General Chemistry 2 • Equilibrium

Temperature Changes on Equilibrium — Predict effects of temperature change using ΔH information

How enthalpy data allows you to predict which direction a reaction shifts when the temperature rises or falls.

An atom with laboratory flask and electron orbit for General Chemistry 2
Inside this lesson 10 sections 5 questions 8 figures

SECTION 1

Historical Context & Motivation

The idea that chemical reactions can reach a state of balance — where forward and reverse processes occur at equal rates — took shape gradually over the nineteenth century. Early industrial chemists noticed that yields of important products such as ammonia and sulfuric acid depended critically on the temperature at which reactors operated, yet they lacked a theoretical framework to explain why. The question of how temperature shifts a reaction's position of equilibrium motivated some of the most foundational work in physical chemistry.

1864 • Law of Mass Action

Cato Guldberg and Peter Waage formulated the law of mass action, providing the first quantitative relationship between concentrations and the position of equilibrium. Their work established the concept of an equilibrium constant (K).

1884 • Le Châtelier's Principle

Henri Louis Le Châtelier published his principle stating that a system at equilibrium responds to a stress by shifting in the direction that partially counteracts that stress. This qualitative rule gave chemists a powerful predictive tool for temperature, pressure, and concentration changes.

1889 • Arrhenius Equation

Svante Arrhenius quantified the relationship between temperature and reaction rate constants, providing the kinetic underpinning for why equilibrium constants depend on temperature.

1901 • Van 't Hoff Equation

Jacobus Henricus van 't Hoff derived the equation relating the temperature dependence of K to the standard enthalpy change (ΔH°). He was awarded the first Nobel Prize in Chemistry partly for this thermodynamic work, which linked Le Châtelier's qualitative insight to rigorous mathematics.

1913 • Haber Process Optimization

Fritz Haber and Carl Bosch applied these equilibrium principles to optimize ammonia synthesis (N₂ + 3 H₂ ⇌ 2 NH₃, ΔH° < 0), choosing moderate temperatures that balanced thermodynamic favorability with kinetic feasibility — a landmark application of temperature–equilibrium theory.

The central question this lesson addresses is deceptively simple: if you know the sign and magnitude of ΔH for a reaction, can you predict how a change in temperature will shift the equilibrium position and alter the equilibrium constant K? The answer, rooted in the interplay between enthalpy, entropy, and free energy, is unequivocally yes — and the reasoning connects Le Châtelier's qualitative principle with the quantitative van 't Hoff equation.

SECTION 2

Core Principles & Definitions

To predict how temperature affects equilibrium, you need to connect three ideas: the nature of the equilibrium constant, the role of enthalpy as a "heat term" in a reaction, and Le Châtelier's principle applied specifically to thermal stress. These ideas work together to form a coherent, predictive framework.

1

Equilibrium Constant K

The thermodynamic equilibrium constant K is a dimensionless quantity fixed at a given temperature. It equals the ratio of product activities to reactant activities, each raised to their stoichiometric coefficients. K changes only when temperature changes — it is unaffected by concentration or pressure perturbations.
2

Enthalpy of Reaction (ΔH)

The standard enthalpy change ΔH° tells you whether a reaction is exothermic (ΔH° < 0, releases heat) or endothermic (ΔH° > 0, absorbs heat). You can conceptually treat heat as a pseudo-reactant or pseudo-product in the balanced equation to reason about temperature effects.
3

Le Châtelier's Principle for Temperature

When temperature increases, the equilibrium shifts in the endothermic direction (the direction that absorbs the added heat). When temperature decreases, it shifts in the exothermic direction. Unlike concentration or pressure changes, a temperature change actually alters the value of K.
4

Exothermic vs. Endothermic Shifts

For an exothermic forward reaction (ΔH° < 0), increasing T shifts equilibrium toward reactants and K decreases. For an endothermic forward reaction (ΔH° > 0), increasing T shifts equilibrium toward products and K increases.
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KEY TAKEAWAY

Think of temperature as a dial that selectively speeds up the reaction that absorbs heat. Imagine a two-lane highway where eastbound traffic represents the forward reaction and westbound traffic represents the reverse. Raising the temperature is like widening whichever lane corresponds to the endothermic direction — more "traffic" (molecular flux) flows that way, and the equilibrium position shifts accordingly. The key insight is that heat is effectively a reactant in endothermic reactions and a product in exothermic reactions, so adding or removing heat is analogous to adding or removing a chemical species.

