Question 10.2: Calculate the equilibrium constant of the reaction I2(g)↽ ⇀2...

Calculate the equilibrium constant of the reaction

I2(g)2 I(g)\mathrm{I}_{2}(g) \rightleftharpoons 2  \mathrm{I}(g)

at 800 K and 1atm, supposing each component as an ideal gas, based on the following data:
v~=214.6 cm1;B=214.6 cm1;Ed=1.5422 eV\tilde{v}=214.6 \mathrm{~cm}^{-1} ; \quad B=214.6 \mathrm{~cm}^{-1} ; \quad E_{\mathrm{d}}=1.5422 \mathrm{~eV}
Here, v~\tilde{v} is the wave number of the vibration, B is the rotational constant, and EdE_{d} is the dissociation energy (also at 0 K) of the I2I_{2} molecule. At the given temperature, the molecule is in its nondegenerate ground state, while the iodine atom is in a degenerate electronic state having a multiplicity of 4.

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We can compute the equilibrium constant K by means of the formula

K=(qI)2NAqI2eEdRTK=\frac{\left(q_{\mathrm{I}}^{\ominus}\right)^{2}}{N_{\mathrm{A}} q_{\mathrm{I}_{2}}^{\ominus}} e^{-\frac{E_{\mathrm{d}}}{R T}}

To compute the standard molecular partition function of the iodine atom, we only have to calculate its translational and electronic contributions, as there are no rotational or vibrational states. The electronic contribution is the number of degeneracy; qI,elq_{\mathrm{I,el}}^{\ominus} = 4. The translational contribution can be calculated using (10.67), in which m is the mass of an iodine atom:

qtrans=(2πmkTh2)3/2V,q^{trans} = (\frac{2πmkT}{h^{2} } )^{3/2}\cdot V,                                    (10.67)

 

m=MINA=126.90447 gmol16.0220×1023 mol1=2.10734×1025 kgm=\frac{M_{\mathrm{I}}}{N_{\mathrm{A}}}=\frac{126.90447 \mathrm{ ~gmol}^{-1}}{6.0220 \times 10^{23} \mathrm{~mol}^{-1}}=2.10734 \times 10^{-25} \mathrm{~kg},

and the ideal gas molar volume V can be obtained by using the equation of state of the ideal gas:
V=RTP=8.314 Jmol1 K1800 K101325 Pa=0.06564 m3/mol.V=\frac{R T}{P}=\frac{8.314 \mathrm{ ~Jmol}^{-1} \mathrm{~K}^{-1} \cdot 800 \mathrm{~K}}{101325 \mathrm{~Pa}}=0.06564 \mathrm{~m}^{3} / \mathrm{mol}.

Thus,

qI, trans =(2πmkTh2)3/2Vq_{\mathrm{I}, \text { trans }}^{\ominus} =\left(\frac{2 \pi m k T}{h^{2}}\right)^{3 / 2} \cdot V \\
=(2π2.10734×1025 kg1.3807×1023JK1800 K(6.626×1034Js)2)3/2\left(\frac{2 \pi \cdot 2.10734 \times 10^{-25} \mathrm{~kg} \cdot 1.3807 \times 10^{-23} \mathrm{JK}^{-1} \cdot 800 \mathrm{~K}}{\left(6.626 \times 10^{-34} \mathrm{Js}\right)^{2}}\right)^{3 / 2} ×0.06564m³.

The result is qI, trans =3.992×1032q_{\mathrm{I}, \text { trans }}^{\ominus}=3.992 \times 10^{32}, which multiplied by the electronic contribution gives qI=1.597×1033.q_{\mathrm{I}}^{\ominus}=1.597 \times 10^{33}.

To compute the standard molecular partition function of the I2I_{2} molecule, we have to calculate all four contributions. The electronic contribution is simple, as there is only a single electronic state available; thus, qI2,elq_{\mathrm{I_{2},el }}^{\ominus} = 1. The translational contribution can be calculated similarly to the case of the iodine atom; the only difference is the molar mass, which is twice that of the atom. The result of the calculation is accordingly 23/22^{3/2} times that of qI,transq_{\mathrm{I,trans }}^{\ominus} ; that is, qI2,trans=1.129×1034.q_{\mathrm{I_{2},trans}}^{\ominus}= 1.129 × 10^{34}.

The rotational contribution can be calculated using (10.85), but with a division by 2, as the I2I_{2} molecule is a homonuclear rotor, with a rotational symmetry factor of σ = 2:

qlinR=kThcBq_{\mathrm{l in}}^{R} = \frac{kT}{hcB}               (10.85)

qI2,rot=kT2hcBq_{\mathrm{I_{2},rot}}^{\ominus} = \frac{kT}{2hcB}

When substituting the actual values, we should be careful with units. The rotational constant B is measured in cm1cm^{-1} units, which should be multiplied by hc to yield energy. Thus, either hcB should be given in SI energy units, or kT should be given in cm1cm^{-1} units. Choosing the latter, we can express the Boltzmann constant as 0.69503 cm1/Kcm^{-1}/K. (As a matter of fact, a division by hc is also included.) The resulting rotational partition function is qI2,rotq_{\mathrm{I_{2},rot}}^{\ominus} = 7454.1.

The vibrational contribution can be calculated using (10.90).

qV=11ehvKTq^{V} = \frac{1}{1-e^{-\frac{hv}{KT} } }                (10.90)

Again, we should be careful using units. The energy of the vibration is given as the wavenumber in cm1cm^{–1} units, thus we can use again the Boltzmann constant given above as k = 0.69503 cm1cm^{–1}/K and consider the vibrational wavenumber as energy, instead of hv. The resulting vibrational partition function is qI2,vibq_{\mathrm{I_{2},vib}}^{\ominus} = 3.126.

Finally, we can multiply the four contributions to get the molecular partition function qI2=2.632×1037.q_{\mathrm{I_{2}}}^{\ominus} = 2.632 ×10^{37}.

When calculating the equilibrium constant, we should again take into account the units of energy. As the zero-point reaction energy is given in eV units, it is useful to use the according units of the gas constant, which is then given as R = 5.189×1019eVK1mol1.10^{19} eV K^{-1} mol^{-1}. The resulting equilibrium constant is 3.104×105.10^{-5}.

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