nucleosynthetic yields

Nucleosynthetic yields refer to the amounts of new chemical elements and isotopes produced by stars during their lifetimes and explosive events like supernovae. These yields are the result of nuclear reactions that occur inside stars, creating elements heavier than hydrogen and helium. When stars die or explode, they release these elements into space, enriching the galaxy. Scientists study these yields to understand how different stars contribute to the chemical makeup of the universe, including the elements found on Earth and in living organisms.