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(dramatic music)

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<v Narrator>Earth is born out of chaos and catastrophe.</v>

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Despite such hostile conditions,

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life emerges on our planet,

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but it must withstand deadly disasters,

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again and again.

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Planet Earth is a wild world.

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Shaken by unimaginable impacts,

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volcanic eruptions that flood the landscape,

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and drastic climate changes that lead to ice ages

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that freeze the world from pole to pole.

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Yet each assault creates a path for something new.

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Life always finds a way,

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despite being constantly put to the test.

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(dramatic music continues)

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Without these catastrophes,

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life as we know it would not exist on our fateful planet.

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Chile.

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In the heart of the Atacama Desert,

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scientists are trying to understand how our home,

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Planet Earth, came into being.

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<v Thomas>Astronomers are like archeologists,</v>

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so we have somehow to reconstruct the past.

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<v Narrator>Professor Thomas Henning is one</v>

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of the world's leading experts on planet formation.

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<v ->We live in a period of discoveries</v>

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and it's really absolutely exciting to be part of this

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and to be part of this great adventure

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to unravel the mysteries of the universe.

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<v Narrator>As the end of the last century came to a close,</v>

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a staggering discovery was made.

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Scientists had measured the slightly shifting light

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of a star.

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From the data, they could tell that a giant object had

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to be pulling on it: a planet.

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This was the first planet outside our own solar system

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to be discovered.

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A so-called exoplanet.

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<v Thomas>It was an absolute game changer,</v>

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I think was one of the most fundamental discoveries.

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And in that time, we can put our solar system context.

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<v Narrator>This newly-found planet is far from unique.</v>

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Scientists believe that in just our galaxy alone,

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there are around 100 billion planets.

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Many could even foster life.

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By researching these distant planets,

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scientists hope that they can shed more light

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on our own planet and its formation,

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but detecting them remains a challenge.

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<v ->One of the technique is actually using a dip</v>

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in the light intensity.

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So let's imagine that the lamp would be the star

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and this would be the planet.

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Then we would see a slight dip in the light intensity,

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and we could conclude

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that a planet crossed the stellar surface.

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<v Narrator>These the so-called transits</v>

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can help determine a variety

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of different exoplanet characteristics,

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from the size of the exoplanet's orbit

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to the radius of the planet itself,

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even its atmosphere.

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But there is one thing this method does not provide.

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<v ->Our ultimate goal is to image planets,</v>

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and that is actually really, really difficult.

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And the reason for that is

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that the central stellar object is over shining the planet.

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<v Narrator>To image distant exoplanets,</v>

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Professor Henning works at a high-tech facility,

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the European Southern Observatory at Mount Parana.

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Located in the Atacama Desert in Northern Chile,

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the astronomical observatory towers above the desert.

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By analyzing exoplanets and their systems,

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scientists can find out how our solar system

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and Planet Earth have formed,

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and they also try to discover

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if there is life in outer space.

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(awe-inspiring music)

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<v Thomas>This is a magic place.</v>

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The landscape is just breathtaking.

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It's one of the greatest places for astronomy.

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We have many clear nights

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and we have very little water in the atmosphere.

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It's very dry, and that's great

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for observing stars and planets.

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<v Narrator>For this reason, a special array</v>

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of telescopes is utilized here

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to help scientists understand the birth of our own planet.

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It is called the VLT or very large telescope.

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Each of the four 27-feet telescopes can take pictures

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of tiny celestial objects over 4 billion times fainter

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than what can be seen with the naked eye.

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But even this is not enough.

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Beneath the telescopes,

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a collection of high-tech systems enables the scientists

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to create a virtual mega telescope.

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<v ->We are not only using a single telescope</v>

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but we are combining four of the big telescopes

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and that provides us with a space resolution

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of 140-meter telescope.

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<v Narrator>With their equipment,</v>

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the scientists can now not only detect, but image planets.

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When the Sun sets, the magic begins.

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Laser beams are used to create artificial guide stars

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to correct the distortions caused by the Earth's atmosphere.

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In the night skies,

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the scientists are looking out for exoplanets,

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especially newborn ones

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as they might deliver important clues

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to understand how planets form.

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In the control room,

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Thomas Henning and his colleague are monitoring

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the telescope's measurements.

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<v ->So I think the telescope is ready to go.</v>

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Okay, let's get started.

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<v Narrator>At a distance of nearly 400 light years,</v>

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the astronomers have identified a young star.

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In its vicinity,

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they are now trying to capture an image of an exoplanet.

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To do this, Thomas Henning is using a stiller coronagraph,

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an instrument that emulates a solar eclipse.

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It blocks out the bright direct light from the star

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so that nearby planets become visible.

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In 2018, the scientists finally succeeded

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in capturing an amazing image.

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<v ->For the first time, we could see a planetary system</v>

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in its birth environment

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so we could practically study a baby planet.

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And this was a very emotional moment

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because I tried that for many years.

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<v Narrator>The picture revealed a disc filled</v>

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with gas and dust surrounding the infant planet,

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leftover material from the formation of the system's star.

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From the image, Professor Henning could tell

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that the baby planet was a gas giant

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at least five times the mass of Jupiter,

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the largest planet in our solar system.

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<v ->We could analyze its atmosphere,</v>

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and everything points to an atmosphere which is very dusty,

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which actually has clouds.

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So it must be something similar

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to the desert here when we have wind.

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<v Narrator>The picture also tells Professor Henning</v>

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something about the dramatic past

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of the exoplanet and its system.

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Because of its massive gravity,

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the planet sucks in everything in its path,

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forcing the region around its orbit

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to become devoid of gas and dust.

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The exoplanet shifts its orbit towards its star,

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sucking in even more material on its way.

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Any smaller objects it comes across are simply consumed,

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even other planets.

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<v ->We see this black stuff here,</v>

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and this is caused by the fact

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that these giant planets clean everything

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so there is no other planets in a catastrophic way.

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They remove all the material from the disc.

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<v Narrator>Since the detection of the first exoplanet,</v>

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thousands of them have now been found

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in our own galaxy alone.

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By witnessing the birth of a planet

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for the first time in history,

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Professor Henning and his team have gathered important data.

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<v ->Our exoplanet research now paves the way to answer three</v>

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of the most fundamental questions mankind can ask.

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First, are we actually alone in the universe?

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Is there life somewhere else?

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Second, how did life actually form

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in the early history of Earth?

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And the third question we can also ask and answer,

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how did Earth form

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and how did our planetary system came about?

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<v Narrator>It is still miraculous</v>

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how our planet has grown from stardust

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to a place fit for life.

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But the latest scientific discoveries

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have shed more and more light

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on how this could have happened.

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The formation of our world

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and the emergence of life are mysteries

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that scientists are trying to solve.

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Laura Kreidberg from the Max Planck Institute for Astronomy

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in Germany is passionate about finding these answers.

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Since her childhood, she has been fascinated

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by the vastness of the cosmos.

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<v ->One of the things I asked my mom</v>

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when I was very young was,

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where is the edge of the universe?

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And she didn't know the answer,

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but I've been asking these questions ever since.

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(somber music)

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For me, looking in the night sky really puts our life

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on Earth in context.

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We know now that almost every other star

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in the sky has at least one planet,

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and when you get to see all of them up there,

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twinkling at us, you can imagine

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that perhaps there's an Earth-like planet

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with people on it wondering about us,

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just the way we would wonder about them.

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<v Narrator>Whether we are alone is still unclear,</v>

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but how our Earth evolved into the place it is today

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is only just beginning to be unraveled.

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The exploration of our solar system

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brings researchers one step closer

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to solving this mystery.

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To understand how our home,

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a small, rocky planet third from the Sun,

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became a place fit for life,

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we need to go back in time to the beginning,

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over 4 1/2 billion years ago.

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Scientists believe that our solar system begins

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as a vast interstellar cloud of gas and dust,

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twisting through the universe without direction.

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Eventually, the cloud collapses in on itself

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after becoming gravitationally unstable,

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forming a solar nebula,

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a spinning, swirling disc of material.

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<v ->And what tends to happen is</v>

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that whatever random motions existed at the beginning,

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those are preserved so you hold on to the rotation.

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But the up and down motion cancels out.

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Material moving down collides with material moving up,

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and so that flattens the disc over time

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and you're left with this rotating flat disc

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that the planets form in.

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<v Narrator>At the center of the disc,</v>

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gravity pulls everything inward.

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<v ->The material at the center got hotter and hotter</v>

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and higher and higher pressure,

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and eventually reached a point where the density

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and the temperature and the pressure were so high

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that hydrogen began to fuse in the core.

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<v Narrator>With the pressure in the core so immense,</v>

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hydrogen atoms begin to combine and form helium,

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releasing a tremendous amount of energy.

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<v ->This is some of the most dramatic events</v>

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in the history of a solar system.

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<v Narrator>With that, our Sun is born.</v>

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A shining mass of chemical elements,

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forging light into the vast darkness.

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The temperature in the core of the Sun

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reaches more than 27 million degrees Fahrenheit,

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driven by internal nuclear reactions.

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It's been estimated every second

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the Sun produces more energy than a billion atomic bombs.

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<v ->The Sun accreted almost all of the gas surrounding it.</v>

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99% of the material went into the Sun,

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but there was a little bit left over

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that formed a little proto-planetary disc.

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We call it a swirling cloud of gas and dust

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around the young star,

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and that's where the planets were born.

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<v Narrator>The little material that remained</v>

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around the heart of the new star was enough

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to form the raw ingredients

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for a new system of planets orbiting around the Sun.

