Celestial hemisphere:  Northern  ·  Constellation: Camelopardalis (Cam)  ·  Contains:  HD24992  ·  HD25090  ·  HD25443  ·  HD25498  ·  HD25638  ·  NGC 1502
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NGC 1502 - Jolly Roger Cluster, Monty Chandler
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NGC 1502 - Jolly Roger Cluster, Monty Chandler
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Description

NGC 1502, The Jolly Roger Cluster,  is a young open cluster of approximately 60 stars in the constellation Camelopardalis. It has a visual magnitude of 6.0 and thus is dimly visible to the naked eye in dark skies. This cluster is located at a distance of approximately 3,500 light years from the Sun, at the outer edge of the Cam OB1 association of co-moving stars, and is likely part of the Orion Arm.  

The Trumpler class of NGC 1502 is II3p, indicating a poorly populated cluster of stars with a wide brightness range. The main sequence turnoff point is not well-defined, so the age estimates range from five to fifteen million years. It is heavily reddened due to interstellar dust.

The reason I chose to image the cluster in a fairly wide field of view (120/840mm) was to collect the core cluster amongst the backdrop of a less cluttered starfield.  I found this better defines the cluster so it doesn't get lost among the stars.  There is a visual double star and eleven variable stars with four candidate variables among the 60 cluster members.  A small family of 60 young stars is easier to relate to burning brightly in our night sky for the entire existance of humans, and millions of years before.

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NGC 1502 - Jolly Roger Cluster, Monty Chandler