Celestial hemisphere:  Northern  ·  Constellation: Cygnus (Cyg)  ·  Contains:  52 Cyg  ·  Filamentary nebula  ·  Lace-work nebula  ·  NGC 6960  ·  The star 52Cyg  ·  Veil nebula
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The Western Veil Nebula, Gabe Shaughnessy
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The Western Veil Nebula

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The Western Veil Nebula, Gabe Shaughnessy
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The Western Veil Nebula

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Description

The Veil nebula is a supernova remnant in the constellation Cygnus about 1500 ly away. The progenitor supernova exploded an estimated 5000-8000 years ago and the full diameter is 3 degrees, giving a size of around 50 ly. The remnant emits radio, infrared, visible light and is also a very bright source of X-rays.

This composite shows the Hydrogen alpha (Ha) and doubly ionized oxygen (OIII) emission of the western portion of the Veil nebula, also known as the Witch's Broom and is close to the bright foreground star 52 Cygni. The emission filaments are thought to be the edge-on view of the thin shell of expanding gas. The entire 3 degree field contains this gas, but it's only in this edge-on view that the shell is visible.

The supernova must've been quite a site to our ancestors. For reference, it's about 4.3x closer than the supernova that left the Crab nebula remnant, M1, in 1054 AD, which had an apparent magnitude of -6.5 at it's peak. For supernovae with the same intrinsic brightness, this would give a 18x increase in brightness, or around 3.2 magnitudes.

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  • The Western Veil Nebula, Gabe Shaughnessy
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    The Western Veil Nebula, Gabe Shaughnessy
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The Western Veil Nebula, Gabe Shaughnessy

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Nebulae