webkit-left;">Observations with NASA's Chandra X-ray Observatory have revealed a massive cloud of multimillion-degree gas in a galaxy about 60 million light years from Earth. The hot gas cloud is likely caused by a collision between a dwarf galaxy and a much larger galaxy called NGC 1232. If confirmed, this discovery would mark the first time such a collision has been detected only in </span><a href="http://chandra.harvard.edu/resources/em_radiation.html" style="line-height: 16px; text-align: -webkit-left; text-decoration: none;">X-rays</a><span style="line-height: 16px; text-align: -webkit-left;">, and could have implications for understanding how galaxies grow through similar collisions.</span></span></div>
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<span style="line-height: 16px; text-align: -webkit-left;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">LEIA MAIS EM </span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://chandra.harvard.edu/photo/2013/ngc1232/index.html" style="background-color: white;">http://chandra.harvard.edu/photo/2013/ngc1232/index.html</a></span></div>
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<h1 class="pr_title" style="border-bottom-color: rgb(0, 91, 160); border-bottom-style: solid; border-bottom-width: 1px; margin: 0px 0px 0.5em; padding: 0.9em 0px 0px; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">A Blue Whirlpool in The River</span></h1>
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<span style="background-color: white;"><span style="color: #073763;"><img src="http://www.eso.org/public/archives/images/screen/eso1231a.jpg" height="371" width="640" /></span></span><br />
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<a href="http://www.eso.org/public/archives/images/screen/eso1231a.jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.eso.org/public/archives/images/screen/eso1231a.jpg</span></a></div>
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<span style="line-height: 16.796875px; text-align: left;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A new image taken with ESO’s Very Large Telescope shows the galaxy NGC 1187. This impressive spiral lies about 60 million light-years away in the constellation of Eridanus (The River). NGC 1187 has hosted two supernova explosions during the last thirty years, the latest one in 2007. This picture of the galaxy is the most detailed ever taken.</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.eso.org/public/videos/eso1231a/" style="background-color: white; margin: 0px; padding: 0px; text-decoration: none;"><img alt="Zooming in on the spiral galaxy NGC 1187" src="http://www.eso.org/public/archives/videos/thumb/eso1231a.jpg" style="border: 0px; margin: 0px; padding: 10px;" width="122" /></a></span><br />
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<a href="http://www.eso.org/public/videos/eso1231a/" style="margin: 0px; padding: 0px; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">PR Video eso1231a</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Zooming in on the spiral galaxy NGC 1187</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.eso.org/public/videos/eso1231b/" style="background-color: white; margin: 0px; padding: 0px; text-decoration: none;"><img alt="Panning across a new VLT image of the spiral galaxy NGC 1187" src="http://www.eso.org/public/archives/videos/thumb/eso1231b.jpg" style="border: 0px; margin: 0px; padding: 10px;" width="122" /></a></span><br />
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<a href="http://www.eso.org/public/videos/eso1231b/" style="margin: 0px; padding: 0px; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">PR Video eso1231b</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Panning across a new VLT image of the spiral galaxy NGC 1187</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">LEIA MAIS EM</span><br />
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<a href="http://www.eso.org/public/news/eso1231/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.eso.org/public/news/eso1231/</span></a></div>
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<a class="ga_static_tracking" href="http://www.eso.org/public/archives/images/screen/eso1231c.jpg" rel="shadowbox" style="margin: 0px; padding: 0px;" title="The spiral galaxy NGC 1187 in the constellation of Eridanus"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="The spiral galaxy NGC 1187 in the constellation of Eridanus" border="0" src="http://www.eso.org/public/archives/images/medium/eso1231c.jpg" height="640" style="border: 0px; margin: 0px; padding: 10px;" width="598" /> </span></a><br />
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<a class="ga_static_tracking" href="http://www.eso.org/public/archives/images/screen/eso1231c.jpg" rel="shadowbox" style="margin: 0px; padding: 0px;" title="The spiral galaxy NGC 1187 in the constellation of Eridanus"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></a></div>
<a class="ga_static_tracking" href="http://www.eso.org/public/archives/images/screen/eso1231c.jpg" rel="shadowbox" style="margin: 0px; padding: 0px;" title="The spiral galaxy NGC 1187 in the constellation of Eridanus"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">This chart shows the location of NGC 1187 in the constellation of Eridanus (The River). This map shows most of the stars visible to the unaided eye under good conditions, and NGC 1187 itself is highlighted with a red circle on the image. This galaxy appears as a faint smudge through medium-sized amateur telescopes under good conditions.</span></div>
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<strong style="margin: 0px; padding: 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Credit:</span></strong></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO, IAU and Sky & Telescope</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.eso.org/public/images/eso1231c/" style="background-color: white;">http://www.eso.org/public/images/eso1231c/</a></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><img src="http://www.raremaps.com/maps/medium/29167.jpg" /></span></span></div>
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<a href="http://www.raremaps.com/gallery/detail/29167/Orion_and_Haase_Lepus_the_Rabbit/Bode.html"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/detail/29167/Orion_and_Haase_Lepus_the_Rabbit/Bode.html</span></a><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Title: </strong>Orion and Haase (Lepus the Rabbit)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1098" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">Johann Ehlert Bode</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>IC 2118</b> (also known as <b>Witch Head Nebula</b> due to its shape), is an extremely faint <a href="http://en.wikipedia.org/wiki/Reflection_nebula" style="background-image: none; text-decoration: none;" title="Reflection nebula">reflection nebula</a> believed to be an ancient supernova remnant or gas cloud illuminated by nearby <a href="http://en.wikipedia.org/wiki/Supergiant" style="background-image: none; text-decoration: none;" title="Supergiant">supergiant</a> star <a href="http://en.wikipedia.org/wiki/Rigel" style="background-image: none; text-decoration: none;" title="Rigel">Rigel</a> in <a href="http://en.wikipedia.org/wiki/Orion_(constellation)" style="background-image: none; text-decoration: none;" title="Orion (constellation)">Orion</a>. It lies in the <a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)" style="background-image: none; text-decoration: none;" title="Eridanus (constellation)">Eridanus</a>constellation, about 900 <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Light-years" style="background-image: none; text-decoration: none;" title="Light-years">light-years</a> from <a href="http://en.wikipedia.org/wiki/Earth" style="background-image: none; text-decoration: none;" title="Earth">Earth</a>. The nature of the dust particles, reflecting blue light better than red, is a factor in giving the Witch Head its blue color. Radio observations show substantial carbon monoxide emission throughout parts of IC 2118 an indicator of the presence of molecular clouds and star formation in the nebula. In fact candidates for pre-main sequence stars and some classic <a class="mw-redirect" href="http://en.wikipedia.org/wiki/T_Tauri_star" style="background-image: none; text-decoration: none;" title="T Tauri star">T-Tauri stars</a> have been found deep within the nebula.<sup class="reference" id="cite_ref-1" style="color: #fff2cc; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/IC_2118#cite_note-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The molecular clouds of IC 2118 are probably juxtaposed to the outer boundaries of the vast <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Orion-Eridanus_Superbubble" style="background-image: none; text-decoration: none;" title="Orion-Eridanus Superbubble">Orion-Eridanus bubble</a>, a giant supershell of molecular hydrogen blown by the high mass stars of the Orion OB1 association. As the supershell expands into the interstellar medium, favorable circumstances for star formation occur. IC 2118 is located in one such area.The wind blown appearance and cometary shape of the bright reflection nebula is highly suggestive of a strong association with the high mass luminous stars of Orion OB1. The fact that the heads of the cometary clouds of IC2118 point northeast towards the association is strong support of that relationship.</span></div>
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<a href="http://en.wikipedia.org/wiki/IC_2118"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://en.wikipedia.org/wiki/IC_2118</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>The Witch Head Nebula </b><br /><b>Credit: </b><a href="mailto:Gary.L.Stevens@jpl.nasa.gov">Gary Stevens</a></span></div>
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<a href="http://apod.nasa.gov/apod/ap010227.html"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://apod.nasa.gov/apod/ap010227.html</span></a></div>
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<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Type</span></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Reflection</span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Right_ascension" style="background-image: none; text-decoration: none;" title="Right ascension"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Right ascension</span></a></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">05<sup style="line-height: 1em;">h</sup> 02<sup style="line-height: 1em;">m</sup> 00.00<sup style="line-height: 1em;">s</sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Declination" style="background-image: none; text-decoration: none;" title="Declination"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Declination</span></a></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-07° 54′ 00.0"</span></td></tr>
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<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Apparent_magnitude" style="background-image: none; text-decoration: none;" title="Apparent magnitude">Apparent magnitude</a><small>(V)</small></span></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">13</span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Angular_diameter" style="background-image: none; text-decoration: none;" title="Angular diameter">Apparent dimensions</a> <small>(V)</small></span></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">3 × 1 <a href="http://en.wikipedia.org/wiki/Degree_(angle)" style="background-image: none; text-decoration: none;" title="Degree (angle)">°</a></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Constellation" style="background-image: none; text-decoration: none;" title="Constellation"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constellation</span></a></th><td style="vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)" style="background-image: none; text-decoration: none;" title="Eridanus (constellation)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Eridanus</span></a></td></tr>
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<span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif; font-size: small;">Baby Stars Brewing in the Witch Head Nebula</span></span></h2>
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<span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif; font-size: small;"><img src="http://www.spitzer.caltech.edu/uploaded_files/graphics/high_definition_graphics/0009/3107/sig06-013_Ti.jpg?1350004365" /></span></span></h2>
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<a href="http://www.spitzer.caltech.edu/images/2288-sig06-013-Baby-Stars-Brewing-in-the-Witch-Head-Nebula"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spitzer.caltech.edu/images/2288-sig06-013-Baby-Stars-Brewing-in-the-Witch-Head-Nebula</span></a><br />
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<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Credit</span></dt>
<dd property="photoshop:Credit" style="margin: 0px; padding: 2px 0px 0px 5px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NASA/JPL-Caltech/L. Rebull (SSC/Caltech)</span></dd>
<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Observers</span></dt>
<dd style="margin: 0px; padding: 2px 0px 0px 5px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">L. Rebull (Spitzer Science Center), T. Spuck (Oil City Area Sr. High School), B. Sepulveda (Lincoln High School), T. Maranto (Phillips Exeter Academy), C. Weehler (Luther Burbank High School), T. Roelofsen (Bassick High School), B. Ehrhart (Oil City Area Sr. High School), D. Bowser II (Oil City Area Sr. High School), M. Greer (Phillips Exeter Academy), J. Preis (Phillips Exeter Academy), P. Weston (Phillips Exeter Academy), A. Hughes (Lincoln High School), N. Sharma (Lincoln High School), J. Herrera (Luther Burbank High School),</span></dd></dl>
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<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Name</span></dt>
<dd style="margin: 0px; padding: 2px 0px 0px 5px;"><span property="dc:subject"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Witch Head Nebula</span></span></dd>
<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Type</span></dt>
<dd property="avm:Subject.Category" style="margin: 0px; padding: 2px 0px 0px 5px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Nebula > Type > Star Formation</span></dd>
<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distance</span></dt>
<dd property="avm:Distance" style="margin: 0px; padding: 2px 0px 0px 5px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">800 Light Years</span></dd></dl>
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<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Position (J2000)</span></dt>
<dd property="avm:Spatial.ReferenceValue" style="margin: 0px; padding: 2px 0px 0px 5px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">RA = 5<sup>h</sup> 7<sup>m</sup> 50.3<sup>s</sup></span></dd><dd property="avm:Spatial.ReferenceValue" style="margin: 0px; padding: 2px 0px 0px 5px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dec = -6° 21' 31.5"</span></dd>
<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Field of View</span></dt>
<dd property="avm:Spatial.ReferenceDimension" style="margin: 0px; padding: 2px 0px 0px 5px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">18.4 x 15.2 arcminutes</span></dd>
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<dd property="avm:Spatial.Rotation" style="margin: 0px; padding: 2px 0px 0px 5px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">North is 1.1° left of vertical</span></dd>
<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constellation</span></dt>
<dd style="margin: 0px; padding: 2px 0px 0px 5px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Eridanus</span></dd></dl>
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<span style="background-color: #073763; line-height: 18px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Eight hundred light-years away in the Orion constellation, a gigantic murky cloud called the "Witch Head Nebula" is teeming with dust-obscured newborn stars waiting to be uncovered. In this image, the super sensitive infrared eyes of NASA's Spitzer Space Telescope reveal 12 new baby stars in a small portion of the cloud commonly referred to as the Witch Head's "pointy chin."</span></span></div>
<a href="http://www.spitzer.caltech.edu/images/2288-sig06-013-Baby-Stars-Brewing-in-the-Witch-Head-Nebula"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spitzer.caltech.edu/images/2288-sig06-013-Baby-Stars-Brewing-in-the-Witch-Head-Nebula</span></a><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1132</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; text-decoration: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_el%C3%ADptica" style="background-image: none; text-decoration: none;" title="Galáxia elíptica">elíptica</a> (E) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Eridanus" style="background-image: none; text-decoration: none;" title="Eridanus">Eridanus</a>. Possui uma declinação de -01° 16' 28" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-image: none;" title="Ascensão recta">ascensão recta</a> de 2 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; text-decoration: none;" title="Hora">horas</a>, 52 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; text-decoration: none;" title="Minuto">minutos</a> e 51,8 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; text-decoration: none;" title="Segundo">segundos</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A galáxia <b>NGC 1132</b> foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/23_de_Novembro" style="background-image: none; text-decoration: none;" title="23 de Novembro">23 de Novembro</a> de <a href="http://pt.wikipedia.org/wiki/1827" style="background-image: none; text-decoration: none;" title="1827">1827</a> por <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-image: none; text-decoration: none;" title="John Herschel">John Herschel</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/NGC_1132">http://pt.wikipedia.org/wiki/NGC_1132</a><span style="font-weight: bold;"></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-weight: bold;">NGC 1132: A Mysterious Elliptical Galaxy</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; font-weight: bold;"><img alt="NGC 1132" src="http://chandra.harvard.edu/photo/2008/ngc1132/ngc1132_w11.jpg" /></span></div>
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<a href="http://chandra.harvard.edu/photo/2008/ngc1132/index.html"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://chandra.harvard.edu/photo/2008/ngc1132/index.html</span></a></div>
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<tr><td style="padding-left: 23px;" valign="top" width="40%"><span class="bold"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Credit </span></span></td><td valign="top" width="60%"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">X-ray: NASA/CXC/Penn State/G. Garmire; Optical: NASA/ESA/STScI/M. West</span></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">This image of the elliptical galaxy NGC 1132 and its surrounding region combines data from NASA's Chandra X-ray Observatory and the Hubble Space Telescope. The blue/purple in the image is the X-ray glow from hot, diffuse gas detected by Chandra. Hubble's data reveal a giant foreground elliptical galaxy, plus numerous dwarf galaxies in its neighborhood, and many much more distant galaxies in the background.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Astronomers have dubbed NGC 1132 a "fossil group" because it contains an enormous amount of dark matter, comparable to the dark matter found in an entire group of galaxies. Also, the large amount of hot gas detected by Chandra is usually found for groups of galaxies, rather than a single galaxy.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Leia mais em <a href="http://chandra.harvard.edu/photo/2008/ngc1132/index.html">http://chandra.harvard.edu/photo/2008/ngc1132/index.html</a></span></div>
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<a href="http://chandra.harvard.edu/photo/2008/ngc1132/ngc1132_hst.jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://chandra.harvard.edu/photo/2008/ngc1132/ngc1132_hst.jpg</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; text-align: left;">Hubble Optical Image of NGC 1132 </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="text-align: left;">The elliptical galaxy NGC 1132 reveals the final result of what may have been a group of galaxies that merged together in the recent past. Another possibility is that the galaxy formed in isolation as a "lone wolf" in a universe ablaze with galaxy groups and clusters. This image of NGC 1132 was taken with Hubble's Advanced Camera for Surveys. Data obtained in 2005 and 2006 through green and near-infrared filters were used in the composite. NGC 1132 is located approximately 318 million light-years away in the constellation Eridanus, the River. </span><a href="http://hubblesite.org/newscenter/archive/releases/2008/07" style="text-align: left; text-decoration: none;" target="_blank">More information at Hubble</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span class="caption" style="background-color: white; color: #073763; line-height: 12px; text-align: left;">(Credit: Optical: NASA/ESA/STScI/M. West)</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; text-align: left;">This image of elliptical galaxy NGC 1132 and its surrounding region shows the X-ray glow from hot, diffuse gas detected by Chandra. Astronomers have dubbed NGC 1132 a "fossil group" because it contains an enormous amount of dark matter, comparable to the dark matter found in an entire group of galaxies. Also, the large amount of hot gas detected by Chandra is usually found for groups of galaxies, rather than a single galaxy. On the right, the white box represents the Hubble Space Telescope's field of view.</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span class="caption" style="background-color: white; color: #073763; line-height: 12px; text-align: left;">(Credit: X-ray:NASA/CXC/Penn State/G. Garmire)</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1700</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; text-decoration: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_el%C3%ADptica" style="background-image: none; text-decoration: none;" title="Galáxia elíptica">elíptica</a> (E4) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Eridanus" style="background-image: none; text-decoration: none;" title="Eridanus">Eridanus</a>. Possui uma declinação de -04° 51' 55" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-image: none; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 4 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; text-decoration: none;" title="Hora">horas</a>, 56 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; text-decoration: none;" title="Minuto">minutos</a> e 56,2 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; text-decoration: none;" title="Segundo">segundos</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A galáxia <b>NGC 1700</b> foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/5_de_Outubro" style="background-image: none; text-decoration: none;" title="5 de Outubro">5 de Outubro</a> de <a href="http://pt.wikipedia.org/wiki/1785" style="background-image: none; text-decoration: none;" title="1785">1785</a> por <a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-image: none; text-decoration: none;" title="William Herschel">William Herschel</a>.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/NGC_1700" style="background-color: white;">http://pt.wikipedia.org/wiki/NGC_1700</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span class="page_title" style="background-color: white; color: #073763; font-size: small; font-variant: small-caps; text-align: left;"><span class="page_title">Giant X-Ray Disk Sheds Light On Galactic Merger</span> </span></span></div>
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<a href="http://chandra.harvard.edu/photo/2002/n1700/n1700_xray.jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://chandra.harvard.edu/photo/2002/n1700/n1700_xray.jpg</span></a></div>
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<span class="caption" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 12px;">Credit: NASA/Ohio U./T.Statler et al.</span></div>
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<em><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The Chandra image of the elliptical galaxy NGC 1700 shows a flattened oval of multi-million degree gas, supporting the idea that it is the result of a merger of two smaller galaxies about 3 billion years ago.</span></em></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 12px; text-align: left;">(Credit: NASA/Ohio U./</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; line-height: 12px; text-align: left;">T.Statler et al.)</span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">.........</span><span style="font-family: Arial, Helvetica, sans-serif;">another version of the Chandra image shows only the low-energy X-rays and reveals a giant inner disk. This disk of 6-million degree gas appears light blue in the multicolor image above.</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><em style="text-align: left;">LEIA MAIS EM </em><a href="http://chandra.harvard.edu/photo/2002/n1700/index.html">http://chandra.harvard.edu/photo/2002/n1700/index.html</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">NGC 1309</b><span style="font-weight: normal; line-height: 19.1875px; text-align: start;"> é uma </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-image: none; font-weight: normal; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a><span style="font-weight: normal; line-height: 19.1875px; text-align: start;"> localizada a cerca de cem milhões de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; font-weight: normal; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="font-weight: normal; line-height: 19.1875px; text-align: start;"> de distância na direção da </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o_de_Er%C3%ADdano" style="background-image: none; font-weight: normal; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Constelação de Erídano">constelação de Erídano</a><span style="font-weight: normal; line-height: 19.1875px; text-align: start;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; font-weight: normal; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="font-weight: normal; line-height: 19.1875px; text-align: start;"> de 11,5, uma declinação de -15º 24' 02" e uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-image: none; font-weight: normal; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="font-weight: normal; line-height: 19.1875px; text-align: start;"> de 3 </span><a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; font-weight: normal; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Hora">horas</a><span style="font-weight: normal; line-height: 19.1875px; text-align: start;">, 22</span><a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; font-weight: normal; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Minuto">minutos</a><span style="font-weight: normal; line-height: 19.1875px; text-align: start;"> e 6,5 </span><a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; font-weight: normal; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Segundo">segundos</a><span style="font-weight: normal; line-height: 19.1875px; text-align: start;">.</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; font-weight: bold;"><a href="http://pt.wikipedia.org/wiki/NGC_1309" style="background-color: white;">http://pt.wikipedia.org/wiki/NGC_1309</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Hubble Snaps Images of a Pinwheel-Shaped Galaxy</span></h2>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://hubblesite.org/newscenter/archive/releases/2006/07/image/a/format/web_print/" style="background-color: white;">http://hubblesite.org/newscenter/archive/releases/2006/07/image/a/format/web_print/</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="line-height: 18px; text-align: start;">Credit:</span><span style="font-weight: normal; line-height: 18px; text-align: start;"> </span><a href="http://www.nasa.gov/" style="font-weight: normal; line-height: 18px; text-align: start;">NASA</a><span style="font-weight: normal; line-height: 18px; text-align: start;">, </span><a href="http://www.spacetelescope.org/" style="font-weight: normal; line-height: 18px; text-align: start;">ESA</a><span style="font-weight: normal; line-height: 18px; text-align: start;">, The </span><a href="http://heritage.stsci.edu/" style="font-weight: normal; line-height: 18px; text-align: start;">Hubble Heritage</a><span style="font-weight: normal; line-height: 18px; text-align: start;"> Team, (</span><a href="http://www.stsci.edu/" style="font-weight: normal; line-height: 18px; text-align: start;">STScI</a><span style="font-weight: normal; line-height: 18px; text-align: start;">/</span><a href="http://www.aura-astronomy.org/" style="font-weight: normal; line-height: 18px; text-align: start;">AURA</a><span style="font-weight: normal; line-height: 18px; text-align: start;">) and A. Riess (</span><a href="http://www.stsci.edu/" style="font-weight: normal; line-height: 18px; text-align: start;">STScI</a><span style="font-weight: normal; line-height: 18px; text-align: start;">)</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Looking like a child's pinwheel ready to be set a spinning by a gentle breeze, this dramatic spiral galaxy is one of the latest viewed by NASA's Hubble Space Telescope. Stunning details of the face-on spiral galaxy, cataloged as NGC 1309, are captured in this color image.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Recent observations of the galaxy taken in visible and infrared light come together in a colorful depiction of many of the galaxy's features. Bright blue areas of star formation pepper the spiral arms, while ruddy dust lanes follow the spiral structure into a yellowish central nucleus of older-population stars. The image is complemented by myriad far-off background galaxies.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">LEIA MAIS EM </span></div>
