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Indiscriminate surface disposal of coal waste in New South Wales has created a serious fire hazard and increased air pollution.A survey of numerous dumps, as well as particular investigations of one badly-constructed dump, showed that factors conducive to ignition and propagation of fires in waste dumps were high contents of combustible material (coal, pyrite, wood. paper. grease), size segregation leading to ready movement of air and moisture shape of the dump (e.g. protruding sections or porous junctions), high ambient air temperatures, bush fires, and even deliberate lighting.Control methods applied in the past tended to be haphazard and unsuccessful. Under Australian conditions the technique recommended for control of existing dump fires, based on experimental work, is to spray the dump with a chemical fire retardant (e.g. a 2 per cent solution of sodium tetra borate and ammonium phosphate), to cover the dump with a suitable soil, and to seal the surface with a I per cent solution of aluminium sulphate or sodium metasilicate. The recommended method of dump construction to prevent fires is to level and seal the site, to construct a firebreak around the dump area, and to build a rectangular dump with minimum size segregation and compacted surfaces.

Jan 1, 1971

By Mostyn G

In the last three decades various theories have been presented to allow the estimation of the force required to cut rock. These have generally relied on an hypothesised mechanism of chip formation.The paper presents results of an experimental program completed on an unjointed artificial rock in which the force and chip geometry were measured during deep cutting with a quarter scale bulldozer tyne. The program included various depths of cut and artificial rock of varying strength. The experimental results are compared with predictions based on three expressions for cutting force. Generally the measured forces are within the range of those predicted but none of the methods predicts the cutting force with any accuracy. It is considered that the discrepancies are due, in part, to the fact the that actual shape of the chip formed in deep cutting is quite different to that assumed in developing the theories and thus the theories cannot be expected to predict the cutting forces. It is concluded that Evans and Nishimatsu's theories predict lower bound estimates of the horizontal cutting forces. Deliac and Fairhurst's approach appears to over estimate the forces required to cut rock. New methods of prediction are required based on the observed mechanisms of failure.

Jan 1, 1993

Production from a major, deep orebody requires the construction of two 6 m diameter, 1000 m deep ventilation shafts over the next three years. Further ventilation upgrades have foreshadowed an additional 1500 m of 6 m diameter shafts beyond that. After reviewing the construction alternatives it was decided to raisebore the first shaft in one pass using Western Mining Corporation's 121R raiseborer and the Wirth sequential head. The significant cost and speed of construction potential of 6 m raiseboring justified the risks associated with this new technology. Large diameter sequential head raiseboring has only been carried out in South Africa. Over the last three years many lessons have been learnt and the technology has progressed to being considered feasible. Operating practice and the optimisation of raiseboring performance for specific ground conditions are the areas requiring further work. The development of large diameter raiseboring in South Africa and the site preparation and initial operation at Z.C. Mines are described. Comment on actual operating experience includes the geotechnical investigations, the raiseborer foundations, cuttings disposal and the drilling of the pilot hole which has progressed to beyond 450 m. Unforeseen difficulties with the verticality of the pilot hole and with mud losses illustrate the types of problems that can be expected.

Jan 1, 1988

Copper was first produced in Australia in 1844, at the Kapunda Mine in South Australia, and, by 18i>0, production exceeded 2,000 tons of copper a year. Output increased ,steadily, reaching a peak of 14,00Qo tons a year in 1867 and 1868, when the Burra Burra and Kapunda Mines in South Australia and the Peak Downs Moine at Clermont, Queensland, were at the height of their production. At this period, Australian copper formed a considerable percentage of the world's supply, its output equalling, for a short time, that of the United States. Production declined to between 3,000 and 4,000 tons a year after the closing of' these three mines between 18717 and 1879, and, at this stage, the Australian output came chiefly from the Wallatoo and Moonta mines in South Australia. About 19000, it began to rise again, with the extension of the railway to the copper fields of Chillagoe and Cloncurry, and, between 1905 and 1912, was at its greatest, with a maximum of 47,774 tons of copper in 1912. During this period, Australia contributed 4,7 per cent. of the world's annual production, and ranked among the six major copper-producing countries of the world (Table 1).

