Skip to content
Licensed Unlicensed Requires Authentication Published by De Gruyter March 31, 2015

Thermal diffusivity of olivine-group minerals at high temperature

  • Maik Pertermann EMAIL logo and Anne M. Hofmeister
From the journal American Mineralogist

Abstract

Thermal diffusivity (D) data from 12 oriented single crystals and seven polycrystalline samples of olivine group minerals were acquired with the laser-fl ash method at temperatures (T) of up to ~1500 °C. Samples included forsterite, Fe-Mg binary olivines, sinhalite, and chrysoberyl; specimens were characterized using infrared spectroscopy and electron microprobe analysis. Crystal orientation and chemistry both affect D. For our single crystals, D[100] > D[001] > D[010] at all temperatures. Thermal diffusivity decreases with increasing T and becomes virtually constant at high temperatures. At room temperature, D[001] of pure forsterite has the highest observed values, but substitution of a small amount of Co in forsterite (0.3 wt% CoO) lowers D by ~20%. Substitution of ~10% Fe for Mg in forsterite, as in typical mantle olivine, lowers D by ~50%. At room temperature, mantle olivine has D = 3.25, 1.66, and 2.59 mm2/s for the [100], [010], and [001] orientations, respectively. The values decrease to 0.93-0.87 mm2/s at 790-985 °C for [100], 0.54-51 mm2/s at 590-740 °C for [010] and 0.83-0.79 mm2/s at 740-890 °C for [001]. Two dunite samples have D of 0.55-0.56 mm2/s at 890-1080 °C, showing the effect of preferred orientation of grains dominated by [010]. Thermal diffusivity of polycrystalline samples is controlled by the large amounts of olivine present; minor phases offset the curves for D(T) from the value of the olivine mineral. Our laser-fl ash measurements isolate the phonon component of heat transfer from radiative transfer and show that the phonon contribution becomes nearly constant for the high temperatures expected in the mantle. The other microscopic component (diffusive radiative transfer) depends strongly on temperature and this temperature dependence likely exerts greater control on mantle convection.

Received: 2005-9-27
Accepted: 2006-6-17
Published Online: 2015-3-31
Published in Print: 2006-11-1

© 2015 by Walter de Gruyter Berlin/Boston

Downloaded on 26.4.2024 from https://www.degruyter.com/document/doi/10.2138/am.2006.2105/html
Scroll to top button