![Distribution of simulated EEC yield (solid contours) and underlying planet population (dotted contours) around FGK-type stars within 20 pc. We show the planetary radius over incident flux distribution, where the color shading represents the relative density of planet occurrences in this parameter space. The colored contours enclose 10% to 100% of the total planet counts, with the innermost contour indicating the highest-density regions. Grey dashed lines represent EEC boundaries around a Sun-like star with S/S⊕ ∈ [0.356, 1.107] and R/R⊕ ∈ [0.8 · S 0.25, 1.4] (Kopparapu et al. 2014; Stark et al. 2019; Quanz et al. 2022b). Top and right margin plots show the individual distributions of incident flux and planetary radius of detected and total underlying populations. Underlying synthetic planet populations are based on Kammerer et al. (2022). -- astro-ph.EP](https://i0.wp.com/astrobiology.com/wp-content/uploads/2025/06/Detecting-Atmospheric-CO2-Trends1.png?resize=1200%2C720&ssl=1)
Identifying key observables is essential for enhancing our knowledge of exoplanet habitability and biospheres, as well as improving future mission capabilities.
Posted inAstronomy & Telescopes, Atmospheres, Climate, Weather, Biosignatures & Paleobiology, Exoplanets, -moons, -comets, Habitable Zones, Imaging & Spectroscopy, Status Report