![]() The location of NGC 1502 (circled) | |
Observation data (J2000 epoch) | |
---|---|
Right ascension | 04h 07m 48.96s[1] |
Declination | +62° 19′ 55.2″[1] |
Distance | 3,452 ly (1,058.4 pc)[1] 3,643+313 −290 ly (1,117+96 −89 pc)[2] |
Apparent magnitude (V) | 6.0[3] |
Apparent dimensions (V) | 9.7′[1] |
Physical characteristics | |
Radius | 5.5 ly (1.7 pc)[4] |
Estimated age | 5 Myr[2] |
Other designations | NGC 1502,[5] Cr 45 |
Associations | |
Constellation | Camelopardalis |
NGC 1502 (also known as the Golden Harp Cluster[6]) is a young[7] open cluster of approximately 60[3] stars in the constellation Camelopardalis, discovered by William Herschel on November 3, 1787.[8] It has a visual magnitude of 6.0 and thus is dimly visible to the naked eye.[3] This cluster is located at a distance of approximately 3,500 light years[1][2] from the Sun, at the outer edge of the Cam OB1 association of co-moving stars, and is likely part of the Orion Arm.[2] The asterism known as Kemble's Cascade appears to "flow" into NGC 1502, but this is just a chance alignment of stars.[9]
The Trumpler class of NGC 1502 is II3p, indicating poorly populated cluster of stars (p) with a wide brightness range (3). The main sequence turnoff point is not well-defined, so the age estimates range from five to fifteen million years.[7] It is heavily reddened due to interstellar dust.[4] One of the brightest candidate members of the cluster is the eclipsing binary SZ Cam, which is a component of a visual double star ADS 2984.[2] There are eleven variable stars and four candidate variables among the cluster members, including a β Cep, two periodic B-type variables, 2–3 eclipsing variables, and an RR Lyrae star.[7] Five members of the cluster are chemically peculiar.[10]
Cantat-Gaudin_Anders_2020
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Topasna_et_al_2018
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O'Meara2007
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Tripathi_et_al_2013
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Simbad
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Michalska_et_al_2009
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Seligman
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Thompson2007
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Paunzen_et_al_2005
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