A general study is presented on the surface geometry of 25 far-side craters along with a detailed study of rim-crest evenness for 15 near-side and far-side craters. Analysis of this preliminary sample of Apollo 15 and 17 data, which includes craters between 1.5 and 275 km in diameter, suggests that most genetic interpretations of craters made from pre-Apollo topographic measurements may require no drastic revision. All measurements were made from topographic profiles generated on a stereoplotter.
Lunar crater morphometry
1973-01-01
Miscellaneous
No indication
English
NTRS | 1972
|Internal Crater Modification on Venus: Implications of Interior Crater Morphometry
British Library Conference Proceedings | 1996
|Crater Morphometry on Venus: Relative Floor Size and Internal Crater Modification
British Library Conference Proceedings | 1995
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