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
Read more (pdf)
Miocene magmatism of Southernmost Tierra del Fuego: evidence of repeated subduction of oceanic spreading ridges in Patagonia.
Cristobal Ramírez, Mauricio Calderon, Benjamin Aspillaga, Gonzalo Galaz, Pierre Yves Descote, Israel Donoso, C. Mark Fanning, Marly Babinski, Fernando Poblete
Abstract
Ridge subduction is known to generate anomalous magmatism before and during the opening of a slab window. High-Sr/Y intermediate magmas and slightly alkaline basalts with transitional arc-to-intraplate (OIB-like) signatures have been reported worldwide in such tectonic settings. Southernmost South America has been affected by the subduction of several spreading ridges from the Late Oligocene to the present. Here we present new geochronological, petrographic, geochemical, and isotopic data to evaluate the petrogenesis of two Early Miocene volcanic units from islands at ≈56°S, formed during subduction of the Nazca–Phoenix spreading ridge. Comparison with igneous suites related to subduction of the Chile Ridge (currently being subducted beneath central Patagonia at ≈46°30′S) reveals notable similarities in timing relative to slab-window formation and in chemical signatures. Furthermore, there is a volcanic arc-gap of around 200 km during the Early Miocene, which coincides with the location of the Nazca–Phoenix slab window. We interpret the chemistry of the high Sr/Y rocks as the result of the melting of a mantle source contaminated by terrigenous material derived from erosion of the accretionary prism associated with young, highly rugose oceanic crust. In contrast, the slightly alkaline magmas reflect lower degrees of partial melting under a different thermal structure of the slab–mantle wedge.