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Why do we humans have such a
connection to the night sky?

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The twinkling lights that seem like
oases out there and yet we're not
sure. Are there habitable worlds?

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Around the world there are a
group of highly intelligent,

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highly trained scientists
that share a surprising belief.

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There are a couple of hundred
billion stars just in our galaxy and

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at least half of them probably have
planets. That's 100 billion
planetary systems.

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How many planets in each system?
let's say five.

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That's a half trillion,
500 billion planets out there.

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Keep in mind, there are 100 billion
other galaxies!

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For these scientists the
vastness of our universe
can mean just one thing -

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the existence of life.

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So to think, "Look, man.
This is the only place where
anything interesting's happening",

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you've gotta be really audacious
to take that point of view.

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But proving it has not
been quite so simple.

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I have conducted many, many
searches, none of which
have produced a discovery.

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Until now.

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In our local neighbourhood, just
200 trillion kilometres from Earth,

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is a planet that we
might find rather familiar.

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The discovery of Gliese 581c
is a marvellous discovery.

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It shows how close we're getting to
planets that remind us of the Earth.

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Occasionally you're sitting on a
plane and they guy next to you says,
"What do you do for a living?".

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"I look for aliens".
I explain a little bit, and almost
every one everyone is interested.

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Nobody says, "That's nice.
I'll go back to my magazine now".

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In the desert, 300 miles north of
San Francisco, Dr Seth Shostak is
waiting for a message from an alien.

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This is SETI,
the front-line in the search for
extra-terrestrial intelligence.

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If a message ever comes our way,
this is where it will be received.

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Anybody who can build a transmitter
can send messages between the stars.

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If we can do that,
maybe they can do it.

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Here we are, the Allen Telescope
Array, - designed to do one thing -

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eavesdrop on any signals that
might be being broadcast our way by
some alien civilisation.

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This vast array of telescopes
is the latest in a long line

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of experiments designed to
eavesdrop on our nearest neighbours.

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As chief astronomer of the project,
Shostak is more confident than most

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that he'll be on the receiving
end of a close encounter.

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There are 42 antennae here now,
you can count them up.

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But eventually the idea is to have
350 and then this thing

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will be able to scan
big chunks of the sky,

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simultaneously observing five, six,
maybe more stars at a time, looking

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for the signal that somebody's out
there, trying to get our attention.

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It's the most powerful experiment
humans have ever attempted -

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to discover if intelligent life
is the exception or the rule
in the cosmos.

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But although it's early days
for Shostak and his team,
the omens are not good.

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The SETI project has been
casting its ear out to the
universe for over 50 years.

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For the founding father of
the search, Dr Frank Drake,
the dream has never changed.

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Back in the 1950s, there were many
scientists interested in ET life,

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but we were well aware that
there were no means even to detect

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planets, let alone microbes,

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or any sign
of non-intelligent life.

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In fact, the only thing open
to us was radio transmissions
from intelligent civilisations.

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Drake was the first scientist to
believe that technology could
answer the biggest question of all.

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Despite widespread scepticism,

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he believed that if there were
intelligent life forms out there

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then the least we could do
is to try and listen to any radio
signals they may be sending out.

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In 1960, we conducted a search for
radio signals from the two nearest

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stars to the Earth that are like
the Sun - Tau Ceti
and Epsilon Eridani.

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But to no-one's surprise,
the search failed.

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We searched for two months.
We didn't find anything.

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And that's actually an important
result, because it showed not every
star in the sky was radiating.

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It also demonstrated that a search
was likely to be a very long
and difficult one.

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Despite putting on a brave face,
Drake and his ideas remained on
the very fringes of astronomy.

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Listening for aliens
just wasn't science.

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Congress people would see that
they could get publicity by

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attacking this project as a
waste of tax-payers' money.

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Using tax-payers' money to search
for little green men was a
common theme.

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So Drake would have to wait for
another generation of scientists

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to bring alien-hunting
in from the cold.

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Being an astronomer is a
bit sacrificial.

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My wife is at home and she misses me.

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I call her up and she says,
"When are you coming home?"

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It's another four, five
nights, I have to tell her.

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Professor Geoff Marcy is a planet
hunter, an explorer of alien worlds.

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Staying up all night means
you don't get much sleep.

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So it's a bit of a sacrifice, but
I wouldn't give it up for anything.
It's such a treasure.

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For the last ten years,
Marcy has come here to

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use the planet's largest telescope
in the hope of finding other worlds.

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The Keck Telescope high up on
Mauna Kea, Hawaii is about as close
as you can get to the stars.

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It's the world's largest, because the
collecting area of the mirror
is the largest in the world.

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The mirror is ten metres across,

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1/10 the length of a football field,
all to collect the starlight

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coming from hundreds or
thousands of light years away.

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But even using the
mighty Keck telescope,

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Pluto, at the edge
of our solar system, is a colossal
4½ billion kilometres away.

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And this is the best image
astronomers have achieved.

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And yet Marcy wanted to look
beyond our solar system,

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to find the hypothetical worlds
that astronomers call exoplanets,
which lie around other stars.

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Like our nearest star,
Proxima Centauri,

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a staggering 40 trillion kilometres
away, or four light years.

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Beyond lies the rest of our
galaxy - an unimaginable
100,000 light years across.

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It's our local neighbourhood
of 200 billion stars.

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Astronomers knew there had
to be planets out there.

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We saw young stars with
proto-planetary disks of gas and dust

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around them, surely making planets.

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But we couldn't detect the planets.

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And the reason is that even with the
largest telescope, like this one,

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the mighty Keck, the planets were
lost in the glare of the host stars.

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The problem is that compared
to the light of a star,

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the reflected light from an
exoplanet is all but invisible.

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The star burns a billion
times more brightly.

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Indeed, even with the Hubble
space telescope, we can't detect
planets directly around nearby stars.

