Titlebook: Dynamics of Comets: Their Origin and Evolution; Proceedings of the 8 Andrea Carusi,Giovanni B. Valsecchi Conference proceedings 1985 Spring

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https://doi.org/10.1007/978-981-19-2141-4e evolution of meteor streams. It is clear that they evolve principally due to the effect of planetary perturbations and radiation pressure. The formation of streams from the breakup of a comet is also discussed. All the evidence, including the recent, discovery of 1983TB points to the correctness o

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We Piano Teachers and Our Demonsing problems: characteristics of cometary activity at large heliocentric distance and uniqueness of comet P/Schwassmann-Wachmann 1 with respect to physical properties, the r?le of Trojans and other small bodies in the outer planetary system concerning comet/asteroid classification, possibilities for

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We Piano Teachers and Our Demonss debris are responsible for both physical and dynamical changes in objects orbiting about Saturn. Physical changes include cratering of large bodies and catastrophic disruption of small bodies. Dynamical changes, which are analyzed in this paper, include orbital alteration (principally of ring part

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