
Tiny Martian Storms May Explain Mars’ Hidden Water Loss
A localized Martian Year 37 dust storm lifted water vapor into the middle atmosphere at levels up to ten times typical, with hydrogen at the exobase rising about 2.5×. This suggests small, regional storms contribute to Mars’s long-term water loss and challenges the idea that southern-summer global events were the main driver, using data from ExoMars TGO, MRO, and the Emirates Mars Mission.

