2016
DOI: 10.1016/j.tecto.2016.02.031
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Tracing the Cambro-Ordovician ferrosilicic to calc-alkaline magmatic association in Iberia by in situ U–Pb SHRIMP zircon geochronology (Gredos massif, Spanish Central System batholith)

Abstract: 18 U-Pb geochronological study of zircons from nodular granites and Qtz-diorites comprising part of 19Variscan high-grade metamorphic complexes in Gredos massif (Spanish Central System batholith) 20 points out the significant presence of Cambro-Ordovician protoliths among the Variscan migmatitic 21 rocks that host the Late Carboniferous intrusive granitoids. Indeed, the studied zone was affected by 22 two contrasted tectono-magmatic episodes, Carboniferous (Variscan) and Cambro-Ordovician. The European Varisca… Show more

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Cited by 20 publications
(13 citation statements)
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“…Therefore, the late Cadomian granites formed by melting of the same meta-greywacke source as the late Variscan granites, but at higher temperatures. This interpretation is consistent with the high content in ferromagnesian components observed in Figure 7 and reinforces the possibility that the most mafic late Cadomian granitoids resulted from particularly high degrees of melting, as proposed for the Cambro-Ordovician ferrosilicic magmatism defined in the central Iberian Massif (Fernández et al, 2008;Castro et al, 2009;Díaz-Alvarado et al, 2016). The CPO late Cadomian granitoids show indeed many geochemical features of the high-silica ferrosilicic magmatic rocks, as defined by Castro et al (2009), such as high FeO and MgO contents (FeOt > 2.5 wt.…”
Section: Discussionsupporting
confidence: 89%
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“…Therefore, the late Cadomian granites formed by melting of the same meta-greywacke source as the late Variscan granites, but at higher temperatures. This interpretation is consistent with the high content in ferromagnesian components observed in Figure 7 and reinforces the possibility that the most mafic late Cadomian granitoids resulted from particularly high degrees of melting, as proposed for the Cambro-Ordovician ferrosilicic magmatism defined in the central Iberian Massif (Fernández et al, 2008;Castro et al, 2009;Díaz-Alvarado et al, 2016). The CPO late Cadomian granitoids show indeed many geochemical features of the high-silica ferrosilicic magmatic rocks, as defined by Castro et al (2009), such as high FeO and MgO contents (FeOt > 2.5 wt.…”
Section: Discussionsupporting
confidence: 89%
“…The analysis of age patterns of detrital and inherited zircon in metasedimentary and igneous rocks, respectively, is commonly used in provenance studies aimed at reconstructing the geodynamic evolution of continents (e.g., Nance et al, 2014 and references therein). On the other hand, zircon inheritance patterns in igneous rocks have been employed relatively little as a petrogenetic tool, despite their considerable potential to provide key information on both magma sources and petrogenetic processes (e.g., Chen and Williams, 1990;Paterson et al, 1992;Williams, 1992Williams, , 2001Zeck and Williams, 2002;Fiannacca et al, 2008Fiannacca et al, , 2013Fiannacca et al, , 2017Jeon et al, 2012;Samperton et al, 2015;Díaz-Alvarado et al, 2016;Jeon and Williams, 2018;Schaltegger and Davies, 2018).…”
Section: Introductionmentioning
confidence: 99%
“…passive margin) plate margin setting (Díez Montes et al, 2010;Martínez Catalán et al, 2004;Montero et al, 2009), and (2) the 'continuous' model that considers a protracted evolution of an active margin (i.e. back-arc basin) that has extended over time from the Ediacaran to the Ordovician (Abati et al, 2010;Díaz-Alvarado et al, 2016;Díez Fernández et al, 2010, 2012Fernandez et al, 2008;Pereira et al, 2018). The above-mentioned tectonic models agree that the Cambro-Ordovician magmatism is related to the development of an intracontinental rifting.…”
Section: Introductionmentioning
confidence: 94%
“…However, this study will focus on the Neoproterozoic-Ordovician CIZ stratigraphy and related magmatism. The oldest Ediacaran to Early Cambrian siliciclastic rocks (Schist Greywacke Complex; SGC,) are unconformably overlain by a Cambro-Ordovician felsic igneous-sedimentary complex, named "Ollo de Sapo Formation" in the north of the CIZ (Díez Montes et al, 2010;Fernandez et al, 2008;Montero et al, 2009), the Urra Formation in the south of the CIZ (Gonçalves, 1971;Solá et al, 2008)and/orOrdovician siliciclastic rocks (including the Armorican quartzites), all intruded by Cambro-Ordovician granitic rocks (Antunes et al, 2009;Bea et al, 2006;Ferreira et al, 2018;Montero et al, 2007Montero et al, , 2009Neiva et al, 2009;Pereira et al, 2018;Talavera et al, 2013), and a few gabbrodioritic rocks (Díaz-Alvarado et al, 2016;Gonçalves, 1971;Solá, 2007).…”
Section: Geological Settingmentioning
confidence: 99%
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