What Reversible Means in Thermodynamics

In everyday chemistry talk a "reversible reaction" is one that runs both ways. Thermodynamics uses the word in a much stricter sense, and the whole of this section rests on that stricter meaning.

Key Point (Definition): A reversible process is one carried out in such a way that the system stays in perfect equilibrium with its surroundings at every instant. Each step is infinitesimal, and an infinitesimal change in the driving condition sends the process the other way.

Nothing real is reversible in this sense, because a finite push is needed to make anything move at a finite rate. A reversible path is an idealised limit that a slow, gently driven process approaches.

Applied to a chemical reaction, the same demand appears in a different dress. Take a general reaction

A+BC+D\mathrm{A} + \mathrm{B} \rightleftharpoons \mathrm{C} + \mathrm{D}

carried out in a closed vessel. Reactants begin to form products. As products build up, they begin to react back. After some time the forward rate and the backward rate become equal, and the amounts of A, B, C and D stop changing. Both reactions are still running, molecule by molecule, at identical rates. This is dynamic equilibrium.

A puzzle sits inside this picture. A spontaneous change at constant temperature and pressure must have ΔG<0\Delta G < 0. At equilibrium both the forward and the backward reaction are proceeding. If each of them had to run downhill in free energy, the mixture would need

ΔGforward<0andΔGbackward<0\Delta G_{forward} < 0 \qquad \text{and} \qquad \Delta G_{backward} < 0

which is impossible, because reversing a reaction reverses the sign of every state-function change:

ΔGbackward=ΔGforward\Delta G_{backward} = -\Delta G_{forward}

Two numbers that are exact negatives of each other cannot both be negative. The only escape is that both are zero.

ΔrG=0at equilibrium\Delta_r G = 0 \quad \text{at equilibrium}

That single line is the criterion this section builds on, and it is worth seeing why it is forced rather than assumed.

The Free Energy Minimum

Follow the Gibbs energy of the whole reaction mixture, not of one substance, as the reaction proceeds. Start with pure reactants and let the reaction move forward step by step until only products remain. The horizontal axis is the extent of reaction: 0 for pure reactants, 1 for complete conversion.

Gibbs energy of a mixture against extent of reaction with a minimum at equilibrium

The curve dips. It has to. Mixing reactants and products always lowers GG below the value either pure state would have on its own, so the graph sags in the middle and passes through a minimum at some composition.

The reaction free energy ΔrG\Delta_r G is the slope of this curve at the composition the mixture currently has. Reading the graph gives the whole story:

  • On the left of the minimum the slope is negative. ΔrG<0\Delta_r G < 0, and the mixture runs forward.
  • On the right of the minimum the slope is positive. Going forward would raise GG, so the mixture runs backward instead.
  • At the minimum the slope is zero. ΔrG=0\Delta_r G = 0, and neither direction lowers GG. The composition stops changing.

Key Point: A reacting mixture at constant temperature and pressure settles at the composition where its Gibbs energy is a minimum. The condition for that point is ΔrG=0\Delta_r G = 0. If the mixture were anywhere else on the curve, it would spontaneously slide towards the minimum.

Two symbols now have to be kept apart, and mixing them up is the single most expensive error in this topic.

Symbol What it is Value at equilibrium
ΔrG\Delta_r G slope of the GG curve at the composition present right now; changes as the reaction proceeds zero
ΔrG\Delta_r G^{\circ} a fixed number for the reaction with every reactant and product in its standard state (1 bar for a gas, unit concentration for a solute), quoted at a stated temperature not zero, except in the special case K=1K = 1

ΔrG\Delta_r G is a variable. ΔrG\Delta_r G^{\circ} is a constant belonging to the balanced equation at a given temperature.

The shape of the curve also explains why no reaction ever runs fully to completion in a closed vessel. The two ends of the curve represent pure reactants and pure products, neither of which contains any mixing. Every intermediate composition is a mixture, and mixing raises entropy, which lowers GG by TΔS-T\Delta S. A composition part-way along therefore has a Gibbs energy below what a straight line joining the two ends would give, and the sag guarantees a minimum somewhere strictly inside. Even a reaction with an enormous KK leaves a trace of reactant behind, because the minimum can never sit exactly at the right-hand edge.

Relating the Standard Gibbs Energy to K

The reaction free energy at any composition is connected to the standard value by

ΔrG=ΔrG+RTlnQ\Delta_r G = \Delta_r G^{\circ} + RT \ln Q

where QQ is the reaction quotient, built from the amounts present at that moment exactly as the equilibrium constant is built from the amounts at equilibrium.

