Theory of Secular Chaos and Mercury's Orbit
Yoram Lithwick (Northwestern), Yanqin Wu (Toronto)

TL;DR
This paper develops a theoretical framework for understanding secular chaos in planetary systems, especially explaining Mercury's chaotic orbit through resonance overlaps, supported by analytical and numerical methods.
Contribution
It introduces a new analytical approach to identify and quantify nonlinear secular resonances and applies it to explain Mercury's chaotic orbit.
Findings
Secular chaos arises from overlapping nonlinear secular resonances.
The 'map of the mean momenta' (MMM) effectively visualizes chaos emergence.
Mercury's chaos threshold involves specific eccentricity and inclination values of Jupiter and Venus.
Abstract
We study the chaotic orbital evolution of planetary systems, focusing on secular (i.e., orbit-averaged) interactions, because these often dominate on long timescales. We first focus on the evolution of a test particle that is forced by multiple massive planets. To linear order in eccentricity and inclination, its orbit precesses with constant frequencies. But nonlinearities can shift the frequencies into and out of secular resonance with the planets' eigenfrequencies, or with linear combinations of those frequencies. The overlap of these nonlinear secular resonances drive secular chaos in planetary systems. We quantify the resulting dynamics for the first time by calculating the locations and widths of nonlinear secular resonances. When results from both analytical calculations and numerical integrations are displayed together in a newly developed "map of the mean momenta" (MMM), the…
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