CHEMISTRY 2 • THERMOCHEMISTRY & THERMODYNAMICS

ΔG° & Equilibrium Constant — Relate ΔG° to equilibrium constant K

Discover how the sign and size of standard free energy change predict exactly where equilibrium lies.

Historical Context & Motivation

For centuries, chemists could observe that some reactions seem to go to completion while others appear to stall partway through. The question of why a reaction favors products or reactants at equilibrium required connecting two seemingly separate ideas: the energy changes that drive a reaction and the ratio of products to reactants at equilibrium. The bridge between these ideas is the equation that links standard Gibbs free energy change (ΔG°) to the equilibrium constant (K). Building this bridge took the combined insights of several brilliant scientists over more than a century.

1824
Carnot & Heat Engines
Sadi Carnot published his analysis of heat engines, laying the groundwork for the concept of entropy and the idea that not all energy is available to do useful work.
1865
Clausius Defines Entropy
Rudolf Clausius coined the term entropy (S) and formulated the Second Law of Thermodynamics, establishing that spontaneous processes increase the total entropy of the universe.
1876
Gibbs Free Energy Introduced
J. Willard Gibbs combined enthalpy (H) and entropy (S) into a single state function, G = H − TS, now called Gibbs free energy. This quantity predicts spontaneity at constant temperature and pressure.
1886
van 't Hoff Relates K to Temperature
Jacobus van 't Hoff showed how the equilibrium constant changes with temperature, earning the first Nobel Prize in Chemistry in 1901 and paving the way for the ΔG° = −RT ln K relationship.
1920s
The Modern Equation Emerges
By the early twentieth century, the relationship ΔG° = −RT ln K was firmly established in chemistry textbooks, unifying thermodynamics and chemical equilibrium into one powerful equation.

The central question this lesson addresses is deceptively simple: if you know how much free energy a reaction releases or absorbs under standard conditions, can you predict the equilibrium constant — and vice versa? The answer is yes, and the equation that connects them is one of the most powerful tools in all of chemistry.

Core Principles & Definitions

Before diving into the math, you need a clear understanding of the two quantities being connected. ΔG° (pronounced "delta G naught") is the standard Gibbs free energy change — the maximum non-expansion work a reaction can perform when all species are in their standard states (1 atm for gases, 1 M for solutions, and pure liquids or solids at 25 °C unless stated otherwise). Meanwhile, K is the equilibrium constant, the ratio of product concentrations (or pressures) to reactant concentrations (or pressures), each raised to its stoichiometric coefficient, measured when the system has reached equilibrium.

1

ΔG° — Standard Free Energy Change

The difference in Gibbs free energy between products and reactants when every substance is in its standard state. A negative ΔG° means the reaction is thermodynamically favorable (spontaneous) under standard conditions.
2

K — Equilibrium Constant

The ratio of product activities (concentrations or partial pressures) to reactant activities at equilibrium. When K > 1, products dominate; when K < 1, reactants dominate.
3

R — Universal Gas Constant

R = 8.314 J/(mol·K). This constant converts between energy units and the temperature-dependent entropy contribution in the equation ΔG° = −RT ln K.
4

T — Absolute Temperature

Temperature must always be in Kelvin (K = °C + 273.15). Since entropy effects scale with temperature, T acts as a multiplier that amplifies or dampens the entropy term.
5

ln K — Natural Logarithm of K

The natural logarithm (base e ≈ 2.718) of the equilibrium constant. Using ln rather than log₁₀ connects directly to the thermodynamic derivation; you can convert with ln K = 2.303 × log₁₀ K.
✦ KEY TAKEAWAY
Think of ΔG° as a hill and K as where a ball will settle. A large negative ΔG° is like a steep downhill slope — the ball (reaction) rolls far toward the product side, so K is large. A large positive ΔG° is an uphill climb — the ball barely moves forward, and K is very small. When ΔG° = 0, the landscape is flat, and K = 1; products and reactants are equally favored.

Visual Explanation — ΔG° and K Relationship

The straight line shows ΔG° = −RT ln K. When ln K is positive (K > 1), ΔG° is negative and the reaction is product-favored. When ln K is negative (K < 1), ΔG° is positive and reactants are favored. The yellow dot marks the crossover point where ΔG° = 0 and K = 1.

The diagram above captures the entire relationship in one picture. The diagonal line has a slope of −RT, which is always negative (since R and T are always positive). This means that as K increases, ΔG° decreases — a larger equilibrium constant corresponds to a more negative (more favorable) standard free energy change. Notice that the line passes through the point where ΔG° = 0 and ln K = 0 (K = 1). This is the dividing line: reactions with K > 1 have negative ΔG° and favor products, while reactions with K < 1 have positive ΔG° and favor reactants.

Mathematical Framework

The central equation of this lesson connects thermodynamics to equilibrium in a single, elegant formula. Let's break it down piece by piece, then look at alternate forms you may encounter.

MASTER EQUATION
ΔG° = −RT ln K
ΔG° = standard Gibbs free energy change (J/mol), R = 8.314 J/(mol·K), T = absolute temperature (K), ln K = natural logarithm of the equilibrium constant.

