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The abundance of long-lived radionuclides and their daughter products provides information on the chemical evolution of the system where they are found. Knowledge of the decay constants for these radionuclides permits to quantify evolutionary histories at time scales, which are comparable to their half-lives.
Because the half-life of 126Sn is short as compared to the age of the solar system, there is no 126Sn left from nucleosynthesis. 126Sn in the present terrestrial environment is therefore limited to contributions from spontaneous fission of 238U and to anthropogenic input. The service determined of the isotope abundance of 126Sn in the same material by thermal ionization mass spectrometry (TIMS) , which minimizes the error contribution to the overall uncertainty of the decay constant.