Browse content similar to Playing with Fire. Check below for episodes and series from the same categories and more!
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Everything around us exists somewhere on a vast scale, | 0:00:05 | 0:00:09 | |
from cold to hot. | 0:00:09 | 0:00:12 | |
The tiniest insects, all of us, the Earth, the stars, | 0:00:13 | 0:00:17 | |
even the universe itself, everything has a temperature. | 0:00:17 | 0:00:21 | |
I'm Dr Helen Czerski. | 0:00:25 | 0:00:27 | |
In this series, I'm going to unlock temperature's deepest mysteries. | 0:00:27 | 0:00:31 | |
Across three programmes, | 0:00:34 | 0:00:35 | |
I'm going to explore the extremes of the temperature scale... | 0:00:35 | 0:00:39 | |
..from some of the coldest temperatures to the very hottest, | 0:00:41 | 0:00:46 | |
and everything in between. | 0:00:46 | 0:00:49 | |
I'm a physicist, so my treasure map is woven from the fundamental | 0:00:49 | 0:00:53 | |
physical laws of the universe, | 0:00:53 | 0:00:55 | |
and temperature is an essential part of that. | 0:00:55 | 0:00:57 | |
It's the hidden energy contained within matter. | 0:00:58 | 0:01:01 | |
And the way that energy endlessly shifts and flows | 0:01:03 | 0:01:08 | |
is the architect that has shaped our planet. | 0:01:08 | 0:01:11 | |
And the universe. | 0:01:13 | 0:01:15 | |
It's not often that I get up at 5am to watch a pond, | 0:01:16 | 0:01:19 | |
but this one's worth watching. | 0:01:19 | 0:01:21 | |
In this programme, I'll be exploring the incredible science of heat. | 0:01:24 | 0:01:29 | |
What temperatures does it reach on the inside there? | 0:01:30 | 0:01:33 | |
-100 million degrees. -That's just a ludicrous number! | 0:01:33 | 0:01:36 | |
I'll reveal how our ability to harness heat lies behind some of | 0:01:38 | 0:01:43 | |
humanity's greatest achievements, | 0:01:43 | 0:01:46 | |
from the molten metals that gave us tools... | 0:01:46 | 0:01:48 | |
..to the searing energy of plasmas | 0:01:52 | 0:01:56 | |
that offer the promise of almost unlimited power. | 0:01:56 | 0:02:00 | |
Temperature is in every single story that nature has to tell, and in this | 0:02:02 | 0:02:06 | |
series, I'll be exploring why, what temperature means, | 0:02:06 | 0:02:10 | |
how it works, and just how deep its influence | 0:02:10 | 0:02:13 | |
on our lives and our world really is. | 0:02:13 | 0:02:15 | |
I love steam engines because they're so raw. | 0:02:47 | 0:02:51 | |
You can see where the energy's coming from and where it's going to. | 0:02:51 | 0:02:55 | |
This one's called Braveheart. It was built in 1951 | 0:02:55 | 0:02:59 | |
and still going strong. | 0:02:59 | 0:03:01 | |
The steam out there is amazing! | 0:03:01 | 0:03:03 | |
WHISTLE BLOWS | 0:03:04 | 0:03:08 | |
Steam locomotives like Braveheart are a symbol of an age | 0:03:14 | 0:03:19 | |
when it seemed that our ability to harness heat knew no bounds... | 0:03:19 | 0:03:23 | |
..allowing us to drive our trains, run our factories, | 0:03:27 | 0:03:31 | |
and propel our ships. | 0:03:31 | 0:03:34 | |
The age of steam was about building machines to get stuff done, | 0:03:34 | 0:03:37 | |
but to get the engineering right, people had to ask previously | 0:03:37 | 0:03:42 | |
unanswered questions about what heat really was. | 0:03:42 | 0:03:45 | |
And with the answers came an understanding of just how much heat | 0:03:48 | 0:03:52 | |
could do for us. | 0:03:52 | 0:03:53 | |
We're going past the modern world and the houses and computers and | 0:03:56 | 0:03:59 | |
technology that we take for granted, | 0:03:59 | 0:04:01 | |
all of which require a control of heat. | 0:04:01 | 0:04:03 | |
All of that is built on the foundation of the Industrial | 0:04:03 | 0:04:07 | |
Revolution, things like this engine. | 0:04:07 | 0:04:09 | |
Right at the heart of the engine is the rawest bit and the first form | 0:04:11 | 0:04:16 | |
of heat humans learned to control, and that is fire. | 0:04:16 | 0:04:20 | |
In all of human history, there can be few moments more | 0:04:40 | 0:04:44 | |
significant than the discovery of fire. | 0:04:44 | 0:04:47 | |
The spark is so brief, | 0:04:56 | 0:04:58 | |
such a tiny flash of light, and yet the start of such a huge story. | 0:04:58 | 0:05:03 | |
A long time ago, perhaps around a million years, our ancestors | 0:05:04 | 0:05:08 | |
could sit around a fire for the first time when they chose. | 0:05:08 | 0:05:13 | |
And I'm sure that fire was just as mesmerising for them as it is for | 0:05:13 | 0:05:17 | |
us, this flood of heat and light conjured up at will. | 0:05:17 | 0:05:20 | |
You don't need any understanding of physics to appreciate this, | 0:05:21 | 0:05:25 | |
or to be fascinated by it. | 0:05:25 | 0:05:27 | |
It must have seemed amazing that something as apparently dead | 0:05:29 | 0:05:34 | |
and inert as wood could suddenly change into flame, | 0:05:34 | 0:05:37 | |
releasing so much heat. | 0:05:37 | 0:05:40 | |
Our ancestors couldn't have known it, | 0:05:42 | 0:05:44 | |
but mastering that spark opened the door | 0:05:44 | 0:05:48 | |
to a whole new way of being human. | 0:05:48 | 0:05:50 | |
The ability to create fire provided our ancestors with warmth, | 0:05:54 | 0:06:00 | |
protection, and a means of cooking food. | 0:06:00 | 0:06:03 | |
But for all the usefulness of fire, | 0:06:05 | 0:06:07 | |
unlocking its full potential was still a long way off. | 0:06:07 | 0:06:12 | |
For almost all of human history, we had no idea what heat could do | 0:06:12 | 0:06:17 | |
for us because we just didn't know what it really was. | 0:06:17 | 0:06:20 | |
It wasn't that long ago that people thought heat was a substance | 0:06:24 | 0:06:28 | |
in its own right. | 0:06:28 | 0:06:29 | |
A weightless fluid called caloric | 0:06:30 | 0:06:33 | |
that could flow in and out of solids and liquids, | 0:06:33 | 0:06:37 | |
altering their temperature. | 0:06:37 | 0:06:39 | |
Not until the early 20th century did we discover that heat isn't | 0:06:41 | 0:06:46 | |
a substance, but something else entirely. | 0:06:46 | 0:06:49 | |
To show you, | 0:06:54 | 0:06:57 | |
I'm going to heat up my favourite snack. | 0:06:57 | 0:06:59 | |
What I've got here are popcorn kernels. | 0:07:00 | 0:07:03 | |
And each one is the seed of a plant. | 0:07:03 | 0:07:06 | |
But inside them, they've got a little bit of water. | 0:07:06 | 0:07:09 | |
What's happening is that energy is flowing into the kernels. | 0:07:09 | 0:07:13 | |
And the water molecules, as they heat up, | 0:07:13 | 0:07:16 | |
are moving faster and faster. | 0:07:16 | 0:07:18 | |
That water, the liquid water, | 0:07:22 | 0:07:24 | |
is being pulled apart and so the liquid is becoming a gas | 0:07:24 | 0:07:28 | |
and the popcorn kernels are filling up with steam. | 0:07:28 | 0:07:31 | |
Every single one of these kernels is now a very small pressure cooker. | 0:07:31 | 0:07:36 | |
And eventually... | 0:07:36 | 0:07:38 | |
POPPING | 0:07:38 | 0:07:40 | |
Ooh! | 0:07:40 | 0:07:42 | |
And the pressure bursts the kernel out of shell. | 0:07:44 | 0:07:49 | |
The whole kernel turns inside out, and then you get popcorn. | 0:07:49 | 0:07:52 | |
That is flying everywhere! | 0:07:52 | 0:07:54 | |
