pith. sign in

arxiv: astro-ph/9903277 · v1 · submitted 1999-03-18 · 🌌 astro-ph

The Origin of Chaos in the Outer Solar System

classification 🌌 astro-ph
keywords analyticchaosjovianplanetsresonancesolarsystemtheory
0
0 comments X
read the original abstract

Classical analytic theories of the solar system indicate that it is stable, but numerical integrations suggest that it is chaotic. This disagreement is resolved by a new analytic theory. The theory shows that the chaos among the Jovian planets results from the overlap of the components of a mean motion resonance among Jupiter, Saturn, and Uranus, and provides rough estimates of the Lyapunov time (10 million years) and the dynamical lifetime of Uranus (10^{18} years). The Jovian planets must have entered the resonance after all the gas and most of the planetesimals in the protoplanetary disk were removed.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.