Colligative Properties of Solutions | General Chemistry 2
Types of Solutions
Solution and solute:
- A solution is a homogeneous mixture where one or more substances (solutes) are uniformly dispersed in another substance (solvent). The solvent typically dictates the phase of the solution, and the particles in a solution are very small, typically less than 1 nanometer in size.
- A solute is the substance that is dissolved in the solvent. The amount of solute relative to the solvent determines the concentration of the solution.
In a saltwater solution:
- Salt (sodium chloride, NaCl) is the solute,
- Water (H2O) is the solvent.
The salt dissolves completely in the water, creating a homogeneous mixture where the salt particles are uniformly distributed at the molecular level.
Saturated, unsaturated, and supersaturated solutions:
- Saturated solution: A solution that contains the maximum amount of solute that can dissolve at a given temperature. Any additional solute added will not dissolve and will remain undissolved in the solution.
- Unsaturated solution: A solution that contains less solute than the maximum amount that can be dissolved at a given temperature. More solute can still be dissolved in the solvent.
- Supersaturated solution: A solution that contains more solute than the solvent can theoretically dissolve at a given temperature. This is an unstable state, and the excess solute can precipitate out of the solution if disturbed.
Colloids:
A colloid is a mixture of a solvent and suspended particles that are larger than those in a true solution but smaller than those in a suspension. The particles in a colloid range in size from 1 to 100 nanometers, making them larger than simple molecules but small enough to remain in suspension and not settle out.
- Hydrophilic colloids: Colloids in which the dispersed particles have an affinity for water. They are usually stable in aqueous solutions.
- Hydrophobic colloids: Colloids in which the dispersed particles do not have an affinity for water. They tend to aggregate and separate from the dispersion medium unless stabilized by surfactants.
Hydrophilic colloids: gelatin, starch.
Hydrophobic colloids: oil droplets in water.
Tyndall effect: This is the scattering of light by colloidal particles. It is a characteristic feature of colloids, where a beam of light passing through the colloid becomes visible due to the scattering by the dispersed particles.
The Solution Process
Steps in the solution process:
- Step 1 - Solute separation: The first step in the solution process involves breaking the intermolecular forces or ionic bonds within the solute. This step requires energy, known as the lattice energy in ionic compounds or the cohesive energy in molecular solutes. The energy required to separate the solute particles is always endothermic.
- Step 2 - Solvent separation: The solvent molecules must also be separated to create space for the solute particles. This step also requires energy and is endothermic. The solvent molecules must overcome their intermolecular forces, such as hydrogen bonding in water, to make room for the solute.
- Step 3 - Solvation (or hydration in water): The final step involves the interaction between solute particles and solvent molecules. Solvent molecules surround the solute particles, stabilizing them in the solution. This step releases energy, making it an exothermic process.
Enthalpy of solution:
The overall enthalpy change of the solution process (ΔHsolution) depends on the balance of energy changes in the three steps:
ΔHsolution = ΔH1 + ΔH2 + ΔH3
ΔHsolution = overall enthalpy change of the solution process
ΔH1 = enthalpy change of the solute separation
ΔH2 = enthalpy change of the solvent separation
ΔH3 = enthalpy change of the solvation
- If ΔHsolution < 0: the dissolution process is exothermic, and the solution will release heat.
- If ΔHsolution > 0: the dissolution process is endothermic, and the solution will absorb heat.
Entropy (S) of the solution process:
The dissolution process often leads to an increase in entropy because the solute particles become more dispersed in the solvent. This increase in disorder usually drives the solution process forward, even if the enthalpy change is positive (endothermic).
