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Pandora's cluster: a galactic crash investigation

Last Updated on Wednesday, 22 June 2011 13:40
Published on Wednesday, 22 June 2011 13:31

An international team of scientists have discovered what appears to be the simultaneous crashing together of at least four separate galaxy clusters. The researchers used telescopes on the ground and in space, including the Hubble Space Telescope and ESO's Very Large Telescope, to study the galaxy cluster Abell 2744, an object now nicknamed Pandora's Cluster and found evidence for the colossal collision. They publish their results in the journal Monthly Notices of the Royal Astronomical Society.

This image combines visible light exposures of galaxy cluster Abell 2744 taken by the NASA/ESA Hubble Space Telescope and the European Southern Observatory’s Very Large Telescope, with X-ray data from NASA’s Chandra X-ray Observatory (which largely detects hot gas shown here in pink) and a mathematical reconstruction of the location of dark matter (depicted in blue). Credit: NASA, ESA, ESO, CXC and D. Coe (STScI) / J. Merten (Heidelberg / Bologna)
When huge clusters of galaxies like Abell 2744 crash together, the resulting mess is a treasure trove of information for astronomers. By investigating what is one of the most complex and unusual colliding clusters in the sky, the team of astronomers has pieced together the history of a cosmic crash that took place over a period of 350 million years.

Julian Merten, one of the lead scientists for the new study, explains: "Like a crash investigator piecing together the cause of an accident, we can use observations of these cosmic pile-ups to reconstruct events that happened over a period of hundreds of millions of years. This can reveal how structures form in the Universe, and how different types of matter interact with each other when they are smashed together."

"We nicknamed it Pandora's Cluster because so many different and strange phenomena were unleashed by the collision. Some of these phenomena had never been seen before," adds Renato Dupke, another member of the team.

Abell 2744 has now been studied in more detail than ever before by combining data from the NASA/ESA Hubble Space Telescope, ESO's Very Large Telescope (VLT), the Japanese Subaru telescope and NASA's Chandra X-Ray Observatory.

The galaxies in the cluster are clearly visible in the Hubble and VLT images. Although the galaxies are bright they make up less than 5% of the mass there. The rest is gas (around 20%), which is so hot that it shines only in X-rays, and dark matter (around 75%), which is completely invisible. To understand what was going on in the collision the team needed to map the positions of all three types of matter in Abell 2744.

Dark matter is particularly elusive as it does not emit, absorb or reflect light (hence its name), but only makes itself apparent through its gravitational attraction. To pinpoint the location of this mysterious substance the team exploited a phenomenon known as gravitational lensing. This is the bending of light rays from distant galaxies as they pass through the gravitational field present in the cluster. The result is a series of telltale distortions in the images of galaxies in the background of the Hubble and VLT observations. By carefully plotting the way that these images are distorted, it is possible to map quite accurately where the mass — and hence the dark matter — actually lies.

By comparison, finding the hot gas in the cluster is simpler as NASA's Chandra X-ray Observatory can observe it directly. These observations are not just crucial to find out where the gas is, but also to show the angles and speeds at which different components of the cluster came together.

When the astronomers looked at the results they found many curious features. "Abell 2744 seems to have formed from four different clusters involved in a series of collisions over a period of some 350 million years. The complicated and uneven distribution of the different types of matter is extremely unusual and fascinating," says Dan Coe, the other lead author of the study.

It seems that the complex collision has separated out some of the hot gas and dark matter so that they now lie apart from each other, and from the visible galaxies. Pandora's Cluster combines several phenomena that have only ever been seen singly in other systems.

Near the core of the cluster is a "bullet", where the gas of one cluster collided with that of another to create a shock wave. The dark matter passed through the collision unaffected.

In another part of the cluster there seem to be galaxies and dark matter, but no hot gas. The gas may have been stripped away during the collision, leaving behind no more than a faint trail.

Even odder features lie in the outer parts of the cluster. One region contains lots of dark matter, but no luminous galaxies or hot gas. A separate ghostly clump of gas has been ejected, which precedes rather than follows the associated dark matter. This puzzling arrangement may be telling astronomers something about how dark matter behaves and how the various ingredients of the Universe interact with each other.

Galaxy clusters are the biggest structures in the cosmos, containing literally trillions of stars. The way they form and develop through repeated collisions has profound implications for our understanding of the Universe. Further studies of Pandora's Cluster, the most complex and fascinating merger yet found, are now underway.



Julian Merten
Institute for Theoretical Astrophysics
Heidelberg, Germany
Tel: +49 6221 54 8987
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Daniel Coe
Space Telescope Science Institute
Baltimore, USA
Tel: +1 410 338 4312
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Oli Usher
Garching, Germany
Tel: +49 89 3200 6855
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The Hubble Space Telescope is a project of international cooperation between ESA and NASA.

This study appears in the paper “Creation of cosmic structure in the complex galaxy cluster merger Abell 2744”, Merten J. et al, Monthly Notices of the Royal Astronomical Society, in press. A preprint of the paper can be downloaded from international team of astronomers consists of J. Merten (Institute for Theoretical Astrophysics, Heidelberg, Germany; INAF-Osservatorio Astronomico di Bologna, Italy), D. Coe (Space Telescope Science Institute, Baltimore, USA), R. Dupke (University of Michigan, USA; Eureka Scientific, USA; National Observatory, Rio de Janeiro, Brazil), R. Massey (University of Edinburgh, Scotland), A. Zitrin (Tel Aviv University, Israel), E.S. Cypriano (University of Sao Paulo, Brazil), N. Okabe (Academia Sinica Institute of Astronomy and Astrophysics, Taiwan), B. Frye (University of San Francisco, USA), F. Braglia (University of British Columbia, Canada), Y. Jimenez-Teja (Instituto de Astrofisica de Andalucia, Granada, Spain), N. Benitez (Instituto de Astrofisica de Andalucia), T. Broadhurst (University of Basque Country, Spain), J. Rhodes (JPL/Caltech, USA), M. Meneghetti (INAF-Osservatorio Astronomico di Bologna, Italy), L. A. Moustakas (Caltech), L. Sodre Jr.(University of Sao Paulo, Brazil), J. Krick (Spitzer Science Center/IPAC/Caltech, USA) and J. N. Bregman (University of Michigan).



The ESO / Hubble press release and associated images can be seen at