WEBVTT

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Brian Cox: Our universe is an enigma,

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an endless, inexhaustible paradox.

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It's largely...

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A dark, cold, and lifeless ocean.

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But within this ocean,

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there are islands...
Blazing with light.

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Galaxies, trillions of them,

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Each one,
home to hundreds of billions of stars,

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and around many of these stars,

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there are planets,

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alien worlds,

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each incomprehensibl y strange.

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There are trillions
of planets in our universe

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and one of them

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nurtured beings capable of
contemplating this cosmic drama,

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miraculously improbable,

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brief candles flickering
against the eternal night.

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As darkness begins to fall,

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if you know that
all those points of light

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that appear one by one
in the darkening sky are distant suns,

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then it's impossible
not to be overwhelmed

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at the sheer scale
and majesty of it all.

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The universe
is infinite in all directions,

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and terrifying in all directions.

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But if you can overcome your fear,
then questions arise.

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And surely the most
profound question of all is,

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”how did all this come to be here?”

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That's a question
that's defined much of human history.

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But it's only in the last century or so

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that we've had the intellectual
and technical tools

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to interrogate nature directly
in search of an answer.

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And we've found
that it looks, for all the world,

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like there was a first moment in time,

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a beginning to the universe
13.8 billion years ago, the big bang.

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For all the world, but not quite,

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because we've begun to suspect
that there's more to it,

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and we've embarked on
a heroic quest to search for

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and to explore the time before the dawn.

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Neil Armstrong: [Can see
everything quite clearly. The light...

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It has a stark beauty all its own.

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B uzz a ld ri n: Magnificent desolation.

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- Beautiful view.
- Armstro n g: Isn't that something?

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William an ders:
For all the people back on earth,

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the crew oprollo 8

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has a message that
we would like to send to you.

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In the beginning, god created
the heaven and the earth.

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And the earth was without form and void,

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and darkness was
upon the face of the deep.

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And god said, ”let there be light'j

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and there was light.

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And god saw the light that it was good.

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Cox: Since we first became
conscious of ourselves,

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We've looked to the heavens,
to those mysterious lights...

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Searching for answers.

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What is the universe?

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How did it come to be?

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And what is our place in the cosmos?

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Cox: We sometimes doubt

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the creation stories
that our ancestors told.

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But those ancient myths
conceal a profound truth.

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The clues to the origins of everything
can be found out there...

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In light which ripples to us
from beyond the stars.

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If we 're going to dare to know
about the origin of the universe,

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then we have to have some evidence.

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And the connection we have
with the deep past is light.

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See, light travels very slowly
on the universal scale,

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only 786, 000 miles a second.

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It takes light eight minutes
to journey from the sun to the earth.

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It takes four years for light
to journey from the next nearest star.

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And that means we see that star
as it was four years in the past.

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So, the further out
into the universe we look,

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the further back in time we look.

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And because we can look
way out into the distant universe,

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we can look back towards
the beginning of time.

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Man 1: Go ahead, Charlie.

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Man 2: Okay,
we have a go for release,

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and we 're gonna be a minute late.

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0ka y, Charlie.

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Cox: In the quest to find the origin
of the universe,

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we need a time machine.

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Man 2: This is discovery.

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Man 1: We concur, Charlie.

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Cox: A telescope so powerful,

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that can peer out
so far into the universe,

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that it can capture
the most ancient light...

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The telescope's released.

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Cox: And carry us back...

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Towards the dawn of time.

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Man 1: Okay, Charlie.

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Cox: The hubble space telescope

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has taken us on
an odyssey through the universe,

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Revealing its gods...
And monsters.

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Our universe is a place of beauty...

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And terror.

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Hubble has shown us
visions of sublime creation...

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And images of awesome destruction,

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illuminating our journey
backwards in time...

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Towards the dawn.

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The Orion nebula, a stellar nursery,

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clouds of gas nurturing newborn stars
in the milky way.

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An image brought to us by light
that left the nebula 7,300 years ago.

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The pillars of creation,

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towering, delicate structures,
light years tall,

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7, 000 years ago.

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The Andromeda galaxy,

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a glittering island of a trillion suns,

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2.5 million years ago.

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A cosmic Rose,

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galaxies colliding
in a celestial dance,

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300 million years ago.

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But hubble's voyage
has taken us even further out

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into the uncharted ocean of space,

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Ever deeper into the darkness,

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Glimpsing countless ancient
and faraway galaxies.

