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Veritasium
The Ridiculous Engineering of Jet Engines
The Ridiculous Engineering of Jet Engines
Veritasium
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39:34 · Nov 17, 2025
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This
is
one
of
the
most
powerful
jet
engines
in
the
world,
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0:00
- This is one of the most powerful jet engines in the world,
0:03
and it actually runs at temperatures 250 degrees Celsius hotter than the melting point
0:08
of the materials that make it up. - That's 1,200 degrees. -
0:11
So the question is,
0:12
why doesn't a jet engine just melt into a puddle?
0:16
(intense music) (jet hovering) - We are right at the boundaries of the laws
0:19
of physics (intense music) -
0:21
That is wild.
0:22
It's at the same temperature now as it would be inside the jet engine.
0:26
But here, they're liquid. (dramatic music) - Every time I get on a plane,
0:29
I'm thinking, "This is never gonna work." - And yet, it does work.
0:33
Right now, there are over 10,000 planes in the sky powered by engines just
0:38
like these.
0:39
Maybe you are on one right now.
0:41
So, how do they work?
0:45
(energetic music) (jet humming) This is a jet engine, specifically a turbofan engine.
0:49
At the front is this giant fan.
0:51
During takeoff, these rotating blades push 1.3 tons of air backwards every second,
0:57
and around 10% of that air gets compressed.
1:00
The compressors force the air into increasingly narrow chambers.
1:04
They compress the air to about 50 times atmospheric pressure.
1:08
And just by doing that, the air heats up to around 600 degrees Celsius.
1:13
This compressed air is then forced into the combustion chamber,
1:16
where fuel is sprayed in through a ring of nozzles
1:19
and ignited. (flames blasting)
1:21
That chemical reaction gives off a lot of heat.
1:24
So the temperature jumps to around 1,500 degrees Celsius.
1:28
So now you've got this high-pressure gas from the combustor
1:30
that just wants to expand,
1:32
and now it's got an incredible amount of thermal energy.
1:36
But between the combustion chamber
1:37
and the outside air is this. (intense music) Rows of turbine blades. (blades humming)
1:42
So,
1:42
in order for the gas to expand and get out,
1:44
it needs to push these turbine blades out of the way.
1:47
And in pushing the blades,
1:49
that is how it transfers its energy to the engine.
1:52
This is where all the power really comes from in modern jets on takeoff,
1:57
each high-pressure turbine blade is generating
1:59
as much power as a Formula 1 car. (car droning)
2:02
And there are 68 of them. (lively music)
2:04
As the gas rushes through the turbine
2:06
and nozzle,
2:07
its pressure drops from around 50 atmospheres down to one,
2:09
and it expands by almost 20 times.
2:12
And that spins these turbine blades up to 12,500 revolutions per minute.
2:18
The fan that is pushing all
2:19
that air backward and all those compressors
2:21
that squeeze the air down,
2:22
all of that is powered by the turbines back here.
2:26
It's a kind of funny, really counterintuitive way to think about an engine.
2:30
It's what's happening in the back that's actually driving everything up front. (pensive music)
2:35
As the hot exhaust gas is shot out the back of the engine,
2:39
it pushes the engine forward.
2:41
That generates thrust.
2:43
But did you know that in a modern passenger jet,
2:45
this accounts for less than 20% the thrust of the engine?
2:49
The vast majority of the thrust, over 80% of it,
2:52
just comes from that big fan at the front of the jet. (numbers beeping)
2:56
Remember how only 10% of the incoming air gets compressed?
2:59
The other 90% bypasses all that.
3:02
It's simply propelled backwards by the fan.
3:04
It goes right around the guts of the engine
3:06
and comes straight out the back.
3:08
The fan pushes that air backwards, so the air pushes the fan forwards.
3:13
That's how you get 80% of the thrust.
3:15
It's basically a huge ducted propeller. (jet hovering) So, why do it this way?
3:20
I mean, why not compress all the incoming air
3:23
and put it all through the combustion chamber
3:25
and turbines?
3:27
(flames blasting) Well, some fighter jets do exactly this,
3:30
and it makes for very powerful engines, but they're also horribly inefficient.
3:35
To see why, remember
3:36
that the impulse pushing the plane forward is equal to the change in the
3:40
momentum of the air backwards.
3:42
So you've got options.
3:43
For example, you could push twice as much air back half as fast,
3:47
or you could push half as much air back twice as fast.
3:51
Both will generate the exact same impulse,
3:53
but the kinetic energy of the air is proportional to v squared.
3:58
So it takes four times
3:59
as much energy to speed up the air in the second case,
4:02
and a lot of that energy is just wasted in the exhaust.
4:05
So, ideally, you want to push
4:07
as much air backwards
4:08
as possible with only a small change in velocity. (enchanted music) That's why jets
4:13
have gotten bigger and bigger over the years,
4:16
and the increasing fraction of bypass air has the added benefit
4:20
that it surrounds the hot exhaust gases,
4:23
and that reduces noise coming away from the jet.
4:26
But there is another major factor when it comes to engine efficiency,
4:30
and that is temperature.
4:31
At cruising altitudes around 35,000 feet,
4:34
the outside air is around negative 55 degrees Celsius, while inside the engine,
4:39
it's over 1,500 degrees Celsius.
4:42
The hot, high-pressure gas inside the engine wants to expand into the much colder,
4:46
lower-pressure air outside.
