Browse content similar to Order Out of Chaos. Check below for episodes and series from the same categories and more!
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We live on a world of wonders... | 0:00:04 | 0:00:06 | |
..a place of astonishing beauty and complexity. | 0:00:08 | 0:00:12 | |
We have vast oceans and incredible weather, | 0:00:14 | 0:00:19 | |
giant mountains and breathtaking landscapes. | 0:00:19 | 0:00:23 | |
If you think that this is all there is, | 0:00:24 | 0:00:27 | |
that our planet exists in magnificent isolation, | 0:00:27 | 0:00:30 | |
then you're wrong. | 0:00:30 | 0:00:31 | |
As a physicist, I'm fascinated by how the laws of nature | 0:00:34 | 0:00:38 | |
that shaped all this | 0:00:38 | 0:00:40 | |
also shaped the worlds beyond our home planet. | 0:00:40 | 0:00:44 | |
I think we're living through the greatest age of discovery our civilisation has known. | 0:00:48 | 0:00:54 | |
We've voyaged to the farthest reaches of the solar system. | 0:00:54 | 0:00:58 | |
We've photographed strange new worlds, | 0:00:58 | 0:01:02 | |
stood in unfamiliar landscapes, tasted alien air. | 0:01:02 | 0:01:06 | |
But what makes the wonders of the solar system even more astonishing is | 0:01:08 | 0:01:13 | |
that it all started as nothing more than a chaotic cloud of gas and dust. | 0:01:13 | 0:01:17 | |
And it was from that cloud that everything in the solar system formed. | 0:01:19 | 0:01:23 | |
All this order - the sun, | 0:01:23 | 0:01:26 | |
the rotating planets, me - | 0:01:26 | 0:01:29 | |
coalesced from a collapsing cloud of dust. | 0:01:29 | 0:01:33 | |
In this film, we'll discover | 0:01:37 | 0:01:39 | |
how the solar system made the journey from chaos into order... | 0:01:39 | 0:01:43 | |
..and see how that cloud gave rise to the solar system's most beautiful wonder - | 0:01:44 | 0:01:49 | |
the majestic rings of Saturn. | 0:01:49 | 0:01:52 | |
We'll discover how Saturn's amazingly varied moons | 0:01:55 | 0:01:59 | |
govern the intricate patterns of the rings, | 0:01:59 | 0:02:02 | |
and how another wonder recently discovered on one of those moons | 0:02:02 | 0:02:06 | |
is changing our ideas | 0:02:06 | 0:02:08 | |
about the nature of the outer solar system. | 0:02:08 | 0:02:11 | |
It's cool! | 0:02:11 | 0:02:12 | |
We'll witness the fundamental forces that control the universe... | 0:02:15 | 0:02:20 | |
It's beginning to come - the end of the world. | 0:02:20 | 0:02:22 | |
..and see how those forces were unleashed | 0:02:22 | 0:02:26 | |
to create the beautifully ordered solar system we live in. | 0:02:26 | 0:02:29 | |
It's only now that we're beginning to understand the origins of that order, | 0:02:33 | 0:02:37 | |
and that has implications for our understanding of the entire solar system, | 0:02:37 | 0:02:41 | |
and, ultimately, of why we are here. | 0:02:41 | 0:02:45 | |
MUEZZIN CHANTS | 0:03:10 | 0:03:17 | |
This is the Great Mosque in the city of Kairouan in Tunisia, | 0:03:20 | 0:03:24 | |
and this mosque is the fourth holiest place in Islam, | 0:03:24 | 0:03:27 | |
and so for the last 14 centuries, the relentless passing of the days | 0:03:27 | 0:03:33 | |
has been celebrated by prayers before dawn, at sunrise, | 0:03:33 | 0:03:38 | |
at noon, at sunset and in the evening. | 0:03:38 | 0:03:43 | |
MUEZZIN CHANTS | 0:03:43 | 0:03:46 | |
The calls to prayer mark out | 0:03:46 | 0:03:49 | |
the passing of time as the sun travels across the sky. | 0:03:49 | 0:03:54 | |
But it's not the sun that's moving. | 0:03:54 | 0:03:57 | |
What we're really observing is the movement of the Earth through space. | 0:03:57 | 0:04:02 | |
This is the ball of rock we live on. | 0:04:09 | 0:04:13 | |
It carries us through cycles of night and day as it turns on its axis every 24 hours. | 0:04:13 | 0:04:20 | |
A year is the time it takes to orbit the sun, | 0:04:20 | 0:04:24 | |
and we have seasons because the Earth's axis is tilted by 23 degrees. | 0:04:24 | 0:04:29 | |
To see how that works, we need to speed time up | 0:04:32 | 0:04:35 | |
so a year passes in just ten seconds. | 0:04:35 | 0:04:38 | |
At this pace, | 0:04:38 | 0:04:40 | |
we can see how the southern and then northern hemispheres | 0:04:40 | 0:04:43 | |
are angled towards the warmth of the sun, | 0:04:43 | 0:04:46 | |
taking us through yearly cycles of summer and winter. | 0:04:46 | 0:04:50 | |
All the rhythms of our lives are governed | 0:04:53 | 0:04:55 | |
by how the Earth travels through space, | 0:04:55 | 0:04:59 | |
and in Tunisia in April, it's springtime. | 0:04:59 | 0:05:03 | |
This is the seasonal flower market in Kairouan, and it's only here | 0:05:18 | 0:05:23 | |
for two months of the year, | 0:05:23 | 0:05:26 | |
because that's when these flowers are in flower. | 0:05:26 | 0:05:30 | |
And it's a beautiful example of how the structure, the clockwork of the solar system | 0:05:30 | 0:05:36 | |
affects things here on Earth in the most unexpected of ways, | 0:05:36 | 0:05:40 | |
because if our Earth's axis wasn't tilted by 23 degrees, then there wouldn't be any seasons, | 0:05:40 | 0:05:46 | |
and if there weren't any seasons, then seasonal flowers wouldn't have evolved | 0:05:46 | 0:05:50 | |
and there wouldn't be a flower market. | 0:05:50 | 0:05:52 | |
But it's not just the Earth. | 0:05:59 | 0:06:01 | |
The whole solar system is full of rhythms. | 0:06:01 | 0:06:05 | |
Each planet orbits the sun at its own distinctive tempo. | 0:06:05 | 0:06:09 | |
Mercury is the fastest. | 0:06:11 | 0:06:13 | |
Closest to the sun, it reaches speeds | 0:06:13 | 0:06:16 | |
of 200,000 kilometres an hour as it completes its orbit in just 88 days. | 0:06:16 | 0:06:22 | |
Venus rotates so slowly that it takes longer to spin on its axis | 0:06:29 | 0:06:34 | |
than it does to go around the sun, | 0:06:34 | 0:06:36 | |
so that on Venus, a day is longer than a year. | 0:06:36 | 0:06:40 | |
Further out, the planets orbit more and more slowly. | 0:06:44 | 0:06:48 | |
Jupiter, the largest planet, takes 12 Earth years to complete each orbit. | 0:06:48 | 0:06:54 | |
And at the very furthest reaches of the solar system, | 0:06:56 | 0:06:59 | |
4.5 billion kilometres from the sun, | 0:06:59 | 0:07:02 | |
Neptune travels so slowly that it hasn't completed a single orbit | 0:07:02 | 0:07:07 | |
since it was discovered in 1846. | 0:07:07 | 0:07:10 | |
The solar system is driven by these rhythms, | 0:07:11 | 0:07:14 | |
so regular that the whole thing could be run by clockwork. | 0:07:14 | 0:07:19 | |
