The Dark Energy Camera (DECam) has captured a high-resolution image of the Corona Australis molecular cloud, revealing a star-forming region that mirrors the swirling aesthetic of Vincent van Gogh’s The Starry Night. Located 430 light-years from Earth, this stellar nursery features dense gas and dust clouds, providing a detailed look at the raw materials of star formation.
The Anatomy of the Corona Australis Molecular Cloud
This molecular cloud spans approximately 16 light-years in diameter, positioning it as one of the closest star-birthing regions to our solar system. The DECam, mounted on the Víctor M. Blanco 4-meter Telescope at the Cerro Tololo Inter-American Observatory (CTIO) in Chile, captured dark lanes of gas and dust that serve as the primary fuel for new stars.
A central feature in the imagery is the reflection nebula NGC 6729. This region glows because interstellar dust reflects light from newborn stars embedded within the cloud. The system is home to R Coronae Australis, a binary star system consisting of a pre-main-sequence star and a red dwarf. These stars complete an orbit every 43 to 47 years. Their intense light not only illuminates the surrounding dust but also ionizes nearby gas to create emission nebulae, adding vibrant color to the region.
Did you know?
The Corona Australis Molecular Cloud is one of the closest regions to Earth where active star formation is currently taking place.
The Chandelier Cluster and Galactic History
Positioned at the top-right of the DECam field of view is the globular cluster NGC 6723, frequently referred to as the “Chandelier Cluster.” While the molecular cloud is a nearby neighbor, this cluster sits roughly 29,000 light-years away. It acts as a backdrop to the more active, local star-forming processes.

The Chandelier Cluster contains a vast population of stars, ranging from tens of thousands to millions. While globular clusters are typically associated with the oldest stars in the Milky Way, the Chandelier Cluster is notable for housing a diverse range of stellar ages, including younger stars.
Future Trends in Deep-Space Imaging
Frequently Asked Questions
How far is the Corona Australis Molecular Cloud from Earth?
What is a reflection nebula?
A reflection nebula, such as NGC 6729, is a cloud of interstellar dust that does not emit its own visible light but shines by reflecting the light of nearby stars.
Why is the Chandelier Cluster significant?
NGC 6723, or the Chandelier Cluster, is a globular cluster containing some of the oldest stars in the Milky Way, located about 29,000 light-years from Earth.
Interested in the latest discoveries from deep space? Subscribe to our newsletter for weekly updates on cosmic events and observatory highlights.
Worth a look