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dc.contributor.authorCambeses, Aitor
dc.contributor.authorScarrow, Jane Hannah 
dc.contributor.authorMontero, Pilar 
dc.contributor.authorMolina, José Francisco 
dc.contributor.authorMoreno, Juan Antonio
dc.date.accessioned2025-01-31T08:34:21Z
dc.date.available2025-01-31T08:34:21Z
dc.date.issued2015
dc.identifier.citationCambeses, A., Scarrow, J. H., Montero, P., Molina, J. F., & Moreno, J. A. (2015). SHRIMP U–Pb zircon dating of the Valencia del Ventoso plutonic complex, Ossa-Morena Zone, SW Iberia: Early Carboniferous intra-orogenic extension-related ‘calc-alkaline’magmatism. Gondwana Research, 28(2), 735-756.. DOI: 10.1016/j.gr.2014.05.013es_ES
dc.identifier.urihttps://hdl.handle.net/10481/101493
dc.description.abstractMantle- and crustal-derived orogenic magmas provide insights into sources tapped during terrane accretion and supercontinent amalgamation. During Pangea formation volumetrically minor, but common, mafic–intermediate ‘calc-alkaline’ stocks intruded coeval granitoid plutons throughout the European Variscan. The Iberian Peninsula preserves the westernmost segment of this Upper Paleozoic orogeny that resulted from collision of Laurentia and Gondwana. Whether the widespread calc-alkaline mafic–intermediate stocks may be used as petrogenetic tectonomagmatic markers of ancient subduction zones is an important question. Early Carboniferous calc- alkaline plutonic rocks from the Ossa-Morena Zone (OMZ), a northern Gondwana continental block, have traditionally been related to subduction. However, recent studies suggest that the tectonomagmatic regime at that time was continental collision. In this context, a link is made between Early Carboniferous intraplating of ultramafic and mafic sills into the mid-crust, the IBERSEIS Reflective Body (IRB), and the Variscan magmatism in the Olivenza–Monesterio antiform of the OMZ. Here we show that the OMZ Valencia del Ventoso plutonic complex comprising alkaline, calc-alkaline, metaluminous and peraluminous compositions formed during the Visean–Bashkirian, c. 334–320 Ma SHRIMP U–Pb zircon. The calc-alkaline character is, apparently, a result of intra-orogenic extension-related interaction of mantle-derived alkaline mafic and crustal-derived peraluminous felsic magma during terrane accretion. The new age is some c. 15–30 million years younger than previously defined and so coeval with IRB formation. All evidence points towards active subduction having ceased prior to the latest Devonian–earliest Carboniferous. Thus the younger age places the Olivenza–Monesterio antiform calc-alkaline magmatism after collision of the OMZ and the South Portuguese Zone, to the south. During Pangea formation other, comparable, Early Carboniferous extensional events have been described in adjacent terranes in northern Gondwana and Avalonia–Laurentia. Whether orogenic mafic magmatism provokes or results from crustal melting apparently depends on the process controlling, and the timing, of the mantle melting event.es_ES
dc.description.sponsorshipAndalusian Grant RNM1595es_ES
dc.description.sponsorshipSpanish Grant CGL2008-02864es_ES
dc.language.isoenges_ES
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internacional*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.subjectVariscanes_ES
dc.subjectOssa-Morena Zonees_ES
dc.subjectZircon geochronologyes_ES
dc.subjectIBERSEIS Reflective Bodyes_ES
dc.subjectMagma mixinges_ES
dc.titleSHRIMP U–Pb zircon dating of the Valencia del Ventoso plutonic complex, Ossa-Morena Zone, SW Iberia: Early Carboniferous intra-orogenic extension-related ‘calc-alkaline’ magmatismes_ES
dc.typejournal articlees_ES
dc.rights.accessRightsopen accesses_ES
dc.identifier.doi10.1016/j.gr.2014.05.013


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