All language subtitles for How the Universe Works Series 8 Part 7 Edge of the Universe 1080p

Narrator: Islands have edges.

Planets have edges.

Even galaxies have edges.

But what about the universe?

As explorers,
as curious humans that we are,

we're obsessed with boundaries
and limits.

And we want to know,

"does the whole thing,
the universe, have a limit?"

does the universe have an edge?
Well, the answer is yes and no.

It depends on
what you mean by edge.

Narrator:
The edge of what we can see?

The edge of where we can go?

Or the edge of reality itself?

Thaller: Looking out to the edge
of the universe

is tremendously important
to understand

our place
in the universe itself.

Bullock: We're talking
about our universe.

We're talking about the thing
that we exist within.

The most fundamental
thing there is,

we're driven to understand it.

There is always a desire to push
the knowledge to the edge.

Narrator:
So, can we ever find

the edge of the universe?

-- Captions by vitac --
www.Vitac.Com

captions paid for by
discovery communications

♪

2016,
the hubble space telescope

turned toward
a dark patch of sky

in the constellation ursa major.

It captured an image
of an indistinct blob of light.

The glow is from a distant
galaxy called gn-z11...

♪

...The most distant galaxy
we've ever observed.

But is this the edge
of the universe?

Thaller: The universe all around
us is filled with galaxies,

so it's kind of natural to say,
"would there be a final galaxy?

If you traveled far enough away,

would you finally be at the very
last galaxy in the universe

looking out into empty space?"

narrator: That's a difficult
question to answer.

Because there's a limit
to how far we can see.

It all comes down
to the speed of light

and the age of the universe.

The key to understanding
the edge of the universe

is that light travels
very, very fast,

but not infinitely fast.

It takes time for it
to get from one place

in the universe to the other.

You open the curtains,
light fills the room.

It doesn't seem
to travel at all.

But over the vast distances
of the universe,

you actually notice
this travel time.

Even the sun
93 million miles away,

the light takes eight minutes
to get to us.

When you look out at the stars,
we start to think of distance

in terms of light-years
because it takes years

for the light
to get from those stars to us.

Then when you look at galaxies,
then you're talking about

millions
or billions of light-years.

Narrator: When we look at the
light from galaxy gn-z11,

we're seeing light emitted
13.4 billion years ago.

You can't really
even find a galaxy

too much farther away than that

because the universe
is only 13.8 billion years old,

and it takes a certain amount of
time for galaxies to even form.

So we're not going to find
too many more galaxies

farther away than this.

If things are far enough away,
there is no way that light

can get to us
in the age of the universe.

What this means
is there's a hard limit

to the edge of the universe
that we can see,

and this is set
by the age of the universe.

Narrator: Gn-z11 sparked
into life

early in the history
of the universe,

just 400 million years
after the big bang.

Before that, there were no stars
to send out light.

Thaller: If you look
in any direction at all,

you get all the way back to
when there were no stars,

no galaxies,
nothing but very, very hot gas,

and that sort of forms
a shell around us.

Narrator: That outer shell is
the cosmic microwave background.

It is the oldest light
in the universe,

the echo of the birth
of the universe,

the big bang.

The edge of our universe,

the very furthest thing
that we can see,

is one of the earliest relics

of the formation
of the universe itself.

That is the cosmic microwave
background.

Narrator: We call this the edge
of our observable universe.

So we have an observable
universe, but beyond that,

even if there
are things out there,

there's no way we can see them

because the light just could
not have gotten to us by now.

Narrator: As the name states,
the observable universe

is simply the part
of the universe we can see.

We can think
of the observable universe

sort of like a spotlight

centered on wherever
you're standing right now

and you can see to the edge of
your spotlight and not beyond.

But if you move a little bit
to the left,

a little bit to the right,

your observable universe
actually moves with you.

Narrator: For someone living
in galaxy gn-z11,

a totally different part of the
universe would be observable.

