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Aluminum 26, {sup 10}Be, and {sup 36}Cl depth profiles in the Canyon Diablo iron meteorite

Journal Article · · Journal of Geophysical Research
DOI:https://doi.org/10.1029/94JE02267· OSTI ID:81655
; ; ;  [1]; ;  [2]
  1. Purdue Univ., West Lafayette, IN (United States)
  2. Los Alamos National Lab., NM (United States)

The authors have measured activities of the long-lived cosmogenic radionuclides {sup 26}Al, {sup 10}Be, and {sup 36}Cl in 12 fragments of the iron meteorite Canyon Diablo and have constructed production rate-versus-depth profiles of those radionuclides. Profiles determined using differential particle fluxes calculated with the LAHET code system are in good agreement with {sup 26}Al, {sup 10}Be, and {sup 36}Cl experimental data, but the agreement for {sup 36}Cl was obtained only after neutron-induced cross sections were modified. Profiles calculated with lunar particle fluxes are much lower than experimental Canyon Diablo profiles. The cosmic ray exposure ages of most samples are near 540 m.y. 34 refs., 4 figs., 2 tabs.

OSTI ID:
81655
Journal Information:
Journal of Geophysical Research, Journal Name: Journal of Geophysical Research Journal Issue: E11 Vol. 99; ISSN JGREA2; ISSN 0148-0227
Country of Publication:
United States
Language:
English

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