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Up to 96% of simulated outer solar systems became unstable in scenarios with larger bursts of solar mass loss

Phys.org reports the instability occurred within 3 billion years of the sun becoming a white dwarf.

Phys.orgPH
1 Source, 11h ago, first seen 11h ago

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Phys.org reports that in scenarios with larger bursts of solar mass loss, up to 96% of simulated outer solar systems became unstable within 3 billion years of the sun becoming a white dwarf.

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Phys.org@physorg_comUp to 96% of simulated outer solar systems became unstable within 3 billion years of the sun becoming a white dwarf in scenarios with larger bursts of solar mass loss. @AAS_Office https://phys.org/news/2026-10-dying-sun-solar-sooner-thought.html?utm_source=twitter.com&utm_medium=social&utm_campaign=v211h
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    Phys.org@physorg_comUp to 96% of simulated outer solar systems became unstable within 3 billion years of the sun becoming a white dwarf in scenarios with larger bursts of solar mass loss. @AAS_Office https://phys.org/news/2026-10-dying-sun-solar-sooner-thought.html?utm_source=twitter.com&utm_medium=social&utm_campaign=v211h
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    Today's Rank

    #19