On the Dynamical Stability of the Solar System
Konstantin Batygin, Gregory Laughlin

TL;DR
This study uses long-term numerical simulations and bifurcation analysis to assess the Solar System's stability, finding it generally stable over 20 billion years but with potential instabilities involving Mercury, Venus, and Mars.
Contribution
It applies a bifurcation method to explore possible unstable evolutions of the Solar System, revealing specific scenarios of planetary collisions and ejections.
Findings
No severe instability over 20 Gyr in classical simulations.
Potential for Mercury to fall into the Sun or collide with Venus.
Mars could be ejected due to Mercury's instability.
Abstract
A long-term numerical integration of the classical Newtonian approximation to the planetary orbital motions of the full Solar System (sun + 8 planets), spanning 20 Gyr, was performed. The results showed no severe instability arising over this time interval. Subsequently, utilizing a bifurcation method described by Jacques Laskar, two numerical experiments were performed with the goal of determining dynamically allowed evolutions for the Solar System in which the planetary orbits become unstable. The experiments yielded one evolution in which Mercury falls onto the Sun at ~1.261Gyr from now, and another in which Mercury and Venus collide in ~862Myr. In the latter solution, as a result of Mercury's unstable behavior, Mars was ejected from the Solar System at ~822Myr. We have performed a number of numerical tests that confirm these results, and indicate that they are not numerical…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
