Home / Series / The Life and Death of Stars / Aired Order / Season 1 / Episode 13

E = mc2—Energy for a Star’s Life

Probe the physics of nuclear fusion, which is the process that powers stars by turning mass into energy, according to Einstein’s famous equation. Then examine two lines of evidence that show what’s happening inside the sun, proving that nuclear reactions must indeed be taking place.

English
  • Runtime 30 minutes
  • Network The Great Courses
  • Created June 5, 2024 by
    Benbou
  • Modified June 5, 2024 by
    Benbou