Concentration Units
Molarity (M):
Molarity is defined as the number of moles of solute dissolved in one liter of solution:
M =
M = molarity (in mol.L-1)
nsolute = moles of solute (in mol)
Vsolution = volume of solution (in L)
Molality (m):
Molality is defined as the number of moles of solute dissolved in one kilogram of solvent:
m =
m = molality (in mol.kg-1)
nsolute = moles of solute (in mol)
msolution = mass of solvent (in kg)
Mass percent (w/w%):
Mass percent is the mass of the solute divided by the total mass of the solution, multiplied by 100:
w/w% = x 100
w/w% = mass percent
msolute = mass of solute (in kg)
msolution = mass of solution (in kg)
msolution = msolute + msolvent
Volume percent (v/v%):
Volume percent is the volume of the solute divided by the total volume of the solution, multiplied by 100:
% v/v = x 100
v/v% = volume percent
Vsolute = volume of solute (in L)
Vsolution = volume of solution (in L)
Mole fraction (χ):
Mole fraction is the ratio of the number of moles of a component to the total number of moles of all components in the solution:
χA =
χA = mole fraction of component A
nA = moles of component A (in mol)
ntot = total moles of all components (in mol)
Parts per million (ppm) and parts per billion (ppb):
These units are used to express very dilute concentrations of substances. Ppm is the number of parts of solute per million parts of the solution, and ppb is the number of parts of solute per billion parts of the solution.
ppm = x 106
ppm = parts per million
msolute = mass of solute (in kg)
msolution = mass of solution (in kg)
Factors Affecting Solubility
Effect of temperature:
- For most solid solutes, solubility increases as the temperature rises. The increased kinetic energy of the molecules at higher temperatures allows more solute particles to overcome the forces holding them in the solid state, thus dissolving in the solvent.
The solubility of sugar in water increases as the temperature is increased. This is why sugar dissolves more quickly in hot water compared to cold water.
- The solubility of gases in liquids typically decreases with an increase in temperature. Higher temperatures provide gas molecules with more energy, allowing them to escape from the solvent into the gas phase more easily.
Carbonated beverages, such as soda, lose carbonation more rapidly when they are warm because the solubility of carbon dioxide decreases as the temperature increases.
Effect of pressure:
Pressure significantly affects the solubility of gases in liquids. According to Henry's Law, the solubility of a gas in a liquid is directly proportional to the partial pressure of the gas above the liquid:
c = kH P
c = molar concentration or solubility (in mol.L-1)
kH = proportionality constant called the Henry's law constant
P = partial pressure of the gas above the liquid (in atm)
The Henry's Law constant varies depending on the gas and the solvent, and it typically decreases with increasing temperature. This constant quantifies how much gas will dissolve in the solvent under a given pressure.
Carbonated beverages are bottled under high pressure to increase the solubility of carbon dioxide in the liquid. When the bottle is opened, the pressure is released, reducing the solubility of CO2, which escapes as bubbles, causing the beverage to go flat.
Vapor-Pressure Lowering
Raoult's law:
Raoult's law states that the vapor pressure of a solvent in an ideal solution is directly proportional to the mole fraction of the solvent in the solution. This law is applicable to solutions where the solute does not volatilize and does not react with the solvent.
Psolution = χsolvent Posolvent
Psolution = vapor pressure of the solvent in the solution (in atm)
χsolvent = mole fraction of the solvent in the solution
Posolvent = vapor pressure of the pure solvent (in atm)
Vapor-pressure lowering:
When a non-volatile solute is added to a solvent, the solute particles occupy space at the surface of the liquid, reducing the number of solvent molecules that can escape into the vapor phase. As a result, the vapor pressure of the solvent above the solution is lower than that of the pure solvent.
