Chapter 9: Phase Diagrams
Welcome to Last Minute Lecture.
This free chapter overview is designed to help students review and understand key concepts.
These summaries supplement not replaced the original textbook, and may not be redistributed or resold.
For complete coverage, always consult the official text.
Have you ever noticed how different materials transform around us?
Like think about a blacksmith, heating iron until it glows, then pounding it into a strong tool.
Oh yeah.
Or even just, you know, ice melting in your drink.
Simple stuff.
Right.
These everyday changes, solid to liquid, or maybe even shifts you can't see inside the material, there happens all the time.
But what if we could actually predict these transformations?
Like really precisely.
Like having a weather map,
but for materials.
Exactly.
A map telling us exactly what state a material will be in, and maybe even how to control it.
Well that's pretty much what phase diagrams are.
And that's our mission today.
We're taking a deep dive into phase diagrams.
These are essentially the ultimate cheat sheets, right?
For understanding how materials,
especially alloys, change their state and internal structure.
Absolutely.
If you're working with materials designing anything from, I don't know, spacecraft components to kitchen appliances, you need to understand these.
So we're going to pull out the key insights from Callister and Rethwish's Material Science and Engineering.
Trying to give you a clear grasp of these, well they can seem complex, but they're really powerful concepts.
Yeah, and what's truly fascinating here is how directly these diagrams connect the theory to the real world.
Practice.
How so?
They're critical because they let us predict a material's microstructure.
That's the internal arrangement of its different parts, its phases.
And that microstructure dictates everything.
Pretty much.
Its strength, how ductile it is, even electrical conductivity, it all links back.
So these diagrams aren't just academic theory.
They're vital for controlling manufacturing.
Things like melting, casting, crystallization.
Okay, so engineers use them to design heat treatments.
Predict how things behave.
Exactly.
Predict behavior under different conditions, design those heat treatments, and ultimately make materials that do exactly what you want them to do.
Create specific, desired properties.
Okay, so to really navigate these maps, we need to learn the language first.
Let's start with some basics.
Foundational terms.
First up,
a component.
What's that?
Right.
Simple one to start.
A component is just a pure metal or maybe a compound that makes up an alloy.
For instance?
Like brass.
The components are copper and zinc.
Simple as that.
Okay.
And you mentioned a system.
Yeah.
System can mean a couple of things.
It might be the specific chunk of material you're looking at, like a ladle full of molten steel.
Or it could mean the whole family of alloys you can make from those components, like the entire iron -carbon system.
It depends on context.
Got it.
Next term.
Mm -hmm.
Solid solution.
This sounds a bit like dissolving sugar in water, but solid.
Kind of.
It's when atoms of at least two different types mix together perfectly within a solid.
The key thing is, they blend into a single new material, but it keeps the original crystal structure of main component, the solvent.
So it's not just a mixture, it's blended at the atomic level.
Exactly.
And that's how we make alloys stronger or tougher than the pure metals they started from.
Like brass.
Again, tougher than pure copper or pure zinc.
But you can't just keep adding stuff indefinitely, right?
There must be a limit.
Precisely.
That's the solubility limit.
It's the absolute maximum concentration of the solute atoms, the stuff you're adding, that can dissolve into the solvent at a specific temperature.
Like your sugar in water example.
Add too much.
And the extra sugar just sits at the bottom.
It won't dissolve.
You've hit the solubility limit for that temperature.
And knowing that limit is crucial because it tells you if you'll get one uniform material or if it'll start separating into distinct parts.
Which brings us nicely to the idea of a phase.
What exactly is a phase in this context?
Okay, so a phase is any part of a system that's homogeneous, meaning it's uniform throughout and has distinct physical and chemical characteristics.
So in the sugar water case?
The liquid syrup is one phase.
Any undissolved solid sugar.
That's a second phase.
They're different physically, liquid versus solid,
and chemically, sugar versus sugar water solution.
But phases don't have to be chemically different.
Nope.
Think about ice and liquid water.
Both H2O, chemically identical.
But they're definitely distinct phases because their physical properties and structure are different.
Same goes for different crystal structures of the same solid material, like iron at different temperatures.
Those are separate phases too.
So if a system has just one phase, it's homogeneous.
Like perfectly dissolved salt water.
Right.
And if it has two or more phases, it's heterogeneous, like oil and water.
Or granite rock.
Most useful alloys are actually heterogeneous mixtures.
They're different phases worked together to give the desired properties.
And when we look closely, say, under a microscope, what we see is the microstructure.
Exactly.
The microstructure tells us how many phases there are, how much of each, and how they're arranged or distributed.
And that structure is hugely influenced by the components, their concentrations, and critically, any heat treatment the material has undergone.
It really dictates the material's overall behavior.
