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The Gaseous State of Matter

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The Gaseous State of Matter. Preparation for College Chemistry Columbia University Department of Chemistry. Chapter Outline. KMT. Gas Laws. Ideal Gas Equation. Gas Stoichiometry. Air Pollution. Preliminary Observations. Molar mass of water: 18g /mole. 6.02x10 23 molecules weigh 18g. - PowerPoint PPT Presentation
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The Gaseous State of Matter Preparation for College Chemistry Columbia University Department of Chemistry
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Page 1: The Gaseous State of Matter

The Gaseous Stateof Matter

Preparation for College ChemistryColumbia UniversityDepartment of Chemistry

Page 2: The Gaseous State of Matter

Chapter Outline

KMT

Gas Laws

Ideal Gas Equation

Gas Stoichiometry

Air Pollution

Page 3: The Gaseous State of Matter

Preliminary Observations

Molar mass of water: 18g /mole

6.02x1023 molecules weigh 18g

Density of water: 1g/cc

18 g liquid water occupies 18mL

18 g gaseous water occupies 22,400mL

Page 4: The Gaseous State of Matter

Kinetic Molecular Theory of Gases

KE =1

2m c =

2p = m c

p

2m

2

v=+10cm/s

c=10cm/s

Wall

-x +x

{v=-10cm/sc=10cm/s

12

mc2 = 32

kT

Page 5: The Gaseous State of Matter

Kinetic Molecular Theory of Gases

Page 6: The Gaseous State of Matter

0 600 1000 1400 1800200

0.4

0.6

0.8

1.0

1.2

1.4

Molecular Speed (ms-1)

# M

olec

ule

s

O2 at 1000°C

O2 at 25°C

Distribution of Molecular SpeedsMaxwell-Boltzmann Distribution

Page 7: The Gaseous State of Matter

RategasARategasB

=dBdA

=MB

MA

Graham’s Law of Effusion

At the same T and P, the rates of Effusion of two gases are inversely proportional to their densities or molar masses.

Page 8: The Gaseous State of Matter

VacuumGas

Naturally occurring Uranium : U-235 / U238 = 1 / 140

2nd step: Diffusion through thousands of membranes (cascades)

1st step: U + 6 F 235 UF6 238 UF6 (g)

R235−UF6

R238−UF6

=m238−UF6

m235−UF6

=352349

=1.0043

3rd step: 235 UF6

235U Fully enriched weapons-grade Uranium

Page 9: The Gaseous State of Matter

State Variables

V = volume (liters, cm3, m3)

T = temperature (in K)

P = pressure (atmospheres, mmHg, kPa)

Page 10: The Gaseous State of Matter

101.325 mbar

29.9 in. Hg

14.7 lb/in2 (PSI)

76 cmHg

760 mmHg760 torr

1 atm

Torricelli’s barometer

At sea level

Page 11: The Gaseous State of Matter

Atmospheric Pressure

150 kmHg height

air

Page 12: The Gaseous State of Matter

0 1 3 5 7

Volume (L)

9

1

2

3

4

5

6

Pre

ssu

re (

atm

)

0

7

Boyle’s Law

PV = C

At Constant TFor an Ideal Gas

P1 V1 = P2 V2

P1

V2

P2

V1

=

2

2

Page 13: The Gaseous State of Matter

0 1 3 5 7

1/V (L-1)

9

1

2

3

4

5

6

Pre

ssu

re (

atm

)

0

7

Boyle’s Law At Constant TFor an Ideal Gas

P =C 1V

⎝ ⎜

⎠ ⎟

2

Page 14: The Gaseous State of Matter

0 1 3 5 7

P

9

1

2

3

4

5

6

PV

0

7

Boyle’s Law At Constant TFor an Ideal Gas

2

Page 15: The Gaseous State of Matter

1

2

3

4

5

6

Vol

um

e (L

)

0

7

-300

T (°C)

-100 100 300 500

Charles’ Law At Constant P for an Ideal Gas

V T

-273°C

Absolute zero

V1V2

=T1T2

Page 16: The Gaseous State of Matter

0

1

2

3

4

5

6

Pre

ssu

re (

atm

)

7

-300

T (°C)

-100 100 300 500

P = CT

P1

T1

P2

T2

=

Gay-Lussac’s Law

At Constant V for an Ideal Gas P T

Page 17: The Gaseous State of Matter

Combined Gas Laws

V1

T1

V2

T2

=

P2 V2

T2

=P1 V1

T1

Charles’ Boyle’s

V1 P1 T2

P2 T1

=V2

P1 V1 = P2 V2

Page 18: The Gaseous State of Matter

STP Conditions

Standard Temperature: 273.15 K= 0°C

Standard Pressure: 1 atm

Reference Points for T and P for comparison

Page 19: The Gaseous State of Matter

Dalton’s Law of Partial Pressures

Ptot = P1 + P2 + P3 + ...

where P1 is the partial pressure of gas 1, etc...

