Would you like to inspect the original subtitles? These are the user uploaded subtitles that are being translated:
1
00:00:00,000 --> 00:00:04,440
NASA's revolutionary Juno probe
2
00:00:04,520 --> 00:00:07,880
is on a daring voyage to Jupiter.
3
00:00:07,960 --> 00:00:13,720
Its goal, to reveal the deepest
mysteries of our solar system.
4
00:00:13,800 --> 00:00:16,560
Everything we see in the solar
system today
5
00:00:16,640 --> 00:00:20,200
is affected by Jupiter somehow,
in the past or now.
6
00:00:20,280 --> 00:00:25,600
All the asteroids, all the planets,
the moons, the comets...everything.
7
00:00:25,680 --> 00:00:28,320
So in many ways, Juno is actually
giving us a view
8
00:00:28,400 --> 00:00:31,720
into the history of our planetary
system, even the history of Earth.
9
00:00:32,960 --> 00:00:35,360
Juno's mission is risky.
10
00:00:35,440 --> 00:00:38,480
Jupiter could eat the
spacecraft...like that.
11
00:00:38,560 --> 00:00:43,520
But by diving perilously close to
this monstrous world,
12
00:00:43,600 --> 00:00:48,000
Juno could change everything we know
about our solar system.
13
00:00:48,080 --> 00:00:51,720
If you want to know what's
happening, you got to get up-close
and personal.
14
00:01:07,040 --> 00:01:10,280
Independence day, 2016...
15
00:01:10,360 --> 00:01:14,520
Juno arrives at Jupiter
and gets to work.
16
00:01:14,600 --> 00:01:17,640
The probe angles its high-resolution
camera
17
00:01:17,720 --> 00:01:20,320
towards this stormy world.
18
00:01:20,400 --> 00:01:23,480
Juno's snaps don't disappoint.
19
00:01:28,760 --> 00:01:32,160
The images returned from Juno are
just beautiful.
20
00:01:42,960 --> 00:01:46,360
Suddenly you have this magnificent
mosaic of this planet.
21
00:01:52,000 --> 00:01:54,560
As a human being, I'm like,
Oh, my gosh, look at this.
22
00:01:54,640 --> 00:01:57,120
"This is amazing. This is coming
back from Jupiter."
23
00:01:58,600 --> 00:02:01,360
These are the closest-ever views of
Jupiter,
24
00:02:01,440 --> 00:02:04,440
a world 500 million miles away.
25
00:02:14,640 --> 00:02:17,960
But we didn't send Juno just to take
pictures.
26
00:02:19,080 --> 00:02:24,400
One of its main goals is to peer deep
into Jupiter's dark heart.
27
00:02:24,480 --> 00:02:27,160
One of the big questions we have
about Jupiter is,
28
00:02:27,240 --> 00:02:29,360
does it have a core?
29
00:02:29,440 --> 00:02:32,360
And you'd think, well, of course
every planet has a core.
30
00:02:32,440 --> 00:02:34,960
The Earth has a core.
Everything does.
31
00:02:35,040 --> 00:02:37,040
Well, it turns out,
Jupiter might not.
32
00:02:39,440 --> 00:02:41,880
Knowing what lies at a planet's core
33
00:02:41,960 --> 00:02:46,520
allows scientists to wind back the
clock billions of years
34
00:02:46,600 --> 00:02:48,760
to the formation of the planets.
35
00:02:49,880 --> 00:02:53,640
If Juno can reveal what lies deep
within Jupiter,
36
00:02:53,720 --> 00:02:55,920
it could change our understanding
37
00:02:56,000 --> 00:02:59,040
of how the gas giant formed.
38
00:02:59,120 --> 00:03:01,920
If Juno finds a solid core,
39
00:03:02,000 --> 00:03:06,560
it could mean Jupiter first formed as
a rocky planet like Earth,
40
00:03:06,640 --> 00:03:09,040
then kept growing.
41
00:03:09,120 --> 00:03:11,440
But if Juno finds no core,
42
00:03:11,520 --> 00:03:14,720
it could mean that Jupiter skipped
the rocky stage
43
00:03:14,800 --> 00:03:17,840
and formed straight from
a cloud of gas.
44
00:03:19,040 --> 00:03:22,360
Answering this question could shine
a light
45
00:03:22,440 --> 00:03:24,440
on other mysteries, too.
46
00:03:25,920 --> 00:03:28,000
If we can figure out how Jupiter
formed,
47
00:03:28,080 --> 00:03:31,720
we can figure out the rest of the
story of the solar system.
48
00:03:34,240 --> 00:03:37,240
So how do you probe down into the
interior of a planet
49
00:03:37,320 --> 00:03:40,400
when all you can really see are the
very tops of the clouds?
50
00:03:40,480 --> 00:03:43,040
Well, incredibly, you can use
gravity.
51
00:03:43,120 --> 00:03:47,240
As Juno orbits Jupiter,
52
00:03:47,320 --> 00:03:51,880
it can sense in its orbit
tiny little variations
53
00:03:51,960 --> 00:03:55,280
in the gravitational pull of
Jupiter.
54
00:03:55,360 --> 00:03:57,920
As Juno speeds towards Jupiter,
55
00:03:58,000 --> 00:04:01,080
gravitational spikes tug at the
craft.
56
00:04:01,160 --> 00:04:06,040
It turns out, some parts of Jupiter
are denser than others.
57
00:04:06,120 --> 00:04:09,760
If Jupiter were some solid ball,
then as Juno passes by it,
58
00:04:09,840 --> 00:04:12,560
as it passes very close
above its cloud tops,
59
00:04:12,640 --> 00:04:15,400
the orbit, the trajectory,
would be very smooth.
60
00:04:15,480 --> 00:04:18,160
But in fact,
if Jupiter has layers
61
00:04:18,240 --> 00:04:20,440
or places where there's more mass
62
00:04:20,520 --> 00:04:23,760
and places where there's less,
then it's gonna pull on Juno
63
00:04:23,840 --> 00:04:25,840
a little bit differently.
64
00:04:25,920 --> 00:04:29,000
Passing over areas of
concentrated mass
65
00:04:29,080 --> 00:04:31,200
gives Juno a speed boost.
66
00:04:32,240 --> 00:04:34,880
So what they do is,
the engineers back on Earth
67
00:04:34,960 --> 00:04:38,080
can basically just say,
"How fast is it moving right now?
68
00:04:38,160 --> 00:04:40,160
How about now? How about now?"
69
00:04:40,240 --> 00:04:44,440
And you build up a map of where
the mass is in Jupiter
70
00:04:44,520 --> 00:04:47,560
underneath the spacecraft
as it passes around.
71
00:04:50,640 --> 00:04:54,880
Juno's instruments begin to map out
the heart of gas giant,
72
00:04:54,960 --> 00:04:59,560
revealing the mysterious core for the
first time.
