Abstract
WE thank Alexander and Schwartzman (AS)1 for bringing to light a significant error in data point 18 (Table 1) of our paper2. Because of a misinterpretation of a verbal communication from Mueller, we omitted sample 30 in our regression of the data from Baadsgard and Mueller3. We confirm that there is no reason for omitting this sample, and that the data indicate that the non-radiogenic argon present cannot be distinguished from atmospheric contamination. We concur with Alexander and Schwartzman, however, on little else, and consider as still valid the four principal points summarised at the end of our paper2: first, the initial 40Ar/36Ar ratios of mantle-derived igneous rocks have increased steadily over the past 800 Myr. Second, the present day 40Ar/36Ar ratios in the upper mantle and atmosphere are very similar. Third, the majority of argon at present in the atmosphere has been derived from the mantle rather than the crust, and fourth, initial 40Ar/36Ar ratios from igneous rocks are potentially more sensitive petrogenetic indicators than strontium or lead isotopes.
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BROWN, J., ODOM, A. & HARPER, C. Argon isotopic evolution of upper mantle (reply). Nature 259, 106–108 (1976). https://doi.org/10.1038/259106a0
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DOI: https://doi.org/10.1038/259106a0
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