Browse content similar to The Pale Blue Dot. Check below for episodes and series from the same categories and more!
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The natural world is beautiful, but complex. | 0:00:10 | 0:00:14 | |
The skies dance with colour. | 0:00:18 | 0:00:20 | |
Yaaaay-ya! | 0:00:20 | 0:00:22 | |
Shapes of great geometrical beauty form and disappear. | 0:00:26 | 0:00:31 | |
And the planet itself is constantly transformed. | 0:00:36 | 0:00:40 | |
But this seemingly infinite complexity... | 0:00:44 | 0:00:46 | |
..is just a shadow of something deeper. | 0:00:49 | 0:00:51 | |
The underlying laws of nature. | 0:00:53 | 0:00:55 | |
The world we live in is beautiful to look at, | 0:00:57 | 0:01:00 | |
but it's even more beautiful to understand. | 0:01:00 | 0:01:03 | |
Light is our window on the universe. | 0:01:21 | 0:01:23 | |
By understanding how light is emitted by the sun, | 0:01:25 | 0:01:29 | |
and how it interacts with the oceans, atmosphere, | 0:01:29 | 0:01:32 | |
and life on our planet, | 0:01:32 | 0:01:35 | |
we can explore worlds beyond our solar system... | 0:01:35 | 0:01:38 | |
..and even search for the telltale signatures of life | 0:01:41 | 0:01:44 | |
amongst the stars. | 0:01:44 | 0:01:46 | |
Night on our planet seems eerie, | 0:02:13 | 0:02:16 | |
other, | 0:02:16 | 0:02:18 | |
as if all the colour has drained away. | 0:02:18 | 0:02:20 | |
But in a few places on Earth, | 0:02:23 | 0:02:25 | |
on just a handful of nights in the year, | 0:02:25 | 0:02:28 | |
colour bursts through. | 0:02:28 | 0:02:30 | |
10,000 years ago, at the end of the last ice age, | 0:02:34 | 0:02:37 | |
the ice sheets melted | 0:02:37 | 0:02:39 | |
and this part of Iceland rose up and drove the coastline back. | 0:02:39 | 0:02:44 | |
That left the Skoga River to tumble over the old sea cliffs | 0:02:44 | 0:02:49 | |
to form that - | 0:02:49 | 0:02:51 | |
Skogafoss, one of Iceland's great waterfalls. | 0:02:51 | 0:02:54 | |
When the sun, moon and Earth align, | 0:03:01 | 0:03:04 | |
moonlight interacts with the spray at the foot of the falls... | 0:03:04 | 0:03:08 | |
..to form a moonbow. | 0:03:11 | 0:03:13 | |
Light leaves the sun, | 0:03:18 | 0:03:20 | |
travels 93 million miles across space, | 0:03:20 | 0:03:24 | |
and reflects off the surface of the moon. | 0:03:24 | 0:03:27 | |
And it enters the Earth's atmosphere, | 0:03:28 | 0:03:30 | |
bounces in and out of water droplets in the waterfall, | 0:03:30 | 0:03:35 | |
and enters my eye. | 0:03:35 | 0:03:36 | |
That sends a signal to my brain, | 0:03:36 | 0:03:39 | |
and I reconstruct the signal as something beautiful. | 0:03:39 | 0:03:42 | |
But the moonbow isn't just beautiful. | 0:03:51 | 0:03:54 | |
It's physics. | 0:03:56 | 0:03:58 | |
Understanding why something's the colour it is tells you something. | 0:04:08 | 0:04:12 | |
It tells you about its structure, | 0:04:12 | 0:04:14 | |
about the processes going on inside, about its history, even. | 0:04:14 | 0:04:18 | |
And because light travels freely across the universe, | 0:04:18 | 0:04:21 | |
we can explore distant worlds using light alone. | 0:04:21 | 0:04:25 | |
We can tell their stories, too. | 0:04:26 | 0:04:28 | |
The reflected light from the moon has its origin in our star, the sun. | 0:04:34 | 0:04:39 | |
Stars illuminate the universe. | 0:04:40 | 0:04:43 | |
They are the source of the light that bathes the planets. | 0:04:43 | 0:04:47 | |
But the processes by which light is emitted by the stars | 0:04:49 | 0:04:53 | |
can be explored here on Earth. | 0:04:53 | 0:04:54 | |
On the 31st August, 2014, | 0:05:08 | 0:05:12 | |
a vast chasm opened up in central Iceland. | 0:05:12 | 0:05:15 | |
At its peak, the Bardabunga volcano | 0:05:26 | 0:05:29 | |
spewed out 350 cubic metres of molten rock every second... | 0:05:29 | 0:05:34 | |
..producing light so bright... | 0:05:40 | 0:05:42 | |
..it could be seen from space. | 0:05:48 | 0:05:50 | |
And just like the sun, lava glows because it's hot. | 0:06:00 | 0:06:05 | |
Just look at that. | 0:06:09 | 0:06:11 | |
It's many months, since the eruption but it's steaming away back there. | 0:06:11 | 0:06:15 | |
We're actually fortunate that it erupted here. | 0:06:15 | 0:06:18 | |
The helicopter pilot told me that if it'd erupted on the glacier, | 0:06:18 | 0:06:22 | |
then we would have been plunged into a perpetual nuclear winter | 0:06:22 | 0:06:26 | |
and civilisation would have been destroyed. | 0:06:26 | 0:06:29 | |
That's not actually quite right, | 0:06:29 | 0:06:30 | |
but it would have been significantly worse. | 0:06:30 | 0:06:33 | |
The amount of ash that went up into the atmosphere | 0:06:33 | 0:06:35 | |
would have been really considerable. | 0:06:35 | 0:06:38 | |
You get a sense of the power and violence of the Earth. | 0:06:38 | 0:06:42 | |
