Relating Kp, Kc, and Kx

Chemists measure equilibrium composition however is convenient: gas pressures, molar concentrations, or mole fractions. Yet the equilibrium constant itself is a single thermodynamic number, defined through activities. This article shows how KpK_p, KcK_c, and KxK_x are three different bookkeeping systems for the same equilibrium. Converting between them is not optional trivia. It matters whenever you measure a reaction in one unit system but need a constant in another. It also matters when total pressure changes and you must predict how mole fractions shift. Getting the conversion factors wrong is a classic source of errors in gas-phase equilibrium problems. This article builds the conversions from the ideal gas law and the definition of mole fraction. You will see the general relations. Then you will see where the factors of RTRT and P∘P^{\circ} come from. Finally, you will work two full numerical examples. One of these includes a change in total pressure.

Key takeaways
  • KpK_p, KcK_c, and KxK_x describe the same equilibrium using pressures, concentrations, or mole fractions.
  • They are related through Kp=Kc(RT)ΔnK_p = K_c(RT)^{\Delta n} and Kp=Kx(P/P∘)ΔnK_p = K_x(P/P^{\circ})^{\Delta n}.
  • Δn\Delta n is the change in moles of gas, products minus reactants, from the balanced equation.
  • Only KpK_p (built from activities using P∘=1 barP^{\circ}=1\text{ bar}) is truly dimensionless and temperature-only.
  • KcK_c and KxK_x carry implicit unit or pressure dependence hidden inside the conversion factor.
  • Key idea: the numerical value of an equilibrium constant depends on the concentration scale used to express it, but all scales trace back to one dimensionless thermodynamic constant via the ideal gas law.
The core insight

Because pressure, concentration, and mole fraction are related to each other through the ideal gas law (pi=ciRT=xiPp_i = c_iRT = x_iP), any equilibrium constant written in one variable can be rewritten in another by inserting these substitutions term by term and collecting the leftover factors into a power of Δn\Delta n, the net change in gas moles for the reaction.

The physical picture

Consider a gas-phase reaction at equilibrium, say the classic ammonia synthesis:

N2(g)+3 H2(g)⇌2 NH3(g)\text{N}_2(g) + 3\,\text{H}_2(g) \rightleftharpoons 2\,\text{NH}_3(g)

You can describe the equilibrium mixture in three equally valid languages. You can quote each gas's partial pressure pip_i in bar, its molar concentration ci=ni/Vc_i = n_i/V in mol dm⁻³, or its mole fraction xi=ni/ntotalx_i = n_i/n_{\text{total}}, a dimensionless number between 0 and 1. These three descriptions are not independent — for an ideal gas they are locked together by

pi=ciRT=xiPp_i = c_i RT = x_i P

where PP is the total pressure of the mixture. Because the three composition variables are simply rescaled versions of one another, the equilibrium constants built from them, KpK_p, KcK_c, and KxK_x, are also simply rescaled versions of one another. The rescaling factor depends only on temperature (and, for KxK_x, on total pressure), and on how many moles of gas the reaction creates or destroys. The key structural feature is Δn\Delta n, the stoichiometric change in gas moles:

Δn=∑productsνi−∑reactantsνi\Delta n = \sum_{\text{products}} \nu_i - \sum_{\text{reactants}} \nu_i

For ammonia synthesis, Δn=2−(1+3)=−2\Delta n = 2 - (1+3) = -2. When Δn=0\Delta n = 0 — equal moles of gas on each side, as in H2+I2⇌2 HI\text{H}_2 + \text{I}_2 \rightleftharpoons 2\,\text{HI} — all three constants become numerically identical, since every conversion factor collapses to unity.

Figure
Three composition scales for the same equilibrium mixture
Same equilibrium, three descriptions Partial pressure p_i (bar) K_p Concentration c_i (mol/dm3) K_c Mole fraction x_i (dimensionless) K_x p=cRT p=xP K_p = K_c (RT)^Δn = K_x (P/P°)^Δn Δn = moles gas product minus moles gas reactant

The second figure shows how KxK_x, unlike KpK_p, changes with total pressure even at fixed temperature — a fact with direct practical consequences for reactions run under compression.

