Dark matter is putting the brakes on our Milky Way galaxy's spin

An artist's impression of the Milky Way galaxy, our cosmic home.
An artist's impression of the Milky Way galaxy, our cosmic home. (Image credit: NASA JPL)

The Milky Way rotates at a whopping 130 miles (210 kilometers) per second, but a new study has found that dark matter has slowed the rotation of its bar by at least 24% since its formation nearly 14 billion years ago. 

"Astrophysicists have long suspected that the spinning bar at the center of our galaxy is slowing down, but we have found the first evidence of this happening," study co-author Ralph Schoenrich, an astrophysicist at University College London, said in a statement.

These new findings not only shed light on the rotation of the Milky Way but also provide an insight into the nature of one of the most elusive materials in the universe — dark matter

 Related: How many stars are in the Milky Way?  

The Milky Way is a barred spiral galaxy with a thick band of stars in the center and large pivoting arms stretching out across the cosmos. Scientists think that a halo of dark matter surrounds the Milky Way, extending out far beyond its visible edge, as occurs at other galaxies. 

In the new study, researchers used data from Gaia, a European Space Agency mission mapping the positions of billions of stars, to study the Hercules Stream, a thick cluster of stars that revolve around the Milky Way at the same rate that the galactic bar itself spins. 

Because the stars in the Hercules Stream are gravitationally trapped by the pivoting bar, slowing down the bar's rotation would cause the stars to creep outward to keep their orbits in sync with the bar's spin.

The researchers found evidence of such an outward cosmic migration when they investigated the chemical makeup of the stars. The Hercules Stream stars are rich in heavier elements, suggesting that these stars formed closer to the galactic center, where stars are about 10 times richer in metals compared to those in the galactic suburbs. 

From these observations, the researchers concluded that the galactic bar had indeed slowed by at least 24%. Raising the question — what has the power to put the brakes on an entire pivoting galaxy?

"The counterweight slowing this spin must be dark matter," Schoenrich said in the statement. "Until now, we have only been able to infer dark matter by mapping the gravitational potential of galaxies and subtracting the contribution from visible matter."

Astronomers believe that dark matter shrouds the Milky Way — and other galaxies — in an elusive halo that extends far out into space. Scientists have estimated that there is five times as much dark matter in the universe as visible matter. 

Though apparently abundant throughout the cosmos, the nature of dark matter remains unknown. But findings published in this study are helping to piece together this mysterious dark matter puzzle.

"Our research provides a new type of measurement of dark matter — not of its gravitational energy but of its inertial mass (the dynamical response), which slows the bar's spin," Schoenrich said. "Our finding also poses a major problem for alternative gravity theories — as they lack dark matter in the halo, they predict no, or significantly too little slowing of the bar."

Alternative gravity theories — such as modified Newtonian dynamics — disregard the notion of dark matter. They instead attempt to explain why the behavior of galaxies doesn't fit within the predictions of general relativity by making tweaks to Einstein's theory of general relativity

The results of this study were published in the Monthly Notices of the Royal Astronomical Society.

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Daisy Dobrijevic
Reference Editor

Daisy Dobrijevic joined Space.com in February 2022 having previously worked for our sister publication All About Space magazine as a staff writer. Before joining us, Daisy completed an editorial internship with the BBC Sky at Night Magazine and worked at the National Space Centre in Leicester, U.K., where she enjoyed communicating space science to the public. In 2021, Daisy completed a PhD in plant physiology and also holds a Master's in Environmental Science, she is currently based in Nottingham, U.K. Daisy is passionate about all things space, with a penchant for solar activity and space weather. She has a strong interest in astrotourism and loves nothing more than a good northern lights chase!