By *Isaac Asimov
In the game
of energy and thermodynamics you
can’t even
break even
Two great laws describe flow and change
of the universal prime mover; it
is never created and never disappears.
What a pleasure it is to be
young, and hopeful, and unsophisticated.
All things are possible, and we are ready in our heart of hearts, to
believe that a fairy godmother may just come and wave her want, and turn our rags
into a lavish costume and our hovel into a mansion. Why shouldn’t an enchanted ring exist
somewhere that will, at a rub, load our pockets with gold and jewels? Or why should not a jinn, slave to our
commands, build a castle for us in the twinkling of an eye and fill it with
dancing girls?
If this
has not happened, we might wistfully imagine that it is only because we just
haven’t been lucky enough to find the fairy godmother, or the enchanted ring,
or the jinn. All we need is that
incredible stroke of luck, and we will have something for nothing.
But never
mind fairies, rings, and jinns; in the real world it is energy that is the
prime mover of all. We can define energy
as anything that makes it possible to do work, anything capable of bringing
about movement against resistance. In
that case, we see at once that there must be various forms of energy.
______________________________
*Chemist, professor, writer—Dr. Asimov kindly
helps you understand the second law of thermodynamics
Smithsonian, v. 1, no. 5, (August,
1970), p. 4-11.
Heat will
make a thread of mercury rise against the pull of gravity; light will turn the
vanes of a radiometer against the slowing effect of friction. Electricity will turn a motor, magnetism
raise a pin, a moving bat hurl a baseball over the fence, exploding dynamite
lift a boulder, a hydrogen bomb in action heave a huge mountain.
Heat,
light, electricity, magnetism, motion, sound, chemical bonds, nuclear
forces—all represent forms of energy, and all are different forms of
essentially the same thing, for one form can be freely turned into
another. Electricity moving through a
wire can produce light, and a paddly rotating rapidly in water can produce
heat. Magnetism can be turned into
electricity, chemical explosions into motion, nuclear reactions into sound, and
so on.
We have
now sharpened the problem of getting something for nothing and can consider it
realistically. Whatever we want costs us
energy, for it is only energy (by definition) that will allow work to be
done. To be sure, we may need other
things as well. To build a palace we
need not only the energy to lift materials but also a certain architectural
knowledge—but we need energy at the very
least. Without energy, all the
architectural knowledge in the world wouldn’t budge one grain of sand.
To get something
for nothing, then, is just another way of saying this: We want to create some
energy that did not exist before.
But, alas,
this apparently can’t be done. In the
1840s, as a result of careful experimentation and measurement, several
physicists came more or less simultaneously to the conclusion that energy cannot
be created. One form of energy can be
converted into another, or transported from one place to another, but that is
as far as we can go.
But wait,
that isn’t all. If energy cannot be
created, neither can it be destroyed.
When energy is used, it doesn’t disappear; it merely goes elsewhere or
is changed into another form. The light
that streams out of a candle does not vanish; it heats up the air and
surroundings about itself. The hot water
in a kettle may cool down but the heat does not disappear; it is transferred to
the outside world.
To express all this, we can say: “energy
can be transferred from one place to another, or transformed from one form to
another, but it can be neither created nor destroyed.” Or, we can put it another way: “The total
quantity of energy in the universe is constant.”
When the total
quantity of something does not change, we say that it is conserved. The two statements given above, then, are two
ways of expressing “the law of conservation of energy.” This law is considered the most powerful and
most fundamental generalization about the universe that scientists have ever
been able to make.
No one
knows why energy is conserved, and no
one can be completely sure it is truly conserved everywhere in the universe and
under all conditions. All that anyone
can say is that in over a century and a quarter of careful measurement,
scientists have never been able to point to a definite violation of energy
conservation, either in the familiar everyday surroundings about us, or in the
heavens above or in the atoms within.
Conservation is the starting point
The study of changes of energy from one form to
another and the transport of energy from one place to another is called
“thermodynamics” (from Greek words meaning “heat motion”), because the earliest
studies of the sort were made on the manner in which heat flowed from one part
of a system to another. For that
reason the law of conservation of energy is sometime called the First Law of
Thermodynamics. It is first because it
is the starting point for all else in the study. Before you can come to any useful conclusions
in thermodynamics, you must accept the fact that energy can be neither created
nor destroyed.
