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Active Mars: A dynamic world

Colin M. Dundas·Patricio Becerra·Shane Byrne·Matthew Chojnacki·Ingrid J. Daubar·Serina Diniega·Candice J. Hansen·Kenneth E. Herkenhoff·Margaret E. Landis·Alfred S. McEwen·Ganna Portyankina·Adomas Valantinas
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Abstract

Mars exhibits diverse surface changes at all latitudes and all seasons. Active processes include impact cratering, aeolian sand and dust transport, a variety of slope processes, changes in polar ices, and diverse effects of seasonal CO 2 frost. The extent of surface change has been surprising and indicates that the present climate is capable of reshaping the surface. Activity has important implications for the Amazonian history of Mars: understanding processes is a necessary step before we can understand their implications and variations over time.

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Journal of Geophysical Research: PlanetsArticle

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Colin M. Dundas, Patricio Becerra, Shane Byrne, Matthew Chojnacki, Ingrid J. Daubar, Serina Diniega, Candice J. Hansen, Kenneth E. Herkenhoff, Margaret E. Landis, Alfred S. McEwen, Ganna Portyankina, Adomas Valantinas. 2021-07-29. Active Mars: A dynamic world. https://doi.org/10.1029/2021je006876

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