Provenance of the Variscan Upper Allochthon (Cabo Ortegal Complex, NW Iberian Massif)

This study focuses on the provenance of the uppermost unit of the Upper Allochthon of the Variscan belt with combined U–Pb and Lu–Hf zircon (LA-ICPMS) and Sm–Nd whole-rock analyses. This unit is represented in the Cabo Ortegal Complex (NW Iberia) by the metasiliciclastic Cariño Gneisses which overla...

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Bibliographic Details
Authors: Albert, Richard, Arenas, Ricardo, Gerdes, A., Fernández-Suárez, Javier, Fuenlabrada, J.M.
Format: article
Status:Versión aceptada para publicación
Publication Date:2014
Country:España
Institution:Consejo Superior de Investigaciones Científicas (CSIC)
Repository:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/123727
Online Access:http://hdl.handle.net/10261/123727
Access Level:Open access
Keyword:Detrital zircons
Provenance
Isotope geochemistry
Variscan Upper Allochthon
Cabo Ortegal Complex
Description
Summary:This study focuses on the provenance of the uppermost unit of the Upper Allochthon of the Variscan belt with combined U–Pb and Lu–Hf zircon (LA-ICPMS) and Sm–Nd whole-rock analyses. This unit is represented in the Cabo Ortegal Complex (NW Iberia) by the metasiliciclastic Cariño Gneisses which overlap ophiolitic units that represent perigondwanan oceanic domains. The data set indicates a maximum depositional age of c. 510 Ma and a c. 1.73 Ga Sm–Nd model age, typifying a late or post Pan-African (or Cadomian) and Eburnean events, which entailed abundant input of juvenile material involving broad mixing with older crustal sources. The Mesoproterozoic activity is scarce and scattered and therefore unlikely to represent a major crust generation pulse in the source area of the siliciclastic unit. The data set also records an Archean orogenic pulse in its source area followed by a long lasting crust reworking process, where the Eburnean juvenile materials intruded. These data are interpreted as indicative of a West Africa Craton provenance, where the siliciclastic series from which the Cariño Gneisses are derived were probably deposited in a back-arc type basin where detritus was mostly sourced by the continent rather than the magmatic arc.