At equilibrium two things are true together: ΔrG=0\Delta_r G = 0, and QQ has reached its equilibrium value KK. Putting both in,

0=ΔrG+RTlnK0 = \Delta_r G^{\circ} + RT \ln K

Key Point: ΔrG=RTlnK=2.303RTlogK\Delta_r G^{\circ} = -RT \ln K = -2.303\,RT \log K

The degree sign is not decoration. The quantity fixed by KK is the standard reaction Gibbs energy, the one for reactants and products all in their standard states. The standard state fixes the pressure and the concentration, at 1 bar and unit concentration, and says nothing about the temperature: ΔrG\Delta_r G^{\circ} and KK both have a value at every temperature, and the numbers in tables are simply the ones measured at 298 K. The plain ΔrG\Delta_r G is zero at equilibrium and carries no information about KK at all. Writing ΔrG=RTlnK\Delta_r G = -RT\ln K without the degree sign says 0=RTlnK0 = -RT \ln K, which forces K=1K = 1 for every reaction in existence.

Rearranged for use in the other direction:

lnK=ΔrGRTlogK=ΔrG2.303RTK=antilog(ΔrG2.303RT)\ln K = -\frac{\Delta_r G^{\circ}}{RT} \qquad \log K = -\frac{\Delta_r G^{\circ}}{2.303\,RT} \qquad K = \mathrm{antilog}\left(-\frac{\Delta_r G^{\circ}}{2.303\,RT}\right)

Units decide whether the arithmetic works. With R=8.314 JK1mol1R = 8.314\ \mathrm{J\,K^{-1}\,mol^{-1}} the product RTRT comes out in Jmol1\mathrm{J\,mol^{-1}}, so ΔrG\Delta_r G^{\circ} must also be in Jmol1\mathrm{J\,mol^{-1}}. Standard Gibbs energies are almost always quoted in kJmol1\mathrm{kJ\,mol^{-1}}, so multiply by 1000 before dividing. Going the other way, a value computed from 2.303RTlogK-2.303\,RT\log K comes out in joules per mole and is divided by 1000 for the usual kilojoule answer.

At 298 K the combination that keeps appearing has a value worth memorising:

2.303RT=2.303×8.314×298=5705 Jmol1=5.705 kJmol12.303\,RT = 2.303 \times 8.314 \times 298 = 5705\ \mathrm{J\,mol^{-1}} = 5.705\ \mathrm{kJ\,mol^{-1}}

so at 298 K, with ΔrG\Delta_r G^{\circ} in kilojoules per mole,

logK=ΔrG5.705\log K = -\frac{\Delta_r G^{\circ}}{5.705}

KK here is dimensionless, because each pressure or concentration in it is measured against the standard state. A logarithm of a quantity with units would be meaningless.

[JEE/NEET] Questions that hand you KpK_p in atmospheres and ask for ΔrG\Delta_r G^{\circ} expect you to feed the bare number into the logarithm. Do not try to carry the unit through.

Reading the Sign and the Size of the Standard Gibbs Energy

Because ΔrG\Delta_r G^{\circ} sits inside a logarithm, small changes in it produce enormous changes in KK. At 298 K:

ΔrG\Delta_r G^{\circ} / kJmol1\mathrm{kJ\,mol^{-1}} logK\log K KK Position of equilibrium
100-100 +17.5+17.5 3.4×10173.4 \times 10^{17} essentially complete
50-50 +8.76+8.76 5.8×1085.8 \times 10^{8} products dominate
10-10 +1.75+1.75 5757 products favoured
00 00 11 comparable amounts
+10+10 1.75-1.75 1.8×1021.8 \times 10^{-2} reactants favoured
+50+50 8.76-8.76 1.7×1091.7 \times 10^{-9} very little product
+100+100 17.5-17.5 3.0×10183.0 \times 10^{-18} negligible product

Scale linking standard Gibbs energy values to equilibrium constants at 298 kelvin

Every extra 5.705 kJmol15.705\ \mathrm{kJ\,mol^{-1}} of negative ΔrG\Delta_r G^{\circ} multiplies KK by ten. A gap of 30 kJ between two reactions is a factor of about 10510^{5} in their equilibrium constants.

