What is the real isotopic signature of dust emitted from Tierra del Fuego?

Fil: Gaiero, D.M. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro de Investigaciones en Ciencias de la Tierra; Argentina.

Detalles Bibliográficos
Autores principales: Gaiero, D. M., Gili, S., Strelin, J., Koestner, E., Chemale Jr, F.
Formato: conferenceObject
Lenguaje:Inglés
Publicado: 2024
Materias:
Acceso en línea:http://hdl.handle.net/11086/551431
Aporte de:
id I10-R141-11086-551431
record_format dspace
institution Universidad Nacional de Córdoba
institution_str I-10
repository_str R-141
collection Repositorio Digital Universitario (UNC)
language Inglés
topic Ciencias de la Tierra
Geociencias
Geología isotópica
Antártica
spellingShingle Ciencias de la Tierra
Geociencias
Geología isotópica
Antártica
Gaiero, D. M.
Gili, S.
Strelin, J.
Koestner, E.
Chemale Jr, F.
What is the real isotopic signature of dust emitted from Tierra del Fuego?
topic_facet Ciencias de la Tierra
Geociencias
Geología isotópica
Antártica
description Fil: Gaiero, D.M. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro de Investigaciones en Ciencias de la Tierra; Argentina.
format conferenceObject
author Gaiero, D. M.
Gili, S.
Strelin, J.
Koestner, E.
Chemale Jr, F.
author_facet Gaiero, D. M.
Gili, S.
Strelin, J.
Koestner, E.
Chemale Jr, F.
author_sort Gaiero, D. M.
title What is the real isotopic signature of dust emitted from Tierra del Fuego?
title_short What is the real isotopic signature of dust emitted from Tierra del Fuego?
title_full What is the real isotopic signature of dust emitted from Tierra del Fuego?
title_fullStr What is the real isotopic signature of dust emitted from Tierra del Fuego?
title_full_unstemmed What is the real isotopic signature of dust emitted from Tierra del Fuego?
title_sort what is the real isotopic signature of dust emitted from tierra del fuego?
publishDate 2024
url http://hdl.handle.net/11086/551431
work_keys_str_mv AT gaierodm whatistherealisotopicsignatureofdustemittedfromtierradelfuego
AT gilis whatistherealisotopicsignatureofdustemittedfromtierradelfuego
AT strelinj whatistherealisotopicsignatureofdustemittedfromtierradelfuego
AT koestnere whatistherealisotopicsignatureofdustemittedfromtierradelfuego
AT chemalejrf whatistherealisotopicsignatureofdustemittedfromtierradelfuego
_version_ 1806948846292434944
spelling I10-R141-11086-5514312024-04-17T19:32:42Z What is the real isotopic signature of dust emitted from Tierra del Fuego? Gaiero, D. M. Gili, S. Strelin, J. Koestner, E. Chemale Jr, F. Ciencias de la Tierra Geociencias Geología isotópica Antártica Fil: Gaiero, D.M. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro de Investigaciones en Ciencias de la Tierra; Argentina. Fil: Gili, S. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro de Investigaciones en Ciencias de la Tierra; Argentina. Fil: Strelin, J. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro de Investigaciones en Ciencias de la Tierra; Argentina. Fil: Strelin, J. Universidad Nacional de Córdoba. Facultad de Ciencias Exactas, Físicas y Naturales. Instituto Antártico Argentino; Argentina. Fil: Koestner, E. IG-UFRGS. Laboratório de Geología Isotópica; Brasil. Fil: Chemale Jr, F. IG-UFRGS. Laboratório de Geología Isotópica; Brasil. Sugden et al. (2009) suggested an on/off switch mechanism that could explain the 20 times increase of dust deposition in Antarctica during the Last Glacial Maximum (LGM), as compared to present day. This suggested switch resides in Patagonian pro-glacial lakes; when glaciers retreat sediments are deposited in the lakes and dust emission ceased in opposition to cold periods, when glacial pour out sediments to the outwash plain, then increasing dust emission. The on/off switch mechanism proposed is supported on age analyses and strontium (Sr) and neodymium (Nd) isotope ratios of ancient lacustrine sediment samples from the Magellan Strait (MS) and from the North Patagonian icefield (NPI). The lacustrine sediments were used as representative of sediments that were disgorged to the outwash plain during the LGM. We argue on the type of samples used to characterize the possible Patagonian outwash sediments deflated during the LGM and accordingly, on the interpretation of the source of this dust. Modern sediments are deflated from the Patagonian surface mainly from widespread ephemeral lakes (Gaiero 2007), which are sporadically refilled with sediments supplied from the surrounding areas mainly through water runoff. The aim of this contribution is to discuss about this and contrast data from both set of samples and discuss about their significance for the interpretation of the isotopic signatures recorded on the sedimentary archives of the Southern Hemisphere (e.g., Antarctic ice cores). Fig. 1 shows that the mean isotopic composition of dry lake sediments (collected from the ancient outwash plain in the San Sebastián Bay area) and dust collected at Río Grande are significantly different compared to MS samples and very similar to sediments representing the Fuegian continental shelf (Basile et al. 2007). Similar to modern dust released from continental Patagonia (north of ~52° S), modern data from Tierra del Fuego could also be explained by a mixing between Jurassic rhyolites and Quaternary volcanic rocks (e.g., Gaiero et al. 2007; Fig. 1). On the contrary, the samples used by Sugden et al. (2009) seem to characterize discrete sources. The isotopic composition of most samples from the MS plots mostly within the compositional field corresponding to the Antarctic Jurassic rhyolites and similar rocks that outcrop out close along the Fuegian Cordillera (Gaiero et al. 2007). In the case of NPI samples, their compositions are similar to the local outcropping Paleozoic plutonic and metasedimentary rocks (Killian and Behrmann 2003). Nevertheless, directly to the W of the NPI, the isotopic composition of Pliocene/Pleistocene Chilean trench sediments (mean 87Sr/86Sr = 0.707 and δNd(0) = -2.1) indicates a variable contribution from other rocks cropping out in the area (e.g., Quaternary volcanic rocks). Why MS and NPI samples are different from modern Patagonian dust? Fil: Gaiero, D.M. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro de Investigaciones en Ciencias de la Tierra; Argentina. Fil: Gili, S. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro de Investigaciones en Ciencias de la Tierra; Argentina. Fil: Strelin, J. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro de Investigaciones en Ciencias de la Tierra; Argentina. Fil: Strelin, J. Universidad Nacional de Córdoba. Facultad de Ciencias Exactas, Físicas y Naturales. Instituto Antártico Argentino; Argentina. Fil: Koestner, E. IG-UFRGS. Laboratório de Geología Isotópica; Brasil. Fil: Chemale Jr, F. IG-UFRGS. Laboratório de Geología Isotópica; Brasil. Geoquímica y Geofísica 2024-04-16T12:04:13Z 2024-04-16T12:04:13Z 2015 conferenceObject http://hdl.handle.net/11086/551431 eng Attribution-NonCommercial-ShareAlike 4.0 International http://creativecommons.org/licenses/by-nc-sa/4.0/ Impreso