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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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Journal ArticleDOI
Binary asteroid population. 2. Anisotropic distribution of orbit poles of small, inner main-belt binaries
Petr Pravec,P. Scheirich,David Vokrouhlický,A. W. Harris,Peter Kusnirak,Kamil Hornoch,D. P. Pray,David Higgins,Adrian Galad,Jozef Vilagi,Štefan Gajdoš,Leonard Kornoš,Julian Oey,Marek Husárik,Walter R. Cooney,John Gross,Dirk Terrell,R. Durkee,J. Pollock,Daniel E. Reichart,K. M. Ivarsen,J. B. Haislip,Aaron P. LaCluyze,Yu. N. Krugly,N. Gaftonyuk,Robert D. Stephens,R. Dyvig,Vishnu Reddy,Vasilij G. Chiorny,Ovidiu Vaduvescu,P. Longa-Peña,P. Longa-Peña,A. Tudorica,A. Tudorica,Brian D. Warner,Gianluca Masi,James W. Brinsfield,Rui Soles Gonçalves,Peter Brown,Z. Krzeminski,O. Gerashchenko,Vasilij G. Shevchenko,Igor Molotov,Franck Marchis,Franck Marchis +44 more
TL;DR: In this paper, it was shown that the binary orbit poles oriented preferentially up/down-right are due to either of the two processes: (i) the YORP tilt of spin axes of their parent bodies toward the asymptotic states near obliquities 0° and 180° (pre-formation mechanism) or (ii) the tilt of the primary components of the already formed binary systems toward the same positions near the asyclic states near the same position.
Journal ArticleDOI
Pumping the eccentricity of exoplanets by tidal effect
TL;DR: In this paper, it was shown that when the orbit of the planet is excited by an outer companion, tidal effects combined with gravitational interactions may give rise to a secular increasing drift on the eccentricity.
Book ChapterDOI
Observations, Modeling and Theory of Debris Disks
TL;DR: The recent growth in interest in debris disks has been driven by observational work that has provided statistics, resolved images, detection of gas in the debris disks, and discoveries of new classes of objects as discussed by the authors.
Journal ArticleDOI
Tidal Evolution of the Spin-Orbit Angle in Exoplanetary Systems
Yuxin Xue,Yasushi Suto,Yasushi Suto,Atsushi Taruya,Atsushi Taruya,Teruyuki Hirano,Teruyuki Hirano,Yuka Fujii,Yuka Fujii,Kento Masuda +9 more
TL;DR: In this paper, a simple system comprising a Sun-like star and a hot Jupiter adopting the equilibrium tide and the inertial wave dissipation effects simultaneously is examined, and it is shown that the combined tidal model works as a very efficient realignment mechanism; it predicts three distinct states of the spin-orbit angle (i.e., parallel, polar, and antiparallel orbits) for a while, but the latter two states eventually approach the parallel spinorbit configuration.
Journal ArticleDOI
Stability criteria for hierarchical triple systems
TL;DR: A summary of stability criteria for hierarchical triple systems over the past few decades is given in this article, where the authors discuss the criteria that are based on the generalisation of the concept of zero velocity surfaces of the restricted three body problem, to the general case.