4:49
It's that difference that lets the engine turn heat into useful work. (ominous music)
4:53
But there's a fundamental limit to how much work any heat engine can get
4:57
from that.
4:57
It's called the Carnot efficiency.
4:59
It's equal to one minus the temperature of the cold outside air divided by
5:03
the temperature of the hot gas inside the combustion chamber. (ominous music)
5:07
So,
5:08
looking at this, you can improve the efficiency of the engine in two ways,
5:12
either fly where the air is colder
5:14
or raise the temperature in the combustion chamber.
5:17
One problem with that, though,
5:18
is that it turned the inside of a jet engine into one of the
5:22
harshest environments we have ever built in
5:25
which machinery has to survive. - To keep a turbine blade whole
5:30
and unaffected within an engine is like putting an ice cube inside your oven,
5:33
turning up to max, leaving for work, coming back after an eight-hour shift,
5:36
and finding it's still completely frozen in the oven.
5:38
That's what we've got to try
5:39
and do within that engine. - It sounds absurd. (intense music) Not only do
5:42
the turbine blades sit in a stream of gas that's over 1,500 degrees Celsius,
5:47
they're also spinning at 12,500 RPM with the tip of each blade slicing through
5:53
the air at nearly 1,900 kilometers per hour.
5:57
Now, every blade wants to fly straight,
5:59
but it's forced to spin in a circle, which means,
6:02
something has to be constantly pulling it inwards.
6:05
That's the centripetal force.
6:07
If you take a representative 300 gram high-pressure turbine blade
6:11
and run it at
6:11
that speed and radius,
6:13
it has to be pulled inwards with a force equal to the weight of
6:16
20 metric tons.
6:17
That's roughly the weight of two London double-decker buses tugging on each blade
6:22
as it spins,
6:23
all while they're glowing hot. (ominous music) To make matters worse, at these temperatures,
6:29
oxygen wants to react with the metal of the blades itself.
6:32
And on top of all that,
6:33
the air rushing through the engine often carries dust, sand,
6:37
and pollutants that can damage and erode the surfaces inside.
6:41
And somehow, these blades have to survive this punishment for tens of thousands of
6:46
flight hours without deforming,
6:49
cracking, or failing.
6:50
They really determine how efficient you can make the engine
6:53
because you can't make the engine
6:55
so hot that the blades can't withstand
6:57
that temperature.
6:58
So they determine the maximum temperature of the combustion chamber, and therefore,
7:02
the maximum efficiency you can realize with a jet engine.
7:06
So what kind of metal could possibly survive these conditions?
7:10
Well, we sent Veritasium producer, Emilia,
7:13
to the Department of Materials Science & Metallurgical at Cambridge University to put some
7:17
different metals to the test. (ominous music) -
7:19
So this is the steel?
7:20
This is the steel sample,
7:21
yes. - Okay. - So we've got about 200 megapascals to start with,
7:24
which is sort of comparable to some of the stress that's seen by these
7:28
components in real applications.
7:30
And we're gonna put that stress on,
7:32
and then slowly increase the temperature. - This is a mild steel.
7:36
It's relatively strong and easy to form into complex shapes.
7:39
It seems like a pretty good bet for a turbine blade.
7:41
And at first, under this load and at these low temperatures,
7:44
it holds up pretty well.
7:46
We're essentially tugging on all the atoms within the metal.
7:49
We're not breaking or forming any bonds.
7:52
We're just making them flex a little.
7:53
And that slightly changes the spacing between the atoms.
7:56
And as a result, the metal gets slightly longer.
7:59
This resulting change in size, specifically the per-unit change in length,
8:03
is what we call strain.
8:05
Critically, at this stage, the material is behaving elastically.
8:08
If we remove the load right now,
8:10
the material just snaps back to its original size.
8:14
In an engine, some elastic deformation like this will occur.
8:17
It can't be too big or it'll cause problems.
8:20
But what we really don't want is plastic deformation if the shape changes permanently.
8:26
And that's exactly what starts to happen
8:28
as we keep increasing the temperature. - It's getting hot now.
8:31
That's a little bit of oxide. (ominous music) There you go,
8:36
see this starting to deform? - Now,
8:38
bonds are breaking and reforming
8:41
as the metal at us deforms permanently. (ominous music)
8:46
But this doesn't happen all at once.
8:48
So I got the mechanical engineer on our team, Henry,
8:51
to build this demo. (ominous music) - Okay,
8:54
so you can see we're getting a bunch of tiny little bubbles,
8:56
and just naturally, they're packing into this hexagonal arrangement.
9:00
And there are actually a lot of materials
9:01
that have atomic structures just like this.
9:03
But you can see it's not perfect.
9:05
Like, right here, you can see there's an extra half-plane of atoms.
9:09
Well, in this case, bubbles,
9:11
this is called an edge dislocation. (ominous music) It becomes really interesting
9:18
when I try to pull this raft apart. (ominous music) You can see these
9:22
little dark lines that zip back
9:24
and forth.
9:25
Those are dislocations, and they move through the lattice.
9:28
As the dislocation moves, it'll cause one plane, a bubbles,
9:32
to sheer past the other one, which shifts the structure by exactly one spacing.
9:36
But there isn't just one dislocation.
9:39
There are plenty of them.
9:40
And altogether, their movement produces dramatic changes in the overall shape. (ominous music) -
9:45
That's exactly what's happening here.
9:47
Everywhere that stress is high enough, billions of dislocations are moving and interacting.
