Richard Hammond Builds a Universe Richard Hammond Builds a Planet


Richard Hammond Builds a Universe

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Planet Earth.

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Our home.

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It's unique.

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It has life.

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But what's amazing, is none of it would exist without the sun,

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the moon and the stars around us.

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We are connected to the universe in the most fundamental ways.

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To find out how, I'm going to have to build my own.

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I'm going to open up a cosmic tool-box and work it out.

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And I'm going to build my universe up here,

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at the top of this impossibly high tower.

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It gives us the perfect platform to make something really big.

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Up here, we can do in seconds

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what it takes nature millions or billions of years to do.

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And to build a universe, I'm going to need a lot of help.

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I'll be honest, I'm faintly nervous.

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Was that it?

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Wow! Beautiful!

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Ohh, this is really difficult!

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I told you, seventies' moves! There they are.

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Like any construction project, there will be mistakes...

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..but from those mistakes, we'll get real insights into what

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makes our universe exactly right for us to exist.

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As an engineering challenge,

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this is about as big as it gets.

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How many times have you marvelled at the stars?

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Depending upon your frame of mind, the stars might appear distant

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and magical, or cold and remote, but the fact is, we are all

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made of the same stuff. And if you were to change anything about them,

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or about us, that connection, that delicate balance, would be lost.

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And this isn't an idle fancy, a romantic notion,

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it's essential, elemental and real.

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Without that connection, we wouldn't be here.'

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And to understand how it works, we need to build a universe.

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It's not a small task...

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..because Earth is in a solar system...

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..which is in just one tiny part of a galaxy...

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..that has over 300 billion stars within it.

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And there are half a trillion galaxies in the universe.

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So the job isn't really done until we build it all,

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from suns to galaxies.

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I'm going to need to construct all of this up here,

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at the top of my tower,

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where there's loads of room.

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To do this, we need to go back to the very start of everything.

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We need to start from scratch.

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In the case of our universe,

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the start of everything was 13.8 billion years ago...

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about.

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I do like a challenge.

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Most scientists agree that before the universe, there was nothing,

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nada.

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But out of that nothing, was created something...

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everything. It all happened in an event called the big bang.

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Thing is, the big bang is actually a misleading name for it

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because it wasn't a bang at all.

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There is an analogy that scientists

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and boffins use to get their head round this event.

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There's no explosion. It wasn't a bang.

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It's more like a balloon.

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The big bang was a rapid expansion, just like inflating a balloon.

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Now, of course, the universe expanded

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a lot quicker than our balloon.

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Unimaginably so.

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In a billionth of a second,

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it was already the size of our solar system.

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But you take the point.

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It's like a big expanding bubble of space.

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But there's something even more bizarre about the big bang.

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That universal expansion had no single point of origin.

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It happened everywhere and all at the same time.

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So one balloon isn't enough to demonstrate it.

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I need countless balloons.

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What's more, the expansion of the big bang is still happening today...

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..which means that wherever I am,

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I'm at the very centre of an expanding universe.

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And wherever you are, you, too, are at the centre of the universe.

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So we've had our big bang, but there is a little problem.

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It's dark.

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There is no light after a big bang because there are no stars.

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So, where can I get a star from?

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Well, fortunately, it turns out they make them

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just off the M40 near Oxford.

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BUZZING AND BEEPING

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Inside this billion-pound

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chamber...

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..we're going to squeeze,

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using colossal magnets, the only thing that was around after

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the big bang - hydrogen gas - until it ignites.

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And that IS a star.

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BUZZING AND BEEPING

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Sounds simple? It isn't. Don't try this at home.

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It is a job for the professionals.

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The chamber will briefly use more power than a city like Birmingham.

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And the ignition countdown begins 100m away,

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in the relative safety of mission control.

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We're now approaching the T minus one minute mark. T minus one minute.

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I'm joining starmaker-in-chief, Professor Steve Cowley.

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Steve, hello. Hello.

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I haven't touched anything and I promise not to

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because you're effectively creating a star here.

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Yeah.

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This looks AMAZING! This looks like I'd want it to look.

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Is it running now?

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We're about to fire it up, and for a few seconds,

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we'll reach the temperature of round about 100 million degrees.

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100 million degrees!

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What if it goes wrong, Steve?

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I mean, it's kind of extreme, isn't it?

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If something goes wrong, and it does do,

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the physicist in charge, she's got a red button,

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basically, and she will press the red button and it will abort the shot.

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The amount of energy in there...

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This isn't that far from my house is where I'm going!

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I live 50 miles away.

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But it does have a wall that's 2m.

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ALARM CLANGS

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What's that?

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It's the panic button. You have to run now.

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I'm not going to bother running. Really, what would be the point?

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If something really did go wrong, you could cause a lot of damage. Right.

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And I'm being allowed to give the trigger command...

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..to turn it on.

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So, what I'm going to do now is

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trigger the creation of a star, briefly, on Earth.

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Um... CLEARS THROAT

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Er, trigger, please.

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Can you accelerate, please?

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OK. Thank you.

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INTERMITTENT BUZZING

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WHOOSHING

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COMPUTERISED VOICE: 'Start.'

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It's starting up now. Right. Electrical current going through it.

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I'll be honest, I'm faintly nervous.

