Let There Be Light! Royal Institution Christmas Lectures


Let There Be Light!

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Scientists have been giving lectures in this theatre

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for nearly 200 years, but 80 years ago, almost to the day,

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something special happened.

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Lecture one, The World Of Captain Gulliver.

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The BBC transmitted a Christmas Lecture

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using a brand-new technology - television.

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-Thank you.

-Science TV was born.

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So, to celebrate, we're recreating famous demonstrations

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and inviting Christmas Lecturers past to the stage to help out.

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The subject of these lectures goes back

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to their founder, Michael Faraday.

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It governs everything we do, from the nuclear furnace in the sun...

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..to the daily school run.

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It makes the whole universe tick

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and getting enough of it is one of the biggest challenges

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facing the whole human race. That subject is energy.

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Welcome to the 2016 80th Anniversary Christmas Lectures.

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APPLAUSE

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This lecture theatre consumes a huge amount of energy.

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We've got the lights,

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we've got the cameras and we've got some air conditioning, too.

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They're all energy guzzlers.

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We can see on our giant meter here...

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So this is no ordinary energy meter.

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We wanted to show you units of energy in a slightly different way.

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We're using AA batteries.

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So, how much do we need for this lecture theatre?

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So, running these lecture theatres requires...

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21,567 AA batteries.

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When I pull this lever here,

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all of that will be turned off.

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So tonight's challenge is,

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can we generate enough energy to power this lecture theatre?

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So along the way, I want to show you the amazing thing called energy.

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So, let's do a countdown.

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ALL: Three, two, one.

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So, this small candle is a good place to start.

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One of the greatest scientists, Michael Faraday,

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worked here at the Royal Institution.

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He gave Christmas Lectures on the chemistry of candles in this theatre

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around 150 years ago, and this is one of his favourite demonstrations,

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which I'm going to try and repeat.

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It's basically, can I relight that candle

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when I put it out without touching the wick?

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It's a bit tricky, but I'll try.

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OK. So...

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let's see.

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OK. You might have missed that - that was very quick -

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but fortunately we have that in slow motion.

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So let's see that in slow motion.

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So you can see the vapour there - that's the vapour -

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and it's going to relight...

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And look at that, it's going to relight the flame.

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So, what's happening there?

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Well, when you think of a candle,

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you think that actually it's the wick that's burning.

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That's not quite right.

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What's happening is that the wax vapour comes up off the candle

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and that is the chemical store.

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And if you time it right,

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you can actually relight the candle without touching the wick,

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as you saw in slow motion.

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So, it looks as if the wick is burning, but it's not, it's the wax.

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And the wax, as I said, is a great energy store.

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And this tells us a very important thing, a principle about energy -

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energy can never be created nor destroyed,

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it only converts from one form to another.

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In this case, the candle is converting

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the chemical energy in the wax to light and heat.

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There's another important principle.

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When energy is converted, we can actually use it to do work.

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And a simple example is again using this candle and a fan.

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OK, so...

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So if you see that, you can see that it's turning.

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So what's happening here is that the heat

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from the candle is rotating this fan.

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In fact, one definition of energy is the ability to do work.

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So, let's get back to our energy meter.

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How does the candle score?

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So, remember, to power our lecture theatre, we need to get up here.

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So, what does candle give us?

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OK, so we're going to see.

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It's going to drop down, drop down...

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OK. 31 AA batteries.

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Actually, it's more than I expected.

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We can see it's not going to be enough to power this lecture theatre.

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So we can scale up a candle to make it more powerful.

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OK, so...

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What we're coming on now...

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It's a very special candle.

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It's made of something called guncotton,

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which you can't get in the shops.

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OK? We're going to see if it's different from the earlier candle.

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Let's see how it does.

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AUDIENCE GASPS

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APPLAUSE

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Right, fortunately - I'm sure you all saw that -

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but what I love to see is in slow motion.

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OK, so we've got it in slow motion.

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So, let's have a look over here.

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So you can see there's the candle there, there's my long wick,

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and there you go.

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So, you might think that this candle has a lot more energy

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than that small candle over there.

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Actually, the difference isn't that much.

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And the reason is, the main difference is to do with power.

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Scientists are very careful about these two words.

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They want to distinguish the words power and energy.

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While both candles have about the same amount of energy,

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the guncotton candle, the one I just burnt,

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releases that energy all at once.

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It's a lot more powerful.

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So, power is simply how fast energy is transferred.

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So, I've already shown you that a candle stores chemical energy

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and it turns it into light and heat.

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But energy comes in loads of other different and amazing forms,

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and to help me explain this,

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it's a great pleasure to introduce a former Christmas Lecturer -

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Professor Richard Dawkins.

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APPLAUSE

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Hi there, Richard.

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Good to see you.

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Richard, it's a great pleasure and I'm glad you could join us

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for this 80th Anniversary Lecture.

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You did an experiment that I really enjoyed watching about 25 years ago,

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back in 1991, and we've got a clip here.

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I'm going to stand here and I'm going to release it,

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and it's going to come... It's going to go over there,

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and it's going to come roaring back towards me,

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and all my instincts are going to tell me to run for it.

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The whole principle is you can't gain energy,

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so it should swing back roughly to its original position.

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It can't go any further.

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But what do you remember about that experiment

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and why did you want to do it?

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Well, I think you're interested in conservation of energy.

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I was interested in showing my faith in science itself.

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As it were, putting if not my life on the line, my head on the line.

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So we're going to try and recreate it,

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but I have a confession, Richard.

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We have made a bit of a difference to the cannonball.

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We've added spikes.

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So we've put a bit of a target here and we're going to make sure

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it allows you to actually position your head perfectly.

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Right, so, we're going to have a bit of a drumroll this time.

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AUDIENCE DRUMROLLS

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Yes!

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APPLAUSE

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What I said last time was that I felt the wind of it and I did again

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this time, but I was told by Robert May,

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a very distinguished Australian scientist, that in Australia,

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when real men do that demonstration,

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they don't hold the cannonball to their head, they hold it down there.

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LAUGHTER

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-Thank you, Richard.

-OK.

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Let's thank Professor Richard Dawkins once again.

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APPLAUSE Thank you, Richard.

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That swinging ball shows that you can't destroy or create energy,

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but you can convert it from one form to another.

