Boomerang Nebula

Boomerang Nebula

The Boomerang Nebula is a bipolar reflection nebula that lies about 5,000 light-years away in the constellation Centaurus. The symmetric cloud appears to have been created by a high-speed wind of gas and dust blowing from an aging asymptotic giant branch (AGB) star at a speed of 164 km/s. This rapid expansion has cooled carbon monoxide molecules in the nebular gas to a mere 1 K – colder even than the cosmic background radiation – making it the coldest region in the cosmos (outside a lab) ever observed. The ultracool Boomerang shines with light from the central star reflected by dust and is believed to be evolving rapidly, on a timescale of about 1,000 years, to the planetary nebula stage.


visual magnitude -
angular size 54"
linear size ~1.3 light-years (0.4 pc)
distance ~5,000 light-years (1,500 pc)
position R.A. 12h 44m 46.1s,
Dec. -54° 31' 12"
other designations ESO 172-7