Exposure History of Separated Phases from the Kapoeta Meteorite

Details Exposure History of Separated Phases from the Kapoeta Meteorite Exposure History of Separated Phases from the Kapoeta Meteorite

Jan 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000stin...0205186c&link_type=abstract

Technical Report, DE2001-757462; UCRL-JC-132357-REV-1

Computer Science

Kapoeta Achondrite, Meteorites, Meteoritic Composition, Radioactive Isotopes, Monte Carlo Method, Isotope Ratios, Geochronology, Aluminum Isotopes, Beryllium Isotopes, Manganese Isotopes, Neon Isotopes, Cosmology, Chlorine

Scientific paper

The cosmogenic radionuclides, Be-10 (1.5 Ma), Al-26 (0.705 Ma), Cl-36 (0.301 Ma), and Mn-53 (3.7 Ma) were measured in selected clasts and matrix samples from the howardite Kapoeta. This work is an extension of that based on Be-10 and Al-26. Recent work based on measurements of cosmogenic Ne-21 suggest the possibility of a complex recent exposure history for Kapoeta. The measurement of these radionuclides, in conjunction with production rates based on Monte Carlo calculations, can constrain exposure conditions and durations. Taken together, the radionuclide data are entirely consistent with a single stage 4(pi) exposure lasting approximately 3 Ma.

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