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There are some mysteries when we look around the solar system, | 0:00:09 | 0:00:12 | |
where the theories really don't match what we see. | 0:00:12 | 0:00:15 | |
Science fact can be a lot weirder than science fiction. | 0:00:20 | 0:00:23 | |
We started finding planets | 0:00:26 | 0:00:27 | |
in places we'd never thought could possibly form a planet. | 0:00:27 | 0:00:31 | |
We had to go back to the drawing board. | 0:00:31 | 0:00:33 | |
How do you make solar systems? How do you make planets? | 0:00:36 | 0:00:38 | |
It's as if somebody took the solar system, | 0:00:40 | 0:00:42 | |
picked it up and shook it real hard. | 0:00:42 | 0:00:45 | |
Our planets might have moved. | 0:00:45 | 0:00:47 | |
They might have moved a lot. | 0:00:47 | 0:00:48 | |
All of a sudden, everything changed. | 0:00:48 | 0:00:50 | |
It's changed the way we look at | 0:00:56 | 0:00:57 | |
almost every process in the solar system. | 0:00:57 | 0:01:00 | |
Sometimes the blood splattered on the wall | 0:01:02 | 0:01:05 | |
can tell you more about what happened | 0:01:05 | 0:01:07 | |
than the body lying on the floor. | 0:01:07 | 0:01:08 | |
The Royal Observatory in Greenwich | 0:01:29 | 0:01:31 | |
is the historical home of British astronomy. | 0:01:31 | 0:01:34 | |
Discoveries have been made here and mysteries unravelled. | 0:01:37 | 0:01:42 | |
It is also home to some unique astronomical treasures. | 0:01:42 | 0:01:46 | |
This is an orrery, | 0:01:49 | 0:01:51 | |
a clockwork model of the solar system, | 0:01:51 | 0:01:54 | |
and for most of the last four centuries | 0:01:54 | 0:01:56 | |
this has been the way we think about the planets in the solar system. | 0:01:56 | 0:02:00 | |
Of course, the scale is all wrong. | 0:02:01 | 0:02:04 | |
But it clearly shows the traditional view of the planets | 0:02:04 | 0:02:07 | |
and their fixed orbits. | 0:02:07 | 0:02:08 | |
In the centre we have the sun | 0:02:08 | 0:02:11 | |
and then, around it, we have the four rocky planets, | 0:02:11 | 0:02:15 | |
tiny Mercury rushing around in the middle, | 0:02:15 | 0:02:18 | |
Venus, the earth with the moon going around it, | 0:02:18 | 0:02:21 | |
and then Mars. | 0:02:21 | 0:02:23 | |
And outside of the inner planets, | 0:02:23 | 0:02:25 | |
we have the gas giants, | 0:02:25 | 0:02:27 | |
Jupiter, the largest planet of all, | 0:02:27 | 0:02:29 | |
and then Saturn with its beautiful ring system. | 0:02:29 | 0:02:32 | |
And then the two outermost planets, Uranus and Neptune. | 0:02:32 | 0:02:35 | |
Astronomers always thought that the planets have been fixed | 0:02:37 | 0:02:40 | |
in these orbits since they formed, more than 4 billion years ago. | 0:02:40 | 0:02:44 | |
Long enough for the earth to develop into the haven it is today | 0:02:45 | 0:02:49 | |
for life to evolve. | 0:02:49 | 0:02:51 | |
A mechanical model like this embodies an idea | 0:02:51 | 0:02:54 | |
of the solar system in which the planets all keep | 0:02:54 | 0:02:57 | |
to these very neat, orderly orbits, | 0:02:57 | 0:03:00 | |
moving essentially in circles and at fixed distances from the sun. | 0:03:00 | 0:03:05 | |
And the natural assumption to make is that everything we see now | 0:03:05 | 0:03:10 | |
formed where it is and has stayed there ever since. | 0:03:10 | 0:03:13 | |
The idea that the planets are fixed in their orbits | 0:03:15 | 0:03:19 | |
has been the bedrock of our understanding for hundreds of years. | 0:03:19 | 0:03:23 | |
But there are some mysteries about our solar system | 0:03:23 | 0:03:26 | |
that mean we may have to rethink everything we thought we knew. | 0:03:26 | 0:03:30 | |
It's time for a brand-new model. | 0:03:33 | 0:03:36 | |
DRAMATIC DRUMBEAT | 0:03:36 | 0:03:38 | |
Recently, astronomers have started to unravel | 0:03:47 | 0:03:50 | |
the mystery of how the solar system came to be. | 0:03:50 | 0:03:52 | |
And to explore it | 0:03:54 | 0:03:56 | |
we first need a more accurate picture of our planets. | 0:03:56 | 0:03:59 | |
We need to alter the scale to reflect the huge difference in size. | 0:04:03 | 0:04:07 | |
For example, Jupiter, the largest planet, | 0:04:07 | 0:04:11 | |
is 11 times the radius of the Earth, | 0:04:11 | 0:04:14 | |
and if you look at the masses, the difference is even greater. | 0:04:14 | 0:04:17 | |
Jupiter has about 300 times the mass of planet Earth. | 0:04:17 | 0:04:21 | |
The sun we've left alone. | 0:04:23 | 0:04:26 | |
If we scaled that up too it would fill half the room. | 0:04:26 | 0:04:31 | |
And, of course, the planets are not all bunched up. | 0:04:31 | 0:04:34 | |
MECHANICAL WHIRRING | 0:04:34 | 0:04:36 | |
We need to push the gas and ice giants much further away. | 0:04:39 | 0:04:42 | |
To be truly accurate, with the planets this size | 0:04:47 | 0:04:50 | |
we'd have to make the orbits several thousand times bigger. | 0:04:50 | 0:04:53 | |
However, exactly how we ended up with this neat | 0:04:59 | 0:05:02 | |
and stable arrangement of planets | 0:05:02 | 0:05:04 | |
is still one of the greatest mysteries in astronomy. | 0:05:04 | 0:05:07 | |
In trying to solve this mystery, | 0:05:14 | 0:05:16 | |
we may discover how the earth came to inhabit | 0:05:16 | 0:05:19 | |
the perfect position for life to evolve. | 0:05:19 | 0:05:21 | |
Getting an earth where we have our earth today | 0:05:23 | 0:05:26 | |
was not a given when this whole solar system started. | 0:05:26 | 0:05:29 | |
We may be able to understand the remarkable chain of events | 0:05:32 | 0:05:36 | |
that created the biggest game of pinball in the galaxy... | 0:05:36 | 0:05:38 | |
The solar system could have done a lot of different things, | 0:05:39 | 0:05:42 | |
it could have evolved in a lot of different ways. | 0:05:42 | 0:05:44 | |
We could have ended up with our Jupiter right next to the sun. | 0:05:44 | 0:05:47 | |
And it looks like it was Jupiter | 0:05:48 | 0:05:50 | |
that defined the fate of the solar system. | 0:05:50 | 0:05:53 | |
The giant planets' story IS the story of our solar system. | 0:05:54 | 0:05:59 | |
We like to think that the earth is really important, | 0:05:59 | 0:06:01 | |
but the truth is that, if you were looking from afar, | 0:06:01 | 0:06:04 | |
our solar system is mainly four big planets and some debris. | 0:06:04 | 0:06:07 | |
Could our place in the universe | 0:06:09 | 0:06:11 | |
really be nothing more than a lucky accident? | 0:06:11 | 0:06:15 | |
The question that really arises | 0:06:15 | 0:06:16 | |
is how common is a solar system like ours? | 0:06:16 | 0:06:20 | |
The mystery of the birth of the solar system is set to unravel. | 0:06:23 | 0:06:27 | |
As they try to work out how our solar system formed, | 0:06:34 | 0:06:37 | |
astronomers have noticed some baffling puzzles. | 0:06:37 | 0:06:40 | |
If we look at the solar system as it is today, | 0:06:40 | 0:06:43 | |
it seems quite neat and simple. | 0:06:43 | 0:06:46 | |
We have four small, rocky planets close to the sun | 0:06:46 | 0:06:49 | |
and then four enormous giants further out. | 0:06:49 | 0:06:53 | |
But when we try to model the formation of the solar system | 0:06:53 | 0:06:56 | |
on a computer, something doesn't quite add up. | 0:06:56 | 0:06:59 | |
It's really hard to get the model | 0:06:59 | 0:07:01 | |
to make the planets in the places where we see them today. | 0:07:01 | 0:07:04 | |
Take, for instance, the curious case | 0:07:09 | 0:07:12 | |
of the undersized planet Mars. | 0:07:12 | 0:07:14 | |
If we look at the rocky innermost planets, | 0:07:14 | 0:07:17 | |
Venus and Earth have about the same mass, | 0:07:17 | 0:07:20 | |
and we'd expect Mars to have a similar mass too, | 0:07:20 | 0:07:22 | |
but it actually doesn't. | 0:07:22 | 0:07:24 | |
It's only about one tenth the mass of the earth or Venus, | 0:07:24 | 0:07:27 | |
