Noble gas composition of subcontinental lithospheric mantle: An extensively degassed reservoir beneath Southern Patagonia

Autores
Jalowitzki, Tiago; Sumino, Hirochika; Conceiçao, Rommulo V.; Orihashi, Yuji; Nagao, Keisuke; Bertotto, Gustavo Walter; Balbinot, Eduardo; Schilling, Manuel R; Gervasoni, Fernanda
Año de publicación
2016
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Patagonia, in the Southern Andes, is one of the few locations where interactions between the oceanic and continental lithosphere can be studied due to subduction of an active spreading ridge beneath the continent. In order to characterize the noble gas composition of Patagonian subcontinental lithospheric mantle (SCLM), we present the first noble gas data alongside new lithophile (Sr-Nd-Pb) isotopic data for mantle xenoliths from Pali-Aike Volcanic Field and Gobernador Gregores, Southern Patagonia. Based on noble gas isotopic compositions, Pali-Aike mantle xenoliths represent intrinsic SCLM with higher (U+Th+K)/(3He, 22Ne, 36Ar) ratios than the mid-ocean ridge basalt (MORB) source. This reservoir shows slightly radiogenic helium (3He/4He =6.84-6.90 RA), coupled with a strongly nucleogenic neon signature (mantle source 21Ne/22Ne =0.085-0.094). The 40Ar/36Ar ratios vary from a near-atmospheric ratio of 510 up to 17700, with mantle source 40Ar/36Ar between 31100+9400−6800 and 54000+14200−9600. In addition, the 3He/22Ne ratios for the local SCLM endmember, at 12.03 ±0.15 to 13.66 ±0.37, are higher than depleted MORBs, at 3He/22Ne =8.31-9.75. Although asthenospheric mantle upwelling through the Patagonian slab window would result in a MORB-like metasomatism after collision of the South Chile Ridge with the Chile trench ca. 14 Ma, this mantle reservoir could have remained unhomogenized after rapid passage and northward migration of the Chile Triple Junction. The mantle endmember xenon isotopic ratios of Pali-Aike mantle xenoliths, which is first defined for any SCLM-derived samples, show values indistinguishable from the MORB source (129Xe/132Xe=1.0833+0.0216−0.0053 and 136Xe/132Xe=0.3761+0.0246−0.0034).The noble gas component observed in Gobernador Gregores mantle xenoliths is characterized by isotopic compositions in the MORB range in terms of helium (3He/4He =7.17-7.37 RA), but with slightly nucleogenic neon (mantle source 21Ne/22Ne =0.065-0.079). We suggest that this MORB-like metasomatism was capable of overprinting the noble gas composition of Gobernador Gregores due to recent metasomatism of the SCLM because of asthenospheric mantle upwelling in response to opening of the Patagonian slab window. The 40Ar/36Ar ratios vary from a near-atmospheric ratio of 380 up to 6560, with mantle source 40Ar/36Ar between 8100+1400−700 and 17700+4400−3100. The lower 40Ar/36Ar ratio of the Gobernador Gregores mantle source, compared with that of Pali-Aike, attests that the Patagonia SCLM was affected significantly by atmospheric contamination associated with the recycled oceanic lithosphere.
