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An overview of vis-nir-swir field spectroscopy - Spectral International

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Definition <strong>of</strong> deposit type<br />

HIGH SULFIDATION SYSTEMS<br />

High sulphidation Au + Cu ore systems develop from the reaction with host rocks<br />

<strong>of</strong> hot acidic magmatic fluids to produce characteristic zoned alteration and later<br />

sulphide and Au + Cu + Ag deposition. Ore systems display permeability controls<br />

governed by lithology, structure and breccias and changes in wall rock alteration<br />

and ore mineralogy with depth <strong>of</strong> formation. One <strong>of</strong> the challenges is to<br />

distinguish the mineralized systems from a group <strong>of</strong> generally non-economic<br />

acidic alteration styles including lithocaps or barren shoulders, steam heated,<br />

magmatic solfatara and acid sulphate alteration.<br />

Original definitions (Heald et al.,1987) suggest that epithermal deposits formed at<br />

temperatures < 300°C and therefore at shallow depths, typically < 1 km.<br />

The term epithermal is therefore used in <strong>field</strong> exploration studies to describe Au ±<br />

Ag ± Cu deposits formed in magmatic arc environments (including rifts) at<br />

shallow depths, most typically above the level <strong>of</strong> formation <strong>of</strong> porphyry Cu-Au<br />

deposits (typically < 1 km), although in many instances associated with<br />

subvolcanic intrusions. Higher level epithermal deposits are commonly formed<br />

later in a deposit paragenesis, and may be telescoped upon deeper earlier<br />

formed deposits, including in some instances porphyry systems which are older,<br />

or part <strong>of</strong> the same overall magmatic event (e.g., Lihir, Corbett et al., 2001b). In<br />

strongly dilational structural environments porphyry-related systems may be<br />

telescoped outwards into the deeper “epithermal” environment (e.g., Cadia,<br />

Maricunga Belt).<br />

In brief, high sulphidation deposits develop in settings where volatile rich<br />

magmatic fluids rise to higher crustal levels without significant interaction<br />

with the host rocks or ground waters. Volatiles (SO2) evolved from the<br />

depressurising fluids oxidize to form a two stage hot acid fluid, the initial stage<br />

<strong>of</strong> which reacts with the host rocks to produce the characteristic zoned acidic<br />

alteration at epithermal crustal levels (Corbett and Leach, 1998). A later liquiddominated<br />

fluid phase deposits sulphides which are characterised by pyrite<br />

with enargite, or the latter’s low temperature polymorph luzonite.<br />

Magmatic rocks are interpreted to represent the ultimate source <strong>of</strong> ore fluids as<br />

demonstrated by the commonly association <strong>of</strong> HS deposits with felsic domes<br />

and phreatomagmatic breccias within flow-dome complexes. Many HS deposits<br />

display associations with porphyry Cu-Au systems <strong>of</strong> similar ages (Nena), or are<br />

collapsed upon and form part <strong>of</strong> the porphyry ores. Fluids responsible for the<br />

formation <strong>of</strong> HS deposits rarely evolve to Au- rich lower sulphidation style ores.<br />

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