Rutgers University astronomers have produced the most advanced galaxy simulations of their kind, which could help reveal the origins of the Milky Way and dozens of small neighboring dwarf galaxies.
Their research also could aid the decades-old search for dark matter, which fills an estimated 27 percent of the universe. And the computer simulations of “ultra-faint” dwarf galaxies could help shed light on how the first stars formed in the universe.
“Our supercomputer-generated simulations provide the highest-ever resolution of a Milky Way-type galaxy,” said co-author Alyson M. Brooks, an associate professor in the Department of Physics and Astronomy in the School of Arts and Sciences at Rutgers University–New Brunswick.
“The high resolution allows us to simulate smaller neighbor galaxies than ever before – the ‘ultra-faint’ dwarf galaxies. These tiny galaxies are mostly dark matter and therefore are some of the best probes we have for learning about dark matter, and this is the first time that they have ever been simulated around a Milky Way-like galaxy. The sheer variety of the simulated galaxies is unprecedented, including one that lost all of its dark matter — similar to what’s been observed in space.”
According to Brooks, the Frontera supercomputer at the Texas Advanced Computing Center is the fastest system she has ever used.
“Most astronomers think it’s computationally unfeasible to run a simulation that resolves these tiny galaxies around the Milky Way, but we’ve done it thanks to cutting-edge supercomputers like Frontera, combined with our state-of-the-art code, ChaNGa, that allows us to take advantage of up to thousands of nodes on supercomputers,” she said.
The Rutgers-led team generated two new simulations of Milky Way-type galaxies and their surroundings. They call them the “DC Justice League Simulations,” naming them after two women who have served on the U.S. Supreme Court: current Associate Justice Elena Kagan and retired Associate Justice Sandra Day O’Connor.
These are cosmological simulations, meaning they begin soon after the Big Bang and model the evolution of galaxies over the entire age of the universe (almost 14 billion years). Bound via gravity, galaxies consist of stars, gas and dust. The Milky Way is an example a large barred spiral galaxy, according to NASA.
In recent years, scientists have discovered “ultra-faint” satellite galaxies of the Milky Way, thanks to digital sky surveys that can reach fainter depths than ever. While the Milky Way has about 100 billion stars and is thousands of light years across, ultra-faint galaxies have a million times fewer stars (under 100,000 and as low as few hundred) and are much smaller, spanning tens of light years.
For the first time, the simulations allow scientists to begin modeling these ultra-faint satellite galaxies around a Milky Way-type galaxy, meaning they provide some of the first predictions for what future sky surveys will discover.
In one simulation, a galaxy lost all its dark matter, and while real galaxies like that have been seen before, this is the first time anyone has simulated such a galaxy. These kinds of results tell scientists what’s possible when it comes to forming galaxies, and they are learning new ways that neighbor galaxies can arise, allowing scientists to better understand what telescopes find.
In about a year, the Large Synoptic Survey Telescope, recently renamed the Vera C. Rubin Observatory, will begin a survey targeting the whole sky and scientists expect to find hundreds of ultra-faint galaxies. In recent years, surveys targeting a small patch of the sky have discovered dozens of them.
“Just counting these galaxies can tell scientists about the nature of dark matter. Studying their structure and the motions of their stars can tell us even more,” said lead author Elaad Applebaum, a Rutgers doctoral student. “These galaxies are also very old, with some of the most ancient stars, meaning they can tell us about how the first stars formed in the universe.”