Formation of V-shaped structures surrounding the fresh Copernicus Crater and its secondary craters are reviewed, and preliminary observations of the more extensively eroded secondary crater field of Theophilus are presented. Results of laboratory simulation of secondary lunar craters to examine their effects on V-shaped ridges are also described.
Lunar secondary craters, part K
1972-01-01
Miscellaneous
No indication
English
NTRS | 1970
|Large lunar secondary craters - Size-range relationships
NTRS | 1979
|NTRS | 1964
|NTIS | 1964
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