SECTION 3

Visual Explanation — Heat as a Reactant or Product

The following diagram illustrates the central conceptual framework for predicting temperature effects on equilibrium. By writing heat explicitly in the balanced equation, you can apply Le Châtelier's principle in exactly the same way you would for a concentration change. Study the two scenarios — exothermic and endothermic — and note how the direction of the shift follows logically from the position of "heat" in each equation.

Temperature Effects on Equilibrium: Two ScenariosEXOTHERMIC REACTION (ΔH° < 0)A + B ⇌ C + D + heat↑ Temperature (add heat):Shift LEFT → K decreases↓ Temperature (remove heat):Shift RIGHT → K increasesENERGY DIAGRAMEnergyReactantsProductsΔH < 0ENDOTHERMIC REACTION (ΔH° > 0)heat + A + B ⇌ C + D↑ Temperature (add heat):Shift RIGHT → K increases↓ Temperature (remove heat):Shift LEFT → K decreasesENERGY DIAGRAMEnergyReactantsProductsΔH > 0Heat written explicitly shows which side of the equation is favored when T changes.
This diagram contrasts the two fundamental cases. In the exothermic case (top), heat appears on the product side; raising T shifts equilibrium to the left. In the endothermic case (bottom), heat appears on the reactant side; raising T shifts equilibrium to the right. The small energy-level sketches reinforce the relative positions of reactant and product energies.

The diagram encodes a simple mnemonic that is worth committing to memory: raising the temperature always favors the endothermic direction. If the forward reaction is exothermic, the reverse reaction is endothermic, so raising T favors the reverse and K decreases. If the forward reaction is endothermic, raising T favors the forward reaction and K increases. The logic is entirely symmetric, and all you need to apply it is the sign of ΔH° and the direction of the temperature change.

SECTION 4

Mathematical Framework — The Van 't Hoff Equation

Le Châtelier's principle gives qualitative predictions — the direction of the shift — but chemistry often demands quantitative answers. How much does K change when temperature changes from T₁ to T₂? The van 't Hoff equation provides exactly this, connecting the temperature dependence of the equilibrium constant to the standard enthalpy of reaction.

VAN 'T HOFF EQUATION (DIFFERENTIAL FORM)

d(lnK)/dT=ΔH°/(RT2)d(ln K) / dT = ΔH° / (R T²)

K = thermodynamic equilibrium constant; T = absolute temperature (K); R = gas constant (8.314 J·mol⁻¹·K⁻¹); ΔH° = standard enthalpy of reaction (J·mol⁻¹). This form shows that when ΔH° > 0, ln K increases with T (K rises), and when ΔH° < 0, ln K decreases with T (K falls).

For practical calculations, we integrate the differential form assuming ΔH° is approximately constant over the temperature range of interest. This assumption is valid when the temperature interval is not too large and heat capacity changes are small.

INTEGRATED VAN 'T HOFF EQUATION

ln(K2/K1)=−(ΔH°/R)×(1/T2−1/T1)ln(K₂ / K₁) = −(ΔH° / R) × (1/T₂ − 1/T₁)

K₁ = equilibrium constant at temperature T₁; K₂ = equilibrium constant at temperature T₂. This equation allows you to calculate K at a new temperature given K at a known temperature and the standard enthalpy of reaction. Note the negative sign in front of ΔH°/R.

CONNECTION TO GIBBS FREE ENERGY

ΔG°=−RTlnK=ΔH°−TΔS°ΔG° = −RT ln K = ΔH° − TΔS°

This fundamental relationship shows why K depends on temperature. As T increases, the −TΔS° term grows in magnitude. For an endothermic reaction (ΔH° > 0) with positive ΔS°, increasing T makes ΔG° more negative, which means K increases. The van 't Hoff equation is derived directly from this thermodynamic identity.

