NGC 1085 is a large spiral galaxy in the constellation of Cetus. Its velocity with respect to the cosmic microwave background is 6,569±16 km/s, which corresponds to a Hubble distance of 316.0 ± 22.1 Mly (96.89 ± 6.79 Mpc). Additionally, 12 non-redshift measurements give a closer mean distance of 276.07 ± 12.60 Mly (84.642 ± 3.862 Mpc). It was discovered by German astronomer Heinrich d'Arrest on 26 September 1865.
NGC 1016 group NGC 1085 is a member of the NGC 1016 galaxy group, which contains 10 members, including NGC 1004, NGC 1016, IC 232, IC 241, IC 1843, UGC 2018, UGC 2019, UGC 2024, and UGC 2051.
Supernovae Two supernovae have been observed in NGC 1085:
SN 2003hk (Type II, mag. 17.6) was discovered by LOTOSS (Lick Observatory and Tenagra Observatory Supernova Searches), and independently by Tom Boles, on 20 August 2003. SN 2025ymh (Type II, mag. 19.55) was discovered by the Large Array Survey Telescope (LAST) on 24 September 2025.
See also List of NGC objects (1001–2000)
References
External links Media related to NGC 1085 at Wikimedia Commons NGC 1085 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


