How "Star In A Jar" Technology Could Change Our World Forever

Markus Gann/Shutterstock

Jonathan O`Callaghan 20 Jan 2017, 17:30

Inside our Sun, hydrogen is constantly being converted into helium, producing a tremendous amount of energy – enough to heat the planets, melt comets, and support life on Earth. So it’d be pretty good if we could replicate that process on our own planet, right?

That’s what scientists have been trying to do for decades now. Nuclear fusion, also known as “star in a jar” technology, has seemingly always been on the horizon but never quite within reach. A number of recent breakthroughs, however, suggest we may soon be mimicking the power of the Sun on Earth.

One of the most recent breakthroughs was made using Germany’s Wendelstein 7-X (W7-X) fusion device. In early December 2016, scientists at the Max Planck Institute in Greifswald managed to sustain a hydrogen plasma in the experimental reactor for a few milliseconds.

It may not sound like a big deal, but this was hugely significant for a number of reasons. First, to kickstart nuclear fusion, extremely high temperatures – about 100 million °C (180 million °F) – are required to make a plasma cloud. This cloud must also be confined by extremely powerful magnets so that it does not touch the cold walls of the reactor.

Second, this process had only previously been achieved with a helium plasma. Hydrogen fusion provides much more energy, so is much more desirable. Just getting to this stage at all at the W7-X has taken 19 years and cost $1.1 billion.

The W-7X is a type of fusion reactor known as a stellarator, which is shaped like a twisted donut to keep the plasma confined, by twisting the magnetic fields around it. Another type of fusion reactor, known as a tokamak, achieves this twisted magnetic field in a different way. They are more regularly shaped donuts, but use a large current to achieve the same twisting effect in the plasma. Both methods have their advantages and disadvantages.

Full Article

If you liked this story, you'll love these

This website uses cookies

This website uses cookies to improve user experience. By continuing to use our website you consent to all cookies in accordance with our cookie policy.