RELICT irradiation of iron-meteorite material by low-energy heavy cosmic-ray nuclei

Details RELICT irradiation of iron-meteorite material by low-energy heavy cosmic-ray nuclei RELICT irradiation of iron-meteorite material by low-energy heavy cosmic-ray nuclei

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975dossr.221..198k&link_type=abstract

Akademiia Nauk SSSR, Doklady, vol. 221, Mar. 1, 1975, p. 198-200. In Russian.

Computer Science

Cosmic Rays, Heavy Nuclei, Iron Meteorites, Meteoritic Composition, Lunar Soil, Particle Energy, Particle Tracks, Silicates

Scientific paper

Measurements were made of the densities of cosmic-ray tracks in eight samples of silicate material from the iron meteorite El'ga and one sample of lunar soil obtained by Luna 20. The track-density gradient in the meteorite glasses is found to be due to irradiation by low-energy (10-15 MeV/nucleon) nuclei of VH-group cosmic rays. The glass and silicate-phase samples have preserved tracks from irradiation which occurred before the accretion of the meteorite material. This is significant for the study of the origin of iron meteorites.

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