Abstract
An 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 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 concentrations along a dated marine sediment. We find no peak at the expected level from 1.7 to 3.2 Myr ago. Possible causes for the discrepancy are discussed.
- Received 10 August 2007
DOI:https://doi.org/10.1103/PhysRevLett.101.121101
©2008 American Physical Society