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                                                                                 Chapter 6 Equilibrium Chemistry  137

                 the most important to chemistry is the study of the changes in energy occurring
                 during a chemical reaction.
                     Consider, for example, the general equilibrium reaction shown in equation 6.1,
                 involving the solutes A, B, C, and D, with stoichiometric coefficients a, b, c, and d.
                                           aA+ bB t cC+ dD                        6.1

                 By convention, species to the left of the arrows are called reactants, and those on the
                 right side of the arrows are called products. As Berthollet discovered, writing a reac-
                 tion in this fashion does not guarantee that the reaction of A and B to produce C and
                 D is favorable. Depending on initial conditions, the reaction may move to the left, to
                 the right, or be in a state of equilibrium. Understanding the factors that determine
                 the final position of a reaction is one of the goals of chemical thermodynamics.
                     Chemical systems spontaneously react in a fashion that lowers their overall free
                 energy. At a constant temperature and pressure, typical of many bench-top chemi-
                 cal reactions, the free energy of a chemical reaction is given by the Gibb’s free en-  Gibb’s free energy
                 ergy function                                                           A thermodynamic function for systems
                                                                                         at constant temperature and pressure
                                            ∆G = ∆H – T ∆S                        6.2    that indicates whether or not a reaction
                                                                                         is favorable (∆G < 0), unfavorable
                 where T is the temperature in kelvins, and ∆G, ∆H, and ∆S are the differences in the  (∆G > 0), or at equilibrium (∆G = 0).
                 Gibb’s free energy, the enthalpy, and the entropy between the products and reactants.
                     Enthalpy is a measure of the net flow of energy, as heat, during a chemical re-  enthalpy
                 action. Reactions in which heat is produced have a negative ∆H and are called  A change in enthalpy indicates the heat
                 exothermic. Endothermic reactions absorb heat from their surroundings and have a  absorbed or released during a chemical
                 positive ∆H. Entropy is a measure of randomness, or disorder. The entropy of an  reaction at constant pressure.
                 individual species is always positive and tends to be larger for gases than for solids
                 and for more complex rather than simpler molecules. Reactions that result in a  entropy
                                                                                         A measure of disorder.
                 large number of simple, gaseous products usually have a positive ∆S.
                     The sign of ∆G can be used to predict the direction in which a reaction moves
                 to reach its equilibrium position. A reaction is always thermodynamically favored
                 when enthalpy decreases and entropy increases. Substituting the inequalities ∆H <0
                 and ∆S > 0 into equation 6.2 shows that ∆G is negative when a reaction is thermo-
                 dynamically favored. When ∆G is positive, the reaction is unfavorable as written
                 (although the reverse reaction is favorable). Systems at equilibrium have a ∆G
                 of zero.
                     As a system moves from a nonequilibrium to an equilibrium position, ∆G must
                 change from its initial value to zero. At the same time, the species involved in the
                 reaction undergo a change in their concentrations. The Gibb’s free energy, there-
                 fore, must be a function of the concentrations of reactants and products.
                     As shown in equation 6.3, the Gibb’s free energy can be divided into two terms.
                                          ∆G = ∆G°+ RT ln Q                       6.3
                 The first term, ∆G°, is the change in Gibb’s free energy under standard-state condi-  standard state
                 tions; defined as a temperature of 298 K, all gases with partial pressures of 1 atm, all  Condition in which solids and liquids are
                 solids and liquids pure, and all solutes present with 1 M concentrations. The second  in pure form, gases have partial pressures
                                                                                         of 1 atm, solutes have concentrations of
                 term, which includes the reaction quotient, Q, accounts for nonstandard-state pres-
                                                                                         1 M, and the temperature is 298 K.
                 sures or concentrations. For reaction 6.1 the reaction quotient is
                                                    c
                                                  CD
                                                 [] [ ] d
                                             Q =    a  b                          6.4
                                                     B
                                                  A
                                                  [] [ ]
                 where the terms in brackets are the molar concentrations of the solutes. Note that
                 the reaction quotient is defined such that the concentrations of products are placed
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