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So, energy comes in lots and lots of different forms and I want to give

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you... I didn't want to give you a long, boring list,

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so instead I thought we'd do something a bit more fun

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and this contraption

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right behind me is called a Rube Goldberg machine,

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and it's been painstakingly put together by my Royal Institution

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team over the last month or so.

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And it's a type of energy cascade and carries on outside this theatre.

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So, I need a volunteer from this side over here.

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OK, I'll rush over.

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OK, so, could you come over here?

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So, can I take your name first?

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-Sophie.

-Sophie, why don't you come on this side?

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So, let's take a seat there.

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We'll sit together. So, Sophie,

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what you're going to do is you're going to help me set off this

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Rube Goldberg machine by something I prepared earlier - this lovely ball.

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So if you just hold on to that and I'd like you to spot how many times

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energy changes from one form to another, OK?

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So we need a big countdown for this, OK?

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Give me a big countdown.

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ALL: Three, two, one.

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It goes. It's going fast.

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So, that is Jacob's Ladder with sparks.

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We've got the fan going off.

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We've got, hopefully, a little boat moving.

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Now, let's see.

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Amazing!

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OK? Let's see what's going to...

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It's going to go out of the lecture theatre.

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Here it goes. So look out for those conversions.

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OK, it knocks out... There's some kinetic energy.

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Elastic energy.

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Look at that. Down the corridor down there.

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There goes the car.

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Oh, the domino effect.

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This is one of my favourite bits, the wave.

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That's the wave there.

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So, plasma ball.

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This is a chemical reaction producing a fluorescent material.

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If you watch, it's going to go down this...

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circular wire. Look at that.

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And then...

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So, if you see, it's going to turn this bicycle wheel.

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And then it's going to pass that -

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that was a magnetic track.

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OK, let's see what's going to happen next.

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So, you can watch out for another chemical reaction.

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So this is out the side.

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It's going to knock over those balls.

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Hopefully it will set off...

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..that ball. It's going to come back, hopefully, very soon,

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through the corridor, through here.

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Back into here. Watch out for it.

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Yeah!

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APPLAUSE

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Yes...

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HE LAUGHS

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So, I gave you a test, or exam, at the beginning of that,

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in the number of energy conversions.

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So, does anybody have a guess of how many there were?

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Anybody shout out a number?

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15?

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20? So, who's going to go for 15?

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Who's going to go for 20?

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Who's going to go for a lot more?

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Well, the actual answer that we worked out

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was roughly about 111 different energy conversions.

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So...

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When we think about energy in our daily lives,

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we often think about one thing, and that's electricity.

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But we don't often see electricity in the raw,

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so I want to make electricity a bit more visible.

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So, could you please welcome Derek Woodroffe, electricity expert?

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I'll go around that side.

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Nice to see you, Derek.

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I love your contraptions here.

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I know they're two separate Tesla coils.

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They make people here at the Royal Institution a bit nervous.

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The last time they had a Tesla coil here in this lecture theatre,

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it fried all the fuses and it turned all the computer text German.

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LAUGHTER

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But these two Tesla coils are different.

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They've actually learned to play music, German music.

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So, Derek, take us away.

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If you could dim the lights as well.

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MUSIC PLAYS

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APPLAUSE

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Right, so what you've seen there is basically a flow of electrons.

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Electrons carry charge.

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So these Tesla coils build up a huge amount of electrons,

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or negative charge. There's such a big build-up of electrical charge

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it's released in a single burst of electricity, or spark,

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that turns air into a conductor.

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And where else do we see this?

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Well, as you can imagine, it's lightning.

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During pretty violent thunderstorms, you get that big build-up of charge.

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So, why are these ones a bit musical?

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Well, changing the frequency of the sparks means that these Tesla coils

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can play different notes.

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So I think we want to hear one more.

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HIGH-PITCHED MUSIC PLAYS

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LAUGHTER AND APPLAUSE

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Thank you, Derek.

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-Pleasure.

-And auf Wiedersehen.

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DEREK LAUGHS

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OK, so let's get back to electricity.

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Electrons always take the fastest route to where they want to go.

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Travelling through the air isn't easy for an electron.

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In contrast, travelling through metal is a lot easier.

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So if you create a metal pathway for the electrons,

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they should always follow it.

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I wanted to test this out,

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so I sent Christmas Lecturer Professor Monica Grady

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to the biggest Tesla coil we could find.

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Hello, Monica, over to you.

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Hi, Saiful, hi, everybody, and look what I've got here.

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It's a Tesla coil and it's much more powerful

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than the one you've seen operating already.

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I am going to get into this Faraday cage here.

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Now, a Faraday cage is named after Michael Faraday

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of Royal Institution fame.

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How it works is the current passes across the wire

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and it doesn't go into the cage.

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So I will be quite safe sitting in there,

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but I'm still going to wear my wellingtons when I get inside,

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just in case.

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Right, well, I'm going to be locked in in a minute.

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It does feel a bit bizarre.

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But what I've got here is I've got a safety pad,

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and that goes under my foot.

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And while my foot is on it, the discharge will work.

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As soon as I take my foot off, everything stops.

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That's part of the safety apparatus.

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I've been instructed not

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to try to put my finger through any of the holes,

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definitely not to touch the wire and, just for once in my life,

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I'm going to be very, very, very obedient.

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Don't like this.

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I think it's better if we get it over with soon.

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So, take it away, Colin.

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Wow, that was stupendous!

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It's one of the really bizarrest

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experiences I've ever had.

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It was just really, really strange.

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And I never felt a thing!

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APPLAUSE

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I have to thank Monica - rather her than me!

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If you don't know about the science,

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you might think that this was very dangerous.

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I can safely predict that you've all been inside a Faraday cage.

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All the metal cars

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that you've driven in or been in, they are Faraday cages.

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That's good to know if you've ever been in thunderstorms.

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So, these Tesla coils have been great,

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but the electricity they produce is just an uncontrolled burst,

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an uncontrolled spark.

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So what we need is a smooth, steady flow of electrons,

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so we're going to have to find another way to power our theatre.

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We need an electrical generator.

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So, this brings us back to Michael Faraday,

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the founder of the Christmas Lectures, and, actually,

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he's one of my scientific heroes.

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He came from very humble beginnings rather than the wealthy elite,

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but he went on to discover a huge amount

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about the fundamental nature of electricity.

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So, one of his inventions was this strange contraption coming in here.

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It may look a bit like a burnt sausage...

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..but actually, this is one of the treasures of the Royal Institution.

