NGC 2642 is a barred spiral galaxy in the constellation of Hydra. Its velocity with respect to the cosmic microwave background is 4632 ± 21 km/s, which corresponds to a Hubble distance of 68.32 ± 4.79 Mpc (~223 million light-years). It was discovered by British astronomer John Herschel on 19 February 1830. According to the SIMBAD database, NGC 2642 is a Seyfert I galaxy, i.e. it has a quasar-like nuclei with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.
Supernovae Three supernovae have been observed in NGC 2642:
SN 2002fj (Type IIn, mag. 15.8) was discovered by Berto Monard on 12 September 2002. SN 2008bh (Type II, mag. 16.3) was discovered by the Lick Observatory Supernova Search (LOSS) and by The CHilean Automatic Supernova sEarch (CHASE) on 23 March 2008. SN 2023aaby (Type Ic, mag. 17.943) was discovered by ATLAS on 14 December 2023.
See also List of NGC objects (2001–3000)
References
External links Media related to NGC 2642 at Wikimedia Commons NGC 2642 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


