Physical Chemistry 1 • Thermodynamic Foundations

Computing ΔG from ΔH & ΔS — Compute ΔG from ΔH and ΔS and temperature

Predicting spontaneity by combining enthalpy, entropy, and temperature into the Gibbs energy equation.

An atom with a chemistry flask and thermometer for physical chemistry fundamentals.
Inside this lesson 10 sections 5 questions 8 figures

SECTION 1

Historical Context & Motivation

The question of why certain chemical reactions proceed forward while others stall has occupied scientists for centuries. Early investigators like Antoine Lavoisier recognized that heat release often accompanies vigorous reactions, leading to the intuition that exothermic processes are inherently favored. However, this notion proved incomplete: endothermic processes—such as the dissolution of ammonium nitrate in water—occur spontaneously despite absorbing heat from the surroundings. The resolution of this puzzle required a new thermodynamic quantity that could account for both energy transfer and the dispersal of energy among microstates. The Gibbs free energy (G) emerged as precisely that quantity, synthesizing the first and second laws of thermodynamics into a single, powerful criterion for spontaneity at constant temperature and pressure.

1824 • Carnot's Heat Engine Analysis

Sadi Carnot published Réflexions sur la puissance motrice du feu, establishing that the efficiency of heat engines depends on temperature differences. This work laid the conceptual groundwork for entropy and the second law, though Carnot did not use those terms.

1850–1865 • Clausius Formalizes Entropy

Rudolf Clausius introduced the concept of entropy (S), defining it as dS = δqrev/T and articulating the second law: the entropy of an isolated system never decreases. This provided the missing piece for understanding why exothermicity alone cannot determine spontaneity.

1873–1878 • Gibbs Introduces the Free Energy Function

Josiah Willard Gibbs, in his landmark papers on heterogeneous equilibria, defined a thermodynamic potential now written as G = H − TS. By combining the enthalpy (H) and entropy (S) at a given temperature (T), Gibbs provided a criterion for spontaneity valid at constant T and P—conditions that describe most laboratory and biological processes.

1923 • Lewis and Randall Systematize Chemical Thermodynamics

Gilbert N. Lewis and Merle Randall published Thermodynamics and the Free Energy of Chemical Substances, which tabulated standard free energies of formation and made the Gibbs equation a routine tool for predicting reaction feasibility across chemistry.

Modern Era • Computational Thermochemistry

Today, density functional theory (DFT) and calorimetric databases allow researchers to compute ΔG for complex reactions, drug–receptor binding, and materials design. The Gibbs–Helmholtz equation underpins fields from metabolic engineering to atmospheric chemistry.

The central question that the Gibbs equation addresses is elegantly simple: given a process with known enthalpy change ΔH and entropy change ΔS, will it proceed spontaneously at temperature T? The answer hinges on the sign of ΔG = ΔH − TΔS, a relationship that balances the energetic favorability of a reaction against the degree to which energy is dispersed.

SECTION 2

Core Principles & Definitions

Before computing ΔG, one must have a firm grasp of its constituent quantities and the conditions under which the Gibbs equation applies. The equation ΔG = ΔH − TΔS is not a definition pulled from thin air; it derives directly from the combined first and second laws of thermodynamics for a process at constant temperature and pressure. Each term embodies a distinct physical concept, and their interplay determines the thermodynamic feasibility of any process.

1

Gibbs Free Energy (ΔG)

The maximum non-expansion work obtainable from a process at constant T and P. When ΔG < 0, the process is spontaneous (thermodynamically favorable); when ΔG > 0, it is nonspontaneous; and when ΔG = 0, the system is at equilibrium.
2

Enthalpy Change (ΔH)

The heat absorbed or released at constant pressure. ΔH < 0 (exothermic) tends to favor spontaneity because it lowers the system's energy, while ΔH > 0 (endothermic) opposes it. Enthalpy captures the energetic driving force.
3

Entropy Change (ΔS)

A measure of the change in the number of accessible microstates—colloquially, the 'dispersal' of energy and matter. ΔS > 0 (increasing disorder) favors spontaneity; ΔS < 0 opposes it. Entropy captures the probabilistic driving force.
4

Temperature (T in Kelvin)

