Article ID Journal Published Year Pages File Type
4702118 Geochimica et Cosmochimica Acta 2014 12 Pages PDF
Abstract

Diffusion of tungsten has been characterized in synthetic forsterite and natural olivine (Fo90) under dry conditions. The source of diffusant was a mixture of magnesium tungstate and olivine powders. Experiments were prepared by sealing the source material and polished olivine under vacuum in silica glass ampoules with solid buffers to buffer at NNO or IW. Prepared capsules were annealed in 1 atm furnaces for times ranging from 45 min to several weeks, at temperatures from 1050 to 1450 °C. Tungsten distributions in the olivine were profiled by Rutherford Backscattering Spectrometry (RBS).The following Arrhenius relation is obtained for W diffusion in forsterite:DW=1.0×10-8exp(-365±28kJmol-1/RT)m2s-1Diffusivities for the synthetic forsterite and natural Fe-bearing olivine are similar, and tungsten diffusion in olivine shows little dependence on crystallographic orientation or oxygen fugacity.The slow diffusivities measured for W in olivine indicate that Hf–W ages in olivine–metal systems will close to diffusive exchange at higher temperatures than other chronometers commonly used in cosmochronology, and that tungsten isotopic signatures will be less likely to be reset by subsequent thermal events.

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Physical Sciences and Engineering Earth and Planetary Sciences Geochemistry and Petrology
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