{"id":711,"date":"2026-06-10T14:36:52","date_gmt":"2026-06-10T14:36:52","guid":{"rendered":"https:\/\/redzine.co.uk\/index.php\/2026\/06\/10\/the-milky-way-was-rewired-by-a-cataclysmic-collision-billions-of-years-ago-now-it-is-on-course-for-another\/"},"modified":"2026-06-10T14:36:52","modified_gmt":"2026-06-10T14:36:52","slug":"the-milky-way-was-rewired-by-a-cataclysmic-collision-billions-of-years-ago-now-it-is-on-course-for-another","status":"publish","type":"post","link":"https:\/\/redzine.co.uk\/index.php\/2026\/06\/10\/the-milky-way-was-rewired-by-a-cataclysmic-collision-billions-of-years-ago-now-it-is-on-course-for-another\/","title":{"rendered":"The Milky Way was rewired by a cataclysmic collision billions of years ago. Now it is on course for another"},"content":{"rendered":"<figure><img decoding=\"async\" src=\"https:\/\/images.theconversation.com\/files\/740421\/original\/file-20260608-57-ujq2uh.jpg?ixlib=rb-4.1.0&amp;rect=1215%2C0%2C7293%2C4862&amp;q=45&amp;auto=format&amp;w=1050&amp;h=700&amp;fit=crop\" \/><figcaption><span class=\"caption\">Composite image of the centre of the Milky Way, created by the Hubble and Spitzer Space Telescopes and the Chandra X-ray Observatory.<\/span> <span class=\"attribution\"><a class=\"source\" href=\"https:\/\/commons.wikimedia.org\/wiki\/File:Center_of_the_Milky_Way_Galaxy_IV_%E2%80%93_Composite.jpg#\/media\/File:Center_of_the_Milky_Way_Galaxy_IV_%E2%80%93_Composite.jpg\">Nasa\/JPL-Caltech\/Esa via Wikimedia Commons<\/a><\/span><\/figcaption><\/figure>\n<p><em>Vasily Belokurov is <a href=\"https:\/\/kavli-prize.vercel.app\/2026-kavli-prize-laureates-announced\">one of three winners<\/a> of the 2026 Kavli Prize in Astrophysics. The award is for \u201cuncovering the fossil evidence of past mergers proving that the Milky Way galaxy\u201d was built through the continuous collision and merging of smaller objects.<\/em><\/p>\n<p>No matter the time or vantage point, from a pre-Neolithic cave to a post-lockdown London high-rise, the predictability of the night sky has always been humanity\u2019s symbol of permanence and reassuring stability.<\/p>\n<p>Yet this apparent calm is deceptive. Our galaxy, the Milky Way, <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2022MNRAS.514..689B\/abstract\">emerged from chaos and turbulence<\/a>, and its constellations are full of migrants, exiles and survivors. Right now, it has <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2023Galax..11...59V\/abstract\">begun to stretch and distort again<\/a>, pulled by a massive companion and heading for an inevitable collision.<\/p>\n<p>How can I be so sure? As a <a href=\"https:\/\/www.ast.cam.ac.uk\/people\/vasily.belokurov\">galactic archaeologist<\/a>, my job is to reconstruct the past of our galaxy and read the signs of its future.<\/p>\n<p>Instead of digging through soil, I use the laws of dynamics and stellar evolution to sift through hundreds of millions of stars \u2013 searching for the most ancient and chemically peculiar among them, interpreting their orbits and piecing together the events that shaped the Milky Way. <a href=\"https:\/\/www.cam.ac.uk\/research\/news\/the-gaia-sausage-the-major-collision-that-changed-the-milky-way\">One ancient encounter<\/a> left scars so deep that, billions of years later, they still define the galaxy around us.<\/p>\n<p>I want to understand what governs the lives of these massive cosmic systems: which changes are nature \u2013 the slow internal evolution of a <a href=\"https:\/\/www.cfa.harvard.edu\/news\/how-disc-galaxies-work\">galaxy disc<\/a> \u2013 and which are nurture, imposed by collisions and mergers.<\/p>\n<p>Questions about the source of <a href=\"https:\/\/theconversation.com\/topics\/dark-matter-95\">dark matter<\/a> underpin it all. This is the invisible substance whose gravity holds galaxies together, but whose true identity remains one of the greatest unsolved puzzles in astrophysics.