Depletion and Excitation of the Asteroid Belt by Migrating Planets

K. J. Walsh (1) , A. Morbidelli (2) , Sean N. Raymond (3) , D. P. O'Brien , A. M. Mandell

1 Department of Archaeology
2 LAGRANGE - Joseph Louis LAGRANGE
3 SSE 2012

A model of early inner Solar System evolution whereby the gas-driven migration of Jupiter and Saturn truncates the disk of planetesimals and creates a depleted and dynamically excited asteroid belt populated from two parent populations.

Domaines: Planétologie et astrophysique de la terre [astro-ph.EP]; Planétologie et astrophysique de la terre [astro-ph.EP]

K. J. Walsh, A. Morbidelli, Sean N. Raymond, D. P. O'Brien, A. M. Mandell. Depletion and Excitation of the Asteroid Belt by Migrating Planets. Asteroids, Comets, Meteors 2012, Proceedings of the conference held May 16-20, 2012 in Niigata, Japan. LPI Contribution No. 1667, id.6157, 2012, 2012, Nigata, Japan. pp.6157. ⟨hal-00752264⟩