Caracterização estrutural da porção sul do greenstone belt de Guarinos, GO

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

Análise do comportamento dos isótopos radiogênicos durante os processos de migmatização

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

Diversity and three-dimensional structures of the alpha Mcr of the methanogenic Archaea from the anoxic region of Tucuruí Lake, in Eastern Brazilian Amazonia

ABSTRACT: Methanogenic archaeans are organisms of considerable ecological and biotechnological interest that produce methane through a restricted metabolic pathway, which culminates in the reaction catalyzed by the Methyl-coenzyme M reductase (Mcr) enzyme, and results in the release of methane. Using a metagenomic approach, the gene of the a subunit of mcr (mcrα) was isolated from sediment sample from an anoxic zone, rich in decomposing organic material, obtained from the Tucuruí hydroelectric dam reservoir in eastern Brazilian Amazonia. The partial nucleotide sequences obtained were 83 to 95% similar to those available in databases, indicating a low diversity of archaeans in the reservoir. Two orders were identified -the Methanomicrobiales, and a unique Operational Taxonomic Unit (OTU) forming a clade with the Methanosarcinales according to low bootstrap values. Homology modeling was used to determine the three-dimensional (3D) structures, for this the partial nucleotide sequence of the mcrα were isolated and translated on their partial amino acid sequences. The 3D structures of the archaean mcrα observed in the present study varied little, and presented approximately 70% identity in comparison with the mcrα of Methanopyrus klanderi. The results demonstrated that the community of methanogenic archaeans of the anoxic C1 region of the Tucurui reservoir is relatively homogeneous.

Estudo da geometria e cinemática das rochas sedimentares arqueanas da mina do Igarapé do Azul – Carajás-PA

Mina de Manganês do Igarapé Azul posiciona-se geologicamente no interior do feixe da Falha Carajás, na porção central do Sistema Transcorrente de Carajás. O depósito do Manganês do Azul relaciona-se a rochas sedimentares pelíticas do Membro Azul, na base da Formação Águas Claras (Arqueano), em contato discordante, acima do Grupo Grão Pará (Nogueira et al, 1995). Três frentes de lavra a céu aberto estão atualmente em andamento na área: (1) Mina Principal (Mina 1), (2) Mina 2 e (3) Mina 3. Nestes locais encontram-se excelentes afloramentos de siltitos intercalados com argilitos e arenitos finos, intercalados com níveis manganesíferos. Essas rochas estão organizadas em conjuntos de dobras e falhas normais e inversas sob deformação heterogênea, particionada em diferentes escalas. As seções geológicas realizadas nas frentes de lavra mostram a predominância de siltitos intercalados com argilitos em contato com rochas pelíticas manganesíferas e minério (bióxido de Mn). Nessas rochas são comuns estruturas primárias tipo hummocky, estratificações cruzadas, e laminações plano-paralelas. O acamamento centimétrico a métrico (em média de 30 a 50 cm ) representa a principal estrutura primária, usada como marcador de deformação, observada nas rochas. A Mina do Igarapé Azul encontra-se dividida em dois blocos, separados por falha normal com rejeito de até dezenas de metros, com o bloco norte alto em relação ao bloco sul. O bloco sul encontra-se pouco deformado, apresentado uma regularidade no acamamento que mergulha com ângulos suaves para sul, colocando a camada de minério sucessivamente em níveis mais profundos na direção S. No bloco norte o acamamento apresenta um comportamento heterogêneo. A deformação é mais expressiva nessa região, estando o nível de minério deformado por dobras e falhas inversas. Além da cinemática vertical, as falhas apresentam deslocamento conjugado destral dando a essas feições um caráter oblíquo. Essa região pode ser definida como um corredor de deformação. O corredor observado no bloco norte, de acordo com os domínios principais separados pelas falhas anteriormente descritas, possui orientação NW-SE, com aproximadamente um quilômetro de extensão, sendo caracterizado por dobras assimétricas curvilineares com eixos de mergulhos suaves (10° a 25°) para NW e SE. Essas dobras são seccionadas por falhas normais sinuosas NW-SE e/ou E-W, com baixo ângulo de mergulho (em torno de 10° a 30°), subordinadas a transcorrências destrais, gerando em escala de detalhes feições como drag folds. Observam-se ainda falhas inversas retas e/ou sinuosas NW-SE e zonas de falhas sub-verticalizadas WNW -ESE. As dobras individuais nesta área são estruturas do tipo reversas, flexurais e com geometria en echelon com orientação semelhante às dobras curvilineares: eixos com baixo ângulo de mergulho (10° a 25°) e caimento para SE. O conjunto de feições anteriormente descrito desenha, em escala quilométrica, um antiforme aberto, provavelmente resultante da acomodação do acamamento em resposta a deformação dessas falhas. O paralelismo entre feições observadas na área da Mina do Igarapé Azul e os lineamentos maiores que desenham a Falha Carajás em planta sugere uma relação com dois importantes episódios deformacionais ocorridos durante a história tectônica da Falha Carajás. As falhas normais associadas a componente direcional destral, de maior expressividade da área da mina, estariam relacionadas ao episódio de transtensão destral responsável pela instalação da Falha Carajás anterior a 2.6 Ga (Pinheiro, 1997). As dobras, as falhas de cavalgamento e as zonas de falhas sub-verticalizadas estariam relacionados a deformações sob regime de transpressão sinistral, um segundo evento atuante na região, responsável pela reativação e inversão da maioria das estruturas próximas à zona da Falha Carajás (Pinheiro, 1997; Pinheiro & Holdsworth, 2000; Lima, 2002).

