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Titania in Australian massive silcretes

dc.contributor.authorEggleton, Richard
dc.contributor.authorTaylor, G
dc.date.accessioned2020-12-20T20:58:19Z
dc.date.available2020-12-20T20:58:19Z
dc.date.issued2017
dc.date.updated2020-11-23T11:22:36Z
dc.description.abstractSelected silcretes formed by cementation of stream sediments and having >90 wt% SiO2, have been examined optically and by scanning electron microscopy. Such silcretes have quartz framework grains cemented by a plasma of quartz and anatase. Both the plasma quartz and the anatase are euhedral where they line cavities in the silcrete. Such quartz is typically up to 5 µm in diameter; the anatase crystals are platy on (001) and 50–100 nm in diameter. Comparison of the SiO2, TiO2 and Zr content of 138 silcretes with that of 2345 Australian stream sediments suggests the source of titania in silcretes is endogenous. The morphology of the quartz and anatase leads to the conclusion that both precipitated in situ.
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0812-0099
dc.identifier.urihttp://hdl.handle.net/1885/218556
dc.language.isoen_AUen_AU
dc.publisherBlackwell Publishing Ltd
dc.sourceAustralian Journal of Earth Sciences
dc.titleTitania in Australian massive silcretes
dc.typeJournal article
local.bibliographicCitation.lastpage10
local.bibliographicCitation.startpage1
local.contributor.affiliationEggleton, Richard , College of Science, ANU
local.contributor.affiliationTaylor, G, University of Canberra
local.contributor.authoruidEggleton, Richard , u6600148
local.description.notesImported from ARIES
local.identifier.absfor040202 - Inorganic Geochemistry
local.identifier.ariespublicationa383154xPUB7464
local.identifier.doi10.1080/08120099.2017.1338617
local.identifier.scopusID2-s2.0-85023781120
local.type.statusPublished Version

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