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At this precise moment,
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on a planet far, far away...
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an alien sunrise ushers in a new day.
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But will alien eyes gaze upon it?
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Or will it go unseen?
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Just another moment
in a vast sterile universe.
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The hunt is on for the answer.
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Magnificent desolation.
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- Beautiful view!
- Isn't that something?
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The Milky Way.
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Hundreds of billions of stars...
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spread across
100,000 light years of space.
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Among them the Sun,
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with eight planets orbiting around it,
including our home.
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Until very recently, these were
the only worlds we knew of.
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The only planets
we could hope to explore
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for signs of life beyond Earth.
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When I first got into astronomy
back in the 1970s,
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we knew of no planets
beyond our solar system.
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We didn't have the technology
to detect them, even if they were there.
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Our neighbourhood was the only place
we could look for life.
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And so the hunt for life began
in our own backyard.
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Over the last few decades,
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multiple missions have explored
our solar system's planets.
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And even some of their moons.
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But to date,
even as we continue to look,
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no convincing evidence of life has
been found on any of these worlds.
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Earth remains one of a kind.
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The only living world around the Sun.
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But as the exploration
of the solar system continued,
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another search had begun...
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for worlds that lie
far beyond these shores.
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You know, the wonderful thing
about astronomy is
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that as we develop better
and better technology
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and accumulate more and more knowledge
about our universe,
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we turn more and more of these points
of light in the sky into worlds.
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I mean, that we've known is
a world for a long time,
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because that is the planet Mars.
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But just above Mars tonight is
a constellation called Pegasus.
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This is the square of Pegasus.
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And we now know that around there is
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a star called 51 Pegasi,
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which has a planet orbiting around it,
a gas giant about the size of Jupiter,
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that goes round that faint point
of light every four days.
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It is wonderful to think
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that, in my lifetime,
in fact in my adult lifetime,
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in the last 25 years,
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we've gone from a universe
that could have been
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devoid of planets beyond
our solar system,
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to a universe that we know
is teeming with places
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that we can search for life.
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Over the last three decades,
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some of the most powerful telescopes
on Earth have joined the hunt,
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searching for planets
unimaginably far away,
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hiding in the dark.
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Planets like 57 Pegasi b.
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The first world outside our solar system
to be detected around a Sun-like star.
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57 Pegasi b is a gas giant,
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around half the mass of Jupiter,
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but far closer to its star.
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Just imagine what that world
might be like.
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A world with skies torn
by titanic winds,
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where its hot interior is
bathed in rain of sapphires.
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In every sense,
57 Pegasi b is an alien world.
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And we soon discovered that the galaxy
is full of planets
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unlike anything seen
in our solar system.
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Planets enveloped by fierce radiation.
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Their surfaces battered and stripped
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by the high energy strobing light
of their star.
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Worlds so cold
their atmospheres are frozen solid.
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Or great swollen planets,
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with the density of Styrofoam.
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And fathomless atmospheres.
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These discoveries prove
that in one sense
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we really are not alone.
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There are other worlds out there
waiting to be explored.
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We estimate
that in the Milky Way Galaxy,
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there are more planets than stars.
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Hundreds of billions of them.
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That's hundreds of billions
of places to look for life.
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But there's a catch.
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Because not all worlds,
by a long stretch,
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are like this one.
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The first planets we found appeared
too bizarre,
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too large,
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and often too close to their stars
for living things to survive.
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To find worlds where life could exist,
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we needed to look
for smaller, rocky planets
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in orbits further from their stars.
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T-minus ten,
nine, eight, seven...
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00:11:02,120 --> 00:11:05,440
We needed to look
for another earth.
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00:11:05,960 --> 00:11:10,360
...three, two,
engine start, one, zero,
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and lift off
of the Delta II rocket with Kepler
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on a search for planets
in some way like our own.
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So the hunt moved to space
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with the launch
of NASA's Kepler space telescope...
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And we have separation.
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...searching for Earth-like worlds
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in the galaxy beyond.
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Kepler crossed 94 million miles
of space,
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until it arrived in a steady orbit
around the Sun,
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from where it looked out
with a fixed and clear gaze,
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to a single patch of sky
in the constellation of Cygnus.
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Exposing its sensitive light meter
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to the light of 150,000 stars,
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it began to look
for Earth-like alien worlds.
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Kepler doesn't detect planets directly.
They are far too small.
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They're just specks of dust
relative to their parent star.
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They're also very faint.
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They don't emit light of their own,
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so they just glow very dimly
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in the reflective ambient light
of their stars.
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So Kepler has
to detect planets indirectly.
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Imagine that a moth just flew
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across the beam of light
from the lighthouse.
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And I wouldn't see the moth.
But if I had a sensitive enough detector
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and everything was lined up properly,
I might just see
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the brightness of the light dim.
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And that is how Kepler detects planets.
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00:14:01,760 --> 00:14:04,800
Imagine there's an alien astronomer
in some distant solar system
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looking back at the Sun,
and everything's lined up
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so they see the Earth trace across
the face of our star.
