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Why are we here? Where do we come from? | 0:00:11 | 0:00:14 | |
These are the most enduring of questions. | 0:00:14 | 0:00:17 | |
And it's an essential part of human nature to want to find the answers. | 0:00:17 | 0:00:22 | |
And we can trace that ancestry back | 0:00:28 | 0:00:30 | |
hundreds of thousands of years to the dawn of humankind. | 0:00:30 | 0:00:34 | |
But in reality, our story extends far further back in time. | 0:00:34 | 0:00:39 | |
Our story starts with the beginning of the universe. | 0:00:39 | 0:00:43 | |
It began 13.7 billion years ago. | 0:00:47 | 0:00:51 | |
And today it's filled with over 100 billion galaxies, | 0:00:56 | 0:00:59 | |
each containing hundreds of billions of stars. | 0:00:59 | 0:01:03 | |
In the series, I want to tell that story | 0:01:09 | 0:01:12 | |
because ultimately we are part of the universe. | 0:01:12 | 0:01:16 | |
So its story is our story. | 0:01:16 | 0:01:19 | |
It's a story that you couldn't tell without something so fundamental | 0:01:24 | 0:01:28 | |
that it's impossible to imagine the universe without it. | 0:01:28 | 0:01:31 | |
It's woven into the very fabric of the cosmos. Time. | 0:01:31 | 0:01:36 | |
The relentless flow of time has driven the evolution of the universe | 0:01:41 | 0:01:46 | |
and created many extraordinary wonders. | 0:01:46 | 0:01:49 | |
These wonders take us from the very first moments in the life | 0:01:51 | 0:01:55 | |
of the universe to its eventual end. | 0:01:55 | 0:01:58 | |
This is Chankillo on the north-western coast of Peru. | 0:02:27 | 0:02:32 | |
And it's one of South America's lesser known archaeological sites. | 0:02:32 | 0:02:37 | |
But, for me, it is surely one of the most fascinating. | 0:02:37 | 0:02:40 | |
Around 2,500 years ago, | 0:02:49 | 0:02:51 | |
a civilisation we know almost nothing about | 0:02:51 | 0:02:54 | |
built this fortified temple in the desert. | 0:02:54 | 0:02:57 | |
Its walls were once brilliant white and covered with painted figures. | 0:03:02 | 0:03:07 | |
Today, all but the smallest fragments | 0:03:11 | 0:03:14 | |
of the decorations are gone. | 0:03:14 | 0:03:15 | |
The details of this culture and all traces of its language are lost. | 0:03:15 | 0:03:21 | |
And yet, if you stand in the right place, you can still experience | 0:03:26 | 0:03:29 | |
the true purpose of Chankillo, | 0:03:29 | 0:03:32 | |
in just the same way as you could the day that it was built. | 0:03:32 | 0:03:36 | |
But, to do that, you have to be here before the sun rises. | 0:03:40 | 0:03:44 | |
These towers form an ancient solar calendar. | 0:03:59 | 0:04:02 | |
Now, at different times of year, | 0:04:02 | 0:04:05 | |
the sunrise point is at a different place on the horizon. | 0:04:05 | 0:04:09 | |
21st December, which here in the southern hemisphere | 0:04:09 | 0:04:12 | |
is the summer solstice, the longest day, | 0:04:12 | 0:04:15 | |
the sun rises just to the right of the right-most tower. | 0:04:15 | 0:04:20 | |
Then, as the year passes, the sun moves through the towers | 0:04:20 | 0:04:24 | |
until on 21st June, the winter solstice, | 0:04:24 | 0:04:28 | |
the shortest day, it rises just to left of the left-most tower. | 0:04:28 | 0:04:33 | |
Actually just in-between that mountain | 0:04:33 | 0:04:35 | |
you can see in the distance and the left-most tower. | 0:04:35 | 0:04:38 | |
So, at any time of year, if you watch the sun rise, | 0:04:38 | 0:04:42 | |
you can measure its position and you can tell, | 0:04:42 | 0:04:45 | |
within an accuracy of two or three days, the date. | 0:04:45 | 0:04:49 | |
Today's date is September the 15th. | 0:04:49 | 0:04:53 | |
So that means the sun | 0:04:53 | 0:04:54 | |
will rise between the fifth and the sixth towers. | 0:04:54 | 0:04:58 | |
Chankillo still works as a calendar | 0:05:10 | 0:05:12 | |
because the sun still rises in the same place today | 0:05:12 | 0:05:16 | |
as it did when these stones were first laid down. | 0:05:16 | 0:05:19 | |
That's a magnificent sight, as the sun burns through the towers. | 0:05:24 | 0:05:29 | |
You can almost feel the presence of the past here. | 0:05:36 | 0:05:39 | |
Imagine what it must have been like. | 0:05:39 | 0:05:41 | |
Thousands of citizens stood here to greet the sun, | 0:05:41 | 0:05:45 | |
which was almost certainly a deity. Almost certainly their god. | 0:05:45 | 0:05:48 | |
What a magnificent achievement. | 0:05:48 | 0:05:51 | |
Probably one of our earliest attempts | 0:05:51 | 0:05:54 | |
to begin to measure the heavens. | 0:05:54 | 0:05:57 | |
Over the millennia, | 0:06:10 | 0:06:12 | |
that desire to measure what's going on in the sky | 0:06:12 | 0:06:16 | |
has led to modern astronomy | 0:06:16 | 0:06:18 | |
and the foundations of our modern civilisation. | 0:06:18 | 0:06:22 | |
I might build one in my garden. | 0:06:31 | 0:06:33 | |
I want one! | 0:06:37 | 0:06:39 | |
The 13 towers that line this ridge stand testament to our | 0:06:48 | 0:06:52 | |
enduring fascination with the clockwork of the heavens. | 0:06:52 | 0:06:57 | |
And to the direct connection between our lives and the cosmos. | 0:06:57 | 0:07:03 | |
The rising and setting of the sun provides an epic heartbeat | 0:07:04 | 0:07:08 | |
that allows us to mark the passage of time. | 0:07:08 | 0:07:11 | |
A day on Earth is the 24 hours | 0:07:19 | 0:07:22 | |
it takes our planet to rotate once on its axis. | 0:07:22 | 0:07:25 | |
Our months are based on the 29-and-a-half days | 0:07:34 | 0:07:37 | |
it takes the moon to wax and wane in the night sky. | 0:07:37 | 0:07:41 | |
And a year is the 365-and-a-quarter days | 0:07:44 | 0:07:48 | |
it takes us to orbit once around the sun. | 0:07:48 | 0:07:52 | |
These familiar timescales mark the passing of our lives. | 0:07:54 | 0:07:59 | |
But the life of the universe plays out on a much grander scale. | 0:07:59 | 0:08:04 | |
