Applied mineral exploration methods, hydrothermal fluids, baro-acoustic decrepitation, CO2 rich fluids
Viewpoints:

How CO2 inclusions form from aqueous fluids

Understanding heterogeneous fluids : why gold is not transported in CO2 fluids

Gold-quartz deposits form from aqueous heterogeneous fluids: NOT from CO2 fluids

Inclusion shapes can prove heterogeneous FI trapping

Disproportional FI trapping from heterogeneous fluids explains gas-dominant systems

A discussion of H2 analysis by mass spectrometry

A mechanism to form H2 in the MS ioniser during analyses


News:

Sangan skarn Fe deposits, Iran

New model 205 decreptiometer

Studies of 6 Pegmatite deposits

A study of the Gejiu tin mine, China


Exploration using palaeo-hydrothermal fluids

Using opaque minerals to understand ore fluids


Understanding baro-acoustic decrepitation.

An introduction to fluid inclusions and mineral exploration applications.



 Interesting Conferences:


AGCC expo, Adelaide, Aust. Oct. 14-18 2018

-----2019-----

ECROFI, June 24-26, Budapest, Hungary

AOGS, Singapore, 28 Jul-2 Aug 2019

SGA, Glasgow Scotland, Aug. 27-30 2019


Comprehensive Geology Conference Calendar


Baro-acoustic decrepitation of samples from the Favona vein, Waihi, NZ


A study of epithermal Au and Ag mineralised quartz from this area on the North Island of NZ was undertaken with Penelope Small and Prof. Andrew Rankin of Kingston University, Surrey and the cooperation of Newmont.

Ten samples were collected from drill core in an attempt to determine spatial temperature and fluid composition variations with depth and horizontal position within the vein.



Interpretation

The samples show low decrepitation intensities, as expected for dominantly vapour filled, high level epithermal fluid inclusions in quartz. However it is still possible to discern important differences between the samples which seem to correlate with Au mineralisation. In particular, there is evidence for the presence of CO2 rich fluids correlated with the best mineralised samples. Despite the low decrepitation intensities, this data clearly shows a strong correlation between known gold grades and the presence of low temperature gas-rich decrepitation.

Additional discussion of the Favona results is here.

There are also variations of the decrepitation temperatures of the main peak near 400 C which suggest the technique is capable of mapping out thermal gradients within the quartz system, and these variations are likely to also correlate with mineralisation potential.

Incomplete sample location information and sparse sampling limit the complete interpretation of this data at present.


These initial plots have been grouped  based on the Au contents of the samples.

high au


The above samples with high Au contents, about  80 g/t, show distinct decrepitation at low temperature near 300 - 350 C which is typical of samples which contain CO2 rich fluid inclusions. These samples are from  an unspecified location, thought to be UW67 (not UW167)  at about 950m RL in the Favona vein.




moderate Au

Samples with moderate Au contents, about 40 g/t, lack this low temperature decrepitation. These samples also have very low intensity of decrepitation which is typical of high level epithermal inclusions, which are often vapour rich and do not decrepitate well. These samples are also from about 950m RL in the Favona vein.





high Au

This sample, with 40 g/t Au shows only background decrepitation. This is interpreted to be a vapour rich area of the vein system. This sample is also from about 950m RL in the Favona vein.




low level Au

This sample with only low level Au of about 1 g/t  shows weak, but distinct decrepitation  and perhaps a hint of CO2 rich inclusions. This sample is located close to the main ore zone and the fluid inclusions indicate that good mineralisation is nearby despite the low chemical analysis result. It is from about 900m RL in the Favona vein.




background au

These samples have < 0.1 g/t Au and are distant from the active workings. The decrepitation results show a lack of CO2 and suggest low mineralisation potential. Note that there are significant differences in the temperature of the main peak and with sufficient  sample coverage these variations might be mapped to show thermal gradients within the quartz vein system. Samples 1878 and 1880 are from the Moonlight area, while sample 1879 is from Deep in the Favona vein, about  700m RL.




background

These samples have only <0.2 g/t Au and lack low temperature decrepitation and CO2. The more intense decrepitation and better shaped peaks suggest this quartz contains more liquid rich inclusions, probably formed at greater depth and pressure than other samples in this study, despite being collected shallower than other samples.
The green plot is the same sample as the red, done at higher instrumental sensitivity.  The  blue, magenta and green plots are 3 splits of the same sample to check for homogeneity. This sample is from the Favona South shoot at about 1000m RL. 




Sample locations


map


The  deposit comprises a swarm of quartz veins, shown here on a surface geology map


surface geology map


The  locations within the mine are shown on this  N-S pseudo section. Samples 1884 and 1885 were wrongly described by the student and are shown here at their probable location.

The thick grey lines are the mine workings and entrance adit.

long section


The sample locations and gold analyses are in this table.


Sample ID Location Sample # Run # Drill Hole From (m) To (m) Box No. Ag (g/t) Au (g/t)
UW140A Fav, 950 RL
1881 H2195 UW140 220.00 219.86 84 128.00 41.67
UW140B Fav, 950 RL
1882 H2196, H2197 UW140 219.80 219.77 84 128.00 41.67
UW140C Fav, 950 RL
1883 H2198 UW140 219.42 219.30 84 128.00 41.67
UW167A Fav 950 RL?
1884 H2199 UW167 296.43 296.25 105 56.80 78.70
UW167B Fav 950 RL?
1885 H2200 UW167 295.75 295.63 105 56.80 78.70
UW100A Moon 800 RL
1878 H2189, H2190 UW100 355.15 355.00 118 2.90 0.12
UW100B Moon 800 RL
1880 H2192, H2194 UW100 350.57 350.43 119 2.90 0.12
UW283a Favona South
1000 RL
1886 H2185, H2186, H2201, H2202 UW283 122.75 122.64 85 1.90 0.23
UW127c Fav, 650 RL
1879 H2193 UW127 537.82 538.00 104 10.80 to 0.14 5.60 to 0.06
UW89d Fav, 900 RL
1877 H2188 UW89 241.65 241.50 83 15.79 to 1.82 3.00 to 0.86



De-convolution of each decrepigram was carried out to determine the individual component skewed-gaussian populations present in each sample and this data is plotted below, where the circle diameter at each temperature is proportional to the decrepitation intensity of that component population.

The better mineralised Favona main shoot (red) has more intense decrepitation and  small but measurable low temperature, gas-rich inclusion decrepitation. The Favona South shoot  (yellow) has less decrepitation and slightly less low temperature gas-rich decrepitation. And the Moonlight area (green) has much less low temperature gas-rich decrepitation.  From this it is seen that the best exploration areas are in fact in the shallow areas of the Favona South shoot, which looks more promising that even the deep samples from the Favona main shoot (sample 1879). The data show that the Moonlight area is not a particularly promising exploration target.

favona bubble plot


Additional discussion of the Favona results is here

Sample number - Run number cross index

Sample descriptions

Fitting of gaussian populations to the overall decrepitation results


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