The great isotopic dichotomy of the early Solar System

Kruijer, Thomas S.; Kleine, Thorsten; Borg, Lars E.

doi:10.1038/s41550-019-0959-9

The great isotopic dichotomy of the early Solar System

Journal Article · Mon Dec 16 00:00:00 UTC 2019 · Nature Astronomy

DOI:https://doi.org/10.1038/s41550-019-0959-9· OSTI ID:1592039

^[1]; ^[2]; Borg, Lars E. ^[1]

Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
Univ. of Münster (Germany)

The isotopic composition of meteorites and terrestrial planets holds important clues about the earliest history of the Solar System and the processes of planet formation. Recent work has shown that meteorites exhibit a fundamental isotopic dichotomy between non-carbonaceous (NC) and carbonaceous (CC) groups, which most likely represent material from the inner and outer Solar System, respectively. Here we review the isotopic evidence for this NC–CC dichotomy, discuss its origin and highlight the far-reaching implications for the dynamics of the solar protoplanetary disk. The NC–CC dichotomy combined with the chronology of meteorite parent-body accretion mandate an early and prolonged spatial separation of inner (NC) and outer (CC) disk reservoirs, lasting between ~1 and ~4 Myr after Solar System formation. This is most easily reconciled with the early and rapid growth of Jupiter’s core, inhibiting substantial exchange of material from inside and outside its orbit. Here, the growth and migration of Jupiter also led to the later implantation of CC bodies into the inner Solar System and, therefore, can explain the co-occurrence of NC and CC bodies in the asteroid belt, and the delivery of volatile and water-rich CC bodies to the terrestrial planets.

View Accepted Manuscript (DOE)

Research Organization:: Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)

Sponsoring Organization:: USDOE National Nuclear Security Administration (NNSA)

Grant/Contract Number:: AC52-07NA27344

OSTI ID:: 1592039

Report Number(s):: LLNL-JRNL--798366; 1000953

Journal Information:: Nature Astronomy, Journal Name: Nature Astronomy Journal Issue: 1 Vol. 4; ISSN 2397-3366

Publisher:: Springer NatureCopyright Statement

Country of Publication:: United States

Language:: English

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Isotopic Evolution of the Inner Solar System Inferred from Molybdenum Isotopes in Meteorites

Journal Article · Thu Jul 16 00:00:00 UTC 2020 · The Astrophysical Journal. Letters (Online) · OSTI ID:1823221

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58 GEOSCIENCES
Jupiter
Meteorites
accretion
isotopes
planetesimals
protoplanetary disk
short-lived radionuclides

The great isotopic dichotomy of the early Solar System

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