The Crecent Nebula - NGC6888 HaOIII (Thomas Richter)

Celestial hemisphere: Northern · Constellation: Cygnus (Cyg) · Contains: Crescent Nebula · NGC 6888

The Crecent Nebula - NGC6888 HaOIII, Thomas Richter

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The Crecent Nebula - NGC6888 HaOIII

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The Crecent Nebula - NGC6888 HaOIII

A short Crecent Nebula in only one night during moonlight.

Object description (wikipedia.org):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.
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 to 400,000 years ago. 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.It is a rather faint object located about 2 degrees SW of Sadr.
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.
Larger telescopes (20 cm or more) reveal the crescent or a Euro sign shape which makes some to call it the "Euro sign nebula".

Astrofreunde-Franken
Narrowband imaging
Nuremberg Public Observatory

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The Crecent Nebula - NGC6888 HaOIII

The Crecent Nebula - NGC6888 HaOIII

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