Document Type
Article
Publication Date
2015
Department
Physics and Astronomy
Keywords
lunar-regolith, regolith-breccia, magnetite, lunar-volatiles, lunar-oxidation
Abstract
Lunar regolith breccias are temporal archives of magmatic and impact bombardment processes on the Moon. Apollo 16 sample 60016 is an ‘ancient’ feldspathic regolith breccia that was converted from a soil to a rock at ~3.8 Ga. The breccia contains a small (70 × 50 μm) rock fragment composed dominantly of an Fe-oxide phase with disseminated domains of troilite. Fragments of plagioclase (An95-97), pyroxene (En74-75, Fs21-22,Wo3-4) and olivine (Fo66-67) are distributed in and adjacent to the Fe-oxide. The silicate minerals have lunar compositions that are similar to anorthosites. Mineral chemistry, synchrotron X-ray Absorption Near Edge Spectroscopy (XANES) and X-ray Diffraction (XRD) studies demonstrate that the oxide phase is magnetite with an estimated Fe3+/ΣFe ratio of ~0.45. The presence of magnetite in 60016 indicates that oxygen fugacity during formation was equilibrated at, or above, the Fe-magnetite or wűstite-magnetite oxygen buffer. This discovery provides direct evidence for oxidised conditions on the Moon. Thermodynamic modelling shows that magnetite could have been formed from oxidisation-driven mineral replacement of Fe-metal or desulphurisation from Fe-sulphides (troilite) at low temperatures (°C) in equilibrium with H2O steam/liquid or CO2 gas. Oxidising conditions may have arisen from vapour transport during degassing of a magmatic source region, or from a hybrid endogenic-exogenic process when gases were released during an impacting asteroid or comet impact.
Source Publication Title
Meteoritics and Planetary Science
Publisher
Wiley
Volume
50
Issue
7
First Page
1157
DOI
10.1111/maps.12462
Recommended Citation
Joy, K. H., Visscher, C., Zolensky, M. E., Mikouchi, T., Hagiya, K., Ohsumi, K., & Kring, D. A. (2015). Identification of Magnetite in Lunar Regolith Breccia 60016: Evidence for Oxidized Conditions at the Lunar Surface. Meteoritics and Planetary Science, 50 (7), 1157. https://doi.org/10.1111/maps.12462
Comments
This is a pre-publication author manuscript of the final, published article. The definitive version is published by Wiley and available from Wiley Online Library (wileyonlinelibrary.com). DOI 10.1111/maps.12462