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Uranium-238

physical science Maturity 11-13 Next article →

Uranium-238, often called U-238, is the most common isotope found in nature. It makes up more than 99% of all natural uranium. While it is not fissile in standard thermal-neutron reactors, it is highly significant in science and energy. A fissile material can sustain a chain reaction, but U-238 cannot. Instead, U-238 is considered fertile. This means it can be transmuted, or changed, into plutonium-239. Plutonium-239 is a fissile isotope that can be used as fuel for nuclear reactors or in weapons. This unique ability makes U-238 a vital resource for future energy production.

The way U-238 interacts with neutrons is quite complex. In a typical reactor, U-238 cannot sustain a chain reaction because of inelastic scattering. This process reduces the energy of neutrons to a level where they cannot cause fast fission in the next generation of nuclei. However, U-238 is fissionable by fast neutrons. These are neutrons with high kinetic energy, specifically more than 1 MeV. When these fast neutrons hit a U-238 nucleus, they can cause it to split. This process can contribute between one and ten percent of all fission reactions in certain reactor designs.

Uranium-238 also acts as a natural safety mechanism in nuclear reactors. It undergoes a process called Doppler broadening. As the temperature of the fuel increases, the neutron absorption resonances of U-238 also increase. This means the material absorbs more neutrons as it gets hotter. This creates a negative feedback mechanism that helps control the reactor. This process helps prevent the nuclear reaction from growing too fast or becoming unstable. It is an essential part of keeping nuclear power plants running safely.

One of the most important aspects of U-238 is its radioactive decay. It is an alpha emitter with a very long half-life of 4.463 billion years. This long half-life means it decays very slowly over vast amounts of time. The decay of U-238 follows a long path called a decay chain, also known as the uranium series. It transforms through several stages, including isotopes like thorium-234, protactinium-234, and uranium-234. Eventually, the chain ends when the material becomes stable lead-206. This predictable decay is used in radiometric dating to find the age of rocks older than 1 million years.

Because of its slow decay, U-238 is a major source of energy for our planet. It is responsible for approximately 40% of the radioactive heat produced within the Earth. This heat comes from the decay of the isotope and its daughter products. As U-238 decays, it also contributes to a geoneutrino signal. Specifically, the decay chain produces six electron anti-neutrinos per U-238 nucleus. These particles can be detected from deep within the Earth. This allows scientists to study the internal processes of our planet from the surface.

Engineers use different forms of uranium for various technological needs. Depleted uranium has a very high concentration of U-238. Low-enriched uranium (LEU) also contains mostly U-238, though it has more U-235 than depleted uranium. Reprocessed uranium is also mainly U-238, but it contains different amounts of other isotopes like U-236 and U-232. U-238 is also excellent for radiation shielding. It is about five times better at blocking gamma rays than lead. Because of its high atomic weight, it can be used in thinner layers to absorb X-rays and gamma rays. Scientists are even testing DUCRETE, a concrete made with uranium dioxide, for storing radioactive waste.

Specialized machines called breeder reactors are designed to make the most of U-238. A breeder reactor creates more fissile material, like plutonium-239, than it actually consumes. This process turns fertile U-238 into usable fuel. In Russia, the BN-600 reactor was a 600-megawatt breeder reactor that produced power. A newer unit, the BN-800, became fully operational in November 2016. While some reactors, like Japan's Monju, have faced safety and design challenges, other nations like China and India have plans for breeder technology. These reactors could potentially provide energy for 10,000 to five billion years.

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