Titlebook: Chronology and Evolution of Mars; Proceedings of an IS Reinald Kallenbach,Johannes Geiss,William K. Hartm Conference proceedings 2001 Sprin

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Geophysical Constraints on the Evolution of Marsickness can be shown to be in agreement with estimates of volcanic production rates from geologic mapping using data from the camera on MGS and previous missions. According to these estimates most of the crust was produced in the Noachian, roughly the first Gyr of evolution. A substantial part of th

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Conference proceedings 2001on. The fur- ther growth of the Earth was sustained by major collisions with planetesimals and planets such as that which resulted in the formation ofthe Earth‘s moon (Hartmann and Davis, 1975; Cameron and Ward, 1976; Wetherill, 1986; Cameron and Benz, 1991). This late accretionary history, which la

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Steuerbarkeit und Beobachtbarkeitir effects on the surface must be taken into account in using impact crater statistics to derive chronologies on Mars. In addition, mapping the locations, relative ages, and orientations of aeolian features can provide insight into Martian weather, climate, and climate history.