All language subtitles for Cosmos S01E06 Deeper, Deeper, Deeper Still (1080p x265 10bit)

We live on one level of existence,
but there are others.

These hidden dimensions of
reality are everywhere.

Far away, across the light years.

Beneath our feet.

And even inside you and me.

We are made of atoms.

There are more atoms in your eye,

than there are stars and all
the galaxies of the known universe.

The same is true of any solid object

larger than the tip of your little finger.

I'm a collection of three
billion, billion, billion

intricately arranged atoms
called Neil Degrasse Tyson.

You are a similar collection
with a different name.

We don't usually think
of ourselves this way

because that level of reality lies
beyond the realm of our senses.

But we're not gonna let that stop us.

We can go deeper into the wonder.

"Deeper, Deeper, Deeper Still"

Atoms let matter
do funny things.

To understand water, you need to
know what its atoms are doing.

Every molecule of water is composed

of two tiny hydrogen atoms

attached to a larger oxygen atom.

That's why we call it H20.

If it's not too hot or too cold,

the molecules can slide
and tumble past each other.

There's still some stickiness
between the molecules,

but not enough to lock them
into a rigid solid.

That's what makes something a liquid.

The sun warms the water.

And with more energy,

the molecules move faster.

That's all that temperature is.

Those molecules are moving fast enough

to break the weak bonds that
hold them to their neighbors.

That's evaporation.

The air we breathe is made of

nitrogen and oxygen molecules

with a scattering of water
vapor and carbon dioxide.

Incoming!

That's condensation.

A dewdrop is the momentary triumph

of condensation over evaporation.

And while it lasts,

it's a little cosmos with its own worlds...

creatures, drama.

To explore the far-flung realms

of this dewdrop,

we're gonna need a ship.

One with twin engines...

science and imagination.

That's a single-celled paramecium,

one of a multitude
of skilled hunter-warriors

that roam the dewdrop.

But they, too, are hunted.

The Dileptus. The paramecium's
mortal enemy.

The paramecium might get lucky
and score a direct hit.

Even if it doesn't,

the recoil from the barrage
will put some distance

between the paramecium and its attacker.

What can I say?

That's life in the dewdrop.

That little guy is tardigrade,

an animal smaller than the head of a pin.

Don't underestimate them.

Tardigrades have been living on this planet

a lot longer than we have.

About 500 million years.

For every one of us,

there's at least a billion of them.

They can make a living anywhere on earth.

In the frigid peaks
of the tallest mountains,

in the cauldrons of erupting volcanoes,

and in the deep ocean vents
at the bottom of the sea.

Tardigrades are so tough,

they can survive naked

in the vacuum of space.

They've survived all five

of the most recent mass
extinctions on this planet.

A visitor from another
world could be forgiven

for thinking of earth as
the planet of the tardigrades.

If we're ever gonna get
to the bottom of this dewdrop,

better get a move on.

Every leaf and tiny clump of moss

has hundreds of thousands

of microscopic mouths called Stomata.

Plants breathe through them,

taking in carbon dioxide

and exhaling the oxygen
that we need to live.

The plants can survive without us.

But we and all the other animals...

we'd be toast without them.

The plants make food out of sunlight.

We animals can't do that.

To see how they do it,

we have to go deeper,

make ourselves
about a thousand times smaller

to get into their treasure house,

the place where they keep the good stuff...

the chlorophyll.

That's the molecule

that converts sunlight into energy.

Every one of those rectangles
is a plant cell.

And those tiny green vehicles

are its energy factories.

If we could steal their trade secrets,

it would trigger
a new industrial revolution.

But to spy on them,

we're gonna need to go deeper still.

What alien world
has the ship of the imagination

carried us to this time?

It's the cosmos...

Contained within a dewdrop.

We're on an industrial espionage mission.

If we can penetrate the trade secrets

of the manufacturing process
in that chloroplast,

let's just say our whole future
hangs in the balance.

This chloroplast is using sunlight

to break water molecules

into atoms of hydrogen and oxygen.

It combines the hydrogen
with carbon dioxide

to make sugar,

and releases the oxygen as a waste product.

To see how it happens,
we have to go even deeper,

get even smaller.

We're talking atomic scale.

Bingo.

This assembly line is the heart

of the molecular industrial complex.

At the molecular level,

things happen too fast for us to see.

So we'll have to slow them down

about a billion times.