73
00:04:59,640 --> 00:05:02,080
What Juno found was this amorphous
mass,
74
00:05:02,160 --> 00:05:04,800
a fuzzy thing in the centre of
Jupiter.
75
00:05:04,880 --> 00:05:07,440
It's not as solid as we expected
76
00:05:07,520 --> 00:05:09,520
if it were just a metal and rock
core,
77
00:05:09,600 --> 00:05:11,600
but there is something there.
78
00:05:12,920 --> 00:05:14,920
In the centre of the planet,
79
00:05:15,000 --> 00:05:17,640
Juno detects hydrogen and rocky
material
80
00:05:17,720 --> 00:05:20,240
dissolved and blended together.
81
00:05:20,320 --> 00:05:24,600
It's a type of planetary core we've
never seen before.
82
00:05:24,680 --> 00:05:28,240
Astronomers are describing it as
fuzzy.
83
00:05:29,240 --> 00:05:31,240
We thought we were gonna find an
avocado.
84
00:05:31,320 --> 00:05:33,800
Instead we found a bowl of chili.
85
00:05:33,880 --> 00:05:37,560
It's a hydrogen fluid
chili con carne.
86
00:05:40,040 --> 00:05:43,880
So none of our models of the
interior of Jupiter turned out
to be correct.
87
00:05:43,960 --> 00:05:46,520
That means we have to go back to the
drawing board.
88
00:05:47,960 --> 00:05:51,600
One theory is that Jupiter didn't
form from rocks or gas
89
00:05:51,680 --> 00:05:54,920
but from tiny pebbles less than an
inch wide,
90
00:05:55,000 --> 00:06:00,600
strewn across the early solar system
4.6 billion years ago.
91
00:06:01,720 --> 00:06:04,520
These pebbles came together.
They accreted
92
00:06:04,600 --> 00:06:06,600
to form a massive object
93
00:06:06,680 --> 00:06:09,520
that was the sort of seed,
the core of Jupiter.
94
00:06:10,520 --> 00:06:12,800
The swarm of pebbles clumped together
95
00:06:12,880 --> 00:06:15,080
to form one giant core
96
00:06:15,160 --> 00:06:17,720
twenty times the mass of Earth.
97
00:06:17,800 --> 00:06:22,760
But these pebbles can't sustain this
growing planet for long.
98
00:06:22,840 --> 00:06:26,440
Eventually, we need to make a jump
from those centimetre-size particles
99
00:06:26,520 --> 00:06:29,640
up to really large things, like
100-kilometer planetesimals,
100
00:06:29,720 --> 00:06:32,520
to really kick-start growth of a
planet.
101
00:06:34,520 --> 00:06:39,600
As Jupiter grows, its appetite
becomes insatiable.
102
00:06:39,680 --> 00:06:42,680
The cores of other
would-be planets are drawn in
103
00:06:42,760 --> 00:06:46,520
by its immense pull
and absorbed on impact,
104
00:06:46,600 --> 00:06:49,760
causing Jupiter's core to transform.
105
00:06:49,840 --> 00:06:53,680
Huge chunks of incoming rock are
mixed up with gas
106
00:06:53,760 --> 00:06:57,240
and the pebbles that originally built
the core.
107
00:06:58,240 --> 00:07:01,520
We think that the core material that
might've been there is actually
108
00:07:01,600 --> 00:07:05,600
dissolved and mixed in
with the rest of the planet.
109
00:07:05,680 --> 00:07:08,000
This mix of rock, gas, and pebbles
110
00:07:08,080 --> 00:07:10,640
leaves the core in a strange state.
111
00:07:10,720 --> 00:07:13,120
Somewhere between solid and liquid
112
00:07:13,200 --> 00:07:15,320
or, in other words, fuzzy.
113
00:07:16,400 --> 00:07:19,520
Once Jupiter's core reaches a
critical mass,
114
00:07:19,600 --> 00:07:24,560
its gravity starts sucking in all
nearby hydrogen gas...
115
00:07:24,640 --> 00:07:27,240
building the iconic Jovian atmosphere
116
00:07:27,320 --> 00:07:29,320
and leaving the fuzzy core
117
00:07:29,400 --> 00:07:33,640
trapped beneath thousands of miles
of thick clouds.
118
00:07:33,720 --> 00:07:37,960
And that is what formed Jupiter as
we know and love it today.
119
00:07:38,040 --> 00:07:42,360
Juno's discovery of Jupiter's fuzzy
core could rewrite the book
120
00:07:42,440 --> 00:07:44,960
on Jupiter's early years.
121
00:07:45,040 --> 00:07:47,360
But Juno is just getting started.
122
00:07:47,440 --> 00:07:49,800
We haven't even scratched the
surface
123
00:07:49,880 --> 00:07:53,440
of the number of mysteries
there are.
124
00:07:53,520 --> 00:07:56,280
There's more to Jupiter than meets
the eye
125
00:07:56,360 --> 00:08:00,800
as Juno's instruments begin to reveal
a darker side
126
00:08:00,880 --> 00:08:03,200
to this giant world.
127
00:08:03,280 --> 00:08:08,040
Jupiter's environment is one of the
most vicious in the solar system,
128
00:08:08,120 --> 00:08:12,320
and that's because of its incredibly
strong magnetic field.
129
00:08:12,400 --> 00:08:16,080
And Juno is caught right in the
middle of it.
130
00:08:20,560 --> 00:08:22,600
The gas giant, Jupiter,
131
00:08:22,680 --> 00:08:26,880
holds clues to the mysteries of our
solar system.
132
00:08:26,960 --> 00:08:29,400
And in 2011, NASA launches
133
00:08:29,480 --> 00:08:32,360
a billion-dollar mission
to uncover them.
134
00:08:32,440 --> 00:08:36,480
MAN: Three, two, one, ignition.
135
00:08:36,560 --> 00:08:42,000
And lift-off of the Atlas V with
Juno on a trek to Jupiter.
136
00:08:43,800 --> 00:08:47,800
To reach its target, Juno embarks on
a five-year journey.
137
00:08:50,800 --> 00:08:54,600
Sending any spacecraft to another
planet is gonna be tough,
138
00:08:54,680 --> 00:08:58,800
but sending one to Jupiter is really
pushing things pretty hard.
139
00:09:00,280 --> 00:09:02,640
Juno weaves through the solar system
140
00:09:02,720 --> 00:09:04,720
with extreme precision.
141
00:09:04,800 --> 00:09:08,000
The craft battles violent temperature
changes
142
00:09:08,080 --> 00:09:11,600
and navigates carefully through the
asteroid belt.
143
00:09:11,680 --> 00:09:14,360
If there's a fleck of dust
in your path
144
00:09:14,440 --> 00:09:16,440
and that thing slams into your
spacecraft,
145
00:09:16,520 --> 00:09:19,160
it could do significant damage.
