Abstract
Crystallographic preferred orientations (CPOs) in olivine are widely used to infer the mechanisms, conditions, and kinematics of deformation of mantle rocks. Recent experiments on water-saturated olivine were the first to produce a complex CPO characterised by bimodal orientation distributions of both [100] and [001] axes and inferred to form by combined activity of (001)[100], (100)[001], and (010)[100] slip. This result potentially provides a new microstructural indicator of deformation in the presence of elevated concentrations of intracrystalline hydrous point defects and has implications for the interpretation of seismic anisotropy. Here, we document a previously unexplained natural example of this CPO type in a xenolith from Lesotho and demonstrate that it too may be explained by elevated concentrations of hydrous point defects. We test and confirm the hypothesis that combined (001)[100], (100)[001], and (010)[100] slip were responsible for formation of this CPO by (1) using high-angular resolution electron backscatter diffraction to precisely characterise the dislocation types present in both the experimental and natural samples and (2) employing visco-plastic self-consistent simulations of CPO evolution to assess the ability of these slip systems to generate the observed CPO. Finally, we utilise calculations based on effective-medium theory to predict the anisotropy of seismic wave velocities arising from the CPO of the xenolith. Maxima in S-wave velocities and anisotropy are parallel to both the shear direction and shear plane normal, whereas maxima in P-wave velocities are oblique to both, adding complexity to interpretation of deformation kinematics from seismic anisotropy.
Original language | English (US) |
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Pages (from-to) | 51-61 |
Number of pages | 11 |
Journal | Earth and Planetary Science Letters |
Volume | 508 |
DOIs | |
State | Published - Feb 15 2019 |
Bibliographical note
Funding Information:We thank Graham Pearson and Peter Nixon for providing a sample of xenolith PHN1611 and David Mainprice for discussions its microstructure. D. Wallis, L.N. Hansen, and A.J. Wilkinson acknowledge support from the Natural Environment Research Council Grant NE/M000966/1 . M. Tasaka acknowledges support through a JSPS Research Fellowship for Young Scientists ( 26-4879 ) and the Japan Society for the Promotion of Science ( 16K17832 ). D.L. Kohlstedt acknowledges support through NASA Grant NNX15AL53G . K.M. Kumamoto acknowledges support through NSF Division of Earth Science grants 1255620 and 1625032 . Any opinions, findings, and conclusions or recommendations expressed in this material are those of the authors and do not necessarily reflect the views of NSF.
Keywords
- HR-EBSD
- VPSC
- crystallographic preferred orientation
- dislocation slip system
- olivine
- seismic properties