All language subtitles for Wonders of the Universe BBC 2011 EP02 Stardust BluRay 1080p x264 AC3 EN_Subtitles01.ENG

PROFESSOR BRIAN COX: Why are we here?
Where do we come from?

These are the most enduring
of güestions.

And it's an essential part of human
nature to want to find the answers.

Now, we can trace our ancestry back
hundreds of thousands of years

to the dawn of humarıkiınd.

But in reality, our story extends
far further back in time.

Our story starts with
the beginning of the universe.

It began 13.7 billion years ago.

And today, it's filled with over
a hundred billion galaxies,

each containing
hundreds of billions of stars.

In this series,
I want to tell that story.

Because ultimately,
we are part of the universe.

So its story İis our story.

This film is about
the stuff that makes us

and where it all came from.

Because understanding our own origins

means uünderstanding
the lives of stars...

...and how their catastrophic deaths
bring new life to the universe.

Because every mountain,
every rock on this planet,

every living thing,
every piece of you and me

was forged in the furnaces of space.

(BIRDS CHIRPING)

(CHİLDREN LAUGHING)

This is Pashupatinath in
the Nepalese capital city of Kathmandu.

And Hindus come here from
all öover India and Nepal

to worship the god Shiva.

In fact, that is Shiva's temple.

Now, Shiva is the god of destruction.

In the Hindu faith,
everything has to be destroyed

so that new things can be created.

And that's why pilgrims come here
to the barıks of the Bagmati River

at the foot of Shiva's temple.

The belief in this cycle of
creation and destruction

lends Pashupatinath
an added significance.

Many of these pilgrims will have come
here at the end of their lives,

to die here and be cremated.

Hindus believe in reincarnation, an
eternal seguence of death and rebirth.

Cremation helps free the soul,
so it's ready for the next life.

They also believe that
the physical elements of the body

are released back to the world

so they can be recycled
in the next stage of creation.

It's an ancient belief
that touches on a deeper truth

about how the universe works.

Every civilization, every religion
across the world has a creation story.

It tells of where we came from,
of how we came to be here

and of what will happen when we die.

Well, I have a different
creation story to tell,

and it's based entirely on
physics and cosmology.

Now, it can tell us what we're made of
and where we came from.

In fact, it can tell us
what everything in the world

is made of and where it came from.

It also answers
that most basic of human needs,

to feel part of something much bigger.

Because to tell this story,

you have to understand
the history of the universe.

And it teaches us that
the path to enlightenment

is not an understanding
of our own lives and deaths,

but the lives and deaths of the stars.

My creation story is the story
of how we were made by the universe.

It explains how every atom in our bodies
was formed not on Farth,

but was created in the depths of space,

through the epic life cycle
of the stars.

And to understand that story,

we will journey to the stars
in all their stages of life.

This is where stars are born, a nebula,

a stellar nursery,
where new stars burst into life.

Those stars will burn
for billions of years,

until their voracious hunger for fuel
forces them to blow up,

to become giants

hundreds of times the size of our sun.

And when they die, stars go out with
the biggest bang in the universe.

But to understand
how we came from the stars,

we must begin our journey
much closer to home.

Well, this is sunrise over Nepal

and those are the tallest mountains
in the world, the Himalayas.

I mean, every one of those peaks
is over six and a half thousand metres.

What a spectacular sight.

But it's incredible to think that just
a few tens of millions of years ago,

those mountains were
something very different.

The Himalayas haven't always
been mountains.

We can find clues to their true origin
by looking at them more closely.

This is Himalayan limestone,

the rock out of which much of
this magnificent mountain range is made.

Now, if you look closely, you can see
a kimd of chalky, granular structure.

Because limestone is made primarily
out of the bodies,

the shells of dead sea creatures,
of coral and polyps.

And when they die, they are put under
immense pressures and sguashed

and eventually form limestone.

So the Himalayas
were once living creatures.

Much of the rock in the Himalayas
was formed at the bottom of an ocean.

And then over millions of years, it was
ralsed up to become these vast peaks.

We've even found fossils
at the top of Mount Everest.

It's a beautiful example of the endless
recycling of the Farth's resources

that has been göorng on
since the dawn of time.

