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• W1130652511 abstract "Planetary interiors are massive heat engines. The heat accumulated during planetary formation and released by the slowly decaying radioactive isotopes present in rocks is transported from the mantle and core out to the surface by thermal diffusion and convection, which ultimately cause planets to cool over geological timescales. Volcanism, plate tectonics (or the lack thereof), the formation of the landforms that shape planetary surfaces and crusts, and the generation of internal magnetic fields in the liquid core, all involve physical processes that crucially depend on the modes of heat transfer at depth. In this chapter, we describe the fundamental mechanisms that control the thermal and chemical evolution of the mantle of terrestrial bodies starting from their formation, which shortly postdates the birth of the solar system, until present. We illustrate how the study of rocks at the extreme temperatures and pressures of deep mantles, combined with observational constraints on the composition, geology, and magnetization of the surface provides a framework upon which theoretical models of global-scale heat transport can be built. These models represent today an invaluable tool to characterize the numerous and complex processes that govern the dynamics and the evolution of planetary interiors." @default.
• W1130652511 created "2016-06-24" @default.
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• W1130652511 date "2014-01-01" @default.
• W1130652511 modified "2023-09-26" @default.
• W1130652511 title "Evolution of Planetary Interiors" @default.
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• W1130652511 doi "https://doi.org/10.1016/b978-0-12-415845-0.00009-8" @default.
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