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“A” students work (without solutions manual ~ 10 problems/night. Alanah Fitch Flanner Hall 402 508-3119 [email protected] Office Hours W – F 2-3 pm Module #11 Thermochemistry

“A” students work (without solutions manual) ~ 10 problems/night

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“A” students work (without solutions manual) ~ 10 problems/night. Alanah Fitch Flanner Hall 402 508-3119 [email protected] Office Hours W – F 2-3 pm. Module #11 Thermochemistry. FITCH Rules. G1: Suzuki is Success G2. Slow me down G3. Scientific Knowledge is Referential - PowerPoint PPT Presentation

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Page 1: “A” students work (without solutions manual) ~  10 problems/night

“A” students work(without solutions manual)~ 10 problems/night.

Alanah FitchFlanner Hall [email protected]

Office Hours W – F 2-3 pm

Module #11Thermochemistry

Page 2: “A” students work (without solutions manual) ~  10 problems/night

FITCH Rules

G1: Suzuki is SuccessG2. Slow me down G3. Scientific Knowledge is ReferentialG4. Watch out for Red HerringsG5. Chemists are LazyC1. It’s all about chargeC2. Everybody wants to “be like Mike”C3. Size MattersC4. Still Waters Run DeepC5. Alpha Dogs eat first

Che

mis

try

Gen

eral

E kq q

r ror k

q q

del

1 2

1 2

1 2

Page 3: “A” students work (without solutions manual) ~  10 problems/night

Set up like others

1. Want to understand how moleculesform and interact.

2. Need a measurement tool and scaling3. Q – measure of the energy within and

1. Between molecules.

Page 4: “A” students work (without solutions manual) ~  10 problems/night

Energy:

w F d

Or transfer heat, q

E E E q wfina l in itia l

w

q

Energy ConsumedDepends onBoth workAnd heat

capacity to do work

Page 5: “A” students work (without solutions manual) ~  10 problems/night

Marie the Jewess, 300 Jabir ibn Hawan, 721-815

Galen, 170 Abbe Jean Picard1620-1682

Galileo Galili1564-1642

Daniel Fahrenheit1686-1737

Evangelista Torricelli1608-1647

Isaac Newton1643-1727

Robert Boyle, 1627-1691

Blaise Pascal1623-1662

Anders Celsius1701-1744

Charles Augustin Coulomb 1735-1806 John Dalton

1766-1844 B. P. Emile Clapeyron1799-1864

Jacques Charles 1778-1850 Germain Henri Hess

1802-1850

Fitch Rule G3: Science is Referential

William ThompsonLord Kelvin, 1824-1907

James Maxwell1831-1879

Johannes D.Van der Waals1837-1923

Justus von Liebig (1803-1873

1825-1898Johann Balmer

James Joule (1818-1889)

Johannes Rydberg1854-1919

Rudolph Clausius1822-1888

Thomas Graham1805-1869

Heinrich R. Hertz, 1857-1894

Max Planck1858-1947

J. J. Thomson1856-1940

Linus Pauling1901-1994

Werner Karl Heisenberg1901-1976

Wolfgang Pauli1900-1958

Count Alessandro Guiseppe Antonio Anastasio Volta, 1747-1827

Georg Simon Ohm 1789-1854

Henri Louis LeChatlier1850-1936

Svante Arrehenius1859-1927

Francois-Marie Raoult1830-1901

William Henry1775-1836physician

Gilbert Newton Lewis1875-1946

Fritz Haber1868-1934

Michael Faraday1791-1867

Luigi Galvani1737-1798

Walther Nernst1864-1941

Lawrence J. Henderson1878-1942

Amedeo Avogadro1756-1856

J. Willard Gibbs1839-1903

Niels Bohr1885-1962 Erwin Schodinger

1887-1961Louis de Broglie (1892-1987)

Friedrich H. Hund1896-1997

Fritz London1900-1954

An alchemist

Ludwig Boltzman1844-1906

Richard AugustCarl Emil Erlenmeyer1825-1909

Johannes NicolausBronsted1879-1947

Thomas MartinLowry1874-1936

James Watt1736-1819

Dmitri Mendeleev1834-1907

Page 6: “A” students work (without solutions manual) ~  10 problems/night

Properties and MeasurementsProperty Unit Reference StateSize m size of earthVolume cm3 mWeight gram mass of 1 cm3 water at specified Temp

(and Pressure)Temperature oC, K boiling, freezing of water (specified

Pressure)1.66053873x10-24g amu (mass of 1C-12 atom)/12quantity mole atomic mass of an element in gramsPressure atm, mm Hg earth’s atmosphere at sea levelEnergy, General

Animal hp horse on tread millheat BTU 1 lb water 1 oF

calorie 1 g water 1 oCKinetic J m, kg, sElectrostatic 1 electrical charge against 1 Velectronic states in atom Energy of electron in vacuum

Electronegativity F Heat flow measurements Reference state?

Page 7: “A” students work (without solutions manual) ~  10 problems/night

To set a “heat flow” scale

1. Defined conditions: how experiment is performedopen flask, closed flask, pressure

2. Define the direction of heat flow by giving a positive or negative number

+ heat - heat?

Does the “system (earth)” gain energy?

For image abovesystem (earth) gains heatfrom surroundings (sun)

Page 8: “A” students work (without solutions manual) ~  10 problems/night

To set a “heat flow” scale

1. Defined conditions: how experiment is performedopen flask, closed flask, pressure

2. Define the direction of heat flow by giving a positive or negative number

+ heat - heat?

We would get a different answer if we asked“Does the “system (sun)” gain energy?”

For this question: thesystem (sun) loses heatto the surroundings (earth)

Page 9: “A” students work (without solutions manual) ~  10 problems/night

First Law of Thermodynamics: Energy is conserved

No universal change in energyJust a transfer of energy

Page 10: “A” students work (without solutions manual) ~  10 problems/night

q>0 q<0

E = constant when System AND surroundings considered!

system system

system

surroundings

q =?

Page 11: “A” students work (without solutions manual) ~  10 problems/night

To set a “heat flow” scale

1. Defined conditions: how experiment is performed open flask, closed flask, pressure

2. Define the direction of heat flow (q) by giving a positive or negative number

q is + when heat flows into the system from the surroundings

q is - when heat flows out of the system into the surroundings

3. Chemical process in the “system” is defined by heat flow

endothermic q>0exothermic q<0

Page 12: “A” students work (without solutions manual) ~  10 problems/night

Properties and MeasurementsProperty Unit Reference StateSize m size of earthVolume cm3 mWeight gram mass of 1 cm3 water at specified Temp

(and Pressure)Temperature oC, K boiling, freezing of water (specified

Pressure)1.66053873x10-24g amu (mass of 1C-12 atom)/12quantity mole atomic mass of an element in gramsPressure atm, mm Hg earth’s atmosphere at sea levelEnergy: Thermal BTU 1 lb water 1 oF

calorie 1 g water 1 oCKinetic J 2kg mass moving at 1m/sEnergy, of electrons energy of electron in a vacuum

Electronegativity F Heat Flow into system = +

Page 13: “A” students work (without solutions manual) ~  10 problems/night

Z n s H aq Z n aq H g( ) ( ) ( ) ( ) 2 22

Constant Atm.pressure

Chemical reactions involve 1. heat exchange

Heat exchangeAt constantPressure

As a review:

who is oxidized?who is reduced?what is the oxidation number on H2?Who is an oxidizing agent?

