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Our Galaxy Has a Hot Side and Now We Know Why
| USA | science | βœ“ Verified - universetoday.com

Our Galaxy Has a Hot Side and Now We Know Why

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Our Galaxy's halo of hot gas is measurably warmer on one side than the other and a team of scientists have found the culprit. The gravitational pull of the Large Magellanic Cloud is drawing the Milky Way slowly southward, compressing the gas in its path and heating it up, much like a piston in an engine. The discovery solves a puzzle that has intrigued astronomers since the temperature difference was first detected in 2024.

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Our Galaxy Has a Hot Side and Now We Know Why By Mark Thompson - April 28, 2026 11:16 PM UTC | Milky Way If you have ever pushed your finger against the hole of a bicycle pump and felt the air grow warm as you compressed it, you already understand the physics at the heart of a new discovery about our own Galaxy. Because it turns out the Milky Way has a hot side and a cool side and the reason why comes down to exactly the same principle. Astronomers have known for some time that our Galaxy is surrounded by an enormous halo of hot gas. This vast, invisible sphere extends far beyond the familiar disc of stars we think of as the Milky Way, and is around two million degrees, several hundred times hotter than the visible surface of the Sun. What puzzled scientists was why one half of this halo appears to be warmer than the other. Data from the eROSITA X-ray observatory, released in 2024, showed that the southern half of the halo runs up to twelve percent hotter than the north. Nobody could quite explain why. The X-ray detectors of the eROSITA X-Ray observatory (Credit : JohannesBuchner) Now a team at the University of Groningen think they have the answer and it involves a neighbour that has been quietly nudging us for billions of years. The Large Magellanic Cloud, the small satellite galaxy visible from Earth's southern hemisphere is a smudge of light in the night sky. It orbits the Milky Way, and its gravity is enough to tug our entire Galaxy slowly in its direction. The Milky Way is currently drifting southward toward it at around forty kilometres per second. That might not sound dramatic, but over vast timescales and distances, it adds up to something significant. As the Milky Way moves, it presses into the gas on its southern side. The Galaxy acts like a piston, compressing the gas in its path and that compressed gas heats up. It is precisely the same effect that warms the air in your bicycle pump, just scaled up to something almost incomprehensibly large. The compute...
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