and that's a mystery that's very hard to explain. | 0:07:27 | 0:07:30 | |
This is the first of four key puzzles | 0:07:32 | 0:07:35 | |
about the birth of the solar system that remain unsolved. | 0:07:35 | 0:07:39 | |
And then, at the edge of the solar system, | 0:07:40 | 0:07:42 | |
the two outermost planets, Uranus and Neptune, | 0:07:42 | 0:07:46 | |
are much further away from the sun than we'd expect. | 0:07:46 | 0:07:49 | |
It's very hard to explain how they could have formed | 0:07:49 | 0:07:52 | |
and become so large at that great distance from the central star. | 0:07:52 | 0:07:56 | |
If we go in and look at the asteroid belt, | 0:07:57 | 0:08:00 | |
there are thousands of small, rocky objects there, | 0:08:00 | 0:08:03 | |
but there are two broad types - | 0:08:03 | 0:08:05 | |
some of them are very rocky and some have more of an icy content. | 0:08:05 | 0:08:09 | |
And yet these two types are actually found | 0:08:09 | 0:08:11 | |
relatively close together. | 0:08:11 | 0:08:13 | |
It seems as though they formed under different circumstances | 0:08:13 | 0:08:16 | |
but they've all ended up in roughly the same place. | 0:08:16 | 0:08:19 | |
And, again, it's a mystery as to how that happened. | 0:08:19 | 0:08:21 | |
And, closer to home, | 0:08:23 | 0:08:25 | |
how to explain the rapid and massive bombardment | 0:08:25 | 0:08:28 | |
that left the moon covered in craters. | 0:08:28 | 0:08:30 | |
There are many mysteries in the solar system, | 0:08:33 | 0:08:36 | |
but by unravelling these four - | 0:08:36 | 0:08:38 | |
the size of Mars, | 0:08:38 | 0:08:39 | |
the formation of the outer planets, | 0:08:39 | 0:08:42 | |
the composition of the asteroid belt | 0:08:42 | 0:08:44 | |
and the bombardment of the moon - | 0:08:44 | 0:08:46 | |
we may be able to explain how our planet Earth | 0:08:46 | 0:08:49 | |
found itself in a perfect position for life to evolve. | 0:08:49 | 0:08:53 | |
And it all starts a long, | 0:08:55 | 0:08:57 | |
long time ago. | 0:08:57 | 0:08:59 | |
DRAMATIC DRUMBEAT | 0:09:01 | 0:09:03 | |
Four and a half billion years ago, | 0:09:13 | 0:09:16 | |
our sun burst into life | 0:09:16 | 0:09:18 | |
from the collapse of a massive cloud of gas and dust. | 0:09:18 | 0:09:21 | |
So, in the beginning, | 0:09:23 | 0:09:24 | |
this is what you have in our early solar system. | 0:09:24 | 0:09:26 | |
You have the young star just born, | 0:09:26 | 0:09:28 | |
and the leftovers, just a cloud of gas, | 0:09:28 | 0:09:33 | |
the nebula, the protoplanetary nebula, | 0:09:33 | 0:09:35 | |
full of hydrogen and helium, | 0:09:35 | 0:09:37 | |
dust and gas, | 0:09:37 | 0:09:40 | |
and ice grains forming. | 0:09:40 | 0:09:42 | |
And from this, eventually, you form the planets. | 0:09:42 | 0:09:46 | |
We know surprisingly little about exactly how planets are formed. | 0:09:47 | 0:09:51 | |
Most mysterious of all is the most important - | 0:09:51 | 0:09:55 | |
the largest of all planets, Jupiter, | 0:09:55 | 0:09:58 | |
which seems to have been made first. | 0:09:58 | 0:10:00 | |
The first-born - giant, massive Jupiter. | 0:10:01 | 0:10:05 | |
The meanest and largest of all the planets. | 0:10:05 | 0:10:08 | |
It sucks up more than half of the existing nebula | 0:10:09 | 0:10:12 | |
and becomes the king of the solar system. | 0:10:12 | 0:10:15 | |
We know that Jupiter is made up almost entirely | 0:10:17 | 0:10:20 | |
of the hydrogen and helium left over in this primordial cloud. | 0:10:20 | 0:10:24 | |
Which means it must have formed incredibly quickly | 0:10:25 | 0:10:29 | |
because, as the new sun heated up, it would have blasted the gas away. | 0:10:29 | 0:10:33 | |
And so there's a time limit. | 0:10:36 | 0:10:38 | |
Jupiter must have formed in the astronomical blink of an eye - | 0:10:38 | 0:10:42 | |
just five million years. | 0:10:42 | 0:10:44 | |
But exactly how it grew so fast and why it grew where it did | 0:10:46 | 0:10:50 | |
remains shrouded in mystery. | 0:10:50 | 0:10:52 | |
It's a mystery that Scott Bolton is hoping to shed some light on. | 0:11:01 | 0:11:05 | |
He's sending a spaceship to Jupiter. | 0:11:06 | 0:11:08 | |
At the Jet Propulsion Laboratory in Pasadena | 0:11:13 | 0:11:17 | |
is NASA's deep space operations centre - | 0:11:17 | 0:11:20 | |
control room for space flights to the moon and beyond... | 0:11:20 | 0:11:24 | |
..including Scott's mission to Jupiter, Juno. | 0:11:28 | 0:11:32 | |
Four...three...two...one... | 0:11:32 | 0:11:35 | |
Ignition and lift-off of the Atlas V with Juno | 0:11:35 | 0:11:41 | |
on a trek to Jupiter. | 0:11:41 | 0:11:43 | |
Juno launched in 2011 | 0:11:46 | 0:11:48 | |
and is currently more than 2 million miles away, | 0:11:48 | 0:11:51 | |
speeding its way to Jupiter at about 150,000mph. | 0:11:51 | 0:11:55 | |
Even at that speed, it's a five-year journey. | 0:11:58 | 0:12:01 | |
In 2016, if all goes according to plan, | 0:12:02 | 0:12:06 | |
the probe will reach Jupiter and go into orbit | 0:12:06 | 0:12:08 | |
around the king of the solar system. | 0:12:08 | 0:12:10 | |
Scott and his entire team will be in this room, watching intensely. | 0:12:14 | 0:12:18 | |
On the day of the Jupiter orbit insertion, | 0:12:20 | 0:12:23 | |
this room will be completely full. | 0:12:23 | 0:12:25 | |
The spacecraft is approaching Jupiter. | 0:12:26 | 0:12:29 | |
It's moving at an incredible speed - like, 150,000mph, or even faster. | 0:12:29 | 0:12:35 | |
And when it gets to Jupiter we have to slow down enough | 0:12:35 | 0:12:39 | |
that Jupiter's gravity field can grab us. | 0:12:39 | 0:12:41 | |
So, we have a rocket on board, | 0:12:43 | 0:12:44 | |
we point it forward and we fire it, | 0:12:44 | 0:12:47 | |
and that rocket has to burn at just the right time | 0:12:47 | 0:12:51 | |
for just the right amount of time | 0:12:51 | 0:12:53 | |
for us to slow down the perfect amount for Jupiter to grab us, | 0:12:53 | 0:12:58 | |
because if it misses we fly right past Jupiter. | 0:12:58 | 0:13:01 | |
There'll be a huge cheer. | 0:13:03 | 0:13:04 | |
Once we get the data down that shows us we're in orbit around Jupiter | 0:13:04 | 0:13:09 | |
the room will explode. | 0:13:09 | 0:13:11 | |
It's the same room where all NASA's critical events are controlled from, | 0:13:11 | 0:13:14 | |
including the recent landing of the Curiosity rover on Mars. | 0:13:14 | 0:13:19 | |
And here you see it's right on that screen. | 0:13:19 | 0:13:22 | |
We'll celebrate just like that. | 0:13:26 | 0:13:28 | |
I can't wait. | 0:13:29 | 0:13:31 | |
Once in orbit, Juno will spend a year circling Jupiter, | 0:13:35 | 0:13:39 | |
gathering vital clues about how it formed. | 0:13:39 | 0:13:42 | |
Some of the most important data | 0:13:44 | 0:13:46 | |
that we really want and can't wait to get | 0:13:46 | 0:13:48 | |
is things that are tied to understanding the early solar system | 0:13:48 | 0:13:52 | |
and how Jupiter formed. | 0:13:52 | 0:13:53 | |
So, we want to know whether there's a core in the middle of Jupiter. | 0:13:53 | 0:13:57 | |
Is there a core of heavy elements, | 0:13:57 | 0:13:59 | |
a concentration of materials, down in the centre? | 0:13:59 | 0:14:01 | |
Or is it the same hydrogen and helium and mixture of gases, | 0:14:01 | 0:14:05 | |
just squeezed down? | 0:14:05 | 0:14:06 | |
Knowing what's at the centre | 0:14:08 | 0:14:10 | |
is a vital clue to understanding how Jupiter was built. | 0:14:10 | 0:14:14 | |
Building planets, whether rocky or gassy, | 0:14:24 | 0:14:28 | |
is a tricky business. | 0:14:28 | 0:14:29 | |
But it's something that Juno will shed some light on. | 0:14:29 | 0:14:32 | |
What Juno's about is actually trying to discover | 0:14:34 | 0:14:36 | |
the recipe for the solar system. | 0:14:36 | 0:14:39 | |