146
00:09:19,240 --> 00:09:22,400
1.7 billion miles into its mission,
147
00:09:22,480 --> 00:09:25,360
Juno finally nears its target,
148
00:09:25,440 --> 00:09:28,000
but the probe is hurtling towards
Jupiter
149
00:09:28,080 --> 00:09:31,520
at 165,000 miles per hour.
150
00:09:33,240 --> 00:09:35,240
Juno is moving really fast.
151
00:09:35,320 --> 00:09:37,920
It's one of the fastest spacecraft
ever.
152
00:09:38,000 --> 00:09:39,720
You need to go fast enough to get
there
153
00:09:39,800 --> 00:09:43,400
but then you need to be slow enough
to be captured by the gravity of the
planet.
154
00:09:43,480 --> 00:09:46,200
You need to get it just right.
155
00:09:46,280 --> 00:09:49,720
Get it wrong and Juno could slam into
the planet
156
00:09:49,800 --> 00:09:52,240
or drift out into deep space.
157
00:09:57,080 --> 00:10:00,640
To successfully get Juno to enter a
stable orbit around Jupiter...
158
00:10:00,720 --> 00:10:02,720
it's almost the same as, say,
159
00:10:02,800 --> 00:10:04,800
shooting a basketball from London
160
00:10:04,880 --> 00:10:07,400
and having it on the land on the
front of the rim in New York
161
00:10:07,480 --> 00:10:09,480
and just sitting there balanced.
162
00:10:09,560 --> 00:10:14,320
I could do it... but can NASA do it
with Juno?
163
00:10:14,400 --> 00:10:16,400
(LAUGHING)
164
00:10:18,200 --> 00:10:20,360
NASA has a neat game plan.
165
00:10:20,440 --> 00:10:22,720
Juno performs a backflip in space
166
00:10:22,800 --> 00:10:25,800
and fires its thruster towards
Jupiter.
167
00:10:25,880 --> 00:10:27,880
Everything is going smoothly.
168
00:10:27,960 --> 00:10:30,560
We're continuing to burn and change
our velocity.
169
00:10:31,640 --> 00:10:35,000
The rocket burns for 35 nail-biting
minutes,
170
00:10:35,080 --> 00:10:39,160
reducing the craft's speed by 1,200
miles per hour.
171
00:10:44,600 --> 00:10:45,600
(CHEERING)
172
00:10:45,680 --> 00:10:48,480
Finally the probe achieves orbit
around Jupiter.
173
00:10:49,640 --> 00:10:53,080
Right on July 4th, during the
fireworks, we just got into orbit.
174
00:10:53,160 --> 00:10:55,800
In many ways,
we're firing a rocket motor.
175
00:10:55,880 --> 00:10:57,880
I mean, it is fireworks.
176
00:11:00,400 --> 00:11:03,840
Safe in orbit, Juno turns its
instruments to the planet
177
00:11:03,920 --> 00:11:06,080
for a critical part of the mission...
178
00:11:06,160 --> 00:11:08,840
Investigating Jupiter's magnetic
field.
179
00:11:11,520 --> 00:11:13,800
Deep below the stormy surface,
180
00:11:13,880 --> 00:11:18,400
liquid metallic hydrogen flows
endlessly around the planet,
181
00:11:18,480 --> 00:11:21,520
producing a huge magnetic field.
182
00:11:21,600 --> 00:11:26,240
This magnetosphere stretches over 600
million miles
183
00:11:26,320 --> 00:11:30,200
beyond the planet,
reaching all the way to Saturn.
184
00:11:35,240 --> 00:11:38,520
To reveal the true scale of Jupiter's
magnetosphere,
185
00:11:38,600 --> 00:11:42,000
planetary scientist Jani Radebaugh
hits the beach.
186
00:11:43,000 --> 00:11:45,040
I've made a little solar system.
187
00:11:45,120 --> 00:11:47,120
So we'll start here at the sun.
188
00:11:47,200 --> 00:11:49,360
We come out here to the Earth.
189
00:11:49,440 --> 00:11:51,800
And now we're going to skip a few
and go out to Jupiter.
190
00:11:51,880 --> 00:11:55,200
And Jupiter is five times as far
away from the sun as the Earth.
191
00:11:55,280 --> 00:11:57,280
Now, we'll go out to Saturn.
192
00:11:58,280 --> 00:12:01,520
Saturn here is ten times as far away
from the sun as the Earth.
193
00:12:01,600 --> 00:12:04,360
And we want to look at the size of
Jupiter's magnetic field.
194
00:12:04,440 --> 00:12:07,280
So we want to draw out the magnetic
field of Jupiter.
195
00:12:07,360 --> 00:12:09,680
It arches around like this...
196
00:12:09,760 --> 00:12:13,440
away from the sun because
the solar wind is impacting
the magnetic field,
197
00:12:13,520 --> 00:12:15,520
dragging it downwind.
198
00:12:15,600 --> 00:12:18,840
So here it comes downwind.
199
00:12:18,920 --> 00:12:20,920
On both sides.
200
00:12:21,000 --> 00:12:23,160
All the way out to the orbit of
Saturn.
201
00:12:25,320 --> 00:12:27,320
Jupiter's magnetosphere stretches
202
00:12:27,400 --> 00:12:30,320
over 600 million miles beyond the
planet.
203
00:12:31,360 --> 00:12:33,920
When you think about structures in
our solar system,
204
00:12:34,000 --> 00:12:35,840
of course,
you think of the giant sun,
205
00:12:35,920 --> 00:12:38,000
you think of massive planets like
Jupiter...
206
00:12:38,080 --> 00:12:42,200
But what if the largest things in
the solar system are things we
really can't see.
207
00:12:42,280 --> 00:12:44,280
And in fact the magnetic field of
Jupiter
208
00:12:44,360 --> 00:12:46,360
and all of the particles trapped
in it
209
00:12:46,440 --> 00:12:49,160
are one of the largest things the
solar system has to offer.
210
00:12:49,240 --> 00:12:52,600
If your eyes could actually see
Jupiter's magnetosphere
211
00:12:52,680 --> 00:12:55,440
and you tried to look at it while
standing on Earth,
212
00:12:55,520 --> 00:12:58,160
it would look about as big in the
sky as the moon.
213
00:12:59,720 --> 00:13:02,040
And within this magnetic field,
214
00:13:02,120 --> 00:13:04,480
Juno faces an invisible threat.
215
00:13:06,280 --> 00:13:09,560
Jupiter has an enormous magnetic
field.
216
00:13:09,640 --> 00:13:12,840
It is so enormous in terms of space,
217
00:13:12,920 --> 00:13:14,920
but also in terms of power.
218
00:13:15,440 --> 00:13:18,400
As Jupiter is bombarded by the solar
wind,
219
00:13:18,480 --> 00:13:20,480
high-energy particles from the sun
220
00:13:20,560 --> 00:13:23,320
are funnelled into deadly radiation
belts,
221
00:13:23,400 --> 00:13:27,120
guided by the giant planet's magnetic
field.
