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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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Relativistic effects in extrasolar planetary systems
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Enceladus's crust as a non-uniform thin shell: II tidal dissipation
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Eccentricity generation in hierarchical triple systems with coplanar and initially circular orbits
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A numerical investigation of coorbital stability and libration in three dimensions
M. H. M. Morais,Fathi Namouni +1 more
TL;DR: In this article, the authors examined the similarities and differences between planar and three dimensional coorbital resonance capture and seek their origin in the stability of coorbits motion at arbitrary inclination.
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Dynamics of planetesimals due to gas drag from an eccentric precessing disc
TL;DR: In this article, the dynamics of individual kilometre-size planetesimals in circumstellar orbits of a tight binary system were analyzed, including both the gravitational perturbations of the secondary star and a non-linear gas drag stemming from an eccentric gas disc with a finite precession rate.