chemical thermodynamics

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AP Chapter 19

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Chemical Thermodynamics. AP Chapter 19. The First Law Of Thermodynamics. Energy can not be created nor destroyed, only transferred between a system and the surroundings. The energy in the universe is constant. Energy is conserved!. Spontaneous Processes. - PowerPoint PPT Presentation

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Page 1: Chemical Thermodynamics

AP Chapter 19

Page 2: Chemical Thermodynamics

Energy can not be created nor destroyed, only transferred between a system and the surroundings.

The energy in the universe is constant.

Energy is conserved!

Page 3: Chemical Thermodynamics

Spontaneous processes occur without outside intervention.

Most reactions are spontaneous in one direction and non-spontaneous in the other direction.

This spontaneity is related to the thermodynamic path the system takes from the initial state to the final state.

Page 4: Chemical Thermodynamics

Irreversible Reactions

Page 5: Chemical Thermodynamics

Spontaneity can depend on the temperature.

Page 6: Chemical Thermodynamics

Reversible process – both the system and the surroundings can be restored to their original states by exactly reversing the process.

Irreversible processes – cannot return to the original process without a permanent change in the surroundings.

Any spontaneous process is irreversible. (It’s not spontaneous in the other direction.)

An iron nail can react with H2O and O2 to form Fe2O3, but the reverse does not happen.

Page 7: Chemical Thermodynamics

Spontaneous processes may be fast or slow.

Many forms of combustion are fast.

Conversion of a diamond to graphite is slow.

Page 8: Chemical Thermodynamics

Thermodynamics can tell us the direction and extent of a reaction, but NOT the speed of a reaction.

Page 9: Chemical Thermodynamics

A measurement of the randomness or disorder of a system.

Page 10: Chemical Thermodynamics

In any spontaneous process, there is always an increase in the entropy of the universe.

For a given change to be spontaneous, ΔSuniv must be positive.

Page 11: Chemical Thermodynamics

The change in entropy of the universe, ΔSuniv = ΔSsystem + ΔSsurroundings

In a reversible process, ΔSuniv = 0.

In an irreversible, (spontaneous) process, ΔSuniv > 0.

Entropy values: J/K

Page 12: Chemical Thermodynamics

The driving force for a spontaneous process is an increase in the entropy of the universe.

Entropy is a thermodynamic function describing the number of arrangements that are available to a system.

Nature proceeds towards the states that have the highest probability of existing.

Page 13: Chemical Thermodynamics

Molecules can undergo 3 types of motion: 1. translational motion 2. vibrational motion 3. rotational motion

A particular combination of motions and locations of the atoms in a system at a particular instant is called a microstate.

Page 14: Chemical Thermodynamics

The probability of occurrence of a particular state depends on the number of ways (microstates) in which that arrangement can be achieved.

Entropy generally increases when ◦ liquids or solutions are formed from solids◦ gases are formed from either solids or liquids◦ or the number of molecules of gas increases

during a chemical reaction.

Page 15: Chemical Thermodynamics
Page 16: Chemical Thermodynamics

The entropy (S) of a perfect crystalline solid at 0 K is zero.

Page 17: Chemical Thermodynamics
Page 18: Chemical Thermodynamics

In reactions involving gaseous molecules, the change in a positional entropy is dominated by the relative numbers of molecules of gas reactants and products

2C2H6(g) + 7O2(g) → 4CO2(g) + 6H2O(g)

9 molecules 10 moleculesΔS increases

Page 19: Chemical Thermodynamics

Entropy changes in the surroundings are primarily determined by heat flow.

Exothermic reactions in a system at constant temperature increase the entropy of the surroundings.

Endothermic reactions in a system at constant temperature decrease the entropy of the surroundings.

The transfer of a given quantity of energy as heat either to or from the surroundings has a greater impact at lower temperatures.

Page 20: Chemical Thermodynamics

ΔS°reaction = ΣnS°products - ΣnS°reactants

Entropy is an extensive property (a function of the number of moles)

Generally, the more complex the molecule, the higher the standard entropy value.

Page 21: Chemical Thermodynamics
Page 22: Chemical Thermodynamics
Page 23: Chemical Thermodynamics

Gibbs Free Energy (G) is a thermodynamic state function that combines enthalpy and entropy.

For a process at constant temperature & pressure, the sign of ΔG relates to the spontaneity of the process.

ΔG = negative, the process is spontaneous ΔG = positive, the process is not spontaneous,

but the reverse process is spontaneous.

At equilibrium, the process is reversible and ΔG is zero.

Page 24: Chemical Thermodynamics

Free energy is the amount of useful work that can be obtained from a process at constant temperature and pressure.

Page 25: Chemical Thermodynamics

Potential energy and Free energy – an analogy between the gravitational-PE change in a boulder rolling down a hill (position a) and the free energy change in a spontaneous reaction (b).The equilibrium position in (a) is given by the minimum gravitational PE available to the system. The equilibrium position in (b) is given by the minimum free energy available to the system.

Page 26: Chemical Thermodynamics

In any spontaneous process at constant temperature and pressure, the free energy always decreases.

Page 27: Chemical Thermodynamics
Page 28: Chemical Thermodynamics

Calculating Free Energy Change (G) (constant temperature and pressure)

ΔG = ΔH – TΔS ΔG is the change in free energy measure in kJ/mol) Δ H is the change in enthalpy (kJ/mol) ΔS is the change in entropy (J/mol K) T is Kelvin Temperature

Page 29: Chemical Thermodynamics
Page 30: Chemical Thermodynamics

Quantity Change in

Enthalpy

Change in

Entropy

Change in Free

Energy

Symbol ΔH ΔS ΔG

Unit kJ/mol J/mol K k J/mol

Definition Heat gained by a

system

Change in

randomness of a

system

Available useful

work

Comments + for endothermic

- for exothermic

+ for increasing

randomness

- for decreasing

randomness

+ for nonspontaneous

- for spontaneous

-ΔG = 0 at equilibrium

Summary of Important Thermodynamic Quantities

Page 31: Chemical Thermodynamics

ΔG = ΔG° + RT ln Q R is the ideal gas constant, 8.314 J/mol-K T is the absolute temperature Q is the reaction quotient that corresponds to the

reaction mixture of interest. Under standard conditions the concentrations of all the

reactants and products are equal to 1. Under standard conditions Q = 1 and therefore, ln Q = 0.

Therefore, ΔG = ΔG° under standard conditions.

Page 32: Chemical Thermodynamics

The standard free energy for any reaction is related to the equilibrium constant.

At equilibrium, ΔG = 0 and Q = K, the equilibrium constant.

At equilibrium: ΔG = -RT ln K

Page 33: Chemical Thermodynamics

The standard free energy change for the following reaction at 25°C is -118.4 kJ/mol:

KClO3(s) → KCl(s) + 3/2 O2(g) Calculate Kp for the reaction at 25°C and the

equilibrium pressure of O2 gas. ΔG° = -RT ln K -118.4 kJ/mol = -(8.314 J/mol K)(298 K)(1kJ/1000 J) ln Kp Ln Kp = 47.8 Kp = e47.8 = 5.68 x 1020

Kp = p3/2 O2

PO2 = Kp2/3 = (5.68 x 1020 )2/3 = 6.9 x 1013 atm

Page 34: Chemical Thermodynamics

ΔG° for any process can be calculated from tabulations of standard free energies of formation – see Tables in Appendix C.

Page 35: Chemical Thermodynamics