The Panzhihua intrusion is one of several large Fe-Ti oxide ore bearing intrusions related to the major flood volcanism of the Emeishan Large Igneous Province (ELIP), SW China. The Panzhihua intrusion in particular has recently become the focus of numerous studies owing to the excellent exposure in large open pit mining operations. The formation of Fe-Ti oxide ore layers has been the focus of these studies and has become a somewhat controversial topic with three separate models currently proposed for ore formation. The gabbroic Panzhihua intrusion extends for ± 19 km along strike, has a maximum thickness of 3000 m and hosts extensive (up to 60 m thick) Fe-Ti oxide ore layers in the lower portions of the intrusion. The intrusion has been divided into five zones: marginal zone (MGZ), lower zone (LZ), middle zone A (MZa), middle zone b (MZb) and the upper zone (UZ). The gabbroic rocks are comprised of plagioclase, clinopyroxene and interstitial Fe-Ti oxides with minor olivine. Apatite is present within the MZb only and shows no correlation with Fe-Ti oxide ore layers. Fe-Ti oxides are present throughout the stratigraphy of the intrusion. This is unlike typical layered intrusions where significant Fe-enrichment through fractionation of Fe-poor silicate phases (i.e. plagioclase) is required before Fe-Ti oxide saturation. There are no oxide-free cumulate rocks at the Panzhihua intrusion, implying either an evolved parent magma or very high Fe content of the source rocks. I present here new mineral composition data, whole-rock major and trace element geochemistry along with whole-rock Sr-Nd isotopes and PGEs in order to constrain the evolution of the Panzhihua parent magma en route from source to chamber and the formation of Fe-Ti oxide ore layers. Furthermore an initial pilot study using O-isotope data is conducted on Ti-magnetite and plagioclase separates from gabbroic vs. ore rocks. Results are coupled with detailed thermodynamic modeling using the software PELE in order to further constrain Fe-Ti oxide ore layer formation. The intrusion is characterised by extreme depletion of PGEs relative to the coeval flood basalts and picrites. High Cu/Pd and Pd/Pt imply two separate stages of S-saturated and S-undersaturated depletion of PGEs. Pd is highly compatible in sulphide and is quickly scavenged by sulphide liquids resulting in an increase in Cu/Pd of the residual liquid. Furthermore decoupling of Pd and Pt can be achieved by either late stage hydrothermal alteration or through S-undersaturated stage of PGE depletion where Pt is scavenged by Pt-rich alloys or oxide minerals. I show that the latter is more likely. Fractionation modeling suggests that the Panzhihua parent magma formed at depth from original picritic magma. This is consistent with several other recent studies on other layered intrusions of the ELIP. Sr-Nd isotopic ratios indicate very little crustal contamination has occurred en route to the current chamber. Sr and Nd concentrations of footwall rocks are too low to produce any significant change in initial Sr and Nd isotopic ratios of the intruding basaltic magmas, indicating that crustal contamination will not be indicated by Sr-Nd isotopic ratios. Gradational change in the Sr-Nd isotope ratios across the MGZ provides strong evidence for formation in an open system by multiple replenishments of progressively less contaminated magmas from depth. Contamination is difficult to constrain but must be occurring prior to emplacement at the current level (low Sr and Nd contents of footwall). A gradational upward decrease in highly incompatible element across the MGZ can then be explained by continuous magma flow, which effectively removes the evolved intercumulus liquids from the growing cumulate pile at the base of the chamber. The initial stages of formation of the Panzhihua intrusion are interpreted to result from prolonged low volume pulses of magma into a slowly opening chamber. The timing of Fe-Ti oxide crystallisation is fundamental in the understanding of the petrogenesis of ore layers. Distinct geochemical variation in whole-rock Fe2O3/TiO2 and Zr/Nb indicates that Timagnetite is the dominant oxide within the lower ± 270 m of the intrusion whereas above this level both Ti-magnetite and ilmenite are present as cumulus phases. This is interpreted to indicate a variation in the fO2 where the lower intrusion crystallises at higher fO2 relative to that above this level. Silicates within the ore layers, in particular plagioclase, are highly embayed and resorped where in contact with Fe-Ti oxides. This characteristic of the silicate grains