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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Main Authors: | , , , , , |
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Format: | Article |
Language: | English |
Published: |
Académie des sciences
2025-01-01
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Series: | Comptes Rendus. Physique |
Subjects: | |
Online Access: | https://comptes-rendus.academie-sciences.fr/physique/articles/10.5802/crphys.227/ |
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