It seems extraordinary that such a well-ordered system | 0:07:19 | 0:07:23 | |
could have come into being spontaneously, | 0:07:23 | 0:07:27 | |
but it is in fact a great example | 0:07:27 | 0:07:29 | |
of the beauty and symmetry that lies at the heart of the universe. | 0:07:29 | 0:07:33 | |
I want to explain how that order emerged from the chaos of space, | 0:07:35 | 0:07:40 | |
because understanding that will help us understand | 0:07:40 | 0:07:44 | |
the origins and formation of the solar system, | 0:07:44 | 0:07:47 | |
and the beauty of its wonders. | 0:07:47 | 0:07:49 | |
These are the Atlas Mountains in North Africa. | 0:08:11 | 0:08:14 | |
According to Roman legend, they held the heavens above the Earth. | 0:08:15 | 0:08:20 | |
And they are one of the finest places to come to view the stars. | 0:08:24 | 0:08:29 | |
From a place like this, it's easy to appreciate the profound effect | 0:08:33 | 0:08:37 | |
that the night sky would have had on our ancestors. | 0:08:37 | 0:08:41 | |
You know, from a modern perspective, | 0:08:48 | 0:08:50 | |
astronomy can seem remote and arcane, | 0:08:50 | 0:08:55 | |
because we've lost our connection with the night sky. | 0:08:55 | 0:08:59 | |
From a city you just don't see a sky look anything like this. | 0:08:59 | 0:09:05 | |
From the darkness of the Atlas Mountains, it's really, truly majestic. | 0:09:05 | 0:09:11 | |
So for our ancestors, | 0:09:12 | 0:09:14 | |
the connection with the night sky would have been incredibly intimate. | 0:09:14 | 0:09:18 | |
They looked into the skies to understand their place in creation, | 0:09:20 | 0:09:24 | |
and the movement of the stars | 0:09:24 | 0:09:25 | |
told them one thing - | 0:09:25 | 0:09:28 | |
they were at the centre of the universe. | 0:09:28 | 0:09:31 | |
Up there is Polaris, the North Star, | 0:09:32 | 0:09:36 | |
and it's almost exactly aligned with the Earth's spin axis, | 0:09:36 | 0:09:40 | |
which means that, as the Earth rotates, | 0:09:40 | 0:09:43 | |
all the stars rotate through the sky around that point. | 0:09:43 | 0:09:47 | |
So it looks for all the world as if the Earth | 0:10:03 | 0:10:07 | |
is at the centre of the universe and the stars rotate around it. | 0:10:07 | 0:10:13 | |
And that's, of course, what the ancients thought for thousands of years, and why not? | 0:10:18 | 0:10:23 | |
Because it's obvious... | 0:10:23 | 0:10:27 | |
but wrong. | 0:10:27 | 0:10:29 | |
To understand the Earth's real position in the solar system, | 0:10:31 | 0:10:34 | |
we need to look at the one set of bodies | 0:10:34 | 0:10:36 | |
that doesn't behave as predictably as the stars. | 0:10:36 | 0:10:40 | |
The Greeks named them "planetes", or "wandering stars", | 0:10:40 | 0:10:45 | |
and we have kept the name "planet" to describe them. | 0:10:45 | 0:10:48 | |
This is Mars, photographed once a week over a period of months. | 0:10:50 | 0:10:56 | |
Rather than travelling in a straight line | 0:10:56 | 0:10:59 | |
across the background of the stars, | 0:10:59 | 0:11:01 | |
it occasionally changes direction and loops back on itself. | 0:11:01 | 0:11:05 | |
It's very hard to explain these retrograde loops | 0:11:07 | 0:11:10 | |
if the Earth is at the centre of the universe. | 0:11:10 | 0:11:14 | |
Understanding the retrograde motion of Mars didn't come easy. | 0:11:17 | 0:11:21 | |
That's why it took over 2,000 years to work out, but I'm going to explain it using a stick and some rocks. | 0:11:21 | 0:11:27 | |
The key thing is that the Earth is not at the centre of the solar system. | 0:11:27 | 0:11:31 | |
The sun is, | 0:11:31 | 0:11:33 | |
and the Earth and Mars go round it | 0:11:33 | 0:11:37 | |
in almost... | 0:11:37 | 0:11:39 | |
circular orbits. | 0:11:39 | 0:11:43 | |
So when Mars is viewed from the Earth, | 0:11:43 | 0:11:45 | |
then it's seen on the sky - | 0:11:45 | 0:11:49 | |
in fact on the constellations of the Zodiac. | 0:11:49 | 0:11:52 | |
So as Mars orbits around and the Earth orbits around, | 0:11:52 | 0:11:56 | |
then from that position, | 0:11:56 | 0:11:57 | |
Mars will look like it's there on the sky. | 0:11:57 | 0:12:01 | |
Mars moves and the Earth moves in THAT position... | 0:12:01 | 0:12:05 | |
..and Mars moves in that direction across the sky, and again, | 0:12:06 | 0:12:12 | |
in that position, | 0:12:12 | 0:12:14 | |
Mars will be here, so it's moving in a straight line across the sky. | 0:12:14 | 0:12:17 | |
But what happens when the Earth overtakes Mars? | 0:12:20 | 0:12:24 | |
Then look at the line of sight. | 0:12:24 | 0:12:27 | |
Mars has moved back to there. | 0:12:27 | 0:12:31 | |
It's reversed its direction. | 0:12:31 | 0:12:33 | |
And it continues to do that | 0:12:34 | 0:12:36 | |
until the Earth gets round to somewhere like there, | 0:12:36 | 0:12:40 | |
and Mars is here, | 0:12:40 | 0:12:42 | |
and the line of sight means it's started moving that way again. | 0:12:42 | 0:12:45 | |
So Mars has executed that strange looping motion on the sky | 0:12:49 | 0:12:53 | |
because the Earth overtook Mars on the inside, and that's why | 0:12:53 | 0:13:00 | |
the retrograde motion happens. | 0:13:00 | 0:13:02 | |
Simple! | 0:13:02 | 0:13:04 | |
Understanding the retrograde loops was one of the major achievements of early astronomy. | 0:13:06 | 0:13:12 | |
It created the concept of the solar system | 0:13:12 | 0:13:16 | |
and allowed us to build the first accurate maps of the planets | 0:13:16 | 0:13:19 | |
and their orbits around the sun. | 0:13:19 | 0:13:22 | |
Once you had this picture of a solar system | 0:13:23 | 0:13:26 | |
running like clockwork, | 0:13:26 | 0:13:28 | |
the sun surrounded by the orbiting planets, | 0:13:28 | 0:13:31 | |
then you might start asking questions like | 0:13:31 | 0:13:34 | |
why is the solar system so ordered, | 0:13:34 | 0:13:37 | |
and how did that order come into existence. | 0:13:37 | 0:13:40 | |
Well, a clue lies in those sweeping, circular motions of the planets. | 0:13:40 | 0:13:47 | |
-RADIO: -..Severe storms over western Oklahoma, 70%. | 0:13:58 | 0:14:03 | |
Other hazardous weather, 80%... | 0:14:03 | 0:14:06 | |
To understand how the solar system came into being, | 0:14:06 | 0:14:10 | |
we need to understand the physical principles that govern the whole universe. | 0:14:10 | 0:14:15 | |
But, of course, the same laws of physics also control the world WE inhabit, | 0:14:15 | 0:14:20 | |
so to discover how the solar system started, | 0:14:20 | 0:14:24 | |
we don't need to look out into space or back in time. | 0:14:24 | 0:14:27 | |