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They would see
the light from the sun dim
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by one hundredth of one percent.
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It's a tiny amount, but it's enough.
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And if they saw
that dimming was regular,
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if they saw the star dim
once every year in this case,
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then they would infer
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that there's a planet orbiting
around the star.
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With its exquisitely sensitive
light meter,
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Kepler sees only
the regular dimming of pixels.
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Just a few bits of information.
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But from those bits, astronomers can
begin to build a picture
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of the worlds that dim the starlight.
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Worlds that might, in some way,
resemble our own.
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Worlds like Kepler-36b.
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The planet was
one of Kepler's earliest discoveries.
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Orbiting a star similar to our own,
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we'd found a world that at first glance,
might seem familiar.
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Weighing in at around four times
the mass of our own planet,
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Kepler-36b was one of the first
of a new class of planet,
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a Super-Earth.
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The Kepler data doesn't
just allow us to say
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there's a planet around that star.
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It allows us to characterise
those planets.
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So, by looking at the precise way
that the light fades
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and then rises again,
and the timing between the dips,
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we can measure the orbit of the planets.
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And if there are multiple planets
in the system,
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we can even estimate their masses.
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So, the Kepler data allows astronomers
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to paint a picture
of the worlds it discovers.
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But the more detailed our picture
of Kepler-36b became,
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the less Earth-like
this super-Earth appeared to be.
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It orbits very close to its star,
circling once every 14 days.
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And, it has company.
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A gigantic gaseous companion
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with an orbit unusually close
to its smaller sibling.
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The proximity of both its star
and sister planet,
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allows us to imagine
the bizarre conditions
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that may exist
on the surface of Kepler-36b.
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The planet may be tidally-locked,
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which would mean that one hemisphere
always faces the star.
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On this side, the punishing heat could
turn the ground molten,
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creating rivers of lava that would
criss-cross the surface.
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The planet could experience
violent eruptions
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as the gravitational pull
of the gas giant triggers
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intense volcanism,
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each time it passes by.
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But Kepler-36b could
also be a planet of ice.
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Because if it's tidally-locked,
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the far side would face permanently
away from the star.
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And we could imagine
a freezing, cold hemisphere
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shrouded in eternal darkness.
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For now, this is all
Just informed speculation.
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But we are beginning to build
a picture of these worlds.
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I mean, imagine a world
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where the sun stays at the same point
in the sky forever.
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So, one side of the planet is
in eternal night
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and the other side in eternal day.
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And even the twilight strip
between day and night,
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we think, would suffer
from extreme conditions.
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So, Kepler-36b just goes to show
there's so much more
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to having a habitable world
than just the composition of the planet.
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There's the details of its orbit,
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and also the nature of the other objects
in the solar system
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that are orbiting
around the star with it.
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Kepler-36b is just one
of thousands of planets
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that Kepler has discovered.
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We now know beyond doubt
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that our galaxy is home
to a diverse collection of alien worlds.
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Each one of the over 4,000 planets
that we've discovered to date,
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is different from all the others.
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They really are an alien
and exotic bunch,
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and there's certainly no planet
that's identical to the planets
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that we know of in our solar system.
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And I think that reveals a deep truth
about the universe.
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Because although the laws of nature
that form the planets are simple
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and the same everywhere,
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and the fundamental ingredients
out of which the planets are made,
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are simple and the same everywhere,
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the nature of a planet also depends
on the history of its formation,
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and the environment
around its parent star,
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out of which the planet formed.
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And those are all radically different.
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So, each planet has
a different story to tell.
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I suppose in that sense,
planets are like human beings.
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And this wholly unexpected
but exciting discovery
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certainly complicates
the search for life.
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We needed to narrow the search
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for planets further,
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but not too far away
from their parent stars.
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Planets at just the right distance
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for their surfaces
potentially to be habitable.
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Alien worlds
with one precious ingredient
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that makes Earth a living planet.
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00:24:18,280 --> 00:24:22,240
Now, you might legitimately ask
can we transfer all the knowledge
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00:24:22,320 --> 00:24:27,080
we have of life here on earth
to planets elsewhere in the universe?
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00:24:27,160 --> 00:24:30,560
Well, I would answer emphatically
"Yes, we can,”
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because the laws
of nature are universal.
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So, the laws of physics
and chemistry that underpin biology
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here, on this planet,
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will apply to every planet
out there in the universe,
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whether we've discovered it or not.
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00:24:51,520 --> 00:24:54,760
The chemistry of life requires
a few basic ingredients.
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Carbon, nitrogen, oxygen, iron.
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And it also requires a ready supply
of high quality energy
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from heat within the planets
or perhaps from starlight.
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00:25:11,880 --> 00:25:14,040
But life here on earth also requires
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one very important fundamental
extra ingredient, which is liquid water.
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Liquid water is
a deceptively complicated substance.
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It's a very powerful solvent.
But it also has structures
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which are constantly forming
and disappearing within it,
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00:25:30,240 --> 00:25:34,280
which act as a kind of scaffolding
around which biology happens.
