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" Interactions Between Physics and Dynamics of Solar System Bodies : "
edited by E. Bois, P. Oberti, J. Henrard.
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BL
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775742
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b595738
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| Main Entry
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edited by E. Bois, P. Oberti, J. Henrard.
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| Title & Author
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Interactions Between Physics and Dynamics of Solar System Bodies : : Proceedings of the International Astronomical Symposium held in Pléneuf-Val-André (France) from June 21 to June 28, 1992\ edited by E. Bois, P. Oberti, J. Henrard.
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| Publication Statement
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Dordrecht : Springer Netherlands, 1993
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(410 pages)
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| ISBN
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9401119023
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: 9789401119023
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| Contents
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Modelling the outcomes of high-velocity impacts between small solar system bodies --; A comparison between 2D and 3D wavelet analysis method for asteroid family dynamical study --; Asteroid "clans": super-families or multiple events? --; Catastrophic fragmentation and formation of families: preliminary results from a new numerical model --; Structure of the asteroid belt for small members --; The Trojan asteroid belt: Proper elements, stability, chaos and families --; Long term evolution of asteroids near a resonance --; The stability of the planetary three-body problem: influence of the secular resonances --; The main mean motion commensurabilities in the planar circular and elliptic problem --; Stochasticity of two comets in resonance with Jupiter --; Orbital evolution of giant comet-like objects --; On a temporary confinement of chaotic orbits of four dimensional symplectic mapping: a test on the validity of the synthetic approach --; A simple mapping for comets in resonance --; Geopotential from space techniques --; Luni-solar effects of geosynchronous orbits at the critical inclination --; Long-periodic variations of the motion of a satellite due to non-resonant tesseral harmonics of a gravity potential --; On the roto-translatory motion of a satellite of an oblate primary --; Canonical elements and Keplerian-like solutions for intermediary orbits of satellites of an oblate planet --; Albedo perturbation models: general formalism and applications to LAGEOS --; Study of a Moon's artificial satellite dynamics valid for all eccentricities and inclinations --; On the fluid and viscoelastic deformations of the planets --; On the tidal variation of the geopotential --; Orbital, rotational and climate interactions --; Lunar and terrestrial tidal effects on the Moon's rotational motion --; Passing through resonance: the excitation and dissipation of the Lunar free libration in longitude --; Stability of the synchronous spin-orbit resonance by construction of librational trapping tori --; Nebular drag and capture into spin-orbit resonance --; Significant high number commensurabilities in the main Lunar problem II: The occurence of Saros-like near periodicities --; Motion of the orbital plane of a satellite due to a secular change of the obliquity of its mother planet --; Fourier analysis of local Lyapunov characteristic exponents for satellite-type motions --; Capture of grains into resonances through Poynting-Robertson drag --; The gravitational influence of satellite Pan on the radial distribution of ring-particles in the region of the Encke-division in Saturn's A ring --; Collisional evolution of the asteroid size distribution: a numerical simulation --; Resonant and secular phenomena in the libration of the Moon --; Precise orbit determination with a short-arc technique --; Spherical coordinates perturbations for small eccentricity orbits --; Dynamical friction induces perturbations on Oort cloud comets --; Poynting-Robertson effects --; Influence of internal load on the non-hydrostatic form of the Moon --; Evolution of asteroidal orbits with high inclinations.
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| Abstract
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This book contains the proceedings of an International Astronomical Symposium devoted to the interactions between physics and dynamics in the solar system, especially with regard to the small bodies (asteroids, comets, meteors). These two topics were traditionally considered as almost independent, but their interactions are increasingly being reviewed as the key to an understanding of the formation and evolution of the solar system. For instance, the rotational dynamics of planets have a profound influence on their climate. On the other hand, a good understanding of the complicated dynamics of asteroids and the identification of families of bodies born from the break-up of a parent body may tell us much about the formation and the evolution of the solar system. All these, and several related questions are discussed in these proceedings, which will be of interest to both physicists and dynamicists. <br/>
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Asteroids -- Congresses.
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Celestial mechanics -- Congresses.
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Comets -- Congresses.
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| Added Entry
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E Bois
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J Henrard
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P Oberti
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| Parallel Title
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Proceedings of the International Astronomical Symposium held in Pléneuf-Val-André (France) from June 21--28, 1992
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