Lithological variation with depth and decoupling of maturity parameters in Apollo 16 regolith core 68001/2
نویسندگان
چکیده
منابع مشابه
Modeling the provenance of the Apollo 16 regolith
[1] The regolith at the Apollo 16 landing site, the only Apollo landing site in the central lunar highlands, contains material derived from a number of sources. A model that accounts for the introduction of basin ejecta and mixing of the megaregolith is used to estimate the abundance of basin material in the Apollo 16 regolith. Megaregolith mixing model estimates of the abundance of primary eje...
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Doses of heavy particles at positions inside the command modules of Apollo missions 8, 12, 14, and 16 correlate well with the calculated effects of solar modulation of the primary cosmic radiation. Differences in doses at different stowage positions indicate that the redistribution of mass within the spacecraft could enhance safety from the biological damage that would otherwise be expected on ...
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Native Silicon and Fe-silicides from the Apollo 16 Lunar Regolith: Extreme Reduction, Metal-silicate Immiscibility, and Shock Melting
Silicon in metallic form – dissolved in Fe-Ni metal, as silicide, or as Si 0 – is rare in solar system materials because its formation requires extremely reducing temperatures or oxidation states or both. Fe-Ni metal in carbonaceous chondrites can contain small proportions of Si [1], as does metal in shocked enstatite chondrites and aubrites [2]. Iron silicides are known from ureilite meteorite...
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ژورنال
عنوان ژورنال: Geochimica et Cosmochimica Acta
سال: 1997
ISSN: 0016-7037
DOI: 10.1016/s0016-7037(97)00140-3