“It was shocking to realize that the Milky Way had a large sibling, and we never knew about it,” said Eric Bell, University of Michigan professor of astronomy in 2018 about his discovery that the Andromeda galaxy (also named M31), our closest large galactic neighbor, shredded and cannibalized a massive galaxy two billion years ago.
Left a halo of stars larger than the Andromeda Galaxy itself
Even though it was mostly shredded, this massive galaxy left behind a rich trail of evidence: an almost invisible halo of stars larger than the Andromeda galaxy itself, an elusive stream of stars and a separate enigmatic compact galaxy, M32. Discovering and studying this decimated galaxy will help astronomers understand how disk galaxies like the Milky Way evolve and survive large mergers.
Long-lost sibling of the Milky Way
This disrupted galaxy, named M32p, was the third-largest member of the Local Group of galaxies, after the Milky Way and Andromeda galaxies. Using computer models, Richard D’Souza and Eric Bell of the University of Michigan’s Department of Astronomy were able to piece together this evidence, revealing this long-lost sibling of the Milky Way. Their findings were published in Nature Astronomy.
Scientists have long known that this nearly invisible large halo of stars surrounding galaxies contains the remnants of smaller cannibalized galaxies. A galaxy like Andromeda was expected to have consumed hundreds of its smaller companions. Researchers thought this would make it difficult to learn about any single one of them.
Using new computer simulations, the scientists were able to understand that even though many companion galaxies were consumed by Andromeda, most of the stars in the Andromeda’s outer faint halo were mostly contributed by shredding a single large galaxy.
The ‘Eureka’ Moment
“It was a ‘eureka’ moment. We realized we could use this information of Andromeda’s outer stellar halo to infer the properties of the largest of these shredded galaxies,” said lead author D’Souza, a postdoctoral researcher at U-M.
“Astronomers have been studying the Local Group—the Milky Way, Andromeda and their companions—for so long. It was shocking to realize that the Milky Way had a large sibling, and we never knew about it,” said co-author Bell.
This galaxy, called M32p, which was shredded by the Andromeda galaxy, was at least 20 times larger than any galaxy which merged with the Milky Way over the course of its lifetime. M32p would have been massive, making it the third largest galaxy in the Local Group after the Andromeda and the Milky Way galaxies.
M32 is a Weirdo–“There isn’t another galaxy like it”
This work might also solve a long-standing mystery: the formation of Andromeda’s enigmatic M32 satellite galaxy, the scientists say. They suggest that the compact and dense M32 is the surviving center of the Milky Way’s long-lost sibling, like the indestructible pit of a plum.
“M32 is a weirdo,” Bell said. “While it looks like a compact example of an old, elliptical galaxy, it actually has lots of young stars. It’s one of the most compact galaxies in the universe. There isn’t another galaxy like it.”
“We don’t think that it was an elliptical,” Bell told The Daily Galaxy, “rather we think that it was likely to be a disk galaxy (because it had gas – as evidenced by the ongoing star formation during the merger, and most galaxies with gas in the local Universe are disks/spiral galaxies).”
Their study may alter the traditional understanding of how galaxies evolve, the researchers say. They realized that the Andromeda’s disk survived an impact with a massive galaxy, which would question the common wisdom that such large interactions would destroy disks and form an elliptical galaxy.
The timing of the merger may also explain the thickening of the disk of the Andromeda galaxy as well as a burst of star formation two billion years ago, a finding which was independently reached by French researchers earlier this year.
“Andromeda would have looked so different 2 Billion Years Ago”
“The Andromeda Galaxy, with a spectacular burst of star formation, would have looked so different 2 billion years ago,” Bell said. “When I was at graduate school, I was told that understanding how the Andromeda Galaxy and its satellite galaxy M32 formed would go a long way towards unraveling the mysteries of galaxy formation.”
“Using models of galaxy formation,” Bell wrote in reply to an email from The Daily Galaxy, “we realized that if a satellite galaxy has gas and is forming stars, that it stops forming stars when it is finally ripped apart by the gravitational forces of the big galaxy – in this case, Andromeda. So, we were able to use other folks’ measurements of the history of star formation in M32, and in M31’s diffuse stellar halo, realized that star formation stopped around 2 billion years ago, and used that to age-date when M32p was destroyed.”
“There is other research – Ivanna Escala (at Carnegie Observatory) has been measuring the chemical composition of stars in Andromeda’s diffuse stellar halo; her results were a little of a surprise to Richard D’Souza and I, and we are thinking about what they tell us about the merger process,” Bell wrote in reply to an email from The Daily Galaxy asking about subsequent research about M32 and M32p. “Richard D’Souza and I actually turned our attention to thinking about satellite galaxies of Andromeda, and are arguing that most of Andromeda’s current satellite galaxies were actually companions of M32p originally, and were given to Andromeda during the merger process.
Source: Richard D’Souza et al, The Andromeda galaxy’s most important merger about 2 billion years ago as M32’s likely progenitor, Nature Astronomy (2018).
The Daily Galaxy, Avi Shporer, MIT Kavli Institute for Astrophysics and Space Research via University of Michigan, Nature, and Eric Bell. Avi was formerly a NASA Sagan Fellow at the Jet Propulsion Laboratory (JPL).
Image top of page: The Andromeda nebula, photographed at the Yerkes Observatory around 1900. To modern eyes, this object is clearly a galaxy. At the time, though, it was described as “a mass of glowing gas,” its true identity unknown. (From the book Astronomy of To-Day, 1909)
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