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dc.contributor.author
Jalowitzki, Tiago  
dc.contributor.author
Sumino, Hirochika  
dc.contributor.author
Conceiçao, Rommulo V.  
dc.contributor.author
Orihashi, Yuji  
dc.contributor.author
Nagao, Keisuke  
dc.contributor.author
Bertotto, Gustavo Walter  
dc.contributor.author
Balbinot, Eduardo  
dc.contributor.author
Schilling, Manuel R  
dc.contributor.author
Gervasoni, Fernanda  
dc.date.available
2018-05-04T17:43:00Z  
dc.date.issued
2016-07  
dc.identifier.citation
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  
dc.identifier.issn
0012-821X  
dc.identifier.uri
http://hdl.handle.net/11336/44159  
dc.description.abstract
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.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
Elsevier Science  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
Noble Gas Isotopes  
dc.subject
Subcontinental Lithospheric Mantle  
dc.subject.classification
Meteorología y Ciencias Atmosféricas  
dc.subject.classification
Ciencias de la Tierra y relacionadas con el Medio Ambiente  
dc.subject.classification
CIENCIAS NATURALES Y EXACTAS  
dc.title
Noble gas composition of subcontinental lithospheric mantle: An extensively degassed reservoir beneath Southern Patagonia  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2018-05-04T14:57:25Z  
dc.journal.volume
450  
dc.journal.pagination
263-273  
dc.journal.pais
Países Bajos  
dc.journal.ciudad
Amsterdam  
dc.description.fil
Fil: Jalowitzki, Tiago. Universidade Federal do Rio Grande do Sul; Brasil  
dc.description.fil
Fil: Sumino, Hirochika. University of Tokyo; Japón  
dc.description.fil
Fil: Conceiçao, Rommulo V.. Universidade Federal do Rio Grande do Sul; Brasil  
dc.description.fil
Fil: Orihashi, Yuji. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. University of Tokyo; Japón  
dc.description.fil
Fil: Nagao, Keisuke. University of Tokyo; Japón  
dc.description.fil
Fil: Bertotto, Gustavo Walter. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de La Pampa; Argentina  
dc.description.fil
Fil: Balbinot, Eduardo. University of Surrey; Reino Unido  
dc.description.fil
Fil: Schilling, Manuel R. Universidad Austral de Chile; Chile  
dc.description.fil
Fil: Gervasoni, Fernanda. Universität Münster; Alemania  
dc.journal.title
Earth and Planetary Science Letters  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1016/j.epsl.2016.06.034  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S0012821X16303211