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The large MIS 4 and long MIS 2 glacier maxima on the southern tip of South America
Indexado
WoS WOS:000663677600004
Scopus SCOPUS_ID:85104927793
DOI 10.1016/J.QUASCIREV.2021.106858
Año 2021
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



We find that the southern section of the Patagonian Ice Sheet was more extensive during Marine Isotope Stage 4 (MIS 4) than during MIS 2, representing the first direct dating of the MIS 4 glacier culmination in South America. Similar to the MIS 2 glacial maxima, within MIS 4 there were multiple advances that we date (n = 6 samples) to between 67.5 +/- 2.1 and 62.1 +/- 2.0 ka. A similarly timed MIS 4 advance was identified in New Zealand, indicating that this is a hemisphere-wide glacier-climate signal, which is further corroborated by South Atlantic and Pacific temperature proxy records. Inboard of the MIS 4 moraine complex, we date a sequence of geomorphically distinct MIS 2 moraines that represent separate major periods of glacial stability. The MIS 2 maximum extent occurred by 27.4 +/- 0.8 ka (n = 4; arithmetic mean, with the standard error of the mean and 3% propagated production rate error) and was followed by at least four more full glacial culminations at 25.7 +/- 0.8 (n = 3), 23.9 +/- 0.8 (n = 5), 19.1 +/- 0.7 (n = 3), and 18.1 +/- 0.6 ka (n = 3), which represent periods when the glacier was in equilibrium with the climate for long enough to form major moraines. About 18 km inboard, this sequence is followed by smaller-scale recessional moraine crests, deposited on drumlinized terrain rather than a moraine drift, that we date to 18.0 +/- 0.8 ka, indicating the glacier was in net retreat at this time. Tentative results from a 2D ice sheet model suggest that the Magallanes lobe may have reached mapped inner and outer MIS 2 moraines from a climate with approximately 4.5 degrees C and 5.5 degrees C cooler summers, respectively, assuming similar to 25% less annual precipitation, relative to modern climate. We hypothesize that during the last glacial cycle, shifts in the subtropical and subantarctic fronts, and related ocean-atmosphere patterns, explain MIS 4 to 2 glacial behavior in the southern mid-latitudes. (C) 2021 Elsevier Ltd. All rights reserved.

Revista



Revista ISSN
Quaternary Science Reviews 0277-3791

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Disciplinas de Investigación



WOS
Geosciences, Multidisciplinary
Geography, Physical
Scopus
Geology
Archeology (Arts And Humanities)
Archeology
Global And Planetary Change
Ecology, Evolution, Behavior And Systematics
SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 Peltier, Carly Mujer Columbia Univ - Estados Unidos
Columbia University - Estados Unidos
Lamont-Doherty Earth Observatory - Estados Unidos
2 Kaplan, Michael Hombre Columbia Univ - Estados Unidos
Lamont-Doherty Earth Observatory - Estados Unidos
Columbia University - Estados Unidos
3 Birkel, Sean D. Hombre UNIV MAINE - Estados Unidos
University of Maine - Estados Unidos
4 Soteres, Rodrigo L. Hombre Pontificia Universidad Católica de Chile - Chile
Universidad de Chile - Chile
5 SAGREDO-TAPIA, ESTEBAN ANDRES Hombre Pontificia Universidad Católica de Chile - Chile
Universidad de Chile - Chile
6 ARAVENA-DONAIRE, JUAN CARLOS Hombre Universidad de Magallanes - Chile
7 ARAOS-ESPINOZA, JOSE MIGUEL Hombre Universidad Alberto Hurtado - Chile
University Alberto Hurtado - Chile
8 MORENO-MONCADA, PATRICIO IVAN Hombre Universidad de Chile - Chile
9 SCHWARTZ-ALDEA, RODRIGO JORGE Hombre Columbia Univ - Estados Unidos
Lamont-Doherty Earth Observatory - Estados Unidos
Columbia University - Estados Unidos
10 Schaefer, J. M. - Columbia Univ - Estados Unidos
Columbia University - Estados Unidos
Lamont-Doherty Earth Observatory - Estados Unidos

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Financiamiento



Fuente
FONDECYT
CONICYT
National Science Foundation
Fondo Nacional de Desarrollo Científico y Tecnológico
National Aeronautics and Space Administration
Lamont-Doherty Earth Observatory, Columbia University
DRI
NSF-BCS
ANID Millennium Science Initiative/Millennium Nucleus Paleoclimate
Fulbright U.S. Student Grant
National Science Foundation, NSF-BCS
NASA GISS Climate Center
LDEO

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



Agradecimiento
This work was supported by the National Science Foundation, NSF-BCS #1263474 (Kaplan, Schaefer) and #1263574 (Birkel) and the LDEO and NASA GISS Climate Center. This work was also supported by funding from Fondecyt 1191435, DRI USA2013-0035, and the ANID Millennium Science Initiative/Millennium Nucleus Paleoclimate NCN17_079 (Moreno, Sagredo, Soteres). We also acknowledge the Fulbright Commission Visiting Scholar Grant (Kaplan), and Fulbright U.S. Student Grant (Peltier), and the National Ph.D. Fellowship grant CONICYT #21161417 (Soteres).
This work was supported by the National Science Foundation , NSF-BCS #1263474 (Kaplan, Schaefer) and # 1263574 (Birkel) and the LDEO and NASA GISS Climate Center. This work was also supported by funding from Fondecyt 1191435 , DRI USA2013-0035 , and the ANID Millennium Science Initiative/Millennium Nucleus Paleoclimate NCN17_079 (Moreno, Sagredo, Soteres). We also acknowledge the Fulbright Commission Visiting Scholar Grant (Kaplan), and Fulbright U.S . Student Grant (Peltier), and the National Ph.D. Fellowship grant CONICYT # 21161417 (Soteres).

Muestra la fuente de financiamiento declarada en la publicación.