988 resultados para Sm-Nd isotope dating


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The Borborema Province has three major subprovinces. The northern subprovince lies north of the Patos shear zone and is comprised of Paleoproterozoic cratonic basement with Archean nuclei, plus overlying Neoproterozoic supracrustal rocks and Brasiliano plutonic rocks. The central subprovince occurs between the Patos and Pernambuco shear zones and is mainly comprised of the Zona Transversal. The southern subprovince occurs between the Pernamabuco shear zone and the Sao Francisco craton and is comprised of a tectonic collage of various blocks, terranes, or domains ranging in age from Archean to Neoproterozoic. This report focuses on the Zona Transversal, especially on Brasiliano rocks for which we have the most new information. Paleoproterozoic gneisses with ages of 2.0-2.2 Ga occur discontinuously throughout the Zona Transversal. The Cariris Velhos suite consists of metavolcanic, metasedimentary, and metaplutonic rocks yielding U-Pb zircon ages of 995-960 Ma. This suite is mainly confined to a 100 km wide belt that extends for more than 700 km within the Alto Pajeu terrane. Sm-Nd model ages in metaigneous rocks cluster about 1.3-1.6 Ga, indicating that older crust was involved in genesis of their magmas. Brasiliano supracrustal rocks dominate the Pianco-Alto Brigida terrane, and they probably also constitute significant parts of the Alto Pajeu and Rio Capibaribe terranes. They are only slightly older than early stages of Brasiliano plutonism, with detrital zircon ages at least as young as 620 Ma; most T(DM) ages range from 1.2 to 1.6 Ga. Brasiliano plutons range from ca. 640 to 540 Ma, and their T(DM) ages range from 1.2 to 2.5 Ga. Previous workers have shown significant correlations among U-Pb ages, Sm-Nd model ages, petrology, and geochemistry, and we are able to reinforce and extend these correlations. Stage I plutons formed 640 -610 Ma and have T(DM) ages less than 1.5 Ga. Stage 11 (610-590 Ma) contains few plutons, but coincides with the peak of compressional deformation, metamorphism, and formation of migmatites. Stage III plutons (590 to ca. 575 Ma) have older T(DM) ages (ca. 1.8-2.0 Ga), as do Stage IV plutons (575 to ca. 550 Ma; T(DM) from 1.9 to 2.4 Ga). Stage III plutons formed during the transition from compressional to transcurrent deformation, while Stage IV plutons are mainly post-tectonic. Stage V plutons (550-530 Ma) are commonly undeformed (except along younger shear zones) and have A-type geochemistry. The five stages have distinct geochemical properties, which suggest that the tectonic settings evolved from early, arc-related magma-genesis (Stage I) to within-plate magma-genesis (Stage V), with perhaps some intermediate phases of extensional environments. (C) 2011 Elsevier Ltd. All rights reserved.

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Os métodos radiométricos (Rb-Sr e Sm-Nd) têm sido aplicados, com sucesso, em rochas sedimentares visando a obtenção de idades deposicionais e informações sobre proveniência. Em muitos casos, apesar dos resultados geologicamente significativos, ainda persistem dúvidas em relação a extensão e interpretação dos dados obtidos. Isto ocorre porque as rochas sedimentares resultam da mistura de fragmentos detríticos de diversas proveniências com diferentes sistemas isotópicos, conseqüentemente, já contendo um registro isotópico da rocha fonte. No caso do método Rb-Sr, aplicado em rochas sedimentares de granulometria fina, pode-se obter idades absolutas para o evento deposicional. Isto é viável desde que este registro isotópico proveniente das rochas fonte seja apagado no momento da deposição, ou seja, deve ocorrer a homogeneização isotópica do Sr no ambiente sedimentar. Para tanto, devem ser observados alguns pré-requisitos em relação a amostragem, granulometria, ambiente deposicional e composição mineralógica das amostras, entre outros. No entanto, ainda existem questionamentos em relação a esta metodologia especialmente quanto à ocorrência e à extensão do processo de homogeneização isotópica do Sr em ambiente sedimentar.(Continua0 O método Sm-Nd, apesar de ser uma técnica relativamente nova quando aplicada a rochas sedimentares, tem se tornado uma ferramenta fundamental para auxílio na determinação de proveniência de rochas sedimentares. As maiores dificuldades estão na correta interpretação dos valores obtidos e sua associação com um ambiente sedimentar, ou seja, de baixa temperatura. Neste trabalho, foram aplicados os métodos radiométricos Rb-Sr e Sm-Nd em amostras de rochas sedimentares coletadas em diferentes contextos geológicos da Bacia do Paraná. Foram tentativamente testados os diferentes parâmetros que atuam no sentido da homogeneização isotópica do Sr e do comportamento do Nd. Os resultados obtidos permitiram aprimorar a metodologia radiométrica Rb-Sr e Sm-Nd quando aplicada em rochas sedimentares, bem como obter resultados sobre a idade deposicional de diferentes unidades sedimentares e, por vezes, sua proveniência.

