8 resultados para Kimberlite magmas

em Biblioteca Digital da Produção Intelectual da Universidade de São Paulo


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The north-western sector of the Gharyan volcanic field (northern Libya) consists of trachytic-phonolitic domes emplaced between similar to 41 and 38 Ma, and small-volume mafic alkaline volcanic centres (basanites, tephrites. alkali basalts. hawaiites and rare benmoreites) of Middle Miocene-Pliocene age (similar to 12-2 Ma). Two types of trachytes and phonolites have been recognized on the basis of petrography, mineralogy and geochemistry. Type-1 trachytes and phonolites display a smooth spoon-shaped REE pattern without negative Europium anomalies. Type-2 trachytes and phonolites show a remarkable Eu negative anomaly, higher concentration in HFSE (Nb-Ta-Zr-Hf), REE and Ti than Type-1 rocks. The origin of Type-1 trachytes and phonolites is compatible with removal of clinopyroxene, plagioclase, alkali feldspar, amphibole. magnetite and titanite starting from benmoreitic magmas. found in the same outcrops. Type-2 trachytes and phonolites could be the result of extensive fractional crystallization starting from mafic alkaline magma, without removal of titanite. In primitive mantle-normalized diagrams, the mafic rocks (Mg#= 62-68, Cr up to 514 ppm, Ni up to 425 ppm) show peaks at Nb and Ta and troughs at K. These characteristics, coupled with low Sr-87/Sr-86(i) (0.7033-0.7038) and positive epsilon(Nd) (from +4.2 to + 5.3) features typical of the mafic anorogenic magmas of the northern African plate and of HIMU-OIB-like magma in general. The origin of the mafic rocks is compatible from a derivation from low degree partial melting (3-9%) shallow mantle sources in the spinel/gamet facies. placed just below the rigid plate in the uppermost low-velocity zone. The origin of the igneous activity is considered linked to passive lithospheric thinning related to the development of continental rifts like those of Sicily Channel (e.g.. Pantelleria and Linosa) and Sardinia (e.g., Campidano Graben) in the Central-Western Mediterranean Sea. (C) 2012 Elsevier B.V. All rights reserved.

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The early phase of post-collisional granitic magmatism in the Camboriu region, south Brazil, is represented by the porphyritic biotite +/- hornblende Rio Pequeno Granite (RPG; 630-620 Ma) and the younger (similar to 610 Ma), equigranular, biotite +/- muscovite Serra dos Macacos Granite (SMG). The two granite types share some geochemical characteristics, but the more felsic SMG constitutes a distinctive group not related to RPG by simple fractionation processes, as indicated by its lower FeOt, TiO2, K2O/Na2O and higher Zr Al2O3, Na2O, Ba and Sr when compared to RPG of similar SiO2 range. Sr-Nd-Pb isotopes require different sources. The SMG derives from old crustal sources, possibly related to the Paleoproterozoic protoliths of the Camboriu Complex, as indicated by strongly negative epsilon Nd-t (-23 to -24) and unradiogenic Pb (e.g., Pb-206/Pb-204 = 16.0-16.3; Pb-207/Pb-204 = 15.3-15.4) and confirmed by previous LA-MC-ICPMS data showing dominant zircon inheritance of Archean to Paleoproterozoic age. In contrast, the RPG shows less negative epsilon Nd-t (-12 to -15) and a distinctive zircon inheritance pattern with no traces of post-1.6 Ga sources. This is indicative of younger sources whose significance in the regional context is still unclear; some contribution of mantle-derived magmas is indicated by coeval mafic dykes and may account for some of the geochemical and isotopic characteristics of the least differentiated varieties of the RPG. The transcurrent tectonics seems to have played an essential role in the generation of mantle-derived magmas despite their emplacement within a low-strain zone. It may have facilitated their interaction with crustal melts which seem to be to a large extent the products of reworking of Paleoproterozoic orthogneisses from the Camboriu Complex. (C) 2012 Elsevier Ltd. All rights reserved.

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The Tamboril-Santa Quiteria Complex is an important Neoproterozoic granitic-migmatitic unit from the Ceara Central Domain that developed from ca. 650 to 610 Ma. In general the granitoids range in composition from diorite to granite with predominance (up to 85%) of granitic to monzogranitic composition with biotite as the main mafic AFM phase. Geochemical and Pb-207/Pb-206 evaporation zircon geochronology studies were applied in a group of these abundant monzogranitic rocks from the region of Novo Oriente in the southern portion of the Ceara Central Domain. In this area the granitoids are weakly peraluminous biotite granitoids and deformed biotite granitoids of high-K calc-alkaline and ferroan composition, which we interpreted as primary magmas (segregated diatexites) derived from the partial melting of crustal material. The close temporal relation of this magmatism with local eclogitic and regional high temperature metamorphism in Ceara Central Domain point out to an orogenic setting, arguably emplaced during the collisional stage. Subordinate coeval juvenile mantle incursions are also present. This crustally derived magmatism is the primary product of the continental thickening that resulted from the collision between the rocks represented by the Amazonian-West African craton (Sao Luiz cratonic fragment) to the northwest and the Paleoproterozoic-Archean basement of the Borborema Province to the southeast along the Transbrasiliano tectonic corridor. (C) 2011 Elsevier Ltd. All rights reserved.