Basaltos almofadados da Suíte Ofiolítica Morro do Agostinho: registros de fundo oceânico na porção centro-oeste do Cinturão Araguaia

Ao longo do domínio de baixo grau metamórfico (porção centro-oeste) do Cinturão Araguaia, afloram dezenas de corpos máficos e/ou ultramáficos de natureza ofiolítica. Cita-se como exemplo a Suíte Ofiolítica Morro do Agostinho nos arredores da cidade de Araguacema (TO) que configura um pequeno corpo isolado que sustenta o Morro do Agostinho e encontra-se encaixado tectonicamente em metarenitos, ardósias e filitos da Formação Couto Magalhães (Grupo Tocantins). A Suíte Ofiolítica Morro do Agostinho é constituída por peridotitos serpentinizados, basaltos e cherts ferríferos todos afetados por incipiente metamorfismo. A associação de basaltos é caracterizada por um expressivo derrame submarino com estruturas em lavas almofadadas, sobrepostas aos peridotitos serpentinizados. Os basaltos foram classificados em tipos maciços e hipovítreos com esferulitos. Os basaltos maciços são homogêneos, com textura intersertal definida, essencialmente, por finas ripas de plagioclásio, clinopiroxênio e raramente olivina, calcocita e calcopirita. Os basaltos hipovítreos apresentam feições texturais formadas por ultrarresfriamento de lavas apresentando esferulitos de plagioclásio, feixes de cristais aciculares e esqueletais de clinopiroxênio e plagioclásio, e cristais com terminações tipo rabo-de-andorinha. Geoquimicamente, os basaltos revelaram natureza subalcalina toleítica, compatíveis com o tipo MORB. As razões (La/Yb)_n < 1 e (La/Sm)_n < 1 apontam, mais especificamente, para magmas do tipo N-MORB na evolução dessas rochas relacionadas ao ambiente de fundo oceânico. Estas rochas revelaram que nos estágios iniciais da evolução do Cinturão Araguaia houve uma fase importante de oceanização da Bacia Araguaia, com exposição de peridotitos do manto litosférico seguido de extravasamento de lavas e sedimentação de cherts e formações ferríferas bandadas em ambiente oceânico profundo. Após o preenchimento sedimentar da Formação Couto Magalhães (Grupo Tocantins), e o descolamento da litosfera oceânica, a fase tectônica principal propiciou a inversão tectônica que levou à exumação dos corpos ofiolíticos, principalmente ao longo de superfícies de cavalgamento, fragmentando-os e misturando-os tectonicamente às rochas supracrustais, acompanhado de metamorfismo regional em condições da fácies xisto verde baixo. A Suíte Ofiolítica Morro do Agostinho representa, assim, um pequeno fragmento alóctone de um segmento litosférico manto/crosta oceânica, bem preservado, do início da evolução da Bacia Araguaia, similar a outros no Cinturão Araguaia, que é um importante registro da fase de oceanização do Cinturão Araguaia, durante o Neoproterozoico.

Petrologia magnética dos granodioritos Água Azul e Água Limpa, porção sul do Domínio Carajás - Pará

