NGC 884

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NGC 884
Double Cluster.jpg
The Double Cluster, NGC 869 (top) and NGC 884 (bottom) with north to the left
Observation data (J2000 epoch)
Constellation Perseus
Right ascension 02h 22.0m[1]
Declination +57° 08′[1]
Distance 7.6 kly[2] (2.3 kpc[2])
Apparent magnitude (V) 3.8[1]
Apparent dimensions (V) 30′
Physical characteristics
Estimated age 12.5 My[2]
Other designations Caldwell 14,[3] Collinder 25, Melotte 14, Raab 10, OCl 353, Chi Per Cluster, χ Persei[1]
See also: Open cluster, List of open clusters

NGC 884 is an open cluster located 7600 light years[2] away in the constellation of Perseus. It is the easternmost of the Double Cluster with NGC 869. NGC 869 and 884 are often designated h and χ Persei, respectively.[4] The cluster is most likely around 12.5[2] million years old. Located in the Perseus OB1 association, both clusters are located physically close to one another, only a few hundred light years apart. The clusters were first recorded by Hipparchus, but have likely been known since antiquity.

The Double Cluster is a favorite of amateur astronomers. These bright clusters are often photographed or observed with small telescopes. Easy to find, the clusters are visible with the unaided eye between the constellations of Perseus and Cassiopeia as a brighter patch in the winter Milky Way. The Double Cluster was also included in the Caldwell catalogue, a catalogue of astronomical objects for amateur observation.[3]

In small telescopes the cluster appears as a beautiful assemblage of bright stars located in a rich star field. Dominated by bright blue stars the cluster also hosts a few orange stars that add to the visual interest. Both clusters together offer a spectacular low magnification view.

External links[edit]

References[edit]

  1. ^ a b c d "NGC 884". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2006-12-22. 
  2. ^ a b c d e Kharchenko; et al. (2005). "Astrophysical Parameters of Galactic Open Clusters". Astronomy and Astrophysics. 438 (3): 1163–1173. Bibcode:2005A&A...438.1163K. arXiv:astro-ph/0501674Freely accessible. doi:10.1051/0004-6361:20042523. 
  3. ^ a b O'Meara, Stephen James (2002). The Caldwell Objects. Cambridge University Press. ISBN 978-0-521-82796-6. 
  4. ^ 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; see 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. 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; see Morton Wagman, Lost Stars, McDonald & Woodward, 2003, ISBN 0939923785, p. 240.