NGC 1281 | |
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![]() A
near-infrared image of NGC 1281. | |
Observation data ( J2000 epoch) | |
Constellation | Perseus |
Right ascension | 03h 20m 06.1s [1] |
Declination | 41° 37′ 48″ [1] |
Redshift | 0.014343 [1] |
Heliocentric radial velocity | 4300 km/s [1] |
Distance | 195.7 ± 3.3 Mly (60 ± 1 Mpc) [2] |
Group or cluster | Perseus Cluster |
Apparent magnitude (V) | 14.5 [1] |
Characteristics | |
Type | E5 [1] |
Mass/Light ratio | 1.7 [3] M☉/ L☉ |
Size | ~17,000 ly (5.2 kpc) (estimated) [1] |
Apparent size (V) | 1.0 x 0.7 [1] |
Half-light radius (physical) | ~4,200 ly (1.3 kpc) (estimated) [3] |
Other designations | |
CGCG 540-108, MCG 7-7-67, PGC 12458 [1] |
NGC 1281 is a compact [3] elliptical galaxy [4] located about 200 million light-years away [3] in the constellation Perseus. [5] NGC 1281 was discovered by astronomer John Dreyer on December 12, 1876. [6] It is a member of the Perseus Cluster. [7] [6]
Like NGC 1277 and NGC 1271, NGC 1281 is a candidate " relic galaxy". [8]
The supermassive black hole in NGC 1281 has an estimated mass of about 10 billion solar masses (1010 M☉). [3] However, Anna Ferré-Mateu et al. estimated the black hole has a mass of no more than 5 billion solar masses. [8]
NGC 1281 | |
---|---|
![]() A
near-infrared image of NGC 1281. | |
Observation data ( J2000 epoch) | |
Constellation | Perseus |
Right ascension | 03h 20m 06.1s [1] |
Declination | 41° 37′ 48″ [1] |
Redshift | 0.014343 [1] |
Heliocentric radial velocity | 4300 km/s [1] |
Distance | 195.7 ± 3.3 Mly (60 ± 1 Mpc) [2] |
Group or cluster | Perseus Cluster |
Apparent magnitude (V) | 14.5 [1] |
Characteristics | |
Type | E5 [1] |
Mass/Light ratio | 1.7 [3] M☉/ L☉ |
Size | ~17,000 ly (5.2 kpc) (estimated) [1] |
Apparent size (V) | 1.0 x 0.7 [1] |
Half-light radius (physical) | ~4,200 ly (1.3 kpc) (estimated) [3] |
Other designations | |
CGCG 540-108, MCG 7-7-67, PGC 12458 [1] |
NGC 1281 is a compact [3] elliptical galaxy [4] located about 200 million light-years away [3] in the constellation Perseus. [5] NGC 1281 was discovered by astronomer John Dreyer on December 12, 1876. [6] It is a member of the Perseus Cluster. [7] [6]
Like NGC 1277 and NGC 1271, NGC 1281 is a candidate " relic galaxy". [8]
The supermassive black hole in NGC 1281 has an estimated mass of about 10 billion solar masses (1010 M☉). [3] However, Anna Ferré-Mateu et al. estimated the black hole has a mass of no more than 5 billion solar masses. [8]