OK, so we have these phases.
How stable are they?
Are they fixed or always trying to change?
Good question.
That leads us to equilibrium.
A system is at equilibrium when its free energy is as low as it can possibly be for that specific temperature, pressure, and composition.
So it's like it's found its most comfortable, stable state.
Pretty much.
Its characteristics won't change over time.
And if you have more than one phase present and their characteristics stay constant, we call that phase equilibrium, like our saturated sugar water solution with the excess sugar sitting there.
That's phase equilibrium.
But you mentioned some materials aren't truly stable.
Right.
Many really important materials, like some high -strength steels or aluminum alloys used in aircraft, are actually in what we call a metastable state.
Metastable.
Meaning they're not truly at equilibrium, not in their lowest energy state.
But, and this is the key, the rate at which they would naturally change towards equilibrium is incredibly, incredibly slow.
So slow they seem stable for all practical purposes, maybe indefinitely.
And sometimes these stuck states are actually better.
Often, yes.
These metastable structures can have much better properties, like higher strength, than the true equilibrium structure would.
So metastability can be very useful technologically.
Wow.
Okay.
So something can look stable but be sort of frozen in a high -energy state.
How do we visualize all these transformations and stable states?
That's where the phase diagrams come in as our maps.
Let's start simple.
With one component, or unary phase diagrams, just one substance involved.
For water.
Exactly.
For a unary diagram, you plot pressure, usually up the vertical axis, against temperature along the horizontal axis.
Imagine the water diagram, figure 9 .2.
You'd see distinct regions labeled solid, ice, liquid, water, and vapor, steam.
And the lines between them.
Those are the phase boundaries.
Crossing one of those lines means a phase transformation is happening, melting, boiling, sublimating.
The lines show the exact conditions where two phases can coexist in equilibrium.
And there's that special point where all three lines meet.
That's the triple point.
A unique, fixed temperature and pressure where solid, liquid, and vapor can all exist
simultaneously in equilibrium.
It's an invariant point.
The conditions are totally fixed.
Okay, that makes sense for a pure substance.
But most engineering materials are mixtures.
Alloys.
What about them?
Right.
Now we get to binary phase diagrams, dealing with two components.
These are the really crucial ones for understanding alloys.
For these, we usually keep the pressure constant, typically just normal atmospheric pressure, one at LM.
So the axes are different.
Yep.
Temperature is still on the vertical axis, but the horizontal axis now represents composition.
It goes from 100 % of component A on one side to 100 % of component B on the other.
And the simplest type is?
The simplest is a binary isomorphous system.
Isomorphous means same structure.
In these systems, the two components are completely soluble in each other, no matter the proportions, in both the liquid state and the solid state.
Like dissolving completely.
Exactly.
A good example is the copper -nickel -cunei system.
If you picture its diagram, figure 9 .3a, you'd see temperature going up and composition along the bottom, say from pure copper to pure nickel.
There are three main regions.
Which are?
At high temperatures, there's a large region where everything is liquid, labeled L.
At low temperatures, there's a region where everything is a single solid solution, labeled alpha.
And sandwiched between them is a two -phase region, labeled Pu plus L, where solid alpha and liquid coexist.
So alpha is the solid solution?
Yes.
In this case, it's a substitutional solid solution of copper and nickel atoms mixed together in an FCC crystal structure.
They mix so well because copper and nickel atoms are quite similar in size and chemical properties.
Okay.
And those lines separating the regions?
Those are key.
The line separating the liquid L region from the two -phase plus L region is called the liquidus line.
Above that line, it's all liquid.
And the line below the two -phase region?
That's the solidus line.
It separates the solid alpha region from the two -phase life plus L region.
Below the solidus line, everything is solid alpha.
So a pure metal melts at one temperature.
Right.
A single point.
But alloys, mixtures like copper nickel, they melt or solidify over a range of temperatures.
That range is exactly the temperature gap between the solidus and liquidus lines at a given composition.
Inside that range, you have both solid and liquid present.
Okay.
So the diagram is like a materials UPS.
How do we actually use it to pull out specific info about an alloy at a certain point?
It boils down to answering three key questions, assuming your alloy is at equilibrium at a given temperature and overall composition.
First,
what phase or phases are present?
How do you find that?
Easy.
You just find your point on the diagram, locate the temperature on the vertical axis, the composition on the horizontal axis.
Whichever region that point falls into, that tells you the phase or phase is present.
Okay.
Using figure 9 .3a, the Cuny diagram,
if you have an alloy of 60 weight percent nickel, 40 % copper, and it's at 1100 degrees Celsius,
find that point.
It falls squarely in the alpha region, so only the solid alpha phase is present.
What if it's in the middle region?
Good question.
Let's say 35 weight percent nickel, 65 % copper at 1250 degrees Celsius.
