1 / 57

Chemistry 102(001) Fall 2012

Chemistry 102(001) Fall 2012. CTH 328 10:00-11:15 am Instructor : Dr. Upali Siriwardane e-mail : upali@latech.edu Office : CTH 311 Phone 257-4941 Office Hours : M,W 8:00-9:00 & 11:00-12:00 am; Tu , Th , F 8:00 - 10:00am.. Exams: 10 :00-11:15 am, CTH 328.

ogden
Download Presentation

Chemistry 102(001) Fall 2012

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. Chemistry 102(001) Fall 2012 CTH 328 10:00-11:15 am Instructor: Dr. UpaliSiriwardane e-mail: upali@latech.edu Office: CTH 311 Phone 257-4941 Office Hours: M,W 8:00-9:00 & 11:00-12:00 am; Tu, Th, F 8:00 - 10:00am.. Exams: 10:00-11:15 am, CTH 328. September 27, 2012 (Test 1): Chapter 13 October 18, 2012 (Test 2): Chapter 14 &15 November 13, 2012 (Test 3):Chapter 16 &18 Optional Comprehensive Final Exam: November 15, 2012 : Chapters 13, 14, 15, 16, 17, and 18

  2. Review of Chapter 6. Energy and Chemical Reactions 6.1 The Nature of Energy 6.2 Conservation of Energy 6.3 Heat Capacity 6.4 Energy and Enthalpy 6.5 Thermochemical Equations 6.6 Enthalpy change for chemical Rections 6.7 Where does the Energy come from? 6.8 Measuring Enthalpy Changes: Calorimetry 6.9 Hess's Law 6.10 Standard Enthalpy of Formation 6.11 Chemical Fuels for Home and Industry 6.12 Food Fuels for Our Bodies

  3. Chapter 18. Thermodynamics: Directionality of Chemical Reactions 18.1 Reactant-Favored and Product-Favored Processes 18.2 Probability and Chemical Reactions 18.3 Measuring Dispersal or Disorder: Entropy 18.4 Calculating Entropy Changes 18.5 Entropy and the Second Law of Thermodynamics 18.6 Gibbs Free Energy 18.7 Gibbs Free Energy Changes and Equilibrium Constants 18.8 Gibbs Free Energy, Maximum Work, and Energy Resources 18.9 Gibbs Free Energy and Biological Systems 18.10 Conservation of Gibbs Free Energy 18.11 Thermodynamic and Kinetic Stability

  4. What forms of energy are found in the Universe? mechanical thermal electrical nuclear mass: E = mc2 others yet to discover

  5. What is 1st Law of Thermodynamics Eenergy is conserved in the Universe All forms of energy are inter-convertible and conserved Energy is neither created nor destroyed.

  6. What exactly is DH? Heat measured at constant pressure qp Chemical reactions exposed to atmosphere and are held at a constant pressure. Volume of materials or gases produced can change. Volume expansion work = -PDV DU = qp + w; DU = qp -PDV qp = DU + PDV; w = -PDV DH = DU + PDV; qp = DH(enthalpy )

  7. What is the internal energy change (DU) of a system? DU is part of energy associated with changes in atoms, molecules and subatomic particles Etotal= Eke + E pe + DU DU = heat (q) + w (work) DU = q + w DU = q -P DV; w =- P DV

  8. How is Internal Energy, DU measured? Heat measured at constant volume qv Chemical reactions take place inside a closed chamber like a bomb calorimeter. Volume of materials or gases produced can not change. ie: work = -PDV= 0 DU = qv + w qv = DU + o; w = 0 DU = qv = DU(internal energy )

  9. Enthalpy Heat changes at constant pressure during chemical reactions Thermochemical equation. eg. H2 (g) + O2 (g) ---> 2H2O(l) DH =- 256 kJ; DH is called the enthalpy of reaction. if DH is + reaction is called endothermic if DH is - reaction is called exothermic

  10. Entropy, S The thermodynamic property related to randomness is ENTROPY, S. Product-favored processes: final state is more DISORDERED or RANDOM than the original. Spontaneity is related to an increase in randomness. Reaction of K with water

