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Saving Doomed Planets: Mass Loss and Angular Momentum Return Boost Hot Jupiter Survival Rates

  • Authors: Grant C. Weldon, Bradley M. S. Hansen, Smadar Naoz

Grant C. Weldon et al 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 10.

Panel (a): the fitted parameters in Equation (A1) from MESA evolutionary models. The color-coding shows A (top left), tbreak (top right), α1 (bottom left), and α2 (bottom right) as a function of the logarithm of stellar flux and the planetary mass. Panel (b): example fit to a MESA cooling curve using the fit parameters from panel (a) for a 2.0MJ planet with a stellar flux of 107 erg s−1 cm−2.

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