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  2. Solar neutrino - Wikipedia

    en.wikipedia.org/wiki/Solar_neutrino

    Diagram showing the Sun's components. The core is where nuclear fusion takes place, creating solar neutrinos. A solar neutrino is a neutrino originating from nuclear fusion in the Sun's core, and is the most common type of neutrino passing through any source observed on Earth at any particular moment.

  3. Neutrino - Wikipedia

    en.wikipedia.org/wiki/Neutrino

    artificial nuclear reactions in nuclear reactors, nuclear bombs, or particle accelerators; during a supernova; during the spin-down of a neutron star; when cosmic rays or accelerated particle beams strike atoms; The majority of neutrinos which are detected about the Earth are from nuclear reactions inside the Sun.

  4. Photodisintegration - Wikipedia

    en.wikipedia.org/wiki/Photodisintegration

    The energy of these rays is sometimes sufficient to start photonuclear reactions resulting in emitted neutrons. One such reaction, 14 7 N (γ,n) 13 7 N, is the only natural process other than those induced by cosmic rays in which 13 7 N is produced on Earth. The unstable isotopes remaining from the reaction may subsequently emit positrons by β ...

  5. Sun - Wikipedia

    en.wikipedia.org/wiki/Sun

    The Sun is the star at the center of the Solar System.It is a massive, nearly perfect sphere of hot plasma, heated to incandescence by nuclear fusion reactions in its core, radiating the energy from its surface mainly as visible light and infrared radiation with 10% at ultraviolet energies.

  6. Nuclear reaction - Wikipedia

    en.wikipedia.org/wiki/Nuclear_reaction

    In nuclear physics and nuclear chemistry, a nuclear reaction is a process in which two nuclei, or a nucleus and an external subatomic particle, collide to produce one or more new nuclides. Thus, a nuclear reaction must cause a transformation of at least one nuclide to another.

  7. Kelvin–Helmholtz mechanism - Wikipedia

    en.wikipedia.org/wiki/Kelvin–Helmholtz_mechanism

    Because nuclear reactions were unknown, the main candidate for the source of solar energy was gravitational contraction. However, it soon was recognized by Sir Arthur Eddington and others that the total amount of energy available through this mechanism only allowed the Sun to shine for millions of years rather than the billions of years that ...

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  9. 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 ...