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Alex McColgan

πŸ‘€ Speaker
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26107 total appearances
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Podcast Appearances

Astrum Space
We're Close to Harnessing the Power of a Star

So much so, that even the kinetic energy provided by the extreme conditions at the heart of the sun

Astrum Space
We're Close to Harnessing the Power of a Star

where protons are travelling around 500 km per second, is wildly insufficient.

Astrum Space
We're Close to Harnessing the Power of a Star

In fact, protons have only around 1,000th of the kinetic energy they require to overcome this barrier.

Astrum Space
We're Close to Harnessing the Power of a Star

It turns out, the only reason the Sun is able to sustain fusion at all is because quantum effects come into play.

Astrum Space
We're Close to Harnessing the Power of a Star

Now, you may remember that according to quantum physics, protons don't just act as particles, they also act as waves.

Astrum Space
We're Close to Harnessing the Power of a Star

This wave behavior means that in 10 to the power 28 proton-proton interactions, the protons can overcome this energy barrier, getting close enough that the strong nuclear force pulls them together.

Astrum Space
We're Close to Harnessing the Power of a Star

This is called quantum tunneling.

Astrum Space
We're Close to Harnessing the Power of a Star

But even when protons are drawn together this way,

Astrum Space
We're Close to Harnessing the Power of a Star

There is yet another effect to contend with.

Astrum Space
We're Close to Harnessing the Power of a Star

The force that mediates the conversion of one of the protons into a neutron is the weak force, which, because it is controlled by the massive W boson, is very inefficient.

Astrum Space
We're Close to Harnessing the Power of a Star

This leads to the more likely product of the proton-proton reaction being a proton pair, which immediately decays back into single protons.

Astrum Space
We're Close to Harnessing the Power of a Star

Together, these effects mean that the rate of proton conversion in our star is extremely slow.

Astrum Space
We're Close to Harnessing the Power of a Star

On average, a proton will wait 10 billion years before undergoing fusion.

Astrum Space
We're Close to Harnessing the Power of a Star

Indeed, the only reason the proton-proton reaction proceeds at all is because there are a heck of a lot of protons in the Sun, allowing it to convert 600 million tonnes of hydrogen

Astrum Space
We're Close to Harnessing the Power of a Star

to 596 tonnes of helium every second.

Astrum Space
We're Close to Harnessing the Power of a Star

This sounds like a lot, but it's actually only a tiny fraction of the hydrogen available for fusion.

Astrum Space
We're Close to Harnessing the Power of a Star

Now, stopping for a moment to look at the big picture, this is very good news for us earthlings.

Astrum Space
We're Close to Harnessing the Power of a Star

It means, instead of annihilating itself in a giant thermonuclear explosion, the sun has been gently burning through its hydrogen stocks for around 4.6 billion years, and will continue to do so for at least a few billion more.

Astrum Space
We're Close to Harnessing the Power of a Star

It's only because protons are so slow at converting into deuterium that we are here at all.

Astrum Space
We're Close to Harnessing the Power of a Star

For fusion on Earth, on the other hand, it is bad news.