Gas-Rich Meteorites: Possible Evidence for Origin on a Regolith

Details Gas-Rich Meteorites: Possible Evidence for Origin on a Regolith Gas-Rich Meteorites: Possible Evidence for Origin on a Regolith

Jan 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974sci...183...73m&link_type=abstract

Science, Volume 183, Issue 4120, pp. 73-74

Computer Science

4

Scientific paper

The asymmetry of irradiation features of grains in the Kapoeta and Fayetteville meteorites suggests irradiation on a regolith before meteorite formation. Chondrules and broken grains require approximately 104 years of irradiation time between formation or fracturing and compaction into the meteorite. Shock erasure of tracks from irradiated Kapoeta feldspars requires a severe shock event during or after meteorite formation.

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