Astronomy:NGC 6362
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Short description: Globular cluster in the constellation Ara
NGC 6362 | |
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NGC 6362 | |
Observation data (J2000 epoch) | |
Class | X[1] |
Constellation | Ara |
Right ascension | 17h 31m 54.99s[2] |
Declination | –67° 02′ 54.0″[2] |
Distance | 24.8 kly (7.6 kpc)[3] |
Apparent magnitude (V) | +8.3[4] |
Apparent dimensions (V) | 9' |
Physical characteristics | |
Metallicity | [math]\displaystyle{ \begin{smallmatrix}\left[\ce{Fe}/\ce{H}\right]\end{smallmatrix} }[/math] = –0.99[5] dex |
Estimated age | 13.57 Gyr[5] |
Other designations | GCl 66, C 1726-670[6] |
NGC 6362 is a globular cluster in the constellation Ara, lying close to Apus in the southern sky. A telescope with a 150mm primary mirror is required to resolve the stars within this irregularly shaped cluster.[4] British astronomer James Dunlop first observed the cluster on 30 June 1826. It is located about 25,000 light-years from Earth and contains a number of blue stragglers.[7][8][9]
Gallery
Detailed view of NGC 6362 globular cluster.[10]
References
- ↑ Shapley, Harlow; Sawyer, Helen B. (August 1927), "A Classification of Globular Clusters", Harvard College Observatory Bulletin 849 (849): 11–14, Bibcode: 1927BHarO.849...11S.
- ↑ 2.0 2.1 Goldsbury, Ryan et al. (December 2010), "The ACS Survey of Galactic Globular Clusters. X. New Determinations of Centers for 65 Clusters", The Astronomical Journal 140 (6): 1830–1837, doi:10.1088/0004-6256/140/6/1830, Bibcode: 2010AJ....140.1830G.
- ↑ Paust, Nathaniel E. Q. et al. (February 2010), "The ACS Survey of Galactic Globular Clusters. VIII. Effects of Environment on Globular Cluster Global Mass Functions", The Astronomical Journal 139 (2): 476–491, doi:10.1088/0004-6256/139/2/476, Bibcode: 2010AJ....139..476P.
- ↑ 4.0 4.1 Dunlop, Storm (2005). Atlas of the Night Sky. Collins. ISBN 978-0-00-717223-8. https://archive.org/details/collinsatlasofni0000dunl.
- ↑ 5.0 5.1 Forbes, Duncan A.; Bridges, Terry (May 2010), "Accreted versus in situ Milky Way globular clusters", Monthly Notices of the Royal Astronomical Society 404 (3): 1203–1214, doi:10.1111/j.1365-2966.2010.16373.x, Bibcode: 2010MNRAS.404.1203F.
- ↑ "NGC 6362". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+6362.
- ↑ Atkinson, Nancy (2012-10-31). "Beautiful Star Cluster Looks Surprisingly Youthful". University Today. http://www.universetoday.com/98277/beautiful-star-cluster-is-surprisingly-youthful/.
- ↑ "Dazzling star cluster holds some deceptively young stars". space on NBCnews.com. space.com. http://www.nbcnews.com/id/49625522.
- ↑ "Hubble Sees an Unexpected Population of Young-Looking Stars". Hubble telescope. nasa.gov. http://www.nasa.gov/mission_pages/hubble/science/ngc6362.html.
- ↑ "An unexpected population of young-looking stars". ESA/Hubble Picture of the Week. http://www.spacetelescope.org/images/potw1244a/.
External links
Original source: https://en.wikipedia.org/wiki/NGC 6362.
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