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NGC 1220

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Open cluster in Perseus
NGC 1220
NGC 1220 from the Digitized Sky Survey (DSS)
Observation data (J2000.0 epoch)
Right ascension03 11 40
Declination53° 20′ 45″
Distance5,900 light-years (1,800 pc)
Apparent magnitude (V)11.8
Apparent dimensions (V)2.6
Physical characteristics
Radius3.4 light-years (1.05 pc)
Estimated age60 million years
Other designationsCr 37, OCL 380
Associations
ConstellationPerseus
See also: Open cluster, List of open clusters

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

The cluster is located at l = 143.04°, b = −3.96° in the galactic coordinate system, and is 120 parsecs above the galactic plane. It is approximately 6 42 east and 10′ 12″ south from the nearest visible star, γ Persei.

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

Notes

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

References

  1. ^ "NGC 1220". Strasbourg Astronomical Data Center. Retrieved 2024-04-02.
  2. ^ Ortolani, S.; Carraro, G.; Covino, S.; Bica, E.; Barbuy, B. (2002-04-09). "A photometric study of the young open cluster NGC 1220". Galactic structure, stellar clusters, and populations. Astronomy & Astrophysics. 391 (1). EDP Sciences (published 2002-07-29): 179–185. doi:10.1051/0004-6361:20020794. hdl:10183/98516.{{cite journal}}: CS1 maint: date and year (link)
  3. ^ "NGC 1220 – Open Cluster in Perseus". The Sky Live. Retrieved 2024-03-30.
  4. Collinder, Per. "On Structural Properties of Open Galactic Clusters and their Spatial Distribution. Catalog of Open Galactic Clusters". Annals of the Observatory of Lund. 2: 4.
  5. "NGC1220". NGC/IC Restoration Project. Retrieved 2024-03-30.
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