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Using direct observational methods,
astronomers were confined within our
own solar system,

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unable to prove even the existence
of exoplanets, let alone life.

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So how do you look for
something you can't see?

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The answer was first proposed in
an obscure paper published in 1952,

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by a Russia astronomer called
Otto Struve.

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Struve theorised that even
though the planets themselves

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were invisible, there was still
a way of unlocking their secrets.

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He knew that each planet was
held in orbit around its star
by an immense gravitational force.

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This force works in two directions.

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The star pulls on the planet but the
planet also pulls back on the star,

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making the star move
with the minutest wobble.

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It's not much, but this wobble is
just big enough

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to make it theoretically detectable
back here on Earth.

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If you have the right technology.

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The real tipping point was not in the
telescopes, we've had big telescopes
for several decades.

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The tipping point was having digital
detectors, like the digital cameras

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that most of us enjoy, with the CCD
light detectors at their backs -
and computers.

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Let's see what kind of a
night we're gonna have here.

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Marcy script underscore
ETA underscore Earth.

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Great. First object on the list...

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Why don't you go ahead
and open the dome slit?

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We're observing 80 stars, night
after night, with one key goal, and
that's to detect Earth-like planets.

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Since the early 1990s, planet
hunters like Marcy have been gazing
to the stars for the tiniest wobble

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that could signal the

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The theory seemed correct.

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They had the right technology,
and yet after years of searching,
the exoplanets were still missing.

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We were confronted
with a contradiction.

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On the one hand, it appeared
that young stars had the right
kind of planet building material,

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but on the other hand,
humanity had failed to find any.

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All the planet hunters had to
keep them going was their faith.

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And the belief of the one man
who has never given up hope.

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It occurred to me, we need to
know how often does life arise,
how often does intelligence arise.

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I recognised that all you had to do
was multiply these factors together

133
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and you have a very prime important
equation, of basic interest,

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because it tells us how many
civilisations there are out there.

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Without any hard evidence,
back in 1960, Frank Drake went

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00:13:27,320 --> 00:13:32,444
about creating an equation
that would answer the big question
once and for all.

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00:13:32,479 --> 00:13:39,639
We have an equation which gives
us N, the number of detectable
civilisations in our galaxy.

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It's based on what we know of
the history of our galaxy

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and particularly the history of our
solar system and of life on Earth.

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The equation defines
all the necessary ingredients for
intelligent life to arise.

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There are seven
factors in the equation.

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Since life needs a home,
it begins with a known observation.

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00:14:02,594 --> 00:14:04,799
For the rate of star
formation, we know that very well.

144
00:14:04,834 --> 00:14:07,605
It's about 20 stars per year.

145
00:14:07,640 --> 00:14:11,724
For the fraction of planets, we
didn't used to know that at all.

146
00:14:11,759 --> 00:14:16,405
Everything else in the equation,
from the number of stars
with planets

147
00:14:16,440 --> 00:14:22,119
to the number of planets
per star capable of supporting life,
was a total mystery.

148
00:14:22,154 --> 00:14:26,760
But over the years, it hasn't
stopped people from guessing.

149
00:14:26,795 --> 00:14:30,004
This is our number N.

150
00:14:30,039 --> 00:14:34,324
The number of technical
civilisations in the galaxy.

151
00:14:34,359 --> 00:14:40,179
Into the now famous, or infamous,
Drake equation goes everything,
from astrophysics, through

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00:14:40,214 --> 00:14:45,999
evolutionary biology to whatever
it is that governs the lifetime
of a detectable civilisation.

153
00:14:46,034 --> 00:14:50,439
Not surprisingly, no-one's solved
it yet, but anyone can have a go.

154
00:14:50,474 --> 00:14:52,719
It's almost a game the
whole family can play.

155
00:14:55,760 --> 00:14:59,579
If you sort of take
the average of people's guesses,

156
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it gives you a total number
of detectable civilisations,

157
00:15:03,434 --> 00:15:05,200
which is about 10,000.

158
00:15:07,240 --> 00:15:08,720
A big number.

159
00:15:10,919 --> 00:15:17,760
And yet with no call from ET, and
no sign of another Earth, Drake's
guess seemed wildly optimistic.

160
00:15:36,119 --> 00:15:40,404
When I was a child, I was living in

161
00:15:40,439 --> 00:15:46,360
We spent evenings
with my sister laying down on the
grass and looking at the sky.

162
00:15:46,395 --> 00:15:49,839
And that's really good
for the imagination.

163
00:15:51,640 --> 00:15:56,439
I'm sure there are other
Earths similar to our own Earth.

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00:15:56,474 --> 00:16:01,239
And on some of them, you
even may have life developing.

165
00:16:02,999 --> 00:16:07,019
Professor Stephane Udry is part of
a Swiss team of planet hunters

166
00:16:07,054 --> 00:16:11,039
who began searching for life-bearing
planets in the mid-'90s.

167
00:16:14,559 --> 00:16:16,965
They had developed a new planet
detector,

168
00:16:17,000 --> 00:16:21,080
which had just been installed at
their observatory in central France.

169
00:16:21,115 --> 00:16:23,124
When you have a new instrument,

170
00:16:23,159 --> 00:16:27,240
you want to check the short-term
precision of the instrument.

171
00:16:29,559 --> 00:16:34,245
Tests of their new detector where
scheduled to last a few weeks.

172
00:16:34,280 --> 00:16:39,159
Among their target stars was
one similar to our own sun,
called Pegasi 51.

173
00:16:40,760 --> 00:16:46,079
The light from Peg 51
should remain constant,
but there seemed to be a problem.

174
00:16:48,360 --> 00:16:49,884
The star...

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00:16:49,919 --> 00:16:52,040
appeared to be wobbling.