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A bacia de Ischigualasto-Villa Unión (Stipanicic e Bonaparte, 1972), que consiste de uma bacia alongada no sentido NW-SE e preenchida por rochas sedimentares Triássicas, foi gerada durante o Eo-Triássico pela reativação de descontinuidades crustais pré-existentes, associadas ao Gondwanides, na região central andina. Esta limitada a oeste, pelo vale do Rio Bermejo, no qual se encontra a zona de sutura do Vale Fértil, que se caracteriza pela borda ativa da bacia. Aqui, apresentar-se-á uma revisão da estratigrafia da bacia de Ischigualasto-Villa Unión, detalhando-se duas áreas chaves do registro estratigráfico inferior da bacia, na região do Cerro Morado e La Torre. Nestas áreas utilizou-se de técnicas estratigráficas e isotópicas (Sm-Nd em rocha total), com o objetivo de estabelecer uma correlação entre seus registros estratigráficos e suas áreas-fonte, além de caracterizar o comportamento tectônico. Ambos os perfis apresentam na porção inferior o preenchimento por um sistema aluvial-fluvial (Formação Tarjados sensu Romer & Jensen, 1966), subdividido em 4 associações de fácies: leques aluviais, canais fluviais, barras longitudinais e planície de inundação; e, na porção superior, o preenchimento por um sistema lacustre-deltáico (Formação Los Chañares sensu Frenguelli, 1944, no Cerro Morado e, Formação Lomas Blancas sensu Bossi e Herbst, 1968, em La Torre), subdividido em 4 associações de fácies: lacustre, pró delta, frente deltáica e planicie deltáica. Sobre as últimas unidades ocorre um lacólito de diabásio (Formação Los Baldecitos) A formação Tarjados apresenta as maiores idades TDM na região do Cerro Morado, variando entre 1,33 e 1,60 Ga, enquanto que em La Torre os valores oscilam entre 1,03 e 1,30 Ga. Isso é interpretado aqui como uma variação da área fonte entre as duas regiões na época de sua sedimentação, cujas regiões poderiam estar compartimentadas em termos tectônicos a época de sua deposição. A formação Los Chañares possui idades TDM variando entre 0,90 e 1,36 Ga, e a formação Lomas Blancas possui idades TDM entre 0,99 e 1,35 Ga, com dominância de valores próximos a 1 Ga nos dois blocos. Os diabásios da formação Los Baldecitos possuem idades TDM entre 0,51 e 0,33 Ga, cujo dado é interpretado com uma extração mantélica próxima a 130 Ma de um manto modificado pela orogenia do Ciclo Gondwânico, ou até mesmo pelo processo de slab break-off da crosta oceânica consumida pela colisão do micro-continente Cuyania com a proto-margem do Gondwana (Ramos, 1999). Todas as rochas dessa formação obtiveram valores de Epsilon Nd positivos. A integração dos dados estratigráficos e isotópicos nos permite interpretar as duas áreas como meio-grábens distintos na etapa inicial de preenchimento, em função da discrepância entre as idades TDM entre as áreas. A partir da transgressão lacustre as áreas-fonte são uniformizadas e o alto estrutural pré-existente é transgredido.

