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25.2 Nuclear Transformations Nuclear Stability and >Decay What determines the type of decay a radioisotope undergoes? 1 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. Nuclear Stability and 25.2 Nuclear Transformations > Decay A nucleus may be unstable and undergo spontaneous decay for different reasons. The neutron-to-proton ratio in a radioisotope determines the type of decay that occurs. 2 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. 25.2 Nuclear Transformations > The nuclear force is an attractive force that acts between all nuclear particles that are extremely close together, such as protons and neutrons in a nucleus. • At these short distances, the nuclear force dominates over electromagnetic repulsions and holds the nucleus together. 3 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. 25.2 Nuclear Transformations > Band of Stability. Interpret Data The stability of a nucleus depends on the ratio of neutrons to protons. • This graph shows the number of neutrons vs. the number of protons for all known stable nuclei. 4 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. 25.2 Nuclear Transformations > Interpret Data • For elements of low atomic number (below about 20), this ratio is about 1. • Above atomic number 20, stable nuclei have more neutrons than protons. 5 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. Nuclear Stability and 25.2 Nuclear Transformations > Decay Some nuclei are unstable because they have too many neutrons relative to the number of protons. • When one of these nuclei decays, a neutron emits a beta particle (fast-moving electron) from the nucleus. – A neutron that emits an electron becomes a proton. 1 0 n 1 1 p + 0 –1 e – This process is known as beta emission. 6 – It increases the number of protons while decreasing the number of neutrons. Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. Nuclear Stability and 25.2 Nuclear Transformations > Decay Radioisotopes that undergo beta emission include the following. 66 29 7 Cu 66 30 14 6 14 7 C Zn + N + 0 –1 0 –1 e e Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. Nuclear Stability and 25.2 Nuclear Transformations > Decay Other nuclei are unstable because they have too few neutrons relative to the number of protons. • These nuclei increase their stability by converting a proton to a neutron. – An electron is captured by the nucleus during this process, which is called electron capture. 59 28 37 18 8 Ni + 0 –1 Ar + 0 –1 e 59 27 Co e 37 17 Cl Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. Nuclear Stability and 25.2 Nuclear Transformations > Decay A positron is a particle with the mass of an electron but a positive charge. • Its symbol is 0 +1 e. • During positron emission, a proton changes to a neutron, just as in electron capture. 8 5 15 8 B 8 4 O 15 7 Be + N + 0 +1 0 +1 e e – the atomic number decreases by 1 and the number of neutrons increases by 1. 9 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. Nuclear Stability and 25.2 Nuclear Transformations > Decay Nuclei that have an atomic number greater than 83 are radioactive. • These nuclei have both too many neutrons and too many protons to be stable. – Therefore, they undergo radioactive decay. • Most of them emit alpha particles. – Alpha emission increases the neutron-to-proton ratio, which tends to increase the stability of the nucleus. 10 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. Nuclear Stability and 25.2 Nuclear Transformations > Decay In alpha emission, the mass number decreases by four and the atomic number decreases by two. 226 88 232 90 11 Ra 222 86 Th 228 88 Rn + 4 2 He Ra + 4 2 He Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. Nuclear Stability and 25.2 Nuclear Transformations > Decay Recall that conservation of mass is an important property of chemical reactions. • In contrast, mass is not conserved during nuclear reactions. • An extremely small quantity of mass is converted into energy released during radioactive decay. 12 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. 25.2 Nuclear Transformations > During nuclear decay, if the atomic number decreases by one but the mass number is unchanged, the radiation emitted is A. a positron. B. an alpha particle. C. a beta particle. D. a proton. 13 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. 25.2 Nuclear Transformations > During nuclear decay, if the atomic number decreases by one but the mass number is unchanged, the radiation emitted is A. a positron. B. an alpha particle. C. a beta particle. D. a proton. 14 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. 25.2 Nuclear Transformations > Half-Life How much of a radioactive sample remains after each halflife? 15 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. Half-Life Section 15.4 & Screen 15.8 • HALF-LIFE is the time it takes for 1/2 a sample is disappear. • The rate of a nuclear transformation depends only on the “reactant” concentration. • Concept of HALF-LIFE is especially useful for 1st order reactions. 16 Half-Life Decay of 20.0 mg of 15O. What remains after 3 half-lives? After 5 half-lives? 17 25.2 Nuclear Transformations > Interpret Graphs A half-life (t12) is the time required for onehalf of the nuclei in a radioisotope sample to decay to products. After each halflife, half of the original radioactive atoms have decayed into atoms of a new element. 18 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. 