When you look up into the night sky, you don't just see stars. | 0:08:08 | 0:08:12 | |
Those tiny points of light are a million different clocks, | 0:08:12 | 0:08:17 | |
whose lifespans mark out the passage of time over billions, | 0:08:17 | 0:08:21 | |
or even trillions, of years. | 0:08:21 | 0:08:23 | |
This film is about the greatest expanses of time. | 0:08:32 | 0:08:36 | |
The deep time that shapes the universe. | 0:08:36 | 0:08:40 | |
From its fiery beginnings, through countless generations of stars, | 0:08:42 | 0:08:46 | |
planets and galaxies, to its eventual demise, | 0:08:46 | 0:08:50 | |
the fate of the universe is determined by the passage of time. | 0:08:50 | 0:08:55 | |
Timescales in the cosmos seem so unimaginably vast, | 0:09:04 | 0:09:08 | |
it's almost impossible to relate to them. | 0:09:08 | 0:09:10 | |
Yet there are places on Earth | 0:09:12 | 0:09:14 | |
where we can begin to encounter time on these universal scales. | 0:09:14 | 0:09:18 | |
This is Ostional on the northern Pacific coast of Costa Rica. | 0:09:26 | 0:09:32 | |
I've come here to witness a natural event that's been happening | 0:09:32 | 0:09:37 | |
long before there were any humans here to see it. | 0:09:37 | 0:09:40 | |
And I suppose it really is a window | 0:09:40 | 0:09:43 | |
into the distant past of life on our planet. | 0:09:43 | 0:09:46 | |
Once the sun has dipped below the horizon | 0:10:09 | 0:10:11 | |
and the moon conspired to make the tides just right, | 0:10:11 | 0:10:16 | |
this beach is visited by prehistoric creatures. | 0:10:16 | 0:10:20 | |
Under the cover of darkness, they emerge from the ocean. | 0:10:31 | 0:10:34 | |
Playa Ostional is one of the few beaches in the world | 0:10:43 | 0:10:46 | |
where large numbers of sea turtles make their nests. | 0:10:46 | 0:10:49 | |
But what makes this truly remarkable is the sheer length of time | 0:11:00 | 0:11:04 | |
scenes like this have been playing out. | 0:11:04 | 0:11:07 | |
This is part of one of the oldest life-cycles on Earth. | 0:11:13 | 0:11:17 | |
On nights like these, for the last 100 million years, turtles like this | 0:11:17 | 0:11:22 | |
have been hauling themselves out of the ocean to lay their eggs. | 0:11:22 | 0:11:27 | |
It's an almost incomprehensible timespan. | 0:11:29 | 0:11:32 | |
100 million years ago, there were dinosaurs roaming the Earth, | 0:11:32 | 0:11:36 | |
but the Earth itself looked very different. | 0:11:36 | 0:11:39 | |
South America was not connected to North America. | 0:11:39 | 0:11:43 | |
North America was somewhere over close to Europe. | 0:11:43 | 0:11:47 | |
Australia was connected to Antarctica. | 0:11:47 | 0:11:50 | |
It really is quite... | 0:11:57 | 0:11:59 | |
wonderful to be so close to such an ancient cycle of life. | 0:11:59 | 0:12:04 | |
I can hear breathing, actually. | 0:12:05 | 0:12:08 | |
So, a remarkable experience. | 0:12:20 | 0:12:23 | |
I mean, it really is beautiful to see that. | 0:12:23 | 0:12:26 | |
On one night of many hundreds of millions of nights | 0:12:26 | 0:12:30 | |
stretching back into the past. | 0:12:30 | 0:12:33 | |
And she's gone. | 0:12:41 | 0:12:43 | |
To witness a moment like this | 0:12:53 | 0:12:56 | |
is to open up a connection to the deep past. | 0:12:56 | 0:12:59 | |
To experience timespans far longer than the history of our own species. | 0:13:02 | 0:13:07 | |
Yet even the 100-million-year story of the turtles | 0:13:09 | 0:13:13 | |
only begins to connect us with the vast sweep of cosmic time. | 0:13:13 | 0:13:18 | |
Our entire solar system is travelling | 0:13:25 | 0:13:28 | |
on an unimaginably vast orbit, | 0:13:28 | 0:13:30 | |
spinning around the centre of our galaxy. | 0:13:30 | 0:13:33 | |
It takes 250 million years to make just one circuit of the Milky Way. | 0:13:40 | 0:13:46 | |
In the entire history of the human race, | 0:13:53 | 0:13:56 | |
we've travelled less than a tenth of 1% of that orbit. | 0:13:56 | 0:14:01 | |
These cycles seem eternal and unchanging, | 0:14:05 | 0:14:10 | |
but as the story of time unfolds, a fundamental truth is revealed. | 0:14:10 | 0:14:15 | |
Nothing lasts forever. | 0:14:20 | 0:14:22 | |
This is the most profound property of time. | 0:14:29 | 0:14:32 | |
And it plays out just as vividly here on Earth | 0:14:37 | 0:14:40 | |
as it does in the depths of space. | 0:14:40 | 0:14:43 | |
Well, this is the Perito Moreno Glacier | 0:15:01 | 0:15:04 | |
in Patagonia in southern Argentina. | 0:15:04 | 0:15:06 | |
And it's one of the hundreds of glaciers | 0:15:06 | 0:15:10 | |
that sweep down the continent from the southern Patagonian ice fields. | 0:15:10 | 0:15:14 | |
And, you know, if you carry on that way, south about 1,000 kilometres, | 0:15:16 | 0:15:21 | |
you get to the end of South America. | 0:15:21 | 0:15:24 | |
From then on, there's nothing to the Antarctic. | 0:15:24 | 0:15:27 | |
And it feels like that today. | 0:15:27 | 0:15:30 | |
The glacier is such a massive expanse of ice that, at first sight, | 0:15:41 | 0:15:45 | |
just like the cycles of the heavens, it appears fixed and unchanging. | 0:15:45 | 0:15:50 | |
Yet, seen close-up, it's continually on the move. | 0:15:59 | 0:16:03 | |
As it has been for tens of thousands of years. | 0:16:03 | 0:16:07 | |
WATER CRASHES | 0:16:12 | 0:16:14 | |
The whole face of the glacier is moving into the lake | 0:16:23 | 0:16:28 | |
something like that much every day. | 0:16:28 | 0:16:31 | |
That means that well over a quarter of a billion tonnes of ice | 0:16:31 | 0:16:36 | |
drop off the face of the glacier into the lake every year. | 0:16:36 | 0:16:40 | |
That's about a million tonnes a day. And you can hear it happening. | 0:16:40 | 0:16:43 | |
Just every now and again, you hear this tremendous cracking sound. | 0:16:43 | 0:16:48 | |
It really is like the place is alive. | 0:16:48 | 0:16:50 | |
