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  • I've now done a bunch of videos on thermodynamics, both

  • in the chemistry and the physics playlist, and I

  • realized that I have yet to give you, or at least if my

  • memory serves me correctly, I have yet to give you the first

  • law of thermodynamics.

  • And I think now is as good a time as any.

  • The first law of thermodynamics.

  • And it's a good one.

  • It tells us that energy-- I'll do it in this magenta color--

  • energy cannot be created or destroyed, it can only be

  • transformed from one form or another.

  • So energy cannot be created or destroyed, only transformed.

  • So let's think about a couple of examples of this.

  • And we've touched on this when we learned mechanics and

  • kinetics in our physics playlist, and we've done a

  • bunch of this in the chemistry playlist as well.

  • So let's say I have some rock that I just throw as fast as I

  • can straight up.

  • Maybe it's a ball of some kind.

  • So I throw a ball straight up.

  • That arrow represents its velocity vector, right?

  • it's going to go up in the air.

  • Let me do it here.

  • I throw a ball and it's going to go up in the air.

  • It's going to decelerate due to gravity.

  • And at some point, up here, the ball is not going to have

  • any velocity.

  • So at this point it's going to slow down a little bit, at

  • this point it's going to slow down a little bit more.

  • And at this point it's going to be completely stationary

  • and then it's going to start accelerating downwards.

  • In fact, it was always accelerating downwards.

  • It was decelerating upwards, and then it'll start

  • accelerating downwards.

  • So here its velocity will look like that.

  • And here its velocity will look like that.

  • Then right when it gets back to the ground, if we assume

  • negligible air resistance, its velocity will be the same

  • magnitude as the upward but in the downward direction.

  • So when we looked at this example, and we've done this

  • tons in the projectile motion videos in the physics

  • playlist, over here we said, look, we have some kinetic

  • energy here.

  • And that makes sense.

  • I think, to all of us, energy intuitively means that you're

  • doing something.

  • So kinetic energy.

  • Energy of movement, of kinetics.

  • It's moving, so it has energy.

  • But then as we decelerate up here, we clearly have no

  • kinetic energy, zero kinetic energy.

  • So where did our energy go?

  • I just told you the first law of thermodynamics, that energy

  • cannot be created or destroyed.

  • But I clearly had a lot of kinetic energy over here, and

  • we've seen the formula for that multiple times, and here

  • I have no kinetic energy.

  • So I clearly destroyed kinetic energy, but the first law of

  • thermodynamics tells me that I can't do that.

  • So I must have transformed that kinetic energy.

  • I must have transformed that kinetic energy

  • into something else.

  • And in the case of this ball, I've transformed it into

  • potential energy.

  • So now I have potential energy.

  • And I won't go into the math of it, but potential energy is

  • just the potential to turn into other forms of energy.

  • I guess that's the easy way to do it.

  • But the way to think about it is, look, the ball is really

  • high up here, and by virtue of its position in the universe,

  • if something doesn't stop it, it's going to fall back down,

  • or it's going to be converted into another form of energy.

  • Now let me ask you another question.

  • Let's say I throw this ball up and let's say we actually do

  • have some air resistance.

  • So I throw the ball up.

  • I have a lot of kinetic energy here.

  • Then at the peak of where the ball is, it's all potential

  • energy, the kinetic energy has disappeared.

  • And let's say I have air resistance.

  • So when the ball comes back down, the air was kind of

  • slowing it down, so when it reaches this bottom point,

  • it's not going as fast as I threw it.

  • So when I reach this bottom point here, my ball is going a

  • lot slower than I threw it up to begin with.

  • And so if you think about what happened, I have a lot of

  • kinetic energy here.

  • I'll give you the formula.

  • The kinetic energy is the mass of the ball, times the

  • velocity of the ball, squared, over 2.

  • That's the kinetic energy over here.

  • And then I throw it.

  • It all turns into potential energy.

  • Then it comes back down, and turns into kinetic energy.

