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NGC 1987

From Wikipedia, the free encyclopedia
Star cluster in the constellation Mensa
NGC 1987
NGC 1987, imaged by theHubble Space Telescope
Observation data (J2000epoch)
Right ascension05h 27m 17.2s[1]
Declination−70° 44′ 15″[1]
Apparent magnitude (V)12.1[1][2]
Physical characteristics
Other designationsESO 56-SC131, GC 1190, h 2885[3]
Associations
ConstellationMensa
See also:Open cluster,List of open clusters

NGC 1987 (also known asESO 56-SC131) is anopen cluster or aglobular cluster located in theMensa constellation and part of theLarge Magellanic Cloud. It was discovered byJohn Herschel on November 3, 1834. Its apparent magnitude is 12.1, and its size is 1.7arc minutes.[1][2][4] It is thought to be around 600 million years old and has a significant number of red ageing stars.[5]

References

[edit]
  1. ^abcd"Object: NGC 1987 (*)".SEDS. Retrieved28 October 2017.
  2. ^ab"NGC 1987".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved28 October 2017.
  3. ^"NGC 1987".SEDS. Retrieved28 October 2017.
  4. ^"NGC 1987 (in the Large Magellanic Cloud)".cseligman. Retrieved28 October 2017.
  5. ^Zinnecker, H.; Ferraro, F.; Fusi Pecci, F.; Renzini, Alvio; Buonanno, R.; Corsi, C.E.; Turndrup, D.M. (1991-02-28)."Infrared Imaging of Intermediate Age LMC/SMC Clusters". In Haynes, Raymond; Milne, Douglas (eds.).The Magellanic Clouds: Proceedings of the 148th Symposium of the International Astronomical Union, held in Sydney, Australia, July 9–13, 1990. New York: Springer Science & Business Media. pp. 228–30.ISBN 9780792311102.

External links

[edit]
  • Media related toNGC 1987 at Wikimedia Commons


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