
Champagne Cluster
This image shows that the Champagne Cluster is actually two galaxy clusters in the process of merging to form an even larger cluster. Bubbles of multimillion-degree gas in galaxy clusters detected by Chandra (purple) are spread throughout the cluster of more than a hundred galaxies, seen in optical light data (red, green, and blue). The hot gas outweighs the combined mass in the individual galaxies of the newly forming cluster. Researchers think further studies of the Champagne Cluster can potentially teach them how dark matter in galaxy clusters reacts to a high-speed collision.
Image Credit: X-ray: NASA/CXC/UCDavis/F. Bouhrik et al.; Optical:Legacy Survey/DECaLS/BASS/MzLS; Image Processing: NASA/CXC/SAO/P. Edmonds and L. Frattare
- X
https://www.nasa.gov/image-detail/champagne/
Image CreditX-ray: NASA/CXC/UCDavis/F. Bouhrik et al.; Optical:Legacy Survey/DECaLS/BASS/MzLS; Image Processing: NASA/CXC/SAO/P. Edmonds and L. Frattare
Size4064x4064px



