Behavior of the Mo, Tl, and U isotope systems during differentiation in the Kilauea Iki lava lake

Richard M. Gaschnig, Shelby T. Rader, Christopher T. Reinhard, Jeremy D. Owens, Noah Planavsky, Xiangli Wang, Dan Asael, Allison Greaney, Rosalind Helz

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Abstract

Stable molybdenum (Mo), thallium (Tl), and uranium (U) isotope ratios were determined in a suite of samples from the 1959 Kilauea eruption and from Kilauea Iki lava lake with the aim of understanding the effects of igneous differentiation on these isotope systems. The samples range from olivine cumulate with MgO up to 27% to internal differentiates with MgO less than 3%, representing a tholeiitic differentiation series. Molybdenum, Tl, and U behave incompatibly during differentiation, and Mo and U isotope ratios do not systematically vary amongst the different samples. δ98Mo values range from −0.17 to −0.31‰ and δ238U values range from −0.20 to −0.38‰. Most individual analyses for both isotope systems overlap within measurement uncertainty (± ~0.7 and ~ 0.6, respectively). Mean δ98Mo and δ238U values are −0.22 ± 0.08‰ (2σ) and − 0.29 ± 0.09‰ (2σ), respectively, which overlap with Pacific mid ocean ridge basalt (MORB). In contrast, Tl isotopes show small but resolvable variations, with ε205Tl ranging from +1.20 to −1.38. The most negative ε205Tl values are confined to some of the lowest [Tl] samples, but the ε205Tl values do not otherwise vary smoothly with MgO or [Tl]. Possible mechanisms for thallium isotope fractionation are considered (e.g., degassing, water leaching, sulfide fractionation) but none are found to be satisfactory. Overall, the lack of resolvable variation in the Mo and U isotope systems and the small magnitude of heterogeneity in the Tl isotope system indicate that differentiation in tholeiitic systems is unlikely to be a major contributor to global variation in these isotope systems.

Original languageEnglish
Article number120239
JournalChemical Geology
Volume574
DOIs
StatePublished - Jul 20 2021

Funding

This research was supported with funding from the National Science Foundation, the NASA Astrobiology Institute, and NASA Exobiology to JDO ( NNX16AJ60G and 80NSSC18K1532 ). A portion of this work was performed at the National High Magnetic Field Laboratory, which is supported by NSF Cooperative Agreement DMR-1157490 and the State of Florida. CTR and NJP acknowledge funding from the NASA Astrobiology Institute. We thank two anonymous reviewers of this manuscript along three anonymous reviewers of an earlier version for their constructive comments.

FundersFunder number
State of Florida
National Science FoundationDMR-1157490
National Aeronautics and Space Administration80NSSC18K1532, NNX16AJ60G
NASA Astrobiology Institute

    Keywords

    • Fractional crystallization
    • Mo isotopes
    • Tl isotopes
    • U isotopes

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