  • But because of air resistance, I have a

  • smaller velocity here.

  • I have a smaller velocity than I did there.

  • Kinetic energy is only dependent on the magnitude of

  • the velocity.

  • I could put a little absolute sign there to show that we're

  • dealing with the magnitude of the velocity.

  • So I clearly have a lower kinetic energy here.

  • So lower kinetic energy here than I did here, right?

  • And I don't have any potential energy left.

  • Let's say this is the ground.

  • We've hit the ground.

  • So I have another conundrum.

  • You know, when I went from kinetic energy to no kinetic

  • energy there, I can go to the first law and

  • say, oh, what happened?

  • And the first law says, oh, Sal, it all turned into

  • potential energy up here.

  • And you saw it turned into potential energy because when

  • the ball accelerated back down, it turned back into

  • kinetic energy.

  • But then I say, no, Mr. First Law of Thermodynamics, look,

  • at this point I have no potential energy, and I had

  • all kinetic energy and I had a lot of kinetic energy.

  • Now at this point, I have no potential energy once again,

  • but I have less kinetic energy.

  • My ball has fallen at a slower rate than I

  • threw it to begin with.

  • And the thermodynamics says, oh, well that's

  • because you have air.

  • And I'd say, well I do have air, but where

  • did the energy go?

  • And then the first law of thermodynamics says, oh, when

  • your ball was falling-- let me see, that's the ball.

  • Let me make the ball yellow.

  • So when your ball was falling, it was rubbing

  • up against air particles.

  • It was rubbing up against molecules of air.

  • And right where the molecules bumped into the wall, there's

  • a little bit of friction.

  • Friction is just essentially, your ball made these molecules

  • that it was bumping into vibrate a little bit faster.

  • And essentially, if you think about it, if you go back to

  • the macrostate/ microstate problem or descriptions that

  • we talked about, this ball is essentially transferring its

  • kinetic energy to the molecules of air that it rubs

  • up against as it falls back down.

  • And actually it was doing it on the way up as well.

  • And so that kinetic energy that you think you lost or you

  • destroyed at the bottom, of here, because your ball's

  • going a lot slower, was actually transferred to a lot

  • of air particles.

  • It was a lot of-- to a bunch of air particles.

  • Now, it's next to impossible to measure exactly the kinetic

  • energy that was done on each individual air particle,

  • because we don't even know what their microstates were to

  • begin with.

  • But what we can say is, in general I transferred some

  • heat to these particles.

  • I raised the temperature of the air particles that the

  • ball fell through by rubbing those particles or giving them

  • kinetic energy.

  • Remember, temperature is just a measure of kinetic-- and

  • temperature is a macrostate or kind of a gross way or a macro

  • way, of looking at the kinetic energy of

  • the individual molecules.

  • It's very hard to measure each of theirs, but if you say on

  • average their kinetic energy is x, you're essentially

  • giving an indication of temperature.

  • So that's where it went.

  • It went to heat.

  • And heat is another form of energy.

  • So that the first law of thermodynamics

  • says, I still hold.

  • You had a lot of kinetic energy, turned into potential,

  • that turned into less kinetic energy.

  • And where did the remainder go?

  • It turned into heat.

  • Because it transferred that kinetic energy to these air

  • particles in the surrounding medium.

  • Fair enough.

  • So now that we have that out of the way, how do we measure

  • the amount of energy that something contains?

  • And here we have something called the internal energy.

  • The internal energy of a system.

  • Once again this is a macrostate, or you could call

  • it a macro description of what's going on.

  • This is called u for internal.

  • The way I remember that is that the word internal does

  • not begin with a U.

  • U for internal energy.

  • Let me go back to my example-- that I had in the past, that I

  • did in our previous video, if you're watching these in

  • order-- of I have, you know, some gas with some movable

  • ceiling at the top.

  • That's its movable ceiling.

  • That can move up and down.

