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Across the world, | 0:00:07 | 0:00:09 | |
a daring and far-fetched experiment is under way. | 0:00:09 | 0:00:13 | |
I'm going to increase more. | 0:00:15 | 0:00:17 | |
It's very risky, but it's worth doing, and also, | 0:00:19 | 0:00:24 | |
if I succeeded, I will be the king. HE LAUGHS | 0:00:24 | 0:00:30 | |
Scientists are attempting a journey that previous generations | 0:00:31 | 0:00:35 | |
have only dreamed of. | 0:00:35 | 0:00:38 | |
I can't imagine a less hospitable place for people. | 0:00:39 | 0:00:42 | |
High pressures, white hot temperatures. | 0:00:42 | 0:00:45 | |
Nasty place. | 0:00:45 | 0:00:47 | |
They are trying to reach the centre of the Earth. | 0:00:51 | 0:00:57 | |
3, 2, 1... | 0:00:57 | 0:00:59 | |
What they are glimpsing is a bizarre and alien world. | 0:01:03 | 0:01:07 | |
We're at a golden age, in terms of the real discovery of the bulk of the deep Earth. | 0:01:09 | 0:01:14 | |
It's really almost a planet within our own big planet. | 0:01:19 | 0:01:22 | |
It's like a forest. | 0:01:24 | 0:01:27 | |
It looks very interesting. | 0:01:29 | 0:01:31 | |
Their work is opening up a window | 0:01:32 | 0:01:35 | |
on one of the great mysteries of the solar system. | 0:01:35 | 0:01:38 | |
The Earth's core. | 0:01:40 | 0:01:43 | |
A hidden world, 4,000 miles, deep beneath your feet. | 0:01:44 | 0:01:51 | |
The Goddard Space Flight Centre | 0:02:05 | 0:02:07 | |
is NASA's mission control for unmanned spacecraft. | 0:02:07 | 0:02:12 | |
From here, scientists manage many of its most important telescopes and satellites. | 0:02:16 | 0:02:21 | |
Space engineer Ken LaBel has devoted his career | 0:02:25 | 0:02:28 | |
to perfecting the smooth running of these explorations of the stars. | 0:02:28 | 0:02:33 | |
But in February 1997, he was thrown into a space mystery, | 0:02:36 | 0:02:41 | |
that would offer clues to what is happening deep within our own Earth's core. | 0:02:41 | 0:02:46 | |
The Hubble Space Telescope was in trouble. | 0:02:49 | 0:02:52 | |
It's a Friday afternoon. I'm at the office, and the phone rings. | 0:02:56 | 0:03:01 | |
Engineer who I've been working with called me and said, | 0:03:01 | 0:03:04 | |
"Well, you know, we newly launched last month, two new instruments. | 0:03:04 | 0:03:07 | |
"We're seeing some problems we weren't anticipating." | 0:03:07 | 0:03:12 | |
Two ground-breaking new instruments had been installed on Hubble. | 0:03:15 | 0:03:19 | |
They were designed to peer into deepest space, | 0:03:19 | 0:03:22 | |
and to find black holes. | 0:03:22 | 0:03:25 | |
But as Hubble criss-crossed the Earth, | 0:03:26 | 0:03:30 | |
the highly sensitive multi-million dollar equipment was malfunctioning. | 0:03:30 | 0:03:34 | |
The event they were seeing were these current spikes. | 0:03:36 | 0:03:40 | |
If a signal is just moving along, | 0:03:40 | 0:03:43 | |
all of a sudden you get some injection of noise so you get a spike. | 0:03:43 | 0:03:47 | |
The issue for this particular device was that the error | 0:03:48 | 0:03:54 | |
could end up being deadly. | 0:03:54 | 0:03:57 | |
It could really take out their system. That was the fear. | 0:03:57 | 0:04:00 | |
They'd lose this big scientific instrument that people spent | 0:04:00 | 0:04:05 | |
most of their lives working on. | 0:04:05 | 0:04:07 | |
What made finding the cause of these potential fatal spikes | 0:04:10 | 0:04:14 | |
so urgent was that they were happening almost every day. | 0:04:14 | 0:04:17 | |
One of the first tasks was to plot just where. | 0:04:19 | 0:04:23 | |
And it soon became clear these weren't random events. | 0:04:28 | 0:04:32 | |
They were tightly clustered across the centre of South America | 0:04:35 | 0:04:39 | |
and the south Atlantic. | 0:04:39 | 0:04:40 | |
It's an excellent indicator that our problem was being | 0:04:41 | 0:04:45 | |
induced by that specific environment, and not because of a thermal issue, | 0:04:45 | 0:04:49 | |
or a potentially a power system issue | 0:04:49 | 0:04:52 | |
or some other type of spacecraft system not working appropriately. | 0:04:52 | 0:04:56 | |
In fact this region of space has developed | 0:04:56 | 0:05:00 | |
a reputation at NASA as a place of strange events. | 0:05:00 | 0:05:04 | |
Astronauts have reported seeing flashes of light there. | 0:05:07 | 0:05:11 | |
Satellites and space shuttle computers malfunction. | 0:05:13 | 0:05:17 | |
It's even become known as space's Bermuda Triangle. | 0:05:17 | 0:05:22 | |
Calling it the Bermuda Triangle is actually a good analogy. | 0:05:24 | 0:05:27 | |
It's been called that several times over the past 20 or more years. | 0:05:27 | 0:05:32 | |
It's a known hazard for spacecraft. | 0:05:32 | 0:05:35 | |
The challenge was now figuring out what in the system was causing it, | 0:05:35 | 0:05:39 | |
and what we could do about it. | 0:05:39 | 0:05:41 | |
But this region of space wasn't only of interest to NASA, | 0:05:46 | 0:05:50 | |
it also held important clues to what's happening in the deep Earth. | 0:05:50 | 0:05:55 | |
It may be hidden 4,000 miles beneath our feet, | 0:06:07 | 0:06:10 | |
but the core of our planet is central to life on Earth. | 0:06:10 | 0:06:14 | |
Because it creates Earth's magnetic field. | 0:06:22 | 0:06:26 | |
A tool for navigation that's vital for some of nature's greatest spectacles. | 0:06:30 | 0:06:35 | |
The mass migrations that take place around the world. | 0:06:35 | 0:06:38 | |
And a tool that helps us explore the planet, too. | 0:06:42 | 0:06:45 | |
But most importantly of all, it helps protect life itself. | 0:06:47 | 0:06:52 | |
Because the magnetic field it generates forms a vital barrier | 0:06:54 | 0:06:58 | |
between us and the dangers of space. | 0:06:58 | 0:07:00 | |
The core of the Earth and its magnetic field certainly played | 0:07:03 | 0:07:08 | |
a role in the evolution of life on Earth. | 0:07:08 | 0:07:11 | |
It shields us from the solar wind, and particles, | 0:07:11 | 0:07:14 | |
boiling off the surface of the sun. | 0:07:14 | 0:07:17 | |
Yet, for all the core's importance, though we have travelled high above our planet, | 0:07:19 | 0:07:26 | |
we've never made it down to reach its heart. | 0:07:26 | 0:07:29 | |
