A peak into the mantle: primary magma generation beneath the Peak Range, central Queensland

dc.contributor.authorPeters, L.
dc.contributor.schoolSchool of Physical Sciencesen
dc.coverage.spatialPeak Range, central Queensland
dc.date.issued2021
dc.descriptionThis item is only available electronically.en
dc.description.abstractThe hotspot-related Tertiary Peak Range (central Queensland) consists of enriched peraluminous rhyolites in the north, and metaluminous trachytes and peralkaline rhyolites in the south. Further petrographical mapping of the southern Peak Range revealed consistency with the Chandler (2018) model of an extended fractionation of an alkali basaltic melt as the source for the enriched intrusion, whereas a heterogeneous intrusion (Campbell’s Peak; a phonolitic intrusion with a basaltic rim abundant in peridotite xenoliths and amphibole megacrysts) 20km NE of the central Peak Range executes a different evolutional pathway. The peridotites are characteristic of metasomatised subcontinental lithospheric mantle (SCLM), enriched from the dehydration of fluids from the subducting slab in eastern Australia during the Late Devonian-Cretaceous. This is apparent in the growth of pargasitic amphibole (modal metasomatism), high concentrations of Rb, La, Ta, U, and sodium-bearing pyroxenes (mild cryptic metasomatism). The amphibole megacrysts are assumed to be a cumulate or fractionation phase in the mantle brought to the surface as xenocrysts in the basalt. Melting models of the peridotite demonstrate a lack of correlation between the basaltic host rock (especially in TiO2 levels), but a strong correlation with the phonolitic intrusion when partially melted (<1%) at ~10kbar and if fractionation of ~15% amphibole was considered. Fractionation modelling of the trachybasalt revealed no direct relationship to the peridotites or phonolitic rocks, suggesting it is unrelated. The spatial and temporal relation of Campbell’s Peak to the Peak Range is similar to the Ernst & Bell (2010) model of linking large igneous provinces (LIPs) and carbonatite intrusions if the central Peak Range is interpreted as the volcanic centre. It is proposed the phonolitic intrusion of Campbell’s Peak is a result of a low degree of partial melting of the SCLM via low temperature magmatism at the outer edge of the mantle plume, with later basaltic eruption resembling more mantle plume, flood basalt mechanisms.en
dc.description.dissertationThesis (B.Sc.(Hons)) -- University of Adelaide, School of Physical Sciences, 2021
dc.identifier.urihttps://hdl.handle.net/2440/140783
dc.language.isoenen
dc.provenanceThis 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/legalsen
dc.subjectHonours; Geology; Peak Range; peridotite xenoliths; mantle melting modelling; mantle metasomatism; amphibole megacrystsen
dc.titleA peak into the mantle: primary magma generation beneath the Peak Range, central Queenslanden
dc.typeThesisen

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