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And our curator, Charlotte - thank you, Charlotte, for coming in -

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is going to hold it for me.

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I'm not allowed to touch it. So, believe it or not, this thing here,

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this tiny machine, totally transformed the way we live.

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It was the spark that ignited the electric revolution

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and it's really the first electrical generator.

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So, how does it work?

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Well, what it's made up of is it's got this metal, magnetic rod,

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as you can see there, and it's actually covered

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by these copper wires.

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And as you move the metal rod in and out through there...

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..that magnetic energy and that movement generates electricity.

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So it's an energy conversion.

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So machines based on this simple contraption power the modern world.

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So, thank you, Charlotte.

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So, how does a modern electrical generator work?

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So let me show you

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through this contraption here.

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So, before, that... The one that Charlotte brought in

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was a static ring where the metal rod went in and out.

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Here, and if the cameras can get close,

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you can see now we've got these copper wires again,

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but this time the magnet is rotating.

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I'll show you it slowly first.

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You can see the red and the greys.

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So let's rotate. But if you spin it fast...

0:23:300:23:33

..you can actually begin to generate electricity by that magnetic energy

0:23:360:23:41

and that movement. And since it's moving continuously,

0:23:410:23:44

it's much faster, it's much more powerful.

0:23:440:23:47

So, this is the basis of almost all modern electricity generation.

0:23:470:23:52

But I'm not muscular enough to actually turn this, so I need

0:23:520:23:57

somebody a bit more muscular.

0:23:570:23:59

I need a volunteer.

0:23:590:24:02

So, the one in green.

0:24:020:24:03

Yes. Come on down.

0:24:030:24:05

APPLAUSE

0:24:050:24:07

Hello, there. Can I take your name first?

0:24:070:24:10

-Daniel.

-Daniel. Well, thanks for coming down.

0:24:100:24:13

What I'm going to try and get you to do is that we've got some lights

0:24:130:24:18

here, so don't start yet.

0:24:180:24:19

We've got some lights here and by turning on each one,

0:24:190:24:24

it kind of increases what's called the load,

0:24:240:24:27

it kind of gets more difficult.

0:24:270:24:29

So if you turn it now, you find it's quite easy, isn't it?

0:24:290:24:32

It's not too bad. So let's see if you can do the bottom one.

0:24:320:24:35

Let's do that one. And then the other ones.

0:24:350:24:38

You've got that one.

0:24:380:24:41

Just a bit faster. I think you can do it.

0:24:420:24:45

That's it, you've got them.

0:24:460:24:48

Right, great. Well done.

0:24:480:24:50

APPLAUSE

0:24:500:24:51

Thank you, Daniel. Go back up there, thank you.

0:24:510:24:54

So, Daniel there converted his muscular energy into kinetic energy

0:25:000:25:05

and into electrical energy. So, let's go to our...

0:25:050:25:08

This energy meter again, the kind of scores on the doors.

0:25:080:25:13

So, this is our target.

0:25:130:25:15

How much has that hand-cranked generator given us?

0:25:150:25:19

Unfortunately, a measly 12 AA batteries, OK?

0:25:200:25:25

So, even if Daniel was at that for a long, long time,

0:25:250:25:29

he wouldn't really generate enough to power this lecture theatre.

0:25:290:25:33

But can we use this principle to get us closer to our target?

0:25:330:25:39

And here I need two more volunteers.

0:25:390:25:43

OK, the one at the end there, and if you wanted to come down.

0:25:430:25:47

OK? If you want to come down.

0:25:470:25:49

APPLAUSE

0:25:490:25:50

-Can I take your name?

-I'm Dan.

-Dan?

-Alex.

-Alex.

0:25:500:25:53

OK, so, we're going to send you on a bit of a journey.

0:25:530:25:57

Not too far, it's just a journey within the Royal Institution.

0:25:570:26:01

So if we could have a couple of our production team to take you away.

0:26:010:26:06

OK, Dan and Alex, thank you.

0:26:060:26:08

So, over the past few weeks,

0:26:100:26:14

my team here has rigged the Royal Institution with lots of different

0:26:140:26:20

types of energy generators

0:26:200:26:24

and thrown in some newer technologies, as well.

0:26:240:26:27

So, as you came into the building -

0:26:270:26:30

I don't know if you noticed - you went over a very special floor.

0:26:300:26:34

It generates electricity out of your footsteps

0:26:340:26:38

and it works a lot like a Faraday's generator.

0:26:380:26:41

So I think we've got some footage. So there - that's the one.

0:26:410:26:44

You see, those steps were pushing magnets into copper coils,

0:26:440:26:50

so it's a bit like the electrical generators I showed you as a display

0:26:500:26:53

and that rod, and it generates a small electric current.

0:26:530:26:57

So, how much energy or electricity did it generate?

0:26:570:27:00

So, let's go back to our energy meter.

0:27:000:27:02

So, it was just for over a week.

0:27:020:27:05

If it comes down...

0:27:050:27:07

Erm... Yes.

0:27:090:27:12

Just one AA battery. We didn't cover a large area -

0:27:120:27:15

obviously a large area would have done a lot better.

0:27:150:27:18

So, up on the roof, you may not believe it,

0:27:180:27:21

but we've actually got a fully functional wind machine

0:27:210:27:25

and wind turbine attached. And that is a live shot right now,

0:27:250:27:29

and you can see it's been raining. I don't know if some of you noticed.

0:27:290:27:32

So that is a live shot of that wind turbine.

0:27:320:27:35

So, is it Alex or Dan up there?

0:27:350:27:37

All right, great, we can see Alex coming.

0:27:370:27:40

-Careful.

-OK, she's coming up the ladder.

0:27:400:27:42

-And, Alex, can you hear me?

-Yeah.

-Oh, great.

0:27:420:27:46

So, we've got that wind turbine up there.

0:27:460:27:48

Can you go and see if you can find out what the reading is from the wind turbine, OK?

0:27:480:27:52

-Four kilowatt-hours.

-Four kilowatt-hours?

0:27:520:27:56

OK, well, thank you, Alex.

0:27:560:27:58

If you want to make your way down, OK? Thank you.

0:27:580:28:01

APPLAUSE

0:28:010:28:03

OK, she said four kilowatt-hours.

0:28:080:28:10

We can actually try and convert that into our energy meter,

0:28:100:28:13

which means we want to do that in AA batteries, OK?

0:28:130:28:15

So let's see what that value is. So, this is our target.

