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(upbeat music)

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We are in one of the greatest periods

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of discovery in humanity's history.

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Finding out more about the universe than ever before.

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At a faster rate than ever before.

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And of these discoveries,

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perhaps the most fascinating of all,

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is that there are other planets, other worlds,

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orbiting other stars far away.

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Exoplanets.

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Today we take for granted that there are exoplanets

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around other stars.

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And yet only a few decades ago, we had not seen one.

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(upbeat music)

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Finding the first done in 1995,

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I think nobody believed us.

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(laughing)

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It was too big.

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(upbeat music)

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Nobody thought

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this was even a thing worth studying.

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Back then, it was considered ridiculous

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to search for exoplanets.

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And it was definitely a taboo subject.

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(upbeat music)

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But what they found never ceases to amaze.

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Nature didn't obey the laws that we had set for ourselves.

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And that was exciting.

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Everything is exotic outside the solar system.

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The types of exoplanets that exist out there,

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it's really, I think,

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as far as your imagination can we reach.

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These are real places we can point to

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and say, "Yeah, this is a planet

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"that'll rain diamonds or sulfuric acid."

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But this quest has a very human face.

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In my heart, I wanna go out there

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and find the planet with oceans and continents

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and breathable air.

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A planet that just like Earth.

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Humans have always been

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fascinated by the heavens.

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And wondered, what is our place within them?

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Since the stars rotate over our heads every night,

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it was only too easy to assume we were right in the middle

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of this never ending spectacle.

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We used to think that the Earth

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was the center of the universe,

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that the planets and the stars all revolved around Earth.

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Then in the 16 century,

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Polish polymath and Catholic canon,

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Nicolaus Copernicus upset the status quo.

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He figured that the apparent motion

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of the stars in the night sky

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was more likely due to the Earth moving, not the stars,

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which he believed were fixed in the heavens.

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Copernicus came along and had a new theory

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that the planets, including Earth, revolved around the Sun.

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And that was considered heretical.

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Suddenly humankind is no longer center stage

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and there is worse to come.

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Turned out that not even the Sun

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is in the center of everything.

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The Sun is one out of a few hundred billion stars

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orbiting the center of the Milky Way,

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which itself is just one galaxy

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out of probably a few hundred billions out there.

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Over the centuries,

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increasingly powerful telescopes

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revealed that the cosmos

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is both teaming with countless stars yet so vast

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that it is mostly empty space.

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If you shrink the Sun down to the size of a grain of salt,

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the Earth would be about two inches away from the salt grain

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and be almost microscopic,

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it'd be the size of a particle of smoke, for instance.

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And then one can ask, "Well, where do I put

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"the next salt grain, the next closest star?"

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That star, that next salt grain

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would be seven and a half miles away.

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So we are just dust grain floating out there.

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But still it might be that we are

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the only very interesting dust grain out there.

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I don't think so though.

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The thing of course that really drives all this is,

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is there life elsewhere in the universe?

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This is the fundamental question

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that we have in astronomy, are we alone?

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The sheer number of stars suggests

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that worlds like our own must exist elsewhere in the cosmos.

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But at the end of the 20 century,

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there is no evidence that exoplanets exist at all.

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And most astronomers believe that theorizing

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about exoplanets and their potential habitability

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is a pointless exercise.

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They're just too small and far away to be observed.

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In the early 1980s, we knew in our hearts philosophically

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that exoplanets must exist.

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But in astronomy evidence is king, it counts for everything.

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And until you see one, there's always a niggling doubt.

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(people speaking indistinctly)

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Exoplanets, it seems

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are an itch that can never be scratched.

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Four, three, two, go for engine start, one.

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(rocket engine roaring)

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But in 1983, a new kind of telescope

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is about to challenge those assumptions.

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(man speaking indistinctly)

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(upbeat music)

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The infrared astronomical satellite or IRAS,

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exploits new technology, sensitive to light

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beyond the range of human vision.

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It's detecting wavelengths where you're seeing heat

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as opposed to what the laypeople

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will call light, visible light.

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All objects in the universe

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emit some level of infrared radiation.

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And although it's invisible,

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we can sometimes feel it as heat.

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We're used to the idea that with an infrared camera,

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we can see people at night while it's pitch black,

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because things that are warm

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show up by their infrared radiation.

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IRAS applies the same principle

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to its survey of the entire sky.

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Point about infrared radiation is,

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it gets to places that visible light can't.

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(laughing)

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{\an8}It can penetrate a cloud of dust around a star.

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{\an8}(gentle music)

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The space between stars

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is filled with bands of gas and dust

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that absorb and scatter visible light

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and block our view of the stars behind them.

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But the longer wavelengths of infrared radiation

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pass much more freely.

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So previously hidden stars that emit

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both visible and infrared light

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are suddenly revealed by the IRAS detector.

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Now I was working at that point on infrared technology

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for big telescopes on the ground.

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So we knew a lot about what IRAS was doing.

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And in some ways that technology was really crude.

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(gentle upbeat music)

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You just let the sky flow over the telescope,

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and then when a bright object comes up, you go bing,

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and you just map the sky bit by bit, as you drift over it.

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There were thousands, millions of new objects.

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It was a revolution.

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Around six months into the survey,

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IRAS detects a bizarre infrared signature

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from the star, Beta Pictoris, 63 light years from Earth.

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(gentle music)

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Beta Pictoris had all this extra infrared radiation

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that was unexpected.

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It wasn't part of the normal thermal spectrum,

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if I can put it that way.

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It's not coming from the star itself.

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So where is this infrared radiation coming from?

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It was a real puzzle.

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We had no idea what it was,

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and that began a big detective story in itself.

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News of the Beta Pictoris anomaly

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reaches a remote observatory and Chile,

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where two NASA astronomers

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decide to pause their survey of our solar system

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and investigate.

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(gentle upbeat music)

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We think perhaps this is a material

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which is being illuminated by the star,

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heating up and generating this excess infrared signature.

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It was a tantalizing piece of evidence

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that maybe there's something out there

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that we should be looking for.

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(gentle upbeat music)

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The telescope itself, it's on the end of a ridge,

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almost like the prow of a ship

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where the landscape falls away on three sides.

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It's rather beautiful.

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But it's also very, very dark

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and very, very clear skies.

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(gentle music)

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In spring of 1984,

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the astronomers turned their optical telescope

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towards the Milky Way.

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(gentle music)

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Beta Pictoris was a star like any other star in the sky.

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So one of thousands and thousands of stars to look at.

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(gentle music)

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But when they tried to see

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what could be causing the infrared access around the star,

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there's a problem.

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(gentle music)

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At the telescope, you really couldn't see anything.

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And that's because the central star,

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there is hundreds of millions of times brighter material

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around that star.

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(gentle music)

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Richard's only option

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is to try and blot out the light of the star

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by making a tiny Sun shield

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that astronomers called a coronagraph.

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A coronagraph is basically a way

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of putting your thumb over the star

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and being able to look at material around the star.

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Coronagraphs are usually

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precision engineered instruments,

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but Richard will need to improvise his artificial eclipse

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using supplies from the stationary cupboard.

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(gentle upbeat music)

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We use these rub-on fonts.

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(gentle upbeat music)

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We'd use the period, a half a millimeter in diameter,

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and you needed to suspend that.

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And at the very, very center of the cross,

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we would fix this tiny period, and that would be our mask.

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(gentle upbeat music)

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And suddenly, low and behold,

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when we looked at Beta Pictoris with a chronograph, wow.

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This extended disc showed up in the images.

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A flattened disc of material surrounding the star.

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What they saw looked like sort of two spikes

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sticking out on either side.

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They saw dust now, not emitting in the infrared,

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but reflecting Sunlight from the star in the center.

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This was called a debris disc.

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What they have found

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is an expansive disc of material, like the rings of Saturn,

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but on a vastly larger scale.

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It's really the fallout of the planet formation process.

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Dust created from collisions between objects

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like asteroids and rocky bodies.

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(gentle music)

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You were seeing the first evidence of extra solar planets.

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(gentle upbeat music)

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It was incredibly exciting, I mean,

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this was the first evidence of the birthplace of planets

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around other stars.

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Richard Terrile's groundbreaking image

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of the Beta Pictoris debris disc

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creates a buzz of anticipation in the astronomy underground.

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(gentle upbeat music)

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Could exoplanets be within our grasp?

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(gentle upbeat music)

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It really opened people's eyes.

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Maybe we're ready for prime time in terms of exoplanets.

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But spotting an exoplanet

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is very different from photographing a debris disc

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bigger than our solar system.

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(gentle music)

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And at decade later, exoplanets

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are still strictly a French interest.

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In the '90s, we had no exoplanets,

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nobody has found anything.

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I mean, the field did not exist at all.

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When 26-year-old Didier Queloz

273
00:12:28,220 --> 00:12:30,710
begins his PhD in astrophysics,

274
00:12:30,710 --> 00:12:33,093
he sticks to more mainstream areas.

275
00:12:34,260 --> 00:12:39,260
My supervisor, Michel Mayor, had a name on binary stars.

276
00:12:39,550 --> 00:12:41,150
That was the business he was in.

277
00:12:43,240 --> 00:12:46,860
Astronomers have been studying binary stars for decades.

278
00:12:46,860 --> 00:12:48,810
That's when two stars orbit each other.

279
00:12:49,830 --> 00:12:51,430
Binary stars are locked

280
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in a complex gravitational dance

281
00:12:53,670 --> 00:12:56,003
that Queloz is tasked with unraveling.