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00:25:39,000 --> 00:25:42,440
Organic molecules are
orientated by that scaffolding
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so they can react together.
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00:25:46,400 --> 00:25:49,760
Now, it is certain
that every living thing
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here on Earth requires
liquid water to survive.
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00:25:54,360 --> 00:25:57,200
And I would say it is
a very good assumption
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00:25:57,280 --> 00:26:01,280
that every living thing anywhere
out there in the universe
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00:26:01,360 --> 00:26:03,240
will require it, too.
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00:26:25,080 --> 00:26:27,840
The universe is filled with water.
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00:26:28,960 --> 00:26:32,680
Great reservoirs have been detected
throughout the galaxy,
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amongst the gas clouds of giant nebulae.
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00:26:40,240 --> 00:26:42,480
But just because water is plentiful,
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00:26:43,120 --> 00:26:46,400
that doesn't mean
that it necessarily ends up
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in oceans on planetary surfaces.
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Of the eight planets
in our solar system,
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00:26:59,280 --> 00:27:04,560
only one has liquid water flowing
permanently on its surface today.
250
00:27:10,000 --> 00:27:14,640
An ocean world where,
long ago, life began.
251
00:27:34,240 --> 00:27:37,920
Around four billion years ago,
life on Earth would have begun
252
00:27:38,000 --> 00:27:41,600
probably in places
not dissimilar to this,
253
00:27:41,680 --> 00:27:45,880
where there's geothermal activity,
a source of energy,
254
00:27:45,960 --> 00:27:49,920
in contact with rich concentrations
of reactive chemical elements
255
00:27:50,000 --> 00:27:54,760
and minerals, but also crucially, that.
256
00:27:54,840 --> 00:27:58,160
The magical solvent, liquid water.
257
00:27:58,240 --> 00:28:04,640
Now, many rocky planets out there
in the galaxy will probably have this,
258
00:28:04,720 --> 00:28:08,440
but far fewer, we think, will have that.
259
00:28:08,520 --> 00:28:12,160
Large bodies of liquid water
on the surface.
260
00:28:12,240 --> 00:28:14,480
So, that's why
there's a kind of a catchphrase
261
00:28:14,560 --> 00:28:16,200
in the astro-biology community,
262
00:28:16,320 --> 00:28:19,440
which is if you want to search for life,
263
00:28:20,560 --> 00:28:22,000
follow the water.
264
00:28:35,800 --> 00:28:37,960
Whilst life on Earth was evolving,
265
00:28:45,120 --> 00:28:47,600
124 light years away,
266
00:28:48,640 --> 00:28:52,680
amidst a collapsing cloud
of gas, dust and ice,
267
00:28:57,680 --> 00:28:59,720
a small star was born.
268
00:29:06,520 --> 00:29:10,080
And the cloud's
swirling leftovers condensed
269
00:29:10,160 --> 00:29:12,560
to form a brand new world.
270
00:29:19,640 --> 00:29:24,200
In 2015, Kepler found a planet
orbiting comfortably
271
00:29:24,280 --> 00:29:26,200
within its star's habitable zone.
272
00:29:41,680 --> 00:29:44,440
More than eight times
the mass of the Earth,
273
00:29:44,520 --> 00:29:47,000
K2-18b is a giant,
274
00:29:57,200 --> 00:29:59,960
with a powerful gravitational pull.
275
00:30:10,040 --> 00:30:11,840
If the planet is rocky,
276
00:30:11,920 --> 00:30:15,240
this may have allowed it to hang on
to a thick atmosphere.
277
00:30:18,320 --> 00:30:22,760
K2-18b might have
all the makings of a water world.
278
00:30:28,920 --> 00:30:34,360
And a legendary space telescope had
Kepler's new discovery in its sights.
279
00:30:40,840 --> 00:30:44,200
The most powerful space telescope
of them all
280
00:30:44,280 --> 00:30:45,400
had joined the hunt.
281
00:30:51,640 --> 00:30:56,440
Hubble examined the light
from K2-18b's parent star,
282
00:30:56,520 --> 00:30:58,520
as the planet passed in front of it,
283
00:31:00,840 --> 00:31:05,160
and detected, what may be,
a faint signature...
284
00:31:06,880 --> 00:31:08,360
of water vapour.
285
00:31:13,600 --> 00:31:16,320
124 light years from Earth,
286
00:31:17,760 --> 00:31:21,840
we may have, at last, found
the evidence of water
287
00:31:21,920 --> 00:31:23,600
on an alien world.
288
00:31:25,000 --> 00:31:27,440
This was the first observation
289
00:31:27,520 --> 00:31:29,400
of water vapour in the atmosphere
290
00:31:29,480 --> 00:31:33,800
of a planet orbiting
in the habitable zone around its star.
291
00:31:33,880 --> 00:31:36,360
Now, admittedly, measurements
of the amount of water vapour
292
00:31:36,440 --> 00:31:37,880
in the atmosphere is pretty wide.
