Chapter 2: Protecting the Ozone Layer Why do we need to do to protect the ozone layer? Isn’t ozone hazardous to human health? Why is the ozone layer getting smaller? What can we do (if anything) to help stop the depletion of our ozone layer? Ozone Formation Energy + 3 O2 2 O3 Energy must be absorbed (endothermic) for this reaction to occur. Ozone is an allotropic form of oxygen. An allotrope is two or more forms of the same element that differ in their chemical structure and therefore their properties. Element oxygen carbon Allotropes O2, O3 graphite, diamond, buckminister fullerenes 2.1 The Regions of the Lower Atmosphere Atmospheric pressure changes with altitude 2.1 The Regions of the Atmosphere Have you ever been in a plane landing in Denver, CO? You may have experienced being thrust forward as the plane uses more energy to stop. There are fewer air molecules at that height, reducing the amount of friction, so a greater amount of energy is needed to stop the plane. Why does it take longer to cook an egg in Denver than it does in New Orleans? There is less air pressure at higher altitudes. Water boils when the vapor pressure of the water molecules exceeds that of the localized air pressure. Because there is less air pressure at higher altitudes, more energy must be supplied (longer time) to get the temperature of the water high enough to cook the egg. 2.1 The ozone layer is a region in the stratosphere with maximum ozone concentration. 2.1 Atomic number (Z) -The number of protons. 8 (nuclear charge) O 16.00 Mass number (A) -The sum of the protons and neutrons. 2.2 2.2 The electrons in the outermost energy levels are called valence electrons. The group number (of the representative elements) on the periodic table tells you the number of valence electrons. Group 1A: 1 valence electron 1A 8A Group 3A: 3 valence electrons 2A 3A 4A 5A 6A 7A 2.2 Isotopes are two or more forms of the same element (same number of protons) whose atoms differ in number of neutrons, and hence in mass. Isotopes of carbon: C-12, C-13, C-14 also written as: 12C 13C 14C 2.2 Representing molecules with Lewis structures: Consider water, H2O: H O H 1. Find sum of valence electrons: 1 O atom x 6 valence electrons per atom = 6 + 2 H atoms x 1 valence electron per atom = +2 8 valence electrons 2. Arrange the electrons in pairs; use whatever electron pairs needed to connect the atoms, then distribute the remaining electron pairs so that the octet rule is satisfied: lone pair O H H bonding pair 2.3 Representing molecules with Lewis structures: Typical valence for selected atoms = the # of bonds an atom typically forms Element Typical valence 1 Classification O 2 divalent N 3 trivalent C 4 tetravalent H, X (X= F, Cl, Br, I) monovalent 2.3 Representing molecules with Lewis structures: Multiple bonds O H O Double bond C C H Triple bond Occasionally a single Lewis structure does not adequately represent the true structure of a molecule, so we use resonance forms: O O O O N N N O O O O O 2.3 Try these; draw valid Lewis structures for: O HNO3 N O CO2 H2S H O O C O Sulfur is under oxygen; think of H2O S H Sulfur is in the 3rd period: it can have an expanded octet H O H2SO4 Can you draw other valid Lewis structures for HNO3? S H O O O H O S H O O O H O O S H O H O 2.3 The Nature of Light Low E High E Wavelength (l) = distance traveled between successive peaks (nm). Frequency (n) = number of waves passing a fixed point in one second (waves/s or 1/s or s-1 or Hz). 2.4 The Electromagnetic Spectrum The various types of radiation seem different to our senses, yet they differ only in their respective l and n. 2.4 Visible: l = 700 - 400 nm ROY G BIV Decreasing wavelength Infrared (IR) : longest of the visible spectrum, heat ray absorptions cause molecules to bend and stretch. Microwaves: cause molecules to rotate. Short l range: includes UV (ultraviolet), X-rays, and gamma rays. 2.4 The wavelength and frequency of electromagnetic radiation are related by: c = ln where c = 3 x 108 m/s (the speed of light) The energy of a photon of electromagnetic radiation is calculated by: E = hn where h = 6.63 x 10-34 J.s (Plank’s constant) Energy and frequency are directly relatedhigher frequency means higher energy. 2.5 What is the energy associated with a photon of light with a wavelength of 240 nm? C = ln E=hn n =C l E = (6.63 x 10-34 J.s) (1.3 x 1015 s-1) E = 8.6 x 10-19 J n = 3 x 108 m/s -9 m = 1.3 x 1015 s-1 10 240 nm x nm UV radiation has sufficient energy to cause molecular bonds to break 2.5 2.6 The Chapman Cycle A steady state condition 2.6 Biological Effects of Ultraviolet Radiation The consequences depend primarily on: 1. The energy associated with the radiation. 2. The length of time of the exposure. 3. The sensitivity of the organism to that radiation. The most deadly form of skin cancer, melanoma, is linked with the intensity of UV radiation and the latitude at which you live. An Australian product uses “smart bottle” technology; bottle color changes from white to blue when exposed to UV light. 2.7 How CFCs Interact with Ozone CFC-11 Freon 11 trichlorofluoromethane CCl3F CFC-12 Freon 12 dichlorodifluoromethane CCl2F2 F F Cl C Cl Cl Cl C F Cl First, UV radiation breaks a carbon-halogen bond: .CClF + Cl. (free radicals) Photon (l < 220 nm) + CCl2F2 2 2.9 The chlorine radical attacks an O3 molecule: 2Cl. + 2O3 2ClO. + 2O2 Then two chlorine monoxide radicals combine: 2 ClO. ClOOCl The ClOOCl molecule then decomposes: UV photon + ClOOCl ClOO. The net reaction is: 2 O3 ClOO. + Cl. Cl. + O2 3O2 The Cl. radicals are free to attack more O3 The Cl. radicals are both consumed and generated; they act as catalysts 2.9 Experimental analyses show that as ClO. concentrations increase, ozone concentration decreases. 2.9 HCFCs are alternatives to CFCs: they decompose more readily in the troposphere so they will not accumulate to the same extent in the stratosphere. HCFC-22 chlorodifluoromethane HCFC-141b dichlorofluoroethane CHClF2 C2H3Cl2F F H C Cl F H H Cl C C H Cl F 2.12 Refrigerants for Automobile Use