Browse content similar to Dead or Alive. Check below for episodes and series from the same categories and more!
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We live on a world of wonders, | 0:00:06 | 0:00:10 | |
a place of astonishing beauty and complexity. | 0:00:10 | 0:00:15 | |
We have vast oceans, incredible weather, | 0:00:17 | 0:00:22 | |
giant mountains and spectacular landscapes. | 0:00:22 | 0:00:26 | |
If you think that this | 0:00:26 | 0:00:28 | |
is all there is, that our planet exists in magnificent isolation, | 0:00:28 | 0:00:33 | |
then you're wrong. | 0:00:33 | 0:00:34 | |
We're part of a much wider ecosystem that extends way beyond | 0:00:35 | 0:00:40 | |
the top of our atmosphere. | 0:00:40 | 0:00:42 | |
I think we're living through the greatest age of discovery our civilisation has known. | 0:00:47 | 0:00:53 | |
We've voyaged to the farthest reaches of the solar system. | 0:00:53 | 0:00:57 | |
We've photographed strange new worlds, | 0:00:57 | 0:01:01 | |
stood in unfamiliar landscapes, tasted alien air. | 0:01:01 | 0:01:05 | |
Now, the laws of physics are simple and they're universal. | 0:01:08 | 0:01:13 | |
What applies here applies everywhere else up there. | 0:01:13 | 0:01:17 | |
But it's fascinating that they can manifest themselves | 0:01:18 | 0:01:22 | |
in so many different ways across the solar system. | 0:01:22 | 0:01:26 | |
In this programme, I'm going to look at how the universal forces of nature | 0:01:27 | 0:01:33 | |
that created all this can also wreak devastation across the solar system. | 0:01:33 | 0:01:39 | |
How they can be the death of a planet... | 0:01:41 | 0:01:44 | |
..and how they can keep other worlds alive. | 0:01:46 | 0:01:50 | |
I can just see pieces of molten rock rising up just below my chin. | 0:01:56 | 0:02:01 | |
These forces are so far reaching, they bridge the depths of space | 0:02:04 | 0:02:09 | |
and transform a world long thought dead | 0:02:09 | 0:02:12 | |
into a world of perpetual change and everlasting youth. | 0:02:12 | 0:02:17 | |
The intense source of heat that powers that eternal change also | 0:02:18 | 0:02:24 | |
drives one of the most spectacular sights in the solar system. | 0:02:24 | 0:02:28 | |
I've come to one of Earth's natural wonders, | 0:03:17 | 0:03:22 | |
the Grand Canyon in Arizona. | 0:03:22 | 0:03:25 | |
It's a place to be humbled by nature. | 0:03:28 | 0:03:32 | |
Well, this is undoubtedly | 0:03:34 | 0:03:36 | |
one of the most beautiful places I've seen on Earth. | 0:03:36 | 0:03:39 | |
From sunrise to sunset, | 0:03:41 | 0:03:43 | |
the changing light brings this immense landscape to life. | 0:03:43 | 0:03:49 | |
I hear stories of people coming here at sunrise with tears in their eyes | 0:03:49 | 0:03:53 | |
at the majesty of the view, and I can see why. | 0:03:53 | 0:03:56 | |
It's incredible to think that this enormous valley | 0:04:00 | 0:04:03 | |
was etched and carved | 0:04:03 | 0:04:05 | |
by the action of running water over just a few million years. | 0:04:05 | 0:04:10 | |
Our knowledge of natural wonders like the Grand Canyon | 0:04:14 | 0:04:17 | |
was once limited to our own planet. | 0:04:17 | 0:04:20 | |
But the space age has brought new worlds into view. | 0:04:22 | 0:04:27 | |
This is Mars, the Red Planet. | 0:04:33 | 0:04:36 | |
Fourth rock out from the sun, it has a canyon so vast | 0:04:36 | 0:04:41 | |
you could fit our own Grand Canyon into one of its side channels. | 0:04:41 | 0:04:44 | |
Named after the space probe that first saw it, | 0:04:50 | 0:04:53 | |
this is the Valles Marineris. | 0:04:53 | 0:04:56 | |
8km deep and over 3,000km long, | 0:05:00 | 0:05:06 | |
on Earth it would run all the way from Los Angeles to New York. | 0:05:06 | 0:05:10 | |
We're beginning to get a deep and quite profound understanding | 0:05:17 | 0:05:22 | |
of the way that Mars has evolved geologically because | 0:05:22 | 0:05:26 | |
we are now there, because we now have eyes and ears on the surface. | 0:05:26 | 0:05:30 | |
And there really is no substitute for actual exploration, for actually | 0:05:30 | 0:05:35 | |
going somewhere and touching it and taking pictures of it. | 0:05:35 | 0:05:38 | |
Look at this picture. | 0:05:42 | 0:05:44 | |
This is a picture of a sunset. | 0:05:45 | 0:05:48 | |
These are pictures of clouds. | 0:05:49 | 0:05:50 | |
It's amazing to think these incredibly familiar-looking photographs | 0:05:53 | 0:05:57 | |
were taken on the surface of Mars. | 0:05:57 | 0:06:00 | |
This picture, | 0:06:02 | 0:06:03 | |
or this amazing colour picture... | 0:06:03 | 0:06:06 | |
I could have got a camera here and just snapped any picture | 0:06:06 | 0:06:09 | |
and it would have looked exactly like this one. | 0:06:09 | 0:06:12 | |
In the Grand Canyon, you can see the Colorado River | 0:06:12 | 0:06:15 | |
running in the bottom of the valley | 0:06:15 | 0:06:17 | |
so you can understand how this landscape was made. | 0:06:17 | 0:06:20 | |
Whereas here on Mars, there's no sign of any water. | 0:06:20 | 0:06:23 | |
So Mars is a puzzling place. | 0:06:24 | 0:06:28 | |
Despite all the similarities between Mars and Earth, | 0:06:31 | 0:06:34 | |
it's the differences between these two planets that are most telling. | 0:06:34 | 0:06:39 | |
Mars is now a desolate dead wasteland, | 0:06:39 | 0:06:43 | |
a world where the processes that sculpted its familiar landscapes | 0:06:43 | 0:06:47 | |
seized up long ago. | 0:06:47 | 0:06:49 | |
It's fascinating for me as a physicist to see how | 0:06:53 | 0:06:56 | |
the same basic simple laws of nature can play out | 0:06:56 | 0:07:02 | |
in such radically different ways, and produce such astonishingly | 0:07:02 | 0:07:08 | |
varied and beautiful and violent and dead worlds | 0:07:08 | 0:07:14 | |
out there, across the solar system. | 0:07:14 | 0:07:17 | |
The Big Island of Hawaii, in the middle of the Pacific Ocean, | 0:07:36 | 0:07:40 | |
holds the key to what happened to Mars. | 0:07:40 | 0:07:42 | |
This is the perfect place to witness how a planet can be kept alive | 0:07:44 | 0:07:48 | |
by nothing more than the simple flow of heat. | 0:07:48 | 0:07:52 | |
You can smell the volcanic ash coming into the... | 0:07:55 | 0:07:58 | |
into the helicopter. And everywhere you look, it looks like a... | 0:07:58 | 0:08:02 | |
It's almost like an apocalyptic scene. | 0:08:02 | 0:08:05 | |
