Cretaceous magmatism in the Antarctic Peninsula and its tectonic implications

Author:

Bastias Joaquin123ORCID,Spikings Richard1,Riley Teal4,Chew David2,Grunow Anne5,Ulianov Alexey6,Chiaradia Massimo1,Burton-Johnson Alex4

Affiliation:

1. Department of Earth Sciences, University of Geneva, 1205 Genève, Switzerland

2. Department of Geology, Trinity College Dublin, College Green, Dublin 2, Ireland

3. Carrera Geología, Facultad de Ingeniería, Universidad Andres Bello, Santiago, Chile

4. British Antarctic Survey, High Cross, Madingley Road, Cambridge CB3 0ET, UK

5. Byrd Polar Research Center, Ohio State University, 108 Scott Hall, 1090 Carmack Road, Columbus, OH 43210, USA

6. Institute of Earth Sciences, University of Lausanne, 1015 Lausanne, Switzerland

Abstract

Periods of cessation, resumption and enhanced arc activity are recorded in the Cretaceous igneous rocks of the Antarctic Peninsula. We present new geochronological (laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS) zircon U–Pb) analyses of 36 intrusive and volcanic Cretaceous rocks, along with LA-ICP-MS apatite U–Pb analyses (a medium-temperature thermochronometer) of 28 Triassic–Cretaceous igneous rocks of the Antarctic Peninsula. These are complemented by new zircon Hf isotope data along with whole-rock geochemistry and isotope (Nd, Sr and Pb) data. Our results indicate that the Cretaceous igneous rocks of the Antarctic Peninsula have geochemical signatures consistent with a continental arc setting and were formed during the intervalc.140–79 Ma, whereas the main peak of magmatism occurred duringc.118–110 Ma. Trends inεHft(zircon) combined with elevated heat flow that remagnetized rocks and reset apatite U–Pb ages suggest that Cretaceous magmatism formed within a prevailing extensional setting that was punctuated by periods of compression. A noteworthy compressive period probably occurred duringc.147–128 Ma, triggered by the westward migration of South America during opening of the South Atlantic Ocean. Cretaceous arc rocks that crystallized duringc.140–100 Ma define a belt that extends from southeastern Palmer Land to the west coast of Graham Land. This geographical distribution could be explained by (1) a flat slab with east-dipping subduction of the Phoenix Plate, or (2) west-dipping subduction of the lithosphere of the Weddell Sea, or (3) an allochthonous origin for the rocks of Alexander Island. A better understanding of the geological history of the pre-Cretaceous rocks of Alexander Island and the inaccessible area of the southern Weddell Sea is required.Supplementary material:A description of the methods used in this study and the complete dataset are available athttps://doi.org/10.6084/m9.figshare.c.6089274

Funder

Instituto Antartico Chileno

Agencia Nacional de Investigación y Desarrollo

Swiss National Science Foundation

Science Foundation Ireland

Publisher

Geological Society of London

Subject

Geology

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