implies early crystallisation prior to Fe-Ti oxides with subsequent disequilibrium conditions resulting in resorption. Furthermore distinct reaction rims of kaersutite amphibole, Fo-enriched olivine, An-enriched plagioclase and pleonaste are observed. The abundance of amphibole suggests H2O involvement in this reaction and consumption of silicates. A model for parent magma crystallisation at various H2O contents indicates that plagioclase crystallisation temperature is very sensitive to H2O content of the parent magma. Plagioclase crystallises early for “dry” compositions but significantly later for “wet” compositions. Fe-Ti oxide ore layers are generally well layered, contain gabbroic xenoliths and are observed raversing/cross-cutting the cumulate stratigraphy. I present here a new model for ore layer formation in order to account for these distinct features of the ore layers. A model invoking multiple replenishments of magma with variable oxide microphenocryst content, H2O content and volume is proposed. Magma evolving in the plumbing system and fed to the Panzhihua chamber is variably enriched in H2O, which results in significantly different crystallisation paths. High H2O magmas (> 2 wt %) crystallise Fe-Ti oxides early whereas low H2O magmas (< 1 wt %) crystallise oxides late. Early pulses of H2O-poor magma crystallise a sequence of plag+cpx+Fe-Ti oxide (±ol). Later pulses of H2Orich magma subsequently intrude the partially crystallised cumulate sequence incorporating and consuming previously crystallised silicates with subsequent early crystallisation of Ti-magnetite and formation of ore layers. H2O-rich magmas likely have suspended Ti-magnetite microphenocrysts as well, which crystallise at depth in the plumbing system. This model can account for the various characteristic features of the Fe-Ti oxide ore layers at the Panzhihua intrusion as well as other Fe-Ti oxide ore bearing intrusions in the region.

Conselho Nacional de Desenvolvimento Científico e Tecnológico / O tema abordado nesta dissertação de mestrado é a petrogênese dos diabásios do Eocretáceo que integram o Enxame de Diques da Serra do Mar na região de Angra dos Reis (RJ). Estes diques intrudem rochas do Terreno Ocidental e do Arco Magmático Rio Negro, inserindo-se no contexto geodinâmico de fragmentação do Gondwana no Cretáceo Inferior. Essas intrusões são subverticais e orientam-se preferencialmente a N039E. Intrusões retilíneas são as mais observadas em campo. Os diabásios são compostos, essencialmente, por plagioclásio e clinopiroxênios (augita e pigeonita). Quartzo, minerais opacos, apatita e olivina ocorrem como minerais acessórios. A composição mineral secundária é marcada pela presença de biotita, uralita e saussurita. Os diabásios estudados compreendem uma série transicional com afinidade toleítica. Os estudos petrológicos revelam a existência de cinco suítes de alto-TiO2, tendo sido as mesmas discriminadas com base nas razões La/Yb de amostras com o mesmo teor de MgO. Destas, apenas a suíte 2 têm quantidade mínima de amostras para avaliação de processos evolutivos. O resultado da modelagem petrogenética aponta que o processo evolutivo mais provável para a geração dos diabásios da suíte 2 é cristalização fracionada sem mudança na assembleia fracionante. As amostras representativas dos líquidos parentais das cinco suítes apresentam razões La/Nb e La/Yb maiores que a unidade, típicas de derivação de fonte enriquecida, que, em várias províncias basálticas continentais, tem sido associada à fusão exclusiva do manto litosférico subcontinental ou a sua participação em processos de mistura de fontes. A discriminação de fontes mantélicas foi feita exclusivamente com base nos teores de elementos traços de amostras representativas de líquidos parentais das cinco suítes discriminadas na área de estudo. Os modelos indicam que todas as cinco suítes estudadas estão relacionadas a fontes harzburgíticas com granada residual. A suíte 5 da área de estudo não pode ser associada à mesma fonte mantélica geradora das suítes 1, 2, 3 e 4 que, por sua vez, se originaram por diferentes quantidades de fusão parcial (respectivamente, 44%, 35%, 31% e 25%) de uma mesma fonte. Cabe ressaltar que a ocorrência de duas suítes, com razões La/Yb muito distintas, porém geograficamente muito próximas, sugere que processos de heterogeneidade mantélica, tipicamente laterais, devem também ocorrer verticalmente. / The petrogenesis of Early Cretaceous dolerites within the Serra do Mar Dyke Swarm in the region of Angra dos Reis (RJ) is presented in this dissertation. The dykes are associated with the Gondwana