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dc.contributor.advisorFrei, Dirk
dc.contributor.authorMisrole, Matthew
dc.date.accessioned2020-12-11T10:51:41Z
dc.date.available2020-12-11T10:51:41Z
dc.date.issued2020
dc.identifier.urihttp://hdl.handle.net/11394/7733
dc.description>Magister Scientiae - MScen_US
dc.description.abstractThe Saldania Belt in southern Africa, a product of the Pan-African Saldanian Orogeny, forms part of a system of Neoproterozoic mobile belts that border and weld older cratons on the African continent. It is a low-grade orogenic belt situated along the southwestern margin of the Kalahari Craton and is composed of several inliers of greenschist facies metasedimentary and metavolcanic rocks (Malmesbury Group), unroofed in megaanticlinal hinges of the Permo-Triassic Cape Fold Belt. The Malmesbury Group rocks were syn- and post-tectonically intruded in a pervasive transpressive regime between 555 Ma and 515 Ma by Neoproterozoic to early Cambrian S-, I- and A-type granites, monzodiorites, gabbros and quartz syenites, which collectively constitute the rocks of the Cape Granite Suite (CGS). Along the south-western coastline of South Africa, the Saldanha Bay Volcanic Complex (which forms part of the CGS) is divided into two eruption centres both of which have been identified as “intra-caldera pyroclastic ignimbrites”. The Postberg eruption centre is situated to the south of the Saldanha Bay entrance and the Saldanha eruption centre is situated to the north of the entrance. Both eruption centres display distinct geochemical signatures, the most apparent being the greater TiO2 concentrations (> 0.25 wt. %) of the Saldanha centre ignimbrites when compared to its Postberg centre counterparts. The Postberg eruption centre consists of S-type rhyolitic ignimbrites which are subdivided into the two geochemically distinct Plankiesbaai and Tsaarsbank Ignimbrites. Small amounts of the Jacobs Bay and Saldanha Ignimbrites (less felsic tephra from the Saldanha eruption centre) are also present in the Postberg eruption centre. A robust geochemical analysis of both the Plankiesbaai and Tsaarsbank magma groups display high SiO2 content (>76 wt. %), a lack of variation in TiO2 and Zr, high Al2O3 and ASI (aluminium saturation index) values (> 1.0 and generally >1.1 which, on average, is higher than the Saldanha eruption centre ignimbrites), low CaO and Na2O, and a highly ferroan character. The Plankiesbaai ignimbrite also display lower #Mg concentration compared to the Tsaarsbank ignimbrite. Typical geochemical trends in the Postberg eruption centre include the lack of variation in Zr content, higher Rb content and lower Sr, Ba, V and Zn concentrations when compared to the tephra of the Saldanha eruption centre found in the Postberg area.en_US
dc.language.isoenen_US
dc.publisherUniversity of the Western Capeen_US
dc.subjectIgnimbriteen_US
dc.subjectGeotectonic developmenten_US
dc.subjectMagmatismen_US
dc.subjectPhenocrystsen_US
dc.subjectPyroclasic Flowsen_US
dc.subjectRhyoliteen_US
dc.subjectSaldanha Bayen_US
dc.subjectSaldania Belten_US
dc.subjectSaldanian Orogenyen_US
dc.subjectS-typeen_US
dc.titleGeochronology and geochemistry of the Postberg ignimbrites, Saldanha, Western Cape, South Africaen_US
dc.rights.holderUniversity of the Western Capeen_US


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