Nuclear Astrophysics

The synthesis of all elements heavier than lithium occurs via nuclear reactions inside stars, and these very processes also provide the energy that makes stars such as the sun emit light and heat.

These heavy nuclei are scattered in to space when a star reaches the end of its lifetime in a massive explosion (supernova), having spent all its nuclear fuel. Subsequently this material condenses to form the next generation of planets and stars.

The study of astrophysical explosions can give us new insights into the cycle of nuclear processes by which the elements are formed.