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Meteoritic analysis demonstrates that radioactive nuclei heavier than iron were present in the early Solar System. Among them, 129I and 247Cm both have a rapid neutron-capture process (r process) origin and decay on the same timescale (≃ 15.6 Myr). We show that the 129I/247Cm abundance ratio in the early Solar System (438±184) is immune to galactic evolution uncertainties and represents the first direct observational constraint for the properties of the last r-process event that polluted the pre-solar nebula. We investigate the physical conditions of this event using nucleosynthesis calculations and demonstrate that moderately neutron-rich ejecta can produce the observed ratio. We conclude that a dominant contribution by exceedingly neutron-rich ejecta is highly disfavoured.more » « less
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Hall, O. ; Davinson, T. ; Estrade, A. ; Liu, J. ; Lorusso, G. ; Montes, F. ; Nishimura, S. ; Phong, V.H. ; Woods, P.J. ; Agramunt, J. ; et al ( , Physics Letters B)null (Ed.)