NGC 5508 is a very large and distant spiral galaxy located in the constellation Boötes. Its velocity relative to the cosmic microwave background is 11,615 ± 15 km/s, which corresponds to a Hubble's law of 171 ± 12 Mpc (~558 million light-years). It was discovered by French astronomer Édouard Stephan in 1882. This galaxy is classified by all sources consulted, except Professor Seligman, as a lenticular galaxy. However, the image obtained from the SDSS survey clearly shows that it is a spiral galaxy. According to the Simbad database, NGC 5508 is a LINER galaxy, i.e. a galaxy whose nucleus exhibits an emission spectrum characterized by broad lines of weakly ionized atoms.
The Hubble distance of neighboring galaxy PGC 50725 is 237.51 ± 16.63 Mpc (~775 million light-years), well beyond NGC 5508. Although they appear as neighbors on the celestial sphere, they do not form a physical galaxy pair.
See also List of NGC objects (5001–6000)
References
External links NGC 5508 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images NGC 5508 on the site of Professor C. Seligman NGC 5508 on the SEDS website NGC 5508 on the NASA/IPAC Extragalactic Database Media related to NGC 5508 at Wikimedia Commons



