IC 361 | |
---|---|
Observation data (J2000 epoch) | |
Right ascension | 04h 18m 56.6s[1] |
Declination | +58° 15′ 07″[1] |
Distance | 10,500 ± 230 ly (3.22 ± 0.07 kpc)[2] |
Apparent magnitude (V) | 11.7[3] |
Apparent dimensions (V) | 6.0′[3] |
Physical characteristics | |
Mass | 2,459±491[4] M☉ |
Radius | 24.5 ly[2] |
Estimated age | 759 Myr[1] |
Other designations | C 0414+581[5] |
Associations | |
Constellation | Camelopardalis |
IC 361 is an open cluster of stars in the constellation Camelopardalis. It was discovered by the British amateur astronomer William F. Denning on February 11, 1893.[6] This cluster is located at a distance of 10,500 ± 230 light-years from the Sun.[2] It is very faint with an apparent visual magnitude of 11.7,[3] requiring a telescope to view. Because of its faintness, this cluster has been poorly studied.[7] The cluster spans an angular size of 6.0′.[3]
This intermediate–age cluster is located in or beyond the Perseus Arm of the Milky Way galaxy.[7] It is situated near dark nebulae, resulting in significant levels of extinction due to interstellar dust. The cluster has a core radius of 2.0′±0.4′ and a cluster radius of 8.0′±0.5′. At an estimated distance of 3.22 kpc this corresponds to a physical core radius of 6.1 ly and a cluster radius of 24.5 ly.[2] It has an estimated age of 759 million years.[1] The cluster is mildly metal deficient, matching the metallicity gradient of the Milky Way.[7]
Two candidate blue stragglers have been identified in this cluster.[8]
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