9:52
The steel starts to deform continuously under this constant load in a process called
9:56
creep.
9:57
It takes energy to break the atomic bonds
10:00
as the dislocation travels through the lattice.
10:02
So, as we ramp up the temperature
10:03
and all the atoms get more thermal energy,
10:06
it no longer requires as much stress to break these bonds,
10:09
becomes much easier for the dislocations to move.
10:12
The metal effectively gets softer.
10:14
Now the steel strength drops so much that the slow,
10:18
time-dependent creep gives way to rapid deformation.
10:21
As it stretches, it rapidly decreases in cross-section, and eventually,
10:26
the remaining metal can no longer bear the load. (ominous music) Now,
10:30
you could try doing similar tests for other metals like this titanium alloy. (ominous
10:36
music) Titanium is about half
10:37
as dense as steel. - Should feel that's quite a bit lighter. - Yeah,
10:40
it's like loads lighter. -
10:41
So if we were to make turbine blades out of titanium,
10:44
each blade would be much lighter,
10:45
and that would reduce the enormous centripetal forces it would experience.
10:49
So it seems like a great choice.
10:51
And at first, it performs really well. - That's 100 degrees.
10:54
It's hanging in there. - But as we push the temperature higher... - Oh,
10:58
I can see some glowing. (energetic music) Oh, look at this, oh,
11:02
it's gone already.
11:04
(Emilia laughs) - Just like the steel, its strength drops rapidly as temperature increases.
11:08
And that's true for most metals. (lively music) Yet, the first jet engine,
11:13
dating back all the way to 1941, actually did use steel turbine blades.
11:18
It was designed by British pilot and engineer Frank Whittle.
11:21
His engine powered the first flight of a British jet aircraft,
11:25
the Gloster E.28/39 prototype.
11:27
When a colleague excitedly told Whittle, "Frank, it flies," he dryly quipped,
11:32
"That was bloody well what it was designed to do, wasn't it?"
11:36
(film whirs) (lively music) But Whittle's prototype had two major flaws.
11:38
The first was that the gas inside the engine,
11:41
only reached temperatures of around 780 degrees Celsius,
11:45
which was one of the reasons it was inefficient.
11:47
And the second was
11:48
that it was only allowed to fly for up to 10 hours.
11:52
Any longer, and it was too likely parts inside the engine would fail.
11:55
And both of these drawbacks were largely due to the steel turbine blades.
11:59
Something that occurred to me is, why aren't they made out of tungsten?
12:03
I mean, because tungsten doesn't melt until 3,400 degrees Celsius,
12:08
which is more than twice the temperature inside a modern jet engine.
12:12
But tungsten is also incredibly dense.
12:14
It's about two and a half times denser than steel, and it's also brittle,
12:19
which makes it hard to manufacture.
12:21
And using a material that heavy wouldn't just make the blade a problem.
12:25
The components that hold the blade in the engine would also have to carry
12:29
much higher loads,
12:30
well beyond what current materials can handle.
12:33
So, you can optimize for one thing, like the melting point,
12:36
or a different thing like strength or weight.
12:39
But the turbine pushes every variable to its limit.
12:43
So what are these blades actually made of?
12:47
(energetic music) Well, to find out,
12:48
we went to Rolls-Royce's precision Casting Facility in Derby,
12:52
and it turns out the world's most advanced metal parts begin life as, well,
12:57
something surprising. (lively music) What is with the,
13:00
like the pink and the green there? - Well, come, I'll show you. - Okay,
13:04
all right. - I'll come
13:04
and show you. - I'm just seeing
13:04
so many cool things around here.
13:06
I'm like, "What is that?
13:07
Why does it look like that?"
13:08
You just enter this room, and I smell the wax. - Yeah,
13:11
yeah. - Smells like a candle factory in here. - Absolutely,
13:13
so investment casting is a really, really ancient technology.
13:17
So our ancestors have been doing investment casting to make jewelry,
13:20
to make weapons for millennia.
13:22
We've just perfected it here to make turbine blades. - It's so wacky.
13:26
This is just not how I'd expect it to happen at all. (intense music)
13:30
Turbine blades strike me
13:31
as one of the most high-tech things in the world. - Yep. -
13:34
And yet,
13:35
this facility is using wax
13:38
as a starting point. - What you will see through our tour today is
13:42
that,
13:42
actually, it's a really highly technological process. (ominous music) This is our wax pattern
13:47
die.
13:48
This is how a turbine blade starts its life.
13:51
So, this is what's gonna go inside the wax pattern, a ceramic core.
13:55
This is gonna create a hollow inside the turbine blade.
13:59
So what's happening now is we're injecting into the die.
14:02
So that's the very start of the life of a turbine blade. -
14:06
That is really neat. - What we'll actually see is
14:08
that a lot of these features,
14:09
such as the aerofoil and the annular surfaces are not touched further.
14:13
So we will cast that,
14:13
and that will remain
14:14
as cast as it goes into the engine. (ominous music) - Every surface here
14:18
has to be perfect
14:19
because this wax is what will become the blade. -
14:23
So Kim is our wax pattern assembler.
14:26
So she's responsible for taking the product straight from that die,
14:30
making sure that things like die lines have been removed.
14:34
So where the die box come together and leave a small amount of flash,
14:37
the operative word in all of wax assembly is smooth. - Every tiny imperfection
14:41
in the wax would become a flaw in the metal.