Os granodioritos Água Azul (GrdAA) e Água Limpa (GrdAL) afloram no extremo sul do Domínio Carajás como dois corpos alongados segundo o trend regional E-W, anteriormente inseridos no Complexo Xingu. O GrdAL é formado essencialmente por biotita-anfibólio granodioritos e muscovita-biotita granodioritos, além de anfibólio-biotita tonalitos subordinados; no GrdAA, epídoto-anfibólio-biotita granodioritos são dominantes, epídoto-anfibólio-biotita tonalitos e (anfibólio)-epídoto-biotita monzogranitos, subordinados. Essas rochas mostram assinaturas geoquímicas afins dos sanukitoides arqueanos. O estudo de suscetibilidade magnética (SM) mostrou valores relativamente baixos para o GrdAL (média de 17,54 × 10^-4 SIv) e o GrdAA (média de 4,19 × 10^-4 SIv). Os estudos dos minerais opacos mostram que a magnetita e a hematita são as fases comuns e que a ilmenita está ausente nessas rochas. O GrdAL contém titanita associada à magnetita, enquanto o GrdAA contém pirita, calcopirita e goethita. No GrdAL, a magnetita é mais abundante e desenvolvida que no GrdAA, justificando, assim, sua SM mais elevada. A martitização da magnetita e a oxidação dos sulfetos, gerando goethita, ocorreram a baixas temperaturas. A correlação positiva entre os valores de SM e os conteúdos modais de opacos, anfibólio, epídoto + allanita e quartzo + K-feldspato, assim como a correlação negativa de SM com biotita e máficos observadas nessas unidades, denunciam uma tendência no aumento de SM no sentido anfibólio tonalitos/anfibólio granodioritos à biotita granodioritos/biotita monzogranitos. Os dados geoquímicos corroboram esse comportamento, com correlação negativa entre os valores de SM e Fe₂O₃T, FeO e MgO, refletindo para as duas unidades uma tendência de aumento nos valores de SM paralelamente à diferenciação magmática. As afinidades geoquímicas e mineralógicas entre essas rochas e os sanukitoides do Domínio Rio Maria sugerem condições de fugacidade de oxigênio entre os tampões HM e FMQ para os granitoides estudados.

Caracterização petrográfica e geoquímica das rochas encaixantes da mineralização de ouro do alvo lavra velha - Ibitiara (BA)

The Lavra Velha gold prospect is located in Ibitiara city, in the Espinhaço Setentrional physiographic domain, on the west edge of Chapada Diamantina – central part of Bahia. It is inserting on Gavião Block, a compartment of São Francisco Cráton (Almeida, 1977). The Lavra Velha gold dump is formed by an association of hydrothermal breccia lodged in acid and intermediate rocks, classifying in tonalite, granodiorite and diorite, with high alteration, cut off by a vein and venules system constituted by hydrothermal association composed by hematite, tourmaline, quarz and sericite, located in the north limit of Ibitiara granite. In the regional geological context the area is represented by Archaean rocks (Paramirim Complex) and Paleoproterozoic rocks (Ibitiara granitoid and Matinos Granite) constituted the basement, following by paleo to mesozoic pluton-vulcanic-sedimentary association of Rio dos Remédios Group, intruded by mafic rocks. It was used geochemistry and petrographic analysis compiling to field works data to characterize the rocks where the gold mineralization is inserting. Previously these rocks were classifying in volcanic rocks of Novo Horizonte Formation. Developing this monograph’s work the petrogenetic characteristics suggesting that these rocks called volcanic actually belong to Ibitiara granitoid as a portion more metamorphosed. The green schist is the predominant metamorphism in the area with low deformation, associated to high concentration of fluid circulating. The hydrothermal alteration is the process responsible for rocks modifications and strong sericitization generalize

Seasonal Variation in Reception of Fin Whale Calls at Five Geographic Areas in the North Pacific

In late August 1991 scientists at the National Oceanic and Atmospheric Administration’s (NOAA) National Marine Mammal Laboratory (NMML) and Pacific Marine Environmental Laboratory (PMEL) began a pilot study to investigate the capability of hydrophones from the US. Navy’s fixed array system to detect large whales in the North Pacific by passive reception of their calls. PMEL had previously established a direct data link from five bottom-mounted arrays of the Navy SOSUS (Sound Surveillance System), via the Naval Oceanographic Processing Facility (NOPF) at Whidbey Island, Washington, to study low-level seafloor seismicity (Fox et al. 1994). PMEL subsequently provided NMML tapes of SOSUS hydrophone data from which whale calls were analyzed. As in an analogous study conducted in the North Atlantic (Nishimura and Conlon 1994, Clark 1995, Mellinger and Clark 1995), calls attributable to whales were received at each SOSUS site at rates that varied seasonally (Anonymous 1996).

Trophic structure on the West Antarctic Peninsula shelf: Detritivory and benthic inertia revealed by delta(13)C and delta(15)N analysis

