By Brooks Hays
Apr 9, 2015
Previous satellite images have suggested the presence of hefty glacial bands spanning the planet's northern and southern hemispheres just beneath the Martian surface. But until now, researchers had not been able to confirm the glacial chemical makeup.
But new radar observations, detailed in the latest issue of Nature, offer some clarity. By studying the movement of the frozen formations over time and comparing the glaciers' behavior with hydraulic models, scientists were able to confirm the presence of H2O.
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