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On scales far beyond human
perception
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00:00:13,360 --> 00:00:16,320
there are strange beasts...
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..exquisite palaces...
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00:00:19,920 --> 00:00:22,120
..wondrous landscapes.
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00:00:23,520 --> 00:00:28,360
Some just a few thousandths
of a millimetre long.
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00:00:28,360 --> 00:00:32,840
Others dominate
the vast expanses of the cosmos.
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00:00:34,440 --> 00:00:37,320
Thanks to ground-breaking
new technologies,
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I'm setting out to explore these
hidden worlds for the first time.
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You're looking at the craters
and bumps and hills
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on the skin of bacteria.
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Mind-blowing to look at that.
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Each one of these dots is a galaxy.
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We have an instrument here that
allows you to look at an atom.
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We can block the Covid-19
virus itself. Yeah.
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And at the tiniest
and the largest scales,
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I'll see how physics
has bizarre consequences.
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My journey will take me to
the frontiers of modern science,
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revealing our latest discoveries and
our biggest unanswered questions.
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This is the story
of how the universe works
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at scales we can't normally see,
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from nanoparticles,
to galactic superclusters.
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These are the very first images ever
recorded of the microscopic world.
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They appeared
in a book called Micrographia,
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written by the 17th century
scientist Robert Hooke,
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using the first microscopes.
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Even at this magnification,
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they seem so unfamiliar.
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With Micrographia,
three-and-a-half centuries ago,
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Hooke started us off
on a voyage of discovery,
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into the universe
at ever-smaller scales.
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As we began to see
the microscopic world,
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we realised that it's very different
from our own.
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These tiny insects have evolved
extraordinary adaptations
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to navigate the world
at scales we can barely imagine,
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because, when you're this small,
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the laws of physics
have unexpected consequences.
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This is a type of wasp
called Megaphragma,
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one of the smallest
flying insects in the world.
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It's just a few tenths
of a millimetre long,
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some five or ten times
smaller than a flea.
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It has wings like paddles..
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..and flies in an unusual way.
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That's because air feels
very different to it
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than it does to us. We're barely
aware of the air around us
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as we move through it.
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And that's because of
the science of air resistance.
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Take a golf ball
and a ping-pong ball.
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It's easier to throw a golf ball
than a ping-pong ball.
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They both have the same surface area
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and so feel the same air resistance.
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But the ping-pong ball is lighter,
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with less momentum and struggles
to push through the air.
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Megaphragma is like
a tiny ping-pong ball,
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with little momentum
for its surface area,
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so, to it, the air
feels more like a liquid
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and it's evolved its unusually
shaped wings to swim through it.
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If you were to make this
the size of a human,
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then it'd be barely able
to move its wings,
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let alone use them to fly.
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00:04:26,080 --> 00:04:31,000
Yet, it's so successively adapted to
the world in which it exists that,
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in recent years, entomologists
have found them all over the world,
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from Africa to the Pacific
to South America,
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even in the woods outside London.
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When we look at even tinier objects,
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ten times smaller than Megaphragma,
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we come to the scale
of a typical animal cell.
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00:04:51,400 --> 00:04:53,920
As we increase magnification,
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the laws of physics
become ever more strange.
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00:05:02,440 --> 00:05:06,160
Professor Susan Anderson
at the University of Nottingham
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uses powerful optical microscopes
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to study human heart cells.
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So, what is it we're seeing there?
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So, this is the sort of detail
that we get in a light microscope.
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We have lots of
individual cells here,
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so we can see individual cells.
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In each you can see nuclei.
So these are the nuclei.
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The little bright spots
are the nucleoli.
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This is the edge of the cell,
and then the cytoplasm of the cell,
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you can't really see
any detail inside.
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So, why is it
that you're looking at these?
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The useful thing about this
is that we can see dynamic cells,
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so the cells that we're looking at
here are human heart muscle cells.
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So we can actually see them beating.
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Oh, wow, right, yes. Yeah.
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Seeing them beat in such detail
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means scientists can begin
to understand why they go wrong.
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You can see the nucleus, you can
see the outline of the cell here.
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You can see lots of them beating
at about 30 beats per minute,
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00:06:02,440 --> 00:06:05,640
which is about half the rate
of a human heart.
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They're from a living heart?
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00:06:07,640 --> 00:06:10,960
It would be difficult to do that
ethically so what we do is
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we obtain stem cells
from human skin.
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We reprogram the human skin cells
back to stem cells
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and then we direct them down
a differentiation pathway
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to being muscle cells
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and we can obviously see
that they are contracting
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and beating like
a heart muscle cell.
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What's actually happening here?
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The cytoplasm contains
lots of contractile filaments
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and they're shortening and
lengthening so that the cell beats.
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There's a whole community of cells
here that are talking to each other
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and they're passing that signal
from cell to cell
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and they're beating on mass.
How does it make you feel
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when you're looking at
these living cells? I love them.
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They've got personality. You know,
they do what they want.
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If the light here is too bright
they will just move,
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they will just walk away.
They're very entertaining.
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00:07:00,400 --> 00:07:04,160
Microscopes are key
to understanding cells,
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because right across
the living world,
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they're tiny compared
to most everyday objects.
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For instance, a 200-tonne blue whale
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and a tiny Megaphragma are both made
of cells that are similar in size,
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roughly between 100th
and a 10th of a millimetre across.
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Why are cells this size?
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The answer lies in the fact
that in certain crucial ways,
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small things are much more effective
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at interacting with
the outside world than big things.
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Here is a lump of titanium.
It's a very reactive metal,
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and I'm going to try and burn it.
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Nothing.
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But here is also titanium
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that has been crushed down
into a powder.
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00:08:08,800 --> 00:08:12,160
Powder titanium
has far more of its surface,
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relative to its volume,
exposed to the air,
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so it's got much more access
to the oxygen in the air
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to help it burn.
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This applies to cells, too.
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Cells absorb nutrients
and oxygen from the outside.
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Being small and, therefore,
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having a large
surface area to volume ratio,
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means they can do this very
effectively.
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If they were significantly larger,
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they wouldn't be able to take in
what they need to survive.
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Ultimately, though, there's
a limit to how small they can be.
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Cells are full of stuff -
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the nucleus, mitochondria,
ribosomes -
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so it's a balance between
making them small enough
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to maximise their
surface area to volume ratio,
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00:09:02,000 --> 00:09:05,640
yet big enough for their parts
to perform their function.
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00:09:07,400 --> 00:09:10,240
And their shape is crucial, too.
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For instance, some cells have found
a way to increase surface area
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without changing volume.
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The cells in the walls
of our digestive tract
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absorb the nutrients needed
to sustain our entire body
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through their surface,
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so this surface needs to be
as large as possible.
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How do they do this?
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How can cells maximise
their surface to volume ratio
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without getting any smaller?
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Well, imagine this balloon
is one of those cells.
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How can I increase its surface area
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without making it
significantly smaller? Well...
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..I can give it fingers.
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I've calculated these five fingers
increase the surface area
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00:10:00,000 --> 00:10:03,480
of this rubber glove by about 50%
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and, remarkably, evolution has
adopted precisely this strategy.
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Welcome to my digestive tract.
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These protuberances
are called microvilli.
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They're each about a
1,000th of a millimetre long,
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but just a few molecules wide,
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and there are millions of them.
They stick out from the cells,
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dramatically increasing
their surface area,
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and therefore their ability
to absorb nutrients.
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Of course, the real thing
is rather more impressive.
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Scientists have calculated that,
because of the microvilli,
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our intestines have increased their
surface area by up to 15 times.
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Modern optical microscopes
have uncovered a strange world
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just a few thousandths
of a millimetre in scale.
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A world very different
from our own.
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All revealed by a device that is
essentially remarkably simple.
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This is a modern but pretty basic
compound microscope,
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and it works on the same principles
as Robert Hooke's microscope
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from 400 years ago.
It's so simple, really,
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because you just have two lenses,
one in front of the other,
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and adjust them until you get
this sharp, magnified image.
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The second lens multiplies
the magnification of the first.
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There is, however, a fundamental
problem with optical microscopes.
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As we increase magnification,
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images get more and more blurry.
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00:12:11,040 --> 00:12:13,680
This is because light is a wave,
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so objects which are smaller
than its wavelength
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are impossible to see clearly,
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which means
optical microscopes hit a wall
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at about 1,000th of a millimetre.
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So the next step downwards
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means ditching light entirely
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and finding something else
to see with,
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like tiny subatomic particles.
Electrons.
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I've found a bit of old technology,
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something older viewers
might recognise.
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I've taken the back off
this old TV set,
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so what you can see here
is called a cathode-ray tube.
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This bit, the cathode,
boils off electrons
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which are then accelerated
in a vacuum
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00:13:01,840 --> 00:13:05,280
to hit the phosphorous screen
at the front.
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00:13:07,160 --> 00:13:09,480
Now, ordinarily on a TV set,
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the electron beam scans across
the whole surface of the screen
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00:13:13,880 --> 00:13:16,680
to produce the picture.
But I've rigged this now
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so that it produces just a single,
narrow beam of electrons
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00:13:20,080 --> 00:13:21,840
forming a spot in the middle.
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00:13:21,840 --> 00:13:24,240
Now, because electrons
are negatively charged,
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they're affected
by a magnetic field.