This volcano is Kilauea, which means spewing. | 0:08:08 | 0:08:13 | |
It's been erupting almost continuously since 1983. | 0:08:13 | 0:08:18 | |
In fact, you can see molten rock flowing down the side | 0:08:18 | 0:08:22 | |
of the mountain just cutting a swathe through the trees. | 0:08:22 | 0:08:25 | |
This might look like widespread destruction, | 0:08:27 | 0:08:31 | |
but volcanic eruptions are Earth's geological heartbeat. | 0:08:31 | 0:08:35 | |
Active volcanoes make our planet a vibrant, living world. | 0:08:35 | 0:08:40 | |
That is the most spectacular demonstration | 0:08:40 | 0:08:43 | |
of our planet being geologically alive that I've ever seen. | 0:08:43 | 0:08:47 | |
A few kilometres north of Kilauea, | 0:08:56 | 0:08:58 | |
you can see just what volcanic action can produce, | 0:08:58 | 0:09:02 | |
given enough time. | 0:09:02 | 0:09:03 | |
The islands of Hawaii were built entirely by volcanoes. | 0:09:06 | 0:09:12 | |
Today, these mountains are the largest volcanoes on our planet, | 0:09:12 | 0:09:18 | |
and we've seen landscapes just like this, on Mars. | 0:09:18 | 0:09:22 | |
It's quite an experience being 4km high. | 0:09:26 | 0:09:29 | |
It makes you out of breath and you sniff a lot because your nose becomes... | 0:09:29 | 0:09:34 | |
And makes you feel like you've had a few drinks. | 0:09:34 | 0:09:36 | |
This is Mauna Kea, | 0:09:38 | 0:09:39 | |
one of the five volcanoes that make up the Big Island of Hawaii. | 0:09:39 | 0:09:43 | |
I've known about it since I was very little | 0:09:43 | 0:09:45 | |
because it's one of the most famous observatories on the planet. | 0:09:45 | 0:09:48 | |
Everywhere you look, surrounded by our eyes to the cosmos. | 0:09:48 | 0:09:55 | |
Although this mountain is 4km above the surface of the Pacific, | 0:09:55 | 0:09:59 | |
it's actually 10km above the surface of the Pacific floor. | 0:09:59 | 0:10:04 | |
That makes it the highest mountain on Earth, | 0:10:04 | 0:10:07 | |
over a kilometre higher than Mount Everest. | 0:10:07 | 0:10:09 | |
But it is a tiny volcano compared to the biggest volcano on the surface of Mars. | 0:10:09 | 0:10:17 | |
This is Olympus Mons, | 0:10:28 | 0:10:30 | |
named after Mount Olympus, the mythical home of the Greek gods. | 0:10:30 | 0:10:35 | |
This vast outpouring of lava stretches over 550km across, | 0:10:35 | 0:10:43 | |
but it's the height of this volcano that is breathtaking. | 0:10:43 | 0:10:46 | |
It soars 25km into the Martian sky, | 0:10:48 | 0:10:52 | |
nearly three times the full height of Mauna Kea. | 0:10:52 | 0:10:57 | |
But Olympus Mons isn't just the tallest volcano in the solar system, | 0:10:57 | 0:11:02 | |
it's the highest mountain we know. | 0:11:02 | 0:11:05 | |
There are striking similarities between the volcanic landscapes | 0:11:07 | 0:11:11 | |
here on Hawaii and the giant volcanoes found on Mars. | 0:11:11 | 0:11:15 | |
These similarities can be traced back billions of years | 0:11:15 | 0:11:20 | |
to the fiery birth of the solar system. | 0:11:20 | 0:11:22 | |
All this heat you can see driving this spectacular volcanic activity | 0:11:25 | 0:11:30 | |
is a relic, a hangover of the Earth's formation. | 0:11:30 | 0:11:33 | |
Now, all the rocky planets - Earth, Mars, Venus, Mercury - were formed in the same way. | 0:11:33 | 0:11:40 | |
They came from a collapsing dust cloud over 4.5 billion years ago. | 0:11:40 | 0:11:46 | |
With the ignition of the sun, our solar system was born. | 0:11:53 | 0:11:57 | |
Little by little, the rocky bodies grew, | 0:11:59 | 0:12:02 | |
falling together under their own gravity. | 0:12:02 | 0:12:05 | |
This process not only generated immense amounts of heat, | 0:12:05 | 0:12:09 | |
it also delivered radioactive material to the cores. | 0:12:09 | 0:12:13 | |
These two ancient sources of heat power Earth's volcanoes to this day, | 0:12:17 | 0:12:24 | |
but the volcanoes on Mars are little more than a petrified memory of a distant past. | 0:12:24 | 0:12:31 | |
When we look down on the surface of Mars, | 0:12:31 | 0:12:34 | |
we see no evidence of this kind of volcanic activity. | 0:12:34 | 0:12:37 | |
As far as we can tell, Mars is a dead world. | 0:12:37 | 0:12:41 | |
Mars must have had similar inner heat to Earth to build its volcanoes. | 0:12:43 | 0:12:48 | |
Yet something obviously happened | 0:12:48 | 0:12:51 | |
to stop the Red Planet's geological heartbeat. | 0:12:51 | 0:12:54 | |
Now, as everyone who's left a hot cup of tea sat on the kitchen table knows, | 0:12:56 | 0:13:00 | |
hot things lose heat to their cooler surroundings, | 0:13:00 | 0:13:04 | |
and what's true for cups of tea, in physics is also true for planets. | 0:13:04 | 0:13:09 | |
This is hot and that up there - space - is cold. | 0:13:09 | 0:13:15 | |
So planets lose heat to space. | 0:13:15 | 0:13:17 | |
Mars is a much smaller planet than the Earth. | 0:13:21 | 0:13:23 | |
It's about half the diameter, it's an eighth of the volume, | 0:13:23 | 0:13:29 | |
so there was much less heat trapped in there to begin with. | 0:13:29 | 0:13:33 | |
Now, planets lose heat to space through their surfaces, | 0:13:33 | 0:13:37 | |
and smaller things have a larger surface area | 0:13:37 | 0:13:41 | |
in relation to their volume than big things. | 0:13:41 | 0:13:45 | |
So that means that Mars will lose its heat to space much quicker than the Earth does. | 0:13:45 | 0:13:51 | |
When the interior of Mars grew cold, | 0:13:55 | 0:13:58 | |
the mighty volcanoes lost their lifeblood. | 0:13:58 | 0:14:01 | |
The Red Planet's geological heart died, | 0:14:01 | 0:14:05 | |
and millions of years ago, the surface of Mars ground to a halt. | 0:14:05 | 0:14:10 | |
The fate of a whole planet was destined | 0:14:11 | 0:14:14 | |
by the simplest of laws of physics. | 0:14:14 | 0:14:17 | |
Since the dawn of human history, we've been able to gaze up into the night sky, | 0:14:31 | 0:14:37 | |
but we're lucky because we're the first generation that's been able | 0:14:37 | 0:14:40 | |
to build machines to actually go to those planets and moons. | 0:14:40 | 0:14:45 | |
And we've found that they're more beautiful, more violent, | 0:14:45 | 0:14:49 | |
more magnificent and fascinating | 0:14:49 | 0:14:51 | |
than we could have possibly imagined. | 0:14:51 | 0:14:53 | |
The more worlds we study, the more we realise | 0:14:56 | 0:14:59 | |