The vapor-pressure lowering (ΔP) can be calculated as:
ΔP = Posolvent - Psolution
= Posolvent (1 - χsolvent)
ΔP = vapor-pressure lowering (in atm)
Posolvent = vapor pressure of the pure solvent (in atm)
Psolution = vapor pressure of the solvent in the solution (in atm)
χsolvent = mole fraction of the solvent in the solution
Alternatively, since χsolute + χsolvent = 1, we can express the vapor-pressure lowering as:
ΔP = Posolvent χsolute
ΔP = vapor-pressure lowering (in atm)
Posolvent = vapor pressure of the pure solvent (in atm)
χsolvent = mole fraction of the solute in the solution
Boiling-Point Elevation
Boiling-point elevation:
Boiling-point elevation (ΔTb) is the increase in the boiling point of a solvent upon the addition of a non-volatile solute. It is defined as the difference between the boiling point of the solution and the boiling point of the pure solvent:
ΔTb = Tb - Tob
ΔTb = boiling-point elevation (in oC)
Tb = boiling point of the solution (in oC)
Tob = boiling point of the pure solvent (in oC)
The change in boiling point is directly proportional to the molal concentration of the solute in the solution:
ΔTb = Kb m
ΔTb = boiling-point elevation (in oC)
Kb = molal boiling-point elevation constant (in oC.kg.mol-1)
m = molality of the solute (in mol.kg-1)
Mechanism:
- Lowered vapor pressure: The addition of a non-volatile solute decreases the solvent's vapor pressure because fewer solvent molecules can escape into the vapor phase. As a result, a higher temperature is required for the vapor pressure to equal atmospheric pressure, leading to a higher boiling point.
- Colligative property: Boiling-point elevation is a colligative property, meaning it depends on the number of solute particles in the solution, not the identity of the solute. This property is particularly useful for determining the molar mass of unknown solutes.
Freezing-Point Depression
Freezing-point depression:
Freezing-point depression (ΔTf) is the decrease in the freezing point of a solvent when a solute is dissolved in it. It is defined as the difference between the freezing point of the pure solvent and the freezing point of the solution:
ΔTf = Tof - Tf
ΔTf = freezing-point depression (in oC)
Tof = freezing point of the pure solvent (in oC)
Tf = freezing point of the solution (in oC)
This effect is proportional to the number of solute particles present in the solution, regardless of their identity:
ΔTf = - Kf x m
ΔTf = freezing-point depression (in oC)
Kf = molal freezing-point depression constant (in oC.mol.kg-1)
m = solution molality (in mol.kg-1)
Mechanism:
- Disruption of freezing: The presence of solute particles interferes with the ability of solvent molecules to arrange themselves into a solid crystalline structure. As a result, the temperature must be lowered further to reach the point where the solvent can solidify.
- Colligative property: Freezing-point depression is a colligative property, meaning it depends only on the number of solute particles in the solution and not on their chemical identity.
Osmotic Pressure
Semipermeable membrane:
A semipermeable membrane allows only certain molecules, such as solvent molecules, to pass through it while blocking solute particles. This differential permeability creates a natural movement of solvent from the region of lower solute concentration to the region of higher solute concentration.
Osmosis:
Osmosis is the process by which solvent molecules move across a semipermeable membrane from a dilute solution (or pure solvent) into a more concentrated solution. This movement continues until the concentrations on both sides of the membrane are equal, or until osmotic pressure is applied to stop the flow.
Osmotic pressure:
Osmotic pressure (Π) is the pressure that must be applied to a solution to prevent the inward flow of water (or another solvent) across a semipermeable membrane. It is directly proportional to the concentration of solute particles in the solution:
Π = M R T
Π = osmotic pressure (in atm)
M = molarity of the solution (in mol.L-1)
R = ideal gas constant = 0.0821 (in L.atm.K-1.mol-1)
T = absolute temperature (in K)
Osmotic pressure is a colligative property, meaning it depends on the number of solute particles in the solution, not their identity. The more solute particles present, the higher the osmotic pressure.
Electrolyte Solutions
Electrolytes:
Electrolytes are substances that, when dissolved in water or other solvents, dissociate into ions. These ions are responsible for conducting electricity in the solution. There are 2 types of electrolytes:
- Strong electrolytes: Completely dissociate into ions in solution, resulting in high electrical conductivity.
