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17-1 CHEM 102, Fall 2014 LA TECH Instructor: Dr. Upali Siriwardane e-mail: [email protected] Office: CTH 311 Phone 257-4941 Office Hours: M,W 8:00-9:30 & 11:00-12:30 am; Tu,Th,F 8:00 - 10:00 am. or by appointment. Test Dates: 10:00-11:15 am., CTH 328 Chemistry 102(02) Fall 2014 September 23, 2014 (Test 1): Chapter 13 October 16, 2014 (Test 2): Chapter 14 &15 November 11, 2014 (Test 3) Chapter 16 &17 November 13, 2014 (Make-up test) comprehensive: Chapters 13-17

Chemistry 102(01) Spring 2014

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Chemistry 102(01) Spring 2014. Instructor: Dr. Upali Siriwardane e-mail : [email protected] Office : CTH 311 Phone 257-4941 Office Hours : M,W 8:00-9:00 & 11:00-12:00 am; Tu,Th,F 9:30 - 11:30 am. or by appointment.  Test Dates : 9:30-10:45 am., CTH 328. - PowerPoint PPT Presentation

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Page 1: Chemistry  102(01) Spring 2014

17-1CHEM 102, Fall 2014 LA TECH

Instructor: Dr. Upali Siriwardane

e-mail: [email protected]

Office: CTH 311

Phone 257-4941

Office Hours: M,W 8:00-9:30 & 11:00-12:30 am;

Tu,Th,F 8:00 - 10:00 am. or by appointment. 

Test Dates: 10:00-11:15 am., CTH 328

Chemistry 102(02) Fall 2014

September 23, 2014 (Test 1): Chapter 13

October 16, 2014 (Test 2): Chapter 14 &15

November 11, 2014 (Test 3) Chapter 16 &17

November 13, 2014 (Make-up test) comprehensive:

Chapters 13-17

Page 2: Chemistry  102(01) Spring 2014

17-2CHEM 102, Fall 2014 LA TECH

Chapter 6. Thermochemistry

6.1 Chemical Hand Warmers 2316.2 The Nature of Energy: Key Definitions 2326.3 The First Law of Thermodynamics: There Is No Free Lunch 2346.4 Quantifying Heat and Work 2406.5 Measuring for Chemical Reactions: Constant-Volume Calorimetry2466.6 Enthalpy: The Heat Evolved in a Chemical Reaction at Constant

Pressure 249

6.7 Constant-Pressure Calorimetry: Measuring 2536.8 Relationships Involving

2556.9 Determining Enthalpies of Reaction from Standard Enthalpies of Formation

2576.1 0 Energy Use and the Environment 263

Page 3: Chemistry  102(01) Spring 2014

17-3CHEM 102, Fall 2014 LA TECH

Chapter 17. Free Energy and Thermodynamics17.1 Nature’s Heat Tax: You Can’t Win and You Can’t Break Even 769

17.2 Spontaneous and Nonspontaneous Processes 771

17.3 Entropy and the Second Law of Thermodynamics 773

17.4 Heat Transfer and Changes in the Entropy of the Surroundings 780

17.5 Gibbs Free Energy 784

17.6 Entropy Changes in Chemical Reactions: Calculating 788

17.7 Free Energy Changes in Chemical Reactions: Calculating 792

17.8 Free Energy Changes for Nonstandard States: The Relationship

between and 798

17.9 Free Energy and Equilibrium: Relating to the Equilibrium Constant

(K)

Page 4: Chemistry  102(01) Spring 2014

17-4CHEM 102, Fall 2014 LA TECH

What forms of energy are found in the Universe?mechanical thermalelectrical Lightnuclearmass: E = mc2

others yet to discover

Page 5: Chemistry  102(01) Spring 2014

17-5CHEM 102, Fall 2014 LA TECH

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.

Page 6: Chemistry  102(01) Spring 2014

17-6CHEM 102, Fall 2014 LA TECH

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.

Page 7: Chemistry  102(01) Spring 2014

17-7CHEM 102, Fall 2014 LA TECH

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

Page 8: Chemistry  102(01) Spring 2014

17-8CHEM 102, Fall 2014 LA TECH

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 )

How is Internal Energy, DU measured?