Summer bloom-derived phytodetritus settles rapidly to the seafloor on the West Antarctic Peninsula (WAP) continental shelf, where it appears to degrade relatively slowly, forming a sediment ""food bank"" for benthic detritivores. We used stable carbon and nitrogen isotopes to examine sources and sinks of particulate organic material (POM) reaching the WAP shelf benthos (550-625 m depths), and to explore trophic linkages among the most abundant benthic megafauna. We measured delta(13)C and delta(15)N values in major megafaunal taxa (n = 26) and potential food sources, including suspended and sinking POM, ice algae, sediment organic carbon, phytodetritus, and macrofaunal polychaetes. The range in delta(13)C values (> 14 parts per thousand) of suspended POM was considerably broader than in sedimentary POC, where little temporal variability in stable isotope signatures was observed. While benthic megafauna also exhibited a broad range of VC values, organic carbon entering the benthic food web appeared to be derived primarily from phytoplankton production, with little input from ice algae. One group of organisms, primarily deposit-feeders, appeared to rely on fresh phytodetritus recovered from the sediments, and sediment organic material that had been reworked by sediment microbes. A second group of animals, including many mobile invertebrate and fish predators, appeared to utilize epibenthic or pelagic food resources such as zooplankton. One surface-deposit-feeding holothurian (Protelpidia murrayi) exhibited seasonal variability in stable isotope values of body tissue, while other surface- and subsurface-deposit-feeders showed no evidence of seasonal variability in food source or trophic position. Detritus from phytoplankton blooms appears to be the primary source of organic material for the detritivorous benthos; however, seasonal variability in the supply of this material is not mirrored in the sediments, and only to a minor degree in the benthic fauna. This pattern suggests substantial inertia in benthic-pelagic coupling, whereby the sediment ecosystem integrates long-term variability in production processes in the water column above. Published by Elsevier Ltd.

Temporal changes in benthic megafaunal abundance and composition across the West Antarctic Peninsula shelf: Results from video surveys

The West Antarctic Peninsula (WAP) shelf experiences intense seasonal and interannual variability in phytoplankton production and particulate-organic-carbon flux to the seafloor. To explore the response of the megabenthic community to this production variability, we conducted video surveys of epibenthic megafauna at three stations on the WAP shelf in Nov-Dec 1999, Mar 2000, Jun 2000, Oct-Nov 2000, and Feb-Mar 2001. The epibenthic megafauna was dominated (>90%) by elasipod holothurians, irregular urchins and anthozoans, with total abundances ranging from 19 to 152 ind. 1 00 m(-2). The abundance of three of the dominant taxa (Protelpidia murrayi, Peniagone vignomi, and Amphipneustes spp.) varied significantly across seasons (p <0.05), although variations were not tightly correlated with the summer bloom cycle. The irregular urchins in the genus Amphipneustes varied 5-fold in abundance at single stations, with maximum densities (an average of 10.1 ind. 100 m(-2)) attained in Jun 2000. Abundances of the elasipod holothurians P. murrayi (1-121 ind. 100 m(-2)) and P. vignoni (0.7-27.5 ind. 100 m(-2)) fell within the range for elasipod holothurians from other bathyal regions measured using image analysis. The abundance of P. murrayi increased up to 6-fold from a single Jun-Oct recruitment pulse, while changes in the abundance of P. vignoni (over 2-fold higher in Feb-Mar 2001) apparently resulted from immigration during the presence of a 1-2 cm thick carpet of fresh phytocletritus. Based on the ratio of the number of fecal casts per individual, elasipod holothurians increased surface-deposit feeding rates by >= 2-fold while phytocletritus was present at the seafloor. Nonetheless, these surface-deposit feeders appeared to feed and egest sediments throughout the winter, which is consistent with year-round persistence of a labile food bank in surficial sediments on the deep WAP shelf.

Factors structuring Fucus communities at open and complex coastlines in the Baltic Sea