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Great part of the gold mineralizations are associated with shearing zones through which circulate a great volume of fluids, that interact with the host rocks, originating leaching or precipitation of chemical elements, including gold. The studied mineralizations are inserted in the Seridó Belt. The tungsten mineralization in Brejuí Mine is hosted in calcsilicate rocks from Jucurutu Formation. The São Francisco auriferous mineralization has as host rocks mica-schists from Seridó Formation, while the Ponta da Serra and Fazenda Simpático mineralizations are hosted in orthogneisses of this fold belt basement. The research conducted on these mineralizations had the purpose of integrate the data of chemical elements behavior during the shearing/mineralizing event, and its influence on the isotopic systems Rb-Sr and Sm-Nd. The studies of chemical mobility in the auriferous mineralizations showed that elements that during the shearing displayed in general an immobile behavior were Al, Ti and Zr. Among the elements that were mobilized during the event, K and Rb showed mass gain in ali belts of transformed rocks, while the elements Ca, Na and Sr normally lost mass. Petrographic studies showed that the minerais biotite and plagioclase, in all investigated mineralizations, played an important role in the chemical reactions occurred in the transformed rocks to the generation of muscovite, cordierite and sillimanite, justifying the input of K to the formation of muscovite, and the release of Na and Ca from plagioclase to the fluid phase. In the São Francisco auriferous mineralization, the results of the Rb-Sr isotopic analysis yielded ages of 645 ± 19 Ma and 596 ± 17 Ma, with both samples, from original and transformed rocks. Two ages, 569 ± 20 Ma. and 554 ± 19 Ma., were obtained with samples frem the transformed rocks domain. These ages suggest that there were two metamorphic pulses during the emplacement of the mineralized shearing zone. The Sm-Nd data yielded TDM ages of 1,31 Ga and 1,26 Ga with 3Nd (0,6 Ga) of -0,26 e -0,40 for the original and final transformed rocks, respectively. In case of the orthogneisses of Caicó Complex, e.g. the Ponta da Serra and Fazenda Simpático mineralizations, the Rb-Sr data did not yield ages with geological significance. In the Ponta da Serra mineralization, the Sm-Nd isotopic data yielded T DM ages of 2,56 Ga and 2,63 Ga to the original rocks and of 2,71 Ga to the mineralized sheared rock, and values of 3Nd (2,0 Ga) between -3,70 e -5,42 to the original and sheared rock, respectively. In the Fazenda Simpático, Sm-Nd data yielded TDM between 2,65 and 2,69 Ga with values of 3Nd (2,0 Ga) between -5,25 e -5,52. Considering the Sm-Nd data, the TDM ages may be admitted as the age of the parental magma extraction, producer of the protoliths of the orthogneisses from Ponta da Serra and Fazenda Simpático mineralizations. The chemical mobility studies showed that in the basement hosted mineralizations, Rb achieved mass while Sr lost mass, as Sm as well as Nd were strongly mobilized. The Sm/Nd ratio remained constant, however, confirming the isochemical character of those elements. In the basement mineralizations, Rb-Sr ages are destituted of geological significance, because of the partial opening of the isotopic system during the tectono-metamorphic transformations. In the tungsten mineralization, the diagram Sm-Nd constructed with the whole-rock data of calcsilicatic and the high-temperature paragenesis (garnet, diopside and iron-pargasitic hornblende) indicated an 631 ± 24 Ma age, while with the whole-rock data and low-temperature paragenesis (vesuvianite, epidote and calcite), a 537 ± 107 Ma age was obtained. These ages, associated with the petrographic observations, suggest that there was a time gap among the hydrothernal events responsible by the formation of the high and low temperature paragenesis in the calcsilicatic rocks mineralized in scheelite

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Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