  11. Physical Process” S[H2O(l)] > S[H2O(s)] at 0° C.

  12. Standard Molar Entropy Values

  13. Chemical Thermodynamics spontaneous reaction – reaction which proceed without external assistance once started chemical thermodynamics helps predict which reactions are spontaneous

  14. Thermodynamics Will the rearrangement of a system decrease its energy? If yes, system is favored to react — a product-favoredsystem. Most product-favored reactions are exothermic. Often referred to as spontaneousreactions. “Spontaneous” does not imply anything about time for reaction to occur. Kinetic factors are more important for certain reactions.

  15. Thermodynamics Standard States • The thermodynamic standard stateof a substance is its most stable pure form under • standard pressure (1 atm) and at some specific temperature (25 ºC or 298 K) • superscript circle is used to denote a thermodynamic quantity that is under standard state conditions: • ΔH = ΔH°ΔS = ΔS°ΔG = ΔG°

  16. 1) Give the definitions of the following: • a) Enthalpy (H): • b) Enthalpy change of a thermo-chemical reaction (DH): • c) Entropy of a substance (S): • d) Entropy change of a chemical reaction(DS): • e) Thermodynamic Standard State(0):

  17. Laws of Thermodynamics Zeroth: Thermal equilibrium and temperature First: The total energy of the universe is constant Second : The total entropy (S) of the universe is always increasing Third : The entropy(S) of a pure, perfectly formed crystalline substance at absolute zero is zero

  18. 2) Give the definitions of the following: • a) ZerothLaw of thermodynamics: • b) First Law of thermodynamics: • c) Second Law of thermodynamics: • d) Third Law of thermodynamics:

  19. universe system surroundings Why is it necessary to divide Universe into System and Surrounding Universe = System + Surrounding

  20. Types of Systems • Isolated system • no mass or energy exchange • Closed system • only energy exchange • Open system • both mass and energy exchange

  21. Why is it necessary to divide Universe into System and Surrounding Universe = System + Surrounding

  22. 3) Why we need to divide universe into surroundings and system for thermodynamic calculations? • Give the signs of the DH (heat) and DS (disorder) and DG ( free energy) when system lose or gain them. • Loss Gain • DH (heat) • DS (disorder) • DG ( free energy)

  23. Second Law of Thermodynamics In the universe the ENTROPY cannot decrease for any spontaneous process The entropy of the universe strives for a maximum in any spontaneous process, the entropy of the universe increases for product-favored process DSuniverse = ( Ssys + Ssurr) > 0 DSuniv = entropy of the Universe DSsys = entropy of the System DSsurr = entropy of the Surrounding DSuniv = DSsys + DSsurr

  24. Entropy of the Universe DSuniv = DSsys + DSsurr DsunivDSsysDSsurr + + + + +(DSsys>DSsurr) - + - + (DSsurr>DSsys)

  25. 4) Explain the ways that DS of the universe, DSuniv could be +.

  26. Entropy and Dissolving

  27. 5) Assign a sign to the entropy change for the following systems. • a) mixing aqueous solutions of NaCl and KNO3 together: • b) spreading grass seed on a lawn: • c) raking and bagging leaves in the fall: • shuffling a deck of cards: • e) raking and burning leaves in the fall:

  28. Expansion of a Gas The positional probability is higher when particles are dispersed over a larger volume Matter tends to expand unless it is restricted

  29. Gas Expansion and Probability

  30. S (gases) > S (liquids) > S (solids) Entropies of Solid, Liquidand Gas Phases

  31. 6) Taking following examples explain how disorder is related to a measuring positional probability) or dispersion among the allowed energy states? • a) Expansion of gases: Two gas molecules trapped in two vessels with a tube with a stop cock.

