Open AccessBook
Solar system dynamics
Reads0
Chats0
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 Indexread more
Citations
More filters
Journal ArticleDOI
Aggregate impacts in Saturn's rings
TL;DR: Barbara et al. as mentioned in this paper studied how collisions between aggregates can lead to destruction or coalescence of these aggregates, with local N -body simulations taking into account the dissipative impacts and gravitational forces between particles.
Journal ArticleDOI
How Special Is the Solar System
TL;DR: In this article, the authors compare the solar system to the many recently discovered exoplanetary systems, and identify two main features that appear to distinguish it from the majority of other systems: (i) the lack of super-Earths, and (ii) the absence of close-in planets.
Journal ArticleDOI
Recent orbital evolution and the internal structures of Enceladus and Dione
Ke Zhang,Francis Nimmo +1 more
TL;DR: In this article, the authors studied the orbital behavior of Enceladus and Dione during their passage through the 2:1 mean-motion resonances to constrain their interior structures, parameterized by the quantity k 2 / Q (assumed constant).
Journal ArticleDOI
Stability of Binary Asteroids
TL;DR: In this paper, the stability and final outcome of a strongly interacting binary asteroid system are considered and the effects of energy dissipation on an asteroid binary system are also considered and are shown to change the stability of the system against escape and impact.
Journal ArticleDOI
Tidal interactions of close-in extrasolar planets: The OGLE cases
TL;DR: In this article, the average and maximum value of the range of dissipation are equivalent to the linear and quadratic dissipation models of Sasselov (2003) for OGLE-TR-56 b.