Find that point B in the figure.
It's in the plus L region.
So both solid alpha and liquid phases are present together.
Okay.
Step one, identify the phases.
What's next?
Step two, what is the composition of each phase?
If your point is in a single phase region, like our first example in the alpha region, then the composition of that phase is simply the same as the overall alloy composition, 60 % nickel.
But what about the two -phase region, like point B?
How do we know the composition of the liquid and the solid alpha?
They can't both be 35 % nickel.
Exactly right.
They can't.
For a two -phase region, you need to use a tie line.
A tie line.
Yeah.
It's just a horizontal line, an isotherm, meaning constant temperature drawn across the two -phase region at the temperature you're interested in, so at 1250 degrees C for our point B example.
Okay.
Draw the line.
Then what?
See where that horizontal line intersects the phase boundaries on either side of the two -phase region.
In the CUNY example, figure 9 .3b, the tie line at 1250 degrees C hits the liquidus line on the left and the solidus line on the right.
And those intersection points tell us the compositions.
Precisely.
You drop vertical lines down from those intersection points to the composition axis at the bottom.
The intersection with the liquidus line tells you the composition of the liquid phase.
See y 'all.
The intersection with the solidus line tells you the composition of the solid alpha phase.
So for our 35 % knee alloy at 1250 degrees C.
Looking at figure 9 .3b, the pie line shows the liquid phase, Cl, has about 31 .5 weight percent nickel, and the solid alpha phase at U has about 42 .5 weight percent nickel.
Notice neither is the overall 35%.
Wow.
Okay.
So the two phases have different compositions determined by the ends of the tie line.
Makes sense.
So third question.
Third question.
What are the mass fractions or percentages of each phase?
How much liquid is there and how much solid alpha?
Okay.
How do we figure that out?
If you're in a single phase region, it's easy.
It's 100 % that phase.
But in a two phase region, we use the lever rule.
The lever rule.
Sounds like physics.
It's a mechanical analogy, like balancing a seesaw or a lever.
Imagine your tie line is the lever and it's balanced on a fulcrum placed at the overall alloy composition, C0.
Our 35 % night point.
Now, the fraction of one phase is determined by the length of the lever arm on the opposite side of the fulcrum divided by the total length of the lever, the whole tie line.
Opposite side.
Okay.
Explain that.
So to find the mass fraction of the liquid phase, WL, you take the length of the tie line segment from the overall composition, C0, over to the solid phase boundary and divide that by the total length of the tie line, CCl.
So the lever arm to the other phase boundary.
You got it.
And similarly, for the mass fraction of the solid alpha phase, you take the length from the overall composition, C0, over to the liquid phase boundary, Cl, and divide that by the total tie line length.
Let's try it for our 35 % night example at 1250 degrees C.
C0 45, Cl is 31 .5, C is 42 .5.
Okay.
So mass fraction liquid, WL, is C0, C0.
That's 42 .5 35 divided by 42 .5 31 .5.
Okay.
7 .5 divided by 11.
That's about 0 .68.
Spot on.
So about 68 % of the mass is liquid.
And the solid alpha, we should be C0, CCl.
Yep.
35, 31 .5 divided by 42 .5 31 .5.
So 3 .5 divided by 11, about 0 .32.
Exactly.
32 % solid alpha.
And notice 0 .68 plus 0 .32 equals 1 .0 or 100%.
It works out.
The lever rule.
Okay.
Seems powerful.
And you mentioned volume fractions.
Right.
The lever rule gives mass fractions.
If you know the densities of the liquid and solid phases, you can convert these mass fractions into volume fractions using some simple equations like 9 .6 and 9 .7 in the book.
Volume fractions are often more intuitive when you're thinking about what the microstructure actually looks like.
Makes sense.
So what does all this mean for how the material actually forms as it cools down?
How do these microstructures develop?
Great question.
Let's think about cooling that 35 weight percent nickel alloy starting from maybe 1300 degrees C where it's all liquid.
We need to consider two scenarios.
Equilibrium cooling and non -equilibrium cooling.
Equilibrium first.
That's the ideal slow case.
Right.
Very, very slow cooling, allowing everything to stay in balance.
As you cool the liquid described in figure 9 .4, you eventually hit the liquidus line.
At that point, the first tiny bit of solid alpha phase starts to form.
And its composition is given by the solidus line at that temperature.
Exactly.
Now, as you continue to cool slowly down through the U plus L region, two things happen simultaneously.
More solid forms, and importantly, the compositions of both the liquid and the solid continuously change, following the liquidus and solidus lines respectively.
Atoms have to diffuse around to make this happen.
So the solid that formed earlier has to change its composition as it cools further.
Yes.
That's key for equilibrium.
