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1 Nuclear Chemistry Chapter 18 Hein and Arena Eugene Passer Chemistry Department Bronx Community College © John Wiley and Sons, Inc Version 2.0 12 th.

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Presentation on theme: "1 Nuclear Chemistry Chapter 18 Hein and Arena Eugene Passer Chemistry Department Bronx Community College © John Wiley and Sons, Inc Version 2.0 12 th."— Presentation transcript:

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2 1 Nuclear Chemistry Chapter 18 Hein and Arena Eugene Passer Chemistry Department Bronx Community College © John Wiley and Sons, Inc Version 2.0 12 th Edition

3 2 Chapter Outline 18.1 Discovery of RadioactivityDiscovery of Radioactivity 18.2 Natural RadioactivityNatural Radioactivity 18.3 Alpha Particles, Beta Particles and Gamma RaysAlpha Particles, BetaParticles and Gamma Rays 18.10 The Atomic BombThe Atomic Bomb 18.11 Nuclear FusionNuclear Fusion 18.4 Radioactive Disintegration SeriesRadioactive DisintegrationSeries 18.5 Transmutation of ElementsTransmutation of Elements 18.9 Nuclear PowerNuclear Power 18.12 Mass-Energy Relationships in Nuclear ReactionsMass-Energy Relationshipsin Nuclear Reactions 18.13 Transuranium ElementsTransuranium Elements 18.6 Artificial RadioactivityArtificial Radioactivity 18.7 Measurement of RadioactivityMeasurement ofRadioactivity 18.8 Nuclear FissionNuclear Fission

4 3 18.1 Discovery of Radioactivity

5 4 Roentgen In 1895 Wilhelm Konrad Roentgen discovered X-rays. Roentgen observed that a vacuum discharge tube enclosed in a thin, black cardboard box had caused a nearby piece of paper coated with the salt barium platinocyanide to glow with phosphorescence.

6 5 Roentgen From this and other experiments he concluded that certain rays, which he called X-rays, were emitted from the discharge tube, and penetrated the box and caused the salt to glow.

7 6 Becquerel Shortly after Roentgen’s discovery, Antoine Henri Becquerel attempted to show a relationship between X-rays and the phosphorescence of uranium salts. Becquerel wrapped a photographic plate in black paper, sprinkled a sample of a uranium salt on it, and exposed it to sunlight.

8 7 Becquerel When Becquerel attempted to repeat the experiment the sunlight was intermittent. He took the photographic plate wrapped in black paper with the uranium sample on it and placed the whole setup in a drawer.

9 8 Becquerel Several days later he developed the film and was amazed to find an intense image of the uranium salt on the plate. He repeated the experiment in total darkness with the same result.

10 9 Radioactivity is the spontaneous emission of particles and/or rays from the nucleus of an atom. Becquerel This proved that the uranium salt emitted rays that affected the photographic plate and that these rays were not a result of phosphorescence due to exposure to sunlight. Elements having this property are radioactive. Two years later, in 1896, Marie Curie coined the name radioactivity.

11 10 Rutherford In 1899 Rutherford began to investigate the nature of the rays emitted by uranium. He found two particles in the rays. He called them alpha and beta particles. Rutherford’s nuclear atom description led scientists to attribute the phenomenon of radioactivity to reactions taking place in the nuclei of atoms.

12 11 Villiard The gamma ray, a third type of emission from radioactive material, was discovered by Paul Villiard in 1900.

13 12DefinitionsDefinitions

14 13 nucleon a proton or a neutron mass number the total number of nucleons in the nucleus.

15 14 isotope atoms of the same element with different masses nuclide any isotope of any atom

16 15 Isotopic Notation

17 16

18 17 C 6 6 protons 12 6 protons + 6 neutrons A nuclide of carbon

19 18 8 8 protons 16 8 protons + 8 neutrons O A nuclide of oxygen

20 19 8 8 protons 17 8 protons + 9 neutrons O A nuclide of oxygen

21 20 8 8 protons 18 8 protons + 10 neutrons O A nuclide of oxygen

22 21

23 22 18.2 Natural Radioactivity

24 23 Radioactive elements continuously undergo radioactive decay or disintegration to form different elements. Radioactivity is a property of an atom’s nucleus. It is not affected by temperature, pressure, chemical change or physical state.

25 24 radioactive decay the process by which a radioactive element emits particles or rays and is transformed into another element.

26 25 Each radioactive nuclide disintegrates at a specific and constant rate, which is expressed in units of half-life. The half-life (t 1/2 ) is the time required for one-half of a specific amount of a radioactive nuclide to disintegrate.

