Age of Jupiter inferred from the distinct genetics and formation times of meteorites

Kruijer, Thomas S.; Burkhardt, Christoph; Budde, Gerrit; Kleine, Thorsten

doi:10.1073/pnas.1704461114

Title: Age of Jupiter inferred from the distinct genetics and formation times of meteorites

Journal Article · Mon Jun 12 00:00:00 EDT 2017 · Proceedings of the National Academy of Sciences of the United States of America

DOI:https://doi.org/10.1073/pnas.1704461114· OSTI ID:1399762

Kruijer, Thomas S. ^[1]; Burkhardt, Christoph ^[2];

^[2]; Kleine, Thorsten ^[2]

Univ. of Munster, Muenster (Germany); Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
Univ. of Munster, Muenster (Germany)

The age of Jupiter, the largest planet in our Solar System, is still unknown. Gas-giant planet formation likely involved the growth of large solid cores, followed by the accumulation of gas onto these cores. Thus, the gas-giant cores must have formed before dissipation of the solar nebula, which likely occurred within less than 10 My after Solar System formation. Although such rapid accretion of the gas-giant cores has successfully been modeled, until now it has not been possible to date their formation. Here, using molybdenum and tungsten isotope measurements on iron meteorites, we demonstrate that meteorites derive from two genetically distinct nebular reservoirs that coexisted and remained spatially separated between ~1 My and ~3–4 My after Solar System formation. The most plausible mechanism for this efficient separation is the formation of Jupiter, opening a gap in the disk and preventing the exchange of material between the two reservoirs. As such, our results indicate that Jupiter’s core grew to ~20 Earth masses within <1 My, followed by a more protracted growth to ~50 Earth masses until at least ~3–4 My after Solar System formation. Furthermore, Jupiter is the oldest planet of the Solar System, and its solid core formed well before the solar nebula gas dissipated, consistent with the core accretion model for giant planet formation.

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

Sponsoring Organization:: USDOE

Grant/Contract Number:: AC52-07NA27344

OSTI ID:: 1399762

Report Number(s):: LLNL-JRNL-731226

Journal Information:: Proceedings of the National Academy of Sciences of the United States of America, Vol. 114, Issue 26; ISSN 0027-8424

Publisher:: National Academy of Sciences, Washington, DC (United States)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 346 works

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The role of Bells in the continuous accretion between theCMandCRchondrite reservoirs Kooten, Elishevah; Cavalcante, Larissa; Wielandt, Daniel Meteoritics & Planetary Science, Vol. 55, Issue 3 https://doi.org/10.1111/maps.13459	journal	March 2020
Astronomical context of Solar System formation from molybdenum isotopes in meteorite inclusions Brennecka, Gregory A.; Burkhardt, Christoph; Budde, Gerrit Science, Vol. 370, Issue 6518 https://doi.org/10.1126/science.aaz8482	journal	November 2020
Meteorite evidence for partial differentiation and protracted accretion of planetesimals. Maurel, Clara; Bryson, James FJ; Lyons, Richard J. American Association for the Advancement of Science (AAAS) https://doi.org/10.17863/cam.57168	journalarticle	January 2020
The Origin of S-Process Isotope Heterogeneity in the Solar Protoplanetary Disk Ek, Mattias; Hunt, Alison C.; Lugaro, Maria Goldschmidt2020, Goldschmidt Abstracts https://doi.org/10.46427/gold2020.655	conference	January 2020
Late metal-silicate separation on the IAB parent asteroid: Constraints from combined W and Pt isotopes and thermal modelling Hunt, Alison C.; Cook, David L.; Lichtenberg, Tim arXiv https://doi.org/10.48550/arxiv.1802.10421	text	January 2018
Chemically defining the building blocks of the Earth Yoshizaki, Takashi; Ash, Richard D.; Yokoyama, Tetsuya arXiv https://doi.org/10.48550/arxiv.1812.11717	preprint	January 2018
Migration of D-type asteroids from the outer Solar System inferred from carbonate in meteorites Fujiya, Wataru; Hoppe, Peter; Ushikubo, Takayuki arXiv https://doi.org/10.48550/arxiv.1905.13620	text	January 2019
Elemental and isotopic variability in solar system materials by mixing and processing of primordial disk reservoirs Burkhardt, Christoph; Dauphas, Nicolas; Hans, Ulrik arXiv https://doi.org/10.48550/arxiv.1907.01276	text	January 2019
Oxygen Isotopic Composition of an Enstatite Ribbon of Probable Cometary Origin Ogliore, Ryan C.; Brownlee, Donald E.; Nagashima, Kazuhide arXiv https://doi.org/10.48550/arxiv.1907.11177	text	January 2019
Origin of Earth's water: sources and constraints Meech, Karen; Raymond, Sean N. arXiv https://doi.org/10.48550/arxiv.1912.04361	text	January 2019
Planet formation: key mechanisms and global models Raymond, Sean N.; Morbidelli, Alessandro arXiv https://doi.org/10.48550/arxiv.2002.05756	text	January 2020
Origin and dynamical evolution of the asteroid belt Raymond, Sean N.; Nesvorny, David arXiv https://doi.org/10.48550/arxiv.2012.07932	text	January 2020
A pebble accretion model for the formation of the terrestrial planets in the Solar System Johansen, Anders; Ronnet, Thomas; Bizzarro, Martin arXiv https://doi.org/10.48550/arxiv.2102.08611	preprint	January 2021
Planetesimal rings as the cause of the Solar System's planetary architecture Izidoro, Andre; Dasgupta, Rajdeep; Raymond, Sean N. arXiv https://doi.org/10.48550/arxiv.2112.15558	text	January 2021
The late accretion and erosion of Vesta’s crust recorded by eucrites and diogenites as an astrochemical window into the formation of Jupiter and the early evolution of the Solar System Turrini, D.; Svetsov, V.; Consolmagno, G. Elsevier https://doi.org/10.7892/boris.116518	text	January 2018

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