that our solar system is a cosmic laboratory. | 0:14:59 | 0:15:03 | |
Even the slightest differences in size or position | 0:15:03 | 0:15:07 | |
can create a world radically different from its neighbours. | 0:15:07 | 0:15:11 | |
So here on Earth, we have one beautiful manifestation of how those | 0:15:15 | 0:15:19 | |
simple laws of nature can play out, how they can build a planet. | 0:15:19 | 0:15:25 | |
In Mars we have another example. | 0:15:25 | 0:15:27 | |
What happens when you take a planet that's smaller than Earth | 0:15:27 | 0:15:31 | |
and move it further away from the sun? | 0:15:31 | 0:15:33 | |
It loses its heat more quickly and it becomes geologically inactive. | 0:15:33 | 0:15:37 | |
But what would happen if you took a planet just like the Earth | 0:15:37 | 0:15:41 | |
and moved it a little closer to the sun? | 0:15:41 | 0:15:43 | |
Well, we know of such a planet. | 0:15:46 | 0:15:49 | |
It's the brightest point of light in our night sky. | 0:15:51 | 0:15:54 | |
So similar in size to our own world, | 0:15:56 | 0:15:59 | |
this planet has been called Earth's twin. | 0:15:59 | 0:16:03 | |
This is Venus. | 0:16:05 | 0:16:06 | |
Orbiting closer to the sun, Venus was named for its shining beauty. | 0:16:08 | 0:16:14 | |
But our planetary twin hides its true identity | 0:16:16 | 0:16:20 | |
beneath a thick blanket of cloud. | 0:16:20 | 0:16:23 | |
Over the last 4.5 billion years, | 0:16:33 | 0:16:35 | |
Venus has turned into an unimaginably oppressive world. | 0:16:35 | 0:16:41 | |
The atmosphere is so dense that the pressure is crushing. | 0:16:41 | 0:16:45 | |
It's 90 times atmospheric pressure here on Earth. | 0:16:45 | 0:16:47 | |
Now, Venus takes 243 days to rotate once on its axis. | 0:16:50 | 0:16:54 | |
That means its day is longer than its year. | 0:16:54 | 0:16:58 | |
So Venus has the hottest average surface temperature, | 0:17:01 | 0:17:04 | |
other than the sun's, anywhere in the solar system - 470 Celsius. | 0:17:04 | 0:17:08 | |
I've come to India, to a place called the Deccan Traps. | 0:17:16 | 0:17:20 | |
Hidden in this lush green landscape are tantalising clues | 0:17:24 | 0:17:28 | |
to understanding how immense heat caused Venus to choke to death. | 0:17:28 | 0:17:33 | |
When you look at this landscape today, | 0:17:34 | 0:17:37 | |
it's incredibly peaceful and beautiful, rolling green hills, | 0:17:37 | 0:17:41 | |
but I think it's astonishing to think | 0:17:41 | 0:17:45 | |
that everything you see down there is lava. | 0:17:45 | 0:17:48 | |
This whole landscape, half a million square kilometres of it, was created | 0:17:48 | 0:17:53 | |
in an ongoing volcanic eruption that lasted for a million years. | 0:17:53 | 0:17:59 | |
If you take away the green foliage, the underlying landscape of lava | 0:18:01 | 0:18:06 | |
is actually very similar to what we see on Venus. | 0:18:06 | 0:18:10 | |
Using radar to peer down through the clouds, | 0:18:13 | 0:18:17 | |
the surface of Venus was finally revealed. | 0:18:17 | 0:18:20 | |
It's covered with floods of solid lava, just like we see in India, | 0:18:20 | 0:18:26 | |
but on a scale many thousands of times larger. | 0:18:26 | 0:18:30 | |
We've also counted over 50,000 volcanoes, | 0:18:30 | 0:18:34 | |
the most on any planet in the solar system. | 0:18:34 | 0:18:38 | |
Venus is a similar size to Earth, | 0:18:38 | 0:18:41 | |
so it may still have a hot geological heart | 0:18:41 | 0:18:44 | |
powering its volcanoes but as yet we haven't witnessed any eruptions. | 0:18:44 | 0:18:50 | |
The ancient floods of lava we see on Venus | 0:18:53 | 0:18:56 | |
and here in India were created in much the same way. | 0:18:56 | 0:19:00 | |
For both planets, this was volcanic activity in overdrive. | 0:19:02 | 0:19:05 | |
The eruptions here in India 65 million years ago | 0:19:05 | 0:19:09 | |
affected the Earth's climate so much that they're thought to have played | 0:19:09 | 0:19:13 | |
a major role in the mass extinction events at the end of the cretaceous period, | 0:19:13 | 0:19:17 | |
which wiped out over two-thirds of the species on Earth. | 0:19:17 | 0:19:21 | |
Now, life on Earth recovered but Venus wasn't so lucky. | 0:19:21 | 0:19:26 | |
The intense volcanic activity on both planets | 0:19:30 | 0:19:33 | |
didn't just blast out molten rock. | 0:19:33 | 0:19:35 | |
It also released copious amounts of gases, like carbon dioxide. | 0:19:35 | 0:19:42 | |
But slight differences in the way the laws of physics played out | 0:19:44 | 0:19:48 | |
on Venus helped push our cosmic twin down a path of no return. | 0:19:48 | 0:19:54 | |
Venus and Earth reacted very differently to the same kind of volcanic cataclysm, | 0:19:56 | 0:20:01 | |
and the reason for that is something that happens so often on Earth | 0:20:01 | 0:20:05 | |
that we take it for granted, and just moan about it. | 0:20:05 | 0:20:07 | |
Rain plays a significant role in keeping our planet a pleasant place to live. | 0:20:16 | 0:20:21 | |
Acting as part of a global recycling system, | 0:20:24 | 0:20:27 | |
rain keeps our atmosphere in balance, | 0:20:27 | 0:20:30 | |
washing out the potent greenhouse gas, carbon dioxide, | 0:20:30 | 0:20:35 | |
ready to be locked away in rocks in our oceans. | 0:20:35 | 0:20:39 | |
But on Venus, the laws of physics have made it impossible | 0:20:42 | 0:20:46 | |
for rainfall to cleanse its atmosphere. | 0:20:46 | 0:20:48 | |
In fact, there's no liquid water at all. | 0:20:48 | 0:20:52 | |
Venus lost its water essentially because it's hotter than the Earth. | 0:20:54 | 0:20:59 | |
You see, temperature is just a measure of how fast things are moving around. | 0:20:59 | 0:21:03 | |
So on Venus the oceans would have evaporated into the atmosphere | 0:21:03 | 0:21:07 | |
and that water in the atmosphere would be moving around | 0:21:07 | 0:21:10 | |
extremely quickly, simply because it's hot. | 0:21:10 | 0:21:13 | |
And Venus is so close to the sun and so hot, | 0:21:13 | 0:21:16 | |
those water molecules are moving so fast that the gravity of the planet | 0:21:16 | 0:21:20 | |
can't continue to hold them in the atmosphere, | 0:21:20 | 0:21:23 | |
and so they simply escape off into space. | 0:21:23 | 0:21:27 | |
With no water, there is no rain on Venus. | 0:21:30 | 0:21:34 | |
For billions of years, there has been nothing | 0:21:34 | 0:21:38 | |
