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Osmotic flow countered by the osmotic pressure

 

Schematic showing the effect of osmotic flow countered by the osmotic pressure (Pi)

Osmotic pressure

Osmotic pressure is the tendency of solvent molecules to move in the direction of lower solvent activity.

 

V Mole fraction : molarity, molality, % w/w and % w/v

V Overview of colligative properties :
V Vapor pressure lowering : CaCl2
V Freezing point depression : examples : Glucose : Urea : Ethanol : NaCl : CaCl2
V Boiling point elevation : Glucose
V Diffusion

V Osmotic pressure

V Relation of osmotic pressure to vapor pressure lowering
V Osmotic pressure of polymers

V Osmotic potential

V Self-generation of osmotic pressure at interfaces
V Reverse osmosis

 

"...the cause of osmosis is the difference that exists between the free energy or activity

of the solvent in the pure state and in solution..."

Alexander Finlay 'Osmotic Pressure' 1919  

Diffusion

Diffusion, particles of a soluble material spread out

 

Diffusion, particles of a soluble material spread out to uniformly distribute themselves

Diffusion is the net movement of particles (for example, molecules or atoms) from a region of high chemical potential (for example, high concentration) to a region of low chemical potential (for example, low concentration), see left. Such diffusion also involves the movement of water in the opposite direction. The movement is due to the statistical outcome of random Brownian motion. The mean squared displacement is proportional to the time elapsed (t) and the diffusivity (D); the averaged net displacement (Δx) being proportional to the square root of the elapsed time.

<Δx2> = 2Dt

With time, the concentrations gradients dissipate. Diffusion increases entropy (randomness), leading to a lower energy state.

Osmotic pressure

When pure liquid water is separated by a membrane, permeable to water but not solute, from a solution containing a solute, water will pass from the pure water side until sufficient extra pressure (π) is caused or applied to the solution side [1872]. Water moves from high to low water activity due to osmosis. The pressure needed to stop the osmotic flow is the osmotic pressure (see below right). At this equilibrium, the vapor pressures of the solution and the pure water are the same. Note that osmotic pressure is an equilibrium thermodynamic effect a and gives no information concerning the rate of passage of the water, which depends primarily on the properties of the membrane [1873]. The osmotic pressure is related to other colligative properties such as freezing point depression [2749]. Either can be used to calculate the other.

 

Net movement of water towards lower activity water

solution, generating osmotic pressure

 

Net movement of water towards lower activity water solution, generating osmotic pressure

 

There is often confusion in the literature between the thermo-dynamic rationale and the kinetic process of osmosis. The thermo-dynamics of the process (e.g. the colligative property) simply describes the tendency for the process to occur but does not describe the mechanism or the rate of the flow of water in an osmotic process, apart from its (impending) direction. Clearly, the (net) rate of water flow depends on the relative rates of flow in the opposite directions. This, in turn, will depend on the ease with which the water molecules may leave the compartments on each side of the membrane, if present (dependent on the mole fraction of 'free' (bulk) water; the water activity), and the ease with which they can pass through such membrane. Water molecules leaving the lower-water-activity compartment will require more energy as they cause the formation of a localized even lower activity water in their wake. Therefore only higher energy water molecules can leave this compartment; necessarily a smaller amount than travel in the opposite direction. Note that the difference in activity may depend on the difference in the concentration of dissolved molecules and ions as discussed for other colligative properties, or may be due to other causes, such as surface interactions. The measured water flux is often much smaller than the theoretical water flux due to concentration polarization and the membrane resistance, together with an allowance for leakage through the membrane (the osmotic reflection coefficient (σ) [3088]).

 

At equilibrium, the chemical potential (μ) of the water must be the same on both sides of the semipermeable membrane. c

 

(1)

chemical potential of pure water at pressure P = chemical potential of a solution at pressure P+osmotic pressure (Pi)

The effect of the solute may be included as for Raoult's law

 

see below d (2)

chemical potential of a solution at pressure P+osmotic pressure (Pi) = chemical potential of pure water at pressure P+osmotic pressure (Pi)+ RTLn(xw)

where xw is the mole fraction of the ‘free’ water (0 < xw < 1). b

 

The change in chemical potential with pressure may be included.