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On the basis of geologic, petrologic, and U-Pb geochronologic data the basement rocks in the east-central part of the Rondonia Tin Province (RTP, southwestern Amazonian craton) are grouped into five lithologic associations: (1) tonalitic gneiss (1.75 Ga); (2) enderbitic granulite (1.73 Ga); (3) paragneiss; (4) granitic and charnockitic augen gneisses (1.57-1.53 Ga); and (5) fine-grained granitic gneiss and charnockitic granulite (1.43-1.42 Ga). The first three are related to development of the Paleoproterozoic Rio Negro-Juruena Province and represent the oldest crust in the region. The tonalitic gneisses and enderbitic granulites show calc-alkaline affinities and Nd isotopic compositions (initial epsilon(Nd) = +0-1 to -1.5; T-DM of 2.2-2.1 Ga) that suggest a continental arc margin setting for the original magmas. The paragneisses yield T-DM values of 2.2-2.1 Ga suggesting that source material was primarily derived from the Ventuari-Tapajos and Rio Negro-Juruena crusts, but detrital zircon ages and an intrusive granitoid bracket deposition between 1.67 and 1.57 Ga. The granitic and charnockitic augen gneisses show predominantly A-type and within-plate granite affinities, but also some volcanic arc granite characteristics. The initial epsilon(Nd) values (+0.6 to +2.0) indicate mixing of magmas derived from depleted mantle and older crustal sources. These rocks are correlated to the 1.60-1.53 Ga Serra da Providencia intrusive suite that reflects inboard magmatism coeval with the Cachoeirinha orogen located to the southeast. The fine-grained granitic gneiss and charnockitic granulites represent the first record of widespread magmatism at 1.43-1.42 Ga in northern Rondonia. Their geochemical signatures and the slightly positive initial epsilon(Nd) values (+0.7 to +1.2) are very similar to those of the most evolved granites of the calc-alkaline Santa Helena batholith farther southeast. U-Pb monazite and Sm-Nd whole-rock-garnet ages demonstrate that a high-grade tectonometa-morphic episode occurred in this region at 1.33-1.30 Ga. This episode attained upper-amphibolite conditions and is interpreted as the peak of the Rondonian-San Ignacio orogeny. The U-Pb and Sm-Nd data presented here and data published on rapakivi granites elsewhere indicate that the east-central part of the RTP is a poly-orogenic region characterized by successive episodes of magmatism, metamorphism, and deformation between 1.75 and 0.97 Ga. (C) 2002 Elsevier B.V. B.V. All rights reserved.

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Este trabalho apresenta dados geocronológicos 207Pb/206Pb de grãos detríticos de zircão obtidos pelo método de evaporação de chumbo e idades-modelo Sm-Nd (TDM) de rochas metassedimentares do Cinturão Araguaia, e discute as possíveis áreas-fonte dessas rochas, buscando investigar a história evolutiva deste cinturão no contexto da amalgamação do Gondwana. As datações em grãos detríticos de zircão de quartzitos da Formação Morro do Campo apontaram idades arqueanas (3,0-2,65 Ga) para o domínio norte (região de Xambioá) e, para o domínio sul (região de Paraíso do Tocantins), revelaram idades meso-neoproterozoicas (1,25-0,85 Ga) e, secundariamente, paleoproterozoicas (1,85-1,70 Ga), sugerindo a existência de áreas fontes distintas para os dois domínios. As idades-modelo Sm-Nd (TDM) obtidas em metapelitos (ardósias, filitos, micaxistos) dos grupos Estrondo e Tocantins apresentaram distribuição bimodal com maior frequência de idades entre 2,1 e 1,4 Ga, com moda entre 1,7 e 1,6 Ga, e outras menos frequentes entre 2,7 e 2,4 Ga, sugerindo mistura de fontes de idade Paleoproterozoica (ou até Arqueana) com fontes mais jovens, provavelmente do Meso-Neoproterozoico. Os principais candidatos a fonte para as rochas do Cinturão Araguaia seriam os segmentos crustais situados a sudeste (Cráton São Francisco, Maciço de Goiás e Arco Magmático de Goiás). Toda a sucessão de rochas sedimentares da bacia oceânica Araguaia e rochas magmáticas associadas a estes segmentos foram transportados, posteriormente, em direção à margem oriental do Cráton Amazônico, durante a tectônica principal de estruturação do Cinturão Araguaia, resultante da amalgamação do supercontinente Gondwana.