Those larger molecules are carbon dioxide.

Each one of them is made

of one carbon and two oxygen atoms.

When sunlight strikes a green
molecule of chlorophyll,

it sets in motion a series
of chemical reactions,

breaking apart water molecules

and freeing energetic electrons.

And that's just the day shift,

when sunlight supplies
the incoming stream of energy.

There's a second shift
that works day and night

using the solar energy kept in reserve.

The energy of the free
electrons is put to work,

combining carbon dioxide with
hydrogen from the water.

The end product is sugar,
which stores the solar energy.

The chloroplast is a three-billion-year-old

solar energy collector.

This sub-microscopic solar battery

is what drives all the forests
and the fields

and the plankton of the seas.

And the animals.

Including us.

The solar-powered biosphere

collects and processes six times more power

than our entire civilization.

We understand on a chemical level

how photosynthesis works.

We can recreate the process
in a laboratory.

But we're not as good at it as plants are.

And it's not surprising,

considering nature has been at
this for billions of years,

and we've only just started.

But if we could figure out

the trade secrets of photosynthesis,

every of other source of energy

we depend on today...

coal, oil, natural gas...

would become obsolete.

Photosynthesis is the ultimate green power.

It doesn't pollute the air

and is, in fact, carbon neutral.

Artificial photosynthesis
on a big enough scale

could reduce the greenhouse effect

that's driving climate change
in a dangerous direction.

Uh-oh, place is evaporating.

Time to get out of here.

How fleeting is the life of a dewdrop.

It condenses from thin air
in the cool of the night,

only to vanish with the heat of the day.

And what of its inhabitants,
the tardigrades?

They'll be fine.

They can go without water for years.

It's hard to imagine,

but plants covered the surface of the earth

for hundreds of millions of years

before they put forth their first flower.

That was about a hundred million years ago,

shortly before the dinosaurs
were wiped out.

Our world must've been a relatively
drab-looking place back then,

dominated by shades of green and brown.

Yeah, there were giant trees
and ferns and other plant life,

but not the purple of an iris

or the crimson of a red, red rose.

Orchids were among
the first flowering species

to appear on earth,
and they're the most diverse.

Darwin was particularly fascinated

by the comet orchid of Madagascar,

a flower whose pollen is hidden
at the bottom

of a very long, thin spur.

There can be no stronger test of an idea

than its predictive power.

On the basis of his theory of evolution

through natural selection,

Darwin speculated that somewhere

on the island of Madagascar,
there must live flying insects

with extraordinarily lengthy tongues,

ones long enough to reach the pollen.

No one had ever seen such a beast there,

but Darwin insisted

that an animal fitting this
description must exist.

Few people at the time believed him.

It wasn't until more than 50 years later

that Darwin was proven right.

In 1903, a huge hawk moth,
called the Morgan's sphinx

was discovered in Madagascar.

Attracted by the Comet Orchid's scent,

the moth slurps its pollen
with its foot-long tongue,

exactly as Darwin expected it would.

It's even more amazing that the
Morgan's sphinx was discovered

when you consider that more than 90%

of Madagascar's rain forest
had been destroyed.

In the years since Darwin's
famous prediction,

this moth species could have
easily become extinct

with all the others...

every one of them a unique
phrase of life's poetry,

written in the atoms by eons of evolution.

Ah, the fragrance of lilacs.

It's one of those scents

that triggers a whole
constellation of associations,

all those junes of long ago.

But how does that happen?

How does a smell prompt a movie
to start running in your head?

It's not something we can see.

Could it be a wave of energy, like light?

Or is it some kind of microscopic particle?

It's actually a molecule.

Every odor we can sense, whether
it comes from burnt toast,

gasoline, or a field of lilacs,

is a cloud of molecules.

These molecules have particular shapes.

When I inhale them,

they stimulate a particular set
of receptor cells in my nose.

An electrical signal
then travels to my brain,

which identifies the scent as lilac.

Other scents are carried by
different molecules

with different shapes.

But when I smell a flower or
the smoke from a campfire

or the grease from a motor gear,

I'm often flooded with memories.

Why is it that a simple thing
such as the scent of a flower

can trigger powerful memories?

It has to do with the way
our brains have evolved.

Our sense of smell kicks in

when the olfactory nerve
in our brain is stimulated.

That nerve is located
very close to the amygdala,

a structure that is integral
to our experience of emotion.

