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High above us, out in space, there are millions of very strange, | 0:00:06 | 0:00:11 | |
but very special chunks of rock tumbling between the planets. | 0:00:11 | 0:00:16 | |
Each one has a different story to tell. | 0:00:16 | 0:00:20 | |
And those stories are important to understanding the story of the solar system. | 0:00:20 | 0:00:26 | |
These are the asteroids... | 0:00:27 | 0:00:30 | |
debris from an extraordinary event... | 0:00:30 | 0:00:33 | |
..The birth of our solar system, 4.5 billion years ago. | 0:00:35 | 0:00:40 | |
Asteroids ARE fossils of the early solar system. | 0:00:40 | 0:00:43 | |
They were accumulated from some of the starting materials from which everything else was made. | 0:00:43 | 0:00:48 | |
But asteroids continue to present a threat to the very future of our planet. | 0:00:48 | 0:00:54 | |
If one of hits, every man woman and child on the planet could die. | 0:00:54 | 0:00:58 | |
Yet asteroids are about far more than destruction. | 0:00:58 | 0:01:02 | |
Around the world there are scientists working to uncover | 0:01:02 | 0:01:05 | |
what these messengers from the solar system tell us about our place in the universe. | 0:01:05 | 0:01:11 | |
They essentially created the solar system we live in and the planet that we live on. | 0:01:11 | 0:01:16 | |
And what they're finding is that while asteroids may not be beautiful, | 0:01:18 | 0:01:22 | |
they do hold a surprising power over life and death on our planet. | 0:01:22 | 0:01:27 | |
Are we alone in the universe? | 0:01:36 | 0:01:39 | |
Are there other unknown planets in the outer solar system? | 0:01:40 | 0:01:43 | |
Are the laws of nature the same everywhere? | 0:01:44 | 0:01:48 | |
Is the solar system stable? | 0:01:48 | 0:01:50 | |
High up above the clouds, Professor Dave Jewitt dares to challenge forces of the unknown. | 0:01:53 | 0:02:00 | |
I like mysteries. | 0:02:00 | 0:02:02 | |
I like to think about the things that are really not understood. | 0:02:02 | 0:02:05 | |
And if I can see some way to do something to address a problem, | 0:02:05 | 0:02:10 | |
that other people haven't really followed through with, then that's what I wanna do. | 0:02:10 | 0:02:15 | |
And right now, he's believes there is nothing more intriguing and mysterious | 0:02:19 | 0:02:24 | |
than the tumbling rocks of the solar system. | 0:02:24 | 0:02:27 | |
If somebody told me 30 years ago I'd be studying asteroids, | 0:02:29 | 0:02:32 | |
I would've said, "Yeah, you're nuts. All the hot science is elsewhere." | 0:02:32 | 0:02:36 | |
Why would I spend my time on an object that basically is not going to go anywhere in my lifetime? | 0:02:36 | 0:02:43 | |
So, how wrong can you be? | 0:02:43 | 0:02:46 | |
And Dave Jewitt is not alone. | 0:02:50 | 0:02:53 | |
Oh, Gosh. I just love asteroids. I suppose it makes me geeky, right? | 0:02:53 | 0:02:59 | |
I love the motion, I love the equations of motion. I love the way all that works. | 0:02:59 | 0:03:04 | |
We've seen very few of them up close, | 0:03:08 | 0:03:10 | |
but every time we see a new one, we learn something new, we find something we weren't expecting. | 0:03:10 | 0:03:15 | |
Asteroids are the debris left over from the solar nebula. | 0:03:20 | 0:03:24 | |
They contain the raw material that never quite made it to form a planet. | 0:03:24 | 0:03:30 | |
In a way, asteroids are fossils of the early solar system. | 0:03:32 | 0:03:35 | |
On the Earth, all the materials we see have been processed | 0:03:35 | 0:03:38 | |
by being sucked into the mantle and blown out of volcanoes, | 0:03:38 | 0:03:41 | |
and so there's no material on the Earth which remembers what it was like when the Earth still formed. | 0:03:41 | 0:03:46 | |
Asteroids are time capsules that contain information | 0:03:50 | 0:03:55 | |
about the earliest times in Solar System history, | 0:03:55 | 0:03:59 | |
information that's been lost from the other planets, | 0:03:59 | 0:04:02 | |
that's been lost from the Earth, lost from the Moon. | 0:04:02 | 0:04:04 | |
Asteroids have been around, and they've seen it all. | 0:04:04 | 0:04:08 | |
Asteroids offer tantalising clues into the earliest moments of our solar system. | 0:04:12 | 0:04:18 | |
But, for these scientists, the problem is, how do you get at them? | 0:04:18 | 0:04:22 | |
For the vast majority of asteroids, we have no information at all, | 0:04:24 | 0:04:30 | |
except the existence of the object and a guess as to how big it is. | 0:04:30 | 0:04:34 | |
This fuzzy image helps explain the problem. | 0:04:39 | 0:04:42 | |
This is what an asteroid looks like through the most powerful optical telescope on earth. | 0:04:42 | 0:04:48 | |
So how do you begin to study an object you can hardly see? | 0:04:50 | 0:04:54 | |
Well, one way is to study these. | 0:04:58 | 0:05:01 | |
Tiny fragments of asteroids that have fallen to earth and broken apart, called meteorites. | 0:05:02 | 0:05:07 | |
This is it's the oldest thing you can hold in your hand, really a piece of history back to the time, | 0:05:11 | 0:05:17 | |
even before the Earth was formed, way, way before we were ever formed. | 0:05:17 | 0:05:23 | |
Almost everything we know about what asteroids are actually made of comes studying these kind of fragments. | 0:05:26 | 0:05:33 | |
Each one has its own history of the solar system, they're like a puzzle that we're trying to understand. | 0:05:33 | 0:05:40 | |
We think some asteroids are made of iron, or at least they were so large | 0:05:40 | 0:05:44 | |
that, when they formed, they heated and melted. | 0:05:44 | 0:05:47 | |
They could get all the iron to their core, | 0:05:47 | 0:05:50 | |
just like the Earth has an iron core. | 0:05:50 | 0:05:52 | |
And when we take a big iron meteor, like this, and slice it open, | 0:05:52 | 0:05:58 | |
the quality of the metal is really quite amazing. It's a very pure metal, | 0:05:58 | 0:06:06 | |
nickel iron, some of the oldest metal in the solar system, in fact. More than 4. 5 billion years old. | 0:06:06 | 0:06:13 | |
So out there in space, there are gigantic boulders, ranging in size from 900 kilometres | 0:06:19 | 0:06:25 | |
to just a few metres and made of primordial metal and dust. | 0:06:25 | 0:06:31 | |
But the more scientists have examined the remains of asteroids, the stranger they get. | 0:06:31 | 0:06:37 | |
It is probably a complete zoo. | 0:06:38 | 0:06:40 | |
And we find the meteorites have a huge variety of types and compositions. | 0:06:40 | 0:06:45 | |
And it's telling us that the asteroids must have a wide variety of compositions as well. | 0:06:45 | 0:06:51 | |
There is one type in particular that has opened a door on the strange and unfamiliar world | 0:06:51 | 0:06:58 | |
that asteroids inhabit out there in the coldness of space. | 0:06:58 | 0:07:02 | |
We think that most asteroids are probably like this, | 0:07:02 | 0:07:05 | |
very stony, like the kind of things we'd find on Earth. | 0:07:05 | 0:07:08 | |
But they have a completely different chemistry than Earth rocks. | 0:07:08 | 0:07:14 | |
They're put together like little bits of rocks all reheated, re-melted and glued together, | 0:07:14 | 0:07:22 | |
And it tells us that the asteroid belt is a place with an incredible impact history, | 0:07:22 | 0:07:27 | |