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Wild, and primitive shoals of stars,

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lighting the way
to their primordial past,

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Until, finally, hubble approached
the farthest shore,

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A galaxy near the dawn of time.

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This is a galaxy called gn—z7 7,

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and it is one of the most
distant galaxies we've ever seen.

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This is light from some
of the first stars in the universe.

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It began itsjourney only
400 million years after the big bang,

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and it's taken 13.4 billion years
to reach us.

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When you think about that, this light
journeyed through the universe,

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and after nine billion years
of itsjourney, the earth formed.

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And then, during the whole history
of our planet,

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it completed the last third of
itsjourney and entered our telescopes.

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So, this is an image
from the edge of time.

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Gn—z7 7 was one
of the very first galaxies,

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formed at a time when the universe
itself was taking shape,

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shortly after the big bang.

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Gn—z7 7 was a strange galaxy
by today's standards.

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T wenty-five times
smaller than the milky way,

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But filled with enormous, violent stars.

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Lurking alongside these volatile giants,

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there were other things,

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delicate objects struggling
in the maelstrom,

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Some of the first planets
in the universe.

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These were strange, primordial worlds,

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and over the horizon
of one of them, a sun Rose,

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Marking a new chapter
in the history of the universe,

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The beginnings of a relationship
between stars and planets...

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That would, billions of years later,

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on a faraway world,

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lead to the origin of life.

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Now, we don't know when or where
the first dawn broke in the universe.

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But what we do know is that
the first dawn was not the first moment.

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The stars and planets
had to come from somewhere.

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So, the first dawn was
preceded by long, dark night.

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Astronomers call this era
the cosmic dark ages.

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If we continue to journey back in time,

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we 'd see shadows
fall across the universe.

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The galaxies would disappear.

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The first primitive stars would
be extinguished... One by one...

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And darkness truly would
be upon the face of the deep.

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Here in the impenetrable gloom
of the cosmic dark ages,

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our quest to understand
the origins of the universe...

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Would seem to end.

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So, how can we peer into the cosmic dark
ages to explore the origin of the universe?

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Well, perhaps counter-intuitively,

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the light from the stars
can still guide us

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because that starlight has been
travelling across the universe

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for millions or even billions
of yea rs to reach us,

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and information about the way
the universe has changed and evolved

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becomes imprinted in that starlight.

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The stars have illuminated
our voyage through time.

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But their light can't guide us
directly across the dark ages.

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Instead, their light can be used
to build maps of the universe

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in space and time...

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That allow us to navigate...

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Towards the moment of creation.

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Cox: And the most valuable light of all

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comes from very particular stars in
the spectacular swansong of their lives.

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Stars exist
in a permanent state of conflict

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because the force of gravity
is relentless.

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Left to its own devices, it will crush
anything and everything without limit.

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But fortunately,
other forces come into play.

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As a star collapses, its core heats up

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and turns into
a giant nuclear fusion reactor.

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Hydrogen is converted into helium
that releases energy

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which creates a pressure
which holds the star up.

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But stars like our sun
burn hundreds of millions

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of tons of hydrogen
into helium every second.

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And although they are big,
they're not infinite in size.

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Stars, just like human beings,
have a lifetime.

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They are subject
to the relentless march of time.

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And for stars like our sun,
the collapse continues

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until it produces a new
and exotic type of star

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known as a white dwarf.

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White dwarfs are strange beasts,

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the fading remains of stars,

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super dense, planetary-sized cores,

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usually composed entirely
of carbon and oxygen.

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Stars that were once a million times
the size of our planet,

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crushed to the size of the earth,

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subjecting the carbon
to extreme pressures,

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and making white dwarfs,
in effect, stellar diamonds.

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These diamond stars
are critically balanced,

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able to resist the relentless
inwards pull of gra vity.

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But only just.

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And that can make them
ticking time bombs.

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In 2078, hubble was in orbit.

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The telescope focused
on a galaxy far, far away,

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Hunting for a distant white dwarf

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that we knew was coming to the end
of its extraordinary life.

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For millions of years,
the white dwarf had remained hidden,

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Locked in orbit around
a much biggest star,

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a red giant.

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As they circled each other,

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the white dwarf's gravity drew in
gas and plasma from the red giant.

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The mass of the white dwarf increased...

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Until it approached a critical limit...

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Known as the chandrasekhar mass...

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And surpassed it...

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Triggering a colossal
thermonuclear reaction.

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The white dwarf detonated...

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In a gigantic explosion
called a supernova

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That millions of light years away,

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was detected by hubble.