breakup and intrude rocks of the so-called Occidental Terrane and the Rio Negro Magmatic Arc within the Late Proterozoic-Ordovician Ribeira Orogen. Tipically, the intrusions are subvertical bearing a N039E preferential trend with sharp, linear contacts with their country rocks. The dolerites are essentially composed of plagioclase and clinopyroxene (augite and pigeonita). Quartz, opaque minerals, apatite and olivine occur as accessory minerals. The secondary phases are biotite, eterog and eterogene. The dolerites constitute a transitional series with tholeiitic affinity. Whole-rock geochemical data reveal the existence of five high-TiO2 suites which were discriminated on the basis of La/Yb ratios for samples with similar MgO contents. Petrogenesis analysis were done for suite 2 only due to scarcity of samples in the other four suites. As such, petrogenetic interpretation and modeling points to fractional crystallization as the likely evolutionary process associated with suite 2 dolerites. Samples representing parental liquids of five the high-TiO2 suites show values of La/Nb and La/Yb ratios greater than unity which points to at least a contribution of the subcontinental lithospheric mantle (SCLM) for their genesis. Nevertheless, source mixing processes may have operated since the marked composition of the SCLM (as the Nb depletion, for instance) tends to obliterate most of the geochemical characteristics of other mantle sources. Petrogenetic eteroge indicates that the all five studied suites are related to harzbugitic sources with residual garnet pointing to a thick SCLM by the time of the Gondwana breakup. Suite 5 cannot be associated with the same mantle source that generated suites 1, 2, 3, and 4 which in turn can be related to different amounts of partial melting from a common mantle source (respectively, 44%, 35%, 31% and 25%). As all five suites are close related in space, processes involving vertical chemical eterogeneities within the SCLM as opposed to lateral ones should be considered when putting constraints on geodynamic models for the Gondwana breakup.

This study is an account of the stratigraphic sequence, the petrography, mineralogy (microprobe investigations of orthopyroxene, clinopyroxene, olivine and plagioclase feldspar), and whole-rock major- and traceelement geochemistry of the silicate cumulates of the Upper Critical Zone in the western Bushveld Complex. Two parts of the study - an investigation of a 350m column incorporating the MG3 and UGI Footwall Units, and a comparison of two additional Upper Critical Zone profiles with a previously compiled profile between the UGI and Bastard Units - are focused on RPM Union Section in the northwestern sector of the Complex. The third part is a detailed vertical and lateral investigation of the Bastard Unit at the top of the Critical Zone, which draws on sampling and data compilation from seventeen profiles in the western limb of the Complex. The MG3 Unit (45m) is made up of a lower chromitite layer overlain by a norite-pyroxenite-anorthosite sequence while the UGlFW Unit (295m) is composed of a related series of lower chromitite layers (MG4) overlain by a pyroxenite-norite-anorthosite sequence capped by the UGI chromitite layer. These mafic cumulates display a distinctive pattern of oscillating cryptic variation in whole-rock Mg/(Mg+Fe), FeO/Ti0₂, Cr/Co and Ni/V ratios through the sequence. Sympathetic oscillations are recorded for compositions of orthopyroxene and plagioclase feldspar and eight subcycles are recognised through the UGlFW Unit. The entire sequence is characterised by the presence of small, spheroidal, embayed and irregularly shaped plagioclase grains which are poikilitically enclosed in cumulus orthopyroxene grains of both pyroxenites and norites. This texture is indicative of partial resorption of pre-existing feldspar primocrysts within the melt prior to their being incorporated into the host orthopyroxene grains. Textural, geochemical and isotopic data suggest that this sequence was built up by periodic additions of fresh, relatively primitive liquid into fractionated resident liquid, and subsequent mixing within the magma chamber. The Bastard Unit sequence, described in Chapter 4, is the last and most complete cyclic unit (c. 60m) of the Critical Zone, and its upper contact defines the boundary between the Critical and Main Zones of the Complex. This Unit can conveniently be sub-divided into a lower part, where orthopyroxene occurs as a cumulus phase, and the upper part which is composed entirely of anorthosite (Giant Mottled Anorthosite). The basal part of