And that's because the barriers to a physical journey to the core are truly formidable. | 0:07:33 | 0:07:40 | |
One place on the American continent, | 0:07:52 | 0:07:55 | |
where you begin to get a sense of the challenges of descending | 0:07:55 | 0:07:59 | |
into the Earth, is a deserted gold mine, Homestake. | 0:07:59 | 0:08:02 | |
Dr Bill Roggenthen is a geologist | 0:08:08 | 0:08:11 | |
and explorer of the subterranean planet. | 0:08:11 | 0:08:15 | |
He's on the 12-minute journey down, to what is now the deepest laboratory in the USA. | 0:08:16 | 0:08:22 | |
There's snow at the surface but underground, | 0:08:29 | 0:08:31 | |
conditions are very different. | 0:08:31 | 0:08:34 | |
It was chilly at the top. | 0:08:35 | 0:08:37 | |
It's still early spring here in South Dakota, | 0:08:37 | 0:08:40 | |
and as we go down, steadily, | 0:08:40 | 0:08:42 | |
the temperature, at least the rock temperature | 0:08:42 | 0:08:46 | |
increases at a rate of around over 22 degrees C per kilometre. | 0:08:46 | 0:08:52 | |
Bill is travelling through the first barrier on any journey to the core. | 0:08:58 | 0:09:03 | |
The Earth's crust. | 0:09:08 | 0:09:11 | |
A shell of rock, typically around 35 kilometres thick. | 0:09:11 | 0:09:16 | |
OK, so now we're standing on the 4,850 foot level, | 0:09:22 | 0:09:27 | |
almost one-and-a-half kilometres below the surface. | 0:09:27 | 0:09:31 | |
Homestake mine is the deepest anyone's managed to dig in the USA. | 0:09:32 | 0:09:36 | |
Here, the rock temperature is around 29 degrees C. | 0:09:45 | 0:09:49 | |
Another kilometre down and it would be hotter than the highest temperature | 0:09:52 | 0:09:55 | |
ever recorded at the surface. | 0:09:55 | 0:09:57 | |
And, right now, we are doing experiments | 0:10:00 | 0:10:03 | |
and getting experiments going at this very deep location. | 0:10:03 | 0:10:07 | |
As scientists probe the inner workings of our planet, | 0:10:12 | 0:10:16 | |
it's not just the temperature they're contending with... | 0:10:16 | 0:10:20 | |
..it's also the pressure. | 0:10:22 | 0:10:23 | |
Any time when you're in the sub-surface | 0:10:31 | 0:10:33 | |
and you make an opening, nature wants to close it. | 0:10:33 | 0:10:37 | |
The deeper you are, | 0:10:37 | 0:10:39 | |
the harder that nature works to try to get rid of that opening. | 0:10:39 | 0:10:44 | |
Here, the rocks are particularly strong. | 0:10:46 | 0:10:50 | |
But such is the weight of the ground above, even at Homestake, | 0:10:50 | 0:10:53 | |
nothing is quite rock solid. | 0:10:53 | 0:10:55 | |
So these instruments here are measuring the movement | 0:10:57 | 0:11:01 | |
of the free surface of the rock way back into the rock itself. | 0:11:01 | 0:11:06 | |
So, even though that movement is very minor, we need to | 0:11:06 | 0:11:10 | |
monitor it to make sure these excavations are remaining stable. | 0:11:10 | 0:11:14 | |
In some areas of the crust, it would be impossible to keep an excavation open at this depth | 0:11:16 | 0:11:21 | |
because, at this intense pressure, | 0:11:21 | 0:11:25 | |
solid rocks can behave like elastic | 0:11:25 | 0:11:27 | |
and even change their constituency to become plastic. | 0:11:27 | 0:11:31 | |
Yet, we're only 0.02% of the way to the centre of the Earth. | 0:11:34 | 0:11:41 | |
So, even at this depth, why it's a huge amount, | 0:11:45 | 0:11:48 | |
the pressure at the Earth's core is 50 million lbs per square inch. | 0:11:48 | 0:11:52 | |
Truly immense. | 0:11:52 | 0:11:54 | |
That means that at the centre of the Earth, | 0:11:59 | 0:12:01 | |
the pressure is three million times that at the surface. | 0:12:01 | 0:12:05 | |
The temperature is over 4,000 degrees Celsius. | 0:12:07 | 0:12:11 | |
As hot as the surface of the sun. | 0:12:11 | 0:12:14 | |
We're an ant, if you will, as we, kind of, | 0:12:17 | 0:12:20 | |
burrow around this part of the world. | 0:12:20 | 0:12:22 | |
Having said that, it's a tremendous opportunity to go down inside | 0:12:22 | 0:12:26 | |
and see at least what this small part of the world | 0:12:26 | 0:12:29 | |
looks like in three dimensions, and that's really exciting. | 0:12:29 | 0:12:33 | |
The vastly increasing pressures and temperatures mean man will | 0:12:35 | 0:12:40 | |
never be able to physically dig to the core. | 0:12:40 | 0:12:43 | |
Scientists have had to search for other means to penetrate any further into the Earth. | 0:12:44 | 0:12:50 | |
People thought I was a little nuts coming here. | 0:13:18 | 0:13:21 | |
Famous people bet me money that I wouldn't stay for more than two years, and they all had to pay. | 0:13:21 | 0:13:26 | |
Professor Rick Aster is one of America's leading explorers | 0:13:29 | 0:13:32 | |
of the inner planet, though he has barely travelled below the surface. | 0:13:32 | 0:13:38 | |
As former President of the Seismological Society of America, | 0:13:40 | 0:13:44 | |
he doesn't need to. | 0:13:44 | 0:13:45 | |
Next to his lab in New Mexico is the university's test site. | 0:13:48 | 0:13:53 | |
It has provided him with a perfect landscape for an alternative way of seeing into the underworld. | 0:13:53 | 0:13:58 | |
Earth tremors - natural and manmade. | 0:14:01 | 0:14:07 | |
Seismology really is the killer application, | 0:14:09 | 0:14:11 | |
when you get right down to it. | 0:14:11 | 0:14:12 | |
It's the only methodology that we have | 0:14:12 | 0:14:15 | |
to remotely study the deep interior of the Earth with any kind of resolution. | 0:14:15 | 0:14:19 | |
Today, Rick is blowing up a tonne of high explosives to generate seismic waves. | 0:14:22 | 0:14:28 | |
Although it's on a small scale, it's exactly the type of thing | 0:14:34 | 0:14:38 | |
that we would need to look through the interior of the entire planet. | 0:14:38 | 0:14:41 | |
WARNING ALARM WAILS | 0:14:42 | 0:14:44 | |
Three seismographs have been set up. | 0:14:47 | 0:14:50 | |
One, just meters away from the explosives. | 0:14:50 | 0:14:53 | |
Another, at one kilometre distance. | 0:14:53 | 0:14:57 | |
And the third, two kilometres from the blast. | 0:14:57 | 0:15:01 | |
They'll measure how the Earth moves in response to the detonation. | 0:15:01 | 0:15:05 | |
Particularly with these shallow explosions, | 0:15:05 | 0:15:09 | |
