Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
11024662 | Geochimica et Cosmochimica Acta | 2018 | 43 Pages |
Abstract
The results show that the apparent diffusivity of total H+ varies both over time and for olivines with different defect populations, and thus H+ does not diffuse at inherently site-specific rates. These variations are due to rapid reactions that may occur between sites as a function of changing defect concentrations. Our experiments reveal three new phenomena: (1) H+ that is associated with the Ti-clinohumite defect, [Ti-2H], can enter and exit olivine at the fastest rate measured. (2) The rate of H+ loss from specific infrared absorption peaks, and in total, may change with progressive dehydration due to the buildup of Fe3+ and redistribution of defects, particularly the rehydration of [Ti-2H]. (3) The following Arrhenius laws appear to apply to total H+ diffusion out of most natural olivines that have been studied experimentally and naturally during dehydration: Daâ¯=â¯10â5.4exp(â130/RT); Dbâ¯=â¯10â6.9exp(â130/RT); and Dcâ¯=â¯10â6.6exp(â130/RT), where R is the gas constant 8.314â¯J/mol K; T is the temperature, the units of the diffusivities (D) are in m2/s; and the activation energy is 130â¯kJ/mol. This rate is slower than proton-polaron redox rate but faster than proton-metal vacancy diffusion and appears to characterize olivine of Foâ¯â¼90 composition in a wide range of conditions, from self-diffusion, to melt inclusion re-equilibration, to mantle xenolith and volcanic phenocryst zonation during ascent.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geochemistry and Petrology
Authors
Elizabeth Ferriss, Terry Plank, Megan Newcombe, David Walker, Erik Hauri,