How do you make solar systems? How do you make planets? | 0:14:39 | 0:14:42 | |
And the stage that we're at is we're collecting the ingredient list | 0:14:42 | 0:14:46 | |
and that's really an important part of any recipe - | 0:14:46 | 0:14:48 | |
first you gather up the ingredients, figure out what they are, | 0:14:48 | 0:14:51 | |
then there's some process that you have to do | 0:14:51 | 0:14:53 | |
in order to bake your cake. | 0:14:53 | 0:14:55 | |
But the exact nature of that process is not entirely clear. | 0:14:56 | 0:15:00 | |
The recipe for a rocky planet, like the earth or Mars, is a slow one. | 0:15:01 | 0:15:07 | |
It can take up to 100 million years. | 0:15:07 | 0:15:10 | |
But the ingredient list is simple - | 0:15:10 | 0:15:13 | |
dust. | 0:15:13 | 0:15:15 | |
Dust starts out in the early solar system | 0:15:15 | 0:15:18 | |
in a very fine grain, like this - even finer. | 0:15:18 | 0:15:21 | |
Then, eventually, they start to stick together through electrostatic forces | 0:15:21 | 0:15:25 | |
and they build bigger and bigger pieces. | 0:15:25 | 0:15:27 | |
Eventually, the rocks got big enough, they started to stick together | 0:15:27 | 0:15:30 | |
to the point where they started to form their own gravity. | 0:15:30 | 0:15:33 | |
But there's a big leap from dust grains | 0:15:34 | 0:15:37 | |
to rocks that are large enough to clump together | 0:15:37 | 0:15:40 | |
through their own gravity. | 0:15:40 | 0:15:41 | |
These rocks, even being so large as they are | 0:15:41 | 0:15:44 | |
that none of us could lift them, | 0:15:44 | 0:15:46 | |
they still don't have important gravity. | 0:15:46 | 0:15:49 | |
Even larger rocks are needed to really start to get enough gravity | 0:15:50 | 0:15:53 | |
to start to attract the rest of the material for it to collapse | 0:15:53 | 0:15:57 | |
and start to form a planet as large as Earth. | 0:15:57 | 0:16:01 | |
It's a slow process, | 0:16:04 | 0:16:06 | |
but there's no rush when it comes to building a rocky planet. | 0:16:06 | 0:16:09 | |
Gas giants, on the other hand, are trickier. | 0:16:11 | 0:16:14 | |
You have to make them fast. | 0:16:14 | 0:16:15 | |
Because Jupiter and the other gas giants | 0:16:18 | 0:16:21 | |
are mostly hydrogen and helium, | 0:16:21 | 0:16:23 | |
and the sun is mostly hydrogen and helium, | 0:16:23 | 0:16:26 | |
that tells us right away that those planets had to have formed | 0:16:26 | 0:16:30 | |
while that nebula of hydrogen and helium was still around. | 0:16:30 | 0:16:33 | |
There are two ways to build a gas giant like Jupiter that fast. | 0:16:35 | 0:16:40 | |
We don't know exactly how Jupiter formed. | 0:16:40 | 0:16:44 | |
The two main theories | 0:16:44 | 0:16:45 | |
are either it has a direct gravitational collapse, | 0:16:45 | 0:16:48 | |
like we think the sun had, from the nebula | 0:16:48 | 0:16:51 | |
and sort of builds, um, from the outside in | 0:16:51 | 0:16:55 | |
and formed Jupiter pretty quickly, | 0:16:55 | 0:16:58 | |
or it starts to build from the inside out. | 0:16:58 | 0:17:01 | |
If it collapsed from the cloud of gas, | 0:17:02 | 0:17:05 | |
then it will be gas all the way through to the centre. | 0:17:05 | 0:17:08 | |
But if the second theory is right, then it first built a rocky core | 0:17:09 | 0:17:13 | |
up to ten times the mass of the Earth, | 0:17:13 | 0:17:15 | |
which then drew in a blanket of gas. | 0:17:15 | 0:17:17 | |
Either way, it had to happen fast. | 0:17:18 | 0:17:21 | |
But if Jupiter was going to build a heavy core that quickly, | 0:17:23 | 0:17:26 | |
it couldn't be done with dust alone. | 0:17:26 | 0:17:28 | |
There was another crucial ingredient. | 0:17:29 | 0:17:32 | |
Ice. | 0:17:33 | 0:17:35 | |
Kevin Walsh is a planet builder. | 0:17:43 | 0:17:45 | |
His job is to create theoretical models | 0:17:47 | 0:17:49 | |
of how the planets in the solar system formed - | 0:17:49 | 0:17:53 | |
models that can best explain the evidence and the clues. | 0:17:53 | 0:17:57 | |
I think that the most likely way that Jupiter formed | 0:17:57 | 0:18:00 | |
was by building a solid core of material | 0:18:00 | 0:18:03 | |
and then hauling the gas down on top of it. | 0:18:03 | 0:18:05 | |
Either way that you form Jupiter, | 0:18:05 | 0:18:07 | |
either from accreting straight from the gas | 0:18:07 | 0:18:09 | |
or building up a rocky core, it has to be done | 0:18:09 | 0:18:12 | |
in four or five million years, | 0:18:12 | 0:18:14 | |
before all of the gas is gone from the disc around the sun. | 0:18:14 | 0:18:17 | |
That's a lot quicker than the time it took | 0:18:19 | 0:18:21 | |
to build a rocky planet from dust alone. | 0:18:21 | 0:18:24 | |
But Jupiter had the help of that extra icy ingredient. | 0:18:26 | 0:18:29 | |
So, we think that the key ingredient | 0:18:32 | 0:18:33 | |
that allowed Jupiter and Saturn to form so fast, | 0:18:33 | 0:18:36 | |
compared to the rocky planets, | 0:18:36 | 0:18:37 | |
is that they formed far enough from the sun | 0:18:37 | 0:18:40 | |
that water could condense from the gas around the sun | 0:18:40 | 0:18:43 | |
and form ice, and increase the density of material | 0:18:43 | 0:18:47 | |
and give you more material to build a larger, rockier core faster. | 0:18:47 | 0:18:51 | |
That could explain how Jupiter built a rocky core so quickly. | 0:18:54 | 0:18:57 | |
But it doesn't explain why it grew where it did. | 0:18:59 | 0:19:03 | |
It's not unreasonable to think | 0:19:04 | 0:19:06 | |
it would form at the place with the most ice. | 0:19:06 | 0:19:09 | |
That's a place called the ice line. | 0:19:11 | 0:19:14 | |
But it's not where Jupiter is today. | 0:19:14 | 0:19:16 | |
So, right now when we look at our solar system, we look at Jupiter | 0:19:18 | 0:19:21 | |
and it's beyond the ice line by a fair bit, | 0:19:21 | 0:19:25 | |
whereas we think it was really advantageous to form Jupiter | 0:19:25 | 0:19:28 | |
right at the ice line. | 0:19:28 | 0:19:30 | |
So already that's suspicious. | 0:19:30 | 0:19:32 | |
If Jupiter was built from a collapsing cloud, | 0:19:37 | 0:19:40 | |
we'd expect it to be further out. | 0:19:40 | 0:19:42 | |
If, on the other hand, it was built from a rocky core, | 0:19:44 | 0:19:48 | |
we'd expect it to be closer to the sun. | 0:19:48 | 0:19:50 | |
But it's not in either of these two places. | 0:19:51 | 0:19:54 | |
So the big question is, | 0:19:54 | 0:19:56 | |
is Jupiter in the wrong place? | 0:19:56 | 0:19:59 | |
To even ask that question has, until recently, been a heresy. | 0:20:08 | 0:20:12 | |
At the historic Chamberlin Telescope in Denver, Colorado, | 0:20:14 | 0:20:19 | |
Kevin Walsh is following in the footsteps | 0:20:19 | 0:20:21 | |
of some famous astronomers. | 0:20:21 | 0:20:23 | |
He's taking a closer look at Jupiter. | 0:20:29 | 0:20:32 | |
You can see Jupiter with the naked eye, | 0:20:34 | 0:20:36 | |
but looking at it through a telescope like this | 0:20:36 | 0:20:39 | |
makes it a lot more fun. | 0:20:39 | 0:20:40 | |
The bands of colour are really clear and crisp | 0:20:41 | 0:20:45 | |
and the moons are real bright. | 0:20:45 | 0:20:46 | |
It comes alive. It becomes a real planet when you look at it through a telescope. | 0:20:46 | 0:20:50 | |
Galileo was the first astronomer to point a telescope at Jupiter, | 0:20:52 | 0:20:56 | |
more than 400 years ago, | 0:20:56 | 0:20:59 | |
and no-one ever questioned that Jupiter will always be, | 0:20:59 | 0:21:02 | |
and has always been, in that same orbit. | 0:21:02 | 0:21:04 | |
Jupiter, right now... | 0:21:06 | 0:21:07 | |
..looks the same as it would have looked for Galileo. | 0:21:09 | 0:21:11 | |
It's a little bigger and brighter through this great telescope, | 0:21:11 | 0:21:14 | |
but it's the same Jupiter, | 0:21:14 | 0:21:15 | |
so if I came back tomorrow night, it'd look the same. | 0:21:15 | 0:21:18 | |
