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Tiêu đề Entropy, Free Energy, and Equilibrium
Trường học University of Chemistry
Chuyên ngành Chemistry
Thể loại Essay
Năm xuất bản 2009
Thành phố City Name
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734 CHAPTER 18 Entropy, Free Energy, and Equilibrium The reaction generally is the system.. In part a, the increase in moles of gas gives a large positive value for LlS:'xn' In part b,

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734 CHAPTER 18 Entropy, Free Energy, and Equilibrium

The reaction generally is the system Therefore,

t.S ~n is t.S ~ys

Recall that here per mole means per mole of

reaction as written [ H~ Section 5 6 ]

Think About It The results

are consistent with the fact that

production of gases causes an

increase in entropy In part (a), the

increase in moles of gas gives a

large positive value for LlS:'xn' In

part (b), the decrease in moles of

gas gives a large negative value for

LlS:'xn- In part (c), where there is no

change in the number of moles of

gas in the reaction, LlS ~xn is positive

but is also fairly small In general,

in cases where there is no net

change in the number of moles of

gas in a reaction, we cannot predict

whether LlS:'xn will be positive or

negative-but we can predict that

it will be a relatively small number

This makes sense given that gases

invariably have greater entropy than

liquids and solids

For reactions involving only liquids a nd sol id s,

predicting the sign of t S" is more difficult,

but i n many such cas e s an increase in the

total number of molecules and/or ions is

accompan ied by an increase in entropy

The standard entropy values of a large number of substances have been measured in 11K· mol

To · caiCi.iiate · tiie ' s ' t ' lliidarci"entrcipy ' di.ange · for ' li ' reaction (ilS~n)' we look up the standard

entro-pie s of the products and reactant s and use Equation 18.7 Sample Problem 18.2 demonstrates this approach

: Strategy Look up standard entropy values and use Equation 18.7 to calculate LlS ~xn ' Just as we did

: · when we calc ul ated sta ndard enthalpies of ' ' reaction, we consider stoichiometric coefficients to be

dimensionless-giving LlS:'xn units of J / K mol

Setup From Appendix 2, SO[CaC03(s)) = 92.9 J /K mol, SO[CaO(s)] = 39.8 JIK mol,

S O [CO zeg) ] = 213.6 JIK mol, S O [N 2 (g)] = 191.5 J / K mol, S O [H 2(g) ] = 131.0 J/K mol,

S O [NH 3 (g) ] = 193.0 JIK mol, SO[CI2(g)] = 223.0 JIK mol, and SO[HCl(g)] = 187.0 JIK mol

Solution

(a) M:'xn = [SO(CaO) + SO (C0 2)] - [SO(CaC03)]

= [(39.8 JIK mol) + (213.6 J / K mol)] - (92.9 J / K mol)

Entropy Changes in the Surroundings

Next we discuss how ilS ~ urr is calculated When an exothermic process takes place in the

sys-tem, the heat transferred to the surroundings increases the motion of the molecules in the surroundings Consequently, there is an increase in the number of microstates and the entropy

of the surroundings increa ses Conversely, an endothermic process in the system absorbs heat from the surroundings and so decrea ses the entropy of the surroundings by slowing molecular motion Remember that for constant-pres s ure processe s, the heat relea se d or absorbed , q, is equal to the enthalpy change of the system, ilH s y s [ ~~ Sectio n 5 . 3] The change in entropy for

the surroundings, ilS s um is directly proportional to ilH sy s :

The minus sign indicates that a negative enthalpy change in the system (an exothermic process) correspond s to a positive entropy change in the surroundings For an endothermic process, the enthalpy change in the system is a po s itive number and corresponds to a negative entropy change

in the surroundings

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SECTION 18.3 The Second and Third Laws of Thermodynamics 735

In addition to being directly proportional to b.H s y s , b.S s urr is inversely propOltional to temperature:

Combining the two expressions gives

Equation 18.9

With Equations 18.8 and 18.9 , we can calculate the entropy change in both the syste m and s

ur-roundings for a chemical reaction , and we can determine whether the reaction i s spontaneous