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The Neoproterozoic post-collisional period in southern Brazil (650-580 Ma) is characterized by substantial volumes of magma emplaced along the active shear zones that compose the Southern Brazilian Shear Belt. The early-phase syntectonic magmatism (630-610 Ma) is represented by the porphyritic, high-K, metaluminous to peraluminous Quatro Ilhas Granitoids and the younger heterogranular, slightly peraluminous Mariscal Granite. Quatro II has Granitoids include three main petrographic varieties (muscovite-biotite granodiorite mbg; biotite monzogranite - bmz: and leucogranite - lcg) that, although sharing some significant geochemical characteristics, are not strictly comagmatic, as shown by chemical and Sr-Nd-Pb isotope data. The most primitive muscovite-biotite granodiorite was produced by contamination of more mafic melts (possibly with some mantle component) with peraluminous crustal melts; the biotite monzogranite, although more felsic, has higher Ca, MgO,TiO2 and Ba, and lower K2O, FeOt, Sr and Rb contents, possibly reflecting some mixing with coeval mafic magmas of tholeiitic affinity; the leucogranite may be derived from pure crustal melts. The Mariscal Granite is formed by two main granite types which occur intimately associated in the same pluton, one with higher K (5-6.5 wt.% K2O) high Rb and lower CaO, Na2O, Ba and Zr as compared to the other (3-5 wt.% of K2O). The two Mariscal Granite varieties have compositional correspondence with fine-grained granites (fgg) that occur as tabular bodies which intruded the Quatro Ilhas Granoitoids before they were fully crystallized, and are inferred to correspond to the Mariscal Granite feeders, an interpretation that is reinforced by similar U-Pb zircon crystallization ages. The initial evolution of the post-collisional magmatism, marked by the emplacement of the Quatro Ilhas Granitoids varieties, activated sources that produced mantle and crustal magmas whose emplacement was controlled both by flat-lying and transcurrent structures. The transition from thrust to transcurrent-related tectonics coincides with the increase in the proportion of crustal-derived melts. The transcurrent tectonics seems to have played an essential role in the generation of mantle-derived magmas and may have facilitated their interaction with crustal melts which seem to be to a large extent the products of reworking of orthogneiss protoliths. (C) 2012 Elsevier B.V. All rights reserved.

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The Niquelandia Complex, Brazil, is one of the world's largest mafic-ultramafic plutonic complexes. Like the Mafic Complex of the Ivrea-Verbano Zone, it is affected by a pervasive high-T foliation and shows hypersolidus deformation structures, contains significant inclusions of country-rock paragneiss, and is subdivided into a Lower and an Upper Complex. In this paper, we present new SHRIMP U-Pb zircon ages that provide compelling evidence that the Upper and the Lower Niquelandia Complexes formed during the same igneous event at ca. 790 Ma. Coexistence of syn-magmatic and high-T subsolidus deformation structures indicates that both complexes grew incrementally as large crystal mush bodies which were continuously stretched while fed by pulses of fresh magma. Syn-magmatic recrystallization during this deformation resulted in textures and structures which, although appearing metamorphic, are not ascribable to post-magmatic metamorphic event(s), but are instead characteristic of the growth process in huge and deep mafic intrusions such as both the Niquelandia and Ivrea Complexes. Melting of incorporated country-rock paragneiss continued producing hybrid rocks during the last, vanishing stages of magmatic crystallization. This resulted in the formation of minor, late-stage hybrid rocks, whose presence obscures the record of the main processes of interaction between mantle magmas and crustal components, which may be active at the peak of the igneous events and lead to the generation of eruptible hybrid magmas. (C) 2012 Elsevier B.V. All rights reserved.

