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00:00:00
- This is one of the most powerful jet engines in the world,
00:00:03
and it actually runs
00:00:04
at temperatures 250 degrees Celsius hotter
00:00:07
than the melting point of the materials that make it up.
00:00:09
- [Assistant] That's 1,200 degrees.
00:00:11
- So the question is, why doesn't a jet engine
00:00:14
just melt into a puddle? (intense music)
00:00:16
(jet hovering) - We are right at the boundaries of the laws of physics
00:00:21
(intense music) - That is wild.
00:00:22
It's at the same temperature now as it would be inside
00:00:25
the jet engine.
00:00:26
But here, they're liquid. (dramatic music)
00:00:28
- Every time I get on a plane,
00:00:29
I'm thinking, "This is never gonna work."
00:00:31
- And yet, it does work.
00:00:33
Right now, there are over 10,000 planes in the sky powered
00:00:37
by engines just like these.
00:00:39
Maybe you are on one right now.
00:00:41
So, how do they work?
00:00:45
(energetic music) (jet humming) This is a jet engine, specifically a turbofan engine.
00:00:49
At the front is this giant fan.
00:00:51
During takeoff, these rotating blades push 1.3 tons
00:00:55
of air backwards every second,
00:00:57
and around 10% of that air gets compressed.
00:01:00
The compressors force the air
00:01:02
into increasingly narrow chambers.
00:01:04
They compress the air
00:01:05
to about 50 times atmospheric pressure.
00:01:08
And just by doing that, the air heats up
00:01:10
to around 600 degrees Celsius.
00:01:13
This compressed air is then forced
00:01:15
into the combustion chamber,
00:01:16
where fuel is sprayed in through a ring of nozzles
00:01:19
and ignited. (flames blasting)
00:01:21
That chemical reaction gives off a lot of heat.
00:01:24
So the temperature jumps to around 1,500 degrees Celsius.
00:01:28
So now you've got this high-pressure gas from the combustor
00:01:30
that just wants to expand,
00:01:32
and now it's got an incredible amount of thermal energy.
00:01:36
But between the combustion chamber
00:01:37
and the outside air is this. (intense music)
00:01:40
Rows of turbine blades. (blades humming)
00:01:42
So, in order for the gas to expand and get out,
00:01:44
it needs to push these turbine blades out of the way.
00:01:47
And in pushing the blades, that is
00:01:49
how it transfers its energy to the engine.
00:01:52
This is where all the power really comes from
00:01:55
in modern jets on takeoff,
00:01:57
each high-pressure turbine blade is generating as much power
00:02:00
as a Formula 1 car. (car droning)
00:02:02
And there are 68 of them.
00:02:04
(lively music) As the gas rushes through the turbine and nozzle,
00:02:07
its pressure drops from around 50 atmospheres down to one,
00:02:09
and it expands by almost 20 times.
00:02:12
And that spins these turbine blades up
00:02:14
to 12,500 revolutions per minute.
00:02:18
The fan that is pushing all that air backward
00:02:20
and all those compressors that squeeze the air down,
00:02:22
all of that is powered by the turbines back here.
00:02:26
It's a kind of funny, really counterintuitive way
00:02:29
to think about an engine.
00:02:30
It's what's happening in the back
00:02:32
that's actually driving everything up front.
00:02:35
(pensive music) As the hot exhaust gas is shot out the back of the engine,
00:02:39
it pushes the engine forward.
00:02:41
That generates thrust.
00:02:43
But did you know that in a modern passenger jet,
00:02:45
this accounts for less than 20% the thrust of the engine?
00:02:49
The vast majority of the thrust, over 80% of it, just comes
00:02:52
from that big fan at the front of the jet.
00:02:55
(numbers beeping)
00:02:56
Remember how only 10% of the incoming air gets compressed?
00:02:59
The other 90% bypasses all that.
00:03:02
It's simply propelled backwards by the fan.
00:03:04
It goes right around the guts of the engine
00:03:06
and comes straight out the back.
00:03:08
The fan pushes that air backwards,
00:03:10
so the air pushes the fan forwards.
00:03:13
That's how you get 80% of the thrust.
00:03:15
It's basically a huge ducted propeller.
00:03:18
(jet hovering) So, why do it this way?
00:03:20
I mean, why not compress all the incoming air
00:03:23
and put it all through the combustion chamber and turbines?
00:03:27
(flames blasting) Well, some fighter jets do exactly this,
00:03:30
and it makes for very powerful engines,
00:03:32
but they're also horribly inefficient.
00:03:35
To see why, remember that the impulse pushing
00:03:37
the plane forward is equal to the change
00:03:39
in the momentum of the air backwards.
00:03:42
So you've got options.
00:03:43
For example, you could push twice
00:03:45
as much air back half as fast,
00:03:47
or you could push half as much air back twice as fast.
00:03:51
Both will generate the exact same impulse,
00:03:53
but the kinetic energy of the air is proportional
00:03:56
to v squared.
00:03:58
So it takes four times as much energy
00:04:00
to speed up the air in the second case,
00:04:02
and a lot of that energy is just wasted in the exhaust.
00:04:05
So, ideally, you want to push as much air backwards
00:04:08
as possible with only a small change in velocity.
00:04:13
(enchanted music) That's why jets have gotten bigger
00:04:14
and bigger over the years,
00:04:16
and the increasing fraction
00:04:18
of bypass air has the added benefit
00:04:20
that it surrounds the hot exhaust gases,
00:04:23
and that reduces noise coming away from the jet.
00:04:26
But there is another major factor when it comes
00:04:28
to engine efficiency, and that is temperature.
00:04:31
At cruising altitudes around 35,000 feet,
00:04:34
the outside air is around negative 55 degrees Celsius,
00:04:38
while inside the engine, it's over 1,500 degrees Celsius.
00:04:42
The hot, high-pressure gas inside the engine wants
00:04:44
to expand into the much colder, lower-pressure air outside.
00:04:49
It's that difference that lets the engine turn heat
00:04:51
into useful work. (ominous music)
00:04:53
But there's a fundamental limit
00:04:54
to how much work any heat engine can get from that.
00:04:57
It's called the Carnot efficiency.
00:04:59
It's equal to one minus the temperature
00:05:01
of the cold outside air divided by the temperature
00:05:04
of the hot gas inside the combustion chamber.
00:05:07
(ominous music) So, looking at this, you can improve the efficiency
00:05:10
of the engine in two ways,
00:05:12
either fly where the air is colder
00:05:14
or raise the temperature in the combustion chamber.
00:05:17
One problem with that, though, is that it turned the inside
00:05:20
of a jet engine into one
00:05:22
of the harshest environments we have ever built
00:05:25
in which machinery has to survive.