It's also very close to the Hippocampus,

which helps us form memories.

The network of neurons
that carry the scent signal

from my nose to my brain
has been fine-tuned

over hundreds of millions
of years of evolution.

It's a survival mechanism that can alert us

to danger or guide us to safety.

If you you can detect the predator

before he's near enough to strike,

or the fire before it traps you
in the forest,

you have a much better chance to survive

and pass on your genes
to the next generation.

That lovely scent
from this field of flowers

sets off a unique combination
of nerve signals.

Only that exact combination
can crack the safe

where the memory of lilacs
is stored inside my brain.

Wonder who they're for.

Maybe we'll find out later.

But first, there's another
hidden cosmos waiting for us.

The plants are softly breathing,

inhaling molecules of carbon dioxide

and exhaling molecules of oxygen.

And I'm doing the opposite.

Unlike snowflakes and fingerprints,

atoms or molecules of the same kind

are utterly identical to one another.

With every breath we take,

we inhale as many molecules
as there are stars

in all the galaxies
in the visible universe.

And every breath we exhale
is circulated through the air,

and mixed gradually across the continents,

it becomes available for others to breathe.

Breathe with me.

We all just inhaled about
100 million molecules

that once passed through
the lungs of everyone

who ever lived before us.

Think of it... This kind
of atomic reincarnation

is another link to our distant ancestors,

including those who first
launched us on our explorations

of the unseen universes.

These universes are as real as you or me,

and they surround us.

There was a moment when we awakened

to a new way of thinking and seeing.

It happened about 2,500 years ago

on the Greek islands that lie

between the empires of the east and west.

There, merchants, tourists
and sailors freely mingled,

exchanging tales of great kings and gods.

In Ionian cities and towns like
Miletus, in what is now Turkey,

the most fundamental elements

of the way we live now first appeared.

Here, for the first time,
reenactments of aspects of life

created and executed by professionals

with the expectation of
touching something deep

within the hearts of the audience,

or just making them laugh...

The first plays, dramas and
comedies, were performed.

Government by the people.

The first inklings, imperfect
then as now, of a democracy,

and the notion that the ordinary citizen

might possess certain rights,

come to us from this time and place.

But in my view, the most
revolutionary innovation of all

to come to us from this
ancient world was the idea

that natural events were
neither punishment nor reward

from capricious gods.

The workings of nature could be explained

without invoking the supernatural.

The first person to express this thought

was a man named Thales.

When the thunder clapped
or the earth quaked,

it was not because something
you did had somehow displeased

the very demanding gods.

No, it was the result of natural processes

that we were capable of understanding.

Though none of the books he is
said to have written survive,

Thales kindled a flame
that still burns to this day:

The very idea of cosmos out of chaos,

a universe governed
by the order of natural laws

that we can actually figure out.

This is the epic adventure that
began in the mind of Thales.

Only a century following Thales' death,

another genius came along.

And he, more than any other,

was the first to discover the existence

of the hidden universes that surround us.

Democritus of Abdera was a true scientist,

a man with a passionate desire
to know the cosmos

and to have fun.

This is the man who once said,
"a life without parties

would be like an endless road
without an end."

You mean, that's it?

That's all there is?

Just a bunch of atoms in a void?

Yep.

Well, think about it.

The world has to be made

of countless indivisible
particles in a void.

Otherwise, nothing could move
or grow, be divided or changed.

Without atoms

and empty space for them to move in,

so don't be sad, my friends.

Just think of the infinite possibilities

that arise from different
arrangements of those atoms.

Here's to the atoms

in this cup and in this wine...

And to the laughter they make possible.

Dispersed through
the Clay of the cup

are microscopic mineral grains,

different kinds of crystals,

each with its own distinctive
atomic architecture.

Mineral structures are exquisite,

but they have a limited repertoire.

A grain of quartz is a lattice
of the same three atoms

repeated, without variation,
over and over again.

Even a relatively complex
mineral lattice like topaz,

composed of ten or so atoms,

can only repeat the identical
atomic structure

again and again.

Toenon,

to free it from the lattice
prison of endless repetition,

you need an atom that can bond
in all directions

with other atoms like itself

as well as with atoms of different kinds.

Behold the carbon atom...

the essential element for life on earth.

Why?

Carbon is special because it can bond with

up to four other atoms at a time.