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The Cretaceous Banhado alkaline complex in southeastern Brazil presents two potassic SiO2-undersaturated series. The high-Ca magmatic series consist of initially fractionated olivine (Fo(92-91)) + diopside (Wo(48-43)En(49-35)Ae(0-7)), as evidenced by the presence of xenocrysts and xenoliths. In that sequence, diopside (Wo(47-38)En(46-37)Ae(0-8)) + phlogopite + apatite + perovskite (Prv(> 92)) crystallized to form the phlogopite melteigite and led to the Ca enrichment of the magma. Diopside (Wo(47-41)En(32-24) Ae(3-14)) continued to crystallize as an early mafic mineral, followed by nepheline (Ne(74.8-70.1)Ks(26.3-21.2)Qz(7.6-0.9)) and leucite (Lc(65-56)) and subsequently by melanite and potassic feldspar (Or(85-99)Ab(1-7)) to form melanite ijolites, wollastonite-melanite urtites and melanite-nepheline syenites. Melanite-pseudoleucite-nepheline syenites are interpreted to be a leucite accumulation. Melanite nephelinite dykes are believed to represent some of the magmatic differentiation steps. The low-Ca magmatic series is representative of a typical fractionation of aegirine-augite (Wo(36-29)En(25-4)Ae(39-18)) + alkali feldspar (Or(57-96)Ab(3-43)) + nepheline (Ne(76.5-69.0)Ks(19.9-14.4)Qz(15.1-7.7)) + titanite from phonolite magma. The evolution of this series from potassic nepheline syenites to sodic sodalite syenites and sodalitolites is attributed to an extensive fractionation of potassic feldspar, which led to an increase of the NaCl activity in the melt during the final stages forming sodalite-rich rocks. Phonolite dykes followed a similar evolutionary process and also registered some crustal assimilation. The mesocratic nepheline syenites showed interactions with phlogopite melteigites, such as compatible trace element enrichments and the presence of diopside xenocrysts, which were interpreted to be due to a mixing/mingling process of phonolite and nephelinite magmas. The geochemical data show higher TiO2 and P2O5 contents and lower SiO2 contents for the high-Ca series and different LILE evolution trends and REE chondrite-normalized patterns as compared to the low-Ca series. The Sr-87/Sr-86, Nd-143/Nd-144, Pb-206/Pb-204 and Pb-208/Pb-204 initial ratios for the high-Ca series (0.70407-0.70526, 0.51242-0.51251, 17.782-19.266 and 38.051-39.521, respectively) were slightly different from those of the low-Ca series (0.70542-0.70583, 0.51232-0.51240, 17.758-17.772 and 38.021-38.061, respectively). For both series, a CO2-rich potassic metasomatized lithospheric mantle enriched the source with rutile-bearing phlogopite clinopyroxenite veins. Kamafugite-like parental magma is attributed to the high-Ca series with major contributions from the melting of the veins. Potassic nephelinite-like parental magma is assigned to the low-Ca series, where the metasomatized wall-rock played a more significant role in the melting process.

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Neste estudo, buscou-se compreender os processos e materiais que contribuíram às fontes mantélicas envolvidas na gênese da Província Magmática do Paraná (PMP). O papel que a crosta, a litosfera e o manto terrestre (raso ou profundo) desempenham na geração de assinaturas químicas e isotópicas em basaltos de derrames continentais e oceânicos tem sido um tema intensamente pesquisado e muito debatido na literatura internacional (e.g., Sheth, 2005). Embora muitos estudos já tenham sido conduzidos na PMP, existe ainda uma grande controvérsia com relação à natureza das regiões-fonte dos magmas (manto litosférico continental ou manto sublitosférico), como também acerca dos mecanismos geodinâmicos que provocam o início da fusão dessas regiões-fonte (e.g., Bellieni et al., 1984; Hawkesworth et al., 1992). Nesse contexto, uma grande quantidade de análises de elementos traço (litófilos e siderófilos), como também dados isotópicos de quatro sistemas de decaimento radioativo (Rb-Sr, Sm-Nd, U-Th-Pb e Re-Os), foram obtidos em basaltos que ocorrem no norte e sul da PMP. A regionalização geoquímica e isotópica (Sr-Nd-Pb) observada nas rochas basálticas da PMP tem sido frequentemente interpretada como resultante da fusão de manto litosférico subcontinental heterogêneo. Entretanto, dados geoquímicos de elementos altamente siderófilos e de razões isotópicas 187Os/188Os, obtidos neste estudo, indicam uma fonte mantélica homogênea, já que os basaltos baixo-TiO2 e alto- TiO2 possuem razões isotópicas de ósmio muito similares (187Os/188Osi = 0,1295±0,0018), as quais são distintas daquelas de manto litosférico subcontinental antigo (Proterozoico ou Arqueano; 187Os/188Os = 0,113). Os dados isotópicos Re-Os exibem uma tendência linear (187Re/188Os versus 187Os/188Os), definindo uma isócrona de boa qualidade (idade = 131,6 ± 2,3 Ma), consistente com as idades obtidas em trabalhos anteriores utilizando o método 40Ar/39Ar. Comumente, a PMP tem sido geneticamente ligada ao hotspot Tristão da Cunha via Rio Grande Rise e Walvis Ridge. No entanto, as razões isotópicas de ósmio determinadas nas rochas da Ilha de Tristão da Cunha são muito distintas daquelas dos basaltos da PMP, reforçando que essa pluma não deve ter contribuído com matéria na gênese dessas rochas. Desta forma, para explicar todas as características isotópicas dos basaltos da PMP é necessário o envolvimento de três componentes mantélicos (Marques et al., 1999). Um deles, empobrecido e semelhante ao DMM, estaria presente na fonte dos basaltos alto-TiO2 e baixo-TiO2, dominando as composições isotópicas de ósmio. Os outros dois componentes enriquecidos (EM-I e EM-II) seriam responsáveis pelas variações nas composições isotópicas de Sr-Nd-Pb. Na gênese dos basaltos alto-TiO2 provavelmente ocorreu envolvimento de crosta continental inferior delaminada (EM-I), enquanto nas rochas baixo-TiO2 há indicação de participação de crosta continental superior reciclada (EM-II). O componente empobrecido possui composição semelhante à de peridotitos de arco, sendo que essa assinatura isotópica pode ter sido gerada por processos metassomáticos relacionados a processos de subducção neoproterozóicas, que teriam modificado o manto astenosférico (DMM). No processo de aglutinação do Gondwana esse manto astenosférico metassomatizado pode ter sido incorporado à base da litosfera, sofrendo posterior refusão, por ocasião da atividade ígnea da PMP.