  • We have a vacuum up there.

  • And I have some gas in here.

  • The internal energy literally is all of the energy that's in

  • the system.

  • So it includes, and for our purposes, especially when

  • you're in a first-year chemistry course, it's the

  • kinetic energy of all the atoms or molecules.

  • And in a future video, I'll actually calculate it for how

  • much kinetic energy is there in a container.

  • And that'll actually be our internal energy plus all of

  • the other energy.

  • So these atoms, they have some kinetic energy because they

  • have some translational motion, if we look at the

  • microstates.

  • If they're just individual atoms, you can't really say

  • that they're rotating, because what does it mean for an atom

  • to rotate, right?

  • Because its electrons are just jumping around anyway.

  • So if they're individual atoms they can't rotate, but if

  • they're molecules they can rotate, if it looks

  • something like that.

  • There could be some rotational energy there.

  • It includes that.

  • If we have bonds-- so I just drew a molecule.

  • The molecule has bonds.

  • Those bonds contain some energy.

  • That is also included in the internal energy.

  • If I have some electrons, let's say that this was not

  • a-- well I'm doing it using a gas, and gases aren't good

  • conductors-- but let's say I'm doing it for a solid.

  • So I'm using the wrong tools.

  • So let's say I have some metal.

  • Those are my metal-- let me do more-- my metal atoms. And in

  • that metal atom, I have, a bunch of electrons-- well

  • that's the same color-- I have a bunch of-- let me use a

  • suitably different color-- I have a bunch

  • of electrons here.

  • And I have fewer here.

  • So these electrons really want to get here.

  • Maybe they're being stopped for some reason, so they have

  • some electrical potential.

  • Maybe there's a gap here, you know, where they can't conduct

  • or something like that.

  • Internal energy includes that as well.

  • That's normally the scope out of what you'd see in a

  • first-year chemistry class.

  • But it includes that.

  • It also includes literally every form of energy that

  • exists here.

  • It also includes, for example, in a metal, if we were to heat

  • this metal up they start vibrating, right?

  • They start moving left and right, or up or down, or in

  • every possible direction.

  • And if you think about a molecule or an atom that's

  • vibrating, it's going from here, and then it goes there,

  • then it goes back there.

  • It goes back and forth, right?

  • And if you think about what's happening, when it's in the

  • middle point it has a lot of kinetic energy, but at this

  • point right here, when it's about to go back, it's

  • completely stationary for a super small moment.

  • And at that point, all of its kinetic energy

  • is potential energy.

  • And then it turns into kinetic energy.

  • Then it goes back to potential energy again.

  • It's kind of like a pendulum, or it's

  • actually harmonic motion.

  • So in this case, internal energy also includes the

  • kinetic energy for the molecules that are moving

  • fast. But it also includes the potential energies for the

  • molecules that are vibrating, they're at that point where

  • they don't have kinetic energy.

  • So it also includes potential energy.

  • So internal energy is literally all of the energy

  • that's in a system.

  • And for most of what we're going to do, you can assume

  • that we're dealing with an ideal gas.

  • Instead of, it becomes a lot more complicated with solids,

  • and conductivity, and vibrations and all that.

  • We're going to assume we're dealing with an ideal gas.

  • And even better, we're going to assume we're dealing with a

  • monoatomic ideal gas.

  • And maybe this is just helium, or neon.

  • One of the ideal gases.

  • They don't want to bond with each other.

  • They don't form molecules with each other.

  • Let's just assume that they're not.

  • They're just individual atoms. And in that case, the internal

  • energy, we really can simplify to it being the kinetic

  • energy, if we ignore all of these other things.

  • But it's important to realize, internal energy is everything.

  • It's all of the energy inside of a system.

  • If you said, what's the energy of the system?

  • Its internal energy.

  • So the first law of thermodynamics says that

  • energy cannot be created or destroyed, only transformed.

  • So let's say that internal energy is changing.

