NGC 6070 is a spiral galaxy in the constellation of Serpens. Its velocity with respect to the cosmic microwave background is 2,102±7 km/s, which corresponds to a Hubble distance of 101.1 ± 7.1 Mly (31.00 ± 2.17 Mpc). However, 26 non-redshift measurements give a closer mean distance of 93.43 ± 3.04 Mly (28.646 ± 0.931 Mpc). It was discovered by German-British astronomer William Herschel on 3 May 1786. NGC 6070 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 6070 group NGC 6070 is a member of the NGC 6070 group (also known as LGG 404). The other two galaxies in the group are UGC 10290 and UGC 10288.
Supernova One supernova has been observed in NGC 6070:
SN 2026ejy (Type II, mag. 18.55) was discovered by GOTO on 25 February 2026.
See also List of NGC objects (6001–7000)
References
External links Media related to NGC 6070 at Wikimedia Commons NGC 6070 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


