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
Trapping and dynamical evolution of interplanetary dust particles in Earth’s quasi-satellite resonance
TL;DR: In this paper, the authors used numerical simulations to model the orbital evolution of interplanetary dust particles (IDPs) evolving inward past Earth's orbit under the influence of radiation pressure, Poynting-Robertson light drag (PR drag), solar wind drag, and gravitational perturbations from the planets.
Journal ArticleDOI
Tides alone cannot explain Kepler planets close to 2:1 MMR
Ari Silburt,Hanno Rein +1 more
TL;DR: In this paper, an optimistic theoretical estimate on the minimum initial eccentricity required by Kepler planets to explain the current observed spacing, and N-body simulations were used to investigate 27 Kepler systems having planets within 6% of the 2:1 MMR.
Journal ArticleDOI
On the stability of the satellites of asteroid 87 Sylvia
Othon C. Winter,L. A. G. Boldrin,E. Vieira Neto,R. Vieira Martins,S. M. Giuliatti Winter,Rodney S. Gomes,F. Marchis,Pascal Descamps +7 more
TL;DR: In this article, the authors studied the stability of the satellites Romulus and Remus in the triple asteroidal system (87) and found that even just 0.1 per cent of this value is enough to keep the satellite's orbital elements with no significant variation.
Journal ArticleDOI
Equilibria in the secular, non-co-planar two-planet problem
TL;DR: In this paper, the authors investigated the dynamics of a planetary system composed of the parent star and two massive planets in mutually inclined orbits, in a wide range of semimajor axes ratios (0.1-0.667), as well as in the whole permitted ranges of energy and total angular momentum.
Journal ArticleDOI
Planets and asteroids in the γ Cephei system
P. E. Verrier,Nick Evans +1 more
TL;DR: The binary star system y Cephei is unusual in that it harbours a stable giant planet around the larger star at a distance only about a tenth of that of the stellar separation as discussed by the authors.