 

(3)

chemical potential of pure water at pressure P+osmotic pressure (Pi) = chemical potential of pure water at pressure P+ integral from pressure P to P+osmotic pressure of (the molar volume of water) dT

Combining equations 1, 2 and 3 and then assuming the molar volume of water (Vm, m3 mol-1 ) varies little within the likely pressure range.

chemical potential of a solution at pressure P+osmotic pressure (Pi) = chemical potential of pure water at pressure P+ integral from pressure P to P+osmotic pressure of (the molar volume of water) dT+ RTLn(xw)

 

 

(4)

-RTLn(xw) = integral from pressure P to P+osmotic pressure of (the molar volume of water) dT = ΠVm

[250] (5)

 

Hence,

Π = -kp T Ln(1-xs)

           where kp is the piezoscopic constant (= R/Vm).

 

When xs is low the following approximation is valid

(6)

Ln(xw) = Ln(1 - xs) = - xs

 

(7)

ΠVm = xsRT

(8)

At low xs,

xs = ns/nw             

 

where ns is the number of moles of solute and nw is the number of moles of water. As the molar volume approximately equals V/nw,

the Van't Hoff equation (9) g

Π= MsRT

 

where Ms = ns/V, the molar concentration of the solute (normally, moles m-3, if in SI units). f

 

The osmotic behavior of glucose solutions

The osmotic behavior of glucose solutions

Opposite shows the osmotic behavior of glucose solutions. e The lower blue line follows the 'ideal' colligative equation, Π= MsRT. The thick red line follows the osmotic pressure as calculated from the experimental freezing point data [70]. The middle green line shows the osmotic pressure calculated from the 'ideal' colligative equation, Π= MsRT , but correcting the concentration errors made by assuming Ln(1 - xs) = - xs and xs = ns/nw (but not the error in the molar volume of water). The dotted black line is the best-fit to the equation,

          Π= RT(Ms+AMs2)               (10)

a commonly used form of approximation [1104], where A = 0.2 M-1 in this case; most of the 'A' parameter is due to the approximations used and not due to non-ideality. The thin red line is described below. Note that at low osmotic pressures, up to about five atmospheres pressure (0.5 MPa) the ideal colligative equation holds well.

Osmotic coefficients of bromides and acetates

Osmotic coefficients of bromides and acetates

Experimental osmotic pressures (Π) may be compared with the 'ideally expected' osmotic pressure (Π0; as from Raoult's law) by the osmotic coefficient (ϕ); ϕ = Π/Π0. The osmotic coefficients of salts vary in a complex ion-specific manner (as ion activities, [2225], see Hofmeister series). For example, at a given concentration, the osmotic coefficients of bromide and iodide salts decreases in the sequence: Li+ > Na+ > K+ > Rb+ > Cs+ (see left), whereas the osmotic coefficients of acetate or fluoride salts decreases in the opposite sequence: Cs+ > Rb+ > K+ > Na+ > Li+ [2224]. The form of the curves involves a drop in activity due to direct contact ion-pairing reducing the apparent salt concentration counteracted by an increase in osmotic coefficients due to the binding of water by the salt and its consequential loss from the dissolving solution, so increasing the apparent concentration. The order of the salts is governed by their tendency to form direct contact ion-pair as opposed to solvent separated ion-pairs.

 

Although osmotic pressure and simple diffusion may be treated as distinct unrelated phenomena [2100], one being thermodynamic and the other kinetic, osmotic pressure presents the driving force (osmosis) for the 'diffusion' of water from a region of high 'free' water concentration to a region of lower 'free' water concentration (e.g. one with higher salt content). Such a relationship cannot exist between a thermodynamic property (osmotic pressure) and a kinetic process (rate of diffusion), but osmosis and diffusion can both be treated using kinetics. A diffusion-based theory for osmotic pressure has been described [1315], which involves a number of assumptions and gives the equation

Pi=MsRTx(xwV^2/(1+xsV))

where xw and xS are the mole fractions of water and solute and V is the volume of the solution (in liters) containing one liter of water. This equation contains no empirical parameters (such as 'A' above in equation 10) and gives a good fit; it is shown as the top thin dashed red line for glucose above. It is noteworthy that this equation is valid for single solutes only and includes the experimentally determined volume (V) term that varies non-linearly with concentration and has some dependency on the size of the solute.

 

Proteins may remove much of the 'free' water from inside cells causing much intracellular water to be osmotically unresponsive. As an example, one molecule of bovine serum albumin may bind 5000-43000 molecules of water [1103]. The osmolality of blood serum is about 282 - 295 mOsm/kg water, close to that of normal saline (0.90% w/v of NaCl, 308 mOsm/L). Serum values greater than 380 mOsm/kg water or less than 240 mOsm/kg water may be fatal.