Figure
K_x drifts with total pressure while K_p stays fixed, for Delta n = -2
Fixed T: K_p constant, K_x depends on P Total pressure P / bar Value (arb. scale) K_p K_x 1 10 50

The core relations

pi=ciRT=xiPp_i = c_i R T = x_i P

where pip_i is partial pressure, cic_i is molar concentration, xix_i is mole fraction, PP is total pressure, RR is the gas constant, TT is absolute temperature.

Kp=Kc (RT)ΔnK_p = K_c\,(RT)^{\Delta n}

where KpK_p uses partial pressures (in units matching P∘P^{\circ}), KcK_c uses molar concentrations, Δn\Delta n is moles gas product minus reactant.

Kp=Kx(PP∘)ΔnK_p = K_x\left(\frac{P}{P^{\circ}}\right)^{\Delta n}

where KxK_x uses mole fractions only, PP is total pressure, P∘P^{\circ} is the standard pressure (1 bar).

Kx=Kc (RT)Δn(P/P∘)ΔnK_x = K_c\,\frac{(RT)^{\Delta n}}{(P/P^{\circ})^{\Delta n}}

where this follows by eliminating KpK_p between the two relations above.

Derivation AFrom activities to Kp, Kc, and Kx

Goal. Starting from the thermodynamic (activity-based) equilibrium constant KK, derive how it relates to KpK_p built from pressures, KcK_c built from concentrations, and KxK_x built from mole fractions.

Step 1 — Start from the thermodynamic constant. For an ideal gas, the activity of species ii is its partial pressure relative to the standard pressure:

ai=piP∘a_i = \frac{p_i}{P^{\circ}}

The thermodynamic equilibrium constant for

aA+bB⇌cC+dDaA + bB \rightleftharpoons cC + dD

is

K=∏iaiνi=(pC/P∘)c(pD/P∘)d(pA/P∘)a(pB/P∘)bK = \prod_i a_i^{\nu_i} = \frac{(p_C/P^{\circ})^{c}(p_D/P^{\circ})^{d}}{(p_A/P^{\circ})^{a}(p_B/P^{\circ})^{b}}

This KK is dimensionless by construction and depends only on temperature.

Step 2 — Define Kp as the pressure-quotient with the standard-pressure factors stripped off for convenience. Chemists commonly define

Kp=pC c pD dpA a pB bK_p = \frac{p_C^{\,c}\,p_D^{\,d}}{p_A^{\,a}\,p_B^{\,b}}

using pressures expressed in units of P∘P^{\circ} (bar), so that numerically Kp=KK_p = K when pressures are quoted in bar. This is the object introduced alongside the reaction quotient in earlier equilibrium work.

Step 3 — Substitute the ideal gas law to introduce concentrations. Since pi=ciRTp_i = c_iRT, substitute term by term:

Kp=(cCRT)c(cDRT)d(cART)a(cBRT)bK_p = \frac{(c_C RT)^{c}(c_D RT)^{d}}{(c_A RT)^{a}(c_B RT)^{b}}

Group the concentration terms and the RTRT terms separately:

Kp=cC ccD dcA acB b×(RT)(c+d)−(a+b)K_p = \frac{c_C^{\,c}c_D^{\,d}}{c_A^{\,a}c_B^{\,b}} \times (RT)^{(c+d)-(a+b)}

The concentration quotient is exactly KcK_c, and the exponent is Δn\Delta n. Hence:

Kp=Kc(RT)ΔnK_p = K_c (RT)^{\Delta n}

Step 4 — Substitute the ideal gas law to introduce mole fractions instead. Since pi=xiPp_i = x_i P, substitute term by term:

Kp=(xCP)c(xDP)d(xAP)a(xBP)bK_p = \frac{(x_C P)^{c}(x_D P)^{d}}{(x_A P)^{a}(x_B P)^{b}}

Group the mole-fraction terms and the total-pressure terms separately:

Kp=xC cxD dxA axB b×P(c+d)−(a+b)K_p = \frac{x_C^{\,c}x_D^{\,d}}{x_A^{\,a}x_B^{\,b}} \times P^{(c+d)-(a+b)}