Cos we're blissfully unaware of it, usually, | 0:06:42 | 0:06:45 | |
but when it breaks through the surface, you see what it can do. | 0:06:45 | 0:06:49 | |
Today the lava has cooled into matt-black rock, | 0:07:02 | 0:07:07 | |
but it's still giving off light. | 0:07:07 | 0:07:09 | |
The thing is, everything's hot. Everything has a temperature. | 0:07:13 | 0:07:17 | |
But if it's cold, it just emits light that we can't see. | 0:07:17 | 0:07:21 | |
This camera can see it, though. | 0:07:21 | 0:07:23 | |
It's called infrared light. | 0:07:23 | 0:07:26 | |
You see there that this lava | 0:07:26 | 0:07:28 | |
is glowing brighter than the background. | 0:07:28 | 0:07:31 | |
Means it's hotter. | 0:07:31 | 0:07:33 | |
So, although we can't see it, | 0:07:37 | 0:07:40 | |
everything shines. | 0:07:40 | 0:07:42 | |
Light fills the universe. | 0:07:47 | 0:07:50 | |
Radio waves are light, X-rays are light. | 0:07:50 | 0:07:53 | |
Visible light is simply the part of the spectrum we can see. | 0:07:53 | 0:07:57 | |
Matter, like lava, or you and me, | 0:08:01 | 0:08:04 | |
is made up of electrically charged particles. | 0:08:04 | 0:08:08 | |
Here's one moving along - | 0:08:08 | 0:08:10 | |
say it's an electron. | 0:08:10 | 0:08:12 | |
Temperature is a measure of how fast those particles are moving around, | 0:08:13 | 0:08:18 | |
how fast they're jiggling. | 0:08:18 | 0:08:19 | |
So, in something hot, | 0:08:19 | 0:08:21 | |
these particles are always bouncing around | 0:08:21 | 0:08:24 | |
and changing direction. | 0:08:24 | 0:08:25 | |
Now, here's a fundamental law of the universe. | 0:08:25 | 0:08:29 | |
When a charged particle changes direction, | 0:08:29 | 0:08:32 | |
it emits a light particle | 0:08:32 | 0:08:35 | |
called a photon. | 0:08:35 | 0:08:37 | |
Light can be thought of as a stream of photons - | 0:08:41 | 0:08:44 | |
particles whose energy corresponds to their colour. | 0:08:44 | 0:08:47 | |
Cooler things, like solid black lava, | 0:08:54 | 0:08:57 | |
emit lower energy photons - infrared light, which our eyes can't detect. | 0:08:57 | 0:09:02 | |
As things get hotter, they can radiate higher-energy photons. | 0:09:08 | 0:09:12 | |
At 1,000 degrees Celsius, molten lava shines with mainly red light, | 0:09:12 | 0:09:17 | |
which our eyes can detect. | 0:09:17 | 0:09:20 | |
The surface of the sun is 5,500 degrees Celsius, | 0:09:21 | 0:09:26 | |
so it can also produce higher-energy green and blue photons | 0:09:26 | 0:09:30 | |
alongside the red. | 0:09:30 | 0:09:31 | |
The white light of the sun | 0:09:34 | 0:09:36 | |
is made up of all the colours of the rainbow. | 0:09:36 | 0:09:39 | |
And when it reaches the Earth, | 0:09:41 | 0:09:43 | |
those individual colours are revealed. | 0:09:43 | 0:09:46 | |
Photons from the sun rain down and enter water droplets. | 0:09:55 | 0:09:59 | |
They reflect off the rear face, | 0:09:59 | 0:10:02 | |
come out of the front again and into your eye. | 0:10:02 | 0:10:05 | |
But the blue photons, the higher-energy ones, | 0:10:05 | 0:10:09 | |
behave differently to the green ones | 0:10:09 | 0:10:11 | |
and the yellow ones and the red ones. | 0:10:11 | 0:10:13 | |
They come out at a shallower angle, | 0:10:13 | 0:10:15 | |
and that's why you get the full spectrum of colours | 0:10:15 | 0:10:19 | |
from the white light of the sun. | 0:10:19 | 0:10:21 | |
And it's this light that paints the Earth. | 0:10:24 | 0:10:26 | |
The colours of our planet arise because of the way photons | 0:10:35 | 0:10:38 | |
from the sun interact with the matter from which the Earth is made. | 0:10:38 | 0:10:42 | |
From space, our planet is a blue world. | 0:10:53 | 0:10:57 | |
And that blue colour arises | 0:10:59 | 0:11:00 | |
because of the way light interacts with water. | 0:11:00 | 0:11:03 | |
And the process is linked to one of the planet's greatest migrations. | 0:11:06 | 0:11:10 | |
Every spring, marine biologist Osvaldo Vasquez | 0:11:25 | 0:11:29 | |
heads out onto the high seas... | 0:11:29 | 0:11:30 | |
-MAN ON RADIO: -...at the port bow, over. | 0:11:32 | 0:11:34 | |
11, 11 o'clock. | 0:11:34 | 0:11:35 | |
..in search of these waters' most awe-inspiring seasonal visitors. | 0:11:37 | 0:11:41 | |
Humpback whales. | 0:11:53 | 0:11:54 | |
Every year, they make the longest migration of any mammal on Earth, | 0:12:01 | 0:12:06 | |
travelling up to 8,000km | 0:12:06 | 0:12:08 | |
from their feeding grounds in the northern Atlantic | 0:12:08 | 0:12:12 | |
to the striking blue waters of the Silver Bank Marine Reserve. | 0:12:12 | 0:12:16 | |
This is the greatest nursery of humpback whales in the world. | 0:12:19 | 0:12:25 | |
85% of the North Atlantic population comes here for breeding, | 0:12:25 | 0:12:31 | |
mating, and giving birth. | 0:12:31 | 0:12:33 | |
So, from this place depends the survival of the species. | 0:12:35 | 0:12:40 | |
