
On Mars, a massive elongated cloud forms daily over the volcano Arsia Mons during the Martian southern spring and summer, stretching up to 1800 km long before vanishing within hours. No atmospheric simulation could explain how such a cloud should exist, until a new study proposed that it forms through homogeneous nucleation, a process long theorized but never before confirmed in real atmospheric conditions. The mechanism involves extreme, rapid cooling as moist air is forced up the volcano's slope, triggering spontaneous ice crystal formation without any dust seed. The discovery also raises the possibility that similar cloud formation could occur in Earth's upper atmosphere.
[00:16] Every morning during Martian southern spring and summer, a massive bright white cloud emerges over the volcano Arsia Mons.


