M27 Dumbbell Nebula in Vulpecula
M27 is a bright, 7.5 magnitude planetary nebula 1360 light years from the Sun and easily detectable with binoculars and small telescopes. It is the type of planetary nebula that our Sun is predicted to produce in about 6 billion years when nuclear fusion ceases and the central mass contracts into an X-ray-emitting central white dwarf. In M27, lighter outer gas layers rich in hydrogen (red) and oxygen (blue) are being expelled outward at 31 km/s forming most of the hot, photon-emitting gas that is detected in this astrophotograph taken with red, green, blue and narrow band OIII filters. It is estimated to have started to form less than 14,600 years ago, and is 2 by 3 light years in size.
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