NGC 5012 is an intermediate spiral galaxy in the constellation of Coma Berenices. Its velocity with respect to the cosmic microwave background is 2,883±19 km/s, which corresponds to a Hubble distance of 138.7 ± 9.8 Mly (42.52 ± 2.99 Mpc). However, 17 non-redshift measurements give a closer mean distance of 122.14 ± 4.22 Mly (37.447 ± 1.295 Mpc). It was discovered by German-British astronomer William Herschel on 10 April 1785. NGC 5012 is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.
NGC 5012 group NGC 5012 is the largest and brightest member of a trio of galaxies. The other two galaxies in the NGC 5012 group (also known as LGG 336) are NGC 5016 and NGC 5012A.
Supernovae Two supernovae have been observed in NGC 5012:
SN 1997eg (Type IIn, mag. 15.6) was discovered by Japanese amateur astronomer Masakatsu Aoki on 4 December 1997. SN 2020kyg (Type Iax[02cx-like], mag. 19.79) was discovered by ATLAS on 24 May 2020.
See also List of NGC objects (5001–6000)
References
External links Media related to NGC 5012 at Wikimedia Commons NGC 5012 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


