This Hubble Space Telescope map shows the four clumps of dark matter in the supercluster Abell 901/902.
Credit: NASA, ESA, C. Heymans (University of British Columbia), M. Gray (University of Nottingham), M. Barden (Innsbruck), STAGES collaboration.
A new map reveals dense pools of invisible matter tipping the scales at 10 trillion times the mass of the sun and housing a cosmic city of ancient galaxies.
The map, presented last week at a meeting of the American Astronomical Society in Austin, Texas, provides indirect evidence for so-called dark matter and how this mysterious substance affects galaxy formation.
Scientists theorize that dark matter, considered to make up about 85 percent of the universe's matter, on which galaxies mature. As the universe evolves, the tug from dark matter's gravitational field causes galaxies to collide and swirl into superclusters.
It's all these gravitational effects, from something that can't be seen, that indicates dark matter exists.
"The dark matter halos are what allow the galaxies to form in the first place. The dark matter is the underlying skeleton of the universe," said Meghan Gray of the University of Nottingham in the United Kingdom, who was part of the map-making team. "Most of the universe is dark matter. Galaxies are just froth on this ocean of dark matter."
Uncovering invisible matter
Gray, Catherine Heymans of the University of British Columbia in Vancouver and colleagues used NASA's Hubble Space Telescope to observe a supercluster called Abell 901/902, which resides 2.6 billion light-years from Earth and spans more than 16 million light-years across.
The astrophysicists measured light from a backdrop of more than 60,000 galaxies after it passed through the supercluster and its . According to Einstein's general relativity theory, the presence of matter can bend spacetime, deflecting the path of a light ray passing through the mass.
"Dark matter leaves a signature in distant galaxies" explained study co-author Ludovic Van Waerbeke of the University of British Columbia. ?For example, a circular galaxy will become more distorted to resemble the shape of a banana if its light passes near a dense region of dark matter.?
By averaging the shape-distortions from the thousands of galaxies, the researchers found four pools of dark matter. And the invisible clumps matched up with the location of hundreds of ancient galaxies, which have experienced a violent history in their passage from the outskirts of the supercluster into the central hubs.
"If the supercluster wasn?t there, you'd still see all of these galaxies in the background," Gray told SPACE.com. "But you put this massive object [in front of them] and your view gets distorted. It's a cosmic optical illusion."
The survey's broader goal is to understand how galaxies are influenced by the environment in which they live.
?The new map of the underlying dark matter in the supercluster is one key piece of this puzzle,? Gray said. ?At the same time, we?re looking in detail at the galaxies themselves.?
The in the central hubs, they are finding, show signs of aging, as they are elliptical, red in color and are no longer forming stars. Disk galaxies reside on the outskirts of the supercluster. These youthful galaxies are blue-hued and buzzing with star birth.
It's these young galaxies that constantly fall into the supercluster, adding to its galactic girth.
"As they come in, either they're interacting with each other more or they're interacting with the dark matter," Gray explained. "Something is happening to change their properties."
The team plans to study individual galaxies in an effort to understand how this supercluster environment shapes and changes galaxies.