Precipitation of pyroxenes and Mg2SiO4 from majoritic garnet: simulation of peridotite exhumation from great depth |
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Authors: | Larissa F. Dobrzhinetskaya Harry W. Green II Alex P. Renfro Krassimir N. Bozhilov Dirk Spengler Herman L. M. van Roermund |
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Affiliation: | Department of Earth Sciences, University of California at Riverside, CA 92521, USA;;Institute of Geophysics and Planetary Physics, University of California at Riverside, CA 92521, USA;;Utrecht University, Faculty of Earth Sciences, Utrecht, The Netherlands |
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Abstract: | Our experimental simulations of the exhumation path of mantle peridotites show that high‐temperature (1400 °C) decompression of lherzolite from 14 to 13 and 12 GPa results in exsolution of interstitial blebs of diopside and Mg2SiO4 (wadsleyite) lamellae from majoritic garnet. At lower pressures (from 8 to 5 GPa, at T = 1400 °C) only enstatite exsolves as blebs at garnet boundaries. Continuous high‐temperature decompression from 14 to 7 GPa produces zoned majoritic garnet containing blebs of exsolved pyroxenes inside garnet rims. No intracrystalline precipitation of pyroxene was observed in garnet, although such lamellae are found in some natural garnet peridotites. The explanation appears to be the three orders of magnitude difference in grain size between experimental and natural specimens. Our data suggest that Mg2SiO4 and diopside exsolutions reflect the deepest point of the exhumation path of garnet peridotites, whereas enstatite precipitation may be restricted to garnets with less majoritic component at shallower depths. |
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