Dissertations / Theses on the topic 'Yilgarn'

[Truncated abstract] A number of controlled and natural seismic sources are utilised to model the Pwave velocity structure of the southwest of the Yilgarn Craton, Western Australia. The Yilgarn Craton is one of the largest pieces of Archaean crust in the world and is known for its gold and nickel deposits in the east and intraplate seismicity in the west. The aim of the project is to link 2D and 3D models of variations in seismic velocity with the local seismicity and geology. A new set of seismic refraction data, acquired in 25 overlapping deployments between 2002 and 2005, has been processed, picked and analysed using forward modelling. The data comprise two perpendicular traverses of three-component recordings of various delay-fired blasts from local commercial quarries. The data were processed using a variety of techniques. Tests were carried out on a number of data enhancement and picking procedures in order to determine the best method for enhancement of delay-fired data. A new method for automatic phase recognition is presented, where the maximum of the derivative of the rectilinearity of a trace is taken as the first break. Complete shot gathers with first break picks for each seismic source are compiled from the overlapping deployments. ... The starting 3D model was based on the models produced by 2D forward modelling. 14 iterations were carried out and the best-fit 3D model was achieved at the 10th iteration. It is 35% better then the current model used to locate earthquakes in this region. The resultant velocity block model was used to iii construct a density block model. A relative gravity map of the southwest of Yilgarn Craton was made. The results of 2D forward modelling, 3D tomography and forward gravity modelling have been compared and it was found that the HVZ is present in all models. Such a zone has been previously seen on a single seismic refraction profile, but it is the first time, this zone has been mapped in 3D. The gravity high produced by the zone coincides with the gravity high observed in reality. There is strong evidence that suggests that the HVZ forms part of the Archaean terrane boundary within the Yilgarn Craton. The distribution of the local seismicity was then discussed in the framework of the new 3D velocity model. A hypothesis, that the primary control on the seismicity in the study area is rotation of the major horizontal stress orientation, is presented. It is also argued that the secondary control on seismicity in the SWSZ is accommodation of movements along major faults.

[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.

This PhD study reports the discovery of three previously unknown mafic dyke swarms in the Yilgarn Craton in Western Australia and the first precise age for a mafic dyke swarm in East Antarctica. These ages fall in key periods of supercontinent cycle between the Neoarchean and the Mesoproterozoic, and make an important contribution to the global database of mafic dykes and Large Igneous Provinces.

4D evolutionary models of ore deposits can be generated by combining multiple geological techniques, including geochronology and isotopic geochemistry, constraining all geological processes within a mineral system. This thesis applies this method to two replacement-type volcanic hosted massive sulphide deposits in the Yilgarn Craton, demonstrating the syn-volcanic nature of the Nimbus deposit, the relationship between the Teutonic Bore camp and the Penzance granite, and proposing tracking of seawater paleo-chemistry for exploration of sedimentary sequences.

Thesis (Ph. D.)--Dept. of Geology and Geophysics, University of Adelaide, 1992.
Typescript (Photocopy). Includes copies of 4 papers by the author as appendix 4 (v. 1). Errata slip inserted. Includes bibliographical references (leaves 170-192 (v. 1)).

Red-brown hardpan occurs extensively in Western Australia in the arid and semi-arid regions of the Murchison, Pilbara and Eastern Goldfields divisions, between longitudes 115ºE and 124ºE and latitudes 23ºs and 30ºs. It occupies an area of about 360,000 sq. km, two thirds of which occurs in the Yilgarn Craton. The purpose of this research is to map the distribution of red-brown hardpan in the Yilgarn Craton of Western Australia; study the relationship between landscape, soil texture and vegetation; investigate the physical characteristics, petrology, mineralogy, geochemistry and cementing agents; and thereby determine the processes invaded in forming red-brown hardpan. The relation of red-brown hardpan to gold is investigated and determined its implications in mineral exploration. The main case study areas were the Goldfields Gas Pipe Line, the Federal Open Pit Gold mines and the Menzies district in the Kalgoorlie-Menzies region of the Eastern Goldfields; areas in and around the Woolgorong Station in the Murchison Province and at the Wiluna Gold Mines in the Northeastern Goldfields. The findings and conclusions of this research are summarised below. Red-brown hardpan occurs at or near the land surface and may vary from less than one metre to more than 10 m thick. It is exclusively developed in colluvium and alluvium, showing varying stages of cementation ranging from weakly cemented through moderate to strongly cemented. In addition, calcrete and red-brown hardpan occurs together in many places, south of the Menzies line, and this distribution suggests that red-brown hardpan was once more extensive and has been subsequently replaced by carbonate to form calcareous red-brown hardpan and calcrete. Red- brown hardpan predominantly occurs in regions with Q50 mm annual rainfall.In present-day higher rainfall (400 to 500 mm) regions, red-brown hardpan is being weathered. There is no relationship between the distribution of mulga (Acacia aneura) and red-brown hardpan. Red-brown hardpan is exclusively developed in colluvium containing a minimum of 20% quartz, 15% clays and 2% iron oxides. It is bright reddish brown to reddish brown, earthy, with a sandy loam texture, blocky structure and porous. Red-brown hardpan is hard (up to 12 MPa), being characterised by sub-horizontal laminations predominantly of uncemented kaolinite. Ped surfaces may be coated by Mn oxide and carbonate which may be precipitated along the laminations. The mineralogy of the cement is complex. Data from XRD, SEM, TEM, EFTEM, FTIR and NIR investigations show poorly-ordered kaolinite and opal-A as the main components. Illuvial multilayered argillaceous cutans containing silica and alumina in a ratio of 2:l form the cement. Secondary silica (SiO2-95%) coatings are common, mainly as opal-A, on ped surfaces and on the inner walls of voids and vughs. Etch pits are developed in these coatings and some of them are filled by kaolinitic clays. Selective dissolution experiments using acid ammonium oxalate show that oxalate- soluble amorphous and poorly ordered silica and alumina in red-brown hardpan have molar ratios of about 1.6 to 2 A1203:SiO2.These results suggest that red-brown hardpans were formed where there was sufficient water during the wet season to dissolve alumina and silica, but insufficient to leach them. During the subsequent dry season, the dissolved alumina and silica was precipitated as poorly-ordered kaolinite and opal-A. Successive dissolution and precipitation led to fusion of poorly-ordered kaolinite and opal-A at a nanometre scale to progressively cement the colluvium. The age of the red-brown hardpans, estimated by paleomagnetic dating of hematite, is from Pleistocene to present. Based on the findings of this research, the red-brown hardpan is redefined and primarily classified on its degree of cementation as: (1) weakly cemented, (2) moderately cemented and (3) strongly cemented. It is further classified chemically into: (1) siliceous, (2) calcareous and (3) ferruginous. In the Yilgarn Craton, red-brown hardpan is believed to occur mainly north of the 'Menzies Line'. However, this study reveals the presence of red-brown hardpan 75- 150 km south of the Menzies Line and the new southern boundary is closer to latitude 29ºs. Geochemical investigation at the Federal Open Pit Gold mines, Broad Arrow, north of Kalgoorlie indicate that there are Au anomalies in red-brown hardpan. Gold concentration is up to 50 ppb against the background anomaly of 10 ppb. Sequential and partial extraction analyses show significant correlation of Au with Ag, Ca, Ce, Co, Mg, Mn and Ni. This suggests that the Au concentration in red-brown hardpan is due to: (a) mechanical dispersion due to reworking of Au-bearing clasts in the sediment and (b) hydromorphic dispersion from the underlying mineralisation. It can therefore be used as a useful sampling medium for gold exploration.