< CRACKING | 0:16:55 | 0:16:58 | |
THUNDEROUS CRASH | 0:17:00 | 0:17:02 | |
You know, it's quite disturbing when these enormous chunks of ice | 0:17:03 | 0:17:07 | |
fall into the lake. | 0:17:07 | 0:17:08 | |
Although this thing seems stable and the movement seems glacially slow, | 0:17:08 | 0:17:12 | |
actually there can be really violent collapses. | 0:17:12 | 0:17:17 | |
It's an incredibly dynamic place to be. | 0:17:17 | 0:17:21 | |
The movement of the glacier | 0:17:32 | 0:17:34 | |
provides an insight into the nature of time. | 0:17:34 | 0:17:38 | |
It is simply the ordering of events into sequences. | 0:17:38 | 0:17:41 | |
One step after another. | 0:17:41 | 0:17:44 | |
As time passes, snow falls, ice forms, | 0:17:47 | 0:17:52 | |
the glacier gradually inches down the valley | 0:17:52 | 0:17:56 | |
and huge chunks of ice fall into the lake below. | 0:17:56 | 0:17:59 | |
But even this simple sequence contains a profound idea. | 0:18:01 | 0:18:07 | |
Events always happen in the same order. | 0:18:09 | 0:18:12 | |
They're never jumbled up and they never go backwards. | 0:18:12 | 0:18:16 | |
RUMBLING | 0:18:26 | 0:18:29 | |
Now that's something that you would never see in reverse. | 0:18:32 | 0:18:36 | |
But, interestingly, there's nothing in the laws of physics | 0:18:36 | 0:18:39 | |
that describe how all those | 0:18:39 | 0:18:41 | |
water molecules are moving around that prevent them | 0:18:41 | 0:18:45 | |
from all getting together on the surface of the lake, | 0:18:45 | 0:18:48 | |
jumping out of the water, sticking together into a block of ice | 0:18:48 | 0:18:52 | |
and then gluing themselves back on to the surface of the glacier again. | 0:18:52 | 0:18:56 | |
But, interestingly, | 0:18:56 | 0:18:58 | |
we do understand why the world doesn't run in reverse. | 0:18:58 | 0:19:03 | |
There is a reason. | 0:19:03 | 0:19:05 | |
We have a scientific explanation. | 0:19:05 | 0:19:08 | |
And it's called the arrow of time. | 0:19:08 | 0:19:11 | |
We never see waves travelling across lakes, | 0:19:21 | 0:19:24 | |
coming together and bouncing chunks of ice back onto glaciers. | 0:19:24 | 0:19:28 | |
We are compelled to travel into the future. | 0:19:31 | 0:19:35 | |
And that's because the arrow of time dictates that as each moment passes, | 0:19:35 | 0:19:40 | |
things change. | 0:19:40 | 0:19:42 | |
And once these changes have happened, they are never undone. | 0:19:42 | 0:19:46 | |
Permanent change is a fundamental part of what it means to be human. | 0:19:51 | 0:19:56 | |
We all age as the years pass by. | 0:19:56 | 0:20:00 | |
People are born, they live, they die. | 0:20:00 | 0:20:04 | |
I suppose it's part of the joy and tragedy of our lives. | 0:20:04 | 0:20:08 | |
But out there in the universe, | 0:20:08 | 0:20:11 | |
those grand and epic cycles appear eternal and unchanging. | 0:20:11 | 0:20:16 | |
But that's an illusion. | 0:20:16 | 0:20:18 | |
You see, in the life of the universe, just as in our lives, | 0:20:18 | 0:20:21 | |
everything is irreversibly changing. | 0:20:21 | 0:20:26 | |
By building change upon change, | 0:20:35 | 0:20:37 | |
the arrow of time drives the evolution of the entire universe. | 0:20:37 | 0:20:42 | |
And as we look out deep into the cosmos, | 0:20:43 | 0:20:47 | |
we can see that story unfold. | 0:20:47 | 0:20:49 | |
This is an image of a tiny piece of night sky | 0:20:52 | 0:20:56 | |
in the constellation of Leo. | 0:20:56 | 0:20:59 | |
It's actually where the mouth of the lion would be. | 0:20:59 | 0:21:02 | |
And, despite appearances, it is one of the most interesting images | 0:21:02 | 0:21:07 | |
taken in recent astronomical history. | 0:21:07 | 0:21:10 | |
The interesting thing is this little red blob here, | 0:21:10 | 0:21:14 | |
which looks very unremarkable. | 0:21:14 | 0:21:17 | |
But what that red blob is is the afterglow | 0:21:17 | 0:21:21 | |
of an enormous cosmic explosion. It's the death of a star. | 0:21:21 | 0:21:26 | |
That was about... | 0:21:26 | 0:21:28 | |
40 or even 50 times the mass of our sun. | 0:21:28 | 0:21:33 | |
Poetically named GRB 090423, it was once a Wolf-Rayet star. | 0:21:38 | 0:21:45 | |
Shrouded by rapidly swirling clouds of gas, | 0:21:50 | 0:21:54 | |
it burned 10,000 times more brightly than our sun. | 0:21:54 | 0:21:58 | |
But because it burned so brightly, it was extremely short-lived. | 0:22:00 | 0:22:05 | |
As it died, the giant star collapsed in on itself. | 0:22:08 | 0:22:11 | |
That caused massive jets of light and stellar material | 0:22:11 | 0:22:15 | |
to be ejected from its poles, | 0:22:15 | 0:22:18 | |
in an explosion that shone with the light of 10 million billion suns. | 0:22:18 | 0:22:23 | |
And it's the afterglow of this catastrophic explosion | 0:22:30 | 0:22:34 | |
that is just visible from our planet as a faint red dot. | 0:22:34 | 0:22:38 | |
But that's not what's so interesting about GRB 090423. | 0:22:44 | 0:22:49 | |
You see, when we look up into the sky, at distant stars and galaxies, | 0:22:49 | 0:22:54 | |
then we're looking back in time | 0:22:54 | 0:22:56 | |
because the light takes time to journey from them to us. | 0:22:56 | 0:23:00 | |
And the light from that red dot has been travelling to us | 0:23:00 | 0:23:05 | |
for almost the entire history of the universe. | 0:23:05 | 0:23:09 | |
You see, what we're looking at here is an event that happened | 0:23:09 | 0:23:14 | |
13 billion years ago. | 0:23:14 | 0:23:15 | |
That's only about 600 million years after the Big Bang. | 0:23:15 | 0:23:20 | |
After the universe began. | 0:23:20 | 0:23:22 | |
So this is something incredibly early in the universe's history. | 0:23:22 | 0:23:26 | |
In fact, this is the oldest single object that we've ever seen. | 0:23:26 | 0:23:33 | |
What we're looking at here is the explosive death | 0:23:33 | 0:23:37 | |
