NGC 1792
NGC 1792 is a spiral galaxy located in the Columba constellation. It was discovered by James Dunlop on October 4, 1826. It is located about 36.4 million light-years away.[3]
Hubble image of NGC 1792
| NGC 1792 | |
|---|---|
 | |
| Observation data (J2000 epoch) | |
| Constellation | Columba |
| Right ascension | 05h 05m 14.454s[1] |
| Declination | −37° 58′ 50.70″[1] |
| Redshift | 0.004059[2] |
| Helio radial velocity | 1214.3 km/s[2] |
| Distance | 36.4 Mly (11.17 Mpc)[3] |
| Apparent magnitude (V) | 10.18[2] |
| Apparent magnitude (B) | 10.68[2] |
| Characteristics | |
| Type | SA(rs)bc |
| Other designations | |
| PGC 16709, ESO 305-6, MCG -6-12-004, ESO LV3050060, IRAS 05035-3802[2] | |
References
- Skrutskie, M.; et al. (2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708.
- "NGC 1792". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-12-12.
- Tully, R. Brent; Courtois, Hélène M.; Sorce, Jenny G. (2016). "Cosmicflows-3". The Astronomical Journal. 152 (2): 21. arXiv:1605.01765. Bibcode:2016AJ....152...50T. doi:10.3847/0004-6256/152/2/50. 50.
External links
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Wikimedia Commons has media related to NGC 1792. |
http://www.skyfactory.org/deepskycatalogue/db_list.asp?q=(Name~contains~NGC1792)
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