Consider the sy nthesi s of ammonia at 25 ° C:

b.H~xn = -92 6 kJ/mol

From Sample Problem 18.2 ( b) , we have b.S ~ y s

( - 92.6 kJ/mol) into Equation 18.9 , we get

-198.5 J /K mol , and substituting b.H ~ y s

A _ -(-92.6 X 1000) J / mol _

uS surr - 298 K - 311 J/K mol The entropy change for the univer se i s

= -199 J/K· mol + 311 J/K· mol

= 112 J/K mol

Because b.S ~niv is positive, the reaction will be s pontaneous at 25 ° C Keep in mind, though , that

just because a reaction is spontaneous doe s not mean that it will occur at an observable rate The

synthesis of ammonia is, in fact, extremely s low at room temperature Thermodynamics can tell

us whether or not a reaction will occur spo ntaneou sly under specific conditions, but it doe s not

tell u s how fast it will occur

Third Law of Thermodynamics

Finally, we consider the third law of thermodynamics briefly in connection with the

determina-tion of s tandard e ntropy So far we have related entropy to micro sta te s the greater the number of

micro sta te s a system possesses , the larger i s the entropy of the syste m Consider a perfect

crystal-line s ub sta nce at absolute zero (0 K) Under these conditions, there i s essentially no molecular

motion and the number of microstates (W) i s 1 ( there i s only o n e way to arrange the atoms or

molecule s to form a perfect crystal) From Equation 18.2 , we write

S = kin W

=klnl=O

According to the third law of thermodynamics, the entropy of a perfect crystalline substance i s

zero at absolute zero As temperature increa ses, molecular motion increases, causing an increa se

in the number of microstates Thu s, the entropy of any substance at any temperature abo ve 0 K

is greater than zero If the crystalline s ub sta nce is impure or imperfect in any way, then it s

entropy i s greater than zero even at 0 K becau se without perfect order there i s more than one

microstate

The important point about the third law of thermodynamics i s that it enables us to determin e

the absolute entropies of substances Starting with the knowled ge that the entropy of . a pure

crys-., talline s ub sta nce is zero at 0 K , we can measure the increase in entropy of the s ub s tance when it

is heated The change in entropy of a s ub stance, b.S, is the difference between the final and initial

entropy values:

b.S = Sf - Si

where Si i s zero if the substance starts at 0 K Therefore , the measur e d change in entropy is equal

to the absolute entropy at the new temperature

f

A lth o ugh the complete details of these measurements are beyond the scope of thi s book , entropy changes are determined in part

by measur i ng the heat capacity of a substance

[ ~~ Section 5.4] as a function of absolute

temperature

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736 CHAPTER 18 Entropy, Free Energy, and Equilibrium

Figure 18 4 Entropy increa s es in

a substance a s temperature increa ses

from absolute zero

T em p era ture ( K )

Gas

The entrop y va lue s arri ved at in this way are ca lled absolute entropies becau se they are true

values-unlike s tandard enthalpies of formation, which ar e derived u s ing an arbitrary reference Becau se the tabulated v alue s are determined at I atm, we usually refer to ab so lute entropies as

standard entropie s, So Figure 18.4 shows the incr e a s e in entropy of a substance a s temperature increases from ab so lute zero At 0 K , it ha s a zero entropy value (assuming that it is a perfect crystalline s ub s tance ) As it i s heated , it s entrop y increa s e s gradually at first because of greater molecular motion within the crystal At the melting point , there is a large increase in entropy as the s olid i s transformed int o the liquid Further heating increa ses the entropy of the liquid again due to increa se d molecular motion At the boiling point , there i s a large increa s e in entropy a s a

re s ult of the liquid-to-vapor tran s ition Beyond that temperature , the entropy of the gas continues

to increa s e with increa s ing temperature

18.3 1 U s ing data from Appendix 2, calc ulate t:.s o ( in 1 1K · mol) for

the following reaction:

18.3 2 Using data from Appendix 2, calculate t:.s o ( in 1 1 K· mol ) for

d ) 242 8 1 1 K· mol

e) -2 42.8 1 1 K· mol

Gibbs Free Energy

According to the se cond law of thermodynamic s, D.Suniv > 0 for a s pontaneou s process We are

u s uall y concerned with and usually measure, however, the propertie s of the system rather than tho se of the s urrounding s or tho se of the univer se overall Ther e fore , it i s convenient to have a thermodynamic function that enables u s to determine whether or not a process i s spontaneous by considering the sys tem alone

We begin with Equation 18.5 For a s pontaneou s process,

D.Suniv = D.Ssys + D.Ssurr > 0

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SECTION 18.4 Gibbs Free Energy 737

Substituting - fUi s y/T for ~SSUIT> we write

~Hsys

~Suniv = ~Ssys + - T > 0

Multiplying both sides of the equation by T gives

Now we have an equation that expresses the second law of thermodynamic s (and predicts whether

or not a proce ss is s pontaneou s) in terms of only the system We no longer need to consider the

surroundings For convenience, we can rearrange the preceding equation, multiply through by -1,

and replace the> sign with a < s ign:

- T~Suni v = ~H sys - T~S s y s < 0

According to this equation, a process carried out at constant pre ss ure and temperature is spo ntaneous

if the changes in enthalpy and entropy of the sys tem are s uch that fUi sys - T~Ssy s is les s than zero

To express the spontaneity of a , proce ss more directly, we introduce another thermodynamic

function called the Gibbs! free energy (G), or simply free energy

Each of the term s in Equation 18.10 pertain s to the system G has units of energy ju s t as Hand

TS do Furthermore, like enthalpy and entropy, free energy is a s tate function The change in free

energy, ~G, of a system for a process that occurs at constant temperature i s

Equation 18.11 enables u s to predict the spontaneity of a process using the change in enthalpy, the

change in entropy, and the ab so lute temperature At constant temperature and pres s ure , for

pro-cesses that are spontaneous as written (in the forward direction ), ~G i s negative For processe s that

are not spontaneous as written but that , are s pontaneous , in the reverse direction , ~G i s po s itive For

systems at equilibrium, ~G is zero

~G< 0

• ~G = 0

The reaction is spontaneous in the forward direction (an d nonspontaneou s in

the reverse direction)

The reaction is nonspontaneou s in the forward direction (and spontaneous in

the reverse direction)

The system is at equilibrium

Often we can predict the s ign of ~G for a proces s if we know the signs of ~H and ~S Table 18.3

shows how we can u se Equation 18.11 to make such prediction s

Based on the information in Table 18.3, you may wonder what constitutes a " low" or a

"high" temperature For the example given in the table , O ° C is the temperature that divide s high

from low Water freezes s pontaneously at temperatures below O ° C, and ice melts spo ntaneou sly at

temperature s above O°C At O °C, a system of ice and water is at equilibrium The temperature that

In this context, free energy is the energy

available to do work Thus, i f a particular pr oces s

is accompanied by a release of usable energy ( i.e., if LiG is negative), this fact alone guarantees

that it is spontaneous, and there is no need

to consider what happens to the rest of the

Negative when T~S > fUi

Po s iti ve when T~S < fUi

Always spo nt a neous

1 Jo s iah Willard Gibbs (1839-1903) American physicist One of the founders of thermodynamics Gibbs was a m odes t

and private indi v idual who spent a lmo st a ll hi s professional lif e at Yale Unive r si ty Be cause he published mo st of his work

in obscure journals, Gibb s ne ver ga ined the eminence that hi s contemporary and admirer Jam es Maxwell did Even today,

ve r y few people o ut side of chemistry and physics have eve r heard of Gibbs

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738 CHAPTER 18 Entropy, Free Energy, and Equilibrium

Think About It Spontaneity is

being negative) and by an increase

heat, it should make sense that

the temperature will shift the

making it "more spontaneous."

