Radiation history of meteoritic and lunar material by track data

Details Radiation history of meteoritic and lunar material by track data Radiation history of meteoritic and lunar material by track data

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....8..128k&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Conference Papers. Volume 8 (A85-2

Physics

Chondrites, Chondrule, Lunar Rocks, Particle Tracks, Solar Cosmic Rays, Breccia, Microcrystals, Olivine, Pyroxenes, Regolith

Scientific paper

Under study were tracks formed by the iron group nuclei of solar cosmic rays observed in microcrystals of olivine and pyroxene from the lithic chondrules of the brecciated chondrite Weston, as well as from the lunar regolith samples and microbreccias of the 'Luna-16', 'Luna-20' and 'Luna-24' sites. The obtained results indicate that the relict irradiation of initial meteorite material took place at the early stage of formation of the solar system bodies, and that formation of the lithic chondrules occured in the processes which were similar to the formation of lunar microbreccias without significant heating.

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