Article ID Journal Published Year Pages File Type
4678681 Earth and Planetary Science Letters 2010 11 Pages PDF
Abstract

Grain growth kinetics of forsterite (Fo) and enstatite (En) in fine grain aggregates of Fo ± En are examined as a function of volume fraction of En (fEn = 0.00 to 0.42). Growth rates fit dn∝ k · t (d: mean grain diameter; n: grain growth exponent; k: growth constant; t: time), where n ∼ 5 for both forsterite and enstatite grains in the enstatite-bearing samples. A negative correlation between kFo and fEn can be expressed as kFo ≈ 0.06 exp [30 fEn (fEn − 1.1)], whereas kEn takes almost constant values for different fEn. In addition, the ratio of dFo/dEn is almost constant during grain growth, and its value becomes smaller with increasing fEn, such that dFo/dEn ≈ 0.74/fEn0.59. Our obtained grain growth parameters and the microstructural characteristics in experimental and natural samples all indicate that the rate-controlling process for grain growth in both experiments and in nature is grain boundary diffusion of Si through grain boundaries of olivine. Thus, we are able to propose a semi-empirical relationship of dAve/ddun≈{exp[30fpx⋅(fpx−1.1)]}15⋅(1+1.35fpx1.59−fpx) (dAve: average grain size in the rock; ddun: average grain size in dunite; fpx: fraction of pyroxenes), which can predict how lithology affects grain size in the upper mantle. Grain size in lherzolite (pyroxenes content of 40%) can be ∼ 4 times smaller than that in dunite (pyroxenes content of 5%). Such grain size reduction through change in lithology can significantly affect viscosity of mantle deformation via grain-size sensitive creep.

Related Topics
Physical Sciences and Engineering Earth and Planetary Sciences Earth and Planetary Sciences (General)
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