Original subtitles

Translated By The Community Of WWW.MY-SUBS.COM

1 Narrator: Billions and billions of galaxies --

the universe is so vast, we can't even imagine

what those numbers mean.

But 14 billion years ago, none of it existed...

until the Big Bang.

The Big Bang is the origin of space

and the origin of time itself.

Narrator: We take a journey through space and time,

from the beginning to the end of the universe itself.

♪ How the Universe Works 1x01 ♪ Big Bang Original Air Date on April 25, 2010

== sync, corrected by elderman ==

This is our world.

Cities... forests...

oceans... people --

everything in the universe is made from matter

created in the first seconds of the Big Bang...

...every star, every planet, every atom, every blade of

grass, every drop of water.

Water is ancient.

The hydrogen atoms in here were born moments after the Big Bang.

Then came everything else.

Narrator: The Big Bang is the defining event

of our universe... and everything in it.

The secrets of our past, our present, and our future are

locked inside this one moment in time.

To unlock the secrets of the Big Bang, we have to travel outside

of our own solar system...

And journey beyond even our own galaxy.

As we travel into deep space, we're actually seeing into

the past... and getting closer to being able to witness

the dawn of time itself.

Passing the first infant galaxies and the first stars...

We arrive back at the moment the universe began and face

the biggest questions in all of science.

This is the Holy Grail of physics.

We want to know why it banged.

We want to know what banged.

We want to know what was there before the bang.

Narrator: To get the answers, we've built machines the size of

cities to simulate conditions

when the universe was created...

''Why are we here?

Where did we come from?''

Does the universe in fact have a beginning or an end?

And, if so, what are they like?

If we find the answer to that, it would be the ultimate triumph

of human reason.

We would know the Mind of God.

Narrator: The origin of the Big Bang is the greatest mystery

of all time.

And the more we learn, the deeper the mystery becomes.

Dr. Kaku: We like to think that our universe is unique.

However, now we're not so sure.

Perhaps there is a multiverse of universes.

Dr. Krauss: Another possibility is that our Big Bang is just one of many

Big Bangs, but it may be one of just an infinite number

of universes.

And there may be other regions in that infinite number of

universes where a Big Bang is just happening today.

Narrator: But there's only one universe we're sure of, and

understanding this one is hard enough.

Since the late 1920s, everything we know about how our universe

works has been turned upside down.

Dr. Krauss: It's important to realize how much our picture of the universe

has changed in the last century.

At the beginning of the 20th century, the conventional

wisdom in science was that the universe was static and eternal.

Narrator: In 1929, that all changed.

At the Mount Wilson observatory above Los Angeles, astronomer

Edwin Hubble discovered galaxies aren't stuck in one place.

Not only are they moving, but they're flying away from Earth

at incredible speeds.

This was the first real evidence of the Big Bang.

All galaxies on average are moving away from us, and,

stranger still, those that were twice as far away were moving

twice as fast.

And those that were three times as far away were moving

three times as fast, and so on.

Everything was moving away from us.

Narrator: It became known as Hubble's Law.

His discovery is still the starting point for exploration

of the Big Bang.

What Hubble convincingly demonstrated, by seeing the

motion of those galaxies, is that the universe is expanding.

Narrator: Theoretically, an expanding universe must have

started from a single point.

By measuring how fast the universe is expanding,

astronomers calculated backwards and figured out when

it burst into life.

People ask the question, ''How do you know that

the universe is 13.7 billion years old?

I mean, smarty-pants, you weren't there

13.7 billion years ago.''

Well, when you watch television on videotape, you hit the stop

button when you see an explosion, and you can run it

backwards and see when it actually took place.

The same thing takes place with cosmology.

We can run the videotape backwards and then calculate

when it all came from a cosmic explosion.

Narrator: You don't have to be an astronomer

to look back in time.

If you gaze up at the night sky, you're seeing stars that are

millions of light-years away, meaning it took the light from

those stars millions of years to get here.

So if you look far enough, you should be able to see

the beginning of the universe.

