Fe-60 and Pu-244 deposited on Earth constrain the r-process yields of recent nearby supernovae
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Wallner, Anton; Froehlich, Michaela; Hotchkis, Michael A; Kinoshita, Norikazu; Paul, M; Martschini, Martin; Pavetich, Stefan; Tims, Steve; Kivel, N; Schumann, D; Honda, M; Matsuzaki, Hiroyuki; Yamagata, T
Description
Half of the chemical elements heavier than iron are produced by the rapid neutron capture process (r-process). The sites and yields of this process are disputed, with candidates including some types of supernovae (SNe) and mergers of neutron stars. We search for two isotopic signatures in a sample of Pacific Ocean crust-iron-60 (Fe-60) (half-life, 2.6 million years), which is predominantly produced in massive stars and ejected in supernova explosions, and plutonium-244 (Pu-244) (half-life, 80.6...[Show more]
Collections | ANU Research Publications |
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Date published: | 2021 |
Type: | Journal article |
URI: | http://hdl.handle.net/1885/294194 |
Source: | Science |
DOI: | 10.1126/science.aax3972 |
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