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The standard free energies of formation and the standard enthalpies of formation at \(298 \mathrm{K}\) for diffuoroacetylene \(\left(\mathrm{C}_{2} \mathrm{F}_{2}\right)\) and hexafluorobenzene \(\left(\mathrm{C}_{6} \mathrm{F}_{6}\right)\) are $$\begin{array}{ccc} & \Delta G_{f}^{\circ}(\mathrm{kJ} / \mathrm{mol}) & \Delta H_{f}^{\circ}(\mathrm{kJ} / \mathrm{mol}) \\ \hline \mathrm{C}_{2} \mathrm{F}_{2}(g) & 191.2 & 241.3 \\\ \mathrm{C}_{6} \mathrm{F}_{6}(g) & 78.2 & 132.8 \end{array}$$ For the following reaction: $$\mathrm{C}_{6} \mathrm{F}_{6}(g) \rightleftharpoons 3 \mathrm{C}_{2} \mathrm{F}_{2}(g)$$ a. calculate \(\Delta S^{\circ}\) at \(298 \mathrm{K}\). b. calculate \(K\) at 298 K. c. estimate \(K\) at \(3000 .\) K, assuming \(\Delta H^{\circ}\) and \(\Delta S^{\circ}\) do not depend on temperature.

Short Answer

Expert verified
a. Calculate \(\Delta S^{\circ}\) at 298 K: By using the relation \(\Delta G^{\circ} = \Delta H^{\circ} - T\Delta S^{\circ}\), we can calculate \(\Delta S^{\circ}\) as follows: \(\Delta G_{rxn}^{\circ} = \Delta H_{rxn}^{\circ} - 298 \Delta S_{rxn}^{\circ}\) Rearranging to solve for \(\Delta S_{rxn}^{\circ}\) gives: \(\Delta S_{rxn}^{\circ} = \frac{\Delta H_{rxn}^{\circ} - \Delta G_{rxn}^{\circ}}{298}\) Substituting the given values: \(\Delta S_{rxn}^{\circ} = \frac{(3\times241.3 - 132.8) - (3\times191.2 - 78.2)}{298}\) \(\Delta S_{rxn}^{\circ} = 297.6 \mathrm{J} / \mathrm{K} \cdot \mathrm{mol}\) b. Calculate \(K\) at 298 K: Using the relation between Gibbs Free Energy and the equilibrium constant, the equation is: \(K = e^{-(\Delta G_{rxn}^{\circ})/RT}\) Substituting values: \(K = e^{-(3\times191.2 - 78.2)/(8.314\times10^{-3}\times298)}\) \(K \approx 9.54\times 10^{-7}\) c. Estimate \(K\) at 3000 K: Assuming \(\Delta H^{\circ}\) and \(\Delta S^{\circ}\) do not depend on temperature, we can use the van't Hoff equation: \(\ln\frac{K_2}{K_1} = \frac{-\Delta H^{\circ}}{R} \left(\frac{1}{T_2} - \frac{1}{T_1}\right)\) We want to find \(K_2\), given \(K_1\) at 298 K and \(T_2 = 3000\, K\). Rearrange the equation: \(K_2 = K_1 \times e^{\frac{-\Delta H^{\circ}}{R} \left(\frac{1}{T_2} - \frac{1}{T_1}\right)}\) Substituting values: \(K_2 = 9.54\times 10^{-7} \times e^{\frac{-(3\times241.3 - 132.8)}{8.314} \left(\frac{1}{3000} - \frac{1}{298}\right)}\) \(K_2 \approx 0.490\)

Step by step solution

01

Calculate ∆G° for the reaction

By subtracting the standard free energies of formation of the reactants from the products, we can find the ∆G° of the reaction at 298K. Use the equation: $$\Delta G_{rxn}^{\circ} = \sum \Delta G_{f,products}^{\circ} - \sum \Delta G_{f,reactants}^{\circ}$$

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Free Energy of Formation
Free energy of formation, denoted by \(\Delta G_f^{\circ}\), represents the change in free energy when one mole of a compound is made from its elements in their standard states. This value helps us understand how spontaneous a reaction is, under standard conditions where pressure is 1 atm and temperature is 25°C or 298 K.

When the free energy of formation is negative, the formation of the compound is spontaneous. If positive, energy is required to form the compound, making it non-spontaneous under standard conditions. In our exercise, - the \(\Delta G_f^{\circ}\) for difluoroacetylene \(\left(\mathrm{C}_2 \mathrm{F}_2\right)\) is 191.2 kJ/mol and - for hexafluorobenzene \(\left(\mathrm{C}_6 \mathrm{F}_6\right)\) is 78.2 kJ/mol.

These values assist in calculating the \(\Delta G^{\circ}_{rxn}\) (reaction free energy change) for the complete chemical reaction, which is essential for determining the equilibrium constant and spontaneity of the reaction.
Standard Enthalpy of Formation
The standard enthalpy of formation, \(\Delta H_f^{\circ}\), is defined as the heat change when one mole of a compound is formed from its elements in their standard states.

