Spurious molybdenum isotope anomalies resulting from non-exponential mass fractionation
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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Additional details
- 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
- Accepted
-
2023-06-15Accepted
- Available
-
2023-06-16Available online
- Available
-
2023-12-11Version of record
- Caltech groups
- Caltech Center for Comparative Planetary Evolution, Division of Geological and Planetary Sciences, Heritage Medical Research Institute
- Publication Status
- Published