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Chapter 15 Thermodynamics. Thermodynamics is the study of “heat” “change”, specifically that accompany physical and chemical processes. Often referred to as thermochemistry . . - PowerPoint PPT Presentation

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Page 1: Chapter 15 Thermodynamics

Chapter 15Thermodynamics

Page 2: Chapter 15 Thermodynamics

Thermodynamics is the study of “heat” “change”, specifically that accompany physical and chemical processes. Often referred to as thermochemistry.

Page 3: Chapter 15 Thermodynamics

We will look at the energy that accompanies chemical changes, not just the heat, so there might be kinetic and potential energy invovled. Typically these are classified as exothermic and endothermic reactions.

Page 4: Chapter 15 Thermodynamics

An exothermic reaction releases energy (usually as heat). This means the products have less energy than the reactants, according to the law of conservation…

Σ(Ereactants) > Σ(Eproducts)

but

Σ(Ereactants) = Σ(Eproducts) + Ereleased

Page 5: Chapter 15 Thermodynamics

An endothermic reaction absorbs energy (usually as heat). This means the products have more energy than the reactants, according to the law of conservation…

Σ(Ereactants) < Σ(Eproducts)

but

Σ(Ereactants) + Eabsorbed= Σ(Eproducts)

Page 6: Chapter 15 Thermodynamics

Often energy diagrams are used to picture what is happening during these reactions. Activation energy is the energy required to start a chemical reaction.

Page 7: Chapter 15 Thermodynamics

It is important to understand how energy is conserved during chemical reactions, even when it doesn’t seem like it is. The First Law of Thermodynamics states that the total energy of the universe is constant, so energy cannot be created or destroyed, just changed from one form to another or moved from one place to another.

Page 8: Chapter 15 Thermodynamics

Enthalpy

Page 9: Chapter 15 Thermodynamics

To account for the energy of a chemical reactions, chemists look at the enthalpy of the reaction. Enthalpy (H) is considered the energy content of the reaction and includes (but not limited to) heat released or absorbed during chemical reactions. (It is often assumed the pressure stays constant – atmospheric.)

Page 10: Chapter 15 Thermodynamics

Enthalpy is a state function, so only the starting and ending conditions matter when calculating the enthalpy change (ΔH).

(This is good news, it makes it easier.)

ΔH = Hproducts – Hreactants

If ΔH = -, reaction is exothermicIf ΔH = +, reaction is endothermic

Why?

Page 11: Chapter 15 Thermodynamics

A balanced chemical equation along with the ΔH is a thermochemical equation, for example:

C2H5OH(l) + 3O2(g) → 2CO2(g) + 3H2O(l) ΔH = 1367 kJ/mole rxn

Or

2CO2(g) + 3H2O(l) → C2H5OH(l) + 3O2(g) ΔH = -1367 kJ/mole rxn

Why?

Page 12: Chapter 15 Thermodynamics

Notice: it is important to specify the state because state changes also include energy changes. For example H2O(s) → H2O(l) would have a +ΔH.

Notice: enthalpy of reaction is per mole of reaction

Page 13: Chapter 15 Thermodynamics

When 2.61 grams of CH3OCH3 is burned (at constant pressure), 82.5 KJ of heat is given off. What is the ΔH of the reaction?

Page 14: Chapter 15 Thermodynamics

How much heat is released by the complete oxidation of 24.2 grams of aluminum? ΔH= -3352 kJ/mol rxn

Page 15: Chapter 15 Thermodynamics

StandardEnthalpy

Page 16: Chapter 15 Thermodynamics

Standard Enthalpies (H°) “°” is a zero, said naught, and refers to zero starting position (think number line)

Standard enthalpies are the natural conditions of the substance at 1 bar (≈ 1 atm) and 25°C

Standard states can be any phase of matter (see periodic table) and include diatomic elements. For solutions it is 1 M.

To determine the standard enthalpy change (ΔH°) requires all reactants and products are in their standard states!

Page 17: Chapter 15 Thermodynamics

Standard Molar Enthalpy of Formation (ΔHf°), sometimes called the “heat of formation”, is the enthalpy for making 1 mole of a substance in it’s standard state from it’s constituent elements in their standard state

The ΔHf° for any element already in it’s standard state (also diatomic) is declared zero

For example: Br2(l) is ΔHf° = 0, but Br2(g) is ΔHf° = 30.91 kJ/mol

Page 18: Chapter 15 Thermodynamics

What about this?

H2(g) + Br2(g) → 2HBr(g) ΔHf° = -72.8 kJ/ mol rxn

Is this the heat of formation for HBr? Why?

Page 19: Chapter 15 Thermodynamics

What about this?