0:28:150:28:19

It's coming down. This is our wind turbine.

0:28:190:28:22

1,569 AA batteries.

0:28:220:28:28

So not too bad, and it wasn't up there for too long.

0:28:280:28:32

We've, finally, sent Dan to the men's toilet.

0:28:320:28:38

Last week we installed a special cell

0:28:380:28:41

that converts wee into electricity.

0:28:410:28:44

So it's wee power.

0:28:440:28:46

So you can see that time-lapse,

0:28:460:28:48

you can see it being installed in one of the toilets upstairs here

0:28:480:28:52

at the Royal Institution. So, we've got Dan here.

0:28:520:28:55

So, Dan, again we've got a reading for how much energy

0:28:550:28:59

that produced from that microbial fuel cell.

0:28:590:29:03

-OK.

-Tell us.

-So, we've got 3.78 at the moment.

0:29:030:29:08

3.78. OK, thank you. Why don't you make your way back here?

0:29:080:29:11

OK, thank you, Dan. APPLAUSE

0:29:110:29:14

So, I want to say a bit more about that fuel cell.

0:29:220:29:25

It's called up microbial fuel cell.

0:29:250:29:27

What it does is it uses bacteria to convert wee into electricity.

0:29:270:29:33

So, all the guys at the Royal Institution

0:29:330:29:36

have been told to use that urinal.

0:29:360:29:38

So, how much energy have we generated from using pee power?

0:29:380:29:43

So let's go back to the meter.

0:29:430:29:46

As usual, the target, and it goes down to...

0:29:460:29:50

..two.

0:29:520:29:54

A wee amount, yes.

0:29:540:29:55

LAUGHTER

0:29:550:29:57

So, that's just two AA batteries.

0:29:570:30:00

So, many of these methods of generating electricity -

0:30:000:30:02

particularly things like wind power - are what we call renewable,

0:30:020:30:07

and that means that the energy is supplied from sources

0:30:070:30:10

that are naturally replenished.

0:30:100:30:12

At the moment, they just aren't

0:30:120:30:15

giving us enough energy by themselves.

0:30:150:30:18

That's true for the lecture theatre

0:30:180:30:20

and it's true for the whole of the UK.

0:30:200:30:23

So that means we still get about 50% of our energy

0:30:230:30:27

or electricity from fossil fuels.

0:30:270:30:30

So these are fossil fuels such as...

0:30:300:30:33

Such as coal and oil.

0:30:340:30:37

This is a bit of a dodgy oil - it tells pretty rude jokes.

0:30:380:30:41

It's called crude oil.

0:30:410:30:43

But also, another fossil fuel is methane.

0:30:450:30:49

So, why do we use fossil fuels?

0:30:500:30:53

Well, two main reasons.

0:30:530:30:55

First, they contain a lot of energy.

0:30:550:30:58

Ooh, that was great.

0:31:020:31:04

So, let's see that in slow motion.

0:31:100:31:12

So you can see, there's the balloon, there's the flame.

0:31:120:31:16

And what's interesting is you see the plastic balloon going off first,

0:31:160:31:20

before you see any ignition of the methane,

0:31:200:31:24

but it'll happen in a minute. There it goes. There it goes.

0:31:240:31:27

So that's what I call a real flame.

0:31:320:31:34

There's another reason behind why we use fossil fuel -

0:31:340:31:38

is that it's buried under our feet, so we can actually get to it.

0:31:380:31:43

But how do we turn that fossil fuel into electricity?

0:31:430:31:47

Well, there's something I've prepared earlier to help me explain.

0:31:470:31:50

It might not look like it, but this is a fossil-fuel power station.

0:31:510:31:57

OK? Well, what we've got here is

0:31:590:32:02

we've got water in this pan and underneath

0:32:020:32:05

we've got the burning fossil fuel - in this case, natural gas.

0:32:050:32:09

And what it's going to do is, that steam from the water

0:32:090:32:14

is going to turn this fan here,

0:32:140:32:18

and that fan is very close to the electrical generator.

0:32:180:32:22

So you can see the coils here.

0:32:220:32:25

It's a bit like the generator we saw earlier.

0:32:250:32:27

And hopefully it will... Just by steam...

0:32:270:32:31

..it will light up these lights here.

0:32:330:32:35

Yes, so you can see there, lights going on.

0:32:350:32:38

And that's just from steam.

0:32:390:32:43

So, in a sense, all power stations can be viewed as giant kettles.

0:32:440:32:49

The only difference is how we boil the water - either coal or gas.

0:32:490:32:55

And in nuclear power stations,

0:32:550:32:58

the heat is from splitting up atoms - usually uranium.

0:32:580:33:03

So, massive power stations like these generate electricity for

0:33:030:33:09

the majority of the world's population.

0:33:090:33:11

I would call them masterpieces of engineering,

0:33:110:33:14

but we rarely see inside them.

0:33:140:33:16

In a way, we take them for granted

0:33:160:33:17

because they generate our electricity.

0:33:170:33:19

So I asked another Christmas lecturer, Professor Tony Ryan,

0:33:190:33:23

to go behind the scenes at Britain's biggest power station.

0:33:230:33:27

Hello, Saiful. Hello, kids in the audience.

0:33:280:33:31

I'm here at Britain's biggest power station.

0:33:310:33:34

It's called Drax and it's enormous.

0:33:340:33:37

I want to show you how it works and how it scales up from the model you

0:33:370:33:41

have in front of you in the theatre.

0:33:410:33:43

The noise in here is incredible.

0:33:490:33:52

There are six generators, each with five turbines.

0:33:520:33:56

They generate enough power for a million households.

0:33:560:34:00

That's the most energy generated anywhere in the UK.

0:34:000:34:05

And the turbines work just like you've seen in the lecture theatre -

0:34:050:34:09

energy gets converted into heat, heat into motion,

0:34:090:34:13

motion into electricity.

0:34:130:34:15

You can't see the turbines themselves

0:34:150:34:17

cos they have to keep running so the lights stay on,

0:34:170:34:20

but we will go look in one that's been taken apart.

0:34:200:34:24

Wow! This is enormous!

0:34:320:34:34

So, this is Steve Austin, the chief turbine engineer.

0:34:350:34:38

So, Steve, how fast does this go round?

0:34:380:34:42

This will spin at 3,000 rpm, or 50 times a second.

0:34:420:34:46

The blade tips, they will spin at 1,250 mph,

0:34:460:34:50

which is 1.6 times the speed of sound.