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How many times a day do you do this?

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'..Eight, seven, six, five, four,

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'three, two, one, zero.'

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There it is. Right.

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Look at the instability, it's shaking.

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This is mind-blowing.

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Inside the chamber is hydrogen.

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It was pretty much the only thing that existed in the darkness

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after the big bang.

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This machine heats and squeezes the hydrogen

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with such force that it ignites, creating a star and light.

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So, what's happening in that chamber right now,

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there, that is...that is a star on Earth.

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What's remarkable is the process of making a star

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doesn't just create light. It also makes brand-new ingredients,

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and this is going to help me build our universe.

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There's little white specks, which is exactly what stars are doing.

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It's turning hydrogen into helium.

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They start with hydrogen and they make helium

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and then they get helium and they make carbon,

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then they make oxygen. All the things you're made of,

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they are made bit by bit by bit in the centre of a star.

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Was that it? That's it.

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And was that the abort button there, you had all the... Whoa...

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Within a star, these different elements are made,

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but how do they then... They've got to get elsewhere.

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So, if it's a big enough star, it explodes -

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that's a supernova explosion - and it spews all that stuff,

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all those things you've made, all the carbon,

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all the iron, all the nickel, all the whatever, right, spews it out

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into the universe as dust, as particles,

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as this, that, and the other.

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These elements are created within it

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and then - boom! - all over the universe.

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Stars not only give us light,

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they are the element factories to build everything else.

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Back at my tower, I can now make light,

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and create all the stuff to build the rest of our universe.

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We just need a star to go supernova.

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A supernova is the biggest explosion there is, and for us

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it's an essential stage in our construction process

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because it takes all those elements created in big stars

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and scatters them everywhere.

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Just one note of caution though -

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when I say "big", I do mean "really, really big".

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And that supernova has now scattered all the ingredients

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we need to build everything.

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Floating around the tower, we've now got carbon,

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oxygen,

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iron...

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..and all the other elements we're going to need

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to make the planets,

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and even us.

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In that sense, everything

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really is stardust - you, me,

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everything you've ever seen

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or touched, or ever will.

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All of it created from the birth and death of a star.

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It's mind-blowing.

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And that cloud of gas and dust, called a nebula, also provides

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the ingredients for other stars.

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So we can now build our own star from it.

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We'll call it the sun.

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The real one took around 50 million years to form.

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Here, we've done it in seconds.

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And orbiting it is the dust and gas we'll need

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to make all the planets in our solar system.

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The first planet to start forming is Jupiter.

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But something's not going to plan.

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The young planet is starting to hoover up

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way too much of the gas and rock.

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And this process

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is slowing it down...

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..causing it to fall inwards, towards the sun.

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Which is a problem,

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because this is the very stuff

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that's going to build all the other planets.

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It's bad. What do we do to stop Jupiter gobbling up

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all our planetary building materials?

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Well, fortunately, I'm told there is a man who knows.

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This is Professor Alexei Filippenko.

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And THIS is a Fresnel lens.

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A simple enough device, but surprisingly powerful.

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Hi, Richard. So, how do we get rid of our rampaging Jupiter problem?

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Oh, well, look. Let me show you a demo that'll help illustrate it.

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Declan, why don't you tilt it there?

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It's on fire. Right away! It is on fire!

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But what's that got to do with Jupiter? It's a bit of wood?

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Yeah, well, what's happening is there's all these photons, all these

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little energetic particles of light coming from the sun and they're

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being focused here on this wood, heating it up, causing it to burn.

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In the case of the early solar system, the sun was much

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brighter than it is now and it acted for hundreds of thousands,

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or millions of years, so the photons were hitting

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the particles of dust and gas and heating them up, causing the

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atoms to actually evaporate away, to be blown out of the solar system.

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That meant that Jupiter was no longer

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slowing down and spiralling into the sun.

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Two things. One - there's a small fire over there.

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Yeah! Two -

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all the stuff in the way of Jupiter, slowing it up, wasn't wood.

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Yeah, I know, but look how powerful the sun is.

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Here's a rock. Why don't you put it right there.

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I don't want to get zapped by your machine.

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Declan won't zap you while you're putting it there.

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And we need to have some safety glasses on because

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it's going to get heated up so much from the trillions of photons

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hitting it that, er, it's actually going to snap, crackle and pop.

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Little pieces will come flying out. You've got more safety than me.

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Well, you know, my eyes are more important.

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I'm an astronomer, OK? OK. So let's put the rock in there...

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I can't argue with that, can I?

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I can't argue with that. I think you're OK.

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CRACKING AND POPPING

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Oh, hang on, that is the rock.

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Yeah, that's the rock flaking off...

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because of all the energetic photons hitting it.

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I am properly impressed with that. That is in seconds.

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It's heating up to 3,000 degrees Fahrenheit, OK?

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Now, over millions of years,

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the material is being blown out of the vicinity of Jupiter,

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so it's not growing any more and also it's not spiralling into the sun.

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So that saves us. Turn it off, Declan, I'm terrified.

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So this is another one of those events that had to happen

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at the right time, in the right place, and to the right extent.

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Too much of this for too long

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and there's nothing left to make your inner planets from.

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Yeah, that's exactly right.

