Destiny Wonders of the Universe


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Why are we here? Where do we come from?

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These are the most enduring of questions.

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And it's an essential part of human nature to want to find the answers.

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And we can trace that ancestry back

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hundreds of thousands of years to the dawn of humankind.

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But in reality, our story extends far further back in time.

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Our story starts with the beginning of the universe.

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It began 13.7 billion years ago.

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And today it's filled with over 100 billion galaxies,

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each containing hundreds of billions of stars.

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In the series, I want to tell that story

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because ultimately we are part of the universe.

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So its story is our story.

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It's a story that you couldn't tell without something so fundamental

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that it's impossible to imagine the universe without it.

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It's woven into the very fabric of the cosmos. Time.

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The relentless flow of time has driven the evolution of the universe

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and created many extraordinary wonders.

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These wonders take us from the very first moments in the life

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of the universe to its eventual end.

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This is Chankillo on the north-western coast of Peru.

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And it's one of South America's lesser known archaeological sites.

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But, for me, it is surely one of the most fascinating.

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Around 2,500 years ago,

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a civilisation we know almost nothing about

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built this fortified temple in the desert.

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Its walls were once brilliant white and covered with painted figures.

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Today, all but the smallest fragments

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of the decorations are gone.

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The details of this culture and all traces of its language are lost.

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And yet, if you stand in the right place, you can still experience

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the true purpose of Chankillo,

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in just the same way as you could the day that it was built.

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But, to do that, you have to be here before the sun rises.

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These towers form an ancient solar calendar.

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Now, at different times of year,

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the sunrise point is at a different place on the horizon.

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21st December, which here in the southern hemisphere

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is the summer solstice, the longest day,

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the sun rises just to the right of the right-most tower.

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Then, as the year passes, the sun moves through the towers

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until on 21st June, the winter solstice,

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the shortest day, it rises just to left of the left-most tower.

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Actually just in-between that mountain

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you can see in the distance and the left-most tower.

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So, at any time of year, if you watch the sun rise,

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you can measure its position and you can tell,

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within an accuracy of two or three days, the date.

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Today's date is September the 15th.

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So that means the sun

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will rise between the fifth and the sixth towers.

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Chankillo still works as a calendar

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because the sun still rises in the same place today

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as it did when these stones were first laid down.

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That's a magnificent sight, as the sun burns through the towers.

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You can almost feel the presence of the past here.

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Imagine what it must have been like.

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Thousands of citizens stood here to greet the sun,

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which was almost certainly a deity. Almost certainly their god.

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What a magnificent achievement.

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Probably one of our earliest attempts

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to begin to measure the heavens.

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Over the millennia,

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that desire to measure what's going on in the sky

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has led to modern astronomy

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and the foundations of our modern civilisation.

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I might build one in my garden.

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I want one!

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The 13 towers that line this ridge stand testament to our

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enduring fascination with the clockwork of the heavens.

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And to the direct connection between our lives and the cosmos.

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The rising and setting of the sun provides an epic heartbeat

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that allows us to mark the passage of time.

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A day on Earth is the 24 hours

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it takes our planet to rotate once on its axis.

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Our months are based on the 29-and-a-half days

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it takes the moon to wax and wane in the night sky.

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And a year is the 365-and-a-quarter days

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it takes us to orbit once around the sun.

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These familiar timescales mark the passing of our lives.

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But the life of the universe plays out on a much grander scale.

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When you look up into the night sky, you don't just see stars.

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Those tiny points of light are a million different clocks,

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whose lifespans mark out the passage of time over billions,

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or even trillions, of years.

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This film is about the greatest expanses of time.

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The deep time that shapes the universe.

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From its fiery beginnings, through countless generations of stars,

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planets and galaxies, to its eventual demise,

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the fate of the universe is determined by the passage of time.

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Timescales in the cosmos seem so unimaginably vast,

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it's almost impossible to relate to them.

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Yet there are places on Earth

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where we can begin to encounter time on these universal scales.

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This is Ostional on the northern Pacific coast of Costa Rica.

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I've come here to witness a natural event that's been happening

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long before there were any humans here to see it.

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And I suppose it really is a window

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into the distant past of life on our planet.

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Once the sun has dipped below the horizon

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and the moon conspired to make the tides just right,

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this beach is visited by prehistoric creatures.

