Geochemical constraints on the origin of the Moon
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Cited by (15)
Lunar core formation: New constraints from metal-silicate partitioning of siderophile elements
2014, Earth and Planetary Science LettersCitation Excerpt :Fig. 1 shows the resulting estimated levels of siderophile element depletion in the lunar mantle due to core formation, based on values from (Walter et al., 2000; Delano, 1986; Righter and Drake, 1996; Newsom and Taylor, 1989; Drake, 1987; Jones and Palme, 2000). In general, the lunar mantle is depleted in siderophile elements relative to the Earthʼs mantle (Drake, 1983; Newsom 1984, 1986). The lunar mantle depletion in the weakly siderophile elements V and Cr is considered to be very similar to the terrestrial mantle depletions of these elements (Dreibus and Wänke, 1979).
Comparative geochemistry of basalts from the moon, earth, HED asteroid, and mars: Implications for the origin of the moon
2001, Geochimica et Cosmochimica ActaRubidium and cesium in the Earth and the Moon
1993, Geochimica et Cosmochimica ActaV, Cr, and Mn in the Earth, Moon, EPB, and SPB and the origin of the Moon: Experimental studies
1989, Geochimica et Cosmochimica ActaExperimental determination of crystal/melt partitioning of Ga and Ge in the system forsterite-anorthite-diopside
1987, Geochimica et Cosmochimica ActaThe unique lunar composition and its bearing on the origin of the Moon
1987, Geochimica et Cosmochimica Acta
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