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But how this material turned into planets

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has always been a subject of debate.

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(gentle music)

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<v ->One of the newest ideas about</v>

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how planets form is called pebble accretion.

264
00:13:55,950 --> 00:13:58,560
And with this idea, the planets are growing out

265
00:13:58,560 --> 00:14:01,293
of small pebbles, so little bit at a time.

266
00:14:02,640 --> 00:14:05,220
<v Narrator>Within the giant disc of gas and dust</v>

267
00:14:05,220 --> 00:14:07,320
that circled the young star,

268
00:14:07,320 --> 00:14:10,950
particles smaller than the width of a human hair

269
00:14:10,950 --> 00:14:14,310
started to clump together and coalesce.

270
00:14:14,310 --> 00:14:17,790
By this, they grew into larger and larger pebbles,

271
00:14:17,790 --> 00:14:20,730
which started to collide with each other.

272
00:14:20,730 --> 00:14:22,770
It's a process that can be compared

273
00:14:22,770 --> 00:14:25,980
to colliding bumper cars at the amusement park.

274
00:14:25,980 --> 00:14:28,320
<v ->In the young solar system, there was a lot of material</v>

275
00:14:28,320 --> 00:14:30,240
that was bumping into each other,

276
00:14:30,240 --> 00:14:33,360
exactly like these bumper cars are bumping into each other.

277
00:14:33,360 --> 00:14:36,450
But eventually, with bumper cars,

278
00:14:36,450 --> 00:14:38,133
you bump and you separate.

279
00:14:40,380 --> 00:14:43,260
But when planets form, the material is actually able

280
00:14:43,260 --> 00:14:46,260
to stick together and grow to form the planets we see today.

281
00:14:47,190 --> 00:14:48,863
Just like when the bumper cars come together

282
00:14:48,863 --> 00:14:51,137
and the one in the middle can't escape.

283
00:14:52,587 --> 00:14:53,940
<v Narrator>Escape from these collisions,</v>

284
00:14:53,940 --> 00:14:57,930
pebbles eventually grew into gigantic bodies of rock,

285
00:14:57,930 --> 00:15:01,110
some the size of the biggest asteroids we find

286
00:15:01,110 --> 00:15:02,733
in the solar system today.

287
00:15:04,320 --> 00:15:07,650
Eventually, some of these objects became large enough

288
00:15:07,650 --> 00:15:11,100
to take on a spherical shape under the influence

289
00:15:11,100 --> 00:15:12,303
of their own gravity.

290
00:15:13,230 --> 00:15:15,840
At this stage, these protoplanets started

291
00:15:15,840 --> 00:15:19,470
to grow faster and faster by consuming all the material

292
00:15:19,470 --> 00:15:21,243
in their orbit around the Sun.

293
00:15:25,440 --> 00:15:28,620
<v ->And these pebbles are able to be vacuumed</v>

294
00:15:28,620 --> 00:15:31,500
into the young, growing planet very, very quickly,

295
00:15:31,500 --> 00:15:35,070
very efficiently, so that we can grow very large planets

296
00:15:35,070 --> 00:15:38,703
on the short timescales that we observe around other stars.

297
00:15:39,930 --> 00:15:42,420
<v Narrator>Growing planets is not unlike</v>

298
00:15:42,420 --> 00:15:44,019
making cotton candy.

299
00:15:44,019 --> 00:15:46,602
(gentle music)

300
00:15:49,800 --> 00:15:54,330
<v ->And now watching this cotton candy slowly grow up</v>

301
00:15:54,330 --> 00:15:57,030
into a big ball, it's almost exactly the same

302
00:15:57,030 --> 00:16:00,600
as a protoplanet accreting more and more gas and dust

303
00:16:00,600 --> 00:16:03,300
as it moves through the proto-planetary disc.

304
00:16:03,300 --> 00:16:04,620
As it moves through its orbit,

305
00:16:04,620 --> 00:16:07,470
you can see it growing larger and larger and larger

306
00:16:07,470 --> 00:16:11,040
until, at the very end, you have a giant planet,

307
00:16:11,040 --> 00:16:12,897
or perhaps cotton candy.

308
00:16:12,897 --> 00:16:15,461
(awe-inspiring music)

309
00:16:15,461 --> 00:16:19,044
(Laura speaking in German)

310
00:16:24,510 --> 00:16:26,640
<v Narrator>The newly-born planets are anchored</v>

311
00:16:26,640 --> 00:16:28,440
by the gravity of the Sun,

312
00:16:28,440 --> 00:16:31,480
which they orbit in various paths.

313
00:16:31,480 --> 00:16:34,290
It is this gravity that keeps these protoplanets

314
00:16:34,290 --> 00:16:38,013
from flying off into the universe or collapsing together.

315
00:16:39,289 --> 00:16:43,110
In the outer solar system, our biggest planets are formed.

316
00:16:43,110 --> 00:16:46,860
They absorb all the gas within the proto-planetary disc,

317
00:16:46,860 --> 00:16:51,860
becoming the gas giants, Jupiter and Saturn,

318
00:16:51,930 --> 00:16:56,853
and the far away ice giants, Uranus and Neptune.

319
00:16:58,500 --> 00:17:00,960
Without any gas left in the disc,

320
00:17:00,960 --> 00:17:04,740
the protoplanets in the inner solar system remain rocky

321
00:17:04,740 --> 00:17:06,750
and relatively small,

322
00:17:06,750 --> 00:17:08,970
becoming terrestrial planets

323
00:17:08,970 --> 00:17:13,970
like Mercury, closest to the Sun, Venus, and Mars.

324
00:17:15,480 --> 00:17:18,930
<v ->We think that planet formation happens pretty quickly.</v>

325
00:17:18,930 --> 00:17:20,580
So after the star forms

326
00:17:20,580 --> 00:17:23,400
and there's this disc of material around it,

327
00:17:23,400 --> 00:17:25,770
after not even 10 million years,

328
00:17:25,770 --> 00:17:28,770
the planets can be fully formed after that.

329
00:17:28,770 --> 00:17:30,210
And that's just the blink of an eye

330
00:17:30,210 --> 00:17:32,163
in the length of the solar system.

331
00:17:33,120 --> 00:17:35,010
<v Narrator>One of those planets has formed</v>

332
00:17:35,010 --> 00:17:38,733
between Venus and Mars, Earth,

333
00:17:39,780 --> 00:17:43,800
born from tiny dust particles like its cousins.

334
00:17:43,800 --> 00:17:47,400
But it's not the blue planet we know today.

335
00:17:47,400 --> 00:17:50,853
Earth is a spinning of red hot rock.

336
00:17:51,720 --> 00:17:53,430
Our barren planet looks

337
00:17:53,430 --> 00:17:57,003
like it could not contain anything related to life.

338
00:17:59,190 --> 00:18:01,710
<v ->The Earth during its very early lifetime</v>

339
00:18:01,710 --> 00:18:04,740
was not a friendly place for life at all.

340
00:18:04,740 --> 00:18:07,620
Imagine yourself standing on top

341
00:18:07,620 --> 00:18:10,680
of the early Earth just after it formed.

342
00:18:10,680 --> 00:18:12,450
This is not a happy place to be.

343
00:18:12,450 --> 00:18:14,580
It is excruciatingly hot.

344
00:18:14,580 --> 00:18:17,280
The surface is so hot that it's molten lava.

345
00:18:17,280 --> 00:18:19,230
You would not survive very long,

346
00:18:19,230 --> 00:18:20,973
but that is not your only problem.

347
00:18:22,230 --> 00:18:24,450
<v Narrator>4 1/2 billion years ago,</v>

348
00:18:24,450 --> 00:18:28,473
the solar system was vastly different from what it is today.

349
00:18:29,400 --> 00:18:32,550
<v ->Not only was the young Earth extremely hot,</v>

350
00:18:32,550 --> 00:18:35,280
extremely inhospitable to life as we know it,

351
00:18:35,280 --> 00:18:38,253
but it was about to face a very enormous challenge.

352
00:18:39,630 --> 00:18:42,990
<v Narrator>A catastrophic event was about to take place</v>

353
00:18:42,990 --> 00:18:46,453
that would change the history of Earth forever.

354
00:18:46,453 --> 00:18:49,120
(ominous music)

355
00:18:50,978 --> 00:18:53,760
(gentle music)

356
00:18:53,760 --> 00:18:56,490
It is the Moon that provides us with evidence

357
00:18:56,490 --> 00:18:58,143
of this first catastrophe.

358
00:18:58,980 --> 00:19:02,640
In 1969, the Apollo 11 mission brought back

359
00:19:02,640 --> 00:19:05,850
the first moon rock samples to earth.

360
00:19:05,850 --> 00:19:09,540
Since then, NASA has retrieved thousands of samples

361
00:19:09,540 --> 00:19:10,713
on their missions.

362
00:19:11,550 --> 00:19:14,940
Because the Moon, unlike our Earth, hasn't changed

363
00:19:14,940 --> 00:19:17,190
as much since its formation,

364
00:19:17,190 --> 00:19:19,500
these samples can help unravel

365
00:19:19,500 --> 00:19:21,993
how the past has shaped our present,

366
00:19:22,830 --> 00:19:25,050
holding the key to the mysteries

367
00:19:25,050 --> 00:19:28,233
of the emergence of the Moon and the Earth alike.

368
00:19:31,500 --> 00:19:32,793
Zurich, Switzerland.

369
00:19:34,070 --> 00:19:37,620
Every year, NASA distributes some of their moon samples

370
00:19:37,620 --> 00:19:40,683
to a select group of scientists around the world.