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OK, a plan.

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I'm going to use light from the sun to clear a path for Jupiter...

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..to stop it slowing and spiralling inwards,

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gobbling all the building materials for our other planets.

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So, let's crank up the light from our sun...

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..and get those photons pumping.

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Jupiter's way is now clear.

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But luckily for us, the perfect amount of stuff

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is left behind to build the rest of our solar system.

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So we've got Jupiter.

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Now, how do we make our other planets?

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To find out what the planet formation was like in the early

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solar system, I need the help of the Texas Roller Derby.

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Excuse me. Sorry.

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Course I do.

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Sorry, ladies, excuse me. Can I join?

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Oh! Do I really need that? You need it to protect your head.

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Right. Well, I'll pop it on. Thank you.

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What's your skate name? Your name on the track, your alter ego?

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Hamster. Yeah, it's a long story.

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What about Slamster? Slamster!

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Oh! I'm loving that! WOMEN: Yeah, that's good.

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What sort of injuries can you acquire doing this?

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BOTH: Broken...everything!

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Broken ankles. Broken teeth. Hands, arms...

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I am really scared!

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You should be scared.

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Now, I know what you're thinking.

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Actually, I've no idea what you're thinking...

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..but bear with me. This is a genuine scientific demonstration

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of what happened in the early solar system.

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See you out there, girls. Oh, scared!

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I should say, I'm not what you'd call a regular skater.

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Imagine the sun in the centre of the track providing the gravity

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to pull around a whole host of rocks of different sizes.

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These wannabe planets are known as planetesimals.

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Some of these planetesimals were large, some very small,

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some moving in crazy orbits.

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U-u-ugh! Yee-ugh! Whoo-uh!

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All of them were affected by one another's gravity.

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So there were HUGE collisions.

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Potential planets were flung out of the solar system.

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And some wannabe planets were destroyed.

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Others had huge chunks ripped off them.

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What happened over just a few million years

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was a sort of planetary carnage.

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Oh! This is really difficult! Ha-ha-ha... Whoo-ooh!

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Eventually, some of the larger, more stable planets emerged

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and took the outside orbital lane.

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Whilst closer to the sun, smaller planets jostled for position.

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The remnants of this orbital tussle, the dead

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and never-to-be planets didn't just disappear, they still exist.

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A graveyard of broken worlds

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now orbits the sun as a ring of debris

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known as the asteroid belt.

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So here we are. Our solar system. There's Jupiter

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and, alongside it, the asteroid belt.

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And then the rest of the planets in our solar system.

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There's Mercury, nearest the sun.

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Its atmosphere has already been burnt away.

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Then Venus,

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a big bash early on has reversed its spin.

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And Mars,

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there's an enormous volcano here...

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..Olympus Mons, three times higher than Everest.

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Then Jupiter, bigger than all the planets put together.

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Saturn with its amazing rings.

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So light, it could float on water.

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Further out, Uranus, where summers last 21 Earth years, as do winters!

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And finally, Neptune.

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Freezing cold with hurricane winds of 1,000 kilometres an hour.

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Of course, there is one planet missing - ours.

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And exactly where it goes is critical

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because we need it to support one very fragile thing - life.

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Earth is unique amongst the planets in our solar system.

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It teems with life.

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Life which comes in countless different forms.

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So what is it that makes Earth so special?

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What do we need for life to exist when we're building a solar system?

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To find out, these scientists are attempting to reach

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one of the most inhospitable and extreme places on Earth.

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Sandro...

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SHE SPEAKS ITALIAN

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How far is it to the lake?

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SHE CONTINUES IN ITALIAN

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Where they're heading is so toxic, it is like an alien planet.

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If they can find life down there, it will help us understand

0:26:460:26:50

the most basic requirements for life in our solar system.

0:26:500:26:55

OK, I'll follow you.

0:26:550:26:57

Be careful.

0:26:570:26:59

To get there, they must risk a perilous 3km descent

0:27:000:27:04

into eastern Italy's Frasassi cave system.

0:27:040:27:07

Caves like these contain some of the last unexplored frontiers on Earth.

0:27:260:27:32

Here I come.

0:27:340:27:36

The expedition is led by

0:27:380:27:40

astrobiologist Professor Jenn Macalady.

0:27:400:27:43

Stay left, it's really tight.

0:27:440:27:46

If you go to the right you are going to get stuck for sure.

0:27:470:27:51

I'm not far behind.

0:27:510:27:53

Use your feet.

0:27:530:27:55

Yes, I am, it's er...

0:27:550:27:58

tight.

0:27:580:27:59

Breathe out.

0:27:590:28:00

Yeah, that's it.

0:28:020:28:03

You got it? Yep.

0:28:080:28:09

You're through! Awesome.

0:28:090:28:11

The things I do for science!

0:28:110:28:14

After six hours, they're approaching the final descent.

0:28:180:28:22

At the bottom, Jenn's hoping to shed light on the minimal

0:28:250:28:29

conditions required for life.

0:28:290:28:31

Aldo, coming down. OK!

0:28:320:28:34

This is the Crystal Lake.

0:28:420:28:45

Wow, it's beautiful.

0:28:450:28:47

OK, I'm going down.

0:28:500:28:51

Deep below its surface is home to what Jenn is looking for.

