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  2. r-process - Wikipedia

    en.wikipedia.org/wiki/R-process

    Abundance peaks for the r-process occur near mass numbers A = 82 (elements Se, Br, and Kr), A = 130 (elements Te, I, and Xe) and A = 196 (elements Os, Ir, and Pt). The r-process entails a succession of rapid neutron captures (hence the name) by one or more heavy seed nuclei, typically beginning with nuclei in the abundance peak centered on 56 Fe.

  3. Triple-alpha process - Wikipedia

    en.wikipedia.org/wiki/Triple-alpha_process

    Fusing with additional helium nuclei can create heavier elements in a chain of stellar nucleosynthesis known as the alpha process, but these reactions are only significant at higher temperatures and pressures than in cores undergoing the triple-alpha process.

  4. Alpha process - Wikipedia

    en.wikipedia.org/wiki/Alpha_process

    The stable alpha elements are: C, O, Ne, Mg, Si, and S. The elements Ar and Ca are "observationally stable". They are synthesized by alpha capture prior to the silicon fusing stage, that leads to Type II supernovae. Si and Ca are purely alpha process elements. Mg can be separately consumed by proton capture reactions.

  5. Stellar nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Stellar_nucleosynthesis

    The need for a physical description was already inspired by the relative abundances of the chemical elements in the solar system. Those abundances, when plotted on a graph as a function of the atomic number of the element, have a jagged sawtooth shape that varies by factors of tens of millions (see history of nucleosynthesis theory). [4]

  6. Nuclear fusion - Wikipedia

    en.wikipedia.org/wiki/Nuclear_fusion

    The release of energy with the fusion of light elements is due to the interplay of two opposing forces: the nuclear force, a manifestation of the strong interaction, which holds protons and neutrons tightly together in the atomic nucleus; and the Coulomb force, which causes positively charged protons in the nucleus to repel each other. [17]

  7. For the First Time Ever, Scientists Have Witnessed the Birth ...

    www.aol.com/first-time-ever-scientists-witnessed...

    The kilonova briefly mimicked the conditions immediately following the Big Bang, and allowed scientists to confirm the source of the heavy elements Strontium and Yttrium for the very first time.

  8. Illinois homeschoolers worry Trump tax credit could lead to ...

    www.aol.com/illinois-homeschoolers-worry-trump...

    (The Center Square) – Homeschool groups have concerns about President-elect Donald Trump’s proposed tax credit as Illinois lawmakers look at regulating the practice. Trump, in a video posted ...

  9. Decorating early for Christmas can boost your happiness, even ...

    www.aol.com/scientific-excuse-decorate-house...

    In order to make Christmas decorations last longer, Mattox and Baker follow these three tips that anyone can apply to their own home or business. 1. Go more natural.