It can connect with many
different kinds of atoms,

as well as other carbon atoms.

It can curl into rings

and string together into chains,

building molecules far more
complex than any crystal.

No other atom has the same flexibility.

Even atoms that have similar
chemical properties,

like silicon,

can't form the amazing variety of molecules

built on carbon.

The carbon-based molecules
we call proteins,

the molecules of life,

contain literally hundreds
of thousands of atoms.

Carbon atoms are the backbone
of the molecules

that make every living thing on earth,

including us.

That's the difference between
rocks and living things.

Life can make enormous molecules

of stunning size and complexity,

freeing matter to improvise,

evolve,

and even love.

Take it easy, dad.

He never actually touched her.

In everyday life on our world,

on the scale of atoms,

material objects never really touch.

Each atom has a tiny nucleus at its center,

surrounded by an electron cloud
of lines of force.

As the atoms approach each other,

the boy's electron clouds

push away the girl's.

More than 99.9% of the matter of any atom

is concentrated in its nucleus.

The nucleus is surrounded
by an electron cloud

which produces an invisible field of force,

and acts like a shock absorber.

The configuration of the electron cloud

determines the nature of an element.

In the ordinary course
of things here on earth,

the nuclei never touch.

We have a sensation of touching,

but that's really just
our invisible force fields

overlapping and repelling each other.

The nucleus is very small

compared to the rest of the atom.

If an atom were the size of this cathedral,

its nucleus would be the size
of that mote of dust.

An atom is mostly empty space.

To understand the nature of matter,

we have to go deeper still,

to a place 100,000 times smaller
than the atom:

Its nucleus.

The simplest and most plentiful atom

in the cosmos is hydrogen.

Its nucleus is a single proton,

which makes hydrogen element number one.

The clouds that surround it

are the realms where
the atom's lone electron

is permitted to roam.

What happens when you have
a nucleus with two protons?

Protons repel each other.

In order to hold them together
in a nucleus,

you need other particles called neutrons.

Their job is to keep the protons

from getting out of line.

They overwhelm the protons

with their strong attractive nuclear force.

A nucleus with two protons
is element number two,

otherwise known as helium.

A nucleus with six protons
is element number six,

which is carbon,

the fundamental building block of life.

The nucleus of a gold atom has 79 protons.

They attract 79 electrons

in clouds around it.

The way light interacts
with those electrons

is what makes gold glitter.

Every additional proton in the nucleus

requires enough neutrons
to bind them together...

Up to a point.

There's an upper limit
to the number of neutrons

you can stuff into a nucleus

before it becomes unstable.

I know a place

where the nuclei of different atoms

actually do touch each other.

The sun looks like a solid object,

but it's not.

It's so hot that all its atoms

are always in their gaseous state.

The bonds that join atoms

to make solids and liquids on earth

are not strong enough to withstand

the heat of the broiling sun.

Those arcing streams of incandescent gas

that dwarf the earth

are guided by magnetic lines of force

that emanate from below
the surface of the sun.

Why is the sun so hot?

Because its own stupendous gravity

is squeezing its atoms together.

The energy of gravity is being transformed

into the energy of moving atoms.

That's what heat is.

The deeper we go into the sun,

the greater the squeezing

and the higher the temperature.

In the heart of the sun,

the atoms are moving so fast

that when they collide, they fuse.

Their nuclei touch.

The sun is a nuclear fusion reactor,

held together by its own gravity.

It's balanced between
the inward pull of gravity

and the outward push of its hot gases.

That balance has lasted billions of years,

providing stability that made possible

the evolution of life on earth.

In the sun's core,

the fusion of hydrogen into helium

releases nuclear energy
in the form of photons.

These particles of light

slowly work their way to the surface,

where they're seen as sunlight.

Helium is the ash
of the sun's nuclear furnace.

The sun is a medium-sized star.

Its core is only a lukewarm
ten million degrees...

hot enough to fuse hydrogen,

but too cold to fuse helium.

There are many stars in the galaxy

that get much hotter,

because they're more massive

and have more gravity.

Such stars fuse helium
into heavier elements,

like carbon and oxygen.

In their old age,

they gently diffuse
these elements into space.

Other stars, more massive yet,

live fast and die young

in cataclysmic supernova explosions.

In our galaxy, such stars go supernova

about once a century.

