NGC 5011 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Centaurus |
Right ascension | 13h 12m 51.848s [1] |
Declination | −43° 05′ 46.25″ [1] |
Redshift | 0.010537 [2] |
Helio radial velocity | 3159 km/s [2] |
Distance | 133.26 ± 18.56 Mly (40.857 ± 5.692 Mpc) [2] |
Apparent magnitude (V) | 11.33 [3] |
Apparent magnitude (B) | 12.14 [3] |
Characteristics | |
Type | E1-2 [2] |
Size | 92,800 ly (28,440 pc) [2] [note 1] |
Apparent size (V) | 1.763′ × 1.552′ [1] [note 1] |
Other designations | |
MGC-07-27-042, PGC 45898 [3] |
NGC 5011 is an elliptical galaxy in the constellation of Centaurus. [2] It was discovered on 3 June 1834 by John Herschel. [4] It was described as "pretty bright, considerably small, round, among 4 stars" by John Louis Emil Dreyer, the compiler of the New General Catalogue. [4]
Several galaxies are not physically associated with NGC 5011, but appear close to NGC 5011 in the night sky. PGC 45847 is a spiral galaxy that is also known as NGC 5011A. [5] PGC 45918 is a lenticular galaxy [6] some 156 million light-years away from the Earth, in the Centaurus Cluster, and is designated NGC 5011B. [7] PGC 45917 is a dwarf galaxy, also designated NGC 5011C. [8] [7] Although NGC 5011B and 5011C appear close together, they are no signs of them interacting. [7] NGC 5011C is actually much closer and is in the Centaurus A/M83 Group, at 13 million light years away. [7]
NGC 12 is an intermediate spiral galaxy in the Pisces constellation. It was discovered by William Herschel on December 6, 1790.
NGC 38 is a spiral galaxy in the constellation Pisces. It was discovered in 1881.
NGC 78 is a pair of galaxies in the constellation Pisces. NGC 78A, which is the more southern galaxy, is a barred spiral galaxy. NGC 78B, which is the more northern galaxy, is an elliptical galaxy. Although the designations NGC 78A and 78B are used today, the designation NGC 78 was formerly used mainly for the northern galaxy.
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 125 is a lenticular galaxy located in the constellation Pisces. It is designated as subclass Sa Ring in the galaxy morphological classification scheme. It lies approximately 235 million light-years away.
NGC 150 is a barred spiral galaxy in the constellation Sculptor. It is about 70 million light years away from the Solar System, and it has a diameter of about 55,000 light years. It was discovered on 20 November 1886, by Lewis A. Swift. The Type II supernova SN 1990K was detected in NGC 150, and was reported to be similar to SN 1987A.
NGC 252 is a lenticular galaxy located in the constellation Andromeda. It was discovered by William Herschel in 1786.
NGC 3610 is an elliptical galaxy in the constellation Ursa Major. It was discovered on 8 April 1793 by William Herschel.
NGC 5002 is a Magellanic spiral galaxy in Canes Venatici. It was discovered by Heinrich d'Arrest in 1865. It is also known as MCG 6-29-51, PGC 45728, UGC 8254.
NGC 5470 is an edge-on spiral galaxy located between 43 and 68 million light-years away in the constellation Virgo. It was discovered by astronomer John Herschel in 1830. It is a member of the Virgo III Groups, a series of galaxies and galaxy clusters strung out to the east of the Virgo Supercluster of galaxies.
NGC 5026 is a barred spiral galaxy or lenticular galaxy in the constellation of Centaurus. It was discovered on 5 June 1834 by John Herschel. It was described as "pretty bright, pretty large, round, gradually brighter middle" by John Louis Emil Dreyer, the compiler of the New General Catalogue.
NGC 1573 is an elliptical galaxy in the constellation of Camelopardalis. It was discovered on 1 August 1883 by Wilhelm Tempel. It was described as "very faint, small" by John Louis Emil Dreyer, the compiler of the New General Catalogue. It is located about 190 million light-years away.
NGC 1077 is a spiral galaxy in the constellation Perseus. It was discovered on 16 August 1886 by Lewis A. Swift. It was described as "very faint, pretty large, extended" by John Louis Emil Dreyer, the compiler of the New General Catalogue.
NGC 5559 is a barred spiral galaxy, located 240 million light-years away in the constellation of Boötes. It was discovered on April 10, 1785 by the astronomer William Herschel.
NGC 7812 as is an intermediate spiral galaxy in the constellation Sculptor, though it might look like it is in Pisces if observed at the wrong angle. The galaxy was discovered on 25 September 1865 by Sir John Hershel. At its widest, it measures approximately 100-thousand light years across, and is 315 million light years away from Earth.
NGC 801 is a spiral galaxy with an active galaxy core in the constellation Andromeda. It is estimated to be 174 million light-years from the Milky Way and has a diameter of approximately 174,400 light-years. The object was discovered on September 20, 1885 by the American astronomer Lewis A. Swift.
NGC 880 is a spiral galaxy located in the constellation Cetus about 590 million light-years from the Milky Way. It was discovered by the American astronomer Francis Leavenworth in 1886.
NGC 2227 is a barred spiral galaxy with a morphological type of SB(rs)c located in the direction of the Canis Major constellation. It was discovered on January 27, 1835, by John Herschel.
NGC 992 is a spiral galaxy in the Aries constellation and is estimated to be 188 million light years from the Milky Way. NGC 992 was discovered by astronomers Lewis A. Swift on September 6, 1886.
NGC 3005 is an edge-on spiral galaxy in the constellation of Ursa Major, discovered by Bindon Stoney on January 25, 1851. It is a member of the NGC 2998 group, which also includes NGC 2998, NGC 3002, NGC 3006, NGC 3008, and a few others.