282
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(gentle music)

283
00:12:58,660 --> 00:13:01,350
He never imagines that his student project

284
00:13:01,350 --> 00:13:04,053
will kickstart the era of exoplanets.

285
00:13:05,710 --> 00:13:09,330
My PhD actually was to design a new equipment

286
00:13:09,330 --> 00:13:11,123
{\an8}that we called a spectrograph.

287
00:13:12,160 --> 00:13:17,060
{\an8}Precise enough to detect tiny change

288
00:13:17,060 --> 00:13:18,893
into the speed of the star.

289
00:13:20,100 --> 00:13:22,700
Subtle speed changes of a large star

290
00:13:22,700 --> 00:13:26,830
can reveal the presence of a much smaller companion star

291
00:13:26,830 --> 00:13:29,170
because the gravitational pull of the companion

292
00:13:29,170 --> 00:13:33,193
as it orbits, makes the main star appear to wobble slightly.

293
00:13:34,480 --> 00:13:36,750
The size of the wobble reflects the size

294
00:13:36,750 --> 00:13:38,153
of the companion star.

295
00:13:39,080 --> 00:13:40,910
And if there is no companion,

296
00:13:40,910 --> 00:13:44,163
then there will be no wobble in the star's position at all.

297
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To be able to detect the smallest stars,

298
00:13:48,840 --> 00:13:50,940
Queloz lanes to measure speed changes

299
00:13:50,940 --> 00:13:55,940
of just 50 meters per second, or 110 miles per hour,

300
00:13:56,050 --> 00:13:59,030
no mean feet and a cosmos and constant,

301
00:13:59,030 --> 00:14:00,823
violent relative motion.

302
00:14:01,950 --> 00:14:04,503
Everything is fast into space.

303
00:14:05,400 --> 00:14:08,623
Like, I mean, the motion of the Earth on its orbit,

304
00:14:10,510 --> 00:14:13,773
it's about 100,000 kilometer per hour.

305
00:14:14,850 --> 00:14:18,240
So your have to fight with all this massive change of speed.

306
00:14:18,240 --> 00:14:21,120
And you're trying to see a tiny, tiny bit.

307
00:14:21,120 --> 00:14:24,530
It is as if you want to measure the speed of a snail

308
00:14:24,530 --> 00:14:25,893
on the wing of a jet.

309
00:14:26,944 --> 00:14:29,034
(laughing)

310
00:14:29,034 --> 00:14:30,860
(jet engines roaring)

311
00:14:30,860 --> 00:14:32,570
I'm not sure the snail will survive on the wing,

312
00:14:32,570 --> 00:14:33,975
but that's about.

313
00:14:33,975 --> 00:14:37,028
(laughing)

314
00:14:37,028 --> 00:14:40,010
(gentle upbeat music)

315
00:14:40,010 --> 00:14:41,380
Queloz' spectrograph

316
00:14:41,380 --> 00:14:45,420
explores the latest advances in computers and fiber optics

317
00:14:45,420 --> 00:14:49,840
and its performance is a surprise, even to him.

318
00:14:49,840 --> 00:14:53,010
I had a goal to reach 50 meter per second,

319
00:14:53,010 --> 00:14:54,790
but I completely overshoot the goal,

320
00:14:54,790 --> 00:14:56,318
I did much better than the goal.

321
00:14:56,318 --> 00:14:57,550
(laughing)

322
00:14:57,550 --> 00:14:59,143
We ended up with 15.

323
00:15:01,080 --> 00:15:03,670
We talking about a tiny motion, which is essentially

324
00:15:03,670 --> 00:15:06,030
the speed of a running man.

325
00:15:06,030 --> 00:15:09,560
Queloz realizes that this unexpected extra sensitivity

326
00:15:09,560 --> 00:15:12,980
to changes speed, means that his spectrograph

327
00:15:12,980 --> 00:15:16,775
could now detect objects much smaller than stars.

328
00:15:16,775 --> 00:15:18,010
(gentle upbeat music)

329
00:15:18,010 --> 00:15:20,040
With this kind of accuracy,

330
00:15:20,040 --> 00:15:23,123
then you open a complete new window, which is the planet.

331
00:15:24,260 --> 00:15:26,550
But like all aspiring astronomers,

332
00:15:26,550 --> 00:15:28,837
Queloz knows that exoplanet hunting is seen

333
00:15:28,837 --> 00:15:31,993
as a disreputable occupation at best.

334
00:15:33,210 --> 00:15:35,810
Back then it was considered ridiculous

335
00:15:35,810 --> 00:15:37,630
to search for exoplanets.

336
00:15:37,630 --> 00:15:40,150
To study them at all, would've been laughable.

337
00:15:40,150 --> 00:15:43,250
And it was definitely a taboo subject.

338
00:15:43,250 --> 00:15:44,880
Making the wrong decision,

339
00:15:44,880 --> 00:15:49,120
could spell career suicide for the young astrophysicist.

340
00:15:49,120 --> 00:15:51,097
And I remember really Michel telling me,

341
00:15:51,097 --> 00:15:53,360
"Look Didier you're not going to find any planet,

342
00:15:53,360 --> 00:15:54,890
"is that okay with you?"

343
00:15:54,890 --> 00:15:58,230
And I say yes, of course, because it's so cool for me

344
00:15:58,230 --> 00:16:00,730
to demonstrate that the machine had the capability

345
00:16:01,890 --> 00:16:03,910
to detect a planet.

346
00:16:03,910 --> 00:16:06,080
In September, 1994,

347
00:16:06,080 --> 00:16:09,660
Didier Queloz begins his search for exoplanets,

348
00:16:09,660 --> 00:16:12,373
high in the mountains of Provence in France.

349
00:16:13,320 --> 00:16:17,740
Meanwhile, his PhD supervisor, goes on vacation to Hawaii,

350
00:16:17,740 --> 00:16:19,763
confident he will not be disturbed.

351
00:16:22,970 --> 00:16:25,870
Queloz has a list of 142 stars

352
00:16:25,870 --> 00:16:28,943
chosen because of their similarity to our own Sun.

353
00:16:30,140 --> 00:16:33,123
And one of these stars was 51 Peg.

354
00:16:34,290 --> 00:16:37,700
51 Pegasi is in the constellation of Pegasus

355
00:16:37,700 --> 00:16:40,606
located 48 light years from Earth.

356
00:16:40,606 --> 00:16:43,273
(gentle music)

357
00:16:44,360 --> 00:16:46,410
Queloz is looking for signs that the star

358
00:16:46,410 --> 00:16:49,840
is wobbling slightly due to the tiny gravitational pull

359
00:16:49,840 --> 00:16:53,609
of an unseen exo planet, as it orbits the star.

360
00:16:53,609 --> 00:16:56,060
(upbeat music)

361
00:16:56,060 --> 00:16:59,240
You take the light from the star and you spread it.

362
00:16:59,240 --> 00:17:01,453
You do a rainbow, what's called the spectra.

363
00:17:03,300 --> 00:17:06,390
Now, when you move the speed of the star,

364
00:17:06,390 --> 00:17:10,223
you going to change the locations of each of this line.

365
00:17:11,060 --> 00:17:13,940
In a way they become reddish or bluish.

366
00:17:13,940 --> 00:17:16,020
And it's very tiny motions,

367
00:17:16,020 --> 00:17:18,420
and you're trying to measure that,

368
00:17:18,420 --> 00:17:20,720
to build up a single point of data,

369
00:17:20,720 --> 00:17:21,978
which is the radial velocity.

370
00:17:21,978 --> 00:17:23,670
(upbeat music)

371
00:17:23,670 --> 00:17:25,290
The tug of an exoplanet

372
00:17:25,290 --> 00:17:27,690
would cause changes in the star's speed

373
00:17:27,690 --> 00:17:30,043
comparable to that of an Olympic runner.

374
00:17:31,110 --> 00:17:35,684
But immediately 51 Pegasi makes Queloz question is methods.

375
00:17:35,684 --> 00:17:39,150
(upbeat music)

376
00:17:39,150 --> 00:17:42,340
I really kind of panicked when I got the first data,

377
00:17:42,340 --> 00:17:45,003
because I think there is a bug in my software.

378
00:17:46,080 --> 00:17:48,030
The problem is that the measurements

379
00:17:48,030 --> 00:17:49,853
seem too good to be true.

380
00:17:51,360 --> 00:17:53,680
The data were telling me a story

381
00:17:53,680 --> 00:17:56,100
that was pointing to a planet,

382
00:17:56,100 --> 00:17:58,803
while I want that star to behave normally.

383
00:18:00,251 --> 00:18:02,500
And I'm trying to debunk the data

384
00:18:02,500 --> 00:18:04,750
and go back to the software,

385
00:18:04,750 --> 00:18:08,190
until I think to myself, I try all I could,

386
00:18:08,190 --> 00:18:09,743
so it must be real.

387
00:18:10,820 --> 00:18:12,460
It must be a planet, it must be a planet.

388
00:18:12,460 --> 00:18:15,060
It's unbelievable, it's unbelievable.

389
00:18:15,060 --> 00:18:17,577
And then I send this fax to Michel,

390
00:18:17,577 --> 00:18:19,462
"I think I'll find a planet."

391
00:18:19,462 --> 00:18:22,180
(upbeat music)

392
00:18:22,180 --> 00:18:23,840
This is a half Jupiter mass

393
00:18:23,840 --> 00:18:26,020
with the four and a half day periods.

