Study Guide

Free Energy of Dissolution

AP Chemistry· AP Chemistry CED — Equilibrium· 14 min read

1. Core Definitions and Context★☆☆☆☆⏱ 2 min

Free energy of dissolution refers to the Gibbs free energy change that occurs when 1 mole of solute dissolves in a solvent at constant temperature and pressure. For AP Chemistry, standard state conditions are 1 atm pressure, 1 M solute concentration, and 298 K unless stated otherwise. The standard free energy of dissolution is denoted , while non-standard free energy change at non-standard concentrations is called .

This topic accounts for 7–9% of the total AP Chemistry exam weight, appearing in both multiple-choice and free-response sections. It bridges core thermodynamics and equilibrium, two central big ideas of the AP Chemistry curriculum.

2. Standard Free Energy and the $\Delta G^\circ$-$K_{sp}$ Relationship★★☆☆☆⏱ 4 min

Dissolution is a homogeneous equilibrium process, so the general relationship between standard Gibbs free energy change and the equilibrium constant applies directly. For the dissolution of a generic ionic solid :

MxAy(s)xMy+(aq)+yAx(aq)M_xA_y(s) \rightleftharpoons xM^{y+}(aq) + yA^{x-}(aq)

The equilibrium constant for this reaction is the solubility product constant . The core formula relating to is:

ΔGsoln=RTlnKsp\Delta G^\circ_{soln} = -RT \ln K_{sp}

Where , and is absolute temperature in Kelvin. This formula directly tells us solubility under standard conditions:

  • If , dissolution is spontaneous, so , and the compound is soluble.

  • If , dissolution is non-spontaneous under standard conditions, so , and the compound is sparingly soluble or insoluble.

  • At , , the boundary between soluble and insoluble behavior.

📐 Worked Example

The of lead(II) chloride () at 298 K is . Calculate for at this temperature, and classify it as soluble or insoluble under standard conditions.

  1. 1

    List given values:

    Ksp=1.6×105,T=298 K,R=0.008314 kJ/(mol\cdotpK)K_{sp} = 1.6 \times 10^{-5}, T = 298 \text{ K}, R = 0.008314 \text{ kJ/(mol·K)}
  2. 2

    Calculate :

    ln(1.6×105)=ln(1.6)+ln(105)0.47011.513=11.043\ln(1.6 \times 10^{-5}) = \ln(1.6) + \ln(10^{-5}) \approx 0.470 - 11.513 = -11.043
  3. 3

    Substitute into the formula:

    ΔGsoln=(0.008314)(298)(11.043)+27.4 kJ/mol\Delta G^\circ_{soln} = - (0.008314)(298)(-11.043) \approx +27.4 \text{ kJ/mol}
  4. 4

    Interpret the result: is positive, so dissolution is non-spontaneous under standard conditions, meaning is sparingly soluble.

3. Calculating $\Delta G^\circ_{soln}$ from $\Delta H^\circ$ and $\Delta S^\circ$, Temperature Dependence★★★☆☆⏱ 5 min

When is not provided, you can calculate using the fundamental Gibbs free energy relation:

ΔGsoln=ΔHsolnTΔSsoln\Delta G^\circ_{soln} = \Delta H^\circ_{soln} - T\Delta S^\circ_{soln}

Here, is the standard enthalpy change when 1 mole of solute dissolves, and is the standard entropy change of dissolution. This formula lets you quantitatively predict how solubility changes with temperature, a common AP exam question:

  • If is positive (endothermic dissolution), increasing makes more negative, increases, and solubility increases.

  • If is negative (exothermic dissolution), increasing makes more positive, decreases, and solubility decreases.

This matches Le Chatelier’s principle but gives a quantitative framework for calculations.

📐 Worked Example

The dissolution of ammonium nitrate is . At 298 K, and . Calculate at 298 K and 350 K, then predict how solubility changes with increasing temperature.

  1. 1

    Convert to kJ to match the units of :

    ΔSsoln=108.7/1000=0.1087 kJ/(mol\cdotpK)\Delta S^\circ_{soln} = 108.7 / 1000 = 0.1087 \text{ kJ/(mol·K)}
  2. 2

    Calculate at 298 K:

    ΔG=25.7(298)(0.1087)=25.732.4=6.7 kJ/mol\Delta G^\circ = 25.7 - (298)(0.1087) = 25.7 - 32.4 = -6.7 \text{ kJ/mol}
  3. 3

    Calculate at 350 K:

    ΔG=25.7(350)(0.1087)=25.738.0=12.3 kJ/mol\Delta G^\circ = 25.7 - (350)(0.1087) = 25.7 - 38.0 = -12.3 \text{ kJ/mol}
  4. 4

    Interpret the result: becomes more negative as temperature increases, so increases, meaning solubility increases with increasing temperature.