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<a href="http://hubblesite.org/newscenter/archive/releases/2006/07/image/a/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/2006/07/image/a/</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Lick Observatory Ground-Based Image of SN2002fk in NGC 1309</span></h2>
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<a href="http://hubblesite.org/newscenter/archive/releases/2006/07/image/b/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/2006/07/image/b/</span></a></div>
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<span style="font-weight: normal; line-height: 18px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SN2002fk as observed from Lick Observatory Kait 0.76 meter telescope in 2002. The location of the supernova is marked on the 2005 Hubble ACS image.</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold;">Credit for Lick Observatory Image:</span> W. Li and A. V. Filippenko (University of California, Berkeley)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold;">Credit for HST Image:</span> <a href="http://www.nasa.gov/">NASA</a>, <a href="http://www.spacetelescope.org/">ESA</a>, The <a href="http://heritage.stsci.edu/">Hubble Heritage</a> Team (<a href="http://www.stsci.edu/">STScI</a>/<a href="http://www.aura-astronomy.org/">AURA</a>), and A. Riess (<a href="http://www.stsci.edu/">STScI</a>)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1614</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; text-decoration: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral_barrada" style="background-image: none; text-decoration: none;" title="Galáxia espiral barrada">espiral barrada</a> (SBc/P) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Eridanus" style="background-image: none; text-decoration: none;" title="Eridanus">Eridanus</a>. Possui uma declinação de -08° 34' 45" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-image: none; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 4 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; text-decoration: none;" title="Hora">horas</a>, 33 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; text-decoration: none;" title="Minuto">minutos</a> e 59,8 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; text-decoration: none;" title="Segundo">segundos</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A galáxia <b>NGC 1614</b> foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/29_de_Dezembro" style="background-image: none; text-decoration: none;" title="29 de Dezembro">29 de Dezembro</a> de <a href="http://pt.wikipedia.org/wiki/1885" style="background-image: none; text-decoration: none;" title="1885">1885</a> por <a href="http://pt.wikipedia.org/wiki/Lewis_A._Swift" style="background-image: none; text-decoration: none;" title="Lewis A. Swift">Lewis A. Swift</a>.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/NGC_1614" style="background-color: white;">http://pt.wikipedia.org/wiki/NGC_1614</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Hubble Interacting Galaxy NGC 1614</span></h2>
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<a href="http://hubblesite.org/newscenter/archive/releases/2008/16/image/bq/format/large_web/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/2008/16/image/bq/format/large_web/</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Object Names:</strong> NGC 1614, Arp 186, Mrk 0617, II Zw 015</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Image Type:</strong> Astronomical</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold;">Credit:</span> <a href="http://www.nasa.gov/">NASA</a>, <a href="http://www.spacetelescope.org/">ESA</a>, the <a href="http://heritage.stsci.edu/">Hubble Heritage</a> (<a href="http://www.stsci.edu/">STScI</a>/<a href="http://www.aura-astronomy.org/">AURA</a>)-<a href="http://www.spacetelescope.org/">ESA</a>/Hubble Collaboration, and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The galaxy system NGC 1614 has a bright optical center and two clear inner spiral arms that are fairly symmetrical. It also has a spectacular outer structure that consists principally of a large one-sided curved extension of one of these arms to the lower right, and a long, almost straight tail that emerges from the nucleus and crosses the extended arm to the upper right. </span></div>
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<a href="http://hubblesite.org/newscenter/archive/releases/2008/16/image/bq/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/2008/16/image/bq/</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1531</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; text-decoration: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_el%C3%ADptica" style="background-image: none; text-decoration: none;" title="Galáxia elíptica">elíptica</a> (E-S0) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Eridanus" style="background-image: none; text-decoration: none;" title="Eridanus">Eridanus</a>. Possui uma declinação de -32° 51' 03" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-image: none;" title="Ascensão recta">ascensão recta</a> de 4 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; text-decoration: none;" title="Hora">horas</a>, 11 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; text-decoration: none;" title="Minuto">minutos</a> e 59,1 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; text-decoration: none;" title="Segundo">segundos</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A galáxia <b>NGC 1531</b> foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/19_de_Outubro" style="background-image: none; text-decoration: none;" title="19 de Outubro">19 de Outubro</a> de <a href="http://pt.wikipedia.org/wiki/1835" style="background-image: none; text-decoration: none;" title="1835">1835</a> por <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-image: none; text-decoration: none;" title="John Herschel">John Herschel</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1532</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; text-decoration: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral_barrada" style="background-image: none; text-decoration: none;" title="Galáxia espiral barrada">espiral barrada</a> (SBb) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Eridanus" style="background-image: none; text-decoration: none;" title="Eridanus">Eridanus</a>. Possui uma declinação de -32° 52' 23" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-image: none; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 4 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; text-decoration: none;" title="Hora">horas</a>, 12 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; text-decoration: none;" title="Minuto">minutos</a> e 03,8 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; text-decoration: none;" title="Segundo">segundos</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A galáxia <b>NGC 1532</b> foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/29_de_Outubro" style="background-image: none; text-decoration: none;" title="29 de Outubro">29 de Outubro</a> de <a href="http://pt.wikipedia.org/wiki/1826" style="background-image: none; text-decoration: none;" title="1826">1826</a> por <a href="http://pt.wikipedia.org/wiki/James_Dunlop" style="background-image: none; text-decoration: none;" title="James Dunlop">James Dunlop</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="font-weight: normal; line-height: 19.1875px;">This photograph was produced by </span><b style="line-height: 19.1875px;"><a class="extiw" href="http://en.wikipedia.org/wiki/European_Southern_Observatory" style="background-image: none; text-decoration: none;" title="en:European Southern Observatory">European Southern Observatory (ESO)</a></b><span style="font-weight: normal; line-height: 19.1875px;">.</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="external text" href="http://www.eso.org/" rel="nofollow">ESO</a><span style="font-weight: normal; line-height: 19.1875px;">/IDA/Danish 1.5 m/R.Gendler and J.-E. Ovaldsen</span></span></div>
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<a href="http://www.eso.org/public/images/ngc1532/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.eso.org/public/images/ngc1532/</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The pair of galaxies NGC 1531/2, engaged in a spirited waltz, is located about 70 million light-years away towards the southern constellation Eridanus (The River). The deformed foreground spiral galaxy laced with dust lanes NGC 1532 is so close to its companion — the background galaxy with a bright core just above the centre of NGC 1532 — that it gets distorted: one of its spiral arms is warped and plumes of dust and gas are visible above its disc. The cosmic dance leads to another dramatic effect: a whole new generation of massive stars were born in NGC 1532 because of the interaction. They are visible as the purple objects in the spiral arms.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">This exquisite image was made using the 1.5-metre Danish telescope at the ESO La Silla Observatory, Chile. It is based on data obtained through three different filters: B, V and R. The field of view is 12 x 12 arcmin.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1518</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; text-decoration: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral_barrada" style="background-image: none; text-decoration: none;" title="Galáxia espiral barrada">espiral barrada</a> (SBd) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Eridanus" style="background-image: none; text-decoration: none;" title="Eridanus">Eridanus</a>. Possui uma declinação de -21° 10' 46" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-image: none; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 4 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; text-decoration: none;" title="Hora">horas</a>, 06 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; text-decoration: none;" title="Minuto">minutos</a> e 49,0 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; text-decoration: none;" title="Segundo">segundos</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A galáxia <b>NGC 1518</b> foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/13_de_Novembro" style="background-image: none; text-decoration: none;" title="13 de Novembro">13 de Novembro</a> de <a href="http://pt.wikipedia.org/wiki/1835" style="background-image: none; text-decoration: none;" title="1835">1835</a> por <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-image: none; text-decoration: none;" title="John Herschel">John Herschel</a>.</span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_1518"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_1518</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://cseligman.com/text/atlas/ngc15.htm#1518"></a><a href="http://cseligman.com/text/atlas/ngc15.htm#1518">http://cseligman.com/text/atlas/ngc15.htm#1518</a></span></div>
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<a href="http://www.blogger.com/blogger.g?blogID=4158372707710982464" name="1518"><big><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1518 (= PGC 14475)</span></b></big></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.blogger.com/blogger.g?blogID=4158372707710982464" name="1518">Discovered (Nov 13, 1835) by </a><a href="http://cseligman.com/text/atlas/discoverers.htm#jfwherschel">John Herschel</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="font-weight: normal;">A 12th-magnitude spiral galaxy (type SB(s)dm) in </span><a href="http://cseligman.com/text/atlas/eridanus.htm#1518" style="font-weight: normal;">Eridanus</a><span style="font-weight: normal;"> (RA 04 06 49.0, Dec -21 10 46)</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The second IC notes (per Howe) "Minute of RA is 00, not 01". Based on a recessional velocity of 920 km/sec, NGC 1517 is about 40 million light years away, in reasonable agreement with redshift-independent distance estimates of 25 to 40 million light years. Given that and its apparent size of 2.9 by 1.4 arcmin, it is about 35 thousand light years across.</span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiSrW2Mp4SLJcngMBZDvyXXck8-RBVrLLfUIL2E5GtQOF4KXno7Kh0VuGC0NoYTxuVJeDmIeR9jBbQr9phjTwNQ_8rrhoeYKIY9qcj9m8Dd70YOZfVGAjkJjRpvDygUQKrFtPrv5TlpB5Wz/s1600/ngc1518.jpg" imageanchor="1" style="background-color: white; margin-left: 1em; margin-right: 1em;"><span style="color: #073763;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiSrW2Mp4SLJcngMBZDvyXXck8-RBVrLLfUIL2E5GtQOF4KXno7Kh0VuGC0NoYTxuVJeDmIeR9jBbQr9phjTwNQ_8rrhoeYKIY9qcj9m8Dd70YOZfVGAjkJjRpvDygUQKrFtPrv5TlpB5Wz/s1600/ngc1518.jpg" height="400" width="400" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-weight: normal;">Above, a 3.6 arcin wide closeup of NGC 1518</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="font-weight: normal;">Below, a detailed view of the northern half of the galaxy </span><small style="font-weight: normal;">(Image Credits: Hubble Legacy Archive)</small></span><br />
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<a href="http://cseligman.com/text/atlas/ngc15.htm#1518"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://cseligman.com/text/atlas/ngc15.htm#1518</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1535 - Eridanus - Nebulosa Nebulosa Planetária</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 04h13m Declinação -12<sup>o</sup>.48<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo Nebulosa Planetária NP Dimensão 0,5 Magnitude 17<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude da Estrela associada 12 <o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">NGC 1535</b><span style="line-height: 19.1875px; text-align: start;"> é uma </span><a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Nebulosa planetária">nebulosa planetária</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Eridanus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Eridanus">constelação de Eridanus</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="William Herschel">William Herschel</a><span style="line-height: 19.1875px; text-align: start;"> em 1785, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="line-height: 19.1875px; text-align: start;"> refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;">(+9,6), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="line-height: 19.1875px; text-align: start;"> amadores ou com equipamentos superiores.</span></span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_1535"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_1535</span></a></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh63r8i6voL8EyxE6Azs1XB0OiKzJzFwGN1xtT5FpaZvVxUtN5cT2mU216YnssCT0nKQJgTkCmGcGJEGHvn96cKiX78AJJxWw1qTA1imAPVqgeZUDj8oUenlFsVuIL0bUMiMpD0sw_tf8gN/s1600/1187+-+image.jpg" imageanchor="1" style="background-color: white; margin-left: 1em; margin-right: 1em;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1234</b> is <a href="http://en.wikipedia.org/wiki/Barred_spiral_galaxy" style="background-image: none; text-decoration: none;" title="Barred spiral galaxy">barred spiral galaxy</a> in the constellation <a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)" style="background-image: none; text-decoration: none;" title="Eridanus (constellation)">Eridanus</a>, discovered by <a class="new" href="http://en.wikipedia.org/w/index.php?title=Francis_Preserved_Leavenworth&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="Francis Preserved Leavenworth (page does not exist)">Francis Preserved Leavenworth</a> in 1886.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Its <a href="http://en.wikipedia.org/wiki/Apparent_magnitude" style="background-image: none; text-decoration: none;" title="Apparent magnitude">apparent magnitude</a> is 14.2</span></div>
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<a href="http://en.wikipedia.org/wiki/NGC_1234"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://en.wikipedia.org/wiki/NGC_1234</span></a></div>
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<table cellpadding="4" class="toccolours vevent mw-content-ltr" style="border: 1px solid rgb(170, 170, 170); color: black; direction: ltr; font-weight: normal; line-height: 19.1875px; padding: 5px; text-align: center; width: 1024px;"><tbody>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 143.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Author</span></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background-image: none; text-decoration: none;" title="en:NASA">en:NASA</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-image: none; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span></td></tr>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; line-height: 19.1875px;"><b>NGC 1300</b> is a <a href="http://en.wikipedia.org/wiki/Barred_spiral_galaxy" style="background-image: none; text-decoration: none;" title="Barred spiral galaxy">barred spiral galaxy</a> about <a class="mw-redirect" href="http://en.wikipedia.org/wiki/1_E23_m" style="background-image: none; text-decoration: none;" title="1 E23 m">61 million</a> <a href="http://en.wikipedia.org/wiki/Light-year" style="background-image: none; text-decoration: none;" title="Light-year">light-years</a> away in the <a href="http://en.wikipedia.org/wiki/Constellation" style="background-image: none; text-decoration: none;" title="Constellation">constellation</a> <a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)" style="background-image: none; text-decoration: none;" title="Eridanus (constellation)">Eridanus</a>. The galaxy is about 110,000 light-years across; just slightly larger than our own galaxy, the <a href="http://en.wikipedia.org/wiki/Milky_Way" style="background-image: none; text-decoration: none;" title="Milky Way">Milky Way</a>. It is a member of the<a href="http://en.wikipedia.org/wiki/Eridanus_Cluster" style="background-image: none; text-decoration: none;" title="Eridanus Cluster">Eridanus Cluster</a>, a cluster of 200 galaxies.<sup class="reference" id="cite_ref-NGC1300_3-0" style="font-weight: normal; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/NGC_1300#cite_note-NGC1300-3" style="background-image: none; text-decoration: none; white-space: nowrap;">[3]</a></sup><sup class="reference" id="cite_ref-atlas_4-0" style="font-weight: normal; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/NGC_1300#cite_note-atlas-4" style="background-image: none; text-decoration: none; white-space: nowrap;">[4]</a></sup> It was discovered by <a class="mw-redirect" href="http://en.wikipedia.org/wiki/John_Frederick_William_Herschel" style="background-image: none; text-decoration: none;" title="John Frederick William Herschel">John Frederick William Herschel</a> in 1835.<sup class="Template-Fact" style="line-height: 1em; white-space: nowrap;">[<i><a href="http://en.wikipedia.org/wiki/Wikipedia:Citation_needed" style="background-image: none; text-decoration: none;" title="Wikipedia:Citation needed"><span title="This claim needs references to reliable sources. (March 2007)">citation needed</span></a></i>]</sup></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; line-height: 18px;"><img alt="File:Hubble2005-01-barred-spiral-galaxy-NGC1300.jpg" src="http://upload.wikimedia.org/wikipedia/commons/thumb/5/52/Hubble2005-01-barred-spiral-galaxy-NGC1300.jpg/800px-Hubble2005-01-barred-spiral-galaxy-NGC1300.jpg" /></span></span></div>
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<a href="http://en.wikipedia.org/wiki/File:Hubble2005-01-barred-spiral-galaxy-NGC1300.jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://en.wikipedia.org/wiki/File:Hubble2005-01-barred-spiral-galaxy-NGC1300.jpg</span></a></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 143.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Source</span></td><td><ul style="line-height: 1.5em;">
<li style="margin-bottom: 0.1em;"><a class="external free" href="http://hubblesite.org/newscenter/archive/releases/2005/01/image/a" rel="nofollow"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/2005/01/image/a</span></a></li>
<li style="margin-bottom: 0.1em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="external free" href="http://www.spacetelescope.org/images/html/opo0501a.html" rel="nofollow">http://www.spacetelescope.org/images/html/opo0501a.html</a> (<a class="external text" href="http://www.spacetelescope.org/images/large/opo0501a.jpg" rel="nofollow">direct link</a>)</span></li>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 143.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Author</span></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NASA, ESA, and The Hubble Heritage Team STScI/AURA)</span></td></tr>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; line-height: 18px;">At Hubble's resolution, a myriad of fine details, some of which have never before been seen, is seen throughout the galaxy's arms, disk, bulge, and nucleus. Blue and red supergiant stars, star clusters, and star-forming regions are well resolved across the spiral arms, and dust lanes trace out fine structures in the disk and bar. Numerous more distant galaxies are visible in the background, and are seen even through the densest regions of NGC 1300</span></span></div>
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<a href="http://hubblesite.org/newscenter/archive/releases/2005/01/image/a/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/2005/01/image/a/</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold;">Credit:</span> <a href="http://www.nasa.gov/">NASA</a>, <a href="http://www.spacetelescope.org/">ESA</a>, and The <a href="http://heritage.stsci.edu/">Hubble Heritage</a> Team (<a href="http://www.stsci.edu/">STScI</a>/<a href="http://www.aura-astronomy.org/">AURA</a>)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold;">Acknowledgment:</span> P. Knezek (WIYN)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Giant Radio Jet Coming from Wrong Kind of Galaxy</span></h1>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://hubblesite.org/newscenter/archive/releases/2003/04/image/b/format/web_print/" style="background-color: white;">http://hubblesite.org/newscenter/archive/releases/2003/04/image/b/format/web_print/</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold; line-height: 18px; text-align: start;">Credit:</span><span style="line-height: 18px; text-align: start;"> </span><a href="http://www.nasa.gov/" style="line-height: 18px; text-align: start;">NASA</a><span style="line-height: 18px; text-align: start;">, W. Keel (University of Alabama), M. Ledlow (Gemini Observatory), F. Owen (NRAO) and AUI/NSF</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://hubblesite.org/newscenter/archive/releases/2003/04/image/a/format/large_web/" style="background-color: white;">http://hubblesite.org/newscenter/archive/releases/2003/04/image/a/format/large_web/</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Jurassic Space: Ancient Galaxies Come Together After Billions of Years</span></h1>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://hubblesite.org/newscenter/archive/releases/2010/08/image/a/format/web_print/" style="background-color: white;">http://hubblesite.org/newscenter/archive/releases/2010/08/image/a/format/web_print/</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Object Name:</strong> HCG 31</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Image Type:</strong> Astronomical</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold;">Credit:</span> <a href="http://www.nasa.gov/">NASA</a>, <a href="http://www.spacetelescope.org/">ESA</a>, S. Gallagher (The University of Western Ontario), and J. English (University of Manitoba)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">These four dwarf galaxies waited billions of years to come together, setting off a fireworks show as thousands of new star clusters come to life. The distorted galaxies are quickly producing massive, hot, young stars that are pumping out ultraviolet radiation, heating up surrounding gas clouds, and causing them to glow.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Such encounters between dwarf galaxies are normally seen billions of light-years away and therefore occurred billions of years ago. But these galaxies, members of Hickson Compact Group 31, are relatively nearby, only 166 million light-years away.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">LEIA MAIS EM <a href="http://hubblesite.org/newscenter/archive/releases/2010/08/image/a/" style="line-height: 19.1875px; text-align: justify;">http://hubblesite.org/newscenter/archive/releases/2010/08/image/a/</a></span></div>
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<a href="http://hubble.hq.eso.org/images/potw1349a/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">A members-only galaxy club</span></a></h2>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://hubble.hq.eso.org/static/archives/images/screen/potw1349a.jpg" height="330" width="640" /></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">This new Hubble image shows a handful of galaxies in the constellation of Eridanus (The River).</span><span style="font-family: Arial, Helvetica, sans-serif;"> NGC 1190</span><span style="font-family: Arial, Helvetica, sans-serif;">, shown here on the right of the frame, stands apart from the rest; it belong to an exclusive club known as Hickson Compact Group 22 (HCG 22).</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">There are four other members of this group, all of which lie out of frame: NGC 1189, NGC 1191, NGC 1192, and NGC 1199. The other galaxies shown here are nearby galaxies 2MASS J03032308-1539079 (centre), and dCAZ94 HCG 22-21 (left), both of which are not part of HCG 22.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">LEIA MAIS EM</span></div>
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<a href="http://hubble.hq.eso.org/images/potw/?search=Eridanus"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubble.hq.eso.org/images/potw/?search=Eridanus</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1190</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; text-decoration: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_lenticular" style="background-image: none; text-decoration: none;" title="Galáxia lenticular">lenticular</a> (S0) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Eridanus" style="background-image: none; text-decoration: none;" title="Eridanus">Eridanus</a>. Possui uma declinação de -15° 39' 44" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-image: none; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 3 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; text-decoration: none;" title="Hora">horas</a>, 03 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; text-decoration: none;" title="Minuto">minutos</a> e 26,0 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; text-decoration: none;" title="Segundo">segundos</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A galáxia <b>NGC 1190</b> foi descoberta em <a href="http://pt.wikipedia.org/wiki/1886" style="background-image: none; text-decoration: none;" title="1886">1886</a> por <a href="http://pt.wikipedia.org/wiki/Frank_Leavenworth" style="background-image: none; text-decoration: none;" title="Frank Leavenworth">Frank Leavenworth</a>.</span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_1190"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_1190</span></a></div>
