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A Survey of Lunar Rock Types and Comparison of the Crusts of Earth and MoonThe principal known types of lunar rocks are briefly reviewed, and their chemical relationships discussed. In the suite of low-KREEP highland rocks, Fe/(Fe + Mg) in the normative mafic minerals increases and the albite content of normative plagioclase decreases as the total amount of normative plagioclase increases, the opposite of the trend predicted by the Bowen reaction principle. Lunar highland samples analyzed are uniformly distributed in this sequence, in which normative plagioclase contents range from ~ 40 percent to ~ 100 percent. The distribution of compositions of rocks from terrestrial layered mafic intrusives is substantially different: here the analyses fall in several discrete clusters (anorthositic rocks, norites, granophyres and ferrogabbros, ultramafics), and the chemical trends noted above are not reproduced. It is suggested that the observed trends in lunar highland rocks could be produced by crystal fractionation in a deep global surface magma system if (1) plagioclase tended to float, upon crystallization, and (2) the magma was kept agitated and well mixed (probably by thermal convection) until crystallization was far advanced and relatively little residual liquid was left. When such a system was finally immobilized, the Fe-, Na-rich residual liquid would produce Fe-rich mafic minerals in the upper levels of the system, but could not much alter the composition of abundant calcic plagioclase. Conversely, the same liquid would produce sodic plagioclase deep in the sequence, but could not much alter the composition of abundant magnesian mafic minerals. After the crustal system solidified, but before extensive cooling had developed a thick, strong lithosphere, mantle convection was able to draw portions of the lunar anorthositic crust down into the mantle in a manner analogous to the present-day behavior of the terrestrial mantle and crust. At depth, the crustal material was heated; KREEP-rich norite was extracted by partial melting and erupted at the surface as a lava, analogous to terrestrial andesite eruptions.
Document ID
19780004984
Acquisition Source
Headquarters
Document Type
Conference Paper
Authors
John A Wood
(Center for Astrophysics Harvard & Smithsonian Cambridge, United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1977
Publication Information
Publication: The Soviet-American Conference on Cosmochemistry of the Moon and Planets
Publisher: National Aeronautics and Space Administration
Volume: Part 1
Subject Category
Lunar and Planetary Science and Exploration
Report/Patent Number
NASA-SP-370-PT-1
Meeting Information
Meeting: Soviet-American Conference on the Cosmochemistry of the Moon and Planets
Location: Moscow
Country: RU
Start Date: June 4, 1974
End Date: June 8, 1974
Sponsors: Union of Soviet Socialist Republics, National Aeronautics and Space Administration
Accession Number
78N12927
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
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