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NASA Facts
National Aeronautics and
Space Administration
Lyndon B. Johnson Space Center
Understanding Space Radiation
FS-2002-10-080-JSC
October 2002
• Altitude above the Earth – at higher altitudes the Earth’s
magnetic field is weaker, so there is less protection against
ionizing particles, and spacecraft pass through the trapped
radiation belts more often.
• Solar cycle – the Sun has an 11-year cycle, which culminates in
a dramatic increase in the number and intensity of solar flares,
especially during periods when there are numerous sunspots.
• Individual’s susceptibility – researchers are still working to
determine what makes one person more susceptible to the
effects of space radiation than another person.
Measuring Radiation
The absorbed dose of radiation is the amount of energy
deposited by radiation per unit mass of material. It is measured
in units of rad (radiation absorbed dose) or in the international
unit of Grays (1 Gray = 1 Gy = 1 Joule of energy per kilogram
of material = 100 rad). The mGy (milliGray = 1/1000 Gray) is
the unit usually used to measure how much radiation the body
absorbs. However, because different types of radiation deposit
energy in unique ways, an equivalent biological dose is used to
estimate the effects of different types of radiation. Equivalent
dose is measured in milliSieverts (mSv). The mSv, therefore,
takes into account not only how much radiation a person
receives, but how much damage that particular type of radiation
can do – the greater the possibility of damage for the same dose
of radiation, the higher the mSv value.
Crews aboard the space station receive an average of 80 mSv
for a six-month stay at solar maximum (the time period with the
maximum number of sunspots and a maximum solar magnetic
field to deflect the particles) and an average of 160 mSv for a
six-month stay at solar minimum (the period with the minimum
number of sunspots and a minimum solar magnetic field).
Although the type of radiation is different, one mSv of space
radiation is approximately equivalent to receiving three chest
x rays. On Earth, we receive an average of two mSv every year
from background radiation alone.
Crew members could receive higher doses of space radiation
during space walks while outside the protective confines of the
space station; however, NASA plans space walks to avoid the
trapped radiation belts around the Earth, and doses on previous
space walks have been kept very small.
Protecting Current and Future Space Station Crews
To determine acceptable levels of risk for astronauts, NASA
follows the standard radiation protection practices recommended
by the U.S. National Academy of Sciences Space Science
Board and the U.S. National Council on Radiation Protection
and Measurements.
Aboard the space station, improving the amounts and types of
shielding in the most frequently occupied locations, such as the
sleeping quarters and the galley, has reduced the crew’s exposure
to space radiation. Materials that have high hydrogen contents,
such as polyethylene, can reduce primary and secondary
radiation to a greater extent than metals, such as aluminum.
Space station crew members each wear physical dosimeters, and
also undergo a biodosimtery evaluation measuring radiation
damage to chromosomes in blood cells (see figure above).
Active monitoring of space radiation levels also can help reduce
the levels of radiation an astronaut receives by helping the
astronauts locate the best-shielded locations on the station.
The monitoring also serves as a warning should radiation levels
increase due to solar disturbances. Following a healthy diet and
lifestyle, including the use of antioxidants following radiation
exposure, should also reduce risks.
Radiation Measurements Aboard
the International Space Station
Below, in alphabetical order, are the many radiation measurement
devices and experiments that have flown to the
International Space Station.
Bonner Ball Neutron Detector
March – December 2001
A Japanese Space Agency experiment that measured the amount
of neutron radiation that entered the space station. Neutron radiation
can affect the blood-forming marrow in bones.
Charged Particle Directional Spectrometers – CPDS
2001 – present
There are three units mounted outside on the station’s S0 truss
that are designed to record the direction from which radiation
strikes. There is another unit inside the station.
Dosimetric Mapping – DOSMAP
March – August 2001
A German Space Agency/European Space Agency experiment
that consisted of four different types of radiation detectors
located throughout the space station, These measured the
amounts and types of radiation that entered the ISS.
Study of Radiation Doses Experienced by Astronauts
in EVA – EVARM
February 2002 – present
These sensors are being used to determine the levels of radiation
space walkers receive in their skin, eyes and blood-forming
organs. EVARM consists of three active dosimeters (placed on
Normal chromosome No. 2
and No. 4 in a postflight
metaphase sample
Damaged chromosome No. 2
in a postflight metaphase
sample
the leg, torso and near the eye) that are read before and after a
space walk. The EVARM data could be used to devise methods
of reducing the amount of radiation astronauts are exposed to
during space walks.
Passive Dosimetry
1999 – present
There are several types of radiation detectors aboard the space
station. The radiation area monitor (RAM) is a small set of thermoluminescent
detectors encased in Lexan plastic that respond
to radiation – the amount of radiation they absorb can be revealed
by applying heat and measuring the amount of visible light
released. RAM units are scattered inside the space station and
are returned to Earth for measurement after periodic space
shuttle visits. The crew passive dosimeter is very similar to
the RAM and is carried by each member of the crew. The
AN/UDR-13 radiac Set (a high-rate dosimeter) is a compact,
handheld or pocket-carried device capable of quickly measuring
doses of gamma or neutron radiation. Data readout and warning
messages are provided by a liquid crystal display on the set.
Phantom Torso
March – August 2001
This unique experiment
measured the effects of
radiation on organs inside
the human body by using
a torso equivalent in
height and weight to an
average adult male. The
torso contained radiation
detectors that measured
how much radiation the
brain, thyroid, stomach,
colon, and heart and lung area received on a daily basis. The
data are still being analyzed to determine how the body reacts
to and shields its internal organs from radiation, information
that will be very important during longer-duration space flights.
Tissue Equivalent Proportional Counter – TEPC
2000 – present
This radiation detector consists of a 2"-diameter by 2"-long
cylindrical cell that is filled with low-pressure propane gas. The
gas is used to simulate the hydrocarbon content of a human cell
that is two microns in diameter. A plastic jacket covering the cell
simulates the properties of adjacent tissue cells. Particles passing
through the gas release electrons, which are collected, helping to
identify the energy of the particles.
Measuring Space Radiation Between the Earth
and Mars
As the Mars Odyssey spacecraft made its way to Mars between
April and October 2001, the Mars radiation environment
experiment (MARIE) measured the amounts and kinds of space
radiation the spacecraft encountered along the way. These data
are essential to understanding how much and what kinds of
radiation future space travelers might encounter on a long trip
to explore the red planet.
Now in orbit around Mars, MARIE continues to measure the
amount of harmful radiation at the planet itself. Unlike Earth,
Mars does not have a global magnetic field to shield it from
solar flares and cosmic rays. Mars’ atmosphere is also less
than one percent as thick as the Earth’s. These two factors
make Mars very vulnerable to space radiation.
Aboard the International Space Station and in our own solar
system, NASA researchers continue to quantify the amounts
of space radiation our explorers face every day and will face
in the future. Understanding space radiation will not only protect
the crew currently aboard the International Space Station, but
those first humans who will continue the exploration of our
solar system.
Related Web Sites
http://spaceresearch.nasa.gov/research_projects/radiation.html
http://www.spaceflight.nasa.gov/station/science/bioastronautics/
Categories: Solar flare
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