1 atm pressure = constant pressure

This means heat flow, q, is enthalpy change

H =enthalpy

Greek: thalpein – to heaten - in

H for (?) heat

q HP

SubscriptReminds us thatPressure is constant

Page 14: “A” students work (without solutions manual) ~  10 problems/night

Chemical reactions involve 1. heat exchange 2. work

constant Atm. pressure

V

Z n s H aq Z n aq H g( ) ( ) ( ) ( ) 2 22

Pressure-Volumework

w P V

Page 15: “A” students work (without solutions manual) ~  10 problems/night

E E E q wfina l in itia l

E q P VP P

Change in volume is typically small for Most reactions

E HP This means we can measure the energy change of A chemical reaction by measuring the heat exchangeAt constant pressure

E H P VP

E H P VP

This is a form of Rule G3

Science is referential

Generally final - initial

Page 16: “A” students work (without solutions manual) ~  10 problems/night

five Navy Avengers

disappeared in the Bermuda Triangle on Dec. 5, 194

First example problem will involve methane

We will prove to ourselves that the Pressure-Volume work is a Small contribution to the total energy change

Page 17: “A” students work (without solutions manual) ~  10 problems/night

MethaneGas RecoveryAt landfills

3 to 8 standard cubic feet of biogas per pound of manure. The biogas usually contains 60 to 70% methane.

Page 18: “A” students work (without solutions manual) ~  10 problems/night

Consider the contribution of volume of gas phase molecules

C H O C O H Og g g l4 2 2 22 2( ) ( ) ( ) ( )

P V n n R Tgas fina l gas in itia l

P V nR T

P V n R T At constant T:

P V m olesL a tm

m ol KK

1 3 0 0 8 2 1 2 9 8.

P V L atm 4 8 9 3 1 6.

P V L atmkJ

L a tmkJ

4 8 9 3 1 6

0 1 0 1 34 9.

..

2mole change

%&$*! Conversions – ifInterested see slide after next

Page 19: “A” students work (without solutions manual) ~  10 problems/night

Consider the contribution of volume change for water in this reaction

C H O C O H Og g g l4 2 2 22 2( ) ( ) ( ) ( )

21 8 1

1

1

1 00 0 3 62

3

3 3m oleH Og

m ol

cm w ater

gw ater

L

cmLl( ) * * * .

P V atm LkJ

L atmkJ

1 0 0 3 6

0 1 0 1 30 0 0 3 6.

..

Energy in kJMost reactions total (q): ~ 1000 kJPV 1 mole gas ~ 2.5 kJPV 2mole liquid water ~ 0.0036 kJ

Sig fig tells us that PV energy small compared to q

%&$*! Conversions – ifInterested see next slide

By the end ofThis moduleWe will see thisIs “true”

Page 20: “A” students work (without solutions manual) ~  10 problems/night

Optional Slide: conversion

a tmx P a

atm

1 0 1 3 2 5 1 0 5.

a tm

x P a

a tm

kg

m sP a

1 0 1 3 2 5 1 0 5 2.

a tmx P a

atm

kg

m sP a

Lcm

L

m

cm

1 0 1 3 2 5 1 0 1 0 1

1 0

5 2 3 3

2

3.

a tmx P a

atm

kg

m sP a

Lcm

L

m

cm

J

kg m

s

kJ

JkJ

1 0 1 3 2 5 1 0 1 0 1

1 0 1 00 1 0 1 3 2 5

5 2 3 3

2

3

2

2

3

..

0 1 0 1 3 2 5 1 0 1 3 2 5 1 0 1 0 1

1 0 1 0

5 2 3 3

2

3

2

2

3

. .kJ

a tm L

x P a

atm

kg

m sP a

cm

L

m

cm

J

kg m

s

kJ

J

Page 21: “A” students work (without solutions manual) ~  10 problems/night

To set a “heat flow” scale1. Defined conditions: how experiment is performed

Constant Pressure2. But not on the path taken (state property)

Heat flowdependsthe conditions

q H H Hreaction cons tp ressure products reac tstan tan

H= enthalpy

Page 22: “A” students work (without solutions manual) ~  10 problems/night

Enthalpy is a state property(measured under constant pressure, but how measured under that constant pressure is not important)

q H

exo therm ic

0

H O hea t H Os2 2( )

H Hproducts reac ts tan

q H

endotherm ic

0

H Hproducts reac tss tan

C H O C O H O hea tg g g l4 2 2 22( ) ( ) ( ) ( )

Think of heat as a reactant

Think of heat as a product

Page 23: “A” students work (without solutions manual) ~  10 problems/night

Enthalpy is an “extensive” property

Depends upon the amount present

C H O C O H O H kJg g g l4 2 2 22 2 8 9 0( ) ( ) ( ) ( )

890kJ of heat is released when 1 mole of methaneReacts with oxygen

8 9 0

1 4

kJ

m oleC H g( )

8 9 0

12 1 7 8 0

44

kJ

m oleC Hm oleC H kJ

gg

( )( )

Page 24: “A” students work (without solutions manual) ~  10 problems/night

Properties and MeasurementsProperty Unit Reference StateSize m size of earthVolume cm3 mWeight gram mass of 1 cm3 water at specified Temp

(and Pressure)Temperature oC, K boiling, freezing of water (specified

Pressure)1.66053873x10-24g amu (mass of 1C-12 atom)/12quantity mole atomic mass of an element in gramsPressure atm, mm Hg earth’s atmosphere at sea levelEnergy, General

Animal hp horse on tread millheat BTU 1 lb water 1 oF

calorie 1 g water 1 oCKinetic J m, kg, sElectrostatic 1 electrical charge against 1 Velectronic states in atom Energy of electron in vacuum

Electronegativity F Heat flow measurements constant pressure, define system vs surroundings

per mole basis (intensive)

Page 25: “A” students work (without solutions manual) ~  10 problems/night

2006 Sept Sci. Am: World Wide Petroleum UsageLand People Transport29% of total use

Land Freight 19%Air People and Freight 5%

Non-transportation

U.S. differs from world in distribution of petroleum use

Transportation = 71.8%

57.8% of Transportation=Personal land transport

= 41.5% of total U.S. consumptionData US DOE 2006

Context for the next example problem

3 Non-transportation

Total transportation=53%

Page 26: “A” students work (without solutions manual) ~  10 problems/night
Page 27: “A” students work (without solutions manual) ~  10 problems/night

H x kJ C H O C O H Og g 1 0 9 1 0 2 2 5 1 6 1 848 1 8 2 2 2. ( ) ( )

H x kJ 1 0 7 1 0 6.

