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3
RadioactivityRadioactivity
• One of the pieces of evidence for the One of the pieces of evidence for the fact that atoms are made of smaller fact that atoms are made of smaller particles came from the work ofparticles came from the work of Marie CurieMarie Curie (1876-1934).(1876-1934).
• She discovered She discovered radioactive decayradioactive decay, , the spontaneous disintegration of the spontaneous disintegration of some elements into smaller pieces.some elements into smaller pieces.
4Nuclear Reactions vs. Nuclear Reactions vs. Normal Chemical Normal Chemical
ChangesChanges• Nuclear reactions involve the nucleusNuclear reactions involve the nucleus• The protons and neutrons are rearrangedThe protons and neutrons are rearranged• This releases a tremendous amount of energyThis releases a tremendous amount of energy• This energy was used to hold the nucleus This energy was used to hold the nucleus
together and is called together and is called binding energybinding energy
• ““Normal” Chemical Reactions involve Normal” Chemical Reactions involve electronselectrons, not protons and neutrons, not protons and neutrons
6
Types of RadiationTypes of Radiation
e01
He42
• Alpha Particle (Alpha Particle (αα) – two protons ) – two protons and two neutrons – a helium nuclei and two neutrons – a helium nuclei with a charge of 2with a charge of 2++
•Beta Particle (Beta Particle (ββ) – an electron) – an electron
•Gamma ray (Gamma ray (γγ) –high energy ) –high energy electromagnetic waves electromagnetic waves 0
0
7
Other Nuclear ParticlesOther Nuclear Particles
e01
n10• NeutronNeutron
• Positron – a positive electronPositron – a positive electron
•Electron capture – electron captured Electron capture – electron captured by the nucleus so found on the reactant by the nucleus so found on the reactant side of the equationside of the equation
•Proton – usually referred to as Proton – usually referred to as hydrogen-1hydrogen-1 H11
-1-10 0 ee
8
Balancing Nuclear ReactionsBalancing Nuclear Reactions
In the reactants and products
Atomic numbers must balanceand
Mass numbers must balance
Use a particle or isotope to fill in the missing protons and neutrons
9
Balancing Nuclear ReactionsBalancing Nuclear Reactions
• Alpha emissionAlpha emission
Note that mass number (A) goes down by 4 and atomic number (Z) goes down by 2.
Nucleons (nuclear particles… protons and neutrons) are rearranged but conserved
10
Balancing Nuclear ReactionsBalancing Nuclear Reactions
• Beta emissionBeta emission
Note that mass number (A) is unchanged and atomic number (Z) goes up by 1.
11
Balancing Nuclear ReactionsBalancing Nuclear ReactionsPositron (Positron (00
+1+1): a positive electron): a positive electron
Electron capture: Electron capture: the capture of an electron
207 207
12
Learning Check
What radioactive isotope is produced in the following alpha bombardment of boron-10?
105B + 4
2He → ? + 10n
13
Learning Check
Nitrogen – 13 plus a neutron is produced by the bombardment of boron?
105B + 4
2He → 137N + 1
0n
14
Write Nuclear Equations!
Write the nuclear equation for the beta emitter Co-60.
6027Co 60
28Ni + 0-1β
16
Half-Life
• The amount of time that it takes for ½ the mass of a radioactive nuclide to decay.
• Each nuclide has a half-life that is unique to that nuclide
17
Half-LifeHalf-Life
Decay of 20.0 mg of Decay of 20.0 mg of 1515O. What remains after 3 half-lives? O. What remains after 3 half-lives? After 5 half-lives?After 5 half-lives?
18
Problem The half life of Polonium-218 is 3.0
minutes. If you begin with 10.0 grams, how much would remain after 9.0 minutes?
Time Mass
0.0 minutes 10.0 grams
3.0 minutes 5.0 grams
6.0 minutes 2.5 grams
9.0 minutes 1.25 grams
19
Your Turn• The original mass of P-32 is 4.0 mg. The half-life of
P-32 is 14.3 days. How much P-32 will remain after 57.2 days?
Time Mass 0.0 days 4.0 mg
14.3 days 2.0 mg 28.6 days 1.0 mg 42.9 days .5 mg 57.2 days .25 mg
20
Radiocarbon DatingRadiocarbon DatingRadioactive C-14 is formed in the upper atmosphere Radioactive C-14 is formed in the upper atmosphere
by nuclear reactions initiated by neutrons in cosmic by nuclear reactions initiated by neutrons in cosmic radiationradiation
1414N + N + 11oon n 1414C + C + 11HH
The C-14 is oxidized to COThe C-14 is oxidized to CO22, which circulates through , which circulates through
the biosphere.the biosphere.
When a plant dies, the C-14 is not replenished.When a plant dies, the C-14 is not replenished.
But the C-14 continues to decay with tBut the C-14 continues to decay with t1/21/2 = 5730 years. = 5730 years.
Activity of a sample can be used to date the sample.Activity of a sample can be used to date the sample.
21
Radiation Exposure• Exposure to radiation can cause cancer and
genetic effects by damaging the DNA.
• Everyone is exposed to environmental background radiation – about .030 to .150 rems is normal
• .500 rems is acceptable according to the U.S. Government.
26
Nuclear FissionNuclear Fission• Fission is the splitting of unstable, Fission is the splitting of unstable,
very heavy nuclei into more stable very heavy nuclei into more stable
nuclei of intermediate mass.nuclei of intermediate mass.
• The process produces an enormous The process produces an enormous
amount of energyamount of energy
28Nuclear Fission & Nuclear Fission & POWERPOWER
• Currently about 103 Currently about 103
nuclear power plants in nuclear power plants in
the U.S. and about 435 the U.S. and about 435
worldwide.worldwide.
• About 20% of the U. S. About 20% of the U. S.
energy comes from energy comes from
nuclear.nuclear.
35
Nuclear Fusion
Fusion small nuclei combine
2H + 3H 4He + 1n +
1 1 2 0
Occurs in the sun and other stars
Energy
37Nuclear Medicine: Nuclear Medicine: ImagingImaging
Thyroid imaging using Tc-99Thyroid imaging using Tc-99
39
Food Food IrradiationIrradiation
•Food can be irradiated with Food can be irradiated with rays from rays from 6060Co or Co or 137137Cs.Cs.•Irradiated milk has a shelf life of 3 mo. Irradiated milk has a shelf life of 3 mo.
without refrigeration.without refrigeration.•USDA has approved irradiation of meats USDA has approved irradiation of meats
and eggs.and eggs.