divides "high" from "low" depends, though , on the individual reaction To determine that

tempera-ture, we must set t1G eq u al to 0 in Equation 18.11 (i.e , the equilibrium condition):

0= t1H - Tt1S

Rearranging to so l ve for T yie ld s

T= t1H

t1S

The temperature that divides high from low for a particular reaction can n ow be calculated if the

val u es of t1H and t1S are known Sample Pr o bl em 18 3 demonstrates the u se of thi s approach

Sample Problem 18.3

According to Table IS.3, a reaction will be spontaneous only at high temperatures if both tlH and

Strategy The temperature that divides high from low is the temperature at which tlH = TtlS

temperature in kelvins; we then convert to degrees Celsius

Practice Problem A reaction will be spontaneous only at low temperatures if both tlH and tlS are

Standard Free-Energy Changes

The introduction of the term ~GO enab l es u s to The"sia'ndardfree~eneiijY ' of'riiaction '(t1G~Xll) is th e free energy change for a reaction when it

write Equation 18.11 as occ ur s under s tandard- s tat e conditions-that i s, when reactant s in th e ir s tandard sta te s are

con-~G O = M ? - T/:,S ve rted to products in their s tandard states The conventions u sed by chemists to define the s tandard

s tates of pure substa n ces and sol uti o n s are

The standard free -energy change for thi s reaction is given by

Equation 18.12 t1G ~xn = [ct1G r (C) + dt1G r ( D ) ) - [at1G r (A) + bt1G r (B))

Equat ion 18.12 can be generalized as follows:

Equation 18.13 t1G~xn = lnt1G r ( pr od uct s) - lmt1G r ( reactants)

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where m and n are stoichiometric coefficients The term !1G J is the standard free energy of mation of a compound that is, the free-energy change that occurs when 1 mole of the compound

for-is synthesized from its con s tituent elements , each in its standard state For the combustion of

graphite,

the standard free-energy change (from Equation 18.13) is

!1G~xn = [!1G H C0 2)] - [!1G ~ (C, graphite) + !1G ~ (02)]

As with standard enthalpy of formation, the standard free energy of formation of any element (in

its most stable allotropic form at 1 atm) is defined as zero Thus ,

!1GJ?(C, graphite) = 0 and

Therefore, the standard free-energy change for the reaction in thi s case is equal to the sta ndard free energy of formation of CO2:

!1G ~xn = !1Gf(C02)

Appendix 2 lists the values of !1G J? at 25 ° C for a number of compounds

Sample Problem 18.4 demonstrate s the calculation of s tandard free-energy changes

!:J.Gf[COz(g)] = -394.4 kllmol, !:J.Gf[H20(l)] = -237.2 kJ/mol, and !:J.Gf[MgO(s)] = - 569.6 kl l mo!

All the other substances are elements in their standard states and have, by definition, !:J.G'f = O

Solution

(a) !:J.G ~n = (!:J.Gf[C02(g)] + 2!:J.Gf[H 2 0( I)]) - (!:J.Gf[CHig)] + 2!:J.Gf[02(g)])

= [(-394.4 kllmol) + (2)(-237.2 kJ/mol)] - [(-50.8 kl lmo l ) + (2)(0 kl lmo l )]

that indicates whether or not a process will occur spontaneously under a given set of conditions

What the sign of !1G o tells u s is the same thing that the magnitude of the equilibrium constant (K)

tell s us [ ~~ Section 15.2] A negative !1G o value corresponds to a large K value (products favored

at equilibrium), wherea s a po s itive !1G o value corresponds to a small K value (reactants favored at equilibrium)

Like equilibrium constants, !1G o values change with temperature One of the uses of

Equa-tion 18.11 is to determine the temperature at which a particular equilibrium will begin to favor

a desired product For example, calcium oxide (CaO), also called quicklime, is an extremely valuable inorganic substance with a variety of industrial uses , including water treatment and

Think About It Note that, like standard enthalpies of formation (DJIf), standard free energies of formation (!:J.G7) depend on the state of matter

Using water as an example,

!:J.Gf[H20(l)] = -237.2 kl l mol and

!:J.Gf[H 20(g)] = -228.6 kJ/mo!