to temper the build-up of volcanic gases in its atmosphere. | 0:21:38 | 0:21:42 | |
Venus ended up cocooned in a thick, high-pressure, | 0:21:45 | 0:21:50 | |
dense blanket of carbon dioxide, | 0:21:50 | 0:21:52 | |
and that made the temperature rise and rise and rise, | 0:21:52 | 0:21:57 | |
turning Venus into the hell-like world we see today. | 0:21:57 | 0:22:02 | |
Compared to scorched Venus and frozen Mars, | 0:22:15 | 0:22:18 | |
our home is a very special ball of rock. | 0:22:18 | 0:22:21 | |
Although governed by the same universal set of rules, | 0:22:23 | 0:22:27 | |
our planet is not too big, not too small, | 0:22:27 | 0:22:31 | |
not too hot, not too cold. | 0:22:31 | 0:22:36 | |
Earth has been called the Goldilocks planet | 0:22:36 | 0:22:39 | |
because everything is just right. | 0:22:39 | 0:22:41 | |
Our world is unique but it doesn't exist in splendid isolation. | 0:22:45 | 0:22:50 | |
It is intimately connected with its cosmic neighbours. | 0:22:50 | 0:22:55 | |
Earth is not the master of its own destiny and it never has been. | 0:22:55 | 0:23:01 | |
The life and death of our planet is influenced by forces | 0:23:01 | 0:23:05 | |
emanating from the very depths of space. | 0:23:05 | 0:23:08 | |
As we better understand our place in space, | 0:23:14 | 0:23:17 | |
we've come to realise that our sharing of the same physical laws | 0:23:17 | 0:23:22 | |
with the other worlds in the solar system | 0:23:22 | 0:23:24 | |
isn't the only connection we have with them, | 0:23:24 | 0:23:27 | |
because those same laws lead to a direct physical connection | 0:23:27 | 0:23:35 | |
between the Earth and the other worlds out there | 0:23:35 | 0:23:38 | |
that is subtle, is complicated, but can sometimes be extremely powerful. | 0:23:38 | 0:23:46 | |
Out in the farthest reaches of the solar system are vast worlds | 0:23:52 | 0:23:57 | |
that have a direct impact on our very existence. | 0:23:57 | 0:24:00 | |
This is our sun from ten billion kilometres away - | 0:24:04 | 0:24:09 | |
just another star in a sea of stars. | 0:24:09 | 0:24:12 | |
But as you head towards the light, you enter a realm of giants. | 0:24:12 | 0:24:17 | |
The furthest planet from the sun is icy Neptune, | 0:24:20 | 0:24:24 | |
with its thick, blue methane atmosphere. | 0:24:24 | 0:24:27 | |
Uranus comes next, the only planet that lies on its back. | 0:24:31 | 0:24:36 | |
Further in towards the sun, and the planets get even bigger. | 0:24:40 | 0:24:45 | |
Saturn, with its beautiful rings of ice. | 0:24:45 | 0:24:49 | |
Finally we reach the king of the giants - Jupiter. | 0:24:54 | 0:24:58 | |
Jupiter is the largest planet in the solar system, | 0:25:01 | 0:25:04 | |
so big you could fit Earth inside it over 1,000 times. | 0:25:04 | 0:25:10 | |
It's made up of the same stuff as our sun - hydrogen and helium - | 0:25:10 | 0:25:15 | |
the most common elements in the universe. | 0:25:15 | 0:25:18 | |
In its thick churning atmosphere, | 0:25:18 | 0:25:20 | |
gigantic storms have raged for centuries. | 0:25:20 | 0:25:24 | |
Now, astrologers have said for years that Jupiter influences our lives, | 0:25:27 | 0:25:32 | |
but we now have scientific evidence that this mighty planet does have | 0:25:32 | 0:25:37 | |
a significant connection with our own small world. | 0:25:37 | 0:25:42 | |
Jupiter is so different to our planet - | 0:25:42 | 0:25:45 | |
you know, a big ball of gas, half a billion kilometres away - | 0:25:45 | 0:25:49 | |
it's difficult to see how it could have anything to do with us at all. | 0:25:49 | 0:25:54 | |
But despite the fact that astrology is a load of rubbish, | 0:25:54 | 0:25:59 | |
Jupiter can, in fact, have a profound influence on our planet | 0:25:59 | 0:26:03 | |
and it's through a force that, well, surrounds us and penetrates us | 0:26:03 | 0:26:09 | |
and binds the galaxy together - gravity. | 0:26:09 | 0:26:13 | |
Gravity is one of the fundamental forces of nature. | 0:26:18 | 0:26:23 | |
It exists between all objects, and the effects | 0:26:23 | 0:26:26 | |
of a gravitational field extend way beyond the planet that creates it. | 0:26:26 | 0:26:32 | |
Gravity is by far the weakest force of nature. But it's the only force | 0:26:36 | 0:26:40 | |
that has an influence across the entire solar system, | 0:26:40 | 0:26:43 | |
and that's because, although it's weak, it has an infinite range. | 0:26:43 | 0:26:47 | |
It never quite goes away. | 0:26:47 | 0:26:48 | |
So, no matter how far you go, you feel the force of gravity | 0:26:48 | 0:26:53 | |
as a planet, although it drops and drops and drops away. | 0:26:53 | 0:26:57 | |
Jupiter has the most powerful gravitational field of all the planets, | 0:27:00 | 0:27:04 | |
and it's the gas giant's gravity that can directly influence | 0:27:04 | 0:27:09 | |
the orbits of asteroids and other wandering space debris. | 0:27:09 | 0:27:14 | |
Jupiter is so massive, by far the most massive planet in the solar system, | 0:27:15 | 0:27:19 | |
that its gravitational field can have a profound influence on passing interplanetary stuff. | 0:27:19 | 0:27:25 | |
It can do three things. | 0:27:25 | 0:27:26 | |
Firstly, it can capture the stuff, literally hoover it up. | 0:27:26 | 0:27:30 | |
Secondly, it can deflect the stuff, | 0:27:30 | 0:27:33 | |
such that it throws it out of the solar system. | 0:27:33 | 0:27:36 | |
But thirdly, and most importantly for us, | 0:27:36 | 0:27:39 | |
it can deflect stuff onto a direct collision course with our planet. | 0:27:39 | 0:27:45 | |
Influenced by Jupiter's gravity, | 0:27:52 | 0:27:55 | |
today, right now, we're highly vulnerable from asteroid impacts. | 0:27:55 | 0:28:00 | |
But we do have sentinels standing guard. | 0:28:01 | 0:28:04 | |
On top of the mountain of Heleakala on the Hawaiian honeymoon island of Maui, | 0:28:07 | 0:28:12 | |
I've come to see Professor Nick Kaiser, who's searching | 0:28:12 | 0:28:16 | |
our solar system for potentially hostile space debris. | 0:28:16 | 0:28:20 | |
The prime task is to try and find killer asteroids, | 0:28:22 | 0:28:26 | |
things that are out there in the solar system | 0:28:26 | 0:28:28 | |
that might hit the Earth. | 0:28:28 | 0:28:30 | |
There's an air of Hollywood about it, isn't there, in some sense? | 0:28:30 | 0:28:33 | |
Well, that's right. I would say a lot more resources have been spent | 0:28:33 | 0:28:37 | |