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00:13:26,720 --> 00:13:29,520
In fact, that's how we control
the direction of the beam.
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00:13:29,520 --> 00:13:33,400
And to show that, I've got a small
magnet at the end of this stick,
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which I can use to distort
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00:13:37,280 --> 00:13:40,480
and move the direction of the beam.
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In fact, you can see
it's produced three spots.
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00:13:46,440 --> 00:13:48,760
That's because there are
three electron beams,
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00:13:48,760 --> 00:13:51,160
because this is a colour TV.
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00:13:51,160 --> 00:13:53,480
Now I've got it working normally.
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The electron beam is scanning across
the whole screen
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to produce the full picture.
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00:13:58,120 --> 00:14:02,440
But I can still distort
this picture using my magnet.
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00:14:11,360 --> 00:14:14,360
So, if magnets can be used
to control and direct
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00:14:14,360 --> 00:14:16,360
the path of an electron beam,
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00:14:16,360 --> 00:14:19,560
they can also be used
to focus a beam of electrons,
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00:14:19,560 --> 00:14:21,920
in the same way that a glass lens
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00:14:21,920 --> 00:14:24,280
can be used to focus
a beam of light.
219
00:14:24,280 --> 00:14:27,440
And this means that we can
use electrons
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00:14:27,440 --> 00:14:30,080
to make an electron microscope.
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00:14:44,040 --> 00:14:47,960
This is a modern electron
microscope and, in many ways,
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00:14:47,960 --> 00:14:52,280
it resembles Robert Hooke's optical
microscope from 400 years ago.
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00:14:52,280 --> 00:14:55,040
But this one uses
a beam of electrons,
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00:14:55,040 --> 00:14:57,960
just like in the back
of that old TV set.
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00:14:59,640 --> 00:15:02,240
Here's where the electron beam
is generated.
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00:15:02,240 --> 00:15:05,400
Electromagnetic lenses
focus the beam here.
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00:15:05,400 --> 00:15:07,920
This is where the object is placed.
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00:15:07,920 --> 00:15:12,120
More lenses here magnify the image
thousands of times.
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00:15:12,120 --> 00:15:15,560
And this is a screen
which turns the electron image
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00:15:15,560 --> 00:15:17,760
into something we can see.
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00:15:17,760 --> 00:15:19,240
With microscopes like this,
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00:15:19,240 --> 00:15:22,400
scientists were suddenly able
to see objects hundreds,
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00:15:22,400 --> 00:15:26,760
even thousands of times smaller than
they'd ever been able to before.
234
00:15:28,680 --> 00:15:33,440
We could see tiny details
on the bodies of insects
235
00:15:33,440 --> 00:15:38,360
and the machinery within cells
that made them function.
236
00:15:38,360 --> 00:15:44,160
And then we came face-to-face
with one of our deadliest enemies.
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00:15:47,280 --> 00:15:52,400
This is an infectious
bronchitis virus.
238
00:15:52,400 --> 00:15:55,480
And these are common cold viruses.
239
00:15:56,520 --> 00:15:59,760
On them, you can see
something strange,
240
00:15:59,760 --> 00:16:04,320
a kind of halo
surrounding the virus.
241
00:16:04,320 --> 00:16:06,840
They were, in fact, tiny spikes,
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00:16:06,840 --> 00:16:11,040
each one just 100 millionth
of a metre across,
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00:16:11,040 --> 00:16:13,720
and they gave the virus
a crown shape.
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00:16:13,720 --> 00:16:16,640
So they named this
new class of viruses
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00:16:16,640 --> 00:16:19,200
after the corona of the sun.
246
00:16:19,200 --> 00:16:22,400
These are all coronaviruses.
247
00:16:25,240 --> 00:16:31,880
In 2020, electron microscopes
helped to identify a new virus -
248
00:16:31,880 --> 00:16:36,480
SARS-CoV-2, or Covid-19.
249
00:16:40,760 --> 00:16:45,440
Professor Pippa Hawes
studies viruses like Covid-19
250
00:16:45,440 --> 00:16:47,280
for the Pirbright Institute.
251
00:16:47,280 --> 00:16:51,920
How have electron microscopes
allowed us to understand Covid-19?
252
00:16:51,920 --> 00:16:55,120
They've been crucial because
they've allowed us to investigate
253
00:16:55,120 --> 00:16:58,480
the structure of the virus,
so we can actually identify it.
254
00:16:58,480 --> 00:17:02,640
So here we have
the Covid-19 virus itself. Yeah.
255
00:17:02,640 --> 00:17:05,920
We can see the spike protein very,
very clearly here,
256
00:17:05,920 --> 00:17:07,520
around the outside of the virus.
257
00:17:07,520 --> 00:17:10,280
And inside is the viral RNA.
258
00:17:11,760 --> 00:17:17,840
Like all viruses, Covid needs to
hijack another cell to reproduce.
259
00:17:17,840 --> 00:17:20,880
What does the virus do
inside the cell?
260
00:17:20,880 --> 00:17:23,280
It takes over the cell machinery.
261
00:17:23,280 --> 00:17:27,280
The RNA gets placed inside
the cytoplasm of the cell.
262
00:17:27,280 --> 00:17:30,560
This RNA is read
by the cellular machinery
263
00:17:30,560 --> 00:17:33,200
and it's translated
into viral proteins
264
00:17:33,200 --> 00:17:36,400
that the virus is using
in order to replicate.
265
00:17:36,400 --> 00:17:39,320
So, by giving it its RNA,
266
00:17:39,320 --> 00:17:42,400
the virus is basically
reprogramming the cell
267
00:17:42,400 --> 00:17:45,640
to get it to do its bidding.
Yes, exactly.
268
00:17:48,200 --> 00:17:53,680
Incredibly, we can now see
exactly how this happens.
269
00:17:53,680 --> 00:17:57,600
What are we looking at here? Where's
the cell and where's the virus?
270
00:17:57,600 --> 00:18:00,960
The outside of the cell is outside
of our field of view. Oh, OK, right.
271
00:18:00,960 --> 00:18:04,160
Yeah. So this is zooming in now
on an infected cell.
272
00:18:04,160 --> 00:18:08,480
These are parts of the cell
that the virus has taken over
273
00:18:08,480 --> 00:18:12,080
and formed into these
double-membrane vesicles.
274
00:18:12,080 --> 00:18:15,960
So, these vesicles, then, are like
the viruses' nest that it builds,
275
00:18:15,960 --> 00:18:18,760
to make a home for itself
so that it can replicate?
276
00:18:18,760 --> 00:18:20,840
Yes, exactly.
It's sometimes called a factory.
277
00:18:20,840 --> 00:18:24,160
It's where it produces more copies
of the viral proteins,
278
00:18:24,160 --> 00:18:25,760
it produces more of the RNA
279
00:18:25,760 --> 00:18:28,240
and where it all comes together
in the new viruses.
280
00:18:28,240 --> 00:18:32,840
And can we see the individual
viruses? Yes, if we go...
281
00:18:32,840 --> 00:18:34,240
Ooh.
282
00:18:34,240 --> 00:18:36,960
Here, these two are viruses
283
00:18:36,960 --> 00:18:40,120
that are actually budding
into this vesicle,
284
00:18:40,120 --> 00:18:42,720
so these are forming viruses.
285
00:18:42,720 --> 00:18:47,200
Sneaky. Yes!
And so, understanding this,
286
00:18:47,200 --> 00:18:50,480
I mean, does it allow us,
then, to combat Covid-19?
287
00:18:50,480 --> 00:18:53,320
We need to know
how the virus infects,
288
00:18:53,320 --> 00:18:55,480
how it replicates and how it leaves,
289
00:18:55,480 --> 00:18:59,960
which would help with antiviral
treatments to prevent the disease.
290
00:19:02,000 --> 00:19:05,480
Seeing things at this scale
has revealed
291
00:19:05,480 --> 00:19:09,360
an incredible new world
to scientists.
292
00:19:24,680 --> 00:19:29,320
They could see and begin to
understand how genetics worked
293
00:19:29,320 --> 00:19:32,760
by seeing single chromosomes.
294
00:19:32,760 --> 00:19:37,400
They could watch a white blood cell
attacking an infection.
295
00:19:37,400 --> 00:19:40,080
And they could now see
beyond the living world,
296
00:19:40,080 --> 00:19:44,120
deep into the materials
that surround us.
297
00:19:45,760 --> 00:19:48,640
How cracks move through metals.
298
00:19:53,000 --> 00:19:58,400
Then, in 1991,
a group in Japan saw this -
299
00:19:58,400 --> 00:20:03,040
strange shapes forming
at the end of a sparking filament.
300
00:20:04,960 --> 00:20:08,040
Ten times smaller than a virus.
301
00:20:08,040 --> 00:20:11,000
They were carbon nanotubes,
302
00:20:11,000 --> 00:20:13,120
each a long cylinder
303
00:20:13,120 --> 00:20:17,360
whose walls were just
a single carbon atom thick.
304
00:20:17,360 --> 00:20:20,600
And they had unexpected properties,
305
00:20:20,600 --> 00:20:25,240
which has led to an explosion
of fascinating new materials.
306
00:20:27,240 --> 00:20:31,520
This is one of the blackest
materials in the world.
