Metamorphism of Solar System Ices

Metamorphism of Solar System Ices
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太阳系冰的变质作用

DOI：
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发表时间：
1998
期刊：
影响因子：
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通讯作者：
K. Kossacki
K. Kossacki
中科院分区：
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文献类型：
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作者：
J. Eluszkiewicz;J. Leliwa;K. Kossacki

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本章回顾了变质过程中的晶粒生长和致密化，因为它们适用于太阳系冰。这些过程受最小表面能的热力学约束，其动力学方程已被材料科学家广泛研究。这些方程的太阳系冰的应用需要有关的材料参数的知识。本章介绍了压实实验中使用的方程和技术。冰变质解释了对各种太阳系天体的几次观测，并可能在它们的内部演化中发挥了重要作用。
This chapter reviews the metamorphic processes of grain growth and densification as they apply to solar system ices. These processes are driven by the thermodynamic constraint of minimum surface energy and their kinetic equations have been studied extensively by material scientists. The application of these equations to solar system ices requires the knowledge of the relevant material parameters. This chapter presents the equations and describes techniques used in compaction experiments. Ice metamorphism explains several observations about various solar system objects and is likely to have played an important role in their internal evolution.