NGC 632 is a lenticular galaxy in the constellation of Pisces. Its velocity with respect to the cosmic microwave background is 2,868±22 km/s, which corresponds to a Hubble distance of 138.0 ± 9.7 Mly (42.30 ± 2.98 Mpc). However, eight non-redshift measurements give a closer mean distance of 125.65 ± 6.74 Mly (38.525 ± 2.066 Mpc). It was discovered by British astronomer John Herschel on 24 September 1830. NGC 632 has a possible active galactic 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 632 has a nucleus which shines in the ultraviolet range, and is thus listed in Markarian's catalogue as Mrk 1002.
NGC 645 Group NGC 632 is a member of the NGC 645 group (also known as LGG 28). This group has 5 galaxies, including NGC 638, NGC 645, UGC 1137, and UGC 1172.
Supernova One supernova has been observed in NGC 632:
SN 1998es (Type Ia-pec, mag. 14.6) was discovered by the Lick Observatory Supernova Search (LOSS) on 13 November 1998.
See also List of NGC objects (1–1000)
References
External links Media related to NGC 632 at Wikimedia Commons NGC 632 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


