The Planetary Geomorphology Image of the Month features work by PSI Research Scientist Matthew Chojnacki on megaripples on the surface 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 paper by Chojnacki, “Widespread Megaripple Activity Across the North Polar Ergs of Mars” that appears in Journal of Geophysical Research: Planets, 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.
Part of the uncertainty when studying planetary polar landforms is the long, cold polar winter that eventually covers the region in carbon dioxide and water ice. For wind-driven bedforms, such as megaripples, that means they are unable to migrate for nearly half of the year. “However, it appears the late spring and summer winds that descend off the polar cap more than make up for these other periods of inactivity,” Chojnacki said.
“Megaripples were found to be widespread across the region and migrating at relatively high rates relative to other sites on Mars that are at lower latitudes. This enhanced activity is likely related to the greater sand fluxes found for neighboring dunes which are driven by summer-time seasonal winds when polar ice is sublimating. This supports the idea that much of the Martian surface is actively being modified and not just ancient or static,” Chojnacki said. “In contrast, other megaripples appear to be stabilized, a likely result of inter-granular ice within low wind areas.”
The project was funded by NASA Mars Data Analysis program grant 80NSSC20K1066.
HiRISE perspective view of north polar dune fields with active megaripples (arrows). Megaripple activity is most evident on the upwind edges of dune fields and in some cases within inter-erg areas. Clusters of contiguous megaripple fields often flanked by ripples and dunes were most common, while occasionally occurrences of mobile megaripple trains atop of bedrock were observed. All images and associated digital terrain models can be accessed at: https://hirise.lpl.arizona.edu/
Credit: NASA/JPL/University of Arizona.
