The first hints about the nature of the elusive dark matter which makes up more than 80 per cent of our universe were picked up by observations of colliding galaxies made with European Southern Observatory's Very Large Telescope (VLT) and the NASA/ESA Hubble Space Telescope.
Using the MUSE instrument on ESO's VLT in Chile, along with images from Hubble in orbit, a team of astronomers studied the simultaneous collision of four galaxies in the galaxy cluster Abell 3827.
Although dark matter cannot be seen, the team could deduce its location using a technique called gravitational lensing. The collision happened to take place directly in front of a much more distant, unrelated source.
The mass of dark matter around the colliding galaxies severely distorted spacetime, deviating the path of light rays coming from the distant background galaxy - and distorting its image into characteristic arc shapes.
The researchers observed the four colliding galaxies and found that one dark matter clump appeared to be lagging behind the galaxy it surrounds.
A lag between dark matter and its associated galaxy is predicted during collisions if dark matter interacts with itself, even very slightly, through forces other than gravity.
Dark matter has never before been observed interacting in any way other than through the force of gravity.
"We used to think that dark matter just sits around, minding its own business, except for its gravitational pull," said lead author Richard Massey at Durham University, UK.
"But if dark matter were being slowed down during this collision, it could be the first evidence for rich physics in the dark sector - the hidden Universe all around us," he said.
"Our observation suggests that dark matter might interact with forces other than gravity, meaning we could rule out some key theories about what dark matter might be," said team member Liliya Williams of the University of Minnesota.
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