Red-brown hardpan occurs extensively in Western Australia in the arid and semi-arid regions of the Murchison, Pilbara and Eastern Goldfields divisions, between longitudes 115ºE and 124ºE and latitudes 23ºs and 30ºs. It occupies an area of about 360,000 sq. km, two thirds of which occurs in the Yilgarn Craton. The purpose of this research is to map the distribution of red-brown hardpan in the Yilgarn Craton of Western Australia; study the relationship between landscape, soil texture and vegetation; investigate the physical characteristics, petrology, mineralogy, geochemistry and cementing agents; and thereby determine the processes invaded in forming red-brown hardpan. The relation of red-brown hardpan to gold is investigated and determined its implications in mineral exploration. The main case study areas were the Goldfields Gas Pipe Line, the Federal Open Pit Gold mines and the Menzies district in the Kalgoorlie-Menzies region of the Eastern Goldfields; areas in and around the Woolgorong Station in the Murchison Province and at the Wiluna Gold Mines in the Northeastern Goldfields. The findings and conclusions of this research are summarised below. Red-brown hardpan occurs at or near the land surface and may vary from less than one metre to more than 10 m thick. It is exclusively developed in colluvium and alluvium, showing varying stages of cementation ranging from weakly cemented through moderate to strongly cemented. In addition, calcrete and red-brown hardpan occurs together in many places, south of the Menzies line, and this distribution suggests that red-brown hardpan was once more extensive and has been subsequently replaced by carbonate to form calcareous red-brown hardpan and calcrete. Red- brown hardpan predominantly occurs in regions with Q50 mm annual rainfall.
In present-day higher rainfall (400 to 500 mm) regions, red-brown hardpan is being weathered. There is no relationship between the distribution of mulga (Acacia aneura) and red-brown hardpan. Red-brown hardpan is exclusively developed in colluvium containing a minimum of 20% quartz, 15% clays and 2% iron oxides. It is bright reddish brown to reddish brown, earthy, with a sandy loam texture, blocky structure and porous. Red-brown hardpan is hard (up to 12 MPa), being characterised by sub-horizontal laminations predominantly of uncemented kaolinite. Ped surfaces may be coated by Mn oxide and carbonate which may be precipitated along the laminations. The mineralogy of the cement is complex. Data from XRD, SEM, TEM, EFTEM, FTIR and NIR investigations show poorly-ordered kaolinite and opal-A as the main components. Illuvial multilayered argillaceous cutans containing silica and alumina in a ratio of 2:l form the cement. Secondary silica (SiO2-95%) coatings are common, mainly as opal-A, on ped surfaces and on the inner walls of voids and vughs. Etch pits are developed in these coatings and some of them are filled by kaolinitic clays. Selective dissolution experiments using acid ammonium oxalate show that oxalate- soluble amorphous and poorly ordered silica and alumina in red-brown hardpan have molar ratios of about 1.6 to 2 A1203:SiO2.
These results suggest that red-brown hardpans were formed where there was sufficient water during the wet season to dissolve alumina and silica, but insufficient to leach them. During the subsequent dry season, the dissolved alumina and silica was precipitated as poorly-ordered kaolinite and opal-A. Successive dissolution and precipitation led to fusion of poorly-ordered kaolinite and opal-A at a nanometre scale to progressively cement the colluvium. The age of the red-brown hardpans, estimated by paleomagnetic dating of hematite, is from Pleistocene to present. Based on the findings of this research, the red-brown hardpan is redefined and primarily classified on its degree of cementation as: (1) weakly cemented, (2) moderately cemented and (3) strongly cemented. It is further classified chemically into: (1) siliceous, (2) calcareous and (3) ferruginous. In the Yilgarn Craton, red-brown hardpan is believed to occur mainly north of the 'Menzies Line'. However, this study reveals the presence of red-brown hardpan 75- 150 km south of the Menzies Line and the new southern boundary is closer to latitude 29ºs. Geochemical investigation at the Federal Open Pit Gold mines, Broad Arrow, north of Kalgoorlie indicate that there are Au anomalies in red-brown hardpan. Gold concentration is up to 50 ppb against the background anomaly of 10 ppb. Sequential and partial extraction analyses show significant correlation of Au with Ag, Ca, Ce, Co, Mg, Mn and Ni. This suggests that the Au concentration in red-brown hardpan is due to: (a) mechanical dispersion due to reworking of Au-bearing clasts in the sediment and (b) hydromorphic dispersion from the underlying mineralisation. It can therefore be used as a useful sampling medium for gold exploration.

This study presents an investigation of detrital, metamorphic, and hydrothermal minerals from siliciclastic metasedimentary rocks of the Illaara and Maynard Hills greenstone belts, central Yilgarn Craton. This research assesses how 4.3 to 3.0 Ga detrital zircon populations came to be found in dispersed metasedimentary rocks, how these rock occurrences relate to each other and what this may reveal about the early Earth and the formation of the Yilgarn Craton.

[Truncated abstract] The Laverton Greenstone Belt (LGB), located in the northeastern part of the Eastern Goldfields Province (EGP) of the Yilgarn Craton, Western Australia, has a total contained gold endowment of over 690t. An important feature of the gold deposits in the LGB is their close spatial association with granitoids, with many gold deposits located adjacent to, or hosted by, granitoids. Recently-proposed genetic models for Archaean orogenic gold deposits have emphasised the role of granitoids in the formation of ore-deposits, but differ significantly in the nature of that role. Some models suggest that the granitoids are a source of ore-fluids and solutes, whereas others suggest that granitoids exert an important structural control on gold mineralisation. Such competing genetic models for gold mineralisation variably propose either a proximal-magmatic or distal-metamorphic, or less commonly distal-magmatic, source for goldbearing fluids, or mixing of fluids from multiple sources. Isotope geochemistry and geochronological studies are used to constrain the source and timing of auriferous fluids at nine gold deposits in the LGB in an attempt to differentiate between conflicting genetic models. To overcome the lack of detailed deposit-scale geological constraints inherent to any regional study, hypotheses generated from regional datasets are tested in a detailed case-study of the Wallaby gold deposit. The Pb-isotope compositions of ore-related sulphides from deposits in the LGB plot along the line representing crustal-Pb in the Norseman-Wiluna Belt of the EGP, with individual deposits clustering with other nearby deposits based on their geographic location. This trend is similar to that recorded in the Kalgoorlie-Norseman region in the southern EGP, and is consistent with a basement Pb reservoir for gold-bearing fluids. As such, data are consistent with a similar fluid source for all gold deposits. The Nd and Sr isotopic composition of goldrelated scheelite in the LGB clusters very tightly. The inferred ore-fluid composition has a slightly positive εNd, similar to ore fluids at other gold deposits in the EGP for which a proximal magmatic source is highly improbable. As such, Sr and Nd data are consistent with a similar fluid source for the gold deposits analysed in the LGB, but cannot unequivocally define that source. The median S, C and O isotopic compositions of ore minerals from all nine different gold deposits studied in the LGB fall in a very narrow range

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.

Two groups of mafic volcanic rocks and three types of granitoids have been identified in the Yalgoo area of Western Australia. Granodiorite records ages of ~2760 Ma and biotite monzogranite ages of 2636 Ma. A 1.85 Ga dolerite dyke is the first Paleoproterozoic dyke identified from the Yilgarn Craton. An indirect age of ~2.63 Ga is inferred for gold mineralization. Geochemical data indicate formation in a continental marginal arc with traces of Hadean crust.

