Searching for Dark Matter in a Galaxy Cluster

Searching for Dark Matter in a Galaxy Cluster

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News release ID: STScI-2007-17
Release Date: May 15, 2007
Image Use: Copyright
About this image

This rich galaxy cluster, catalogued as Cl 0024+17, is allowing astronomers to probe the distribution of dark matter in space. The blue streaks near the center of the image are the smeared images of very distant galaxies that are not part of the cluster. The distant galaxies appear distorted because their light is being bent and magnified by the powerful gravity of Cl 0024+17, an effect called gravitational lensing.

Dark matter cannot be seen because it does not shine or reflect light. Astronomers can only detect its influence by how its gravity affects light. By mapping the distorted light created by gravitational lensing, astronomers can trace how dark matter is distributed in the cluster. While mapping the dark matter, astronomers found a dark-matter ring near the cluster's center. The ring's discovery is among the strongest evidence that dark matter exists.

The Hubble observations were taken in November 2004 by the Advanced Camera for Surveys.

Dark Matter, Galaxies, Galaxy Clusters, Observations


NASA, ESA, M.J. Jee and H. Ford (Johns Hopkins University)