NGC 5185 is a spiral galaxy in the constellation of Virgo. Its velocity with respect to the cosmic microwave background is 7,683±20 km/s, which corresponds to a Hubble distance of 369.6 ± 25.9 Mly (113.32 ± 7.94 Mpc). Additionally, 16 non-redshift measurements give a similar mean distance of 374.23 ± 10.11 Mly (114.738 ± 3.101 Mpc). It was discovered by German-British astronomer William Herschel on 19 March 1787. NGC 5185 is a Seyfert II galaxy, i.e. it has a quasar-like nucleus with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.
LDC 985 Group NGC 5185 is a member of a group of galaxies known as LDC 985. The other five galaxies in the group are NGC 5181, NGC 5207, NGC 5221, NGC 5222, NGC 5230.
Supernovae Three supernovae have been observed in NGC 5185:
SN 2006br (Type Ia, mag. 17.8) was discovered by Tim Puckett and G. Sostero on 25 April 2006. SN 2006dz (type unknown, mag. 20.0) was discovered by the Carnegie Supernova Project on 31 May 2006. SN 2021gvm (Type II, mag. 19.5747) was discovered by the Zwicky Transient Facility on 21 March 2021.
See also List of NGC objects (5001–6000)
References
External links Media related to NGC 5185 at Wikimedia Commons NGC 5185 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