This equation tells you that ΔG° and K are two sides of the same coin. If you know one, you can calculate the other. Notice the negative sign: a positive ln K (meaning K > 1) gives a negative ΔG°, confirming that product-favored reactions are thermodynamically spontaneous under standard conditions.

SOLVING FOR K
K = e^(−ΔG° / RT)
Rearranged from the master equation. Raise e (≈ 2.718) to the power of −ΔG°/(RT). Make sure ΔG° is in joules, not kilojoules, before dividing by RT.
ALTERNATE FORM (BASE 10)
ΔG° = −2.303 RT log₁₀ K
Since ln K = 2.303 × log₁₀ K, you can use common logarithms instead. This form is convenient when your calculator gives log₁₀ more readily than ln.
⚠️ Unit Warning
The most common error is a unit mismatch. R = 8.314 J/(mol·K), so ΔG° must be in joules per mole when you plug into the equation. If your ΔG° is given in kJ/mol, multiply by 1000 first. Forgetting this step will give you an answer that is off by a factor of 1000 in the exponent — a catastrophic error.
GENERAL FREE ENERGY (NON-STANDARD CONDITIONS)
ΔG = ΔG° + RT ln Q
Q = reaction quotient (same form as K but using current, non-equilibrium concentrations). At equilibrium, Q = K and ΔG = 0, which directly gives ΔG° = −RT ln K.

The last equation above is actually where ΔG° = −RT ln K comes from. At equilibrium, the system has no remaining driving force to shift in either direction, so ΔG (not ΔG°) equals zero. Substituting ΔG = 0 and Q = K into ΔG = ΔG° + RT ln Q gives 0 = ΔG° + RT ln K, which rearranges to ΔG° = −RT ln K. This derivation shows that the master equation is not arbitrary — it is a direct consequence of the definition of equilibrium.

Detailed Breakdown — How ΔG° Maps to K

It is helpful to see concrete numbers that illustrate the sensitivity of K to ΔG°. Because K depends exponentially on ΔG°, even modest changes in free energy produce enormous changes in the equilibrium constant. The table below shows values at 298 K (25 °C).

ΔG° and K values at T = 298 K
ΔG° (kJ/mol)ln KK (approx.)Interpretation
−57.4+23.21.1 × 10¹⁰Essentially goes to completion
−17.1+6.9≈ 1000Strongly product-favored
−5.7+2.3≈ 10Moderately product-favored
001Neither side favored
+5.7−2.3≈ 0.1Moderately reactant-favored
+17.1−6.9≈ 0.001Strongly reactant-favored
+57.4−23.29.1 × 10⁻¹¹Essentially does not proceed
The color gradient runs from green (ΔG° ≪ 0, products dominate) through yellow (ΔG° = 0, balanced) to red (ΔG° ≫ 0, reactants dominate). Three real-world examples illustrate different positions along this spectrum.

The exponential relationship is the crucial takeaway from this section. A change of just 5.7 kJ/mol in ΔG° at 298 K changes K by a factor of about 10. That means a reaction with ΔG° = −57 kJ/mol has an equilibrium constant roughly 10¹⁰ times larger than one with ΔG° = 0. This extreme sensitivity is why small energy differences can completely shift which side of a reaction wins.

Worked Example — Calculating K from ΔG°

Let's work through a complete problem. Suppose the synthesis of ammonia at 25 °C has ΔG° = −33.0 kJ/mol for the reaction N₂(g) + 3 H₂(g) ⇌ 2 NH₃(g). Find the equilibrium constant K.

Finding K from ΔG° for the Haber Reaction at 25 °C
1
Step 1 — Identify Given ValuesΔG° = −33.0 kJ/mol, T = 25 °C = 298 K, R = 8.314 J/(mol·K). The reaction is N₂(g) + 3 H₂(g) ⇌ 2 NH₃(g).
ΔG° = −33.0 kJ/mol = −33,000 J/mol
2
Step 2 — Convert UnitsSince R is in J/(mol·K), convert ΔG° from kJ to J by multiplying by 1000.
ΔG° = −33,000 J/mol ✓
3
Step 3 — Solve for ln KRearrange ΔG° = −RT ln K to get ln K = −ΔG° / (RT). Plug in the numbers: ln K = −(−33,000) / (8.314 × 298) = 33,000 / 2477.6.
ln K = 13.32
4
Step 4 — Solve for KTake the exponential of both sides: K = e¹³·³² . Use your calculator: e¹³·³² ≈ 6.1 × 10⁵.
K ≈ 6.1 × 10⁵
5
Step 5 — Interpret the ResultSince K is much greater than 1, the reaction strongly favors products at equilibrium under standard conditions at 25 °C. This is consistent with ΔG° being negative — the reaction is spontaneous. However, remember that K tells us about the position of equilibrium, not the rate. In practice, the Haber reaction requires high temperature and a catalyst to proceed at a useful speed.

