Chapter 1: Chemical Equilibrium Part 12 SABIS Grade 11 (Level M) Chemistry


1.9 Factors which Determine Equilibrium

Factors which Determine Equilibrium







Consider how the golf ball situation shown in Figure 1.17 will change when the station wagon is driven over a bumpy road. Now the golf balls are shaken and jostled about; they roll around and collide with each other. Every now and then one of the golf balls even accumulates enough energy (through collisions) to return to the upper level of the station wagon floor. Of course, any golf ball that is bounced up tends to roll back down to the lower level a little later. As this bumpy ride continues, a state is reached in which golf balls are being jostled up to the higher level at the same rate they are rolling back down to the lower level. Then “equilibrium” exists. Some of the golf balls are on the lower level and some on the upper level. Since the rate of rolling up equals the rate of rolling down, a dynamic balance exists.





Now let us review what happens as we warm a solid substance from a very low temperature to a very high temperature. As the temperature is raised, small energy differences become unimportant. Thus, if the temperature of the solid is raised too much, the lower energy of the regular solid becomes unimportant compared with the random thermal energies. The solid melts, surrendering this energy stability in return for the randomness of the liquid state. If the temperature is raised still further, the energies of attraction among the molecules become unimportant compared with the random thermal energies. Then the liquid vaporizes, surrendering the lower potential energy afforded by the molecules remaining close together in favor of the still higher randomness of the gaseous state. If we raise the temperature still further, the energies that hold molecules together begin to become unimportant compared with random thermal energies. Finally, at extremely high energies, molecules no longer exist—all is chaos. This is the chemical situation within the Sun. Since at such high energies chemical reactions become unimportant, all chemists on the Sun are out of work. We’d better return to room temperature to apply our knowledge of equilibrium to chemical systems within our interest.