the Unit (≤ 18m) comprises a thin chromitite layer < O.5cm) overlain by a pyroxenite-melanorite-norite-leuconorite sequence. The basal pyroxenite is orthocumulate in character and rapidly gives way to norites and leuconorites. A distinct threefold subdivision emerges within the Giant Mottled Anorthosite which is predominantly an adcumulate which becomes orthocumulate in character at its top. Apart from minor deviations in thicknesses these lithologies are recorded over the entire strike-length covered in this study. Profiles of cryptic variation are compiled for orthopyroxene, plagioclase and whole-rock data and show that the Bastard Unit displays a characteristic pattern which is maintained throughout the western Bushveld Complex. A minor yet distinctive reversal in cryptic variation is revealed at a level which is stratigraphically variable within the lower Giant Mottled Anorthosite, and results in a double cuspate pattern. A remarkable feature of the basal Bastard pyroxenites is that although the modal proportion of mafic to felsic constituents varies systematically away from the northwestern sector, the Mg/(Mg+Fe) ratio of orthopyroxenes remains constant at 0.804 over a lateral strike distance of 171km. Within the upper part of the Unit the orthopyroxene is markedly Fe-rich and it is here that inverted primary pigeonite appears for the first time as a cumulus phase. In addition, K-feldspar, oscillatory zoned plagioclase grains and high levels of incompatible trace elements are noted at this level. On the basis of the data presented it is concluded that the Bastard Unit represents the crystallisation of a final, relatively large influx of hotter primitive liquid, with upper Critical Zone affinities, and subsequent mixing with a column of cooler (less dense) supernatant liquid which had in part hybridized with the overlying Main Zone magma. It is hypothesised that this new liquid was emplaced as a basal flow beneath supernatant liquid and that it initiated the deposition of mafic cumulates at its base. The supernatant liquid is interpreted as representing the fractionated residuum produced by crystallisation of earlier cyclic units, with plagioclase on the liquidus, and that it contained an abundance of small plagioclase primocrysts in suspension. Development of the Unit can be viewed as a two-stage process. In the lower half of the unit, chemical and physical parameters typical of the new magma dominated the crystallisation process, and resulted in cumulates very similar to other relatively complete Upper Critical Zone units. In the upper, leucocratic sequence, above a minor reversal, crystallisation was from a liquid which was the product of mixing of a minor pulse of primitive liquid with the reservoir of hybridized supernatant liquid. Although the Bastard Unit is not continuous around the entire Western limb of the Complex, it is concluded that it developed in a single, or connected, magma chamber and that its irruptive feeder zone was located in the proximal northwestern facies of the Complex.

The Snake River Plain (SRP) is one of the best-preserved examples of continental hotspot volcanis, with a continuous record of volcanism that extends over 16 Ma to the present. Yellowstone-Snake River Plain records the migration of plume-tail volcanism from inception at the Bruneau-Jarbridge caldera complex at 12.6 Ma to its present locus, under the Yellowstone Plateau. Records kept by the Snake River Plain volcanic actions include rhyolite lavas and ignimbritesm minor coeval basalts, and an overlying veneer of younger basalts. The central SRP has received comparatively little attention in the past. The Kimama core hole was drilled as part of Project Hotspot, the Snake River Scientific Drilling Project, which seeks to understand the long-term volcanic and sediment logical history of the SRP volcanic province. The Kimama core hole is the only part of the SRP that has not been scientifically drilled and cored to a significant depth in the past. Investigations of subsurface stratigraphy in continental volcanic provinces such as the SRP-YP are limited by the by the relatively low depth and spatial distribution of cored wells. The study of the Kimama core provides us with a continuous record of basalt and minor sediment deposition. The long-term volcanic history of the SRP, documented by moving magma and its composition, demonstrates that magmatism is mantle plume-derived. Our investigation of the Kimama core, combined with new mantle tomography, provides evidence that refutes non-plume models for the origin of the Snake River Plain volcanic province.

