NGC 1217 is a spiral galaxy in the constellation of Fornax. Its velocity with respect to the cosmic microwave background is 6,282±15 km/s, which corresponds to a Hubble distance of 302.2 ± 21.2 Mly (92.66 ± 6.49 Mpc). Additionally, one non-redshift measurement provides a much closer distance estimate of 199.93 Mly (61.300 Mpc). It was discovered by British astronomer John Herschel on 23 October 1835. NGC 1217 has an 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 1217 is also 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. It is also a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.
Supernova One supernova has been observed in NGC 1217:
SN 2025ygq (Type Ia, mag. 18.483) was discovered by ATLAS on 22 September 2025.
See also List of NGC objects (1001–2000)
References
External links Media related to NGC 1217 at Wikimedia Commons NGC 1217 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


