Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
9522678 | Earth and Planetary Science Letters | 2005 | 15 Pages |
Abstract
Antigorite dehydration has been studied in situ using time-resolved X-ray diffraction (XRD) in the 1.1-5.5 GPa pressure range. The sequence of XRD spectra reveals that the high-temperature stability limit of antigorite is decreased by 50-100 °C under H2O-unsaturated conditions. The decomposition of antigorite into the high-temperature products, forsterite + enstatite, proceeds via an intermediate assemblage of forsterite and a “talc-like” phase, observed within a temperature interval of 130 ± 20 °C. The analysis of the transformation-time data using the Avrami model suggests that the breakdown of antigorite and the “talc-like” phase is kinetically controlled by surface growth processes at the edges of grains. The overall transformation rates are 10 to 100 times faster than those observed in water-saturated experiments, and show that the H2O activity is a strong driving force for dehydration. The breakdown of antigorite in subducting oceanic mantle with such kinetics would result in a fluid discharge rate of the order of 10â 6 to 10â 8 sâ 1. This is faster than the viscous relaxation of serpentinites, and could lead to brittle failure or weakening of pre-existing faults. This provides an explanation for the seismicity in the lower plane of double seismic zones.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Earth and Planetary Sciences (General)
Authors
Jean-Philippe Perrillat, Isabelle Daniel, Kenneth T. Koga, Bruno Reynard, Hervé Cardon, Wilson A. Crichton,