293
00:31:37,960 --> 00:31:42,320
It's somewhere between 0.01 percent
and 50 percent.
294
00:31:42,400 --> 00:31:44,560
I mean, this is a planet
that's a long way away.
295
00:31:44,640 --> 00:31:45,920
But, for comparison,
296
00:31:46,000 --> 00:31:51,520
our planet has a few percent
water vapour in its atmosphere.
297
00:31:51,640 --> 00:31:54,240
So, that observation is important
for two reasons.
298
00:31:54,320 --> 00:31:56,480
One is, it is not zero.
299
00:31:56,560 --> 00:31:58,880
There is water vapour in the atmosphere.
300
00:31:58,960 --> 00:32:02,560
But, secondly, if the measurement
is at the lower end,
301
00:32:02,640 --> 00:32:05,440
a few percent of water vapour
in the atmosphere,
302
00:32:05,520 --> 00:32:10,360
then that is consistent
with this world being a planet
303
00:32:10,440 --> 00:32:14,200
with oceans on its surface.
304
00:32:20,160 --> 00:32:22,920
The nature of this planet is
currently the subject
305
00:32:23,000 --> 00:32:25,360
of intense scientific debate.
306
00:32:27,000 --> 00:32:30,120
The planet may be
more like a mini-Neptune,
307
00:32:31,560 --> 00:32:33,160
a gas planet.
308
00:32:36,920 --> 00:32:40,960
But, it is possible to dream
of a rocky alien world
309
00:32:41,040 --> 00:32:43,320
with skies full of clouds,
310
00:32:47,640 --> 00:32:50,240
where water droplets collect,
311
00:32:52,080 --> 00:32:53,680
and eventually fall,
312
00:32:58,720 --> 00:33:00,960
feeding vast oceans...
313
00:33:03,520 --> 00:33:07,680
that cover the surface
of a massive planet.
314
00:33:10,640 --> 00:33:12,280
A water world,
315
00:33:21,040 --> 00:33:23,160
where the elixir of life...
316
00:33:25,000 --> 00:33:26,800
is in plentiful supply.
317
00:33:34,120 --> 00:33:35,840
K218-b is exciting
318
00:33:35,920 --> 00:33:38,360
because it's the smallest world
319
00:33:38,440 --> 00:33:41,000
with an atmosphere
that we've been able to analyse.
320
00:33:41,080 --> 00:33:43,840
And we've found
that its mass and density,
321
00:33:43,920 --> 00:33:45,960
and composition of its atmosphere,
322
00:33:46,040 --> 00:33:50,080
and it's orbit are consistent
with it being a world with water.
323
00:33:51,920 --> 00:33:56,040
And it might be a world
with oceans on its surface.
324
00:33:56,120 --> 00:33:58,200
We don't know for sure,
325
00:33:58,280 --> 00:34:02,360
but just imagine
what that small, faraway world
326
00:34:02,440 --> 00:34:06,080
around a faint red star might be like.
327
00:34:13,560 --> 00:34:16,400
Kepler went on to make
many more discoveries...
328
00:34:28,200 --> 00:34:31,400
until, in October 2018,
329
00:34:31,480 --> 00:34:33,960
it finally ran out of fuel.
330
00:34:40,640 --> 00:34:46,720
After nine years, it had found
over 2500 alien worlds...
331
00:34:53,760 --> 00:34:59,400
showing us just how common
potentially Earth-like planets might be.
332
00:35:12,560 --> 00:35:16,280
We estimate that there may
be around 20 billion
333
00:35:16,360 --> 00:35:18,680
potentially Earth-like worlds,
334
00:35:18,760 --> 00:35:22,320
that's rocky planets
in the habitable zone around a star
335
00:35:22,400 --> 00:35:27,120
that may support liquid water
on the surface, in our galaxy.
336
00:35:27,200 --> 00:35:31,400
That is 20 billion
potential homes for life.
337
00:35:42,160 --> 00:35:44,440
Now, we don't know the probability
338
00:35:44,520 --> 00:35:48,560
that given the right conditions,
life will begin on a planet.
339
00:35:48,960 --> 00:35:51,960
But we do have evidence, from our world.
340
00:35:52,040 --> 00:35:54,160
What we know is that here on Earth,
341
00:35:54,240 --> 00:35:56,960
life began pretty much
as soon as it could
342
00:35:57,040 --> 00:35:59,360
after the Earth had formed
and cooled down,
343
00:35:59,440 --> 00:36:01,920
and the oceans formed on its surface.
344
00:36:02,000 --> 00:36:04,280
So that might suggest
that whilst there isn't
345
00:36:04,360 --> 00:36:06,680
a sense of inevitability
about the origin of life
346
00:36:06,760 --> 00:36:08,360
given the right conditions,
347
00:36:08,440 --> 00:36:12,000
it might, at least,
be reasonably probable.
348
00:36:12,080 --> 00:36:15,040
So, I think that there is
at least a chance
349
00:36:15,120 --> 00:36:19,320
that life may have begun
on some, perhaps many,
350
00:36:19,400 --> 00:36:23,120
of those 20 billion Earth-like worlds
out there in our galaxy.