Three readings to hold on to:

  • ΔrG\Delta_r G^{\circ} large and negative gives K1K \gg 1. At equilibrium the mixture is mostly products, and the reaction is described as going nearly to completion.
  • ΔrG\Delta_r G^{\circ} positive gives K<1K < 1. The equilibrium mixture is mostly reactants.
  • ΔrG=0\Delta_r G^{\circ} = 0 gives K=1K = 1, an equilibrium with reactants and products in comparable amounts.

Three traps sit alongside them.

A positive ΔrG\Delta_r G^{\circ} does not mean the reaction cannot happen. It means KK is small, so only a trace of product forms before equilibrium is reached. Ozone from oxygen at room temperature has K2.5×1029K \approx 2.5 \times 10^{-29}, and a tiny equilibrium amount of ozone does exist.

ΔrG=0\Delta_r G^{\circ} = 0 does not mean "no reaction". It means the equilibrium constant is exactly 1.

A negative ΔrG\Delta_r G^{\circ} says the standard mixture would run forward. Whether a particular mixture in front of you runs forward depends on ΔrG\Delta_r G, which needs QQ as well: the mixture moves forward while Q<KQ < K and backward while Q>KQ > K.

Exothermic Reactions, Entropy and the Size of K

Substituting ΔrG=ΔrHTΔrS\Delta_r G^{\circ} = \Delta_r H^{\circ} - T\Delta_r S^{\circ} into the equilibrium relation splits KK into an enthalpy part and an entropy part:

RTlnK=ΔrHTΔrS-RT\ln K = \Delta_r H^{\circ} - T\Delta_r S^{\circ}

lnK=ΔrHRT+ΔrSR\ln K = -\frac{\Delta_r H^{\circ}}{RT} + \frac{\Delta_r S^{\circ}}{R}

A strongly exothermic reaction has ΔrH\Delta_r H^{\circ} large and negative, which makes the first term large and positive, so ΔrG\Delta_r G^{\circ} is likely to be large and negative and KK large. Strongly exothermic reactions are expected to have big equilibrium constants and to go nearly to completion. A strongly endothermic reaction usually has the opposite: ΔrG\Delta_r G^{\circ} large and positive, KK far below 1, and very little product.

"Likely" is doing real work in that sentence. The second term, ΔrS/R\Delta_r S^{\circ}/R, can pull the result the other way, and the first term shrinks as TT rises while the second does not.

Ammonia synthesis, N2(g)+3H2(g)2NH3(g)\mathrm{N_2(g) + 3H_2(g) \rightleftharpoons 2NH_3(g)}, is exothermic (ΔrH=92.4 kJmol1\Delta_r H^{\circ} = -92.4\ \mathrm{kJ\,mol^{-1}}) but four moles of gas become two, so ΔrS=198.7 JK1mol1\Delta_r S^{\circ} = -198.7\ \mathrm{J\,K^{-1}\,mol^{-1}}. At 298 K the enthalpy term wins and K6.6×105K \approx 6.6 \times 10^{5}. Raise the temperature and TΔrST\Delta_r S^{\circ} grows more negative in the combination ΔrHTΔrS\Delta_r H^{\circ} - T\Delta_r S^{\circ}, so ΔrG\Delta_r G^{\circ} climbs towards zero and KK collapses. Above about 465 K the standard Gibbs energy turns positive.

Limestone decomposition, CaCO3(s)CaO(s)+CO2(g)\mathrm{CaCO_3(s) \rightarrow CaO(s) + CO_2(g)}, is the mirror image. It is endothermic (ΔrH=+178.3 kJmol1\Delta_r H^{\circ} = +178.3\ \mathrm{kJ\,mol^{-1}}), yet a gas is produced from a solid, so ΔrS=+160.6 JK1mol1\Delta_r S^{\circ} = +160.6\ \mathrm{J\,K^{-1}\,mol^{-1}}. At 298 K, K1023K \approx 10^{-23}. Above 178300/160.6=1110 K178300/160.6 = 1110\ \mathrm{K} the entropy term takes over, ΔrG\Delta_r G^{\circ} turns negative and KK exceeds 1, which is why lime kilns are run near 1200 K.

Key Point: The sign of ΔrH\Delta_r H^{\circ} is a good first guess at the size of KK, never a proof. ΔrS\Delta_r S^{\circ} and the temperature settle the matter through ΔrG=ΔrHTΔrS\Delta_r G^{\circ} = \Delta_r H^{\circ} - T\Delta_r S^{\circ}.

