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Using data from Appendix \(C\), calculate \(\Delta G^{\circ}\) for the following reactions. Indicate whether each reaction is spontaneous under standard conditions. (a) \(2 \mathrm{SO}_{2}(g)+\mathrm{O}_{2}(g) \longrightarrow 2 \mathrm{SO}_{3}(g)\) (b) \(\mathrm{NO}_{2}(g)+\mathrm{N}_{2} \mathrm{O}(g) \longrightarrow 3 \mathrm{NO}(g)\) (c) \(6 \mathrm{Cl}_{2}(g)+2 \mathrm{Fe}_{2} \mathrm{O}_{3}(s) \longrightarrow 4 \mathrm{FeCl}_{3}(s)+3 \mathrm{O}_{2}(g)\) (d) \(\mathrm{SO}_{2}(g)+2 \mathrm{H}_{2}(g) \longrightarrow \mathrm{S}(s)+2 \mathrm{H}_{2} \mathrm{O}(g)\)

Short Answer

Expert verified
(a) \(\Delta G^{\circ} = -140.52 \, \mathrm{kJ/mol}\), the reaction is spontaneous. (b) \(\Delta G^{\circ} = 106.10 \, \mathrm{kJ/mol}\), the reaction is not spontaneous. (c) \(\Delta G^{\circ} = -117.04 \, \mathrm{kJ/mol}\), the reaction is spontaneous. (d) \(\Delta G^{\circ} = -174.33 \, \mathrm{kJ/mol}\), the reaction is spontaneous.

Step by step solution

01

(a) Given reaction, Gibbs free energy values, and Formula

The reaction is: \[ 2 \mathrm{SO}_{2}(g)+\mathrm{O}_{2}(g) \longrightarrow 2 \mathrm{SO}_{3}(g) \] The standard Gibbs free energy values (\(\Delta G^{\circ}_{f}\)) are: \( \Delta G^{\circ}_{f}(\mathrm{SO}_{2}) = -300.13 \, \mathrm{kJ/mol} \) \( \Delta G^{\circ}_{f}(\mathrm{O}_{2}) = 0 \, \mathrm{kJ/mol} \) \( \Delta G^{\circ}_{f}(\mathrm{SO}_{3}) = -370.39 \, \mathrm{kJ/mol} \) We will apply the formula for \(\Delta G^{\circ}\).
02

(a) Calculation of \(\Delta G^{\circ}\) for the reaction

Using the formula, we have: \[ \Delta G^{\circ} = [2(-370.39) - (2(-300.13) + 0)] \, \mathrm{kJ/mol} \] Simplifying the expression: \[ \Delta G^{\circ} = [-740.78 + 600.26] \, \mathrm{kJ/mol} = -140.52 \, \mathrm{kJ/mol} \] Since \(\Delta G^{\circ}<0\), the reaction is spontaneous under standard conditions.
03

(b) Given reaction, Gibbs free energy values, and Formula

The reaction is: \[ \mathrm{NO}_{2}(g)+\mathrm{N}_{2}\mathrm{O}(g) \longrightarrow 3\mathrm{NO}(g) \] The standard Gibbs free energy values (\(\Delta G^{\circ}_{f}\)) are: \( \Delta G^{\circ}_{f}(\mathrm{NO}_{2}) = 51.30 \, \mathrm{kJ/mol} \) \( \Delta G^{\circ}_{f}(\mathrm{N}_{2}\mathrm{O}) = 104.20 \, \mathrm{kJ/mol} \) \( \Delta G^{\circ}_{f}(\mathrm{NO}) = 87.20 \, \mathrm{kJ/mol} \) We will apply the formula for \(\Delta G^{\circ}\).
04

(b) Calculation of \(\Delta G^{\circ}\) for the reaction

Using the formula, we have: \[ \Delta G^{\circ} = [3(87.20) - (51.30 + 104.20)] \, \mathrm{kJ/mol} \] Simplifying the expression: \[ \Delta G^{\circ} = [261.60 - 155.50] \, \mathrm{kJ/mol} = 106.10 \, \mathrm{kJ/mol} \] Since \(\Delta G^{\circ}>0\), the reaction is not spontaneous under standard conditions.
05

(c) Given reaction, Gibbs free energy values, and Formula

The reaction is: \[ 6 \mathrm{Cl}_{2}(g)+2 \mathrm{Fe}_{2}\mathrm{O}_{3}(s) \longrightarrow 4\mathrm{FeCl}_{3}(s)+3\mathrm{O}_{2}(g) \] The standard Gibbs free energy values (\(\Delta G^{\circ}_{f}\)) are: \( \Delta G^{\circ}_{f}(\mathrm{Cl}_{2}) = 0 \, \mathrm{kJ/mol} \) \( \Delta G^{\circ}_{f}(\mathrm{Fe}_{2}\mathrm{O}_{3}) = -740.40 \, \mathrm{kJ/mol} \) \( \Delta G^{\circ}_{f}(\mathrm{FeCl}_{3}) = -399.46 \, \mathrm{kJ/mol} \) \( \Delta G^{\circ}_{f}(\mathrm{O}_{2}) = 0 \, \mathrm{kJ/mol} \) We will apply the formula for \(\Delta G^{\circ}\).
06