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Under the cover of darkness, they emerge from the ocean.

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Playa Ostional is one of the few beaches in the world

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where large numbers of sea turtles make their nests.

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But what makes this truly remarkable is the sheer length of time

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scenes like this have been playing out.

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This is part of one of the oldest life-cycles on Earth.

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On nights like these, for the last 100 million years, turtles like this

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have been hauling themselves out of the ocean to lay their eggs.

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It's an almost incomprehensible timespan.

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100 million years ago, there were dinosaurs roaming the Earth,

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but the Earth itself looked very different.

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South America was not connected to North America.

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North America was somewhere over close to Europe.

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Australia was connected to Antarctica.

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It really is quite...

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wonderful to be so close to such an ancient cycle of life.

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I can hear breathing, actually.

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So, a remarkable experience.

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I mean, it really is beautiful to see that.

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On one night of many hundreds of millions of nights

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stretching back into the past.

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And she's gone.

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To witness a moment like this

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is to open up a connection to the deep past.

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To experience timespans far longer than the history of our own species.

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Yet even the 100-million-year story of the turtles

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only begins to connect us with the vast sweep of cosmic time.

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Our entire solar system is travelling

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on an unimaginably vast orbit,

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spinning around the centre of our galaxy.

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It takes 250 million years to make just one circuit of the Milky Way.

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In the entire history of the human race,

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we've travelled less than a tenth of 1% of that orbit.

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These cycles seem eternal and unchanging,

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but as the story of time unfolds, a fundamental truth is revealed.

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Nothing lasts forever.

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This is the most profound property of time.

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And it plays out just as vividly here on Earth

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as it does in the depths of space.

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Well, this is the Perito Moreno Glacier

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in Patagonia in southern Argentina.

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And it's one of the hundreds of glaciers

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that sweep down the continent from the southern Patagonian ice fields.

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And, you know, if you carry on that way, south about 1,000 kilometres,

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you get to the end of South America.

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From then on, there's nothing to the Antarctic.

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And it feels like that today.

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The glacier is such a massive expanse of ice that, at first sight,

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just like the cycles of the heavens, it appears fixed and unchanging.

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Yet, seen close-up, it's continually on the move.

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As it has been for tens of thousands of years.

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WATER CRASHES

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The whole face of the glacier is moving into the lake

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something like that much every day.

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That means that well over a quarter of a billion tonnes of ice

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drop off the face of the glacier into the lake every year.

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That's about a million tonnes a day. And you can hear it happening.

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Just every now and again, you hear this tremendous cracking sound.

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It really is like the place is alive.

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< CRACKING

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THUNDEROUS CRASH

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You know, it's quite disturbing when these enormous chunks of ice

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fall into the lake.

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Although this thing seems stable and the movement seems glacially slow,

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actually there can be really violent collapses.

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It's an incredibly dynamic place to be.

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The movement of the glacier

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provides an insight into the nature of time.

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It is simply the ordering of events into sequences.

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One step after another.

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As time passes, snow falls, ice forms,

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the glacier gradually inches down the valley

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and huge chunks of ice fall into the lake below.

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But even this simple sequence contains a profound idea.

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Events always happen in the same order.

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They're never jumbled up and they never go backwards.

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RUMBLING

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Now that's something that you would never see in reverse.

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But, interestingly, there's nothing in the laws of physics

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that describe how all those

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water molecules are moving around that prevent them

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from all getting together on the surface of the lake,

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jumping out of the water, sticking together into a block of ice

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and then gluing themselves back on to the surface of the glacier again.

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But, interestingly,

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we do understand why the world doesn't run in reverse.

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There is a reason.

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We have a scientific explanation.

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And it's called the arrow of time.

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We never see waves travelling across lakes,

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coming together and bouncing chunks of ice back onto glaciers.

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We are compelled to travel into the future.

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And that's because the arrow of time dictates that as each moment passes,

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things change.

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And once these changes have happened, they are never undone.

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Permanent change is a fundamental part of what it means to be human.

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We all age as the years pass by.

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People are born, they live, they die.

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I suppose it's part of the joy and tragedy of our lives.

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But out there in the universe,

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those grand and epic cycles appear eternal and unchanging.

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But that's an illusion.

