The book begins with the Big Bang and the creation of light elements, then progresses to stellar nucleosynthesis, explaining how stars fuse heavier elements in their cores. Finally, it delves into supernovae, where the heaviest elements are created and dispersed. A unique aspect of this book is its accessible approach to complex topics, providing clear explanations and examples while avoiding excessive jargon.
Through astronomical observations, nuclear physics experiments, and cosmological simulations, How Elements Form offers a holistic view, connecting theoretical physics with observational astronomy.