asteroids colliding into each other, breaking apart, reforming. | 0:07:27 | 0:07:31 | |
And so when we see these meteorite samples, | 0:07:31 | 0:07:34 | |
it's telling us about that amazing collision history in the asteroid belt. | 0:07:34 | 0:07:38 | |
Over 90% of asteroids are found in an orbit between Jupiter and Mars, called the main belt. | 0:07:41 | 0:07:48 | |
Almost 200 million kilometres across, it is home to millions of these orbiting rocks. | 0:07:48 | 0:07:54 | |
But perhaps the most pressing question is whether any of them | 0:07:54 | 0:07:58 | |
are on a collision course with planet Earth. | 0:07:58 | 0:08:01 | |
Arizona's arid desert air | 0:08:12 | 0:08:14 | |
makes it the perfect place for a very special kind of job. | 0:08:14 | 0:08:18 | |
This is the where people come to hunt asteroids. | 0:08:23 | 0:08:27 | |
I started out hunting asteroids about 12 years ago, as an amateur. | 0:08:30 | 0:08:34 | |
I had read an article in a popular magazine, | 0:08:36 | 0:08:39 | |
and that got me really interested in the field because not too many people were working there. | 0:08:39 | 0:08:44 | |
It might not seem it, but Richard Kowalski is in the front line of defending planet Earth. | 0:08:47 | 0:08:54 | |
Every night when I come up to the telescope, I do have it in the back of my head | 0:08:54 | 0:08:59 | |
that every person on the planet does have a vested interest in what I'm doing. | 0:08:59 | 0:09:03 | |
If one hits, there's the potential that every man, woman and child on the planet could die. | 0:09:03 | 0:09:10 | |
Richard wants to discover any asteroids that could be on a collision course with Earth. | 0:09:22 | 0:09:28 | |
This is our largest telescope it's a 60-inch or 1.5m F2. | 0:09:37 | 0:09:43 | |
It's the telescope that we've been using for approximately five years now. | 0:09:43 | 0:09:48 | |
We discover as many as 3,000 new asteroids every night. | 0:09:48 | 0:09:53 | |
But what Richard fears | 0:10:00 | 0:10:01 | |
is that one of them could create destruction like this, or worse. | 0:10:01 | 0:10:05 | |
Baringer Crater is just a few hundred kilometres | 0:10:05 | 0:10:09 | |
from Richard's telescope. | 0:10:09 | 0:10:11 | |
It is 1 kilometre across and 200 metres deep. | 0:10:15 | 0:10:20 | |
It was made when a 300,000-tonne asteroid smashed into Earth, 50,000 years ago. | 0:10:20 | 0:10:27 | |
The Earth has been hit in the past and will be hit again in the future. | 0:10:27 | 0:10:32 | |
What we'd like to do is to be able to discover these objects before they hit the Earth. | 0:10:32 | 0:10:37 | |
So, one of the great challenges for scientists is to understand | 0:10:45 | 0:10:50 | |
what would happen if an asteroid were to strike planet Earth...now. | 0:10:50 | 0:10:55 | |
Pete Schultz wants to understand the unique nature of the explosion caused | 0:11:04 | 0:11:08 | |
if an asteroid were to impact with the Earth's surface. | 0:11:08 | 0:11:12 | |
It takes a truly odd piece of equipment. | 0:11:12 | 0:11:14 | |
OK. We're getting close. | 0:11:20 | 0:11:21 | |
This was serial number one, it was built during the Apollo time, | 0:11:28 | 0:11:31 | |
I guess it's because they thought there would be several of them made | 0:11:31 | 0:11:34 | |
but this is the first one and the last one and it's the only one like it in the world. | 0:11:34 | 0:11:39 | |
This is NASA's vertical gun range. | 0:11:42 | 0:11:44 | |
It was built to study how impacts affected the moon, | 0:11:44 | 0:11:47 | |
as the astronauts prepared to make the first lunar landing. | 0:11:47 | 0:11:51 | |
We are armed, gated and reset. | 0:11:51 | 0:11:55 | |
Today, Professor Pete Schultz uses it to model precisely the dynamics of an asteroid impact. | 0:11:57 | 0:12:04 | |
We know that these asteroid impacts are bad, | 0:12:04 | 0:12:07 | |
but you want to understand really HOW bad. | 0:12:07 | 0:12:12 | |
Schultz uses the NASA gun to fire projectiles at very high speed | 0:12:14 | 0:12:18 | |
to simulate an asteroid hitting the Earth. | 0:12:18 | 0:12:22 | |
So for this experiment, we are going to fire this tiny quarter-inch aluminium sphere at very high speeds, | 0:12:22 | 0:12:28 | |
up around 5km per second, and we'll see what kind of crater it produces. | 0:12:28 | 0:12:33 | |
The target it will hit is made of sand. | 0:12:35 | 0:12:38 | |
So we use sand because it records the shock effects very clearly. | 0:12:38 | 0:12:44 | |
Outside of the impact chamber are special, super hi-speed cameras | 0:12:46 | 0:12:49 | |
that can film at up to 1 million frames per second, | 0:12:49 | 0:12:53 | |
capturing every detail of the impact and the aftermath for analysis. | 0:12:53 | 0:12:59 | |
OK, lights out. Everything good? | 0:12:59 | 0:13:03 | |
OK, we're out of here. | 0:13:03 | 0:13:04 | |
We have high voltage, warning lights. | 0:13:11 | 0:13:16 | |
And...rolling. | 0:13:17 | 0:13:19 | |
The ball travels 15 times faster than the speed of sound. | 0:13:29 | 0:13:34 | |
And it incinerates, exactly like some asteroids would. | 0:13:34 | 0:13:38 | |
Perfect. Perfect. | 0:13:40 | 0:13:42 | |
Now we're seeing the fire ball come in, | 0:13:42 | 0:13:44 | |
it's brighter than the sun and then, kapow, it hits the surface, geez. | 0:13:44 | 0:13:49 | |
This whole region down range would have been incinerated. | 0:13:49 | 0:13:54 | |
It would have been incinerated just by this plasma, this exploding vapour plume, engulfing everything. | 0:13:54 | 0:14:02 | |
There would have been winds that would have been going so fast, | 0:14:02 | 0:14:06 | |
it could pick up houses and spread them hundreds of kilometres away. | 0:14:06 | 0:14:10 | |
This would have been armageddon. | 0:14:12 | 0:14:16 | |
Experiments like this reveal several important things. | 0:14:21 | 0:14:25 | |
One is that it's not just the impact, | 0:14:25 | 0:14:27 | |
it's all that vapour that runs down range. | 0:14:27 | 0:14:30 | |
In fact, you can see areas here where there was so much wind it actually carved out pieces of this landscape. | 0:14:30 | 0:14:38 | |
So what these experiments help us do, | 0:14:38 | 0:14:41 | |
they actually allow us to witness the event, | 0:14:41 | 0:14:44 | |
see it in real time, and try to understand | 0:14:44 | 0:14:47 | |
the processes that are going on. | 0:14:47 | 0:14:50 | |
It's really complex | 0:14:50 | 0:14:52 | |
but we have to see it to understand it. | 0:14:52 | 0:14:55 | |
So asteroid impacts unleash a trail of destruction | 0:14:57 | 0:15:01 | |
far greater than suggested simply by the footprint of the crater alone. | 0:15:01 | 0:15:06 | |
It means they are far more complex, and dangerous, | 0:15:06 | 0:15:09 | |
than many had previously thought. | 0:15:09 | 0:15:11 | |
One of the enduring puzzles, | 0:15:20 | 0:15:21 | |
ever since asteroids were first discovered 200 hundred years ago, | 0:15:21 | 0:15:25 | |
is why they come anywhere close to the Earth in the first place. | 0:15:25 | 0:15:29 | |
Most of the time, asteroids | 0:15:35 | 0:15:37 | |
are in a stable orbit between Mars and Jupiter. | 0:15:37 | 0:15:40 | |
But some go wandering, leaving their orbit to propel themselves | 0:15:44 | 0:15:49 | |
through space, and coming under the influence of Jupiter's gravity... | 0:15:49 | 0:15:53 | |
