 An ingot of Plutonium-238, the typical power source used by NASA for its probes. (Source: Discovery News)
 The Cassini probe (pictured), the Voyager probes, and the Pioneer probes are all powered by Pu-238. NASA does not have enough Pu-238 to power its upcoming Mars Space Laboratory mission. (Source: Space Pictures)
Radioactive isotope is vital for powering deep-space probes
Europe,
a leader in nuclear power, has announced that it intends to lend its
American counterparts a hand by making Pu-238 for NASA. David
Southwood, ESA's director of science and robotic exploration, in an
interview with Spaceflight
Now,
states, "Our target is to have an independent capability, which
may help our American friends."
Since
the Pioneer and Voyager
missions of the 1970s, NASA has been using the radioactive
plutonium-238 (or Pu-238) isotope to power its deep space missions.
The radioactive source has a very long half-life of 87.7 years.
Over that period it slowly decays, releasing a steady stream of
thermal energy in the process. That thermal energy is harvested
by radioisotope
thermoelectric generators (RTGs) in the probes to make
power.
More recent missions to use the technology include
the Cassini
Equinox and New
Horizons missions.
Unfortunately, NASA's plutonium
stockpile has almost been exhausted, even as agency prepares its
new Mars
Space Laboratory which will require the isotope for power.
There's really no alternative currently for NASA, as the operational
range of many of its missions place it well outside the spatial
volume where the sun's rays are strong enough to provide a decent
level of solar power.
At a base level, NASA's plutonium
shortage is due to the fact that Pu-238 production is expensive and
tightly regulated. The U.S. Department of Energy, due to budget
cuts, lacks the money to fund additional production.
Despite
the fact that the material is not fissible -- hence cannot be made
into atomic bombs -- tight regulations are further constraining the
supply, limiting trade to only a couple potential candidates.
One of those candidates -- Russia -- is locked in a contract dispute
with NASA, essentially ruling out its possibility as a source for
now.
Jim Adams, deputy director of NASA's planetary
science division optimistically states, "If we close another
deal with the Russians for another delivery of plutonium-238, or get
domestic production restarted, there's sufficient plutonium well out
past the Outer Planets Flagship Mission."
Fortunately,
the European Space Agency is looking to come to NASA's rescue,
announcing that it will begin producing Pu-238 and offering it to its
American partner. Europe is a world leader in nuclear power,
with the majority of EU member France's power coming from nuclear
energy.
The move will allow it to provide fuel for the $4.5B
joint U.S.-Europe flagship mission to the Jovian moon Europa -- fuel
that NASA currently lacks. The ESA's Southwood states, "To
see see ourselves as a serious planetary science partner on the world
stage with the United States, we're building up our nuclear
capability for European-built RTGs. We are building for a
pretty major capability being available in Europe in the 2020s."
The
final production decision for the nuclear isotope will take place in
2011 or 2014 at EU council meetings.
Another perhaps
possibility for both the EU and U.S. is to alternatively produce
Americium-241. This radioactive isotope has the advantage of
being plentiful (it is found in most nuclear
waste) and has an extremely long half life of 432.2 years.
However, its power output (114 watts decay heat/kg) is much lower
than Pu-238's (560 watts decay heat/kg). And it is more
dangerous and hard to handle.
Warns Adams, "Plutonium-238
is an alpha emitter, and you can shield alpha particles with a piece
of paper. It's neutrons that damage people, and americium is
more a neutron emitter than plutonium-238."
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