176
00:16:54,200 --> 00:17:01,520
The thinking was, "Oh, that should
be some crazy effect of the star
that could explain the observations".

177
00:17:03,399 --> 00:17:10,239
They tried to reject, one after the
other, all the possible explanations.

178
00:17:10,274 --> 00:17:14,719
And at the end, the best explanation
was the presence of a planet.

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00:17:18,519 --> 00:17:21,525
With ingenuity and
a little bit of luck,

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00:17:21,560 --> 00:17:26,079
the Swiss had discovered the first
planet outside our solar system.

181
00:17:28,919 --> 00:17:35,559
It was massive,
half the mass of Jupiter, but in a
rapid orbit lasting only four days.

182
00:17:37,160 --> 00:17:43,200
The planet was so close to its star,
that surface temperatures
exceed 1,000 degrees Centigrade.

183
00:17:50,759 --> 00:17:55,119
Being part of these teams
finding planets around other stars

184
00:17:55,154 --> 00:17:57,445
is very exciting in that sense.

185
00:17:57,480 --> 00:18:02,360
That's really a new
domain that is opening in science.

186
00:18:04,239 --> 00:18:08,319
The discovery of this planet
opened the flood gates.

187
00:18:08,354 --> 00:18:12,176
Hundreds of exoplanets
have since been discovered,

188
00:18:12,211 --> 00:18:15,999
but none of them have
proved suitable for life.

189
00:18:25,480 --> 00:18:31,079
My favourite planet
is a little planet that orbits
the star Gliese 756.

190
00:18:31,114 --> 00:18:33,880
My favourite
planetary system is called 55 Cancri.

191
00:18:34,000 --> 00:18:34,045
My favourite
planetary system is called 55 Cancri.

192
00:18:34,080 --> 00:18:37,599
There are two planets which I have
an emotional attachment to.

193
00:18:37,634 --> 00:18:39,684
It has an orbit of two days.

194
00:18:39,719 --> 00:18:41,884
The planets of the star Tau Ceti.

195
00:18:41,919 --> 00:18:44,319
That means
its seasons occur in two days.

196
00:18:44,354 --> 00:18:46,365
And the star Epsilon Eridani.

197
00:18:46,400 --> 00:18:49,284
So summer-winter would alternate
in two days.

198
00:18:49,319 --> 00:18:53,440
It's like the solar system because
it's a planet like Jupiter
on a Jupiter-like orbit.

199
00:18:53,475 --> 00:18:55,845
Those stars were my targets

200
00:18:55,880 --> 00:19:01,080
when I first searched for the first
evidence of extra terrestrial life
in 1960.

201
00:19:01,115 --> 00:19:04,879
It's unlike the solar system because
it has three other planets that are

202
00:19:04,914 --> 00:19:07,720
very close into the star,
hot Jupiter-type planets.

203
00:19:09,800 --> 00:19:15,080
In the last decade, astronomers
have found over 260 exoplanets,

204
00:19:15,115 --> 00:19:18,279
most of them searingly hot
gas-giants.

205
00:19:19,920 --> 00:19:23,725
As a biologist, I don't really have
a favourite exoplanet at the moment,

206
00:19:23,760 --> 00:19:27,999
because the astronomers keep
finding me hot Jupiters and they
don't do much good for biology.

207
00:19:28,034 --> 00:19:30,836
What I'm looking for is
something really Earth-like.

208
00:19:30,871 --> 00:19:33,639
Something that's got a
good chance of liquid water.

209
00:19:33,674 --> 00:19:35,320
And then I'll have a favourite.

210
00:19:40,719 --> 00:19:43,960
So just how rare is our blue planet?

211
00:19:47,879 --> 00:19:52,599
Dr Lynn Rothschild is an
astrobiologist who has studied our
own solar system

212
00:19:52,634 --> 00:19:55,999
in an effort to understand
what makes Earth so special.

213
00:19:58,879 --> 00:20:03,519
Let's pretend that this fire here is
our sun and that this rock is Venus.

214
00:20:03,554 --> 00:20:08,160
It's about as close to the sun you
can get and still have liquid water.

215
00:20:08,195 --> 00:20:11,760
So the orbit of Venus
would be, say, like this.

216
00:20:13,879 --> 00:20:18,320
This is getting pretty hot, cos
I'm awfully close to the sun here.

217
00:20:20,679 --> 00:20:24,840
Now on the other extreme, this is
Mars, which is the farthest planet

218
00:20:24,875 --> 00:20:27,877
from the sun that has any chance
of liquid water.

219
00:20:27,912 --> 00:20:30,844
There's no liquid surface
water today, but we know

220
00:20:30,879 --> 00:20:34,320
that there used to be in the past.
So let's trace the orbit of Mars.

221
00:20:37,440 --> 00:20:42,520
Now right between these two circles,
where the orbit of Mars would be

222
00:20:42,555 --> 00:20:47,005
and the orbit of Venus,
this is where liquid water is stable.

223
00:20:47,040 --> 00:20:50,959
And right in this habitable zone
in our solar system is planet Earth.

224
00:20:50,994 --> 00:20:53,960
Our beautiful watery world
that's just covered with life.

225
00:21:00,220 --> 00:21:02,924
Just 10% closer in,

226
00:21:02,959 --> 00:21:04,720
and Earth would no longer be capable

227
00:21:04,755 --> 00:21:07,519
of supporting liquid water.

228
00:21:15,120 --> 00:21:20,040
Almost miraculously,
Earth slots right into the
heart of the habitable zone.

229
00:21:25,280 --> 00:21:30,639
Giving this once lifeless rock
just the right elements for
life to take hold and flourish.

230
00:21:41,119 --> 00:21:45,079
Over billions of years,
microbes, plants and animals

231
00:21:45,114 --> 00:21:49,040
have transformed Earth into
a living, breathing world.