00:05:28
- To keep a turbine blade whole
00:05:30
and unaffected within an engine is like putting an ice cube
00:05:32
inside your oven, turning up to max, leaving for work,
00:05:35
coming back after an eight-hour shift,
00:05:36
and finding it's still completely frozen in the oven.
00:05:38
That's what we've got to try and do within that engine.
00:05:40
- It sounds absurd.
00:05:42
(intense music) Not only do the turbine blades sit
00:05:44
in a stream of gas that's over 1,500 degrees Celsius,
00:05:47
they're also spinning at 12,500 RPM
00:05:51
with the tip of each blade slicing
00:05:53
through the air at nearly 1,900 kilometers per hour.
00:05:57
Now, every blade wants to fly straight,
00:05:59
but it's forced to spin in a circle,
00:06:02
which means, something has
00:06:03
to be constantly pulling it inwards.
00:06:05
That's the centripetal force.
00:06:07
If you take a representative 300 gram
00:06:09
high-pressure turbine blade and run it at that speed
00:06:12
and radius, it has to be pulled inwards with a force equal
00:06:15
to the weight of 20 metric tons.
00:06:17
That's roughly the weight
00:06:18
of two London double-decker buses tugging on each blade
00:06:22
as it spins, all while they're glowing hot.
00:06:26
(ominous music) To make matters worse, at these temperatures, oxygen wants
00:06:29
to react with the metal of the blades itself.
00:06:32
And on top of all that, the air rushing
00:06:34
through the engine often carries dust, sand,
00:06:37
and pollutants that can damage
00:06:38
and erode the surfaces inside.
00:06:41
And somehow, these blades have to survive this punishment
00:06:44
for tens of thousands
00:06:46
of flight hours without deforming, cracking, or failing.
00:06:50
They really determine how efficient you can make the engine
00:06:53
because you can't make the engine so hot
00:06:55
that the blades can't withstand that temperature.
00:06:58
So they determine the maximum temperature
00:07:00
of the combustion chamber,
00:07:01
and therefore, the maximum efficiency you can realize
00:07:04
with a jet engine.
00:07:06
So what kind
00:07:07
of metal could possibly survive these conditions?
00:07:10
Well, we sent Veritasium producer, Emilia,
00:07:13
to the Department of Materials Science & Metallurgical
00:07:15
at Cambridge University
00:07:16
to put some different metals to the test.
00:07:19
(ominous music) - So this is the steel?
00:07:20
This is the steel sample, yes.
00:07:21
- Okay. - So we've got
00:07:22
about 200 megapascals to start with,
00:07:24
which is sort of comparable to some of the stress
00:07:27
that's seen by these components in real applications.
00:07:30
And we're gonna put that stress on,
00:07:32
and then slowly increase the temperature.
00:07:34
- [Derek] This is a mild steel.
00:07:36
It's relatively strong and easy to form into complex shapes.
00:07:39
It seems like a pretty good bet for a turbine blade.
00:07:41
And at first, under this load
00:07:43
and at these low temperatures, it holds up pretty well.
00:07:46
We're essentially tugging on all the atoms within the metal.
00:07:49
We're not breaking or forming any bonds.
00:07:52
We're just making them flex a little.
00:07:53
And that slightly changes the spacing between the atoms.
00:07:56
And as a result, the metal gets slightly longer.
00:07:59
This resulting change in size,
00:08:01
specifically the per-unit change in length,
00:08:03
is what we call strain.
00:08:05
Critically, at this stage,
00:08:06
the material is behaving elastically.
00:08:08
If we remove the load right now,
00:08:10
the material just snaps back to its original size.
00:08:14
In an engine, some elastic deformation like this will occur.
00:08:17
It can't be too big or it'll cause problems.
00:08:20
But what we really don't want is plastic deformation
00:08:23
if the shape changes permanently.
00:08:26
And that's exactly what starts to happen
00:08:28
as we keep increasing the temperature.
00:08:30
- [Howard] It's getting hot now.
00:08:31
That's a little bit of oxide.
00:08:35
(ominous music) There you go, see this starting to deform?
00:08:38
- [Derek] Now, bonds are breaking
00:08:40
and reforming as the metal at us deforms permanently.
00:08:45
(ominous music)
00:08:46
But this doesn't happen all at once.
00:08:48
So I got the mechanical engineer on our team,
00:08:50
Henry, to build this demo.
00:08:53
(ominous music) - Okay, so you can see we're getting a bunch
00:08:55
of tiny little bubbles, and just naturally,
00:08:57
they're packing into this hexagonal arrangement.
00:09:00
And there are actually a lot of materials
00:09:01
that have atomic structures just like this.
00:09:03
But you can see it's not perfect.
00:09:05
Like, right here,
00:09:06
you can see there's an extra half-plane of atoms.
00:09:09
Well, in this case, bubbles,
00:09:11
this is called an edge dislocation.
00:09:16
(ominous music)
00:09:17
It becomes really interesting when I try
00:09:19
to pull this raft apart.
00:09:21
(ominous music)
00:09:22
You can see these little dark lines that zip back and forth.
00:09:25
Those are dislocations, and they move through the lattice.
00:09:28
As the dislocation moves, it'll cause one plane, a bubbles,
00:09:32
to sheer past the other one, which shifts the structure
00:09:34
by exactly one spacing.
00:09:36
But there isn't just one dislocation.
00:09:39
There are plenty of them.
00:09:40
And altogether, their movement produces dramatic changes
00:09:42
in the overall shape.
00:09:45
(ominous music) - [Derek] That's exactly what's happening here.
00:09:47
Everywhere that stress is high enough,
00:09:49
billions of dislocations are moving and interacting.
00:09:52
The steel starts to deform continuously
00:09:54
under this constant load in a process called creep.
00:09:57
It takes energy to break the atomic bonds
00:10:00
as the dislocation travels through the lattice.
00:10:02
So, as we ramp up the temperature
00:10:03
and all the atoms get more thermal energy,
00:10:06
it no longer requires as much stress to break these bonds,
00:10:09
becomes much easier for the dislocations to move.
00:10:12
The metal effectively gets softer.
00:10:14
Now the steel strength drops so much
00:10:17
that the slow, time-dependent creep gives way
00:10:19
to rapid deformation.
00:10:21
As it stretches, it rapidly decreases in cross-section,
00:10:25
and eventually, the remaining metal can no longer bear
00:10:27
the load. (ominous music)
00:10:30
Now, you could try doing similar tests
00:10:32
for other metals like this titanium alloy.
00:10:36
(ominous music) Titanium is about half as dense as steel.
00:10:38
- Should feel that's quite a bit lighter.
00:10:39
- Yeah, it's like loads lighter.
00:10:41
- [Derek] So if we were to make turbine blades out
00:10:43
of titanium, each blade would be much lighter,
00:10:45
and that would reduce
00:10:46
the enormous centripetal forces it would experience.
00:10:49
So it seems like a great choice.
00:10:51
And at first, it performs really well.
