NGC 64 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Cetus |
Right ascension | 00h 17m 30.368s [1] |
Declination | −06° 49′ 28.69″ [1] |
Redshift | 0.024384 [2] |
Helio radial velocity | 7312 ± 9 km/s [2] |
Apparent magnitude (V) | 13.2 [3] |
Characteristics | |
Type | SB(s)bc [2] |
Apparent size (V) | 1.5' × 1.1' [2] |
Other designations | |
NGC 64, MCG 01-01-068, PGC 1149. |
NGC 64 is a barred spiral galaxy discovered by Lewis Swift in 1886, and is located in the Cetus constellation. [3]
NGC 5890 is an unbarred lenticular galaxy in the constellation Libra. It was discovered in April 1785 by Ormond Stone.
NGC 1728 is a spiral galaxy in the constellation Eridanus. The galaxy is listed in the New General Catalogue. It was discovered on November 10, 1885 by the astronomer Edward Emerson Barnard.
NGC 59 is a lenticular galaxy in the constellation Cetus. It is a probable member of the Sculptor Group. It is approximately 17 million light-years away.
NGC 80 is a lenticular galaxy located in the constellation Andromeda. It is interacting with NGC 47 and NGC 68, and is the brightest cluster galaxy of the NGC 80 group, a galaxy group named after it.
NGC 81 is a lenticular galaxy estimated to be about 270 million light-years away in the constellation of Andromeda.
NGC 83 is an elliptical galaxy estimated to be about 260 million light-years away in the constellation of Andromeda. It was discovered by John Herschel in 1828 and its apparent magnitude is 14.2.
NGC 96 is a lenticular galaxy estimated to be about 290 million light-years away in the constellation of Andromeda. It was discovered by Guillaume Bigourdan in 1884 and its apparent magnitude is 17.
NGC 97 is an elliptical galaxy estimated to be about 230 million light-years away in the constellation of Andromeda. It was discovered by John Herschel in 1828 and its apparent magnitude is 13.5.
NGC102 is a lenticular galaxy estimated to be about 330 million light-years away in the constellation of Cetus. It was discovered by Francis Leavenworth in 1886 and its apparent magnitude is 14.
NGC 93 is an interacting spiral galaxy estimated to be about 260 million light-years away in the constellation of Andromeda. It was discovered by R. J. Mitchell in 1854. The galaxy is currently interacting with NGC 90 and has some signs of interacting with it.
NGC 94 is a lenticular galaxy in the constellation Andromeda. It was discovered by Guillaume Bigourdan in 1884. This object is extremely faint and small. A little above the galaxy is NGC 96. NGC 94 is about 260 million light-years away and 50,000 light-years across.
NGC 157 is an intermediate spiral galaxy in the constellation of Cetus. The compiler of the New General Catalogue, John Louis Emil Dreyer noted that NGC 157 was "pretty bright, large, extended, between 2 considerably bright stars". It was discovered on December 13, 1783 by William Herschel.
NGC 149 is a lenticular galaxy in the Andromeda constellation. It was discovered by Édouard Stephan on October 4, 1883.
NGC 161 is a lenticular galaxy in the Cetus constellation. It was discovered on November 21, 1886, by Lewis A. Swift.
NGC 3319 is a barred spiral galaxy in the constellation Ursa Major. It was discovered by William Herschel on Feb 3, 1788. It is rich in gas and lacks a galactic bulge.
NGC 902 is a barred spiral galaxy in the constellation Cetus. It is estimated to be 314 million light-years from the Milky Way and has a diameter of approximately 50,000 ly. NGC 902 was discovered on November 28, 1885 by Francis Leavenworth.
NGC 910 is an elliptical galaxy in the constellation of Andromeda. NGC 910 was discovered on October 17, 1786 by the German-British astronomer William Herschel. It is the brightest galaxy in the cluster Abell 347.
NGC 812 is a spiral galaxy located in the Andromeda constellation, an estimated 175 million light-years from the Milky Way. NGC 812 was discovered on December 11, 1876 by astronomer Édouard Stephan.
NGC 656 is a barred lenticular galaxy located in the Pisces constellation about 175 million light-years from the Milky Way. It was discovered by the Prussian astronomer Heinrich d'Arrest in 1865.
NGC 5384 is a lenticular galaxy in the constellation Virgo. It was discovered on May 8, 1864, by the astronomer Albert Marth. It is located about 250 million light-years away.