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The Gibbs free energy of a reacting mixture, $\\mathrm{\\Delta G}$, is given by the following equation:

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$\\mathrm{\\Delta G=\\Delta G^\\circ + RTln(Q)}$,

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where $\\mathrm{\\Delta G^\\circ}$ is the standard Gibbs free energy, in $\\mathrm{J \\space mol^{-1}}$;  $\\mathrm{R=8.314\\space J \\space K^{-1}\\space mol^{-1}}$ is the universal gas constant;  $\\mathrm{T}$ is the temperature of the system, in $\\mathrm{K}$; and $\\mathrm{Q}$ is the reaction quotient, given by:

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$\\mathrm{Q=\\frac{[C]^c[D]^d}{[A]^a[B]^b}}$   for the reaction      $\\mathrm{aA\\space +\\space bB\\space\\rightleftharpoons\\space cC\\space +\\space dD}$.

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We are asked to calculate $\\mathrm{\\Delta G}$ for the standard formation of ammonia. By considering the stoichiometries of hydrogen and nitrogen within ammonia, we can fairly easily deduce the chemical equation for this formation:

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$\\mathrm{N_2\\space +\\space 3H_2\\space\\rightleftharpoons\\space 2NH_3}$ .

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We must, however, pay attention to the fact that we will eventually be using $\\mathrm{\\Delta G^\\circ}$, for the standard formation of ammonia, i.e. the formation of 1 mole of ammonia under standard conditions. Thus, we half the stoichiometries of our equation:

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$\\mathrm{0.5N_2\\space +\\space 1.5H_2\\space\\rightleftharpoons\\space NH_3}$ .

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This gives us a reaction quotient of:

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$\\mathrm{Q=\\frac{[NH_3]}{[N_2]^{0.5}[H_2]^{1.5}}}$.

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Since all three substances are gaseous at $\\mathrm{298\\space K}$, we swap out their 'concentrations' for their partial pressures:

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$\\mathrm{Q=\\frac{p_{_{NH_3}}}{p_{_{N_2}}^{0.5}p_{_{H_2}}^{1.5}}}$ .

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Substituting this expression for $\\mathrm{Q}$ into our original equation, we now have:

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$\\mathrm{\\Delta G=\\Delta G^\\circ + RTln(\\frac{p_{_{NH_3}}}{p_{_{N_2}}^{0.5}p_{_{H_2}}^{1.5}})}$ .

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We are given the temperature of the system, $\\mathrm{T=298\\space K}$; and the partial pressures of all three gases, $\\mathrm{p_{_{NH_3}}=\\var{dpformat(nh3,1)}\\space bar}$, $\\mathrm{p_{_{N_2}}=\\var{dpformat(n2,1)}\\space bar}$, and $\\mathrm{p_{_{H_2}}=\\var{dpformat(h2,1)}\\space bar}$ .

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We are also given the equilibrium constant for the standard formation of ammonia, $\\mathrm{k=\\var{scientificnumberlatex(siground(k,5))}}$. From this, we can calculate the standard Gibbs free energy of formation, using the formula:

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$\\mathrm{\\Delta G^\\circ =-RTln(k)}$

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$\\mathrm{\\Rightarrow\\space\\space\\space\\Delta G^\\circ =-8.314\\times 298\\times ln(\\var{scientificnumberlatex(siground(k,5))})=\\var{standard} \\space J \\space mol^{-1}}$

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We can thus calculate $\\mathrm{\\Delta G}$ for our reaction:

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$\\mathrm{\\Delta G=\\var{standard} + (8.314\\times 298\\times ln[\\frac{\\var{dpformat(nh3,1)}}{{\\var{dpformat(n2,1)}}^{0.5}\\times{\\var{dpformat(h2,1)}}^{1.5}}])=\\var{sigformat(gibbs,3)}\\space J\\space mol^{-1}}$ .

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To quote our answer in the units asked for, we divide by one thousand to obtain:

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$\\mathrm{\\Delta G=\\var{sigformat(gibbskj,3)}\\space kJ\\space mol^{-1}}$ .

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The Gibbs free energy we have calculated is negative, which tells us that the reaction will proceed spontaneously in the forward direction, i.e. ammonia will be formed. Thus, the quantity of ammonia will increase.

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The equilibrium constant for the standard formation of ammonia is found to be $\\mathrm{\\var{scientificnumberlatex(siground(k,5))}}$ at $\\mathrm{298\\space K}$.

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What is the Gibbs free energy of formation of ammonia when the partial pressures of the $\\mathrm{N_2}$, $\\mathrm{H_2}$ and $\\mathrm{NH_3}$ (treated as perfect gases) are $\\mathrm{\\var{dpformat(n2,1)}\\space bar}$, $\\mathrm{\\var{dpformat(h2,1)}\\space bar}$, and $\\mathrm{\\var{dpformat(nh3,1)}\\space bar}$ respectively?

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[[0]] $\\mathrm{kJ\\space mol^{-1}}$

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Will the quantity of ammonia increase or decrease in this case?

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[[1]]

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