NGC 958 is a barred spiral galaxy in the constellation of Cetus. Its velocity with respect to the cosmic microwave background is 5505 ± 17 km/s, which corresponds to a Hubble distance of 81.20 ± 5.69 Mpc (~265 million light-years). However, 19 non-redshift measurements give a closer distance of 58.93 ± 12.91 Mpc (~192 million light-years). The galaxy was discovered by German-British astronomer William Herschel on 20 September 1784. NGC 958 is a Seyfert II Galaxy, i.e. it has a quasar-like nuclei with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable. The NASA/IPAC Extragalactic Database (NED) lists NGC 958 as a luminous infrared galaxy (LIRG).
Supernovae Three supernovae have been observed in NGC 958:
SN 2005A (Type Ia, mag. 17.1) was discovered by the Lick Observatory Supernova Search (LOSS) on 5 January 2005. SN 2022ao (Type Ic, mag. 17.997) was discovered by ATLAS on 5 January 2022. SN 2022acbu (Type II, mag. 20.34) was discovered by the Zwicky Transient Facility on 30 November 2022.
See also List of NGC objects (1–1000)
References
External links Media related to NGC 958 at Wikimedia Commons NGC 958 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