And the important point here | 0:07:57 | 0:07:59 | |
is that the heat energy is all about movement. | 0:07:59 | 0:08:01 | |
As atoms and molecules take energy on board, they start to speed up. | 0:08:06 | 0:08:10 | |
The faster the movement, the hotter the substance is. | 0:08:13 | 0:08:17 | |
And the crucial point about all this movement or energy | 0:08:20 | 0:08:25 | |
is its extraordinary ability to transform things. | 0:08:25 | 0:08:29 | |
Even matter itself. | 0:08:32 | 0:08:34 | |
I've come to Alderley Edge in Cheshire. | 0:08:40 | 0:08:42 | |
-This goes around your back... -So this is just going round there. | 0:08:42 | 0:08:45 | |
-That's right. -..to see some early evidence of how we learnt to take | 0:08:45 | 0:08:48 | |
advantage of this hidden ability of heat. | 0:08:48 | 0:08:51 | |
Dating back some 4,000 years, | 0:08:55 | 0:08:58 | |
the Alderley Edge mines are some of the oldest in Britain. | 0:08:58 | 0:09:02 | |
Mind the steps. It's a bit slippery in places. | 0:09:04 | 0:09:07 | |
Nigel Dibben from the Derbyshire Caving Club | 0:09:07 | 0:09:10 | |
has offered to take me inside. | 0:09:10 | 0:09:12 | |
Is your light on? There's mine on. | 0:09:13 | 0:09:16 | |
Follow me in. | 0:09:17 | 0:09:19 | |
Just mind your head here. It gets a bit low. | 0:09:23 | 0:09:25 | |
-So this is all man made? -This is all man made. | 0:09:25 | 0:09:28 | |
You can see some of these pick marks on the wall along here. | 0:09:30 | 0:09:33 | |
I tell you what, | 0:09:42 | 0:09:44 | |
this is not the easiest commute for anyone coming to work down here. | 0:09:44 | 0:09:47 | |
Whatever's down the other end must have been pretty valuable. | 0:09:47 | 0:09:50 | |
After a few more minutes, we come to the heart of the mine. | 0:09:55 | 0:10:00 | |
This is what I really want you to have a look at. | 0:10:00 | 0:10:03 | |
That's spectacular! | 0:10:03 | 0:10:05 | |
That is a fabulous colour, isn't it? | 0:10:05 | 0:10:07 | |
It's such an unexpected colour to find in the gloom, isn't it? | 0:10:07 | 0:10:10 | |
And have a look down here as well. | 0:10:10 | 0:10:13 | |
There's a bit more down the bottom, this shaft here. | 0:10:13 | 0:10:16 | |
-Oh, yeah, a huge, great big stripe of it. -Down the bottom there. | 0:10:16 | 0:10:19 | |
This mineral is chrysocolla, and it's dissolved into water | 0:10:24 | 0:10:28 | |
that's dripping through the rock here, and then it's been redeposited | 0:10:28 | 0:10:31 | |
in this beautiful sheet. | 0:10:31 | 0:10:32 | |
And the spectacular colour is a hint | 0:10:32 | 0:10:35 | |
as to why those early miners came down here. | 0:10:35 | 0:10:38 | |
The pure version of the mineral that the miners were after is this. | 0:10:38 | 0:10:43 | |
And this is malachite. | 0:10:44 | 0:10:46 | |
When I was a kid, I was fascinated by semi-precious gems, | 0:10:47 | 0:10:50 | |
and it was malachite that got me started on that. | 0:10:50 | 0:10:53 | |
I couldn't leave it alone. | 0:10:53 | 0:10:54 | |
It's a beautiful, deep, rich, green colour. | 0:10:54 | 0:10:58 | |
And it's not just me - it's been | 0:10:58 | 0:10:59 | |
used by humans for millennia as a green | 0:10:59 | 0:11:02 | |
pigment because of the way it looks. | 0:11:02 | 0:11:04 | |
But malachite doesn't just have style, it has substance. | 0:11:06 | 0:11:09 | |
Because when you take malachite and heat it up, | 0:11:12 | 0:11:15 | |
you start to transform it. | 0:11:15 | 0:11:17 | |
Malachite is a mineral, | 0:11:19 | 0:11:21 | |
which means it's made of lots of different types of atoms, | 0:11:21 | 0:11:24 | |
all bound up together, but you can't see what's in there. | 0:11:24 | 0:11:27 | |
But once you heat it up, you can drive off the smaller atoms, | 0:11:27 | 0:11:31 | |
the carbon and then the oxygen, | 0:11:31 | 0:11:33 | |
and then what you have left is the element that's at the heart of this, | 0:11:33 | 0:11:36 | |
which is this. | 0:11:36 | 0:11:38 | |
It's copper, the first metal to be smelted from its ore. | 0:11:38 | 0:11:42 | |
Copper is strong and malleable and shiny. | 0:11:42 | 0:11:45 | |
It's completely different from the mineral it came from. | 0:11:45 | 0:11:48 | |
And the clear implication is that heat can change things. | 0:11:48 | 0:11:52 | |
And so it wasn't far to the next step of the imagination. | 0:11:52 | 0:11:55 | |
Because if heat can change this into this, what else can it do? | 0:11:55 | 0:11:59 | |
The answer came when people realised that just as heat can turn rock into | 0:12:02 | 0:12:07 | |
metal, so with a little know-how | 0:12:07 | 0:12:10 | |
it could also be used to alter the metal itself. | 0:12:10 | 0:12:14 | |
In the year 793, Anglo-Saxon Britain came under attack... | 0:12:22 | 0:12:27 | |
..when Viking raiders first landed on the Northumbrian coast. | 0:12:33 | 0:12:37 | |
While the Vikings' reputation as fearsome warriors is | 0:12:43 | 0:12:47 | |
well-documented, what's less well-known is their skilful | 0:12:47 | 0:12:51 | |
craft work, especially with metals. | 0:12:51 | 0:12:55 | |
A skill calling not only for a sense of design, but also a sophisticated | 0:12:58 | 0:13:04 | |
understanding of temperature. | 0:13:04 | 0:13:06 | |
To find out more, I've come to meet historical blacksmith Jason Green. | 0:13:15 | 0:13:20 | |
-And how hot will it get in there? -Around 1,300 degrees. | 0:13:25 | 0:13:29 | |
Under Jason's watchful eye, I'm going to attempt to make a Viking | 0:13:29 | 0:13:34 | |
dagger, a process that starts with heating up a small piece of steel, | 0:13:34 | 0:13:39 | |
before hammering it into shape. | 0:13:39 | 0:13:41 | |
-That's it. -OK. | 0:13:44 | 0:13:47 | |
Not setting the grass on fire. | 0:13:47 | 0:13:48 | |
-The only way you're going to learn is to do it. -By doing it. | 0:13:48 | 0:13:51 | |
Right, well, there is going to be a lot of doing, isn't there? | 0:13:51 | 0:13:54 | |
You can feel as it cools, it suddenly stops going anywhere! | 0:13:59 | 0:14:02 | |
-Yeah, it starts getting harder. -Yeah. | 0:14:02 | 0:14:04 | |
Blow by blow, my dagger starts to take shape. | 0:14:05 | 0:14:08 | |
Both externally and, more importantly, deep inside the metal. | 0:14:09 | 0:14:15 | |
We don't tend to think of metals | 0:14:17 | 0:14:19 | |
as being crystals, but in fact they are. | 0:14:19 | 0:14:22 | |
That means their atoms are arranged | 0:14:25 | 0:14:28 | |
into a highly regular, repeating pattern. | 0:14:28 | 0:14:30 | |
What's happening as we heat is that the crystals are changing because | 0:14:34 | 0:14:38 | |
the heat makes them slightly more mobile, | 0:14:38 | 0:14:41 | |
it allows you to push atoms around. | 0:14:41 | 0:14:44 | |
As I hammer away, each impact rearranges the atoms inside... | 0:14:45 | 0:14:50 | |
..creating tiny knots within the crystalline structure. | 0:14:52 | 0:14:56 | |
As these knots accumulate, | 0:14:58 | 0:15:00 | |
it becomes harder for the atoms to move over each other. | 0:15:00 | 0:15:04 | |
And this helps make the metal stronger. | 0:15:06 | 0:15:09 | |
And so all of this raw action, | 0:15:12 | 0:15:16 | |
this hammering, thumping, and the heating, | 0:15:16 | 0:15:19 | |