This thesis deals with physical factors and biological interactions affecting the distribution of two fucoid species, Fucus vesiculosus and F. serratus, in the Baltic Sea. Studies have been carried out in two quite different environments: an archipelago, and an open rocky coast. The archipelago has an extremely long coastline with a heterogeneous submerged landscape of different substrate types, slopes, water qualities, and degrees of wave exposure. The factors influencing F. vesiculosus distribution, morphology and epiphyte composition were studied in the Stockholm archipelago using field surveys and spatial modelling in Geographic information systems (GIS). A GIS-method to estimate wave exposure was developed and validated by comparing the result to an index based on vertical zonation of lichens. Wave exposure was considered an important factor for predicting the distribution of F. vesiculosus by its ability to clean hard surfaces from silt, and a predictive model was constructed based on the information of wave exposure and slope of the shore. It is suggested that the lower distribution boundary of attached F. vesiculosus is set by sediment in sheltered parts of the archipelago, and by light availability in highly wave exposed parts. The morphology of F. vesiculosus was studied over a wave exposure gradient, and several characters responded in accordance with earlier studies. However, when separating effects of wave exposure from effects of other confounding water property parameters, only thallus width was significantly different. Several water property parameters were shown to be correlated with wave exposure in the Stockholm archipelago, and the mechanism responsible for the effects on F. vesiculosus morphology is discussed. The composition of epiphytes on F. vesiculosus varied over a wave exposure gradient with a positive correlation to Elachista fucicola, and a negative to Chorda filum. At an open coast the physical environment is much less heterogeneous compared to an archipelago. The distributions of F. vesiculosus, F. serratus, turf-forming algae, and the seafloor substrate, were surveyed along the open coasts of Öland and Gotland. Turf-forming algae dominated all hard substrates in the area, and Polysiphonia fucoides was most abundant. At the Gotland coast F. vesiculosus was less abundant than at the Öland coast, and F. serratus occurred only in the southern-most part. Fucus serratus was increasingly more common towards south which was interpreted as an effect mainly of the Baltic salinity gradient, or the variation of salinity that has occurred in the past. The effects of turf-forming algae and sediment on F. serratus recruitment at 7 m depth off the Öland east coast were studied in the field, and by laboratory experiments. Almost no recruits were found in the algal turf outside the F. serratus patches. More fine sediment was found in the turf than in the F. serratus patches, suggesting that the turf accumulates sediment by decreasing resuspension. Both filamentous algae and sediment decreased the attachment ability of F. serratus zygotes and survival of recruits, and sediment had the strongest effect. It is therefore suggested that F. serratus has difficulties recruiting outside its patches, and that these difficulties are enforced by the eutrophication of the Baltic Sea, which has favoured growth of filamentous algae and increased sedimentation. An overall conclusion is that Fucus distribution is affected by large-scale-factors, such as the eutrophication and salinity changes of the Baltic Sea, as well as by small-scale variation in wave exposure, substrate and slope, and by surface competition with neighbouring species.

Geochronological and structural evolution of the western and central Kaoko Belt in NW Namibia

This thesis focusses on the tectonic evolution and geochronology of part of the Kaoko orogen, which is part of a network of Pan-African orogenic belts in NW Namibia. By combining geochemical, isotopic and structural analysis, the aim was to gain more information about how and when the Kaoko Belt formed. The first chapter gives a general overview of the studied area and the second one describes the basis of the Electron Probe Microanalysis dating method. The reworking of Palaeo- to Mesoproterozoic basement during the Pan-African orogeny as part of the assembly of West Gondwana is discussed in Chapter 3. In the study area, high-grade rocks occupy a large area, and the belt is marked by several large-scale structural discontinuities. The two major discontinuities, the Sesfontein Thrust (ST) and the Puros Shear Zone (PSZ), subdivide the orogen into three tectonic units: the Eastern Kaoko Zone (EKZ), the Central Kaoko Zone (CKZ) and the Western Kaoko Zone (WKZ). An important lineament, the Village Mylonite Zone (VMZ), has been identified in the WKZ. Since plutonic rocks play an important role in understanding the evolution of a mountain belt, zircons from granitoid gneisses were dated by conventional U-Pb, SHRIMP and Pb-Pb techniques to identify different age provinces. Four different age provinces were recognized within the Central and Western part of the belt, which occur in different structural positions. The VMZ seems to mark the limit between Pan-African granitic rocks east of the lineament and Palaeo- to Mesoproterozoic basement to the west. In Chapter 4 the tectonic processes are discussed that led to the Neoproterozoic architecture of the orogen. The data suggest that the Kaoko Belt experienced three main phases of deformation, D1-D3, during the Pan-African orogeny. Early structures in the central part of the study area indicate that the initial stage of collision was governed by underthrusting of the medium-grade Central Kaoko zone below the high-grade Western Kaoko zone, resulting in the development of an inverted metamorphic gradient. The early structures were overprinted by a second phase D2, which was associated with the development of the PSZ and extensive partial melting and intrusion of ~550 Ma granitic bodies in the high-grade WKZ. Transcurrent deformation continued during cooling of the entire belt, giving rise to the localized low-temperature VMZ that separates a segment of elevated Mesoproterozoic basement from the rest of the Western zone in which only Pan-African ages have so far been observed. The data suggest that the boundary between the Western and Central Kaoko zones represents a modified thrust zone, controlling the tectonic evolution of the Kaoko belt. The geodynamic evolution and the processes that generated this belt system are discussed in Chapter 5. Nd mean crustal residence ages of granitoid rocks permit subdivision of the belt into four provinces. Province I is characterised by mean crustal residence ages <1.7 Ga and is restricted to the Neoproterozoic granitoids. A wide range of initial Sr isotopic values (87Sr/86Sri = 0.7075 to 0.7225) suggests heterogeneous sources for these granitoids. The second province consists of Mesoproterozoic (1516-1448 Ma) and late Palaeo-proterozoic (1776-1701 Ma) rocks and is probably related to the Eburnian cycle with Nd model ages of 1.8-2.2 Ga. The eNd i values of these granitoids are around zero and suggest a predominantly juvenile source. Late Archaean and middle Palaeoproterozoic rocks with model ages of 2.5 to 2.8 Ga make up Province III in the central part of the belt and are distinct from two early Proterozoic samples taken near the PSZ which show even older TDM ages of ~3.3 Ga (Province IV). There is no clear geological evidence for the involvement of oceanic lithosphere in the formation of the Kaoko-Dom Feliciano orogen. Chapter 6 presents the results of isotopic analyses of garnet porphyroblasts from high-grade meta-igneous and metasedimentary rocks of the sillimanite-K-feldspar zone. Minimum P-T conditions for peak metamorphism were calculated at 731±10 °C at 6.7±1.2 kbar, substantially lower than those previously reported. A Sm-Nd garnet-whole rock errorchron obtained on a single meta-igneous rock yielded an unexpectedly old age of 692±13 Ma, which is interpreted as an inherited metamorphic age reflecting an early Pan-African granulite-facies event. The dated garnets survived a younger high-grade metamorphism that occurred between ca. 570 and 520 Ma and apparently maintained their old Sm-Nd isotopic systematics, implying that the closure temperature for garnet in this sample was higher than 730 °C. The metamorphic peak of the younger event was dated by electronmicroprobe on monazite at 567±5 Ma. From a regional viewpoint, it is possible that these granulites of igneous origin may be unrelated to the early Pan-African metamorphic evolution of the Kaoko Belt and may represent a previously unrecognised exotic terrane.