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That white dwarf star,

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or to be more precise, the supernova
that it became, has a name.

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It's called sn 2078gv.

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And even though it is
70 million light years away,

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it is so bright
that we could make a movie on it.

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I mean, imagine now, this is a star
the size of a planet

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ending its life with a flash of light

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that's as bright as five billion suns.

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Now, although supernova like these
only shine for a few days,

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they cast a profound light
out across the universe.

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We've given a name to
the sorts of superno va hubble saw.

00:27:11.561 --> 00:27:14.201
They're called type 7a supernovae

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and they're common enough to allow us
to map the evolution of the universe.

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Type 1A supernovae
really are nature's gift to us

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because they all explode
in the same way.

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That means that they all shine
with the same brightness.

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And that means that if we see one
that's dimmer, it must be farther away.

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And that allows us to measure

00:27:43.761 --> 00:27:46.401
the distance to the galaxy
that contains the supernova.

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And because they shine so bright,

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we can see them
tens of billions of light years away.

00:27:52.601 --> 00:27:54.881
That means that we can measure
the distance to galaxies

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all the way out towards the edge
of the observable universe.

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But there's other information
encoded in the light.

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When we look at the light
from distant supernova explosions,

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we see something very interesting,
and very surprising,

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because the light
from every single supernova

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that's not in our neighbourhood
is redder that it should be.

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The further away the supernova,
the redder the light.

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It's called a redshift.

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Now, light has a wavelength,

00:28:55.321 --> 00:28:59.041
and the longer the wavelength,
the redder the light.

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So, the explanation is that,

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during the time the light has been
travelling from the supernova to us,

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space itself has been stretching,
and that stretched the light.

00:29:10.521 --> 00:29:14.361
And that means that
the universe is expanding.

00:29:18.481 --> 00:29:22.761
In our quest to find the origin
of the universe, this is a vital clue.

00:29:25.281 --> 00:29:27.761
Because if the universe
is expanding today,

00:29:28.841 --> 00:29:32.201
then, tomorrow,
everything will be farther apart.

00:29:37.201 --> 00:29:42.081
And it follows that, yesterday,
everything was closer together.

00:29:44.241 --> 00:29:46.601
So, if we want to understand
how it all began,

00:29:50.281 --> 00:29:52.161
we have to wind back time

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through billions of yesterdays.

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We have to go back to a time
before the earth and the sun,

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To a time before the galaxies,

00:30:26.441 --> 00:30:30.441
And all the while,
the universe is shrinking,

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getting ever smaller,
denser, and hotter,

00:30:40.521 --> 00:30:45.161
until we arrive at the most famous
moment in the history of the universe.

00:31:10.001 --> 00:31:12.601
Our universe is a place
of infinite variety.

00:31:20.721 --> 00:31:23.601
There are galaxies of exquisite beauty,

00:31:27.761 --> 00:31:30.521
stars of stupendous power,

00:31:34.961 --> 00:31:40.001
and planets...
Countless brave new worlds.

00:31:57.001 --> 00:31:59.521
Galaxies, stars, and planets

00:31:59.601 --> 00:32:02.841
are the things that make
our universe remarkable.

00:32:09.441 --> 00:32:13.561
They are the things that make it
more than a barren expanse.

00:32:22.521 --> 00:32:26.441
How did a universe of light and life

00:32:26.521 --> 00:32:30.441
emerge from the cataclysm
of the big bang?

00:32:35.401 --> 00:32:37.601
Unfortunately, we don't know.

00:32:37.681 --> 00:32:40.721
We don't even know
if the universe had a beginning.

00:32:40.801 --> 00:32:44.481
But we do know a great deal
about how the universe evolved

00:32:44.561 --> 00:32:48.001
from a very different state
a long time in the past.

00:32:48.081 --> 00:32:50.881
We know that 13.8 billion years ago,

00:32:50.961 --> 00:32:55.081
this space that I'm standing in now
and the space you're standing in now

00:32:55.161 --> 00:32:58.521
and all the space out to the edge
of the observable universe

00:32:58.601 --> 00:33:03.441
containing two trillion galaxies
was very hot and very dense,

00:33:03.521 --> 00:33:05.681
and has been expanding ever since.

00:33:06.161 --> 00:33:10.921
Now, that implies that way back,
everything was closer together,

00:33:11.001 --> 00:33:14.041
everything was contained
in a very small speck.

00:33:14.121 --> 00:33:16.601
But how small was that speck?

00:33:17.201 --> 00:33:18.761
How did it come to be?

