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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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Orbital evolution of the Gefion and Adeona asteroid families: close encounters with massive asteroids and the Yarkovsky effect
TL;DR: In this article, the authors investigated the effect of close encounters on two families, Gefion and Adeona, that have high encounter probabilities with 1 Ceres, by far the largest asteroid in the main belt.
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Predicting Planets in Known Extrasolar Planetary Systems. I. Test Particle Simulations
Rory Barnes,Sean N. Raymond +1 more
TL;DR: In this article, the authors examined the known planetary systems by placing massless test particles in between the planets and integrating for 1-10 million years and found that some systems, such as HD 168443 and HD 74156, eject nearly all test particles within 2 million years.
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Formation and evolution of planetary systems in presence of highly inclined stellar perturbers
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The interior structure of Mercury and its core sulfur content
TL;DR: In this paper, depth-dependent interior structure models of Mercury are calculated for several plausible chemical compositions of the core and of the mantle, and the expected precision on the moment of inertia is estimated to a precision of about 50 km.
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Spiral structure when setting up pericentre glow : possible giant planets at hundreds of AU in the HD 141569 disk
TL;DR: In this paper, the impact of introducing a planet on an eccentric orbit into a dynamically cold planetesimal disk is discussed, where the surface density distribution of an extended disk exhibits two spirals, one exterior the other interior to the planet's orbit.