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Mars Has a Cloud 1,100 Miles Long, and It Keeps Coming Back

Every Martian year, as southern spring approaches, a cloud forms over the volcano Arsia Mons and stretches westward for some 1,100 miles — a tail of white vapour…

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Mars and the Valles Marineris canyon system. Photo: NASA, public domain, via Wikimedia Commons.
Mars and the Valles Marineris canyon system. Photo: NASA, public domain, via Wikimedia Commons.

Every Martian year, as southern spring approaches, a cloud forms over the volcano Arsia Mons and stretches westward for some 1,100 miles — a tail of white vapour longer than the distance from London to Rome, unfurling over a few hours and dissolving by midday. Scientists call it the Arsia Mons Elongated Cloud, and a re-analysis of data from ESA’s Mars Express orbiter, using a new meteorological model, has now sharpened our picture of how this colossal, clockwork phenomenon works.

The cloud’s regularity is what makes it precious. Mars weather is usually described in the vocabulary of chaos — planet-wrapping dust, wandering frost. The Arsia cloud instead behaves like a machine: the same volcano, the same season, the same morning hours, a plume that grows at extraordinary speed and vanishes on schedule. That clockwork quality turns it into a natural laboratory for Martian atmospheric dynamics, a single reproducible experiment the planet runs annually for orbiting instruments.

The new modelling work digs into the mechanism: moist air forced up the volcano’s slopes in the cold morning, condensing at altitude, then sheared westward by high winds into the famous tail. Understanding the details — how much water vapour the process lifts, and where it goes — feeds directly into the bigger question of Mars’s modern water cycle, which in turn governs everything from frost formation to the chemistry future landers will dig into.

There is also an archival moral to the story. The re-analysis was performed on data from a spacecraft launched more than two decades ago. Mars Express has outlived most of the missions sent to relieve it, and its instruments keep answering questions nobody had thought to ask when they were built — a reminder that in planetary science, data is an endowment, and modelling is how the interest compounds.

Next southern spring, the volcano will make its cloud again, on schedule, indifferent to being watched. The scientists will be watching anyway. On a planet we mostly know as dead, the Arsia cloud is a pulse — regular, enormous and still being taken.

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