Temperature acts as a weighting factor for the entropy term. At low T, the enthalpy term dominates; at high T, the TΔS term dominates. This is why some reactions become spontaneous only above a crossover temperature.
5

Constant T & P Condition

The Gibbs equation applies rigorously when temperature and pressure remain constant throughout the process. These are the conditions most relevant to bench chemistry, biochemistry, and atmospheric science. Under other constraints, alternative potentials (e.g., Helmholtz free energy A = U − TS) may be more appropriate.
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KEY TAKEAWAY

Think of ΔG as a tug-of-war between two teams. Team Enthalpy pulls toward lower energy (exothermic = favorable), while Team Entropy pulls toward greater dispersal (increasing disorder = favorable). Temperature is the referee who decides how loudly Entropy's voice is heard: at low temperatures, Enthalpy dominates the outcome; at high temperatures, Entropy's pull becomes overwhelming. A negative ΔG means the combined pull favors the products side.

SECTION 3

Visual Explanation — The Spontaneity Landscape

The four possible sign combinations of ΔH and ΔS generate four distinct regimes of spontaneity. This quadrant diagram is one of the most useful visualizations in chemical thermodynamics: it shows at a glance whether a reaction is always spontaneous, never spontaneous, or spontaneous only above or below a characteristic crossover temperature Tcrossover = ΔH/ΔS.

Spontaneity Quadrant Diagram: Sign Combinations of ΔH and ΔSΔS →+−ΔH −ΔH +ALWAYS SPONTANEOUSΔH < 0, ΔS > 0ΔG = (−) − T(+) < 0Both terms favor productsExample: Combustion of CH₄SPONTANEOUS AT LOW TΔH < 0, ΔS < 0ΔG = (−) − T(−)Enthalpy wins at low TExample: Freezing of H₂OSPONTANEOUS AT HIGH TΔH > 0, ΔS > 0ΔG = (+) − T(+)Entropy wins at high TExample: CaCO₃ decompositionNEVER SPONTANEOUSΔH > 0, ΔS < 0ΔG = (+) − T(−) > 0Both terms oppose productsExample: 3 O₂ → 2 O₃
The four quadrants show how the signs of ΔH and ΔS determine spontaneity. The top-right (green) quadrant is always spontaneous because both enthalpy and entropy favor the process. The bottom-left (red) quadrant is never spontaneous because both terms oppose it. The mixed-sign quadrants (amber and violet) depend on temperature: one is spontaneous at low T, the other at high T.

The diagram above captures a crucial insight: the temperature-dependent cases (amber and violet quadrants) possess a crossover temperature at which ΔG = 0, calculated as Tcrossover = ΔH/ΔS. Below this temperature the enthalpy term dominates; above it the TΔS term takes over. This crossover temperature often corresponds to a phase transition temperature (e.g., the boiling point or melting point of a substance under standard conditions), illustrating the deep connection between phase equilibria and the Gibbs equation.

SECTION 4

Mathematical Framework

The Gibbs free energy equation can be derived rigorously from the combined first and second laws. For a closed system undergoing a reversible process at constant T and P, the first law gives dU = δq − PdV. Defining enthalpy as H = U + PV, we obtain dH = δq at constant P. The second law requires that for any spontaneous process δq ≤ TdS (Clausius inequality). Combining these, dH ≤ TdS, which rearranges to dH − TdS ≤ 0, or equivalently d(H − TS) ≤ 0 at constant T. Since G ≡ H − TS, the criterion for spontaneity becomes dG ≤ 0 at constant T and P.

GIBBS FREE ENERGY EQUATION

ΔG=ΔH−TΔSΔG = ΔH − TΔS

Where ΔG = change in Gibbs free energy (J or kJ), ΔH = change in enthalpy (J or kJ), T = absolute temperature (K), ΔS = change in entropy (J/K or kJ/K). All quantities must use consistent units: if ΔH is in kJ, then ΔS must be in kJ/K (or convert J/K → kJ/K by dividing by 1000).

STANDARD-STATE GIBBS ENERGY CHANGE

ΔG°=ΔH°−TΔS°ΔG° = ΔH° − TΔS°

The superscript ° denotes standard-state conditions (1 bar, specified temperature—often 298.15 K). Standard values are tabulated and can be combined via Hess's law: ΔH° = ΣΔH°f(products) − ΣΔH°f(reactants), and similarly for ΔS°.

