The radioactive nuclei with short half-lives present during early Solar System formation provide crucial evidence of nucleosynthetic processes and the isolation timeframe of Solar System materials.
Abundance ratios derived from decay-daughter nuclei of short-lived radionuclides reveal important information about the chronology of the early Solar System and its nucleosynthetic events.
The correlations between measured meteoric ratios and interstellar medium predictions indicate an isolation time of Solar System materials within their parent molecular clouds before solar birth.
The study of short-lived radionuclides produced in stellar environments affirms that the Sun was born from giant molecular clouds with substantial lifetimes, such as Scorpius-Centaurus.
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