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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Introduction: The Evolved Workplace,e show that the generic occurrence of rings for the case of rotating short-range potentials can be extended to the case of gravitational potentials. The consecutive collision periodic orbits created by saddle-center bifurcations are of central importance.

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Origins of the Congress of WestphaliaThe problem of three bodies when one of them is a gyrostat is considered. Using the symmetries of the system we carry out two reductions. Global considerations about the conditions for relative equilibria are made. Finally, we restrict to an approximated model of the dynamics and a complete study of the relative equilibria is made.

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Introduction: The Evolved Workplace,Rotational motion of a rigid satellite moving in a circular orbit around an oblate planet is considered. For a case of a symmetric satellite, we prove non-integrability of equations of motion applying Morales-Ramis extension of Ziglin theory.

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Range-Of-Motion

Non-Integrability of a Certain Problem of Rotational Motion of a Rigid SatelliteRotational motion of a rigid satellite moving in a circular orbit around an oblate planet is considered. For a case of a symmetric satellite, we prove non-integrability of equations of motion applying Morales-Ramis extension of Ziglin theory.

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Teresa Gómez Reus,Terry Gifford inside the orbit of Jupiter and vice versa. During this transition, the comet can be captured temporarily by Jupiter for one to several orbits around Jupiter. The interior heliocentric orbit is typically close to the 3:2 resonance while the exterior heliocentric orbit is near the 2:3 resonance. An

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