Example: If you drove an automobile 1.50x102 miles at 17.5 miles/gal you consume a certain number of gallons of gasoline. If you burn thatnumber of gallons of gasoline at constant pressure how much heat would be released? Assume the gasoline is pure octane with a density of the octane 0.690 g/mL?

1 5 01

1 7 5.

.m i

ga l

m i

Strategy: need moles of octane consumed (Golden Bridge)

miles gallons gramsdensitympg

molesMolar mass

heatH

1 5 01

1 7 5

3 7 8 5 2.

.

.m i

ga l

m i

L

ga l

1 5 0

1

1 7 5

3 7 8 5 2 1 0 3

..

.m i

ga l

m i

L

ga l

m L

L

1 5 0

1

1 7 5

3 7 8 5 2 1 0 0 6 9 038 8

8 8

..

. .m i

ga l

m i

L

ga l

m L

L

gC H

m L C H

1 5 0

1

1 7 5

3 7 8 5 2 1 0 0 6 9 0 1

11 4

38 8

8 8

8 8

8 8

..

. .m i

ga l

m i

L

ga l

m L

L

gC H

m L C H

m oleC H

gC H

1 5 0

1

1 7 5

3 7 8 5 2 1 0 0 6 9 0 1

11 4

1 0 9 1 0

2

38 8

8 8

8 8

8 8

4

8 8

..

. . .m i

ga l

m i

L

ga l

m L

L

gC H

m L C H

m oleC H

gC H

x kJ

m oleC H

H kJ 1 0 7 0 2 4 3 9 5 5, , .

3 sig figWe will use part of this problemAgain:

3 7 8 5 2 1 0 0 6 9 0 1

11 4

1 0 9 1 0

2

1 2 4 8 6 138 8

8 8

8 8

8 8

4

8 8

. . . ,L

gal

m L

L

gC H

m L C H

m oleC H

gC H

x kJ

m oleC H

kJ

ga l

Page 28: “A” students work (without solutions manual) ~  10 problems/night

Rules

1.Enthalpy is an extensive property (depends upon number of moles)2.Enthalpy change for a reaction is equal in magnitude, but opposite

in sign, to the enthalpy for the reverse reaction

3. Enthalpy change depends upon the state of the reactant and products

H x kJ C H O C O H Og g 1 0 9 1 0 2 2 5 1 6 1 848 1 8 2 2 2. ( ) ( )

H x kJ 1 0 9 1 0 4.

H kJ 4 4

1 6 1 8 2 2 52 2 8 1 8 2C O H O C H Og g( ) ( )

H O H Ol g2 2( ) ( )

Page 29: “A” students work (without solutions manual) ~  10 problems/night

ENERGY measurementa) change in temperatureb) some function specific to the material and how

it is organized (bonds)

Page 30: “A” students work (without solutions manual) ~  10 problems/night

25

O

HH

OH

H

O

H

H

O

H

H

O

HH

O

H

H

O

HH

OH

H

O

H

H

O

H

H

O

HH

O

H

H

heat 25 oC15 oC

ENERGY change is a function of a) temperatureb) material E k

q q

del

1 2

Page 31: “A” students work (without solutions manual) ~  10 problems/night

ENERGY measurementa) change in temperatureb) some function specific to the material and how

it is organized (bonds)

q C t t

q C t

fina l in itia l

C = heat capacity = heat required to raise the temperature of the system 1oC

units: J/oC

q m c t

m = mass c = specific heat of a pure substance

Pure material

Page 32: “A” students work (without solutions manual) ~  10 problems/night

http://www.lsbu.ac.uk/water/molecule.html

Electrons on Oxygen sit“out there” causing largeElectrostatic potential Oriented on the electrons

Electron density of waterShape and charge distributionOn water

ch e densityq

rarg

C(liquidH2O)=4.18J/g-oC

Liquid water is very strongly organizeddue to the polarity of the molecule, so it has a high specific heat

Page 33: “A” students work (without solutions manual) ~  10 problems/night

Material Specific Heats c, (J/g-K)Pb(s) 0.12803Pb(l) 0.16317Cu(s) 0.382Fe(s) 0.446Cl2(g) 0.478C(s) 0.71CO2(g) 0.843NaCl(s) 0.866Al(s) 0.89C6H6(l)1.72H2O(g) 1.87C2H5OH(l) 2.43H2O(l) 4.18

Ability to storeheat in a substanceis variable.

Specific heats, c, of various substances in various physical states

Page 34: “A” students work (without solutions manual) ~  10 problems/night

O

HH

OH

H

O

H

H

O

H

H

O

HH

O

H

H

He

He

He

He

He

He

For the same amount of energy, easier to break electrostatic attraction of He compared to water with it’s localized charge

Page 35: “A” students work (without solutions manual) ~  10 problems/night

q m c t

Mass of water:

Example: 1.00 cup of water is heated from 25.0 oC to 100.0 oC. Howmany joules were used to heat the water?

t K 7 5

1 0 01

4

1

1 0 5 7.

.cup

q t

cups

L

q t

1 0 0. cup 1 0 0

1

4. cup

q t

cups

1 0 0

1

4

1

1 0 5 7

1 0 1

12 3 6 5 1

3

..

.cupq t

cups

L

q t

m L

L

g

m Lg

t C Co o 1 0 0 2 5 t T Tfina l in itia l

t Co 7 5

q x J 7 4 1 1 0 4.

q 7 4 1 4 8 5 3.

q gJ

gKK

2 3 6 5 1

4 1 87 5.

.

q kJ 7 4 1.

Page 36: “A” students work (without solutions manual) ~  10 problems/night

Example 2: 1 cup of dry soil (specific heat, c = 0.800 J/gK; density =1.28 g/cm3). Calculate the Joules required to raise the temperature of the dry soil from 25oC to 100

oC.

1 0 01

4

1

1 0 5 7

1 0 1 2 8

12 3 6 5 1 1 2 8 3 0 2 7

3

..

.. . .cup

q t

cups

L

q t

m L

L

g

m Lg g

q gJ

gKK

3 0 2 7

0 87 5.

.

q J kJdry so il 1 8 1 6 4 1 8 1, .

q kJw ater 7 4 1.