of one of the first stars in the universe. | 0:23:37 | 0:23:40 | |
As it evolves, the universe passes through distinct eras. | 0:23:53 | 0:23:58 | |
Vast ages, whose beginnings and endings | 0:24:00 | 0:24:03 | |
are marked by unique milestones. | 0:24:03 | 0:24:06 | |
The births and deaths of its wonders. | 0:24:08 | 0:24:12 | |
The moment the first stars were born is one of the most important changes | 0:24:18 | 0:24:22 | |
in the evolution of the cosmos. | 0:24:22 | 0:24:24 | |
It signals the end of the Primordial Era | 0:24:27 | 0:24:30 | |
and marks the beginning of the second great age of the universe. | 0:24:30 | 0:24:36 | |
The time in which we live. | 0:24:36 | 0:24:39 | |
The Stelliferous Era - | 0:24:39 | 0:24:42 | |
the age of the stars. | 0:24:42 | 0:24:44 | |
Starlight illuminates the night sky and starlight illuminates our days. | 0:24:50 | 0:24:56 | |
Our sun is just one of 200 billion stars in our galaxy. | 0:24:56 | 0:25:01 | |
Our galaxy is one of 100 billion in the observable universe. | 0:25:01 | 0:25:06 | |
And countless islands of countless stars. | 0:25:06 | 0:25:11 | |
Although the universe is over 13 billion years old, | 0:25:23 | 0:25:27 | |
we still love close to the stars of the Stelliferous Era. | 0:25:27 | 0:25:31 | |
It's an age of astonishing beauty and complexity in the universe. | 0:25:31 | 0:25:36 | |
The cosmos is absolutely awash with stars surrounded by | 0:25:40 | 0:25:45 | |
nebulae and systems of planets. | 0:25:45 | 0:25:48 | |
Countless billions of worlds that we've yet to explore. | 0:25:48 | 0:25:53 | |
But the cosmos isn't static and unchanging. | 0:26:00 | 0:26:04 | |
It won't always be this way. | 0:26:04 | 0:26:07 | |
Because, as the arrow of time plays out, | 0:26:07 | 0:26:11 | |
it produces a universe that is as dynamic as it's beautiful. | 0:26:11 | 0:26:16 | |
We've seen stars born and we've seen stars die. | 0:26:23 | 0:26:27 | |
And we know that tomorrow won't be the same as today | 0:26:27 | 0:26:31 | |
because the arrow of time says | 0:26:31 | 0:26:34 | |
the future will always be different from the past. | 0:26:34 | 0:26:38 | |
But what drives this evolution? | 0:26:40 | 0:26:42 | |
Why is there a difference between the past and the future? | 0:26:42 | 0:26:48 | |
Why is there an arrow of time at all? | 0:26:48 | 0:26:51 | |
We all have an intuitive understanding of the arrow of time. | 0:27:13 | 0:27:17 | |
It seems obvious to us that things change and the future | 0:27:21 | 0:27:25 | |
will be different to the past. | 0:27:25 | 0:27:27 | |
We know that because we see the effects | 0:27:32 | 0:27:35 | |
of the passing years all around us. | 0:27:35 | 0:27:38 | |
This is Kolmanskop, an abandoned diamond mining town | 0:27:48 | 0:27:51 | |
in southern Namibia. | 0:27:51 | 0:27:53 | |
This entire town was founded in 1908, | 0:28:02 | 0:28:05 | |
when a worker who was building the railway from the port of Luderitz | 0:28:05 | 0:28:10 | |
inland into the centre of Namibia found a single diamond | 0:28:10 | 0:28:14 | |
here in this desert. | 0:28:14 | 0:28:16 | |
For 40 years, this was a thriving community of up to 1,000 people. | 0:28:32 | 0:28:37 | |
A place where you could become a millionaire, | 0:28:37 | 0:28:40 | |
picking diamonds out of the sand. | 0:28:40 | 0:28:42 | |
While the money rolled in, they built grand houses | 0:28:46 | 0:28:49 | |
and lived a champagne lifestyle in the desert. | 0:28:49 | 0:28:52 | |
But when the diamonds dried up, the town was abandoned. | 0:28:55 | 0:28:59 | |
And for half a century | 0:28:59 | 0:29:01 | |
it's fallen into disrepair as it's slowly reclaimed by the sands. | 0:29:01 | 0:29:06 | |
The processes at play here at Kolmanskop | 0:29:22 | 0:29:25 | |
are happening everywhere in the universe. | 0:29:25 | 0:29:28 | |
Because it isn't simply permanent change | 0:29:28 | 0:29:31 | |
that's central to the arrow of time. | 0:29:31 | 0:29:34 | |
It's decay. | 0:29:34 | 0:29:35 | |
But the scientific explanation for why that is... | 0:29:37 | 0:29:41 | |
..didn't come from attempting to understand | 0:29:43 | 0:29:45 | |
the effects of time in the universe. | 0:29:45 | 0:29:47 | |
It came from trying to build a faster train. | 0:29:48 | 0:29:51 | |
Back in the 19th century, | 0:29:54 | 0:29:56 | |
engineers were concerned with the efficiency of steam engines. | 0:29:56 | 0:30:00 | |
How hot should the fire be? | 0:30:00 | 0:30:03 | |
What substance should you boil in the steam engine? | 0:30:03 | 0:30:06 | |
Should it be water or something else? | 0:30:06 | 0:30:09 | |
These were profound questions. | 0:30:09 | 0:30:11 | |
And out of those questions arose the science of thermodynamics. | 0:30:11 | 0:30:15 | |
It's when concepts like heat and temperature and energy | 0:30:15 | 0:30:18 | |
entered the scientific vocabulary for the first time. | 0:30:18 | 0:30:22 | |
Now, along with that deeper understanding | 0:30:22 | 0:30:26 | |
emerged what is probably the most important law of physics | 0:30:26 | 0:30:30 | |
for understanding the evolution of the universe | 0:30:30 | 0:30:33 | |
and the passage of time. | 0:30:33 | 0:30:35 | |
It's called the Second Law of Thermodynamics. | 0:30:35 | 0:30:39 | |
The reason the Second Law of Thermodynamics was so profound | 0:30:44 | 0:30:47 | |
was because, at its heart, it contained a radically new concept. | 0:30:47 | 0:30:53 | |
Something physicists call "entropy". | 0:30:53 | 0:30:57 | |
Entropy explains why, left to the mercy of the elements, | 0:30:59 | 0:31:03 | |
mortar crumbles, glass shatters and buildings collapse. | 0:31:03 | 0:31:08 | |
And a good way to understand how is to think of objects | 0:31:12 | 0:31:15 | |
not as single things, | 0:31:15 | 0:31:16 | |
but as being made up of many constituent parts. | 0:31:16 | 0:31:20 | |
Like the individual grains that make up this pile of sand. | 0:31:20 | 0:31:24 | |