⚠

Sign Convention Checkpoint

A common source of error is mishandling the negative sign in the integrated van 't Hoff equation. When ΔH° is negative (exothermic) and T₂ > T₁, the quantity (1/T₂ − 1/T₁) is negative, so −(ΔH°/R) × (negative) yields a negative value for ln(K₂/K₁), meaning K₂ < K₁. This confirms the qualitative prediction: raising the temperature of an exothermic reaction decreases K.

SECTION 5

Detailed Breakdown — How K Varies with Temperature

The integrated van 't Hoff equation predicts that a plot of ln K versus 1/T yields a straight line with slope −ΔH°/R. This graphical relationship, sometimes called the van 't Hoff plot, is one of the most important tools in chemical thermodynamics. The sign of the slope immediately tells you whether the forward reaction is exothermic or endothermic, and the magnitude gives ΔH°. The following diagram illustrates both cases.

Van 't Hoff Plot: ln K vs 1/T1/T (K⁻¹) →ln K →high 1/T = low Tlow 1/T = high TExothermic(ΔH° < 0)slope = +|ΔH°|/R(positive slope)Endothermic(ΔH° > 0)slope = −|ΔH°|/R(negative slope)ln(K₂/K₁) = −(ΔH°/R)(1/T₂ − 1/T₁)slope = −ΔH°/Ry-intercept ≈ ΔS°/RMoving left along the x-axis corresponds to increasing temperature.
The van 't Hoff plot reveals the sign of ΔH° directly from the slope. The red line (exothermic) has a positive slope (−ΔH°/R is positive when ΔH° < 0), meaning ln K increases as 1/T increases — i.e., K is larger at lower temperatures. The cyan line (endothermic) has a negative slope, meaning K is larger at higher temperatures. Remember that moving leftward along the x-axis corresponds to higher T.
Reaction TypeSign of ΔH°Effect of ↑ T on KEquilibrium Shift
ExothermicΔH° < 0K decreasesShifts toward reactants (left)
EndothermicΔH° > 0K increasesShifts toward products (right)
ExothermicΔH° < 0K increasesShifts toward products (right) when T ↓
EndothermicΔH° > 0K decreasesShifts toward reactants (left) when T ↓

Summary of temperature effects on K for exothermic and endothermic reactions

SECTION 6

Worked Example — Calculating K at a New Temperature

Consider the industrial synthesis of ammonia: N₂(g) + 3 H₂(g) ⇌ 2 NH₃(g), with ΔH° = −92.2 kJ·mol⁻¹. At 298 K the equilibrium constant is K₁ = 6.0 × 10⁵. What is K at 500 K?

Finding K₂ for Ammonia Synthesis at 500 K

  1. 1

    Step 1 — Identify Given Values

    We have: K₁ = 6.0 × 10⁵ at T₁ = 298 K; ΔH° = −92.2 kJ·mol⁻¹ = −92 200 J·mol⁻¹; T₂ = 500 K; R = 8.314 J·mol⁻¹·K⁻¹. We need to find K₂.
    ΔH° = −92 200 J·mol⁻¹, T₁ = 298 K, T₂ = 500 K
  2. 2

    Step 2 — Write the Integrated Van 't Hoff Equation

    ln(K₂ / K₁) = −(ΔH° / R) × (1/T₂ − 1/T₁). We substitute our known values into this expression.
  3. 3

    Step 3 — Calculate the Temperature Reciprocal Term

    1/T₂ − 1/T₁ = 1/500 − 1/298 = 0.002000 − 0.003356 = −0.001356 K⁻¹.
    1/T₂ − 1/T₁ = −1.356 × 10⁻³ K⁻¹
  4. 4

    Step 4 — Calculate −ΔH°/R

    −ΔH° / R = −(−92 200) / 8.314 = +11 090 K. Note the double negative: ΔH° is negative, and the equation has a leading negative sign, so the product is positive.
    −ΔH°/R = +11 090 K
  5. 5

