Luna 24 - Lateral heterogeneity in the lunar crustResults of petrological investigations of Luna 24 soil samples are compared with data from Apollo and other Luna missions in order to determine the large scale composition of the lunar surface and crust. Modal analysis of the 90 to 150 micron soil fraction and electron microprobe analysis of glass spheres and fragments of the Luna 24 core sample are presented. High and low MgO mare basalt compositional clusters are found, suggesting the derivation of southern Mare Crisium basalts from two magmas. A model of Luna 24 soils as being composed of a mixture of glass-poor mare material and glass-rich highland material is found to be consistent with glass and agglutinate modal abundances. Comparisons show that potassium, and by inference all lithophile trace elements, are depleted on the eastern limb of the moon relative to the central nearside. The observed depletion is interpreted to be characteristic of the underlying crust and mantle as well as the surface.
Document ID
19790048507
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Warner, J. L. (NASA Johnson Space Center Houston, Tex., United States)
Simonds, C. H. (Northrop Services, Inc. Houston, Tex., United States)
Mcgee, P. E. (Northrop Services, Inc. Houston, TX, United States)
Cochran, A. (Lockheed Electronics Co., Inc. Houston, Tex., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1978
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Mare Crisium: The view from Luna 24; Conference