European Space Agency
2 December 2015
ESA Science and Robotic Exploration Communication Officer
Tel: +31 71 565 6799
Mob: +31 61 594 3 954
University of Geneva, Switzerland and INAF-IASF, Milano, Italy
University of Durham, UKand University of KwaZulu-Natal, Durban, South Africa
ESA XMM-Newton Project Scientist
ESA Directorate of Science and Robotic Exploration
Tel: +34 91 8131 184
Components of the galaxy cluster Abell 2744, also known as the Pandora Cluster: galaxies (white), hot gas (red) and dark matter (blue).
Galaxy clusters are the most massive cosmic structures held together by gravity, consisting of galaxies, hot gas and dark matter. They sit in the densest hubs of the filamentary ‘cosmic web’ that pervades the Universe.
Using ESA’s XMM-Newton X-ray observatory, astronomers have detected three massive filaments flowing towards the core of Abell 2744 and connecting it with the cosmic web. The filaments also consist of galaxies, hot gas and dark matter. One of them can be seen as the elongated structure on the left side of the image, another one is visible towards the upper right, and the third one below the cluster, slightly towards the right.
There are also two structures – one on the lower left of the cluster, the other in the upper central part of the image – which are not physically linked to the cluster but are the projection of more distant structures viewed along the same line of sight.
The astronomers detected the hot gas in the cluster and filaments with X-ray observations and the galaxies with optical observations. To reconstruct the distribution of dark matter, they used the gravitational lensing effect that the mass of the cluster and filaments exerts on more distant galaxies.
Abell 2744 has a mass of almost two million billion times the mass of our Sun. Light from the cluster galaxies and gas travelled for over 3 billion years to reach Earth.
The image measures about half a degree across. The image is sprinkled with foreground stars belonging to our Galaxy, the Milky Way, which are visible as the roundish objects with diffraction spikes.
ESA’s XMM-Newton X-ray observatory has revealed three massive filaments of hot gas flowing towards a cluster of galaxies, uncovering a portion of the cosmic skeleton that pervades the entire Universe.
Galaxies tend to congregate, forming groups and even larger agglomerates called clusters. These clusters are the most massive cosmic structures held together by gravity. As well as galaxies, they contain large amounts of hot gas and even larger amounts of invisible dark matter.
On a grander scale, galaxies and galaxy clusters appear to be linked in a gigantic filamentary network, with the most massive clusters sitting in the densest hubs of this ‘cosmic web’.
Computer simulations indicate that the cosmic web, which consists primarily of dark matter and some ordinary matter, behaves as the scaffolding of the cosmos, providing the framework for stars, galaxies and clusters to form and evolve.
In the past few decades, astronomers have detected the threadlike structure of the cosmic web in the large-scale distribution of galaxies, and found hints that diffuse gas is arranged in a similar way.
Four galaxy clusters embedded in the cosmic web, the wispy network of both dark and baryonic matter that is believed to pervade the Universe. This image was extracted from a numerical simulation of the formation and evolution of cosmic structure.
Four very massive galaxy clusters are visible where the concentration of galaxies (shown in white and purple) is higher. Two of the clusters, in the lower left corner of the image, are in the early phases of a merging process; the other two clusters can be seen in the central part of the image, just above the centre. The filamentary structure formed by the four clusters extends toward the right side of the image, where several less massive systems can be seen.
Galaxy clusters form in the densest knots of the cosmic web, where filaments intersect. The density of gas in the filaments that link the clusters is represented with different colours, with dark brown indicating less dense regions and brighter colours (from orange to yellow and green) indicating increasingly denser regions.
The image shows a portion of the cosmic web that spans about 260 million light-years across.
A new study using ESA’s XMM-Newton X-ray observatory has now uncovered a handful of filaments made of galaxies, gas and dark matter that are flowing towards one of the most massive galaxy clusters in the Universe, obtaining the first, unambiguous detection of gas in the cosmic web.
