00:00:00
Life is chaos.
The whole universe is chaos.
00:00:04
Whether it's the terrible state of my office
or the slow degradation of my body into dust,
00:00:09
the universe tends toward disorder.
00:00:12
But why, why is the universe structured in
this terrible and callous way?
00:00:17
Well, it turns out that it's not really the
universe's fault.
00:00:19
If you think about it there's only one way, or at best, maybe a few ways for things to be arranged in an organized way.
00:00:25
But there are nearly infinite other ways for
those same things to be arranged.
00:00:30
The simple rules of probability dictate that
it's much more likely for stuff,
00:00:34
whether it's the stuff on my desk or the particles
and energy that make up my concept of self,
00:00:38
to be in one of the many disorganized states
than in one of the few organized states.
00:00:43
It's simple math and it's unavoidable.
00:00:45
So unavoidable that it is in fact our Second
Law of Thermodynamics, which says that:
00:00:50
"Any spontaneous process increases the disorder
or randomness of the universe."
00:00:56
Processes that don't increase the disorder of the universe require work to be done in opposition to the disorder,
00:01:01
and are in fact often impossible to achieve.
00:01:04
The very act of putting one system in order
requires that other systems become disordered.
00:01:09
Think of it this way: Your lunch was composed
of an extremely ordered set of molecules.
00:01:14
And it gave you the energy to clean up your
house, maybe.
00:01:17
And it had to be broken down into less ordered
nutrient molecule for you to do that.
00:01:21
Carbohydrates, proteins, and lipids, and those
molecules were broken down even further as
00:01:25
they were converted to energy in your cells,
00:01:28
and your body used some of that energy to
power your muscles as you cleaned your house.
00:01:32
But a bunch of that energy was used to do things like keep your heart beating, and breathe, and make sweat,
00:01:37
and some of that was lost to the surroundings in the form of random movement, and most importantly, heat.
00:01:42
By the time you've finished your house may be orderly but the remains of your lunch molecules are all over the place.
00:01:48
And that's only one of the many systems that
became less orderly while you worked.
00:01:52
So yes, cleaning your house in fact increased
the overall disorder of the universe.
00:01:57
Next time someone gives you a hard time about the state of your house you can tell them that.
00:02:01
Obviously disorder is a pretty big deal in the universe, and that makes it a pretty big deal in chemistry.
00:02:06
So scientists have a special name for it:
entropy.
00:02:09
Entropy is a measure of molecular randomness,
or disorder.
00:02:12
And even though people complain about
the disorder in their lives, it's not all bad news.
00:02:17
Entropy helps make chemical reactions possible,
00:02:19
and it helps us predict how much useful work
can be extracted from a reaction.
00:02:23
We all have to live with disorder so you might
as well understand it.
00:02:26
For the next ten minutes I want you to embrace
the chaos.
00:02:29
[Theme Muusic]
00:02:39
So what does the Second Law of Thermodynamics
mean when it says:
00:02:42
"Any spontaneous process increases the disorder
of the universe."
00:02:46
"Spontaneous" simply means a process that
doesn't need outside energy to keep it going.
00:02:51
And it goes the other way too, anything that increases the disorder of the universe happens spontaneously.
00:02:55
That doesn't mean disorderly things will always
happen though, other factors may interfere.
00:03:00
The reaction to change a diamond into graphite,
for example, would be thermodynamically spontaneous.
00:03:04
It wouldn't have to be forced along by outside
energy,
00:03:07
but the bonds in the diamond are so stable
that essentially it never gets started.
00:03:11
Lots of other chemical reactions are like
this too.
00:03:13
So even though we think of "spontaneous" meaning sudden and impulsive, like the majority of mall lip piercings,
00:03:18
in chemistry "spontaneous" doesn't tell you
how quickly something happens,
00:03:21
it only means a reaction is thermodynamically capable of happening without outside energy to move it along.
