Sculpting of Martian brain terrain reveals the drying of ancient Mars
Shenyi Zhang, Lei Zhang, Yutian Ke, Jinhai Zhang

TL;DR
This study combines morphological analysis and numerical modeling to reveal that Martian brain terrain formed through initial freeze-thaw processes followed by sublimation-driven sculpting, indicating a climate shift from wet to dry on Mars.
Contribution
It introduces a quantitative system and a numerical model to explain MBT formation, highlighting the role of sublimation in shaping Martian terrain.
Findings
Self-organized transport alone cannot produce the observed relief of MBT.
Sublimation-driven sculpting accounts for the majority of relief features.
MBT formation involved a transition from liquid water processes to dry sublimation effects.
Abstract
The Martian brain terrain (MBT), characterized by its unique brain-like morphology, is a potential geological archive for finding hints of paleoclimatic conditions during its formation period. The morphological similarity of MBT to self-organized patterned ground on Earth suggests a shared formation mechanism. However, the lack of quantitative descriptions and robust physical modeling of self-organized stone transport jointly limits the study of the thermal and aqueous conditions governing MBT's formation. Here we established a specialized quantitative system for extracting the morphological features of MBT, taking a typical region located in the northern Arabia Terra as an example, and then employed a numerical model to investigate its formation mechanisms. Our simulation results accurately replicate the observed morphology of MBT, matching its key geometric metrics with deviations…
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