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Early Earth mantle heterogeneity revealed by light oxygen isotopes of Archaean komatiites

Nature Geoscience volume 10, pages 871875 (2017) | Download Citation

Abstract

Geodynamic processes on early Earth, especially the interaction between the crust and deep mantle, are poorly constrained and subject to much debate. The rarity of fresh igneous materials more than 3 billion years old accounts for much of this uncertainty. Here we examine 3.27-billion-year-old komatiite lavas from Weltevreden Formation in the Barberton greenstone belt, which is part of the Kaapvaal Craton in Southern Africa. We show that primary magmatic compositions of olivine are well preserved in these lavas based on major and trace element systematics. These komatiitic lavas represent products of deep mantle plumes. Oxygen isotope compositions (δ18O) of the fresh olivine measured by laser fluorination are consistently lighter (about 2‰) than those obtained from modern mantle-derived volcanic rocks. These results suggest a mantle source for the Weltevreden komatiites that is unlike the modern mantle and one that reflects mantle heterogeneity left over from a Hadean magma ocean. The anomalously light δ18O may have resulted from fractionation of deep magma ocean phases, as has been proposed to explain lithophile and siderophile isotope compositions of Archaean komatiites.

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Acknowledgements

Field work by G.R.B. and K.K. was funded by a grant from the National Science Foundation. Laboratory work by H.B. was partially provided by the strategic priority research program (B) of CAS (XDB18010104) and China NSFC grant 41490635. We would like to thank E. Marshall and J. Barnes of the Stable Isotope lab in the University of Texas at Austin Department of Geological Sciences for their assistance performing oxygen isotope measurements.

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Affiliations

  1. Department of Geology and Geophysics, Louisiana State University, Baton Rouge, Louisiana 70803, USA

    • Benjamin L. Byerly
    • , Keena Kareem
    • , Huiming Bao
    •  & Gary R. Byerly
  2. School of Earth & Space Sciences, Peking University, Beijing 100871, China

    • Huiming Bao

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Contributions

B.L.B. performed analyses and authored the final manuscript. K.K. performed analyses and contributed to early versions of the manuscript. H.B. performed analyses and assisted in authoring the final manuscript. G.R.B. conceived the project, collected samples from the field with K.K., and assisted in authoring the final manuscript.

Competing interests

The authors declare no competing financial interests.

Corresponding author

Correspondence to Benjamin L. Byerly.

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https://doi.org/10.1038/ngeo3054