• DOI:10.1086/323617
• Corpus ID: 15699567

Experimental Limit to Interstellar 244Pu Abundance

@article{Paul2001ExperimentalLT,
  title={Experimental Limit to Interstellar 244Pu Abundance},
  author={M. Paul and A. Valenta and Irshad Ahmad and Dan Berkovits and C. Bordeanu and S A Ghelberg and Yasuhiro Hashimoto and Allen Hershkowitz and S. Jiang and Takashi Nakanishi and Kazushi Sakamoto},
  journal={The Astrophysical Journal Letters},
  year={2001},
  volume={558},
  pages={L133 - L135}
}

• M. Paul, A. Valenta, +8 authors K. Sakamoto
• Published 12 June 2001
• Environmental Science, Physics
• The Astrophysical Journal Letters

Short-lived nuclides, now extinct in the solar system, are expected to be present in the interstellar medium (ISM). Grains of ISM origin were recently discovered in the inner solar system and at Earth orbit and may accrete onto Earth after ablation in the atmosphere. A favorable matrix for detection of such extraterrestrial material is presented by deep-sea sediments with very low sedimentation rates (0.8-3 mm kyr-1). We report here on the measurement of Pu isotopic abundances in a 1 kg deep-sea dry sediment collected in 1992 in the North Pacific. Our estimate of (3 ± 3) × 105 244Pu atoms in the Pu-separated fraction of the sample shows no excess over the expected stratospheric nuclear fallout content and, under reasonable assumptions, sets a limit of 0.2 244Pu atoms cm-2 yr-1 for extraterrestrial deposition. Using the available data on the ISM steady-state flux on Earth, we derive a limit of 2 × 10-11 g 244Pu (g ISM)-1 for the abundance of 244Pu in the ISM.