NGC 1954 is a large spiral galaxy in the constellation of Lepus. Its velocity with respect to the cosmic microwave background is 3,172 ± 4 km/s, which corresponds to a Hubble distance of 46.8 ± 3.3 Mpc Mpc (~153 million light-years). It was discovered by German-British astronomer William Herschel on 14 December 1786. The galaxy features two thin arcs which contain HII regions. The galaxy forms a pair with NGC 1957, which lies 5.1 arcminutes away. Other nearby galaxies include IC 2132, MCG -02-14-016, and MCG -03-15-006.
Supernovae Three supernovae have been observed in NGC 1954:
SN 2010ko (Type Ia, mag. 16.8) was discovered by Simone Leonini on 5 December 2010. SN 2011fi (Type II, mag. 17.8), was discovered by Kōichi Itagaki on 27 August 2011. SN 2013ex (Type Ia, mag. 15.6) was discovered by the All Sky Automated Survey for SuperNovae (ASAS-SN) on 19 August 2013.
See also List of NGC objects (1001–2000)
References
External links Media related to NGC 1954 at Wikimedia Commons NGC 1954 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


