The Big Bang produced almost only the two lightest elements, hydrogen and helium. Everything heavier — the carbon in your cells, the oxygen you breathe, the calcium in your bones, the iron in your blood — was forged inside stars. Stars spend their lives fusing light elements into heavier ones, and when massive stars die in supernova explosions, they scatter those elements across space and forge some of the heaviest ones in the blast itself.
So the material in your body was cooked in stars that lived and died before the sun existed, drifted through space, and eventually collected into the cloud that formed our solar system. This isn't poetry — it's nucleosynthesis, confirmed by matching the elemental abundances we observe with the physics of stellar interiors. Every atom heavier than helium in you has been through the core of at least one star.
In 1957 four scientists — Margaret Burbidge, Geoffrey Burbidge, William Fowler, and Fred Hoyle — published a landmark paper, known ever since by their initials as B²FH, that worked out the nuclear reactions by which stars build up the periodic table from hydrogen. Fred Hoyle had earlier made a startling prediction: for carbon to be produced in the quantities we observe, the carbon nucleus had to have a specific energy state, which experimenters then went and found exactly where he said it would be. The B²FH framework explained why the universe contains the elements it does, in the proportions it does. William Fowler shared the 1983 Nobel Prize for this work. It transformed 'we are made of star-stuff' from a metaphor into measured physics.