1. Chapter 17 Lecture © 2014 Pearson Education, Inc. Sherril Soman Grand Valley State University Lecture Presentation Chapter 17 Free Energy and Thermodynamics

2. © 2014 Pearson Education, Inc. First Law of Thermodynamics You can’t win! The first law of thermodynamics is that energy cannot be created or destroyed. –The total energy of the universe cannot change. –But you can transfer it from one place to another.   E universe = 0 =  E system +  E surroundings

3. © 2014 Pearson Education, Inc. First Law of Thermodynamics Conservation of energy For an exothermic reaction, “lost” heat from the system goes into the surroundings. There are two ways energy is “lost” from a system: –Converted to heat, q –Used to do work, w Energy conservation requires that the energy change in the system is equal to the heat released plus work done. –  E = q + w –  E =  H + P  V  E is a state function. –Internal energy change independent of how done

4. © 2014 Pearson Education, Inc. The Energy Tax You can’t break even! To recharge a battery with 100 kJ of useful energy will require more than 100 kJ because of the second law of thermodynamics. Every energy transition results in a “loss” of energy. –An “energy tax” demanded by nature –Conversion of energy to heat, which is “lost” by heating up the surroundings

5. © 2014 Pearson Education, Inc. Heat Tax Fewer steps generally results in a lower total heat tax.

6. © 2014 Pearson Education, Inc. Thermodynamics and Spontaneity Thermodynamics predicts whether a process will occur under the given conditions. –Processes that will occur are called spontaneous. Nonspontaneous processes require energy input to go. Spontaneity is determined by comparing the chemical potential energy of the system before the reaction with the free energy of the system after the reaction. –If the system after reaction has less potential energy than before the reaction, the reaction is thermodynamically favorable. Spontaneity ≠ fast or slow

7. © 2014 Pearson Education, Inc. Reversibility of Process Any spontaneous process is irreversible because there is a net release of energy when it proceeds in that direction. –It will proceed in only one direction. A reversible process will proceed back and forth between the two end conditions. –Any reversible process is at equilibrium. –This results in no change in free energy. If a process is spontaneous in one direction, it must be nonspontaneous in the opposite direction.

8. © 2014 Pearson Education, Inc. Comparing Potential Energy The direction of spontaneity can be determined by comparing the potential energy of the system at the start and the end.

9. © 2014 Pearson Education, Inc. Thermodynamics versus Kinetics Figure 17.4

10. © 2014 Pearson Education, Inc. Diamond → Graphite Graphite is more stable than diamond, so the conversion of diamond into graphite is spontaneous. But don’t worry, it’s so slow that your ring won’t turn into pencil lead in your lifetime (or through many of your generations).

11. © 2014 Pearson Education, Inc. Spontaneous Processes Spontaneous processes occur because they release energy from the system. Most spontaneous processes proceed from a system of higher potential energy to a system at lower potential energy. –Exothermic But there are some spontaneous processes that proceed from a system of lower potential energy to a system at higher potential energy. –Endothermic How can something absorb potential energy, yet have a net release of energy?

12. © 2014 Pearson Education, Inc. Melting Ice When a solid melts, the particles have more freedom of movement. More freedom of motion increases the randomness of the system. When systems become more random, energy is released. We call this energy, entropy.

13. © 2014 Pearson Education, Inc. Melting Ice Melting is an endothermic process, yet ice will spontaneously melt above 0 °C. More freedom of motion increases the randomness of the system. When systems become more random, energy is released. We call this energy, entropy.

14. © 2014 Pearson Education, Inc. Water Evaporating

15. © 2014 Pearson Education, Inc. Factors Affecting Whether a Reaction Is Spontaneous There are two factors that determine whether a reaction is spontaneous. They are the enthalpy change and the entropy change of the system. The enthalpy change,  H, is the difference in the sum of the internal energy and PV work energy of the reactants to the products. The entropy change,  S, is the difference in randomness of the reactants compared to the products.