on making movies about killer asteroids than actually finding them. | 0:28:37 | 0:28:41 | |
Anything that's a kilometre in size, if it hit the Earth it would be devastating. | 0:28:41 | 0:28:46 | |
It would probably kill nearly everyone on the planet. | 0:28:46 | 0:28:49 | |
Each night, using a revolutionary billion-pixel digital sensor, | 0:28:54 | 0:28:59 | |
the team scans a vast swathe of the sky. | 0:28:59 | 0:29:02 | |
Mind your head! | 0:29:02 | 0:29:04 | |
They're looking for any unidentified objects that might be heading our way. | 0:29:04 | 0:29:10 | |
So any one of these points of light could in fact be an asteroid? | 0:29:10 | 0:29:13 | |
That's right. And it's very likely, | 0:29:13 | 0:29:15 | |
in fact, it's almost certain that there are asteroids in that image. | 0:29:15 | 0:29:20 | |
The problem is, how do you figure out which ones they are? | 0:29:20 | 0:29:23 | |
Yeah. | 0:29:23 | 0:29:24 | |
The camera captures several images of the same patch of sky taken minutes apart. | 0:29:26 | 0:29:32 | |
The team can then see if anything has moved, | 0:29:32 | 0:29:35 | |
relative to the background of stars. | 0:29:35 | 0:29:37 | |
What we've done here is taken two images and subtracted them, | 0:29:37 | 0:29:41 | |
and you see the stars have nearly all gone away. | 0:29:41 | 0:29:44 | |
There's a couple of interesting things left. | 0:29:44 | 0:29:47 | |
If you look over here, you see a dark thing and a white thing, | 0:29:47 | 0:29:51 | |
so that's something which was THERE in the first image | 0:29:51 | 0:29:55 | |
and THERE in the second image. And there's another one here. | 0:29:55 | 0:29:59 | |
So even on this tiny patch of sky, we've already detected two objects. | 0:29:59 | 0:30:03 | |
What that means is, when we do that kind of analysis | 0:30:03 | 0:30:06 | |
on a whole field of view, we'll detect hundreds of objects. | 0:30:06 | 0:30:10 | |
The beauty of our night sky belies the potential danger it holds in store. | 0:30:14 | 0:30:20 | |
Over 2,000 objects have been identified that pass close to the Earth, | 0:30:20 | 0:30:26 | |
with something like 400 that could be on a future collision course. | 0:30:26 | 0:30:31 | |
And all of these menacing lumps of rock, at some point, | 0:30:33 | 0:30:37 | |
come under Jupiter's gravitational influence. | 0:30:37 | 0:30:41 | |
Now, if you ever needed a demonstration of how congested the space is near the Earth, | 0:30:41 | 0:30:48 | |
just look at this movie of the near-Earth objects, | 0:30:48 | 0:30:53 | |
so here's Mercury, Venus, the Earth, Mars and out here is Jupiter. | 0:30:53 | 0:30:58 | |
Here's the asteroid belt, but look at the congestion in there. | 0:30:58 | 0:31:02 | |
Every one of those points of light is an asteroid that we know of. | 0:31:02 | 0:31:08 | |
Just look at the Earth swimming through them, so when you look up into the nice clear night sky and | 0:31:08 | 0:31:13 | |
you want to be reassured that we're all nice and safe, | 0:31:13 | 0:31:16 | |
just remember this movie. | 0:31:16 | 0:31:18 | |
Our planet is on a deadly journey. | 0:31:22 | 0:31:26 | |
Earth is trapped in a cosmic game of dodgeball as it orbits the sun, | 0:31:26 | 0:31:31 | |
a game where the gravitational stranglehold of Jupiter regularly throws asteroids our way. | 0:31:31 | 0:31:39 | |
Jupiter's gravitational influence on passing space debris | 0:31:52 | 0:31:56 | |
has made our planet a world under constant bombardment. | 0:31:56 | 0:32:00 | |
One of the most famous meteorite impact sites is the Barringer crater in Arizona. | 0:32:02 | 0:32:07 | |
50,000 years ago, | 0:32:08 | 0:32:12 | |
a 300,000 ton, 50 metre in diameter lump of iron and nickel entered the Earth's atmosphere | 0:32:12 | 0:32:19 | |
and made this crater, and it should remind us | 0:32:19 | 0:32:23 | |
that our environment doesn't just stop at the top of our atmosphere. | 0:32:23 | 0:32:27 | |
Our environment stretches out into the solar system, | 0:32:27 | 0:32:31 | |
to the very edges of the solar system, to wherever this rock came from. | 0:32:31 | 0:32:34 | |
In the grand scheme of things, | 0:32:38 | 0:32:40 | |
the asteroid that struck here was relatively small and innocuous. | 0:32:40 | 0:32:46 | |
But there are much larger impact craters hidden in Earth's landscapes | 0:32:57 | 0:33:01 | |
that have far more devastating tales to tell. | 0:33:01 | 0:33:05 | |
200 years ago, white settlers crossed the ancient Appalachian mountains here in America | 0:33:10 | 0:33:17 | |
to seek new land out west. | 0:33:17 | 0:33:20 | |
Little did they know what they were walking into. | 0:33:20 | 0:33:23 | |
Well, this place to me feels like the very definition of small town America. | 0:33:25 | 0:33:30 | |
It's on the border between Virginia, Kentucky and Tennessee. | 0:33:30 | 0:33:34 | |
It's the kind of town where you feel that | 0:33:34 | 0:33:37 | |
nothing much has changed for the last 100 years. | 0:33:37 | 0:33:40 | |
But this place was the site, | 0:33:42 | 0:33:45 | |
way back in history, of a violent cosmic intervention. | 0:33:45 | 0:33:49 | |
This is Middlesboro, Kentucky. | 0:33:53 | 0:33:56 | |
It's a town built inside a meteorite impact crater. | 0:33:56 | 0:34:01 | |
The asteroid that struck here would have been huge, about half a kilometre across, | 0:34:06 | 0:34:12 | |
hitting the Earth well over 200 million years ago. | 0:34:12 | 0:34:16 | |
I find it fascinating that when you look out of this view, you don't really see an obvious crater. | 0:34:19 | 0:34:25 | |
And indeed, it wasn't until the 1960s that anybody had any idea that there was | 0:34:25 | 0:34:30 | |
a colossal impact from space | 0:34:30 | 0:34:33 | |
just over there, centred right on the 18th hole of the golf course. | 0:34:33 | 0:34:38 | |
We now know where the giant asteroid that struck here could have come from. | 0:34:43 | 0:34:48 | |
Located between Jupiter and Mars is a vast reservoir of rocky debris that forms the asteroid belt, | 0:34:56 | 0:35:04 | |
and it's this ancient rubble that Jupiter, our neighbourhood giant, can nudge towards the Earth. | 0:35:04 | 0:35:10 | |
Well, here's my model of the solar system. | 0:35:17 | 0:35:20 | |
There's the sun in the middle, | 0:35:20 | 0:35:23 | |
then the Earth, Mars, Jupiter, | 0:35:23 | 0:35:29 | |
and the asteroids sort of scattered in between the big region | 0:35:29 | 0:35:33 | |