Once that
is accepted, we might decide that even so we have not entirely lost. In the game of the universe maybe we can
still win. If we can’t get something for
nothing, maybe the First Law will allow us to get something for almost nothing.
For instance, heat is a form of energy,
and we can make it do work. Moreover it
is all around us—in the earth under our feet, in the air, in lakes and oceans
and winter snows. Suppose we take a quantity of heat and change it into
work. In doing so, we haven’t destroyed
the heat, we have only transferred it to another place or perhaps changed it
into another energy form. Why can’t we
then simply gather it up, wherever it is and in whatever form, and use it again
and again and again?
If we can
do so, then even if we can’t create energy out of nothing we can at least start
with just a little energy and make it do any amount of work. By using the energy of a burning candle over
and over we could move the world; and it would be a greedy man indeed who
wouldn’t be satisfied, or who would
Smithsonian, v. 1, no. 5, (August,
1970), p. 4-11.
complain he wasn’t really getting something for
nothing.
Alas, it sounds good, but it can’t be
done. The trouble is that once energy is
used, it still exists, but it is spread out thinner. The heat of the burning candle spreads out
into the air all about and into all the things the warm air comes into contact
with.
For that heat to work again, it has to be
collected from the surroundings and concentrated again so that the candle flame
is re-created. Heat can be concentrated, energy can
be collected—but it takes energy to do so, invariably more energy than the
energy you are concentrating and collecting.
(Think of
your air conditioner. It collects heat
from a cool room and discharges it, at higher temperature, into the outside
air. Why not use just such a heat pump
to concentrate heat where we want it?
Then we could let the heat flow once again from a hot place to a cold
place, making it turn motors, lift weights and generate electric currents as it
went. We’ve found a jinn after all! But there is a joker in the deck that
overrides the jinn. More energy is
needed to run the air conditioner than we can get back by letting the heat run
back from hot to cold.)
What is the sense in using fresh energy to
collect dissipated old energy, and using more to get less? You might as well use the fresh to begin
with. It is more economical. In short, in your attempt to use the same old
energy over and over again, you would be using up more energy than if you made
up your mind to use each bit of energy just once.
You can’t get
around it. What the laws of
thermodynamics really say is that in the great game of the universe, you can’t win! You can’t get something for nothing, or even
for nearly nothing.
(Through
the centuries inventors have been trying to beat this game and invent
perpetual-motion machines. With rolling
balls and swinging weights and spinning wheels they have tried repeatedly to
make a machine that would run on, once strated, getting just a little energy
from gravity or some other source to overcome the little bit of friction in its
bearings. Such a machine, if you could
make it, would be a perpetual-motion machine of the kind that would violate the
laws of thermodynamics. Nobody has
succeeded; nobody ever will; very few, if any, are still trying.)
All work and no waste are impossible
This impossibility is a hard
thing to accept, and the indomitable human spirit is bound to fall back to the
next line of defense. If it is true that
you can’t win, then perhaps you can at least break even. In other words, given a certain supply of energy,
perhaps you can at least turn it all
into work.
Smithsonian, v. 1, no. 5, (August,
1970), p. 4-11.
This
problem came up when the steam engine was first developed in the 18th
Century. To begin with, the early
engines were extremely
inefficient. Great quantities of fuel
were burned, but most of the energy was wasted in heating up the world
generally; very little ended in such useful work as pumping water.
Naturally,
one assumes that if one could only cut down on friction, prevent the flow of
heat in unwanted directions, make the general design more efficient, one could
eventually build a machine that would turn all
the energy into work.
The first person
to point out that this was not so, that even a perfect steam engine could not turn all energy to work, was a
French physicist, Sadi Carnot.
He
demonstrated in 1824 that the steam engine did work because part of its system
was quite hot (the part that consisted of steam) and part was quite cold (the
part that consisted of the cold water that condensed the steam). The heat energy present was, in other words,
in greater-than-average concentration in one place and less-than-average
concentration in another. The engine
worked by taking some heat from the hot part, transforming some of it into
work, and dumping some of the heat into the cold part. Unfortunaetely you always had to dump some
heat into the cold part; you couldn’t transform all the heat you extracted into
useful work. The fraction of energy that
could be turned into work by a steam engine depended upon the difference in
heat concentration (that is, “temperature”) between the hot part of the system
and the cold part.
