1 / 27

Chapter 16

Chapter 16. Spontaneity, entropy and free energy. Spontaneous. A reaction that will occur without outside intervention. We can’t determine how fast. We need both thermodynamics and kinetics to describe a reaction completely. Thermodynamics compares initial and final states.

andrew
Download Presentation

Chapter 16

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. Chapter 16 Spontaneity, entropy and free energy

  2. Spontaneous • A reaction that will occur without outside intervention. • We can’t determine how fast. • We need both thermodynamics and kinetics to describe a reaction completely. • Thermodynamics compares initial and final states. • Kinetics describes pathway between.

  3. Thermodynamics • 1st Law- the energy of the universe is constant. • Keeps track of thermodynamics doesn’t correctly predict spontaneity. • Entropy (S) is disorder or randomness • 2nd Law the entropy of the universe increases.

  4. Entropy • Defined in terms of probability. • Substances take the arrangement that is most likely. • The most likely is the most random. • Calculate the number of arrangements for a system.

  5. 2 possible arrangements • 50 % chance of finding the left empty

  6. 4 possible arrangements • 25% chance of finding the left empty • 50 % chance of them being evenly dispersed

  7. 4 possible arrangements • 8% chance of finding the left empty • 50 % chance of them being evenly dispersed

  8. Gases • Gases completely fill their chamber because there are many more ways to do that than to leave half empty. • Ssolid <Sliquid <<Sgas • there are many more ways for the molecules to be arranged as a liquid than a solid. • Gases have a huge number of positions possible.

  9. Entropy • Solutions form because there are many more possible arrangements of dissolved pieces than if they stay separate. • 2nd Law • DSuniv = DSsys + DSsurr • If DSuniv is positive the process is spontaneous. • If DSuniv is negative the process is spontaneous in the opposite direction.

  10. For exothermic processes DSsurr is positive. • For endothermic processes DSsurr is negative. • Consider this process H2O(l)® H2O(g) • DSsys is positive • DSsurr is negative • DSuniv depends on temperature.

  11. Temperature and Spontaneity • Entropy changes in the surroundings are determined by the heat flow. • An exothermic process is favored because by giving up heat the entropy of the surroundings increases. • The size of DSsurr depends on temperature • DSsurr = -DH/T

  12. - + ? DSsurr DSuniv Spontaneous? DSsys - - - No, Reverse + + + Yes + - ? At High temp. At Low temp.

  13. Gibb's Free Energy • G=H-TS • Never used this way. • DG=DH-TDS at constant temperature • Divide by -T • -DG/T = -DH/T-DS • -DG/T = DSsurr + DS • -DG/T = DSuniv • If DG is negative at constant T and P, the Process is spontaneous.

  14. Let’s Check • For the reaction H2O(s) ® H2O(l) • DSº = 22.1 J/K mol DHº =6030 J/mol • Calculate DG at 10ºC and -10ºC • Look at the equation DG=DH-TDS • Spontaneity can be predicted from the sign of DH and DS.

  15. Spontaneous? DS DH DG=DH-TDS + - At all Temperatures At high temperatures, “entropy driven” + + At low temperatures, “enthalpy driven” - - Not at any temperature, Reverse is spontaneous - +

  16. Third Law of Thermo • The entropy of a pure crystal at 0 K is 0. • Gives us a starting point. • All others must be>0. • Standard Entropies Sº ( at 298 K and 1 atm) of substances are listed. • Products - reactants to find DSº (a state function). • More complex molecules higher Sº.

  17. Free Energy in Reactions • DGº = standard free energy change. • Free energy change that will occur if reactants in their standard state turn to products in their standard state. • Can’t be measured directly, can be calculated from other measurements. • DGº=DHº-TDSº • Use Hess’s Law with known reactions.

  18. Free Energy in Reactions • There are tables of DGºf . • Products-reactants because it is a state function. • The standard free energy of formation for any element in its standard state is 0. • Remember- Spontaneity tells us nothing about rate.

  19. Spontaneous? DS DH DG=DH-TDS + - At all Temperatures At high temperatures, “entropy driven” + + At low temperatures, “enthalpy driven” - - Not at any temperature, Reverse is spontaneous - +

  20. Third Law of Thermo • The entropy of a pure crystal at 0 K is 0. • Gives us a starting point. • All others must be>0. • Standard Entropies Sº ( at 298 K and 1 atm) of substances are listed. • Products - reactants to find DSº (a state function) • More complex molecules higher Sº.

  21. Free Energy in Reactions • DGº = standard free energy change. • Free energy change that will occur if reactants in their standard state turn to products in their standard state. • Can’t be measured directly, can be calculated from other measurements. • DGº=DHº-TDSº • Use Hess’s Law with known reactions.

  22. Free Energy in Reactions • There are tables of DGºf • Products-reactants because it is a state function. • The standard free energy of formation for any element in its standard state is 0. • Remember- Spontaneity tells us nothing about rate.

  23. Free energy and Pressure • DG = DGº +RTln(Q) where Q is the reaction quotients (P of the products /P of the reactants). • CO(g) + 2H2(g) ® CH3OH(l) • Would the reaction be spontaneous at 25ºC with the H2 pressure of 5.0 atm and the CO pressure of 3.0 atm? • DGºf CH3OH(l) = -166 kJ • DGºf CO(g) = -137 kJ DGºf H2(g) = 0 kJ

  24. How far? • DG tells us spontaneity at current conditions. When will it stop? • It will go to the lowest possible free energy which may be an equilibrium. • At equilibrium DG = 0, Q = K • DGº = -RTlnK

  25. DGº K =0 =1 <0 >0 >0 <0

  26. Temperature dependence of K • DGº= -RTlnK = DHº - TDSº • ln(K) = DHº/R(1/T)+ DSº/R • A straight line of lnK vs 1/T

  27. Free energy And Work • Free energy is that energy free to do work. • The maximum amount of work possible at a given temperature and pressure. • Never really achieved because some of the free energy is changed to heat during a change, so it can’t be used to do work.

More Related