Jan 1, 1943

By Borshoff J, Von Pechmann E

The uranium mineralization in the White's East area of The Embayment is hosted by Lower Proterozoic schists of the Masson Formation which have undergone polyphase de- formation and upper greenschist metamorphism. Significant mineralization is also present in apatite rocks. The ore zones occur near an unconformity with overlying Middle Proterozoic sandstone and breccia conglomerate. Kink breccias and fracture systems related to post Middle Proterozoic reverse faults are the con- trols for mineralizing fluid migration. Pitchblende is the main uranium mineral and it occurs as fine disseminated grains, fibrous webs, clusters composed of botryoidal aggregates and locally as veins. Two genera- tions of uranium mineralization are present. The first generation (pitchblende I) occurs as fine grained inclusions within chlorite II, and the second (pitchblende II) as hydraulic fracture networks and massive veins intimately associated with sericite-hematite-chlorite III. Two hydrothermal alteration phases have affected both Lower Proterozoic and Middle Proterozoic sequences. The most extensive alteration mineral is chlorite, of which a number of varieties has been identified. Mg-rich chlorites are generally associated with the first phase alteration assemblages and are commonly replaced by hematite, seri- cite and Mg-Fe chlorites in massive pitch- blende zones. Other alteration minerals in- clude tourmaline, apatite, talc, quartz, magnesite, graphite, pyrite and rutile.

Jan 1, 1984

Gold-rich porphyry copper deposits areimportant sources of gold in the circum-Pacific region: 26 major deposits contain >7000 tonnes of gold. The deposits occur in a variety of subduction-related settings, and may be underlain by crust that is undergoing either extension or compression and that is either oceanic or cratonic in character. The deposits are associated intimately with composite porphyry stocks, which commonly were emplaced into coeval andesitic volcanic piles. The stocks range in composition from low-K calc-alkaline through high-K calc-alkaline to potassic alkaline. Much of the copper and gold were introduced as components of K-silicate alteration, which may undergo partial overprinting by intermediate argillic assemblages. Advanced argillic alteration is widespread in the shallow parts of the systems whereas sericitic alteration at deeper levels tends to be restricted. Gold distribution generally follows that of copper, which is present mainly as chalcopyrite with or without bornite. The gold is in the native state and occluded by cr in close proximity to the copper-iron and/or iron sulphides. The magmas and metals necessary for the generation of gold-rich porphyry deposits were derived mainly from subcrustal sources, with the subducted slab believed to play a pivotal role.

Jan 1, 1990

Rockbursts, as they occur in South African deep level gold mines, have a lot in common with natural earthquakes. Both violently release seismic energy and cause damage to underground and surface structures. Rockbursts are the main cause of fatalities in deep gold mines and the problem may increase in severity with future mining at greater depths. Although the emphasis in Rock mechanics is on the prevention of rockbursts, prediction would provide a partial solution to the rockburst problem. A research project was initiated in 1981 on Western Deep Levels to investigate the possibility of detecting and identifying precursive microseismic activity. This project has succeeded in locating potential sources of seismic events with reasonable confidence. The timing of these events may be estimated with less confidence, and an important parameter, namely the potential size of the rockburst, still cannot be determined. An example of a large seismic event and its associated precursive activity are discussed. Practical prediction systems will, at least for some time, involve subjective decision making which will place a new responsibility on the mine manager as well as the rockburst specialist. The moral pressure on the manager as the final decision maker will probably be greater than the fear of leqal prosecution.

Jan 1, 1986

By Scherbatsky VB, zon BM, Babushkin NM, Kitaev BI, Shabel&apos

The structure and hydrodynamics of the raceway zone of a blast furnace was studied on a cold model representing a sector containing two tuyeres. The model differed from the usual in that it was prov- ided with continuous flow of the coke layer at pre- determined rates, had provision for changing the tuyere parameters (diameter, protrusion, inclinat- ion) and irrigation of the layer with liquid. A combination probe was developed which per- mitted simultaneous measurement of the pressure field both across the area and through the height of the layer as well as determining the topography of the raceway. The velocity fields in the layer were measured with a specially made impulse thermo- anemometer. The determining criteria of the model were taken as the relationships between the energy of the blast and the particles, the dimensions of the raceway and the cross-section of the tuyere. The model established the effects of the tuy- ere structural parameters, blast parameters and amount of liquid products of smelting on the con- figuration of the raceway, the structure of the layer, pressure and velocity fields in the vicinity of the tuyeres and in the vertical direction through the layer. The properties of the raceway formation and the structure of the layer in motion have been clarified.