Named for the groundbreaking astronomer, the Hubble Space

Telescope allows us to look deep into the universe, back in time,

and closer to the moment of the Big Bang.

But for scientists, winding back the clock to the Big Bang

was only the first step.

Dr. Kaku: When people first hear about the Big Bang theory, they say,

well, where did it take place?

lt took place over there.

lt took place over there.

Where did it take place?

Actually, it took place everywhere, because the universe

itself was extremely small at that time.

Narrator: These are only some of the most abstract and

difficult concepts there are.

So here's a mind-bender.

What came before the Big Bang?

The philosophers in ancient times used to say how could

something arise from nothing?

And what's amazing to me is that the laws of physics

allow that to happen.

And it means that our whole universe, everything we see,

everything that matters to us today, could have arisen out of

precisely nothing.

Narrator: It's one of the biggest hurdles to understanding

the Big Bang.

First you have to buy into the premise that something was

created out of nothing.

It's impossible to describe the moment of creation

in human language.

All we know is that from what may have been nothing, we go to

a state of... almost infinite density and infinite temperature

and infinite violence.

Narrator: Understanding how nothing turned into something

may be the greatest mystery of our universe.

But if you understand that, you start to understand the

Big Bang, when time and space began,

and the great big explosion created everything.

Narrator: At the dawn of time, the universe explodes into

existence from absolutely nothing into everything.

But everything is actually a single point, infinitely small,

unimaginably hot, a super-dense speck of pure energy.

The Big Bang was so immense that it brought into existence

all of the mass and all of the energy contained in all of the

400 billion galaxies we see in our universe in a region smaller

than the size of a single atom.

The entire observable universe was a millionth of a billionth

of a centimeter across at that time.

Everything was compressed into an incredibly hot, dense region.

Narrator: It's not even matter yet, just a point of

raging energy.

lt was the beginning of the universe and everything in it.

Everything was simple.

All the forces that we know about today

were one and the same.

The universe was amorphous.

lt had no structure.

Narrator: In that instant of creation, all the laws of

physics, the very forces that engineer our universe,

began to take shape.

The first force to emerge was gravity.

The fate of the universe -- its size, structure, and everything

in it -- was decided in that moment.

Carlos Frenk studies how gravity shaped the universe by creating

artificial universes in this supercomputer.

He gives each one a different amount of gravity.

The first one he tried had too little, resulting in,

well, nothing.

Dr. Frenk: Gravity has saved our universe, for if gravity was

weaker than it is, we would have a very boring universe in which

everything would be flying apart so fast that there would be

no galaxies forming.

Narrator: Next, he programmed a universe with

too much gravity.

Dr. Frenk: If gravity was stronger than we think it is, again,

we'll end up with a failed universe.

Everything will end up in black holes.

lt has to be just so.

lt has to be just right.

Narrator: Lucky for us, the Big Bang got it just right --

the perfect amount of gravity.

ln the turmoil of forces after gravity emerged, still a

fraction of a second after the Big Bang, a shock wave of energy

erupted and expanded the universe in all directions

at incredible speed.

Dr. Krauss: All of space expanded by an unbelievably large factor in

a fraction of a second.

We think that in less than a millionth of a millionth of

a millionth of a millionth of a second, space expanded by

a factor bigger than a million, million, million, million times.

Narrator: And for the record,

that's faster than the speed of light.

But, wait, doesn't that break one of the laws of physics?

Even schoolchildren know that, ''You can't go faster than

the speed of light.''

But I say there's a loophole there.

You see, nothing can go faster than light,

nothing being empty space.

Narrator: Don't worry.

This idea gives even the best minds in science a headache.

But it's critical to understanding

the early universe.

Scientists think it took less than a millionth of a millionth

of a millionth of a millionth of a second for the universe to

expand from the size of an atom to a baseball.

That may not sound like much, but it's like a golf ball

expanding to the size of the Earth

in the same amount of time.

That means it was expanding faster than the speed of light.

That's fast.

So many things were happening so fast in the early universe,

because everything was so close together,

that we needed a new unit of time to describe things.

Narrator: It's called Planck time.

