Depletion and Excitation of the Asteroid Belt by Migrating Planets
Langue
en
Communication dans un congrès
Ce document a été publié dans
Asteroids, Comets, Meteors 2012, Proceedings of the conference held May 16-20, 2012 in Niigata, Japan. LPI Contribution No. 1667, id.6157, 2012, Asteroids, Comets, Meteors 2012, Proceedings of the conference held May 16-20, 2012 in Niigata, Japan. LPI Contribution No. 1667, id.6157, 2012, 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. 2012-05, vol. 1667, p. 6157
Résumé en anglais
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 ...Lire la suite >
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.< Réduire
Origine
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