CROSSOVER (EQUILIBRIUM) TEMPERATURE

Tcrossover=ΔH/ΔST_crossover = ΔH / ΔS

At this temperature, ΔG = 0 and the system is at equilibrium. This equation is valid when ΔH and ΔS share the same sign. Above or below Tcrossover, the sign of ΔG flips, toggling spontaneity.

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Unit Consistency Warning

The most common source of error in ΔG calculations is a unit mismatch between ΔH and TΔS. Enthalpy changes are typically reported in kJ/mol, while entropy changes are often in J/(mol·K). Always convert ΔS from J/(mol·K) to kJ/(mol·K) by dividing by 1000 before substituting into ΔG = ΔH − TΔS, or convert ΔH to J/mol by multiplying by 1000.

It is worth emphasizing the assumptions embedded in the equation ΔG = ΔH − TΔS. First, temperature must be constant throughout the process—if T varies, one must integrate using the Gibbs–Helmholtz equation. Second, pressure must be constant (the Helmholtz energy A = U − TS is the analogous potential for constant T and V). Third, the equation as written assumes that ΔH and ΔS are approximately temperature-independent, which is valid over modest temperature ranges but breaks down when heat capacities change significantly.

SECTION 5

Detailed Breakdown — The Four Spontaneity Cases

Understanding the four cases arising from the sign combinations of ΔH and ΔS is essential for rapid qualitative predictions. The table below summarizes each case, provides the condition for spontaneity, and offers a physically intuitive example. After the table, a graphical depiction shows how ΔG varies linearly with temperature for each case, reinforcing the concept of the crossover temperature.

CaseΔHΔSSpontaneityExample
1< 0 (exothermic)> 0 (disorder increases)Always spontaneous (ΔG < 0 at all T)Combustion: CH₄ + 2O₂ → CO₂ + 2H₂O
2> 0 (endothermic)< 0 (disorder decreases)Never spontaneous (ΔG > 0 at all T)3 O₂(g) → 2 O₃(g)
3< 0 (exothermic)< 0 (disorder decreases)Spontaneous at low T (T < ΔH/ΔS)Freezing: H₂O(l) → H₂O(s)
4> 0 (endothermic)> 0 (disorder increases)Spontaneous at high T (T > ΔH/ΔS)CaCO₃(s) → CaO(s) + CO₂(g)

The four sign combinations of ΔH and ΔS and their spontaneity implications

ΔG vs. Temperature for Four Spontaneity CasesΔG (kJ/mol)Temperature (K)+−0Case 1ΔH<0, ΔS>0Case 2ΔH>0, ΔS<0Case 3ΔH<0, ΔS<0T_crossCase 4ΔH>0, ΔS>0T_cross
This graph plots ΔG as a function of temperature for each of the four cases. Case 1 (green) remains below zero at all temperatures because ΔG = (negative) − T(positive) only becomes more negative. Case 2 (red) stays above zero. Cases 3 (amber) and 4 (violet) cross the ΔG = 0 axis at Tcrossover, marked by filled circles.

Notice that all four lines are straight—this is because ΔG = ΔH − TΔS is a linear function of T when ΔH and ΔS are temperature-independent. The y-intercept of each line equals ΔH (the value of ΔG at 0 K), and the slope equals −ΔS. A positive ΔS gives a negative slope (ΔG decreases with T), while a negative ΔS gives a positive slope (ΔG increases with T). This graphical interpretation is invaluable for reasoning about how changing the temperature affects the thermodynamic feasibility of a process.

SECTION 6

Worked Example

Consider the thermal decomposition of calcium carbonate, a reaction of industrial importance in cement production:

CaCO3(s) → CaO(s) + CO2(g)

Given: ΔH° = +178.3 kJ/mol, ΔS° = +160.5 J/(mol·K). Determine (a) ΔG° at 298 K, (b) ΔG° at 1500 K, and (c) the crossover temperature.