is changing things at a very tiny scale inside the metal itself. | 0:15:19 | 0:15:23 | |
And that's what gives iron and steel | 0:15:23 | 0:15:25 | |
its strength and that's why it's so useful. | 0:15:25 | 0:15:28 | |
But a blade's strength doesn't come from hammering alone. | 0:15:28 | 0:15:31 | |
It also requires clever manipulation of its temperature. | 0:15:34 | 0:15:39 | |
The knife's now back in the forge, glowing cherry red, | 0:15:39 | 0:15:42 | |
and that means it's about 800 degrees C. | 0:15:42 | 0:15:44 | |
And that matters because the crystal structure at this temperature, | 0:15:44 | 0:15:48 | |
this is the one we want. It's very strong, it's really useful. | 0:15:48 | 0:15:51 | |
If I let it cool down slowly, | 0:15:51 | 0:15:53 | |
it will change back to the room temperature structure. | 0:15:53 | 0:15:56 | |
And so in order to keep this crystal structure, so it's a useful knife, | 0:15:57 | 0:16:01 | |
this is what we do... | 0:16:01 | 0:16:03 | |
..which is very satisfying! | 0:16:04 | 0:16:06 | |
As the hot metal is plunged into the water, | 0:16:14 | 0:16:17 | |
its temperature plummets in just a few seconds. | 0:16:17 | 0:16:20 | |
By cooling it so quickly, | 0:16:23 | 0:16:25 | |
the atoms haven't got time to shift into the shape that they want to | 0:16:25 | 0:16:28 | |
have, and so they're stuck, locked in with a very strong structure. | 0:16:28 | 0:16:32 | |
Finally, one last round of heating to remove any remaining brittleness. | 0:16:34 | 0:16:40 | |
There we go. One finished fighting blade. | 0:16:43 | 0:16:46 | |
I'm so impressed that with such simple tools | 0:16:46 | 0:16:48 | |
you can make something so useful. | 0:16:48 | 0:16:50 | |
That's brilliant. Thank you very much. | 0:16:50 | 0:16:53 | |
By turning wood into flames, | 0:16:58 | 0:17:02 | |
rock into metal, | 0:17:02 | 0:17:06 | |
and soft metal into hard, | 0:17:06 | 0:17:09 | |
our ancestors' growing understanding that heat could transform matter | 0:17:09 | 0:17:14 | |
altered the course of human civilisation. | 0:17:14 | 0:17:17 | |
But for thousands of years, | 0:17:22 | 0:17:23 | |
this knowledge was only applied to solids. | 0:17:23 | 0:17:26 | |
The next leap forward would see people using heat to exploit another | 0:17:29 | 0:17:33 | |
form of matter, one with astonishing potential. | 0:17:33 | 0:17:37 | |
Gas. | 0:17:40 | 0:17:41 | |
But to understand how gases respond to heat, | 0:17:44 | 0:17:47 | |
we first need to take a step back and look at what gases are | 0:17:47 | 0:17:52 | |
and how they behave. | 0:17:52 | 0:17:54 | |
Humans love a bit of spectacle, | 0:18:03 | 0:18:05 | |
anything with colour and music and fun. | 0:18:05 | 0:18:08 | |
But the stereotype of a scientific experiment is almost exactly the | 0:18:08 | 0:18:11 | |
opposite, a dusty basement with someone who hasn't seen daylight for | 0:18:11 | 0:18:15 | |
a week, writing down measurements that no one will ever read. | 0:18:15 | 0:18:18 | |
But there have been exceptions. There have been experiments | 0:18:21 | 0:18:24 | |
set up with the theatrical drama to match their scientific significance. | 0:18:24 | 0:18:29 | |
And one of my favourites happened in 1654, and it was all organised | 0:18:29 | 0:18:33 | |
by a man called Otto von Guericke. | 0:18:33 | 0:18:35 | |
The aim of the experiment was to demonstrate a very specific and | 0:18:38 | 0:18:42 | |
extraordinary property of gases. | 0:18:42 | 0:18:45 | |
And heading up the guest list was none other than the Holy | 0:18:48 | 0:18:51 | |
Roman Emperor, Ferdinand III. | 0:18:51 | 0:18:54 | |
When the Emperor and his guests were all seated, | 0:18:57 | 0:18:59 | |
it was time for the star of the show, and that was two metal | 0:18:59 | 0:19:03 | |
hemispheres like these, with flat inner surfaces. | 0:19:03 | 0:19:06 | |
Von Guericke placed the two hemispheres together and then | 0:19:06 | 0:19:09 | |
started to take out the air from the inside. | 0:19:09 | 0:19:12 | |
This created a vacuum which held the two halves of the sphere together. | 0:19:14 | 0:19:18 | |
And it was what Von Guericke | 0:19:21 | 0:19:22 | |
did next that made everyone pay attention. | 0:19:22 | 0:19:24 | |
He set up a team of horses on either side... | 0:19:27 | 0:19:30 | |
..put the sphere in between, | 0:19:32 | 0:19:34 | |
and gave the command for the horses to pull. | 0:19:34 | 0:19:36 | |
To show you what happened next, | 0:19:41 | 0:19:43 | |
we're going to attach our sphere to the modern equivalent | 0:19:43 | 0:19:47 | |
of Von Guericke's horses - a pair of 4X4s. | 0:19:47 | 0:19:51 | |
Stand by. | 0:19:54 | 0:19:56 | |
I'm actually quite nervous. | 0:19:57 | 0:19:59 | |
Three, two, one. | 0:19:59 | 0:20:02 | |
Go! | 0:20:02 | 0:20:03 | |
So the tension's out of the rope. | 0:20:07 | 0:20:09 | |
So now a little bit on the accelerator, just up to 1,000. | 0:20:12 | 0:20:15 | |
Feel it taking the strain. | 0:20:18 | 0:20:19 | |
OK. Keep going up to 1,300. | 0:20:23 | 0:20:26 | |
Can feel it in the car. | 0:20:35 | 0:20:37 | |
OK, up to 1,600. | 0:20:37 | 0:20:39 | |
The engine is not happy! | 0:20:41 | 0:20:43 | |
I think we might have established the sphere really works. | 0:20:48 | 0:20:51 | |
OK, let's pause there, so stop. | 0:20:51 | 0:20:53 | |
It's impressive. It really is impressive. | 0:20:56 | 0:20:58 | |
Just as our sphere stood up to a pair of 4X4s, | 0:21:02 | 0:21:06 | |
so Von Guericke's was also able | 0:21:06 | 0:21:08 | |
to resist the pull of two sets of horses. | 0:21:08 | 0:21:12 | |
To Von Guericke, it was the proof of something he'd long suspected, | 0:21:16 | 0:21:20 | |
that gases like air exert an incredibly strong force. | 0:21:20 | 0:21:25 | |
All the air around me looks completely calm, but it isn't. | 0:21:33 | 0:21:37 | |
It's a gigantic, three-dimensional game of molecular bumper cars. | 0:21:37 | 0:21:41 | |
Even in one cubic centimetre of air, | 0:21:41 | 0:21:44 | |
there are nearly 30 million trillion air molecules and they're bumping | 0:21:44 | 0:21:49 | |
into each other all the time. | 0:21:49 | 0:21:50 | |
Just one molecule will collide several billion times every second. | 0:21:50 | 0:21:56 | |
And every single collision gives a little bit of a push, and so if they | 0:21:56 | 0:21:59 | |
bump into us, they push, and that's what air pressure is. | 0:21:59 | 0:22:03 | |
And the question then is - | 0:22:03 | 0:22:04 | |
if I'm being pushed on by this pressure all the time, | 0:22:04 | 0:22:07 | |
why aren't I being squeezed? | 0:22:07 | 0:22:09 | |
And the answer is that every time I breathe in, | 0:22:11 | 0:22:14 | |
I'm taking air molecules into my lungs. | 0:22:14 | 0:22:16 | |
And they're pushing out on the walls of my lungs and because the | 0:22:16 | 0:22:20 | |
inward push and the outward push exactly balance, I don't notice. | 0:22:20 | 0:22:24 | |
And that was why Von Guericke needed to generate a vacuum. | 0:22:28 | 0:22:31 | |
You can only see how strong air pressure really is when you take | 0:22:31 | 0:22:35 | |
away the push from the other side. At the end of the demonstration, | 0:22:35 | 0:22:39 | |
all they needed to do was let a little bit of air back in and it was | 0:22:39 | 0:22:44 | |