The Motzfeldt centre is one of four major alkaline centres belonging to the Igaliko complex of South Greenland. The melts parental to the Motzfeldt centre are interpreted from Hf isotopes to be derived form a common mantle source which experienced subsequent isotopic contamination from older crustal components during the interval between segregation and emplacement. Magmatism within the centre commenced with the emplacement of the Motzfeldt Sø Formation at 1273 ± 8 Ma. This unit is unique within the Motzfeldt intrusion as it is characterised by a high degree of textural and mineralogical variability and hosts localised Nb, Ta, U, Th, Zr and REE mineralisation associated with pyrochlore and late-stage REE bearing carbonate phases. Biotite halogen contents show that in addition to enrichment of incompatible elements the MSF and Motzfeldt centre in general is particularly rich in F. The elevated F content is inferred to have extended the crystallisation interval of the melt and facilitated fractionation down to relatively low temperatures. The unusual enrichment of F and incompatible elements in the MSF is suggested to represent the first and most evolved melts extracted from the top of a stratified storage chamber at depth. The MSF is also characterised by pervasive subsolidus alteration, giving the rock and region a striking brick red colour. Pb-Pb pyrochlore studies indicate that alteration in the formation was effectively synchronous (1267 ± 6 Ma), with the magmatic age of emplacement. Fluid inclusion studies suggest that contemporaneous to the exsolution of juvenile, high salinity, F-rich fluids was the wholesale influx of hydrothermally convected low salinity groundwaters through the formation. The presence of pervasive late-stage hematite and calcite throughout the MSF suggests that the oxidation potential of the bulk fluid increased above the hematite-magnetite buffer during the waning stages of the hydrothermal phase. Mineralisation was promoted by this shift in fluid composition, reducing the complexing potential of fluid ligands and facilitating mineralisation within the high-levels units of the intrusion where alteration is most intense. Economic mineralisation associated with the centre is inferred to be largely sourced from the parental melts, however the role the hydrothermal phase played was particularly important in locally mobilising and concentrating incompatible elements within the high-level units of the formation.

During the Geological Survey of Canada’s Cumberland Peninsula Integrated Geoscience project a ~150km long NE-SW trending volcanic belt, now termed the North Touak-Cape Dyer volcanic belt, was mapped. The volcanic rocks that comprise the belt are dominantly green weathering komatiitic rocks with some black weathering tholeiitic occurrences. Given the similar stratigraphic position, textures, mineralogy, and geochemical characteristics of the volcanic rocks throughout the belt they have been termed the Totnes Road formation, after the locality from which they were first described. The komatiitic rocks possess numerous unusual characteristics for ultramafic volcanic rocks including: fragmental textures, lack of spinifex texture, young eruption age (Paleoproterozoic), eruption through ancient continental crust, and enrichment in the HFSEs including the REEs. This places them in the uncommon and poorly understood sub-type of komatiites termed Karasjok-type komatiites. Given the ultramafic nature of the rocks and their within-plate geochemical signatures, a mantle plume is the most likely source of these rocks, with the komatiites being sourced from the hot plume axis and the tholeiites from the cooler plume head. Incorporation and melting of mantle enriched by the addition of subduction zone recycled, garnet-bearing eclogitic material, beneath thick lithosphere could cause the rocks geochemical enrichment. Stratigraphically overlying the Totnes Road formation is a variety of chemical sedimentary rocks including chert, sulphide and silicate facies iron formation, and sulphide-rich boulders. Given their consistent stratigraphic position and parallel REE patterns, these rocks have been interpreted as a co-genetic suite and are grouped under the Clephane Bay formation, after a locality that exposes a spectacular section of the chemical rocks. The variety of lithologies is believed to be due to mixing of hydrothermal and detrital inputs during deposition within an anoxic basin. Regional correlations in the area are tentative due to the lack of available geochronological and geochemical data. Mafic-ultramafic volcanic occurrences to both the north and the south of the Cumberland Peninsula show remarkably similar geochemical characteristics to the Totnes Road formation. Thus it is possible that one plume was the source for numerous volcanic occurrences within in the region but more detailed study is required to prove or disprove this possibility.

