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Updated: Jun 28, 2025

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Published on: February 21, 2017
Carbonate-Metal Reactions in the Lower Mantle
Anne H Davis1, Bethany A Chidester2, Eran Greenberg3
1Department of the Geophysical Sciences, The University of Chicago, 5734 S. Ellis Avenue, Chicago, Illinois 60637, United States.
In the lower mantle, carbonates remain stable despite reactions with metals. High pressure increases the temperature required for these reactions, making carbonates the primary carbon phase in Earth's deep interior.
Area of Science:
- Geochemistry
- Mineral Physics
- High-Pressure Science
Background:
- Carbonates are crucial carbon reservoirs in the Earth's mantle.
- Their behavior in the lower mantle, particularly phase relations and transport properties, is poorly understood.
- Understanding carbonate stability is key to comprehending deep carbon cycles.
Purpose of the Study:
- To investigate the stability of carbonates under lower mantle conditions.
- To determine the reaction products between carbonates and iron alloys at high pressures and temperatures.
- To assess the role of carbonates as carbon-bearing phases in the deep Earth.
Main Methods:
- High-pressure, high-temperature experimental studies were conducted on the Fe-Si-Ca-Mg-C-O system.
- Experiments reached pressures up to 124 GPa and temperatures up to 3200 K.
- Analysis of reaction products to determine phase stability.
Main Results:
- Carbonates react with iron alloys to form silicates, iron carbides, and oxides.
- The reaction temperature increases with pressure, shifting stability fields.
- Carbon exhibits lower siderophilicity than silicon at high pressures.
Conclusions:
- Along a geotherm, carbonates are the stable carbon-bearing phase in the lowermost mantle.
- These findings impact models of deep carbon cycling and mantle composition.
- Carbonate stability is pressure-dependent, influencing carbon's fate in the deep Earth.
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