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Ozone Layer

Author: Sophia

what's covered
In this lesson, you will learn about the ozone layer. Specifically, this lesson covers:

Table of Contents

1. What is Ozone?

Ozone is a colorless and tasteless gas. However, unlike oxygen, which is odorless, colorless, and tasteless, ozone has an odor to it. Sometimes the odor is described as a pungent chlorine-like smell. It also can be described as the smell that accompanies an electrical discharge. Unlike oxygen, ozone is not involved in combustion. Ozone is also a bactericide (kills bacteria), decolorizer (removes color from water), and deodorizer (removes odor from water). These properties make ozone very useful in water treatment. Ozone is used in swimming pools, hot tubs, and even bottled water.

Ozone has the molecular formula Oblank subscript 3. Ozone is formed from oxygen. The formation of ozone requires energy. This energy can be in the form of lightning or sunlight. Ozone is a very toxic chemical and is considered a pollutant near the surface of the Earth. However, stratospheric ozone is necessary to protect us from dangerous ultraviolet radiation.

EXAMPLE

The uses of ozone depend on its reactivity with other substances. It can be used as a bleaching agent for oils, waxes, fabrics, and starch, by oxidizing the colored compounds in these substances to colorless compounds. Thus, it is an alternative to chlorine as a disinfectant for water.

A space-filling model shows three atoms labeled, “O,” bonded to one another in a triangular shape. Two Lewis structures connected by a double-ended arrow are shown as well. In the left image, an oxygen atom with one lone pair of electrons is double bonded to another oxygen with two lone pairs of electrons to the left and single bonded to an oxygen with three lone pairs of electrons to the right. The right image is a mirror image of the left.

term to know
Ozone
A colorless, tasteless, and toxic gas formed from oxygen that is considered a pollutant near the surface of the Earth; however, stratospheric ozone is necessary to protect us from dangerous ultraviolet radiation.

2. What is in Sunlight?

The figure includes a portion of the electromagnetic spectrum which extends from gamma radiation at the far left through x-ray, ultraviolet, visible, infrared, terahertz, and microwave to broadcast and wireless radio at the far right. At the top of the figure, inside a grey box, are three arrows. The first points left and is labeled, “Increasing energy E.” A second arrow is placed just below the first which also points left and is labeled, “Increasing frequency nu.” A third arrow is placed just below which points right and is labeled, “Increasing wavelength lambda.” Inside the grey box near the bottom is a blue sinusoidal wave pattern that moves horizontally through the box. At the far left end, the waves are short and tightly packed. They gradually lengthen moving left to right across the figure, resulting in significantly longer waves at the right end of the diagram. Beneath the grey box are a variety of photos aligned above the names of the radiation types and a numerical scale that is labeled, “Wavelength lambda ( m ).” This scale runs from 10 superscript negative 12 meters under gamma radiation increasing by powers of ten to a value of 10 superscript 3 meters at the far right under broadcast and wireless radio. X-ray appears around 10 superscript negative 10 meters, ultraviolet appears in the 10 superscript negative 8 to 10 superscript negative 7 range, visible light appears between 10 superscript negative 7 and 10 superscript negative 6, infrared appears in the 10 superscript negative 6 to 10 superscript negative 5 range, teraherz appears in the 10 superscript negative 4 to 10 superscript negative 3 range, microwave infrared appears in the 10 superscript negative 2 to 10 superscript negative 1 range, and broadcast and wireless radio extend from 10 to 10 superscript 3 meters. Labels above the scale are placed to indicate 1 n m at 10 superscript negative 9 meters, 1 micron at 10 superscript negative 6 meters, 1 millimeter at 10 superscript negative 3 meters, 1 centimeter at 10 superscript negative 2 meters, and 1 foot between 10 superscript negative 1 meter and 10 superscript 0 meters. A variety of images are placed beneath the grey box and above the scale in the figure to provide examples of related applications that use the electromagnetic radiation in the range of the scale beneath each image. The photos on the left above gamma radiation show cosmic rays and a multicolor PET scan image of a brain. A black and white x-ray image of a hand appears above x-rays. An image of a patient undergoing dental work, with a blue light being directed into the patient's mouth is labeled, “dental curing,” and is shown above ultraviolet radiation. Between the ultraviolet and infrared labels is a narrow band of violet, indigo, blue, green, yellow, orange, and red colors in narrow, vertical strips. From this narrow band, two dashed lines extend a short distance above to the left and right of an image of the visible spectrum. The image, which is labeled, “visible light,” is just a broader version of the narrow bands of color in the label area. Above infrared are images of a television remote and a black and green night vision image. At the left end of the microwave region, a satellite radar image is shown. Just right of this and still above the microwave region are images of a cell phone, a wireless router that is labeled, “wireless data,” and a microwave oven. Above broadcast and wireless radio are two images. The left most image is a black and white medical ultrasound image. A wireless AM radio is positioned at the far right in the image, also above broadcast and wireless radio.

