摘要: Evaporation and condensation played a major role in producing chemical and/or isotopic variations the early solar system, which have been recorded primitive meteorites. Experimental studies on evaporation of various planetary materials started 1970's to reproduce compositions textures constituents In recent decade, many experiments minerals melts carried out obtain fundamental kinetic parameters comprehend (or isotopic) fractionations system terms evolution. simulation should be combined with or analyses meteorites observational theoretical proto-planetary disk for complete understanding The history experimental under conditions some progresses are reviewed this paper.
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