H2(g) + Br2(g) → 2HBr(g) ΔHf° = -72.8 kJ/ mol rxn

Is this the heat of formation for HBr? Why?

Remember, heats of formation are for one mole of the substance formed!

Page 20: Chapter 15 Thermodynamics

Hess’s Law

Page 21: Chapter 15 Thermodynamics

Hess’s Law states that the enthalpy for a reaction is the same whether it occurs by one step or by many.

For example, what is the ΔHf° of CH4 ifC(graphite) + H2(g) → CH4(g)

The problem is that this reaction would never occur, so we cannot measure the ΔHf° to put it in a chart, so how can we find ΔHf° if all we could measure is ΔH°?

Page 22: Chapter 15 Thermodynamics

We can use Hess’s Law and reactions that would occur and be measureable to calculate the ΔHf° for CH4.

C(graphite) + O2(g) → CO2(g) ΔH° = -393.5 kJ/molH2(g) + ½O2(g) → H2O(l) ΔH° = -295.8 kJ/molCH4(g) + 2O2(g) → CO2(g) + 2H2O(l) ΔH° = -890.3 kJ/mol

We need to make the above add up to C(graphite) + H2(g) → CH4(g)

How do we manipulate the equations? 1. Start by getting the reactants and products on the correct

side of the arrow. 2. Then multiply so unwanted parts cancel.3. Don’t forget to do to ΔH° what you do to the equation.4. Add up the equations and ΔH° values.

Page 23: Chapter 15 Thermodynamics

C(graphite) + O2(g) → CO2(g) ΔH° = -393.5 kJ/molH2(g) + ½O2(g) → H2O(l) ΔH° = -295.8 kJ/molCH4(g) + 2O2(g) → CO2(g) + 2H2O(l) ΔH° = -890.3 kJ/mol

Page 24: Chapter 15 Thermodynamics

What is the heat of reaction forC2H4(g) + H2O(l) → C2H5OH(l)

ifC2H5OH(l) + 3O2(g) → 2CO2(g) + 3H2O(l) ΔH° = -1367 kJ/molC2H4(g) + 3O2(g) → 2CO2(g) + 2H2O(l) ΔHf° = -1411 kJ/mol

Is this a ΔHf° or just a ΔH° ?

Page 25: Chapter 15 Thermodynamics

Another use of Hess’s law allows us to calculate the heat of a reaction if all the heats of formation are known (or can be looked up).

ΔH°reaction = Σn ΔHf°products - Σn ΔHf°reactants

Multiply by the number of moles before summing, and don’t forget the ΔHf° of an element in it’s standard state is zero.

Page 26: Chapter 15 Thermodynamics

What is the heat of reaction forC2H4(g) + H2O(l) → C2H5OH(l)

IfΔHf° C2H4(g) = 52.3 kJ/molΔHf° H2O(l) = -285.8 kJ/molΔHf° C2H5OH(l) = -277.7 kJ/mol

Page 27: Chapter 15 Thermodynamics

What is the ΔHf° for PbO(s, yellow)?

PbO(s, yellow) + CO(g) → Pb(s) + CO2(g) ΔH° = -65.69 kJΔHf° for CO2(g) = -393.5 kJ/mol ΔHf° for CO(g) = -110.5 kJ/mol

Page 28: Chapter 15 Thermodynamics

Bond Energy

Page 29: Chapter 15 Thermodynamics

Bond Energy is the amount of energy needed to break one mole of bonds of a covalent substance in gaseous state.

Bond energies increase as the strength of the bonds increase, so it can indicate the amount of bonds (why?) or the stability of the bond (what’s that mean?).

Page 30: Chapter 15 Thermodynamics

For example:

H2(g) → 2H(g)

To break this H-H bond takes 436 kJ/mol (see page 610 for a lot of bond energies)

Why is it positive?Why is it per mole?What is the ΔH° of this reaction?Is this ΔHf°?

Page 31: Chapter 15 Thermodynamics

So bond energies could tell us the ΔHf° in some particular instances.

Another example:H2(g) + Br2(g) → 2HBr(g)

What has to occur for this to happen?Which steps should have positive bond energies and which should have negative?Would the B. E. be related to ΔH°? To ΔHf°?

Page 32: Chapter 15 Thermodynamics

H2(g) + Br2(g) → 2HBr(g)

H2(g) → 2H(g) B.E. = 436 kJ/molBr2(g) → 2Br(g) B.E. = 193 kJ/molH(g) + Br(g) → HBr(g) B.E. = -366 kJ/mol

What is the ΔH°rxn of HBr? What would be the ΔHf°?

