The results of a point-by-point examination of the Goldstone topography data in the Martian highlands suggest that, at the 100 m range resolution, the rims of large craters are barely distinguishable against the surrounding terrain. Craters are described topographically.
Topography of large craters on Mars: Implications for the highlands resurfacing history
1987-01-01
Conference paper
No indication
English
Resurfacing History of the Venusian Plains Based on Distribution of Impact Craters
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