Overview
- Observations indicate the vortex interior is about 40°C colder from near the surface up to roughly 30 km than surrounding air.
- At these temperatures, scarce water vapor freezes onto the ice cap, removing the usual ozone-destroying chemistry and allowing ozone to surge.
- The team combined ESA Trace Gas Orbiter ACS composition profiles with NASA Mars Climate Sounder temperature maps to target measurements inside the vortex.
- Because the north polar region is in darkness during winter, measurements were possible when the vortex became distorted, offering a rare look into polar-night chemistry.
- The findings were presented by Kevin Olsen and colleagues at the EPSC-DPS2025 meeting in Helsinki, with implications for models of past UV shielding and for ESA’s Rosalind Franklin rover mission planned for 2028.