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Titlebook: Dynamics and Evolution of Minor Bodies with Galactic and Geological Implications; Proceedings of the C S. V. M. Clube,S. Yabushita,J. Henra

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A Model Of The Galactic Tidal Interaction With The Oort Comet Cloud, was inside 15 AU we assume that planetary perturbations would have removed the comet from the . energy distribution accessible by the galactic tide. Comets which had their perihelia changed from beyond 15 AU to within 5 AU in a single orbit are taken to be observable. We are able to track the evolu
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Origin Of Oort Cloud Comets In The Interstellar Space,ditional Oort Cloud (Oort, 1950) could be captured from the interstellar medium. However, we note that the so called Kuiper belt (Kuiper, 1951) of comets cannot arise through this process. Therefore we have to ask how necessary the concept of the yet unobserved Kuiper belt is for the theory of short
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Collective Resonant Phenomena On Small Bodies In The Solar System,tion. Numerical results obtained in an other context show that the competition between the Poynting-Robertson drag and the gravitational interaction of grains near the 2/1 resonance might be very important in the long run for the structure of meteor streams.
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