Transcript
What’s going on in the centre of all stars is small nuclei of atoms are bing joined together to make bigger ones. It’s a process we’d like to harness to power the Earth.
The fusion reaction that we do in JET is a reaction between two isotopes of hydrogen. JET is a very large device. I mean, if you stand next to it you are dwarfed by its scale. But in order to get to the stage where we can actually burn a plasma, fully self-sustaining fusion, we have to go to the next stage which is ITER. ITER is twice the size of JET. Really an enormous device.
This award of the Glazebrook medal is an award for Culham. I’m very lucky to have an extraordinarily clever, strong, motivated, skillful set of people.
We’ll be there at the finishing line. We’ll be there when fusion is actually a power source that people get some of their electricity from.
Solar visualisation: NASA/ESA Helioviewer project
NGC3314 overlapping galaxies: NASA, ESA, the hubble heritage team (STScI/AURA) – ESA/Hubble collaboration, and W. Keel (University of Alabama)
Superbubble in the large magellanic cloud: NASA/CXC/U.Mich/S.Oey, IR: NASA/JPL, Optical: ESO/WFI/2.2-m
ITER images and video: The ITER Organisation
Martyn James Bull { Writer + Filmmaker + Creative Director } 