| NGC 3951 | |
|---|---|
| SDSS image of NGC 3951. | |
| Observation data (J2000 epoch) | |
| Constellation | Leo |
| Right ascension | 11h 53m 41.2s [1] |
| Declination | 23° 22′ 56″ [1] |
| Redshift | 0.021535 [1] |
| Heliocentric radial velocity | 6456 km/s [1] |
| Distance | 301 Mly (92.3 Mpc) [1] |
| Apparent magnitude (V) | 14.0 [1] |
| Absolute magnitude (B) | -22.62 [1] |
| Characteristics | |
| Type | Sa [1] |
| Size | ~112,000 ly (34.33 kpc) (estimated) [1] |
| Apparent size (V) | 1.16′ × 0.62′ [1] |
| Other designations | |
| UGC 06867, CGCG 127-099, MCG +04-28-090, PGC 037288 [1] | |
NGC 3951 is a spiral galaxy located 300 million light-years away [2] in the constellation Leo. It was discovered on April 10, 1785, by astronomer William Herschel. [3] NGC 3951 is a member of a group of 5 galaxies known as [T2015] nest 100412 or the UGC 6846 Group, [4] which is part of the Coma Supercluster. [5] Other members of the group are UGC 6846, UGC 6855, IC 739, and 2MASX J11543515+2352505. [4]
NGC 3951 is a LINER galaxy, [6] host to a supermassive black hole with an estimated mass of 1 × 108 M☉. [7]