| NGC 1260 | |
|---|---|
| NGC 1260 imaged by the Hubble Space Telescope | |
| Observation data (J2000 epoch) | |
| Constellation | Perseus |
| Right ascension | 03h 17m 27.2s [1] |
| Declination | +41° 24′ 19″ [1] |
| Redshift | 0.01919 [1] |
| Heliocentric radial velocity | 5753 ± 14 km/s [1] |
| Distance | 250 ± 1.6 Mly (76.7 ± 0.5 Mpc) [2] |
| Apparent magnitude (V) | 14.3 [1] |
| Characteristics | |
| Type | S0/a [1] |
| Apparent size (V) | 1.1′ × 0.5′ [1] |
| Other designations | |
| UGC 02634, PGC 012219, MCG +07-07-047 [1] | |
NGC 1260 is a spiral or lenticular galaxy [3] located 250 million light years away from earth in the constellation Perseus. [4] It was discovered by astronomer Guillaume Bigourdan on 19 October 1884. [5] NGC 1260 is a member of the Perseus Cluster [6] [3] and forms a tight pair with the galaxy PGC 12230. [3] This galaxy is dominated by a population of many old stars. [7]
In 2006, it was home to the second brightest supernova in the observable universe, supernova SN 2006gy. This supernova was the most energetic and brightest supernova on record so far. [8]