Dynamics of Jupiter Trojans during the 2:1 mean motion resonance crossing of Jupiter and Saturn
F. Marzari (Dept. of Physics, Univ. of Padova, Italy), H. Scholl (Obs., de la Cote d'Azur, Nice, France)
TL;DR
This paper investigates how Jupiter Trojans' orbits evolved during the early Solar system as Jupiter and Saturn crossed the 2:1 mean motion resonance, affecting their stability and distribution.
Contribution
It provides new insights into the dynamical behavior of Jupiter Trojans during planetary migration and resonance crossing events.
Findings
Jupiter Trojans experienced significant orbital changes during resonance crossing.
The stability of Trojans was affected by planetary migration patterns.
Resonance crossing played a key role in shaping Trojan populations.
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.
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