1000 resultados para 260301 Geochronology and Isotope Geochemistry
Resumo:
Results of studies of mineralogy, geochemistry, and isotope parameters (d13C, d34S, d180, and 87Sr/86Sr) of carbonates and barites from sediments of the Deryugin Basin in the Sea of Okhotsk are presented. Diagenetic nature of carbonates and barites formed due to prolonged activity of cold seeps acting along a fracture zone and supplying methane- and barium saturated fluids is determined. Any signs for hydrothermal activity were not observed.
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Identifying terrigenous sources in deep-sea sediments may reveal temporal trends in paleocirculation and the relative role of eolian, upwelled, and hemipelagic Fe sources to surface waters. Bulk elemental and isotopic geochemistry of deep-sea sediments recovered during Ocean Drilling Program Leg 177 in the southeastern Atlantic sector of the Southern Ocean reveal several important aspects of paleocirculation and terrigenous provenance. The sites studied span 43°-53°S and represent different oceanographic settings relative to regional hydrography and sediment type. Bulk sediment geochemistry indicates that terrigenous provenance varied over the past 600 k.y. Site 1089, the northernmost site, exhibits clear glacial-interglacial variability in provenance, while provenance appears to vary regardless of climate state at the more southerly sites (Site 1093 and 1094). Nd and Sr isotopes and Sm/Nd ratios of the terrigenous fraction indicate that study sites have geochemically distinguishable provenance. Nd and Sr isotopes further suggest that Sites 1089 and 1094 both contain detrital components that originated in South America over the past 30 k.y.; however, Site 1089 is also influenced by southern African sources and the strength of the Agulhas Current. The e-Nd data support a more hemipelagic source for the terrigenous material rather than an eolian source based on comparisons with Antarctic ice core data and known sea-ice extent.
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As a result of their relative concentration towards the respective Atlantic margins, the silicic eruptives of the Parana (Brazil)-Etendeka large igneous province are disproportionately abundant in the Etendeka of Namibia. The NW Etendeka silicic units, dated at similar to132 Ma, occupy the upper stratigraphic levels of the volcanic sequences, restricted to the coastal zone, and comprise three latites and five quartz latites (QL). The large-volume Fria QL is the only low-Ti type. Its trace element and isotopic signatures indicate massive crustal input. The remaining NW Etendeka silicic units are enigmatic high-Ti types, geochemically different from low-Ti types. They exhibit chemical affinities with the temporally overlapping Khumib high-Ti basalt (see Ewart et al. Part 1) and high crystallization temperatures (greater than or equal to980 to 1120degreesC) inferred from augite and pigeonite phenocrysts, both consistent with their evolution from a mafic source. Geochemically, the high-Ti units define three groups, thought genetically related. We test whether these represent independent liquid lines of descent from a common high-Ti mafic parent. Although the recognition of latites reduces the apparent silica gap, difficulty is encountered in fractional crystallization models by the large volumes of two QL units. Numerical modelling does, however, support large-scale open-system fractional crystallization, assimilation of silicic to basaltic materials, and magma mixing, but cannot entirely exclude partial melting processes within the temporally active extensional environment. The fractional crystallization and mixing signatures add to the complexity of these enigmatic and controversial silicic magmas. The existence, however, of temporally and spatially overlapping high-Ti basalts is, in our view, not coincidental and the high-Ti character of the silicic magmas ultimately reflects a mantle signature.
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40Ar/39Ar geochronology of muscovite and biotite grains genetically related to gold and Be–Ta–Li pegmatites from the Seridó Belt (Borborema province, NE Brazil) yield well-defined, reliable plateau ages. This information, combined with data about paragenetic and field relationships, reveals Cambro-Ordovician mineralization ages (520 and 500–506 Ma) for the orogenic gold deposits in the Seridó Belt. Biotite ages of 525±2 Ma, which represent the mean weighted results of the incremental heating analysis of six biotite single crystals, record the time of pegmatite emplacement and reactivation of Brasiliano/Pan-African strike-slip shear zones. These results, along with previous structural evolution studies, suggest that shear zones formed during the Brasiliano/Pan-African event were reactivated in the Upper Cambrian–Lower Ordovician. Mineralization occurs late in the history of the orogen.