So that distant galaxy is at the
edge of our observable universe,

and we are at the edge
of their observable universe.

We have different spotlights.

One of the wonderful things
to think about

is that there are other spheres
around other galaxies,

there are other aliens
looking up into the sky tonight

wondering what the true
extent of the universe is.

Narrator: The true extent
of our universe

doesn't end with galaxy gn-z11.

But when astronomers use
the hubble space telescope

to accurately measure
the distance to gn-z11,

they find something shocking.

It's 32 billion
light-years away,

three times further
than thought possible.

Plait: So if nothing can travel
faster than light

and we measure the distance
to this galaxy,

how can it be
32 billion light-years away?

Narrator:
There hasn't been enough time

in the history of the universe

for light from gn-z11
to reach us.

There must be some mistake here.
Right?

Plait: At this point,
your brain

is probably thinking
of leaping out

of your skull
and running around screaming.

Trust me, I know.
I'm an astronomer.

I've been doing this
my whole life,

and this stuff twists
my imagination up.

It's really hard to grasp this.

How do we see a galaxy that's
32 billion light-years away

and only 13.4 billion years old?

Narrator: Gn-z11 is further away
than it should be

because something strange
is going on with our universe.

It's expanding.

And if the universe
is expanding,

then where does its edge lie

and can we ever reach it?

♪

narrator:
13.8 billion years ago,

a speck of energy
burst into life.

We call it the big bang --

space and time
pushed out in all directions.

Ever since, our universe
has expanded.

But the way it's expanding
makes finding an edge

a major challenge.

The universe is expanding

and expands according
to a very simple law

that the farther away a galaxy
is from us,

the faster it appears
to be receding away from us.

Narrator: The furthest galaxies
are moving at very high speeds.

The most distant galaxy
we've ever spotted, gn-z11,

seems to have moved 32 billion
light-years away from us

in just 13.4 billion years.

That's faster than
the speed of light.

We can measure the speeds
with which galaxies

are moving away from us,

and many, many galaxies
are moving away from us

at speeds faster
than the speed of light.

This sounds like
it's breaking the law, right?

There's this idea
that you've all been told

that relativity
says nothing goes faster

than the speed of light.

Okay, you've been lied to.

Plait: Space itself can do
what it wants.

It makes the rules,
it can break the rules.

That rule applies to matter,
not to space itself.

Space can expand
at whatever rate it wants.

Simple way to think of this
expansion law is imagine

standing on
an infinite rubber sheet

that stretches all the way out
into the distance

and you're standing
on the same place.

You can mark it
with a little "x."

now, all the sheet expands
in every direction.

So if it expands
by a factor of two,

another galaxy that was, say,
one foot away from you

is now two feet away from you
as we stretch the sheet,

but another galaxy
was 10 feet away from you.

Expand that by a factor of 2

and now
it's 20 feet away from you.

So in the same amount of time,
one galaxy moved one foot,

where another galaxy
moved 10 feet.

So the more stuff there is,

the more elastic
between you and another galaxy,

the more it seems
to expand away from you.

Narrator: Expansion means
our observable universe

stretches for a colossal
46 billion light-years

in all directions,
92 billion light-years across...

...And getting bigger
by the second.

Bullock: This number is
so incomprehensibly large

that it's difficult to wrap
your brain around.

There are trillions of galaxies
within this volume.

It's staggering.

It's so much larger than
anything we're familiar with.

Narrator:
If we were to travel

to the edge
of the observable universe,

we would enter even more
unfamiliar territory.

Imagine we're in
an ultra-fast spaceship.

We leave the solar system,
then the milky way.

As we travel deeper
into intergalactic space,

things start to get
really weird.

For every million light-years
we go from the milky way,

the galaxies move away from us

at around 13 miles
per second faster.

We have to accelerate
just to keep up.

But the galaxies keep on moving,
always beyond our reach.