371
00:19:42,690 --> 00:19:44,430
Professor Maria Schonbachler

372
00:19:44,430 --> 00:19:47,310
at the Swiss Federal Institute of Technology

373
00:19:47,310 --> 00:19:49,113
is one of those recipients.

374
00:19:54,180 --> 00:19:56,070
<v Interpreter>They are much more valuable than gold.</v>

375
00:19:56,070 --> 00:20:00,630
So a gram like that is about 10 or 20 times more valuable.

376
00:20:00,630 --> 00:20:02,460
The lunar surface is very old

377
00:20:02,460 --> 00:20:04,770
and has hardly changed compared to the Earth,

378
00:20:04,770 --> 00:20:06,840
and that helps us decipher the secrets

379
00:20:06,840 --> 00:20:09,240
of the early Earth and the early Moon.

380
00:20:09,240 --> 00:20:11,820
The Moon is like a window back into the past,

381
00:20:11,820 --> 00:20:13,443
and I find that fascinating.

382
00:20:15,870 --> 00:20:17,850
<v Narrator>Professor Schonbachler is looking</v>

383
00:20:17,850 --> 00:20:21,450
for particular chemical signatures in the lunar rocks

384
00:20:21,450 --> 00:20:24,363
that might reveal clues about their origins.

385
00:20:25,200 --> 00:20:28,680
In an experiment, she now wants to compare the composition

386
00:20:28,680 --> 00:20:31,323
of the Moon to the composition of Earth.

387
00:20:33,630 --> 00:20:36,660
<v Interpreter>Here we have a dissolved sample of the Moon</v>

388
00:20:36,660 --> 00:20:38,733
and this is an Earth sample from Hawaii.

389
00:20:41,250 --> 00:20:42,720
Now we can analyze these

390
00:20:42,720 --> 00:20:45,543
and see how closely related Earth and Moon are.

391
00:20:48,420 --> 00:20:50,520
<v Narrator>Using isotope analysis,</v>

392
00:20:50,520 --> 00:20:54,600
Maria can compare the samples on an atomic level.

393
00:20:54,600 --> 00:20:57,270
She's particularly struck by the composition

394
00:20:57,270 --> 00:21:00,180
of the respective chromium isotopes.

395
00:21:00,180 --> 00:21:02,403
The measured values are astounding.

396
00:21:04,170 --> 00:21:05,910
<v Interpreter>What we see here are the measurements</v>

397
00:21:05,910 --> 00:21:08,103
from the Earth sample and the Moon sample.

398
00:21:09,030 --> 00:21:10,950
All the bars are identical.

399
00:21:10,950 --> 00:21:12,000
That means the Earth

400
00:21:12,000 --> 00:21:15,060
and the Moon have exactly the same fingerprint,

401
00:21:15,060 --> 00:21:19,110
and that in turn tells us they must be very closely related.

402
00:21:19,110 --> 00:21:22,980
So the Earth and the Moon are geological twins.

403
00:21:22,980 --> 00:21:25,683
The question now is, how did that come about?

404
00:21:29,880 --> 00:21:31,380
<v Narrator>There are multiple theories</v>

405
00:21:31,380 --> 00:21:33,990
about how the Moon was formed.

406
00:21:33,990 --> 00:21:36,660
The results of the analysis suggest

407
00:21:36,660 --> 00:21:39,030
that its formation is closely linked

408
00:21:39,030 --> 00:21:40,833
to the history of Earth.

409
00:21:43,080 --> 00:21:45,660
<v ->People have wondered for a really long time</v>

410
00:21:45,660 --> 00:21:48,233
how Earth's moon formed, and there have been a lot

411
00:21:48,233 --> 00:21:50,400
of different ideas how it happened.

412
00:21:50,400 --> 00:21:54,120
One of them was that the Moon actually was a little piece

413
00:21:54,120 --> 00:21:56,520
of the Earth that got broken off early

414
00:21:56,520 --> 00:21:58,563
in the lifetime of the planet.

415
00:21:59,790 --> 00:22:01,740
Another idea was that the Earth

416
00:22:01,740 --> 00:22:04,110
and Moon actually formed at the same time

417
00:22:04,110 --> 00:22:08,220
from the proto-planetary disc, like a little binary system.

418
00:22:08,220 --> 00:22:11,790
But the theory that has the most support now

419
00:22:11,790 --> 00:22:14,433
is actually much more spectacular.

420
00:22:17,910 --> 00:22:20,340
<v Narrator>4.5 billion years ago,</v>

421
00:22:20,340 --> 00:22:24,390
planetary embryos were circling around the Sun,

422
00:22:24,390 --> 00:22:27,060
together with a countless number of smaller

423
00:22:27,060 --> 00:22:29,373
but still huge chunks of rocks.

424
00:22:30,240 --> 00:22:33,723
The early solar system was a hazardous place.

425
00:22:37,560 --> 00:22:40,773
Maria Schonbachler can read this in the Moon's surface.

426
00:22:42,540 --> 00:22:44,430
<v Interpreter>The exciting thing about the Moon is</v>

427
00:22:44,430 --> 00:22:46,950
that its surface is very old.

428
00:22:46,950 --> 00:22:50,190
That means if we study the Moon, we also study the history

429
00:22:50,190 --> 00:22:52,773
of the Earth because it's a mirror image.

430
00:22:53,730 --> 00:22:56,070
And if we now look at the surface of the Moon

431
00:22:56,070 --> 00:22:58,050
and see all these craters,

432
00:22:58,050 --> 00:23:00,630
some of which are also extremely old,

433
00:23:00,630 --> 00:23:02,460
then we know that early Earth

434
00:23:02,460 --> 00:23:07,230
also suffered many impacts from asteroids or comets,

435
00:23:07,230 --> 00:23:08,283
just like the Moon.

436
00:23:10,170 --> 00:23:12,240
<v ->Just after the planets formed,</v>

437
00:23:12,240 --> 00:23:15,390
the solar system was a very dangerous place to be.

438
00:23:15,390 --> 00:23:17,940
There was material leftover from planet formation

439
00:23:17,940 --> 00:23:19,350
that was flying around.

440
00:23:19,350 --> 00:23:20,820
Collisions were common,

441
00:23:20,820 --> 00:23:22,920
and the Earth was about to experience one

442
00:23:22,920 --> 00:23:26,553
of the most catastrophic collisions in its entire history.

443
00:23:27,450 --> 00:23:30,030
<v Narrator>In the early days of our solar system,</v>

444
00:23:30,030 --> 00:23:32,193
Earth was being bombarded.

445
00:23:34,380 --> 00:23:37,020
<v ->The young solar system was a very violent place</v>

446
00:23:37,020 --> 00:23:38,733
and collisions were common.

447
00:23:41,010 --> 00:23:43,170
<v Narrator>But the most apocalyptic collision</v>

448
00:23:43,170 --> 00:23:46,563
in the history of our Earth was about to take place.

449
00:23:49,080 --> 00:23:53,100
At this time, Earth was an ocean of molten lava,

450
00:23:53,100 --> 00:23:55,170
hundreds of miles in depth,

451
00:23:55,170 --> 00:23:57,360
perpetually stirred up by the impacts

452
00:23:57,360 --> 00:23:59,283
of asteroids and comets.

453
00:24:00,210 --> 00:24:02,913
It had nearly reached its final size,

454
00:24:04,740 --> 00:24:07,950
but approaching from the dark void was Theia,

455
00:24:07,950 --> 00:24:11,313
a massive protoplanet the size of Mars.

456
00:24:12,150 --> 00:24:14,520
Like Earth, it had been growing quickly

457
00:24:14,520 --> 00:24:17,460
by consuming everything in its path

458
00:24:17,460 --> 00:24:20,746
and now it was heading straight for Earth.

459
00:24:20,746 --> 00:24:23,413
(ominous music)

460
00:24:25,955 --> 00:24:28,705
(impact booming)

461
00:24:33,060 --> 00:24:36,393
The impact of Theia nearly destroyed Earth.

462
00:24:37,260 --> 00:24:40,050
Vaporized chunks of our young planet's crust

463
00:24:40,050 --> 00:24:41,703
were thrown into space.

464
00:24:45,690 --> 00:24:49,140
<v ->The scale of this impact is hard to even imagine.</v>

465
00:24:49,140 --> 00:24:52,500
It was a hundred million times larger

466
00:24:52,500 --> 00:24:55,770
than the impact to Earth that we think killed the dinosaurs.

467
00:24:55,770 --> 00:25:00,030
The impact was so strong that Theia was obliterated,

468
00:25:00,030 --> 00:25:04,440
and what was left over was chunks of both Theia

469
00:25:04,440 --> 00:25:06,420
and the surface of the Earth

470
00:25:06,420 --> 00:25:10,200
that were ejected into orbit around Earth itself

471
00:25:10,200 --> 00:25:12,183
and were held in by Earth's gravity.

472
00:25:15,450 --> 00:25:18,540
That debris cloud flattened into a disc,

473
00:25:18,540 --> 00:25:21,960
not so different from the original disc around the young Sun

474
00:25:21,960 --> 00:25:23,550
where the first planets formed.

475
00:25:23,550 --> 00:25:26,430
As material orbited around the young Earth,

476
00:25:26,430 --> 00:25:28,380
you had small pebbles, small grains,

477
00:25:28,380 --> 00:25:30,603
bumping into each other that grew and grew.

478
00:25:32,670 --> 00:25:35,370
<v Narrator>Gas, dust, and rock coalesced</v>

479
00:25:35,370 --> 00:25:39,063
into a spherical shape that continued to orbit Earth.

