The effect of melt infiltration on metagranitic rocks: the Snieznik dome, Bohemian Massif

0505819 - GFÚ 2020 RIV GB eng J - Článek v odborném periodiku
Štípská, P. - Hasalová, P. - Powell, R. - Závada, Prokop - Schulmann, K. - Racek, M. - Aguilar, C. - Chopin, F.
The effect of melt infiltration on metagranitic rocks: the Snieznik dome, Bohemian Massif.
Journal of Petrology. Roč. 60, č. 3 (2019), s. 591-618. ISSN 0022-3530. E-ISSN 1460-2415
Institucionální podpora: RVO:67985530
Klíčová slova: orthogneiss migmatite * fluid-assisted melting * eclogite facies * melt percolation * exhumation
Obor OECD: Geology
Impakt faktor: 3.451, rok: 2019
Způsob publikování: Open access
https://academic.oup.com/petrology/article/60/3/591/5307756

Highly deformed banded phengite-biotite metagranite from the Snieznik dome in the Bohemian Massif has been modified locally to have stromatic, schlieren or nebulitic textures typical of migmatites. This occurred mostly along subvertical deformation zones at eclogite-facies conditions, at a scale of several centimetres to several metres, mostly parallel to the foliation. The transition from banded to migmatite types of orthogneiss is marked by an increase in the amount of phases interstitial along grain boundaries in the dynamically recrystallized monomineralic feldspar and quartz aggregates, and by increasing consumption of recrystallized K-feldspar grains by fine-grained plagioclase and quartz, as well as myrmekite (intergrowth of Pl-Qz). The new minerals are in textural equilibrium with phengite. The myrmekite, quartz and feldspars can be coarse-grained (grain size 05cm). These features are considered to be the result of grain-scale melt infiltration that caused dissolution-reprecipitation along grain boundaries in the presence of phengite. The infiltration was pervasive at the grain scale, but localized at hand-specimen to outcrop scales. All the rock types have the same mineral assemblage of Grt-Ph-Bt-Ttn-Kfs-Pl-Qz +/- Rt +/- Ilm. They have similar garnet, phengite and biotite compositions, and based on mineral equilibria modelling we infer equilibration at a pressure of 15-17GPa and a temperature of 690-740 degrees C. Because the rocks are inferred to be H2O-undersaturated and above the temperature conditions of the wet solidus, infiltration must have involved a hydrous melt, as opposed to an H2O fluid. Stability of melt-bearing mineral assemblages and mineral compositions are almost independent of the melt proportion in the system, thus explaining the identical assemblage and mineral compositions observed in all the migmatite types. This precludes the estimation of the amount of melt infiltrated.
Trvalý link: http://hdl.handle.net/11104/0297192