Page 9: Chemistry  102(01) Spring 2014

17-9CHEM 102, Fall 2014 LA TECH

EnthalpyHeat changes at constant pressure

during chemical reactionsThermochemical equation. eg.

H2 (g) + O2 (g) ---> 2H2O(l) DH =- 256 kJ; DH is called the enthalpy of reaction.if DH is + reaction is called endothermicif DH is - reaction is called exothermic

Page 10: Chemistry  102(01) Spring 2014

17-10CHEM 102, Fall 2014 LA TECH

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

Entropy, S

Page 11: Chemistry  102(01) Spring 2014

17-11CHEM 102, Fall 2014 LA TECH

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

Page 12: Chemistry  102(01) Spring 2014

17-12CHEM 102, Fall 2014 LA TECH

DGo = DHo - T DSo

1. If DH is negative it helps product to be favored2. If DS is positive it helps product to be favored 3. If DG is negative reaction is product favored Gibbs free energy change = difference between the enthalpy of a system and the product of its absolute temperature and entropypredictor of spontaneity Total energy change of the system -

energy lost in disordering the system

Gibbs Free Energy, G

Page 13: Chemistry  102(01) Spring 2014

17-13CHEM 102, Fall 2014 LA TECH

Thermodynamics Standard States The thermodynamic standard state of 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°

Page 14: Chemistry  102(01) Spring 2014

17-14CHEM 102, Fall 2014 LA TECH

Hydrogen ΔHof

(kJ/mol)ΔGo

f (kJ/mol) So (J/mol K)

H2 (g) 0 0 130.7H (g) 218.0 203.2 114.7

H2O (l) -285.8 -237.1 69.9H2O (g) -241.8 -228.6 188.8H2O2 (l) -187.8 -120.4 109.6

Standard Thermodynamic Data

ΔHo

f - Standard Enthalpy of Formation

ΔGo

f - Standard Free Energy of Formation

So

- Standard Free Energy of Formation

Page 15: Chemistry  102(01) Spring 2014

17-15CHEM 102, Fall 2014 LA TECH

Standard Molar Entropy Values

Page 16: Chemistry  102(01) Spring 2014

17-16CHEM 102, Fall 2014 LA TECH

Chemical Thermodynamicsspontaneous reaction – reaction which

proceed without external assistance once started

chemical thermodynamics helps predict which reactions are spontaneous

Page 17: Chemistry  102(01) Spring 2014

17-17CHEM 102, Fall 2014 LA TECH

Will the rearrangement of a system decrease its energy?

If yes, system is favored to react — a product-favored system.

Most product-favored reactions are exothermic.Often referred to as spontaneous reactions.“Spontaneous” does not imply anything about time for

reaction to occur. Kinetic factors are more important for certain reactions.

Thermodynamics

Page 18: Chemistry  102(01) Spring 2014

17-18CHEM 102, Fall 2014 LA TECH

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):

Page 19: Chemistry  102(01) Spring 2014

17-19CHEM 102, Fall 2014 LA TECH

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

Page 20: Chemistry  102(01) Spring 2014

17-20CHEM 102, Fall 2014 LA TECH

2) Give the definitions of the following:

a) Zeroth Law of thermodynamics:

b) First Law of thermodynamics:

 

c) Second Law of thermodynamics:

 

d) Third Law of thermodynamics:

Page 21: Chemistry  102(01) Spring 2014

17-21CHEM 102, Fall 2014 LA TECH

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

system surroundings

universe

Boundary?

Page 22: Chemistry  102(01) Spring 2014

17-22CHEM 102, Fall 2014 LA TECH

Types of Systems

Isolated system

no mass or energy exchange

Closed system

only energy exchange

Open system

both mass and energy exchange

Page 23: Chemistry  102(01) Spring 2014

17-23CHEM 102, Fall 2014 LA TECH

Universe = System + Surrounding

Why is it necessary to divide Universe into System and Surrounding

Page 24: Chemistry  102(01) Spring 2014

17-24CHEM 102, Fall 2014 LA TECH

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)

