Year: 2026
Type: article
Abstract: ABSTRACT Magma generation and transport govern planetary evolution. Although oxygen is the most abundant anion in Earth’s silicate interior, its role in magma is conventionally ignored, with magma oxygen contents assumed to be simply fixed by cation stoichiometry. Here we show, using high-pressure and high-temperature experiments supported by molecular dynamics simulations, that silicate magma can incorporate substantially more oxygen than permitted by traditional valence-state constraints. Excess oxygen acts as a previously unrecognized volatile component, increasing in concentration from near zero at 1 atm to > ∼5 wt.% above 5 GPa, more than five times the maximum oxygen increase attainable in Earth’s solid mantle through iron redox changes. As oxygen-rich magmas ascend and decompress, their capacity to retain excess oxygen decreases, driving the release of O2. This behaviour provides a direct mechanism with the potential to link mantle melting to oxidation of Earth’s shallow interior and atmosphere, and identifies magma as a dynamic reservoir in planetary oxygen cycles.
Source: National Science Review
DOI: 10.1093/nsr/nwag539
Institutions: Center for High Pressure Science and Technology Advanced Research, Center for High Pressure Science & Technology Advanced Research, Northwestern Polytechnical University, State Key Laboratory of Solidification Processing, Vrije Universiteit Amsterdam, Shanghai Advanced Research in Physical Sciences
Language: English
Subfield: Geophysics
Field: Earth and Planetary Sciences
Domain: Physical Sciences
Open Access status: gold
Estimated APC paid: $2,000
OpenAlex ID: W7204156154
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