The greater the
difference in temperature between two parts of the same system, the greater the
fraction of the heat energy we can turn into work. This difference in temperature becomes a
maximum when all the heat in the
system is concentrated in one part and none
is concentrated in another.
The trouble is
that physicists have shown it is impossible to concentrate all the heat in a system in one particular part of it. Even to approach total concentration takes an
enormous effort.
If a steam engine uses ordinary steam for
its hot part and ice water for its cold, the difference in temperature is such
that only 27 percent of the total heat energy could be converted into work,
even if the steam engine were perfect in every other respect, if it lost no
heat to the outside, if there were no friction, and so on.
Like water, energy flows downhill
This is true of any system that uses energy of any
kind. To make any system useful, to
allow it to turn energy into work, there must always be a difference in energy
concentration in different parts of the system.
There must be a high-energy concentration here and a low-energy
concentration there, and the work to be got out of the system depends not on
the toatl energy, but on the difference in energy concentration within the
system.
We can say: “No
device can deliver work unless there is a difference in energy concentration
within the system, no matter how much total energy is used.”
That is
one way of stating what is called the Second Law of Thermodynamics. It is one of many ways; all of them are
equivalent although some very sophisticated mathematics and physics is involved
in showing the equivalence.
Since
there is never any way of reaching an ultimate difference in energy
concentration, never any way of putting all
the energy into one part of the system and none
into another, we can never turn every bit of the energy of a system into
work. Some of the energy always manages
to get away from us without being turned into work.
What the Second
Law tells us, then, is that in the great game of the universe, we not only
cannot win; we cannot even break even!
Given energy at
two different levels of concentration, we will note as part of the common
experience of mankind that there is always a spontaneous transfer of energy
from the place of higher concentration to
the place of lower concentration and never vice versa. For instance, heat will flow, of itself, from
a hot
Smithsonian, v. 1, no. 5, (August,
1970), p. 4-11.
body into a cold body, but not vice versa. Water will flow sponatneously downhill, but
not vice versa. Physicists can show
that this principle explains why devices will convert energy into work when
there is a difference in energy concentration within the system. Spontaneous energy flow from high to low
produces the work.
The statement
about spontaneous energy flow is therefore another way of expressing the Second
Law. It is equivalent to our earlier expression
(the impossibility of converting all of any amount of energy into work) in the
following sense: The energy that cannot be converted must be dumped into a cold
place, and hence we have a flow of this energy from hot to cold.
But work is
never done instantaneously. It
invariably occupies time. What happens
during that time? Suppose we
consider a steam engine with a portion of itself that is at high-heat
concentration and another portion that is at low-heat concentration. By the Second Law, the heat flows from high
to low and in the process some of the heat is turned into work. If the heat flow happened all at once and was
converted into work in zero time, then we would at least get all the work out
of the energy flow that we could. But it
takes time, and as time passes, some of the heat in the high-concentration
portion is pouring out into other parts of the universe. Meanwhile, heat from other parts of the
universe is pouring into the low-concentration portion. In other words, the hot part of the steam
engine is cooling faster than you would expect just from its transfer of heat
to the cold portion. The cold portion,
on the other hand, is warming faster than you would think just from its receipt
of heat from the hot portion. The difference in temperature is dropping
faster than you would expect from the work done.
A German
physicist, Rudolf Clausius, pointed out this fact in 1865. He invented a quantity consisting of the
change in heat divided by the temperature, and called it “entropy.” He showed that entropy was a measure of the
quantity of energy not capable of conversion into work.
Energy available is always getting less
In any physical change that takes place by itself the
entropy always increases. In the case of
the steam engine it is because there is heat flow to and from the
universe. If a boulder rolls down the
mountainside, there is increase of entropy because of friction and air
resistance. An electric current flowing
from one pole of a battery to another encounters resistance from whatever it
passes through and hence experiences increase in entropy.
To be sure, we
can imagine ideal cases. A rock might
fall through a perfect vacuum; an electric current might flow through a perfect
conductor. In these cases, there is no
entropy increase.