Petrogenesis of dunite, wehrlite and websterite xenoliths from Kimberley, South Africa: Origin as mantle peridotites of cumulates

Dunite, wehrlite and websterite xenoliths occur amongst a large abundance of mantle xenoliths in kimberlites of the Kimberley cluster in South Africa. Up to know they have mostly been neglected. On the basis of texture, major and trace elements, oxygen isotopes as well as Re-Os isotope characteristics, they can be subdivided into two groups. A coarse-grained mantle peridotite group, comprising dunite, wehrlite and websterite xenoliths, that are similar to fertile peridotites and represent upper mantle assemblages that are differently influenced by mantle metasomatism. And a cumulate group, containing fine-grained Fe-rich dunite xenoliths that represent cumulates of flood basalt magmatism related to ~183 Ma Karoo and ~2.7 Ga Ventersdorp events in southern Africa. Dunite, wehrlite and websterite xenoliths have preserved a complex history of melt depletion and metasomatic re-enrichment events, which gives information about the different re-enrichment stages of the subcratonic lithospheric mantle and the spatial differences within the Kaapvaal craton upper mantle. Websterite xenoliths comprise orthopyroxene (40-85 Vol. %), clinopyroxene (5-42 Vol. %), garnet (4-10 Vol. %) and subordinately olivine, while dunite and wehrlite xenoliths contain predominantly olivine (65-100 Vol %) and subordinately orthopyroxene, clinopyroxene and garnet. High melt depletion and a dunitic to harzburgitic protolith composition are reflected by high forsterite (Fo90-92) and high olivine NiO contents (2800-5000 ppm) and high orthopyroxene Mg# (Mg/(Mg+Fe)) of 0.91-0.93. Re-depletion ages of predominantly 2.9 Ga reflect a minimum age of melt depletion. Melt depletion ceased in conjunction with collision of the Kimberley block with the Witwatersrand block ~2.9 Ga ago. Subduction related re-fertilisation of the previously depleted mantle xenoliths is documented by i) amoeboid textured orthopyroxene, clinopyroxene and garnet, which crystallized in schlieren along olivine grain boundaries, ii) high whole-rock SiO2, Al2O3, CaO, TiO2, FeO contents, iii) low oxygen isotope ratios in clinopyroxene and garnet of 4.8-5.4 ‰ and 4.7-5.3 ‰, respectively and iv) trace element compositions of wehrlitic clinopyroxene and garnet in equilibrium with high-pressure partial melts of eclogite. Trace element disequilibrium of orthopyroxene with clinopyroxene and garnet indicates a separate origin for orthopyroxene, on one side as primary mantle orthopyroxene in dunite and wehrlite xenoliths and on the other side as reaction product with Si-rich melts produced by partial melting of eclogite. This reaction triggered replacement of olivine by orthopyroxene in the surrounding mantle and produced the typical Si-rich composition of Kaapvaal mantle peridotites. Partial melting of eclogite at higher temperatures produced a second metasomatic melt with lower SiO2, but higher Al2O3, CaO, FeO, Ti, Zr, Hf and a low oxygen isotope ratio. This melt triggered clinopyroxene and locally garnet and rutile crystallization in percolation veins, replacing olivine and orthopyroxene in the Kaapvaal upper mantle. Additionally, websterite xenoliths have experienced late stage cryptic metasomatism by the host kimberlite melt, changing the trace element composition of clinopyroxene, orthopyroxene and garnet to different extent. Hence websterite and most fertile lherzolite xenoliths have experienced three metasomatic events: i) reaction with high-Si melt, ii) percolation of subduction related silica melt with lower SiO2 content and iii) cryptic metasomatism by kimberlite. In contrast, dunite and wehrlite xenoliths have only experienced the second metasomatic event. They represent mantle lithologies further away from metasomatising agents. The Fe-rich dunites comprise olivine neoblasts with subordinate olivine porphyroclasts and parallel-orientated needles of ilmenite, which may enclose spinel. The lower forsterite and NiO contents of olivine in Fe-rich dunites compared to mantle peridotite xenoliths (Fo87-89 vs. Fo93-95 and 1300-2800ppm vs. 2200-3900 ppm, respectively), rules out a restitic origin. Cr-rich spinels are remnants of the original cumulate mineralogy that survived a late stage metasomatic overprint related to the production of the host kimberlite, producing ilmenite and phlogopite in some samples. Olivine porphyroclasts and neoblasts have different trace element compositions, the latter having high Ti, V, Cr and Ni and low Zn, Zr and Nb contents, indicating contrasting origins for neoblasts and porphyroclasts. The dunites have high 187Os/188Os ratios (0.11-0.15) indicating young (Phanerozoic) model ages for most samples, whereas three samples show isotopic mixtures between Phanerozoic neoblasts and ancient porphyroclastic material. Most Fe-rich dunite xenoliths can be interpreted as cumulates of fractional crystallization of Karoo magmatism, whereas the porphyroclasts are interpreted to be remnants from the much earlier Archaean Ventersdorp magmatism.