Page 33: Chapter 15 Thermodynamics

Internal Energy

Page 34: Chapter 15 Thermodynamics

Internal Energy (E) represents all the energy contained within a substance, and is a state function.

The internal energy of a system includes both heat (q) and the mechanical work of the system (w), thus

ΔE = q + w

Why is this another representation for the first law of thermodynamics?

Page 35: Chapter 15 Thermodynamics

ΔE = q + w

q is + if heat is absorbed into the systemq is - if heat is given off by the systemw is + if work is done to the systemw is - if work is done by the system

thusE is + (absorbs energy) if q and w are both +E is - (releases energy) if q and w are both -E is + or - if q and w are different in signs, depending on which is larger

Page 36: Chapter 15 Thermodynamics

ΔE = q + w

q can be:q = m c ΔTq = m Hf

q = m Hv

w can be:w = f Δd (like a piston moving)w = -P ΔV(like a balloon inflating)

because P is always +, w depends onthe sign of ΔV

Page 37: Chapter 15 Thermodynamics

More about work:

If the volume remains constant (sealed vessel) then -P ΔV = 0, so w = 0, so ΔE = qv only

Also w = -P ΔV = -Δn R T, where Δn is the change in moles of the gases (R and T are always positive, so w depends on Δn)

Page 38: Chapter 15 Thermodynamics

Predict the sign of w in each of these examples, and then state what that means:

2NH4NO3(S) → 2N2(g) + 4H2O(g) + O2(g)

H2(g) + Cl2(g) → 2HCl(g)

2SO2(g) + O2(g) → 2SO3(g)

Page 39: Chapter 15 Thermodynamics

Enthaply and Internal Energy

Page 40: Chapter 15 Thermodynamics

To correctly determine the enthalpy of a reaction, we need the entire energy of the system (E) and we need to account for any work it did (PV).

For example, the enthalpy for the combustion of one mole of ethanol at constant pressure is -1367 kJ. The change in internal energy of ethanol when combusted is only -1365 kJ. What happens to the other 2 kJ of energy?

Page 41: Chapter 15 Thermodynamics

Thus, ΔH = ΔE + P ΔV

and ΔH = q + w + P ΔVand ΔH = q + -P ΔV + P ΔV at constant T and Pso ΔH = qp (at constant pressure)

also, ΔH = ΔE + Δn R T (constant T and P)

Page 42: Chapter 15 Thermodynamics

A system receives 93 J of electrical work, performs 227 J of pressure-volume work, and releases 155 J of heat. What is the change to the internal energy of the system?

Page 43: Chapter 15 Thermodynamics

What is the amount of work done when one mole of brown nitrogen dioxide is converted into colorless dinitrogen tetroxide at 10.0° C?

Page 44: Chapter 15 Thermodynamics

Spontaneity

Page 45: Chapter 15 Thermodynamics

One of the biggest concerns of thermodynamics is predicting whether a particular process would occur under a certain set of conditions. In other words, would the reactants spontaneously form products, or just stay as reactants?

If the reaction will proceed, then it is spontaneous, or the products are thermodynamically favored.

Otherwise it is nonspontaneous, or the products are not thermodynamically favored.

Page 46: Chapter 15 Thermodynamics

Note: the speed of a reaction has nothing to do with whether or not it is thermodynamically favorable

For example, C(diamond) → C(graphite), is thermodynamically favorable, but takes so long you would have to wait millions of years for the diamond in your ring to turn to graphite.

The rate at which a thermodynamically favored reaction proceeds will be a topic for later (chapter 16).

Page 47: Chapter 15 Thermodynamics

Typically two factors will make a reaction thermodynamically favorable (spontaneous):

a decrease in the energy of the productsIs that endothermic or exothermic?

an increase in the disorder, or spread-out-ed-ness

The second factor can be so strong a driving force that is it our Second Law of Thermodynamics - the disorder of the universe is always increasing (although within a system is can decrease).

Page 48: Chapter 15 Thermodynamics

Entropy

Page 49: Chapter 15 Thermodynamics

Entropy (S) is a measure of the disorder of a system, and is a state function. The greater the disorder, the greater the entropy.

If the entropy of a system increases, the reaction is likely to be spontaneous, but it does not have to be spontaneous to get an increase in entropy.

If the entropy of a system decreases, the entropy of the surroundings must increase by a greater amount so the entropy of the universe still increases.

Page 50: Chapter 15 Thermodynamics

When entropy increases, ΔS = +

When entropy decreases, ΔS = -

ΔSuniverse must always be +

Can you cool your house by leaving the refrigerator door open?

To clean up your room is to make it more orderly, how does the ΔSuniverse still increase?