The whales' life cycle is intricately linked | 0:12:43 | 0:12:46 | |
to the interaction between the light of the sun | 0:12:46 | 0:12:49 | |
and the water of the ocean. | 0:12:49 | 0:12:51 | |
In order to understand their behaviour, | 0:12:55 | 0:12:58 | |
we need to go beneath, and to see, | 0:12:58 | 0:13:00 | |
with our own eyes, what is happening there. | 0:13:00 | 0:13:03 | |
Not just on the surface - underwater. | 0:13:05 | 0:13:07 | |
Yep, yep, yep. | 0:13:32 | 0:13:34 | |
Slow down. Slow down. | 0:13:55 | 0:13:58 | |
Slow down, stay down. | 0:13:58 | 0:14:00 | |
WHALES SING SOFTLY | 0:14:09 | 0:14:11 | |
The reason humpbacks come here to give birth | 0:14:17 | 0:14:20 | |
is because the shallow waters around Silver Bank are exceptionally warm. | 0:14:20 | 0:14:25 | |
Whales are warm-blooded animals, | 0:14:29 | 0:14:32 | |
and when they give birth, | 0:14:32 | 0:14:35 | |
they have a very skinny calf with no blubber. | 0:14:35 | 0:14:39 | |
They need a warm environment, as they had inside Mother. | 0:14:41 | 0:14:44 | |
So here, Silver Bank, is warm and is protected. | 0:14:45 | 0:14:49 | |
So it's suitable for giving birth. | 0:14:49 | 0:14:51 | |
As photons of light rain down onto the ocean, | 0:14:54 | 0:14:57 | |
they strike water molecules, | 0:14:57 | 0:15:00 | |
and some of this energy goes into making them jiggle around, | 0:15:00 | 0:15:03 | |
increasing their speed and, therefore, their temperature. | 0:15:03 | 0:15:08 | |
But it takes an awful lot of energy to heat the oceans, | 0:15:10 | 0:15:14 | |
and so it's only here, | 0:15:14 | 0:15:16 | |
exposed to the full glare of the equatorial sun, | 0:15:16 | 0:15:19 | |
that enough energy is absorbed | 0:15:19 | 0:15:21 | |
to raise the water temperature to a balmy 26 degrees. | 0:15:21 | 0:15:26 | |
The perfect conditions for mothers to raise their calves. | 0:15:26 | 0:15:31 | |
The calves are really very cute | 0:15:46 | 0:15:48 | |
because they are like puppies. | 0:15:48 | 0:15:51 | |
But underwater, it weighs one tonne. So...it's a big puppy. | 0:15:52 | 0:15:56 | |
But not all of the photons that enter the water are absorbed. | 0:16:01 | 0:16:05 | |
Some of them bounce straight back out again, | 0:16:05 | 0:16:08 | |
and it's these photons that reach our eyes | 0:16:08 | 0:16:11 | |
and create the blue of the oceans. | 0:16:11 | 0:16:14 | |
To understand why it's mainly red photons that are absorbed | 0:16:21 | 0:16:24 | |
rather than the blue ones, | 0:16:24 | 0:16:26 | |
we need to take a closer look at the structure of water. | 0:16:26 | 0:16:30 | |
This is called Thingvellir. | 0:17:07 | 0:17:09 | |
That's a rough pronunciation. | 0:17:11 | 0:17:14 | |
But in Icelandic, it means "parliament valley", | 0:17:14 | 0:17:17 | |
because the Vikings used to meet here over a thousand years ago | 0:17:17 | 0:17:21 | |
and had the world's first parliament. | 0:17:21 | 0:17:23 | |
The thing is, it's not actually a valley, | 0:17:23 | 0:17:25 | |
in the sense that it wasn't cut by a river or a glacier. | 0:17:25 | 0:17:29 | |
It's actually formed | 0:17:29 | 0:17:31 | |
by the continents themselves splitting apart. | 0:17:31 | 0:17:34 | |
So that is the American continental plate | 0:17:34 | 0:17:37 | |
and that is the Eurasian continental plate. | 0:17:37 | 0:17:41 | |
And if you just go about a mile down the road, | 0:17:41 | 0:17:44 | |
this place is flooded, and you can dive in it. | 0:17:44 | 0:17:47 | |
The rift is filled with glacial meltwater that seeps down | 0:17:53 | 0:17:57 | |
from Iceland's frozen interior. | 0:17:57 | 0:17:59 | |
The sun's rays are much weaker here. | 0:18:03 | 0:18:06 | |
But, wherever sunlight hits water molecules, | 0:18:06 | 0:18:09 | |
it always produces the same colour. | 0:18:09 | 0:18:11 | |
How's that feel? | 0:18:20 | 0:18:21 | |
That's good. | 0:18:23 | 0:18:24 | |
Quite nice in here, actually. | 0:18:40 | 0:18:42 | |
Look how blue this water is. | 0:18:59 | 0:19:00 | |
You can see for miles. | 0:19:01 | 0:19:03 | |
I've never seen anything like it. | 0:19:03 | 0:19:06 | |
The reason for that purity is that the water's come 50km, | 0:19:06 | 0:19:12 | |
sometimes going deep underground, | 0:19:12 | 0:19:16 | |
and being filtered by these rocks. | 0:19:16 | 0:19:19 | |
So it's some of the coldest, purest water you can imagine. | 0:19:19 | 0:19:23 | |
Really, really spectacular - look at that. | 0:19:24 | 0:19:29 | |
You can see forever. | 0:19:29 | 0:19:30 | |
Descending deeper into the fissure, | 0:19:38 | 0:19:40 | |
the effect on the colour of my drysuit | 0:19:40 | 0:19:43 | |
hints at the process by which | 0:19:43 | 0:19:45 | |
the oceans acquire their distinctive blue. | 0:19:45 | 0:19:48 | |
Well, now we're down at about, erm... | 0:19:55 | 0:19:57 | |
..well, 12 metres. | 0:19:58 | 0:20:00 | |
And you see that down here, my beautiful red diving suit | 0:20:01 | 0:20:06 | |