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You see, in the life of the universe, just as in our lives,

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everything is irreversibly changing.

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By building change upon change,

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the arrow of time drives the evolution of the entire universe.

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And as we look out deep into the cosmos,

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we can see that story unfold.

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This is an image of a tiny piece of night sky

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in the constellation of Leo.

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It's actually where the mouth of the lion would be.

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And, despite appearances, it is one of the most interesting images

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taken in recent astronomical history.

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The interesting thing is this little red blob here,

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which looks very unremarkable.

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But what that red blob is is the afterglow

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of an enormous cosmic explosion. It's the death of a star.

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That was about...

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40 or even 50 times the mass of our sun.

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Poetically named GRB 090423, it was once a Wolf-Rayet star.

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Shrouded by rapidly swirling clouds of gas,

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it burned 10,000 times more brightly than our sun.

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But because it burned so brightly, it was extremely short-lived.

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As it died, the giant star collapsed in on itself.

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That caused massive jets of light and stellar material

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to be ejected from its poles,

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in an explosion that shone with the light of 10 million billion suns.

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And it's the afterglow of this catastrophic explosion

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that is just visible from our planet as a faint red dot.

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But that's not what's so interesting about GRB 090423.

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You see, when we look up into the sky, at distant stars and galaxies,

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then we're looking back in time

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because the light takes time to journey from them to us.

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And the light from that red dot has been travelling to us

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for almost the entire history of the universe.

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You see, what we're looking at here is an event that happened

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13 billion years ago.

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That's only about 600 million years after the Big Bang.

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After the universe began.

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So this is something incredibly early in the universe's history.

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In fact, this is the oldest single object that we've ever seen.

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What we're looking at here is the explosive death

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of one of the first stars in the universe.

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As it evolves, the universe passes through distinct eras.

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Vast ages, whose beginnings and endings

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are marked by unique milestones.

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The births and deaths of its wonders.

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The moment the first stars were born is one of the most important changes

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in the evolution of the cosmos.

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It signals the end of the Primordial Era

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and marks the beginning of the second great age of the universe.

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The time in which we live.

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The Stelliferous Era -

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the age of the stars.

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Starlight illuminates the night sky and starlight illuminates our days.

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Our sun is just one of 200 billion stars in our galaxy.

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Our galaxy is one of 100 billion in the observable universe.

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And countless islands of countless stars.

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Although the universe is over 13 billion years old,

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we still love close to the stars of the Stelliferous Era.

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It's an age of astonishing beauty and complexity in the universe.

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The cosmos is absolutely awash with stars surrounded by

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nebulae and systems of planets.

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Countless billions of worlds that we've yet to explore.

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But the cosmos isn't static and unchanging.

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It won't always be this way.

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Because, as the arrow of time plays out,

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it produces a universe that is as dynamic as it's beautiful.

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We've seen stars born and we've seen stars die.

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And we know that tomorrow won't be the same as today

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because the arrow of time says

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the future will always be different from the past.

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But what drives this evolution?

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Why is there a difference between the past and the future?

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Why is there an arrow of time at all?

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We all have an intuitive understanding of the arrow of time.

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It seems obvious to us that things change and the future

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will be different to the past.

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We know that because we see the effects

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of the passing years all around us.

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This is Kolmanskop, an abandoned diamond mining town

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in southern Namibia.

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This entire town was founded in 1908,

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when a worker who was building the railway from the port of Luderitz

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inland into the centre of Namibia found a single diamond

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here in this desert.

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For 40 years, this was a thriving community of up to 1,000 people.

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A place where you could become a millionaire,

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picking diamonds out of the sand.

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While the money rolled in, they built grand houses

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and lived a champagne lifestyle in the desert.

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But when the diamonds dried up, the town was abandoned.

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And for half a century

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it's fallen into disrepair as it's slowly reclaimed by the sands.

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The processes at play here at Kolmanskop

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are happening everywhere in the universe.

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Because it isn't simply permanent change

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that's central to the arrow of time.

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It's decay.

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But the scientific explanation for why that is...

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..didn't come from attempting to understand

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the effects of time in the universe.

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It came from trying to build a faster train.

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Back in the 19th century,

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engineers were concerned with the efficiency of steam engines.

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How hot should the fire be?

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What substance should you boil in the steam engine?

