Hybrid Accretion of Carbonaceous Chondrites by Radial Transport across the Jupiter Barrier

Research output: Contribution to journalJournal articlepeer-review

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Hybrid Accretion of Carbonaceous Chondrites by Radial Transport across the Jupiter Barrier. / van Kooten, Elishevah; Schiller, Martin; Moynier, Frederic; Johansen, Anders; Haugbolle, Troels; Bizzarro, Martin.

In: Astrophysical Journal, Vol. 910, No. 1, 70, 03.2021.

Research output: Contribution to journalJournal articlepeer-review

Harvard

van Kooten, E, Schiller, M, Moynier, F, Johansen, A, Haugbolle, T & Bizzarro, M 2021, 'Hybrid Accretion of Carbonaceous Chondrites by Radial Transport across the Jupiter Barrier', Astrophysical Journal, vol. 910, no. 1, 70. https://doi.org/10.3847/1538-4357/abd9c8

APA

van Kooten, E., Schiller, M., Moynier, F., Johansen, A., Haugbolle, T., & Bizzarro, M. (2021). Hybrid Accretion of Carbonaceous Chondrites by Radial Transport across the Jupiter Barrier. Astrophysical Journal, 910(1), [70]. https://doi.org/10.3847/1538-4357/abd9c8

Vancouver

van Kooten E, Schiller M, Moynier F, Johansen A, Haugbolle T, Bizzarro M. Hybrid Accretion of Carbonaceous Chondrites by Radial Transport across the Jupiter Barrier. Astrophysical Journal. 2021 Mar;910(1). 70. https://doi.org/10.3847/1538-4357/abd9c8

Author

van Kooten, Elishevah ; Schiller, Martin ; Moynier, Frederic ; Johansen, Anders ; Haugbolle, Troels ; Bizzarro, Martin. / Hybrid Accretion of Carbonaceous Chondrites by Radial Transport across the Jupiter Barrier. In: Astrophysical Journal. 2021 ; Vol. 910, No. 1.

Bibtex

@article{e6500b1e6cbc4175a973abc9dd9ad5f0,
title = "Hybrid Accretion of Carbonaceous Chondrites by Radial Transport across the Jupiter Barrier",
abstract = "Understanding the origin of chondritic components and their accretion pathways is critical to unraveling the magnitude of mass transport in the protoplanetary disk, as well as the accretionary history of the terrestrial planet region and, by extension, its prebiotic inventory. Here we trace the heritage of pristine components from the relatively unaltered CV chondrite Leoville through their mass-independent Cr and mass-dependent Zn isotope compositions. Investigating these chondritic fractions in such detail reveals an onion-shell structure of chondrules, which is characterized by Cr-54- and Zn-66-poor cores surrounded by increasingly Cr-54- and Zn-66-rich igneous rims and an outer coating of fine-grained dust. This is interpreted as a progressive addition of Cr-54- and Zn-66-rich, CI-like material to the accretion region of these carbonaceous chondrites. Our findings show that the observed Cr isotopic range in chondrules from more altered CV chondrites is the result of chemical equilibration between the chondrules and matrix during secondary alteration. The Cr-54-poor nature of the cores of Leoville chondrules implies formation in the inner solar system and subsequent massive outward chondrule transport past the Jupiter barrier. At the same time, CI-like dust is transferred inward. We propose that the accreting Earth acquired CI-like dust through this mechanism within the lifetime of the disk. This radial mixing of the chondrules and matrix shows the limited capacity of Jupiter to act as an efficient barrier and maintain the proposed noncarbonaceous and carbonaceous chondrite dichotomy over time. Finally, also considering current astrophysical models, we explore both inner and outer solar system origins for the CV chondrite parent body.",
keywords = "Protoplanetary disks",
author = "{van Kooten}, Elishevah and Martin Schiller and Frederic Moynier and Anders Johansen and Troels Haugbolle and Martin Bizzarro",
year = "2021",
month = mar,
doi = "10.3847/1538-4357/abd9c8",
language = "English",
volume = "910",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing, Inc",
number = "1",

}

RIS

TY - JOUR

T1 - Hybrid Accretion of Carbonaceous Chondrites by Radial Transport across the Jupiter Barrier

AU - van Kooten, Elishevah

AU - Schiller, Martin

AU - Moynier, Frederic

AU - Johansen, Anders

AU - Haugbolle, Troels

AU - Bizzarro, Martin

PY - 2021/3

Y1 - 2021/3

N2 - Understanding the origin of chondritic components and their accretion pathways is critical to unraveling the magnitude of mass transport in the protoplanetary disk, as well as the accretionary history of the terrestrial planet region and, by extension, its prebiotic inventory. Here we trace the heritage of pristine components from the relatively unaltered CV chondrite Leoville through their mass-independent Cr and mass-dependent Zn isotope compositions. Investigating these chondritic fractions in such detail reveals an onion-shell structure of chondrules, which is characterized by Cr-54- and Zn-66-poor cores surrounded by increasingly Cr-54- and Zn-66-rich igneous rims and an outer coating of fine-grained dust. This is interpreted as a progressive addition of Cr-54- and Zn-66-rich, CI-like material to the accretion region of these carbonaceous chondrites. Our findings show that the observed Cr isotopic range in chondrules from more altered CV chondrites is the result of chemical equilibration between the chondrules and matrix during secondary alteration. The Cr-54-poor nature of the cores of Leoville chondrules implies formation in the inner solar system and subsequent massive outward chondrule transport past the Jupiter barrier. At the same time, CI-like dust is transferred inward. We propose that the accreting Earth acquired CI-like dust through this mechanism within the lifetime of the disk. This radial mixing of the chondrules and matrix shows the limited capacity of Jupiter to act as an efficient barrier and maintain the proposed noncarbonaceous and carbonaceous chondrite dichotomy over time. Finally, also considering current astrophysical models, we explore both inner and outer solar system origins for the CV chondrite parent body.

AB - Understanding the origin of chondritic components and their accretion pathways is critical to unraveling the magnitude of mass transport in the protoplanetary disk, as well as the accretionary history of the terrestrial planet region and, by extension, its prebiotic inventory. Here we trace the heritage of pristine components from the relatively unaltered CV chondrite Leoville through their mass-independent Cr and mass-dependent Zn isotope compositions. Investigating these chondritic fractions in such detail reveals an onion-shell structure of chondrules, which is characterized by Cr-54- and Zn-66-poor cores surrounded by increasingly Cr-54- and Zn-66-rich igneous rims and an outer coating of fine-grained dust. This is interpreted as a progressive addition of Cr-54- and Zn-66-rich, CI-like material to the accretion region of these carbonaceous chondrites. Our findings show that the observed Cr isotopic range in chondrules from more altered CV chondrites is the result of chemical equilibration between the chondrules and matrix during secondary alteration. The Cr-54-poor nature of the cores of Leoville chondrules implies formation in the inner solar system and subsequent massive outward chondrule transport past the Jupiter barrier. At the same time, CI-like dust is transferred inward. We propose that the accreting Earth acquired CI-like dust through this mechanism within the lifetime of the disk. This radial mixing of the chondrules and matrix shows the limited capacity of Jupiter to act as an efficient barrier and maintain the proposed noncarbonaceous and carbonaceous chondrite dichotomy over time. Finally, also considering current astrophysical models, we explore both inner and outer solar system origins for the CV chondrite parent body.

KW - Protoplanetary disks

U2 - 10.3847/1538-4357/abd9c8

DO - 10.3847/1538-4357/abd9c8

M3 - Journal article

VL - 910

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 1

M1 - 70

ER -

ID: 259828334