So that's the view - | 0:21:18 | 0:21:20 | |
the planets that we look at now seem like they never change. | 0:21:20 | 0:21:23 | |
And why would they change? | 0:21:23 | 0:21:25 | |
This was the bedrock of our understanding - | 0:21:27 | 0:21:30 | |
that the planets' orbits are fixed. | 0:21:30 | 0:21:32 | |
The first hint of something odd came 35 years ago | 0:21:37 | 0:21:41 | |
from astronomers trying to calculate how the solar system formed. | 0:21:41 | 0:21:44 | |
They kept getting a strange result. | 0:21:46 | 0:21:49 | |
Some of those calculations were suggesting that it was possible | 0:21:49 | 0:21:53 | |
that a planet like Jupiter could have been moved around. | 0:21:53 | 0:21:56 | |
It was a result so crazy that it was totally ignored. | 0:21:57 | 0:22:01 | |
So if you built a model to try to understand | 0:22:01 | 0:22:03 | |
some of the events of the early solar system | 0:22:03 | 0:22:05 | |
and your model is telling you that planets could have migrated or moved, | 0:22:05 | 0:22:09 | |
that Jupiter could have moved, | 0:22:09 | 0:22:10 | |
then it was telling you that you probably made a mistake. | 0:22:10 | 0:22:13 | |
So the idea of planet migration, it was just never possible. | 0:22:13 | 0:22:17 | |
Just didn't seem possible. | 0:22:17 | 0:22:18 | |
But in 1995, astronomers were forced to face up to the impossible. | 0:22:23 | 0:22:29 | |
The mystery began to unravel when dramatic evidence was uncovered | 0:22:31 | 0:22:35 | |
from somewhere completely unexpected. | 0:22:35 | 0:22:37 | |
Astronomer Chris Watson | 0:22:54 | 0:22:56 | |
is searching for the weirdest places in the galaxy. | 0:22:56 | 0:22:59 | |
He's a planet hunter, one of a growing band of astronomers | 0:23:01 | 0:23:05 | |
involved in the hunt for exoplanets - | 0:23:05 | 0:23:08 | |
alien worlds circling around other stars. | 0:23:08 | 0:23:11 | |
It's one of the hottest fields in astronomy. | 0:23:13 | 0:23:15 | |
Up until now, or until recently, we've only had one planetary system | 0:23:17 | 0:23:22 | |
that we could study, and that was the solar system, | 0:23:22 | 0:23:24 | |
the planets around the sun. | 0:23:24 | 0:23:26 | |
And there are about 100 billion stars in our galaxy | 0:23:26 | 0:23:29 | |
and there are about 100 billion galaxies in the universe, | 0:23:29 | 0:23:32 | |
and we could only study one. | 0:23:32 | 0:23:34 | |
But the study of planets and planetary systems exploded | 0:23:36 | 0:23:39 | |
with the amazing discovery in 1995 | 0:23:39 | 0:23:42 | |
of a planet orbiting around another star. | 0:23:42 | 0:23:45 | |
Less than 20 years ago, we first found another planet | 0:23:47 | 0:23:50 | |
around another star that's like our sun | 0:23:50 | 0:23:52 | |
and that was a dramatic breakthrough. | 0:23:52 | 0:23:55 | |
And we now know of over 1,000 planets. | 0:23:55 | 0:23:59 | |
And they're very strange - | 0:23:59 | 0:24:00 | |
these are nothing like our solar system | 0:24:00 | 0:24:03 | |
and, in some cases, I think really science fact | 0:24:03 | 0:24:06 | |
could be a lot weirder than science fiction. | 0:24:06 | 0:24:09 | |
The planets they have been finding look stranger than anyone imagined. | 0:24:11 | 0:24:15 | |
We've found planets around binary stars, | 0:24:21 | 0:24:24 | |
where you actually have two stars orbiting each other, | 0:24:24 | 0:24:27 | |
a bit like Tatooine off of Star Wars. | 0:24:27 | 0:24:29 | |
That would be a magical world if you had a habitable planet there, | 0:24:29 | 0:24:33 | |
because you would imagine | 0:24:33 | 0:24:35 | |
you'd actually have two shadows on everything | 0:24:35 | 0:24:37 | |
and two stars in the sky, as well. | 0:24:37 | 0:24:39 | |
None of the planets found have been remotely like home. | 0:24:46 | 0:24:50 | |
Recently, a planet was discovered a little bit bigger than Earth, | 0:24:52 | 0:24:56 | |
but incredibly close to its star. | 0:24:56 | 0:24:58 | |
It's probably a rocky world, but it's so hot | 0:24:58 | 0:25:02 | |
it would actually be molten, | 0:25:02 | 0:25:04 | |
so...it'd be this, but the actual lava on it. | 0:25:04 | 0:25:07 | |
And most puzzling of all are the largest planets, | 0:25:08 | 0:25:12 | |
so weird as to seem impossible. | 0:25:12 | 0:25:14 | |
What was strange when we first discovered these planets | 0:25:16 | 0:25:19 | |
is they were massive worlds, | 0:25:19 | 0:25:21 | |
they were gas giants much like Jupiter. | 0:25:21 | 0:25:24 | |
But these were much, much closer to their parent stars. | 0:25:24 | 0:25:27 | |
Jupiter lives out in the cold outer reaches of our solar system, | 0:25:30 | 0:25:35 | |
taking 12 years to orbit the sun. | 0:25:35 | 0:25:37 | |
But these alien giants were found in the fiery heat, | 0:25:38 | 0:25:42 | |
right next to their star, | 0:25:42 | 0:25:43 | |
hurtling around in crazy orbits of just a few days. | 0:25:43 | 0:25:47 | |
They were nicknamed "hot Jupiters". | 0:25:48 | 0:25:51 | |
They're right up against the host star, | 0:25:55 | 0:25:57 | |
and it's amazing, they really... | 0:25:57 | 0:25:59 | |
At the time, we thought, "How did they get there? | 0:25:59 | 0:26:01 | |
"They really shouldn't be there." | 0:26:01 | 0:26:03 | |
Other scientists were thinking, "Well, you're a bit crazy, | 0:26:03 | 0:26:06 | |
"these Jupiters should not be that close to the star." | 0:26:06 | 0:26:09 | |
Everyone was baffled by the existence of hot Jupiters. | 0:26:12 | 0:26:15 | |
They were planets that, quite simply, shouldn't exist. | 0:26:15 | 0:26:19 | |
In theory, the only place you could build a gas giant | 0:26:22 | 0:26:26 | |
would be out in the cold, far away from a star, | 0:26:26 | 0:26:30 | |
because that's the only place | 0:26:30 | 0:26:32 | |
you can find the necessary ingredients. | 0:26:32 | 0:26:34 | |
What I'm holding in my hand is a lump of dry ice, | 0:26:36 | 0:26:39 | |
and this represents the building blocks | 0:26:39 | 0:26:42 | |
of planets like Jupiter. | 0:26:42 | 0:26:44 | |
And this is fine - it's quite happy out here, | 0:26:44 | 0:26:48 | |
far away from the fire that represents our sun | 0:26:48 | 0:26:51 | |
or any other star that one of these gas giants might be forming round. | 0:26:51 | 0:26:55 | |
But look at what happens when I bring it closer to the fire. | 0:26:55 | 0:27:01 | |
Too close to the star and the ice just turns to gas. | 0:27:04 | 0:27:07 | |
And without ice you can't build a gas giant. | 0:27:08 | 0:27:12 | |
So there's very little left after just a few minutes. | 0:27:12 | 0:27:16 | |
And what this means | 0:27:16 | 0:27:19 | |
is that gas giants can't form close to the star. | 0:27:19 | 0:27:24 | |
The building blocks just cannot exist that close. | 0:27:24 | 0:27:28 | |
They have to have formed further away | 0:27:28 | 0:27:30 | |
where the raw materials can exist. | 0:27:30 | 0:27:32 | |
If these hot Jupiters couldn't have formed where we find them, | 0:27:35 | 0:27:39 | |
it could only mean one thing. | 0:27:39 | 0:27:41 | |
So we think that, in actual fact, | 0:27:41 | 0:27:44 | |
these gas giants form further out, | 0:27:44 | 0:27:48 | |
then they actually move towards the star, | 0:27:48 | 0:27:50 | |
they actually migrate inwards. | 0:27:50 | 0:27:53 | |
The planets are on the move. | 0:27:56 | 0:27:59 | |
The discovery that planets could change orbit | 0:28:02 | 0:28:05 | |
was a shocking revelation. | 0:28:05 | 0:28:07 | |
It turned the world of planetary science on its head. | 0:28:07 | 0:28:11 | |
The implications of a planet the size of Jupiter | 0:28:12 | 0:28:15 | |
roaming freely around a planetary system | 0:28:15 | 0:28:18 | |
could be devastating. | 0:28:18 | 0:28:20 | |
Over recent years, the search for exoplanets has exploded. | 0:28:23 | 0:28:28 | |
So here we are, nearly 2,400 metres up | 0:28:30 | 0:28:33 | |
