NGC 6993 is a large barred spiral galaxy in the constellation of Capricornus. Its velocity with respect to the cosmic microwave background is 5,824±18 km/s, which corresponds to a Hubble distance of 280.2 ± 19.6 Mly (85.91 ± 6.02 Mpc). It was discovered by American astronomer Francis Leavenworth on 8 July 1885. NGC 6993 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.
Galaxy group NGC 6993 is a member of a small group of three galaxies known as [CHM2007] LDC 1426. The other two galaxies are ESO 529-5 and ESO 529-10.
Supernova One Supernova has been observed in NGC 6993:
SN 2020pvb (Type IIn, mag. 21.04) was discovered by Pan-STARRS on 18 July 2020. This supernova was initially detected during a pre-explosion outburst, with the actual supernova occurring several weeks later. Spectral signatures and a plateau-like light curve led scientists to classify SN 2020pvb as Type IIn-P, similar to SN 1994W, SN 2009kn, and SN 2011ht.
Image gallery
See also List of NGC objects (6001–7000)
References
External links Media related to NGC 6993 at Wikimedia Commons NGC 6993 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images



