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- W2002602852 abstract "Martian craters in the size range 10–250 km follow a log normal size-frequency distribution law. Analysis techniques based on the log normal model yield possible evidence for the size-frequency evolution of crater-producing bodies. Some regions on Mars display excessive depletions of either large or small craters; the most likely causes of the depletions are considered. Apparently, eolian sedimentation has markedly altered the population of small craters south of −30° latitude. The general effects of crater obliteration in the southern hemisphere appear to be confined to diameters of less than 20 km. A strong depletion of large craters in a large region centered at 35° latitude and 10° west longitude may indicate locations of subsurface ice." @default.
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- W2002602852 date "1977-12-10" @default.
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- W2002602852 title "A size-frequency study of large Martian craters" @default.
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- W2002602852 doi "https://doi.org/10.1029/jb082i036p05807" @default.
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