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Introductory Chemistry , 3 rd Edition

Introductory Chemistry , 3 rd Edition. Radioactivity and Nuclear Chemistry. 2009, Prentice Hall. Properties of Radioactivity. Radioactive rays can ionize matter. Cause uncharged matter to become charged. Basis of Geiger counter and electroscope. Radioactive rays have high energy.

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Introductory Chemistry , 3 rd Edition

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  1. Introductory Chemistry, 3rd Edition Radioactivity and Nuclear Chemistry 2009, Prentice Hall

  2. Properties of Radioactivity • Radioactive rays can ionize matter. • Cause uncharged matter to become charged. • Basis of Geiger counter and electroscope. • Radioactive rays have high energy. • Radioactive rays can penetrate matter. • Radioactive rays cause phosphorescent chemicals to glow. • Basis of scintillation counter.

  3. What Is Radioactivity? • Release of tiny, high-energy particles from an atom. • Particles are ejected from the nucleus.

  4. Types of Radioactive Rays • Rutherford discovered there were three types of radioactivity: 1. Alpha rays (a): • Have a charge of +2 c.u. and a mass of 4 amu. • What we now know to be helium nucleus. 2. Beta rays (b): • Have a charge of -1 c.u. and negligible mass. • Electron-like. 3. Gamma rays (g): • Form of light energy (not particle like a and b).

  5. a g b Penetrating Ability of Radioactive Rays 0.01 mm 1 mm 100 mm Pieces of lead

  6. Order of Strength of Ionizing and Penetrating Ability • Ionizing ability = a > b > g. • Penetrating ability = a < b < g.

  7. Facts About the Nucleus • Very small volume compared to volume of the atom. • Essentially entire mass of atom. • Very dense. • Composed of protons and neutrons that are tightly held together. • Nucleons.

  8. Facts About the Nucleus • Every atom of an element has the same number of protons; equal to the atomic number (Z). • Atoms of the same elements can have different numbers of neutrons. • Isotopes. • Different atomic masses. • Isotopes are identified by their mass number (A). • Mass number = number of protons + neutrons.

  9. Important Atomic Symbols

  10. Radioactivity • Radioactive nuclei spontaneously decompose into smaller nuclei. • Radioactive decay. • We say that radioactive nuclei are unstable. • The parent nuclide is the nucleus that is undergoing radioactive decay; the daughter nuclide are the new nuclei that are made. • Decomposing involves the nuclide emitting a particle and/or energy. • All nuclides with 84 or more protons are radioactive.

  11. Transmutation • Rutherford discovered that during the radioactive process, atoms of one element are changed into atoms of a different element—transmutation. • In order for one element to change into another, the number of protons in the nucleus must change.

  12. Chemical Processes vs. Nuclear Processes • Chemical reactions involve changes in the electronic structure of the atom. • Atoms gain, lose, or share electrons. • No change in the nuclei occurs. • Nuclear reactions involve changes in the structure of the nucleus. • When the number of protons in the nucleus changes, the atom becomes a different element.

  13. Nuclear Equations • We describe nuclear processes using nuclear equations. • Use the symbol of the nuclide to represent the nucleus. • Atomic numbers and mass numbers are conserved.

  14. Alpha Emission • An  particle contains 2 protons and 2 neutrons. • Helium nucleus. • Loss of an alpha particle means: • Atomic number decreases by 2. • Mass number decreases by 4.

  15. a Decay

  16. Beta Emission • A  particle is like an electron. • Moving much faster. • Produced from the nucleus. • When an atom loses a  particle, its: • Atomic number increases by 1. • Mass number remains the same. • In beta decay, a neutron changes into a proton.

  17. b Decay

  18. Gamma Emission • Gamma (g) rays are high-energy photons of light. • No loss of particles from the nucleus. • No change in the composition of the nucleus, however, the arrangement of the nucleons changes. • Same atomic number and mass number. • Generally occurs after the nucleus undergoes some other type of decay and the remaining particles rearrange.

  19. Positron Emission • Positron has a charge of 1+ c.u. and negligible mass. • Anti-electron. • When an atom loses a positron from the nucleus, its: • Mass number remains the same. • Atomic number decreases by 1. • Positrons appear to result from a proton changing into a neutron.

  20. b+ Decay

  21. Beta emission: Neutron changing into a proton. • Positron emission: Proton changing into a neutron. Particle Changes

  22. Nuclear Equations • In the nuclear equation, mass numbers and atomic numbers are conserved. • We can use this fact to determine the identity of a daughter nuclide if we know the parent and mode of decay.

  23. Example—Write the Nuclear Equation for Positron Emission from C-11. 1. Write the nuclide symbols for both the starting radionuclide and the particle.

  24. Example—Write the Nuclear Equation for Positron Emission from C-11, Continued. 2. Set up the equation. • Emitted particles are products. • Captured particles are reactants.

  25. Example—Write the Nuclear Equation for Positron Emission from C-11, Continued. 3. Determine the mass number and atomic number of the missing nuclide. • Mass and atomic numbers are conserved.

