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The New General Catalogue object NGC 48 is a barred spiral galaxy located approximately 79.3 million light-years from the Solar System [2] in the constellation Andromeda. See also [ edit ]
NGC 317 is a pair of interacting galaxies, consisting of a lenticular galaxy NGC 317A (also designated as PGC 3442) and a spiral galaxy NGC 317B (also designated as PGC 3445), in the constellation Andromeda. It was discovered on October 1, 1885 by Lewis Swift. [2]
UGC 1840, also known as Arp 145, are a pair of interacting galaxies located 250 million light-years away from the Solar System in the Andromeda constellation. [2] The earliest known reference to the pair of galaxies is in part 2 of the Morphological Catalogue of Galaxies, published in 1964, where it is listed as MCG +07-06-002.
NGC 700 is a lenticular galaxy located 200 million light-years away [2] in the constellation Andromeda. NGC 700 was discovered by astronomer Bindon Stoney on October 28, 1850. [3] It is also a member of Abell 262. [4] [5] The galaxy PGC 6924 is often misidentified as NGC 700. [3]
NGC 218, also known as UGC 480, is a spiral galaxy located approximately 500 million light-years from the Sun [2] in the constellation Andromeda. It was discovered on October 17, 1876 by Édouard Stephan , and is interacting with the galaxy PGC 2726 .
Download QR code; Print/export Download as PDF; Printable version; In other projects Wikimedia Commons; ... NGC 425 is a spiral galaxy in the constellation of Andromeda.
NGC 7686 is a moderately-sized open cluster in the constellation Andromeda, containing about 80 stars. [2] At magnitude 5.6, it is an easy target for binoculars and small telescopes. [3] According to Johnson et al. (1961), the "color-magnitude diagram shows merely a uniform scatter with no significant tendency to show a cluster main sequence ...
NGC 708 is an elliptical galaxy located 240 million light-years away [2] in the constellation Andromeda and was discovered by astronomer William Herschel on September 21, 1786. [3] It is classified as a cD galaxy [ 4 ] [ 5 ] and is the brightest member of Abell 262 .