NGC 6300 is a barred Seyfert spiral galaxy located in the constellation Ara. It is classified as SB(rs)b in the galaxy morphological classification scheme and was discovered by the Scottish astronomer James Dunlop on 30 June 1826.[3] NGC 6300 is located at about 51 million light years away from Earth. It is suspected that a massive black hole (300,000 times the mass of Sun) may be at its center, pulling all the nearby objects into it. In turn, it emits large amounts of X-rays.[1][4][5]

NGC 6300
NGC 6300 as seen through the New Technology Telescope (NTT)
Observation data (J2000 epoch)
ConstellationAra
Right ascension17h 16m 59.5s[1]
Declination−62° 49′ 40″[1]
Redshift0.003699±0.000010[1]
Heliocentric radial velocity1109±3 km/s[1]
Galactocentric velocity997±5 km/s[1]
Distance50.9 million light years (15.6 million parsecs)
Characteristics
TypeSB(rs)b[1]
Size64,000 light years
Apparent size (V)4.30 × 2.8[2]
Other designations
ESO 101-25, VV 734, IRAS17123-6245 and PGC 60001
References: NASA/IPAC extragalactic datatbase, http://spider.seds.org/

See also

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References

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  1. ^ a b c d e f g "Object No. 1 - NGC 6300". NASA/IPAC extragalactic database. NASA/IPAC. Retrieved 4 October 2015.
  2. ^ "Revised NGC Data for NGC 6300". Seds. Retrieved 4 October 2015.
  3. ^ "NGC 6300 (= PGC 60001)". cseligman. Retrieved 4 October 2015.
  4. ^ "NGC 6300". The NGC/IC Project. Archived from the original on 20 May 2012. Retrieved 4 October 2015.
  5. ^ "ESO's New Technology Telescope Revisits NGC 6300". ESO. Retrieved 4 October 2015.
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