Abstract

The Strona-Ceneri Zone is located south of the Insubric line, where Alpine overprint is mainly brittle and of low grade or even absent. Apart from the unmetamorphic Permo-Carboniferous sediments and intrusiva the Strona-Ceneri Zone is an Ordovician gneiss complex composed of paragneisses, migmatites, peraluminous orthogneisses and banded amphibolites associated with meta-gabbros and meta-ultramafics. Despite of the individual characters of the other Ordovician gneiss terranes north of the Insubric line, most prominently the Aar Massif, the Gotthard, Silvretta and Ötztal nappes, they show analogous lithological formations and pre-Mesozoic structures indicating similar genetic processes. A revision of geological maps and new field observations in these gneiss terranes indicate characteristic spatial relationships of banded amphibolite formations with migmatites and orthogneisses. The contrasting chemistries of the peraluminous rocks (para- and orthogneisses) and the basaltic amphibolites with a lack of intermediate lithologies in between can be explained by the setting of peraluminous arc magmatism within a subduction–accretion complex. In this model the amphibolites represent primary basalts which ponded at the base of the subduction–accretion complex and delivered the heat for the production of peraluminous melts. Volume estimations indicate a “zone of intermingling” composed of immiscible basalts and peraluminous melts with a total thickness of several kilometers. In this “zone of intermingling” the protoliths of the banded amphibolite formations were generated. Steep strike-slip faults, which are important structures for the syn-magmatic cratonization of subduction–accretion complexes, provide pathways for the emplacement of magmas, migmatites and intermingled materials. This results in the formation of steeply oriented sheets of orthogneisses, deformed migmatites and banded amphibolite formations, respectively. Finally, the paper lists many other peri-Gondwanan regions with an early Paleozoic peraluminous arc magmatism, indicating a similar setting on a global scale.

Highlights

  • Albert Heim (1921, p. 65) stated that “The Alps, despite of the many magmatic rocks, are not a magmatic orogen.” the majority of magmatites is much older than the Alpine orogeny

  • Other than collisional orogens with subhorizontal nappes or continental arcs composed of complex spheroidal batholiths, cratonized subduction–accretion complexes create a steeply structured crust consisting of intercalated sheets of paragneisses, orthogneisses, migmatites and banded amphibolite formations (Zurbriggen 2015)

  • 7 Conclusions Following conclusions can be made: 1. The orthogneisses, paragneisses, migmatites and amphibolites of the pre-Variscan basement units in the Alps indicate a common history during the Cenerian orogeny in early Paleozoic times

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Summary

Introduction

Albert Heim (1921, p. 65) stated that “The Alps, despite of the many magmatic rocks, are not a magmatic orogen.” the majority of magmatites is much older than the Alpine orogeny. 65) stated that “The Alps, despite of the many magmatic rocks, are not a magmatic orogen.”. The majority of magmatites is much older than the Alpine orogeny. They were generated either (i) in late Paleozoic related to the formation of Pangaea and subsequent Permian transtension, or (ii) during the Ordovician orogeny at the periphery of Gondwana (Bussien et al 2011; Zurbriggen 2015 and references therein). Von Raumer et al (2015) and Villaseca et al (2016), just to mention two of many more studies, developed comprehensive reconstructions of the early Paleozoic magmatic event, for which Zurbriggen (2017) has suggested the new term “Cenerian orogeny”.

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