Dissertations / Theses on the topic 'Neoarchean'

The Neoarchean was a time of enhanced continental crust formation and wide-spread mafic magmatism related to global mantle melting. Mafic and ultramafic intrusions were emplaced across a large portion of the Ungava craton of the Northeast Superior Province, synchronous with the crystallization of large volumes of ca. 2.74-2.70 Ga intermediate to felsic plutonic rocks. The ca. 2.72-2.70 Ga mafic/ultramafic intrusions are locally known as the Qullinaaraaluk, Chateguay and Couture plutonic suites, and are herein referred to as the Q-suite. The Q-suite plutons have relatively unfractionated MREE/HREE ratios, variably elevated LREE/MREE ratios and strong depletions in HFSE, in particular Nb and Ta. The high Th/Yb ratios and chondritic to strongly radiogenic initial 143Nd/144Nd (2.72 Ga) ratios of the Q-suite intrusions suggest that their "calc-alkaline" trace element profiles may reflect the addition of significant tonalite-trondhjemite-granodiorite (TTG) component. The interaction between the Q-suite magmas and TTG crust is also evident in "hybrid" domains of intermediate-SiO2 content (50-65 wt. %) that form along the margins of some intrusions. These "hybrid" domains strongly resemble the intermediate-SiO2 members of the voluminous ca. 2.74-2.70 Ga pyroxene-bearing granitoids that make up more than 20% of the exposed surface of the Ungava craton. Mass-balance and thermodynamic modelling suggests that pyroxene-bearing granitoids with ~65 wt. % SiO2 contain a significant juvenile (Q-suite) component modified by 40-50 % addition of trondhjemitic melt of the pre 2.74 Ga TTG crust.Analyses of olivine (FoMax ≤ 0.84) from peridotitic and dunitic cores of the Q-suite intrusions (Mg-number≤ 0.82), suggest that their parental magmas were enriched in Fe relative to present-day MORB, or hot-spot related magmas. The Q-suite intrusions of western and southern Ungava craton crystallized from magmas of subalkaline affinity, in contrast to the intrusions of the north-central Ungava craton which are mildly subalkaline to mildly alkaline (transitional). Parental liquid compositions of the subalkaline and transitional Q-suite intrusions estimated using the program alphaMELTS are Fe-rich high-Mg basalts (MgO = 10 wt. %, FeOTOT = 13.5 wt.%, Al2O3 = 15 wt.% ), and Al-poor ferropicrites (MgO ~14 wt. %, FeOTOT = 17 wt.%, Al2O3 = 6.6 wt.%), respectively. These compositional differences may reflect melting of compositionally heterogeneous Fe-rich mantle sources under similar P-T conditions, or different degrees of melting of a common Fe-rich mantle source under different P-T conditions. The transitional parental magmas appear to represent high degree melts that last equilibrated with a harzburgitic residue, whereas the subalkaline parental magmas appear to represent lesser-degree partial melts that last equilibrated with a lherzolitic mantle residue. The craton-wide distribution of Q-suite plutons and the large inferred Q-suite component in the ca. 2.74-2.70 Ga pyroxene-granitoids, suggests that ferropicritic underplating may have been a significant driving force in the reworking of the Ungava craton. Ferropicrites of similar age have also been emplaced into the southern and western Superior Province, as well as the Slave, W. Churchill, Kaapvaal, Yilgarn and Karelia cratons. The identification of ferropicritic rocks in at least five other Archean cratons suggests that melting of Fe-rich mantle domains may have had an important role in global cratonization ca. 2.7 Ga.
Le Néoarchéen est caractérisé par un magmatisme mafique répandu relié à la fusion partielle du manteau à l'échelle globale et par une période intense de formation de croûte continentale. Des intrusions mafiques et ultramafiques sont mises en place dans l'ensemble du craton de l'Ungava, dans le secteur nord-est de la Province du Supérieur, simultanément à la cristallisation de grand volume de roches plutoniques de composition intermédiaire et felsique datées de ~2,72-2,70 Ga. Les intrusions mafiques et ultramafiques de ~2,72-2,70 Ga incluant les suites plutoniques Quillinaaraaluk, Chateguay et Couture forment une suite plutonique nommée ici la « suite-Q ». Les ratios Th/Yb sont élevés et les ratios initiaux de 143Nd/144Nd de la suite-Q sont chondritiques à fortement radiogéniques, ce qui suggèrent que leurs signatures en éléments traces typiques des roches calco-alcalines reflètent l'addition d'un volume important de roches de type TTG. L'interaction entre les magmas de la suite-Q et la croûte composée de TTGs s'observe également le long des marges de certaines intrusions, marges qui sont caractérisées par des concentrations en SiO2 plus élevées et représentent des zones compositionnelles hybrides. Ces marges hybrides sont semblables aux unités à composition intermédiaire en SiO2 appartenant aux granitoïdes à pyroxènes (~2,74- 2,70 Ga) qui représentent plus de 20% de la surface exposée du craton de l'Ungava. Des calculs indiquent que les granitoïdes à pyroxènes avec 65% poids de SiO2 contiennent une composante juvénile significative (suite-Q) modifiée par l'addition de 40-50 % d'un liquide trondhjémitique dérivé de la fusion partielle de la croûte de type TTG mise en place avant 2,74 Ga.Les analyses d'olivine des coeurs péridotitiques et dunitiques des intrusions de la suite-Q suggèrent que leurs magmas parents étaient enrichis en fer par rapport aux MORB ou aux magmas de points chauds modernes. Les intrusions de la suite-Q situées dans le secteur ouest et sud du craton de l'Ungava ont cristallisé à partir de magmas à affinité sub-alcaline contrairement à celles du centre-nord qui sont de compositions modérément sub-alcalines à légèrement alcalines (transitionnelles). Les liquides parentaux des intrusions sub-alcalines et transitionnelles de la suite-Q, modélisés à l'aide du logiciel alphaMELTS, sont des liquides basaltiques riches en fer et en magnésium et des liquides ferropicritiques pauvres en aluminium respectivement. Les différences compositionnelles peuvent être attribuées à la fusion de sources mantelliques riches en fer, à composition hétérogène, sous des conditions de pression et de température similaires, ou à différents degrés de fusion d'une source mantellique commune, riche en fer, sous des conditions de pression et de température différentes. Les magmas parents transitionnels semblent avoir été produits par des degrés de fusion partielle élevés et auraient par la suite été équilibrés avec un résidu harzburgitique du manteau. Au contraire, les magmas parents sub-alcalins pourraient représenter des magmas issus de degrés de fusion partielle plus faibles suivis de l'équilibrage de ces magmas avec un résidu lherzolitique du manteau.La grande distribution des plutons de la suite-Q dans le craton de l'Ungava et l'importante contribution d'une composante de la suite-Q dans les granitoïdes à pyroxènes âgés de ~2,74-2,70 Ga indiquent que l'accrétion par sous-placage de ferropicrite aurait joué un rôle moteur significatif dans le remaniement du craton. Des ferropicrites d'âges similaires ont également été mises en place dans le sud et l'ouest de la Province du Supérieur, ainsi que dans les cratons Slave, Churchill Ouest, Kaapvaal, Yilgarn et Karelia. L'identification de roches ferropicritiques dans au moins cinq autres cratons Archéens suggère que la fusion partielle de domaines mantelliques riches en fer aurait joué un rôle primordial dans la « cratonisation » globale à ~2,7 Ga.

The boundary between the western and central domains of the Wabigoon subprovince has been considered to represent a ca. 2.7 Ga suture between juvenile Neoarchean volcanic rocks in the west and granitoid rocks with Mesoarchean ancestry in the central Wabigoon. The nature and timing of interaction between these two terranes was examined southeast of the Sturgeon Lake greenstone belt within the central Wabigoon, where amphibolite-facies supracrustal remnants are dismembered by Neoarchean plutonic rocks and shear zones. Of the 4 preserved ductile deformation fabrics, D1 and D2 are bracketed by a 2718 +/- 7 Ma tonalite gneiss and crosscutting 2715 Ma tonalite dyke. The main penetrative S3 foliation affects most units, including quartz-rich sandstone deposited after 2701 Ma. A 2697 Ma granodiorite dyke cutting S3 in mafic and metasedimentary rocks provides a lower bracket on D3. Regional implications can be drawn from the observation of 2725--2715 Ma D1 and D2 deformation events in the central Wabigoon. These constraints overlap with an early deformation event in the Pipestone Lake area of the western Wabigoon (2727--2712 Ma; Edwards and Stauffer, 1999). (Abstract shortened by UMI.)

Algoma-type banded iron formation is common in Neoarchean greenstone belts, and many of its distinctive features such as the banding of iron-rich and silica-rich material and deposition in volcanic terranes have been ascribed to their deposition related to volcanic-hydrothermal activity and cyclic variability in depositional pathways. The work presented in this thesis tests these assumptions and presents a model for the deposition and post-depositional processes now represented by the petrography and geochemistry of a 2.73 Ga type-locality of Algoma-type BIF in Temagami, ON. Adsorption of components onto the surface of Fe-oxyhydroxides forming in the anoxic Neoarchean water column is the most likely process capable of transferring silica, as well as trace quantities of transition metals, rare earth elements, Ge, P, U and other components to the sediment. The petrogenesis of the Temagami BIF lithologies suggests ongoing recrystallization processes and volume loss reactions leading to the formation of magnetite layers, while jasper is identified as the most pristine lithology best representative of the initially deposited Fe-oxyhydroxide-silica gel. Recrystallization and volume loss reactions are controlled by the ongoing dewatering during compaction and diagenesis, without the influence of external hydrothermal or metamorphic fluids. When corrected for the volume loss and small amounts of clastic contamination, little residual variability can be observed in the composition of jasper and magnetite layers, indicative of an originally homogenous primary precipitate instead of sorted and layered material deposited on the seafloor. This model is in stark contrast to previous interpretations of seasonal variability in biologic activity, cyclical seasonal or hydrothermal events responsible for primary layering in BIF. Instead, very little direct input of hydrothermal components is recorded in the chemistry of the Temagami BIF, and elements abundant in high-temperature hydrothermal fluids such as sulfur are instead sourced from atmospheric sources and deposited by bacterial pathways. Lack of primary chemical variability and non-hydrothermally sourced components captured in BIF argue against a genetic link to local hydrothermal venting, but rather an open ocean depositional setting. As such, the Temagami BIF does not represent a marker horizon related to local or regional hydrothermal venting and potential formation of associated massive sulfide deposits but reflects processes and the chemistry of the open Neoarchean ocean.

The North Caribou Terrane forms the core of Superior Province and records a protracted history of crustal growth and modification. At the centre of the North Caribou Terrane, lies the North Caribou greenstone belt, which is surrounded by granitoids of diverse compositions and ages. This study reports whole-rock geochemistry, zircon and titanite geochronology, and hornblende geobarometry on these plutonic rocks. Although zircons as old as 3132 ± 7 Ma were found, the main magmatic pulse occurred between 2880 and 2830 Ma, and geobarometry indicates tectonic thickening during this period. This was followed by widespread hydrothermal alteration and limited magmatism from 2760 to 2680 Ma, and shallow, brittle-ductile intrusions at circa 2630 Ma. From 2730 to 2630 Ma, intrusions were emplaced at increasingly shallow crustal levels. All of the rocks, except for the youngest pegmatitic intrusions, show similar patterns in major and trace elements, with a general trend toward more evolved compositions through time. These patterns indicate that the granitoids record mostly reworking of early intrusions, which is also consistent with patterns observed in the geochronology.

The ca. 2720 Ma Vermilion, Shebandowan, Winston Lake, and Manitouwadge greenstone belts (VGB, SGB, WGB, and MGB, respectively) are located along the northern margin of the Wawa subprovince. They are interpreted to have formed in broadly similar rifted arc to back-arc environments, but their base and precious endowment and, in particular, their endowment in VMS deposits, differ markedly. These difference is metal endowment reflect differences in their metallogenic history that were examined by comparing their regional, belt-scale lithostratigraphy, chemostratigraphy, petrogenesis and tectonic history constrained by new U-Pb zircon geochronology. The MGB is the most VMS-endowed and isotopically juvenile (Pb and Nd) greenstone belt. It has a trace element chemostratigraphy that is consistent with a rifted arc to back-arc environment. The trace element chemostratigraphy of the WGB is also consistent with a rifted-arc to back arc geodynamic setting. The Winston Lake VMS deposits formed during early rifting of the arc and their timing is tightly constrained at ca. 2720 Ma by U-Pb ages of the host felsic strata and post-VMS Zenith gabbro. The Zn-dominated VMS mineralization formed from hydrothermal fluids that were <300 ° and were possibly boiling in relatively shallow water. The trace element chemostratigraphy of the VGB, SGB, and WGB indicates a plume-driven rifted arc to back-arc geodynamic settings. The composition of VMS mineralization, lithofacies, and alteration in these belts are consistent with a relatively shallower-water environment, which may have compromised VMS formation. The high-Mg andesites that are typical of, but restricted to, the SGB formed during compressional “hot” subduction, which resulted in the development of a thicker arc crust. This thicker crust may have inhibited VMS formation, but favoured the formation of magmatic sulphide and gold mineralization. New detrital and magmatic zircon U-Pb geochronology allowed comparison and correlation of lithostratigraphy and metallogeny between the greenstone belts. U-Pb ages within the VGB also defined younger, Timiskaming-type volcanic and sedimentary strata that are coeval with similar deposits in the SGB. These strata are spatially and temporally associated with gold mineralization in both belts and are coeval with similar deformation and magmatic events in the WGB and along the northern margin of the Wawa-Abitibi terrane. This indicates that the formation of Timiskaming-type pull apart basins in the northern part of the Wawa-Abitibi terrane were synchronous, and earlier than in the southern part, which is consistent with oblique convergence of the Wawa-Abitibi terrane onto the Superior Province. Detrital zircon geochronology also revealed the presence of a >2720 Ma iv zircon population within the Timiskaming-type sedimentary strata of the SGB. This is consistent with their derivation from the Wabigoon subprovince and suggests trans-terrane transport of detritus in a foreland –type basin resulting from uplift of the Wabigoon subprovince during accretion of the Wawa subprovince.

