2013
DOI: 10.1016/j.lithos.2013.05.006
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SHRIMP U–Pb zircon geochronology and thermal modeling of multilayer granitoid intrusions

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Cited by 39 publications
(11 citation statements)
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“…Taking into account the compositional and textural features shown above, it may be inferred that the ages between 309 and 297Ma (average=300±4Ma) calculated for Group-I uraninite display the age of magmatic uraninite crystallization. This age overlaps with zircon ages (309 to 303Ma) from granites surrounding Los Santos skarn (Bea et al, 2004;Díaz Alvarado et al, 2013;Gutiérrez-Alonso et al, 2011;Valle Aguado et al, 2005;Zeck et al, 2007).…”
Section: The Significance Of the Chemical Uraninite Ages From Los Sansupporting
confidence: 61%
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“…Taking into account the compositional and textural features shown above, it may be inferred that the ages between 309 and 297Ma (average=300±4Ma) calculated for Group-I uraninite display the age of magmatic uraninite crystallization. This age overlaps with zircon ages (309 to 303Ma) from granites surrounding Los Santos skarn (Bea et al, 2004;Díaz Alvarado et al, 2013;Gutiérrez-Alonso et al, 2011;Valle Aguado et al, 2005;Zeck et al, 2007).…”
Section: The Significance Of the Chemical Uraninite Ages From Los Sansupporting
confidence: 61%
“…The tectono-metamorphic evolution of the northern half of the CIZ includes four main phases of ductile deformation (Díaz-Alvarado et al, 2013 and references therein): D 1 (upright and E-vergent folds coupled with contractional deformation), ~360-337Ma; D 2 (extensional detachments), ~337-316Ma; D 3 (upright folds and a new extensional episode), ~316-300Ma; and D 4 (upright folds and shear bands only described for the eastern part of the Spanish Central System (SCS)). Dating of zircon from Variscan granitoids reveals that most magmatism in the western part of the SCS occurred during the D 3 phase (309 to 303Ma) (Bea et al, 2004;Díaz Alvarado et al,…”
Section: Geological Settingmentioning
confidence: 99%
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“…The hypotheses that support rather continuous magmatic activity are mainly derived from the combined interpretation of radiometric ages of granitoids obtained by different methods 40 Ar- 39 Ar, K-Ar; e.g., Serrano Pinto et al, 1987;Díaz Alvarado et al, 2013;Martínez Catalán et al, 2014) and the numerical modeling of the thermal evolution of the orogen, including radioactive heat production (e.g., Bea et al, 1999Bea et al, , 2003Bea, 2012;Alcock et al, 2015). In essence, these hypotheses view melt production in the collisional scenario mainly as the result of severe crustal thickening of a fertile (graywacke and pelite rich) crust followed by an interval of thermal relaxation (e.g., Martínez-Catalán et al, 2014) accompanied by melting of the thickened crust.…”
Section: Introductionmentioning
confidence: 99%
“…The Gredos batholith has been revealed during the last decade as one of the most outstanding and voluminous granitic exposures (more than 300 km in length and 60 km in width) to explore the interactions between intrusive magmas and a medium-to highgrade crustal sections. The batholith is mainly composed of Bt ±Crd granodiorites and monzogranites and minor amounts of basic rocks [Scarrow et al, 2009] that depict a Krich calc-alkaline suite characteristic of I-type post-collisional batholiths [Castro, 2019], emplaced during late D2 and D3 Variscan phases (320-290 Ma) [Díaz Alvarado et al, 2013;Díaz-Alvarado et al, 2011]. Detailed studies of the central area of the batholith have evidenced a laminar structure formed by mostly migmatitic host-rocks and intrusive layers.…”
Section: Field Relations Supporting Assimilation and Magma Contaminationmentioning
confidence: 99%