0:34:500:34:52

And how often do you have to look inside them to make sure everything's OK?

0:34:520:34:56

Well, we run for eight years in between inspections,

0:34:560:34:59

but this turbine in particular has run for 34 years,

0:34:590:35:02

which is about 270,000 hours in service.

0:35:020:35:05

For most of its life, Drax burned coal.

0:35:080:35:12

But we're going to stop using coal

0:35:120:35:14

for power in the UK over the next ten years.

0:35:140:35:17

So Drax has switched to using these - compressed biomass pellets -

0:35:170:35:22

and they're stored in these massive domes

0:35:220:35:25

that are bigger than the Albert Hall.

0:35:250:35:27

Up and down the country,

0:35:270:35:29

huge power stations like this are keeping the lights on,

0:35:290:35:33

the ovens cooking, the homes heated,

0:35:330:35:36

all operating on the same principles identified by Michael Faraday

0:35:360:35:41

over 200 years ago.

0:35:410:35:42

OK, thank you, Tony, for that.

0:35:510:35:53

As we know, burning fossil fuels is a major problem in terms of

0:35:530:35:59

releasing carbon dioxide, which contributes to global warming.

0:35:590:36:04

But right now, fossil fuels are

0:36:040:36:06

still a very useful source of energy.

0:36:060:36:08

So, where do fossil fuels get their energy from?

0:36:080:36:11

Millions of years ago,

0:36:110:36:14

coal, oil and gas

0:36:140:36:17

used to be living things - plants and animals.

0:36:170:36:21

And these plants and animals got their energy from the sun.

0:36:210:36:26

So in the very long term, fossil fuels are essentially...

0:36:260:36:30

..solar-powered. And this begs the question -

0:36:310:36:35

where does the sun get its energy from?

0:36:350:36:38

Right at the start of the lecture,

0:36:380:36:40

we defined energy as the ability to do work.

0:36:400:36:44

But there's another way to define energy,

0:36:440:36:46

through the most famous equation of all time.

0:36:460:36:50

Anyone know what that equation is?

0:36:500:36:53

-AUDIENCE:

-E=mc squared.

0:36:530:36:56

E=mc squared. There we have it there.

0:36:560:37:00

E is for energy, m is for mass

0:37:010:37:06

and c is a huge number -

0:37:060:37:09

the speed of light.

0:37:090:37:11

This was formulated over a century ago by one of the most famous

0:37:110:37:15

scientists of all time, Albert Einstein.

0:37:150:37:18

This famous equation tells us a very important fact -

0:37:190:37:25

mass, the stuff that makes up the whole world, makes us up,

0:37:250:37:29

is equivalent to energy.

0:37:290:37:31

They are interchangeable - just different forms.

0:37:320:37:35

This tells us a tiny amount of mass contains

0:37:350:37:39

a colossal amount of energy.

0:37:390:37:41

So I was racking my brain, trying to find a good way of visualising this,

0:37:440:37:49

and we've done some very complicated calculations.

0:37:490:37:52

We've come up with the most sophisticated example.

0:37:520:37:55

My pants.

0:37:570:37:58

You'd be amazed at how much energy there is in these pants.

0:38:000:38:06

According to that famous equation we just said - E=mc squared -

0:38:060:38:10

they contain enough energy to power the city of Birmingham.

0:38:100:38:14

Lucky Birmingham! So, er, let's put it there.

0:38:160:38:19

So let's put it to the test.

0:38:190:38:22

We're going to burn those pants and there is a scientific term for it -

0:38:220:38:27

it's called burn, pants, burn.

0:38:270:38:30

And let's see, OK?

0:38:320:38:35

Right. We're going to...

0:38:350:38:37

Just to speed up the reaction, we're going to use some liquid oxygen...

0:38:370:38:41

..and just to see the effects. So let me get this going.

0:38:430:38:47

Yeah, I never liked those pants, actually, so...

0:39:030:39:06

So, is that enough energy, do you think, to power Birmingham?

0:39:080:39:12

I don't think so.

0:39:140:39:15

So, in scientific terms, we call that liar, liar, pants on fire.

0:39:150:39:19

And that's because the energy in those pants is hard to get at.

0:39:210:39:25

My pants are hard to get at, as well!

0:39:260:39:29

Simply setting them on fire...

0:39:290:39:31

..only releases the energy of the bonds holding the atoms together.

0:39:330:39:38

So if you really want to power Birmingham,

0:39:380:39:41

the atoms need to undergo a series of nuclear reactions,

0:39:410:39:46

either to split them or fuse them together.

0:39:460:39:49

It's only then that the mass releases that vast amount of energy

0:39:500:39:56

we saw from our equation, E=mc squared.

0:39:560:39:59

So, this helps us understand why the sun is so powerful.

0:39:590:40:04

It's converting

0:40:050:40:07

enormous amounts of mass all the time - mostly hydrogen -

0:40:070:40:12

into vast amounts of raw energy in the form of heat and light.

0:40:120:40:16

It's actually the biggest energy converter in the whole solar system.

0:40:170:40:22

So, can we do the same thing here on Earth?

0:40:230:40:27

And the simple answer is, yes, we can.

0:40:270:40:30

What we're seeing here...

0:40:300:40:32

..works on the same principle.

0:40:340:40:36

It's basically converting the mass of hydrogen directly into energy.

0:40:360:40:41

It's a hydrogen bomb,

0:40:410:40:44

the most destructive weapon in the world.

0:40:440:40:47

But there is hope that we can carry out a more controlled version of

0:40:480:40:52

this reaction we've just seen, and it's called nuclear fusion.

0:40:520:40:56

So, what is nuclear fusion?

0:40:570:40:58

To help me answer that question, I'd like you to welcome,

0:41:000:41:02

from the UK Atomic Energy Authority, Professor Ian Chapman.

0:41:020:41:05

-Hello, Ian.

-Hi, Saiful, how are you?

0:41:100:41:12

Thank you for joining us, Ian.

0:41:140:41:17

This is a very interesting contraption.

0:41:170:41:19

I know it's related to nuclear fusion.

0:41:190:41:20

Tell us a bit more.

0:41:200:41:22

So, to get nuclear fusion to happen here on earth

0:41:220:41:25

we have to get the fuel incredibly hot,

0:41:250:41:27

sort of "ten times hotter than the centre of the sun" hot.