394
00:18:26,020 --> 00:18:28,453
And that was what came up out of the data.

395
00:18:29,640 --> 00:18:32,510
I said to Michel, the distance of the orbiting body

396
00:18:32,510 --> 00:18:35,090
is 20 times closer to the distance

397
00:18:35,090 --> 00:18:36,590
between the Earth and the Sun.

398
00:18:37,460 --> 00:18:38,913
So the planet's very hot.

399
00:18:40,690 --> 00:18:43,190
After checking and rechecking the data,

400
00:18:43,190 --> 00:18:46,480
in October, 1995, the first exoplanet

401
00:18:46,480 --> 00:18:48,883
around a Sun-like star is announced.

402
00:18:50,060 --> 00:18:51,940
Well, we went live with that.

403
00:18:51,940 --> 00:18:54,232
And I think nobody believed us.

404
00:18:54,232 --> 00:18:55,530
(laughing)

405
00:18:55,530 --> 00:18:57,620
(gentle upbeat music)

406
00:18:57,620 --> 00:18:58,520
I remember this time

407
00:18:58,520 --> 00:19:00,420
because I was in graduate school at the time.

408
00:19:00,420 --> 00:19:03,679
And it was just wow, like so, so crazy.

409
00:19:03,679 --> 00:19:06,700
(upbeat music)

410
00:19:06,700 --> 00:19:08,280
And the reason this was so crazy

411
00:19:08,280 --> 00:19:12,100
is our Jupiter takes years to go around the Sun.

412
00:19:12,100 --> 00:19:15,423
But this planet orbits its star in a few days.

413
00:19:16,730 --> 00:19:19,170
Not only did we definitely not have gas giants,

414
00:19:19,170 --> 00:19:20,920
so close to our own Sun,

415
00:19:20,920 --> 00:19:23,343
we didn't think planets could even form there.

416
00:19:24,490 --> 00:19:28,963
How do you get a planet like that, so close to its star?

417
00:19:30,210 --> 00:19:32,610
The accepted theory of planet formation

418
00:19:32,610 --> 00:19:35,840
has gas giants forming only in the cold outer reaches

419
00:19:35,840 --> 00:19:37,283
of planetary systems.

420
00:19:38,720 --> 00:19:43,070
Assuming this new found signal was a planet,

421
00:19:43,070 --> 00:19:45,093
it would have to have broken all rules.

422
00:19:46,490 --> 00:19:48,370
The planet would've had to form somewhere else,

423
00:19:48,370 --> 00:19:49,911
far out from the star.

424
00:19:49,911 --> 00:19:51,600
(gentle upbeat music)

425
00:19:51,600 --> 00:19:53,550
And it would've had to migrate,

426
00:19:53,550 --> 00:19:55,770
would've interact with the gas

427
00:19:55,770 --> 00:19:59,859
or with other planets in the system and move inwards.

428
00:19:59,859 --> 00:20:02,240
(gentle upbeat music)

429
00:20:02,240 --> 00:20:04,860
That means that big planet came orbiting in

430
00:20:04,860 --> 00:20:07,900
destroyed all the small planets in its path.

431
00:20:07,900 --> 00:20:09,690
That shouldn't happen.

432
00:20:09,690 --> 00:20:12,240
That meant our solar system was quite different

433
00:20:12,240 --> 00:20:14,150
from what they were finding.

434
00:20:14,150 --> 00:20:15,740
(gentle upbeat music)

435
00:20:15,740 --> 00:20:17,530
And that was a tough pill to swallow for us,

436
00:20:17,530 --> 00:20:19,077
for many people.

437
00:20:20,290 --> 00:20:22,800
The community was absolutely convinced

438
00:20:22,800 --> 00:20:25,880
a planet, like Jupiter, can only be there.

439
00:20:25,880 --> 00:20:28,013
So you have to imagine that you are coming up

440
00:20:28,013 --> 00:20:31,100
with the first planet ever on orbiting a star,

441
00:20:31,100 --> 00:20:33,000
which is already a world premier,

442
00:20:33,000 --> 00:20:34,720
but the planet to come up with,

443
00:20:34,720 --> 00:20:36,930
it's not at all the one you expect.

444
00:20:36,930 --> 00:20:40,203
I mean, it was impossible to swallow, it was too big.

445
00:20:41,480 --> 00:20:43,940
But resistance is futile

446
00:20:43,940 --> 00:20:45,950
when Queloz' breakthrough technique

447
00:20:45,950 --> 00:20:48,530
leads to the discovery of a handful more,

448
00:20:48,530 --> 00:20:50,400
close-orbiting gas giants.

449
00:20:50,400 --> 00:20:54,390
In the following months, his achievement is undeniable

450
00:20:54,390 --> 00:20:57,873
and hot Jupiters become a new category of planetary body.

451
00:20:59,640 --> 00:21:03,960
Finding 51 Peg, in 1995, we kicked the door open.

452
00:21:03,960 --> 00:21:06,540
At that time, I was very proud

453
00:21:06,540 --> 00:21:09,380
to demonstrate the machine would do it,

454
00:21:09,380 --> 00:21:10,940
I mean, eventually.

455
00:21:10,940 --> 00:21:12,730
Well I was very far to realize

456
00:21:12,730 --> 00:21:16,260
it eventually turned out to be only six months.

457
00:21:16,260 --> 00:21:17,984
Really this what happened.

458
00:21:17,984 --> 00:21:18,962
(laughing)

459
00:21:18,962 --> 00:21:21,500
(gentle upbeat music)

460
00:21:21,500 --> 00:21:25,627
That moment in the mid '90s was when everything changed.

461
00:21:25,627 --> 00:21:26,980
(gentle music)

462
00:21:26,980 --> 00:21:29,540
Nature, didn't obey the laws

463
00:21:29,540 --> 00:21:31,360
that we had set for ourselves.

464
00:21:31,360 --> 00:21:32,460
And that was exciting.

465
00:21:33,630 --> 00:21:36,991
51 Pegasi b really tilted over our perspective

466
00:21:36,991 --> 00:21:41,991
of the solar system as just one possible realization

467
00:21:42,560 --> 00:21:44,283
of what can actually happen.

468
00:21:45,780 --> 00:21:48,890
But 51 Pegasi b, also triggers

469
00:21:48,890 --> 00:21:50,323
a more basic instinct.

470
00:21:51,370 --> 00:21:54,630
The main reaction that we had from the public

471
00:21:54,630 --> 00:21:57,347
and from the media, was to ask right away,

472
00:21:57,347 --> 00:21:59,175
"Is that life on that planet?"

473
00:21:59,175 --> 00:22:00,750
(gentle music)

474
00:22:00,750 --> 00:22:02,590
The idea of life is so profoundly

475
00:22:02,590 --> 00:22:04,700
connected into the society,

476
00:22:04,700 --> 00:22:06,950
then as soon as there is a little bit of a hint,

477
00:22:06,950 --> 00:22:09,335
then you start to ignite the fire.

478
00:22:09,335 --> 00:22:10,940
(gentle upbeat music)

479
00:22:10,940 --> 00:22:13,300
Inspired by 51 Pegasi,

480
00:22:13,300 --> 00:22:16,320
another young astrophysicist decides to tackle

481
00:22:16,320 --> 00:22:17,850
the formidable challenge

482
00:22:17,850 --> 00:22:20,980
of searching for life on exoplanets.

483
00:22:20,980 --> 00:22:22,200
I just love imagining

484
00:22:22,200 --> 00:22:24,830
that there's some kind of life out there.

485
00:22:24,830 --> 00:22:28,150
In my heart, I wanna go out there and find the planet

486
00:22:28,150 --> 00:22:29,700
that's just like Earth,

487
00:22:29,700 --> 00:22:33,800
with oceans and continents and breathable air,

488
00:22:33,800 --> 00:22:35,636
a planet around a Sun-like star.

489
00:22:35,636 --> 00:22:37,270
(gentle music)

490
00:22:37,270 --> 00:22:39,290
Sara focuses on the idea

491
00:22:39,290 --> 00:22:41,850
that the atmospheres of exoplanets

492
00:22:41,850 --> 00:22:44,853
could contain clues to biological processes.

493
00:22:45,990 --> 00:22:50,040
The search for life by way of gases in an atmosphere,

494
00:22:50,040 --> 00:22:53,163
this idea has been around for nearly a century.

495
00:22:54,500 --> 00:22:56,630
Our atmosphere here on Earth has oxygen,

496
00:22:56,630 --> 00:22:59,740
which fills our atmosphere to 20% by volume,

497
00:22:59,740 --> 00:23:03,633
is only here because of plants and photosynthetic bacteria.

498
00:23:04,520 --> 00:23:07,743
And without those who continuously replenish oxygen,

499
00:23:08,610 --> 00:23:10,810
our Earth's atmosphere would have no oxygen.

500
00:23:11,720 --> 00:23:14,360
The idea that an exoplanet atmosphere

501
00:23:14,360 --> 00:23:17,393
might carry the fingerprints of any life, is attractive.

502
00:23:18,440 --> 00:23:20,500
But putting that theory into practice

503
00:23:20,500 --> 00:23:22,213
has a major stumbling block.

504
00:23:24,840 --> 00:23:26,170
Well, that time we didn't know

505
00:23:26,170 --> 00:23:29,004
if we could detect exoplanet atmospheres.

