NGC 4172 is a spiral galaxy in the constellation of Ursa Major. Its velocity with respect to the cosmic microwave background is 9,449±11 km/s, which corresponds to a Hubble distance of 454.6 ± 31.8 Mly (139.37 ± 9.76 Mpc). Additionally, 11 non-redshift measurements give a closer mean distance of 431.86 ± 14.35 Mly (132.409 ± 4.400 Mpc). It was discovered by German-British astronomer William Herschel on 14 April 1789. NGC 4172 is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.
Supernova One supernova has been observed in NGC 4172:
SN 2006az (Type Ia, mag. 17.1) was discovered by Jack B. Newton, L. Cox, and Tim Puckett on 23 March 2006.
See also List of NGC objects (4001–5000)
References
External links Media related to NGC 4172 at Wikimedia Commons NGC 4172 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


