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
2 pages
Report
No indication
English
Astrogeology , Craters , Highlands , Mars surface , Topography , Degradation , Erosion , Terrain
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