NGC 6919 is an intermediate spiral galaxy in the constellation of Microscopium. Its velocity with respect to the cosmic microwave background is 6,458±14 km/s, which corresponds to a Hubble distance of 310.7 ± 21.8 Mly (95.25 ± 6.67 Mpc). However, 12 non-redshift measurements give a closer mean distance of 246.36 ± 8.67 Mly (75.533 ± 2.658 Mpc). It was discovered by British astronomer John Herschel on 2 September 1836. NGC 6919 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 1408 Group NGC 6919 is a member of a small group of galaxies known as [CHM2007] LDC 1408. The other four galaxies in the group are ESO 285-31, ESO 285-32, ESO 285-40, and ESO 285-42.
Supernova One supernova has been observed in NGC 6919:
SN 2025ezt (Type II, mag. 18.144) was discovered by ATLAS on 20 March 2025.
See also List of NGC objects (6001–7000)
References
External links Media related to NGC 6919 at Wikimedia Commons NGC 6919 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