16. © 2014 Pearson Education, Inc. Enthalpy Change  H generally measured in kJ/mol Stronger bonds = more stable molecules A reaction is generally exothermic if the bonds in the products are stronger than the bonds in the reactants. –Exothermic = energy released;  H is negative. A reaction is generally endothermic if the bonds in the products are weaker than the bonds in the reactants. –Endothermic = energy absorbed;  H is positive. The enthalpy change is favorable for exothermic reactions and unfavorable for endothermic reactions.

17. © 2014 Pearson Education, Inc. Entropy Entropy is a thermodynamic function that increases as the number of energetically equivalent ways of arranging the components increases, S. – S generally J/mol S = k ln W –k = Boltzmann constant = 1.38 × 10 −23 J/K –W is the number of energetically equivalent ways a system can exist. Unitless Random systems require less energy than ordered systems.

18. © 2014 Pearson Education, Inc. Salt Dissolving in Water

19. © 2014 Pearson Education, Inc. W These are energetically equivalent states for the expansion of a gas. It doesn’t matter, in terms of potential energy, whether the molecules are all in one flask, or evenly distributed. But one of these states is more probable than the other two.

20. © 2014 Pearson Education, Inc. Macrostates → Microstates This macrostate can be achieved through several different arrangements of the particles.

21. © 2014 Pearson Education, Inc. Macrostates → Microstates These microstates all have the same macrostate. So there are six different particle arrangements that result in the same macrostate.

22. © 2014 Pearson Education, Inc. Macrostates and Probability There is only one possible arrangement that gives state A and one that gives state B. There are six possible arrangements that give state C. Therefore, state C has higher entropy than either state A or state B. The macrostate with the highest entropy also has the greatest dispersal of energy. There is six times the probability of having the state C macrostate than either state A or state B.

23. © 2014 Pearson Education, Inc. Changes in Entropy,  S  S = S final − S initial Entropy change is favorable when the result is a more random system. –  S is positive. Some changes that increase the entropy are as follows: –Reactions whose products are in a more random state Solid more ordered than liquid; liquid more ordered than gas –Reactions that have larger numbers of product molecules than reactant molecules –Increase in temperature –Solids dissociating into ions upon dissolving

24. © 2014 Pearson Education, Inc. SS For a process where the final condition is more random than the initial condition,  S system is positive and the entropy change is favorable for the process to be spontaneous. For a process where the final condition is more orderly than the initial condition,  S system is negative and the entropy change is unfavorable for the process to be spontaneous.   S system  S reaction =  n(S° products ) −  n(S° reactants )

25. © 2014 Pearson Education, Inc. Entropy Change in State Change When materials change state, the number of macrostates it can have changes as well. –The more degrees of freedom the molecules have, the more macrostates are possible. –Solids have fewer macrostates than liquids, which have fewer macrostates than gases.

26. © 2014 Pearson Education, Inc. Entropy Change and State Change Figure 17.5 pg 823

27. © 2014 Pearson Education, Inc. The Second Law of Thermodynamics The second law of thermodynamics says that the total entropy change of the universe must be positive for a process to be spontaneous. –For reversible process  S univ = 0 –For irreversible (spontaneous) process  S univ > 0  S universe =  S system +  S surroundings If the entropy of the system decreases, then the entropy of the surroundings must increase by a larger amount. –When  S system is negative,  S surroundings must be positive and big for a spontaneous process.

28. © 2014 Pearson Education, Inc. Heat Flow, Entropy, and the Second Law According to the second law, heat must flow from water to ice because it results in more dispersal of heat. The entropy of the universe increases. When ice is placed in water, heat flows from the water into the ice.

29. © 2014 Pearson Education, Inc. Heat Transfer and Changes in Entropy of the Surroundings The second law demands that the entropy of the universe increase for a spontaneous process. Yet processes like water vapor condensing are spontaneous, even though the water vapor is more random than the liquid water. If a process is spontaneous, yet the entropy change of the process is unfavorable, there must have been a large increase in the entropy of the surroundings. The entropy increase must come from heat released by the system; the process must be exothermic!