Page 37: “A” students work (without solutions manual) ~  10 problems/night

Because water has a high heat capacity it takes longer than air or soil to warm up and longer to cool down

LandWater

Lag

Page 38: “A” students work (without solutions manual) ~  10 problems/night

The temperature change in 24 hours in summer for water is not muchleading to big differences between lake and land

Land

Lake

1. Hot air rises over land

2. Cold air from Lake moves to fill in (Lake Breeze)

1. Hot air rises over Lake

2. Cold air moves in from land (Land breeze)

and thus a lake breeze

Page 39: “A” students work (without solutions manual) ~  10 problems/night

Heat capacity of large bodiesOf water affect human activity

Page 40: “A” students work (without solutions manual) ~  10 problems/night

Example 3: Heat capacity of the metal block of a car combustion engine. Assume that a Prius 1.5 L, 4 cylinder 176.6 kg engine block is made of iron. The specific heat of iron is 440 J/kg-C. If I drive 8 miles twice a day (to work and back) at an average 42 mpg, what fraction of the total available enthalpy in 1 gallon of octane is consumed in heating the engine block from 25oC to 100oC?

q m c t

q kgJ

kg CC kJ

2 0 0

4 4 01 0 0 2 5 5 8 2 8,

H x kJ C H O C O H Og g 1 0 9 1 0 2 2 5 1 6 1 848 1 8 2 2 2. ( ) ( )

Compare to heat available from combustion of 1 gallon of octane (from before

3 7 8 5 2 1 0 0 6 9 0 1

11 4

1 0 9 1 0

2

1 2 4 8 6 138 8

8 8

8 8

8 8

4

8 8

. . . ,L

gal

m L

L

gC H

m L C H

m oleC H

gC H

x kJ

m oleC H

kJ

ga l

4 2

1 8

5 8 2 8

1

2 7 7 3 0m iles

ga l

trip

m iles

kJ eng ine hea ting

trip

kJ hea ting

ga l

, ,

5 8 2 8

1 2 4 8 6 11 0 0 2 2 2 %

,

,.

kJ

kJ

Let’s compare to whatI measure

Page 41: “A” students work (without solutions manual) ~  10 problems/night

Heating the engine block

3 9 3 1

3 91 0 0 2 0 5 %

m pg

m pg.

Prius 1

4 3 3 4

4 31 0 0 2 0 %

m pg

m pg

Prius 2

Page 42: “A” students work (without solutions manual) ~  10 problems/night

Properties and MeasurementsProperty Unit Reference StateSize m size of earthVolume cm3 mWeight gram mass of 1 cm3 water at specified Temp

(and Pressure)Temperature oC, K boiling, freezing of water (specified

Pressure)1.66053873x10-24g amu (mass of 1C-12 atom)/12quantity mole atomic mass of an element in gramsPressure atm, mm Hg earth’s atmosphere at sea levelEnergy, General

Animal hp horse on tread millheat BTU 1 lb water 1 oF

calorie 1 g water 1 oCKinetic J m, kg, sElectrostatic 1 electrical charge against 1 Velectronic states in atom Energy of electron in vacuum

Electronegativity F Heat flow measurements constant pressure, define system vs surroundings

per mole basis (intensive) Calorimetry

Page 43: “A” students work (without solutions manual) ~  10 problems/night

q qreaction ca lorim eter

If the temperature of the water rises (heat flow into water)then heat must have been lost from the reaction

Relate reaction heat To the calorimeter heat

Page 44: “A” students work (without solutions manual) ~  10 problems/night

Example: When 1.00 g of ammonium nitrate, NH4NO3, is added to 50.0 g of water in a coffee-cup calorimeter, it dissolves:

and the temperature of the water drops from 25.00 to 23.32 oC. Assuming that all the heat absorbed by the reactions comes from the water, calculate q for the reaction system.

N H N O N H N Os aq aq4 3 4 3( ) ( ) ( )

q Jca lorim eter 3 5 1 1 2.A 1 degree change in Celsus Is a 1 degree change in Kelvin

q Jca lorim eter 3 5 1

qJ

KKca lorim eter

2 0 9 1 6 8.

q gJ

gKC Cca lorim eter

o o

5 0 0 4 1 8 2 3 3 2 2 5 0 0. . . . q qreaction ca lorim eter

q m c tca lorim eter

q Jreaction 3 5 1

q Jreaction 3 5 1

Page 45: “A” students work (without solutions manual) ~  10 problems/night

q q C treaction reaction ca l Heat capacity of the calorimeter

In some problemsYou will Need to determineThis numberIn one step andThen go on

Not all calorimeters can be based on

q q m c treaction ca lorim eter

Page 46: “A” students work (without solutions manual) ~  10 problems/night

Example: The reaction between hydrogen and chlorine

can be studied in a bomb calorimeter. It is found that when a 1.00 g sample of H2 reacts completely, the temperature rises from 20.00 to 29.82 oC. Taking the heat capacity of the calorimeter to be 9.33 kJ/oC, calculate the amount of heat evolved in the reaction.

H C l H C lg g g g( ) ( ) ( ) 2 2

q C treaction ca l

qkJ

CC Creaction o

o o

9 3 3 2 9 8 2 2 0 0 0. . .

q kJreaction 9 1 6.

Heat evolved?Calorimeter heat capacity = 9.33 kJ/oCTinitial =20.00 oCT final = 29.82 oC

q

Page 47: “A” students work (without solutions manual) ~  10 problems/night

Example: Salicyclic acid, C7H6O3, is one of the starting materials in the manufacture of aspirin. When 1.00 g of salicylic acid burns in a bomb calorimeter, the temperature rises to 32.11oC from 28.91 oC. The temperature in the bomb calorimeter increases by 2.48oC when the calorimeter absorbs 9.37 kJ. How much heat is given off when one mole of salicylic acid is burned?

1.00 g of C7H6O3

Tinitial 32.11oCTfinal 29.91oC9.37kJ required to cause 2.48 oC change

q C treaction ca l

???

CkJ

Cca l o9 3 7

2 4 8

.

.

qkJ

Creaction o

9 3 7

2 4 83 2 11 2 9 9 1

.

.. .

q kJreaction 8 3 1 2 1.

11 3 8

1

8 3 1 2 1

13 1 5 8 5 9 87 6 3

7 6 3

7 6 3 7 6 3

m oleC H OgC H O

m oleC H O

kJ

gC H OkJ

..

3 1 6 kJ

Page 48: “A” students work (without solutions manual) ~  10 problems/night

Combine

calorimetry

2 2 5 1 6 1 88 1 8 2 2 2C H O C O H Og g ( ) ( )

To get reaction enthalpies

Reaction stoichiometry

Page 49: “A” students work (without solutions manual) ~  10 problems/night

N H N O N H N Os aq aq4 3 4 3( ) ( ) ( )

1 g was reacted

Example 2 What is the enthalpy change for the reaction

If exactly 1 g of ammonium nitrate is reacted in a bomb calorimeter made with 50 g of water and the temperature of the water drops from 25.00 oC to 23.32 oC?

q H Jreaction cons tlabpressu retan 3 5 1

q Jreaction 3 5 1

q Jreaction 3 5 1 1 2.

qJ

CCreaction o

o

2 0 9 1 6 8.

q q gJ

g CC Creaction ca lorim eter o

o o

5 0 0 4 1 8 2 3 3 2 2 5 0 0. . . .