♪

♪

plait: Imagine you're a sprinter
on a racetrack.

If you're running towards
the finish line,

it may take you a few seconds
to cross it.

But now imagine that that finish
line is moving away from you.

If it's moving away from you at
the same speed you're running,

you'll never reach it.

And if it's moving faster
than the runner,

then even faster runners
won't reach it.

And that's sort of what we're
seeing here with the universe.

Narrator:
Beyond a certain distance,

galaxies are racing away from us
faster than the speed of light.

It's a line called
the cosmic event horizon.

And 97% of galaxies we see
in the observable universe

are beyond this line
and unreachable,

including gn-z11.

They're sort of teasing us
to say, "look at me,

what a nice piece
of real estate."

but we know even if we started
going there now,

we could never reach them.

Narrator: Anything that has
crossed the cosmic event horizon

is out of our reach forever.

But that's not the full picture

because the expansion rate
of the universe is changing.

A little over 20 years ago,
astronomers discovered

that the current rate
of the universe's expansion

is accelerating,
it's speeding up.

Narrator: Astronomers suspect
a mysterious force is at work --

dark energy.

Dark energy is what we think
is pushing the universe apart,

causing this
accelerating expansion.

And the origin and true
physical nature of dark energy

is a big mystery.

Narrator: Thanks to dark energy,
more and more galaxies

are crossing
the cosmic event horizon

and leaving
the observable universe.

These galaxies...

Are lost to us forever.

Plait: There are galaxies
that we can see today

that in a few million years,
say, we won't be able to see

because the edge of
the observable universe

has basically moved in closer
than that galaxy.

That's going to happen
all the time.

And in a trillion years
or something like that,

all these galaxies
that we see in our sky

will be completely invisible

because they'll be beyond
the edge of the universe.

Thaller: So eventually,
every last galaxy

will be so far away from us

that light cannot reach us
through that expanding space.

It's almost as if you're driving
through a dark desert

in your car
and the very, very last town

that ever exists
has gone over the horizon

and they'll never be
any light again.

We can see less
and less of the universe

as we go into the future.

What a strange thought.

So that means we should build
all the telescopes we can now.

Narrator: There's a limit
to the universe we can see,

even with the most
advanced telescopes.

But what lies beyond

is one of the biggest
mysteries in astronomy.

The greater universe
could be stranger

than our wildest imagination.

Plait:
When you stand on the beach

and you look at the horizon

and you kind of think,
"oh, what beautiful lands

are there beyond the horizon?

Things I've never
imagined before."

it's so natural.

It's so human to ask,
"what lies beyond that?

What is the true extent
of the universe?"

♪

narrator:
The observable universe

contains trillions of galaxies.

It's about 92 billion
light-years across...

...But astronomers believe

this isn't the full extent
of the universe.

What we don't know is how much
of the universe

is our observable universe.

It could be a tiny,
microscopic speck of this

much more vast universe.

We just don't know.

Carroll: We have no idea
how much stuff there is

outside the observable universe,

but because by definition, it's
outside the observable universe,

we really don't know right now.

Narrator:
So what is out there?

One theory says that space
outside the observable universe

is pretty much the same
as our own cosmic neighborhood.

It's just more universe.
It's just like here.

It's just far enough away
that we can't see it.

So it's not like there's bizarre
places where time runs backwards

or aliens have two heads,
well, yeah, maybe.

Narrator: But further out

in the deepest parts
of the greater universe,

all bets are off.

We expect that as you go sort of
twice or three times

beyond the observable universe,

it's probably very similar
to the universe we inhabit.

But if you go a thousand times
or a million times farther,

who knows what you might see?

It might be very, very different
if we go far enough away.

Narrator: Strangely,
it all comes back

to the expansion of the universe

and one crucial detail
in that process.

There was a brief moment

in the very early history
of the universe

where its expansion
accelerated hugely.

This acceleration
is called inflation,

and in a brief moment,
the universe itself expanded

at multiple times
the speed of light.

