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Objectives Time: Four hours ObjectivesA. Teacher:
B. At the conclusion of this unit the student should be able to --
Investigation and Building Background 1. Introduce term: Students have little knowledge of radiation (terminology) and no useful
meanings for the term. 2. Resources:
3. Experiment:
4. Generalizing: a. Materials needed for the Cloud Chamber:
b. Vocabulary: detecting and measuring radiation
c. Materials for measuring radiation with the Geiger counter
Questions
After Cloud Chamber Experiment Because you could not see the radiation, what kind of observation did you experience? What is happening to the radioactive source? What radiation "footprints" did you see? Describe them. After the Geiger Counter Measurements Why do we measure radiation exposure? When you use a Geiger counter to survey a radioactive substance, why is it important to know what the background radiation level is? Has anyone you know been helped or harmed by radiation? ReferenceThe Harnessed Atom, Teacher's Edition, U.S. Department of Energy. Lesson PlanNote: Give each student a 5x7 index card as he/she enters the classroom. Greeting... "Radiation" (written on the board) When you see or hear this word what do you think about? What do you think it means? I would like you to share your thoughts with me by writing on the card what you thought about when I wrote "radiation" on the board. Do not put your name on the card! [Collect the cards and mix them up. Read several out loud to the class and stimulate discussion on each. Do not attempt to connect any child with a particular note. Write key words from student opinion on the board for future reference.] Introduction Radiation is all around us. It comes from the Earth and from outer space. Many forms of radiation are invisible -- we can't feel it, see it, taste it, or smell it. Yet, it can be detected and measured when present. We measure ionizing radiation in units called millirems. But what is radiation? Radioactive materials are composed of atoms that are unstable. An unstable atom gives off its excess energy until it becomes stable. The energy emitted is radiation. We can classify radiation as being either natural and man-made. As I mentioned a moment ago, the Earth is surrounded by radiation. Every day, for example, we are exposed to radon, a radioactive gas from uranium found in soil dispersed in the air; from radioactive potassium in our food and water; from uranium, radium, and thorium in the Earth's crust; and from cosmic rays and the sun. These types of radiation are called natural or background radiation. In the U.S. we are exposed to an average of 300 millirems of natural radiation each year (a millirem is a unit of measure for exposure to radiation). This amounts to natural radiation accounting for nearly 85 percent of our total annual exposure. Where does the remaining 15 percent come from? Man-made sources. Man-made radiation sources that people can be exposed to include tobacco, television, medical x-rays, smoke detectors, lantern mantles, nuclear medicine, and building materials. Adding it all up, the average American is exposed to a total of about 360 millirems a year from natural and man-made radiation. The sources of radiation are shown in Classroom Activity 1. Generally, when we think of exposure to radiation, we need to look at radioactive atoms produced in nuclear reactors and described as being unstable. They are unstable because they undergo a disintegrating process called decaying. During this process, unstable atoms becomes stable, throwing off (emitting) radiation in the form of rays and/or particles. How fast a radioactive atom decays into a stable atom depends on the atom itself. For example, the range in the rate of decay among isotopes goes from fractions of seconds to several billion years (e.g., uranium). Let's take a look at uranium-238 to illustrate the decay chain. As U-238 decays it changes into thorium-230, which changes into radium-226, which changes into radon-218, which changes into bismuth-214, and finally into lead-206 (a stable element). One peculiar thing about radioactive atoms is that no one knows exactly when the element will decay and give off radiation. There is, however, a pattern relating to how long it takes for an isotope to lose half of its radioactivity. The pattern is called half-life. If an atom, for example, has a half-life of 10 years, half of its atoms will decay in 10 years. Then in another 10 years half of that amount will decay and so on. While there are several different forms of radiation, we're going to concentrate on just three that result from the decay of radioactive isotopes: alpha, beta, and gamma. Beta particles are high energy electrons. Both alpha and beta particles are emitted from unstable isotopes. The alpha particle, consisting of two protons and two neutrons, is relatively large compared to beta particles. Gamma rays have no mass. Because of its size and electrical charge (+2), the alpha particle has a relatively slow speed and low penetrating distance (one to two inches in air). Alpha particles are easily stopped by a thin sheet of paper or the body's outer layer of skin. Since they do not penetrate the outer (dead) layer of skin, they present little or no hazard when they are external to the body. However, alpha particles are