Common implementations of geostatistical methods, kriging and simulation, ignore the fact that geochemical data are usually reported in weight percent, sum to a constant, and are thus compositional in nature. The constant sum implies that rescaling has occurred and this can be shown to produce spurious correlations. Compositional geostatistics is an approach developed to ensure that the constant sum constraint is respected in estimation while removing dependencies on the spurious correlations. This study tests the applicability of this method against the commonly implemented ordinary cokriging method. The sample data are production blast cuttings analyses drawn from a producing iron ore mine in Western Australia. Previous studies using the high spatial density blast hole data and compositional geostatistical approach returned encouraging results, results other practitioners suggested were due to the high spatial density. This assertion is tested through sub-sampling of the initial data to create four subsets of successively lower spatial densities representing densities, spacings, and orientations typical of the different stages of mine development. The same compositional geostatistical approach was then applied to the subsets using jack-knifing to produce estimates at the removed data locations. Although other compositional geostatistical solutions are available, the additive logratio (alr) approach used in this study is the simplest to implement using commercially available software. The advantages of the logratio methodology are the removal of the constant sum constraint, allowing the resulting quantities to range freely within the real space and, importantly, the use of many proven statistical and geostatistical methods. The back transformation of linear combinations of these quantities and associated estimation variances to the constrained sample space is known to be biased; this study used numerical integration by Gauss-Hermite quadrature to overcome this drawback. The Aitchison and Euclidean distances were used to quantify both the univariate and compositional errors between the estimates and original sample values from each estimation method. The errors of each method are analysed using common descriptive and graphical criteria including the standardised residual sum of squares and an assessment of the accuracy and precision. The highest spatial density dataset is equally well reproduced by either method. The compositional method is generally more accurate and precise than the conventional method. In general the compositional error analyses favour the compositional techniques, producing more geologically plausible results, and which sum to the required value. The results support the application of the logratio compositional methodology to low spatial density data over the commonly implemented ordinary cokriging.

The Comet Gold Mine is in the Murchison mineral field which lies within the Yilgarn Craton of Western Australia. Several different geophysical methods were used in this study to define the geophysical signatures of sedimentary iron formations (SIF) and altered basalt associated with gold mineralisation. The geophysical surveys carried out at the Comet Gold Mine were gravity, sub-audio magnetics (SAM), transient electromagnetics (TEM) and downhole geophysical logging. Data from previous geophysical surveying were also used, and these included highresolution aeromagnetics and TEMPEST airborne electromagnetics. Other exploration information, such as geology and drillhole data, were integrated with geophysical results to study the geophysical responses and generate a geophysical interpretation map.The main aim of this study was to generate an understanding of the various geophysical responses of geology and gold mineralisation in the Comet Mine area for future gold exploration in this region. Particularly, the study focused on the ability of the SAM method to map out geology and geophysical response for gold mineralisation. The response from SAM surveying has been investigated over an area of 13 sq kms. The SAM surveying was completed using a transmitter current of 5-8 Amp with a 50% duty cycle at 4 Hz frequency, which was considered the best setting for the Comet area. The SAM anomalies were compared to results from other geophysical methods. The results of all geophysical surveying suggested that the TEM method was also effective for identifying altered sulphide and magnetic altered rock associated with gold mineralisation.Experiments were carried out using SAM surveying with electrodes in standard surface pits and pits placed directly into the gold mineralised structure. Both surveys showed very similar results, so in this area, surface electrode pits work well for current injection during SAM surveys. The similarities are probably due to the lack of conductive regolith cover in the Comet Mine area.The SAM response was studied for survey grids using different electrode positions and directions. Experiments in changing SAM electrode position over the same area were carried out along and across geological strike to detect the different geological structure directions. The EQMMR response was different for electrodes oriented at 90º when surveys were repeated over the same area. SAM mainly measures conductive features running sub-parallel to the electrode direction, but the EQMMIP response was mostly the same, despite the difference in electrode direction. In addition, the EQMMIP result was very similar for rotated grids, with some distortion occurring around the main EQMMR anomaly near the Venus open cut pit. Therefore, SAM chargeability was not strongly polarised along the electrode direction like the EQMMR response. This is consistent with the theory of MIP that the method detects the effect of induced polarisation in the earth by virtue of the magnetic fields associated with current flow in polarisable bodies within the earth.Gravity data were collected along in 4 transects 500 m apart and at 50 m station spacing. 3D gravity modelling using polygonal shapes was completed to a good fit with felsic and mafic rocks by having rock units dip to the SE. Euler depth solution calculations were applied to locate contacts and deep gravity sources. Gravity surveying has also proved to be a useful survey method for geological mapping and locating regional structures.Ground TEM survey data were used at the Venus prospect to map out conductive zones at depths ranging from 30 to 90 m. All anomaly bodies were interpreted to have a SE dip. The modelled ground TEM results were compared to TEMPEST airborne electromagnetic conductivity depth slices. Both EM survey results showed reasonably similar patterns, but the ground TEM method provided more reliable conductor locations and depth estimations that correlated well with the drilling information and downhole conductivity logging.Geophysical logs of natural gamma and inductive conductivity were surveyed in 5 drillholes that intersected gold alteration zones. The alteration zones associated with gold mineralised sediments, sulphide and magnetic minerals were identified in the downhole logs as increased conductivity, with a sight increase in the natural gamma response. Natural gamma was usually high above a background of host rock in the gold mineralised shear zones. This was likely due to K associated with the clay rich SIF units, and sericite and biotite from gold related alteration. During this study, drillhole CTRC028 was drilled into a modelled TEM anomaly, and gold mineralised SIF was intersected at the predicted location from the model.Geophysical survey information (magnetics, gravity, SAM and TEM) and anomalies in the Comet area were found to be primarily controlled by the local structures and mineralisation along these structures. Modelled ground TEM results were compared to TEMPEST airborne, EM data and showed reasonably similar patterns. The geophysical survey data also highlights black shale units, which can produce a false target commonly running parallel to the sulphide altered fault zones and SIF units, because of graphite and sulphide in the black shale.The TEMPEST data were a valuable guide to bedrock conductivity over the outline project area at Comet, and the follow–up ground TEM and SAM survey data was very useful for accurately pin-pointing anomalies for drill testing.Geophysical and geological data analysed in this study was used to generate a geophysical interpretation map at 1:5,000 scale. The new interpretation of geological units and structures at Comet will provide geologists with a better understand about the geological and structural setting for mineralisation in the Comet area. For example, the Comet Fault represents a faulted limb of the Comet fold structure that has both limbs dipping to the SE, and plunges to the NE. Magnetic anomalies associated with SIF are considered to correlate with some gold bearing horizons and the location of the Comet Fault, that has become more siliceous and altered by sulphide minerals and magnetite minerals.It is recommended that other prospect areas in the region should be surveyed using the SAM method in order to identify shallow gold bearing structures and improve geological interpretations ahead of drilling.

Geologically-constrained inversion of geophysical data is a powerful method for predicting geology beneath cover. The process seeks 3D physical property models that are consistent with the geology and explain measured geophysical responses. The recovered models can guide mineral explorers to prospective host rocks, structures, alteration and mineralisation. This thesis provides a comprehensive analysis of how the University of British Columbia Geophysical Inversion Facility (UBC–GIF) gravity and magnetic inversions can be applied to subsurface mapping and exploration by demonstrating the necessary approach, data types, and typical results. The non-uniqueness of inversion demands that geological information be included. Commonly available geological data, including structural and physical property measurements, mapping, drilling, and 3D interpretations, can be translated into appropriate inversion constraints using tools developed herein. Surface information provides the greatest improvement in the reliability of recovered models; drilling information enhances resolution at depth. The process used to prepare inversions is as important as the geological constraints themselves. Use of a systematic workflow, as developed in this study, minimises any introduced ambiguity. Key steps include defining the problem, preparing the data, setting inversion parameters and developing geological constraints. Once reliable physical property models are recovered they must be interpreted in a geological context. Where alteration and mineralisation occupy significant volumes, the mineralogy associated with the physical properties can be identified; otherwise a lithological classification of the properties can be applied. This approach is used to develop predictive 3D lithological maps from geologically-constrained gravity and magnetic inversions at several scales in the Agnew-Wiluna greenstone belt in Australia’s Yilgarn Craton. These maps indicate a spatial correlation between thick mafic-ultramafic rock packages and gold deposit locations, suggesting a shared structural control. The maps also identify structural geometries and relationships consistent with the published regional tectonic framework. Geophysical inversion provides a framework into which geological and geophysical data sets can be integrated to produce a holistic prediction of the subsurface. The best possible result is one that cannot be dismissed as inconsistent with some piece of geological knowledge. Such a model can only be recovered by including all available geological knowledge using a consistent workflow process.

