Nuclear fusion
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 The Sun is a main-sequence star, and thus generates its energy by nuclear fusion of hydrogen nuclei into helium. In its core, the Sun fuses 620 million metric tons of hydrogen each second. |
Nuclear fusion is the process by which two or more atomic nuclei join together, or "fuse", to form a single heavier nucleus. During this process, matter is not conserved because some of the mass of the fusing nuclei is converted to energy which is released. Fusion is the process that powers active stars.
- Related: Aneutronic fusion, Focus fusion, Fusion power, Helium-3, Impulse generator, ITER, National Ignition Facility, Neutron generator, Neutron source, Nuclear fission, Nuclear physics, Nuclear reactor, Nucleosynthesis, Periodic table, Polywell, Pulsed power, Teller–Ulam design, Thermonuclear fusion, Timeline of nuclear fusion, Triple-alpha process
| NuclearFiles.org NuclearFiles.org www.nuclearfiles.org - Web |
| Annotated bibliography for nuclear fusion from the... Annotated bibliography for nuclear fusion from the Alsos Digital Library for Nuclear Issues alsos.wlu.edu/qsearch.aspx?browse=science/Fusion - Web |
| ITER (International Thermonuclear Experimental Rea... ITER (International Thermonuclear Experimental Reactor) website www.iter.org - Web |
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| CCFE (Culham Centre for Fusion Energy) website CCFE (Culham Centre for Fusion Energy) website www.fusion.org.uk - Web |
| JET (Joint European Torus) website JET (Joint European Torus) website www.jet.efda.org - Web |