Always double-check to make sure you have selected the right value from the table

,

The sign of !:J.GO does indicate whether or not

a process is spontaneous when all reactants a na

products are in their standard states, but this is

very seldom the case

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740 CHAPTER 18 Entropy, Free Energy, and Equilibrium

An important piece of information for th e chemist re s pon s ible for maximizing CaO

produc-tion i s the temperature at which the decomposition equilibrium of CaC03 begin s to favor products

We can mak e a reliable estimate of that temperature as follows First we calculate b H o and b S o for

the r eact ion at 2S o C, u s ing the data in Appendix 2 To determine b H o , we apply Equation S 1 9:

5" val ue s are · tabulated using joules, whe r eas

Becau se b G o is a large po s itive numb e r, the reaction does not favor product formation at 2S o C

(298 K) And, becau se b H o and b S o are both positive, we know that b G o will be negative (product formation will be favored ) at high temperatures We can determine what constitutes a high tem- perature for this reaction by calculating the temperature at which b G o is zero

At still higher temperatures , b G o becomes increasingly negative, thus favoring product formation

even more Note that in this example we u se d the b H o and b S o values at 2S o C to calculate changes

t o b G o at much higher temperature s Becau s e both b H o and b S o actually change with ture , this approach doe s not give us a truly accurate value for b G o , but it does give us a rea s onably

tempera-good estimate

Equation 18.11 can al so be used to calculate the change in entropy that accompanies a phase

change At the temperature at which a phase change occurs (i.e., the melting point or boiling point

of a s ub sta nc e), the sys tem i s at equilibrium (b G = 0 ) Therefore , Equation 18.11 become s

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SECTION 18 4 Gibbs Free Energy 741

or

0= tlH - TtlS

tlS = tlH

T

Consider the ice-water equilibrium For the ice-to-water transition, tlH i s the molar heat of fusion

(see Table 12.8) and T is the melting point The entropy change is therefore

6010 Ilmo l

tlSic e + wa t er = 273 K = 22.0 I lK · mol

Thu s, when 1 mole of ice melts at O D C, there i s an incr ease in entropy of 22.0 I l K· mol The

increase in entropy i s con s i ste nt with the increa se in micro s tate s from solid to liquid Co n ve r se l y,

for the water-to-ice transition, the decrease in entropy i s given by

tlS = -6010 I l mol = -220 I lK · I

The sa me approach can be applied to the water-to-steam transition In thi s case, tlH i s the heat of

vaporization and T is the boiling point of water Sample Problem 18.5 examines the pha se tran s

i-tion s in benzene

Sample Problem 18.S

The molar heats of fusion and vaporization of benzene are 10.9 and 31.0 kJ / m o l , respectively

Strategy The solid-liquid transition at the melting point and the liquid-vapor transition at the boiling

Setup The melting point of benzene is 5.5 + 273.15 = 278.7 K and the boiling point is 80.1 +

Practice Problem The molar heats of fusion and vaporization of argon are 1.3 and 6.3 kJ / m o l ,

respectively, and argon's melting point and boiling point are -190°C and -186°C, respectively

Calculate the entropy changes for the fusion and vaporization of argon

Checkpoint 18.4 Gibbs Free Energy

a) nonspontaneous at all temperatures

b) spontaneous at all temperatures

d) spontaneous at low temperatures

18 4 2 At what temperature (in 0c) does a

Think About It For the same

transition

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742 CHAPTER 18 Entropy, Free Energy, and Equilibrium

Eve n for a react ion that s tarts with all reactan ts

and products in their standard states, as soon

as the reaction begin s , th e conc entra tions of all

species change and standard- st ate conditions

no longer exist

The Q used in Equation 18 1 4 can be eith e r Q ,

( for reactions that take plac e in so lution) o r Qp

( for reactions that take place in the gas ph as e )