most of the energy actually goes into the air. | 0:15:09 | 0:15:11 | |
What I'm interested in is how much goes into the Earth. | 0:15:11 | 0:15:14 | |
5... | 0:15:15 | 0:15:18 | |
4... | 0:15:18 | 0:15:21 | |
3... | 0:15:21 | 0:15:23 | |
2... | 0:15:23 | 0:15:25 | |
1. | 0:15:25 | 0:15:26 | |
-Always impressive. -HE CHUCKLES | 0:15:35 | 0:15:39 | |
There's no doubt that that sent a lot of energy into the ground. | 0:15:39 | 0:15:42 | |
I think we'll see a very strong signal from this explosion. | 0:15:42 | 0:15:47 | |
This is what you see when you set off one tonne of explosives. | 0:15:47 | 0:15:52 | |
A supersonic shockwave. | 0:15:56 | 0:15:58 | |
But, hidden from view, | 0:15:59 | 0:16:00 | |
a second pressure wave is travelling through the Earth. | 0:16:00 | 0:16:04 | |
A seismic wave. | 0:16:06 | 0:16:07 | |
And, it's what happens to this wave, underground, | 0:16:14 | 0:16:18 | |
that Rick is interested in. | 0:16:18 | 0:16:20 | |
Very close to the explosion we see a very simple signal. | 0:16:21 | 0:16:25 | |
We see the seismic waves generated as a very sharp impulse | 0:16:25 | 0:16:31 | |
travelling through the Earth, passing the seismograph, and it's over in just a second or two. | 0:16:31 | 0:16:35 | |
At one and two kilometres, | 0:16:35 | 0:16:38 | |
we see the development of a very rich wave train of scattered energies, | 0:16:38 | 0:16:43 | |
scattering off the topography, the landscape, | 0:16:43 | 0:16:45 | |
and scattering off the interior of the Earth, so that the signal is drawn out from this strong signal | 0:16:45 | 0:16:51 | |
that was generated at the site. | 0:16:51 | 0:16:53 | |
The further seismic waves travel, the more revealing they can be. | 0:16:57 | 0:17:02 | |
Because the speed at which they move through the ground changes | 0:17:03 | 0:17:08 | |
depending on the constituency of the material they pass through. | 0:17:08 | 0:17:13 | |
The speed of the wave tells us, basically, how stiff the rocks are. | 0:17:13 | 0:17:17 | |
That can tell us a lot about what's going on within the Earth. | 0:17:17 | 0:17:21 | |
If you're studying a volcano, for instance, | 0:17:21 | 0:17:23 | |
the speed of seismic waves slows down tremendously | 0:17:23 | 0:17:26 | |
when it goes through magma, as opposed to rock. | 0:17:26 | 0:17:30 | |
But to create seismic waves, which are able to pass all the way through the centre of the Earth, | 0:17:35 | 0:17:41 | |
and out the other side... | 0:17:41 | 0:17:43 | |
you need seismic events bigger than this one. | 0:17:43 | 0:17:46 | |
Earthquakes. | 0:17:54 | 0:17:55 | |
The shockwaves of major Earthquakes radiate through the globe. | 0:18:01 | 0:18:07 | |
Scientists have gained a form of X-ray vision into the heart of the Earth | 0:18:07 | 0:18:11 | |
by analysing the speed at which they travel. | 0:18:11 | 0:18:14 | |
It's revealed that we aren't simply living on one solid chunk of rock. | 0:18:17 | 0:18:22 | |
The Earth is made up of different layers. | 0:18:25 | 0:18:28 | |
First, is the Earth's thin crust. | 0:18:30 | 0:18:33 | |
The Earth's crust is really, really thin. | 0:18:35 | 0:18:37 | |
It's about 0.3% of the way to the centre of the Earth. | 0:18:37 | 0:18:42 | |
Then there's the mantle, | 0:18:43 | 0:18:45 | |
made of rocks turned malleable by the extreme heat and pressure. | 0:18:45 | 0:18:50 | |
The Earth's mantle is made of rocks that are, in some ways, similar to what we see at the crust, | 0:18:55 | 0:19:00 | |
although their chemistry is a little different. | 0:19:00 | 0:19:03 | |
But then the waves hit something else and, crucially, | 0:19:03 | 0:19:09 | |
they slow down. | 0:19:09 | 0:19:10 | |
To a seismologist, that could only mean one thing. | 0:19:21 | 0:19:25 | |
The fact that seismic waves travel down through | 0:19:28 | 0:19:31 | |
the mantle in a certain manner and then they hit the outer core, which | 0:19:31 | 0:19:35 | |
has a much slower seismic velocity, indicated the Earth had a core. | 0:19:35 | 0:19:40 | |
Indeed, it had an enormous core and it's molten. | 0:19:40 | 0:19:44 | |
It has a viscosity that's not much greater than water. | 0:19:44 | 0:19:48 | |
So it's an enormous ocean of white-hot, molten metal. | 0:19:48 | 0:19:54 | |
Seismology has managed to reveal the Earth's core. | 0:20:00 | 0:20:04 | |
A huge sea inside our planet, the size of Mars. | 0:20:05 | 0:20:10 | |
But that wasn't all seismology detected. | 0:20:15 | 0:20:19 | |
Scientists found signals of something else inside this sea of molten metal - | 0:20:22 | 0:20:28 | |
an inner core. | 0:20:28 | 0:20:29 | |
But for years, quite what it's like remained an enigma. | 0:20:33 | 0:20:36 | |
CLASSICAL MUSIC | 0:20:44 | 0:20:47 | |
The biggest breakthrough into the nature of this elusive inner core | 0:20:49 | 0:20:52 | |
has come from a seismologist working as far away from the violence of Earthquakes as you can imagine. | 0:20:52 | 0:20:58 | |
CLASSICAL MUSIC | 0:20:58 | 0:21:03 | |
Dr Arwen Deuss took on a puzzle that had baffled every previous seismologist. | 0:21:03 | 0:21:08 | |
So we have this mystery. | 0:21:14 | 0:21:16 | |
We have an Earth which has a solid mantle and a fluid core. | 0:21:16 | 0:21:21 | |
And people have discovered that there was actually an inner core inside this fluid outer core, | 0:21:22 | 0:21:28 | |
but people didn't know for sure if this inner core was solid or fluid. | 0:21:28 | 0:21:32 | |
It was a very difficult problem to solve. | 0:21:33 | 0:21:37 | |
Arwen wasn't to be deterred. | 0:21:42 | 0:21:45 | |
She suspected that the inner core was solid and was determined to prove it. | 0:21:45 | 0:21:50 | |
If you want to prove that the inner core is solid, | 0:21:54 | 0:21:59 | |
there's one specific wave you need to find, which is a tiny wave, | 0:21:59 | 0:22:02 | |
and a really difficult wave to observe in seismograms, | 0:22:02 | 0:22:05 | |
which we would call the shear wave, which can only travel through solid material. | 0:22:05 | 0:22:09 | |
If Arwen could find a shear wave that had passed through | 0:22:13 | 0:22:17 | |
the centre of the Earth, she'd prove the inner core was solid. | 0:22:17 | 0:22:20 | |
But there was a major problem. | 0:22:24 | 0:22:26 | |
