Paragenesis of gold-sulphide mineralisation Wyoming One and Caloma Two Tomingley Gold Project

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Paragenesis of gold-sulphide mineralisation Wyoming One and Caloma Two Tomingley Gold Project Macquarie Arc Conference / AIG Honours Bursary Alexander Cherry Supervisors: A/Prof. David Cohen Dr. Ian Graham

Site location Modified from Glen et al. (2007)

The Tomingley Gold Deposits K-Ar age date of mineralisation 453.3 9.2 Ma Late Ordovician Interpreted age of Mingelo Volcanics 463-455 Ma (Crawford et al., 2007) Interpreted age of Cotton Formation Latest Ordovician to Early Silurian (Percival and Glen, 2007) Image courtesy of Terry Ransted

Wyoming One and Caloma Two Images courtesy of David Meates

Aims Describe the paragenesis of the TGP deposits Describe the mineralogy Determine the nature of the gold/sulphide relationship. Has gold been remobilised? Assess the sulphur isotope signature of the deposits. Assess the orogenic classification of the TGP.

Orogenic vs. Intrusion-Related From Goldfarb et al., 2005

Orogenic vs. Intrusion-Related Characteristics Orogenic Au Intrusion-Related Au Tectonic setting Deformed continental margin arcs, emplaced in structural highs during late compression Deformed continental margin, emplaced during transition to extensional regimes Structural complexity Mineralisation style/geometry Overprinting Mineralisation assemblages Relative timing of emplacement Potential metal/fluid sources Variable, high complexity common, particularly in brittle-ductile regimes Structurally controlled; large veins, vein arrays, saddle reefs, replacement of Fe-rich rock Strong overprinting common; multiple vein events common Reduced sulphides (e.g. Py, Apy Po, Loe, Sb, Hg), minor base sulphides Late synorogenic Subducted/subcreted crust and/or supracrustal rocks and/or deep granitoids Usually little complexity Commonly sheeted veins, lesser breccias, veins and disseminations Possible minor overprinting due to later structures Reduced sulphides (e.g. Py, Apy Po, Loe, Cpy, Sph, Gal) Polymetallic assemblages common (e.g. Mo, W, Sn) Post deformational Shallow granitoids and/or supracrustal rocks

Methods 1. Visual Mineralogical Logging Petrography 2. Qualitative Electron microprobe mapping Backscatter electron images X-ray Diffraction 3. Elemental field portable X-ray Fluorescence ICP-OES Company assays 4. Quantitative Electron microprobe point analysis Sulphur isotopes

Alteration Feldspars altered to albite Sericite replacement of feldspars Carbonate spotting Chlorite replacement

Veins Early quartz veinlet Calcite veinlet Quartz-ankerite veins

Mineralisation (Py and Apy) Fine opaque diagenetic pyrite/pyrrhotite grains Fine Apy inside a larger, subhedral Py Py Apy Py Apy

Mineralisation (Cpy and Sph) Sph with Cpy rimming Py Sph with Cpy Cpy Au Sph Cpy

Mineralisation (Au)

Gold - sulphide relationship Gold <1 to 45 μm grains. Fracture controlled. Remobilisation unlikely. Sulphide At least two generations of pyrite and arsenopyrite. Chalcopyrite and sphalerite occur as cavity and fracture fill and fine irregular grains. Before nitric acid etching After nitric acid etching Relationship Gold, chalcopyrite and sphalerite; coeval and relatively late.

Electron Microprobe Maps - BSE

Electron Microprobe Maps

Electron Microprobe Maps - BSE

Electron Microprobe Maps

S-isotopes and potential fluid sources Bulk rock δ 34 S signatures determined through aqua regia digestion of five samples. Similarity of signatures suggests nearby black shales being a potential source of sulphur. Sample No. δ 34 S Sulphide VCDT Wyoming One -8.2 Pyrite Wyoming One -8.6 Arsenopyrite Caloma Two -8.1 Pyrite Caloma Two -7.7 Arsenopyrite Caloma Two (unmineralised) -7.8 Pyrrhotite (black shale) The black shales may have been the main sulphur source. Prograde metamorphism of diagenetic pyrite to pyrrhotite may have overprinted the original δ 34 S signature of ore sulphides. δ 34 S values between -8 and -1 were found by Downes (2009).

Paragenetic sequence

Orogenic vs. Intrusion- Related Most likely to be orogenic Deformation of mineralisation Only minor base metals observed (Cpy and Sph) Gold fineness is typical for orogenic deposits (approx. 875) Occurrence of Au mineralisation all along the Parkes Thrust Kink bands Bent albite twins From Downes, 2009

Main Findings Sulphides appear to have been emplaced over more than one event. Gold is later than but is spatially associated (fracture controlled) with the main pyrite and arsenopyrite. And appears to be temporally associated with chalcopyrite and sphalerite. More likely to be orogenic than intrusion-related. The mineralogy of the two drill holes/deposits are very similar. Main difference between deposits is structural. Further work is needed! More S-isotopes, LA-ICPMS. Extend to the other two deposits.

Thanks to: The AIG for the bursary support and to SMEDG for the opportunity to present tonight. Supervisors: Dr Ian Graham and A/Prof David Cohen Alkane Resources: Terry Ransted and Dave Meates UNSW Analytical Centre: Dr Karen Privat, Dr Yu Wang and Dorothy Yu Thin sections: Joanne Wilde Isotopic Inc.: Dr Anita Andrew

Lithologies

Geochemical classification of lithology Winchester and Floyd, 1977 Pearce et al., 1984

Image courtesy of Terry Ransted

Wyoming One drill hole base metal assays against gold grade

Caloma Two drill hole base metal assays against gold grade