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Topics for Today Greenhouse Gases: How do they keep us warm?

Topics for Today Greenhouse Gases: How do they keep us warm?

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Topics for Today Greenhouse Gases: How do they keep us warm? Slide 2 Readings for Today 3.4 Vibrating Molecules and the Greenhouse Effect Slide 3 Topics for Friday Climate Change: A Global Problem? Quiz #7 (of 11)!! Slide 4 Readings for Friday 3.8 Methane and other greenhouse gases 3.10 Responding to science with policy changes 3.11 The Kyoto Protocol on Climate Change 3.12 Global warming and ozone depletion May even bleed into Monday. Slide 5 Announcements!!! Slide 6 Bring back your radon disks!! Slide 7 Announcements! Nice, warm weather Please remember: Do not wear shorts or sandals to lab!! Slide 8 Exam Regrading Same process as Exam 1. Slide 9 Topics for Today Greenhouse Gases: How do they keep us warm? Slide 10 Review from Monday Slide 11 Review The Greenhouse Effect Slide 12 Review from a long time ago. Lecture 15. ( ( Slide 13 Gamma rays X-rays May ionize the molecule What happens when molecule absorbs light? Slide 14 Gamma rays X-rays May ionize the molecule UV light May break bonds in the molecule Slide 15 Gamma rays X-rays May ionize the molecule UV light May break bonds in the molecule Visible light Usually doesnt do much w/out help Slide 16 Gamma rays X-rays May ionize the molecule UV light May break bonds in the molecule Visible light Usually doesnt do much w/out help Infrared Important for climate change coming up!! Slide 17 Gamma rays X-rays May ionize the molecule UV light May break bonds in the molecule Visible light Usually doesnt do much w/out help Infrared Important for climate change coming up!! What happens to a molecule when it absorbs IR? Slide 18 Figure 3.17 Among other motions, this includes stretching and bending! Slide 19 Slide 20 Gamma rays X-rays May ionize the molecule UV lightMay break bonds in the molecule Visible lightUsually doesnt do much w/out help InfraredVibrates Molecule What happens to a molecule when it absorbs IR? Slide 21 Q: When will IR cause a molecule to vibrate? A: When there is a dipole moment! Slide 22 Dipole Moment: Unequal distribution of charge! Where have we seen dipole moments before? Slide 23 Polar Bonds: Unequal sharing of electrons in a chemical bond. Still a covalent bond! RESULTS IN AN UNEQUAL DISTRIBUTION OF CHARGE!! From Lecture 19 or so Slide 24 HCl -- ++ H H H N ---- ++++ ++++ ++++ ---- ++++ ++++ O HH A bunch of polar molecules That is, they have dipoles Slide 25 What about some other molecules? OCO.. Slide 26 OCO Carbon Dioxide Polar or nonpolar bonds? Slide 27 OCO.. Carbon Dioxide Polar bonds ---- ---- ++++ Slide 28 Carbon Dioxide Polar or nonpolar molecule? OCO.. ---- ---- ++++ Slide 29 Carbon Dioxide Nonpolar Molecule So, no overall dipole moment But CO 2 is a greenhouse gas! Why does it absorb IR radiation? OCO.. ---- ---- ++++ Slide 30 The IR can cause (or induce) a dipole moment! Slide 31 Possible Vibrations for CO 2 Think ELECTRONEGATIVITY!!! Slide 32 Symmetric Stretch Both out, both in Keeps linear shape Slide 33 Symmetric Stretch Both out, both in Keeps linear shape Slide 34 Symmetric Stretch Both out, both in Keeps linear shape Does this induce a dipole moment? Slide 35 Asymmetric Stretch One in and one out Keeps linear shape Slide 36 Asymmetric Stretch One in and one out Keeps linear shape Slide 37 Asymmetric Stretch One in and one out Keeps linear shape Does this induce a dipole moment? Slide 38 Bend Bends in one plane Loses linear shape Slide 39 Bend Bends in one plane Loses linear shape Slide 40 Bend Bends in one plane Loses linear shape Does this induce a dipole moment? Slide 41 Bend Bends in another plane Loses linear shape Same as the other bend, just in a different plane Slide 42 Figure 3.17 IR vibrations for a linear 3 atom molecule Slide 43 Bending in each plane http://chemistry.boisestate.edu/rbanks/spectroscopy/co2vibrations.gif Slide 44 CO 2 bending and stretching Summary Symmetric Stretch Asymmetric Stretch Bend 1 Bend 2 Which of these is able to produce a dipole moment? CO 2 has THREE possible ways to absorb IR!! How do we measure this? Slide 45 Spectrophotometry Sort of Slide 46 Figure 3.15 in your Text What are wavenumbers? Slide 47 4 m = 4000 nm! What is transmittance ? Slide 48 The opposite of absorbance! Absorbance Slide 49 Review The Greenhouse Effect Slide 50 http://www.spaceguarduk.com/cd/dict/dictionary/infrared.htm Slide 51 Where is visible light? Higher Energy Lower Energy Slide 52 Slide 53 What happens when a molecule absorbs light? It depends