Nuclear Reactions Activity Nuclear reactions are those that involve changes inside the nucleus of an atom. (This is opposed to chemical reactions, which involve changing the electrons around the nucleus.) There are basically two types of nuclear reactions: fusion and fission. Nuclear fusion is the joining together of two or more nuclei to form a single, larger nucleus. Nuclear fission is the splitting of a nucleus into a smaller nucleus and one or more nuclear particles. Nuclear reactions are often regarded as elusive and exotic, but they occur as frequently as chemical reactions. The evidence of nuclear decay is usually subtle and invisible, and these changes went unnoticed by scientists until the turn of the 20th century. However, when evidence of nuclear reactions is readily apparent, it can be spectacular. Both nuclear fusion and nuclear fission reactions are accompanied by some type of radioactive decay. Radioactive decay occurs when an unstable nucleus spontaneously emits high-energy nuclear particles, becoming more stable. There are three basic types of radioactive decay: alpha decay, beta decay, and gamma radiation. Alpha decay occurs when a nucleus emits a particle of two protons and two neutrons, called an alpha-particle. (notated: α or 24He2+) Beta decay occurs when a nucleus emits an electron or a positron, called a beta-particle. (notated: β- = electron, β+ = positron) Note: Beta decay is always accompanied by the release of a neutrino (notated: ν). A neutrino is like an electron without a charge. Gamma radiation occurs when a nucleus emits high energy electromagnetic radiation. (notated: γ) Use the atom boards to model the types of nuclear reactions discussed below. Part I: Nuclear Fusion Nuclear fusion is perhaps best known by its ominous manifestation, the hydrogen bomb. But you are witness to nuclear fusion almost every day of your life. The sun is powered by an ongoing (for billions of years) nuclear fusion reaction. The sun primarily burns hydrogen, fusing it into helium, but heavier elements are also fused in the sun and in other stars. For that matter, astronomers believe that all elements in the universe were created in stars by the process of nuclear fusion! The sun uses hydrogen atoms to fuse them into helium atoms in a three-step process called a proton-proton fusion chain. Use the atom board to model this process: Record the nuclear equation for each step on numbers 1-3 of your answer sheet. 1. 2. 3. Two protons fuse together forming a hydrogen-2 nucleus, and release a positron and a neutrino. One proton fuses with the hydrogen-2 nucleus, forming a helium-3 nucleus, and release a gamma ray Two helium-3 nuclei fuse to form a helium-4 nucleus, while releasing two protons Notice that no electrons are mentioned in the above description of fusion. This is because a nuclear fusion reaction is very exothermic, and takes place at such high temperatures that matter is in the plasma state. Electrons are dissociated from nuclei in the plasma state. Part II: Nuclear Fission and Half-Life Like nuclear fusion, nuclear fission is accompanied by the release of thermal energy. Unlike nuclear fusion, which is a rare event on Earth, nuclear fission is commonplace. The scorching hot temperatures of the deep Earth are due in part to countless fission reactions. All around the globe (even in the permafrost of the arctic circle) if you dig deep enough, you’ll find that the Earth’s crust can reach temperatures of 400°C! In nature, nuclear fission is a spontaneous process that occurs when unstable isotopes decay into more stable forms. Different isotopes decay at widely different rates. The more unstable the isotope, the more quickly it decays. The more stable the isotope, the more slowly it decays. The measure of how quickly an isotope decays is called its half-life. Half-life is defined as the time it takes for half of a sample of a substance to decay into a more stable form. 2 For example, cobalt-60 decays into nickel-60 and has a halflife of 5 years. If you had a 6-gram sample of cobalt-60, in 5 years you would have 3 grams of cobalt-60 and 3 grams of nickel-60. In ten years you have 1.5 grams of cobalt-60 and 4.5 grams of nickel-60. In fifteen years you would have 0.75 grams of cobalt-60 and 5.25 grams of nickel-60. And so on… Radioactive Decay of Cobalt-60 6 Mass (grams) 5 4 3 cobalt-60 nickel-60 2 1 0 0 5 10 15 20 25 30 35 40 45 50 55 60 65 70 75 80 85 90 95 100 Time (years) Hale life can be calculated by the following formula: Ct = Co•(1/2)t/t1/2 Where Ct = amount of radioactive substance that still remains Co = the original amount of radioactive substance t = is time elapsed t1/2 = half-life of the decaying substance 3 Record your responses to the following problems on numbers 4-8 on your answer sheet. 4. Beryllium-10 decays into boron-10 with a half-life of 2,700,000 years. a. Create a beryllium-10 atom on your atom board. Record the isotopic notation of beryllium-10. b. Now create a boron-10 atom on your atom board. Record the isotopic notation of boron-10. c. What type of radioactive decay occurred to produce boron10 from beryllium-10? d. Record the nuclear equation for this transformation. 5. Calcium-41 decays into potassium-41 with a half-life of 100,000 years. a. Create a calcium-41 atom on your atom board. Record the isotopic notation of calcium-41. b. Now create a potassium-41 atom on your atom board.Record the isotopic notation of potassium-41. c. What type of radioactive decay occurred to produce potassium-41 from calcium-41? d. Record the nuclear equation for this transformation. 6. Iron-59 decays into cobalt-59 with a half-life of 45 days. a. Create an iron-59 atom on your atom board. Record the isotopic notation of iron-59. b. Now create a cobalt-59 atom on your atom board. Record the isotopic notation of cobalt-59. c. What type of radioactive decay occurred to produce cobalt-59 from iron-59? d. Record the nuclear equation for this transformation. 7. Uranium-238 decays into thorium-234 with a half-life of 4.51 x 109 years. a. Since the atom board is not big enough to model this atom, simply record the isotopic notation of uranium-238. b. Record the isotopic notation of thorium-234. c. What type of radioactive decay occurred to produce thorium-234 from uranium-238? d. Record the nuclear equation for this transformation. 4