480
00:25:39,930 --> 00:25:43,833
A new world was created, the Moon.

481
00:25:45,270 --> 00:25:47,793
But it was far from the one we know today.

482
00:25:48,990 --> 00:25:50,670
Right after its formation,

483
00:25:50,670 --> 00:25:53,160
the Moon was about 17 times closer

484
00:25:53,160 --> 00:25:55,473
to our planet than it is today.

485
00:25:56,310 --> 00:26:00,300
Its proximity to Earth had dire consequences,

486
00:26:00,300 --> 00:26:02,490
bringing violent instability

487
00:26:02,490 --> 00:26:04,743
to the molten planet it orbited.

488
00:26:05,760 --> 00:26:08,493
Earth had passed its baptism of fire.

489
00:26:09,660 --> 00:26:12,660
But even a long time after the impact,

490
00:26:12,660 --> 00:26:15,060
our planet was far from being a place

491
00:26:15,060 --> 00:26:16,833
where life could emerge.

492
00:26:21,060 --> 00:26:22,680
How this happened is one

493
00:26:22,680 --> 00:26:24,720
of the key questions that scientists

494
00:26:24,720 --> 00:26:27,720
at the Max Planck Institute for Solar System Research

495
00:26:27,720 --> 00:26:30,153
in Gottingen, Germany want to answer.

496
00:26:31,200 --> 00:26:34,200
One of them is Dr. Fred Goesmann.

497
00:26:34,200 --> 00:26:37,320
He participated in the European Space Agency's

498
00:26:37,320 --> 00:26:41,220
Rosetta Mission, where a probe was sent to a comet

499
00:26:41,220 --> 00:26:45,270
to look for earliest traces of life in our solar system.

500
00:26:45,270 --> 00:26:46,830
<v ->People came up with the idea in Europe,</v>

501
00:26:46,830 --> 00:26:48,120
let's fly to a comet.

502
00:26:48,120 --> 00:26:52,080
Let's not just fly past it, let's go to the comet,

503
00:26:52,080 --> 00:26:54,900
orbit it, land on it, and see what it's made of.

504
00:26:54,900 --> 00:26:57,960
And so the question is, did comets bring something

505
00:26:57,960 --> 00:27:00,273
which helped for life to emerge on Earth?

506
00:27:01,530 --> 00:27:06,330
<v Narrator>The comet known as 67P/Churyumov-Gerasimenko</v>

507
00:27:06,330 --> 00:27:08,880
was on an elliptical journey stretching

508
00:27:08,880 --> 00:27:10,920
between Jupiter at one end

509
00:27:10,920 --> 00:27:14,670
and the region between Earth and Mars at the other.

510
00:27:14,670 --> 00:27:18,690
The plan was for the Rosetta probe to travel with the comet,

511
00:27:18,690 --> 00:27:21,720
before dispatching a lander to the comet's surface

512
00:27:21,720 --> 00:27:23,613
to collect invaluable data.

513
00:27:24,510 --> 00:27:27,060
Fred Goesmann developed a special instrument

514
00:27:27,060 --> 00:27:29,010
for Rosetta's lander, Philae,

515
00:27:29,010 --> 00:27:32,580
that's capable of measuring the properties of the comet.

516
00:27:32,580 --> 00:27:36,330
<v ->Philae is a little bit of a small beast landing on a comet</v>

517
00:27:36,330 --> 00:27:38,100
and it has eyes, which are the camera,

518
00:27:38,100 --> 00:27:41,430
it's got a sense of feeling, which is the feet,

519
00:27:41,430 --> 00:27:42,990
and this thing was the nose.

520
00:27:42,990 --> 00:27:44,190
It is a chemical instrument.

521
00:27:44,190 --> 00:27:45,780
It's sniffing for molecules

522
00:27:45,780 --> 00:27:48,933
and identifying them by technical means.

523
00:27:49,800 --> 00:27:53,010
<v Narrator>In 2004, the Rosetta probe was launched</v>

524
00:27:53,010 --> 00:27:55,860
on its billion-kilometer journey.

525
00:27:55,860 --> 00:27:57,960
After a flight of 10 years,

526
00:27:57,960 --> 00:28:01,770
the spacecraft finally reached its destination.

527
00:28:01,770 --> 00:28:05,460
The optical instruments onboard Rosetta catched a glimpse

528
00:28:05,460 --> 00:28:07,173
of the strange looking comet.

529
00:28:09,660 --> 00:28:12,030
<v ->And it slowly grew in size, and you saw,</v>

530
00:28:12,030 --> 00:28:14,460
oh no, it looks like a rubber duck.

531
00:28:14,460 --> 00:28:16,893
And it was pretty clear, don't call it a duck.

532
00:28:17,850 --> 00:28:22,110
<v Narrator>Rosetta entered the orbit of Comet 67P.</v>

533
00:28:22,110 --> 00:28:25,443
Then, Philae was released to land on the surface.

534
00:28:29,220 --> 00:28:31,980
<v ->The landing itself was really exciting.</v>

535
00:28:31,980 --> 00:28:34,200
We saw images of the camera system of the orbiter

536
00:28:34,200 --> 00:28:35,520
that the legs had unfolded.

537
00:28:35,520 --> 00:28:36,353
It worked.

538
00:28:36,353 --> 00:28:37,770
The legs were nicely spread out,

539
00:28:37,770 --> 00:28:41,130
and so the thing came down and then we heard touchdown.

540
00:28:41,130 --> 00:28:42,600
We are on ground.

541
00:28:42,600 --> 00:28:44,640
People at ESA were cheering and everything,

542
00:28:44,640 --> 00:28:47,190
and then the engineers scratched their heads

543
00:28:47,190 --> 00:28:50,790
and said, no, it's moving.

544
00:28:50,790 --> 00:28:52,390
And that was really frightening.

545
00:28:53,430 --> 00:28:55,170
<v Narrator>The landing gear did not appear</v>

546
00:28:55,170 --> 00:28:56,763
to be working as planned.

547
00:28:58,530 --> 00:29:03,030
<v ->What we have here is one of the three landing legs.</v>

548
00:29:03,030 --> 00:29:05,460
So in order to stay on the cometary surface,

549
00:29:05,460 --> 00:29:07,800
which we already knew would be very difficult,

550
00:29:07,800 --> 00:29:12,060
we gave this lander harpoons, claws, teeth, everything.

551
00:29:12,060 --> 00:29:13,830
And this is one of the feet.

552
00:29:13,830 --> 00:29:16,470
When these paws touch the surface

553
00:29:16,470 --> 00:29:19,770
and they experience a force, are being pushed back,

554
00:29:19,770 --> 00:29:23,100
they could retract and push forward,

555
00:29:23,100 --> 00:29:24,930
we called it an ice screw.

556
00:29:24,930 --> 00:29:28,170
The idea was, well, you touch the surface

557
00:29:28,170 --> 00:29:29,700
and you recognize that

558
00:29:29,700 --> 00:29:32,610
by some motion in the mechanical system.

559
00:29:32,610 --> 00:29:35,460
And once that happened, you fire harpoons into the comet

560
00:29:35,460 --> 00:29:36,720
and then you secure everything.

561
00:29:36,720 --> 00:29:39,780
You pull the rope of the harpoon and everything.

562
00:29:39,780 --> 00:29:40,613
Nope.

563
00:29:41,730 --> 00:29:43,920
<v Narrator>The harpoons that should anchor Philae</v>

564
00:29:43,920 --> 00:29:46,113
to the landing spot failed.

565
00:29:46,980 --> 00:29:49,590
Untethered, Philae bounced off the comet

566
00:29:49,590 --> 00:29:51,540
for the next two hours.

567
00:29:51,540 --> 00:29:55,023
Finally, the lander settled in the shadow of a cliff.

568
00:29:56,340 --> 00:30:00,000
<v ->The final position where it came to rest was so awkward.</v>

569
00:30:00,000 --> 00:30:01,500
It wasn't standing on its legs.

570
00:30:01,500 --> 00:30:02,850
It was kind of up way,

571
00:30:02,850 --> 00:30:05,370
one leg was really pointing upwards.

572
00:30:05,370 --> 00:30:08,670
The drill was kind of poking into nowhere.

573
00:30:08,670 --> 00:30:10,023
It didn't reach the ground.

574
00:30:11,310 --> 00:30:13,710
So it did all its motions,

575
00:30:13,710 --> 00:30:15,180
but it didn't give us a sample

576
00:30:15,180 --> 00:30:18,900
because it couldn't touch anything.

577
00:30:18,900 --> 00:30:21,060
<v Narrator>It seemed that the billion-dollar mission</v>

578
00:30:21,060 --> 00:30:25,650
to find out more about the origin of life had failed.

579
00:30:25,650 --> 00:30:30,270
But despite things not going to plan, samples were taken.

580
00:30:30,270 --> 00:30:33,420
<v ->We were a bit fortunate because we hit the ground,</v>

581
00:30:33,420 --> 00:30:35,460
and obviously stuff was excavated

582
00:30:35,460 --> 00:30:37,650
and there was a plume of something coming up.

583
00:30:37,650 --> 00:30:39,510
And this very initial measurement

584
00:30:39,510 --> 00:30:41,370
where we just switch on the mass spectrometer

585
00:30:41,370 --> 00:30:43,830
to see what the environment tells us,

586
00:30:43,830 --> 00:30:47,100
only these two tiny minutes of measurements

587
00:30:47,100 --> 00:30:49,080
gave us a brilliant spectrum.

