Uranium ore-forming systems of the - Geoscience Australia

Uranium ore-forming systems of the Lake Frome regionsuggest that the Beverley and Four Mile deposits were unlikely to have formed along the samefluid flow pathway, as discussed below.The present-day groundwater flow in the proposed Four Mile East mining zone was modeled byJeuken (2008). His conceptual model was similar to the model depicted in Figure 7.3, thoughJeuken (2008) used a pseudo-3D modeling approach using a multi-layer 2D geometry. Accordingto the results of his modelling, the groundwater is expected to flow to the north-east, through thehydraulic constriction across the Poontana Fault Zone and then to the east into the Lake Fromearea (Figures 7.8 and 7.9 in Jeuken, 2008). The recharge to the Eyre Formation is mostly frominfiltration to the southwest of the Four Mile deposit where the Eyre Formation crops out. Jeuken(2008) concluded that the conceptual model is hydraulically feasible, and can be further calibratedusing realistic aquifer properties and boundary conditions that are supported by real data.In our models, most of the fluid recharge occurs within the Eyre Formation, both for pre-, andpost-Paralana Fault groups of models (for example, cf. Figs 7.4 and 7.7). This raises the questionof the source of uranium, as most of the fluid flow bypasses the MPI (mostly, “runs off”). In part,this problem was considered separately in a group of models where we imposed a layer of MtPainter rocks with permeabilities higher than the permeabilities of the Eyre Formation.For the tested range of scenarios, the exposed top of the Paralana Fault (if characterised bypermeabilities equal to, or higher than the permeability of the Eyre Formation) acts simultaneouslyas a zone of major recharge of a surficial fluid component, and minor discharge of deeplycirculated fluids into permeable units below the surface. The fluids discharged at the top of theParalana Fault could have penetrated to significant depths and could have been heated totemperatures from 50 to 200°C (Figs. 7.4 to 7.6, and 7.8, 7.9). The geochemical modellingcalculations of Brugger et al. (2005) and Jaireth et al. (2008b) imply contributions of relatively“reduced” and “oxidized” fluids with different uranium-bearing capacities. In particular, thefluids re-equilibrated with the Mt Painter rocks at elevated temperatures will have limited capacityto transport significant uranium. In any case, the fluid fluxes associated with the discharge fromthe the Paralana Fault are 1-2 orders of magnitude less than fluid fluxes associated with thesurficial fluids recharging within the Eyre Formation.Given the limitations imposed by the boundary conditions of the tested models (namely, the top ofthe models is open to fluid flux but is set to a fixed temperature), we cannot model the dischargeof the heated Paralana Spring waters onto the surface of the model. However, the model doesdemonstrate heat transport along the Paralana Fault when we specify slightly elevatedpermeabilities of rocks within the Mt Painter Domain (e.g., the change from 10 17 to 10 16 m 2 ,Figs 7.4 to 7.6).In the case of “single-domain” MPI models (where the tracer was initially distributed exclusivelywithin the coherent MPI rocks), the tracer is quickly leached from the MPI block, starting from thetop western part of the model (e.g., Fig. 7.4) (note that the striping in tracer plots in Figs. 7.4, 7.6and 7.7 is a plotting artefact). Analysis of the intermediate calculation results (i.e., within 0 to10,000 years) shows that the tracer is partially removed through a minor discharge zone within theEyre Formation, but also propagates to the east within the Eyre Formation (still visible in Fig.7.6). The tracer exhibits similar behaviour in all the models, with most of the tracer washed outfrom the depicted parts of the Paleogene and Neogene units by 10,000 years. Within the “layereddomain”models, the tracer displays similar behaviour as well, with Figs. 7.8 and 7.9 alsodemonstrating propagation of the tracer from the top MPI layer deep into the Paralana Fault Zone.The simple fluid flow pattern observed in virtually all models (namely, the eastward flow withinthe Eyre Formation and, the Cadna-owie Formation in non-overpressured models) has verystraightforward implications for the genetic models for the Four Mile and Beverley deposits. ThePage 87 of 151