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...
Những tác giả chính: | Teyssandier, J, Terquem, C |
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Định dạng: | Journal article |
Ngôn ngữ: | English |
Được phát hành: |
Oxford University Press
2014
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