14:43
So this takes an incredible amount of skill. (ominous music) -
14:47
Then it's the case of getting
14:48
that wax pattern attached to the unit runner to create the assembly. - I
14:51
mean,
14:51
the thought that occurs to me, right?
14:53
Shouldn't you be doing this with a robot? - Can, you know, like- - Yeah, yeah,
14:57
yeah.
14:57
So, Rolls-Royce has facilities that do this by robot,
15:00
but our facility in particular is very much focused on bringing in those new
15:04
products.
15:05
And it's far, far easier for us to work with human beings to develop
15:10
that method of manufacture that's going to bring the next generation of product through.
15:14
- I'll bet,
15:14
I can see the skill here,
15:15
like it's phenomenal. - Absolutely. - I'll just make a mess of it. - Absolutely,
15:18
so would I. - Would you like a go? - No. (laughs) (ominous music)
15:21
Once the wax assembly is perfect,
15:23
it's ready for the next stage. - Everything that is wax is gonna become air,
15:28
it's gonna become negative space, right?
15:29
It's gonna become our cavity.
15:31
And then we're gonna fill
15:32
that air with metal. (ominous music)
15:34
So we take that wax assembly,
15:35
and we've gotta build a shell. (pensive music) Shell is made of many different
15:40
layers.
15:40
It's a zircon-based shell system.
15:43
We're gonna dip into a primary story.
15:45
It's really quite thin,
15:46
like a light syrup
15:47
or a thin honey. - Oh yeah. (pensive music) -
15:50
And what that's designed to do is map all of those really complex geometric
15:53
features. - Beautiful. (engine droning) It's like making icing. -
15:58
So that's actually the analogy we use.
16:00
So, it's a bit like
16:01
if you put icing on top of a bun
16:03
or a cake,
16:04
you need to sprinkle it with some sugar afterwards, otherwise,
16:06
it's all gonna slop off the top.
16:08
So we've got the slurry on there.
16:09
We're gonna get a nice even coat, drain it,
16:11
make sure that it's an even thin layer.
16:13
And then we're gonna sand,
16:14
and that's then gonna set
16:16
that layer in place. -
16:17
So cool. (machine droning) Whoa. (machine droning) We're
16:21
then gonna dry it,
16:22
so it's air-dried for many, many hours.
16:24
And then we can create our backup layers.
16:26
So our backup layers, it's a much thicker slurry, more like a treacle,
16:29
and the sand is much coarser, more like a granulated sugar.
16:32
And we're gonna maybe put four, five, maybe even six layers to back up,
16:36
because what we need is we need a mold
16:38
that can withstand that casting parameters
16:41
that we're putting in the die.
16:41
You know, it's got a lot of work to do. - The wax is
16:45
then melted out,
16:47
and the mold is fired.
16:48
Oh, yeah. (machine whooshing) That is wild.
16:52
Cleaned and tested to make sure there aren't any cracks.
16:55
When it's done, this shell is ready to hold molten metal. - This is
16:59
a billet of alloy that's gonna fill the whole of
17:01
that mold.
17:02
So just that amount of metal is gonna fill
17:04
that whole mold there. - It doesn't look like an F. (ominous music) This
17:08
is a nickel alloy.
17:09
The first nickel alloys used in jet engines were developed in the 1940s.
17:13
By adding chromium and cobalt,
17:15
engineers created alloys that could handle 800 to 900 degrees Celsius,
17:20
around 100 degrees hotter than the steel used before.
17:23
And these alloys could keep their strength for thousands of hours,
17:27
a tenfold improvement in life.
17:29
But the real breakthrough came
17:31
when they added a touch of aluminum. (film whirring)
17:33
So we wanted to see how it held up under the same lab conditions
17:36
as the steel and titanium. - What temperature are we in now? - Oh,
17:40
that's 700 degrees. - 700, so the steel's long gone. - Steel's, long gone.
17:45
That's 800 degrees. 800, yes. (flames blasting) - In around this temperature,
17:50
it's actually getting stronger. (ominous music)
17:53
So why would heating a metal make it stronger?
17:56
Well, when these nickel alloys were first used in jet engines,
17:59
no one actually knew.
18:01
But about 10 years later,
18:02
electron microscopes had improved enough for engineers to finally see what was happening inside.
18:08
(ominous music) As we zoom in on the alloy,
18:10
a pattern emerges.
18:12
The microstructure isn't uniform.
18:14
Instead, it kind of looks like a city grid made up of blocks with
18:18
rods in between them.
18:20
Only, each block is so small,
18:22
over 300 would line up across the width of a human hair. (ominous music)
18:26
Now,
18:26
surprisingly, both the rods
18:28
and the blocks are made up of the exact same atoms,
18:30
mostly nickel with a little aluminum.
18:33
They even have the same crystal structure,
18:35
a grid of tiny cubes with atoms sitting at the corners
18:38
and at the center of each face.
18:40
The only difference is that the atoms are arranged slightly differently.
18:44
In the road structure, the aluminum and nickel can take any spot.
18:48
There is no repeating sequence from cube to cube.
18:51
And this is known as the gamma phase.
18:53
But in the blocks, aluminum always takes the corner spots, and nickel the faces,
18:59
and you get a perfect repeating pattern cube after cube.
19:02
This is the gamma prime phase.
19:04
And it's this difference
19:05
that is crucial when a dislocation tries to glide through the lattice.
19:09
In the rods, this motion is easy.