2N=28.024H=4.043O=48.00 80.05

3 5 1

1

8 0 0 5 2 8 1 0 0 2 8 1J

g

g

m ol

J

m ol

kJ

m ol

. .

N H N O N H N O H kJs aq aq4 3 4 3 2 8 1( ) ( ) ( ) .

H

Page 50: “A” students work (without solutions manual) ~  10 problems/night

N H N O N H N O H kJs aq aq4 3 4 3 2 8 1( ) ( ) ( ) .

Where did the per/mole go?

The reaction was written as a per/moleEnthalpy is understood as a per/mole of reactant (or as the reaction

is written)

Page 51: “A” students work (without solutions manual) ~  10 problems/night

N H N O N H N O H kJs aq aq4 3 4 3 2 8 1( ) ( ) ( ) .

Thermochemical Equation Rules

1. Value of H applies when products and reactants are at same temperature, 25oC unless otherwise specified.

2. Sign of H, indicates whether reaction, when carried out at constant pressure, is exothermic or endothermic

3. ΔH sign changes when reaction is reversed

4. Stoichiometry is important4. Phases of all species must be specified5. Values of H is same regardless of method used to calculate it (Hess’s Law)

1 11

When there are noCoefficients it is understood thatIt is “1”

N H N O N H N O H kJaq aq s4 3 4 3 2 8 1( ) ( ) ( ) .

Page 52: “A” students work (without solutions manual) ~  10 problems/night

Using a coffee-cup calorimeter, it is found that when an ice cube weighing 24.6 g melts, it absorbs 8.19 kJ of heat. Calculate for the phase change represented by the thermochemical equation

H O H Os l2 2( ) ( )

8 1 9

2 4 6

.

.

kJ

g ice

8 1 9

2 4 6

1 8 0 22

2

.

.

.kJ

g

g

m oleice

H O

H O

8 1 9

2 4 6

1 8 0 21 6 0 02

2

2

.

.

..

kJ

g

g

m olem ole kJ

ice

H O

H OH O

8 1 9

2 4 6

1 8 0 212

2

2

.

.

.kJ

g

g

m olem ole

ice

H O

H OH O

Example illustrating importance of phases

Page 53: “A” students work (without solutions manual) ~  10 problems/night

H O H Og g l2

1

2 2 2( ) ( ) ( )

An example of several of the rules using Fuel Cells

HkJ

kJ H O H Og g l

5 7 1 6

22 8 6 2

1

2 2 2

.( ) ( ) ( )

Fuel cells use the reaction:

Calculate the enthalpy for the equation above given that:

H kJ H O H Ol g g 5 7 1 6 2 22 2 2. ( ) ( ) ( )

Reverse reaction:

H kJ H O H Og g l 5 7 1 6 2 22 2 2. ( ) ( ) ( )

scale

Here we got a number by coming “at it” from an odd direction

Page 54: “A” students work (without solutions manual) ~  10 problems/night

Hess’s law

Germain Henri Hess1802-1850 born in Geneva SwitzerlandProfessor of ChemistryAt St. Petersburg Technological Institute

The value of H for a reaction is the same whether it occurs in one step or in a series of steps (enthalpy (constant P, T) is a state function)

Page 55: “A” students work (without solutions manual) ~  10 problems/night

Marie the Jewess, 300 Jabir ibn Hawan, 721-815

Galen, 170 Abbe Jean Picard1620-1682

Galileo Galili1564-1642

Daniel Fahrenheit1686-1737

Evangelista Torricelli1608-1647

Isaac Newton1643-1727

Robert Boyle, 1627-1691

Blaise Pascal1623-1662

Anders Celsius1701-1744

Charles Augustin Coulomb 1735-1806 John Dalton

1766-1844 B. P. Emile Clapeyron1799-1864

Jacques Charles 1778-1850 Germain Henri Hess

1802-1850

Fitch Rule G3: Science is Referential

William ThompsonLord Kelvin, 1824-1907

James Maxwell1831-1879

Johannes D.Van der Waals1837-1923

Justus von Liebig (1803-1873

1825-1898Johann Balmer

James Joule (1818-1889)

Johannes Rydberg1854-1919

Rudolph Clausius1822-1888

Thomas Graham1805-1869

Heinrich R. Hertz, 1857-1894

Max Planck1858-1947

J. J. Thomson1856-1940

Linus Pauling1901-1994

Werner Karl Heisenberg1901-1976

Wolfgang Pauli1900-1958

Count Alessandro Guiseppe Antonio Anastasio Volta, 1747-1827

Georg Simon Ohm 1789-1854

Henri Louis LeChatlier1850-1936

Svante Arrehenius1859-1927

Francois-Marie Raoult1830-1901

William Henry1775-1836physician

Gilbert Newton Lewis1875-1946

Fritz Haber1868-1934

Michael Faraday1791-1867

Luigi Galvani1737-1798

Walther Nernst1864-1941

Lawrence J. Henderson1878-1942

Amedeo Avogadro1756-1856

J. Willard Gibbs1839-1903

Niels Bohr1885-1962 Erwin Schodinger

1887-1961Louis de Broglie (1892-1987)

Friedrich H. Hund1896-1997

Fritz London1900-1954

An alchemist

Ludwig Boltzman1844-1906

Richard AugustCarl Emil Erlenmeyer1825-1909

Johannes NicolausBronsted1879-1947

Thomas MartinLowry1874-1936

James Watt1736-1819

Dmitri Mendeleev1834-1907

Page 56: “A” students work (without solutions manual) ~  10 problems/night

C O C Os g g( ) ( ) ( ) 1

2 2

It is difficult to measure the heat evolved for this reaction because it occurs as the partial burning of carbon in the presence of other reactionsinvolving the complete burning of carbon

H kJ C O C Os g g 3 9 3 5 2 2. ( ) ( ) ( )

To solve rearrange equations to get CO on right hand side

Example of how Hess’s law is useful

CO2(g)

CO(g) +1/2O2(g)

This is theNumber we wantBut can’t actually measure

C(s) + O2(g)

Get to the number by an alternativePath (State function!)

H kJ C O O C Og g g 5 6 6 0 2 22 2. ( ) ( ) ( )

Related to 2CO + O2….

Page 57: “A” students work (without solutions manual) ~  10 problems/night

H kJ0 11 0 5 . C O C Os g g( ) ( ) ( ) 1

2 2

H kJ C O C O

H kJ C O C O O

s g g

g g g

02 2

02 2

3 9 3 5

2 8 3 0

.