588
00:30:49,080 --> 00:30:50,580
For me, when I was seeing it,

589
00:30:50,580 --> 00:30:53,397
it was the most sexy mass spectrum in the world,

590
00:30:53,397 --> 00:30:55,200
and it still is.

591
00:30:55,200 --> 00:30:56,880
<v Narrator>After a thorough analysis</v>

592
00:30:56,880 --> 00:31:00,990
of the measurements, the comet's properties were revealed.

593
00:31:00,990 --> 00:31:05,700
It contained carbon, hydrogen, oxygen, nitrogen,

594
00:31:05,700 --> 00:31:06,993
and even more.

595
00:31:08,550 --> 00:31:10,950
<v ->We found molecules, organic molecules.</v>

596
00:31:10,950 --> 00:31:13,020
And if you put them in the right environment,

597
00:31:13,020 --> 00:31:15,180
they would be suitable to combine

598
00:31:15,180 --> 00:31:17,893
and to build anything you need in order to have life.

599
00:31:17,893 --> 00:31:20,400
I would say that if you have a planet

600
00:31:20,400 --> 00:31:21,930
and many comets fall onto it

601
00:31:21,930 --> 00:31:24,030
and they are of such composition,

602
00:31:24,030 --> 00:31:25,800
it would create an environment

603
00:31:25,800 --> 00:31:28,143
which life would be happy to thrive on.

604
00:31:29,700 --> 00:31:31,380
<v Narrator>Whether it was really comets</v>

605
00:31:31,380 --> 00:31:34,920
that started life on Earth is debated,

606
00:31:34,920 --> 00:31:37,710
but even if they did deliver the building blocks,

607
00:31:37,710 --> 00:31:42,630
our planet needed a radical change to enable life to evolve.

608
00:31:42,630 --> 00:31:46,290
There was still another ingredient that was missing.

609
00:31:46,290 --> 00:31:47,123
Water.

610
00:31:48,660 --> 00:31:51,480
Comets like 67P originate

611
00:31:51,480 --> 00:31:55,680
from beyond the orbit of Neptune or even farther out

612
00:31:55,680 --> 00:32:00,360
and are supposed to carry a lot of water in the form of ice.

613
00:32:00,360 --> 00:32:02,640
Many scientists, therefore, believe

614
00:32:02,640 --> 00:32:05,703
that comets also brought water to Earth.

615
00:32:06,870 --> 00:32:10,470
High resolution images of comet 67P

616
00:32:10,470 --> 00:32:13,863
indeed show the presence of water ice on the surface,

617
00:32:14,790 --> 00:32:16,950
but the analysis of the atomic makeup

618
00:32:16,950 --> 00:32:19,800
of the comet water shows that it is different

619
00:32:19,800 --> 00:32:21,573
from the water we have on Earth.

620
00:32:22,500 --> 00:32:24,030
This means that water

621
00:32:24,030 --> 00:32:27,750
on Earth cannot have been delivered by comets.

622
00:32:27,750 --> 00:32:30,033
It must have come from somewhere else.

623
00:32:32,700 --> 00:32:35,400
On September 12th, 2019,

624
00:32:35,400 --> 00:32:39,540
more than 500 people along the North Sea coast reported

625
00:32:39,540 --> 00:32:42,660
seeing a strange phenomenon across the sky

626
00:32:42,660 --> 00:32:43,863
in broad daylight.

627
00:32:44,820 --> 00:32:46,890
While filming a selfie video,

628
00:32:46,890 --> 00:32:50,340
a kite surfer from Northern Germany captured the event

629
00:32:50,340 --> 00:32:54,120
in the background, a flash of bright light.

630
00:32:54,120 --> 00:32:57,633
It was a meteorite on its way down to Earth.

631
00:32:58,590 --> 00:33:00,890
Professor Thorsten Kleine, director

632
00:33:00,890 --> 00:33:04,380
of the Max Planck Institute for Solar System Research,

633
00:33:04,380 --> 00:33:06,000
wants to find out if this piece

634
00:33:06,000 --> 00:33:09,240
of rock can help solve the riddle of water.

635
00:33:09,240 --> 00:33:11,730
<v ->A day after the flash, a 25-gram piece</v>

636
00:33:11,730 --> 00:33:15,090
of a meteorite has been found near Flensburg in Germany.

637
00:33:15,090 --> 00:33:17,820
It would've looked just like this, a black rock,

638
00:33:17,820 --> 00:33:19,350
not very spectacular looking,

639
00:33:19,350 --> 00:33:21,513
but scientifically extremely interesting.

640
00:33:22,890 --> 00:33:24,150
<v Narrator>The analysis shows</v>

641
00:33:24,150 --> 00:33:27,780
that the meteorite is nearly as old as the solar system,

642
00:33:27,780 --> 00:33:30,333
and that it is a piece from an asteroid.

643
00:33:31,230 --> 00:33:33,690
While comets are icy with tails

644
00:33:33,690 --> 00:33:36,270
and come from the outer solar system,

645
00:33:36,270 --> 00:33:39,000
asteroids are rocky and mainly stay

646
00:33:39,000 --> 00:33:41,853
in a belt between Mars and Jupiter.

647
00:33:43,170 --> 00:33:46,110
Because of their relative proximity to the Sun,

648
00:33:46,110 --> 00:33:49,170
they usually do not consist of ice.

649
00:33:49,170 --> 00:33:53,460
Nevertheless, the analysis in the lab shows Thorsten Kleine

650
00:33:53,460 --> 00:33:56,490
that they do carry a precious cargo.

651
00:33:56,490 --> 00:33:59,340
<v ->If you look into this, we can find hydrogen and oxygen,</v>

652
00:33:59,340 --> 00:34:02,430
the building blocks of water, bound into minerals.

653
00:34:02,430 --> 00:34:05,610
But most importantly, we can also find the signature is the

654
00:34:05,610 --> 00:34:08,820
same as it is for water from the Earth.

655
00:34:08,820 --> 00:34:09,990
That means that the water

656
00:34:09,990 --> 00:34:12,603
on our planet might have come from asteroids.

657
00:34:13,590 --> 00:34:15,540
<v Narrator>Further research also revealed</v>

658
00:34:15,540 --> 00:34:19,200
that mineral-bound-water-containing asteroids initially came

659
00:34:19,200 --> 00:34:21,870
together to form our planet.

660
00:34:21,870 --> 00:34:23,940
This means water could have been on Earth

661
00:34:23,940 --> 00:34:27,453
from the beginning, albeit not in liquid form.

662
00:34:31,080 --> 00:34:33,660
But how did the mineral-bound water transform

663
00:34:33,660 --> 00:34:35,640
the hellish early Earth into something

664
00:34:35,640 --> 00:34:37,323
that could host life one day?

665
00:34:38,250 --> 00:34:39,810
Over millions of years,

666
00:34:39,810 --> 00:34:43,113
the hot molten planet cooled enough to form a crust.

667
00:34:44,070 --> 00:34:47,370
The heat below the surface released, amongst others,

668
00:34:47,370 --> 00:34:51,003
oxygen and hydrogen that was bound in the minerals.

669
00:34:51,960 --> 00:34:55,080
The out gassing formed an atmosphere.

670
00:34:55,080 --> 00:34:57,420
Water vapor condensed and fell

671
00:34:57,420 --> 00:34:59,643
onto the rocky planet as rain.

672
00:35:00,600 --> 00:35:02,940
It rained for millions of years,

673
00:35:02,940 --> 00:35:05,493
long enough to create the first oceans.

674
00:35:07,290 --> 00:35:10,440
The world that had once been a ball of fire

675
00:35:10,440 --> 00:35:13,143
had become a world of water.

676
00:35:14,910 --> 00:35:17,940
200 million years after its formation,

677
00:35:17,940 --> 00:35:20,970
Earth is covered with liquid water.

678
00:35:20,970 --> 00:35:24,540
But despite this, there is no life yet

679
00:35:24,540 --> 00:35:28,980
because our planet is still a hostile place.

680
00:35:28,980 --> 00:35:31,443
One reason for this is our Moon.

681
00:35:32,400 --> 00:35:34,800
The impact of Theia has caused Earth

682
00:35:34,800 --> 00:35:39,063
to become bound to a new moon, and this is causing havoc.

683
00:35:39,900 --> 00:35:43,860
Over 4 billion years ago, the Moon was very different

684
00:35:43,860 --> 00:35:45,213
to what it is today.

685
00:35:46,380 --> 00:35:49,500
<v ->Just after the Moon formed, it was much closer</v>

686
00:35:49,500 --> 00:35:51,510
to the Earth than the Moon is today.

687
00:35:51,510 --> 00:35:53,340
More than 10 times closer.

688
00:35:53,340 --> 00:35:56,430
So it would've appeared very large in the sky,

689
00:35:56,430 --> 00:35:59,610
and not only that, but it would still be incredibly hot

690
00:35:59,610 --> 00:36:02,460
from the violent impact that formed it,

691
00:36:02,460 --> 00:36:04,440
and so it would be glowing.

692
00:36:04,440 --> 00:36:06,790
You'd be able to see it even during the daytime

693
00:36:08,284 --> 00:36:09,930
<v Narrator>With an object this large</v>

694
00:36:09,930 --> 00:36:11,520
and this close to Earth,

695
00:36:11,520 --> 00:36:14,283
cataclysmic effects shook our planet.

696
00:36:15,480 --> 00:36:18,030
<v ->The most important force that governs the motion</v>

697
00:36:18,030 --> 00:36:20,580
of the Earth and Moon is gravity.