a force that accelerates them towards Earth. | 0:15:53 | 0:15:58 | |
Scientists have been hunting for | 0:15:58 | 0:16:00 | |
an explanation for this strange behaviour. | 0:16:00 | 0:16:03 | |
Steve Chesley of NASA's Jet Propulsion Lab in California | 0:16:13 | 0:16:18 | |
has made a study of a 200 billion tonne asteroid called Golevka. | 0:16:18 | 0:16:23 | |
This is a model of Golevka, it's actually about | 0:16:23 | 0:16:27 | |
500 metres across, say the size of a football stadium. | 0:16:27 | 0:16:30 | |
Um, it rotates in this direction. | 0:16:30 | 0:16:33 | |
As you can see, it has a very angular shape to it. | 0:16:33 | 0:16:36 | |
He set out to investigate | 0:16:37 | 0:16:40 | |
a 100-year-old theory that said asteroids were powered | 0:16:40 | 0:16:43 | |
by the sun itself, what's called the Yarkovsky effect. | 0:16:43 | 0:16:48 | |
The Yarkovsky effect is a very small acceleration of the asteroid, | 0:16:48 | 0:16:52 | |
and what it is, is, if you take a model, | 0:16:52 | 0:16:54 | |
you see the sun is hitting the asteroid, | 0:16:54 | 0:16:56 | |
warming the surface. As the asteroid rotates, | 0:16:56 | 0:16:59 | |
that hot surface radiates the heat out | 0:16:59 | 0:17:01 | |
in a different direction into space | 0:17:01 | 0:17:03 | |
and that causes an acceleration, very slight acceleration | 0:17:03 | 0:17:05 | |
coming from the photons that are emitted from the asteroid. | 0:17:05 | 0:17:09 | |
The idea is that this acceleration, slight as it is, | 0:17:09 | 0:17:11 | |
can have significant effect upon orbit of the asteroid | 0:17:11 | 0:17:15 | |
over millions of years. | 0:17:15 | 0:17:16 | |
It was an intriguing idea. | 0:17:19 | 0:17:20 | |
What sent asteroids out of their orbit | 0:17:21 | 0:17:24 | |
and on a path towards Earth was photon propulsion. | 0:17:24 | 0:17:27 | |
But what was lacking, | 0:17:27 | 0:17:30 | |
was proof. | 0:17:30 | 0:17:31 | |
The Arecibo telescope is over 300 metres in diameter. | 0:17:39 | 0:17:43 | |
It's one of the most powerful telescopes in the world. | 0:17:43 | 0:17:47 | |
And it uses radar to map the precise position of objects in deep space. | 0:17:47 | 0:17:51 | |
It was this telescope that would allow Steve Chesley | 0:17:55 | 0:17:57 | |
to detect any tiny alterations | 0:17:57 | 0:18:00 | |
in the orbit of asteroid Golevka | 0:18:00 | 0:18:02 | |
more than 15 million kilometres out in space. | 0:18:02 | 0:18:05 | |
We knew that it would be in one place | 0:18:08 | 0:18:10 | |
if the Yarkovsky effect wasn't acting on it, | 0:18:10 | 0:18:13 | |
and would be over here if it was acting and our models were correct. | 0:18:13 | 0:18:16 | |
When Steve and his team studied the data the results were unequivocal. | 0:18:16 | 0:18:22 | |
We knew, from the radar measurements, | 0:18:22 | 0:18:25 | |
where Golevka was within a few tens of metres | 0:18:25 | 0:18:29 | |
and yet, it was actually 12 or 15 kilometres away | 0:18:29 | 0:18:32 | |
from where it was predicted to be without the Yarkovsky effect. | 0:18:32 | 0:18:36 | |
So these very precise radar observations, allowed us to see | 0:18:36 | 0:18:39 | |
the twelve kilometre displacement caused by the Yarkovsky effect. | 0:18:39 | 0:18:43 | |
So photons, those elementary, massless, particles of light, | 0:18:46 | 0:18:50 | |
really can create a tiny force. | 0:18:50 | 0:18:52 | |
The force is about | 0:18:54 | 0:18:56 | |
one ounce on Earth - say the weight of a shot glass | 0:18:56 | 0:18:58 | |
is - that's the force | 0:18:58 | 0:19:00 | |
on this huge asteroid the size of a football stadium. | 0:19:00 | 0:19:05 | |
Even for me, it's truly remarkable, it's dramatic, that a force | 0:19:05 | 0:19:09 | |
so slight can have such dramatic changes | 0:19:09 | 0:19:11 | |
on individual asteroids' orbits over millions of years. | 0:19:11 | 0:19:15 | |
Steve Chesley's research | 0:19:18 | 0:19:20 | |
means that, for as long as the sun is shining, | 0:19:20 | 0:19:23 | |
there will be a force that could send one of those asteroids | 0:19:23 | 0:19:27 | |
hurtling on a journey towards Earth. | 0:19:27 | 0:19:29 | |
Needless to say, this isn't good news. | 0:19:33 | 0:19:36 | |
But with a threat like this, what can you do? | 0:19:36 | 0:19:40 | |
Well, for now, there's really only one thing you can do... | 0:19:46 | 0:19:49 | |
and that's to keep an eye out for them. | 0:19:49 | 0:19:52 | |
Watching for asteroids is what Richard Kowalski does, | 0:20:07 | 0:20:11 | |
night after night, at his observatory in the Arizona desert. | 0:20:11 | 0:20:15 | |
What you can see on this screen is we have divided | 0:20:15 | 0:20:18 | |
the sky into thousands of areas, | 0:20:18 | 0:20:20 | |
we then choose a number of these areas into a single block | 0:20:20 | 0:20:25 | |
which will then tell the telescope | 0:20:25 | 0:20:28 | |
to observe each individual area in succession. | 0:20:28 | 0:20:31 | |
Once it's gotten to the last area, | 0:20:31 | 0:20:33 | |
it then goes back to the first area and repeats the process. | 0:20:33 | 0:20:38 | |
Over the course of an hour, | 0:20:48 | 0:20:50 | |
the telescope repeatedly scans the same areas of the sky. | 0:20:50 | 0:20:54 | |
While the stars appear stationary, the telescope can spot | 0:20:57 | 0:21:00 | |
any other objects that change position... | 0:21:00 | 0:21:03 | |
which could be asteroids. | 0:21:03 | 0:21:05 | |
As you can see, on this screen is the sequence of four images | 0:21:08 | 0:21:11 | |
that came from the telescope. | 0:21:11 | 0:21:13 | |
These objects around the screen are not moving | 0:21:13 | 0:21:16 | |
so we know that they are stars, | 0:21:16 | 0:21:18 | |
but this object in the centre is moving and thus we know | 0:21:18 | 0:21:21 | |
that is an asteroid. | 0:21:21 | 0:21:23 | |
The importance of surveying for near Earth asteroids | 0:21:25 | 0:21:28 | |
is asteroid impact on the Earth is truly the only natural disaster | 0:21:28 | 0:21:32 | |
that we can actually predict before it happens. | 0:21:32 | 0:21:35 | |
So whenever Richard finds an asteroid he thinks could be | 0:21:39 | 0:21:42 | |
on a collision course with Earth, he immediately files a report. | 0:21:42 | 0:21:46 | |
It goes to the central body whose job is to monitor | 0:21:49 | 0:21:51 | |
possible asteroid impacts. | 0:21:51 | 0:21:54 | |
Just outside Boston, is the home of the Minor Planet Centre. | 0:22:09 | 0:22:13 | |
It's director is Tim Spahr | 0:22:15 | 0:22:17 | |
and his job is to keep track of every asteroid in the solar system. | 0:22:17 | 0:22:22 | |
This is the nerve centre | 0:22:24 | 0:22:26 | |
of the entire asteroid field. | 0:22:26 | 0:22:27 | |
If somebody discovers something, it has to come through here | 0:22:27 | 0:22:30 | |
and our job is to then distribute that to the rest of the world. | 0:22:30 | 0:22:33 | |
Asteroids' elusiveness is part of the thrill. | 0:22:34 | 0:22:37 | |
In some cases, | 0:22:37 | 0:22:39 | |
if you're studying an asteroid | 0:22:39 | 0:22:41 | |
that's moving extremely fast, er, we ambush it. | 0:22:41 | 0:22:44 | |
We go ahead of where we think it will be in and set the telescope up | 0:22:44 | 0:22:46 | |
in that area and then hope that it comes through the field like that. | 0:22:46 | 0:22:50 | |
