The solubility of TiO2 in olivine:: implications for the mantle wedge environment

被引:20
作者
Dobrzhinetskaya, L [1 ]
Bozhilov, KN
Green, HW
机构
[1] Univ Calif Riverside, Inst Geophys & Planetary Phys, Riverside, CA 92521 USA
[2] Univ Calif Riverside, Dept Earth Sci, Riverside, CA 92521 USA
基金
美国国家科学基金会;
关键词
olivine; titanium solubility; mantle wedge; deep subduction;
D O I
10.1016/S0009-2541(99)00107-2
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
One characteristic of many subduction-zone garnet peridotites is that they contain titanium-bearing phases not otherwise found in mantle rocks. In particular, titanoclinohumite and/or its breakdown assemblage consisting of symplectic intergrowths of olivine and ilmenite is common in many of these bodies. The Alpe Arami garnet Iherzolite of the Swiss Alps, while lacking titanoclinohumite, displays instead large numbers of FeTiO3 rod-shaped precipitates in the oldest generation of olivine, amounting to approximately 1% by volume, indicating that at some time in its past, the peridotite experienced conditions under which the solubility of TiO2 in olivine was > 0.6 wt.%. In order to test the hypothesis that the environment of very high solubility of TiO2 in olivine is to be found at very high pressures, we have conducted experiments on Iherzolite 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 TiO2 was not detected in olivine at 5 GPa, 1400 K where it coexists with rutile, when rutile disappeared from the paragenesis, the solubility climbed to 0.4 wt.% at 8 GPa, 0.5 wt.% at 10 GPa and to > 1.0 wt.% at 12 GPa, 1700 K. These results support our previous interpretations from titanate morphology and abundance that the Ape Arami massif has surfaced from P = 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. (C) 1999 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:357 / 370
页数:14
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