NGC 3120 is an intermediate spiral galaxy in the constellation of Antlia. Its velocity with respect to the cosmic microwave background is 3,105±22 km/s, which corresponds to a Hubble distance of 149.4 ± 10.5 Mly (45.80 ± 3.22 Mpc). However, 17 non-redshift measurements give a much closer mean distance of 97.19 ± 5.92 Mly (29.800 ± 1.816 Mpc). It was discovered by British astronomer John Herschel on 22 January 1838. NGC 3120 has a possible active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.
NGC 3038 Group NGC 3120 is a member of the NGC 3038 group (also known as LGG 184). This group has 6 galaxies, including NGC 3038, NGC 3087, IC 2532, ESO 373-21, and ESO 373-26.
Supernovae Two supernovae have been observed in NGC 3120:
SN 1999ca (Type II, mag. 17) was discovered by S. Woodings, R. Martin, and A. Williams on 27 April 1999. SN 2010F (Type II, mag. 14.8) was discovered by The CHilean Automatic Supernova sEarch (CHASE) on 13 January 2010.
See also List of NGC objects (3001–4000)
References
External links Media related to NGC 3120 at Wikimedia Commons NGC 3120 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images }


