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Silcrete: an Australian perspective

dc.contributor.authorTaylor, G
dc.contributor.authorEggleton, Richard
dc.date.accessioned2021-09-15T22:51:50Z
dc.date.issued2017
dc.date.updated2020-11-23T11:07:26Z
dc.description.abstractWe know how most rocks are formed. Silcrete is something of an enigma, for although there are many interpretations of the origins of individual silcrete bodies, such as those in the Paris Basin, England, Botswana and central Australia, an overarching hypothesis capable of explaining all occurrences is still to be found. This paper reviews the literature of research on predominantly Australian silcretes as well as reviewing their occurrence, mineralogy, geochemistry and petrology. Silcrete ages and paleoclimatic significance are also reviewed. Most silcretes are formed low in landscapes along fluvial tracts or lakes but, some may form at breakaway margins as a result of lateral groundwater movement. Following silicification and landscape inversion, many silcretes are left high in the landscape. Most silcretes must form in climates where there is an abundance of water, perhaps seasonally, and of organic acids. The age of a silcrete can be constrained by the fossils it may contain; ages of Australian silcretes so established range through most of the Cenozoic. Lacking fossil evidence, sediments of known stratigraphic age that have been silcreted can only provide a maximum age for the silcrete. Many silcretes in eastern Australia are overlain by basalt, but the age of the basalt can only give the minimum age of the silcreted host below it, not of the silcrete. Silcretes commonly exhibit a number of fabrics; externally glerp structures (also called cockade, ropy or botryoidal), and internally pedogenic and geopetal titaniferous grain-cap fabrics. We conclude that silcretes are formed by the precipitation of silica in various forms, almost always along with titania as anatase, at the time of cementation. Anatase occurs either where it is precipitated or by illuviation, commonly becoming concentrated as geopetal caps or coatings on larger detrital framework grains. This implies that the fluids moving the cementing components largely move downward through the silcreted host. Alternating Ti-rich and Ti-poor laminae in the caps show this process can be repetitious.en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0812-0099en_AU
dc.identifier.urihttp://hdl.handle.net/1885/247910
dc.language.isoen_AUen_AU
dc.publisherBlackwell Publishing Ltden_AU
dc.rights© 2017 Geological Society of Australiaen_AU
dc.sourceAustralian Journal of Earth Sciencesen_AU
dc.subjectAnataseen_AU
dc.subjectduricrusten_AU
dc.subjectgreybillyen_AU
dc.subjectporcellaniteen_AU
dc.subjectquartzen_AU
dc.subjectsilcreteen_AU
dc.titleSilcrete: an Australian perspectiveen_AU
dc.typeJournal articleen_AU
local.contributor.affiliationTaylor, G, University of Canberraen_AU
local.contributor.affiliationEggleton, Richard, College of Science, ANUen_AU
local.contributor.authoruidEggleton, Richard, u6600148en_AU
local.description.embargo2099-12-31
local.description.notesImported from ARIESen_AU
local.identifier.absfor040306 - Mineralogy and Crystallographyen_AU
local.identifier.absfor040399 - Geology not elsewhere classifieden_AU
local.identifier.ariespublicationa383154xPUB8416en_AU
local.identifier.doi10.1080/08120099.2017.1318167en_AU
local.identifier.scopusID2-s2.0-85028547579
local.publisher.urlhttps://www.wiley.com/en-gben_AU
local.type.statusPublished Versionen_AU

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