Most people only think about visible light when they think of sunlight. But sunlight consists of all forms of light or electromagnetic radiation (see the image above). The majority of sunlight is visible light, ultraviolet (UV) light, and infrared (IR) light, but there are also cosmic rays, x-rays, microwaves, and other various forms of electromagnetic radiation. However, we will focus on the main three forms of sunlight (UV, IR, and visible light).

Visible light is the form of sunlight that humans can see. It includes red, orange, yellow, green, blue, and violet light. While humans can only see this small sliver of light, other animals can see more of the electromagnetic spectrum. Pit vipers can “see” or detect infrared radiation using the pits on their faces. Reindeer, butterflies, bumblebees, and hawks can see or detect ultraviolet radiation.

did you know
Humans actually do have the ability to see ultraviolet radiation. But it only occurs in people with aphakia, who do not have the lens in their eye. This lens, like a pair of sunglasses, filters out ultraviolet radiation from entering the eye. Without the lens, the ultraviolet radiation can enter the eye for us to detect it. But before you go thinking about removing your lens, the lens protects the eye from that dangerous ultraviolet radiation and is also used to focus visible light on the retina so we can see. The most famous person with aphakia is the artist, Monet, who had cataracts so bad that he had his lens removed from his eye late in his life.

When we see visible light we are actually seeing the reflection of light off a surface. For example, if you see someone wearing a blue shirt (or perceive it as blue), the shirt is absorbing all colors of light except blue, which is being reflected off of the shirt so you can perceive the shirt as blue. An orange shirt absorbs all colors except orange. A white shirt absorbs no colors and reflects all, a mixture of all forms of visible light is perceived as white light. When you see black, all colors are being absorbed and nothing is being reflected.

IN CONTEXT

Infrared light is the form of sunlight that provides warmth to the Earth. If you go outside and feel the heat of the sun, you are feeling the effects of infrared light. Infrared light falls just below red on the electromagnetic spectrum (in terms of energy or frequency). So, infrared light is actually weaker than red light. Infrared light is used to warm the atmosphere. You will learn much more about infrared light in the next lesson on climate change.

The final main form of sunlight is ultraviolet radiation. Ultraviolet is just above violet on the electromagnetic spectrum (in terms of energy or frequency). So, UV is actually stronger than violet light. UV light is strong enough to break covalent bonds, which can result in chemical changes in atoms and molecules.


3. UV Light

UV light is a dangerous form of electromagnetic radiation that has a higher frequency than visible light. UV light and all other forms of light with higher frequencies than UV light (x-rays, gamma rays, and cosmic rays) are dangerous and damaging forms of electromagnetic radiation. Our atmosphere filters out almost all of the very deadly forms of radiation, but UV light is one dangerous form of electromagnetic radiation that can get to the surface of the Earth, where it can cause a lot of damage.