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Relation of osmotic pressure to vapor pressure lowering

An alternative definition of the osmotic pressure of a solution of given uniform concentration at a given temperature is the liquid pressure under which the internal vapor pressure of such solution is equal to the vapor pressure of the pure solvent [2750]. The interface between liquid water and the gas phase is a form of semipermeable membrane, with water molecules able to pass through (by evaporation and condensation) but non-volatile solutes held within the liquid phase. It is unsurprising, therefore, that the osmotic pressure should be related to the lowering of vapor pressure. The relationship is

V ˣ dP = v ˣ dp

where V is the volume of the vapor at vapor pressure P and v is the volume of the solvent in the solution at liquid pressure p [2786].

 

The vapor pressure lowering is given by                                      Psolute = xwPpure liquid

Therefore,                                                                  Ppure liquid - Psolute = Ppure liquid ˣ (1 - xw)

From the gas laws (PV=RT) and  (xs =  1 - xw),          Ppure liquid - Psolute = xsRT/Vg               

where Vg is the molar volume of the gaseous solvent.

Relation of osmotic pressure to vapor pressure

 

Relation of osmotic pressure to vapor pressure

 

Compare this equation with equation 7 above for dilute solutions

Π = xsRT/Vm

where Vm is the molar volume of the liquid solvent. For water at STP, the ratio Vg/Vm = 1232.

Therefore,                   Ppure liquid - Psolute = Π/1232              at STP

 

For example from experiment, the vapor pressure lowering of a 1 M solution of NaCl at 100 °C, 101,325 Pa is 3.360 kPa. From the Van't Hoff equation, the osmotic pressure of this solution is 2000 ˣ 8.314 ˣ 373.15 = 6.205 MPa. At 100 °C, Vg/Vm = 1613 comparing well to the ratio of the pressures of 6205/3.36 = 1846 considering the approximations, experimental data error, and non-ideality involved.

 

Increasing solutes lower the water activity and the vapor pressure of a solution. The vapor pressure of a solution is increased by increasing the pressure on it. The osmotic pressure is the liquid pressure under which the vapor pressure of the solution is equal to the vapor pressure of the pure solvent. Both the osmotic pressure and the vapor pressure are intensive properties of solutions. As, at constant temperature and composition, ΔG=V ˣ Δp , the pressure change is related to the free energy change; that is, the amount of work that the system can perform.

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Osmotic pressure of polymers

At low concentrations in good solvents, linear polymers obey the Van't Hoff equation but not at higher concentrations. For all solvents at higher concentrations, this gives rise to complex osmotic behavior with far greater than expected (from Van't Hoff equation) osmotic pressures that depend on the degree of polymerization and the interaction between the chains. Polymer chains have random configurations sweeping through space and occupying much larger volumes than the molecular partial volume. The empirical equation Π = RT(Ms+AMs2) is often used, where A is the second virial coefficient that takes into account the interaction between two chains. Note that equation (4) ΠVm = -RTLn(xw) still holds throughout this section but the approximation Ln(xw) = Ln(1 - xs) = - xs presents greater error and should not be used. The polymers effectively remove (screen) some of the solvent from the solution by reducing the 'free' volume of solvent available.

 

Osmotic pressure of pullulan from [2709]

osmotic pressure of pullulan from [2709]

As the concentration of the neutral polymers increases, an overlap between the chains increases with increasing contacts between the monomers and the solution is no longer homogenous. Under these conditions, the des Cloiseaux law

Π ∝ Ms9/4

 

holds[2710] (see right [2709]). At low concentrations, the Van't Hoff equation osmotic pressure (πvH ) is given by,

osmotic pressure equation 1

where C is polymer mass concentration, Mp is polymer molecular weight, Mm is monomer molecular weight, and N is the number of monomers in the polymer chain. As the concentration increases (often called the semidilute regime), the osmotic pressure (π) varies as [2710],

osmotic pressure equation 2

where C* is a characteristic N-dependent polymer concentration associated with the crossover between the dilute and semidilute regimes (see figure above right) and k is a structurally-specific constant. C* has been related to the partial specific volume (V bar) [2710],

osmotic pressure equation 3

giving                                        osmotic pressure equation 5                and                osmotic pressure equation 5

with log-log plots of the osmotic pressure against mass concentration changing from unit gradient to a gradient of 9/4 around C* (polyelectrolytes change from 9/8 gradient to a gradient of 9/4 [2710c]).