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Should it be water or something else?

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These were profound questions.

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And out of those questions arose the science of thermodynamics.

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It's when concepts like heat and temperature and energy

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entered the scientific vocabulary for the first time.

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Now, along with that deeper understanding

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emerged what is probably the most important law of physics

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for understanding the evolution of the universe

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and the passage of time.

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It's called the Second Law of Thermodynamics.

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The reason the Second Law of Thermodynamics was so profound

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was because, at its heart, it contained a radically new concept.

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Something physicists call "entropy".

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Entropy explains why, left to the mercy of the elements,

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mortar crumbles, glass shatters and buildings collapse.

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And a good way to understand how is to think of objects

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not as single things,

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but as being made up of many constituent parts.

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Like the individual grains that make up this pile of sand.

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Now, entropy is a measure of how many ways I can rearrange those

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grains and still keep the sand pile the same.

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And there are trillions and trillions and trillions

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of ways of doing that.

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I mean, pretty much anything I do to this sand pile,

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if I mess the sand around and move it around,

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then it doesn't change the shape or the structure at all.

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So, in the language of entropy,

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this sand pile has high entropy because there are many, many ways

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that I can rearrange its constituents and not change it.

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Now let me create some order in the universe.

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Now, there are approximately as many sand grains in this sand castle

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as there are in the sand pile.

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But now, virtually anything I do to it will mess it up,

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will remove the beautiful order from this structure.

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And because of that, the sand castle has a low entropy.

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It's a much more ordered state.

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So, many ways of rearranging the sand grains

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without changing the structure, high entropy.

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Very few ways of rearranging the sand grains

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without changing the structure, without disordering it, low entropy.

0:32:420:32:48

Imagine I was to leave this castle in the desert all day.

0:32:560:33:00

Then it's obvious what's going to happen.

0:33:000:33:02

The desert winds are going to blow the sand around

0:33:020:33:06

and this castle is going to disintegrate.

0:33:060:33:10

Is going to become less ordered. It's going to fall to bits.

0:33:100:33:13

But think about what's happening on the fundamental level.

0:33:160:33:20

I mean, the wind is taking the sand off the castle

0:33:200:33:24

and blowing it over there somewhere and making a sand pile.

0:33:240:33:28

There's nothing fundamental in the laws of physics

0:33:280:33:31

that says that the wind couldn't pick up some sand from over here,

0:33:310:33:36

deposit it here

0:33:360:33:38

and deposit it in precisely the shape of a sand castle.

0:33:380:33:42

In principle, the wind could spontaneously build a sand castle

0:33:420:33:47

out of a pile of sand.

0:33:470:33:48

There's no reason why that couldn't happen.

0:33:590:34:01

It's just extremely, extremely unlikely because there

0:34:010:34:05

are very few ways of organising this sand so that it looks like a castle.

0:34:050:34:10

It's overwhelmingly more likely

0:34:170:34:19

that when the wind blows the sand around

0:34:190:34:21

it will take the low entropy structure of the castle

0:34:210:34:25

and turn it into a high entropy structure, the sand pile.

0:34:250:34:29

So, entropy always increases. Why is that?

0:34:370:34:41

Because it's overwhelmingly more likely that it will.

0:34:410:34:45

It seems incredible that a law that says that sand castles

0:34:550:34:58

don't spontaneously form on the wind

0:34:580:35:02

could solve one of the deepest mysteries in physics.

0:35:020:35:05

But by saying entropy always increases,

0:35:080:35:11

the Second Law of Thermodynamics is able to explain

0:35:110:35:15

why time only runs in one direction.

0:35:150:35:18

The Second Law of Thermodynamics, for me, demonstrates everything

0:35:340:35:38

that's powerful and beautiful and profound about physics.

0:35:380:35:42

You see, here's a law that entered science

0:35:420:35:45

as a way of talking about how heat moves around

0:35:450:35:47

and the efficiency of steam engines.

0:35:470:35:49

But it ended up being able to explain one of the great mysteries

0:35:490:35:54

in the history of science.

0:35:540:35:57

Why is there a difference between the past and the future?

0:35:570:36:00

You see, the second law says

0:36:000:36:03

that everything tends from order to disorder.

0:36:030:36:07

That means that there is a difference

0:36:070:36:10

between the past and future.

