Please use this identifier to cite or link to this item: https://zone.biblio.laurentian.ca/handle/10219/3691
Full metadata record
DC FieldValueLanguage
dc.contributor.authorHastie, Evan Carman George-
dc.date.accessioned2021-06-08T17:55:27Z-
dc.date.available2021-06-08T17:55:27Z-
dc.date.issued2021-04-29-
dc.identifier.urihttps://zone.biblio.laurentian.ca/handle/10219/3691-
dc.description.abstractUnderstanding ore forming processes and their control on mineralization is essential for the proper classification of Archean, and also younger, Au deposits and mineral exploration success. This study evaluates Archean Au-forming processes using examples across the Superior Province (Canada), with an emphasis on the Swayze area in the Abitibi greenstone belt. It combines detailed field mapping with various discriminants (e.g., in-situ stable isotopes, whole rock and trace-element geochemistry, LA-ICP-MS elemental mapping and chemistry of native gold) to differentiate between orogenic and intrusion-related Au deposits. Based on previous work and newly generated data on 44 deposits, the dataset suggests that Ag, Te and Hg are the only metals consistently associated with Au across different deposit types. Although these metals represent universal elemental vectors for Au exploration, other criteria such as rock and mineral textures, timing of Au mineralization, stable isotope data, and bulk geochemistry must be used to differentiate between Au-deposit types. An important finding is the recognition of a distinct subset of intrusion-related Archean deposits related to sanukitoid-type magmatism. These deposits, generally younger than 2690 Ma, predate shearing and are characterized by Te and Hg elemental associations, relatively high fO2, and δ34S ≤ -5‰. They differ from other intrusion related deposits in terms of their timing and geochemistry and, thus, require a different exploration strategy. Of importance to both academia and industry is the origin of late-stage high-grade Au zones in many deposits. This study suggests such zones result from coupled dissolution-reprecipitation of Au-bearing sulfides and generation of polymetallic Au melts and/or Au nanoparticles, which aggregate as coarse native gold. Both of the processes can elegantly explain ultra high-grade gold zones and are widely applicable to many Au deposits formed throughout Earth’s history.en_US
dc.language.isoenen_US
dc.subjectGolden_US
dc.subjectAuen_US
dc.subjectArcheanen_US
dc.subjectSwayze areaen_US
dc.subjectAbitibi greenstone belten_US
dc.subjectsuperior provinceen_US
dc.subjectAu-forming processesen_US
dc.subjecteconomic geologyen_US
dc.subjectgeochemistryen_US
dc.subjectJeromeen_US
dc.subjectKentyen_US
dc.subjectRundleen_US
dc.subjectNamexen_US
dc.subject4Ken_US
dc.subjectAu remobilizationen_US
dc.subjectdissolution-reprecipitationen_US
dc.subjectgold nanoparticleen_US
dc.subjectS isotopesen_US
dc.subjectO isotopesen_US
dc.subjectLA-ICP MSen_US
dc.subjectTEMen_US
dc.subjectSEM-EDSen_US
dc.subjectTIMSen_US
dc.subjectSIMSen_US
dc.titleGold metallogeny of the southern Swayze Area, Abitibi Greenstone Belten_US
dc.typeThesisen_US
dc.description.degreeDoctor of Philosophy (PhD) in Mineral Deposits and Precambrian Geologyen_US
dc.publisher.grantorLaurentian University of Sudburyen_US
Appears in Collections:Mineral Deposits and Precambrian Geology - Doctoral theses

Files in This Item:
File Description SizeFormat 
Evan Hastie PhD Thesis (Final Revised) (1).pdf1_16.98 MBUnknownView/Open


Items in LU|ZONE|UL are protected by copyright, with all rights reserved, unless otherwise indicated.