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Solar system dynamics
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In this paper, the two-body problem and the restricted three body problem are considered. And the disturbing function is extended to include the spin-orbit coupling and the resonance perturbations.Abstract:
Preface 1 Structure of the solar system 2 The two-body problem 3 The restricted three-body problem 4 Tides, rotation and shape 5 Spin-orbit coupling 6 The disturbing function 7 Secular perturbations 8 Resonant perturbations 9 Chaos and long-term evolution 10 Planetary rings Appendix A Solar system data Appendix B Expansion of the disturbing function Indexread more
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The effect of close-in giant planets' evolution on tidal-induced migration of exomoons
TL;DR: In this paper, the authors put together numerical models of exomoon tidal-induced orbital evolution, results of planetary evolution and interior structure models, to study the final fate of exomorphs around evolving close-in gas giants.
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Instability zones for satellites of asteroids: The example of the (87) Sylvia system
Julien Frouard,Audrey Compère +1 more
TL;DR: In this article, the stability of the (87) Sylvia system and of the neighborhood of its two satellites is investigated using numerical integrations considering the non-sphericity of Sylvia, as well as the mutual perturbation of the satellites and the solar perturbations.
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Transforming Dust to Planets
TL;DR: In this article, the authors review recent progress in understanding how nebular dust and gas are converted into the planets of the present-day solar system, focusing particularly on the "Grand Tack" and pebble accretion scenarios.
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A semi-analytical model for secular dynamics of test particles in hierarchical triple systems
TL;DR: In this article, a semi-analytical model is formulated up to an arbitrary order in the semimajor axis ratio of the inner and outer binaries to describe the long-term (secular) dynamics of test particles in hierarchical triple systems.
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Secular behavior of exoplanets: self-consistency and comparisons with the planet-planet scattering hypothesis
Miles L. Timpe,Miles L. Timpe,Rory Barnes,Rory Barnes,R. Kopparapu,R. Kopparapu,Sean N. Raymond,Richard Greenberg,Noel Gorelick +8 more
TL;DR: In this article, the authors examined the apsidal behavior of known multi-planet systems by doubling the sample size and including observational uncertainties, and showed that the most likely planetary mass function prior to planet-planet scattering follows a power law with index -1.1.