- Weak electrolytes: Partially dissociate into ions in solution, resulting in lower electrical conductivity.
- Sodium chloride (NaCl), potassium hydroxide (KOH), hydrochloric acid (HCl) are strong electrolytes.
- Acetic acid (CH₃COOH), ammonia (NH₃), weak organic acids, and bases are weak electrolytes.
Van 't Hoff factor (i):
The van 't Hoff factor represents the number of particles into which a solute dissociates in solution. It can be expressed as:
i =
i = van 't Hoff factor
nparticles = moles of particles in solution
nsolute = moles of solute dissolved
Thus, i is 1 for all nonelectrolytes, and greater than 1 for strong electrolytes.
i (Sucrose): 1; i (NaCl): 2; i (KBr): 2; i (CaCl2): 3; i (FeCl3): 4.
Colligative properties of electrolyte solutions:
Electrolyte solutions exhibit colligative properties such as boiling-point elevation, freezing-point depression, and osmotic pressure. The presence of more ions (as in strong electrolytes) amplifies these effects compared to nonelectrolyte solutions. The equations for colligative properties are modified as follows:
ΔTb = i Kb m
ΔTb = boiling-point elevation (in oC)
i = van't Hoff factor
Kb = molal boiling-point elevation constant (in oC.kg.mol-1)
m = molality of the solute (in mol.kg-1)
ΔTf = - i Kf x m
ΔTf = freezing-point depression (in oC)
i = van't Hoff factor
Kf = molal freezing-point depression constant (in oC.mol.kg-1)
m = solution molality (in mol.kg-1)
Π = i M R T
Π = osmotic pressure (in atm)
i = van't Hoff factor
M = molarity of the solution (in mol.L-1)
R = ideal gas constant = 0.0821 (in L.atm.K-1.mol-1)
T = absolute temperature (in K)
Check your knowledge about this Chapter
Colligative properties are physical properties of solutions that depend on the number of dissolved solute particles, rather than the type of particles. These properties include vapor-pressure lowering, boiling-point elevation, freezing-point depression, and osmotic pressure.
The impact of solute particles on these properties is directly related to the concentration of the particles; for example, adding more solute particles will further lower the vapor pressure and increase the boiling point and osmotic pressure of the solution, while also causing a greater decrease in the freezing point. These effects occur because the presence of solute particles disrupts the orderly process of solvent molecules entering the gas phase or forming a solid, thus altering the physical behavior of the solvent.
The solubility of a substance is significantly influenced by the chemical nature of both the solute (the substance being dissolved) and the solvent (the substance doing the dissolving).
According to the principle "like dissolves like," polar solvents, such as water, are more effective at dissolving polar solutes or ionic compounds, because the solvent can effectively surround the solute particles and separate them into solution due to similar intermolecular forces. Nonpolar solvents, on the other hand, are better at dissolving nonpolar solutes, because the intermolecular forces between solute and solvent are similarly weak, allowing the solute to blend into the solvent with ease.
Additionally, specific solute-solvent interactions, such as hydrogen bonding and dipole-dipole interactions, can either enhance or reduce solubility depending on compatibility.
The role of intermolecular forces in the solution process is crucial for determining whether a substance will dissolve in a solvent. During solvation, solute particles must overcome their intermolecular forces to separate and disperse among the solvent molecules. In turn, the solvent molecules must overcome their intermolecular forces to accommodate the solute particles. Successful dissolution occurs when the solute-solvent interactions are strong enough to offset the energy required to break apart the solute and solvent's intermolecular attractions. Consequently, similar intermolecular forces between solute and solvent, such as hydrogen bonding or dipole-dipole interactions, often lead to better solubility.