almost as though the pressure hadn't been there. | 0:22:44 | 0:22:46 | |
The ability of molecules to exert pressure is one of the most | 0:22:56 | 0:23:01 | |
fundamental properties of not just air, but all gases. | 0:23:01 | 0:23:04 | |
But Von Guericke's discovery also raised an important question. | 0:23:09 | 0:23:13 | |
If cold air molecules could have such a powerful effect, | 0:23:15 | 0:23:19 | |
what might be achieved if those same molecules were heated up? | 0:23:19 | 0:23:24 | |
I've travelled to the north of England to meet a bunch | 0:23:36 | 0:23:39 | |
of enthusiasts with a head for heights. | 0:23:39 | 0:23:42 | |
Harry Stringer is from the Pennine Region Balloon Association. | 0:23:45 | 0:23:49 | |
He's been flying hot air balloons for over 25 years. | 0:23:51 | 0:23:55 | |
-So, where are we going today? -Well, we'll clear the tree tops here... | 0:23:57 | 0:24:01 | |
-That sounds like a good start! -Yeah, and then we'll go up | 0:24:01 | 0:24:04 | |
-to about 1,000 feet. -OK. -Hands on. | 0:24:04 | 0:24:07 | |
Hands on. | 0:24:08 | 0:24:10 | |
The very first hot-air balloon, launched in 1783, was the brainchild | 0:24:10 | 0:24:16 | |
of two brothers called Joseph and Etienne Montgolfier. | 0:24:16 | 0:24:20 | |
Oh, we're free. | 0:24:20 | 0:24:22 | |
OK, we're way. | 0:24:22 | 0:24:24 | |
One story goes that Joseph had been staring into his fireplace one | 0:24:25 | 0:24:30 | |
evening, when he had the idea of filling a paper bag with hot-air. | 0:24:30 | 0:24:34 | |
On letting the bag go, he observed that it began to rise. | 0:24:36 | 0:24:40 | |
And this encouraged the brothers to repeat the experiment, but this time | 0:24:41 | 0:24:46 | |
with a much larger, purpose-built balloon. | 0:24:46 | 0:24:49 | |
Until the 1780s, | 0:25:02 | 0:25:03 | |
the sky was just a place for clouds and birds, and humans certainly | 0:25:03 | 0:25:07 | |
didn't go up there. But when the first balloons came along, | 0:25:07 | 0:25:10 | |
people could look up and wonder, what's it like up there? | 0:25:10 | 0:25:14 | |
And the problem, if you were curious about the sky, | 0:25:14 | 0:25:17 | |
was that gravity was holding you down to the ground. | 0:25:17 | 0:25:20 | |
But the really ingenious thing about hot-air balloons is how they use | 0:25:20 | 0:25:24 | |
heat, together with the force of gravity itself, to get around this. | 0:25:24 | 0:25:29 | |
The mechanism of these is beautifully simple. | 0:25:38 | 0:25:41 | |
There's a bag above me, filled with hot-air. | 0:25:41 | 0:25:43 | |
What the burner does is it allows the balloonist to play around with | 0:25:43 | 0:25:46 | |
the density of the air by controlling its temperature. | 0:25:46 | 0:25:49 | |
And as the air inside there is heated up, | 0:25:49 | 0:25:52 | |
and it could get up to 100 Celsius, it expands. | 0:25:52 | 0:25:55 | |
As the air expands, its individual molecules push outwards, | 0:25:58 | 0:26:03 | |
making the air inside the balloon less dense. | 0:26:03 | 0:26:06 | |
And that's where gravity comes into play. | 0:26:08 | 0:26:11 | |
Gravity is pulling everything, | 0:26:11 | 0:26:13 | |
everything I can see, down to the ground. | 0:26:13 | 0:26:15 | |
But because the air inside the balloon is less dense than the air | 0:26:15 | 0:26:19 | |
around it, everything around us is being pulled down more, | 0:26:19 | 0:26:23 | |
so it's squeezing the less dense balloon upwards and so balloonists | 0:26:23 | 0:26:27 | |
are floating on top of the denser air around them. | 0:26:27 | 0:26:30 | |
But temperature doesn't just enable a balloon to rise, | 0:26:36 | 0:26:39 | |
it also controls how it falls. | 0:26:39 | 0:26:42 | |
So, how do you make us come down? | 0:26:47 | 0:26:49 | |
We'll have a parachute vent. It's massive. You can see it. | 0:26:49 | 0:26:53 | |
I could pull this red line... | 0:26:54 | 0:26:56 | |
-Yeah. -..and it will open the valve and then I just close it and the | 0:26:56 | 0:27:01 | |
gulp of hot air loss will cause the balloon to descend. | 0:27:01 | 0:27:04 | |
-We are safe. -Can we stand up now? -We can. We can. | 0:27:18 | 0:27:22 | |
The discovery that heating up air could make it expand enough to lift | 0:27:23 | 0:27:28 | |
people into the skies was a milestone in human innovation. | 0:27:28 | 0:27:32 | |
And it wasn't long before we began to put that very same heat energy | 0:27:34 | 0:27:39 | |
to a much more practical purpose. | 0:27:39 | 0:27:41 | |
It was something that emerged from a very 18th-century problem. | 0:27:53 | 0:27:56 | |
300 years ago, mine owners in Britain | 0:28:02 | 0:28:04 | |
were facing a serious crisis. | 0:28:04 | 0:28:06 | |
Since many ore deposits sat well below the water table, | 0:28:12 | 0:28:16 | |
they were finding that their mines could go only as deep | 0:28:16 | 0:28:20 | |
as the drainage technology at the time allowed, | 0:28:20 | 0:28:23 | |
resulting in many mines going out of business. | 0:28:23 | 0:28:26 | |
What was needed was a way to haul all that water up to the surface, | 0:28:29 | 0:28:34 | |
so that the miners could get to the ore below. | 0:28:34 | 0:28:37 | |
And in 1712, an ironmonger called Thomas Newcomen hit upon the answer, | 0:28:40 | 0:28:46 | |
with the world's first commercial steam engine. | 0:28:46 | 0:28:49 | |
And it worked by harnessing | 0:28:52 | 0:28:53 | |
the immense energy contained within hot steam. | 0:28:53 | 0:28:57 | |
The principle behind Newcomen's engine is exactly the same one that | 0:29:03 | 0:29:07 | |
Otto von Guericke had demonstrated. | 0:29:07 | 0:29:09 | |
And that is how hard air pressure can push, | 0:29:09 | 0:29:12 | |
especially when there's a vacuum on the other side. | 0:29:12 | 0:29:15 | |
I've got a plastic bottle here | 0:29:15 | 0:29:17 | |
with some water in the bottom, and I'm going to put it in the microwave | 0:29:17 | 0:29:20 | |
to heat the water up. | 0:29:20 | 0:29:21 | |
What's happening inside the microwave is that the water | 0:29:26 | 0:29:29 | |
molecules are being given energy and they're not just heating up, | 0:29:29 | 0:29:32 | |
but some of them are turning into a gas, into steam. | 0:29:32 | 0:29:35 | |
And that steam is starting to fill up the bottle. | 0:29:35 | 0:29:39 | |
And it's what happens next that's important. | 0:29:39 | 0:29:41 | |
Tip it into this water here. | 0:29:45 | 0:29:48 | |
SHE LAUGHS | 0:29:50 | 0:29:52 | |
And you can see that what happens is that the bottle has been crushed | 0:29:52 | 0:29:57 | |
and it's now full of water. | 0:29:57 | 0:29:59 | |
And the reason for that is that as it filled up with steam, | 0:29:59 | 0:30:02 | |
the air was pushed out. | 0:30:02 | 0:30:04 | |
And then when I cooled the steam down, | 0:30:04 | 0:30:06 | |
it condensed from a gas back into a liquid, | 0:30:06 | 0:30:09 | |
which takes up much less space. | 0:30:09 | 0:30:11 | |
So there's a partial vacuum left in bottle and so there was all the air | 0:30:13 | 0:30:17 | |
pressure pushing in, nothing pushing back, and the bottle was crushed. | 0:30:17 | 0:30:22 | |
This is the principle that Newcomen used to drive his engine. | 0:30:29 | 0:30:32 | |
