For
molecules of a liquid to evaporate, they must be located near the surface, they have to be moving in the proper direction, and have sufficient
kinetic energy to overcome liquid-phase
intermolecular forces. When only a small proportion of the molecules meet these criteria, the rate of evaporation is low. Since the kinetic energy of a molecule is proportional to its temperature, evaporation proceeds more quickly at higher temperatures. As the faster-moving molecules escape, the remaining molecules have lower average kinetic energy, and the temperature of the liquid decreases. This phenomenon is also called
evaporative cooling. This is why evaporating
sweat cools the human body. Evaporation also tends to proceed more quickly with higher flow rates between the gaseous and liquid phase and in liquids with higher
vapor pressure. For example, laundry on a clothes line will dry (by evaporation) more rapidly on a windy day than on a still day. Three key parts to evaporation are heat,
atmospheric pressure (determines the percent humidity), and air movement. On a molecular level, there is no strict boundary between the liquid state and the vapor state. Instead, there is a
Knudsen layer, where the phase is undetermined. Because this layer is only a few molecules thick, at a macroscopic scale a clear
phase transition interface cannot be seen. Liquids that do not evaporate visibly at a given temperature in a given gas (e.g., cooking oil at room
temperature) have molecules that do not tend to transfer energy to each other in a pattern sufficient to frequently give a molecule the heat energy necessary to turn into vapor. However, these liquids
are evaporating. It is just that the process is much slower and thus significantly less visible.
Evaporative equilibrium = 1
atm. If evaporation takes place in an enclosed area, the escaping molecules accumulate as a
vapor above the liquid. Many of the
molecules return to the liquid, with returning molecules becoming more frequent as the
density and
pressure of the vapor increases. When the process of escape and return reaches an
equilibrium, the vapor is said to be "saturated", and no further change in either
vapor pressure and density or liquid temperature will occur. For a system consisting of vapor and liquid of a pure substance, this equilibrium state is directly related to the vapor pressure of the substance, as given by the
Clausius–Clapeyron relation: : \ln \left( \frac{ P_2 }{ P_1 } \right) = - \frac{ \Delta H_{\rm vap } }{ R } \left( \frac{ 1 }{ T_2 } - \frac{ 1 }{ T_1 } \right) 2/P1 = −
ΔHvap/
R((1/T2)-(1/T1)) --> where
P1,
P2 are the vapor pressures at temperatures
T1,
T2 respectively, Δ
Hvap is the
enthalpy of vaporization, and
R is the
universal gas constant. The rate of evaporation in an open system is related to the vapor pressure found in a closed system. If a liquid is heated, when the vapor pressure reaches the ambient pressure the liquid will
boil. The ability for a molecule of a liquid to evaporate is based largely on the amount of
kinetic energy an individual particle may possess. Even at lower temperatures, individual molecules of a liquid can evaporate if they have more than the minimum amount of kinetic energy required for vaporization. == Factors influencing the rate of evaporation ==