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Reactions and physical conditions during metamorphism of Liassic aluminous black shales and marls in central Switzerland

^a The Morton K. Blaustein, Department of Earth and Planetary Sciences, The Johns Hopkins University, Baltimore, Maryland 21218 USA
^b Institute of Mineralogy and Petrography, Bernoullistrasse 30, CH-4056 Basel, Switzerland
^c Institut für Mineralogie und Petrographie, ETH-Zentrum, Sonneggstrasse 5, CH-8082, Zürich, Switzerland

¹ e-mail: klivi{at}jhu.edu

² Deceased

This paper was presented at the "Mica 2000" meeting in Rome, Italy (November 2000)

The aluminous Liassic (lower Jurassic) shales, slates, and marls of the Central Swiss Alps were investigated by electron microprobe (EMP) and scanning electron microscopy (SEM) to determine the physical conditions of low grade metamorphism. The samples investigated experienced metamorphism from the diagenetic (100°C) to the epizonal grade (450°C). Temperatures estimated from Fe-Mg exchange equilibria between chlorite and chloritoid agree with calcite-dolomite geother-mometry and previous workers' estimates. In the upper anchizone, calcite-dolomite temperatures record peak temperatures ca. 330°C. Epizone rocks in the Urseren Zone record ca. 400–450°C. Calculations of T-X phase equilibria in the CaO-MgO-FeO-Al₂O₃-SiO₂-H₂O-CO₂-CH₄ system with excess quartz and graphite were used to predict the stability fields of aluminous minerals and coexisting fluid compositions. The assemblage Sud + Dol + Qtz + Gr is stable over a temperature interval of 300–360°C. Calculations predict that, in CO₂-bearing fluids, reactions that form the index minerals margarite, sudoite, and chloritoid predominantly involve carbonate minerals. Margarite is not predicted to form in fluids dominated by CH₄. Temperatures recorded by T-X phase equilibria in the anchizone (330°C) agree well with calcite-dolomite thermometry. Temperatures recorded by T-X phase equilibria in the epizone (330–360°C) are significantly lower than calcite-dolomite temperatures (400–480°C).

The calculated fluid composition in the anchizone is CO₂-rich (y_CO2 = CO₂/(CO₂ + H₂O) = 0.2), whereas the epizone fluids are richer in H₂O (y_CO2 = 0.02–0.06). Fluid-flux calculations based on phase equilibria and reaction progress indicate that there was significant fluid infiltration in both the anchizone and epizone. The anchizone samples recorded a flux of ca. 6 x 10³ cm³ fluid/cm² rock with a flux increase to at least 2 x 10⁵ cm³/cm² in the epizone. These values are comparable to calculated fluxes during Devonian regional metamorphism in New England. Results show that careful mineral analysis can yield data appropriate for the estimation of sub-greenschist facies metamorphic conditions in aluminous low-grade rocks.

Key-words: Low-grade metamorphism, phase equilibria, aluminous shale, fluid infiltration.

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