Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
4742172 | Physics of the Earth and Planetary Interiors | 2010 | 11 Pages |
Abstract
The mantle X-discontinuity, usually assigned to positive seismic velocity reflectors in the 260-330Â km depth range, has proved difficult to explain in terms of a single mineralogical phase transformation in part because of its depth variability. The coesite to stishovite transition of SiO2 matches deeper X-discontinuity depths but requires 5-10% free silica in the mantle to match observed impedance contrast. The orthoenstatite (OEn) to high-pressure clinoenstatite (HPCen) transformation of MgSiO3 also broadly coincides with depths of the X but requires chemically depleted and orthoenstatite-rich lithology at 300Â km depth in order to match observed seismic impedance contrast. On the basis of high-pressure infrared spectroscopy, X-ray diffraction, and Raman spectroscopy, we show that 1300Â ppm variation of H2O content in MgSiO3 can displace the transition of low-pressure clinoenstatite (LPCen) to HPCen by up to 2Â GPa, similar to previous quench experiments on the OEn to HPCen phase transition, where about 30-45Â km (1.0-1.5Â GPa) of deflection could occur per 0.1Â wt% H2O. If the mantle X-discontinuity results from pyroxene transitions in a depleted harzburgite layer, because of the strong influence of minor amounts of water on the transformation boundary, the depth of the mantle X-discontinuity could serve as a potentially sensitive indicator of water content in the upper mantle.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
Steven D. Jacobsen, Zhenxian Liu, Tiziana Boffa Ballaran, Elizabeth F. Littlefield, Lars Ehm, Russell J. Hemley,