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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. Proton–proton chain - Wikipedia

    en.wikipedia.org/wiki/Proton–proton_chain

    At the Sun's core temperature of 15.5 million K the PP process is dominant. The PP process and the CNO process are equal at around 20 MK. [1] Scheme of the proton–proton branch I reaction. The proton–proton chain, also commonly referred to as the p–p chain, is one of two known sets of nuclear fusion reactions by which stars convert ...

  4. Stellar nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Stellar_nucleosynthesis

    Hydrogen fusion (nuclear fusion of four protons to form a helium-4 nucleus [20]) is the dominant process that generates energy in the cores of main-sequence stars. It is also called "hydrogen burning", which should not be confused with the chemical combustion of hydrogen in an oxidizing atmosphere.

  5. File:Nuclear fusion forces diagram.svg - Wikipedia

    en.wikipedia.org/wiki/File:Nuclear_fusion_forces...

    Diagram illustrating, in a schematic way, the technical difficulties of nuclear fusion, which much bring positively charged nuclei close enough so that the nuclear force will kick in. To demonstrate this I have drawn the ranges of the various forces as colored regions.

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

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

    What is nuclear fusion, ... In order to replicate the chemical process that powers stars in the universe, researchers at the National Ignition Facility employed the world’s most energetic lasers ...

  7. CNO cycle - Wikipedia

    en.wikipedia.org/wiki/CNO_cycle

    The CNO-I process was independently proposed by Carl von Weizsäcker [5] [6] and Hans Bethe [7] [8] in the late 1930s. The first reports of the experimental detection of the neutrinos produced by the CNO cycle in the Sun were published in 2020 by the BOREXINO collaboration. This was also the first experimental confirmation that the Sun had a ...

  8. Triple-alpha process - Wikipedia

    en.wikipedia.org/wiki/Triple-alpha_process

    Nuclear fusion reaction of two helium-4 nuclei produces beryllium-8, which is highly unstable, and decays back into smaller nuclei with a half-life of 8.19 × 10 −17 s, unless within that time a third alpha particle fuses with the beryllium-8 nucleus [3] to produce an excited resonance state of carbon-12, [4] called the Hoyle state, which ...

  9. Inside the Nuclear Fusion Facility That Changed the World - AOL

    www.aol.com/inside-nuclear-fusion-facility...

    The primary impetus for NIF’s construction was the promise that fusion reactions ignited by the facility’s powerful lasers would yield data that would help the U.S. maintain its nuclear ...