Evolution of eccentricity and orbital inclination of migrating planets in 2:1 mean motion resonance

We determine, analytically and numerically, the conditions needed for a system of two migrating planets trapped in a 2:1 mean motion resonance to enter an inclination-type resonance. We provide an expression for the asymptotic equilibrium value that the eccentricity $e_{\rm i}$ of the inner planet r...

সম্পূর্ণ বিবরণ

গ্রন্থ-পঞ্জীর বিবরন
প্রধান লেখক: Teyssandier, J, Terquem, C
বিন্যাস: Journal article
ভাষা:English
প্রকাশিত: Oxford University Press 2014