4.4 Article

Variations in the transient prograde geothermal gradient from chloritoid-staurolite equilibria: a case study from the Barrovian and Buchan-type domains in the Bohemian Massif

Journal

JOURNAL OF METAMORPHIC GEOLOGY
Volume 25, Issue 1, Pages 19-35

Publisher

WILEY
DOI: 10.1111/j.1525-1314.2006.00674.x

Keywords

Barrovian and Buchan metamorphism; Bohemian Massif; chloritoid-staurolite; prograde geotherm; pseudosection

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Thermodynamic modelling of metamorphic rocks increases the possibilities of deciphering prograde paths that provide important insights into early orogenic evolution. It is shown that the chloritoid-staurolite transition is not only an indicator of temperature on prograde P-T paths, but also a useful indicator of pressure. The approach is applied to the Moravo-Silesian eastern external belt of the Bohemian Massif, where metamorphic zones range from biotite to staurolite-sillimanite. In the staurolite zone, inclusions of chloritoid occur in garnet cores, while staurolite is included at garnet rims and is widespread in the matrix. Chloritoid X-Fe = 0.91 indicates transition to staurolite at 5 kbar and 550 degrees C and consequently, an early transient prograde geothermal gradient of 29 degrees C km(-1). The overall elevated thermal evolution is then reflected in the prograde transition of staurolite to sillimanite and in the achievement of peak temperature of 660 degrees C at a relatively low pressure of 6.5 kbar. To the south and to the west of the studied area, high-grade metamorphic zones record a prograde path evolution from staurolite to kyanite and development of sillimanite on decompression. Transition of chloritoid to staurolite was reported in two places, with chloritoid X-Fe = 0.75-0.80, occurring at 8-10 kbar and 560-580 degrees C, and indicating a transient prograde geothermal gradient of 16-18 degrees C km(-1). These data show variable barric evolutions along strike and across the Moravo-Silesian domain. Elevated prograde geothermal gradient coincides with areas of Devonian sedimentation and volcanism, and syn- to late Carboniferous intrusions. Therefore, we interpret it as a result of heat inherited from Devonian rifting, further fuelled by syntectonic Carboniferous intrusions.

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