S.S. Hopkins
The vanadium isotopic composition of lunar basalts
Hopkins, S.S.; Prytulak, J.; Barling, J.; Russell, S.S.; Coles, B.J.; Halliday, A.N.
Authors
Professor Julie Prytulak julie.prytulak@durham.ac.uk
Visitor
J. Barling
S.S. Russell
B.J. Coles
A.N. Halliday
Abstract
We present the first high-precision vanadium (V) isotope data for lunar basalts. Terrestrial magmatic rock measurements can display significant V isotopic fractionation (particularly during (Fe, Ti)oxide crystallisation), but the Earth displays heavy V (i.e. higher 51V/50V) isotopic compositions compared to meteorites. This has been attributed to early irradiation of meteorite components or nucleosynthetic heterogeneity. The Moon is isotopically-indistinguishable from the silicate Earth for many refractory elements and is expected to be similar in its V isotopic composition. Vanadium isotope ratios and trace element concentrations were measured for 19 lunar basalt samples. Isotopic compositions are more variable (∼2.5‰) than has been found thus far for terrestrial igneous rocks and extend to lighter values. Magmatic processes do not appear to control the V isotopic composition, despite the large range in oxide proportions in the suite. Instead, the V isotopic compositions of the lunar samples are lighter with increasing exposure age (). Modelling nuclear cross-sections for V production and burnout demonstrates that cosmogenic production may affect V isotope ratios via a number of channels but strong correlations between V isotope ratios and ⁎ [Fe]/[V] implicate Fe as the primary target element of importance. Similar correlations are found in the latest data for chondrites, providing evidence that most V isotope variation in chondrites is due to recent cosmogenic production via Fe spallation. Contrary to previous suggestions, there is no evidence for resolvable differences between the primary V isotopic compositions of the Earth, Moon, chondrites and Mars.
Citation
Hopkins, S., Prytulak, J., Barling, J., Russell, S., Coles, B., & Halliday, A. (2019). The vanadium isotopic composition of lunar basalts. Earth and Planetary Science Letters, 511, 12-24. https://doi.org/10.1016/j.epsl.2019.01.008
Journal Article Type | Article |
---|---|
Acceptance Date | Jan 3, 2019 |
Online Publication Date | Feb 1, 2019 |
Publication Date | Feb 1, 2019 |
Deposit Date | Feb 1, 2019 |
Publicly Available Date | Feb 5, 2019 |
Journal | Earth and Planetary Science Letters |
Print ISSN | 0012-821X |
Electronic ISSN | 1385-013X |
Publisher | Elsevier |
Peer Reviewed | Peer Reviewed |
Volume | 511 |
Pages | 12-24 |
DOI | https://doi.org/10.1016/j.epsl.2019.01.008 |
Public URL | https://durham-repository.worktribe.com/output/1308726 |
Files
Published Journal Article
(1.2 Mb)
PDF
Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/
Copyright Statement
© 2019 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license(http://creativecommons.org/licenses/by/4.0/).
You might also like
Rhenium isotope variations in Icelandic groundwaters and hydrothermal systems
(2024)
Journal Article
Rhenium Isotopes Record Oxidative Weathering Intensity in Sedimentary Rocks
(2024)
Journal Article
Rhenium elemental and isotopic variations at magmatic temperatures
(2024)
Journal Article
No V-Fe-Zn isotopic variation in basalts from the 2021 Fagradalsfjall eruption
(2023)
Journal Article