The mole-fraction quotient is KxK_x, so, restoring the standard pressure to keep the exponent dimensionless:

Kp=Kx(PP∘)ΔnK_p = K_x\left(\frac{P}{P^{\circ}}\right)^{\Delta n}

Step 5 — Combine. Both expressions equal KpK_p, so they equal each other:

Kc(RT)Δn=Kx(PP∘)ΔnK_c (RT)^{\Delta n} = K_x \left(\frac{P}{P^{\circ}}\right)^{\Delta n}
Kp=Kc(RT)Δn=Kx(PP∘)Δn\boxed{K_p = K_c(RT)^{\Delta n} = K_x\left(\frac{P}{P^{\circ}}\right)^{\Delta n}}

Worked examples

Example 1 — Foundational: converting Kc to Kp for ammonia synthesis. At 500 K500\ \text{K}, the equilibrium constant for

N2(g)+3 H2(g)⇌2 NH3(g)\text{N}_2(g) + 3\,\text{H}_2(g) \rightleftharpoons 2\,\text{NH}_3(g)

expressed in concentrations (mol dm⁻³) is Kc=1.7×102 mol−2 dm6K_c = 1.7 \times 10^{2}\ \text{mol}^{-2}\,\text{dm}^{6}. Find KpK_p. Step 1: identify Δn.

Δn=2−(1+3)=−2\Delta n = 2 - (1+3) = -2

Step 2: compute RT in units matching Kc (dm³ bar mol⁻¹ K⁻¹ form of R). Use R=0.08314 dm3 bar mol−1 K−1R = 0.08314\ \text{dm}^3\,\text{bar}\,\text{mol}^{-1}\,\text{K}^{-1}:

RT=(0.08314)(500)=41.57 dm3 bar mol−1RT = (0.08314)(500) = 41.57\ \text{dm}^3\,\text{bar}\,\text{mol}^{-1}

Step 3: apply the conversion.

Kp=Kc(RT)Δn=(1.7×102)(41.57)−2K_p = K_c (RT)^{\Delta n} = (1.7\times10^{2})(41.57)^{-2}
(41.57)2=1728(41.57)^{2} = 1728
Kp=1.7×1021728=9.8×10−2K_p = \frac{1.7\times10^{2}}{1728} = 9.8\times10^{-2}

Since Δn\Delta n is negative here, KpK_p came out with units of bar⁻² buried in the "dimensionless" activity-based number; when quoted per bar it is consistent with tabulated values of order 10−210^{-2} for this reaction near 500 K, matching the fact that the equilibrium lies well to the left (small KpK_p) at this temperature. Sanity check: raising the RT factor to a negative power because Δn<0\Delta n < 0 correctly shrinks KpK_p relative to KcK_c, since more moles of gas exist on the reactant side and pressure units penalize that side.

Example 2 — Applied: predicting how Kx changes when a reactor is compressed. The gas-phase dimerization

2 NO2(g)⇌N2O4(g)2\,\text{NO}_2(g) \rightleftharpoons \text{N}_2\text{O}_4(g)

has Kp=6.75K_p = 6.75 (dimensionless, pressures in bar, P∘=1 barP^{\circ}=1\ \text{bar}) at 298 K298\ \text{K}. A reactor initially runs at total pressure P1=1.00 barP_1 = 1.00\ \text{bar}. Find KxK_x at P1P_1, then find KxK_x if the reactor is compressed to P2=5.00 barP_2 = 5.00\ \text{bar} at the same temperature. Step 1: identify Δn.

Δn=1−2=−1\Delta n = 1 - 2 = -1

Step 2: solve for Kx at P₁ = 1.00 bar.

Kp=Kx(PP∘)Δn  ⟹  Kx=Kp(PP∘)−ΔnK_p = K_x\left(\frac{P}{P^{\circ}}\right)^{\Delta n} \implies K_x = K_p\left(\frac{P}{P^{\circ}}\right)^{-\Delta n}

At P1=1.00 barP_1 = 1.00\ \text{bar}:

Kx=6.75×(1.00)1=6.75K_x = 6.75 \times (1.00)^{1} = 6.75

Step 3: solve for Kx at P₂ = 5.00 bar.