At the heart of Newcomen's engine lay a large metal cylinder, | 0:30:33 | 0:30:37 | |
housing a piston and filled with hot steam. | 0:30:37 | 0:30:40 | |
Cooling this steam with water simultaneously created a vacuum | 0:30:42 | 0:30:48 | |
and caused the weight of the atmosphere to push down on the | 0:30:48 | 0:30:52 | |
piston, driving the engine. | 0:30:52 | 0:30:54 | |
The cylinder was then refilled with hot steam and the cycle repeated. | 0:30:54 | 0:30:59 | |
Soon, Newcomen's steam engines were popping up all over Britain. | 0:31:03 | 0:31:08 | |
Each one a symbol of heat's ability to perform useful work. | 0:31:10 | 0:31:14 | |
But Newcomen's design had one major weakness. | 0:31:19 | 0:31:23 | |
The brilliant thing about steam engines is that they convert heat | 0:31:26 | 0:31:29 | |
energy, this type of energy you can't really see, into mechanical | 0:31:29 | 0:31:33 | |
work, the sort of thing that can push pistons | 0:31:33 | 0:31:36 | |
and turn wheels and do practical things. | 0:31:36 | 0:31:39 | |
And Newcomen's engine worked, but it was spectacularly inefficient - | 0:31:40 | 0:31:45 | |
of all the energy and the coal that went in, | 0:31:45 | 0:31:48 | |
only one or 2% was converted into useful, mechanical work. | 0:31:48 | 0:31:52 | |
The mystery was why. | 0:31:56 | 0:31:58 | |
Where was all that heat energy going? | 0:32:00 | 0:32:02 | |
And what could be done to retrieve it? | 0:32:02 | 0:32:05 | |
To discover the answer, I've come to Coldharbour Mill in Devon. | 0:32:09 | 0:32:12 | |
Originally built in 1797, | 0:32:15 | 0:32:17 | |
it's one of the oldest steam-powered woollen mills left in Britain. | 0:32:17 | 0:32:21 | |
OK, so we won't kill anybody with the other end... | 0:32:23 | 0:32:25 | |
John Jasper runs the mill's giant steam engine. | 0:32:27 | 0:32:30 | |
-Like this. -Like that? -You are a natural. Right. -OK. | 0:32:30 | 0:32:33 | |
And the first thing any steam engine needs, of course, is steam. | 0:32:33 | 0:32:37 | |
And today, John's invited me to help him make some. | 0:32:37 | 0:32:40 | |
-So, tell me about these boilers. -This is a Lancashire boiler. | 0:32:44 | 0:32:47 | |
It holds 20,000 gallons of water. | 0:32:47 | 0:32:50 | |
Above that water level, you have steam. | 0:32:50 | 0:32:53 | |
-And you get a bit of steam... -Great. | 0:32:56 | 0:32:58 | |
So it's basically a sort of steam kettle. | 0:32:58 | 0:33:00 | |
So these bits are the heating elements. | 0:33:00 | 0:33:02 | |
Effectively you're shovelling fire into the heating elements... | 0:33:02 | 0:33:05 | |
-That's it. -And then all of this is the kettle, which is full of water. | 0:33:05 | 0:33:08 | |
-That's right. -But instead of coming out of the spout... | 0:33:08 | 0:33:10 | |
-Yes. -..it goes to a steam engine. | 0:33:10 | 0:33:12 | |
It just takes a little longer to get to the boil. | 0:33:12 | 0:33:14 | |
-I'd better do some more shovelling then! -Yeah. | 0:33:16 | 0:33:19 | |
The engine here is a descendant of a type that was built to address the | 0:33:23 | 0:33:26 | |
problem of Newcomen's lost energy. | 0:33:26 | 0:33:29 | |
It was designed by a Scottish instrument maker called James Watt. | 0:33:32 | 0:33:36 | |
Watt had recently become familiar with a new theory of heat. | 0:33:39 | 0:33:43 | |
Creating steam is all about putting heat energy into water, | 0:33:47 | 0:33:51 | |
but there's this strange observation, | 0:33:51 | 0:33:53 | |
which is that as you start to heat water up, | 0:33:53 | 0:33:56 | |
you see the thermometer rise and it goes up and up and up, | 0:33:56 | 0:34:00 | |
and then it gets to 100 degrees and it won't go any further. | 0:34:00 | 0:34:03 | |
So you can be pumping in huge amounts of heat energy and yet | 0:34:03 | 0:34:08 | |
the thermometer isn't moving. | 0:34:08 | 0:34:10 | |
And that's because once water reaches its boiling point, | 0:34:14 | 0:34:17 | |
all that heat energy is being used up to turn the water into steam. | 0:34:17 | 0:34:23 | |
And that led to the idea that there are two forms of heat. | 0:34:24 | 0:34:28 | |
There's the sort which causes the thermometer to rise, | 0:34:28 | 0:34:31 | |
but there's another type and that is the energy needed just to turn the | 0:34:31 | 0:34:35 | |
water from a liquid into a gas at the same temperature. | 0:34:35 | 0:34:40 | |
And that heat is called latent heat. | 0:34:40 | 0:34:42 | |
The amount of latent heat needed to turn water from a liquid | 0:34:46 | 0:34:50 | |
into a gas is enormous. | 0:34:50 | 0:34:53 | |
And the reason that all this matters for steam engines is that steam | 0:34:54 | 0:34:57 | |
is expensive in terms of energy. | 0:34:57 | 0:35:00 | |
And when you've got it, you certainly don't want to waste it. | 0:35:00 | 0:35:03 | |
It was this revelation that creating steam requires huge amounts | 0:35:09 | 0:35:15 | |
of latent heat that was one of the main reasons why Newcomen's engine | 0:35:15 | 0:35:20 | |
was so wasteful. | 0:35:20 | 0:35:21 | |
At the heart of every steam engine, there's a piston. | 0:35:24 | 0:35:27 | |
That's where the hot gas molecules | 0:35:27 | 0:35:29 | |
are pushing to create mechanical work. | 0:35:29 | 0:35:32 | |
The problem with Newcomen's engine was that in order to reset, | 0:35:32 | 0:35:37 | |
the water needed to be condensed, cooled down. | 0:35:37 | 0:35:40 | |
And that happened inside the piston, | 0:35:40 | 0:35:42 | |
so the metal itself had to be cooled down as well. | 0:35:42 | 0:35:45 | |
And then you needed to use more steam energy to heat it up again | 0:35:45 | 0:35:50 | |
to create the next stroke. | 0:35:50 | 0:35:51 | |
In order to conserve all that valuable steam, | 0:35:52 | 0:35:56 | |
Watt came up with an ingenious invention. | 0:35:56 | 0:35:59 | |
Watt's solution was a condenser and this is it. | 0:36:03 | 0:36:06 | |
So instead of having the condensation happening inside the | 0:36:08 | 0:36:12 | |
piston, the steam was vented out to a separate chamber and that was | 0:36:12 | 0:36:16 | |
where the condensation occurred. | 0:36:16 | 0:36:19 | |
And the reason it was a brilliant solution was that the hot parts of | 0:36:21 | 0:36:24 | |
the engine stayed hot and the cool parts of the engine stayed cool. | 0:36:24 | 0:36:27 | |
And much less heat was wasted. | 0:36:27 | 0:36:29 | |
Watt's great insight | 0:36:35 | 0:36:37 | |
that the more an engine can conserve heat, the more efficient it will be, | 0:36:37 | 0:36:42 | |
was a watershed moment in the history of steam power. | 0:36:42 | 0:36:45 | |
Other improvements followed, | 0:36:48 | 0:36:50 | |
such as the introduction of steam at high pressure | 0:36:50 | 0:36:54 | |
to generate even greater force. | 0:36:54 | 0:36:56 | |
These innovations ushered in a mechanical revolution... | 0:36:58 | 0:37:01 | |
..founded upon the energy of hot gas molecules. | 0:37:03 | 0:37:06 | |
But as our population grew and our coal supplies dwindled, | 0:37:09 | 0:37:13 | |
so we began to turn elsewhere for our energy. | 0:37:13 | 0:37:17 | |
And in some places, | 0:37:20 | 0:37:22 | |
that's involved tapping into a different source of heat... | 0:37:22 | 0:37:25 | |
