Search for Supernova-Produced Fe60 in a Marine Sediment

C. Fitoussi, G. M. Raisbeck, K. Knie, G. Korschinek, T. Faestermann, S. Goriely, D. Lunney, M. Poutivtsev, G. Rugel, C. Waelbroeck, and A. Wallner
Phys. Rev. Lett. 101, 121101 – Published 19 September 2008

Abstract

An Fe60 peak in a deep-sea FeMn crust has been interpreted as due to the signature left by the ejecta of a supernova explosion close to the solar system 2.8±0.4Myr ago [Knie et al., Phys. Rev. Lett. 93, 171103 (2004)]. In an attempt to confirm this interpretation with better time resolution and obtain a more direct flux estimate, we measured Fe60 concentrations along a dated marine sediment. We find no Fe60 peak at the expected level from 1.7 to 3.2 Myr ago. Possible causes for the discrepancy are discussed.

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  • Received 10 August 2007

DOI:https://doi.org/10.1103/PhysRevLett.101.121101

©2008 American Physical Society

Authors & Affiliations

C. Fitoussi1, G. M. Raisbeck1, K. Knie2,5, G. Korschinek2, T. Faestermann2, S. Goriely3, D. Lunney1, M. Poutivtsev2, G. Rugel2, C. Waelbroeck4, and A. Wallner5

  • 1Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM) IN2P3/CNRS, Université Paris Sud, Bâtiment 108, 91405 Orsay, France
  • 2Fakultät für Physik, Technische Universität München, James-Franck-Straße 1, 85747 Garching, Germany
  • 3Institut d’Astronomie et d’Astrophysique, C.P. 226, Université Libre de Bruxelles, Boulevard Du Triomphe, B-1050 Brussels, Belgium
  • 4Laboratoire des Sciences du Climat et de l’Environnement, Domaine du CNRS, 91198 Gif-sur-Yvette, France
  • 5VERA Laboratory, Fakultät für Physik, Universität Wien, Währinger Straße 17, A-1090 Vienna, Austria

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Vol. 101, Iss. 12 — 19 September 2008

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