232
00:21:56,199 --> 00:21:59,085
A world where one evolutionary line

233
00:21:59,120 --> 00:22:02,959
has led to modern humankind
and civilisation.

234
00:22:11,720 --> 00:22:15,659
But even with our civilisation's
most advanced technology,

235
00:22:15,694 --> 00:22:19,599
finding other planets like Earth
has proved impossible.

236
00:22:21,759 --> 00:22:26,044
Rotator is vertical, angle mode zero.

237
00:22:26,079 --> 00:22:31,519
The very factors that enable life, a
small planet at a safe distance from

238
00:22:31,554 --> 00:22:37,417
the sun, means the telltale wobbles
that these planets produce are tiny.

239
00:22:37,452 --> 00:22:42,985
Our Earth, when it orbits the sun,
causes our sun to wobble with a speed

240
00:22:43,020 --> 00:22:48,519
of 1/10th of one metre per second,
a smaller motion than we can detect.

241
00:22:50,879 --> 00:22:56,919
Or there could be another, more
profound explanation for the
missing Earth-like planets.

242
00:22:58,479 --> 00:23:03,045
It's possible that other stars
didn't have planets around them.

243
00:23:03,080 --> 00:23:07,719
That we're just one of the
freaks of nature that grew
up on a rocky planet.

244
00:23:09,479 --> 00:23:14,399
Either way, despite
decades of searching, until 2007,

245
00:23:14,434 --> 00:23:17,319
Earth remained entirely alone.

246
00:23:31,040 --> 00:23:38,720
Between the Andes mountains and
the Pacific Ocean, on the remote
southern edge of the Atacama desert

247
00:23:38,755 --> 00:23:43,400
lies one of the most extraordinary
observatories on Earth.

248
00:23:47,600 --> 00:23:50,484
The high elevation
and the low rainfall,

249
00:23:50,519 --> 00:23:57,000
just one millimetre a year, makes it
the perfect place for uninterrupted
views of the southern night sky.

250
00:23:57,035 --> 00:24:00,159
Please come in, I have
something to show you in here.

251
00:24:03,920 --> 00:24:11,199
Professor Stephane Udry is the proud
owner of a machine which could
change the course of human history.

252
00:24:11,234 --> 00:24:16,485
Inside this big box is an enclosure
and inside there is a vacuum tank

253
00:24:16,520 --> 00:24:21,765
with the instrument,
that is the most sensitive in the
world now for planet detection.

254
00:24:21,800 --> 00:24:29,879
With this instrument we can detect
low mass planet five, ten times
the mass of the Earth. Can we go in?

255
00:24:29,914 --> 00:24:36,405
No. Of course not, because just
opening the door will destroy
the measurement for a few days.

256
00:24:36,440 --> 00:24:44,440
Because we need to have a very stable
instrument to be able to repeat the
measurement with the same precision,

257
00:24:44,475 --> 00:24:47,559
day after day,
month after month, years after years.

258
00:24:53,640 --> 00:24:56,799
And that's exactly
what they've been doing.

259
00:24:59,240 --> 00:25:04,680
They drew up a list of a thousand
targets taken from the Gliese
Catalogue of Nearby Stars

260
00:25:04,715 --> 00:25:07,204
and began measuring and
re-measuring each candidate,

261
00:25:07,239 --> 00:25:12,479
hunting for wobbles that had
previously been too small to detect.

262
00:25:23,559 --> 00:25:27,804
But one star
caught Stephane's attention.

263
00:25:27,839 --> 00:25:33,964
Gliese 581 was in our
target list since the beginning.

264
00:25:33,999 --> 00:25:41,200
Categorised as Gliese 581a,
it's a red dwarf star,
a third of the mass of our own sun.

265
00:25:45,200 --> 00:25:52,520
When the wobble was plotted
it revealed 581b, a massive
planet the size of Neptune,

266
00:25:52,555 --> 00:25:54,684
close into the star

267
00:25:54,719 --> 00:25:58,559
and orbiting once every 5½ days.

268
00:25:58,594 --> 00:26:00,525
It was no Earth,

269
00:26:00,560 --> 00:26:05,240
but the star's wobble held some fine
detail that intrigued Stephane.

270
00:26:06,960 --> 00:26:10,765
We noticed that there was
something else in the system.

271
00:26:10,800 --> 00:26:16,165
There seemed to another, smaller
planet lurking in the detail.

272
00:26:16,200 --> 00:26:23,685
That something else
could be a five Earth
mass planet very close to the star.

273
00:26:23,720 --> 00:26:31,119
If Stephan's hunch was right,
it would be the smallest planet
ever detected around a distant sun.

274
00:26:31,154 --> 00:26:33,559
And this planet
seemed to be habitable.

275
00:26:35,199 --> 00:26:41,000
We got excited because the distance
was just right for the planet to
possibly be in the habitable zone.

276
00:26:46,520 --> 00:26:49,605
After years of hunting, the search

277
00:26:49,640 --> 00:26:52,924
for the first "Second Earth"
was over.

278
00:26:52,959 --> 00:26:56,559
European astronomers have spotted
a new planet outside our solar system

279
00:26:56,594 --> 00:26:58,725
which closely resembles
the planet Earth.

280
00:26:58,760 --> 00:27:02,280
The probability that there
is life somewhere else in
the Universe goes up a bit.

281
00:27:02,315 --> 00:27:06,120
This latest find has
set the world of astronomy alight.

282
00:27:14,239 --> 00:27:17,319
For the Swiss team,
the breakthrough was a triumph.

283
00:27:22,199 --> 00:27:26,919
It is always very exciting
to be the first one to know.

284
00:27:26,954 --> 00:27:31,605
The discovery of Gliese 581c
is a marvellous discovery.

285
00:27:31,640 --> 00:27:36,200
It shows how
close we are were getting to
planets that remind us of the Earth.

