NGC 5082 is a lenticular galaxy in the constellation of Centaurus. Its velocity with respect to the cosmic microwave background is 4,153±46 km/s, which corresponds to a Hubble distance of 199.8 ± 14.3 Mly (61.25 ± 4.38 Mpc). However, three non-redshift measurements give a closer mean distance of 152.97 ± 3.46 Mly (46.900 ± 1.060 Mpc). It was discovered by British astronomer John Herschel on 3 June 1834. NGC 5082 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 5082 group NGC 5082 is a member of a small group of galaxies named after it. The other two galaxies in the NGC 5082 group (also known as LGG 348) are ESO 270-7 and ESO 270-14.
Supernova One supernova has been observed in NGC 5082:
SN 1958F (type unknown, mag. 16) was discovered by Milton L. Humason on 13 June 1958.
See also List of NGC objects (5001–6000)
References
External links NGC 5082 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


