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Tellurium isotope compositions of calcium-aluminum-rich inclusions

Fehr, Manuela A.; Rehkämper, Mark; Halliday, Alex N.; Hattendorf, Bodo and Günther, Detlef (2009). Tellurium isotope compositions of calcium-aluminum-rich inclusions. Meteoritics and Planetary Science, 44(7) pp. 971–984.

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DOI (Digital Object Identifier) Link: http://dx.doi.org/10.1111/j.1945-5100.2009.tb00782.x
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Abstract

A 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 (2s) for 126Te/125Te was ~15‰ and ~2‰ 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‰ for 126Te/124Te, whereas 3 ng Te could be measured to a precision of about 0.6‰.
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 ≈ 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 (T½ = 234,500 years) and the most precise analysis provided a e126Te value of 1 +/- 6 (e126Te = 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.

Item Type: Journal Article
Copyright Holders: 2009 The Meteoritical Society
ISSN: 1086-9379
Academic Unit/Department: Science
Interdisciplinary Research Centre: Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
Item ID: 18141
Depositing User: Manuela Fehr
Date Deposited: 03 Sep 2009 09:15
Last Modified: 23 Nov 2012 13:59
URI: http://oro.open.ac.uk/id/eprint/18141
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