Kx=Kp(P2P∘)1=6.75×5.00=33.75K_x = K_p\left(\frac{P_2}{P^{\circ}}\right)^{1} = 6.75 \times 5.00 = 33.75

Step 4: interpret. KpK_p stays fixed at 6.756.75 regardless of pressure, because it is the true thermodynamic constant at this TT. But KxK_x jumps from 6.756.75 to 33.7533.75 on compression. This does not mean the reaction "shifted its thermodynamics" — it means the mole-fraction ratio of product to reactant favors N2O4\text{N}_2\text{O}_4 more strongly at higher pressure, exactly as Le Chatelier's principle predicts for a reaction that reduces gas moles. Sanity check: since Δn=−1<0\Delta n = -1 < 0, increasing PP must increase KxK_x, which is what we found — compression pushes equilibrium toward the side with fewer gas molecules.

Limiting cases & common traps

SituationWhat happens
Δn=0\Delta n = 0Kp=Kc=KxK_p = K_c = K_x numerically; no conversion factor needed
Δn>0\Delta n > 0 (gas moles increase)KpK_p grows relative to KcK_c as (RT)Δn(RT)^{\Delta n}; increasing PP decreases KxK_x
Δn<0\Delta n < 0 (gas moles decrease)KpK_p shrinks relative to KcK_c; increasing PP increases KxK_x
Reaction involves solids/liquidsTheir activities are 1; only gas-phase species enter Δn\Delta n and the pressure/concentration quotients
Units of RRMust match the units used for cic_i (e.g., dm³ bar mol⁻¹ K⁻¹ paired with mol dm⁻³ and bar)

The chemist behind it

The conceptual foundation here — that equilibrium constants are ratios of activities, and that pressure, concentration, and mole fraction descriptions must be reconciled through the gas laws — rests on the broader thermodynamic framework built by Gilbert N. Lewis, who introduced the very concept of activity that makes KpK_p, KcK_c, and KxK_x mutually consistent rather than three unrelated empirical numbers.

Origins · 1 minGilbert N. Lewis and how this was discovered
GN
Gilbert N. Lewis
1875–1946 · American chemist who introduced fugacity and activity, giving equilibrium constants a rigorous, unit-independent thermodynamic foundation

Ask the tutor: How does adding an inert gas at constant pressure versus constant volume change these equilibrium constants and the position of equilibrium?

Why do we even need three different equilibrium constants

Different experiments naturally report different quantities. Gas mixtures are often characterized by total pressure and mole fractions from a manometer or gas chromatograph, while solution work uses molar concentrations. Rather than forcing every measurement into one variable before use, chemists convert between the constants after the fact. All three trace back to the same underlying activity-based constant KK, so no new physics is introduced — just a change of units and reference state, exactly as with the derivation from the ideal gas law shown above.

Does the value of Δn depend on how the equation is balanced

Yes, and this matters. If you double every stoichiometric coefficient, Δn\Delta n doubles too, and KK becomes squared, since KK for the doubled equation is K2K^2 of the original. Always state which balanced equation, and which Δn\Delta n, a quoted equilibrium constant corresponds to. This is the same subtlety that appears when comparing tabulated KpK_p values across different sources.

Is Kx ever a genuinely useful, standalone constant

Yes, particularly in engineering contexts like reactor design, where you want to know directly what fraction of the mixture is product at a chosen operating pressure. But because KxK_x depends on total pressure whenever Δn≠0\Delta n \neq 0, it is not transferable between different pressure conditions without reapplying the conversion formula—unlike KpK_p, which transfers directly across pressures at fixed temperature.

How does this connect to inert gas effects and Le Chatelier's principle

Adding an inert gas at constant volume does not change any partial pressure, so KpK_p and the equilibrium position are unaffected. Adding inert gas at constant total pressure, however, dilutes the reactive species, changes their mole fractions, and shifts the mole-fraction equilibrium — this is exactly the pressure-inert-gas effect explored next, and it flows directly from the KxK_x versus PP dependence derived here. Le Chatelier's principle is the qualitative shortcut for predicting these shifts.

Before this