Celestial hemisphere:  Northern  ·  Constellation: Cygnus (Cyg)  ·  Contains:  Crescent Nebula  ·  HD192003  ·  HD192020  ·  HD192163  ·  HD192182  ·  HD192303  ·  HD192361  ·  HD228185  ·  HD228243  ·  HD228289  ·  HD228304  ·  HD228324  ·  HD228376  ·  LBN 203  ·  NGC 6888  ·  Sh2-105
NGC 6888 Crescent Nebula - HOO, Jerry Macon
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NGC 6888 Crescent Nebula - HOO

NGC 6888 Crescent Nebula - HOO, Jerry Macon
Powered byPixInsight

NGC 6888 Crescent Nebula - HOO

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Description

CDK20: FL 2280mm,  F/4.5,  0.34 arcsec/pixel raw
Imaged: 5/31/2022, 6/1/2022, 6/2/2022

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"
(Wikipedia)

My Collections:
Abell Planetary Nebulae (Complete)
Galaxies
Messier Objects
Planetary Nebulae
Sharpless 2 Objects

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NGC 6888 Crescent Nebula - HOO, Jerry Macon