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CHAPTER 22 Nuclear Chemistry Types of Radiation  Isotopes - atoms of the same element with the same number of protons but different numbers of neutrons  Radioisotopes – isotope with an unstable nucleus that emits radiation to become a more stable nucleus  Radioactive Decay – spontaneous reaction in which unstable nuclei lose energy in the form of nuclear particles Nuclear Stability  Why do atoms decay anyway…  need stable ratio of neutrons to protons • Small atoms are stable with a 1 to 1 ratio of protons to neutrons • As the atomic number increases, atoms tend to have more neutrons than protons with stable ratio increasing to 1 to 1.5  The type of unbalance that is present in the nucleus determines the type of decay. Nuclear Stability Half-life  Half-life (t½)  Time required for half the atoms of a radioactive nuclide to decay.  Shorter half-life = less stable. C. Johannesson Half-life mf  m ( ) 1 n i 2 mf: final mass mi: initial mass n: # of half-lives Half-life  Fluorine-21 has a half-life of 5.0 seconds. If you start with 25 g of fluorine-21, how many grams would remain after 60.0 s? GIVEN: WORK: t½ = 5.0 s mi = 25 g mf = ? total time = 60.0 s n = 60.0s ÷ 5.0s n = 12 mf = mi (½)n mf = (25 g)(0.5)12 mf = 0.0061 g Types of Nuclear Particles Alpha particle (α)  Composition: 2 protons, 2 neutrons  Symbol: 4He or α  Charge: +2  Penetrating power: low, stopped by paper or cloth Beta particle (β)  Composition: 1 electron  Symbol: -1 e  Charge: -1  Penetrating power: 100 times greater than alpha, stopped by wood or concrete Gamma ray (γ )  Composition: electromagnetic waves  Symbol: γ  Charge: 0  Penetrating power: 1000 times greater than beta, stopped by lead or 6 feet of concrete Types of Nuclear Decay  Alpha Emission 238 92 parent nuclide U Th  He 234 90 daughter nuclide 4 2 alpha particle Numbers must balance!! Types of Nuclear Decay  Beta Emission 131 53 I 131 54 Xe  e 0 -1 electron  Positron Emission 38 19 K 38 18 C. Johannesson Ar  0 1 e positron Types of Nuclear Decay  Electron Capture 106 47 Ag  e  0 -1 106 46 Pd electron  Transmutation  One element becomes another. Fission vs. fusion Fission  splitting a nucleus into two or more smaller nuclei  1 g of 235U = 3 tons of coal 235 92 U Fission  chain reaction - self-propagating reaction  critical mass mass required to sustain a chain reaction Fusion  combining of two nuclei to form one nucleus of larger mass  thermonuclear reaction – requires temp of 40,000,000 K to sustain  1 g of fusion fuel = 20 tons of coal  occurs naturally in stars 2 1 H H 3 1 C. Johannesson Fission vs. Fusion F I S S I O N  235U is limited  danger of meltdown  toxic waste  thermal pollution F U S I O N     fuel is abundant no danger of meltdown no toxic waste not yet sustainable