Narrator: Inflation was
a formative moment

for our universe.

By the time it stopped,

the universe's basic
characteristics were set.

There are these
fundamental constants

that describe the phenomena
in our universe,

the fundamentals of matter
and light and space-time.

Narrator:
But some scientists think

there could be regions
of the greater universe

where inflation
has never stopped.

The idea is the greater universe
is expanding at an insane speed,

but here and there,
occasionally a little region

will stop inflating and
just expand at the normal rate.

Inflation can end somewhere

and that gives rise
to the universe we live in,

while inflation
continues somewhere else.

Narrator:
Parts of the greater universe

that continued to inflate

would be left
with different laws of physics.

This incredibly violent
inflation process

is actually monkeyed with
the very fabric of space itself,

so that a lot of the things
that we were taught

that are laws of physics
are different there.

Carroll: So in an essence,

inflation gives us
a very natural way

to make this patchwork quilt of
different parts of the universe

where things seem different.

So what we could imagine
is a super large-scale structure

where there's different regions
of the universe, domains,

and each domain has different
local laws of physics.

Narrator: These different parts
of the universe

are separated by frontiers
called domain walls.

We have similar boundaries
on earth.

Whenever you have something that
can be in many different states,

you can end up with domain wall.

If our fish swimming around
in the arctic near an iceberg,

there will be a domain boundary

between the water
being in the liquid state

where I am and the solid state
inside the ice.

So a domain wall is just a wall
between two domains.

If it's water,
this could be ice,

this could be liquid.

If you're talking about space,

this could be a kind of space
maybe you can live in.

This could be a kind of space
where you don't want to be.

Narrator: Crossing a domain wall
would be very bad news

for anyone who dared to try.

Cross that domain wall
and the laws of physics

could change dramatically.

The number of dimensions
could change.

If we were somehow able to
travel to places in the universe

where the laws of physics
are different,

we would die

because all of the chemistry
going on in our bodies

depends very, very sensitively
on the laws of physics.

So you could just dissipate like
thanos snap and you're gone.

Narrator: Domain walls
might be the closest

we get to locating
an edge in the universe.

Depends on how
you define the edge.

If it is the realm where the
laws of our universe operate,

then these domain walls are in
essence the age of the universe.

Narrator:
But this is all just theory.

If we ever really are
to work out

what the true size
and shape of the universe is,

we're going to have to look
for clues that are close to us.

Narrator: Clues that could
answer the ultimate question,

how big is the rest
of the greater universe

and could it go on forever?

♪

narrator:
For tens of thousands of years,

mankind has gazed in wonder
at the vastness of the cosmos,

but just how extensive is it?

If we could answer
that question,

it might help us to understand
our place in the universe.

One of the fundamental
questions in science

is how big is the universe?

O'dowd: To answer the question,
"how big is the universe?"

we have to answer the question,
"what shape is the universe?"

and by shape, I mean geometry.

I mean, how is the universe
curved on its largest scales?

Sutter: If we are to discover
that the universe

does have some
sort of geometric curvature,

then this might imply that it
wraps around in on itself

over incredibly large distances.

And that if you could travel
in one direction long enough,

you would end up
at your starting point.

Another version is
that the universe

is more like
an infinite flat plane.

Okay?
No curvature at all.

The further you travel,
well, the further you get

and you never get back
to where you started.

Narrator: To work out the shape
of something,

we would normally just step back
and take a look.

But clearly moving outside
the universe is a nonstarter.

Bullock:
You can't jump on a rocket

and fly a thousand times larger
than our cosmic horizon

and see what the shape
of the universe is.

We just can't do that.

Thaller: Our human perspective
on the larger universe

is so limited.

So if we want to figure out
what the larger shape

and scale of the universe is,

we're going to have to be
very clever indeed.

Narrator:
One way to be clever

is to think of the geometry
of the universe

in its simplest terms.