286
00:27:36,235 --> 00:27:39,804
It shows that potential
life-bearing planets exist.

287
00:27:39,839 --> 00:27:44,600
When you know, when you realise it,
and you are the only one,
it's like being in the spaceship

288
00:27:44,635 --> 00:27:48,519
coming to a planet and being the
first one to see the landscape.

289
00:27:50,559 --> 00:27:54,759
For those tempted to make
the journey, pick a clear night

290
00:27:54,794 --> 00:27:57,719
and look for the constellation
Libra.

291
00:27:57,754 --> 00:27:59,644
Invisible to the naked eye,

292
00:27:59,679 --> 00:28:04,760
Gliese 581 lies just north of the
brightest star in the constellation.

293
00:28:08,640 --> 00:28:14,360
Remarkably, it's one of our
closest neighbours,
a shade over 20 light years distant.

294
00:28:17,360 --> 00:28:20,565
At the heart of the
system is the parent star.

295
00:28:20,600 --> 00:28:28,239
Close by is 581b,
16 times more massive than Earth and
too hot for life to survive.

296
00:28:30,080 --> 00:28:34,760
Beyond, just on the inner warm
edge of the habitable zone,

297
00:28:34,795 --> 00:28:38,404
lies Gliese 581c -

298
00:28:38,439 --> 00:28:43,000
the smallest and most
Earth-like exoplanet yet detected.

299
00:28:54,800 --> 00:29:02,079
At last, scientists have
found another planet that may
just be capable of supporting life.

300
00:29:05,559 --> 00:29:07,444
Not much out here.

301
00:29:07,479 --> 00:29:10,279
See if there's any under the rock.

302
00:29:10,314 --> 00:29:13,879
Nope. A lot of UV radiation.

303
00:29:22,119 --> 00:29:25,759
Nothing green, nothing
coloured I can see. Very dry.

304
00:29:25,794 --> 00:29:31,404
For astrobiologists
like Dr Lynn Rothschild,

305
00:29:31,439 --> 00:29:37,199
its discovery means they can begin
to imagine what it would be like
to spend a day on a Super-Earth.

306
00:29:43,080 --> 00:29:48,280
We're up here on the edge of
the Atacama desert in Chile
right near the Bolivian border.

307
00:29:50,319 --> 00:29:55,080
You can see it's very dry, in fact,
one of the driest places on Earth.

308
00:29:58,920 --> 00:30:03,999
This is a great place to get an
idea of what an extra-solar planet,

309
00:30:04,034 --> 00:30:06,679
for example Gliese 581c,
might be like.

310
00:30:31,160 --> 00:30:36,604
Let's imagine that
we're on Gliese 581c.

311
00:30:36,639 --> 00:30:40,319
There's an awful lot of rocks around.
It's dry.

312
00:30:41,919 --> 00:30:45,619
The planet's mass is
five times that of Earth.

313
00:30:45,654 --> 00:30:49,284
This means that gravity
will pull twice as hard.

314
00:30:49,319 --> 00:30:52,160
Whereas on the moon, the
astronauts could jump with no effort,

315
00:30:52,195 --> 00:30:56,405
on this planet you would
be suffering from extra gravity.

316
00:30:56,440 --> 00:31:01,920
If you took a rock and you threw
it, it would come crashing down,

317
00:31:01,955 --> 00:31:04,285
much faster than that of the Earth.

318
00:31:04,320 --> 00:31:08,679
High gravity will affect the
look of the planet. No mountains.

319
00:31:08,714 --> 00:31:11,280
Just low hills and vast plains.

320
00:31:12,920 --> 00:31:16,485
And the last thing is it's
close to the parent star,

321
00:31:16,520 --> 00:31:22,040
and so the radiation from the sun
would be much stronger on Earth.

322
00:31:22,075 --> 00:31:25,400
Here we're getting burned,
there we would probably be fried.

323
00:31:34,080 --> 00:31:37,244
The planet's red dwarf star
will dominate the sky -

324
00:31:37,279 --> 00:31:40,959
a fiery ball five times larger
than our own sun back home.

325
00:31:40,994 --> 00:31:43,204
And a few hours into their trip,

326
00:31:43,239 --> 00:31:48,159
interstellar visitors will discover
that this sun never moves.

327
00:31:54,879 --> 00:31:57,159
The planet is so close to its star

328
00:31:57,194 --> 00:32:01,320
that immense gravitational forces
have united the two.

329
00:32:04,520 --> 00:32:09,639
They're tidally locked,
with the planet presenting
just one face to the light.

330
00:32:12,399 --> 00:32:15,525
On the Earth, we're used to getting
up in the morning, the sun rises.

331
00:32:15,560 --> 00:32:20,920
We have our midday meal,
in the evening we have dinner,
if we're lucky, we get a nice sunset.

332
00:32:20,955 --> 00:32:25,320
But on something like Gliese 581c
it would be totally different.

333
00:32:30,279 --> 00:32:35,760
If I wanted to see the equivalent
of a sunset, I'd be the one who'd
have to get into the car and move.

334
00:32:39,879 --> 00:32:42,604
Beyond this point is the dark side

335
00:32:42,639 --> 00:32:47,999
of the planet, perpetually turned
outwards to the cold of space.

336
00:32:49,800 --> 00:32:53,360
I wouldn't want to live here,
I wouldn't want to be a colonist

337
00:32:53,395 --> 00:32:57,204
on another world that
was barren like this.

338
00:32:57,239 --> 00:33:03,240
I'd take even a year-long field trip,
but I wouldn't sign up for
the rest of my life.

339
00:33:07,640 --> 00:33:12,525
Comfortable as Gliese 581c
may be for a day trip,

340
00:33:12,560 --> 00:33:20,280
for life to exist there, for it
truly to be second Earth, it must
have one other vital ingredient.