351
00:36:25,400 --> 00:36:29,400
But I think there are
two questions about life.
352
00:36:29,480 --> 00:36:33,080
One question is about the origin,
and the existence of microbes,
353
00:36:33,160 --> 00:36:35,440
but often, when we speak about aliens,
354
00:36:35,520 --> 00:36:40,480
what we really mean is not microbes,
but complex creatures.
355
00:36:40,560 --> 00:36:44,320
Indeed, things that we can
speak to, civilisations.
356
00:36:44,400 --> 00:36:47,640
What is the probability there will be
other civilisations out there
357
00:36:47,720 --> 00:36:49,000
in the Milky Way?
358
00:36:49,360 --> 00:36:52,800
Well, again, the answer is,
we don't know.
359
00:36:52,880 --> 00:36:55,680
But there are observations we can make.
360
00:36:55,760 --> 00:36:58,640
Patterns we can see in the Milky Way
361
00:36:58,720 --> 00:37:01,920
that might allow us
to make an educated guess.
362
00:37:40,240 --> 00:37:42,200
We don't know precisely
363
00:37:42,280 --> 00:37:46,400
how we highly-intelligent
complex creatures came to be here.
364
00:37:56,560 --> 00:37:58,920
But we do know, for certain,
365
00:37:59,000 --> 00:38:01,440
that life on Earth didn't
begin this way.
366
00:38:04,960 --> 00:38:08,080
We are the product of a story
that has been playing out
367
00:38:08,160 --> 00:38:11,480
for over a quarter
of the age of the Universe.
368
00:38:14,720 --> 00:38:16,280
From microbes...
369
00:38:17,400 --> 00:38:23,000
to a global technological civilisation,
reaching out for others.
370
00:38:24,920 --> 00:38:28,840
For now, at least,
we remain surrounded by silence.
371
00:38:28,920 --> 00:38:32,560
The messages we've sent out
into the cosmos remain unanswered,
372
00:38:32,640 --> 00:38:35,440
and the telescopes we use
to scan the skies
373
00:38:35,520 --> 00:38:38,480
for alien signals remain quiet.
374
00:38:38,560 --> 00:38:40,080
Now, that's not to say, of course,
375
00:38:40,160 --> 00:38:42,680
that there aren't
other civilisations out there.
376
00:38:42,760 --> 00:38:46,720
We may have been looking
for the wrong thing, in the wrong place.
377
00:38:46,840 --> 00:38:51,560
But I think the answer to the question
of the great silence can be found here,
378
00:38:51,640 --> 00:38:52,720
on Earth.
379
00:38:52,800 --> 00:38:56,960
Because, here, it took
four billion years of stability
380
00:38:57,040 --> 00:38:58,600
for a civilisation to emerge.
381
00:38:58,680 --> 00:39:01,320
That is a vast amount of time.
382
00:39:01,400 --> 00:39:04,520
And when we look to the other worlds
out there in the Milky Way,
383
00:39:04,600 --> 00:39:08,560
it's those two things,
stability and time,
384
00:39:08,640 --> 00:39:12,160
that appear to be
very rare commodities indeed.
385
00:39:21,840 --> 00:39:27,080
In 2013, the European Space Agency
launched the Gaia Space Telescope.
386
00:39:30,320 --> 00:39:35,560
Its mission, to survey the stars
of our galaxy, the Milky Way.
387
00:39:37,840 --> 00:39:40,640
Billions of stars have been mapped.
388
00:39:44,920 --> 00:39:49,880
Each star, a potential host
for alien worlds.
389
00:39:54,160 --> 00:39:57,960
And patterns are
already beginning to emerge.
390
00:40:11,960 --> 00:40:14,840
Not all stars exist alone.
391
00:40:20,240 --> 00:40:22,520
Some have company.
392
00:40:30,840 --> 00:40:32,760
And, bizarre as they seem,
393
00:40:32,840 --> 00:40:35,400
Gaia has discovered around a million
394
00:40:35,480 --> 00:40:38,960
of these binary
or multiple star systems.
395
00:40:43,560 --> 00:40:46,120
We've known for a long time
that binary star systems,
396
00:40:46,200 --> 00:40:49,280
and indeed, multiple star systems exist,
397
00:40:49,360 --> 00:40:52,880
but we didn't know
precisely how common they are.
398
00:40:55,040 --> 00:40:58,120
But now, we have
a huge amount of high-precision data,
399
00:40:58,200 --> 00:41:00,760
including the Gaia data, which tells us
400
00:41:00,840 --> 00:41:05,080
that around 50 percent
of all sun-like stars are
401
00:41:05,160 --> 00:41:06,680
in multiple star systems.
402
00:41:06,760 --> 00:41:10,760
And for more massive stars,
that number is 80 percent.
403
00:41:15,640 --> 00:41:20,160
So, how does the prevalence
of multiple star systems in the galaxy
404
00:41:20,240 --> 00:41:23,800
shift the odds in the hunt
for another Earth?
