Fluid dynamics of planetary differentiation

The basic structure of the terrestrial planets—an iron-rich metallic core surrounded by a silicate mantle—was established during their accretion, when widespread melting allowed the metal and silicate phases to separate. The transfer of chemical elements and heat between the metal and silicate that...

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Bibliographic Details
Main Authors: Deguen, Renaud, Huguet, Ludovic, Landeau, Maylis, Lherm, Victor, Maller, Augustin, Wacheul, Jean-Baptiste
Format: Article
Language:English
Published: Académie des sciences 2025-01-01
Series:Comptes Rendus. Physique
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Online Access:https://comptes-rendus.academie-sciences.fr/physique/articles/10.5802/crphys.227/
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