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The stability of the solar system and of small stellar systems

Author: Yoshihide Kozai; International Astronomical Union. Commission 7.
Publisher: Dordrecht ; Boston : D. Reidel Pub. Co., [1974]
Series: Copernicus Symposium, 1.; International Astronomical Union.; Symposium
Edition/Format:   Print book : English
Summary:

Proceedings of IAU Symposium No. 62 held in Warsaw, Poland, September 5-8, 1973

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Genre/Form: Conference papers and proceedings
Congresses
Document Type: Book
All Authors / Contributors: Yoshihide Kozai; International Astronomical Union. Commission 7.
ISBN: 9027704589 9789027704580 9027704597 9789027704597
OCLC Number: 1328817
Notes: At head of title: International Astronomical Union. Union astronomique internationale.
"Sponsored by Commission 7 (Celestial Mechanics) and cosponsored by Commissions 4 (Ephemerides) and 37 (Star Clusters and Associations) of the IAU and by IUTAM."
Description: vi, 313 pages : illustrations ; 25 cm.
Contents: Stability Theory in Celestial Mechanics.- Modern Dynamical Systems Theory.- The Present State of the n-Body Problem.- Bode's Law.- Distribution of the Mean Motions of Planets and Satellites and the Development of the Solar System.- Can the Solar System be Quantized?.- On the Original Distribution of the Asteroids.- The Origin of Commensurabilities in the Satellite Systems.- The Origin of the Asteroid Ring.- Orbits of Trojan Asteroids.- The Role of Saturn's Oblateness in the Mimas-Tethys Resonance.- Stability of Asteroidal Motion in the Hecuba Gap.- Secular Perturbations for Asteroids Belonging to Families.- The Formation of Disks by Inelastic Collisions of Gravitating Particles. Applications to the Dynamics of the Saturn's Ring and to the Formation of the Solar System.- Stationary Solutions of the Averaged Three-Body Problem and Some Problems of Planet Motion Stability.- Integrable Cases of Satellite Problem with the Third Body and the Oblate Planet.- The Global Solution in the Problem of the Critical Inclination.- Retrograde Satellites in the Circular Plane Restricted Three-Body Problem.- A Note on a Separation of Equations of Variation of the Elliptic Restricted Three-Body Problem into Hill's Equations.- Comet Schwassmann-Wachmann 3 (1930 VI).- The Motion of Comet Westphal in 1852-1974.- The Motion of Comet Encke-Backlund over 1901-1970.- An Iterative Method of General Planetary Theory.- On the Calculation of Secular Perturbations in the Case of Close Commensurability.- Long Period Terms in the Solar System.- On the Theory of the Galilean Satellites of Jupiter.- Conditions for Escape and Retention.- Influence of the Dynamical Figure of the Moon on Its Rotational-Translational Motion.- A Comparison of the Mean-Value and Initial-Value Solutions of the Ideal Resonance Problem with an Application in Rigid-Body Mechanics.- Statistics of Three-Body Experiments.- The Role of Binaries in Cluster Dynamics.- On the Stability of Small Clusters or Cluster Remnants.- The Dynamical Evolution of Trapezium Systems.- The Stability of Triple Stellar Systems.- Sur un invariant integral du probleme des n corps: Consequence de l'homogeneite du potential.- Numerical Experiments on Expanding Gravitational Systems.- Numerical Experiments on the Stability of Spherical Stellar Systems.- On the `Thermodynamics' of Self-Gravitating N-Body Systems.- Dynamics and Clusters of Galaxies.- Dynamical Friction Effects on the Motion of Stars in Rotating Spherical Clusters.- On the Disappearance of Isolating Integrals in Dynamical Systems with More than Two Degrees of Freedom.
Series Title: Copernicus Symposium, 1.; International Astronomical Union.; Symposium
Responsibility: edited by Y. Kozai.

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