30. © 2014 Pearson Education, Inc. Entropy Change in the System and Surroundings When the entropy change in a system is unfavorable (negative), the entropy change in the surroundings must be favorable (positive), and large in order to allow the process to be spontaneous. Cartoon from page 825

31. © 2014 Pearson Education, Inc. Heat Exchange and  S surroundings When a system process is exothermic, it adds heat to the surroundings, increasing the entropy of the surroundings When a system process is endothermic, it takes heat from the surroundings, decreasing the entropy of the surroundings. The amount the entropy of the surroundings changes depends on its original temperature. –The higher the original temperature, the less effect addition or removal of heat has.

32. © 2014 Pearson Education, Inc.

33. Temperature Dependence of  S surroundings When heat is added to surroundings that are cool it has more of an effect on the entropy than it would have if the surroundings were already hot. Water freezes spontaneously below 0 °C because the heat released on freezing increases the entropy of the surroundings enough to make  S positive. –Above 0 °C the increase in entropy of the surroundings is insufficient to make  S positive.

34. © 2014 Pearson Education, Inc. Quantifying Entropy Changes in Surroundings The entropy change in the surroundings is proportional to the amount of heat gained or lost. –q surroundings = −q system The entropy change in the surroundings is also inversely proportional to its temperature. At constant pressure and temperature, the overall relationship is as follows:

35. © 2014 Pearson Education, Inc. Gibbs Free Energy and Spontaneity It can be shown that −T  S univ =  H sys −T  S sys. The Gibbs free energy, G, is the maximum amount of work energy that can be released to the surroundings by a system for a constant temperature and pressure system. –Gibbs free energy is often called the chemical potential because it is analogous to the storing of energy in a mechanical system.   G sys =  H sys −T  S sys Because  S univ determines if a process is spontaneous,  G also determines spontaneity.  S univ is positive when spontaneous, so  G is negative.

36. © 2014 Pearson Education, Inc. Gibbs Free Energy,  G A process will be spontaneous when  G is negative.   G will be negative when –  H is negative and  S is positive. Exothermic and more random –  H is negative and large and  S is negative but small. –  H is positive but small and  S is positive and large. Or high temperature  G will be positive when  H is positive and  S is negative. –Never spontaneous at any temperature. When  G = 0 the reaction is at equilibrium.

37. © 2014 Pearson Education, Inc. Free Energy Change and Spontaneity

38. © 2014 Pearson Education, Inc.  G,  H, and  S

39. © 2014 Pearson Education, Inc. Standard Conditions The standard state is the state of a material at a defined set of conditions. Gas = pure gas at exactly 1 atm pressure. Solid or Liquid = pure solid or liquid in its most stable form at exactly 1 atm pressure and temperature of interest. –Usually 25 °C Solution = substance in a solution with concentration 1 M.

40. © 2014 Pearson Education, Inc. The Third Law of Thermodynamics: Absolute Entropy The absolute entropy of a substance is the amount of energy it has due to dispersion of energy through its particles. The third law states that for a perfect crystal at absolute zero, the absolute entropy = 0 J/mol ∙ K. –Therefore, every substance that is not a perfect crystal at absolute zero has some energy from entropy. –Therefore, the absolute entropy of substances is always positive.

41. © 2014 Pearson Education, Inc. Standard Absolute Entropies S° Extensive Entropies for 1 mole of a substance at 298 K for a particular state, a particular allotrope, a particular molecular complexity, a particular molar mass, and a particular degree of dissolution

42. © 2014 Pearson Education, Inc. Standard Absolute Entropies

43. © 2014 Pearson Education, Inc. Relative Standard Entropies: States The gas state has a larger entropy than the liquid state at a particular temperature. The liquid state has a larger entropy than the solid state at a particular temperature.

44. © 2014 Pearson Education, Inc. Relative Standard Entropies: Molar Mass The larger the molar mass, the larger the entropy. Available energy states are more closely spaced, allowing more dispersal of energy through the states.

45. © 2014 Pearson Education, Inc. Relative Standard Entropies: Allotropes The less constrained the structure of an allotrope is, the larger its entropy The fact that the layers in graphite are not bonded together makes it less constrained.