We just need to look around us. | 0:14:27 | 0:14:30 | |
One of the remarkable things about the laws of nature is that they're universal, | 0:14:30 | 0:14:35 | |
and that means that the same laws that describe the formation of the solar system | 0:14:35 | 0:14:39 | |
can also describe the most mundane things here on Earth, like the motion of water as it drains from the sink. | 0:14:39 | 0:14:46 | |
These spinning spirals are seen all across the universe. | 0:14:50 | 0:14:53 | |
We see them everywhere because the laws of physics are the same everywhere. | 0:14:53 | 0:14:59 | |
I've come here to Oklahoma to see how those laws can unleash forces | 0:15:03 | 0:15:07 | |
that drive some of the most powerful and destructive phenomena in the atmosphere of our planet - | 0:15:07 | 0:15:12 | |
tornadoes. | 0:15:12 | 0:15:14 | |
Oklahoma is in the middle of what is known as Tornado Alley. | 0:15:16 | 0:15:20 | |
-No, no, no! Tornado! Tornado! -Oh, my God! | 0:15:20 | 0:15:22 | |
Yep, it's huge. | 0:15:22 | 0:15:24 | |
-Oh, wow! -Big, big, big. -Look at that thing! | 0:15:24 | 0:15:27 | |
Look at it spin! | 0:15:27 | 0:15:28 | |
Every year, hundreds of twisters tear across the landscape. | 0:15:28 | 0:15:33 | |
They're incredibly dangerous and destructive, | 0:15:33 | 0:15:37 | |
and their key feature is that same spinning spiral. | 0:15:37 | 0:15:40 | |
Don Giuliano is a professional storm chaser. | 0:15:51 | 0:15:54 | |
He's going to help me try to get close to a tornado. | 0:15:54 | 0:15:59 | |
That little developing storm there is this. | 0:15:59 | 0:16:02 | |
It's a severe thunderstorm that is capable of producing a tornado. | 0:16:02 | 0:16:06 | |
Anywhere inside that purple area, it's possible that a tornado could be there or is moving that way. | 0:16:06 | 0:16:11 | |
And what would happen if, in this car, we - deliberately or not - went straight through it? | 0:16:11 | 0:16:17 | |
It would probably pick up our car and toss it | 0:16:17 | 0:16:19 | |
a quarter of a mile through the air and crush it into a little ball. | 0:16:19 | 0:16:24 | |
I'm going to just do a U-turn. | 0:16:24 | 0:16:26 | |
THEY LAUGH | 0:16:26 | 0:16:28 | |
'Bizarre as it sounds, | 0:16:32 | 0:16:34 | |
'the processes that drive these vast storm systems | 0:16:34 | 0:16:38 | |
'are the same as would have been seen 5 billion years ago at the start of the solar system.' | 0:16:38 | 0:16:44 | |
Everything that we know and see around us was formed from a nebula - | 0:16:49 | 0:16:54 | |
a giant cloud of gas and dust. | 0:16:54 | 0:16:57 | |
Drifting across light years of space, | 0:16:58 | 0:17:01 | |
that cloud remained unchanged for millions of years. | 0:17:01 | 0:17:06 | |
But then something happened that caused it to coalesce | 0:17:06 | 0:17:10 | |
into the solar system we have today. | 0:17:10 | 0:17:12 | |
It's thought that a supernova, | 0:17:16 | 0:17:18 | |
the explosive death of a nearby star, | 0:17:18 | 0:17:21 | |
sent shockwaves through the nebula. | 0:17:21 | 0:17:24 | |
This caused a clump to form in the heart of the cloud. | 0:17:24 | 0:17:29 | |
Because it was more dense, its gravitational pull was stronger | 0:17:29 | 0:17:33 | |
and it started to pull in more and more gas. | 0:17:33 | 0:17:37 | |
Soon the whole cloud was collapsing, and crucially, it began to spin. | 0:17:37 | 0:17:42 | |
It's a feature of all things that spin | 0:17:47 | 0:17:50 | |
that if they contract, they must also rotate faster. | 0:17:50 | 0:17:53 | |
It's a universal principle called the conservation of angular momentum. | 0:17:53 | 0:17:58 | |
Just pull off anywhere here. | 0:17:58 | 0:18:00 | |
'It's this that leads to those spinning spirals, | 0:18:00 | 0:18:04 | |
'and it applies equally well to the early solar system | 0:18:04 | 0:18:07 | |
'and storms like these. | 0:18:07 | 0:18:10 | |
'As the giant thunderheads build, | 0:18:10 | 0:18:12 | |
'they suck up hot air and contract, | 0:18:12 | 0:18:16 | |
'and like the cloud that built the solar system, | 0:18:16 | 0:18:19 | |
'when they contract, they spin faster and faster.' | 0:18:19 | 0:18:23 | |
On Earth in storms like this, | 0:18:26 | 0:18:28 | |
conservation of angular momentum means that you get, in the most extreme case, tornadoes. | 0:18:28 | 0:18:33 | |
You get very rapidly rotating columns of air | 0:18:33 | 0:18:36 | |
where the wind speeds can rise to 300, 400, even sometimes 500 kilometres an hour. | 0:18:36 | 0:18:42 | |
It's very similar to the process that occurred early in the formation of the solar system, | 0:18:42 | 0:18:47 | |
when a collapsing cloud of dust got, for some reason, a little bit of spin, | 0:18:47 | 0:18:52 | |
and as that dust cloud collapsed, the spin rate has to speed up and speed up. | 0:18:52 | 0:18:57 | |
That's what you can see in storms like this when tornadoes are formed. | 0:18:57 | 0:19:01 | |
The spin of the big storm system can become concentrated and speeded up | 0:19:01 | 0:19:06 | |
in, well, a tornado. | 0:19:06 | 0:19:09 | |
You get immense wind speeds, although the wind speed isn't too gentle now. | 0:19:09 | 0:19:13 | |
And it looks pretty wild up there, I've got to say. | 0:19:13 | 0:19:17 | |
In fact, I've never... Look at that. | 0:19:17 | 0:19:19 | |
I've rarely seen such dramatic clouds. | 0:19:19 | 0:19:23 | |
And apparently, we've got about five minutes before the end of the world, | 0:19:31 | 0:19:36 | |
so we have to get back in the car. | 0:19:36 | 0:19:39 | |
There's thunder and lightning and there was a report earlier from this storm | 0:19:39 | 0:19:43 | |
of hail the size of baseballs, and I don't want one of those on my head. | 0:19:43 | 0:19:47 | |
PATTERING | 0:19:47 | 0:19:49 | |
-Let's get back to the car. -Let's go. | 0:19:49 | 0:19:52 | |
It's beginning to come - the end of the world! | 0:19:52 | 0:19:55 | |
'This storm never developed into a tornado, but when they do, | 0:20:04 | 0:20:10 | |
'you can really see the conservation of angular momentum in action.' | 0:20:10 | 0:20:14 | |
Huge tornado, look at that! | 0:20:14 | 0:20:17 | |
'As the storm contracts, its core rotates faster and faster | 0:20:17 | 0:20:22 | |
'until a column of violently rotating air descends from the cloud.' | 0:20:22 | 0:20:27 | |
Man, look at that funnel! | 0:20:27 | 0:20:29 | |
'The awesome spinning power of tornadoes has incredibly destructive effects, | 0:20:30 | 0:20:35 | |
'but it's this same phenomenon | 0:20:35 | 0:20:37 | |
'that is responsible for creating the stability of the solar system, | 0:20:37 | 0:20:42 | |