00:10:53
- That's 100 degrees.
00:10:54
It's hanging in there.
00:10:56
- [Derek] But as we push the temperature higher...
00:10:58
- [Howard] Oh, I can see some glowing.
00:11:01
(energetic music) Oh, look at this, oh, it's gone already.
00:11:04
(Emilia laughs) - [Derek] Just like the steel, its strength drops rapidly
00:11:07
as temperature increases.
00:11:08
And that's true for most metals.
00:11:12
(lively music) Yet, the first jet engine, dating back all the way
00:11:14
to 1941, actually did use steel turbine blades.
00:11:18
It was designed by British pilot and engineer Frank Whittle.
00:11:21
His engine powered the first flight
00:11:23
of a British jet aircraft, the Gloster E.28/39 prototype.
00:11:27
When a colleague excitedly told Whittle,
00:11:29
"Frank, it flies," he dryly quipped, "That was bloody well
00:11:33
what it was designed to do, wasn't it?"
00:11:36
(film whirs) (lively music) But Whittle's prototype had two major flaws.
00:11:38
The first was that the gas
00:11:40
inside the engine, only reached temperatures
00:11:42
of around 780 degrees Celsius, which was one
00:11:45
of the reasons it was inefficient.
00:11:47
And the second was that it was only allowed
00:11:50
to fly for up to 10 hours.
00:11:52
Any longer, and it was too likely parts
00:11:54
inside the engine would fail.
00:11:55
And both of these drawbacks were largely due
00:11:57
to the steel turbine blades.
00:11:59
Something that occurred to me is,
00:12:01
why aren't they made out of tungsten?
00:12:03
I mean, because tungsten doesn't melt
00:12:06
until 3,400 degrees Celsius,
00:12:08
which is more than twice the temperature
00:12:10
inside a modern jet engine.
00:12:12
But tungsten is also incredibly dense.
00:12:14
It's about two and a half times denser than steel,
00:12:17
and it's also brittle, which makes it hard to manufacture.
00:12:21
And using a material
00:12:22
that heavy wouldn't just make the blade a problem.
00:12:25
The components that hold the blade in the engine would
00:12:28
also have to carry much higher loads,
00:12:30
well beyond what current materials can handle.
00:12:33
So, you can optimize for one thing, like the melting point,
00:12:36
or a different thing like strength or weight.
00:12:39
But the turbine pushes every variable to its limit.
00:12:43
So what are these blades
00:12:45
actually made of? (energetic music)
00:12:47
Well, to find out, we went
00:12:48
to Rolls-Royce's precision Casting Facility in Derby,
00:12:52
and it turns out the world's
00:12:53
most advanced metal parts begin life as, well,
00:12:57
something surprising.
00:12:59
(lively music) What is with the, like the pink and the green there?
00:13:02
- Well, come, I'll show you. - Okay, all right.
00:13:03
- I'll come and show you. - I'm just seeing
00:13:04
so many cool things around here.
00:13:06
I'm like, "What is that?
00:13:07
Why does it look like that?"
00:13:08
You just enter this room, and I smell the wax.
00:13:11
- Yeah, yeah. - Smells like
00:13:12
a candle factory in here.
00:13:13
- Absolutely, so investment casting is a really,
00:13:15
really ancient technology.
00:13:17
So our ancestors have been doing investment casting
00:13:19
to make jewelry, to make weapons for millennia.
00:13:22
We've just perfected it here to make turbine blades.
00:13:25
- It's so wacky.
00:13:26
This is just not how I'd expect it to happen at all.
00:13:29
(intense music)
00:13:30
Turbine blades strike me as one
00:13:31
of the most high-tech things in the world.
00:13:33
- Yep. - And yet,
00:13:35
this facility is using wax as a starting point.
00:13:39
- What you will see through our tour today is that,
00:13:42
actually, it's a really highly technological process.
00:13:45
(ominous music)
00:13:46
This is our wax pattern die.
00:13:48
This is how a turbine blade starts its life.
00:13:51
So, this is what's gonna go inside the wax pattern,
00:13:54
a ceramic core.
00:13:55
This is gonna create a hollow inside the turbine blade.
00:13:59
So what's happening now is we're injecting into the die.
00:14:02
So that's the very start of the life of a turbine blade.
00:14:06
- That is really neat. - What we'll actually see is
00:14:08
that a lot of these features, such as the aerofoil
00:14:10
and the annular surfaces are not touched further.
00:14:13
So we will cast that, and that will remain as cast
00:14:15
as it goes into the engine.
00:14:17
(ominous music) - [Derek] Every surface here has to be perfect
00:14:19
because this wax is what will become the blade.
00:14:22
- So Kim is our wax pattern assembler.
00:14:26
So she's responsible for taking the product straight
00:14:29
from that die, making sure
00:14:31
that things like die lines have been removed.
00:14:34
So where the die box come together
00:14:35
and leave a small amount of flash,
00:14:37
the operative word in all of wax assembly is smooth.
00:14:40
- [Derek] Every tiny imperfection in the wax would become
00:14:42
a flaw in the metal.
00:14:43
So this takes an incredible amount of skill.
00:14:47
(ominous music) - Then it's the case of getting that wax pattern attached
00:14:49
to the unit runner to create the assembly.
00:14:51
- I mean, the thought that occurs to me, right?
00:14:53
Shouldn't you be doing this with a robot?
00:14:55
- Can, you know, like- - Yeah, yeah, yeah.
00:14:57
So, Rolls-Royce has facilities that do this by robot,
00:15:00
but our facility in particular is very much focused
00:15:03
on bringing in those new products.
00:15:05
And it's far, far easier for us to work with human beings
00:15:09
to develop that method of manufacture that's going
00:15:11
to bring the next generation of product through.
00:15:13
- I'll bet, I can see the skill here,
00:15:15
like it's phenomenal. - Absolutely.
00:15:16
- I'll just make a mess of it.
00:15:17
- Absolutely, so would I.
00:15:18
- Would you like a go? - No. (laughs)
00:15:21
(ominous music) Once the wax assembly is perfect,
00:15:23
it's ready for the next stage.
00:15:25
- Everything that is wax is gonna become air,
00:15:28
it's gonna become negative space, right?
00:15:29
It's gonna become our cavity.
00:15:31
And then we're gonna fill that air with metal.
00:15:34
(ominous music) So we take that wax assembly, and we've gotta build a shell.
00:15:38
(pensive music) Shell is made of many different layers.
00:15:40
It's a zircon-based shell system.
00:15:43
We're gonna dip into a primary story.
00:15:45
It's really quite thin, like a light syrup or a thin honey.
00:15:48
- Oh yeah.
00:15:50
(pensive music) - [Henry] And what that's designed to do is map all
00:15:51
of those really complex geometric features.
00:15:54
- Beautiful. (engine droning)
00:15:56
It's like making icing.
