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- W267548847 abstract "Introduction: The Sinus Sabaeus Quadrangle (0°S to 30°S and 0°E to 45°E) was selected as a representative highly cratered region to characterize the morphometry of 530 fresh and degraded craters greater that 10 km in diameter. Individual MOLA tracks were utilized rather than gridded data to avoid artifacts due to sparse data. An additional 320 craters were included in crater counts but were not morphometrically analyzed because of 1) poor MOLA coverage; 2) strong modification by later impacts, or 3) breaching of the crater wall by entering or exiting fluvial channels (not a closed depositional system). Each crater was visually assigned a degree of degradation using the standard classification system [1,2,3], ranging from ‘A’ for fresh to ‘E’ for highly degraded craters. Qualitative characteristics were used in conjunction with the quantitative morphometric measurements to examine the properties of crater modification within the quadrangle as a function of crater diameter, location within the quadrangle and elevation. A variety of measurements and analyses were conducted [4], but we report here results related to determining the processes responsible for degradation. Relative Crater Depth: One measure of the degree of crater degradation is the relative crater depth, R, which we define as: ( ) R H h H = − ," @default.
- W267548847 created "2016-06-24" @default.
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- W267548847 date "2004-01-01" @default.
- W267548847 modified "2023-09-27" @default.
- W267548847 title "CRATER DEGRADATION IN THE MARTIAN HIGHLANDS: MORPHOMETRIC ANALYSIS OF THE SINUS SABAEUS REGION AND SIMULATION MODELING SUGGEST FLUVIAL PROCESSES. N. Forsberg-Taylor" @default.
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