  26. Example—Write the Nuclear Equation for Positron Emission from C-11, Continued. 4. Determine the element from the atomic number.

  27. Practice—Write a Nuclear Equation for Each of the Following: • Alpha emission from Th-238. • Beta emission from Ne-24. • Positron emission from N-13.

  28. Practice—Write a Nuclear Equation for Each of the Following, Continued: • Alpha emission from Th-238. • Beta emission from Ne-24. • Positron emission from N-13.

  29. Detecting Radioactivity • To detect when a phenomenon is present, you need to identify what it does: • Radioactive rays can expose light-protected photographic film. • Use photographic film to detect the presence of radioactive rays—film badges.

  30. Detecting Radioactivity, Continued 2. Radioactive rays cause air to become ionized. • An electroscope detects radiation by its ability to penetrate the flask and ionize the air inside. • Geiger-Müller counter works by counting electrons generated when Ar gas atoms are ionized by radioactive rays.

  31. Detecting Radioactivity 3. Radioactive rays cause certain chemicals to give off a flash of light when they strike the chemical. • A scintillation counter is able to count the number of flashes per minute.

  32. Natural Radioactivity • There are small amounts of radioactive minerals in the air, ground, and water. • It’s even in the food you eat! • The radiation you are exposed to from natural sources is called background radiation.

  33. Half-Life • Each radioactive isotope decays at a unique rate. • Some fast, some slow. • Not all the atoms of an isotope change simultaneously. • Rate is a measure of how many of them change in a given period of time. • Measured in counts per minute, or grams per time. • The length of time it takes for half of the parent nuclides in a sample to undergo radioactive decay is called the half-life.

  34. Half-Lives of Various Nuclides

  35. Half-Life • Half of the radioactive atoms decay each half-life.

  36. How Long Is the Half-Life of this Radionuclide?

  37. Decay Series • In nature, often one radioactive nuclide changes in another radioactive nuclide. • Daughter nuclide is also radioactive. • All of the radioactive nuclides that are produced one after the other until a stable nuclide is made is called a decay series. • To determine the stable nuclide at the end of the series without writing it all out: • Count the number of a and b decays. • From the mass nunmber, subtract 4 for each a decay. • From the atomic number, subtract 2 for each a decay and add 1 for each b.

  38. U-238 Decay Series

  39. Practice—Write All the Steps in the U-238 Decay Series and Identify the Stable Isotope at the End of the Series. • a, b, b, a, a, a, a, b, a, b, a, b, b, a

  40. a a b b U-238 Th-234 Pa-234 U-234 Th-230 a a a b a Ra-226 Rn-222 Po-218 At-218 Bi-214 b b a b a Po-214 Pb-210 Bi-210 Po-210 Pb-206 Practice—Write All the Steps in the U-238 Decay Series and Identify the Stable Isotope at the End of the Series, Continued. • a, b, b, a, a, a, a, b, a, b, a, b, b, a Great granddaughter Great great granddaughter Daughter Granddaughter

  41. Object Dating • Mineral (geological). • Compare the amount of U-238 to Pb-206. • Compare amount of K-40 to Ar-40. • Archeological (once living materials). • Compare the amount of C-14 to C-12. • C-14 radioactive with half-life = 5730 years. • While substance is living, C-14/C-12 is fairly constant. • CO2 in air is ultimate source of all C in body. • Atmospheric chemistry keeps producing C-14 at the same rate it decays. • Once dies, C-14/C-12 ratio decreases. • Limit up to 50,000 years.

  42. Radiocarbon DatingC-14 Half-Life = 5730 Years

  43. Radiocarbon Dating

  44. Example 17.5—A Skull Believed to Belong to an Early Human Being Is Found to Have a C-14 Content 3.125% of that Found in Living Organisms. How Old Is the Skull? • From Table 17.2, when the concentration of C-14 is 3.125% of that found in living organisms, the age of the object is 28,560 years.

  45. Nonradioactive Nuclear Changes • A few nuclei are so unstable, that if their nuclei are hit just right by a neutron, the large nucleus splits into two smaller nuclei. This is called fission. • Small nuclei can be accelerated to such a degree that they overcome their charge repulsion and smash together to make a larger nucleus. This is called fusion. • Both fission and fusion release enormous amounts of energy. • Fusion releases more energy per gram than fission.

  46. + energy!! Fission

  47. Fission Chain Reaction • A chain reaction occurs when a reactant in the process is also a product of the process. • In the fission process it is the neutrons. • So you only need a small amount of neutrons to start the chain. • Many of the neutrons produced in the fission are either ejected from the uranium before they hit another U-235 or are absorbed by the surrounding U-238. • Minimum amount of fissionable isotope needed to sustain the chain reaction is called the critical mass.

  48. Fission Chain Reaction

  49. Fissionable Material • Fissionable isotopes include U-235, Pu-239, and Pu-240. • Natural uranium is less than 1% U-235. • The rest is mostly U-238. • Not enough U-235 to sustain chain reaction. • To produce fissionable uranium the natural uranium must be enriched in U-235: • To about 7% for “weapons grade.” • To about 3% for “reactor grade.”

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