4.1 Article

53Mn and 60Fe in iron meteorites-New data, model calculations

期刊

METEORITICS & PLANETARY SCIENCE
卷 55, 期 4, 页码 818-831

出版社

WILEY
DOI: 10.1111/maps.13466

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资金

  1. Swiss National Science Foundation [SNF 200021-159562]
  2. Australian Research Council [DP140100136, DP180100495, DP180100496]
  3. Group of Eight Australia-Germany Joint Research Co-operation Scheme

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We measured specific activities of the long-lived cosmogenic radionuclides Fe-60 in 28 iron meteorites and Mn-53 in 41 iron meteorites. Accelerator mass spectrometry was applied at the 14 MV Heavy Ion Accelerator Facility at ANU Canberra for all samples except for two which were measured at the Maier-Leibnitz Laboratory, Munich. For the large iron meteorite Twannberg (IIG), we measured six samples for Mn-53. This work doubles the number of existing individual Fe-60 data and quadruples the number of iron meteorites studied for Fe-60. We also significantly extended the entire Mn-53 database for iron meteorites. The Mn-53 data for the iron meteorite Twannberg vary by more than a factor of 30, indicating a significant shielding dependency. In addition, we performed new model calculations for the production of Fe-60 and Mn-53 in iron meteorites. While the new model is based on the same particle spectra as the earlier model, we no longer use experimental cross sections but instead use cross sections that were calculated using the latest version of the nuclear model code INCL. The new model predictions differ substantially from results obtained with the previous model. Predictions for the Fe-60 activity concentrations are about a factor of 2 higher, for Mn-53, they are similar to 30% lower, compared to the earlier model, which gives now a better agreement with the experimental data.

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