So, you know, it's actually ambushing. | 0:22:50 | 0:22:51 | |
And then when you get the asteroid, then you chase it down and follow it. | 0:22:51 | 0:22:55 | |
Not surprisingly, keeping track of thousands of objects in the sky | 0:22:59 | 0:23:03 | |
isn't something that you can do in your head. | 0:23:03 | 0:23:07 | |
Thankfully, help is at hand. | 0:23:07 | 0:23:10 | |
This is really the brains of the Minor Planet Centre right in here. | 0:23:10 | 0:23:13 | |
This computer system has information about where asteroids are, | 0:23:13 | 0:23:17 | |
where they will be in the future. | 0:23:17 | 0:23:19 | |
All the observations all the software is in here. | 0:23:19 | 0:23:21 | |
We definitely need it to be running all the time, we need it to be safe. | 0:23:21 | 0:23:25 | |
We need everything working here. | 0:23:25 | 0:23:28 | |
-< -Do you feel a sense of responsibility? | 0:23:28 | 0:23:30 | |
I definitely feel a sense of responsibility | 0:23:30 | 0:23:32 | |
for keeping a track of the asteroids. I feel like it's our duty, | 0:23:32 | 0:23:36 | |
it's our task to do that and I do feel personally responsible for it. | 0:23:36 | 0:23:40 | |
And the task facing Tim, is growing rapidly. | 0:23:44 | 0:23:46 | |
In 1999, only 10,000 asteroids were known of. | 0:23:48 | 0:23:52 | |
Since then, hundreds of thousands more, | 0:23:52 | 0:23:55 | |
of all shapes and sizes, have been discovered. | 0:23:55 | 0:23:58 | |
Tim has developed a map to visualise their location. | 0:23:58 | 0:24:03 | |
And on that map, there's one class of asteroid | 0:24:05 | 0:24:07 | |
he's concerned with above all - | 0:24:07 | 0:24:09 | |
those near-Earth asteroids closest to our planet. | 0:24:09 | 0:24:13 | |
On the screen here is a map of the solar system. | 0:24:13 | 0:24:20 | |
The Sun in the centre, and the third planet up there would the Earth. | 0:24:20 | 0:24:24 | |
The red dots in here are actually near-Earth asteroids, | 0:24:24 | 0:24:27 | |
the green ones are the regular main belt asteroids. | 0:24:27 | 0:24:31 | |
There are over 7,000 near-Earth asteroids, | 0:24:32 | 0:24:36 | |
but there's one type they are particularly concerned to locate. | 0:24:36 | 0:24:40 | |
Those asteroids that are over one kilometre in diameter. | 0:24:41 | 0:24:46 | |
These are the monsters of the skies. | 0:24:47 | 0:24:49 | |
An Earth impact with one of these | 0:24:49 | 0:24:52 | |
would spell catastrophe for the planet. | 0:24:52 | 0:24:55 | |
If a one-kilometre diameter asteroid were to hit, say, New York City, | 0:24:55 | 0:25:00 | |
that would very likely affect people in you know, 100 miles away. | 0:25:00 | 0:25:06 | |
It might kill people 100 miles away. So you're talking, really, | 0:25:06 | 0:25:09 | |
a catastrophe, instantaneously, as soon as it hits. | 0:25:09 | 0:25:13 | |
Tim's data reveals | 0:25:13 | 0:25:15 | |
that there are 900 asteroids bigger than a kilometre | 0:25:15 | 0:25:20 | |
in those dangerous near-Earth orbits. | 0:25:20 | 0:25:23 | |
But the big question - | 0:25:25 | 0:25:27 | |
are any of them on a collision course with Earth? | 0:25:27 | 0:25:31 | |
Right now, | 0:25:39 | 0:25:41 | |
there's no information that any of those large objects | 0:25:41 | 0:25:43 | |
will hit the Earth in the next 100 years. | 0:25:43 | 0:25:46 | |
So we're safe from impacts of those objects for at least 100 years. | 0:25:46 | 0:25:49 | |
But there are still smaller asteroids | 0:25:49 | 0:25:52 | |
than one kilometre that we have not yet discovered. | 0:25:52 | 0:25:55 | |
So I can't say we're safe from them | 0:25:55 | 0:25:57 | |
because we don't know where they are, just yet. | 0:25:57 | 0:25:59 | |
So, for now, we are safe from a catastrophic asteroid impact. | 0:25:59 | 0:26:06 | |
Even if the thousands of smaller asteroids might still pose a threat. | 0:26:08 | 0:26:12 | |
However another group of scientists have a very different mystery | 0:26:13 | 0:26:17 | |
about asteroids to investigate. | 0:26:17 | 0:26:19 | |
One that may help solve one of the greatest quandaries | 0:26:21 | 0:26:24 | |
about life on Earth. | 0:26:24 | 0:26:25 | |
This is Maunu Kea | 0:26:35 | 0:26:36 | |
in Hawaii. It is home | 0:26:36 | 0:26:39 | |
to some of the most powerful telescopes in the world. | 0:26:39 | 0:26:42 | |
For 30 years, Professor Dave Jewitt | 0:26:47 | 0:26:50 | |
has used them to probe deep into the solar system. | 0:26:50 | 0:26:53 | |
And once Dave interrogates deep space, | 0:26:55 | 0:26:58 | |
it's rarely ever the same again. | 0:26:58 | 0:27:00 | |
In 1992, | 0:27:03 | 0:27:04 | |
I discovered the first objects found beyond Neptune | 0:27:04 | 0:27:07 | |
since Pluto. | 0:27:07 | 0:27:09 | |
The biggest discovery in the solar system | 0:27:09 | 0:27:11 | |
since the discovery of the asteroids. | 0:27:11 | 0:27:13 | |
It was a discovery that led to Pluto losing its status as a planet, | 0:27:13 | 0:27:19 | |
something the world had taken for granted for over 60 years. | 0:27:19 | 0:27:22 | |
It established Dave's reputation as a pioneering astronomer. | 0:27:22 | 0:27:26 | |
It's important not to work on things that other people are working on. | 0:27:26 | 0:27:30 | |
All you'll do is get the same result as everybody else. You won't make | 0:27:30 | 0:27:34 | |
any discoveries, you'll just confirm what is already known. | 0:27:34 | 0:27:37 | |
Dave's desire to journey where others fear to tread | 0:27:40 | 0:27:43 | |
has led him to this. | 0:27:43 | 0:27:46 | |
This bright dot with a long hazy tail is called Elst-Pizarro. | 0:27:48 | 0:27:54 | |
It was found alongside all the other asteroids in the asteroid belt. | 0:27:56 | 0:28:00 | |
The problem was, it just didn't look like an asteroid. | 0:28:00 | 0:28:04 | |
So why did it seem so out of place? | 0:28:06 | 0:28:10 | |
it didn't look like the other asteroids so it was a freak. | 0:28:10 | 0:28:13 | |
And it got a lot of attention straightaway, | 0:28:13 | 0:28:16 | |
because it was such a remarkable object. | 0:28:16 | 0:28:18 | |
Nobody had seen anything like that before. | 0:28:18 | 0:28:21 | |
What had got them excited was that to astronomers, | 0:28:23 | 0:28:27 | |
asteroids normally look like this. | 0:28:27 | 0:28:29 | |
Just a point of light. | 0:28:29 | 0:28:31 | |
No dust cloud, and definitely no tail. | 0:28:31 | 0:28:35 | |
For years Elst-Pizarro, with its orbit of an asteroid | 0:28:38 | 0:28:41 | |
but strange fuzzy appearance, left scientists baffled. | 0:28:41 | 0:28:46 | |
Until finally, someone suggested an explanation. | 0:28:46 | 0:28:50 | |
Finally, a paper came out saying | 0:28:53 | 0:28:55 | |
it must be due to the collision between two asteroids. | 0:28:55 | 0:28:59 | |
So two asteroids slammed into each other | 0:28:59 | 0:29:01 | |
with high speed, and shattered | 0:29:01 | 0:29:04 | |
and produced a cloud of dust. | 0:29:04 | 0:29:06 | |
So the strange tail was thought to be the debris from a collision | 0:29:08 | 0:29:12 | |
between Elst-Pizarro and another asteroid. | 0:29:12 | 0:29:15 | |
And, very quickly, | 0:29:16 | 0:29:18 | |
most of the scientific world forgot about Elst-Pizarro. | 0:29:18 | 0:29:22 | |
But Dave didn't. | 0:29:23 | 0:29:24 | |
He had a hunch that there was more to this puzzling little light in the sky than at first appeared. | 0:29:27 | 0:29:33 | |
