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Nuclear Chemistry:
Like regular chemistry, only different.

Nuclear reactions involve the atomic nucleus. Regular chemical reactions
involve only the outer electrons of atoms. In a chemical reaction, elements do
not change from one to another. When an atomic nucleus changes, it is very
probable that the products will be different elements than the reactants.
The energy needed to change an atomic nucleus is much greater than the energy
needed to rearrange the valence electrons of atoms. While we are surrounded by
many naturally occuring radioactive materials,
the nuclear chemist must use accelerators
and reactors
to achieve the extreme energies needed for their reactions.
Fission is a nuclear reaction in which a very heavy nucleus is split into
two approximately equal fragments. This process, known as a chain reaction,
releases several neutrons which in turn split more nuclei. If it is not
controlled, a nuclear explosion can occur. The photograph above is a ground
explosion of twenty pounds of plutonium releasing the energy equal to 70 million
pounds of TNT. See an air burst
equal to 2,180 million pounds of TNT.
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Man's first controlled nuclear reaction - December 2, 1942, at 3:25
p.m.  |
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Man's first atomic explosion - July 16, 1945, at 5:29:45 a.m.  |
Day 2
| Fusion is a nuclear reaction in which two or more small nuclei
are forced together to form one larger nucleus. The energy released
during a fusion reaction is much greater than in a fission reaction.
Transmutation - a change in the
number of protons in the nucleus producing an atom with a different
atomic number.
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Click on the drawing to tour the accelerators
at Fermilab. |
Transmutation can be represented with a nuclear equation. The earliest
artificial transmutation was performed by Lord Rutherford in 1911. Nitrogen-14
was bombarded with alpha particles, producing Oxygen-17 and protons. The nuclear
equation for this reaction looks like this:
14
7 |
N + |
4
2 |
He  |
17
8 |
O + |
1
1 |
H |
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This is a balanced equation. The total mass number (top) is 18
on both sides and the total charge (bottom) is +9 on both sides.
Changing the nucleus of an atom often turns it into another element. For
this reason, you rarely have the same elements on both sides of balanced
nuclear equations. |
Nuclear equations
must be balanced just like regular chemical equations.
To balance nuclear equations, follow these two rules:
- Mass number is conserved in a nuclear change.
The sum of the mass numbers before the change must equal the sum of the mass
numbers after the change.
- Electric charge is conserved in a nuclear change.
The total electric charge on subatomic particles and nuclei before and after
the change must be equal.
This
is a nuclear chemical symbol:
The element is represented by its
chemical symbol.
The top number is the mass number
- total protons and neutrons.
The bottom number is the atomic
number - number of protons, or positive charges.
Nuclear particles and nuclear
equations:
Alpha
particle
Beta particle, an electron
Beta-plus
particle, a positron
Neutron
Proton
K-capture - An atomic nucleus captures an electron
from its own innermost energy level. When this happens, the atomic number is
decreased by one and the mass number remains the same.
In an equation, K-capture looks like this:
100
44 |
Ru + |
0
-1 |
e  |
100
43 |
Tc |
Homework
Assignment:
This assignment must be turned in by the beginning of class tomorrow to
receive credit.
- Complete and balance the following equations:
| a. |
7
3 |
Li + |
1
1 |
H  |
4
2 |
He |
|
|
| b. |
3
1 |
H + |
2
1 |
H  |
1
0 |
n |
|
|
| c. |
14
6 |
C  |
14
7 |
N |
|
|
| d. |
9
4 |
Be + |
4
2 |
He  |
12
6 |
C |
|
|
| e. |
26
12 |
Mg + |
1
0 |
n  |
0
+1 |
e |
|
|
| f. lead-214 decays by beta emission |
|
|
| g. bismuth-214 decays by beta emission |
|
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| h. polonium-214 decays by alpha emission |
Day 3
Not all isotopes of an element are equally stable. A completely stable
isotope is one whose nucleus will not spontaneously decay. A completely unstable
isotope would be one whose nucleus spontaneously decays completely. Most
isotopes fall somewhere in between. It is possible to predict which isotopes
will be the most stable using the following general rules:
- The greater the binding energy per nucleon, the more stable the nucleus.
- Nuclie of low atomic numbers with a 1:1 neutron to proton ratio are very
stable.
- The most stable nuclei tend to contain an even number of both protons and
neutrons.
Half-life:
The length of time it takes for one-half of the atoms of a radioactive nuclide
to disintegrate. The rate of disintegration is measured in a unit called a becquerel,
Bq.
| Half-Life Table |
| Nuclide |
Half-life |
Decay Type |
6
2 He |
0.802 seconds |
Beta-minus |
227
92 U |
1.3 minutes |
Alpha and Gamma |
3
1 H |
12.3 years |
Beta-minus |
14
6 C |
5730 years |
Beta-minus |
235
92 U |
7.1 x 10 8 years |
Alpha and Gamma |
Nuclear Decay Calculator
Radiation and living things:
All radiation, whether particles or waves, has an effect on living things.
If the radiation has enough energy, it can penetrate living cells and disrupt
their processes. This is particularly dangerous if DNA or RNA molecules are
affected. Very small changes in this genetic material can cause mutations and
cancer. Large amounts of radiation released into the upper atmosphere can
quickly travel around the world. This map
shows how wind carried the radiation from Chernobyl in 1986. Because of the
dangers involved, the measurement of radiation around living things is
important. Radiation used to be measured in rads and rems. These
units have been changed to fit within the International System of Measurement.
The amount of radiation being produced by a source is now measured grays,
Gy. One gray is equal to the transfer of one joule of energy to one
kilogram of living tissue. The damage to tissue is better indicated by the
absorbed dose of radiation, which is measured in sieverts, Sv. A
sievert is equal to a gray multiplied by factors that determine how much of the
energy transferred was actually absorbed by the tissue.
We are always being exposed to radiation found naturally in our environment.
This radiation is known as background radiation and is equal to about
0.001 Sv/year. Here is a general idea about radiation amounts:
- A single medical X-ray produces about 0.2 mSv (0.0002 Sv)
- Nuclear reactor workers are permitted to receive up to 0.05 Sv/year
- An exposure of 1 Sv/hour results in radiation poisoning
- Exposure to 3 to 5 Sv/hour results in death in 50% of the cases
Food Irradiation:
It has been found that food spoilage can be prevented by exposing it to gamma
radiation from 6027Co. Depending on the dose level,
irradiated food may last for weeks or even years without refrigeration and with
no change in the taste or consistency of the food. The U.S. Food and Drug
Administration has approved the irradiation of some foods with dosages up to
1000 grays.
Care to guess which of these has been exposed to radiation?
Portfolio
Assignment:
- Batteries used in heart pacemakers contain plutonium-238. The half-life
of plutonium-238 is 27.1 years. If your original sample contains 2.57 x 109
atoms of 23894Pu, how much time will pass
before the amount is reduced to 5.02 x 106 atoms?
- Do a quick Internet search for "radiation sterilization".
Write one paragraph giving your ideas about the safety of food
irradiation.
- Commercial fusion reactors have been a dream for years because of their
"clean" fuel (hydrogen) and waste (helium). The problem has been
the cost of containing the reaction. While an experimental fusion reactor
as been in operation at Princeton University for years, it takes more
electricity to run the reactor than the reactor can produce. A group of
scientists from the U.S., Japan, Russia, and other European countries is
working on a new reactor design at a site in California. Do an Internet
search for "International Thermonuclear Experimental Reactor".
What is the status of this project?
Research Links:
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