00:15:58
- [Henry] So that's actually the analogy we use.
00:16:00
So, it's a bit like if you put icing on top of a bun
00:16:03
or a cake, you need to sprinkle it
00:16:05
with some sugar afterwards,
00:16:06
otherwise, it's all gonna slop off the top.
00:16:08
So we've got the slurry on there.
00:16:09
We're gonna get a nice even coat, drain it, make sure
00:16:11
that it's an even thin layer.
00:16:13
And then we're gonna sand,
00:16:14
and that's then gonna set that layer in place.
00:16:17
- So cool. (machine droning)
00:16:19
Whoa. (machine droning)
00:16:21
We're then gonna dry it,
00:16:22
so it's air-dried for many, many hours.
00:16:24
And then we can create our backup layers.
00:16:26
So our backup layers, it's a much thicker slurry,
00:16:28
more like a treacle,
00:16:29
and the sand is much coarser, more like a granulated sugar.
00:16:32
And we're gonna maybe put four, five, maybe even six layers
00:16:35
to back up, because what we need is we need a mold
00:16:38
that can withstand
00:16:39
that casting parameters that we're putting in the die.
00:16:41
You know, it's got a lot of work to do.
00:16:44
- The wax is then melted out,
00:16:47
and the mold is fired.
00:16:48
Oh, yeah.
00:16:50
(machine whooshing) That is wild.
00:16:52
Cleaned and tested to make sure there aren't any cracks.
00:16:55
When it's done, this shell is ready to hold molten metal.
00:16:59
- This is a billet of alloy
00:17:00
that's gonna fill the whole of that mold.
00:17:02
So just that amount
00:17:03
of metal is gonna fill that whole mold there.
00:17:05
- It doesn't look like an F.
00:17:06
(ominous music)
00:17:07
This is a nickel alloy.
00:17:09
The first nickel alloys used in jet engines were developed
00:17:12
in the 1940s.
00:17:13
By adding chromium and cobalt,
00:17:15
engineers created alloys that could handle 800
00:17:18
to 900 degrees Celsius,
00:17:20
around 100 degrees hotter than the steel used before.
00:17:23
And these alloys could keep their strength for thousands
00:17:26
of hours, a tenfold improvement in life.
00:17:29
But the real breakthrough came when they added
00:17:31
a touch of aluminum. (film whirring)
00:17:33
So we wanted to see
00:17:34
how it held up under the same lab conditions
00:17:36
as the steel and titanium.
00:17:38
- [Emilia] What temperature are we in now?
00:17:40
- [Howard] Oh, that's 700 degrees.
00:17:43
- [Emilia] 700, so the steel's long gone.
00:17:44
- Steel's, long gone.
00:17:45
That's 800 degrees.
00:17:46
800, yes. (flames blasting)
00:17:48
- [Derek] In around this temperature,
00:17:50
it's actually getting stronger.
00:17:53
(ominous music) So why would heating a metal make it stronger?
00:17:56
Well, when these nickel alloys were first used
00:17:58
in jet engines, no one actually knew.
00:18:01
But about 10 years later,
00:18:02
electron microscopes had improved enough for engineers
00:18:05
to finally see what was happening inside.
00:18:08
(ominous music) As we zoom in on the alloy, a pattern emerges.
00:18:12
The microstructure isn't uniform.
00:18:14
Instead, it kind of looks like a city grid made up of blocks
00:18:18
with rods in between them.
00:18:20
Only, each block is so small,
00:18:22
over 300 would line up across the width of a human hair.
00:18:26
(ominous music) Now, surprisingly, both the rods
00:18:28
and the blocks are made up of the exact same atoms,
00:18:30
mostly nickel with a little aluminum.
00:18:33
They even have the same crystal structure,
00:18:35
a grid of tiny cubes with atoms sitting at the corners
00:18:38
and at the center of each face.
00:18:40
The only difference is
00:18:41
that the atoms are arranged slightly differently.
00:18:44
In the road structure,
00:18:45
the aluminum and nickel can take any spot.
00:18:48
There is no repeating sequence from cube to cube.
00:18:51
And this is known as the gamma phase.
00:18:53
But in the blocks, aluminum always takes the corner spots,
00:18:57
and nickel the faces,
00:18:59
and you get a perfect repeating pattern cube after cube.
00:19:02
This is the gamma prime phase.
00:19:04
And it's this difference
00:19:05
that is crucial when a dislocation tries to glide
00:19:08
through the lattice.
00:19:09
In the rods, this motion is easy.
00:19:11
Each layer of atoms can shear smoothly past the next,
00:19:14
leaving the structure looking unchanged behind it.
00:19:17
But if you try to do the same thing in the blocks,
00:19:19
well, now you're actually changing the order of the atoms,
00:19:22
nickel and aluminum end up sitting in the wrong places.
00:19:26
That takes energy, so the lattice resists it.
00:19:29
So, when a dislocation moving
00:19:30
through the rods hits a block, it gets stuck.
00:19:33
And that's what makes this alloy so strong.
00:19:35
- [Henry] But if you keep pushing
00:19:37
and the stress gets high enough,
00:19:38
dislocation can finally force its way in.
00:19:41
The catch is that this dislocation leaves the lattice
00:19:43
in such a high-energy mess that the only way
00:19:46
that it can keep moving is if there's a second one
00:19:48
right behind it that puts things back in order.
00:19:51
So in the gamma prime phase, dislocations have
00:19:53
to travel in pairs, called super dislocations.
00:19:56
- I need that creation of those super dislocations,
00:20:00
and I need that very high stress to be able to shear.
00:20:02
So that's why the strength is very high
00:20:04
relative to other alloys.
00:20:06
What happens is, ultimately,
00:20:07
because you're shearing through that gamma prime
00:20:10
with two dislocations,
00:20:11
as the temperature continuously increases,
00:20:13
you're adding more and more thermal energy in the material.
00:20:15
What happens is the atoms are gonna vibrate
00:20:16
more and more and more.
00:20:17
So there's a likelihood, as I'm doing this
00:20:20
and I'm oscillating in three dimensions,
00:20:22
that the thermal energy is gonna drive me
00:20:25
to actually slip down rather than just slip in one plane.
00:20:29
So, now, if one cross slips,
00:20:31
they're no longer on the same plane.
00:20:32
Think of it as if we're standing in line,
00:20:35
and the only way that you can move is I push you, right?
00:20:38
And then, I keep on pushing you,
00:20:39
and then suddenly, you drop.
00:20:40
So if I now try to push you, I cannot find you, right?
00:20:43
You're not in front of me anymore.
00:20:44
Your shoulders are now below me.
00:20:46
- Well, how do you touch 'em? (laughs)
00:20:49
(Jaafar laughs) - I should have used the other example, you pushing me.
00:20:51
But anyway. (both laughing)
00:20:53
But it's exactly that.
