NGC 3318 is a barred spiral galaxy in the constellation of Vela. Its velocity with respect to the cosmic microwave background is 3,077±22 km/s, which corresponds to a Hubble distance of 148.0 ± 10.4 Mly (45.38 ± 3.19 Mpc). However, 20 non-redshift measurements give a much closer mean distance of 122.47 ± 2.40 Mly (37.550 ± 0.735 Mpc). It was discovered by British astronomer John Herschel on 2 March 1835. NGC 3318 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.
NGC 3318 group NGC 3318 is part of a galaxy group that bears its name. The NGC 3318 group (also known as LGG 199) has at least 9 galaxies, including NGC 3250, NGC 3250E, NGC 3250B, NGC 3318B, ESO 317-17, ESO 317-19, ESO 317-21, and ESO 317-23.
Supernovae Three supernovae have been observed in NGC 3318:
SN 2000cl (Type IIn, mag. 14.8) was discovered by French amateur astronomer Robin Chassagne (bio-fr) on 26 May 2000. SN 2017ahn (Type II, mag. 18.0896) was discovered by the Distance Less Than 40 Mpc Survey (DLT40) on 8 February 2017. SN 2020aze (Type II, mag. 17.1224) was discovered by DLT40 on 26 January 2020.
See also List of NGC objects (3001–4000)
References
External links Media related to NGC 3318 at Wikimedia Commons NGC 3318 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