Page 25: Chemistry  102(01) Spring 2014

17-25CHEM 102, Fall 2014 LA TECH

Second Law of ThermodynamicsIn the universe the ENTROPY cannot decrease for

any spontaneous processThe entropy of the universe strives for a

maximumin any spontaneous process, the entropy of the

universe increasesfor product-favored processDSuniv = DSsys + DSsurr

DSuniverse = ( Ssys + Ssurr) > 0 DSuniv = entropy of the UniverseDSsys = entropy of the SystemDSsurr = entropy of the Surrounding

universe

system surroundings

Page 26: Chemistry  102(01) Spring 2014

17-26CHEM 102, Fall 2014 LA TECH

Entropy of the UniverseVarious ways Dsuniv could become +

DSuniv = DSsys + DSsurr

Dsuniv DSsys DSsurr

+ + ++ +(DSsys>DSsurr) - + + (DSsurr>DSsys)

Page 27: Chemistry  102(01) Spring 2014

17-27CHEM 102, Fall 2014 LA TECH

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

DSuniv = DSsys + DSsurr

+    

+    

+    

Page 28: Chemistry  102(01) Spring 2014

17-28CHEM 102, Fall 2014 LA TECH

Entropy and Dissolving

Page 29: Chemistry  102(01) Spring 2014

17-29CHEM 102, Fall 2014 LA TECH

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: d) shuffling a deck of cards:

e) raking and burning leaves in the fall:

Page 30: Chemistry  102(01) Spring 2014

17-30CHEM 102, Fall 2014 LA TECH

Expansion of a GasThe positional

probability is higher when particles are dispersed over a larger volume

Matter tends to expand unless it is restricted

Page 31: Chemistry  102(01) Spring 2014

17-31CHEM 102, Fall 2014 LA TECH

Gas Expansion and Probability

Page 32: Chemistry  102(01) Spring 2014

17-32CHEM 102, Fall 2014 LA TECH

Entropies of Solid, Liquidand Gas Phases

S (gases) > S (liquids) > S (solids)

Page 33: Chemistry  102(01) Spring 2014

17-33CHEM 102, Fall 2014 LA TECH

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.

  

Page 34: Chemistry  102(01) Spring 2014

17-34CHEM 102, Fall 2014 LA TECH

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

Page 35: Chemistry  102(01) Spring 2014

17-35CHEM 102, Fall 2014 LA TECH

Entropy and Molecular Structure

Page 36: Chemistry  102(01) Spring 2014

17-36CHEM 102, Fall 2014 LA TECH

Entropy, S

Entropies of ionic solids depend on coulombic attractions.

So

(J/K•mol)

MgO 26.9

NaF 51.5

Page 37: Chemistry  102(01) Spring 2014

17-37CHEM 102, Fall 2014 LA TECH

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

Page 38: Chemistry  102(01) Spring 2014

17-38CHEM 102, Fall 2014 LA TECH

Entropy of a Solution of a Gas

Page 39: Chemistry  102(01) Spring 2014

17-39CHEM 102, Fall 2014 LA TECH

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)

Page 40: Chemistry  102(01) Spring 2014

17-40CHEM 102, Fall 2014 LA TECH

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 +

Page 41: Chemistry  102(01) Spring 2014

17-41CHEM 102, Fall 2014 LA TECH

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

Page 42: Chemistry  102(01) Spring 2014

17-42CHEM 102, Fall 2014 LA TECH

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)

Page 43: Chemistry  102(01) Spring 2014

17-43CHEM 102, Fall 2014 LA TECH

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)

Page 44: Chemistry  102(01) Spring 2014

17-44CHEM 102, Fall 2014 LA TECH

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

mol•J/K 109+ = K 373.15

J/mol 40,700 = Tq = SD

Page 45: Chemistry  102(01) Spring 2014

17-45CHEM 102, Fall 2014 LA TECH

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

Page 46: Chemistry  102(01) Spring 2014

17-46CHEM 102, Fall 2014 LA TECH

Phase TransitionsHeat of Fusionenergy associated with phase transition solid-to-

liquid or liquid-to-solidDGfusion = 0 = DHfusion - T DSfusion

0 = DHfusion - T DSfusion

DHfusion = T DSfusion

Heat of Vaporizationenergy associated with phase transition gas-to-

liquid or liquid-to-gasDHvaporization = T DSvaporization

Page 47: Chemistry  102(01) Spring 2014

17-47CHEM 102, Fall 2014 LA TECH

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.

