DI005-0023
Water-induced Diamond Formation at the Earth’s Core-Mantle Boundary

Wednesday, 9 December 2020
Poster
Byeongkwan Ko1, Stella Chariton2, Vitali B Prakapenka2, Bin Chen3, Shule Yu1, Edward Garnero4, Mingming Li5 and Sang-Heon Dan Shim1, (1)Arizona State University, Tempe, AZ, United States, (2)University of Chicago, Center for Advanced Radiation Sources, Chicago, IL, United States, (3)University of Hawaii at Manoa, Hawaii Institute of Geophysics and Planetology, Honolulu, HI, United States, (4)Arizona State Univ, Tempe, AZ, United States, (5)Arizona State University, School of Earth and Space Exploration, Tempe, AZ, United States
Abstract:
A recent seismic study reported thin layered structures with unusually high shear wave velocities at the core-mantle boundary (CMB) beneath Central America and Caribbean (Yu et al., in review). The ultra-high velocity zones (UHVZs) are characterized by a shear velocity increase up to 18% relative to PREM. Among a few possibilities, a diamond-bearing structure can account for such high Vs of UHVZs because of the exceptionally higher Vs of diamond (~13 km/s at the CMB) than the main minerals of the mantle. Previous experiments showed that paraffin reacts with metallic iron and form FeHx and diamond at 58-66 GPa and 3220-3710 K, suggesting that hydrogen can limit the carbon solubility in metallic iron (Hirose et al., 2019). However, whether diamond can form directly from the iron-carbon alloy at the CMB conditions has never been studied. We report experimental results of Fe3C + H2O reaction in the laser-heated diamond anvil cells (LHDACs) combined with the in-situ X-ray diffraction at 120 GPa and 3000-4000 K. We observed diffraction lines of diamond, together with pyrite-type FeOOH and fcc-FeHx. The X-ray diffraction analysis suggests the reaction of Fe3C + yH2O -> y/2FeOOH + (3-y/2)FeHx + C. The newly discovered UHVZs may be explained by a diamond-bearing structure that forms and accumulates in some regions at the CMB where water is supplied by subducted materials. Furthermore, this reaction could be a mechanism for carbon loss from the outer core into the mantle over a significant part of Earth’s history (e.g., due to deep subduction).