M27- The Dumbbell Nebula

M27 - The Dumbbell Nebula

The Dumbbell Nebula in Vulpecula.  The largest of the class of planetary nebulae, M27's distance is estimated to be about 900 light years.  The central star is magnitude 13.5 and as with all planetary nebulae it is a hot bluish dwarf.  The nebula is formed by the ejection of material from the hot central star.  More information about this fascinating object can be found at the Messier Index - M27.  

The above image is an LRGB color composite consisting of Luminance, Red, Green and Blue-filtered exposures of 22, 38, 32, and 42 minutes, respectively.   The image was taken using a 4.3" William Optics FLT110 refractor on a Losmandy G11 mount and an SXV-H9 CCD camera on 2 July 2008.        The below version is the fullsize crop of the nebula region from the above image.

M27 - The Dumbbell Nebula

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