Image Details
Caption: Figure 4.
Left: the best-fit clear-atmosphere RCTE and VULCAN forward models against the visit 2 Eureka1 reduction. Right: the respective pressure–temperature profiles of each model. Even though chemical disequilibrium with VULCAN provides a better fit to the data, the resulting pressure–temperature profiles are virtually the same.
© 2026. The Author(s). Published by the American Astronomical Society.