222
00:13:27,200 --> 00:13:31,360
The magnetic field traps charged
particles coming from the sun
223
00:13:31,440 --> 00:13:34,200
and circulates them around that
system
224
00:13:34,280 --> 00:13:37,480
and just bombards anything in the
vicinity,
225
00:13:37,560 --> 00:13:40,320
including our fragile little
spacecraft.
226
00:13:42,360 --> 00:13:46,360
Close to the planet, radiation levels
are up to 30 times greater
227
00:13:46,440 --> 00:13:48,440
than inside the reactor core room
228
00:13:48,520 --> 00:13:51,200
during the Chernobyl disaster.
229
00:13:51,280 --> 00:13:53,280
This is radiation.
230
00:13:53,360 --> 00:13:56,600
This is bad news. These particles,
they would hit you.
231
00:13:56,680 --> 00:13:59,760
They would rupture your DNA,
rupture your cell structures,
232
00:13:59,840 --> 00:14:01,840
and you would die.
233
00:14:03,280 --> 00:14:08,440
This blistering radiation is bad news
for the spacecraft too.
234
00:14:08,520 --> 00:14:10,680
The charged particles threaten to
destroy
235
00:14:10,760 --> 00:14:13,440
electronic and navigational systems,
236
00:14:13,520 --> 00:14:16,240
but Juno has armoured up.
237
00:14:17,280 --> 00:14:21,120
It's not some delicate, beautiful,
gossamer thing
238
00:14:21,200 --> 00:14:23,360
that you are sending to orbit
Jupiter.
239
00:14:23,440 --> 00:14:25,440
It's more like a tank.
240
00:14:25,520 --> 00:14:27,520
You have to protect this thing
or else
241
00:14:27,600 --> 00:14:29,600
it's not going to last very long
at all.
242
00:14:31,160 --> 00:14:34,400
We've got a couple hundred pounds
of titanium
243
00:14:34,480 --> 00:14:36,680
on the spacecraft
just trying to shield us
244
00:14:36,760 --> 00:14:39,000
from what Jupiter might throw at us.
245
00:14:39,080 --> 00:14:42,200
So it is, in a sense, like an
armoured tank going into war.
246
00:14:43,640 --> 00:14:46,560
Lightweight titanium is tough.
247
00:14:46,640 --> 00:14:50,080
Juno's half inch thick shielding
blocks 99%
248
00:14:50,160 --> 00:14:52,440
of Jupiter's vicious radiation.
249
00:14:52,520 --> 00:14:54,520
But even at this reduced rate,
250
00:14:54,600 --> 00:14:57,000
Juno can't survive the bombardment
for long.
251
00:14:57,080 --> 00:15:00,480
So the craft sets itself on a
unique orbit
252
00:15:00,560 --> 00:15:02,680
around the gas giant.
253
00:15:06,960 --> 00:15:09,240
It actually has a very long orbit
254
00:15:09,320 --> 00:15:11,880
where it spends most of its time
far away.
255
00:15:11,960 --> 00:15:14,440
And then every once in a while
dives in and goes,
256
00:15:14,520 --> 00:15:16,520
"Oh, hot, hot, hot.
I zoomed in too much,"
257
00:15:16,600 --> 00:15:19,080
and then goes safely away to
communicate and process
258
00:15:19,160 --> 00:15:21,160
and then back in again.
259
00:15:23,160 --> 00:15:25,160
Juno takes a mighty gamble
260
00:15:25,240 --> 00:15:27,600
diving deep into these radiation
belts
261
00:15:27,680 --> 00:15:30,320
to achieve one of its key objectives,
262
00:15:30,400 --> 00:15:33,800
mapping Jupiter's giant magnetic
field.
263
00:15:33,880 --> 00:15:36,880
And as Juno swoops around the planet,
264
00:15:36,960 --> 00:15:40,840
it reveals something scientists have
never seen before.
265
00:15:42,520 --> 00:15:45,800
Planetary scientist Dan Durda
demonstrates.
266
00:15:45,880 --> 00:15:49,920
We can use a pretty simple, even
elementary school level experiment
267
00:15:50,000 --> 00:15:52,600
of the structure of the Earth's
magnetic field
268
00:15:52,680 --> 00:15:55,200
by shaking some iron filings
269
00:15:55,280 --> 00:15:57,320
across the surface
270
00:15:57,400 --> 00:15:59,760
of very simple bar magnet
with a north and south pole.
271
00:15:59,840 --> 00:16:03,800
Earth's magnetic field forms a
perfect bubble around our planet,
272
00:16:03,880 --> 00:16:06,880
protecting us from solar radiation
and cosmic rays.
273
00:16:06,960 --> 00:16:09,520
If I can get these little iron
fillings to come out here...
274
00:16:09,600 --> 00:16:12,200
And already I can see,
275
00:16:12,280 --> 00:16:14,920
the sort of classic outlines
276
00:16:15,000 --> 00:16:19,120
of the north and south magnetic
field lines that are coming out
of our planet.
277
00:16:19,200 --> 00:16:23,920
The Earth's magnetic field is pretty
well behaved in this way. It's what
we call a dipolar field.
278
00:16:24,000 --> 00:16:27,960
It has a very distinct north and
south magnetic pole.
279
00:16:28,040 --> 00:16:31,800
Lucky for us, Earth's magnetic field
is pretty stable.
280
00:16:31,880 --> 00:16:36,640
But new results from Juno suggests
that Jupiter may not be so fortunate.
281
00:16:37,840 --> 00:16:40,920
Jupiter's magnetic field is much
more complex than this.
282
00:16:41,000 --> 00:16:43,040
Jupiter is not going to play by
those rules.
283
00:16:43,120 --> 00:16:46,920
Its magnetic fields are going to do
whatever it wants.
284
00:16:47,000 --> 00:16:50,680
And the generation of that magnetic
field
285
00:16:50,760 --> 00:16:53,760
is so complex
and so twisted and and so wild
286
00:16:53,840 --> 00:16:58,400
that the magnetic field is gonna
have very strange shapes
287
00:16:58,480 --> 00:17:00,720
that we're just now beginning to
understand.
288
00:17:00,800 --> 00:17:04,200
When you look at the Earth, we have
a fairly simple magnetic field.
289
00:17:04,280 --> 00:17:08,120
It's like a giant bar magnet with a
north and south magnetic pole.
290
00:17:08,200 --> 00:17:10,200
Well, Jupiter has that as well.
291
00:17:10,280 --> 00:17:13,520
This is called a dipolar field.
It's got two poles.
292
00:17:13,600 --> 00:17:16,080
But it also has a third pole.
293
00:17:17,960 --> 00:17:19,960
Juno's magnetic field maps
294
00:17:20,040 --> 00:17:22,040
shows a north and south pole
295
00:17:22,120 --> 00:17:25,720
and a bizarre magnetic disturbance at
Jupiter's equator.