Page 48: Chemistry  102(01) Spring 2014

17-48CHEM 102, Fall 2014 LA TECH

Can calc. that DHo

rxn = DHosystem = -571.7 kJ

2 H2(g) + O2(g) 2 H2O(liq)DSo

sys = -326.9 J/KEntropy Changes in the Surroundings

TH-

= T

q = systemsurrgssurroundin

DD oS

K 298.15J/kJ) kJ)(1000 (-571.7 - = gssurroundin

oSD

= +1917 J/K

2nd Law of Thermodynamics

Page 49: Chemistry  102(01) Spring 2014

17-49CHEM 102, Fall 2014 LA TECH

2 H2(g) + O2(g) 2 H2O(liq)DSo

sys = -326.9 J/KDSo

surr = +1917 J/KDSo

uni = +1590. J/KThe entropy of the universe is increasing, so

the reaction is product-favored.

2nd Law of Thermodynamics

Page 50: Chemistry  102(01) Spring 2014

17-50CHEM 102, Fall 2014 LA TECH

Gibbs Free Energy, GDSuniv = DSsurr + DSsys

Multiply through by (-T)-TDSuniv = DHsys - TDSsys

-TDSuniv = DGsystem

Under standard conditions —

DGo = DHo - TDSo

D S univ = -D H sys

T + D S sys

Page 51: Chemistry  102(01) Spring 2014

17-51CHEM 102, Fall 2014 LA TECH

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

Page 52: Chemistry  102(01) Spring 2014

17-52CHEM 102, Fall 2014 LA TECH

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 DSuni and temperature?  

Page 53: Chemistry  102(01) Spring 2014

17-53CHEM 102, Fall 2014 LA TECH

The sign of DG indicates whether a reaction will occur spontaneously.

+ Not spontaneous

0 At equilibrium

- Spontaneous

The fact that the effect of DS will vary as a function of temperature is important.

This can result in changing the sign of DG.

Free energy, DG

Page 54: Chemistry  102(01) Spring 2014

17-54CHEM 102, Fall 2014 LA TECH

The sign of DG indicates whether a reaction will occur spontaneously.

Therefore Ecell value have to be + (positive) for spontaneous redox reaction

DG = -nFEcell

n = number of electrons transferred

F = Faraday constant ((96500 C/mol)

Ecell = E½(cathode)- E½(anode)

DG and Ecell

Page 55: Chemistry  102(01) Spring 2014

17-55CHEM 102, Fall 2014 LA TECH

How do you calculate DG at different T and PDG = DGo + RT ln Q Q = reaction quotientat equilibrium DG = 00 = DGo + RT ln K DGo = - RT ln KIf you know DGo you could calculate K or

vice versa.

Nerst Equation, since DG = -nFEcell

Page 56: Chemistry  102(01) Spring 2014

17-56CHEM 102, Fall 2014 LA TECH

11) Define the following: d) How you decided from the sign of DG whether and

chemical reaction is?  i) Spontaneous ii) Never take place iii) Equilibrium e) How is Gibbs Free Energy change (DG°) related to Ecell:

f) How is non standard (DG) related to (DG°) and Q (reaction quotient)

Page 57: Chemistry  102(01) Spring 2014

17-57CHEM 102, Fall 2014 LA TECH

11) Define the following:g) How is standard (DG°) related to Keq (equilibrium constant)?

Page 58: Chemistry  102(01) Spring 2014

17-58CHEM 102, Fall 2014 LA TECH

Gibbs Free Energy, G

DGo = DHo - TDSo

DHo DSo DGo Reactionexo(-) increase(+) - Prod-favoredendo(+) decrease(-) + React-

favoredexo(-) decrease(-) ? T dependentendo(+) increase(+) ? T

dependent

Page 59: Chemistry  102(01) Spring 2014

17-59CHEM 102, Fall 2014 LA TECH

12) Predict the DGsys changes for different signs of DHsys and DSsys at low/high temperatures for the equation:

DGsys = DHsys - TDSsys

  DGsys DHsys - DTDSsys

a)      

b)      

c)      

d)