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This oblique view of the crater Isidorus D was taken with the panoramic
camera on Apollo 16. Isidorus D is about 15 km in diameter and is located
in the highlands between Mare Tranquillitatis and Mare Nectaris. Evidence
of avalanching (Howard, 1973) and of other types of downslope movement
of material are clearly visible on the inner walls of the crater. The streaks
resembling shooting stars on the left wall appear to be avalanche scars.
The avalanches probably were spearheaded by large blocks followed by fine-grained
material. On the near wall (arrow) a larger landslide terminates in a straight
line against the relatively flat crater floor. In the shadowed part of
the crater wall many short irregular benches or narrow terraces mark the
tops of masses of slumped material. The brightness of the avalanche scars
is an indication of their freshness; in general, freshly exposed lunar
materials are brighter than undisturbed materials nearby. -
F.E.-B.
Report Source: NASA SP-362, Page 125, Figure 119
This web page was created by Francis Ridge
for The Lunascan Project
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