Mining 101

1. Metals and Minerals The building blocks of the earth are called elements, which are substances that cannot be broken down by chemical or physical action into simpler entities. Elements that are ‘'workable’' (eg malleable) are termed metals (they are also usually good conductors of heat and electricity). Of the 92 elements, eight account for 98% of the composition of the crust (the earth''s outer layer; see later): oxygen (46.5%), silica (27.5%), aluminium (8%), iron (5%), calcium (3.5%), sodium (3%), potassium (2.5%) and magnesium (2%). By contrast, gold constitutes less than 0.0000004% of the earth''s crust. Elements bond together in chemical compounds of definite ratios to form solid crystalline substances known as minerals, of which there are many thousand different types. (Coal is a mineral, mainly comprising the carbon element.)
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Rock is a solid mass of mineral grains, and there are four main rock-forming mineral groups: Silicates - contain silicon and oxygen Oxides - the elements bond to oxygen Sulphides - the elements bond to sulphur Carbonates - the elements bond to carbon/oxygen. The most common minerals are all oxides: SiO2 (comprising 59.1% of the earth''s crust), Al2O3 (15.2%), CaO (5.1%) and FeO (3.7%). Where minerals are sufficiently concentrated (see later), they are called ‘'mineral deposits’' and these become ''ore deposits'' when the elements within the mineral can be recovered economically. Mining is usually about the recovery of the ‘'metal’' elements. These concentrations are usually measured as the proportion of the constituent metal in the overall deposit (this might include several different minerals but the measurement will exclude the surrounding ‘'waste’' rock). For the less valuable metals (copper, lead etc) this is usually measured as a few parts per hundred (eg 3% copper; Cu) while the precious metals will be measured in terms of parts per million (eg 6 grams/tonne gold; Au). Note that there are 1,000 grams in a kilogram and 1,000 kilograms in a tonne, so that 1 gram/tonne = 1 ppm. The search for diamonds is akin to looking for the proverbial ‘'needle in a haystack’'. Diamond grades are typically 5 carat per 100 tonne (the normal ‘'unit’' of measurement), ie 1 gram for every 100 tonnes (1 part per 100 million). Because of the huge range in the value of diamonds (based on size, colour and clarity), grades are often given in terms of value. A typical mined-diamond value is US$200/carat, ie an ore grade of only US$10/tonne in the example above. Note also that if the size of the average stone is 1 carat, then there will only be one stone per 20-tonne truck ! As an aside, it is often said that only one kimberlite pipe in one hundred is diamondiferous, and only one diamondiferous pipe in a hundred is economic to mine.
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Metals are often categorised into groups to reflect common usage or properties. Precious (Noble) Metals These are resistant to weathering (ie they do not rust) and are usually mined in their native (ie pure, elemental) state. Examples are gold, silver and the platinum-group metals (PGMs). Base Metals So called because they are capable of combining with an acid to form a salt, eg: Copper - Chalcopyrite (CuFeS2) and Chalcocite (Cu2S) Lead - Galena (PbS), Anglesite (PbSO4) and Cerusite (PbCO3) Zinc - Sphalerite (ZnS) and Smithsonite (ZnCO3) Nickel - Pentlandite (2FeS.NiS) and laterites Ferrous Metals In addition to iron itself, this category includes those metals that have a strong chemical affinity with iron, eg: Chromium - Chromite (FeCr2O4) Cobalt - Cobaltite (CoAsS) and Smaltite (CoAs2) Molybdenum - Molybdenite (MoS2) Manganese - Braunite (Mn2O3), Hausmanite (Mn3O4) and Pyrolusite Non-Ferrous Metals These are the metals that have no affinity with iron (and also included the base metals), eg: Aluminium - Bauxite (Al2O3.2H2O) Magnesium - Magnesite (MgCO3) and brines Tin - Cassiterite (SnO2) Speciality Metals These are those metals whose unusual (exotic) properties make them valuable in specific usages, eg: Cadmium - Greenockite (CdS), which is found as a coating on zinc ores, and is usually mined by-product of base-metal sulphides Mercury - Native metal and as Cinnabar (HgS) Titanium - Ilmenite (FeO.TiO2) and Rutile (TiO2) Zirconium - Zircon sand and Baddeleyite Other Mined Minerals These are those valuable minerals that either can not be characterized as metals (eg coal) or where the mineral is used in its mineral form without extracting the metal (eg salt, which is sodium chloride): Industrial minerals - Salt, limestone, marble etc Energy minerals - Coal, oil, gas and uranium Gemstones - Diamonds, rubies etc
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2. Geology\r\n\r\nThe consensus amongst scientists is that our solar system began about 5,000 million years ago, and planet Earth formed from a superheated cloud of dust and gas (following the ‘'Big Bang’'). The Earth is believed to comprise a deep interior (the core), surrounded by a zone of heavy rock (the mantle) and a thin outer skin (the crust). Cooling from the core outwards sets up convection currents, and as these reach the crust the patterns they set up have been instrumental in forming a series of interlocking crustal plates.\r\n\r\nPlate tectonics is a relatively new theory and has revolutionised the way geologists think about the Earth. The size and position of the plates change over time. The edges of the plates, where they move against each other (the so-called mobile belts) are sites of intense geologic activity; such as earthquakes, volcanoes and mountain building (and mineralisation). Periods of mountain-building are referred to as orogeny, the most recent of which started 200 million years ago (about the time the first mammals appeared).