NGC 5172 is an intermediate spiral galaxy in the constellation of Coma Berenices. Its velocity with respect to the cosmic microwave background is 4,308±19 km/s, which corresponds to a Hubble distance of 207.2 ± 14.5 Mly (63.53 ± 4.46 Mpc). However, 13 non-redshift measurements give a closer mean distance of 164.63 ± 11.65 Mly (50.477 ± 3.572 Mpc). It was discovered by British astronomer John Herschel on 7 May 1826. NGC 5172 has a possible active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars. According to Abraham Mahtessian, NGC 5172 and NGC 5190 form a pair of galaxies.
Supernovae Two supernovae have been observed in NGC 5172:
SN 1998cc (Type Ib, mag. 18.1) was discovered by the Lick Observatory Supernova Search (LOSS) on 15 May 1998. SN 2001R (Type II, mag. 18.5) was discovered by LOTOSS (Lick Observatory and Tenagra Observatory Supernova Searches) on 6 January 2001.
See also List of NGC objects (5001–6000)
References
External links Media related to NGC 5172 at Wikimedia Commons NGC 5172 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


