The petrogenesis and Ni-Cu-PGE Potential of the Dido Batholith, North Queensland, Australia
Creators: name: Best, FC
Publisher: name: University Of Tasmania
Year: 2023

description: The Dido Batholith is a large north- to northeasterly-trending batholith, ~90 km long and up to 30 km wide, located along the southeastern margin of the Precambrian Georgetown Region (Greenvale Province), northern Queensland, Australia. It overlaps the contact between the Georgetown Region Precambrian rocks and the Early Palaeozoic volcano-sedimentary units of the northern end of the Tasman Fold Belt System. Hornblende-biotite tonalites and granodiorites are the dominant lithologies comprising this batholith, although an intermediate phase comprising hornblende-biotite diorites and gabbronorites dominates the southeastern quarter. Four elongate, km-scale, and several smaller mafic to ultramafic bodies (UMB) are hosted within this intermediate phase. All UMB are crosscut by abundant, texturally variable felsic to mafic dykes. New U-Pb zircon dates indicate that the diorite-gabbronorite phase crystallised at ~470 Ma, whereas the tonalite-granodiorite phase (named the Main Felsic Mass: MFM), UMB and associated mafic dykes crystallised at ~430 Ma. These new dates have led to the informal renaming of the older dioritic-gabbronorite phase as the Phantom Diorite, whereas the 430 Ma phases remain a part of the Dido Suite. The km-scale UMB, which form the focus of this study, are layered cumulate sequences which represent open-system intrusions emplaced at shallow- to mid-crustal levels (15 ‚Äö- 25 km). They are divided into two petrographically and geochemically distinct varieties: (1) the low-Fe UMB (3 intrusions), comprising dunites, wehrlites, troctolites and olivine gabbro which contain variable amounts of olivine (Fo85 ‚Äö- 72), clinopyroxene (Mg# 0.87 ‚Äö- 0.73), plagioclase (An92-72) and chromites; and (2) the high-Fe UMB (1 intrusion), comprising dunites, wehrlites and pyroxenites which lack chromites and contain abundant, early crystallising Fe-Ti oxides and hornblende and less primitive olivines (Fo78-72) and pyroxenes (Mg# 0.87 ‚Äö- 0.73) than the low-Fe UMB. The high-Fe UMB displays moderate 87Sr/86Sr(430) (0.705932 ‚Äö- 0.706231) and negative ˜í¬µNd(430) (-3.1 to -4.0), whereas the low-Fe UMB displays lower 87Sr/86Sr(430) (0.703836 ‚Äö- 0.705318) and more positive ˜í¬µNd(430) (-0.9 to +3.7) values. Using the composition of cumulus minerals and mafic dykes, it is estimated that the parent magmas of the low-Fe UMB contained 8 ‚Äö- 10 wt.% of both MgO and FeOt , whereas the high-Fe UMB parent magmas were more evolved, having higher FeOt (12 ‚Äö- 16 wt.%) and lower MgO (6.2 ‚Äö- 8.2 wt.%), Ni and Cr contents. The primary magmas of both the high- and low-Fe UMB are interpreted as mantlederived arc rift or back-arc tholeiites. Crustal contamination during ascent is suggested to be responsible for the LREE-enriched and Nb- and Ti-depleted nature of the UMB parent magmas. Two-component isotope mixing models suggest that the addition of variable amounts (&lt;5% in the low-Fe UMB and 9- 10% in the high-Fe UMB) of 2000 ‚Äö- 2500 Ma igneous crustal contaminant to tholeiitic melts derived from a slightly enriched mantle source can account for isotopic compositions of the UMB. Although both the high-Fe and low-Fe UMB are interpreted as initially evolving along the tholeiitic liquid line of descent (LLD), the ultimate differentiation trend recorded by the high-Fe UMB is more akin to calcalkaline fractionation, leading to tonalitic compositions. The higher volumes and relatively late addition of crustal contaminants to the high-Fe UMB magmas (i.e. after they had experienced strong Feenrichment) is suggested to have resulted in this apparent shift in LLD. The 430 Ma Dido MFM is a medium-K calc-alkaline intrusion, with relatively low 87Sr/86Sr(430) (0.706746), negative ˜í¬µNd(430) (-4.8) and a TDM age of ~1390 Ma. It shows fractionated REE profiles ([La/Yb]CN = 9.0 ‚Äö- 10.3) and contains magmatic zircons with negative ˜í¬µHf(430) values (-0.9 to -5.9). The MFM is interpreted to have originated from a fractionated, mantle-derived melt which assimilated ~12% of 2000 - 2500 Ma igneous protocrust during ascent. It is difficult to establish the exact relationship between the different phases of the Dido Suite although it is thought likely that most of the differences in magmatic trends between the individual phases are attributable to the physical conditions of magmatic evolution in the crust, rather than differences in initial magma types as: (a) isotopic differences between the individual UMB and MFM can be explained by variations in the amount of crustal contaminants assimilated into a common, mantlederived magma, and the timing of this assimilation; (b) fractionation of cumulates similar to those comprising the low-Fe UMB likely drove the residual tholeiitic magma to become more enriched in Fe and H2O; and (3) later crustal contamination of such