The size distribution of the lunar fines is measured, and small but significant differences are found between the Apollo 11 and 12 samples as well as among the Apollo 12 core samples. The observed differences in grain size distribtuion in the core samples are related to surface transportation processes, and the importance of a sedimentation process versus meteoritic impact gardening of the mare grounds is discussed. The optical and the radio frequency electrical properties are measured and are also found to differ only slightly from Apollo 11 results.
Some physical properties of Apollo 12 lunar samples
1971-04-01
Miscellaneous
No indication
English
Some physical properties of Apollo 12 lunar samples
NTRS | 1971
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NTRS | 1972
|Magnetic properties of Apollo 11 lunar samples
NTRS | 1970
|Organics in APOLLO Lunar Samples
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|Luminescence of Apollo 11 and Apollo 12 lunar samples
NTRS | 1971
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