27 26 The half-life of 131 I is 8 days. How much 131 I from a 32-g sample remains after five half-lives? Take a perpendicular line from any multiple of 8 days on the x-axis to the line on the graph. half-lives number of days amount remaining 0 32 g 1 8 16 g 2 16 8 g Trace a horizontal line from this point on the plotted line to the y-axis and read the corresponding grams of 131 I. 3 24 4 g 4 32 2 g 5 40 1 g 18.1

28 27 Nuclides are said to be either stable (nonradioactive) or unstable (radioactive). Elements that have an atomic number greater than 83 are naturally radioactive. Some of the naturally occurring nuclides of elements 81, 82 and 83 are radioactive and some are stable.

29 28 No stable isotopes of element 43 (technetium) or of element 61 (promethium) are known. Only a few naturally occurring elements that have atomic numbers less than 81 are radioactive.

30 29 Radioactivity is believed to be a result of an unstable ratio of neutrons to protons in the nucleus. Stable nuclides of elements up to about atomic number 20 generally have about a 1:1 neutron-to-proton ratio.

31 30 When the neutron to proton ratio is too high or too low, alpha, beta, or other particles are emitted to achieve a more stable nucleus. In elements above atomic number 20, the neutron-to-proton ratio in the stable nuclides gradually increases to about 1.5:1 in element number 83 (bismuth).

32 31

33 32 18.3 Alpha Particles, Beta Particles and Gamma Rays

34 33 Marie Curie, in a classic experiment, proved that alpha and beta particles are oppositely charged. radiation passes between the poles of an electromagnet a radioactive source was placed inside a lead block Alpha rays are less strongly deflected to the negative pole. Gamma rays are not deflected by the magnet. Beta rays are strongly deflected to the positive pole. three types of radiation are detected by a photographic plate 18.1

35 34 Alpha Particles

36 35 It consists of two protons and two neutrons. It has a mass of 4 amu. It has a charge of +2. The symbols of an alpha particle are An alpha particle is a helium nucleus.

37 36 Loss of an alpha particle from the nucleus results in loss of 4 in the mass number (A) loss of 2 in the atomic number (Z)

38 37 Formation of thorium from the radioactive decay of uranium can be written as or mass number decreases by 4 atomic number decreases by 2

39 38 To have a balanced nuclear equation the sum of the mass numbers (superscripts) on both sides of the equation must be equal. the sum of the atomic numbers (subscripts) on both sides of the equation must be equal. sum of mass numbers = 238 sum of atomic numbers = 92

40 39 Beta Particles

41 40 Its charge is -1. The symbols of the beta particle are The beta particle is identical in mass and charge to an electron.

42 41 A proton and a beta particle are formed by the decomposition of a neutron. The beta particle leaves the nucleus and the proton remains in the nucleus. n  p + e 1010 1111 0

43 42 Loss of a beta particle from the nucleus results in –no change in the mass number –an increase of 1 in the atomic number Pa  U + e 234 91 234 92 0

44 43 Gamma Rays

45 44 It is emitted by radioactive nuclei. It has no measurable mass. It has no electrical charge. The symbol of a gamma ray is A gamma ray is a high energy photon. 

46 45 Loss of a gamma ray from the nucleus results in –no change in the mass number –no change in atomic number

47 46 Write an equation for the loss of an alpha particle from the nuclide 194 Pt.

48 47 78 protons Pt 78 194 78 protons + 116 neutrons A nuclide of platinum Atomic number (number of protons in the nucleus) Mass number (sum of protons and neutrons in the nucleus) Write an equation for the loss of an alpha particle from the nuclide 194 Pt.

49 48 Write an equation for the loss of an alpha particle from the nuclide 194 Pt. Loss of an alpha particle, 4 He, results in a decrease of 4 in the mass number and a decrease of 2 in the atomic number. Mass of new nuclide:A-4 194 – 4 = 190 or A = mass number Atomic number of new nuclide:Z-278 – 2 = 76or Z = atomic number Element number 76 is Os, osmium. The equation is

50 49 What nuclide is formed when 194 Ra loses a beta particle from its nucleus?

51 50 88 protons Ra 88 228 88 protons + 140 neutrons A nuclide of radium Atomic number (number of protons in the nucleus) Mass number (sum of protons and neutrons in the nucleus) What nuclide is formed when 194 Ra loses a beta particle from its nucleus?

