NGC 1868

In today's world, NGC 1868 is a topic that has captured the attention of millions of people around the world. Whether due to its historical relevance, its impact on current society, or its influence on popular culture, NGC 1868 is a phenomenon that has generated debate, admiration and controversy. In this article, we will explore the different facets of NGC 1868, analyzing its importance in different areas and examining how it has evolved over time. From its appearance on the public scene to its multiple interpretations, NGC 1868 is a topic that leaves no one indifferent, and its relevance remains palpable today.

NGC 1868
Photograph of NGC 1868 taken by the Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationDorado
Right ascension05h 14m 36s[1]
Declination−63° 57′ 18″[1]
Distance~163000 ly (~50000 pc)
Apparent magnitude (V)11.57[1]
Apparent dimensions (V)2.7' × 2.7'[1]
Physical characteristics
Other designationsNGC 1868, ESO 85-56, KMHK 674, LW 169[1]
See also: Globular cluster, List of globular clusters

NGC 1868 is a globular cluster in the Large Magellanic Cloud in the constellation Dorado.[2] It was discovered by John Herschel in 1834.[2] The cluster is fairly metal-poor and as a result appears relatively blue. It maintains an abundant population of mature giant branch stars which have been used to fit its age to roughly 700 million years old.[3] The cluster is located in a relatively sparse region of the Large Magellanic Cloud which has allowed it to be studied relatively free of crowding from background stars.[3]

References

  1. ^ a b c d e "NGC 1868". SIMBAD. Centre de données astronomiques de Strasbourg.
  2. ^ a b Seligman, Courtney. "Celestial Atlas: NGC Objects: NGC 1850 - 1899". cseligman.com. Archived from the original on 9 September 2015. Retrieved 13 July 2015.
  3. ^ a b Flower, P. J.; Geisler, D.; Olszewski, E. W.; Hodge, P. (1980). "1980ApJ...235..769F Page 769". The Astrophysical Journal. 235: 769. Bibcode:1980ApJ...235..769F. doi:10.1086/157680. Retrieved 2023-04-12.


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