The Kalgoorlie Terrane of the Yilgarn Craton, Western Australia, containing about 60% (~11 Mt) of the world’s known komatiite-hosted nickel sulphide resources, is the world’s best studied and economically most important province for this mineral deposit type. Although increasingly mature in terms of nickel exploration, the Kalgoorlie Terrane is believed to contain significant additional undiscovered nickel endowment. Using the data-rich Kalgoorlie Terrane, this thesis develops a benchmark methodology that combines geological knowledge with spatial analysis and mathematical-statistical methods to estimate undiscovered nickel resources.In the proposed methodology, nickel sulphide deposits are considered realisations of stochastic mineralisation processes and are analysed within the following framework. Komatiites in the Kalgoorlie Terrane constitute the full sample space or the permissive tract. Disjoint, naturally bound individual komatiite bodies that make up the sample space are used as the spatial analysis units. Some komatiite bodies within the sample space contain nickel sulphide deposits (mineralised) and others do not (unmineralised). In this study, the most explored mineralised komatiite bodies constitute local control areas against which nickel resources in the less explored komatiite bodies can be assessed. The concept of local control areas is analogous to the concept of global control areas which are well explored parts of permissive areas for particular deposit types worldwide.Spatial point pattern analyses showed that the spatial distribution of mineralised komatiite bodies within the sample space is clustered. In contrast, nickel sulphide deposits in individual komatiite bodies are either randomly distributed or dispersed, and not clustered. This absence of deposit clustering within individual komatiite bodies indicates that the intensity of the deposit pattern of each komatiite body may be adequately expressed as deposit density (number of deposits per km[superscript]2). In global quantitative resource assessments, regression analysis of the well established power law relationship between deposit density and size of global control areas provides a robust method for estimating the number of deposits.In this study a power law relationship reminiscent of that in global models was found between the sizes of control areas and deposit density. In addition, this study establishes another power law relationship between nickel endowment density (nickel metal per km[superscript]2) and the sizes of control areas. Deposit and endowment density regression models based on the two power laws suggested that, respectively, 59 to 210 (mean 114) nickel sulphide deposits and 3.0 to 10.0 Mt (mean 5.5 Mt) nickel metal remained undiscovered in demonstrably mineralised komatiite bodies within the Kalgoorlie Terrane. More emphasis is placed on endowment density which may be more intrinsic to the Kalgoorlie Terrane than deposit density because deposit counts are confounded by definitional ambiguities emanating from orebody complexities. Thus the spatial pattern of mineral deposits may not coincide with the spatial pattern of mineral endowment as demonstrated by spatial centrographic analyses in this study.To estimate the amount of undiscovered nickel metal in the entire Kalgoorlie Terrane and not just in the demonstrably mineralised komatiite bodies, Zipf’s law was applied. According to Zipf’s law, the size of the largest deposit is twice the size of the second, thrice the size of the third, four times the fourth, and so on. Based on the currently known size of Mt. Keith deposit, the largest nickel sulphide deposit in the Kalgoorlie Terrane, Zipf’s law indicates that the terrane is nearly mature in terms of nickel exploration and contains only about 3.0 Mt nickel metal in undiscovered resources. The collective implication of the regression and Zipf’s law estimates is that in the Kalgoorlie Terrane, no significant nickel resources are likely to be contained in the known komatiites that are presently not demonstrably mineralised. However if, as widely speculated, the actual size of Mt. Keith deposit is about twice the currently known size, Zipf’s law predicts 10.0 Mt nickel metal in undiscovered nickel endowment for the Kalgoorlie Terrane. The additional 7.0 Mt undiscovered nickel metal endowment is attributed to opening up of a new exploration search space through deeper resource delineation, within an otherwise nearly mature terrane.

[Formulae and special characters can only be approximated here. Please see the pdf version of the abstract for an accurate reproduction.] The formation of world-class Archean orogenic gold deposits in the Eastern Goldfields Province of Western Australia was the result of a critical combination of physical and chemical processes that modified a single and widespread ore-fluid along fluid pathways and at the sites of gold deposition. Increased gold endowment in these deposits is associated with efficient regional-scale fluid focusing mechanisms and the influence of multiple ore-depositional processes at the deposit-scale. Measurement of the complexity of geologic features, as displayed in high-quality geologic maps of uniform data density, can be used to highlight areas that influence regional-scale hydrothermal fluid flow. Useful measurements of geological complexity include fractal dimensions of map patterns, density and orientation of faults and lithologic contacts, and proportions of rock types. Fractal dimensions of map patterns of lithologic contacts and faults highlight complexity gradients. Steep complexity gradients, between domains of high and low fractal dimensions within a greenstone belt, correspond to district-scale regions that have the potential to focus the flow of large volumes of hydrothermal fluid, which is critical for the formation of significant orogenic gold mineralization. Steep complexity gradients commonly occur in greenstone belts where thick sedimentary units overly more complex patterns of lithologic contacts, associated with mafic intrusive and mafic volcanic units. The sedimentary units in these areas potentially acted as seals to the hydrothermal Mineral Systems, which resulted in fluid-pressure gradients and increased fluid flow. The largest gold deposits in the Kalgoorlie Terrane and the Laverton Tectonic Zone occur at steep complexity gradients adjacent to thick sedimentary units, indicating the significance of these structural settings to gold endowment. Complexity gradients, as displayed in surface map patterns, are an indication of three-dimensional connectivity along fluid pathways, between fluid source areas and deposit locations. Systematic changes in the orientation of crustal-scale shear zones are also significant and measurable map features. The largest gold deposits along the Bardoc Tectonic Zone and Boulder-Lefroy Shear Zone, in the Eastern Goldfields Province, occur where there are counter-clockwise changes in shear zone orientation, compared to the average orientation of the shear zone along its entire length. Sinistral movement along these shear zones resulted in the formation of district-scale dilational jogs and focused hydrothermal fluid-flow at the Golden Mile, New Celebration and Victory-Defiance deposits. Faults and lithologic contacts are the dominant fluid pathways in orogenic gold Mineral Systems, and measurements of the density of faults and contacts are also a method of quantifying the complexity of geologic map patterns on high-quality maps. Significantly higher densities of pathways in areas surrounding larger gold deposits are measurable within 20- and 5-kilometer search radii around them. Large variations in the sulfur isotopic composition of ore-related pyrites in orogenic gold deposits in the Eastern Goldfields Province are the result of different golddepositional mechanisms and the in-situ oxidation of a primary ore fluid in specific structural settings. Phase separation and wall-rock carbonation are potentially the most common mechanisms of ore-fluid oxidation and gold precipitation. The influence of multiple gold-depositional mechanisms increases the potential for significant ore-fluid oxidation, and more importantly, provides an effective means of increasing gold endowment. This explains the occurrence of negative δ34S values in ore-related pyrites in some world-class orogenic gold deposits. Sulfur isotopic compositions alone cannot uniquely define potential gold endowment. However, in combination with structural, hydrothermal alteration and fluid inclusion studies that also seek to identify multiple ore-forming processes, they can be a useful indicator. The structural setting of a deposit is also a potentially important factor controlling ore-fluid oxidation and the distribution of δ34S values in ore-related pyrites. At Victory-Defiance, the occurrence of negative δ34S(py) values in gently-dipping dilational structures, compared to more positive δ34S(py) values in steeply-dipping compressional structures, is potentially associated with different gold-depositional mechanisms that developed as a result of fluid-pressure fluctuations during different stages of the fault-valve cycle. During the pre-failure stage, when fluids are discharging from faults, fluid-rock interaction is the dominant gold-depositional mechanism. Phase separation and back-mixing of modified ore-fluid components are dominant during and immediately after faulting. Under appropriate conditions, any, or all, of these three mechanisms can oxidize orogenic gold fluids and cause gold deposition. The influence of multiple gold-depositional mechanisms during fault-valve cycles at dilational jogs, where fluid pressure fluctuations are interpreted to be most severe, can potentially explain both the large gold endowment of the giant to world-class Golden Mile, New Celebration and Victory-Defiance deposits along the Boulder-Lefroy Shear Zone, and the presence of gold-related pyrites with negative δ34S values in these deposits. This study highlights the interplay that exists between physical and chemical processes in orogenic gold Mineral Systems, during the transport of ore fluids in pathways from original fluid reservoirs to deposit sites. Potentially, a single and widespread orogenic ore-fluid could become oxidized, and lead to the formation of ore-related sulfides with variable sulfur isotopic compositions, depending on the nature and orientation of major fluid pathways, the nature of wall-rocks through which it circulates, and the precise ore-depositional processes that develop during fault-valve cycles.

