Multiple crustal sources for post-tectonic I-type granites in the Hercynian Iberian Belt

被引:0
|
作者
C. Villaseca
F. Bellido
C. Pérez-Soba
K. Billström
机构
[1] Universidad Complutense,Departamento de Petrología y Geoquímica, Centro mixto UCM
[2] Instituto Geológico y Minero de España,CSIC, Facultad de Geología
[3] Swedish Museum of Natural History,undefined
来源
Mineralogy and Petrology | 2009年 / 96卷
关键词
Crustal Level; Compositional Field; Mafic Microgranular Enclave; Alumina Saturation Index; Central Iberian Zone;
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学科分类号
摘要
A post-tectonic plutonic array of felsic I-type granites crops out in the western Hercynian Iberian Belt. Isotope (Sr, Nd, Pb) data favour the absence of an important input of juvenile magmas in late- to post- tectonic Hercynian felsic magmatism in western Iberia, but suggest a reworking of different crustal protoliths, including oceanic metabasic rocks accreted to mid-to-lower crustal levels during the early stages of the collision. I-type granites were derived from different meta-igneous protoliths ranging from metabasic to felsic compositions depending on their geographical position from the external (e.g. Galicia—N Portugal, GNP) to the innermost continental areas (Spanish Central System and Los Pedroches Batholiths). The GNP I-type plutons related to eo-Hercynian accretional terranes have lower initial 87Sr/86Sr ratios, lower negative εNd values, and higher 206Pb/204Pb ratios than other I-type granites of the Central Iberian zone. These more isotopically primitive Hercynian I-type granites are important in tracking pre-Hercynian accreted oceanic lithosphere terranes.
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页码:197 / 211
页数:14
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