Tucker said the lack of a shock wave, and the fact that the images reveal less heat than expected, might indicate the merger is near completion and things have settled down. Or, he said, perhaps the dynamics of cosmic mergers are different than anticipated.
Either way, the observations represent an important step towards learning more.
"Now we can begin to understand the physics of these mergers, which are among the most energetic events in the universe," said Maxim Markevitch of the Harvard-Smithsonian Center for Astrophysics and leader of the international team that analyzed the observations. "The pressure and density maps of the cluster show a sharp boundary that can only exist in the moving environment of a merger."
Clusters and superclusters
The two merging clusters together make up a larger galaxy cluster known as Abell 2142. The entire supercluster is 6 million light-years across.
Galaxy clusters grow to such vast sizes by using their gravity to pull in other small galaxies over billions of years. The enormous systems are filled with clouds of hot gas whose mass matches that of all the stars in all the galaxies of the cluster.
Our own Milky Way is part of a group of a dozen or more galaxies, all somewhat isolated but surrounded by the Virgo supercluster. Whether the group might one day join the larger cluster is unclear.
"We're heading towards the center [of the supercluster]," Tucker said. "Maybe in many billions of years we may become part of it."
The new images were made in August, 1999, and released this week. The results will be reported in an upcoming issue of the Astrophysical Journal.