The Comet Gold Mine is in the Murchison mineral field which lies within the Yilgarn Craton of Western Australia. Several different geophysical methods were used in this study to define the geophysical signatures of sedimentary iron formations (SIF) and altered basalt associated with gold mineralisation. The geophysical surveys carried out at the Comet Gold Mine were gravity, sub-audio magnetics (SAM), transient electromagnetics (TEM) and downhole geophysical logging. Data from previous geophysical surveying were also used, and these included highresolution aeromagnetics and TEMPEST airborne electromagnetics. Other exploration information, such as geology and drillhole data, were integrated with geophysical results to study the geophysical responses and generate a geophysical interpretation map.
The main aim of this study was to generate an understanding of the various geophysical responses of geology and gold mineralisation in the Comet Mine area for future gold exploration in this region. Particularly, the study focused on the ability of the SAM method to map out geology and geophysical response for gold mineralisation. The response from SAM surveying has been investigated over an area of 13 sq kms. The SAM surveying was completed using a transmitter current of 5-8 Amp with a 50% duty cycle at 4 Hz frequency, which was considered the best setting for the Comet area. The SAM anomalies were compared to results from other geophysical methods. The results of all geophysical surveying suggested that the TEM method was also effective for identifying altered sulphide and magnetic altered rock associated with gold mineralisation.
Experiments were carried out using SAM surveying with electrodes in standard surface pits and pits placed directly into the gold mineralised structure. Both surveys showed very similar results, so in this area, surface electrode pits work well for current injection during SAM surveys. The similarities are probably due to the lack of conductive regolith cover in the Comet Mine area.
The SAM response was studied for survey grids using different electrode positions and directions. Experiments in changing SAM electrode position over the same area were carried out along and across geological strike to detect the different geological structure directions. The EQMMR response was different for electrodes oriented at 90º when surveys were repeated over the same area. SAM mainly measures conductive features running sub-parallel to the electrode direction, but the EQMMIP response was mostly the same, despite the difference in electrode direction. In addition, the EQMMIP result was very similar for rotated grids, with some distortion occurring around the main EQMMR anomaly near the Venus open cut pit. Therefore, SAM chargeability was not strongly polarised along the electrode direction like the EQMMR response. This is consistent with the theory of MIP that the method detects the effect of induced polarisation in the earth by virtue of the magnetic fields associated with current flow in polarisable bodies within the earth.
Gravity data were collected along in 4 transects 500 m apart and at 50 m station spacing. 3D gravity modelling using polygonal shapes was completed to a good fit with felsic and mafic rocks by having rock units dip to the SE. Euler depth solution calculations were applied to locate contacts and deep gravity sources. Gravity surveying has also proved to be a useful survey method for geological mapping and locating regional structures.
Ground TEM survey data were used at the Venus prospect to map out conductive zones at depths ranging from 30 to 90 m. All anomaly bodies were interpreted to have a SE dip. The modelled ground TEM results were compared to TEMPEST airborne electromagnetic conductivity depth slices. Both EM survey results showed reasonably similar patterns, but the ground TEM method provided more reliable conductor locations and depth estimations that correlated well with the drilling information and downhole conductivity logging.
Geophysical logs of natural gamma and inductive conductivity were surveyed in 5 drillholes that intersected gold alteration zones. The alteration zones associated with gold mineralised sediments, sulphide and magnetic minerals were identified in the downhole logs as increased conductivity, with a sight increase in the natural gamma response. Natural gamma was usually high above a background of host rock in the gold mineralised shear zones. This was likely due to K associated with the clay rich SIF units, and sericite and biotite from gold related alteration. During this study, drillhole CTRC028 was drilled into a modelled TEM anomaly, and gold mineralised SIF was intersected at the predicted location from the model.
Geophysical survey information (magnetics, gravity, SAM and TEM) and anomalies in the Comet area were found to be primarily controlled by the local structures and mineralisation along these structures. Modelled ground TEM results were compared to TEMPEST airborne, EM data and showed reasonably similar patterns. The geophysical survey data also highlights black shale units, which can produce a false target commonly running parallel to the sulphide altered fault zones and SIF units, because of graphite and sulphide in the black shale.
The TEMPEST data were a valuable guide to bedrock conductivity over the outline project area at Comet, and the follow–up ground TEM and SAM survey data was very useful for accurately pin-pointing anomalies for drill testing.
Geophysical and geological data analysed in this study was used to generate a geophysical interpretation map at 1:5,000 scale. The new interpretation of geological units and structures at Comet will provide geologists with a better understand about the geological and structural setting for mineralisation in the Comet area. For example, the Comet Fault represents a faulted limb of the Comet fold structure that has both limbs dipping to the SE, and plunges to the NE. Magnetic anomalies associated with SIF are considered to correlate with some gold bearing horizons and the location of the Comet Fault, that has become more siliceous and altered by sulphide minerals and magnetite minerals.
It is recommended that other prospect areas in the region should be surveyed using the SAM method in order to identify shallow gold bearing structures and improve geological interpretations ahead of drilling.

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

Typescript (Photocopy)
Includes copies of 4 papers by the author as appendix 4 (v. 1)
Errata slip inserted
Bibliography: leaves 170-192 (v. 1)
2 v. : ill., maps ; 30 cm.
Title page, contents and abstract only. The complete thesis in print form is available from the University Library.
Thesis (Ph.D.)--Dept. of Geology and Geophysics, University of Adelaide, 1992

This thesis brings together four individual studies of the geochemistry of the pyrites from the ~2.7 Ga Eastern Goldfields Superterrane Greenstone Belt (EGST), Yilgarn Craton, Western Australia. The data are used to provide a synthesis of the sulfur cycles in the Neoarchean, with a particular focus on the nature and origin of sulfur species in the (near) surface environment before the pervasive rise in oxygen. Multi-sulfur isotopes were analyzed for pyrites from relatively deep-water marine cherts and shales that are interbedded with the ~2.7 Ga EGST greenstone lava flows. The observed D33S anomalies for the EGST pyrites at or above the mantle value, implying a component of atmospheric elemental sulfur, and little or no contribution from negative D33S seawater sulfate. Variations in D33S and d34S are interpreted to be due to changes in the relative contributions of photolytic S0 and hydrothermal H2S to the growing pyrite crystals. Detailed time-series S isotopic trend show that D33S changes are dominated by local variations in the hydrothermal flux through seafloor vents rather than global changes in the atmospheric compositions. The marked global increase in D33S in Neoarchean sedimentary pyrites is attributed to the emergence of several cratons above sea level, accompanied by synchronous subaerial felsic volcanism, at ~2,650 Ma. The ~2.7 Ga Kapai Slate contains pyrite corona nodules, with distinctive cores and mantles. The cores are enriched in highly compatible trace elements (Ni, Ag, Bi, etc.), but depleted in incompatible elements (Mo and Tl), relative to the mantles. The striking feature of the data is the remarkable linear correlations between the compatible elements (R > 0.95) and their inverse correlation with incompatible Mo. A two-stage model is proposed for the formation of nodules. The cores crystallized slowly from stagnant pore fluid prior to the eruption of the overlying Paringa Basalt, whereas the mantles crystallized rapidly in conjunction with the eruption of the basalt. Deposition of the basalt compacted the unconsolidated Kapai clays, driving out the pore fluid, which had a profound impact on the geochemistry of nodule mantles. The relative compatibilities of the analyzed trace elements are also estimated, which provide a new constraint on the partition coefficients of the trace elements between Archean ocean water and sedimentary pyrite. A detailed quadruple S isotopic study were conducted for the Kapai Slate pyrite nodules. Statistical methods are applied to show that the best-fit lines for the S isotopic compositions of these pyrites have D36S/D33S gradients varying between -0.7 and -1.1, in agreement with most other studies of Archean sedimentary pyrites. Two of these best-fit lines, however, have positive intercepts on both the D36S and D33S axes. The observed linear relationship between D36S and D33S preludes the mixing between different atmospheric S reservoirs. It can, however, be modelled using a combination of at least two reactions, which simultaneously fractionate SO2 in a single atmospheric reservoir by utilizing different light bandwidths. A mathematical model is provided to constrain the S-MIF contribution from each of the likely photochemical reactions. It is suggested that this process can be called simultaneous fractionation. Finally, multi-sulfur isotopes were used to trace the sources of sulfur in the ~2.7 Ga Teutonic Bore Volcanic Complex VMS deposits to evaluate the ore formation model, and to quantitatively estimate the relative contribution of different sulfur reservoirs. The magmatic input, other than wallrock leaching, dominates the production of ore fluids. Most important, the quantity of seawater sulfur in the whole sulfur budget may be related to the size of the VMS deposits. The multi-sulfur isotope is shown to have great potential for investigating the genesis of metal sulfides mineral deposits in future economic geology studies.

