NGC 1585 is a spiral galaxy in the constellation of Caelum. Its velocity with respect to the cosmic microwave background is 4,635 ± 31 km/s, which corresponds to a Hubble distance of 68.4 ± 4.8 Mpc (~223 million light-years). It was discovered by British astronomer John Herschel on 1 December 1837. The SIMBAD database lists NGC 1585 as a Seyfert I 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.
Supernovae Two supernovae have been observed in NGC 1585:
SN 2023vio (Type Iax [02cx-like], mag. 19.053) was discovered by ATLAS on 17 October 2023. SN 2025xes (Type Ia, mag. 16.81) was discovered by ATLAS on 10 September 2025.
See also List of NGC objects (1001–2000)
References
External links Media related to NGC 1585 at Wikimedia Commons NGC 1585 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