307
00:20:31,520 --> 00:20:34,600
See, it might look to you
like a flat black square
308
00:20:34,600 --> 00:20:37,360
but, in fact,
if you look at it side on,
309
00:20:37,360 --> 00:20:41,000
or even at the back, you can see
it's got contours, it's got dents.
310
00:20:41,000 --> 00:20:43,400
And yet, looking at it face on,
311
00:20:43,400 --> 00:20:46,280
there's nothing,
just pure blackness.
312
00:20:47,960 --> 00:20:49,880
Now, normally when we see objects,
313
00:20:49,880 --> 00:20:52,640
light bounces off of them
into our eyes
314
00:20:52,640 --> 00:20:54,800
at different wavelengths
and different angles
315
00:20:54,800 --> 00:20:59,480
so we can see colour and shape. But
this is like a Harry Potter spell.
316
00:20:59,480 --> 00:21:03,520
Light falls on the surface
and then just disappears forever.
317
00:21:05,200 --> 00:21:07,320
What's perhaps most surprising
318
00:21:07,320 --> 00:21:11,440
is that this paint
is made of nanotubes.
319
00:21:14,320 --> 00:21:16,520
The paint, called Vantablack,
320
00:21:16,520 --> 00:21:20,760
is the invention of nanotechnology
scientist Ben Jensen.
321
00:21:23,320 --> 00:21:25,680
So it just looks like
a black surface here,
322
00:21:25,680 --> 00:21:29,320
but talk me through
what it looks like if you zoom in.
323
00:21:29,320 --> 00:21:32,280
So, if you imagine
a forest of trees,
324
00:21:32,280 --> 00:21:34,720
but the trees are thousands
of metres tall
325
00:21:34,720 --> 00:21:37,440
and they're all straight
and they're all equally spaced.
326
00:21:37,440 --> 00:21:39,760
So light comes in, photons come in,
327
00:21:39,760 --> 00:21:42,160
and they effectively bounce
between the trees
328
00:21:42,160 --> 00:21:44,600
and then they're absorbed
after a number of bounces.
329
00:21:44,600 --> 00:21:46,600
So, as you can see on here,
330
00:21:46,600 --> 00:21:50,160
it looks like a very,
very thick, lush carpet.
331
00:21:50,160 --> 00:21:53,760
So light coming in gets in between
the nanotubes and bounces around
332
00:21:53,760 --> 00:21:56,960
and is eventually absorbed
into the substrate.
333
00:21:56,960 --> 00:21:59,680
It looks like a brush. Yes, exactly.
334
00:22:03,320 --> 00:22:07,040
I want to get across to you just
how black this material is.
335
00:22:08,280 --> 00:22:10,480
This card has been painted
with the blackest
336
00:22:10,480 --> 00:22:12,320
commercially available paint.
337
00:22:12,320 --> 00:22:14,840
It's called Black 3.0.
338
00:22:14,840 --> 00:22:17,120
And, yeah, it looks very black.
339
00:22:17,120 --> 00:22:20,640
But put it alongside the Vantablack,
340
00:22:20,640 --> 00:22:23,520
and if I shine a light on them,
341
00:22:23,520 --> 00:22:27,360
you can see the paint
just looks grey in comparison.
342
00:22:27,360 --> 00:22:29,080
And even more impressive,
343
00:22:29,080 --> 00:22:33,200
if I make an angle so that
the light bounces off the surface
344
00:22:33,200 --> 00:22:34,960
and hopefully into the camera,
345
00:22:34,960 --> 00:22:38,280
you can see that this paint
looks a lot brighter
346
00:22:38,280 --> 00:22:40,320
because the light
has been reflected.
347
00:22:40,320 --> 00:22:43,320
But if I do the same thing
with the Vantablack,
348
00:22:43,320 --> 00:22:45,640
you should see no difference at all.
349
00:22:45,640 --> 00:22:49,520
All the light is being absorbed.
None of it is reflected.
350
00:22:52,000 --> 00:22:56,960
What is it useful for? So its main
uses are in satellite systems,
351
00:22:56,960 --> 00:22:59,520
for controlling
stray light from the sun,
352
00:22:59,520 --> 00:23:02,000
the moon and the Earth
when you're looking out at stars.
353
00:23:02,000 --> 00:23:04,280
It's also used for calibrating
infrared cameras
354
00:23:04,280 --> 00:23:07,920
that look at the Earth for global
warming studies. And terrestrially,
355
00:23:07,920 --> 00:23:11,760
it's used to protect cars
with autonomous driving modes
356
00:23:11,760 --> 00:23:13,880
from sunlight
entering the camera systems
357
00:23:13,880 --> 00:23:16,560
and causing ghosting
and loss of signal.
358
00:23:19,160 --> 00:23:21,760
For me,
this is an entirely unexpected
359
00:23:21,760 --> 00:23:26,720
and surprising property of nanotubes
and, more importantly,
360
00:23:26,720 --> 00:23:32,040
this is nanotechnology that
we can see. Or, rather, not see.
361
00:23:33,600 --> 00:23:36,920
Glimpsing tiny nanotubes
was impressive,
362
00:23:36,920 --> 00:23:39,400
but could we go even further?
363
00:23:39,400 --> 00:23:44,320
By the 1980s, scientists were
trying to see ever smaller things,
364
00:23:44,320 --> 00:23:47,040
using a completely different
approach.
365
00:23:47,040 --> 00:23:50,920
They wondered if they could
see by feeling.
366
00:23:50,920 --> 00:23:54,000
Basically, the idea was
to mimic the way the needle
367
00:23:54,000 --> 00:23:56,040
on an old record player works.
368
00:24:01,000 --> 00:24:04,480
A stylus passes along a groove
on a record
369
00:24:04,480 --> 00:24:07,800
and the tiny bumps
vibrate the needle,
370
00:24:07,800 --> 00:24:09,880
making music.
371
00:24:09,880 --> 00:24:11,880
MUSIC PLAYS
372
00:24:11,880 --> 00:24:12,920
MUSIC STOPS
373
00:24:14,040 --> 00:24:17,720
But, of course, the tip
of a record player stylus
374
00:24:17,720 --> 00:24:21,920
is far too big to feel something
as small as an atom.
375
00:24:21,920 --> 00:24:25,160
But then, in 1982, two scientists -
376
00:24:25,160 --> 00:24:28,000
Heinrich Rohrer and Gerd Binnig -
377
00:24:28,000 --> 00:24:30,000
had an ingenious idea.
378
00:24:30,000 --> 00:24:34,520
They put a thin metal spike
into a corrosive liquid.
379
00:24:34,520 --> 00:24:36,120
Using electrical currents,
380
00:24:36,120 --> 00:24:39,600
they slowly dissolved away
the tip of the spike
381
00:24:39,600 --> 00:24:43,040
so that just a very thin needle
of metal remained.
382
00:24:43,040 --> 00:24:46,720
Its tip was just
a few atoms in diameter.
383
00:24:48,000 --> 00:24:51,040
But how could this needle see?
384
00:24:51,040 --> 00:24:55,120
One idea was to harness
an unusual force of nature.
385
00:24:57,640 --> 00:24:59,800
This is a gecko.
386
00:24:59,800 --> 00:25:04,000
Its feet stick to the glass
using a tiny attractive force
387
00:25:04,000 --> 00:25:06,240
called the van der Waals force.
388
00:25:09,000 --> 00:25:13,240
Van der Waals forces exist
because of a rather quirky aspect
389
00:25:13,240 --> 00:25:15,640
of atoms and molecules.
390
00:25:15,640 --> 00:25:19,200
Think of an atom as a tiny
positively charged nucleus
391
00:25:19,200 --> 00:25:23,360
surrounded by a cloud
of negatively charged electrons.
392
00:25:25,640 --> 00:25:29,600
But, crucially,
these electron clouds aren't static,
393
00:25:29,600 --> 00:25:33,440
they fluctuate in shape,
often randomly.
394
00:25:33,440 --> 00:25:35,720
So the clouds can become lopsided,
395
00:25:35,720 --> 00:25:38,840
with more electrons on one side
than on the other.
396
00:25:40,800 --> 00:25:43,520
Because opposite charges attract,
397
00:25:43,520 --> 00:25:45,720
the negative end of one molecule
398
00:25:45,720 --> 00:25:48,800
is pulled towards
the positive end of another.
399
00:25:48,800 --> 00:25:53,160
The force that an individual atom
feels is, of course, minuscule.
400
00:25:53,160 --> 00:25:56,640
But these effects can add up.
401
00:25:56,640 --> 00:26:00,000
And this, in turn, means that
the molecules on the surface
402
00:26:00,000 --> 00:26:02,080
of an object can sometimes
403
00:26:02,080 --> 00:26:07,120
feel pulled towards the molecules
on the surface of a nearby object.
404
00:26:09,000 --> 00:26:12,800
And that's what the gecko
is taking advantage of.
405
00:26:14,000 --> 00:26:18,720
A gecko's feet are covered
with billions of tiny structures
406
00:26:18,720 --> 00:26:20,520
called spatulae.
407
00:26:21,760 --> 00:26:24,040
When these press against the glass,
408
00:26:24,040 --> 00:26:28,120
they flatten out,
creating a huge surface area.