This measure allows us to understand the energy changes involved in creating a compound. A negative \(\Delta H_f^{\circ}\) indicates that the formation of the compound releases energy (exothermic), while a positive value means it absorbs energy (endothermic).

For example, in our exercise setup:
  • Difluoroacetylene has a \(\Delta H_f^{\circ} = 241.3\) kJ/mol, which shows it requires energy input for formation.
  • Hexafluorobenzene has \(\Delta H_f^{\circ} = 132.8\) kJ/mol, also requiring energy for formation.
These values are fundamental when calculating the reaction's enthalpy change, particularly when assessing reactions at various temperatures.
Equilibrium Constant
The equilibrium constant, \(K\), is an essential concept that describes the ratio of concentrations of products to reactants at equilibrium. It tells us the extent of a reaction; whether it favors formation of products or reactants.

At standard conditions, \(\Delta G^{\circ}\) is related to \(K\) through the equation: \[\Delta G^{\circ} = -RT \ln K\]where - \(R\) is the universal gas constant (8.314 J/mol·K) and - \(T\) is the temperature in Kelvin.

In our exercise, calculating \(K\) at different temperatures allows insights into how equilibrium shifts:
  • At 298 K, this calculation uses values from \(\Delta G^{\circ}_{rxn}\).
  • At 3000 K, changes in \(\Delta H^{\circ}\) and \(\Delta S^{\circ}\) can be assumed constant to estimate \(K\).
This adaptability helps understand how reactions may behave under different environmental temperatures.
Entropy Change
Entropy change, \(\Delta S^{\circ}\), measures the disorder or randomness introduced by a reaction. It is essential because it helps determine the spontaneity of a process in conjunction with enthalpy.

In a chemical context, a positive change in entropy often corresponds to increased disorder, which on a microscopic level means more available microstates or different configurations a system can adopt.

For our exercise, calculating \(\Delta S^{\circ}_{rxn}\) involves determining the entropy contribution of both reactants and products. This value is critical as it, alongside \(\Delta H^{\circ}\), helps to assess the overall \(\Delta G^{\circ}\) of the system, ultimately influencing the equilibrium constant and the feasibility of the chemical process. Understanding \(\Delta S^{\circ}\) aids significantly in thermodynamics as it reassures which direction the reaction naturally favors.

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Most popular questions from this chapter

For the process \(\mathrm{A}(l) \longrightarrow \mathrm{A}(g),\) which direction is favored by changes in energy probability? Positional probability? Explain your answers. If you wanted to favor the process as written, would you raise or lower the temperature of the system? Explain.

The standard enthalpy of formation of \(\mathrm{H}_{2} \mathrm{O}(l)\) at \(298 \mathrm{K}\) is \(-285.8 \mathrm{kJ} / \mathrm{mol} .\) Calculate the change in internal energy for the following process at \(298 \mathrm{K}\) and 1 atm: $$\mathrm{H}_{2} \mathrm{O}(l) \rightarrow \mathrm{H}_{2}(g)+1 / 2 \mathrm{O}_{2}(g) \quad \Delta E^{\circ}=?$$ (Hint: Using the ideal gas equation, derive an expression for work in terms of \(n, R,\) and \(T .\) )

Consider the reaction $$\mathrm{H}_{2}(g)+\mathrm{Br}_{2}(g) \rightleftharpoons 2 \mathrm{HBr}(g)$$ where \(\Delta H^{\circ}=-103.8 \mathrm{kJ} / \mathrm{mol} .\) In a particular experiment, equal moles of \(\mathrm{H}_{2}(g)\) at 1.00 atm and \(\mathrm{Br}_{2}(g)\) at 1.00 atm were mixed in a 1.00-L flask at \(25^{\circ} \mathrm{C}\) and allowed to reach equilibrium. Then the molecules of \(\mathrm{H}_{2}\) at equilibrium were counted using a very sensitive technique, and \(1.10 \times 10^{13}\) molecules were found. For this reaction, calculate the values of \(K, \Delta G^{\circ},\) and \(\Delta S^{\circ} .\)

Consider a weak acid, HX. If a 0.10-M solution of HX has a \(\mathrm{pH}\) of 5.83 at \(25^{\circ} \mathrm{C},\) what is \(\Delta G^{\circ}\) for the acid's dissociation reaction at \(25^{\circ} \mathrm{C} ?\)

Human DNA contains almost twice as much information as is needed to code for all the substances produced in the body. Likewise, the digital data sent from Voyager II contained one redundant bit out of every two bits of information. The Hubble space telescope transmits three redundant bits for every bit of information. How is entropy related to the transmission of information? What do you think is accomplished by having so many redundant bits of information in both DNA and the space probes?

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