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The Limits of Tidal Circularization and Atmospheric Escape for Mini-Neptunes and Super-Earths: The Case of TOI-2257 b

  • Authors: Michael Kent A. Olohoy, Yukari Aubrey D. Gelani, Rory Barnes

Michael Kent A. Olohoy et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 6.

Change in eccentricity Δe of TOI-2257 b (super-Earth case) as a function of initial e and log-transformed tidal τ. The contour lines represent Δe as the planet experiences tidal effects throughout the simulation. Higher τ values result in greater eccentricity decay.

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