..one that's responsible for some of the most violent natural phenomena | 0:37:28 | 0:37:33 | |
on the planet. | 0:37:33 | 0:37:34 | |
Just a short distance from Reykjavik | 0:37:47 | 0:37:50 | |
lies one of Iceland's top tourist attractions... | 0:37:50 | 0:37:53 | |
..an outdoor health spa known as the Blue Lagoon. | 0:37:56 | 0:37:59 | |
This is the real attraction around here. | 0:38:03 | 0:38:05 | |
Lovely warm water at 38 Celsius. | 0:38:05 | 0:38:09 | |
And full of minerals which are apparently very good for you. | 0:38:09 | 0:38:12 | |
So on a day like today and in a country with a reputation for being | 0:38:12 | 0:38:15 | |
chilly, this is clearly the perfect place to relax. | 0:38:15 | 0:38:19 | |
But despite appearances, this is no natural beauty spot. | 0:38:27 | 0:38:32 | |
In fact, the Blue Lagoon is entirely man-made... | 0:38:32 | 0:38:36 | |
..fed by hot water from the nearby Svartsengi geothermal power station. | 0:38:40 | 0:38:45 | |
Every day, Svartsengi produces enough electricity | 0:38:53 | 0:38:57 | |
for around 130,000 homes. | 0:38:57 | 0:39:00 | |
And the source of all that power is the same heat energy that created | 0:39:04 | 0:39:09 | |
Iceland in the first place. | 0:39:09 | 0:39:11 | |
Down below my feet, the Earth is far hotter than it is up here. | 0:39:22 | 0:39:25 | |
There's a huge amount of heat energy available, and anything that takes | 0:39:25 | 0:39:29 | |
advantage of it is known as a geothermal power source, | 0:39:29 | 0:39:32 | |
literally heat from the Earth. | 0:39:32 | 0:39:35 | |
The deeper you go, the hotter it gets. | 0:39:35 | 0:39:38 | |
To tap into that heat, Svartsengi sits above 13 boreholes, | 0:39:39 | 0:39:44 | |
stretching two kilometres into the rock below. | 0:39:44 | 0:39:48 | |
The basic premise here is that a mixture of hot water and steam is | 0:39:52 | 0:39:56 | |
pumped up from deep down and the steam is separated out and sent | 0:39:56 | 0:40:00 | |
through a turbine that generates 75 megawatts of electricity. | 0:40:00 | 0:40:04 | |
That goes into the grid. | 0:40:04 | 0:40:06 | |
And then the same steam comes back around and reheats the water and | 0:40:06 | 0:40:10 | |
that supplies domestic hot water | 0:40:10 | 0:40:12 | |
for about 20,000 homes on this peninsula. | 0:40:12 | 0:40:15 | |
For the engineers around here, | 0:40:16 | 0:40:18 | |
the hot water beneath their feet is just one massive treasure trove. | 0:40:18 | 0:40:23 | |
Utilising the heat of the planet itself has allowed us to take steam | 0:40:27 | 0:40:32 | |
power to a new level. | 0:40:32 | 0:40:34 | |
But today, scientists are attempting | 0:40:40 | 0:40:42 | |
to harness another even hotter form of energy... | 0:40:42 | 0:40:46 | |
..derived from a strange type of matter that here on Earth makes the | 0:40:49 | 0:40:53 | |
occasional spectacular appearance. | 0:40:53 | 0:40:56 | |
Inside the University of Manchester's high-voltage lab, | 0:41:13 | 0:41:17 | |
a team of researchers is getting ready to recreate one of the most | 0:41:17 | 0:41:22 | |
awesome natural phenomena on the planet. | 0:41:22 | 0:41:24 | |
Lightning. | 0:41:27 | 0:41:29 | |
This beast of a device is an impulse generator, | 0:41:36 | 0:41:38 | |
and this one is capable of generating two million volts | 0:41:38 | 0:41:42 | |
between the bottom and the top. | 0:41:42 | 0:41:44 | |
And here's how it works. | 0:41:44 | 0:41:46 | |
Normally, when you get a voltage, electric charge will flow. | 0:41:46 | 0:41:49 | |
But here, each of these red things is a capacitor, and so the electric | 0:41:49 | 0:41:54 | |
charge can't go anywhere. It's stored on the plates. | 0:41:54 | 0:41:56 | |
And that means that energy is building up. | 0:41:56 | 0:41:59 | |
And it's this point here that's the important bit | 0:42:06 | 0:42:09 | |
because when the switch over there is pressed, | 0:42:09 | 0:42:11 | |
all of that charge is going to get dumped through that point in around | 0:42:11 | 0:42:16 | |
a millionth of a second. | 0:42:16 | 0:42:18 | |
Here to show me what that means in practice is Dr Vidy Peesapati. | 0:42:20 | 0:42:25 | |
So, what we're going to do right now is make sure that no one else can | 0:42:25 | 0:42:28 | |
walk in, so if you want to press the black button... | 0:42:28 | 0:42:31 | |
-That one? -Yes. That's the one. -SIREN | 0:42:31 | 0:42:34 | |
Now it's ready. Now we basically have to set our voltage... | 0:42:34 | 0:42:37 | |
Under Vidy's supervision, I'm going to trigger a lightning strike... | 0:42:37 | 0:42:42 | |
-You want to press F4 on the keyboard. -That one? -Yeah. | 0:42:42 | 0:42:45 | |
..which we'll also capture using a high-speed camera. | 0:42:46 | 0:42:49 | |
-Now it's charging. -So we can see the voltage going up here. | 0:42:51 | 0:42:54 | |
Absolutely. So, it takes around 60 seconds for the entire kit to be | 0:42:54 | 0:42:57 | |
-charged up. -When this gets to the end, we'll be ready to go. | 0:42:57 | 0:43:00 | |
We'll let the siren go, telling us there's going to be a flashover. | 0:43:00 | 0:43:04 | |
And it automatically triggers the first stage. | 0:43:04 | 0:43:07 | |
60 seconds later, and the generator is ready to fire. | 0:43:07 | 0:43:12 | |
So, when I hear the siren... SIREN | 0:43:15 | 0:43:17 | |
CRACK | 0:43:21 | 0:43:24 | |
-That is an echo and a half, isn't it? Wow! -It is very loud. | 0:43:24 | 0:43:27 | |
And that is basically a sonic boom. | 0:43:27 | 0:43:28 | |
-It's like a giant electric whip crack. -It is, absolutely. | 0:43:28 | 0:43:32 | |
But it's only when you play back the slow motion video that you begin to | 0:43:33 | 0:43:37 | |
see exactly what lightning really is... | 0:43:37 | 0:43:40 | |
CRACK | 0:43:42 | 0:43:43 | |
..a superheated channel of air, with so much energy | 0:43:43 | 0:43:47 | |
that it's become an entirely different form of matter. | 0:43:47 | 0:43:52 | |
We're used to the idea of three states of matter - solid, liquid and | 0:43:55 | 0:43:59 | |
gas, but what we've got here is a fourth, | 0:43:59 | 0:44:01 | |
because the source of all of that light is a plasma. | 0:44:01 | 0:44:05 | |
From the sun's fiery surface | 0:44:10 | 0:44:15 | |
to the clouds of interstellar gas known as nebulae, | 0:44:15 | 0:44:19 | |
plasmas are found across our solar system and beyond. | 0:44:19 | 0:44:23 | |
And it's this superheated form of matter that scientists are hoping | 0:44:25 | 0:44:30 | |
will enable them to unlock a brand-new type of energy... | 0:44:30 | 0:44:33 | |
..by manipulating one of its strangest properties. | 0:44:37 | 0:44:41 | |
This is a Crookes tube, named after the British physicist William | 0:44:43 | 0:44:47 | |
Crookes, who was one of the people to design and use it in the 1870s. | 0:44:47 | 0:44:50 | |
This was the piece of equipment that opened the door to plasma physics. | 0:44:50 | 0:44:55 | |
It's a sealed glass vessel and it's got two electrodes - | 0:44:55 | 0:44:59 | |
the negative one here, and a positive one here. | 0:44:59 | 0:45:02 | |
And on the inside, there's just a little bit of gas | 0:45:02 | 0:45:04 | |
at very low pressure. | 0:45:04 | 0:45:06 | |
And when Crookes turned up the voltage, this is what he saw. | 0:45:08 | 0:45:12 | |