But
approximations to such ideals—a planet moving through outer space, an electric
current moving through a superconducting metal—are highly special. If we consider the ordinary systems we work
with, we can say: “In any energy transfer, there is an increase in entropy.”
This, too, is a
way of expressing the Second Law. In
fact, a good brief way of stating the First and Second Laws of Thermodynamics
is: “The total energy content of the universe is constant, and the total
entropy is continually increasing.” This
means that although the universe never loses any energy, less and less of that
energy can be converted into work as time goes on.
The Second Law
can be interpreted in terms of atomic theory, and the Scottish mathematician
James Clerk Maxwell did so in the 1860s.
Heat can be
viewed, for instance, as being represented by the random movements of the
separate particles (either atoms or molecules) making up some body of
matter. The greater the average velocity of particle motion, the
higher the temperature.
When two
particles collide, they bounce apart and some momentum (mass multiplied by
velocity) is transferred from one to the other.
The transfer can take place in any fashion, but the most likely result
is that the particle with greater momentum will lose some, and the particle
with less momentum will gain. In short,
if all the particles are the same size, the faster particle will slow down
after collision and the slower particle speed up. It is possible, of course, that a fast
particle may just happen to bounce off faster,
and the slow one slower, but it is unlikely.
Let us suppose
there is a one-in-ten chance that a fast particle will bounce off a slow
particle and become faster in the process.
The chance of six fast particles all
bouncing off faster from six slow particles will be one in ten times ten times
ten times ten times ten, or one in a million.
The chance of 96 fast particles all bouncing off faster at the same time
from 96 slow particles would be only one in a
trillion-trillion-trillion-trillion-trillion-trillion-trillion-trillion.
Suppose you took
a kettle of water containing uncounted trillions of particles and put it over a
fire. It might be that more than half of
the hot, very-fast moving particles in the hot gasses of the fire might strike
the kettle and bounce off moving still faster.
In that case, the water in the kettle would get cooler while the fire
got hotter. The Second Law would be
violated. From a philosophical viewpoint
one can argue that this process is possible and that the Second Law is no law
at all—just a tendency that is more likely to be followed than violated. But the chance of its happening is so small
that there is no way of writing it in ordinary figures. If you tried to write: one chance in
such-and-such a number, the surface of the earth wouldn’t be large enough to
hold all the zeros you would have to write.
That is why the
entropy of the universe constantly increases—because the collisions of atoms
and molecules tend always to chop off energy extremes. Wherever energy is more concentrated than
usual, that concentration drops; where it is less concentrated than usual, that
concentration rises.
It is also
possible to think of entropy in terms of order and disorder. Something is orderly when its individual
parts are arranged according to some simple rule we can quickly grasp. We can then predict from each part something
about the next part. The simpler the
rule, the easier the prediction, and the greater the order. This statement originally applied to the
order and disorder in physical systems, and it can be related to their heat and
energy content. But with a little
extension we can apply it to a lot of common everyday situations.
Disorder is so easy; order is so hard
Consider a deck of cards.
You might have it arranged as follows: ace of spades, two of spades,
three of spades and so on, followed by hearts, clubs and diamonds, each suit
arranged from ace to king. That is very
orderly; for if you show me any card (the seven of clubs, for instance), I will
instantly tell you the next card (the eight of clubs). Even if you put the four suits together
differently, or arrange each suit in a sequence that runs from king down to
ace, they still represent order.
We might also
arrange the cards so that they are alternately red and black, but without any
consideration for numbers or suits. If I
am shown the seven of clubs, I can predict that the next card will be a red card,
but that is all.
Red-and-black-in-alternation still represents some order, then, but not
much. It should be obvious, though,
that if you consider all the possible arrangements of the 52 cards in a deck,
the number of arrangements that allow you to make predictions about a card from
the preceeding one is a small, a very
small, portion of the whole.
Suppose you
shuffle a deck in such a way that it can fall into any arrangement. The chances that the arrangement will be one of
the few that will allow even a small amount of prediction, and will therefore
have at least a small amount of order, are not great.
