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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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Spin–orbit resonance, transit duration variation and possible secular perturbations in KOI‐13
Gy. M. Szabó,Gy. M. Szabó,András Pál,András Pál,Aliz Derekas,A. E. Simon,A. E. Simon,Tamás Szalai,László L. Kiss,László L. Kiss +9 more
TL;DR: In this paper, the authors analyzed publicly available Kepler Q2-Q3 short-cadence observations, revealing a continuous light variation with a period of Prot = 25.43 ± 0.05 h and a half-amplitude of 21 ppm, which is linked to stellar rotation.
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Survey of Kozai dynamics beyond Neptune
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Stability limits for the quasi-satellite orbit
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Dynamical stability of imaged planetary systems in formation: application to hl tau
TL;DR: In this article, the authors consider the hypothesis that these gaps are carved by planets, and present a general framework for understanding the dynamical stability of such systems over typical disk lifetimes, providing estimates for the maximum planetary masses.