Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/98295
Type: Thesis
Title: Copper - Gold exploration in the Middleback Ranges; source(s) of fluids and metals
Author: Cave, B. J.
Issue Date: 2010
School/Discipline: School of Physical Sciences
Abstract: The Moola Prospect of the Middleback Ranges, South Australia is an epigenetic, hypothermal copper-gold prospect that displays several clear genetic affinities with IOCG deposits/prospects in the Gawler Craton, although from this study alone classification of the mineralisation is imprudent. A broad study on the mineral paragenesis and geochemistry of the deposit was carried out on a single drill core provided by OneSteel, the holder of the tenement encompassing the Moola Prospect. The mineralisation, characterised by pyrite + chalcopyrite, hematite and magnetite, is hosted by the Palaeoproterozoic metavolcanic / volcaniclastic, Myola Volcanics and an unnamed, undated fine-grained microgranite that intrudes the Myola Volcanics. This unnamed, undated microgranite, displays geochemical and petrological similarities with the Myola Volcanics from which it‘s thought to be partial derived from its anatexis; likely being a Wertigo Granite equivalent. Four alteration assemblages were observed in the Moola Prospect drill core and placed into the following paragenic sequence; Na (Ca-Fe) characterised by the formation of albite; sericite replacing K-feldspar and plagioclase and alteration increasing towards sericite veining; chlorite with alteration increasing towards chlorite-mica±epidote veins; late stage quartz, quartz-carbonate, carbonate flooding, that hosts mineralisation. Ore mineral paragenesis occurs in an overlapping sequence; the first mineral precipitated was magnetite that was later extensively martitised, with hematite followed by pyrite and minor heamatite + pyrite, pyrite + chalcopyrite, then chalcopyrite. Later supergene alteration altered the chalcopyrite to native copper and malachite. Sphalerite precipitation couldn‘t be constrained from petrological evidence alone. Iron oxide and sulphide chemistry, and sulphur isotopes from the sulphides support this paragenesis, and constrains precipitation of sphalerite between the pyrite only and chalcopyrite only phases. Iron oxide chemistry also revealed the presence of illmentite in the core, however could only constrain illmentite precipitation as, coeval to after haematite precipitation. Sulphur isotopes revealed evidence for an additional late stage pyrite precipitation, after the chalcopyrite only phase. Bulk rock composition was quite variable with some altered samples showing strong enrichments of Fe2O3, SiO2, CaO, K2O, Na2O SO3, MnO, P2O5 and MgO. Strong enrichment of CaO and/or SiO2 in some of the altered samples, but not others, suggests that the quartz-carbonate alteration represented by this geochemical signature is sporadic in nature. Depletion in SiO2 in some of the altered samples could also represent the consumption of silica during the Na-Ca-Fe alteration event. Enrichment of SO3 in the altered samples likely directly represents alteration related to the precipitation of sulphide ore minerals. Trace element and rare earth element compositional changes from alteration shows enrichments of Cu, U, Pb, Li, B, Mn and V likely relating to alteration associated with mineralisation. εNd (1590Ma) values of the Moola Prospect together with εNd (1590Ma) versus whole rock Cu concentration and Co: Ni ratios of pyrite, indicates a crustal derived, with minor mantle input for the sources of metals. Sulphur isotopes and trace element whole rock geochemistry indicates a primitive/ magmatic fluid source is responsible for alteration and/ or mineralisation.
Dissertation Note: Thesis (B.Sc.(Hons)) -- University of Adelaide, School of Earth and Environmental Sciences, 2010
Where: Gawler Craton, Middleback Ranges, South Australia
Keywords: Honours; Geology
Description: This item is only available electronically.
Provenance: This electronic version is made publicly available by the University of Adelaide in accordance with its open access policy for student theses. Copyright in this thesis remains with the author. This thesis may incorporate third party material which has been used by the author pursuant to Fair Dealing exceptions. If you are the author of this thesis and do not wish it to be made publicly available, or you are the owner of any included third party copyright material you wish to be removed from this electronic version, please complete the take down form located at: http://www.adelaide.edu.au/legals
Appears in Collections:School of Physical Sciences

Files in This Item:
File Description SizeFormat 
01frontGeoHon.pdf195.07 kBAdobe PDFView/Open
02wholeGeoHon.pdf8.75 MBAdobe PDFView/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.