0:41:270:41:31

So this... Obviously, we're not doing that here,

0:41:310:41:33

but this is a demonstration of what happens when we do do that.

0:41:330:41:37

So when we put the fuel under these incredibly intense temperatures,

0:41:370:41:41

you make the fuel very energetic and when you do that,

0:41:410:41:45

the ions and electrons which are inside the gas separate.

0:41:450:41:48

So you separate those charged particles

0:41:480:41:50

and that gives you a plasma,

0:41:500:41:52

and that's what you can see inside this cage in here.

0:41:520:41:55

So this sort of beautiful cloud, this ball of light, is a plasma.

0:41:550:41:58

OK, you've mentioned the word "plasma". So, what is plasma?

0:41:580:42:01

So, plasma is the fourth state of matter.

0:42:010:42:03

So you have solid, then a liquid, then a gas, and then a plasma.

0:42:030:42:07

And a plasma is essentially a very energetic gas, where you've

0:42:070:42:10

heated up the gas to extreme energies

0:42:100:42:12

and the ions and the electrons have separated,

0:42:120:42:14

so you have a charged ball of ionised gas.

0:42:140:42:17

You've brought us another interesting contraption here.

0:42:170:42:21

I understand that plasma isn't easy to control,

0:42:210:42:25

so how do you control plasma?

0:42:250:42:26

That's exactly the difficulty with having fusion reactors,

0:42:260:42:29

is controlling the plasma. So again,

0:42:290:42:31

we're going to spark a current through this tube and once again

0:42:310:42:35

we have this plasma.

0:42:350:42:36

But because the plasma is charged, so you have ions and electrons here,

0:42:360:42:40

it will feel a magnetic field. So I have a simple magnet.

0:42:400:42:42

If I put the magnet near it,

0:42:420:42:44

you can see how the plasma is reacting to the magnet -

0:42:440:42:47

it moves because the magnetic field is near it.

0:42:470:42:50

So let me have a go at that. It looks really good. So, basically,

0:42:500:42:53

you're just using the fact that it's charged to control it with this kind

0:42:530:42:58

of magnetic field, or a strong magnet.

0:42:580:43:00

Exactly, and that's how you would go about building a fusion reactor,

0:43:000:43:03

because, as I said, you have a fuel which is incredibly hot,

0:43:030:43:06

so you need to keep it away from the wall of the reactor.

0:43:060:43:09

And we do that by creating a sort of magnetic cage,

0:43:090:43:11

a magnetic bottle to hold the fuel in.

0:43:110:43:14

OK. Will we see a nuclear fusion reactor very soon?

0:43:140:43:19

That's what we're hoping for.

0:43:190:43:20

So we're building a machine in the south of France right now.

0:43:200:43:23

That will be a proof of principle.

0:43:230:43:25

It will get ten times the amount of energy out that we put in to get

0:43:250:43:28

the reaction going in the first place,

0:43:280:43:30

on a sort of 500-megawatt scale,

0:43:300:43:32

and soon thereafter we hope to be building reactors.

0:43:320:43:34

-Great. Well, thank you, Ian Chapman.

-Thank you.

0:43:340:43:37

APPLAUSE

0:43:370:43:39

So, fusion works on a large scale.

0:43:430:43:47

It could mean unlimited quantities of electricity with hardly any

0:43:470:43:52

carbon emissions. Obviously,

0:43:520:43:54

this is a scientific challenge and it will take years to crack.

0:43:540:43:58

So let me return to that giant nuclear furnace in the sky, the sun,

0:43:580:44:03

the light that never goes out.

0:44:030:44:05

So, did you know that in just two hours,

0:44:070:44:10

enough energy from the sun hits the Earth to power human activity

0:44:100:44:16

for a whole year?

0:44:160:44:18

We can already convert the sun's energy

0:44:180:44:21

directly into electricity using...

0:44:210:44:23

..solar panels.

0:44:240:44:26

And this is something I'm really excited about -

0:44:260:44:28

it's one of my research areas.

0:44:280:44:30

So for this next bit, I need a volunteer,

0:44:300:44:34

and somebody who is not scared of heights.

0:44:340:44:37

OK, I should come over to this side. I haven't been over there.

0:44:370:44:39

So, yeah, do you want to come through? Come on.

0:44:390:44:42

Hello. Hello, there.

0:44:470:44:48

-Can I take your name?

-Natasha.

0:44:480:44:50

Natasha. This is Natasha.

0:44:500:44:52

So, Natasha, I asked about scared of heights

0:44:520:44:54

because you're going on a journey, as well.

0:44:540:44:57

So, one of the production team is going to take you off

0:44:570:45:00

to look at some interesting technology, OK?

0:45:000:45:02

So, back to our big challenge.

0:45:020:45:04

Can we power this lecture theatre?

0:45:040:45:09

I've covered the roof of the Royal Institution with solar panels.

0:45:090:45:13

So this is actually a live shot. And it is live, you can tell -

0:45:130:45:17

it's raining, covered in water - and they've been plugged into a battery.

0:45:170:45:22

So there's the battery, and that's the live shot, looking very wet.

0:45:220:45:26

And that line there...

0:45:260:45:28

..has gone down and it's come into this lecture theatre.

0:45:290:45:33

And that is the line.

0:45:330:45:35

So we're going to try and test it out.

0:45:350:45:37

Let's see if our volunteer, Natasha, has got up to the roof.

0:45:370:45:41

OK, here comes Natasha.

0:45:410:45:42

She's on the roof and we're going to

0:45:420:45:45

try and get a reading of our battery.

0:45:450:45:48

Natasha, can you hear me?

0:45:480:45:49

-Yes, I can.

-OK.

0:45:490:45:51

-So, can you give us a reading from that battery?

-Certainly.

0:45:510:45:55

The power is...

0:45:560:45:58

110, and that's 4.7 kilowatt-hours.

0:45:580:46:02

And do you want to read us the number below that, as well?

0:46:020:46:06

That's 97%.

0:46:060:46:07

OK. Well, thank you, Natasha.

0:46:070:46:09

I think you deserve to come back out of the wind and rain.

0:46:090:46:11

OK, thank you.

0:46:110:46:13

Let's give us our reading on our energy meters.

0:46:180:46:20

We've got a couple of readings.

0:46:200:46:22

So, that was our target...

0:46:220:46:24

..and we're down to...

0:46:250:46:26

..2,314 AA batteries

0:46:280:46:33

from those solar panels.