0:36:100:36:12

In the past, the universe was more ordered.

0:36:120:36:14

In the future, the universe will be less ordered.

0:36:140:36:18

And that means there's a direction to the passage of time.

0:36:180:36:21

So the Second Law of Thermodynamics has introduced the concept

0:36:210:36:27

of an arrow of time into science.

0:36:270:36:30

The arrow of time has been playing out

0:36:380:36:40

in Kolmanskop since the mining facility was abandoned in 1954.

0:36:400:36:45

But in the universe,

0:36:480:36:49

it's been playing out for almost 14 billion years.

0:36:490:36:53

And it will have profound consequences.

0:36:530:36:56

Because it means stars cannot shine forever.

0:37:040:37:07

Including the star at the centre of our solar system.

0:37:070:37:12

At the end of its life, the sun won't simply fade away to nothing.

0:37:140:37:19

As it begins to run out of fuel, its core will collapse

0:37:220:37:27

and the extra heat this generates

0:37:270:37:29

will cause its outer layers to expand.

0:37:290:37:31

In around a billion years' time,

0:37:390:37:41

this will have a catastrophic effect on our fragile world.

0:37:410:37:45

Gradually, the Earth will become hotter and hotter.

0:37:520:37:55

So there will be one last perfect day on Earth.

0:37:550:37:59

But eventually the existence of all life on this planet

0:37:590:38:03

will become impossible.

0:38:030:38:05

TICKING

0:38:050:38:09

Long after a life has disappeared, the sun will have grown so much

0:38:090:38:14

it will fill the entire horizon.

0:38:140:38:16

It will become a red giant.

0:38:230:38:24

The last phase of its life.

0:38:240:38:27

Our planet might not survive to this point.

0:38:370:38:39

But, if it does, little more than a scorched and barren rock will remain

0:38:390:38:45

to witness the final death throes of our star.

0:38:450:38:49

In six billion years, our sun will explode.

0:39:000:39:04

Throwing vast amounts of gas and dust out into space,

0:39:040:39:08

to form a gigantic nebula.

0:39:080:39:10

And at its heart will beat a faintly glowing ember.

0:39:180:39:22

All that remains of our once magnificent sun.

0:39:220:39:26

It will be smaller than the size of the Earth.

0:39:260:39:28

Less than a millionth of its current volume

0:39:280:39:31

and a fraction of its brightness.

0:39:310:39:34

Our sun will have become a white dwarf.

0:39:340:39:37

With no fuel left to burn,

0:39:460:39:49

a white dwarf's faint glow comes from the last residual heat

0:39:490:39:53

from its extinguished furnace.

0:39:530:39:55

The sun is now dead.

0:39:580:40:00

Its remains slowly cooling in the freezing temperatures of deep space.

0:40:000:40:05

Looking at it from where the Earth is now,

0:40:100:40:12

it would only generate the same amount of light

0:40:120:40:15

as the full moon on a clear night.

0:40:150:40:17

The fate of the sun IS the same as for all stars.

0:40:230:40:27

One day, they must all eventually die

0:40:270:40:30

and the cosmos will be plunged into eternal night.

0:40:300:40:34

And this is the most profound consequence of the arrow of time.

0:40:340:40:39

Because this structured universe that we inhabit,

0:40:390:40:42

and all its wonders - the stars, the planets and the galaxies -

0:40:420:40:46

cannot last forever.

0:40:460:40:49

The cosmos will eventually fade and die.

0:40:490:40:54

First will come the end of the Stelliferous Era.

0:40:570:41:00

The end of the age of starlight.

0:41:000:41:03

The largest stars are the first to disappear,

0:41:080:41:11

violently collapsing into black holes.

0:41:110:41:13

Just a few million years after their formation.

0:41:130:41:16

But long after they're gone, just one type of star will remain.

0:41:190:41:23

This is a picture of the nearest star to our solar system,

0:41:270:41:31

Proxima Centauri.

0:41:310:41:32

It's only 4.2 light years away. But the reason it doesn't stand out

0:41:320:41:36

against the much more distant stars in this photograph

0:41:360:41:39

is that Proxima Centauri is incredibly tiny.

0:41:390:41:43

It's a kind of star known as a red dwarf star.

