Coordinates: Sky map 15h 49m 49.5423s, −29° 23′ 12.797″

NGC 6000

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NGC 6000
An oval-shaped spiral galaxy, of which only the centre and lower half is in frame. Its centre is mainly golden in colour with a white glowing core, while its thick spiral arms are mostly blue, particularly at the outskirts; the colours merge in between. Dark lanes of dust swirl through the centre, blocking some of its light. Stars and distant galaxies can be seen around the edges on a black background.
The southern half of NGC 6000 imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationScorpius
Right ascension15h 49m 49.5423s[1][2]
Declination−29° 23′ 12.797″[1]
Redshift0.007315±0.000003[1]
Heliocentric radial velocity2193±1 km/s[1]
Galactocentric velocity2140±2 km/s
Distance88.84 ± 7.70 Mly (27.240 ± 2.362 Mpc)[1]
Apparent magnitude (V)13.01[1]
Absolute magnitude (V)-20.89 +/- 0.36
Characteristics
TypeSB(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 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).[1] However, 5 non-redshift measurements give a closer mean distance of 88.84 ± 7.70 Mly (27.240 ± 2.362 Mpc).[3] It was discovered by British astronomer John Herschel on 8 May 1834.[4] 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.[5]

Supernovae

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Two supernovae have been observed in NGC 6000:

  • SN 2007ch (Type II, mag. 17.2) was discovered by L. A. G. "Berto" Monard on 11 May 2007.[6][7]
  • SN 2010as (Type Ib/Ic, mag. 15.5) was discovered by The CHilean Automatic Supernova sEarch (CHASE) on 19 March 2010.[8][9]

See also

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References

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  9. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
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  • Error creating thumbnail: File missing Media related to Lua error in Module:Commons_link at line 62: attempt to index field 'wikibase' (a nil value). at Wikimedia Commons


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