Fil: Jalowitzki, Tiago. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Sumino, Hirochika. University of Tokyo; Japón
Fil: Conceiçao, Rommulo V.. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Orihashi, Yuji. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. University of Tokyo; Japón
Fil: Nagao, Keisuke. University of Tokyo; Japón
Fil: Bertotto, Gustavo Walter. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de La Pampa; Argentina
Fil: Balbinot, Eduardo. University of Surrey; Reino Unido
Fil: Schilling, Manuel R. Universidad Austral de Chile; Chile
Fil: Gervasoni, Fernanda. Universität Münster; Alemania
Materia
Noble Gas Isotopes
Subcontinental Lithospheric Mantle
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/44159

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network_name_str CONICET Digital (CONICET)
spelling Noble gas composition of subcontinental lithospheric mantle: An extensively degassed reservoir beneath Southern PatagoniaJalowitzki, TiagoSumino, HirochikaConceiçao, Rommulo V.Orihashi, YujiNagao, KeisukeBertotto, Gustavo WalterBalbinot, EduardoSchilling, Manuel RGervasoni, FernandaNoble Gas IsotopesSubcontinental Lithospheric Mantlehttps://purl.org/becyt/ford/1.5https://purl.org/becyt/ford/1Patagonia, in the Southern Andes, is one of the few locations where interactions between the oceanic and continental lithosphere can be studied due to subduction of an active spreading ridge beneath the continent. In order to characterize the noble gas composition of Patagonian subcontinental lithospheric mantle (SCLM), we present the first noble gas data alongside new lithophile (Sr-Nd-Pb) isotopic data for mantle xenoliths from Pali-Aike Volcanic Field and Gobernador Gregores, Southern Patagonia. Based on noble gas isotopic compositions, Pali-Aike mantle xenoliths represent intrinsic SCLM with higher (U+Th+K)/(3He, 22Ne, 36Ar) ratios than the mid-ocean ridge basalt (MORB) source. This reservoir shows slightly radiogenic helium (3He/4He =6.84-6.90 RA), coupled with a strongly nucleogenic neon signature (mantle source 21Ne/22Ne =0.085-0.094). The 40Ar/36Ar ratios vary from a near-atmospheric ratio of 510 up to 17700, with mantle source 40Ar/36Ar between 31100+9400−6800 and 54000+14200−9600. In addition, the 3He/22Ne ratios for the local SCLM endmember, at 12.03 ±0.15 to 13.66 ±0.37, are higher than depleted MORBs, at 3He/22Ne =8.31-9.75. Although asthenospheric mantle upwelling through the Patagonian slab window would result in a MORB-like metasomatism after collision of the South Chile Ridge with the Chile trench ca. 14 Ma, this mantle reservoir could have remained unhomogenized after rapid passage and northward migration of the Chile Triple Junction. The mantle endmember xenon isotopic ratios of Pali-Aike mantle xenoliths, which is first defined for any SCLM-derived samples, show values indistinguishable from the MORB source (129Xe/132Xe=1.0833+0.0216−0.0053 and 136Xe/132Xe=0.3761+0.0246−0.0034).The noble gas component observed in Gobernador Gregores mantle xenoliths is characterized by isotopic compositions in the MORB range in terms of helium (3He/4He =7.17-7.37 RA), but with slightly nucleogenic neon (mantle source 21Ne/22Ne =0.065-0.079). We suggest that this MORB-like metasomatism was capable of overprinting the noble gas composition of Gobernador Gregores due to recent metasomatism of the SCLM because of asthenospheric mantle upwelling in response to opening of the Patagonian slab window. The 40Ar/36Ar ratios vary from a near-atmospheric ratio of 380 up to 6560, with mantle source 40Ar/36Ar between 8100+1400−700 and 17700+4400−3100. The lower 40Ar/36Ar ratio of the Gobernador Gregores mantle source, compared with that of Pali-Aike, attests that the Patagonia SCLM was affected significantly by atmospheric contamination associated with the recycled oceanic lithosphere.Fil: Jalowitzki, Tiago. Universidade Federal do Rio Grande do Sul; BrasilFil: Sumino, Hirochika. University of Tokyo; JapónFil: Conceiçao, Rommulo V.. Universidade Federal do Rio Grande do Sul; BrasilFil: Orihashi, Yuji. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. University of Tokyo; JapónFil: Nagao, Keisuke. University of Tokyo; JapónFil: Bertotto, Gustavo Walter. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de La Pampa; ArgentinaFil: Balbinot, Eduardo. University of Surrey; Reino UnidoFil: Schilling, Manuel R. Universidad Austral de Chile; ChileFil: Gervasoni, Fernanda. Universität Münster; AlemaniaElsevier Science2016-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/44159Jalowitzki, Tiago; Sumino, Hirochika; Conceiçao, Rommulo V.; Orihashi, Yuji; Nagao, Keisuke; et al.; Noble gas composition of subcontinental lithospheric mantle: An extensively degassed reservoir beneath Southern Patagonia; Elsevier Science; Earth and Planetary Science Letters; 450; 7-2016; 263-2730012-821XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1016/j.epsl.2016.06.034info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S0012821X16303211info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-03T09:52:11Zoai:ri.conicet.gov.ar:11336/44159instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-03 09:52:11.644CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Noble gas composition of subcontinental lithospheric mantle: An extensively degassed reservoir beneath Southern Patagonia
title Noble gas composition of subcontinental lithospheric mantle: An extensively degassed reservoir beneath Southern Patagonia
spellingShingle Noble gas composition of subcontinental lithospheric mantle: An extensively degassed reservoir beneath Southern Patagonia
Jalowitzki, Tiago
Noble Gas Isotopes
Subcontinental Lithospheric Mantle
title_short Noble gas composition of subcontinental lithospheric mantle: An extensively degassed reservoir beneath Southern Patagonia
title_full Noble gas composition of subcontinental lithospheric mantle: An extensively degassed reservoir beneath Southern Patagonia
title_fullStr Noble gas composition of subcontinental lithospheric mantle: An extensively degassed reservoir beneath Southern Patagonia
title_full_unstemmed Noble gas composition of subcontinental lithospheric mantle: An extensively degassed reservoir beneath Southern Patagonia
title_sort Noble gas composition of subcontinental lithospheric mantle: An extensively degassed reservoir beneath Southern Patagonia
dc.creator.none.fl_str_mv Jalowitzki, Tiago
Sumino, Hirochika
Conceiçao, Rommulo V.