That is why,
when you shuffle cards thoroughly, you would be most astonished to find, when
you are through, that the cards have ended up with each suit in a perfect
sequence—ace of spades, two of spades, and so on—or even red-black, red-black
all the way to the end. Let us take
another example. When a platoon of
soldiers marches past four abreast and in perfect step, that represents a high
degree of order. When we see one rank of
four soldiers move by, we can predict exactly what the next rank will pass by,
how many will be in it, whether they will be moving their right feet or left at
the moment of passing, and so on. Other
examples of order would have soldiers moving two abreast or in single file or
one rank marching and the next skipping, in alternation.
But suppose you
considered all the different possible ways in which the individual soldiers of
a
platoon could pass by if each consulted his own tastes only
and paid no attention to the others.
Some might be strolling, some
walking, some running, some hopping perhaps, some in this direction, some in
that. The number of ways of passing without any perceptible order is much
higher than the number of ways with
order.
Consequently, if
you told the soldiers of a platoon to move from one point to another at will,
you would be utterly surprised if, when each did exactly as he pleased, they
just all happened to move four abreast and in step. In fact, if they were already moving four
abreast and in step and were suddenly told to do as they pleased, you would
expect the entire platoon to break formation and become disorderly. In short, in every possible situation you can
think of, the number of ways of being disorderly is much, much greater than the
number of ways of being orderly.
This is exactly
comparable to the fact that the number of ways in which extremes get choopped
off in the random collisions of particles is much, much greater than the number
of ways in which extremes get more extreme.
Another way of
stating the Second Law, then, is: “The universe is constantly getting more
disorerly.”
Viewed that way,
we can see the Second Law all around us.
We have to work hard to straighten a room, but left to itself, it
becomes a mess again very quickly and very easily. Even if we never enter it, it becomes dusty
and musty. How difficult to maintain
houses, and machinery, and our own bodies in perfect workding order; how easy
to let them deteriorate. In fact, all we
have to do is nothering, and everything dteriorates, collapses, breaks down,
wears out, all by itself—and that is what the Second Law is all about.
Maybe life is the great exception
You can argue, of course, that the phenomenon of life may
be an exception. Life on earth has
steadily grown more complex, more versatile, more elaborate, more orderly, over
the billions of years of the planet’s existance. From no life at all, living molecules were
developed, then living cells, then living conglomerates of cells, worms,
vertebrates, mammals, finally Man. And
in Man is a three-pound brain which, as far as we know, is the most complex and
orderly arrangement of matter in the universe.
How could the human brain develop out of the primeval slime? How could that vast increase in order (and
therefore that vast decrease in entropy) have taken place?
The answer is it
could not have taken place without a tremendous source of energy constantly
bathing the earth, for it is on that energy that life subsists. Remove the sun, and the human brain would not
have developed—or the primeval slime, either.
And in the billions of years that it took for the human brain to
develop, the increase in entropy that took place in the sun was far greater;
far, far greater than the decrease
that is represented by the evolution required to develop the human brain.
But where did
it all start? If the universe is running
down into utter disorder, what made it orderly to begin with? Where did the order come from that it is
steadily losing? What set up the
extremes that are steadily being chipped away?
Scientists are
still arguing the point. Some think the
universe originally had its matter and energy all smashed together into one
huge “comic egg”—a situation something like a tremendous deck of cards all
arranged in order. The cosmic egg
exploded, and ever since, for billions of years, the universe has been running
down; the deck of cards is being shuffled and shuffled and shuffled.
Others think
that there is some process in the universe that spontaneously decreases
entropy, some naural process that unshuffles and reorders the cards. We don’t know what it can be, perhaps because
it takes place under conditions we cannot observe and cannot duplicate in the
laboratory—say in the center of exploding galaxies. Perhaps, in that case, as some parts of the
universe run down, others build up.
Then again, it may be that once the universe runs down, the random
collisions of particles may—after some unimaginable span of years—just happen
to bring about an at-least-partial unshuffling.
After all, if you shuffle and
reshuffle cards ceaselessly for a trillion years, you may violate the Second
Law and end up with an arrangement
possessing at least some order, just
by the laws of chance.
Once that
happens, the universe begins to run down again at once. Perhaps, then, we live in a universe that was
partially restored to order after a quadrillion years of having been run
down. We are now running down
again. After the unvierse is compeltely
run down, another quadrillion years or so may see a section of it ushuffled
once more.
Stars and
galaxies will then form again, and life may be established here and there, and
finally some science writer will sit down and begin to wonder again where it
all came from and where it all will end.

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