0:28:510:28:55

It's a long way down, folks.

0:28:580:29:00

Down here, all the normal things

0:29:040:29:06

you need to support life have disappeared.

0:29:060:29:09

Shall I come all the way down?

0:29:100:29:13

There is no light.

0:29:130:29:14

No animals or plants to feed off.

0:29:160:29:19

And where they're going, there's no oxygen.

0:29:190:29:22

We made it.

0:29:240:29:25

The water is even poisonous

0:29:300:29:33

but Jenn is hoping to find life there.

0:29:330:29:36

The hunt will involve one of the most dangerous dives on the planet.

0:29:400:29:44

Preparing to make the 80-foot plunge is ex-Navy diver Alejandro Crocetti.

0:29:450:29:51

Perfecto.

0:29:520:29:53

His dive time is strictly limited.

0:29:550:29:57

Any kind of cave diving is very dangerous, because

0:30:000:30:03

if there's a problem, you can't just pop up to the surface.

0:30:030:30:06

You have a long way to go.

0:30:060:30:07

But also, in this particular case, the water is actually toxic.

0:30:080:30:12

So the chemicals that are dissolved in the water come through the skin,

0:30:120:30:16

so that if you stay in that water for a while, then you become sick.

0:30:160:30:20

You start to have symptoms

0:30:230:30:24

that prevent you from making good decisions.

0:30:240:30:27

Very quickly the passages become tighter and tighter.

0:30:290:30:32

There is no room to manoeuvre.

0:30:320:30:35

As soon as you move, you suspend all the sediment that's on the bottom

0:30:350:30:40

and the visibility goes to zero very quickly.

0:30:400:30:42

Fish would die instantly here.

0:30:440:30:47

Very quickly the water will become sulphidic, more cloudy,

0:30:490:30:53

more difficult to navigate through.

0:30:530:30:55

We're not meant to be there really.

0:30:560:30:58

It's a place where we can stay only for a few moments.

0:30:580:31:01

Finally, they find what they've been looking for.

0:31:150:31:19

These weird alien fingers are alive.

0:31:250:31:29

They are bacteria,

0:31:330:31:35

living on nothing more than rock dissolved in toxic water.

0:31:350:31:39

Wow!

0:31:500:31:54

Look at that, this is beautiful.

0:31:550:31:58

Were there a lot like this?

0:31:590:32:00

Multi. Multi? Si.

0:32:000:32:04

Amazing sample, bravo. Grazie.

0:32:040:32:07

This is life that we don't really understand yet.

0:32:170:32:20

It's from water that's toxic, it's hostile, there's no oxygen.

0:32:200:32:25

Where we've lost all the light, almost nothing to live on.

0:32:250:32:28

All that's left really is water and rocks,

0:32:280:32:31

and yet there's this beautiful form just full of interesting, weird,

0:32:310:32:38

strange life, and it's extraordinary, because it represents

0:32:380:32:42

something new that will help us explore for life on other planets.

0:32:420:32:48

One of the things that we can learn from a sample like this is that

0:32:510:32:55

wherever we have rocks and water, then somehow

0:32:550:33:00

the water is going to allow life to thrive

0:33:000:33:04

because it allows things to mix.

0:33:040:33:06

It allows the rock to interact with life.

0:33:060:33:09

So water is really, as we understand life, the most essential ingredient.

0:33:100:33:15

Life as we know it can't exist without water

0:33:230:33:27

but it must be liquid.

0:33:270:33:30

Water, of course, comes in several different states.

0:33:300:33:33

And where it is in our solar system is key.

0:33:380:33:42

Too close to our sun, and water boils away.

0:33:430:33:47

Too far away, like in the rings of Saturn...

0:33:500:33:54

..and water freezes as hard as iron.

0:33:550:33:58

Where we place our planet, then, is critical

0:34:080:34:11

if we want to have liquid water.

0:34:110:34:13

But how much leeway do we have? What about here near Mars,

0:34:130:34:18

about 142 million miles from the sun?

0:34:180:34:21

Well, to find out if Mars is suitable for liquid water,

0:34:270:34:31

and for life, first you've got to get there.

0:34:310:34:34

Mars.

0:34:390:34:40

And NASA's rover, driving on the surface.

0:34:450:34:49

Well, as close as you can get to its surface...

0:34:520:34:55

..in Houston, Texas.

0:34:570:34:59

Don't look at the bulldozer, that gives away that it's not Mars.

0:34:590:35:02

Just so you know, that's not there!

0:35:020:35:04

Or those cars. It spoils the effect!

0:35:040:35:06

And my guide is NASA astronaut, Mike Gernhardt.

0:35:080:35:12

Would it look anything like this? Yeah.

0:35:120:35:15

NASA wants to put humans on the Red Planet in the next 20 years.

0:35:190:35:24

Their goal is to find life.

0:35:250:35:28

Problem is, despite there being hundreds of old river beds on Mars,

0:35:330:35:38

all images show that the liquid water has vanished from the surface.

0:35:380:35:42

So, what's happened to it?

0:35:480:35:49

NASA is developing the kit to take us to the Red Planet to find out.

0:35:520:35:57

This is Building Nine.

0:35:590:36:01

A place I dreamt of as a kid...