\r\n\r\nWhere plates ‘'collide’', one plate might slide beneath (subduction), or ride above (obduction), another plate. Such movements are often accompanied by the intrusion into the crust of molten rock (magma) from the mantle. The magma cools to form igneous rock.\r\n\r\nThere are broadly two types of igneous rock:\r\nLight (felsic) rocks that are rich in silica and aluminium, eg granites.\r\nDark and heavy (mafic) rocks rich in iron and magnesia, eg gabbro.\r\n\r\nWhere the magma reaches the surface of the crust it is extruded and cools very quickly as lava to form fine-grained volcanic rocks, eg basalt.\r\n\r\nThe igneous activity associated with mobile belts is often accompanied by the introduction of hydrothermal fluids rich in minerals, giving rise to some of the world''s biggest mineral deposits (eg the copper deposits of the Andes). A present-day example of such hydrothermal activity is in the South Pacific where ‘'black smokers’' on the seafloor are currently depositing metal sulphides along the junction of two tectonic plates.\r\n\r\nOver geological time, some plates fuse together and new ones form, and, away from the edges of existing plates, the older rocks form the ancient ‘'basement’', or cratons (also termed shields). ‘'Fossilised’' mobile belts are preserved in cratons as Greenstone belts, which are a major source of gold deposits (eg in Western Australia, the Canadian Shield and West Africa).\r\n\r\nThe crust and its plates are subject to constant erosion and the resultant material is re-deposited as sediment in rivers, lakes and seas, eventually consolidating into layers or strata – sedimentary rocks.\r\n\r\nThese sedimentary rocks fall into two categories:\r\nClastic - Fragments brought together by ice, water or wind (eg sandstone).\r\nChemical - Precipitation of dissolved materials (eg forming limestone); with evaporates (eg rock salt from sea water) being a particular type.\r\n\r\nIn many areas of the globe, sedimentary rocks cover the basement and cratons entirely. Minerals contained in the sediments may accumulate in economic quantities.\r\n\r\nOver millions of years, sedimentary rocks are subject to heat and pressure as a result of igneous intrusions, mountain-building activity or the weight of the overlying sediments, to form metamorphic rocks. Hence a limestone becomes a marble, shale becomes a slate, sandstone becomes a quartzite, etc. The gold deposits of South Africa''s Witwatersrand and the iron-ore deposits in the Pilbara district of Western Australia are examples of sedimentary deposits that have been metamorphosed.\r\n\r\nAccording to the amount of heat and pressure, the original sediments can eventually be metamorphosed to schists, and volcanic/igneous rocks can be metamorphosed to form gneisses. Metamorphism often remobilises and reconcentrates the contained metals to form new deposits. The world''s cratons consist entirely of metamorphic rocks.
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General Deposit Types Sedimentary deposits can be in the form of lenses and pods, often deposited along bedding planes or in fractures, faults and fissures. Under certain conditions, eg warm climate and shallow seas, sediments accumulate in large basins, and minerals become increasingly concentrated as salts as a result of evaporation. Many of the world''s large deposits of potash, nitrate, phosphate and rock salt have formed in this fashion. Deposits in igneous rocks can also occur as lenses and pods, and in fractures, faults and fissures. They can also be distributed through the rock as fine disseminations and in small quartz veinlets as stockworks (typical of porphyry copper). Such deposits tend to be of large size and low grade. They often possess a surface (or supergene) zone that has been enriched in metals as a result of weathering. Beneath this zone, the ore unaffected by weathering is termed primary (or hypogene). Massive deposits (see below) are of higher grade and consist almost entirely of sulphide minerals. They are generally associated with metamorphic terrain. Where their deposition is associated with volcanic activity, they are termed volcanic massive sulphides (VMS). Where deposits associated with volcanic activity are stratified they have been referred to as sedimentary exhalative (sedex) deposits. A number of the world''s most important deposits of nickel, chromite, copper and platinum occur in mafic rocks (see above) in layered igneous intrusions. The metals occur at distinct horizons, reflecting the pressure and temperature at which they formed as the magma cooled down. The platinum and palladium deposits of the Bushveld complex in southern Africa are of this type. One particular type of mafic rock, kimberlite, is the world''s principal source of diamonds. Diamonds are formed (from carbon) in the mantle under extreme temperature and pressure, and are carried to the surface in kimberlite pipes. These occur throughout the world but very few contain diamonds, and even fewer have diamond concentrations of economic interest (as noted above). Alluvial deposits are formed where material resulting from weathering and erosion is transported by rivers and streams and re-deposited. The mineral must be chemically stable and physically resistant to survive the process (restricting such deposits to precious metals, diamonds and other gemstones). Alluvial deposits are relatively recent in age and are generally unconsolidated. Laterite deposits are a product of tropical weathering and comprise a mixture of oxide and hydroxide minerals and clays. Bauxite, the chief ore of aluminium, is a laterite, and there are vast deposits in Brazil and Guinea. There are also important deposits of nickel laterite (eg in New Caledonia and Cuba). Where mineral deposits are formed at the same time as the host rock they are termed syngenetic. Where they have been introduced afterwards, they are termed epigenetic.
