NGC 1872

NGC 1872 is an open cluster within the Large Magellanic Cloud in the constellation Dorado. It was discovered by James Dunlop in 1826.[3]

NGC 1872
NGC 1872, a rich cluster of thousands of stars lying in our small neighbouring galaxy, the Large Magellanic Cloud, 3′ view Credit: ESA/Hubble and NASA
Observation data (J2000 epoch)
Constellation	Dorado[1]
Right ascension	05^h 13^m 11.7^s[2]
Declination	−69° 18′ 45″[2]
Apparent magnitude (V)	11.4[2]
Apparent dimensions (V)	1′[2]
Physical characteristics

NGC 1872 has characteristics of both globular clusters and open clusters - it is visually as rich as a typical globular but is much younger, and, like many open clusters, has bluer stars. Such intermediate clusters are common in the Large Magellanic Cloud.[3]

Gallery

• 
  NGC 1872 wide field view.

References

1. R. W. Sinnott, ed. (1988). The Complete New General Catalogue and Index Catalogue of Nebulae and Star Clusters by J. L. E. Dreyer. Sky Publishing Corporation and Cambridge University Press. ISBN 978-0-933346-51-2.
2. "NGC 1872". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2007-05-02.
3. "NGC 1872: open or globular cluster?". Hubble Space Telescope. ESA. Archived from the original on 13 July 2015. Retrieved 13 July 2015.

External links

• NGC 1872 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images