To calculate the molality of a solution, you divide the number of moles of solute by the mass of the solvent in kilograms. The formula is:
m =
m = molality (in mol.kg-1)
nsolute = moles of solute (in mol)
msolution = mass of solvent (in kg)
Molality is preferred over molarity when dealing with temperature-dependent studies because molality is not affected by changes in temperature; it relies on mass, which does not change with temperature like volume. This distinction makes molality especially useful for colligative property calculations which are influenced by the amount of solute particles, not their concentration in volume.
Raoult's Law states that the vapor pressure of a volatile component in a solution is directly proportional to its mole fraction in the solution. This law indicates that the presence of a non-volatile solute lowers the vapor pressure of the solvent in a solution because the solute molecules occupy some of the surface area, reducing the number of solvent molecules that can escape into the vapor phase. As a result, the solution has a lower vapor pressure compared to the pure solvent, which is a phenomenon known as vapor-pressure lowering.
Ionic and polar solutes have a significant impact on vapor pressure because they dissociate in solution to form ions or interact strongly with the solvent molecules through dipole-dipole interactions, respectively. This strong solute-solvent interaction makes it more difficult for the solvent molecules to escape into the gas phase, which reduces the rate of evaporation. Consequently, the solution's vapor pressure, which depends on the number of solvent molecules in the gas phase, is lower than that of the pure solvent. Nonpolar solutes do not form such strong interactions with the solvent molecules and therefore have a less pronounced effect on the vapor pressure.
Boiling-point elevation occurs when a solute is dissolved in a solvent, causing the boiling point of the solution to be higher than that of the pure solvent. This phenomenon is due to the fact that the presence of solute particles lowers the solvent's vapor pressure, requiring a higher temperature to reach the vapor pressure necessary for boiling.
The quantitative determination of boiling-point elevation is described by the formula:
ΔTb = Kb m
ΔTb = boiling-point elevation (in oC)
Kb = molal boiling-point elevation constant (in oC.kg.mol-1)
m = molality of the solute (in mol.kg-1)
Freezing-point depression occurs when a solute is dissolved in a solvent, causing the freezing point of the solution to be lower than that of the pure solvent. This phenomenon happens because the presence of solute particles interferes with the formation of the solid lattice structure that is typical of the frozen solvent. As a result, additional energy (lower temperature) is required to solidify the solution.
Freezing-point depression is calculated using the formula:
ΔTf = - Kf x m
ΔTf = freezing-point depression (in oC)
Kf = molal freezing-point depression constant (in oC.mol.kg-1)
m = solution molality (in mol.kg-1)
Osmotic pressure is the pressure required to prevent the flow of solvent molecules through a semi-permeable membrane from a region of lower solute concentration to a region of higher solute concentration. It is a colligative property, meaning it is influenced by the number of solute particles in a solution rather than their identity.
The osmotic pressure is directly proportional to the molarity of the solute particles in the solution, according to the formula:
Π = M R T
Π = osmotic pressure (in atm)
M = molarity of the solution (in mol.L-1)
R = ideal gas constant = 0.0821 (in L.atm.K-1.mol-1)
T = absolute temperature (in K)
Therefore, increasing the concentration of solute particles increases the osmotic pressure.
The van't Hoff factor (i) quantifies the number of particles an electrolyte produces when dissolved in water. For colligative properties, which depend on the number of particles in solution (not their identity), the van't Hoff factor is crucial. Electrolytes that ionize completely have a van't Hoff factor greater than 1, amplifying colligative effects like boiling-point elevation and freezing-point depression. In contrast, nonelectrolytes have a factor of 1, as they do not produce additional particles.
The dissociation or association of solute molecules in solution can significantly affect colligative properties because these properties depend on the number of particles in solution, not their identity. When a solute dissociates into ions, the number of particles in the solution increases, which intensifies colligative effects such as boiling-point elevation and freezing-point depression. Conversely, when solute molecules associate, the number of particles decreases, diminishing the effect on colligative properties. So, the calculated effect on the colligative properties using the van't Hoff factor, which accounts for the actual number of particles formed from the solute, can offer a more precise understanding of these changes.