\t\t\t\t\t\t06\/06\/2024<\/span> Our galaxy has collided with many others in its lifetime. ESA\u2019s Gaia space telescope\u00a0now reveals that the most recent of these crashes took place billions of years later than we thought.<\/p>\n<\/div>\n 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 wrinkles that still ripple through different families of stars, affecting how they move and behave in space.<\/p>\n One of Gaia\u2019s aims is to unravel the history of our galaxy by studying these wrinkles \u2013 something it\u2019s doing by pinpointing the positions and motions of over 100 000 stars near to our own, a tiny fraction of the about two billion sources it observes.<\/p>\n<\/p><\/div>\n \t\t\t\t<\/p>\n <\/figcaption><\/figure>\n \u201cWe get wrinklier as we age, but our work reveals that the opposite is true for the Milky Way. It\u2019s a sort of cosmic Benjamin Button, getting less wrinkly over time,\u201d says Thomas Donlon of the Rensselaer Polytechnic Institute and University of Alabama in Huntsville, USA, and lead author of the new Gaia study. \u201cBy looking at how these wrinkles dissipate over time, we can trace when the Milky Way experienced its last big crash \u2013 and it turns out this happened billions of years later than we thought.\u201d<\/p>\n These galactic wrinkles were only found by Gaia in 2018. This study is the first to accurately determine the timing of the collision that made the wrinkles, by comparing observations with cosmological simulations.<\/p>\n<\/p><\/div>\n The Milky Way\u2019s 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 \u2018last major merger\u2019. As the name suggests, this is the last time our galaxy experienced a significant collision with another galaxy \u2013 proposed to be a massive dwarf galaxy that flooded the Milky Way with stars that pass very close to our galaxy\u2019s centre.<\/p>\n Scientists had dated this merger to between eight and eleven billion years ago, when the Milky Way was in its infancy, and it is known as Gaia-Sausage-Enceladus (GSE). But data from Gaia \u2013 released as part of the telescope\u2019s Data Release 3 in 2022 \u2013 now suggests that another merger may have delivered the unusually moving stars.<\/p>\n<\/p><\/div>\n \u201cFor the wrinkles of stars to be as clear as they appear in Gaia data, they must have joined us less than three billion years ago \u2013 at least five billion years later than was previously thought,\u201d adds co-author Heidi Jo Newberg, also of Rensselaer Polytechnic Institute. \u201cNew wrinkles of stars form each time the stars swing back and forth through the centre of the Milky Way. If they\u2019d joined us eight billion years ago, there would be so many wrinkles right next to each other that we would no longer see them as separate features.\u201d<\/p>\n 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 three billion years ago.<\/p>\n<\/p><\/div>\n There is evidence for the GSE merger taking place far back in the Milky Way\u2019s 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.<\/p>\n In 2020, Thomas led the study that identified wrinkles of stars in the Milky Way, and compared these to simulations of different possible mergers. \u201cWe 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 \u2013 a method we used in this new study too,\u201d says Thomas. \u201cBy 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.\u201d<\/p>\n 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\u2019s 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.<\/p>\n \u201cThe Milky Way\u2019s history is constantly being rewritten at the moment, in no small part thanks to new data from Gaia,\u201d adds Thomas. \u201cOur 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.<\/p>\n \u201cThis result \u2013 that a large portion of the Milky Way only joined us within the last few billion years \u2013 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.\u201d<\/p>\n It\u2019s 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.<\/p>\n<\/p><\/div>\n This finding joins a stream of results from Gaia that are rewriting the history of our cosmic home. 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.<\/p>\n \u201cGaia is a hugely productive mission that\u2019s transforming our view of the cosmos,\u201d says Timo Prusti, Project Scientist for Gaia at ESA. \u201cResults like this are made possible due to incredible teamwork and collaboration between a huge number of scientists and engineers across Europe and beyond.\u201d<\/p>\n \u201cThis 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 \u2013 our home galaxy in particular.\u201d<\/p>\n<\/p><\/div>\n \u2018The Debris of the \u2018Last Major Merger\u2019 is Dynamically Young\u2019 by Donlon et al. (2023) is published in\u00a0Monthly Notices of the Royal Astronomical Society<\/i>. https:\/\/doi.org\/10.1093\/mnras\/stae1264<\/p>\n The study uses data from Gaia\u2019s Data Release 3: https:\/\/www.cosmos.esa.int\/web\/gaia\/dr3<\/p>\n ESA\u2019s Gaia space telescope\u00a0was launched on 19 December 2013 and has been surveying the skies since 2014. In this time, the mission has flipped our understanding of the Milky Way on its head, unveiling its shape and structure and revealing how mergers have affected the stars that call our galaxy home. Read more about some of the telescope’s key achievements.<\/p>\n For more information, please contact:<\/b><\/p>\n ESA Media Relations<\/p>\n Email:\u202fmedia@esa.int<\/p>\n<\/p><\/div>\n
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<\/div>Strange motions<\/h2>\n
\n\t\t\t\n\t\t<\/div>\n<\/p><\/div>\nRewriting history<\/h2>\n
Incredible collaboration<\/h2>\n
Notes for editors<\/h2>\n