CaltechAUTHORS
  A Caltech Library Service

The genesis of Variscan (Hercynian) plutonic rocks: Inferences from Sr, Pb, and O studies on the Maladeta igneous complex, central Pyrenees (Spain)

Michard-Vitrac, Annie and Albarede, Francis and Dupuis, Christian and Taylor, Hugh P., Jr. (1980) The genesis of Variscan (Hercynian) plutonic rocks: Inferences from Sr, Pb, and O studies on the Maladeta igneous complex, central Pyrenees (Spain). Contributions to Mineralogy and Petrology, 72 (1). pp. 57-72. ISSN 0010-7999. doi:10.1007/bf00375568. https://resolver.caltech.edu/CaltechAUTHORS:20221026-664855800.3

Full text is not posted in this repository. Consult Related URLs below.

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20221026-664855800.3

Abstract

The Maladeta plutonic complex formed during the latest stages of the Variscan orogeny. It was emplaced into the Paleozoic sedimentary sequence of the Pyrenees. The eastern part, investigated in the present study, consists of an early intrusion of cumulate gabbronorites followed in order of emplacement by the main biotite-hornblende granodiorite, which was itself intruded by two small stocks of two-mica cordierite granite. An ⁸⁷Rb-⁸⁷Sr isochron dates the granodiorite at 277±7 m.y. with an initial (⁸⁷Sr/⁸⁶Sr)₀ ratio of 0.7117±3. Gabbroic rocks have lower strontium initial ratios, down to 0.7092, while those of granite range from that of the granodiorite up to about 0.715. The three rock types have distinctive δ¹⁸O values: 8.7 to 9.6 for the gabbronorites, 9.4 to 10.4 for the granodiorites and 10.3 to 11.8 for the granites. Lead isotopic compositions of rocks and feldspars are all radiogenic. Feldspars give consistent Pb model ages around 280 m.y., with μ and κ values of about 9.7 and 4.05, respectively. No pristine, mantle-derived magma was found among the investigated samples and the rocks cannot be related to one another by any simple mechanism of fractional crystallization. Some type of mixing process involving two end members seems to be required: a high-¹⁸O, high-⁸⁷Sr material that is clearly of crustal origin, and a lower-¹⁸O, lower-⁸⁷Sr end member derived from the mantle. Examination of various mixing models does not support magma mixing nor assimilation of crustal rocks by a mafic magma. The most acceptable model involves melting at different levels of a vertically-zoned source in the continental crust; this source was formed by mixing between mantle-derived magmas and crustal metasediments. This material was apparently thickened, tectonically downwarped and partially melted. None of the Maladeta magma-types appear to have been derived at a consuming plate boundary.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/bf00375568DOIArticle
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Caltech Division of Geological and Planetary Sciences3280
Issue or Number:1
DOI:10.1007/bf00375568
Record Number:CaltechAUTHORS:20221026-664855800.3
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20221026-664855800.3
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:117578
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:01 Nov 2022 21:15
Last Modified:01 Nov 2022 21:15

Repository Staff Only: item control page