00:33:19.121 --> 00:33:23.321
Well, we used to think
that the universe emerged in that state,

00:33:23.401 --> 00:33:26.041
very hot and very dense
at the beginning of time,

00:33:26.121 --> 00:33:28.841
and we used to call that the big bang.

00:33:28.921 --> 00:33:34.321
But now, we strongly suspect
that the universe existed before that.

00:33:34.401 --> 00:33:39.881
And in that sense, it is possible
to speak of a time before the big bang.

00:33:50.081 --> 00:33:53.841
So, what was the universe like
before the big bang?

00:33:58.361 --> 00:34:02.561
The first thing to say
is that it was very strange.

00:34:07.641 --> 00:34:11.441
There was no matter.

00:34:11.521 --> 00:34:14.961
All that existed was spacetime

00:34:15.041 --> 00:34:17.961
and energy, an ocean of energy,

00:34:19.201 --> 00:34:23.321
almost still, but gently rippling.

00:34:33.881 --> 00:34:35.281
Before the big bang,

00:34:35.361 --> 00:34:39.841
the universe was a cold,
alien, featureless place.

00:34:43.761 --> 00:34:48.201
Picture it as a near still ocean
of energy filling the void.

00:34:49.081 --> 00:34:51.321
Although it contained no structures,

00:34:51.401 --> 00:34:56.561
that energy did have an effect
on space. It caused it to stretch.

00:34:59.361 --> 00:35:02.001
Not the gentle expansion we see today,

00:35:02.081 --> 00:35:05.281
but unimaginably violent expansion.

00:35:05.361 --> 00:35:08.201
That expansion is known as inflation.

00:35:12.201 --> 00:35:17.481
Think of a speck,
a tiny, insignificant patch of space,

00:35:23.321 --> 00:35:27.881
Insignificant, except that
many billions of years later,

00:35:28.561 --> 00:35:33.441
this speck would have grown to
become our entire observable universe.

00:35:36.881 --> 00:35:41.241
The speck expanded at a phenomenal rate,

00:35:41.321 --> 00:35:43.801
an exponential expansion...

00:35:47.001 --> 00:35:48.841
That lasted...

00:35:49.881 --> 00:35:55.481
Just a few billion, billion, billion,
billionths of a second.

00:35:59.281 --> 00:36:01.801
Now, the speck continued to expand

00:36:01.881 --> 00:36:04.161
until it was about
the size of this cave.

00:36:04.241 --> 00:36:07.761
And then, inflation
drew rapidly to a close,

00:36:07.841 --> 00:36:11.081
and all the energy in that ocean
that was driving the expansion

00:36:11.161 --> 00:36:14.921
was dumped into space
and formed the ingredients

00:36:15.001 --> 00:36:18.041
of everything
in our observable universe.

00:36:18.121 --> 00:36:21.961
I mean, imagine that.
A space about this size

00:36:22.041 --> 00:36:26.281
filled with enough energy
to form two trillion galaxies.

00:36:27.321 --> 00:36:28.961
That's what we call the big bang.

00:36:39.041 --> 00:36:41.281
So the big bang was not,

00:36:41.361 --> 00:36:44.881
as we commonly imagine,
some kind of explosion.

00:36:47.881 --> 00:36:52.521
It was actually
a transformation of energy into matter.

00:36:59.801 --> 00:37:03.881
And the fossilised remains
of these momentous events,

00:37:03.961 --> 00:37:08.481
the memory of the rippling ocean
of energy that drove inflation

00:37:08.561 --> 00:37:11.681
became imprinted into our universe.

00:37:13.121 --> 00:37:17.561
In fact, these fossilised ripples
shaped our universe,

00:37:18.521 --> 00:37:23.681
influencing where each galaxy
and star emerged,

00:37:23.761 --> 00:37:26.881
each planet and moon.

00:37:31.161 --> 00:37:33.481
But how do we know all this?

00:37:36.921 --> 00:37:39.841
How do we know
that there was a big bang?

00:37:41.321 --> 00:37:43.321
How do we know there were

00:37:43.401 --> 00:37:47.041
ripples in an ocean of energy
before the big bang?

00:37:54.241 --> 00:37:55.761
The answer is...

00:37:58.481 --> 00:38:00.121
Cox: That we've seen them.

00:38:52.681 --> 00:38:55.721
Cox: Planck scanned the entire cosmos

00:38:58.041 --> 00:38:59.601
looking for light.

00:39:10.841 --> 00:39:14.121
Not light from galaxies or stars,

00:39:16.961 --> 00:39:19.681
but light from the beginning of time.

