The histories of ordinary chondrite parent bodies - U, Th-He age distributions

Details The histories of ordinary chondrite parent bodies - U, Th-He age distributions The histories of ordinary chondrite parent bodies - U, Th-He age distributions

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991metic..26..161w&link_type=abstract

Meteoritics (ISSN 0026-1114), vol. 26, June 1991, p. 161-167.

Computer Science

28

Chondrites, Chronology, Meteoritic Composition, Radioactive Age Determination, Helium, Histories, Solar System Evolution, Thermal Environments, Thorium, Uranium

Scientific paper

Age patterns observed in meteorite groups reflect the different thermal or impact histories experienced by their parent bodies. To assess the number of ordinary chondrite (OC) parent bodies, rare-gas data in the Schultz and Kruse (1989) data base were used to calculate U, Th-He gas-retention ages. Most H- and LL-chondrite ages are high; about 81 percent are greater than 2.2 Ga. In contrast, most L-chondrite ages are low; about 69 percent are not greater than 2.2 Ga, and about 35 percent are not greater than 0.9 Ga. The latter fraction is substantially lower than the value of 44 percent given by Heymann (1967). The difference is attributed to the preferential inclusion of shocked L chondrites in early studies. Broad age peaks in the H and LL groups near 3.4 Ga probably reflect thermal loss during metamorphism, but in the H distribution there is a hint of minor outgassing "events" near 1 Ga. The L/LL chondrites have chemical properties intermediate between and unresolvable from L and LL chondrites. The high ages of most L/LL chondrites are evidence against these originating on the L parent body; the L/LL age distribution is consistent with an origin on the LL parent body or on an independent body.

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