Chemistry: Atoms First

# 12.3The Second and Third Laws of Thermodynamics

Chemistry: Atoms First12.3 The Second and Third Laws of Thermodynamics

### Learning Objectives

By the end of this section, you will be able to:
• State and explain the second and third laws of thermodynamics
• Calculate entropy changes for phase transitions and chemical reactions under standard conditions

### The Second Law of Thermodynamics

In the quest to identify a property that may reliably predict the spontaneity of a process, we have identified a very promising candidate: entropy. Processes that involve an increase in entropy of the systemS > 0) are very often spontaneous; however, examples to the contrary are plentiful. By expanding consideration of entropy changes to include the surroundings, we may reach a significant conclusion regarding the relation between this property and spontaneity. In thermodynamic models, the system and surroundings comprise everything, that is, the universe, and so the following is true:

$ΔSuniv=ΔSsys+ΔSsurrΔSuniv=ΔSsys+ΔSsurr$

To illustrate this relation, consider again the process of heat flow between two objects, one identified as the system and the other as the surroundings. There are three possibilities for such a process:

1. The objects are at different temperatures, and heat flows from the hotter to the cooler object. This is always observed to occur spontaneously. Designating the hotter object as the system and invoking the definition of entropy yields the following:
$ΔSsys=−qrevTsysandΔSsurr=qrevTsurrΔSsys=−qrevTsysandΔSsurr=qrevTsurr$
The arithmetic signs of qrev denote the loss of heat by the system and the gain of heat by the surroundings. Since Tsys > Tsurr in this scenario, the magnitude of the entropy change for the surroundings will be greater than that for the system, and so the sum of ΔSsys and ΔSsurr will yield a positive value for ΔSuniv. This process involves an increase in the entropy of the universe.
2. The objects are at different temperatures, and heat flows from the cooler to the hotter object. This is never observed to occur spontaneously. Again designating the hotter object as the system and invoking the definition of entropy yields the following:
$ΔSsys=qrevTsysandΔSsurr=−qrevTsurrΔSsys=qrevTsysandΔSsurr=−qrevTsurr$
The arithmetic signs of qrev denote the gain of heat by the system and the loss of heat by the surroundings. The magnitude of the entropy change for the surroundings will again be greater than that for the system, but in this case, the signs of the heat changes will yield a negative value for ΔSuniv. This process involves a decrease in the entropy of the universe.
3. The temperature difference between the objects is infinitesimally small, TsysTsurr, and so the heat flow is thermodynamically reversible. See the previous section’s discussion). In this case, the system and surroundings experience entropy changes that are equal in magnitude and therefore sum to yield a value of zero for ΔSuniv. This process involves no change in the entropy of the universe.

These results lead to a profound statement regarding the relation between entropy and spontaneity known as the second law of thermodynamics: all spontaneous changes cause an increase in the entropy of the universe. A summary of these three relations is provided in Table 12.1.

The Second Law of Thermodynamics
ΔSuniv > 0 spontaneous
ΔSuniv < 0 nonspontaneous (spontaneous in opposite direction)
ΔSuniv = 0 reversible (system is at equilibrium)
Table 12.1

For many realistic applications, the surroundings are vast in comparison to the system. In such cases, the heat gained or lost by the surroundings as a result of some process represents a very small, nearly infinitesimal, fraction of its total thermal energy. For example, combustion of a fuel in air involves transfer of heat from a system (the fuel and oxygen molecules undergoing reaction) to surroundings that are infinitely more massive (the earth’s atmosphere). As a result, qsurr is a good approximation of qrev, and the second law may be stated as the following:

$ΔSuniv=ΔSsys+ΔSsurr=ΔSsys+qsurrTΔSuniv=ΔSsys+ΔSsurr=ΔSsys+qsurrT$

We may use this equation to predict the spontaneity of a process as illustrated in Example 12.4.

### Example 12.4

#### Will Ice Spontaneously Melt?

The entropy change for the process
$H2O(s)⟶H2O(l)H2O(s)⟶H2O(l)$

is 22.1 J/K and requires that the surroundings transfer 6.00 kJ of heat to the system. Is the process spontaneous at −10.00 °C? Is it spontaneous at +10.00 °C?

#### Solution

We can assess the spontaneity of the process by calculating the entropy change of the universe. If ΔSuniv is positive, then the process is spontaneous. At both temperatures, ΔSsys = 22.1 J/K and qsurr = −6.00 kJ.

At −10.00 °C (263.15 K), the following is true:

$ΔSuniv=ΔSsys+ΔSsurr=ΔSsys+qsurrT=22.1 J/K+−6.00×103J263.15 K=−0.7J/KΔSuniv=ΔSsys+ΔSsurr=ΔSsys+qsurrT=22.1 J/K+−6.00×103J263.15 K=−0.7J/K$

Suniv < 0, so melting is nonspontaneous (not spontaneous) at −10.0 °C.

At 10.00 °C (283.15 K), the following is true:

$ΔSuniv=ΔSsys+qsurrT=22.1J/K+−6.00×103J283.15 K=+0.9 J/KΔSuniv=ΔSsys+qsurrT=22.1J/K+−6.00×103J283.15 K=+0.9 J/K$

Suniv > 0, so melting is spontaneous at 10.00 °C.

