Dark matter packs a punch: Milky Way's spiral arms formed by intergalactic collision

Supercomputer simulations by Christopher W. Purcell, postdoctoral research associate in the Department of Physics and Astronomy in Pitt's School of Arts and Sciences, and colleagues report their findings in a paper titled "The Sagittarius Impact as an Architect of Spirality and Outer Rings in the Milky Way."

This paper is the first to identify Sagittarius as the architect of spiral structure in our Milky Way. "It presents a new and somewhat unexpected way of thinking about why the galaxy we live in looks the way it does," says Purcell.

"Cosmologically speaking, it demonstrates the idea that relatively small impacts like this can have a dramatic impact on the structure of galaxies throughout the universe," he adds. This idea had been assumed theoretically, but never demonstrated.

Purcell's collaborators include University of California High-Performance AstroComputing Center (UC-HIPACC)-affiliates James S. Bullock, Erik J. Tollerud, and Miguel Rocha, all at the University of California at Irvine. The fifth coauthor is Sukanya Chakrabarti at Florida Atlantic University.

In the field of cosmology, supercomputer simulations are the only laboratories for scientific experimentation. With supercomputers, astronomers can recreate a small-scale simulation or model of distant, violent events that occurred over billions of years, and observe that model in sped-up time, in order to make predictions that can be tested by actual observations of the universe.

Purcell's findings are based on supercomputer simulations he conducted for his PhD at the University of California, Irvine, and in the lab of Pitt professor of physics and astronomy Andrew Zentner.

Interestingly, Purcell's simulations revealed that even more important than the stars of the Sagittarius Dwarf was its halo of invisible "dark matter"—equal in mass to all the stars in the Milky Way.

Visible matter makes up less than five percent of the universe, while nearly a quarter of the universe is made of transparent dark matter. Its existence is felt only through its gravitational influence. It is now known that every galaxy, including the Sagittarius Dwarf (precollision) and our own Milky Way, resides at the center of a giant halo of dark matter several times larger in radius and many times greater in mass.

"When all the dark matter smacked into the Milky Way, 80 to 90 percent of it was stripped off," Purcell says. That first impact—more than two billion years ago—produced instabilities that were quickly amplified, eventually forming the spiral arms and ring structures in the outskirts of our own galaxy.

In his dissertation, Purcell focused on the question: What effects have the repeated collisions with the Sagittarius Dwarf had on the Milky Way?

Throughout the past few decades, conventional wisdom has been that the Milky Way was relatively unperturbed for the past several million years. Whatever spiral structure exists, these arms, were just a result of the Milky Way disc evolving in isolation.

Since the Sagittarius Dwarf was discovered, astronomers have tried to match up debris from that galaxy to what they saw in the universe. In 2003, infrared telescopes and supercomputers that traced the orbital motions of its stars has revealed that the Sagittarius Dwarf had actually collided with the Milky Way twice—once 1.9 billion years ago and again 0.9 billion years ago.

Enlarge

Computer simulations visualized the disk of the Milky Way Galaxy for three cases: no impact with a dwarf galaxy, impact with a Sgr dwarf galaxy of lower mass, and impact with a Sgr dwarf galaxy of higher mass. Our Galaxy is shown both edge-on and face-on in the inset panels, and the sun's location is marked as a yellow dot, and the present location of the Sagittarius dwarf's remnant core is marked as a pink dot, as shown after more than two billion years of isolated evolution. Shown in the background is a global rendering of the "light Sgr" tidal debris and the Milky Way disk. Credit: Chris Purcell/HI-PACC

Researchers found that the collision set up instabilities—fluctuations in density of stars—in the flat disk of the rotating Milky Way. Our galaxy rotates faster toward its center than toward its edges, so those instabilities were stretched and sheared, leading to the formation of spiral arms.

The simulations also revealed that the impact gave rise to ring-like structures found at the edges of our galaxy.

The second impact affected the Milky Way less, giving rise to only milder, less dense spiral-creating waves, because the Sagittarius Dwarf had by then lost most of its dark matter mass.

Without the dark matter to hold the dwarf galaxy together, its visible stars began to be pulled apart by the Milky Way's huge gravitational field and tidal forces.

"The dominant cosmology in astrophysics is one that's very violent on small scales. Galaxies like the Milky Way are constantly being bombarded by these small dwarf galaxies. It had not been appreciated prior to our work just how dramatic those impacts could be on the stellar disc itself," says Purcell. "We expected to find some more subtle signatures of an impact like this—a flare in the outer disc, like bell-bottom jeans. We expected to see some mild morphological changes to the Milky Way. But we did not expect to see a spiral structure begin to emerge as a result of these impacts. That was something we didn't foresee."

Indeed, Purcell and collaborators delayed publication for several months while they made sure they understood why they were seeing these results. "We had to convince ourselves that we weren't crazy," he jokes.

Today, long streamers of stars from the dismembered dwarf galaxy arch over and around the Milky Way, and "right now, billions and billions of dark matter particles from the Sagittarius Dwarf are raining down onto the Earth," said Purcell. "Meantime, the Sun itself is revolving around the center of the Milky Way Galaxy, in a complex and still-evolving system of multiple spiral arms."

We're just a few million years short of a third impact, Purcell says. But how can the researchers tell?

"We can tell when we look toward the center of the Milky Way," says Purcell. "Immediately on the opposite side of us, we can see this blob of stars crashing into the southern face of the disc from beneath. We can measure the velocities of these stars. We know that the dwarf galaxy is just about to smash the disc—in only another 10 million years."

Provided by University of Pittsburgh