Abstract:
:Nucleosynthetic isotope variability among solar system objects provides insights into the accretion history of terrestrial planets. We report on the nucleosynthetic Fe isotope composition (μ54Fe) of various meteorites and show that the only material matching the terrestrial composition is CI (Ivuna-type) carbonaceous chondrites, which represent the bulk solar system composition. All other meteorites, including carbonaceous, ordinary, and enstatite chondrites, record excesses in μ54Fe. This observation is inconsistent with protracted growth of Earth by stochastic collisional accretion, which predicts a μ54Fe value reflecting a mixture of the various meteorite parent bodies. Instead, our results suggest a rapid accretion and differentiation of Earth during the ~5-million year disk lifetime, when the volatile-rich CI-like material is accreted to the proto-Sun via the inner disk.
journal_name
Sci Advjournal_title
Science advancesauthors
Schiller M,Bizzarro M,Siebert Jdoi
10.1126/sciadv.aay7604subject
Has Abstractpub_date
2020-02-12 00:00:00pages
eaay7604issue
7issn
2375-2548pii
aay7604journal_volume
6pub_type
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