698
00:36:20,580 --> 00:36:22,740
The Earth is exerting a gravitational pull

699
00:36:22,740 --> 00:36:24,543
on the Moon and vice versa.

700
00:36:25,500 --> 00:36:27,420
Similarly, when you're on a carousel

701
00:36:27,420 --> 00:36:30,330
and you're moving quickly around the center,

702
00:36:30,330 --> 00:36:33,750
there's a centrifugal force that is pushing you outwards

703
00:36:33,750 --> 00:36:35,340
and that's the exact same force

704
00:36:35,340 --> 00:36:38,623
that would be at play with the Earth and the Moon.

705
00:36:38,623 --> 00:36:42,070
<v Narrator>The moon tore at our young planet's surface.</v>

706
00:36:44,460 --> 00:36:48,120
<v ->This was a very dramatic environment for the early Earth.</v>

707
00:36:48,120 --> 00:36:52,380
The Moon's tidal forces were driving enormous waves

708
00:36:52,380 --> 00:36:55,290
in Earth's ocean, so every wave crashing on the shore

709
00:36:55,290 --> 00:36:57,390
would've been like a tsunami at that time.

710
00:36:58,770 --> 00:37:00,690
<v Narrator>The world of water was shaken</v>

711
00:37:00,690 --> 00:37:03,603
by the enormous force the Moon exerted.

712
00:37:04,470 --> 00:37:06,240
<v ->The Earth, during its early lifetime,</v>

713
00:37:06,240 --> 00:37:08,850
experienced some very tumultuous years.

714
00:37:08,850 --> 00:37:10,950
So you can think of the Earth kind of

715
00:37:10,950 --> 00:37:13,293
as a teenager early on in its life.

716
00:37:14,250 --> 00:37:15,690
<v Narrator>Not only the proximity</v>

717
00:37:15,690 --> 00:37:18,720
to the Moon was causing havoc at this time,

718
00:37:18,720 --> 00:37:22,770
Earth itself was also spinning up to six times faster

719
00:37:22,770 --> 00:37:25,590
around its axis than it is today.

720
00:37:25,590 --> 00:37:27,990
It was a wild planet.

721
00:37:27,990 --> 00:37:29,520
<v ->Just after the Moon was formed,</v>

722
00:37:29,520 --> 00:37:32,250
the Earth was spinning very, very fast.

723
00:37:32,250 --> 00:37:35,970
The length of the day was only about four hours.

724
00:37:35,970 --> 00:37:36,870
<v Narrator>Earth was far</v>

725
00:37:36,870 --> 00:37:39,720
from the hospitable world we have today,

726
00:37:39,720 --> 00:37:42,360
but this was about to change.

727
00:37:42,360 --> 00:37:45,900
The Moon, the very thing that was causing so much stress,

728
00:37:45,900 --> 00:37:50,190
was also about to help Earth take a vital step towards life.

729
00:37:50,190 --> 00:37:51,990
<v ->The Moon was tugging on the Earth</v>

730
00:37:51,990 --> 00:37:54,780
so strongly it actually caused

731
00:37:54,780 --> 00:37:58,590
something called tidal friction, which caused energy

732
00:37:58,590 --> 00:38:01,533
to be lost from the early Earth-Moon system.

733
00:38:02,700 --> 00:38:03,630
<v Narrator>Due to the fact</v>

734
00:38:03,630 --> 00:38:05,850
that the Moon tugs at our planet,

735
00:38:05,850 --> 00:38:08,400
the tides were created.

736
00:38:08,400 --> 00:38:12,120
Huge waves bulge out and exert a gravitational pull

737
00:38:12,120 --> 00:38:14,340
on their own on the Moon.

738
00:38:14,340 --> 00:38:16,560
Because it takes time for all that water

739
00:38:16,560 --> 00:38:18,330
to shift and pile up,

740
00:38:18,330 --> 00:38:20,910
the bulging oceans don't exactly match up

741
00:38:20,910 --> 00:38:22,830
with the position of the Moon.

742
00:38:22,830 --> 00:38:25,470
They are always a little out of sync.

743
00:38:25,470 --> 00:38:29,910
This creates friction that slows Earth's own rotation,

744
00:38:29,910 --> 00:38:32,130
albeit very slowly.

745
00:38:32,130 --> 00:38:37,130
Every 50,000 years, the days become one second longer.

746
00:38:37,620 --> 00:38:39,600
This also creates forces

747
00:38:39,600 --> 00:38:42,150
that change the Moon's orbital speed,

748
00:38:42,150 --> 00:38:45,453
causing it to slowly fall away into space.

749
00:38:47,910 --> 00:38:51,030
<v ->Today, the Moon is still moving away from the Earth,</v>

750
00:38:51,030 --> 00:38:54,330
little bit by little bit, about four centimeters per year.

751
00:38:54,330 --> 00:38:56,430
As the Moon moves away,

752
00:38:56,430 --> 00:38:58,590
the gravitational pull is a little bit less

753
00:38:58,590 --> 00:39:00,240
and that allows the Earth's rotation

754
00:39:00,240 --> 00:39:03,000
to slow down just a tiny bit.

755
00:39:03,000 --> 00:39:06,930
As this happens, the moon will slowly move away.

756
00:39:06,930 --> 00:39:09,453
The amount of friction decreases,

757
00:39:10,560 --> 00:39:14,340
leaving the Earth in a much more placid and calm place

758
00:39:14,340 --> 00:39:15,815
for the origin of life.

759
00:39:15,815 --> 00:39:16,950
(awe-inspiring music)

760
00:39:16,950 --> 00:39:18,237
<v Narrator>As time passed</v>

761
00:39:18,237 --> 00:39:20,700
and the Moon continued to move away,

762
00:39:20,700 --> 00:39:23,580
our days gradually got longer

763
00:39:23,580 --> 00:39:27,630
and Earth's rotation got slower and slower.

764
00:39:27,630 --> 00:39:31,860
The new Moon finally brought stability to our planet,

765
00:39:31,860 --> 00:39:35,433
setting the stage for life to begin.

766
00:39:39,660 --> 00:39:43,170
At the Ludwig Maximilian University in Munich, Germany,

767
00:39:43,170 --> 00:39:44,850
scientists want to find out

768
00:39:44,850 --> 00:39:47,733
how life might have evolved on early Earth.

769
00:39:48,870 --> 00:39:53,013
For Professor Oliver Trapp, chemistry is the key to life.

770
00:39:54,960 --> 00:39:57,090
<v ->You can create new molecules,</v>

771
00:39:57,090 --> 00:40:00,150
you can create new functionality,

772
00:40:00,150 --> 00:40:03,270
and you can make absolute new matter,

773
00:40:03,270 --> 00:40:05,370
which didn't exist before.

774
00:40:05,370 --> 00:40:09,690
And this was already fascinating me as a child.

775
00:40:09,690 --> 00:40:10,830
<v Narrator>In his laboratory,</v>

776
00:40:10,830 --> 00:40:12,990
Professor Trapp wants to understand

777
00:40:12,990 --> 00:40:17,400
how life formed over 4.3 billion years ago.

778
00:40:17,400 --> 00:40:19,740
<v ->My goal of this research is</v>

779
00:40:19,740 --> 00:40:24,740
that we discover a mechanism which led to evolution.

780
00:40:25,890 --> 00:40:29,103
<v Narrator>Oliver Trapp wants to form life in a test tube.</v>

781
00:40:30,210 --> 00:40:33,300
<v ->We try to simulate the processes</v>

782
00:40:33,300 --> 00:40:35,970
which took place on the early Earth.

783
00:40:35,970 --> 00:40:37,470
<v Narrator>Trapp's work is based</v>

784
00:40:37,470 --> 00:40:39,810
on a groundbreaking experiment.

785
00:40:39,810 --> 00:40:43,530
In 1953, biologist and chemist, Stanley Miller,

786
00:40:43,530 --> 00:40:45,510
and his mentor, Harold Urey,

787
00:40:45,510 --> 00:40:48,660
built a setup that tries to show that life emerged

788
00:40:48,660 --> 00:40:50,880
from a primordial soup.

789
00:40:50,880 --> 00:40:54,155
They injected ammonia, methane, and water vapor

790
00:40:54,155 --> 00:40:57,930
into an enclosed glass container to simulate

791
00:40:57,930 --> 00:41:00,540
what were then believed to be the conditions

792
00:41:00,540 --> 00:41:03,000
of Earth's early atmosphere.

793
00:41:03,000 --> 00:41:08,000
Finally, Miller and Urey also replicated lightning strikes.

794
00:41:08,340 --> 00:41:13,140
<v ->They induced a reaction by making sparks,</v>

795
00:41:13,140 --> 00:41:17,250
and the amazing outcome was that they observed the formation

796
00:41:17,250 --> 00:41:18,900
of amino acids.

797
00:41:18,900 --> 00:41:20,970
<v Narrator>Amino acids are the molecules</v>

798
00:41:20,970 --> 00:41:23,130
that combine to form proteins

799
00:41:23,130 --> 00:41:26,250
and are the building blocks of life on Earth.

800
00:41:26,250 --> 00:41:28,590
The experiment laid the foundation

801
00:41:28,590 --> 00:41:31,560
to further research on the origin of life,

802
00:41:31,560 --> 00:41:34,320
but Miller and Urey made one mistake.

803
00:41:34,320 --> 00:41:36,210
<v ->What they didn't know at this time</v>

804
00:41:36,210 --> 00:41:38,460
was the composition of the atmosphere.