00:03:27
Though come to think of it, I imagine that spontaneous lip piercings cause a fair amount of disorder as well,
00:03:32
especially upon arriving home.
00:03:34
Entropy is another state function.
00:03:35
It doesn't depend on the pathway the system
took to reach its current state.
00:03:38
So even though we can't measure the entropy of reactants or products directly, we can calculate them.
00:03:43
We can also calculate the change in entropy during a reaction exactly like we can for the change in enthalpy,
00:03:49
by subtracting the sum of the reactant values
from the sum of the product values.
00:03:53
In other words, the formulas look exactly
the same, just substituting "S"
00:03:56
(which for some reason is used to denote entropy)
for "Delta H F".
00:04:00
Notice we dropped the "Delta"s on the right
side of the formula
00:04:03
because we know absolute values for entropy
of individual reactants and products.
00:04:08
We keep the "Delta" on the left
00:04:09
because we're calculating the change in entropy that occurs when the reactants rearrange into products.
00:04:14
What the heck is this good for?
00:04:15
Well, we can explain a mysterious thing, which
is how reactions occur spontaneously in nature
00:04:21
even though there's no energy given off, or
even they suck energy out of the environment,
00:04:25
and seem to go up the energy ladder instead
of down.
00:04:28
Let's try it out with a real reaction here
on my desk -- this is one of my favorites.
00:04:33
This is barium hydroxide octahydrate and this
is ammonium chloride.
00:04:37
Usually we do chemical reactions in aqueous solution because most solids don't interact easily,
00:04:43
but this pair is exception to that rule; they
react readily in solid form.
00:04:47
This reaction absorbs a lot of heat from the surroundings, making everything around it feel cold.
00:04:51
Now to show you how cold it gets, I'm going
to do something here.
00:04:55
And you're just going to have to assume you
understand what I'm doing.
00:04:59
"What am I doing? What is happening? Why am
I doing this? That's weird Hank.
00:05:03
Why are you doing that?" And then I put that
on there.
00:05:07
So now I've dumped barium hydroxide in this beaker, I'm gonna dump the ammonium chloride in.
00:05:11
And now one of the by-products of this reaction is ammonia so I'm gonna have to smell that, but you don't.
00:05:18
Oooh ye-eah, look at that slush.
00:05:21
I think we've reacted pretty much completely here and so we should, if all things have gone properly --
00:05:28
yep, that's pretty cool --- sucked enough heat out of the block of wood to actually freeze it to the beaker.
00:05:37
Normally in chemistry a reaction that proceeds spontaneously and yet absorbs heat is really weird.
00:05:44
Basically I have a hard time believing what
I just did.
00:05:47
So what does entropy have to do with this
little freak show?
00:05:51
You might think it has something to do with taking the heat from the surroundings to make the system colder,
00:05:55
but while that's counter-intuitive and cool,
that's not all of it.
00:05:57
You might also think that it has to do with two solids combining to form a whole bunch more liquids and gases,
00:06:03
and that IS a big part, but still not all.
00:06:06
To understand what we just saw a little better,
we need to put it all together.
00:06:09
Let's start by finding out exactly how much heat it did absorb and what happened to the entropy as well.
00:06:15
First, we'll find the enthalpy change using
Hess's Law and standard enthalpies of formation.
00:06:20
We can use the coefficients from the balanced chemical equation to fill in the number of moles for each substance.
00:06:25
Then we have to look up a whole bunch of numbers
00:06:27
(remember, you can find tables like this online and probably in the back of your chemistry textbook too).
00:06:31
When we plug the standard enthalpies of formation
into the formula and do the math,
00:06:35
we find that the change in standard enthalpy
is plus 166 kilojoules.
00:06:39
It's positive, which makes sense because the
reaction absorbed the thermal energy,
00:06:43
enough to create about a half a kilogram of ice if it had been surrounded by water instead of air and fingers.
00:06:48
Next, we'll find the entropy change: remember,
the basic equation is the same.
