Published June 3, 2026 | Version v7

Metal saturation experiments and compositional modelling for the lunar mantle

  • 1. ROR icon Ruhr University Bochum
  • 2. Ruhr-University Bochum
  • 3. Universidade Federal de Rio Grande to Sul

Description

"This dataset contains supporting data tables for the manuscript:
Fonseca, R. O. C., Beyer, C., Schuth, S., & Leitzke, F. P. (2026). The case for metal saturation in the lunar mantle. Advances in Geochemistry and Cosmochemistry, 2(1), 754. https://doi.org/10.33063/agc.v2i1.754

EPMA raw data.xlsx: Electron microprobe raw data for melt, metal and olivine major element composition (and detection limits) of experimental run products

Data Tables.xlsx: Six main text tables from Fonseca et al. (2026) that provide: calculated oxygen fugacities, experimental starting compositions, experimental run conditions, summary of the major and trace element contents of each of the experimental run products, calculated modal abundances and mineral/melt partition coefficients

Supplementary Tables: Modeled HSE, Mo and W abundances of lunar parental magmas; compilation of literature values for high-field strength and highly siderophile elements in lunar basalts.

fO2 calculation from metal-silicate equilibria.xlsx: Spreadsheet that can be used to calculate fO2 of metal-silicate-melt experiments, using the Fe and S contents of metal and FeO contents of coexisting silicate melt based on the activity composition relationships for the Fe-FeS system depicted in Buono, A. S., & Walker, D. (2011). The Fe-rich liquidus in the Fe–FeS system from 1 bar to 10 GPa. Geochimica et Cosmochimica Acta, 75(8), 2072-2087. Also included, is the Monte-Carlo error propagation method used to determine uncertainties on calculated fO2 values. 

Data Sources:

Brunfelt, A. O., & Steinnes, E. (1971). A neutron-activation scheme developed for the determination of 42 elements in lunar material. Talanta, 18(12), 1197-1208.
Day, J. M., Pearson, D. G., & Taylor, L. A. (2007). Highly siderophile element constraints on accretion and differentiation of the Earth-Moon system. Science, 315(5809), 217-219. https://doi.org/10.1126/science.1133355
Neal C.R. (2001) Interior of the moon: The presence of garnet in the primitive deep lunar mantle. J. Geophys. Res. 106, 27865-27885.
Morrison G.H., Gerard J.T., Kashuba A.T., Gangadharam E.V., Rothenberg A.M., Potter N.M. and Miller G.B. (1970) Elemental abundances of lunar soil and rocks. Proc. Apollo 11 Lunar Sci. Conf. 1383-1392.
Newsom, H. E., & Maehr, S. A. (1993, March). Core formation in the Moon: The mystery of the excess depletion of Mo, W and P. In In Lunar and Planetary Inst., Twenty-Fourth Lunar and Planetary Science Conference. Part 3: NZ p 1071-1072 (SEE N94-20636 05-91) (Vol. 24).
Klein C., Drake J.C. and Frondel C. (1971) Mineralogical, petrological, and chemical features of four Apollo 12 lunar microgabbros. Proc. 2nd Lunar Sci. Conf. 265-284.
Neal C.R. (2001) Interior of the moon: The presence of garnet in the primitive deep lunar mantle. J. Geophys. Res. 106, 27865-27885.
Taylor, S. R., Muir, P., & Kaye, M. (1971). Trace element chemistry of Apollo 14 lunar soil from Fra Mauro. Geochimica et Cosmochimica Acta, 35(9), 975-981.
Wänke, H., Wlotzka, F., Baddenhausen, H., Balacescu, A., Spettel, B., Teschke, F., ... & Rieder, R. (1971). Apollo 12 samples: Chemical composition and its relation to sample locations and exposure ages, the two-component origin of the various soil samples and studies on lunar metallic particles. In Proceedings of the Lunar Science Conference, vol. 2, p. 1187 (Vol. 2, p. 1187).
Wänke, H., Baddenhausen, H., Balacescu, A., Teschke, F., Spettel, B., Dreibus, G., ... & Begemann, F. (1972). Multielement analyses of lunar samples and some implications of the results. In Proceedings of the Lunar Science Conference, vol. 3, p. 1251 (Vol. 3, p. 1251).

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Cites
Journal article: 10.1126/science.1133355 (DOI)
Is supplement to
Journal article: 10.33063/agc.v2i1.754 (DOI)