How did the Crescent nebula (NGC 6888) form?

The Crescent Nebula (NGC 6888) is about 5,600 light-years away in Cygnus. Its shape comes from the fast stellar winds of the Wolf-Rayet star at its center, which collide with material the star itself shed earlier in its life. The nebula is a clash between what the star is blowing out today and what it expelled before.

Astrophotographer Aloke Palsikar captured it from Pie Town, New Mexico, using 3 hours of exposure in Hα and OIII filters with a 12-inch f/4.9 astrograph. Those filters explain the orange-red tones (hydrogen) and the blue-green rim (oxygen).

A 2000 NASA APOD, based on Hubble data, put this nebula at about 4,700 light-years away.

The central star, WR 136, will likely explode as a supernova within the next million years.

The Star That Blew Its Own Nebula: How the Crescent Nebula Formed
Crescent nebula: The stellar wind collision that sculpted this cosmic gem.

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