The Mesoproterozoic rocks of the Bysteek and Koenap Formations of the Arribees Group are exposed within a NW-SE striking antiformal structure comprised of mafic granulites and metapelitic diatexites, and a number of marble and calc-silicate rock layers. The mafic granulites of the Bysteek Formation show a typological variety of anatectic features, including nebulitic, stromatitic mesosomes, melanosomes, quartz syenitic leucocratic vein networks and syenitic pools. Melanosomes consist of hedenbergitic to diopside-rich clinopyroxene (XMg: 0.40), anorthitic plagioclase (An90), with some quartz, minor apatite and titanite. Anatexis was caused by biotite dehydration melting and formed a melt of probably granitic composition. The leucosome composition ranges from either alkali-feldspar-granitic to plagioclase rich or granitic. This variation is interpreted as a result of variable extraction of melt from the source to granitic pools. The diatexites of the Koenap Formation are most likely of metapelitic or meta-greywacke origin. They are texturally variable but always contain high modal contents of alkali feldspar and quartz which generally form magmatic textures. Almandine-rich garnet (XMg: 0.18-0.25), cordierite (XMg: 0.71) form secondary biotite, sillimanite and magnetite during retrograde breakdown. Thermodynamic modelling of mafic granulite compositions suggests peak P-T conditions of ~865 °C and 8.6 kbar. Occasionally, garnet rich in ferric iron (XAdr: 0.55) forms by plagioclase-clinopyroxene breakdown under oxidising conditions at ~6 kilobar and ~ 800 °C. At the same stage amphibole forms in some melanosomes. P-T estimations for the diatexites based on thermodynamic modelling suggest the equilibration of the assemblage garnet, cordierite, alkali feldspar and melt at ~860 °C and 5.5 kbar. Conditions comparable to the peak pressure in the mafic granulites could not be established. However, since the diatexites and the mafic granulites are closely related in the field and no evidence of juxtaposition after the thermal peak exists, the P-T record of the diatexites might be incomplete

Conselho Nacional de Desenvolvimento Científico e Tecnológico / Lamprófiros e diabásios alcalinos afloram no litoral dos estados de São Paulo e Rio de Janeiro e integram o Enxame de Diques da Serra do Mar (EDSM). Essas rochas ocorrem sob a forma de diques e intrudem o Orógeno Ribeira, de idade Neoproterozóica/Cambro-Ordoviciana, inserindo-se no contexto geodinâmico de abertura do Oceano Atlântico Sul durante o Cretáceo Superior. Essas intrusões são subverticais e orientam-se preferencialmente a NE-SW, seguindo a estruturação das rochas encaixantes. Os lamprófiros são classificados como monchiquitos e camptonitos e exibem, respectivamente, textura hipocristalina e holocristalina. Apresentam também textura panidiomórfica, fenocristais de clinopiroxênio e olivina, imersos em matriz formada essencialmente por esses mesmos minerais, além de biotita, kaersutita e minerais opacos. O camptonito apresenta ainda plagioclásio na matriz. Os diabásios alcalinos são hipocristalinos a holocristalinos, equigranulares a inequigranulares, com fenocristais de olivina e/ou clinopiroxênio e/ou plagioclásio, em uma matriz composta essencialmente por esses minerais. As rochas estudadas caracterizam séries alcalinas miaskíticas, com os lamprófiros sendo tanto sódicos, potássicos e ultrapotássicos e os diabásios alcalinos como predominantemente sódicos. Modelagens petrogenéticas envolvendo possíveis processos evolutivos mostram que é improvável que os lamprófiros sejam cogenéticos por processos evolutivos envolvendo tanto cristalização fracionada, com ou sem assimilação concomitante, quanto hibridização. O mesmo ocorre para os diabásios alcalinos. A discriminação de fontes mantélicas foi feita com base nos teores de elementos traços de amostras representativas de líquidos parentais e indica que esse magmatismo alcalino está relacionado a fontes lherzolíticas com fusão parcial na zona de estabilidade do espinélio, isto é, a poucas profundidades. Os dados litogeoquímicos e isotópicos do sistema Sr-Nd das rochas estudadas sugerem tanto o envolvimento de fontes férteis, associadas ao manto sublitosférico, quanto de fontes enriquecidas, relacionadas ao manto litosférico subcontinental. Modelagens de mistura binária revelam que a petrogênese dos lamprófiros e diabásios alcalinos envolveu uma grande participação de um componente fértil misturado com contribuições menores de um componente enriquecido. Idades TDM (760-557 Ma) obtidas sugerem remobilização do manto litosférico no Neoproterozóico, talvez relacionadas à subducção da Placa São Francisco preteritamente à colisão do Orógeno Ribeira. Altas razões CaO/Al2O3 para os líquidos lamprofíricos menos evoluídos, altos teores de Zr, correlações