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Contained Source Radiation
Safety Training
Module 1: Radiation Properties
This module provides information about the following topics:
The Atom
Radiation
Radioactive Decay
Alpha Particle Radiation
Beta Particle Radiation
Gamma Ray Radiation
X-Ray Radiation
Radiation Units
Half-Life
The Atom (top)
The Bohr Model of the atom consists of a central nucleus composed of neutrons
and protons surrounded by a number of orbital electrons equal to the number
of protons.
Protons are positively charged, while neutrons have no charge. Each has
a mass of about 1 atomic mass unit or amu. Electrons are negatively charged
and have mass of 0.00055 amu.
The number of protons in a nucleus determines the element of the atom.
For example, the number of protons in uranium is 92 while the number in
neon is 10. The proton number is often referred to as Z.
An element may have several isotopes. An isotope of an element is comprised
of atoms containing the same number of protons as all other isotopes of
that element, but each isotope has a different number of neutrons than
other isotopes of that element. Isotopes may be expressed using the nomenclature
Neon-20 or 20Ne10, where 20 represents the combined number of neutrons
and protons in the atom (often referred to as the mass number A), and 10
represents the number of protons (the atomic number Z).
While many isotopes are stable, others are not. Unstable isotopes normally
release energy by undergoing nuclear transformations (also called decay)
through one of several radioactive processes described later in this module.
Elements are arranged in the periodic table with increasing Z. Radioisotopes
are arranged by A and Z in the chart of the nuclides.
Go to a detailed periodic table of the nuclides.
Radiation (top)
Radiation is energy transmitted through space in the form of electromagnetic
waves or energetic particles. Electromagnetic radiation, like light or
radio waves, has no mass or charge. The following chart shows the electromagnetic
spectrum.

This training is concerned with radiation that has sufficient energy to
remove electrons from atoms in materials through which the radiation
passes. This process is called ionization,
and the high frequency electromagnetic
waves and energetic particles that can produce ionizations are called
ionizing radiations. Examples of ionizing radiation include:
- Alpha particle radiation
- Beta particle radiation
- Neutrons
- Gamma rays
- X-rays
Nonionizing radiations are not energetic enough to ionize atoms and interact
with materials in ways that create different hazards than ionizing radiation.
Examples of nonionizing radiation include:
- Microwaves
- Visible light
- Radio waves
- TV waves
- Ultraviolet light
Radioactive Decay (top)
The atomic structure for certain isotopes of elements is naturally unstable.
Radioactivity is the natural and spontaneous process by which the unstable
atoms of an isotope of an element transform or decay to a different state
and emit or radiate excess energy in the form of particles or waves. These
emissions are energetic enough to ionize atoms and are called ionizing
radiation. Depending on how the nucleus loses this excess energy, either
a lower energy atom of the same form results or a completely different
nucleus and atom is formed.
A given radioactive isotope decays through a specific transformation or
set of transformations. The type of emissions, along with the energy of
the emissions, that result from the radioactive decay are unique to that
isotope. For instance, an atom of phosphorus-32 decays to an atom of non-radioactive
sulfur-32, accompanied by the emission of a beta particle with an energy
up to 1.71 million electron-volts.
The following sections describe the radiations associated with the radioactive
decay of the radioisotopes most commonly used in research at Princeton
University.
Alpha Particle Radiation
(top)
An alpha particle consists of two neutrons and two protons ejected from
the nucleus of an atom. The alpha particle is identical to the nucleus
of a helium atom.
Examples of alpha emitters are radium, radon, thorium, and uranium.
Because alpha particles are charged and relatively heavy, they interact
intensely with atoms in materials they encounter, giving up their energy
over a very short range. In air, their travel distances are limited to
no more than a few centimeters. As shown in the following illustration,
alpha particles are easily shielded against and can be stopped by a single
sheet of paper.

Since alpha particles cannot penetrate the dead layer of the skin, they
do not present a hazard from exposure external to the body.
However, due to the very large number of ionizations they produce in a
very short distance, alpha emitters can present a serious hazard when they
are in close proximity to cells and tissues such as the lung. Special precautions
are taken to ensure that alpha emitters are not inhaled, ingested or injected.
Beta Particle Radiation (top)
A beta particle is an electron emitted from the nucleus of a radioactive
atom.
Examples of beta emitters commonly used in biological research are: hydrogen-3
(tritium), carbon-14, phosphorus-32, phosphorus-33, and sulfur-35.
Beta particles are much less massive and less charged than alpha particles
and interact less intensely with atoms in the materials they pass through,
which gives them a longer range than alpha particles. Some energetic beta
particles, such as those from P-32, will travel up to several meters in
air or tens of mm into the skin, while low energy beta particles, such
as those from H-3, are not capable of penetrating the dead layer of the
skin. Thin layers of metal or plastic stop beta particles.
All beta emitters, depending on the amount present, can
pose a hazard if inhaled, ingested or absorbed into the body. In addition,
energetic beta emitters are capable of presenting an external radiation
hazard, especially to the skin.
Bremsstrahlung
An important consideration in shielding beta particle radiation is the
ability of beta particles to produce a secondary radiation called bremsstrahlung.
Bremsstrahlung are x-rays produced when beta particles or other electrons
decelerate while passing near the nuclei of atoms. The intensity of bremsstrahlung
radiation is proportional to the energy of the beta particles and the atomic
number of the material through which the betas are passing.
Consequently, bremsstrahlung radiation is generally not a concern for
lower energy beta emitters such as carbon-14 and sulfur-35, but the
higher energy betas from phosphorus-32 can produce significant bremsstrahlung,
especially when passing through shielding materials such as lead. Lower
atomic number materials such as Plexiglas are preferred shielding materials
for high energy emitters such as phosphorus-32.
Gamma Ray Radiation (top)
A gamma ray is a packet (or photon) of electromagnetic radiation emitted
from the nucleus during radioactive decay and occasionally accompanying
the emission of an alpha or beta particle. Gamma rays are identical in
nature to other electromagnetic radiations such as light or microwaves
but are of much higher energy.
Examples of gamma emitters are:
- Cobalt-60
- Zinc-65
- Cesium-137
- Radium-226.
Like all forms of electromagnetic radiation, gamma rays have no mass or
charge and interact less intensively with matter than ionizing particles.
Because gamma radiation loses energy slowly, gamma rays are able to travel
significant distances. Depending upon their initial energy, gamma rays
can travel tens or hundreds of meters in air.

