In this article, we will explore the fascinating world of NGC 6300, a topic that has captured the attention of millions of people around the world. From its origins to its impact on today's society, NGC 6300 has generated debates and reflections on its relevance in various fields. Along these lines, we will immerse ourselves in its history, analyze its most relevant aspects and examine its influence in different areas. With an in-depth approach, this reading invites you to discover and better understand the nuances and complexities that characterize NGC 6300, offering new perspectives and reflections on this exciting topic.
NGC 6300 | |
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![]() NGC 6300 as seen through the New Technology Telescope (NTT) | |
Observation data (J2000 epoch) | |
Constellation | Ara |
Right ascension | 17h 16m 59.5s[1] |
Declination | −62° 49′ 40″[1] |
Redshift | 0.003699±0.000010[1] |
Heliocentric radial velocity | 1109±3 km/s[1] |
Galactocentric velocity | 997±5 km/s[1] |
Distance | 50.9 million light years (15.6 million parsecs) |
Characteristics | |
Type | SB(rs)b[1] |
Size | 64,000 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/ |
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]