Search results
Results from the WOW.Com Content Network
The constellation's most obvious deep-sky object is the naked-eye Andromeda Galaxy (M31, also called the Great Galaxy of Andromeda), the closest spiral galaxy to the Milky Way and one of the brightest Messier objects. Several fainter galaxies, including M31's companions M110 and M32, as well as the more distant NGC 891, lie within Andromeda.
The Andromeda Galaxy is a barred spiral galaxy and is the nearest major galaxy to the Milky Way. It was originally named the Andromeda Nebula and is cataloged as Messier 31 , M31 , and NGC 224 . Andromeda has a D 25 isophotal diameter of about 46.56 kiloparsecs (152,000 light-years ) [ 8 ] and is approximately 765 kpc (2.5 million light-years ...
The constellation Andromeda as depicted in Urania's Mirror by Sidney Hall, c. 1825. Andromeda is represented in the Northern sky by the constellation Andromeda, mentioned by the astronomer Ptolemy in the 2nd century, which contains the Andromeda Galaxy. Several constellations are associated with the myth.
NGC 67 is an elliptical galaxy located in the constellation Andromeda that was discovered on October 7, 1855, by R. J. Mitchell, who described it as "extremely faint, very small, round". The galaxy belongs to the NGC 68 group, which also contains the galaxies NGC 68, NGC 69, NGC 70, NGC 71, NGC 72, and possibly NGC 74.
Andromeda I is a dwarf spheroidal galaxy (dSph) [5] about 2.40 [4] million light-years away in the constellation Andromeda. Andromeda I is part of the local group of galaxies and a satellite galaxy of the Andromeda Galaxy (M31). It is roughly 3.5 degrees south and slightly east of M31. [6]
NGC 512, also occasionally referred to as PGC 5132 or UGC 944, is a spiral galaxy in the constellation Andromeda. [2] It is located approximately 217 million light-years from the Solar System [4] and was discovered on 17 November 1827 by astronomer John Herschel. [5]
NGC 4565 is a giant spiral galaxy more luminous than the Andromeda Galaxy. [6] Much speculation exists in literature as to the nature of the central bulge. In the absence of clear-cut dynamical data on the motions of stars in the bulge, the photometric data alone cannot adjudge among various options put forth.
Andromeda XXII, And XXII, And 22, Pisces VI, Psc VI, Triangulum I, Tri I [3] Andromeda XXII ( Pisces VI , Triangulum I ) is a low surface brightness dwarf spheroidal galaxy about 940–1,033 kiloparsecs (3.07 × 10 ^ 6 –3.37 × 10 ^ 6 ly) away from the Sun in the constellation Pisces , of the Local Group .