<\/p>\n<p>The Milky Way is the one galaxy where stellar motions can be measured in extraordinary detail. This allows cosmologists including myself to construct our most precise map yet of dark matter: <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2021MNRAS.501.5964D\/abstract\">how far it reaches<\/a>, <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2019PhRvD..99b3012E\/abstract\">how dense it is around the Sun<\/a>, <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2023MNRAS.521.4936K\/abstract\">what shape<\/a> it has and <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2015MNRAS.454.3542E\/abstract\">how smooth or lumpy it may be<\/a>. If we can build this map in enough detail, we may begin to understand not just where dark matter is, but what it is.<\/p>\n<figure><figcaption><span class=\"caption\">Francesca Fragkoudi and Mark Lovell, Durham University.<\/span><\/figcaption><\/figure>\n<h2>A cataclysmic collision<\/h2>\n<p>Our work has been transformed by a revolution in open sky surveys. From 2000, the <a href=\"https:\/\/impact.sloan.org\/share-tactics-bad63e328931\">Sloan Digital Sky Survey<\/a> showed what becomes possible when vast astronomical datasets are made public, enabling discoveries far beyond the goals for which the survey was first built.<\/p>\n<p>And since 2014, <a href=\"https:\/\/www.esa.int\/Science_Exploration\/Space_Science\/Gaia\/Last_starlight_for_ground-breaking_Gaia\">Gaia, the European space telescope<\/a>, has taken this transformation to another level by mapping the positions and motions of nearly 2 billion stars, turning the galaxy into a vast archaeological record. No ruins, no shards and no bones \u2013 only stars that hold the clues.<\/p>\n<figure class=\"align-right zoomable\">\n            <a href=\"https:\/\/images.theconversation.com\/files\/740426\/original\/file-20260608-57-4pwbzu.png?ixlib=rb-4.1.0&amp;q=45&amp;auto=format&amp;w=1000&amp;fit=clip\"><img decoding=\"async\" alt=\"The Milky Way mapped.\" src=\"https:\/\/images.theconversation.com\/files\/740426\/original\/file-20260608-57-4pwbzu.png?ixlib=rb-4.1.0&amp;q=45&amp;auto=format&amp;w=237&amp;fit=clip\"><\/a><figcaption>\n              <span class=\"caption\">The Milky Way mapped with SDSS data.<\/span><br \/>\n              <span class=\"attribution\"><a class=\"source\" href=\"https:\/\/www.ast.cam.ac.uk\/people\/vasily.belokurov\">Vasily Belokurov<\/a>, <a class=\"license\" href=\"http:\/\/creativecommons.org\/licenses\/by-nc-nd\/4.0\/\">CC BY-NC-ND<\/a><\/span><br \/>\n            <\/figcaption><\/figure>\n<p>The clearest giveaway that something cataclysmic took place long ago in our galaxy is the migrants we observe: stars that were not born in the Milky Way.<\/p>\n<p>While native stars mostly travel together, circling the galactic centre in the great rotating flow of the disc, migrants cut across that order. They slide past the locals, plunge into the inner galaxy, then fly back out to its outskirts, again and again.<\/p>\n<p>These unusual orbits go hand-in-hand with unusual chemistry. Most of the migrant stars are less enriched in heavier elements than the locally born population. Their chemical composition is a sign of a slower rate of evolution that is typical of a dwarf galaxy.<\/p>\n<p>This makes the migrants doubly valuable. They are both fossils of the Milky Way\u2019s violent past, and probes of its outer regions, travelling where the local stars rarely go.<\/p>\n<h2>How the Milky Way was rewired<\/h2>\n<p>One of the central ideas in the theory of cosmic structure formation is that galaxies grow hierarchically. Smaller galaxies <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2005ApJ...635..931B\/abstract\">fall into larger ones and are torn apart<\/a>, leaving their stars behind as migrants.