0:46:330:46:35

OK, and by the way, I've used a small bit of electricity to make

0:46:360:46:39

a solar-powered snack.

0:46:390:46:42

So watch this.

0:46:420:46:43

Very burnt toast.

0:46:450:46:47

See? But that was directly from

0:46:470:46:49

the solar panels hooked onto that battery and down here.

0:46:490:46:53

So, those panels up there are made of silicon,

0:46:540:46:58

but take a look at these.

0:46:580:47:01

These are next-generation solar panels, solar materials.

0:47:010:47:06

As you can see, much more flexible. A bit lighter, as well.

0:47:060:47:10

And they're made of much more exotic materials -

0:47:100:47:15

copper, indium, gallium and selenium.

0:47:150:47:19

And we're going to hook them up...

0:47:200:47:22

I'm just going to put this down here.

0:47:220:47:24

OK? We're going to hook them up

0:47:280:47:30

to this electric spark generator.

0:47:300:47:35

And what the solar panel here will do

0:47:350:47:38

is try and generate electricity directly.

0:47:380:47:42

And what we need is some - obviously - light,

0:47:420:47:45

light directly onto those panels.

0:47:450:47:48

And in this case, we've got a couple of lamps there.

0:47:480:47:52

So we need the lights on, OK?

0:47:520:47:54

And I'm going to turn this.

0:47:540:47:55

So we can probably dim the lights a bit.

0:47:580:48:00

Yeah?

0:48:050:48:07

So we've done it - we've got some sparks flying

0:48:070:48:10

just from this panel here and a couple of lights.

0:48:100:48:13

And the lights off, and it stops.

0:48:130:48:16

So, basically, it wouldn't work without that light energy.

0:48:160:48:20

So, new, exotic materials and new-generation panels like this

0:48:220:48:25

are really changing how we can use solar design.

0:48:250:48:29

So, how much of the sun's energy can solar panels harness?

0:48:290:48:33

To understand that, we need to understand light.

0:48:330:48:36

Sunlight isn't made up of just one colour -

0:48:360:48:39

it's made up of lots of different colours, all mixed together.

0:48:390:48:43

To show you this, I've got a very bright light to simulate the sun.

0:48:430:48:47

It's got a special filter that splits light

0:48:470:48:50

into its component parts.

0:48:500:48:52

So each one of these colours carries a certain amount of energy.

0:48:520:48:56

So this is split up, so you can see this here.

0:48:560:48:59

That's like a typical rainbow that you see and we are unweaving

0:48:590:49:04

the rainbow there. But, for this,

0:49:040:49:07

the data on that computer actually is going to read out the different

0:49:070:49:11

energy levels. But, for that, we do need a volunteer.

0:49:110:49:15

So, can I take your name?

0:49:150:49:16

-Tess.

-Tess.

0:49:160:49:17

So, Tess, when I ask you to,

0:49:170:49:19

can you shout out the numbers that you see on that computer screen?

0:49:190:49:23

Is that OK? Great.

0:49:230:49:24

So, what we have here is a solar panel a bit like the ones on

0:49:240:49:27

the roof that you saw earlier. And what it does - it's very clever -

0:49:270:49:30

it tells us the different energy levels across that spectrum.

0:49:300:49:35

And what it's trying to show us is that there are different energies

0:49:350:49:39

within the different colours.

0:49:390:49:41

So let's see what we get from the readout.

0:49:410:49:43

I'm going to start at the blue end, since I'm on this side here.

0:49:430:49:46

So, Tess, if you could start telling us some values.

0:49:460:49:49

So it starts off probably at zero, so what have you got at the moment?

0:49:490:49:53

-Eight.

-Eight, OK.

0:49:530:49:55

So let me move along a bit further.

0:49:550:49:57

10. 14.

0:49:580:50:00

14? So already, when we're getting towards the kind of greeny colour,

0:50:000:50:04

we're getting to 14. OK. How about around yellow?

0:50:040:50:07

-What have we got for yellow?

-12.

0:50:070:50:09

12. OK, we're going towards orange.

0:50:090:50:12

-Ten.

-Ten, and now the red end, right down here...

0:50:120:50:17

-Six.

-Six.

0:50:170:50:19

So you can see straightaway that all the numbers,

0:50:190:50:22

in a very general way, are not the same.

0:50:220:50:24

So, solar panels can't capture all wavelengths of light -

0:50:270:50:32

they stop working at certain regions in the spectrum,

0:50:320:50:36

depending on the material they're made of.

0:50:360:50:39

Tackling this issue is one of the big challenges

0:50:400:50:44

of solar-cell design.

0:50:440:50:46

It's one of my research areas, as well.

0:50:460:50:48

But compared to most other things,

0:50:490:50:52

solar cells are still very efficient.

0:50:520:50:55

They can already do some pretty amazing things.

0:50:550:50:59

I want to show you one of my favourites -

0:50:590:51:02

a plane powered using nothing but energy from the sun.

0:51:020:51:08

So we're going to speak to the two pilots of this plane,

0:51:080:51:12

Bertrand Piccard and Andre Borschberg, right now,

0:51:120:51:16

on the line from Switzerland.

0:51:160:51:17

Yes, hello from Switzerland.

0:51:190:51:20

Landing now at BBC.

0:51:220:51:23

Thank you for joining us, Andre. Thank you for joining us, Bertrand.

0:51:250:51:29

With pleasure.

0:51:290:51:30

Tell us how far you've got with your solar-powered plane.

0:51:300:51:32

With Solar Impulse, we went the furthest we could go.

0:51:320:51:35

That means all around the world.

0:51:350:51:38

Tell us a bit about the plane itself.

0:51:380:51:40

So, imagine the task for the engineers that were led by Andre,

0:51:400:51:45

to make a plane that was the size of

0:51:450:51:49

a jumbo jet, 236 feet wingspan,

0:51:490:51:53

and the weight of a family car - two tonnes.

0:51:530:51:55

It's really, absolutely amazing.

0:51:550:51:57

Nobody thought we could do it.

0:51:570:51:59

But if you are a pioneer, an explorer,

0:51:590:52:02

you don't listen to people who say it's impossible.

0:52:020:52:05

You use their scepticism as a motivation,

0:52:050:52:09

as a stimulation, to prove that you can do it.

0:52:090:52:12

What was the toughest part of the journey?

0:52:120:52:14

But of course, for us, the difficulty

0:52:140:52:16

and the challenge was to fly over the ocean.

