The late Oligocene-early Miocene marine transgression of Patagonia

FLORENCIA BECHIS; FELIPE PÉREZ; RICARDO RIFFO; SVEN NIELSEN; VICTOR A. RAMOS; ALFONSO ENCINAS; KENNET FINGER; PABLO BERNABÉ; LUIS BUATOIS; VÍCTOR VALENCIA; ANDRÉS FOLGUERA; PATRICIO ZAMBRANO; FRANCISCA TAPIA; DARÍO ORTS; JOSÉ CUITIÑO

The evolution of the Chilean-Argentinean Andes

Springer Earth System Sciences

Lugar: Berlin; Año: 2018; p. 443 - 474

The most important Cenozoic marine transgression in Patagonia occurred during the late Oligocene?early Miocene when marine waters of Pacific and Atlantic origin flooded most of southern South America including the present Patagonian Andes between ~41° and 47°S. The age, correlation, and tectonic setting of the different marine formations deposited during this period is debated. However, recent studies based principally on U-Pb geochronology and Sr isotope stratigraphy indicate that all of these units had accumulated during the late Oligocene?early Miocene. The marine transgression flooded a vast part of southern South America and, according to paleontologic data, probably permitted, for the first time in the history of this area, the transient connection between the Pacific and Atlantic oceans. Marine deposition started in the late Oligocene?earliest Miocene (~26?23 Ma) and was probably caused by a regional event of extension related to a major plate reorganization in the Southeast Pacific. Progressive extension and crustal thinning allowed a generalized marine flooding of Patagonia that reached its maximum extension at ~20 Ma. It was followed by a phase of compressive tectonics that started around 19?16 Ma and led to the growth of the Patagonian Andes. The youngest (~19?15 Ma) marine deposits that accumulated in the eastern Andean Cordillera and the extra-Andean regions are coeval with fluvial synorogenic deposits and probably had accumulated under a compressive regime.