.

( ) ( ) ( )

( ) ( ) ( )

H kJ C O C O Og g g 2 8 3 0 2

1

2 2. ( ) ( ) ( )

CO2(g)

CO(g) +1/2O2(g)

C(s) + O2(g)

HkJ

C O C O Og g g

5 6 6 0

2 2

1

2 2

.( ) ( ) ( )

H kJ C O C O Og g g 5 6 6 0 2 22 2. ( ) ( ) ( )

H kJ C O O C Og g g 5 6 6 0 2 22 2. ( ) ( ) ( )

H kJ 11 0 5.

H kJ C O C Os g g 3 9 3 5 2 2. ( ) ( ) ( )

1

2 2O g( )C O C Os g g( ) ( ) ( ) 1

2 2

Page 58: “A” students work (without solutions manual) ~  10 problems/night

Enthalpies of Formation

Rather than getting the enthalpy for each reaction from a bombcalorimeter use a smaller number of standard reactions from whichHess’s law can be applied to get all the remainder reactions ofinterest

Invoke Rule G5: Chemists are Lazy

Enthalpy associated with standard reaction isenthalpy of formation

which is the enthalpy change when one mole of compound is formed at constant pressure of 1 atm and a fixed temperature, ordinarily 25oC, from the elements in their stable states at that pressure and temperature. STP (Standard Temperature and Pressure)

This allows us to look at enthalpy of compoundsnot reactions which reduces total data which mustBe acquired (Chemists are Lazy!!!)

Page 59: “A” students work (without solutions manual) ~  10 problems/night

H kJ N O N OfO

g a tm C g a tm C g a tm C 8 8 21

2 2 1 2 5 2 1 2 5 2 1 2 5( , , ) ( , , ) ( , , )

Standard molar enthalpy of formation of a compound

1 atm pressure25oC

From elements in their stable states at

1

1 is “understood”

Most Hfo are negative meaning that formation

of the compound from the elements is ordinarily exothermic

Elements in their stable states at 1atm, 25oC have a standardmolar enthalpy of 0

Why?

Page 60: “A” students work (without solutions manual) ~  10 problems/night

Elements in their stable states at 1atm, 25oC have a standardmolar enthalpy of 0

H H HF e sO

F e sO

atm C F e sO

atm C( ) ( ) , ( ) ,

1 2 5 1 2 50

Products (standard state) - Reactants (standard state) = 0

F e F es s

Page 61: “A” students work (without solutions manual) ~  10 problems/night

H kJ N O N OfO

g a tm C g a tm C g a tm C 8 8 21

2 2 1 2 5 2 1 2 5 2 1 2 5( , , ) ( , , ) ( , , )

Standard molar enthalpy of formation of a compound

1 atm pressure25oC

From elements in their stable states at

Most Hfo are negative meaning that formation

of the compound from the elements is ordinarily exothermic

For aqueous ions, the enthalpy is scaled relative to theproton

H HfO

aq 0

Page 62: “A” students work (without solutions manual) ~  10 problems/night

Do we detect any patterns?

Fe(s) 0Pb(s) 0Li(s) 0Mg(g) 0Mn(s) 0Hg(l) 0Ni(s) 0N2(g) 0O2(s) 0P4(s) 0K(s) 0Rb(s) 0

H fO

kJ/mol

Sc(s) 0Si(s) 0Na(s) 0S(s,rhombic) 0Ti(s) 0Zn(s) 0

H fO

kJ/mol

Common non-metalsHave specific formsIn which theyAre standard

Al(s) 0Ba(s) 0Be(s) 0Br2(g) 0Ca(s) 0C(s,graphite) 0Cs(s) 0Cl2(g) 0Cr(s) 0Cu(s) 0F2(g) 0H2(g) 0H+(aq) 0I2(s) 0

H fO kJ/mol

Group 17 with exceptionOf I2 are gases in Stable, standard state

MOST metals are elemental solids (metal) in standard state

Page 63: “A” students work (without solutions manual) ~  10 problems/night

Properties and MeasurementsProperty Unit Reference StateSize m size of earthVolume cm3 mWeight gram mass of 1 cm3 water at specified Temp

(and Pressure)Temperature oC, K boiling, freezing of water (specified

Pressure)1.66053873x10-24g amu (mass of 1C-12 atom)/12quantity mole atomic mass of an element in gramsPressure atm, mm Hg earth’s atmosphere at sea levelEnergy, General

electronic states in atom Energy of electron in vacuum

Electronegativity F

Heat flow measurements constant pressure, define system vs surroundingsper mole basis (intensive)

Standard Molar Enthalpy 25 oC, 1 atm, from stable stateHf

o Haq+ =0

Page 64: “A” students work (without solutions manual) ~  10 problems/night

Calculation of Ho standard enthalpy change of a reaction

1 atm pressure25oC

H n H n HOf productso

f reac tso , , tan

1. The coefficients of products and reactants in the thermochemical equation must be taken into account

2. Elements in standard states can be omitted because heats of formation are zero

2 22 3 2 3A l F e O F e A l Os s s s( ) ( ) ( ) ( )

H H HOf A l Oo

f F e Oo

s , ,2 3 2 3

H H HOf A l Oo

f F e so , , ( )2 3

2 H H H H HOf A l Oo

f F e so

f F e Oo

f A l so

s , , ( ) , , ( )2 3 2 3

2 2

H O 1 6 6 9 8 8 2 2 1 6. . AppendixOJO!

H kJ m olO 1 6 6 9 8 8 2 2 1 6 8 4 7 6 5. . . /

Page 65: “A” students work (without solutions manual) ~  10 problems/night

Calculation of Ho standard enthalpy change of hot and cold packs

1 atm pressure25oC

H n H n HOf productso

f reac tso , , tan

N H N O N H N Os aq aq4 3 4 3, , ,

H H H HO

f N H

o

f N O

of N H N Oo

aq aq s , , ,

, , ,4 3 4 3

AppendixCompound ΔHf

o, kJ/molNH4NO3,s -365.6NH4

+,aq -132.5

NO3-aq -205.0

MgSO4,s -1284.9Mg2+

aq -466.8SO4

2-aq -909.3

Fe,s 0O2,g 0Fe2O3,s -1118.4

H O 1 3 2 5 2 0 5 0 3 6 5 6. . .

HkJ

m olO 3 3 7 5 3 6 5 6 2 8. .

Compares well to the calorimetry calc. (28.1kJ/mol)!

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http://biochempress.com/Files/IECMD_2003/IECMD_2003_027.pdf

http://webmineral.com/data/Hexahydrite.shtml

http://www.lsbu.ac.uk/water/hofmeist.html

H O 4 6 6 8 9 0 9 3 1 2 8 4 9. . .