25.2 Nuclear Transformations > Comparing Half-Lives Half-lives can be as short as a second or as long as billions of years. Half-Lives of Some Naturally Occurring Radioisotopes Isotope 19 Half-life Radiation emitted Carbon-14 5.73 × 103 years b Potassium-40 1.25 × 109 years b, g Radon-222 3.8 days a Radium-226 1.6 × 103 years a, g Thorium-234 24.1 days b, g Uranium-235 7.0 × 108 years a, g Uranium-238 4.5 × 109 years a Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. 25.2 Nuclear Transformations > Half-Life Comparing Half-Lives • Scientists use half-lives of some longterm radioisotopes to determine the age of ancient objects. • Many artificially produced radioisotopes have short half-lives, which makes them useful in nuclear medicine. – Short-lived isotopes are not a longterm radiation hazard for patients. 20 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. 25.2 Nuclear Transformations > Half-Life Comparing Half-Lives Uranium-238 decays through a complex series of unstable isotopes to the stable isotope lead-206. • The age of uraniumcontaining minerals can be estimated by measuring the ratio of uranium-238 to lead-206. • Because the half-life of uranium-238 is 4.5 × 109 years, it is possible to use its half-life to date rocks as old as the solar system. 21 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. 25.2 Nuclear Transformations > Half-Life Radiocarbon Dating Plants use carbon dioxide to produce carbon compounds, such as glucose. • The ratio of carbon-14 to other carbon isotopes is constant during an organism’s life. • When an organism dies, it stops exchanging carbon with the environment and its radioactive 14 6 C atoms decay without being replaced. • Archaeologists can use this data to estimate when an organism died. 22 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. 25.2 Nuclear Transformations > Half-Life Exponential Decay Function You can use the following equation to calculate how much of an isotope will remain after a given number of half-lives. A = A0 1 2 n • A stands for the amount remaining. • A0 stands for the initial amount. • n stands for the number of half-lives. 23 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. 25.2 Nuclear Transformations > Half-Life Exponential Decay Function A = A0 1 2 n • The exponent n indicates how many times A0 must be multiplied by 12 to determine A. 24 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. 25.2 Nuclear Transformations > Sample Problem 25.1 Using Half-Lives in Calculations Carbon-14 emits beta radiation and decays with a half-life (t 12 ) of 5730 years. Assume that you start with a mass of 2.00 × 10–12 g of carbon-14. a. How long is three half-lives? b. How many grams of the isotope remain at the end of three half-lives? 25 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. 25.2 Nuclear Transformations > Sample Problem 25.1 1 Analyze List the knowns and the unknowns. • To calculate the length of three half-lives, multiply the half-life by three. • To find the mass of the radioisotope 1 remaining, multiply the original mass by 2 for each half-life that has elapsed. KNOWNS UNKNOWNS t12 = 5730 years 3 half-lives = ? years initial mass (A0) = 2.00 × 10–12 g mass remaining = ? g number of half-lives (n) = 3 26 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. 25.2 Nuclear Transformations > Sample Problem 25.1 2 Calculate Solve for the unknowns. a. Multiply the half-life of carbon-14 by the total number of half-lives. t 12 × n = 5730 years × 3 = 17,190 years 27 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. 25.2 Nuclear Transformations > Sample Problem 25.1 2 Calculate Solve for the unknowns. b. The initial mass of carbon-14 is reduced by one-half for each half-life. So, multiply by 12 three times. Remaining mass = 2.00 × 10–12 g × 12 ×12 × 12 = 0.250 × 10–12 g = 2.50 × 10–13 g 28 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. 25.2 Nuclear Transformations > Sample Problem 25.1 2 Calculate Solve for the unknowns. b. You can get the same answer by using the equation for an exponential decay function. 3 1 n 1 –12 g) = (2.00 × 10 2 2 () A = A0 = (2.00 × 10–12 () g)( ) 1 8 = 0.250 × 10–12 g = 2.50 × 10–13 g 29 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. 25.2 Nuclear Transformations > The half-life of phosphorus-32 is 14.3 days. How many milligrams of phosphorus-32 remain after 100.1 days if you begin with 2.5 mg of the radioisotope? 30 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. 25.2 Nuclear Transformations > The half-life of phosphorus-32 is 14.3 days. How many milligrams of phosphorus-32 remain after 100.1 days if you begin with 2.5 mg of the radioisotope? 1 half-life n = 100.1 days × = 7 half-lives 14.3 days 1 n 1 7 2 = (2.5 mg) 2 1 = (2.5 mg) 128 () A = A0 31 () ( ) = 2.0 × 10 –2 mg Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. 25.2 Nuclear Transformations > Which of the following always changes when transmutation occurs? A. The number of electrons B. The mass number C. The atomic atomicnumber number D. The number of neutrons 32 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. 25.2 Nuclear Transformations > Key Equation A = A0 33 1 2 n Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. Kinetics of Radioactive Decay Activity (A) = Disintegrations/time Activity (A) = (k)(N) where N is the number of atoms Decay is first order, and so ln (A/Ao) = -kt The half-life of radioactive decay is t1/2 = 0.693/k 34 35 36