409
00:26:30,520 --> 00:26:33,640
Billions of atoms
are now in contact.
410
00:26:37,720 --> 00:26:40,080
Then the tiny van der Waals forces
411
00:26:40,080 --> 00:26:43,920
combine and hold the gecko in place.
412
00:26:43,920 --> 00:26:46,080
And this was one of the forces
413
00:26:46,080 --> 00:26:50,360
Binnig and Rohrer
believed they could harness.
414
00:26:50,360 --> 00:26:52,440
When a tiny stylus -
415
00:26:52,440 --> 00:26:55,920
and remember, its tip
is just a few atoms wide -
416
00:26:55,920 --> 00:26:59,000
approaches atoms on the surface
of the material,
417
00:26:59,000 --> 00:27:02,000
this is when the van der Waals
forces come into play.
418
00:27:02,000 --> 00:27:05,560
Just like the spatulae
on the foot of a gecko
419
00:27:05,560 --> 00:27:09,400
feels an attractive force between it
and the molecules on the surface
420
00:27:09,400 --> 00:27:14,440
of the glass, so the stylus
feels a force pulling it towards
421
00:27:14,440 --> 00:27:19,560
or pushing it away from the atoms
as it passes over the surface.
422
00:27:20,680 --> 00:27:24,800
Measuring minuscule forces
like these can paint a picture
423
00:27:24,800 --> 00:27:27,880
of the surface at the tiniest scale.
424
00:27:29,120 --> 00:27:32,440
This is a modern
atomic force microscope.
425
00:27:33,720 --> 00:27:36,120
Dr Georgina Benn is using it
426
00:27:36,120 --> 00:27:39,080
to understand
one of our deadliest enemies.
427
00:27:40,360 --> 00:27:43,400
I'm going to be imaging E coli,
428
00:27:43,400 --> 00:27:45,000
which are a type of bacteria.
429
00:27:45,000 --> 00:27:48,520
So, with a normal microscope, we
could look at just the bacteria.
430
00:27:48,520 --> 00:27:51,200
But we need our atomic force
microscope to be able to see
431
00:27:51,200 --> 00:27:52,440
the details on the surface.
432
00:27:53,720 --> 00:27:56,160
Why are we looking at
the surface of E coli?
433
00:27:56,160 --> 00:27:59,680
So, E coli are really good
at resisting antibiotics
434
00:27:59,680 --> 00:28:02,120
because they have this extra
protective layer
435
00:28:02,120 --> 00:28:05,360
around the outside, and we want to
know how the protective layer
436
00:28:05,360 --> 00:28:09,040
is arranged so that we can help
people design antibiotics
437
00:28:09,040 --> 00:28:12,840
that can get through the protective
layer more efficiently.
438
00:28:12,840 --> 00:28:16,800
So this is the full cell?
The full bacteria? Yeah.
439
00:28:16,800 --> 00:28:21,320
So you can sort of start to see
features on the surface.
440
00:28:23,200 --> 00:28:28,280
And these are already well below
optical microscopy kind of sizes.
441
00:28:28,280 --> 00:28:31,840
Right. My scan's going to be
500 nanometres wide.
442
00:28:31,840 --> 00:28:35,200
So we're now looking at the surface
of the bacteria? Yes. Yes.
443
00:28:35,200 --> 00:28:38,480
This is really impressive.
444
00:28:38,480 --> 00:28:41,120
What we're looking at here
is bacteria skin
445
00:28:41,120 --> 00:28:43,920
and, you know, you're looking at
the craters and bumps
446
00:28:43,920 --> 00:28:46,800
and hills on the skin of bacteria,
447
00:28:46,800 --> 00:28:51,920
to find these weak spots
that we can attack with antibiotics.
448
00:28:53,920 --> 00:28:58,080
Each one of these black spots
is a hole on the bacteria,
449
00:28:58,080 --> 00:29:02,520
which is about three millionths
of a millimetre wide.
450
00:29:02,520 --> 00:29:06,600
These are the holes
that let water and nutrients
451
00:29:06,600 --> 00:29:09,040
in and out of the cell. Right.
452
00:29:09,040 --> 00:29:12,840
So we're looking at how they're
arranged, relative to each other.
453
00:29:12,840 --> 00:29:14,640
And what's interesting is that
454
00:29:14,640 --> 00:29:18,560
we've got this really tight lattice
of pores.
455
00:29:18,560 --> 00:29:21,960
And then sometimes there are these
gaps in your lattice.
456
00:29:21,960 --> 00:29:25,920
So those are the weak spots?
We don't know. Oh, OK.
457
00:29:25,920 --> 00:29:28,480
So we want to know...
That's, like, a next question -
458
00:29:28,480 --> 00:29:32,880
why these are important, why they
would be there in the first place?
459
00:29:32,880 --> 00:29:38,120
So we know that some kind of patches
will make the membrane weaker.
460
00:29:39,480 --> 00:29:41,080
And some of them will not.
461
00:29:41,080 --> 00:29:44,400
So, if you could get
the bacteria to mutate
462
00:29:44,400 --> 00:29:48,680
so that it generates these weak
spots... Yeah, or maybe...
463
00:29:48,680 --> 00:29:52,080
..then you can attack it?
Yes, or maybe get a drug
464
00:29:52,080 --> 00:29:56,680
that will make these weak spots,
and then we could apply antibiotic.
465
00:30:01,000 --> 00:30:03,120
With the atomic force microscope,
466
00:30:03,120 --> 00:30:07,760
we began to see more detail
of the world than ever before.
467
00:30:07,760 --> 00:30:10,520
But it had its limitations.
468
00:30:10,520 --> 00:30:15,320
They are most effective at seeing
features on a flat surface.
469
00:30:16,960 --> 00:30:19,880
But atoms also connect up
in three dimensions,
470
00:30:19,880 --> 00:30:22,720
often forming very complicated
shapes which, in turn,
471
00:30:22,720 --> 00:30:24,680
affects their behaviour.
472
00:30:24,680 --> 00:30:27,880
How, then, can we see these shapes?
473
00:30:27,880 --> 00:30:32,440
Remember how visible light has a
limit because of its wavelength?
474
00:30:32,440 --> 00:30:35,200
Well, it turns out
there's another form of light
475
00:30:35,200 --> 00:30:38,200
which has a much, much smaller
wavelength.
476
00:30:42,600 --> 00:30:44,320
X-rays.
477
00:30:44,320 --> 00:30:47,680
Crucially,
X-rays have very short wavelength
478
00:30:47,680 --> 00:30:51,360
when compared to visible light. Now,
the wavelengths of visible lights
479
00:30:51,360 --> 00:30:54,360
are just under
a millionth of a metre
480
00:30:54,360 --> 00:30:55,960
but the wavelengths of X-rays
481
00:30:55,960 --> 00:30:59,000
are typically
several thousand times shorter,
482
00:30:59,000 --> 00:31:02,600
at around a tenth
of a billionth of a metre.
483
00:31:04,520 --> 00:31:06,920
But there are many differences.
484
00:31:06,920 --> 00:31:09,400
Our eyes can't detect X-rays.
485
00:31:09,400 --> 00:31:11,800
More importantly, they pack a punch.
486
00:31:11,800 --> 00:31:15,600
X-rays contain much more energy
than rays of visible light.
487
00:31:15,600 --> 00:31:20,000
The intense energy of X-rays
enables them to pass unhindered
488
00:31:20,000 --> 00:31:23,040
through soft tissue,
like flesh and blood,
489
00:31:23,040 --> 00:31:28,920
which is as transparent to X-rays
as glass is to visible light.
490
00:31:28,920 --> 00:31:33,560
The larger atoms that make up
our bones do stop X-rays,
491
00:31:33,560 --> 00:31:36,560
so when you see an image like this,
492
00:31:36,560 --> 00:31:39,520
you're literally seeing
an X-ray shadow,
493
00:31:39,520 --> 00:31:43,520
cast by your bones
on photographic paper.
494
00:31:43,520 --> 00:31:45,560
This begs the question,
495
00:31:45,560 --> 00:31:49,600
can X-rays, which have
such short wavelengths,
496
00:31:49,600 --> 00:31:54,400
be used to see things that are
just too small for visible light?
497
00:31:55,960 --> 00:31:58,840
The first hints that this
might be possible
498
00:31:58,840 --> 00:32:01,280
came in the early 20th century.
499
00:32:01,280 --> 00:32:06,000
Scientists noticed that when they
shone X-rays through crystals,
500
00:32:06,000 --> 00:32:10,760
they produced weird spots
arranged in patterns.
501
00:32:10,760 --> 00:32:12,920
These images may not
look like much,
502
00:32:12,920 --> 00:32:15,000
but think of them as a kind of code.
503
00:32:15,000 --> 00:32:19,120
And by crackling it,
you can deduce the way the atoms
504
00:32:19,120 --> 00:32:21,680
in the crystal are arranged.
505
00:32:21,680 --> 00:32:24,920
This process of turning images
like these into an understanding
506
00:32:24,920 --> 00:32:29,000
of how substances are structured
down at the atomic scale
507
00:32:29,000 --> 00:32:31,400
is known as X-ray crystallography.