Using this information, determine if liquid water will spontaneously freeze at the same temperatures. What can you say about the values of Suniv?

Entropy is a state function, and freezing is the opposite of melting. At −10.00 °C spontaneous, +0.7 J/K; at +10.00 °C nonspontaneous, −0.9 J/K.

### The Third Law of Thermodynamics

The previous section described the various contributions of matter and energy dispersal that contribute to the entropy of a system. With these contributions in mind, consider the entropy of a pure, perfectly crystalline solid possessing no kinetic energy (that is, at a temperature of absolute zero, 0 K). This system may be described by a single microstate, as its purity, perfect crystallinity and complete lack of motion means there is but one possible location for each identical atom or molecule comprising the crystal (W = 1). According to the Boltzmann equation, the entropy of this system is zero.

$S=klnW=kln(1)=0S=klnW=kln(1)=0$

This limiting condition for a system’s entropy represents the third law of thermodynamics: the entropy of a pure, perfect crystalline substance at 0 K is zero.

We can make careful calorimetric measurements to determine the temperature dependence of a substance’s entropy and to derive absolute entropy values under specific conditions. Standard entropies are given the label $S298°S298°$ for values determined for one mole of substance at a pressure of 1 bar and a temperature of 298 K. The standard entropy change (ΔS°) for any process may be computed from the standard entropies of its reactant and product species like the following:

$ΔS°=∑νS298°(products)−∑νS298°(reactants)ΔS°=∑νS298°(products)−∑νS298°(reactants)$

Here, ν represents stoichiometric coefficients in the balanced equation representing the process. For example, ΔS° for the following reaction at room temperature

$mA+nB⟶xC+yD,mA+nB⟶xC+yD,$

is computed as the following:

$=[xS298°(C)+yS298°(D)]−[mS298°(A)+nS298°(B)]=[xS298°(C)+yS298°(D)]−[mS298°(A)+nS298°(B)]$

Table 12.2 lists some standard entropies at 298.15 K. You can find additional standard entropies in Appendix G.

Standard Entropies (at 298.15 K, 1 atm)
Substance $S298°S298°$ (J mol−1 K−1)
carbon
C(s, graphite) 5.740
C(s, diamond) 2.38
CO(g) 197.7
CO2(g) 213.8
CH4(g) 186.3
C2H4(g) 219.5
C2H6(g) 229.5
CH3OH(l) 126.8
C2H5OH(l) 160.7
hydrogen
H2(g) 130.57
H(g) 114.6
H2O(g) 188.71
H2O(l) 69.91
HCI(g) 186.8
H2S(g) 205.7
oxygen
O2(g) 205.03
Table 12.2

### Example 12.5

#### Determination of ΔS°

Calculate the standard entropy change for the following process:
$H2O(g)⟶H2O(l)H2O(g)⟶H2O(l)$

#### Solution

The value of the standard entropy change at room temperature, $ΔS298°,ΔS298°,$ is the difference between the standard entropy of the product, H2O(l), and the standard entropy of the reactant, H2O(g).
$ΔS298°=S298°(H2O(l))−S298°(H2O(g))=(70.0 Jmol−1K−1)−(188.8 Jmol−1K−1)=−118.8Jmol−1K−1ΔS298°=S298°(H2O(l))−S298°(H2O(g))=(70.0 Jmol−1K−1)−(188.8 Jmol−1K−1)=−118.8Jmol−1K−1$

The value for $ΔS298°ΔS298°$ is negative, as expected for this phase transition (condensation), which the previous section discussed.

Calculate the standard entropy change for the following process:
$H2(g)+C2H4(g)⟶C2H6(g)H2(g)+C2H4(g)⟶C2H6(g)$

−120.6 J mol−1 K−1

### Example 12.6

#### Determination of ΔS°

Calculate the standard entropy change for the combustion of methanol, CH3OH:
$2CH3OH(l)+3O2(g)⟶2CO2(g)+4H2O(l)2CH3OH(l)+3O2(g)⟶2CO2(g)+4H2O(l)$

#### Solution

The value of the standard entropy change is equal to the difference between the standard entropies of the products and the entropies of the reactants scaled by their stoichiometric coefficients.
$ΔS°=ΔS298°=∑νS298°(products)−∑νS298°(reactants)ΔS°=ΔS298°=∑νS298°(products)−∑νS298°(reactants)$
$[2S298°(CO2(g))+4S298°(H2O(l))]−[2S298°(CH3OH(l))+3S298°(O2(g))]={[2(213.8)+4×70.0]−[2(126.8)+3(205.03)]}=-161.1J/mol·K[2S298°(CO2(g))+4S298°(H2O(l))]−[2S298°(CH3OH(l))+3S298°(O2(g))]={[2(213.8)+4×70.0]−[2(126.8)+3(205.03)]}=-161.1J/mol·K$

Calculate the standard entropy change for the following reaction:
$Ca(OH)2(s)⟶CaO(s)+H2O(l)Ca(OH)2(s)⟶CaO(s)+H2O(l)$

24.7 J/mol·K

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