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Ar-40/Ar-39 incremental heating ages for twenty one grains of cryptomelane, collected at 0, 42, 45, and 60 in depths in the Cachoeira Mine weathering profile, Minas Gerais, permit calculating long-term (10 Ma time scale) weathering rate (saprolitization rate) in SE Brazil. Pure well-crystallized cryptomelane grains with high K contents (3-5 wt.%) yield reliable geochronological results. The Ar-40/Ar-39 plateau ages obtained decrease from the top to the bottom of the profile (12.7 +/- 0.1 to 7.6 +/- 0.1 Ma at surface; 7.6 +/- 0.2 to 6.1 +/- 0.2 Ma at 42 m; and 7.1 +/- 0.2 to 5.9 +/- 0.1 Ma at 45 in; 6.6 +/- 0.1 to 5.2 +/- 0.1 Ma at 60 in), yielding a weathering front propagation rate of 8.9 +/- 1.1 m/m.y. From the geochronological results and the mineral transformations implicit by the current mineralogy in the weathering profiles, it is possible to calculate the saprolitization rate for the Cachoeira Mine lithologies and for adjacent weathering profiles developed on granodiorites and scbists. The measured weathering front propagation rate yields a saprolitization rate of 24.9 +/- 3.1 t/km(2)/yr. This average long-term (> 10 Ma) saprolitization rate is consistent with mass balance calculations results for present saprolitization rates in weathering watersheds. These results are also consistent with longterm saprolitization rates estimated by combining cosmogenic isotope denudation rates with mass balance calculations. (c) 2005 Elsevier B.V All rights reserved.
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This study presents the first attempt to constrain the evolution of the North Anatolian Fault Zone (NAFZ) by age dating and isotope tracing of clay minerals formed during near-surface faulting. Extensive illitic clay mineralisation occurred along the NAFZ related to hydrothermal alteration of the fault gouges and pseudotachylytes. Samples representing the pre-fault protoliths outside the fault zone do not contain authigenic illitic clay minerals indicating that hydrothermal processes were confined to the areas within the fault zone. K-Ar age data indicate that the hydrothermal system and the associated illite authigenesis initiated at similar to 57 Ma. This process is interpreted to reflect the onset of significant strike-slip or transtensional faulting immediately after the continental collision related to the closure of the Neotethys Ocean. Following the initiation of the fault movements in the latest Paleocene-Early Eocene, displacements along the NAFZ have continued, with probably intensified fault activities at similar to 26 Ma and later than similar to 8 Ma. Oxygen isotope compositions of the illitic clays from different locations along the NAFZ are similar, with narrow ranges in delta O-18 values indicating clay precipitation from fluids with similar oxygen isotope compositions and crystallisation temperatures. The delta O-18 and delta D values of the calculated fluid isotopic composition (delta O-18=5.9 parts per thousand to 11.2 parts per thousand, delta D=-59 parts per thousand to -73 parts per thousand) are consistent with metamorphic and magmatic origin of fluids mobilised during active tectonism. The interpretation of the fluid flow history of the NAFZ is in agreement with that reported previously for some well-known large-scale high-angle fault zones, which similarly developed along collisional-type orogenic belts and are commonly associated with significant mesothermal ore mineralisation. (c) 2005 Elsevier B.V. All rights reserved.
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This study concerns the Dublin Gulch intrusion-related gold system, Yukon Territory, Canada. Located 85 km, north northwest of the town of Mayo, YT, the property hosts a 3.3 M oz Au deposit associated with a mid-Cretaceous pluton. A detailed, 8 stage, hydrothermal paragenesis has been constructed for the deposit. At least two discrete fluids are responsible for sulfide mineralization at Dublin Gulch. The latter of the two hydrothermal fluids is responsible for the majority of Au endowment on the property. Geochemical signatures of mineralization support this finding, displaying distinct populations of arsenopyrite compositions and sulfur isotopes for each fluid. Lead isotopes from sulfosalts associated with the second fluid suggest hydrothermal scavenging from country rocks. Geochronology and petrogenetic studies show that a short lived intrusive event c. 93-94 Ma took place at Dublin Gulch and that the main Au mineralising fluid may be linked to a yet unseen intrusion at depth.