By the time you cool just below the solidus line, the last drop of liquid disappears.
And you're left with a solid alpha phase that has a completely uniform composition 35 % nickel throughout.
But that requires atoms moving around in the solid, which sounds slow.
What happens in real life with faster cooling?
Ah, now we get to non -equilibrium cooling.
You nailed it.
Diffusion in solids is often very slow compared to cooling rates in industrial processes like casting.
Atoms just don't have enough time to rearrange themselves perfectly to maintain equilibrium compositions.
So what's the result?
You often get what's called a chord structure.
The very centers of the solid grains, which solidified first at higher temperatures, will be richer in the higher melting point element, in this case, nickel.
As cooling continues, the layers solidifying later towards the outside of the grains become progressively richer in the lower melting point element, copper.
So you get non -uniform grains, like little bulls -eyes of composition.
Exactly.
This microscopic segregation can lead to weaker or less consistent properties compared to a uniform material.
Can you fix it?
Often, yes.
You can perform a homogenization heat treatment.
This involves heating the solidified alloy to a temperature below the solidus line, but high enough for diffusion to become significant.
Holding it there allows atoms to move around and even out those concentration differences, eliminating the chord structure.
Okay.
And how do these compositions affect the final mechanical properties, like strength?
Generally for isomorphous systems like copper -nickel, adding the second component increases strength and hardness.
This is called solid solution strengthening.
It usually peaks somewhere in the middle compositions, as shown in figure 9 .6a.
What about ductility, the ability to stretch or bend?
Ductility usually is the opposite.
It tends to decrease as you add more the second element, often showing a minimum value at some intermediate composition, figure 9 .6b.
So there's often a trade -off between strength and ductility when alloying.
All right.
We've covered isomorphous systems complete mixing, but you said many systems have limited solubility.
Yes.
And that leads to different, often more complex phase diagrams.
This brings us to binary eutectic systems.
Eutectic.
What does that mean?
Eutectic comes from Greek, meaning easily melted.
These systems have a special composition that melts at a lower temperature than any other composition in that system.
Okay.
What does the eutectic diagram look like?
Say for copper -silver, QAG, figure 9 .7.
It looks more complex than the isomorphous one.
You'll still have temperature versus composition.
You'll see regions at the ends representing solid solutions, like an alpha phase, mostly copper with a little silver dissolved, and a beta phase, mostly silver with a little copper dissolved, but their solubility is limited.
So unlike cunei, they don't mix completely in the solid state.
Correct.
The boundary line showing the limit of solubility in the solid state is called a solvus line.
You still have liquidus and solidus lines too, but the shapes are different.
You'll see regions labeled OO, liquid L, and also two -phase regions like OO plus L plus L, and importantly, LU plus VET at lower temperatures.
And the key feature is the eutectic reaction.
Exactly.
There is a specific point on the diagram called the eutectic point, point E in figure 9 .7.
It has a specific composition, the eutectic composition CE, and occurs at a specific temperature, the eutectic temperature TE.
For QAG, it's 71 .9W0 %G at 779 degrees C.
What happens at that point?
At the eutectic temperature, as the liquid with the eutectic composition cools, it undergoes the eutectic reaction.
The entire liquid transforms isothermally at constant temperature into two distinct solid phases simultaneously.
The reaction is liquid solid alpha plus solid beta.
One liquid becomes two solids all at once.
Precisely.
There's a horizontal line on the diagram at the eutectic temperature called the eutectic isotherm.
It represents the lowest temperature at which any liquid can exist in equilibrium in this system.
You mentioned lead tin, PBSN is another example, figure 9 .8.
Yes, a very important one, especially for solders.
It looks quite similar to QAG.
The lead -rich solid phase is alpha, the tin -rich solid phase is beta.
The eutectic point for PBSN is at 61 .9 weight percent tin at 183 degrees Celsius.
That's quite a low melting point.
It is.
And that specific composition, or ones very close to it, like 60 -40 solder, melts sharply at that low temperature, which makes it ideal for joining electronic components without damaging them.
And can we still use tie lines and the lever rule in these eutectic diagrams?
Absolutely.
The principles are exactly the same.
If you're in a two -phase region, like the nu plus region, you draw a tie line at your temperature of interest.
The ends tell you the compositions of the alpha and beta phases.
Then you use the lever rule with your overall alloy composition to find the mass fractions of alpha and beta.
Okay, let's take an example.
Problem 9 .2 uses a 40W percent ensent 60W2 percent TB alloy at 150 degrees phi, looking at figure 9 .9.
Right.
Find that point B on the diagram.
It's well within the few plus region below the eutectic temperature.
Draw a tie line horizontally at 150 degrees C across that region.
Okay.
Where does it hit the boundaries?
