NGC 4162 is a spiral galaxy in the constellation of Coma Berenices. Its velocity with respect to the cosmic microwave background is 2,878±21 km/s, which corresponds to a Hubble distance of 138.5 ± 9.8 Mly (42.45 ± 2.99 Mpc). However, 19 non-redshift measurements give a closer mean distance of 118.00 ± 5.96 Mly (36.179 ± 1.828 Mpc). It was discovered by German-British astronomer William Herschel on 10 April 1785. NGC 4162 has an 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.
Supernovae Three supernovae have been observed in NGC 4162:
SN 1965G (type unknown, mag. 14) was discovered by Mexican astronomer Guillermo Haro on 23 March 1965. SN 2001hg (Type II, mag. 17.4) was discovered by Tim Puckett and Ajai Sehgal on 4 December 2001. SN 2019edo (Type II, mag. 16.7) was discovered by ASAS-SN on 27 April 2019.
See also List of NGC objects (4001–5000)
References
External links Media related to NGC 4162 at Wikimedia Commons NGC 4162 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