805
00:41:38,460 --> 00:41:43,460
They assumed that we had an atmosphere with methane gas,

806
00:41:43,740 --> 00:41:46,773
and it turned out in the 90s that this was wrong.

807
00:41:47,940 --> 00:41:49,410
<v Narrator>Professor Trapp now wants</v>

808
00:41:49,410 --> 00:41:51,210
to repeat this experiment,

809
00:41:51,210 --> 00:41:55,050
but this time he's incorporating the latest understanding

810
00:41:55,050 --> 00:41:58,440
of the composition of ancient planet Earth.

811
00:41:58,440 --> 00:42:01,920
The starting ingredients is the inorganic matter

812
00:42:01,920 --> 00:42:04,143
that was available on early Earth.

813
00:42:06,630 --> 00:42:07,950
<v ->So we are starting really</v>

814
00:42:07,950 --> 00:42:09,960
from very, very simple molecules.

815
00:42:09,960 --> 00:42:13,740
We had carbon dioxide in the atmosphere.

816
00:42:13,740 --> 00:42:18,740
We had water also as vapor, as steam in the air,

817
00:42:19,170 --> 00:42:21,003
and, of course, nitrogen.

818
00:42:21,930 --> 00:42:24,120
<v Narrator>But Oliver Trapp also adds</v>

819
00:42:24,120 --> 00:42:26,580
a dissolved meteorite to the mix

820
00:42:26,580 --> 00:42:28,470
to duplicate the bombardments

821
00:42:28,470 --> 00:42:31,080
that took place on early Earth.

822
00:42:31,080 --> 00:42:35,670
By this, he creates simple organic molecules.

823
00:42:35,670 --> 00:42:39,300
Now, Professor Trapp puts this primordial soup

824
00:42:39,300 --> 00:42:41,850
into a container, together with water,

825
00:42:41,850 --> 00:42:44,760
which is heated to induce evaporation,

826
00:42:44,760 --> 00:42:46,710
replicating the water cycle

827
00:42:46,710 --> 00:42:50,100
as it may have been 4 billion years ago.

828
00:42:50,100 --> 00:42:54,480
Then comes the final important step of the experiment.

829
00:42:54,480 --> 00:42:55,920
<v ->This is a Tesla coil.</v>

830
00:42:55,920 --> 00:43:00,600
It generates sparks and this simulates day and night cycles,

831
00:43:00,600 --> 00:43:03,420
which is very important to have the energy

832
00:43:03,420 --> 00:43:06,510
from the Sun in our reaction setup.

833
00:43:06,510 --> 00:43:11,215
And I expect that this will trigger new reactions

834
00:43:11,215 --> 00:43:13,983
and provide new material.

835
00:43:15,480 --> 00:43:18,330
<v Narrator>1 million volts ionize the air</v>

836
00:43:18,330 --> 00:43:19,743
and generate lightning.

837
00:43:21,120 --> 00:43:22,920
Each flash replicates a day

838
00:43:22,920 --> 00:43:26,583
on which the Sun supplies our young planet with energy.

839
00:43:27,750 --> 00:43:32,643
By doing so, Professor Trapp simulates years of evolution.

840
00:43:34,470 --> 00:43:36,600
<v ->This actually doesn't look like much.</v>

841
00:43:36,600 --> 00:43:38,190
It looks like water.

842
00:43:38,190 --> 00:43:40,890
But if the experiment worked,

843
00:43:40,890 --> 00:43:43,740
we will have the first building blocks of life.

844
00:43:43,740 --> 00:43:45,960
<v Narrator>The molecules are much too small</v>

845
00:43:45,960 --> 00:43:47,940
for the eye to see.

846
00:43:47,940 --> 00:43:51,870
Using a gas chromatograph, Professor Trapp can find out

847
00:43:51,870 --> 00:43:55,110
what has formed in his primordial soup.

848
00:43:55,110 --> 00:43:58,620
<v ->This is adenosine, cytosine, and guanosine,</v>

849
00:43:58,620 --> 00:44:01,710
and these are the DNA building blocks.

850
00:44:01,710 --> 00:44:04,080
So far, we have not formed life,

851
00:44:04,080 --> 00:44:08,070
but I'm pretty sure that with this we can continue,

852
00:44:08,070 --> 00:44:10,950
and we will see the formation of life

853
00:44:10,950 --> 00:44:14,703
in a test tube starting from inorganic material.

854
00:44:15,927 --> 00:44:17,400
<v Narrator>It is these compounds</v>

855
00:44:17,400 --> 00:44:19,980
which would eventually kickstart the evolution

856
00:44:19,980 --> 00:44:21,543
of life on Earth.

857
00:44:22,410 --> 00:44:24,270
Over millions of years,

858
00:44:24,270 --> 00:44:26,640
these building blocks would replicate

859
00:44:26,640 --> 00:44:29,100
and assemble into cell membranes

860
00:44:29,100 --> 00:44:33,003
until eventually a single-celled organism emerged.

861
00:44:34,080 --> 00:44:38,160
This organism, which lived around 4 billion years ago,

862
00:44:38,160 --> 00:44:40,770
would become known as LUCA,

863
00:44:40,770 --> 00:44:44,070
our last universal common ancestor.

864
00:44:44,070 --> 00:44:46,917
But where on Earth did life begin?

865
00:44:46,917 --> 00:44:50,310
(dramatic music)

866
00:44:50,310 --> 00:44:55,260
One possibility is the deep sea around hydrothermal vents.

867
00:44:55,260 --> 00:44:57,900
Chimneys formed where seawater comes

868
00:44:57,900 --> 00:45:01,140
into contact with magma on the ocean floor,

869
00:45:01,140 --> 00:45:05,100
resulting in streams of super-heated plumes.

870
00:45:05,100 --> 00:45:07,170
But life may as well have formed

871
00:45:07,170 --> 00:45:11,160
in scalding, highly acidic hot springs environments,

872
00:45:11,160 --> 00:45:14,763
like those found today in the Yellowstone National Park.

873
00:45:16,020 --> 00:45:18,750
Eventually, the organism's ancestors

874
00:45:18,750 --> 00:45:21,453
will make the first step outside of water.

875
00:45:22,380 --> 00:45:26,313
How and why this happened is only just being revealed,

876
00:45:27,360 --> 00:45:29,730
but what is clear already is

877
00:45:29,730 --> 00:45:34,380
that our hostile Earth plays the central role

878
00:45:34,380 --> 00:45:36,573
in the evolution of life.

879
00:45:41,790 --> 00:45:44,010
One of the best places to understand

880
00:45:44,010 --> 00:45:47,880
just how hostile our early planet was can be found

881
00:45:47,880 --> 00:45:50,430
right here on Earth today.

882
00:45:50,430 --> 00:45:53,943
The Atacama is one of the driest deserts in the world.

883
00:45:54,930 --> 00:45:57,630
Here, a team of German biologists try

884
00:45:57,630 --> 00:46:01,260
to trace the ways in which early life evolved.

885
00:46:01,260 --> 00:46:04,050
And they want to find out how life was able

886
00:46:04,050 --> 00:46:06,796
to gain a foothold outside of water.

887
00:46:06,796 --> 00:46:08,875
<v ->Hi, Michael.</v>
<v ->Hi, Luis.</v>

888
00:46:08,875 --> 00:46:10,407
Nice to meet you.
<v ->Nice to meet you.</v>

889
00:46:10,407 --> 00:46:11,421
<v ->Hi, I'm Patrick.</v>

890
00:46:11,421 --> 00:46:12,600
Nice to meet you.
<v ->Hi, Luis.</v>

891
00:46:12,600 --> 00:46:14,700
Nice to meet you.
<v ->Hello.</v>

892
00:46:14,700 --> 00:46:17,460
<v Narrator>The Pan de Azucar National Park is part</v>

893
00:46:17,460 --> 00:46:19,650
of the Atacama Desert.

894
00:46:19,650 --> 00:46:21,330
Within the park, there is supposed

895
00:46:21,330 --> 00:46:25,440
to be an area which is particularly hostile to life,

896
00:46:25,440 --> 00:46:27,963
a place that is closed to the public.

897
00:46:30,810 --> 00:46:34,080
The deeper Patrick Jung and Michael Lakatos venture

898
00:46:34,080 --> 00:46:35,250
into the desert,

899
00:46:35,250 --> 00:46:38,490
the more barren the landscape becomes.

900
00:46:38,490 --> 00:46:42,990
Here, it is so dry that seemingly nothing grows anymore.

901
00:46:42,990 --> 00:46:45,453
The perfect place to search for life.

902
00:46:46,500 --> 00:46:47,880
On the desert floor,

903
00:46:47,880 --> 00:46:51,603
a dark crust is the only unusual thing they discover.

904
00:46:55,140 --> 00:46:57,233
<v Interpreter 1>Can you imagine what that might be?</v>

905
00:46:58,620 --> 00:47:00,240
<v Interpreter 2>It's mineral.</v>

906
00:47:00,240 --> 00:47:01,830
<v Interpreter 1>Do you really think so?</v>

907
00:47:01,830 --> 00:47:04,430
<v Interpreter 2>Yes. Those are black pebbles here.</v>

908
00:47:05,310 --> 00:47:06,600
<v Narrator>Closer analysis</v>

909
00:47:06,600 --> 00:47:10,200
of the desert floor amazes the scientists.

910
00:47:10,200 --> 00:47:13,320
Tiny dark cracks run through the pebbles.

911
00:47:13,320 --> 00:47:14,460
For the experts,

912
00:47:14,460 --> 00:47:18,333
this is a possible sign of biological activity.