  • So I have this system, and someone tells me, look, the

  • internal energy is changing.

  • So delta U, that's just a capital delta that says, what

  • is the change an internal energy?

  • It's saying, look, if your internal energy is changing,

  • your system is either having something done to it, or it's

  • doing something to someone else.

  • Some energy is being transferred to it

  • or away from it.

  • So, how do we write that?

  • Well the first law of thermodynamics, or even the

  • definition of internal energy, says that a change in internal

  • energy is equal to heat added to the system-- and once again

  • a very intuitive letter for heat, because heat does not

  • start with Q, but the convention is

  • to use Q for heat.

  • The letter h is reserved for enthalpy, which is a very,

  • very, very similar concept to heat.

  • We'll talk about that maybe in the next video.

  • It's equal to the heat added to the system, minus the work

  • done by the system.

  • And you could see this multiple ways.

  • Sometimes it's written like this.

  • Sometimes it's written that the change in internal energy

  • is equal to the heat added to the system, plus the work done

  • on the system.

  • And this might be very confusing, but you should just

  • always-- and we'll really kind of look at this 100 different

  • ways in the next video.

  • And actually this is a capital U.

  • Let me make sure that I write that as a capital U.

  • But we're going to do it 100 different ways.

  • But if you think about it, if I'm doing work I lose energy.

  • I've transferred the energy to someone else.

  • So this is doing work.

  • Likewise, if someone is giving me heat that is increasing my

  • energy, at least to me these are reasonably intuitive

  • definitions.

  • Now if you see this, you say, OK, if my energy is going up,

  • if this is a positive thing, I either have to have this go

  • up, or work is being done to me.

  • Or energy is being transferred into my system.

  • I'll give a lot more examples of what exactly that means in

  • the next video.

  • But I just want to make you comfortable

  • with either of these.

  • Because you're going to see them all the time, and you

  • might even get confused even if your teacher

  • uses only one of them.

  • But you should always do this reality check.

  • When something does work, it is transferring energy to

  • something else, right?

  • So if you're doing work, it'll take away, this is taking

  • away, your internal energy.

  • Likewise, heat transfer is another way for energy to go

  • from one system to another, or from one entity to another.

  • So if my total energy is going up, maybe heat is being added

  • to my system.

  • If my energy is going down, either heat is being taken

  • away from my system, or I'm doing more work on something.

  • I'll do a bunch of examples with that.

  • And I'm just going to leave you with this video with some

  • other notation that you might see.

  • You might see change in internal energy is equal to

  • change-- let me write it again-- change in internal

  • energy, capital U.

  • You'll sometimes see it as, they'll write a delta Q, which

  • kind of implies change in heat.

  • But I'll explain it in a future video why that doesn't

  • make a full sense, but you'll see this a lot.

  • But you can also view this as the heat added to the system,

  • minus the change in work, which is a little

  • non-intuitive because when you talk about heat or work you're

  • talking about transferring of energy.

  • So when you talk about change in transfer it becomes a

  • little-- So sometimes a delta work, they just mean this

  • means that work done by a system.

  • So obviously if you have some energy, you do some work,

  • you've lost that energy, you've given it to someone

  • else, you'd have a minus sign there.

  • Or you might see it written like this, change in internal

  • energy is equal to heat added-- I won't say even this

  • kind of reads to me as change in heat.

  • I'll just call this the heat added-- plus the work done

  • onto the system.

  • So this is work done to, this is work done by the system.

  • Either way.

  • And you shouldn't even memorize this, you should just

  • always think about it a little bit.

  • If I'm doing work I'm going to lose energy.

  • If work is done to me I'm going to gain energy.

  • If I lose heat, if this is a negative number, I'm going to

  • lose energy.

  • If I gain heat I'm going to gain energy.

  • Anyway, I'll leave you there for this video, and in the

  • next video we'll really try to digest this internal energy

  • formula 100 different ways.

I've now done a bunch of videos on thermodynamics, both

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