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NGC 2360

Coordinates:Sky map07h 17m 42s, −15° 38′ 00″
From Wikipedia, the free encyclopedia
Open cluster in the constellation Canis Major
NGC 2360
Observation data (J2000epoch)
Right ascension07h 17m 43s[1]
Declination−15° 38′ 29″[1]
Apparent magnitude (V)7.2[2]
Apparent dimensions (V)13[2]
Physical characteristics
Other designationsCaroline's Cluster,[3]Caldwell 58,Cr 134,Mel 64[3]
Associations
ConstellationCanis Major
See also:Open cluster,List of open clusters
Map showing the location of NGC 2360

NGC 2360 (also known asCaroline's Cluster[3] orCaldwell 58) is anopen cluster in theconstellationCanis Major. It was discovered on 26 February 1783[4] byCaroline Herschel, who described it as a "beautiful cluster of pretty compressed stars near 1/2 degree in diameter".[5] Her notes were overlooked until her brotherWilliam included the cluster in his 1786 catalogue of 1000 clusters and nebulae and acknowledged her as the discoverer.[4] The cluster lies 3.5 degrees east ofGamma Canis Majoris and less than one degree northwest of theeclipsing binary starR Canis Majoris; it has a combinedapparent magnitude of 7.2.[5] It is 13 arc minutes in diameter.[2] By the western edge of the cluster is the unrelated star, 5.5-magnitudeHD 56405.[6]

American astronomerOlin J. Eggen surveyed the cluster in 1968, concluding that the brightest star in the field, magnitude-8.96HD 56847, is likely to lie in the field and not a true member of the cluster. He also identified one or possibly twoblue stragglers.[7] These are unexpectedly hot and luminous stars that appear younger than surrounding stars, and have likely developed by sucking matter off companion stars.[8] Four are now recognised to be in the cluster.[9] By analysing the masses of the smallest stars that have evolved intored giants—namely, stars of 1.8 or 1.9 solar masses—Swiss astronomers Jean-Claude Mermilliod andMichel Mayor were able to date the age of the cluster at 2.2 billion years.[10] The cluster has a diameter of around 15 light-years and is located 3700 light-years from Earth.[5]


Sirius andM41 (lower right),M50 (upper left), and NGC 2360 (lower left)

Notes

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  1. ^ab"Results for NGC 2360".NGC/IC Project Database. Archived fromthe original on 2012-05-20. Retrieved2010-12-03.
  2. ^abc"SEDS Online NGC Database".Results for NGC 2360. Retrieved2010-12-03.
  3. ^abc"NGC 2360".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2010-12-03.
  4. ^abHoskin, Michael (2005)."Caroline Herschel as observer"(PDF).Journal for the History of Astronomy.36 (4):373–406.Bibcode:2005JHA....36..373H.doi:10.1177/002182860503600402.S2CID 118428465.
  5. ^abcO'Meara, Stephen James (2002).The Caldwell Objects.Cambridge University Press. pp. 231–33.ISBN 978-0-521-82796-6.
  6. ^Streicher, Magda (April 2006)."Caroline Herschel's Deepsky Discoveries"(PDF).Deepsky Delights. The Astronomical Society of Southern Africa. pp. 234–36. Retrieved16 March 2014.
  7. ^Eggen, Olin J. (1968)."The Intermediate-Age Cluster NGC 2360"(PDF).The Astrophysical Journal.152:83–87.Bibcode:1968ApJ...152...83E.doi:10.1086/149526.
  8. ^Fellman, Megan (17 October 2011)."Astronomers Explain 'Blue Stragglers'".News. Evanston, Illinois:Northwestern University. Retrieved18 March 2014.
  9. ^Ahumada, J. A.; Lapasset, E. (2007)."New catalogue of blue stragglers in open clusters".Astronomy and Astrophysics.463 (2):789–97.Bibcode:2007A&A...463..789A.doi:10.1051/0004-6361:20054590.
  10. ^Mermilliod, Jean-Claude; Mayor, Michel (1990)."Red Giants in Open Clusters. III – Binarity and Stellar Evolution in Five Intermediate-age Clusters: NGC 2360, 2423, 5822, 6811, and IC 4756"(PDF).Astronomy and Astrophysics.273 (1):61–72.Bibcode:1990A&A...237...61M.

External links

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Wikimedia Commons has media related toNGC 2360.


NGC
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Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
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NGC
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Nebulae
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NGC
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