H H H HO

f M g

o

f SO

of M gSOo

a q a q s , , ,

, ,2

42

4

HkJ

m olO 1 3 7 6 1 1 2 8 4 9 9 1 2, . . .

M gSO sH O

42

, M gSO M gsH O

aq422

, M gSO M g SOsH O

aq aq42

422

, ,

Liquid waterhttp://www.edinformatics.com/math_science/info_water.htm

Products are more stable, lower in the energywell, than reactants

Page 67: “A” students work (without solutions manual) ~  10 problems/night

Example: Calculate the Ho for the combustion of one mole of methane CH4 according to the equation

Given the standard enthalpies of formation at 25oC, 1 atm from AppendixkJ/mol

O2(g) 0CO2(g) -393.5H2O(g) -241.8CH4(g) -74.8

C H O C O H Og g g g4 2 2 22 2( ) ( ) ( ) ( )

H n H n HOf productso

f reac tso , , tan

H m olH OkJ

m olH Om olC O

kJ

m olC OO

2 2 4 1 8 1 3 9 3 52

22

2

. .

2 0 1 7 4 82

24

2 4

m olOkJ

m olOm olC H

kJ

m olC H.

Page 68: “A” students work (without solutions manual) ~  10 problems/night

Example: Calculate the Ho for the combustion of one mole of methane CH4 according to the equation

C H O C O H Og g g g4 2 2 22 2( ) ( ) ( ) ( )

H m olH OkJ

m olH Om olC O

kJ

m olC OO

2 2 4 1 8 1 3 9 3 52

22

2

. .

2 0 1 7 4 82

24

2 4

m olOkJ

m olOm olC H

kJ

m olC H.

H kJ kJ kJO 8 7 7 1 0 7 4 8 8 0 2 3 0. . .

Can also “reverse” the problem (inside out socks)

Sig figs? H kJO 8 0 2 3.

Page 69: “A” students work (without solutions manual) ~  10 problems/night

Example: Calculate the standard enthalpy of formation for octane

H x kJ C H O C O H Oog g 1 0 9 1 0 2 2 5 1 6 1 84

8 1 8 2 2 2. ( ) ( )

H H HOf productso

f reac tso , , tan

H x kJ H

H

Of productso

f reac tso

1 0 9 1 0 4. ,

, tan

2 2 5

08 1 8

8 1 82

2

m olC H xkJ

m olC Hm olO

kJ

m olO

x x kJ 1 0 9 7 1 0 3.

Given the standard enthalpies of formation at 25oC, 1 atmkJ/mol

O2(g) 0CO2(g) -393.5H2O(g) -241.8CH4(g) -74.8

1 0 9 1 0 1 6 3 9 3 5 1 82 4 1 84

22

22

. ..

( )( )

( )( )

x kJ m olC OkJ

m olC Om olH O

kJ

m olH Ogg

gg

1 0 9 1 0 6 2 9 6 4 3 5 2 4 2 04. .x kJ kJ kJ x

1 0 9 1 0 8 7 0 4 8 24. .x kJ kJ x

2 1 9 5 2 2. kJ x

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Bond Enthalpy

B r B r H kJg g2 2 1 9 3( )

The change in enthalpy when 1 mole of bonds is broken in the gaseousState.

Rule G3: Science is referential!

C l C l H kJg g2 2 2 4 3( ) Which has a stronger bondEnthalpy?

Page 71: “A” students work (without solutions manual) ~  10 problems/night

For covalent bonds, bond enthalpies depend on?

Bond length Overall structure of the molecule

Bond Bond Pauling's atomic EnthalpyLength ΔE.N. radii Single Bond

pm (pm) kJ/mol(Average)

Cl-Cl 199 0 99 243Br-Br 228 0 114 193I--I 267 0 133 151

H--F 92 1.8 (37) 64 568H--Cl 127 1 (37) 99 432H--Br 141 0.8 (37) 114 366H--I 161 0.5 (37) 133 298

C--F 135 1.5 77 64 488C--Cl 177 0.7 77 99 330C--Br 194 0.5 77 114 288C--I 214 0.2 77 133 216

Bond Bond Pauling's atomic EnthalpyLength ΔE.N. radii Single Bond

pm (pm) kJ/mol(Average)

Cl-Cl 199 0 99 243Br-Br 228 0 114 193I--I 267 0 133 151

H--F 92 1.8 (37) 64 568H--Cl 127 1 (37) 99 432H--Br 141 0.8 (37) 114 366H--I 161 0.5 (37) 133 298

C--F 135 1.5 77 64 488C--Cl 177 0.7 77 99 330C--Br 194 0.5 77 114 288C--I 214 0.2 77 133 216

C--F 135 1.5 77 64 488C--O 143 1 77 66 360C--N 147 0.5 77 70 308C--C 154 0 77 348

H--H 74 0 -37 436H--O 96 1.3 (37) 66 366H--N 101 0.8 (37) 70 391H--C 109 0.3 (37) 77 413

Bond length is nice, but it doesn’tReally relate to the Periodic tableAND it isn’t the whole story

Electronegativities? Can explain some trends

Bond Bond Pauling's atomic EnthalpyLength ΔE.N. radii Single Bond

pm (pm) kJ/mol(Average)

Cl-Cl 199 0 99 243Br-Br 228 0 114 193I--I 267 0 133 151

H--F 92 1.8 (37) 64 568H--Cl 127 1 (37) 99 432H--Br 141 0.8 (37) 114 366H--I 161 0.5 (37) 133 298

C--F 135 1.5 77 64 488C--Cl 177 0.7 77 99 330C--Br 194 0.5 77 114 288C--I 214 0.2 77 133 216

C--F 135 1.5 77 64 488C--O 143 1 77 66 360C--N 147 0.5 77 70 308C--C 154 0 77 348

H--H 74 0 -37 436H--O 96 1.3 (37) 66 366H--N 101 0.8 (37) 70 391H--C 109 0.3 (37) 77 413

H--H 74 0 -37 436H--C 109 0.3 (37) 77 413H--N 101 0.8 (37) 70 391H--O 96 1.3 (37) 66 366

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Bond Bond Pauling's atomic EnthalpyLength ΔE.N. radii Single Bond

pm (pm) kJ/mol(Average)

Cl-Cl 199 0 99 243Br-Br 228 0 114 193I--I 267 0 133 151

H--F 92 1.8 (37) 64 568H--Cl 127 1 (37) 99 432H--Br 141 0.8 (37) 114 366H--I 161 0.5 (37) 133 298

C--F 135 1.5 77 64 488C--Cl 177 0.7 77 99 330C--Br 194 0.5 77 114 288C--I 214 0.2 77 133 216

Bond Bond Pauling's atomic EnthalpyLength ΔE.N. radii Single Bond

pm (pm) kJ/mol(Average)

