Chapter 19 Chemical Thermodynamics

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Transcript Chapter 19 Chemical Thermodynamics

Topic 9 Chapter 18 Chemical Thermodynamics

Chemical Thermodynamics © 2009, Prentice-Hall, Inc.

First Law of Thermodynamics • You will recall from Chapter 6 that energy cannot be created nor destroyed.

• Therefore, the total energy of the universe is a constant.

• Energy can, however, be converted from one form to another or transferred from a system to the surroundings or vice versa.

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Spontaneous Processes • Spontaneous processes are those that can proceed without any outside intervention.

• The gas in vessel

B

will spontaneously effuse into vessel

A

, but once the gas is in both vessels, it will

not

spontaneously return to vessel

B

.

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Spontaneous Processes Processes that are spontaneous in one direction are nonspontaneous in the reverse direction.

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Spontaneous Processes • Processes that are spontaneous at one temperature may be nonspontaneous at other temperatures.

• Above 0  C it is spontaneous for ice to melt.

• Below 0  C the reverse process is spontaneous.

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Reversible Processes In a reversible process the system changes in such a way that the system and surroundings can be put back in their original states by exactly reversing the process.

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Irreversible Processes • Irreversible processes cannot be undone by exactly reversing the change to the system.

• Spontaneous processes are irreversible .

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Entropy •

Entropy

(

S

) is a term coined by Rudolph Clausius in the 19th century.

• Clausius was convinced of the significance of the ratio of heat delivered and the temperature at which it is delivered, .

T

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Entropy • Entropy can be thought of as a measure of the randomness of a system .

• It is related to the various modes of motion in molecules.

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Entropy • Like total energy,

E

, and enthalpy,

H

, entropy is a state function .

• Therefore, 

S

=

S

final 

S

initial Chemical Thermodynamics © 2009, Prentice-Hall, Inc.

Entropy For a process occurring at constant temperature (an isothermal process), the change in entropy is equal to the heat that would be transferred if the process were reversible divided by the temperature: 

S

=

q

rev

T

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Second Law of Thermodynamics The second law of thermodynamics states that the entropy of the universe increases for spontaneous processes , and the entropy of the universe does not change for reversible processes.

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Second Law of Thermodynamics In other words: For reversible processes: 

S

univ = 

S

system + 

S

surroundings = 0 For irreversible processes: 

S

univ = 

S

system + 

S

surroundings > 0 Chemical Thermodynamics © 2009, Prentice-Hall, Inc.

Second Law of Thermodynamics These last truths mean that as a result of all spontaneous processes the entropy of the universe increases .

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Entropy on the Molecular Scale • Ludwig Boltzmann described the concept of entropy on the molecular level.

• Temperature is a measure of the average kinetic energy of the molecules in a sample.

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Entropy on the Molecular Scale • Molecules exhibit several types of motion: – Translational : Movement of the entire molecule from one place to another.

– Vibrational : Periodic motion of atoms within a molecule.

– Rotational : Rotation of the molecule on about an axis or rotation about  bonds.

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Entropy on the Molecular Scale • Boltzmann envisioned the motions of a sample of molecules at a particular instant in time.

– This would be akin to taking a snapshot of all the molecules.

• He referred to this sampling as a microstate of the thermodynamic system.

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Entropy on the Molecular Scale • Each thermodynamic state has a specific number of microstates,

W

, associated with it.

• Entropy is where

k S

=

k

ln

W

is the Boltzmann constant, 1.38  10  23 J/K.

Chemical Thermodynamics © 2009, Prentice-Hall, Inc.

Entropy on the Molecular Scale • The change in entropy for a process, then, is 

S

=

k

ln

W

final 

k

ln

W

initial 

S

=

k

ln ln

W

final ln

W

initial • Entropy increases with the number of microstates in the system.

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Entropy on the Molecular Scale • The number of microstates and, therefore, the entropy tends to increase with increases in – Temperature.

– Volume.

– The number of independently moving molecules.

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Entropy and Physical States • Entropy increases with the freedom of motion of molecules.

• Therefore,

S

(

g

) >

S

(

l

) >

S

(

s

) Chemical Thermodynamics © 2009, Prentice-Hall, Inc.

Solutions Generally, when a solid is dissolved in a solvent, entropy increases.

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Entropy Changes • In general, entropy increases when – Gases are formed from liquids and solids; – Liquids or solutions are formed from solids; – The number of gas molecules increases; – The number of moles increases.

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Third Law of Thermodynamics The entropy of a pure crystalline substance at absolute zero is 0.

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Standard Entropies • These are molar entropy values of substances in their standard states.

• Standard entropies tend to increase with increasing molar mass.

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Standard Entropies Larger and more complex molecules have greater entropies.

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Entropy Changes Entropy changes for a reaction can be estimated in a manner analogous to that by which 

H

is estimated: 

S

 = 

n

S

 (products) — 

m

S

 (reactants) where

n

and

m

are the coefficients in the balanced chemical equation.

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Entropy Changes in Surroundings • Heat that flows into or out of the system changes the entropy of the surroundings.

