Titanium-rich phases in the Earth's transition zone and lower mantle: Evidence from experiments in the system MgO-SiO2-TiO2(±Al2O3) at 10-24 GPa and 1600 °C

Phase relations in the MgSiO3-MgTiO3 and Mg3Al2Si3O12-MgTiO3 systems were studied at 10-24 GPa and1600 °C using a high-pressure Kawai-type multianvil apparatus. We investigated the full range of starting compositions for the enstatite-geikielite system to derive a P-X phase diagram and synthesize titanium-bearingphases, such as olivine/wadsleyite, rutile, pyroxene, MgTiSi2O7 weberite, bridgmanite and MST-bridgmanite ina wide pressure range. Olivine and pyroxene in run products are characterized by a low titanium content (b0.6and b0.3 wt% TiO2, respectively) whereas the content of TiO2 in wadsleyite reaches 2 wt% at 12 GPa. The concentration of Ti in MgTiSi2O7 weberite decreases with pressure from 52 wt% TiO2 at 14 GPa to 43 wt% TiO2 at 18 GPa.Two perovskite-type structures (MgSiO3 bridgmanite and Mg(Si,Ti)O3 bridgmanite) were detected in the studiedsystem. MgSiO3 bridgmanite (Brd) is formed at a pressure of N20 GPa and characterized by significant titaniumsolubility (up to 13 wt% TiO2 at 24 GPa). Mg(Si,Ti)O3 perovskite is formed at a pressure of N17 GPa. The concentration of TiO2 in this phase varies from 29 wt% to 49 wt%. It was found that addition of Ti to the system moves theboundaries of Ol/Wad phase transformations to lower pressures. Addition of Al to the starting material allows usto simulate the composition of natural Ti-rich garnets and bridgmanites. It is important to note that garnet in thePrp-Gkl system is stable throughout a wide pressure range (10-24 GPa). Al incorporation does not affect the distribution of titanium between two types of bridgmanite. It is shown that high contents of Ti stabilizebridgmanite-like compounds at considerably lower pressure than that at the lower mantle/transition zoneboundary. Our experiments simulate the composition of natural Ti-rich primary garnet found in eclogite fromthe Sulu ultrahigh-pressure (UHP) terrane.