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There is a well documented relationship between Au mineralized quartz and CO2 rich fluid inclusions within that quartz, indicating the CO2 rich nature of the parent hydrothermal fluids. This relationship has been suggested to be a function of CO2 buffering the pH of the geothermal fluids in a range which enhances gold solubility. It is also known that the acoustic decrepitation method can identify quartz formed from fluids which had high CO2 contents, as CO2 rich fluid inclusions decrepitate upon heating at temperatures well below that of aqueous inclusions trapped under the same pressure and temperature conditions. CO2 contents at least as low as 5 mole % are readily detectable using the acoustic decrepitation method.
The decrepitation method has been applied to a number of gold deposits in Victoria and shows that CO2 is a common but not ubiquitous constituent of the fluid systems which deposited the quartz and gold. Although the precise relationship between CO2 and gold is not clear, the method provides a means to 'fingerprint' quartz veins as an exploration guide. Samples from the Meguma terrane in Nova Scotia also show widespread but variable levels of CO2 rich fluids in the gold deposits.
Knowledge of the CO2 contents of quartz systems is a valuable exploration tool and the acoustic decrepitation method is the easiest way to acquire this information for exploration purposes as it is an automated and quick instrumental procedure.
Key words: fluid inclusions, gold, carbon dioxide, decrepitation.
The relationship between gold mineralised quartz and formational fluids which were rich in CO2 is well documented but has not been effectively used in exploration for gold because of the difficulty of measuring CO2 contents in fluid inclusions using the traditional microthermometric methods. Some authors have also stressed the importance of methane and nitrogen over carbon dioxide and inferred that it is necessary to use expensive laser raman analyses to obtain useful gas analyses from fluid inclusions. However, the acoustic decrepitation method readily determines the total contents of these gases in fluid inclusions without the need for tedious microscope work or complicated sample preparation. High contents of these gases in fluid inclusions gives a distinctly recognizable low temperature decrepitation response between 200 C and 300 C. This decrepitation behavior is due to the CO2 (and other non-condensing gases) expanding upon heating in approximate accordance with the gas law, PV=nRT, whereas aqueous inclusions undergo condensation to a liquid phase and do not generate significant internal pressure upon heating until after the liquid and vapour phases homogenize. Consequently the CO2 rich inclusions develop high internal pressures sufficient to burst the host mineral grain at much lower temperatures than the aqueous inclusions. (Figure 1) The gas law applies to all species of gases and so the presence of methane or nitrogen does not reduce this effect unless there is some other fundamental difference in the trapping or preservation conditions of the inclusions.
Decrepitation analyses from deposits in the Victorian goldfields show that CO2 is a common but variable constituent in the auriferous quartz and may thus be used to distinguish between different generations of quartz formed from different hydrothermal fluids of potentially different Au potential (i.e. to 'fingerprint' potentially auriferous quartz). Although the levels of CO2 in fluid inclusions from the Victorian deposits are quite modest (in contrast to the very high CO2 contents in quartz from the Archaean metamorphogenic deposits in Western Australia), samples with noticeable CO2 levels often correlate with known mineralization, as at the Central Deborah mine in Bendigo. In other locations, such as at Ballarat, the CO2 rich quartz does not correlate well with the Au analyses, but this quartz is quite inhomogeneous on a scale of centimetres, indicating considerable variation in the parental fluids during deposition.
Samples from the Meguma terrane in Nova Scotia have been compared with those from Victoria and many but not all of the Nova Scotia deposits are also associated with CO2 rich fluids.
Acoustic decrepitation is a sensitive and quick method to obtain
fluid CO2
compositional information from fluid inclusions which represent
the
original ore forming fluids. This information is very useful in
exploration for Au bearing quartz and is an important step in
making
use of fluid inclusion data to assist in exploration, rather than
merely consigning fluid inclusion studies to post-discovery
genetic
research.
When heated, pure gas inclusions will follow a path close to the
CO2
isochore (magenta) line and quickly develop enough internal
pressure
to decrepitate at low temperature. However aqueous inclusions will
follow a path along the vapour-liquid curve for water (blue) until
they homogenise at the homogenisation point, and then along the
water
isochore (green) and will not develop a high internal pressure
until
above the homogenisation temperature. Inclusions containing mixed
water and gases will follow paths between these two extremes.