And we are part of that system.

Every atom in my body was
once part of something else.

So an ancient tree
or a dinosaur or a rock,

in fact, definitely a rock.

And the reason that the rocks
of the Earth can become living things

and then living things
will return to the rocks of the Earth

is because everything is made
of the same basic ingredients.

Those ingredients are
the chemical elemenits,

the building blocks
of everything on Earth.

Elements like hydrogen, helium, lithium,
beryllium, boron, carbon, nitrogen,

öxygen, fluorine, neon,
sodium, magnesium,

aluminium, silicon, phosphorus...

Everything in the world is made up of
the same basic set of chemical elements,

just assembled in different ways.

So these mountains, the Himalayas,
are made of limestone.

And that's calcium carbonate.

Now, calcium, carbon and oxygen

are three of the elements
that are vital for life.

The calcium in my teeth and bones,
oöxygen in the air that I breathe

and carbon in
every organic molecule in my body.

Now, you're probably pretty familiar

with those elements
in their combined forms,

but you very rarely
see the elements on their own.

There's a good reason
why many of the elements

are not found in
their raw forms in nature.

They are extremely reactive.

This is sodium.

As you can see, it's a silvery metal.
It's also guite reactive.

In fact, it's so reactive
that when you drop it into water,

you get a violent,
almost explosive, reaction.

Which is all the more surprising

when you think that
when combined with chlorine,

this forms sodium chloride,

salt, which is vital for life.

Excellent.

(LAUGHING)

And that's why I love chemistry
almost as much as physics.

It's this reactivity
that enables the elements

to combine with öone another
to make new substances.

MAN 1: İt's goöne.
MAN 2: Where the hell's it gone?

(COX LAUGHING)

That, in turn, has allowed the Farth
to develop its endless variety.

And that vartety includes us.

So to explain where we come from,

we must also explain
where the elemenis come from.

We now know that the Earth
is made of 92 chemical elements.

And that's pretty amazing, if you think
of the complexity that we see around us.

We also know that
everything beyond Earth,

everything we can see in the universe,
is made of those same 92 elemenits.

And notice that I didn't say
we think that's what they're made of.

I said we know
that's what they're made of,

because we carı prove it.

The chemistry set we have on Farth
extends far beyond the planet.

We have set foot on the moon

and know that it's rich in
helium, silver and water.

We've sent robot landers
to our neighbouring planets

and discovered that Mars
is rich in iron,

which has combined with öoxygen
to form its familiar rusty red colour.

And we know that Venus'
thick atmosphere is full of sulphur.

We've sent spacecraft
to the edge of the solar system

to discover that Neptune is rich
in organic molecules like methane.

But what of the rest of the universe?

It seems impossible that we could
discover what the stars are made of

because they're so far away.

Even the nearest star, Proxima Centauri,

is ten thousand times
more distant than Neptune,

4.2 light years from Farth.

And the nearest galaxy, Andromeda,
is another 2.5 million light years away.

Yet despite these vast distances,

these alien worlds are
constantliy sending us signals,

telling us exactly
what they are made of.

Our only contact with the distant stars

is their light that's journeyed
across the universe to reach us.

And encoded in that light

is the key to understanding
what the universe is made of.

And it's all down to a particular
property of the chemical elements.

You see, when you heat the elements,
when you burn them,

then they give off light.

And each element gives off
its own unigue set of colours.

So this is strontium and it burns
with a beautiful red colour.

Sodium is yellow.

Potassium is lilac.

And copper is blue.

Fach element has
its own characteristic colour.

It's this property that telis us
what the stars are made of.

But it's a little more complicated

than simply looking at the colour
of the light that each star emits.

You can see why by looking at the light
From our nearest star, the sun.

This is a spectrum of
the light taken from our sun.

And at first glance
it looks very familiar,

it looks like a stretched-out rainbow,

because that's exactly
what a rainbow is,

it's the spectrum of the light
from the sun in the sky.

But if you look a bit more closely,

then you see that
this spectrum is covered in black lines.

These are called absorption lines.

Fach element within our sun

not only emits light
of a certain colour,

it also absorbs light
of the same colour.