<\/p>\n<p>In the Milky Way, the largest ancient structure of this kind is known as <a href=\"https:\/\/www.simonsfoundation.org\/2018\/07\/04\/gaia-sausage-galaxy\/\">Gaia-Sausage-Enceladus<\/a>. It is the remains of a vanished galaxy that collided with our own between 8 and 11 billion years ago (the \u201csausage\u201d refers to a pattern in its stars\u2019 motions).<\/p>\n<figure class=\"align-center zoomable\">\n            <a href=\"https:\/\/images.theconversation.com\/files\/740442\/original\/file-20260608-57-3wp45r.jpg?ixlib=rb-4.1.0&amp;q=45&amp;auto=format&amp;w=1000&amp;fit=clip\"><img decoding=\"async\" alt=\"Artist&apos;s impression of the young Milky Way colliding with another galaxy around 10 billion years ago.\" src=\"https:\/\/images.theconversation.com\/files\/740442\/original\/file-20260608-57-3wp45r.jpg?ixlib=rb-4.1.0&amp;q=45&amp;auto=format&amp;w=754&amp;fit=clip\"><\/a><figcaption>\n              <span class=\"caption\">Artist\u2019s impression of the young Milky Way colliding with another galaxy around 10 billion years ago.<\/span><br \/>\n              <span class=\"attribution\"><a class=\"source\" href=\"https:\/\/people.ast.cam.ac.uk\/~vasily\/gaia_sausage\/info.html\">Vasily Belokurov, based on image by Juan Carlos Mu\u00f1oz\/ESO<\/a>, <a class=\"license\" href=\"http:\/\/creativecommons.org\/licenses\/by-nc-sa\/4.0\/\">CC BY-NC-SA<\/a><\/span><br \/>\n            <\/figcaption><\/figure>\n<p>The Milky Way also did not go through that crash unscathed. The collision rewired and reshaped it.<\/p>\n<p>Some of these changes are easily visible in the data. Stars from the old disc were <a href=\"https:\/\/astrobites.org\/2019\/10\/08\/the-biggest-splash\/\">splashed<\/a> into our galaxy\u2019s <a href=\"https:\/\/www.cfa.harvard.edu\/news\/tilt-our-stars-shape-milky-ways-halo-stars-realized\">halo<\/a>, becoming exiles in the place where they were born. A <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2018ApJ...863L..28M\/abstract\">new posse of star clusters<\/a> were also acquired.<\/p>\n<p>At the same time, we think something even more momentous was taking place. The encounter changed the orientation of the <a href=\"https:\/\/www.lancashire.ac.uk\/news\/milky-way-star-forming-disc\">Milky Way\u2019s disc<\/a>, and its alignment with the <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2007A%26A...469..387T\/abstract\">dark matter halo<\/a>.<\/p>\n<p>While dark matter is <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2014JPhG...41f3101R\/abstract\">too diffuse to dominate our Solar System<\/a>, in the outer galaxy it is the main gravitating mass \u2013 <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020PhRvD.101b3006O\/abstract\">moving, streaming<\/a> and, in the standard picture, <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2008MNRAS.391.1685S\/abstract\">clumping into a hierarchy of lumps<\/a>.<\/p>\n<p>Around the Milky Way, this dark matter forms a vast halo, much larger than the luminous part of our galaxy. We often imagine this halo as a sparse, round cloud, but Gaia has helped show <a href=\"https:\/\/aasnova.org\/2021\/10\/18\/featured-image-an-asymmetric-dark-matter-halo\/\">this picture is too simple<\/a>.<\/p>\n<p>The dark halo can be stretched out of shape by a major encounter. Like a ship beginning to list, <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2023MNRAS.518.2870D\/abstract\">the Milky Way started to lean<\/a> \u2013 not suddenly, not visibly, but over billions of years.<\/p>\n<figure class=\"align-center zoomable\">\n            <a href=\"https:\/\/images.theconversation.com\/files\/740424\/original\/file-20260608-57-bxt795.jpg?ixlib=rb-4.1.0&amp;q=45&amp;auto=format&amp;w=1000&amp;fit=clip\"><img decoding=\"async\" alt=\"View of the Southern sky shows the Milky Way and (far right, close to horizon) two galactic neighbours, the Small and Large Magellanic Clouds.