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Solar system dynamics

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TLDR
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 Index

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On the Flux of Extrasolar Dust in Earth’s Atmosphere

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Some orbital characteristics of lunar artificial satellites

TL;DR: In this paper, an analytical theory with numerical simulations to study the orbital motion of lunar artificial satellites is presented, considering the problem of an artificial satellite perturbed by the non-uniform distribution of mass of the Moon and by a third body in elliptical orbit (Earth is considered).
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Quasi-satellite orbits in the general context of dynamics in the 1:1 mean motion resonance: perturbative treatment

TL;DR: In this paper, the authors investigated the properties of the quasi-satellite regimes in the context of the spatial restricted circular three-body problem "Sun-planet-asteroid" and constructed evolutionary equations which describe the long-term behaviour of the orbital elements of an asteroid.
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Three-body capture of irregular satellites: Application to Jupiter

TL;DR: In this article, the authors investigate a new theory of the origin of the irregular satellites of the giant planets: capture of one member of a ∼100-km binary asteroid after tidal disruption.
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On quasi-periodic motions around the triangular libration points of the real Earth–Moon system

TL;DR: In this article, the problem of finding a dynamical substitute for the two triangular libration points of the real Earth-Moon system is revisited and the linearized central flow around it is described.
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Trending Questions (1)
What are the values of the mass parameters µ for the 11 subsystems of the Solar System?

The values of the mass parameters µ for the 11 subsystems of the Solar System are not provided in the given information.