4. Non-Standard Free Energy and Classifying Solution Saturation★★★☆☆⏱ 5 min

When a solution is not at equilibrium (not saturated), we use the non-standard Gibbs free energy change of dissolution, which follows the general relation:

ΔGsoln=ΔGsoln+RTlnQ\Delta G_{soln} = \Delta G^\circ_{soln} + RT \ln Q

Where is the reaction quotient, calculated the same way as but using current ion concentrations instead of equilibrium concentrations. The sign of tells us which direction the reaction proceeds to reach equilibrium:

  • : Dissolution is spontaneous, so more solid will dissolve → solution is unsaturated ()

  • : System is at equilibrium, no net change → solution is saturated ()

  • : Precipitation (reverse reaction) is spontaneous, so ions will precipitate → solution is supersaturated ()

📐 Worked Example

For dissolution at 298 K, . A solution has and . Calculate and classify the solution.

  1. 1

    Write the expression for :

    Q=[Pb2+][Cl]2Q = [Pb^{2+}][Cl^-]^2
  2. 2

    Calculate :

    Q=(0.001)(0.001)2=1×109Q = (0.001)(0.001)^2 = 1 \times 10^{-9}
  3. 3

    Substitute into the formula:

    ΔGsoln=27.4+(0.008314)(298)(ln1×109)27.4+(2.478)(20.72)23.9 kJ/mol\Delta G_{soln} = 27.4 + (0.008314)(298)(\ln 1 \times 10^{-9}) \approx 27.4 + (2.478)(-20.72) \approx -23.9 \text{ kJ/mol}
  4. 4

    Interpret: is negative, so dissolution is spontaneous, meaning the solution is unsaturated.

✓ Quick check
  1. A student measures of silver sulfate () at 298 K as . What is the correct and solubility classification?

    • , soluble

    • , sparingly soluble

    • , sparingly soluble

    • , soluble

    Reveal answer
    1

    Since , is negative, so is positive (+28 kJ/mol), which corresponds to sparingly soluble.

5. Common Pitfalls

Wrong move:

Using instead of when calculating from

Why:

Students remember from gas law problems and use it by mistake, leading to a value that is 3 orders of magnitude incorrect

Correct move:

Always confirm the value of before starting: use (or ) for all Gibbs free energy calculations

Wrong move:

Forgetting to convert from J/(mol·K) to kJ/(mol·K) when calculating

Why:

is almost always reported in kJ/mol, while is reported in J/(mol·K), so leaving in J gives a value 1000x too large

Correct move:

As a first step, divide by 1000 to convert to kJ/(mol·K) before substituting into the formula

Wrong move:

Claiming a positive means the compound never dissolves in water

Why:

Students confuse standard with non-standard ; many sparingly soluble compounds dissolve to a small extent even if is positive

Correct move:

Interpret as telling you the equilibrium extent of dissolution: positive means , so only small amounts dissolve at equilibrium, not that no dissolution occurs

Wrong move:

Getting the sign of wrong when starting from (e.g., getting a negative for )

Why:

Students forget that of a number less than 1 is negative, so the two negative signs multiply to a positive

Correct move:

After calculating, always check your sign: always gives positive , always gives negative

Wrong move:

Claiming a positive means the solution is unsaturated

Why:

Students mix up the direction of spontaneity: positive means the reverse reaction (precipitation) is spontaneous

Correct move:

Always pair and : precipitation spontaneous supersaturated

Wrong move:

Using Celsius temperature instead of Kelvin in calculations

Why:

Students are used to Celsius for enthalpy problems where temperature differences are identical, but calculations require absolute temperature

Correct move:

Always convert any given Celsius temperature to Kelvin by adding 273 (acceptable for AP exams) before substituting into the formula

6. Quick Reference Cheatsheet

Category

Formula

Notes

Standard from

, in Kelvin. soluble, sparingly soluble

Standard from and

Convert from J/(mol·K) to kJ/(mol·K) before calculation. in Kelvin

Non-standard for dissolution

ion product = for

Unsaturated solution

,

Forward dissolution is spontaneous; more solid will dissolve

Saturated solution

,

System at equilibrium; no net change in concentration

Supersaturated solution

,

Reverse precipitation/crystallization is spontaneous

Temperature dependence of solubility

solubility increases with T; solubility decreases with T

What's Next

Free energy of dissolution bridges core thermodynamics and solubility equilibrium, and it is a prerequisite for multiple key topics that follow in AP Chemistry. Immediately after mastering this topic, you will move on to predicting precipitation reactions, where you compare and to determine if a precipitate forms when two solutions are mixed. Without understanding how relates to and for dissolution, you cannot correctly predict precipitation behavior, a common AP FRQ topic. This topic also feeds into the broader study of colligative properties, where free energy changes of dissolution drive boiling point elevation and freezing point depression, and into acid-base equilibrium, where the dissociation of weak acids and bases follows the same - relationship derived here.