By looking for these black lines
in the sun's light,

we can simply read off a list of its
constituent elements, like a barcode.

For example, these two black lines

in the yellow bit of the spectrum
are sodium.

You can see iron.
Right down here, you can see hydrogen.

So by looking at these lines
in precise detail,

you can work out exactly
what elements are present in the sun.

And it turns out that
that's about 7096 hydrogen,

289 helium and 294 the rest.

And you can do this
not only for the sun,

but for any of the stars
you can see in the sky,

and you can measure exactly
what they're made of.

So that star there is Polaris,
the pole star. And you can see that

because all the other stars in the
night sky appear to rotate around it.

Now, it's 430 light years away.

But we know just by looking at the light

that it has about the same
heavy element abundance as our sun,

but it's got markedly less carbon
and a lot more nitrogen.

And the same applies for other stars.

Vega, the second brightest star
in the northern sky,

has only about a third of
the metal content of our sun,

whereas other stars are metal-heavy.

Sirius, the dog star, contains
three times as much iron as the sun.

And Proxima Centauri
is rich in magnesium.

But although the guantities of
the elements may vary,

wherever we look across space,

we only ever find the same
92 elements that we find on Farth.

We are made of the same stuff
as the stars and the galaxies.

But where did all this matter come from?

And how did it become
the complex universe we see today?

In order to understand
where we came from,

we have to understand events
that happened

in the first few seconds
of the life of the universe.

You see, when the universe began,
it was unimaginably hot and dense.

We literally don't have
the scientific language to describe it.

But it was,
in a very real sense, beautiful.

There was no structure,
there was certainly no matter.

It was exactly the same,
whichever way you look at it.

We can get some idea
of how the universe developed

from this state of pure symmetry

by looking at the behaviour of water
in this remarkable landscape.

These are the El Tatio geysers,
high in the Chilean Andes.

As the boiling water
bubbles up through the ground

to meet the freezing mountain air,

water can be found in
all three of its natural phases,

vapour, liguid and ice.

In its hottest state,
water is, like the early universe,

an undifferentiated cloud.

But as it cools,
it suddenly behaves very differentiy.

You see, if you look at
a cloud of steam,

it looks the same from every direction,

but as it cools down, as it lands on
this plate of freezing cold glass,

then it immediately crystallises out,
it turns into solid water, ice.

As the ice crystals form,

the symmetry of the water vapour
disappears from view

and complex,
beautiful structure emerges.

In the same way, we think that
the universe, as it cooled,

went through a series of these events
where structure emerged.

One of the most important

was about a billionth of a second
after the Big Bang.

In that moment, an important part of
the symmetry of the universe was broken.

Known as electroweak symmetry breaking,

this was the moment when
subatomic particles acguired mass,

substance for the first time.

Amongst them were the guarks.

As the universe continued to cool,

those guarks joined together
to form larger, more complex structures

called protons and neutrons.

Way before the universe
was a minute old,

the guarks had been locked away
inside the protons and the neutrons.

They are the building blocks
of all atomic nuclei,

the building blocks of the elements.

These same protons and neutrons
are with us to this day.

They form the hearts,
the nuclei, of all atoms.

Just a few seconds after
the beginning of the universe,

the fundamental building blocks
of everything had been created.

Well, it sounds ridiculous.

The fact that everything you need
to make up me

and everything on planet Earth

and, in fact, every star and
every galaxy in the sky

was there after the first minutes
in the life of the universe.

It's almost unbelievable,

but we have extremely strong
experimental evidence

to suggest that that is
the way that it is.

Well, from that point on,
it was just, in a sense,

a process of assembling those bits
into more and more complex things.

That is an incredibly
fascinating story in itself.

To teli that story,

we must look deep inside the atom,
to the nucleus at its centre.

Here we can see how
protons and neutrons are assembled

to build up the 92 different elements.

Now, the wonderful thing about the
construction of the chemical elements

is that it's so simple.

I suppose you could
call it child's play.

So imagine these bubbles are
my universal chemistry set.

And the single bubbles
would just be single protons.

That's the nucleus
of the simplest chemical element.

The element with a single proton
in its nucleus is hydrogen.

And from hydrogen,
you can make all the other elements.