[Truncated abstract] The Neoarchean (2800 to 2600 Ma) Eastern Goldfields Superterrane (EGST) comprises elongated belts of deformed and metamorphosed volcanic and sedimentary rocks intruded by granitoids. The Superterrane is made up of five distinct tectonostratigraphic terranes. From west to east these are the Kalgoorlie, Gindalbie, Kurnalpi, Laverton and Duketon Terranes. The Kalgoorlie Terrane is characterised by 2720 to 2680 Ma marine mafic-ultramafic volcanic successions interlayered with, and overlain by, 2710 to 2660 Ma dominantly trondhjemite-tonalite-dacite (TTD) dacititic volcaniclastic rocks (Black Flag Group). The adjacent Gindalbie and Kurnalpi terranes are characterised by 2720 to 2680 Ma calc-alkaline volcanic successions representing oceanic island arcs. To the west of the EGST, the Youanmi Terrane is characterised by older, dominantly 3000 to 2900 Ma greenstone rocks and complex granitoid batholiths derived from older crustal sources. The southern Kalgoorlie Terrane comprises five elongate NNW-trending tectono-stratigraphic domains. Three principal marine komatiitic to basaltic suites, collectively referred to as the Kambalda Sequence, are present, including the wellpreserved massive to pillowed Lower and Upper Basalt Sequences, separated by the Komatiite Unit, as well as numerous dyke suites. The Lower Basalt Sequence comprises the Woolyeenyer Formation, Lunnon, Wongi, Scotia, Missouri Basalts and Burbanks and Penneshaw Formations, whereas the Upper Basalt Sequence contains the Paringa, Coolgardie, Big Dick, Devon Consols, Bent Tree, and Victorious basalts. ... Instead, the data suggest that discrete PGE-bearing phase (s) fractionated from the basaltic magmas. Such phases could be platinum group minerals (PGM; e.g. laurite) and/or alloys, or discrete PGE-rich nuggets. In summary, data on the three magmatic sequences record decompression melting of three distinct mantle sources: (1) long-term depleted asthenosphere for prevalent depleted tholeiitic and komatiitic basalts, and komatiites; (2) long-term enriched asthenosphere for Paringa Basalts and similarly enriched rocks; and (3) shortterm enriched continental lithospheric mantle (CLM) for HREE and Al-depleted dykes. Some of these rocks were contaminated by TTD-type melts. Taken with the existing geophysical and xenocrystic zircon data, the most straightforward interpretation is eruption of a zoned mantle plume at the margin of rifted continental lithosphere. The Kalgoorlie Terrane extensional basin was subsequently tectonically juxtaposed with the adjacent arc-like Gindalbie and Kurnalpi Terranes at approximately 2660 Ma at the start of orogeny in a Cordilleran-style orogen to form the EGST. Collectively, uncontaminated basalts have Nb/Th of 8-16, compared to 8-12 reported for the Lunnon basalts in a previous study. To a first approximation these asthenosphere melts are complementary to average Archean upper continental crust with Nb/Th =2, consistent with early growth of large volumes of continental crust rather than models of steady progressive growth.

The Archean basement rocks in Shandong Province are important components of the Eastern Block in the North China Craton, consisting predominantly of granitoid gneisses with minor mafic and felsic supracrustal rocks and charnockites. They are exposed, from west to east, in the Luxi Granite-Greenstone Terrane, Yishui Terrane and Jiaodong Terrane, of which the low-grade Luxi Granite-Greenstone Terrane has been well studied, whereas little work has been done on the medium- to high-grade Yishui and Jiaodong Terranes. Controversies have long surrounded the timing of crustal growth and tectonic setting of these two terranes. This project is designed to resolve these issues by integrating field investigations, petrography, geochronology, geochemistry and metamorphism of the Yishui and Jiaodong Terranes. New zircon U-Pb data from the major lithologies have revealed that the Jiaodong Terrane experienced multi-stage magmatism at ~2.9 Ga, ~2.7 Ga and 2.6-2.5 Ga followed by two metamorphic events at ~2.50 Ga and 1.9-1.8 Ga, whereas the Yishui Terrane underwent single magmatism at 2.57-2.53 Ga followed by a single metamorphic event at ~2.50 Ga. Zircon Hf isotopic data have revealed that the Jiaodong Terrane underwent juvenile crustal growth with significant ancient crustal material additions at 3.4-3.1 and 2.8-2.7 Ga, while the Yishui Terrane experienced juvenile crustal growth with significant addition of crustal material at 2.8-2.7 Ga. Both the Jiaodong and Yishui Terranes experienced crustal reworking with minor juvenile additions at 2.6-2.5 Ga. Whole-rock compositions and Nd isotopes from the Jiaodong granitoid gneisses suggest that their protoliths are typical Archean tonalitic-trondhjemitic-granodioritic (TTG) suite. They are high in SiO2, Al2O3, Na2O, Sr and Sr/Y ratios, but low in MgO, K2O, TiO2, Cr, Ni, Y and Mg#. They are generally enriched in light rare earth elements and large ion lithophile elements, depleted in heavy rare earth elements and high field strength elements, with slight Eu anomalies. Two groups of granitoid gneisses have been recognized: low- and high-HREE groups, of which the former was generated from partial melting of metabasaltic rocks leaving eclogite in the residue, whereas the latter was formed by partial melting of metabasaltic rocks leaving garnet-amphibolite in the residue. Whole-rock Nd isotopes reveal that the protoliths of Mesoarchean granitoid gneisses were derived mainly from juvenile sources, whereas the early Neoarchean granitoid gneisses were derived from juvenile sources with significant additions of crustal material and the late Neoarchean granitoid gneisses were mainly derived from continental crustal sources. These features indicate that the protoliths of the Jiaodong granitoid gneisses were possibly formed by partial melting of thickened lower crust related to underplating of mafic magmas. Mafic granulites (~2.50 Ga) of the Yishui Terrane show three distinct mineral assemblages corresponding to the pre-peak, peak and post-peak metamorphic stages, with P-T conditions constrained at 660-730℃/<6.6 kbar, 800-820℃ /8.0-8.5 kbar and 686-710℃/7.6-8.6 kbar, respectively, by using THERMOCALC pseudosection modeling. The results define an anticlockwise P-T path involving near-isobaric cooling following the peak metamorphism, suggesting that the ~2.50 Ga metamorphism was most likely related to the intrusion and underplating of mantle-derived magmas. Collectively, the results of this study suggest that the underplating of mantle-derived magmas was most likely related to a mantle plume, which is favored to account for the significant Neoarchean crustal growth and the large-scale metamorphism at the end of Neoarchean in Shandong Province as well as the whole Eastern Block in the North China Craton.
published_or_final_version
Earth Sciences
Doctoral
Doctor of Philosophy

Thesis (Ph.D.)--Indiana University, Dept. of Geological Sciences, 2004.
Title from PDF t.p. (viewed Dec. 1, 2008). Source: Dissertation Abstracts International, Volume: 66-01, Section: B, page: 0161. Chair: Lisa M. Pratt.

Lithium Cesium Tantalum (LCT) pegmatites are important resources for rare metals like Cesium, Lithium or Tantalum, whose demand increased markedly during the past decade. At present, Cs is known to occur in economic quantities only from the two LCT pegmatite deposits at Bikita located in Zimbabwe and Tanco in Canada. Host for this Cs mineralisation is the extreme rare zeolite group mineral pollucite. However, at Bikita and Tanco, pollucite forms huge massive, lensoid shaped and almost monomineralic pollucite mineralisations that occur within the upper portions of the pegmatite. In addition, both pegmatite deposits have a comparable regional geological background as they are hosted within greenstone belts and yield a Neoarchean age of about 2,600 Ma. Furthermore, at present the genesis of these massive pollucite mineralisations was not yet investigated in detail. Major portions of Western Australia consist of Meso- to Neoarchean crustal units (e.g., Yilgarn Craton, Pilbara Craton) that are known to host a large number of LCT pegmatite systems. Among them are the LCT pegmatite deposits Greenbushes (Li, Ta) and Wodgina (Ta, Sn). In addition, small amounts of pollucite were recovered from one single diamond drill core at the Londonderry pegmatite field. Despite that, no systematic investigations and/or exploration studies were conducted for the mode of occurrence of Cs and especially that of pollucite in Western Australia. In the course of the present study nineteen individual pegmatites and pegmatite fields located on the Yilgarn Craton, Pilbara Craton and Kimberley province have been visited and inspected for the occurrence of the Cs mineral pollucite. However, no pollucite could be detected in any of the investigated pegmatites. Four of the inspected LCT-pegmatite systems, namely the Londonderry pegmatite field, the Mount Deans pegmatite field, the Cattlin Creek LCT pegmatite deposit (Yilgarn Craton) and the Wodgina LCT pegmatite deposit (Pilbara Craton) was sampled and investigated in detail. In addition, samples from the Bikita pegmatite field (Zimbabwe Craton) were included into the present study in order to compare the Western Australian pegmatites with a massive pollucite mineralisation bearing LCT pegmatite system. This thesis presents new petrographical, mineralogical, mineralchemical, geochemical, geochronological, fluid inclusion and stable and radiogenic isotope data. The careful interpretation of this data enhances the understanding of the LCT pegmatite systems in Western Australia and Zimbabwe. All of the four investigated LCT pegmatite systems in Western Australia, crop out in similar geological settings, exhibit comparable internal structures, geochemistry and mineralogy to that of the Bikita pegmatite field in Zimbabwe. Furthermore, in all LCT pegmatite systems evidences for late stage hydrothermal processes (e.g., replacement of feldspars) and associated Cs enrichment (e.g., Cs enriched rims on mica, beryl and tourmaline) is documented. With the exception of the Wodgina LCT pegmatite deposit, that yield a Mesoarchean crystallisation age (approx. 2,850 Ma), all other LCT pegmatite systems gave comparable Neoarchean ages of 2,630 Ma to 2,600 Ma. The almost identical ages of the LCT pegmatite systems of the Yilgarn and Zimbabwe cratons suggests, that the process of LCT pegmatite formation at the end of the Neoarchean was active worldwide. Nevertheless, essential distinguishing feature of the Bikita pegmatite field is the presence of massive pollucite mineralisations that resulted from a process that is not part of the general development of LCT pegmatites and is associated with the extreme enrichment of Cs. The new findings of the present study obtained from the Bikita pegmatite field and the Western Australian LCT pegmatite systems significantly improve the knowledge of Cs behaviour in LCT pegmatite systems. Therefore, it is now possible to suggest a genetical model for the formation of massive pollucite mineralisations within LCT pegmatite systems. LCT pegmatites are generally granitic in composition and are interpreted to represent highly fractionated and geochemically specialised derivates from granitic melts. Massive pollucite mineralisation bearing LCT pegmatites evolve from large and voluminous pegmatite melts that intrude as single body along structures within an extensional tectonic setting. After emplacement, initial crystallisation will develop the border and wall zone of the pegmatites, while due to fractionated crystallisation immobile elements (i.e., Cs, Rb) become enriched within the remaining melt and associated hydrothermal fluids. Following this initial crystallisation, a relatively small portion (0.5–1 vol.%) of immiscible melt or fluid will separate during cooling. This immiscible partial melt/fluid is enriched in Al2O3 and Na2O, as well as depleted in SiO2 and will crystallise as analcime. In addition, this melt might allready contains up to 1–2 wt.% Cs2O. However, due to the effects of fluxing components (e.g., H2O, F, B) this analcime melt becomes undercooled which prevents crystallisation of the analcime as intergranular grains. Since this analcime melt exhibits a lower relative gravity when compared to the remaining pegmatite melt the less dense analcime melt will start to ascent gravitationally and accumulate within the upper portion of the pegmatite sheet. At the same time, the remaining melt will start to crystallise separately and form the inner portions of the pegmatite. This crystallisation is characterised by still ongoing fractionation and enrichment of incompatible elements (i.e., Cs, Rb) within the last crystallising minerals (e.g., lepidolite) or concentration of these incompatible elements within exsolving hydrothermal fluids. As analcime and pollucite form a continuous solid solution series, the analcime melt is able to incorporate any available Cs from the melt and/or associated hydrothermal fluids and crystallise as Cs-analcime in the upper portion of the pegmatite sheet. Continuing hydrothermal activity and ongoing substitution of Cs will then start to shift the composition from Cs-analcime composition towards Na-pollucite composition. In addition, if analcime is cooled below 400 °C it is subjected to a negative thermal expansion of about 1 vol.%. This contraction results in the formation of a prominent network of cracks that is filled by late stage minerals (e.g., lepidolite, quartz, feldspar and petalite). Certainly, prior to filling, this network of cracks enhances the available conduits for late stage hydrothermal fluids and the Cs substitution mechanism within the massive pollucite mineralisation. Furthermore, during cooling of the pegmatite, prominent late stage mineral replacement reactions (e.g., replacement of K-feldspar by lepidolite, cleavelandite, and quartz) as well as subsolidus self organisation processes in feldspars take place. These processes are suggested to release additional incompatible elements (e.g., Cs, Rb) into late stage hydrothermal fluids. As feldspar forms large portions of pegmatite a considerable amount of Cs is released and transported via the hydrothermal fluids towards the massive pollucite mineralisation in the upper portion of the pegmatite. Consequently, the initial analcime can accumulate enough Cs in order to shift its composition from the Cs-analcime member (>2 wt.% Cs2O) towards the Na-pollucite member (23–43 wt.% Cs2O) of the solid solution series. The timing of this late stage Cs enrichment is interpreted to be quasi contemporaneous or immediately after the complete crystallisation of the pegmatite melt. However, much younger hydrothermal events that overprint the pegmatite are also interpreted to cause similar results. Hence, it has been demonstrated that the combination of this magmatic and hydrothermal processes is capable to generate an extreme enrichment in Cs in order to explain the formation of massive pollucite mineralisations within LCT pegmatite systems. This genetic model can now be applied to evaluate the potential for occurrences of massive pollucite mineralisations within LCT pegmatite systems in Western Australia and worldwide
Lithium-Caesium-Tantal-(LCT) Pegmatite repräsentieren eine bedeutende Quelle für seltene Metalle, deren Bedarf im letzten Jahrzehnt beträchtlich angestiegen ist. Im Falle von Caesium sind zurzeit weltweit nur zwei LCT-Pegmatitlagerstätten bekannt, die abbauwürdige Vorräte an Cs enthalten. Dies sind die LCT-Pegmatitlagerstätten Bikita in Simbabwe und Tanco in Kanada. Das Wirtsmineral für diese Cs-Mineralisation ist das extrem selten auftretende Zeolith-Gruppen-Mineral Pollucit. In den Lagerstätten Bikita und Tanco bildet Pollucit dagegen massive, linsenförmige und fast monomineralische Pollucitmineralisationen, die in den oberen Bereichen der Pegmatitkörper anstehen. Zusätzlich befinden sich beide Lagerstätten in geologisch vergleichbaren Einheiten. Die Nebengesteine sind Grünsteingürtel die ein neoarchaisches Alter von ca. 2,600 Ma aufweisen. Die Bildung derartiger massiver Pollucitmineralisationen ist bis jetzt noch nicht detailliert untersucht worden. Große Bereiche von Westaustralien werden von meso- bis neoarchaischen Krusteneinheiten (z.B. Yilgarn Kraton, Pilbara Kraton) aufgebaut, von denen auch eine große Anzahl an LCT-Pegmatitsystemen bekannt sind. Darunter befinden sich unter anderem die LCT-Pegmatitlagerstätten Greenbushes (Li, Ta) und Wodgina (Ta, Sn). Zusätzlich wurden kleine Mengen an Pollucit in einer einzigen Kernbohrung im Londonderry Pegmatitfeld angetroffen. Ungeachtet dessen, wurden in Westaustralien bis jetzt keine systematischen Untersuchungen und/oder Explorationskampagnen auf Vorkommen von Cs und speziell der von Pollucit durchgeführt. Im Verlauf dieser Studie wurden insgesamt neunzehn verschiedene Pegmatitvorkommen und Pegmatitfelder des Yilgarn Kratons, Pilbara Kratons und der Kimberley Provinz auf das Vorkommen des Minerals Pollucit untersucht. Allerdings konnte in keinem der untersuchten LCT-Pegmatitsystemen Pollucit nachgewiesen werden. Von vier der untersuchten LCT-Pegmatitsystemen, dem Londonderry Pegmatitfeld, dem Mount Deans Pegmatitfeld, der Cattlin Creek LCT-Pegmatitlagerstätte (Yilgarn Kraton) und der Wodgina LCT-Pegmatitlagerstätte (Pilbara Kraton) wurden detailliert Proben entnommen und weitergehend untersucht. Zusätzlich wurden die massiven Pollucitmineralisationen im Bikita Pegmatitfeld beprobt und in die detailierten Untersuchungen einbezogen. Der Probensatz aus dem Bikita Pegmatitfeld dient als Referenzmaterial mit dem die Pegmatitproben aus Westaustralien verglichen werden. Die vorliegende Arbeit fasst die wesentlichen Ergebnisse der petrographischen, mineralogischen, mineralchemischen, geochemischen und geochronologischen Untersuchungen sowie der Flüssigkeitseinschlussuntersuchungen und stabilen und radiogenen Isotopenzusammensetzungen zusammen. Alle vier der in Westaustralien untersuchten LCT-Pegmatitsysteme kommen in geologisch ähnlichen Rahmengesteinen vor, weisen einen vergleichbaren internen Aufbau, geochemische Zusammensetzung und Mineralogie zu dem des Bikita Pegmatitfeldes in Simbabwe auf. Weiterhin konnten in allen LCT-Pegmatitsystemen Hinweise für späte hydrothermale Prozesse (z.B. Verdrängung von Feldspat) nachgewiesen werden, die einhergehend mit einer Anreicherung von Cs verbunden sind (z.B. Cs-angereicherte Säume um Glimmer, Beryll und Turmalin). Mit der Ausnahme der Wodgina LCT-Pegmatitlagerstätte, in der ein mesoarchaisches Kristallisationsalter (ca. 2,850 Ma) nachgewiesen wurde, lieferten die Altersdatierungen in den anderen LCT-Pegmatitsystemen übereinstimmende neoarchaische Alter von 2,630 Ma bis 2,600 Ma. Diese fast identischen Alter der LCT-Pegmatitsysteme des Yilgarn und Zimbabwe Kratons suggerieren, dass die Prozesse, die zur LCT-Pegmatitbildung am Ende des Neoarchaikums führten, weltweit aktiv waren. Ungeachtet dessen stellt das Vorhandensein von massiver Pollucitmineralisation das Alleinstellungsmerkmal des Bikita Pegmatitfeldes dar, welche sich infolge eines Prozesses gebildet haben der nicht Bestandteil der üblichen LCT-Pegmatitentwicklung ist und sich durch eine extreme Anreicherung an Cs unterscheidet. Die neuen Ergebnisse die in dieser Studie von den Bikita Pegmatitfeld und den Westaustralischen LCT-Pegmatitsystemen gewonnen wurden, verbessern das Verständnis des Verhaltens von Cs in LCT-Pegmatitsystemen deutlich. Somit ist es nun möglich, ein genetisches Modell für die Bildung von massiven Pollucitmineralisationen in LCT-Pegmatitsystemen vorzustellen. LCT-Pegmatite weisen im Allgemeinen eine granitische Zusammensetzung auf und werden als Kristallisat von hoch fraktionierten und geochemisch spezialisierten granitischen Restschmelzen interpretiert. Die Bildung von massiven Pollucitmineralisationen ist nur aus großen und voluminösen Pegmatitschmelzen, die als einzelner Körper entlang von Störungen in extensionalen Stressregimen intrudieren möglich. Nach Platznahme der Schmelze bildet die beginnende Kristallisation zunächst die Kontakt- und Randzone des Pegmatits, wobei infolge von fraktionierter Kristallisation die immobilen Elemente (v.a. Cs, Rb) in der verbleibenden Restschmelze angereichert werden. Im Anschluss an diese erste Kristallisation entmischt sich nach Abkühlung eine sehr kleine Menge (0.5–1 vol.%) Schmelze und/oder Fluid von der Restschmelze. Diese nicht mischbare Teilschmelze/-fluid ist angereichert an Al2O3 und Na2O sowie verarmt an SiO2 und kristallisiert als Analcim. Zusätzlich kann diese Schmelze bereits mit 1–2 wt.% Cs2O angereichert sein. Aufgrund der Auswirkung von Flussmitteln (z.B. H2O, F, B) wird allerdings der Schmelzpunkt dieser Analcimschmelze herabgesetzt und so die Kristallisation des Analcims als intergranulare Körner verhindert. Da diese Analcimschmelze im Vergleich zu der restlichen Schmelze eine geringere relative Dichte besitzt, beginnt sie gravitativ aufzusteigen und sich in den oberen Bereichen des Pegmatitkörpers zu akkumulieren. Währenddessen beginnt die restliche Schmelze separat zu kristallisieren und die inneren Bereiche des Pegmatits zu bilden. Diese Kristallisation ist einhergehend mit fortschreitender Fraktionierung und der Anreicherung von inkompatiblen Elementen (v.a. Cs, Rb) in den sich als letztes bildenden Mineralphasen (z.B. Lepidolit) oder der Konzentration der inkompatiblen Element in die sich entmischenden hydrothermalen Fluiden. Da Analcim und Pollucit eine lückenlose Mischungsreihe bilden, ist die Analcimschmelze in der Lage, alles verfügbare Cs von der Restschmelze und/oder assoziierten hydrothermalen Fluiden an sich zu binden und als Cs-Analcim im oberen Bereich des Pegmatitkörpers zu kristallisieren. Fortschreitende hydrothermale Aktivität und Substitution von Cs verschiebt dann die Zusammensetzung des Analcims von der Cs-Analcim- zu Na-Pollucitzusammensetzung. Zusätzlich erfährt der Analcim bei Abkühlung unter 400 °C eine negative thermische Expansion von ca. 1 vol.%. Diese Kontraktion führt zu der Bildung des markanten Rissnetzwerkes das durch späte Mineralphasen (z.B. Lepidolit, Quarz, Feldspat und Petalit) gefüllt wird. Vor der Mineralisation allerdings, erhöht dieses Netzwerk an Rissen die verfügbaren Wegsamkeiten für die späten hydrothermalen Fluide und begünstigt somit den Cs-Substitutionsmechanismus in der massiven Pollucitmineralisation. Weiterhin kommt es bei der Abkühlung des Pegmatits zu späten Mineralverdrängungsreaktionen (z.B. Verdrängung von K-Feldspat durch Lepidolit, Cleavelandit und Quarz), sowie zu Subsolidus-Selbstordnungsprozessen in Feldspäten. Diese Prozesse werden weiterhin interpretiert inkompatible Elemente (z.B. Cs, Rb) in die späten hydrothermalen Fluide freizusetzen. Da Feldspäte große Teile der Pegmatite bilden, kann somit eine beträchtliche Menge an Cs freigeben werden und durch die späten hydrothermalen Fluide in die massive Pollucitmineralisation in den oberen Bereichen des Pegmatitkörpers transportiert werden. Infolgedessen ist es möglich, dass genügend Cs frei gesetzt werden kann, um die Zusammensetzung innerhalb der Mischkristallreihe von Cs-Analcim (>2 wt.% Cs2O) zu Na-Pollucit (23–43 wt.% Cs2O) zu verschieben. Die zeitliche Einordnung dieser späten Cs-Anreicherung wird als quasi zeitgleich oder im direkten Anschluss an die vollständige Kristallisation der Pegmatitschmelze interpretiert. Es kann allerdings nicht vernachlässigt werden, dass auch jüngere hydrothermale Ereignisse, die den Pegmatitkörper nachträglich überprägen, ähnliche hydrothermale Prozesse hervorrufen können. Somit konnte gezeigt werden, dass es durch Kombination dieser magmatischen und hydrothermalen Prozessen möglich ist, genügend Cs anzureichern, um die Bildung von massiven Pollucitmineralisationen in LCT-Pegmatitsystemen zu ermöglichen. Dieses genetische Modell kann nun dazu genutzt werden, um das Potential von Vorkommen von massiven Pollucitmineralisationen in LCT-Pegmatitsystemen in Westaustralien und weltweit besser einzuschätzen