508
00:32:35,400 --> 00:32:38,560
For a sense of how
X-ray crystallography works,
509
00:32:38,560 --> 00:32:41,080
let's say each of these
Christmas trees
510
00:32:41,080 --> 00:32:44,800
represents one of the atoms
that makes up the crystal.
511
00:32:44,800 --> 00:32:48,920
To keep it simple, let's say
they're all arranged in neat rows,
512
00:32:48,920 --> 00:32:50,520
just like these trees.
513
00:32:53,960 --> 00:32:57,640
What's important is that
the wavelength of the X-rays
514
00:32:57,640 --> 00:33:01,360
striking the crystal is about
the same as the distance
515
00:33:01,360 --> 00:33:06,360
between the rows of atoms, or the
rows of trees in our analogy.
516
00:33:08,800 --> 00:33:11,920
Imagine an X-ray
reflecting off the surface
517
00:33:11,920 --> 00:33:14,280
and the layer beneath.
518
00:33:14,280 --> 00:33:17,000
The beam that travels down
to the next layer
519
00:33:17,000 --> 00:33:21,040
has a longer journey,
and that is key.
520
00:33:22,760 --> 00:33:25,200
If the waves are now out of step
521
00:33:25,200 --> 00:33:28,760
and the peak of one coincides
with the trough of the other,
522
00:33:28,760 --> 00:33:31,720
they then combine and cancel out.
523
00:33:33,080 --> 00:33:35,400
But if they're in step,
524
00:33:35,400 --> 00:33:37,360
the peaks combine,
525
00:33:37,360 --> 00:33:41,440
making a larger wave
and a bright dot on the screen.
526
00:33:44,520 --> 00:33:46,000
By carefully measuring
527
00:33:46,000 --> 00:33:48,720
the angle at which
the X-rays strike the crystal,
528
00:33:48,720 --> 00:33:51,440
where the dots appear,
where they disappear,
529
00:33:51,440 --> 00:33:54,280
you can deduce the structure
of the crystal.
530
00:33:56,440 --> 00:33:58,880
By decoding images like this,
531
00:33:58,880 --> 00:34:02,320
scientists in the early 20th century
were able to deduce
532
00:34:02,320 --> 00:34:05,720
the structures of simple crystals,
like rock salt.
533
00:34:05,720 --> 00:34:09,160
The atoms are arranged
at each corner of a cube
534
00:34:09,160 --> 00:34:13,400
and the cubes repeat
to form a 3D lattice.
535
00:34:13,400 --> 00:34:16,440
Most importantly, it meant
we now knew the distance
536
00:34:16,440 --> 00:34:20,880
between the atoms. It's a third
of a billionth of a metre.
537
00:34:23,320 --> 00:34:26,840
But for me, the story
of X-ray crystallography
538
00:34:26,840 --> 00:34:28,960
really comes into its own
539
00:34:28,960 --> 00:34:33,160
because of one of the great heroes
of British science -
540
00:34:33,160 --> 00:34:35,920
Dorothy Crowfoot Hodgkin.
541
00:34:37,200 --> 00:34:41,000
At Cambridge and Oxford
in the 1930s and '40s,
542
00:34:41,000 --> 00:34:45,760
Hodgkin became fascinated
by X-ray crystallography
543
00:34:45,760 --> 00:34:50,040
and she quickly established herself
as one of the leading researchers.
544
00:34:52,360 --> 00:34:55,720
Her first big challenge
came during the Second World War
545
00:34:55,720 --> 00:34:58,720
and her work on penicillin.
546
00:34:58,720 --> 00:35:02,400
Scientists had already noticed
that the newly discovered penicillin
547
00:35:02,400 --> 00:35:05,520
had incredible
antibacterial properties.
548
00:35:05,520 --> 00:35:08,240
It could stop infections
in their tracks,
549
00:35:08,240 --> 00:35:11,800
literally bringing patients
back from the brink of death.
550
00:35:11,800 --> 00:35:15,680
Now in the throws of war,
understanding it and producing it
551
00:35:15,680 --> 00:35:18,280
in quantity was more important
than ever.
552
00:35:21,080 --> 00:35:23,920
But penicillin was still a mystery,
553
00:35:23,920 --> 00:35:27,680
with a handful of atoms arranged
in an unknown structure.
554
00:35:27,680 --> 00:35:31,000
So Hodgkin set her laboratory
a challenge -
555
00:35:31,000 --> 00:35:35,160
use X-ray crystallography
to learn its structure.
556
00:35:38,520 --> 00:35:43,560
Georgina Ferry is a science writer
and biographer of Dorothy Hodgkin.
557
00:35:43,560 --> 00:35:44,920
Tell me about penicillin.
558
00:35:44,920 --> 00:35:48,600
What was so difficult about
understanding its structure?
559
00:35:48,600 --> 00:35:51,920
The structure was unknown
and, naturally,
560
00:35:51,920 --> 00:35:54,480
the organic chemists
all came to Dorothy and said
561
00:35:54,480 --> 00:35:58,880
would she like to have a go at this?
The first problem with it was that
562
00:35:58,880 --> 00:36:01,240
it doesn't make terribly
good crystals.
563
00:36:01,240 --> 00:36:05,760
These are not ideal for putting
into the X-ray apparatus.
564
00:36:05,760 --> 00:36:09,200
It took a while before they managed
to get a version of penicillin
565
00:36:09,200 --> 00:36:14,160
that she was able to get
a good image from. That image...
566
00:36:16,960 --> 00:36:18,560
..looks like this.
567
00:36:18,560 --> 00:36:24,000
These are spots on photographic film
that have been made by X-rays
568
00:36:24,000 --> 00:36:27,560
coming out of the crystal
and hitting the photographic film.
569
00:36:27,560 --> 00:36:29,720
The dots are at different
intensities. Some of them
570
00:36:29,720 --> 00:36:32,480
are very black, there's some
down here that are very faint.
571
00:36:32,480 --> 00:36:36,560
And what she had to do
was carry out a complicated
572
00:36:36,560 --> 00:36:38,720
mathematical calculation,
573
00:36:38,720 --> 00:36:42,040
which then enabled her
to begin to understand
574
00:36:42,040 --> 00:36:45,880
where there was
what's known as density
575
00:36:45,880 --> 00:36:47,640
in the molecule and in the crystal.
576
00:36:47,640 --> 00:36:50,840
And density means there's an atom
there. And the final stage
577
00:36:50,840 --> 00:36:54,520
once you've done all those
calculations, is to...
578
00:36:58,600 --> 00:37:02,000
..to...essentially
draw a contour map.
579
00:37:02,000 --> 00:37:04,640
This represents
a slice through the molecule
580
00:37:04,640 --> 00:37:06,920
and the numbers that are
written down
581
00:37:06,920 --> 00:37:09,920
represent the density
of the electrons.
582
00:37:09,920 --> 00:37:13,600
And what she's done is join up
areas of equivalent density,
583
00:37:13,600 --> 00:37:15,880
and that shows you that's a place
where there's an atom,
584
00:37:15,880 --> 00:37:17,840
because there's a lot of
intensity there.
585
00:37:17,840 --> 00:37:19,760
We're looking at a 2D picture here.
586
00:37:19,760 --> 00:37:23,960
So how did Hodgkin then
go to the full 3D structure?
587
00:37:23,960 --> 00:37:27,920
What you want to do
is take a number of slices,
588
00:37:27,920 --> 00:37:31,280
stack those one above the other,
and that'll show you
589
00:37:31,280 --> 00:37:34,280
the three dimensional structure
of the molecule.
590
00:37:37,320 --> 00:37:41,600
So, you can see, what we've got here
is a stack of Perspex sheets
591
00:37:41,600 --> 00:37:43,640
of equal distances apart.
592
00:37:43,640 --> 00:37:47,800
And on each sheet, you've got
the contour lines drawn,
593
00:37:47,800 --> 00:37:49,360
as we were looking at before. Mm.
594
00:37:49,360 --> 00:37:51,240
And if you're looking down
from the top,
595
00:37:51,240 --> 00:37:54,480
you can see the three dimensional
structure.
596
00:37:54,480 --> 00:37:57,920
This is the structure of penicillin
597
00:37:57,920 --> 00:38:02,600
that Hodgkin came up with
after some four years of research.
598
00:38:02,600 --> 00:38:04,880
These are the carbon atoms,
599
00:38:04,880 --> 00:38:08,520
and they're connected by
chemical bonds to other atoms.
600
00:38:08,520 --> 00:38:12,960
Oxygen, hydrogen, nitrogen, sulphur.
601
00:38:12,960 --> 00:38:15,440
But it's this section here
602
00:38:15,440 --> 00:38:19,000
that explains
its incredible efficacy.
603
00:38:19,000 --> 00:38:21,960
It's called a beta-lactam ring
604
00:38:21,960 --> 00:38:26,040
and it seems to give penicillin
its wondrous ability.
605
00:38:26,040 --> 00:38:30,320
It binds to a part of the cell wall
of most bacteria,
606
00:38:30,320 --> 00:38:32,040
killing them dead.
607
00:38:32,040 --> 00:38:37,640
Understanding how penicillin works
was a revolution in medicine.
608
00:38:37,640 --> 00:38:41,400
Hodgkin's work spawned
a generation of new antibiotics,
609
00:38:41,400 --> 00:38:44,640
effective against
many aggressive bacteria,
610
00:38:44,640 --> 00:38:47,680
saving millions of lives.
