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  2. Nuclear fusion - Wikipedia

    en.wikipedia.org/wiki/Nuclear_fusion

    Nuclear fusion is the process that powers active or main-sequence stars and other high-magnitude stars, where large amounts of energy are released. A nuclear fusion process that produces atomic nuclei lighter than iron-56 or nickel-62 will generally release energy.

  3. Fusion power - Wikipedia

    en.wikipedia.org/wiki/Fusion_power

    Fusion power is a proposed form of power generation that would generate electricity by using heat from nuclear fusion reactions.In a fusion process, two lighter atomic nuclei combine to form a heavier nucleus, while releasing energy.

  4. The Hope and Hype of Fusion Energy, Explained - AOL

    www.aol.com/news/hope-hype-fusion-energy...

    Nuclear fusion is the reverse of nuclear fission, which powers the nuclear plants we’re all familiar with. Fission splits atoms of very heavy, unstable isotopes like uranium 235 and captures the ...

  5. Iron peak - Wikipedia

    en.wikipedia.org/wiki/Iron_peak

    Light elements such as hydrogen release large amounts of energy (a big increase in binding energy) when combined to form heavier nuclei. Conversely, heavy elements such as uranium release energy when converted to lighter nuclei through alpha decay and nuclear fission. 56 28 Ni is the most thermodynamically favorable in the cores of high-mass stars.

  6. Explained: What nuclear fusion breakthrough means [Video] - AOL

    www.aol.com/news/nuclear-fusion-could-change...

    What is nuclear fusion, ... which the New York Times noted is the equivalent of a pound of TNT, the chemical reaction was achieved, resulting in the release of 3 megajoules of energy. ...

  7. Why the nuclear fusion breakthrough won't prevent ... - AOL

    www.aol.com/news/why-nuclear-fusion-breakthrough...

    Nuclear fusion is when two light atomic nuclei combine to form a single heavier one and release massive amounts of energy. It’s essentially the more powerful inverse of nuclear fission, a ...

  8. Proton–proton chain - Wikipedia

    en.wikipedia.org/wiki/Proton–proton_chain

    The total energy yield of one whole chain is 26.73 MeV. Energy released as gamma rays will interact with electrons and protons and heat the interior of the Sun. Also kinetic energy of fusion products (e.g. of the two protons and the 4 2 He from the p–p I reaction) adds energy to the plasma in the Sun.

  9. We have 'ignition': Fusion breakthrough draws energy gain - AOL

    www.aol.com/news/ignition-fusion-breakthrough...

    U.S. scientists have achieved “ignition” — a fusion reaction that produced more energy than it took to create — a critical milestone for nuclear fusion and a step forward in the pursuit of ...