Ozone in the Atmosphere

Similar documents
Section 2: The Atmosphere

Atmosphere. Earth's atmosphere is a mixture of gases, solids, and liquids that surround the planet.

ATOC 3500/CHEM 3151 Air Pollution Chemistry Lecture 1

The Atmosphere and Atmospheric Energy Chapter 3 and 4

8.8 - Gases. These are assumptions that can be made about 99% of the gases we come in contact with which are called ideal gases.


AT 350 EXAM #1 February 21, 2008

Unit 3 Review Guide: Atmosphere

Common Elements: Nitrogen, 78%

2/22/ Atmospheric Characteristics

Chapter 4 Lesson 1: Describing Earth s Atmosphere

Ozone: Earth s shield from UV radiation

STRATOSPHERIC OZONE DEPLETION. Adapted from K. Sturges at MBHS

Guided Reading Chapter 16: The Atmosphere

NATS 101 Section 13: Lecture 31. Air Pollution Part II

The Atmosphere. Composition of the Atmosphere. Section 2

The Atmosphere. Characteristics of the Atmosphere. Section 23.1 Objectives. Chapter 23. Chapter 23 Modern Earth Science. Section 1

Chemistry of Ozone. Explain the following terms: resonance, resonance hybrid, delocalisation

Topic # 13 (cont.) OZONE DEPLETION IN THE STRATOSPHERE Part II

9.5 Troposphere. Describe the characteristics and importance of the troposphere. Explain temperature inversion and its role in the troposphere.

(for tutoring, homework help, or help with online classes)

Atmosphere. Transfer in the Atmosphere

RADIATION and the EM Spectrum

Chapter 2 Protecting the Ozone Layer. The Ozone Hole

OBJECTIVES: By the end of today s lesson, you will be able to. SWBAT list the layers of the atmosphere and describe the characteristics of each one.

The Atmosphere - Chapter Characteristics of the Atmosphere

Chapter 2: Protecting the Ozone Layer

Discuss Yesterday s Lab. What Do We Know? Funny Ozone Video. Ozone Layer Defined! Ozone Layer. Warm-Up 3/3/2015

1 Characteristics of the Atmosphere

Environmental Science Chapter 13 Atmosphere and Climate Change Review

I T A T I O N H B I T B T V A O C J K M R S A T M O S P H E R E

Prentice Hall EARTH SCIENCE. Tarbuck Lutgens

Table of Contents. Chapter: Atmosphere. Section 1: Earth's Atmosphere. Section 2: Energy Transfer in the Atmosphere. Section 3: Air Movement

This site aims to provide information on the chemistry of ozone and provide some useful links to other pages.

Property Ozone Vs Oxygen. Molecular Formula: O3 O2. Molecular Mass: Color: light blue Colourless

Topic # 15 OZONE DEPLETION IN THE STRATOSPHERE. see pp in Class Notes

Unit 9. Atmosphere. Natural Science 1º ESO Antonio Jesús Moreno Quintero. Colegio Guadalete. Attendis.

Directed Reading. Section: Solar Energy and the Atmosphere RADIATION. identical point on the next wave. waves

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds. What is an atmosphere? Planetary Atmospheres

Q U E S T I O N S. 2/ The sun sends us (several correct answers) Light Energy Fire Warmth Rain

Light Matter Interactions: Theory and Applications (LMITA) What is Light?

1. The frequency of an electromagnetic wave is proportional to its wavelength. a. directly *b. inversely

The Atmosphere. Topic 3: Global Cycles and Physical Systems. Topic 3: Global Cycles and Physical Systems. Topic 3: Global Cycles and Physical Systems

Overview of Photosynthesis

Characteristics of the Atmosphere

Physical Geography 1st Exam

1 Characteristics of the Atmosphere

Ozone Depletion. Dana Desonie, Ph.D. Say Thanks to the Authors Click (No sign in required)

In the space provided, write the letter of the description that best matches the term or phrase. as waves. thermosphere

Layers of the Atmosphere

Earth s Atmosphere. Composition

Chapter 2 Protecting the Ozone Layer

2.1 Ozone. Ozone O 3. Oxygen O 2 1/30/2015 CHM 107

The Atmosphere: Structure and Temperature

Surface Processes and the Hydrosphere Unit Heating the Earth s Atmosphere Chapter 11 (pg )

Measurements of Ozone. Why is Ozone Important?

