k Veil nebula supernova remnant NGC 6960 Veil nebula supernova remnant NGC 6960, optical image. This wisp of glowing gas is part of a much larger spherical shell called the Cygnus Loop. The shell comprises stellar material ejected in a supernova, the explosive death of a massive star. The supernova forming this shell is thought to have occurred between 58000 years ago. The gas was cast off into space at high speeds, and when it impacted the interstellar medium it compressed and heated it, forming a glowing plasma. The bright star at upper right is 52 Cygni, which is unrelated to the supernova. The distance to the nebula is a matter of debate, with estimates ranging from 1400 to 2600 light years. It lies in the constellation Cygnus. Stock Photo - Afloimages
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Veil nebula supernova remnant  NGC 6960  Veil nebula supernova remnant  NGC 6960 , optical image. This wisp of glowing gas is part of a much larger spherical shell called the Cygnus Loop. The shell comprises stellar material ejected in a supernova, the explosive death of a massive star. The supernova forming this shell is thought to have occurred between 5 8000 years ago. The gas was cast off into space at high speeds, and when it impacted the interstellar medium it compressed and heated it, forming a glowing plasma. The bright star at upper right is 52 Cygni, which is unrelated to the supernova. The distance to the nebula is a matter of debate, with estimates ranging from 1400 to 2600 light years. It lies in the constellation Cygnus.
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Veil nebula supernova remnant (NGC 6960)

Veil nebula supernova remnant (NGC 6960), optical image. This wisp of glowing gas is part of a much larger spherical shell called the Cygnus Loop. The shell comprises stellar material ejected in a supernova, the explosive death of a massive star. The supernova forming this shell is thought to have occurred between 5-8000 years ago. The gas was cast off into space at high speeds, and when it impacted the interstellar medium it compressed and heated it, forming a glowing plasma. The bright star at upper right is 52 Cygni, which is unrelated to the supernova. The distance to the nebula is a matter of debate, with estimates ranging from 1400 to 2600 light years. It lies in the constellation Cygnus.

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