To understand just how short a Planck time is, consider this.

There are more units of Planck time in one second than all the

seconds since the Big Bang.

The math is mind-blowing.

There are more than 31 million seconds in a year, and it's been

14 billion years since the Big Bang.

So multiply 31 ,556,926 by 14 billion, and what you get is

a really big number.

Dr. Krauss: It's a time scale that's so small that all human intuition

goes out the window.

If we look at our watches and measure one second,

we can ask, how many Planck times is that?

Well, it is a billion, billion, billion, billion, billion

Planck times.

Narrator: So, now the Big Bang is only a few Planck times

old, an exploding mass of pure energy expanding faster than

the speed of light.

ln the next few Planck times, the universe as we know it

will be born.

Narrator: A fraction of a second after the Big Bang,

the universe is so small it can fit in the palm of your hand.

But in another tiny fraction of a second, it expands to

the size of the Earth.

Then, moving faster than the speed of light, it grows larger

than our solar system.

And it's still just a raging storm of superheated energy.

lt would be hotter and denser and more violent than anything

that we can experience in the universe today.

Even the interior of a star is calm and serene by comparison

to the violence of the earliest moments of the Big Bang.

Temperatures were so hot that even the atoms of your body

would disintegrate -- so hot, in fact, that the atoms would be

ripped apart.

Narrator: How hot?

Trillions of degrees hot.

But as the universe continues to expand, it also begins to cool.

Dropping temperatures trigger the next stage in

the universe's evolution.

The raw energy of the explosion transforms into

tiny subatomic particles.

It's the first matter in the universe.

This conversion of energy into matter was predicted by

Albert Einstein years before anyone started talking about

the Big Bang.

It's the one scientific equation every schoolkid knows.

There is one very familiar formula.

And that is e equals mc squared.

lt says something about the creation of the universe.

lt says even if the universe is created just out of pure energy,

that because energy can be converted to matter and matter

to energy, that you can get all of the stuff that we see in the

universe from this pure energetic event.

Narrator: Einstein's little equation had a big impact.

lt led to the first nuclear bombs.

ln a nuclear explosion, a small amount of matter is converted

into an enormous amount of energy.

As the universe was forming, the exact opposite happened.

Pure energy transformed into particles of matter.

You don't need to create matter in the beginning.

You just need energy.

And energy alone can lead to the creation of an entire universe.

Narrator: In just a fraction of a second after the Big Bang,

the building blocks of our universe begin to take shape.

But this first matter is like nothing we see today.

The stuff of matter has been very different over the age

of the universe.

What we now think is normal matter was not at all normal in

the earliest moments of the Big Bang.

Narrator: That's because condition were so extreme.

There were no atoms yet.

But there were tiny subatomic particles.

ln the earliest moments of the Big Bang, the universe was

so hot and dense, there were great amounts of energy.

And so particles were being created all the time, and energy

and matter were transferring back and forth in this hot,

dense soup.

Narrator: That earliest matter was too unstable to start

forming the universe as we know it.

Think of it like this.

imagine rush hour at Grand Central in New York City

as that superheated early universe.

The commuters racing through the main concourse are

subatomic particles.

If you look at a crowd of people -- a large crowd of

people -- they may appear random.

That random, quirky motion is very similar than what was

happening in the particles in the universe in the earliest

moments of the Big Bang.

Narrator: The extreme temperature of the early

universe energizes the subatomic particles.

They appear.

They disappear.

They race around at incredible speeds.

It's pure chaos.

It's like people.

If they're excited and running around fast to catch trains at

a train station, they'll be moving around quickly.

But eventually, they calm down and get slower.

That's what's been happening to our universe, in a sense.

The particles are moving around very fast.

And as the universe cools down, the particles move more slowly

and, in some sense, less random.

Narrator: As the universe cools, the particles stop

changing back into energy.

Now there are more and more subatomic particles, but it's

still a hot, violent place.

All this is happening in fractions of a second

too small to detect.

But the Big Bang is moving into a critical stage now, a titanic

battle between matter and the one thing that can destroy the

universe before it even gets started... antimatter.

