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Chapter 3: Global Warming

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Title: Chapter 3: Global Warming


1
Chapter 3 Global Warming
Chem 100 Lecture 5 February
1, 2005
2
Questions
  • What is the greenhouse effect?
  • Is the concentration of CO2 really increasing?
  • How much CO2 do we produce?
  • Is the earth really warming?
  • What molecules contribute to the greenhouse
    effect?
  • Molecular structure

3
Earths atmosphere traps solar energy
  • Radiation from sun hits the atmosphere
  • Some reflected back
  • Some absorbed
  • Ex molecules such as O3 absorb UV radiation
  • Most visible radiation is unabsorbed passes
    thru atmosphere (eventually absorbed by the
    earth)
  • Earth warms radiates heat as IR radiation

Earth basically converts visible radiation
to IR radiation
4
The atmosphere traps energy
  • Certain compounds in the atmosphere (such as CO2)
    absorb IR radiation and then re-emit the
    radiation
  • This traps the energy that would have been
    radiated away from Earth
  • 84 of the radiated heat is absorbed by the
    atmosphere reradiated back to the earth.
  • A balance (steady-state) exists between
    maintaining the earths temperature and climate.

5
What might change the balance?
  • Decreasing levels of O3
  • Would allow more UV radiation to reach the earth
  • This radiation can be transformed to IR that will
    be radiated away from earth
  • Increased levels of CO2 (and other compounds that
    absorb emit IR radiation)

6
Sources/sinks of atmospheric CO2
  • Sources
  • Respiration
  • CO2 byproduct
  • Decomposition
  • Microbial byproduct
  • Combustion
  • Forest fires
  • Fossil fuels
  • Sinks
  • Oceans
  • CO2 dissolves in waterthe amt depends on temp
    currents
  • Minerals
  • Limestone CaCO3
  • Photosynthesis
  • 6CO2 H2O ? C6H12O6 6O2

Ideally, sources and sinks are balanced
atmospheric CO2 concentrations remains constant.
7
Sources and sinks roughly balanced on a per/year
basis
Over time, amount increases
8
The Carbon Cycle
9
Connection b/w CO2 global temp?
  • Historical records
  • Estimate of atmospheric CO2 vs. time temp vs.
    time show a similar pattern

Deuterium is heavier than hydrogen ?Deuterium
wont evaporate as easily as hydrogen ?As
temperature increases, more evaporation
occurs, and the concentration of deuterium
is higher High D/H ratio correlates to high temps
Does this prove that CO2 increases cause temp
increases?
10
Temperature can affect CO2
  • Oceans can store more CO2 at cooler temps
  • Note that sodas go flat faster at higher temps
    (higher temps allow gas to escape more quickly)

11
Trend in Recent Times
  • CO2 concentrations seem to have risen by 25 from
    1957 1993
  • Global temperature has increased between 0.4 and
    0.8oC from 1880 1990
  • Are these changes significant, or just a blip
    in the historical record?

12
Identifying a greenhouse gas
  • Some
  • Greenhouse gases
  • CO2, CH4, H2O
  • All absorb emit IR radiation
  • Some
  • non-greenhouse gases
  • O2, N2
  • Do not absorb emit IR radiation

What gives a molecule the ability to absorb
emit IR radiation? Before we get to this, we
need to understand molecular structure
13
Intro to Molecular Structure
Diatomic atoms can ONLY have a linear shape
If there are 3 or more atoms, the molecule may
not be linear

H O H
O
H
H

14
General Rule for structure
  • The most stable arrangement is the one that keeps
    repelling e- as far away as possible.
  • This includes e- in bonds, lone pair e-, and
    single e-

15
Stepwise procedure
  • Determine of e- groups around the central atom
    (draw Lewis Structures)

CO2
H2O
CH4
2) Most stable shape is the one in which the e-
are as far apart as possible
Ex for 4 e- groups
16
Molecular structure of NH3
4
How many e- groups around N are there?
  • Lone pair e- are less tightly held to the central
    atom than the e- in bonds, so lone pair of e- are
    extra repulsive.
  • Repel the e- in the N-H bonds pushing the H atoms
    closer together

107.5o
Triangular pyramidal structure
17
Molecular structure of water
4
How many e- groups around O are there?
Oxygen has 2 lone pairs of e- so the H atoms are
pushed together even more
104.5o
Bent shape
18
Molecular structure of ozone
How many e- groups?
3
  • Furthest apart 3 e- groups can be is 120o
  • Again, lone pair of e- have more repulsion and
    force O atoms to be slightly closer than 120o

Trigonal planar
19
Molecular structure of CO2
2
How may e- groups around C are there?
linear
20
Summary Table
Total e- pairs
2
3
4
21
Absorption of different energy radiation leads to
different effects
  • IR radiation (l 10-5 m) has less energy than
    UV radiation (l 10-8 m)
  • Not enough energy to break bonds
  • But this IS enough energy to cause
  • bond vibration
  • Similarly, microwaves (l 10-2 m) have less
    energy than IR.
  • This energy is enough to rotate molecules
  • Microwave ovens work by exciting (through
    rotation) water molecules in food.

22
Molecular Vibrations
  • Bonds can be thought of as springs
  • Different bond strengths correspond to different
    spring tensions.
  • Springs with more tension require absorption of a
    higher energy IR photon for vibration to occur
  • Photon frequency (n) vibration frequency
  • Only certain types of vibrations are able to
    absorb radiation

23
Types of vibrations possible for CO2
  • Symmetric vibration

2. Asymmetric vibration
  • Bending vibration
  • in-plane

4. Bending vibration out of plane
  • Different vibrations correspond to different
    energies of IR radiation
  • It is easier to bend a molecule than stretch it
  • Therefore, bending will occur with absorption of
    lower energy IR
  • radiation

24
Vibrations that absorb radiation
  • In order to absorb radiation, the vibration must
    involve a change in the overall electron charge
    distribution
  • Radiation is a changing electric field
  • Only a changing electric field in the molecule
    can interact with it
  • Atoms have different abilities to attract bonding
    e-
  • In , bonding e- are shared but they
    tend to be more around O than the C
  • O has more electronegativity
  • (O has a stronger pull for the e- than C)

-
-

25
Electronegativity trend in periodic table
Increasing electronegativity
26
Only Vibrations with a change in charge
distribution absorb radiation
-
-
  • Symmetric vibration


-
-

2. Asymmetric vibration
  • Bending vibration
  • in-plane

-
-

4. Bending vibration out of plane
-
-

27
Some requirements for absorbing IR radiation
  • Molecule must have more than 1 atom
  • Need more than 1 type of atom
  • These molecules dont absorb IRbecause the atoms
    in the molecules have the same electronegativity,
    there is no partial and partial to the bond
  • Thus, there would be no change in the charge
    distribution during vibration

28
Greenhouse effect
The greenhouse gas molecule absorbs IR energy,
and the molecule vibrates. The molecule can go
back to a normal (non-vibrational) state by
emitting energy back to Earth.
29
IR spectroscopy
IR spectrum of CO2
A 1/T A absorbance T transmission Low T
High A
An instrument called an IR spectrometer can
measure the IR absorbed by a molecule
30
IR tutorial with molecular vibration animations
From http//chemistry.beloit.edu/Warming/pages/i
nfrared.html
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