0:36:030:36:05

..and as an adult.

0:36:060:36:08

You do have the coolest garage in the world.

0:36:110:36:13

Yep, we got some really cool stuff. This thing is called the Robonaut.

0:36:130:36:17

This is actually on the International Space Station at this point.

0:36:170:36:20

This is called the Space Exploration Vehicle.

0:36:200:36:22

This would be going to an asteroid, or possibly

0:36:220:36:25

a moon of Mars like Phobos.

0:36:250:36:27

Then with the reaction-controlled jets, we can hop.

0:36:270:36:31

And an astronaut is on the end of a robot arm and we can have

0:36:310:36:34

that on Mars, or the moon, or whatever planets we end up going to.

0:36:340:36:38

All of this really informs us how to support these deep space missions.

0:36:380:36:43

It's... Talking to you is just like going through a movie plot,

0:36:430:36:46

constantly, it's so...

0:36:460:36:48

Right, that all makes perfect sense...if you're you.

0:36:480:36:52

RECORDING: 'We're now approaching the T minus one minute mark.

0:36:520:36:55

'T minus one minute. T minus one minute.'

0:36:550:36:57

And this is how man might get to Mars - the Orion spaceship.

0:36:570:37:02

Are we getting in? We're going to get in.

0:37:020:37:05

Oh! I so want to get in. A born astronaut, me.

0:37:050:37:08

Here I go! Right, climbing across.

0:37:080:37:11

You could bang your head on many things in here.

0:37:110:37:14

Ye-ow!

0:37:140:37:15

Yeah. Oh, yeah.

0:37:150:37:17

Ooh! Yeah, I am so in.

0:37:180:37:22

All right, good job!

0:37:220:37:23

'T minus 20 seconds and counting.'

0:37:230:37:25

'Having been to space, Mike's going to take me

0:37:250:37:28

'through what a Mars launch would be like.'

0:37:280:37:31

So, you climb in here.

0:37:310:37:33

'Ten, nine...' You're strapped in.

0:37:330:37:36

'Ignition sequence has started.'

0:37:360:37:38

Then there's check lists you go through.

0:37:380:37:40

'Five, four...'

0:37:400:37:41

The clock hits zero... '..two, one, zero...'

0:37:410:37:45

..and, all of a sudden, you have this big thrust in your back.

0:37:450:37:48

And you're going up into space.

0:37:520:37:54

'And we have liftoff.'

0:37:550:37:57

We're going to be going faster than we ever have before

0:38:000:38:04

so it's going to be a, you know, a real sporty ride.

0:38:040:38:08

Sporty, that's a good word. Vigorous.

0:38:080:38:10

'Liftoff...'

0:38:110:38:13

So, four of us in here? Yep.

0:38:130:38:17

Mars. Mars.

0:38:170:38:18

It's not a short trip, is it? It isn't.

0:38:180:38:21

Generally think of it as a nine-month trip out.

0:38:210:38:24

Nine months?!

0:38:240:38:26

What if somebody snores? I snore.

0:38:260:38:27

I have actually flown in space with a guy that snored

0:38:270:38:30

so loud that it kept me awake for days actually.

0:38:300:38:33

Were you not just tempted to, you know, let him out?

0:38:330:38:35

Nah, you can't do that.

0:38:350:38:37

'OK, Houston, go in 30 seconds.'

0:38:370:38:39

INDISTINCT RESPONSE

0:38:390:38:40

'Mark one bravo.'

0:38:400:38:42

Having reached the Red Planet, we now need to get out

0:38:440:38:48

and search for Mars's water.

0:38:480:38:50

So, I'll need one of these.

0:38:520:38:54

Can I just say, this is an amazing privilege to get to do this.

0:38:550:38:59

This is the Z1, next gen prototype.

0:38:590:39:04

Besides me, Bruce Willis is the only non-astronaut who's ever been

0:39:040:39:08

cleared to wear a real spacesuit. Oh, yeah.

0:39:080:39:11

It's kind of like putting on a big onesie.

0:39:110:39:14

Do I look faintly ridiculous?

0:39:140:39:15

Ha-ha, yes!

0:39:150:39:17

Wow! That's a glove and a half.

0:39:200:39:23

That is serious.

0:39:230:39:24

The NASA team are now putting me

0:39:260:39:28

through a full Mars atmosphere suit simulation.

0:39:280:39:31

That's got to go all the way up until we get to four three,

0:39:310:39:34

which is operating pressure. OK. Sound good? Yes. OK

0:39:340:39:37

I'm waiting for a massive burst of claustrophobia.

0:39:440:39:47

'The atmosphere on Mars is incredibly thin, just 1% of Earth's,

0:39:480:39:53

'so we need to pump up the suit, like inflating a tyre,

0:39:530:39:57

'to hold my body together.'

0:39:570:39:58

Swallowing. You're looking worried. Doing OK? I'm fine!

0:39:580:40:01

Great. You're starting to look more muscular now, you know.

0:40:010:40:05

No, I actually am, I'm actually flexing. We're at three.

0:40:050:40:07

Three PSI. Three PSI.

0:40:070:40:08

Four, one.

0:40:080:40:10

Four, one. Popping ears.

