| NGC 5011 | |
|---|---|
| HST image of NGC 5011B (right) and NGC 5011C (left) | |
| Observation data (J2000 epoch) | |
| Constellation | Centaurus |
| Right ascension | 13h 12m 51.848s [1] |
| Declination | −43° 05′ 46.25″ [1] |
| Redshift | 0.010537 [2] |
| Heliocentric 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]