Jan 1, 1981

Laboratory experiments have been used tostudy a wide range of convective processes which are significant for the formation of rocks and the ores that form in them. Metal-rich solutions flowing through the sea floor produce 'black smoker' chimneys; both the size and structure of a solid chimney and the height to which the plume of effluent rises above it can be predicted using model experiments. Analogues of processes in solidifying magmas can also be studied using crystallizing aqueous solutions. The release of lighter or denser residual fluid as crystallization proceeds, and the resulting compositional convection, have a vital influence on the differentiation of initially homogeneous magma and on the evolution of stratified magma chambers. Mixing during the replenishment of magma chambers, and its dependence on the rate of filling and on the fluid properties, have also been studied on the laboratory scale. Experiments carried out in different geometries have been applied here to the formation of platinum and chromite ores and komatiite lavas. Larger-scale mantle convection, in particular the motion of subducting plates and plumes rising from the core-mantle boundary, also determine the tectonic settings in which ore bodies form. These phenomena too can be usefully investigated in laboratory experiments using very viscous fluids.

Jan 1, 1990

By Gemmell J. B

Zinc-bearing massive sulphide deposits have been mined in Tasmania since 1900. The current major producers are Hellyer and Rosebery, with total resource tonnages (mined plus reserves) of 16 Mt (million tonnes) and 24.8 Mt respectively. These deposits belong to the class of seafloor volcanic-hosted massive sulphides (VHMS) and are located within the Mt Read Volcanics, a narrow belt of continental margin calcalkaline volcanics of Cambrian age. Compared to other Australian VHMS deposits, and world-wide MVT and Sedex deposits, the Tasmanian examples clearly stand-out due to their high metal grades, averaging over 17 per cent Pb+Zn. The deposits vary in morphology from mound style (Hellyer) to sheet style (Rosebery) with other combinations including stacked lenses (Que River) and disrupted cross-cutting bodies (Hercules). All deposits show the classic VHMS zonation from an Fe-Cu-bearing base to a Zn-Pb-Ba-rich top. Zinc, gold and silver tenor commonly increases toward the stratigraphic top of the deposits. The ores have been deformed during regional metamorphism, resulting in folding, shearing and recrystallisation of sulphide lenses. In addition to the major deposits, a number of small massive sulphide prospects occur throughout the volcanic belt and the potential for the discovery of further large, deeply buried deposits remains high.

Jan 1, 1993

Black coals occur in most of the major sedimentary basins in Australia. In addition to the better known Permian coal occurrences of the Sydney, Bowen, Oaklands and Galilee Basins, coals of Permian age occur in the Arckaringa Basin in South Australia, the Bonaparte Basin in Northern Territory and the Collie, Perth and Canning Basins in Western Australia and the Tasmania Basin in Tasmania. Coals of Triassic age occur in the Ipswich Callide and Tarong Basins in Queensland, the Tasmania Basin in Tasmania and the Leigh Creek area in South Aus- tralia. Coal bearing rocks of Jurassic age occur in the Mulgildie Basin and Maryborough Basins in Queensland and in both the Queensland and New South Wales portions of the Clarence Moreton Basin and Surat Basins. They also occur in the Perth Basin in Western Australia. Rocks of Cretaceous age known to contain coal occur in the Styx, Maryborough and Laura Basins in Queensland, the Gippsland Basin in Victoria and both the Queensland and New South Wales portions of the Surat Basin. The coal measures have been deposited in a variety of sedimentary environments and the coals vary widely with regard to thickness, extent, banding characteristics, maceral and ash content. However, they are generally of low rank and most are suitable only for steaming.