Now, entropy is a measure of how many ways I can rearrange those | 0:31:27 | 0:31:31 | |
grains and still keep the sand pile the same. | 0:31:31 | 0:31:34 | |
And there are trillions and trillions and trillions | 0:31:34 | 0:31:38 | |
of ways of doing that. | 0:31:38 | 0:31:39 | |
I mean, pretty much anything I do to this sand pile, | 0:31:39 | 0:31:42 | |
if I mess the sand around and move it around, | 0:31:42 | 0:31:45 | |
then it doesn't change the shape or the structure at all. | 0:31:45 | 0:31:48 | |
So, in the language of entropy, | 0:31:48 | 0:31:50 | |
this sand pile has high entropy because there are many, many ways | 0:31:50 | 0:31:55 | |
that I can rearrange its constituents and not change it. | 0:31:55 | 0:31:59 | |
Now let me create some order in the universe. | 0:31:59 | 0:32:04 | |
Now, there are approximately as many sand grains in this sand castle | 0:32:11 | 0:32:15 | |
as there are in the sand pile. | 0:32:15 | 0:32:18 | |
But now, virtually anything I do to it will mess it up, | 0:32:18 | 0:32:22 | |
will remove the beautiful order from this structure. | 0:32:22 | 0:32:26 | |
And because of that, the sand castle has a low entropy. | 0:32:26 | 0:32:30 | |
It's a much more ordered state. | 0:32:30 | 0:32:32 | |
So, many ways of rearranging the sand grains | 0:32:32 | 0:32:35 | |
without changing the structure, high entropy. | 0:32:35 | 0:32:39 | |
Very few ways of rearranging the sand grains | 0:32:39 | 0:32:42 | |
without changing the structure, without disordering it, low entropy. | 0:32:42 | 0:32:48 | |
Imagine I was to leave this castle in the desert all day. | 0:32:56 | 0:33:00 | |
Then it's obvious what's going to happen. | 0:33:00 | 0:33:02 | |
The desert winds are going to blow the sand around | 0:33:02 | 0:33:06 | |
and this castle is going to disintegrate. | 0:33:06 | 0:33:10 | |
Is going to become less ordered. It's going to fall to bits. | 0:33:10 | 0:33:13 | |
But think about what's happening on the fundamental level. | 0:33:16 | 0:33:20 | |
I mean, the wind is taking the sand off the castle | 0:33:20 | 0:33:24 | |
and blowing it over there somewhere and making a sand pile. | 0:33:24 | 0:33:28 | |
There's nothing fundamental in the laws of physics | 0:33:28 | 0:33:31 | |
that says that the wind couldn't pick up some sand from over here, | 0:33:31 | 0:33:36 | |
deposit it here | 0:33:36 | 0:33:38 | |
and deposit it in precisely the shape of a sand castle. | 0:33:38 | 0:33:42 | |
In principle, the wind could spontaneously build a sand castle | 0:33:42 | 0:33:47 | |
out of a pile of sand. | 0:33:47 | 0:33:48 | |
There's no reason why that couldn't happen. | 0:33:59 | 0:34:01 | |
It's just extremely, extremely unlikely because there | 0:34:01 | 0:34:05 | |
are very few ways of organising this sand so that it looks like a castle. | 0:34:05 | 0:34:10 | |
It's overwhelmingly more likely | 0:34:17 | 0:34:19 | |
that when the wind blows the sand around | 0:34:19 | 0:34:21 | |
it will take the low entropy structure of the castle | 0:34:21 | 0:34:25 | |
and turn it into a high entropy structure, the sand pile. | 0:34:25 | 0:34:29 | |
So, entropy always increases. Why is that? | 0:34:37 | 0:34:41 | |
Because it's overwhelmingly more likely that it will. | 0:34:41 | 0:34:45 | |
It seems incredible that a law that says that sand castles | 0:34:55 | 0:34:58 | |
don't spontaneously form on the wind | 0:34:58 | 0:35:02 | |
could solve one of the deepest mysteries in physics. | 0:35:02 | 0:35:05 | |
But by saying entropy always increases, | 0:35:08 | 0:35:11 | |
the Second Law of Thermodynamics is able to explain | 0:35:11 | 0:35:15 | |
why time only runs in one direction. | 0:35:15 | 0:35:18 | |
The Second Law of Thermodynamics, for me, demonstrates everything | 0:35:34 | 0:35:38 | |
that's powerful and beautiful and profound about physics. | 0:35:38 | 0:35:42 | |
You see, here's a law that entered science | 0:35:42 | 0:35:45 | |
as a way of talking about how heat moves around | 0:35:45 | 0:35:47 | |
and the efficiency of steam engines. | 0:35:47 | 0:35:49 | |
But it ended up being able to explain one of the great mysteries | 0:35:49 | 0:35:54 | |
in the history of science. | 0:35:54 | 0:35:57 | |
Why is there a difference between the past and the future? | 0:35:57 | 0:36:00 | |
You see, the second law says | 0:36:00 | 0:36:03 | |
that everything tends from order to disorder. | 0:36:03 | 0:36:07 | |
That means that there is a difference | 0:36:07 | 0:36:10 | |
between the past and future. | 0:36:10 | 0:36:12 | |
In the past, the universe was more ordered. | 0:36:12 | 0:36:14 | |
In the future, the universe will be less ordered. | 0:36:14 | 0:36:18 | |
And that means there's a direction to the passage of time. | 0:36:18 | 0:36:21 | |
So the Second Law of Thermodynamics has introduced the concept | 0:36:21 | 0:36:27 | |
of an arrow of time into science. | 0:36:27 | 0:36:30 | |
The arrow of time has been playing out | 0:36:38 | 0:36:40 | |
in Kolmanskop since the mining facility was abandoned in 1954. | 0:36:40 | 0:36:45 | |
But in the universe, | 0:36:48 | 0:36:49 | |
it's been playing out for almost 14 billion years. | 0:36:49 | 0:36:53 | |
And it will have profound consequences. | 0:36:53 | 0:36:56 | |
Because it means stars cannot shine forever. | 0:37:04 | 0:37:07 | |
Including the star at the centre of our solar system. | 0:37:07 | 0:37:12 | |
At the end of its life, the sun won't simply fade away to nothing. | 0:37:14 | 0:37:19 | |
As it begins to run out of fuel, its core will collapse | 0:37:22 | 0:37:27 | |
and the extra heat this generates | 0:37:27 | 0:37:29 | |
will cause its outer layers to expand. | 0:37:29 | 0:37:31 | |
In around a billion years' time, | 0:37:39 | 0:37:41 | |
this will have a catastrophic effect on our fragile world. | 0:37:41 | 0:37:45 | |
Gradually, the Earth will become hotter and hotter. | 0:37:52 | 0:37:55 | |