506
00:23:29,004 --> 00:23:30,640
(gentle music)

507
00:23:30,640 --> 00:23:34,020
The astronomy community wanted to know why are we bothering?

508
00:23:34,020 --> 00:23:36,470
We can barely detect the planets,

509
00:23:36,470 --> 00:23:38,334
why are we studying the atmospheres?

510
00:23:38,334 --> 00:23:40,580
(gentle upbeat music)

511
00:23:40,580 --> 00:23:43,100
A breakthrough comes in 1999

512
00:23:43,100 --> 00:23:44,950
when a hot Jupiter is detected,

513
00:23:44,950 --> 00:23:47,439
as it crosses the face of its star.

514
00:23:47,439 --> 00:23:49,830
(gentle upbeat music)

515
00:23:49,830 --> 00:23:50,890
The method involves

516
00:23:50,890 --> 00:23:54,283
measuring the dip in intensity of starlight as it transits.

517
00:23:55,510 --> 00:23:59,080
And suggests an intriguing possibility,

518
00:23:59,080 --> 00:24:01,610
could the atmosphere of a transiting planet

519
00:24:01,610 --> 00:24:03,962
leave its mark on that starlight?

520
00:24:03,962 --> 00:24:05,470
(gentle upbeat music)

521
00:24:05,470 --> 00:24:08,410
My prediction was that gases in the planet atmosphere,

522
00:24:08,410 --> 00:24:11,093
or their signature, gets imprinted on the starlight.

523
00:24:12,430 --> 00:24:14,430
The molecules in the atmosphere

524
00:24:14,430 --> 00:24:17,200
should absorb certain wavelengths of starlight

525
00:24:17,200 --> 00:24:21,930
as it passes through, leaving telltale gaps in the spectrum.

526
00:24:21,930 --> 00:24:25,220
And by comparing the star when it's by itself

527
00:24:25,220 --> 00:24:27,090
to when the planet's in front of the star

528
00:24:27,090 --> 00:24:28,890
then we can then pick out what gases

529
00:24:28,890 --> 00:24:30,557
are in the planet atmosphere.

530
00:24:30,557 --> 00:24:33,230
(gentle upbeat music)

531
00:24:33,230 --> 00:24:35,060
It's not as straightforward as it sounds

532
00:24:35,060 --> 00:24:37,779
because the signal of the atmosphere is tiny.

533
00:24:37,779 --> 00:24:39,830
(gentle upbeat music)

534
00:24:39,830 --> 00:24:42,410
Think of the atmosphere like the skin of an onion

535
00:24:43,517 --> 00:24:48,517
and that whole onion in front of a giant, glowing backdrop.

536
00:24:48,614 --> 00:24:51,960
(gentle music)

537
00:24:51,960 --> 00:24:54,250
After years working on her theory,

538
00:24:54,250 --> 00:24:58,490
Sara finally proves the skeptics wrong in 2001,

539
00:24:58,490 --> 00:25:00,640
when the element sodium is detected

540
00:25:00,640 --> 00:25:04,883
in the clouds of a gas giant, 159 light years from Earth.

541
00:25:06,720 --> 00:25:09,300
Using my prediction, and it was the first time ever

542
00:25:09,300 --> 00:25:10,720
that an exoplanet atmosphere

543
00:25:10,720 --> 00:25:13,113
had been observed and identified.

544
00:25:15,110 --> 00:25:17,346
And that was just a wow moment.

545
00:25:17,346 --> 00:25:19,140
(gentle music)

546
00:25:19,140 --> 00:25:20,910
Sodium is quickly followed

547
00:25:20,910 --> 00:25:24,053
by other elements and molecules, including water,

548
00:25:24,950 --> 00:25:28,000
suggesting a tantalizing possibility,

549
00:25:28,000 --> 00:25:31,189
could a hot Jupiter host living organisms?

550
00:25:31,189 --> 00:25:33,120
(gentle music)

551
00:25:33,120 --> 00:25:35,320
All life as we know it needs liquid water.

552
00:25:36,460 --> 00:25:41,250
But the hot Jupiters, they're way too hot for water clouds.

553
00:25:41,250 --> 00:25:43,680
(gentle music)

554
00:25:43,680 --> 00:25:45,750
So close to its star,

555
00:25:45,750 --> 00:25:47,290
that means its surface temperature

556
00:25:47,290 --> 00:25:50,293
is probably above a thousand degrees Celsius.

557
00:25:52,650 --> 00:25:55,710
So there is water in hot Jupiter atmospheres,

558
00:25:55,710 --> 00:25:58,653
but it's just way too hot for liquid water.

559
00:26:00,110 --> 00:26:01,820
Which means there's no chance

560
00:26:01,820 --> 00:26:03,720
that there is life in the first place.

561
00:26:05,250 --> 00:26:08,263
Hot Jupiters are both exotic and deadly.

562
00:26:09,110 --> 00:26:11,971
But are they typical of all exoplanets?

563
00:26:11,971 --> 00:26:14,134
(gentle music)

564
00:26:14,134 --> 00:26:17,930
In the early 2000s, we definitely had a skewed view

565
00:26:17,930 --> 00:26:20,570
of planets and planetary systems.

566
00:26:20,570 --> 00:26:22,930
We could only find big planets,

567
00:26:22,930 --> 00:26:24,493
big planets close to the star.

568
00:26:25,500 --> 00:26:28,720
Gas giants like 51 Pegasi b were found

569
00:26:28,720 --> 00:26:31,673
because of their gravitational influence on their star,

570
00:26:32,640 --> 00:26:36,400
a method that works best for spotting, very large exoplanets

571
00:26:36,400 --> 00:26:38,570
in very tight orbits,

572
00:26:38,570 --> 00:26:42,170
and misses any small, rocky Earth-like worlds,

573
00:26:42,170 --> 00:26:44,095
if they exist at all.

574
00:26:44,095 --> 00:26:46,110
(gentle music)

575
00:26:46,110 --> 00:26:48,660
Hot Jupiters, they're interesting.

576
00:26:48,660 --> 00:26:49,493
But if you're saying,

577
00:26:49,493 --> 00:26:52,240
"I want to know about life and a galaxy."

578
00:26:52,240 --> 00:26:55,223
It is not the information you seek.

579
00:26:56,930 --> 00:26:58,330
The search for exoplanets

580
00:26:58,330 --> 00:27:01,763
capable of sustaining life will need a different approach.

581
00:27:03,550 --> 00:27:07,620
T-minus 10, nine, eight, seven,

582
00:27:07,620 --> 00:27:10,753
{\an8}six, five, four, three.

583
00:27:10,753 --> 00:27:13,226
Oh, oh my God.

584
00:27:13,226 --> 00:27:14,810
I can't believe it.

585
00:27:14,810 --> 00:27:16,030
(people laughing)

586
00:27:16,030 --> 00:27:19,180
In 2009, the Kepler space telescope

587
00:27:19,180 --> 00:27:20,883
launches from Cape Canaveral.

588
00:27:22,260 --> 00:27:24,140
(people laughing)

589
00:27:24,140 --> 00:27:27,570
Kepler was just a little, little, tiny mission

590
00:27:27,570 --> 00:27:29,677
that pokes its nose into the galaxy and says,

591
00:27:29,677 --> 00:27:30,957
"What's out there?"

592
00:27:31,887 --> 00:27:32,730
(gentle upbeat music)

593
00:27:32,730 --> 00:27:35,120
The Kepler mission is a sky survey

594
00:27:35,120 --> 00:27:37,810
dedicated to finding Earth-like exoplanets

595
00:27:37,810 --> 00:27:40,080
around Sun-like stars

596
00:27:40,080 --> 00:27:44,094
and is the brainchild of NASA scientist, Bill Borucki.

597
00:27:44,094 --> 00:27:45,170
(gentle upbeat music)

598
00:27:45,170 --> 00:27:46,510
We want to go into space.

599
00:27:46,510 --> 00:27:48,763
We wanna explore the stars.

600
00:27:49,690 --> 00:27:53,120
Finding the extent of intelligence in any universe.

601
00:27:53,120 --> 00:27:57,920
The only way you can do that is to prove ahead of time

602
00:27:57,920 --> 00:28:00,440
that most stars have planets.

603
00:28:00,440 --> 00:28:02,090
If there are no planets out there,

604
00:28:02,090 --> 00:28:03,335
there's no life out there.

605
00:28:03,335 --> 00:28:05,060
(gentle music)

606
00:28:05,060 --> 00:28:08,050
Borucki's plan is to detect small exoplanets

607
00:28:08,050 --> 00:28:10,320
as they transit their star,

608
00:28:10,320 --> 00:28:13,403
not individually, but on an incredible scale.

609
00:28:15,330 --> 00:28:18,570
The mission concept was to have a wide field of view,

610
00:28:18,570 --> 00:28:20,453
to observe many, many stars.

611
00:28:21,990 --> 00:28:24,402
A hundred thousand stars at one time.

612
00:28:24,402 --> 00:28:27,652
(gentle upbeat music)

613
00:28:28,940 --> 00:28:30,970
The technological challenge

614
00:28:30,970 --> 00:28:34,020
was to be able to detect minute changes.

615
00:28:34,020 --> 00:28:39,020
And by minute, I mean one part in a hundred thousand dip

616
00:28:39,760 --> 00:28:43,513
in the light of a star as the planet crossed in front of it.