405
00:41:25,880 --> 00:41:30,960
Could Earth-like planets exist
in multiple star systems?
406
00:41:31,040 --> 00:41:34,520
And, if so, what might their fate be?
407
00:41:40,440 --> 00:41:43,880
In 2020, we may have found a clue.
408
00:41:44,920 --> 00:41:50,280
A planet the size of Mars, floating
freely through the galaxy.
409
00:41:52,000 --> 00:41:54,440
A so-called rogue world.
410
00:41:56,360 --> 00:41:59,960
But planets can't form alone
in interstellar space.
411
00:42:00,840 --> 00:42:02,680
So, where did it come from?
412
00:42:19,360 --> 00:42:20,920
Dawn...
413
00:42:28,200 --> 00:42:30,880
ushered in not by one star...
414
00:42:35,560 --> 00:42:36,760
but two.
415
00:42:46,320 --> 00:42:50,280
Perhaps the rogue world grew up
in a close binary system.
416
00:43:04,360 --> 00:43:07,800
Subject to the gravitational pull
of two stars...
417
00:43:15,600 --> 00:43:18,000
its orbit may have been unstable...
418
00:43:26,480 --> 00:43:30,680
as its parent stars fought
to control its destiny.
419
00:43:44,480 --> 00:43:46,920
But, even in single star systems,
420
00:43:47,000 --> 00:43:50,240
the weak gravitational interactions
between the planets
421
00:43:50,320 --> 00:43:51,960
can change their orbits.
422
00:43:52,040 --> 00:43:55,680
Now, in a double star system,
the planets are not only subjected
423
00:43:55,760 --> 00:43:57,960
to the gravitational pulls
of each other,
424
00:43:58,040 --> 00:44:00,840
they're subjected
to the stronger gravitational pull
425
00:44:00,920 --> 00:44:02,560
of another star.
426
00:44:02,640 --> 00:44:06,000
So, even if a planet gets
into a stable orbit,
427
00:44:06,080 --> 00:44:10,440
it's very likely that it won't
stay in that orbit for long.
428
00:44:10,520 --> 00:44:11,840
So, in double star systems,
429
00:44:11,920 --> 00:44:16,440
the line between order
and chaos is very thin indeed.
430
00:44:21,920 --> 00:44:25,040
Even subtle changes
in a planet's orbit can lead
431
00:44:25,120 --> 00:44:27,560
to dramatic changes in climate.
432
00:44:28,600 --> 00:44:33,680
And that's why the surface conditions
on planets in double star systems may
433
00:44:33,760 --> 00:44:37,920
be unlikely to remain
stable enough for long enough
434
00:44:38,000 --> 00:44:40,520
for intelligent life to evolve.
435
00:44:48,680 --> 00:44:51,640
And the changes
in the orbits of planets can
436
00:44:51,720 --> 00:44:55,480
sometimes be anything but subtle.
437
00:45:14,640 --> 00:45:16,760
A close encounter...
438
00:45:18,840 --> 00:45:22,920
may have given the rogue world
a final gravitational Kick...
439
00:45:43,840 --> 00:45:45,600
flinging it outwards...
440
00:45:49,480 --> 00:45:53,600
and releasing it
from the grip of its parent stars,
441
00:45:59,280 --> 00:46:01,200
setting it loose...
442
00:46:06,600 --> 00:46:09,080
on a journey through the galaxy.
443
00:46:24,080 --> 00:46:26,640
Far from the warmth of its stars,
444
00:46:28,240 --> 00:46:32,320
any liquid water the rogue world
might once have had...
445
00:46:36,840 --> 00:46:38,520
Would have frozen solid.
446
00:46:44,000 --> 00:46:47,040
Any atmosphere that once protected it...
447
00:46:55,000 --> 00:46:58,320
would have frozen out onto the surface.
448
00:47:02,360 --> 00:47:04,760
The rogue would have become a world...
449
00:47:07,400 --> 00:47:12,240
with conditions
that no living thing could endure.
450
00:47:15,160 --> 00:47:19,440
An entire planet alone and adrift,
451
00:47:26,280 --> 00:47:31,080
only to be detected by us,
millions of years later.
452
00:47:32,920 --> 00:47:36,560
A small Earth-like rogue planet...
453
00:47:38,360 --> 00:47:40,760
roaming the darkness of space
454
00:47:41,560 --> 00:47:43,040
for eternity.
455
00:47:53,840 --> 00:47:57,920
This lonely, wandering planet is
not a unique world.
456
00:47:58,000 --> 00:48:00,320
Although rogue planets are
very difficult to detect,
457
00:48:00,400 --> 00:48:05,360
it's estimated that there may be
over 100 billion of them in our galaxy.
458
00:48:05,440 --> 00:48:08,600
Rogue planets might be
the most common type of planet
459
00:48:08,680 --> 00:48:09,680
in the Milky Way.
