You are in the accessibility menu

Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/41620
Full metadata record
DC FieldValueLanguage
dc.contributor.authorRocha-Junior, Eduardo R. V.-
dc.contributor.authorPuchtel, Igor S.-
dc.contributor.authorMarques, Leila S.-
dc.contributor.authorWalker, Richard J.-
dc.contributor.authorMachado, Fabio B.-
dc.contributor.authorNardy, Antonio J. R.-
dc.contributor.authorBabinski, Marly-
dc.contributor.authorFigueiredo, Ana M. G.-
dc.date.accessioned2014-05-20T15:32:49Z-
dc.date.accessioned2016-10-25T18:09:10Z-
dc.date.available2014-05-20T15:32:49Z-
dc.date.available2016-10-25T18:09:10Z-
dc.date.issued2012-07-01-
dc.identifierhttp://dx.doi.org/10.1016/j.epsl.2012.04.050-
dc.identifier.citationEarth and Planetary Science Letters. Amsterdam: Elsevier B.V., v. 337, p. 164-173, 2012.-
dc.identifier.issn0012-821X-
dc.identifier.urihttp://hdl.handle.net/11449/41620-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/41620-
dc.description.abstractBasalts of the Parana continental flood basalt (PCFB) province erupted through dominantly Proterozoic continental crust during the Cretaceous. In order to examine the mantle source(s) of this major flood basalt province, we studied Os, Sr, Nd, and Pb isotope systematics, and highly siderophile element (HSE) abundances in tholeiitic basalts that were carefully chosen to show the minimal effects of crustal contamination. These basalts define a precise Re-Os isochron with an age of 131.6 +/- 2.3 Ma and an initial Os-187/Os-188 of 0.1295 +/- 0.0018 (gamma Os-187 = +2.7 +/- 1.4). This initial Os isotopic composition is considerably more radiogenic than estimates of the contemporary Depleted Mantle (DM). The fact that the Re-Os data define a well constrained isochron with an age similar to Ar-40/Ar-39 age determinations, despite generally low Os concentrations, is consistent with closed-system behavior for the HSE. Neodymium, Sr, and Pb isotopic data suggest that the mantle source of the basalts had been variably hybridized by melts derived from enriched mantle components. To account for the combined Os, Nd, Sr, and Pb isotopic characteristics of these rocks, we propose that the primary melts formed from metasomatized asthenospheric mantle (represented by arc-mantle peridotite) that underwent mixing with two enriched components, EM-I and EM-II. The different enriched components are reflected in minor isotopic differences between basalts from southern and northern portions of the province.The Tristan da Cunha hotspot has been previously suggested to be the cause of the Parana continental flood basalt magmatism. However, present-day Tristan da Cunha lavas have much higher Os-187/Os-188 isotopic compositions than the source of the PCFB. These data, together with other isotopic and elemental data, preclude making a definitive linkage between the Tristan plume and the PCFB. (C) 2012 Elsevier B.V. All rights reserved.en
dc.description.sponsorshipNSF-
dc.description.sponsorshipConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)-
dc.description.sponsorshipCoordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)-
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)-
dc.format.extent164-173-
dc.language.isoeng-
dc.publisherElsevier B.V.-
dc.sourceWeb of Science-
dc.subjectParana continental flood basaltsen
dc.subjectRe-Os isotopic systematicsen
dc.subjectTristan da Cunhaen
dc.subjecthighly siderophile elementsen
dc.subjectmantle plumeen
dc.titleRe-Os isotope and highly siderophile element systematics of the Parana continental flood basalts (Brazil)en
dc.typeoutro-
dc.contributor.institutionUniversidade Federal do Rio Grande do Sul (UFRGS)-
dc.contributor.institutionUniversidade de São Paulo (USP)-
dc.contributor.institutionUniversity of Maryland-
dc.contributor.institutionUniversidade Federal de São Paulo (UNIFESP)-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.contributor.institutionInstituto de Pesquisas Energéticas e Nucleares (IPEN)-
dc.description.affiliationUniversidade Federal do Rio Grande do Sul (UFRGS), Inst Geociencias, BR-91501970 Porto Alegre, RS, Brazil-
dc.description.affiliationUniv São Paulo, Inst Astron Geofis & Ciencias Atmosfer, BR-05508090 São Paulo, Brazil-
dc.description.affiliationUniv Maryland, Dept Geol, College Pk, MD 20742 USA-
dc.description.affiliationUniv Fed São Paulo, Dept Ciencias Exatas & Terra, São Paulo, Brazil-
dc.description.affiliationUniv Estadual Paulista, Inst Geociencias & Ciencias Exatas, Rio Claro, SP, Brazil-
dc.description.affiliationUniv São Paulo, Inst Geociencias, BR-05422970 São Paulo, Brazil-
dc.description.affiliationInst Pesquisas Energet & Nucl, BR-05508000 São Paulo, Brazil-
dc.description.affiliationUnespUniv Estadual Paulista, Inst Geociencias & Ciencias Exatas, Rio Claro, SP, Brazil-
dc.description.sponsorshipIdNSF: EAR-0946629-
dc.identifier.doi10.1016/j.epsl.2012.04.050-
dc.identifier.wosWOS:000307431800018-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofEarth and Planetary Science Letters-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

There are no files associated with this item.
 

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.