The tie line intersects the boundary of the alpha phase field, the solvus line, at about 1150 percent sen.
So the alpha phase composition, C, is 11 percent sen, is 89 percent sen.
It intersects the beta phase boundary at about 98 percent sen.
So the beta phase composition is 98 percent sen, sen, 2 percent sen, sen.
And the amounts.
Problem 9 .3 calculates mass fractions using the lever rule.
Yeah.
For the 40 percent en alloy, C0, C0, C0, 40.
Mass fraction alpha, 98, 40, 98, 11, and equals 58, 87, which is about 0 .67 or 67 percent.
So mass fraction beta must be 1 .67 equals 0 .33 or 33 percent.
Exactly.
Well, calculate it.
C0, C0, 40, 11, 98, 11 equals 29, 87, which is 0 .33.
And again, you could convert these to volume fractions using densities, which might give different percentages if the densities of alpha and beta are very different as they are in PBSN.
So the eutectic reaction is key.
How does this affect the microstructures that form when these alloys cool down?
Are they uniform, like in the isomorphous case?
Generally no.
The microstructures in eutectic systems can be quite varied and interesting, depending on the composition.
Let's use lead tin as our example and think about four cases.
Case one.
Case one.
Very low tin content, like composition C1 in figure 9 .11.
As it cools from liquid, it just passes through the L plus region and becomes solid alpha phase, maybe with a little tin dissolved.
Looks pretty uniform, similar to the isomorphous case.
Okay.
Case two.
Case two.
A bit more tin, but still less than the maximum that can dissolve an alpha at the eutectic temperature, like C2 in figure 9 .12.
It cools, forming solid alpha grains, but then as it cools further below the eutectic temperature, it crosses the solvus line.
The solubility limit line in the solid state.
Right.
The alpha phase becomes super saturated with tin, so tiny particles of the beta phase rich in tin start to precipitate out and grow within the solid alpha grains.
You end up with alpha grains containing small beta particles.
Interesting.
Case three.
The special one.
Case three.
The alloy has exactly the eutectic composition.
C3 in figure 9 .13, 61 .9 percentage and not.
As this liquid cools and hits the eutectic temperature, 183 degrees C, the entire liquid transforms via the eutectic reaction L plus no.
And what does that microstructure look like?
It forms a very characteristic eutectic structure.
Usually it consists of alternating thin layers or plates called lamellae of the two solid phases, alpha and beta, that grow together.
If you looked at it under a microscope, like figure 9 .14, you'd see colonies of these parallel stripes often looking like a fingerprint or mother of pearl.
Wow, layered stripes of alpha and beta.
Why does it form like that?
It's all about diffusion, shown conceptually in figure 9 .15.
For the liquid to transform into alpha, PB rich, and beta, lead atoms need to move to the growing alpha layers, and tin atoms need to move to the growing beta layers.
This layered structure minimizes the distance atoms have to diffuse, making the transformation happen efficiently.
Clever stuff.
Okay, final case.
Case four.
Case four.
An alloy composition that is not eutectic, but still cools down through the eutectic isotherm, like C4 in figure 9 .1C, which is hypotectic, meaning less tin than eutectic.
What happens here?
As it cools from liquid, it first enters a two -phase region, say L plus A.
Large crystals of the primary phase, in this case primary alpha, start to form and grow.
As they grow, the remaining liquid becomes richer in tin, until the temperature reaches the eutectic isotherm, 183 degrees C.
At this point, the remaining liquid has exactly the eutectic composition, and that liquid then transforms into the lamellar eutectic structure, alpha plus beta layers.
So the final microstructure is a mix.
Exactly.
You see relatively large, distinct regions of the primary alpha phase that form first, surrounded by the colonies of the fine lamellar eutectic structure that formed later.
Figure 9 .17 shows this kind of structure.
We need a term for these distinct parts.
We call them microconstituents.
A microconstituent is an element of the microstructure with an identifiable characteristic structure.
So in this case, the primary alpha is one microconstituent, and the entire eutectic structure, the lamellar mix of alpha and beta, is the other microconstituent.
Can we calculate how much primary alpha versus how much eutectic structure we get?
Yes.
We use the lever rule again, but apply it slightly differently, as shown in Figure 9 .18.
To find the fraction of the primary alpha microconstituent, you use a tie line at the eutectic temperature, but only consider the segment between the boundary of the alpha phase field, a prox, 18 .3 % N for PBSN, and the eutectic composition, 61 .9 % at N.
You put the fulcrum at your overall alloy composition, C4.
So it tells you the fraction of stuff that formed before the eutectic reaction.
Precisely.
And the lever arm to the other side tells you the fraction of the eutectic microconstituent.