46. © 2014 Pearson Education, Inc. Relative Standard Entropies: Molecular Complexity Larger, more complex molecules generally have larger entropy. More energy states are available, allowing more dispersal of energy through the states.

47. © 2014 Pearson Education, Inc. “Places” for Energy in Gaseous NO

48. © 2014 Pearson Education, Inc. Relative Standard Entropies Dissolution Dissolved solids generally have larger entropy, distributing particles throughout the mixture.

49. © 2014 Pearson Education, Inc. The Standard Entropy Change,  S The standard entropy change is the difference in absolute entropy between the reactants and products under standard conditions.  Sº reaction = (∑n p Sº products ) − (∑n r Sº reactants ) –Remember, although the standard enthalpy of formation,  H f °, of an element is 0 kJ/mol, the absolute entropy at 25 °C, S°, is always positive.

50. © 2014 Pearson Education, Inc. Calculating  G  At 25 °C At temperatures other than 25  C –Assuming the change in  H o reaction and  S o reaction is negligible Or

51. © 2014 Pearson Education, Inc. Standard Free Energies of Formation The free energy of formation (  G f °) is the change in free energy when 1 mol of a compound forms from its constituent elements in their standard states. The free energy of formation of pure elements in their standard states is zero. Insert Table 17.3

52. © 2014 Pearson Education, Inc.  G Relationships If a reaction can be expressed as a series of reactions, the sum of the  G values of the individual reaction is the  G of the total reaction.  G is a state function. If a reaction is reversed, the sign of its  G value reverses. If the amount of materials is multiplied by a factor, the value of the  G is multiplied by the same factor. –The value of  G of a reaction is extensive.

53. © 2014 Pearson Education, Inc. What’s “Free” about Free Energy? The free energy is the maximum amount of energy released from a system that is available to do work on the surroundings. For many exothermic reactions, some of the heat released due to the enthalpy change goes into increasing the entropy of the surroundings, so it is not available to do work. And even some of this free energy is generally lost to heating up the surroundings.

54. © 2014 Pearson Education, Inc. Free Energy of an Exothermic Reaction C (s, graphite) + 2 H 2(g) → CH 4(g)  H° rxn = −74.6 kJ = exothermic  S° rxn = −80.8 J/K = unfavorable  G° rxn = −50.5 kJ = spontaneous  G° is less than  H° because some of the released heat energy is lost to increase the entropy of the surroundings.

55. © 2014 Pearson Education, Inc. Free Energy and Reversible Reactions The change in free energy is a theoretical limit as to the amount of work that can be done. If the reaction achieves its theoretical limit, it is a reversible reaction.

56. © 2014 Pearson Education, Inc. Real Reactions In a real reaction, some (if not most) of the free energy is “lost” as heat. Therefore, real reactions are irreversible.

57. © 2014 Pearson Education, Inc.  G under Nonstandard Conditions   G =  G  only when the reactants and products are in their standard states. – Their normal state at that temperature – Partial pressure of gas = 1 atm – Concentration = 1 M  Under nonstandard conditions,  G =  G  + RTlnQ. – Q is the reaction quotient.  At equilibrium,  G = 0.  G  = −RTlnK

58. © 2014 Pearson Education, Inc. Free Energy versus Pressure for Water

59. © 2014 Pearson Education, Inc.  Gº and K Because  G rxn = 0 at equilibrium, then  Gº = −RTln(K). When K < 1,  Gº is positive and the reaction is spontaneous in the reverse direction under standard conditions. –Nothing will happen if there are no products yet! When K > 1,  Gº is negative and the reaction is spontaneous in the forward direction under standard conditions. When K = 1,  Gº is 0 and the reaction is at equilibrium under standard conditions.

60. © 2014 Pearson Education, Inc.

61. Combining these two equations  G° =  H° − T  S°  G° = −RTln(K) It can be shown that This equation is in the form y = mx + b. The graph of ln(K) versus inverse T is a straight line with slope and y-intercept. Why Is the Equilibrium Constant Temperature Dependent?