A hunch that, if proved correct, might help solve one of the great mysteries of life here on Earth. | 0:29:35 | 0:29:41 | |
Dave decided to investigate, and began looking for someone to work with. | 0:29:46 | 0:29:50 | |
Somebody with a head for the challenge. | 0:29:50 | 0:29:53 | |
When Dave suggested that I look at this object, I didn't actually know anything about it. | 0:30:01 | 0:30:05 | |
Nothing had really been said about it in the last 6 years since it's been discovered, | 0:30:05 | 0:30:10 | |
so I just decided, OK, it's just an interesting thing to take a look at. | 0:30:10 | 0:30:14 | |
Dave and Henry knew that if Elst-Pizarro's fuzzy tail really had been caused by a collision | 0:30:17 | 0:30:22 | |
the debris should have dispersed by now, | 0:30:22 | 0:30:25 | |
and Elst-Pizarro should look like a normal asteroid again. | 0:30:25 | 0:30:30 | |
But when they looked again, what they saw was that the tail was still there. | 0:30:30 | 0:30:35 | |
It was strong evidence the collision theory was wrong. | 0:30:35 | 0:30:39 | |
Collisions are very, very rare. | 0:30:42 | 0:30:45 | |
Either Elst-Pizarro is the unluckiest asteroid in the solar system, that keeps getting whacked | 0:30:45 | 0:30:49 | |
and producing dust in that way, which doesn't make any sense, | 0:30:49 | 0:30:52 | |
or there's another mechanism for producing the dust. | 0:30:52 | 0:30:55 | |
Elst-Pizarro's appearance remained an anomaly. | 0:30:56 | 0:31:00 | |
Dave and Henry realised that if they were going to make any real sense of it | 0:31:00 | 0:31:05 | |
they needed to find another example of an asteroid behaving in the same strange way. | 0:31:05 | 0:31:10 | |
Dave and Henry's problem was that, in the 200 years since asteroids were discovered, | 0:31:10 | 0:31:15 | |
Elst-Pizarro was the only one like it. | 0:31:15 | 0:31:18 | |
Finding another one could be a complete wild goose chase. | 0:31:21 | 0:31:25 | |
Using the giant telescopes on Mauna Kea, Dave and Henry began to hunt through the asteroid belt. | 0:31:29 | 0:31:36 | |
For four years, they scanned the skies. | 0:31:37 | 0:31:40 | |
They studied 300 more asteroids. | 0:31:43 | 0:31:46 | |
All of them looked identical... | 0:31:48 | 0:31:50 | |
..except for one. | 0:31:52 | 0:31:54 | |
When we saw these images, I didn't know what to think actually. | 0:31:58 | 0:32:02 | |
Maybe this is what we've been looking for all this time. | 0:32:02 | 0:32:05 | |
But we were maybe just a bit nervous. You know, we may be on the... the cusp of something big. | 0:32:05 | 0:32:12 | |
What they'd seen was an asteroid | 0:32:14 | 0:32:17 | |
sporting a tiny, faint fan-shaped tail. | 0:32:17 | 0:32:20 | |
Just like with Elst-Pizarro, they were convinced it was impossible | 0:32:22 | 0:32:26 | |
this tail was created by a collision between asteroids. | 0:32:26 | 0:32:30 | |
They had another explanation that to many seemed unthinkable. | 0:32:30 | 0:32:34 | |
This is an image of a comet. | 0:32:36 | 0:32:37 | |
They are objects that are thought to have been born | 0:32:39 | 0:32:42 | |
in the freezing outer reaches of the solar system. | 0:32:42 | 0:32:46 | |
They have long, elliptical orbits | 0:32:46 | 0:32:48 | |
that bring them towards the sun and the Earth. | 0:32:48 | 0:32:51 | |
And in comets the tail is a sign of something very special inside the centre. | 0:32:52 | 0:32:57 | |
Ice. | 0:32:59 | 0:33:00 | |
Their appearance is due to the vaporisation of the ice, that blows material off to make a tail. | 0:33:04 | 0:33:09 | |
So they have this distinctive appearance, basically of having a long tail of dust. | 0:33:09 | 0:33:13 | |
For 200 years the asteroid belt was thought to be | 0:33:16 | 0:33:19 | |
an orbiting collection of dry lumps of rock and metal. | 0:33:19 | 0:33:23 | |
Dave and Henry's new idea was that those asteroids they had observed | 0:33:24 | 0:33:29 | |
might look fuzzy and have tails because they too actually had ice inside them. | 0:33:29 | 0:33:33 | |
It was a radical suggestion, because scientists had always thought | 0:33:35 | 0:33:39 | |
asteroid orbits were far too close to the sun for them to be icy. | 0:33:39 | 0:33:43 | |
People were uncomfortable, | 0:33:46 | 0:33:48 | |
because of this prevailing idea that the asteroids are rocky, | 0:33:48 | 0:33:52 | |
and the comets are icy, and there should be nothing in-between. | 0:33:52 | 0:33:55 | |
The reason why ice in the asteroids mattered so much | 0:33:58 | 0:34:02 | |
is that it could help explain something that makes our planet unique in the solar system. | 0:34:02 | 0:34:06 | |
Our beautiful blue planet is the only one to have an abundant supply of liquid water. | 0:34:18 | 0:34:23 | |
Around 70% of the Earth's surface is covered by the oceans. | 0:34:27 | 0:34:32 | |
But there has always been a mystery as to where all this water actually came from. | 0:34:34 | 0:34:39 | |
For a decade, Dave Jewitt has been investigating this problem, | 0:34:45 | 0:34:50 | |
because scientists have established that when Earth formed, over 4.5 billion years ago, | 0:34:50 | 0:34:56 | |
it used to be a very different kind of place. | 0:34:56 | 0:34:59 | |
The early Earth was really hot. It formed from hot material in orbit around the sun. | 0:35:05 | 0:35:10 | |
So hot that we think the entire surface of the Earth | 0:35:10 | 0:35:13 | |
was covered by liquid lava for the first 100 million years, | 0:35:13 | 0:35:17 | |
a bit like the land that we see behind us. | 0:35:17 | 0:35:20 | |
Dave believes the searing heat of molten rock | 0:35:20 | 0:35:23 | |
would have had a profound effect on the Earth's early climate. | 0:35:23 | 0:35:27 | |
Because it was so hot, we also think the early Earth was very dry. | 0:35:29 | 0:35:32 | |
It's like putting something in the oven and baking it for too long. | 0:35:32 | 0:35:35 | |
It comes out bone dry. We think the Earth was bone dry when it formed. | 0:35:35 | 0:35:39 | |
That would means that the lush, wet climate that we enjoy today | 0:35:41 | 0:35:45 | |
must be the result of some dramatic events long after the Earth was born. | 0:35:45 | 0:35:49 | |
The Earth got its water some time after it had formed and cooled down, | 0:35:51 | 0:35:55 | |
by being hit by objects that carried water from somewhere else in the solar system. | 0:35:55 | 0:36:01 | |
If Dave and Henry were right, a constant stream of icy asteroids hitting the early Earth | 0:36:01 | 0:36:06 | |
could have played a vital role in bringing our planet its water. | 0:36:06 | 0:36:10 | |
But for all their observations, they hadn't actually seen ice on an asteroid. | 0:36:12 | 0:36:17 | |
So the one problem with our observations is that they only told us what the object looked like | 0:36:17 | 0:36:22 | |
and with that information we knew... we thought we could only explain it with the presence of ice | 0:36:22 | 0:36:29 | |
but we couldn't actually prove that that was the case. | 0:36:29 | 0:36:33 | |
The last piece of the jigsaw finally arrived early this year, | 0:36:37 | 0:36:42 | |
with help from the mighty telescopes of Maunu Kea. | 0:36:42 | 0:36:45 | |
Andy Rivkin makes the invisible visible, | 0:36:49 | 0:36:53 | |
by using a NASA telescope to look at objects using infrared light. | 0:36:53 | 0:36:57 | |