is no longer quite as red as it was. HE LAUGHS | 0:20:06 | 0:20:09 | |
In fact, it's looking quite black. | 0:20:10 | 0:20:12 | |
And the reason for that... | 0:20:13 | 0:20:14 | |
..is the structure of water molecules themselves. | 0:20:15 | 0:20:19 | |
See, a water molecule is an oxygen with two hydrogens attached. | 0:20:21 | 0:20:26 | |
And when the light streams into the water, the red light | 0:20:27 | 0:20:32 | |
is just the right energy to start those molecules vibrating, | 0:20:32 | 0:20:37 | |
and they do. They start going like that... | 0:20:37 | 0:20:41 | |
and like that.... | 0:20:41 | 0:20:43 | |
and even like that. | 0:20:43 | 0:20:45 | |
So all the energy in the red light is taken, | 0:20:45 | 0:20:48 | |
making the water molecules wobble and vibrate. | 0:20:48 | 0:20:51 | |
The blue light doesn't do that. | 0:20:54 | 0:20:56 | |
So the blue light can scatter around in the water | 0:20:56 | 0:20:59 | |
relatively unimpeded. | 0:20:59 | 0:21:01 | |
And that's why water is blue. | 0:21:02 | 0:21:05 | |
Cool, isn't it? | 0:21:07 | 0:21:08 | |
Vibrations inside the water molecules themselves | 0:21:19 | 0:21:22 | |
give the oceans their colour. | 0:21:22 | 0:21:24 | |
The weaker bonds between water molecules also absorb sunlight. | 0:21:25 | 0:21:29 | |
Together, these processes absorb so much energy | 0:21:31 | 0:21:34 | |
that there isn't a lot left to increase the sea temperature. | 0:21:34 | 0:21:38 | |
WHALE SQUEAKS | 0:21:38 | 0:21:40 | |
Which is why humpbacks must travel so far | 0:21:40 | 0:21:43 | |
to find water warm enough to give birth. | 0:21:43 | 0:21:45 | |
WHALE SINGS | 0:21:55 | 0:21:57 | |
Because water is hard to heat up, | 0:22:05 | 0:22:07 | |
the temperature of the oceans remains very stable, | 0:22:07 | 0:22:11 | |
creating the perfect conditions for life to thrive. | 0:22:11 | 0:22:15 | |
Liquid water is the essential ingredient | 0:22:26 | 0:22:29 | |
for any life-supporting world. | 0:22:29 | 0:22:32 | |
Oceans cover 70% of the Earth's surface, | 0:22:35 | 0:22:40 | |
their distinctive blue broadcasting to the universe | 0:22:40 | 0:22:44 | |
the message that Earth is a possible home for life. | 0:22:44 | 0:22:48 | |
And beyond the waves, on the land, | 0:22:53 | 0:22:56 | |
we see life's other signature colour - | 0:22:56 | 0:22:59 | |
a blanket of green plants. | 0:22:59 | 0:23:01 | |
As with all living things, they depend on water to survive. | 0:23:03 | 0:23:07 | |
And when the seasonal rains recede, | 0:23:07 | 0:23:10 | |
the land reverts to the arid colours of the naked earth. | 0:23:10 | 0:23:14 | |
The intense African sun | 0:23:26 | 0:23:29 | |
delivers 1,000 watts of solar power per square metre, | 0:23:29 | 0:23:33 | |
baking the plains of the Serengeti to dust. | 0:23:33 | 0:23:37 | |
Scorched brown - | 0:23:41 | 0:23:43 | |
barely a single blade of green grass survives. | 0:23:43 | 0:23:46 | |
For the Maasai, the dry season means months of hunger and hardship. | 0:23:50 | 0:23:55 | |
Parakapuni and his son and brother | 0:24:00 | 0:24:03 | |
must say goodbye to their home valley... | 0:24:03 | 0:24:05 | |
..and drive their cows across the plains | 0:24:07 | 0:24:10 | |
in search of enough grass and water | 0:24:10 | 0:24:13 | |
to keep them alive until the rains return. | 0:24:13 | 0:24:15 | |
At the end of their long journeys, | 0:24:55 | 0:24:57 | |
Maasai warriors from across the Serengeti | 0:24:57 | 0:25:00 | |
gather on the banks of Lake Masek. | 0:25:00 | 0:25:03 | |
But survival on the plains of the Serengeti | 0:25:36 | 0:25:39 | |
forces Parakapuni and his family to spend the dry season apart. | 0:25:39 | 0:25:44 | |
Because while he tends the cattle, | 0:25:47 | 0:25:50 | |
his wife Nomipuni must stay behind | 0:25:50 | 0:25:52 | |
to look after those too young or too old to make the trip... | 0:25:52 | 0:25:57 | |
..and eke out an existence on the brown, lifeless plains. | 0:25:58 | 0:26:02 | |
With the cows away, | 0:26:29 | 0:26:30 | |
the family must survive on their meagre stores | 0:26:30 | 0:26:33 | |
of maize flour and water. | 0:26:33 | 0:26:35 | |
YOUNGER CHILD WAILS | 0:26:38 | 0:26:39 | |
THUNDER RUMBLES | 0:27:30 | 0:27:31 | |
Now, after four long months apart, | 0:27:31 | 0:27:34 | |
things are about to change. | 0:27:34 | 0:27:37 | |
NOMIPUNI: | 0:27:47 | 0:27:49 | |
The coming of the rains means the grass can grow again. | 0:28:07 | 0:28:10 | |
Revived, new shoots emerge, | 0:28:19 | 0:28:23 | |
packed with the green pigment chlorophyll... | 0:28:23 | 0:28:26 | |
..which allows plants to harvest the sun's energy. | 0:28:30 | 0:28:34 | |
And the plains are transformed from dusty brown to vibrant green. | 0:28:39 | 0:28:45 | |
In just a few days, the landscape is reborn. | 0:28:50 | 0:28:54 | |
I suppose we think of green as the colour of life, | 0:29:15 | 0:29:17 | |
