[astro-ph.EP]. The habitable zone (HZ) boundaries calculated with the Clima one-dimensional radiative-convective equilibrium (RCE) model have served as a standard reference for exoplanet target selection for three decades, but they […]
![Dependence of habitable zone boundaries on planetary mass. The inner edge is the runaway greenhouse limit and the outer edge is the maximum greenhouse limit, shown for 0.1, 1, and 5 M⊕ planets. Both edges are color coded by planetary mass. Dashed curves show the R. K. Kopparapu et al. (2014, Equation (4)) boundaries. [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/11/Validation.png?resize=1200%2C717&ssl=1)
[astro-ph.EP]. The habitable zone (HZ) boundaries calculated with the Clima one-dimensional radiative-convective equilibrium (RCE) model have served as a standard reference for exoplanet target selection for three decades, but they […]