Vapor Pressure, Boiling and Freezing Temperatures of a Solution
Uri Lachish, guma science
Addition of solute molecules to a liquid elevates its boiling temperature and
reduces its vapor pressure and freezing temperature. These phenomena, as well as
osmosis, depend only on the solute concentration and not on its type, and are
called colligative properties of solutions.
The process of elastic collisions of particles with a moving wall is a
general mechanism of transforming their microscopic kinetic energy into
macroscopic mechanical work, and vice versa . This mechanism accounts for the
colligative properties .
Whenever molecules evaporate from a liquid the boundary layer between the
liquid and the vapor will move. When the liquid contains a non volatile solute,
the moving boundary will transfer energy to the solute molecules. This energy is
included in the evaporation process, therefore, it will affect the vapor
pressure and boiling temperature of a solution. Similarly, during freezing, or
melting, the boundary movement between the solution and pure solid will affect
the freezing temperature. In both cases the moving boundary works against the
osmotic pressure generated by the solute.
Vapor pressure of a solution:
Consider a vessel of constant volume that contains a liquid and its vapors. A
molecule at the liquid surface will leave it to the vapor phase if its kinetic
energy is higher than the binding energy to the liquid. On the other hand, all
molecules at the vapor phase that hit the liquid surface will stay with it.
During equilibrium the rate of evaporation from the liquid will be equal to the
rate of condensation to it.
According to the Maxwell- Boltzmann
distribution function the evaporation rate is proportional to
e-Li/RT, while the condensation rate is proportional to the
vapor concentration (N/V). Li is the molar heat of
evaporation. It is the amount of heat supplied to a liquid in order to evaporate
one mole. R is the gas constant and T the absolute temperature.
The condensation rate is proportional to the vapor concentration, and
therefore, also to the pressure p = (N/V)RT. Therefore, at equilibrium:
p = αRT e-Li/RT (1)
where α is a proportion factor.
When liquid evaporates from a solution surface, the boundary will do work
against the osmotic pressure of the solute. This work is included in the
evaporation process and there will be a need of more energy for it. Therefore,
the evaporation rate from a solution is somewhat slower than evaporation from a
pure liquid, and consequently, the solution's vapor pressure is lower than that
of a pure liquid.
When one mole of a liquid evaporates from a solution surface, the surface
will do the work πv against the osmotic pressure
π. v is the volume of one mole of
solution. By van't Hoff
formula the osmotic pressure is π = cRT, where
c is the solute concentration.
The solution heat of evaporation is:
Ls = Li + πv =
Li + cRTv (2)
therefore, the solution vapor pressure will be:
ps = αRT e-Ls/RT =
αRT e-(Li/RT +x) (3)
where x = cv is the molar fraction of the solute.
Division of equations (1)-(3), and exponent expansion to first order, yields
for dilute solutions:
ps/p = e-x = 1-x (4)
This is Raoult's law.
It relates the vapor pressure reduction of a solution, compared to the pure
liquid, to the solute's molar fraction.
Boiling temperature elevation:
Boiling occurs in a liquid in an open vessel when its vapor pressure is equal
to the external pressure pexternal. The liquid heats up and
its vapor pressure increases until it reaches the external pressure. Then
boiling starts. Since the vapor pressure of a solution is lower than that of the
pure liquid it will reach the external pressure at higher temperature.
Consequently, the boiling temperature of the solution will be higher than that
of the pure liquid.
The boiling condition for a pure liquid is determined by equation (1):
pexternal = αRTi
where Ti is the boiling temperature of the pure liquid.
Similarly, the boiling condition for the solution is given by equation (3):
pexternal = αRTs
e-(Li/RTs + x) (6)
where Ts is the boiling temperature of the solution.
pexternal is eliminated from these two equations:
Tie-(Li/R)(1/Ti - 1/Ts) =
Both exponent terms in equation (7) are small, therefore, they can be
expanded to first order (e-x = 1 - x), and after some algebra:
Ts - Ti = Tsx - (Ts -
Denoting ΔT = Ts - Ti,
and after more algebra:
(R(Ts)2/(Li + RTs))x
This approximate formula relates the change of the boiling temperature
ΔT to the molar fraction of the solute x.
Freezing temperature reduction:
The reduction of the freezing temperature is similar to the elevation of the
boiling temperature. When the solid melts the boundary between it and the liquid
will move. If the liquid contains solute molecules, then the work done by the
osmotic pressure will supply some of the heat of melting and less heat will be
required externally. This effect results the reduction of the melting or
freezing temperature. Similar calculation yields temperature reduction:
ΔT = -(RTTs/L)x
where L is the molar heat of melting.
- F.W. Sears and G.L. Salinger, "Thermodynamics, Kinetic Theory and
statistical Thermodynamics", 3rd Ed., 16th printing, Addison
Wesley, Reading Massachusetts (1986)
- U. Lachish, "Derivation of Some Basic Properties of Ideal Gases and
Solutions from Processes of Elastic Collisions", J. Chem. Ed., 55, 369
On the net: 15, December, 1998
Osmosis Reverse Osmosis and Osmotic Pressure what they are
Osmosis and Thermodynamics
van't Hoff's Evidence
By the author:
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Full page: http://urila.tripod.com/Thermoelectric.pdf, February 2014.
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- Thermodynamics Research Laboratory,
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