So there will be one last perfect day on Earth. | 0:37:55 | 0:37:59 | |
But eventually the existence of all life on this planet | 0:37:59 | 0:38:03 | |
will become impossible. | 0:38:03 | 0:38:05 | |
TICKING | 0:38:05 | 0:38:09 | |
Long after a life has disappeared, the sun will have grown so much | 0:38:09 | 0:38:14 | |
it will fill the entire horizon. | 0:38:14 | 0:38:16 | |
It will become a red giant. | 0:38:23 | 0:38:24 | |
The last phase of its life. | 0:38:24 | 0:38:27 | |
Our planet might not survive to this point. | 0:38:37 | 0:38:39 | |
But, if it does, little more than a scorched and barren rock will remain | 0:38:39 | 0:38:45 | |
to witness the final death throes of our star. | 0:38:45 | 0:38:49 | |
In six billion years, our sun will explode. | 0:39:00 | 0:39:04 | |
Throwing vast amounts of gas and dust out into space, | 0:39:04 | 0:39:08 | |
to form a gigantic nebula. | 0:39:08 | 0:39:10 | |
And at its heart will beat a faintly glowing ember. | 0:39:18 | 0:39:22 | |
All that remains of our once magnificent sun. | 0:39:22 | 0:39:26 | |
It will be smaller than the size of the Earth. | 0:39:26 | 0:39:28 | |
Less than a millionth of its current volume | 0:39:28 | 0:39:31 | |
and a fraction of its brightness. | 0:39:31 | 0:39:34 | |
Our sun will have become a white dwarf. | 0:39:34 | 0:39:37 | |
With no fuel left to burn, | 0:39:46 | 0:39:49 | |
a white dwarf's faint glow comes from the last residual heat | 0:39:49 | 0:39:53 | |
from its extinguished furnace. | 0:39:53 | 0:39:55 | |
The sun is now dead. | 0:39:58 | 0:40:00 | |
Its remains slowly cooling in the freezing temperatures of deep space. | 0:40:00 | 0:40:05 | |
Looking at it from where the Earth is now, | 0:40:10 | 0:40:12 | |
it would only generate the same amount of light | 0:40:12 | 0:40:15 | |
as the full moon on a clear night. | 0:40:15 | 0:40:17 | |
The fate of the sun IS the same as for all stars. | 0:40:23 | 0:40:27 | |
One day, they must all eventually die | 0:40:27 | 0:40:30 | |
and the cosmos will be plunged into eternal night. | 0:40:30 | 0:40:34 | |
And this is the most profound consequence of the arrow of time. | 0:40:34 | 0:40:39 | |
Because this structured universe that we inhabit, | 0:40:39 | 0:40:42 | |
and all its wonders - the stars, the planets and the galaxies - | 0:40:42 | 0:40:46 | |
cannot last forever. | 0:40:46 | 0:40:49 | |
The cosmos will eventually fade and die. | 0:40:49 | 0:40:54 | |
First will come the end of the Stelliferous Era. | 0:40:57 | 0:41:00 | |
The end of the age of starlight. | 0:41:00 | 0:41:03 | |
The largest stars are the first to disappear, | 0:41:08 | 0:41:11 | |
violently collapsing into black holes. | 0:41:11 | 0:41:13 | |
Just a few million years after their formation. | 0:41:13 | 0:41:16 | |
But long after they're gone, just one type of star will remain. | 0:41:19 | 0:41:23 | |
This is a picture of the nearest star to our solar system, | 0:41:27 | 0:41:31 | |
Proxima Centauri. | 0:41:31 | 0:41:32 | |
It's only 4.2 light years away. But the reason it doesn't stand out | 0:41:32 | 0:41:36 | |
against the much more distant stars in this photograph | 0:41:36 | 0:41:39 | |
is that Proxima Centauri is incredibly tiny. | 0:41:39 | 0:41:43 | |
It's a kind of star known as a red dwarf star. | 0:41:43 | 0:41:46 | |
It's only about 11-12% the mass of our sun. | 0:41:46 | 0:41:50 | |
But to our eyes it would appear to shine 18,000 times less brightly. | 0:41:50 | 0:41:56 | |
But red dwarves do have one advantage over their much more | 0:41:58 | 0:42:01 | |
luminous and magnificent stellar brethren. | 0:42:01 | 0:42:06 | |
And that's because they're so small, | 0:42:06 | 0:42:09 | |
they burn their nuclear fuel incredibly slowly, | 0:42:09 | 0:42:13 | |
so they have lifespans of trillions of years. | 0:42:13 | 0:42:16 | |
And that means that stars like Proxima Centauri | 0:42:16 | 0:42:20 | |
will be the last living stars in the universe. | 0:42:20 | 0:42:24 | |
If we survive into the far future of the universe, | 0:42:29 | 0:42:33 | |
then it's possible to imagine our distant descendants building | 0:42:33 | 0:42:38 | |
their civilisation around red dwarves | 0:42:38 | 0:42:41 | |
to capture the energy from those last fading embers of stars, | 0:42:41 | 0:42:46 | |
just as our ancestors crowded around campfires | 0:42:46 | 0:42:51 | |
for warmth on cold winter's nights. | 0:42:51 | 0:42:54 | |
The reason why Proxima Centauri | 0:43:13 | 0:43:15 | |
burns so slowly is because its small size and low gravity | 0:43:15 | 0:43:19 | |
mean its core is under much lower pressure than larger stars. | 0:43:19 | 0:43:23 | |
This also means that its interior is constantly churning, | 0:43:25 | 0:43:29 | |
whipping up the surface into a fiery turmoil. | 0:43:29 | 0:43:32 | |
Explosive solar flares occur almost continually, | 0:43:35 | 0:43:39 | |
even though it burns so dimly. | 0:43:39 | 0:43:41 | |
But Proxima Centauri will eventually die. | 0:43:43 | 0:43:48 | |
And like our sun, it too will become a white dwarf. | 0:43:48 | 0:43:52 | |
As the age of starlight ends, | 0:43:53 | 0:43:55 | |
all but the dimmest flicker of light in the universe will go out. | 0:43:55 | 0:44:00 | |
The faint glow of white dwarves will provide the only illumination | 0:44:00 | 0:44:05 | |
in a dark and empty void, littered with dead stars and black holes. | 0:44:05 | 0:44:12 | |
By this point, the universe will be 100 trillion years old. | 0:44:14 | 0:44:19 | |
And yet, even now, | 0:44:22 | 0:44:24 | |
the vast majority of its lifespan still lies ahead of it. | 0:44:24 | 0:44:29 | |
There are few places on Earth where you can get an inkling | 0:44:46 | 0:44:49 | |
of what the far future has in store. | 0:44:49 | 0:44:53 | |
This is Namibia's Skeleton Coast, | 0:45:06 | 0:45:08 | |
where the cold water to the South Atlantic | 0:45:08 | 0:45:11 | |