19:11
Each layer of atoms can shear smoothly past the next,
19:14
leaving the structure looking unchanged behind it.
19:17
But if you try to do the same thing in the blocks, well,
19:20
now you're actually changing the order of the atoms,
19:22
nickel and aluminum end up sitting in the wrong places.
19:26
That takes energy, so the lattice resists it.
19:29
So, when a dislocation moving through the rods hits a block, it gets stuck.
19:33
And that's what makes this alloy
19:34
so strong. - But
19:36
if you keep pushing
19:37
and the stress gets high enough,
19:38
dislocation can finally force its way in.
19:41
The catch is that this dislocation leaves the lattice in such a high-energy mess
19:45
that the only way
19:46
that it can keep moving is
19:47
if there's a second one right behind it
19:49
that puts things back in order.
19:51
So in the gamma prime phase, dislocations have to travel in pairs,
19:55
called super dislocations. - I need that creation of those super dislocations,
20:00
and I need that very high stress to be able to shear.
20:02
So that's why the strength is very high relative to other alloys.
20:06
What happens is, ultimately, because you're shearing through that gamma prime with two dislocations,
20:11
as the temperature continuously increases,
20:13
you're adding more and more thermal energy in the material.
20:15
What happens is the atoms are gonna vibrate more and more and more.
20:17
So there's a likelihood, as I'm doing this and I'm oscillating in three dimensions,
20:22
that the thermal energy is gonna drive me to actually slip down rather than
20:27
just slip in one plane.
20:29
So, now, if one cross slips, they're no longer on the same plane.
20:32
Think of it as if we're standing in line,
20:35
and the only way that you can move is I push you, right?
20:38
And then, I keep on pushing you, and then suddenly, you drop.
20:40
So if I now try to push you, I cannot find you, right?
20:43
You're not in front of me anymore.
20:44
Your shoulders are now below me. - Well, how do you touch 'em?
20:47
(laughs) (Jaafar laughs) - I should have used the other example, you pushing me.
20:51
But anyway. (both laughing) But it's exactly that.
20:54
It's the exact same analogy.
20:56
There's nothing to push me anymore.
20:57
There's like, I am not able to do it. (ominous music) -
21:00
So now you've got these two dislocations
21:02
that are on different planes,
21:03
so they can't travel together anymore.
21:05
And as a result, they're both now locked into place.
21:08
And you can see that effect on this graph.
21:10
While steel and titanium strength drops off, in the nickel super alloy,
21:14
you actually get a peak.
21:15
That's because the extra thermal energy lets more dislocations cross-slip and get separated.
21:20
And it's that that shuts down the motion of dislocations.
21:23
But if gamma prime is so strong,
21:26
why don't we just make the entire turbine blade out of it?
21:29
Well, that strength comes at a cost.
21:30
Gamma prime stops the dislocation so effectively that it becomes brittle.
21:35
All it takes is one crack or a sudden impact,
21:37
and it could lead to a sudden failure.
21:40
So the real trick is in striking the right balance between enough gamma prime
21:44
to trap the dislocations
21:45
and to prevent this creep,
21:46
but also enough gamma to keep the alloy ductile,
21:49
so that it can bend without breaking. - And in our test,
21:52
you can see exactly how that plays out. - A 1,000 degrees,
21:56
and still nothing. - Still nothing. (ominous music) (mold clanks) - There we go.
22:01
- Oh my gosh. (suspense music) - That's 1,100 degrees C. - It's stretching.
22:10
(suspense music) I mean,
22:10
it's still holding up like- - It's doing a good job.
22:13
That's 1,200 degrees C. - 1,200. (laughs) - That's the temperature program that stops.
22:19
And it's still surviving. - Still going. - But if you push the temperature too far,
22:24
even this alloy reaches its limits.
22:26
Cross-slip becomes easier.
22:27
The paired dislocations can now hop between the planes together,
22:31
and the ordered cubes of gamma primes start to dissolve.
22:34
So the dislocations break free, and it finally gives out. - Oh,
22:38
it may have just, did it break? - Oh, yeah, yeah, it did,
22:40
it broke. - But strength alone isn't what makes these alloys special.
22:45
When you heat up the alloy,
22:46
aluminum at the surface reacts with oxygen to form a thin continuous layer of
22:51
aluminum oxide.
22:52
Unlike the brittle oxides that form on other materials like steel or titanium,
22:56
this layer stays intact at high temperatures,
22:59
protecting the metal below. (suspense music) And by adding other elements,
23:03
we can tune these super alloys.
23:05
Each one brings a specific property that we want.
23:08
Most modern super alloys contain as many as 10 different elements,
23:12
all carefully balanced in their relative abundances for the desired properties.
23:16
Chromium improves resistance to oxidation and corrosion.
23:20
Cobalt, titanium, niobium, tantalum, and vanadium help stabilize the gamma prime phase.
23:25
Molybdenum and iron strengthen the gamma matrix.
23:28
And then there's rhenium.
23:29
Rhenium has one of the highest melting points of any metal at 3,180 degrees
23:33
Celsius.
23:35
It's second only to tungsten.
23:37
In the nickel super alloy, It slows the atomic-scale rearrangements,
23:41
enhancing the alloy's resistance to deformation even at temperatures above 1,000 degrees Celsius.
23:46
It's one of the rarest elements in the Earth's crust at less than one
23:50
part per billion.
