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Chem 108

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Title: Chem 108


1
Chem 108
  • Environmental chem

2
  • 1 A diatomic molecule has the structure shown.
    Based on the use of outer shell electrons, what
    is a reasonable identity for "X" in the
    structure?
  • A)X Ne B)X F C)X O D)X N
  • 2 For these three parts of the electromagnetic
    spectrum, which is the correct order of
    increasing wavelength?
  • A) visible, ultraviolet, infrared
  • B) infrared, visible, ultraviolet
  • C) ultraviolet, visible, infrared
  • D) ultraviolet, infrared, visible

3
Light
  • Electromagnetic spectrum The entire range of
    radiant energy
  • Visible spectrum that which we see with our eyes
  • Wavelength The distance between successive
    peaks of a wave l
  • Frequency the number of waves passing a point in
    unit time n
  • C ln

4
Light
  • For Electromagnetic radiation
  • Speed of Light 3x108 m/s(in a vacuum)
  • Its not just a good Idea its the law its the
    fastest speed there is
  • From this
  • Frequencync/l wavelength lc/n
  • Red light has a wavelength of 650 nm what is its
    frequency
  • blue light has a frequency of 7.5 x10 14 What is
    its wavelength

5
Light
  • The shorter the wavelength the higher the
    frequency the more energy light has
  • Order the following in order of highest to lowest
    energy
  • Infrared microwave visible ultraviolet
  • (These are not in order)
  • Order them in from longest to shortest wavelength

6
Light
  • Light is quantized that is to say the smallest
    step you can have is one wavelength
  • no half steps.
  • We express this using Plancks constant
  • Ehn
  • We view light as packets of waves containing a
    specific amount of energy.
  • The effect of this is that it interacts with
    matter in stepwise fashion

7
Light
  • When light interacts with matter it interacts in
    a quantized way
  • First recognized by Einstein as the photoelectric
    effect (why he actually won the Nobel prize)
  • its not the intensity of a light source that
    causes interaction its the wavelength.
  • you will never tan under visible or IR light
    only under uv light

8
IR
UV
Vis
9
What does UV do
  • Breaks bonds

10
Biological Effects of Ultraviolet Radiation
  • The consequences depend primarily on
  • The energy associated with the radiation, and
  • The sensitivity of the organism to that radiation.

2.7
11
What does UV do to the body
  • Breaks bonds
  • broken bonds typically break so that each atom is
    electron deficient so they go around looking for
    a way to resolve that.
  • dimerization of DNA is a common solution
  • DNA is electron rich
  • DNA has to be able to be copied dimers interfere
    with copying
  • mistakes in copying lead to cancer

12
How ozone helps us
13
  • UV-A 320 -400
  • least energetic most prevalent
  • UV-B 280-320
  • More damaging than UV-A most absorbed by Ozone
  • UV-C 200-280
  • Most damaging lowest presence as we are screened
    by O2 and O3 in stratosphere

14
The UV index
  • http//www.epa.gov/sunwise/uviscale.html

15
The UV index
  • 2 or less Low
  • A UV Index reading of 2 or less means low danger
    from the sun's UV rays for the average person
  • Wear sunglasses on bright days. In winter,
    reflection off snow can nearly double UV
    strength.
  • If you burn easily, cover up and use sunscreen.
  • Look Out Below
  • Snow and water can reflect the sun's rays. Skiers
    and swimmers should take special care. Wear
    sunglasses or goggles, and apply sunscreen with
    an SPF of at least 15. Remember to protect areas
    that could be exposed to UV rays by the sun's
    reflection, including under the chin and nose.
  • 3 - 5 Moderate
  • A UV Index reading of 3 to 5 means moderate risk
    of harm from unprotected sun exposure.
  • Take precautions, such as covering up, if you
    will be outside.
  • Stay in shade near midday when the sun is
    strongest.
  • Me and My Shadow
  • An easy way to tell how much UV exposure you are
    getting is to look for your shadow
  • If your shadow is taller than you are (in the
    early morning and late afternoon), your UV
    exposure is likely to be low.
  • If your shadow is shorter than you are (around
    midday), you are being exposed to high levels of
    UV radiation. Seek shade and protect your skin
    and eyes.

