LA-ICP-MS study of IAB and IIIAB irons and pallasites: Sub-solidus HSE behavior

dc.contributor.authorMullane, Een
dc.contributor.authorAlard, Oen
dc.contributor.authorGounelle, Men
dc.contributor.authorRussell, Sarah Sen
dc.date.accessioned2026-01-01T09:41:14Z
dc.date.available2026-01-01T09:41:14Z
dc.date.issued2004en
dc.description.abstractWe report the concentration of the platinum group elements (PGE) in addition to the highly siderophile elements (HSE) Re and Au, obtained using LA-ICP-MS, in spatially resolved FeNi-metal (kamacite and taenite) from a suite of IIIAB irons and Brenham main group pallasite (MGP). These samples are products of fractional crystallization and define a coherent magmatic trend, from the least evolved (Henbury and Wabar) to the most evolved (Mount Edith). Fractional crystallization continued after segregation of the pallasite parent melt, and incorporation of olivine into this metal melt did not affect the highly siderophile element systematics. Solid metal –liquid metal partition coefficients indicate the following compatibility: (1) highly compatible (Re, Os and Ir), (2) moderately compatible (Pt, Ru and Rh), and (3) incompatible (Pd and Au). This compatibility sequence is broadly consistent with the melting point systematics of the HSE. The highly fractionated HSE pattern of the evolved IIIAB and Brenham pallasite indicates that nonmetallic elements such as S play a fundamental role in the evolution of planetisimal core. Taenite – kamacite partition coefficients (DT/K) illustrate that all of the HSE enter preferentially taenite during subsolidus partitioning and that subsolidus partitioning is comparable between magmatic and nonmagmatic irons. DT/K appears to be independent of the physical conditions prevailing on the parent bodies and the light element molar fraction in the bulk composition, but instead the controlling factors on DT/K behaviour seems to be a combination of the degree of atomic symmetry coupled with atomic radius. D 2004 Elsevier B.V. All rights reserved.en
dc.description.statusPeer-revieweden
dc.format.extent24en
dc.identifier.issn1086-9379en
dc.identifier.otherWOS:000222990600130en
dc.identifier.scopus4043062344en
dc.identifier.urihttps://hdl.handle.net/1885/733799493
dc.language.isoenen
dc.relation.ispartofseries67th Annual Meeting of the Meteoritical-Societyen
dc.sourceMeteoritics and Planetary Scienceen
dc.titleLA-ICP-MS study of IAB and IIIAB irons and pallasites: Sub-solidus HSE behavioren
dc.typeJournal articleen
dspace.entity.typePublicationen
local.bibliographicCitation.lastpage28en
local.bibliographicCitation.startpage5en
local.contributor.affiliationAlard, O; Geochemistry, Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationRussell, Sarah S; The Natural History Museum, Londonen
local.identifier.citationvolume39en
local.identifier.pure584d06ad-6d37-4b1c-823f-9beb82d444afen
local.identifier.urlhttps://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=anu_research_portal_plus2&SrcAuth=WosAPI&KeyUT=WOS:000222990600130&DestLinkType=FullRecord&DestApp=WOS_CPLen
local.identifier.urlhttps://www.scopus.com/pages/publications/4043062344en
local.type.statusPublisheden

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