NGC 1868 explained

NGC 1868
Epoch:J2000
Constellation:Dorado
Ra:[1]
Dist Ly:~163000 ly
Dist Pc:~50000 pc
Appmag V:11.57
Size V:2.7' × 2.7'
Names:NGC 1868, ESO 85-56, KMHK 674, LW 169
Image Size:250

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.

External links

Notes and References

  1. NGC 1868.
  2. Web site: Seligman. Courtney. Celestial Atlas: NGC Objects: NGC 1850 - 1899. cseligman.com. 13 July 2015. https://web.archive.org/web/20150909235341/http://cseligman.com/text/atlas/ngc18a.htm. live. 9 September 2015.
  3. Web site: 1980ApJ...235..769F Page 769 . 2023-04-12 . adsabs.harvard.edu.