but actually, it's the colour that life throws away, | 0:29:17 | 0:29:21 | |
waste green photons reflected back into our eyes. | 0:29:21 | 0:29:25 | |
Plants absorb most of the rest of the rainbow, | 0:29:25 | 0:29:28 | |
the blue and red photons, | 0:29:28 | 0:29:30 | |
and use their energy to power photosynthesis. | 0:29:30 | 0:29:33 | |
Photosynthesis is the process by which plants harness light. | 0:29:36 | 0:29:42 | |
They are the bridge between nuclear reactions 93 million miles away | 0:29:42 | 0:29:47 | |
and life on Earth. | 0:29:47 | 0:29:49 | |
Energy released from nuclear fusion reactions in the sun's core | 0:29:52 | 0:29:56 | |
heats everything up and shakes electrons around, | 0:29:56 | 0:29:59 | |
and those electrons will emit photons, | 0:29:59 | 0:30:03 | |
which travel across space for eight minutes, | 0:30:03 | 0:30:06 | |
and then hit an electron in a chlorophyll molecule. | 0:30:06 | 0:30:11 | |
But instead of that energy being dissipated away as heat, | 0:30:11 | 0:30:15 | |
chlorophyll is clever, | 0:30:15 | 0:30:17 | |
and ultimately the energy imparted to that electron | 0:30:17 | 0:30:21 | |
is used to do all sorts of clever things | 0:30:21 | 0:30:23 | |
through an intricate piece of machinery. | 0:30:23 | 0:30:26 | |
Split water up, force electrons onto carbon dioxide, | 0:30:26 | 0:30:29 | |
and ultimately, build sugars, which allows the plant to grow. | 0:30:29 | 0:30:34 | |
On the plains of the Serengeti, the intricate process of photosynthesis | 0:30:38 | 0:30:43 | |
means Parakapuni can begin the long journey to rejoin his family. | 0:30:43 | 0:30:48 | |
After months apart, the greening of the Serengeti | 0:31:00 | 0:31:04 | |
transforms the harshest of environments | 0:31:04 | 0:31:06 | |
into a place the Maasai can call home. | 0:31:06 | 0:31:10 | |
Animals eat plants that feed on sunlight. | 0:32:12 | 0:32:15 | |
In this way, the sun's energy powers the entire food chain. | 0:32:21 | 0:32:25 | |
But photosynthesis does more than provide life with energy. | 0:32:31 | 0:32:35 | |
Around two and a half billion years ago, it began to transform | 0:32:39 | 0:32:42 | |
the composition of the Earth's atmosphere itself, | 0:32:42 | 0:32:46 | |
by filling it with a waste product - oxygen. | 0:32:46 | 0:32:50 | |
The gas upon which all complex life depends. | 0:32:50 | 0:32:54 | |
Without air to breathe, there would be no intelligent life on Earth. | 0:33:04 | 0:33:08 | |
We rely absolutely on the oxygen that forms | 0:33:15 | 0:33:18 | |
a fifth of the thin blue line that envelops our planet. | 0:33:18 | 0:33:22 | |
And, perhaps paradoxically, | 0:33:29 | 0:33:32 | |
why the sky is blue is best explained | 0:33:32 | 0:33:35 | |
in the dead of night. | 0:33:35 | 0:33:37 | |
It's a beautiful, crisp autumn night here in the south of England. | 0:33:50 | 0:33:53 | |
Rolling hills illuminated by moonlight. | 0:33:53 | 0:33:56 | |
Which is the light from the sun | 0:33:58 | 0:34:00 | |
reflected off the surface of the moon. | 0:34:00 | 0:34:02 | |
It's quite silent, actually, almost eerie. | 0:34:05 | 0:34:08 | |
But out there, the Earth's shadow is racing through space, | 0:34:08 | 0:34:12 | |
and actually it's just beginning to cut off | 0:34:12 | 0:34:15 | |
the top left-hand corner of the moon. | 0:34:15 | 0:34:18 | |
On a few nights every decade, | 0:34:22 | 0:34:24 | |
the sun, moon and Earth line up | 0:34:24 | 0:34:28 | |
to create one of the wonders of the night sky. | 0:34:28 | 0:34:31 | |
A total lunar eclipse. | 0:34:31 | 0:34:33 | |
You get a real sense of the celestial mechanics in action | 0:34:36 | 0:34:40 | |
during an eclipse. | 0:34:40 | 0:34:42 | |
The sun is somewhere over there behind me, | 0:34:42 | 0:34:45 | |
shining on our planet, | 0:34:45 | 0:34:47 | |
and our planet is casting a shadow through space, | 0:34:47 | 0:34:51 | |
which falls on the surface of our satellite, the moon. | 0:34:51 | 0:34:55 | |
As the Earth moves between the moon and the sun, | 0:35:00 | 0:35:03 | |
it blocks light from falling directly onto the lunar surface. | 0:35:03 | 0:35:07 | |
Now the moon is completely covered by the Earth's shadow. | 0:35:15 | 0:35:18 | |
But it's not completely blank. | 0:35:19 | 0:35:21 | |
It's glowing a deep blood red. | 0:35:21 | 0:35:24 | |
At the height of the eclipse, the only photons reaching the moon | 0:35:28 | 0:35:32 | |
have passed through the atmosphere of our planet. | 0:35:32 | 0:35:35 | |
And it's red because of the way that light | 0:35:39 | 0:35:42 | |
interacts with the Earth's atmosphere. | 0:35:42 | 0:35:45 | |
Imagine the rain photons passing through the atmosphere | 0:35:45 | 0:35:49 | |
from the sun, all the colours of the rainbow. | 0:35:49 | 0:35:52 | |
Well, the blue photons, the higher-energy photons, | 0:35:52 | 0:35:56 | |
have a higher probability of bouncing off the molecules | 0:35:56 | 0:36:00 | |
