Titlebook: Solar and Extra-Solar Planetary Systems; Lectures Held at the Iwan P. Williams,Nicolas Thomas Book 2001 Springer-Verlag Berlin Heidelberg 2

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Meteors, Meteor Showers and Meteoroid Streams,y are came somewhat later with a true understanding of meteor showers being no more than 150 or so years old. The recognition of the processes involved in the formation of a stream is even younger, starting only in the early fifties. Here, we wish to review our current state of knowledge and describ

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0075-8450 rest in the physics and evolution dynamics of solar systems. The present book has grown out of a set of lectures by leading experts in the field within the framework of the well-known EADN summer schools. It addresses primarily graduate students and young researchers but will be equally useful for s

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The Giant Planets,ositions, and their cloud structures. The abundance ratios of the giant planets, inferred from their spectral properties, are reviewed, and the implications of these parameters in terms of formation and evolution models are discussed.

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The Formation of Planets, of a protoplanetary nebula into a disk and the subsequent accretion of planets from planetesimals within this disk. The last section presents the formation and the evolution of planetary atmospheres within this formation scenatio.

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Dynamics of the Solar System,ion. Newtonian gravitation also permits chaotic motion. The properties of chaotic systems are examined together with applications to the long-term dynamical evolution of objects in the solar system. Planetary ring systems are used to illustrate particular aspects of the nature of resonant phenomena in the solar system.

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Physical Processes Associated with Planetary Satellites,te them with examples from throughout the Solar System. In particular, satellite sphericity, cratering, resurfacing, the effects of surface frosts, the presence of tenuous atmospheres, and satellites as sources of heavy ions in planetary magnetospheres are discussed.

放弃

Meteors, Meteor Showers and Meteoroid Streams,d in the formation of a stream is even younger, starting only in the early fifties. Here, we wish to review our current state of knowledge and describe the physics involved in the formation and evolution.

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Book 2001ework of the well-known EADN summer schools. It addresses primarily graduate students and young researchers but will be equally useful for scientists in search of a comprehensive tutorial account that goes beyond the material found in standard textbooks.

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