| NGC 4146 | |
|---|---|
| NGC 4146 imaged by SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Coma Berenices |
| Right ascension | 12h 10m 18.4s [1] |
| Declination | 26° 25′ 54″ [1] |
| Redshift | 0.021758 [1] |
| Heliocentric radial velocity | 6523 km/s [1] |
| Distance | 300 Mly (93 Mpc) [1] |
| Apparent magnitude (V) | 13.59 [1] |
| Characteristics | |
| Type | (R)SAB(s)ab [1] |
| Size | ~156,200 ly (47.89 kpc) (estimated) [1] |
| Apparent size (V) | 1.4′ × 1.3′ [1] |
| Other designations | |
| UGC 07163, CGCG 158-036, MCG +05-29-028, PGC 038721 [1] | |
NGC 4146 is a spiral galaxy located 300 million light-years away [2] in the constellation Coma Berenices. It was discovered on April 6, 1785, by astronomer William Herschel. [3] NGC 4146 is a field galaxy and is part of the Coma Supercluster. [4] [5]
NGC 4146 is a type 2 seyfert galaxy, [6] and is host to a supermassive black hole with an estimated mass of 4.1 × 108 M☉. [7]
One supernova has been observed in NGC 4146. SN 1963D (type unknown, mag. 15.8) was discovered by Leonida Rosino on January 22, 1963. [8] [9]