So you can see that this is quite noisy, but there's | 0:45:19 | 0:45:22 | |
a green glow down this end of the tube. | 0:45:22 | 0:45:26 | |
Crookes called this eerie light radiant matter. | 0:45:27 | 0:45:31 | |
Crookes didn't understand what was going on, but we do. | 0:45:34 | 0:45:38 | |
And it's this. | 0:45:38 | 0:45:40 | |
When high voltage is applied across the two electrodes, | 0:45:40 | 0:45:43 | |
it frees up negatively charged electrons from the gas inside | 0:45:43 | 0:45:48 | |
that are then accelerated towards the flat end of the tube. | 0:45:48 | 0:45:52 | |
As they strike the glass, they excite the molecules on the surface, | 0:45:54 | 0:45:58 | |
causing them to give off light. | 0:45:58 | 0:46:01 | |
And it's the free movement of electrons like this that is the | 0:46:04 | 0:46:07 | |
defining characteristic of a plasma. | 0:46:07 | 0:46:09 | |
And which gives it one of its most distinctive properties. | 0:46:11 | 0:46:14 | |
I've got a magnet here, just a small one. | 0:46:16 | 0:46:18 | |
When I bring the magnet in here, you can see that beam of electrons is | 0:46:18 | 0:46:23 | |
being pushed to one side or the other. | 0:46:23 | 0:46:25 | |
It's being deflected by the magnet. | 0:46:25 | 0:46:28 | |
So I can actually control what's going on inside a plasma, | 0:46:31 | 0:46:35 | |
using electric and magnetic fields, | 0:46:35 | 0:46:37 | |
and that is what makes a plasma really interesting. | 0:46:37 | 0:46:40 | |
It's this in-built electromagnetism that's opened up the possibility of | 0:46:46 | 0:46:52 | |
one day channelling the enormous energy inside super hot plasma | 0:46:52 | 0:46:57 | |
and putting it to use... | 0:46:57 | 0:46:58 | |
..by exploiting here on Earth a different source of energy, | 0:47:00 | 0:47:05 | |
the very same type of energy that powers our sun. | 0:47:05 | 0:47:09 | |
Inside a vast hangar at the Culham Science Centre near Oxford | 0:47:19 | 0:47:24 | |
sits a machine so complex | 0:47:24 | 0:47:26 | |
it contains well over 100,000 separate parts. | 0:47:26 | 0:47:30 | |
This is a fusion reactor. | 0:47:32 | 0:47:35 | |
Its job is to channel streams of extremely hot plasma and use them | 0:47:35 | 0:47:41 | |
to manipulate matter at the atomic scale. | 0:47:41 | 0:47:43 | |
The aim is to unleash the power of the atom itself and reach | 0:47:48 | 0:47:53 | |
the holy grail of physics. | 0:47:53 | 0:47:55 | |
Nuclear fusion. | 0:47:57 | 0:47:58 | |
There's no way anyone would be this close to a fusion reactor if it was | 0:48:06 | 0:48:10 | |
running because it throws off enormous numbers of neutrons | 0:48:10 | 0:48:13 | |
which can do a lot of damage and that's why everything | 0:48:13 | 0:48:16 | |
around me here is surrounded in concrete, three metres thick. | 0:48:16 | 0:48:19 | |
Just at the moment, they're in a maintenance phase, | 0:48:19 | 0:48:22 | |
so we can get a little bit closer. | 0:48:22 | 0:48:24 | |
Here to give me a tour of the reactor is Dr Joanne Flanagan. | 0:48:25 | 0:48:30 | |
What exactly is it that all of this kit is trying to do? | 0:48:31 | 0:48:35 | |
We are essentially trying to create an artificial star. | 0:48:35 | 0:48:37 | |
Actually, we do, we create artificial stars. | 0:48:37 | 0:48:40 | |
We take hydrogen gas and heat it up to very high temperatures, where it | 0:48:45 | 0:48:49 | |
becomes ionised, it becomes a plasma. | 0:48:49 | 0:48:52 | |
What sort of temperatures does it reach on the inside there? | 0:48:52 | 0:48:55 | |
We routinely reach temperatures of about 100 million degrees, | 0:48:55 | 0:48:58 | |
which is about ten times hotter than the centre of the sun. | 0:48:58 | 0:49:01 | |
That's just a ludicrous number! | 0:49:01 | 0:49:03 | |
It's a number you can't even get your head around. | 0:49:03 | 0:49:05 | |
It's a crazy hot temperature. We need such high temperatures | 0:49:05 | 0:49:08 | |
because hydrogen nuclei repel each other. | 0:49:08 | 0:49:10 | |
To get them to stick, we need them to collide at high speed. | 0:49:10 | 0:49:13 | |
And that's fundamentally what temperature is. | 0:49:13 | 0:49:16 | |
High-speed particles. | 0:49:16 | 0:49:17 | |
Right, how do you make any thing that hot? | 0:49:17 | 0:49:20 | |
The first step is to run a current through the plasma, | 0:49:20 | 0:49:23 | |
like an old-style electrical light bulb. | 0:49:23 | 0:49:26 | |
And that gets us to a few tens of millions of degrees. | 0:49:26 | 0:49:29 | |
But then we need to pull additional heating systems online to boost us | 0:49:32 | 0:49:36 | |
-the rest of the way. -So you're just throwing everything at it | 0:49:36 | 0:49:39 | |
to get energy into it. | 0:49:39 | 0:49:41 | |
Since there's no material on Earth that can withstand temperatures | 0:49:42 | 0:49:46 | |
of 100 million degrees, the scientists instead | 0:49:46 | 0:49:51 | |
contain the plasma by using its electromagnetism. | 0:49:51 | 0:49:55 | |
At the heart of the reactor lies a giant metal doughnut called a | 0:49:58 | 0:50:04 | |
tokamak that uses a powerful magnetic field to keep the plasma | 0:50:04 | 0:50:09 | |
confined long enough for the collisions | 0:50:09 | 0:50:11 | |
that cause fusion to happen. | 0:50:11 | 0:50:13 | |
To show me how it works, Jo takes me inside a full-sized mock-up. | 0:50:15 | 0:50:21 | |
The plasma would be in the space that we're in here and the magnetic | 0:50:21 | 0:50:24 | |
fields, where do they go? | 0:50:24 | 0:50:26 | |
The magnetic fields curve around in the shape of the vessel. | 0:50:26 | 0:50:31 | |
They have a sort of onion-like structure and they hold the plasma | 0:50:31 | 0:50:34 | |
to the shape of this vessel, | 0:50:34 | 0:50:36 | |
about five centimetres away from the edges. | 0:50:36 | 0:50:38 | |
And the plasma is then here in the middle, is it? | 0:50:38 | 0:50:41 | |
Right where you are. | 0:50:41 | 0:50:43 | |
As all this plasma is heated up, | 0:50:43 | 0:50:46 | |
so the hydrogen nuclei inside accelerate, | 0:50:46 | 0:50:49 | |
getting faster and faster until they reach a speed where they can get | 0:50:49 | 0:50:54 | |
close enough to fuse. | 0:50:54 | 0:50:56 | |
So, once you've had a successful collision, what happens next? | 0:50:59 | 0:51:02 | |
Then you have a very fast neutron that comes out of that reaction. | 0:51:02 | 0:51:07 | |
So it's the neutrons that are carrying the energy out is their | 0:51:07 | 0:51:11 | |
-speed. -Yes. -That will go flying off and it will heat something up. | 0:51:11 | 0:51:15 | |
Yeah. | 0:51:15 | 0:51:16 | |
The idea is that you would have a lithium blanket surrounding the | 0:51:20 | 0:51:24 | |
entire device which would capture | 0:51:24 | 0:51:25 | |
those neutrons and heat up, and you'd have heat | 0:51:25 | 0:51:28 | |
exchanger pipes that run through that blanket that would then heat | 0:51:28 | 0:51:32 | |
water to drive the steam turbines. | 0:51:32 | 0:51:34 | |
But if we're ever to master the searing temperatures of fusion, | 0:51:38 | 0:51:43 | |
then there's one major obstacle that still has to be overcome. | 0:51:43 | 0:51:47 | |
Because for now at least, we've yet to find a way of getting | 0:51:50 | 0:51:53 | |
