The lunar regolith: Chemistry and petrology of Luna 24 grain size fractions
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Cited by (13)
Polarimetry of moonlight: A new method for determining the refractive index of the lunar regolith
2016, IcarusCitation Excerpt :Studies of lunar soil have shown that the composition of the regolith changes with grain size. An important finding is that, when compared to coarser grains, the smallest fraction of grains within mare soils are consistently richer in plagioclase, and are depleted in elements (e.g. Fe, Mg) associated with ferromagnesian minerals (Evenson et al., 1974; Korotev, 1976; Laul et al., 1987; Papike et al., 1981; Taylor et al., 2003). A hypothesis that may account for this is that a greater proportion of plagioclase from disaggregated mare basalt is concentrated in the finer grain size fraction (Korotev, 1976; Papike et al., 1982; Laul et al., 1987).
Precise determination of the isotopic composition of potassium: Application to terrestrial rocks and lunar soils
1995, Geochimica et Cosmochimica ActaReply to "Geochemistry of grain-size fractions of Luna 24 soil" by R. L. Korotev
1989, Geochimica et Cosmochimica ActaManufacture of glass and mirrors from lunar regolith simulant
2019, Journal of Materials Science
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