23:52
And more than 80% of what we mine ends up right here in jet
23:56
engines. (ominous music) -
23:58
But even with these advancements in alloy chemistry,
24:01
there's still one fundamental problem.
24:04
And that's that metals are crystalline.
24:06
Any metal you see from the tip of this ballpoint pen to the spoon
24:10
in my coffee cup,
24:12
they're all actually made up of millions of little crystals stuck together.
24:16
It's kind of like grains in the sugar cube.
24:18
If I crush it... (ominous music) It's not like I've broken any individual crystal,
24:24
I've just broken them apart.
24:26
It's the boundaries between the grains that are the weak point.
24:29
And it's the same thing in a metal. (ominous music) - So,
24:32
if we zoom out from the gamma and gamma prime structure,
24:34
it looks something like this.
24:36
One crystal is basically a three-dimensional lattice of atoms all lined up in the
24:40
same orientation.
24:41
But the crystals themselves are all in different orientations.
24:45
So where they meet, their lattices don't line up.
24:47
And that mismatch leaves more open spaces and broken bonds.
24:51
And you also get defects there, like vacancies and impurities,
24:55
all of which make grain boundaries the weakest point.
24:58
And this also has another consequence.
25:00
It makes it easier for atoms to move along the boundaries.
25:04
They become kind of super highways for atomic diffusion.
25:07
This becomes even more of a problem at high temperatures
25:09
when atoms have more energy to move around,
25:12
add stress like the massive centrifugal loads on a turbine blade,
25:16
and the grains can actually start to slide past each other.
25:20
The whole structure slowly deforms, stretching,
25:23
almost like warm taffy. (ominous music) As long as it has grains in it,
25:27
it will creep, and fail far more easily.
25:30
And that's a really hard problem to solve because normally,
25:33
as a molten alloy cools, tiny crystals start to form all throughout the liquid.
25:38
So you have to find some way to control them. - This is one
25:42
of our furnaces.
25:43
They're all induction-heated, there's no kind of gas, fire, or anything like that,
25:47
and they're all under vacuum.
25:48
So, we only cast to the vacuum in the absence of any atmosphere,
25:51
but particularly oxygen, which is obviously metallurgically gonna cause us all kinds of problems
25:55
with oxides. - You start by pouring molten super alloy into a ceramic mold
25:59
that's mounted vertically and heated to about the same temperature
26:02
as the melt.
26:03
The mold fills from the root up toward the tip.
26:06
At the very bottom of the mold sits a copper plate cooled by water.
26:10
Its surface is patterned with tiny grooves
26:12
that act as nucleation points for the first crystals to start to form.
26:16
It's here that solidification begins.
26:18
Then, the entire mold is slowly lowered out of the hot zone,
26:22
so the solidification continues in just one direction. - It's a very slow process
26:27
in the magnitude of hours.
26:29
Once that's finished, the whole machine will then index round,
26:32
and it will push the completed mold up out of the other side. -
26:37
Oh. (machine humming) Wow. -
26:38
So our casting temperatures are roughly 1,500 degrees Celsius. - It's kind of at
26:43
the same temperature now
26:44
as it would be inside the jet engine. - Exactly. - It's absurd,
26:47
they like, you're making the turbine blades at the same temperature
26:50
that they're gonna operate,
26:51
but they like, here, they're liquid. (ominous music) Now,
26:53
if we just did that on its own,
26:55
you'd end up with a blade
26:56
that looks like this. (ominous music) - Here's a directionally solidified blade.
27:02
And what you can probably see there is the contrast between the grains.
27:07
These are all different crystals,
27:08
but they're all running on this axis of the blade,
27:12
which makes it significantly stronger than an alloy that is cast,
27:16
where all of the crystals are separate from each other. -
27:19
So those are like individual crystals. - These are individual crystals,
27:22
yeah, absolutely.
27:23
So we are looking at- - Wow. - At crystals on kind of a macro level,
27:27
where normally, we'd be talking about crystals on a micro level. (ominous music) -
27:31
In a rotating turbine,
27:33
the blade is being pulled along its length.
27:35
With columnar crystals all lined up along this span,
27:38
the blade can carry those stresses far more effectively.
27:41
There are no grain boundaries that cut across the blade,
27:43
creating weak points for it to crack.
27:45
But scientists have found a way to do even better.
27:48
If you introduce a bend in the mold just above the chill plate,
27:52
something strange happens.
27:54
The number of columnar crystals that make it through drops sharply.
27:58
And if you add another bend, even fewer survive. (ominous music) So,
28:02
engineers added a helical passage known
28:05
as the pigtail here at the bottom of the mold. - The pigtail is
28:08
doing the job to select the single crystal.
28:11
The spiral is gonna choke out every other grain bar one.
28:15
So we're only gonna have one grain
28:17
that is then gonna grow through the entirety of
28:20
that blade,
28:21
and cast that blade as a single crystal.
28:23
Or at least, that's the theory. - That's crazy. -
28:26
So this is a starter attached to a spiral
28:29
that we've etched so
28:29
that we can reveal
28:30
that structure.
28:31
So you can see down at the bottom,
28:33
we are starting to grow directionally solidified grains.
28:38
But as we get up here,
28:39
we can start to see that we're growing directionally solidified grains.
28:43
And then, as we're going up the spiral,
28:47
the grains are starting to be choked out by the upper surfaces of
28:49
that spiral until,
28:51
when we get to the top, we're just as a single crystal.