These explosions are far hotter
than the core of the sun...

hot enough to transform elements like iron

into all the heavier ones

and spew them into space.

The large magellanic cloud

is a neighboring galaxy of our milky way.

It's visible in the skies
of the Southern hemisphere.

When a supernova explodes,

its brightness rivals

that of its entire galaxy.

But all that light
is only about one percent

of the energy liberated in the explosion.

The rest of the energy is
carried off by the most common

and the most mysterious
particles in the cosmos.

There are trillions of them
passing through you right now,

and yet tracking down even one of them

will take us to one of
the strangest places on earth.

Stalking the wild neutrino

is the rarest of sport.

The lengths one must go to track them down

is nothing short of astonishing.

Welcome to Super Kamiokande,

the subterranean Japanese
neutrino detection chamber.

We're more than a half mile
beneath earth's surface.

You might ask,
"well, who in their right mind

would bury an astronomical
observatory so far underground?"

Those who hunt the most elusive
prey in the cosmos:

The neutrino.

This enormous array of light detectors

surrounding 50,000 tons of distilled water

is a trap designed to catch neutrinos only.

Other particles, such as cosmic rays...

mostly protons and electrons
that rain down from space...

cannot get through all that rock above us.

But matter poses no obstacle to a neutrino.

A neutrino could pass through
100 light-years of steel

without even slowing down.

Neutrinos hardly interact
with matter at all.

That's why you need so much of it

to catch even one of them.

On those rare occasions when a neutrino

actually does collide with
a particle of ordinary matter,

it produces a ghostly,
ring-shaped flash of light.

We're lying in wait

for a particle that weighs next to nothing.

Even the miniscule electron

has more than a million times its mass...

There!

When the supernova in
the large magellanic cloud

blew its top in 1987,

this is what it would have
looked like in here.

Now remember, the large magellanic cloud

is in our Southern hemisphere,

so the neutrinos didn't come through

that half-mile of rock above us,

they had to pass through
the thousands of miles

of rock and iron below us
to reach this detector.

But the coolest thing
was that those neutrinos

hit earth three hours before

the light from the supernova did.

If nothing can travel faster than light,

how could that possibly be?

This is a dead star walking.

It may look normal, but deep within it

something cataclysmic is happening.

This blue super giant star

has already begun to explode inside.

Like rats deserting
a sinking ship, the neutrinos

produced in the heart of the exploding star

race outward at near the speed of light,

through overlying mass

in only a few seconds.

But the shock wave of the exploding gas

plods along from the center of the star

at 1/10,000 the speed of light

until it finally reaches

the star's surface,

turning it into supernova 1987a.

It took hours for the explosion

to reach the surface of the star
and blow it wide open,

exposing the super hot core.

The neutrinos had
an insurmountable head start.

That's why the flash of light
arrived on earth

so much later than the shower of neutrinos.

Before anyone had ever snared
the wild neutrino,

it existed in the mind
of a theoretical physicist.

Just as Charles Darwin knew

there must be
an extremely long-nosed creature

flying around somewhere in Madagascar,

a 20th-century physicist
named Wolfgang Pauli...

was desperately seeking a particle

to rescue one of the pillars of
modern physics,

the law of the conservation of energy.

So why didn't I flinch?

Because the laws of science
differ fundamentally

from those of other human endeavors.

In order for an idea
to become a scientific law,

it has to unbreakable.

That's why I was willing to bet this face

on the laws of conservation of energy.

Now, if you try this at home,

take care not to give
the cannonball a push.

That's adding energy,

and the ball will surely
come back and do some damage.

You just have to let it go, like this.

By lifting the ball,

you give it gravitational energy,

which is the potential
to fall and accelerate.

The cannonball is going fastest

when it's at the bottom of its arc,

and at that moment,

it's converted all
of its gravitational energy

to the energy of motion.

As it swings, the cannonball
is constantly exchanging

one of these two kinds of energy
for the other,

but the total amount of energy
remains constant.

That's an example of the
law of conservation of energy.

Once the cannonball is released,

it can never gain more energy
than it had to begin with.

It has no way to fly up and break my nose.

The energy accounting books
are always strictly balanced.

There's no such thing as cheating.

So in the 20th century,

when physicists first calculated
the energy of atoms precisely,

they were startled to discover

an apparent violation of this law.

They found that in some radioactive atoms,

the nucleus can spontaneously
eject an electron.

This transforms the atom
into a different element.

