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Nuclear Chemistry

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Title: Nuclear Chemistry


1
Nuclear Chemistry
2
Radioactivity
  • Energy or particles emitted fr an unstable
    nucleus
  • Light, heat, alpha, beta particles gamma rays

3
Types of Radiation
  • 4
  • Alpha(?)He nucleus 2He
  • 0
  • Beta (ß) an electron -1e high kinetic E
  • Gamma(?) high penetrating energy
  • ß ? can penetrate skin cause radiation
    sickness, cancer, or death
  • Geiger counter device to detect environmental
    radiation wh triggers electrical signals th are
    counted

4
Uses of Radiation
  • Tracers- water, oil flow drugs
  • Cancer treatment (gamma radiation)
  • Radiation bombards cancer cells
  • Carbon dating- determines relative age of items
    by measuring the ratio of stable and RA nuclei

5
Nuclear Equations
  • Sum of the mass s on the left right sides of
    the equation must be equal!
  • Sum of the electrical charges on the left right
    sides of the equation must be equal!
  • Decay RA particle is emitted (product)
  • Bombardment or Capture RA particle is a
    reactant
  • Other RA particles
  • 1 1
  • Proton 1H Neutron 0n
  • 2 0
  • Deutron 1H Neutrino (positron) e

6
Nuclear Stability
  • Of 1500 known isotopes, only 264 are stable
  • Stability depends upon the neutronproton ratio
  • Band of Stability (see graph) location of stable
    nuclei outside of this area, nuclei undergo
    spontaneous RA decay
  • Region A too many neutrons turn a neutron
    into a proton by emitting a ß particle
  • 1 1 0
  • 0n -gt 1H -1-e ß-decay emission

7
Nuclear Stability-cont.
  • Region B too many protons
  • Converts proton -gt neutron
  • an e- is captured
  • 59 0 59
  • 28Ni -1e -gt 27Co
  • Region C esp. heavy too many protons and
    neutrons
  • Emits alpha particles
  • 204 200 4
  • 82Pb -gt 80Hg 2He
  • All nuclei gt 82 are RA most undergo alpha
    emission

8
Half Life
  • The time it takes for half the RA elements in a
    sample to decay
  • 100 -gt 50 -gt 25 -gt 12.5 -gt 6.25 -gt etc.
  • Ea radioisotope has a unique half life fr
    milliseconds to 1000s of years
  • Decay series - the successive transformations of
    a RA isotope until a stable isotope is formed

9
Transmutation Reactions
  • Transmutation - conversion of an atom of one
    element into an atom of another element
  • Spontaneous/natural - Radioisotopes th decay
    14 14 6C -gt 7N
  • Artificial - when high E particles ( protons,
    neutrons, alpha) bombard the nucleus
  • 14 4 18
  • 7N 2He -gt 9F
  • Transuranium elements
  • atomic gt 92
  • Do not occur in nature
  • Radioactive
  • Synthesized by bombardment

10
Nuclear Fission
  • Splitting atoms nucleus broken into smaller
    nuclei by bombardment w/ neutrons
  • Forms 2 unequal nuclei
  • Emits neutrons lg amts of E
  • Chain rxn self-propagating
  • Released neutrons strike other nuclei they
    undergo fission releasing more E neutrons

11
Nuclear Fission Reactors
  • Core
  • Fuel Rods
  • Control Rods
  • Moderators
  • Coolant
  • Steam Turbine
  • Cooling Tower
  • Nuclear E -gt Heat E -gt Mechanical E -gt Electrical
    E

12
Nuclear Fission-cont
  • Atomic Bomb - uncontrolled chain rxn
  • Releases huge amts of E radiation
  • Killing burning for miles
  • Radiation w/ long half-lives
  • Radiation sickness, cancer, death
  • Requires a critical mass (min amt of material) to
    sustain the rxn

13
Nuclear Waste
  • Dangerous -emits radiation for 1000s of years
  • Storage- currently at reactor sites
  • Burial Yucca Mt ???
  • Vitrification - sealed in glass

14
Nuclear Fusion
  • Sun releases E via
  • 2 nuclei combine to produce a nucleus of heavier
    mass
  • 1 0 4
  • 4 1H 2 -1e -gt 2He Energy
  • Only occurs when temp is gt 40,000,000 C

15
Energy Mass in Nuclear Rxns
  • When the total mass of reactants products in a
    nuclear rxn are compared, mass seems to
    disappear!!
  • Nuclear Rxn
  • E mc2 E energy (joules)
  • m mass (kg)
  • C speed of light
  • 3.00x 108 m/s

16
Energy Mass in Nuclear Rxns
  • Loss of mass is proportional to E given off!
  • Helps explain why a stable nucleus stays together
  • Mass defect - the mass of a nucleus is slightly
    less than the sum of the individual masses of the
    protons neutrons th comprise it.

17
Energy Mass in Nuclear Rxns
  • Lower E a more stable nucleus
  • Binding E the amt of E needed to break s
    nucleus into its individual protons neutrons
    (neucleons)

18
Energy Mass in Nuclear Rxns
  • BE can be calculated fr mass defect
  • Mass of 1 mole of Hg-200
  • 199.9244g
  • Mass of 80 moles of protons
  • 120 moles of neutrons
  • 201.6228g

19
Energy Mass in Nuclear Rxns
  • 201.6228 g
  • - 199.9244 g
  • 1.6984 g
  • Use this mass in E mc2 to find BE
  • Most stable nuclei have a mass around 60

20
Energy Mass in Nuclear Rxns
  • Light nuclei give off E gain stability when
    they fuse together
  • Heavy nuclei give off E when they break apart
    (fission)

21
Radon Gas
  • Naturally occurring decay product from U-238
  • Emits alpha radiation
  • Cause of lung cancer property concerns
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