460
00:48:11,080 --> 00:48:13,080
And, although we think
most of them were torn away
461
00:48:13,160 --> 00:48:15,880
from their star soon after formation,
462
00:48:16,480 --> 00:48:21,240
this does suggest that star systems are
not always stable places,
463
00:48:21,320 --> 00:48:25,120
where complex life could evolve
over billions of years.
464
00:48:37,680 --> 00:48:41,400
Our hunt for another living planet has
only just begun.
465
00:48:45,400 --> 00:48:47,880
Yet, we've already learnt so much.
466
00:48:54,920 --> 00:48:57,920
We found our first rocky worlds.
467
00:49:00,040 --> 00:49:03,880
Some in the habitable zone
around their stars.
468
00:49:12,240 --> 00:49:17,440
Some, potentially,
with liquid water on the surface.
469
00:49:18,760 --> 00:49:23,880
Candidate worlds for future missions
to search for evidence of life.
470
00:49:29,080 --> 00:49:33,280
But we've also found hordes
of bizarre, tortured worlds,
471
00:49:35,760 --> 00:49:38,000
orbiting around violent stars,
472
00:49:46,600 --> 00:49:49,600
and a multitude of rogue planets...
473
00:49:51,560 --> 00:49:56,200
where complex life,
as we understand it seems impossible.
474
00:50:04,640 --> 00:50:08,920
Perhaps it's these worlds
that hint at the reason why,
475
00:50:10,560 --> 00:50:14,440
for now, one planet stands apart...
476
00:50:20,160 --> 00:50:21,440
alone.
477
00:50:34,160 --> 00:50:37,560
Our planet seems to have
largely escaped the violence,
478
00:50:37,640 --> 00:50:40,000
the chaos, and the constant change
479
00:50:40,080 --> 00:50:42,720
that seems to characterise
a galaxy like the Milky Way.
480
00:50:43,320 --> 00:50:46,160
Yes, there's been
the odd mass extinction,
481
00:50:46,240 --> 00:50:49,360
but there's been
an unbroken chain of life here on Earth,
482
00:50:49,440 --> 00:50:52,440
stretching back four billion years.
483
00:50:52,520 --> 00:50:54,040
And if that's what you need
484
00:50:54,120 --> 00:50:57,000
to go from the origin of life
to a civilisation,
485
00:50:57,080 --> 00:51:01,440
then, although there may be billions
of worlds out there where life began,
486
00:51:01,520 --> 00:51:04,880
there may be very few civilisations.
487
00:51:04,960 --> 00:51:09,480
But that's just an opinion.
It's an educated guess.
488
00:51:09,560 --> 00:51:12,240
And, given the profound nature
of the question,
489
00:51:12,320 --> 00:51:15,240
no matter how educated the guess,
490
00:51:15,320 --> 00:51:18,800
I think it would be ridiculous
for us to stop looking
491
00:51:18,880 --> 00:51:22,360
both inside our galaxy and beyond.
492
00:51:25,720 --> 00:51:29,080
For, we may have just received
the first glimpse...
493
00:51:30,440 --> 00:51:33,600
of a world beyond the Milky Way...
494
00:51:41,760 --> 00:51:44,760
around 30 million light years away,
495
00:51:44,880 --> 00:51:48,960
nestled in the spiral arms
of the Whirlpool Galaxy.
496
00:51:53,560 --> 00:51:56,120
A world the size of Saturn.
497
00:52:04,600 --> 00:52:08,040
A find that marks
an expansion of our horizons.
498
00:52:13,200 --> 00:52:17,440
The beginning of the hunt
for extra-galactic planets.
499
00:52:21,120 --> 00:52:24,480
The potential discovery
of a planet orbiting around a star,
500
00:52:24,560 --> 00:52:28,600
in another galaxy is something
that I never thought I'd see.
501
00:52:28,680 --> 00:52:31,560
And it opens up
the intriguing possibility
502
00:52:31,640 --> 00:52:34,160
that we might be able to explore
not only the question,
503
00:52:34,240 --> 00:52:39,040
"Are we alone in our galaxy?"
but, "Are we alone in the universe?"”
504
00:52:42,240 --> 00:52:46,960
And the answer to that question
may lie far in the future.
505
00:52:47,040 --> 00:52:49,520
We might never answer that question.
506
00:52:49,600 --> 00:52:53,840
But I said, the question
"Are we alone?" is profound,
507
00:52:53,920 --> 00:52:55,720
because answering it would teach us
508
00:52:55,800 --> 00:52:58,640
much more
about what it means to be human.
509
00:53:02,760 --> 00:53:06,120
Well, I think we become
a little bit more human
510
00:53:06,200 --> 00:53:08,920
with every world that we explore,
511
00:53:09,000 --> 00:53:12,800
because that ability
to lay the foundations,
512
00:53:12,880 --> 00:53:17,840
to explore questions to which we may
never receive answers in our lifetime,
513
00:53:17,920 --> 00:53:21,800
questions for our children
or our grandchildren to answer,
514
00:53:21,880 --> 00:53:25,360
Is a fundamental part
of what it means to be human.
