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All of these units are meaningless until one has some idea
of how bad one of them is for you. Here are some rules
of thumb that may be off by factors of two from one
case to the next:
- Instant Death:
It takes a monumental radiation dose to kill outright,
typically something like 5000 R (50 Grays)
"whole-body" - i.e. half a million ergs
of energy deposited in every gram of your body.
This amount of energy wipes out your central nervous system
(CNS) immediately when delivered all at once.
Needless to say, only the military mind makes a strong
distinction between this and the next level down.
- Overnight Death:
Approximately 900 R (9 Grays) whole-body
will accomplish the same thing as 50 Grays
but it takes about a day.
- Ugly Death:
A somewhat lower dose, around 500 R (5 Grays)
causes severe "radiation sickness"
(i.e. nausea, hair loss, skin lesions, etc.)
as the body's short-lived cells fail to provide
new generations to replace their normal mortality
("cell reproductive death").
It is not this trauma which usually kills, however,
but the complications that arise from a lack of
resistance to infection, due in turn to the
lack of new generations of white blood cells.
If you survive the initial radiation sickness
and avoid infection, you will probably recover
completely in the short term; but you are very
likely to develop cancer (especially leukemia)
in later years (usually some 10-20 years later!)
and your offspring, if any, will have
a high probability of genetic mutations.
- Sub-Acute Exposures:
From a whole-body dose of around 100 R (1 Gray)
delivered in less than about a week, you are
unlikely to notice any immediate severe symptoms.
However, you are likely to develop leukemia
in 10-30 years, and there is a significant chance
of genetic mutations in your offspring.
A whole-body exposure of 5 R delivered over 1 year
was believed in 1970 to represent 1.8 "doubling doses"
-- i.e. it was thought to multiply your odds of
developing cancer by a factor of 2.8 if maintained
year after year. At that time it was also the
legal exposure limit for radiation workers in the
U.S.A., set by the Atomic Energy Commission (AEC) there.
Presumably quite a few people received this exposure
for a few years, although it is unusual
for more than a small fraction of workers to receive
the maximum allowed exposure.
For perspective, it is noteworthy that a series of
spinal X-rays is apt to give an exposure of 1-4 R
locally, and that an afternoon on Wreck Beach in
midsummer often produces a painful sunburn that
represents 10-20 R to the skin; the resultant burn
is a bona fide radiation burn and is just as
dangerous as any other kind! In fact, the overwhelming
majority of all radiation-induced cancer fatalities
on Earth can be attributed directly to far ultraviolet
from our favourite nuclear fusion power plant in the sky:
the Sun.
- Marginal Exposures:
The average exposure from natural sources of radiation
is on the order of 300 mR per year. As of 1979
this was also the Canadian legal limit for public
exposure from artificial sources. Whether an extra
300 mR makes a significant difference epidemiologically
in the incidence of cancer depends almost entirely on
what one considers significant; however, it is a fact
that the statistical difference between populations
that have received such an exposure "artificially"
and those who have not
is smaller than the statistical differences between
populations with different eating habits, who live in
different regions, who have different types of jobs,
etc. This is partly because of the wide variety
in the amount and type of natural
radiation exposure.
Before we go on to discuss sources of radiation,
it is important to note that different organs or body parts
have dramatically different resistance to radiation.
The hands, in particular, are able to withstand
radiation doses that would kill if the whole body were
subjected to them! The lens of the eye and
the gonads are considered to be the most
vulnerable and should be protected first.
Next: Sources of Radiation
Up: How Bad is How Much of What, and
Previous: Units
Jess H. Brewer -
Last modified: Mon Nov 23 13:46:32 PST 2015