00:20:55
It's the exact same analogy.
00:20:56
There's nothing to push me anymore.
00:20:57
There's like, I am not able to do it.
00:21:00
(ominous music) - So now you've got these two dislocations
00:21:02
that are on different planes,
00:21:03
so they can't travel together anymore.
00:21:05
And as a result, they're both now locked into place.
00:21:08
And you can see that effect on this graph.
00:21:10
While steel and titanium strength drops off,
00:21:12
in the nickel super alloy, you actually get a peak.
00:21:15
That's because the extra thermal energy
00:21:17
lets more dislocations cross-slip and get separated.
00:21:20
And it's that that shuts down the motion of dislocations.
00:21:23
But if gamma prime is so strong,
00:21:26
why don't we just make the entire turbine blade out of it?
00:21:29
Well, that strength comes at a cost.
00:21:30
Gamma prime stops the dislocation so effectively
00:21:33
that it becomes brittle.
00:21:35
All it takes is one crack or a sudden impact,
00:21:37
and it could lead to a sudden failure.
00:21:40
So the real trick is in striking the right balance
00:21:42
between enough gamma prime to trap the dislocations
00:21:45
and to prevent this creep,
00:21:46
but also enough gamma to keep the alloy ductile,
00:21:49
so that it can bend without breaking.
00:21:51
- [Derek] And in our test,
00:21:52
you can see exactly how that plays out.
00:21:55
- A 1,000 degrees, and still nothing.
00:21:57
- Still nothing.
00:22:00
(ominous music) (mold clanks) - [Howard] There we go.
00:22:01
- [Emilia] Oh my gosh.
00:22:03
(suspense music) - [Howard] That's 1,100 degrees C.
00:22:07
- It's stretching.
00:22:10
(suspense music) I mean, it's still holding up like-
00:22:12
- It's doing a good job.
00:22:13
That's 1,200 degrees C.
00:22:16
- [Emilia] 1,200. (laughs) - [Howard] That's the temperature program that stops.
00:22:19
And it's still surviving.
00:22:21
- [Emilia] Still going. - But if you push the temperature too far,
00:22:24
even this alloy reaches its limits.
00:22:26
Cross-slip becomes easier.
00:22:27
The paired dislocations can now hop
00:22:29
between the planes together,
00:22:31
and the ordered cubes of gamma primes start to dissolve.
00:22:34
So the dislocations break free,
00:22:36
and it finally gives out.
00:22:37
- [Howard] Oh, it may have just, did it break?
00:22:39
- Oh, yeah, yeah, it did, it broke.
00:22:41
- But strength alone isn't what makes these alloys special.
00:22:45
When you heat up the alloy, aluminum at the surface reacts
00:22:48
with oxygen to form a thin continuous layer
00:22:50
of aluminum oxide.
00:22:52
Unlike the brittle oxides
00:22:53
that form on other materials like steel or titanium,
00:22:56
this layer stays intact at high temperatures,
00:22:59
protecting the metal below.
00:23:01
(suspense music) And by adding other elements,
00:23:03
we can tune these super alloys.
00:23:05
Each one brings a specific property that we want.
00:23:08
Most modern super alloys contain as many
00:23:10
as 10 different elements,
00:23:12
all carefully balanced in their relative abundances
00:23:14
for the desired properties.
00:23:16
Chromium improves resistance to oxidation and corrosion.
00:23:20
Cobalt, titanium, niobium, tantalum,
00:23:22
and vanadium help stabilize the gamma prime phase.
00:23:25
Molybdenum and iron strengthen the gamma matrix.
00:23:28
And then there's rhenium.
00:23:30
Rhenium has one of the highest melting points
00:23:32
of any metal at 3,180 degrees Celsius.
00:23:35
It's second only to tungsten.
00:23:37
In the nickel super alloy,
00:23:39
It slows the atomic-scale rearrangements,
00:23:41
enhancing the alloy's resistance
00:23:42
to deformation even at temperatures
00:23:44
above 1,000 degrees Celsius.
00:23:46
It's one of the rarest elements in the Earth's crust
00:23:49
at less than one part per billion.
00:23:52
And more than 80%
00:23:53
of what we mine ends up right here in jet engines.
00:23:58
(ominous music) - But even with these advancements in alloy chemistry,
00:24:01
there's still one fundamental problem.
00:24:04
And that's that metals are crystalline.
00:24:06
Any metal you see from the tip of this ballpoint pen
00:24:09
to the spoon in my coffee cup, they're all actually made up
00:24:13
of millions of little crystals stuck together.
00:24:16
It's kind of like grains in the sugar cube.
00:24:18
If I crush it...
00:24:21
(ominous music) It's not like I've broken any individual crystal,
00:24:24
I've just broken them apart.
00:24:26
It's the boundaries between the grains
00:24:28
that are the weak point.
00:24:29
And it's the same thing in a metal.
00:24:31
(ominous music) - So, if we zoom out from the gamma
00:24:33
and gamma prime structure, it looks something like this.
00:24:36
One crystal is basically a three-dimensional lattice
00:24:39
of atoms all lined up in the same orientation.
00:24:41
But the crystals themselves are
00:24:43
all in different orientations.
00:24:45
So where they meet, their lattices don't line up.
00:24:47
And that mismatch leaves more open spaces and broken bonds.
00:24:51
And you also get defects there,
00:24:53
like vacancies and impurities,
00:24:55
all of which make grain boundaries the weakest point.
00:24:58
And this also has another consequence.
00:25:00
It makes it easier for atoms to move along the boundaries.
00:25:04
They become kind of super highways for atomic diffusion.
00:25:07
This becomes even more
00:25:08
of a problem at high temperatures when atoms have
00:25:10
more energy to move around,
00:25:12
add stress like the massive centrifugal loads
00:25:15
on a turbine blade, and the grains can actually start
00:25:18
to slide past each other.
00:25:20
The whole structure slowly deforms, stretching,
00:25:23
almost like warm taffy.
00:25:25
(ominous music) As long as it has grains in it, it will creep,
00:25:28
and fail far more easily.
00:25:30
And that's a really hard problem to solve
00:25:32
because normally, as a molten alloy cools,
00:25:35
tiny crystals start to form all throughout the liquid.
00:25:38
So you have to find some way to control them.
00:25:41
- This is one of our furnaces.
00:25:43
They're all induction-heated, there's no kind of gas, fire,
00:25:46
or anything like that, and they're all under vacuum.
00:25:48
So, we only cast to the vacuum in the absence
00:25:50
of any atmosphere, but particularly oxygen,
00:25:52
which is obviously metallurgically gonna cause us all kinds
00:25:54
of problems with oxides.
00:25:56
- [Derek] You start by pouring molten super alloy
00:25:58
into a ceramic mold that's mounted vertically
00:26:00
and heated to about the same temperature as the melt.
