Nickel and Chromium Stable Isotopic Composition of Ureilites: Implications for the Earth's Core Formation and Differentiation of the Ureilite Parent Body

Ke Zhu*, Jean Alix Barrat, Akira Yamaguchi, Olivier Rouxel, Yoan Germain, Jessica Langlade, Frederic Moynier

*Corresponding author for this work

Research output: Contribution to journalArticle (Academic Journal)peer-review

10 Citations (Scopus)

Abstract

We report the first Ni and Cr stable isotope data for ureilite meteorites that are the mantle residue of a carbon-rich differentiated planet. Ureilites have similar Ni stable isotope compositions as chondrites, suggesting that the core-mantle differentiation of ureilite parent body (UPB) did not fractionate Ni isotopes. Since the size of Earth is potentially larger than that of UPB; with diameter >690 km), resulting in higher temperatures at the core-mantle boundary of Earth, it can be predicted that the terrestrial core formation may not directly cause Ni stable isotope fractionation. On the other hand, we also report high-precision Cr stable isotope composition of ureilites, including one ureilitic trachyandesite (ALM-A) that is enriched in lighter Cr stable isotopes relative to the main-group ureilites, which suggests that the partial melting occurred on UPB. The globally heavy Cr in the UPB compared to chondrites can be caused by sulfur-rich core formation processes.

Original languageEnglish
Article numbere2021GL095557
JournalGeophysical Research Letters
Volume49
Issue number7
DOIs
Publication statusPublished - 16 Apr 2022

Bibliographical note

Funding Information:
We thank Steve Jacobsen for editorial handling, and Matthew Jerram and one anonymous reviewer for insightful comments. K. Zhu thanks the Alexander von Humboldt Foundation for a postdoctoral fellowship, the China Scholarship Council (CSC) for a PhD fellowship (#201706340161), and Purple Mountain Observation, CAS (host: Weibiao Hsu and Yun Jiang) for a guest fellowship during his stay in Nanjing in summer 2021. F. Moynier acknowledges funding from the European Research Council under the H2020 framework program/ERC consolidator Grant Agreement (#101001282‐METAL) and financial support of the UnivEarthS Labex program at Sorbonne Paris Cité (#ANR‐10‐LABX‐0023 and #ANR‐11‐IDEX‐0005‐02), and the ANR through a chaire d'excellence Sorbonne Paris Cité. Parts of this work were supported by IPGP multidisciplinary program PARI, by Region île‐de‐France SESAME Grants no. 12015908, EX047016 and the IdEx Université de Paris grant, ANR‐18‐IDEX‐0001, and the DIM ACAV+. Pierre Burckel and Pascale Louvat were appreciated for analysis on ICP‐MS and MC‐ICP‐MS at IPGP, respectively. US Antarctic meteorite samples were recovered by the Antarctic Search for Meteorites (ANSMET) program, which has been funded by NSF and NASA, and characterized and curated by the Department of Mineral Sciences of the Smithsonian Institution and the Astromaterials Acquisition and Curation Office at NASA Johnson Space Center. Open access funding enabled and organized by Projekt DEAL.

Funding Information:
We thank Steve Jacobsen for editorial handling, and Matthew Jerram and one anonymous reviewer for insightful comments. K. Zhu thanks the Alexander von Humboldt Foundation for a postdoctoral fellowship, the China Scholarship Council (CSC) for a PhD fellowship (#201706340161), and Purple Mountain Observation, CAS (host: Weibiao Hsu and Yun Jiang) for a guest fellowship during his stay in Nanjing in summer 2021. F. Moynier acknowledges funding from the European Research Council under the H2020 framework program/ERC consolidator?Grant Agreement (#101001282-METAL) and financial support of the UnivEarthS Labex program at Sorbonne Paris Cit? (#ANR-10-LABX-0023 and #ANR-11-IDEX-0005-02), and the ANR through a chaire d'excellence Sorbonne Paris Cit?. Parts of this work were supported by IPGP multidisciplinary program PARI, by Region ?le-de-France SESAME Grants no. 12015908, EX047016 and the IdEx Universit? de Paris grant, ANR-18-IDEX-0001, and the DIM ACAV+. Pierre Burckel and Pascale Louvat were appreciated for analysis on ICP-MS and MC-ICP-MS at IPGP, respectively. US Antarctic meteorite samples were recovered by the Antarctic Search for Meteorites (ANSMET) program, which has been funded by NSF and NASA, and characterized and curated by the Department of Mineral Sciences of the Smithsonian Institution and the Astromaterials Acquisition and Curation Office at NASA Johnson Space Center. Open access funding enabled and organized by Projekt DEAL.

Publisher Copyright:
© 2022 The Authors.

Keywords

  • core formation
  • Cr stable isotopes
  • mantle heterogeneity
  • Ni stable isotopes
  • partial melting
  • ureilites

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