NGC 5694 explained

NGC 5694
Epoch:J2000
Class:VII
Constellation:Hydra
Ra:[1]
Dist Ly:114,100ly
Appmag V:10.2[2]
Size V:3.6
Metal Fe:–1.74
Age:13.44 Gyr
Names:Caldwell 66

NGC 5694 (also known as Caldwell 66) is a globular cluster in the constellation Hydra. It was discovered in 1784 by William Herschel.

Characteristics

This globular cluster is located at a distance of 114000ly from the Sun and 96000ly from the Galactic Center[3] and is one of the oldest known globular clusters in the Milky Way Galaxy, forming nearly 12 billion years ago.[4]

Its chemical composition is highly peculiar, being highly (to nearly solar levels) enriched in alpha elements, suggesting an extragalactic origin before being captured by the Milky Way.

See also

Notes and References

  1. NGC 5694 . 2010-12-07.
  2. Web site: SEDS NGC Catalog Online . Results for NGC 5694 . 2010-12-07.
  3. Harris, W.E.. 1996. A Catalog of Parameters for Globular Clusters in the Milky Way. The Astronomical Journal. 112. 1487. 10.1086/118116. 1996AJ....112.1487H.
  4. Web site: NGC/IC Project . Results for NGC 5694 . 2010-12-07 . dead . https://web.archive.org/web/20120520010558/http://www.ngcicproject.org/ngcicdb.asp . 2012-05-20.