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NGC 869 and NGC 884, The Double Cluster
NGC 869 and NGC 884
Exposure Data
  • Image Field of View: 53.81' x 35.87'
  • Camera Field of View: 74.76' x 49.83'
  • Scope: 130 mm f/8 triplet apochromatic refractor
  • Focal Length: 1,025 mm
  • Focal Ratio: f/8
  • Camera: Modified Canon T2i (550D)
  • ISO: 400
  • Exposure: 80 minutes total
    • 4 x 600 seconds
    • 8 x 300 seconds
  • Filter: None
  • SQM: 20.80

NGC 869 (left) and NGC 884 (right) are two open clusters that make up the Double Cluster in the constellation of Perseus.

At a distance of 7,000 light-years, the clusters are separated by only a couple of hundred light-years in space.

The clusters are relatively young at 5.6 and 3.2 million years old respectively.

Both clusters are 30 arcminutes in diameter and shine at magnitude 4.3 and 4.4.

They were cataloged by Hipparcos in 130 B.C. but were almost certainly known long before that since they can be seen by the unaided eye from a dark sky location.

South is up in the above image.

NGC 869, NGC 884
  • Catalogs:
    • NGC 869, h Persei, Cl 24, Mel 13
    • NGC 884, Chi Persei, Cl 25, Mel 14
  • Common Name: Double Cluster
  • Object Type: Open Clusters
  • Magnitude:
    • NGC 869: 5.3v
    • NGC 884: 6.1v
  • Size: 18' each
  • Constellation: Perseus
  • Image Field Centered At:
    • RA: 02h 20m 45s
    • Dec: +57° 11' 26"




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