    Step 5 — Compute ln(K₂/K₁)

    ln(K₂ / K₁) = (11 090)(−1.356 × 10⁻³) = −15.04. The negative result confirms our qualitative prediction: because the reaction is exothermic, raising the temperature decreases K.
    ln(K₂/K₁) = −15.04
  6. 6

    Step 6 — Solve for K₂

    K₂ / K₁ = e⁻¹⁵·⁰⁴ = 3.25 × 10⁻⁷. Therefore K₂ = (6.0 × 10⁵)(3.25 × 10⁻⁷) ≈ 0.20. The equilibrium constant has dropped from 6.0 × 10⁵ at 298 K to approximately 0.20 at 500 K — a decrease of over six orders of magnitude, strongly favoring reactants at the higher temperature.
    K₂ ≈ 0.20 at 500 K
ℹ

Industrial Significance

This result explains a famous compromise in the Haber process. Thermodynamically, low temperatures favor ammonia production (larger K), but kinetically the reaction is too slow below about 400 °C. Industrial plants therefore operate at 400–500 °C with an iron catalyst, accepting a smaller K in exchange for a practical reaction rate. High pressure (150–300 atm) is used to further shift the equilibrium toward the product side, partially compensating for the unfavorable temperature effect.

SECTION 7

Strengths, Limitations, and Common Pitfalls

While the Le Châtelier approach and the van 't Hoff equation are powerful predictive tools, they come with assumptions and limitations that you should recognize to avoid errors on exams and in research.

StrengthsLimitations
Le Châtelier's principle gives quick, qualitative predictions requiring only the sign of ΔH°.Qualitative only — cannot tell you how much K changes without the van 't Hoff equation.
The integrated van 't Hoff equation gives quantitative K values at any temperature.Assumes ΔH° is constant over the temperature range. For large ΔT, heat capacity corrections (Kirchhoff's equation) are needed.
Van 't Hoff plots allow experimental determination of ΔH° from equilibrium data alone.Non-linearity in van 't Hoff plots indicates temperature-dependent ΔH°, requiring more complex models.
The framework applies universally to all equilibria: chemical, phase, solubility, and complex-formation.Temperature affects K but says nothing about how fast equilibrium is re-established — kinetics must be considered separately.
Connects seamlessly to Gibbs free energy: ΔG° = −RT ln K = ΔH° − TΔS°.For reactions where ΔH° ≈ 0, the temperature effect on K is negligible and dominated by entropy considerations.

Strengths and limitations of Le Châtelier's principle and the van 't Hoff equation for temperature effects

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COMMON PITFALL

A frequent exam error is confusing a shift in equilibrium position with a change in K. When you add a reactant at constant temperature, Q < K and the system shifts right — but K itself does not change. Only a temperature change alters K. Think of K as the thermostat setting: adding more fuel (reactant) makes the fire burn hotter temporarily, but the thermostat setting hasn't changed — only adjusting the thermostat (temperature) actually resets the target.

SECTION 8

Connection to Advanced Thermodynamic Theory

The van 't Hoff equation is a simplified form of a more general thermodynamic relationship. In advanced courses — particularly physical chemistry and chemical engineering thermodynamics — you will encounter extensions that account for the temperature dependence of ΔH° itself, non-ideal behavior, and multi-component phase equilibria.

Concept (This Course)Advanced Extension
ΔH° assumed constant over T₁ to T₂Kirchhoff's equation: dΔH°/dT = ΔCₚ°, leading to a temperature-dependent ΔH° in the van 't Hoff integration
K expressed as Kₚ or Kc using ideal-gas or ideal-solution assumptionsThermodynamic K expressed in terms of fugacities or activities, accounting for non-ideal behavior via fugacity coefficients or activity coefficients
Qualitative Le Châtelier prediction of shift directionQuantitative Gibbs energy minimization using Lagrange multipliers, especially for multi-reaction systems
Van 't Hoff plot as a straight lineCurved van 't Hoff plots analyzed with polynomial ΔH°(T) models or the Clarke–Glew equation
ΔG° = ΔH° − TΔS° at a single temperatureEllingham diagrams plotting ΔG° vs. T for metallurgical and materials applications

