NGC 5605 is an intermediate spiral galaxy in the constellation of Libra. Its velocity with respect to the cosmic microwave background is 3635 ± 18 km/s, which corresponds to a Hubble distance of 174.9 ± 12.3 Mly (53.61 ± 3.76 Mpc). In addition, three non redshift measurements give a farther distance of 194.72 ± 0.68 Mly (59.700 ± 0.208 Mpc). The galaxy was discovered by German-British astronomer William Herschel on 11 May 1784. The SIMBAD database lists NGC 5605 as a Seyfert II Galaxy, i.e. it has a quasar-like nucleus with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.
Unique Trio of Supernovae NGC 5605 is the only galaxy known where three supernovae were visible at the same time:
SN 2022bn (Type Ib, mag. 18.55) was discovered by ATLAS on 5 January 2022. SN 2022ec (Type II, mag. 18.835) was discovered by ATLAS on 7 January 2022. SN 2022pv (Type II, mag. 19.165) was discovered by ATLAS on 13 January 2022.
See also List of NGC objects (5001–6000)
References
External links Media related to NGC 5605 at Wikimedia Commons NGC 5605 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