in the Earth's atmosphere so they scatter around. | 0:36:00 | 0:36:03 | |
That just leaves the lower-energy red photons, | 0:36:05 | 0:36:08 | |
which have a much lower probability of bouncing around, | 0:36:08 | 0:36:12 | |
and therefore can pass through the Earth's atmosphere | 0:36:12 | 0:36:15 | |
relatively unscathed. | 0:36:15 | 0:36:17 | |
So they are the ones that make it onto the moon's surface, | 0:36:17 | 0:36:22 | |
and reflect back into my eye, and that's why, | 0:36:22 | 0:36:25 | |
in a lunar eclipse, you get a blood-red moon. | 0:36:25 | 0:36:28 | |
And by day, the blue photons the atmosphere scatters | 0:36:40 | 0:36:44 | |
are what paint the skies blue. | 0:36:44 | 0:36:46 | |
So when you look up into the sky on a summer's day | 0:36:50 | 0:36:52 | |
and see that deep blue, | 0:36:52 | 0:36:54 | |
what you're actually seeing is blue photons | 0:36:54 | 0:36:58 | |
scattering around off the molecules in the atmosphere. | 0:36:58 | 0:37:01 | |
Red, green, blue - | 0:37:08 | 0:37:12 | |
the primary colours of our planet. | 0:37:12 | 0:37:15 | |
The Earth is painted by the photons that rain down | 0:37:15 | 0:37:18 | |
from the surface of the sun. | 0:37:18 | 0:37:20 | |
But for us to see them, those photons must take one final journey. | 0:37:22 | 0:37:28 | |
Salma lives with her seven-year-old son Majidil | 0:37:53 | 0:37:56 | |
on the banks of the Gorai River in Bangladesh. | 0:37:56 | 0:37:59 | |
This is a vibrant place to grow up. | 0:38:18 | 0:38:21 | |
But unlike the other children, Majidil can't experience it. | 0:38:22 | 0:38:27 | |
For us to see, photons must travel into our eyes, | 0:38:49 | 0:38:54 | |
but Majidil was born with severe cataracts. | 0:38:54 | 0:38:57 | |
The lenses of his eyes are so clouded, | 0:38:59 | 0:39:01 | |
he's been effectively blind since birth. | 0:39:01 | 0:39:05 | |
But today, Majidil's life is about to change. | 0:39:26 | 0:39:30 | |
His family are making the eight-hour journey to the capital, Dhaka. | 0:39:38 | 0:39:42 | |
Because this afternoon, | 0:39:50 | 0:39:51 | |
Majidil will undergo surgery designed to restore his sight. | 0:39:51 | 0:39:55 | |
If the surgery is successful, | 0:40:14 | 0:40:16 | |
replacing his faulty lenses with artificial ones | 0:40:16 | 0:40:20 | |
will allow light to travel directly into Majidil's eyes. | 0:40:20 | 0:40:23 | |
It's at the back of the eye that photons collide with cells | 0:40:36 | 0:40:39 | |
in the retina, sensitive to red, green, and blue light... | 0:40:39 | 0:40:43 | |
..and trigger the nerve impulses that allow us to see in colour. | 0:40:46 | 0:40:50 | |
BICYCLE BELL RINGS | 0:41:04 | 0:41:08 | |
THEY SPEAK ENCOURAGINGLY TO HIM | 0:41:26 | 0:41:29 | |
For the first time in his life, | 0:41:40 | 0:41:42 | |
photons are able to enter Majidil's eyes unimpeded. | 0:41:42 | 0:41:45 | |
For the first time in his life, he can see. | 0:41:53 | 0:41:57 | |
Our eyes reveal to us the colours of the Earth. | 0:42:46 | 0:42:49 | |
MAJIDIL LAUGHS | 0:42:49 | 0:42:51 | |
The first step towards understanding their meaning. | 0:42:54 | 0:42:58 | |
The blue that signals the presence of liquid water. | 0:43:04 | 0:43:07 | |
The green that marks out our planet as a home for complex life. | 0:43:10 | 0:43:15 | |
And, in this most distant image of the Earth ever taken, | 0:43:18 | 0:43:22 | |
from six billion kilometres away, | 0:43:22 | 0:43:25 | |
by the Voyager spacecraft, | 0:43:25 | 0:43:27 | |
the sunlight bouncing off our atmosphere | 0:43:27 | 0:43:30 | |
reveals our planet as a pale blue dot | 0:43:30 | 0:43:33 | |
hanging in the void of space. | 0:43:33 | 0:43:36 | |
And even from this distance, anyone who happened to be looking | 0:43:38 | 0:43:43 | |
could tell our planet contained the ingredients for life. | 0:43:43 | 0:43:48 | |
Because in the most delicate colour signals, | 0:43:49 | 0:43:52 | |
we have measured with precision what the universe is made of. | 0:43:52 | 0:43:56 | |
And those signals can be glimpsed at the very edge of our own atmosphere. | 0:44:02 | 0:44:07 | |
What are we drawing? | 0:44:22 | 0:44:24 | |
A sun dragon. | 0:44:24 | 0:44:26 | |
What's a sun dragon? | 0:44:26 | 0:44:27 | |
It's just like a sun. | 0:44:27 | 0:44:29 | |
And it's got smoke coming out of its mouth. | 0:44:30 | 0:44:34 | |
Cos it's starting to make fire on the world. | 0:44:36 | 0:44:40 | |
SHE PRETENDS TO BREATHE FIRE | 0:44:40 | 0:44:41 | |
Now, let's just do them there. | 0:44:42 | 0:44:46 | |
We need to get ready to go, don't we? | 0:44:46 | 0:44:48 | |
Push. | 0:44:50 | 0:44:51 | |
For seven years, the Nation family have been consumed by an obsession. | 0:44:51 | 0:44:55 | |
Ready to drop everything at a moment's notice, | 0:44:58 | 0:45:01 | |
in pursuit of a light show like no other. | 0:45:01 | 0:45:04 | |
