Scientists are particularly interested in the Martian dunes because they represent areas where the surface changes enough that the same material does not get a taste of the harsh environment.
Martian forts move at a fraction of the speed of those found on Earth. This gives an idea of how thinner the feeling is in the Red Planet than on Earth.
Recently, NASA shared a unique image of Mars’ frozen docks. In the high altitudes of Mars ’northern flat plains, the sand dunes inhabit this 5-kilometer frozen crater.
Some docks are detached from the main area and appear to ascend the crater slope and form a gully-like shape.
A series of darkly colored polygonal patterns reveal the surface of the main area of the docks. These patterns can be the result of seasonal freezing processes.
Many of the steepest, steepest, sloping slopes suggest the onset of gill formation.
Several textures can be seen on the crater floor. These textures incorporate lobate and striped patterns indicating seasonal melting due to sublimating ice.
The wide downstream movement of materials on the crater slope is similar to the movement of the tiffany, except that they are not usually defined by special alcoves, cut channels, or sediment aprons. These are signs of gulli elsewhere on the planet.