The enthalpy of vaporization of ethanol is \(38.7 \mathrm{kJ} / \mathrm{mol}\) at its boiling point \(\left(78^{\circ} \mathrm{C}\right) .\) Determine \(\Delta S_{\mathrm{sys}}, \Delta S_{\text {surr }}\) and \(\Delta S_{\text {univ }}\) when 1.00 mole of ethanol is vaporized at \(78^{\circ} \mathrm{C}\) and 1.00 atm.

Short Answer

Expert verified
When 1.00 mole of ethanol is vaporized at 78°C and 1.00 atm, the change in entropy for the system (ΔS_sys) is 313.88 J/mol·K, the change in entropy for the surroundings (ΔS_surr) is -313.88 J/mol·K, and the change in entropy for the universe (ΔS_univ) is 0 J/mol·K.

Step by step solution

01

1. Convert temperature to Kelvin

We will convert the boiling point from Celsius to Kelvin by adding 273.15: T = 78 + 273.15 = 351.15 K
02

2. Determine the change in entropy for the system (ΔS_sys)

The ΔS_sys can be found using the enthalpy of vaporization (ΔH_vap) and the boiling point: ΔS_sys = ΔH_vap / T (Keep in mind to convert ΔH_vap to J/mol before dividing, since 1 kJ = 1000 J) ΔS_sys = (38.7 kJ/mol * 1000 J/1 kJ) / 351.15 K ΔS_sys = 110270 J/mol / 351.15 K ΔS_sys = 313.88 J/mol·K
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3. Determine the change in entropy for the surroundings (ΔS_surr)

The ΔS_surr can be found using the formula: ΔS_surr = -ΔH_sys / T ΔS_surr = -(38.7 kJ/mol * 1000 J/1 kJ) / 351.15 K ΔS_surr = -110270 J/mol / 351.15 K ΔS_surr = -313.88 J/mol·K
04

4. Determine the change in entropy for the universe (ΔS_univ)

Now that we have the changes in entropy for the system and surroundings, we can determine the change in entropy for the universe by summing ΔS_sys and ΔS_surr: ΔS_univ = ΔS_sys + ΔS_surr ΔS_univ = 313.88 J/mol·K + (-313.88 J/mol·K) ΔS_univ = 0 J/mol·K Our results are ΔS_sys = 313.88 J/mol·K, ΔS_surr = -313.88 J/mol·K, and ΔS_univ = 0 J/mol·K.

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Key Concepts

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

Enthalpy of Vaporization
The enthalpy of vaporization (ΔH_{vap}) is a crucial concept when considering the phase transition of a substance from a liquid to a gas. This term refers to the amount of energy needed to vaporize one mole of a liquid at constant pressure. It is measured in kilojoules per mole (kJ/mol).

In the context of the exercise, for ethanol, the enthalpy of vaporization is given as 38.7 kJ/mol at its boiling point. Understanding this concept is essential because it reflects the strength of intermolecular forces within the liquid; more energy is required to vaporize substances with stronger bonds between molecules. The calculation of the system's entropy change (ΔS_{sys}) during vaporization uses this value along with the substance's boiling point converted to Kelvin.

When a substance vaporizes, the system absorbs heat, which means that the enthalpy of vaporization is a positive value since the process is endothermic. Intuitively, a high enthalpy of vaporization indicates that the substance requires a significant amount of energy to undergo phase change from liquid to gas, which can infer a high degree of order or strong molecular interactions in the liquid phase.
Kelvin Temperature Conversion
Temperature conversion to Kelvin (K) is a fundamental step in thermodynamics to ensure that calculations are accurate. Kelvin is the SI base unit of temperature and is used in scientific equations to measure absolute temperature. To convert Celsius (C) to Kelvin, one simply adds 273.15 to the Celsius temperature.

In the provided exercise, the conversion was necessary to calculate the entropy change. Students frequently make the mistake of either forgetting to convert Celsius to Kelvin or using an incorrect conversion factor. It is imperative to remember that the Kelvin scale starts at absolute zero, which is theoretically the coldest possible temperature where particles have minimal thermal motion. Therefore, 0 K (absolute zero) is equivalent to -273.15°C. Using Kelvin allows for the use of true ratios and differences in thermodynamic equations — vital when calculating the entropy change during vaporization, where being even a small amount off in temperature can result in a considerable error in the calculated entropy.
Entropy of the Universe
The concept of entropy of the universe (ΔS_{univ}) is central to the second law of thermodynamics, which states that in any spontaneous process, the total entropy of the universe must increase. Entropy measures the disorder or randomness of a system; an increase in entropy signifies a system's progression towards more disorder.

