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The noble gas systematics of late-orogenic H 2 O-CO 2 fluids, Mt Isa, Australia

dc.contributor.authorKendrick, Mark
dc.contributor.authorHonda, Masahiko
dc.contributor.authorOliver, N H S
dc.contributor.authorPhillips, David
dc.date.accessioned2015-12-10T23:22:46Z
dc.date.issued2011
dc.date.updated2016-02-24T08:12:34Z
dc.description.abstractThe noble gases (He, Ne, Ar, Kr and Xe) are powerful geochemical tracers because they have distinctive isotopic compositions in the atmosphere, crust and mantle. This study illustrates how noble gases can be used to trace fluid origins in high-temperature metamorphic and mineralising environments; and at the same time provides new information on the composition of noble gases in deeper parts of the crust than have been sampled previously.We report data for H2O and CO2 fluid inclusions trapped at greenschist to amphibolite facies metamorphic conditions associated with three different styles of mineralisation and alteration in the Proterozoic Mt Isa Inlier of Australia. Sulphide fluid inclusions are dominated by crustal 4He. However, co-variations in fluid inclusion 20Ne/22Ne, 21Ne/22Ne, 40Ar/36Ar and 136Xe/130Xe indicate noble gases were derived from three or more reservoirs. In most cases, the fluid inclusions elemental noble gas ratios (e.g. Ne/Xe) are close to the ranges expected in sedimentary and crystalline rocks. However, the elemental ratios have been modified in some of the samples providing evidence for independent pulses of CO2, and interaction of CO2 with high-salinity aqueous fluids.Compositional variation is attributed to mixing of: (i) magmatic fluids (or deeply sourced metamorphic fluids) characterised by basement-derived noble gases with 20Ne/22Ne~8.4, 21Ne/22Ne~0.4, 40Ar/36Ar~40,000 and 136Xe/130Xe~8; (ii) basinal-metamorphic fluids with a narrow range of compositions including near-atmospheric values and (iii) noble gases derived from the meta-sedimentary host-rocks with 20Ne/22Ne~8-9.8, 21Ne/22Ne<0.1, 40Ar/36Ar<2500 and 136Xe/130Xe~2.2.These data provide the strongest geochemical evidence available for the involvement of fluids from two distinct geochemical reservoirs in Mt Isa's largest ore deposits. In addition the data show how noble gases in fluid inclusions can provide information on fluid origins, the composition of the crust's major lithologies, fluid-rock interactions and fluid-fluid mixing or immiscibility processes.
dc.identifier.issn1872-9533
dc.identifier.urihttp://hdl.handle.net/1885/66660
dc.publisherPergamon-Elsevier Ltd
dc.sourceGeochimica et Cosmochimica Acta
dc.subjectKeywords: amphibolite; carbon dioxide; crustal structure; fluid inclusion; greenschist facies; host rock; isotopic composition; isotopic ratio; mineralization; noble gas; ore deposit; reservoir; sulfide; tracer; Australia; Mount Isa; Queensland
dc.titleThe noble gas systematics of late-orogenic H 2 O-CO 2 fluids, Mt Isa, Australia
dc.typeJournal article
local.bibliographicCitation.issue6
local.bibliographicCitation.lastpage1450
local.bibliographicCitation.startpage1428
local.contributor.affiliationKendrick, M A, University of Melbourne
local.contributor.affiliationHonda, Masahiko, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationOliver, N H S, James Cook University
local.contributor.affiliationPhillips, David, University of Melbourne
local.contributor.authoruidHonda, Masahiko, u8604264
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor040201 - Exploration Geochemistry
local.identifier.absseo840202 - Mining and Extraction of Copper Ores
local.identifier.absseo840204 - Mining and Extraction of Iron Ores
local.identifier.ariespublicationf2965xPUB1322
local.identifier.ariespublicationu4027924xPUB335
local.identifier.citationvolume75
local.identifier.doi10.1016/j.gca.2010.12.005
local.identifier.scopusID2-s2.0-79951515061
local.identifier.thomsonID000287682500003
local.type.statusPublished Version

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