00:26:03
The mold fills from the root up toward the tip.
00:26:06
At the very bottom of the mold sits
00:26:08
a copper plate cooled by water.
00:26:10
Its surface is patterned with tiny grooves that act
00:26:12
as nucleation points
00:26:13
for the first crystals to start to form.
00:26:16
It's here that solidification begins.
00:26:18
Then, the entire mold is slowly lowered out of the hot zone,
00:26:22
so the solidification continues in just one direction.
00:26:25
- It's a very slow process in the magnitude of hours.
00:26:29
Once that's finished,
00:26:30
the whole machine will then index round,
00:26:32
and it will push the completed mold
00:26:34
up out of the other side.
00:26:36
- Oh.
00:26:37
(machine humming) Wow.
00:26:38
- So our casting temperatures are
00:26:40
roughly 1,500 degrees Celsius.
00:26:42
- It's kind of at the same temperature now as it would be
00:26:45
inside the jet engine. - Exactly.
00:26:47
- It's absurd, they like,
00:26:48
you're making the turbine blades
00:26:49
at the same temperature that they're gonna operate,
00:26:51
but they like, here, they're liquid.
00:26:53
(ominous music) Now, if we just did that on its own, you'd end up
00:26:56
with a blade that looks like this.
00:26:59
(ominous music) - Here's a directionally solidified blade.
00:27:02
And what you can probably see there is the contrast
00:27:05
between the grains.
00:27:07
These are all different crystals,
00:27:08
but they're all running on this axis of the blade,
00:27:12
which makes it significantly stronger
00:27:14
than an alloy that is cast,
00:27:16
where all of the crystals are separate from each other.
00:27:18
- So those are like individual crystals.
00:27:20
- [Henry] These are individual crystals, yeah, absolutely.
00:27:23
So we are looking at- - Wow.
00:27:25
- At crystals on kind of a macro level,
00:27:27
where normally, we'd be talking
00:27:28
about crystals on a micro level.
00:27:31
(ominous music) - In a rotating turbine,
00:27:33
the blade is being pulled along its length.
00:27:35
With columnar crystals all lined up along this span,
00:27:38
the blade can carry those stresses far more effectively.
00:27:41
There are no grain boundaries
00:27:42
that cut across the blade, creating weak points
00:27:44
for it to crack.
00:27:45
But scientists have found a way to do even better.
00:27:48
If you introduce a bend in the mold
00:27:51
just above the chill plate, something strange happens.
00:27:54
The number of columnar crystals that make it
00:27:56
through drops sharply.
00:27:58
And if you add another bend, even fewer survive.
00:28:02
(ominous music) So, engineers added a helical passage known
00:28:05
as the pigtail here at the bottom of the mold.
00:28:07
- The pigtail is doing the job to select the single crystal.
00:28:11
The spiral is gonna choke out every other grain bar one.
00:28:15
So we're only gonna have one grain that is then gonna grow
00:28:18
through the entirety of that blade,
00:28:21
and cast that blade as a single crystal.
00:28:23
Or at least, that's the theory.
00:28:25
- That's crazy.
00:28:26
- So this is a starter attached to a spiral
00:28:29
that we've etched so that we can reveal that structure.
00:28:31
So you can see down at the bottom, we are starting
00:28:35
to grow directionally solidified grains.
00:28:38
But as we get up here, we can start to see
00:28:40
that we're growing directionally solidified grains.
00:28:43
And then, as we're going up the spiral,
00:28:47
the grains are starting to be choked out
00:28:48
by the upper surfaces of that spiral until, when we get
00:28:51
to the top, we're just as a single crystal.
00:28:54
And then, that then allows that
00:28:55
to grow right the way through the blade.
00:28:57
- Yeah, that's amazing.
00:28:58
- And what we should end up with is a blade like this.
00:29:01
So this is a blade of a single crystal.
00:29:04
It's a really impressive thing to look at.
00:29:07
(ominous music) The shimmer is beautiful.
00:29:08
- Yeah.
00:29:09
- Even after the blade solidifies,
00:29:11
it's still not ready for the engine.
00:29:13
It's heated again, almost to its melting point.
00:29:16
And that might sound risky
00:29:17
because we've spent all this time making sure it's
00:29:19
a perfect single crystal.
00:29:21
But this heating step lets the atoms shuffle around
00:29:24
just enough to spread out evenly,
00:29:27
and form the final desired microstructure of the gamma
00:29:30
and gamma prime phases
00:29:31
that make these super alloys so strong.
00:29:34
- And as if casting, as a single crystal is not enough,
00:29:37
actually, the orientation of that crystal is
00:29:40
also of paramount significance.
00:29:42
So you may have cast this as a single crystal,
00:29:45
but if the crystal orientation is off
00:29:48
by a certain amount,
00:29:49
you get completely different stress responses
00:29:52
within that blade.
00:29:53
- Today, after decades of development, over 95%
00:29:57
of blades can be cast successfully as single crystals.
00:30:01
Just think about how incredible that is.
00:30:04
We've gone from a turbine blade that contained on the order
00:30:06
of 50,000 crystal grains down to just one.
00:30:10
When we grow these things, they don't solidify
00:30:13
as a uniform front.
00:30:15
On a microscopic scale,
00:30:16
the solidification front looks like a forest
00:30:19
of tiny tree-like branches called dendrites
00:30:22
that are pushing their way into the liquid.
00:30:24
At first glance, it looks messy, like millions
00:30:27
of separate trees jostling for space.
00:30:30
There are up to 10 elements in there,
00:30:32
each with its own density and melting point.
00:30:35
Yet somehow, every one of those trees is locked
00:30:39
into the exact same crystal lattice.
00:30:42
So the final crystal is comprised of more than six times 10
00:30:46
to the 24 atoms,
00:30:47
that is more stars than there are
00:30:50
in the observable universe.
00:30:51
When all these atoms are repeating the same pattern,
00:30:55
perfectly aligned from root to tip,
00:30:58
this completely transformed what jet engines can do.
00:31:01
Single-crystal blades can withstand stresses
00:31:03
and temperatures that would destroy ordinary alloys.
00:31:06
They last up to nine times longer against creep
00:31:09
and thermal fatigue,
00:31:10
and are more than three times more resistant
00:31:12
to corrosion than blades made from multiple grains.
00:31:15
That's why modern jet engines can now run for 25,000 hours
00:31:19
between major overhauls,
00:31:21
something that would've been unthinkable
00:31:22
before single crystal blades.
00:31:25
(suspense music) And the impact has been huge.
00:31:27
Between 1960 and 2010,
00:31:29
jet aircraft became about 55% more fuel efficient.
00:31:33
And a huge part of that improvement comes down
00:31:35
to advances in these nickel super alloys.
00:31:38
Back in the 1960s,
00:31:40
flying was a luxury few could afford.
