NGC 1220
Open cluster in Perseus
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NGC 1220 is a young compact open cluster in the constellation Perseus. It was discovered by John Herschel in 1831.[5]
Rightascension03h 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]
| NGC 1220 | |
|---|---|
NGC 1220 from the Digitized Sky Survey (DSS) | |
| Observation data (J2000.0 epoch) | |
| Right ascension | 03h 11m 40s[1][Note 1] |
| Declination | 53° 20′ 45″[2][Note 2] |
| Distance | 5,900 light-years (1,800 pc)[2] |
| Apparent magnitude (V) | 11.8[3] |
| Apparent dimensions (V) | 2.6′[1] |
| Physical characteristics | |
| Radius | 3.4 light-years (1.05 pc)[2] |
| Estimated age | 60 million years[2] |
| Other designations | Cr 37, OCL 380[2][4] |
| Associations | |
| Constellation | Perseus |
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]