Strengths, Limitations & Common Misconceptions

Strengths and limitations of the ΔG° = −RT ln K relationship
FeatureStrengthLimitation
Predicting directionThe sign of ΔG° immediately tells you whether K > 1 or K < 1Only applies at the specific temperature used in the calculation
Quantitative powerA single equation lets you calculate exact K values from tabulated ΔG°f dataRequires accurate ΔG° values, which may have measurement uncertainty
Speed vs. equilibriumTells you where equilibrium lies (thermodynamics)Says nothing about how fast the reaction reaches equilibrium (kinetics)
Standard vs. actual conditionsProvides a baseline prediction for standard statesΔG° ≠ ΔG; actual conditions may differ from standard states, and the reaction quotient Q matters for non-standard conditions
💡 Common Misconception
Many students confuse ΔG° with ΔG. Remember: ΔG° is a fixed value for a given reaction at a given temperature — it is the free energy change when all species start in their standard states. ΔG (without the degree symbol) is the free energy change at whatever non-standard conditions actually exist. At equilibrium, ΔG = 0, but ΔG° is generally not zero (unless K happens to equal 1).
✦ KEY TAKEAWAY
Think of ΔG° as a weather forecast and K as the actual weather at equilibrium. The forecast (ΔG°) tells you whether to expect rain (products) or sunshine (reactants), and K tells you exactly how much rain or sunshine you will get. But the forecast does not tell you when the rain will arrive — that is the job of kinetics (reaction rates and activation energy).

Connection to Advanced Theory

The equation ΔG° = −RT ln K is a gateway to more advanced topics you will encounter if you continue into college chemistry, biochemistry, or chemical engineering. Here is how it connects to the bigger picture.

How ΔG° = −RT ln K connects to advanced topics
This Lesson (ΔG° = −RT ln K)Advanced Extension
K at one temperatureThe van 't Hoff equation lets you calculate K at a different temperature using ΔH°: ln(K₂/K₁) = −(ΔH°/R)(1/T₂ − 1/T₁)
ΔG° from tablesIn biochemistry, ΔG°' (the "biochemical standard") uses pH 7 instead of pH 0, because biological systems operate near neutral pH
Single reactionCoupled reactions: a non-spontaneous reaction (positive ΔG°) can be driven forward by pairing it with a highly spontaneous one (like ATP hydrolysis)
ΔG = ΔG° + RT ln QElectrochemistry: the Nernst equation E = E° − (RT/nF) ln Q is the electrical equivalent, linking cell potential to non-standard conditions

If you plan to study AP Chemistry, college-level physical chemistry, or biochemistry, mastering the ΔG°-K relationship is essential. It serves as the foundation for understanding how organisms harness energy, how batteries work, and how industrial chemists optimize reaction conditions. Every one of these applications starts with the same core idea: free energy determines the position of equilibrium.

Practice Problems

PROBLEM 1 — CONCEPTUAL
A reaction has a standard free energy change of ΔG° = −15 kJ/mol at 298 K. Without doing any calculation, predict whether K is greater than, less than, or equal to 1. Explain your reasoning.
PROBLEM 2 — BASIC CALCULATION
Calculate the equilibrium constant K for a reaction with ΔG° = −10.5 kJ/mol at T = 298 K. Use R = 8.314 J/(mol·K).
PROBLEM 3 — INTERMEDIATE
The equilibrium constant for a certain reaction at 37 °C (body temperature, 310 K) is K = 2.5 × 10⁻³. Calculate ΔG° at this temperature and state whether the reaction is spontaneous under standard conditions.
PROBLEM 4 — APPLIED
The dissolution of silver chloride in water, AgCl(s) ⇌ Ag⁺(aq) + Cl⁻(aq), has Ksp = 1.77 × 10⁻¹⁰ at 25 °C. Calculate ΔG° for this process. Then explain what this tells you about the solubility of AgCl.
PROBLEM 5 — CRITICAL THINKING
Reaction A has ΔG° = −40 kJ/mol at 298 K. Reaction B has ΔG° = −40 kJ/mol at 500 K. Both reactions have the same ΔG°. Will they have the same equilibrium constant K? Calculate K for each and explain what role temperature plays even when ΔG° is identical.

Lesson Summary

The equation ΔG° = −RT ln K is the bridge between thermodynamics and equilibrium. Standard Gibbs free energy change (ΔG°) measures the tendency of a reaction to proceed under standard conditions, while the equilibrium constant (K) quantifies the ratio of products to reactants at equilibrium. When ΔG° is negative, K > 1 and products are favored. When ΔG° is positive, K < 1 and reactants are favored. When ΔG° equals zero, K = 1 and neither side dominates.

To use the equation, always express ΔG° in joules (not kilojoules) and temperature in Kelvin. The relationship is exponential, meaning small changes in ΔG° produce large changes in K. Remember that this equation tells you where equilibrium lies, not how fast the system gets there — kinetics is a separate matter. Mastering this relationship prepares you for advanced topics like the van 't Hoff equation, the Nernst equation in electrochemistry, and coupled reactions in biochemistry.

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