Au‐Ag‐Hg and Au‐Ag alloys in Nokomai and Nevis valley placers, northern Southland and Central Otago, New Zealand, and their implications for placer‐source relationships
Abstract:Gold in Quaternary placers in the Nevis and Nokomai valleys is dominantly a-phase Au-Ag-Hg alloy (c.<10 wt% each of Ag and Hg) with subordinate Au-Ag alloy. The α-Au-Ag-Hg alloy is typically coarse grained (up to 2 cm), angular, and rarely flattened or folded. Crystalline texture, quartz intergrowths, and psuedo-hexagonal crystal pluck cavities are common. Fluvial transport distance estimates based on maximum flatness index of Au-Ag-Hg alloy particles are typically <10-20 km. Coarse (up to 2 cm) crystalline ci… Show more
“…Despite the potential usefulness of gold compositions for paragenetic studies of gold deposits in Otago, no data are yet available from hydrothermal veins. This lack of data has been highlighted by Youngson et al (2002) and Falconer (2003), who have identified geochemically distinctive Hg-rich placer gold (up to 10 wt% Hg) in deposits presumed to be derived from hydrothermally emplaced veins in the Otago Schist. Hence, knowledge of the mercury content of gold in Otago Schist hydrothermal veins has potential for linking placer deposits to sources, and determination of the geometry of paleodrainage systems.…”
Section: Introductionmentioning
confidence: 93%
“…These Hg-bearing alloys are thought to be hydrothermal in origin but no primary source for the gold has been found. The Hg-bearing gold is accompanied by abundant alluvial cinnabar in the Nevis and Nokomai valleys, and some primary genetic relationship between the cinnabar and Hg-bearing gold has been inferred (Youngson et al 2002). Cinnabar-bearing veins occur within basement rocks on the southwestern side of the schist belt ( Fig.…”
Section: Introductionmentioning
confidence: 99%
“…Au-Ag-Hg alloys occur in late Quaternary placer deposits in the Nevis valley and Nokomai valley on the southwestern side of the Otago Schist belt (Youngson et al 2002) (Fig. 1).…”
A regional study of gold from Otago Schist vein deposits from both Caples and Torlesse Terranes has revealed the presence of both Au-Ag and Au-Ag-Hg alloys in both terranes. Almost all Hg-bearing gold occurs in east Otago vein systems, and Hg-free gold occurs in central and northwest Otago vein systems, irrespective of host terrane. One Central Otago mineralised zone has up to 1.7 wt% Hg in the gold. Au-Ag alloy (3-8 wt% Ag) is typical for gold found in most Torlesse-hosted vein deposits, and Au-Ag-Hg alloys with 1-4 wt% Hg are found in vein material from the Torlesse-hosted Hyde-Macraes Shear Zone. Au-Ag-Hg alloy (3-8 wt% Ag, 2-8 wt% Hg) is found in many Caples-hosted vein deposits. There is no relationship between depth of vein emplacement and Hg content of gold, as both high and low Hg gold are found in shallow-formed (<2 km) and deep-formed (>6 km) deposits. There is no spatial relationship between Hg-bearing gold and cinnabar-bearing veins that occur in Caples Terrane rocks on the southern edge of the schist belt. Mercury-bearing placer gold in eastern Southland may have been derived from erosion of east Otago veins. The source of Hg-bearing placer gold in northern Southland is unknown as yet.