Cl-Cl 199 0 99 243Br-Br 228 0 114 193I--I 267 0 133 151

H--F 92 1.8 (37) 64 568H--Cl 127 1 (37) 99 432H--Br 141 0.8 (37) 114 366H--I 161 0.5 (37) 133 298

C--F 135 1.5 77 64 488C--Cl 177 0.7 77 99 330C--Br 194 0.5 77 114 288C--I 214 0.2 77 133 216

C--F 135 1.5 77 64 488C--O 143 1 77 66 360C--N 147 0.5 77 70 308C--C 154 0 77 348

H--H 74 0 -37 436H--O 96 1.3 (37) 66 366H--N 101 0.8 (37) 70 391H--C 109 0.3 (37) 77 413

Bond Bond Pauling's atomic EnthalpyLength ΔE.N. radii Single Bond

pm (pm) kJ/mol(Average)

Cl-Cl 199 0 99 243Br-Br 228 0 114 193I--I 267 0 133 151

H--F 92 1.8 (37) 64 568H--Cl 127 1 (37) 99 432H--Br 141 0.8 (37) 114 366H--I 161 0.5 (37) 133 298

C--F 135 1.5 77 64 488C--Cl 177 0.7 77 99 330C--Br 194 0.5 77 114 288C--I 214 0.2 77 133 216

C--F 135 1.5 77 64 488C--O 143 1 77 66 360C--N 147 0.5 77 70 308C--C 154 0 77 348

H--H 74 0 -37 436H--O 96 1.3 (37) 66 366H--N 101 0.8 (37) 70 391H--C 109 0.3 (37) 77 413

H--H 74 0 -37 436H--C 109 0.3 (37) 77 413H--N 101 0.8 (37) 70 391H--O 96 1.3 (37) 66 366

Bond Bond Pauling's atomic EnthalpyLength E.N. radii Single Bond

pm (pm) kJ/mol(Average)

H--H 74 2.2 37 436C--C 154 2.5 77 348Cl-Cl 199 3.2 99 243S-S 205 2.6 104 226

Br-Br 228 3 114 193N-N 145 3 70 159I--I 267 2.7 133 151O-O 148 3.5 66 145

??

Bottom line – atomic radii ΔE.N. seem to “best” determine bond enthalpies

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Bond enthalpies increase Single <Double < TripleBut not by multiples of the single bond

Bond Enthalpy (kJ/mol)X-X X=X X=X

C-C 347 612 820 measured694 1041 calc.

N-N 159 418 941 measured318 477 calc.

C-N 293 615 890 measured586 879 calc.

C-O 351 715 1075 measured702 1053 calc.

http://chemviz.ncsa.uiuc.edu/content/doc-resources-bond.html

Page 74: “A” students work (without solutions manual) ~  10 problems/night

Your book’s emphasis on bond enthalpies?

Relates to the energyreleased ortaken up

By a reaction

If Bonds of Reactants stronger than bonds products endothermic

We will take up the issue of bond enthalpy when discussingsolids

Page 75: “A” students work (without solutions manual) ~  10 problems/night

Examples we have examined about energy so far

H kJ 11 0 5. C O C Os g g( ) ( ) ( ) 1

2 2

H kJ C O C Os g g 3 9 3 5 2 2. ( ) ( ) ( )

Fossil fuel burning (coal)

H x kJ C H O C O H Og g 1 0 9 1 0 2 2 5 1 6 1 848 1 8 2 2 2. ( ) ( )

Fossil fuel burning (octane)

H kJ C H O C O H Og g g l 8 9 0 2 24 2 2 2( ) ( ) ( ) ( )

Fossil fuel burning (methane)

Hydrogen Fuel Cell

H kJ H O H Og g l 2 8 6 2

1

2 2 2( ) ( ) ( )

Page 76: “A” students work (without solutions manual) ~  10 problems/night

Energy Density Pure octane

Page 77: “A” students work (without solutions manual) ~  10 problems/night

FITCH Rules

G1: Suzuki is SuccessG2. Slow me down G3. Scientific Knowledge is ReferentialG4. Watch out for Red HerringsG5. Chemists are LazyC1. It’s all about chargeC2. Everybody wants to “be like Mike”C3. Size MattersC4. Still Waters Run DeepC5. Alpha Dogs eat first

Che

mis

try

Gen

eral

E kq q

r rel

1 2

1 2

Page 78: “A” students work (without solutions manual) ~  10 problems/night

“A” students work(without solutions manual)~ 10 problems/night.

Alanah FitchFlanner Hall [email protected]

Office Hours W – F 2-3 pm

Page 79: “A” students work (without solutions manual) ~  10 problems/night

Summary Slides

A B hea t C q endo therm ichea t to system

A B hea t C q exo therm ichea t to surround in gs

q cm t t cm tfina l in itia l

c is a measure of the intermolecular interactions; very large forwater = measure of the polarity of the water molecule

q H entha lpych ange H Hcons tp ressure products reac tstan tan

H H O H O

H H O H O

fu sion H O s l

vaporiza tion H O l g

, ( ) ( )

, ( ) ( )

2

2

2 2

2 2

Says something aboutintermolecular interactions (polarity!)

Page 80: “A” students work (without solutions manual) ~  10 problems/night

HkJ

kJ H O H Og g l

5 7 1 6

22 8 6 2

1

2 2 2

.( ) ( ) ( )

H kJ H O H Ol g g 5 7 1 6 2 22 2 2. ( ) ( ) ( )

H kJ H O H Og g l 5 7 1 6 2 22 2 2. ( ) ( ) ( )

An example of Hess’s Law

H H HOf productso

f reac tso , , tan

H kJ N O N OfO

g a tm C g a tm C g a tm C 8 8 21

2 2 1 2 5 2 1 2 5 2 1 2 5( , , ) ( , , ) ( , , )

An example of a reaction of standard molar enthalpy of formation

H E P V

H E P V P Vproducts reac ts

tan

Page 81: “A” students work (without solutions manual) ~  10 problems/night

Properties and MeasurementsProperty Unit Reference StateSize m size of earthVolume cm3 mWeight gram mass of 1 cm3 water at specified Temp

(and Pressure)Temperature oC, K boiling, freezing of water (specified

Pressure)1.66053873x10-24g amu (mass of 1C-12 atom)/12quantity mole atomic mass of an element in gramsPressure atm, mm Hg earth’s atmosphere at sea levelEnergy, General

electronic states in atom Energy of electron in vacuum

Electronegativity F

Heat flow measurements constant pressure, define system vs surroundingsper mole basis (intensive)

Standard Molar Enthalpy 25 oC, 1 atm, from stable stateHf

o Haq+ =0

Page 82: “A” students work (without solutions manual) ~  10 problems/night

“A” students work(without solutions manual)~ 10 problems/night.

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Office Hours W – F 2-3 pm