NGC 2980 is an intermediate spiral galaxy in the constellation of Sextans. Its velocity with respect to the cosmic microwave background is 6,088±24 km/s, which corresponds to a Hubble distance of 292.9 ± 20.5 Mly (89.79 ± 6.30 Mpc). However, 12 non-redshift measurements give a closer mean distance of 257.99 ± 9.79 Mly (79.100 ± 3.003 Mpc). It was discovered by German-British astronomer William Herschel on 27 March 1786. NGC 2980 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.
Supernovae Two supernovae have been observed in NGC 2980:
SN 2006ba (Type IIb, mag. 18.4) was discovered by Berto Monard on 19 March 2006. SN 2009lm (Type II-P, mag. 18.5) was discovered by the Lick Observatory Supernova Search (LOSS) on 17 November 2009.
See also List of NGC objects (2001–3000)
References
External links Media related to NGC 2980 at Wikimedia Commons NGC 2980 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