Jan 1, 1975

WINDING engines are one of the most important units in the equipment of a mine. Upon the winding machinery depends not only the output of the mine, but it supplies in most cases the only means by which workmen enter and return from the mine, and consequently the utmost care and attention is desirable in its design. The efficiency of a direct acting winding engine, as a machine is very low. In other words, the proportion between the useful work performed and the actual work the engine is capable of performing (under the most favourable conditions) is very small. The reasons for this are:-1. The intermittent nature of the work; the engine is stopped from 20 to 25 %(or even more) of the time which would constitute a useful day's work.2. The large amount of power that is absorbed applying the brakes to bring the load to rest.3. That the net useful load raised is small in comparison with dead load to be lifted, and the parts to be set in motion.4. That, owing to the frequent stops, initial condensation in the cylinders is always greater than in a continuously running engine, whilst radiation from steam pipes, valve chests, &c., goes on whether the engine is running or...

Jan 1, 1911

By Holliday R, Floyd JM

A laboratory investigation was carried out to determine the distribution of gold between the products of lead-zinc concentrate smelting in the Imperial Smelting Furnace (ISF). Bullion, speiss and slag from the ISF at Cockle Creek were used as the starting materials to evaluate the effect of gold and copper content of products on the distribution of gold between phases under conditions simulating those in the ISF hearth. The ratio of gold in bullion to gold in speiss has a mean value of approximately 1.6 and is independent of the gold content of the bullion. The distribution coefficient of gold between bullion and speiss is dependent on the copper level in speiss and is lowered by increasing copper content in speiss. The ratio of gold in bullion to gold in slag is in the range 25 to 5700 and dependent on the gold content of the bullion. For low gold concentrations in bullion of the order of 1 g/t and a bullion to slag ratio of 1:3 the gold loss to slag is expected to be approx- imately 23%. In all tests the gold in slag remained low, in the range 0.05 to 0.5 ppm provided metal prills were not suspended in Slag.

Jan 1, 1986

By Perring CS, Hill RE, Barnes SJ, Vallance SA

The Maggie Hays nickel sulphide deposit is located at latitude 32¦ 15 'S, longitude 120¦ 30' E on the Lake Johnston (SI 51-1) 1:250 000 map sheet. The deposit occurs in the Lake Johnston greenstone belt, in the Southern Cross Province of the Archaean Yilgarn Block, 500 kilometres east of Perth, Western Australia (Figure 1). The remoteness of the Lake Johnston greenstone belt and its poor access, restricted previous exploration activities and the full appreciation of the geology and its Ni-sulphide potential. It was not until 1991, when Forrestania Gold NL commenced exploration activities, that the geology of the ultramafic units and their potential to host significant concentrations of Ni sulphides were clearly established. This paper, which describes the geology and the characteristics of the Maggie Hays deposit, is based on the results of exploration by Forrestania Gold NL and a collaborative research agreement between CSIRO Division of Exploration and Mining and Forrestania Gold as reported by Perring, Barnes and Hill (1994), Perring and Hill (1995), Perring (1995 a and b) and Barnes, Perring and Reilly (1995). A comprehensive description of the geology, petrology and geochemistry of the deposit is being prepared for publication by CSIRO (Pemng, Hill and Barnes, in press).

Jan 1, 1996

By Lightfoot BW, Wand PD, Towne DV

Sampling and e.m.f. probes were used in the liquid flow from the blast furnace and in the forehearth to evaluate the performance of the copper smelting system at E.R. & S. Significant variations in temperature, oxygen potential and copper content with slag depth and with position in the forehearth indicated that convective currents were causing considerable stirring in the forehearth. This was attributed to temperature fluctuations in the stream from the blast furnace, which resulted in colder slag being underlain by hotter matte. Tracer tests in the feed to the smelter and in the feed to the forehearth revealed considerable holdup of material in the plant and confirmed that the forehearth involved small scale turbulence but little large scale mixing. The results indicated that the copper content of slag continuously tapped from the forehearth could be lowered by at least 0.15% if better settling could be achieved and means of attaining this are discussed. As part of the investigation the recovery of copper from spent refractory bricks recycled through the smelter was evaluated. It was found that the recovery was high but it seems likely that the brick material is partly responsible for a build up of solid material in the forehearth.