AST 105 Intro Astronomy The Solar System

Planetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc.

LECTURE 6 - THE EARTH'S ATMOSPHERE

Chapter 2. Heating Earth's Surface & Atmosphere

Lecture Outlines PowerPoint. Chapter 16 Earth Science 11e Tarbuck/Lutgens

Tananyag fejlesztés idegen nyelven

ELECTROMAGNETIC SPECTRUM All waves travel the SAME speed (the speed of light) 300,000 km/sec (186,000 miles/sec) in a vacuum

1 Characteristics of the Atmosphere

An Interpretation of Natural Healing of Ozone Holes

Lecture 14 - Radiative equilibrium and the atmospheric greenhouse effect

Name Team Period. Station #1 (drawing)

Unit 2 Meteorology Test **Please do not write on this test** 5. El Nino & La Nina 6. Photosynthesis 7. Coriolis Effect 8.

UTTAM SCHOOL FOR GIRLS PSA WORKSHEET: SCIENCE GRADE: VI

Let s Think for a Second

Chapter 5: Light and Matter: Reading Messages from the Cosmos

HSC Chemistry. Chemical Monitoring and Management. DUXCollege. Term 1 Week 7. Student name:. Class code:.. Teacher name:.

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds. What is an atmosphere? Earth s Atmosphere. Atmospheric Pressure

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds

The Earth is surrounded by a blanket of air, which we call the atmosphere. It reaches over 560 kilometers

atmosphere: a mixture a gases that surrounds the planet Earth.

Grade 7 Revision sheet Key Answer. Kingdom of Bahrain Ministry of Education Ahlia School -ABCD

Climate Change Lecture Notes

Planetary Atmospheres (Chapter 10)

Table of Contents. Chapter: Atmosphere. Section 1: Earth's Atmosphere. Section 2: Energy Transfer in the Atmosphere. Section 3: Air Movement

COMPOSITION OF THE ATMOSPHERE

The Layered Atmosphere:

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds. What is an atmosphere? About 10 km thick

). It is a gas produced naturally in the stratosphere where it strongly absorbs incoming

Outline. Planetary Atmospheres. General Comments about the Atmospheres of Terrestrial Planets. General Comments, continued

Lecture 25: Atmosphere & environment

5. In which diagram is the observer experiencing the greatest intensity of insolation? A) B)

Chapter 02 Energy and Matter in the Atmosphere

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds

Key Concept Heat in Earth s atmosphere is transferred by radiation, conduction, and convection.

Light and Matter: Reading Messages from the Cosmos. White light is made up of many different colors. Interactions of Light with Matter

Characteristics of the Atmosphere

OZONE AND ULTRAVIOLET RADIATION

Topic # 14 OZONE DEPLETION IN THE STRATOSPHERE

C) wavelength C) eastern horizon B) the angle of insolation is high B) increases, only D) thermosphere D) receive low-angle insolation

ATMOSPHERE PACKET CHAPTER 22 PAGES Section 1 page 546

3. Which color of the visible light has the shortest wavelength? A) violet B) green C) yellow D) red

Chemistry 1500: Chemistry in Modern Living. Topic 1: The Air We Breathe. States of Matter, Reactions, and Risk

Clever Catch Weather Ball Question and Answer Sheets

Your web browser (Safari 7) is out of date. For more security, comfort and the best experience on this site: Update your browser Ignore

Transcription:

Ozone in the Atmosphere Why are we concerned with ozone? This simple molecule affects us in very important ways. It protects us, as well as all animals and plants on our planet, from the harm that ultraviolet radiation from the sun would cause. Ozone is a very reactive molecule and too much of it close to the ground causes damage to our lungs. First, a little about its properties. Ozone, or O3, is produced when elemental oxygen, O2, is broken apart by an electric discharge or UV light. The sharp odor after a lightning storm is due to ozone. Ozone is much more reactive with other molecules than O2. It is a gas with a slight blue color under normal conditions with a boiling point of -119 deg C and a melting point of -192.5 deg C. The solid has a dark blue-violet color. While we examine the chemistry of ozone, we'll explore the bonding in simple molecules, the nature of energy, some key chemical reactions, and the energy changes caused by chemical reactions. Last time you reviewed Lewis structures and electronic bookkeeping. This is a simple but adequate bonding model that tells us about the number of bonds atoms can make and something about electron density in molecules. Today we'll have an overview of ozone. The next lectures concern different types of energy and the way light energy interacts with ozone. Outline The Ozone Layer Ozone and Smog Industrial Applications Homework The Ozone Layer The Solar Spectrum To understand the importance of ozone in the atmosphere, we first must understand the nature of the energy that comes to us from the sun. The sun and other stars are very hot and so radiate energy. Specifically, we call this energy electromagnetic energy. We can characterize electromagnetic radiation according to its wavelength. Remember that the energy of the radiation is inversely proportional to the wavelength. Chemistry 104 Prof. Shapley page 1

E = hc/λ The shape of the intensity vs. wavelength curve depends on the temperature of the emitting object. The higher the temperature, the higher is the maximum intensity and the lower the wavelength of this maximum. The maximum intensity of the sun's output of radiation is in the visible light region. At the top of the atmosphere, approximately 7% of the radiation is in the ultraviolet, 41% in the visible, and 52% in the infrared. The intensity of electromagnetic radiation that reaches the surface of our planet is considerably less than that at the top of the atmosphere. Something in the atmosphere filters out energy. The highest energy light is most effectively filtered out. This is very important because high energy light (gamma rays, x-rays, UV-radiation) penetrates the cells of living things and causes damage to them. Chemistry 104 Prof. Shapley page 2

Molecular Filters Consider the figure at right. The magenta filter blocks some wavelength of light, the cyan and yellow filter block others. When the 3 filters are combined, all wavelengths of visible light are blocked and the color appears black. The atmosphere consists of many molecular and atomic filters that each block a certain range of wavelengths of light. With the combined effect of all of these, most of the harmful radiation from the sun is blocked before it reaches the plants and animals on the surface of the Earth. In the highest region of the atmosphere, the ionosphere, atoms such as N absorb very high energy light and lose electrons. N + energy N + + e - Below that, in the mesosphere, strongly-bonded molecules such as N2 absorb energy and break apart. N2 + energy 2 N Below that, in the stratosphere, ozone absorbs nearly all the ultraviolet radiation (between 200 and 310 nm). In the lowest region of the atmosphere, the troposphere, colored molecules absorb some visible light and other molecules (H2O, CO2) absorb infrared or heat energy. Ozone in the Stratosphere Ozone has a low concentration throughout the atmosphere but there is a region in the stratosphere where its concentration is higher than anywhere else. About 90% of the ozone in the atmosphere is located within a band centered at 25 km above the surface. Ozone's concentration within the ozone layer is 0.2 to 0.4 ppm. Typical concentrations in unpolluted air closer to the surface is 0.03 ppm. The ozone in the ozone layer absorbs 97-99% of all the ultraviolet light that passes into the stratosphere. Chemistry 104 Prof. Shapley page 3