296
00:17:25,800 --> 00:17:29,320
And it's like Jupiter just sprouted
a third arm,
297
00:17:29,400 --> 00:17:31,400
and that's kind of mysterious.
298
00:17:32,440 --> 00:17:34,440
On magnetic field maps,
299
00:17:34,520 --> 00:17:38,080
north poles show up red and south
poles blue.
300
00:17:38,160 --> 00:17:40,920
So scientists are calling this second
south pole
301
00:17:41,000 --> 00:17:43,000
the Great Blue Spot.
302
00:17:43,080 --> 00:17:45,640
Everyone knows about the
Great Red Spot,
303
00:17:45,720 --> 00:17:49,080
but Jupiter now has a
Great Blue Spot as well.
304
00:17:49,160 --> 00:17:51,560
This magnetic disturbance reflects
305
00:17:51,640 --> 00:17:53,960
Jupiter's stormy interior.
306
00:17:54,040 --> 00:17:57,800
You have these fast-moving winds
blowing on the magnetic field,
307
00:17:57,880 --> 00:18:01,760
and they're actually shearing it
apart and moving the field around.
308
00:18:01,840 --> 00:18:04,520
It's not necessarily a storm,
although it could be.
309
00:18:04,600 --> 00:18:07,320
It maybe is better to think of it as
a magnetic storm.
310
00:18:10,480 --> 00:18:12,600
Turbulence inside Jupiter could be
311
00:18:12,680 --> 00:18:16,400
twisting up the magnetic field to
drive the Great Blue Spot
312
00:18:16,480 --> 00:18:18,480
and the deadly radiation belts
313
00:18:18,560 --> 00:18:21,520
that Juno must navigate through.
314
00:18:21,600 --> 00:18:26,680
Unlike Earth, Jupiter is not really
a solid mass for the most part.
315
00:18:26,760 --> 00:18:29,520
So all of its clouds and gases
316
00:18:29,600 --> 00:18:32,000
are moving at slightly different
rates
317
00:18:32,080 --> 00:18:34,520
and that actually makes
the magnetic field
318
00:18:34,600 --> 00:18:39,240
that's generated very variable and
highly changing.
319
00:18:39,320 --> 00:18:42,160
For us to have a variable magnetic
field like Jupiter does,
320
00:18:42,240 --> 00:18:44,400
the entire Earth would have to be
molten.
321
00:18:44,480 --> 00:18:46,480
We really don't want that to happen.
322
00:18:46,560 --> 00:18:48,560
With each orbit of Jupiter,
323
00:18:48,640 --> 00:18:52,040
Juno unravels more mysteries of this
giant planet.
324
00:18:52,120 --> 00:18:54,120
But Jupiter's deepest secret
325
00:18:54,200 --> 00:18:57,560
could shine a light on our own
origins.
326
00:18:57,640 --> 00:19:00,960
If we want to understand the Earth
and our place in the solar system,
327
00:19:01,040 --> 00:19:03,360
Juno has found that a lot of those
mysteries
328
00:19:03,440 --> 00:19:05,440
are locked up there in Jupiter.
329
00:19:11,000 --> 00:19:14,680
The Juno spacecraft is uncovering the
secrets of Jupiter
330
00:19:14,760 --> 00:19:18,400
from its swirling cloud tops to its
dark heart.
331
00:19:18,480 --> 00:19:23,160
But Juno's discoveries go beyond the
gas giant itself.
332
00:19:23,240 --> 00:19:28,160
They could answer mysteries about our
own planet.
333
00:19:28,240 --> 00:19:32,960
Jupiter is the key to the formation
of the solar system,
334
00:19:33,040 --> 00:19:35,120
which means it's the key to
understanding
335
00:19:35,200 --> 00:19:37,520
how the Earth formed.
336
00:19:37,600 --> 00:19:40,960
Juno is actually giving us a view
into the history of our planetary
system,
337
00:19:41,040 --> 00:19:43,680
even the history of Earth.
338
00:19:43,760 --> 00:19:46,680
4.6 billion years ago,
339
00:19:46,760 --> 00:19:52,680
a mammoth cloud of hydrogen gas and
cosmic dust collapses,
340
00:19:52,760 --> 00:19:55,640
sparking nuclear fusion.
341
00:19:55,720 --> 00:19:57,720
From the resulting chaos,
342
00:19:57,800 --> 00:20:00,640
one star, four rocky worlds,
343
00:20:00,720 --> 00:20:03,600
and four gassy giants are born
344
00:20:03,680 --> 00:20:06,040
to form our solar system.
345
00:20:08,400 --> 00:20:10,760
There's these distinct zones of the
solar system...
346
00:20:10,840 --> 00:20:12,560
rocky and metallic in the
inner part,
347
00:20:12,640 --> 00:20:14,760
gaseous and water-rich in the
outer part.
348
00:20:14,840 --> 00:20:17,520
And even without thinking about that
too hard,
349
00:20:17,600 --> 00:20:21,400
it kind of makes sense cos getting
close to the sun, it's warmer.
350
00:20:21,480 --> 00:20:23,840
Out farther away from the sun,
it's cooler.
351
00:20:26,040 --> 00:20:28,640
But the Earth breaks the mould.
352
00:20:28,720 --> 00:20:33,520
Our planet has far more life-giving
water than theories predict.
353
00:20:33,600 --> 00:20:35,840
The Earth formed in a part of the
solar system that,
354
00:20:35,920 --> 00:20:38,240
you'd think normally should be
probably pretty dry
355
00:20:38,320 --> 00:20:40,320
cos it was pretty close to the sun.
356
00:20:40,400 --> 00:20:45,280
Our planet is just 150 million miles
from the sun,
357
00:20:45,360 --> 00:20:49,680
putting us inside what scientists
call the snow line.
358
00:20:49,760 --> 00:20:53,160
Inside this line, the sun is powerful
enough
359
00:20:53,240 --> 00:20:56,640
to evaporate water during a planet's
formation.
360
00:20:58,320 --> 00:21:00,880
Inside the snow line,
the temperatures are high
361
00:21:00,960 --> 00:21:03,560
and there's a lot of energy
from the sun nearby.
362
00:21:03,640 --> 00:21:05,840
Too close to the sun,
those gaseous
363
00:21:05,920 --> 00:21:08,520
and ice-rich materials
just can't exist.
364
00:21:08,600 --> 00:21:10,760
They're evaporated away by the heat
of the sun.
365
00:21:12,400 --> 00:21:15,880
Our watery world should be a dry rock
in space.
366
00:21:17,120 --> 00:21:19,640
Understanding how water got to the
Earth is so important
367
00:21:19,720 --> 00:21:22,520
because it wouldn't be there in the
very, very beginning.
368
00:21:23,960 --> 00:21:27,280
But Jupiter could hold the answer to
this mystery.