“…Despite the potential usefulness of gold compositions for paragenetic studies of gold deposits in Otago, no data are yet available from hydrothermal veins. This lack of data has been highlighted by Youngson et al (2002) and Falconer (2003), who have identified geochemically distinctive Hg-rich placer gold (up to 10 wt% Hg) in deposits presumed to be derived from hydrothermally emplaced veins in the Otago Schist. Hence, knowledge of the mercury content of gold in Otago Schist hydrothermal veins has potential for linking placer deposits to sources, and determination of the geometry of paleodrainage systems.…”
Section: Introductionmentioning
confidence: 93%
“…These Hg-bearing alloys are thought to be hydrothermal in origin but no primary source for the gold has been found. The Hg-bearing gold is accompanied by abundant alluvial cinnabar in the Nevis and Nokomai valleys, and some primary genetic relationship between the cinnabar and Hg-bearing gold has been inferred (Youngson et al 2002). Cinnabar-bearing veins occur within basement rocks on the southwestern side of the schist belt ( Fig.…”
Section: Introductionmentioning
confidence: 99%
“…Au-Ag-Hg alloys occur in late Quaternary placer deposits in the Nevis valley and Nokomai valley on the southwestern side of the Otago Schist belt (Youngson et al 2002) (Fig. 1).…”
A regional study of gold from Otago Schist vein deposits from both Caples and Torlesse Terranes has revealed the presence of both Au-Ag and Au-Ag-Hg alloys in both terranes. Almost all Hg-bearing gold occurs in east Otago vein systems, and Hg-free gold occurs in central and northwest Otago vein systems, irrespective of host terrane. One Central Otago mineralised zone has up to 1.7 wt% Hg in the gold. Au-Ag alloy (3-8 wt% Ag) is typical for gold found in most Torlesse-hosted vein deposits, and Au-Ag-Hg alloys with 1-4 wt% Hg are found in vein material from the Torlesse-hosted Hyde-Macraes Shear Zone. Au-Ag-Hg alloy (3-8 wt% Ag, 2-8 wt% Hg) is found in many Caples-hosted vein deposits. There is no relationship between depth of vein emplacement and Hg content of gold, as both high and low Hg gold are found in shallow-formed (<2 km) and deep-formed (>6 km) deposits. There is no spatial relationship between Hg-bearing gold and cinnabar-bearing veins that occur in Caples Terrane rocks on the southern edge of the schist belt. Mercury-bearing placer gold in eastern Southland may have been derived from erosion of east Otago veins. The source of Hg-bearing placer gold in northern Southland is unknown as yet.
“…It formed by the reworking of pre-Holocene material. Youngson et al (2002) have recorded such placers by residual concentration on the floor of the slowly incising valleys from New Zealand. The covariance of Mn and Ti in zone A is due to the presence of a significant amounts of pyrophanite (MnTiO 3 ) in the solid solution series with ilmenite (FeTiO 3 ) which is intergrown with rutile in the nigrine aggregates (Dill et al, 2006).…”
Section: Stages Iv-v: Colluvial-alluvial Placer and Duricrust II Formmentioning
“…Quantitative microprobe spot analyses were done using wavelength dispersion and a 5 ^m beam diameter. Mercury content of gold was determined using the data correction method described by Youngson et al (2002).…”
Small quantities (<1 m3 ) of arsenic-rich ore processing residues were piled outside the Golden Point battery, east Otago, by historic gold miners immediately before mining ceased. The residues originally contained concentrates (c. 10-fold) of gold-bearing pyrite and arsenopyrite, with abundant scheelite, and contain up to 10 wt% arsenic and 20 wt% iron. These concentrates were roasted to oxidise the sulfide minerals and release their contained gold. The gold was extracted by mercury amalgamation, and the residues are now enriched in mercury (up to 0.1 wt%) compared to original ore. Oxidation of the material has resulted in formation of crystalline scorodite (FeAsO 4 O), and amorphous iron oxyhydroxide. These three oxidised minerals have been locally (millimetre scale) dissolved and reprecipitated in the surficial environment, causing cementation of some residues. Minor relict pyrite remains in the residues, and oxidation of this maintains acid conditions (pH 2.2-3) in the residues. The scorodite and bukovskyite have been remarkably chemically stable in this acid oxidised environment over the >60 yr since the residues were abandoned. As long as the acidification continues, scorodite will remain stable.
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