00:39:48.121 --> 00:39:50.961
This is a photograph
of the distant past.

00:39:51.321 --> 00:39:53.361
It's the most ancient light
in the universe.

00:39:53.441 --> 00:39:58.401
This is light that's travelled for
almost 13.8 billion years to reach us.

00:39:58.921 --> 00:40:01.121
It's a photograph of the entire sky,

00:40:01.201 --> 00:40:03.329
a celestial sphere, if you like,

00:40:03.353 --> 00:40:05.481
every direction
that we can look,

00:40:05.561 --> 00:40:08.321
and it's been laid flat
so we can see it all.

00:40:09.121 --> 00:40:12.321
It's called the cosmic microwave
background radiation,

00:40:12.401 --> 00:40:14.681
and it's an almost featureless glow.

00:40:14.761 --> 00:40:18.161
There were no stars
and no galaxies in this universe.

00:40:18.961 --> 00:40:20.561
Now, you might ask the question,

00:40:20.641 --> 00:40:23.401
"well, if there were
no stars and there were no galaxies,

00:40:23.481 --> 00:40:25.441
"then, where's the light coming from?"

00:40:25.521 --> 00:40:29.361
The answer is, the light
is coming from the universe itself.

00:40:29.441 --> 00:40:32.681
Because this is only a few hundred
thousand years after the big bang,

00:40:32.761 --> 00:40:35.041
so, the universe was hot.

00:40:35.121 --> 00:40:39.681
So, what you're seeing here
is the afterglow of the big bang.

00:40:55.641 --> 00:41:00.481
The most revealing thing
about this picture is the detail,

00:41:08.561 --> 00:41:09.881
The variation.

00:41:21.921 --> 00:41:23.361
This pattern is one of

00:41:23.441 --> 00:41:26.921
the most important discoveries
in all of human history

00:41:27.001 --> 00:41:30.121
because it represents
one of the necessary steps

00:41:30.201 --> 00:41:32.521
in the story of how we came to be here.

00:41:42.641 --> 00:41:46.881
See, that still ocean of energy
that drove the rapid expansion

00:41:46.961 --> 00:41:51.841
of space during inflation
could not be entirely still.

00:41:52.161 --> 00:41:54.241
There had to be ripples in the ocean.

00:41:54.321 --> 00:41:58.441
It's a consequence of the laws
of nature, as we understand them.

00:42:04.801 --> 00:42:08.601
And those ripples in the ocean
were imprinted into our universe

00:42:08.681 --> 00:42:12.761
through the big bang
that emerged as those areas

00:42:12.841 --> 00:42:16.081
of slightly different density
in the young universe.

00:42:17.961 --> 00:42:21.721
And then, as the universe
continued to expand and cool,

00:42:21.801 --> 00:42:24.481
the regions that were
slightly denser collapsed

00:42:24.561 --> 00:42:27.761
to form the first stars and galaxies.

00:42:28.641 --> 00:42:31.921
50, without those ripples,
we would not exist.

00:42:36.841 --> 00:42:40.641
But there's one more extraordinary thing
about these ripples.

00:42:41.841 --> 00:42:44.641
And that's the fact
that we predicted them

00:42:44.721 --> 00:42:47.441
before we knew they existed.

00:42:49.561 --> 00:42:53.881
And then, we ventured into space
to test our theory.

00:42:54.881 --> 00:42:59.601
Planck's observation of the afterglow
of the big bang is strong evidence

00:42:59.681 --> 00:43:02.641
for our outlandish creation saga,

00:43:04.441 --> 00:43:10.281
the story of the speck,
the ripples, and inflation.

00:43:16.081 --> 00:43:19.001
These ripples, then,
are the seeds of our creation,

00:43:19.081 --> 00:43:21.921
and we dared to guess that they exist

00:43:22.001 --> 00:43:24.881
from our vantage point here,
on a small planet

00:43:24.961 --> 00:43:29.241
13.8 billion years
after the moment of creation.

00:43:30.081 --> 00:43:35.281
And then, because we're scientists,
we decided to launch a spacecraft

00:43:35.361 --> 00:43:39.961
out into space, and capture
the oldest light in the universe.

00:43:40.041 --> 00:43:43.241
And we saw that our guess was correct.

00:43:44.001 --> 00:43:46.921
We dared to imagine
a time before the dawn,

00:43:47.001 --> 00:43:51.961
and we proved that
our creation story is not a myth.

00:43:59.321 --> 00:44:05.161
So, here is the creation story
as told by science.

