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Terminal Instability of the Solar System Triggered by Stochastic Solar Mass Loss

  • Authors: Konstantin Batygin, Jim Fuller, Fred C. Adams

Konstantin Batygin et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure B1.

Instability onset times as a function of ejection granularity. Each point is one realization’s instability onset (circles: ejections throughout the giant-branch phases; squares: AGB-only; leftward triangles: systems already unstable during the mass-loss epoch), from the 48-seed grid of 3 Gyr integrations; fractions at right give unstable/integrated counts. As Mej grows, the distribution both fills in (higher total instability) and slants toward earlier onsets, terminating at fiducial Mej in a substantial population that never survives the mass loss at all. The gray curve traces the earliest onset at each Mej.

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