meet the Namib Desert. | 0:45:11 | 0:45:13 | |
And it is one of the most inhospitable places on Earth. | 0:45:13 | 0:45:16 | |
Back in the 17th century, | 0:45:16 | 0:45:18 | |
Portuguese sailors used to call this place the "gates to hell" | 0:45:18 | 0:45:22 | |
because this dense fog | 0:45:22 | 0:45:23 | |
that you see pretty much every morning along this coast, | 0:45:23 | 0:45:27 | |
coupled with the constantly shifting shape of the sandbanks, | 0:45:27 | 0:45:31 | |
meant that over the years, | 0:45:31 | 0:45:34 | |
literally thousands of ships were wrecked along this coastline. | 0:45:34 | 0:45:37 | |
And even if you made it to shore, that wasn't the end of your problems | 0:45:43 | 0:45:46 | |
because the currents are so strong here | 0:45:46 | 0:45:49 | |
that there is no way of rowing back out to sea. | 0:45:49 | 0:45:52 | |
If you look that way, | 0:45:52 | 0:45:53 | |
there's just hundreds of miles of inhospitable desert. | 0:45:53 | 0:45:57 | |
So, it genuinely was a place of no return. | 0:45:59 | 0:46:04 | |
If you were shipwrecked here, this WAS the end of your universe. | 0:46:04 | 0:46:09 | |
This is the Eduard Bohlen. | 0:46:20 | 0:46:22 | |
She was once an ocean-going steamer, | 0:46:22 | 0:46:25 | |
ferrying passengers and cargo between here and Europe. | 0:46:25 | 0:46:28 | |
On 5th September, 1909, she ran aground in thick fog. | 0:46:32 | 0:46:37 | |
Yet, like all the vessels wrecked along this shoreline, | 0:46:43 | 0:46:47 | |
the time it takes her to decay to nothing | 0:46:47 | 0:46:50 | |
will be far longer than her time at sea. | 0:46:50 | 0:46:52 | |
In the far future of the cosmos, | 0:46:57 | 0:47:00 | |
a similar destiny awaits the remaining white dwarves. | 0:47:00 | 0:47:04 | |
A black dwarf will be the final fate of those last stars. | 0:47:10 | 0:47:14 | |
White dwarves that have become so cold | 0:47:14 | 0:47:17 | |
that they barely emit any more heat or light. | 0:47:17 | 0:47:20 | |
Black dwarves are dark, dense decaying balls of degenerate matter. | 0:47:25 | 0:47:30 | |
Little more than the ashes of stars. | 0:47:30 | 0:47:33 | |
Their constituent atoms are so severely crushed | 0:47:34 | 0:47:39 | |
that black dwarves are a million times denser than our sun. | 0:47:39 | 0:47:44 | |
Stars take so long to reach this point, | 0:47:44 | 0:47:47 | |
that after nearly 14 billion years | 0:47:47 | 0:47:49 | |
we believe there are currently no black dwarves in the universe. | 0:47:49 | 0:47:54 | |
But despite never seeing one, | 0:47:54 | 0:47:57 | |
we can still predict how they will end their days. | 0:47:57 | 0:48:00 | |
Just as the iron than makes up this ship | 0:48:00 | 0:48:03 | |
will eventually rust and be carried away by the desert winds, | 0:48:03 | 0:48:08 | |
so we think that the matter inside black dwarves, | 0:48:08 | 0:48:12 | |
the last matter in the universe, | 0:48:12 | 0:48:14 | |
will eventually evaporate away and be carried off | 0:48:14 | 0:48:19 | |
into the void as radiation, | 0:48:19 | 0:48:21 | |
leaving absolutely nothing behind. | 0:48:21 | 0:48:25 | |
With the black dwarves gone, | 0:48:34 | 0:48:36 | |
there won't be a single atom of matter left. | 0:48:36 | 0:48:39 | |
All that will remain of our once rich cosmos | 0:48:42 | 0:48:45 | |
will be particles of light and black holes. | 0:48:45 | 0:48:49 | |
After an unimaginable length of time, | 0:48:55 | 0:48:59 | |
even the black holes will have evaporated | 0:48:59 | 0:49:02 | |
and the universe will be nothing but a sea of photons, | 0:49:02 | 0:49:06 | |
gradually tending towards the same temperature, | 0:49:06 | 0:49:10 | |
as the expansion of the universe cools them towards absolute zero. | 0:49:10 | 0:49:14 | |
And when I say "unimaginable period of time," I really mean it. | 0:49:23 | 0:49:26 | |
It's 10,000 trillion trillion | 0:49:26 | 0:49:28 | |
trillion trillion trillion trillion trillion trillion years. | 0:49:28 | 0:49:33 | |
How big's that number? | 0:49:33 | 0:49:35 | |
If I were to start counting with a single atom representing one year | 0:49:35 | 0:49:41 | |
then there wouldn't be enough atoms in the entire universe | 0:49:41 | 0:49:45 | |
to get anywhere near that number. | 0:49:45 | 0:49:48 | |
Once the very last remnants | 0:49:54 | 0:49:56 | |
of the very last stars have finally decayed away to nothing, | 0:49:56 | 0:50:00 | |
and everything reaches the same temperature, | 0:50:00 | 0:50:04 | |
the story of the universe finally comes to an end. | 0:50:04 | 0:50:08 | |
For the first time in its life, | 0:50:12 | 0:50:14 | |
the universe will be permanent and unchanging. | 0:50:14 | 0:50:18 | |
Entropy finally stops increasing | 0:50:18 | 0:50:20 | |
because the cosmos cannot get any more disordered. | 0:50:20 | 0:50:25 | |
Nothing happens and it keeps not happening. | 0:50:25 | 0:50:29 | |
Forever. | 0:50:29 | 0:50:31 | |
It's what's known as the heat death of the universe. | 0:50:36 | 0:50:38 | |
An era when the cosmos will remain vast and cold and desolate | 0:50:38 | 0:50:44 | |
for the rest of time. | 0:50:44 | 0:50:46 | |
But that's because there is no difference between the past, | 0:50:46 | 0:50:49 | |
the present and the future. | 0:50:49 | 0:50:51 | |
There's no way of measuring the passage of time | 0:50:51 | 0:50:55 | |
because nothing in the cosmos changes. | 0:50:55 | 0:50:58 | |
The arrow of time has simply ceased to exist. | 0:50:58 | 0:51:02 | |
It's an inescapable fact of the universe, | 0:51:13 | 0:51:16 | |
written into the fundamental laws of physics. | 0:51:16 | 0:51:19 | |
The entire cosmos will die. | 0:51:19 | 0:51:22 | |
Every single one of the 200 billion stars in our galaxy will go out. | 0:51:27 | 0:51:33 | |
And just as the death of the sun means the end of life on our planet, | 0:51:36 | 0:51:41 | |
so the death of every star | 0:51:41 | 0:51:43 | |
