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GEOPHYSICAL RESEARCH LETTERS,
VOL. 33,
L24301,
doi:10.1029/2006GL028130,
2006
Retrograde mica in deep crustal granulites: Implications for crustal seismic anisotropy
K. Mahan
Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California, USA
Abstract
The primary contributor to seismic anisotropy in deep continental crust is commonly thought to be crystallographically preferred
orientation of anisotropic mica and amphibole. The abundance of these hydrous phases is very sensitive to temperature, pressure,
and fluid content. Consequently, the thermodynamic stability of these phases provides important information with which to
interpret seismic anisotropy in crustal studies. An example is given of the evolution of anhydrous, mica-absent, lower crustal
felsic granulite to a mica-rich (20–40% mode) tectonite during exhumation along a crustal-scale shear zone, which should significantly
influence the potential seismic anisotropy of the structure. This phenomenon may occur in the Himalayan orogen where a seismically
anisotropic layer has been recently interpreted as the Main Himalayan Thrust. The apparent southward strengthening of anisotropy
along the thrust may be due to an increase in mica content as rocks in the mid-crustal channel are hydrated and cool through
the granulite-amphibolite transition.
Received 15
September
2006;
accepted 14
November
2006;
published 16
December
2006.
Keywords: anisotropy;
lower crust;
shear zones;
mica;
granulites.
Index Terms: 7205 Seismology: Continental crust (1219); 8159 Tectonophysics: Rheology: crust and lithosphere (8031); 3660 Mineralogy and Petrology: Metamorphic petrology; 8012 Structural Geology: High strain deformation zones; 8045 Structural Geology: Role of fluids.
Read Full Article (file size: 332169 bytes) Cited by
Citation: Mahan, K.
(2006),
Retrograde mica in deep crustal granulites: Implications for crustal seismic anisotropy,
Geophys. Res. Lett.,
33,
L24301,
doi:10.1029/2006GL028130.
Copyright 2006 by the American Geophysical Union.
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