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<a href="http://hubble.hq.eso.org/images/potw1103a/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Islands of stars in the river</span></a></h2>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The spiral galaxy <b>NGC 1345</b> and its loose and ragged arms dominate this rich image from the NASA/ESA Hubble Space Telescope. It is a member of the Eridanus Galaxy Cluster — a group of about 70 galaxies that lies 85 million light-years away in the constellation of Eridanus (the River). This region of the night sky is well populated with bright galaxies, with the Fornax Cluster of galaxies also nearby on the celestial sphere, although the two clusters are actually separated by about 20 million light-years. Collectively, they are known as the Fornax Supercluster or the Southern Supercluster.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">John Herschel discovered NGC 1345 in 1835 from South Africa. He described it as small and very faint and it is still far from easy to see it even with quite a large amateur telescope, where it appears as a small, circular fuzz.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">LEIA MAIS EM <a href="http://hubble.hq.eso.org/images/potw/?search=Eridanus" style="line-height: normal;">http://hubble.hq.eso.org/images/potw/?search=Eridanus</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1345</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; text-decoration: none;" title="Galáxia">galáxia</a> {{{typ}}} localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Eridanus" style="background-image: none; text-decoration: none;" title="Eridanus">Eridanus</a>. Possui uma declinação de -17° 46' 45" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-image: none;" title="Ascensão recta">ascensão recta</a> de 3 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; text-decoration: none;" title="Hora">horas</a>, 29 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; text-decoration: none;" title="Minuto">minutos</a> e 31,5 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; text-decoration: none;" title="Segundo">segundos</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A galáxia <b>NGC 1345</b> foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/11_de_Dezembro" style="background-image: none; text-decoration: none;" title="11 de Dezembro">11 de Dezembro</a> de <a href="http://pt.wikipedia.org/wiki/1835" style="background-image: none; text-decoration: none;" title="1835">1835</a> por <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-image: none; text-decoration: none;" title="John Herschel">John Herschel</a>.</span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_1345"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_1345</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">NASA Telescopes Help Discover Surprisingly Young Galaxy</span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Object Name:</strong> Abell 383</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold;">Credit:</span> <a href="http://www.nasa.gov/">NASA</a>, <a href="http://www.spacetelescope.org/">ESA</a>, J. Richard (Center for Astronomical Research/Observatory of Lyon, France), and J.-P. Kneib (Astrophysical Laboratory of Marseille, France)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="import" style="font-weight: bold;">Acknowledgment:</span> M. Postman (<a href="http://www.stsci.edu/">STScI</a>)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Astronomers have uncovered one of the youngest galaxies in the distant universe, with stars that formed 13.5 billion years ago, a mere 200 million years after the Big Bang. The finding addresses questions about when the first galaxies arose, and how the early universe evolved.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NASA's Hubble Space Telescope was the first to spot the newfound galaxy. Detailed observations from the W.M. Keck Observatory on Mauna Kea in Hawaii revealed the observed light dates to when the universe was only 950 million years old; the universe formed about 13.7 billion years ago.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">LEIA MAIS EM <a href="http://hubblesite.org/newscenter/archive/releases/2011/12/image/a/" style="line-height: 19.1875px; text-align: justify;">http://hubblesite.org/newscenter/archive/releases/2011/12/image/a/</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Lensing Galaxy Cluster Abell 383 (Annotated)</span></h2>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 19.1875px;"><span style="background-color: white; color: #073763; font-weight: bold; line-height: normal; text-align: -webkit-left;">Abell 383: Getting a Full Picture of an Elusive Subject</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Abell 383" src="http://chandra.harvard.edu/photo/2012/a383/a383_w33.jpg" /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://chandra.harvard.edu/photo/2012/a383/index.html" style="background-color: white;">http://chandra.harvard.edu/photo/2012/a383/index.html</a></span></div>
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<tr><td valign="top" width="60%"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">X-ray: NASA/CXC/Caltech/A.Newman et al/Tel Aviv/A.Morandi & M.Limousin; Optical: NASA/STScI, ESO/VLT, SDSS</span></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 16px; text-align: -webkit-left;">Two teams of astronomers have used data from NASA's Chandra X-ray Observatory and other telescopes to map the distribution of </span><a href="http://chandra.harvard.edu/xray_astro/dark_matter/" style="line-height: 16px; text-align: -webkit-left; text-decoration: none;">dark matter</a><span style="line-height: 16px; text-align: -webkit-left;"> in a galaxy cluster known as Abell 383, which is located about 2.3 billion light years from Earth.</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 16px;">LEIA MAIS EM </span><a href="http://chandra.harvard.edu/photo/2012/a383/index.html" style="text-align: justify;">http://chandra.harvard.edu/photo/2012/a383/index.html</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-weight: bold; text-align: -webkit-left;">Abell 521: A Galaxy Cluster Mash-up</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">X-ray (NASA/CXC/INAF/G.Brunetti et al.); Radio (NRAO/NSF/INAF/G.Brunetti et al.)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; line-height: 16px; text-align: -webkit-left;">This composite image shows the galaxy cluster Abell 521, located about 2.9 billion light years from Earth.</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 16px; text-align: -webkit-left;">LEIA MAIS EM </span><a href="http://chandra.harvard.edu/photo/2008/a521/index.html">http://chandra.harvard.edu/photo/2008/a521/index.html</a></span></div>
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<a href="http://upload.wikimedia.org/wikipedia/commons/thumb/0/0f/Earth%27s_Location_in_the_Universe_SMALLER_%28JPEG%29.jpg/1024px-Earth%27s_Location_in_the_Universe_SMALLER_%28JPEG%29.jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://upload.wikimedia.org/wikipedia/commons/thumb/0/0f/Earth%27s_Location_in_the_Universe_SMALLER_%28JPEG%29.jpg/1024px-Earth%27s_Location_in_the_Universe_SMALLER_%28JPEG%29.jpg</span></a><br />
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 143.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Author</span></td><td><a href="http://commons.wikimedia.org/wiki/User:Azcolvin429" style="background-image: none;" title="User:Azcolvin429"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Andrew Z. Colvin</span></a></td></tr>
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<a href="http://sg.hu/cikkek/88133/ujabb_jelek_utalnak_a_cp_sertesre"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://sg.hu/cikkek/88133/ujabb_jelek_utalnak_a_cp_sertesre</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O TEXTO ABAIXO É DE UMA SIMPLICIDADE ÍMPAR, a meu ver, NA EXPLICAÇÃO SOBRE AS ESTRUTURAS DO UNIVERSO.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A síntese e a tradução livre e literal foi realizada por mim, Janine.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="font-weight: normal;">Direitos autorais </span><span style="font-weight: normal; line-height: 13.5pt; text-align: start;">© 2013 A AstroGnom.</span></span></h3>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://de.spacechris.com/2013/05/12/was-ist-ein-void-die-strukturen-des-universums/#comments">http://de.spacechris.com/2013/05/12/was-ist-ein-void-die-strukturen-des-universums/#comments</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://de.spacechris.com/2013/05/12/ein-dankeschon-an-chris-hadfield/"><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial;">Ein ‘Dankeschön’ an Chris Hadfield</span></a> <span lang="EN-US">– Agradecimento a Chris Hadfield<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">von<span class="apple-converted-space"> </span></span><span class="fn"><a href="http://de.spacechris.com/author/admin/"><span style="text-align: start;"><span lang="EN-US">Spacechris</span></span></a></span><span class="fn"> <span lang="EN-US">– De </span></span><a href="http://de.spacechris.com/author/admin/"><span lang="EN-US">http://de.spacechris.com/author/admin/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="font-weight: normal;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Was ist ein “Void”? Die Strukturen des Universums<o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">What is a "Void"?</span><span lang="EN-US"> </span><span lang="EN-US">The </span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">structures of the universe<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Síntese e tradução livre e literal realizada a partir da versão inglesa por Janine Milward<o:p></o:p></span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O que é um “Void”? As Estruturas do Universo<o:p></o:p></span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É preciso que saibamos que nosso universo não é sem-estrutura. Mesmo em escalas imensas, uma estrutura pode ser encontrada. Para melhor compreendermos essa realidade, temos que fazer uma enorme viagem.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ao fazermos um ZOOM a partir da Terra e em direção à imensidão do universo, estaremos primeiramente encontrando 7 planetas que, juntamente com nossa Terra, se movimentam em torno de uma estrela, o Sol. Planetas e Sol formam o Sistema Solar. <o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando o zoom se amplia, descobrimos muitas estrelas, outros sistemas solares. Estes sistemas solares vivenciam em conjunto uma estrutura chamada Galáxia. Nossa Galáxia é conhecida por nós como Via Lactea. Quando nosso zoom se amplia ainda mais, encontramos uma vizinhança de nossa Galáxia, algumas outras galáxias – como, por exemplo, a galáxia Andromeda. Estas galáxias foram Grupos ou Aglomerados. A Via Lactea e Andromeda e outras galáxias menores em nossa vizinhança formam o chamado Grupo Local. O Grupo Local contém cerca de 500 galáxias e possui um diâmetro aproximado de 7 milhões de anos-luz.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ao aprofundarmos o zoom, encontraremos muitas dessas galáxias e que vão formando estruturas. Os Aglomerados de galáxias se encontram com outros Aglomerados e são formados aquilo que denominamos de Superaglomerados. Nosso Grupo Local pertence ao Superaglomerado Virgo. Esse Superaglomerado possui cerca de 200 Aglomerados de galáxias e possui um diâmetro de cerca de 200 milhões de anos-luz.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Porém, as dimensões continuam em suas amplitudes e quando usamos o zoom para ainda além os Superaglomerados, podemos notar que estes Superaglomerados também formam estruturas que são chamadas de Filamentos. Um famoso Filamento é referido como A Grande Muralha (The Great Wall). A Grande Muralha possui um comprimento aproximado de 500 milhões de anos-luz e possui altura de cerca de 300 milhões de anos-luz e 15 milhões de anos-luz de espessura.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ainda mais distante, estaremos encontrando a Grande Muralha Sloan (Sloan Great Wall) – também um Filamento porém de dimensão inteiramente diferente. A Grande Muralha Sloan possui um comprimento aproximado de 1.3 bilhões de anos-luz!<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">Agora que esclarecemos sobre as estruturas no espaço, podemos começar a conversar sobre o Void, o Vazio. Mencionamos as maiores estruturas do universo – os Filamentos todos ligados entre si como se fosse uma malha de favo de mel. Entre os Filamentos, existe o Void, o Nada, o Vazio. Não existe nada no Vazio, nem gás, nem poeira e certamente nem estrelas ou planetas. No entanto, acredita-se que a tão comentada Matéria Escura exista nos Voids – mesmo que não emita luz ou radiação quaisquer e que, portanto, não é visível.</span><span style="font-family: Arial, sans-serif; font-size: 9pt;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif; font-size: 9pt;"> </span><a href="http://de.spacechris.com/wp-content/uploads/2013/05/BD1BFD36787B70613DED5EA727862.jpg" style="text-align: start; text-decoration: none;"><img alt="Filament-Struktur und Voids" class="size-medium wp-image-2079" src="http://de.spacechris.com/wp-content/uploads/2013/05/BD1BFD36787B70613DED5EA727862-300x180.jpg" height="180" style="border: 1px solid rgb(204, 204, 204); height: auto; margin: 4px 4px 0px; max-width: 98.5%; padding: 0px;" width="300" /></a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Die erkennbaren “Fäden” sind die Filamente, welche aus den Superhaufen bestehen. Die leeren Zwischenräume sind die Voids. (Quelle: MPA Garching)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The recognizable "threads" are the filaments, which consist of the supercluster.</span><span lang="EN-US"> </span><span lang="EN-US">The empty spaces are the voids.(Source: MPA Garching)<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os "fios" reconhecíveis são os filamentos, que consistem na superaglomerados.<span class="apple-converted-space"> </span>Os espaços vazios são os espaços vazios.<span class="apple-converted-space"> </span>(Fonte: MPA Garching)<o:p></o:p></span></div>
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<a href="http://de.spacechris.com/2013/05/12/was-ist-ein-void-die-strukturen-des-universums"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://de.spacechris.com/2013/05/12/was-ist-ein-void-die-strukturen-des-universums</span></a></div>
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<a href="http://www.whillyard.com/science-pages/voids.html"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.whillyard.com/science-pages/voids.html</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Cosmic voids, and supervoids, are large volumes of space that are devoid of matter. This includes normal matter, in the form of galaxies, and dark matter. Initially, astronomers were not sure if the voids contained dark matter, even though there were no galaxies, but recent observations show that the halos of dark matter are not present. The filamentary structure of galactic superclusters surrounds the voids. While space is mostly empty, voids are large volumes, tens of megaparsecs across. The largest confirmed supervoids are about 100 Mpc (325 million light-years) or more across . The larger known voids include the Boötes Supervoid, and the Northern and Southern Local Supervoids. To explain the cold spot in the cosmic microwave background (CMB), some astronomers propose a huge supervoid, tentatively dubbed the Eridanus or Great supervoid. The Capricornus void is another disputed void, but would be around 230 Mpc across. This link has some of the latest information on<a href="http://www.universetoday.com/2008/08/17/dark-matter-is-missing-from-cosmic-voids/" target="_blank">cosmic voids</a>. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The Eridanus Supervoid, or Great Void, is conjectural, and has been suggested as a way to explain the "cold spot" in the cosmic microwave background radiation, or CMB. This would be an extraordinarily large region of the universe, at least 150 Mpc or 500 million light-years across, and possibly twice this figure. It is also very distant at between 1.8 Gpc and 3 Gpc (6 to 10 billion light-years). Many astronomers and cosmologists do not accept the supervoid theory for the aberration in the CMB, but many of the alternatives are even more astounding including cosmic textures and parallel universes. So the jury remains out on this one. </span></div>
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<a href="http://www.whillyard.com/science-pages/voids.html"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.whillyard.com/science-pages/voids.html</span></a></div>
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<a href="http://en.wikipedia.org/wiki/Void_(astronomy)"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://en.wikipedia.org/wiki/Void_(astronomy)</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">In <a href="http://en.wikipedia.org/wiki/Astronomy" style="background-image: none; text-decoration: none;" title="Astronomy">astronomy</a>, <b>voids</b> are the vast empty spaces between <a href="http://en.wikipedia.org/wiki/Galaxy_filament" style="background-image: none; text-decoration: none;" title="Galaxy filament">filaments</a> (the largest-scale structures in the <a href="http://en.wikipedia.org/wiki/Universe" style="background-image: none; text-decoration: none;" title="Universe">Universe</a>), which contain <a href="http://en.wikipedia.org/wiki/Void_galaxy" style="background-image: none; text-decoration: none;" title="Void galaxy">very few</a>, or no, <a href="http://en.wikipedia.org/wiki/Galaxy" style="background-image: none; text-decoration: none;" title="Galaxy">galaxies</a>. They were first discovered in 1978 during a pioneering study by Stephen Gregory and <a href="http://en.wikipedia.org/wiki/Laird_A._Thompson" style="background-image: none; text-decoration: none;" title="Laird A. Thompson">Laird A. Thompson</a> at the <a href="http://en.wikipedia.org/wiki/Kitt_Peak_National_Observatory" style="background-image: none; text-decoration: none;" title="Kitt Peak National Observatory">Kitt Peak National Observatory</a>.<sup class="reference" id="cite_ref-1" style="color: #fff2cc; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Void_(astronomy)#cite_note-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup> Voids typically have a diameter of 11 to 150 <a href="http://en.wikipedia.org/wiki/Parsec#Megaparsecs_and_gigaparsecs" style="background-image: none; text-decoration: none;" title="Parsec">megaparsecs</a>; particularly large voids, defined by the absence of rich <a href="http://en.wikipedia.org/wiki/Supercluster" style="background-image: none; text-decoration: none;" title="Supercluster">superclusters</a>, are sometimes called "supervoids". Voids located in high-density environments are smaller than voids situated in low-density spaces of the universe.<sup class="reference" id="cite_ref-2" style="color: #fff2cc; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Void_(astronomy)#cite_note-2" style="background-image: none; text-decoration: none; white-space: nowrap;">[2]</a></sup> Voids are believed to have been formed by <a href="http://en.wikipedia.org/wiki/Baryon_acoustic_oscillations" style="background-image: none; text-decoration: none;" title="Baryon acoustic oscillations">baryon acoustic oscillations</a> in the <a href="http://en.wikipedia.org/wiki/Big_Bang" style="background-image: none; text-decoration: none;" title="Big Bang">Big Bang</a>—collapses of mass followed by implosions of the compressed <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Baryonic_matter" style="background-image: none; text-decoration: none;" title="Baryonic matter">baryonic matter</a>. Starting from initially small<a href="http://en.wikipedia.org/wiki/Anisotropy" style="background-image: none; text-decoration: none;" title="Anisotropy">anisotropies</a> due to <a href="http://en.wikipedia.org/wiki/Quantum_fluctuation" style="background-image: none; text-decoration: none;" title="Quantum fluctuation">quantum fluctuations</a> in the early Universe, the anisotropies grew larger in scale over time. Regions of higher density collapsed more rapidly under gravity, eventually resulting in the large-scale, foam-like structure or “cosmic web” of voids and galaxy filaments seen today.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Voids appear to correlate with the observed temperature of the <a href="http://en.wikipedia.org/wiki/Cosmic_microwave_background" style="background-image: none; text-decoration: none;" title="Cosmic microwave background">cosmic microwave background</a> (CMB), due to the <a href="http://en.wikipedia.org/wiki/Sachs%E2%80%93Wolfe_effect" style="background-image: none; text-decoration: none;" title="Sachs–Wolfe effect">Sachs–Wolfe effect</a>. Colder regions correlate with voids, whereas hotter regions correlate with filaments, because of <a href="http://en.wikipedia.org/wiki/Gravitational_redshift" style="background-image: none; text-decoration: none;" title="Gravitational redshift">gravitational redshifting</a>. As the Sachs–Wolfe effect is only significant if the Universe is dominated by <a href="http://en.wikipedia.org/wiki/Radiation" style="background-image: none; text-decoration: none;" title="Radiation">radiation</a> or <a href="http://en.wikipedia.org/wiki/Dark_energy" style="background-image: none; text-decoration: none;" title="Dark energy">dark energy</a>, the existence of voids is significant in providing physical evidence for dark energy. <sup class="reference" id="cite_ref-3" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Void_(astronomy)#cite_note-3" style="background-image: none; text-decoration: none; white-space: nowrap;">[3]</a></sup></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.sttff.net/AST_MAP010.html" style="background-color: white;">http://www.sttff.net/AST_MAP010.html</a></span></div>
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<span style="line-height: 18px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The Virgo Cluster, however, is merely a minor </span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">member of a much larger whole. The </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">neighboring superclusters are massive, most </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">of them three and four times larger than the </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Virgo Cluster and spanning a distance of some </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">100 million light years. These leviathans in </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">turn form massive chains and walls that </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">weave throughout the cosmos. Between </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">them exists, quite literally, nothing. These </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">giant voids are hundreds of millions of light </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">years in diameter and most of them contain </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">absolutely nothing at all. No stars. No galaxy.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18px; text-align: start;">No matter.</span></span></div>
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<span style="line-height: 18px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">LEIA MAIS EM </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span style="line-height: 19.1875px;">The </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Eridanus_Supervoid" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Eridanus Supervoid">Eridanus Supervoid</a></b><span style="line-height: 19.1875px;"><b> </b>is the largest </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Supervoid" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Supervoid">supervoid</a><span style="line-height: 19.1875px;"> (an area of the </span><a href="http://en.wikipedia.org/wiki/Universe" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Universe">universe</a><span style="line-height: 19.1875px;"> devoid of</span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Galaxies" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Galaxies">galaxies</a><span style="line-height: 19.1875px;">) discovered as of 2007. At a diameter of about one billion </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Light_year" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Light year">light years</a><span style="line-height: 19.1875px;"> it is much larger than any other known void. It was discovered by linking a "cold spot" in the </span><a href="http://en.wikipedia.org/wiki/Cosmic_microwave_background" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Cosmic microwave background">cosmic microwave background</a><span style="line-height: 19.1875px;"> to an absence of </span><a href="http://en.wikipedia.org/wiki/Radio_galaxy" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Radio galaxy">radio galaxies</a><span style="line-height: 19.1875px;"> in data of the </span><a href="http://en.wikipedia.org/wiki/United_States" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="United States">United States</a><span style="line-height: 19.1875px;"> </span><a href="http://en.wikipedia.org/wiki/National_Radio_Astronomy_Observatory" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="National Radio Astronomy Observatory">National Radio Astronomy Observatory</a><span style="line-height: 19.1875px;">'s </span><a href="http://en.wikipedia.org/wiki/Very_Large_Array" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Very Large Array">Very Large Array</a><span style="line-height: 19.1875px;"> Sky Survey.</span><sup class="reference" id="cite_ref-2" style="font-weight: normal; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)#cite_note-2" style="background-image: none; text-decoration: none; white-space: nowrap;">[2]</a></sup><span style="line-height: 19.1875px;"> There is some speculation that the void may be due to </span><a href="http://en.wikipedia.org/wiki/Quantum_entanglement" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Quantum entanglement">quantum entanglement</a><span style="line-height: 19.1875px;"> between </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Our_universe" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Our universe">our universe</a><span style="line-height: 19.1875px;"> and </span><a href="http://en.wikipedia.org/wiki/Multiverse" style="background-image: none; line-height: 19.1875px; text-decoration: none;" title="Multiverse">another</a><span style="line-height: 19.1875px;">.</span><sup class="reference" id="cite_ref-3" style="font-weight: normal; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)#cite_note-3" style="background-image: none; text-decoration: none; white-space: nowrap;">[3]</a></sup><sup class="reference" id="cite_ref-4" style="font-weight: normal; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)#cite_note-4" style="background-image: none; text-decoration: none; white-space: nowrap;">[4]</a></sup></span></div>
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<pre><span style="white-space: normal;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.atlasoftheuniverse.com/nearsc.html" style="text-align: left;">http://www.atlasoftheuniverse.com/nearsc.html</a></span></span><div style="white-space: normal;">
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<img alt="Massive voids separate galaxy superclusters across the Universe" src="http://i1-news.softpedia-static.com/images/news2/Large-Cosmic-Void-May-Be-a-Black-Hole-2.jpg" /></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a href="http://news.softpedia.com/newsImage/Large-Cosmic-Void-May-Be-a-Black-Hole-2.jpg/" style="background-color: white;">http://news.softpedia.com/newsImage/Large-Cosmic-Void-May-Be-a-Black-Hole-2.jpg/</a></span></h3>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="text-align: start; white-space: normal;">Image comment:</b><span style="text-align: start; white-space: normal;"> Massive voids separate galaxy superclusters across the Universe</span> <b style="text-align: start; white-space: normal;">Image credits:</b><span style="text-align: start; white-space: normal;"> NASA / ESA</span></span></div>