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In-situ uplifted portions of oceanic crust at the central dome of the Atlantis Massif (Mid-Atlantic Ridge, 30°N) were drilled during Expeditions 304 and 305 of the Integrated Ocean Drilling Program (IODP) and a 1.4 km section of predominantly gabbroic rocks with minor intercalated ultramafic rocks were recovered. Here we characterize variations in sulfur mineralogy and geochemistry of selected samples of serpentinized peridotites, olivine-rich troctolites and diverse gabbroic rocks recovered from Hole 1309D. These data are used to constrain alteration processes and redox conditions and are compared with the basement rocks of the southern wall of the Atlantis Massif, which hosts the Lost City Hydrothermal Field, 5 km to the south. The oceanic crust at the central dome is characterized by Ni-rich sulfides reflecting reducing conditions and limited seawater circulation. During uplift and exhumation, seawater interaction in gabbroic-dominated domains was limited, as indicated by homogeneous mantle-like sulfur contents and isotope compositions of gabbroic rocks and olivine-rich troctolites. Local variations from mantle compositions are related to magmatic variability or to interaction with seawater-derived fluids channeled along fault zones. The concomitant occurrence of mackinawite in olivine-rich troctolites and an anhydrite vein in a gabbro provide temperature constraints of 150-200 °C for late circulating fluids along local brittle faults below 700 m depth. In contrast, the ultramafic lithologies at the central dome represent domains with higher seawater fluxes and higher degrees of alteration and show distinct changes in sulfur geochemistry. The serpentinites in the upper part of the hole are characterized by high total sulfide contents, high d34Ssulfide values and low d34Ssulfate values, which reflect a multistage history primarily controlled by seawater-gabbro interaction and subsequent serpentinization. The basement rocks at the central dome record lower oxygen fugacities and more limited fluid fluxes compared with the serpentinites and gabbros of the Lost City hydrothermal system. Our studies are consistent with previous results and indicate that sulfur speciation and sulfur isotope compositions of altered oceanic mantle sequences commonly evolve over time. Heterogeneities in sulfur geochemistry reflect the fact that serpentinites are highly sensitive to local variations in fluid fluxes, temperature, oxygen and sulfur fugacities, and microbial activity.
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The Paleo- to Meso-Proterozoic Jabiluka unconformity related uranium mine is located within the Alligator River Uranium Field, found in the Northern Territories, Australia. The uranium ore is hosted in the late middle Paleoproterozoic Cahill Formation, which is unconformably overlain by a group of unmetamorphosed conglomerates known as the Kombolgie subgroup. The Kombolgie subgroup provided the source for oxidized basinal brines, carrying U as the mobile form U(VI), which interacted with reducing lithologies in the Cahill formation, thus reducing U(VI) to the solid U(IV), and leading to the precipitation of uraninite (UO2). In order to characterize fluid interaction with the ore body and compare that to areas without mineralization, several isotopic tracers were studied on a series of clay samples from drill core at Jabiluka as well as in barren areas throughout the ARUF. Among the potential tracers, three were selected: U (redox sensitive and recent fluid mobilization), Fe (redox sensitive), and Li (fractionated by hydrothermal fluids and adsorption reactions). δ238U values were found to be closely linked to the mineralogy, with samples with higher K/Al ratios (indicating high illite and low chlorite concentrations) having higher δ238U values. This demonstrates that 235U preferentially absorbs onto the surface of chlorite during hydrothermal circulation. In addition, δ234U values lie far from secular equilibrium (δ234U of 30‰), indicating there was addition or removal of 234U from the surface of the samples from recent (<2.5Ma) interactions of mobile fluids. δ57Fe values were found to be related to lithology and spatially to known uranium deposits. Decreasing δ57Fe values were found with increasing depth to the unconformity in a drill hole directly above the ore zone, but not in drill holes in the barren area. Similarly to δ238U, δ7Li is found to correlate with mineralogy, with higher δ7Li values associated with samples with more chlorite. In addition, higher δ7Li values are found at greater depth throughout the basin, indicating that the direction of the mineralizing fluid circulation was upwards from the Cahill formation to the Kombolgie subgroup.