between Mars and Jupiter. | 0:35:33 | 0:35:35 | |
In fact they extend over 150 million miles, | 0:35:35 | 0:35:38 | |
which is further than the distance from the Earth to the sun. | 0:35:38 | 0:35:43 | |
This is my coffee, by the way, which doesn't represent anything. | 0:35:44 | 0:35:48 | |
I'll put it over there. But now and again, | 0:35:50 | 0:35:53 | |
because of collisions in the asteroid belt, a stray asteroid | 0:35:53 | 0:35:56 | |
will get thrown into the position where they keep rhythmically meeting Jupiter over and over again. | 0:35:56 | 0:36:02 | |
And because Jupiter is such a massive planet, | 0:36:02 | 0:36:04 | |
that means that it gets a kick, it gets a gravitational kick. | 0:36:04 | 0:36:08 | |
And that changes the orbit of these asteroids and over time, their orbit | 0:36:08 | 0:36:12 | |
can become, well, elongated or elliptical rather than circular. | 0:36:12 | 0:36:17 | |
That means that they can get thrown | 0:36:17 | 0:36:19 | |
into the inner solar system and cross the orbits | 0:36:19 | 0:36:23 | |
of the inner planets, including the orbit of the Earth. | 0:36:23 | 0:36:27 | |
And you get a potentially catastrophic collision. | 0:36:27 | 0:36:30 | |
Jupiter was once thought to be our protector, | 0:36:37 | 0:36:41 | |
its enormous gravity swallowing up dangerous asteroids. | 0:36:41 | 0:36:47 | |
Yet we now realise its gravitational influence can propel some of those asteroids in our direction. | 0:36:47 | 0:36:53 | |
But surprisingly, catastrophic impacts with space debris might not be a bad thing, | 0:36:55 | 0:37:01 | |
at least, in Earth's past. | 0:37:01 | 0:37:04 | |
Impacts from space shaped our planet. | 0:37:07 | 0:37:10 | |
They made our world what it is today. | 0:37:10 | 0:37:12 | |
Take life on Earth, for example. | 0:37:12 | 0:37:15 | |
Now, it's possible, or probable even, | 0:37:15 | 0:37:18 | |
that impacts on a colossal scale changed the climate so much | 0:37:18 | 0:37:23 | |
that huge swathes of life on Earth were wiped out, | 0:37:23 | 0:37:26 | |
creating ecological niches into which other species could evolve - | 0:37:26 | 0:37:32 | |
us, for example. | 0:37:32 | 0:37:33 | |
It's incredible to think that a planet | 0:37:36 | 0:37:39 | |
half a billion kilometres away could dictate the fate of our world. | 0:37:39 | 0:37:45 | |
Jupiter's immense gravity bridges the depths of space | 0:37:45 | 0:37:50 | |
and even though its power could one day devastate Earth, | 0:37:50 | 0:37:54 | |
that same gravitational field breathes life into other corners of the solar system. | 0:37:54 | 0:38:02 | |
For better or worse, | 0:38:02 | 0:38:03 | |
Jupiter's powerful gravitational field has had a direct influence on our planet. | 0:38:03 | 0:38:09 | |
We're part of a much wider ecosystem that extends to the very edges of the solar system, | 0:38:09 | 0:38:15 | |
and that ecosystem is bound together by the force of gravity, | 0:38:15 | 0:38:20 | |
and it's gravity that has power to bring worlds to life. | 0:38:20 | 0:38:25 | |
Our understanding of the solar system began much closer to home. | 0:38:34 | 0:38:39 | |
Gazing down at us, it was our moon, with its regularly changing face, | 0:38:41 | 0:38:46 | |
that first fired our interest in worlds beyond our own. | 0:38:46 | 0:38:51 | |
When we could look further out, we discovered the solar system was full | 0:38:53 | 0:38:58 | |
of moons, each invisibly connected to their parent planets by gravity. | 0:38:58 | 0:39:04 | |
Our moon is a cold, geologically dead world, but the powerful gravitational bond | 0:39:09 | 0:39:15 | |
that exists between another moon and its parent planet has done something astonishing. | 0:39:15 | 0:39:23 | |
It has brought this moon to life, | 0:39:23 | 0:39:25 | |
making it the most violent place in the solar system. | 0:39:25 | 0:39:30 | |
400 years ago, it was Galileo who first looked up at the night sky through a telescope. | 0:39:31 | 0:39:38 | |
Turning his attention to Jupiter, he noticed that this giant planet was not alone. | 0:39:38 | 0:39:45 | |
Oh, yeah! | 0:39:48 | 0:39:50 | |
Absolutely magnificent. | 0:39:50 | 0:39:52 | |
You see a disc surrounded by... | 0:39:53 | 0:39:56 | |
Well, I can see three points of light. | 0:39:56 | 0:39:58 | |
Galileo, over several nights, saw four points of light. | 0:39:58 | 0:40:01 | |
And he correctly surmised that those are actually moons, other worlds in orbit around Jupiter. | 0:40:01 | 0:40:07 | |
Jupiter's four largest moons are named after the four lovers of the Greek god Zeus. | 0:40:13 | 0:40:19 | |
Furthest out is Callisto. | 0:40:21 | 0:40:24 | |
Then there's huge Ganymede, the largest moon in the solar system. | 0:40:24 | 0:40:29 | |
Next is icy Europa, | 0:40:31 | 0:40:34 | |
and finally, the small, yellow-tinged moon nearest to Jupiter, Io. | 0:40:34 | 0:40:40 | |
So the legend goes, Zeus tried to protect his lover, Io, by turning her into a cow | 0:40:43 | 0:40:48 | |
to hide her from the jealous gaze of his wife, Hera. | 0:40:48 | 0:40:52 | |
But it didn't work, and Hera sent a gadfly to torment Io. | 0:40:52 | 0:40:58 | |
And it was prescient in a way to name that satellite Io, the tormented moon. | 0:40:58 | 0:41:05 | |
Because we've since learned that it is indeed an incredibly tormented world. | 0:41:05 | 0:41:10 | |
For 400 years, we expected Io to be as dead as our own moon. | 0:41:14 | 0:41:19 | |
But in the late 1970s, when the first spacecraft passed by Jupiter, | 0:41:20 | 0:41:26 | |
we finally saw Io up close. | 0:41:26 | 0:41:29 | |
But it didn't make any sense, as here was a moon with no meteorite impact craters. | 0:41:32 | 0:41:39 | |
Now, it's impossible to believe that Io could have escaped | 0:41:42 | 0:41:46 | |
the bombardment that we see on our moon and practically every | 0:41:46 | 0:41:50 | |
other body in the solar system, so the only explanation is that that surface is young. | 0:41:50 | 0:41:55 | |
It must have been recently produced, and that in turn means that Io, | 0:41:55 | 0:42:01 | |
that tiny moon of Jupiter out there, must be a geologically active world. | 0:42:01 | 0:42:08 | |
The truth about Io would blow us away. | 0:42:10 | 0:42:14 | |
We may not have stood on Io, but there are places we can go here on Earth to help unlock its secrets. | 0:42:23 | 0:42:30 | |
This is Ethiopia in East Africa. | 0:42:33 | 0:42:35 | |
