Secular variations of magma source compositions in the North Patagonian batholith from the Jurassic to Tertiary: Was mélange melting involved?

Author:

Castro Antonio1,Rodriguez Carmen2,Fernández Carlos3,Aragón Eugenio4,Pereira Manuel Francisco5,Molina José Francisco6

Affiliation:

1. Instituto Andaluz de Ciencias de la Tierra (IACT), Consejo Superior de Investigaciones Científicas–Universidad de Granada (CSIC-UGR), 18100 Armilla, Granada, Spain

2. Geosciences Barcelona (formerly ICTJA), Consejo Superior de Investigaciones Científicas (CSIC), 08028 Barcelona, Spain

3. Departamento de Ciencias de la Tierra, Universidad de Huelva, 21007 Huelva, Spain

4. Facultad de Ciencias Naturales y Museo, Universidad Nacional de la Plata, B1900 La Plata, Buenos Aires, Argentina

5. Instituto de Ciências da Terra (ICT), Departamento de Geociências, Escola de Ciências e Tecnologia (ECT), Universidade de Évora, 7000-670 Évora, Portugal

6. Departamento de Mineralogía y Petrología, Universidad de Granada, Campus Univeristario de Fuentenueva, 18071 Granada, Spain

Abstract

Abstract This study of Sr-Nd initial isotopic ratios of plutons from the North Patagonian batholith (Argentina and Chile) revealed that a secular evolution spanning 180 m.y., from the Jurassic to Neogene, can be established in terms of magma sources, which in turn are correlated with changes in the tectonic regime. The provenance and composition of end-member components in the source of magmas are represented by the Sr-Nd initial isotopic ratios (87Sr/86Sr and 143Nd/144Nd) of the plutonic rocks. Our results support the interpretation that source composition was determined by incorporation of varied crustal materials and trench sediments via subduction erosion and sediment subduction into a subduction channel mélange. Subsequent melting of subducted mélanges at mantle depths and eventual reaction with the ultramafic mantle are proposed as the main causes of batholith magma generation, which was favored during periods of fast convergence and high obliquity between the involved plates. We propose that a parental diorite (= andesite) precursor arrived at the lower arc crust, where it underwent fractionation to yield the silicic melts (granodiorites and granites) that formed the batholiths. The diorite precursor could have been in turn fractionated from a more mafic melt of basaltic andesite composition, which was formed within the mantle by complete reaction of the bulk mélanges and the peridotite. Our proposal follows model predictions on the formation of mélange diapirs that carry fertile subducted materials into hot regions of the suprasubduction mantle wedge, where mafic parental magmas of batholiths originate. This model not only accounts for the secular geochemical variations of Andean batholiths, but it also avoids a fundamental paradox of the classical basalt model: the absence of ultramafic cumulates in the lower arc crust and in the continental crust in general.

Publisher

Geological Society of America

Subject

Stratigraphy,Geology

Reference91 articles.

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