This relation also makes two practical routes available. Measuring ΔrH\Delta_r H^{\circ} by calorimetry and getting ΔrS\Delta_r S^{\circ} from tabulated entropies gives ΔrG\Delta_r G^{\circ}, and hence a prediction of KK at any temperature before the reaction is ever run. Measuring KK in the laboratory runs the calculation backwards and yields ΔrG\Delta_r G^{\circ}.

One more consequence is worth extracting from the same equation. Since ΔrH\Delta_r H^{\circ} and ΔrS\Delta_r S^{\circ} change only slowly with temperature, lnK\ln K is very nearly a straight line when plotted against 1/T1/T, with slope ΔrH/R-\Delta_r H^{\circ}/R and intercept ΔrS/R\Delta_r S^{\circ}/R. Measuring KK at several temperatures and drawing that line is the standard way of extracting a reaction enthalpy without ever using a calorimeter. For an exothermic reaction the slope is positive, so KK falls as the temperature is raised; for an endothermic reaction the slope is negative and KK climbs with temperature. That is the quantitative version of the familiar statement that heating shifts an endothermic equilibrium towards products.

The Third Law and Absolute Entropies

Molecules in a substance move in three ways: they travel (translation), they spin (rotation), and their bonds stretch and bend (vibration). Cooling drains all three. Entropy falls with temperature, and the natural question is how far it can fall.

For a pure substance built into a perfect crystal, every particle is fixed at a lattice site and every motion is frozen out at absolute zero. Exactly one arrangement of the whole crystal is available, so there is no disorder left to count.

Key Point: Third law of thermodynamics — the entropy of a perfectly crystalline pure substance is zero at absolute zero, S=0S = 0 at T=0 KT = 0\ \mathrm{K}.

The wording is deliberately narrow. Glasses, solutions and supercooled liquids freeze their disorder in place as they are cooled: the particles stop moving, but they stop in a jumbled arrangement rather than an ordered one. Both theory and measurement show that such substances keep a residual entropy at 0 K, and the third law does not claim otherwise.

Entropy rising from zero at absolute zero with jumps at melting and boiling

Why a true zero is useful

With a genuine zero fixed, entropy can be measured on an absolute scale rather than as a difference. Cool a sample to near 0 K, warm it in small steps, and add up the contributions:

S298=0 K298 KqrevTS_{298} = \sum_{0\ \mathrm{K}}^{298\ \mathrm{K}} \frac{q_{rev}}{T}

with a jump of ΔHtrans/Ttrans\Delta H_{trans}/T_{trans} added at each phase change. The result is the standard molar entropy SS^{\circ}, quoted in JK1mol1\mathrm{J\,K^{-1}\,mol^{-1}} at 298 K and 1 bar. Values for pure substances are all positive.

Substance SS^{\circ} / JK1mol1\mathrm{J\,K^{-1}\,mol^{-1}}
C\mathrm{C} (graphite, s) 5.7
CaO(s)\mathrm{CaO(s)} 39.7
H2O(l)\mathrm{H_2O(l)} 70.0
CaCO3(s)\mathrm{CaCO_3(s)} 92.9
H2(g)\mathrm{H_2(g)} 130.7
H2O(g)\mathrm{H_2O(g)} 188.8
N2(g)\mathrm{N_2(g)} 191.6
NH3(g)\mathrm{NH_3(g)} 192.5
O2(g)\mathrm{O_2(g)} 205.0
CO2(g)\mathrm{CO_2(g)} 213.8

A standard entropy change then follows by a Hess-type sum:

ΔrS=νS(products)νS(reactants)\Delta_r S^{\circ} = \sum \nu\, S^{\circ}(\text{products}) - \sum \nu\, S^{\circ}(\text{reactants})

The contrast with enthalpy

No experiment measures the absolute enthalpy of a substance. A calorimeter reports the heat exchanged during a change, which is a difference in HH, and there is no third law for enthalpy to supply a zero. The gap is filled by a convention: an element in its reference state is assigned ΔfH=0\Delta_f H^{\circ} = 0, and every other enthalpy of formation is quoted relative to that choice.

The two situations look similar on the page and are completely different underneath. ΔfH(O2,g)=0\Delta_f H^{\circ}(\mathrm{O_2},\,g) = 0 is a bookkeeping decision. S(O2,g)=205.0 JK1mol1S^{\circ}(\mathrm{O_2},\,g) = 205.0\ \mathrm{J\,K^{-1}\,mol^{-1}} is a measured quantity, and it is nowhere near zero.