We're being flown out by military helicopter to the very hot, | 0:42:35 | 0:42:41 | |
very inhospitable, Afar region in the north-east of the country. | 0:42:41 | 0:42:46 | |
And this is what I've come to see. | 0:42:51 | 0:42:54 | |
It's one of the rarest geological phenomena on our planet, | 0:43:03 | 0:43:08 | |
a volcano with a lake of molten lava. | 0:43:08 | 0:43:11 | |
As the sun goes down, the lava lake comes to life. | 0:43:14 | 0:43:19 | |
This volcano is called Erta Ale by the local Afar people. | 0:43:25 | 0:43:30 | |
It means "smoking mountain". | 0:43:30 | 0:43:32 | |
For many, this place is a vision of hell. | 0:43:36 | 0:43:40 | |
Yet it holds the key to understanding Io, a world over half a billion kilometres away. | 0:43:46 | 0:43:53 | |
This hot, tortured landscape of lava will be our home for the next three days. | 0:43:55 | 0:44:01 | |
Temperatures here reach 50 Celsius in the shade and we're camping right on top of the volcano. | 0:44:01 | 0:44:08 | |
But we're in good hands, as Io specialist Dr Ashley Davies is part of the team. | 0:44:12 | 0:44:17 | |
It is absolutely spectacular, isn't it? | 0:44:21 | 0:44:24 | |
-Extraordinarily beautiful. -You feel like you're looking into the core of the planet. | 0:44:24 | 0:44:29 | |
It's a window into the interior of the Earth, so magma is rising up | 0:44:29 | 0:44:34 | |
from some kilometres down, circulating through the surface and then sinking back down again. | 0:44:34 | 0:44:39 | |
It is very difficult to breathe, it's very acidic and very bitter. | 0:44:39 | 0:44:43 | |
The magma has gases in it, | 0:44:43 | 0:44:47 | |
and as it comes up to the surface, just like when you pour | 0:44:47 | 0:44:50 | |
out a bottle of Coca-Cola, the gases come out. | 0:44:50 | 0:44:54 | |
So what we have here is sulphur dioxide, hydrogen sulphide, | 0:44:54 | 0:44:58 | |
water vapour, carbon dioxide, coming out of the magma | 0:44:58 | 0:45:03 | |
before the magma then cools and sinks down, and that's what we're breathing now, it's incredibly unpleasant. | 0:45:03 | 0:45:08 | |
This volcanic phenomenon is a product of immense amounts | 0:45:13 | 0:45:16 | |
of primordial heat escaping from inside our planet. | 0:45:16 | 0:45:21 | |
Yet we have seen something similar in the far reaches of the solar system. | 0:45:23 | 0:45:28 | |
Io is the same size as our moon and should be a cold, dead world. | 0:45:32 | 0:45:37 | |
Yet our first glimpses of Io revealed it as seething with heat, alive with volcanic activity. | 0:45:42 | 0:45:49 | |
Just one of the many lava lakes on Io releases more heat than all Earth's volcanoes put together. | 0:45:51 | 0:45:58 | |
If we were to stand on the surface of Io now, | 0:46:05 | 0:46:07 | |
what would be the similarities and what would be the differences? | 0:46:07 | 0:46:11 | |
The lake would probably appear very, very similar to this, except for the scale. | 0:46:11 | 0:46:15 | |
The lava lakes on Io are vastly larger. | 0:46:15 | 0:46:18 | |
The biggest one, we think, is 180km in diameter. | 0:46:18 | 0:46:22 | |
180km? So that would stretch way... obviously way beyond the horizon on Earth! | 0:46:22 | 0:46:26 | |
Yeah, it's almost beyond description, | 0:46:26 | 0:46:29 | |
to see something that size and it's just this huge pool of molten lava. | 0:46:29 | 0:46:34 | |
Io is the most volcanic place in the solar system, | 0:46:39 | 0:46:43 | |
endlessly pumping out heat into the cold vacuum of space. | 0:46:43 | 0:46:49 | |
But what's really interesting is that it's so small that it shouldn't be volcanic at all. | 0:46:55 | 0:47:01 | |
It was one of the greatest surprises of planetary science | 0:47:08 | 0:47:11 | |
when these massive volcanoes were discovered on Io. | 0:47:11 | 0:47:14 | |
Mighty planets like Mars - has big volcanoes. | 0:47:14 | 0:47:17 | |
They're not erupting anymore, they haven't erupted for a long time. | 0:47:17 | 0:47:21 | |
Venus, lots of volcanoes there, but they haven't been erupting in a long time, probably. | 0:47:21 | 0:47:26 | |
And here we have Io, which is just insanely volcanic. | 0:47:26 | 0:47:29 | |
It's just pumping out vast amounts of energy in a zone, in a part of | 0:47:29 | 0:47:32 | |
the solar system where it was thought that everything was dead. | 0:47:32 | 0:47:36 | |
Everything we now know about Io comes from looking at it from a distance, | 0:47:43 | 0:47:48 | |
but measuring the heat pumping out of this lava lake | 0:47:48 | 0:47:51 | |
will give us a better idea of the true scale of the heat loss on Io. | 0:47:51 | 0:47:56 | |
Far from being a benign, bubbling cauldron, | 0:47:59 | 0:48:01 | |
this volcano has the power to kick off at a moment's notice. | 0:48:01 | 0:48:07 | |
I can just see pieces of molten rock rising up just below my chin, | 0:48:11 | 0:48:17 | |
and with it a cloud of heat, absolutely overpowering heat. | 0:48:17 | 0:48:21 | |
There must be a hell... a hell of an eruption going on. | 0:48:21 | 0:48:26 | |
Seeing active volcanism like this on such a small moon like Io | 0:48:31 | 0:48:35 | |
changed our view of the workings of the solar system. | 0:48:35 | 0:48:38 | |
A world like Io, having such a powerful internal heat source, cries out for an explanation. | 0:48:40 | 0:48:47 | |
You see, Io is far too small a world to have retained any internal heat | 0:48:47 | 0:48:54 | |
to have the same heat source that powers the Earth's volcanoes. | 0:48:54 | 0:49:00 | |
So something else must be driving that powerful volcanism on Io. | 0:49:00 | 0:49:06 | |
New images sent back from recent space probes confirm that Io is a surprising and bizarre world. | 0:49:10 | 0:49:17 | |
Being so far from the sun, Io's surface is mostly very cold. | 0:49:23 | 0:49:27 | |
It is covered in frozen sulphur, which gives it its yellow colour. | 0:49:29 | 0:49:32 | |
Yet Io is pockmarked by cauldrons of molten lava. | 0:49:35 | 0:49:40 | |
You know, I think it is remarkable, and fortunate in a sense, | 0:49:42 | 0:49:47 | |
that you can come to a place like this on our planet and just | 0:49:47 | 0:49:52 | |
get the tiniest sense of what it must be like | 0:49:52 | 0:49:56 | |
to stand on the edge of one of those magnificent lava lakes on Io. | 0:49:56 | 0:50:01 | |
When we first saw hot volcanic action on Io, | 0:50:04 | 0:50:07 | |
it was quite a surprise for most planetary scientists. | 0:50:07 | 0:50:11 | |