341
00:33:31,560 --> 00:33:35,120
Water is the one thing life on
Earth has in common, so we think

342
00:33:35,155 --> 00:33:37,244
looking for water on other planets

343
00:33:37,279 --> 00:33:39,680
is a way to look for
life on those planets.

344
00:33:46,879 --> 00:33:50,600
For astrophysicists like
Sean Raymond, finding water

345
00:33:50,635 --> 00:33:53,360
on other worlds is the key
to finding life.

346
00:33:56,479 --> 00:34:02,199
Every day in his laboratory,
he makes new solar systems
from scratch.

347
00:34:02,234 --> 00:34:06,757
So the way we do this
is computer simulations
of a disc of rocks orbiting

348
00:34:06,792 --> 00:34:11,280
a star, and we let them collide and
let their orbits evolve, and such.

349
00:34:11,315 --> 00:34:14,439
And it turns out these take
quite a long time to do.

350
00:34:14,474 --> 00:34:18,324
Over the months,
Sean's computer calculates

351
00:34:18,359 --> 00:34:22,599
how alien planetary systems
evolve over millions of years.

352
00:34:33,399 --> 00:34:36,599
Here's a movie of one of these
simulations. You can see everything

353
00:34:36,634 --> 00:34:39,045
on the inner disc
starts off red meaning, quite dry.

354
00:34:39,080 --> 00:34:42,325
All these guys start off
being the size of the moon,
or actually a little smaller.

355
00:34:42,360 --> 00:34:47,245
And then the number of bodies
is going down as they collide
and grow into larger things.

356
00:34:47,280 --> 00:34:51,160
And by about 10 million years or so,
a planet almost the size of the
Earth is formed right there.

357
00:34:51,195 --> 00:34:53,600
And you can see it's still red.

358
00:34:55,239 --> 00:34:59,400
These new planets are all dry.
Only far out from the star

359
00:34:59,435 --> 00:35:03,240
are temperatures low enough
for water to collect.

360
00:35:05,439 --> 00:35:09,640
It's not until a little later...
you'll see in a second, it
gets collided by something that's

361
00:35:09,675 --> 00:35:15,037
blue and turns - right there,
it went from being completely dry to
having some water.

362
00:35:15,072 --> 00:35:20,400
And that process of water
delivery continues over the next
100 million years or so.

363
00:35:23,120 --> 00:35:26,805
Over this time,
icy comets and asteroids from

364
00:35:26,840 --> 00:35:32,679
the outer solar system are drawn
inwards towards the young planets.

365
00:35:32,714 --> 00:35:37,400
Shaun's theory is they bring
with them vast amounts of water,

366
00:35:40,080 --> 00:35:44,360
transforming dead worlds
into blue planets.

367
00:35:44,395 --> 00:35:46,364
That's a pretty good Earth analogue.

368
00:35:46,399 --> 00:35:50,120
And we think this is how the solar
system terrestrial planets formed.

369
00:35:51,759 --> 00:35:55,204
Sean has run
hundreds of simulations.

370
00:35:55,239 --> 00:35:59,199
And each time, some something
happens to the planets
in the habitable zone -

371
00:36:01,040 --> 00:36:06,524
they nearly all have water.
Water is very abundant.

372
00:36:06,559 --> 00:36:12,240
In the solar system,
water is two to four times more
abundant than rock and iron.

373
00:36:15,560 --> 00:36:19,680
It looks like Earth might, on
average, be a little bit water-poor.

374
00:36:19,715 --> 00:36:23,800
And many planets may end up
with a lot more water than the Earth.

375
00:36:23,835 --> 00:36:27,725
Including the newly discovered 581c.

376
00:36:27,760 --> 00:36:32,919
Gliese 581c especially, is very
exciting, a very big discovery.

377
00:36:32,954 --> 00:36:37,077
These planets would have acquired
some water-rich material, so they

378
00:36:37,112 --> 00:36:41,200
probably have some water contents
comparable to Earth at least.

379
00:36:42,839 --> 00:36:45,244
Far from being a barren rock,

380
00:36:45,279 --> 00:36:49,359
this new planet may be
awash with liquid water.

381
00:36:54,480 --> 00:36:58,564
But in their rush to tell
the world of another world,

382
00:36:58,599 --> 00:37:03,600
the Swiss had overlooked one
thing - the planet's atmosphere.

383
00:37:05,199 --> 00:37:08,205
We got very excited about Gliese 581c

384
00:37:08,240 --> 00:37:13,040
when we realised that it was just at
the right distance from the star.

385
00:37:13,075 --> 00:37:17,805
But then, talking with specialists
of the evolution of atmospheres

386
00:37:17,840 --> 00:37:21,800
on the planet, they told us
that maybe the greenhouse effect
could be big.

387
00:37:21,835 --> 00:37:25,804
And so the temperature could be too
high for the development of life.

388
00:37:25,839 --> 00:37:30,960
If the planet's atmosphere
contains too much water
vapour or carbon dioxide...

389
00:37:30,995 --> 00:37:36,124
a runaway greenhouse
effect could take hold.

390
00:37:36,159 --> 00:37:41,279
Rather than resembling Earth,
581c could be a super-Venus.

391
00:37:46,239 --> 00:37:48,124
Instead of liquid water,

392
00:37:48,159 --> 00:37:53,480
steam would shroud a searingly hot
world, incapable of supporting life.

393
00:38:00,800 --> 00:38:03,924
It's probably too hot
to be habitable.

394
00:38:03,959 --> 00:38:11,880
If it has water at all,
which is doubtful, that water would
be boiled off, evaporated and gone.

395
00:38:11,915 --> 00:38:17,364
581c may, after all, lie on the
hot side of the habitable zone,

396
00:38:17,399 --> 00:38:22,399
but the light the Swiss team were
collecting from the planet's star
held another surprise.