In thermodynamic processes such as vaporization, we look at the entropy change in the system (ΔS_{sys}) and the surroundings (ΔS_{surr}) to determine the overall entropy change of the universe. The exercise demonstrates that the entropy gained by the system is exactly counterbalanced by the entropy lost by the surroundings, leading to no net change in the universe's entropy. However, this result is peculiar for processes occurring at the boiling point under equilibrium conditions, since it is assumed that the process is reversible and does not consider external irreversibilities.

Under typical conditions, when 1 mole of a liquid vaporizes, the disorder of the system increases (positive ΔS_{sys}) because the molecules in the vapor phase are more dispersed than in the liquid phase. Simultaneously, the surroundings generally decrease in entropy (negative ΔS_{surr}) because energy is removed from the surroundings to accomplish this phase change. Nevertheless, the second law assures us that the sum of these changes (ΔS_{univ}) will be positive for any real, irreversible process.

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Most popular questions from this chapter

Consider the following reaction at \(298 \mathrm{K}:\) $$2 \mathrm{SO}_{2}(g)+\mathrm{O}_{2}(g) \longrightarrow 2 \mathrm{SO}_{3}(g)$$ An equilibrium mixture contains \(\mathrm{O}_{2}(g)\) and \(\mathrm{SO}_{3}(g)\) at partial pressures of 0.50 atm and 2.0 atm, respectively. Using data from Appendix \(4,\) determine the equilibrium partial pressure of \(\mathrm{SO}_{2}\) in the mixture. Will this reaction be most favored at a high or a low temperature, assuming standard conditions?

Predict the sign of \(\Delta S_{\text {surr }}\) for the following processes. a. \(\mathrm{H}_{2} \mathrm{O}(l) \longrightarrow \mathrm{H}_{2} \mathrm{O}(g)\) b. \(\mathrm{I}_{2}(g) \longrightarrow \mathrm{I}_{2}(s)\)

For ammonia ( \(\mathrm{NH}$$_3\)), the enthalpy of fusion is \(5.65 \mathrm{kJ} / \mathrm{mol}\) and the entropy of fusion is \(28.9 \mathrm{J} / \mathrm{K} \cdot\) mol. a. Will \(\mathrm{NH}_{3}(s)\) spontaneously melt at \(200 . \mathrm{K} ?\) b. What is the approximate melting point of ammonia?

Impure nickel, refined by smelting sulfide ores in a blast furnace, can be converted into metal from \(99.90 \%\) to \(99.99 \%\) purity by the Mond process. The primary reaction involved in the Mond process is $$\mathrm{Ni}(s)+4 \mathrm{CO}(g) \rightleftharpoons \mathrm{Ni}(\mathrm{CO})_{4}(g)$$ a. Without referring to Appendix \(4,\) predict the sign of \(\Delta S^{\circ}\) for the above reaction. Explain. b. The spontaneity of the above reaction is temperature-dependent. Predict the sign of \(\Delta S_{\text {surr}}\) for this reaction. Explain. c. For \(\mathrm{Ni}(\mathrm{CO})_{4}(g), \Delta H_{\mathrm{f}}^{\circ}=-607 \mathrm{kJ} / \mathrm{mol}\) and \(S^{\circ}=417 \mathrm{J} / \mathrm{K}\) mol at 298 K. Using these values and data in Appendix 4 calculate \(\Delta H^{\circ}\) and \(\Delta S^{\circ}\) for the above reaction. d. Calculate the temperature at which \(\Delta G^{\circ}=0(K=1)\) for the above reaction, assuming that \(\Delta H^{\circ}\) and \(\Delta S^{\circ}\) do not depend on temperature.

Consider the following reaction at \(800 . \mathrm{K}:\) $$\mathrm{N}_{2}(g)+3 \mathrm{F}_{2}(g) \longrightarrow 2 \mathrm{NF}_{3}(g)$$ An equilibrium mixture contains the following partial pressures: \(P_{\mathrm{N}_{2}}=0.021 \mathrm{atm}, P_{\mathrm{F}_{2}}=0.063 \mathrm{atm}, P_{\mathrm{NF}_{3}}=0.48\) atm. Calculate \(\Delta G^{\circ}\) for the reaction at \(800 .\) K.

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