Relationship between meteoric 10Be and NO3− concentrations in soils along Shackleton Glacier, Antarctica

Outlet glaciers that flow through the Transantarctic Mountains (TAM) experienced changes in ice thickness greater than other coastal regions of Antarctica during glacial maxima. As a result, ice-free areas that are currently exposed may have been covered by ice at various points during the Cenozoic,...

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Published in:Earth Surface Dynamics
Main Authors: Diaz, Melisa A., Corbett, Lee B., Bierman, Paul R., Adams, Byron J., Wall, Diana H., Hogg, Ian D., Fierer, Noah, Lyons, W. Berry
Format: Text
Language:English
Published: 2021
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Online Access:https://doi.org/10.5194/esurf-9-1363-2021
https://esurf.copernicus.org/articles/9/1363/2021/
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description Outlet glaciers that flow through the Transantarctic Mountains (TAM) experienced changes in ice thickness greater than other coastal regions of Antarctica during glacial maxima. As a result, ice-free areas that are currently exposed may have been covered by ice at various points during the Cenozoic, complicating our understanding of ecological succession in TAM soils. Our knowledge of glacial extent on small spatial scales is limited for the TAM, and studies of soil exposure duration and disturbance, in particular, are rare. We collected surface soil samples and, in some places, depth profiles every 5 cm to refusal (up to 30 cm) from 11 ice-free areas along Shackleton Glacier, a major outlet glacier of the East Antarctic Ice Sheet. We explored the relationship between meteoric 10 Be and <math xmlns="http://www.w3.org/1998/Math/MathML" id="M6" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><msubsup><mi mathvariant="normal">NO</mi><mn mathvariant="normal">3</mn><mo>-</mo></msubsup></mrow></math> <svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="25pt" height="16pt" class="svg-formula" dspmath="mathimg" md5hash="a33a7d42b70ca1fe513ac92c5832eec2"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="esurf-9-1363-2021-ie00004.svg" width="25pt" height="16pt" src="esurf-9-1363-2021-ie00004.png"/></svg:svg> in these soils as a tool for understanding landscape disturbance and wetting history and as exposure proxies. Concentrations of meteoric 10 Be spanned more than an order of magnitude across the region ( 2.9×10 8 to 73×10 8 atoms g −1 ) and are among the highest measured in polar regions. The concentrations of <math xmlns="http://www.w3.org/1998/Math/MathML" id="M11" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><msubsup><mi mathvariant="normal">NO</mi><mn mathvariant="normal">3</mn><mo>-</mo></msubsup></mrow></math> <svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="25pt" height="16pt" class="svg-formula" dspmath="mathimg" md5hash="eb51cd45ba2a21283d090226a04e61ba"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="esurf-9-1363-2021-ie00005.svg" width="25pt" height="16pt" src="esurf-9-1363-2021-ie00005.png"/></svg:svg> were similarly variable and ranged from ∼1 µ g g −1 to 15 mg g −1 . In examining differences and similarities in the concentrations of 10 Be and <math xmlns="http://www.w3.org/1998/Math/MathML" id="M17" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><msubsup><mi mathvariant="normal">NO</mi><mn mathvariant="normal">3</mn><mo>-</mo></msubsup></mrow></math> <svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="25pt" height="16pt" class="svg-formula" dspmath="mathimg" md5hash="822fcc3376206f5298bc14405cca7022"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="esurf-9-1363-2021-ie00006.svg" width="25pt" height="16pt" src="esurf-9-1363-2021-ie00006.png"/></svg:svg> with depth, we suggest that much of the southern portion of the Shackleton Glacier region has likely developed under a hyper-arid climate regime with minimal disturbance. Finally, we inferred exposure time using 10 Be concentrations. This analysis indicates that the soils we analyzed likely range from recent exposure (following the Last Glacial Maximum) to possibly >6 Myr. We suggest that further testing and interrogation of meteoric 10 Be and <math xmlns="http://www.w3.org/1998/Math/MathML" id="M21" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><msubsup><mi mathvariant="normal">NO</mi><mn mathvariant="normal">3</mn><mo>-</mo></msubsup></mrow></math> <svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="25pt" height="16pt" class="svg-formula" dspmath="mathimg" md5hash="8a28d0a06c83cc478fcb3953dfc5e6ea"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="esurf-9-1363-2021-ie00007.svg" width="25pt" height="16pt" src="esurf-9-1363-2021-ie00007.png"/></svg:svg> concentrations and relationships in soils can provide important information regarding landscape development, soil evolution processes, and inferred exposure durations of surfaces in the TAM.