Deciphering petrological signatures of reactive melt stagnation and cooling in the oceanic mantle underneath ultraslow-spreading ridges

The global mid-ocean ridge system creates oceanic crust and lithosphere that covers more than two-thirds of the Earth. Basalts are volumetrically the most important rock type sampled at mid-ocean ridges. For this reason, our present understanding of upper mantle dynamics and the chemical evolution of the earth is strongly influenced by the study of mid-ocean ridge basalts (MORB). However, MORB are aggregates of polybarically generated small melt increments that can undergo a variety of physical and chemical processes during their ascent and consequently affect their derivative geochemical composition. Therefore, MORB do not represent “direct” windows to the underlying upper mantle. Abyssal peridotites, upper mantle rocks recovered from the ocean floor, are the residual complement to MORB melting and provide essential information on melt extraction from the upper mantle. In this study, abyssal peridotites are examined to address these overarching questions posed by previous studies of MORB: How are basaltic melts formed in the mantle, how are they extracted from the mantle and what physical and chemical processes control mantle melting? The number of studies on abyssal peridotites is small compared to those on basalts, in part because seafloor exposures of abyssal peridotites are relatively rare. For this reason, abyssal peridotite characteristics need to be considered in the context of subaerially exposed peridotites associated with ophiolites, orogenic peridotite bodies and basalt-hosted xenoliths. However, orogenic peridotite bodies are mainly associated with passive continental margins, most ophiolites are formed in supra-subduction zone settings, and peridotite xenoliths are often contaminated by their host magma. Therefore, studies of abyssal peridotites are essential to understanding the primary characteristics of the oceanic upper mantle free from the influence of continental rifting, subduction and tectonic emplacement processes. Nevertheless, numerous processes such as melt stagnation and cooling-induced, inter-mineral exchange can affect residual abyssal peridotite compositions after the cessation of melting. The aim of this study is to address these post-melting modifications of abyssal peridotites from a petrological-geochemical perspective. The samples in this study were dredged along the axis of the ultraslow-spreading Gakkel Ridge in the Arctic Ocean within the “Sparsely Magmatic Zone”, a 100 km ridge section where only mantle rocks are exposed. During two expeditions (ARK XVII-2 in 2001 and ARK XX-2 in 2004), exceptionally fresh peridotites were recovered. The boulders and cobbles collected cover a range of mantle rock compositions, with most characterized as plagioclase-free spinel peridotites or plagioclase- spinel peridotites. This thesis investigates melt stagnation and cooling processes in the upper mantle and is divided into two parts. The first part focuses on processes in the stability field of spinel peridotites (>10 kb) such as melt refertilization and cooling related trace element exchange, while the second part investigates processes in the stability field of plagioclase peridotites (< 10 kb) such as reactive melt migration and melt stagnation. The dissertation chapters are organized to follow the theoretical ascent of a mantle parcel upwelling beneath the location where the samples were collected.

