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  2. 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 ...

  3. Stellar nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Stellar_nucleosynthesis

    They fuse helium until the core is largely carbon and oxygen. The most massive stars become supergiants when they leave the main sequence and quickly start helium fusion as they become red supergiants. After the helium is exhausted in the core of a star, helium fusion will continue in a shell around the carbon–oxygen core. [20] [24]

  4. Helium flash - Wikipedia

    en.wikipedia.org/wiki/Helium_flash

    Fusion of helium in the core of low-mass stars. A helium flash is a very brief thermal runaway nuclear fusion of large quantities of helium into carbon through the triple-alpha process in the core of low-mass stars (between 0.8 solar masses (M ☉) and 2.0 M ☉ [1]) during their red giant phase.

  5. Carbon-burning process - Wikipedia

    en.wikipedia.org/wiki/Carbon-burning_process

    In stars between 4 and 11 solar masses, the 16 O already produced by helium fusion in the previous stage of stellar evolution manages to survive the carbon-burning process pretty well, despite some of it being used up by capturing 4 He nuclei. [1] [8] So the result of carbon burning is a mixture mainly of oxygen, neon, sodium and magnesium. [3] [5]

  6. Supernova nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Supernova_nucleosynthesis

    Supernova nucleosynthesis is the nucleosynthesis of chemical elements in supernova explosions.. In sufficiently massive stars, the nucleosynthesis by fusion of lighter elements into heavier ones occurs during sequential hydrostatic burning processes called helium burning, carbon burning, oxygen burning, and silicon burning, in which the byproducts of one nuclear fuel become, after ...

  7. Dredge-up - Wikipedia

    en.wikipedia.org/wiki/Dredge-up

    The third dredge-up occurs after a star enters the asymptotic giant branch, after a flash occurs in a helium-burning shell. The third dredge-up brings helium, carbon, and the s-process products to the surface, increasing the abundance of carbon relative to oxygen; in some larger stars this is the process that turns the star into a carbon star. [3]

  8. Eric Stonestreet Says His “Modern Family ”Costars Are the ...

    www.aol.com/eric-stonestreet-says-modern-family...

    Nearly five years after their beloved series wrapped, the Modern Family cast is still as close as ever.. In an exclusive interview with PEOPLE, star Eric Stonestreet, 53, spoke about his tight ...

  9. Alpha process - Wikipedia

    en.wikipedia.org/wiki/Alpha_process

    Creation of elements beyond carbon through alpha process. The alpha process, also known as alpha capture or the alpha ladder, is one of two classes of nuclear fusion reactions by which stars convert helium into heavier elements. The other class is a cycle of reactions called the triple-alpha process, which consumes only helium, and produces ...