Dynamics of Jupiter Trojans during the 2:1 mean motion resonance crossing of Jupiter and Saturn

Abstract

We study the dynamics of Jupiter Trojans in the early phase of the Solar system while the outer planets migrated due to their interaction with the planetesimal disk.

arXiv comment10 pages, 17 figures

References in corpus (4)

• Evolution of Planetary Systems in Resonance
• On the origin of the Trojan asteroids: Effects of Jupiter's mass accretion and radial migration
• The Capture of Centaurs as Trojans
• Survival of Trojan-Type Companions of Neptune During Primordial Planet Migration

Cited by in corpus (6)

• Preliminary Results from NEOWISE: An Enhancement to the Wide-field Infrared Survey Explorer for Solar System Science
• The resonant structure of Jupiter's trojan asteroids-II. What happens for different configurations of the planetary system
• Albedos of Small Jovian Trojans
• A Peculiar Family of Jupiter Trojans: the Eurybates
• Secondary resonances and the boundary of effective stability of Trojan motions
• The Stability of Uranus Trojans Over the Age of the Solar System