Article 5VY3X Widespread Megaripple Activity Detected Across the North Polar Region of Mars

Widespread Megaripple Activity Detected Across the North Polar Region of Mars

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Widespread Megaripple Activity Detected Across the North Polar Region of Mars:

Megaripples, intermediate-scale bedforms caused by the action of the wind, have been studied extensively and thought to be largely inactive relics of past climates, save for a few exceptions. A new paper by Planetary Science Institute Research Scientist Matthew Chojnacki shows that abundant megaripple populations were identified across the north polar region of Mars and were found to be migrating with dunes and ripples.

Megaripples on Mars are about 1 to 2 meters tall and have 5 to 40 meter spacing, where there size falls between ripples that are about 40 centimeters tall with 1 to 5 meter spacing and dunes that can reach hundreds of meters in height with spacing of 100 to 300 meters. Whereas the megaripples migration rates are slow in comparison (average of 0.13 meters per Earth year), some of the nearby ripples were found to migrate an average equivalent of 9.6 meters per year over just 22 days in northern summer - unprecedented rates for Mars. These high rates of sand movement help explain the megaripple activity.

"Using repeat HiRISE images acquired over long durations - six Mars years or 13 Earth years - we examined the dynamic activity of polar bedforms. We found the thin Martian atmosphere can mobilize some coarse-grained megaripples, overturning prior notions that these were static relic landforms from a past climate. We mapped megaripples and adjacent bedforms across the north polar sand seas, the most expansive collection of dune fields on Mars," said Chojnacki, lead author of "Widespread Megaripple Activity Across the North Polar Ergs of Mars" that appears in Journal of Geophysical Research: Planets.

Journal Reference:
Matthew Chojnacki, David A. Vaz, Simone Silvestro, et al. Widespread Megaripple Activity Across the North Polar Ergs of Mars, Journal of Geophysical Research: Planets (DOI: 10.1029/2021JE006970)

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