Then, if you want the total fraction of alpha phase, including primary alpha and the alpha within the eutectic structure, you use the lever rule across the entire alpha plus beta field at a temperature below the eutectic, just like we did before.
And non -equilibrium cooling affects these too.
Oh yes.
Rapid cooling can lead to cored primary phases and can shift the relative amounts, often resulting in more eutectic structure than predicted by the equilibrium diagram.
Okay, we've covered isomorphous and eutectic systems, but I imagine diagrams can get even more complicated.
They certainly can.
Many real -world systems involve more than just the simple alpha and beta phases at the ends.
You can have intermediate phases or compounds.
Well, you might have intermediate solid solutions.
These are distinct solid solution phases that exist at compositions within the diagram, not just near the pure components.
The copper -zinc -brass diagram, figure 9 .19, is full of them beta, gamma, delta, epsilon phases.
They have different crystal structures and properties from the terminal alpha and eta phases.
And compounds.
You can also have intermetallic compounds.
These have a specific fixed chemical formula like Mg2Pb in the magnesium -lead system, figure 9 .20.
On the phase diagram, they often appear as vertical lines, indicating a fixed composition.
These compounds can be very hard and brittle.
Do these intermediate phases melt differently?
Some melt congruently, meaning they transform from solid to liquid at a single temperature without changing composition, just like a pure element, or the Mg2Pb compound at point M in figure 9 .20.
Others might melt incongruently, involving other phases.
And besides the eutectic reaction, are there other important invariant reactions?
Yes, several others, where three phases coexist in equilibrium at a specific temperature and composition.
A really important one is the eutectoid reaction.
Eutectoid.
Sounds like eutectic.
Similar idea, but it happens entirely in the solid state.
A single solid phase transforms into two different solid phases upon cooling.
So, solid one, solid two, plus solid three.
The copper -zinc diagram, figure 9 .21, shows one.
The delta phase transforms into gamma plus epsilon at 560 degrees C.
Okay.
Any others?
Another key one is the peritectic reaction.
Here, upon cooling, a liquid phase and one solid phase react to form a different solid phase.
So, liquid plus solid one is solid two.
Again, the q -z diagram shows an example.
Delta phase plus liquid transforms into epsilon phase at 598 degrees C.
Eutectic, eutectoid, peritectic.
Lots of transformations.
Is there a rule governing all this?
There is.
It's a fundamental thermodynamic rule called the Gibbs phase rule.
It relates the number of phases P that can coexist in equilibrium, the number of components C, and the number of degrees of freedom, basically.
The independent variables like temperature, pressure, or composition you can change while still staying in that equilibrium state.
What's the rule itself?
It's usually written as P plus F equals C plus N, where N is the number of non -compositional variables like temperature and pressure.
For most binary diagrams where pressure is fixed, N one, so the rule simplifies to P plus F equals C plus one.
Since C two, for binary systems, it's P plus F equals three.
How does that help interpret the diagram?
Let's use QAG, figure 9 .23.
Okay.
In a single phase region, like L or nu du A, P one, so F three P equals three one equals two.
Two degrees of freedom.
This means you need to specify both temperature and composition to uniquely define the state of the system.
Makes sense.
What about a two -phase region, like nu plus L?
Here P two.
So F equals three P equals three two equals one.
Only one degree of freedom.
If you specify the temperature, the compositions of the two phases are automatically fixed by the ends of the tie line.
Or if you specify the composition of one phase, the temperature and the other phase's composition are fixed.
And at an invariant point, like the eutectic reaction, there are three phases, L, U, are in equilibrium, so P three.
Then F three P equals three, three equals zero.
Zero degrees of freedom.
Everything is fixed.
The temperature is the eutectic temperature, and the compositions of all three phases are fixed.
You can't change anything and still have all three phases coexisting.
The Gibbs phase rule.
Underlying principle.
Okay, let's unpack this.
This is a big one.
The iron -iron carbide, FA3C phase diagram.
You said this is maybe the most important one.
Arguably, yes.
It's the basis for understanding all steels and cast irons, which are incredibly dominant structural materials.
This diagram, figure 9 .24, is essential.
Okay, let's break it down.
What are the key phases here?
At room temperature, the main phase in pure iron or low carbon steel is ferrit, or alpha iron, CUFI.
It has a BCC, body -centered cubic crystal structure.
Crucially, it can dissolve very little carbon max, about 0 .022 weight percent at 727 degrees C.
It's relatively soft and magnetic.
Figure 9 .25A shows what it looks like.
Okay, soft ferrite.
What else?
As you heat iron up, it transforms into austenite, or gamma iron, nufa.
This has an FCC, face -centered cubic structure.
The really important thing about austenite is that it can dissolve a lot more carbon up to 2 .14 weight percent at 1147 degrees C.
Those FCC interstitial sites are bigger.