Gamma radiation is typically shielded using very dense materials (the
denser the material, the more chance that a gamma ray will interact with
atoms in the material) such as lead or other dense metals.
Gamma radiation particularly can present a hazard from exposures external
to the body.
X-Ray Radiation (top)
Like a gamma ray, an x-ray is a packet (or photon) of electromagnetic
radiation emitted from an atom, except that the x-ray is not emitted from
the nucleus. X-rays are produced as the result of changes in the positions
of the electrons orbiting the nucleus, as the electrons shift to different
energy levels.
Examples of x-ray emitting radioisotopes are iodine-125 and iodine-131.
X-rays can be produced during the process of radioactive decay or as bremsstrahlung
radiation. Bremsstrahlung radiation are x-rays produced when high-energy
electrons strike a target made of a heavy metal, such as tungsten or copper.
As electrons collide with this material, some have their paths deflected
by the nucleus of the metal atoms. This deflection results in the production
of x-rays as the electrons lose energy. This is the process by which an
x-ray machine produces x-rays.
Like gamma rays, x-rays are typically shielded using very
dense materials such as lead or other dense metals.
X-rays particularly can present a hazard from exposures external to the
body.
Radiation Units (top)
Quantity
The quantity of radioactive material present is generally measured in
terms of activity rather than mass, where activity is a measurement of
the number of radioactive disintegrations or transformations an amount
of material undergoes in a given period of time. Activity is related to
mass, however, because the greater the mass of radioactive material, the
more atoms are present to undergo radioactive decay.
The two most common units of activity are the Curie or the Becquerel (in
the SI system).
| 1 Curie (Ci) = 3.7 x 10
disintegrations per
second (dps) |
| 1 Becquerel (Bq) = 1 disintegration per second (dps) |
Obviously, 1 Curie is a large amount of activity, while 1 Becquerel is
a small amount. In the typical Princeton University laboratory, millicurie
and microcurie (or kilo and MegaBecquerel) amounts of radioactive material
are used.
| 1 millicurie = 2.2 x 10 disintegrations per minute (dpm) = 3.7
x 10
Bq = 37 MBq |
| 1 microcurie = 2.2 x 10
disintegrations per minute (dpm) = 3.7
x 10
Bq = 37 kBq |
Intensity
For the purposes of radiation protection, it is not always useful to describe
the potential hazard of a radioactive material in terms of its activity.
For instance, 1 millicurie of tritium a centimeter from the body poses
a much different hazard than 1 millicurie of phosphorus-32 a centimeter
from the body.
Consequently, it is often preferable to measure radiation by describing
the effect of that radiation on the materials through which it passes.
The three main quantities which describe radiation field intensity are
shown in the following table:
| Quantity |
Unit |
What is Measured |
Amount |
| Exposure |
Roentgen (R)
Coulombs/kg |
Amount of charge produced in 1 kg of air by x- or gamma rays |
1 R = 2.58 x 10
Cb/kg |
| Absorbed Dose |
Rad
Gray (Gy) |
Amount of energy absorbed in 1 gram of matter from radiation |
1 rad = 100 ergs*/gram
1 Gy = 100 rad |
| Dose Equivalent |
Rem
Sievert (Sv) |
Absorbed dose modified by the ability of the radiation to cause
biological damage |
rem = rad x Quality Factor |
Coulombs/kilogram, the Gray, and the Sievert are the SI units for these
quantities.
Go to optional information about the meaning
of these quantities and units.
Half-Life (top)
Radioactive materials decay at exponential rates unique to each radioisotope.
Half-life is the time required for a given amount of some radioactive material
to be reduced to one-half of its original activity.
The following table shows half-lives for radioisotopes commonly used in
Contained sources at Princeton University:
Radioisotope |
Half-Life |
Sodium-22 |
2.6 yr |
Iron-55 |
2.7 yr |
Cobalt-57 |
271.8 days |
Cobalt-60 |
5.3 yr |
Strontium-90 |
29.1 yr |
Cesium-137 |
30.1 yr |
Polonium-210 |
138.4 days |
Radium-226 |
1600 yr |
Americium-241 |
432.7 yr |
Go to an on-line calculator that will calculate the activity of these
common radionuclides at any elapsed time.
This is the end of the Radiation Properties Module, which
is the first of seven Contained Source Radiation Basics modules. The next
module
is the Background Radiation & Other Sources of Exposure Module.
Go to Module 2 (Background
Radiation and Other Sources of Exposure)
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