A clump of dark matter has apparently been left behind after a violent collision of galaxy clusters.
This dark matter clump contains far fewer galaxies than would be expected if the dark matter and galaxies hung together.
Astronomers used Chandra, Hubble, and the Canada-France-Hawaii, and Subaru telescopes to observe Abell 520, which is 2.4 billion light years away.
This latest result agrees with a similar conclusion that was announced in 2007.
This composite image shows the distribution of dark matter, galaxies, and hot gas in the core of the merging galaxy cluster Abell 520, formed from a violent collision of massive galaxy clusters that is located about 2.4 billion light years from Earth.
Data from NASA’s Chandra X-ray Observatory show the hot gas in the colliding clusters colored in green. The gas provides evidence that a collision took place. Optical data from NASA’s Hubble Space Telescope and the Canada-France-Hawaii Telescope (CFHT) in Hawaii are shown in red, green, and blue. Starlight from galaxies within the clusters, derived from observations by the CFHT and smoothed to show the location of most of the galaxies, is colored orange.
The blue-colored areas pinpoint the location of most of the mass in the cluster, which is dominated by dark matter. Dark matter is an invisible substance that makes up most of the universe’s mass. The dark-matter map was derived from the Hubble observations, by detecting how light from distant objects is distorted by the cluster galaxies, an effect called gravitational lensing. The blend of blue and green in the center of the image reveals that a clump of dark matter (which can be seen by mousing over the image) resides near most of the hot gas, where very few galaxies are found.
This finding confirms previous observations of a dark-matter core in the cluster announced in 2007. The result could present a challenge to basic theories of dark matter, which predict that galaxies should be anchored to dark matter, even during the shock of a powerful collision.
|Fast Facts for Abell 520:|
|Credit||NASA, ESA, CFHT, CXO, M.J. Jee (University of California, Davis), and A. Mahdavi (San Francisco State University)|
|Scale||8.5 arcmin across (about 5.4 million light years)|
|Category||Groups & Clusters of Galaxies|
|Coordinates (J2000)||RA 04h 54m 03.80s | Dec +02º 53′ 33.00″|
|Observation Date||7 pointings between Oct 10, 2000 and Jan 11, 2008|
|Observation Time||148 hours 38 min. (6 days 4 hours 38 min)|
|Obs. ID||528, 4215, 7703, 9424-9426, 9430|
|Color Code||Optical (Red, Green, Blue); X-ray (Green); Mass (Blue); Luminosity (Orange)|
|References||arXiv:1202.6368; Jee, M. et al, 2012, ApJ 747, 96|
|Distance Estimate||2.4 billion light years (z=0.201)|
|Release Date||March 2, 2012|