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<strong style="background-color: white; line-height: 14px; text-align: justify;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">In a new study, a team of astronomers proposes that a so-called Universe-in-mas black hole is responsible for the development of</span><span style="font-family: Arial, Helvetica, sans-serif;"> an incredibly-large void in the constellation Eridanus.</span></span></strong></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 14px; white-space: normal;"><b> </b></span><a href="http://news.softpedia.com/news/Large-Cosmic-Void-May-Be-a-Black-Hole-201721.shtml">http://news.softpedia.com/news/Large-Cosmic-Void-May-Be-a-Black-Hole-201721.shtml</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span class="mw-headline" id="Supervoid">Supervoid</span><span class="mw-editsection" style="-webkit-user-select: none; color: #fff2cc; display: inline-block; font-weight: normal; line-height: 1em; margin-left: 1em; padding-right: 0.25em; unicode-bidi: -webkit-isolate; vertical-align: baseline; white-space: nowrap;"><span class="mw-editsection-bracket">[</span><a href="http://en.wikipedia.org/w/index.php?title=Eridanus_(constellation)&action=edit&section=3" style="background-image: none; text-decoration: none;" title="Edit section: Supervoid">edit</a><span class="mw-editsection-bracket">]</span></span></span></h3>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>The <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Eridanus_Supervoid" style="background-image: none; text-decoration: none;" title="Eridanus Supervoid">Eridanus Supervoid</a></b> is the largest <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Supervoid" style="background-image: none; text-decoration: none;" title="Supervoid">supervoid</a> (an area of the <a href="http://en.wikipedia.org/wiki/Universe" style="background-image: none; text-decoration: none;" title="Universe">universe</a> devoid of<a class="mw-redirect" href="http://en.wikipedia.org/wiki/Galaxies" style="background-image: none; text-decoration: none;" title="Galaxies">galaxies</a>) discovered as of 2007. At a diameter of about one billion <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Light_year" style="background-image: none; text-decoration: none;" title="Light year">light years</a> it is much larger than any other known void. It was discovered by linking a "cold spot" in the <a href="http://en.wikipedia.org/wiki/Cosmic_microwave_background" style="background-image: none; text-decoration: none;" title="Cosmic microwave background">cosmic microwave background</a> to an absence of <a href="http://en.wikipedia.org/wiki/Radio_galaxy" style="background-image: none; text-decoration: none;" title="Radio galaxy">radio galaxies</a> in data of the <a href="http://en.wikipedia.org/wiki/United_States" style="background-image: none; text-decoration: none;" title="United States">United States</a> <a href="http://en.wikipedia.org/wiki/National_Radio_Astronomy_Observatory" style="background-image: none; text-decoration: none;" title="National Radio Astronomy Observatory">National Radio Astronomy Observatory</a>'s <a href="http://en.wikipedia.org/wiki/Very_Large_Array" style="background-image: none; text-decoration: none;" title="Very Large Array">Very Large Array</a> Sky Survey.<sup class="reference" id="cite_ref-2" style="color: #fff2cc; font-weight: normal; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)#cite_note-2" style="background-image: none; text-decoration: none; white-space: nowrap;">[2]</a></sup> There is some speculation that the void may be due to <a href="http://en.wikipedia.org/wiki/Quantum_entanglement" style="background-image: none; text-decoration: none;" title="Quantum entanglement">quantum entanglement</a> between <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Our_universe" style="background-image: none; text-decoration: none;" title="Our universe">our universe</a> and <a href="http://en.wikipedia.org/wiki/Multiverse" style="background-image: none; text-decoration: none;" title="Multiverse">another</a>.<sup class="reference" id="cite_ref-3" style="color: #fff2cc; font-weight: normal; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)#cite_note-3" style="background-image: none; text-decoration: none; white-space: nowrap;">[3]</a></sup><sup class="reference" id="cite_ref-4" style="color: #fff2cc; font-weight: normal; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Eridanus_(constellation)#cite_note-4" style="background-image: none; text-decoration: none; white-space: nowrap;">[4]</a></sup></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">See also: <a class="mw-redirect" href="http://en.wikipedia.org/wiki/WMAP_cold_spot" style="background-image: none; text-decoration: none;" title="WMAP cold spot">WMAP cold spot</a></span></div>
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<tr><td valign="top" width="416"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><b>Astronomers have found an enormous void in space</b></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><b style="background-color: white;"> that measures nearly a billion light-years across.</b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">It is empty of both normal matter - such as galaxies and stars -</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"> and the mysterious "dark matter" that cannot be seen directly with telescopes.</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"> The "hole" is located in the direction of the Eridanus constellation</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"> and has been identified in data </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">from a survey of the sky made at radio wavelengths.</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; font-size: small;"> <a href="http://news.bbc.co.uk/2/hi/science/nature/6962185.stm">http://news.bbc.co.uk/2/hi/science/nature/6962185.stm</a></span></span></td></tr>
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<pre style="white-space: normal;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"></span><h3 class="entry-header" style="border: 0px; line-height: 19px; margin: 1px 0px 10px;">
<a href="http://www.dailygalaxy.com/my_weblog/2010/08/the-eridanus-void-does-a-megamassive-black-hole-onebillion-light-years-across-exist-a-galaxy-most-po.html" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">The Eridanus Void: Does a MegaMassive Black Hole One-Billion Light Years Across Exist? (A 'Galaxy' Most Popular)</span></a></h3>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">n the Constellation Eridanus appears to be improbable given current cosmological models. A radical and controversial theory proposes that it is a "universe-in-mass black hole" rather than hypothetical dark matter responsible for the phenomenon described as the expanding-accelerating universe. This radical theory of cosmology suggests that stars at the edge of the Hubble length universe are being consumed by a universe-in-mass black hole.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">In August of 2007, astronomers at the University of Minnesota located a gigantic hole in the universe. This empty space, stretching nearly a billion light-years across, is devoid of any matter such as galaxies, stars, and gas, and neither does it contain the strange and mysterious dark matter, which can be detected but not seen.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: normal; text-align: left;">by </span><b style="border: 0px; line-height: normal; margin: 0px; padding: 0px; text-align: left;"><a href="http://www.newscientist.com/search?rbauthors=David+Shiga" style="border: 0px; margin: 0px; padding: 0px; text-decoration: none;">David Shiga</a></b></span></div>
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<span style="line-height: normal; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The new survey mapped the positions of more than 100,000 galaxies. The black strips are areas the survey did not cover because matter in our own galaxy blocked the view (Illustration: Chris Fluke/Swinburne University of Technology)</span></span></div>
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<span style="text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Enormous cosmic voids and giant concentrations of matter have been observed in a new galaxy survey, one of the biggest completed so far. One of the voids is so large that it is difficult to explain where it came from.</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The survey also found some enormous voids – regions of space that are relatively empty, including one that is about 3.5 billion light years across.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">"This is as big as I've ever seen," survey team member <a href="http://www.cfa.harvard.edu/~huchra/" style="border: 0px; margin: 0px; padding: 0px; text-decoration: none;" target="ns">John Huchra</a> of the Harvard-Smithsonian Center for Astrophysics told <b style="border: 0px; margin: 0px; padding: 0px;">New Scientist</b>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Another <a href="http://www.newscientist.com/article/dn12546-biggest-void-in-space-is-1-billion-light-years-across.html" style="border: 0px; margin: 0px; padding: 0px; text-decoration: none;">large void</a> about 1 billion light years across was discovered previously.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">In fact the newly found void is so large that it is difficult to fit into our present understanding of the universe on the largest scales. Computer simulations show that gravity causes galaxies and galaxy clusters to get closer together over time, with voids growing between the clusters.</span></div>
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<a href="http://www.newscientist.com/article/dn16903-new-cosmic-map-reveals-colossal-structures.html#.UqoNRtJDtx2"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.newscientist.com/article/dn16903-new-cosmic-map-reveals-colossal-structures.html#.UqoNRtJDtx2</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Biggest void in space is 1 billion light years across</span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"> by <span style="border: 0px; margin: 0px; padding: 0px;"><a href="http://www.newscientist.com/search?rbauthors=Anil+Ananthaswamy" style="border: 0px; margin: 0px; padding: 0px; text-decoration: none;">Anil Ananthaswamy</a></span></span></h1>
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<a href="http://www.newscientist.com/data/images/ns/cms/dn12546/dn12546-2_519.jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.newscientist.com/data/images/ns/cms/dn12546/dn12546-2_519.jpg</span></a></div>
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<span style="line-height: normal; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The biggest known hole in the universe has left a cold-spot in the cosmic microwave radiation (Illustration: Bill Saxton, NRAO/AUI/NSF, NASA)</span></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Radio astronomers have found the biggest hole ever seen in the universe. The void, which is nearly a billion light years across, is empty of both normal matter and dark matter. The finding challenges theories of large-scale structure formation in the universe.</span></span></h1>
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<span style="text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The void, which is about 6 billion to 10 billion light years away, is considerably larger than any found before. Until now, optical surveys have found no voids larger than 80 megaparsecs wide - making the new hole 40 times larger in volume than the previous record holder.</span></span></div>
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<span style="text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Computer simulations that recreate the formation of clusters and super-clusters have never seen voids of this size. That could be because modellers have not simulated large enough volumes to see such a void, says Rudnick. If they did, maybe a void would emerge. "It is an open question whether this will create problems for structure formation," he says.</span></span></div>
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<span style="text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">LEIA MAIS EM </span></span></div>
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<a href="http://www.newscientist.com/article/dn12546-biggest-void-in-space-is-1-billion-light-years-across.html#.UqoOntJDtx0"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.newscientist.com/article/dn12546-biggest-void-in-space-is-1-billion-light-years-across.html#.UqoOntJDtx0</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Acessando a Animação abaixo, você poderá saber melhor sobre </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">ERIDANUS SUPERVOID</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> (e também sobre Fornax Cluster):</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: normal;">The Scale of the Universe - Interactive </b><span style="line-height: normal;"></span><br style="line-height: normal;" /><b style="line-height: normal;">Flash Animation Credit & Copyright: </b><span style="line-height: normal;"></span><a href="http://htwins.net/" style="line-height: normal;">Cary & Michael Huang</a></span></div>
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<a href="http://apod.nasa.gov/apod/ap120312.html"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://apod.nasa.gov/apod/ap120312.html</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Explanation: </b>What does the universe look like on small scales? On large scales? <a href="http://apod.nasa.gov/apod/ap100725.html">Humanity</a> is discovering that the universe is a very different place on every proportion that has been explored. For example, so far as we know, every tiny proton is <a href="http://en.wikipedia.org/wiki/Identical_particles">exactly the same</a>, but every <a href="http://apod.nasa.gov/apod/ap120107.html">huge galaxy</a> is different. On more familiar scales, a small glass table top to a human is a <a href="http://en.wikipedia.org/wiki/Fantastic_Voyage">vast plane</a> of strange smoothness to a <a href="http://www.youtube.com/watch?v=47CIdUld8eQ">dust mite</a> -- possibly <a href="http://www.wisegeek.com/where-does-dust-come-from.htm">speckled</a> with cell boulders. Not all scale lengths are <a href="http://www.youtube.com/watch?v=4PKjF7OumYo">well explored</a> -- what happens to the smallest mist droplets you sneeze, for example, is a topic of active research -- and possibly useful to know to help <a href="http://en.wikipedia.org/wiki/Airborne_disease">stop the spread</a> of disease. The <a href="http://htwins.net/scale2/">above interactive flash animation</a>, a modern version of the classic video <a href="http://apod.nasa.gov/apod/ap110201.html">Powers of Ten</a>, is a new window to many of the <a href="http://apod.nasa.gov/apod/ap100120.html">known scales</a> of our universe. By moving the scroll bar across the bottom, you can explore a <a href="http://www.kruger-2-kalahari.com/images/the-long-the-tall-and-the-short-21373953.jpg">diversity of sizes</a>, while clicking on different items will bring up descriptive information.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Authors & editors: </b><a href="http://www.phy.mtu.edu/faculty/Nemiroff.html">Robert Nemiroff</a> (<a href="http://www.phy.mtu.edu/">MTU</a>) & <a href="http://antwrp.gsfc.nasa.gov/htmltest/jbonnell/www/bonnell.html">Jerry Bonnell</a> (<a href="http://www.astro.umd.edu/">UMCP</a>)<br /><b>NASA Official: </b>Phillip Newman <a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply">Specific rights apply</a>.<br /><a href="http://www.nasa.gov/about/highlights/HP_Privacy.html">NASA Web Privacy Policy and Important Notices</a><br /><b>A service of:</b> <a href="http://astrophysics.gsfc.nasa.gov/">ASD</a> at <a href="http://www.nasa.gov/">NASA</a> / <a href="http://www.nasa.gov/centers/goddard/">GSFC</a><br /><b>&</b> <a href="http://www.mtu.edu/">Michigan Tech. U.</a></span></center>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NA CONSTELAÇÃO DE ERIDANUS, O RIO ERIDANO:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif; font-size: small;">Named Stars Index - </span><span style="font-family: Arial, Helvetica, sans-serif; font-size: small;">The Night Sky Atlas</span></span></h1>
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<tr><td colspan="5" height="36" valign="bottom"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Eridanus: Visible in July before dawn, to March after dusk, best in November.</span></td></tr>
<tr><td class="starName" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=2.971&declination=-40.304&viewAngle=25"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Acamar</span></a></td><td class="starGreek" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">θ2</span></td><td class="starGreek" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Theta 2</span></td><td class="description" style="padding-left: 5px; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">´end of the river´ (before Achernar was added)</span></td><td class="starName" style="padding-left: 5px; padding-right: 5px;"><a href="http://www.astro.uiuc.edu/~jkaler/sow/acamar.html" target="starnotes" title="Jim Kaler´s star notes for Acamar"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Jim Kaler Notes</span></a></td></tr>
<tr><td class="starName" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=1.629&declination=-57.237&viewAngle=25"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Achernar</span></a></td><td class="starGreek" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">α</span></td><td class="starGreek" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Alpha</span></td><td class="description" style="padding-left: 5px; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">´end of the river´</span></td><td class="starName" style="padding-left: 5px; padding-right: 5px;"><a href="http://www.astro.uiuc.edu/~jkaler/sow/achernar.html" target="starnotes" title="Jim Kaler´s star notes for Achernar"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Jim Kaler Notes</span></a></td></tr>
<tr><td class="starName" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=2.940&declination=-8.898&viewAngle=25"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Azha</span></a></td><td class="starGreek" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">η</span></td><td class="starGreek" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Eta</span></td><td class="description" style="padding-left: 5px; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">´hatching place´</span></td><td class="starName" style="padding-left: 5px; padding-right: 5px;"><a href="http://www.astro.uiuc.edu/~jkaler/sow/azha.html" target="starnotes" title="Jim Kaler´s star notes for Azha"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Jim Kaler Notes</span></a></td></tr>
<tr><td class="starName" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=5.131&declination=-5.086&viewAngle=25"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Cursa</span></a></td><td class="starGreek" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">β</span></td><td class="starGreek" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Beta</span></td><td class="description" style="padding-left: 5px; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">´chair/footstool of Orion´</span></td><td class="starName" style="padding-left: 5px; padding-right: 5px;"><a href="http://www.astro.uiuc.edu/~jkaler/sow/cursa.html" target="starnotes" title="Jim Kaler´s star notes for Cursa"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Jim Kaler Notes</span></a></td></tr>
<tr><td class="starName" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=3.721&declination=-9.763&viewAngle=25"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Rana</span></a></td><td class="starGreek" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">δ</span></td><td class="starGreek" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Delta</span></td><td class="description" style="padding-left: 5px; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">´frog´</span></td><td class="starName" style="padding-left: 5px; padding-right: 5px;"><a href="http://www.astro.uiuc.edu/~jkaler/sow/rana.html" target="starnotes" title="Jim Kaler´s star notes for Rana"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Jim Kaler Notes</span></a></td></tr>
<tr><td class="starName" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=3.967&declination=-13.509&viewAngle=25"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Zaurak</span></a></td><td class="starGreek" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">γ</span></td><td class="starGreek" nowrap="1" style="padding-left: 5px; padding-right: 5px;" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Gamma</span></td><td class="description" style="padding-left: 5px; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">´boat´</span></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">DSO Names - The Night Sky Atlas</span></h1>
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<tr><td colspan="5" height="36" valign="bottom"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Eridanus: Visible in August before dawn, to April after dusk, best in December.</span></td></tr>
<tr><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; vertical-align: top;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=4.2383&declination=-12.7383&viewAngle=20.0"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Cleopatra´s Eye</span></a></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="150"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">NGC1535</span></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">04h 14.3m</span></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">-12° 44.3´</span></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="300"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">(Alicia Tristan)</span></td></tr>
<tr><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; vertical-align: top;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=4.4133&declination=-21.1833&viewAngle=20.0"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Eridanus Globular Cluster</span></a></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="150"></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">04h 24.8m</span></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">-21° 11.0´</span></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="300"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">(Sky Catalogue 2000.0)</span></td></tr>
<tr><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; vertical-align: top;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=3.4067&declination=-21.5433&viewAngle=20.0"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Holmberg VI</span></a></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="150"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">NGC1325A</span></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">03h 24.4m</span></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">-21° 32.6´</span></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="300"></td></tr>
<tr><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; vertical-align: top;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=3.9867&declination=-21.3333&viewAngle=20.0"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Horologium Dwarf</span></a></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="150"></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">03h 59.2m</span></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">-21° 20.0´</span></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="300"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">also Schuster´s Spiral</span></td></tr>
<tr><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; vertical-align: top;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=3.9867&declination=-21.3333&viewAngle=20.0"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Schuster´s Spiral</span></a></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="150"></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">03h 59.2m</span></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">-21° 20.0´</span></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="300"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">also Horologium Dwarf</span></td></tr>
<tr><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; vertical-align: top;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=5.115&declination=-7.2167&viewAngle=20.0"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Witch Head Nebula</span></a></td><td class="data" style="padding-left: 5px; padding-right: 5px; vertical-align: top;" width="150"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">IC2118</span></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">05h 06.9m</span></td><td class="data" nowrap="1" style="padding-left: 5px; padding-right: 5px; text-align: right; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">-07° 13.0´<br /><br /><a href="http://www.nightskyatlas.com/dsoNames.jsp">http://www.nightskyatlas.com/dsoNames.jsp</a></span><br />
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<b><span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Principal Stars of Eridanus - The Night Sky Atlas<o:p></o:p></span></span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a href="http://www.nightskyatlas.com/stardata.jsp?id=ERI"><span lang="EN-US">http://www.nightskyatlas.com/stardata.jsp?id=ERI</span></a><o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Multiple Stars of Eridanus - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">NGC Objects in Eridanus - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a href="http://www.nightskyatlas.com/ngcData.jsp?id=ERI"><span lang="EN-US">http://www.nightskyatlas.com/ngcData.jsp?id=ERI</span></a><o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">IC Objects in Eridanus - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Abell Galaxy Clusters - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a href="http://www.nightskyatlas.com/catAbell.jsp"><span lang="EN-US">http://www.nightskyatlas.com/catAbell.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="https://www.raremaps.com/gallery/detail/31524op/_Eridanus_Stars_Heightened_in_Gold/Bayer.html">https://www.raremaps.com/gallery/detail/31524op/_Eridanus_Stars_Heightened_in_Gold/</a><a href="https://www.raremaps.com/gallery/detail/31524op/_Eridanus_Stars_Heightened_in_Gold/Bayer.html">Bayer.html</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong style="color: #fff2cc; text-align: start;">Map Maker: </strong><span style="color: #fff2cc; text-align: start;"></span><a href="https://www.raremaps.com/gallery/browse/creator_id/247" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-align: start; text-decoration: none;">Johann Bayer</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas – As Constelações - são como janelas que se abrem para a infinitude do universo e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e sendo por nossa mente conscientizado. Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">COM UM ABRAÇO ESTRELADO,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>REFERÊNCIAS BIBLIOGRÁFICAS impressas:</b><o:p></o:p></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">COMPILAÇÃO E TRADUÇÃO literal (quando necessária) de Janine Milward:<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As Cartas Celestes foram realizadas por Mario Jaci Monteiro e escaneadas por Janine<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- </span><b>Mario Jaci Monteiro</b> , <b>As Constelações, Cartas Celestes</b> -<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- <b>Wil Tirion - Atlas of the Night Sky</b> - The Hamlyn Publishing Group Limited, London, England</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- <b>Antonin Rükl - The Hamlyn Encyclopedia of Stars & Planets</b> - The Hamlyn Publishng Group Limited, London, England</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- <b>Richard Hinckley Allen, Star Names, Their Lore and Meaning</b>, Dover Publications, Inc, New York, USA</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- <b>Bernard Pellequer - Pequeno Guia do Céu</b> - Editora Martins Fontes, São Paulo, Brasil</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- <b>Identificação do Céu</b> (Livro que foi sendo revisado e reeditado algumas vezes) de autoria de <b>Fernando Vieira</b>,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Secretaria Municipal de Cultura, Fundação Planetário da Cidade do Rio de Janeiro<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(com dedicatória do próprio autor para mim em Curso de Identificação do Céu,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em 30/07/1999))<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do <b>Atlas Celeste</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">de autoria de <b>Ronaldo Rogério de Freitas Mourão</b>,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(com dedicatória do próprio autor para mim<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em evento realizado no Museu de Astronomia do Rio de Janeiro,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em 16/06/1989)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As Cartas Celestes foram realizadas por Mario Jaci Monteiro e escaneadas por Janine<span lang="PT"><br /></span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- </span><b>Mario Jaci Monteiro</b> , <b>As Constelações, Cartas Celestes</b> -<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC - com dedicatória do autor para mim, em março de 2004 (quando Mário Jaci generosamente me presenteou com um instrumento de observação (kepleriano) artesanalmente construído por ele).<o:p></o:p></span></div>
