The composition of Earth’s core is a fundamental property of the Earth’s deep interior, defining its present structure and long term thermal and magnetic evolution. However, the composition of the core is not well understood, with several combinations of light elements being able to satisfy the traditional constraints from cosmochemistry, core formation and seismology. The classic view of inner core formation does not include the necessity for liquids to be supercooled to below their melting point before freezing. Attempts to calculate the magnitude of this supercooling have found that several binary core compositions are incompatible with inner core nucleation. Here we show, through molecular dynamics simulations, that nucleation from an Fe1−xCx=0.1-0.15 composition is compatible with a range of geophysical constraints. Whilst not a complete description of core chemistry, our results demonstrate that inner core nucleation places a strong constraint on the composition of Earth’s core that may allow discrimination between previously identified potential compositions. The composition of Earth’s inner core can be constrained by the supercooling required for its formation. Based on molecular dynamic simulations this work shows that inner core nucleation from an iron-carbon composition fits geophysical constraints.
Constraining Earth’s core composition from inner core nucleation
A. Wilson,Christopher J Davies,Andrew M Walker,Dario Alfè
Published 2025 in Nature Communications
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- Publication year
2025
- Venue
Nature Communications
- Publication date
2025-09-04
- Fields of study
Medicine, Physics, Geology
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- Source metadata
Semantic Scholar, PubMed
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