Unfortunately we cannot measure the ΔSuniverse, so it is understood all talk of ΔS is ΔSsystem.

Page 51: Chapter 15 Thermodynamics

In order to measure the ΔSsystem we needed a zero mark, so the Third Law of Thermodynamics states that the entropy of a perfect crystalline solid at absolute zero is zero.

As temperature increases, the particles increase in movement, so their entropy increases. Entropy values are tabulated at 25°C and 1 mole amount, so these values are actually S° values.

Is it possible for these values to be either + or -?

Page 52: Chapter 15 Thermodynamics

Now with a zero mark, ΔS° can be determined…

ΔS°rxn = Σ n S°products - Σ n S°reactants

BEWARE! Entropy is usually measured in J/mol K, not kJ like enthalpy. Some conversions are necessary anytime entropy and enthalpy are algebraically put together.

Page 53: Chapter 15 Thermodynamics

Rockets can use the following reaction as propulsion: N2H4(l) + 2H2O2(l) → N2(g) + 4H2O(g)

ΔH° = -642.2 kJ/molWhat is the ΔS° (appendix K) and would this reaction be thermodynamically favorable (spontaneous)?

Page 54: Chapter 15 Thermodynamics

Predict the sign of ΔS° for the following:1. Melting, Freezing, Vaporizing,

Condensing, Subliming, Depositing2. General warming and cooling3. Increasing and Decreasing Volume4. Mixing two or more things together5. A reaction producing more or less moles

of substances compared to the reactants

Page 55: Chapter 15 Thermodynamics

Gibbs Free Energy

Page 56: Chapter 15 Thermodynamics

Car engines used to be about 30-40% efficient in the conversion of the chemical potential energy in gasoline to kinetic energy. In order to get more fuel efficient cars, the engines have become more efficient at this conversion, but we will NEVER reach 100% efficiency.

Why? It might help to consider the combustion of octane and that cars need their pistons moved to have kinetic energy.

C8H18 + O2 → CO2 + H2O

Page 57: Chapter 15 Thermodynamics

Gibbs free energy is considered a measure of how much useful energy is available in a chemical reaction (available = free for use). Gibbs energy is a state function.

G = H - T S (T is in K)

ΔG = ΔH - T ΔS at constant T and P

Page 58: Chapter 15 Thermodynamics

If there is a decrease in the Gibbs Free Energy, then ΔG = -, and the reaction is considered thermodynamically favorable, so the reactants will form products.

If ΔG = + then the reaction is not thermodynamically favorable and the reactants will probably just sit there not reacting.

If ΔG = 0, then neither the products nor the reactants are favored, which means equilibrium has been established in the system.

Page 59: Chapter 15 Thermodynamics

Just like with our other functions, there is a ΔG°. Standard conditions for ΔG are 1 bar (1 atm) and 298 K, and assumes a reaction proceeds to 100% products. We can also determine a ΔGf° and the ΔGf° for an element in it’s natural state is still zero. See appendix K for values.

ΔG°rxn = Σ n Gf°products - Σ n Gf°reactants

ΔG° is usually measured in kJ/mol

Page 60: Chapter 15 Thermodynamics

What is the ΔG°rxn for N2(g) + O2(g) → 2NO(g)? Is this reaction thermodynamically favorable?

Page 61: Chapter 15 Thermodynamics

What is the ΔG°rxn for N2(g) + O2(g) → 2NO(g)? Use ΔG° = ΔH° - T ΔS° Is this reaction thermodynamically favorable?

Page 62: Chapter 15 Thermodynamics

It is VERY important you know how to predict when a reaction will be thermodynamically favorable or not. To be spontaneous, G must be -.

How can G be -?

ΔH - T ΔS = ΔG- + - spont. all T+ + T - spont. with large T- - T - spont. with small T

+ - + not spont. all T- - T + not spont. with large T+ + T + not spont. with small T

Page 63: Chapter 15 Thermodynamics

So sometimes the temperature of a reaction can determine whether it is spontaneous. We can calculate what temperature this would be.

A reaction would change from spontaneous ↔ nonspontaneous as ΔG changes from + ↔ -, in other words, when ΔG = 0.

So ΔG = ΔH - T ΔS and 0 = ΔH - T ΔS solve for T,

T =ΔHΔS

Page 64: Chapter 15 Thermodynamics

Consider this reversible reaction: Br2(l) → Br2(g)

At what temperature does this change spontaneity?What is significant about this temperature?

Page 65: Chapter 15 Thermodynamics

Calorimetry -Application of

Thermodynamics

Page 66: Chapter 15 Thermodynamics

Why use a bomb calorimeter?Why cannot the heat absorbed by the water be considered all the heat given off by the food?