(c) Calculation of \(\Delta G^{\circ}\) for the reaction

Using the formula, we have: \[ \Delta G^{\circ} = [4(-399.46) + 3(0) - (6(0) + 2(-740.40))] \, \mathrm{kJ/mol} \] Simplifying the expression: \[ \Delta G^{\circ} = [-1597.84 + 1480.80] \, \mathrm{kJ/mol} = -117.04 \, \mathrm{kJ/mol} \] Since \(\Delta G^{\circ}<0\), the reaction is spontaneous under standard conditions.
07

(d) Given reaction, Gibbs free energy values, and Formula

The reaction is: \[ \mathrm{SO}_{2}(g)+2\mathrm{H}_{2}(g) \longrightarrow \mathrm{S}(s)+2\mathrm{H}_{2}\mathrm{O}(g) \] The standard Gibbs free energy values (\(\Delta G^{\circ}_{f}\)) are: \( \Delta G^{\circ}_{f}(\mathrm{SO}_{2}) = -300.13 \, \mathrm{kJ/mol} \) \( \Delta G^{\circ}_{f}(\mathrm{H}_{2}) = 0 \, \mathrm{kJ/mol} \) \( \Delta G^{\circ}_{f}(\mathrm{S}) = 0 \, \mathrm{kJ/mol} \) \( \Delta G^{\circ}_{f}(\mathrm{H}_{2}\mathrm{O}) = -237.23 \, \mathrm{kJ/mol} \) We will apply the formula for \(\Delta G^{\circ}\).
08

(d) Calculation of \(\Delta G^{\circ}\) for the reaction

Using the formula, we have: \[ \Delta G^{\circ} = [0 + 2(-237.23) - (-300.13 + 2(0))] \, \mathrm{kJ/mol} \] Simplifying the expression: \[ \Delta G^{\circ} = [-474.46 + 300.13] \, \mathrm{kJ/mol} = -174.33 \, \mathrm{kJ/mol} \] Since \(\Delta G^{\circ}<0\), the reaction is spontaneous under standard conditions.

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Key Concepts

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

Understanding Thermodynamics in Gibbs Free Energy Calculations
Thermodynamics, a branch of physics, investigates the relationships between heat, work, temperature, and energy. In the context of chemical reactions, thermodynamics allows us to predict whether a process will occur spontaneously through the concept of Gibbs free energy (\( \triangle G \)). Gibbs free energy is a thermodynamic potential that combines the concepts of enthalpy (\( H \)), entropy (\( S \)), and temperature (\( T \)) in the equation \( \triangle G = \triangle H - T\triangle S \). A negative value of \( \triangle G \) indicates a spontaneous process under constant pressure and temperature, which means the reaction can occur without any external energy input. Conversely, a positive \( \triangle G \) value suggests that the reaction is non-spontaneous under the same conditions and requires additional energy to proceed. Zero \( \triangle G \) indicates a system at equilibrium, meaning the forward and reverse reactions occur at the same rate. Understanding Gibbs free energy is paramount for students of chemistry, as it provides critical insights into the feasibility of chemical reactions and the energy changes involved.

To make thermodynamics more accessible for learners, providing examples with real-life applications helps in understanding abstract concepts. For example, the energy released during the combustion of fuel in an engine or the energy required for the synthesis of biochemical compounds can be analyzed through Gibbs free energy calculations. To enhance clarity, educators can break down each term in the Gibbs free energy equation and explore how changes in temperature or entropy affect the spontaneity of reactions.
Spontaneous Reactions and Gibbs Free Energy
Spontaneous reactions are processes that proceed on their own without the need for continuous external energy. It's a common misconception that 'spontaneous' implies that a reaction occurs quickly. In reality, spontaneity refers to the direction in which a process naturally proceeds, and it can be either rapid or extremely slow. For example, the rusting of iron is a spontaneous process, yet it occurs over a lengthy period.

The sign of the Gibbs free energy change (\( \triangle G \)) in a reaction determines spontaneity. If \( \triangle G < 0 \), the process is spontaneous; if \( \triangle G > 0 \), it is non-spontaneous and requires external energy; and if \( \triangle G = 0 \), the system is at equilibrium. To deepen students' understanding, educators might use analogies, such as comparing spontaneous reactions to a ball rolling downhill without any push needed. In contrast, non-spontaneous reactions are like pushing a ball uphill, requiring effort. Furthermore, explaining that the rate of a reaction (how fast it occurs) is not the same as spontaneity can help students differentiate between kinetics and thermodynamics—two key aspects of chemical reactions.
Standard Conditions in Gibbs Free Energy Calculations
Standard conditions, usually denoted by the degree sign (\( ^{\text{o}} \) ), refer to a specific set of conditions under which the measurements of thermodynamic properties are reported and compared. For Gibbs free energy changes, standard conditions mean a pressure of 1 bar (or approximately 1 atmosphere) for gases, a concentration of 1 mol/L for solutions, and pure substances in their most stable forms at 1 bar and 25°C (298.15K). These conditions are not to be confused with standard temperature and pressure (STP), which is defined as 0°C and 1 atmosphere.