Les indices aurifères Orfée, Orfée Est et Le Moyne-extension sont encaissés par des formations de fer archéennes, à 300 m du contact entre la subprovince de La Grande et d’Opinaca, dans la région d’Eeyou Istchee Baie James, Québec, Canada. La zone Orfée (~0,2 Mt à 14,5 g/t Au) a une épaisseur apparente de 40 m et une extension latérale sur 100 m; des valeurs en or atteignent 93,7 g/t Au sur 1 m. Vers le nord, les formations de fer sont en contact faillé avec des amphibolites localement minéralisées (max. 4 g/t Au). Des wackes juste faiblement minéralisées bordent les formations de fer au sud. L’ensemble lithologique est fortement déformé et métamorphisé au faciès des amphibolites syn D₂/M₂. L’or natif est associé avec la pyrrhotite semi-massive à massive, concentrée dans des pièges structuraux syn D₂ et D₃. Des inclusions d’or natif dans la pyrrhotite et dans des silicates métamorphiques, des reliques de pyrite dans la pyrrhotite et la löllingite aurifère suggèrent l’introduction de l’or pre à syn métamorphisme. La mise en place de la minéralisation a été restreinte entre 2703 ±7 Ma, âge d’un dyke dioritique pre à syn minéralisation, et 2613 ±0,4 Ma, âge d’une intrusion de granite pegmatitique post minéralisation. Deux âges modèles moyens pondérés, obtenues par datation Re-Os sur l’arsénopyrite/löllingite aurifère, sont beaucoup plus jeunes que la mise en place de la minéralisation. Ces âges, 2582 ±13 Ma et 2557 ±12 Ma, représentent la rétroversion de la löllingite en arsenopyrite lors du métamorphisme rétrograde M₃. L’or natif associée avec des altérations rétrogrades (e.g. chlorite, épidote, séricite et prehnite) au long des fractures suggèrent la remobilisation de la minéralisation. L’or à Orfée est interprété comme étant orogénique (2703 Ma à 2613 Ma), pre à syn métamorphique (M₂), remobilisé lors d’un événement rétrograde (M₃; 2582 Ma à 2557 Ma).
The Orfée, Orfée Est and Le Moyne-extension showings, hosted by Archean iron formations, are located 300 m north of the contact between the La Grande and the Opinaca subprovinces, in the Eeyou Istchee Baie James area, Quebec, Canada. The Orfée showing (~0.2 Mt at 14.5 g/t Au) has an apparent thickness of 40 m and a continuous lateral extension of 100 m; gold values reach up to 93.7 g/t Au. Towards the north, locally mineralized amphibolites (4 g/t Au) are in faulted contact with the iron formations. A wacke unit, bordering the BIFs to the south, is only very weakly mineralized. Syn D₂/M₂, the lithological assemblage is highly deformed and metamorphosed up to amphibolite facies. The native gold is associated with semi-massive to massive pyrrhotite, concentrated in D₂ and D₃ structural traps. Native gold inclusions in pyrrhotite and in metamorphic silicates, relicts of pyrite in pyrrhotite and gold bearing löllingite suggest gold mineralization was introduced pre to syn metamorphism. The gold mineralization emplacement was constraint between 2703 ±7 Ma, age of a dioritic dyke intruded pre to syn mineralization, and 2613 ±0.4 Ma, age of a pegmatitic granite injected post mineralization. Two weighted average model ages of 2582 ±13 and 2557 ±12 Ma for gold-bearing arsenopyrite were obtained by Re-Os dating. These ages most likely represent the retroversion of löllingite to arsenopyrite during a M₃ retrograde metamorphic event. Native gold associated with retrograde alterations (e.g. chlorite, epidote, sericite and prehnite) along fractures suggest gold remobilization. In summary, the gold from Orfée is interpreted to be orogenic (2703 Ma to 2613 Ma), pre to syn M₂ metamorphism, remobilized during a retrograde metamorphic event (M₃; 2582 Ma to 2557 Ma).

The Wallace Lake greenstone belt is located on the southern margin of the Uchi-Sachigo-Goudalie superterrane within the volcanic-rich Uchi subprovince of the Superior Province in southeastern Manitoba, Canada. Its stratigraphy consists of a Mesoarchean complex constituted of alluvial conglomerate derived from ca. 3000 Ma tonalite, overlain by a crustal contaminated mafic-ultramafic volcanic sequence. Both units were deformed and then intruded by a 2.92 Ga tonalite body and related dyke swarm. Thrust sheets of a tholeftic volcanic sequence of unknown age, of oceanic plateau affinity tectonically overlie this Mesoarchean complex. The tectonic assembly was associated with regional SW directed compression, resulting in NW-trending folding and faulting. No metamorphic break is observed within this tectonic package despite major faulting related to this event. Neoarchean (<2709 Ma) greywacke and polymictic conglomerate unconformably overlie these units, and were deformed by dextral transcurrent deformation. Finally, fault bounded low-strain alluvial greywackes mark the last recorded stratigraphic and structural event affecting this area.

The Neoarchean Stillwater Complex (Montana, USA) and the Paleoproterozoic Bushveld Complex (South Africa), two of the world’s largest layered intrusions, have been cornerstones for the study of magmatic processes in the Earth’s crust. Mafic layered intrusions are natural laboratories for assessing the emplacement, crystallization, and cooling mechanisms of mantle-derived basaltic magmas. Most layered intrusions do not yet have robust geochronological frameworks from the base to the top of their stratigraphic successions. Zircon is recognized as a relatively common accessory mineral in the Stillwater and Bushveld intrusions and crystallized from highly fractionated interstitial melt at near-solidus temperatures (980-720°C). High-precision geochronologic frameworks established for both intrusions by U-Pb zircon dating, combined with trace element and hafnium isotope compositions of zircon, reveal extended durations of magmatism (3-5 million years) and non-stratigraphic or out-of-sequence ages for both intrusions. Dating of platinum group element deposits in both intrusions (J-M Reef, Stillwater; Merensky Reef, Bushveld) indicates that they are intrusion-wide time markers that crystallized synchronously over large distances (>300 km, Bushveld). The recognition that zircon can be successfully extracted from mafic-ultramafic rocks associated with magmatic ore deposits provides new opportunities for assessing the timing and duration of mineralization processes in layered intrusions worldwide. Zircon from a thick anorthosite horizon in the Stillwater Complex has been identified as a reference material for U-Pb geochronology of Archean rocks (>2.5 Ga) and fills an important gap in the geologic timescale for the application of precise and accurate U-Pb geochronology. Collectively, the dating results indicate that both the Stillwater Complex and Bushveld Complex do not represent the products of progressively crystallized magma chambers but instead formed as stacks of amalgamated sills representing repeated injections of magma at different stratigraphic levels. These conclusions call into question current concepts regarding the origin of layered intrusions and challenge us to rethink our understanding of the timescales of magma processes throughout Earth history.
Science, Faculty of
Earth, Ocean and Atmospheric Sciences, Department of
Graduate