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<a href="http://hubblesite.org/newscenter/archive/releases/2008/16/image/bq/format/xlarge_web/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/2008/16/image/bq/format/xlarge_</span></a></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-4158372707710982464.post-50567143161483584242013-11-30T07:13:00.003-08:002015-04-07T13:25:24.207-07:00Breve Roteiro de Viagem Celeste<span style="background-color: white;"><span style="color: #073763;"><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="text-align: center;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo </span><span style="text-align: center;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...; </span><span style="text-align: center;">bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.</span><br /><span style="text-align: center;"><br /></span><span style="text-align: center;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh7ypZi-NoGtD4mL_T7WtidiKx5bAe9boWNjRYQJQ8HK35SmwX8KDkKVv7yrYXtCIznizrxivXLgejr_OelpjIwz9MfByUdoJonfbabbJ_S0XmdL9RJB0K4lXch-ceccEwyH8H15PSehm7B/s1600/png.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh7ypZi-NoGtD4mL_T7WtidiKx5bAe9boWNjRYQJQ8HK35SmwX8KDkKVv7yrYXtCIznizrxivXLgejr_OelpjIwz9MfByUdoJonfbabbJ_S0XmdL9RJB0K4lXch-ceccEwyH8H15PSehm7B/s640/png.png" height="624" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Um Passeio pelo Céu Noturno </b><br /><b>do Sítio das Estrelas</b></span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">OBSERVAÇÃO DE CONSTELAÇÕES E ESTRELAS</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">À VISTA DESARMADA OU ATRAVÉS DE BINÓCULOS</span></b></div>
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<i><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></i></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Breve Roteiro de Viagem Celeste</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">para os tempos do Outono, Inverno, Primavera e Verão</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">no Sítio das Estrelas</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Latitude 21s52 e da Longitude 43w00</span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dois Dedos Iniciais de Prosa sobre o Céu no Sítio das Estrelas</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando eu pensei em me afastar da cidade grande, do Rio de Janeiro, meu desejo era o de morar sob as estrelas, num lugar aonde eu pudesse sempre estar comungando com suas luzes e com suas (quase) eternidades... E logo ao chegar ao pedaço de terra que me apareceu para ser por mim adquirido, o nome <i>Sítio das Estrelas</i> me veio de imediato à mente.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Sítio das Estrelas é um lugar bastante apropriado para se olhar o céu estrelado. A bem da verdade, já foi melhor... Quando aqui cheguei, em 1998, a provinciana cidadezinha docemente chamada de Mar de Hespanha ainda abrigava uma população pequena. Com o tempo, a cidade foi crescendo e casas foram sendo construídas para abrigar as novas famílias, os bairros surgiram e a iluminação feérica também! Sendo assim, no Sítio das Estrelas, nosso norte não é nada bom pela presença da cidade próxima e também nosso noroeste, da mesma forma, porque ali podemos ver a iluminação crescente advinda da cidade de Juiz de Fora, distante a cerca de 60 quilômetros! Portanto, norte e noroeste acabam ficando comprometidos com a poluição luminosa... mas, mesmo assim, sempre podemos observar grandes espetáculos. No entanto, nosso leste e nosso sul e o zênite são bem mais interessantes, sem dúvida alguma... por enquanto... </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Aqui podemos ver a olho nú as duas Nuvens de Magalhães, a Cabeleira de Berenice, A Colmeia de Abelhas (M-44) ou Presépio, a Caixinha de Jóias, A Espada do Órion (M-42).... Também podemos acompanhar alguns serpenteados nos céus: o rio Eridanus começando bem ao sul e terminando aos pés do Gigante e Caçador Órion; a Hydra com sua cabeça triangular começando bem próxima ao Presépio e caminhando delicadamente, delineando, algumas constelações como a Taça, o Corvo, a Virgem, indo se esconder na Balança; a Cabeça da Serpente guardando as maravilhosas estrelas da Corona Borealis; a preciosidade e delicadeza das estrelinhas que compõem a Corona Australis; a Cabeleira de Berenice, quase um enxame de estrelas extremamente tímidas entre o Leão garboso e o Boieiro... Felicidade indescritível também é podermos nadar junto aos dois Peixes em seu mar celeste após termos quase que surfado nas ondas marolantes das estrelinhas tímidas e em ziguezague do Aquário, o Aguadeiro, advindos do Capricórnio que mais parece uma fraldinha de nenê... Infelizmente não dá para ver Andrômeda, a galáxia, a olho nu porque para os lados do norte e noroeste situa-se a cidade de Mar de Hespanha.... e um tantinho mais adiante, ocupando o noroeste e parte do oeste, situa-se a cidade de Juiz de Fora.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Bem, caro Caminhante, para o leitor que entende um pouquinho do céu estrelado, os nomes acima mencionados evocam emoção, estremecimento e felicidade: ver tudo isso a olho nú significa que o céu desse lugar é bem escuro e transparente..... Para o leigo, tudo isso significa o tanto que podemos ainda aprender juntos, realizando um verdadeiro Passeio pelo Céu Noturno do Sítio das Estrelas!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Confesso ao Caminhante que sinto um imenso prazer em morar num lugar onde posso jantar olhando para algum Planeta caindo no oeste... (no carnaval passado, a Caminhante que aqui esteve, levantou seus olhos do prato e se viu ‘pega’ por uma luz intensa, no oeste..., e me perguntou: “que luz é aquela?” Eu respondi: “é Júpiter!”); posso acordar sob o albedo de Vênus ou de Júpiter resvalando por sobre minha cama; posso dormir sob a mira dos raios luminosos da Lua Cheia ou de outras Luas mais tímidas; posso, sempre que quero, sair para o gramado para saudar as estrelas, os planetas, me deixar surpreender por um risco cruzando os céus, uma estrela cadente... e fazer um pedido...; posso suspirar ao apontar para Omega Centauri com meus simples binóculos e então, em noites <i>verdadeiramente escuras</i> e transparentes, <i>tentar</i> divisar este belíssimo objeto, com a visão enviesada...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Eu diria, caro Caminhante, que me encanta o céu estrelado e é por isso que vim viver no Sítio das Estrelas.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Grande parte de minha vida noturna é dedicada a me deixar ser coberta pelo manto estrelado da nossa Via Láctea... e observar as luzes piscantes das estrelas observadas a olho nú – algumas vezes bem sumidas, fugidias (como aquelas da Cabeleira de Berenice, Aquário, Presépio, Hidra, Rio Eridano, por exemplo); a lâmpada acesa dos Planetas movendo-se para frente e para trás contra o pano de fundo das constelações, o caminho que a Lua, doce e mutável Lua vai traçando noite após noite, dia após dia; os chumaços de algodão que vão percorrendo os céus nos revelando a Galáxia onde vivemos e seu revirão na cauda do Escorpião..., bem como outras galáxias... agrupamentos, nebulosas...; um rasgo de luz de um meteoro cruzando o céu.... - todos marchando através da abóbada celeste, revelando seus segredos e sua beleza!</span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O CÉU DO OUTONO</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">no Sítio das Estrelas</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">OBSERVAÇÃO DE CONSTELAÇÕES E ESTRELAS</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">À VISTA DESARMADA OU ATRAVÉS DE BINÓCULOS</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando o outono chega, aqui na Zona da Mata das Minas Gerais, as chuvas do verão vão escasseando de tal forma até se tornarem apenas uma lembrança... As noites voltam a mostrar suas estrelas em céu sem nuvens e o ar bem mais seco permite que suas luzes fiquem bem mais brilhantes e piscantes contra o pano de fundo da escuridão da abóbada celeste. Por que não aproveitarmos esses tempos de início seca do outono para observarmos o céu noturno, em belo passeio?</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ao começar nosso <i>tour</i> celeste, nestes dias de março, podemos ainda bem observar o adeus dos mares aonde a Baleia Cetus e os Peixes nadam vigorosamente... Também já nos despedimos do grande quadrado do cavalo alado Pégasus colado à constelação de Andrômeda e entre ambos, a luz fugidia e a olho nú bem enviesado da Galáxia com o nome da donzela que se apresenta maravilhosamente a nossos olhos revestidos com um simples par de binóculos e melhor ainda, através das lentes do telescópio.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Vale a pena observarmos um dos dois círculos formados pelas estrelas dos Peixes quase ao centro do grande quadrado formado pela constelação de Pegasus, imensa constelação, realmente. É bem neste ponto que encontra-se o Ponto Vernal, o equinócio da primavera.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Olhando em linha quase reta para o sul, poderemos ainda ver a Pequena Nuvem já quase caindo no oeste enquanto a Grande Nuvem de Magalhães ainda a acompanha de longe, permanecendo um pouco mais de tempo nos céus. Aqui na roça, um antigo caseiro meu, as chamava de as Mulas do Presépio! Pobre Fernão de Magalhães que nos perdoe!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando o céu escurece por todo, já também o Carneiro, Áries, se coloca em posição de caída no horizonte oeste, levando consigo, mais ao norte, o herói Perseus que caminha juntamente com aquelas que nos chamam a atenção e nos trazem seus suspiros: as Plêiades que sempre me parecem um tercinho, um rosário.... por que não contá-las? Quatro, cinco, seis, sete.... doze....?</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Estamos entrando, então, nos campos aonde o Touro pasta... e encontramos Aldebarã, o Olho do Touro, sua alfa - como é avermelhada, esta gigante.... será que algum dia poderemos vê-la explodindo em supernova? E as Hyades, não parecem uma arvorezinha de natal? Visto do sul, o Touro fica de cabeça para baixo...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Já quase caindo no oeste e bem mais ao sul de Cetus, ainda nos atrai a beleza de Achernar, o começo (ou o fim) do Rio Eridanus. O Eridanus corre sinuoso e tímido através dos céus até se encontrar com Rigel, o pé do Gigante Órion. Esse Rio tão belo pode apenas ser observado em céus escuros e transparentes, longe das luzes urbanas... assim como no Sítio das Estrelas.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Órion é reconhecidamente uma das mais belas constelação do céu estrelado. Seu Cinturão, as chamadas Três Marias (Alnilan, Mintaka e Alnitak), carregam a linha do equador celeste, ou seja, ao vermos o Gigante, podemos distinguir aquilo que pertence mais ao norte e aquilo que pertence mais ao sul.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Nesse momento de preciosa escuridão, por que não divisarmos todos os detalhes da figura do Gigante poderoso dos céus? Adoro ver seu Escudo, desafiadoramente enfrentando o Olho do Touro, Aldebarã. Sua cabeça é simples porém seus ombros trazem duas preciosidades: Belatrix e Betelgeuse. Porém, o melhor de Órion pode ser divisado a olho nú, apreciado através de binóculos e transformando o sonho em realidade através de bons telescópios: M42, seu berço de estrelas, parte da Espada do Gigante Caçador dos céus. Rigel é a estrela-beta desta constelação e é a seus pés que o Rio Eridanus começa a acontecer, já tendo sido anunciado anteriormente (pois caminha de volta ao leste) por sua Foz realizada pela estrela-alfa Achernar</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Não podemos nos esquecer que os Cães seguem o Gigante Órion em suas caçadas: O Cão Maior e o Cão Menor. Sírius, a mais bela e mais brilhante do céu, é sem dúvida, sempre esperada com ansiedade. Ainda no Cão Maior, binóculos podem ajudar no achado de chumaços simpáticos de estrelas, algumas que pertencem ao Cão Maior e outras que já fazem parte da Popa do Navio. Procyon, alfa do Cão Menor, vem sempre quase junto a Sírius, porém um tantinho atrás, como se fosse uma dama de companhia e já fazendo parte da côrte dos irmãos gêmeos Castor e Pollux.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela pisca bem ao norte... quem será? É Capela, alfa do Cocheiro! Realmente, esta estrela sempre nos chama a atenção pois que se encontra num lugar do céu do norte pouco habitado por grandes luzes.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Se bem percebermos, Já desde Perseus, passando pelo Cocheiro, caminhando entre o Touro e os pés dos Gêmeos e inundando o Cão Maior com seu brilho esfumaçado, realçando Sírius e navegando o Navio capitaneado por Canopus adentro (o Navio foi desmembrado em Popa, Vela, Carina)... e mergulhando no Cruzeiro do Sul (que volta a nos encantar com sua presença no céu do outono), enfim, marcando sua presença inefavelmente e inegavelmente, eis que vemos a Via Láctea com sua mancha esbranquiçada, algodão divino, leite derramado por tantas e tantas estrelas.... Em céus escuros como aqui no Sítio das Estrelas, bem podemos divisar o Saco de Carvão e outras manchas escuras na via esbranquiçada ao longo do Cruzeiro e redondezas e também enxames de algodão brilhante - como a Caixinha de Jóias, por exemplo. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E, ajudados por um bom par de binóculos, podemos nos deixar deslumbrar com a visão de Omega Centauri, um chumaço de estrelas conjugadas e formando um brilhante grande círculo! Falando em Centauro, por que não apreciarmos suas estrelas ponteadoras de seus pés, Alfa e Beta Centauri - sendo que a primeira nos apresenta o lugar onde se encontra Próxima Centauri, assim nomeada por ser a estrela mais próxima de nós, terráqueos, de nosso sistema solar. A bem da verdade, Alfa Centauri - também conhecida como Bungula ou Rigelkent - é um sistema triplo acolhendo a estrela mais perto de nós..</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Também outros belíssimos tesouros podem ser vistos entre o Cão Maior e o Cruzeiro do Sul (muitos deles na Popa do Navio), chumaços de estrelas formando belíssimos aglomerados que podem ser divisados a olho nú em lugares de céu bem escuros e transparentes.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Em abril, o tempo se afirma em sua secura e quando a noite cai, podemos sempre observar os dois Gêmeos celestes, Castor e Pólux caminhando, literalmente pisando sobre a Via Láctea. É bem nos Gêmeos, na altura do ombro de Pólux, que se encontra o ponto do solstício de junho, trazendo o inverno para o sul e o verão para o norte, o ponto aonde a Terra se encontra mais distante em seu <i>tour</i> ao redor do Sol. As estrelinhas de Castor e Pólux podem ser estudadas bem esmiuçadamente porque aparecem bem distintamente em céus da roça escura, sem luz elétrica. (Confesso a você, Caminhante dos Céus, que o Sol transitava pelas pernas dos Gêmeos quando eu nasci!).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A ausência de luz elétrica e de poluição da atmosfera nesses tempos de abril e maio e junho, nos deixam entrever a constelação tímida de Câncer, o Caranguejo. Aqui no Sítio das Estrelas certamente podemos ver (e ver bem) M-44, o Presépio, ou a Colmeia de Abelhas, um verdadeiro berço de estrelas-crianças que viajam juntas e formam para nossos olhos uma lua cheia de luzes fugazes. É interessantes sabermos que o Caminho da Eclíptica passa pelo Presépio e é sempre uma grande honra podermos observar Planetas - ou mesmo a Lua crescendo ou minguando, sem muita luminosidade, é claro - sendo aconchegados pela grande lua cheia de estrelinhas tímidas que compõem o berço do Presépio!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Junto ao Caranguejo, em direção ao sul, podemos ver a Cabeça da Hydra e seu corpo sinuoso de estrelas pouco cintilantes rastejando pelos céus, enredilhando-se na Taça, no Corvo, na Virgem, finalizando, aparentemente, nas duas estrelas ponteadoras da Balança... Alfard, a alfa e o Coração da Hydra, bate avermelhadamente na noite escura e silenciosa.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Estamos agora nos dirigindo para nosso encontro com o garboso Leão, com suas estrelas alpha e beta, Regulus e Denébola, uma das patas dianteiras e a cauda do vigoroso felino. Mais ao norte do Leão, podemos com certeza, nos deliciar com grande parte do corpo da Ursa Maior, constelação norteante que aponta também para a Ursa Menor, que traz em sua cauda, a Estrela Polar (longe de nossos olhos do sul).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Bem ao sul, o Cruzeiro chega mais cedo a cada noite, sendo devidamente anunciado pelas duas estrelas que formam os pés do Centauro. A estrela alpha do Centauro, Rigel Kent, é um conjunto de três estrelas sendo que uma delas é a chamada Próxima Centauro... e por que? Porque é a estrela mais próxima de nós, de nosso Sistema Solar!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Aproveite as noites de maio para melhor observar as estrelas do sul ainda mais ao sul do que o Cruzeiro. A Mosca é perfeitamente divisada assim como o Triângulo Austral. Por que não procurarmos pelo ponto do sul verdadeiro, o pólo sul? Não é difícil de chegarmos ao polo sul quando estamos sob um céu escuro e transparente porque as constelações que o rodeiam, mesmo que compostas de tímidas estrelas, podem ser bem delineadas.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É realmente interessante observarmos o fato de que todo o céu mais ao sul tende a ir se concentrando, concentrando, como se estivesse passando por um funil.... Assim, as constelações e suas estrelas mais ao sul parecem deslizar ao longo da abóbada celeste como se fizessem uma elipse alongada, começando no sudeste, passando pelo zênite voltado para o sul e finalizando no sudoeste. Constelações como o Escorpião e o Corvo, por exemplo, apresentam seu rastejar e seu vôo, respectivamente, inteiramente contidos dentro dessa elipse alongada. O Navio também parece navegar nos mares celestes realizando esse trajeto, porém de maneira bem mais aproximada ao pólo sul, realmente. Podemos pensar, como num exemplo, o sul como uma vasilha em seu ponto de encontro com a mesa, em sua base, e a abertura da vasilha, seu vazio, como representativo do norte (será que me expliquei bem?)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Ah, eu gostaria de poder um dia ir a algum ponto bem ao sul do Planeta para poder observar o Cruzeiro do Sul e o Navio, por exemplo, durante toda a noite, assim como se dançassem uma roda de cantigas celestes! Ah, eu gostaria de um dia poder ir a algum ponto bem ao norte do Planeta para poder observar o Navio navegando alhures, distante, e espraiando-se pelo oceano sem fim!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tenho sempre um imenso prazer quando o Corvo começa a fazer seu vôo pelos céus, cruzando o leste mais o sul, fazendo quase uma meia-girada simbolizando um real vôo, até desaparecer no horizonte oeste, ao longo de sua passagem de alguns meses no ano.... Já desde final de março, início de abril, que podemos ver este pássaro nos céus, radioso, voando, voando, deslizando com seu vôo suave pela abóbada dos céus do sul.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">No entanto, não podemos nos esquecer que o Leão também já vem rugindo desde há bastante tempo nos céus... Visto do sul, o Leão está de cabeça para baixo porém sempre nos deixando entrever sua juba, seu pé Régulus, seu corpo iluminado por estrelas simpáticas e finalmente, sua cauda vibrante, Denébola. O Caminho da Eclíptica passa por Regulus e então é muito comum que possamos observar esta estrela sendo conjugada com a Lua ou com algum Planeta!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A noite vai andando, maio vai seguindo seu rumo e o céu também vai andando, como num carrossel iluminado.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mais ao norte do Leão, podemos ver o Leão Menor e umas poucas estrelinhas dos pés da Ursa Maior.... Mais ao sul, o chumaço de algodão, o leite derramado das estrelas da Via Láctea, continua invadindo o sul, sempre brilhante, enquanto que ao norte, vai desaparecendo sua luz tímida como um sonho desvanecedor... Noite adentrada, essa Via Láctea e luminosa nos traz o Escorpião, surgindo vagarosamente no leste mais ao sul, trazendo em sua cauda o revirão da Galáxia, o ponto de mutação, onde a cobra morde a cauda....</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Porém, ainda no céu do começo da noite do meses de maio e junho e acompanhando o vôo do Corvo bem de perto, a Virgem chega radiosa com sua alfa, a estrela Spica. O Caminho da Eclíptica passa por Spica e é bem comum podermos observar a Lua ou algum Planeta conjugando-se à esta estrela.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Um dedinho antes da constelação da Virgem, encontra-se o ponto de interseção das linhas da eclíptica e do equador, o equinócio. Virgem traz consigo a Balança, com suas duas estrelas perfazendo os dois pratos: Zubenelgenubi e Zubenelschamalli (que antigamente eram consideradas as Garras do animalzinho rastejante dos céus e, sem dúvida alguma, isso faz o maior sentido). O Caminho da Eclíptica passa pelas estrelas ponteadoras da Balança e, da mesma forma, passa bem próxima à Antares, a estrela alfa do Escorpião. Depois de passar próxima à Antares, o Caminho da Eclíptica adentra a 13<sup>a</sup>. constelação do Zodíaco, Ophiúco, aquele que segura a Serpente que pode ser delineada em sua cauda e também em sua cabeça (esta última terminando aos pés da Coroa Boreal, como se quisesse guardá-la.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Olhando mais ao norte, podemos nos deliciar com a presença de Arcturus, no Boieiro. Em locais de céu escuro – assim como no Sítio das Estrelas -, podemos divisar as tímidas estrelinhas que formam as mechas da Cabeleira de Berenice, constelação quase apagada, entre o Leão e o Boieiro. Ver a olho nú as mechas dos cabelos da bela egípcia é um real privilégio.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Em junho, quando cai a noite, já temos a figura maravilhante do Escorpião toda desenhada entre o algodão doce da Via Láctea... Como já dissemos, o Escorpião é antecedido por suas duas garras, as estrelas alpha e beta da Balança.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A cabeça deste animalzinho rastejante sobre a Via Láctea é realmente incrível, levando até seu coração batendo avermelhadamente, Antares, a rival de Ars, Marte.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É realmente belo o desenho que as estrelas do Escorpião vão nos mostrando... várias estrelas duplas que disputam a acuracidade de nossa visão... (me lembro de meu primeiro namorado me dizendo que éramos tão próximos um do outro quanto aquelas duas estrelas que formam uma das curvas do Escorpião.... palavras ao vento.... não o vejo há mais de 45 anos...). A cauda do Escorpião é realmente assustadora com a presença fulminante de Schaula... finalizando com alguns objetos maravilhosos, M-7, M-8, M-6, chumaços de algodão, bom de olhar a olho nú, melhor ainda de binóculos e telescópio.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Nesta região do céu entre o Escorpião e o Sagitário, naquela direção e além daquela poeira de estrelas, encontra-se o chamado Centro de nossa Galáxia, a Via Láctea. E como tudo no universo realiza um movimento de rotação em torno de si mesmo e em torno de algum outro objeto magnetizador, também nossa Via-Láctea realiza esse movimento.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Não podemos deixar de mencionar a imperdível visão da Coroa Austral sendo enlaçada pelo Sagitário! A Coroa Austral é de uma delicadeza ímpar, realmente. Se mantivermos quase a mesma direção do céu, estaremos encontrando, bem mais ao norte, a Coroa Boreal, tão bela quanto a outra Coroa e encontrando-se bem situada entre estrelas de primeiríssima grandeza como Arcturus, a alfa do Boieiro, e Vega, a alfa da Lira e próxima ao herói Hercules.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Com o andar da noite e das estrelas, outras constelações vão se aprontando, por assim dizer, para entrarem no palco da vida...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Não será tempo de irmos dormir?! Ah, eu diria para você passar uma noite em claro apenas para observar a girada da Via Láctea enquanto o céu vai caminhando todo de leste para oeste, carregando suas estrelas, planetas, constelações.... A visão do girar da Via Láctea é algo que nos deixa sem palavras....</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Se você tiver a oportunidade de estar num lugar onde o céu seja escuro e transparente, poderá observar a imensa pavimentação de algodão de estrelas - a Via-Láctea - aparentemente centralizando-se no Escorpião e cobrindo o céu estrelado em direção ao norte, passando por Sagitário, pela Águia até alcançar o Cisne..., e em direção ao sul encontrando-se com nosso Cruzeiro do Sul, com o Navio, com o Cão Maior seguido do Gigante Órion e aparentemente concluindo-se no Cocheiro.... Deste ponto bem ao sul e se você estiver em Latitude bem mais ao norte do Planeta, poderá ainda comungar com a pavimentação de algodão de estrelas fazendo parte do Mito de Andromeda, a donzela acorrentada, enredilhando Perseus, seu herói salvador, Cassiopéia, sua malvada madrasta, e seu pai, o Rei Cepheus - todas constelações bem ao norte - e, finalmente a Via Lactea realiza seu encontro com o Cisne.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Obviamente que aquilo que vemos e acompanhamos como o Revirão da Via Láctea durante a passagem noturna do Escorpião aliado ao Sagitário é um movimento aparente – pois que, na realidade, esse aparente movimento se dá em função do movimento de rotação da nossa Terra, nosso tão querido Planeta.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Revirão da Via Láctea é um espetáculo imperdível e inesquecível e que nos traz uma realidade da mecânica celeste que vai além à realidade que vemos do caminhar das constelações e suas estrelas, todas advindas do horizonte leste, galgando as alturas dos céus e concluindo seu passear no horizonte oeste - com as constelações e estrelas mais ao sul realizando seu caminhar em elipse do sudeste ao sudoeste e com as constelações e estrelas mais ao norte realizando seu caminhar de maneira mais espraiada, digamos assim. A realidade do Revirão da Via Láctea parece varrer os céus, como se essa varrição viesse do sul em direção ao norte ou vice-versa..., como se fosse uma hélice, algo assim, cobrindo todas as direções, ao longo da noite e ao longo do caminhar do Escorpião, fundamentalmente. A realidade do Revirão da Via Láctea, quando o percebemos realmente - em lugares de céus escuros e transparentes e que nos apresentem o chumaço de algodão do caminho desta Via iluminada em bom estilo! -, nos faz tremer não somente de emoção como também em nosso labirinto interior, é quase como se perdêssemos o chão, ficamos zonzos, tontos, quase caímos, quase perdemos o equilíbrio. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os braços da Via Láctea, centralizados no corpo do Escorpião, vão varrendo o céu vindo do sudeste, caminhando para o leste, passando pelo noroeste, pelo norte, pelo noroeste, pelo oeste... e ainda pelo sudoeste, pelo sul, novamente pelo sudeste, noite após noite. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Não deixe de dar uma olhada no Céu do Inverno, se você estiver desejoso de passar a noite inteira observado as constelações e suas estrelas em marcha céu adentro céu afora... ou se você estiver retornando de um programa noturno e perder o sono... ou se você gostar de acordar bem cedo, já com o canto do galo...</span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O CÉU DO INVERNO</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">No Sítio das Estrelas</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">OBSERVAÇÃO DE CONSTELAÇÕES E ESTRELAS</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Aqui na Zona da Mata das Minas Gerais, o inverno traz tempo frio, chás, cafés, casacos, gorros, meias, cobertores.... e muita vontade de olhar as estrelas porque ainda o céu está seco (antes das queimadas se aventurarem a maltratar as matas, normalmente a partir do final de julho e cobrindo os meses de agosto e setembro... até que as benditas chuvas retornem, mais para o outubro).