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A high-resolution carbon and oxygen isotope analysis of Late Oxfordian-Early Kimmeridgian deep-shelf sediments of southern Germany is combined with investigation of nannofossil assemblage composition and sedimentological interpretations in order to evaluate the impact of regional palaeoenvironmental conditions on isotopic composition of carbonates. This study suggests that carbonate mud was essentially derived from the Jura shallow platform environments and also that the isotopic signature of carbonates deposited in the Swabian Alb deep shelf indirectly expresses the palaeoenvironmental evolution of the platform. Short-term fluctuations in delta(13) C and delta(18)O are probably controlled by changes in salinity (fresh-water input versus evaporation) in platform environments. Long-term fluctuations in carbon and oxygen isotope record throughout the Late Oxfordian-Early Kimmeridgian result from the interplay of increasing temperature and decreasing humidity, which both control the trophic level. Changes from mesotrophic to oligotrophic conditions in platform environments and in the deep-shelf surface waters are inferred. During the Late Oxfordian (Bimammatum Subzone to Planula Zone), the delta(13)C curve displays a positive shift of about 1 parts per thousand, which is comparable in intensity to global perturbations of the carbon cycle. This evident isotopic shift has not been documented yet in other basinal settings. It can be reasonably explained by local palaeoenvironmental changes on the Jura platform (salinity, temperature, and nutrient availability) that controlled platform carbonate production, and the geochemistry of overlying waters. However, increasing carbonate production on the Jura platform and related positive delta(13)C shifts recorded in the Swabian Alb deep shelf are the regional signatures of climatic changes affecting other palaeogeographical domains of Europe in which the carbonate production increased throughout the Late Oxfordian. (C) 2002 Elsevier Science B.V. All rights reserved.
Resumo:
THESIS ABSTRACT : Stable isotope geochemistry is used to help resolve a large number of geological questions. In order to do this, it is essential to understand the different mechanisms that govern isotopic fractionation processes between different phases and to identify the conditions required to reach equilibrium fractionation. However, at low temperatures, these processes are poorly constrained and many factors can induce differential partitioning of the isotopes between sectors of a mineral species and the fluid during mineral growth. This can result in so-called 'sector zoning' of a mineral species. The aim of this thesis is to evaluate the occurrence of sector zoning of the oxygen isotopes and trace elements in natural α-quartz crystals and to identify the reasons for such zoning. The implications for the fluid-mineral interactions are studied in the context of the Alpine metamorphism. The approach chosen has focused on examining the crystal structure, cathodoluminescence appearance (CL), and on relating elemental (e.g. Li, Na, Al, P, K, Ca, Ge, Ti, Fe) to stable oxygen isotope compositions between and along different growth sectors. Low temperature quartz samples were selected from Alpine veins in different localities, where growth conditions have already been well constrained. The mineralogy as well as the isotopic compositions of the host rocks were also investigated, in order to interpret the variations obtained between the different growth stages in the framework of fluid-rock interaction during Alpine metamorphism. Depending on the growth conditions, most of the studied quartz is strongly zoned in CL, and it reveals corresponding zonations in the trace element content (e.g. growth zoning). Aluminium, substituting for Si in the lattice, was found in concentrations up to 1000's ppma, and its distribution is strongly related to Li and H and to a lesser extent, to Ge. Elemental sector zoning is evident from the distribution of these three elements since they exhibit differences in their respective concentrations between faces for distinct growth zones, with prismatic faces having the lowest Al contents. Quartz from veins in magmatic rocks, for example, tend to have lower Al concentrations and similar concentrations of Li and Ti suggesting also a contribution of these elements from the host rock. The relationship between Al and Li is still correlated. Only Alpine crystals grown at higher temperatures (~400°C) without any CL zoning feature are free of these impurities and do not show such zoning characteristics. Differences in the δ18O values were measured between different faces principally in the AIenriched growth zones or stages. These results were confirmed by the means of two different methods (in situ/non in situ). However, it