28:54
And then, that then allows
28:55
that to grow right the way through the blade. - Yeah,
28:58
that's amazing. - And what we should end up with is a blade like this.
29:01
So this is a blade of a single crystal.
29:04
It's a really impressive thing to look at. (ominous music) The shimmer is beautiful.
29:09
- Yeah. - Even after the blade solidifies,
29:11
it's still not ready for the engine.
29:13
It's heated again, almost to its melting point.
29:16
And that might sound risky
29:17
because we've spent all this time making sure it's a perfect single crystal.
29:21
But this heating step lets the atoms shuffle around just enough to spread out
29:26
evenly,
29:27
and form the final desired microstructure of the gamma
29:30
and gamma prime phases
29:31
that make these super alloys
29:33
so strong. - And
29:34
as if casting,
29:35
as a single crystal is not enough, actually,
29:37
the orientation of that crystal is also of paramount significance.
29:42
So you may have cast this as a single crystal,
29:45
but if the crystal orientation is off by a certain amount,
29:49
you get completely different stress responses within that blade. - Today, after decades of development,
29:56
over 95% of blades can be cast successfully as single crystals.
30:01
Just think about how incredible that is.
30:04
We've gone from a turbine blade
30:05
that contained on the order of 50,000 crystal grains down to just one.
30:10
When we grow these things, they don't solidify as a uniform front.
30:15
On a microscopic scale,
30:16
the solidification front looks like a forest of tiny tree-like branches called dendrites
30:22
that are pushing their way into the liquid.
30:24
At first glance, it looks messy, like millions of separate trees jostling for space.
30:30
There are up to 10 elements in there,
30:32
each with its own density and melting point.
30:35
Yet somehow, every one of those trees is locked into the exact same crystal
30:41
lattice.
30:42
So the final crystal is comprised of more than six times 10 to the
30:46
24 atoms,
30:47
that is more stars than there are in the observable universe.
30:51
When all these atoms are repeating the same pattern,
30:55
perfectly aligned from root to tip, this completely transformed what jet engines can do.
31:01
Single-crystal blades can withstand stresses and temperatures that would destroy ordinary alloys.
31:06
They last up to nine times longer against creep and thermal fatigue,
31:10
and are more than three times more resistant to corrosion than blades made from
31:14
multiple grains.
31:15
That's why modern jet engines can now run for 25,000 hours between major overhauls,
31:21
something that would've been unthinkable before single crystal blades. (suspense music)
31:25
And the impact has been huge.
31:27
Between 1960 and 2010, jet aircraft became about 55% more fuel efficient.
31:33
And a huge part of
31:34
that improvement comes down to advances in these nickel super alloys.
31:38
Back in the 1960s, flying was a luxury few could afford.
31:42
A one-way flight from New York to Paris would set you back $310,
31:46
which is about $3,750 adjusted for inflation.
31:50
But as engines became more efficient,
31:52
able to handle hotter cores and equipped with much larger fans,
31:56
airlines could carry more people farther using less fuel.
32:00
So, tickets got cheaper and air travel exploded.
32:03
Today, at any given moment,
32:04
there are roughly 10,000 to 14,000 planes in the sky.
32:08
That scale of movement is possible
32:10
because of these turbine blades. (jet hovering) In the furnace,
32:16
the nickel super alloy outperforms all the other samples,
32:19
surviving up to 1,200 degrees Celsius.
32:22
But wait, that's still 300 degrees less than the temperature inside a jet engine.
32:27
So why don't the blades melt?
32:29
Well, there are two final layers of defense.
32:32
The first is built into the shape of the blade itself. - We
32:36
then have to leach the core out.
32:37
So we do that in a caustic solution of potassium-sodium hydroxide under pressure
32:44
and temperature to leach the core out,
32:47
that will leave those core passages completely empty. -
32:51
And those passages are the real secret to the turbine blade survival. -
32:55
So as the air's flowing through,
32:57
it is turbulent, and as such,
32:58
it can remove much more heat from the surface of the blade. - Yeah.
33:02
- Than it was. - Is it these ridges here
33:04
that we're talking about? - Exactly,
33:04
yeah, yeah, these ridges here. - They're intentional to the trip the flow into-
33:08
- Trip and turbulate
33:09
that air flow so
33:10
that it's removing as much heat
33:12
as possible from the metal.
33:13
So then we get onto the really juicy part, which is film cooling.
33:16
So we talked about the ice cube in the ovens
33:18
that keeping our blades
33:20
as cool as possible.
33:21
So this is where we start to drill in what we call film cool
33:24
holes.
33:25
And what we're aiming to do is we're aiming to get into those cooling
33:29
passages.
33:29
So we saw that core earlier on.
33:31
They are the cooling passages inside.
33:34
And these holes have got to get right into those cooling passages to allow
33:37
the air to come out.
33:39
And the air is
33:40
then gonna blow as a film over the surface of the blade,
33:43
a film-cool hole to create a film of air,
33:46
which is preventing that metal from melting in those temperatures. - This cooling air
33:52
isn't exactly cold.
33:54
It actually comes from the high-pressure compressor section of the engine at around 600
33:59
degrees Celsius.
33:59
But that is cool enough to help keep the blades from melting.
34:02
But it's still not quite enough.
34:04
And you can't just add more cooling air
34:07
because every extra bit of air you use from the compressor,
34:10
you lose from thrust, and actually make the engine less efficient.
