Mystery of the dark markings on Mars could finally be solved
This image from NASA’s Mars Reconnaissance Orbiter (MRO) shows streaks forming on slopes when dust cascades downhill. (NASA)
Mysterious dark streaks on Mars, observed since the 1970s, are likely due to wind and dust activity rather than water, according to new research.
Researchers used a machine learning algorithm to analyze 500,000 streaks from over 86,000 NASA Mars Reconnaissance Orbiter images, creating a global Martian map.
The study found that recurring slope lineae (RSLs) are not associated with factors suggesting liquid or frost, but rather with above-average wind speed and dust deposition.
Older slope streaks likely form when dust slides off slopes due to seismic activity, winds, or meteoroid impacts, appearing near recent impact craters.
The findings cast doubt on the interpretation of slope streaks and RSLs as habitable environments, suggesting a dry origin of formation.