Petrological and geochronological investigations on the individual nappes of the Meran-Mauls nappe stack (Austroalpine unit/South Tyrol, Italy)

Author:

Pomella Hannah1,Costantini Daniel2,Aichholzer Paul1,Reiser Martin3,Schuster Ralf3,Tropper Peter4

Affiliation:

1. Institute of Geology , University of Innsbruck , Innrain 52f , Innsbruck , Austria .

2. Landesamt für Geologie und Baustoffprüfung , Eggentaler Straße 48 - 39053 Kardaun, Autonomous Province of Bozen , Italy .

3. Geologische Bundesanstalt , Neulinggasse 38, 1030 Wien , Austria .

4. Institute of Mineralogy and Petrography , University of Innsbruck , Innrain 52f , Innsbruck , Austria .

Abstract

Abstract The Meran-Mauls nappe stack is part of the Austroalpine unit in South Tyrol (Italy). There it holds a special position directly in front of the Southalpine Dolomites indenter and west of the Tauern Window. It is situated in the hanging wall of the Southalpine unit, above a NW dipping segment of the Periadriatic fault system, namely the Meran-Mauls fault. Also all other sides are defined by Oligocene-Miocene strike-slip and normal faults. Based on recent mapping the Meran-Mauls nappe stack consists of three nappes separated by NW to NNW dipping shear zones. The lowermost nappe in the southwest is represented by the Schenna (Scena) unit. It is overlain along the Masul shear zone by a nappe consisting of the Hirzer (Punta Cervina) unit and the Pens (Pennes) unit including Triassic (meta)sediments. Separated by the Fartleis fault the St. Leonhard (San Leonardo) unit forms the uppermost nappe. The aim of this study is to describe the individual units and the separating structural elements more properly, based on new structural, petrological, geothermobarometric and geochronological data and to compare these units to other Austroalpine elements in the vicinity. Sillimanite-bearing paragneiss, minor amphibolite and quartzite as well as a distinct marble layer close to its base characterise the Schenna unit. Further, it contains pegmatite dikes, presumably Permian in age. Amphibolite-facies P-T conditions of c. 0.55 ± 0.15 GPa and 600 ± 100°C are thus correlated with a Permian metamorphic imprint. The Masul shear zone mostly consists of mylonitic paragneiss of the Hirzer unit. It is pre-Alpine in age and probably formed during the Jurassic. For the paragneiss of the Hirzer unit upper greenschist- to amphibolite-facies metamorphic conditions of 0.4-0.50 ± 0.15 GPa and 550 ± 70°C are attributed to the Variscan tectonometamorphic imprint. The whole Pens unit represents a shear zone. Due to the occurrence of Permotriassic (meta)-sediments within this shear zone, it is an Alpine structure, as well as the bordering Fartleis fault. Rb/Sr biotite ages yield sometimes partly reset pre-Alpine age values in the whole Meran-Mauls nappe stack, indicating a pervasive anchizonal to lowermost greenschist-facies metamorphic overprint during the Eoalpine tectonometamorphic event. Tectonostratigraphically the Meran-Mauls nappe stack can be attributed to the Drauzug-Gurktal nappe system. The latter forms the uppermost structural element of the Austroalpine nappe stack and thus only shows a weak Eoalpine metamorphic overprint. With respect to its special lithologic composition the Schenna unit can be correlated with the Tonale unit in the southwest and the Strieden-Komplex in the east.

Publisher

Austrian Geological Society (OGG)

Subject

General Medicine

Reference86 articles.

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2. AA.VV., online first. Carta Geologica d’Italia alla scala 1:50.000, Foglio 009 Anterselva. Servizio Geologico d’Italia - ISPRA. https://www.isprambiente.gov.it/Media/carg/9_ANTERSELVA/Foglio.html

3. Andreatta, C., 1948. La “Linea di Pejo” nel massiccio dell’Ortles e le sue miloniti. Acta geologica alpina 1, 1-63.

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