Nuclear Equations

Balancing nuclear equations is done by keeping the "sum of the nucleon numbers" and the "sum of the atomic numbers" the same on each side of the yield sign. Thus one may predict one of the reactants or products if all other substances are given.

The radiation types may be summarized as follows:
Radiation TypeSymbol
Alpha42He
Beta0-1e
Gamma00g *
Positron0+1e
Neutron01n
* g = greek symbol gamma


Examples:
23892U ---> ______ + 23490Th

For the missing product:
the nucleon number = 4. (238-234)
the atomic number = 2. (92-90)
thus the radiation type is 42He.


146C ---> ______ + 0-1e

For the missing product:
the nucleon number = 14. (14-0)
the atomic number = 7. (6-(-1))
thus the daughter isotope is 147N.


_______ ---> 157N + 0+1e

For the missing reactant:
the nucleon number = 15. (15+0)
the atomic number = 8. (7+1)
thus the parent isotope is 158O.


12151Sb + 11H ---> ______ + 10n

For the missing product:
the nucleon numbers = 121. (121 + 1 - 1)
the atomic number = 52. (51 + 1 -0)
thus the isotope is 12152Te



Half Life Problem

In a typical half life problem you are predicting the amount and/or counts per minute of a radiosope that is left after a given number of years. Another form is predicting the age of an object by measuring how much radiation is left, knowing the normal number of counts per minute for the object at time = 0 (now).

In half life tables:
time increases by half life, and grams, as well as counts per minute (CPM), drop in half for each successive half life. Time always starts at "0".


In a typical example:
If a radiosotope has a half life of 15 days and one currently has 200 grams of the isotope, and it has a counting rate of 1000 CPM (counts per minute), calculate how many grams of the radioisotope is left, and its counting rate, after 75 days.

Time015304560 75
Grams200100502512.56.25
CPM100050025012562.531.25