on the volcanic island of La Palma. | 0:28:33 | 0:28:37 | |
What you can see before you are suites of professional telescopes | 0:28:37 | 0:28:42 | |
and what we're going to do is we're going to use one of these | 0:28:42 | 0:28:46 | |
telescopes to actually look at planets orbiting another star. | 0:28:46 | 0:28:50 | |
So, this cloud can be a bit of a problem. | 0:28:51 | 0:28:54 | |
Normally it's not so cloudy, but we are in the depths of winter | 0:28:54 | 0:28:57 | |
and this is actually quite local cloud. | 0:28:57 | 0:28:59 | |
20 years ago, all these telescopes were busy looking at stars. | 0:29:01 | 0:29:06 | |
Now, increasingly, many are focusing on planets. | 0:29:06 | 0:29:10 | |
There's quite a few telescopes here, and probably every night | 0:29:11 | 0:29:16 | |
there's some project related to extrasolar planets going on. | 0:29:16 | 0:29:20 | |
It is a really rich, blossoming field of astronomy. | 0:29:20 | 0:29:25 | |
And, provided the clouds clear, | 0:29:29 | 0:29:32 | |
tonight Chris will be pointing his telescope | 0:29:32 | 0:29:35 | |
at an exoplanet called WASP-84 b. | 0:29:35 | 0:29:37 | |
These clouds will clear. | 0:29:39 | 0:29:41 | |
But, even with clear skies, | 0:29:47 | 0:29:49 | |
spotting alien planets is no easy matter. | 0:29:49 | 0:29:52 | |
To see other planets in our solar system from Earth is pretty easy. | 0:30:04 | 0:30:09 | |
So this candle represents our sun | 0:30:09 | 0:30:11 | |
and if I pop down this little rock, representing a planet, | 0:30:11 | 0:30:15 | |
you can clearly see the reflected sunlight. | 0:30:15 | 0:30:17 | |
But even the nearest stars are so far away | 0:30:19 | 0:30:22 | |
that the reflected light from the planets gets completely lost. | 0:30:22 | 0:30:25 | |
So, now we have our star, much further away, | 0:30:27 | 0:30:30 | |
and if I put my planet down, | 0:30:30 | 0:30:32 | |
while it's still reflecting the starlight, | 0:30:32 | 0:30:35 | |
because you're so far away, | 0:30:35 | 0:30:36 | |
the reflected light is actually drowned out | 0:30:36 | 0:30:39 | |
in the glare of the star itself. | 0:30:39 | 0:30:41 | |
Because the planets are so hard to see, | 0:30:45 | 0:30:47 | |
astronomers have found other ways to detect them. | 0:30:47 | 0:30:50 | |
One of the best ways is actually to watch and see | 0:30:50 | 0:30:54 | |
if the planet actually crosses in front of the star. | 0:30:54 | 0:30:58 | |
So, if we were an alien civilisation looking back at our solar system, | 0:30:58 | 0:31:03 | |
we happen to catch Jupiter transiting the face of our sun, | 0:31:03 | 0:31:07 | |
we would see a 1% dip in the sunlight. | 0:31:07 | 0:31:11 | |
For a planet a lot smaller, like the Earth, | 0:31:11 | 0:31:15 | |
that dip is much, much smaller - it's minuscule. | 0:31:15 | 0:31:19 | |
And that's why it's so, so difficult to detect these. | 0:31:19 | 0:31:22 | |
But techniques have improved dramatically | 0:31:28 | 0:31:30 | |
and now, for astronomers like Chris Watson, | 0:31:30 | 0:31:33 | |
planet-hunting is all part of a night's work. | 0:31:33 | 0:31:36 | |
This is our telescope, Telescopio Nazionale Galileo, | 0:31:44 | 0:31:48 | |
and this will be our baby for the night. | 0:31:48 | 0:31:50 | |
The skies are clearing beautifully, | 0:31:54 | 0:31:56 | |
so I think we're in for a really nice night ahead. | 0:31:56 | 0:31:59 | |
Thanks to ground-based telescopes like this, | 0:32:01 | 0:32:04 | |
as well as space telescopes like NASA's Kepler mission, | 0:32:04 | 0:32:07 | |
thousands of planets have now been found. | 0:32:07 | 0:32:10 | |
And not just planets, but entire planetary systems. | 0:32:12 | 0:32:15 | |
So this is the Kepler Orrery, | 0:32:23 | 0:32:25 | |
which shows the orbits and the sizes of planets. | 0:32:25 | 0:32:29 | |
So these are candidates that the Kepler space mission has found. | 0:32:29 | 0:32:33 | |
So these are transiting planets. | 0:32:33 | 0:32:36 | |
They don't, however, look much like we'd expect. | 0:32:36 | 0:32:39 | |
And up there, on the top left, | 0:32:39 | 0:32:41 | |
you can see the orbits of the four innermost planets of our solar system | 0:32:41 | 0:32:47 | |
from Mercury out to Mars. | 0:32:47 | 0:32:49 | |
What you can see is the huge diversity | 0:32:49 | 0:32:54 | |
of all the different planetary systems. | 0:32:54 | 0:32:56 | |
Each set of rings shows a different planetary system | 0:32:59 | 0:33:03 | |
and each blob, a different planet, with its size and orbit. | 0:33:03 | 0:33:06 | |
They break every rule in the book | 0:33:08 | 0:33:10 | |
and make us look like the odd one out. | 0:33:10 | 0:33:12 | |
So we have large gas giant planets in there, | 0:33:14 | 0:33:18 | |
and then you can see the really short period, | 0:33:18 | 0:33:22 | |
really weird solar systems. | 0:33:22 | 0:33:25 | |
They really don't look anything like our own solar system. | 0:33:26 | 0:33:29 | |
Some of these planets actually have orbits of just a few hours. | 0:33:29 | 0:33:35 | |
There's even systems spiralling around multiple planets in here. | 0:33:36 | 0:33:40 | |
That one's weird. What's going on here? | 0:33:43 | 0:33:45 | |
Who knows what we might discover in this rich smorgasbord of planets? | 0:33:57 | 0:34:01 | |
It is ridiculous, actually. | 0:34:04 | 0:34:05 | |
HE CHUCKLES | 0:34:05 | 0:34:07 | |
What is going on with that? | 0:34:07 | 0:34:09 | |
Extraordinary worlds. | 0:34:12 | 0:34:13 | |
Some may host life. | 0:34:16 | 0:34:18 | |
Our exploration of these alien worlds | 0:34:21 | 0:34:23 | |
is only just beginning, | 0:34:23 | 0:34:26 | |
but already they're revealing some incredible secrets. | 0:34:26 | 0:34:29 | |
Tonight, Chris and his team are training the telescope | 0:34:36 | 0:34:39 | |
on a star they known has a hot Jupiter orbiting it. | 0:34:39 | 0:34:42 | |
INDISTINCT CONVERSATION | 0:34:42 | 0:34:45 | |
They hope to reveal just how devastating | 0:34:48 | 0:34:51 | |
a migrating gas giant could be. | 0:34:51 | 0:34:53 | |
So this star that we're looking at, WASP-84, | 0:34:55 | 0:34:58 | |
was actually discovered to have a transiting planet around it. | 0:34:58 | 0:35:01 | |
That transiting planet, we know at the moment, | 0:35:01 | 0:35:04 | |
is about a little bit less massive than Jupiter. | 0:35:04 | 0:35:08 | |
And we know its orbital period, | 0:35:08 | 0:35:10 | |
so its year is about eight-and-a-half days, | 0:35:10 | 0:35:12 | |
and we're going to follow it as it transits the star. | 0:35:12 | 0:35:16 | |
A planet the size of Jupiter | 0:35:16 | 0:35:19 | |
orbiting its star once every eight days | 0:35:19 | 0:35:22 | |
is already pretty weird. | 0:35:22 | 0:35:24 | |
But some of these alien worlds have even weirder orbits than that. | 0:35:24 | 0:35:28 | |
-What's the air mass with that, then? -About 1.25? | 0:35:28 | 0:35:32 | |
'We would expect the planet and the star' | 0:35:32 | 0:35:35 | |
to be spinning in the same way. | 0:35:35 | 0:35:37 | |
But we see quite a few systems where that is just not the case. | 0:35:37 | 0:35:41 | |
Some of these planets are going completely the wrong way. | 0:35:42 | 0:35:46 | |
If the star is spinning clockwise, | 0:35:47 | 0:35:49 | |
the planet is spinning anti-clockwise. | 0:35:49 | 0:35:52 | |
-169, we're talking about. -Yeah, it's about... | 0:35:52 | 0:35:55 | |
A planet orbiting in the wrong direction | 0:35:55 | 0:35:57 | |
is a sign of some truly cataclysmic event. | 0:35:57 | 0:35:59 | |
And tonight, as it passes in front of its star, | 0:36:01 | 0:36:04 | |
Chris will be able to analyse the orbit of WASP-84 b. | 0:36:04 | 0:36:07 | |
'The purpose of these observations is actually' | 0:36:08 | 0:36:11 | |
to see whether we have a nicely aligned system - | 0:36:11 | 0:36:15 | |
a bit like the planets we have in our solar system, | 0:36:15 | 0:36:17 | |