00:06:52
We put in the number of moles from the balanced
chemical equation
00:06:54
and the standard entropies from the table
00:06:56
and a quick calculation tells us that the change in standard entropy is 590 joules per Kelvin.
00:07:02
A positive result means the entropy of the
reaction increased,
00:07:05
meaning the products were more disordered
than the reactants.
00:07:09
Note that the standard enthalpy is in kilojoules while the standard entropy is in joules per Kelvin.
00:07:14
The energy units should match, so let's call
the standard entropy 0.594 kilojoules per Kelvin.
00:07:19
It doesn't look like much right now, but wait,
there's more.
00:07:23
Those numbers don't explain why the reaction
proceeds spontaneously,
00:07:26
even though it scavenges all that heat from
the environment.
00:07:29
But Josiah Willard Gibbs, he found a way to
explain it, and he didn't even mean to.
00:07:34
Gibbs was interested in the amount of energy in a system that was available or free to do useful work.
00:07:40
Today, we call this Gibbs free energy or sometimes the standard free energy or simply free energy of the system.
00:07:47
Like enthalpy or entropy, Gibbs free energy is a state function, so it can be calculated the same way.
00:07:52
We simply substitute "Delta G," which stands
for Gibbs free energy, for "Delta H" or "S."
00:07:56
The standard free energy of formation, written
like this,
00:08:00
is the change of free energy that occurs when a substance is formed from its elements at a standard state.
00:08:05
It's analogous to the standard enthalpy of formation that we use to calculate change in enthalpy.
00:08:09
Like enthalpy and entropy, we can't directly
the free energy change of the whole reaction.
00:08:13
So scientists created a baseline by setting
the standard free energy change of formation
00:08:18
for an element in its most stable form at
standard state to zero.
00:08:23
The standard free energy change of formation
for a compound, then,
00:08:26
is just the difference between its standard
free energy and that baseline.
00:08:29
But what if you don't know the standard free energies of formation for the products and reactants?
00:08:34
Well, they're often listed in tables, but
sometimes the ones you need aren't available.
00:08:39
Never fear, Willard Gibbs has an app for that.
It's actually a formula, but he figured it out.
00:08:44
In 1873, Gibbs calculated that at constant
pressure and temperature,
00:08:48
the change in standard Gibbs free energy for
a reaction equal the change in standard enthalpy
00:08:53
minus the product of the temperature and the
change in standard entropy.
00:08:57
In other words, the amount of free energy a reaction makes available to do work depends on two
00:09:01
and only two things: the enthalpy change,
the amount of heat the reaction transfers,
00:09:06
and the entropy change, the amount of disorder
it creates at a given temperature.
00:09:11
So which is more important, the heat transfer
or the disorder? Well, it depends.
00:09:15
A large change in enthalpy can determine the
direction of a free energy change,
00:09:19
even if the entropy changes in the opposite
direction, and vice versa.
00:09:22
If the absolute value of the change in enthalpy is greater than the absolute value of the product of the temperature
00:09:28
and the change in entropy (or "T Delta S"),
then we say that the reaction is enthalpy-driven.
00:09:33
this means that the flow of thermal energy
provides most of the free energy in the reaction.
00:09:38
On the other hand, if the absolute value of "T Delta S" is greater than the absolute value of the enthalpy change,
00:09:43
we call the reaction entropy-driven, meaning increasing disorder provides most of the reaction's free energy.
00:09:49
Which type was the barium hydroxide reaction?
00:09:52
Well, I'm gonna say that the temperature in here is about 25 degrees Celsius, or 298.15 Kelvin,
00:09:58
because I'm awesome like that -- I can just
tell.
00:10:00
When we multiply that by the change in entropy
that we calculated,
00:10:04
0.594 kilojoules per kelvin,
we get a value of 177 kilojoules.
00:10:07
If we compare that to the change in enthalpy
we calculated, 166 kilojoules,
00:10:12
it is clear that the "T Delta S" is higher than the "Delta H", so the reaction is entropy-driven -- no surprise there.
