Calcrete Sampling for Gold Exploration

Resurgence in Au exploration during the past decade has been characterised by a considerable emphasis and dependence on geochemical procedures. This has been made possible, firstly, by marked improvements in analytical sensitivity over those previously available and secondly, of particular importance to exploration in Australia, by a better understanding of the distribution of Au in the regolith, which has led to the optimisation of sample media. These developments have given exploration companies the ability to seek and detect subtle and widespread geochemical signatures of concealed Au mineralisation and provided an enhanced capability to interpret the data. As a consequence, several new discoveries have been made, even in areas that have been intensively explored in the past. In the deeply weathered Yilgarn Craton (WA), and in equivalent areas elsewhere in Australia and overseas, Au has accumulated in the upper lateritic gravels and duricrusts of the regolith, probably during humid climatic periods in the Tertiary. The laterites may not only be Au ores in themselves, but research by CSIRO and CRC LEME has shown them to be very important sample media, (eg Anand and Smith, 1992). In many areas, however, the laterite has been eroded and hence is unavailable as a sample medium and chemical modification under more and conditions since the Tertiary has leached Au from the upper saprolite. This has greatly increased the difficulties of exploration, particularly where reliance was placed on sampling between 2 and 15 m of the surface. Further research, however, has demonstrated that, despite this leaching, recent remobilisation of An has caused it to concentrate in a specific soil component, pedogenic carbonate, usually in the top I - 2 m, thereby giving surface expression even to mineralisation that is concealed by over 20 in of leached overburden. Secondary carbonates, commonly referred to as calcrete, may precipitate as calcite and/or dolomite in regoliths where the average annual rainfall is less than about 600 mm. Pedogenic carbonates are those that form in unsaturated (vadose) soil horizons. They are widely distributed in the Gawler and Yilgarn Cratons. In the Yilgarn Craton south of about 30¦S ('the Menzies Line'), they are seemingly more abundant over more basic rocks and towards the south east (Figure 1). In contrast, groundwater calcretes form in saturated (phreatic) environments, typically in the axes of major drainages north of the Menzies Line. These are known to accumulate economically-significant grades of U but not, apparently, An.