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Open Source Training Modules |
Open Source Radiation Safety Training Module 1: Radiation Properties
This module provides information about the following topics:
![]() (diagram courtesy of the University of Michigan Student Chapter of the Health Physics Society) 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 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:
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:
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. |
| 1 Curie (Ci) = 3.7 x1010 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 109 disintegrations per minute (dpm) = 3.7 x 107 Bq = 37 MBq |
| 1 microcurie = 2.2 x 106 dpm = 3.7 x 104 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 10-4 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
1 Sv = 100 rem |
Coulombs/kilogram, the Gray, and the Sievert are the SI units for these quantities.
Go to more detailed information about the meaning of these quantities and units
(diagram courtesy of the University of Michigan Student Chapter of the Health Physics Society )
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 half-life values for radioisotopes vary widely. For example,
the following table shows half-lives for radioisotopes commonly used
at
Princeton University:
| Radioisotope |
|
| Hydrogen-3 |
|
| Carbon-14 |
|
| Phosphorus-32 |
|
| Phosphorus-33 |
|
| Sulfur-35 |
|
| Iodine-125 |
|
This is the end of the Radiation Basics Module, which is the first of four Radiation Basics modules. The next module is the Background Radiation & Other Sources of Exposure Module.
Go to Module 2 (Background Radiation)
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For a disclaimer and information regarding the use of this page, see the disclaimer notice. Web page comments: marcians@princeton.edu. |