NGC 112 is a barred spiral galaxy located in the constellation Andromeda. It was discovered by American astronomer Lewis Swift on September 17, 1885. The galaxy lies approximately 295 million light-years from Earth, and is about 75,000 light-years in diameter. [4]

NGC 112 是 仙女座 的一個 星系。 星等 為13.8， 赤經 為26分48.8秒， 赤緯 為31°42'10"。 在1885年9月17日首次被 路易斯·斯威夫特 發現。 NGC 112是一个非常暗、非常小的、圆形的星系，距地球約2.95億 光年，直徑約7萬5千 光年。

NGC 112 NGC 112 is a spiral galaxy located in the constellation of Andromeda. The NGC is a catalog of 7,840 nebulae, star clusters, and galaxies. Here are the key stats on NGC 112: ... Right Ascension (RA) units = HH:MM:SS.SS Declination (Dec) units = DD:MM:SS.SS

NGC 112是位于仙女座的一个星系。 它的赤经为 0 26.7，赤纬为 31° 43′。

NGC 112 is a Spiral Galaxy located in the constellation of Andromeda in the northern hemisphere. NGC 112's distance from Earth is 278,292,929.27 light years. NGC 112 is called NGC 112 in the New General Catalogue (NGC).

NGC 112 is a barred spiral galaxy located in the constellation Andromeda. It was discovered by American astronomer Lewis Swift on September 17, 1885. The galaxy lies approximately 295 million light-years from Earth, and is about 75,000 light-years in diameter.

NGC 112 is a barred spiral galaxy located in the constellation Andromeda. It was discovered by American astronomer Lewis Swift on September 17, 1885. The galaxy lies approximately 295 million light-years from Earth, and is about 75,000 light-years in diameter. [4] Quick Facts Observation data (J2000 epoch), Constellation ...

NGC 112 is a Spiral Galaxy in the Andromeda constellation. NGC 112 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. Given its B magnitude of 14.5, NGC 112 is visible with the help of a telescope having an aperture of 20 inches (500mm) or more.

NGC 112 是 仙女座 的一个 星系。 星等 为13.8， 赤经 为26分48.8秒， 赤纬 为31°42'10"。 在1885年9月17日首次被 路易斯·斯威夫特 发现。 NGC 112是一个非常暗、非常小的、圆形的星系，距地球约2.95亿 光年，直径约7万5千 光年。

NGC 112 est une galaxie spirale située dans la constellation d'Andromède. Sa vitesse par rapport au fond diffus cosmologique est de 5 978 ± 23 km/s, ce qui correspond à une distance de Hubble de 88,2 ± 6,2 Mpc (∼288 millions d' al) 1.