on the wavelength Slide 54 Gamma rays X-rays May ionize the molecule UV lightMay break bonds in the molecule Visible lightUsually doesnt do much w/out help InfraredVibrates Molecule What happens to a molecule when it absorbs IR? Slide 55 What happens when a molecule absorbs light? AND on the molecule. It depends on the wavelength Slide 56 Summary For a molecule to absorb IR radiation, it must 1) Permanently have an uneven distribution of charge (dipole) Slide 57 HCl -- ++ H H H N ---- ++++ ++++ ++++ ---- ++++ ++++ O HH Polar molecules have dipole moments Slide 58 Summary For a molecule to absorb IR radiation, it must 1) Permanently have an uneven distribution of charge (dipole) OR 2) Vibrate in a way that can CREATE an uneven distribution of charge (dipole) Nonpolar molecules MAY or MAY NOT absorb IR radiation Slide 59 CO 2 bending and stretching Summary Symmetric Stretch Asymmetric Stretch Bend 1 Bend 2 Slide 60 Summary For a molecule to absorb IR radiation, it must 1) Permanently have an uneven distribution of charge (dipole) OR 2) Vibrate in a way that can CREATE an uneven distribution of charge Nonpolar molecules MAY or MAY NOT absorb IR radiation Slide 61 Do N 2, O 2, or Ar absorb IR radiation? Slide 62 O O.. NN 1) Polar or nonpolar molecules? 2) Can we vibrate these to produce a dipole moment? Ar Slide 63 These molecules / atoms are NOT GHGs. 1) They are nonpolar 2) They cannot vibrate to create an unequal distribution of charge. Slide 64 Summary For a molecule to absorb IR radiation, it must 1) Permanently have an uneven distribution of charge (dipole) OR 2) Vibrate in a way that can CREATE an uneven distribution of charge -A molecule with 3+ atoms Slide 65 How about water? H H O.. Is water polar? But it can also vibrate!! Slide 66 Water vapor is an extremely strong absorber of IR And a very potent GHG!! Slide 67 Water Vapor Figure 3.16 Slide 68 Figure 3.15 in your Text CO 2 Slide 69 Water Vapor Figure 3.16 CO 2 absorbs here Slide 70 Water Vapor Figure 3.16 CO 2 absorbs here Different molecules absorb different wavelengths! Slide 71 Does an increase in water vapor lead to an increase in Earths temperature? Slide 72 On one hand Slide 73 Water Vapor Figure 3.16 Slide 74 On one handOn the other hand Slide 75 Interactions with Clouds Clouds Condensed water on a seed particle Reflects solar radiation Slide 76 Review What is the Greenhouse Effect? Slide 77 The Greenhouse Effect Solar radiation Long-wave radiation Greenhouse Gases Greenhouse gases are transparent to incoming solar radiationGreenhouse gases are transparent to incoming solar radiation Greenhouse gases absorb the infrared light which is emitted from the earthGreenhouse gases absorb the infrared light which is emitted from the earth This traps energy in the earths atmosphereThis traps energy in the earths atmosphere Slide 78 Slide 79 About 80% of the heat emitted from the surface is trapped in the atmosphere Slide 80 The Earths atmosphere is about 380 ppm CO 2 The average temperature is about 59 o F Slide 81 What would the average temperature of Earth be with no CO 2 ? About -4 o F! Slide 82 About 80% of the heat emitted from the surface is trapped in the atmosphere Any more than this 80% is called the enhanced greenhouse effect. Slide 83 Some people are worried that this will lead to climate change (global warming) Slide 84 Greenhouse gases CH 4 CO 2 H 2 O N 2 O (nitrous oxide) CFCs and replacements Slide 85 Greenhouse gases CH 4 CO 2 H 2 O N 2 O (nitrous oxide) CFCs and replacements DONE! Slide 86 Water Vapor Figure 3.16 Slide 87 Water Vapor Extremely strong dipole moment (Very good at absorbing IR) Most abundant greenhouse gas (varies from 0-4% of the atmosphere) Slide 88 Some GHGs CFCs HCFCs HFCs CO 2 CH 4 N2ON2O O3O3 H2OH2O Slide 89 What makes greenhouse gases more potent? N2ON2O CFCs HCFCs HFCs CH 4 CO 2 CH 4 O3O3 H2OH2O Slide 90 1) Atmospheric Lifetime Slide 91 Methane Atmospheric lifetime about 10 years Removed by the hydroxyl radical we will see this reaction Monday! Slide 92 CFCs Atmospheric lifetime >> 100 years Destroyed in the stratosphere by UV-C Slide 93 1) Atmospheric Lifetime 2) Atmospheric Concentration Slide 94 Concentration of CO 2 is about 370 ppm. Slide 95 Slide 96 CFC concentrations are around 0.007 ppm Slide 97 1) Atmospheric Lifetime 2) Atmospheric Concentration 3) How efficiently can the molecule absorb IR? Slide 98 CO 2 bending and stretching Summary Symmetric Stretch Asymmetric Stretch Bend 1 Bend 2 CO 2 has only 3 vibrations Slide 99 CFCs CFCs have at least 10 possible vibrations!! CFCs are much more efficient at trapping IR than CO 2. This is due to the more complicated SHAPE