where the star spins in the same direction as the planet orbits. | 0:36:17 | 0:36:22 | |
Or do we have something that would be the smoking gun | 0:36:22 | 0:36:26 | |
of a really violent interaction | 0:36:26 | 0:36:29 | |
which has maybe scattered that planet into one of these weird orbits? | 0:36:29 | 0:36:34 | |
So, perhaps over the poles, | 0:36:34 | 0:36:35 | |
or actually spinning in the opposite direction to that of the star. | 0:36:35 | 0:36:40 | |
But the big question is | 0:36:41 | 0:36:43 | |
what could be the cause of such planetary upheaval? | 0:36:43 | 0:36:46 | |
Whoa! | 0:36:46 | 0:36:48 | |
After following the transit through the night, | 0:36:52 | 0:36:54 | |
Chris has the verdict on Planet WASP-84 b. | 0:36:54 | 0:36:58 | |
So, the transit's finished. We've had a quick look at the data | 0:37:00 | 0:37:04 | |
and what we've found has actually taken us a bit by surprise. | 0:37:04 | 0:37:09 | |
We thought that this planet system would be misaligned. | 0:37:09 | 0:37:12 | |
Now that we've had a look at the data, | 0:37:12 | 0:37:14 | |
it looks as though it's actually aligned. | 0:37:14 | 0:37:16 | |
WASP-84 b turns out to be orbiting the right way. | 0:37:18 | 0:37:21 | |
But Chris has found many of these hot Jupiters | 0:37:23 | 0:37:25 | |
that are travelling in completely the wrong direction. | 0:37:25 | 0:37:28 | |
It's evidence of how, in migrating, they must have caused havoc. | 0:37:30 | 0:37:34 | |
With these very strange orbits, | 0:37:36 | 0:37:38 | |
it looks as though it's been a very violent process. | 0:37:38 | 0:37:42 | |
To actually take one of these planets | 0:37:42 | 0:37:44 | |
and just chuck it into a different orbit, | 0:37:44 | 0:37:48 | |
that's very violent. | 0:37:48 | 0:37:50 | |
One of the easiest ways to do that is to have a collision. | 0:37:50 | 0:37:54 | |
Take two planets, interaction between them, | 0:37:54 | 0:37:58 | |
and you can eject one planet | 0:37:58 | 0:38:00 | |
and fling the other planet really close in to the star. | 0:38:00 | 0:38:04 | |
These giant gas planets are the bully of the playground. | 0:38:09 | 0:38:13 | |
They have the power to throw other planets around | 0:38:14 | 0:38:17 | |
like a game of cosmic pinball. | 0:38:17 | 0:38:19 | |
Beasts the size of Jupiter are so vast | 0:38:23 | 0:38:26 | |
they can eject entire planets from the system. | 0:38:26 | 0:38:28 | |
They can launch them into crazy polar orbits. | 0:38:32 | 0:38:35 | |
They even have the power to destroy entire worlds. | 0:38:39 | 0:38:42 | |
A planet like Jupiter, the mass of Jupiter, the size of it, | 0:38:49 | 0:38:53 | |
just dominates planetary systems, | 0:38:53 | 0:38:55 | |
and it's got the power to really decide | 0:38:55 | 0:38:58 | |
the fate of the other planets. | 0:38:58 | 0:39:01 | |
I think we'd be quite glad there's not a hot Jupiter in our system. | 0:39:03 | 0:39:07 | |
We wouldn't be seeing this. | 0:39:07 | 0:39:09 | |
We've discovered other systems where planets migrate | 0:39:18 | 0:39:21 | |
and hot Jupiters cause havoc. | 0:39:21 | 0:39:23 | |
But what about our own solar system? | 0:39:24 | 0:39:26 | |
Our planets certainly seem fixed in their rigid, clockwork orbits. | 0:39:28 | 0:39:33 | |
Our earth has been the same distance from the sun for 4.5 billion years. | 0:39:43 | 0:39:49 | |
Long enough to create an atmosphere, | 0:39:50 | 0:39:52 | |
build mountains, | 0:39:52 | 0:39:54 | |
and for life to evolve. | 0:39:54 | 0:39:55 | |
But the evidence from other planetary systems now means | 0:39:57 | 0:40:01 | |
a complete rethink on how and where our planets formed. | 0:40:01 | 0:40:05 | |
When we started discovering planets around other stars, | 0:40:05 | 0:40:09 | |
we started finding planets in completely unexpected places, | 0:40:09 | 0:40:12 | |
places we never thought could possibly form a planet. | 0:40:12 | 0:40:15 | |
We had to go back to the drawing board and say, | 0:40:15 | 0:40:18 | |
"Wow, planets can move. | 0:40:18 | 0:40:19 | |
"Planets can really move. Maybe that happened here." | 0:40:19 | 0:40:22 | |
It's a big leap, and to make that leap | 0:40:26 | 0:40:29 | |
and say things might have been completely unstable, | 0:40:29 | 0:40:33 | |
totally chaotic for a time period, that's really hard to imagine. | 0:40:33 | 0:40:38 | |
But that's the leap that we need to take. | 0:40:38 | 0:40:41 | |
The crazy results that suggest Jupiter might have changed orbit | 0:40:43 | 0:40:47 | |
might not be mistakes after all. | 0:40:47 | 0:40:50 | |
Instead, migration could be the key that unlocks | 0:40:51 | 0:40:55 | |
many of the mysteries of how our solar system came to be. | 0:40:55 | 0:40:58 | |
Now that we've taken this tool of planetary migration that we started | 0:40:58 | 0:41:01 | |
to understand by looking at planets around other stars, | 0:41:01 | 0:41:04 | |
we've realised that it's absolutely critical to understand | 0:41:04 | 0:41:07 | |
how our solar system formed and evolved. | 0:41:07 | 0:41:10 | |
And central to it all is mighty Jupiter. | 0:41:10 | 0:41:13 | |
Certainly in our planetary system, Jupiter is the key. | 0:41:13 | 0:41:16 | |
It's over three hundred times more massive than the Earth, | 0:41:16 | 0:41:19 | |
so Jupiter wins. | 0:41:19 | 0:41:22 | |
Jupiter decides what happens. | 0:41:22 | 0:41:23 | |
The inescapable truth seems to be that planets move. | 0:41:26 | 0:41:31 | |
And, if it can happen in exoplanetary systems, | 0:41:31 | 0:41:34 | |
it can happen in ours. | 0:41:34 | 0:41:36 | |
If we want to make a model that explains | 0:41:36 | 0:41:38 | |
how our solar system came to be, | 0:41:38 | 0:41:40 | |
we have to break the brass rods and set the planets free. | 0:41:40 | 0:41:44 | |
Once we accept the idea that the planets can move, | 0:41:48 | 0:41:53 | |
we can begin to explain some of the unsolved mysteries of the solar system. | 0:41:53 | 0:41:57 | |
In particular, why Mars is so small | 0:42:02 | 0:42:06 | |
and the curious composition of the asteroid belt. | 0:42:06 | 0:42:09 | |
Kevin Walsh has developed a model of the early solar system | 0:42:28 | 0:42:32 | |
that involves a wild dance of the planets. | 0:42:32 | 0:42:34 | |
It's an intricate and chaotic dance, | 0:42:38 | 0:42:40 | |
and if it had gone slightly differently | 0:42:40 | 0:42:43 | |
it could have stopped our developing solar system in its tracks. | 0:42:43 | 0:42:46 | |
In his model, Jupiter takes a wild ride through the solar system. | 0:42:48 | 0:42:52 | |
It takes us right back to the moment of birth, | 0:42:58 | 0:43:01 | |
when Jupiter had just formed from the cloud of gas. | 0:43:01 | 0:43:04 | |
The key is that, though Jupiter is really big, | 0:43:06 | 0:43:08 | |
it's 300 times the mass of the earth, | 0:43:08 | 0:43:10 | |
the gas disc around the sun was much more massive, | 0:43:10 | 0:43:13 | |
so the gas can actually push Jupiter in towards the sun. | 0:43:13 | 0:43:16 | |
As soon as it was born, Jupiter began to migrate inwards. | 0:43:17 | 0:43:22 | |
Over the course of half a million years, | 0:43:22 | 0:43:25 | |
it spiralled in towards the sun. | 0:43:25 | 0:43:27 | |
It was on its way to becoming a hot Jupiter. | 0:43:28 | 0:43:31 | |
So, the idea that you could form something as big as Jupiter | 0:43:33 | 0:43:36 | |
and have it pushed inward by the gas disc | 0:43:36 | 0:43:38 | |
actually makes a fair amount of sense, | 0:43:38 | 0:43:40 | |
because we see it, we see it all over. | 0:43:40 | 0:43:42 | |
But something stopped Jupiter from crashing into the sun | 0:43:46 | 0:43:49 | |
or ending up as a hot Jupiter. | 0:43:49 | 0:43:51 | |
So, if it formed and started migrating inwards, | 0:43:52 | 0:43:55 | |
there must have been a mechanism to stop it | 0:43:55 | 0:43:57 | |
