OPHIOLITES ET SCHISTES LUSTRÉS CORSES: MODES DE GISEMENT, COMPARAISONS ALPINES

Authors

  • Marcel Lemoine Directeur de Recherches honoraire au CNRS, 40 Avenue de l’Europe, F- 78760 Marly-le-Roi, France
  • Alain Gauthier Professeur au Lycée Fesch, F-20000 Ajaccio, France

DOI:

https://doi.org/10.4454/ofioliti.v27i2.180

Keywords:

Abstract

Corsican ophiolites are highly comparable with those of the Alps: they comprise mantle-derived serpentinites, gabbros and basalts; no sheeted dyke complex is known. Between the basalts and/or sediments and the underlying serpentinites and gabbros, the contact is normal, i.e. not tectonical, and is often marked by a few cm to a few tens of metres of sedimentary breccias (so-called ophicalcites). Concluding, both Corsican and Alpine ophiolites derive from a slow-spreading ocean such as the Atlantic. Locally, in some parts of the Alps (e.g. Queyras) as well in parts of Corsica (Altiani-Vezzani; Cap Corse), Upper Jurassic to Lower Cretaceous tectonic activity is marked by ophiolitic detrital supply including huge ophiolitic olistoliths embedded in the Lower Cretaceous “Palombini”.

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Published

2002-07-01

How to Cite

Lemoine, M., & Gauthier, A. (2002). OPHIOLITES ET SCHISTES LUSTRÉS CORSES: MODES DE GISEMENT, COMPARAISONS ALPINES. Ofioliti, 27(2), 103-108. https://doi.org/10.4454/ofioliti.v27i2.180

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Articles