Active Mars: A Dynamic World Article Swipe
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C. M. Dundas
,
P. Becerra
,
Shane Byrne
,
M. Chojnacki
,
I. J. Daubar
,
S. Diniega
,
C. J. Hansen
,
K. E. Herkenhoff
,
M. E. Landis
,
A. S. McEwen
,
Ganna Portyankina
,
Adomas Valantinas
·
YOU?
·
· 2021
· Open Access
·
· DOI: https://doi.org/10.1029/2021je006876
· OA: W3178258103
YOU?
·
· 2021
· Open Access
·
· DOI: https://doi.org/10.1029/2021je006876
· OA: W3178258103
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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