The Corona Australis Molecular Cloud and the Chandelier Cluster View and zoom

View and zoom The Corona Australis Molecular Cloud and the Chandelier Cluster

Zoom 100%

· Picture of the day

The Corona Australis Molecular Cloud and the Chandelier Cluster

Download image

Downloads retain the usage rights shown in the creator credit.

The Southern Crown (Corona Australis) dazzles with young and ancient celestial jewels. The Corona Australis Cloud is a collage of reflection and emission nebulae on the left of today’s image. At 430 light years away, this cloud is one of the closest star-forming regions to Earth. It contains gas cool enough (-260 Celsius or -440 Fahrenheit) to collapse into protostars. Recently formed stars paint blue hues across the cloud as their light reflects off surrounding material. The waltz of the R Coronae Australis binary system stirs up the nebula NGC 6729. The younger of the pair ionizes nearby gas with its ultraviolet light, causing it to glow. The Chandelier Cluster (NGC 6723) dangles from the top right, but is actually tens of thousands of light years farther away than its apparent star-forming neighbor. While NGC 6723 experienced multiple periods of star formation creating slightly younger stars, the chandelier twinkles with stars almost as old as the universe.

Image credit: DES/DOE/FNAL/DECam/CTIO/NOIRLab/NSF/AURA Image Processing: T.A. Rector (UAA/NOIRLab), R. Colombari & M. Zamani (NOIRLab) Text: Keighley Rockcliffe (NASA GSFC, UMBC CSST, CRESST II)