Benoit Côté
129I and 247Cm in meteorites constrain the last astrophysical source of solar r-process elements
Côté, Benoit; Eichler, Marius; Yagüe, Andrés; Vassh, Nicole; R. Mumpower, Matthew; Világos, Blanka; Soós, Benjámin; Arcones, Almudena; M. Sprouse, Trevor; Surman, Rebecca; Pignatari, Marco; Pet?, Mária K.; Wehmeyer, Benjamin; Rauscher, Thomas; Lugaro, Maria
Authors
Marius Eichler
Andrés Yagüe
Nicole Vassh
Matthew R. Mumpower
Blanka Világos
Benjámin Soós
Almudena Arcones
Trevor M. Sprouse
Rebecca Surman
Marco Pignatari
Mária K. Pet?
Benjamin Wehmeyer
Thomas Rauscher
Maria Lugaro
Abstract
Meteoritic analysis demonstrates that radioactive nuclei heavier than iron were present in the early Solar System. Among them, $^{129}$I and $^{247}$Cm both have a rapid neutron-capture process ($r$ process) origin and decay on the same timescale ($\simeq$ 15.6 Myr). We show that the $^{129}$I/$^{247}$Cm abundance ratio in the early Solar System (438$\pm$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.
Citation
Côté, B., Eichler, M., Yagüe, A., Vassh, N., R. Mumpower, M., Világos, B., …Lugaro, M. (2021). 129I and 247Cm in meteorites constrain the last astrophysical source of solar r-process elements. Science, 371(6532), 945-948. https://doi.org/10.1126/science.aba1111
Journal Article Type | Article |
---|---|
Acceptance Date | Jan 25, 2021 |
Online Publication Date | Feb 26, 2021 |
Publication Date | Feb 26, 2021 |
Deposit Date | Dec 17, 2020 |
Publicly Available Date | Mar 22, 2021 |
Journal | Science |
Print ISSN | 0036-8075 |
Publisher | American Association for the Advancement of Science |
Peer Reviewed | Peer Reviewed |
Volume | 371 |
Issue | 6532 |
Pages | 945-948 |
DOI | https://doi.org/10.1126/science.aba1111 |
Keywords | Solar and Stellar Astrophysics; High Energy Astrophysical Phenomena; Nuclear Theory |
Public URL | https://hull-repository.worktribe.com/output/3523740 |
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Copyright Statement
This is the author's version of the work. It is posted here by permission of the AAAS for personal use, not for redistribution. The definitive version was published in Science vol. 371, 26 Feb 2021, 10.1126/science.aba1111
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