Short-lived isotope systems can be utilized to track differentiation processes that had occurred during Earth’s early history. Both the 182Hf-182W and 146Sm-142Nd systems are sensitive to silicate fractionation events due to differing parent-daughter incompatibilities. The 182Hf-182W system is also affected by metal-silicate fractionation events due to the siderophile nature of W. An increasing number of mantle-derived rocks, mainly formed during the Archean (4.0-2.5 Ga), have presented variable anomalies in the daughter products of both systems, indicating their sources contain isotope signatures established shortly after the formation of the Earth. Some Archean Fe-rich primitive magmas known as ferropicrites, have been suggested to derive from mantle domains that differentiated after the crystallization of a Hadean (>4.0 Ga) magma ocean. In order to investigate the potential involvement of a Hadean source in the petrogenesis of Archean ferropicrites, we have studied the Nd and W isotopic compositions of rocks from the Pulpwood-Playter Harbour sequence in the Wawa subprovince, Ontario, Canada. This sequence is composed of ferropicritic intrusive rocks and lavas in association with tholeiitic mafic lavas. A 147Sm-143Nd isochron including all lithologies yields an age of 2681±51 Ma (MSWD =6.6) with an initial 143Nd of +2.5. This Nd initial isotopic composition indicates the rocks were derived from a long-term incompatible-element depleted mantle source. Both the ferropicritic and the tholeiitic rocks plot on the same isochron, suggesting they derived from the same mantle source, despite their different geochemical compositions. Negative 142Nd anomalies compared to the Nd terrestrial standard were found in the majority of the rocks studied here, yielding an average μ142Nd value of -2.0±3.9. Although not resolvable from the terrestrial standard given iii the current analytical precision, the fact that almost all analysed samples exhibit negative μ142Nd values could suggest the influence of a Hadean source in their formation. If this is the case, a single early silicate fractionation event occurring between 4.56 and 4.47 Ga could explain both the ε143Nd and μ142Nd values obtained for the studied rocks. Alternatively, the involvement of eclogitic material, with a Hadean basaltic protolith, interacting with Archean peridotitic mantle could explain the Nd isotopic composition of the ferropicrites, but this would not account for the identical isotopic composition of the tholeiites – thus rendering a garnet pyroxenite source improbable. One intrusive ferropicritic sample yielded a resolvable 182W excess of +14.1 ±6.7 ppm. If this excess 182W is characteristic of the Pulpwood-Playter Harbour sequence, it indicates the decoupling of 182Hf-182W and 146Sm-142Nd systems. This decoupling could be explained by early metal-silicate fractionation recorded in the Hf-W systematics of these rocks or the contribution of Fe-rich meteoritic material into the source of ferropicrites.

Dissertação (mestrado)—Universidade de Brasília, Instituto de Geociências, Programa de Pós-Graduação em Geologia, 2018.
Submitted by Raquel Almeida (raquel.df13@gmail.com) on 2018-05-15T16:26:56Z No. of bitstreams: 1 2018_VictorBotelhoPerezGarcia.pdf: 2313547 bytes, checksum: d593399c348afe0ec7985407648f4b34 (MD5)
Approved for entry into archive by Raquel Viana (raquelviana@bce.unb.br) on 2018-05-23T10:30:14Z (GMT) No. of bitstreams: 1 2018_VictorBotelhoPerezGarcia.pdf: 2313547 bytes, checksum: d593399c348afe0ec7985407648f4b34 (MD5)
Made available in DSpace on 2018-05-23T10:30:14Z (GMT). No. of bitstreams: 1 2018_VictorBotelhoPerezGarcia.pdf: 2313547 bytes, checksum: d593399c348afe0ec7985407648f4b34 (MD5) Previous issue date: 2018-05-23
Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq).
O depósito GT-34, localizado a 12 km a SW da mina Sequerinho, Carajás, norte do Brasil, representa uma ocorrência incomum de Ni relacionado ao sistema Iron-OxideCopper-Gold (IOCG) regional. Ocorre ao longo de uma zona de cisalhamento subvertical de orientação NE-SW marcado por zonas de alteração alcáli-Fe encaixado em granitos a tonalitos. A aleração inicial Na-Mg e alteração Ca pervasiva formam, respectivamente, marialiate-ortopiroxênio e hornblenda-plagioclásio-clinopiroxênio. A mineralização de Ni ocorre na forma de brechas com a matriz rica em pentlandita-pirrotita-apatita e fragmentos arredondados compostos dominantemente por fragmentos da alteração Ca. Veios tardios de alteração K-Fe com magnetita ou hematita (alteração K-Fe (Mt) e alteração K-Fe (Hem), respectivamente) remobilizam parcialmente a mineralização, reprecipitando-a como calcopirita-pirrotita-magnetita (alteração K-Fe (Mt)) e como milerita-pirita-apatita (alteração K-Fe (Hem)). A alteração K-Fe (Mt) ocorre como veios irregulares ricos em flogopita-talco, enquanto a alteração K-Fe (Hem) ocorre como veios bem delimitados com K-feldspato-albita-quartzo-clorita-calcita-epidoto. As características iniciais do fluido associado a alteração Na-Mg precisam ser anidras para a estabilização do ortopiroxênio e de elevada salinidade para formação da marialita. Um fluido imiscível composto por CO2-NaCl é sugerido para a atingir tais características. A presença do ortopiroxênio indica temperaturas >700°C. Estudo experimentais indicam que marialiata não se forma a partir de fluidos ricos em NaCl a pressões >7 kbar a temperatura >700°C. A ausência de quartzo pode ocorrer devido a sua dissolução causada por fluidos ricos em NaCl sob pressões >5 kbar e temperaturas similares, também determinado experimentalmente. Cristais de zircão foram recuperados da alteração NaMg inicial e da alteração tardia K-Fe (Mt) fornecendo uma idade concordante de 2.724±4 Ga, corroborando a formação Neoarqueana do depósito GT-34, similar aos demais depósitos IOCG em Carajás. A temperatura >700°C e pressão entre 5–7 kbar, eventuais fluidos evaporíticos não podem estar presentes, sendo necessário uma fonte magmática. As idades obtidas nesse estudo se sobrepõe a idade do magmatismo bimodal Neoarqueano (2.75-2.70 Ga), suportando uma origem magmática-hidrotermal. As condições determinadas para o depósito GT-34 elevam a temperatura inicial do sistema IOCG de Carajás em pelo menos 200°C com pressões podendo chegar até 7 kbar, tornondo-o a mais profunda ocorrência associada ao sistema IOCG de Carajás conhecida até então.
The GT-34 deposit, which is located 12 km SW of the Sequerinho copper-gold mine, Carajás Province, northern Brazil, represents an unusual Ni occurrence related to a regional Iron-Oxide-Copper-Gold (IOCG) system. It occurs along a NE-SW-trending sub-vertical shear zone marked by progressive alkali-Fe alteration zones hosted in tonalite to granite intrusions. Initial Na-Mg and pervasive Ca alteration forms the unique marialite-orthopyroxene and hornblende-plagioclase-clinopyroxene associations, respectively. Nickel mineralization occurs as breccias in a pentlandite-pyrrhotite-apatiterich matrix with rounded fragments chiefly of Ca-alteration parageneses. Late-stage veins of K-Fe magnetite and hematite (K-Fe (Mt) and K-Fe (Hem)) alterations partially remobilize the mineralization, reprecipitating as chalcopyrite-pyrrhotite-magnetite and as millerite-pyrite-apatite, respectively. Potassium-Fe (Mt) occurs as irregular phlogopitetalc-rich veins, while K-Fe (Hem) occurs as sharp K-feldspar-albite-quartz-chloritecalcite-epidote veins. Initial fluid characteristics associated with Na-Mg alteration require anhydrous conditions for orthopyroxene stability and high salinity for marialite formation. An immiscible CO2-NaCl fluid is therefore associated with such conditions. The presence of orthopyroxene indicates temperatures >700°C. Experimental studies indicate that marialite does not form with NaCl-rich fluid at pressures >7 kbar under such temperatures. The absence of quartz might be caused by NaCl dissolution at pressures >5 kbar, as determined experimentally with the same temperature conditions. Zircon crystal were recovered from the initial Na-Mg alteration and late-stage K-Fe (Mt) alteration yielding a concordant 2.724±4 Ga age, corroborating the GT-34 Neoarchean formation similar to other IOCG deposits in Carajás. At >700°C and 5–7 kbar, an eventual evaporitic fluid source would not be present, making a magmatic fluid source necessary. The age constrains obtained in this study overlaps the bimodal Neoarchean magmatism (2.75-2.70 Ga), supporting a magmatic-hydrothermal origin. Determination of such conditions raises the initial temperature of the Carajás IOCG system at least 200°C and pressure up to 7 kbar, making GT-34 the deepest IOCG-related occurrence known to date for this province.

The Neoarchaean Agnew-Wiluna greenstone belt (AWB) of the Kalgoorlie Terrane, within the Eastern Goldfields Superterrane (EGS) of the Yilgarn Craton, Western Australia, contains several world-class, komatiite-hosted, nickel-sulphide ore bodies. These are commonly associated with felsic volcanic successions, many of which are considered to have a tonalite-trondhjemite-dacite (TTD) affinity. The Cosmos greenstone sequence lies on the western edge of the AWB and this previously unstudied mineralised volcanic succession contrasts markedly in age, geochemistry, emplacement mechanisms and probable tectonic setting to that of the majority of the AWB and wider EGS. Detailed subsurface mapping has shown that the footwall to the Cosmos mineralised ultramafic sequence consists of an intricate succession of both fragmental and coherent extrusive lithologies, ranging from basaltic andesites through to rhyolites, plus later-formed felsic and basaltic intrusions. The occurrence of thick sequences of amygdaloidal intermediate lavas intercalated with extensive sequences of dacite lapilli tuff, coupled with the absence of marine sediments or hydrovolcanic products, indicates the succession was formed in a subaerial environment. Chemical composition of the non-ultramafic lithologies is typified by a high-K calc-alkaline to shoshonite signature, indicative of formation in a volcanic arc setting. Assimilation-fractional crystallisation modelling has shown that at least two compositionally distinct sources must be invoked to explain the observed basaltic andesite to rhyolite magma suite. High resolution U-Pb dating of several units within the succession underpins stratigraphic relationships established in the field and indicates that the emplacement of the Cosmos succession took place between ~2736 Ma and ~2653 Ma, making it significantly older and longer-lived than most other greenstone successions within the Kalgoorlie Terrane. Extrusive periodic volcanism spanned ~50 Myrs with three cycles of bimodal intermediate/felsic and ultramafic volcanism occurring between ~2736 Ma and ~2685 Ma. Periodic intrusive activity, related to the local granite plutonism, lasted for a further ~32 Myrs or until ~2653 Ma. The Cosmos succession either represents a separate, older terrane in its own right or it has an autochthonous relationship with the AWB but volcanism initiated much earlier in this region than currently considered. Dating of the Cosmos succession has demonstrated that high-resolution geochronology within individual greenstone successions can be achieved and provides more robust platforms for interpreting the evolution of ancient mineralised volcanic successions. The geochemical affinity of the Cosmos succession indicates a subduction zone was operating in the Kalgoorlie Terrane by ~2736 Ma, much earlier than considered in current regional geodynamic models. The Cosmos volcanic succession provides further evidence that plate tectonics was in operation during the Neoarchaean, contrary to some recently proposed tectonic models.

Includes abstract.
Includes bibliographical references.
The Archaean Francistown Granite-Greenstone Complex in NE Botswana is an integral part of the southwestern margin of the Zimbabwe Craton. It includes a suite of geochemically diverse Neoarchaean granitoids and mafic dominated-supracrustal assemblages. All the supracrustal rocks and mafic intrusions have undergone greenschist to lower amphibolite facies metamorphism, but most mafic intrusions have preserved original igneous textures. The Francistown Granite Greenstone Complex likely represents an arc complex that developed along an active continental margin in the Neoarchaean. This thesis presents new geological, geochemical and geochronological data with which to evaluate the crustal evolution of the NE Botswana, and with which to formulate a geodynamic model for better understanding of the Archaean crustal growth flanking the southwestern margin of the Zimbabwe Craton

The Kaapvaal craton of southern Africa and the Pilbara craton of Western Australia, two of the best-preserved Archean cratons in the world, are covered by remarkably similar early Precambrian cover sequences. This has led to the proposal of the so-called Vaalbara hypothesis, which promotes the existence of the two cratons as a single crustal entity, and possibly, Earth’s oldest assembled continent in Neoarchean-early Paleoproterozoic times. Previous studies have failed to prove the existence of Vaalbara conclusively, principally due to a lack of reliable ages or because of uncertainty and gaps in the paleomagnetic record from the Kaapvaal craton. During the present study paleomagnetic samples were collected from selected Neoarchean- Paleoproterozoic cover sequences of the Kaapvaal craton for the establishment of well-defined paleomagnetic poles. In addition, the Hartswater Group of the Ventersdorp Supergroup was sampled for zircon SHRIMP analyses in order to constrain the ages of poles defined from that succession. The paleopoles established here, together with existing paleopoles from the Kaapvaal craton, are used to evaluate the apparent polar wander path of the craton during the Neoarchean-Paleoproterozoic and are compared with poles of similar age from the Pilbara craton as a test of the Vaalbara hypothesis. Regarding the age of the Hartswater Group, zircon SHRIMP ages of 2735 ± 3 Ma and 2724 ± 6 Ma cast doubt on younger ages from the Klipriviersberg Formation, which comprise the base of the Ventersdorp Supergroup. Traditional (younger) age constraints from the Ventersdorp Supergroup do not support the original Vaalbara correlation. A new correlation is suggested here, taking the new ages into account, showing that the Ventersdorp Supergroup overlaps in time with the Fortescue Group of the Pilbara craton. Most importantly, the new ages also provide constraints on the magnetization within the Platberg Group and the Allanridge Formation. Six new paleopoles, of various quality, are added to the existing database from that craton. These poles from the ~2.73 Ga Platberg Group and ~2.7Ga Allanridge Formation of the Ventersdorp Supergroup, the ~2.5Ga lower Transvaal Supergroup, the lower two unconformitybounded sequences of the Waterberg Group (2.05 Ga and ~1.99 Ga) and the upper Soutpansberg Group (~1.76 Ga) have, together with existing poles from the Kaapvaal craton, led to the definition of an APWP for that craton for a period ~2.78 to ~1.76 Ga. Particularly the poles from the Waterberg and Soutpansberg Groups provided the information to identify complexities (looping) in the APWP that have gone unrecognized in the past. The paleomagnetic data gathered and the newly defined APWP could be used in conjunction with geological evidence from the Kaapvaal and Pilbara cratons to evaluate, and validate, the Vaalbara hypothesis. A good match between the APWP’s of the two cratons for the period ~2.78 to ~2.70 Ga and the geological features (lithology and structure) of the two cratons provide the best evidence that Vaalbara existed as a cratonic unit in the late Archean. Paleomagnetic data constrain the position of the Pilbara craton in immediate proximity to the northwest of the Kaapvaal craton (in a Kaapvaal reference frame). The position of the Zimbabwe craton relative to the Pilbara and Kaapvaal cratons is still unresolved, but indications are that it was most likely in a proximal position to the Kaapvaal craton at 2.7 Ga in a configuration not much different from its present day configuration. This would imply that Vaalbara was most probably the Earth’s oldest assembled continent as proposed by earlier workers. The new paleomagnetic data further suggest that Vaalbara did not exist anymore at ~2.0Ga. When evaluated in conjunction with geological evidence a strong argument can be made for the existence of the Vaalbaran continent up until ~2.22 Ga and that the Pilbara and Kaapvaal cratons became separate entities from about ~2.05 Ga.
Prof. NJ Beukes Prof. DAD Evans

