The vanadium isotopic composition of lunar basalts
The vanadium isotopic composition of lunar basalts
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DOI:
10.1016/j.epsl.2019.01.008
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发表时间:
2019-04
影响因子:
5.3
通讯作者:
S. Hopkins;J. Prytulak;J. Barling;S. Russell;B. Coles;A. Halliday
中科院分区:
文献类型:
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作者:
S. Hopkins;J. Prytulak;J. Barling;S. Russell;B. Coles;A. Halliday
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 (ie higher 51 V/50 V) 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 (t e). 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 t e⁎[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.