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Certamente, é ainda o Escorpião e o ponto que leva à centralidade da Via Láctea que nos chama a atenção.... Portanto, eu aconselharia você, Caminhante dos Céus, a retornar o ponto anterior onde eu tentei descrever o Revirão da Via Láctea.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Porém, com o contínuo andamento do céu (a cada noite, tudo chega mais cedo 4 minutos), podemos agora ver bem o Sagitário, quando a noite cai. É sempre interessante observarmos o fato de que esta constelação também é denominada de Bule de Chá..., porque se parece mesmo com um! </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">No ponto entre o Escorpião e o Sagitário, em lugares de céu escuro como o Sítio das Estrelas e em noites secas e transparentes, podemos ver que a Via Láctea vai recebendo vários buracos imensos de puro negrume.... verdadeiras belezas de luz e vazio para serem fotografadas!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A Via de Chumaço de Algodão, a Via Láctea, encontra a Águia que voa sempre orientada por sua estrela alfa, Altair, e este pássaro acaba sendo avizinhado por constelações pequenas e muitíssimo simpáticas, Sagitta, a Flecha, e o Delfim, por exemplo, que também são enredilhadas pelo caminho leitoso. Ainda em direção mais ao norte, a Via Láctea parece, a meus olhos, encontrar o Cisne que traz sua cauda a estrela alfa, Deneb, e ali se esfumaçar mais e mais, rumo norte mais aprofundado e distanciado de meus olhos. A Via Láctea estará iluminando os caminhos de constelação bem ao norte, como Cepheus, Cassiopéia, Perseus (e passando próxima à Andromeda e ao Cavalo Pegasus) e novamente retornando aos nossos olhos do sul através o Cocheiro, com sua belíssima estrela-alfa Capella, e então retomando a conversa com os Gêmeos Castor e Pollux, acompanhando o Gigante Òrion conduzindo seus dois Cães e já nos enleando a visão com a bela Sirius acompanhada da tímida Procium... até que o clarão dos raios avermelhados do Sol começam a inundar o horizonte leste....</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A Via Láctea pode bem ser vista até Deneb, aqui no Sítio das Estrelas... Quando a noite cai, o revirão dessa Via parece ter chegado à sua conclusão.... porém ainda podemos acompanhá-lo varrendo a noite, quase com puxando as estrelas que chegam no leste e empurrando as estrelas do meio do céu para caírem no horizonte oeste.... Os braços da Via Láctea, centralizados no corpo do Escorpião, vão varrendo o céu vindo do sudeste, caminhando para o leste, passando pelo noroeste, pelo norte, pelo noroeste, pelo oeste... e ainda pelo sudoeste, pelo sul, novamente pelo sudeste, noite após noite. É um girar intenso, como se fosse um dançarino sufi, girando e girando e girando e nos trazendo o êxtase.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Cruzeiro do Sul aparece bem alto, o mais alto que consegue chegar, acompanhando a caída do Navio no horizonte oeste e trazendo maior brilho às presenças do Escorpião, do Sagitário.... e certamente, da Via Láctea que continua fazendo seu revirão noite a dentro. Não se esqueça, Caminhante, de bem observar os Sacos de Carvão e dos conjuntos brilhantes de estrelas juntinhas que vão se formando após o Cruzeiro e indo em direção ao Navio que navega bem mais distanciado, em mares longínquos, buscando por outras paragens e retornando apenas na madrugada anunciadora das estrelas e suas constelações que vão surgir no leste.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Arcturus também continua encantando nossa visão.... e para aqueles que possuem um norte escuro e de horizonte baixo, a Ursa Maior se insinua querendo também trazer consigo o Dragão (desaparecido nesta latitude).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Porém, os céus do norte estão felizes com a presença da Coroa Boreal, que parece um colar que todas as mulheres gostariam de usar! Porém, cautela! Esse valoroso colar é guardado por Hércules que ainda mal se articula em sua figura engraçada surgindo no horizonte leste mais ao norte... E também guardado pela cabeça da cobra que o Ofiúco segura.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando agosto entra trazendo suas queimadas e já uma certa poluição tirando a escuridão plena e a transparência cristalina dos céus da roça, com sorte, ainda podemos nos deliciar com as travessuras do desajeitado Hércules, agora mais alto no céu do norte, acompanhado, em lugares de horizonte bem baixo, pelo Dragão que guarda as estrelas que rodeiam o polo norte, longe de nossa visão.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Digo que o Hércules é todo desajeitado porque é assim que o vejo. Lembro-me bem da primeira vez que o delineei, eu até ri, mesmo!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Cada vez mais o Cruzeiro do Sul cai em direção ao horizonte oeste mais ao sul ao mesmo tempo que também o Escorpião vai alcançando o meio do céu seguido do Sagitário, com seu Bule de Chá, que dá lugar ao Capricórnio que começa a querer se levantar no horizonte leste, ainda ao sul.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Nesse tempo do inverno já bem andado, eu adoro ver minha estrela preferida, Vega, tocando sua Lyra e surgindo atrás dos morros do leste mais ao norte.... Sempre que eu me vejo diante da Lyra segurada por Vega,sua alfa, eu me flagro suspirando, inteiramente enleada, como se pudesse escutar o doce som das cordas desta constelação! </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A bem da verdade, o céu do inverno nos presenteia com um triângulo de estrelas muito interessantes: Altair, alfa da Águia, Vega, alfa da Lyra, e Deneb, alfa do Cisne. São estrelas belíssimas que fazem parte de belíssimas constelações! </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Cisne é de uma perfeição incrível em seu vôo, parece estar sempre alçando vôo, abrindo suas asas imensas, buscando as alturas, sempre.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A Águia sempre surge apresentando três estrelas - uma delas, Altair, sua alfa - que caminham sempre juntas e que podem ser vistas após a conclusão de todo o corpo do Capricórnio, com seu aspecto de fraldinha tecida por estrelas suaves que delineiam a figura desta constelação.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É bom também observarmos, ainda entre o Sagitário e seu Bule de Chá e o Capricórnio, um pequeno grupo de estrelas que sugere uma pequena cruz, um tímido diamante, algo assim, verdadeira maravilha para ser visto em lugares de céus bem escuros e transparentes.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Eu aconselharia o Caminhante dos Céus aguardar a chegada do Capricórnio e da Águia para então olhar mais ao norte e se encantar com a Lira... e um tantinho mais tarde ainda, suspirar com o Cisne voando amplamente nos céus estrelados. E, olhando mais ao sul, observarmos o vôo do Grou balizado por sua estrela-alfa, Al Nair.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A partir de então, podemos olhar para os lados do sul e observarmos a chegada do Peixe Austral com sua estrela-alfa, Fomalhaut. Estamos bem já sendo colhidos pelas ondas marolantes e em verdadeiro zigue-zague formadas pelo Aguadeiro, Aquário! A meu ver, esta constelação é um dos eventos mais interessantes a ser observado nos céus estrelados e isso somente pode acontecer em lugares de céus realmente escuros e transparentes!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Bem ao sul, podemos observar pássaros voando, Fênix e Tucano. No entanto, a estrela que realmente nos chama a atenção é Achernar, a alfa do Rio Erídano, sua Foz, e este Rio vai correndo sinuosamente e através suas tímidas estrelas até encontrar os pés do Gigante Órion, em Rigel, sua estrela-beta, já em terra firme. É interessante repararmos o fato de que o Rio Erídano caminha em direção ao leste e neste momento de inverno, podemos acompanhar seu desaguar junto ao Gigante caçador do Escorpião porque a constelação de Órion ainda pode ser vista em todo seu esplendor de estrelas ao final da noite, quando o galo desentrelaça suas asas e começa a cantar anunciando um novo dia que não tarda a chegar! (Aqui no Sítio das Estrelas meu simpático galo nos acorda com seu canto por volta das quatro horas da matina!).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Nos céus do norte, é interessante observarmos que as estrelinhas marolantes do Aguadeiro parecem querer se entrelaçar com as estrelas também tímidas dos Peixes. Nesse momento estamos diante de um mito realmente encantador que apresenta no céu estrelado do norte todos os componentes de sua estória, começando pelo Cavalo Pegasus em seu grande quadrado sendo seguido por Andromeda, a donzela acorrentada numa ilha por sua madrasta Cassiopéia esposa de Cepheus. Andromeda será salva pelo herói Perseus. A Via Láctea ilumina com seu leite as constelações do pai, da madrasta e do herói salvador, todas bem ao norte e não muito facilmente identificáveis aqui, no Sítio das Estrelas (porque para estes lados fica a cidadezinha de Mar de Hespanha e sua iluminação pouco generosa com o céu estrelado).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">... ‘Stamos em pleno mar... - como diria o poeta português, Camões. Ao sul dos Peixes nos deparamos com a imensidade da constelação de Cetus, a Baleia que quer devorar a bela donzela acorrentada, Andromeda. Este é um mar interessante pois que também apresenta a Foz do Rio Erídano e todo seu correr sinuoso, desde o sul até o sudeste, para encontrar os pés do Gigante Órion, já em terra firme. No entanto, este mar interessante nos apresenta, bem ao fundo (do ponto de vista de quem está bem ao norte, certamente) a estrela maravihosa e alfa do Navio, seu capitão Canopus! Sempre que virmos Canopus podemos ter a certeza de que Sirius chegará logo depois! E Sirius faz parte da comitiva do Gigante Órion, com seus Cães Maior e Menor, todos já em terra firme.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Não podemos deixar de divisar os dois círculos formados pelas cabeças dos dois Peixes. Um destes circulo encontra-se logo ao norte do grande quadrado do Cavalo Pegasus e é bem ali que podemos encontrar o chamado Ponto Vernal, o lugar onde a Eclíptica encontra-se com o Equador Celeste.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Olhando para o sul, poderemos ver a Pequena Nuvem seguida pela Grande Nuvem de Magalhães. Aqui na roça, um antigo caseiro meu, as chamava de as Mulas do Presépio de Jesus! Fernão de Magalhães que nos perdoe!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os mares terminam deixando entrar em cena as duas estrelas ponteadoras de Áries, o Carneiro, e depois, surge o campo onde o Touro pasta, sempre antecedido pelas estrelas que choram, as Pleiades, um tercinho de estrelas, verdadeira maravilha sempre a ser visitada por nossos olhos...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Já estamos na madrugada sonolenta quando entra em cena o Gigante Órion acompanhado do Cão Maior e este embelezando os céus com a presença de Sirius, a bela das belas. A Via Láctea já retorna à nossa visão, o Navio vai se mostrando por inteiro, os Gêmeos já se mostram conversantes, como sempre... </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Não deixe de dar uma olhada no Céu da Primavera, se você estiver desejoso/a de passar a noite inteira observado as constelações e suas estrelas em marcha céu adentro céu afora... ou se você estiver retornando de um programa noturno e perder o sono... ou se você gostar de acordar bem cedo, já com o canto do galo...</span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O CÉU DA PRIMAVERA</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">No Sítio das Estrelas</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">OBSERVAÇÃO DE CONSTELAÇÕES E ESTRELAS</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">À VISTA DESARMADA OU ATRAVÉS DE BINÓCULOS</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Cruzeiro do Sul já se despede de nossas noites quando chega outubro. E num movimento de seguimento, o Escorpião também desliza em seu caminho rumo ao sudoeste, carregando consigo o Sagitário, a Coroa Boreal, Hércules...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A côrte do céu, no entanto, está formada pelo triângulo do norte, a maravilhosa Vega tocando sua Lyra, a esplendorosa Altair voando a Águia e a não menos formosa, Deneb, a cauda do belo Cisne.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ainda rodeando Altair, encontramos algumas pequeninas constelações que são verdadeiras preciosidades: Sagitta, a Flecha, o Delfim, Equuleus - constelações compostas por tímidas estrelas que podem ser vistas apenas em locais de céus escuros e transparentes.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É bom tempo para estudarmos as estrelas que formam o grande triângulo do Capricórnio e também nos prepararmos para mergulhar dentre as estrelinhas marolantes do Aquário.... já entrevendo a chegada do cavalo alado Pégasus, no horizonte leste mais ao norte.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Também já surge no leste, mais ao sul, o pássaro Grou, uma verdadeira beleza voadora nos céus balizado por sua estrela alfa Al Nair, ao mesmo tempo, que já no mar ao sul do Aquário, podemos ver o Peixe Austral com sua bela estrela Fomalhaut.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Se o tempo ajudar e se a seca comprometida pelas queimadas não estiver maculando nosso céu, por que não continuarmos a estudar os Peixes? Por que não nos embevecermos com a visão das Nuvens de Magalhães?</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Com novembro chegam as chuvas... tão ansiadas chuvas - aqui na Zona da Mata das Minas Gerais! Benditas águas que caem dos céus, despencadas, quem sabe, pelas águas do Aquário, do Peixe Austral, e também com o aparecimento dos Peixes que nadam juntos com a Baleia Cetus.... Entre o Aquário e os Peixes, existe o ponto da interseção da eclíptica com o equador celeste, o ponto vernal trazendo o equinócio. Este ponto também apresenta-se bem próximo ao grande quadrado de estrelas que formam o Pegasus, o cavalo alado que carrega Perseus em sua intenção de salvar Andromeda, a bela - e é interessante observarmos que também esta Galáxia nossa irmã encontra-se nos arredores do ponto vernal.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O cavalo alado Pégasus já salva a heroína acorrentada, Andrômeda, um tanto que antecedidos, em norte bem baixo, por Cepheus.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Cruzeiro do Sul bem como o Escorpião se despedem do palco dos céus do anoitecer... Porém, Achernar, a foz do Rio Eridanus novamente surge, brilhante e maviosa, no leste do sul bem sul mesmo!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Em dezembro, se as chuvas nos derem alguma trégua, podemos nos deixar maravilhar com a linha sinuosa do caminho que o Rio Eridanus segue... mesmo que ainda não possamos ver o gigante caçador Órion, ao anoitecer, apenas um tanto mais tarde em noite de já quase verão quente.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ao norte, em horizonte bem baixo, Cassiopéia nos deixa ver algumas de suas estrelinhas. Andrômeda e o cavalo alado Pégasus surgem imponentes no meio do céu. Por que não procurarmos por Andromeda, a Galáxia? Mesmo com um simples par de binóculos, esta visão se faz encantadora: é uma emoção imensa, realmente, observarmos nossa querida irmã... porque mais dia menos dia possivelmente nos uniremos a ela de maneira a nos tornamos irmãs siamesas... No horizonte leste, mais ao norte, entra Áries, o Carneiro, ao lado do Triângulo.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A noite vai seguindo seu curso e novamente podemos nos deixar encantar pela via leitosa, a Via Láctea, fazendo parte dos céus do norte, vindo de Perseus e ladeando as Pleiades (que bom, assim essa preciosidade da constelação do Touro não fica comprometida pelo chumaço de algodão) bem como a cabeça do Touro sempre nos mostrando seu Olho Iluminado, Aldebarã. A Via Láctea abençoa o Cocheiro e sua bela estrela-alfa, Capella, e então segue rumando mais ao sul, encostando no Gigante Órion, sempre garboso e pronto para caçar o Escorpião (que mora do outro lado do céu exatamente para não ser caçado!) e enchendo de luz esfumaçada, esbranquiçada, o Cão Maior que nos brinda com a majestosa presença da mais bela da noite, Sirius, a mais brilhante dos céus e também tão próxima a nós (somente 8 anos-luz de distância).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O mito da donzela acorrentada, Andromeda, começa a desaparecer de nossas vistas, com o horizonte oeste engolindo Cepheu, o Cavalo Alado Pegasus, Andromeda, a Baleia Cetus, Cassiopéia... e, com a entrada em cena de Áries e do Touro, também Perseus começa a se despedir de nós. Aquário e Peixes também saem do palco estelar. O belo Triangulo formado pelos três pássaros, Águia, Cisne e Vultur (outra denominação para a Lira), também podem ser vistos apenas no começo das noites de dezembro, caindo no horizonte oeste logo depois.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ao longo da noite, Achernar começa a carregar o sinuoso Rio Erídano consigo, caindo no horizonte oeste, enquanto Canopus vai capitaneando o Navio que vai surgindo cada vez mais belo, mais imponente, silenciosamente singrando as águas celestes. Também o Navio acaba sendo encontrado pela Via Láctea que busca encantar nossa visão acendendo o Cruzeiro do Sul, o Centauro, todos ao sul...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Caminho da Eclíptica já nos deixou ver os Gêmeos conversadores, o Presépio no Caranguejo sendo guardado pela cabeça da Hydra e emocionado por seu coração laranja, Alfard, e esta cobra da água já se mostrou rastejando através a Taça e o Corvo, saudando o Leão, a Virgem, e encontrando a Balança.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Não deixe de dar uma olhada no Céu do Verão, se você estiver desejoso/a de passar a noite inteira observado as constelações e suas estrelas em marcha céu adentro céu afora... ou se você estiver retornando de um programa noturno e perder o sono... ou se você gostar de acordar bem cedo, já com o canto do galo...</span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O CÉU DO VERÃO</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">OBSERVAÇÃO DE CONSTELAÇÕES E ESTRELAS</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Em janeiro, se as chuvas nos derem uma trégua – pelo menos durante o anoitecer... aqui na Zona da Mata das Minas Gerais – podemos nos deitar no deck em frente ao grande lago do Sítio das Estrelas e nos deixar levar pelas estrelas e suas histórias celestes....</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Todo o mito de Andrômeda salva por Perseus cavalgando seu cavalo alado Pégasus está no céu, na ilha do céu, onde a donzela foi acorrentada por sua madrasta Cassiopéia que não pode ser vista adequadamente nesta latitude... Nesse mar, estão o Aguadeiro (Aquário), o Peixe Austral, os Peixes juntamente com Cetus, a Baleia... ao mesmo tempo que voam nos céus celestes os pássaros Grou e Fênix, mais ao norte. Com a entrada do Carneiro, Áries, parece que pisamos em terra e no entanto, já nos deparamos com um rio, o Eridanus, que agora, em janeiro, já nos leva a ver o gigante caçador Órion, em cujas pernas suas águas começam, em terra firme...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sempre que vemos o Órion surgindo ao anoitecer, também estaremos revendo as Plêiades, irmãs chorosas, o Touro com seu belo olho avermelhado, Aldebarã, as Hyades.... ao norte, novamente Capela nos chama a atenção, como se fosse um farol!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sem dúvida alguma, essa parte dos céus estrelados nos deixa absolutamente enleados, quase que sem respiração... porque a Via Láctea nos abençoa com sua presença esfumaçada e escondendo vários pontos interessantes a serem observados através nossos binóculos.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sírius, a rainha da noite, também nos encanta a visão nesse já quase final de verão, fevereiro de nossos carnavais... Procyon segue Sírius, como sempre, e ambas estrelas seguem o caçador gigante Órion... Canopus volta a capitanear seu imenso Navio (desmembrado em Popa, Vela e Carina - não sei por qual razão....) E eis que ao leste, bem ao sul, bem ao sul... retorna o Cruzeiro aos nossos céus da noite!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mais ao norte, podemos ver os dois Gêmeos conversando animadamente a caminho do meio do céu. Câncer continua protegendo em seu ventre seu ninho de estrelinhas-crianças, o Presépio. A Hydra também re-aparece em sua cabeça triangular, mostrando depois seu coração, Alphard.... e com o andar da noite e dos meses, todo o seu corpo serpenteando várias constelações...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Leão surge garboso como sempre com suas estrelas Regulus e Denebola - a primeira na pata e a segunda, na cauda -, dando lugar à Virgem que surge antecipada pelo vôo do Corvo. Sempre a Virgem nos faz voltar nossa visão para a encantadora Spica, sua estrela-alfa. E sempre também a Virgem nos faz voltar nosso desejo de observarmos a luz amarelada e intensíssima advinda de Arcturus, a estrela-alfa do Boeiro. Não podemos nos esquecer que entre o Leão e o Boieiro existe a Cabeleira de Berenice, um presente dos céus escuros e transparentes, realmente.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Se olharmos para os céus do norte, poderemos divisar o Leão Menor, os Cães de Caça, e com muita sorte, as patas da Ursa Maior. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Se olharmos para os céus do sul, estaremos suspirando mais e mais com a visão encantadora, cativante, maravilhante, da Via Láctea realizando seu caminho através o Navio, a Cruz, o Centauro e preenchendo todos os espaços que unem estas duas últimas constelações ao Escorpião que entra em cena trazendo nossos olhares mais e mais ao sul, sendo antecedido por suas duas Garras, ou seja, a constelação da Balança.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sempre que o Cruzeiro do Sul aponta para seu momento máximo de zênite possível para uma constelação muitíssimo ao sul e muito próxima ao pólo sul..., entra em cena a majestosa constelação do Escorpião!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Entrando no palco celeste o Escorpião, é tempo de nos deixarmos maravilhar com a Via Láctea encontrando seu ponto máximo de concentração, digamos assim, pois aos pés desse rastejante animal celeste encontra-se o ponto para onde podemos dirigir nossos pensamentos para encontrarem o centro de nossa Galáxia!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Para enfeitarmos e saudarmos esse evento, sempre podemos nos brindar com a doce visão da Coroa Austral, já bem próxima a Sagitário, e da Coroa Boreal, entre o Boieiro e Hercules e guardado pela cabeça da serpente que o Ofiuco segura.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Se o Caminhante estiver num lugar de norte bem baixo, realmente, poderá tentar observar algumas estrelas que compõem o Dragão que guarda o norte dos céus estrelados, o pólo norte.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando o galo estiver cantando, ainda antes do Sol surgir no horizonte leste anunciado por clarões avermelhados..., com sorte poderemos novamente nos fazer felizes como a entrada em cena do Capricórnio apontando para o norte que acolhe a estrela Vega, a alfa da doce e bela e sutil Lyra, e nos trazendo a esperança da chegada próxima da Águia, também acolhida pela Via Láctea, e sempre nos mostrando suas três estrelas que voam juntas!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Não deixe de dar uma olhada no Céu do Outono, se você estiver desejoso/a de passar a noite inteira observado as constelações e suas estrelas em marcha céu adentro céu afora... ou se você estiver retornando de um programa noturno e perder o sono... ou se você gostar de acordar bem cedo, já com o canto do galo...</span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Março marca o final do verão e o início do outono...</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando o outono chega, aqui na Zona da Mata das Minas Gerais, as chuvas do verão vão escasseando de tal forma até se tornarem apenas uma lembrança... As noites voltam a mostrar suas estrelas em céu sem nuvens e o ar bem mais seco permite que suas luzes fiquem bem mais brilhantes e piscantes contra o pano de fundo da escuridão da abóbada celeste. Por que não aproveitarmos esses tempos de início seca do outono para observarmos o céu noturno, em belo passeio?</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ao começar nosso <i>tour</i> celeste, nestes dias de final de março.......................................................................................................................................................................................................................................................... (você pode retornar ao começo de nosso texto.... porém, já certamente sabedor de alguns dos tesouros dos céus estrelados!)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sítio das Estrelas</span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-4158372707710982464.post-72707372687017955132013-11-30T07:13:00.001-08:002015-04-07T13:25:57.092-07:00Meu Amor pelas Estrelas<span style="background-color: white;"><span style="color: #073763;"><br /></span></span>
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<tr><td><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh0VSg3woks0qa9wKGLCvRrhyMWT6qER4dqitETgrMvPGow3ObgccQmokGTo9X0-9f09AE_ljkXi6HVfhe6U29YS07sEfyEpD29NGRDqysDNb1OeYJrRnY_3fI-S-xytaW7hRNEH9ZzqbDP/s1600/mapa+do+universo+que+vemos+em+positivo.gif" imageanchor="1" style="margin-left: auto; margin-right: auto; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh0VSg3woks0qa9wKGLCvRrhyMWT6qER4dqitETgrMvPGow3ObgccQmokGTo9X0-9f09AE_ljkXi6HVfhe6U29YS07sEfyEpD29NGRDqysDNb1OeYJrRnY_3fI-S-xytaW7hRNEH9ZzqbDP/s640/mapa+do+universo+que+vemos+em+positivo.gif" height="480" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></td></tr>
<tr><td class="tr-caption" style="font-size: 13px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: xx-small;"><span style="text-align: start;">Fonte da Imagem: http://www.atlasoftheuniverse.com/galchart.html</span><span style="text-align: start;"> </span><a href="http://www.atlasoftheuniverse.com/me.html" style="color: #bf9000; text-align: start; text-decoration: none;">Richard Powell</a><span style="text-align: start;">.</span><span style="text-align: start;"><br /></span></span></td></tr>
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<tr><td><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgHrmadPxraNkqhml9G_UGvKDJiNW3kjAS_UAG9IfA47PoQTi18vgZQK5nZw5rveUgUEgnkO3vlSfvwpcaZfKrn0oGDJi8tSh8QHlJkYkv_I0YFkhXLh_nHcrT4ZlyaZSScPRqRN7j5dBKJ/s1600/800px-Earth's_Location_in_the_Universe_SMALLER_(JPEG).jpg" imageanchor="1" style="margin-left: auto; margin-right: auto; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgHrmadPxraNkqhml9G_UGvKDJiNW3kjAS_UAG9IfA47PoQTi18vgZQK5nZw5rveUgUEgnkO3vlSfvwpcaZfKrn0oGDJi8tSh8QHlJkYkv_I0YFkhXLh_nHcrT4ZlyaZSScPRqRN7j5dBKJ/s1600/800px-Earth's_Location_in_the_Universe_SMALLER_(JPEG).jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></td></tr>
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<a href="http://commons.wikimedia.org/wiki/File:Earth%27s_Location_in_the_Universe_SMALLER_(JPEG).jpg" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: xx-small;">http://commons.wikimedia.org/wiki/File:Earth%27s_Location_in_the_Universe_SMALLER_(JPEG).jpg</span></a></div>
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<span lang="PT" style="line-height: 48px;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Da Terra ao Céu .......................<o:p></o:p></span></b></span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT" style="line-height: 36px;">.........................................................................................</span><span lang="PT" style="line-height: 36px;"><o:p></o:p></span></span></b></div>
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<span lang="PT" style="line-height: 48px;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">................................ e ao Infinito ...................<o:p></o:p></span></b></span></div>
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<span lang="PT" style="line-height: 22px;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">CONSTELAÇÕES, ESTRELAS E OBJETOS CELESTES<o:p></o:p></span></b></span></div>
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<span lang="PT" style="line-height: 22px;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(sob o ponto de vista do Mundo Ocidental)<o:p></o:p></span></b></span></div>
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<span lang="PT" style="line-height: 22px;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> SUAS HISTÓRIAS, SEUS MITOS, SEUS SIGNIFICADOS<o:p></o:p></span></b></span></div>