369
00:21:28,520 --> 00:21:30,760
To solve the riddle of Earth's water,
370
00:21:30,840 --> 00:21:33,840
Juno aims to discover where
Jupiter was born.
371
00:21:35,680 --> 00:21:40,320
Understanding how and where and when
Jupiter formed is critical.
372
00:21:40,400 --> 00:21:44,600
Because it has really dominated
the entire evolution of the
solar system.
373
00:21:44,680 --> 00:21:46,680
It's the biggest planet by far.
374
00:21:46,760 --> 00:21:51,040
It's the biggest thing out there,
that's moving everything around.
375
00:21:51,120 --> 00:21:53,480
Any water in the early solar system
376
00:21:53,560 --> 00:21:57,200
could have been moved around by
Jupiter's mighty gravity.
377
00:21:57,280 --> 00:22:00,200
So if Juno can trace Jupiter's
history,
378
00:22:00,280 --> 00:22:03,040
that could explain why we find H2O
379
00:22:03,120 --> 00:22:05,440
where it's least expected.
380
00:22:05,520 --> 00:22:09,280
We know that planets can move closer
to the sun and farther out
381
00:22:09,360 --> 00:22:11,880
while they're forming and even after
they form.
382
00:22:11,960 --> 00:22:15,520
So how do we figure out where
Jupiter formed?
383
00:22:15,600 --> 00:22:20,200
The key is how much water is locked
up inside Jupiter.
384
00:22:20,280 --> 00:22:23,120
If we can understand how Jupiter
385
00:22:23,200 --> 00:22:25,200
built a relationship with water,
386
00:22:25,280 --> 00:22:27,280
we can understand how water got
387
00:22:27,360 --> 00:22:31,200
distributed all throughout the solar
system including here on Earth.
388
00:22:34,080 --> 00:22:37,120
If Juno can measure the water content
of Jupiter,
389
00:22:37,200 --> 00:22:39,480
it will solve a 20 year old mystery.
390
00:22:42,360 --> 00:22:45,000
December, 1995.
391
00:22:45,080 --> 00:22:49,920
NASA's Galileo probe begins a fatal
dive into Jupiter's atmosphere.
392
00:22:51,680 --> 00:22:54,760
When it did, it was able to measure
393
00:22:54,840 --> 00:22:57,320
the atmosphere around it and
detect water.
394
00:22:57,400 --> 00:22:59,600
And the thing is, it didn't.
395
00:22:59,680 --> 00:23:02,720
Didn't find any, and that's weird.
396
00:23:02,800 --> 00:23:04,960
Everything was bone dry.
397
00:23:05,040 --> 00:23:07,640
So why in the world did Jupiter's
atmosphere look dry?
398
00:23:08,880 --> 00:23:12,000
If the results from the Galileo probe
are correct,
399
00:23:12,080 --> 00:23:14,280
Then 4.6 billion years ago
400
00:23:14,360 --> 00:23:16,560
Jupiter formed closer to the sun.
401
00:23:18,320 --> 00:23:20,960
But that's not the whole story.
402
00:23:21,040 --> 00:23:25,160
20 years later, NASA sends Juno to
get a second opinion.
403
00:23:26,440 --> 00:23:30,600
Juno is an orbiter so it's loaded
with instruments and detectors
404
00:23:30,680 --> 00:23:34,320
to look down on Jupiter and try to
figure out everything going on.
405
00:23:35,800 --> 00:23:40,200
Juno doesn't have to risk it's life
to hunt for water.
406
00:23:40,280 --> 00:23:42,880
The craft pierced through Jupiter's
thick clouds
407
00:23:42,960 --> 00:23:45,320
using a microwave radiometer
408
00:23:45,400 --> 00:23:48,560
- to detect H2
- O from a safe distance.
409
00:23:48,640 --> 00:23:50,640
Using these microwaves,
410
00:23:50,720 --> 00:23:53,800
Juno builds up a global map of
Jupiter's water.
411
00:23:54,800 --> 00:23:59,200
What Juno has found is, yeah,
there's plenty of water in Jupiter.
412
00:23:59,280 --> 00:24:02,440
It's just that Galileo happened to
hit a dry spot.
413
00:24:02,520 --> 00:24:05,080
But, in fact, if it had come in
almost anywhere else,
414
00:24:05,160 --> 00:24:07,160
it would've seen plenty of water.
415
00:24:09,040 --> 00:24:11,960
Juno's findings may give scientists
a clue
416
00:24:12,040 --> 00:24:14,800
to understanding where Jupiter
originally formed.
417
00:24:16,080 --> 00:24:19,080
It seems apparent now that Jupiter
418
00:24:19,160 --> 00:24:22,800
didn't form in its present location.
419
00:24:22,880 --> 00:24:27,440
The leading theory is that Jupiter
formed just beyond the Snow line -
420
00:24:27,520 --> 00:24:30,360
the boundary between the dry
inner solar system
421
00:24:30,440 --> 00:24:32,800
and the wet outer solar system.
422
00:24:32,880 --> 00:24:35,960
But we find Jupiter is twice as far
away from the sun
423
00:24:36,040 --> 00:24:38,320
as where that original Snow line
would've been.
424
00:24:38,400 --> 00:24:40,520
So this is telling us something
interesting.
425
00:24:42,640 --> 00:24:45,960
Jupiter may have wandered from its
original position,
426
00:24:46,040 --> 00:24:48,040
causing unimaginable chaos.
427
00:24:49,040 --> 00:24:51,400
As Jupiter moved around,
things got hit
428
00:24:51,480 --> 00:24:53,560
and knocked out of the solar system.
429
00:24:53,640 --> 00:24:56,040
It essentially scatters everything
in its path.
430
00:24:56,120 --> 00:24:58,760
It's the biggest player.
It's the biggest planet.
431
00:24:58,840 --> 00:25:00,840
Everything moves for it.
432
00:25:02,240 --> 00:25:06,360
As Jupiter bulldozes towards
the outer solar system,
433
00:25:06,440 --> 00:25:09,360
it slings ice ridged asteroids
and comets
434
00:25:09,440 --> 00:25:12,440
in towards the sun and towards Earth.
435
00:25:15,920 --> 00:25:17,920
Jupiter would literally,
in some sense,
436
00:25:18,000 --> 00:25:20,920
have snow ploughed into the inner
solar system.
437
00:25:21,000 --> 00:25:23,080
A whole wave of water rich
planetesimals
438
00:25:23,160 --> 00:25:26,680
that would've delivered much of our
Earth's oceans.
439
00:25:28,160 --> 00:25:31,240
Juno has helped answer why Earth
is habitable
440
00:25:31,320 --> 00:25:34,120
despite being so close to the sun.
441
00:25:34,200 --> 00:25:36,600
So it was worth going all that
distance,
442
00:25:36,680 --> 00:25:39,560
sending Juno all the way out there
to get that closer look.