But by considering simple laws of physics, it didn't surprise everyone. | 0:50:11 | 0:50:16 | |
Just weeks before Voyager arrived at Jupiter, three scientists made a prediction, | 0:50:16 | 0:50:22 | |
and it was one of those predictions that, when you see it, is almost obvious. | 0:50:22 | 0:50:29 | |
It was using physics that had been known for hundreds of years, but nobody had thought of it. | 0:50:29 | 0:50:33 | |
They predicted that Io should have an intense internal heat source because of its unique position | 0:50:33 | 0:50:40 | |
in the solar system, very close to a giant planet and surrounded by other large moons. | 0:50:40 | 0:50:47 | |
Io sits about the same distance from Jupiter as our own moon does from Earth, | 0:50:52 | 0:50:58 | |
but don't forget that orbiting outside Io are its sister moons, Europa and Ganymede. | 0:50:58 | 0:51:04 | |
Io is under the influence not just of the massive gravitational pull | 0:51:06 | 0:51:10 | |
of Jupiter, but also the additional pull of its neighbouring moons. | 0:51:10 | 0:51:15 | |
It's this gravitational tug of war that conspires to breathe life into Io. | 0:51:15 | 0:51:22 | |
Now, Io has a very interesting relationship with Europa and Ganymede, | 0:51:24 | 0:51:29 | |
because for every four orbits that Io makes around the planet, | 0:51:29 | 0:51:34 | |
Europa goes around almost exactly twice | 0:51:34 | 0:51:39 | |
and Ganymede goes around just once. | 0:51:39 | 0:51:43 | |
Periodically, they line up together, bang, bang, bang, and Io gets | 0:51:43 | 0:51:48 | |
a powerful gravitational kick on a very regular basis. | 0:51:48 | 0:51:54 | |
And that has the effect of moving Io out of the nice circular orbit | 0:51:54 | 0:52:00 | |
into an elliptical or an eccentric orbit. | 0:52:00 | 0:52:03 | |
Io comes close to Jupiter and then far away from Jupiter, and then close to Jupiter again. | 0:52:03 | 0:52:09 | |
And because Jupiter's gravity is so big, that has the effect of stretching and squashing Io. | 0:52:09 | 0:52:15 | |
Now, imagine it was a squash ball. If you stretch and squash and stretch and squash, | 0:52:15 | 0:52:20 | |
then it gets hot by friction, and the same thing happens to this moon. | 0:52:20 | 0:52:23 | |
The power of the gravitational interaction between Jupiter and Io is extraordinary. | 0:52:23 | 0:52:30 | |
It contorts the shape of this tiny moon, moving rock as if it were nothing more than water. | 0:52:30 | 0:52:37 | |
Now, this crater is about, what, 30 metres from the base | 0:52:39 | 0:52:44 | |
that you can see down there up to the edge of the rim. | 0:52:44 | 0:52:48 | |
Now, Io, when it orbits around Jupiter every 1.8 days, | 0:52:48 | 0:52:53 | |
flexes by something like 100 metres. | 0:52:53 | 0:52:56 | |
That's three times the height of that crater. | 0:52:56 | 0:53:00 | |
Remember, Io's surface is pretty much like this, | 0:53:00 | 0:53:04 | |
solid rock, so imagine how much energy that takes, | 0:53:04 | 0:53:09 | |
and all that energy comes from Jupiter's gravitational field, | 0:53:09 | 0:53:13 | |
and that is the energy that powers the volcanoes. | 0:53:13 | 0:53:16 | |
Io is a world beyond our imagination. | 0:53:27 | 0:53:30 | |
Its unique gravitational connections | 0:53:30 | 0:53:34 | |
provide a seemingly inexhaustible supply of heat. | 0:53:34 | 0:53:38 | |
As well as its huge lava lakes, the heat also powers | 0:53:38 | 0:53:42 | |
the largest volcanic eruptions in the solar system. | 0:53:42 | 0:53:46 | |
Molten rock and gas blasts out from the frigid surface. | 0:53:54 | 0:53:59 | |
The gas expands, shattering lava into a giant fountain of fine particles. | 0:53:59 | 0:54:06 | |
With weak gravity and a sparse atmosphere, | 0:54:12 | 0:54:16 | |
Io's volcanic plumes can reach 500 km above the moon's surface. | 0:54:16 | 0:54:21 | |
This incredible phenomenon, volcanism, comes from the simplest of laws of physics, | 0:54:41 | 0:54:49 | |
the law that says that heat contained in a planet | 0:54:49 | 0:54:53 | |
must eventually find a way to escape into the coldness of space. | 0:54:53 | 0:54:58 | |
But what a spectacular way for the laws of physics to play out. | 0:54:58 | 0:55:03 | |
In the most unexpected of places, | 0:55:05 | 0:55:08 | |
in the coldest reaches of the solar system, | 0:55:08 | 0:55:11 | |
the laws of physics created a fiery world of wonder, | 0:55:11 | 0:55:16 | |
and Io is not alone. | 0:55:16 | 0:55:18 | |
Many of the hundreds of moons in the solar system | 0:55:18 | 0:55:22 | |
are not dead, barren and uninteresting worlds, | 0:55:22 | 0:55:27 | |
but active, often violent and always beautiful worlds of wonder. | 0:55:27 | 0:55:34 | |
Io is fascinating. | 0:55:38 | 0:55:41 | |
It doesn't derive its energy from an internal heart source in the same way that the Earth does. | 0:55:41 | 0:55:46 | |
It extracts energy from its orbit around its giant parent planet, | 0:55:46 | 0:55:51 | |
Jupiter, and for all those reasons, Io is a wonder of the solar system. | 0:55:51 | 0:55:57 | |
Our exploration of the planets and moons orbiting our star | 0:56:22 | 0:56:26 | |
has given us valuable insights into the nature of our own world. | 0:56:26 | 0:56:30 | |
Our view of the Earth's place in space has been turned on its head. | 0:56:33 | 0:56:39 | |
Out there are many truly violent and hostile worlds, | 0:56:39 | 0:56:46 | |
but they're driven by the same laws that shape and control our own world. | 0:56:46 | 0:56:53 | |
And so, I suppose, | 0:56:53 | 0:56:55 | |
it's in many ways a miracle that we exist at all. | 0:56:55 | 0:57:00 | |
Our solar system is like a cosmic laboratory. | 0:57:02 | 0:57:07 | |
Until we went there, we had no idea of what the laws of nature could produce. | 0:57:07 | 0:57:13 | |
I think one of the most important lessons that our exploration | 0:57:14 | 0:57:17 | |
of the solar system has taught us is that the laws of nature | 0:57:17 | 0:57:23 | |
can create vastly different worlds with the tiniest of changes. | 0:57:23 | 0:57:29 | |
We now see how the life and death of planets and moons | 0:57:32 | 0:57:37 | |
is governed by interconnections which span the solar system, | 0:57:37 | 0:57:42 | |
and we wouldn't be here if it wasn't for those connections. | 0:57:42 | 0:57:46 | |
Subtitles by Red Bee Media Ltd | 0:58:16 | 0:58:19 | |
E-mail [email protected] | 0:58:19 | 0:58:22 |