00:44:08.721 --> 00:44:11.761
In the beginning,
there was an ocean of energy

00:44:12.361 --> 00:44:16.561
that drove a rapid expansion
of space known as inflation.

00:44:18.561 --> 00:44:20.041
There were ripples in the ocean.

00:44:25.041 --> 00:44:29.961
As inflation ended, the ocean of energy
was converted into matter,

00:44:31.801 --> 00:44:33.321
then the big bang.

00:44:40.081 --> 00:44:43.881
And the pattern of the ripples
was imprinted into our universe...

00:44:45.401 --> 00:44:48.241
As regions of slightly different density

00:44:48.321 --> 00:44:53.441
in the hydrogen and helium gas
that formed shortly after the big bang.

00:45:14.601 --> 00:45:16.921
The denser regions of gas collapsed...

00:45:20.881 --> 00:45:22.841
To form the first stars...

00:45:36.441 --> 00:45:37.921
And the first galaxies.

00:45:42.161 --> 00:45:44.201
And nine billion years later,

00:45:47.641 --> 00:45:50.841
a new star formed in the milky way...

00:45:53.081 --> 00:45:54.721
The sun.

00:46:02.881 --> 00:46:05.601
The star was joined by eight planets...

00:46:07.721 --> 00:46:10.521
Including earth.

00:46:16.601 --> 00:46:21.961
And nearly 73.8 billion years
after it all began,

00:46:22.721 --> 00:46:24.721
we emerged...

00:46:26.641 --> 00:46:29.161
Blinking into the light.

00:46:59.241 --> 00:47:01.681
Man:
"To see the earth as it truly is,

00:47:01.761 --> 00:47:06.401
”small and blue and beautiful
in that eternal silence where it floats,

00:47:06.481 --> 00:47:09.801
”is to see ourselves
as riders on the earth together,

00:47:10.761 --> 00:47:14.441
”brothers on that bright loveliness
in the eternal cold,

00:47:15.361 --> 00:47:19.241
”brothers who know now
they are truly brothers. ”

00:47:24.601 --> 00:47:26.521
Cox: We all have moments of wonder.

00:47:28.001 --> 00:47:29.681
We all dream.

00:47:31.281 --> 00:47:35.281
Our thoughts float free,
soaring across the earth

00:47:36.161 --> 00:47:38.961
and out into a canopy of stars.

00:47:42.881 --> 00:47:47.561
In our most reflective moments,
I think we all understand that

00:47:47.641 --> 00:47:51.801
small, though we are,
we are connected to the universe.

00:47:53.401 --> 00:47:56.241
We are collections of simple atoms,

00:47:57.881 --> 00:48:00.441
but atoms arranged remarkably,

00:48:03.601 --> 00:48:08.801
with the urge to explore the universe,
and to comprehend it,

00:48:14.361 --> 00:48:19.801
And celebrate our own place
in this great cosmic saga.

00:48:25.881 --> 00:48:30.201
And if we follow that saga back,
it takes us on a pilgrimage...

00:48:34.201 --> 00:48:36.641
To a time before the dawn,

00:48:41.801 --> 00:48:47.441
And to strange ripples that existed
in a universe before our own.

00:48:59.761 --> 00:49:02.401
I think we all must wonder
about the meaning of it all.

00:49:03.321 --> 00:49:06.041
What does it mean to be human?
Why do we exist?

00:49:06.121 --> 00:49:08.001
Why does anything exist at all?

00:49:08.881 --> 00:49:11.921
These do not sound
like scientific questions.

00:49:12.001 --> 00:49:15.961
They sound like questions
for philosophy or theology, even.

00:49:16.601 --> 00:49:18.721
But I think
they are scientific questions

00:49:18.801 --> 00:49:23.681
because they're questions about nature,
they're questions about the universe

00:49:24.081 --> 00:49:27.561
and the way to understand the universe
is to observe it.

00:49:27.641 --> 00:49:31.561
And we've seen ripples in the most
ancient light in the universe,

00:49:31.641 --> 00:49:35.161
laid down by events
that happened before the big bang.

00:49:35.241 --> 00:49:37.969
We've seen billions
of galaxies written

00:49:37.993 --> 00:49:40.721
across the sky in
a giant cosmic web.

00:49:40.801 --> 00:49:44.321
And we've seen thousands of planets
orbiting around distant stars,

00:49:44.401 --> 00:49:46.841
worlds beyond imagination.

00:49:47.441 --> 00:49:49.561
Now, the lesson to me is clear.