Narrator: Everything in the universe is made from matter,

from the smallest rock to the largest star.

And all the matter there will ever be was created from the

pure energy of the Big Bang.

Einstein's equation, e equals mc squared,

says that energy transforms into matter.

But it was just a theory.

Today science is able to test that theory.

This is CERN in Switzerland,

home to the world's largest machine.

It's the size of a city and engineered to re-create the

conditions millionths of a second after the Big Bang.

If we want to probe ever-smaller scales,

paradoxically we need an ever-bigger machine.

There's just no other way of doing it, so big machines mean

small physics, means early times and, therefore, getting closer

and closer to the origin of the universe itself.

Narrator: This monster machine is called a collider.

It's designed to take us back to those first fractions of

a second after the Big Bang.

It's a 12-foot-wide concrete-line circular tunnel

17 miles around.

The collider makes tiny particles of matter smash into

each other at almost the speed of light.

For a split second,

those collisions generate turbocharged energy

similar to the explosive force of the Big Bang.

And then that pure energy briefly transforms into matter,

just like it did nearly 14 billion years ago.

But a monster machine needs a monster detector

to see these collisions.

This detector is five stories tall and weighs over 7,000 tons.

And 7,000 tons -- to give you a sense of perspective -- is the

weight of the Eiffel Tower.

Narrator: But as big as it is, it can't see the actual

particles of new matter.

They hang around for just a split second and move so fast it

can only record their trails.

There's a lot of energy in these particles.

They move very, very quickly, and so you need a very large

amount of detector in order to be able to map the path of these

particles very precisely.

So, the detector is so big because you need

better resolution.

lt works exactly the same at a camera.

The more pixels you have, the better the picture.

It's exactly the same here.

We just have a five-story camera.

Narrator: Scientists hope that it'll reveal just how

energy transforms into matter...

But not just any matter -- the kind of matter that emerged

14 billion years ago at the dawn of time itself.

But the dawn of time was a critical moment in the birth of

the universe, because pure energy also produced one of the

most dangerous things in the universe -- antimatter.

That's right, antimatter -- it's real.

Dr. Kaku: Antimatter is the mirror image of ordinary matter.

However, matter has one charge,

and antimatter has the opposite charge.

If there was an anti-me made out of antimatter, that person, in

principle, could look exactly like me -- same personality

quirks, same everything, except, of course, when I decide to

shake his hand.

At that point, we both would blow ourselves to smithereens in

a gigantic nuclear explosion.

Narrator: Matter with a positive charge locks horns with

its archenemy, antimatter, with a negative charge.

The fate of the universe hangs in the balance

of this epic battle.

Equal amounts of matter and antimatter will cancel each

other out -- not good.

A universe with equal amounts of matter and antimatter is

equivalent to a universe with no matter at all, because the

matter and antimatter will annihilate back into

pure radiation.

And there'll be nothing interesting -- no stars and

galaxies and people in between.

Narrator: Like a cosmic game of Risk, the side with the most

soldiers wins.

The score was very close, but there was a winner.

Dr. Krauss: For every billion particles of antimatter, there were a

billion and one particles of matter.

That was the moment of creation.

The one extra particle of matter in each little volume survives,

survives enough to form all the matter we see in the stars and

galaxies today.

Narrator: One in a billion might not sound like much, but

it's enough to build a universe.

Dr. Kaku: We're the leftovers.

So, believe it or not, everything you see around you,

the atoms of your body, the atoms of the stars, are nothing

but leftovers -- leftovers from this ancient collision between

matter and antimatter.

Narrator: Lucky for us, there was enough left over to make all

the stars and planets.

And the universe is still less than one second old.

But now it's swarming with tiny, primitive particles.

The next stage is assembling those tiny particles into

the first atoms.

Narrator: Give or take a couple of Planck times, the

universe is nearly a second old and still a very strange place.

But matter has won the battle with antimatter.

And now it's time to build the universe.

It's still extremely hot and expanding incredibly fast.

When the universe was a second old, the particles in it

were very different than the particles we see today.

