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How a Dwarf Galaxy Shook the Milky Way ⚡ экспресс

Original: "Galactic seismology: can a disc-crossing impulse explain the large-scale perturbations in the Milky Way's disc?"
arXiv:2602.05296 · 2026-02-05 · CC BY 4.0 · ⏱ 1 min · Galaxies
One massive collision explains the spirals and the disk warp, but unexplained waves hint at other impacts.
Abstract

Before its fall, the Sagittarius dwarf galaxy (Sgr) had a mass of ~10^11 M⊙ and over the last 5–6 billion years, repeatedly crossing the Milky Way’s disk, it lost a great deal of matter. The observed disk disturbances—spiral arms, corrugations, phase spiral, and the Lz–V_R wave—had been linked individually to these encounters. The new study performs a holistic analysis: can a single impulse from a crossing explain all of them at once? Modeling the encounter with a perturbing body like Sgr showed that one passage satisfactorily reproduces the local corrugations and arm segments (Outer, Local, Carina-Sagittarius); thus, the last significant impulse occurred 700–1200 million years ago. The Lz–V_R wave and phase spiral also emerge during this period and broadly match observations, but not in detail. Therefore, the last crossing of Sagittarius about a billion years ago may be the main cause of large-scale disk distortions, yet additional factors such as the Galactic bar or interactions with other satellites are needed to explain the Lz–V_R wave.

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The Sagittarius galaxy plunged into the disk of the Milky Way and passed through again and again, like a stone thrown into a still pond. Each strike left ripples: waves and warps in the star field. Once, Sagittarius brimmed with invisible mass (dark matter), but the collisions stripped away its gas and stars, turning it into a faint trail.

Astronomers simulated the last major impact about a billion years ago to see if it could spawn spiral arms, a warped disk, and subtle oscillations in star velocities. Motion measurements via spectroscopy confirmed: the impact explains the arms and warp, but more complex wave patterns aren’t fully reproduced. So our Galaxy remembers other shoves — from the dense central bar or other dwarf companions.

The most surprising part: Sagittarius itself has nearly vanished, but its dark matter likely still permeates the Milky Way, invisibly swaying stellar orbits. Like cosmic detectives, scientists piece together the Galaxy’s violent past.

🎯 The Sagittarius dwarf galaxy is still visible in the sky as a faint ribbon of stars, stretched thin by the Milky Way's gravity.

Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterAlbert Einstein
Tags
galaxy dark matter spectroscopy
Laws
Doppler effectgravitational lensingMaxwell's equationsPlanck's lawPlanck–Einstein relationWien's displacement law
Original: arXiv:2602.05296 · CC BY 4.0 · bridge42worlds