The variation of cosmogenic Kr and Xe in a core from Estherville mesosiderite: direct evidence that the lunar 131Xe anomaly is a depth effect

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Kr and Xe were measured by a stepwise heating technique in three samples of a drill core in the ``Minnesota'' fragment of the Estherville mesosiderite. The cosmogenic 78Kr/83Kr decreased from the ``top'' sample to the ``bottom'' sample (``top'' = 0.163 +/- 0.005, ``bottom'' = 0.151 +/- 0.005) while the cosmogenic 131Xe/126Xe ratio increased (``top'' = 5.58 +/- 0.35, ``bottom'' = 6.92 +/- 0.17). Cosmic-ray track studies have shown that the ``top'' sample was indeed closer to the preatmospheric surface than the ``bottom'' sample by ~ 10 cm. This is the first direct evidence, in a sample of known geometry, that the cosmogenic 131Xe/126Xe ratio increases as a function of depth, and as such, confirms the hypothesis that the lunar 131Xe anomaly is a bona fide depth effect due to resonance neutron capture in 130Ba.

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