Key facts
- Constellation
- Dorado
- Right ascension
- 05 17 9.0
- Declination
- −64 ° 57 ′ 35 ″
- Heliocentric radial velocity
- 1363 km/s
- Distance
- 51 Mly (15.5 Mpc )
- Absolute magnitude b
- −16.4
- Type
- Scd
- Mass
- 4 × 10 (Stellar mass) M ☉
- Size
- ~63,200 ly (19.37 kpc ) (estimated)
- Apparent size v
- 2.9' × 0.8'
via Wikipedia infobox
Wikidata facts
- Distance from Earth
- 14
- Image
- NGC 1892 hst 09042 25 R814 B450 hst 06359 06 G606.png
Show 11 more facts
- catalog code
- Gaia DR2 4663665160049782528
- galaxy morphological type
- Sb
- Commons category
- NGC 1892
- time of discovery or invention
- 1834-00-00
- redshift
- 0.004546
- apparent magnitude
- 9.645
- right ascension
- 79.28759399573970
- declination
- -64.95966737213230
- radial velocity
- 1323
- right ascension component of proper motion
- -1.447
- declination component of proper motion
- 0.610
Sources (3)
via Wikidata · CC0
~1 min read
Article
NGC 1892 is a spiral galaxy located approximately 51 million light-years away the constellation Dorado. It was discovered November 30, 1834 by John Herschel. NGC 1892 is a member of the NGC 1947 Group which is part of the Southern Supercluster.
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. NGC 1892 is also host to a nuclear star cluster with an estimated mass of 7.381 million M☉, and a supermassive black hole with an estimated mass 4.7 million M☉.
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via Wikidata sitelinks · CC0