NGC 4051 | |
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![]() NGC 4051 imaged by the Hubble Space Telescope | |
Observation data (J2000 epoch) | |
Constellation | Ursa Major |
Right ascension | 12h 03m 09.686s [1] |
Declination | +44° 31′ 52.54″ [1] |
Redshift | 0.002336 [2] |
Heliocentric radial velocity | 700 km/s [2] |
Distance | 54.14 ± 0.98 Mly (16.6 ± 0.3 Mpc) [3] |
Group or cluster | Ursa Major Cluster |
Apparent magnitude (V) | 12.92 [4] |
Apparent magnitude (B) | 11.08 [4] |
Characteristics | |
Type | SAB(rs)bc [2] |
Size | 78,800 ly (24,160 pc) [2] [note 1] |
Apparent size (V) | 6.00′ × 4.98′ [2] [note 1] |
Other designations | |
IRAS 12005+4448, UGC 7030, PGC 38068, CGCG 243-038 [4] [2] |
NGC 4051 is an intermediate spiral galaxy in the constellation of Ursa Major. [2] It was discovered on 6 February 1788 by John Herschel. [5]
NGC 4051 contains a supermassive black hole with a mass of 1.73 million M☉. [6] This galaxy was studied by the Multicolor Active Galactic Nuclei Monitoring 2m telescope. [7]
The galaxy is a Seyfert galaxy that emits bright X-rays. However, in early 1998 the X-ray emission ceased as observed by the Beppo-SAX satellite. X-ray emission had risen back to normal by August 1998. [8]
NGC 4051 is a member of the Ursa Major Cluster. [9] [10] [11] Its peculiar velocity is −490 ± 34 km/s, consistent with the rest of the cluster. [3]
Three supernovae have been discovered in NGC 4051:
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