was determined that the Al concentrations do not affect significantly oxygen isotope fractionations at 300°C. The results altogether suggest that the presence of sector zoning in quartz crystals is real, but not universal, and henceforth should be taken into consideration for any use of these systems. The occurrence of disequilibrium partitioning has been enhanced and is possibly related to kinetic processes as well as structural effects that do not affect similarly trace element incorporation and isotopic fractionation. In situ measurements also revealed fine scale δ18O zonations along growth paths that are useful to constrain fluid-rock interactions during Alpine metamorphism. Variations in the δ18O values present along growth vectors indicate changes in the fluid composition and origin. Association with oxygen isotope composition of the host rock allows for the deduction of interactions between rocks, veins and consequently fluids, as well as fluid regimes. RESUME DE LA THESE : A basses températures, (i.e. <400°C) les différents mécanismes qui régissent le fractionnement isotopique ainsi que les conditions nécessaires pour établir un état d'équilibre sont peu connus et nombre de paramètres peuvent entraîner un partitionnement chimique différentiel entre différents secteurs d'un minéral et le fluide en contact. Ainsi, ce travail de thèse a pour but d'évaluer la possible présence de zonages sectoriels en isotopes de l'oxygène mais aussi en éléments traces dans des cristaux naturels de quartz-α de basses températures, ainsi que les raisons d'un tel phénomène et enfin ses implications sur les interactions fluide-roche, principalement dans le cadre du métamorphisme Alpin. La structure et l'apparence en cathodoluminescence (CL) des échantillons ont été caractérisées avant de retracer en détail les compositions en élément traces (Li, Na, Al, P, K, Ca, Ge, Ti, Fe) et en isotopes de l'oxygène, le long et entre différents secteurs. Les échantillons de quartz sélectionnés proviennent majoritairement de veines Alpine de différentes localités, où les conditions de croissance ont été déjà bien caractérisées. Les compositions minéralogiques et isotopiques de la roche encaissante ont aussi été examinées, pour contraindre les variations obtenues dans un contexte Alpin. Selon leurs conditions de croissance, la plupart des cristaux étudiés sont fortement zonés, ce qui est souligné par un zonage des concentrations en éléments traces (e.g. zonage de croissance). L'Aluminium, qui peut se substituer à la Silice dans le réseau cristallin, a été retrouvé jusqu'en très grandes concentrations dans certaines zones (plusieurs milliers de ppma). De plus, la distribution en Al est fortement liée à celles de Li et H, ainsi que dans une moindre mesure à Ge. La présence de zonage sectoriel est évidente au niveau de ces éléments qui montrent de larges différences de concentrations entre différentes faces pour une même zone de croissance, avec les concentrations les plus basses retrouvées dans les faces prismatiques. Les quartz de veines situées dans des roches magmatiques par exemple possèdent des concentrations en Li et Ti de même ordre de grandeur, confirmant le rôle de la composition de la roche encaissante. La relation Li/Al est toujours fortement présente, mais ce rapport est fonction de la face mesurée. Seuls les cristaux Alpins de plus hautes températures (400°C) ne possédant pas de zones en CL ne présentent aucune de ces caractéristiques. Des différences dans les valeurs de δ18O de zones identiques enrichies en Al ont clairement été mesurées entre les différentes faces r, z, et m, mais aussi au sein d'une même seule zone, indiquant que le fractionnement a probablement eu lieu en déséquilibre. Il a été déterminé que la présence d'Al dans ces teneurs n'avait qu'un faible effet sur le fractionnement isotopique de l'oxygène. L'utilisation de deux méthodes différentes a permis d'obtenir des résultats in situ et non in situ concordants. La comparaison des résultats obtenus permet de démontrer que le zonage sectoriel est bien présent dans certains cristaux de quartz, et dépend des conditions de formation. La présence d'un partitionnement différentiel des éléments traces peut être due à des effets cinétiques aussi bien que structuraux, alors que le zonage sectoriel des isotopes de l'oxygène aurait d'autres origines. Il est alors évident que la possibilité de zonage sectoriel doit être désormais pris en considération avant toute interprétations de données isotopiques de cristaux zonés. Les mesures in situ ont de plus permis de distinguer de fines variations des valeurs δ18O au cours de la croissance, qui peuvent aider à retracer la circulations des fluides dans les Alpes durant cette période. En association avec les compositions des roches encaissantes, ii est possible de déduire les interactions entre roches, veines, et