52 51 The loss of a beta particle from a 194 Ra nucleus means a gain of 1 in the atomic number with no essential change in mass. Mass of new nuclide:A-0 228 – 0 = 228 or A = mass number Atomic number of new nuclide: Z-(-1) Z = atomic number 88 + 1 = 89or What nuclide is formed when 194 Ra loses a beta particle from its nucleus? The equation is

53 52 Penetrating Power of Radiation

54 53 The ability of radioactive rays to pass through various objects is in proportion to the speed at which they leave the nucleus. Thin sheet of aluminum – stops  and  particles. 18.2 Thin sheet of paper – stops  particles. 5-cm lead block – will reduce, but not completely stop  radiation

55 54

56 55 18.4 Radioactive Disintegration Series

57 56 The naturally occurring radioactive elements with a higher atomic number than lead fall into three orderly disintegration series. Each series proceeds from one element to the next with the loss of either an alpha or a beta particle, finally ending in a nonradioactive nuclide.

58 57 –The uranium series starts with 238 U and ends with 206 Pb. 92 82 –The thorium series starts with 232 Th and ends with 208 Pb. 90 82 –The actinium series starts with 235 U and ends with 207 Pb. 92 82

59 58 A fourth series begins with the synthetic element plutonium. –The neptunium series begins with 241 Pu and ends with 238 Bi. 94 83

60 59 18.3 The uranium disintegration series. 238 U decays by a series of alpha (  ) and beta (  ) emissions to the stable nuclide 208 Pb.

61 60 18.5 Transmutation of Elements

62 61 Transmutation is the conversion of one element into another by either natural or artificial means. Transmutation occurs spontaneously in natural radioactive disintegrations.

63 62 Alchemists for hundreds of years attempted to transmute mercury and lead into gold by artificial means. They were never successful. The first artificial transmutation occurred in 1919 when Rutherford succeeded in producing oxygen from nitrogen.

64 63 Some of these transmutations are:

65 64 18.6 Artificial Radioactivity

66 65 Irene and Frederick Curie observed that the bombardment of aluminum-27 with alpha particles resulted in the emission of neutrons and positrons.

67 66 When alpha particle bombardment is halted neutron emission stops, but positron emission continues. This suggested that neutron emission and positron emission were a result of separate reactions.

68 67 Further investigation on their part showed that when aluminum-27 is bombarded with alpha particles phosphorous-30 is produced.

69 68 Phosphorous-30 is radioactive, has a 2.5 minute half-life, and decays to silicon- 30 with the emission of a positron.

70 69 The radioactivity of nuclides produced in this manner is known as artificial or induced radioactivity. The Joliot-Curies received the Nobel Prize in chemistry in 1935 for the discovery of artificial, or induced, radioactivity.

71 70 18.7 Measurement of Radioactivity

72 71 Radiation from a radioactive source can be measured by a variety of instruments. –Geiger counters –film badges –scintillation counters

73 72 The curie is the unit indicating the rate of decay of a radioactive substance. One curie (Ci) = 3.7 x 10 10 disintegrations per second. This very high radiation level is the amount of radiation emitted by 1 gram of radium in one second. Because a curie is so large the millicurie (one thousandth of a curie) and the microcurie (one millionth of a curie) are more commonly used.

74 73

75 74 18.8 Nuclear Fission

76 75 In nuclear fission, a heavy nuclide splits into two or more intermediate sized fragments when struck in a particular way by a neutron As the atom splits, it releases energy and two or three other neutrons, each of which can cause another nuclear fission.

77 76 Characteristics of Nuclear Fission 1.Upon absorption of a neutron, a heavy nuclide splits into one or more smaller nuclides (fission products). 2.The mass of the nuclides ranges from abut 70-160 amu. 3.Two or more neutrons are produced from the fission of each atom.

78 77 Characteristics of Nuclear Fission 4.Large quantities of energy are produced as a result of the conversion of a small amount of mass into energy. 5.Many nuclides produced are radioactive and continue to decay until they reach a stable nucleus.

79 78 Each time fission occurs three neutrons and two nuclei are produced. 18.5 Fission of 235 U

80 79 In a chain reaction the products cause the reaction to continue or magnify. For a chain reaction to continue, enough fissionable material must be present so that each atomic fission causes, on average, at least one additional fission.

81 80 The minimum quantity of an element needed to support a self-sustaining chain reaction is called the critical mass. Since energy is released in each atomic fission, chain reactions provide a steady supply of energy.

82 81 18.6 Fission and chain reaction of 235 U.

83 82 18.9 Nuclear Power

84 83 A nuclear power plant is a thermal power plant in which heat is produced by a nuclear reactor instead of by combustion of fossil fuel. The major components of a nuclear reactor are:b –an arrangement of nuclear fuel, called the reactor core. –a control system, which regulates the rate of fission and thereby the rate of heat generation.

