The Crescent Nebula is a cosmic cloud glowing as it’s blasted by radiation from a rare type of star
Pictures of the Crescent Nebula, NGC 6888, and facts about this beautiful deep-sky emission nebula powered by an ageing Wolf-Rayet star.
By
Published: Monday, 12 August 2024 at 12:18 PM
The Crescent Nebula, or NGC 6888 as it is formally known, is a distinctive emission nebula that stretches about 25 lightyears across and is located about 5,000 lightyears away from Earth in the Cygnus constellation.
Discovered by William Herschel in 1792, the Crescent Nebula is produced by a type of star known as a Wolf-Rayet.
These are are massive stellar objects that are ageing and losing mass at an incredibly high rate.
That’s certainly the case with this Wolf Rayet: the star is shedding its outer layers into space at a rate equivalent to the mass of the Sun about every 10,000 years.
This violent and rapid ejection has produced a dense shell of scorching hot material that gives the nebula its shape, while the complex structures seen within the bubble are likely the result of stellar winds colliding and interacting with older material ejected by the star long ago.
It is thought that the star at the centre of the Crescent Nebula – known as WR 136 – will eventually end its life in a dramatic stellar explosion known as a supernova.