397
00:38:24,479 --> 00:38:30,480
After decades of fruitless
searching for habitable worlds,
out popped another one.

398
00:38:32,079 --> 00:38:34,364
We had to wait for one more year

399
00:38:34,399 --> 00:38:39,879
before being able to actually find
another planet a bit further out.

400
00:38:39,914 --> 00:38:42,480
There is a third
planet in the system.

401
00:38:48,319 --> 00:38:54,520
They'd discovered a second
super-Earth in the same system -

402
00:38:54,555 --> 00:38:56,840
Gliese 581d.

403
00:38:57,960 --> 00:39:02,739
This world lies on the far,
cold edge of the habitable zone.

404
00:39:02,774 --> 00:39:07,484
On first calculations, this
would make it a giant frozen world.

405
00:39:07,519 --> 00:39:14,399
But if it too enjoys a greenhouse
effect, then it could be just
warm enough for liquid water.

406
00:39:15,999 --> 00:39:20,400
If there is some atmosphere,
and a greenhouse effect,
then the temperature could

407
00:39:20,435 --> 00:39:22,959
be even better on that planet
for the development of life.

408
00:39:28,119 --> 00:39:31,764
Perched on opposite edges
of the habitable zone,

409
00:39:31,799 --> 00:39:35,439
the conditions on the planets
in this system will be harsh.

410
00:39:37,040 --> 00:39:39,800
Perhaps too harsh
for life to survive.

411
00:39:46,799 --> 00:39:52,959
Here on Earth, Dr Lynn Rothschild
is investigating places where
conditions mirror the extreme

412
00:39:52,994 --> 00:39:57,200
environments found on
both the G581 planets.

413
00:39:59,079 --> 00:40:03,719
We're up here in the altiplano
in Bolivia. Up at about...

414
00:40:03,754 --> 00:40:06,644
well over 4,000m, or 15,000ft.

415
00:40:06,679 --> 00:40:11,959
In the winter it's frozen - it's not
a whole lot warmer in the summer,

416
00:40:11,994 --> 00:40:14,125
and yet life lives up here.

417
00:40:14,160 --> 00:40:19,799
Every place we've gone that's
cold - the Antarctic,
the ice caps, we've found life.

418
00:40:19,834 --> 00:40:23,360
And even under here, there's plenty
that's growing. It's just amazing.

419
00:40:28,959 --> 00:40:33,840
So life in the freezing
conditions of the outer
planet is a possibility.

420
00:40:43,599 --> 00:40:49,360
And even the on the inner hotter
world, where temperatures could
exceed the boiling point of water,

421
00:40:49,395 --> 00:40:52,917
scientists are beginning to
understand how life could survive.

422
00:40:52,952 --> 00:40:56,439
We don't actually know how life
actually got started on Earth.

423
00:40:56,474 --> 00:40:59,919
But we do know that when we look
at modern organisms,

424
00:40:59,954 --> 00:41:02,804
and at their evolution,
the most ancient ones

425
00:41:02,839 --> 00:41:06,960
seem to be the ones that
live at extremely high temperatures,

426
00:41:06,995 --> 00:41:09,320
just like these areas around here.

427
00:41:15,519 --> 00:41:17,725
Indeed, the more scientists look,

428
00:41:17,760 --> 00:41:22,800
the wider the range of habitats
they find in which living
organisms can thrive.

429
00:41:22,835 --> 00:41:27,920
So this gives us hope, this gives
us optimism that when we go elsewhere

430
00:41:27,955 --> 00:41:31,045
to other worlds,
that there might be life.

431
00:41:31,080 --> 00:41:35,840
For now, no-one knows for sure if
life could survive in the massive,

432
00:41:35,875 --> 00:41:38,319
strange worlds of the G581 system.

433
00:41:43,520 --> 00:41:47,919
And Earth-bound planet hunting may
have reached the end of the line.

434
00:41:47,954 --> 00:41:51,639
Because to find true
Earth-sized planets,

435
00:41:51,674 --> 00:41:54,200
the hunt is moving into space.

436
00:42:11,679 --> 00:42:15,200
This is a spaceship factory.

437
00:42:17,960 --> 00:42:22,325
In these category A clean rooms,
machines are built

438
00:42:22,360 --> 00:42:26,640
that their designers hope will
unlock the secrets of the universe.

439
00:42:26,675 --> 00:42:29,240
That's the interferometer.

440
00:42:33,519 --> 00:42:38,204
There's the focus mechanisms right
here. Here's one focus mechanism.

441
00:42:38,239 --> 00:42:42,960
This is the actual focus mechanism.
This is the flight hardware.
Wonderful.

442
00:42:42,995 --> 00:42:48,320
Today the team are midway through
assembling their latest mission -

443
00:42:48,355 --> 00:42:51,519
the giant Kepler space telescope.

444
00:42:57,719 --> 00:43:05,119
But it's not scheduled to fly
until 2009, so currently
the spaceship is in bits.

445
00:43:05,154 --> 00:43:09,200
This is where the primary mirror
is gonna sit, on top of this.

446
00:43:09,235 --> 00:43:13,277
So that measures how well
you've got the optics aligned?

447
00:43:13,312 --> 00:43:17,284
That's right, you
can measure how well it's working.

448
00:43:17,319 --> 00:43:21,360
Leading the NASA team assembling
the space telescope is Bill Borucki.

449
00:43:21,395 --> 00:43:26,000
It's magnificent, it's just
wonderful to see it come together.

450
00:43:26,035 --> 00:43:29,799
We've been planning
this for years and years.

451
00:43:29,834 --> 00:43:31,324
So to actually see it here...

452
00:43:31,359 --> 00:43:34,160
This is the flight equipment,
this will go into space.

453
00:43:34,195 --> 00:43:36,165
It's this
that will make our discovery.

