Astrochemistry: The Chemical Evolution of the Universe and Life's Origins

The journey begins shortly after the Big Bang, when the universe cooled enough for the first atomic nuclei to form, primarily hydrogen and helium. These light elements became the raw materials for the first stars. Through nuclear fusion within stars, heavier elements such as carbon, oxygen, and nitrogen were created. This process, known as nucleosynthesis, seeded the universe with the chemical ingredients necessary for the formation of molecules and, eventually, life.

Astrochemistry also relies heavily on the laws of physics, particularly thermodynamics and quantum mechanics, to explain how atoms bond and react under extreme cosmic conditions. Interstellar space may seem empty, but it contains gas and dust at very low densities and temperatures where unique chemical reactions take place. These reactions are not commonly observed on Earth, making their study essential for a complete understanding of chemistry in the universe.