443
00:25:43,400 --> 00:25:45,440
Our solar system plays host
444
00:25:45,520 --> 00:25:48,400
to some epic natural wonders.
445
00:25:48,480 --> 00:25:51,080
The ice geysers of Enceladus,
446
00:25:51,160 --> 00:25:53,360
the giant rings of Saturn,
447
00:25:53,440 --> 00:25:57,400
the Martian mega volcano,
Olympus Mons.
448
00:25:57,480 --> 00:25:59,880
But in July, 2017,
449
00:25:59,960 --> 00:26:03,680
NASA's Juno probe skims the surface
of Jupiter
450
00:26:03,760 --> 00:26:07,440
and photographs the most famous
natural wonder.
451
00:26:07,520 --> 00:26:10,480
A fierce hurricane-like storm
452
00:26:10,560 --> 00:26:13,600
that's been raging for hundreds of
years.
453
00:26:15,400 --> 00:26:19,120
When you think of Jupiter, one of
the most visually stunning,
454
00:26:19,200 --> 00:26:23,200
most iconic features of the
atmosphere is the Great Red Spot.
455
00:26:23,280 --> 00:26:26,680
There is nothing like Jupiter's Red
Spot in our entire solar system.
456
00:26:27,680 --> 00:26:30,960
As Juno soars over the
Great Red Spot,
457
00:26:31,040 --> 00:26:33,240
it looks down onto a storm
458
00:26:33,320 --> 00:26:36,120
over 10,000 miles across.
459
00:26:39,360 --> 00:26:41,520
This is the most extreme storm.
460
00:26:41,600 --> 00:26:44,560
The winds are blowing continuously
at 400 miles an hour.
461
00:26:48,560 --> 00:26:52,160
Earth's most powerful Category Five
hurricanes
462
00:26:52,240 --> 00:26:56,160
are less than half as powerful
as the storm on Jupiter.
463
00:26:57,920 --> 00:27:00,080
The Great Red Spot is the
464
00:27:00,160 --> 00:27:02,440
greatest hurricane that you've ever
imagined.
465
00:27:02,520 --> 00:27:04,840
But that's not all.
466
00:27:04,920 --> 00:27:08,360
Juno's microwave radiometer allows
scientists to see through
467
00:27:08,440 --> 00:27:11,680
Jupiter's cloud layers
for the first time.
468
00:27:12,920 --> 00:27:16,400
Juno has instrumentation that's able
to look underneath.
469
00:27:16,480 --> 00:27:20,600
So one of the things we did was, we
looked at how deep are the roots?
470
00:27:20,680 --> 00:27:24,760
Juno peers down into the eye of this
monster storm.
471
00:27:24,840 --> 00:27:29,560
It spots temperature changes that
follow the storm's iconic shape.
472
00:27:29,640 --> 00:27:32,160
Tracing the roots of the
Great Red Spot
473
00:27:32,240 --> 00:27:34,440
deep into the Jovian atmosphere.
474
00:27:35,560 --> 00:27:40,720
They found out that it goes down
over 200 miles deep into the
atmosphere.
475
00:27:40,800 --> 00:27:43,200
There's nothing like that on Earth
476
00:27:43,280 --> 00:27:46,440
Weather satellites circling the Earth
show the greatest
477
00:27:46,520 --> 00:27:49,280
cyclones of our planet
can reach heights
478
00:27:49,360 --> 00:27:51,520
of around ten miles.
479
00:27:51,600 --> 00:27:55,520
But Jupiter's Great Red Spot is 20
times taller.
480
00:27:56,760 --> 00:27:58,960
I think that really brings into
perspective
481
00:27:59,040 --> 00:28:01,200
the massive scale of this planet.
482
00:28:02,520 --> 00:28:05,360
The dizzying depths of the storm is
made possible
483
00:28:05,440 --> 00:28:07,800
by Jupiter's vast hidden atmosphere.
484
00:28:07,880 --> 00:28:10,200
A seemingly endless spinning mass
485
00:28:10,280 --> 00:28:13,200
made up of hydrogen and helium.
486
00:28:13,280 --> 00:28:17,960
Jupiter doesn't have a solid surface
like the Earth does.
487
00:28:18,040 --> 00:28:21,400
And so right away, if you were to
dive into Jupiter's clouds
488
00:28:21,480 --> 00:28:25,040
things are gonna be really
different. This atmosphere's
tremendously thick.
489
00:28:25,120 --> 00:28:27,440
As you're going in
the pressure is going up.
490
00:28:28,920 --> 00:28:31,760
As soon as you start plunging down
into that atmosphere
491
00:28:31,840 --> 00:28:34,680
there's more and more.
There's not just a 100 miles of air,
492
00:28:34,760 --> 00:28:38,320
there's a 1,000 miles of air,
10,000 miles of air above you.
493
00:28:38,400 --> 00:28:42,240
And not only would your ears pop
deep in the Jovian atmosphere,
494
00:28:42,320 --> 00:28:44,520
your entire body would pop
495
00:28:44,600 --> 00:28:47,800
and, in fact,
all of your molecules would pop.
496
00:28:49,760 --> 00:28:52,280
Juno's vast turbulent atmosphere
497
00:28:52,360 --> 00:28:56,880
hosts the deepest storm
mankind has ever seen.
498
00:28:56,960 --> 00:28:58,960
And Juno's discoveries
499
00:28:59,040 --> 00:29:01,240
gets scientists wondering...
500
00:29:01,320 --> 00:29:03,320
Could the Great Red Spot
501
00:29:03,400 --> 00:29:06,280
be behind another of Jupiter's
mysteries,
502
00:29:06,360 --> 00:29:09,840
the planet's surprisingly warm
atmosphere?
503
00:29:12,440 --> 00:29:15,080
Jupiter lurks out in our
outer solar system,
504
00:29:15,160 --> 00:29:17,720
where everything is very cold,
the sun is very dim
505
00:29:17,800 --> 00:29:20,320
when you get that far away.
506
00:29:20,400 --> 00:29:23,280
Jupiter is five times farther from
the sun than we are.
507
00:29:23,360 --> 00:29:26,160
So it's only getting four percent of
the amount of energy
508
00:29:26,240 --> 00:29:27,680
from the sun that we do.
509
00:29:27,760 --> 00:29:30,720
But there's something heating up
the atmosphere of Jupiter.
510
00:29:30,800 --> 00:29:34,720
There are parts of it that are
many times warmer than we can
explain with sunlight.
511
00:29:34,800 --> 00:29:37,680
The question is, of course,
where is that energy coming from?
512
00:29:39,240 --> 00:29:42,200
Juno swoops in for another pass
on Jupiter,
513
00:29:42,280 --> 00:29:46,040
turning its high resolution cameras
on the raging storm below.