The Ozone Hole Until recently, the concentration of ozone in the stratosphere was nearly constant. However, manmake chemicals such as the FREON used in refrigerators and air conditioners destroy it. Over the course of the winter, reactive molecules build up in stratospheric clouds over the poles. The light and heat of the early spring causes these molecules to combine with ozone, resulting in a hole in the ozone layer. UV radiation can reach the Earth's surface under this hole in the protective ozone layer. International treaties are now limiting the amount of ozone-damaging chemicals that are released. Ozone and Smog Ozone and Health Ozone in the stratosphere protects us from dangerous UV radiation but ozone close to the Earth is toxic to both animals and plants. People exposed to ozone develop respiratory symptoms (coughing, throat irritation, wheezing) and loss of some lung function. People with asthma, older adults, and infants are particularly sensitive. Long-term exposure to ozone may cause people to develop asthma. Chemistry 104 Prof. Shapley page 4

Air Quality and Smog As you drive from Champaign-Urbana towards Chicago you see a brown layer on the horizon. It is worse in the summer than in the winter. Once you arrive in the city, you might notice some odor or irritation to your lungs and it's harder to exercise. Plants don't seem to grow as well as they do back in Champaign-Urbana. What is the cause of all this? It is photochemical smog. Geography also plays a role. In Chicago, the "windy city", the smog never gets as bad as it does in Los Angeles because the winds from across the plains dilute it. The Los Angeles basin holds the air above LA and prevents the smog from dissipating. Photochemical smog is a mixture of many organic and inorganic gas phase molecules. It contains ozone, nitrogen oxides, and organic molecules. Typically, we estimate the amount of smog by measuring the concentration of one component, ozone. Smog is: Toxic to plants and animals Decreases photosynthesis activity by ~50%s Responsible for 10-40% yearly loss in the growth of crops outside the cities Responsible for a 50% loss of trees in Los Angeles area What is needed to form smog? 1. volatile organic molecules from internal combustion engines or power plants 2. nitrogen oxides from internal combustion engines or power plants 3. sunlight 4. oxygen The Air Quality Index is an index that is used to report daily air quality and the concentration of the five most common ambient air pollutants: ground-level ozone, particulate matter, carbon monoxide, sulfur dioxide, and nitrogen dioxide. Chemistry 104 Prof. Shapley page 5

The ozone level changes day-to-day. You can check the level today on the ozone map. Note that the ozone level goes up through the day and is reduced at night. Metropolitan areas on the east and west coasts of the US typically have a higher ozone level than we do in central Illinois. A picture from a day in 2007 is shown below. Industrial Applications of Ozone Chemistry 104 Prof. Shapley page 6

Wastewater Disinfection Ozone kills many bacteria, protozoa, and viruses that cause disease in humans. It destroys the cell walls of the organisms, reacts with many molecules within the cell, and damages nucleic acids in the nucleus. For wastewater treatment, ozone is generated on site by passing an electric discharge through oxygen or air. Ozone is more effective than chlorine for wastewater treatment but it is expensive, the gas is toxic and corrosive, and it doesn't work well when the water has high levels of suspended solids. Bleaching The color in colored materials is often due to conjugated carbon-carbon double bonds in the molecules that make it up. A conjugated molecule has carbon-carbon double bonds alternating with carbon-carbon single bonds. Ozone adds to some of the carbon-carbon double bonds and eliminates the color. Using ozone as a bleach can be better for the environment than bleaches like Clorox (NaOCl) because it doesn't add harmful byproducts in water. Chemical Synthesis: Ozonolysis Ozone reacts with carbon-carbon double bonds. In combination with other reactants, it adds oxygen and breaks these bonds. Ozonolysis is an important step in the synthesis of many pharmaceutical agents. Ozone reacts with the double bond in this molecule. After several steps (not shown here) a new molecule with a C-OH unit is formed. Molecules that have carbon connected to OH groups are called alcohols. Chemistry 104 Prof. Shapley page 7

In this example, ozone again reacts with a carbon-carbon double bond. After additional steps, the product of the reaction is a new molecule with a CHO unit. Molecules like this are called aldehydes. Chemistry 104 Prof. Shapley page 8