Evolution of olivine lattice preferred orientation during simple shear in the mantle
Evolution of olivine lattice preferred orientation during simple shear in the mantle
Date
2008-04-03
Authors
Warren, Jessica M.
Hirth, Greg
Kelemen, Peter B.
Hirth, Greg
Kelemen, Peter B.
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Abstract
Understanding the variation of olivine lattice preferred orientation (LPO) as a function of shear
strain is important for models that relate seismic anisotropy to the kinematics of deformation. We
present results on the evolution of olivine orientation as a function of shear strain in samples from
a shear zone in the Josephine Peridotite (southwest Oregon). We find that the LPO in harzburgites
re-orients from a pre-existing LPO outside the shear zone to a new LPO with the olivine [100] maximum aligned sub-parallel to the shear direction between 168% and 258% shear strain. The strain
at which [100] aligns with the shear plane is slightly higher than that observed in experimental
samples, which do not have an initial LPO. While our observations broadly agree with the experimental observations, our results suggest that a pre-existing LPO influences the strain necessary
for LPO alignment with the shear direction. In addition, olivine re-alignment appears to be dominated by slip on both (010)[100] and (001)[100], due to the orientation of the pre-existing LPO.
Fabric strengths, quantified using both the J- and M- indices, do not increase with increasing shear
strain. Unlike experimental observations, our natural samples do not have a secondary LPO peak.
The lack of a secondary peak suggests that subgrain rotation recrystallization dominates over grain
boundary migration during fabric re-alignment. Harzburgites exhibit girdle patterns among [010]
and [001] axes, while a dunite has point maxima. Combined with the observation that harzburgites
are finer grained than dunites, we speculate that additional phases (i.e., pyroxenes) limit olivine
grain growth and promote grain boundary sliding. Grain boundary sliding may relax the requirement for slip on the hardest olivine system, enhancing activation of the two easiest olivine slip
systems, resulting in the [010] and [001] girdle patterns. Overall, our results provide an improved
framework for calibration of LPO evolution models.
Description
Author Posting. © Elsevier B.V., 2008. This is the author's version of the work. It is posted here by permission of Elsevier B.V. for personal use, not for redistribution. The definitive version was published in Earth and Planetary Science Letters 272 (2008): 501-512, doi:10.1016/j.epsl.2008.03.063.