Andean Geology is becoming an English-language journal
This transition will be effective starting July 1, 2026. All submissions but obituaries and comments, and those part of special issues, will be required to be submitted in English
Call for Papers
Special Issue: Advances in Paleontology in Chile: Opportunities and Challenges for a Synthesis
Edited by:
- Marcelo Rivadeneira, CEAZA
- Enrique Bostelmann, Sernageomin
- Martín Chávez-Hoffmeister, CIAHN
- Joseline Manfroi, CIAHN
- Philippe Moisan, Universidad de Atacama
- Karen Moreno, Universidad Austral de Chile
- Sven Nielsen, Universidad Austral de Chile
- Ana Valenzuela-Toro, CIAHN
- Natalia Villavicencio, Universidad de O'Higgins
Submission status: Open between March 1, 2026, and November 30, 2026
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Special Issue: Geoethics in Chile and Latin America - Contextual reflections for responsible geoscience
Edited by:
- Luisa Pinto, Universidad de Chile
- Hernán Bobadilla, Politecnico di Milano
- Tania Villaseñor, Pontificia Universidad Católica de Chile
- Pablo Ramírez, Universidad de Chile
- Millarca Valenzuela, Universidad Católica del Norte
Submission status: Open between August 15, 2025, and April 30, 2026
Departamento de Geología, Facultad de Ciencias Físicas y Matemáticas, Universidad de Chile. Plaza Ercilla 803, Santiago, Chile.
Géosciences Environnement Toulouse, Université de Toulouse, CNRS, IRD, UPS, CNES, 31400 Toulouse, France.
Present address: Departamento de Ingeniería en Minas, Universidad de Santiago de Chile, Libertador Bernardo O’Higgins #3363, Santiago, Chile. Chile
Michel de Saint-Blanquat
Géosciences Environnement Toulouse, Université de Toulouse, CNRS, IRD, UPS, CNES, 31400 Toulouse, France. France
Francisco Hervé
Departamento de Geología, Facultad de Ciencias Físicas y Matemáticas, Universidad de Chile. Plaza Ercilla 803, Santiago, Chile.
Carrera de Geología, Universidad Andrés Bello, Sazié 2119, Santiago. Chile
Mireille Polvé
Géosciences Environnement Toulouse, Université de Toulouse, CNRS, IRD, UPS, CNES, 31400 Toulouse, France. France
Diego Morata
Departamento de Geología, Facultad de Ciencias Físicas y Matemáticas, Universidad de Chile. Plaza Ercilla 803, Santiago, Chile.
Centro de Excelencia en Geotermia de los Andes (CEGA, ANID-Fondap), Universidad de Chile, Plaza Ercilla 803, Santiago, Chile. Chile
Phillipe de Parseval
Géosciences Environnement Toulouse, Université de Toulouse, CNRS, IRD, UPS, CNES, 31400 Toulouse, France. France
Mathieu Benoit
Géosciences Environnement Toulouse, Université de Toulouse, CNRS, IRD, UPS, CNES, 31400 Toulouse, France. France
Geochemistry of Cenozoic plutonic rocks in the extra-Andean southern Patagonia as evidence for a magmatic arc migration process
Alejandro Sánchez Valenzuela, Michel de Saint-Blanquat, Francisco Hervé, Mireille Polvé, Diego Morata, Phillipe de Parseval, Mathieu Benoit
Abstract
In this work, we present the results of a petrographic and geochemical study that involves seven Cenozoic plutons located in a NS trending belt in western Patagonia, south of the present Chile Triple-Junction and to the east of the present magmatic arc. Four plutons were studied in the northern end, and three in the southern part of the belt. The petrographic and geochemical characteristics (major and trace element contents, eNdt, 87Sr/86Sr initial ratios), of these plutons are different enough to propose a further classification for them: Only the Monte Balmaceda intrusive complex in the southern end of the belt is alkaline (sensu stricto). The Río de Las Nieves and San Lorenzo plutons in the northern area, and the Torres del Paine intrusive complex, in the southern area have “intra-plate transitional” calc-alkaline affinity. Paso de Las Llaves and Cerro Negro del Ghío plutons in the northern area, and Cerro Donoso pluton in the southern area show “arc transitional” calc-alkaline character. The “transitional” character, together with the pluton’s location, and their regional geological context, can be explained by a Mio-Pliocene eastward arc migration coeval with the beginning of the Chile Rise subduction. A slab flattening hypothesis is favoured to explain the arc-migration, which together with the different length and time of arrival of the Chile Rise segments to the subduction zone, contributed to the heterogeneous geochemistry of the studied plutons.