There were no atoms.

Nothing that we recognize in the room around us today

yet existed.

Narrator: Now all that begins to change.

Temperatures continue to cool.

And as the primitive particles keep slowing down, they start

bonding together to form the atoms of the first elements.

The first one to form is hydrogen.

Then over the next three minutes, the universe begins to

create two more elements -- helium and lithium.

We went from a universe that was infinitely small to a

universe that was light-years in size.

ln the first three minutes, essentially everything

interesting that was going to happen in the universe happened.

Narrator: Well, not quite.

If you were there, you couldn't see it.

Dr. Kaku: When we look at the night sky, we can see literally

billions of years into the past, and we think it's always

been that way.

Nope, not true.

380,000 years after the Big Bang -- that's when the universe

began to become transparent.

But before then, it was milky.

Narrator: There is a milky soup of loose electrons.

The young universe has to cool down enough for the electrons

to slow down and stick to new atoms.

lt took a long time for all of the hydrogen, helium, and

lithium atoms in the universe to form.

Scientists calculate it took 380,000 years for the electrons

to slow down enough so that the universe could start

mass-producing atoms.

When that happens, the milky fog clears.

The first light escapes and races across the universe.

Nearly 14 billion years later, two young scientists in

New Jersey pick it up by accident.

ln 1964, Arno Penzias and Robert Wilson were mapping

radio signals across our galaxy.

Everywhere they looked, they picked up a strange

background hum.

They first suspected their equipment.

Maybe pigeon droppings on the antenna were causing

the strange signal.

But after cleaning the antenna, the mysterious hum remained.

So much for pigeon droppings.

Penzias delivered a talk at Princeton University.

And according to lore, one person in the back said, ''Either

you have discovered the effects of bird droppings or the

creation of the universe.''

Narrator: It was in fact the moment of creation, nearly

14 billion years ago, when those first atoms got their electrons.

That's the moment when the milky cloud clears and the new

universe comes into view for the first time.

To capture better images of this critical event, NASA launched

the Cosmic Background Explorer Satellite, or COBE.

They pointed it out into space, where it took the temperature

of the universe.

By measuring differences in temperature across space,

they created the first map of our early universe.

The images were called the Face of God.

We got gorgeous pictures -- baby pictures of the infant

universe when it was 380,000 years of age.

But there were problems with it.

The picture was very fuzzy.

The COBE results were simply not good enough.

Man: Mission looking good. Liftoff.

Narrator: So NASA launched an even more advanced satellite,

WMAP, the Wilkinson Microwave Anisotropy Probe.

ln 2001 , David Spergel was part of the team looking for a

clearer image of the early universe.

lt was exciting to go to the Cape.

lt was one of these moments we were sitting there, watching

this -- I was there with my family --

watching the rocket go off.

lt was very exciting when, within about a day, we were able

to get our first signal from the satellite and know it was

working and working properly.

Narrator: This is the most detailed picture of the early

universe ever taken, just 380,000 years after

the Big Bang.

The red and yellow areas are warmer, the blue and

green regions cooler.

And those temperature differences are clues to the

future structure of the universe.

You see tiny variations in temperature.

Those tiny variations in temperature reflect small

variations in density.

This region has more matter.

This region has less matter.

Narrator: Like a blueprint for the construction of our

universe, this image shows us where there's more matter and

where there's less.

Regions with no matter will become empty space.

Areas with denser matter will become the construction sites of

galaxies, stars, and planets.

These are the fluctuations that will grow to form galaxies.

So if it wasn't for those little density fluctuations, you and I

would not be here today.

Narrator: Our universe is now 380,000 years old and trillions

and trillions of miles across.

Clouds of hydrogen and helium gas float through space.

lt will take another 200 million years before those

gases create the first stars.

These first stars ignited the universe into what must have

been the most amazing fireworks.

The universe went from the dark ages to an age of splendor when

the first stars illuminated the gas and the universe began to

glow in majestic fashion.

I wish I'd been there.

Dr. Krauss: It was like Christmas tree lights turning on.