format Text
author Diaz, Melisa A.
Corbett, Lee B.
Bierman, Paul R.
Adams, Byron J.
Wall, Diana H.
Hogg, Ian D.
Fierer, Noah
Lyons, W. Berry
spellingShingle Diaz, Melisa A.
Corbett, Lee B.
Bierman, Paul R.
Adams, Byron J.
Wall, Diana H.
Hogg, Ian D.
Fierer, Noah
Lyons, W. Berry
Relationship between meteoric 10Be and NO3− concentrations in soils along Shackleton Glacier, Antarctica
author_facet Diaz, Melisa A.
Corbett, Lee B.
Bierman, Paul R.
Adams, Byron J.
Wall, Diana H.
Hogg, Ian D.
Fierer, Noah
Lyons, W. Berry
author_sort Diaz, Melisa A.
title Relationship between meteoric 10Be and NO3− concentrations in soils along Shackleton Glacier, Antarctica
title_short Relationship between meteoric 10Be and NO3− concentrations in soils along Shackleton Glacier, Antarctica
title_full Relationship between meteoric 10Be and NO3− concentrations in soils along Shackleton Glacier, Antarctica
title_fullStr Relationship between meteoric 10Be and NO3− concentrations in soils along Shackleton Glacier, Antarctica
title_full_unstemmed Relationship between meteoric 10Be and NO3− concentrations in soils along Shackleton Glacier, Antarctica
title_sort relationship between meteoric 10be and no3− concentrations in soils along shackleton glacier, antarctica
publishDate 2021
url https://doi.org/10.5194/esurf-9-1363-2021
https://esurf.copernicus.org/articles/9/1363/2021/
long_lat ENVELOPE(-37.200,-37.200,-54.133,-54.133)
geographic Antarctic
East Antarctic Ice Sheet
Shackleton
Shackleton Glacier
Transantarctic Mountains
geographic_facet Antarctic
East Antarctic Ice Sheet
Shackleton
Shackleton Glacier
Transantarctic Mountains
genre Antarc*
Antarctic
Antarctica
Ice Sheet
Shackleton Glacier
genre_facet Antarc*
Antarctic
Antarctica
Ice Sheet
Shackleton Glacier
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op_doi https://doi.org/10.5194/esurf-9-1363-2021
container_title Earth Surface Dynamics
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spelling ftcopernicus:oai:publications.copernicus.org:esurf86244 2023-05-15T14:02:17+02:00 Relationship between meteoric 10Be and NO3− concentrations in soils along Shackleton Glacier, Antarctica Diaz, Melisa A. Corbett, Lee B. Bierman, Paul R. Adams, Byron J. Wall, Diana H. Hogg, Ian D. Fierer, Noah Lyons, W. Berry 2021-10-14 application/pdf https://doi.org/10.5194/esurf-9-1363-2021 https://esurf.copernicus.org/articles/9/1363/2021/ eng eng doi:10.5194/esurf-9-1363-2021 https://esurf.copernicus.org/articles/9/1363/2021/ eISSN: 2196-632X Text 2021 ftcopernicus https://doi.org/10.5194/esurf-9-1363-2021 2021-10-18T16:22:31Z Outlet glaciers that flow through the Transantarctic Mountains (TAM) experienced changes in ice thickness greater than other coastal regions of Antarctica during glacial maxima. As a result, ice-free areas that are currently exposed may have been covered by ice at various points during the Cenozoic, complicating our understanding of ecological succession in TAM soils. Our knowledge of glacial extent on small spatial scales is limited for the TAM, and studies of soil exposure duration and disturbance, in particular, are rare. We collected surface soil samples and, in some places, depth profiles every 5 cm to refusal (up to 30 cm) from 11 ice-free areas along Shackleton Glacier, a major outlet glacier of the East Antarctic Ice Sheet. We explored the relationship between meteoric 10 Be and <math