00:49:49.681 --> 00:49:54.641
We won't answer the deepest questions by
being introverted, by looking inwards.

00:49:54.721 --> 00:49:58.561
We will answer them by lifting
our gaze above the horizon

00:49:58.641 --> 00:50:02.481
and looking outwards
into the universe beyond the stars.

00:50:03.081 --> 00:50:07.601
We used to look to the sky
and see only questions.

00:50:07.681 --> 00:50:10.041
Now, we're beginning to see answers.

00:50:43.001 --> 00:50:45.241
Kimberly arcan d:
Hubble is a very special telescope.

00:50:45.321 --> 00:50:47.521
It's kind of like
the celebrity telescope

00:50:47.601 --> 00:50:49.681
and for a really good reason.

00:50:50.361 --> 00:50:54.681
It was the first time that we were
able to launch such a powerful,

00:50:54.761 --> 00:50:56.961
large optical telescope into space.

00:50:59.681 --> 00:51:03.481
Mason: The earth's atmosphere
kind of blurs out lots of our images.

00:51:03.561 --> 00:51:05.321
And so, by putting
the telescope in space,

00:51:05.401 --> 00:51:09.641
we get these precise,
crystal clear images of our universe.

00:51:09.721 --> 00:51:13.601
Man: Three, two, one, and lift-off

00:51:13.681 --> 00:51:17.041
of space shuttle discovery
with the hubble space telescope,

00:51:17.121 --> 00:51:19.601
our window on the universe.

00:51:19.721 --> 00:51:23.721
Carole haswell: The feeling that you get
when the space shuttle takes off,

00:51:23.801 --> 00:51:28.041
there's just a sort of...
The sound and the vibrations,

00:51:28.121 --> 00:51:30.681
it's just incredibly awe-inspiring.

00:51:34.641 --> 00:51:36.441
Man: All rocket boosters
have done their job.

00:51:36.721 --> 00:51:38.961
Man 1: Go ahead Charlie.

00:51:39.721 --> 00:51:41.261
Man 2: Okay,
we have a go for release,

00:51:41.281 --> 00:51:42.921
and we 're gonna be a minute late.

00:51:59.201 --> 00:52:01.801
Haswell: We were all sort of
sitting on the edge of our seats,

00:52:01.881 --> 00:52:03.841
waiting for the very first images

00:52:03.921 --> 00:52:06.961
where hubble is showing us
what it can see in the universe,

00:52:07.881 --> 00:52:12.361
and that turned into
an unexpectedly long wait.

00:52:15.161 --> 00:52:16.681
Newsreader: Engineers have discovered

00:52:16.761 --> 00:52:19.401
that the giant telescope
has a warped mirror,

00:52:19.481 --> 00:52:22.601
which means the images
sent back to NASA are distorted.

00:52:24.881 --> 00:52:29.321
Haswell: We had this very, very
precisely engineered mirror,

00:52:29.401 --> 00:52:33.921
but it had been very precisely
engineered to the wrong shape.

00:52:37.041 --> 00:52:40.601
For the first three years in the life
of the hubble, it wasn't producing

00:52:40.681 --> 00:52:43.641
the wonderful images
that everyone had expected.

00:52:45.881 --> 00:52:48.921
Haswe ll: The solution
was the same solution

00:52:49.001 --> 00:52:52.081
to the fact that, as a kid,
I couldn't read the blackboard.

00:52:52.161 --> 00:52:55.801
The solution was basically
to fit the telescope

00:52:55.881 --> 00:52:59.801
with corrective optics,
or something analogous to spectacles.

00:52:59.881 --> 00:53:02.321
Man: And we have a go
for main engine start.

00:53:02.881 --> 00:53:07.401
Five, four, three, two, one,

00:53:08.561 --> 00:53:11.841
and we have lift off
lift off of the space shuttle endeavou r

00:53:11.921 --> 00:53:15.361
on an ambitious mission
to service the hubble space telescope.

00:53:15.721 --> 00:53:17.961
Jeff Hoffman: It's kind ofamazing
that we have to be able

00:53:18.041 --> 00:53:22.801
to position this optical equipment to
an accuracy of better than a millimetre,

00:53:22.881 --> 00:53:26.761
something that we 'd have trouble doing
even on the ground, in your bare hands.

00:53:27.481 --> 00:53:30.441
Man: Firm handshake
with mr hubble's telescope.

00:53:31.161 --> 00:53:33.221
Woman: We copy that...