par conséquent fluides, au cours de différentes étapes. RESUME GRAND PUBLIC : La géochimie des isotopes stables a pris beaucoup d'importance depuis ces dernières années pour aider à résoudre nombre de questions géologiques, en se basant sur les caractéristiques du fractionnement isotopiques pour différents systèmes. Il est donc nécessaire d'avoir une connaissance approfondie des mécanismes qui s'appliquent au fractionnement isotopique entre les minéraux et les fluides à partir desquels ils se forment. Ces mécanismes ont été bien approchés par différents types de calibrations pour des systèmes à hautes températures, cependant cela n'est pas aussi évident pour les systèmes à des températures inférieures à 400-500°C. Ce travail de thèse a pour but d'aider à la description et la compréhension des phénomènes qui peuvent affecter le fractionnement isotopique à basses températures, ainsi que leurs implications, à partir de l'étude de cristaux de quartz. Le choix des échantillons s'est porté sur des cristaux naturels formés à des températures inférieures ou égales à 400°C, provenant majoritairement de fissures hydrothermales Alpines dont les conditions de formation ont déjà été déterminées. L'étude des cristaux Alpin permet de plus de replacer les résultats obtenus dans le contexte du métamorphisme Alpin au cours du Miocène (21-13 Ma). Après examen de la structure et de la morphologie des cristaux, et leur caractérisation par cathodoluminescence (CL), des analyses chimiques détaillées sur les éléments en traces pouvant entrer dans le réseau cristallin du quartz comme impuretés (i.e. Li, Na, Al, P, K, Ca, Ge, Ti), et des isotopes stables de l'oxygène, ont été menées. En fonction des conditions de croissance, la plupart des cristaux présentent des zonations, qui peuvent être facilement reliées à la distribution des éléments traces analysés par microsonde électronique, sonde ionique (SIMS) et LA-ICPMS. De fortes concentrations d'Aluminium (plusieurs milliers de parties par million atomique) ont pu être observées dans les zones les plus externes des cristaux. De plus, les concentrations en Al et en Li sont toujours corrélées; la présence d'Hydrogène déduite à partir d'analyses par FTIR suit cette même tendance. Les différentes faces des cristaux présentent des concentrations distinctes d'Al, Li et H pour des mêmes zones de croissance, avec par exemple les concentrations les plus faibles dans les zones des faces prismatiques. Cela implique la présence d'un zonage sectoriel, qui a déjà été observé principalement dans des carbonates mais jamais décrit auparavant pour des quartz. Seuls les cristaux alpins homogènes en CL dont la croissance s'est faite à plus haute température (400°C) ne présentent aucune de ces caractéristiques. Par analogie avec le zonage sectoriel en Al, élément qui se substitue au Si dans le réseau cristallin du quartz, il est possible de penser qu'un zonage sectoriel pourrait aussi s'appliquer aux isotopes de l'oxygène. Des précédentes études avaient en effet émis cette hypothèse. Nos résultats ont été obtenus à partir d'analyses à la fois in- situ par SIMS, et par extraction assistée par laser-CO2 sur des parties de quartz soigneusement séparées, et sont en accord entre les deux méthodes. Un zonage sectoriel est en effet bien présent pour les cristaux alpins, mais principalement au niveau des zones très riches en Aluminium. Cependant, il a été déterminé que la présence d'Al dans ces teneurs avait un effet plus que minimal sur le fractionnement isotopique de l'oxygène. Des différences importantes ont été observées entre les faces r & z mais aussi au sein d'une même et seule zone, indiquant que le fractionnement a pu avoir lieu en déséquilibre, ce qui est aussi visible au niveau des valeurs totalement opposées entre faces pour la dernière phase de croissance de certains cristaux. Ainsi l'association de ces résultats laisse suggérer que la présence d'un zonage sectoriel peut être liée à différents paramètres tels que le taux de croissance ou la structure de surface du cristal, mais qui n'affectent pas de la même façon l'incorporation des éléments traces et le fractionnement isotopique. La possibilité d'un zonage sectoriel est importante à prendre en compte lors de toute interprétation de données isotopiques. Les analyses des isotopes de l'oxygène effectuées par SIMS ont aussi permis de distinguer des variations importantes à petite échelle au cours de la croissance. Des mesures faites par laser CO2 sur certaines roches encaissantes, ont permis distinguer plusieurs étapes dans la croissance des minéraux et de déduire le rôle de l'encaissant et le type de fluide. En association avec de précédentes études, il a été ainsi possible de mieux contraindre la formation de ces cristaux dans le contexte alpin et la circulation de fluide au cours du métamorphisme alpin durant le Miocène.