How do you differentiate a tiny inner core shear wave, | 0:22:26 | 0:22:30 | |
from the cacophony of other waves reverberating through the Earth? | 0:22:30 | 0:22:36 | |
It's like a needle in a haystack. | 0:22:37 | 0:22:38 | |
It's not something that pops out of the piece of paper | 0:22:38 | 0:22:42 | |
when you look out the seismogram. | 0:22:42 | 0:22:43 | |
So we realised we had to do something different if you want to find it. | 0:22:43 | 0:22:47 | |
We couldn't repeat what other people had done. | 0:22:47 | 0:22:49 | |
The hunt was on. | 0:22:52 | 0:22:54 | |
A new approach to finding an inner core shear wave was needed. | 0:22:55 | 0:22:59 | |
And Arwen found it in an incredible property of the Earth... | 0:23:02 | 0:23:05 | |
The way in which the whole planet resonates | 0:23:10 | 0:23:12 | |
when it has been struck by an Earthquake. | 0:23:12 | 0:23:16 | |
Now when the Earth is hit by a major Earthquake, it's like a big hammer | 0:23:23 | 0:23:27 | |
hits a string of a musical instrument, | 0:23:27 | 0:23:31 | |
and that will start playing all the different tones of the Earth. | 0:23:31 | 0:23:34 | |
NOTES RESONATE | 0:23:35 | 0:23:37 | |
Now if we know that there's all these thousands of different tones | 0:23:37 | 0:23:41 | |
happening in the Earth, | 0:23:41 | 0:23:43 | |
what we can do is we can propose two different hypotheses. | 0:23:43 | 0:23:47 | |
We can calculate what all these tones would look like for an Earth with a fluid inner core. | 0:23:50 | 0:23:55 | |
And we can calculate what all these tones look like for an Earth with a solid inner core. | 0:23:58 | 0:24:03 | |
By comparing the predictions, she finally knew where to look for the elusive shear wave. | 0:24:05 | 0:24:10 | |
If she found it, she'd prove the inner core was solid. | 0:24:13 | 0:24:18 | |
So this little peak here is our needle in the haystack. | 0:24:18 | 0:24:22 | |
That is the thing we are going to be looking for in the real data. | 0:24:22 | 0:24:26 | |
All she needed now was an Earthquake to test her theory on. | 0:24:27 | 0:24:31 | |
A perfect candidate was a magnitude 7.9 quake that had | 0:24:35 | 0:24:40 | |
occurred in 1996, under the Flores Sea in Indonesia. | 0:24:40 | 0:24:43 | |
It was big. | 0:24:47 | 0:24:50 | |
And it was deep. | 0:24:50 | 0:24:52 | |
So it's one of the ideal Earthquakes to look for these inner core shear waves. | 0:24:54 | 0:24:58 | |
She started collating the data of this quake | 0:25:00 | 0:25:03 | |
from 47 different seismic stations across the world. | 0:25:03 | 0:25:06 | |
This red box is where you would expect a wave from the inner core to arrive. | 0:25:07 | 0:25:11 | |
Her hope was that the signal would eventually emerge | 0:25:14 | 0:25:18 | |
through the noise created by thousands of other seismic waves. | 0:25:18 | 0:25:22 | |
When we get to 40, we can see a little peak starting to appear. | 0:25:25 | 0:25:30 | |
The question is, when we start adding more stations, | 0:25:30 | 0:25:33 | |
is that bump going to grow or not? | 0:25:33 | 0:25:35 | |
Arwen added station after station. | 0:25:36 | 0:25:39 | |
This is what we're looking for. By adding more stations, | 0:25:41 | 0:25:44 | |
the peak gets bigger, so this is quite exciting. | 0:25:44 | 0:25:46 | |
She was on the brink of answering this fundamental question about the Earth's inner core. | 0:25:48 | 0:25:54 | |
We add our last station, 47, and now we have a really large signal there. | 0:25:55 | 0:26:00 | |
That's our needle in the haystack. | 0:26:04 | 0:26:06 | |
We've got a really nice, strong, big arrival, | 0:26:06 | 0:26:09 | |
proving that the inner core is solid. | 0:26:09 | 0:26:11 | |
This shear wave, which could only pass through solid material, | 0:26:14 | 0:26:18 | |
had travelled through the centre of the Earth. | 0:26:18 | 0:26:22 | |
Arwen had discovered that sitting inside our planet | 0:26:24 | 0:26:28 | |
is a solid metal ball, almost the size of the moon. | 0:26:28 | 0:26:31 | |
But our solid inner core is proving stranger than Arwen could ever have imagined. | 0:26:39 | 0:26:45 | |
Say you had an Earthquake at the North Pole and a seismometer at the South Pole, | 0:26:46 | 0:26:52 | |
then a wave that would travel from the North Pole to the South Pole | 0:26:52 | 0:26:56 | |
would arrive up to five seconds faster than from east to west if they go through the inner core. | 0:26:56 | 0:27:01 | |
And we had no idea how to explain that. | 0:27:03 | 0:27:06 | |
Seismology on its own simply can't unlock all the inner core's secrets | 0:27:08 | 0:27:12 | |
but it seemed to be the only real way scientists could reveal them. | 0:27:12 | 0:27:17 | |
Until now. | 0:27:20 | 0:27:21 | |
In Japan, one man has pioneered a new technique to investigate the mysterious inner core. | 0:27:30 | 0:27:37 | |
Because Kei Hirose is a scientist determined to leave the surface world behind, | 0:27:38 | 0:27:46 | |
and complete an impossible mission to see the centre of the Earth. | 0:27:46 | 0:27:50 | |
We cannot go into the centre of the Earth, | 0:27:53 | 0:27:57 | |
but we can recreate the conditions | 0:27:57 | 0:28:01 | |
corresponding at the centre of the Earth in my own laboratory, | 0:28:01 | 0:28:07 | |
and it's a kind of journey to the centre of the Earth. | 0:28:07 | 0:28:10 | |
I'll try to be the first person to reach there. | 0:28:10 | 0:28:14 | |
It's very risky but it's worth doing, | 0:28:14 | 0:28:17 | |
and also, if I succeeded... | 0:28:17 | 0:28:22 | |
..I'll be the king! HE LAUGHS | 0:28:24 | 0:28:26 | |
This is the SPring-8 Synchrotron Radiation Facility. | 0:28:33 | 0:28:37 | |
Kei's using its powerful equipment | 0:28:39 | 0:28:41 | |
in his attempt to recreate the immense temperatures | 0:28:41 | 0:28:44 | |
and pressures found at the inner core. | 0:28:44 | 0:28:47 | |
Somewhere rather more convenient to study. | 0:28:47 | 0:28:50 | |
Oops. | 0:28:53 | 0:28:55 | |
OK. So, as a diamond it looks beautiful, | 0:28:57 | 0:29:00 | |
and then I put it on to the seed. | 0:29:00 | 0:29:04 | |
The first part of his mission is to simulate the pressures | 0:29:09 | 0:29:12 | |
found at the centre of the Earth. | 0:29:12 | 0:29:14 | |
It took him ten years and hundreds of shattered diamonds to design an enormously powerful vice, | 0:29:16 | 0:29:23 | |