This thesis has two principle objectives: to provide geochronological data for the Late Archean Murchison Province of Western Australia and to assess the strengths and limitations of the ion microprobe zircon dating technique. A project was conducted to provide zircon U/Pb age measurements on seven granitoid samples from the Murchison granite-greenstone terrain. These data represent the first systematic U/Pb age survey for the granitoids from this 100,000 km2 region. The oldest sample found in region was from a pegmatite-banded gneiss which contained a complex zircon population, the best estimate for the emplacement age for the magmatic precursor is circa 2919 ± 12 Ma (1cr). Two samples of recrystallized monzogranite, by far the dominant lithology in the region, gave emplacement ages of 2704 ± 51 and 2681 ± 6 Ma. Two samples from the southern post-folding granitoid suite gave ages of 2641 ± 5 and 2602 ± 14 Ma. Two samples collected from a pluton previously assigned to the northern post-folding granitoid suite gave ages of 2760 ± 8 and 2784 ± 22 Ma; this pluton has now been reinterpreted as a heretofore unrecognized synvolcanic suite which may be coeval with the nearby Mount Farmer greenstones. In addition to providing the first zircon age determinations for the major granitoid units in the area, these data also constrain the eruption ages of the two greenstone sequences and the timing of the regional deformation and metamorphic events. The absence of mid-Archean or older xenocrysts implies that the central Murchison Province is solely a product of Late Archean crustal growth. The success of this project was closely linked to the availability of a detailed tectonic model based on extensive field mapping by the Geological Survey of Western Australia. During this survey of the Murchison Province a unique sample was encountered which gave unusually reversely discordant U/Pb systematics. An extensive investigation of this phenomena revealed the presence of a well-mixed, highly radiogenic Pb which apparently entered the zircon population at circa 0 Ma. Based on isotope dilution data, it appears that the sputtering characteristics of this external component deviated significantly from the calibration standard which was used to determine the ion microprobes U/Pb discrimination factor. A second field-oriented project was conducted at Poona Rock, a typical outcrop of the 3500 km2 Murgoo Gneisses located along the western margin of the Murchison Province. Ion microprobe zircon analyses of six samples from this isolated outcrop all gave Late Archean emplacement ages. Because of the rapid evolution of Poona Rock, these data provided a rare opportunity to define precisely the age of the deformation which is seen on both the local and regional scales. This led to an extensive investigation of the accuracy and precision of the ion microprobe method. It was discovered that the ages calculated could be significantly affected by the assumptions made during the data assessment process. In complex data sets, the use of error estimates based on Poisson ion counting resulted in certain samples being designated as outliers which, when using more generous error assignments based on observed internal reproducibilities, apparently were part of the magmatic population. The complex U/Pb systematics observed in the samples were further attested to by the zircon structures and morphologies seen in these six samples. All analyses reported here were tested for excess internal error in their Pb/Pb ratios. The seven scans of the mass spectrum were compared to a mixing line joining the mean of the seven scans and an assumed common Pb end-member. In many cases it was found that the observed scatter of the data away from this mixing line was greater than that predicted by the best-possible-limit imposed by the observed ion count rates. A further refinement to the data assessment was the introduction of a best-fit plane technique for calculating the concordia intercept ages of a pool of data. This method has two advantages over data assessment based on the mean 207PbJ206pb ratio: this 3-dimensional approach requires neither an assumed common Pb composition nor an assumed 0 Ma lower concordia intercept. Despite these advantages, the best-fit plane method is unable to define a magmatic age when a population contains numerous measurements which diverge only slightly from the main population. Finally, an assessment of the 312 measurements conducted on the SL3 standard showed the presence of a previously unrecognized and significant fractionation of the Pb isotopic spectrum. The magnitude of the ion microprobe's fractionation is estimated at between 3 and 5%o per mass unit. This conclusion is directly dependent on the 572 Ma age which has been assigned to the SL3 standard.

This thesis presents the results of a detailed study of the mineralogy and paragenesis of gold at the Sunrise Dam gold deposit. The Sunrise Dam mine is the largest gold deposit in the Archean Laverton Tectonic Zone of the Eastern Goldfields Province, Yilgarn Craton, Western Australia. A number of previous studies have established the geology, geochemistry and geochronology, but the nature of the gold mineralogy and distribution has remained poorly characterized. Mineralogical studies have established a paragenetic sequence consisting of five hydrothermal stages (D1, D2, D3, D4a and D4b) which are generally in accord with the major deformation events at Sunrise Dam gold deposit. The D4a stage was the dominant episode of Au deposition, followed, in importance by the D4b stage, which is characterized by more diverse ore mineralogy including base metal sulfides, sulfosalts, and telluride minerals. Based on EPMA results, native gold in D4a stage has higher purity, with a small range of Ag variations (fineness 923 ~ 977, average 945), than that of the D4b stage (fineness 596 ~ 983, average 899), in which fineness values decrease systematically in accord with mineral paragenesis, reflecting that gold deposition was from a progressively compositionally evolving hydrothermal fluid with respect to Au/Ag ratios. The occurrences of As-rich pyrites are restricted to steeply-dipping ore bodies, which are most likely structurally connected at various level by channel ways through which As-rich (D4a) hydrothermal fluid migrating upward. There is a systematic variation in composition of the tetrahedrite-group minerals ranging from Sb to As end-members with highly variable Zn:Fe ratios, which correlates with the later paragenetic stages (D3, D4a, and D4b) and mineral associations. The composition of the tetrahedrite-group minerals is useful as a petrogenetic indicator of the evolution of the hydrothermal mineralizing systems with time. A total of thirteen telluride mineral species, including two unnamed phases, were identified in the D4 veins. Among them nagyágite, the complex Pb-Sb-Au tellurosulfide is most abundant. The deposit is the second occurrence of this mineral in the Yilgarn Craton. Compositionally, nagyágite from Sunrise Dam conforms to ideal stoichiometry, with negligible As content and Au/(Au+Te) ratio of 0.325. The diverse mineralogy of the post-D4 veinlets relative to the host veins is attributed to small-scale reaction fronts established along zones of replacement. The presence of Au-Ag tellurides in D4 veins and the character of their breakdown products have implications for the gold recovery as well as for the genetic interpretation of the deposit. During the D4b stage, Au-richer telluride and Au-richer native gold mineralization formed earlier than Ag-(Au)-telluride and Ag-richer gold mineralization. Values of f(Te2) and f(S2) for the early telluride assemblages were determined at 300°C to be -10.7 to -7.8 (log fTe2) and 11.4 to -8.6( log fS2 ). The Au content of arsenian pyrite and arsenopyrite from four mineralizing stages (D1, D3, D4a and D4b) was measured using in-situ LA-ICP-MS. The average Au concentration is 44.5 ppm in pyrite (n = 224) with maximum value of 3,067 ppm, and 1,483 ppm in arsenopyrite (n = 35) with maximum value of 5,767 ppm, which are the highest concentrations reported for the Yilgarn Craton. The concentrations of invisible Au in arsenian pyrite at Sunrise Dam varies with mineralizing events, mineral paragenesis, and textural type. Gold is strongly enriched in D4a stage pyrite (average 80.8 ppm) and to a lesser extent in D4b pyrite (average 16.8 ppm). Pyrite from D1 (average 3.55 ppm) and D3 (average 2.96 ppm) show much lower levels of Au enrichment. The presence of metallic Au below the Au solubility limit in the Sunrise Dam pyrite is interpreted as evidence of an epigenetic origin for Au mineralization. Small-scale remobilization during dissolution-reprecipitation (D4a) and recrystallization (post-D4b) processes resulted in the Au enrichment and the upgrading of Au during successive hydrothermal events in the deposit. The speciation of Au at Sunrise Dam and the exceptional size of the deposit are the result of multiple fluid flow and multiple Au-precipitating mechanisms over a single plumbing system.

