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JWST MIRI Reveals a Potential Atmosphere on the Ultrahot Rocky Planet TOI-431b

  • Authors: Cole Smith, Brandon Park Coy, Megan Weiner Mansfield, Rafael Luque, Anjali A. A. Piette, Qiao Xue, Michael Zhang, Jacob L. Bean, Madison Brady, Peter Gao, Jegug Ih, Eliza M.-R. Kempton, Edwin Kite, Daniel Koll, Jaume Orell-Miquel, Enric Palle

Cole Smith et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 2.

Contour plot showing the brightness temperatue of TOI-431b in the LRS bandpass as a function of the planetŠs Bond albedo and heat redistribution efficiency. The solid black line is the derived dayside temperature in the LRS bandpass, and the dotted lines show ±1 and 2σ dayside temperatures respectively. This shows that the planet is more than 1.8σ inconsistent with being a bare dark rock. Colored points show Bond albedo and heat redistribution values for solar system bodies, adopted from Q. Xue et al. (2024).

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