using the tips of the jewels. | 0:29:23 | 0:29:25 | |
Next, we can load the samples, and these are very tiny. | 0:29:26 | 0:29:31 | |
Between the points Kei puts a sample... | 0:29:33 | 0:29:37 | |
a shard of iron nickel alloy. | 0:29:37 | 0:29:39 | |
The material scientists believe makes up the inner core. | 0:29:39 | 0:29:42 | |
At the Earth's surface, it's composed of lots of tiny crystals. | 0:29:45 | 0:29:50 | |
Kei hopes to show what happens to its structure | 0:29:50 | 0:29:53 | |
under the extreme conditions found at the inner core. | 0:29:53 | 0:29:57 | |
OK, that's fine. | 0:29:59 | 0:30:02 | |
He uses the vice to raise the sample pressure to that of the inner core. | 0:30:05 | 0:30:09 | |
It's equivalent to three medium times, atmospheric pressure, | 0:30:11 | 0:30:16 | |
so it is very high pressure. But we just use a screwdriver | 0:30:16 | 0:30:22 | |
to increase the pressure, to such extreme conditions. | 0:30:22 | 0:30:25 | |
It's very simple. | 0:30:25 | 0:30:28 | |
Part one of the mission complete. Now for stage two. | 0:30:37 | 0:30:42 | |
Kei has to heat the sample to 4,700 Kelvin. | 0:30:42 | 0:30:47 | |
A temperature found at the inner core, and on the surface of the sun. | 0:30:47 | 0:30:53 | |
The beam of an infrared laser will be focused on the sample to raise its temperature. | 0:31:01 | 0:31:05 | |
At the beginning of the experiment, Kei shines X-rays through the sample to create an image. | 0:31:12 | 0:31:18 | |
The iron nickel crystals form a pattern of two concentric rings. | 0:31:21 | 0:31:25 | |
So this image tells us what is going on inside the sample, | 0:31:26 | 0:31:29 | |
under high pressure and high temperature. | 0:31:29 | 0:31:32 | |
OK, so let's go. | 0:31:34 | 0:31:36 | |
As the power of the laser is increased, | 0:31:39 | 0:31:41 | |
the temperature of the sample rises. | 0:31:41 | 0:31:44 | |
OK, so the sample is already about 1,500 Kelvins. | 0:31:47 | 0:31:52 | |
Let's take the X-ray defraction images. | 0:31:55 | 0:31:58 | |
And as the temperature grows, | 0:32:00 | 0:32:01 | |
the iron nickel crystal structure begins to change. | 0:32:01 | 0:32:05 | |
And now the temperature is about, OK, it's about 3,000 Kelvins. | 0:32:10 | 0:32:16 | |
A uniform circular structure has all but gone, | 0:32:16 | 0:32:19 | |
and crystals appear to be clumping together. | 0:32:19 | 0:32:22 | |
Oh, now, the temperature is very high. It's almost close to the temperature at the core. | 0:32:29 | 0:32:35 | |
You know, I'm very nervous at this moment. | 0:32:35 | 0:32:38 | |
I'm going to increase more, OK? | 0:32:40 | 0:32:43 | |
Oh, look at this. | 0:32:48 | 0:32:49 | |
It is already 4,000 Kelvins, which is the real core temperature, | 0:32:49 | 0:32:54 | |
and take another pattern here. | 0:32:54 | 0:32:57 | |
Welcome to Kei's inner core of the Earth. | 0:33:02 | 0:33:05 | |
For the first time, he has shown how iron nickel alloy crystals | 0:33:05 | 0:33:09 | |
undergo a dramatic transformation under the pressures and temperatures | 0:33:09 | 0:33:14 | |
found at the inner core. | 0:33:14 | 0:33:15 | |
I think we should stop here. It's successful, we are very fortunate. | 0:33:20 | 0:33:26 | |
We sometimes fail the experiment, but this time we are very lucky. | 0:33:26 | 0:33:33 | |
Good. | 0:33:33 | 0:33:34 | |
These X-ray images give us a real insight into the physical nature of the inner core. | 0:33:38 | 0:33:42 | |
It's iron nickel alloy, but not as we know it. | 0:33:44 | 0:33:49 | |
So, this is the first image. | 0:33:49 | 0:33:51 | |
We have rings and it became spotty during heating. | 0:33:51 | 0:33:58 | |
And the size of the crystal of iron nickel alloy increased | 0:33:58 | 0:34:02 | |
by 1,000 times at core pressure and temperature, in our experiment, | 0:34:02 | 0:34:09 | |
just in ten minutes. | 0:34:09 | 0:34:11 | |
Over millions of years, under the extreme heat and pressure | 0:34:15 | 0:34:18 | |
found at the core, these crystals could have grown to huge lengths. | 0:34:18 | 0:34:22 | |
We may have very big crystals at the centre of the Earth. | 0:34:25 | 0:34:29 | |
Maybe up to ten kilometres. | 0:34:29 | 0:34:33 | |
It's like a forest. | 0:34:33 | 0:34:34 | |
It looks very interesting. | 0:34:37 | 0:34:39 | |
Kei believes this forest of crystals makes up the solid inner core of our Earth, | 0:34:44 | 0:34:48 | |
with the crystals all pointing in the direction of the north pole. | 0:34:50 | 0:34:53 | |
This could now explain why seismic waves travel through the core faster north to south, | 0:34:55 | 0:35:01 | |
along the grain of the crystals, | 0:35:01 | 0:35:03 | |
than east to west, across them. | 0:35:03 | 0:35:05 | |
We tried many, many times, but we always failed. | 0:35:07 | 0:35:13 | |
But we finally did and, you know, I realise how important it is. | 0:35:13 | 0:35:20 | |
And, you know, probably it's a big achievement in my life. | 0:35:20 | 0:35:27 | |
Kei's discovery is a significant step forward in our understanding of the core. | 0:35:30 | 0:35:35 | |
But scientists' revelation of a white-hot metallic inner world | 0:35:40 | 0:35:44 | |
raises another, more fundamental question. | 0:35:44 | 0:35:47 | |
Why is the core of our planet so very different from everything | 0:35:50 | 0:35:54 | |
we know at the rocky surface? | 0:35:54 | 0:35:56 | |
The answer would ultimately turn out to be central to the story of life on Earth. | 0:35:58 | 0:36:04 | |
Professor Dave Stevenson has made a career out of studying what lies | 0:36:13 | 0:36:17 | |
beneath the surface of all planets in the solar system. | 0:36:17 | 0:36:19 | |
I love looking at things that are difficult to understand, | 0:36:22 | 0:36:26 | |
that are difficult to get to. So I've always been fascinated by cores. | 0:36:26 | 0:36:32 | |
But one aspect of why | 0:36:32 | 0:36:36 | |
I find Earth's core so fascinating, | 0:36:36 | 0:36:39 | |
is that it - I believe - | 0:36:39 | 0:36:41 | |
contains a memory of what happened in the history of the Earth. | 0:36:41 | 0:36:47 | |
He believes to truly understand our core, we need to look up to the stars... | 0:36:56 | 0:37:02 | |
..and go back to our planet's birth, in the violent collisions that | 0:37:07 | 0:37:11 | |