85 84

86 85 In the United States breeder reactors are used to generate nuclear power. Breeder reactors use U 3 O 8 that is enriched with scarce, fissionable U-235. In a breeder reactor, excess neutrons convert nonfissionable isotopes, such as U-238 or Th-232, to fissionable isotopes, Pu-239 or U-233.

87 86 18.10 The Atomic Bomb

88 87 The atomic bomb is a fission bomb. “Wild” or uncontrolled fission occurs in an atom bomb, whereas in a nuclear reactor the fission is carefully controlled. A minimum critical mass of fissionable material is required for a bomb.

89 88 When a quantity of fissionable material smaller than the critical mass is used, too many neutrons escape and a chain reaction does not occur. The fissionable material of an atomic bomb is stored as two or more subcritical masses and are then brought together to achieve a nuclear detonation.

90 89 Uranium-235 and plutonium-239 are the nuclides used to construct an atomic bomb. 99.3% of uranium is nonfissionable uranium-238. Uranium-238 can be transmuted to fissionable plutonium- 239.

91 90 18.11 Nuclear Fusion

92 91 Nuclear fusion is the process of uniting two light elements to form one heavier element.

93 92 The masses of the two nuclei that fuse into a single nucleus are greater than the mass of the nucleus formed by their fusion. tritiumdeuterium3.0150 amu 1.0079 amu 4.0026 amu 4.0229 amu 4.0229 amu – 4.0026 amu = 0.0203 amu The difference in mass is released as energy.

94 93 Fusion reactions require temperatures on the order of tens of millions of degrees for initiation. Such temperatures are present in the Sun but have been produced only momentarily on earth.

95 94 Fusion power will be far superior to fission power because –Virtually infinite amounts of energy are possible from fusion power. –While uranium supplies are limited, deuterium supplies are abundant. –It is estimated that the deuterium present in a cubic mile of seawater used as fusion fuel can provide more energy than the petroleum reserves of the entire world.

96 95 Fusion power will be far superior to fission power because –Fusion power is much “cleaner” than fission power. –Fusion reactions (unlike uranium and plutonium fission reactions) do not produce large amounts of long-lived and dangerously radioactive isotopes.

97 96 18.12 Mass-Energy Relationship in Nuclear Reactions

98 97 In fission reactions, about 0.1% of the mass of the reactants is converted into energy. 7.016 g 1.008 g4.003 g 8.024 g 8.024 g – 8.006 g = 0.018 g 8.006 g In fusion reactions as much as 0.5% of the mass of the reactants may be changed into energy. The energy equivalent of this mass is 1.62 x 10 12 J. This is 4,000,000 times greater than the energy released from the combustion of 1 mol of carbon.

99 98 The mass of a nucleus is less than the sum of the masses of the protons and neutrons that makes up that nucleus. The difference between the mass of the protons and the neutrons in a nucleus is known as the mass defect. The energy equivalent to this difference in mass is known as the nuclear binding energy.

100 99 The nuclear binding energy is the amount of energy that would be required to break a nucleus into its individual protons and neutrons. The higher the binding energy, the more stable the nucleus.

101 100 Neutrons and protons attain more stable arrangements through nuclear fission or fusion reactions. –when uranium undergoes fission the products have less mass (greater binding energy) than the reactants. –when hydrogen and lithium fuse to form helium, the helium has less mass (greater binding energy) than the hydrogen and lithium.

102 101 Calculate the mass defect and the nuclear binding energy for an  particle (helium nucleus). 1.0 g = 9.0 x 10 13 J when converted into energy Data:proton mass = 1.0073 g neutron mass = 1.0087 g/mol  mass = 4.0015 g/mol Solution: First calculate the sum of the individual parts of an  particle: = 2.0146 g/mol2 x 1.0073 g2 protons: 2 neutrons:2 x 1.0087 g= 2.0174 g/mol 4.0320 g/mol

103 102 Calculate the mass defect and the nuclear binding energy for an  particle (helium nucleus). Mass defect: the difference between the mass of the  particle and its component parts. mass defect = 0.0305 g/mol mass of component particles = 4.0320 g/mol mass of  particle = 4.0015 g/mol Nuclear binding energy: convert mass defect to its energy equivalent:

104 103 18.13 Transuranium Elements

105 104 transuranium elements follow uranium in the periodic table and have atomic numbers greater than 92. They are synthetic radioactive elements; none of them occur naturally.

106 105 The first transuranium element, number 93, was discovered in 1939 by Edwin McMillan who named it neptunium for the planet Neptune. In 1941, element 94, plutonium, was identified as a beta-decay product of neptunium. Plutonium is one of the most important fissionable elements known today.

107 106


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