Orihashi, Yuji
Nagao, Keisuke
Bertotto, Gustavo Walter
Balbinot, Eduardo
Schilling, Manuel R
Gervasoni, Fernanda
author Jalowitzki, Tiago
author_facet Jalowitzki, Tiago
Sumino, Hirochika
Conceiçao, Rommulo V.
Orihashi, Yuji
Nagao, Keisuke
Bertotto, Gustavo Walter
Balbinot, Eduardo
Schilling, Manuel R
Gervasoni, Fernanda
author_role author
author2 Sumino, Hirochika
Conceiçao, Rommulo V.
Orihashi, Yuji
Nagao, Keisuke
Bertotto, Gustavo Walter
Balbinot, Eduardo
Schilling, Manuel R
Gervasoni, Fernanda
author2_role author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Noble Gas Isotopes
Subcontinental Lithospheric Mantle
topic Noble Gas Isotopes
Subcontinental Lithospheric Mantle
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.5
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Patagonia, in the Southern Andes, is one of the few locations where interactions between the oceanic and continental lithosphere can be studied due to subduction of an active spreading ridge beneath the continent. In order to characterize the noble gas composition of Patagonian subcontinental lithospheric mantle (SCLM), we present the first noble gas data alongside new lithophile (Sr-Nd-Pb) isotopic data for mantle xenoliths from Pali-Aike Volcanic Field and Gobernador Gregores, Southern Patagonia. Based on noble gas isotopic compositions, Pali-Aike mantle xenoliths represent intrinsic SCLM with higher (U+Th+K)/(3He, 22Ne, 36Ar) ratios than the mid-ocean ridge basalt (MORB) source. This reservoir shows slightly radiogenic helium (3He/4He =6.84-6.90 RA), coupled with a strongly nucleogenic neon signature (mantle source 21Ne/22Ne =0.085-0.094). The 40Ar/36Ar ratios vary from a near-atmospheric ratio of 510 up to 17700, with mantle source 40Ar/36Ar between 31100+9400−6800 and 54000+14200−9600. In addition, the 3He/22Ne ratios for the local SCLM endmember, at 12.03 ±0.15 to 13.66 ±0.37, are higher than depleted MORBs, at 3He/22Ne =8.31-9.75. Although asthenospheric mantle upwelling through the Patagonian slab window would result in a MORB-like metasomatism after collision of the South Chile Ridge with the Chile trench ca. 14 Ma, this mantle reservoir could have remained unhomogenized after rapid passage and northward migration of the Chile Triple Junction. The mantle endmember xenon isotopic ratios of Pali-Aike mantle xenoliths, which is first defined for any SCLM-derived samples, show values indistinguishable from the MORB source (129Xe/132Xe=1.0833+0.0216−0.0053 and 136Xe/132Xe=0.3761+0.0246−0.0034).The noble gas component observed in Gobernador Gregores mantle xenoliths is characterized by isotopic compositions in the MORB range in terms of helium (3He/4He =7.17-7.37 RA), but with slightly nucleogenic neon (mantle source 21Ne/22Ne =0.065-0.079). We suggest that this MORB-like metasomatism was capable of overprinting the noble gas composition of Gobernador Gregores due to recent metasomatism of the SCLM because of asthenospheric mantle upwelling in response to opening of the Patagonian slab window. The 40Ar/36Ar ratios vary from a near-atmospheric ratio of 380 up to 6560, with mantle source 40Ar/36Ar between 8100+1400−700 and 17700+4400−3100. The lower 40Ar/36Ar ratio of the Gobernador Gregores mantle source, compared with that of Pali-Aike, attests that the Patagonia SCLM was affected significantly by atmospheric contamination associated with the recycled oceanic lithosphere.