0:41:430:41:46

It's only about 11-12% the mass of our sun.

0:41:460:41:50

But to our eyes it would appear to shine 18,000 times less brightly.

0:41:500:41:56

But red dwarves do have one advantage over their much more

0:41:580:42:01

luminous and magnificent stellar brethren.

0:42:010:42:06

And that's because they're so small,

0:42:060:42:09

they burn their nuclear fuel incredibly slowly,

0:42:090:42:13

so they have lifespans of trillions of years.

0:42:130:42:16

And that means that stars like Proxima Centauri

0:42:160:42:20

will be the last living stars in the universe.

0:42:200:42:24

If we survive into the far future of the universe,

0:42:290:42:33

then it's possible to imagine our distant descendants building

0:42:330:42:38

their civilisation around red dwarves

0:42:380:42:41

to capture the energy from those last fading embers of stars,

0:42:410:42:46

just as our ancestors crowded around campfires

0:42:460:42:51

for warmth on cold winter's nights.

0:42:510:42:54

The reason why Proxima Centauri

0:43:130:43:15

burns so slowly is because its small size and low gravity

0:43:150:43:19

mean its core is under much lower pressure than larger stars.

0:43:190:43:23

This also means that its interior is constantly churning,

0:43:250:43:29

whipping up the surface into a fiery turmoil.

0:43:290:43:32

Explosive solar flares occur almost continually,

0:43:350:43:39

even though it burns so dimly.

0:43:390:43:41

But Proxima Centauri will eventually die.

0:43:430:43:48

And like our sun, it too will become a white dwarf.

0:43:480:43:52

As the age of starlight ends,

0:43:530:43:55

all but the dimmest flicker of light in the universe will go out.

0:43:550:44:00

The faint glow of white dwarves will provide the only illumination

0:44:000:44:05

in a dark and empty void, littered with dead stars and black holes.

0:44:050:44:12

By this point, the universe will be 100 trillion years old.

0:44:140:44:19

And yet, even now,

0:44:220:44:24

the vast majority of its lifespan still lies ahead of it.

0:44:240:44:29

There are few places on Earth where you can get an inkling

0:44:460:44:49

of what the far future has in store.

0:44:490:44:53

This is Namibia's Skeleton Coast,

0:45:060:45:08

where the cold water to the South Atlantic

0:45:080:45:11

meet the Namib Desert.

0:45:110:45:13

And it is one of the most inhospitable places on Earth.

0:45:130:45:16

Back in the 17th century,

0:45:160:45:18

Portuguese sailors used to call this place the "gates to hell"

0:45:180:45:22

because this dense fog

0:45:220:45:23

that you see pretty much every morning along this coast,

0:45:230:45:27

coupled with the constantly shifting shape of the sandbanks,

0:45:270:45:31

meant that over the years,

0:45:310:45:34

literally thousands of ships were wrecked along this coastline.

0:45:340:45:37

And even if you made it to shore, that wasn't the end of your problems

0:45:430:45:46

because the currents are so strong here

0:45:460:45:49

that there is no way of rowing back out to sea.

0:45:490:45:52

If you look that way,

0:45:520:45:53

there's just hundreds of miles of inhospitable desert.

0:45:530:45:57

So, it genuinely was a place of no return.

0:45:590:46:04

If you were shipwrecked here, this WAS the end of your universe.

0:46:040:46:09

This is the Eduard Bohlen.

0:46:200:46:22

She was once an ocean-going steamer,

0:46:220:46:25

ferrying passengers and cargo between here and Europe.

0:46:250:46:28

On 5th September, 1909, she ran aground in thick fog.

0:46:320:46:37

Yet, like all the vessels wrecked along this shoreline,

0:46:430:46:47

the time it takes her to decay to nothing

0:46:470:46:50

will be far longer than her time at sea.

0:46:500:46:52

In the far future of the cosmos,

0:46:570:47:00

a similar destiny awaits the remaining white dwarves.

0:47:000:47:04

A black dwarf will be the final fate of those last stars.

0:47:100:47:14

White dwarves that have become so cold

0:47:140:47:17

that they barely emit any more heat or light.

0:47:170:47:20

Black dwarves are dark, dense decaying balls of degenerate matter.

0:47:250:47:30

Little more than the ashes of stars.

