| NGC 6000 | |
|---|---|
.jpg) The southern half of NGC 6000 imaged by theHubble Space Telescope | |
| Observation data (J2000epoch) | |
| Constellation | Scorpius |
| Right ascension | 15h 49m 49.5423s[1][2] |
| Declination | −29° 23′ 12.797″[1] |
| Redshift | 0.007315±0.000003[1] |
| Heliocentric radial velocity | 2193±1 km/s[1] |
| Galactocentric velocity | 2140±2 km/s |
| Distance | 88.84 ± 7.70 Mly (27.240 ± 2.362 Mpc)[1] |
| Apparent magnitude (V) | 13.01[1] |
| Absolute magnitude (V) | -20.89 +/- 0.36 |
| Characteristics | |
| Type | SB(s)bc[1] |
| Size | ~66,600 ly (20.43 kpc) (estimated)[1] |
| Apparent size (V) | 1.9′ × 1.6′[1] |
| Other designations | |
| ESO 450- G 020,IRAS 15467-2914,MCG -05-37-003,PGC 56145[1] | |
References: NASA/IPAC extragalactic database,http://spider.seds.org/,http://cseligman.com | |
NGC 6000 is abarred spiral galaxy located in the constellationScorpius. Its velocity with respect to thecosmic microwave background is2,328±9 km/s, which corresponds to aHubble distance of 112.0 ± 7.9 Mly (34.33 ± 2.41 Mpc).[1] However, 5non-redshift measurements give a closer mean distance of 88.84 ± 7.70 Mly (27.240 ± 2.362 Mpc).[3] It was discovered by British astronomerJohn Herschel on 8 May 1834.[4] It is designated asSB(s)bc in thegalaxy morphological classification scheme, and is the brightest of all the galaxies in the constellation Scorpius.
NGC 6000 is aSeyfert II galaxy, i.e. it has aquasar-like nucleus with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.[5]
Twosupernovae have been observed in NGC 6000:
Media related toNGC 6000 at Wikimedia Commons | Thisspiral galaxy article is astub. You can help Wikipedia byexpanding it. |
