Airless, thin residual, and hazy-inversion atmospheres all match TRAPPIST-1 b's eclipse and phase curve data, so a single 15 µm eclipse depth is not enough to conclude a planet is airless.
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Constraints on the possible atmospheres on TRAPPIST-1 b: insights from 3D climate modeling
Airless, thin residual, and hazy-inversion atmospheres all match TRAPPIST-1 b's eclipse and phase curve data, so a single 15 µm eclipse depth is not enough to conclude a planet is airless.