The Chemistry of Interstellar and Intergalactic Space

Abstract

This paper delves into the fascinating processes that underlie the formation of elements in stars and the explosive aftermath of supernovae. We explore the nuclear fusion reactions occurring within stars, elucidating the birth of elements from hydrogen to heavier metals. Additionally, we investigate the crucial role of supernovae in scattering these newly formed elements into space, enriching the cosmos with the diversity of elements we observe today. Through a blend of theoretical models and observational data, this paper offers an in-depth understanding of how stars and supernovae contribute to the elemental composition of the universe.