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Pelican Nebula
The long beak of the Pelican Nebula looks more like the head of a prehistoric Pterydactyl than the head of a bird.  The eye is ghostly dark, but the nearby bright star hints of a displaced eyeball.  The Pelican Nebula is part of a huge cloud of hydrogen gas, termed an H-II region by astronomers, illuminated by a nearby star.  Like other H-II regions, the hydrogen gas is excited by the stellar energy, and then emits its own light at the characteristic red wavelength of hydrogen. 

Located at a distance of 1500  light-years in the direction of the constellation Cygnus the Swan,  the Pelican Nebula is separated from the adjacent larger North American Nebula by a broad band of light-absorbing dark clouds. 

This image combined 84 Luminance images with a red filter, with 20 red, 20 green, and 28 blue one-minute images, for a total imaging time of 2 hours 32 minutes.  An ST10XME camera was used through a 4 inch refractor. 
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