Le gisement de Beattie est situé dans la ceinture de roches vertes de l'Abitibi, à proximité de la faille Porcupine-Destor, et est associé à une syénite porphyrique. Les corps minéralisés ont une ressource totale inférée de 2,77Moz contenu dans 56,2Mt de minerai à 1,53g/t d'or. Dans le gisement de Beattie, deux styles de minéralisation sont présents, à contrôle lithologique et à contrôle structural. La minéralisation à contrôle lithologique est limitée exclusivement à la syénite altérée en carbonates de fer. Cette minéralisation représente du minerai à basse teneur mais fort tonnage, dans lequel l'or est porté par la pyrite arsénifère et l'arsénopyrite. L'or est « invisible »; il se présente sous la forme de solution-solide dans le cœur poreux et riche en arsenic des pyrites. La minéralisation à contrôle structural est présente uniquement dans des zones de cisaillement adjacentes et incluses dans la syénite. Le minerai est à haute teneur dans des zones de brèches silicifiées à caractère hydraulique et tectonique, dans des veines de quartz cherteux, dans des veines polymétalliques intensément silicifiées, et dans des dykes de syénite trachytique très altérée. L'or y est visible sous forme d'éléctrum dans les microfractures des pyrites bréchifiées. Les deux styles de minéralisation et les altérations font partie d'une évolution paragénetique commune dans un environnement magmatique-hydrothermal. Des phases initiales oxydantes ont évolué en conditions réduites à la faveur de fluides magmatiques et externes riches en CO2. Ce changement d'état d'oxydation a entraîné la précipitation des sulfures et la cristallisation de l'or « invisible » dans la pyrite arsénifère et l'arsénopyrite. Une phase d'altération ultérieure, dominée par des fluides hydrothermaux riches en silice, a pour résultat la bréchification des sulfures et leur redistribution dans des corridors siliceux, ainsi que la remobilisation de l'or dans les microfractures des pyrites bréchifiées. Les compositions calculées de δ18O et δD sur les veines de quartz associées à cet évènement tardif sont respectivement 7.67%o et -66%o, indiquant une dominance des fluides magmatiques avec une probable composante métamorphique. Cet évènement syn-métamorphique (transition D2-D3) est associé à un fort enrichissement en Hg, Te, Mo, Ag, Sb, As, et Se. Le style de cristallisation de l'or dans le gisement de Beattie est une conséquence de la dominance des régimes en systèmes ouverts, tant au niveau de l'incorporation dans le magma de l'arsenic qui contrôle la précipitation de l'or « invisible », que de la circulation tardive de fluides hydrothermaux riches en silice qui sont à l'origine de la remobilisation de l'or. Le gisement de Beattie partage des affinités avec des gisements associés aux intrusions (Intrusion Related Gold Deposit), des gisements épithermaux à tendance neutre à intermédiaire, et des gisements de type mésothermaux. ______________________________________________________________________________ MOTS-CLÉS DE L’AUTEUR : Gisement d'or, porphyre Archéen, or invisible, remobilisation de l'or