Pgas = Ptotal – PH2O (table 11.3 p. 387)

where PH2O is the vapor pressure of water at the specified

temperature. Most often used in collection of insoluble gases

over water. In open systems, Ptotal = Patm

Pn = Xn Ptotal

Xn =nn

n1 + n2 + n3 + ...

Molar fraction of gasn

Page 20: The Gaseous State of Matter

Gay-Lussac’s Law of combining volumes

Avogadro’s Law

1809

1811

“When measured at the same T and P, the ratios of the V of reacting gases are small whole numbers”

“Equal volumes of different gases at the same T and P containthe same number of molecules”

Page 21: The Gaseous State of Matter

Consequences of Avogadro’s Law

1. Explanation of Gay-Lussac’s combining volumes law. Diatomic nature of elemental gases.

2. Method for determining molar masses of gases. The molar Volume.

3. Firm foundation of KMT: gases consists of microscopic particles

Page 22: The Gaseous State of Matter

Density of Gases

dV

=m

But V = f (P, T) dgasT ,P

Gas M(g/mol) d(g/L)

STPGas M(g/mol)

STPd(g/L)

H2

CH4

NH3

C2 H2

HCNCO

N2

air

H2S

HCl

F2

CO2

C3 H8

O3

SO2

Cl2

2.016

16.0417.03

26.04

27.03

28.01

28.02

28.9

32.00 1.4370.90 3.17

2.86

2.14

1.97

1.96

1.70

1.63

1.5234.09

36.46

38.00

44.01

44.09

48.00

64.071.25

1.25

1.21

1.16

0.760

0.716

0.900

1.29O2

Page 23: The Gaseous State of Matter

nT

PV

Ideal Gas Equation

TV

For one mole of a gas at STP, R constant:

(1 atm)(22.4L)

273K=R = 0.082

L-atm

mol-K

nV

nT

P=V R

=R TP V m

M

= n R TP V

=R T

MmPV

=PM

dRT

Equation of State1

PV

Page 24: The Gaseous State of Matter

Ideal Gas Equation

[pressure][Volume]

[temperature][mol]=[R] =

[force][volume]

[area][temperature][mol]

=[force][length]

[temperature][mol]=

[energy]

[temperature][mol]

R = 8.134 J mol-1 K-1 ~ 2 Cal mol -1 K-1

The ideal gas constant has energy/mol degrees dimensions

[R]

Page 25: The Gaseous State of Matter

Gas Stoichiometry

Cu(s) + 4H+ + 2NO3- (aq) Cu+2 (aq) + 2NO2 (aq) + 2H2O

Concentrated nitric acid acts on copper and produces nitrogen dioxide and dissolved copper. 6.80 g Cu is consumed and NO2 is collected at a pressure of .970atm and a temperature of 45°C (318 K) . Calculate the volume of NO2 produced.

63.55 g Cu

1 mol Cux6.80 g Cu x

1 mol Cu

2 mol NO2 = 0.214 mol NO2

n R T

P=V = 5.76 L NO2

Page 26: The Gaseous State of Matter

Real Gases

Follow the ideal gas law at sufficiently low densities

Gas molecules attract one another

Both factors increase in importance when the molecules are close together (high P. low T).

Gas molecules occupy a finite volume

n R T

P V=z

Deviations from ideality are quantified by the Compressibility factor z

Page 27: The Gaseous State of Matter

Real GasesIntermolecular Forces

0

0.5

1.0

1.5

Com

pres

sibi

lity

fac

tor 2.0

0

P (atm)200 400 600 800

Ideal Gas

H2

CH4

N2

Page 28: The Gaseous State of Matter

0

0.5

1.0

1.5

Com

pres

sibi

lity

fac

tor 2.0

0

P (atm)200 400 600 800

Ideal Gas

600 °C

-100 °C

25 °C

Nitrogen at several T

Page 29: The Gaseous State of Matter

Van der Waals Equation (1873)

P +an2

V2

⎝ ⎜ ⎜

⎠ ⎟ ⎟ V −nb( ) =nRT

b = constant representing volume excluded per mole of molecules

a = depends on the strength of attractive forces

n2

V2Proportional to reduction of wall collisions due to cluster formation.

Page 30: The Gaseous State of Matter

Air Pollution

Upper and Lower Atmosphere Ozone

Sulfur Dioxide

Nitrogen Oxides

Green House Effect

Page 31: The Gaseous State of Matter

Upper atmosphere Ozone

O2

h 2O

O2 O+ O3

O2O+O3

+ heat

CCl3F CCl2F . + Cl .

Cl . + O3 ClO . + O2

+ O O2 + Cl .

Allotropic Transformation

Ozone shield

Ozone Layer Destruction

Chain propagation

h

h

ClO .

Page 32: The Gaseous State of Matter

O2 + O + M O3< 3 ppm Ozone alert, M= N2 or O2

Radical Oxidation

Acid Rain Precursor

Tropospheric Chemistry

NO2 NO + O

h Photochemical Smog

SO2 + OH SO2OH

SO2OH + O2 SO3 + OOH

OOH O + OH

Page 33: The Gaseous State of Matter

http://www.epa.gov/globalwarming/emissions/index.html


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