Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/137032
Type: Thesis
Title: C, Sr and Cr isotope constraints on the depositional environment and palaeo-redox of the Neoarchean Fortescue Group, Pilbara Craton, WA
Author: Scarabotti, L
Issue Date: 2019
School/Discipline: School of Physical Sciences
Abstract: The Tumbiana and Hardey Formations of the Fortescue group in the northern Pilbara Craton are Neoarchean sedimentary rocks dated at 2.7 Ga, with questionable palaeo-depositional environments ranging from possibly marine to continental lacustrine settings. In this study, we applied a set of traditional, novel isotopic (C, Sr and Cr) and trace element (REE, Zn/Fe) tracers which were analysed in Neoarchean carbonates from recently recovered drill core 18ABAD01 intersecting the Tumbiana and Hardey Formations. This study generated high-resolution δ13C and 87Sr/86Sr records, which provide convincing evidence for the non-marine nature of these sediments, suggesting that these deposits were formed in a Neoarchean lacustrine system. Furthermore, this study applied palaeo-redox proxies such as δ53Cr and Zn/Fe ratios to infer past redox conditions during deposition of stromatolite-bearing carbonates from the Tumbiana Formation. Overall, results show these carbonates formed in a lacustrine settings and in the presence of shallow oxic waters, the latter likely produced due to local O2 input from stromatolitic/ photosynthetic communities. Finally, the results of this study have implications for the origin of local sediment-hosted stratiform copper SSC deposits. Importantly, the palaeo-redox data from the Tumbiana Formation supports the existence of local pool oxic waters that could thus aid the formation of SSC deposits.
Dissertation Note: Thesis (B.Sc.(Hons)) -- University of Adelaide, School of Physical Sciences, 2019
Where: Pilbara Craton, Western Australia
Keywords: Honours; Geology; depositional environments; palaeo-redox; Fortescue Group; Pilbara Craton; Tumbiana Formation; Hardey Formation; chromium isotopes; strontium isotopes; REE
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
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