UV light is the form of light with wavelengths from 100 to 400 nm. As a note, the visible spectrum of light starts at 400 nm (violet light) and ends at 700 nm (red light). We classify UV light into three bands, UV-A, UV-B, and UV-C.

  • UV-C consists of UV light with a wavelength of 100 to 280 nm.
  • UV-B band consists of UV light with a wavelength of 280 to 315 nm.
  • UV-A band consists of UV light with a wavelength of 315 to 400 nm.
Recall that UV light is strong enough to break covalent bonds and that our atmosphere is made of almost 21% oxygen gas. The covalent bond in oxygen gas absorbs UV light up to about 240 nm before it will break. What does this mean? It means that all UV light from 100 to 240 nm is absorbed by oxygen gas in our atmosphere, causing the oxygen covalent bond to shatter. In the process, oxygen gas is converted to ozone, while it absorbs all the dangerous forms of UV light from 100 to 240 nm.

3 straight O subscript 2 left parenthesis g right parenthesis space rightwards arrow from blank to h nu of space 2 straight O subscript 3 left parenthesis g right parenthesis

The covalent bond in ozone will absorb UV light from around 200 nm to 340 nm before the covalent bond in ozone will break. When the bond breaks in ozone, it converts the ozone back to oxygen.

straight O subscript 3 left parenthesis g right parenthesis space rightwards arrow with ultraviolet space light on top space straight O left parenthesis g right parenthesis space plus space straight O subscript 2 left parenthesis g right parenthesis

Overall, oxygen absorbs dangerous UV-C radiation from 100 to 240 nm and forms ozone in the process. Ozone absorbs dangerous UV-C and UV-B radiation from 200 to 340 nm reforming oxygen in the process. It has been determined that up to 300 million tons of ozone is created and destroyed in this process each day. As oxygen converts to ozone and back to oxygen, almost all the dangerous UV light (UV-C and UV-B) is absorbed and destroyed in the process. This process protects us from the dangerous forms of UV radiation.

The picture below summarizes the ozone cycle. In a slow process, UV light from the sun breaks apart (photolyzed) an oxygen atom, which then is rapidly converted to ozone, which rapidly decomposes via UV light to form oxygen. This interconversion between ozone and oxygen is a rapidly occurring reaction that transforms UV light from the sun into thermal energy, which heats up the stratosphere. Finally, in a slow process, the ozone reacts with chlorine or some other atom.

term to know
UV Light
A dangerous form of electromagnetic radiation that has a higher frequency than visible light.

4. Depletion of the Ozone Layer

people to know
The 1995 Nobel Prize in Chemistry was shared by Paul J. Crutzen, Mario J. Molina, and F. Sherwood Rowland for their work in atmospheric chemistry, particularly concerning the formation and decomposition of ozone. Molina, a Mexican citizen, carried out the majority of his work at the Massachusetts Institute of Technology (MIT).

A photograph is shown of Mario Molina. To the right of the photo, an image of Earth’s southern hemisphere is shown with a central circular region in purple with a radius of about half that of the entire hemisphere. Just outside this region is a narrow royal blue band, followed by an outer thin turquoise blue band. The majority of the outermost region is green. Two small bands of yellow are present in the lower regions of the image.

In 1974, Molina and Rowland published a paper in the journal Nature detailing the threat of chlorofluorocarbon gases to the stability of the ozone layer in the Earth’s upper atmosphere. The ozone layer protects the Earth from solar radiation by absorbing ultraviolet light. As chemical reactions deplete the amount of ozone in the upper atmosphere, a measurable “hole” forms above Antarctica, and an increase in the amount of solar ultraviolet radiation—strongly linked to the prevalence of skin cancers—reaches the Earth’s surface. The work of Molina and Rowland was instrumental in the adoption of the Montreal Protocol, an international treaty signed in 1987 that successfully began phasing out the production of chemicals linked to ozone destruction.

