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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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Obliquity variations of a moonless Earth
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On the Inclination Distribution of the Jovian Irregular Satellites
TL;DR: In this paper, the authors show that many high-inclination orbits are unstable due to solar and planetary perturbations, by causing particles to strike (or to escape) their planet, considerably broaden this zone of avoidance.
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Star hoppers: planet instability and capture in evolving binary systems
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A transition in circumbinary accretion discs at a binary mass ratio of 1:25
Daniel J. D'Orazio,Zoltan Haiman,Paul C. Duffell,Andrew MacFadyen,Brian D. Farris,Brian D. Farris +5 more
TL;DR: In this article, the authors study circumbinary accretion discs in the framework of the restricted three-body problem (R3Bp) and via numerically solving the height-integrated equations of viscous hydrodynamics.
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Modeling of lightcurves of binary asteroids
P. Scheirich,Petr Pravec +1 more
TL;DR: In this article, a numerical method for inverting long-period components of lightcurves of asynchronous binary asteroids is presented, and the pole solutions and size ratios for 1999 KW4 and 2000 DP107 are in good agreement with independent estimates from radar measurements.