Every Martian spring, fans of dust are blown out from under the seasonal layer of carbon dioxide ice that forms a polar cap over the winter.
Gas blowing out from under the ice carries with it a load of dust that is deposited on the surface in a direction determined by the wind at the time of the eruption. Like windsocks,
these fans in a polar area we’ve dubbed Macclesfield, record the direction that the wind was blowing.
A citizen science task at
Planet Four enlists the public to outline the fans. Their measurements go into a data base that will ultimately help us to understand weather on Mars.
ID:
ESP_064469_0945date: 27 April 2020
altitude: 245 km
https://uahirise.org/hipod/ESP_064469_0945
NASA/JPL-Caltech/University of Arizona
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