NGC 7292 is a barred irregular galaxy in the constellation of Pegasus. Its velocity with respect to the cosmic microwave background is 652±24 km/s, which corresponds to a Hubble distance of 31.4 ± 2.5 Mly (9.62 ± 0.76 Mpc). However, six non-redshift measurements give a larger mean distance of 38.55 ± 4.13 Mly (11.820 ± 1.266 Mpc). It was discovered by French astronomer Édouard Stephan on 29 August 1872. NGC 7292 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.
Supernovae Two supernovae have been observed in NGC 7292.
SN 1964H (Type II, mag. 13.5) was discovered by Howard Stiles Gates on 16 June 1964. SN 2026fov (Type II, mag. 13.5) was discovered by Kōichi Itagaki on 14 March 2026. It was located 11".6 east and 24".5 north of the center of NGC 7292.
See also List of NGC objects (7001–7840)
References
External links Media related to NGC 7292 at Wikimedia Commons NGC 7292 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