I'm Aurora Chaser! | 0:45:08 | 0:45:10 | |
They've left their home on the Sussex coast | 0:45:15 | 0:45:18 | |
for the cold climes of northern Norway... | 0:45:18 | 0:45:21 | |
73, 98, 97. | 0:45:21 | 0:45:23 | |
69, 98, 100. | 0:45:25 | 0:45:27 | |
..spending their weekends | 0:45:27 | 0:45:29 | |
chasing one of the planet's most extraordinary phenomena - | 0:45:29 | 0:45:33 | |
the Northern lights. | 0:45:33 | 0:45:35 | |
Aurora borealis. | 0:45:35 | 0:45:36 | |
It's an addiction. It's an absolute full-blown addiction. | 0:45:39 | 0:45:43 | |
It's a buzz and it's a rush of adrenaline. | 0:45:43 | 0:45:46 | |
And it is a holding of your breath and...wow. | 0:45:46 | 0:45:50 | |
The aurora was once thought to be caused | 0:45:52 | 0:45:54 | |
by dragons fighting in the sky. | 0:45:54 | 0:45:56 | |
But today, we know its ethereal light | 0:45:59 | 0:46:01 | |
is created by charged particles known as the solar wind | 0:46:01 | 0:46:05 | |
interacting with the gases of the upper atmosphere. | 0:46:05 | 0:46:09 | |
Our eldest, Aurora, she's 11. | 0:46:14 | 0:46:16 | |
She's fascinated by, | 0:46:16 | 0:46:17 | |
why do those different gases | 0:46:17 | 0:46:18 | |
make those different colours? | 0:46:18 | 0:46:20 | |
She's quite fascinated by it. Oce... | 0:46:20 | 0:46:23 | |
she likes the pink, because she likes pink. | 0:46:23 | 0:46:25 | |
It's her favourite colour, so pink's cool. | 0:46:25 | 0:46:27 | |
Anything else, just wake me up if it goes pink. | 0:46:27 | 0:46:30 | |
And Lyrica is quite a fact box on everything. | 0:46:30 | 0:46:33 | |
She can explain to you what causes an aurora, | 0:46:33 | 0:46:36 | |
where it comes from, the technical names, | 0:46:36 | 0:46:38 | |
and, you know, what the magnetic field does | 0:46:38 | 0:46:41 | |
and how it stops the solar wind from harming us. | 0:46:41 | 0:46:44 | |
But the aurora is elusive. | 0:46:49 | 0:46:51 | |
To see it, conditions have to be just right. | 0:46:51 | 0:46:55 | |
Here we go! | 0:46:59 | 0:47:01 | |
Clear dark skies must combine with strong solar winds. | 0:47:01 | 0:47:06 | |
You're going to burn it. | 0:47:15 | 0:47:16 | |
All the family can do is wait. | 0:47:28 | 0:47:31 | |
Oh, oh, oh, oh. I can see some uprights there. | 0:47:56 | 0:47:59 | |
Oh, wow. | 0:48:01 | 0:48:04 | |
-Oh, yeah. -Here we go. Look at it. | 0:48:13 | 0:48:15 | |
Beautiful! | 0:48:17 | 0:48:19 | |
Look at it! | 0:48:20 | 0:48:22 | |
Look how bright that is up there, look! | 0:48:23 | 0:48:25 | |
Yay! Yes! | 0:48:34 | 0:48:36 | |
Now that's what I'm talking about. | 0:48:37 | 0:48:40 | |
Look. Ooh! | 0:48:42 | 0:48:44 | |
Look, look, look, look, look! Corona, corona! | 0:48:47 | 0:48:50 | |
-Look at it. -Look at the reds at the top! | 0:48:51 | 0:48:54 | |
-Stunning. -Wow. | 0:48:54 | 0:48:56 | |
Oh, oh, oh! | 0:49:01 | 0:49:02 | |
Oh, look at that. | 0:49:02 | 0:49:05 | |
-And on the left, on the left, look, there's some pink. -Yay! | 0:49:07 | 0:49:10 | |
Look, look, look, look, look! | 0:49:10 | 0:49:12 | |
But the aurora isn't simply beautiful. | 0:49:14 | 0:49:17 | |
It contains information. | 0:49:17 | 0:49:19 | |
As charged particles strike gas atoms, | 0:49:25 | 0:49:29 | |
a photon of light is released. | 0:49:29 | 0:49:30 | |
And because the atoms of every element have a unique structure, | 0:49:34 | 0:49:38 | |
each one gives off a photon of a unique colour. | 0:49:38 | 0:49:42 | |
The green comes from oxygen atoms, | 0:49:46 | 0:49:49 | |
pink from nitrogen. | 0:49:49 | 0:49:51 | |
Yes! | 0:50:00 | 0:50:02 | |
The colours dancing across the sky | 0:50:05 | 0:50:07 | |
reveal the composition of our atmosphere. | 0:50:07 | 0:50:10 | |
And it's these fingerprints encoded in photons of light | 0:50:13 | 0:50:17 | |
that have shown us the entire universe. | 0:50:17 | 0:50:21 | |
In the last few hundred years, | 0:51:16 | 0:51:18 | |
astronomers have gazed out from the edges of our home world... | 0:51:18 | 0:51:22 | |
..and dreamt of the universe beyond. | 0:51:24 | 0:51:27 | |
In the shadow of the Eiger, that is the Sphinx. | 0:51:36 | 0:51:40 | |
And despite appearances, | 0:51:40 | 0:51:41 | |
it isn't the lair of some Alpine super-villain. | 0:51:41 | 0:51:45 | |
It's an observatory. | 0:51:45 | 0:51:46 | |
It was built in 1937, and since then, | 0:51:46 | 0:51:48 | |
astronomers have been coming here from all over the world | 0:51:48 | 0:51:52 | |
to look at the night sky. | 0:51:52 | 0:51:53 | |
And by decoding messages hidden in the light reaching our telescopes, | 0:52:03 | 0:52:09 | |
we've discovered the true nature of the cosmos. | 0:52:09 | 0:52:12 | |
That's an aurora in a box. | 0:52:18 | 0:52:20 | |
It's a tube full of hydrogen gas that's heated up. | 0:52:20 | 0:52:24 | |
And what you're seeing in that pinky-red colour | 0:52:24 | 0:52:28 | |
are the fundamental laws of nature themselves in action. | 0:52:28 | 0:52:33 | |