happened during the formation of the solar system billions of years ago. | 0:37:11 | 0:37:16 | |
The Earth's core formed through | 0:37:21 | 0:37:26 | |
a very energetic set of events. | 0:37:26 | 0:37:31 | |
Let's go back to the beginning. | 0:37:31 | 0:37:33 | |
Imagine that you were bashing together bodies that were about the size of Mars. | 0:37:33 | 0:37:40 | |
And when you do that, you produce an enormous amount of heat. | 0:37:40 | 0:37:45 | |
EXPLOSIVE BOOM | 0:37:54 | 0:37:56 | |
The early solar system was a brutal and chaotic place. | 0:37:56 | 0:38:00 | |
But out of this fury, the conditions needed to forge our core were created. | 0:38:04 | 0:38:10 | |
Heat. | 0:38:17 | 0:38:18 | |
When you heat a mixture of solid material that is in the form of rock and iron, | 0:38:20 | 0:38:28 | |
to very high temperatures, the iron will separate. | 0:38:28 | 0:38:34 | |
It is heavy, and so it will sink under gravity to the centre | 0:38:34 | 0:38:40 | |
of the Earth and the core will be formed. | 0:38:40 | 0:38:42 | |
It's this separation of molten rock and metal that makes the outer layers of the Earth so different... | 0:38:47 | 0:38:54 | |
..from the core inside. | 0:38:56 | 0:38:57 | |
And the Earth's baptism of fire had another legacy. | 0:39:05 | 0:39:08 | |
As the intense heat at the centre of our planet escaped, | 0:39:10 | 0:39:14 | |
it caused the liquid metal within the core to move. | 0:39:14 | 0:39:17 | |
This ceaseless motion in the depths of the Earth is what creates | 0:39:22 | 0:39:26 | |
the magnetic field we experience at the surface. | 0:39:26 | 0:39:30 | |
If you want to generate a magnetic field, the way the Earth does it, | 0:39:35 | 0:39:40 | |
you need a metal. That's fine, iron is a metal, it needs to be liquid, | 0:39:40 | 0:39:44 | |
that means it has to be hot. But you also need a temperature difference. | 0:39:44 | 0:39:49 | |
As the heat flows from the hot inner core to the cooler mantle, it causes | 0:39:52 | 0:39:57 | |
convection currents to form within the molten metal of the outer core. | 0:39:57 | 0:40:01 | |
Those motions, through the process of electromagnetic induction, | 0:40:07 | 0:40:13 | |
is the way in which the magnetic field is generated. | 0:40:13 | 0:40:17 | |
And it's the generation of this magnetic field that is so vital to life on Earth. | 0:40:19 | 0:40:26 | |
Because as charged particles are blown off the sun, | 0:40:31 | 0:40:35 | |
the magnetosphere deflects them, | 0:40:35 | 0:40:39 | |
creating a safe haven for our planet. | 0:40:39 | 0:40:42 | |
This magnetic field is providing scientists with new insights | 0:40:49 | 0:40:53 | |
into what's happening at the centre of the Earth... | 0:40:53 | 0:40:57 | |
moment by moment. | 0:40:57 | 0:40:58 | |
Geophysicist, Dan Lathrop, is on a mission to build a remarkable machine. | 0:41:13 | 0:41:18 | |
He hopes it will do something no supercomputer has managed. | 0:41:21 | 0:41:25 | |
Recreate the motions of molten metal in the core, to generate a magnetic field. | 0:41:27 | 0:41:32 | |
He started small, | 0:41:34 | 0:41:35 | |
but in his search for answers, the models have just got bigger... | 0:41:35 | 0:41:40 | |
and bigger. | 0:41:40 | 0:41:42 | |
What we don't know about the core is really details about the flows, | 0:41:51 | 0:41:56 | |
and details about the magnetic fields inside the core. | 0:41:56 | 0:42:00 | |
We know a bit about what happens at the surface, | 0:42:00 | 0:42:02 | |
but this is a very thick layer of liquid metal | 0:42:02 | 0:42:05 | |
and what happens underneath the surface is really a mystery to us. | 0:42:05 | 0:42:09 | |
The experiment is fraught with danger. | 0:42:16 | 0:42:19 | |
Dan plans to fill his core with 12 tons of molten sodium metal - | 0:42:19 | 0:42:24 | |
a highly volatile element - | 0:42:24 | 0:42:28 | |
and then spin it at up to 85 miles an hour. | 0:42:28 | 0:42:31 | |
This is really as close to a model of the Earth as we're going to have. | 0:42:40 | 0:42:44 | |
This device sets up a swirling mass of liquid metal as a mimic | 0:42:44 | 0:42:48 | |
of what happens in deep Earth, but in a way that we | 0:42:48 | 0:42:51 | |
can directly probe the flows, the rotating motions, | 0:42:51 | 0:42:55 | |
and look at them in more detail than we could ever do for the Earth's core. | 0:42:55 | 0:42:58 | |
He hopes this gargantuan model of the core will help explain | 0:42:58 | 0:43:03 | |
something strange about the behaviour of Earth's magnetic field. | 0:43:03 | 0:43:07 | |
It's never fixed, but constantly fluctuating. | 0:43:10 | 0:43:14 | |
So, while most people think of the Earth's magnetic field | 0:43:14 | 0:43:18 | |
as just being a simple north and south, it's really very complicated. | 0:43:18 | 0:43:24 | |
There are patches of weaker field, patches of stronger field, | 0:43:24 | 0:43:28 | |
all those are moving about the planet, some becoming weaker, | 0:43:28 | 0:43:32 | |
some becoming stronger, in a very complex way. | 0:43:32 | 0:43:34 | |
One thing is clear though. | 0:43:37 | 0:43:39 | |
If the magnetic field is continually changing, | 0:43:39 | 0:43:42 | |
then that must be caused by how the metal moves within the outer core. | 0:43:42 | 0:43:47 | |
Early experiments have already hinted at what could be happening. | 0:43:53 | 0:43:58 | |
Dan injected fluorescent dye into the rotating machine. | 0:44:04 | 0:44:08 | |
The results suggest the core is place of great turbulence, | 0:44:12 | 0:44:15 | |
filled with eddies and currents. | 0:44:15 | 0:44:18 | |
You might think of the core, like the atmosphere of the Earth, | 0:44:22 | 0:44:26 | |
being a very restless place with storms and fronts and bad weather. | 0:44:26 | 0:44:30 | |
Very complicated turbulent motions, very complicated sets of vortices, | 0:44:30 | 0:44:36 | |
all interacting with each other. | 0:44:36 | 0:44:38 | |
And those drive motions like the convection we see in the atmosphere, | 0:44:38 | 0:44:43 | |
billowing upwards motions in clouds. | 0:44:43 | 0:44:45 | |
All of those then are shaped by the rotation of the core. | 0:44:45 | 0:44:50 | |
And these deep motions interact with electric currents, | 0:44:50 | 0:44:54 | |
drive electric currents and cause the Earth's main magnetic field. | 0:44:54 | 0:44:58 | |