Variation of stable silicon isotopes: Analytical developments and applications in Precambrian geochemistry

Die vorliegende Dissertation behandelt die Gesamtgesteinsanalyse stabiler Siliziumisotope mit Hilfe einer „Multi Collector-ICP-MS“. Die Analysen fanden in Kooperation mit dem „Royal Museum for Central Africa“ in Belgien statt. Einer der Schwerpunkte des ersten Kapitels ist die erstmalige Analyse des δ30Si –Wertes an einem konventionellen Nu PlasmaTM „Multi-Collector ICP-MS“ Instrument, durch die Eliminierung der den 30Si “peak” überlagernden 14N16O Interferenz. Die Analyse von δ30Si wurde durch technische Modifikationen der Anlage erreicht, welche eine höherer Massenauflösung ermöglichten. Die sorgsame Charakterisierung eines adäquaten Referenzmaterials ist unabdingbar für die Abschätzung der Genauigkeit einer Messung. Die Bestimmung der „U.S. Geological Survey“ Referenzmaterialien bildet den zweiten Schwerpunkt dieses Kapitales. Die Analyse zweier hawaiianischer Standards (BHVO-1 and BHVO-2), belegt die präzise und genaue δ30Si Bestimmung und bietet Vergleichsdaten als Qualitätskontrolle für andere Labore. Das zweite Kapitel befasst sich mit kombinierter Silizium-/Sauerstoffisotope zur Untersuchung der Entstehung der Silizifizierung vulkanischer Gesteine des „Barberton Greenstone Belt“, Südafrika. Im Gegensatz zu heute, war die Silizifizierung der Oberflächennahen Schichten, einschließlich der „Chert“ Bildung, weitverbreitete Prozesse am präkambrischen Ozeanboden. Diese Horizonte sind Zeugen einer extremen Siliziummobilisierung in der Frühzeit der Erde. Dieses Kapitel behandelt die Analyse von Silizium- und Sauerstoffisotopen an drei unterschiedlichen Gesteinsprofilen mit unterschiedlich stark silizifizierten Basalten und überlagernden geschichteten „Cherts“ der 3.54, 3.45 und 3.33 Mill. Jr. alten Theespruit, Kromberg und Hooggenoeg Formationen. Siliziumisotope, Sauerstoffisotope und die SiO2-Gehalte demonstrieren in allen drei Gesteinsprofilen eine positive Korrelation mit dem Silizifizierungsgrad, jedoch mit unterschiedlichen Steigungen der δ30Si-δ18O-Verhältnisse. Meerwasser wird als Quelle des Siliziums für den Silizifizierungsprozess betrachtet. Berechnungen haben gezeigt, dass eine klassische Wasser-Gestein Wechselwirkung die Siliziumisotopenvariation nicht beeinflussen kann, da die Konzentration von Si im Meerwasser zu gering ist (49 ppm). Die Daten stimmen mit einer Zwei-Endglieder-Komponentenmischung überein, mit Basalt und „Chert“ als jeweilige Endglieder. Unsere gegenwärtigen Daten an den „Cherts“ bestätigen einen Anstieg der Isotopenzusammensetzung über der Zeit. Mögliche Faktoren, die für unterschiedliche Steigungen der δ30Si-δ18O Verhältnisse verantwortlich sein könnten sind Veränderungen in der Meerwasserisotopie, der Wassertemperatur oder sekundäre Alterationseffekte. Das letzte Kapitel beinhaltet potentielle Variationen in der Quellregion archaischer Granitoide: die Si-Isotopen Perspektive. Natriumhaltige Tonalit-Trondhjemit-Granodiorit (TTG) Intrusiva repräsentieren große Anteile der archaischen Kruste. Im Gegensatz dazu ist die heutige Kruste kaliumhaltiger (GMS-Gruppe: Granit-Monzonite-Syenite). Prozesse, die zu dem Wechsel von natriumhaltiger zu kaliumhaltiger Kruste führten sind die Thematik diesen Kapitels. Siliziumisotopenmessungen wurden hier kombiniert mit Haupt- und Spurenelementanalysen an unterschiedlichen Generationen der 3.55 bis 3.10 Mill. Yr. alten TTG und GMS Intrusiva aus dem Arbeitsgebiet. Die δ30Si-Werte in den unterschiedlichen Plutonit Generationen zeigen einen leichten Anstieg der Isotopie mit der Zeit, wobei natriumhaltige Intrusiva die niedrigste Si-Isotopenzusammensetzung aufweisen. Der leichte Anstieg in der Siliziumisotopenzusammensetzung über die Zeit könnte auf unterschiedliche Temperaturbedingungen in der Quellregion der Granitoide hinweisen. Die Entstehung von Na-reichen, leichten d30Si Granitoiden würde demnach bei höheren Temperaturen erfolgen. Die Ähnlichkeit der δ30Si-Werte in archaischen K-reichen Plutoniten und phanerozoischen K-reichen Plutoniten wird ebenfalls deutlich.