454
00:43:36,200 --> 00:43:41,080
I'm delighted to see all
the details that seem to be right.

455
00:43:46,399 --> 00:43:52,359
When Kepler flies,
it will undertake a four-year
mission to seek out new worlds.

456
00:43:54,519 --> 00:43:56,924
But it won't be looking for wobbles.

457
00:43:56,959 --> 00:44:04,640
Instead, Kepler will be hunting for
planets that pass in front of their
stars, creating a tell-tale wink.

458
00:44:04,675 --> 00:44:08,840
Looking at the star, it seems to
wink, it gets dimmer for a while.

459
00:44:08,875 --> 00:44:12,124
Like it closed its eye for a second
and then opened it.

460
00:44:12,159 --> 00:44:16,359
This is because the planet
moved in front of it
and blocked some of its light.

461
00:44:16,394 --> 00:44:18,604
It happens in our solar system too.

462
00:44:18,639 --> 00:44:25,640
We had a transit, Mercury going in
front of the sun fairly recently,
we could see that with a telescope.

463
00:44:27,600 --> 00:44:30,439
For the wink technique to work,

464
00:44:30,474 --> 00:44:33,244
a space telescope is essential.

465
00:44:33,279 --> 00:44:36,924
Free from the interference of
Earth's atmosphere, it gives

466
00:44:36,959 --> 00:44:41,279
Kepler an uninterrupted view of a
very special part of the galaxy.

467
00:44:41,314 --> 00:44:43,764
Kepler only looks at
one area of the sky.

468
00:44:43,799 --> 00:44:47,960
It's a good area for us, in that
it has a huge number of stars.

469
00:44:47,995 --> 00:44:51,279
Kepler will scan the same
100,000 stars

470
00:44:51,314 --> 00:44:54,285
over its entire four-year mission,

471
00:44:54,320 --> 00:44:58,524
constantly measuring
the brightness of each one.

472
00:44:58,559 --> 00:45:04,139
And from day one, it will be
sensitive enough to detect the wink

473
00:45:04,174 --> 00:45:09,719
of an Earth-sized planet crossing
its sun, tens of light years away.

474
00:45:12,440 --> 00:45:18,279
It's always very exciting, because
we've always wanted to know - are
there lots of Earths out there?

475
00:45:18,314 --> 00:45:22,440
Geoff Marcy and Stephane Udry
and all these other people
are extremely competitive.

476
00:45:22,475 --> 00:45:25,564
They want to find planets,
they want the answers too.

477
00:45:25,599 --> 00:45:29,319
Well, we all do, and the best
way to do that is to co-operate.

478
00:45:29,354 --> 00:45:33,004
There's a bit of a race going
on, but it's a delightful race.

479
00:45:33,039 --> 00:45:38,519
The competition is lovely, and it
makes us get up in the morning,
go to work, and work a little harder.

480
00:45:38,554 --> 00:45:41,245
So who's gonna
find the first Earth-sized object?

481
00:45:41,280 --> 00:45:46,239
We are. Kepler's going to find the
first Earths in the habitable zone.

482
00:45:49,240 --> 00:45:56,639
Between them, the planet hunters
are beginning to define the first
galactic map of Earth-like worlds.

483
00:46:00,879 --> 00:46:07,920
At last, a phone directory for those
listening for a message from ET.

484
00:46:11,359 --> 00:46:14,120
They're gonna allow us to
sharpen our gaze of the heavens,

485
00:46:14,155 --> 00:46:16,045
where we're pointing these antennas,

486
00:46:16,080 --> 00:46:20,400
trying to pick up a signal,
they're gonna tell us, "You don't
have to look at every star,

487
00:46:20,435 --> 00:46:24,537
"these ones have planets", and
eventually they'll be able to say,

488
00:46:24,572 --> 00:46:28,639
"These are the ones that have
planets the same size as Earth."

489
00:46:28,674 --> 00:46:31,444
And ten years after that,
they'll be able to say,

490
00:46:31,479 --> 00:46:36,205
"These are the ones with oxygen
or methane in their atmosphere.

491
00:46:36,240 --> 00:46:41,400
"So they have some biology, and
it's up to you to find out if any
of that biology is smart or not."

492
00:46:43,760 --> 00:46:49,799
Rather than the entire galaxy of 200
billion stars, in the future, SETI

493
00:46:49,834 --> 00:46:55,839
need only tune into the handful of
star systems that Kepler discovers.

494
00:47:01,680 --> 00:47:05,404
Everything has caused us
to become more optimistic.

495
00:47:05,439 --> 00:47:09,320
We really believe in the next 20
years or so, we're going to learn

496
00:47:09,355 --> 00:47:12,760
a great deal more
about life beyond Earth

497
00:47:12,795 --> 00:47:16,404
detected that life

498
00:47:16,439 --> 00:47:21,004
and perhaps even intelligent
life elsewhere in our galaxy.

499
00:47:21,039 --> 00:47:26,004
Remember, there's a flip side to
this - it could be that advanced

500
00:47:26,039 --> 00:47:32,880
technological civilisations, species,
are a rarity, one in a million,
maybe one in a billion.

501
00:47:32,915 --> 00:47:38,640
If so, we humans could be
quite a precious rarity
in the Milky Way galaxy.

502
00:47:38,675 --> 00:47:42,405
Maybe, in fact,
they're not out there watching us.

503
00:47:42,440 --> 00:47:46,920
We may be the ones to be the first
to go out and explore the galaxy.

504
00:47:55,519 --> 00:47:57,365
If you'd like to explore

505
00:47:57,400 --> 00:47:59,420
Dr Frank Drake's famous equation

506
00:47:59,455 --> 00:48:01,405
and come up with your own estimate

507
00:48:01,440 --> 00:48:05,280
of the number of alien
civilisations in the galaxy,

508
00:48:05,315 --> 00:48:08,119
log on to:

