NGC 5612 is a spiral galaxy in the constellation of Apus. Its velocity with respect to the cosmic microwave background is 2,790±42 km/s, which corresponds to a Hubble distance of 134.2 ± 9.8 Mly (41.16 ± 3.01 Mpc). Additionally, two non-redshift measurements give a closer mean distance of 127.36 ± 14.51 Mly (39.050 ± 4.450 Mpc). It was discovered by British astronomer John Herschel on 23 May 1835. NGC 5612 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.
LDC 1118 group NGC 5612 belongs to the 6 member galaxy group known as LDC 1118. The other galaxies in the group include IC 4522, IC 4555, ESO 22-10, LEDA 235897, and LEDA 5061296.
Supernova One supernova has been observed in NGC 5612:
SN 2004ch (Type II, mag. 16) was discovered by the Perth Automated Supernova Search on 28 May 2004.
See also List of NGC objects (5001–6000)
References
External links Media related to NGC 5612 at Wikimedia Commons NGC 5612 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


