July 31, 2009

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27 & 28

LPOD-July31-09.jpg

images by Damian Peach

Crater morphology depends strongly on crater diameter. Craters smaller than about 15 km have simple bowl shapes, and ones larger than about 30 km have terraces, central peaks and broad flat floors. In between is a transition zone with rim scallops marking where individual wall masses collapsed onto the floor, often surrounding small hills in the crater center. Back in the early 1970's Chuck Wood

Technical Details
Euler: May 28th, 2007. C14 with SKYnyx 2.0M, Barbados, W.I.
Grove: May 23rd, 2007. C14 with SKYnyx 2.0M, Barbados, W.I.

Related Links
Rükl plate 14 & 20
Damian's new gallery of lunar images.

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