玄武岩
风化土
天体生物学
陨石
月球地质
地质学
火成岩
月母马
地球化学
辉长岩
矿物学
物理
作者
A. E. J. Engel,Celeste G. Engel
出处
期刊:Science
[American Association for the Advancement of Science]
日期:1970-01-30
卷期号:167 (3918): 527-528
被引量:32
标识
DOI:10.1126/science.167.3918.527
摘要
Samples of igneous "gabbro," "basalt," and lunar regolith have compositions fundamentally different from all meteorites and terrestrial basalts. The lunar rocks are anhydrous and without ferric iron. Amounts of titanium as high as 7 weight percent suggest either extreme fractionation of lunar rocks or an unexpected solar abundance of titanium. The differences in compositions of the known, more "primitive" rocks in the planetary system indicate the complexities inherent in defining the solar abundances of elemizents and the initial compositions of the earth and moon.
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