Lithium Cesium Tantalum (LCT) pegmatites are important resources for rare metals like Cesium, Lithium or Tantalum, whose demand increased markedly during the past decade. At present, Cs is known to occur in economic quantities only from the two LCT pegmatite deposits at Bikita located in Zimbabwe and Tanco in Canada. Host for this Cs mineralisation is the extreme rare zeolite group mineral pollucite. However, at Bikita and Tanco, pollucite forms huge massive, lensoid shaped and almost monomineralic pollucite mineralisations that occur within the upper portions of the pegmatite. In addition, both pegmatite deposits have a comparable regional geological background as they are hosted within greenstone belts and yield a Neoarchean age of about 2,600 Ma. Furthermore, at present the genesis of these massive pollucite mineralisations was not yet investigated in detail. Major portions of Western Australia consist of Meso- to Neoarchean crustal units (e.g., Yilgarn Craton, Pilbara Craton) that are known to host a large number of LCT pegmatite systems. Among them are the LCT pegmatite deposits Greenbushes (Li, Ta) and Wodgina (Ta, Sn). In addition, small amounts of pollucite were recovered from one single diamond drill core at the Londonderry pegmatite field. Despite that, no systematic investigations and/or exploration studies were conducted for the mode of occurrence of Cs and especially that of pollucite in Western Australia. In the course of the present study nineteen individual pegmatites and pegmatite fields located on the Yilgarn Craton, Pilbara Craton and Kimberley province have been visited and inspected for the occurrence of the Cs mineral pollucite. However, no pollucite could be detected in any of the investigated pegmatites. Four of the inspected LCT-pegmatite systems, namely the Londonderry pegmatite field, the Mount Deans pegmatite field, the Cattlin Creek LCT pegmatite deposit (Yilgarn Craton) and the Wodgina LCT pegmatite deposit (Pilbara Craton) was sampled and investigated in detail. In addition, samples from the Bikita pegmatite field (Zimbabwe Craton) were included into the present study in order to compare the Western Australian pegmatites with a massive pollucite mineralisation bearing LCT pegmatite system. This thesis presents new petrographical, mineralogical, mineralchemical, geochemical, geochronological, fluid inclusion and stable and radiogenic isotope data. The careful interpretation of this data enhances the understanding of the LCT pegmatite systems in Western Australia and Zimbabwe. All of the four investigated LCT pegmatite systems in Western Australia, crop out in similar geological settings, exhibit comparable internal structures, geochemistry and mineralogy to that of the Bikita pegmatite field in Zimbabwe. Furthermore, in all LCT pegmatite systems evidences for late stage hydrothermal processes (e.g., replacement of feldspars) and associated Cs enrichment (e.g., Cs enriched rims on mica, beryl and tourmaline) is documented. With the exception of the Wodgina LCT pegmatite deposit, that yield a Mesoarchean crystallisation age (approx. 2,850 Ma), all other LCT pegmatite systems gave comparable Neoarchean ages of 2,630 Ma to 2,600 Ma. The almost identical ages of the LCT pegmatite systems of the Yilgarn and Zimbabwe cratons suggests, that the process of LCT pegmatite formation at the end of the Neoarchean was active worldwide. Nevertheless, essential distinguishing feature of the Bikita pegmatite field is the presence of massive pollucite mineralisations that resulted from a process that is not part of the general development of LCT pegmatites and is associated with the extreme enrichment of Cs. The new findings of the present study obtained from the Bikita pegmatite field and the Western Australian LCT pegmatite systems significantly improve the knowledge of Cs behaviour in LCT pegmatite systems. Therefore, it is now possible to suggest a genetical model for the formation of massive pollucite mineralisations within LCT pegmatite systems. LCT pegmatites are generally granitic in composition and are interpreted to represent highly fractionated and geochemically specialised derivates from granitic melts. Massive pollucite mineralisation bearing LCT pegmatites evolve from large and voluminous pegmatite melts that intrude as single body along structures within an extensional tectonic setting. After emplacement, initial crystallisation will develop the border and wall zone of the pegmatites, while due to fractionated crystallisation immobile elements (i.e., Cs, Rb) become enriched within the remaining melt and associated hydrothermal fluids. Following this initial crystallisation, a relatively small portion (0.5–1 vol.%) of immiscible melt or fluid will separate during cooling. This immiscible partial melt/fluid is enriched in Al2O3 and Na2O, as well as depleted in SiO2 and will crystallise as analcime. In addition, this melt might allready contains up to 1–2 wt.% Cs2O. However, due to the effects of fluxing components (e.g., H2O, F, B) this analcime melt becomes undercooled which prevents crystallisation of the analcime as intergranular grains. Since this analcime melt exhibits a lower relative gravity when compared to the remaining pegmatite melt the less dense analcime melt will start to ascent gravitationally and accumulate within the upper portion of the pegmatite sheet. At the same time, the remaining melt will start to crystallise separately and form the inner portions of the pegmatite. This crystallisation is characterised by still ongoing fractionation and enrichment of incompatible elements (i.e., Cs, Rb) within the last crystallising minerals (e.g., lepidolite) or concentration of these incompatible elements within exsolving hydrothermal fluids. As analcime and pollucite form a continuous solid solution series, the analcime melt is able to incorporate any available Cs from the melt and/or associated hydrothermal fluids and crystallise as Cs-analcime in the upper portion of the pegmatite sheet. Continuing hydrothermal activity and ongoing substitution of Cs will then start to shift the composition from Cs-analcime composition towards Na-pollucite composition. In addition, if analcime is cooled below 400 °C it is subjected to a negative thermal expansion of about 1 vol.%. This contraction results in the formation of a prominent network of cracks that is filled by late stage minerals (e.g., lepidolite, quartz, feldspar and petalite). Certainly, prior to filling, this network of cracks enhances the available conduits for late stage hydrothermal fluids and the Cs substitution mechanism within the massive pollucite mineralisation. Furthermore, during cooling of the pegmatite, prominent late stage mineral replacement reactions (e.g., replacement of K-feldspar by lepidolite, cleavelandite, and quartz) as well as subsolidus self organisation processes in feldspars take place. These processes are suggested to release additional incompatible elements (e.g., Cs, Rb) into late stage hydrothermal fluids. As feldspar forms large portions of pegmatite a considerable amount of Cs is released and transported via the hydrothermal fluids towards the massive pollucite mineralisation in the upper portion of the pegmatite. Consequently, the initial analcime can accumulate enough Cs in order to shift its composition from the Cs-analcime member (>2 wt.% Cs2O) towards the Na-pollucite member (23–43 wt.% Cs2O) of the solid solution series. The timing of this late stage Cs enrichment is interpreted to be quasi contemporaneous or immediately after the complete crystallisation of the pegmatite melt. However, much younger hydrothermal events that overprint the pegmatite are also interpreted to cause similar results. Hence, it has been demonstrated that the combination of this magmatic and hydrothermal processes is capable to generate an extreme enrichment in Cs in order to explain the formation of massive pollucite mineralisations within LCT pegmatite systems. This genetic model can now be applied to evaluate the potential for occurrences of massive pollucite mineralisations within LCT pegmatite systems in Western Australia and worldwide.:Contents Abstract . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . iii Zusammenfassung . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . v Versicherung . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . vii Acknowledgments . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . ix Contents . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . xi 1. Introduction 1 1.1. Motivation and Scope of the Thesis . . . . . . . . . . . . . . . . . . . . . . . . 1 1.2. Structure of the Thesis . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5 2. Fundamentals 7 2.1. The Alkali Metal Cesium . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7 2.1.1. Distribution of Cesium . . . . . . . . . . . . . . . . . . . . . . . . . . . 7 2.1.2. Mineralogy of Cesium . . . . . . . . . . . . . . . . . . . . . . . . . . . 8 2.1.3. Geochemical Behaviour of Cesium . . . . . . . . . . . . . . . . . . . . 13 2.1.4. Economy of Cesium . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15 2.2. Pollucite – (Cs,Na)2Al2Si4O12×H2O . . . . . . . . . . . . . . . . . . . . . . . . 16 2.2.1. Crystal Structure . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 16 2.2.2. Analcime–Pollucite–Series . . . . . . . . . . . . . . . . . . . . . . . . . 17 2.2.3. Formation of Pollucite . . . . . . . . . . . . . . . . . . . . . . . . . . . 17 2.2.4. Pollucite Occurences . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21 2.3. Pegmatites . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 34 2.3.1. General Characteristics of Pegmatites . . . . . . . . . . . . . . . . . . 34 2.3.2. Controls on Pegmatite Formation and Evolution . . . . . . . . . . . . . 40 2.3.3. Pegmatite Age Distribution and Continental Crust Formation . . . . . . 43 3. Geological Settings of Archean Cratons 47 3.1. Zimbabwe Craton . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 47 3.1.1. Tectonostratigraphic Subdivision . . . . . . . . . . . . . . . . . . . . . 48 3.1.2. Tectonometamorphic Evolution of the Northern Limpopo Thrust Zone . 49 3.1.3. Pegmatites within the Zimbabwe Craton . . . . . . . . . . . . . . . . . 52 3.1.4. Masvingo Greenstone Belt . . . . . . . . . . . . . . . . . . . . . . . . . 53 3.1.5. Geological Setting of the Bikita Pegmatite District . . . . . . . . . . . . 58 3.2. Yilgarn Craton . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 62 3.2.1. Tectonostratigraphic Framework and Geological Development . . . . . 62 3.2.2. Tectonic Models for the Development . . . . . . . . . . . . . . . . . . . 70 3.2.3. Pegmatites within the Yilgarn Craton . . . . . . . . . . . . . . . . . . . 76 3.2.4. Geological setting of the Londonderry Pegmatite Field . . . . . . . . . . 76 3.2.5. Geological Setting of the Mount Deans Pegmatite Field . . . . . . . . . 85 3.2.6. Geological Setting of the Cattlin Creek Pegmatite Deposit . . . . . . . . 91 3.3. Pilbara Craton . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 99 3.3.1. Tectonostratigraphic Framework and Geological Development . . . . . 99 3.3.2. Tectonic Model for the Development . . . . . . . . . . . . . . . . . . . 101 3.3.3. Pegmatites within the Pilbara Craton . . . . . . . . . . . . . . . . . . . 105 3.3.4. Geological Setting of the Wodgina Pegmatite District . . . . . . . . . . 106 4. Fieldwork and Sampling of Selected Pegmatites and Pegmatite Fields 115 4.1. Bikita Pegmatite Field . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 115 4.2. Londonderry Pegmatite Field . . . . . . . . . . . . . . . . . . . . . . . . . . . . 115 4.2.1. Londonderry Feldspar Quarry Pegmatite . . . . . . . . . . . . . . . . . 115 4.2.2. Lepidolite Hill Pegmatite . . . . . . . . . . . . . . . . . . . . . . . . . . 117 4.2.3. Tantalite Hill Pegmatite . . . . . . . . . . . . . . . . . . . . . . . . . . . 118 4.3. Mount Deans Pegmatite Field . . . . . . . . . . . . . . . . . . . . . . . . . . . 118 4.3.1. Type I – Flat Lying Pegmatites . . . . . . . . . . . . . . . . . . . . . . . 118 4.3.2. Type II – Steeply Dipping Pegmatites . . . . . . . . . . . . . . . . . . . 120 4.4. Cattlin Creek Pegmatite . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 120 4.5. Wodgina LCT-Pegmatite Deposit . . . . . . . . . . . . . . . . . . . . . . . . . . 121 4.5.1. Mount Tinstone Pegmatite . . . . . . . . . . . . . . . . . . . . . . . . . 123 4.5.2. Mount Cassiterite Pegmatite . . . . . . . . . . . . . . . . . . . . . . . . 123 5. Petrography and Mineralogy 139 5.1. Quantitative Mineralogy by Means of Mineral Liberation Analysis . . . . . . . . 141 5.2. Mineralogical and Petrographical Characteristics of Individual Mineral Groups . 141 5.2.1. Feldspar . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 141 5.2.2. Quartz . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 144 5.2.3. Mica . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 146 5.2.4. Pollucite . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 147 5.2.5. Petalite . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 149 5.2.6. Spodumene . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 149 5.2.7. Beryl . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 154 5.2.8. Tourmaline . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 155 5.2.9. Apatite . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157 5.2.10. Ta-, Nb- and Sn-oxides . . . . . . . . . . . . . . . . . . . . . . . . . . 157 5.3. Reconstruction of the General Crystallisation Sequence . . . . . . . . . . . . . 162 6. Geochemistry 165 6.1. Major Elements . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 165 6.2. Selected Minor and Trace Elements . . . . . . . . . . . . . . . . . . . . . . . . 174 6.3. Fractionation Indicators . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 175 6.4. Rare Earth Elements . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 185 7. Geochronology 193 7.1. 40Ar/39Ar-Method on Mica . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 193 7.1.1. Bikita Pegmatite Field . . . . . . . . . . . . . . . . . . . . . . . . . . . 194 7.1.2. Mount Deans Pegmatite Field . . . . . . . . . . . . . . . . . . . . . . . 195 7.1.3. Londonderry Pegmatite Field . . . . . . . . . . . . . . . . . . . . . . . 195 7.1.4. Cattlin Creek Pegmatite . . . . . . . . . . . . . . . . . . . . . . . . . . 195 7.1.5. Wodgina Pegmatite . . . . . . . . . . . . . . . . . . . . . . . . . . . . 198 7.2. Th-U-Total Pb Monazite Dating . . . . . . . . . . . . . . . . . . . . . . . . . . . 201 7.2.1. Monazite Ages . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 201 7.3. U/Pb Dating of Selected Ta-, Nb- and Sn-Oxide Minerals . . . . . . . . . . . . 203 7.3.1. Bikita Pegmatite Field . . . . . . . . . . . . . . . . . . . . . . . . . . . 203 7.3.2. Londonderry Pegmatite Field . . . . . . . . . . . . . . . . . . . . . . . 203 7.3.3. Mount Deans Pegmatite Field . . . . . . . . . . . . . . . . . . . . . . . 206 7.3.4. Cattlin Creek Pegmatite . . . . . . . . . . . . . . . . . . . . . . . . . . 206 7.3.5. Wodgina Pegmatite . . . . . . . . . . . . . . . . . . . . . . . . . . . . 207 8. Fluid Inclusion Study 211 8.1. Bikita Pegmatite Field . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 211 8.2. Wodgina Pegmatite . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 211 8.3. Carbon Isotope Analysis on Fluid Inclusion Gas of Selected Mineral Phases . . 212 9. Stable and Radiogenic Isotopes 217 9.1. Whole Rock Sm/Nd-Isotopy . . . . . . . . . . . . . . . . . . . . . . . . . . . . 217 9.1.1. New Whole Rock Sm/Nd Data . . . . . . . . . . . . . . . . . . . . . . 217 9.2. Lithium Isotope Analysis on Selected Mineral Phases . . . . . . . . . . . . . . . 220 9.2.1. New Lithium Isotope Data . . . . . . . . . . . . . . . . . . . . . . . . . 220 10.Discussion 227 10.1. Regional Geological and Tectonomagmatic Development . . . . . . . . . . . . 227 10.1.1. Constraints from Field Evidence . . . . . . . . . . . . . . . . . . . . . . 227 10.1.2. Petrographical and Mineralogical Constraints . . . . . . . . . . . . . . 229 10.1.3. Geochemical Constraints . . . . . . . . . . . . . . . . . . . . . . . . . 230 10.1.4. Isotopic Constraints . . . . . . . . . . . . . . . . . . . . . . . . . . . . 232 10.1.5. Constraints from Fluid Inclusion Data . . . . . . . . . . . . . . . . . . . 233 10.1.6. Geochronological Constrains . . . . . . . . . . . . . . . . . . . . . . . 233 10.2. Massive Pollucite Mineralisations . . . . . . . . . . . . . . . . . . . . . . . . . . 243 10.2.1. Unique Characteristics of Massive Pollucite Mineralisations . . . . . . . 243 10.2.2. New Concepts for the Formation of Massive Pollucite Mineralisations . . 252 10.3. Genetic Model for the Formation of Massive Pollucite Mineralisations within LCT Pegmatite Systems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 264 11.Summary and Conclusions 267 References 273 Lists of Abbreviations 309 General Abbreviations . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 309 Mineral Abbreviations . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 310 List of Figures 311 List of Tables 315 Appendix 317 A. Legend for Topographic Maps 319 B. Sample List 323 C. Methodology 331 C.1. Quantitative Mineralogy by Means of Mineral Liberation Analysis . . . . . . . . 331 C.2. Geochemistry . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 331 C.3. 40Ar/39Ar-Method on Mica . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 335 C.4. Th-U-Total Pb Monazite Dating . . . . . . . . . . . . . . . . . . . . . . . . . . . 335 C.5. U/Pb Dating of Selected Ta-, Nb- and Sn-Oxide Minerals . . . . . . . . . . . . 336 C.6. Fluid Inclusion Study . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 337 C.7. Whole Rock Sm/Nd-Isotopy . . . . . . . . . . . . . . . . . . . . . . . . . . . . 338 C.8. Lithium Isotope Analysis on Selected Mineral Phases . . . . . . . . . . . . . . . 338 D. Data – Mineral Liberation Analysis 341 E. Data – Geochemistry 345 F. Data – Geochronology 349 G. Data – Stable and Radiogenic Isotopes 353
Lithium-Caesium-Tantal-(LCT) Pegmatite repräsentieren eine bedeutende Quelle für seltene Metalle, deren Bedarf im letzten Jahrzehnt beträchtlich angestiegen ist. Im Falle von Caesium sind zurzeit weltweit nur zwei LCT-Pegmatitlagerstätten bekannt, die abbauwürdige Vorräte an Cs enthalten. Dies sind die LCT-Pegmatitlagerstätten Bikita in Simbabwe und Tanco in Kanada. Das Wirtsmineral für diese Cs-Mineralisation ist das extrem selten auftretende Zeolith-Gruppen-Mineral Pollucit. In den Lagerstätten Bikita und Tanco bildet Pollucit dagegen massive, linsenförmige und fast monomineralische Pollucitmineralisationen, die in den oberen Bereichen der Pegmatitkörper anstehen. Zusätzlich befinden sich beide Lagerstätten in geologisch vergleichbaren Einheiten. Die Nebengesteine sind Grünsteingürtel die ein neoarchaisches Alter von ca. 2,600 Ma aufweisen. Die Bildung derartiger massiver Pollucitmineralisationen ist bis jetzt noch nicht detailliert untersucht worden. Große Bereiche von Westaustralien werden von meso- bis neoarchaischen Krusteneinheiten (z.B. Yilgarn Kraton, Pilbara Kraton) aufgebaut, von denen auch eine große Anzahl an LCT-Pegmatitsystemen bekannt sind. Darunter befinden sich unter anderem die LCT-Pegmatitlagerstätten Greenbushes (Li, Ta) und Wodgina (Ta, Sn). Zusätzlich wurden kleine Mengen an Pollucit in einer einzigen Kernbohrung im Londonderry Pegmatitfeld angetroffen. Ungeachtet dessen, wurden in Westaustralien bis jetzt keine systematischen Untersuchungen und/oder Explorationskampagnen auf Vorkommen von Cs und speziell der von Pollucit durchgeführt. Im Verlauf dieser Studie wurden insgesamt neunzehn verschiedene Pegmatitvorkommen und Pegmatitfelder des Yilgarn Kratons, Pilbara Kratons und der Kimberley Provinz auf das Vorkommen des Minerals Pollucit untersucht. Allerdings konnte in keinem der untersuchten LCT-Pegmatitsystemen Pollucit nachgewiesen werden. Von vier der untersuchten LCT-Pegmatitsystemen, dem Londonderry Pegmatitfeld, dem Mount Deans Pegmatitfeld, der Cattlin Creek LCT-Pegmatitlagerstätte (Yilgarn Kraton) und der Wodgina LCT-Pegmatitlagerstätte (Pilbara Kraton) wurden detailliert Proben entnommen und weitergehend untersucht. Zusätzlich wurden die massiven Pollucitmineralisationen im Bikita Pegmatitfeld beprobt und in die detailierten Untersuchungen einbezogen. Der Probensatz aus dem Bikita Pegmatitfeld dient als Referenzmaterial mit dem die Pegmatitproben aus Westaustralien verglichen werden. Die vorliegende Arbeit fasst die wesentlichen Ergebnisse der petrographischen, mineralogischen, mineralchemischen, geochemischen und geochronologischen Untersuchungen sowie der Flüssigkeitseinschlussuntersuchungen und stabilen und radiogenen Isotopenzusammensetzungen zusammen. Alle vier der in Westaustralien untersuchten LCT-Pegmatitsysteme kommen in geologisch ähnlichen Rahmengesteinen vor, weisen einen vergleichbaren internen Aufbau, geochemische Zusammensetzung und Mineralogie zu dem des Bikita Pegmatitfeldes in Simbabwe auf. Weiterhin konnten in allen LCT-Pegmatitsystemen Hinweise für späte hydrothermale Prozesse (z.B. Verdrängung von Feldspat) nachgewiesen werden, die einhergehend mit einer Anreicherung von Cs verbunden sind (z.B. Cs-angereicherte Säume um Glimmer, Beryll und Turmalin). Mit der Ausnahme der Wodgina LCT-Pegmatitlagerstätte, in der ein mesoarchaisches Kristallisationsalter (ca. 2,850 Ma) nachgewiesen wurde, lieferten die Altersdatierungen in den anderen LCT-Pegmatitsystemen übereinstimmende neoarchaische Alter von 2,630 Ma bis 2,600 Ma. Diese fast identischen Alter der LCT-Pegmatitsysteme des Yilgarn und Zimbabwe Kratons suggerieren, dass die Prozesse, die zur LCT-Pegmatitbildung am Ende des Neoarchaikums führten, weltweit aktiv waren. Ungeachtet dessen stellt das Vorhandensein von massiver Pollucitmineralisation das Alleinstellungsmerkmal des Bikita Pegmatitfeldes dar, welche sich infolge eines Prozesses gebildet haben der nicht Bestandteil der üblichen LCT-Pegmatitentwicklung ist und sich durch eine extreme Anreicherung an Cs unterscheidet. Die neuen Ergebnisse die in dieser Studie von den Bikita Pegmatitfeld und den Westaustralischen LCT-Pegmatitsystemen gewonnen wurden, verbessern das Verständnis des Verhaltens von Cs in LCT-Pegmatitsystemen deutlich. Somit ist es nun möglich, ein genetisches Modell für die Bildung von massiven Pollucitmineralisationen in LCT-Pegmatitsystemen vorzustellen. LCT-Pegmatite weisen im Allgemeinen eine granitische Zusammensetzung auf und werden als Kristallisat von hoch fraktionierten und geochemisch spezialisierten granitischen Restschmelzen interpretiert. Die Bildung von massiven Pollucitmineralisationen ist nur aus großen und voluminösen Pegmatitschmelzen, die als einzelner Körper entlang von Störungen in extensionalen Stressregimen intrudieren möglich. Nach Platznahme der Schmelze bildet die beginnende Kristallisation zunächst die Kontakt- und Randzone des Pegmatits, wobei infolge von fraktionierter Kristallisation die immobilen Elemente (v.a. Cs, Rb) in der verbleibenden Restschmelze angereichert werden. Im Anschluss an diese erste Kristallisation entmischt sich nach Abkühlung eine sehr kleine Menge (0.5–1 vol.%) Schmelze und/oder Fluid von der Restschmelze. Diese nicht mischbare Teilschmelze/-fluid ist angereichert an Al2O3 und Na2O sowie verarmt an SiO2 und kristallisiert als Analcim. Zusätzlich kann diese Schmelze bereits mit 1–2 wt.% Cs2O angereichert sein. Aufgrund der Auswirkung von Flussmitteln (z.B. H2O, F, B) wird allerdings der Schmelzpunkt dieser Analcimschmelze herabgesetzt und so die Kristallisation des Analcims als intergranulare Körner verhindert. Da diese Analcimschmelze im Vergleich zu der restlichen Schmelze eine geringere relative Dichte besitzt, beginnt sie gravitativ aufzusteigen und sich in den oberen Bereichen des Pegmatitkörpers zu akkumulieren. Währenddessen beginnt die restliche Schmelze separat zu kristallisieren und die inneren Bereiche des Pegmatits zu bilden. Diese Kristallisation ist einhergehend mit fortschreitender Fraktionierung und der Anreicherung von inkompatiblen Elementen (v.a. Cs, Rb) in den sich als letztes bildenden Mineralphasen (z.B. Lepidolit) oder der Konzentration der inkompatiblen Element in die sich entmischenden hydrothermalen Fluiden. Da Analcim und Pollucit eine lückenlose Mischungsreihe bilden, ist die Analcimschmelze in der Lage, alles verfügbare Cs von der Restschmelze und/oder assoziierten hydrothermalen Fluiden an sich zu binden und als Cs-Analcim im oberen Bereich des Pegmatitkörpers zu kristallisieren. Fortschreitende hydrothermale Aktivität und Substitution von Cs verschiebt dann die Zusammensetzung des Analcims von der Cs-Analcim- zu Na-Pollucitzusammensetzung. Zusätzlich erfährt der Analcim bei Abkühlung unter 400 °C eine negative thermische Expansion von ca. 1 vol.%. Diese Kontraktion führt zu der Bildung des markanten Rissnetzwerkes das durch späte Mineralphasen (z.B. Lepidolit, Quarz, Feldspat und Petalit) gefüllt wird. Vor der Mineralisation allerdings, erhöht dieses Netzwerk an Rissen die verfügbaren Wegsamkeiten für die späten hydrothermalen Fluide und begünstigt somit den Cs-Substitutionsmechanismus in der massiven Pollucitmineralisation. Weiterhin kommt es bei der Abkühlung des Pegmatits zu späten Mineralverdrängungsreaktionen (z.B. Verdrängung von K-Feldspat durch Lepidolit, Cleavelandit und Quarz), sowie zu Subsolidus-Selbstordnungsprozessen in Feldspäten. Diese Prozesse werden weiterhin interpretiert inkompatible Elemente (z.B. Cs, Rb) in die späten hydrothermalen Fluide freizusetzen. Da Feldspäte große Teile der Pegmatite bilden, kann somit eine beträchtliche Menge an Cs freigeben werden und durch die späten hydrothermalen Fluide in die massive Pollucitmineralisation in den oberen Bereichen des Pegmatitkörpers transportiert werden. Infolgedessen ist es möglich, dass genügend Cs frei gesetzt werden kann, um die Zusammensetzung innerhalb der Mischkristallreihe von Cs-Analcim (>2 wt.% Cs2O) zu Na-Pollucit (23–43 wt.% Cs2O) zu verschieben. Die zeitliche Einordnung dieser späten Cs-Anreicherung wird als quasi zeitgleich oder im direkten Anschluss an die vollständige Kristallisation der Pegmatitschmelze interpretiert. Es kann allerdings nicht vernachlässigt werden, dass auch jüngere hydrothermale Ereignisse, die den Pegmatitkörper nachträglich überprägen, ähnliche hydrothermale Prozesse hervorrufen können. Somit konnte gezeigt werden, dass es durch Kombination dieser magmatischen und hydrothermalen Prozessen möglich ist, genügend Cs anzureichern, um die Bildung von massiven Pollucitmineralisationen in LCT-Pegmatitsystemen zu ermöglichen. Dieses genetische Modell kann nun dazu genutzt werden, um das Potential von Vorkommen von massiven Pollucitmineralisationen in LCT-Pegmatitsystemen in Westaustralien und weltweit besser einzuschätzen.:Contents Abstract . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . iii Zusammenfassung . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . v Versicherung . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . vii Acknowledgments . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . ix Contents . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . xi 1. Introduction 1 1.1. Motivation and Scope of the Thesis . . . . . . . . . . . . . . . . . . . . . . . . 1 1.2. Structure of the Thesis . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5 2. Fundamentals 7 2.1. The Alkali Metal Cesium . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7 2.1.1. Distribution of Cesium . . . . . . . . . . . . . . . . . . . . . . . . . . . 7 2.1.2. Mineralogy of Cesium . . . . . . . . . . . . . . . . . . . . . . . . . . . 8 2.1.3. Geochemical Behaviour of Cesium . . . . . . . . . . . . . . . . . . . . 13 2.1.4. Economy of Cesium . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15 2.2. Pollucite – (Cs,Na)2Al2Si4O12×H2O . . . . . . . . . . . . . . . . . . . . . . . . 16 2.2.1. Crystal Structure . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 16 2.2.2. Analcime–Pollucite–Series . . . . . . . . . . . . . . . . . . . . . . . . . 17 2.2.3. Formation of Pollucite . . . . . . . . . . . . . . . . . . . . . . . . . . . 17 2.2.4. Pollucite Occurences . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21 2.3. Pegmatites . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 34 2.3.1. General Characteristics of Pegmatites . . . . . . . . . . . . . . . . . . 34 2.3.2. Controls on Pegmatite Formation and Evolution . . . . . . . . . . . . . 40 2.3.3. Pegmatite Age Distribution and Continental Crust Formation . . . . . . 43 3. Geological Settings of Archean Cratons 47 3.1. Zimbabwe Craton . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 47 3.1.1. Tectonostratigraphic Subdivision . . . . . . . . . . . . . . . . . . . . . 48 3.1.2. Tectonometamorphic Evolution of the Northern Limpopo Thrust Zone . 49 3.1.3. Pegmatites within the Zimbabwe Craton . . . . . . . . . . . . . . . . . 52 3.1.4. Masvingo Greenstone Belt . . . . . . . . . . . . . . . . . . . . . . . . . 53 3.1.5. Geological Setting of the Bikita Pegmatite District . . . . . . . . . . . . 58 3.2. Yilgarn Craton . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 62 3.2.1. Tectonostratigraphic Framework and Geological Development . . . . . 62 3.2.2. Tectonic Models for the Development . . . . . . . . . . . . . . . . . . . 70 3.2.3. Pegmatites within the Yilgarn Craton . . . . . . . . . . . . . . . . . . . 76 3.2.4. Geological setting of the Londonderry Pegmatite Field . . . . . . . . . . 76 3.2.5. Geological Setting of the Mount Deans Pegmatite Field . . . . . . . . . 85 3.2.6. Geological Setting of the Cattlin Creek Pegmatite Deposit . . . . . . . . 91 3.3. Pilbara Craton . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 99 3.3.1. Tectonostratigraphic Framework and Geological Development . . . . . 99 3.3.2. Tectonic Model for the Development . . . . . . . . . . . . . . . . . . . 101 3.3.3. Pegmatites within the Pilbara Craton . . . . . . . . . . . . . . . . . . . 105 3.3.4. Geological Setting of the Wodgina Pegmatite District . . . . . . . . . . 106 4. Fieldwork and Sampling of Selected Pegmatites and Pegmatite Fields 115 4.1. Bikita Pegmatite Field . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 115 4.2. Londonderry Pegmatite Field . . . . . . . . . . . . . . . . . . . . . . . . . . . . 115 4.2.1. Londonderry Feldspar Quarry Pegmatite . . . . . . . . . . . . . . . . . 115 4.2.2. Lepidolite Hill Pegmatite . . . . . . . . . . . . . . . . . . . . . . . . . . 117 4.2.3. Tantalite Hill Pegmatite . . . . . . . . . . . . . . . . . . . . . . . . . . . 118 4.3. Mount Deans Pegmatite Field . . . . . . . . . . . . . . . . . . . . . . . . . . . 118 4.3.1. Type I – Flat Lying Pegmatites . . . . . . . . . . . . . . . . . . . . . . . 118 4.3.2. Type II – Steeply Dipping Pegmatites . . . . . . . . . . . . . . . . . . . 120 4.4. Cattlin Creek Pegmatite . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 120 4.5. Wodgina LCT-Pegmatite Deposit . . . . . . . . . . . . . . . . . . . . . . . . . . 121 4.5.1. Mount Tinstone Pegmatite . . . . . . . . . . . . . . . . . . . . . . . . . 123 4.5.2. Mount Cassiterite Pegmatite . . . . . . . . . . . . . . . . . . . . . . . . 123 5. Petrography and Mineralogy 139 5.1. Quantitative Mineralogy by Means of Mineral Liberation Analysis . . . . . . . . 141 5.2. Mineralogical and Petrographical Characteristics of Individual Mineral Groups . 141 5.2.1. Feldspar . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 141 5.2.2. Quartz . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 144 5.2.3. Mica . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 146 5.2.4. Pollucite . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 147 5.2.5. Petalite . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 149 5.2.6. Spodumene . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 149 5.2.7. Beryl . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 154 5.2.8. Tourmaline . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 155 5.2.9. Apatite . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157 5.2.10. Ta-, Nb- and Sn-oxides . . . . . . . . . . . . . . . . . . . . . . . . . . 157 5.3. Reconstruction of the General Crystallisation Sequence . . . . . . . . . . . . . 162 6. Geochemistry 165 6.1. Major Elements . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 165 6.2. Selected Minor and Trace Elements . . . . . . . . . . . . . . . . . . . . . . . . 174 6.3. Fractionation Indicators . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 175 6.4. Rare Earth Elements . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 185 7. Geochronology 193 7.1. 40Ar/39Ar-Method on Mica . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 193 7.1.1. Bikita Pegmatite Field . . . . . . . . . . . . . . . . . . . . . . . . . . . 194 7.1.2. Mount Deans Pegmatite Field . . . . . . . . . . . . . . . . . . . . . . . 195 7.1.3. Londonderry Pegmatite Field . . . . . . . . . . . . . . . . . . . . . . . 195 7.1.4. Cattlin Creek Pegmatite . . . . . . . . . . . . . . . . . . . . . . . . . . 195 7.1.5. Wodgina Pegmatite . . . . . . . . . . . . . . . . . . . . . . . . . . . . 198 7.2. Th-U-Total Pb Monazite Dating . . . . . . . . . . . . . . . . . . . . . . . . . . . 201 7.2.1. Monazite Ages . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 201 7.3. U/Pb Dating of Selected Ta-, Nb- and Sn-Oxide Minerals . . . . . . . . . . . . 203 7.3.1. Bikita Pegmatite Field . . . . . . . . . . . . . . . . . . . . . . . . . . . 203 7.3.2. Londonderry Pegmatite Field . . . . . . . . . . . . . . . . . . . . . . . 203 7.3.3. Mount Deans Pegmatite Field . . . . . . . . . . . . . . . . . . . . . . . 206 7.3.4. Cattlin Creek Pegmatite . . . . . . . . . . . . . . . . . . . . . . . . . . 206 7.3.5. Wodgina Pegmatite . . . . . . . . . . . . . . . . . . . . . . . . . . . . 207 8. Fluid Inclusion Study 211 8.1. Bikita Pegmatite Field . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 211 8.2. Wodgina Pegmatite . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 211 8.3. Carbon Isotope Analysis on Fluid Inclusion Gas of Selected Mineral Phases . . 212 9. Stable and Radiogenic Isotopes 217 9.1. Whole Rock Sm/Nd-Isotopy . . . . . . . . . . . . . . . . . . . . . . . . . . . . 217 9.1.1. New Whole Rock Sm/Nd Data . . . . . . . . . . . . . . . . . . . . . . 217 9.2. Lithium Isotope Analysis on Selected Mineral Phases . . . . . . . . . . . . . . . 220 9.2.1. New Lithium Isotope Data . . . . . . . . . . . . . . . . . . . . . . . . . 220 10.Discussion 227 10.1. Regional Geological and Tectonomagmatic Development . . . . . . . . . . . . 227 10.1.1. Constraints from Field Evidence . . . . . . . . . . . . . . . . . . . . . . 227 10.1.2. Petrographical and Mineralogical Constraints . . . . . . . . . . . . . . 229 10.1.3. Geochemical Constraints . . . . . . . . . . . . . . . . . . . . . . . . . 230 10.1.4. Isotopic Constraints . . . . . . . . . . . . . . . . . . . . . . . . . . . . 232 10.1.5. Constraints from Fluid Inclusion Data . . . . . . . . . . . . . . . . . . . 233 10.1.6. Geochronological Constrains . . . . . . . . . . . . . . . . . . . . . . . 233 10.2. Massive Pollucite Mineralisations . . . . . . . . . . . . . . . . . . . . . . . . . . 243 10.2.1. Unique Characteristics of Massive Pollucite Mineralisations . . . . . . . 243 10.2.2. New Concepts for the Formation of Massive Pollucite Mineralisations . . 252 10.3. Genetic Model for the Formation of Massive Pollucite Mineralisations within LCT Pegmatite Systems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 264 11.Summary and Conclusions 267 References 273 Lists of Abbreviations 309 General Abbreviations . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 309 Mineral Abbreviations . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 310 List of Figures 311 List of Tables 315 Appendix 317 A. Legend for Topographic Maps 319 B. Sample List 323 C. Methodology 331 C.1. Quantitative Mineralogy by Means of Mineral Liberation Analysis . . . . . . . . 331 C.2. Geochemistry . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 331 C.3. 40Ar/39Ar-Method on Mica . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 335 C.4. Th-U-Total Pb Monazite Dating . . . . . . . . . . . . . . . . . . . . . . . . . . . 335 C.5. U/Pb Dating of Selected Ta-, Nb- and Sn-Oxide Minerals . . . . . . . . . . . . 336 C.6. Fluid Inclusion Study . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 337 C.7. Whole Rock Sm/Nd-Isotopy . . . . . . . . . . . . . . . . . . . . . . . . . . . . 338 C.8. Lithium Isotope Analysis on Selected Mineral Phases . . . . . . . . . . . . . . . 338 D. Data – Mineral Liberation Analysis 341 E. Data – Geochemistry 345 F. Data – Geochronology 349 G. Data – Stable and Radiogenic Isotopes 353

