Articles | Volume 15, issue 4
https://doi.org/10.5194/se-15-387-2024
https://doi.org/10.5194/se-15-387-2024
Research article
 | 
03 Apr 2024
Research article |  | 03 Apr 2024

Fast uplift in the southern Patagonian Andes due to long- and short-term deglaciation and the asthenospheric window underneath

Veleda A. P. Muller, Pietro Sternai, and Christian Sue

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Cited articles

Aniya, M.: Holocene variations of Ameghino glacier, southern Patagonia, Holocene, 6, 247–252, https://doi.org/10.1177/095968369600600211, 1996. 
Aniya, M., Sato, H., Naruse, R., Skvarca, P., and Casassa, G.: Recent glacier variations in the Southern Patagonia icefield, South America, Arct. Alp. Res., 29, 1–12, https://doi.org/10.1177/095968369600600211, 1997. 
Ávila, P. and Dávila, F. M.: Heat flow and lithospheric thickness analysis in the Patagonian asthenospheric windows, southern South America, Tectonophysics, 747, 99–107, https://doi.org/10.1016/j.tecto.2018.10.006, 2018. 
Ávila, P. and Dávila, F. M.: Lithospheric thinning and dynamic uplift effects during slab window formation, southern Patagonia (45–55° S), J. Geodynam., 133, 101689, https://doi.org/10.1016/j.jog.2019.101689, 2020. 
Ávila, P., Ávila, M., Dávila, F. M., Ezpeleta, M., and Castellano, N. E.: Patagonian landscape modeling during Miocene to Present-day slab window formation, Tectonophysics, 862, 229971, https://doi.org/10.1016/j.tecto.2023.229971, 2023. 
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Short summary
Uplift rates up to 40 mm yr−1 are measured by GNSS in the southern Patagonian Icefield, a remainder of the Patagonian Ice Sheet that covered the Andes in the Last Glacial Maximum (LGM) at 26 ka. Using numerical modelling, we estimate an increase of 150 to 200 °C of the asthenospheric temperature due to the slab window under southern Patagonia, and we show that post-glacial rebound, after the long-term LGM and the short-term Little Ice Age (400 a), contributed to the modern uplift rate budget.