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Titlebook: Solar System Ices; Based on Reviews Pre B. Schmitt,C. Bergh,M. Festou Book 19981st edition Kluwer Academic Publishers 1998 Planet.Planetary

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Amorphous Water Icee timescale of the solar system, due to activation energy barriers that prevent restructuring from one form into another. In this regime of temperature (T < 220 K) and pressure (P < 0.2 GPa), there is no thermodynamic equilibrium. All structural transitions are time dependent and irreversible.
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UV Photochemistry of Ices which solar system ices are exposed (photon irradiation and charged particle bombardement) are taken into account as well as the variation of these processes with the type of object considered (planet, satellite, comet, rings.) and its environment. An attempt is made in each case to assess the rela
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Origin and Evolution of Comets, Icy Planets and Satellitesysical processes that, starting from the dust particles present in the primitive solar nebula, can lead to the formation of the primary icy objects. We see how these objects can form and explain the present distribution and dynamical characteristics of the comets and icy planets. We examine the form
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