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dc.contributor.authorFehr, M. A.
dc.contributor.authorRehkämper, M.
dc.contributor.authorHalliday, A. N.
dc.contributor.authorHattendorf, B.
dc.contributor.authorGünther, D.
dc.date.accessioned2021-02-12T22:53:44Z
dc.date.available2021-02-12T22:53:44Z
dc.date.issued2009-01-01
dc.identifier.citationFehr, M. A., Rehkämper, M., Halliday, A. N., Hattendorf, B., & Günther, D. (2009). Tellurium isotope compositions of calcium‐aluminum‐rich inclusions. Meteoritics & Planetary Science, 44(7), 971-984.
dc.identifier.issn1945-5100
dc.identifier.doi10.1111/j.1945-5100.2009.tb00782.x
dc.identifier.urihttp://hdl.handle.net/10150/656589
dc.description.abstractA method for the precise and accurate determination of the tellurium (Te) isotope compositions of calcium-aluminum-rich inclusions (CAIs) has been developed. The technique utilizes multiple-collector inductively coupled plasma-mass spectrometry (MC-ICPMS) with either Faraday detectors or a dual ion-counting system. The external reproducibility (2-sigma) for 126Te/125Te was ~15 per mil and ~2 per mil when 3 pg and 65 pg of Te were analyzed with the electron multipliers. Measurements performed on 200 pg of Te using Faraday detectors and time-resolved software displayed an external reproducibility of ~8 per mil for 126Te/124Te, whereas 3 ng Te could be measured to a precision of about 0.6 per mil. Analyses of five CAIs from the Allende chondrite yielded Te concentrations that range from 12 to 537 ppb and the inclusions are therefore depleted in Te relative to bulk Allende by factors of about 2 to 86. The Sn/Te ratios of the CAIs are also fractionated compared to bulk Allende (which displays 124Sn/128Te is approximately equal to 0.1) with 124Sn/128Te ratios of about 0.1 to 2.5. The Te isotope measurements for these refractory inclusions yielded no 126Te excesses from the decay of the short-lived radionuclide 126Sn (tau-1/2 = 234,500 years) and the most precise analysis provided a epsilon-126Te value of 1 +/- 6 (epsilon-126Te = 126Te/ 124Te normalized to 122Te/124Te = 0.53594 and reported relative to the JMC Te standard). Minor differences in the Te isotope composition of the CAIs relative to the terrestrial standard and bulk Allende hint at the presence of small deficits in r-process Te isotopes or excess of s-process Te, but these nucleosynthetic anomalies are barely resolvable given the analytical uncertainties. Hence, it is also conceivable that these effects reflect small unresolved analytical artifacts.
dc.language.isoen
dc.publisherThe Meteoritical Society
dc.relation.urlhttps://meteoritical.org/
dc.rightsCopyright © The Meteoritical Society
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.subjectCalcium-aluminum-rich inclusions (CAIs)
dc.subjectisotope geochemistry
dc.subjectextinct radionuclides
dc.subjectMC-ICP-MS
dc.titleTellurium isotope compositions of calcium-aluminum-rich inclusions
dc.typeArticle
dc.typetext
dc.identifier.journalMeteoritics & Planetary Science
dc.description.collectioninformationThe Meteoritics & Planetary Science archives are made available by the Meteoritical Society and the University of Arizona Libraries. Contact lbry-journals@email.arizona.edu for further information.
dc.eprint.versionFinal published version
dc.description.admin-noteMigrated from OJS platform February 2021
dc.source.volume44
dc.source.issue7
dc.source.beginpage971
dc.source.endpage984
refterms.dateFOA2021-02-12T22:53:44Z


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