Three patterns in the table are worth carrying into an exam hall. Gases have far larger SS^{\circ} than liquids, which in turn beat solids: compare H2O(g)\mathrm{H_2O(g)} at 188.8 with H2O(l)\mathrm{H_2O(l)} at 70.0. Hard, tightly bonded solids sit at the bottom, which is why graphite manages only 5.7. And within a phase, the more atoms a molecule carries, the more ways it has of vibrating and the higher its entropy, so CO2\mathrm{CO_2} at 213.8 outranks O2\mathrm{O_2} at 205.0.

[Board] A question that asks for ΔrS\Delta_r S^{\circ} of a reaction between elements is testing exactly this. The elements contribute their full SS^{\circ} values; only their ΔfH\Delta_f H^{\circ} values vanish.

Question 1: Equilibrium constant from a standard Gibbs energy

For a reaction at 298 K the standard Gibbs energy change is 13.6 kJmol1-13.6\ \mathrm{kJ\,mol^{-1}}. Find the equilibrium constant.

Answer:

I use ΔrG=2.303RTlogK\Delta_r G^{\circ} = -2.303\,RT\log K and solve for logK\log K.

logK=ΔrG2.303RT\log K = -\frac{\Delta_r G^{\circ}}{2.303\,RT}

The Gibbs energy is in kilojoules and RR is in joules, so I convert first: ΔrG=13600 Jmol1\Delta_r G^{\circ} = -13600\ \mathrm{J\,mol^{-1}}.

2.303RT=2.303×8.314×298=5705.8 Jmol12.303\,RT = 2.303 \times 8.314 \times 298 = 5705.8\ \mathrm{J\,mol^{-1}}

logK=136005705.8=+2.383\log K = -\frac{-13600}{5705.8} = +2.383

K=antilog(2.383)=2.4×102K = \mathrm{antilog}\,(2.383) = 2.4 \times 10^{2}

Ans: K=2.4×102K = 2.4 \times 10^{2} Watch out: Forgetting the factor of 1000 gives logK=0.00238\log K = 0.00238 and K1.0K \approx 1.0, which looks harmless and is completely wrong.

Question 2: Standard Gibbs energy from a very small K

Calculate ΔrG\Delta_r G^{\circ} for 32O2(g)O3(g)\mathrm{\dfrac{3}{2}O_2(g) \rightarrow O_3(g)} at 298 K, given Kp=2.47×1029K_p = 2.47 \times 10^{-29}.

Answer:

I need the logarithm of a number smaller than 1, so it will be negative.

logKp=log2.47+log1029=0.39329=28.607\log K_p = \log 2.47 + \log 10^{-29} = 0.393 - 29 = -28.607

ΔrG=2.303RTlogKp=(5705.8)×(28.607)\Delta_r G^{\circ} = -2.303\,RT\log K_p = -(5705.8)\times(-28.607)

ΔrG=+1.632×105 Jmol1\Delta_r G^{\circ} = +1.632 \times 10^{5}\ \mathrm{J\,mol^{-1}}

Ans: ΔrG=+163 kJmol1\Delta_r G^{\circ} = +163\ \mathrm{kJ\,mol^{-1}} Watch out: Two minus signs multiply to a plus. A tiny KK must give a large positive ΔrG\Delta_r G^{\circ}, so a negative answer here is a signal to recheck.

Question 3: An equilibrium constant of exactly 10

The equilibrium constant for a reaction at 298 K is 10. Find ΔrG\Delta_r G^{\circ}.

Answer:

log10=1\log 10 = 1, which makes the arithmetic almost nothing.

ΔrG=2.303RTlogK=(5705.8)(1)=5705.8 Jmol1\Delta_r G^{\circ} = -2.303\,RT\log K = -(5705.8)(1) = -5705.8\ \mathrm{J\,mol^{-1}}

Ans: ΔrG=5.7 kJmol1\Delta_r G^{\circ} = -5.7\ \mathrm{kJ\,mol^{-1}} Watch out: This is the number behind the shortcut logK=ΔrG/5.705\log K = -\Delta_r G^{\circ}/5.705 at 298 K, with ΔrG\Delta_r G^{\circ} in kJmol1\mathrm{kJ\,mol^{-1}}.

Question 4: What a zero standard Gibbs energy means

A reaction has ΔrG=0\Delta_r G^{\circ} = 0 at 500 K. State what this says about the equilibrium mixture, and say whether it means the reaction does not occur.