Comparison of general chemistry and advanced thermodynamic treatments of temperature–equilibrium relationships

Even at the general chemistry level, recognizing these connections is valuable. The Gibbs–Helmholtz equation, ∂(ΔG°/T)/∂T = −ΔH°/T², is the parent equation from which the van 't Hoff equation is derived. When you substitute ΔG° = −RT ln K and differentiate, the van 't Hoff equation falls out directly. This derivation reinforces a key message: the equilibrium constant is ultimately governed by the balance of enthalpic and entropic contributions to the free energy, and temperature determines the relative weight of these two terms.

SECTION 9

Practice Problems

Question 1: CONCEPTUAL

The dissolution of ammonium nitrate in water is endothermic (ΔH° > 0): NH₄NO₃(s) → NH₄⁺(aq) + NO₃⁻(aq). If you increase the temperature of the water, will more or less ammonium nitrate dissolve at equilibrium? Explain your reasoning using Le Châtelier's principle.
Show answer
More ammonium nitrate will dissolve. Because the dissolution process is endothermic, heat can be treated as a "reactant": heat + NH₄NO₃(s) ⇌ NH₄⁺(aq) + NO₃⁻(aq). Increasing the temperature adds heat to the system, and by Le Châtelier's principle the equilibrium shifts in the direction that consumes the added heat — the forward (dissolution) direction. The equilibrium constant Kₛₚ increases with temperature, meaning the solubility increases. This is consistent with the general observation that the solubility of most salts increases with temperature when dissolution is endothermic.

Question 2: BASIC CALCULATION

For the reaction 2 SO₂(g) + O₂(g) ⇌ 2 SO₃(g), ΔH° = −198 kJ·mol⁻¹ and K = 4.0 × 10²⁴ at 298 K. Determine whether K at 500 K will be larger or smaller than 4.0 × 10²⁴, and calculate ln(K₂/K₁) using the integrated van 't Hoff equation.
Show answer
K will be smaller at 500 K because the forward reaction is exothermic (ΔH° < 0), and raising T favors the reverse (endothermic) direction. Using ln(K₂/K₁) = −(ΔH°/R)(1/T₂ − 1/T₁): 1/T₂ − 1/T₁ = 1/500 − 1/298 = −1.356 × 10⁻³ K⁻¹. −ΔH°/R = −(−198 000)/8.314 = +23 810 K. ln(K₂/K₁) = (23 810)(−1.356 × 10⁻³) = −32.3. This very large negative value means K₂/K₁ = e⁻³²·³ ≈ 9.2 × 10⁻¹⁵, confirming that K drops dramatically. K₂ ≈ (4.0 × 10²⁴)(9.2 × 10⁻¹⁵) ≈ 3.7 × 10¹⁰ — still large but many orders of magnitude smaller than at 298 K.

Question 3: INTERMEDIATE

The water–gas shift reaction is CO(g) + H₂O(g) ⇌ CO₂(g) + H₂(g), with ΔH° = −41.2 kJ·mol⁻¹. At 700 K, K = 8.68. (a) Calculate K at 1000 K. (b) At which temperature is the yield of H₂ higher? Explain.
Show answer
(a) Using the integrated van 't Hoff equation: 1/T₂ − 1/T₁ = 1/1000 − 1/700 = 0.001000 − 0.001429 = −4.286 × 10⁻⁴ K⁻¹. −ΔH°/R = −(−41 200)/8.314 = 4955 K. ln(K₂/K₁) = (4955)(−4.286 × 10⁻⁴) = −2.124. K₂/K₁ = e⁻²·¹²⁴ = 0.1195. K₂ = 8.68 × 0.1195 = 1.04. (b) The yield of H₂ is higher at 700 K because K is larger (8.68 vs. 1.04), meaning the equilibrium lies further to the product side. Since the forward reaction is exothermic, lowering the temperature from 1000 K to 700 K increases K and favors product formation. In industrial hydrogen production, this trade-off between equilibrium yield and reaction kinetics is addressed using catalysts that enable acceptable rates at moderate temperatures.