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<span lang="PT" style="line-height: 22px;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E SUAS SINTETIZADAS DESCRIÇÕES<o:p></o:p></span></b></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Reunião das Informações,<o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">suas traduções para a língua portuguesa (quando necessário),<o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Compilação bem como Comentários Pessoais:<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><i><span lang="PT"><span style="background-color: white; color: #073763;">Janine Milward</span></span></i></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><span lang="PT"><br /></span></i><i><span lang="PT"><br /></span></i><i><span lang="PT"><br /></span></i></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Though my soul may set in darkness, it will rise in perfect light;<br />I have loved the stars too fondly to be fearful of the night.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> (traduzindo livremente) :</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apesar de minha alma permanecer na escuridão, ela ascenderá plenamente iluminada,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Meu amor pelas estrelas tem sido grande demais para que eu tema a (escuridão da) noite</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">.......ou .. para que eu tema a morte)."<br /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Este poema é o grande companheiro das noites solitárias dos amantes das estrelas.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Momento de Reverência à Astronomia</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Transcrevo o belíssimo poema de SARAH WILLIAMS</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> que tão bem descreve o amor à Astronomia, o respeito à passagem do conhecimento do mestre para o discípulo, a tristeza do não-reconhecimento dos pares contemporâneos a respeito do trabalho realizado, a emoção de se unir ao mestre reverenciado e às estrelas quando chega o momento da morte... Morte que nunca é temida por todos aqueles que amaram a escuridão da noite e as luzes das estrelas...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>The Old Astronomer to His Pupil</b><br /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><i>Sarah Williams</i></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Reach me down my Tycho Brahe, I would know him when we meet,<br />When I share my later science, sitting humbly at his feet;<br />He may know the law of all things, yet be ignorant of how<br />We are working to completion, working on from then to now.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Pray remember that I leave you all my theory complete,<br />Lacking only certain data for your adding, as is meet,<br />And remember men will scorn it, 'tis original and true,<br />And the obliquy of newness may fall bitterly on you.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">But, my pupil, as my pupil you have learned the worth of scorn,<br />You have laughed with me at pity, we have enjoyed to be forlorn,<br />What for us are all distractions of men's fellowship and smiles;<br />What for us the Goddess Pleasure with her meretricious smiles.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">You may tell that German College that their honor comes too late,<br />But they must not waste repentance on the grizzly savant's fate.<br />Though my soul may set in darkness, it will rise in perfect light;<br />I have loved the stars too fondly to be fearful of the night.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">...............</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">"Reach me down my Tycho Brahe, I would know him when we meet"</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A poeta Sarah Williams nestes versos bem descreveu o sentimento do velho astrônomo em seu leito de morte, deixando seu conhecimento como herança para seu discípulo...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ele pede ao seu discípulo para lhe trazer o retrato pintado de Tycho Brahe, o grande mestre astrônomo anterior a Kepler, a Galileu....para reconhecê-lo quando se encontrarem... E o velho astrônomo tem certeza de que – apesar de Tycho Brahe saber a lei sobre todas as coisas, ainda assim não sabe o que o velho astrônomo já acumulou de conhecimentos, dando continuidade ao trabalho da astronomia desde aquele tempo mais antigo até aquele momento...trabalho esse que, humildemente, o velho astrônomo anseia por compartilhar com o antigo mestre..... Essa é a primeira estrofe.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A segunda estrofe começa com o velho astrônomo deixando como herança ao seu discípulo sua teoria já completa, ao mesmo tempo que fazendo seu herdeiro saber que a esta teoria ele deverá acrescentar mais e mais informações. E o avisa: os homens zombarão dele – apesar de sua teoria se provar original e verdadeira. E sentencia: a ignorância em relação ao novo conhecimento cairá como fel sobre o discípulo.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Na terceira estrofe e nos dois primeiros versos da quarta estrofe, o velho astrônomo devaneia sobre as zombarias e o não-reconhecimento que o discípulo teve oportunidade de vivenciar junto ao seu mestre e sobre o bom-humor e temperança com que ambos tiveram que enfrentar tais vicissitudes...... Também assinala que qualquer honraria agora chegaria tarde demais...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os dois últimos versos da última estrofe são de uma beleza ímpar:</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">"Though my soul may set in darkness, it will rise in perfect light;</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">I have loved the stars too fondly to be fearful of the night."</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Assim, o velho astrônomo termina sua vida dizendo (traduzindo livremente) :</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">"Apesar de minha alma permanecer na escuridão, ela ascenderá plenamente iluminada,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Meu amor pelas estrelas tem sido grande demais para que eu tema a (escuridão da) noite</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">.......ou .. para que eu tema a morte)."</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esse último verso tem sido o grande companheiro<br />de todos aqueles que amam verdadeiramente as estrelas, sejam astrônomos ou não....</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The Old Astronomer to his Pupil</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- Poema de Sarah Williams</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">"Best Loved Poems of the American People"</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Hazel Felleman, ed. Garden City Publishing Co.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Garden City, NY. 1936, pp. 613-614</span></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.3ap.org/sarahWilliams.shtml" style="text-decoration: none;">http://www.3ap.org/sarahWilliams.shtml</a><br /><br /></span><br />
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<b><span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ATLAS DO UNIVERSO</span></span></b></div>
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<a href="http://www.atlasoftheuniverse.com/index.html" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.atlasoftheuniverse.com/index.html</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">This website belongs to <a href="http://www.atlasoftheuniverse.com/me.html" style="text-decoration: none;">Richard Powell</a>.</span></div>
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<span style="text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.atlasoftheuniverse.com/galchart.html</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US"> </span><span lang="EN-US">- </span><b><span lang="EN"><span lang="EN-US"><a href="http://en.wikipedia.org/wiki/Supercluster" style="text-decoration: none;">http://en.wikipedia.org/wiki/</a></span></span></b></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg8P4d6Iaqw9a8Y4MXM7k0r2xIY3gFdLstR4SNcANF0J_9ICIU0pV2m5B2NVW9o_mBXezXgoVZircopTqjm0ubjQBzGtLd2049no12bTWLyNHKkygpXyplOAFHSkS3wr2CRMZ1NVtaIXQFA/s1600/our+home+in+the+unvierse.jpg" imageanchor="1" style="background-color: white; margin-left: 1em; margin-right: 1em;"><span style="color: #073763;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg8P4d6Iaqw9a8Y4MXM7k0r2xIY3gFdLstR4SNcANF0J_9ICIU0pV2m5B2NVW9o_mBXezXgoVZircopTqjm0ubjQBzGtLd2049no12bTWLyNHKkygpXyplOAFHSkS3wr2CRMZ1NVtaIXQFA/s640/our+home+in+the+unvierse.jpg" height="358" width="640" /></span></a></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Extraído do Vídeo </span><br />
<h1 class="yt" id="watch-headline-title" style="border: 0px; font-weight: normal; line-height: normal; margin: 0px 0px 5px; overflow: hidden; padding: 0px; text-align: center; text-overflow: ellipsis; white-space: nowrap; word-wrap: normal;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span class="watch-title yt-uix-expander-head" dir="ltr" id="eow-title" style="-webkit-user-select: auto; border: 0px; cursor: auto; margin: 0px; padding: 0px;" title="Gaia... mapping one billion stars">Gaia... mapping one billion stars - </span><a class="g-hovercard yt-uix-sessionlink yt-user-name " data-name="watch" data-sessionlink="ei=ffeqUoeUH-WKggLauYCwAg&feature=watch" data-ytid="UCIBaDdAbGlFDeS33shmlD0A" dir="ltr" href="https://www.youtube.com/user/ESA?feature=watch" style="border: 0px; cursor: pointer; display: inline-block; font-weight: bold; height: 22px; line-height: 13px; margin: 0px 0px 0px 10px; padding: 0px; text-align: start;">European Space Agency, ESA</a></span></h1>
<a href="https://www.youtube.com/watch?v=skcqEdQ11PQ&feature=youtube_gdata"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">https://www.youtube.com/watch?v=skcqEdQ11PQ&feature=youtube_gdata</span></a></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-4158372707710982464.post-54553826599389455942013-11-30T07:11:00.001-08:002015-04-07T13:27:01.551-07:00Referências Bibliográficas Impressas e Virtuais - meu projeto Da Terra ao Céu e ao Infinito<span style="background-color: white;"><span style="color: #073763;"><br /></span></span>
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<span lang="PT" style="line-height: 36px;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Projeto</span></b></span></div>
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<span lang="PT" style="line-height: 36px;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: medium;">Da Terra ao Céu<o:p></o:p></span></b></span></div>
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<span lang="PT" style="line-height: 36px;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="font-size: medium;">e ao Infinito</span><o:p></o:p></span></b></span></div>
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<span lang="PT" style="line-height: 22px;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">CONSTELAÇÕES, ESTRELAS E OBJETOS CELESTES<o:p></o:p></span></b></span></div>
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<span lang="PT" style="line-height: 22px;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(sob o ponto de vista do Mundo Ocidental)<o:p></o:p></span></b></span></div>
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<span lang="PT" style="line-height: 22px;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SUAS HISTÓRIAS, SEUS MITOS, SEUS SIGNIFICADOS<o:p></o:p></span></b></span></div>
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<span lang="PT" style="line-height: 22px;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E SUAS SINTETIZADAS DESCRIÇÕES</span></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="PT">Reunião das Informações,</span></b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="PT">suas traduções para a língua portuguesa (quando necessário),</span></b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="PT">Compilação e Comentários Pessoais:</span></b><o:p></o:p></span></div>
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<b style="line-height: 13.5pt;"><i><span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></span></i></b></div>
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<span style="color: #bf9000; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo</span></span></div>
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<span style="color: #bf9000; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763; line-height: 18px; text-align: start;">bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.</span></span></div>
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<span style="color: #bf9000; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span></span></div>
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<b><span lang="EN-US"><b><span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Algumas </span></span></b></span></b></div>
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<b><span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">REFERÊNCIAS BIBLIOGRÁFICAS IMPRESSAS E VIRTUAIS</span></span></b></div>
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<b><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Alguns dados</span></b></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>(tais como Ascensão Reta e Declinação, em muitos dos casos)</b><b><o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>são época/equinócio 1980</b><b><o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>e devem requerer do Caminhante do Céu</b><b><o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>alguma pequena retificação.</b><b><o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Obrigada por sua compreensão.</b><b><o:p></o:p></b></span></div>
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<span lang="EN-US"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">BIBLIOGRAFIA VIRTUAL:</span></b></span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Informações atualizadas e preciosas</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>sobre os Objetos Celestiais de seu interesse:</b><b><o:p></o:p></b></span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">NASA/IPAC EXTRAGALACTIC DATABASE</span></b></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Search for Objects by Object Name</span></h2>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="text-decoration: none;"><b>http://ned.ipac.caltech.edu/</b></a><b><o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="text-decoration: none;"><b>http://ned.ipac.caltech.edu/forms/byname.html</b></a><b><o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><em><b><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></b></em><span class="apple-converted-space"><b><i><span lang="EN-US"> </span></i></b></span><em><b><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></b></em></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="The Night Sky Atlas logo image" src="http://www.nightskyatlas.com/logo.gif" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><b><span lang="EN-US"><o:p></o:p></span></b></span></div>
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<b><span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.</span></span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Internet STELLAR DATABASE</span></center>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="text-decoration: none;"><b><span lang="EN-US">http://www.stellar-database.com/</span></b></a><b><span lang="EN-US"><o:p></o:p></span></b></span></div>
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<b><span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<o:p></o:p></span></span></b></div>
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<span style="background-color: white; color: #073763; font-size: x-small;">DOCdb</span></h1>
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<span style="background-color: white;"><span style="color: #073763;">Deep Sky Observer's Companion – the online database</span></span></div>
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<a href="http://www.docdb.net/index.php" style="background-color: white; text-decoration: none;"><span style="color: #073763;">http://www.docdb.net/index.php</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="An Atlas of The Universe" src="http://www.atlasoftheuniverse.com/atlas.gif" height="64" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="320" /></span></div>
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<tr><td class="tr-caption" style="font-size: 13px;"><span style="color: #fff2cc; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">http://www.atlasoftheuniverse.com/galchart.html</span></span></td></tr>
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<b><b><span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ATLAS DO UNIVERSO</span></span></b></b></div>
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<a href="http://www.atlasoftheuniverse.com/index.html" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.atlasoftheuniverse.com/index.html</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">This website belongs to <a href="http://www.atlasoftheuniverse.com/me.html" style="text-decoration: none;">Richard Powell</a>. You may copy this website in its entirety for personal use. Schools and colleges can copy this website for their own internal use. It is always acceptable to use this website for classroom projects.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Text</span></h2>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">All of the text on this website is my intellectual property. You are free to copy, and distribute the text, for <em>non-commercial</em> purposes only, and you must cite this website if you use any of the text in a derivative work. Commercial use of the text must be restricted to small quotations and should cite this website.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Maps and Diagrams</span></h2>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">All of the maps and diagrams on this website belong to me, and are free for anyone to use under the following conditions. They are licenced under a <a href="http://creativecommons.org/licenses/by-sa/2.5/" rel="license" style="text-decoration: none;">Creative Commons Attribution-ShareAlike 2.5 Licence</a>. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">The Night Sky Atlas</span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="The Night Sky Atlas logo image" src="http://www.nightskyatlas.com/logo.gif" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /><b><span lang="EN-US"><br /></span></b></span></div>
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<a href="http://www.nightskyatlas.com/index.jsp" style="text-align: center; text-decoration: none;"><span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.nightskyatlas.com/index.jsp</span></span></a></div>
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<b><span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars. Data sources: Bright Star Catalog from the <a href="http://adc.gsfc.nasa.gov/" style="text-decoration: none;">Astronomical Data Center</a>, star names list from <a href="http://www.naic.edu/~gibson/starnames/" style="text-decoration: none;">Steven Gibson</a>, all-sky Milky Way image by <a href="http://home.arcor-online.de/axel.mellinger/" style="text-decoration: none;">Axel Mellinger</a>. The data used in this product, in whole or in part, is used with permission of <a href="http://www.ngcicproject.org/" style="text-decoration: none;">The NGC/IC Project LLC</a>. Many thanks go to those who maintain and make available their astronomy datasets without which this sky atlas would not have been possible. Permission for any use of these chart images is granted, provided that the original website address remains visible on all images. Enjoy!</span></div>
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<tr><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://upload.wikimedia.org/wikipedia/commons/b/b6/Earth%27s_Location_in_the_Universe_%28JPEG%29.jpg" height="80" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; margin-left: auto; margin-right: auto; padding: 8px;" width="640" /></span></td></tr>
<tr><td class="tr-caption" style="font-size: 13px;"><a href="http://upload.wikimedia.org/wikipedia/commons/b/b6/Earth%27s_Location_in_the_Universe_%28JPEG%29.jpg" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">http://upload.wikimedia.org/wikipedia/commons/b/b6/Earth%27s_Location_in_the_Universe_%28JPEG%29.jpg</span></a></td></tr>
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<table cellpadding="2" class="toccolours vcard layouttemplate" style="border: 1px solid rgb(170, 170, 170); color: #bf9000; direction: ltr; line-height: 19.1875px; padding: 5px; text-align: justify; width: 1112px;"><tbody>
<tr><th class="fileinfo-paramfield" style="padding-right: 0.4em; text-align: right; width: 158.140625px;"><div style="line-height: 1.5em; margin-bottom: 0.5em; margin-top: 0.4em;">
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</th><td style="border: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></td><td style="border: none; text-align: right;"><a class="internal" href="http://upload.wikimedia.org/wikipedia/commons/b/b6/Earth%27s_Location_in_the_Universe_%28JPEG%29.jpg" style="background-image: none; text-decoration: none;" title="Earth's Location in the Universe (JPEG).jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Full resolution</span></a></td></tr>
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<table cellpadding="4" class="toccolours vevent mw-content-ltr" style="border-bottom-color: rgb(170, 170, 170); border-bottom-style: solid; border-left-color: rgb(170, 170, 170); border-left-style: solid; border-right-color: rgb(170, 170, 170); border-right-style: solid; border-width: 0px 1px 1px; direction: ltr; margin-top: -8px; padding: 0px 5px 5px; text-align: justify; width: 1112px;"><tbody>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_desc" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 156.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Description</span></td><td class="description"><div class="description en" lang="en" style="direction: ltr;">
<div style="line-height: 1.5em; margin-bottom: 0.5em; margin-top: 0.4em;">
<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Versions:</span></b></div>
<ul style="line-height: 1.5em; list-style-image: initial; list-style-position: initial; margin: 0.5em 0px; padding: 0px 2.5em;">
<li style="border: none; margin: 0px 0px 0.1em; padding: 0.25em 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A smaller stacked version of the image is available <a href="http://commons.wikimedia.org/wiki/File:Earth%27s_Location_in_the_Universe_SMALLER_(JPEG).jpg" style="background-image: none; text-decoration: none;" title="File:Earth's Location in the Universe SMALLER (JPEG).jpg">here</a> for users with slower browsers.</span></li>
<li style="border: none; margin: 0px 0px 0.1em; padding: 0.25em 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A vertical version of the image is available <a href="http://commons.wikimedia.org/wiki/File:Earth%27s_Location_in_the_Universe_VERTICAL_(JPEG).jpg" style="background-image: none; text-decoration: none;" title="File:Earth's Location in the Universe VERTICAL (JPEG).jpg">here</a>.</span></li>
<li style="border: none; margin: 0px 0px 0.1em; padding: 0.25em 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">An alternative/older version of the image is available <a href="http://commons.wikimedia.org/wiki/File:Universe_Reference_Map_(Location)_001.jpeg" style="background-image: none; text-decoration: none;" title="File:Universe Reference Map (Location) 001.jpeg">here</a>.</span></li>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_date" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 156.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Date</span></td><td><time class="dtstart" datetime="2012-04-04" style="display: inline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">4 April 2012</span></time></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 156.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Source</span></td><td><span class="int-own-work"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Own work</span></span></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 156.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Author</span></td><td><a href="http://commons.wikimedia.org/wiki/User:Azcolvin429" style="background-image: none; text-decoration: none;" title="User:Azcolvin429"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Andrew Z. Colvin</span></a></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_ver" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 156.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Other versions</span></td><td><div style="line-height: 1.5em; margin-bottom: 0.5em; margin-top: 0.4em;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Derivative works of this file:</span></div>
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<li style="border: none; margin: 0px 0px 0.1em; padding: 0.25em 0px;"><a href="http://commons.wikimedia.org/wiki/File:Position_der_Erde_im_Universum_4x2.png" style="background-image: none; text-decoration: none;" title="File:Position der Erde im Universum 4x2.png"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Position der Erde im Universum 4x2.png</span></a></li>
<li style="border: none; margin: 0px 0px 0.1em; padding: 0.25em 0px;"><a href="http://commons.wikimedia.org/wiki/File:Home_in_Relation_to_Everything.png" style="background-image: none; text-decoration: none;" title="File:Home in Relation to Everything.png"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Home in Relation to Everything.png</span></a></li>
</ul>
</td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESA / HUBBLE</span></div>
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<a href="http://www.spacetelescope.org/" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spacetelescope.org/</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">This webpage reproduces a section of </span></div>
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<b><span class="larger"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/home.html" style="text-decoration: none;" target="index"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Star Names</span></a></span></b></div>
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<a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/home.html" style="text-decoration: none;" target="index"><b><span class="larger"><span class="small"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Their Lore and Meaning </span></span></span></b></a></div>
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<b><b><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/home.html" style="text-decoration: none;" target="index"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">by</span></a></b></b></div>
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<b><b><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/home.html" style="text-decoration: none;" target="index"><span class="larger"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Richard Hinckley Allen </span></span></a></b></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">as reprinted</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">in the Dover edition, 1963</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US"> </span><b><span lang="EN-US">Richard Hinckley Allen, Star Names, Their Lore and Meaning</span></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="text-align: center;">Copyright </span><a class="copyright" href="http://www.lindahall.org/index.shtml" style="text-align: center; text-decoration: none;">Linda Hall Library of Science, Engineering, & Technology</a><span style="text-align: center;"> 2005</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="text-align: center;">From </span><a class="copyright" href="http://www.lindahall.org/services/digital/index.shtml" style="text-align: center; text-decoration: none;">Digital Services</a><span style="text-align: center;"> & </span><a class="copyright" href="http://www.lindahall.org/collections/histofsci.shtml" style="text-align: center; text-decoration: none;">History of Science Department</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Tartu Observatoorium" border="0" src="http://www.aai.ee/muuseum/Images/cicon200.gif" height="141" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; text-align: start;" width="200" /><span style="text-align: start;"> </span></span></div>
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<a href="http://www.aai.ee/muuseum/Uranomeetria/HTML/index.html" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.aai.ee/muuseum/Uranomeetria/HTML/index.html</span></a></div>