515
00:53:25,440 --> 00:53:30,080
It's a fundamental part
of what makes us so special,
516
00:53:30,160 --> 00:53:32,560
here on this little world,
517
00:53:32,640 --> 00:53:37,760
looking up at the stars,
whether we're alone or not.
518
00:53:53,960 --> 00:53:58,440
Five. Four. Three. Two.
519
00:53:58,520 --> 00:54:00,520
Engines start. One. Zero.
520
00:54:00,600 --> 00:54:04,000
And, lift off
of the Delta II rocket with Kepler,
521
00:54:04,080 --> 00:54:05,760
on a search for planets,
522
00:54:05,840 --> 00:54:09,400
in some way, like our own.
523
00:54:09,480 --> 00:54:12,360
We had worked together, thousands
of people worked together,
524
00:54:12,440 --> 00:54:14,880
and it's all coming together.
525
00:54:15,960 --> 00:54:17,520
And we have separation.
526
00:54:19,200 --> 00:54:22,120
It was so emotional to see
the project they had worked on
527
00:54:22,200 --> 00:54:25,400
for so many years or decades
finally go to space,
528
00:54:25,480 --> 00:54:29,440
and all that hope and promise,
all bundled up in the machinery.
529
00:54:37,080 --> 00:54:39,440
Kepler was an immediate success,
530
00:54:39,520 --> 00:54:44,280
discovering over 2,000 new planets
in its first four years of operation.
531
00:54:50,160 --> 00:54:52,360
But in the summer of 2012,
532
00:54:52,440 --> 00:54:55,840
the team faced a challenge
that threatened the entire mission.
533
00:55:00,000 --> 00:55:02,560
One of the things that
the Kepler Mission needs to operate
534
00:55:02,640 --> 00:55:04,960
are reaction wheels
that spin and hold it on target.
535
00:55:07,600 --> 00:55:11,200
So, it always points
at the same stars, and doesn't jiggle.
536
00:55:11,280 --> 00:55:13,200
Well, we had four wheels that did that.
537
00:55:15,400 --> 00:55:18,360
And we knew that we only
had a couple of spare gyroscopes,
538
00:55:18,440 --> 00:55:22,200
and we knew that spacecraft tend
to have gyros fail.
539
00:55:27,080 --> 00:55:28,920
And, after a while, it failed.
540
00:55:29,000 --> 00:55:31,520
Three months later,
the second one failed.
541
00:55:31,600 --> 00:55:32,800
And, since we needed three,
542
00:55:32,880 --> 00:55:36,160
we could no longer look
at the Kepler field of view.
543
00:55:38,800 --> 00:55:41,880
I had hope that they'll figure out
a way to work with two gyros,
544
00:55:41,960 --> 00:55:43,240
and, indeed, they did.
545
00:55:47,560 --> 00:55:50,920
So, the very clever people,
the engineers and scientists said,
546
00:55:51,000 --> 00:55:55,680
"What we can use, is we'll use
the sunshine for the third wheel.
547
00:55:55,760 --> 00:55:58,000
"We'll make this thing
reflect sunlight off it,
548
00:55:58,080 --> 00:56:01,000
"we'll use the other two wheels,
and now, we can point in the sky.”
549
00:56:03,880 --> 00:56:08,600
The faint pressure of sunlight
helped stabilise the telescope.
550
00:56:09,080 --> 00:56:11,080
That was, kind of,
good news, actually,
551
00:56:11,160 --> 00:56:15,080
because it meant Kepler was gonna
have to go off the Kepler field now,
552
00:56:15,160 --> 00:56:18,520
and we could get all kinds
of other stars and observe them,
553
00:56:18,600 --> 00:56:21,720
and so, it actually was a boon
for stellar astronomy.
554
00:56:24,360 --> 00:56:27,200
After another four years
of discoveries,
555
00:56:27,280 --> 00:56:32,120
in total it had found
over 2,600 planets,
556
00:56:32,200 --> 00:56:37,080
making it, by far, our most successful
planet-hunter to date.
557
00:56:40,040 --> 00:56:44,040
It was sad when they sent
the command to shut everything down.
558
00:56:44,120 --> 00:56:45,760
You know, it's asleep now.
559
00:56:45,840 --> 00:56:49,720
It's in orbit around the sun.
It will continue that orbit.
560
00:56:49,800 --> 00:56:52,880
But since it launched from Earth,
it will come back to Earth.
561
00:56:52,960 --> 00:56:56,720
It will come and visit us again
in about 40 years,
562
00:56:56,800 --> 00:56:58,960
and my hope is people will say,
563
00:56:59,040 --> 00:57:02,600
"This is a historic telescope.
It told us about all these planets”,
564
00:57:02,680 --> 00:57:05,080
and they will go up
and pick up this telescope
565
00:57:05,160 --> 00:57:06,280
and bring it back to Earth,
566
00:57:06,360 --> 00:57:10,440
and put in the Air and Space Museum
for us all to admire.
47263
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