NGC 4168 is an elliptical galaxy in the constellation of Virgo. Its velocity with respect to the cosmic microwave background is 2,609±24 km/s, which corresponds to a Hubble distance of 125.5 ± 8.9 Mly (38.48 ± 2.72 Mpc). However, 13 non-redshift measurements give a closer mean distance of 98.35 ± 10.89 Mly (30.154 ± 3.338 Mpc). It was discovered by German-British astronomer William Herschel on 8 April 1784. NGC 4168 is 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.
Virgo cluster NGC 4168 is a member of the Virgo Cluster.
Supernova One supernova has been observed in NGC 4168:
SN 2026acd (Type Ia, mag. 18.876) was discovered by ATLAS on 14 January 2026.
See also List of NGC objects (4001–5000)
References
External links Media related to NGC 4168 at Wikimedia Commons NGC 4168 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


