Martian Xenon Components in Basaltic Shergottite Meteorites
作者： Katherine Delene Ocker Stone
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摘要: Analyses of Chassigny, Nakhla, and ALH84001 reveal, in addition to a Xe component from the martian atmosphere, second loosely attributed "interior." This appears be mixture solarand fission(Pu) derived xenon components. The proportions are consistent each meteorite but vary meteorite. working hypothesis is that this variation reflects different contributions solar (mantle-derived) fission (crustal-derived) parent
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