The infrared part of the spectrum is useful | 0:36:57 | 0:37:00 | |
because it contains information about the composition of asteroids and other objects, | 0:37:00 | 0:37:04 | |
and so by observing there you get a better handle on the composition | 0:37:04 | 0:37:08 | |
than you would if you observed only in the visible. | 0:37:08 | 0:37:10 | |
Andy studies the shape of the infrared spectrum reflected off the surface of asteroids, | 0:37:12 | 0:37:17 | |
because tiny differences in the peaks and troughs can reveal what the surface is made of. | 0:37:17 | 0:37:23 | |
Andy became interested in an asteroid called 24 Themis. | 0:37:25 | 0:37:30 | |
The shape of its spectrum | 0:37:30 | 0:37:32 | |
meant something very odd must be happening at its surface. | 0:37:32 | 0:37:36 | |
We started by comparing it to other materials and objects that we thought might be similar. | 0:37:36 | 0:37:41 | |
We tried comparing it to other asteroids, but it didn't look like any of the other asteroids. | 0:37:41 | 0:37:45 | |
We tried comparing it to meteorites, and it didn't look like any other meteorites. | 0:37:45 | 0:37:50 | |
So we knew we had to come up with some other explanation. | 0:37:50 | 0:37:53 | |
Finally, in April this year, Andy and his team published their explanation | 0:37:58 | 0:38:04 | |
as to why 24 Themis gives off such a strange kind of light. | 0:38:04 | 0:38:09 | |
We found that water ice was actually the best choice, and that was really exciting, because | 0:38:09 | 0:38:14 | |
it was the first time, certainly that we knew of, that anyone had found water ice out in the asteroid belt. | 0:38:14 | 0:38:19 | |
Even though it had been suspected for some time | 0:38:19 | 0:38:22 | |
that it could be out there, no-one had ever seen it. | 0:38:22 | 0:38:26 | |
Andy had finally proved an asteroid really could be icy. | 0:38:32 | 0:38:36 | |
It now seems certain the strange behaviour and tails | 0:38:40 | 0:38:44 | |
seen by Dave and Henry on their asteroids was caused by ice too. | 0:38:44 | 0:38:49 | |
DAVE: I think any time you make a discovery it's exciting. | 0:38:51 | 0:38:55 | |
Any time you find a new thing, it's a big thrill. | 0:38:55 | 0:38:58 | |
Definitely a big thrill, yeah. | 0:38:58 | 0:39:00 | |
Cos it's hard. | 0:39:00 | 0:39:02 | |
It means that asteroids could have played | 0:39:04 | 0:39:07 | |
one of the most important roles in creating the Earth we see today. | 0:39:07 | 0:39:12 | |
We know that asteroids did hit the Earth, for billions of years. | 0:39:15 | 0:39:19 | |
The question is what the asteroids brought with them. | 0:39:19 | 0:39:21 | |
We previously thought mostly rock and metal. | 0:39:21 | 0:39:23 | |
Now we understand that the asteroids would also have brought | 0:39:23 | 0:39:27 | |
a lot more water and ice than we'd previously suspected. | 0:39:27 | 0:39:30 | |
These discoveries are starting to change our understanding of the solar system. | 0:39:31 | 0:39:36 | |
Water and ice really are abundant in the asteroid belt. | 0:39:36 | 0:39:41 | |
And that maybe water and ice | 0:39:42 | 0:39:45 | |
is more abundant throughout the entire inner solar system. | 0:39:45 | 0:39:50 | |
Finding the water in the asteroid belt is the key to starting to change | 0:39:50 | 0:39:55 | |
our thinking about where Earth's water may have come from. | 0:39:55 | 0:39:59 | |
Astronomers still don't know how much of Earth's water came from asteroids | 0:40:04 | 0:40:10 | |
and how much from other sources of ice such as comets. | 0:40:10 | 0:40:13 | |
Without that water, of course, life on Earth could not exist. | 0:40:16 | 0:40:20 | |
Which provokes what is perhaps the most intriguing question of all. | 0:40:23 | 0:40:28 | |
Did asteroids play a role in the creation of life? | 0:40:28 | 0:40:32 | |
Not far from San Francisco, California, | 0:40:46 | 0:40:49 | |
there are scientists pondering this very question. | 0:40:49 | 0:40:53 | |
Scott Sandford wants to investigate whether the basic chemicals of life could have been formed in space, | 0:40:53 | 0:40:59 | |
perhaps even on an asteroid. | 0:40:59 | 0:41:01 | |
So he's created the conditions of deep space in a machine. | 0:41:02 | 0:41:06 | |
This machine has been developed to allow us to simulate environmentsthat are out in space, | 0:41:09 | 0:41:14 | |
either in the interstellar medium, events where stars form, | 0:41:14 | 0:41:17 | |
or the environments, let's say, in the icy satellites of planets in the outer solar system. | 0:41:17 | 0:41:22 | |
Environments that have low temperatures, no air, so vacuum, and high radiation fields. | 0:41:22 | 0:41:29 | |
He wants to see if the complex carbon molecules that are essential to life | 0:41:32 | 0:41:36 | |
could be created from the much simpler chemicals found in space. | 0:41:36 | 0:41:40 | |
In this chamber is a sample probe covered in a tiny layer of water, methanol and pyrimidine | 0:41:43 | 0:41:50 | |
that is frozen to just 20 degrees above absolute zero, and exposed to intense ultraviolet light. | 0:41:50 | 0:41:57 | |
In this particular experiment we're looking at whether certain conditions will form one of the nucleobases, | 0:41:57 | 0:42:03 | |
so one of the molecules that makes up our DNA. | 0:42:03 | 0:42:06 | |
And from his analysis of samples from experiments like this, | 0:42:08 | 0:42:13 | |
Scott has made a remarkable discovery. | 0:42:13 | 0:42:16 | |
By processing ices of the type we see out in space, we can make | 0:42:17 | 0:42:20 | |
some of the building blocks that we see in biology on the Earth today. | 0:42:20 | 0:42:25 | |
We're making the building blocks of life, that's what we're finding. | 0:42:25 | 0:42:29 | |
Just because you can create these building blocks of life in a lab, | 0:42:31 | 0:42:35 | |
it doesn't mean it really happens on an asteroid. | 0:42:35 | 0:42:38 | |
So Scott has carefully examined meteorite samples to see if they contain traces of these chemicals. | 0:42:39 | 0:42:46 | |
In some classes of meteorites, which we think | 0:42:46 | 0:42:49 | |
come from asteroids, we find a variety of organic compounds. | 0:42:49 | 0:42:53 | |
And these include things that some people are familiar with, | 0:42:53 | 0:42:56 | |
like amino acids, the building blocks of proteins in our bodies, | 0:42:56 | 0:42:59 | |
but also materials like the nucleobases, the building blocks of DNA. | 0:42:59 | 0:43:04 | |
So hidden within the rock could have been the materials | 0:43:06 | 0:43:09 | |
that made possible the emergence of life on Earth. | 0:43:09 | 0:43:12 | |
And that means that when asteroids struck Earth billions of years ago | 0:43:15 | 0:43:21 | |
they could have completely transformed our planet. | 0:43:21 | 0:43:23 | |
Asteroids could have played an important role in getting life started on Earth | 0:43:26 | 0:43:30 | |
by delivering the raw starting materials that we need to get everything going to get life started. | 0:43:30 | 0:43:35 | |
It seems the story of life on Earth is inextricably linked to the story... | 0:43:38 | 0:43:43 | |
of asteroids. | 0:43:43 | 0:43:44 | |
The possibility that asteroids hold the key to some of the deepest mysteries about our planet explains | 0:44:01 | 0:44:08 | |
