A team of scientists from the University of Rochester discovered that the surface of Mars features soil patterns similar to Earth's coldest regions, known as solifluction lobes.
These wave-like formations on Mars closely resemble Earth's solifluction lobes in shape and geometric pattern, suggesting a deeper link between the two planets in terms of landscape formation.
The Martian solifluction lobes, on average 2.6 times taller than Earth's, were likely formed by freeze-sublimate cycles due to scarce surface water and colder temperatures on Mars.
This discovery provides insights into Mars' ancient climate and the potential presence of ice or past water, offering valuable information for future missions and understanding planetary environments.