'because it was the conservation of angular momentum | 0:20:42 | 0:20:45 | |
'that stopped the early solar system collapsing completely.' | 0:20:45 | 0:20:48 | |
Oh, my God, that's going to be violent. | 0:20:48 | 0:20:51 | |
While gravity caused the nebula to contract, its conserved spin | 0:20:57 | 0:21:02 | |
gave rise to a force that balanced the inward pull of gravity | 0:21:02 | 0:21:06 | |
and allowed a stable disc to form. | 0:21:06 | 0:21:09 | |
When the sun ignited, it lit up this spinning disc. | 0:21:12 | 0:21:16 | |
And within the disc, the planets formed, | 0:21:18 | 0:21:21 | |
all orbiting the sun in their regular, clockwork patterns. | 0:21:21 | 0:21:27 | |
In just a few hundred million years, | 0:21:42 | 0:21:44 | |
the cloud had collapsed to form a star system, | 0:21:44 | 0:21:49 | |
our solar system, | 0:21:49 | 0:21:51 | |
the sun surrounded by planets, | 0:21:51 | 0:21:53 | |
and the journey from chaos into order had begun. | 0:21:53 | 0:21:58 | |
And there's no better place to see the results of that journey | 0:21:58 | 0:22:01 | |
than in what I think is one of the wonders of the solar system. | 0:22:01 | 0:22:06 | |
Of all the solar system's wonders, | 0:22:12 | 0:22:15 | |
there is a place we can go where the processes that built the solar system | 0:22:15 | 0:22:20 | |
are still in action today... | 0:22:20 | 0:22:22 | |
..a place of outstanding beauty and complexity... | 0:22:24 | 0:22:29 | |
..a place that has entranced astronomers for centuries... | 0:22:31 | 0:22:36 | |
..the planet Saturn. | 0:22:39 | 0:22:41 | |
This is NASA's Jet Propulsion Laboratory, | 0:22:51 | 0:22:53 | |
and I've known about this place, or its address - Oak Grove Drive, Pasadena, California - | 0:22:53 | 0:22:58 | |
since I was very small, because I wrote to them in 1975 | 0:22:58 | 0:23:01 | |
to ask for pictures from the surface of Mars taken by Viking, and they sent them. | 0:23:01 | 0:23:06 | |
But today, this is the control centre for Cassini, which is our one, | 0:23:06 | 0:23:10 | |
and to date, only, spacecraft in orbit around Saturn. | 0:23:10 | 0:23:14 | |
Cassini was launched in 1997. | 0:23:24 | 0:23:27 | |
It is the largest, most sophisticated spacecraft ever sent to the outer solar system. | 0:23:27 | 0:23:33 | |
Its purpose is to study Saturn and its rings, and since 2004, | 0:23:39 | 0:23:44 | |
it has been sending back the most amazing pictures. | 0:23:44 | 0:23:48 | |
They reveal that the rings are impossibly intricate, | 0:23:50 | 0:23:54 | |
made up of thousands upon thousands of individual bands and gaps. | 0:23:54 | 0:23:59 | |
The whole system is surrounded by a network of moons. | 0:24:01 | 0:24:06 | |
Part of Cassini's mission is to discover how the rings | 0:24:09 | 0:24:12 | |
came to be like this, how all this incredible structure was created. | 0:24:12 | 0:24:18 | |
Because, strange as it seems, | 0:24:20 | 0:24:22 | |
these beautiful patterns are as close as we can get | 0:24:22 | 0:24:26 | |
to the disc that formed the solar system, | 0:24:26 | 0:24:30 | |
and that is why the Saturnian system has so much to tell us. | 0:24:30 | 0:24:35 | |
I mean, I like to think of it as like a miniature solar system. | 0:24:40 | 0:24:43 | |
The moons are the equivalent of the planets and Saturn is the equivalent of the sun. | 0:24:43 | 0:24:47 | |
'Carl Murray has spent a lifetime studying Saturn's rings.' | 0:24:47 | 0:24:52 | |
In the rings, we're learning something about our own origins, if you like, | 0:24:53 | 0:24:57 | |
because the physical processes that go on in the rings | 0:24:57 | 0:25:00 | |
and their interaction with the small moons | 0:25:00 | 0:25:03 | |
are probably similar to what went on in the early solar system after the planets formed, | 0:25:03 | 0:25:08 | |
and there's still a ring or debris left over from the formation of the planets. | 0:25:08 | 0:25:13 | |
So if you looked at the solar system 4.5 billion years ago, the sun at the centre, | 0:25:13 | 0:25:18 | |
-you'd have a disc of dust not unlike Saturn's ring system? -That's right. | 0:25:18 | 0:25:25 | |
But if we can't understand a disc of material that's in our own back yard, | 0:25:25 | 0:25:30 | |
what chance do we have of understanding | 0:25:30 | 0:25:32 | |
a disc that's long since disappeared - the one out of which the solar system formed? | 0:25:32 | 0:25:37 | |
So it's the same processes, but we've got this incredible opportunity with Cassini | 0:25:37 | 0:25:42 | |
to observe things happening in front of our eyes. | 0:25:42 | 0:25:45 | |
Using the data from Cassini, we are able to recreate Saturn's rings in incredible detail. | 0:25:52 | 0:25:58 | |
We can journey from the vast scale of the disc | 0:26:01 | 0:26:04 | |
to the minute structure of individual ringlets. | 0:26:04 | 0:26:08 | |
All the rings are in motion, orbiting Saturn at immense speeds. | 0:26:15 | 0:26:21 | |
Like the planets orbiting the sun, the rings nearest Saturn are | 0:26:21 | 0:26:25 | |
the fastest, travelling at over 80,000 kilometres an hour. | 0:26:25 | 0:26:29 | |
And while the rings appear solid, casting shadows onto the planet, | 0:26:31 | 0:26:35 | |
they are also incredibly delicate. | 0:26:35 | 0:26:39 | |
The main disc of the rings is over 100,000 kilometres across, | 0:26:39 | 0:26:43 | |
but as little as three metres thick. | 0:26:43 | 0:26:46 | |
Saturn's rings are undoubtedly beautiful | 0:27:02 | 0:27:05 | |
and, when you see those magnificent pictures from Cassini, | 0:27:05 | 0:27:10 | |
it's almost impossible to imagine that that level of intricacy and beauty and symmetry | 0:27:10 | 0:27:16 | |
could have emerged spontaneously, but emerge spontaneously it did. | 0:27:16 | 0:27:20 | |
And for that reason alone, Saturn's rings are one of my wonders of the solar system. | 0:27:20 | 0:27:26 | |
But there's more than that because, in studying the origin and evolution of Saturn's rings, | 0:27:26 | 0:27:33 | |
we've begun to gain valuable insights into the origins and evolutions of our own solar system. | 0:27:33 | 0:27:40 | |
To try to understand the true nature of Saturn's rings, I've come to this glacial lagoon in Iceland. | 0:27:59 | 0:28:05 | |
There are two things the boat driver told me about these icebergs. | 0:28:11 | 0:28:16 | |
One is that they can come up from the bottom of the seabed | 0:28:16 | 0:28:20 | |
without any warning at all, | 0:28:20 | 0:28:22 | |
fly up to the surface, tip the boat over and then you die. | 0:28:22 | 0:28:28 | |