Question 4: APPLIED

A biochemist measures the equilibrium constant for a protein-folding reaction at two temperatures: K = 12.5 at 25 °C and K = 3.8 at 37 °C. (a) Determine ΔH° for the folding reaction, assuming it is approximately constant over this range. (b) Is folding exothermic or endothermic? (c) Predict what happens to the protein at 50 °C.
Show answer
(a) T₁ = 298 K, K₁ = 12.5; T₂ = 310 K, K₂ = 3.8. ln(K₂/K₁) = ln(3.8/12.5) = ln(0.304) = −1.190. 1/T₂ − 1/T₁ = 1/310 − 1/298 = 3.226 × 10⁻³ − 3.356 × 10⁻³ = −1.299 × 10⁻⁴ K⁻¹. ΔH° = −R × ln(K₂/K₁) / (1/T₂ − 1/T₁) = −8.314 × (−1.190) / (−1.299 × 10⁻⁴) = −76 100 J·mol⁻¹ = −76.1 kJ·mol⁻¹. (b) ΔH° is negative, so folding is exothermic. This makes physical sense: folding typically involves forming favorable intramolecular contacts (hydrogen bonds, van der Waals interactions) that release energy. (c) At 50 °C (323 K), K will decrease further because raising the temperature of an exothermic reaction shifts equilibrium toward the unfolded (reactant) state. This is consistent with thermal denaturation — proteins tend to unfold at elevated temperatures.

Question 5: CRITICAL THINKING

Consider a reaction with ΔH° = +50 kJ·mol⁻¹ and ΔS° = +150 J·mol⁻¹·K⁻¹. (a) At what temperature does K = 1? (b) Sketch qualitatively how ln K varies with 1/T, and identify the regions where K > 1 and K < 1. (c) Explain physically why the reaction becomes spontaneous above a certain temperature despite being endothermic, connecting your answer to the interplay of ΔH° and TΔS°.
Show answer
(a) K = 1 when ΔG° = 0, which occurs when ΔH° = TΔS°. T = ΔH°/ΔS° = 50 000/150 = 333 K (60 °C). (b) Since ΔH° > 0, the van 't Hoff plot has a negative slope (slope = −ΔH°/R < 0). At 1/T = 1/333 = 3.00 × 10⁻³ K⁻¹, ln K = 0. For 1/T < 3.00 × 10⁻³ (T > 333 K), ln K > 0 so K > 1 — products are favored. For 1/T > 3.00 × 10⁻³ (T < 333 K), ln K < 0 so K < 1 — reactants are favored. (c) Although the reaction is endothermic (unfavorable enthalpy), it has a large positive ΔS° (favorable entropy). At low temperatures, the −TΔS° term is not large enough to overcome the positive ΔH°, so ΔG° > 0 and K < 1. As temperature increases, the magnitude of −TΔS° grows linearly while ΔH° remains approximately constant. Above 333 K, −TΔS° exceeds ΔH° in magnitude, making ΔG° negative and K > 1. This entropy-driven behavior is common in processes like dissolution of certain salts, melting, and protein denaturation.

SUMMARY

Lesson Summary

Summary

Temperature is the only common stress that changes the value of the equilibrium constant K. By treating heat as a pseudo-reactant or pseudo-product, Le Châtelier's principle predicts that raising the temperature favors the endothermic direction (K increases for endothermic forward reactions; K decreases for exothermic forward reactions), while lowering the temperature favors the exothermic direction.

Quantitatively, the van 't Hoff equation — ln(K₂/K₁) = −(ΔH°/R)(1/T₂ − 1/T₁) — relates the change in K to the standard enthalpy of reaction ΔH° and the temperature change. A van 't Hoff plot (ln K vs. 1/T) yields a straight line whose slope is −ΔH°/R, providing both the sign and magnitude of ΔH° from experimental equilibrium data. The underlying thermodynamic connection — ΔG° = ΔH° − TΔS° = −RT ln K — reveals that temperature tunes the relative importance of enthalpy and entropy in determining the position of equilibrium.

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