NGC 5875 is a spiral galaxy in the constellation of Boötes. Its velocity with respect to the cosmic microwave background is 3585 ± 6 km/s, which corresponds to a Hubble distance of 52.87 ± 3.70 Mpc (~173 million light-years). It was discovered by German-British astronomer William Herschel on 1 May 1788. The SIMBAD database lists NGC 5875 as 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.
Supernovae Two supernovae have been observed in NGC 5875:
SN 2022oqm (Type Ic-pec, mag. 17.3) was discovered by the Zwicky Transient Facility on 11 July 2022. This supernova has been described as one of the brightest calcium-rich supernovae known. SN 2023ldh (Type IIn, mag. 20.7423) was discovered by the Zwicky Transient Facility on 28 May 2023.
See also List of NGC objects (5001–6000)
References
External links Media related to NGC 5875 at Wikimedia Commons NGC 5875 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