611
00:38:49,520 --> 00:38:53,400
And these techniques,
still widely used today,
612
00:38:53,400 --> 00:38:57,840
famously went on to unlock
the structure of DNA.
613
00:39:00,640 --> 00:39:04,200
Despite the achievements
of X-ray crystallography,
614
00:39:04,200 --> 00:39:07,680
it was still an indirect method
of seeing,
615
00:39:07,680 --> 00:39:10,040
and only worked for crystals.
616
00:39:10,040 --> 00:39:15,040
To see even smaller things
would require something else.
617
00:39:15,040 --> 00:39:19,760
It seemed electron microscopes
held the most potential,
618
00:39:19,760 --> 00:39:23,520
but they had a huge
technical problem.
619
00:39:23,520 --> 00:39:25,680
Their electromagnetic lenses
620
00:39:25,680 --> 00:39:29,680
were fundamentally different
from glass ones.
621
00:39:29,680 --> 00:39:33,320
One of the most common problems
that affects lenses
622
00:39:33,320 --> 00:39:35,800
is called spherical aberration.
623
00:39:35,800 --> 00:39:38,800
You see, the way lenses work
is that they bend the light
624
00:39:38,800 --> 00:39:42,080
that travels through them.
But the amount of bending
625
00:39:42,080 --> 00:39:45,840
depends on which part of the lens
the light travels through.
626
00:39:47,000 --> 00:39:50,640
So, when I try to focus the sun,
for instance,
627
00:39:50,640 --> 00:39:53,840
I can never quite focus to a point.
628
00:39:53,840 --> 00:39:57,840
Which means,
at high magnifications especially,
629
00:39:57,840 --> 00:40:01,520
parts of the image will always blur.
630
00:40:01,520 --> 00:40:04,920
Electron microscope lenses
are exactly the same,
631
00:40:04,920 --> 00:40:08,520
they also suffer
from spherical aberration.
632
00:40:08,520 --> 00:40:10,520
And at high magnification,
633
00:40:10,520 --> 00:40:14,040
the blurring was making
the images unusable.
634
00:40:14,040 --> 00:40:17,720
Now, for glass lenses,
this issue can be minimised.
635
00:40:17,720 --> 00:40:21,000
You add a second lens,
a concave lens,
636
00:40:21,000 --> 00:40:23,440
which corrects for the first one,
637
00:40:23,440 --> 00:40:26,440
giving us a much sharper point.
638
00:40:26,440 --> 00:40:30,760
But this solution doesn't work
with electron microscopes.
639
00:40:30,760 --> 00:40:33,920
The lenses of electron microscopes
are fundamentally different
640
00:40:33,920 --> 00:40:38,840
from glass ones. There simply is
no equivalent of a concave lens.
641
00:40:38,840 --> 00:40:43,640
The physics of electrons and
electromagnetic fields forbids it.
642
00:40:43,640 --> 00:40:46,040
So it seemed
that electron microscopes
643
00:40:46,040 --> 00:40:48,080
would always suffer from blurriness
644
00:40:48,080 --> 00:40:50,440
at very high levels
of magnification.
645
00:40:56,560 --> 00:41:02,160
The question was whether we could
delve deeper to see even smaller.
646
00:41:02,160 --> 00:41:06,000
Well, the next breakthrough
that changed everything
647
00:41:06,000 --> 00:41:08,360
took place here in Germany.
648
00:41:13,080 --> 00:41:18,720
Two teams of headstrong scientists
started to question the orthodoxy.
649
00:41:18,720 --> 00:41:20,840
There were three in Germany -
650
00:41:20,840 --> 00:41:23,080
Theoretician Harald Rose,
651
00:41:23,080 --> 00:41:25,840
experimentalist Max Haider,
652
00:41:25,840 --> 00:41:28,560
material scientist Knut Urban -
653
00:41:28,560 --> 00:41:33,560
and an American team
led by Ondrej Krivanek.
654
00:41:33,560 --> 00:41:35,680
Everybody expected us to fail,
655
00:41:35,680 --> 00:41:39,040
and so we knew we could
only exceed expectations.
656
00:41:39,040 --> 00:41:43,080
Each stubbornly believed
that they could somehow overturn
657
00:41:43,080 --> 00:41:45,640
the established prevailing science
658
00:41:45,640 --> 00:41:49,040
and make an electron microscope
that could see more.
659
00:41:49,040 --> 00:41:51,640
Perhaps even atoms.
660
00:41:51,640 --> 00:41:56,720
Was it a big challenge, then,
to persuade the science world
661
00:41:56,720 --> 00:42:01,240
that here was something that was
going to change the field?
662
00:42:01,240 --> 00:42:05,520
The science world, at that time,
had essentially given up
663
00:42:05,520 --> 00:42:08,640
to have aberration-corrected
electron optics.
664
00:42:08,640 --> 00:42:13,840
They decided that hardware
aberration correction
665
00:42:13,840 --> 00:42:17,480
will be unthinkable.
They said it was impossible?
666
00:42:17,480 --> 00:42:21,000
That it was impossible.
We had three different people.
667
00:42:21,000 --> 00:42:24,000
Theoretician, experimentalist
and material scientists,
668
00:42:24,000 --> 00:42:26,080
and I think this three together,
669
00:42:26,080 --> 00:42:28,240
that was just a point
for its success.
670
00:42:28,240 --> 00:42:32,160
Their approach used
multiple electron magnets,
671
00:42:32,160 --> 00:42:35,160
multipoles to distort the image,
672
00:42:35,160 --> 00:42:38,040
squeezing out the worst
of the aberration.
673
00:42:38,040 --> 00:42:40,920
Then a second lens
reformed the image,
674
00:42:40,920 --> 00:42:45,120
now almost aberration free. But
getting it right was challenging.
675
00:42:45,120 --> 00:42:48,960
It would require sophisticated
arrangements of multipoles,
676
00:42:48,960 --> 00:42:52,280
sensitive cameras
and powerful computers.
677
00:43:18,200 --> 00:43:19,600
To bring it back again.
678
00:43:22,000 --> 00:43:25,840
For years, they struggled
to get their new lenses to work,
679
00:43:25,840 --> 00:43:29,680
and the rest of the scientific
community remained sceptical.
680
00:43:29,680 --> 00:43:33,520
I had a lovely comment
from a professor at Stanford
681
00:43:33,520 --> 00:43:36,920
who told me, "Ondrej,
you're burying your career."
682
00:43:36,920 --> 00:43:40,400
But then, in June 1997,
683
00:43:40,400 --> 00:43:43,280
their stubbornness
began to pay off.
684
00:43:43,280 --> 00:43:48,280
And soon they caught glimpses of
the building blocks of all matter
685
00:43:48,280 --> 00:43:51,640
with unprecedented clarity.
686
00:43:51,640 --> 00:43:55,400
Here's a typical image
without aberration correction.
687
00:43:55,400 --> 00:43:58,400
Now watch as it's added in.
688
00:43:58,400 --> 00:44:03,000
The white blurs resolve
into two clear dots,
689
00:44:03,000 --> 00:44:07,080
each one a single atom of silicone.
690
00:44:09,960 --> 00:44:12,000
Finally, you could see atoms.
691
00:44:12,000 --> 00:44:14,960
This was a real jump in innovation.
692
00:44:14,960 --> 00:44:17,360
This was a real paradigm change.
693
00:44:17,360 --> 00:44:20,240
What was it like when you saw
those first images?
694
00:44:20,240 --> 00:44:21,800
Seeing is believing,
695
00:44:21,800 --> 00:44:25,360
and the mission impossible
was not impossible.
696
00:44:25,360 --> 00:44:29,560
They had achieved
a scientific miracle.
697
00:44:29,560 --> 00:44:33,120
It was like if you have a huge fog.
698
00:44:33,120 --> 00:44:35,560
But suddenly, the fog goes.
699
00:44:35,560 --> 00:44:37,600
Suddenly, you see everything.
700
00:44:37,600 --> 00:44:40,480
A new kind of electron microscope.
701
00:44:40,480 --> 00:44:43,480
It was brilliant.
It was so unbelievable.
702
00:44:43,480 --> 00:44:48,240
And it's the most important effect
of aberration correction.
703
00:44:48,240 --> 00:44:52,600
By 2020, they'd gone
from academic outcasts
704
00:44:52,600 --> 00:44:56,360
to world-renowned scientists.
705
00:44:56,360 --> 00:44:58,800
The images that came out
are truly spectacular,
706
00:44:58,800 --> 00:45:01,200
like the one on the cover of Nature.
That's kind of like
707
00:45:01,200 --> 00:45:03,600
if you're a model and you get
on the cover of Vogue.
708
00:45:03,600 --> 00:45:08,400
And they had defined
a new kind of science.
709
00:45:08,400 --> 00:45:10,280
I think we are on the way
710
00:45:10,280 --> 00:45:13,800
to make high precision
electron microscopy
711
00:45:13,800 --> 00:45:17,000
a part of science in general.
712
00:45:33,880 --> 00:45:36,880
The next stage
of this journey downwards
713
00:45:36,880 --> 00:45:38,720
happened in Manchester,
714
00:45:38,720 --> 00:45:42,720
with the discovery
of an incredible new material -
715
00:45:42,720 --> 00:45:44,160
graphene.