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A Província Magmática do Paraná-Etendeka, ou ainda Formação Serra Geral assim definida na estratigrafia da Bacia do Paraná, constitui um dos maiores registros vulcânicos em área continental do planeta. O grande volume de magma é evidenciado não só pelas rochas expostas, que contemplam o sul e parte do sudeste brasileiro, mas também pela forte heterogeneidade geoquímica e petrográfica das rochas básicas, intermediárias e ácidas, que integram a placa Sul-Americana. Os trabalhos que abordam a caracterização geoquímica dos diferentes tipos de magmas, obtidos por meio de coleta sistemática de superfície são bastante abundantes, porem pouco são aqueles que abordam a quimioestratigrafia dos basaltos por meio de poços de sondagem buscando as relações estratigráficas aplicadas ao entendimento da evolução dos diferentes tipos de magmas, fontes, intervalo de idades e variações petrográficas sem a influência direta de falhas tectônicas que interferiam no aspecto fidedigno dos dados. Com isso, este trabalho em andamento, com 15 sequencias vulcânicas completas obtidas por meio de poços de sondagem nos estados de São Paulo e Paraná, com até 1156 metros de espessura, são investigados para elementos maiores, traços, terras-raras, isótopos (Pb, Sr e Nd) e idades (Ar-Ar) buscando a compreensão de processos de diferenciação magmática in situ e até mesmo considerações sobre o grau de fusão, fontes mantélicas envolvidas, correlação com a parte sul da província magmática e relação com a fase rifte da placa sul-americana. Os resultados, ainda que preliminares, mostraram que a média da espessura de cada pulso magmático é de 35 metros de rocha basáltica variando de 2 até 90 metros, sendo que a pilha mais profunda alcança 970 metros na região noroeste do estado de São Paulo podendo chegar até 1200 se for considerado a espessura dos sills intrudidos nos sedimentos paleozoicos sotopostos. Já os dados geoquímicos mostraram que as regiões investigadas são compostas exclusivamente por basaltos toleíticos do tipo alto-Ti, com concentrações em TiO2 variando entre 1,77% e 3,66% e MgO de 2,88% até 4,95%, podendo ser divididos em dois subtipos distintos, denominados de Pitanga e Paranapanema conforme classificação de Peate et al. (1992). O primeiro está enriquecido em Nb (8%), K (9%), La (11%), Ce (18%), P (8%), Nd (20%), Zr (19%), Sm (17%), Eu (15%) e Ti (15%) em relação ao segundo. Também é possível verificar que os magmas se alternam na posição estratigráfica sendo iniciado pelo tipo Pitanga (em contato direto com os arenitos eólicos da Formação Botucatu) seguindo pelo magma Paranapanema onde o primeiro, em espessura, e dominante em 60% em relação ao segundo. Por fim, mesmo que o trabalho ainda esteja em fase inicial, é possível concluir que os basaltos investigados podem ter sido abastecidos por mais de uma câmara magmática, que extravasaram suas lavas em épocas distintas, iniciando com basaltos do tipo Pitanga, em contato com os arenitos da Formação Botucatu, e encerrando a pilha edificada com aqueles do tipo Paranapanema.