Isotope Anomalies in Tellurium in Interstellar Diamonds

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Origin of Elements in the Solar System

Abstract

The isotopic composition of Te has been measured in a purified sample of interstellar microdiamonds from the Allende meteorite. Small positive anomalies were only found in 128Te (4.0 ± 0.3‰) and 130Te (9.3 ± 2.0‰) from three analyses of the Allende microdiamond sample EB#2. The magnitude of the anomalies are smaller than in the heavy noble gases, although the absolute amount of anomalous Te is greater than that of anomalous Xe in the same sample. The anomalies in Te can be interpreted in terms of standard r-process nucleosynthesis followed by rapid separation of the stable isotopes from their radioactive precursors.

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References

  • Anders, E. and Grevesse, N.: 1989, “Abundances of the elements: Meteoritic and solar”, Geochim. Cosmochim. Acta 53, 197–214.

    Article  CAS  Google Scholar 

  • Anders, E. and Zinner, E.: 1993, “Interstellar grains in primitive meteorites: diamond, silicon carbide, and graphite”, Meteoritics 28, 490–514.

    CAS  Google Scholar 

  • Ballad, R.V., Oliver L.L., Downing, R.G. and Manuel O.K.: 1979, “Isotopes of Te, Xe and Kr in Allende meteorite retain record of nucleosynthesis”, Nature 227, 615–620.

    Article  Google Scholar 

  • Clayton, D.D.: 1989, “Origin of heavy xenon in meteoritic diamonds”, Ap. J. 340, 613–619.

    Article  CAS  Google Scholar 

  • Heymann, D. and Dziczkaniec M.: 1979, “Xenon from intermediate zones of supernovae”, Lunar Planet Sci. 10, 1943–1959.

    Google Scholar 

  • Heymann, D. and Dziczkaniec, M.: 1981, “Tellurium, should it be isotopically anomalous in the Allende Meteorite?” Geochim. Cosmochim. Acta 45, 1829–1834.

    Article  CAS  Google Scholar 

  • Howard, W.M, Meyer, B.S. and Clayton, D.D.: 1992, “Heavy-element abundances from a neutron burst that produces Xe-H”, Meteoritics 27, 404–412.

    Article  CAS  Google Scholar 

  • Huss, G.R. and Lewis, R.S.: 1994a, “Noble gases in presolar diamonds I: Three distinct components and their implications for diamond origins”, Meteoritics 29, 791–810.

    Article  CAS  Google Scholar 

  • Huss, G.R. and Lewis R.S.: 1994b, “Noble gases in presolar diamonds II: Component abundances reflect thermal processing”, Meteoritics 29, 811–829.

    Article  CAS  Google Scholar 

  • Lewis, R.S., Huss, G.R. and Lugmair, G.: 1991a, “Finally, Ba and Sr accompanying Xe-HL in diamonds from Allende”, Lunar Planet. Sci. 22, 807–808.

    Google Scholar 

  • Lewis, R.S., Huss, G.R., Anders, E., Liu, Y.G. and Schmitt, R.A.: 1991b, “Elemental abundance patterns in presolar diamonds”, Meteoritics 26, 363–364.

    Google Scholar 

  • Loss, R.D., Rosman, K.J.R. and De Laeter, J.R.: 1990, “The isotopic composition of Zn, Pd, Ag, Cd and Te in the Allende meteorite”, Geochim. Cosmochim. Acta 54, 3525–3536.

    Article  CAS  Google Scholar 

  • Ott, U.: 1996, “Interstellar diamond xenon and timescales of supernova ejecta”, Ap. J. 463, 344–348.

    Article  CAS  Google Scholar 

  • Richter, S., Ott, U. and Begemann, F.: 1998, “Tellurium in pre-solar diamonds as an indicator, for rapid separation of supernova ejecta”, Nature 391, 261–26

    Article  CAS  Google Scholar 

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© 2002 Kluwer Academic Publishers

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Maas, R. et al. (2002). Isotope Anomalies in Tellurium in Interstellar Diamonds. In: Manuel, O. (eds) Origin of Elements in the Solar System. Springer, Boston, MA. https://doi.org/10.1007/0-306-46927-8_30

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  • DOI: https://doi.org/10.1007/0-306-46927-8_30

  • Publisher Name: Springer, Boston, MA

  • Print ISBN: 978-0-306-46562-8

  • Online ISBN: 978-0-306-46927-5

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