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Modern thermohaline circulation plays a role in latitudinal heat transport and in deep-ocean ventilation, yet ocean circulation may have functioned differently during past periods of extreme warmth, such as the Cretaceous. The Late Cretaceous (100-65 Ma) was an important period in the evolution of the North Atlantic Ocean, characterized by opening ocean gateways, long-term climatic cooling and the cessation of intermittent periods of anoxia (oceanic anoxic events, OAEs). However, how these phenomena relate to deep-water circulation is unclear. We use a proxy for deep-water mass composition (neodymium isotopes; e-Nd) to show that, at North Atlantic ODP Site 1276, deep waters shifted in the early Campanian (~78-83 Ma) from e-Nd values of ~-7 to values of ~-9, consistent with a change in the style of deep-ocean circulation but >10 Myr after a change in bottom water oxygenation conditions. A similar, but more poorly dated, trend exists in e-Nd data from DSDP Site 386. The Campanian e-Nd transition observed in the North Atlantic records is also seen in the South Atlantic and proto-Indian Ocean, implying a widespread and synchronous change in deep-ocean circulation. Although a unique explanation does not exist for the change at present, we favor an interpretation that invokes Late Cretaceous climatic cooling as a driver for the formation of Southern Component Water, which flowed northward from the Southern Ocean and into the North Atlantic and proto-Indian Oceans.

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The development of widespread anoxic conditions in the deep oceans is evidenced by the accumulation and preservation of organic-carbon-rich sediments, but its precise cause remains controversial. The two most popular hypotheses involve (1) circulation-induced increased stratification resulting in reduced oxygenation of deep waters or (2) enhanced productivity in the surface ocean, increasing the raining down of organic matter and overwhelming the oxic remineralization potential of the deep ocean. In the periodic development of deep-water anoxia in the Pliocene-Pleistocene Mediterranean Sea, increased riverine runoff has been implicated both as a source for nutrients that fuel enhanced photic-zone productivity and a source of a less dense freshwater cap leading to reduced circulation, basin-wide stagnation, and deep-water oxygen starvation. Monsoon-driven increases in Nile River discharge and increased regional precipitation due to enhanced westerly activity-two mechanisms that represent fundamentally different climatic driving forces-have both been suggested as causes of the altered freshwater balance. Here we present data that confirm a distinctive neodymium (Nd) isotope signature for the Nile River relative to the Eastern Mediterranean-providing a new tracer of enhanced Nile outflow into the Mediterranean in the past. We further present Nd isotope data for planktonic foraminifera that suggest a clear increase in Nile discharge during the central intense period of two recent anoxic events. Our data also suggest, however, that other regional freshwater sources were more important at the beginning and end of the anoxic events. Taken at face value, the data appear to imply a temporal link between peaks in Nile discharge and enhanced westerly activity.

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The Pacific Ocean is the largest water body on Earth, and circulation in the Pacific contributed significantly to climate evolution in the latest Cretaceous, the culmination of a period of long-term cooling. Here, we present new high-resolution late Campanian to Maastrichtian benthic and planktic foraminiferal stable isotope data and a neodymium (Nd) isotope record obtained from sedimentary ferromanganese oxide coatings of Ocean Drilling Program Hole 1210B from the tropical Pacific Ocean (Shatsky Rise). These new records resolve 13 million years in the latest Cretaceous, providing insights into changes in surface and bottom water temperatures and source regions of deep to intermediate waters covering the carbon isotope excursions of the Campanian-Maastrichtian Boundary Event (CMBE) and the Mid-Maastrichtian event (MME). Our new benthic foraminiferal d18O and Nd isotope records together with published Nd isotope data show markedly parallel trends across the studied interval over a broad range of bathyal to abyssal water depths interpreted to reflect changes in the intensity of deep-ocean circulation in the tropical Pacific. In particular, we observe a three-million-year-long period of cooler conditions in the early Maastrichtian (72.5 to 69.5 Ma) when a concomitant change toward less radiogenic seawater Nd isotope signatures probably marks a period of enhanced admixture and northward flow of deep waters with Southern Ocean provenance. We suggest this change to have been triggered by intensified formation and convection of deep waters in the high southern latitudes, a process that weakened during the MME (69.5 to 68.5 Ma). The early Maastrichtian cold interval is closely related to the negative and positive carbon isotope trends of the CMBE and MME. The millions-of-years long duration of these carbon cycle perturbations suggests a tectonic forcing of climatic cooling, possibly related to changes in ocean basin geometry and bathymetry.