16
The UV index
  • 6 - 7 High
  • A UV Index reading of 6 to 7 means high risk of
    harm from unprotected sun exposure. Apply a
    sunscreen with a SPF of at least 15. Wear a
    wide-brim hat and sunglasses to protect your
    eyes.
  • Protection against sunburn is needed.
  • Reduce time in the sun between 10 a.m. and 4 p.m.
  • Cover up, wear a hat and sunglasses, and use
    sunscreen.
  • Made in the Shades
  • Wearing sunglasses protects the lids of your eyes
    as well as the lens.
  • 8 - 10 Very High
  • A UV Index reading of 8 to 10 means very high
    risk of harm from unprotected sun exposure.
    Minimize sun exposure during midday hours, from
    10 a.m. to 4 p.m. Protect yourself by liberally
    applying a sunscreen with an SPF of at least 15.
    Wear protective clothing and sunglasses to
    protect the eyes.
  • Take extra precautions. Unprotected skin will be
    damaged and can burn quickly.
  • Minimize sun exposure between 10 a.m. and 4 p.m.
    Otherwise, seek shade, cover up, wear a hat and
    sunglasses, and use sunscreen.
  • Stay in the Game
  • Be careful during routine outdoor activities such
    as gardening or playing sports. Remember that UV
    exposure is especially strong if you are working
    or playing between the peak hours of 10 a.m. and
    4 p.m. Don't forget that spectators, as well as
    participants, need to wear sunscreen and eye
    protection to avoid too much sun.

17
The UV index
  • 11
  • A UV Index reading of 11 or higher means extreme
    risk of harm from unprotected sun exposure. Try
    to avoid sun exposure during midday hours, from
    10 a.m. to 4 p.m. Apply sunscreen with an SPF of
    at least 15 liberally every 2 hours.
  • Take all precautions. Unprotected skin can burn
    in minutes. Beachgoers should know that white
    sand and other bright surfaces reflect UV and
    will increase UV exposure.
  • Try to avoid sun exposure between 10 a.m. and 4
    p.m.
  • Seek shade, cover up, wear a hat and sunglasses,
    and use sunscreen.
  • Beat the Heat
  • It is possible to go outside when the UV Index is
    11 or higher. Make sure you always seek shade,
    wear a hat, cover up, wear 99-100 UV-blocking
    sunglasses, and use sunscreen. Or you can opt to
    stay indoors and take the opportunity to relax
    with a good book rather than risk dangerous
    levels of sun exposure.

18
How ozone helps us
  • For every 6 decrease in Ozone we expect to see a
    12 increase in skin cancer
  • Fortunately is mostly non melanoma type
  • From 1973 ozone measured about Arosa Switzerland
    has decreased Approximately 6. (Fig 2.17)

19
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20
?????
?240-320
21
How is Ozone Made
  • The Chapman Cycle
  • Step 1
  • O2 ????? ? 2O
  • Step 2
  • O O2? O3
  • UV absorbtion by Ozone
  • O3 ?240-320 ? O O2

Step 3 O O3? 2O2
22
Where ozone is found
23
How much is there
  • Not much
  • 1018 to 1019 Molecules m3 in the stratosphere
  • thats 183 ppb (0.2 ppm)
  • If you brought it together as a isolated band at
    1 ATM it would be 1/8th inch thick
  • A lot
  • 3 x 108 Tons Formed and consumed daily

24
What governs the amount of stratospheric ozone
  • The amount of UV radiation
  • more at the poles than at the equator.
  • the incident angle of radiation is higher at the
    poles
  • Seasonal variation Summer levels are Higer than
    winter levels
  • 22 year Solar cycle
  • Distribution by upper atmospheric winds
  • Both natural and man made chemicals that degrade
    ozone.

25
The Antarctic Ozone hole
From the NASA Web Site
26
What do we think is causing the Hole.
  • Presence of Chlorofluorocarbons in the
    stratosphere

27
The Evidence
As ClO. concentrations increase, ozone
concentration decreases. We will see that ClO.
is a product of CFC degradation.



2.9
28
l ? Cl . .CCl2F
2Cl . ? Cl2
29
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30
Catalytic Cycles For Ozone Loss General Idea
O3 X ? XO O2 O XO ? X O2 Net O3
O ? 2 O2 X is a catalyst
The catalyst is neither created nor destroyedbut
the rate for the catalytic cycle Ox removal in
this case depends on catalyst concentrations
31
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32
Chlorofluorocarbons
  • Great refrigerants
  • Previous chemicals where amonia and H2S
  • Great propellants
  • Aerosol cans
  • Non-toxic Non-flammable Inert
  • Used for asthma inhalers

33
Additional compound that affect Ozone
  • Other Haloforms
  • Non toxic fire suppressants
  • Halon 1211 (bromochlorodifluoromethane, CF2ClBr)
  • Halon 1301 (bromotrifluoromethane, CBrF3)
  • Not so benign
  • Carbon tetrachloride CCl4
  • Formerly Used both as fire suppressant and dry
    cleaning fluid

34
Next Up
  • What to do What to Do?

35
Where we are
  • Completed 2.8
  • some bits of 2.9-11 covered today next lecture
    will focus on sections 2.9-2.13
  • Work problems 1-18 25-36 41-43
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