M 27
 

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Description: Known as the "Dumbbell Nebula," M27 is formed from gases expelled by an aging, giant star. These gases are ionized by radiation from this star and re-emit light in the visible wavelengths.
 
Constellation: Vulpecula
 
Distance: 1 thousand light years
 
Apparent Size: 5.8'
 
Date: 28 july 2005
 
Equipment: 12"RC @ f/9, ST10XME, AP1200
 
Exposure: 2 hours Ha (6nm Astrodon)