negativas Zr/Hf e Ti/Eu e associação com carbonatitos indicam condições metassomáticas de alto CO2/H2O. Em escala local, modelos geodinâmicos baseados na astenosfera não isotérmica parecem mais aplicáveis. No entanto, modelos geodinâmicos baseados na astenosfera isotérmica (com o envolvimento de plumas) parecem mais indicados num contexto regional, considerando-se outras províncias alcalinas contemporâneas e correlatas. / Alkaline lamprophyres and alkaline diabases of the Serra do Mar Dyke Swarm (SMDS) outcrop along the Southeastern Brazil. These dykes intrude rocks of the so-called Rio Negro Magmatic Arc within the Late Proterozoic-Ordovician Ribeira Orogen and are associated with the opening of South Atlantic Ocean during the Late Cretaceous. Typically, the intrusions are subvertical bearing a NE-SW preferential trend which follows the main lineaments in the area. The lamprophyres are classified as monchiquites and camptonites and show holocrystalline and hypocrystalline textures, respectively. They also have panidiomorphic texture and olivine and clinopyroxene phenocrysts within a matrix composed essentially by these same minerals, kaersutite and biotite. Camptonites still have plagioclase in the matrix. The alkaline diabases are holo- to hypocrystalline, equi- to inequigranular rocks with olivine and/or clinopyroxene and/or plagioclase phenocrysts in a matrix composed essentially by these minerals. These alkaline rocks have miaskitic compositions. Lamprophyres are sodic, potassic and ultrapotassic and alkaline diabases are predominantly sodic. Petrogenetic modeling indicates that lamprophyres are unlikely to be cogenetic by evolutionary processes involving either fractional crystallization, with or without concomitant assimilation, or hybridization. The same applies to the alkaline diabases. Modal-batch partial melting models using samples representing parental liquids indicate that these alkalines mafic rocks are related to lherzolitic sources and that partial melting occurred in the spinel stability field, pointing to a thin continental lithosphere in the region. Lithogeochemical and Sr-Nd isotopic data show that the petrogenesis of these alkaline rocks can be assigned to mixing of mantle sources. Binary mixing models and assimilation tests reveal that the petrogenesis of the lamprophyres and alkaline diabases involve a large amount of participation of a fertile component with small contribution of an enriched component. TDM model ages for the studied rocks suggest remobilization ages of the of the lithospheric mantle during the Neoproterozoic, possibly related to the subduction of the San Francisco plate prior to the collision of the Ribeira Orogen. The high CaO/Al2O3 ratios of less evolved lamprophyric melts, high Zr contents, Zr/Hf and Ti/Eu negative correlations and association with carbonatites point to high CO2/H2O conditions during metassomatism of the subcontinental lithospheric mantle. Geodynamic models based on the non-isothermal asthenospheric mantle seem to apply to the studied mafic alkaline magmatism on a local scale although the isothermal asthenospheric mantle model appears to conceal the petrogenesis of other coeval alkaline provinces in central and southeastern Brazil.

Conselho Nacional de Desenvolvimento Científico e Tecnológico / Lamprófiros e diabásios alcalinos afloram no litoral dos estados de São Paulo e Rio de Janeiro e integram o Enxame de Diques da Serra do Mar (EDSM). Essas rochas ocorrem sob a forma de diques e intrudem o Orógeno Ribeira, de idade Neoproterozóica/Cambro-Ordoviciana, inserindo-se no contexto geodinâmico de abertura do Oceano Atlântico Sul durante o Cretáceo Superior. Essas intrusões são subverticais e orientam-se preferencialmente a NE-SW, seguindo a estruturação das rochas encaixantes. Os lamprófiros são classificados como monchiquitos e camptonitos e exibem, respectivamente, textura hipocristalina e holocristalina. Apresentam também textura panidiomórfica, fenocristais de clinopiroxênio e olivina, imersos em matriz formada essencialmente por esses mesmos minerais, além de biotita, kaersutita e minerais opacos. O camptonito apresenta ainda plagioclásio na matriz. Os diabásios alcalinos são hipocristalinos a holocristalinos, equigranulares a inequigranulares, com fenocristais de olivina e/ou clinopiroxênio e/ou plagioclásio, em uma matriz composta essencialmente por esses minerais. As rochas estudadas caracterizam séries alcalinas miaskíticas, com os lamprófiros sendo tanto sódicos, potássicos e ultrapotássicos e os diabásios alcalinos como predominantemente sódicos. Modelagens petrogenéticas envolvendo possíveis processos evolutivos mostram que é improvável que os lamprófiros sejam cogenéticos por processos evolutivos envolvendo tanto cristalização fracionada, com ou sem assimilação