xmlns="http://www.w3.org/1998/Math/MathML" id="M6" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><msubsup><mi mathvariant="normal">NO</mi><mn mathvariant="normal">3</mn><mo>-</mo></msubsup></mrow></math> <svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="25pt" height="16pt" class="svg-formula" dspmath="mathimg" md5hash="a33a7d42b70ca1fe513ac92c5832eec2"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="esurf-9-1363-2021-ie00004.svg" width="25pt" height="16pt" src="esurf-9-1363-2021-ie00004.png"/></svg:svg> in these soils as a tool for understanding landscape disturbance and wetting history and as exposure proxies. Concentrations of meteoric 10 Be spanned more than an order of magnitude across the region ( 2.9×10 8 to 73×10 8 atoms g −1 ) and are among the highest measured in polar regions. The concentrations of <math xmlns="http://www.w3.org/1998/Math/MathML" id="M11" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><msubsup><mi mathvariant="normal">NO</mi><mn mathvariant="normal">3</mn><mo>-</mo></msubsup></mrow></math> <svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="25pt" height="16pt" class="svg-formula" dspmath="mathimg" md5hash="eb51cd45ba2a21283d090226a04e61ba"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="esurf-9-1363-2021-ie00005.svg" width="25pt" height="16pt" src="esurf-9-1363-2021-ie00005.png"/></svg:svg> were similarly variable and ranged from ∼1 µ g g −1 to 15 mg g −1 . In examining differences and similarities in the concentrations of 10 Be and <math xmlns="http://www.w3.org/1998/Math/MathML" id="M17" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><msubsup><mi mathvariant="normal">NO</mi><mn mathvariant="normal">3</mn><mo>-</mo></msubsup></mrow></math> <svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="25pt" height="16pt" class="svg-formula" dspmath="mathimg" md5hash="822fcc3376206f5298bc14405cca7022"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="esurf-9-1363-2021-ie00006.svg" width="25pt" height="16pt" src="esurf-9-1363-2021-ie00006.png"/></svg:svg> with depth, we suggest that much of the southern portion of the Shackleton Glacier region has likely developed under a hyper-arid climate regime with minimal disturbance. Finally, we inferred exposure time using 10 Be concentrations. This analysis indicates that the soils we analyzed likely range from recent exposure (following the Last Glacial Maximum) to possibly >6 Myr. We suggest that further testing and interrogation of meteoric 10 Be and <math xmlns="http://www.w3.org/1998/Math/MathML" id="M21" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><msubsup><mi mathvariant="normal">NO</mi><mn mathvariant="normal">3</mn><mo>-</mo></msubsup></mrow></math> <svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="25pt" height="16pt" class="svg-formula" dspmath="mathimg" md5hash="8a28d0a06c83cc478fcb3953dfc5e6ea"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="esurf-9-1363-2021-ie00007.svg" width="25pt" height="16pt" src="esurf-9-1363-2021-ie00007.png"/></svg:svg> concentrations and relationships in soils can provide important information regarding landscape development, soil evolution processes, and inferred exposure durations of surfaces in the TAM. Text Antarc* Antarctic Antarctica Ice Sheet Shackleton Glacier Copernicus Publications: E-Journals Antarctic East Antarctic Ice Sheet Shackleton Shackleton Glacier ENVELOPE(-37.200,-37.200,-54.133,-54.133) Transantarctic Mountains Earth Surface Dynamics 9 5 1363 1380