Abstract
The mantle X-discontinuity, usually assigned to positive seismic velocity reflectors in the 260-330km 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 300km 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 1300ppm variation of H2O content in MgSiO3 can displace the transition of low-pressure clinoenstatite (LPCen) to HPCen by up to 2GPa, similar to previous quench experiments on the OEn to HPCen phase transition, where about 30-45km (1.0-1.5GPa) of deflection could occur per 0.1wt% 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.
| Original language | English |
|---|---|
| Pages (from-to) | 234-244 |
| Number of pages | 11 |
| Journal | Physics of the Earth and Planetary Interiors |
| Volume | 183 |
| Issue number | 1-2 |
| DOIs | |
| State | Published - Nov 2010 |
Keywords
- Clinoenstatite
- Enstatite
- MgSiO
- Water
- X-discontinuity
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