Jan 1, 1981

Broken Hill South Limited's discovery of phosphate deposits in the northwest of Queensland in 1966 prompted intensive exploration which has proved phosphate rock in excess of 2,000 million tons at ten separate deposits. Systematic exploration for phosphate in Australia was initiated by the Company in 1964. Early in 1966, an investigation of oil wells in the Georgina Basin in the Northern Territory and Queensland revealed widespread anomalous phosphate in early Middle Cambrian Beetle Creek Formation and Thorntonia Lime- stone. Phosphorites recognised in oil wells in the southeastern part of the Basin, Queensland, led to the discovery of the Duchess deposits, Exploration of the Beetle Creek Formation since 1966 has disclosed nine other sizeable deposits north of Duchess around the eastern margin of the Basin. The Lady Annie and the adjoining Lady Jane deposits, by reason of their location, 160 miles south of the Gulf of Carpentaria, are expected to be the first to be brought into production. Beneficiation testing and engineering investigations commenced in 1967. Transport between the deposits and various port sites in the Gulf of Carpentaria has been extensively studied and a slurry pipeline as a means of transport to a deep water island port, is now being investigated.

Jan 1, 1971

The Pasminco mine at Rosebery in north western Tasmania is a medium sized underground base and precious metals mine. In April 1992 a major wedge failure of approximately 5000 t occurred in the backs of a main access drive to the 18 level H Lens orebody. This collapse prevented access to 190 000 t of ore which had been scheduled for production in July - August 1992. At the time of the collapse, the mine was in a transition period between mining small pillar remnants of several other orebodies and developing to the new deeper J Lens orebody.The development at this orebody was behind schedule and it was necessary to find a cost-effective and timely alternative to a 75 m bypass drive around the fall area.A Lysaght- Fletcher multiplate steel arch was available on-site from a deferred surface road project and it was decided to use this arch to regain access through the fall area. Due to the danger of continued minor falls, the entire 18 m long, 3.95 m high x 4.5 m wide tunnel had to be assembled in the 4.7 m wide x 5 m high accesss drive and pushed into the fall area as a single unit.

Jan 1, 1993

By J Bartlett, P Quigley

Historical research has played a significant role in the rebirth of the Bendigo Goldfield. The historical research undertaken by the company has been directed to specific areas such as verifying the total gold production of the field, the gold production from defined blocks on each of the major anticlines, the extent of workings of each mine which exceeded 200 m depth, the size and style of reefs mined in each shaft and also within specific domains of the field. Application of this data has assisted in the determination of possible dimensions of different reef styles and the location of mineralisation within each reef system. Description of grade variation, percentage of quartz and the amount and species of accessory sulphide minerals, as well as early geotechnical observations accompanying stoping methodologies, provides valuable analogues for reef structure being defined in the current program. Historical information on shafts on the two anticlines the company is exploring has allowed the postulation and recognition of repetition of reef development within the same stratigraphy in the hinge zones of the adjacent folds. The similarities of mineralisation styles across the field within both specific lithological units and structural setting has had important implications in respect to exploration drill targeting and the estimation of grade and tonnes.