716
00:45:44,160 --> 00:45:47,680
The new electron microscopes
revealed that graphene
717
00:45:47,680 --> 00:45:52,240
was a sheet of carbon
just a single atom thick.
718
00:45:52,240 --> 00:45:57,440
And incredible strength was just
one of its unexpected properties.
719
00:45:58,760 --> 00:46:03,400
So, just how impressive is graphene?
Well, I've come here to this lab
720
00:46:03,400 --> 00:46:06,000
to carry out what's called
a stress test.
721
00:46:06,000 --> 00:46:08,440
I've got two strips of plastic here.
722
00:46:08,440 --> 00:46:12,480
It's a stretchy polymer. One of them
is just the pure polymer,
723
00:46:12,480 --> 00:46:17,080
the other contains just 3% graphene
mixed in with it.
724
00:46:17,080 --> 00:46:21,360
And I want to stretch them
to find out how much force is needed
725
00:46:21,360 --> 00:46:23,360
to snap these strips.
726
00:46:25,960 --> 00:46:28,640
First up is the pure polymer.
727
00:46:34,920 --> 00:46:37,480
Ah. There we go.
It's gone? It's gone.
728
00:46:37,480 --> 00:46:42,920
So that snapped at...?
533 newtons.
729
00:46:42,920 --> 00:46:44,800
533 newtons.
730
00:46:44,800 --> 00:46:48,720
So that's about two... Two bags
of cement. Two bags of cement.
731
00:46:48,720 --> 00:46:50,840
So now you're going to swap it
with the graphene...
732
00:46:50,840 --> 00:46:52,720
Yes, I'm going to reset...
..implanted one.
733
00:46:52,720 --> 00:46:56,640
..reset the machine
with the graphene ones. OK? OK.
734
00:47:03,720 --> 00:47:04,760
OK.
735
00:47:17,080 --> 00:47:20,200
OK, so it's now hit 500 newtons.
736
00:47:20,200 --> 00:47:24,480
We've now already overtaken
the non-graphene. Yes.
737
00:47:24,480 --> 00:47:29,000
And it looks pretty healthy, as far
as I can tell. It's healthy, yes.
738
00:47:30,400 --> 00:47:34,480
It's coming up to 750 newtons now.
740, 750.
739
00:47:39,400 --> 00:47:43,520
We're now... And now
it's coming up to 1,000 newtons.
740
00:47:43,520 --> 00:47:45,320
And still going strong.
741
00:47:47,880 --> 00:47:49,360
And...
742
00:47:57,800 --> 00:48:00,000
STRIP SNAPS
Oh! So that was about...
743
00:48:00,000 --> 00:48:04,640
So the final force was 1,074.
744
00:48:04,640 --> 00:48:06,360
So that's double.
745
00:48:06,360 --> 00:48:09,320
Twice as much force was needed
to snap this polymer,
746
00:48:09,320 --> 00:48:13,680
compared with the one without the
graphene. That is pretty impressive.
747
00:48:13,680 --> 00:48:16,440
A huge improvement
with just a few percent
748
00:48:16,440 --> 00:48:21,320
of graphene mixed in with the
polymer. Yeah. That's incredible.
749
00:48:22,720 --> 00:48:27,120
Graphene has shaken the scientific
community to its core,
750
00:48:27,120 --> 00:48:30,720
and yet was discovered
almost by chance
751
00:48:30,720 --> 00:48:33,160
by scientist Andre Geim
752
00:48:33,160 --> 00:48:37,240
as he was searching for
ever thinner slithers of graphite.
753
00:48:37,240 --> 00:48:41,000
Talk to me through
what happened on that night,
754
00:48:41,000 --> 00:48:45,000
when you realised your eureka
moment. 20 years ago,
755
00:48:45,000 --> 00:48:48,840
I realised that just
taking Scotch tape,
756
00:48:48,840 --> 00:48:52,840
putting piece of graphite
between the Scotch tape,
757
00:48:52,840 --> 00:48:57,840
peeling the Scotch tape like that,
leaves small pieces of graphite.
758
00:48:57,840 --> 00:48:59,920
Is that something we can
demonstrate here? Yeah.
759
00:48:59,920 --> 00:49:02,000
Because, we have a piece
of graphite. Yeah.
760
00:49:02,000 --> 00:49:07,480
You can take this piece
of graphite...
761
00:49:07,480 --> 00:49:10,600
..and without much trouble...
762
00:49:10,600 --> 00:49:15,360
You can, of course, make it thinner
by repeating this procedure.
763
00:49:15,360 --> 00:49:17,360
But if you shine lights through,
764
00:49:17,360 --> 00:49:22,040
you eventually start finding
flakes which are transparent,
765
00:49:22,040 --> 00:49:24,480
and that actually was
the Eureka moment.
766
00:49:24,480 --> 00:49:27,400
Because being reasonably
well educated,
767
00:49:27,400 --> 00:49:33,280
I realised that if flakes
of graphite are transparent,
768
00:49:33,280 --> 00:49:35,120
they're really, really thin.
769
00:49:35,120 --> 00:49:38,440
Probably initially those were
ten layers thick
770
00:49:38,440 --> 00:49:41,880
but eventually we went down
to a single layer.
771
00:49:45,200 --> 00:49:48,520
It's hard to overstate
just how excited scientists
772
00:49:48,520 --> 00:49:51,000
and engineers are about graphene,
773
00:49:51,000 --> 00:49:54,400
so let me just remind you
what graphene is.
774
00:49:54,400 --> 00:49:58,960
It's just a single flat sheet of
carbon atoms all bonded together.
775
00:49:58,960 --> 00:50:01,320
But that would be really
under-selling it
776
00:50:01,320 --> 00:50:04,320
because at around
a third of a nanometre,
777
00:50:04,320 --> 00:50:07,600
it's just a single
carbon atom thick,
778
00:50:07,600 --> 00:50:11,360
making it the thinnest material
ever made.
779
00:50:11,360 --> 00:50:15,640
For a sense of why graphene
is so extraordinary,
780
00:50:15,640 --> 00:50:19,720
we have to understand its physics
at the atomic scale.
781
00:50:19,720 --> 00:50:23,240
Each sheet is made up
of repeating hexagons.
782
00:50:23,240 --> 00:50:25,480
At each corner is a carbon atom
783
00:50:25,480 --> 00:50:28,760
that's bonded powerfully
to three others.
784
00:50:28,760 --> 00:50:32,680
Those bonds are the source
of the material's strength,
785
00:50:32,680 --> 00:50:36,160
but they also seem to produce
other strange properties.
786
00:50:36,160 --> 00:50:39,280
Each carbon atom bonds
to its three neighbours
787
00:50:39,280 --> 00:50:41,680
by sharing electrons with them.
788
00:50:41,680 --> 00:50:44,160
But not all the electrons
are used for this.
789
00:50:44,160 --> 00:50:47,280
One electron
from each atom is spare.
790
00:50:47,280 --> 00:50:50,840
These free electrons
can zip around unhindered,
791
00:50:50,840 --> 00:50:54,560
and this has huge consequences
because it means that graphene
792
00:50:54,560 --> 00:50:58,720
can be made to conduct electricity
incredibly efficiently.
793
00:50:59,920 --> 00:51:02,960
There are high hopes
that it will enable new kinds
794
00:51:02,960 --> 00:51:05,120
of electronic components,
795
00:51:05,120 --> 00:51:08,960
revolutionising batteries
with much greater storage,
796
00:51:08,960 --> 00:51:11,280
and also solar power generation,
797
00:51:11,280 --> 00:51:16,560
water filtration, material science
and quantum computing.
798
00:51:17,800 --> 00:51:20,200
Of course, this is still
early days in graphene research
799
00:51:20,200 --> 00:51:24,440
but there is, without doubt,
much to play for.
800
00:51:24,440 --> 00:51:29,080
The discovery of graphene brings
us towards the end of this story,
801
00:51:29,080 --> 00:51:30,520
because with the newest
802
00:51:30,520 --> 00:51:33,520
aberration-corrected
electron microscopes,
803
00:51:33,520 --> 00:51:37,560
we're now able to see
on the smallest scales imaginable.
804
00:51:43,440 --> 00:51:45,440
Professor Quentin Ramasse
805
00:51:45,440 --> 00:51:49,480
runs some of the biggest
electron microscopes in the world.
806
00:51:49,480 --> 00:51:52,680
He's going to zoom
into a sample of graphene,
807
00:51:52,680 --> 00:51:56,480
until we can see individual atoms.
808
00:51:56,480 --> 00:51:59,560
OK, what are you going to
show me here?
809
00:51:59,560 --> 00:52:03,840
So, we've prepared some graphene
samples for you.
810
00:52:03,840 --> 00:52:07,800
The samples are on a copper grid
just millimetres wide.
811
00:52:07,800 --> 00:52:12,240
Let me put it here and actually
place it into the sample holder.
812
00:52:12,240 --> 00:52:15,520
That's the three millimetre sample?
That's the three millimetre sample,
813
00:52:15,520 --> 00:52:18,040
and now, hopefully, you can already
see... I can see the grid.
814
00:52:18,040 --> 00:52:20,920
So they're essentially
just copper bars.