0:40:100:40:13

We're at operating pressure. Operating pressure. Wow!

0:40:130:40:16

So, the arms are a little bit long for you in the suit

0:40:160:40:19

but that's as small as they go because you're at the small end...

0:40:190:40:22

This is like every shopping trip I've ever been on!

0:40:220:40:25

The legs are a bit long on the jeans, sir,

0:40:250:40:27

but that's the shortest we have. All right!

0:40:270:40:30

OK! Yeah, it's...

0:40:300:40:31

Why did I know it wasn't going to fit?

0:40:310:40:34

So the next thing, we're going to release you from the donning stand.

0:40:340:40:37

I only have short legs, so the bigger steps thing...

0:40:430:40:46

MUSIC: "Stayin' Alive" The Bee Gees

0:40:500:40:51

It had to happen. I told you - seventies' moves, there they are.

0:40:570:41:01

I am super impressed.

0:41:010:41:02

My daughters will be just cringing, "Dad, don't dance!"

0:41:020:41:06

I'm dancing, yeah. See, look, girls, there it is.

0:41:060:41:10

Suddenly I feel like doing this a lot.

0:41:100:41:13

Oh, yeah, moonwalk!

0:41:130:41:15

Were I on Mars right now,

0:41:200:41:21

the atmosphere on the other side of this suit would be very different.

0:41:210:41:24

What's it like? Yeah, it's basically almost no atmosphere.

0:41:240:41:28

As we stand here, we're at 14.7 pounds per square inch,

0:41:280:41:31

on Mars the pressure is roughly ten torr,

0:41:310:41:34

which is like one hundredth of this.

0:41:340:41:36

What would happen to me if I didn't have this?

0:41:370:41:40

You'd be dead pretty soon. You'd probably have

0:41:400:41:42

a couple to three minutes, and then that would be it.

0:41:420:41:45

Clearly that's bad. Well, thank heavens for this thing then.

0:41:450:41:50

'Mars is relatively close to Earth,

0:41:500:41:53

'yet we certainly couldn't live there.

0:41:530:41:56

'So, for life, what's wrong with the Red Planet?'

0:41:560:41:59

Well, Mike's going to show us, with just a glass of water and a pump.

0:41:590:42:06

So that's a pump and you're just pumping the air out of here

0:42:100:42:13

until, you're creating a vacuum in there. Exactly.

0:42:130:42:16

It actually won't be a pure vacuum, it'll be the same

0:42:160:42:18

pressure as we have on Mars, which is very low but not complete vacuum.

0:42:180:42:23

So you're just taking the air out to lower the pressure. Exactly.

0:42:230:42:27

There it goes. There it goes.

0:42:290:42:31

So there's no extra heat in there, that isn't at 100 degrees C?

0:42:320:42:36

In fact that could be at zero degrees C.

0:42:360:42:38

This is why you should always be careful with your spacesuit on Mars.

0:42:430:42:46

Exactly.

0:42:460:42:47

You don't want that happening to your blood. It's bad news.

0:42:470:42:51

And that's why, so far as you know,

0:42:510:42:52

there isn't any liquid water on Mars? Right.

0:42:520:42:55

The atmosphere is so thin that if there were any liquid water,

0:42:550:42:58

it would just evaporate like that.

0:42:580:43:00

So, suddenly, holding on to your atmosphere becomes

0:43:010:43:04

critical to keep your water along with it, how do you do that?

0:43:040:43:07

So you need the right combination of things and one of them

0:43:070:43:11

is the planet size because that effects the gravity,

0:43:110:43:13

and if you don't have enough gravity then the atmosphere that was there

0:43:130:43:17

will eventually go away. And then, as the atmospheric

0:43:170:43:19

pressure drops, then the liquid water goes away.

0:43:190:43:22

So there's this optimal size planet

0:43:220:43:24

and Earth just happens to be one of those, so you need all these

0:43:240:43:28

things to line up just, you know, shoot through the holes

0:43:280:43:31

of the Swiss cheese in order to get the right combination to have life.

0:43:310:43:34

And no liquid water, no life?

0:43:340:43:37

Yeah.

0:43:370:43:39

Complicated things to build, planets that you can live on,

0:43:390:43:41

as it turns out.

0:43:410:43:43

So there are a couple of things to think about

0:43:490:43:52

when positioning our planet.

0:43:520:43:54

The best place to put our planet for us is exactly where we are,

0:43:560:44:01

93 million miles away from the sun, third rock along,

0:44:010:44:06

in the part of space that we've called the "habitable zone",

0:44:060:44:08

where we get just enough of a slug of the sun's energy -

0:44:080:44:12

not too much or too little.

0:44:120:44:14

It's a zone where water doesn't instantly freeze...

0:44:170:44:21

..but also doesn't boil away.

0:44:220:44:25

Both Earth and Mars are in that zone.

0:44:320:44:36

But even then, as we've discovered with Mars,

0:44:410:44:44

a planet has to be big enough to hold on to its water

0:44:440:44:48

with an atmosphere to stop it escaping into space.

0:44:480:44:51

So our planet has to be not only in just the right place,

0:44:510:44:55

it has to be just the right size to support life.

0:44:550:44:58

Where we place our planet needs to be precisely right.

