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Uranium-235

physical science Maturity 11-13 Next article →

Uranium-235, often called U-235, is a specific isotope of the element uranium. An isotope is a version of an element that has a different atomic weight. In nature, U-235 is quite rare, making up only about 0.72% of all natural uranium. Most uranium found on Earth is actually a different isotope called uranium-238. What makes U-235 so significant is that it is fissile. This means it can sustain a nuclear chain reaction. This unique property allows it to release massive amounts of energy through a process called fission.

Nuclear fission reaction
Nuclear fission reaction

Nuclear fission is the mechanism that releases this energy. The process begins when a U-235 nucleus is bombarded by a neutron. When the neutron strikes the nucleus, the atom splits apart. This split releases a large amount of energy and several new neutrons. If these new neutrons strike other U-235 nuclei, they cause more fission events. This creates a self-sustaining chain reaction. For a reaction to stay critical, at least one neutron from a fission event must strike another nucleus. If the reaction is sustained, it is said to be in a critical state. The specific amount of U-235 needed to reach this state is called the critical mass.

Nuclear fission reaction
Nuclear fission reaction

Scientists use different types of technology to manage these reactions. Some reactor types, such as heavy water reactors or graphite moderated reactors, can run on natural uranium. However, light water reactors require uranium that has undergone enrichment. Enrichment is a process that increases the proportion of U-235 by removing some of the U-238. Some specialized machines, like research reactors or those in nuclear submarines, use highly enriched uranium (HEU). HEU contains a much higher percentage of U-235. In nuclear weapons, the reaction is uncontrolled to create an explosion. To control power in a reactor, engineers use control rods. These rods contain elements like boron, cadmium, or hafnium that strongly absorb neutrons.

Nuclear fission reaction
Nuclear fission reaction

Our understanding of this isotope began in 1935. A scientist named Arthur Jeffrey Dempster discovered U-235. Since that discovery, the material has been used for both energy and weaponry. For example, the Little Boy atomic bomb used in Hiroshima on August 6, 1945, was made of highly enriched uranium. It featured a large tamper to help the reaction. While most modern nuclear weapons use plutonium-239 for the primary stage, HEU is still used in the secondary stage. In these designs, the highly enriched uranium acts as an ignitor for the fusion fuel.

The energy released during fission is immense. One single fission event of U-235 releases about 202.5 MeV of energy as heat in a thermal reactor. This total energy is composed of several parts. For instance, 169.1 MeV comes from the kinetic energy of fission fragments. Another 4.8 MeV comes from the kinetic energy of prompt neutrons. About 7.0 MeV is carried by prompt gamma rays. Additionally, 8.8 MeV escapes the reactor as anti-neutrinos. When looking at mass, the fission of one atom releases 19.54 TJ/mol, which is 83.14 TJ/kg.

Nuclear fission reaction
Nuclear fission reaction

Uranium-235 is also a subject of study in nuclear decay. It is an alpha emitter, meaning it releases alpha particles as it decays. This process turns U-235 into thorium-231. U-235 is the main progenitor of the actinium series. This is one of the principal decay chains among actinides. Because U-235 is the longest-lived primordial nuclide, it starts a long chain of changes. This series includes many other elements like astatine, bismuth, francium, and radium. Eventually, the decay process leads to the formation of stable lead-207. The half-life of U-235 is 704 million years.

Nuclear fission reaction
Nuclear fission reaction

Finally, U-235 helps scientists study the history of the universe through radiometric dating. By looking at the ratio of U-235 to U-238, researchers can calculate how much time has passed. This helps determine when these nuclei were formed during stellar nucleosynthesis. In 1957, a landmark paper by B2FH explained the r-process. This is the process by which these nuclei form in events like supernovae or kilonovae. Scientists use these ratios to estimate the age of the Milky Way. They can even study different scenarios, such as a single supernova or a continuous series of supernovae. This connection to the stars allows us to use a tiny atom to understand the vast history of space.

Nuclear fission reaction
Nuclear fission reaction
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