and bring it back out to the outer part of the solar system. | 0:43:57 | 0:44:00 | |
We think the key to stop its inward migration, to keep it | 0:44:00 | 0:44:03 | |
from going all the way in towards the sun is the presence of Saturn. | 0:44:03 | 0:44:08 | |
While Jupiter was on its wild ride, Saturn was born. | 0:44:08 | 0:44:12 | |
Saturn is also growing. It's going through the same process Jupiter did. | 0:44:12 | 0:44:16 | |
It's building a big core and it's getting really massive, | 0:44:16 | 0:44:19 | |
and once it gets really massive as well it can move in the disc also. | 0:44:19 | 0:44:23 | |
And it too began spiralling in towards the sun. | 0:44:23 | 0:44:26 | |
So as Saturn is racing inwards, it gets very close to Jupiter | 0:44:26 | 0:44:30 | |
and they actually get close enough that they get locked in a resonance | 0:44:30 | 0:44:33 | |
where their orbital periods are closely aligned | 0:44:33 | 0:44:35 | |
and they interact very closely gravitationally. | 0:44:35 | 0:44:38 | |
Now, when these two get really close | 0:44:38 | 0:44:41 | |
it actually stops Jupiter's inward migration. | 0:44:41 | 0:44:44 | |
The two planets were involved in a kind of gravitational dance. | 0:44:44 | 0:44:48 | |
And, as they came close, Jupiter changed direction | 0:44:48 | 0:44:52 | |
and was flung back to the outer solar system... | 0:44:52 | 0:44:54 | |
..just like a sailing ship changing course in a grand tack. | 0:44:56 | 0:44:59 | |
So this theory called the grand tack is called that | 0:45:03 | 0:45:06 | |
because our planets are moving inwards | 0:45:06 | 0:45:09 | |
and they get really close and they stop and they turn and they go back | 0:45:09 | 0:45:12 | |
outwards, and it's kind of like a sailboat tacking across the wind. | 0:45:12 | 0:45:15 | |
Jupiter's wild ride could explain two key mysteries - | 0:45:15 | 0:45:19 | |
first, why Mars is so small. | 0:45:19 | 0:45:22 | |
So, when Jupiter migrates inwards | 0:45:22 | 0:45:25 | |
it kind of snowploughs all the rocky material it sees, | 0:45:25 | 0:45:29 | |
it snowploughs it and pushes it inwards. | 0:45:29 | 0:45:31 | |
Much of the dust and rocky debris | 0:45:32 | 0:45:34 | |
that would have gone on to build Mars got pushed out of the way. | 0:45:34 | 0:45:38 | |
So, by Jupiter coming in and clearing out all of this | 0:45:39 | 0:45:42 | |
material on its way, it kind of reduces the total | 0:45:42 | 0:45:45 | |
amount of material that Mars can feed on to grow, | 0:45:45 | 0:45:49 | |
and so Mars ends up kind of being starved of rocky material | 0:45:49 | 0:45:52 | |
and only grows to be a tenth the mass of the earth. | 0:45:52 | 0:45:55 | |
And this explains why Mars is the planetary runt we see today. | 0:45:57 | 0:46:02 | |
The theory also explains why the asteroid belt has an icy ring | 0:46:06 | 0:46:10 | |
and a rocky ring so close together. | 0:46:10 | 0:46:13 | |
During its travels, Jupiter scattered everything in its path. | 0:46:22 | 0:46:25 | |
It threw rocks from the inner part of the solar system outwards... | 0:46:28 | 0:46:31 | |
..and ice from the outer reaches inwards... | 0:46:35 | 0:46:38 | |
..leaving the two distinct bands we see today. | 0:46:40 | 0:46:42 | |
That's how we end up with two different types of material | 0:46:44 | 0:46:47 | |
sitting on top of each other in the middle of the asteroid belt | 0:46:47 | 0:46:49 | |
in a very small region. | 0:46:49 | 0:46:51 | |
So Jupiter's wild ride could explain two key mysteries - | 0:46:51 | 0:46:55 | |
the size of Mars and the composition of the asteroid belt. | 0:46:55 | 0:46:58 | |
And if it had travelled any further in | 0:47:00 | 0:47:03 | |
the earth itself may have become a very different type of planet. | 0:47:03 | 0:47:07 | |
But the birth of the solar system | 0:47:14 | 0:47:16 | |
wasn't the only turbulent time in its history. | 0:47:16 | 0:47:19 | |
About 500 million years later, 4 billion years ago, | 0:47:21 | 0:47:25 | |
the solar system entered its teenage years - | 0:47:25 | 0:47:28 | |
an intense period of trouble, chaos and uncertainty. | 0:47:28 | 0:47:32 | |
It's a period of turbulence that could explain | 0:47:34 | 0:47:37 | |
two further mysteries... | 0:47:37 | 0:47:39 | |
..the craters on the moon | 0:47:41 | 0:47:43 | |
and the birth of Uranus and Neptune. | 0:47:43 | 0:47:45 | |
There are some mysteries when we look around the solar system, | 0:47:51 | 0:47:54 | |
where the theories really don't match what we see. | 0:47:54 | 0:47:57 | |
If we just take a bunch of small icy objects | 0:47:59 | 0:48:02 | |
from which Uranus and Neptune were made, | 0:48:02 | 0:48:05 | |
put them out in the outer part of the solar system in our computer | 0:48:05 | 0:48:08 | |
models and watch how they grow, it turns out they can't grow at all. | 0:48:08 | 0:48:13 | |
A couple of billion miles away from these ice giants, on the moon, | 0:48:15 | 0:48:19 | |
there's a clue that Hal Levison believes | 0:48:19 | 0:48:21 | |
could help solve the puzzle. | 0:48:21 | 0:48:24 | |
In fact, the moon is covered in clues. | 0:48:24 | 0:48:27 | |
So, when you look at the moon, | 0:48:28 | 0:48:30 | |
some of these biggest crater impact basins, like here and here, | 0:48:30 | 0:48:34 | |
all formed in a very short period of time | 0:48:34 | 0:48:37 | |
that we call the Late Heavy Bombardment. | 0:48:37 | 0:48:40 | |
It came roughly 500 million years after the birth of the solar system, | 0:48:40 | 0:48:45 | |
when all the planets had long formed. | 0:48:45 | 0:48:47 | |
And all of a sudden, out of the blue, | 0:48:49 | 0:48:51 | |
the moon got clobbered by big objects coming in and hitting it. | 0:48:51 | 0:48:57 | |
And that indicates that you had this very violent upheaval | 0:48:57 | 0:49:02 | |
and the only way that we can form an influx like this, stuff raining | 0:49:02 | 0:49:07 | |
down in onto the moon, is through changing the orbits of the planets. | 0:49:07 | 0:49:14 | |
To account for this violent upheaval, | 0:49:15 | 0:49:17 | |
Hal and some colleagues devised a new model. | 0:49:17 | 0:49:20 | |
It explains why we now see Uranus and Neptune | 0:49:21 | 0:49:24 | |
in places they can't possibly have formed. | 0:49:24 | 0:49:27 | |
We think what happened is they formed closer to the sun | 0:49:28 | 0:49:31 | |
and got delivered to where we see them today. | 0:49:31 | 0:49:34 | |
Uranus and Neptune must have formed much closer in, | 0:49:36 | 0:49:40 | |
where there was plenty of icy material, | 0:49:40 | 0:49:42 | |
and beyond them was a neat disc of icy, comet-like objects. | 0:49:42 | 0:49:46 | |
But this was not a stable system, | 0:49:48 | 0:49:51 | |
and a series of small changes led to a period of utter chaos. | 0:49:51 | 0:49:56 | |
These objects leak out of this disc, | 0:49:56 | 0:49:59 | |
get gravitationally scattered by all these planets, | 0:49:59 | 0:50:03 | |
like billiard balls going around, | 0:50:03 | 0:50:05 | |
and get eventually ejected to interstellar space by Jupiter. | 0:50:05 | 0:50:08 | |
That causes the planets' orbits to slightly spread over time | 0:50:12 | 0:50:16 | |
and what we think happened is that Jupiter | 0:50:16 | 0:50:19 | |
and Saturn got to the point where Jupiter goes around the sun | 0:50:19 | 0:50:24 | |
exactly twice for every time Saturn moves around the sun. | 0:50:24 | 0:50:28 | |
And that allows their tugs on one another to become much stronger | 0:50:28 | 0:50:33 | |
and as a result, Jupiter and Saturn get a little excited, | 0:50:33 | 0:50:37 | |
their orbits become less circular and more inclined | 0:50:37 | 0:50:40 | |
and they start getting... sort of tugging on one another. | 0:50:40 | 0:50:43 | |
Uranus and Neptune, which are much smaller than Jupiter and Saturn, feel | 0:50:43 | 0:50:47 | |
