NGC 6453

In this article, we are going to delve into the fascinating world of NGC 6453. From its impact on today's society to its relevance in history, NGC 6453 has played a crucial role in different areas. Throughout these pages, we will analyze the impact NGC 6453 has had on people's lives, examining its influence on culture, art, politics and technology. Additionally, we will explore how NGC 6453 has evolved over time, adapting to the changing circumstances and challenges of the modern world. Get ready to immerse yourself in a journey that will lead you to discover the true importance of NGC 6453 in our lives. Do not miss it!
NGC 6453
NGC 6453, imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
ClassIV [1]
ConstellationScorpius
Right ascension17h 50m 51.71s [2]
Declination−34° 35′ 59.60″ [2]
Distance37.8 kly (11.6 kpc) [1][3]
Apparent magnitude (V)10.10 [1]
Apparent dimensions (V)21.5′[1]
Physical characteristics
Mass169,000 [3] M☉
Metallicity = –1.50 [3] dex
Other designationsESO 393-SC 036, GC 5878, h 3707[4]
See also: Globular cluster, List of globular clusters

NGC 6453 is a globular cluster approximately 37,000 light-years away from Earth in the constellation of Scorpius.[3][2]

The cluster is located approximately 1 kpc (~3,260 light-years) from the Galactic Center,[5] which results in confounded view of the cluster from the Solar System due to many intervening clouds of cosmic dust.[6]

The cluster measures nearly 8' across, and its brightest stars are no brighter than 14th magnitude.[6]

Observational history

NGC 6453 was discovered by John Herschel on June 8, 1837,[7][1][6] while he was observing from the Cape of Good Hope in South Africa.[8] He included the cluster as "h 3708" in his 1864 Catalogue of Nebulae and Clusters of Stars, and Danish-Irish astronomer John Dreyer later added the cluster to his New General Catalogue as object number 6453.[6] Dreyer described the cluster as "considerably large, irregularly round, pretty much brighter (in the) middle, round".[6]

See also

References

  1. ^ a b c d e "SEDS". spider.seds.org. Retrieved December 5, 2017.
  2. ^ a b c "NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved December 5, 2017.
  3. ^ a b c d Boyles, J.; et al. (November 2011), "Young Radio Pulsars in Galactic Globular Clusters", The Astrophysical Journal, 742 (1): 51, arXiv:1108.4402, Bibcode:2011ApJ...742...51B, doi:10.1088/0004-637X/742/1/51, S2CID 118649860.
  4. ^ "New General Catalog Objects: NGC 6450 - 6499". cseligman.com. Retrieved 2017-12-08.
  5. ^ Ortolani, S.; Bica, E.; Barbuy, B. (1999), "Blue horizontal branch globular clusters towards the bulge: Terzan 9, NGC 6139 and NGC 6453", Astronomy and Astrophysics Supplement Series, 138 (2): 267–273, Bibcode:1999A&AS..138..267O, doi:10.1051/aas:1999275
  6. ^ a b c d e Harrington, Philip S. (2010). "Medium-scope challenges". Cosmic Challenge: The Ultimate Observing List for Amateurs. Cambridge University Press. p. 241. ISBN 9781139493680.
  7. ^ "Data for NGC 6453". www.astronomy-mall.com. Retrieved December 9, 2017.
  8. ^ "Universe Today". www.universetoday.com. 19 June 2009. Retrieved December 5, 2017.
Wikimedia Commons has media related to NGC 6453.
Wikious
Boobota
Sagapedia