Affiliation:
1. Department of Earth, Marine and Environmental Sciences University of North Carolina Chapel Hill NC USA
2. Sorbonne Université CNRS‐INSU Institut des Sciences de La Terre de Paris ISTeP UMR 7193 Paris France
3. Department of Earth Science University of California, Santa Barbara Santa Barbara CA USA
Abstract
AbstractMeter‐ to hectometer‐size horizons of carbonate‐bearing talcschists are found along or near the contacts between the different Liguro‐Piemont subduction slices. Through mineral and bulk‐rock geochemistry, fluid inclusion analyses, and titanite U‐Pb geochronology, this study shows that these horizons formed by the transformation of serpentinites, at conditions close to peak burial, due to fluid infiltration sourced from surrounding sediments. These rocks containing large amounts of carbonates and high concentrations of fluid‐mobile elements may be significant for carbon cycling and contribute to the composition of arc magmas once the main constitutive assemblage destabilizes at high‐pressure and high‐temperature conditions. Following fluid infiltration, the formation of talc likely controlled strain localization in these horizons, enhancing in turn the ingression of external fluids and creating a positive feedback loop between deformation and fluid infiltration. We suggest that these rocks may have acted as major rheological weaknesses responsible for material offscraping from the downgoing plate.
Publisher
American Geophysical Union (AGU)
Subject
Geochemistry and Petrology,Geophysics
Cited by
9 articles.
订阅此论文施引文献
订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献