The first stage
is to stick two protons together.

(LAUGHS) Look at that!
That was two bubbles stuck together.

Now, what happens when you stick
two protons together is

one of the protons turns into a neutron.

And that is called deuterium.

Devterium is still a form of hydrogen,

because it has only one proton
in its nucleus

and it is the number of protons
that defines the element.

It's öonly when
two deuterium nuclei are combined

that a new element is created.

Take two deuteriums
and fuse them together

and you get a nucleus with
two protons and two neutrons.

That's helium,
the second simplest element.

And then it's just a guestion of adding
more and more protons and neutrons.

Well, there's an incredibly
complicated nucleus.

That's about 12 things stuck together.

So that would be probably carbon-12,
which is six protons and six neutrons.

And you can carry on building
more and more complex elements

all the way up to
the heaviest element in the universe,

to uranium and beyond.

Simple and beautiful physics.

This process of building the elements
is called nuclear fusion.

It allows the simplest of ingredients

to create the infinite variety
of the universe.

But although this bubble metaphor makes
creating new elements seem simple,

it is in reality incredibiy
difficult to achieve...

so difficult that there's only place
in nature that it happens.

İt's in stars like our sun
that the elements are assembled.

They are the öonly places in the universe
hot enough and dense enough

to fuse atoms together.

Even then, only a fraction of the star

reaches the extreme
temperatures necessary.

The sun is 6000 degrees Celsius
at its surface,

not nearly hot enough to power fusion.

But deep below, where the temperature
reaches 15 million degrees,

the sun fuses hydrogen into helium
at a furfous rate.

Every second it burns
600 million tonnes of hydrogen.

As it does so, it releases
the huge amounts of heat and light

that brings our planet to life.

It is this process of
converting öone element into another

that allows us to exist.

But for all its power,
the sun only converts

hydrogen, the simplest element,
into helium, the next simplest.

But there are over 90 other elements
present in our universe.

So where did they all come from?

Hf the heavier elements are not
being made in stars like the sun,

then there must be somewhere else in
the universe where they are assembled.

It's important to know,

because it's the elements beyond helium
that give our world its complexity.

And when it comes to planet Farth
and human beings,

there's öone element
that is particularly important.

Carbon.

Life is completely dependent on carbon.

I mean, I'm made of about a billion
billion billon carbon atoms,

as is every human being out there,
every living thing on the planet.

Imagine how many carbon atoms that is.

So where does
all that carbon come from?

Well, it comes from the only place in
the universe where elements are made.

Stars.

But in order for us tolive,
a star must die.

Stars in the prime of their lives,
like our sun,

are önly hot enough to make helium.

Forming the heavier elements
reguires much higher temperatures,

temperatures that can only be reached
at the end of a star's life.

Looking out into space,

you miğht think that the cosmos
is a constant, unchanging place,

the stars will always be there.

But in fact, the stars are only
a temporary feature in the sky.

And though they may burn brightiy
for many millions or billiorns of years,

they can only live for as long as
they have a supply of hydrogen to burn.

When a star runs out of hydrogen,
it begins to die.

But it doesn't go guretiy.

Rather than cooling,
the star becomes much hotter,

until there's a sudden flash.

Then the star starts to expand.

Over tens of thousands of years,

it balloons to many hundreds of times
its previous size.

But in this bloated state,

the star is unable to
mailntain its surface temperature.

As it cools, it takes on the
characteristic colour of a dying star.

It has become a red giant.

These are pictures of
a red giant star in our galaxy,

a star called Betelgeuse.

Now, it's öone of our nearest neighbours
in cosmic terms,

it's only about 600 light years away.

But it's the size that's astonishing.

If you were to put the sun there,
then Venus would be about there,

and the Earth about there,
and Mars here.

And in fact, you could fit
everything in the solar system

all the way out to Jupiter
inside the star.

Now, because it's so big,
even though it is 600 light years away,

you can see detail on its surface.

So these, these are sunspots on
the surface of Betelgeuse.

But it's not what's going on on
the surface that's really interesting.

To understand where carbon
comes from in the universe,

we have to understand what's going on
deep in the heart of the star.

