Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/92057
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dc.contributor.authorCorrick, A.J.-
dc.coverage.spatialAdelaide Geosyncline, Flinders Ranges, South Australiaen
dc.date.issued2012-
dc.identifier.urihttp://hdl.handle.net/2440/92057-
dc.descriptionThis item is only available electronically.en
dc.description.abstractVariations in the carbon isotopic composition (δ13C) of carbonate rocks can reflect climatic and biological events throughout geologic time. However, a number of Neoproterozoic carbonate-bearing successions show spatially reproducible negative shifts in δ13C which reach as low as -12 ‰, a magnitude incompatible with current carbon cycle models. The largest of these shifts is known as the ‘Wonoka Anomaly’ after the Ediacaran Wonoka Formation in South Australia. This anomaly closely precedes the widespread appearance of macroscopic multicellular life in the geologic record, suggesting a link between potential changes in carbon cycle dynamics and the widespread rise of complex life in the Ediacaran. Alternatively, spatially reproducible, negative δ13C shifts in Quaternary carbonate platforms are known to result from diagenesis and can be demonstrated to be diachronous by biostratigraphic constraints unavailable in the Neoproterozoic. This study investigates the origin of the carbonate within the Wonoka Formation, to determine the marine and diagenetic influences on its carbon isotopic composition. Sedimentological, petrographic and isotopic analyses show the carbonate phase associated with anomalously negative δ13C values is a carbonate cement of no obvious internal origin, while the return to typical marine δ13C values is characterised by the appearance of identifiable marine carbonate grains. Isotopic analysis of this cement reveals a strong linear co-variation between δ13C and δ18O, a characteristic associated with meteoric diagenesis. Thus the Wonoka Anomaly is interpreted here as the result of cementation by meteoric water in association with small-scale changes in sea level. Given that meteoric water is depleted in δ13C by organic matter, the presence of meteoric carbonate cement in the Wonoka Formation implies significant terrestrial photosynthetic life in the late Neoproterozoic. Therefore the Wonoka Anomaly likely represents some of the earliest development of the terrestrial biosphere, rather than whole ocean secular change.en
dc.language.isoenen
dc.subjectHonours; Geology; Wonoka Anomaly; Carbon; Carbon Isotopes; Wonoka Formation; Ediacaran; Neoproterozoic; Diagenesis; Adelaide Geosyncline; South Australiaen
dc.titleResolving the Diagenetic and Marine Influences on the Carbon Isotopic Composition of the Ediacaran Wonoka Formation, South Australiaen
dc.typeThesisen
dc.contributor.schoolSchool of Earth and Environmental Sciencesen
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.description.dissertationThesis (B.Sc.(Hons)) -- University of Adelaide, School of Earth and Environmental Sciences, 2012-
Appears in Collections:School of Physical Sciences

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