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Two-point Arrhenius and van ’t Hoff

4 min read· unreviewed

Questions write these equations in several different-looking ways. They are all the same equation, and each comes from one line of algebra. Once you can derive it, you never need to remember which way round the fractions go.

Arrhenius: from one temperature to two

Start from the and take natural logs:

k=A e−Ea/RT⟹ln⁡k=ln⁡A−EaRTk = A\,e^{-E_\mathrm{a}/RT} \quad\Longrightarrow\quad \ln k = \ln A - \frac{E_\mathrm{a}}{RT}

Write it at two temperatures, T1T_1 and T2T_2:

ln⁡k1=ln⁡A−EaRT1ln⁡k2=ln⁡A−EaRT2\ln k_1 = \ln A - \frac{E_\mathrm{a}}{RT_1} \qquad \ln k_2 = \ln A - \frac{E_\mathrm{a}}{RT_2}

Subtract the first from the second. ln⁡A\ln A cancels, and ln⁡k2−ln⁡k1=ln⁡(k2/k1)\ln k_2 - \ln k_1 = \ln(k_2/k_1):

ln⁡k2k1=−EaR(1T2−1T1)\ln\frac{k_2}{k_1} = -\frac{E_\mathrm{a}}{R}\left(\frac{1}{T_2}-\frac{1}{T_1}\right)

That is the . The only assumption is that AA and EaE_\mathrm{a} do not change between the two temperatures.

van ’t Hoff: the same algebra for K

Here the starting point is thermodynamics, not kinetics. Two expressions for ΔG∘\Delta G^\circ (see ):

ΔG∘=−RTln⁡KandΔG∘=ΔH∘−TΔS∘\Delta G^\circ = -RT\ln K \qquad\text{and}\qquad \Delta G^\circ = \Delta H^\circ - T\Delta S^\circ

Set them equal and divide by −RT-RT:

ln⁡K=−ΔH∘RT+ΔS∘R\ln K = -\frac{\Delta H^\circ}{RT} + \frac{\Delta S^\circ}{R}

This has exactly the shape of ln⁡k=ln⁡A−Ea/RT\ln k = \ln A - E_\mathrm{a}/RT. Write it at T1T_1 and T2T_2 and subtract; ΔS∘/R\Delta S^\circ/R cancels just as ln⁡A\ln A did:

ln⁡K2K1=−ΔH∘R(1T2−1T1)\ln\frac{K_2}{K_1} = -\frac{\Delta H^\circ}{R}\left(\frac{1}{T_2}-\frac{1}{T_1}\right)

That is the , assuming ΔH∘\Delta H^\circ and ΔS∘\Delta S^\circ are constant over the range.

Arrheniusvan ’t Hoff
Constantrate constant kkequilibrium constant KK
Energy termEaE_\mathrm{a}, always positiveΔH∘\Delta H^\circ, either sign
Cancels on subtractingln⁡A\ln AΔS∘/R\Delta S^\circ/R
Raising TTalways increases kkincreases KK only if endothermic

One equation, many looks

All of these say the same thing, written for kk (swap in KK and ΔH∘\Delta H^\circ for van ’t Hoff):

FormWhat changed
ln⁡k2k1=−EaR(1T2−1T1)\ln\dfrac{k_2}{k_1} = -\dfrac{E_\mathrm{a}}{R}\left(\dfrac{1}{T_2}-\dfrac{1}{T_1}\right)as derived
ln⁡k2k1=EaR(1T1−1T2)\ln\dfrac{k_2}{k_1} = \dfrac{E_\mathrm{a}}{R}\left(\dfrac{1}{T_1}-\dfrac{1}{T_2}\right)minus sign used to swap the bracket
ln⁡k1k2=EaR(1T2−1T1)\ln\dfrac{k_1}{k_2} = \dfrac{E_\mathrm{a}}{R}\left(\dfrac{1}{T_2}-\dfrac{1}{T_1}\right)minus sign used to flip the ratio
ln⁡k2k1=Ea(T2−T1)RT1T2\ln\dfrac{k_2}{k_1} = \dfrac{E_\mathrm{a}(T_2-T_1)}{RT_1T_2}bracket over a common denominator
log⁡10k2k1=Ea2.303 R(1T1−1T2)\log_{10}\dfrac{k_2}{k_1} = \dfrac{E_\mathrm{a}}{2.303\,R}\left(\dfrac{1}{T_1}-\dfrac{1}{T_2}\right)base-10 logs: ln⁡x=2.303log⁡10x\ln x = 2.303\log_{10}x

Worked example

A rate constant doubles between 298 K and 308 K. Find EaE_\mathrm{a}.

ln⁡2=Ea8.314(1298−1308)=Ea8.314×1.090×10−4\ln 2 = \frac{E_\mathrm{a}}{8.314}\left(\frac{1}{298}-\frac{1}{308}\right) = \frac{E_\mathrm{a}}{8.314}\times 1.090\times10^{-4}

So Ea=0.693×8.314/(1.090×10−4)≈5.29×104E_\mathrm{a} = 0.693 \times 8.314 / (1.090\times10^{-4}) \approx 5.29\times10^{4} J mol⁻¹, or 52.9 kJ mol⁻¹. This is the origin of the old rule of thumb that rates double for every 10 K rise.

Quick check

  1. 1 of 3

    Which of these is **not** the same equation as ln⁡k2k1=−EaR(1T2−1T1)\ln\frac{k_2}{k_1} = -\frac{E_\mathrm{a}}{R}\left(\frac{1}{T_2}-\frac{1}{T_1}\right)?

  2. 2 of 3

    For an exothermic reaction (ΔH∘<0\Delta H^\circ < 0), what happens to K when the temperature rises from T1T_1 to T2T_2?

  3. 3 of 3

    In the van ’t Hoff derivation, ΔH∘\Delta H^\circ plays the part of EaE_\mathrm{a}. What plays the part of ln⁡A\ln A, and why does it disappear from the two-point form?

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