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High Sun views such as this often show fascinating dark and bright
patterns that would be overwhelmed by highlights or shadows if the Sun
were lower in the sky. This view of the 17-km-wide crater Jansen B shows
numerous bright avalanche deposits on the steep crater walls, apparently
originating at outcrop ledges near the top of the wall. Most avalanches
stop in a moat at the base of the wall, but a few in the foreground extend
out onto the irregular, inward- sloping floor. The floor is a jumble of
slump blocks. Avalanching appears to be a major means of erosion on steep
lunar slopes. -K.A.H.
This web page was created by Francis Ridge
for The Lunascan Project
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