Austenite is non -magnetic, and it's the key phase for heat -treating steels.
Figure 9 .25B shows its typical grain structure.
Higher carbon solubility in austenite, got it.
Any other iron phases?
There's also delta ferrite, mynaphahe at very high temperatures, also BCC, but it's less technologically important for most applications.
And the iron carbide part, is that a phase?
Yes.
The diagram technically goes up to 6 .70 weight percent carbon, which corresponds to the intermediate compound cementite, chemical formula F3C.
Cementite is extremely hard and brittle.
Its presence, even in small amounts mixed with ferrite, is what gives steel its strength.
Is cementite stable?
Technically, it's metastable.
Given enough time at high temperature, it would slowly decompose into alpha iron and graphite.
But under normal conditions and timescales, it's effectively stable and is treated as an equilibrium phase in this diagram.
Okay, ferrite, austenite, cementite.
What are the key invariant reactions on this diagram, the special points?
Two main ones for us.
There's a eutectic reaction way up at 1147 degree C and 4 .30 weight percent carbon.
Here, liquid transforms into austenite plus cementite, LU plus Fe3C.
This is mainly relevant for the solidification of cast irons.
The other one.
You said it was vital for steels.
Yes, the eutectoid reaction.
This happens at 727 degree C and a composition of 0 .76 weight percent carbon.
Here, solid austenite transforms into solid alpha ferrite plus solid cementite at 0 .022 per C plus Fe3C, 6 .7 per C.
This transformation is absolutely fundamental to steel microstructures and heat treatment.
Eutectoid.
One solid becomes two solids.
Okay.
And how do we classify these alloys based on carbon?
Generally, irons have very little carbon, less than 0 .008W2 percent, basically pure ferrite.
Steels are defined as having between 0 .008 and 2 .14W2 percent carbon.
Their typical room temperature microstructure is a mix of ferrite and cementite.
Cast irons have more carbon, from 2 .14 up to 6 .78 percent, although commercial ones are usually below 4 .5 percent.
Right.
So focusing on steels, how do these microstructures actually develop during slow cooling?
This must be where things like perlite come in.
Exactly.
Let's consider slow cooling equilibrium scenarios.
First, imagine we have steel with exactly the eutectoid composition.
0 .76 weight percent carbon, figure 9 .26.
We cool it down from the austenite region,
say, from 800 degrees C.
What happens?
Nothing happens until we hit the eutectoid temperature, 727 degrees C.
At that exact temperature, all the austenite transforms isothermally via the eutectoid reaction, plus Fe3C, into a specific micro -constituent called perlite.
Perlite.
Use it.
Perlite is a lamellar structure, just like the eutectic structure we discussed.
It consists of fine, alternating layers or plates of alpha ferrite, which is soft and ductile, and cementite, which is hard and brittle.
Under a microscope, figure 9 .27, it often has a pearly or iridescent look, hence the name.
Layers of ferrite and cementite.
How does that form?
Again, it's diffusion, figure 9 .28.
As the austenite transforms, carbon atoms need to move out of the regions becoming ferrite, which has low carbon solubility, and into the regions becoming cementite, which is carbon -rich.
The layered structure minimizes the diffusion distance, allowing both phases to grow cooperatively.
So eutectoid steel becomes 100 % perlite on slow cooling.
What if we have less carbon than that?
Hypotectoid steel.
Good question.
Let's take a steel with, say, 0 .4 % carbon, composition C0s in figure 9 .29.
We cool it from the austenite region.
As it enters the U plus 2 phase region below the A3 line, crystals of ferrite start to form, usually nucleating at the austenite grain boundaries.
This ferrite that forms before the eutectoid reaction is called pro -tectoid ferrite.
Okay, so alpha starts forming first.
What happens to the remaining austenite?
As the pro -tectoid ferrite forms, it rejects carbon into the remaining austenite, so the austenite gets progressively richer in carbon.
This continues until the temperature reaches the eutectoid line, 727 degrees sap.
At this point, the remaining austenite has reached exactly 0 .76 % carbon, the eutectoid composition.
And that austenite then transforms.
Exactly.
That remaining austenite transforms into perlite, the lamellar nu plus F3C mixture.
So the final microstructure at room temperature consists of regions of the relatively soft pro -tectoid ferrite mixed with colonies of the harder perlite.
Figure 9 .30 shows a typical example.
Can we calculate how much pro -tectoid ferrite versus perlite we get?
Yes, using the lever rule again.
We draw a tie line just above the eutectoid temperature across the nu plus region, extending from the ferrite boundary 0 .022 per cc to the austenite boundary, austenite boundary 0 .76 per cc.
Put the fulcrum at your overall alloy composition, 0 .4 per c in our example.
