Deep ice as a geochemical reactor: insights from iron speciation and mineralogy of dust in the Talos Dome ice core (East Antarctica)

Thanks to its insolubility, mineral dust is considered a stable proxy in polar ice cores. With this study we show that below an ice-depth of 1000 m, the Talos Dome ice core (Ross Sea sector of East Antarctica) presents evident and progressive signs of post-depositional processes affecting the minera...

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Main Authors: Baccolo, Giovanni, Delmonte, Barbara, Stefano, Elena, Cibin, Giannantonio, Crotti, Ilaria, Frezzotti, Massimo, Hampai, Dariush, Iizuka, Yoshinori, Marcelli, Augusto, Maggi, Valter
Format: Text
Language:English
Published: 2021
Subjects:
Online Access:https://doi.org/10.5194/tc-2021-162
https://tc.copernicus.org/preprints/tc-2021-162/
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spelling ftcopernicus:oai:publications.copernicus.org:tcd94853 2023-05-15T14:02:17+02:00 Deep ice as a geochemical reactor: insights from iron speciation and mineralogy of dust in the Talos Dome ice core (East Antarctica) Baccolo, Giovanni Delmonte, Barbara Stefano, Elena Cibin, Giannantonio Crotti, Ilaria Frezzotti, Massimo Hampai, Dariush Iizuka, Yoshinori Marcelli, Augusto Maggi, Valter 2021-06-29 application/pdf https://doi.org/10.5194/tc-2021-162 https://tc.copernicus.org/preprints/tc-2021-162/ eng eng doi:10.5194/tc-2021-162 https://tc.copernicus.org/preprints/tc-2021-162/ eISSN: 1994-0424 Text 2021 ftcopernicus https://doi.org/10.5194/tc-2021-162 2021-07-05T16:22:15Z Thanks to its insolubility, mineral dust is considered a stable proxy in polar ice cores. With this study we show that below an ice-depth of 1000 m, the Talos Dome ice core (Ross Sea sector of East Antarctica) presents evident and progressive signs of post-depositional processes affecting the mineral dust records. We applied a suite of established and cutting edge techniques to investigate the properties of dust present in the Talos Dome ice core, ranging from concentration and grain-size to elemental-composition and Fe-mineralogy. Results show that through acidic/oxidative weathering, the conditions of deep ice at Talos Dome promote the dissolution of specific minerals and the englacial formation of others, deeply affecting dust primitive features. The expulsion of acidic atmospheric species from ice-grains and their concentration in localized environments is likely the main process responsible for englacial reactions and is related with ice re-crystallization. Deep ice can be seen as a "geochemical reactor" capable of fostering complex reactions which involve both soluble and insoluble impurities. Fe-bearing minerals can efficiently be used to explore such transformations. Text Antarc* Antarctica East Antarctica ice core Ross Sea Copernicus Publications: E-Journals East Antarctica Ross Sea Talos Dome ENVELOPE(158.000,158.000,-73.000,-73.000)
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description Thanks to its insolubility, mineral dust is considered a stable proxy in polar ice cores. With this study we show that below an ice-depth of 1000 m, the Talos Dome ice core (Ross Sea sector of East Antarctica) presents evident and progressive signs of post-depositional processes affecting the mineral dust records. We applied a suite of established and cutting edge techniques to investigate the properties of dust present in the Talos Dome ice core, ranging from concentration and grain-size to elemental-composition and Fe-mineralogy. Results show that through acidic/oxidative weathering, the conditions of deep ice at Talos Dome promote the dissolution of specific minerals and the englacial formation of others, deeply affecting dust primitive features. The expulsion of acidic atmospheric species from ice-grains and their concentration in localized environments is likely the main process responsible for englacial reactions and is related with ice re-crystallization. Deep ice can be seen as a "geochemical reactor" capable of fostering complex reactions which involve both soluble and insoluble impurities. Fe-bearing minerals can efficiently be used to explore such transformations.
format Text
author Baccolo, Giovanni
Delmonte, Barbara
Stefano, Elena
Cibin, Giannantonio
Crotti, Ilaria
Frezzotti, Massimo
Hampai, Dariush
Iizuka, Yoshinori
Marcelli, Augusto
Maggi, Valter
spellingShingle Baccolo, Giovanni
Delmonte, Barbara
Stefano, Elena
Cibin, Giannantonio
Crotti, Ilaria
Frezzotti, Massimo
Hampai, Dariush
Iizuka, Yoshinori
Marcelli, Augusto
Maggi, Valter
Deep ice as a geochemical reactor: insights from iron speciation and mineralogy of dust in the Talos Dome ice core (East Antarctica)
author_facet Baccolo, Giovanni
Delmonte, Barbara
Stefano, Elena
Cibin, Giannantonio
Crotti, Ilaria
Frezzotti, Massimo
Hampai, Dariush
Iizuka, Yoshinori
Marcelli, Augusto
Maggi, Valter
author_sort Baccolo, Giovanni
title Deep ice as a geochemical reactor: insights from iron speciation and mineralogy of dust in the Talos Dome ice core (East Antarctica)
title_short Deep ice as a geochemical reactor: insights from iron speciation and mineralogy of dust in the Talos Dome ice core (East Antarctica)
title_full Deep ice as a geochemical reactor: insights from iron speciation and mineralogy of dust in the Talos Dome ice core (East Antarctica)
title_fullStr Deep ice as a geochemical reactor: insights from iron speciation and mineralogy of dust in the Talos Dome ice core (East Antarctica)
title_full_unstemmed Deep ice as a geochemical reactor: insights from iron speciation and mineralogy of dust in the Talos Dome ice core (East Antarctica)
title_sort deep ice as a geochemical reactor: insights from iron speciation and mineralogy of dust in the talos dome ice core (east antarctica)
publishDate 2021
url https://doi.org/10.5194/tc-2021-162
https://tc.copernicus.org/preprints/tc-2021-162/
long_lat ENVELOPE(158.000,158.000,-73.000,-73.000)
geographic East Antarctica
Ross Sea
Talos Dome
geographic_facet East Antarctica
Ross Sea
Talos Dome
genre Antarc*
Antarctica
East Antarctica
ice core
Ross Sea
genre_facet Antarc*
Antarctica
East Antarctica
ice core
Ross Sea
op_source eISSN: 1994-0424
op_relation doi:10.5194/tc-2021-162
https://tc.copernicus.org/preprints/tc-2021-162/
op_doi https://doi.org/10.5194/tc-2021-162
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