Inert gases from Apollo 11 and Apollo 12 fines: Reversals in the trends of relative element abundances |
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Authors: | A Yaniv and D Heymann |
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Institution: | aDepartments of Geology and Space Science, Rice University, Houston, Texas 77001, USA |
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Abstract: | On the basis of the4He/20Ne ratios in feldspathic particles from Apollo 11, basaltic fragments from Apollo 11, and magnetic separates from Apollo 12 fines, one expects the former to have the highest, and the Apollo 12 material to have the lowest84Kr/132Xe ratios. This is not the case; the84Kr/132Xe ratios from sample 12070 are substantially greater than those from the feldspathic and basaltic fragments in 10084. The trend-reversal in the feldspathic particles could be due to the trapping of genuine primordial lunar Kr and Xe. The reversal in the Apollo 11 basaltic fragments might be due to periodicnear-quantitative loss of the lighter gases by impact heating, with the Apollo 11 fines containing a relatively large proportion of strongly heated fragments. |
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