617
00:28:44,880 --> 00:28:48,190
And can it do that all the way across

618
00:28:48,190 --> 00:28:50,924
that field of a hundred thousand stars?

619
00:28:50,924 --> 00:28:53,320
(gentle upbeat music)

620
00:28:53,320 --> 00:28:55,830
Bill first pitched his scheme to NASA

621
00:28:55,830 --> 00:28:58,900
in the 1980s, when technology had little chance

622
00:28:58,900 --> 00:29:00,193
of meeting the challenge.

623
00:29:01,062 --> 00:29:02,290
(gentle upbeat music)

624
00:29:02,290 --> 00:29:06,130
When Bill Borucki first proposed this crazy technique

625
00:29:06,130 --> 00:29:08,510
of looking for transits,

626
00:29:08,510 --> 00:29:10,560
I think it wasn't really taken seriously.

627
00:29:12,030 --> 00:29:15,880
In 1983, I used to walk into NASA headquarters

628
00:29:15,880 --> 00:29:18,640
telling them they had to fund this mission.

629
00:29:18,640 --> 00:29:20,220
And they would hide in their office,

630
00:29:20,220 --> 00:29:21,800
they would hide under their desks

631
00:29:21,800 --> 00:29:23,250
'cause I would harangue them.

632
00:29:25,080 --> 00:29:28,220
I have to say that Bill Borucki

633
00:29:28,220 --> 00:29:30,260
was one of the most tenacious

634
00:29:30,260 --> 00:29:33,340
and dedicated scientists I've come across.

635
00:29:33,340 --> 00:29:34,950
If you're in the space game,

636
00:29:34,950 --> 00:29:37,427
you've gotta be prepared for the long haul.

637
00:29:37,427 --> 00:29:38,860
(gentle upbeat music)

638
00:29:38,860 --> 00:29:43,430
But NASA was never gonna invest four or $500 million

639
00:29:43,430 --> 00:29:47,163
in a mission unless they knew for sure that this would work.

640
00:29:50,450 --> 00:29:54,320
The discovery of 51 Pegasi b in 1995,

641
00:29:54,320 --> 00:29:57,899
encourages NASA to take a chance with Bill's mission.

642
00:29:57,899 --> 00:29:59,550
(gentle music)

643
00:29:59,550 --> 00:30:02,390
Up to this point, people had speculated

644
00:30:02,390 --> 00:30:04,080
that there were planets around other stars,

645
00:30:04,080 --> 00:30:06,353
but no one had any empirical proof.

646
00:30:08,000 --> 00:30:10,880
The fact that there was a detection

647
00:30:11,760 --> 00:30:14,166
added scientific credibility.

648
00:30:14,166 --> 00:30:15,830
(gentle music)

649
00:30:15,830 --> 00:30:19,010
25 years after Bill conceived his mission,

650
00:30:19,010 --> 00:30:22,823
Kepler's search for Earth-like exoplanet is ready to begin.

651
00:30:24,258 --> 00:30:26,925
(gentle music)

652
00:30:28,740 --> 00:30:30,920
Far above the Earth's atmosphere,

653
00:30:30,920 --> 00:30:34,800
the telescope will enjoy a clear view of the Milky Way

654
00:30:34,800 --> 00:30:37,593
that ground-based astronomers can only dream of.

655
00:30:39,920 --> 00:30:42,270
Ambitious or foolhardy,

656
00:30:42,270 --> 00:30:44,403
nothing like it has been tried before.

657
00:30:45,580 --> 00:30:47,970
But finally, we look at the stars

658
00:30:48,900 --> 00:30:52,083
and there are 10s of billions of stars shining.

659
00:30:53,170 --> 00:30:54,691
It's beautiful.

660
00:30:54,691 --> 00:30:57,150
(upbeat music)

661
00:30:57,150 --> 00:30:59,330
And within a few hours, the data shows

662
00:30:59,330 --> 00:31:03,350
that one of the stars that we know has a planet,

663
00:31:03,350 --> 00:31:04,798
shows a transit.

664
00:31:04,798 --> 00:31:06,140
(upbeat music)

665
00:31:06,140 --> 00:31:07,230
The exoplanet

666
00:31:07,230 --> 00:31:10,593
is an incredible 750 light years from Earth.

667
00:31:11,500 --> 00:31:15,080
And Kepler passes its first test.

668
00:31:15,080 --> 00:31:17,573
And that told us this instrument's working.

669
00:31:18,430 --> 00:31:20,400
And we were so delighted.

670
00:31:20,400 --> 00:31:22,193
Just ecstatic.

671
00:31:25,390 --> 00:31:27,820
Finding an exoplanet you already know about

672
00:31:27,820 --> 00:31:29,160
is one thing,

673
00:31:29,160 --> 00:31:32,519
but Bill's sky survey is a huge gamble.

674
00:31:32,519 --> 00:31:33,800
(gentle music)

675
00:31:33,800 --> 00:31:35,610
Transit technique only works

676
00:31:35,610 --> 00:31:38,910
when that planet is rotating in exactly the same plane

677
00:31:38,910 --> 00:31:40,150
that you're looking at.

678
00:31:40,150 --> 00:31:44,223
You're basically eliminating 99% of the stars.

679
00:31:45,430 --> 00:31:49,090
But even so there were so many stars with planets

680
00:31:49,090 --> 00:31:50,770
that the transit technique

681
00:31:50,770 --> 00:31:52,783
was just finding dozens and dozens.

682
00:31:54,230 --> 00:31:56,910
All it does is take picture, after picture, after picture,

683
00:31:56,910 --> 00:32:00,130
every six seconds, the same field of view, the same stars.

684
00:32:00,130 --> 00:32:03,010
It's designed to be the most boring mission

685
00:32:03,010 --> 00:32:04,605
that has ever built.

686
00:32:04,605 --> 00:32:06,340
(gentle music)

687
00:32:06,340 --> 00:32:08,290
At the core of the Kepler mission

688
00:32:08,290 --> 00:32:11,270
is Bill's desire to find Earth-like planets

689
00:32:11,270 --> 00:32:13,732
in the habitable zone of their star.

690
00:32:13,732 --> 00:32:15,580
(gentle music)

691
00:32:15,580 --> 00:32:18,400
Also known as the Goldilocks Zone,

692
00:32:18,400 --> 00:32:21,900
this is the region that is neither too hot nor too cold

693
00:32:21,900 --> 00:32:23,530
for liquid water.

694
00:32:23,530 --> 00:32:26,460
Where life, as we know it, can thrive.

695
00:32:26,460 --> 00:32:29,050
The mission was tuned very, very carefully,

696
00:32:29,050 --> 00:32:31,740
Earth-like planets in the habitable zone,

697
00:32:31,740 --> 00:32:34,233
where water could exist on the surface.

698
00:32:35,470 --> 00:32:38,270
Kepler needs to observe three or four transits

699
00:32:38,270 --> 00:32:40,770
to confirm an exoplanet detection,

700
00:32:40,770 --> 00:32:43,180
so needs to last three or four years

701
00:32:43,180 --> 00:32:44,943
to catch Earth-like orbits.

702
00:32:46,000 --> 00:32:48,770
The whole thing was so fundamental and groundbreaking

703
00:32:48,770 --> 00:32:51,910
because Bill's not just detecting planets,

704
00:32:51,910 --> 00:32:54,740
but then finding the subset of planets

705
00:32:54,740 --> 00:32:56,740
that were in the habitable zone,

706
00:32:56,740 --> 00:32:59,485
where life might have appeared.

707
00:32:59,485 --> 00:33:03,299
(gentle upbeat music)

708
00:33:03,299 --> 00:33:05,580
In the lobbies of our main administrative building,

709
00:33:05,580 --> 00:33:07,610
we had a chart which had indicators,

710
00:33:07,610 --> 00:33:10,490
which would show you how many exoplanets were discovered,

711
00:33:10,490 --> 00:33:13,390
how many exoplanets were discovered in the habitable zone.

712
00:33:14,610 --> 00:33:15,990
These numbers would grow and grow and grow,

713
00:33:15,990 --> 00:33:16,950
and we'd suddenly discover

714
00:33:16,950 --> 00:33:18,380
that we didn't have enough digits

715
00:33:18,380 --> 00:33:21,414
to encompass all the planets that were being discovered.

716
00:33:21,414 --> 00:33:25,350
(gentle upbeat music)

717
00:33:25,350 --> 00:33:27,640
We're here today to announce new discoveries

718
00:33:27,640 --> 00:33:29,530
from NASA's Kepler mission.

719
00:33:29,530 --> 00:33:32,360
After four years staring into the Milky Way,

720
00:33:32,360 --> 00:33:35,450
Bill Borucki is ready to reveal his top picks

721
00:33:35,450 --> 00:33:38,113
from the hundreds of planets discovered so far.

722
00:33:39,210 --> 00:33:42,240
Today of like to announce, we have found two planets,

723
00:33:42,240 --> 00:33:44,650
that in a habitable zone of another star,

724
00:33:44,650 --> 00:33:47,370
and they are the best candidates found to date.

725
00:33:47,370 --> 00:33:50,520
They may have the possibility of water as well.

726
00:33:50,520 --> 00:33:53,310
(audience applauds)

727
00:33:53,310 --> 00:33:55,890
More than 1200 light years away,

728
00:33:55,890 --> 00:33:59,580
the most Earth-like of the two is called Kepler-62f

729
00:34:00,660 --> 00:34:04,260
and Borucki's data suggests it could be a water world

730
00:34:04,260 --> 00:34:06,623
completely covered by a vast ocean.

