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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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Outcomes and duration of tidal evolution in a star-planet-moon system
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Dynamics of quadruple systems composed of two binaries: stars, white dwarfs, and implications for Ia supernovae
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A Lunar L2 Navigation, Communication, and Gravity Mission
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Lissajous and Halo Orbits in the Restricted Three-Body Problem
TL;DR: The analytical values obtained after a second order resonant perturbation theory are in very good agreement (in some cases up to the fourth decimal digit) with the numerical values found in the literature.