Episode description
Stars have cores hot and dense enough to force atomic nuclei together, forming larger, heavier nuclei in a process known as fusion. In this process, the mass of the end products is slightly less than the mass of the initial atoms. But that “lost” mass doesn’t disappear — it’s converted to energy ... a lot of energy. So, can we harness this energy to power the world? George Zaidan investigates. This TED-Ed lesson was directed by Igor Ćorić, Artrake Studio, narrated by George Zaidan and the music is by Cem Misirlioglu and Brooks Ball.
Want to help shape TED’s shows going forward? Fill out our survey!
Learn more about TED Membership here!
Hosted on Acast. See acast.com/privacy for more information.
For the best experience, listen in Metacast app for iOS or Android
Open in Metacast