731
00:34:08,096 --> 00:34:10,440
(water gushing)

732
00:34:10,440 --> 00:34:13,080
The reason that we call it, perhaps a water world,

733
00:34:13,080 --> 00:34:17,200
is because given its mass and radius, it could in fact

734
00:34:17,200 --> 00:34:21,243
harbor a huge envelope of water on the surface.

735
00:34:21,243 --> 00:34:23,810
(gentle music)

736
00:34:23,810 --> 00:34:27,210
All sorts of life could exist in that ocean.

737
00:34:27,210 --> 00:34:29,010
Could you have all sorts of little creatures

738
00:34:29,010 --> 00:34:30,220
and fish to eat them,

739
00:34:30,220 --> 00:34:31,960
and fish that don't want to be eaten,

740
00:34:31,960 --> 00:34:33,900
so they learn to fly out of the ocean,

741
00:34:33,900 --> 00:34:35,925
like our flying fish do?

742
00:34:35,925 --> 00:34:37,370
(gentle music)

743
00:34:37,370 --> 00:34:40,313
Kepler-62f was certainly a high point.

744
00:34:41,250 --> 00:34:43,030
We were delighted to find that.

745
00:34:43,030 --> 00:34:45,600
And so were our sponsors at NASA headquarters

746
00:34:45,600 --> 00:34:46,955
who paid for this.

747
00:34:46,955 --> 00:34:49,460
(audience applauds)

748
00:34:49,460 --> 00:34:51,020
But behind the scenes,

749
00:34:51,020 --> 00:34:53,770
the Kepler mission faces a crisis.

750
00:34:53,770 --> 00:34:57,210
The telescope's ability to stare at the same patch of sky

751
00:34:57,210 --> 00:35:00,060
depends on four gyroscopic stabilizers

752
00:35:00,060 --> 00:35:01,913
called reaction wheels.

753
00:35:02,910 --> 00:35:05,429
That guidance system was so good,

754
00:35:05,429 --> 00:35:08,260
the image of the same star sent a same pixel,

755
00:35:08,260 --> 00:35:10,560
month after a month.

756
00:35:10,560 --> 00:35:15,030
But in 2013, two of the reaction wheels fail.

757
00:35:15,030 --> 00:35:17,010
That meant we could no longer point

758
00:35:17,010 --> 00:35:18,483
at that area of the sky.

759
00:35:19,400 --> 00:35:23,040
Telescope still worked, but we couldn't point there anymore.

760
00:35:25,720 --> 00:35:28,877
Really, really a tense, tense period.

761
00:35:28,877 --> 00:35:30,250
(upbeat music)

762
00:35:30,250 --> 00:35:31,870
I thought the mission was done for.

763
00:35:31,870 --> 00:35:33,950
I thought, well, got a good run,

764
00:35:33,950 --> 00:35:36,193
got a lot of good data, but it's done for.

765
00:35:37,070 --> 00:35:39,210
But Borucki is not done yet.

766
00:35:39,210 --> 00:35:41,257
Perhaps the mission can be salvaged.

767
00:35:41,257 --> 00:35:42,190
(upbeat music)

768
00:35:42,190 --> 00:35:45,900
The team sent out an all-points bulletin,

769
00:35:45,900 --> 00:35:49,313
you know, "Help, help, help" to the aerospace community.

770
00:35:51,060 --> 00:35:53,810
All objects in space feel a slight push

771
00:35:53,810 --> 00:35:55,590
from the light of the Sun,

772
00:35:55,590 --> 00:35:57,963
a phenomenon called solar pressure.

773
00:35:59,070 --> 00:36:03,320
Bill learns that this might be the solution to the problem.

774
00:36:03,320 --> 00:36:04,387
The engineers have pointed out,

775
00:36:04,387 --> 00:36:06,167
"You know, we've got two wheels

776
00:36:06,167 --> 00:36:09,533
"and we've got the Sun shining, pushing on the spacecraft.

777
00:36:10,937 --> 00:36:14,896
"We'll arrange it so the Sun acts like one of the wheels."

778
00:36:14,896 --> 00:36:16,490
(upbeat music)

779
00:36:16,490 --> 00:36:19,210
Each square meter of a satellite like Kepler

780
00:36:19,210 --> 00:36:21,700
feels solar pressure equivalent to the weight

781
00:36:21,700 --> 00:36:23,143
of a grain of salt on Earth.

782
00:36:24,200 --> 00:36:27,530
The engineers hope that this tiny force will be enough

783
00:36:27,530 --> 00:36:30,390
to stabilize the drifting telescope.

784
00:36:30,390 --> 00:36:32,030
(upbeat music)

785
00:36:32,030 --> 00:36:36,550
Clever idea, the way you use the very pressure

786
00:36:36,550 --> 00:36:39,150
of the radiation from the Sun

787
00:36:39,150 --> 00:36:43,300
as a countervailing force and thereby maintain stability

788
00:36:43,300 --> 00:36:45,240
and extend the life of the mission,

789
00:36:45,240 --> 00:36:46,653
to collect even more data.

790
00:36:47,970 --> 00:36:50,610
The ingenious fix is a success,

791
00:36:50,610 --> 00:36:52,330
but stabilizes the telescope

792
00:36:52,330 --> 00:36:55,040
for much shorter periods than before,

793
00:36:55,040 --> 00:36:56,943
with consequences for the mission.

794
00:36:58,010 --> 00:37:00,220
You could find short period of planets,

795
00:37:00,220 --> 00:37:02,330
giant plants with one or two orbits,

796
00:37:02,330 --> 00:37:06,690
but it didn't allow us to continue the original mission

797
00:37:06,690 --> 00:37:08,556
for finding Earths.

798
00:37:08,556 --> 00:37:11,139
(gentle music)

799
00:37:12,640 --> 00:37:13,740
We needed more time.

800
00:37:14,998 --> 00:37:16,620
And so we were not able to find

801
00:37:16,620 --> 00:37:20,213
that possibly true Earth analog.

802
00:37:21,300 --> 00:37:24,080
On October the 30th, 2018,

803
00:37:24,080 --> 00:37:27,330
the Kepler space telescope runs out of fuel.

804
00:37:27,330 --> 00:37:30,310
(gentle music)

805
00:37:30,310 --> 00:37:33,070
The mission accomplished its objective.

806
00:37:33,070 --> 00:37:37,228
So, okay, it died, it did its job.

807
00:37:37,228 --> 00:37:38,510
(gentle music)

808
00:37:38,510 --> 00:37:42,620
The Kepler discovers over 2,600 exoplanets

809
00:37:42,620 --> 00:37:45,290
with several hundred in the habitable zone.

810
00:37:45,290 --> 00:37:48,540
But the real surprise is the incredible diversity

811
00:37:48,540 --> 00:37:49,593
of these worlds.

812
00:37:51,120 --> 00:37:53,850
Kepler found so many new types of planets,

813
00:37:53,850 --> 00:37:56,660
just wow, opened up our eyes.

814
00:37:56,660 --> 00:37:59,330
The planetary systems weren't like ours at all.

815
00:37:59,330 --> 00:38:02,260
They had at big planets were we had little planets.

816
00:38:02,260 --> 00:38:04,850
Giant planets, bigger than Jupiter,

817
00:38:04,850 --> 00:38:07,636
little tiny planets disintegrating.

818
00:38:07,636 --> 00:38:09,340
(gentle music)

819
00:38:09,340 --> 00:38:13,400
Kepler really showed that there's an interstellar zoo

820
00:38:13,400 --> 00:38:15,565
of planetary worlds.

821
00:38:15,565 --> 00:38:16,920
(gentle music)

822
00:38:16,920 --> 00:38:20,110
The types of exoplanets that exist out there

823
00:38:20,110 --> 00:38:22,828
it's really, as far as your imagination can reach.

824
00:38:22,828 --> 00:38:24,850
(gentle upbeat music)

825
00:38:24,850 --> 00:38:26,880
At NASA's jet propulsion lab,

826
00:38:26,880 --> 00:38:29,770
observational data from surveys like Kepler

827
00:38:29,770 --> 00:38:31,980
is used to model the conditions

828
00:38:31,980 --> 00:38:35,403
on some of the extraordinary worlds in the cosmic zoo.

829
00:38:36,826 --> 00:38:39,270
It's really taking what data we have available to us,

830
00:38:39,270 --> 00:38:41,330
and then using our imagination

831
00:38:41,330 --> 00:38:43,300
to try and understand what their weather,

832
00:38:43,300 --> 00:38:44,880
what their atmospheres might be like.

833
00:38:44,880 --> 00:38:46,810
And really start to hammer down

834
00:38:46,810 --> 00:38:48,860
on whether or not there's life out there.

835
00:38:50,200 --> 00:38:51,230
The number crunching

836
00:38:51,230 --> 00:38:53,690
has led to some astonishing conclusions

837
00:38:53,690 --> 00:38:56,283
about the exoplanets in our backyard.

838
00:38:57,600 --> 00:39:00,500
55 Cancri e, what's not imagination

839
00:39:00,500 --> 00:39:04,620
is the fact that we can actually see the star by eye.

840
00:39:04,620 --> 00:39:05,610
(gentle music)

841
00:39:05,610 --> 00:39:09,350
40 light years away, 55 Cancri e

842
00:39:09,350 --> 00:39:11,859
is twice the size of Earth.