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Deposit Summary Diamond Pipes: Formed at least 150 km below the surface (where temperatures and pressures are extreme enough to create diamonds, rather than graphite or coal, from the element carbon). These kimberlite mineral accumulations only become economic when they are brought to the surface by volcanic activity. Epithermal: Formed by hydrothermal volcanic activity that pushes magma (and the contained minerals) through vents (to form extensive vein systems). An important source of gold and silver, normally as ‘'native’' metal rather than in a mineral (and are the most likely type of deposit for high-grade, ‘'bonanza’'-type discoveries). Laterites: A deeply weathered mixture of oxide and hydroxide minerals and clays (usually found in the tropics). These form the main orebodies for aluminium, and an increasingly important source of nickel (although recovery of the latter is a still problematic process). Lode: Found in Greenstone belts (see above), these deposits are an important source of precious metals and cluster around large regional fault zones. Although usually narrow and inconsistent (and so hard to identify) they can extend to great depths. Magmatic: As molten rock cools, the minerals crystallise and sink to the base. They are usually tabular, or lens-like, in shape, and form many of the world''s great base-metal sulphide deposits, especially copper and nickel (and also some oxide deposits of iron, titanium and chrome). Massive: Nothing to do with size, rather a mineralisation (made up almost entirely of sulphides) that is homogeneous and conforms to the host rock''s structure (usually indicating that it was formed at the same time). These orebodies are relatively easy to understand and mine. Placer: Minerals that have been eroded from the primary source and transported (normally by water action) and then deposited in a sedimentary bed. The mineral must be chemically stable and physically resistant to survive this process (restricting such deposits to precious metals and gemstones). Porphyry: Typical of deposits (especially copper) formed by igneous activity, with both the intrusion and host rock being severely fractured, with the mineralisation forming veins. The deposits are usually large but low grade, although subsequent leaching and precipitation can form areas of substantially higher grades (supergene enrichment).
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3. Exploration As mentioned above, minerals must group in a sufficient concentration if they are to be economically recovered. This circumstances that are likely to lead to this process must be understood, and suitable locations identified, before a deposit stands any realistic chance of being identified. Geologists will examine general structural maps (rock types and faulting patterns) before making a decision on where to drill. Most of the world''s mines are centred on the ancient ‘'shield’' rocks of the Precambrian orogeny (comprising the Archaean period of 4.6 billion to 2.6 billion years ago, and the Proterozoic period of 2.6 billion to 570 million years ago). This is because the mountain-building activity, which helped concentrate many minerals, was intense in this early period of the planet''s life. The stages of exploration for these various orebodies might include: Geophysical Surveys - Airborne evaluation of magnetic or density anomalies, which are good indications of areas prospective for mineral deposits. Mapping - Consolidation of the surface expressions into a single plane for better understanding of the likely deposit configuration. Sampling - Collection of stream sediments, surface boulders or earth (the latter usually from trenches dug across a prospective area). The material is then analysed to test for anomalous concentrations of metals to establish drilling targets. Drilling - Recovery, for analysis, of either rock chips (at various depths) or cores (collection of the latter is by using diamond-encrusted circular drill bits and core barrels). Modelling - Evaluation of grades and known structures (often using computer models) to determine the likely deposit configuration. Infill Drilling - The drilling of extra holes to increasing confidence in the orebody model. Feasibility Studies - Various scenarios tested (at different metals prices) to determine if the deposit can be extracted profitably. The last such study is called a ‘'bankable’' feasibility study as it is used to secure funding. There are various classifications for ore deposits, depending upon the certainty that the configuration is understood (this is usually a function of the number of drill holes): Inferred Evidence suggests that there are minerals worth investigating; sometimes described as ‘'Potential’'. Resource - Indicated: Initial drilling has identified that there is mineralisation but the configuration is uncertain. - Measured: Tonnage has been calculated but drilling not sufficient to be sure of the orebody''s continuity. Reserve - Probable: Further testing has raised the level of confidence such that initial funding can usually commence. - Proved: Orebody is well understood, and the tonnages and grades established beyond reasonable doubt.
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