Wind has long been known to be a factor in the Red Planet's topography and climate, creating dust storms that can be visible to astronomers on Earth.
But data about the strength, frequency and origin of winds has been sketchy, and many specialists had expected that gusts strong enough to move sand would be rare on a planet with such a thin atmosphere.
"We observed that martian sand dunes are currently migrating and that their migration speed varies with the season, which is at odds with the common view of a static martian landscape and very rare sand-moving winds," study co-author Francois Ayoub of the California Institute of Technology's planetary sciences division told AFP.
"From these measurements, we estimated the sand flux and its seasonal variability," said Ayoub. Next, they calculated the wind speed and strength required to move the sand, and the frequency.
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"Winds on Mars can be strong and can reach hurricane speed (more than 120 kilometres per hour or 75 miles per hour)," Ayoub said.
"In our study area, sand-moving wind occurs almost daily" throughout much of the year, he added.
And the data may aid future rover missions from Earth.
"An accurate prediction of the wind and sand load is important to avoid the rover to be 'sandblasted' without being prepared for it," explained Ayoub.
"The (NASA) rover Curiosity, which is about to cross an active dune field in Gale crater will most probably have to sustain sand blows. From a scientific point of view, these findings could indicate areas on Mars deserving more attention from observation orbiters for their peculiar wind/sand/erosion behaviours."
The study was published in the journal Nature Communications.