Other
Scientific paper
Sep 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994metic..29..570w&link_type=abstract
Meteoritics (ISSN 0026-1114), vol. 29, no. 5, p. 570-580
Other
41
Chronology, Ilmenite, Krypton, Lunar Composition, Lunar Soil, Moon, Solar Corpuscular Radiation, Solar Wind, Xenon, Argon, Chemical Composition, Helium, Isotopes, Neon, Ratios
Scientific paper
We present Kr and Xe isotope data obtained by closed system stepped etching of ilmenite separates from two lunar samples exposed to the solar corpuscular radiation at different epochs. Helium, neon, and argon in the same samples were reported to consist of two components: isotopically unfractionated solar wind (SW) released in the first steps, and an isotopically heavier component (SEP) released later and, thus, sited at larger depth. The same release characteristic is now observed for the heavy noble gases. We also conclude that solar Kr and Xe consist of two isotopically different components, implanted with different energies. The SW-Kr in a recently irradiated soil has a composition very close to atmospheric Kr, which agrees with other newly reported data from stepped etch- and combustion runs. No clear evidence for temporally variable SW-Kr or SW-Xe spectra was found. 'Surface correlated' Kr and Xe components 'SUCOR' and 'BEOC 12001' are a mixture of SW and SEP. The isotopic fractionation factors relating SW and SEP are close to the square of the mass ratios for all five noble gases. We infer that the measured Kr/Xe ratio in ilmenite is essentially identical to this ratio in the solar corpuscular radiation.
Baur Heinrich
Wieler Rainer
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