843
00:39:11,859 --> 00:39:14,490
(gentle music)

844
00:39:14,490 --> 00:39:17,503
It's in a ridiculously close orbit around its star.

845
00:39:18,970 --> 00:39:22,973
So surface temperatures might well be above 1,000 Calvin.

846
00:39:25,880 --> 00:39:29,500
So when I think of 55 Cancri e, I just think of lava.

847
00:39:29,500 --> 00:39:30,590
(laughing)

848
00:39:30,590 --> 00:39:34,492
None of the solids on the surface are able to stay solid.

849
00:39:34,492 --> 00:39:36,300
(gentle music)

850
00:39:36,300 --> 00:39:39,500
The lavas way too hard to remain liquid all the time.

851
00:39:39,500 --> 00:39:43,283
So there will be some kind of silicate gas as well.

852
00:39:44,210 --> 00:39:46,390
On the backside of the planet,

853
00:39:46,390 --> 00:39:51,000
it might well be that the gaseous rock steam atmosphere

854
00:39:51,000 --> 00:39:54,890
forms droplets, and actually rains out.

855
00:39:54,890 --> 00:39:55,960
And what does it rain out?

856
00:39:55,960 --> 00:39:57,483
Then of course rocks.

857
00:39:58,430 --> 00:40:01,842
So that's a very weird atmospheric scenario.

858
00:40:01,842 --> 00:40:04,425
(gentle music)

859
00:40:06,520 --> 00:40:09,070
Despite the apocalyptic conditions,

860
00:40:09,070 --> 00:40:12,233
this could be the most precious exoplanet yet discovered.

861
00:40:13,313 --> 00:40:16,680
If you look at the star that 55 Cancri e is orbiting,

862
00:40:16,680 --> 00:40:20,470
is actually a lot more carbon-rich than that at the Sun.

863
00:40:20,470 --> 00:40:24,119
So 55 Cancri e might be a carbon world.

864
00:40:24,119 --> 00:40:25,660
(gentle upbeat music)

865
00:40:25,660 --> 00:40:27,870
What happens in a planetary system

866
00:40:27,870 --> 00:40:30,530
where there's more carbon than oxygen,

867
00:40:30,530 --> 00:40:32,470
there could be a layer or part of the planet

868
00:40:32,470 --> 00:40:34,219
that has diamonds.

869
00:40:34,219 --> 00:40:35,950
(gentle upbeat music)

870
00:40:35,950 --> 00:40:38,257
These are real places we can point to and say,

871
00:40:38,257 --> 00:40:41,367
"Yeah, this indeed is a planet that'll rain,

872
00:40:41,367 --> 00:40:44,766
"you know, diamonds, or has a surface of liquid lava."

873
00:40:44,766 --> 00:40:45,850
(gentle upbeat music)

874
00:40:45,850 --> 00:40:48,250
These are the worlds that exist in our universe.

875
00:40:50,300 --> 00:40:53,830
55 Cancri e is a nightmare world

876
00:40:53,830 --> 00:40:56,360
where life must be impossible.

877
00:40:56,360 --> 00:40:59,270
But in 2017 and equally bizarre,

878
00:40:59,270 --> 00:41:02,820
but utterly different planetary system is discovered

879
00:41:02,820 --> 00:41:05,560
at about the same distance from Earth.

880
00:41:05,560 --> 00:41:06,710
TRAPPIST-1 is a system

881
00:41:06,710 --> 00:41:11,433
comprised of seven closely-packed planets

882
00:41:11,433 --> 00:41:14,130
that are all roughly Earth-sized,

883
00:41:14,130 --> 00:41:17,222
orbiting what's called an M dwarf star.

884
00:41:17,222 --> 00:41:18,710
(gentle music)

885
00:41:18,710 --> 00:41:20,370
The TRAPPIST-1 system is exciting

886
00:41:20,370 --> 00:41:22,920
because it looks like our solar system.

887
00:41:22,920 --> 00:41:25,200
It's got a whole bunch of planets

888
00:41:25,200 --> 00:41:29,801
and maybe two or three of them are in a habitable zone.

889
00:41:29,801 --> 00:41:31,610
(gentle upbeat music)

890
00:41:31,610 --> 00:41:33,030
And that's really exciting.

891
00:41:33,030 --> 00:41:34,570
It's just, you know, this is the model

892
00:41:34,570 --> 00:41:36,550
that we all had in our minds

893
00:41:36,550 --> 00:41:38,650
of what could happen around all the stars.

894
00:41:40,290 --> 00:41:44,830
The star itself is a much cooler, redder

895
00:41:44,830 --> 00:41:47,290
and smaller star than the Sun.

896
00:41:47,290 --> 00:41:49,870
And indeed the solar system around TRAPPIST

897
00:41:49,870 --> 00:41:52,000
is tucked in closer to this star.

898
00:41:52,000 --> 00:41:54,850
You get the same kind of temperatures you get from Earth.

899
00:41:56,630 --> 00:41:58,480
This mini solar system

900
00:41:58,480 --> 00:42:01,010
could even have liquid water oceans.

901
00:42:01,010 --> 00:42:02,340
(gentle upbeat music)

902
00:42:02,340 --> 00:42:04,540
The orbital configuration indicates

903
00:42:04,540 --> 00:42:06,610
the planets may have migrated

904
00:42:06,610 --> 00:42:08,758
from further from their star, originally.

905
00:42:08,758 --> 00:42:10,440
(upbeat music)

906
00:42:10,440 --> 00:42:11,850
And so they've had the opportunity

907
00:42:11,850 --> 00:42:13,893
to accumulate a lot of ice,

908
00:42:14,860 --> 00:42:17,133
which then melted to form water.

909
00:42:21,100 --> 00:42:22,830
So if it were possible to stand

910
00:42:22,830 --> 00:42:25,100
or float on a TRAPPIST-1 planet,

911
00:42:25,100 --> 00:42:28,260
then you would see the star is much closer,

912
00:42:28,260 --> 00:42:31,349
but it's also dimer and redder than our own Sun.

913
00:42:31,349 --> 00:42:33,192
(upbeat music)

914
00:42:33,192 --> 00:42:35,380
You wouldn't just have a moon in the sky,

915
00:42:35,380 --> 00:42:37,980
but instead you'd be seeing the neighboring planets.

916
00:42:39,070 --> 00:42:41,030
Everything that we would see was our human eye

917
00:42:41,030 --> 00:42:41,973
would be red.

918
00:42:43,030 --> 00:42:44,190
Plants with green leaves,

919
00:42:44,190 --> 00:42:46,080
they would appear black to our eye.

920
00:42:46,080 --> 00:42:48,498
I mean, everything is exotic.

921
00:42:48,498 --> 00:42:49,360
(upbeat music)

922
00:42:49,360 --> 00:42:52,860
M Dwarf stars, like TRAPPIST-1 are so dim

923
00:42:52,860 --> 00:42:55,920
that from Earth they're to the naked eye,

924
00:42:55,920 --> 00:42:59,330
but they're the most common type of star in the galaxy,

925
00:42:59,330 --> 00:43:02,193
outnumbering Sun-like stars 10 to one.

926
00:43:03,350 --> 00:43:05,280
This is the majority of stars out there.

927
00:43:05,280 --> 00:43:06,810
And the majority of stars

928
00:43:06,810 --> 00:43:08,760
might have these little mini solar systems

929
00:43:08,760 --> 00:43:10,573
with habitable, like planets.

930
00:43:11,970 --> 00:43:13,210
TRAPPIST-1 offers

931
00:43:13,210 --> 00:43:15,223
a recognizable template for life.

932
00:43:16,060 --> 00:43:18,730
But could recent observations of our nearest star,

933
00:43:18,730 --> 00:43:23,000
Proxima Centauri, suggest we already have neighbors.

934
00:43:23,000 --> 00:43:25,583
(upbeat music)

935
00:43:27,940 --> 00:43:29,720
Proxima Centauri b, I think,

936
00:43:29,720 --> 00:43:31,950
has captured a lot of people's imagination

937
00:43:31,950 --> 00:43:35,760
because it's one of the closest systems we can investigate.

938
00:43:35,760 --> 00:43:37,883
It's only four light years away.

939
00:43:39,450 --> 00:43:40,700
It's in the habitable zone.

940
00:43:40,700 --> 00:43:41,860
So as heated by the star,

941
00:43:41,860 --> 00:43:44,203
it should be the right temperature for life.

942
00:43:45,150 --> 00:43:48,263
Sounds positive, but then things get weird.

943
00:43:50,610 --> 00:43:55,610
We think that it is tightly locked to its star,

944
00:43:55,720 --> 00:43:59,010
like the moon is locked to the Earth.

945
00:43:59,010 --> 00:44:03,503
That means one hemisphere is facing the star permanently.

946
00:44:05,190 --> 00:44:06,170
So could a world

947
00:44:06,170 --> 00:44:09,610
split between permanent day and eternal night,

948
00:44:09,610 --> 00:44:11,364
ever support life?

949
00:44:11,364 --> 00:44:13,520
(gentle upbeat music)

950
00:44:13,520 --> 00:44:16,500
We think any water on Proxima Centauri b

951
00:44:16,500 --> 00:44:19,613
would probably end up on the night side and frozen.

952
00:44:21,460 --> 00:44:23,760
But ice that's forming on the night side

953
00:44:23,760 --> 00:44:25,950
could start to creep towards the day side,

954
00:44:25,950 --> 00:44:28,003
and it would start to melt.