Answer:

I put the value into the relation.

0=2.303RTlogKlogK=0K=10 = -2.303\,RT\log K \quad \Rightarrow \quad \log K = 0 \quad \Rightarrow \quad K = 1

An equilibrium constant of 1 means reactants and products are present in comparable amounts once equilibrium is reached. The reaction certainly occurs; it just does not go far in either direction. The quantity that is zero at equilibrium is ΔrG\Delta_r G, not ΔrG\Delta_r G^{\circ}, and here the two happen to coincide only because K=1K = 1.

Ans: K=1K = 1; reactants and products in comparable amounts, and the reaction does occur. Watch out: ΔrG=0\Delta_r G^{\circ} = 0 and "no reaction" are unrelated statements.

Question 5: Standard Gibbs energy from a dissociation percentage

At 333 K, N2O4\mathrm{N_2O_4} is 50 per cent dissociated at a total pressure of 1 bar. Calculate ΔrG\Delta_r G^{\circ} for N2O4(g)2NO2(g)\mathrm{N_2O_4(g) \rightleftharpoons 2NO_2(g)} at this temperature.

Answer:

I start from 1 mol of N2O4\mathrm{N_2O_4} and let half of it dissociate.

At equilibrium: N2O4=10.5=0.5 mol\mathrm{N_2O_4} = 1 - 0.5 = 0.5\ \mathrm{mol}, NO2=2×0.5=1.0 mol\mathrm{NO_2} = 2 \times 0.5 = 1.0\ \mathrm{mol}, total =1.5 mol= 1.5\ \mathrm{mol}.

Mole fractions: xN2O4=0.5/1.5=0.333x_{\mathrm{N_2O_4}} = 0.5/1.5 = 0.333 and xNO2=1.0/1.5=0.667x_{\mathrm{NO_2}} = 1.0/1.5 = 0.667.

With a total pressure of 1 bar the partial pressures in bar are the same numbers, so

Kp=(pNO2)2pN2O4=(0.667)20.333=1.33K_p = \frac{(p_{\mathrm{NO_2}})^2}{p_{\mathrm{N_2O_4}}} = \frac{(0.667)^2}{0.333} = 1.33

ΔrG=2.303RTlogKp=(2.303)(8.314)(333)log1.33\Delta_r G^{\circ} = -2.303\,RT\log K_p = -(2.303)(8.314)(333)\,\log 1.33

=(6376)(0.1249)=796 Jmol1= -(6376)(0.1249) = -796\ \mathrm{J\,mol^{-1}}

Ans: ΔrG=0.80 kJmol1\Delta_r G^{\circ} = -0.80\ \mathrm{kJ\,mol^{-1}} Watch out: Each mole of N2O4\mathrm{N_2O_4} that dissociates gives two moles of NO2\mathrm{NO_2}. Using 0.5 mol of NO2\mathrm{NO_2} instead of 1.0 mol wrecks both KpK_p and the sign of the answer.

Question 6: K for ammonia synthesis at 298 K

For N2(g)+3H2(g)2NH3(g)\mathrm{N_2(g) + 3H_2(g) \rightleftharpoons 2NH_3(g)}, ΔrH=92.4 kJmol1\Delta_r H^{\circ} = -92.4\ \mathrm{kJ\,mol^{-1}} and ΔrS=198.7 JK1mol1\Delta_r S^{\circ} = -198.7\ \mathrm{J\,K^{-1}\,mol^{-1}}. Find KK at 298 K.

Answer:

I find ΔrG\Delta_r G^{\circ} first, working entirely in joules.

ΔrG=ΔrHTΔrS=92400(298)(198.7)\Delta_r G^{\circ} = \Delta_r H^{\circ} - T\Delta_r S^{\circ} = -92400 - (298)(-198.7)

=92400+59213=33187 Jmol1= -92400 + 59213 = -33187\ \mathrm{J\,mol^{-1}}

logK=331875705.8=5.817\log K = -\frac{-33187}{5705.8} = 5.817

K=antilog(5.817)=6.6×105K = \mathrm{antilog}\,(5.817) = 6.6 \times 10^{5}

Ans: ΔrG=33.2 kJmol1\Delta_r G^{\circ} = -33.2\ \mathrm{kJ\,mol^{-1}}, K=6.6×105K = 6.6 \times 10^{5} Watch out: ΔrS\Delta_r S^{\circ} is negative, so TΔrS-T\Delta_r S^{\circ} is a positive addition. Subtracting it instead gives 151.6 kJ-151.6\ \mathrm{kJ} and an absurdly large KK.