​​IN CONTEXT

Molina and Rowland demonstrated that chlorine atoms from human-made chemicals can catalyze ozone destruction in a process similar to that by which NO accelerates the depletion of ozone.

NO left parenthesis g right parenthesis space plus space straight O subscript 3 left parenthesis g right parenthesis space rightwards arrow space NO subscript 2 left parenthesis g right parenthesis space plus space straight O subscript 2 left parenthesis g right parenthesis

Chlorine atoms are generated when chlorocarbons or chlorofluorocarbons—once widely used as refrigerants and propellants—are photochemically decomposed by ultraviolet light or react with hydroxyl radicals. A sample mechanism is shown here using methyl chloride.

CH subscript 3 Cl space plus space OH space rightwards arrow space Cl space plus space other space products

Chlorine radicals break down ozone and are regenerated by the following catalytic cycle:

table attributes columnalign left end attributes row cell Cl space plus thin space straight O subscript 3 space rightwards arrow space ClO space plus space straight O subscript 2 end cell row cell ClO space plus space straight O space rightwards arrow space Cl space plus space straight O subscript 2 end cell row cell overall space reaction colon space straight O subscript 3 space plus space straight O space rightwards arrow space 2 straight O subscript 2 end cell end table

A single monatomic chlorine can break down thousands of ozone molecules. Luckily, the majority of atmospheric chlorine exists as the catalytically inactive forms Clblank subscript 2 and ClONOblank subscript 2.

After receiving his portion of the Nobel Prize, Molina continued his work in atmospheric chemistry at MIT, until his death in 2020.

did you know
Ozone forms naturally in the upper atmosphere by the action of ultraviolet light from the sun on the oxygen there. Most atmospheric ozone occurs in the stratosphere, a layer of the atmosphere extending from about 10 to 50 kilometers above the Earth’s surface. This ozone acts as a barrier to harmful ultraviolet light from the sun by absorbing it via a chemical decomposition reaction.

straight O subscript 3 left parenthesis g right parenthesis space rightwards arrow with ultraviolet space light on top space straight O left parenthesis g right parenthesis space plus space straight O subscript 2 left parenthesis g right parenthesis

The reactive oxygen atoms recombine with molecular oxygen to complete the ozone cycle. The presence of stratospheric ozone decreases the frequency of skin cancer and other damaging effects of ultraviolet radiation. It has been clearly demonstrated that chlorofluorocarbons, CFCs (known commercially as Freons), which were present as aerosol propellants in spray cans and as refrigerants, caused depletion of ozone in the stratosphere. This occurred because ultraviolet light also causes CFCs to decompose, producing atomic chlorine. The chlorine atoms react with ozone molecules, resulting in a net removal of Oblank subscript 3 molecules from the stratosphere.

There is a worldwide effort to reduce the amount of CFCs used commercially, and the ozone hole is already beginning to decrease in size as atmospheric concentrations of atomic chlorine decrease.

summary
In this lesson, you learned about ozone, including its structure and its uses. You also learned what is in sunlight, including what each form of sunlight does. You next learned specifically about UV light. You learned how it is formed and what function it serves in our stratosphere. Finally, you learned about the depletion of the ozone layer that is caused by chemicals such as Freon (CFCs).

Best of luck in your learning!

Source: THIS TUTORIAL HAS BEEN ADAPTED FROM OPENSTAX “CHEMISTRY: ATOMS FIRST 2E”. ACCESS FOR FREE AT Chemistry: Atoms First 2e. LICENSE: CREATIVE COMMONS ATTRIBUTION 4.0 INTERNATIONAL

Terms to Know
Ozone

A colorless, tasteless, and toxic gas formed from oxygen that is considered a pollutant near the surface of the Earth; however, stratospheric ozone is necessary to protect us from dangerous ultraviolet radiation.

UV Light

A dangerous form of electromagnetic radiation that has a higher frequency than visible light.