About this episode
The evolution of our Sun from ordinary star into red giant is radically different from the evolution of much more massive stars towards their end-points: supernova explosions followed by black holes.
This lecture will contrast the relevant nuclear physics and thermodynamics that determine these very different outcomes.
A lecture by Katherine Blundell OBE recorded on 18 January 2023 at David Game College, London.
The transcript and downloadable versions of the lecture are available from the Gresham College website: https://www.gresham.ac.uk/watch-now/end-stars
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