Imagine this old prison in Rio
is a dying star like Betelgeuse.

Out there is the bright surface,
shining off into space.

As I descend deeper and deeper
into the prison,

the conditions will become hotter
and hotter and denser and denser,

until down there, in the heart
of the star, is the core,

and it's in there that all
the ingredients of life are made.

Deep in its core,

the star is fighting a futile battle
agalrnst its own gravity.

As it desperately tries to stop itself
collapsing under its own weight

new elements are made
in a seguence of separate stages.

Stage one is while there is still
a supply of hydrogen to burn.

Whilst the star is burning hydrogen
to helium in the core,

vast amounts of energy are released,
arıd that energy escapes,

literally creating an outward pressure
which balances the force of gravity

and, well, it holds the star up
and keeps it stable.

But eventually the hydrogen in the core
will run out

and at that point,
the fusion reactions will stop,

no more energy will be released,

and that outward pressure
will disappear.

Now, at that point, the core will start
to collapse very rapidly,

leaving a shell

of hydrogen and helium behind.

Beneath this shell
as the core collapses,

the temperature rises again,

until, at a hundred million degrees,
stage two starts

and helium nuclei
begğin to fuse together.

Now, helium fusion does two things.

Firstly, more energy is released,
and so the collapse is halted.

But secondly, two more elements
are produced in that process.

Carbon,

oxygen. Two elements vital for life.

So this is where all the carbon
in the universe comes from.

Every atom of carbon in my hand,

every atom of carbon in
every living thing on the planet

was produced in
the heart of a dying star.

Now, compared to the lifetime of a star,

the creation process of carbon and
oxygen is over in the blink of an eye,

because in only about a million years,

the supply of helium
in the core is used up,

and for stars as massive as the sun,
that's where fusion stops,

because there isn't
enough gravitational energy

to compress the core any further
and restart fusion.

But for massive stars like Betelgeuse,
the fusion process can continue.

When the helium runs out

gravity takes over again
and the collapse continues.

The temperature rises önce more,
launching stage three,

in which carbon fuses into magnesium,
neon, sodium and aluminium.

And so it goes on, core collapse,

followed by the next stage of fuston
to create more elemenis,

each stage hotter and shorter
than the last.

And eventually, in a final stage
that lasts only a couple of days,

the heart of the star is transformed
into almost pure iron,

whose chemical symbol is Fe.

This is where the fusion process stops.

In its millions of years of life,

the star has made
all the common elements,

the stuff that makes up
9926 of the Farth.

The core is now a solid ball
of those elemenits,

stacked on top of each other in layers.

On the outside,
there's a shell of hydrogen,

beneath it a layer of helium,

then carbon and öoxygen
and all the other elements,

all the way down to
the very heart of the star.

And once that has fused into solid iron,

the star has only seconds left to live.

When a star runs out of fuel,

then it can no longer release energy
through fusion reactions,

and then there's only one thing
that can happen.

In about the same amount of time
it takes this prison block to crumble,

the entire star falls in on itself.

This is the destiny that awaits
most of the stars in the universe.

Yet even the implosion of a star
only forges the first 26 elemenis.

What of the remaining elements,
some of which are vital for life,

and many of which we hold most precious?

(BIRDS CHIRPING)

These are the remote forests
of northern California.

A hundred years ago,
this whole area was teeming with people,

all in search of öone element.

And the reason they were here
can still be found

in the Original Sixteen to One mine.

This once stood at the centre
of the Califormia gold rush.

And tharıks to a gülrk of geology,

it continues to yield its precious
bounty over a hundred years later.

The unigue thing about this place
is that it sits right on the divide

between the North American plate
anıd the Pacific plate.

You see a divide there,
between the rock and guartz.

And then right up there
you can see the top ofit.

Now, in between the faults,
this rock, the guartz, formed.

Then 140 million years ago,
in the Jurassic period,

when the dinosaurs were
running around above our heads,

hot water welled up and flowed.

And that water deposited the gold
through the seams of guartz.

And so, all the miners have to do,

all they have to do
is follow the seams of guartz,

and over hundreds of years they've found
vast amounts of gold deposited there.

Well, this is what
all the fuss is about.

