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CHEMICAL-REACTION
EQUILIBRIA
CHAPTER
13
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13.1 THE REACTION COORDINATE
The general chemical reaction :
...... 44332211 ++→++ Av Av Av Av
where | vi | is a stoichiometric coefficient and A
istands for a
chemical formula.
For vi :
Positive ( + for !roduct "egative ( # for reactants
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Example :
$%4 + %
2& ' $& + 3%
2
The stoichiometric numers are :
14
−=CH v 12
−=O H v 1=COv 32= H v
The stoichiometric numer for an inert s!ecies is )ero.
*ince
ε d
v
dn
v
dn
v
dn
v
dn===== ...
4
4
3
3
2
2
1
1
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The general relation etween a differential change dni in the
numer of moles of a reacting s!ecies and dε is :
dni = vi dε ( i 1 , 2 ,-. N
This variale ε called the reaction coordinate, characteri)es the
etent or degree to which a reaction has ta/en !lace.
∫ ∫ = ε
ε 0
0
d vdn i
n
n i
i
i
or
ε iii
vnn
+=0
( i 1 , 2 ,-. N
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*ummation over all s!ecies ields :
∑∑∑ +==i
i
i
i
i
i vnnn ε 0
or n = n0 + vε
where ∑≡i
inn ∑≡i
inn00 ∑≡
i
ivv
Thus the mole fractions yi of the s!ecies !resent are related to ε :
ε
ε
vn
vn
n
n y
iii
i
+
+==
0
0
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Example 13.2
$onsider a vessel which initiall contains onl no mol of water
va!or. f decom!osition occurs according to the reaction,
22221 O H O H +→
find e!ressions which relate the numer of moles and the mole
fraction of each chemical s!ecies to the reaction coordinate ε.
Solution 13.2
For the given reaction2
1
2
111 =++−=v
!!lication of 5s. (13.4 and(13.6 ields:
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ε −= 02nn O H
ε
ε
2
10
0
2
+
−=n
n y O H
ε =2 H n
ε
ε
2
10
2
+=
n y H
ε 2
12=On
ε
ε
2
12
1
0
2
+=
n
yO
The fractional decom!osition of water va!or is:
( )00
00
0
0 2
nn
nn
n
nn O H ε ε =−−=−
Thus when no 1, ε is identified with the fractional decom!osition of
the water va!or.
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∑= j
j jii d vdn ε ,
fter integration :
j j
jiii vnn ε ∑+= ,0
*umming over all s!ecies ields :
j
j i
ji
i
j
j
ji
i
i vnvnn ε ε ∑ ∑∑∑∑
+=+=
,0,0
For the mole fraction:
∑
∑
+
+=
j j j
j
j jii
ivn
vn
yε
ε
0
,0
( i 1 , 2 ,-. N
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13.2 APPLICATION OF
EQUILIBRIUM CRITERIA TO
CHEMICAL REACTIONS t the e5uilirium state :
( dGt )T , P
0
The total 7is energ Gt is a minimum
ts differential is )ero.
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13.3 THE STANDARD GIBBS-ENERGY
CHANGE
AND THE EQUILIBRIUM CONSTANT The fundamental !ro!ert relation for single#!hase sstems,
!rovides an e!ression for the total differential of the 7is
energ: ( ) ( ) ( ) ∑+−=i
iidndT S dP nV nGd µ
f changes in mole numers ni occur as the result of a single
chemical reaction in a closed sstem , then each dni ma e
re!laced the !roduct vi dε .
( ) ( ) ( )
∑+−=
i
ii d vdT S dP nV nGd ε µ
*ince nG is a state function , the right side of this an eact
differential e!ression :
( ) ( )
P T
t
P T i
ii
GnGv
,,
∂
∂=
∂
∂=∑
ε ε
µ
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For chemical#reaction e5uilirium :
0=∑i
iiv µ
8ecall the definition of the fugacit of a s!ecies in solution :
( ) iii f RT T 9ln+Γ= µ
For a !ure s!ecies i in its standard start at the same tem!erature :
( )
iii f RT T G ln+Γ =
The difference etween these two e5uations is :
i
iii
f
f RT G
9ln=− µ
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For the e5uilirium state of a chemical reaction :
( )[ ] 09ln =+∑i
iiii f f RT Gv
( ) 09ln =+ ∑∑ i
vii
i
iii f f RT Gv
( ) RT
Gv f f i ii
i
v
ii
i ∑∏ −
=
9ln
( )∏ =i
v
ii K f f i9ln
where
∆−≡
RT
G K
e!
