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Mars Cloud Mystery Solved: Exotic Physics at Play
23 Oct
Summary
- A 1,000-mile-long Martian cloud forms and dissipates daily.
- Scientists modeled the cloud, revealing novel homogeneous nucleation.
- Extreme conditions and a volcano drive the unique cloud formation.

A colossal, thread-like cloud that stretches over 1,000 miles near the Martian volcano Arsia Mons has baffled scientists since 2018. This daily phenomenon, observed during the planet's spring and summer, has now been successfully modeled for the first time. Researchers discovered that the cloud's formation is driven by exotic physics, specifically homogeneous nucleation. This process allows water vapor to directly transform into ice crystals without the assistance of dust or salt particles, a phenomenon previously considered theoretical and never directly observed in nature.
The formation of the Arsia Mons Elongated Cloud (AMEC) requires extreme conditions: a rapid 30-degree Celsius temperature drop within 10 minutes and high humidity. The towering Arsia Mons volcano plays a critical role, as wind currents create powerful waves that propel moist air to high altitudes. This atmospheric process, though hypothesized for other planets like Venus and Earth, has never been observed due to the exceptionally high humidity levels required, exceeding those found on Earth by over 100,000 times. The successful modeling provides remarkable insight into Mars' atmospheric dynamics, previously less understood than Earth's.