Special Issue dedicated to Francisco Hervé: Global tectonic processes of the ancient southwestern Gondwana margin in South America and the Antarctic Peninsula
Edited by:
- Mauricio Calderón, PhD, Universidad del Desarrollo, Chile
- Paula Castillo, PhD, Universität Münster, Deutschland
- Robert Pankhurst, PhD ScD, United Kingdom
Submission status: Extended until September 30, 2025
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 March 31, 2026
Departamento de Geología, Facultad de Ciencias Físicas y Matemáticas, Universidad de Chile, Plaza Ercilla 803, Santiago, Chile.
Carrera de Geología, Facultad de Ingeniería, Universidad Andrés Bello, Av. República 220, Santiago, Chile. Chile
Mauricio Calderón
Carrera de Geología, Facultad de Ingeniería, Universidad del Desarrollo, Av. Plaza 680, Las Condes, Santiago, Chile. Chile
Gianfranco Gregorina
Carrera de Geología, Facultad de Ingeniería, Universidad Andrés Bello, Av. República 220, Santiago, Chile. Chile
The orbicular granodiorite of Recoba Hill in the North Patagonian Batholith
Aníbal Soto, Francisco Hervé, Mauricio Calderón, Gianfranco Gregorina
Abstract
A small body of orbicular granodiorite crops out on the Recoba Hill, immediately east of the town of Chaitén, in the mainland area called Chiloé continental, in southern Chile. The rock comprises cm-sized igneous cores with a single shell of fine-grained plagioclase-quartz-K-feldspar assemblages. It is hosted in a Miocene granodiorite, and it is crosscut by aplite and mafic dikes. No other mention of orbicular rocks has to date been reported for the >1,000 km long North Patagonian Batholith, suggesting that the conditions necessary for their formation were infrequent. Thermobarometric determinations indicate pressures lower than 2 kbar (less than 6 km depth) for its formation, a level much shallower than the estimated source depth of the older rocks of the batholith.