913
00:47:21,150 --> 00:47:21,983
<v Interpreter>I have another idea.</v>

914
00:47:21,983 --> 00:47:23,260
You got that water bottle?

915
00:47:26,250 --> 00:47:27,360
<v Narrator>The scientists know</v>

916
00:47:27,360 --> 00:47:30,930
that this rock does not absorb water.

917
00:47:30,930 --> 00:47:33,960
If it does, this would be a clear sign

918
00:47:33,960 --> 00:47:36,453
that it has been penetrated by an organism.

919
00:47:39,990 --> 00:47:41,490
<v Interpreter 1>You see how it changes?</v>

920
00:47:41,490 --> 00:47:42,960
<v Interpreter 2>Oh, yeah.</v>

921
00:47:42,960 --> 00:47:44,783
<v Interpreter 1>Now let's give it a moment.</v>

922
00:47:46,560 --> 00:47:48,030
I'm going to look through there again,

923
00:47:48,030 --> 00:47:50,223
but I think I can see it turning green.

924
00:47:52,740 --> 00:47:54,090
<v Narrator>A change in color</v>

925
00:47:54,090 --> 00:47:56,100
would also indicate the presence

926
00:47:56,100 --> 00:47:57,993
of an organism in the stone.

927
00:47:59,340 --> 00:48:00,270
<v Interpreter>We just found out</v>

928
00:48:00,270 --> 00:48:01,950
that these are microorganisms

929
00:48:01,950 --> 00:48:04,290
that are sitting on these little pebbles,

930
00:48:04,290 --> 00:48:06,120
and now we have to take our instruments

931
00:48:06,120 --> 00:48:08,220
to find out what they are doing here,

932
00:48:08,220 --> 00:48:09,480
how they can survive,

933
00:48:09,480 --> 00:48:11,793
and what kind of microorganisms they are.

934
00:48:15,390 --> 00:48:16,440
<v Narrator>The scientists want</v>

935
00:48:16,440 --> 00:48:21,150
to find out whether these microorganisms are actually alive.

936
00:48:21,150 --> 00:48:24,060
For this, they are using a measuring device

937
00:48:24,060 --> 00:48:27,633
that is capable of detecting photosynthetic activity.

938
00:48:28,590 --> 00:48:31,530
First, they measure the dry rock.

939
00:48:31,530 --> 00:48:35,193
The red color of the display means no activity.

940
00:48:38,010 --> 00:48:39,030
<v Interpreter 1>So hold on.</v>

941
00:48:39,030 --> 00:48:40,503
I sprinkle it with water now.

942
00:48:44,580 --> 00:48:46,080
You can start the measurement.

943
00:48:49,410 --> 00:48:50,880
<v Interpreter 2>That's amazing.</v>

944
00:48:50,880 --> 00:48:53,040
<v Interpreter 1>It's alive.</v>

945
00:48:53,040 --> 00:48:55,110
We found out that there's a color change

946
00:48:55,110 --> 00:48:56,880
of the photosynthetic signal.

947
00:48:56,880 --> 00:48:59,520
That is, it flips from red to green and blue,

948
00:48:59,520 --> 00:49:03,060
and that shows us we actually have photosynthetic activity

949
00:49:03,060 --> 00:49:04,563
here, and therefore life.

950
00:49:07,290 --> 00:49:09,000
<v Narrator>With a field microscope,</v>

951
00:49:09,000 --> 00:49:10,290
the scientists now want

952
00:49:10,290 --> 00:49:13,320
to find out which organisms have been able

953
00:49:13,320 --> 00:49:16,383
to survive in this hostile environment.

954
00:49:19,740 --> 00:49:20,573
<v Interpreter 1>Michael, come here</v>

955
00:49:20,573 --> 00:49:23,430
and take a look at this.

956
00:49:23,430 --> 00:49:26,823
When I adjust the focus, you can see that there is a lichen.

957
00:49:28,590 --> 00:49:31,110
So you can see the fungal structures,

958
00:49:31,110 --> 00:49:33,240
and here the green algae.

959
00:49:33,240 --> 00:49:35,133
And also here. It's everywhere.

960
00:49:36,600 --> 00:49:38,663
<v Interpreter 2>That's really beautiful.</v>

961
00:49:39,690 --> 00:49:42,480
<v Narrator>Lichens are symbiotic microorganisms</v>

962
00:49:42,480 --> 00:49:46,290
that exist on Earth for about 400 million years.

963
00:49:46,290 --> 00:49:49,653
In this case, they consist of an algae and a fungus.

964
00:49:50,880 --> 00:49:53,790
<v Interpreter 1>The algae is photosynthetically active,</v>

965
00:49:53,790 --> 00:49:56,730
so it converts light, CO2 from the air,

966
00:49:56,730 --> 00:49:58,710
and water into sugars,

967
00:49:58,710 --> 00:50:02,040
and these sugars can be taken up by the fungus partner.

968
00:50:02,040 --> 00:50:02,913
It feeds on them.

969
00:50:03,750 --> 00:50:07,020
And in return, the fungus partner positions the algae

970
00:50:07,020 --> 00:50:09,060
in the lichen in an optimal position

971
00:50:09,060 --> 00:50:10,980
in the organism that is formed

972
00:50:10,980 --> 00:50:14,760
so that the algae can optimally photosynthesize.

973
00:50:14,760 --> 00:50:16,590
Only through this symbiosis can

974
00:50:16,590 --> 00:50:19,520
these individual partners survive here together

975
00:50:19,520 --> 00:50:21,063
in the Atacama Desert.

976
00:50:23,820 --> 00:50:25,830
<v Narrator>But from where does the organism</v>

977
00:50:25,830 --> 00:50:28,263
in this area get the vital water?

978
00:50:30,180 --> 00:50:31,710
<v Interpreter 1>We are in one of the driest</v>

979
00:50:31,710 --> 00:50:33,600
and oldest deserts on earth,

980
00:50:33,600 --> 00:50:36,120
but still we are only about 12 kilometers

981
00:50:36,120 --> 00:50:38,580
from the coast that is over here.

982
00:50:38,580 --> 00:50:41,940
Water vapor rises there, condenses out as fog,

983
00:50:41,940 --> 00:50:44,940
and then moves very flat across the landscape.

984
00:50:44,940 --> 00:50:47,280
That's a super small amount of water input,

985
00:50:47,280 --> 00:50:50,163
but that amount is enough to make life possible here.

986
00:50:52,830 --> 00:50:53,760
<v Narrator>With a drone,</v>

987
00:50:53,760 --> 00:50:56,070
the scientists now want to get an overview

988
00:50:56,070 --> 00:50:58,473
of the distribution of these organisms.

989
00:51:00,990 --> 00:51:03,480
<v Interpreter 1>Yeah. Go up a little bit more.</v>

990
00:51:03,480 --> 00:51:04,800
Right.

991
00:51:04,800 --> 00:51:07,500
Now if you go to the left another bit.

992
00:51:07,500 --> 00:51:09,510
<v Narrator>Gradually, the full extent</v>

993
00:51:09,510 --> 00:51:11,583
of the growth is revealed.

994
00:51:12,660 --> 00:51:15,410
<v Interpreter 1>Look at this. It's really everywhere.</v>

995
00:51:17,790 --> 00:51:20,700
<v Narrator>Patrick Jung and Michael Lakatos suspect</v>

996
00:51:20,700 --> 00:51:23,790
that the lichens here form a superorganism,

997
00:51:23,790 --> 00:51:27,120
comparable to a coral reef that covers large parts

998
00:51:27,120 --> 00:51:29,433
of the hostile Atacama Desert.

999
00:51:31,560 --> 00:51:33,450
<v Interpreter 1>The microorganisms that we found here</v>

1000
00:51:33,450 --> 00:51:35,940
are adapted to extreme locations.

1001
00:51:35,940 --> 00:51:36,960
By working together,

1002
00:51:36,960 --> 00:51:39,780
they have made this leap into the landscape,

1003
00:51:39,780 --> 00:51:41,910
and that's a comparable situation

1004
00:51:41,910 --> 00:51:44,583
to what we find in the early history of the Earth.

1005
00:51:45,480 --> 00:51:47,343
Through these abilities out of the cooperation

1006
00:51:47,343 --> 00:51:50,490
and symbiosis of adapted microorganisms,

1007
00:51:50,490 --> 00:51:54,033
life that originated in water might have leaped on land.

1008
00:51:56,160 --> 00:51:59,100
<v Narrator>After almost 4 billion years,</v>

1009
00:51:59,100 --> 00:52:04,050
life has developed innumerable characteristics and forms.

1010
00:52:04,050 --> 00:52:05,820
In the course of evolution,

1011
00:52:05,820 --> 00:52:09,870
highly complex living beings have developed.

1012
00:52:09,870 --> 00:52:13,770
But the road to the diversity we have today is a long

1013
00:52:13,770 --> 00:52:18,770
and rocky one that puts life to the test again and again.

1014
00:52:21,270 --> 00:52:24,030
However, one thing is for sure.

1015
00:52:24,030 --> 00:52:25,410
Without catastrophes,

1016
00:52:25,410 --> 00:52:28,320
like the apocalyptic collision with Theia,

1017
00:52:28,320 --> 00:52:31,980
life on Earth as we know it today

1018
00:52:31,980 --> 00:52:33,231
would not exist.

1019
00:52:33,231 --> 00:52:36,398
(awe-inspiring music)

1020
00:52:39,985 --> 00:52:42,735
(dramatic music)

1021
00:53:09,081 --> 00:53:12,664
(dramatic music continues)