0:47:300:47:33

Their constituent atoms are so severely crushed

0:47:340:47:39

that black dwarves are a million times denser than our sun.

0:47:390:47:44

Stars take so long to reach this point,

0:47:440:47:47

that after nearly 14 billion years

0:47:470:47:49

we believe there are currently no black dwarves in the universe.

0:47:490:47:54

But despite never seeing one,

0:47:540:47:57

we can still predict how they will end their days.

0:47:570:48:00

Just as the iron than makes up this ship

0:48:000:48:03

will eventually rust and be carried away by the desert winds,

0:48:030:48:08

so we think that the matter inside black dwarves,

0:48:080:48:12

the last matter in the universe,

0:48:120:48:14

will eventually evaporate away and be carried off

0:48:140:48:19

into the void as radiation,

0:48:190:48:21

leaving absolutely nothing behind.

0:48:210:48:25

With the black dwarves gone,

0:48:340:48:36

there won't be a single atom of matter left.

0:48:360:48:39

All that will remain of our once rich cosmos

0:48:420:48:45

will be particles of light and black holes.

0:48:450:48:49

After an unimaginable length of time,

0:48:550:48:59

even the black holes will have evaporated

0:48:590:49:02

and the universe will be nothing but a sea of photons,

0:49:020:49:06

gradually tending towards the same temperature,

0:49:060:49:10

as the expansion of the universe cools them towards absolute zero.

0:49:100:49:14

And when I say "unimaginable period of time," I really mean it.

0:49:230:49:26

It's 10,000 trillion trillion

0:49:260:49:28

trillion trillion trillion trillion trillion trillion years.

0:49:280:49:33

How big's that number?

0:49:330:49:35

If I were to start counting with a single atom representing one year

0:49:350:49:41

then there wouldn't be enough atoms in the entire universe

0:49:410:49:45

to get anywhere near that number.

0:49:450:49:48

Once the very last remnants

0:49:540:49:56

of the very last stars have finally decayed away to nothing,

0:49:560:50:00

and everything reaches the same temperature,

0:50:000:50:04

the story of the universe finally comes to an end.

0:50:040:50:08

For the first time in its life,

0:50:120:50:14

the universe will be permanent and unchanging.

0:50:140:50:18

Entropy finally stops increasing

0:50:180:50:20

because the cosmos cannot get any more disordered.

0:50:200:50:25

Nothing happens and it keeps not happening.

0:50:250:50:29

Forever.

0:50:290:50:31

It's what's known as the heat death of the universe.

0:50:360:50:38

An era when the cosmos will remain vast and cold and desolate

0:50:380:50:44

for the rest of time.

0:50:440:50:46

But that's because there is no difference between the past,

0:50:460:50:49

the present and the future.

0:50:490:50:51

There's no way of measuring the passage of time

0:50:510:50:55

because nothing in the cosmos changes.

0:50:550:50:58

The arrow of time has simply ceased to exist.

0:50:580:51:02

It's an inescapable fact of the universe,

0:51:130:51:16

written into the fundamental laws of physics.

0:51:160:51:19

The entire cosmos will die.

0:51:190:51:22

Every single one of the 200 billion stars in our galaxy will go out.

0:51:270:51:33

And just as the death of the sun means the end of life on our planet,

0:51:360:51:41

so the death of every star

0:51:410:51:43

will extinguish any possibility of life in the universe.

0:51:430:51:47

The fact that the sun will die and it will incinerate the Earth

0:51:510:51:56

and obliterate all life on our planet in the process,

0:51:560:52:00

might sound a bit depressing to you.

0:52:000:52:02

You might legitimately ask,

0:52:020:52:04

"Well, surely you could build a universe in a different way?

0:52:040:52:08

"Surely you could build it

0:52:080:52:09

"so it didn't have to descend from order into chaos?"

0:52:090:52:13

Well, the answer is no,

0:52:130:52:14

you couldn't, if you wanted life to exist in it.

0:52:140:52:18

The arrow of time,

0:52:240:52:25

the sequence of changes that slowly leads the universe to its death,

0:52:250:52:30

is the very same thing that creates the conditions

0:52:300:52:33

for life in the first place.

0:52:330:52:35

Because it takes time for matter to form

0:52:400:52:42

and it takes time for gravity to pull it together

0:52:420:52:46

into stars and planets.

