Best Practices for Determination of Initial 10 Be/ 9 Be in Early Solar System Materials by Secondary Ion Mass Spectrometry
Autor: | Meenakshi Wadhwa, E. T. Dunham, Steven J. Desch, Richard L. Hervig |
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Rok vydání: | 2020 |
Předmět: |
Radionuclide
Solar System Materials science 010401 analytical chemistry Short lived radionuclides Mineralogy Geology 010502 geochemistry & geophysics 01 natural sciences 0104 chemical sciences Cosmochemistry Ion Secondary ion mass spectrometry Geochemistry and Petrology Mean square weighted deviation 0105 earth and related environmental sciences |
Zdroj: | Geostandards and Geoanalytical Research. 44:695-710 |
ISSN: | 1751-908X 1639-4488 |
DOI: | 10.1111/ggr.12329 |
Popis: | Beryllium-10 (t1/2 = 1.4 Ma) is a short-lived radionuclide present in the early Solar System. It is produced solely by irradiation reactions and can provide constraints on the astrophysical environment of the Sun's formation. Calcium- and aluminium-rich inclusions (CAIs), the first solids formed in the Solar System, show clear evidence for live 10Be at their time of formation, but it is unclear whether they record the same initial 10Be/9Be ratio. In this study, we examine the secondary ion mass spectrometry methods used to determine the initial 10Be/9Be ratio in meteoritic inclusions. Based on analyses of synthesised matrix-matched glass reference materials, we show that the effects of differing major element bulk compositions on the secondary ion yields of Be and B are minor for relevant phases. We demonstrate the importance of using the mean square weighted deviation (MSWD) to interpret the significance of the initial 10Be/9Be value. For thirty-two CAIs, we re-calculated the regressions using literature data, finding that several have unacceptably high MSWD. We calculate the effects of possible sources of isotopic disturbance. Finally, we outline best practices for reporting 10Be-10B data, to enable a more refined determination of the initial 10Be/9Be ratio in the early Solar System. |
Databáze: | OpenAIRE |
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