955
00:44:28,848 --> 00:44:32,015
(gentle upbeat music)

956
00:44:33,050 --> 00:44:36,260
There is a region, a rim or a ring

957
00:44:36,260 --> 00:44:39,590
around the planet that we refer to as The Terminator,

958
00:44:39,590 --> 00:44:41,680
The Terminator zone, the transition zone

959
00:44:41,680 --> 00:44:44,220
between bright and dark,

960
00:44:44,220 --> 00:44:47,040
where the conditions might be just very favorable

961
00:44:47,040 --> 00:44:49,195
for life to have formed.

962
00:44:49,195 --> 00:44:51,130
(gentle upbeat music)

963
00:44:51,130 --> 00:44:52,940
These organisms would have to deal

964
00:44:52,940 --> 00:44:56,130
with the perils of being so close to their star.

965
00:44:56,130 --> 00:44:58,563
A particularly volatile red dwarf.

966
00:45:00,080 --> 00:45:03,060
Though the smallest and dimmest kind of star,

967
00:45:03,060 --> 00:45:05,600
at less than 5 billion years old,

968
00:45:05,600 --> 00:45:10,020
Proxima Centauri is very young for a red dwarf

969
00:45:10,020 --> 00:45:12,593
and is prone to violent outbursts.

970
00:45:13,830 --> 00:45:17,320
When a red dwarf is young, it emits a lot more radiation,

971
00:45:17,320 --> 00:45:18,932
including stellar flares.

972
00:45:18,932 --> 00:45:20,150
(upbeat music)

973
00:45:20,150 --> 00:45:23,753
So the planet's also going to be blasted with radiation.

974
00:45:24,620 --> 00:45:28,900
Proxima Centauri b may be getting flared every week,

975
00:45:28,900 --> 00:45:32,000
but the flare probably wouldn't kill life.

976
00:45:32,000 --> 00:45:33,920
You know, there's always the dark side of the planet.

977
00:45:33,920 --> 00:45:36,190
There's always the oceans, if there are oceans.

978
00:45:36,190 --> 00:45:38,470
So I'm not too worried about life itself,

979
00:45:38,470 --> 00:45:39,700
not being able to survive.

980
00:45:39,700 --> 00:45:42,533
It just will create a very tricky landscape.

981
00:45:44,760 --> 00:45:46,480
The violent stellar activity

982
00:45:46,480 --> 00:45:49,540
could also create a spectacular light show

983
00:45:49,540 --> 00:45:52,374
for those brave enough to venture out.

984
00:45:52,374 --> 00:45:53,980
(gentle upbeat music)

985
00:45:53,980 --> 00:45:55,540
It could be that there's periodically

986
00:45:55,540 --> 00:45:57,300
a transfer of high energy particles

987
00:45:57,300 --> 00:45:58,700
from the star to the planet,

988
00:45:59,680 --> 00:46:01,980
creating an Aurora that might be ever present.

989
00:46:03,120 --> 00:46:05,730
So could Proxima Centauri b,

990
00:46:05,730 --> 00:46:07,333
be a home from home?

991
00:46:09,690 --> 00:46:12,532
Well, Proxima Centauri b is the closest world,

992
00:46:12,532 --> 00:46:15,004
other than our solar system.

993
00:46:15,004 --> 00:46:16,390
(gentle upbeat music)

994
00:46:16,390 --> 00:46:20,980
So one of the first places that humankind will explore,

995
00:46:20,980 --> 00:46:25,076
if we go interstellar will be Proxima Centauri b.

996
00:46:25,076 --> 00:46:26,630
(gentle upbeat music)

997
00:46:26,630 --> 00:46:30,130
In Proxima Centauri b we could discover

998
00:46:30,130 --> 00:46:33,550
that Earth really does have a twin,

999
00:46:33,550 --> 00:46:35,303
just not an identical twin.

1000
00:46:36,419 --> 00:46:38,760
(gentle music)

1001
00:46:38,760 --> 00:46:42,350
Progress in exoplanet research is staggering,

1002
00:46:42,350 --> 00:46:44,670
but everything we know has been discovered

1003
00:46:44,670 --> 00:46:46,063
in a single generation.

1004
00:46:47,630 --> 00:46:50,320
We take for granted that there are exoplanets

1005
00:46:50,320 --> 00:46:52,360
orbiting around other stars.

1006
00:46:52,360 --> 00:46:56,638
And yet only a few decades ago, we had not seen one.

1007
00:46:56,638 --> 00:46:59,120
(gentle music)

1008
00:46:59,120 --> 00:47:01,370
{\an8}Less than 40 years after Richard Terrile

1009
00:47:01,370 --> 00:47:05,520
{\an8}photographed the fuzzy debris disc around Beta Pictoris,

1010
00:47:05,520 --> 00:47:07,940
this astonishing footage of an exoplanet

1011
00:47:07,940 --> 00:47:11,225
actually orbiting the star was released.

1012
00:47:11,225 --> 00:47:14,330
(gentle music)

1013
00:47:14,330 --> 00:47:17,350
We've come from these crude images in a coronagraph

1014
00:47:17,350 --> 00:47:20,943
to actually seeing an exoplanet orbiting that star.

1015
00:47:21,961 --> 00:47:23,860
It's very, very exciting to see that progression,

1016
00:47:23,860 --> 00:47:26,347
see that evolution of our knowledge.

1017
00:47:26,347 --> 00:47:27,230
(gentle music)

1018
00:47:27,230 --> 00:47:30,490
Beta Pictoris b, it's actually called a super Jupiter

1019
00:47:30,490 --> 00:47:33,300
because it's more massive than Jupiter.

1020
00:47:33,300 --> 00:47:34,660
We've also been able to measure

1021
00:47:34,660 --> 00:47:36,663
the rotation rate of the planet.

1022
00:47:37,630 --> 00:47:39,380
This might actually resemble Jupiter,

1023
00:47:39,380 --> 00:47:41,800
in that it should have a lot of bands and vortices

1024
00:47:41,800 --> 00:47:43,963
that rotate in the atmosphere.

1025
00:47:43,963 --> 00:47:46,730
(gentle music)

1026
00:47:46,730 --> 00:47:47,790
We were the first to see it.

1027
00:47:47,790 --> 00:47:51,239
And now it's to this interstellar zoo.

1028
00:47:51,239 --> 00:47:53,200
(gentle music)

1029
00:47:53,200 --> 00:47:55,480
It's a great thing to have on your resume.

1030
00:47:55,480 --> 00:47:57,020
(gentle music)

1031
00:47:57,020 --> 00:47:58,800
Every advance in technology

1032
00:47:58,800 --> 00:48:02,490
has added new detail to the exoplanet story,

1033
00:48:02,490 --> 00:48:06,186
but are we any closer to answering the big question?

1034
00:48:06,186 --> 00:48:08,200
(gentle music)

1035
00:48:08,200 --> 00:48:11,323
Are we at the cusp of finding life today?

1036
00:48:14,490 --> 00:48:16,270
I would say no,

1037
00:48:16,270 --> 00:48:18,010
but we have a roadmap.

1038
00:48:18,010 --> 00:48:20,430
We know what we are looking for.

1039
00:48:20,430 --> 00:48:23,110
And we are developing the technology

1040
00:48:23,110 --> 00:48:25,110
to look for those traces

1041
00:48:25,110 --> 00:48:28,025
that we think could be evidence of life.

1042
00:48:28,025 --> 00:48:28,890
(gentle music)

1043
00:48:28,890 --> 00:48:31,120
We look at the missions that are being planned,

1044
00:48:31,120 --> 00:48:33,070
that are such huge telescopes,

1045
00:48:33,070 --> 00:48:35,373
that we can see the atmospheres of planets.

1046
00:48:36,390 --> 00:48:37,980
What's in that atmosphere?

1047
00:48:37,980 --> 00:48:39,483
Is there some signs of life?

1048
00:48:40,430 --> 00:48:42,003
Maybe even see the planets?

1049
00:48:42,890 --> 00:48:46,090
Well, we see the ingredients for life everywhere,

1050
00:48:46,090 --> 00:48:48,460
but most of the universe is, I would say,

1051
00:48:48,460 --> 00:48:49,823
hostile towards life.

1052
00:48:51,060 --> 00:48:53,160
But I don't know, I don't feel the need to speculate.

1053
00:48:53,160 --> 00:48:54,640
The great thing about astronomy

1054
00:48:54,640 --> 00:48:58,293
is it won't be long before we have better answers.

1055
00:48:59,460 --> 00:49:01,850
And that all of our speculations and dreams,

1056
00:49:01,850 --> 00:49:04,637
we can see which one of those are real.

1057
00:49:04,637 --> 00:49:07,038
(gentle music)

1058
00:49:07,038 --> 00:49:10,413
The universe is far more exciting than it was 40 years ago

1059
00:49:10,413 --> 00:49:13,350
when our imaginations didn't comprehend

1060
00:49:13,350 --> 00:49:15,350
the different environments that we have.

1061
00:49:16,230 --> 00:49:19,230
But I think the future is also gonna be very, very exciting.

1062
00:49:20,090 --> 00:49:22,970
You know, this first step was finding planets,

1063
00:49:22,970 --> 00:49:25,274
the next step is finding life.

1064
00:49:25,274 --> 00:49:27,857
(gentle music)

