JWST eclipse data show HD 3167 b has a cooler dayside than a bare rock, indicating an atmosphere on this least-irradiated USP super-Earth with such evidence.
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The sky-projected obliquity of TOI-1259Ab is measured as λ = 6+21−22° and the true 3D obliquity as ψ = 24+14−12° (ψ < 48° at 95 % confidence), indicating a well-aligned orbit too wide for tidal realignment.
citing papers explorer
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An Atmosphere on the Ultra-Short Period super-Earth HD 3167 b
JWST eclipse data show HD 3167 b has a cooler dayside than a bare rock, indicating an atmosphere on this least-irradiated USP super-Earth with such evidence.
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TOI-1259Ab: A Warm Jupiter Orbiting a K-dwarf White-Dwarf Binary is on a Well-aligned Orbit
The sky-projected obliquity of TOI-1259Ab is measured as λ = 6+21−22° and the true 3D obliquity as ψ = 24+14−12° (ψ < 48° at 95 % confidence), indicating a well-aligned orbit too wide for tidal realignment.