Bullock: When we talk about
the geometry of the universe,

we really are talking
about geometry.

In order to do geometry,
you have to take measures.

You need a cosmic ruler
to do this,

and it turns out
there's a great cosmic ruler

known as baryon
acoustic oscillations.

Narrator: Baryonic acoustic
oscillations are ripples

in the cosmic
microwave background,

the oldest light
in the universe.

As the universe expanded,

these ripples were imprinted
in space in a uniform way.

They provide a cosmic ruler

to measure vast
distances over time,

so we can gauge
if the universe expands

in curved space
or over a flat plane.

Bullock:
When we use these cosmic rulers

to try to back out
the shape of the universe,

we're sure
to a few percent accuracy

that the universe is flat.

Narrator:
If the universe is flat,

we could set off
traveling into the cosmos

and continue traveling forever.

There may be no edge
to our universe

because a flat universe
can be an infinite universe.

Now we're thinking of
the universe as something

that really does
go on forever,

that the stars and galaxies
never have an end,

and how can something
truly infinite really exist?

Infinity is weird
because it's a concept of,

because it's endless.

What does that mean? Who knows?
I don't know.

Plait: Infinity is a concept
more than anything else.

Our brains aren't
evolved for that.

We evolved living in the plains.

We were apes looking for food.

We weren't evolved to think
about the universe

and all of this stuff.

Oluseyi: I just can't stop
contemplating this stuff.

The idea of infinity
and these large numbers

and even the tininess
of everything.

It's nuts.

Yeah, thinking about infinity
makes my head hurt a little bit.

Narrator: An infinite universe
has profound implications

for understanding our place
in the cosmos.

It guarantees we're not alone.

Carroll:
But if the universe is infinite,

then there could be
an infinite number of galaxies

that have planets with life,
an infinite number without life,

then because life
did appear here on earth,

it's physically possible,

therefore,
it will definitely happen

elsewhere in the universe.

Narrator: In a flat universe,

alien life could come in
an infinite number of forms,

but there is an altogether
stranger guarantee.

If the universe has no edge,
this means that

things that seem like they are
impossible become possible.

Every possible arrangement
of matter,

every possible history.

A galaxy of a solar system
of a planet like earth

is possible

and is happening right now
in parallel to us

somewhere over there.

Freese: So that means that there
has to be another place

that has a galaxy just like ours

and it would have an earth
just like ours.

It would have people who would
have another version of you,

another version of me.

It's 100% guaranteed that there
is another max tegmark out there

having exactly this conversation
and in fact many of them.

Narrator: An infinite universe
full of max tegmarks

may be a strange concept,

but what's truly mind-bending
is understanding

the physics of a flat universe.

If the universe is infinite
and it's expanding,

what's it expanding into
and what did it expand from?

Was there ever an edge
to the universe?

Fortunately, the answer is that
it doesn't make sense

to ask that question.

Everything is expanding,

including the universe
that we exist within.

So in fact, it's not expanding
into anything

because it is everything.

♪

narrator: To help understand
what's going on

in an infinite universe,

we need to go back
to the big bang.

We want to think of the big bang
as an explosion in space,

like it happened someplace,

but there wasn't any place
before the big bang.

Space existed inside
of the big bang itself.

So it's not an explosion
in space,

it's an explosion of space.

We're sometimes told that
at the big bang,

the universe started out very,
very small and then got big,

but how can a finite point
become infinite?

Well, if the universe
is infinite,

then it was also infinite
at the big bang.

This is a tough thing
to think about.

Think about it this way.

In an infinite universe,
the galaxies go on forever

and now there's a great
distance between every galaxy.

But once upon a time,

the galaxies
were closer together,

say half their current
distance apart,

but they still went on forever.

The universe was still infinite.

Narrator:
In a flat universe,

space was infinite
from the beginning.

There was never
a single point in space

where the big bang happened.

It happened everywhere.