Secondly, if you take some of it and take it home, it's absolutely brilliant in whisky | 0:28:28 | 0:28:34 | |
because the water is pure, a thousand years old, | 0:28:34 | 0:28:40 | |
no pollutants in it and it makes whisky taste superb. | 0:28:40 | 0:28:43 | |
So it's either death or whisky. | 0:28:43 | 0:28:46 | |
That's my kind of pond! | 0:28:46 | 0:28:48 | |
But I'm really here because the structure of the rings | 0:28:52 | 0:28:55 | |
is remarkably similar to the way these icebergs float in the lagoon, | 0:28:55 | 0:29:01 | |
because, despite appearances, the rings aren't solid. | 0:29:03 | 0:29:07 | |
Each ring is made up of hundreds of ringlets | 0:29:07 | 0:29:11 | |
and each ringlet is made up of billions of separate pieces. | 0:29:11 | 0:29:16 | |
Caught within the grasp of Saturn's gravity, the ring particles | 0:29:17 | 0:29:22 | |
independently orbit around the planet in an impossibly thin layer. | 0:29:22 | 0:29:27 | |
-Thanks, see you in a minute. -Yeah hopefully. | 0:29:27 | 0:29:30 | |
But the similarity doesn't end with the layout. | 0:29:32 | 0:29:36 | |
It also lies in what the rings and the icebergs are made of, | 0:29:36 | 0:29:40 | |
and that explains why the rings are so bright. | 0:29:40 | 0:29:44 | |
Well, this is why we can see Saturn's rings from Earth, | 0:29:54 | 0:29:58 | |
because this is what they're made of. | 0:29:58 | 0:30:00 | |
They're made of beautiful pure water ice, sparkling in the sunlight, | 0:30:00 | 0:30:06 | |
billions of these pieces, a billion kilometres away from Earth. | 0:30:06 | 0:30:10 | |
Most of the pieces are, well, smaller than that, less than a centimetre. | 0:30:17 | 0:30:23 | |
Many are micron size ice crystals, but some are as big as this iceberg. | 0:30:23 | 0:30:29 | |
Some are as big as houses. | 0:30:29 | 0:30:31 | |
Some can be over a kilometre across. | 0:30:31 | 0:30:35 | |
Imagine sitting on one! | 0:30:35 | 0:30:37 | |
Imagine this were a piece of Saturn's rings. What a view. | 0:30:37 | 0:30:41 | |
This is the closest we can get to Saturn's rings on Earth | 0:30:47 | 0:30:51 | |
and the view would be remarkably similar. | 0:30:51 | 0:30:54 | |
Billions of chunks of ice shining brightly as they catch the sunlight. | 0:30:58 | 0:31:04 | |
And the reason the rings shine so brightly is that, like the icebergs, | 0:31:07 | 0:31:13 | |
the rings are constantly changing. | 0:31:13 | 0:31:16 | |
As the ring particles orbit Saturn, | 0:31:18 | 0:31:21 | |
they're continually crashing into each other and collecting into giant | 0:31:21 | 0:31:25 | |
clusters that are endlessly forming and breaking apart. | 0:31:25 | 0:31:30 | |
As they collide, the particles shatter | 0:31:31 | 0:31:34 | |
exposing bright new faces of ice that catch the sunlight. | 0:31:34 | 0:31:40 | |
It's because of this constant recycling that the rings are | 0:31:40 | 0:31:43 | |
able to stay as bright and shiny as they were when they formed. | 0:31:43 | 0:31:48 | |
For me, one of the most remarkable things about Saturn's rings | 0:31:58 | 0:32:03 | |
is their dynamism, their constant renewal. | 0:32:03 | 0:32:07 | |
It's because of that dynamism that we can see them at all. | 0:32:07 | 0:32:10 | |
That's why they're clean, that's why they reflect sunlight and we can see them from Earth. | 0:32:10 | 0:32:16 | |
It's, I suppose, a bit like a city that people come and go, buildings | 0:32:16 | 0:32:22 | |
get torn down and rebuilt but the city always remains the same. | 0:32:22 | 0:32:27 | |
So it is with Saturn's rings. | 0:32:27 | 0:32:29 | |
They're different today than they were a thousand years ago. | 0:32:29 | 0:32:32 | |
They'll be different in a hundred or a thousand years' time | 0:32:32 | 0:32:36 | |
but that structure and that beauty, that magnificence will always remain. | 0:32:36 | 0:32:43 | |
Saturn's rings are magnificent for more than just their beauty... | 0:32:55 | 0:33:00 | |
..because by looking at the rings | 0:33:01 | 0:33:03 | |
we can begin to understand our own origins. | 0:33:03 | 0:33:07 | |
And the key to understanding the rings can be found orbiting around them. | 0:33:13 | 0:33:19 | |
Oh! | 0:33:26 | 0:33:27 | |
That is absolutely incredible. | 0:33:27 | 0:33:30 | |
You can see the rings are completely end on. | 0:33:30 | 0:33:35 | |
I mean, when you see that, I've looked at the sky, I've looked | 0:33:35 | 0:33:38 | |
at Saturn hundreds of times but I've never seen it through a telescope like this | 0:33:38 | 0:33:42 | |
and you really get a feeling it's a planet. | 0:33:42 | 0:33:46 | |
I know what Galileo thought when he said that the planet had ears. | 0:33:47 | 0:33:52 | |
He didn't have one of these telescopes, though. | 0:33:52 | 0:33:55 | |
And I can see one, two, three, | 0:33:55 | 0:33:59 | |
four, five moons around the planet. | 0:33:59 | 0:34:04 | |
It's just incredibly beautiful. | 0:34:04 | 0:34:06 | |
Seen like this, it's easy to appreciate how Saturn | 0:34:10 | 0:34:14 | |
is like a mini-solar system with the moons orbiting like planets around the sun. | 0:34:14 | 0:34:21 | |
From Earth we can only see a few of the larger moons. | 0:34:21 | 0:34:24 | |
But in total, Saturn has more than 60 moons, | 0:34:26 | 0:34:30 | |
and seen close up, they are a weird and wonderful bunch. | 0:34:30 | 0:34:34 | |
Dione is typical of Saturn's icy moons. | 0:34:36 | 0:34:39 | |
It looks similar to our own moon but its composition is very different. | 0:34:39 | 0:34:45 | |
It's about two-thirds water but the surface temperature is minus | 0:34:45 | 0:34:50 | |
190 degrees Celsius, and at those temperatures, the surface behaves pretty much like solid rock. | 0:34:50 | 0:34:57 | |
Iapetus is known as the yin and yang moon, | 0:35:00 | 0:35:04 | |
one half clean ice, | 0:35:04 | 0:35:07 | |
the other coated in black, dusty deposits. | 0:35:07 | 0:35:11 | |
The giant moon, Titan, is bigger than the planet Mercury. | 0:35:17 | 0:35:20 | |
But the unique thing about Titan | 0:35:20 | 0:35:23 | |
is this atmosphere which is four times as dense as the Earth's. | 0:35:23 | 0:35:29 | |
It's rich in organic molecules and it's thought that the chemistry | 0:35:29 | 0:35:32 | |
is very similar to that of the primordial Earth before life began. | 0:35:32 | 0:35:38 | |
And Hyperion is a moon unlike any other. | 0:35:42 | 0:35:47 | |
It's not even round and its battered surface has the texture of a sponge. | 0:35:47 | 0:35:51 | |
And one theory for that is that it's actually a captured comet | 0:35:56 | 0:36:00 | |