  32. 6) Taking following examples explain how disorder is related to a measuring positional probability) or dispersion among the allowed energy states. • b) Distribution of Kinetic energy at 0, 25 and 100°C for O2

  33. Entropy and Molecular Structure

  34. Entropy, S Entropies of ionic solids depend on coulombic attractions. So (J/K•mol) MgO 26.9 NaF 51.5

  35. Qualitative Guidelines for Entropy Changes Entropies of gases higher than liquids higher than solids Entropies are higher for more complex structures than simpler structures Entropies of ionic solids are inversely related to the strength of ionic forces Entropy increases when making solutions of pure solids or pure liquids in a liquid solvent Entropy decrease when making solutions of gases in a liquid

  36. Entropy of a Solution of a Gas

  37. 7) Arrange following in the order of increasing entropy? • a) C(s) (diamond) • b) C(s) (graphite) • c) O2(g) • d) CO2(g) • e) CO(g) • f) Hg(l)

  38. Entropy Change Entropy (DS) normally increase (+) for the following changes: i) Solid ---> liquid (melting) + ii) Liquid ---> gas + iii) Solid ----> gas most + iv) Increase in temperature + v) Increasing in pressure(constant volume, and temperature) + vi) Increase in volume +

  39. Qualitative prediction of DS of Chemical Reactions • Look for (l) or (s) --> (g) • If all are gases: calculate Dn Dn = Sn (gaseous prod.) - S n(gaseous reac.) N2 (g) + 3 H2 (g) --------> 2 NH3 (g) Dn = 2 - 4 = -2 If Dn is -DS is negative (decrease in S) If Dn is +DS is positive (increase in S)

  40. Predict DS! 2 C2H6(g) + 7 O2(g)--> 4 CO2(g) + 6H2O(g) 2 CO(g) + O2(g)-->2 CO2(g) HCl(g) + NH3(g)-->NH4Cl(s) H2(g) + Br2(l) --> 2 HBr(g)

  41. 8) Taking following physical and chemical changes qualitatively predict the sign of DS. • a) 2H2O (g) ------> 2 H2O (l) • b) 2H2O (g) ------> 2 H2 (g) + O2 (g) • c) N2(g) + 3 H2 (g) ------> 2 NH3 (g)

  42. Entropy Changes for Phase Changes For a phase change, DSSYS = qSYS/T (q = heat transferred) Boiling Water H2O (liq)  H2O(g) DH = q = +40,700 J/mol

  43. 9) How is entropy related to the heat and temperature?

  44. Phase Transitions Heat of Fusion energy associated with phase transition solid-to-liquid or liquid-to-solid DGfusion = 0 = DHfusion - T DSfusion 0 = DHfusion - T DSfusion DHfusion = T DSfusion Heat of Vaporization energy associated with phase transition gas-to-liquid or liquid-to-gas DHvaporization = T DSvaporization

  45. 10) The normal boiling point of benzene is 80.1°C and heat of evaporation (∆H°vap)is 30.7 kJ/mol. Calculate the ∆Ssurr (in J/K mol) for the evaporation of benzene.

  46. 2nd Law of Thermodynamics 2 H2(g) + O2(g)  2 H2O(liq) DSosys = -326.9 J/K Entropy Changes in the Surroundings Can calc. that DHorxn = DHosystem = -571.7 kJ = +1917 J/K

  47. 2nd Law of Thermodynamics 2 H2(g) + O2(g)  2 H2O(liq) DSosys = -326.9 J/K DSosurr = +1917 J/K DSouni = +1590. J/K The entropy of the universe is increasing, so the reaction is product-favored.

  48. H -D sys S = + S D D univ sys T Gibbs Free Energy, G DSuniv = DSsurr + DSsys Multiply through by (-T) -TDSuniv = DHsys - TDSsys -TDSuniv = DGsystem Under standard conditions — DGo = DHo - TDSo

  49. Gibbs Free Energy, G DGo = DHo - T DSo Gibbs free energy change = difference between the enthalpy of a system and the product of its absolute temperature and entropy predictor of spontaneity Total energy change for system - energy lost in disordering the system

  50. 11) Define the following: • a) Gibbs Free Energy (G): • b) Gibbs Free Energy change for a reaction (DG): • c) How is DGsys is related to DSuniand temperature?

More Related