Constraints on the possible atmospheres on TRAPPIST-1 b: insights from 3D climate modeling
Year: 2025
Type: article
Abstract: Context. JWST observations of the secondary eclipse of TRAPPIST-1 b at 12.8 and 15 µm revealed a very bright dayside. These measurements are consistent with an absence of atmosphere. Previous 1D atmospheric modeling also excludes – at first sight – CO2-rich atmospheres. However, only a subset of the possible atmosphere types has been explored, and ruled out, to date. Recently, a full thermal phase curve of the planet at 15 µm with JWST has also been observed, allowing for more information on the thermal structure of the planet. Aims. We first looked for atmospheres capable of producing a dayside emission compatible with secondary eclipse observations. We then tried to determine which of these are compatible with the observed thermal phase curve. Methods. We used a 1D radiative-convective model and a 3D global climate model (GCM) to simulate a wide range of atmospheric compositions and surface pressures. We then produced observables from these simulations and compared them to available emission observations. Results. We found several families of atmospheres compatible at 2σ with the eclipse observations. Among them, some feature a flat phase curve and can be ruled out with the observation, and some produce a phase curve still compatible with the data (i.e., thin N2 –CO2 atmospheres, and CO2 atmospheres rich in hazes). We also highlight different 3D effects that could not be predicted from 1D studies (redistribution efficiency, atmospheric collapse). Conclusions. The available observations of TRAPPIST-1 b are consistent with an airless planet, which is the most likely scenario. A second possibility is a thin CO2-poor residual atmosphere. However, our study shows that different atmospheric scenarios can result in a high eclipse depth at 15 µm. It may therefore be hazardous, in general, to conclude on the presence of an atmosphere from a single photometric point.
Source: Astronomy and Astrophysics
Institutions: Centre National de la Recherche Scientifique, École Polytechnique, Université Paris Sciences et Lettres, Institut d'Astrophysique de Paris, Sorbonne Université, Laboratoire de Météorologie Dynamique, Institut Polytechnique de Paris, Laboratoire d'Astrophysique de Bordeaux, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Université Paris-Saclay, Observatoire de Paris, Astrophysique, Instrumentation et Modélisation, Sorbonne Paris Cité, University of Geneva, Institut de Planétologie et d'Astrophysique de Grenoble, Université Grenoble Alpes, American University, University of Liège
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
SDG: Climate action
Open Access status: gold
Estimated APC paid: $1,865
Awards: G5874472907, G8240302720
OpenAlex ID: W4413850812