0:52:460:52:48

The arrow of time creates a bright window

0:52:530:52:55

in the universe's adolescence.

0:52:550:52:58

During which, life is possible.

0:52:580:53:00

But it's a window that doesn't stay open for long.

0:53:070:53:11

As a fraction of the lifespan of the universe,

0:53:140:53:17

as measured from its beginning to the evaporation

0:53:170:53:21

of the last black hole,

0:53:210:53:23

life, as we know it, is only possible for one thousandth

0:53:230:53:28

of a billion billion billionth billion billion billionth

0:53:280:53:32

billion billion billionth of a per cent.

0:53:320:53:35

And that's why, for me,

0:53:370:53:39

the most astonishing wonder of the universe isn't a star

0:53:390:53:44

or a planet or a galaxy.

0:53:440:53:47

It isn't a thing at all.

0:53:470:53:49

It's an instant in time.

0:53:490:53:52

And that time is now.

0:53:520:53:55

Humans have walked the Earth for just the smallest fraction

0:54:030:54:07

of that briefest of moments in deep time.

0:54:070:54:11

But in our 200,000 years on this planet,

0:54:140:54:16

we've made remarkable progress.

0:54:160:54:19

It was only 2,500 years ago that we believed that the sun was a god

0:54:220:54:27

and measured its orbit with stone towers,

0:54:270:54:30

built on the top of a hill.

0:54:300:54:32

Today, the language of curiosity is not sun gods, but science.

0:54:320:54:39

And we have observatories that are almost infinitely more sophisticated

0:54:390:54:44

than the 13 towers, that can gaze out deep into the universe.

0:54:440:54:49

And, perhaps even more remarkably,

0:54:520:54:55

through theoretical physics and mathematics,

0:54:550:54:57

we can calculate what the universe will look like

0:54:570:55:01

in the distant future.

0:55:010:55:03

And we can even make concrete predictions about its end.

0:55:030:55:08

And I believe it's only by continuing

0:55:150:55:17

our exploration of the cosmos

0:55:170:55:19

and the laws of nature that govern it,

0:55:190:55:22

that we can truly understand ourselves

0:55:220:55:26

and our place in this universe of wonders.

0:55:260:55:29

And that's what we've done in our brief moment on Planet Earth.

0:55:330:55:38

In 1977, a space probe called Voyager 1

0:55:410:55:45

was launched on a grand tour of the solar system.

0:55:450:55:49

And it visited the great gas giant planets -

0:55:490:55:52

Jupiter and Saturn - and made some wonderful discoveries

0:55:520:55:56

before heading off towards interstellar space.

0:55:560:56:00

13 years later, after its mission was almost over,

0:56:020:56:06

it turned around and took one last picture of its home solar system.

0:56:060:56:12

This is that picture.

0:56:120:56:14

And the beautiful thing about this picture

0:56:170:56:20

is this single pixel of light

0:56:200:56:24

suspended against the blackness of space.

0:56:240:56:26

Because that pixel, that point, is Planet Earth.

0:56:260:56:31

The most distant picture of our planet ever taken.

0:56:310:56:34

6 billion kilometres away.

0:56:340:56:37

And whilst I suppose it has very limited scientific value,

0:56:470:56:51

for me, this tiny point of light

0:56:510:56:54

is the most powerful and profound demonstration

0:56:540:56:58

of perhaps the most human of qualities.

0:56:580:57:01

Our unique ability to reflect on the universe's existence

0:57:010:57:06

and our place within it.

0:57:060:57:08

Just as we, and all life on Earth, stand on this tiny speck

0:57:130:57:18

adrift in infinite space, so life in the universe will only exist

0:57:180:57:25

for a fleeting bright instance in time

0:57:250:57:29

because life, just like the stars and the planets and the galaxies,

0:57:290:57:35

is just a temporary structure on the long road from order to disorder.

0:57:350:57:40

But that doesn't make us insignificant

0:57:490:57:52

because we are the cosmos made conscious.

0:57:520:57:54

Life is the means by which the universe understands itself.

0:57:540:57:59

And, for me, our true significance lies in our ability

0:58:020:58:06

and our desire to understand and explore this beautiful universe.

0:58:060:58:12

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0:58:550:58:58

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