Jan 1, 2003

Morning Star Gold aims to enter the ranks of Australia's gold producers, revitalising the Eastern Victorian Goldfi elds in the second half of 2010 - the fi rst gold production in around 50 years from the Morning Star Gold mine, which was once Australia's largest under WMC. This presentation will outline the redevelopment of the Morning Star Gold Mine from exploration to production. Morning Star Gold NL's (MCO) key project area is centred at the historic mining town of Woods Point and nearby Matlock (to the southeast) and Gaffney's Creek (to the northwest), all of which are located in the lower part of the Victorian Alps roughly 60 kms south of Mansfield. Morning Star has literally numerous historic mines and gold bearing 'dykes' on its tenements, many with a rich production history of high-grade gold from quartz reefs and alluvial sources. The area encompassing the Woods Point goldfi eld and the multiple high-grade gold bearing dyke structures located north towards Jamieson and south towards Walhalla formed one of the most significant mining fields in Australian history. Historical gold production was at least 155 t or around six million ounces of over a century of mining with an average production grade exceeding 27 g per tonne. The bulk of this recorded production came from just a handful of mines and of those only three were mined to any great depth. One of the key historical production hubs in this area was the famous 'Morning Star' mine, which is situated adjacent to Woods Point township. The Morning Star mine produced almost one million ounces at 27 grams per tonne, operating fairly continuously between 1861 and 1959 with a break after Jan 1939 due to the devastating 'Black Friday' bush fi res across eastern Victoria. During the early 1940s, the Morning Star was Australia's biggest gold mine. The Morning Star mine along with Walhalla ensured that this goldfield was third behind Bendigo and Ballarat as Victoria's biggest hardrock gold production centre. Morning Star Gold has rebuilt its 100 per cent owned 'Morning Star' mine with a view to producing gold in the second half of 2010. Morning Star is exploring its regional dykes in order to estimate an overall gold endowment and rank local production sources to feed its proposed mill at the Morning Star mine site. Key initial targets (all within 11 kms of the Morning Star mine) are the Waverly, All Nations, Rose of Denmark, Hunts, Wallaby and Loch Fyne dykes, all of which historically produced high grade gold, much of it gained from only shallow workings above the water table in the weathered zone of rocks. Historically the Morning Star mine was developed over 24 levels to a depth of 940 m via one large vertical shaft and a smaller, deeper inclined shaft at the 1900 feet level underground. At present MCO has dewatered and completely refurbished all infrastructure to the ten level (~310 m below surface). MCO knows there are a number of substantially under-explored and undeveloped or partially developed but not stoped areas within the Morning Star mine. As a result, MCO has been carrying out extensive channel sampling and an underground diamond drilling program targeting areas of the mine that were largely unexplored and undeveloped by the last operators of the mine - Western Mining Corp Ltd (Gold Mines of Australia). Four thousand, fi ve hundred pages of archival WMC records have helped the cause significantly. The shaft refurbishment and reconstruction stage is complete. This has been a program that originally commenced back in 1993 and has cost around $22 M. This refurbishment paved the way for the extensive underground resource focused diamond drilling program, which MCO completed in 2008 with two company-owned and operated drill rigs from drill cuddies on level 9 (900 feet underground) of the mine. This drilling, which encountered some stunning grades intersections and multiple visible gold hits, has outlined further production opportunities including 0.4 m @ 1392 g/t Au (MS 410). Metallurgical testing conducted by Gekko Systems of samples obtained from the exploration program found gravity concentration and a leach circuit gave recoveries of ~95 per cent to 99 per cent, or ~92 per cent from gravity alone at a coarse crush (300 ¦m). Currently, the plan is to use gravity to fi rstly produce dore bars on-site from the free milling gold and secondly a saleable concentrate for CIL processing off-site. A purpose built 10 t/h (~80 000 t/a) gravity treatment plant was subsequently ordered from Gekko and is expected to be installed onsite and commissioned in the Q3 2010. The plant features fi ne crushing with a vertical shaft impactor, followed by gold concentration by inline pressure jig, inline spinner and Wilfley table. This is an ABSTRACT ONLY. No paper was prepared for this presentation.