The lever arm towards the austenite side tells you the fraction of pro -tectoid ferrite.
The arm towards the ferrite side tells you the fraction of austenite that will become perlite.
See figure 9 .31 and equations 9 .20, 9 .21.
Makes sense.
Now what if we have more carbon than eutectoid, but still less than 2 .14 % hyper -eutectoid Okay, let's say we have 1 .1 % carbon, composition C1 in figure 9 .32.
We cool from the austenite region.
This time as we cross the boundary into the plus FA3C region, the olymium line, the phase that starts to form first is pro -tectoid cementite.
It usually forms along the austenite grain boundary.
So hard brittle cementite forms first this time.
Right.
And as it forms, it takes carbon out of the remaining austenite, making the austenite poorer in carbon.
This continues until, again, we reach 727 degrees C.
At this point, the remaining austenite has been depleted down to exactly 0 .76 % carbon.
And it transforms to perlite.
You got it.
That remaining austenite transforms into perlite.
So the final microstructure is islands or networks of the hard pro -tectoid cementite mixed with colonies of perlite.
Figure 9 .33 shows this.
And we can calculate the amounts here too.
Yep.
Same lever rule principle, just applied differently.
Just above 727 degrees C, use a tie line across the tuna plus F3C region, extending from the austenite boundary 0 .76 % C to the cementite boundary, 6 .70 % C.
Put the fulcrum at your overall alloy composition, 1 .1 % C.
The lever arm towards the austenite side gives the fraction of pro -tectoid cementite.
The arm towards the cementite side gives the fraction of austenite that becomes perlite.
Figure 9 .31 again, equations 9 .22, 9 .23.
It's amazing how changing just the carbon content shifts the balance between ferrite, cementite, and perlite, giving different properties.
Do other elements added to steel affect this diagram?
Oh, profoundly.
Adding elements like chromium, nickel, molybdenum, vanadium, etc.
common in alloys, steels dramatically alters the FeF3C diagram.
They can significantly shift the eutectoid temperature up or down, figure 9 .34, and also change the eutectoid carbon composition, figure 9 .35.
This is fundamental to how we create alloy steels with specific hardness, toughness, corrosion resistance, and high temperature strength.
It opens up a whole world beyond plain carbon steels.
Wow, we really have journeyed through a lot today, haven't we, from the basic definitions like components and phases?
Yeah, through the simple water diagram then into binary systems.
Right, the isomorphous like copper -nickel, learning about tie lines, the lever rule, then the eutectics like lead tin with that special reaction and the layered microstructure.
And finally, the big one, iron carbon, understanding ferrite, austenite, cementite, and how perlite forms in eutectoid, hypoeutectoid, and hyper -eutectoid steels.
Exactly.
We've seen how these diagrams are truly like maps, guiding us through material transformations.
They help predict what phases are present, their compositions, their amounts, and we touched on equilibrium versus the realities of non -equilibrium cooling, which is so important in practice.
It really shows how microstructure is key.
Absolutely.
And how it's controlled by composition and thermal history, all visualized through these diagrams.
They're just invaluable tools for materials engineers.
So here's something to maybe hue on.
Think about designing the next generation of materials, maybe of super lightweight, incredibly strong alloy for, I don't know, a hypersonic plane, or maybe a perfectly reliable, environmentally friendly solder for microelectronics.
Designing those materials relies entirely on this fundamental understanding how elements interact, how phases transform at different temperatures.
Now imagine,
what new, maybe revolutionary properties could we unlock if we could gain even finer control over these phase transformations, maybe in even more complex systems with three, four, five components?
What's possible then?
That is a fascinating thought.
Where could that lead?
No.
Okay.
We really hope this deep dive into phase diagrams has given you a solid footing, a good foundation for understanding this is a crucial part of material science.
Yeah, hopefully it makes navigating those diagrams a bit less daunting.
Thank you so much for joining us on the deep dive.
And a special thank you from the whole last minute lecture team.
β This audio and summary are simplified educational interpretations and are not a substitute for the original text.
Using this chapter to study? Last Minute Lecture is free and student-run. If it helped, consider supporting the project.
Support LML β₯Related Chapters
- Gibbs Free Energy & Binary Phase DiagramsIntroduction to the Thermodynamics of Materials
- Thermodynamics & Phase DiagramsPhase Transformations in Metals and Alloys
- Phase Equilibrium in One-Component SystemsIntroduction to the Thermodynamics of Materials
- Fugacity, Activity, and Ellingham DiagramsFundamentals of Metallurgical Thermodynamics
- Introduction & Key Thermodynamic TermsIntroduction to the Thermodynamics of Materials
- Metallic Structures II: Topologically Close-Packed PhasesStructure of Materials: An Introduction to Crystallography, Diffraction and Symmetry