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NGC 6000

Coordinates: Sky map 15h 49m 49.5423s, −29° 23′ 12.797″
From Wikipedia, the free encyclopedia
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]

NGC 6000 has a glowing yellow centre with glittering blue outskirts.[6]

Supernovae

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Two supernovae have been observed in NGC 6000:

See also

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References

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  1. 1 2 3 4 5 6 7 8 9 10 11 "Results for object NGC 6000". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 21 September 2025.
  2. "Revised NGC Data for NGC 6000". Seds. Retrieved 3 October 2015.
  3. "Distance Results for NGC 6000". NASA/IPAC Extragalactic Database. NASA. Retrieved 21 September 2025.
  4. "NGC 6000 (= PGC 56145)". cseligman. Retrieved 3 October 2015.
  5. "NGC 6000". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 21 September 2025.
  6. "Yellow and blue, old and new". www.esahubble.org.
  7. Monard, L. A. G. (2007). "Supernova 2007ch in NGC 6000". Central Bureau Electronic Telegrams (961): 1. Bibcode:2007CBET..961....1M.
  8. "SN 2007ch". Transient Name Server. IAU. Retrieved 21 September 2025.
  9. Maza, J.; Hamuy, M.; Antezana, R.; Gonzalez, L.; Silva, S.; Folatelli, G.; Cartier, R.; Forster, F.; Marchi, S.; Rojas, A.; Pignata, G.; Cifuentes, M.; Conuel, B.; Reichart, D.; Ivarsen, K.; Haislip, J.; Crain, A.; Foster, D.; Nysewander, M.; Lacluyze, A. (2010). "Supernova 2010as in NGC 6000". Central Bureau Electronic Telegrams (2215): 1. Bibcode:2010CBET.2215....1M.
  10. "SN 2010as". Transient Name Server. IAU. Retrieved 21 September 2025.
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  • Wikimedia Commons logo Media related to NGC 6000 at Wikimedia Commons