The concept of standard conditions is critical because it provides a reference point that enables scientists and students to compare the thermodynamic properties of reactions consistently. When students calculate Gibbs free energy changes under standard conditions, as in the exercise above, they are able to assess the spontaneity of reactions without additional variables that could complicate their understanding. By emphasizing the importance of these conditions, we can help students realize that the \( \triangle G \) values they calculate are not universal for all situations but pertain to those specific conditions. Therefore, it's crucial to always check the conditions under which a reaction occurs to determine the correct spontaneity and feasibility of the process.

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Most popular questions from this chapter

The standard entropies at \(298 \mathrm{~K}\) for certain of the group \(4 \mathrm{~A}\) elements are as follows: \(\mathrm{C}(s\), diamond \()=2.43 \mathrm{~J} / \mathrm{mol}-\mathrm{K} ; \quad \mathrm{Si}(s)=18.81 \mathrm{~J} / \mathrm{mol}-\mathrm{K} ;\) \(\mathrm{Ge}(s)=31.09 \mathrm{~J} / \mathrm{mol}-\mathrm{K} ; \quad\) and \(\quad \mathrm{Sn}(s)=51.18 \mathrm{~J} / \mathrm{mol}-\mathrm{K}\) All but Sn have the diamond structure. How do you account for the trend in the \(S^{\circ}\) values?

The reaction $$ \mathrm{SO}_{2}(g)+2 \mathrm{H}_{2} \mathrm{~S}(g) \rightleftharpoons 3 \mathrm{~S}(s)+2 \mathrm{H}_{2} \mathrm{O}(g) $$ is the basis of a suggested method for removal of \(\mathrm{SO}_{2}\) from power-plant stack gases. The standard free energy of each substance is given in Appendix C. (a) What is the equilibrium constant for the reaction at \(298 \mathrm{~K} ?\) (b) In principle, is this reaction a feasible method of removing \(\mathrm{SO}_{2} ?\) (c) If \(P_{\mathrm{SO}_{2}}=P_{\mathrm{H}_{2} \mathrm{~s}}\) and the vapor pressure of water is 25 torr, calculate the equilibrium \(\mathrm{SO}_{2}\) pressure in the system at \(298 \mathrm{~K}\) (d) Would you expect the process to be more or less effective at higher temperatures?

About \(86 \%\) of the world's electrical energy is produced by using steam turbines, a form of heat engine. In his analysis of an ideal heat engine, Sadi Carnot concluded that the maximum possible efficiency is defined by the total work that could be done by the engine, divided by the quantity of heat available to do the work (for example from hot steam produced by combustion of a fuel such as coal or methane). This efficiency is given by the ratio \(\left(T_{\text {high }}-T_{\text {low }}\right) / T_{\text {high }}\), where \(T_{\text {high }}\) is the temperature of the heat going into the engine and \(T_{\text {low }}\) is that of the heat leaving the engine. (a) What is the maximum possible efficiency of a heat engine operating between an input temperature of \(700 \mathrm{~K}\) and an exit temperature of \(288 \mathrm{~K} ?\) (b) Why is it important that electrical power plants be located near bodies of relatively cool water? (c) Under what conditions could a heat engine operate at or near \(100 \%\) efficiency? (d) It is often said that if the energy of combustion of a fuel such as methane were captured in an electrical fuel cell instead of by burning the fuel in a heat engine, a greater fraction of the energy could be put to useful work. Make a qualitative drawing like that in Figure \(5.10\) that illustrates the fact that in principle the fuel cell route will produce more useful work than the heat engine route from combustion of methane.

One way to derive Equation \(19.3\) depends on the observation that at constant \(T\) the number of ways, \(W\), of arranging \(m\) ideal-gas particles in a volume \(V\) is proportional to the volume raised to the \(m\) power: $$ W \propto V^{m} $$ Use this relationship and Boltzmann's relationship between entropy and number of arrangements (Equation 19.5) to derive the equation for the entropy change for the isothermal expansion or compression of \(n\) moles of an ideal gas.

(a) What is the meaning of the standard free-energy change, \(\Delta G^{\circ}\), as compared with \(\Delta G\) ? (b) For any process that occurs at constant temperature and pressure, what is the significance of \(\Delta G=0 ?(c)\) For a certain process, \(\Delta G\) is large and negative. Does this mean that the process necessarily occurs rapidly?

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