Published September 2023 | Version Supplemental material
Journal Article Open

Spurious molybdenum isotope anomalies resulting from non-exponential mass fractionation

  • 1. ROR icon Brown University
  • 2. ROR icon University of Münster
  • 3. ROR icon California Institute of Technology
  • 4. ROR icon Max Planck Institute for Solar System Research

Abstract

Mass-independent (nucleosynthetic) Mo isotope anomalies are uniquely useful for constraining genetic relationships among meteoritic and planetary materials and, by extension, the origin and nature of Earth's late-stage building blocks. The meaningful interpretation of such data, however, critically depends on the accurate correction of any natural and analytical mass-dependent isotope fractionation, which is commonly assumed to follow the 'exponential law'. Here, using new high-precision Mo isotope data for a diverse set of terrestrial samples, we show that mass-dependent Mo isotope fractionation in nature typically does not adhere to this law, but is instead dominated by equilibrium and Rayleigh processes. We demonstrate that even moderate degrees of such non-exponential fractionation (i.e., mass-dependent isotope fractionation deviating from the exponential law) can result in significant spurious mass-independent Mo isotope anomalies that, when misinterpreted as nucleosynthetic anomalies, can lead to erroneous conclusions, particularly with respect to Earth's accretion history. Consequently, assessing the magnitude and origin of mass-dependent fractionation will be essential for future efforts to precisely determine the mass-independent Mo isotope composition of bulk silicate Earth and to identify potential nucleosynthetic isotope anomalies in terrestrial rocks.

Copyright and License

© 2023 Elsevier GmbH. All rights reserved.

Acknowledgement

We are grateful to S. Tappe (UiT) for providing the kimberlite samples, A. Montanari (OGC) for providing the Frontale sample, and the Denver Museum of Nature & Science for providing the Denver Basin samples (on loan to S. Bowring, MIT). This study was supported by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) – Project-ID 263649064 – TRR 170 (to T.K.) and a Geochemistry Option Postdoctoral Fellowship by Caltech (to G.B.). F.T. is grateful for support from a Walter De Logi grant from Caltech for 2019–2021, the Caltech Center for Comparative Planetary Evolution, National Science Foundation (NSF) grants EAR-1824002 and MGG-2054892, a Packard Fellowship, a research award from the Heritage Medical Research Institute, and start-up funds provided by Caltech. We thank several reviewers for their constructive comments on different versions of this manuscript. This is TRR 170 publication no. 195.

Supplemental Material

Fig. S1. Mass-dependent Mo isotope variations for samples and processed standard materials as function of Mo yield and amount of Mo (PDF).

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Related works

Funding

Deutsche Forschungsgemeinschaft
263649064 – TRR 170
California Institute of Technology
National Science Foundation
EAR-1824002
National Science Foundation
MGG-2054892
David and Lucile Packard Foundation
Packard Fellowship

Dates

Accepted
2023-06-15
Accepted
Available
2023-06-16
Available online
Available
2023-12-11
Version of record

Caltech Custom Metadata

Caltech groups
Caltech Center for Comparative Planetary Evolution, Division of Geological and Planetary Sciences (GPS), Heritage Medical Research Institute
Publication Status
Published