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lternative e!ression for :
RT
G K
∆−≡ln
lso definition : ∑∆≡∆i
iGG
K is a function of tem!erature onl .
In spite of its dependence on temperature , K is called the
equilibrium constant for the reaction ;
∑i iiGv
, represented by ΔG˚ , is called the
standard Gibbs-energy change of reaction ,
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13.4 EFFECT OF TEMPERATURE
ON THE EQUILIBRIUM CONSTANT
The de!endence of ;G< on T :
( )2 RT
H
dT
RT Gd ∆−=
∆
Then ecome:
2
ln
RT
H
dT
K d ∆=
5uation aove gives the effect of tem!erature on e5uilirium
constant and hence on the e5uilirium conversion.
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=hen ; H <
negative eothermic reaction
!ositive endothermic reaction
f ; H < is assumed inde!endent of T, then:
′−
∆
−=′ T T R
H
K
K 11ln
This a!!roimate e5uation im!lies that a !lot of ln K vs the
reci!rocal of asolute tem!erature is a straight line. Figure
13.2 in tetoo/, shows a !lot of ln K vs 1>T for a numer of
common reactions, illustrates this near linearit.
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The rigorous develo!ment of the effect of tem!erature on
the e5uilirium constant is ased on the definition of the
7is energ , written for a chemical s!ecies in its standard
state:
G˚ i = H˚
i TS˚
i
?ulti!lication vi and summation over all s!ecies gives:
∑∑∑ −=i
ii
i
ii
i
ii S vT H vGv
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s a result of the definition of standard !ro!ert change of
reaction, this reduces to:
;G˚=; H˚ T ;S˚
=here the standard heat of reaction and standard entro!
change is related to tem!erature:
dT RC R H H
T
T P
∫ ∆+∆=∆0
0
∫ ∆+∆=∆
T
T
P
T
dT
R
C RS S
00
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%owever
0
000
T
G H S
∆−∆=∆
whence
∫ ∫ ∆
−∆
+∆
+∆−∆
=∆ T
T
P T
T
P
o
T
dT
R
C dT
R
C
T RT
H
RT
H G
RT
G
00
10
0
00
and
RT
G K
∆−=ln
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The !receding e5uation ma e reorgani)ed so as to factor
into three terms , each re!resenting a asic contriution
to its value :
K = K 0 K
! K
"
K 0 re!resents the e5uilirium constant at reference
tem!erature T 0:
∆−≡
0
00
RT G K
−∆
=T
T
RT
H K 0
0
01 1e!
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∆−
∆−= ∫ ∫
T
T
P T
T
P
T
dT
R
C dT
R
C
T K
00
1e!2
with heat ca!acities given :
( ) ( )( ) ( )
−∆
+
+−
∆+
−
∆+
−
−∆= 2
2
20
22
0
2
02
1
2
121
@
11
2
11
lne! τ
τ
τ
τ τ
τ
τ
τ
τ τ
T
#
CT $T A K
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13.5 EVALUATION OF EQUILIBRIUM
CONSTANTS
Example 13.4
$alculate the e5uilirium constant for the va!or#!hase
hdration of ethlene at 146 and at 320A$ from data given in!!. $.