34:14
So every turbine blade is also coated with two protective layers.
34:19
First, a thin metallic bond coat that resists oxidation, and then a ceramic topcoat.
34:25
Even though it's only about a quarter of a millimeter thick,
34:28
this ceramic coating can keep the metal beneath it 100 to 170 degrees cooler
34:33
than it would otherwise be.
34:35
And this is the final barrier that stops the blades from melting.
34:38
So, now we've got this insane piece of engineering
34:41
that can survive the 1,500-degree gas.
34:44
The intense load and the oxidation problem should be solved.
34:49
Well, it would be, except for one thing, (ominous music) - At 36,000 feet,
34:55
you wouldn't believe this,
34:56
but there's dirt and dust in the atmosphere
34:59
that our engines are ingesting. (ominous music) The dirt
35:02
and dust comes,
35:03
it sticks on the blades, but it also goes through the whole cooling circuit,
35:08
and it walks the cooling from getting through to cool the blades,
35:14
and then the blades burn up.
35:15
Usually, every time I get on a plane, I'm thinking,
35:17
"This is never gonna work." (laughs) No,
35:20
I mean it's incredible how an engine can work 'cause there's
35:23
so many moving pieces,
35:24
there's so many parts to the environment, so terrible.
35:27
And now, we have this dust and dirt,
35:29
which is really bad. (intense music) - I am at Testbed 80,
35:33
and they're about to fire up this jet engine
35:36
and then throw dust into it.
35:39
The same stuff that makes up sand and volcanic ash,
35:42
exactly what real engines encounter in flight. - So this engine is the 97K.
35:47
It goes on the A350 and is our high-thrust version of that.
35:50
So 97,000 pounds of thrust is what this engine's producing.
35:54
When we're running a bit an engine like this,
35:56
we try and carefully recreate exactly what happens in service,
36:02
(intense music) - How much dust goes in the engine? - Not very much.
36:05
It was surprising when I found out exactly how much we put in.
36:07
It's in the order of tablespoons worth per cycle. - So, I (indistinct) master on.
36:13
Condition power on. (fan swooshing) (buttons clicking) Master fuel lever on.
36:17
Start request in three, two, one.
36:20
Now. (computer beeps) (intense music) (blades swooshing) - So,
36:28
what does the dust actually do inside a jet engine? - So,
36:32
once it goes through to the hot section of the engine
36:34
and hits kind of turbine blades,
36:36
it's gonna be melted.
36:37
And so, it sticks to the outside of our turbine components
36:41
and it slowly rips layers of
36:43
that thermal barrier coating off.
36:46
And then, you lose your temperature reduction that comes from the barrier coating,
36:51
so that your nickel alloy underneath it gets hotter and hotter,
36:54
and that's when it starts to deteriorate the turbine. (blades swooshing) - That's why
37:02
engineers at Rolls-Royce are still refining these blades,
37:05
developing new ceramic coatings designed to resist mold and dust,
37:08
and extend the life of the turbine by up to 30%.
37:12
That's just the latest step in a story that's been unfolding for decades.
37:15
These blades have been refined
37:17
and perfected to the point where they operate right at the edge of what
37:21
is physically possible.
37:23
You're always on a knife-edge, pushing every material,
37:26
every process to the limit to build an engine
37:28
that can do the seemingly impossible,
37:30
run hotter than its own melting point.
37:33
The more I learned about the brutal environment these blades have to survive,
37:37
the more it felt like they shouldn't work at all.
37:40
And yet, they do.
37:42
Every day, these machines carry millions of people across the world
37:46
and we barely stop to think about them,
37:48
they're a monument to human ingenuity.
37:51
What happens when we refuse to accept limits,
37:53
when we turn the impossible into the routine?
38:01
(ominous music) (scene change zooms) (ominous music) I can't grow a single-crystal turbine blade
38:04
in my kitchen,
38:05
but with the help from this video sponsor, KiwiCo,
38:07
I can grow a crystal garden with my kids.
38:11
This month, they sent us their Crystal Garden Chemistry Kit.
38:14
We set everything in place, mixed up the chemical solution,
38:16
and then watched as colorful crystals started to bloom over the next 48 hours.
38:21
Every few hours, my kids would run back to check how much the garden
38:24
had grown.
38:25
They were totally fascinated, and it sparked so many questions about crystals and atoms,
38:30
how things arrange.
38:31
Pretty soon, we were talking about how metals are crystalline, too,
38:34
and setting ourselves the challenge of growing one giant crystal turbine-blade style. (camera shuttering)
38:39
I love how simple KiwiCo makes this.
38:42
Everything we needed came right in the box,
38:44
so we could just open it up and dive straight in, doing the experiment.
38:48
And it's not just chemistry.
38:49
They've got crates for robotics, engineering, art, design techniques, and so much more.
38:54
There is something for every age
38:56
and interest. (scene change chimes) KiwiCo crates also make a great gift for the
39:00
holidays.
39:01
It's creative, hands-on,
39:02
and gives kids something they can actually make
39:04
and be proud of. - They're kind of messy. - Mm-hmm. -
39:08
And like hard to make,
39:11
but not too hard,
39:12
but hard enough to make it fun. - So if you wanna try out KiwiCo,
39:16
click the link in the description or scan this QR code.
39:19
Use my code Veritasium to get 50% off your first monthly crate.
39:23
I wanna thank KiwiCo for sponsoring this video,
39:25
and I want to thank you for watching.
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