Recent advances in high-precision
potassium (K) isotopic analysis
have found considerable isotopic variation in rock samples of the
Earth’s continental and oceanic crusts; however, it is still
uncertain whether there is any resolvable inter-mineral and mineral-melt
K isotopic fractionation during igneous and metamorphic processes.
Here, we report K isotope compositions of mineral separates from three
extremely well-preserved igneous rocks (intrusive/extrusive and mafic/intermediate/felsic)
in order to investigate possible inter-mineral and mineral-melt K
isotopic fractionation at magmatic temperatures. For the first time,
we found large inter-mineral fractionation of K isotopes in natural
samples (up to 1.072‰), where plagioclase displays a significant
enrichment of heavier K isotopes compared to potassium feldspar and
biotite in granite. In addition, we also observed smaller but measurable
K isotope fractionation (0.280 ± 0.030‰) between ternary
feldspar phenocrysts and matrices in a trachyandesite, as well as
a comparable isotope fractionation (0.331 ± 0.010‰) between
plagioclase and the bulk in a gabbroic intrusive rock. We also evaluated
such results by comparing the theoretically calculated equilibrium
K isotope fractionation factors between relevant igneous minerals
in the literature and this study. In general, the measured inter-mineral
fractionations are consistent with the theoretical calculations (i.e.,
plagioclase is enriched in heavier isotopes compared to potassium
feldspar). Specifically, the measured K isotope fractionation between
the phenocryst rim and matrix in the trachyandesite agrees well with
the calculated equilibrium isotope fractionation. However, the measured
K isotope fractionations between the phenocryst core and matrix as
well as between plagioclase and K-feldspar are significantly larger
(by a factor of ∼2–3) than the calculated isotope fractionations,
which suggest isotopic disequilibrium due to kinetic processes. Using
a range of plagioclase-melt isotope fractionation factors inferred
from the theoretical calculations in this study, we modeled the K
isotopic fractionation during the formation of lunar anorthositic
crust, and the result shows a negligible effect on the K isotopic
compositions in both lunar crust and mantle. The K isotopic difference
between the Earth and the Moon, therefore, cannot be the result of
lunar magma ocean differentiation. Finally, we evaluate the effect
of observed inter-mineral fractionations on K–Ar and 40Ar–39Ar dating. This study indicates that the variation
of the 40K/K ratio would contribute a maximum 0.08% error
to the K–Ar and 40Ar–39Ar age
uncertainties. We propose a refined 40K/total K ratio as
0.00011664 ± 0.00000011 (116.64 ± 0.11 ppm) instead of the
conventional value, 0.0001167(2), for the present Earth. Because some
minerals fractionate K isotopes, ultrahigh-precision age dating with
the K–Ca–Ar dating systems must measure the K isotope
fractionation in the same mineral fractions used for age dating.