Solution 13.4
First determine values for ;, ;B, ;$, and ;C for the
reaction:
C " H
%(&) + H
"O (&) ' C
" H
OH (&)
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The meaning of ; is indicated : (C " H
OH # (C
" H
% #
( H "O. Thus, from the heat#ca!acit data of Tale $. 1:
; 3.61D # 1.424 # 3.4E0 # 1.3E@
;B (20.001 # 14.34 # 1.460 10#3 4.16E l0#3
;$ (#@.002 + 4.32 # 0.000 10#@ #1.@10 10#@
;C (#0.000 # 0.000 # 0.121 106 #0.121 106
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Galues of ; H"*
and ;G"*
at 2D.16 for the hdration reaction are
found from the heat#of#formation and 7is#energ#of#formation data
from Tale $.4:
; H"*
#236,100 # 62,610 # (#241,D1D #46,E2 H mol#1
;G"*
#1@D,40 # @D,4@0 # (#22D,6E2 #D,3ED H mol#1
For T 146 + 2E3.16 41D.16 , values of the integrals in 5. (13.1D
are:
C$P%(2D.16,41D.16I#1.3E@,4.16E#3,#1.@10#@,#0.121 +6 #23.121
C$P*(2D.16,41D.16I#1.3E@,4.16E#3,#1.@10#@,#0.121 +6 #0.0@24
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*ustitution of values into 5. (13.1D for a reference tem!erature of
2D.16 gives:
( )( ) ( )( ) [email protected]@F24.016.41D
121.23
16.41D314.D
EF2,46
16.2FD314.D
EF2,463ED,D41D
=+
−
+
−
+
+−
=
∆ RT
G
For T 320 + 2E3.16 63.16 ,
C$P%(2D.16,63.16I#1.3E@,4.16E#3,#1.@10#@,#0.121 +6
22.@32
C$P*(2D.16,63.16I#1.3E@,4.16E#3,#1.@10#@,#0.121 +6 0.01E31
=hence,
( ) ( ) ( ) ( )
16.6F3
@32.22
16.6F3314.D
EF2,46
16.2FD314.D
EF2,463ED,D6F3 =−+−+
+−=
∆
RT
G
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Finall,
J41D.16: ln K #1.36@ and K 1.443 10#1
J63.16: ln K #6.D2D@ and K 2.42 10#3
!!lication of 5s. (13.21, (13.22, and (13.24 !rovides an
alternative solution to this eam!le. B 5. (13.21,
( ) ( )3@@.2
16.2D314.D
3ED,De!0 == K
( ) ( ) 4E3.1D
16.2FD314.D
EF2,46
0
0 −=−
=∆ RT
H
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?oreover,
=ith these values, the following results are readil otained:
T K K K 0
K !
K "
K
2D.16 1 2.3@@ 1 1 2.3@@
41D.16 1.4026 2.3@@ 4.D610#3 0.D@0 1.44310#1
63.16 1.D4 2.3@@ 1.02310#4 0.E4 2.4210#3
$learl, the influence of K !, is far greater than that of K
". This
is a t!ical result, and accounts for the fact that the lines on
Fig. 13.2 are nearl linear.
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13.6 REELATION OF EQUILIBRIUM
CONSTANTS TO COMPOSITION
The standard state for gas is the ideal gas#state of the !ure
gas at the standard#state !ressure P < of 1 ar.
*ince for ideal gas : f˚ i = P˚
Thus :
P
f
f
f i
i
i99
=and K
P
f
i
v
i
i
=
∏
9
where the constant K is a function of tem!erature onl .
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For a fied tem!erature the com!osition at e5uilirium must
change with !ressure in such a wa that
( ) K P f
i
v
i
i =∏ 9
The fugacit is related to the fugacit coefficient :
P y f iii φ 99 =*ustitution of this e5uation :
( ) K P
P y
v
i
v
ii
i
−
=∏ φ 9
where
∑≡i ivv and P < is the standard Lstate !ressure if 1 ar ,
e!ressed in the same
remains constant .
units used for P .
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for a !ure s!ecies can e evaluated from a generali)ed
correlation once the e5uilirium T and P are s!ecified .
For !ressure sufficientl low or tem!erature sufficientl high,
the e5uilirium ehaves essentiall as an ideal gas
For ideal solution :
( ) K P
P
y
v
i
v
ii
i
−
=∏ φ
iφ
( ) K
P
P y
v
i
v
ii
−
=∏
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For reaction occurring in li5uid !hase :
K
f
f
i
v
i
i
i
=
∏
9
*ince iiii f - f γ =9
The fugacit ratio e!resses :
==
i
iii
i
iii
i
i
f
f -
f
f -
f
f γ
γ 9
the fugacities of li5uids are wea/ function of !ressure .
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For reaction that ta/e !lace in high !ressure
( ) ( )
( )
−= ∑∏
i
ii
i
v
ii V v
RT
P P K - i
e!γ
For low !ressure :
( ) K -i
v
iii =∏ γ
f the e5uilirium miture is an ideal solution , then .i
is unit :
( ) K -i
v
ii =∏
This sim!le relation is /nown as the law of mass action. *ince
li5uids often form nonideal solutions, e5uation aove can e
e!ected in man instances to ield !oor result .