why scientists have always dreamt of reaching out into space and bringing back a pristine asteroid sample. | 0:44:08 | 0:44:14 | |
And earlier this year, that wish may finally have come true. | 0:44:16 | 0:44:21 | |
In June, one of the strangest space missions in history came to an end. | 0:44:31 | 0:44:36 | |
It might look like a firework display, but this | 0:44:41 | 0:44:44 | |
is actually a Japanese spacecraft re-entering the Earth's atmosphere. | 0:44:44 | 0:44:48 | |
Seven years after it first left the Earth, the Hayabusa probe landed in the Australian desert. | 0:44:54 | 0:45:01 | |
The scientific team were careful to handle the crashed probe with extreme caution. | 0:45:03 | 0:45:08 | |
Because within this small container is what scientists hope will be the | 0:45:11 | 0:45:15 | |
first ever asteroid sample collected directly from space. | 0:45:15 | 0:45:20 | |
The sample consists a lot of little grains, and some of the grains are as small as ten microns, | 0:45:20 | 0:45:26 | |
so ten millionths of a metre across, so this is a particle smaller than the width of a human hair. | 0:45:26 | 0:45:32 | |
Even in a microscope it looks like a dot, OK, and so, um, | 0:45:32 | 0:45:36 | |
the analyses of such small samples is obviously complicated. | 0:45:36 | 0:45:41 | |
Obviously our hope is that some of that material really is from | 0:45:41 | 0:45:45 | |
the asteroid, but at this point we don't know for sure one way or the other. | 0:45:45 | 0:45:49 | |
It may be months or even years, before the team discovers what if anything these grains can reveal. | 0:45:49 | 0:45:56 | |
While many scientists are excited about what | 0:45:56 | 0:45:59 | |
asteroids might tell us about the beginnings of life on Earth, | 0:45:59 | 0:46:02 | |
new research suggests that it is how asteroids might put an end to life that should really concern us. | 0:46:02 | 0:46:09 | |
On the 6th of October 2008 | 0:46:18 | 0:46:20 | |
asteroid hunter Richard Kowalski saw something that would | 0:46:20 | 0:46:24 | |
help change the assessment of the threat presented by asteroid impacts. | 0:46:24 | 0:46:27 | |
The night was proceeding normally and up on the screen came another asteroid. | 0:46:27 | 0:46:34 | |
As I continued to make observations throughout the night it appeared to be moving slightly faster. | 0:46:34 | 0:46:39 | |
And this indicates that the object is close to the Earth. | 0:46:39 | 0:46:43 | |
As with any other asteroid, Richard reported what he'd found to the Minor Planet Center. | 0:46:43 | 0:46:50 | |
I got up in the morning, about 7 o'clock. | 0:46:53 | 0:46:56 | |
I had a message from the computer saying, "could not compute an orbit for a particular object". | 0:46:56 | 0:47:02 | |
I grabbed the observations of this object and I computed an orbit | 0:47:02 | 0:47:06 | |
and it was immediately apparent, right then, that that object was going to hit the Earth. | 0:47:06 | 0:47:12 | |
and sort of ominous fashion, it said it was in 19 hours. | 0:47:12 | 0:47:17 | |
Following a strict written protocol, Tim quickly reported the findings | 0:47:19 | 0:47:23 | |
to NASA's asteroid investigation team in California. | 0:47:23 | 0:47:26 | |
We got a call from Tim Spahr | 0:47:29 | 0:47:31 | |
at the Minor Planet Center saying we had an | 0:47:31 | 0:47:33 | |
impacter coming in, in less than 24 hours. | 0:47:33 | 0:47:36 | |
So that woke me up. | 0:47:36 | 0:47:37 | |
NASA's expert on asteroid orbits, Steve Chesley, immediately started to verify the data. | 0:47:39 | 0:47:45 | |
Steve The first thing I saw was a 1.000, | 0:47:45 | 0:47:48 | |
100% probability of impact and erm, in less than a days' time. | 0:47:48 | 0:47:51 | |
This I'd never seen, anything like this outside of simulations and software testing. | 0:47:51 | 0:47:55 | |
An asteroid strike would create a huge explosion. | 0:47:57 | 0:48:00 | |
NASA feared this might be mistaken for a nuclear bomb. | 0:48:00 | 0:48:04 | |
We wanted folks to know that this was a natural event by mother nature | 0:48:04 | 0:48:08 | |
rather than some sort of a man-made event like a missile or something dreadful. | 0:48:08 | 0:48:14 | |
Information passed rapidly up the chain of command. | 0:48:14 | 0:48:17 | |
So, NASA headquarters notified the Whitehouse | 0:48:17 | 0:48:20 | |
that this was coming. | 0:48:20 | 0:48:22 | |
Everyone wanted to know where it would strike | 0:48:22 | 0:48:25 | |
NASA predicted a remote area of the Nubian desert. | 0:48:26 | 0:48:31 | |
AT quarter to three in the morning, NASA were proved right. | 0:48:39 | 0:48:46 | |
The explosion created a vast fireball burning as hot as the sun. | 0:48:46 | 0:48:50 | |
It was so big and so hot, this image was captured by a weather satellite. | 0:48:52 | 0:48:57 | |
As dawn broke, the smoke trail it left behind was still visible from the ground. | 0:49:00 | 0:49:05 | |
I definitely think the impact was a wake-up call. | 0:49:07 | 0:49:11 | |
I have to admit I never thought I'd see that in my career, where we would | 0:49:11 | 0:49:14 | |
discover something that would hit the Earth later that day. | 0:49:14 | 0:49:17 | |
What makes this impact so worrying is that this asteroid was too small | 0:49:19 | 0:49:24 | |
for anyone to see until it was very, very close to the Earth | 0:49:24 | 0:49:29 | |
For one scientist, it's was a salutary reminder that | 0:49:32 | 0:49:37 | |
we cannot afford to ignore the threat posed by small asteroids. | 0:49:37 | 0:49:40 | |
Physicist Mark Boslough uses one of the world's most powerful | 0:49:42 | 0:49:46 | |
supercomputers to study the hazards facing our planet, from climate change to nuclear explosions. | 0:49:46 | 0:49:53 | |
But for years, he's been fascinated by a strange event at the beginning of the last century, | 0:49:53 | 0:50:00 | |
and what it might tell us about the threat of asteroid impacts. | 0:50:00 | 0:50:04 | |
On June 30th 1908, without warning, | 0:50:07 | 0:50:11 | |
a massive explosion wiped out | 0:50:11 | 0:50:14 | |
over 1,500 square kilometres of Siberian forest. | 0:50:14 | 0:50:17 | |
Millions of trees were destroyed. | 0:50:17 | 0:50:23 | |
Scientists thought it had been caused by an asteroid strike. | 0:50:23 | 0:50:27 | |
But then why was there no sign of any kind of impact crater? | 0:50:29 | 0:50:34 | |
The answer is that the devastation had to be caused by an asteroid attack of a very particular kind. | 0:50:35 | 0:50:42 | |
The explosion was caused by an asteroid that entered the atmosphere, | 0:50:44 | 0:50:48 | |
got close to the surface and exploded before it hit the ground. | 0:50:48 | 0:50:52 | |
That explosion created a blast wave with hurricane-force winds | 0:50:52 | 0:50:56 | |
that knocked trees over for thousands of square miles. | 0:50:56 | 0:51:00 | |
Scientists call it an air burst - a massive explosion in the atmosphere rather than on the ground. | 0:51:04 | 0:51:11 | |
As it enters the atmosphere at speeds of up to 20 kilometres per second | 0:51:14 | 0:51:18 | |
the air resistance decelerates the | 0:51:18 | 0:51:20 | |
asteroid so fast it breaks apart in a huge explosion. | 0:51:20 | 0:51:25 | |
And crucially, it is small asteroids that are most likely to explode in this way. | 0:51:27 | 0:51:32 | |
Most of the damage from an explosion like this is actually the blast waves, it's the very high winds. | 0:51:32 | 0:51:38 | |
