NGC 869

NGC 869
The Double Cluster, NGC 869 (right) and NGC 884 (left) with north to the top
Observation data (J2000 epoch)
Constellation Perseus
Right ascension 02h 19.1m[1]
Declination +57° 09′[1]
Distance 7.6 kly[2] (2.3 kpc[2])
Apparent magnitude (V) 3.7[1]
Apparent dimensions (V) 30′
Physical characteristics
Mass - M☉
Radius 33.15 ly
Estimated age 13 My [2]
Notable features -
Other designations

Collinder 24,[1] Melotte 13,[1]

h Per,[1] h Persei[1]

NGC 869 is an open cluster located 7600 light years away in the constellation of Perseus.[2] The cluster is most likely around 13 million years old.[2] It is the westernmost of the Double Cluster with NGC 884. NGC 869 and 884 are often designated h and χ Persei, respectively. Some confusion surrounds what Bayer intended by these designations. It is sometimes claimed that Bayer could not have resolved the pair into two patches of nebulosity, and that Chi refers to the Double Cluster and h to a nearby star.[3] Bayer's Uranometria chart for Perseus does not show them as nebulous objects, but his chart for Cassiopeia does, and they are described as Nebulosa Duplex in Schiller's Coelum Stellatum Christianum, which was assembled with Bayer's help.[4] The clusters are both located in the Perseus OB1 association, a few hundred light years apart from each other. The clusters were first recorded by Hipparchus, but have likely been known since antiquity.

The Double Cluster is often photographed and observed with small telescopes. The clusters are visible with the unaided eye between the constellations of Perseus and Cassiopeia as a brighter patch in the winter Milky Way. In small telescopes the cluster appears as an assemblage of bright stars located in a rich star field. Dominated by bright blue stars, the cluster also hosts a few orange stars.

References

  1. 1 2 3 4 5 6 7 "NGC 869". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2006-12-22.
  2. 1 2 3 4 5 Slesnick; Hillenbrand, Lynne A.; Massey, Philip (2002). "The Star Formation History and Mass Function of the Double Cluster h and Chi Persei". Astrophysical Journal. 576 (2): 880–893. arXiv:astro-ph/0205130. Bibcode:2002ApJ...576..880S. doi:10.1086/341865.
  3. ↑ Stephen James O'Meara and Daniel W.E. Green, 2003, "The Mystery of the Double Cluster", Sky and Telescope, Vol. 105, No. 2 (February 2003), p. 116–119.
  4. ↑ Morton Wagman, Lost Stars, McDonald & Woodward, 2003, ISBN 0939923785, p. 240.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.