NGC 5888 is a barred spiral galaxy in the constellation of Boötes. Its velocity with respect to the cosmic microwave background is 8,817±8 km/s, which corresponds to a Hubble distance of 424.1 ± 29.7 Mly (130.04 ± 9.10 Mpc). It was discovered by German-British astronomer William Herschel on 9 April 1787. NGC 5888 is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms. It also has an active galaxy 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 5888, together with NGC 5886, form a gravitationally bound pair of galaxies.
Supernovae Three supernovae have been observed in NGC 5888:
SN 2007Q (Type II, mag. 17.8) was discovered by Tim Puckett and Jack Newton on 3 January 2007. SN 2010fv (Type II, mag. 20.1) was discovered by Lick Observatory Supernova Search (LOSS) on 1 July 2010. SN 2018lev (Type II, mag. 18.77) was discovered by Gaia Photometric Science Alerts on 29 December 2018.
See also List of NGC objects (5001–6000)
References
External links Media related to NGC 5888 at Wikimedia Commons NGC 5888 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