• For an isothermal process: 

S

surr = 

q

sys

T

• At constant pressure,

q

sys 

H

 for the system.

is simply Chemical Thermodynamics © 2009, Prentice-Hall, Inc.

Entropy Change in the Universe • The universe is composed of the system and the surroundings.

• Therefore, 

S

universe = 

S

system + 

S

surroundings • For spontaneous processes 

S

universe > 0 Chemical Thermodynamics © 2009, Prentice-Hall, Inc.

Entropy Change in the Universe • Since 

S

surroundings and

q

system 

q

system

T

= 

H

system This becomes: 

S

universe

=

S

system + 

H

system

T

Multiplying both sides by 

T

, we get 

T

S

universe = 

H

system 

T

S

system Chemical Thermodynamics © 2009, Prentice-Hall, Inc.

Gibbs Free Energy • 

T

S

universe energy, 

G

.

is defined as the Gibbs free • When 

S

negative.

universe is positive, 

G

is • Therefore, when 

G

is negative, a process is spontaneous.

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Gibbs Free Energy 1. If 

G

is negative, the forward reaction is spontaneous.

2. If 

G

is 0, the system is at equilibrium.

3. If 

G

is positive, the reaction is spontaneous in the reverse direction.

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Standard Free Energy Changes Analogous to standard enthalpies of formation are standard free energies of formation, 

G

f

.

G

 = 

n

G

f

(products)  

m

G

f

(reactants) where

n

and

m

coefficients.

are the stoichiometric Chemical Thermodynamics © 2009, Prentice-Hall, Inc.

Free Energy Changes At temperatures other than 25 ° C, 

G

° = 

H

 

T

S

 How does 

G

 change with temperature?

Chemical Thermodynamics © 2009, Prentice-Hall, Inc.

Free Energy and Temperature • There are two parts to the free energy equation:  

H

 — the enthalpy –

T

S

 — the entropy term term • The temperature dependence of free energy, then comes from the entropy term.

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Free Energy and Temperature Chemical Thermodynamics © 2009, Prentice-Hall, Inc.

Free Energy and Equilibrium Under any conditions, standard or nonstandard, the free energy change can be found this way: 

G

= 

G

 +

RT

ln

Q

(Under standard conditions, all concentrations are 1

M

, so

Q

= 1 and ln

Q

= 0; the last term drops out.)

R

is the gas constant (8.314 J/K • mol)

T

is the absolute temperature (K)

Q

is the reaction quotient (Products / Reactants) Chemical Thermodynamics © 2009, Prentice-Hall, Inc.

Free Energy and Equilibrium • At equilibrium,

Q

=

K

, and 

G

= 0.

• The equation becomes 0 = 

G

 +

RT

ln

K

• Rearranging, this becomes 

G

 = 

RT

ln

K

or,

K

= e 

G

RT

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G 0

= 

RT

ln

K

Chemical Thermodynamics 18.6

© 2009, Prentice-Hall, Inc.

Energetics of Ionic Bonding By accounting for all three energies (ionization energy, electron affinity, and lattice energy), we can get a good idea of the energetics involved in such a process.

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Covalent Bond Strength • Most simply, the strength of a bond is measured by determining how much energy is required to break the bond.

• This is the bond enthalpy .

• The bond enthalpy for a Cl-Cl bond,

D

(Cl-Cl), is measured to be 242 kJ/mol.

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Bond Enthalpy and Bond Length • We can also measure an average bond length for different bond types.

• As the number of bonds between two atoms increases, the bond length decreases.

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Average Bond Enthalpies • This table lists the average bond enthalpies for many different types of bonds.

• Average bond enthalpies are positive, because bond breaking is an endothermic process.

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Average Bond Enthalpies NOTE: These are

average

bond enthalpies, not absolute bond enthalpies; the C-H bonds in methane, CH 4 , will be a bit different than the C-H bond in chloroform, CHCl 3 .

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Enthalpies of Reaction • Yet another way to estimate 

H

for a reaction is to compare the bond enthalpies of bonds broken to the bond enthalpies of the new bonds formed .

• In other words, 

H rxn

=  (bond enthalpies of bonds broken)  (bond enthalpies of bonds formed) Chemical Thermodynamics © 2009, Prentice-Hall, Inc.

Enthalpies of Reaction CH 4 (

g

) + Cl 2 (

g

)  CH 3 Cl (

g

) + HCl (

g

) In this example, one C-H bond and one Cl-Cl bond are broken; one C-Cl and one H-Cl bond are formed.

Chemical Thermodynamics © 2009, Prentice-Hall, Inc.

Enthalpies of Reaction So, 

H

H

= [

D

= Reactants - Products (C-H) +

D

(Cl-Cl)] - [

D

(C-Cl) +

D

(H-Cl)] = [(413 kJ) + (242 kJ)] - [(328 kJ) + (431 kJ)] = (655 kJ) - (759 kJ) = -104 kJ Chemical Thermodynamics © 2009, Prentice-Hall, Inc.