| NGC 1282 | |
|---|---|
| A near-infrared image of NGC 1282. | |
| Observation data (J2000 epoch) | |
| Constellation | Perseus |
| Right ascension | 03h 20m 12.1s [1] |
| Declination | 41° 22′ 01″ [1] |
| Redshift | 0.007135 [1] |
| Heliocentric radial velocity | 2,139 km/s [1] |
| Distance | 230 Mly (70 Mpc) [1] |
| Group or cluster | Perseus Cluster |
| Apparent magnitude (V) | 13.87 [1] |
| Characteristics | |
| Type | E [1] |
| Size | ~115,000 ly (35.3 kpc) (estimated) [1] |
| Apparent size (V) | 1.4 x 1.1 [1] |
| Other designations | |
| CGCG 540-109, MCG 7-7-68, PGC 12471, UGC 2675 [1] | |
NGC 1282 is an elliptical galaxy [2] located about 230 million light-years away [3] in the constellation Perseus. [4] It was discovered by astronomer Guillaume Bigourdan on October 23, 1884. [5] NGC 1282 is a member of the Perseus Cluster. [5] [6]
A type Ia supernova designated as SN 2008fh was detected near NGC 1282 [7] on either July 30, [7] [8] or August 30, 2008. [9] [10] Oddly, though, the supernova was not associated with the galaxy. [8]