considered internal hazards, because when they come into contact with live tissue they cause a large number of ionizations to occur in small areas, thus causing damage to tissues and cells. Beta radiation, while faster and lighter than alpha radiation, can travel through about 10 feet of air and penetrate very thin layers of materials such as aluminum foil. However, while clothing will stop most beta particles, they can penetrate the live layers of skin tissue. Therefore, beta radiation is considered to be both an internal and external (to skin only) hazard. Thin layers of metals and plastics can be used to shield individuals from beta radiation. Gamma radiation, high energy light, is a little different. It is a type of electromagnetic wave, just like radio waves, light waves, and x-rays. Gamma radiation is a very strong type of electromagnetic wave. It is has no weight and travels at the speed of light. This is much faster than alpha and beta radiation. Because of their penetrating capability, gamma rays are considered both internal and external hazards. Thick walls of cement, lead, or steel are needed to stop it. Alpha, beta, and gamma radiations are also known as ionizing radiation. Ionizing radiation is especially harmful because it can change the chemical makeup of many things, including the delicate chemistry of the human body and other living organisms. For this reason it is a good idea to avoid unnecessary exposure to all ionizing radiation. The problem is simply this: large amounts of radiation -- far above the levels encountered in daily life -- can produce cancer and genetic defects in living organisms. Radiation causes damage and alters the body's normal cells and normal cell function. This breakdown in normal cell function may result in an uncontrolled growth of cells, hence the potential for malignant/cancerous tumors. Whether the source of radiation is natural or man-made, whether it is a small dose of radiation or a large dose, there will be some biological effects. A diagram can show the biological effect of ionizing radiation. Radiation causes ionizations of atoms that will affect molecules that may affect cells that may effect tissues that may affect organs that may affect the whole body. [Write the following on the board] Although we tend to think of biological effects in terms of the effect of radiation on living cells, in actuality, ionizing radiation, by definition, interacts only with atoms by a process called ionization. Thus, all biological damage effects begin when radiation interacts with atoms forming the cells in the human body. As a result, radiation effects on humans proceed from the lowest to the highest level as noted on the board. [Radiation causes ionizations of atoms that will affect molecules that may affect cells that may effect tissues that may affect organs that may affect the whole body.] Experiment A: The Cloud Chamber While radiation cannot be seen, the cloud chamber allows you to see the tracks it leaves in a dense gas. [Complete Classroom Activity 1] Experiment B: Using the Geiger Counter How radioactive are different materials? [Complete Classroom Activities 2 and 3] Answers to Questions from "Radiation" Unit Outline:
After Cloud Chamber Experiment
After the Geiger Counter Measurements
Classroom ActivitiesClassroom Activity 1 How Can You See the Footprints of Radiation? While radiation cannot be seen, the cloud chamber allows you to see the tracks it leaves in a dense gas. Materials
First, paint the bottom of the container with black paint and let it dry. Then cut the blotter paper into a strip about as wide as the height of the container. Cut two windows in the strip, as shown, and place it against the inside of the container. Directions: Pour enough ethyl alcohol into the cloud chamber to cover the bottom
of the container. The blotter paper will absorb most of it. Place the cloud chamber on the dry ice to super-chill it. Wait about five minutes. Darken the room. Shine the flashlight through the windows of the chamber while looking through the lid. You should see "puffs" and "trails" coming from the source. These are the "footprints" of radiation as it travels through the alcohol vapor. The vapor condenses as the radiation passes through. This is much like the vapor trail left by high flying jets. Do you see radiation in the cloud chamber? ________ Other Ideas To Explore Try to identify these footprints:
Caution: Dry ice should be handled very carefully! It can burn unprotected skin. Classroom Activity 2 How radioactive are different materials? Materials
Directions:
The lowest?__________________________ Why?_________________________________________ Classroom Activity 3 Personal Radiation Dose We live in a radioactive world and always have. Radiation is all around us as a part of our natural environment. It is measured in millirems (mrems). The annual average dose per person from all sources is about 350 mrems, but it is not uncommon for any of us to receive more than that in a given year (largely due to medical procedures). International standards allow up to 2,000 mrems a year exposure for those who work with and around radioactive material. To find your average annual dose (mrems), use the interactive Personal Annual Radiation Dose Calculator or this printer friendly worksheet .
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