that fight, feel that tension and as a result, their orbits just go nuts. | 0:50:47 | 0:50:52 | |
In a sudden period of chaos, Uranus and Neptune | 0:50:54 | 0:50:57 | |
were flung out into the orbits we see today. | 0:50:57 | 0:51:00 | |
The ice giants, Uranus and Neptune, get scattered into this disc | 0:51:02 | 0:51:05 | |
that existed outside their orbits, and that thing went kaplooie. | 0:51:05 | 0:51:08 | |
Vast lumps of ice were scattered everywhere, | 0:51:13 | 0:51:17 | |
raining into the inner solar system | 0:51:17 | 0:51:19 | |
and bombarding the earth and the moon. | 0:51:19 | 0:51:21 | |
Every square inch of the earth at one time got hit | 0:51:25 | 0:51:29 | |
due to this instability, so it was not a very safe place to be. | 0:51:29 | 0:51:33 | |
We had this view that the solar system was this nice clock | 0:51:35 | 0:51:39 | |
and things just moved around in nice regular ways. | 0:51:39 | 0:51:42 | |
What this new model shows is a real paradigm shift. | 0:51:43 | 0:51:47 | |
It says that the solar system is not this nice, safe, quiescent place, | 0:51:47 | 0:51:53 | |
but can go through periods of intense violence. | 0:51:53 | 0:51:56 | |
This new model of the solar system is now dynamic and turbulent. | 0:51:58 | 0:52:02 | |
The prime mover in all this upheaval is our playground bully, Jupiter. | 0:52:04 | 0:52:09 | |
Such a bully, in fact, that David Nesvorny believes that Jupiter | 0:52:16 | 0:52:21 | |
may have been responsible for the ultimate planetary crime. | 0:52:21 | 0:52:24 | |
He ran the new model over and over again | 0:52:26 | 0:52:29 | |
with slightly different starting conditions. | 0:52:29 | 0:52:31 | |
I ran about 3,000, 4,000 models like this, | 0:52:33 | 0:52:38 | |
just playing with the initial state | 0:52:38 | 0:52:41 | |
and at a time, I considered the standard theory, | 0:52:41 | 0:52:44 | |
which was that the outer solar system had four planets. | 0:52:44 | 0:52:48 | |
His results were alarming - | 0:52:49 | 0:52:52 | |
change the starting conditions even slightly | 0:52:52 | 0:52:55 | |
and the solar system looks very different. | 0:52:55 | 0:52:57 | |
Frequently, what happened in my simulation was that Jupiter | 0:52:59 | 0:53:02 | |
just slingshots Uranus and Neptune from the solar system | 0:53:02 | 0:53:05 | |
and they ended somewhere in interstellar space. | 0:53:05 | 0:53:09 | |
So that wasn't right. | 0:53:09 | 0:53:11 | |
Obviously not right. | 0:53:11 | 0:53:13 | |
Then David had a radical idea. | 0:53:15 | 0:53:18 | |
If Neptune and Uranus didn't get flung out of the solar system, | 0:53:18 | 0:53:21 | |
maybe something else did. | 0:53:21 | 0:53:23 | |
I couldn't quite fit the solar system, how it looks like today. | 0:53:25 | 0:53:29 | |
So I was thinking and thinking and thinking, and then I thought, | 0:53:30 | 0:53:34 | |
"How about if the solar system had an extra planet?" | 0:53:34 | 0:53:37 | |
He started investigating the possibility | 0:53:41 | 0:53:44 | |
that an entire planet might have gone missing. | 0:53:44 | 0:53:47 | |
As ever, the prime suspect was Jupiter. | 0:53:49 | 0:53:53 | |
So, now I am pointing at Jupiter, | 0:53:56 | 0:53:59 | |
so I can see the disc of Jupiter, | 0:53:59 | 0:54:02 | |
and then, nicely aligned, four giant moons. | 0:54:02 | 0:54:07 | |
It has a huge influence... | 0:54:08 | 0:54:10 | |
..and could have had an even bigger influence in the past. | 0:54:11 | 0:54:14 | |
It may even have been able to eject an entire planet | 0:54:19 | 0:54:22 | |
from our solar system. | 0:54:22 | 0:54:24 | |
This is the solar system. | 0:54:25 | 0:54:27 | |
The sun is in the middle... | 0:54:27 | 0:54:29 | |
..then we have the terrestrial planets. | 0:54:30 | 0:54:32 | |
Then there's the asteroid belt and the outer planets. | 0:54:32 | 0:54:36 | |
To get the arrangement of planets we see today, David thinks | 0:54:37 | 0:54:41 | |
we once had an extra ice giant but it was thrown out by Jupiter. | 0:54:41 | 0:54:45 | |
I start playing with the possibility that we had an additional planet. | 0:54:46 | 0:54:53 | |
So the best case I have found was when I placed | 0:54:53 | 0:54:57 | |
this third ice giant between Saturn and Uranus initially, | 0:54:57 | 0:55:02 | |
somewhere here. | 0:55:02 | 0:55:04 | |
What happens in this case is that during the instability, | 0:55:04 | 0:55:07 | |
this planet evolves, has close encounters with Jupiter | 0:55:07 | 0:55:11 | |
and Saturn and gets ejected from the solar system. | 0:55:11 | 0:55:15 | |
The ejected planet may have been a sacrificial lamb | 0:55:27 | 0:55:31 | |
that saved us from Jupiter's destructive powers | 0:55:31 | 0:55:34 | |
and allowed our planets to settle in the pattern we see today. | 0:55:34 | 0:55:37 | |
So, what became of our missing lonely planet? | 0:55:40 | 0:55:43 | |
In the simulations I have, the planet is ejected from the solar system | 0:55:44 | 0:55:49 | |
with a speed of about 1km per second. | 0:55:49 | 0:55:52 | |
But this happened about four billion years ago, so do your math. | 0:55:54 | 0:55:59 | |
It will end up very far from the solar system, | 0:56:01 | 0:56:03 | |
so today it can be almost anywhere in the galaxy. | 0:56:03 | 0:56:07 | |
20 years ago, the mystery of the solar system began to unravel. | 0:56:20 | 0:56:24 | |
Evidence from alien worlds shattered the long-held view | 0:56:26 | 0:56:29 | |
that our planets have fixed orbits. | 0:56:29 | 0:56:32 | |
It led to a whole new understanding of a turbulent and dynamic past... | 0:56:34 | 0:56:37 | |
..which makes us wonder, might things have turned out differently? | 0:56:39 | 0:56:43 | |
The solar system could have done a lot of different things, | 0:56:43 | 0:56:46 | |
it could have evolved in a lot of different ways. | 0:56:46 | 0:56:49 | |
What we see in our own solar system | 0:56:49 | 0:56:51 | |
is the result of a lot of unlikely or random events, | 0:56:51 | 0:56:57 | |
and so our solar system is unique. | 0:56:57 | 0:56:59 | |
Ending up with a stable system of planets was just a fluke, | 0:57:03 | 0:57:07 | |
a lucky roll of the dice. | 0:57:07 | 0:57:09 | |
It's amazing we survived at all. | 0:57:10 | 0:57:12 | |
Getting an earth where we have our earth today was not a given | 0:57:12 | 0:57:17 | |
when this whole solar system started. | 0:57:17 | 0:57:19 | |
It took all these series of events to get a rocky planet | 0:57:19 | 0:57:22 | |
of this size at this distance with this amount of water | 0:57:22 | 0:57:25 | |
to build the earth that we live on today. | 0:57:25 | 0:57:28 | |
The fate of the entire solar system, including the earth, | 0:57:30 | 0:57:34 | |
was defined above all by the movements of our gas giant, Jupiter. | 0:57:34 | 0:57:38 | |
If Jupiter's orbit moved differently, | 0:57:40 | 0:57:43 | |
if Jupiter moved into the inner solar system, | 0:57:43 | 0:57:46 | |
then it's unlikely that the earth would be here. | 0:57:46 | 0:57:49 | |
Of all the planetary systems so far discovered, | 0:57:51 | 0:57:54 | |
it seems we are the only one with the lucky roll of the dice. | 0:57:54 | 0:57:58 | |
You might think that maybe the solar system that we have here | 0:57:59 | 0:58:02 | |
is actually the oddball and that the natural order | 0:58:02 | 0:58:05 | |
of things are these other systems that we think of as weird. | 0:58:05 | 0:58:09 | |
And, if we are so unusual, | 0:58:11 | 0:58:13 | |
will we ever find anywhere else in the universe so welcoming to life? | 0:58:13 | 0:58:17 | |
Even though our solar system might be...let's say one in a million - | 0:58:19 | 0:58:23 | |
that may seem like a really small number - | 0:58:23 | 0:58:26 | |
there are 100 billion stars in the galaxy. | 0:58:26 | 0:58:29 | |
So even something as unlikely as our solar system, | 0:58:29 | 0:58:32 | |
there may be lots of them around. | 0:58:32 | 0:58:35 |