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For s!ecies at low concentration in a5ueous solution,
%enrMs law can e use :
iii /0 f =9where
i is a constant which de!endent on tem!erature and
/i is molalit .
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13.7 EQUILIBRIUM
CONVERSIONS FOR SINGLE
REACTIONS Example 13.5
The water#gas#shift reaction, $&(g + %2&(g ' $&
2(g + %
2(g
is carried out under the different sets of conditions descried elow.
$alculate the fraction of steam reacted in each case. ssume the
miture ehaves as an ideal gas.
(aThe reactants consist of 1 mol of %2& va!or and 1 mol of $&. The
tem!erature is 1,100 and the !ressure is 1 ar.
(*ame as (a ece!t that the !ressure is 10 ar.
(*ame as (a ece!t that 2 mol of "2 is included in the reactants.
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(dThe reactants are 2 mol of %2& and 1 mol of $&. &ther
conditions are the same as in (a.
(eThe reactants are 1 mol of %2& and 2 mol of $&. &ther
conditions are the same as in (a.
(fThe initial miture consists of 1 mol of %2&, 1 mol of $&,and 1 mol of $&
2. &ther conditions are the same as in (a.
(g *ame as (a ece!t that the tem!erature is 1,@60 K .
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Solution 13.5
(a For the given reaction at 1,100 , 104>T .06, and
Fig. 13.2 !rovides the value. ln K 0 or K 1. For this reaction
01111 =−−+== ∑i
ivv . *ince the reaction miture is an ideal
1
2
22 == K y y
y y
O H CO
CO H
B 5. (13.6:
2
1 1CO y
ε −=
2
12
1
O H y ε −=
22
1CO y
ε =
22
1 H y
ε =
gas, 5. (13.2D a!!lies, and here ecomes:
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*ustitution of these values into 5. ( gives:
( )
11
2
2
=
− 1
1
ε
ε
Therefore the fraction of the steam that reacts is 0.6.
( *ince v 0 , the increase in !ressure has no effect on the
ideal#gas reaction, and ε1 is still 0.6.
or ε1 0.6
(c The "2 does not ta/e !art in the reaction, and serves onl as a
diluent. t does increase the initial numer of moles no from 2 to 4,
and the mole fractions are all reduced a factor of 2. %owever,
5. ( is unchanged and reduces to the same e!ression as
efore. Therefore, ε1 is again 0.6.
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(d n this case the mole fractions at e5uilirium are:
3
1 1
CO y
ε −
= 3
22
1
O H y
ε −
= 32
1
CO y
ε
= 32
1
H y
ε
=
and 5. ( ecomes:
( ) ( ) 121
2
=−− 11
1
ε ε
ε
The fraction of steam that reacts is then 0.@@E>2 0.333
or ε1 0.@@E
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(e%ere the e!ressions for y$& and y%2& are interchanged , ut this
leaves the e5uilirium e5uation the same as in (d. Therefore ε1
0.@@E, and the fraction of steam that reacts is 0.@@E.
(f n this case 5. ( ecomes:
( )
( ) 1
1
12 =
−
+
1
11
ε
ε ε
The fraction of steam reacted is 0.333.
or ε1 0.333
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(g t 1,@60 K , 104>T @.0@, and from Fig. 13.2, in #1.16
or 0.31@.
Therefore 5. ( ecomes:
1
2
=− 1
1
ε
ε
The reaction is eothermic, and conversion decreases with increasing
tem!erature.
or ε1 0.3@
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13. PHASE RULE AND DUHEM!S
THEOREM FOR REACTING
SYSTEM
This is !hase rule for reacting sstems.
2 = " 3 4 + " 35
where 4 is numer of !hases , " numer of chemical s!ecies
and r is numer of inde!endent chemical reactions at
e5uilirium within the sstem .
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13." MULTIREACTION EQUILIBRIA
j
i
v
i
i K f
f ji
=
∏
,9
where j is the reaction inde.
For gas !hase reaction :
j
i
v
i K P
f ji
=
∏
,9
For the e5uilirium miture is an ideal#gas,
( ) j
v
v
i K P
y j
ji
−
=∏
,