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The shifting sands of Mars; Words count for counting; A flea’s mighty genome; The disappearing wild oyster

The shifting sands of Mars

Mars has weather. A new analysis of NASA photos has revealed that the dramatic sand dunes around the Martian North Pole, long considered static remnants of the Red Planet’s stormy past, change shape from season to season as a result of surprisingly dynamic forces of nature. Researchers at the University of Arizona examined hundreds of high-quality photos of the dark basalt undulations, some of them 100 feet tall, taken by the Mars Reconnaissance Orbiter over the course of two Martian years, the equivalent of four years on Earth. The images revealed that the Texas-sized dune zone is one of the planet’s most active regions. The researchers discovered that in the Martian winter, the sand is coated with a blanket of dry ice, which turns into a gas in the spring, destabilizing the dunes and triggering avalanches. The new images also provide evidence that winds in Mars’ thin atmosphere, previously thought to be too weak to lift even a grain of basalt, actually blow hard enough to fill ravines and gullies with sand in just a single Martian year. Understanding the dunes’ seasonal shifts will be “a key first step” toward understanding “how Mars changed over time,” study co-author Alfred McEwen tells ScienceDaily.com. “The level of erosion in just one Mars year was really astonishing,” says co-author Candice Hansen. “This is a very un-Earthly process.”

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