The Archaean Yilgarn Craton of Western Australia consists of a high-grade gneiss terrain (Western Gneiss Terrain) and three granite-greenstone provinces: the Murchison, Southern Cross and Eastern Goldfields Provinces. Most of the previous geochronological studies were conducted in the Eastern Goldfields Province, particularly in the Norseman-Kalgoorlie region, and in the northern part of the Western Gneiss Terrain (i.e. Narryer Gneiss Complex). The remaining parts of the Yilgarn Craton are less well dated. Due, in part, to the lack of precise and accurate geochronological data, the origin and evolution of the craton is still controversial. This study focuses primarily on the granite-greenstone terrains of the Yilgarn Craton, in particular those of the Murchison and Southern Cross Provinces. U-Pb zircon geochronology was carried out using the Sensitive High Resolution Ion Microprobe (SHRIMP). Sm-Nd isotopic systematics of selected granitoids were also determined to trace their source and the timing of separation from the mantle. These investigations provide geochronological constraints on the timing of formation of the supracrustal rocks and emplacem nt of granitoids, as well as information about the underlying basement in the studied areas. The data are used to test the stratigraphic subdivision schemes for the Murchison Province, to determine stratigraphic positions of the Gum Creek and Lake Johnston greenstone belts in the Southern Cross Province, and to discuss the spatial and temporal distributions of the volcanic and plutonic episodes and timing of mineralisation. The late Archaean granite-greenstone terrains of the Yilgarn Craton developed during three distinct thermal events at ca. 3.0-2.90 Ga, ca. 2.8 Ga and ca. 2.76-2.60 Ga. There are two major volcanic and plutonic episodes in the Yilgarn Craton. Volcanic rocks formed between ca. 3.0-2.90 Ga and ca. 2.76-2.70 Ga, and plutonic rocks between ca. 3.0-2.90 and ca. 2.76-2.60 Ga. The ca. 2.8 Ga volcanic event is spatially and temporally restricted and is not accompanied by synvolcanic plutonism of the same age. Geochronological comparison across the Yilgarn Craton indicates that the granite­ greenstone terrains have shared a common evolutionary history since at least ca. 3.0 Ga and that the gneiss terrain in the western Yilgarn Craton was not brought in tectonic contact with the granite-greenstone terrains (e.g. the Murchison Province) until ca. 2.70-2.60 Ga when cratonisation occurred. Xenocrystic zircons record, not only the three thermal events in the lower crust noted above, but also provide useful information about the age of the basement to the granite-greenstone terrains. The presence of ca. 3.0-3.9 Ga xenocrysts, combined with evidence from geophysical and Pb and Sm-Nd isotopic data, imply that all granite-greenstone terrains in the Yilgarn Craton formed above, or at least in association with, a pre­ existing continental crust. In the Murchison Province, two greenstone sequences, the ca. 3.0 Ga Luke Creek and the ca. 2.8 Ga Mount Farmer Groups had been previously proposed. However, the results of this study, in combination with previous geochronology, reveal that three greenstone sequences were developed in this province during separate volcanic episodes at ca. 3.0-2.93 Ga, ca. 2.8, and ca. 2.76-2.70 Ga. The Mount Farmer Group is shown to be ca. 2.7 Ga, not ca. 2.8 Ga as had previously been thought. The present study provides evidence for the existence of a third province-wide greenstone succession at ca. 2.8 Ga, which lies unconformably between the other two sequences. This observation indicates that the ca. 2.8 Ga stratigraphic unit cannot be the uppermost component of the Luke Creek Group as formerly suggested. The new results support the newly proposed, informal, process-based stratigraphic classification for the northern part of the province (Hallberg et al., personal communication, 1997; see also Pidgeon and Hallberg, in press). Most granitoids in the Murchison Province were emplaced between ca. 2.76 and 2.60 Ga. Intrusion of the oldest external recrystallised monzogranites, which occupy large areas surrounding the greenstone belts, and the oldest small to medium-sized internal plutons that truncate the greenstones and tectonic features associated with folding, commenced at ca. 2.76 Ga. These intrusions are synchronous with the onset of deposition of the youngest greenstone sequence in the province, indicating that they developed in a single thermal-magmatic event. No consistent geochronologic relationship was found between regional and internal plutons and between the ages and sizes of granitoids, although the oldest plutons tend to be small. Similarly, no correlation was found between the degree of deformation and the timing of intrusion. It is apparent that field-based observations at isolated outcrops cannot be used to predict the relative order of granitoid emplacement. The ca. 2.7 Ga ages obtained for the Gum Creek greenstone belt do not support the previous suggestion that the greenstones from this belt can be correlated with the ca. 2.93-3.0 Ga sequence found in the Murchison Province, and with the lower sequence of similar age recognised in the Southern Cross Province. The studied rock units apparently belong to the ca. 2.7 Ga upper greenstone sequence in the Southern Cross Province, which is broadly synchronous with the youngest greenstone sequence developed in the Murchison Province. The Lake Johnston greenstone belt has an age of ca. 2.9 Ga, and thus forms part of the lower sequence of the Southern Cross Province. Ages determined for the granitoids in the Gum Creek greenstone belt are between ca. 2638-2722 Ma, similar to those dated elsewhere within the Southern Cross and Murchison Provinces. Most Nd model ages for the studied granitoids lie between ca. 2.93 and 3.10 Ga, which are typically a few hundreds of million years older than their emplacement ages, but are similar to, or slightly older than, the oldest (ca. 2.91-2.94 Ga) xenocrysts in these samples and the oldest (ca. 2.93-2.98 Ga) greenstone sequence in the Murchison Province. The results suggest that the crustal rocks, with an average age of 2.93-2.98 Ga, are the main sources of the granitoids. The time interval between ca. 2.98 and 3.0 Ga appears to be a major period of crustal formation in the Murchison Province. Although the data imply different sources for the various granitoid suites in the Murchison Province, the voluminous regional and the main suite of the internal plutons, appear to have been derived from the same, or isotopically similar, source regions. The stratabound volcanic massive sulphide mineralisation at Golden Grove in the Murchison Province is constrained to have formed between 2953±7 and 2945±4 Ma, predating similar mineralisation in the Eastern Goldfields Province by about 250 million years. The formation of komatiites and associated Ni mineralisation at the Maggie Hays nickel prospect in the Lake Johnston greenstone belt, is constrained to lie between 2921±4 and 2903±5 Ma, about 200 million years before their counterparts in the adjacent Eastern Goldfields Province. Samples from the Kanowna Belle mine (- 20 km northeast of Kalgoorlie in the Eastern Goldfields Province), which is the first discovery of a major gold deposit hosted by felsic porphyry in the Yilgarn Craton, were dated in order to constrain the two stages of mineralisation identified by petrographic, fluid inclusion, and stable isotope studies. The early stage of mineralisation has an age of 2695±4 Ma, which is ca. 60 million years older than the accepted age of 2630±10 Ma for the main gold forming event in the Yilgarn Craton, making it the oldest recorded gold mineralisation event in the region. Younger events occurred between ca. 2630 and 2650 Ma, broadly synchronous with the principal period of gold mineralisation in the region. These results, combined with existing data, indicate that significant gold mineralisation occurred over at least 90, and possibly as much as 130 million years, in the Yilgarn Craton.