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The Adula nappe belongs to the Lower Penni- nic domain of the Central Swiss Alps. It consists mostly of pre-Triassic basement lithologies occurring as strongly folded and sheared gneisses of various types with mafic boudins. We propose a new lithostratigraphy for the northern Adula nappe basement that is supported by detailed field investigations, U-Pb zircon geochronology, and whole-rock geochemistry. The following units have been identified: Cambrian clastic metasediments with abundant carbonate lenses and minor bimodal magmatism (Salahorn Formation); Ordovician metapelites associated with amphibolite boudins with abundant eclogite relicts representing oceanic metabasalts (Trescolmen Formation); Ordovician peraluminous metagranites of calc-alkaline affinity ascribed to subduction-related magmatism (Ga- renstock Augengneiss); Ordovician metamorphic volcanic- sedimentary deposits (Heinisch Stafel Formation); Early Permian post-collisional granites recording only Alpine orogenic events (Zervreila orthogneiss). All basement lithologies except the Permian granites record a Vari- scan ? Alpine polyorogenic metamorphic history. They document a complex Paleozoic geotectonic evolution consistent with the broader picture given by the pre- Mesozoic basement framework in the Alps. The internal consistency of the Adula basement lithologies and the stratigraphic coherence of the overlying Triassic sediments suggest that most tectonic contacts within the Adula nappe are pre-Alpine in age. Consequently, me ́lange models for the Tertiary emplacement of the Adula nappe are not consistent and must be rejected. The present-day structural complexity of the Adula nappe is the result of the intense Alpine ductile deformation of a pre-structured entity.
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The present research is aimed at studying the charnockites and associated rocks of the Madurai Granulite Block (MGB), especially in terms of their field settings, texture, mineralogy, and mineral chemistry analyzing their petrogenesis with the help of thermobarometrical studies and geochronological constraints. The mechanism of charnockitization by the influx of CO2 rich fluids and its relation to the graphite mineralization is actually a matter of discussion and study. The objectives of the present study are, to delineate petrological and structural relationship of charnockites and associated gneissic rocks, to study the field and petrogenetic aspects of graphite mineralization in the MGB, to establish and re-evaluate the P-T conditions of formation of the rocks with the aid of thermbarometric computations and to compare with the earlier studies, characterization of graphite with XRD, Raman spectroscopy and isotope studies together with a search in to its genesis and its relation to the high-grade metamorphism of the terrain, to evaluate the role of CO2 bearing fluids in the processes of charnockitization as well as in the genesis of graphite within the high-grade terrain and to delineate the metamorphic geochronology of selected rocks using ‘monazite dating’ technique with EPMA.
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The Kerala region which forms a significant segment of the south—western Indian shield, dominantly comprises charnockites, khondalites and migmatitic gneisses of Precambrian age. Recent investigations have revealed the occurrences of a number of younger granite and syenite plutons in this region, .spatially related to regional fault—lineaments. The granite of Ambalavayal in Wynad district of northern Kerala is a typical member of this suite of intrusives. The thesis is based on a comprehensive study in terms of geology, petrology, geochemistry and petrogenesis of the Ambalavayal granite, basement gneisses, associated pegmatites, quartz veins and related mineralization that together cover an area of about 90 sq km in wynad district of northern Kerala