NGC 1427 | |
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![]() Hubble Space Telescope image of NGC 1427 | |
Observation data (J2000 epoch) | |
Constellation | Fornax |
Right ascension | 03h 42m 19.4s[1] |
Declination | −35° 23′ 33″[1] |
Redshift | 0.004630[1] |
Heliocentric radial velocity | 1388 ± 3 km/s[1] |
Distance | 71 ± 8 Mly (21.9 ± 2.4 Mpc)[2] |
Group or cluster | Fornax Cluster |
Apparent magnitude (V) | 11.8[1] |
Absolute magnitude (V) | −20.43[3] |
Characteristics | |
Type | E5[1] |
Mass | 7.9×1010 (Stellar mass)/9.4×1010 (Total Mass)[4] M☉ |
Size | ~109,200 ly (33.49 kpc) (estimated)[1] |
Apparent size (V) | 3.6 x 2.5[1] |
Notable features | Low-luminosity elliptical galaxy |
Other designations | |
ESO 358- G 052, MCG -06-09-021, FCC 276, PGC 13609[1] |
NGC 1427 is a low-luminosity elliptical galaxy[5] located approximately 71 million light-years away from Earth.[2] It was discovered by John Frederick William Herschel on November 28, 1837.[6] It is a member of the Fornax Cluster.[7][8] The galaxy has a stellar mass of 7.9 × 1010 M☉, and a total mass of 9.4 × 1010 M☉.[4] However, the mass of the dark matter halo surrounding the galaxy is around 4.3 × 1012 M☉.[9]
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