Die vorliegende Doktorarbeit präsentiert neue petrologische Untersuchungen an hochgradig metamorphen Gesteinen des Beit Bridge, Mahalapye und Phikwe Komplexes, welche gemeinsam die Central Zone des Limpopo Belt im südlichen Afrika bilden. Die Ergebnisse liefern detaillierte Informationen über die pro- und retrograde Druck-Temperatur-(P-T)-Entwicklung der drei Komplexe und bilden, in Einklang mit geochronologischen Daten, die Grundlage für die Erstellung eines einheitlichen geodynamischen Modells der Bildung der Central Zone des Limpopo Belt. Die abgeleiteten P-T Pfade wurden anhand detaillierter Untersuchungen an quartzgesättigten und - untersättigten Metapeliten bis Metabasiten erstellt, wobei sechs Sillimanit-Granat-Cordierit Gneisse, vier (Granat)- Biotit-Plagioklas Gneisse, zwei Granat-Orthopyroxen-Biotit- Kalifeldspat-Plagioklas Gneisse, ein Granat-Cordierit-Orthoamphibol Fels, ein Granat-Biotit Amphibolit und ein Granat-Klinopyroxen Amphibolit untersucht wurden. PT Punkte und P-T Entwicklungen wurden mit Hilfe von konventionellen Geothermobarometern und quantitativen Phasendiagrammen in den Systemen Na2O - CaO - K2O - FeO - MgO - Al2O3 - SiO2 - H2O - TiO2 - O(NCKFMASHTiO) und MnO - TiO2 - Na2O - CaO - K2O - FeO - MgO - Al2O3 - SiO2 - H2O (MnTiNCKFMASH) berechnet und abgeleitet. Die Phasendiagramme wurden mit den Programmen THERMOCALC und THERIAK-DOMINO berechnet. Petrologische Informationen, speziell solche, die durch den Vergleich von beobeachteten/gemessenen mit thermodynamisch berechneten Mineralparagenesen, -zonierungen, -zusammensetzungen und Modalgehalten erhalten wurden zeigen, in Kombination mit neuen und bereits existierenden geochronologischen Daten, dass Gesteine der drei untersuchten Komplexe geringfügig unterschiedliche P-T Entwicklungen zu verschiedenen Zeiten durchliefen. Proben aus der Gegend des Bulai Plutons (Beit Bridge Komplex) belegen ein hochgradig metamorphes Ereignis im Neoarchaikum um ~2.64 Ga (M2), mit peak-metamorphen Bedingungen von ~850°C/8-9 kbar und einer retrograden Dekompression mit gleichzeitiger Abkühlung zu ~750°C/5-6 kbar. Diese metamorphe Entwicklung erfolgte vermutlich im geodynamischen Umfeld eines Magmatischen Bogens. Im Gegensatz hierzu dokumentieren Proben des Mahalapye und Phikwe Komplexes metamorphe Entwicklungen im Paläoproterozoikum um ~2.03-2.05 Ga (M3), die sich zudem im prograden Verlauf der Metamorphose voneinander unterscheiden. Metamorphe Gesteine des Mahalapye Komplexes kennzeichnet eine Hochtemperatur- Niedrigdruck-(HT-LP)- Metamorphose mit schwacher prograder Dekompression von ~650°C/7 kbar nach ~800°C/5.5 kbar, die mit der Platznahme von ausgedehnten granitischen Intrusionen um ~2.06-2.02 Ga einherging. Metamorphe Gesteine des Phikwe Komplexes hingegen zeigen eine gleichzeitige Druck- und Temperaturzunahme von ~600°C/6 kbar nach ~750°C/8 kbar, die nicht mit Magmatismus im Paläoproterozoikum assoziiert war. Es wird gefolgert, dass die HT-LP metamorphe Entwicklung des Mahalapye Komplexes ihre Ursache in dem magmatischen „Underplating“ heisser mafischer Schmelzen, als Ergebnis südost- erichteter Subduktion während der Kheis-Magondy Orogenese, und/oder der zeitgleichen Aktivität von Mantel Plumes, in Zusammenhang mit der Bildung des Bushveld Komplexes, hat. Im Gegensatz hierzu belegen die Gesteine des Phikwe Komplexes eine prograde Druck- und Temperaturzunahme, hervorgerufen durch eine fortschreitende Krustenstapelung um ~2.03 Ga. Diese Stapelung ist bereits für zahlreiche andere geologischen Einheiten des Limpopo Belt belegt. Sie wird als eine Folge der endenden Annäherung/Kollision zwischen dem Kaapvaal und Zimbabwe Kraton interpretiert, welche durch südost-gerichtete Kompression im Zuge der Kheis-Magondy Orogenese zw. ~2.06 und 1.90 Ga hervorgerufen wurde
This study presents new petrological results obtained from high-grade metamorphic rocks of the Beit Bridge, Mahalapye and Phikwe Complexes, which constitute the Central Zone of the Limpopo Belt in southern Africa. These results provide detailed information about the prograde and retrograde pressure-temperature (P-T) evolution of the three investigated complexes and, in concert with geochronological data, form the basis for the development of a coherent geodynamic model for the evolution of the Limpopo’s Central Zone. The P-T paths were inferred by the thorough investigation of silica-saturated and silica- undersaturated metapelitic and metabasic rocks, comprising six sillimanite-garnet-cordierite gneisses, four (garnet)-biotite-plagioclase gneisses, two garnet-orthopyroxene-biotite-Kfeldspar-plagioclase gneisses, one garnet- cordierite-orthoamphibole fels, one garnet-biotite amphibolite, and one garnet-clinopyroxene amphibolite. P-T points and P-T evolutions were derived by the application of conventional geothermobarometers, and quantitative phase diagrams in the systems Na2O - CaO - K2O - FeO - MgO - Al2O3 - SiO2 - H2O - TiO2 - O (NCKFMASHTiO), and MnO - TiO2 - Na2O - CaO - K2O - FeO - MgO - Al2O3 - SiO2 - H2O (MnTiNCKFMASH) - using the computer software THERMOCALC and THERIAK-DOMINO. The petrological information, in particular those obtained by comparison between observed and thermodynamically calculated mineral assemblages, zonations and modes, in combination with new and existing geochronological data provide evidence that rocks from the three investigated complexes underwent slightly different P-T evolutions at different times. The samples from the Bulai Pluton area (Beit Bridge Complex) provide evidence for a Neoarchean high-grade metamorphic event at ~2.64 Ga (M2), with peak P-T conditions of ~850°C at 8-9 kbar, and a decompression-cooling path to ~750°C at 5-6 kbar. This metamorphic evolution perhaps took place in a magmatic arc setting. In contrast, samples from the Mahalapye and Phikwe Complex document a Palaeoproterozoic event at ~2.03-2.05 Ga (M3), and were subject to different styles of prograde metamorphism. Metamorphic rocks from the Mahalapye Complex experienced a high-temperature low-pressure (HT-LP) metamorphic overprint, accompanied by the emplacement of voluminous granite bodies between 2.06 and 2.02 Ga, and provide evidence for a slightly prograde decompression from ~650°C/7 kbar to ~800°C/5.5 kbar. In contrast, the metamorphic rocks from the Phikwe Complex provide evidence for a simultaneous pressure and temperature increase from ~600°C/6 kbar to ~750°C/8 kbar, in the absence of significant Palaeoproterozoic magmatism. The HT-LP metamorphic evolution of the Mahalapye Complex is interpreted to be initiated by the underplating of hot mafic melts, either formed in response to SE-subduction during the Kheis-Magondi orogeny, and/or by contemporaneous mantle plume activities related to the formation of the Bushveld Complex. In contrast, the prograde pressure and temperature increase reflected by the rocks from the Phikwe Complex rather reflects successive crustal stacking at ~2.03 Ga. This stacking, which is also reported from many other units throughout the Limpopo Belt, is interpreted to result from the final convergence between the Kaapvaal and Zimbabwe Cratons, perhaps caused by SE-directed compression in response to the Kheis-Magondi orogeny between ~2.06 and 1.90 Ga

