Lunar Rock Compositions and Some Interpretations
- 30 January 1970
- journal article
- research article
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 167 (3918) , 527-528
- https://doi.org/10.1126/science.167.3918.527
Abstract
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 elements and the initial compositions of the earth and moon.Keywords
This publication has 3 references indexed in Scilit:
- Preliminary Examination of Lunar Samples from Apollo 11Science, 1969
- Meteoritic, solar and terrestrial rare-earth distributionsPhysics and Chemistry of the Earth, 1966
- Chemical Characteristics of Oceanic Basalts and the Upper MantleGSA Bulletin, 1965