Overview

• A global catalog of over 500,000 Martian slope streaks was created using machine learning and 86,000 high-resolution satellite images.
• Geostatistical analysis links these features to wind, dust deposition, and seismic activity, ruling out liquid water or frost as their origin.
• The findings indicate that these locations are unlikely to support life, reducing contamination concerns for future Mars missions.
• Slope streaks often form near impact craters, while recurring slope lineae (RSLs) are associated with dust devils and rockfalls.
• The study underscores the role of dust dynamics in shaping Mars' surface and climate, with millions of tons of material potentially transported annually.