What tectonic processes were operating in the Archean, and whether they were similar to the “modern-style” plate tectonics seen operating today, is a fundamental question about Archean geology. The Superior Province is the largest piece of preserved Archean crust on Earth. As such it provides an excellent opportunity to study Archean tectonic processes. Much work has been completed in the southern part of the Superior Province. A well-documented series of discrete, southward younging orogenies related to a series of northward dipping subduction zones, has been proposed for amalgamating this part of the Superior Province. The tectonic evolution in the northwestern Superior Province is much less constrained, and it is unclear if it is related to the series of subduction zones in the southern part of the Superior Province, or if it is related to an entirely different process. Such ideas need to be tested in order to develop a concise model for the Meso – and Neoarchean tectonic evolution of the northwestern Superior Province. To this end, a field mapping, U-Pb geochronology, Nd isotope, and lithogeochemistry study was undertaken in the Island Lake greenstone belt. This granite-greenstone belt is part of the northern margin of the North Caribou terrane, a larger reworked Mesoarchean crustal block located in the northwestern Superior Province. U-Pb TIMS zircon geochronology data shows that the Island Lake greenstone belt experienced a long and complex geological history that included the deposition of three distinct volcanic assemblages at ca. 2897 Ma, 2852 Ma, and 2744 Ma, as well as a younger clastic sedimentary group, the Island Lake group. All of these volcanic assemblages include felsic and mafic volcanic rocks, as well as a suite of contemporaneous plutonic rocks. The U-Pb data set shows that the Savage Island shear zone, a regional fault structure that transects the Island Lake greenstone belt, is not a terrane-bounding feature as correlative supracrustal assemblages are observed on both sides of it. The Nd isotope data shows that the volcanic assemblages and contemporaneous plutons have been variably contaminated by an older ca. 3.0 Ga crustal source. The mafic volcanic rocks in the assemblages have two distinct geochemical signatures, and show a pattern of decreasing crustal contamination with decreasing age. Together these data suggests that the Meso – and Neoarchean volcanic assemblages are part of an intact primary volcanic stratigraphy that were built on the same ca. 3.0 Ga basement and have autochthonous relationships with each other. This basement is the North Caribou terrane. The youngest sedimentary group in the belt, the Island Lake group, was deposited between 2712 Ma and 2699 Ma. It consists of “Timiskaming-type” sedimentary rocks, and is the youngest clastic sedimentary package in the belt. A detailed study of detrital zircons in units from the stratigraphic bottom to the top of the sedimentary group indicates an age pattern of detrital zircons that is most consistent with a scenario in which sediments were deposited in inter-diapiric basins created by diapirism and sagduction (i.e., vertical tectonic) processes. During the diapiric ascent of the felsic material, inter-diapiric basins were formed in the synclines between adjacent domes, into which sediments were deposited. U-Pb zircon TIMS geochronology identified two ages of deformation in the Island Lake greenstone belt. Two dykes that crosscut an older, D1 foliation place a minimum age of ca. 2723 Ma on the D1 deformation, and two syn-kinematic dykes date movement along two transpressional shear zones to 2700 Ma. Together all these data indicate that the tectonic evolution in the Island Lake greenstone belt and in the northwestern Superior Province took place in three main stages. The first two stages involved the generation of Meso – and Neoarchean volcanic assemblages and contemporaneous plutonic rocks due to southward dipping subduction under the North Caribou micro-continent. The third stage involved the deposition of late “Timiskaming-type” sediments during vertical tectonic processes in conjunction with horizontal tectonic movement along late transpressional shear zones at ca. 2.70 Ga. At the end of this process the North Superior superterrane was terminally docked to the North Caribou terrane along the North Kenyon fault. This study shows that while a version of horizontal or “modern” style plate tectonics were operating in the Archean, vertical tectonic processes were also occurring and that these processes operated synchronously in the Neoarchean.

Masters dissertation school of Geosciences, University of the Witwatersrand 2017
The aim of this study was to investigate and evaluate the 3D structural architecture around the Vredefort dome in the Witwatersrand basin, in particular the unexposed southern portion. This was done in order to establish strato-tectonic relationships, first order deformation structures, and basement architecture. The outcomes provide a more detailed architecture around the central uplift that may be used in future work aimed at examining the nature of giant terrestrial impacts. In summary, the integration of borehole, surface mapping, and 2D reflection seismic data provides a well constrained 3D geological model of the dome, central uplift, and adjacent areas (covering approximately 11600 km2). Seven structural features are discussed from the 3D modelling results. These include, (1) a normal fault in the lower West Rand Group, (2) an undulate, normal faulted truncation plane, constrained as post-West Rand Group and pre or early-Central Rand Group, (3) a truncation plane and local enhanced uplift constrained as pre to syn-VCF, (4) a listric fault system, constrained as post-Klipriviersberg Group and syn-Platberg Group, (5) a truncation plane, constrained as syn-Black Reef Formation, (6) folds, including a large asymmetric, gentle anticline here named the Vaal Dam Anticline, constrained as post-Magaliesberg Formation and pre-Vredefort impact, and (7) a listric fault across the southeastern margin of the Vredefort dome, constrained as late to post-central uplift formation. The findings support previous work by Tinker et al. (2002), Ivanov (2005), Alexandre et al. (2006), Dankert and Hein (2010), Manzi et al. (2013), Jahn and Riller (2015), and Reimold and Hoffmann (2016). However the findings oppose various parts of previous work by Friese et al. (1995), Henkel and Reimold (1998), and Reimold and Koeberl (2014). A new term is also proposed for the periclinal folds located around the central uplift, i.e., impact-type curvature-accommodation folds. This study demonstrates the importance of integrating multiple sources of data into a single 3D spatial environment in order to better refine and distinguish impact-related deformation from the pre-existing basement architecture.
MT 2017

The provenance of the Neoarchaean Ventersdorp Supergroup and several age-related supracrustal successions was analysed to gain insight into the geotectonic evolution of the Kaapvaal Craton during the transition from the Archaean to Proterozoic Eras. The studied successions include, besides the siliciclastic formations of the Ventersdorp Supergroup, the upper Wolkberg and Buffelsfontein Groups, the Godwan Formation and the Schmidtsdrift Subgroup of the basal Transvaal Supergroup in Griqualand West. Petrographic, whole rock geochemical and Sm-Nd isotopic analyses were combined with SHRIMP U-Pb age dating of detrital zircons. Furthermore, Rb-Sr isotopic studies were carried out on carefully selected suites of samples from surface exposure or, wherever possible, on deep diamond drill core. The Ventersdorp Supergroup is an up to 5 km thick undeformed, only slightly metamorphosed volcano-sedimentary succession deposited on the Kaapvaal Craton between 2714 Ma and 2665 Ma. A lack of major time hiati to the underlying Mesoarchaean Witwatersrand Supergroup and covering Neoarchaean to Palaeoproterozoic Transvaal Supergroup render the Ventersdorp Supergroup very well suited for the investigation of the geotectonic evolution of the Kaapvaal Craton near the Archaean-Proterozoic boundary. This is supported by its excellent preservation, which also allowed detailed studies of sedimentological structures, such as seismites indicating Neoarchaean earthquakes. The provenance analyses carried out on the clastic formations of the Ventersdorp Supergroup point to a gradual change in tectonic evolution from typically Archaean to post-Archaean processes rather than a drastic, unique transition in the case of the Kaapvaal Craton. Texturally immature wackes of the Kameeldoorns Formation, representing the oldest clastic units of the Ventersdorp Supergroup, are derived mainly from Mesoarchaean source rocks, whereas the stratigraphically younger Bothaville Formation displays geochemical signatures comparable with Archaean trondhjemite-tonalite granodiorite-suites (TTGs), thus suggesting crustal addition in the so-called ‘Archaean-style’. The extension of provenance analyses to supracrustal successions that are tentatively correlated with the Bothaville Formation, revealed contributions from granitoid V sources that formed under post-Archaean and Archaean conditions. Furthermore, the geochemical data for all analysed formations support a passive margin setting. Arc settings, as indicated in some samples, are due to the input of less fractionated volcanic material that provides evidence of distal volcanism. Analyses of Nd-isotopic systematics and U-Pb ages of detrital zircons revealed a Mesoarchaean age for the source rocks of the formations. U-Pb age dating of detrital zircons of the Godwan Formation suggests that this formation is of Mesoarchaean age, and therefore not a correlative of the other Neoarchaean successions. Hence, the results suggest that the continental crust of the Kaapvaal Craton was thick enough since the Mesoarchaean (2.8 - 3.1 Ga) to allow long-term crustal recycling, and therefore modern plate tectonic processes could have operated earlier than on other well-studied cratonic blocks. During the Neoarchaean, however, crustal thickening of the Kaapvaal Craton took place by accretion of Archaean-style TTGs along the margins of the craton. Thus, Archaean and post-Archaean tectono-magmatic processes co-existed. Furthermore, the Neoarchaean supracrustal successions represent the first sedimentation events on an entirely stabilised and tectonically quiescent Kaapvaal Craton. Input from distal volcanic sources marks the last sign of volcanic activity prior to the craton-wide deposition of carbonate rocks of the Transvaal Supergroup. Geochronological data also imply a connection of the Neoarchaean Kaapvaal Craton to further cratonic blocks that may hold source rocks for the studied formations, as for some small age populations of older detrital zircons (ca. 3.1 - 3.4 Ga), no suitable source area could be identified on the Kaapvaal Craton itself. However, it seems unlikely that the Zimbabwe Craton was one of these cratonic blocks, because the Rb-Sr whole rock ages of all studied formations yield a model age of 2092 ± 55 Ma, which is thought to correspond to a craton-wide influence of the 2.05 Ga old Bushveld Igneous Complex on the Rb-Sr isotope systematics of all analysed clastic successions. This influence is apparently missing in the Southern and Central Marginal Zones of the Limpopo Belt, suggesting that the collision between the Kaapvaal and Zimbabwe Cratons only took place after the emplacement of the Bushveld Igneous Complex, i.e. after 2.05 Ga.
Dr. U. Zimmermann Prof. J. Gutzmer

The Late Archean Magmatic Event (LAME), ca. 2.7 Ga, was the greatest crustal addition event in Earth history. My focus is the Superior Province of Canada, where LAME occurred ca. 2.75 – 2.65 Ga. Mantle plumes impinged on the Abitibi subprovince, where ~ 16 km regional thickness of tonalite-trondhjemite-granodiorite (TTG) melt was produced. Granites (sensu stricto) were the last magmatic phase of LAME, with a Superior-wide regional thickness of ~ 1 – 3 km. Assuming a crustal source for both TTG and granites, I use 1-D thermal models to investigate the origin of TTG in the Abitibi subprovince and that of late granites in the Superior Province. Melting curves appropriate to the source of TTG and granites are used to determine the thickness of melt produced in the models. I show that the incorporation of upward melt transfer into a standard model of lower crustal melting may increase the amount of predicted melt by ~ 1/(1-f), where f denotes the fraction of melt that is on average being extracted from the source rocks. Partitioning of heat producing elements between melt and restite reduces the amount of melt produced, but the effect is secondary compared to the increase in melt production through upward melt transfer. For the Abitibi subprovince, I show that the emplacement of a single plume coupled with the emplacement of a 12-km-thick greenstone cover can generate a maximum of ~ 9-km-thickness of TTG melt. However, the emplacement of a series of plumes, each coupled with the emplacement of a 3-km-thick greenstone cover and a 10-km-thick sill results in ~ 20-km-thickness of TTG melt. My model incorporates delamination of restitic eclogite. Finally, I show that late granites in the Superior Province may have resulted from thickening of a crust that had been “pre-heated” during earlier arc activity and that prolonged granitic magmatism observed in some areas of the Superior Province may be explained by late underthrusting of fertile source rocks into deeper and hotter regions of the crust.