NGC 1220

Open cluster in Perseus From Wikipedia, the free encyclopedia

NGC 1220 is a young compact open cluster in the constellation Perseus. It was discovered by John Herschel in 1831.[5]

Quick facts Observation data (J2000.0 epoch), Right ascension ...
NGC 1220
NGC 1220 from the Digitized Sky Survey (DSS)
Observation data (J2000.0 epoch)
Right ascension03h 11m 40s[1][Note 1]
Declination53° 20 45[2][Note 2]
Distance5,900 light-years (1,800 pc)[2]
Apparent magnitude (V)11.8[3]
Apparent dimensions (V)2.6[1]
Physical characteristics
Radius3.4 light-years (1.05 pc)[2]
Estimated age60 million years[2]
Other designationsCr 37, OCL 380[2][4]
Associations
ConstellationPerseus
See also: Open cluster, List of open clusters
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The cluster is located at l = 143.04°, b = −3.96° in the galactic coordinate system, and is 120 parsecs above the galactic plane.[1][2] It is approximately 6m 42s east and 10′ 12″ south from the nearest visible star, γ Persei.[3]

NGC 1220 consists of approximately 26 stars with spectral types between A0 and B9, although the majority fall between A5 and B5.[2]

Notes

  1. Exact values for seconds vary from 40.0s (Ortolani et al. (2002)) to 40.8s (SIMBAD).
  2. Estimates for arcseconds vary from 38″ (SIMBAD) to 53.4″ (NED).

References

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