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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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Origin and Evolution of the Cometary Reservoirs
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Viscous hydrodynamics simulations of circumbinary accretion discs: variability, quasi-steady state and angular momentum transfer
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Effects of thermal radiation on the dynamics of binary NEAs
Matija Ćuk,Joseph A. Burns +1 more
TL;DR: In this article, the authors explore the Yarkovsky force on a non-spherical body, called the YORP effect, which can modify the orbit of a synchronously rotating secondary in a binary system.
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Measurement of the Spin-Orbit Misalignment of KOI-13.01 from its Gravity-Darkened Kepler Transit Lightcurve
TL;DR: In this paper, the asymmetry of the KOI-13.01 transit lightcurve was modeled assuming a gravity-darkened rapidly rotating host star in order to constrain the system's spin-orbit alignment and transit parameters.