The Asteroid Belt as a Relic From a Chaotic Early Solar System
Andre Izidoro, Sean N. Raymond, Arnaud Pierens, Alessandro Morbidelli,, Othon C. Winter, David Nesvorny

TL;DR
This paper proposes that the chaotic early orbits of Jupiter and Saturn could explain the current dynamical excitation of the asteroid belt, offering a new perspective on Solar System formation.
Contribution
It demonstrates that chaos in the early gas giants' orbits can account for asteroid belt excitation without requiring large mass deficits or specific migration models.
Findings
Chaotic early orbits of Jupiter and Saturn can excite asteroid orbits.
Resonance jumps caused by chaos occur over tens of millions of years.
Early chaos in the Solar System is consistent with current orbital configurations.
Abstract
The orbital structure of the asteroid belt holds a record of the Solar System's dynamical history. The current belt only contains Earth masses yet the asteroids' orbits are dynamically excited, with a large spread in eccentricity and inclination. In the context of models of terrestrial planet formation, the belt may have been excited by Jupiter's orbital migration. The terrestrial planets can also be reproduced without invoking a migrating Jupiter; however, as it requires a severe mass deficit beyond Earth's orbit, this model systematically under-excites the asteroid belt. Here we show that the orbits of the asteroids may have been excited to their current state if Jupiter and Saturn's early orbits were chaotic. Stochastic variations in the gas giants' orbits cause resonances to continually jump across the main belt and excite the asteroids' orbits on a timescale of…
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