首页> 中文期刊> 《地球化学》 >阿波罗-17(70017-291)高钛月海玄武岩的化学组成及其成因的探讨

阿波罗-17(70017-291)高钛月海玄武岩的化学组成及其成因的探讨

         

摘要

Chemical, petrological and mineralogical studies on 70017-291 Mare basalt indicate that the mare basalt belongs to Type B of A-17 basalts with a texture of plagioclasepoikilitic ilmenite basalt. The mean chemical composition of this basalt is as follows:SiO2 39.01, TiO2 11.32, Al2O3 9.24, FeO 18.52, MgO 8.61, CaO 10.86 (%). INAA measurements were made on the basalt for major, minor and trace elements. Seven pyroxene grains in the Apollo 17 were also analyzed by microprobe. They show two compositions, one for pigeonite, and the other for augite-subcalicaugite. The mean composition of pigeonite is Wo10.85, En59.33 Fs30, and that of augite-subcalic augite Wo25 En41.5Fs38.3. Plagioclase grains have a composition ranging from An30 to An96. The plagioclase contains detectable iron (averaging 0.74%), potassium (0.089% in average) and titanium(averaging 0.16%). The mean composition of ihnenite is TiO2 53.98%, FeO 41.02%,Al2O3 0.21%, MgO 2.41%, Cr2O3 0.74%. The Ti-high mare basalt (70017-291) was formed by partial melting of the early cumulates through assimilation and migmatization. On the whole, mare basalts seem to be of multigenesis.

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