10Be in Australasian microtektites compared to tektites: Size and geographic controls

High 10Be contents in tektites reported in literature are taken as evidence of a source material, melted at the impact site, enriched in atmospheric 10Be; i.e., a soil or sediment. In 0.8 Ma Australasian tektites, 10Be content increases with distance from the putative impact location in Indochina, w...

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Published in:Geology
Main Authors: P. Rochette, R. Braucher, L. Folco, C. S. Horng, G. Aumaître, D. L. Bourlès, K. Keddadouche
Other Authors: Rochette, P., Braucher, R., Folco, L., Horng, C. S., Aumaître, G., Bourlès, D. L., Keddadouche, K.
Format: Article in Journal/Newspaper
Language:English
Published: 2018
Subjects:
Online Access:http://hdl.handle.net/11568/928454
https://doi.org/10.1130/G45038.1
https://pubs.geoscienceworld.org/gsa/geology/article/46/9/803/545183/10Be-in-Australasian-microtektites-compared-to
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spelling ftunivpisairis:oai:arpi.unipi.it:11568/928454 2024-04-14T08:04:03+00:00 10Be in Australasian microtektites compared to tektites: Size and geographic controls P. Rochette R. Braucher L. Folco C. S. Horng G. Aumaître D. L. Bourlès K. Keddadouche Rochette, P. Braucher, R. Folco, L. Horng, C. S. Aumaître, G. Bourlès, D. L. Keddadouche, K. 2018 STAMPA http://hdl.handle.net/11568/928454 https://doi.org/10.1130/G45038.1 https://pubs.geoscienceworld.org/gsa/geology/article/46/9/803/545183/10Be-in-Australasian-microtektites-compared-to eng eng info:eu-repo/semantics/altIdentifier/wos/WOS:000442904600019 volume:46 firstpage:803 lastpage:806 numberofpages:4 journal:GEOLOGY http://hdl.handle.net/11568/928454 doi:10.1130/G45038.1 info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-85054133486 https://pubs.geoscienceworld.org/gsa/geology/article/46/9/803/545183/10Be-in-Australasian-microtektites-compared-to info:eu-repo/semantics/openAccess info:eu-repo/semantics/article 2018 ftunivpisairis https://doi.org/10.1130/G45038.1 2024-03-21T19:02:25Z High 10Be contents in tektites reported in literature are taken as evidence of a source material, melted at the impact site, enriched in atmospheric 10Be; i.e., a soil or sediment. In 0.8 Ma Australasian tektites, 10Be content increases with distance from the putative impact location in Indochina, with geographic averages from 69 × 106 atoms/g (Indochina) to 136 × 106 atoms/g (Australia). Here we report, for the first time, 10Be contents in microtektites collected from Antarctica and the South China Sea. We show that microtektites are ~30 × 106 atoms/g richer in 10Be than tektites from the same geographic areas. Antarctic microtektites, with an average 10Be content of 184 × 106 atoms/g after correction for in situ production, are the richest impact glass ever measured. The simplest explanation for such systematic size and geographic trends is that the source depth of the melt within the target surface decreases with ejection velocity. Indeed, higher initial kinetic energy implies higher launch distances and higher fragmentation of the ejecta. Antarctic microtektite source depth may tentatively be restricted to the upper tens of centimeters at the impact site. Alternative models invoking a marine or loessic sediment source, or a secondary enrichment in the microtektite (either by atmospheric scavenging, selective fractionation by volatilization, or post-depositional contamination) fail to reproduce the observed relationships. Article in Journal/Newspaper Antarc* Antarctic Antarctica ARPI - Archivio della Ricerca dell'Università di Pisa Antarctic Geology 46 9 803 806
institution Open Polar
collection ARPI - Archivio della Ricerca dell'Università di Pisa
op_collection_id ftunivpisairis
language English
description High 10Be contents in tektites reported in literature are taken as evidence of a source material, melted at the impact site, enriched in atmospheric 10Be; i.e., a soil or sediment. In 0.8 Ma Australasian tektites, 10Be content increases with distance from the putative impact location in Indochina, with geographic averages from 69 × 106 atoms/g (Indochina) to 136 × 106 atoms/g (Australia). Here we report, for the first time, 10Be contents in microtektites collected from Antarctica and the South China Sea. We show that microtektites are ~30 × 106 atoms/g richer in 10Be than tektites from the same geographic areas. Antarctic microtektites, with an average 10Be content of 184 × 106 atoms/g after correction for in situ production, are the richest impact glass ever measured. The simplest explanation for such systematic size and geographic trends is that the source depth of the melt within the target surface decreases with ejection velocity. Indeed, higher initial kinetic energy implies higher launch distances and higher fragmentation of the ejecta. Antarctic microtektite source depth may tentatively be restricted to the upper tens of centimeters at the impact site. Alternative models invoking a marine or loessic sediment source, or a secondary enrichment in the microtektite (either by atmospheric scavenging, selective fractionation by volatilization, or post-depositional contamination) fail to reproduce the observed relationships.
author2 Rochette, P.
Braucher, R.
Folco, L.
Horng, C. S.
Aumaître, G.
Bourlès, D. L.
Keddadouche, K.
format Article in Journal/Newspaper
author P. Rochette
R. Braucher
L. Folco
C. S. Horng
G. Aumaître
D. L. Bourlès
K. Keddadouche
spellingShingle P. Rochette
R. Braucher
L. Folco
C. S. Horng
G. Aumaître
D. L. Bourlès
K. Keddadouche
10Be in Australasian microtektites compared to tektites: Size and geographic controls
author_facet P. Rochette
R. Braucher
L. Folco
C. S. Horng
G. Aumaître
D. L. Bourlès
K. Keddadouche
author_sort P. Rochette
title 10Be in Australasian microtektites compared to tektites: Size and geographic controls
title_short 10Be in Australasian microtektites compared to tektites: Size and geographic controls
title_full 10Be in Australasian microtektites compared to tektites: Size and geographic controls
title_fullStr 10Be in Australasian microtektites compared to tektites: Size and geographic controls
title_full_unstemmed 10Be in Australasian microtektites compared to tektites: Size and geographic controls
title_sort 10be in australasian microtektites compared to tektites: size and geographic controls
publishDate 2018
url http://hdl.handle.net/11568/928454
https://doi.org/10.1130/G45038.1
https://pubs.geoscienceworld.org/gsa/geology/article/46/9/803/545183/10Be-in-Australasian-microtektites-compared-to
geographic Antarctic
geographic_facet Antarctic
genre Antarc*
Antarctic
Antarctica
genre_facet Antarc*
Antarctic
Antarctica
op_relation info:eu-repo/semantics/altIdentifier/wos/WOS:000442904600019
volume:46
firstpage:803
lastpage:806
numberofpages:4
journal:GEOLOGY
http://hdl.handle.net/11568/928454
doi:10.1130/G45038.1
info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-85054133486
https://pubs.geoscienceworld.org/gsa/geology/article/46/9/803/545183/10Be-in-Australasian-microtektites-compared-to
op_rights info:eu-repo/semantics/openAccess
op_doi https://doi.org/10.1130/G45038.1
container_title Geology
container_volume 46
container_issue 9
container_start_page 803
op_container_end_page 806
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