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• W2486696937 endingPage "541" @default.
• W2486696937 startingPage "517" @default.
• W2486696937 abstract "Although scientists had previously believed that the chemical elements were synthesized only in stars, the discovery of the Oko reactor has revealed that a nuclear fire had existed in the earth billions of years ago. The existence of 83-m.y. 244Pu in the early solar system, on the other hand, may be regarded as a direct evidence that elements heavier than uranium were synthesized in supernova. Variations in the ratios of stable isotopes of 0, Ne, Mg, Ca, Ti, Kr, Ag, Te, Xe, Ba, Ce, Nd, Sm, and Gd in meteorites have recently been reported and these anomalies are generally attributed to the heterogeneity of the solar nebula at the time of its condensation. Decay products of 16-m.y. 129I, 6.5-m.y. 107Pd and 0.73-m.y. 26Al have also been identified in various meteorites, but the origins of these extinct radionuclides are not yet fully understood. It seems, however, that the anomalies observed in the stable isotopes of various elements in meteorites and the occurrence of extinct radionuclides such as 129I, 107Pd and 26Al can be explained as due to a combined effect of mass-fractionation, neutron-capture and spallation processes which took place prior to and/or during the formation of the solar system." @default.
• W2486696937 created "2016-08-23" @default.
• W2486696937 creator A5049289428 @default.
• W2486696937 date "1982-01-01" @default.
• W2486696937 modified "2023-09-26" @default.
• W2486696937 title "RADIOACTIVE AND STABLE ISOTOPES IN THE EARLY SOLAR SYSTEM" @default.
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• W2486696937 doi "https://doi.org/10.1016/b978-0-08-027544-4.50046-0" @default.
• W2486696937 hasPublicationYear "1982" @default.
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