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- W1639429766 abstract "The global cratering records are examined on the basis of planetary images to establish for each planet the global succession of stratigraphic units and the variations in crater densities among these global provinces. Crater density on a global scale on each of the planets is mapped to establish the range of variation of crater density of post-highland plains for Mercury, moon, and Mars. A narrow diameter-range (5-10 km) was chosen for this purpose. Crater abundance in this size range has been continuously mapped for available coverage for each of the three planets. Craters in this size range superposed on the plains usually display pristine morphology suggesting that most were formed after the plains. Evidently, most preexisting craters in this size range were erased by the plains-forming processes." @default.
- W1639429766 created "2016-06-24" @default.
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- W1639429766 date "1977-01-01" @default.
- W1639429766 modified "2023-09-27" @default.
- W1639429766 title "Historical variations in the density and distribution of impacting debris in the inner solar system - Evidence from planetary imaging" @default.
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