that has drifted in from the distant reaches of the solar system and been captured by Saturn's gravity. | 0:36:00 | 0:36:07 | |
But the moons of Saturn aren't just a celestial freak show. | 0:36:09 | 0:36:13 | |
They're the driving force behind the beauty and structure of the rings. | 0:36:13 | 0:36:19 | |
The most remarkable of them is hidden in one of the outer rings. | 0:36:24 | 0:36:29 | |
Buried in the heart of the E-ring is a moon that is rapidly becoming | 0:36:29 | 0:36:34 | |
one of the most fascinating places in the solar system - Enceladus. | 0:36:34 | 0:36:40 | |
Enceladus has long been an astronomical curiosity | 0:36:42 | 0:36:46 | |
because it's the most reflective object in the solar system, | 0:36:46 | 0:36:50 | |
but we've known little about it because Enceladus is tiny, | 0:36:50 | 0:36:55 | |
only 400 kilometres across, and over a billion kilometres away. | 0:36:55 | 0:37:02 | |
It's only now we have these amazing images from Cassini | 0:37:02 | 0:37:05 | |
that we can see just how strange it is. | 0:37:05 | 0:37:10 | |
Its heavily cratered northern hemisphere looks like any other icy moon, | 0:37:10 | 0:37:15 | |
but the southern hemisphere tells a very different story. | 0:37:15 | 0:37:19 | |
It's almost completely free from craters, | 0:37:19 | 0:37:22 | |
which means that the surface is probably newly formed. | 0:37:22 | 0:37:27 | |
It's scarred by canyons and riven by cracks. | 0:37:27 | 0:37:31 | |
It all looks remarkably similar to the geology of Earth, but carved in ice rather than rock. | 0:37:31 | 0:37:38 | |
And right over the South Pole are the Tiger Stripes, | 0:37:41 | 0:37:45 | |
four parallel trenches over 130 kilometres long, and possibly hundreds of metres deep. | 0:37:45 | 0:37:52 | |
They look just like tectonic fault lines. | 0:37:54 | 0:37:56 | |
This is what tectonic faults look like on Earth. | 0:38:07 | 0:38:10 | |
This is the continental divide in Iceland where the American and European plates are spreading apart. | 0:38:12 | 0:38:19 | |
The cliffs at the edge of the plates look out over a plain of new crust | 0:38:21 | 0:38:26 | |
formed from molten lava pushing up from the centre of the Earth. | 0:38:26 | 0:38:31 | |
Carolyn Porco, head of the Cassini imaging team, | 0:38:40 | 0:38:44 | |
thinks that something similar may be happening on Enceladus. | 0:38:44 | 0:38:48 | |
It is one of the most unique places in all the solar system and you can tell that just by looking at it. | 0:38:50 | 0:38:56 | |
And we think that it's possible that there is something similar | 0:38:56 | 0:39:00 | |
to what's happening right here, where you might get slushy ice, | 0:39:00 | 0:39:03 | |
viscous ice that comes up through the cracks, OK? | 0:39:03 | 0:39:07 | |
And creates more surface ice, the way you get more crust created right here, | 0:39:07 | 0:39:12 | |
pushing things out to the side and it's buckling by the time it gets to what is now the mountains. | 0:39:12 | 0:39:17 | |
So it really is similar to Iceland actually where you're getting lava | 0:39:17 | 0:39:21 | |
welling up from the surface and creating new land, so in the same way you've got ice? | 0:39:21 | 0:39:26 | |
We think. In fact it gives us an indication of just how this whole system down there may be working. | 0:39:26 | 0:39:32 | |
The next clue that something was happening under the surface | 0:39:33 | 0:39:37 | |
came when Cassini flew directly over the South Pole. | 0:39:37 | 0:39:42 | |
Thermal readings showed hot spots under the Tiger Stripes. | 0:39:42 | 0:39:46 | |
For some reason, the stripes were much hotter than the rest of the moon. | 0:39:46 | 0:39:51 | |
Cassini has found the unthinkable. | 0:39:51 | 0:39:54 | |
It's found that this southern tip of Enceladus is excessively warm. | 0:39:54 | 0:39:59 | |
There's more heat coming out of the south polar cap, if you will, | 0:39:59 | 0:40:03 | |
of Enceladus than is coming out of the equatorial regions. | 0:40:03 | 0:40:06 | |
It would be like saying there's more heat coming out of Antarctica than the Equator on Earth. | 0:40:06 | 0:40:11 | |
Then, one day in November 2005, | 0:40:11 | 0:40:14 | |
Cassini photographed Enceladus just as the sun was setting behind it. | 0:40:14 | 0:40:19 | |
What it saw became one of the most remarkable discoveries ever made in the outer solar system. | 0:40:22 | 0:40:29 | |
The backlit images reveal giant fountains erupting from the South Pole, | 0:40:29 | 0:40:36 | |
volcanoes blasting out ice instead of rock. | 0:40:36 | 0:40:41 | |
And those images blew everybody away. | 0:40:41 | 0:40:43 | |
I mean that was like game over, you know! | 0:40:43 | 0:40:46 | |
Here you have these dozen or more narrow jets and they just look ghostly and fantastic. | 0:40:46 | 0:40:54 | |
Just a few miles away from the continental divide | 0:40:57 | 0:41:00 | |
is an area that can help us understand the ice fountains. | 0:41:00 | 0:41:04 | |
This is one of Earth's hot spots where the volcanic heat of | 0:41:06 | 0:41:11 | |
the planet's core bubbles up to just below the surface. | 0:41:11 | 0:41:15 | |
Until a few years ago, Enceladus was thought to be an | 0:41:15 | 0:41:18 | |
unremarkable world, a small frozen barren lump of rock and ice. | 0:41:18 | 0:41:25 | |
But those fountains of ice erupting thousands of kilometres out into space mean that there's something | 0:41:25 | 0:41:31 | |
incredibly interesting going on beneath its surface. | 0:41:31 | 0:41:34 | |
It's here we find the Earthly phenomenon most like the ice fountains... | 0:41:45 | 0:41:49 | |
..geysers. | 0:41:52 | 0:41:54 | |
They form when underground pockets of water suddenly boil | 0:41:55 | 0:41:58 | |
and explode into the air. | 0:41:58 | 0:42:01 | |
Geysers on Earth require three things. | 0:42:10 | 0:42:14 | |
They require a ready source of water, | 0:42:14 | 0:42:17 | |
they require an intense source of heat just below the surface | 0:42:18 | 0:42:22 | |
and they need just the right geological plumbing. | 0:42:22 | 0:42:25 | |
So if the geysers on Enceladus are similar, then that raises the | 0:42:25 | 0:42:29 | |
intriguing possibility that there's an ocean of liquid water beneath the surface of the moon and it | 0:42:29 | 0:42:36 | |
raises a very interesting question because Enceladus is far too small | 0:42:36 | 0:42:40 | |
to have retained any meaningful source of heat at its core, so where does that heat come from? | 0:42:40 | 0:42:46 | |
On Earth, the geysers are driven by the intense temperatures inside the | 0:42:54 | 0:42:58 | |