Computing ΔG° for the Decomposition of CaCO₃

  1. 1

    Step 1 — Identify Given Values and Check Units

    We are given ΔH° = +178.3 kJ/mol and ΔS° = +160.5 J/(mol·K). Notice that ΔH is in kJ while ΔS is in J. We must convert ΔS to kJ/(mol·K): ΔS° = 160.5 J/(mol·K) × (1 kJ / 1000 J) = 0.1605 kJ/(mol·K). This step prevents the most common computational error in Gibbs energy calculations.
    ΔS° = 0.1605 kJ/(mol·K)
  2. 2

    Step 2 — Compute ΔG° at T = 298 K

    Substitute into ΔG° = ΔH° − TΔS°: ΔG° = 178.3 kJ/mol − (298 K)(0.1605 kJ/(mol·K)) = 178.3 − 47.8 = +130.5 kJ/mol. Since ΔG° > 0, the decomposition is nonspontaneous at 298 K under standard conditions. This is consistent with everyday experience: limestone does not decompose at room temperature.
    ΔG°(298 K) = +130.5 kJ/mol (nonspontaneous)
  3. 3

    Step 3 — Compute ΔG° at T = 1500 K

    ΔG° = 178.3 − (1500)(0.1605) = 178.3 − 240.8 = −62.5 kJ/mol. Now ΔG° < 0, indicating the reaction is spontaneous at 1500 K. At elevated temperatures, the positive TΔS term overwhelms the positive ΔH, driving the decomposition forward. This is why lime kilns operate at temperatures well above 1000 K.
    ΔG°(1500 K) = −62.5 kJ/mol (spontaneous)
  4. 4

    Step 4 — Determine the Crossover Temperature

    At the crossover temperature, ΔG° = 0, so ΔH° = TΔS°. Solving: Tcrossover = ΔH°/ΔS° = 178.3 kJ/mol ÷ 0.1605 kJ/(mol·K) = 1111 K (≈ 838 °C). Above this temperature the reaction is spontaneous; below it, nonspontaneous. This corresponds well with the known decomposition temperature of CaCO₃ in industrial practice.
    T_crossover = 1111 K (838 °C)
  5. 5

    Step 5 — Interpret the Results

    This example illustrates Case 4 from our classification: ΔH > 0 and ΔS > 0 (an endothermic reaction that increases disorder via gas production). The reaction requires high temperatures for the entropy term TΔS to dominate. Note that our assumption of temperature-independent ΔH and ΔS introduces modest error at 1500 K; for precise engineering calculations, one would incorporate heat capacity corrections using ΔCp data via Kirchhoff's equations.

SECTION 7

Strengths, Limitations & Common Pitfalls

The Gibbs equation ΔG = ΔH − TΔS is among the most widely used relationships in physical chemistry, but its power comes with important caveats. Understanding where the equation excels and where it breaks down is essential for applying it correctly across diverse chemical contexts.

StrengthsLimitations
Provides a single criterion (sign of ΔG) for spontaneity at constant T and P—no need to separately track system and surroundings entropy.Assumes constant temperature and pressure; inapplicable to adiabatic explosions, shock waves, or rapid combustion where T changes dramatically during the process.
Uses readily available tabulated data (ΔH°_f, S° values) enabling rapid calculations for a vast range of reactions.Standard values are typically tabulated at 298 K; extrapolation to other temperatures requires heat capacity corrections (Kirchhoff's equation) that are often neglected.
Connects directly to equilibrium constants via ΔG° = −RT ln K, bridging thermodynamics and equilibrium analysis.Predicts thermodynamic feasibility only—says nothing about kinetics. A reaction with ΔG < 0 may still be infinitely slow without a catalyst (e.g., diamond → graphite).
Allows qualitative reasoning via the four-quadrant framework for quick assessments without detailed calculations.Treats ΔH and ΔS as temperature-independent, which can introduce significant error over large temperature ranges (ΔCpC_p ≠ 0).
Applicable to phase transitions, chemical reactions, biochemical processes, and electrochemistry (ΔG = −nFE).Does not apply to open systems exchanging matter with surroundings; the chemical potential μ must be used instead.

Strengths and limitations of the Gibbs equation ΔG = ΔH − TΔS

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KEY TAKEAWAY

The Gibbs equation is like a compass that tells you which direction a process will go, but it cannot tell you how fast you will get there. A negative ΔG guarantees that the thermodynamic driving force points toward products, but a kinetic barrier—analogous to a mountain range between you and your destination—can make the journey effectively impossible on practical timescales. Always pair thermodynamic analysis with kinetic considerations.

