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- W2212167065 abstract "High-resolution images of Martian surfaces captured by the MGS/MOC provide the first opportunities to study simple craters ranging down to 15m in diameter. Variations in the morphology of such small craters across different terrain and landform types provide insights into the nature of the target material as well as the geological processes acting on the surface since the craters formed. Our study focuses on simple craters less than one kilometer in diameter observed within 13 discrete regions of Mars. These regions represent a range of different landforms including volcanic flanks and calderas, i outwash plains, fossae, and northern plains. Crater depths were determined from shadow length measurements using an approach that does not depend on the shadow crossing through the center of the crater. To minimize the effects of illumination conditions, only images with solar incidence angles greater than 70 degrees were used. In each region we measured the depths (d) and diameters (D) of at least 15 craters for a total sample size of 687 craters." @default.
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- W2212167065 date "2001-01-01" @default.
- W2212167065 modified "2023-09-27" @default.
- W2212167065 title "Properties of Martian Surfaces from the Morphology of Small Impact Craters - Abstract" @default.
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