0:45:090:45:13

It must go between Mars and Venus,

0:45:150:45:19

bang in the middle of the habitable zone.

0:45:190:45:22

So there we are.

0:45:240:45:25

All our planets in place around what scientists call

0:45:250:45:28

a middle-aged yellow dwarf - our sun.

0:45:280:45:32

We've built our solar system! Wonderful.

0:45:320:45:35

We started with a supernova...

0:45:430:45:46

..which created light, and the ingredients to make our sun.

0:45:530:45:58

Then we made eight planets, including one just like ours...

0:46:030:46:10

..in the perfect place to support life.

0:46:130:46:15

Except that's not all.

0:46:210:46:24

Can you imagine the Earth without stars in the sky? Miserable.

0:46:240:46:29

We need more than that one star, we need a whole galaxy of them.

0:46:290:46:33

Still, that's easy. Build one star, you've built them all.

0:46:330:46:36

We've made over 300 billion stars

0:46:430:46:46

and put them all together into a galaxy.

0:46:460:46:49

Just like the one we live in, the Milky Way.

0:46:510:46:54

And we've put our sun with its solar system right out here,

0:46:560:47:01

in a sleepy backwater on the outer edge.

0:47:010:47:04

Astronomers have even given it a galactic address.

0:47:070:47:11

Seriously, anyone can reach us at the local fluff,

0:47:110:47:14

inside the local bubble at the Gould Belt of the galaxy's Orion arm.

0:47:140:47:18

I don't know what number.

0:47:180:47:20

Anyway, it's a good job we are out in the galactic sticks

0:47:200:47:24

because we wouldn't want to make the mistake of being

0:47:240:47:27

too close to the centre of things.

0:47:270:47:28

Because that is where lurks a supermassive black hole.

0:47:340:47:38

Yep, they really do exist.

0:47:380:47:41

These are once-giant stars that have collapsed in on themselves,

0:47:410:47:45

pulling in millions of other stars around them.

0:47:450:47:49

They sit at the centre of most galaxies,

0:47:490:47:51

including our own Milky Way.

0:47:510:47:54

Their gravity is so strong

0:47:540:47:56

that not even light can escape its violent pull.

0:47:560:47:59

I think it's best we stay well away from that.

0:48:030:48:07

Where we are is exactly where we want to be.

0:48:070:48:10

This galactic neighbourhood really works for us.

0:48:100:48:14

But if we're building a universe, we need more than one galaxy.

0:48:170:48:20

We need a whole ocean of them.

0:48:200:48:24

Some spiral, some spidery, some lens-shaped,

0:48:240:48:27

but each of them beautiful and unique.

0:48:270:48:29

And scientists have calculated that, to fill our universe,

0:48:380:48:42

we need more stars than grains of sand on all the beaches on Earth.

0:48:420:48:47

But all is not well in the universe we've built.

0:48:530:48:57

The galaxies are flying apart.

0:49:050:49:07

I'm missing something that holds them together.

0:49:100:49:13

What have we forgotten?

0:49:160:49:18

Our universe is missing a vital ingredient.

0:49:240:49:28

It's something that produces a massive gravitational force.

0:49:280:49:33

Without it, the universe would disintegrate.

0:49:330:49:37

Below my feet, is a lab full of people, all trying to find

0:49:400:49:44

the stuff that holds the universe together.

0:49:440:49:47

Which is why I'm heading 1.3km underground.

0:49:470:49:50

Scientists have worked out that what glues the galaxies together is

0:49:570:50:01

the most common stuff there is.

0:50:010:50:05

It makes up a staggering 85% of everything.

0:50:110:50:15

They named it "dark matter".

0:50:180:50:20

Problem is, it's totally invisible and undetectable.

0:50:200:50:25

But that may be about to change,

0:50:270:50:29

thanks to scientists like Professor Rick Gaitskell.

0:50:290:50:32

No music?

0:50:340:50:36

Well, they did actually put some in once upon a time. And?

0:50:360:50:39

Nobody could agree on what to play!

0:50:390:50:42

OK.

0:50:420:50:43

We also had a light in here at one point, it was all mod cons.

0:50:430:50:47

Rick's built a dark matter detector

0:50:480:50:50

that's so sensitive he's had to protect it under 1.3km of rock.

0:50:500:50:57

Why have we stopped here? I think this is it.

0:50:580:51:01

These are scientists, not miners.

0:51:090:51:12

I have a desperate urge to sing...

0:51:120:51:13

SINGS: # Hi-ho, Hi-ho! # I'm not going to.

0:51:130:51:16

And they've spent $100 million to look for something

0:51:160:51:22

you can't see,

0:51:220:51:25

you can't touch...

0:51:250:51:26

..and we haven't even found.

0:51:290:51:31

And this is what they've spent their money on.

0:51:390:51:42

So, is that it?

0:51:420:51:44

Yep, that's the dark matter detector. Or rather,

0:51:440:51:47

this is the water tank that surrounds our dark matter detector.

0:51:470:51:51

I'm not being funny but it's like being in my loft,

0:51:510:51:54

except I bet there's no dead pigeons in there,

0:51:540:51:57

it's a pretty specialised environment.

0:51:570:51:59

It's got to be very clean.

