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Invisible gold revealed in supergene and hypogene environments

Invisible gold revealed in supergene and hypogene environments

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<strong>Invisible</strong> <strong>gold</strong> <strong>revealed</strong> <strong>in</strong> <strong>supergene</strong> <strong>and</strong><strong>hypogene</strong> <strong>environments</strong>M<strong>in</strong>erals Down UnderRob Hough, Ryan Noble, David Gray


Hidden depositsInsert presentation title


Yilgarn Craton – Sal<strong>in</strong>ityModelledgroundwatersal<strong>in</strong>ities <strong>in</strong> theYilgarn Craton(Comm<strong>and</strong>er, 1989)KilometresInsert presentation title


Dissolved Au Concentration – Yilgarn Craton706050Frequency(%) 40NorthernCentralKalgoorlie3020100.005 - 0.010.01 - 0.020.02 - 0.040.04 - 0.10 - 0.00500.1 - 0.20.2 - 0.40.4 - 1> 1Insert presentation titleDissolved Au range (ppb)


Supergene depletion of Au <strong>in</strong> the Yilgarn CratonKilometresInsert presentation title


Complex regolith materialsInsert presentation title


Laser ablation transect of Au distributionInsert presentation title


Alunite rich ve<strong>in</strong>s with<strong>in</strong> slabby ferricrete (transported) Mount GibsonBulk analyses of: Au 0.1 ppm, As 36 ppm, Cu 85 ppm.Au: 2.9 ppmCu: 320 ppmAs: 430 ppmPb: 420 ppmAu: 1.5 ppmCu: 280 ppmAs: 340 ppmPb: 560 ppmF<strong>in</strong>e-gra<strong>in</strong>ed, Fe-sta<strong>in</strong>edkaol<strong>in</strong>ite/aluniteAu: 1.6 ppm, As: 360 ppm, Cu:290 ppm. Pb: 700 ppm(EMPA/LA-ICPMS)300 μmHough et al., 2005; 2007Insert presentation title


4Dissolved Au vs. Fe (pH < 5.4)AuCl 2- + Fe 2+ + 2H 2 O ⇒ Au (S) + FeOOH + 2Cl - + 3H +Dissolved Au (ppb)321pH 3.4,Eh 600 mVNorthernCentralKalgoorlieEastern215 ppmFe00 10 20 30 40 50 60Insert presentation titleDissolved Fe (ppm)


Golden Virg<strong>in</strong> Pit, Parker Range (WA)Insert presentation title


Primary <strong>gold</strong> <strong>in</strong> quartz, iron oxide (after sulphide).13-15 % Ag <strong>in</strong> the Au-Ag gra<strong>in</strong>s4 mmsulphidef<strong>in</strong>e Au <strong>in</strong> qz1 mmInsert presentation title


Quartz ve<strong>in</strong> block from 30 m depthIron oxide rich fracture surface100 μm1cmInsert presentation title


SEM: Back-scattered electron imagesInsert presentation title


Th<strong>in</strong> films – overlap illustrates thickness effectson atomic number contrastInsert presentation title


Electron transparent <strong>gold</strong>Insert presentation title


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Octahedra precipitated later (dry<strong>in</strong>g phenomenon)Insert presentation title


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Faraday 1850 – changed <strong>gold</strong> sols blue from red‘known phenomena seemed to <strong>in</strong>dicate that a mere variation <strong>in</strong> thesize of [<strong>gold</strong>] particles gave rise to a variety of resultant colours’Insert presentation title


Nanoparticulate <strong>gold</strong>• Colloidal suspension• Affects UV-Vis <strong>and</strong> colour ofsuspensions• Controlled growth of size <strong>and</strong>shape of particleTsuji et al., 2005• Stable form of transport: colloidcan rema<strong>in</strong> stable up to 400°C(relevant to hydrothermaltransport)Insert presentation title


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Gold nanoparticles <strong>in</strong> refractory oresPalenik et al., 2004Insert presentation title


Gold chloride evaporation: Extractable <strong>gold</strong>Insert presentation title


Hough et al. 2008 GeologyAfter An<strong>and</strong>. 2007Insert presentation title


arytes – evaporite ‘rose’Insert presentation title


Us<strong>in</strong>g LA ICP MS to study nature of <strong>gold</strong> <strong>in</strong> calcreteL<strong>in</strong>tern, 2008LA ICPMS traverse across polishedsection of Au-rich calcrete (arrowed)• 20 samples studied to date• Au is “nuggetty”• Au-rich zones not related to other geochemistrye.g. Ca• Au peaks appear not related to micro fabricfeatures• Results consistent with evapotranspiration modelfor Au accumulation <strong>in</strong> calcrete120000counts 197 Au80000400000Insert presentation title0 2000 4000 6000 8000 10000 12000 14000 16000 18000 20000 22000 24000 26000 28000distance (μm)


Maia-96 at the Australian Synchrotron – XFM l<strong>in</strong>eRecent data from XFM beaml<strong>in</strong>e, AS December 2008 trialsRun (#304): Bounty deposit, WARegolith, calcreteMel L<strong>in</strong>tern, CSIRO 2009Au correlated with BrAuBrAPS: 117 x 203 pixels(0.7 x 1.1 mm 2 )1 s dwell, 6 x 6 µm 2 pixelsTranslucent to high-energyX-rays: Rb K, Sr K, beamDr Mel L<strong>in</strong>ternCSIRO Exploration <strong>and</strong> M<strong>in</strong><strong>in</strong>gBr-Au-Fe RGB compositeXANES: Au+ ionicXFM beaml<strong>in</strong>e, 20.1 keVBeam size φ ~ 1 µm 210 x 10 mm 2 , 8000 x 8000 pixels (1.25 µm, 0.6 ms “dwell” per pixel)Sr-Fe-Rb RGB compositeGeoPIXE 4.6 Dynamic AnalysisInsert presentation title


Colloidal nanoparticulate <strong>gold</strong> <strong>and</strong> sulphates:Evaporation• Stable colloidal transport of <strong>gold</strong>, some differences <strong>in</strong>precipitate from different lig<strong>and</strong>s but still {111}crystals.• See<strong>in</strong>g ‘<strong>Invisible</strong>’ <strong>gold</strong>.• Gold transport <strong>in</strong> areas where sal<strong>in</strong>e groundwaters<strong>in</strong>teract with <strong>gold</strong> deposits worldwide.• Sulphates an important m<strong>in</strong>eral host for <strong>gold</strong> <strong>in</strong> theregolith <strong>in</strong>clud<strong>in</strong>g <strong>in</strong> weathered sedimentsInsert presentation title


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