Capture into first-order resonances and long-term stability of pairs of equal-mass planets

DOI10.1007/S10569-018-9848-2zbMath1447.70028arXiv1808.08059OpenAlexW3098928970WikidataQ112116057 ScholiaQ112116057MaRDI QIDQ1785900

Aurélien Crida, Gabriele Pichierri, Alessandro Morbidelli

Publication date: 2 October 2018

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1808.08059

zbMATH Keywords

stabilityexoplanetsplanet formationsemi-analyticalmean motion resonancesN-body simulations

Mathematics Subject Classification ID

Orbital mechanics (70M20)

Related Items (2)

An integrable model for first-order three-planet mean motion resonances ⋮ Normal forms for the Laplace resonance

Cites Work

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• The main mean motion commensurabilities in the planar circular and elliptic problem
• On the co-orbital motion in the planar restricted three-body problem: the quasi-satellite motion revisited
• Resonant periodic motion and the stability of extrasolar planetary systems
• Stationary orbits in resonant extrasolar planetary systems
• Motion of two planets with periods commensurable in the ratio 2?1 solutions of the hori auxiliary system
• Solar System Dynamics

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