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• W2035225535 abstract "A considerable fraction of multi-planet systems discovered by the observational surveys of extrasolar planets reside in mild proximity to first-order mean motion resonances. However, the relative remoteness of such systems from nominal resonant period ratios (e.g. 2:1, 3:2, 4:3) has been interpreted as evidence for lack of resonant interactions. Here we show that a slow divergence away from exact commensurability is a natural outcome of dissipative evolution and demonstrate that libration of critical angles can be maintained tens of percent away from nominal resonance. We construct an analytical theory for the long-term dynamical evolution of dissipated resonant planetary pairs and confirm our calculations numerically. Collectively, our results suggest that a significant fraction of the near-commensurate extrasolar planets are in fact resonant and have undergone significant dissipative evolution." @default.
• W2035225535 created "2016-06-24" @default.
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• W2035225535 date "2012-11-20" @default.
• W2035225535 modified "2023-10-09" @default.
• W2035225535 title "DISSIPATIVE DIVERGENCE OF RESONANT ORBITS" @default.
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• W2035225535 doi "https://doi.org/10.1088/0004-6256/145/1/1" @default.
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