For a one-phase spherical Stefan problem with melting-temperature boundary value and supercooling , use the latent-to-sensible heat ratio . Large separates heat diffusion from slow interface motion. The exterior harmonic temperature is . The Stefan condition gives the displayed radius equation with . This is the large inverse-Stefan number convention; the common sensible-to-latent Stefan number is .
The Gibbs--Thomson relation depresses a spherical interface's equilibrium temperature by . For , its interface is warmer than the supercooled ambient and heat loss drives growth. For , its interface is colder than the ambient and heat gain drives melting. The equilibrium radius is unstable because the derivative of the quasistatic radius velocity at is positive.
In the quasistatic spherical model, . Separating the radius equation gives , which is finite and evaluates to the displayed expression. Near disappearance, . The time diverges logarithmically as the initial radius approaches the critical radius from below.

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