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Science 14 January 1983:
Vol. 219. no. 4581, pp. 127 - 135
DOI: 10.1126/science.219.4581.127

Articles

Cosmic-Ray Record in Solar System Matter

Robert C. Reedy 1, James R. Arnold 2, and Devendra Lal 3

1 Staff member in the Nuclear Chemistry Group, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, and is currently a visiting scientist at Max-Planck-Institut für Chemie, D-6500 Mainz, Federal Republic of Germany
2 Professor in the Department of Chemistry, University of California at San Diego, La Jolla 92093, and director of the California Space Institute
3 Director of the Physical Research Laboratory, Navrangpura, Ahmedabad 380009 India, and visiting professor at Scripps Institution of Oceanography, La Jolla, California 92093

The energetic nuclei in cosmic rays interact with meteoroids, the moon, planets, and other solar system matter. The nuclides and heavy nuclei tracks produced by the cosmic-ray particles in these targets contain a wealth of information about the history of the objects and temporal and spatial variations in the particle fluxes. Most lunar samples and meny meteorites have complex histories of cosmicray exposure from erosion, gardening, fragmentation, orbital changes, and other processes. There appear to be variations in the past fluxes of solar particles, and possibly also galactic cosmic rays, on time scales of 104 to 107 years.


THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
Understanding the Lunar Surface and Space-Moon Interactions.
P. Lucey, R. L. Korotev, J. J. Gillis, L. A. Taylor, D. Lawrence, B. A. Campbell, R. Elphic, B. Feldman, L. L. Hood, D. Hunten, et al. (2006)
Reviews in Mineralogy and Geochemistry 60, 83-219
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An Overview of Isotopic Anomalies in Extraterrestrial Materials and Their Nucleosynthetic Heritage.
J. L. Birck (2004)
Reviews in Mineralogy and Geochemistry 55, 25-64
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History of Meteorites from the Moon Collected in Antarctica.
O. Eugster and O. EUGSTER (1989)
Science 245, 1197-1202
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Accelerator Mass Spectrometry for Measurement of Long-Lived Radioisotopes.
D. Elmore, D. ELMORE, and F. M. PHILLIPS (1987)
Science 236, 543-550
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