M 103 Open Cluster

(NGC 581)

Open Full Size Picture 2479 x 1739 (Alt F4 to close)

Photo Details:

• Instrument: Takahashi FS-102 on Vixen GP-DX..
• Filters: None.
• Exposure:  2 x 60 ISO800 - 4 x 120 ISO400 - 2 x 180 ISO400 - 1 x 300 ISO200 NR on.
• Camera: Canon 20D.
• Software: RegiStax, Photoshop CS2.
• Location: 10 22 29.33 E -  59 11 47.83 N.
• Date: 11.01.2006.
• Local Time: 23.23
• Comments: No darks or flats used.
• Guiding: Unguided
• Explanation: Almost full moon. Processing of starclusters are difficult.
• A brief explanation written by a professional astronomer. Bright blue stars highlight the open cluster known as M103. The gas clouds from which these stars condensed has long dispersed. Of the stars that were formed, the brightest, bluest, and most massive have already used up their nuclear fuel and self-destructed in supernova explosions. A 20 million-year age for M103 was estimated by finding the brightest main-sequence stars that still survive and theoretically computing their lifetimes. In fact, a formerly blue star has recently evolved off the main sequence and is visible above as the red giant star near the cluster center. In general, yellow stars like our Sun are usually less bright and hence less prominent in open clusters than their massive blue cousins. Light takes about 14 years to cross M103. Although visible with binoculars toward the constellation of Cassiopeia, M103's great distance of 8000 light years makes it appear four times smaller than a full moon.

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