Crescent Nebula

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Crescent Nebula
Emission nebula
File:NGC 6888.png
The Crescent Nebula, captured with a color camera, narrowband filter, and high-speed amateur telescope
Observation data: J2000.0 epoch
Right ascension20h 12m 7s[1]
Declination+38° 21.3′[1]
Distance5,000 ly
Apparent magnitude (V)+7.4
Apparent dimensions (V)18′ × 12′
ConstellationCygnus
DesignationsNGC 6888,[1] Sharpless 105, Caldwell 27
See also: Lists of nebulae

The Crescent Nebula (also known as NGC 6888, Caldwell 27, Sharpless 105) is an emission nebula in the constellation Cygnus, about 5000 light-years away from Earth. It was discovered by William Herschel in 1792.[2] It is formed by the fast stellar wind from the Wolf-Rayet star WR 136 (HD 192163) colliding with and energizing the slower moving wind ejected by the star when it became a red giant around 250,000 years ago[3]. The result of the collision is a shell and two shock waves, one moving outward and one moving inward. The inward moving shock wave heats the stellar wind to X-ray-emitting temperatures.

Visibility

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The Crescent Nebula is a rather small object located about 2 degrees Southwest of Sadr. While considered bright by astronomical imaging standards, visually it is relatively faint. For most telescopes it requires a UHC or OIII filter to see. Under favorable circumstances a telescope as small as 8 cm (with filter) can see its nebulosity. With higher magnification, it has been reported to have a resemblance to a Euro sign shape leading to a nickname the "Euro Sign Nebula."[4]

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See also

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References

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  • Crescent Nebula on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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