 

The osmotic behavior of branched polymers is complicated by the degree and order of the branching with the osmotic pressure dependent on the 'free' volume of solvent available.

 

When the solvent is water, there are two ways that water becomes bound (i.e. not 'free' water) due to the number of monomers; water hidden from the bulk due to the above overlapping of the polymer chains and water held strongly to the monomers by electrostatic and/or hydrogen bonds. As there is likely to be overlap between these effects they may well be only partially or insignificantly additive. As above, the osmotic behavior of polyelectrolytes in water depends on the mass concentration relative to that concentration at which the molecules overlap in solution [1493]. Polyelectrolyte gels are may swell to a much greater extent (e.g. hydrogels) than neutral gels due to the presence of counter-ions increasing the osmotic pressure. The elasticity of the gel counteracts this by exerting pressure on the contained water.

 

Shows the area that polymers cannot penetrate

 

cartoon showing the area that polymers cannot penetrate
A different effect occurs is suspensions of inert particles in polymer solutions. It is found that such particles do not exert any osmotic pressure. However, the solution between them (see right) exerts a negative pressure that drives the particle together and destabilizes their suspension [2786]. This negative pressure causes an outward flow of water from the high activity polymer free volume between the inert particles, towards the lower activity polymer bulk solution, and consequently an attraction between these inert particles. The magnitude of this force depends on the product of the osmotic pressure and the cross-sectional area of the excluded volume. Effectively, the small access to biomolecules between the inert particles acts as a semipermeable membrane.

 

The same phenomenon applies to inert surfaces with narrow clefts and pores, such as the ZIF-8 material h that has great energy storage capacity (up to 30 MPa negative osmotic pressure in 2M NaCl) due to its sub-nanometric pores [2791].

 

Interfaces can also generate osmotic pressure without the requirement for dissolved solutes [1772, 2057].

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Osmotic potential

The osmotic potential (Ψπ) of pure water is defined to be zero (0 Pa), with solutions having negative values, in pressure units. Thus at low concentrations, Ψπ is given by the Van't Hoff equation, Ψπ = - MsRT. If a living cell is surrounded by a more concentrated solution (more negative osmotic potential), the cell (hypotonic) will tend to lose water to the surrounding environment whereas if the living cell is surrounded by a less concentrated solution (less negative osmotic potential), the cell (hypertonic) will tend to gain water from the surrounding environment; water flowing from higher osmotic potential to lower osmotic potential. In osmosis, water molecules move down the water potential gradient, from a high water potential to a lower water potential. Water moves from the ground surrounding trees to their upper branches in response to differences in the osmotic potential between the roots and the leaves, where water evaporates (transpiration [2434]) to increase solute concentration and decrease water potential. The maximum height that a tree (122-130 m) can grow depends on the maximum water potential (~2 MPa) that can be generated in the leaves compatible with retaining the water within the leaf cells [2246].

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Footnotes

a An osmotic pressure is a physical quantity dependent only on the concentration and temperature of the solution. Osmotic pressure can also apply to gases [2100]. [Back]

 

b Thus it is the mole fraction of water that is important, not the water concentration by itself. [Back]

 

c Similar derivations hold for the osmotic pressure in liquids other than water. [Back]

 

d The energy change occurring over a small change (dx) in the mole fraction of water (xw) is RTdx/xw. Therefore the total energy change going from pure water (xw= 1) to this new value (xw) is RT times the integral dx of 1/xw = RTLn(xw/1) = RTLn(xw). [Back]

 

e The osmotic properties of carbohydrate aqueous solutions from vapor pressure determinations have been described [2556]. [Back]

 

f This Van't Hoff equation for the osmotic pressure (Π = MsRT) has the same algebraic form as the Ideal Gas Law (PV = nRT) as n/V = Ms. Thus the (ideal) osmotic pressure of a solute behaves as though it is alone as an (ideal) gas within the space occupied by the volume of the solution. As first stated by Van't Hoff in 1892 however, this conceptual picture may mislead. [Back]

 

g Jacobus Henricus van't Hoff, Jr. (30 August 1852 - 1 March 1911) was a Dutch chemist and the first winner of the Nobel Prize in Chemistry (1901), partially for this work. [Back]

 

h Zeolitic imidazolate frameworks (ZIFs) are topologically isomorphic with zeolites, but with the tetrahedrally-coordinated transition metal ions connected by imidazolate linkers rather than silica. [Back]

 

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This page was established in 2006 and last updated by Martin Chaplin on 8 November, 2017


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