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Coupled Photochemical–Climate Modeling of Plausible Tenuous Outgassed Atmospheres on the TRAPPIST-1 Planets

  • Authors: Megan T. Gialluca, Victoria S. Meadows, Andrew P. Lincowski, Trent B. Thomas, P. C. Hinton, David Brain, David Crisp

Megan T. Gialluca et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 2.

Examples illustrating the compositional and pressure–temperature ranges of the atmospheric archetypes found in this study. Temperature and gas mixing ratio profiles (as a function of atmospheric pressure) for H2O, CO2, O2, O, O3, and CO are shown for examples of every archetype atmosphere for T-1 c and e. The top row (peach colored background) shows profiles for T-1 c and the bottom row (white colored background) shows T-1 e profiles. When available, atmospheric cases are shown both without (solid lines) and with SO2 contributions of either 1% (dashed line), 0.1% (dashed–dotted line), or 100 ppm (dotted line) injected into the bottom layer.

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