NGC 1250
Lenticular galaxy in the constellation Perseus
From Wikipedia, the free encyclopedia
NGC 1250 is an edge-on lenticular galaxy located about 275 million light-years away[2] in the constellation Perseus.[3] It was discovered by astronomer Lewis Swift on Oct 21, 1886.[4] NGC 1250 is a member of the Perseus Cluster.[5]
| NGC 1250 | |
|---|---|
SDSS image of NGC 1250. | |
| Observation data (J2000 epoch) | |
| Constellation | Perseus |
| Right ascension | 03h 15m 21.1s[1] |
| Declination | 41° 21′ 20″[1] |
| Redshift | 0.020061[1] |
| Heliocentric radial velocity | 6014 km/s[1] |
| Distance | 276 Mly (84.5 Mpc)[1] |
| Group or cluster | Perseus Cluster |
| Apparent magnitude (V) | 13.96[1] |
| Characteristics | |
| Type | S0^0[1] |
| Apparent size (V) | 2.1 x 0.9[1] |
| Other designations | |
| UGC 2613, MCG +07-07-040, PGC 12098[1] | |