1 / 15

Lecture 8: The Second and Third Laws of Thermodynamics

Lecture 8: The Second and Third Laws of Thermodynamics. Reading: Zumdahl 10.5, 10.6 Outline Definition of the Second Law Determining D S Definition of the Third Law. The Second Law.

jewel
Download Presentation

Lecture 8: The Second and Third Laws of Thermodynamics

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Lecture 8: The Second and Third Laws of Thermodynamics Reading: Zumdahl 10.5, 10.6 Outline Definition of the Second Law Determining DS Definition of the Third Law

  2. The Second Law • The Second Law: In any spontaneous process, there is always an increase in the entropy of the universe. • From our definitions of system and surroundings: DSuniverse = DSsystem + DSsurroundings

  3. There are only three possibilities: If DSuniv > 0, then the process is spontaneous. If DSuniv < 0, then the process is spontaneous in the opposite direction. If DSuniv = 0, the system is in equilibrium. • Here’s the catch: We need to know DS for both • the system and surroundings to predict whether a • reaction will be spontaneous.

  4. Consider a reaction driven by heat flow from the surroundings at constant pressure: Exothermic Process: DSsurr = heat/T Endothermic Process: DSsurr = -heat/T (Note: sign of DS is from the surrounding’s point of view!) Heat transferred = qP,surr = - qP,system= -DHsys

  5. Example: calculating DSsur What is DSsurr for the following reaction at 298 K? Sb4O6(s) + 6C(s) 4Sb(s) + 6CO2(g) DH = 778 kJ DSsurr= -DH/T = -778 kJ/298K = -2.6 kJ/K

  6. The Third Law of Thermodynamics Recall: in determining enthalpy changes (∆H) we had standard state values to use for reference. Q: Do standard reference states exist for entropy S? The Third Law: The entropy S of a perfect crystal at absolute zero (0 degrees K ) is zero. The third law provides the reference state for use in calculating absolute entropies.

  7. What is a Perfect Crystal? Perfect crystal at 0 K, so S =0 Crystal deforms for T > 0 K, slight random motions (wiggling in place), S>0

  8. Standard Entropies With reference to this state, standard entropies have been tabulated (Appendix 4). Recall, entropy S is a state function; therefore, the entropy change for a chemical reaction can be calculated as follows:

  9. Example: calculating DS°rxn Balance the following reaction and determine DS°rxn Fe(s) + H2O(g) Fe2O3(s) + H2(g) 2Fe(s) + 3H2O(g) Fe2O3(s) + 3H2(g) DS°rxn = (S°(Fe2O3(s)) + 3S°H2(g)) - (2S°Fe(s) + 3S°H2O(g)) DS°rxn = -141.5 J/K

  10. Example: determining rxn spontaneity Is the following reaction spontaneous at 298 K? (That is to say, is DS°univ > 0?) 2Fe(s) + 3H2O(g) Fe2O3(s) + 3H2(g) DS°rxn = DS°system= -141.5 J/K DS°surr = -DH°sys/T = -DH°rxn/T DH°rxn= DH°f(Fe2O3(s)) + 3DH°f(H2(g)) - 2DH°f(Fe(s)) - 3 DH°f(H2O(g))

  11. DH°rxn= -100 kJ DS°surr = -DH°sys/T = 348 J/K DS°univ = DS°sys + DS°surr = -141.5 J/K + 348 J/K = 207.5 J/K DS°univ > 0 ; therefore, yes, the reaction is spontaneous

  12. Entropy and Phase Changes Phase Change: Reaction in which a substance goes from one phase of state to another. Example: H2O(l) H2O(g) @ 373 K Key point: phase changes are equilibrium processes such that: DSuniv = 0

  13. H2O(l) H2O(g) @ 373 K So, DS°rxn = S°(H2O(g)) - S°(H2O(l)) = 195.9 J/K - 86.6 J/K = 109.1 J/K and, DS°surr = -DHsys/T = -40.7 kJ/373 K = -109.1 J/K Therefore, DSuniv = DSsys + DSsurr = 0

  14. Another example Determine the temperature at which liquid bromine boils: Br2(l) Br2(g) DS°rxn = S°(Br2 (g)) - S°(Br2(l)) = 245.38 J/K - 152.23 J/K = 93.2 J/K

  15. DS°surr = - DS°sys = -93.2 J/K = -DHsys/T Therefore, calculate DHsys and solve for T! 0 Now, DH°rxn = DH°f(Br2(g)) - DH°f(Br2(l)) = 30.91 kJ - 0 = 30.91 kJ (standard state) Finally, -93.2 J/K = -30.91 kJ/T Tboiling = 331.6 K

More Related