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The Milky Way Galaxy is literally teeming with exoplanets; thousands ofplanets have been discovered, with thousands more planet candidates identified.Terrestrial-like planets are quite common around other stars, and are expectedto be detected in large numbers in the future. Such planets are the primarytargets in the search for potentially habitable conditions outside the solarsystem.  Determining the atmospheric composition of exoplanets is mandatory tounderstand their origin and evolution, as atmospheric processes play crucialroles in many aspects of planetary architecture. In this work we construct andexploit a 1D radiative transfer model based on the discrete-ordinates method inplane-parallel geometry. Radiative results are linked to a convective flux thatredistributes energy at any altitude producing atmospheric profiles inradiative-convective equilibrium. The model has been applied to a large number(6250) of closely dry synthetic \ce{CO2} atmospheres, and the resultingpressure and thermal profiles have been interpreted in terms of parametervariability. Although less accurate than 3D general circulation models, notproperly accounting for e.g., clouds and atmospheric and ocean dynamics, 1Ddescriptions are computationally inexpensive and retain significant value byallowing multidimensional parameter sweeps with relative ease.

A systematic study of \ce{CO2} planetary atmospheres and their link to the stellar environment