0:51:590:52:01

The water inside this tank is extremely pure and it isolates our

0:52:010:52:05

detector from all the radioactivity in the rock, and even you.

0:52:050:52:09

And in terms of search instruments, this is

0:52:090:52:11

one of the biggest in the world or the best or...?

0:52:110:52:14

This is the most sensitive dark matter detector in the world

0:52:140:52:16

and we're running it right now. It's on? It's on.

0:52:160:52:19

So, how does the detector work?

0:52:270:52:30

Well, suspended inside it is a capsule of a special gas

0:52:300:52:34

called xenon.

0:52:340:52:36

It's the same stuff that's in this novelty toy.

0:52:370:52:40

It's very nice, it's a pleasing distraction,

0:52:450:52:47

but why are you holding that thing?

0:52:470:52:49

We've filled this plasma ball with xenon

0:52:490:52:52

and we're exciting it using electricity.

0:52:520:52:55

As you can see, light is being generated.

0:52:550:52:57

The dark matter detector works on exactly the same principle.

0:52:570:53:00

We filled it with xenon,

0:53:000:53:02

and when a dark matter particle comes in, the particle directly

0:53:020:53:06

excites the atoms, and the atoms emit light, which we then detect.

0:53:060:53:10

So that's the event you're waiting to observe. It's not a giant one of

0:53:110:53:14

these, but that's to illustrate the idea of seeing those interactions.

0:53:140:53:18

That's right, and the particle events we're looking for

0:53:180:53:21

are extremely infrequent.

0:53:210:53:22

We're operating this detector for weeks, months, years,

0:53:220:53:27

looking for very, very occasional dark matter particles to

0:53:270:53:31

interact with the xenon and we'll see the light coming from it.

0:53:310:53:33

It sounds complicated and it is.

0:53:450:53:48

Rick's been searching for dark matter particles for 23 years.

0:53:480:53:53

But scientists know it must exist,

0:53:530:53:57

because they can see the effects of its gravity

0:53:570:54:00

holding galaxies together.

0:54:000:54:03

If they can detect it,

0:54:030:54:05

they'll have solved one of the greatest mysteries in science.

0:54:050:54:08

Rick, would it ruin millions of pounds' worth of research

0:54:110:54:16

and years, decades in fact, of your own work if I turn the lights on?

0:54:160:54:20

Don't touch any one of those buttons! That's six months' delay.

0:54:200:54:25

I won't touch anything. Hands in pockets.

0:54:250:54:27

The first live results have started streaming in.

0:54:290:54:32

So, any of these spikes, that spike, that could be it,

0:54:320:54:36

one of greatest moments in science ever?

0:54:360:54:38

That spike could be it, the event you're looking for?

0:54:380:54:42

That's right. So, if that one was it,

0:54:420:54:45

proof of the existence of dark matter, and I'm here? Yep.

0:54:450:54:48

Will I get my name on it?

0:54:480:54:49

Well I was here. If that's it, I was here just then.

0:54:490:54:52

If it is that event, we'll name it after you.

0:54:520:54:54

Every day you enjoy your unusual commute a mile under the ground.

0:54:540:54:59

If that happens, if that's the day that those spikes occur,

0:55:000:55:05

it's a big deal!

0:55:050:55:07

It will be an amazing feeling.

0:55:070:55:09

I think you'll hear the celebration.

0:55:090:55:11

Um, even though we're a mile underground it will be quite a roar.

0:55:110:55:15

I'll hear the champagne corks open!

0:55:150:55:18

But I haven't got time to hang around talking about champagne.

0:55:210:55:24

I need to head back to the tower

0:55:240:55:26

to add some elusive dark matter to the cosmic mix right now.

0:55:260:55:31

And it's working.

0:55:430:55:44

The gravity of the dark matter is pulling our galaxies back together.

0:55:460:55:51

Disaster averted.

0:55:570:55:59

Scientists have crunched all the numbers relating to dark matter

0:56:000:56:04

through a supercomputer and come up with a way of seeing it.

0:56:040:56:08

And for the first time, we can show you what that looks like.

0:56:080:56:11

Each of these points of light is a galaxy made up of billions of stars.

0:56:180:56:23

They are held together in a vast gravitational web,

0:56:260:56:31

created by ribbons of dark matter.

0:56:310:56:33

Adding that missing matter to a map of the universe

0:56:410:56:45

means we can actually see how we, here on our planet,

0:56:450:56:48

really are connected to even the remotest star.

0:56:480:56:52

And it's...it's kind of beautiful.

0:56:520:56:54

This vast web of dark matter...

0:57:040:57:07

..holds the entire universe together.

0:57:090:57:12

As you look up on a clear night at that band across the sky,

0:57:460:57:51

you're looking into the heart of the Milky Way -

0:57:510:57:55

a tiny part of the great web of galaxies.

0:57:550:57:59

We are connected to it all

0:58:020:58:04

because we are made of the same stuff.

0:58:040:58:07

And if anything had been a bit different -

0:58:110:58:14

the Earth a bit too small,

0:58:140:58:16

the sun too bright,

0:58:160:58:19

the other planets too big,

0:58:190:58:21

or the solar system in the wrong place in our galaxy...

0:58:210:58:26

..then we simply wouldn't be here.

0:58:290:58:32

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