An infinite universe offers
infinite possibilities

but no edge to space.

But there may be
another kind of edge,

one that will only reveal itself
if the universe dies.

♪

narrator: We live in an infinite
and expanding universe.

Space has no edge.
It goes on forever.

♪

but there could be a different
kind of edge to our universe,

an edge of time.

The universe seems to have begun

13.8 billion years ago
in the past,

so there's some inclination,
some impression,

that it's finite in time.

What we call the big bang is,
as far as we understand it,

a beginning,
a start of the universe.

The universe has a finite age.

Now, does it have an edge
in the future?

Narrator: We used to think
that time would someday

come to a catastrophic end,

along with the planets,
galaxies,

and all life in the universe.

If we know there's a big bang,
if we know the universe started,

it expanded and cooled,
it's very natural to wonder

whether or not someday
the expansion will stop,

reverse, and come back,
and that's a big crunch.

♪

narrator: In a big crunch,

our expanding universe
would begin to contract.

Stars and planets would smash
into each other.

Galaxies would collide,

and all of the life left
in space would be compressed

with all the other matter
into a singularity.

♪

if this theory is true,
then the universe

would have both a beginning
and an end of time.

If we live in a universe
that will expand,

stop expanding,
and then go back into a crunch,

then it has,
in effect, two edges.

Narrator: But there's a much
stranger possibility.

Perhaps the end is
but a beginning,

where the universe
is a oscillating universe.

It has a big bang
like beginning,

it expands to a maximum size,

and then goes back
into a big crunch

and does that over and over.

Narrator: We could be residents
of a universe

created from the ashes
of another,

a single universe in a stream
of bouncing universes...

...Each full of galaxies,
planets, and life.

But our most recent observations
of the universe suggest

a big crunch isn't in the cards.

Once again, dark energy is key.

For a while we didn't know
if the expansion of the universe

was going to slow, stop,

and reverse itself
because of gravity.

There are all these galaxies
in the universe

and they're pulling on
each other by their gravity.

And if the expansion
isn't fast enough,

that gravity might be strong
enough to stop the expansion

and re-collapse the universe.

Now with dark energy,

we know that there's no way
that can happen.

The universe is going
to expand forever

because dark energy is
pumping it full of acceleration.

In order for there
to be a big crunch,

our understanding of dark energy
would have to change a lot.

That is, dark energy would have
to be extremely weird

and turn off in some very funny
way for the universe

to suddenly stop expanding
and re-collapse.

Narrator:
Without a big crunch,

there is no future edge to time.

Carroll: The universe is not
only expanding,

but it's being driven
by dark energy

to expand faster and faster
and the dark energy

doesn't dilute away,
as far as we can tell.

So the simplest idea
is that the universe

will simply continue to expand
eternally toward the future.

Narrator: Just like space,
time will go on forever.

That might sound like a better
fate for life and the universe,

but it's not.

Freese: One of the consequences
of this dark energy

that's causing the acceleration
of the universe

is that we eventually are
headed towards the big chill.

I should say, "we're eventually
headed towards the big chill."

so the universe is getting
colder and colder

and things are getting more
and more spread out.

So the accelerated and continual

and forever expansion
of our universe

might make for a frankly
depressing end to time itself.

The ultimate entropy-based
heat death of the universe

where you would walk out
and see no stars in the sky,

see absolutely nothing.

There will come one day when the
very last star in the universe

just fizzles out and that is it.

Narrator: In the future,

space will be a cold, dark
and infinite void,

where time goes on forever.

There will be nothing to do

but suffer
in the eternal expanse.

It's our inevitable fate
that there's no future edge

of time in the universe.

But even if there isn't an edge
to the universe,

could there be edges
within the universe?

If you wanted to visit the edge
of the universe,

then go find your nearest
black hole and jump on in

because that's a one-way trip.

Narrator: If you cross this
edge, you will never return.