The physicists were mystified.

The energy of the escaped electron

plus that of the new element

adds up to less than the energy
in the original nucleus.

But the law says,

"thou shall not destroy or create energy."

So where did the missing energy go?

In 1930...

Wolfgang Pauli predicted

there must be an undiscovered particle,

one that makes off with the missing energy.

At the time, Pauli lamented

that such a phantom particle
might be so minute,

swift and evasive

as to forever defy detection.

But that was a rare failure
of his imagination

because science is always searching

for a way to go deeper still.

A generation later,

Pauli's neutrinos were actually
detected for the first time

in radiation from a nuclear reactor.

And we've been finding them,
with difficulty, ever since.

There are scientists today

who are trying to find a way
to ride those neutrinos

all the way back to the beginning of time.

We'll go as far as they have gone

to come up against the wall of forever.

The wall of
forever is nothing new.

Our ancestors came up against it

almost as soon as they first
started imagining it.

A million dawns ago,
in the 13th century bc,

the Egyptian this temple at Abu Simbel

to honor the Pharaoh Ramses II,

depicted here in four colossal statues.

Reigning even above even this mighty king

is the falcon-headed Ra-Harakhti,

God of the sun.

The temple was designed

so that the light from the rising sun

could only enter the sanctuary
on two days every year.

As the rays enter the temple,

they burnish the statues of the gods

with their golden light

before penetrating the sanctuary.

Even then, one God remains in shadow.

Ptah, lord of creation,

as if the origin of the universe

must forever be concealed.

Feel the sun on your face.

The energy that warms you

began its journey
some ten million years ago

in the heart of the sun.

Unlike neutrinos,

the photons needed

that long to work their way out
from the core to the surface.

Why?

Because they were colliding
billions of times per second

with the sun's atoms, every collision

sending them off in a random direction.

But once they finally reached the surface,

they were free

to dash nonstop, at the speed of light,

in a mere eight minutes and 20 seconds

from the sun to you.

Ten-million-year-old light on your face.

What was happening

when that light left the heart of the sun?

The cosmic calendar compresses

the entire 13.8 billion year history

of the universe into a single year.

Every month represents
about a billion years.

Every day, about 40 million years.

The universe is so old that,
on the cosmic calendar,

ten million years ago
only takes us back as far as...

6:00 P.M. on the last evening

of the last day of the year.

And what about us?

Humans had yet to evolve.

Ten million years ago,

our ancestors were anthropoid apes,

swinging through the trees of Africa.

To us, ten million years
seems like a long time,

but it's only the length of an afternoon

on the timescale of the cosmos.

The sun began fusing hydrogen

4,500 million years ago...

August 31 on the cosmic calendar.

Our milky way galaxy

is about 10,000 million years old.

The first galaxies formed about
a few billion years earlier.

Something keeps me from going
any further back in time.

What is this?

It's the nature of light and time.

Because light travels at a finite speed,

to look across space

is to look back in time.

So the farther we see,

the older the light.

This is as far back
in the history of the cosmos

as we can see with light.

It's a baby picture of universe,

when it was only 380,000 years old.

That's 15 minutes into January 1

on the cosmic calendar.

If we look as far as we can see
in any direction

using microwave telescopes,

this is what we see,

the glow left over from the Big Bang.

Imagine that all the matter and energy

of the observable universe

was concentrated into something

no larger than this.

That's the size of the universe

when it was a trillionth of a trillionth

of a trillionth of a second old.

All the matter and energy
of the hundred billion galaxies

now splayed out across
the billions of light-years

were once pent up

in something the size of a marble.

Can you imagine how tightly packed

that marble must have been?

Far too dense for any kind
of light to move through it,

but no obstacle for the likes of neutrinos.

The big bang must have produced
stupendous numbers of neutrinos,

which flew unhindered

through that inconceivable crush of matter.

The very thing that makes them
almost impossible to detect

is what allows neutrinos
to sail through the curtain

that conceals the beginning of time.

Where are they now?

They are here, they're there,

everywhere throughout the universe.

Neutrinos from creation are within you.

From a marble...

To the cosmos.

This is the road that Thales
and Democritus put us on

some 2,500 years ago...

a road of endless searching,

a relentless, systematic hunt
for new worlds

and an ever-deepening
understanding of nature.

Who among you will pick up that torch

and take us down that next stretch of road?