Based on the physics of nuclear explosions, | 0:51:41 | 0:51:45 | |
the original air burst model estimates the Tunguska explosion | 0:51:45 | 0:51:49 | |
must have been 1,000 times bigger than the nuclear bombs at Hiroshima and Nagasaki. | 0:51:49 | 0:51:54 | |
But crucially, the air burst model suggests the | 0:51:56 | 0:51:59 | |
asteroid would have packed this huge destructive force | 0:51:59 | 0:52:03 | |
even though it was as small as 100 metres in diameter. | 0:52:03 | 0:52:07 | |
But Mark realised there was another problem. | 0:52:07 | 0:52:11 | |
The model was ignoring a crucial difference between nuclear bomb air bursts, and asteroids. | 0:52:11 | 0:52:18 | |
Asteroids are extremely heavy and move so fast that they carry huge momentum | 0:52:19 | 0:52:25 | |
He created a new simulation to investigate the effect this would have on their destructive power. | 0:52:27 | 0:52:33 | |
In this simulation I include more of the physics to be more realistic, you can see that the main shockwave | 0:52:34 | 0:52:40 | |
doesn't come out of the point of the explosion, but it comes out from the point where the fireball descends to. | 0:52:40 | 0:52:46 | |
so by the time the shockwave hit the ground it's much stronger | 0:52:46 | 0:52:49 | |
than it would otherwise be so there is more damage on the ground, | 0:52:49 | 0:52:52 | |
because the destructive power was carried downward. | 0:52:52 | 0:52:55 | |
Based on Mark's new calculations, the devastation at Tunguska could have been caused | 0:52:58 | 0:53:04 | |
by an asteroid only one third as large as previous estimates. | 0:53:04 | 0:53:09 | |
Perhaps as small as 30-50 metres in diameter. | 0:53:09 | 0:53:13 | |
And for him this carries a worrying implication. | 0:53:13 | 0:53:17 | |
Smaller asteroids are more dangerous than we used to think and because there are so many | 0:53:20 | 0:53:24 | |
more smaller asteroids than bigger asteroids we need to take that risk more seriously than we used to. | 0:53:24 | 0:53:31 | |
Mark's work means scientists may have to redraw the asteroid threat map. | 0:53:33 | 0:53:37 | |
If a Tunguska scale asteroid exploded over London or New York it | 0:53:37 | 0:53:41 | |
would be very destructive, it would be as destructive as a nuclear bomb exploding over one of those cities. | 0:53:41 | 0:53:47 | |
Scientists estimate that there could be over a million of these kinds of asteroids up in space. | 0:53:49 | 0:53:55 | |
But nobody knows where they are, or where they are headed. | 0:53:55 | 0:54:00 | |
A 2010 report by the American National Academies of Sciences, | 0:54:06 | 0:54:10 | |
was so concerned about the potential threat | 0:54:10 | 0:54:13 | |
to Earth from the smallest kind of asteroids, that it has called for a new survey to track them down. | 0:54:13 | 0:54:19 | |
The problems is that even for dedicated asteroid hunters like | 0:54:22 | 0:54:26 | |
Richard Kowalski, they are extremely hard to find. | 0:54:26 | 0:54:30 | |
Many of them are as dark as a charcoal briquette and we see them by reflected sunlight. | 0:54:30 | 0:54:36 | |
So you can imagine a 100-metre charcoal briquette out in space is going to be kind of hard to see. | 0:54:36 | 0:54:42 | |
And that means that if an asteroid like this is heading for Earth, | 0:54:46 | 0:54:50 | |
we might only see it when it is very close, with very little warning. | 0:54:50 | 0:54:55 | |
There's a reasonable chance that you'll see it for the first time, on | 0:54:55 | 0:55:00 | |
it's terminal trajectory, just days, or weeks, before the impact. | 0:55:00 | 0:55:05 | |
If that were to happen, there is nothing that anyone could to stop it from hitting the Earth. | 0:55:07 | 0:55:14 | |
For the public authorities, the only option, would be to try to get | 0:55:16 | 0:55:20 | |
the thousands or even millions of people out of the impact zone. | 0:55:20 | 0:55:24 | |
I think Katrina, Hurricane Katrina, | 0:55:28 | 0:55:31 | |
really illustrated how hard it is to evacuate a large area. | 0:55:31 | 0:55:34 | |
It's not set up that we have an asteroid evacuation plan | 0:55:36 | 0:55:40 | |
in place right now. | 0:55:40 | 0:55:42 | |
I know it's been discussed at the UN, but if we were to be | 0:55:44 | 0:55:50 | |
issued 3 days' warning, I really don't know what would happen. | 0:55:50 | 0:55:54 | |
And it wouldn't be very good. | 0:55:54 | 0:55:55 | |
I'm sure we're not ready for that yet. | 0:55:55 | 0:55:58 | |
However far away they may be, | 0:56:08 | 0:56:10 | |
and however difficult to find, | 0:56:10 | 0:56:12 | |
scientists now understand that Earth's past | 0:56:12 | 0:56:15 | |
and its future cannot be separated from these tiny rocks of destiny. | 0:56:15 | 0:56:20 | |
The quest to understand them will continue on Earth and from space. | 0:56:20 | 0:56:26 | |
NASA currently has a spacecraft en route to visit two of the largest asteroids | 0:56:31 | 0:56:36 | |
in the solar system. | 0:56:36 | 0:56:37 | |
It will arrive in July 2011. | 0:56:37 | 0:56:41 | |
And President Obama has challenged NASA to send astronauts to an asteroid by 2025. | 0:56:41 | 0:56:47 | |
200 years after they were first discovered, | 0:56:47 | 0:56:50 | |
solar system science has finally entered the age of the asteroids. | 0:56:50 | 0:56:55 | |
The good, the bad and the ugly. | 0:56:55 | 0:56:59 | |
Are asteroids bad, good or ugly? | 0:56:59 | 0:57:02 | |
I'd say all of the above. | 0:57:02 | 0:57:05 | |
I wouldn't say that asteroids are good or bad. | 0:57:05 | 0:57:08 | |
They essentially created the solar system we live in | 0:57:08 | 0:57:11 | |
and the planet that we live on. | 0:57:11 | 0:57:13 | |
They've shaped the Earth in ways, it's safe to say, humans wouldn't be around | 0:57:13 | 0:57:18 | |
but for the asteroid impact. | 0:57:18 | 0:57:20 | |
I take asteroids like people - I take them as I find them | 0:57:20 | 0:57:24 | |
and try to learn their individual foibles. | 0:57:24 | 0:57:27 | |
I think ultimately asteroids will be our friends | 0:57:27 | 0:57:31 | |
because they have the capability of giving us resources for use as we try to explore | 0:57:31 | 0:57:36 | |
and extend our reach into space. | 0:57:36 | 0:57:38 | |
Asteroids are certainly not ugly. Asteroids are beautiful. | 0:57:38 | 0:57:42 | |
The ones that we don't understand, I think that makes them more beautiful. | 0:57:42 | 0:57:48 | |
That's the beauty of science. That's why we keep doing it. | 0:57:48 | 0:57:51 | |
It's to try to learn more things and when we get a curve ball thrown in, | 0:57:51 | 0:57:55 | |
that's part of the process. That's the fun. | 0:57:55 | 0:57:59 | |
I have an asteroid named after myself. It's (2956) Yeomans. | 0:58:03 | 0:58:08 | |
That's quite a hoot. | 0:58:08 | 0:58:10 | |
I do have an asteroid and this is it. | 0:58:12 | 0:58:16 | |
(17857) Hsieh 1998KR1 | 0:58:16 | 0:58:20 | |
I have an asteroid. It's called (6434) Jewitt. It makes me feel like I'm part of the cosmos. | 0:58:24 | 0:58:31 | |
I have an asteroid named after me. Pete Schulz. It looks like I've got a bullet with my name on it. | 0:58:33 | 0:58:39 | |
HE LAUGHS | 0:58:39 | 0:58:41 | |
Subtitling by Red Bee Media Ltd | 0:58:42 | 0:58:45 | |
E-mail: [email protected] | 0:58:45 | 0:58:47 |