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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/44159
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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 https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf 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) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
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CONICET Digital (CONICET) |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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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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1842269142075310080 |
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13.13397 |