The universe began to light up in all directions, until you

form the beautiful mosaic we now see today.

Narrator: More and more stars turn on.

1 billion years after the Big Bang, the first galaxy forms.

Over the next 8 billion years, countless more take shape.

Then about 5 billion years ago, in a quiet corner of one of

those galaxies, gravity begins to draw in dust and gas.

Gradually they clump together and give birth to a star,

our Sun.

9 billion years after the Big Bang, our tiny solar system

springs to life, and with it, planet Earth.

Everything there is exists because of the Big Bang,

and it's still going on.

Our universe is still expanding.

But it won't just keep going forever.

Our universe had a beginning, and it will also have an end.

Narrator: In the 14 billion years since the Big Bang,

galaxies have been created...

Filled with stars, planets, and moons.

And the universe has been expanding the whole time.

We've learned space is quite big -- at least 150 billion

light-years across.

Narrator: The universe may be infinite.

lt might literally go on forever.

The answer is there doesn't have to be anything,

in principle.

The universe could be infinite, and there's no outside, or it

could be closed on itself.

lt could be such that if I looked far enough in that

direction I'd see the back of my head.

Narrator: We may never know if the Big Bang produced a

universe that goes on forever.

But we do know that the Big Bang hasn't stopped yet.

The Big Bang is really continuing now.

We're continuing to bang, if you want, in the sense that the

expansion of the universe is continuing.

One of the most astounding discoveries in the last few

years has been the realization that our universe is not slowing

down, like we once thought, but it's actually speeding up.

It's accelerating.

It's in a runaway mode.

We now believe there's something called dark energy, the energy

of nothing, that is pushing the galaxies apart and is killing

the universe.

Narrator: We can't see this destructive force, and we have

no idea why it exists.

But it could mean the end of everything created in

the Big Bang.

If dark energy continues pushing the universe apart, our

Milky Way galaxy could become a lonely outpost.

100 billion years from now, most of our galactic neighbors will

be out of sight.

Stars will burn out.

Galaxies will grow dark.

Even atoms will tear apart.

The birth of the universe, the Big Bang, was over in a flash.

But the death of our universe will take almost forever.

That great philosopher of the western world, Woody Allen, once said

eternity is an awful long time, especially toward the end.

Narrator: Figuring out how our universe will end is as dark

a mystery as the Big Bang.

lt could collapse back in on itself, like a balloon when

the air is let out.

So, would the universe end with a Big Crunch, a reverse of

the Big Bang, or would it end by expanding out and becoming

cold and dark?

If you wished, would it end in fire or ice, or with a bang or

a whimper?

Narrator: If the universe collapses, it might trigger

another Big Bang.

Maybe that's already happened, and we're just one in a

long line of universes.

Personally, I believe in continual genesis -- that is,

there's a never-ending process whereby universes collide, split

apart, give birth to new universes, perhaps with

different laws of physics within each universe.

Maybe this isn't the first time it's happened.

Maybe it's cyclic, and it goes around and around again,

eventually will collapse, and the whole thing will

start over again.

Narrator: One universe or many, they all start with a Big Bang.

Dr. Krauss: Everything that makes us human -- the atoms in our

bodies, the jewelry we wear, all the things that lead to the

tragedy of life and the beauty and the excitement, love,

everything else -- arose because of processes that happened

14 billion years ago.

And if we really want to understand ourselves at some

fundamental level, we really have to understand the Big Bang.

Narrator: 14 billion years ago, the Big Bang created time

and space, our whole vast universe, and everything in it,

including us.

Dr. Kaku: Some people ask the question,

''What's in it for me?''

The Big Bang gave us everything we see around us -- the

distribution of galaxies and stars.

lt set into motion the creation of elements that we see

in the universe.

And even the laws of physics themselves, we think, were born

at the instant of creation.

Narrator: Everything started with the Big Bang, one brief

moment in time 14 billion years ago, that contains the answers

to our greatest questions about our past, our present,

and our future.

Each discovery brings us one step closer to understanding

how the universe works.

== sync, corrected by elderman ==