SECTION 8

Connection to Advanced Theory

The equation ΔG = ΔH − TΔS serves as a gateway to several advanced thermodynamic frameworks. Understanding how this foundational relationship extends into more sophisticated theory provides essential context for subsequent coursework in statistical mechanics, chemical kinetics, and electrochemistry.

Foundational ConceptAdvanced ExtensionKey Equation or Idea
ΔG° at a single temperatureTemperature dependence of ΔG° via the Gibbs–Helmholtz equation[∂(ΔG/T)/∂T]_P = −ΔH/T²
ΔG° = ΔH° − TΔS°ΔG° = −RT ln K (van't Hoff isotherm)Links free energy to the equilibrium constant K
Standard-state ΔG°Non-standard ΔG via the reaction quotient QΔG = ΔG° + RT ln Q
ΔG for chemical reactionsΔG for electrochemical cellsΔG = −nFE (Faraday's law connection)
Macroscopic ΔSStatistical mechanics interpretationS = kBk_B ln Ω (Boltzmann's entropy)

How ΔG = ΔH − TΔS connects to advanced thermodynamic relationships

The relationship ΔG° = −RT ln K is particularly powerful because it quantifies the position of equilibrium directly from thermodynamic data. If you know ΔH° and ΔS° at 298 K, you can compute ΔG° and then immediately determine K. The van't Hoff equation, d(ln K)/d(1/T) = −ΔH°/R, further reveals how K shifts with temperature—a direct consequence of the temperature dependence of ΔG. These extensions demonstrate that the simple equation ΔG = ΔH − TΔS is not merely a computational tool but the conceptual nucleus of chemical thermodynamics.

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Looking Ahead

In subsequent chapters, you will use the equation ΔG = ΔG° + RT ln Q to predict reaction direction under non-standard conditions, and you will explore how activity coefficients modify Q for non-ideal solutions. The temperature dependence of ΔH and ΔS via heat capacities—captured by Kirchhoff's equations—allows you to compute accurate ΔG values far from 298 K. Each of these extensions builds directly on the framework established in this lesson.

SECTION 9

Practice Problems

Question 1: CONCEPTUAL

A reaction has ΔH < 0 and ΔS < 0. Without performing a calculation, explain whether increasing the temperature will make the reaction more or less spontaneous. What physical significance does the crossover temperature Tcrossover have for this system?
Show answer
Increasing the temperature will make this reaction less spontaneous. With ΔS < 0, the −TΔS term becomes more positive as T rises, adding to ΔG and eventually making it positive. The crossover temperature Tcrossover = ΔH/ΔS is where ΔG = 0 and the system is at equilibrium. Below Tcrossover, the exothermic enthalpy term dominates, making the reaction spontaneous; above it, the unfavorable entropy term prevails, making it nonspontaneous. For example, freezing water is spontaneous below 273 K but not above it—273 K is the crossover temperature for the liquid-to-solid phase transition at 1 atm.

Question 2: BASIC CALCULATION

For a certain reaction, ΔH° = −92.2 kJ/mol and ΔS° = −198.7 J/(mol·K). Calculate ΔG° at 298 K and determine whether the reaction is spontaneous under standard conditions.
Show answer
First, convert ΔS° to kJ/(mol·K): ΔS° = −198.7 / 1000 = −0.1987 kJ/(mol·K). Then apply ΔG° = ΔH° − TΔS° = −92.2 − (298)(−0.1987) = −92.2 + 59.2 = −33.0 kJ/mol. Since ΔG° = −33.0 kJ/mol < 0, the reaction is spontaneous at 298 K under standard conditions. Note that both ΔH and ΔS are negative, placing this in the 'spontaneous at low T' category. The crossover temperature would be T = −92.2 / −0.1987 ≈ 464 K; above this temperature, the reaction becomes nonspontaneous.