Aug 1, 2010

By D J. Alchin

Most of South AfricaÆs high-grade iron ore resources are hosted within a fault-controlled structural basin in rocks of the Palaeoproterozoic Transvaal Supergroup in the Northern Cape Province of South Africa. Iron mineralisation occurs as individual orebodies in fault-bounded basins or as fold-controlled concordant lenses around an unconformity plane above the Kuruman Banded Iron Formation. The Sishen mine near Kathu and the beeshoek mine and Sishen South deposit near Postmasburg lie on the northern and southern border of a major domal structure known as the Maremane dome, respectively. The effects and structural constraints of at least three orogenic compressive episodes and several intermittent extensional episodes on the formation, erosion and preservation of iron mineralisation on the Maremane dome and surrounding environs were investigated. Ventersdorp impactogenal rift basin development at ~2.78 - 2.64 Ga, finalised with the deposition of the volcano-sedimentary Vryburg Formation during the thermal subsidence stage at ~2.64 - 2.6 Ga, and was followed by tectonic quiescence/stability and an extensive marine transgression across the entire Kaapvaal craton. The drowning event led to the formation of a carbonate platform with the deposition of the Schmidtsdrif and Campbellrand subgroups conformably above the Vryburg Formation at ~2.6 - 2.52 Ga. The initiation of distal (to the west of the Kaapvaal craton) off-craton oceanic rifting, causing submarine volcanism and associated hydrothermal activity, led to the deposition of initially manganiferous chert (Wolhaarkop Formation) followed by banded ironstone formations (Manganore Iron/Kuruman Formation) of the Asbestos Hill Subgroup at ~2.52 - 2.46 Ga. Initial passive margin rifting along the N-S oriented western edge of the Kaapvaal craton, initiated at the end of Ghaap Group time (during Koegas Subgroup deposition) at ~2.46 - 2.35 Ga, formed a prominent system of N-S striking, westerly dipping normal faults. Easterly directed crustal compression in post-Ghaap Group time in response to the Kalahari Orogeny (accretion of Rehoboth craton along western edge (Kalahari suture zone) of the Kaapvaal craton at ~2.35 - 2.24 Ma led to the formation of large-scale regional, N-trending F1-folds. Partial to complete inversion of the Koegas passive margin rift system (ie reverse dip-slip reactivation of the N-S striking normal fault system to high-angle reverse faults and dextral strike-slip reactivation of the Ventersdorp rift system developed in the Archaean basement), was followed by uplift, erosion and formation of a regional angular unconformity (Postmasburg unconformity). Uplift was accompanied by deposition of fluvio-glacial sediments of the Makganyene Formation (Lower Postmasburg Group) within an intracratonic peripheral foreland basin setting unconformable above Ghaap Group strata at ~2.35 - 2.24 Ga. Post-orogenic crustal relaxation and rifting caused extensional reactivation of the N-trending Palaeoproterozoic passive margin rift system and NE-trending Neoarchaean Ventersdorp impactogenal rift system, forming a fault-controlled depository for the volcano-sedimentary Upper Postmasburg Group at ~2.24 - 2.1 Ga. Deceleration in rifting was succeeded by thermal subsidence of the Upper Postmasburg Group rift, erosion, formation of a regional angular unconformity and deposition of clastic sediments of the Lower Olifantshoek Supergroup unconformable above Postmasburg Group strata at ~2.1 - 1.93 Ga. Renewed rifting led to the deposition of volcano-sedimentary units of the Upper Olifantshoek Supergroup within a rift system superimposed on the Postmasburg Group rift depository at ~1.93 - 1.83 Ga. Easterly directed crustal compression during the Kheis Orogeny at ~1.83 - 1.73 Ga led to renewed inversion of rift structures of the Postmasburg Group and Olifantshoek Supergroup depository, N-trending F2 folding and thin-skinned thrusting of older rock units eastwards over the cratonic cover, thereby utilising planes of weakness in the strata such as prominent unconformities and lithological contrast boundaries as principal dTcollements. NNW-directed crustal compression in response to Lomanian (Namaqua-Natal) Orogeny at ~1.15 - 1.0 G along the southern margin of the Kaapvaal craton, resulted in minor sinistral strike-slip reactivation of the N-S striking fault system, the formation of extensional NNW-SSE striking fracture/fault zones and the development of ENE-trending F3 folds forming a F2/F3 fold interference pattern. Post-Lomanian tectonic events (eg the Pan-African Orogeny at ~650 - 500 Ma, the Cape Orogeny at ~310 - 240 Ma, and the Gondwana breakup at 205 - 120 Ma), caused only comparatively minor extensional reactivation of the pre-existing fault systems. Iron mineralisation was ultimately preserved from erosion by Kheis Orogeny-related N-trending F2 synclines and Lomanian Orogeny-related ENE-trending F3 synclines, in particular areas of interference between F2 and F3 synclines representing comparatively deep semi-circular trough- like depressions, as well as in half grabens formed adjacent to reactivated westerly dipping N-S normal faults. Support for relating the iron and manganese mineralisation to structurally controlled hydrothermal fluid flow during the Kheis orogenic event has also been found, and ongoing research is aimed at confirming and refining the hydrothermal model for iron ore mineralisation in the Northern Cape.

Jan 1, 2007