The Dumbbell Nebula (M27)

Posted by Brock
on Wednesday, September 26, 2012
The Dumbbell Nebula (also known as Messier 27, M 27, or NGC 6853) is a planetary nebula (PN) in the constellation Vulpecula, at a distance of about 1,360 light years. This object was the first planetary nebula to be discovered; by Charles Messier in 1764. At its brightness of visual magnitude 7.5 and its diameter of about 8 arc minutes, it is easily visible in binoculars, and a popular observing target in amateur telescopes. It is a shell of gas that was expelled from the nebula's central star. This object gets the name "dumbbell" from its hourglass, or dumbbell-like shape. A 13th magnitude star at the center of the nebula illuminates it from within. M27 is the brightest and most impressive object of its kind, and with a magnitude of 7.5 can be easily seen using any optical instrument.
Telescope Celestron C11  Camera Canon 60Da with 6.3 focal reducer
ISO 3200    Exposures 25 x's  60 seconds
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