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Abstract
Large Low Shear Velocity Provinces (LLSVPs) in the lowermost mantle are key to understanding the chemical composition and thermal structure of the deep Earth, but their origins have long been debated. Bridgmanite, the most abundant lower-mantle mineral, can incorporate extensive amounts of iron (Fe) with effects on various geophysical properties. Here our high-pressure experiments and ab initio calculations reveal that a ferric-iron-rich bridgmanite coexists with an Fe-poor bridgmanite in the 90 mol% MgSiO3–10 mol% Fe2O3 system, rather than forming a homogeneous single phase. The Fe3+-rich bridgmanite has substantially lower velocities and a higher VP/VS ratio than MgSiO3 bridgmanite under lowermost-mantle conditions. Our modeling shows that the enrichment of Fe3+-rich bridgmanite in a pyrolitic composition can explain the observed features of the LLSVPs. The presence of Fe3+-rich materials within LLSVPs may have profound effects on the deep reservoirs of redox-sensitive elements and their isotopes.
Dense Fe3+-rich bridgmanite can explain the seismic features of Large Low Shear Velocity Provinces, as it can form large-scale thermochemical piles in the deep mantle that remain stable throughout Earth’s history.
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1 University of Science and Technology of China, Laboratory of Seismology and Physics of Earth’s Interior, School of Earth and Space Sciences, Hefei, China (GRID:grid.59053.3a) (ISNI:0000000121679639); University College London, Department of Earth Sciences, London, UK (GRID:grid.83440.3b) (ISNI:0000000121901201)
2 Michigan State University, Department of Earth and Environmental Sciences, East Lansing, USA (GRID:grid.17088.36) (ISNI:0000 0001 2150 1785)
3 University of Michigan, Department of Earth and Environmental Sciences, Ann Arbor, USA (GRID:grid.214458.e) (ISNI:0000000086837370)
4 Arizona State University, School of Earth and Space Exploration, Tempe, USA (GRID:grid.215654.1) (ISNI:0000 0001 2151 2636)
5 University of Science and Technology of China, Laboratory of Seismology and Physics of Earth’s Interior, School of Earth and Space Sciences, Hefei, China (GRID:grid.59053.3a) (ISNI:0000000121679639); University of Science and Technology of China, National Geophysical Observatory at Mengcheng, Hefei, China (GRID:grid.59053.3a) (ISNI:0000000121679639); CAS Center for Excellence in Comparative Planetology, USTC, Hefei, China (GRID:grid.59053.3a) (ISNI:0000000121679639)