will extinguish any possibility of life in the universe. | 0:51:43 | 0:51:47 | |
The fact that the sun will die and it will incinerate the Earth | 0:51:51 | 0:51:56 | |
and obliterate all life on our planet in the process, | 0:51:56 | 0:52:00 | |
might sound a bit depressing to you. | 0:52:00 | 0:52:02 | |
You might legitimately ask, | 0:52:02 | 0:52:04 | |
"Well, surely you could build a universe in a different way? | 0:52:04 | 0:52:08 | |
"Surely you could build it | 0:52:08 | 0:52:09 | |
"so it didn't have to descend from order into chaos?" | 0:52:09 | 0:52:13 | |
Well, the answer is no, | 0:52:13 | 0:52:14 | |
you couldn't, if you wanted life to exist in it. | 0:52:14 | 0:52:18 | |
The arrow of time, | 0:52:24 | 0:52:25 | |
the sequence of changes that slowly leads the universe to its death, | 0:52:25 | 0:52:30 | |
is the very same thing that creates the conditions | 0:52:30 | 0:52:33 | |
for life in the first place. | 0:52:33 | 0:52:35 | |
Because it takes time for matter to form | 0:52:40 | 0:52:42 | |
and it takes time for gravity to pull it together | 0:52:42 | 0:52:46 | |
into stars and planets. | 0:52:46 | 0:52:48 | |
The arrow of time creates a bright window | 0:52:53 | 0:52:55 | |
in the universe's adolescence. | 0:52:55 | 0:52:58 | |
During which, life is possible. | 0:52:58 | 0:53:00 | |
But it's a window that doesn't stay open for long. | 0:53:07 | 0:53:11 | |
As a fraction of the lifespan of the universe, | 0:53:14 | 0:53:17 | |
as measured from its beginning to the evaporation | 0:53:17 | 0:53:21 | |
of the last black hole, | 0:53:21 | 0:53:23 | |
life, as we know it, is only possible for one thousandth | 0:53:23 | 0:53:28 | |
of a billion billion billionth billion billion billionth | 0:53:28 | 0:53:32 | |
billion billion billionth of a per cent. | 0:53:32 | 0:53:35 | |
And that's why, for me, | 0:53:37 | 0:53:39 | |
the most astonishing wonder of the universe isn't a star | 0:53:39 | 0:53:44 | |
or a planet or a galaxy. | 0:53:44 | 0:53:47 | |
It isn't a thing at all. | 0:53:47 | 0:53:49 | |
It's an instant in time. | 0:53:49 | 0:53:52 | |
And that time is now. | 0:53:52 | 0:53:55 | |
Humans have walked the Earth for just the smallest fraction | 0:54:03 | 0:54:07 | |
of that briefest of moments in deep time. | 0:54:07 | 0:54:11 | |
But in our 200,000 years on this planet, | 0:54:14 | 0:54:16 | |
we've made remarkable progress. | 0:54:16 | 0:54:19 | |
It was only 2,500 years ago that we believed that the sun was a god | 0:54:22 | 0:54:27 | |
and measured its orbit with stone towers, | 0:54:27 | 0:54:30 | |
built on the top of a hill. | 0:54:30 | 0:54:32 | |
Today, the language of curiosity is not sun gods, but science. | 0:54:32 | 0:54:39 | |
And we have observatories that are almost infinitely more sophisticated | 0:54:39 | 0:54:44 | |
than the 13 towers, that can gaze out deep into the universe. | 0:54:44 | 0:54:49 | |
And, perhaps even more remarkably, | 0:54:52 | 0:54:55 | |
through theoretical physics and mathematics, | 0:54:55 | 0:54:57 | |
we can calculate what the universe will look like | 0:54:57 | 0:55:01 | |
in the distant future. | 0:55:01 | 0:55:03 | |
And we can even make concrete predictions about its end. | 0:55:03 | 0:55:08 | |
And I believe it's only by continuing | 0:55:15 | 0:55:17 | |
our exploration of the cosmos | 0:55:17 | 0:55:19 | |
and the laws of nature that govern it, | 0:55:19 | 0:55:22 | |
that we can truly understand ourselves | 0:55:22 | 0:55:26 | |
and our place in this universe of wonders. | 0:55:26 | 0:55:29 | |
And that's what we've done in our brief moment on Planet Earth. | 0:55:33 | 0:55:38 | |
In 1977, a space probe called Voyager 1 | 0:55:41 | 0:55:45 | |
was launched on a grand tour of the solar system. | 0:55:45 | 0:55:49 | |
And it visited the great gas giant planets - | 0:55:49 | 0:55:52 | |
Jupiter and Saturn - and made some wonderful discoveries | 0:55:52 | 0:55:56 | |
before heading off towards interstellar space. | 0:55:56 | 0:56:00 | |
13 years later, after its mission was almost over, | 0:56:02 | 0:56:06 | |
it turned around and took one last picture of its home solar system. | 0:56:06 | 0:56:12 | |
This is that picture. | 0:56:12 | 0:56:14 | |
And the beautiful thing about this picture | 0:56:17 | 0:56:20 | |
is this single pixel of light | 0:56:20 | 0:56:24 | |
suspended against the blackness of space. | 0:56:24 | 0:56:26 | |
Because that pixel, that point, is Planet Earth. | 0:56:26 | 0:56:31 | |
The most distant picture of our planet ever taken. | 0:56:31 | 0:56:34 | |
6 billion kilometres away. | 0:56:34 | 0:56:37 | |
And whilst I suppose it has very limited scientific value, | 0:56:47 | 0:56:51 | |
for me, this tiny point of light | 0:56:51 | 0:56:54 | |
is the most powerful and profound demonstration | 0:56:54 | 0:56:58 | |
of perhaps the most human of qualities. | 0:56:58 | 0:57:01 | |
Our unique ability to reflect on the universe's existence | 0:57:01 | 0:57:06 | |
and our place within it. | 0:57:06 | 0:57:08 | |
Just as we, and all life on Earth, stand on this tiny speck | 0:57:13 | 0:57:18 | |
adrift in infinite space, so life in the universe will only exist | 0:57:18 | 0:57:25 | |
for a fleeting bright instance in time | 0:57:25 | 0:57:29 | |
because life, just like the stars and the planets and the galaxies, | 0:57:29 | 0:57:35 | |
is just a temporary structure on the long road from order to disorder. | 0:57:35 | 0:57:40 | |
But that doesn't make us insignificant | 0:57:49 | 0:57:52 | |
because we are the cosmos made conscious. | 0:57:52 | 0:57:54 | |
Life is the means by which the universe understands itself. | 0:57:54 | 0:57:59 | |
And, for me, our true significance lies in our ability | 0:58:02 | 0:58:06 | |
and our desire to understand and explore this beautiful universe. | 0:58:06 | 0:58:12 | |
Subtitles by Red Bee Media Ltd | 0:58:55 | 0:58:58 |