00:31:42
A one-way flight from New York
00:31:43
to Paris would set you back $310,
00:31:46
which is about $3,750 adjusted for inflation.
00:31:50
But as engines became more efficient,
00:31:52
able to handle hotter cores
00:31:54
and equipped with much larger fans,
00:31:56
airlines could carry more people farther using less fuel.
00:32:00
So, tickets got cheaper and air travel exploded.
00:32:03
Today, at any given moment, there are roughly 10,000
00:32:06
to 14,000 planes in the sky.
00:32:08
That scale of movement is possible
00:32:10
because of these turbine blades.
00:32:15
(jet hovering) In the furnace, the nickel super alloy outperforms
00:32:18
all the other samples,
00:32:19
surviving up to 1,200 degrees Celsius.
00:32:22
But wait, that's still 300 degrees less
00:32:24
than the temperature inside a jet engine.
00:32:27
So why don't the blades melt?
00:32:29
Well, there are two final layers of defense.
00:32:32
The first is built into the shape of the blade itself.
00:32:35
- We then have to leach the core out.
00:32:37
So we do that in a caustic solution
00:32:40
of potassium-sodium hydroxide under pressure
00:32:44
and temperature to leach the core out,
00:32:47
that will leave those core passages completely empty.
00:32:51
- [Derek] And those passages are the real secret
00:32:53
to the turbine blade survival.
00:32:54
- So as the air's flowing through, it is turbulent,
00:32:58
and as such, it can remove much more heat
00:33:00
from the surface of the blade.
00:33:01
- Yeah. - Than it was.
00:33:03
- Is it these ridges here that we're talking about?
00:33:04
- Exactly, yeah, yeah, these ridges here.
00:33:05
- [Derek] They're intentional to the trip the flow into-
00:33:08
- Trip and turbulate that air flow so that it's removing
00:33:11
as much heat as possible from the metal.
00:33:13
So then we get onto the really juicy part,
00:33:15
which is film cooling.
00:33:16
So we talked about the ice cube in the ovens
00:33:18
that keeping our blades as cool as possible.
00:33:21
So this is where we start to drill in
00:33:23
what we call film cool holes.
00:33:25
And what we're aiming to do is we're aiming
00:33:27
to get into those cooling passages.
00:33:29
So we saw that core earlier on.
00:33:31
They are the cooling passages inside.
00:33:34
And these holes have got
00:33:35
to get right into those cooling passages
00:33:37
to allow the air to come out.
00:33:39
And the air is then gonna blow as a film over the surface
00:33:42
of the blade, a film-cool hole to create a film
00:33:46
of air, which is preventing
00:33:47
that metal from melting in those temperatures.
00:33:50
- This cooling air isn't exactly cold.
00:33:54
It actually comes from the high-pressure compressor section
00:33:56
of the engine at around 600 degrees Celsius.
00:33:59
But that is cool enough
00:34:00
to help keep the blades from melting.
00:34:02
But it's still not quite enough.
00:34:04
And you can't just add more cooling air
00:34:07
because every extra bit of air you use from the compressor,
00:34:10
you lose from thrust,
00:34:12
and actually make the engine less efficient.
00:34:14
So every turbine blade is also coated
00:34:17
with two protective layers.
00:34:19
First, a thin metallic bond coat that resists oxidation,
00:34:23
and then a ceramic topcoat.
00:34:25
Even though it's only about a quarter of a millimeter thick,
00:34:28
this ceramic coating can keep the metal beneath it
00:34:31
100 to 170 degrees cooler than it would otherwise be.
00:34:35
And this is the final barrier
00:34:36
that stops the blades from melting.
00:34:38
So, now we've got this insane piece of engineering
00:34:41
that can survive the 1,500-degree gas.
00:34:44
The intense load and the oxidation problem should be solved.
00:34:49
Well, it would be, except for one thing,
00:34:53
(ominous music) - At 36,000 feet, you wouldn't believe this,
00:34:56
but there's dirt and dust in the atmosphere
00:34:59
that our engines are ingesting.
00:35:02
(ominous music) The dirt and dust comes, it sticks on the blades,
00:35:04
but it also goes through the whole cooling circuit,
00:35:08
and it walks the cooling from getting through
00:35:11
to cool the blades, and then the blades burn up.
00:35:15
Usually, every time I get on a plane,
00:35:17
I'm thinking, "This is never gonna work." (laughs)
00:35:19
No, I mean it's incredible how an engine can work
00:35:23
'cause there's so many moving pieces, there's so many parts
00:35:25
to the environment, so terrible.
00:35:27
And now, we have this dust and dirt, which is really bad.
00:35:31
(intense music) - I am at Testbed 80,
00:35:33
and they're about to fire up this jet engine
00:35:36
and then throw dust into it.
00:35:39
The same stuff that makes up sand and volcanic ash,
00:35:42
exactly what real engines encounter in flight.
00:35:44
- So this engine is the 97K.
00:35:47
It goes on the A350
00:35:48
and is our high-thrust version of that.
00:35:50
So 97,000 pounds of thrust is what this engine's producing.
00:35:54
When we're running a bit an engine like this, we try
00:35:56
and carefully recreate exactly what happens in service,
00:36:02
(intense music) - How much dust goes
00:36:03
in the engine? - Not very much.
00:36:05
It was surprising when I found out
00:36:06
exactly how much we put in.
00:36:07
It's in the order of tablespoons worth per cycle.
00:36:11
- So, I (indistinct) master on.
00:36:13
Condition power on.
00:36:16
(fan swooshing) (buttons clicking) Master fuel lever on.
00:36:17
Start request in three, two, one.
00:36:20
Now. (computer beeps)
00:36:28
(intense music) (blades swooshing) - So, what does the dust actually do inside a jet engine?
00:36:31
- So, once it goes through to the hot section of the engine
00:36:34
and hits kind of turbine blades, it's gonna be melted.
00:36:37
And so, it sticks to the outside of our turbine components
00:36:41
and it slowly rips layers
00:36:43
of that thermal barrier coating off.
00:36:46
And then, you lose your temperature reduction
00:36:49
that comes from the barrier coating,
00:36:51
so that your nickel alloy underneath it gets hotter
00:36:53
and hotter, and that's when it starts
00:36:54
to deteriorate the turbine.
00:36:58
(blades swooshing)
00:37:01
- That's why engineers at Rolls-Royce are still refining
00:37:04
these blades, developing new ceramic coatings designed
00:37:07
to resist mold and dust,
00:37:08
and extend the life of the turbine by up to 30%.
00:37:12
That's just the latest step in a story
00:37:13
that's been unfolding for decades.
00:37:15
These blades have been refined
00:37:17
and perfected to the point
00:37:19
where they operate right at the edge
00:37:21
of what is physically possible.