“This was an unexpected and most welcome discovery,” says Dominique Eckert of the University of Geneva, Switzerland, lead author of the paper reporting the new results in the journal Nature this week.
The object of the study is Abell 2744, which has been nicknamed the Pandora Cluster owing to its complex and jumbled structure. It is composed of at least four smaller components that are merging.
“We knew that this is an incredibly massive cluster hosting active processes at its core, and seeing its direct connection to the cosmic web confirms our picture of how structures form in the Universe,” adds Dr Eckert.
From 30 hours of observations by XMM-Newton in December 2014, the astronomers detected five large structures of hot gas that seem to be linked to the core of Abell 2744.
Comparing the X-ray data with optical observations, they identified the galaxies that belong to the various filaments, recognising that three of them are physically connected to the cluster, while the other two are the projection of more distant structures viewed along the same line of sight.
Just like the cluster, the filaments also contain plenty of dark matter. The astronomers have reconstructed its distribution by studying the ‘gravitational lensing’ effect that the mass of the cluster and filaments exerts on distant galaxies, modifying the path of their light and so increasing their brightness and twisting their shapes as seen by us.
“We initially looked at the inner core of Abell 2744 with the Hubble Space Telescope, with the aim of using the cluster as a strong magnifying lens to detect background galaxies that would be otherwise too faint to observe,” explains co-author Mathilde Jauzac from the University of Durham, UK.
“After the discovery of X-ray gas in these filaments, we decided to look at the gravitational lensing effect also in the outskirts of the cluster, where background galaxies are only weakly distorted and magnified, but still enable us to study the dark matter distribution near the cluster as well as in the nearby filaments.”
The combination of observations at different wavelengths revealed how the various components of Abell 2744 and its surroundings coexist.
From the X-ray data, the astronomers measured the density and temperature of the gas and compared it with the predictions from theory. With gas temperatures of 10–20 million degrees celsius, the filaments are much colder than the centre of the cluster, where the gas reaches 100 million degrees, but hotter than the average temperature in the cosmic web, estimated to be several million degrees.
The gas and galaxies in the filaments amount to about a tenth of the total mass – the rest being dark matter – which also agrees with expectations.
While the measurements match well with the astronomers’ theoretical scenario, caution is always in order when drawing conclusions about the Universe as a whole.
“What we observed is a very special configuration of dense filaments close to an exceptionally massive cluster. We need a much larger sample of less-dense filaments to investigate the nature of the cosmic web in greater detail,” says Dr Eckert.
For more in-depth investigations, astronomers will have to wait for ESA’s Athena X-ray telescope, planned for launch in 2028.
Athena’s extraordinary sensitivity will make it possible to survey hot gas in the cosmic web across the sky, detecting faint and diffuse filaments and even identifying some of the atomic elements in the gas.
“With the discovery of filaments around Abell 2744, we are witnessing the build-up of the cosmic web in one of the busiest places in the known Universe, a crucial step in the study of the formation of galaxies and galaxy clusters,” says Norbert Schartel, ESA XMM-Newton Project Scientist.
See the full article here .
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The European Space Agency (ESA), established in 1975, is an intergovernmental organization dedicated to the exploration of space, currently with 19 member states. Headquartered in Paris, ESA has a staff of more than 2,000. ESA’s space flight program includes human spaceflight, mainly through the participation in the International Space Station program, the launch and operations of unmanned exploration missions to other planets and the Moon, Earth observation, science, telecommunication as well as maintaining a major spaceport, the Guiana Space Centre at Kourou, French Guiana, and designing launch vehicles. ESA science missions are based at ESTEC in Noordwijk, Netherlands, Earth Observation missions at ESRIN in Frascati, Italy, ESA Mission Control (ESOC) is in Darmstadt, Germany, the European Astronaut Centre (EAC) that trains astronauts for future missions is situated in Cologne, Germany, and the European Space Astronomy Centre is located in Villanueva de la Cañada, Spain.