This is the gold
as it comes out of the ground.

And it's unusually pure, as gold goes.
This is about 8596 pure gold.

But it can also be foundlike this.

And this is a gold nugget that was
found in a river, on a riverbed.

And it's a heavy piece of gold,

it's between about one
and one and a half ounces,

which means that at today's prices,
it's worth about $2,000.

And it's that inherent value that makes
mines like this worth operating.

(PIANO PLAYING)

But there's something a bit odd
about the value we attach to gold.

Throughout history, people have
göne to extraordinary lengths

to get their hands on
this most precious substance.

Which is strange, because it isn't
particularly useful for anything.

Most of the gold that's been
extracted throughout human history

has ended up as jewellery.

But it has got one thing going for it,
and that's that it is incredibly rare.

All the göld mined from the Farth
in all of human history

would only just fill
three Olympic-sized swimming pools.

And it's that scarcity
that makes gold valuable.

But gold is just one of
many rare elemenits.

There over 60 elements
heavier than iron in the universe.

Some are valuable like gold,
silver, platinum.

Some are vital for life,
like copper and zinc.

And some are just useful.
Like uranium, tin and lead.

But across the universe,

there are vanishingly small amounts
of those heavy elements.

The reason for that scarcity

is that creating substantial amounts
of the heaviest elements

reguires some of
the rarest conditions in the universe.

And we need to look far into space
to find them.

In a galaxy of a hundred billion stars,

these conditions will exist, on average,
for less than a minute in every century.

That's because they are only created

in the final death throes
of the very largest stars,

stars of at least
nine times the mass of our sun.

Only they can reach
the extreme temperatures needed

to create large amounts
of the heavy elements.

Deep in the heart of the star,
the core finally succumbs to gravity.

1t falls in on itself
with enormous speed...

and rebounds with colossal force.

As the blast wave collides with
the outer layers of the star,

it generates the highest temperatures
in the universe,

a hundred billion degrees.

These conditions last
for just 15 seconds,

but it's enough to form
the heaviest elemenits, like gold.

It's called a supernova,

the most powerful explosion
in the universe.

You know, it's guite a thought
that something as precious to us

as the gold in a wedding ring

was actually forged in
the death of a distant star

millions of light years away,
billions of years ago.

Despite the rarity of supernovae,

when they do happen, they are
the most dramatic events in the sky.

This is a picture of
the Tarantula Nebula,

which is a cloud of gas and dust

in the Large Magellanic cloud, which is
a satellite galaxy of the Milky Way.

And this is what it looks like
on any clear, starry night of the year.

But on one night in 1987,
the Tarantula Nebula looked like that.

You see that a new, bright star
has appeared in the sky.

This is a supernova explosion,
the explosive death of a massive star.

And they are incredibly violent
cosmic events,

as this picture beautifully shows.

This is a galaxy about
55 million light years away from Earth,

but this is a supernova explosion
in that galaxy.

And you see that it is shining
as brightly as the galactic core.

There may be a billion suns
in that core,

and öne supernova
can shine as brightly as that.

Yet to really appreciate
the scale of these explosions,

we would need to see one up close,

to see a star die in our own galaxy,
the Milky Way.

Although on average there's öne big
supernova in each galaxy every century,

there hasn't been öne in the Milky Way
since the birth of modern science.

The last was in 1604,
so we're long overdue.

Astronomers are now searching the skies

for the star that is
most likely to go supernova.

And amongst the leading candidates,
there's a familiar name.

This is the constellation of Orion,
and this is Betelgeuse.

And we know it's extremely unstable

because it's dimmed by about 1596
in the last 10 years.

Now, astronomers think that this star
could go supernova at any moment.

That could mean
arnıy time in the next million years,

but egually it could explode tomorrow.

And Betelgeuse is only
600 light years away.

Now, when it goes,
Betelgeuse will be incredibly bright.

It will be by far
the brightest star in the sky.

It may shine as brightly as a full moon.

It will be almost a second sun
in the daylight.

In this single instant,
Betelgeuse will release more energy

than our sun will produce
in its entire lifetime.

As the star is torn apart,
it will fire out into space

all the elements
that it created in its life and death.

