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dc.contributor.authorStüeken, Eva E.
dc.contributor.authorBuick, Roger
dc.contributor.authorLyons, Timothy W.
dc.date.accessioned2020-09-23T23:35:58Z
dc.date.available2020-09-23T23:35:58Z
dc.date.issued2019-11-01
dc.identifier261444867
dc.identifiercaa38268-5eaa-4edd-bb07-d381814f2362
dc.identifier85073028831
dc.identifier000496875000008
dc.identifier.citationStüeken , E E , Buick , R & Lyons , T W 2019 , ' Revisiting the depositional environment of the Neoproterozoic Callanna Group, South Australia ' , Precambrian Research , vol. 334 , 105474 . https://doi.org/10.1016/j.precamres.2019.105474en
dc.identifier.issn0301-9268
dc.identifier.otherRIS: urn:386DC0A4049E09E70C7EB0A6B8800F9F
dc.identifier.otherORCID: /0000-0001-6861-2490/work/65014425
dc.identifier.urihttps://hdl.handle.net/10023/20677
dc.descriptionFunding was provided by the NASA postdoctoral program (EES) and by the NASA Astrobiology Institute through the Virtual Planetary Laboratory (RB, Cooperative Agreement No. NNA13AA93A) and the Alternative Earths Center (TWL, Cooperative Agreement No. NNA15BB03A). The Earth-Life Transitions Program of the NSF provided additional funds to TWL.en
dc.description.abstractThe Callanna Group was deposited around 800 million years ago (Ma) during an interval in Earth’s history that saw a transition towards a more oxygenated atmosphere, increasing biodiversity among eukaryotic microfossils and climatic perturbations culminating in low-latitude glaciations. Previous researchers proposed that the Callanna basin was lacustrine and highly alkaline, which could provide important new insights into environmental cause-effect relationships at this time. To further interrogate these records, we examined standard biogeochemical proxies, including organic carbon and nitrogen isotopes, iron speciation, metal abundances and carbonate-associated sulfate. Much of the primary information has been lost because the rocks of the Callanna Group have experienced extensive metamorphism up to amphibolite facies and are altered by modern weathering. However, relics of these proxies, combined with sedimentological features, preserve evidence of redox stratification within this basin. Furthermore, our observations, in particular weakly fractionated nitrogen isotopes and abundant gypsum pseudomorphs, are incompatible with the interpretation of high alkalinity. The high salt content and occurrences of tidal indicators are most parsimoniously explained by frequent incursions of seawater. Thus, the Callanna Group cannot speak straightforwardly to environmental conditions in non-marine habitats at this time. Lastly, the absence of a large carbon isotope anomaly indicates that these rocks do not correlate with the Bitter Springs Formation.
dc.format.extent2314001
dc.language.isoeng
dc.relation.ispartofPrecambrian Researchen
dc.subjectCallanna Groupen
dc.subjectNeoproterozoicen
dc.subjectEvaporitesen
dc.subjectMetamorphic alterationen
dc.subjectGE Environmental Sciencesen
dc.subjectDASen
dc.subjectSDG 14 - Life Below Wateren
dc.subject.lccGEen
dc.titleRevisiting the depositional environment of the Neoproterozoic Callanna Group, South Australiaen
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. School of Earth & Environmental Sciencesen
dc.contributor.institutionUniversity of St Andrews. St Andrews Centre for Exoplanet Scienceen
dc.identifier.doi10.1016/j.precamres.2019.105474
dc.description.statusPeer revieweden
dc.date.embargoedUntil2020-09-24


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