Equilibrium vapor pressure can be defined as the pressure reached when a condensed phase is in equilibrium with its own vapor. In the case of an equilibrium solid, such as a
crystal, this can be defined as the pressure when the rate of
sublimation of a solid matches the rate of dissolution to form a vapor. For most solids this pressure is very low, but some notable exceptions are
naphthalene,
dry ice (the vapor pressure of dry ice is 5.73 MPa (831 psi, 56.5 atm) at 20 °C, which causes most sealed containers to rupture), and ice. All solid materials have a vapor pressure. However, due to their often extremely low values, measurement can be rather difficult. Typical techniques include the use of
thermogravimetry and gas transpiration. There are a number of methods for calculating the sublimation pressure (i.e., the vapor pressure) of a solid. One method is to estimate the sublimation pressure from extrapolated liquid vapor pressures (of the supercooled liquid), if the
heat of fusion is known, by using this particular form of the Clausius–Clapeyron relation: :\ln\,P^{\rm sub}_{\rm s} = \ln\,P^{\rm sub}_{\rm l} - \frac{\Delta_{\rm fus}H}{R} \left( \frac{1}{T_{\rm sub}} - \frac{1}{T_{\rm fus}} \right) where: • P^{\rm sub}_{\rm s} is the sublimation pressure of the solid component at the temperature T_{\rm sub} . • P^{\rm sub}_{\rm l} is the extrapolated vapor pressure of the liquid component at the temperature T_{\rm sub} . • \Delta_{\rm fus}H is the heat of fusion. • R is the
gas constant. • T_{\rm sub} is the sublimation temperature. • T_{\rm fus} is the melting point temperature. This method assumes that the heat of fusion is temperature-independent, ignores additional transition temperatures between different solid phases, and it gives a fair estimation for temperatures not too far from the melting point. It also shows that the sublimation pressure is lower than the extrapolated liquid vapor pressure (Δfus
H > 0) and the difference grows with increased distance from the melting point. ==Boiling point of water==