Those elements will spread out
to become a nebula,

a rich chemical cloud
drifting through space.

And at the heart of the nebula
will be a tiny beacon of light,

the remnant of a star, öonce more than
a billion and a half kilometres across,

that has been crushed
out of all recognition by gravity.

This is Betelgeuse, the neutron star.

And it's how this önce mighty star
Will end its life.

Now, once Betelgeuse is gone,

the constellation of Orion
will look very different.

I mean,
there'll just be a hole in the sky

where that brilliant,
bright red star once shone.

But it's in the deaths of old stars
that new stars are born.

It's very much like the cycle
of death and rebirth here on Earth,

but played out on a cosmic scale.

And you can see that happening today
in the constellation of Orion,

because in the sword handle,
you can see this, the Orion nebula.

Now, it's nothing more than

a misty patch of light in
the night sky to the naked eye.

But if you look more closely, you see
that there is a lot more going on.

The Orion nebula is öone of
the wonders of the universe.

Hidden in its clouds
are bright points of light.

These are new stars

forming from the elements
blown out by supernova explosions.

New stars being born
from the remains of dead ones.

And it's from this universal process
of death and rebirth that we emerged,

because it was in a nebula
just like this, five billion years ago,

that our sun was formed.

Around it, a network of planets formed.

Among them was the Farth.

Everything we find on the Farth today
also originated in that nebula.

But that is not the end of the story
of how the universe created us.

Because when we look
deep into the nebula,

we don't just see individual elements,

we see greater complexity,
the seeds of our own existence.

This is a spectrum of
the light from the Orion nebula

taken by the Herschel space telescope.

So it really is a picture of light
from interstellar space.

You know, I wouldn't normally show you
a graph like this,

but this is fascinating,
because what it shows

is that that gas cloud,
the Orion nebula,

is not just a cloud of elements.

There's complex chemistry here
happening in deep space.

Because each peak on this graph
corresponds to a different molecule

and there are some molecules present
that I suppose are guite obvious.

There's water, there's sulphur dioxide.

But there are also
complex carbon compounds in here.

So there's methanol,
there's hydrogen cyanide,

there's formaldehyde,
there's dimethyl ether.

So what we're seeing here
is complex carbon chemistry

happening in deep space.

That carbon chemistry is the beginning
of the chemistry of life.

And there is surprising evidence
that this chemistry

may have had a direct impact
on the evolution of life on Farth.

That evidence comes from meteorites,

debris left over from
the formation of the solar system

that occasionally collides
with the Farth.

One of the most productive places
for finding meteorites

is the Atacama Desert
in the High Andes of South America.

This is a meteorite,

a piece of rock that fell to Earth from
somewhere out there in the solar system.

And it is certainly older
than any rock you can see here.

It's probably older than any rock
you can find anywhere on Earth,

because it formed from
the primordial gas cloud,

that nebula that collapsed

to form the sun and the planets
over four and a half billion years ago.

So it's incredibly ancient.

Now, this is a slice,
a cross-section through a meteorite.

You see those little
brown areas in there?

Well, in those brown areas
we've found amino acids,

the building blocks of proteins,

which are the building blocks of me,
the building blocks of life.

Incredibly complex carbon compounds.

So this says that
the complex carbon chemistry you need

to send you on the path to life

was happening out there in space
four and a half billion years ago.

So the first amino acids on Farth,
the fundamental building blocks of life,

may have formed in the depths of space

and been delivered to the Farth
on meteorites.

When we look out into space,
we are looking into our own origins,

because we are truly
children of the stars.

And written into every atom
and every molecule of our bodies

is the entire history of the universe,
from the Big Bang to the present day.

Our story is the story of the universe.

Every piece of everyone,

of everything you love
and everything you hate,

of the thing you hold most precious,
was assembled by the forces of nature

in the first few minutes
of the life of the universe,

transformed in the hearts of stars
or created in their fiery deaths.

And when you die,

those pieces will be
returned to the universe

in the endless cycle
of death and rebirth.

What a wonderful thing it is
to be a part of that universe.

And what a story, what a majestic story.

(ACROSS THE UÜNİVERSE
BY DAVID BOWLIE PLAYING)