Researchers have found that Mars's northern polar ice cap is quite young, providing insights into the planet's interior.
The team used techniques to measure glacial isostatic adjustment, revealing ongoing deformation in response to the weight of the ice.
The Martian ice cap measures approximately 1000 kilometers in diameter and up to three kilometers thick, causing depression in the underlying rocky crust.
By studying glacial isostatic rebound on Mars, researchers concluded that the planet's north polar cap is relatively young and deforms the ground beneath it.
The small deformation rates suggest that Mars's upper mantle is cold, highly viscous, and stiffer compared to Earth's upper mantle.
Understanding how ice affects planetary surfaces helps scientists probe deep beneath the surfaces of rocky planets like Mars and Earth.
Measurements of depression and rebound provide insights into the viscosity of the mantle rocks and the characteristics of planetary construction.
The team estimated that Mars's north pole surface area is subsiding at rates of up to 0.13 millimeters per year, indicating a cold Martian interior.
The age of Mars's north polar ice cap is estimated to be between 2 and 12 million years, making it one of the youngest large-scale features on the planet.
The findings highlight the presence of local melt zones in the mantle near the equator, contrasting with the cold mantle underneath the north pole.