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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