more energy out from a fusion reactor... | 0:51:53 | 0:51:56 | |
..than we put in. | 0:51:58 | 0:51:59 | |
Fusion is such an enticing idea - there's no shortage of fuel, | 0:52:06 | 0:52:10 | |
there's almost no pollution, it would solve so many problems. | 0:52:10 | 0:52:13 | |
But impressive as all of this is, | 0:52:14 | 0:52:16 | |
it might not be the technology that crosses the line first. | 0:52:16 | 0:52:21 | |
Several years ago, | 0:52:21 | 0:52:23 | |
an idea came along that it might be possible to generate fusion in a | 0:52:23 | 0:52:27 | |
tiny bubble of gas inside a liquid. | 0:52:27 | 0:52:29 | |
Theory had predicted that by collapsing a bubble of gas | 0:52:32 | 0:52:35 | |
incredibly quickly, it might be possible to get the molecules inside | 0:52:35 | 0:52:41 | |
to heat up enough for fusion to occur. | 0:52:41 | 0:52:43 | |
But it couldn't be made to work in practice. | 0:52:44 | 0:52:47 | |
And the idea was discredited. It was basically thrown away. | 0:52:49 | 0:52:53 | |
But some new science has been done | 0:52:53 | 0:52:55 | |
and bubbles are back in the world of fusion. | 0:52:55 | 0:52:58 | |
Just up the road from the reactor | 0:53:07 | 0:53:09 | |
is one of the companies behind this technique. | 0:53:09 | 0:53:12 | |
And I've come to meet its co-founder, Dr Nick Hawker. | 0:53:15 | 0:53:19 | |
So, Nick, what's your solution to the problem of fusion? | 0:53:22 | 0:53:25 | |
The idea is instead of trying to hold the plasma together with | 0:53:25 | 0:53:29 | |
magnetic fields, you use an implosion of some kind | 0:53:29 | 0:53:32 | |
to both compress and heat the plasma. | 0:53:32 | 0:53:35 | |
And how do you set that up? How does that work in practice? | 0:53:35 | 0:53:38 | |
This is a plastic target. | 0:53:38 | 0:53:40 | |
In the middle is a little spherical cavity. | 0:53:40 | 0:53:42 | |
And then what we have is a high velocity projectile. | 0:53:42 | 0:53:45 | |
That comes in and it hits this side here. | 0:53:45 | 0:53:47 | |
That creates an enormously high pressure on this surface. | 0:53:47 | 0:53:50 | |
So the idea is that when you compress the gas in there, | 0:53:50 | 0:53:52 | |
because you do it so quickly, it heats up, | 0:53:52 | 0:53:54 | |
and that's where the energy comes from? | 0:53:54 | 0:53:56 | |
That's right, yeah. | 0:53:56 | 0:53:58 | |
The plasma exists for a few hundred nanoseconds. | 0:53:58 | 0:54:00 | |
To heat the pocket of gas inside the target, | 0:54:03 | 0:54:06 | |
Nick and his team hit it with a projectile, | 0:54:06 | 0:54:09 | |
travelling at almost 30,000 kilometres per hour. | 0:54:09 | 0:54:12 | |
SIREN | 0:54:15 | 0:54:17 | |
-Is everything armed? -Everything is now armed. | 0:54:17 | 0:54:20 | |
Three, two, one, fire. | 0:54:22 | 0:54:24 | |
By filming the moment of impact with high-speed cameras set to record | 0:54:29 | 0:54:34 | |
at a billion frames per second, | 0:54:34 | 0:54:36 | |
the team have been able to capture the precise moment the plasma forms. | 0:54:36 | 0:54:41 | |
On the left of the screen is the view of the gas pocket from side on. | 0:54:45 | 0:54:49 | |
And on the right, the view from behind. | 0:54:51 | 0:54:53 | |
So you can see the shock - | 0:54:53 | 0:54:55 | |
this dark stuff here is the shock coming through. | 0:54:55 | 0:54:58 | |
That's the first shock which goes into the gas and even that is enough | 0:54:58 | 0:55:02 | |
to heat it a lot and it starts to turn... | 0:55:02 | 0:55:04 | |
Well, it turns into a plasma and starts to glow. | 0:55:04 | 0:55:06 | |
As the projectile strikes the target, | 0:55:08 | 0:55:11 | |
the gas collapses in on itself, | 0:55:11 | 0:55:13 | |
causing the molecules inside to heat up so violently that they emit | 0:55:13 | 0:55:19 | |
a light, briefly turning into a plasma. | 0:55:19 | 0:55:22 | |
It's beautiful, isn't it? You get this bright light | 0:55:24 | 0:55:27 | |
and it's a circle and then it becomes a ring | 0:55:27 | 0:55:29 | |
and the centre of it goes dark. | 0:55:29 | 0:55:31 | |
It's a very pretty way of doing it, isn't it? | 0:55:33 | 0:55:36 | |
This beautiful circle that appears out of nowhere. | 0:55:36 | 0:55:38 | |
And what sort of temperatures are reached in here? | 0:55:38 | 0:55:40 | |
Average temperature is something like | 0:55:40 | 0:55:42 | |
in the tens of thousands of Kelvin. | 0:55:42 | 0:55:45 | |
So this isn't hot enough for fusion, but you can... | 0:55:50 | 0:55:53 | |
If you hit it faster, can you reach the temperatures you need? | 0:55:53 | 0:55:56 | |
Yes, it's all about the velocity. | 0:55:56 | 0:55:58 | |
We think we need to go two or three times faster than this gun. | 0:55:58 | 0:56:01 | |
So we're looking at electromagnetically launching | 0:56:01 | 0:56:03 | |
a projectile to try to get to higher and higher velocities | 0:56:03 | 0:56:07 | |
and then to the temperatures we need for fusion. | 0:56:07 | 0:56:10 | |
But potentially you can get a huge amount of energy out of it, | 0:56:10 | 0:56:12 | |
-if it works. -Well, a cavity this size, | 0:56:12 | 0:56:15 | |
if you burned all the fuel in there, | 0:56:15 | 0:56:17 | |
that would release about the same amount of energy as a barrel of oil, | 0:56:17 | 0:56:19 | |
so it's an enormous amount of energy. | 0:56:19 | 0:56:22 | |
I think it's very likely that fusion energy, | 0:56:29 | 0:56:32 | |
this technology made possible by fantastically high temperatures, | 0:56:32 | 0:56:36 | |
will form a significant power source in the future of our civilisation, | 0:56:36 | 0:56:40 | |
but the exciting thing about it is | 0:56:40 | 0:56:42 | |
that we don't know which path it's going to take. | 0:56:42 | 0:56:46 | |
This is the adventure of science and engineering. | 0:56:46 | 0:56:49 | |
Even though there's not yet one clear solution, | 0:56:52 | 0:56:55 | |
when it comes to fusion, the game is afoot. | 0:56:55 | 0:56:58 | |
In this series, | 0:57:04 | 0:57:05 | |
we've learned how nothing would exist without temperature. | 0:57:05 | 0:57:08 | |
From the searing heat of the early Earth | 0:57:09 | 0:57:14 | |
to the cooling that transformed it and allowed life to flourish, | 0:57:14 | 0:57:19 | |
temperature has been fundamental to the story of our planet. | 0:57:19 | 0:57:23 | |
But it has also driven our story. | 0:57:26 | 0:57:29 | |
As our understanding of temperature has grown, | 0:57:31 | 0:57:34 | |
so we've learned how to use it... | 0:57:34 | 0:57:37 | |
..to create new materials, | 0:57:39 | 0:57:42 | |
drive our machines... | 0:57:42 | 0:57:44 | |
..and to advance our technology. | 0:57:46 | 0:57:49 | |
Temperature is such a big idea, encapsulated in just one number. | 0:57:50 | 0:57:56 | |
As a physicist, it's the first thing I measure. | 0:57:56 | 0:57:59 | |
And as a human, it's the first thing I feel. | 0:57:59 | 0:58:02 | |
And yet our direct experience | 0:58:02 | 0:58:04 | |
of temperature is limited to a really narrow range. | 0:58:04 | 0:58:07 | |
But once you learn about what's beyond that, the extreme | 0:58:07 | 0:58:11 | |
heat, the extreme cold, and all the subtleties in between, | 0:58:11 | 0:58:14 | |
it's clear that the possibilities that temperature offers are endless. | 0:58:14 | 0:58:19 |