planet, hot enough to melt rock and power volcanoes. | 0:42:58 | 0:43:03 | |
But Enceladus is so tiny that its core should be frozen solid. | 0:43:07 | 0:43:13 | |
Enceladus must be getting its heat from somewhere else, and it's | 0:43:15 | 0:43:20 | |
thought that it might come from its peculiar orbit around Saturn. | 0:43:20 | 0:43:26 | |
So the next thing to investigate was whether or not you could have, | 0:43:27 | 0:43:31 | |
what we call, tidal forces flex Enceladus, | 0:43:31 | 0:43:36 | |
and that simply arises because the orbit of Enceladus is eccentric, meaning it's elliptical, | 0:43:36 | 0:43:41 | |
out of round, and as it encircles Saturn in its orbit, | 0:43:41 | 0:43:45 | |
it gets close to Saturn and then far away, close and far away, | 0:43:45 | 0:43:49 | |
and the gravitational pull changes as it moves in its orbit | 0:43:49 | 0:43:53 | |
so that means the body's flexing and, if it's flexing, | 0:43:53 | 0:43:56 | |
it means it's undergoing friction inside this. | 0:43:56 | 0:43:58 | |
This is a major process for injecting energy that turns into heat into a body like Enceladus. | 0:43:58 | 0:44:05 | |
As Enceladus orbits, Saturn's gravity actually distorts the shape of the moon. | 0:44:07 | 0:44:13 | |
It's thought that this heats the interior of the moon just enough | 0:44:13 | 0:44:17 | |
to melt a small underground ocean of water. | 0:44:17 | 0:44:22 | |
As it contacts the vacuum of space, that water vaporises and explodes out | 0:44:22 | 0:44:28 | |
of the moon creating this wonder of the solar system. | 0:44:28 | 0:44:32 | |
These geysers are incredibly impressive natural phenomena | 0:44:39 | 0:44:44 | |
but they pale into insignificance compared to the ice fountains of Enceladus. | 0:44:44 | 0:44:50 | |
It's so cool. | 0:44:53 | 0:44:54 | |
While this geyser erupts every few minutes, blasting boiling water 20 metres into the air... | 0:44:58 | 0:45:04 | |
..on Enceladus the plumes are thought to be erupting constantly. | 0:45:07 | 0:45:12 | |
For them, the sky is the limit. | 0:45:12 | 0:45:14 | |
Bursting through the surface at 1,300 kilometres an hour, | 0:45:22 | 0:45:26 | |
they soar up into space for thousands of kilometres. | 0:45:26 | 0:45:30 | |
They must be one of the most impressive sights in the solar system. | 0:45:31 | 0:45:36 | |
Any liquid water instantly freezes into tiny ice crystals. | 0:45:37 | 0:45:42 | |
Some of it falls back onto the surface, giving the moon its reflective icy sheen. | 0:45:42 | 0:45:47 | |
But the rest keeps going all the way round Saturn. | 0:45:49 | 0:45:53 | |
The ice fountains are creating one of Saturn's rings as we watch. | 0:45:53 | 0:45:59 | |
The whole E-ring is made from pieces of Enceladus. | 0:45:59 | 0:46:04 | |
But Enceladus is not the only moon that shapes the rings. | 0:46:06 | 0:46:10 | |
Saturn's other moons also play a crucial role in creating these | 0:46:12 | 0:46:16 | |
beautiful patterns and they do so in mysterious ways. | 0:46:16 | 0:46:22 | |
The Sahara desert may seem an unlikely place to come to explain Saturn's rings, | 0:46:38 | 0:46:44 | |
but the behaviour of the sand in the desert can help us understand how the moons form the patterns in the rings. | 0:46:44 | 0:46:51 | |
At first sight the Sahara desert seems an immensely chaotic place, | 0:46:55 | 0:47:00 | |
just billions of grains of sand being blown randomly around by the desert winds but actually, | 0:47:00 | 0:47:07 | |
look a little bit closer, and you start to see an immense amount of order. | 0:47:07 | 0:47:12 | |
There are sand dunes as far as the eye can see, | 0:47:12 | 0:47:16 | |
and a remarkable thing is that the angles of the front | 0:47:16 | 0:47:21 | |
of all the sand dunes are exactly the same. | 0:47:21 | 0:47:24 | |
Now in the Sahara, the emergence of that order is driven by the desert | 0:47:24 | 0:47:29 | |
winds blowing always in the same direction, | 0:47:29 | 0:47:33 | |
day after day, year after year, moving the sand around. | 0:47:33 | 0:47:37 | |
In the Saturnian system, the order and beauty and intricacy | 0:47:37 | 0:47:42 | |
of the rings is driven obviously not by wind, | 0:47:42 | 0:47:46 | |
but by a different force, the force of gravity. | 0:47:46 | 0:47:49 | |
As the moons orbit Saturn, their gravitational influence sweeps through the rings. | 0:47:56 | 0:48:02 | |
In these amazing images, we can actually watch the moons as they work. | 0:48:06 | 0:48:12 | |
We can see gravity in action. | 0:48:14 | 0:48:17 | |
As the moons pass close to the rings, their gravitational pull | 0:48:17 | 0:48:21 | |
tugs the ring particles towards them, distorting the shape of the rings. | 0:48:21 | 0:48:27 | |
The F-ring, one of the outer rings, is twisted into a spiral shape | 0:48:28 | 0:48:34 | |
by two moons, Prometheus and Pandora. | 0:48:34 | 0:48:38 | |
In this video taken by Cassini, you can see how Prometheus | 0:48:38 | 0:48:42 | |
drags plumes of material away as it passes close to the rings. | 0:48:42 | 0:48:47 | |
These short-range gravitational effects account for many of the patterns in the rings. | 0:48:49 | 0:48:55 | |
But sometimes the moons can exert their pull over much greater distances, | 0:48:58 | 0:49:05 | |
and the way they do so reveals the subtlety with which gravity can work. | 0:49:05 | 0:49:11 | |
Well, here's a model of the Saturnian system with Saturn in the middle | 0:49:14 | 0:49:19 | |
and the magnificent ring system going around the outside, | 0:49:19 | 0:49:23 | |
and the first thing you notice when you look at the rings is a huge gap called the Cassini division. | 0:49:23 | 0:49:29 | |
Now what could possibly have caused that? | 0:49:29 | 0:49:32 | |
Well, it's all down to one of Saturn's moons called Mimas | 0:49:32 | 0:49:37 | |
which orbits well outside the ring system. | 0:49:37 | 0:49:40 | |
And how could something that far outside the rings | 0:49:40 | 0:49:43 | |
have any influence at all on the particles inside the rings? | 0:49:43 | 0:49:47 | |
Well, it's all down to a phenomena called orbital resonance. | 0:49:47 | 0:49:51 | |
Now the particles in the Cassini division have an interesting relationship with the moon, Mimas | 0:49:51 | 0:49:56 | |
because they orbit around Saturn twice for every single | 0:49:56 | 0:50:00 | |
orbit of Mimas, and that has an interesting consequence. | 0:50:00 | 0:50:04 | |
Imagine there's a particle inside the Cassini division. | 0:50:04 | 0:50:08 | |
Then every second year for this particle they meet up with Mimas. | 0:50:08 | 0:50:14 | |
