The solubility of TiO in olivine: implications for the mantle

One characteristic of many subduction zone garnet peridotites is that they contain titanium-bearing phases not otherwise Ž . found in mantle rocks. In particular, titanoclinohumite TiCH andror its breakdown assemblage consisting of symplectic intergrowths of olivine and ilmenite is common in many of these bodies. The Alpe Arami garnet lherzolite of the Lepontine Alps, while lacking TiCH, displays instead large numbers of FeTiO rod-shaped precipitates in the oldest generation of 3 olivine, amounting to approximately 1% by volume, indicating that at some time in its past, the peridotite experienced conditions under which the solubility of TiO in olivine was greater than 0.6 wt.%. In order to test the hypothesis that the 2 environment of very high solubility of TiO in olivine is to be found at very high pressures, we have conducted experiments 2 on lherzolite compositions with added ilmenite at pressures between 5 and 12 GPa and temperatures of 1350–1700 K. Our results on anhydrous compositions show that, whereas solubility of TiO was not detected in olivine at 5 GPa, 1400 K where 2 it coexists with rutile, when rutile disappeared from the paragenesis, the solubility climbed to 0.5 wt.% at 8 and 10 GPa, and to 1 wt.% at 12 GPa, all at 1600 K. These results support our previous interpretations from titanate morphology and Ž . abundance that the Alpe Arami massif has surfaced from depths )300 km corresponding to pressures )10 GPa but remove the need to suggest a deeper origin and possible precursor phase such as wadsleyite. They also support the hypothesis that garnet peridotites with unusual Ti-bearing phases reflect a unique mantle environment occurring in the mantle wedge overlying subduction zones. q 2000 Elsevier Science B.V. All rights reserved.