Cosmogenic 26Al was measured in six samples from two cores of the Keyes chondrite, previously analyzed for spallogenic 3He, 21Ne, and 38Ar. Specific activities varied from 68.9 ± 5.4 dpm/kg near the center (depth, ∼30 cm) to 50.9 ± 3.7 near the postatmospheric surface (depth, ∼3 cm). The data are consistent with an approximately linear decrease in 26Al activity with radial distance r from the center of Keyes: (26Al)obs/(26Al)calc = 1.04 (±0.05) − 0.0104 (±0.0032)(r). The measured 26Al (dpm/kg)/21Ne(10−8 cm3/g) ratio is constant at 6.13 ± 0.18 for the six samples, corresponding to an average atomic production ratio of 0.222 for the meteorite.
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P. J. Cressy (1975) studied this question.
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