0:52:160:52:19

We flew over land with the first airplane,

0:52:190:52:21

so I think we knew how to fly such an airplane,

0:52:210:52:24

but to go over the ocean for many days, many nights,

0:52:240:52:27

we didn't know if the airplane would be able to make it,

0:52:270:52:30

we didn't know if we could forecast the weather well enough,

0:52:300:52:32

and of course, we didn't know if

0:52:320:52:33

a pilot in fact could sustain such a long flight.

0:52:330:52:36

Because you have to understand that it's an aeroplane that can

0:52:360:52:39

fly forever, at least theoretically.

0:52:390:52:42

The sun is charging the batteries

0:52:420:52:44

and running the motors during the day flight,

0:52:440:52:46

in order to fly through the night with the batteries

0:52:460:52:49

and reach the next sunrise.

0:52:490:52:51

So my flight from America to Europe across the Atlantic

0:52:510:52:55

was three days and three nights and, for all this time,

0:52:550:52:58

you have to be like in the science-fiction film -

0:52:580:53:01

you look at the sun, you look at your electric motors turning,

0:53:010:53:05

you think, "Wow! That's the future. That's a fairy tale."

0:53:050:53:08

No fuel, no pollution, no noise, flying forever.

0:53:080:53:12

And it's not the future.

0:53:120:53:13

What is magic with clean technologies

0:53:130:53:16

is that it is the present.

0:53:160:53:17

It's what is allowed now by renewable energies.

0:53:170:53:21

So we currently see planes carrying 200 to 300 people.

0:53:210:53:25

Do you ever see a time when

0:53:250:53:26

solar-powered planes could do the same?

0:53:260:53:28

I would be crazy to answer "yes" and stupid to answer "no",

0:53:280:53:33

because today we don't have the technology for that,

0:53:330:53:36

but Charles Lindbergh neither had the technology to do it

0:53:360:53:39

when he crossed the Atlantic in 1927 and, nevertheless, it happened.

0:53:390:53:44

Thank you, Andre. Thank you, Bertrand.

0:53:440:53:47

Bye-bye for now.

0:53:470:53:48

-With pleasure. Bye-bye.

-Bye-bye. Take care.

0:53:480:53:52

Solar power is unlikely to give us all the energy in the UK because

0:54:030:54:07

we have a limited land space.

0:54:070:54:09

And it's a challenge during the winter months -

0:54:090:54:12

at least here in northern Europe - but with more research,

0:54:120:54:16

they will play a bigger role in the future.

0:54:160:54:19

So, finally, let's return to our big question -

0:54:190:54:23

can we power the lecture theatre using the mix of energy sources

0:54:230:54:28

that we've generated here?

0:54:280:54:30

OK, so, there's only one way to find out, as ever,

0:54:320:54:35

and that is to look at our scores on our energy meter.

0:54:350:54:38

So, let's have a final drumroll, please.

0:54:380:54:42

Come on, give us a big drumroll.

0:54:420:54:44

Let's see how far we got.

0:54:470:54:48

So, first, our candles.

0:54:480:54:51

And it was a little blip.

0:54:530:54:56

What about our special floor?

0:54:560:54:58

Tiny. Our wind turbine?

0:55:000:55:03

A bit better. Our wee power?

0:55:050:55:07

Yeah, a drip, really, isn't it?

0:55:090:55:12

And lastly, our solar panels.

0:55:120:55:14

There.

0:55:150:55:17

And that gives us a total of 3,937 AA batteries.

0:55:170:55:23

Well, even with all that clever equipment, we've not made it.

0:55:260:55:30

That's because this lecture theatre, and society as a whole,

0:55:300:55:34

is incredibly energy hungry.

0:55:340:55:36

To reach the target in a week,

0:55:370:55:39

we'd have to use nine times as many solar panels,

0:55:390:55:43

or 14 wind turbines on the roof.

0:55:430:55:46

Unless, of course, we unlocked the energy in these -

0:55:470:55:52

my pants - through nuclear fusion.

0:55:520:55:55

That would light up the whole of Piccadilly.

0:55:550:55:59

I'm optimistic the energy gap will be filled.

0:55:590:56:03

And as this is our 80th anniversary, I want to celebrate.

0:56:030:56:08

So, please welcome one of the stars

0:56:080:56:10

of this year's Great British Bake Off, Selasi.

0:56:100:56:14

CHEERING AND APPLAUSE

0:56:140:56:17

Great. Great to see you.

0:56:230:56:25

Great to see you, buddy.

0:56:250:56:27

-Welcome, Selasi. Thanks for joining us.

-Thank you.

0:56:280:56:30

You were one of our family favourites.

0:56:300:56:33

What's it like, being on The Great British Bake Off?

0:56:330:56:37

It's really fun, so if you ever

0:56:370:56:39

change your mind about science you can...

0:56:390:56:42

You can go in. But it was really, really fun. Very challenging.

0:56:420:56:45

-So, could you begin to ice that last cake there...

-Sure.

0:56:450:56:49

..while I explain what we've got here?

0:56:490:56:51

So, these cakes represent the different years

0:56:510:56:55

and the different amounts, or proportions, of energy

0:56:550:56:58

used in the UK to generate our energy.

0:56:580:57:02

So, 80 years ago - it's our 80th anniversary...

0:57:020:57:05

1936, and you can see the big,

0:57:050:57:08

gigantic black slice,

0:57:080:57:11

indicating that coal dominated 80 years ago.

0:57:110:57:14

And we've come on a long way.

0:57:140:57:16

If you now go to this year, renewables in green, coal in black.

0:57:160:57:22

For the first time, this year,

0:57:220:57:25

the UK generated more energy from renewables than from coal.

0:57:250:57:29

So, our goal in the future is to double our renewables.

0:57:300:57:35

So this last cake that Selasi has beautifully iced

0:57:350:57:39

represents our ambition.

0:57:390:57:43

So, not since Faraday's day has there been a more exciting time

0:57:430:57:47

to be inventing new ways of generating energy.

0:57:470:57:51

So get thinking - your ideas make a difference in the future.

0:57:510:57:57

In the next lecture,

0:57:570:57:59

we're going to look at how humans and other animals use energy.

0:57:590:58:04

So join us to find out if we can supercharge the human body.

0:58:040:58:09

Thank you and goodnight.

0:58:090:58:11

APPLAUSE

0:58:110:58:13

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