Anyone who has spent time at a swimming pool has seen something like this image. It looks like shadows on the bottom of a pool from ripples on the surface. But wind, instead of water, is involved in making this dizzying pattern of dunes on Mars.
Explore the image from NASA’s HiRISE camera aboard the Mars Reconnaissance Orbiter of sand dunes in Olympia Undae on Mars. Olympia Undae forms a vast sea of sand surrounding the Martian north pole. Zoom in closer and tiny ripples and grooves appear. These features are formed by wind blowing from a constant direction as well as the larger dunes.
We find patterns of sand dunes like this on Earth but what excites scientists more is what makes up the dunes. Gypsum is a light-colored, chalky, whitish mineral. Gypsum forms in the presence of liquid water and these dunes are full of the mineral. Scientists are working to track down the source of the mineral and when in Mars’ wetter past it formed.
By The Riviera Times
By CritterKeeper
By Sarah Q. Brett