Dan's model is opening up a new window on the inner Earth. | 0:45:03 | 0:45:07 | |
Our core may be a dynamo, but it's no simple one. | 0:45:09 | 0:45:14 | |
Vast vortices and whirlpools create a magnetic field constantly in flux. | 0:45:16 | 0:45:21 | |
And that causes unexpected phenomena that scientists are only now beginning to understand. | 0:45:21 | 0:45:29 | |
Dr Jack Connerney has devoted his career at NASA | 0:45:42 | 0:45:45 | |
to studying the magnetic fields of planets | 0:45:45 | 0:45:48 | |
right across the solar system. | 0:45:48 | 0:45:50 | |
Here at NASA's test facility, | 0:45:52 | 0:45:55 | |
he's even got the ability to recreate the magnetic field of any heavenly body. | 0:45:55 | 0:46:01 | |
But something that's really fascinated him | 0:46:03 | 0:46:06 | |
are the changes that are happening to Earth's magnetosphere. | 0:46:06 | 0:46:09 | |
And how they're related to the turbulent molten metal dynamo | 0:46:09 | 0:46:13 | |
that is our core. | 0:46:13 | 0:46:15 | |
The dynamo is electrically conducting fluid in motion, | 0:46:19 | 0:46:23 | |
so when you have motion of that fluid, | 0:46:23 | 0:46:26 | |
it carries with it the magnetic field. | 0:46:26 | 0:46:29 | |
So, if you can look at how the magnetic field evolves in time, | 0:46:29 | 0:46:33 | |
you are actually looking at how the fluid motion | 0:46:33 | 0:46:38 | |
on the dynamo surface is evolving in time. | 0:46:38 | 0:46:41 | |
So, by tracking the change in the magnetic field, | 0:46:41 | 0:46:45 | |
we can essentially image the fluid motion on the surface of the core. | 0:46:45 | 0:46:50 | |
By collating thousands of observations | 0:46:52 | 0:46:55 | |
and the data from many satellites, | 0:46:55 | 0:46:57 | |
scientists have been able to piece together a map | 0:46:57 | 0:47:00 | |
of how Earth's magnetic field has been changing over the centuries. | 0:47:00 | 0:47:05 | |
What they've discovered is that, over the last 180 years, | 0:47:09 | 0:47:12 | |
it's been steadily weakening. | 0:47:12 | 0:47:14 | |
Right now, the Earth field is decreasing fairly significantly, | 0:47:16 | 0:47:20 | |
fairly rapidly. | 0:47:20 | 0:47:21 | |
But, for Jack, | 0:47:24 | 0:47:26 | |
there's one area of the magnetic field that particularly stands out. | 0:47:26 | 0:47:30 | |
It's a region in our magnetosphere | 0:47:35 | 0:47:38 | |
that's been weakening faster than any other. | 0:47:38 | 0:47:41 | |
This is a map of the magnetic field, a contour map, | 0:47:45 | 0:47:49 | |
and what you see here evolving in time, over hundreds of years, | 0:47:49 | 0:47:53 | |
is a patch of very weak field in blue | 0:47:53 | 0:47:57 | |
that slowly expands in size, | 0:47:57 | 0:48:00 | |
becomes progressively weaker and weaker in field magnitude, | 0:48:00 | 0:48:05 | |
and, as it does so, it's going to drift westward, slowly. | 0:48:05 | 0:48:09 | |
This is the map scientists have created | 0:48:11 | 0:48:14 | |
that shows just how a weakness in the Earth's magnetic field | 0:48:14 | 0:48:18 | |
has been growing over 400 years. | 0:48:18 | 0:48:20 | |
The blue patch of field is half the strength of that towards the poles. | 0:48:23 | 0:48:29 | |
And scientists have given it a name. | 0:48:29 | 0:48:31 | |
That weak field is the South Atlantic Anomaly. | 0:48:33 | 0:48:36 | |
This region is still growing and, in just 200 years, | 0:48:41 | 0:48:44 | |
it may cover the entire Southern Hemisphere. | 0:48:44 | 0:48:47 | |
It's evidence that something truly remarkable is happening | 0:48:53 | 0:48:56 | |
deep beneath our feet in the core. | 0:48:56 | 0:48:58 | |
The first place the effects of it are felt aren't here on Earth, | 0:49:02 | 0:49:07 | |
but high in space. | 0:49:07 | 0:49:09 | |
And that's why NASA is so interested in the South Atlantic Anomaly. | 0:49:13 | 0:49:17 | |
And in the core. | 0:49:17 | 0:49:18 | |
It was the South Atlantic Anomaly that was to prove key | 0:49:22 | 0:49:25 | |
to the space emergency that threatened the Hubble telescope. | 0:49:25 | 0:49:28 | |
Two new multimillion-dollar instruments | 0:49:30 | 0:49:34 | |
were repeatedly malfunctioning. | 0:49:34 | 0:49:36 | |
And the upsets were occurring in just one area. | 0:49:36 | 0:49:40 | |
Right in the heart of the South Atlantic Anomaly. | 0:49:41 | 0:49:45 | |
Ken LaBel and his team needed to find out | 0:49:51 | 0:49:54 | |
how the two phenomena could be related. | 0:49:54 | 0:49:56 | |
They knew that the weak field at the South Atlantic Anomaly | 0:49:59 | 0:50:02 | |
has one very significant effect on the structure of the magnetosphere. | 0:50:02 | 0:50:07 | |
In that region of the South Atlantic, | 0:50:07 | 0:50:09 | |
the Earth's magnetic field has a dip in it. | 0:50:09 | 0:50:13 | |
In that region, the magnetic field changes its shape. | 0:50:13 | 0:50:17 | |
It comes closer to the Earth. | 0:50:17 | 0:50:19 | |
As the magnetic shield protects Earth from solar radiation, | 0:50:19 | 0:50:24 | |
then in this dip charged particles like protons | 0:50:24 | 0:50:28 | |
must be able to travel closer to our planet. | 0:50:28 | 0:50:31 | |
Could these protons be causing the trouble with Hubble? | 0:50:36 | 0:50:40 | |
Within two weeks, | 0:50:42 | 0:50:44 | |
we had a test set built, | 0:50:44 | 0:50:45 | |
and we went to one of the cyclotrons in the US to do some testing. | 0:50:45 | 0:50:50 | |
And lo and behold, this part was quite susceptible to protons. | 0:50:50 | 0:50:54 | |
The very culprit we'd expect to see issues with in the South Atlantic Anomaly. | 0:50:54 | 0:50:59 | |
Every time Hubble passed through the South Atlantic Anomaly, | 0:51:03 | 0:51:07 | |
it entered an exposed region of space. | 0:51:07 | 0:51:10 | |
It was bombarded by charged particles. | 0:51:12 | 0:51:16 | |
So, each of these events that we're seeing, | 0:51:19 | 0:51:22 | |
those nine events in the first ten days, | 0:51:22 | 0:51:25 | |
was a single proton hitting the sensitive portion of these devices. | 0:51:25 | 0:51:31 | |
But, making the equipment completely proton proof | 0:51:31 | 0:51:36 | |
was simply too difficult, even for NASA. | 0:51:36 | 0:51:39 | |
Something else needed to be done. | 0:51:39 | 0:51:42 | |
