Dayside Temperature (occultation): 1967 K |
JWST-MIRI | JWST MIRI reveals a potential atmosphere on the ultra-hot rocky planet TOI-431b2026, Cole Smith, Brandon Park Coy et al. |
results are best explained by the presence of an atmosphere |
Dayside Temperature (occultation): 1520 K |
Spitzer | Low 4.5 μm Dayside Emission Disfavors a Dark Bare-Rock scenario for the Hot Super-Earth TOI-431 b2025, Christopher Monaghan, Pierre-Alexis Roy et al. |
Tentative measurement of secondary eclipse (depth of 33±22 ppm) |