Please use this identifier to cite or link to this item: http://hdl.handle.net/1893/33894
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dc.contributor.authorAli-Bik, Mohamed Wen_UK
dc.contributor.authorTaman, Zeinaben_UK
dc.contributor.authorEl Kalioubi, Baheren_UK
dc.contributor.authorAbdel Wahab, Waelen_UK
dc.date.accessioned2022-01-28T01:01:04Z-
dc.date.available2022-01-28T01:01:04Z-
dc.date.issued2012-02-14en_UK
dc.identifier.urihttp://hdl.handle.net/1893/33894-
dc.description.abstractEnormous quantities of practically untapped talc–magnesite rocks are distributed in the Wadi Barramiya area in intimate spatial and genetic association with the ophiolitic serpentinites. These deposits are an important potential source of magnesia, which is used in a broad spectrum of strategic industries. Barramiya ophiolitic serpentinites represent obducted oceanic slices onto island-arc successions. They occur as elongated mountainous ranges in the form of anticlinal–synclinal sheets demarcating the general ENE-WSW brittle–ductile shear zones of the area. The serpentinite-hosted talc–magnesite deposits of Barramiya area are located: (a) along major faults that cut the serpentinite slices, or (b) at thrust contacts between obducted serpentinites and other mélange components (more siliceous country rocks of island-arc affinity). The latter were regionally metamorphosed at greenschist up to middle amphibolite facies conditions. The talc–magnesite rocks represent in situ fissure-fed metasomatic products of serpentinite precursors via extensive rock–fluid interactions. The main fluids involved in the transformation processes of serpentinites to talc–magnesite were SiO2aqueous solutions and CO2. The deposits located along the fault systems cutting the serpentinite-host are magnesite-rich, whereas those located at the contacts between serpentinites and the more siliceous country rocks are typically talc-rich. Based on the proportional distribution of talc and magnesite in conjunction with other accessories, the rocks have been distinguished into assemblages. Their characteristics, petrogenesis and evolution from serpentinite precursors are elaborated in the light of their petrography, XRD, EDAX, and XRF data. Constraints on the conditions of their formation include temperature of about 490 °C and a maximum XCO2 of about 0.13. New mapping was undertaken for the area using remote sensing and GIS techniques. Accordingly, the Barramiya talc–carbonate rocks were more precisely mapped as separate layers and their reserve estimation was accomplished.en_UK
dc.language.isoenen_UK
dc.publisherElsevier Limiteden_UK
dc.relationAli-Bik MW, Taman Z, El Kalioubi B & Abdel Wahab W (2012) Serpentinite-hosted talc-magnesite deposits of Wadi Barramiya area, Eastern Desert, Egypt: Characteristics, petrogenesis and evolution. Journal of African Earth Sciences, 64, pp. 77-89. https://doi.org/10.1016/j.jafrearsci.2011.11.002en_UK
dc.rightsThe publisher does not allow this work to be made publicly available in this Repository. Please use the Request a Copy feature at the foot of the Repository record to request a copy directly from the author. You can only request a copy if you wish to use this work for your own research or private study.en_UK
dc.rights.urihttp://www.rioxx.net/licenses/under-embargo-all-rights-reserveden_UK
dc.subjectBarramiyaen_UK
dc.subjectTalc–carbonatesen_UK
dc.subjectTalc carbonatesen_UK
dc.subjectSerpentiniteen_UK
dc.subjectOphioliteen_UK
dc.subjectPetrogenesisen_UK
dc.titleSerpentinite-hosted talc-magnesite deposits of Wadi Barramiya area, Eastern Desert, Egypt: Characteristics, petrogenesis and evolutionen_UK
dc.typeJournal Articleen_UK
dc.rights.embargodate2999-12-31en_UK
dc.rights.embargoreason[1-s2.0-S1464343X11001889-main.pdf] The publisher does not allow this work to be made publicly available in this Repository therefore there is an embargo on the full text of the work.en_UK
dc.identifier.doi10.1016/j.jafrearsci.2011.11.002en_UK
dc.citation.jtitleJournal of African Earth Sciencesen_UK
dc.citation.issn1464-343Xen_UK
dc.citation.volume64en_UK
dc.citation.spage77en_UK
dc.citation.epage89en_UK
dc.citation.publicationstatusPublisheden_UK
dc.citation.peerreviewedRefereeden_UK
dc.type.statusVoR - Version of Recorden_UK
dc.author.emailzeinab.smillie@stir.ac.uken_UK
dc.citation.date15/11/2011en_UK
dc.contributor.affiliationEgyptian National Research Centreen_UK
dc.contributor.affiliationAin Shams Universityen_UK
dc.contributor.affiliationAin Shams Universityen_UK
dc.contributor.affiliationEgyptian National Research Centreen_UK
dc.identifier.isiWOS:000301686900008en_UK
dc.identifier.scopusid2-s2.0-84855882940en_UK
dc.identifier.wtid1784747en_UK
dc.contributor.orcid0000-0002-0089-1793en_UK
dc.date.accepted2011-11-01en_UK
dcterms.dateAccepted2011-11-01en_UK
dc.date.filedepositdate2022-01-27en_UK
rioxxterms.apcnot requireden_UK
rioxxterms.typeJournal Article/Reviewen_UK
rioxxterms.versionVoRen_UK
local.rioxx.authorAli-Bik, Mohamed W|en_UK
local.rioxx.authorTaman, Zeinab|0000-0002-0089-1793en_UK
local.rioxx.authorEl Kalioubi, Baher|en_UK
local.rioxx.authorAbdel Wahab, Wael|en_UK
local.rioxx.projectInternal Project|University of Stirling|https://isni.org/isni/0000000122484331en_UK
local.rioxx.freetoreaddate2261-10-16en_UK
local.rioxx.licencehttp://www.rioxx.net/licenses/under-embargo-all-rights-reserved||en_UK
local.rioxx.filename1-s2.0-S1464343X11001889-main.pdfen_UK
local.rioxx.filecount1en_UK
local.rioxx.source1464-343Xen_UK
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