The amount of obliteration suffered by Martian impact craters is quantified by comparing measurable attributes of the current crater shape to those values expected for a fresh crater of identical size. Crater diameters are measured from profiles obtained using photoclinometry across the structure. The relationship between the diameter of a fresh crater and a crater depth, floor width, rim height, central peak height, etc. was determined by empirical studies performed on fresh Martian impact craters. We utilized the changes in crater depth and rim height to judge the degree of obliteration suffered by Martian impact craters.
Degradation studies of Martian impact craters
1991-01-01
Conference paper
No indication
English
Impact Craters on Martian Volcanoes
British Library Conference Proceedings | 1994
|Impact Craters on Martian Volcanoes
British Library Conference Proceedings | 1994
|NTIS | 1971
|Martian craters - Number density.
NTRS | 1968
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