It was determined after a lot of work, | 0:51:42 | 0:51:45 | |
both in testing and in environmental predictions, | 0:51:45 | 0:51:49 | |
trying to come up with risk analyses, | 0:51:49 | 0:51:52 | |
that, every time instruments pass the South Atlantic Anomaly, | 0:51:52 | 0:51:56 | |
they turn off. | 0:51:56 | 0:51:59 | |
It's never an even battle when you are dealing with | 0:52:02 | 0:52:05 | |
something on as large a scale as the core and the magnetic field. | 0:52:05 | 0:52:09 | |
So, a good story in the end for those instruments. | 0:52:11 | 0:52:15 | |
Hubble's delicate sensors were now safe | 0:52:18 | 0:52:22 | |
from the strange behaviour of the core deep under the South Atlantic. | 0:52:22 | 0:52:26 | |
But the Anomaly is evidence of changes deep within the Earth | 0:52:30 | 0:52:34 | |
that could ultimately have consequences for more than just satellites. | 0:52:34 | 0:52:39 | |
To understand what these changes might be, | 0:52:47 | 0:52:49 | |
scientists began mapping the magnetic field far below the ground. | 0:52:49 | 0:52:55 | |
As we step down and look deeper and deeper inside the Earth, | 0:52:55 | 0:53:00 | |
the field both grows in magnitude | 0:53:00 | 0:53:03 | |
and it becomes more complex in structure and polarity. | 0:53:03 | 0:53:07 | |
Scientists discovered that the simple North-South divide | 0:53:09 | 0:53:12 | |
we experience at the surface | 0:53:12 | 0:53:14 | |
breaks down at the level of the core. | 0:53:14 | 0:53:17 | |
Under the South Atlantic, there are patches, indicated in green, | 0:53:19 | 0:53:23 | |
where the magnetic field has actually flipped and points North. | 0:53:23 | 0:53:28 | |
The combined effect of these patches, | 0:53:31 | 0:53:34 | |
where the polarity of the field is reversed, | 0:53:34 | 0:53:37 | |
is such to weaken the field over the South Atlantic. | 0:53:37 | 0:53:40 | |
That weak field is the South Atlantic Anomaly. | 0:53:40 | 0:53:43 | |
What could be happening | 0:53:52 | 0:53:54 | |
in the molten metal ocean of the outer core to create these patches? | 0:53:54 | 0:54:00 | |
Dan Lathrop thinks he knows. | 0:54:00 | 0:54:03 | |
It's really the moving liquid metal's ability | 0:54:08 | 0:54:12 | |
to drag and stretch and twist the magnetic field. | 0:54:12 | 0:54:15 | |
In the same sense as we talk about a storm, | 0:54:18 | 0:54:21 | |
when the air is being a particularly violent or unusual patch of weather, | 0:54:21 | 0:54:25 | |
then there's some sort of flow structure down in the core under the South Atlantic | 0:54:25 | 0:54:29 | |
that changed in such a way as to forcibly reverse the magnetic field. | 0:54:29 | 0:54:34 | |
When scientists looked at the Earth's entire magnetic field at the level of the core, | 0:54:36 | 0:54:42 | |
they discovered this perfect storm under the South Atlantic wasn't a one-off event. | 0:54:42 | 0:54:47 | |
In fact, there are multiple patches where the field has flipped. | 0:54:50 | 0:54:54 | |
Could these changes be harbingers of an even bigger shift? | 0:54:56 | 0:55:01 | |
So, there's a very good chance that that South Atlantic Anomaly, | 0:55:03 | 0:55:08 | |
that reversal at the level of the core, could deepen and spread, | 0:55:08 | 0:55:12 | |
and that these small reversed patches in the Northern Hemisphere | 0:55:12 | 0:55:15 | |
could also deepen and spread, | 0:55:15 | 0:55:16 | |
and result in an overall reversal of the North-South pattern, | 0:55:16 | 0:55:20 | |
the biggest structure in the magnetic field. | 0:55:20 | 0:55:22 | |
So, if enough of these storms joined forces | 0:55:24 | 0:55:28 | |
in the molten metal of the outer core, | 0:55:28 | 0:55:31 | |
the Earth's magnetic field could reach a tipping point... | 0:55:31 | 0:55:35 | |
..and flip. | 0:55:36 | 0:55:38 | |
It's not a change that would happen overnight. | 0:56:06 | 0:56:09 | |
The shifting flows of the core | 0:56:09 | 0:56:12 | |
could take between 1,000 and 10,000 years to reverse our field. | 0:56:12 | 0:56:17 | |
During this period, though, | 0:56:21 | 0:56:23 | |
there would be some intriguing phenomena that we would all notice. | 0:56:23 | 0:56:28 | |
During the reversal, the structure of the Earth's magnetic field | 0:56:28 | 0:56:32 | |
could be more complicated than what we have now. | 0:56:32 | 0:56:36 | |
So, instead of a north and south main pole, | 0:56:36 | 0:56:38 | |
one could have two north poles and two south poles, | 0:56:38 | 0:56:41 | |
or poles occurring at the Equator. | 0:56:41 | 0:56:44 | |
The animals that rely on the core's magnetic field to navigate | 0:56:46 | 0:56:50 | |
would have to find some other means to guide their migrations. | 0:56:50 | 0:56:54 | |
And, the wandering magnetic poles would bring the Northern lights | 0:56:57 | 0:57:01 | |
to unexpected locations. | 0:57:01 | 0:57:04 | |
It wouldn't be the first time the flows of the outer core | 0:57:05 | 0:57:09 | |
have undergone a dramatic change. | 0:57:09 | 0:57:12 | |
Magnetised rocks contain a history of the core's turbulent past. | 0:57:16 | 0:57:21 | |
We have very solid evidence that the Earth's magnetic field | 0:57:21 | 0:57:25 | |
has reversed many hundreds of times in the Earth's history. | 0:57:25 | 0:57:29 | |
So, the fact that we've seen so many changes and reversals, | 0:57:31 | 0:57:35 | |
and so many changes in the historical times of the field, | 0:57:35 | 0:57:38 | |
really gives us a view of the outer core being a very active place. | 0:57:38 | 0:57:42 | |
It's not a question of IF the Earth is going to reverse its magnetic field, but WHEN. | 0:57:42 | 0:57:46 | |
How soon this might be is one of the many mysteries of the core. | 0:57:50 | 0:57:55 | |
But these remarkable experiments | 0:57:56 | 0:57:59 | |
are now creating a real picture of the deep Earth | 0:57:59 | 0:58:03 | |
to replace the fantasies of science fiction. | 0:58:03 | 0:58:07 | |
We may never be able to go there. | 0:58:11 | 0:58:13 | |
But we have a sense of what a journey might be like. | 0:58:15 | 0:58:19 | |
One thing is certain, though... | 0:58:22 | 0:58:24 | |
..this strange inner world is only STARTING to reveal its secrets. | 0:58:26 | 0:58:31 | |
Subtitles by Red Bee Media Ltd | 0:58:48 | 0:58:51 | |
E-mail [email protected] | 0:58:51 | 0:58:54 |