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A colorful, glowing nebula that reaches beyond the top and bottom of the image. This translucent cloud of gas holds wispy and thin filaments with hard edges in some places, and puffy and opaque in others. Blue, red, and yellow colors mix together, showing light emitted by different types of atoms in the hot gas. Scattered across the colorful nebula are bright and point-like foreground and background stars. The background is black.
Hubble · Caldwell 34 · ESA/Hubble & NASA, R. Sankrit

Veil Nebula

Supernova remnant in Cygnus · 2,400 light-years

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TypeSupernova remnant
ConstellationCygnus
Right ascension20h 45m 58s
Declination+30° 36′
Object distance2,400 light-years
Apparent size210′ (arc-minutes)
Approx. true diameter146.6 light-years across
Also known asC34 · NGC 6960 · Filamentary Nebula · Western Veil
Caldwell 34, popularly known as the Veil Nebula, is a supernova remnant (NGC 6960) in Cygnus — the glowing wreckage of an exploded star. It appears as number 34 in the Caldwell catalogue, Sir Patrick Moore's 1995 list of 109 bright deep-sky objects for amateur astronomers. It spans roughly 210 arc-minutes on the sky. It is one of the showpiece objects Sir Patrick Moore chose for his Caldwell list of bright targets the Messier catalogue left out.

Although it appears about 210′ wide on the sky, its real span is roughly 146.6 light-years — the difference is a measure of how far away it lies.

Observing Veil Nebula

Veil Nebula lies in the constellation Cygnus and is best placed in the evening sky around August. Its maximum altitude above the horizon depends on your latitude. It is best placed for observers in the northern hemisphere, and sits low for those far south.

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Sources

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