They tell you that a single proton, which is the nucleus of hydrogen, | 0:52:33 | 0:52:39 | |
and a single electron, can only behave in certain ways. | 0:52:39 | 0:52:43 | |
The electrons can only go in certain places around the proton, | 0:52:43 | 0:52:47 | |
so when you heat them up, | 0:52:47 | 0:52:49 | |
they can only jump high up. | 0:52:49 | 0:52:51 | |
And then when they cool down, | 0:52:53 | 0:52:54 | |
they can only fall back in a specific way, | 0:52:54 | 0:52:57 | |
releasing light of a particular energy | 0:52:57 | 0:53:00 | |
which equals a particular colour. | 0:53:00 | 0:53:02 | |
And those laws don't just apply here on Earth. | 0:53:02 | 0:53:05 | |
They apply everywhere across the universe. | 0:53:05 | 0:53:08 | |
So anywhere that you see glowing hydrogen gas, let's say in a nebula, | 0:53:08 | 0:53:13 | |
heated up by young stars, then you'll see that specific colour. | 0:53:13 | 0:53:18 | |
Vast clouds of glowing hydrogen | 0:53:25 | 0:53:28 | |
create some of the most spectacular sights in the cosmos... | 0:53:28 | 0:53:31 | |
..their pink hue revealing the identity of the gas | 0:53:35 | 0:53:38 | |
from which they're made. | 0:53:38 | 0:53:40 | |
And what's true for nebulae | 0:53:52 | 0:53:55 | |
is true for everything in the universe. | 0:53:55 | 0:53:58 | |
By analysing the light from the stars, | 0:54:01 | 0:54:03 | |
we know that they're not just twinkling lights in the sky. | 0:54:03 | 0:54:07 | |
They're other suns made out of the same stuff as ours. | 0:54:07 | 0:54:10 | |
And if there are other suns, then there must be other planets - | 0:54:10 | 0:54:14 | |
maybe even other Earths. | 0:54:14 | 0:54:16 | |
By understanding the origin of the colours of our world - | 0:54:32 | 0:54:36 | |
the blue of its oceans... | 0:54:37 | 0:54:39 | |
..the green of its life... | 0:54:42 | 0:54:43 | |
..and the colours dancing in its atmosphere... | 0:54:47 | 0:54:50 | |
..we've uncovered the colour signature | 0:54:52 | 0:54:54 | |
of a life-supporting planet. | 0:54:54 | 0:54:56 | |
And because we understand the signature of our own world, | 0:55:01 | 0:55:05 | |
we can look for worlds like ours elsewhere in the cosmos. | 0:55:05 | 0:55:10 | |
Here's what I think is the most wonderful thought of all. | 0:55:17 | 0:55:20 | |
When you look out to those distant star systems and planets, | 0:55:20 | 0:55:25 | |
you're connected to them. | 0:55:25 | 0:55:27 | |
An electron somewhere out there | 0:55:27 | 0:55:30 | |
radiated a photon | 0:55:30 | 0:55:33 | |
which hit an electron | 0:55:33 | 0:55:35 | |
in your eye. | 0:55:35 | 0:55:38 | |
Alien photons crossing light years of space, | 0:55:38 | 0:55:41 | |
entering your retina and carrying stories of distant worlds. | 0:55:41 | 0:55:45 | |
In the constellation of Pegasus, around a sun-like star, | 0:55:52 | 0:55:56 | |
there's a planet called Osiris. | 0:55:56 | 0:55:58 | |
It's way closer to its parent star than Mercury is to our sun, | 0:55:58 | 0:56:03 | |
but it's a massive gas giant, a hot Jupiter. | 0:56:03 | 0:56:07 | |
And by measuring the light that shines through its atmosphere, | 0:56:07 | 0:56:10 | |
we found that the atmosphere is full of hydrogen and methane and water. | 0:56:10 | 0:56:16 | |
And just 24 light years away in the constellation of Scorpius, | 0:56:19 | 0:56:23 | |
there's a small, rocky world, one of the most earthlike worlds we know. | 0:56:23 | 0:56:28 | |
It orbits around a red dwarf star, | 0:56:28 | 0:56:31 | |
which is one of three stars in the system. | 0:56:31 | 0:56:35 | |
A planet with three suns in the sky. | 0:56:35 | 0:56:38 | |
In the last 20 years, | 0:56:42 | 0:56:44 | |
we've found hundreds of planets around distant suns. | 0:56:44 | 0:56:48 | |
We've began to analyse their atmospheres, | 0:56:48 | 0:56:50 | |
and search for life-giving water. | 0:56:50 | 0:56:53 | |
Science is about gathering data, | 0:57:01 | 0:57:04 | |
information about the natural world, | 0:57:04 | 0:57:06 | |
and trying to understand it. | 0:57:06 | 0:57:07 | |
And put like that, it seems a bit dry. | 0:57:07 | 0:57:10 | |
But when that information carries stories of alien worlds | 0:57:10 | 0:57:15 | |
around distant suns hundreds of light years away, | 0:57:15 | 0:57:18 | |
that's a whole different thing. | 0:57:18 | 0:57:20 | |
Astronomy turns data into dreams - | 0:57:20 | 0:57:24 | |
dreams of worlds of ice and snow, | 0:57:24 | 0:57:27 | |
dreams of world with hemispheres | 0:57:27 | 0:57:30 | |
in perpetual day and permanent night. | 0:57:30 | 0:57:33 | |
Dreams of world with moons and moonbows, | 0:57:33 | 0:57:36 | |
and perhaps, just perhaps, | 0:57:36 | 0:57:39 | |
alien astronomers observing the light | 0:57:39 | 0:57:42 | |
passing through the atmosphere of our blue world, | 0:57:42 | 0:57:45 | |
and dreaming of us. | 0:57:45 | 0:57:47 |