Transcript Slides

ENGINE, Potsdam, 12.01.2007
Reactive transport model of silicification at
the Mount Isa Copper deposit, Australia
Michael Kühn1,3 and Klaus Gessner2,3
1Applied
Geophysics, RWTH Aachen University
2School of Earth and Geographical Sciences, University of Western Australia
3Exploration and Mining, CSIRO
pmd CRC
Parallels between Soultz-sous-Forêts and Mount Isa
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Fluid flow in fractured systems
Mineralization in crystalline rocks
Precipitation / dissolution pattern
Permeability evolution over time
 Hypotheses testing applying reactive transport
Outline
• Mount Isa Copper – location, deposit, model
• SHEMAT / Processing SHEMAT
• Fluid flow driver?
– Free thermal convection
– Hydraulic head driven flow
• Silicification pattern (quartz body development)
due to the fluid flow driving process
• Conclusion – What have we learned?
Mount Isa location
Mount Isa Copper deposit
6 km x 5 km x 3 km
Mount Isa fault
Urquhart shale
envelope
Paroo fault
goCAD to
SHEMAT
Field observations – quartz body
Urquhart shale
envelope
Paroo fault
Mount Isa fault
SHEMAT / Processing SHEMAT (Clauser 2003)
• Coupled flow, heat, transport,
and chemical processes
• Geochemical reactions
between solids and fluids
• Reactive Transport
– PHRQPITZ (Pitzer’s
approach) for low to high
salinities but seawater
system only
– PHREEQC (Debye-Hückel)
for low salinities but
increased chemical system
Free thermal convection (high permeability Urquhart)
Urquhart shale
envelope
Mount Isa fault
Paroo fault
Free thermal convection (low permeability Urquhart)
Mount Isa fault
Paroo fault
Quartz body: observation vs. simulation
high
permeability
Urquhart shale envelope
Mount Isa fault
Paroo fault
low
permeability
Forced flux / hydraulic head driven flow into faults
Urquhart shale
envelope
Mount Isa fault
Darcy flux 1E-08 m/s
 free convection flux
Paroo fault
Quartz body: observation vs. simulation
Forced flux / no convection
50 % impermeable
Conclusions
• Process driving fluid flow?
– free thermal convection
– hydraulic head driven flow
• Considering conditions required
to form the observed quartz body
suggests: rather hydraulic head
driven flow than free convection
Acknowledgements
• Thanks to:
– Florian Dobert who contributed to the
presented work,
– the pmd*CRC for financial support in previous
years during my work with CSIRO,
– Xstrata Copper for financial support and the
contribution of valuable field data
Thank you