NGC 1278 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Perseus |
Right ascension | 03h 19m 54.1s[1] |
Declination | 41° 33′ 48″[1] |
Redshift | 0.020314[1] |
Heliocentric radial velocity | 6090 km/s[1] |
Distance | 231 Mly (70.7 Mpc)[1] |
Group or cluster | Perseus Cluster |
Apparent magnitude (V) | 13.57[1] |
Characteristics | |
Type | E pec[1] |
Size | ~130,000 ly (40 kpc) (estimated)[1] |
Apparent size (V) | 1.5 x 1.3[1] |
Other designations | |
IC 1907, UGC 02670, PGC 012438, CGCG 540-105, MCG +07-07-065[1] |
NGC 1278 is an elliptical galaxy located about 230 million light-years away[2] in the constellation Perseus.[3] NGC 1278 was discovered by astronomer Heinrich d'Arrest on February 14, 1863. It was then rediscovered by astronomer Guillaume Bigourdan on October 22, 1884 and was later listed as IC 1907.[4] NGC 1278 is a member of the Perseus Cluster[5][4] and is a low-luminosity AGN (LLAGN).[6]
One supernova, SN 2016ajf (type Ia, mag. 16.9), was discovered in NGC 1278 on 18 February, 2016.[7]