Diffusion of a multi-species component and its role in oxygen and water transport in silicates
- Creators
- Zhang, Youxue
- Stolper, E. M.
- Wasserburg, G. J.
Abstract
An important but poorly understood factor that affects diffusion rates is the role of speciation during diffusion of a multi-species component. The diffusion of such a component is complicated by the different diffusion coefficient of each species and the interconversion reactions among the species. These complexities can be treated by a diffusion equation that incorporates the diffusive fluxes of all species contributing to the concentration of the component. The effects of speciation on the diffusion of the component can be investigated experimentally in some simple cases by measuring concentration profiles of all species developed during diffusion experiments or by studying some of their other consequences. Experimental data on water diffusion in rhyolitic glasses indicate that although dissolved water is present as two species. H_2O molecules and OH groups, molecular H_2O is the dominant diffusing species at very low to high water concentrations. This explains the apparently complex behavior of water diffusion. Experimental data on oxygen diffusion in some silicates using ^(18)O tracers in the form of H_(2)^(18)O are consistent with the idea that ^(18)O transport is dominated by diffusion of H_2O molecules even at lower water contents (ppm or less). This explains why oxygen transport depends on the presence of water and generally depends on water fugacity linearly. For this mode of oxygen transport, there is a simple theoretical relationship between the effective total oxygen diffusion coefficient and the total water diffusion coefficient that is a function of only the water concentration of the silicate at low water content. This relationship appears to describe quantitatively the existing data over a wide range in water contents and diffusion coefficients in several phases.
Additional Information
© 1991 Elsevier Science Publishers B.V. Received 18 June 1990. Accepted 31 October 1990. We thank Professors M.S. Peterson, G.R. Rossman, H.P. Taylor for helpful discussions, Professor C.E. Langmuir for editorial handling, and three anonymous reviewers. Contribution 4939 of Division of Geological and Planetary Sciences, Caltech. This work was supported through grants from the National Aeronautics and Space Administration (NAGW-1472 to E.M.S.), the National Science Foundation (EAR-8916707 to E.M.S.) and the Department of Energy (DE-FG03-88ER13851 to G.J.W.).Additional details
- Eprint ID
- 33378
- Resolver ID
- CaltechAUTHORS:20120820-161958837
- NASA
- NAGW-1472
- NSF
- EAR-891707
- Department of Energy (DOE)
- DE-FG03-88ER13851
- Created
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2012-08-21Created from EPrint's datestamp field
- Updated
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2021-11-09Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences
- Other Numbering System Name
- Caltech Division of Geological and Planetary Sciences
- Other Numbering System Identifier
- 4939