00:53:33.241 --> 00:53:37.121
The vice president and I
wanted to call you and congratulate you

00:53:37.201 --> 00:53:39.681
on one of the most spectacular
space missions in our history.

00:53:43.481 --> 00:53:48.201
Arcand: And when hubble opened
its eyes after they were corrected,

00:53:48.281 --> 00:53:52.521
the views that we were able to get
from that telescope changed forever

00:53:52.601 --> 00:53:57.441
the way we understood and visualised
the universe that we live in.

00:54:02.801 --> 00:54:07.121
The pictures are remarkable.
The trouble with hubble is over.

00:54:12.521 --> 00:54:15.441
David kaiser: It's really hard
to remember what it was like

00:54:15.521 --> 00:54:17.481
before we had
the hubble space telescope.

00:54:17.961 --> 00:54:20.761
We've gotten so used to these
extraordinary photographs

00:54:20.841 --> 00:54:23.841
of the near, of the far,
of the very, very far.

00:54:29.001 --> 00:54:30.961
Mason: I think, any time I look at
a hubble image,

00:54:31.041 --> 00:54:32.841
my mind gets blown a little bit.

00:54:34.561 --> 00:54:38.641
I was the kid that had, like, printouts
of hubble images in their locker.

00:54:43.801 --> 00:54:48.481
Anybody, whether they have the heart
of an astronomer or soul of a poet,

00:54:48.561 --> 00:54:51.241
they're going to find things
in the images from hubble

00:54:51.321 --> 00:54:55.201
that just appeal to them
from the point of pure wonder.

00:55:06.201 --> 00:55:08.641
Haswell: Hubble has
not only done the things

00:55:08.721 --> 00:55:12.041
that people expected and hoped it would,

00:55:12.121 --> 00:55:13.921
but it's actually done a lot of things

00:55:14.001 --> 00:55:16.281
that nobody would have
dared to dream of.

00:55:19.561 --> 00:55:20.861
Kaiser: One of the biggest discoveries

00:55:20.881 --> 00:55:23.361
that came from using
the hubble space telescope

00:55:23.441 --> 00:55:25.641
is that, not only is our universe
getting bigger,

00:55:25.721 --> 00:55:29.641
it's not just expanding and stretching,
it's actually getting bigger faster.

00:55:33.121 --> 00:55:37.561
We can well imagine that the universe
is going to continue to expand

00:55:37.641 --> 00:55:41.481
and get so big that, eventually,
the galaxies will just disappear.

00:55:41.561 --> 00:55:46.281
They'll be so far away from us and
moving so rapidly that we have no hope

00:55:46.361 --> 00:55:49.841
of seeing any light from them,
and that's a real possibility

00:55:49.921 --> 00:55:51.921
for what could happen in the future.

00:55:55.241 --> 00:55:56.781
Kaiser: We still have these mysteries of

00:55:56.801 --> 00:56:01.401
what's really driving
this new phase of accelerated expansion,

00:56:01.481 --> 00:56:04.321
and we're building new tools
to try to refine those questions.

00:56:19.641 --> 00:56:23.001
Larry gladney: The hubble telescope
which was a marvel for its time

00:56:23.081 --> 00:56:26.201
is really far behind
what we would design today.

00:56:30.361 --> 00:56:34.401
It will be completely outclassed
by the next generation telescope,

00:56:34.481 --> 00:56:38.761
the James webb space telescope,
which will see even deeper than hubble.

00:56:43.001 --> 00:56:47.241
Haswell: And that will give us
unprecedented detailed views.

00:56:47.321 --> 00:56:51.241
We can use it to see through
some of the very dense,

00:56:51.321 --> 00:56:55.601
murky dust clouds and actually see
stars in the process of forming.

00:56:56.881 --> 00:57:01.281
We also can use it to look further
and further back in time.

00:57:03.641 --> 00:57:07.161
That's going to be a very, very exciting
story which is going to unfold,

00:57:07.241 --> 00:57:09.561
I think, within
the next three or four years.

00:57:21.161 --> 00:57:24.481
Hubble is still king
because it's still a big observatory

00:57:24.561 --> 00:57:27.561
in comparison
to what we've had in space before.

00:57:28.841 --> 00:57:31.801
Hubble is a unique instrument
for making discoveries that

00:57:31.881 --> 00:57:34.201
no other telescope
could possibly ha ve made.

00:57:39.441 --> 00:57:42.041
I think, when you think
about an image of space,

00:57:42.121 --> 00:57:44.361
when you think about space,
you think of a hubble image.