AS15-9721(P)

Figure 108

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 Click here for lunar chart showing location

(F. Ridge: The location of this crater was not given in SP-362, p.116, but the lunar chart on p. 104 linked above shows Figure 108 to be on the lunar far side). Another fine example of a small crater with extensive bright rays. It presumably was formed by meteoroid impact. Both light and dark rocks are visible in the walls, indicating that more than one layer of rock was penetrated. Rays formed by secondary craters, blocks, and pulverized ejecta extend more than 13 crater diameters beyond the crater proper. The marked irregularity of the pattern southeast of the crater probably was caused by topographic irregularities that deflected the radially outward movement of the ejecta. Arrows indicate smaller bright- rayed craters.   -M.W.
 
 

Report Source: NASA SP-362, Page 116, Figure 108

This web page was created by Francis Ridge for The Lunascan Project
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