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• W2000791282 abstract "The isotopic composition of Mg is investigated in meteoritic, lunar and terrestrial feldspar samples and standard reagents using a mass spectrometer with on-line data processing. Isotopically enriched standards were run demonstrating a resolution of better than five parts in 104 for the26Mg/24Mg ratio.No26Mg/24Mganomalies are found in any samples analyzed to within experimental errors. (These analyses include some samples run by Clarke, de Laeter, Schwarcz and Shane [1] and found by them to have26Mg/24Mg anomalies of 4–6 parts in 103 relative to terrestrial values.) There is at the present time no positive evidence indicating the existence of26Al in the early solar system. From these results, limits are placed on the amount of26Al(τ½ = 7.4 × 105yr) and the resulting heating effects in the solar system at the time of crystallization of the meteorites. It is clear that when the meteorites solidified,26Al was not an important heat source; however, this would not rule out the possibility that a few million years prior to solidification26Al was a major heat source." @default.
• W2000791282 created "2016-06-24" @default.
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• W2000791282 date "1970-12-01" @default.
• W2000791282 modified "2023-10-14" @default.
• W2000791282 title "The isotopic abundance of26Mg and limits on26Al in the early solar system" @default.
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• W2000791282 doi "https://doi.org/10.1016/0012-821x(70)90063-4" @default.
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