Volatility inversion of silicon and magnesium oxides during the evaporation of HASP glasses on the moon

Abstract

An inversion of SiO₂ and MgO volatility occurs during high-temperature melt evaporation in the CaO–MgO–Al₂O₃–SiO₂ (CMAS) system. This results in that SiO₂, which is usually more volatile than MgO, becomes less volatile during the evaporation of melts enriched in the refractory oxides CaO and Al₂O₃. The volatility inversion is adequately explained within the theory of acid–base interaction of silicate melt components developed by D.S. Korzhinskii. The compositions of high-Al₂O₃ and SiO₂-poor glasses (known as HASP glasses) from the lunar regolith show a systematic decrease in MgO/SiO₂ with increasing CaO content, which is a direct consequence of the influence of acid–base effects.