NGC 1892 | |
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![]() NGC 1892 imaged by the Hubble Space Telescope | |
Observation data (2000.0 epoch) | |
Constellation | Dorado |
Right ascension | 05h 17m 9.0s [1] |
Declination | −64° 57′ 35″ [1] |
Redshift | 0.004546 [1] |
Heliocentric radial velocity | 1363 km/s [1] |
Distance | 51 Mly (15.5 Mpc) [2] |
Apparent magnitude (V) | 12.83 [1] [3] |
Absolute magnitude (B) | −16.4 [2] |
Characteristics | |
Type | Scd [2] |
Mass | 4×109 (Stellar mass) [2] M☉ |
Size | ~63,200 ly (19.37 kpc) (estimated) [1] |
Apparent size (V) | 2.9' × 0.8' [1] [3] |
Other designations | |
MCG+03-01-030, 2MFGC 4320, 2MASX J05170905-6457354, IRAS 05169-6500, PGC 17042 [4] |
NGC 1892 is a spiral galaxy located approximately 51 million light-years away [5] the constellation Dorado. It was discovered November 30, 1834 by John Herschel. [3] NGC 1892 is a member of the NGC 1947 Group [6] [7] [8] which is part of the Southern Supercluster. [7]
NGC 1892, despite being a spiral galaxy, has a central bulge which is morphologically more similar to dwarf irregular galaxies. The galaxy's central bulge which is highly irregular, is obscured by a dust lane. [9] NGC 1892 is also host to a nuclear star cluster [10] with an estimated mass of 7.381 million M☉, [11] and a supermassive black hole with an estimated mass 4.7 million M☉. [12]
A probable supernova of type IIP was photographed by the Carnegie-Irvine Galaxy Survey (CGS) in 2004, [13] but it was not noticed until Brazilian amateur astronomer Jorge Stockler de Moraes compared the CGS image to one he took in January 2017. [5]