♪

[ applause ]

narrator: April 2019,

an international team
of astronomers

makes a special announcement.

And we are delighted to be able
to report to you today

that we have seen and taken
a picture of a black hole.

Here it is.

[ applause ]

♪

narrator: It's a picture
of a supermassive black hole

at the center of the m87 galaxy
54 million light-years away.

It may also be the first image
of an edge in the universe.

Black holes create
a really interesting scenario

when we think about space
and the universe having edges.

Narrator: The edge between space
outside and inside a black hole

is called the event horizon.

Bullock: The event horizon
of a black hole

is a region within which,
once you cross inside,

the gravitational tug
is so strong

that even light cannot escape,
which means nothing can escape

once you cross
inside the event horizon.

So that really
is sort of an edge

because it really does
create a boundary.

♪

narrator: The event horizon is
not a physical barrier in space.

Event horizon is an edge
of the part of the universe

we can visit,
but it's not an edge

in the sense
that there's anything there.

You would just pass
right through it

if you actually got right up
to that place.

So it's sort of
a conceptual boundary

between two different parts
of the universe.

Narrator: If we sent a man to
probe into a black hole,

it would be a one-way trip.

The event horizons of
black holes are a sort of edge

because, once you pass through
an event horizon,

you are cut off
from the rest of the universe.

You can never go back out.

You are outside of our universe.

Once you've crossed
inside that region,

you are never coming back out,
and that's an edge.

Narrator:
Once inside the black hole,

the probe would be in
a separate part of space,

cut off from the rest
of the universe.

Sutter: Falling through the
event horizon of a black hole

is like jumping over
the edge of a cliff.

You can see the edge
and you can see the edge go by,

and then when you're at
the bottom, you can look up

and see what's happening
at the top of the cliff,

but you can never go back.

Narrator: At the bottom
of this black-hole cliff

sits a singularity,

a region of space where the laws
of physics go off the rails.

Deep toward that singularity
could be as surprising

as you might imagine
and yet still a possibility.

If you map the space-time
around a black hole

in a very particular way,

there emerges a sort of mirror
universe, a parallel universe,

on the other side
of the black hole,

identical to our own and
traversable by the black hole.

♪

narrator: So black holes are not
just edges to our universe,

they may also be gateways
to other universes.

Bullock: It's highly conjecture,

but if there's ever going
to be a space, or region,

where you're making connections
with, say, some other universe,

a black hole, in principle,
could be a portal to that.

Narrator:
But it's highly unlikely

that anyone will ever want

to venture beyond
an event horizon to find out,

and our pursuits of the other
edges in the cosmos

offer little hope either.

We can never travel beyond
the cosmic event horizon.

We will never be able
to see beyond the edge

of our observable universe.

So can we ever hope to discover
the true edge

of the greater universe
or find out if it even has one?

My feeling is that probably
we should not think

about edges for the universe.

Everything you've ever seen
in your life is finite,

it has an inside
and the outside, it has an edge.

The universe
might not be like that.

It's probably not like that.

There's probably no sense in
which the universe has an edge.

We used to think that
the ultimate limits

on the future life
were set by nature,

we couldn't get off the planet,

or there was nothing beyond
our solar system.

Now we realized
we have this vast,

vast cosmos out there
and that the ultimate limits

are actually simply
our own imagination

and our ability
to do great things with it

rather than self-destruct.

Our future destiny
is in our own hands

and I find that very empowering.

Thaller:
It is beautifully frustrating

to realize how limited we are,

to realize that we're probably
never going to get a true view

of the real extent
of the universe.

We should keep an open mind,
we should be humble,

but I think that we should
give up on the idea

that things should have edges

because that's what
we're familiar with.

The universe
is something special.

Sutter: What matters to us, and
will only ever matter to us,

is the observable universe

because that's the limit
of what we can see

and that is the limit
of what we can know.

So there is an edge
to the universe,

there's an edge
to what we can know.