The formation of Pangea

The making of Pangea is the result of large-scale amalgamation of continents and micro-continents, which started at the end of the Neoproterozoic with the formation of Gondwana. As pieces were added to Gondwana on its South-American, Antarctica and Australia side, ribbon-like micro-continents were d...

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Main Authors: Stampfli, G.M., Hochard, C., Vérard, C., Wilhem, C., Raumer, Jürgen F. von
Language:English
Published: 2013
Subjects:
Online Access:http://doc.rero.ch/record/31872/files/rau_fp.pdf
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spelling ftreroch:oai:doc.rero.ch:20130426085630-GP 2023-05-15T13:51:53+02:00 The formation of Pangea Stampfli, G.M. Hochard, C. Vérard, C. Wilhem, C. Raumer, Jürgen F. von 2013-04-26T06:58:04Z http://doc.rero.ch/record/31872/files/rau_fp.pdf eng eng http://doc.rero.ch/record/31872/files/rau_fp.pdf 2013 ftreroch 2023-02-16T17:25:11Z The making of Pangea is the result of large-scale amalgamation of continents and micro-continents, which started at the end of the Neoproterozoic with the formation of Gondwana. As pieces were added to Gondwana on its South-American, Antarctica and Australia side, ribbon-like micro-continents were detached from its African and South-Chinese side: Cadomia in the late Neoproterozoic, Avalonia and Hunia in the Ordovician, Galatia in the Devonian and Cimmeria in the Permian. Cadomia was re- accreted to Gondwana, but the other ribbon-continents were accreted to Baltica, North-China, Laurussia or Laurasia. Finding the origin of these numerous terranes is a major geological challenge. Recently, a global plate tectonic model was developed together with a large geological/geodynamic database, at the Lausanne University, covering the last 600 Ma of the Earth's history. Special attention was given to the placing of Gondwana derived terranes in their original position, using all possible constraints. We propose here a solution for the Variscan terranes, another paper deals with the Altaids. The Galatian super-terrane was detached from Gondwana in the Devonian, during the opening of Paleotethys, and was quickly separated into four sub-terranes that started to by-pass each other. The leading terranes collided at the end of the Devonian with the Hanseatic terrane detached from Laurussia. In the Carboniferous, Gondwana started to impinge onto the amalgamated terranes, creating the Variscan chain and the Pangean super-continent. East of Spain Paleotethys remained opened until the Triassic, subducting northward under Laurasia. Roll-back of the Paleotethyan slab triggered the collapse of most of the European Variscan orogen, which was replaced by series of Permian rifts, some of them becoming oceanized back-arc basins during the Triassic. Major force changes at the Pangean plate limits at the end of the Triassic provoked its break-up, through the opening of the proto-Caribbean, central-Atlantic, Alpine-Tethys oceanic seaways. Other/Unknown Material Antarc* Antarctica RERO DOC Digital Library
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language English
description The making of Pangea is the result of large-scale amalgamation of continents and micro-continents, which started at the end of the Neoproterozoic with the formation of Gondwana. As pieces were added to Gondwana on its South-American, Antarctica and Australia side, ribbon-like micro-continents were detached from its African and South-Chinese side: Cadomia in the late Neoproterozoic, Avalonia and Hunia in the Ordovician, Galatia in the Devonian and Cimmeria in the Permian. Cadomia was re- accreted to Gondwana, but the other ribbon-continents were accreted to Baltica, North-China, Laurussia or Laurasia. Finding the origin of these numerous terranes is a major geological challenge. Recently, a global plate tectonic model was developed together with a large geological/geodynamic database, at the Lausanne University, covering the last 600 Ma of the Earth's history. Special attention was given to the placing of Gondwana derived terranes in their original position, using all possible constraints. We propose here a solution for the Variscan terranes, another paper deals with the Altaids. The Galatian super-terrane was detached from Gondwana in the Devonian, during the opening of Paleotethys, and was quickly separated into four sub-terranes that started to by-pass each other. The leading terranes collided at the end of the Devonian with the Hanseatic terrane detached from Laurussia. In the Carboniferous, Gondwana started to impinge onto the amalgamated terranes, creating the Variscan chain and the Pangean super-continent. East of Spain Paleotethys remained opened until the Triassic, subducting northward under Laurasia. Roll-back of the Paleotethyan slab triggered the collapse of most of the European Variscan orogen, which was replaced by series of Permian rifts, some of them becoming oceanized back-arc basins during the Triassic. Major force changes at the Pangean plate limits at the end of the Triassic provoked its break-up, through the opening of the proto-Caribbean, central-Atlantic, Alpine-Tethys oceanic seaways.
author Stampfli, G.M.
Hochard, C.
Vérard, C.
Wilhem, C.
Raumer, Jürgen F. von
spellingShingle Stampfli, G.M.
Hochard, C.
Vérard, C.
Wilhem, C.
Raumer, Jürgen F. von
The formation of Pangea
author_facet Stampfli, G.M.
Hochard, C.
Vérard, C.
Wilhem, C.
Raumer, Jürgen F. von
author_sort Stampfli, G.M.
title The formation of Pangea
title_short The formation of Pangea
title_full The formation of Pangea
title_fullStr The formation of Pangea
title_full_unstemmed The formation of Pangea
title_sort formation of pangea
publishDate 2013
url http://doc.rero.ch/record/31872/files/rau_fp.pdf
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_relation http://doc.rero.ch/record/31872/files/rau_fp.pdf
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