This content requires Adobe Flash Player version
or later.
Either you do not have Adobe Flash Player installed,
or your version is too old,
or there is a problem with your Flash installation and we were unable to detect it.
From white dwarfs to black holes as stellar end stages, from the atomic dimensions in nuclear physics to sizes of stars and distances that take thousands of years to cross travelling at the speed of light in galaxies, Anna Demming speaks to Professor Friedrich Thielemann about his research on the origin of the elements and the evolution of stars and galaxies.
Astronomical complexity: The origin of the elements