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<b style="text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uranomeetria</span></b></div>
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<a href="http://www.aai.ee/muuseum/Uranomeetria/HTML/bayer.htm" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Bayer</span></a></div>
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<a href="http://www.aai.ee/muuseum/Uranomeetria/HTML/hevelius.htm" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Hevelius</span></a></div>
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<a href="http://www.aai.ee/muuseum/Uranomeetria/HTML/semleri.htm" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Semleri</span></a></div>
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<a href="http://www.aai.ee/muuseum/Uranomeetria/HTML/bode.htm" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Bode</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.aai.ee/muuseum/Uranomeetria/HTML/reissig.htm" style="text-decoration: none;">Reissig</a> <a href="http://www.aai.ee/muuseum/Uranomeetria/HTML/index.html" style="text-decoration: none;">http://www.aai.ee/muuseum/Uranomeetria/HTML/index.html</a></span></div>
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<a href="http://www.aai.ee/muuseum/Uranomeetria/HTML/braun.htm" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Braun</span></a></div>
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<a href="http://www.aai.ee/muuseum/Uranomeetria/HTML/heis.htm" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Heis</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="font-weight: bold;">Bayer, Johannes</span> 1572-1625</span></div>
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<a href="http://www.aai.ee/muuseum/Uranomeetria/HTML/index.html" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.aai.ee/muuseum/Uranomeetria/HTML/index.html</span></a></div>
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<span style="font-weight: bold; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Johann Hevelius (1611-1687)</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Hevelius_A_03" src="http://www.aai.ee/muuseum/Uranomeetria/HTML/hevelius_a_03.jpg" height="200" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="131" /></span></div>
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<a href="http://www.aai.ee/muuseum/Uranomeetria/HTML/index.html" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.aai.ee/muuseum/Uranomeetria/HTML/index.html</span></a></div>
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<span style="font-weight: bold; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tartu Observatooriumi Virtuaalne Muuseum</span></span></div>
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<a href="http://www.aai.ee/muuseum/Main/HTML/index.html" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.aai.ee/muuseum/Main/HTML/index.html</span></a></div>
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<a href="http://www.raremaps.com/index.html" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/index.html</span></a></div>
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<a href="http://www.raremaps.com/gallery/browse/category/Curiosities/Celestial" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/browse/category/Curiosities/Celestial</span></a></div>
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<span lang="PT"><b><span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">HEAVENS ABOVE</span></span></b></span></div>
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<span lang="PT"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.heavens-above.com/constellation</span></b></span></div>
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<span style="background-color: white; color: #073763;"><b><span lang="EN-US" style="font-family: Arial, sans-serif;">DOCdb</span></b><span lang="EN-US" style="font-size: 12pt;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span lang="EN-US" style="font-family: Arial, sans-serif;">Deep Sky Observer's Companion – the online database</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;"><a href="http://www.docdb.net/object_index.php"><span lang="EN-US">http://www.docdb.net/object_</span></a></span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif; font-size: 12pt;">listing objects by constellation</span><o:p></o:p></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">PROGRAMA STELLARIUM 0.11.1</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sempre em Ilustrações para a Latitude 21s52 e Longitude 43w00.</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh1gqBNg5vfuc0pyDZyI_YW9WriC3lddbYGGhrZbcUMiWKI-hFruwNHnHy81hFleJ1kRgagYo_bMHdH43TUFqWiw24QURR6WGyziZs9YTowMvxF1He6vnsto5s8N-3wKSdJLB_O3Gz61Nvb/s1600/logo+mario+jaci.jpg" imageanchor="1" style="clear: left; float: left; line-height: normal; margin-bottom: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh1gqBNg5vfuc0pyDZyI_YW9WriC3lddbYGGhrZbcUMiWKI-hFruwNHnHy81hFleJ1kRgagYo_bMHdH43TUFqWiw24QURR6WGyziZs9YTowMvxF1He6vnsto5s8N-3wKSdJLB_O3Gz61Nvb/s200/logo+mario+jaci.jpg" height="200" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="128" /></span></a><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: normal;"></span><br /></span><br />
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<span style="line-height: normal;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">AS CARTAS CELESTES REALIZADAS POR MARIO JACI E QUE CONSTAM DESSE TRABALHO - Da Terra ao Céu e ao Infinito - foram escaneadas por mim, Janine, e trabalhadas no programa Corel Photo-Paint X3. </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- </span><b>Mario Jaci Monteiro</b> , <b>As Constelações, Cartas Celestes</b> -<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC </span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh1Go_vnXA9ccsJvY3GM15w66EfhvPl97gQU3VQ9ftXGaBywFvx-60rBHW3YVcNluly4FZcLURO9YchCk43RgT-54iKaZwVXjhKE-EkfHVacrW1lROsas0ZeuyYNXxCwP8rA7heuEpuXcdj/s1600/logo+urania's+mirror.jpg" imageanchor="1" style="clear: left; float: left; margin-bottom: 1em; margin-right: 1em; text-align: justify; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh1Go_vnXA9ccsJvY3GM15w66EfhvPl97gQU3VQ9ftXGaBywFvx-60rBHW3YVcNluly4FZcLURO9YchCk43RgT-54iKaZwVXjhKE-EkfHVacrW1lROsas0ZeuyYNXxCwP8rA7heuEpuXcdj/s200/logo+urania's+mirror.jpg" height="200" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="139" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="text10" style="font-style: italic; line-height: 20px;">Urania’s Mirror</span><span class="text9" style="line-height: 20px;"> is a boxed set of 32 constellation cards first published by Samuel Leigh of the Strand, London, in or shortly before 1825. The engraver was Sidney Hall but authorship was coyly attributed to “a lady”. Peter Hingley, librarian of the Royal Astronomical Society in London, has established that the true author was almost certainly the Reverend Richard Rouse Bloxam of Rugby</span></span></div>
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<a href="http://www.ianridpath.com/atlases/urania.htm" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.ianridpath.com/atlases/urania.htm</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="text11" style="font-weight: bold; line-height: 20px;">Copyright notice: </span><span class="text9" style="line-height: 20px;">The scans on this page, and the larger versions to which they link, are </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="text9" style="line-height: 20px;">© Ian Ridpath</span><span class="text9" style="line-height: 20px;">.</span></span></div>
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<span class="text9" style="line-height: 20px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> You may use them for non-commercial and educational purposes provided appropriate credit is given</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 20.796875px; text-align: start;">Created by an anonymous young lady of London in the early 1800s to make the study of astronomy "familiar and amusing," the original constellation cards included in </span><i style="border: 0px none; line-height: 20.796875px; margin: 0px; padding: 0px; text-align: start;">THE NIGHT SKY: A View of the Heavens,</i><span style="line-height: 20.796875px; text-align: start;"> feature the constellations visible in the Northern Hemisphere. The sumptuous illustrations capture the inspiration of Classical mythology. The stars on the cards are perforated according to their relative magnitude, and when the cards are held up to the light, the natural appearance of the constellations is visible, making it easy for the viewer to pinpoint the constellations in the night sky.</span></span></div>
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<h1 class="milo" id="yui_3_8_1_1_1378757982314_1018" itemprop="name" style="border: 0px none; font-weight: normal; line-height: 25px; margin: 0px; padding: 0px; position: relative;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">The Night Sky: A View of the Heavens Kit</span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> <a href="http://www.barnesandnoble.com/w/the-night-sky-barnes-noble-books/1006330921?ean=9780760761687&itm=1&usri=9780760761687" style="text-decoration: none;">http://www.barnesandnoble.com/w/the-night-sky-barnes-noble-books/1006330921?ean=9780760761687&itm=1&usri=9780760761687</a></span></div>
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<b style="text-align: justify;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">TERRA AGORA E LUA HOJE</span></b></div>
<div id="moon" style="height: 65px; line-height: 11px; margin: 0px auto; text-align: justify; width: 180px;">
<a href="http://www.albinoblacksheep.com/flash/moonsong" style="text-decoration: none;" target="_blank"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="moon phase" src="http://www.albinoblacksheep.com/image/moon/64/moon4.png" height="64" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 0px; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" title="Just like outside, the moon looks like this tonight." width="64" /></span></a></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">BIBLIOGRAFIA IMPRESSA:</span></b></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg0ByksQYAEN9c-esjRllxCDZPetj5XWg0Eb-d_LENob2GajDTxJar3Pmc0Aux7jVEE3SeWS5iWQUO00nkGFn3K09P1s7hUqK_HoJJym73QUKe4uFePgHtLVA_NmLpK1d68iTJ3nH3MQ-Wu/s1600/logo+will+tirion.jpg" imageanchor="1" style="clear: left; float: left; margin-bottom: 1em; margin-right: 1em; text-align: justify; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg0ByksQYAEN9c-esjRllxCDZPetj5XWg0Eb-d_LENob2GajDTxJar3Pmc0Aux7jVEE3SeWS5iWQUO00nkGFn3K09P1s7hUqK_HoJJym73QUKe4uFePgHtLVA_NmLpK1d68iTJ3nH3MQ-Wu/s200/logo+will+tirion.jpg" height="200" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="140" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- </span><b><span lang="EN-US">Wil Tirion - Atlas of the Night Sky</span></b><span lang="EN-US"> - The Hamlyn Publishing Group Limited, London, England<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- </span><b><span lang="EN-US">Antonin Rükl - The Hamlyn Encyclopedia of Stars & Planets</span></b><span lang="EN-US"> - The Hamlyn Publishng Group Limited, London, England<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- </span><b><span lang="EN-US">Richard Hinckley Allen, Star Names, Their Lore and Meaning</span></b><span lang="EN-US">, Dover Publications, Inc, New York, USA <o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- <b>Bernard Pellequer - Pequeno Guia do Céu</b> - Editora Martins Fontes, São Paulo, Brasil<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- <b>Identificação do Céu</b> (Livro que foi sendo revisado e reeditado algumas vezes) de autoria de <b>Fernando Vieira</b>,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Secretaria Municipal de Cultura, Fundação Planetário da Cidade do Rio de Janeiro<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(com dedicatória do próprio autor para mim em Curso de Identificação do Céu, em 30/07/1999))</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do <b>Atlas Celeste</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">de autoria de <b>Ronaldo Rogério de Freitas Mourão</b>,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(com dedicatória do próprio autor para mim<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em evento realizado no Museu de Astronomia do Rio de Janeiro,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em 16/06/1989)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- </span><b>Mario Jaci Monteiro</b> , <b>As Constelações, Cartas Celestes</b> -<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC - com dedicatória do autor para mim, em março de 2004 (quando Mário Jaci generosamente me presenteou com um instrumento de observação (kepleriano) artesanalmente construído por ele).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">AS CARTAS CELESTES REALIZADAS POR MARIO JACI E QUE CONSTAM DESSE TRABALHO - Da Terra ao Céu e ao Infinito - foram escaneadas por mim, Janine, e trabalhadas no programa Corel Photo-Paint X3. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-4158372707710982464.post-66448694281045330392013-11-30T07:10:00.002-08:002015-04-07T13:27:54.024-07:00Meu Projeto DA TERRA AO CÉU E AO INFINITO<div class="MsoNormal" style="font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22px; margin: 0cm 0cm 0pt; text-align: center;">
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<b><span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763;">AO INFINITO.................</span></span></b></div>
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<b><i><span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763;">Janine Milward</span></span></i></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span style="font-size: medium;">Da Terra ao Céu e ao Infinito</span></b> </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">é um Projeto meu que se propõe trazer ao conhecimento do Caminhante do Céu, do Amigo das Estrelas, as 88 Constelações acolhendo seus dados, seus mitos, suas histórias, suas estrelas, suas nebulosas, seus aglomerados globulares e abertos, seus aglomerados de galáxias, seus superaglomerados...., suas muralhas de luz e de sombra...., enfim, tudo aquilo que astronomicamente pode caber em nossos alfarrábios - ou pelo menos, tudo aquilo que eu, Janine, simples amante dos céus estrelados, conseguir amealhar a partir de minha compreensão ainda e sempre simplesmente amadora e respeitosamente braheana.</span><br />
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<b style="font-family: 'Times New Roman'; line-height: normal; text-indent: 0px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="background-color: white; text-decoration: none;">http://daterraaoceueaoinfinito.blogspot.com.br/</a></span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.atlasoftheuniverse.com/galchart.html" style="text-decoration: none;"> </a><img src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh0VSg3woks0qa9wKGLCvRrhyMWT6qER4dqitETgrMvPGow3ObgccQmokGTo9X0-9f09AE_ljkXi6HVfhe6U29YS07sEfyEpD29NGRDqysDNb1OeYJrRnY_3fI-S-xytaW7hRNEH9ZzqbDP/s400/mapa+do+universo+que+vemos+em+positivo.gif" height="300" style="-webkit-box-shadow: rgba(0, 0, 0, 0.498039) 1px 1px 5px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.498039) 1px 1px 5px; padding: 8px;" width="400" /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Fonte da Imagem: </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.atlasoftheuniverse.com/galchart.html<span style="text-align: start;"> </span><a href="http://www.atlasoftheuniverse.com/me.html" style="color: #274e13; text-align: start; text-decoration: none;">Richard Powell</a><span style="font-weight: bold; text-align: start;">.</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: large;">Meu Projeto</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><strong><span style="background-color: white; color: #073763; font-size: large;">DA TERRA AO CÉU E AO INFINITO</span></strong></span></div>
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<b><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: large;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="background-color: white;">http://daterraaoceueaoinfinito.blogspot.com.br/</a></span></b></div>
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<b><span lang="PT" style="font-size: 11pt; line-height: 22px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">CONSTELAÇÕES, ESTRELAS E OBJETOS CELESTES </span></span></b><br />
<b><span lang="PT" style="font-size: 11pt; line-height: 22px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(sob o ponto de vista do Mundo Ocidental)</span></span></b><br />
<span style="background-color: white; color: #073763;"><b><span lang="PT" style="font-size: 11pt; line-height: 22px;"><span style="font-family: Arial, Helvetica, sans-serif;"> </span></span></b><b><span lang="PT" style="font-size: 11pt; line-height: 22px;"><span style="font-family: Arial, Helvetica, sans-serif;">SUAS HISTÓRIAS, SEUS MITOS, SEUS SIGNIFICADOS, </span></span></b></span><br />
<span style="background-color: white; color: #073763;"><b><span lang="PT" style="font-size: 11pt; line-height: 22px;"><span style="font-family: Arial, Helvetica, sans-serif;">SUAS IMAGENS </span></span></b><b><span lang="PT" style="font-size: 11pt; line-height: 22px;"><span style="font-family: Arial, Helvetica, sans-serif;">E SUAS SINTETIZADAS DESCRIÇÕES</span></span></b></span></div>
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<span style="background-color: white; color: #073763;"><b><span lang="PT" style="font-size: 11pt; line-height: 22px;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></span></b><b><span lang="PT" style="font-size: 11pt; line-height: 22px;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></span></b></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> - AS CONSTELAÇÕES -</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> são como janelas que se abrem para a infinitude do universo</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">entre o céu e a terra...,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> bem como percebendo que o caos, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">vagarosamente, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">vai se tornando Cosmos</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> e este por nossa mente sendo conscientizado.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quer dizer, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> <b><span style="font-size: large;">Constelações </span></b></span><br />
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"> já sendo apresentadas em suas Páginas próprias</span><span style="font-family: Arial, Helvetica, sans-serif;">:</span></span><br />
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<span style="background-color: white; color: #073763;"><span style="font-family: "Arial","sans-serif"; font-weight: bold;">ANDROMEDA, </span><span style="font-family: "Arial","sans-serif";"> </span></span><br />
<span style="background-color: white; color: #073763;"><b><span style="font-family: "Arial","sans-serif";">A PRINCESA </span></b><b><span style="font-family: "Arial","sans-serif";">ACORRENTADA</span></b></span><br />
<span style="background-color: white; color: #073763;"><b><span style="font-family: "Arial","sans-serif";"> </span></b><a href="http://sobreandromeda.blogspot.com.br/"><b>http://sobreandromeda.blogspot.com.br/</b></a></span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000; font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;">ANTLIA, A MÁQUINA PNEUMÁTICA</span><span style="color: #320763; font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"> </span></span></b><br />
<a href="http://sobreantlia.blogspot.com.br/"><b><span style="background-color: white; color: #073763;">http://sobreantlia.blogspot.com.br/</span></b></a></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, sans-serif;">APUS, A AVE-DO-PARAÍSO </span></b><br />
<a href="http://sobreapus.blogspot.com.br/"><b><span style="background-color: white; color: #073763; font-family: "Arial","sans-serif";">http://sobreapus.blogspot.com.br/</span></b></a></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: "Arial","sans-serif"; font-weight: bold;">AQUARIUS, O AGUADEIRO</span><span style="font-family: "Arial","sans-serif";"> </span></span><br />
<a href="http://sobreaquarius.blogspot.com.br/"><b><span style="background-color: white; color: #073763;">http://sobreaquarius.blogspot.com.br/</span></b></a></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, sans-serif;">AQUILA, A ÁGUIA </span></b><br />
<span style="background-color: white; color: #073763;"><b><span style="font-family: Arial, sans-serif;"> </span></b><a href="http://sobreaquila.blogspot.com.br/"><b>http://sobreaquila.blogspot.com.br/</b></a><b><span style="color: #244061; font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR; mso-themecolor: accent1; mso-themeshade: 128;"><o:p></o:p></span></b></span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000; font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;">ARA, O ALTAR</span><span style="color: #320763; font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"> </span></span></b><br />
<b><span style="color: #073763; font-family: "Arial","sans-serif";"><a href="http://sobreara.blogspot.com.br/" style="background-color: white;">http://sobreara.blogspot.com.br/</a></span></b></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: "Arial","sans-serif"; font-weight: bold;">ARGO NAVIS, O NAVIO</span><span style="font-family: "Arial","sans-serif";"> </span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> <a href="http://sobreargonavis.blogspot.com.br/"><b><span style="color: #244061; font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR; mso-themecolor: accent1; mso-themeshade: 128; text-decoration: none; text-underline: none;">http://sobreargonavis.blogspot.com.br</span></b></a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="color: #244061; font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;">Esta constelação, o Navio, fazia parte do grupo de 48 constelações relacionado por Ptolomeu.</span><span style="font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"> </span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;">Porém, <b>La Caille dividiu o Navio em Carina, Vela e Puppis: Quilha, Vela e Popa</b></span></div>
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<b style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763;">ARGO NAVIS, O NAVIO</span></b></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://sobreargonavis.blogspot.com.br/2013/11/argo-navis-o-navio-argus.html"><span style="color: #244061; font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR; text-decoration: none; text-underline: none;">http://sobreargonavis.blogspot.com.br/2013/11/argo-navis-o-navio-argus.html</span></a><span style="font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><br /><b>CARINA, A QUILHA</b></span><a href="http://sobreargonavis.blogspot.com.br/2013/11/carina-quilha-do-navio-argus.html"><span style="color: #244061; font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR; text-decoration: none; text-underline: none;">http://sobreargonavis.blogspot.com.br/2013/11/carina-quilha-do-navio-argus.html</span></a><span style="font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><br /><b>PUPPIS, A PÓPA</b></span><a href="http://sobreargonavis.blogspot.com.br/2013/11/puppis-popa-ou-proa-de-argo-navis-o.html"><span style="color: #244061; font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR; text-decoration: none; text-underline: none;">http://sobreargonavis.blogspot.com.br/2013/11/puppis-popa-ou-proa-de-argo-navis-o.html</span></a><span style="font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><br /><b>VELA, A VELA</b></span><a href="http://sobreargonavis.blogspot.com.br/2013/11/vela-em-argo-navis-o-navio-argus.html"><span style="color: #244061; font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR; text-decoration: none; text-underline: none;">http://sobreargonavis.blogspot.com.br/2013/11/vela-em-argo-navis-o-navio-argus.html</span></a></span><span style="font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>AS NUVENS DE MAGALHÃES</b></span></span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://sobrenuvensdemagalhaes.blogspot.com.br/"><b style="background-color: white;">http://sobrenuvensdemagalhaes.blogspot.com.br/</b></a></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>CANCER, O CARANGUEJO</b> </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> <a href="http://sobrecaranguejo.blogspot.com.br/"><b>http://sobrecaranguejo.blogspot.com.br/</b></a></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>CORONA AUSTRALIS E CORONA BOREALIS</b></span></span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://sobrecoronaaustraliseborealis.blogspot.com.br/"><b style="background-color: white;">http://sobrecoronaaustraliseborealis.blogspot.com.br/</b></a></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>CORVUS, O CORVO</b> </span></span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><a href="http://sobrecorvus.blogspot.com.br/" style="background-color: white;">http://sobrecorvus.blogspot.com.br/</a></b></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>CRUX, O CRUZEIRO DO SUL</b></span></span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://sobrecrux.blogspot.com.br/" style="background-color: white;">http://sobrecrux.blogspot.com.br/</a></span><br />
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<span style="color: #632423; mso-themecolor: accent2; mso-themeshade: 128;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">ERIDANUS, O RIO ERIDANO DOS CÉUS ESTRELADOS</b></span></span></div>
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<a href="http://sobreeridanus.blogspot.com.br/"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">http://sobreeridanus.blogspot.com.br/</b></span></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><span style="font-weight: bold;">LYRA, A LIRA</span> </span><br />
<b><span style="color: #073763; font-family: "Arial","sans-serif";"><a href="http://sobrelyra.blogspot.com/" style="background-color: white;">http://sobrelyra.blogspot.com/</a></span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000; font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;">OPHIUCUS, O SERPENTÁRIO,</span><span style="color: #320763; font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"> </span></b><b>E</b></span></div>
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<span style="background-color: white; color: #073763;"><b><span style="font-family: Arial, Helvetica, sans-serif;">SERPENS CAPUT E SERPENS CAUDA, A SERPENTE </span> </b><b><span style="color: #244061; font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR; mso-themecolor: accent1; mso-themeshade: 128; text-decoration: none; text-underline: none;"><a href="http://sobreophiucuseserpens.blogspot.com.br/">http://sobreophiucuseserpens.blogspot.com.br/</a></span></b></span><br />
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<b><span style="background-color: white; color: #073763; font-family: "Arial","sans-serif";">VIRGO, A VIRGEM </span></b><br />
<span style="background-color: white; color: #073763;"><a href="http://sobrevirgo.blogspot.com/"><b>http://sobrevirgo.blogspot.com/</b></a><span style="font-family: "Arial","sans-serif";"> </span></span><br />
<span style="background-color: white; color: #073763;"><span style="font-family: "Arial","sans-serif";"><br /></span><span style="font-family: "Arial","sans-serif";"><b>LONGA JORNADA NOITE ADENTRO: O Revirão da Via Lactea</b></span></span><br />
<span style="color: #073763; font-family: "Arial","sans-serif";"><b><a href="http://oreviraodavialactea.blogspot.com.br/" style="background-color: white;">http://oreviraodavialactea.blogspot.com.br/</a></b></span></div>
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<span style="font-weight: bold;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Boa Leitura e Bons Estudos!</span></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763;">Com um abraço estrelado,<br />Janine Milward</span></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://www.raremaps.com/maps/medium/35567.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<a href="http://www.raremaps.com/gallery/detail/35567/Le_Globe_Celeste/De%20La%20Croix.html" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/detail/35567/Le_Globe_Celeste/De%20La%20Croix.html</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Title: </strong>Le Globe Celeste</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/3554" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; text-decoration: none;">Pherotee De La Croix</a></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.com