Recent progress on interstellar radionuclides on Earth and the Moon
Authors:
- Dominik KollDKDominik Koll
- Sebastian FichterSFSebastian Fichter
- Michael HotchkisMHMichael Hotchkis
- Martin MartschiniMMMartin Martschini
- Silke MerchelSMSilke Merchel
- Stefan PavetichSPStefan Pavetich
- Annabel RolofsARAnnabel Rolofs
- Steve TimsSTSteve Tims
- Sebastian ZwickelSZSebastian Zwickel
- Anton WallnerAWAnton Wallner
Open Access
- 12 May 2025
- journal article
- review article
- Published by Springer Nature in The European Physical Journal A
- Vol. 61 (5) , 1-10
Abstract
The detection of interstellar radionuclides in geological archives provides insights into nucleosynthesis in stars and stellar explosions as well as interstellar medium dynamics in the Local Bubble and the Local Interstellar Cloud. In this work, current projects to detect interstellar radionuclides with accelerator mass spectrometry will be reviewed. These projects aim to address unsolved questions regarding the timing and the origin of the influxes and to establish new radionuclides for future searches. For the first time, experimental evidence for an inhomogeneous deposition of interstellar $$^{60}$$ Fe on Earth will be presented and another potential source for $$^{60}$$ Fe on Earth and the Moon, primary galactic cosmic rays, will be introduced.
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Funding Information
- Australian Research Council (DP18010049, DP180100495)
- European Union (ChETEC-INFRA, project no. 10100832)
- Australian Institute of Nuclear Science and Engineering (Postgraduate Research Award (PGRA))
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