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Artículo

O-H-Sr-Nd isotope constraints on the origin of the Famatinian magmatic arc, NW Argentina

Alasino, Pablo HoracioIcon ; Casquet, César Martín; Pankhurst, Robert; Rapela, Carlos WashingtonIcon ; Dahlquist, Juan AndrésIcon ; Recio, Clemente; Baldo, Edgardo Gaspar AgustinIcon ; Larrovere, Mariano AlexisIcon ; Ramacciotti, Carlos DinoIcon
Fecha de publicación: 12/2020
Editorial: Cambridge University Press
Revista: Geological Magazine
ISSN: 0016-7568
Idioma: Inglés
Tipo de recurso: Artículo publicado
Clasificación temática:
Geología

Resumen

We report a study of whole-rock O-H-Sr-Nd isotopes of Ordovician igneous and metamorphic rocks exposed at different crustal palaeodepths along c. 750 km in the Sierras Pampeanas, NW Argentina. The isotope compositions preserved in the intermediate rocks (mostly tonalite) (average δ18O = +8.7 ± 0.5‰, δD = -73 ± 14‰, 87Sr/86Srt = 0.7088 ± 0.0001 and ϵNdt = -4.5 ± 0.6) show no major difference from those of most of the mafic rocks (average δ18O = +8 ± 0.8‰, δD = -84 ± 18‰, 87Sr/86Srt = 0.7082 ± 0.0016 and ϵNdt = -4 ± 1.1), suggesting that most of their magmas acquired their crustal characteristics in the mantle. The estimate of assimilation of crustal material (δ18O = +12.2 ± 1.7‰, δD = -89 ± 21‰, 87Sr/86Srt = 0.7146 ± 0.0034 and ϵNdt = -6.9 ± 0.7) by the tonalite is in most samples within the range 10-20%. Felsic magmas that reached upper crustal levels had isotope values (δ18O = +9.9 ± 1.5‰, δD= -76 ± 5‰, 87Sr/86Srt = 0.7067 ± 0.0010, ϵNdt = -3.5 ± 1.4) suggesting that they were not derived by fractionation of the contaminated intermediate magmas, but evolved from different magma batches. Some rocks of the arc, both igneous (mostly gabbro and tonalite) and metamorphic, underwent restricted interaction with meteoric fluids. Reported values of δ18O of magmatic zircons from the Famatinian arc rocks (+6 to +9‰) are comparable to our δ18O whole-rock data, indicating that pervasive oxygen isotope exchange in the lower crust was not a major process after zircon crystallization.
Palabras clave: CONTINENTAL GROWTH , FAMATINIAN ARC MAGMATISM , NON-HOMOGENIZED MAGMATIC SYSTEM , STABLE AND RADIOGENIC ISOTOPES
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info:eu-repo/semantics/restrictedAccess Excepto donde se diga explícitamente, este item se publica bajo la siguiente descripción: Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Unported (CC BY-NC-SA 2.5)
Identificadores
URI: http://hdl.handle.net/11336/143707
DOI: http://dx.doi.org/10.1017/S0016756820000321
URL: https://www.cambridge.org/core/journals/geological-magazine/article/abs/ohsrnd-i
Colecciones
Articulos(CRILAR)
Articulos de CENTRO REGIONAL DE INV. CIENTIFICAS Y TRANSFERENCIA TECNOLOGICA DE ANILLACO
Citación
Alasino, Pablo Horacio; Casquet, César Martín; Pankhurst, Robert; Rapela, Carlos Washington; Dahlquist, Juan Andrés; et al.; O-H-Sr-Nd isotope constraints on the origin of the Famatinian magmatic arc, NW Argentina; Cambridge University Press; Geological Magazine; 157; 12; 12-2020; 2067-2080
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