Chemical Equilibrium
In this part of the chapter, the equilibrium criterion dG]
T, p
5 0 introduced in Sec. 14.1
is used to study the equilibrium of reacting mixtures. The objective is to establish the
composition present at equilibrium for a specified temperature and pressure. An
important parameter for determining the equilibrium composition is the equilibrium
constant. The equilibrium constant is introduced and its use illustrated by several
solved examples. The discussion is concerned only with equilibrium states of reacting
systems, and no information can be deduced about the rates of reaction. Whether an
equilibrium mixture would form quickly or slowly can be determined only by con-
sidering the chemical kinetics, a topic that is not treated in this text.
14.2 Equation of Reaction Equilibrium
In Chap. 13 the conservation of mass and conservation of energy principles are applied
to reacting systems by assuming that the reactions can occur as written. However, the
extent to which a chemical reaction proceeds is limited by many factors. In general, the
composition of the products actually formed from a given set of reactants, and the relative
amounts of the products, can be determined only from experiment. Knowledge of the
composition that would be present were a reaction to proceed to equilibrium is frequently
useful, however. The equation of reaction equilibrium introduced in the present section
provides the basis for determining the equilibrium composition of a reacting mixture.
14.2.1
Introductory Case
Consider a closed system consisting initially of a gaseous mixture of hydrogen and
oxygen. A number of reactions might take place, including
1H
2
1
1
2
O
2
S
d
1H
2
O (14.18)
1H
2
S
d
2H (14.19)
1O
2
S
d
2O (14.20)
Let us consider for illustration purposes only the first of the reactions given above,
in which hydrogen and oxygen combine to form water. At equilibrium, the system
will consist in general of three components: H
2
, O
2
, and H
2
O, for not all of the hydro-
gen and oxygen initially present need be reacted. Changes in the amounts of these
components during each differential step of the reaction leading to the formation of
an equilibrium mixture are governed by Eq. 14.18. That is
dn
H
2
52dn
H
2
O
,
dn
O
2
52
1
2
dn
H
2
O
(14.21a)
where dn denotes a differential change in the respective component. The minus signs
signal that the amounts of hydrogen and oxygen present decrease when the reaction
proceeds toward the right. Equations 14.21a can be expressed alternatively as
2dn
H
2
1
5
2dn
O
2
1
2
5
dn
H
2
O
1
(14.21b)
which emphasizes that increases and decreases in the components are proportional
to the stoichiometric coefficients of Eq. 14.18.
Equilibrium is a condition of balance. Accordingly, as suggested by the direction of
the arrows in Eq. 14.18, when the system is at equilibrium, the tendency of the hydrogen
and oxygen to form water is just balanced by the tendency of water to dissociate into
oxygen and hydrogen. The equilibrium criterion dG]
T, p
5 0 can be used to determine
the composition at an equilibrium state where the temperature is T and the pressure is p.
This requires evaluation of the differential dG]
T, p
in terms of system properties.
14.2 Equation of Reaction Equilibrium 853
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