Astronomers at Stanford University in California have finally found evidence for the existence of elusive dark matter – something that was, until recently, considered just hypothetical.
Dark matter accounts for approximately 27% of the mass and energy in the observable universe – and has remained invisible to scientists until now.
BYPASS THE CENSORS
Sign up to get unfiltered news delivered straight to your inbox.
The discovery was made by accident as astronomers examining a massive nearby galaxy found a strange distortion on its edge. The distortion, it turns out, was a smaller, invisible galaxy composed entirely of dark matter.
“We can find these invisible objects in the same way that you can see rain droplets on a window,” lead author Yashar Hezaveh said in a statement. Like raindrops, the massive clumps of matter warp objects seen through them. Hezaveh, an astronomer at Stanford University in California, worked with a team of scientists that used a massive radio telescope, the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile, to find a clump of missing matter in the outer rim of a larger galaxy that.
“You know they are there because they distort the image of the background objects,” Hezaveh said.
Solving the crisis
Observing objects in the distant universe can challenge the limits of current technology . As a shortcut, astronomers can rely on a much older tool: massive galaxies large enough to distort space-time. As predicted by Albert Einstein’s general theory of relativity, the enormous collections of stars serve as magnifying glasses by causing light to bend as it passes by. The distant light curves around the nearer galaxy, creating a so-called “Einstein ring.” This reveals faraway objects behind the nearby galaxy.
Scientists take advantage of the gravitational lensing phenomenon to study incredibly distant galaxies, many of which formed only a few billion years after the universe’s Big Bang.
The team of astronomers noticed that the newly updated ALMA’s image of an Einstein ring known as SDP.81 contained a strange distortion, unveiled only after thousands of computers working together searched for subtle anomalies. The unprecedented detail of the star-free region around the closer lensing galaxy, known as the halo, revealed a distinctive clump of matter less than one-thousandth the mass of the Milky Way. This clump’s location and mass, and the fact that no object could be spotted in the region suggested that the cluster could be an extremely faint dwarf galaxy of dark matter lying nearly 4 billion light-years from Earth.
Dark matter makes up more than three-fourths of the matter in the universe, but cannot be seen via visible light or electromagnetic radiation. Instead, scientists must use distortions produced by dark matter’s gravity to detect the material.
In the case of galaxies, smaller dark-matter clusters could help astronomers solve a long-standing puzzle. Theory predicts that most galaxies should host dwarf galaxies in their halos, but few of these smaller galaxies have been spotted. Only about 40 of the predicted thousands of such galaxies have been seen orbiting the Milky Way.
“This discrepancy between observed satellites and predicted abundances has been a major problem in cosmology for nearly two decades, even called a ‘crisis’ by some researchers,” said team member Neal Dalal, of the University of Illinois.
“If these dwarf objects are dominated by dark matter, this could explain the discrepancy while offering new insights into the true nature of dark matter,” he said.
According to the researchers, ALMA may bring more of these dark matter satellites to light. With its incredible sensitivity, the enormous array of instruments could pinpoint other invisible dwarf galaxies hovering around the edges of natural magnifying glasses throughout the universe.
“This is an amazing demonstration of the power of ALMA,” said team member Gilbert Holder, of McGill University in Canada. “We are now confident that ALMA can efficiently discover these dwarf galaxies.
“Our next step is to look for more of them.”