They end up in the same place in space and that means that this particle will get a kick | 0:50:14 | 0:50:21 | |
or a tug from Mimas's gravity on a regular basis, every second year. | 0:50:21 | 0:50:26 | |
Bang, bang, bang! And that alters the orbit of anything that's in | 0:50:26 | 0:50:31 | |
the Cassini division, and actually has the effect of throwing it out, of clearing a gap in the rings. | 0:50:31 | 0:50:37 | |
And in fact, much of the complex and beautiful structure of Saturn's rings | 0:50:37 | 0:50:43 | |
is down to these orbital resonances, | 0:50:43 | 0:50:46 | |
not only with Mimas, but with one or more of the 61 known | 0:50:46 | 0:50:52 | |
moons of Saturn that orbit outside, and indeed some inside, the rings. | 0:50:52 | 0:50:58 | |
And for me, that's part of the wonder of Saturn's rings. | 0:51:08 | 0:51:12 | |
Their beauty is such a good illustration of how gravity can carve order out of chaos. | 0:51:12 | 0:51:19 | |
But more than that, understanding how Saturn's moons shape the rings | 0:51:23 | 0:51:28 | |
can shed light on the events that shaped the early solar system, | 0:51:28 | 0:51:33 | |
events that helped create the world we live in. | 0:51:33 | 0:51:36 | |
Resonance can be much more than a delicate sculptor | 0:51:38 | 0:51:42 | |
because it's not only small moons that can enter orbital resonance. | 0:51:42 | 0:51:46 | |
It's now thought that billions of years ago the two giants of the solar system, Jupiter and Saturn, | 0:51:46 | 0:51:52 | |
entered a resonance and that unleashed forces that could move entire planets, | 0:51:52 | 0:51:57 | |
and that made the solar system an incredibly turbulent and violent place. | 0:51:57 | 0:52:03 | |
The solar system is full of craters, the record of a long history of cataclysmic impacts. | 0:52:09 | 0:52:16 | |
But there was one period 3.6 billion years ago | 0:52:24 | 0:52:28 | |
when the whole solar system was turned inside out | 0:52:28 | 0:52:32 | |
by the same forces of orbital resonance that shaped Saturn's rings. | 0:52:32 | 0:52:37 | |
We now believe that the giant planets formed much closer to the sun than they are today. | 0:52:40 | 0:52:46 | |
Their orbits drifted for hundreds of millions of years | 0:52:49 | 0:52:53 | |
until Jupiter and Saturn fell into a resonant pattern. | 0:52:53 | 0:52:58 | |
Once every cycle, the two planets aligned in exactly the same spot, | 0:52:58 | 0:53:03 | |
creating a gravitational surge | 0:53:03 | 0:53:07 | |
that played havoc with the orbits of all the planets. | 0:53:07 | 0:53:11 | |
Neptune was catapulted outwards and smashed into the ring of comets | 0:53:11 | 0:53:16 | |
surrounding the solar system, with dramatic consequences. | 0:53:16 | 0:53:20 | |
For a hundred million years, the solar system turned into | 0:53:27 | 0:53:31 | |
a shooting gallery as a rain of comets ploughed through it. | 0:53:31 | 0:53:36 | |
Millions of comets were scattered in all directions, peppering the planets. | 0:53:39 | 0:53:45 | |
It was called the Late Heavy Bombardment. | 0:53:45 | 0:53:48 | |
It created many of the craters we see throughout the solar system today. | 0:53:53 | 0:53:59 | |
It left scars all over our moon... | 0:53:59 | 0:54:03 | |
..and it had a lasting impact on the Earth as well. | 0:54:04 | 0:54:08 | |
The only impact craters we see on Earth today, | 0:54:12 | 0:54:14 | |
like this one in Arizona, were made much more recently, | 0:54:14 | 0:54:18 | |
but they reveal the scale of these impacts. | 0:54:18 | 0:54:22 | |
Now today, impacts like this are relatively rare, | 0:54:29 | 0:54:33 | |
although they will happen again, | 0:54:33 | 0:54:34 | |
but during the Late Heavy Bombardment, | 0:54:34 | 0:54:37 | |
the Earth was hit by thousands of objects with sizes | 0:54:37 | 0:54:40 | |
far in excess of the object that made this crater, | 0:54:40 | 0:54:43 | |
and the environment was changed radically and dramatically. | 0:54:43 | 0:54:47 | |
But those changes weren't necessarily catastrophic because it's now thought | 0:54:47 | 0:54:53 | |
that a significant amount of the water in the Earth's oceans was delivered by the impacts of | 0:54:53 | 0:54:58 | |
water-rich comets and other objects during the Late Heavy Bombardment, | 0:54:58 | 0:55:04 | |
and that means that impacts could have played a key role in the development of life on Earth. | 0:55:04 | 0:55:11 | |
Before the Late Heavy Bombardment, the Earth was a barren rock. | 0:55:16 | 0:55:21 | |
Afterwards, it supported the oceans that would become the crucible for life. | 0:55:25 | 0:55:30 | |
Without the water delivered in the Late Heavy Bombardment, life on Earth may never have evolved. | 0:55:41 | 0:55:48 | |
It's quite a thought that all this may have | 0:55:53 | 0:55:57 | |
been caused by the violent resonances generated by the orbiting planets. | 0:55:57 | 0:56:02 | |
The story of the solar system is the story of the creation of order out of chaos. | 0:56:08 | 0:56:14 | |
The planets and their moons were created by the same universal laws, | 0:56:15 | 0:56:20 | |
the delicate interaction between gravity and angular momentum | 0:56:20 | 0:56:25 | |
that led to the spinning patterns we see around us today. | 0:56:25 | 0:56:28 | |
Ultimately, that journey created the finest example of those forces in action... | 0:56:38 | 0:56:45 | |
..because, in creating the solar system, | 0:56:47 | 0:56:50 | |
those forces that sculpted order out of chaos also created | 0:56:50 | 0:56:55 | |
the best and most beautiful laboratory for studying how the solar system works - Saturn's rings. | 0:56:55 | 0:57:02 | |
It's often the case in science that answers to the most profound | 0:57:12 | 0:57:16 | |
questions can come from the most unexpected of places. | 0:57:16 | 0:57:20 | |
Saturn's rings were initially studied because of their beauty, but understanding | 0:57:20 | 0:57:25 | |
their formation and evolution has led to a deep understanding | 0:57:25 | 0:57:30 | |
of how form and beauty and order can emerge from violence and chaos. | 0:57:30 | 0:57:35 | |
And that understanding can be spread across the entire solar system | 0:57:35 | 0:57:40 | |
and remember that you and me are part of the solar system. | 0:57:40 | 0:57:44 | |
You and me are ordered structures formed from the chaos | 0:57:44 | 0:57:48 | |
of the primordial dust cloud 4.5 billion years ago, | 0:57:48 | 0:57:53 | |
and that is one of the wonders of the solar system. | 0:57:53 | 0:57:56 | |
Subtitles by Red Bee Media Ltd | 0:58:24 | 0:58:26 | |
E-mail [email protected] | 0:58:26 | 0:58:28 |