Reactant s and products in a chemical reaction are almost always in something other than their

standard sta te s - that is , s olution s u s ually have concentrations other than 1 M and gases usually have pre ss ure s other than 1 atm To determine whether or not a reaction i s s pontaneous, there- fore, we mu s t take into account the actual concentrations and/or pressure s of the species involved

And although we can determine t:: G o from tabulated values, we need to know t:: G to determine

spo ntaneity

The relationship between t:: G and t:: G o, which is derived from thermodynamics, i s

Equation 18.14 t:: G = t:: G o + RTln Q

where R i s the gas constant ( 8.314 11K· mol or 8.314 X 10 - 3 kllK mol), T is the absolute tem

- , pe ' ratiiie' at w hI c h ' the ' reac"ii"on ' takes' pi ace : and ' Q i s the reaction quotient [ ~~ Secti on 15.2] Thus ,

t:: G depend s on two terms: t:: G o and RT In Q For a given reaction at temperature T, the value

the reaction mixtur e

Con s ider the following equilibrium:

Using Equation 18.13 and information from Appendix 2 , we find that t:: G o for thi s reaction at

25 ° C i s 2.60 kl l mol The value of t:: G, however, depends on the pressure s of all three gaseous spe

-cies If we st art with a mixture of gases in which PH 2 = 2 0 atm, PIz = 2.0 atm , and PHI = 3.0 atm, the reaction quotient , Qp, i s

(P HI )2

Qp = ( PHz)(PIz )

= 2.25 Using this value in Equation 18 14 gives

(3.0)2 9.0 (2.0)(2.0) 4 0

Becau se t:: G is positive, we conclude that , s tarting with the se concentrations , the forward reactio n

will not occur s pontaneously a s written Instead, the r eve r se reaction will occur spontaneously and the sys tem will reach equilibrium by consuming part of the HI initially present and producing more H 2 and I2

If, on the other hand, we start with a mixture of gases in which PH = 2.0 atm, PI = 2 0 atm,

1

-

-4

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SECTION 18.5 Free Energy and Chemical Equilibrium 743

Using this value in Equation 18.14 gives

AG = 2.6 kJ + 8.314 X 10-3 kJ (298 K)(ln 0.25 )

= - 0.8 kJ/mol

With a negative value for AG, the reaction will be spontaneous as written in the forward

direc-tion In this case, the system will achieve equilibrium by consuming so me of the H 2 and 12 to

produce more HI

Sample Problem 18.6 u ses AG o and the reaction quoti e nt to determine in which direction a

reaction is s pontaneou s

Sample Problem 18.6

The equilibrium constant, Kp , for the reaction

is 0.1l3 at 298 K, which corresponds to a standard free-energy change of 5.4 kllmo! In a certain

experiment, the initial pressures are PN 0 = 0.453 atm and PNO = 0.122 atm Calculate 6.G for the

Because 6.G is negative, the reaction proceeds spontaneously from left to right to reach equilibrium

Practice Problem A 6.G o for the reaction

HzCg) + 12(g) :;:::, ~ 2HI(g)

is 2.60 kllmol at 25°C Calculate 6.G, and predict the direction in which the reaction is spontaneous

if the starting concentrations are P

H 2 = 3.5 atm, P

I 2 = 1.5 atm, and PHI = 1.75 atm

Practice Problem B What is the minimum partial pressure of 1 2 required for the preceding reaction

to be spontaneous in the forward direction at 25°C if the partial pressures of H 2 and HI are 3.5 and

1.75 atm, respectively?