an evolved, Fe-enriched magma, and fractionation of Fe-Ti oxide-rich cumulates to produce the high-Fe UMB, may have generated a calc-alkaline LLD, eventually producing magmas with MFM-like compositions and isotopic signatures akin to the high-Fe UMB. As the latter process would require large volumes of mafic magmas and produce large cumulate sequences not seen at the current exposure level, these processes are required to have occurred at deeper crustal levels. The 470 Ma Phantom Diorite is a medium-K calc-alkaline intrusion. It is geochemically similar to the Dido high-Fe UMB, displaying relatively low 87Sr/86Sr(470) (0.705775 to 0.706100), negative ˜í¬µNd(430) (- 3.0 to -4.3) and TDM ages of 1333 ‚Äö- 1461 Ma, with fractionated REE profiles ([La/Yb]CN = 6.1 ‚Äö- 10.4) and containing magmatic zircons with negative ˜í¬µHf(470) values (-1.64 and -8.69). These similarities suggest that (1) the Phantom Diorite and Dido Suite originated from the mixing of geochemically similar mantle-derived and crustal components and (2) that there was little change in the tectonic setting, and composition of the lithosphere beneath the Greenvale Province between the MidOrdovician (470 Ma) and Silurian (430 Ma). The striking geochemical similarities between the Dido high-Fe UMB and Phantom Diorite suggest both underwent a similar degree of crustal contamination (~8 ‚Äö- 12%). Geochemistry and mineral compositions suggest that the 470 Ma Phantom Diorite and 430 Ma Dido Suite originated in an arc-backarc setting. Furthermore, although no Proterozoic rocks outcrop east of the Dido Batholith (the approximate position of the Tasman Line), the identified involvement of Proterozoic crustal contaminants in the genesis of the Dido Suite supports the ascent of these magmas through the Georgetown Region Precambrian crust of the North Australian craton. This, in turn, indicates genesis in a continental margin (Andean- or Mexican-type) arc setting, probably in an arc that was actively rifting, given the tholeiitic nature of the primary magmas of the Dido UMB (and possibly the Dido MFM and Phantom Diorite). This finding largely supports the presence of a west-dipping subduction zone beneath the Greenvale Province during the Ordovician and Silurian. As most of the large Ni-Cu-Platinum-group element (PGE) deposits worldwide have formed where mantle-derived melts intersect or are focussed along large faults in continental rift zones or rifted continental margins, Anglo American plc identified the southeast margin of the Georgetown Region, and specifically the Dido UMB, as a target for magmatic Ni-Cu-PGE deposits. No mineralisation has been found associated with the UMB. Rocks comprising the low-Fe UMB contain &lt;1000 ppm Cu and &lt;40 ppb of both Pt and Pd, whereas the high-Fe UMB rocks have similar Cu concentrations to the former but are generally more PGE-enriched (containing up to 160 ppb of both Pt and Pd). Geochemical discriminators suggest that the magmas that formed the km-scale UMB were chalcophile elementdepleted, having undergone a previous S-saturation event (i.e. significant sulphide-deposition) at depth. Furthermore, based on their lower Cu/Zr ratios and highly Ni-depleted composition, the high-Fe magmas are interpreted to have experienced greater chalcophile metal loss than the low-Fe magmas. The PGE-enrichment in the high-Fe cumulates is therefore explained by the addition of PGE to the high-Fe magmas from an external source. Many economic Ni-Cu-PGE intrusions are interpreted as being formed from (a) the addition of batches of PGE-enriched magmas to resident, chalcophile element-depleted magmas (e.g. the Marac‚àö¬8s deposit); or (b) scavenged PGE-rich sulphides which were carried to accessible crustal levels by later injections of magma (e.g. the Platreef). Either of these mechanisms could potentially account for the minor PGE-enrichment in the high-Fe UMB. Although there is no evidence to suggest that large volumes of PGE-enriched sulphides were added to the Dido UMB magmas, considering the minimal exploration completed to date and the new PGE data suggesting the likely presence of significant volumes of PGE-rich sulphides at depth in this magmatic system, the UMB cannot be ruled out as potential targets for Ni-Cu-PGE deposits. Furthermore, although convergent settings rarely host economic Ni-Cu-PGE mineralisation, important exceptions such as the Aguablanca deposit (Spain), indicate that feeders or conduits to intrusions emplaced in local extensional regimes within subduction-related environments can generate important Ni-Cu sulphide deposits. Small mafic intrusions in convergent margin settings, particularly where local extension regimes are evident, should therefore not be overlooked in exploration for new Ni-Cu sulphide deposits and the remaining unexplored Dido UMB, including the high-Fe varieties and any other contemporaneous mafic-ultramafic intrusions in the surrounding area, should be evaluated on a case by case basis.