UGC 2885 (Rubin's Galaxy, nicknamed "Godzilla galaxy") is a large barred spiral galaxy of type SA(rs)c in the constellation Perseus. It is 232 million light-years (71 Mpc) from Earth and measures 463,000 ly (142,000 pc) across, making it one of the largest known spiral galaxies. It is also a possible member of the Pisces-Perseus supercluster. UGC 2885 is a spiral galaxy with a relatively low surface brightness. The central bulge is the most prominent feature of this galaxy, where a faint bar crosses its center. On 17 January 2002, the explosion of a type II supernova was detected as .
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| - UGC 2885 (de)
- UGC 2885 (it)
- UGC 2885 (ja)
- UGC 2885 (pl)
- Galáxia UGC 2885 (pt)
- UGC 2885 (ru)
- UGC 2885 (en)
- UGC 2885 (zh)
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| - UGC 2885 ist eine Riesen-Spiralgalaxie vom Hubble-Typ SA(rs)c im Sternbild Perseus, welche etwa 262 Millionen Lichtjahre von der Milchstraße entfernt ist und einen Durchmesser von etwa 463.000 Lichtjahren besitzt. Die Supernova SN 2002F wurden hier beobachtet. (de)
- UGC 2885は、ペルセウス座にある巨大な渦巻銀河。ヴェラ・ルービンが銀河の回転曲線問題の考察に使ったことから「ルービンの銀河 (英: Rubin's Galaxy)」、またあまりに巨大なことから「ゴジラ銀河 (英: Godzilla galaxy)」などのニックネームが付けられている。カタログ名の「UGC」は、ウプサラ銀河カタログ (Uppsala General Catalogue of Galaxies) の略称。 (ja)
- UGC 2885 — спиральная галактика без перемычки, расположенная на расстоянии 232 млн световых лет от Солнца в созвездии Персея. В галактике вспыхнула сверхновая SN 2002F типа II, её пиковая видимая звездная величина составила 18,1. (ru)
- UGC 2885是一个位于英仙座距地球3.13亿光年的无棒螺旋星系。 (zh)
- UGC 2885 (Rubin's Galaxy, nicknamed "Godzilla galaxy") is a large barred spiral galaxy of type SA(rs)c in the constellation Perseus. It is 232 million light-years (71 Mpc) from Earth and measures 463,000 ly (142,000 pc) across, making it one of the largest known spiral galaxies. It is also a possible member of the Pisces-Perseus supercluster. UGC 2885 is a spiral galaxy with a relatively low surface brightness. The central bulge is the most prominent feature of this galaxy, where a faint bar crosses its center. On 17 January 2002, the explosion of a type II supernova was detected as . (en)
- UGC 2885 è una galassia a spirale situata nella costellazione di Perseo alla distanza di circa 310 milioni di anni luce dalla Terra.È membro periferico del Superammasso di Perseo-Pesci. La galassia ha una bassa luminosità superficiale. Le stelle presenti nel disco sono state strappate via gravitazionalmente da altre galassie. All'osservazione l'aspetto più rilevante è il gigantesco nucleo galattico, mentre i bracci di spirale sono talmente deboli che possono essere osservati solo dopo lunga esposizione nella banda dell'infrarosso. (it)
- UGC 2885 – duża galaktyka spiralna z poprzeczką typu SA (rs) c w gwiazdozbiorze Perseusza. Znajduje się w odległości 232 mln lat świetlnych od Ziemi a jej rozmiary wynoszą 463 tys. lat świetlnych, co czyni ją jedną z największych znanych galaktyk spiralnych. Jest także możliwym członkiem supergromady w Perseuszu-Rybach. UGC 2885 jest galaktyką spiralną o stosunkowo niskiej jasności powierzchniowej. Centralne wybrzuszenie jest najbardziej widoczną cechą tej galaktyki, gdzie jej środek przecina słaba poprzeczka. (pl)
- A UGC 2885 (Uppsala General Catalogue 2885) é uma galáxia espiral com um brilho superficial relativamente baixo. A protuberância central é a característica mais proeminente desta galáxia, onde uma barra fraca cruza seu centro. A falta de interação é evidente pela estrutura quase perfeita dos braços e discos em espiral, falta de caudas das marés e taxa modesta de formação de estrelas - aproximadamente 0,5 massa solar / ano. Em 17 de janeiro de 2002, a explosão de uma supernova tipo II foi detectada como SN 2002F. (pt)
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| - IRAS03497+3526,MCG+06-09-012, TC 49, Z 039.8+3527 (en)
- UGC2885 (en)
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| - UGC 2885 by Hubble Space Telescope. (en)
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| - IRAS 03497+3526, MCG+06-09-012, TC 49, Z 039.8+3527 (en)
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