815
00:52:23,440 --> 00:52:25,200
Under the optical microscope,
816
00:52:25,200 --> 00:52:28,640
I can just make out holes
in the sheet of carbon
817
00:52:28,640 --> 00:52:31,560
within the grid,
where the graphene flakes are.
818
00:52:31,560 --> 00:52:33,240
To see them in more detail,
819
00:52:33,240 --> 00:52:37,960
he now switches the sample into
a powerful electron microscope.
820
00:52:37,960 --> 00:52:41,120
So what we're looking at now
is the same image
821
00:52:41,120 --> 00:52:43,760
as we had
under the optical microscope?
822
00:52:43,760 --> 00:52:46,520
You can already recognise
there's two shadows here,
823
00:52:46,520 --> 00:52:49,120
the corners of those grid squares.
824
00:52:49,120 --> 00:52:51,640
But in the middle here,
you recognise what you also saw
825
00:52:51,640 --> 00:52:55,000
on the optical microscope,
which are those circle holes,
826
00:52:55,000 --> 00:52:59,920
inside which is the graphene that
we're going to go and look at.
827
00:53:01,800 --> 00:53:06,560
Slowly getting closer
and closer and closer.
828
00:53:06,560 --> 00:53:10,240
We're going to be zooming into
graphene much further in.
829
00:53:10,240 --> 00:53:13,160
Almost gives you vertigo when...
A little bit, yes.
830
00:53:13,160 --> 00:53:15,960
..you realise
how much we're zooming in.
831
00:53:15,960 --> 00:53:17,880
OK, so, what are we looking at here?
832
00:53:17,880 --> 00:53:22,360
This is a patch of graphene
that's about 500 nanometres across.
833
00:53:22,360 --> 00:53:25,520
How does this, then, compare to
the thickness of a human hair?
834
00:53:25,520 --> 00:53:27,720
It would be...?
Several metres across.
835
00:53:27,720 --> 00:53:29,880
Several metres across in diameter?
Yes.
836
00:53:29,880 --> 00:53:32,080
That's how... OK, right.
That's how small it is.
837
00:53:32,080 --> 00:53:34,640
And yet, we're still only
halfway in our journey down.
838
00:53:34,640 --> 00:53:37,600
Not even... Not even halfway.
..of the way there. OK.
839
00:53:37,600 --> 00:53:41,080
And so what we're trying to do,
really, is zoom in even further
840
00:53:41,080 --> 00:53:43,760
on that little black speck.
Go for it.
841
00:53:43,760 --> 00:53:47,800
So we'll start reducing
the magnification slowly.
842
00:53:47,800 --> 00:53:50,760
I'll go to magnify it
ten times this time,
843
00:53:50,760 --> 00:53:53,800
trying to not go too fast
so that you can really keep...
844
00:53:53,800 --> 00:53:55,720
You don't want to spoil
the surprise for me.
845
00:53:55,720 --> 00:53:57,720
You don't want to spoil
the surprise, no.
846
00:54:01,400 --> 00:54:03,640
If you notice,
the shape of this hole,
847
00:54:03,640 --> 00:54:06,240
it's about the shape of Africa,
I would say.
848
00:54:06,240 --> 00:54:10,800
It's now getting to a size that is
more foreign to everyday life,
849
00:54:10,800 --> 00:54:14,760
especially when you start realising
that this patch is going to be
850
00:54:14,760 --> 00:54:17,000
100 times smaller still.
851
00:54:17,000 --> 00:54:19,760
But let's zoom in and hopefully see
852
00:54:19,760 --> 00:54:22,560
what we are here to see,
which are single atoms.
853
00:54:24,200 --> 00:54:25,800
So this is now that same patch,
854
00:54:25,800 --> 00:54:27,680
and you notice that it is very dark.
855
00:54:27,680 --> 00:54:30,640
You might just about start
being able to recognise
856
00:54:30,640 --> 00:54:33,880
some pattern in the middle,
some very faint lines
857
00:54:33,880 --> 00:54:37,360
which correspond to
the hexagonal lattice in graphene.
858
00:54:37,360 --> 00:54:39,880
But if you look closely
on the original image
859
00:54:39,880 --> 00:54:41,880
that we still have on screen here,
860
00:54:41,880 --> 00:54:45,880
you see small, round blobs that are
perhaps a little bit brighter.
861
00:54:45,880 --> 00:54:48,960
And they are brighter because,
those atoms are heavier,
862
00:54:48,960 --> 00:54:50,840
and we happen to know
they're silicone.
863
00:54:50,840 --> 00:54:53,200
But just to demonstrate,
I can move that scan box
864
00:54:53,200 --> 00:54:55,560
around one of those single atoms
and, hopefully,
865
00:54:55,560 --> 00:54:58,000
it'll light up like a Christmas
light in the middle.
866
00:55:00,520 --> 00:55:02,280
And there it is.
867
00:55:02,280 --> 00:55:05,280
Because it is heavier,
it appears brighter on the image.
868
00:55:05,280 --> 00:55:07,840
So that entire bright patch
869
00:55:07,840 --> 00:55:10,600
is a single atom of silicone?
870
00:55:10,600 --> 00:55:15,120
And yet it's a blob, it's a patch.
It's not the picture of an atom
871
00:55:15,120 --> 00:55:17,600
that we learn about at school,
with a nucleus and electrons
872
00:55:17,600 --> 00:55:20,280
buzzing around the outside.
So what is exactly...?
873
00:55:20,280 --> 00:55:24,720
It remains reasonably abstract. What
we see is this average structure
874
00:55:24,720 --> 00:55:29,040
of subatomic particles, and that
gives us this average round shape.
875
00:55:29,040 --> 00:55:32,520
We've magnified this sample
that we've taken out
876
00:55:32,520 --> 00:55:36,960
from a sample box and put into the
microscope by several million times
877
00:55:36,960 --> 00:55:39,080
to see on the screen
this magnification.
878
00:55:39,080 --> 00:55:40,840
So a tenth of a billionth
of a metre.
879
00:55:40,840 --> 00:55:43,280
We've come a long way
since Robert Hooke.
880
00:55:43,280 --> 00:55:45,520
THEY LAUGH
881
00:55:45,520 --> 00:55:48,000
For me, as a theoretical physicist,
882
00:55:48,000 --> 00:55:51,160
an atom is just abstract
mathematics -
883
00:55:51,160 --> 00:55:56,200
an equation, an idea. But to see
one of them with my own eyes,
884
00:55:56,200 --> 00:55:58,360
the building blocks of everything,
885
00:55:58,360 --> 00:56:01,600
just ten millionths
of a millimetre across,
886
00:56:01,600 --> 00:56:04,120
is nothing less than miraculous.
887
00:56:04,120 --> 00:56:08,040
I still can't get my head
around the fact
888
00:56:08,040 --> 00:56:11,440
that I'm looking at
individual atoms.
889
00:56:11,440 --> 00:56:14,160
Well, look, I'll tell you. Yeah.
890
00:56:14,160 --> 00:56:19,680
I mean, I've spent my career
studying atomic nuclei,
891
00:56:19,680 --> 00:56:22,400
but, for me,
it's always been abstract.
892
00:56:22,400 --> 00:56:28,640
The notion that we're looking at
an individual atom here...
893
00:56:28,640 --> 00:56:30,360
And I love the analogy
894
00:56:30,360 --> 00:56:34,560
that there are more atoms
in a single glass of water
895
00:56:34,560 --> 00:56:39,640
than there are glasses of water in
all the oceans of the world, right?
896
00:56:39,640 --> 00:56:43,640
Atoms are tiny. They are tiny.
The fact that we have an instrument
897
00:56:43,640 --> 00:56:47,800
here that allows you
to look at an atom...
898
00:56:47,800 --> 00:56:50,720
I... The novelty doesn't wear off?
899
00:56:50,720 --> 00:56:52,480
It definitely doesn't, no.
900
00:56:52,480 --> 00:56:55,320
I might be either simple-minded
or single-minded,
901
00:56:55,320 --> 00:56:58,680
but seeing those single atoms is,
902
00:56:58,680 --> 00:57:01,840
I think, something I'll want to do
for the rest of my life.
903
00:57:01,840 --> 00:57:04,760
And it's just
a wonderful thing to see.
904
00:57:14,320 --> 00:57:18,960
We've now entered a realm in which
we can see individual atoms,
905
00:57:18,960 --> 00:57:23,160
and it's leading us into a new world
of single atom physics,
906
00:57:23,160 --> 00:57:27,080
chemistry, biology,
engineering and medicine.
907
00:57:27,080 --> 00:57:32,480
It's all so new that it's impossible
to say where it's going to take us.
908
00:57:32,480 --> 00:57:35,960
But as we learn more
about our world,
909
00:57:35,960 --> 00:57:38,480
from insects, to cells,
910
00:57:38,480 --> 00:57:40,960
to the atoms that make us,
911
00:57:40,960 --> 00:57:45,040
I know there'll be
many more wonders to discover.
912
00:57:46,480 --> 00:57:49,160
Next time, I go big.
913
00:57:49,160 --> 00:57:53,920
As I journey from our solar system
out to galactic superclusters,
914
00:57:53,920 --> 00:57:57,680
I'll confront the biggest mysteries
in our universe.
74040
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