AusGeo News June 2011 Issue No. 102
Gravity datasets point to a link between the Mount Isa and Broken Hill mineral provinces
The Broken Hill Block and the Eastern Succession of the Mount Isa Inlier are two of the most highly mineralised provinces in Australia. They are also among the most highly mineralised Proterozoic provinces in the world.
Since the early ideas of Bill Laing, a consultant and academic (Laing and Beardsmore 1986; Laing 1996), for a 'Diamantina Orogen' connecting the Eastern Succession of the Mount Isa Inlier with the Broken Hill Block, similarities in the geological histories of these provinces have led many researchers (such as Betts et al 2002; Giles et al 2004; Betts and Giles 2006) to infer that they were contiguous through much of the Proterozoic. These similarities, which are detailed in Kositcin (2010) and illustrated in Figure 1, include:
Although there is a general consensus that these provinces were contiguous through much of the later Paleoproterozoic, the relative position and orientation of these provinces when they were contiguous is contentious.
The Broken Hill Block contains the world's largest single sediment-hosted zinc-lead-silver deposit (Broken Hill) plus a number of small iron-oxide-copper-gold (IOCG) deposits (for example, Portia, Kalkaroo). The Eastern Succession contains major IOCG deposits (such as Ernest Henry, Mount Dore, and Mount Elliott) as well as a number of significant sediment-hosted zinc-lead-silver deposits (for example, Cannington, Pegmont). The zinc-lead-silver deposits in both provinces formed at ~1690 to 1680 Ma, whereas the iron-oxide copper-gold deposits formed between ~1520 and 1500 Ma (King and Thomson 1953; Page and Laing 1992; Gibson and Nutman 2004; Huston 2009; Duncan et al 2011).
To account for similarities presented above, Betts et al (2002) and Giles et al (2002, 2004) proposed that the Kimban Orogeny (and the Strangways Orogeny in the Arunta Province) was a consequence of collision between the Gawler Craton (as part of the Mawson Continent) and the North Australian Craton (including the Arunta and Mount Isa provinces) between around 1740 Ma and 1690 Ma. Betts and Giles (2006) modified this model so that crust east of the Kalinjala Mylonite Zone in the Gawler Province was originally part of the North Australian Craton and the proto-Gawler Province to the west was the colliding terrane during the Kimban-Strangways Orogeny. In these models, the ~1720 Ma Kimban Orogeny is interpreted to connect with the Strangways Orogeny in the Arunta Province to form an approximately east–west trending collisional belt. This interpretation requires the South Australian Craton (including the Gawler and Curnamona provinces) to be rotated 52 degrees counterclockwise relative to its current position. This places the Curnamona Province adjacent to the current southern subsurface extent of the Mount Isa Province and Georgetown Region (Giles et al 2004) thus linking the Eastern Succession and Willyama Supergroup (Broken Hill Block) as part of the same stratigraphic package.
Alternatively, based on studies in the Mount Isa Province Gibson et al (2008) proposed a Basin-and-Range-style model in which crustal evolution was dominated by extension along the eastern margin of Proterozoic Australia. In this interpretation, the north-south relative positions of the North Australian and South Australian cratons did not change significantly through the Paleo- to Mesoproterozoic.
Hence, there is significant controversy as to the relative position, rotated or not, of the Gawler and Mount Isa provinces. Potential field datasets, including gravity and aeromagnetic datasets, have the potential to resolve this controversy as large-scale geophysical trends should be less susceptible to re-orientation and have fewer complexities of interpretation than geological datasets. However, the age of geophysical trends, in many cases, cannot be established conclusively. Figure 2a illustrates the variations in the Bouger gravity field for the eastern margin of Proterozoic Australia. This dataset and the aeromagnetic dataset are characterised by a major (under cover) boundary along the southern margin of the Mount Isa Province that truncates a broadly north–south geophysical grain.
Although less certain, the geophysical data in the Curnamona Province are also characterised by a north–south grain and a northern boundary (Boundary 2 on figure 2b) sub-parallel to the boundary that defines the southern margin of the Mount Isa Province (Boundary 1). To further assess this north–south trend, Figure 2b juxtaposes the Curnamona Province with the Mount Isa Province using the sub-parallel boundaries discussed above. This fit is remarkable: not only are the trends continuous, but individual linear anomalies in the gravity dataset can be traced across the province boundaries. If the Curnamona Province was rotated 52 degrees counterclockwise relative to the Mount Isa Province, the trends should not be traceable across the now separated province boundaries. This relationship is considered to favour a simple geological link without rotation, which is more consistent with models such as Gibson et al (2008) and the original interpretations of Bill Laing.
The white band in Figure 2b is intended to indicate that the Broken Hill Block and the Mount Isa Eastern Succession were not juxtaposed directly. Rather, they would have been separated by attenuated crust. The zone between the two boundaries in Figure 2a is characterised by crust that is significantly thinner than crust in either the Broken Hill Block or the Mount Isa Eastern Succession (30 to 35 kilometres, including ~5 kilometres of Paleozoic basins, compared to 40 to 45 kilometres, or more: Collins 1991; Meixner and Holgate 2009). It is possible that the attenuation of the crust was accompanied by granite emplacement (Meixner and Holgate 2009), as indicated by the large gravity lows in Figure 2a.
This reconstruction has important implications for the mineral potential of Proterozoic Australia, particularly its eastern margin. The Curnamona and Mount Isa Provinces are some of the most highly mineralised provinces in the world, and large parts of these provinces are under cover. The reconstruction discussed above suggests that the southern extension of the Mount Isa Province under cover has high potential for both sediment-hosted zinc-lead-silver and iron oxide copper-gold deposits. This potential will extend into the inferred attenuated crust between the two boundaries. In addition, younger parts of the Curnamona Province, particularly the Paragon and Sundown Groups, may have potential for sediment-hosted zinc-lead-silver deposits akin to the Mount Isa and Hilton-George Fisher deposits.
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