Titlebook: Dynamics of Natural and Artificial Celestial Bodies; Proceedings of the U Halina Pretka-Ziomek,Edwin Wnuk,David L. Richardso Conference pro

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Origins of the Congress of Westphaliahe philosophy of the initial integrator, we average the drag terms, but we do not make any expansion in series of eccentricity or inclination. We show our results, especially capture around asymmetric equilibria, and compare them to those found by Beaué and Ferraz-Mello (1993, 1994) and Liou et al. (1979).

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Origins of the Congress of Westphaliag an appropriate fundamental model to each case. Only a part of resonances match known fundamental models. An extended fundamental model is proposed to account for some complicated phenomena. Most of the double resonance cases still remain unexplored.

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Introduction: The Evolved Workplace,plain the relationship that we have found between the values of the Fast Lyapunov Indicator, the order of the periodic orbits and also the minimum number of iterations needed to obtain the Fast Lyapunov Indicator values.

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On the Relationship Between Fast Lyapunov Indicator and Periodic Orbits for Symplectic Mappingsplain the relationship that we have found between the values of the Fast Lyapunov Indicator, the order of the periodic orbits and also the minimum number of iterations needed to obtain the Fast Lyapunov Indicator values.

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ckiewicz University in Poznan, Poland and held in Poznan, from 3 to 7 July 2000. The purpose of the workshop was to identify future research in celestial mech­ anics and encourage collaboration among scientists from eastem and westem coun­ tries. There was a full program of invited and contributed p

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Introduction: The Evolved Workplace, orbits present in some models is of particular interest because it rises, on the one hand, the question of the origin of those chaotic motions and, on the other hand, the question of whether an equilibrium stellar system can be built when the bulk of the stars that make it up behave chaotically.

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Origins of the Congress of Westphaliaing that the stiffness of the ring is large and the dissipation is small enough, we study the quasi-static motion which is set in after free elastic oscillations have damped. In particular, the steady-state motions in the weakly elliptic orbit are found and their stability is investigated.

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