Warren, C. J.; Smye, A. J.; Kelley, S. P. and Sherlock, S. C.
|DOI (Digital Object Identifier) Link:||https://doi.org/10.1111/j.1525-1314.2011.00956.x|
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New single-grain-fusion muscovite and paragonite 40Ar/39Ar data from eclogite and blueschist units exposed in the Tauern Window, Eastern Alps yield a range of apparent ages from 90 to 23 Ma. These apparent ages are generally older than expected for 40Ar/39Ar cooling ages, given constraints from other geochronological systems such as Rb–Sr and U–Pb. Numerical Ar-in-muscovite diffusion models for Tauern Window nappe P–T paths in an open system suggest that 40Ar/39Ar ages should lie between 29 and 24 Ma, and that they should constrain cooling and decompression following the post-high pressure Barrovian overprint. The measured ranges of apparent 40Ar/39Ar dates suggest that the assumption of open system behaviour is not valid for this region. The local and/or regional generation of fluid during exhumation promoted pervasive recrystallization of high pressure lithologies throughout the Tauern Window to greenschist and amphibolite facies assemblages. The old apparent 40Ar/39Ar white mica dates in all lithologies are therefore interpreted as being due to inefficient removal of grain boundary Ar by the grain boundary fluids during the Barrovian overprint, due to high Ar concentrations or limited connectivity or both. This caused spatially (mm-scale) and temporally variable fluxes of Ar out of, and probably into, white mica in both metasedimentary and metabasic lithologies.
|Item Type:||Journal Article|
|Copyright Holders:||2011 Blackwell Publishing Ltd|
|Keywords:||40Ar/39Ar; Alps; fluid flow; high pressure metamorphism; Tauern Window; white mica|
|Academic Unit/School:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Environment, Earth and Ecosystem Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Clare Warren|
|Date Deposited:||20 Oct 2011 13:42|
|Last Modified:||29 Nov 2016 17:09|
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