Fil: Jalowitzki, Tiago. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Sumino, Hirochika. University of Tokyo; Japón
Fil: Conceiçao, Rommulo V.. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Orihashi, Yuji. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. University of Tokyo; Japón
Fil: Nagao, Keisuke. University of Tokyo; Japón
Fil: Bertotto, Gustavo Walter. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de La Pampa; Argentina
Fil: Balbinot, Eduardo. University of Surrey; Reino Unido
Fil: Schilling, Manuel R. Universidad Austral de Chile; Chile
Fil: Gervasoni, Fernanda. Universität Münster; Alemania
description Patagonia, in the Southern Andes, is one of the few locations where interactions between the oceanic and continental lithosphere can be studied due to subduction of an active spreading ridge beneath the continent. In order to characterize the noble gas composition of Patagonian subcontinental lithospheric mantle (SCLM), we present the first noble gas data alongside new lithophile (Sr-Nd-Pb) isotopic data for mantle xenoliths from Pali-Aike Volcanic Field and Gobernador Gregores, Southern Patagonia. Based on noble gas isotopic compositions, Pali-Aike mantle xenoliths represent intrinsic SCLM with higher (U+Th+K)/(3He, 22Ne, 36Ar) ratios than the mid-ocean ridge basalt (MORB) source. This reservoir shows slightly radiogenic helium (3He/4He =6.84-6.90 RA), coupled with a strongly nucleogenic neon signature (mantle source 21Ne/22Ne =0.085-0.094). The 40Ar/36Ar ratios vary from a near-atmospheric ratio of 510 up to 17700, with mantle source 40Ar/36Ar between 31100+9400−6800 and 54000+14200−9600. In addition, the 3He/22Ne ratios for the local SCLM endmember, at 12.03 ±0.15 to 13.66 ±0.37, are higher than depleted MORBs, at 3He/22Ne =8.31-9.75. Although asthenospheric mantle upwelling through the Patagonian slab window would result in a MORB-like metasomatism after collision of the South Chile Ridge with the Chile trench ca. 14 Ma, this mantle reservoir could have remained unhomogenized after rapid passage and northward migration of the Chile Triple Junction. The mantle endmember xenon isotopic ratios of Pali-Aike mantle xenoliths, which is first defined for any SCLM-derived samples, show values indistinguishable from the MORB source (129Xe/132Xe=1.0833+0.0216−0.0053 and 136Xe/132Xe=0.3761+0.0246−0.0034).The noble gas component observed in Gobernador Gregores mantle xenoliths is characterized by isotopic compositions in the MORB range in terms of helium (3He/4He =7.17-7.37 RA), but with slightly nucleogenic neon (mantle source 21Ne/22Ne =0.065-0.079). We suggest that this MORB-like metasomatism was capable of overprinting the noble gas composition of Gobernador Gregores due to recent metasomatism of the SCLM because of asthenospheric mantle upwelling in response to opening of the Patagonian slab window. The 40Ar/36Ar ratios vary from a near-atmospheric ratio of 380 up to 6560, with mantle source 40Ar/36Ar between 8100+1400−700 and 17700+4400−3100. The lower 40Ar/36Ar ratio of the Gobernador Gregores mantle source, compared with that of Pali-Aike, attests that the Patagonia SCLM was affected significantly by atmospheric contamination associated with the recycled oceanic lithosphere.
publishDate 2016
dc.date.none.fl_str_mv 2016-07
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/44159
Jalowitzki, Tiago; Sumino, Hirochika; Conceiçao, Rommulo V.; Orihashi, Yuji; Nagao, Keisuke; et al.; Noble gas composition of subcontinental lithospheric mantle: An extensively degassed reservoir beneath Southern Patagonia; Elsevier Science; Earth and Planetary Science Letters; 450; 7-2016; 263-273
0012-821X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/44159
identifier_str_mv Jalowitzki, Tiago; Sumino, Hirochika; Conceiçao, Rommulo V.; Orihashi, Yuji; Nagao, Keisuke; et al.; Noble gas composition of subcontinental lithospheric mantle: An extensively degassed reservoir beneath Southern Patagonia; Elsevier Science; Earth and Planetary Science Letters; 450; 7-2016; 263-273
0012-821X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1016/j.epsl.2016.06.034
info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S0012821X16303211
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
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eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
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application/pdf
application/pdf
dc.publisher.none.fl_str_mv Elsevier Science
publisher.none.fl_str_mv Elsevier Science
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
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reponame_str CONICET Digital (CONICET)
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instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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