By definition , AG = 0 and Q = K at equilibrium, where K i s the equilibrium constant Thus,

Think About It Remember, a

can be spontaneous if the starting concentrations of reactants and

products are such that Q < K

In this equation and the o n e that f ollows , K IS _

for reaction s that take place in solution an d Ko

f or reactions that take place in the gas p hase

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744 CHAPTER 18 Entropy, Free Energy, and Equilibrium

Multimedia

Chemic al Equilibrium equilibrium

., " Multimedia

Ch emical Kinet i cs - interact iv e react i on

coordinate diag ram

The sign of 6 GO tells us the same thing that the

magnitude of K tells u s The sign of 6G tells us

the same thing as the comparison of Q and K

values [ ~~ Section 15.4]

Figure 18.5 (a) !:lG o < O At

equilibrium, there is a significant

conversion of reactants to products

(b) !:lG o > O At equilibrium,

reactants are favored over products

In both cases, the net reaction toward

equilibrium is from left to right

(reactants to products) if Q < K and

right to left (products to reactants) if

Q > K At equilibrium, Q = K

18.15 is one of the most important equations in thermodynamics because it enables us to find the

It is s ignificant that Equation 18.15 relates the equilibrium constant to the standard

s how s plots of the free energy of a reacting system versus the extent of the reaction for two tion s Table 18.4 summarizes the relationship between the magnitude of an equilibrium constant

tells us the relative amounts of products and reactants when equilibrium is reached, not the

f - Extent of reaction - - - 1

(b)

GO (products)

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SECTION 18.5 Free Energy and Chemical Equilibrium 745

Products are favored

Neither products nor reactants are favored

Reactant s are favored

For reaction s with very large or very s mall equilibrium co n sta nt s, it can be ve r y

difficult-so metimes impossible to determine K values by mea s uring the concentrations of the reactant s

and product s Consider, for example, the formation of nitric oxide fro m molecular nitrogen and

molecular oxygen:

At 25 ° C, th e equilibrium constant, Kp , is

The very small value of Kp mean s that the concentration of NO at equilibrium will be exceedingly

low and, for all intents and purpo ses, impo ss ible to m eas ure directly In s uch a case, the

equilib-rium constant i s more conveniently d e termined using 6.G o, which can be calcu lated either fro m

tabulated 6.G t' values or from 6.H o and 6.s o

Sample Problems 18 7 and 18.8 s h ow how to u se 6.G o to calculate K and how to u se K to calculate 6.G o , re s pectively

Sample Problem 18.7

Using data from Appendix 2, calculate the equilibrium constant, K p, for the following reaction at

25 ° C :

Strategy Use data from Appendix 2 and Equation 18.13 to calculate t:: G o for the reaction Then use

Equation 1 8 15 to solve for K p

Practice Problem Using data from Appendix 2, calculate the equilibrium constant, K p , for the

following reaction at 25 ° C:

Think About It This is an extremely small equilibrium constant, which is consistent with

We know from everyday experience

spontaneously into its constituent elements at 25 ° C

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746 CHAPTER 18 Entropy, Free Energy, and Equilibrium

Think About It The relatively

large, positive !J.G o , like the very

small K value, corresponds to a

process that lies very far to the left

Note that the K in Equation 18.15

can be any type of K c (K a ' Kb, Ksp'

etc.) or Kp

Sample Problem 18.8

The equilibrium constant, Ksp ' for the dissolution of silver chloride in water at 25°C,

AgCl(s) :;::, = =' Ag +( aq) + Cl - (aq)

is 1.6 X 10-10 Calculate !J.G o for the process

Strategy Use Equation 18.15 to calculate !J.G o

Setup R = 8.314 X 10 - 3 kJlK mol and T = (25 + 273) = 298 K

18 5 1 For the reaction

for which 6.G o = - 1.2 kJ / mol at 25°C

Without knowing the pressures of the reactants and the product, we know that

18.5.3 The !J.G o for the reaction

is -33.3 kJ / mol at 25°C What is the

value of K p?

a) 2 X 10 - 6

b) 7 X 105

c) 3 X 10 - 70 d) 1

e) I X 10 - 1

18.5.4 The K s p for iron(III) hydroxide

[Fe(OH)3J is 1.1 X 10 - 36 at 25°C For the process

determine 6.G o (in kJ/mo l ') at 25°C

Thermodynamics in Living Systems

Many biochemical reactions have a positive I1G o val u e, yet they are essential to the maintenance

of life In living systems, these reactions are coupled to a n energetically favorable process, one

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