
Mars’s longest morning cloud may form ice without dust
A white cloud stretching as far as 1,800 kilometers across Mars may owe its extraordinary shape to an unusual way of making ice. Computer simulations suggest water vapor can form new ice particles without first attaching to dust.
The finding concerns the Arsia Mons Elongated Cloud, a recurring morning feature downwind of one of Mars’s giant volcanoes. Jorge Hernández-Bernal of LMD/CNRS/Sorbonne Université in Paris led the modeling study, published in Nature Geoscience.
Using observations from the European Space Agency’s Mars Express, the team investigated why conventional cloud models failed to reproduce the long tail. Adding a process called homogeneous ice nucleation produced the cloud’s defining features, although several measurements still differed substantially.
The results offer a physical explanation for a familiar orbital spectacle. They do not yet constitute direct observational confirmation of the proposed particle-forming process.