The ecology of subterranean ecosystems and stygofauna (subterranean aquatic animals) has largely been unexplored in an Australian context. The Yilgarn region of Western Australia is known as a biodiversity hotspot in relation to stygofauna from isolated calcrete aquifers, and it is home to the most diverse assemblage of subterranean, predatory diving beetles in the world. This study used extensive grids of boreholes to access calcrete aquifers at Sturt Meadows and Laverton Downs pastoral stations to investigate how subterranean species interact with their external and internal environment, focusing on six subterranean beetle species. A mix of traditional ecological monitoring and next-generation sequencing methods were employed to examine the following specific questions: What are the types of prey available in these calcrete systems and how do they change in abundance over time? What are the natural gut microbial communities associated with these predatory beetle species? Moreover, can metagenomic analyses be used to identify trophic differences among species, including adults and larvae, and determine whether beetle species eat other beetle species? Ecological monitoring over an 11-year period identified that rainfall and, in particular, major recharge events are important for the diversity and distribution of stygofauna within the calcrete at Sturt Meadows. Average taxon richness was highest shortly after periods of high rainfall, and when dominant taxa (i.e. amphipods and copepods) were excluded, evenness decreased after both high and low rainfall suggesting that dominant taxa are an important factor driving the system. Common taxa (i.e. amphipods and copepods) within the calcrete had broad distributions and high abundance levels, while rare taxa (oligochaete worms) had restricted distributions and low abundances. All taxon groups had lower abundances and narrower distributions after periods of intermediate and low rainfall. Over the 11-year period, the majority of boreholes sampled did not show changes in evenness, suggesting that the Sturt Meadows calcrete is a reasonably stable ecosystem with episodic fluctuations, most likely attributed to rainfall events. The gut microbiome was investigated in six beetle species from two separate aquifers using random shotgun sequencing (metagenomic analyses). The bacterial and viral communities were investigated separately, but the investigation showed similar results as follows: In both the viral and bacterial analyses the microbial communities varied greatly by location and there was a distinct signature in the microbial communities depending on whether samples were collected from aquifers or laboratory aquaria. There were also distinct differences among the beetle species and their stage of development (adult versus larvae), which are most likely accounted for by trophic differences among the beetles. In both the bacterial and viral analyses a large number of the sequences were novel and unable to be identified, suggesting major differences in their microbiome compared to previously studied invertebrates. The unknown sequences will once identified, provide further insights into the microbial communities of these subterranean environments. Like the bacteria, viral sequences provided evidence that calcretes had been influenced by anthropogenic activities on the surface, with a large number of vertebrate viruses infiltrating the calcrete system. The mitochondrial (mt) genomes of four of the beetle species, Limbodessus palmulaoides and P. macrosturtensis, P. mesosturtensis and P. microsturtensis, were characterised to provide a framework for future trophic analyses of the beetle gut contents and as a basis for further assessment of the molecular evolution of mtDNA genes associated with evolution underground. The mt genomes were all consistent with both previously sequenced dytiscid beetle mt genomes and the inferred ancestral insect mt genome. All four mt genomes were circular, contained the expected 37 genes and ranged from 16,504 to 16,868 bp. The overall structure (gene number, orientation and order) was consistent with the ancestral insect mt genome, and the genome size variation resulting from length variation of intergenic regions and the CR is consistent with other surface dytiscid species sequenced. These ecological and molecular analyses show a complex interconnected system between the surface and subterranean environments. They also demonstrate that metagenomics research can be used effectively for investigating the trophic ecology of species, particularly in taxa where traditional methods are ineffective or difficult to undertake. Preliminary analyses of the beetle metagenomes suggested that the beetle species at Sturt Meadows are not only eating other invertebrates from the calcrete but are also eating the other beetle species. This result may have been difficult to elucidate using traditional methods (e.g. metabarcoding) given how closely related the beetle species are to each other. This research also highlights that the subterranean beetles provide an excellent model system, not only for future microbiome work but also for investigating the adaptive and regressive evolution of the genome associated with moving from surface to underground habitats.
Thesis (Ph.D.) -- University of Adelaide, School of Biological Sciences, 2018

The Bellerophon gold deposit in the St Ives camp, Yilgarn craton, Western Australia, has been studied to assess the importance of magmatic systems in the formation of ancient gold deposits. The majority of the gold grains occur in the quartz-albite-carbonate-pyrite veins and quartz-pyrite veins. Intense albite and hematite alteration surrounds the mineralized veins, which show enrichment in Na, S, and Sr, and depletion in K, Cs, Rb, Cr, V, and Ni, compared with their unaltered equivalents. During mineralization, Bi, Te, Pb, and Mo were introduced together with Au. Multi sulfur isotopes measurements of pyrites that are genetically related to the gold mineralization from the Bellerophon, Victory, and Wallaby deposits in the Yilgarn craton, and the Beattie deposit from the Abitibi belt, Canada, show that the sulfur in the gold-bearing fluid is dominated by mass dependent fractionation (MDF), which requires the fluid to have a mantle origin or to have been derived from magma of mantle origin. Three types of fluid inclusions were identified: Type I low salinity carbon dioxide inclusions, Type II high salinity aqueous inclusions, and Type III disordered carbon bearing high salinity aqueous inclusions. Type I fluid inclusions can be further divided into Type Ia and Type Ib with high and low ratios of carbon dioxide to water, respectively. The similarity between homogenization temperatures, and the occurrence of the Type Ia and Types II inclusions within the same clusters suggest that they formed by liquid immiscibility at about 300 degree celcius. Type III fluid inclusions, which have high temperature (exceed 550 degree celcius), high salinity (38 weight percent NaCl equiv.), and a redox state that lies close to the carbon dioxide and methane buffer, are interpreted to represent the parental hydrothermal fluid. The exsolution of methane from the hydrothermal fluid, during fluid immiscibility, lead to oxidation of the remaining fluid, which in turn triggered gold precipitation. Two types of hydrothermal scheelite were identified in association with mineralization, Type I, which is enriched in the middle rare earth elements (REE), and Type II, which has a flat REE pattern. Hydrothermal apatite has a similar REE pattern to the Type I scheelite. Metamorphic apatites are distinct from the hydrothermal apatite and scheelite in geochemistry. The Sr isotopes composition of hydrothermal scheelite is similar to that of apatite from the host rocks, which indicates that the Sr isotopes in hydrothermal fluid have been modified by interaction with the wall rocks. The wide range of Sr isotopic compositions suggests that the ore-forming fluid has been transported over a long distance. The age of the Bellerophon gold deposit was determined by Ar-Ar dating muscovite extracted from ore veins. The age obtained was 2614 Ma, which is appreciably younger than the associated monzonite intrusions, which have U-Pb zircon age of 2660 Ma, and cannot be the source of the mineralization. Combining all the published ages for gold mineralization in Yilgarn craton showed that the mineralization form over an extended period from ca. 2700 Ma to ca. 2600Ma.

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