00:10:19
Even though the reaction absorbed a lot of thermal energy, this phenomenon was dwarfed by the increase in entropy.
00:10:25
And this makes sense, because the balanced
equation goes from three total moles of solids,
00:10:31
with their molecules locked in place, to one mole of solid, ten moles of liquid, and two moles of gas.
00:10:38
This is a massive increase in disorder,
00:10:40
because in addition to the fact that there are now 13 moles of particles to move around instead of just 3,
00:10:45
the liquid and gas are particularly good at
moving around,
00:10:48
so most of those particles are in random motion,
no longer stuck in one spot,
00:10:53
causing a large increase in disorder, or entropy.
00:10:55
But here's the coolest part, Gibbs formula also tells us whether the reaction is spontaneous or not.
00:11:00
We know all systems tend toward the lowest possible energy state, whether its a ball rolling down a hill,
00:11:05
elastic springing back into shape, or positive
and negative ions forming a bond.
00:11:10
"Delta G" is a type of energy, obviously, so it spontaneously approaches the minimum possible level.
00:11:16
So if the value for "Delta G" is negative, that is if the free energy decreases, the reaction is spontaneous.
00:11:22
Reactions that are able to release free energy
don't need external energy to make them proceed,
00:11:27
and that's the very definition of a spontaneous
reaction.
00:11:30
So if "Delta G" is positive, the reaction is non-spontaneous, but the reverse reaction is spontaneous.
00:11:35
If "Delta G" is zero, the reaction is in an equilibrium state and no discernible occurs in either direction.
00:11:41
So what about the reaction I just did?
00:11:43
Is it spontaneous at room temperature? Can
it occur without energy driving it along?
00:11:47
Well, yes because we just watched it happen,
but let's do the math!
00:11:50
Using Gibbs Formula and plugging in the numbers
we've calculated so far,
00:11:53
we see that the Gibbs free energy for this
reaction is negative 11 kilojoules.
00:11:58
It is indeed spontaneous, because it releases energy instead of requiring it in order to get started.
00:12:03
The energy that was produced was used to rearrange
the bonds in the reactants,
00:12:06
to make smaller product molecules, to break
attractions between molecules,
00:12:10
and to push some of the particles apart from
solid form into liquid and gas form,
00:12:14
which increased the entropy of the system.
00:12:16
So even though the reaction absorbed a lot of thermal energy, it didn't NEED that energy to make it proceed,
00:12:22
because the large change in entropy alone
was enough to keep things moving along.
00:12:26
So Gibbs formula confirms our earlier results with just one little subtraction -- pretty smart guy.
00:12:32
And now, some of his smartness has been transferred
into you,
00:12:36
now that you've watched this episode of Crash
Course Chemistry.
00:12:39
If you paid any attention, you learned:
00:12:41
that it's hard to stay organized because there
are so many ways to be disorganized,
00:12:46
that the second law of thermodynamics says
disorder, or entropy, happens everywhere,
00:12:50
and that the change in entropy ultimately depends on how much room molecules have to move around in,
00:12:55
how much heat heat energy they have to give off in reactions, and the temperature around them.
00:12:59
You learned about Josiah Willard Gibbs and his formula to calculate the Gibbs free energy for a reaction,
00:13:04
that both entropy and Gibbs free energy are
state functions,
00:13:07
and that the sign of the Gibbs free energy
tell us whether or not a reaction is spontaneous.
00:13:12
This episode of Crash Course Chemistry was
written by Edi Gonzalez.
00:13:15
The script was edited by Blake de Pastino, and our chemistry consultant was Dr. Heiko Langner.
00:13:20
It was filmed, edited and directed by Nicholas Jenkins. Our script supervisor was Caitlin Hofmeister.
00:13:25
Our sound designer is Michael Aranda, and
our graphics team is Thought Cafe.