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• W2031704455 abstract "Martian intracrater splotches and related streaks are studied with global data on their occurrence and regional data on color and morphology. The fraction of craters with splotches is greatest at high latitudes. Splotch occurrence is not strongly correlated with surface properties such as albedo and thermal inertia except where these correlate with substantial sediment cover. Large numbers of splotches are or include dunes, especially at high southern latitudes. Color data show that the dune and nondune materials in splotches are part of one related group of materials that may be of similar composition but varying particle sizes. The color data also show that some streaks are simply material deflated from splotches and mixed with local plains material while other streaks are more complex and may involve erosion of thin surface layers by material blown from the splotches. Splotches appear to be trapped eolian sand but probably have been formed by a great variety of mechanisms. A large percentage of craters with splotches show evidence of complex histories of sediment deposition and erosion. Many splotches may be lag deposits from erosion of regional sediment cover. Present sediment budgets in splotches are not known, but there is some evidence for loss of material and no evidence for resupply from outside the craters." @default.
• W2031704455 created "2016-06-24" @default.
• W2031704455 creator A5011232501 @default.
• W2031704455 date "1984-02-01" @default.
• W2031704455 modified "2023-10-18" @default.
• W2031704455 title "Martian intracrater splotches: Occurrence, morphology, and colors" @default.
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• W2031704455 doi "https://doi.org/10.1016/0019-1035(84)90066-6" @default.
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