concomitante, quanto hibridização. O mesmo ocorre para os diabásios alcalinos. A discriminação de fontes mantélicas foi feita com base nos teores de elementos traços de amostras representativas de líquidos parentais e indica que esse magmatismo alcalino está relacionado a fontes lherzolíticas com fusão parcial na zona de estabilidade do espinélio, isto é, a poucas profundidades. Os dados litogeoquímicos e isotópicos do sistema Sr-Nd das rochas estudadas sugerem tanto o envolvimento de fontes férteis, associadas ao manto sublitosférico, quanto de fontes enriquecidas, relacionadas ao manto litosférico subcontinental. Modelagens de mistura binária revelam que a petrogênese dos lamprófiros e diabásios alcalinos envolveu uma grande participação de um componente fértil misturado com contribuições menores de um componente enriquecido. Idades TDM (760-557 Ma) obtidas sugerem remobilização do manto litosférico no Neoproterozóico, talvez relacionadas à subducção da Placa São Francisco preteritamente à colisão do Orógeno Ribeira. Altas razões CaO/Al2O3 para os líquidos lamprofíricos menos evoluídos, altos teores de Zr, correlações negativas Zr/Hf e Ti/Eu e associação com carbonatitos indicam condições metassomáticas de alto CO2/H2O. Em escala local, modelos geodinâmicos baseados na astenosfera não isotérmica parecem mais aplicáveis. No entanto, modelos geodinâmicos baseados na astenosfera isotérmica (com o envolvimento de plumas) parecem mais indicados num contexto regional, considerando-se outras províncias alcalinas contemporâneas e correlatas. / Alkaline lamprophyres and alkaline diabases of the Serra do Mar Dyke Swarm (SMDS) outcrop along the Southeastern Brazil. These dykes intrude rocks of the so-called Rio Negro Magmatic Arc within the Late Proterozoic-Ordovician Ribeira Orogen and are associated with the opening of South Atlantic Ocean during the Late Cretaceous. Typically, the intrusions are subvertical bearing a NE-SW preferential trend which follows the main lineaments in the area. The lamprophyres are classified as monchiquites and camptonites and show holocrystalline and hypocrystalline textures, respectively. They also have panidiomorphic texture and olivine and clinopyroxene phenocrysts within a matrix composed essentially by these same minerals, kaersutite and biotite. Camptonites still have plagioclase in the matrix. The alkaline diabases are holo- to hypocrystalline, equi- to inequigranular rocks with olivine and/or clinopyroxene and/or plagioclase phenocrysts in a matrix composed essentially by these minerals. These alkaline rocks have miaskitic compositions. Lamprophyres are sodic, potassic and ultrapotassic and alkaline diabases are predominantly sodic. Petrogenetic modeling indicates that lamprophyres are unlikely to be cogenetic by evolutionary processes involving either fractional crystallization, with or without concomitant assimilation, or hybridization. The same applies to the alkaline diabases. Modal-batch partial melting models using samples representing parental liquids indicate that these alkalines mafic rocks are related to lherzolitic sources and that partial melting occurred in the spinel stability field, pointing to a thin continental lithosphere in the region. Lithogeochemical and Sr-Nd isotopic data show that the petrogenesis of these alkaline rocks can be assigned to mixing of mantle sources. Binary mixing models and assimilation tests reveal that the petrogenesis of the lamprophyres and alkaline diabases involve a large amount of participation of a fertile component with small contribution of an enriched component. TDM model ages for the studied rocks suggest remobilization ages of the of the lithospheric mantle during the Neoproterozoic, possibly related to the subduction of the San Francisco plate prior to the collision of the Ribeira Orogen. The high CaO/Al2O3 ratios of less evolved lamprophyric melts, high Zr contents, Zr/Hf and Ti/Eu negative correlations and association with carbonatites point to high CO2/H2O conditions during metassomatism of the subcontinental lithospheric mantle. Geodynamic models based on the non-isothermal asthenospheric mantle seem to apply to the studied mafic alkaline magmatism on a local scale although the isothermal asthenospheric mantle model appears to conceal the petrogenesis of other coeval alkaline provinces in central and southeastern Brazil.

<p> A petrological and geochemical study has been carried out on some Archean mafic and felsic volcans of Dome Township, Central Red Lake area, Ontario. Included are a discussion on petrographic descriptions along with chemical investigations of the rocks and a discussion concerning the general problem of petrogenesis. Analytical methods used are explained, and di scussions of the results are included. </p> / Thesis / Bachelor of Arts (BA)