00:37:23
You're always on a knife-edge, pushing every material,
00:37:26
every process to the limit to build an engine
00:37:28
that can do the seemingly impossible,
00:37:30
run hotter than its own melting point.
00:37:33
The more I learned about the brutal environment
00:37:35
these blades have to survive, the more it felt
00:37:38
like they shouldn't work at all.
00:37:40
And yet, they do.
00:37:42
Every day, these machines carry millions of people
00:37:45
across the world and we barely stop to think about them,
00:37:48
they're a monument to human ingenuity.
00:37:51
What happens when we refuse
00:37:52
to accept limits, when we turn the impossible
00:37:55
into the routine?
00:38:01
(ominous music) (scene change zooms) (ominous music) I can't grow a single-crystal turbine blade in my kitchen,
00:38:05
but with the help from this video sponsor, KiwiCo,
00:38:07
I can grow a crystal garden with my kids.
00:38:11
This month, they sent us their Crystal Garden Chemistry Kit.
00:38:14
We set everything in place, mixed up the chemical solution,
00:38:16
and then watched as colorful crystals started
00:38:19
to bloom over the next 48 hours.
00:38:21
Every few hours, my kids would run back to check
00:38:23
how much the garden had grown.
00:38:25
They were totally fascinated,
00:38:26
and it sparked so many questions about crystals
00:38:29
and atoms, how things arrange.
00:38:31
Pretty soon, we were talking
00:38:32
about how metals are crystalline, too,
00:38:34
and setting ourselves the challenge
00:38:36
of growing one giant crystal turbine-blade style.
00:38:39
(camera shuttering) I love how simple KiwiCo makes this.
00:38:42
Everything we needed came right in the box,
00:38:44
so we could just open it up
00:38:45
and dive straight in, doing the experiment.
00:38:48
And it's not just chemistry.
00:38:49
They've got crates for robotics,
00:38:51
engineering, art, design techniques, and so much more.
00:38:54
There is something for every age and interest.
00:38:57
(scene change chimes) KiwiCo crates also make a great gift for the holidays.
00:39:01
It's creative, hands-on,
00:39:02
and gives kids something they can actually make
00:39:04
and be proud of.
00:39:05
- They're kind of messy. - Mm-hmm.
00:39:08
- And like hard to make, but not too hard,
00:39:12
but hard enough to make it fun.
00:39:14
- So if you wanna try out KiwiCo,
00:39:16
click the link in the description or scan this QR code.
00:39:19
Use my code Veritasium
00:39:20
to get 50% off your first monthly crate.
00:39:23
I wanna thank KiwiCo for sponsoring this video,
00:39:25
and I want to thank you for watching.

Description:

How does a jet engine not melt? Sponsored by KiwiCo - Use code VERITASIUM to get 50% off your first monthly KiwiCo Crate! https://www.kiwico.com/VERITASIUM Want to start your own crystal garden? https://www.kiwico.com/crystalchemistry Our friends at Science Alert are doing a sweepstakes where you can win a 5-day space themed vacation for two. The itinerary includes a trip to the Kennedy Space Center in Florida for astronaut training and a meet and greet with a NASA astronaut. If you’d like to be entered in the draw, just subscribe to their free science newsletter Spark. No purchase necessary. Open to US residents only. Enter here: https://www.sciencealert.com/newsletter We have a tabletop game launching! Check it out here! - https://www.kickstarter.com/projects/elements-of-truth/elements-of-truth-by-veritasium?ref=bgt9se If you’re looking for a molecular modelling kit, try Snatoms, a kit I invented where the atoms snap together magnetically - https://snatoms.com/ Sign up for the Veritasium newsletter for weekly science updates - https://www.veritasium.com/newsletter ▀▀▀ 0:00 How a jet engine works 3:18 Why are jet engines so big? 5:17 The Inside of a Jet Engine 8:49 Edge Dislocation 11:11 The First Jet Engine 12:48 Inside the Rolls-Royce Precision Casting Facility 17:07 Nickel Superalloys - Gamma Prime 23:58 Crystal Structure 25:38 Making a Turbine Blade 32:22 Why don’t turbine blades melt? 35:30 Throwing Sand Into a Jet Engine ▀▀▀ A big thanks to Ben Todd, James Banks, Ben Fifoot, Doug Smith, Stefan Wagner, Rumaanah Hoosen and the rest of the team at Rolls-Royce. A huge thanks also to Professor Howard Stone and Dr George Wise from the University of Cambridge. We’re also incredibly grateful to Professor Jaafar A. El-Awady, Dr Karen A Thole, Professor Cathie Rae, Professor Paul Withey, Professor Pedro Patrício, Professor José Tavares and Ryan Moreman for their time and expertise. Thanks to Institute for Materials, Ruhr University Bochum, SFB Transregio 103 for the animation showing the microstructure of the nickel superalloy. Full youtube video here - https://www.youtube.com/watch?v=wYHch5QIWTQ Thanks to Professor Hongbiao Dong for the animation showing the grain selection in a single crystal turbine blade. Full youtube video here: https://www.youtube.com/watch?v=br9iaeYYxSM References: https://docs.google.com/document/d/1Nd3KqiBy7v54U9HcMqFFcCnVMPVqreXngbioLAL4tvs/edit?tab=t.0 ▀▀▀ Special thanks to our Patreon supporters: Adam Foreman, Albert Wenger, Alex Porter, Alexander Tamas, Anton Ragin, Anupam Banerjee, armedtoe, Bertrand Serlet, Blake Byers, Bruce, Dave Kircher, David Johnston, David Tseng, Evgeny Skvortsov, Garrett Mueller, Gnare, gpoly, Hayden Christensen, Ibby Hadeed, Jeromy Johnson, Jon Jamison, Juan Benet, KeyWestr, Kyi, Lee Redden, Marinus Kuivenhoven, Matthias Wrobel, Meekay, meg noah, Michael Bush, Michael Krugman, Orlando Bassotto, Paul Peijzel, Richard Sundvall, Robert Oliveira, Sam Lutfi, Tj Steyn, Ubiquity Ventures & wolfee ▀▀▀ Writers - Emilia Gyles, Casper Mebius & Derek Muller Producer & Director - Emilia Gyles Presenters - Derek Muller & Henry Van Dyck Editor - Trenton Oliver Camera Operators - Jack Coathupe, Justin Wood, Emilia Gyles, Henry Van Dyck & Derek Muller Animators - Mike Radjabov, Emma Wright & Fabio Albertelli Additional Editors - James Stuart & Peter Nelson Researcher - Aakash Singh Bagga Thumbnail Designers - Ren Hurley, Ben Powell & Abdallah Rabah Production Team - Josh Pitt, Matthew Cavanagh, Anna Milkovic & Katy Southwood Executive Producers - Casper Mebius & Derek Muller Additional video/photos supplied by Getty Images, Storyblocks Music from Epidemic Sound

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