\" src=\"https:\/\/images.theconversation.com\/files\/740424\/original\/file-20260608-57-bxt795.jpg?ixlib=rb-4.1.0&amp;q=45&amp;auto=format&amp;w=754&amp;fit=clip\"><\/a><figcaption>\n              <span class=\"caption\">View of the Southern sky shows the Milky Way and (far right, close to horizon) two galactic neighbours, the Small and Large Magellanic Clouds.<\/span><br \/>\n              <span class=\"attribution\"><a class=\"source\" href=\"https:\/\/commons.wikimedia.org\/wiki\/File:360-degree_Panorama_of_the_Southern_Sky.jpg\">H.H. Heyer\/ESO via Wikimedia Commons<\/a>, <a class=\"license\" href=\"http:\/\/creativecommons.org\/licenses\/by-nc-nd\/4.0\/\">CC BY-NC-ND<\/a><\/span><br \/>\n            <\/figcaption><\/figure>\n<h2>A new galactic dance<\/h2>\n<p>Unusually compared with many galaxies of similar mass, the Milky Way was allowed ample time to recover from the shock of the \u201csausage merger\u201d. No other cosmic cataclysm appears to have shaken our Galaxy since, letting it settle into a quiet, uneventful life. That is, until now.<\/p>\n<p>The <a href=\"https:\/\/www.nasa.gov\/image-article\/large-magellanic-cloud\/\">Large Magellanic Cloud<\/a> (LMC), currently our galaxy\u2019s most massive companion, is already pulling at the Milky Way, disturbing its halo again. In an echo of what happened some 10 billion years ago, the <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2021MNRAS.501.2279V\/abstract\">Milky Way is being drawn into an accelerating dance<\/a> with this neighbouring dwarf galaxy, recoiling in response to the LMC\u2019s approach.<\/p>\n<p>This is a dance that only one galaxy is likely to survive intact. A new chapter of migration, survival and adaptation has begun.<\/p>\n<p>None of this spoils the beauty of the night sky \u2013 it deepens it. The calm band of light above us is not a symbol of permanence, but the visible reminder of a long survival.<\/p>\n<p>The Milky Way has been broken, rebuilt and is now being disturbed again. Its stars remember the past; their motions reveal the future. What looks eternal is, in truth, a moment in a much longer story.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/counter.theconversation.com\/content\/284721\/count.gif\" alt=\"The Conversation\" width=\"1\" height=\"1\" \/><\/p>\n<p class=\"fine-print\"><em><span>Vasily Belokurov has received funding from the European Research Council, the Leverhulme Trust, and the Science and Technology Facilities Council.<\/span><\/em><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Composite image of the centre of the Milky Way, created by the Hubble and Spitzer Space Telescopes and the Chandra X-ray Observatory. Nasa\/JPL-Caltech\/Esa via Wikimedia Commons Vasily Belokurov is one of three winners of the 2026 Kavli Prize in Astrophysics. The award is for \u201cuncovering the fossil evidence of past mergers proving that the Milky [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[1],"tags":[],"class_list":["post-711","post","type-post","status-publish","format-standard","hentry","category-uncategorized"],"_links":{"self":[{"href":"https:\/\/redzine.co.uk\/index.php\/wp-json\/wp\/v2\/posts\/711","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/redzine.co.uk\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/redzine.co.uk\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/redzine.co.uk\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/redzine.co.uk\/index.php\/wp-json\/wp\/v2\/comments?post=711"}],"version-history":[{"count":0,"href":"https:\/\/redzine.co.uk\/index.php\/wp-json\/wp\/v2\/posts\/711\/revisions"}],"wp:attachment":[{"href":"https:\/\/redzine.co.uk\/index.php\/wp-json\/wp\/v2\/media?parent=711"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/redzine.co.uk\/index.php\/wp-json\/wp\/v2\/categories?post=711"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/redzine.co.uk\/index.php\/wp-json\/wp\/v2\/tags?post=711"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}