Question 3: INTERMEDIATE

The synthesis of ammonia is given by N₂(g) + 3 H₂(g) → 2 NH₃(g). Using ΔH° = −92.4 kJ/mol and ΔS° = −198.4 J/(mol·K), calculate (a) ΔG° at 298 K, (b) ΔG° at 800 K, and (c) the temperature at which the reaction is at equilibrium under standard conditions. Discuss the implications for industrial ammonia production.
Show answer
(a) Convert ΔS° = −0.1984 kJ/(mol·K). ΔG°(298) = −92.4 − (298)(−0.1984) = −92.4 + 59.1 = −33.3 kJ/mol (spontaneous). (b) ΔG°(800) = −92.4 − (800)(−0.1984) = −92.4 + 158.7 = +66.3 kJ/mol (nonspontaneous). (c) Tcrossover = 92.4 / 0.1984 = 466 K (193 °C). The Haber process operates at ~700–800 K (where ΔG° > 0) because high temperature is needed for adequate reaction rates; the thermodynamic penalty is offset by using high pressures (Le Chatelier's principle shifts equilibrium toward fewer moles of gas) and continuously removing NH₃. This beautifully illustrates that thermodynamic nonspontaneity under standard conditions does not preclude practical viability when process conditions are adjusted.

Question 4: APPLIED

In biological systems, the hydrolysis of ATP at 37 °C (310 K) and pH 7 yields ΔG°' ≈ −30.5 kJ/mol. If a coupled biosynthetic reaction requires ΔG = +18.0 kJ/mol, what is the overall ΔG when the two reactions are coupled? Is the coupled process spontaneous? How many moles of ATP would need to be hydrolyzed to drive a reaction requiring +75 kJ/mol?
Show answer
When reactions are coupled, their ΔG values are additive: ΔGtotal = (−30.5) + (+18.0) = −12.5 kJ/mol. Since the overall ΔG < 0, the coupled process is spontaneous. For the second part, we need n × (−30.5) + 75 < 0, giving n > 75/30.5 ≈ 2.46. Since n must be an integer, at least 3 moles of ATP must be hydrolyzed (ΔGtotal = 3(−30.5) + 75 = −91.5 + 75 = −16.5 kJ/mol). This principle of energetic coupling is central to bioenergetics: cells routinely use ATP hydrolysis to drive thermodynamically unfavorable biosynthetic reactions.

Question 5: CRITICAL THINKING

A student claims: 'If ΔG° for a reaction is positive, the reaction can never produce any products.' Critically evaluate this statement. In your analysis, distinguish between ΔG° and ΔG, reference the equation ΔG = ΔG° + RT ln Q, and explain what actually determines the direction a reaction proceeds at any given moment.
Show answer
The student's claim is incorrect. ΔG° is the free energy change when all species are at standard concentrations (1 M or 1 bar). A positive ΔG° means the equilibrium constant K < 1 (since ΔG° = −RT ln K), so products are not favored at equilibrium—but 'not favored' does not mean 'absent.' At equilibrium, both reactants and products coexist, with products present at lower concentrations than reactants. Furthermore, the reaction direction at any instant is governed by ΔG = ΔG° + RT ln Q, where Q is the reaction quotient. Even for a reaction with ΔG° > 0, if Q is very small (e.g., starting with pure reactants, Q → 0), then RT ln Q → −∞, making ΔG < 0 and driving the reaction forward until Q = K. Thus, every reaction proceeds forward to some extent from pure reactants. The student has conflated ΔG° (a fixed quantity at a given T) with ΔG (a composition-dependent quantity that determines instantaneous spontaneity).

SUMMARY

Lesson Summary

Summary

The Gibbs free energy equation ΔG = ΔH − TΔS unifies the enthalpy (energetic driving force) and entropy (dispersal driving force) into a single criterion for spontaneity at constant T and P. The temperature acts as a weighting factor for the entropy term: at low T, ΔH dominates; at high T, TΔS dominates. Four sign combinations of ΔH and ΔS produce four distinct spontaneity regimes, with temperature-dependent cases exhibiting a crossover temperature T = ΔH/ΔS where ΔG = 0 and the system is at equilibrium.

When performing calculations, always ensure unit consistency between ΔH (typically kJ/mol) and ΔS (typically J/(mol·K))—convert ΔS to kJ/(mol·K) by dividing by 1000. Remember that ΔG predicts thermodynamic feasibility but not kinetic rate. The Gibbs equation connects forward to the equilibrium constant via ΔG° = −RT ln K, to non-standard conditions via ΔG = ΔG° + RT ln Q, and to electrochemistry via ΔG = −nFE, making it the central hub of chemical thermodynamics.

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