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High-CO2 Climates and Observables in the Outer Habitable Zone

  • Authors: Daria Pidhorodetska, Edward W. Schwieterman, Thomas J. Fauchez, Martin Turbet

Daria Pidhorodetska et al 2026 The Astrophysical Journal 1009 .

  • Provider: AAS Journals

Caption: Figure 7.

Modeled transmission (left column) and emission (right column) spectra for planetary “edge cases” around TRAPPIST-1 at pCO2 = 5 bar. Blue spectral lines indicate the highest insolation considered that does not reach equilibrium. Red, orange, and yellow spectral lines denote insolation values that reach equilibrium and are considered to be habitable planets. Temperature values that correspond to these insolation values can be found in Table 3.

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