Question 7: How much a change in standard Gibbs energy changes K

Reaction A has ΔrG=10.0 kJmol1\Delta_r G^{\circ} = -10.0\ \mathrm{kJ\,mol^{-1}} at 298 K and reaction B has ΔrG=20.0 kJmol1\Delta_r G^{\circ} = -20.0\ \mathrm{kJ\,mol^{-1}} at the same temperature. Compare their equilibrium constants.

Answer:

logKA=100005705.8=1.753KA=56.6\log K_A = \frac{10000}{5705.8} = 1.753 \quad \Rightarrow \quad K_A = 56.6

logKB=200005705.8=3.505KB=3.2×103\log K_B = \frac{20000}{5705.8} = 3.505 \quad \Rightarrow \quad K_B = 3.2 \times 10^{3}

Doubling the magnitude of ΔrG\Delta_r G^{\circ} doubles logK\log K, which squares KK. Checking: (56.6)2=3.2×103(56.6)^2 = 3.2 \times 10^{3}.

Ans: KA=57K_A = 57, KB=3.2×103K_B = 3.2 \times 10^{3}; KB=(KA)2K_B = (K_A)^2 Watch out: KK is not proportional to ΔrG\Delta_r G^{\circ}. Doubling ΔrG\Delta_r G^{\circ} does not double KK.

Question 8: The temperature at which K becomes 1

For CaCO3(s)CaO(s)+CO2(g)\mathrm{CaCO_3(s) \rightarrow CaO(s) + CO_2(g)}, ΔrH=+178.3 kJmol1\Delta_r H^{\circ} = +178.3\ \mathrm{kJ\,mol^{-1}} and ΔrS=+160.6 JK1mol1\Delta_r S^{\circ} = +160.6\ \mathrm{J\,K^{-1}\,mol^{-1}}. Find the temperature at which K=1K = 1, and state what happens above it.

Answer:

K=1K = 1 makes logK=0\log K = 0, so ΔrG=0\Delta_r G^{\circ} = 0 at that temperature.

0=ΔrHTΔrST=ΔrHΔrS0 = \Delta_r H^{\circ} - T\Delta_r S^{\circ} \quad \Rightarrow \quad T = \frac{\Delta_r H^{\circ}}{\Delta_r S^{\circ}}

T=178300 Jmol1160.6 JK1mol1=1110 KT = \frac{178300\ \mathrm{J\,mol^{-1}}}{160.6\ \mathrm{J\,K^{-1}\,mol^{-1}}} = 1110\ \mathrm{K}

Above 1110 K the term TΔrST\Delta_r S^{\circ} exceeds ΔrH\Delta_r H^{\circ}, so ΔrG\Delta_r G^{\circ} becomes negative and KK rises above 1. Decomposition then produces CO2\mathrm{CO_2} at a useful pressure.

Ans: T=1110 KT = 1110\ \mathrm{K}; above it ΔrG<0\Delta_r G^{\circ} < 0 and K>1K > 1 Watch out: ΔrH\Delta_r H^{\circ} in kJ and ΔrS\Delta_r S^{\circ} in J must be brought to the same unit before dividing, or the answer comes out 1000 times too small.

Question 9: Standard entropy change from absolute entropies

Using SS^{\circ} values of 191.6191.6 for N2(g)\mathrm{N_2(g)}, 130.7130.7 for H2(g)\mathrm{H_2(g)} and 192.5 JK1mol1192.5\ \mathrm{J\,K^{-1}\,mol^{-1}} for NH3(g)\mathrm{NH_3(g)}, find ΔrS\Delta_r S^{\circ} for N2(g)+3H2(g)2NH3(g)\mathrm{N_2(g) + 3H_2(g) \rightarrow 2NH_3(g)}.

Answer:

I take products minus reactants, weighting each by its coefficient.

ΔrS=2S(NH3)[S(N2)+3S(H2)]\Delta_r S^{\circ} = 2\,S^{\circ}(\mathrm{NH_3}) - \left[S^{\circ}(\mathrm{N_2}) + 3\,S^{\circ}(\mathrm{H_2})\right]

=2(192.5)[191.6+3(130.7)]= 2(192.5) - \left[191.6 + 3(130.7)\right]

=385.0[191.6+392.1]=385.0583.7= 385.0 - \left[191.6 + 392.1\right] = 385.0 - 583.7

=198.7 JK1mol1= -198.7\ \mathrm{J\,K^{-1}\,mol^{-1}}

Four moles of gas become two, so a negative value is what the equation leads me to expect.

