NGC 6000 is a barred spiral galaxy located in the constellation Scorpius. Its velocity with respect to the cosmic microwave background is 2,328±9 km/s, which corresponds to a Hubble distance of 112.0 ± 7.9 Mly (34.33 ± 2.41 Mpc). However, 5 non-redshift measurements give a closer mean distance of 88.84 ± 7.70 Mly (27.240 ± 2.362 Mpc). It was discovered by British astronomer John Herschel on 8 May 1834. It is designated as SB(s)bc in the galaxy morphological classification scheme, and is the brightest of all the galaxies in the constellation Scorpius. NGC 6000 is 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. NGC 6000 has a glowing yellow centre with glittering blue outskirts.
Supernovae Two supernovae have been observed in NGC 6000:
SN 2007ch (Type II, mag. 17.2) was discovered by Berto Monard on 11 May 2007. SN 2010as (Type Ib/Ic, mag. 15.5) was discovered by The CHilean Automatic Supernova sEarch (CHASE) on 19 March 2010.
See also List of NGC objects (5001–6000)
References
External links Media related to NGC 6000 at Wikimedia Commons


