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Iron and nickel isotope compositions of presolar silicon carbide grains from supernovae

Kodolányi, János; Stephan, Thomas; Trappitsch, Reto; Hoppe, Peter; Pignatari, Marco; Davis, Andrew M.; Pellin, Michael J.

Authors

János Kodolányi

Thomas Stephan

Reto Trappitsch

Peter Hoppe

Marco Pignatari

Andrew M. Davis

Michael J. Pellin



Abstract

© 2017 Elsevier Ltd. We report the carbon, silicon, iron, and nickel isotope compositions of twenty-five presolar SiC grains of mostly supernova (SN) origin. The iron and nickel isotope compositions were measured with the new Chicago Instrument for Laser Ionization, CHILI, which allows the analysis of all iron and nickel isotopes without the isobaric interferences that plagued previous measurements with the NanoSIMS. Despite terrestrial iron and nickel contamination, significant isotopic anomalies in 54 Fe/ 56 Fe, 57 Fe/ 56 Fe, 60 Ni/ 58 Ni, 61 Ni/ 58 Ni, 62 Ni/ 58 Ni, and 64 Ni/ 58 Ni were detected in nine SN grains (of type X). Combined multi-isotope data of three grains with the largest nickel isotope anomalies ( > 100‰ or < -100‰ in at least one isotope ratio, when expressed as deviation from the solar value) are compared with the predictions of two SN models, one with and one without hydrogen ingestion in the He shell prior to SN explosion. One grain's carbon-silicon-iron-nickel isotope composition is consistent with the prediction of the model without hydrogen ingestion, whereas the other two grains' isotope anomalies could not be reproduced using either SN models. The discrepancies between the measured isotope compositions and model predictions may indicate element fractionation in the SN ejecta prior to or during grain condensation, and reiterate the need for three-dimensional SN models.

Citation

Kodolányi, J., Stephan, T., Trappitsch, R., Hoppe, P., Pignatari, M., Davis, A. M., & Pellin, M. J. (2018). Iron and nickel isotope compositions of presolar silicon carbide grains from supernovae. Geochimica et cosmochimica acta, 221, 127-144. https://doi.org/10.1016/j.gca.2017.05.029

Journal Article Type Article
Acceptance Date May 20, 2017
Online Publication Date May 29, 2017
Publication Date Jan 15, 2018
Deposit Date Jun 28, 2018
Journal Geochimica et Cosmochimica Acta
Print ISSN 0016-7037
Publisher Elsevier
Peer Reviewed Peer Reviewed
Volume 221
Pages 127-144
DOI https://doi.org/10.1016/j.gca.2017.05.029
Keywords Nucleosynthesis; Iron isotopes; Nickel isotopes; Supernova; Chicago instrument for laser ionization
Public URL https://hull-repository.worktribe.com/output/556790
Publisher URL https://www.sciencedirect.com/science/article/pii/S0016703717303149