Ans: ΔrS=198.7 JK1mol1\Delta_r S^{\circ} = -198.7\ \mathrm{J\,K^{-1}\,mol^{-1}} Watch out: The elements N2\mathrm{N_2} and H2\mathrm{H_2} contribute their full entropies. Setting them to zero, the way ΔfH\Delta_f H^{\circ} of an element is set to zero, gives +385+385 and the wrong sign.

Question 10: Two zeros that are not the same kind

Explain why ΔfH\Delta_f H^{\circ} of graphite is zero at 298 K while SS^{\circ} of graphite is 5.7 JK1mol15.7\ \mathrm{J\,K^{-1}\,mol^{-1}} and not zero.

Answer:

No experiment gives the absolute enthalpy of a substance. A calorimeter measures heat exchanged during a change, which is a difference in HH, and nothing supplies a natural zero. Chemists therefore choose one: every element in its reference state is assigned ΔfH=0\Delta_f H^{\circ} = 0 at 298 K, and all other formation enthalpies are quoted against that choice. It is a convention.

Entropy is different, because the third law supplies a real zero. A perfect crystal of graphite has S=0S = 0 at 0 K. Warming it to 298 K adds entropy in measurable amounts, obtained by summing qrev/Tq_{rev}/T from the heat capacity data. The figure 5.7 JK1mol15.7\ \mathrm{J\,K^{-1}\,mol^{-1}} is that accumulated total, a measured quantity rather than an agreed one.

Ans: ΔfH=0\Delta_f H^{\circ} = 0 is a chosen reference; S=5.7S^{\circ} = 5.7 is an absolute value measured from the third-law zero at 0 K. Watch out: Graphite is chosen as the reference form of carbon; diamond has ΔfH=+1.9 kJmol1\Delta_f H^{\circ} = +1.9\ \mathrm{kJ\,mol^{-1}}, not zero.

Question 11: Standard Gibbs energy from K at a temperature other than 298 K

An equilibrium constant is 4.0×1024.0 \times 10^{-2} at 500 K. Calculate ΔrG\Delta_r G^{\circ}.

Answer:

The temperature is not 298 K, so the shortcut value 5705.8 does not apply and I recompute the factor.

2.303RT=2.303×8.314×500=9573 Jmol12.303\,RT = 2.303 \times 8.314 \times 500 = 9573\ \mathrm{J\,mol^{-1}}

logK=log(4.0×102)=0.6022=1.398\log K = \log (4.0 \times 10^{-2}) = 0.602 - 2 = -1.398

ΔrG=(9573)(1.398)=+13383 Jmol1\Delta_r G^{\circ} = -(9573)(-1.398) = +13383\ \mathrm{J\,mol^{-1}}

Ans: ΔrG=+13.4 kJmol1\Delta_r G^{\circ} = +13.4\ \mathrm{kJ\,mol^{-1}} Watch out: K<1K < 1 always gives a positive ΔrG\Delta_r G^{\circ}, at any temperature. Use that as a check before writing the answer down.

Question 12: A large positive standard Gibbs energy

At 298 K a reaction has ΔrG=+100 kJmol1\Delta_r G^{\circ} = +100\ \mathrm{kJ\,mol^{-1}}. Find KK and comment on how far the reaction goes.

Answer:

logK=1000005705.8=17.526\log K = -\frac{100000}{5705.8} = -17.526

K=antilog(17.526)=100.474×1018=3.0×1018K = \mathrm{antilog}\,(-17.526) = 10^{0.474} \times 10^{-18} = 3.0 \times 10^{-18}

An equilibrium constant of 3×10183 \times 10^{-18} means the equilibrium mixture is reactants with a barely detectable trace of product. The reaction is not forbidden; it simply stops almost at once.

Ans: K=3.0×1018K = 3.0 \times 10^{-18}; a negligible amount of product at equilibrium. Watch out: Handling antilog(17.526)\mathrm{antilog}(-17.526) needs the logarithm split as 18+0.474-18 + 0.474. Reading it as 1017.510^{-17.5} and rounding to 3×10173 \times 10^{-17} is off by a factor of ten.