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Gaia: Milky Way's last major collision was surprisingly recent

Gaia: Milky Way's last major collision was surprisingly recent
Visualization of a 'wrinkly' halo of stars around the Milky Way. Credit: Halo stars: ESA/Gaia/DPAC, T Donlon et al. 2024; Background Milky Way and Magellanic Clouds: Stefan Payne-Wardenaar

Our galaxy has collided with many others in its lifetime. ESA's Gaia space telescope now reveals that the most recent of these crashes took place billions of years later than we thought.

The Milky Way has grown over time as other galaxies have approached, collided with, and been torn apart and consumed by our galaxy. Each collision triggered that still ripple through different families of stars, affecting how they move and behave in space.

One of Gaia's aims is to unravel the history of our galaxy by studying these wrinkles—something it's doing by pinpointing the positions and motions of over 100,000 stars near to our own, a tiny fraction of the about 2 billion sources it observes.

"We get wrinklier as we age, but our work reveals that the opposite is true for the Milky Way. It's a sort of cosmic Benjamin Button, getting less wrinkly over time," says Thomas Donlon of the Rensselaer Polytechnic Institute and University of Alabama in Huntsville, U.S., and lead author of the new Gaia study published in Monthly Notices of the Royal Astronomical Society.

"By looking at how these wrinkles dissipate over time, we can trace when the Milky Way experienced its last big crash—and it turns out this happened billions of years later than we thought."

These galactic wrinkles were only found by Gaia in 2018. That study is the first to accurately determine the timing of the collision that made the wrinkles, by comparing observations with cosmological simulations.

Strange motions

The Milky Way's halo contains a large group of stars with unusual orbits, many of those thought to have been adopted into our galaxy during an event that astronomers call the "last major ." As the name suggests, this is the last time our galaxy experienced a significant collision with another galaxy—proposed to be a massive dwarf galaxy that flooded the Milky Way with stars that pass very close to our galaxy's center.

Scientists had dated this merger to between 8 and 11 billion years ago, when the Milky Way was in its infancy, and it is known as Gaia-Sausage-Enceladus (GSE). But data from Gaia—released as part of the telescope's Data Release 3 in 2022—now suggests that another merger may have delivered the unusually moving stars.

"For the wrinkles of stars to be as clear as they appear in Gaia data, they must have joined us less than 3 billion years ago—at least 5 billion years later than was previously thought," adds co-author Heidi Jo Newberg, also of Rensselaer Polytechnic Institute.

"New wrinkles of stars form each time the stars swing back and forth through the center of the Milky Way. If they'd joined us 8 billion years ago, there would be so many wrinkles right next to each other that we would no longer see them as separate features."

The finding suggests that rather than these stars originating from the ancient GSE merger, they must have come from a more recent event dubbed the Virgo Radial Merger, which took place less than 3 billion years ago.

This animation shows a merger beginning some 9.7 billion years ago and continuing to near-present day. It shows the spiral Milky Way in the centre of the frame, with our galaxy’s two prominent satellite galaxies (the Large and Small Magellanic Clouds) visible to the lower right. A red cloud of stars is shown moving across the frame – this is a dwarf galaxy colliding with the Milky Way. This galaxy is shown being ripped apart as a result of the collision. At around 7 billion years ago, the animation increases in resolution to better show the ‘cloud’ of new stars that is drawn into the Milky Way from this colliding dwarf. These stars create a ‘halo’ of stars around our galaxy, a large starry component that extends outwards in all directions (this halo has been visually enhanced in this simulation, but in reality is very dim compared to the galactic disc). Shortly after the collision, the inner galaxy looks messy and wrinkly, but a long time after it becomes smooth. Gaia is observing these wrinkles to trace and rewrite the history of the Milky Way. The space telescope is uniquely placed to explore the myriad stars in our skies, and has compiled an unrivalled dataset of the positions, distances and motions of around 1.5 billion stars to date. The new Gaia finding reveals that the wrinkles we see in the Milky Way were likely caused by a dwarf galaxy colliding with the Milky Way around 2.7 billion years ago – in other words, a large portion of the Milky Way only joined us within the last few billion years. Credit: European Space Agency

Rewriting history

There is evidence for the GSE merger taking place far back in the Milky Way's history. However, recent work has questioned whether a massive ancient merger is actually needed to explain the properties of the Milky Way as we see it today, and whether all of the stars originally associated with the GSE are from the same merger event.

In 2020, Thomas led the study that identified wrinkles of stars in the Milky Way, and compared these to simulations of different possible mergers.

"We can see how the shapes and number of wrinkles change over time using these simulated mergers. This lets us pinpoint the exact time when the simulation best matches what we see in real Gaia data of the Milky Way today—a method we used in this new study too," says Thomas.

"By doing this, we found that the wrinkles were likely caused by a dwarf galaxy colliding with the Milky Way around 2.7 billion years ago. We named this event the Virgo Radial Merger."

Since then, Thomas and colleagues have further explored this merger, slowly refining the idea that many of the oddly moving stars and debris in the Milky Way's inner halo were delivered to our galaxy from a much more recent galaxy collision than the GSE. They have also clarified that the stars originally associated with the GSE may have originated from multiple mergers, some ancient.

"The Milky Way's history is constantly being rewritten at the moment, in no small part thanks to new data from Gaia," adds Thomas. "Our picture of the Milky Way's past has changed dramatically from even a decade ago, and I think our understanding of these mergers will continue to change rapidly.

"This result—that a large portion of the Milky Way only joined us within the last few billion years—is a big change from what astronomers thought up until now. Many popular models and ideas about how the Milky Way grows would expect a recent head-on collision with a dwarf galaxy of this mass to be very rare."

It's likely that the Virgo Radial Merger brought in a family of other small dwarf galaxies and star clusters with it, which would have all joined the Milky Way at around the same time. Future exploration will reveal which of these smaller objects that were previously thought to be related to an ancient GSE are actually related to a more recent Virgo Radial Merger instead.

Incredible collaboration

This finding joins a stream of results from Gaia that are rewriting the history of our cosmic home. The is uniquely placed to explore the myriad stars in our skies, and has compiled an unrivaled dataset of the positions, distances and motions of around 1.5 billion stars to date.

"Gaia is a hugely productive mission that's transforming our view of the cosmos," says Timo Prusti, Project Scientist for Gaia at ESA. "Results like this are made possible due to incredible teamwork and collaboration between a huge number of scientists and engineers across Europe and beyond."

"This finding improves what we know of the many complicated events that shaped the Milky Way, helping us better understand how galaxies are formed and shaped—our home galaxy in particular."

More information: Thomas Donlon et al, The debris of the 'last major merger' is dynamically young, Monthly Notices of the Royal Astronomical Society (2024). DOI: 10.1093/mnras/stae1264

Citation: Gaia: Milky Way's last major collision was surprisingly recent (2024, June 6) retrieved 23 June 2024 from
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