Growth of the Patagonian Andes since the Mid Jurassic to the Present

FOLGUERA, ANDRES; GIANNI, GUIDO M.; NAVARRETE, CESAR; ECHAURREN, ANDRES; ORTS, DARÍO; FERNÁNDEZ PAZ, LUCÍA; IANNELLI, SOFÍA B.; LITVAK, VANESA D.; ENCINAS, ALFONSO

Congreso; XV Congreso Geológico Chileno; 2018

The Patagonian Andes have been constructed through several deformational stages. Thus, Jurassic within plate contractionalsystems has alternated with periods of extension associated with the emplacement of the Karoo-Ferrar LIP producing proto-Andean mountain systems. These deformations are explained by a particular deformational field imposed by the southwarddisplacement of South America, the Weddell sea opening and mechanical weakening imposed by the hotspot activity. This chaoticsystem is replaced at the Early Cretaceous by an intra- back-arc extensional system that is inverted in the late Early Cretaceousproducing a first integrated foreland basin and a broad fold and thrust belt. This exceptional development of the fold and thrustbelt coincides with the eastward advance of the arc activity which is interpreted in terms of a shallow subducted slab configurationassociated with a stable seismic ridge impacting at the Patagonian trench. These Cretaceous contractional structures are affectedby Eocene deformations that are variable in mechanics depending on the latitude: While some segments of the fold and thrustbelt are extensionally reactivated, others are contractionally reactivated. This variable behavior is interpreted as due to the obliquecollision of a seismic ridge from north to south that produced slab windows alternated with segments where transform segmentscollided. Latest Eocene to Oligocene tectonics is characterized by widespread extension with back- and intra-arc basins andthe outstanding detachment of Los Chonos fore-arc sliver. This extensional stage ends at the earliest Miocene with Atlantic andPacific-derived transgressions that could be interpreted in terms of thermal subsidence and/or dynamic subsidence in a contextof the steepening of the Nazca subducted slab. The Chonos fore-arc block accretes in early Miocene times producing a broadfold and thrust belt that reaches Central Patagonia in mid-Miocene times. This process is accompanied by mild east-ward arcmigrations at the edges of the Chonos accretion zone interpreted as subducted slab shallowing. Late Miocene deformation isfocused on out-of-sequence thrusts that produce the rain shadow conditions that characterize Patagonia producing strong biotachanges. Mild Quaternary reactivations of the Miocene systems are the late expression of this uplift.