514
00:29:48,440 --> 00:29:50,840
The storm unleashes vicious
turbulence
515
00:29:50,920 --> 00:29:53,080
into the surrounding atmosphere,
516
00:29:53,160 --> 00:29:55,360
giving scientists the clue they need
517
00:29:55,440 --> 00:29:57,960
to explain the planet's high
temperature.
518
00:29:59,200 --> 00:30:02,360
The Great Red Spot is a giant
hurricane
519
00:30:02,440 --> 00:30:06,880
that's powered by heat deep in the
core of Jupiter.
520
00:30:06,960 --> 00:30:10,880
But it has such violent and chaotic
motion,
521
00:30:10,960 --> 00:30:13,000
it's mixing up the atmosphere
around it.
522
00:30:16,760 --> 00:30:20,520
The thunder storms on Jupiter are
gonna be generating booming thunder
523
00:30:20,600 --> 00:30:22,720
just the same way they do here on
the Earth.
524
00:30:24,680 --> 00:30:26,800
Thunder clouds and sound waves
525
00:30:26,880 --> 00:30:28,880
rippling through the storm.
526
00:30:31,720 --> 00:30:34,680
A sound wave is
527
00:30:34,760 --> 00:30:37,680
a wave of pressure, of compression,
528
00:30:37,760 --> 00:30:42,240
where air molecules or water
molecules get compacted.
529
00:30:42,320 --> 00:30:45,440
They get squeezed together.
When you squeeze something together,
530
00:30:45,520 --> 00:30:48,480
they are lot closer together and
they're gonna get pretty hot.
531
00:30:51,240 --> 00:30:55,200
These sound waves shoot up 500 miles
above the storm
532
00:30:56,440 --> 00:30:59,440
where they break,
converting sound energy into heat.
533
00:31:00,840 --> 00:31:03,600
The sound waves,
they crash together
534
00:31:03,680 --> 00:31:07,000
creating tremendous amount
of energy, heating the gases
around them.
535
00:31:09,600 --> 00:31:12,760
The Great Red Spot has helped heat
the Jovian atmosphere
536
00:31:12,840 --> 00:31:14,840
for hundreds of years.
537
00:31:14,920 --> 00:31:19,280
But new images suggest that this
may be about to change.
538
00:31:20,600 --> 00:31:25,560
Jupiter's red spot is so big, it's
bigger than Earth by a long shot.
539
00:31:25,640 --> 00:31:28,680
It seems like it would be an
incredibly stable thing.
540
00:31:28,760 --> 00:31:31,960
It's just there and it's always been
there and it always will be.
541
00:31:32,040 --> 00:31:34,120
Recently we've seen it changing.
542
00:31:36,040 --> 00:31:40,600
When NASA's Voyager Space Probe
visited Jupiter in 1979,
543
00:31:40,680 --> 00:31:44,800
it observed a storm twice the
diameter of the Earth.
544
00:31:44,880 --> 00:31:46,880
In 2017,
545
00:31:46,960 --> 00:31:49,800
Juno's images showed the
Great Red Spot
546
00:31:49,880 --> 00:31:52,760
has lost one-third of its width.
547
00:31:52,840 --> 00:31:54,840
But that's not all.
548
00:31:54,920 --> 00:31:57,760
Despite the storm's shrinking size,
549
00:31:57,840 --> 00:32:00,640
it's actually getting taller.
550
00:32:00,720 --> 00:32:03,560
The Great Red Spot is being stretched
and forced
551
00:32:03,640 --> 00:32:06,640
into Jupiter's upper atmosphere.
552
00:32:06,720 --> 00:32:09,440
The storms in the Great Red Spot
is kind of like
553
00:32:09,520 --> 00:32:11,600
the clay on a potter's wheel
where,
554
00:32:11,680 --> 00:32:14,880
as you bring your hands closer
together to draw the clay in,
555
00:32:14,960 --> 00:32:18,080
the closer your hands are,
the taller the pottery becomes.
556
00:32:18,160 --> 00:32:21,760
And similarly for the storm,
as it becomes smaller at the base
557
00:32:21,840 --> 00:32:24,040
it raises taller to the
upper atmosphere.
558
00:32:25,480 --> 00:32:29,920
It's getting taller. And we see
storms do the same thing on Earth
and when it does that
559
00:32:30,000 --> 00:32:33,760
the wind shear will take the top of
the storm off and drag it apart.
560
00:32:33,840 --> 00:32:36,320
So we'll be watching it over the
next few years
561
00:32:36,400 --> 00:32:38,920
to see if that's what happens on
Jupiter as well.
562
00:32:40,640 --> 00:32:44,400
It may be only a matter of time
before Jupiter's high altitude winds
563
00:32:44,480 --> 00:32:47,440
tear the iconic storm to shreds.
564
00:32:47,520 --> 00:32:52,480
The most famous storm of our solar
system may soon disappear.
565
00:32:52,560 --> 00:32:55,040
But Juno reveals other storms
566
00:32:55,120 --> 00:32:57,960
hidden in the strangest of places.
567
00:33:04,160 --> 00:33:06,520
NASA's Juno probe has voyaged
568
00:33:06,600 --> 00:33:09,600
billions of miles across the solar
system,
569
00:33:09,680 --> 00:33:12,960
to reveal the mysteries of gas giant
Jupiter.
570
00:33:13,040 --> 00:33:18,000
But there's one part of Jupiter that
has remained hidden until now.
571
00:33:18,080 --> 00:33:20,880
Before Juno, our view of Jupiter
was very limited.
572
00:33:20,960 --> 00:33:23,120
We'd never actually flown over
the poles.
573
00:33:23,200 --> 00:33:25,560
It's something that's very hard to
do on Jupiter.
574
00:33:25,640 --> 00:33:28,520
We don't have other missions that
have done this.
575
00:33:28,600 --> 00:33:30,920
In August, 2016,
576
00:33:31,000 --> 00:33:35,400
Juno's flight plan takes the
spacecraft into unknown territory
577
00:33:35,480 --> 00:33:39,960
to reveal Jupiter's mysterious Polar
regions for the first time.
578
00:33:41,120 --> 00:33:43,320
The first time we looked
at the pole,
579
00:33:43,400 --> 00:33:46,360
it didn't look anything like
the Jupiter we knew.
580
00:33:48,880 --> 00:33:50,880
We never would've guessed that was
Jupiter
581
00:33:50,960 --> 00:33:52,960
if somebody had shown that to us.
582
00:33:55,240 --> 00:33:59,640
Juno's camera reveals a strange blue
expanse that puzzle scientists.
583
00:34:02,640 --> 00:34:06,880
The electric colour could be due to
chemical changes in the clouds
584
00:34:06,960 --> 00:34:09,200
brought on by a lack of sunlight.
585
00:34:09,280 --> 00:34:13,280
But what Juno spots inside the blue
clouds is even stranger.
586
00:34:16,840 --> 00:34:19,560
Giant central cyclones spin around
each pole
587
00:34:19,640 --> 00:34:22,000
at 200 miles per hour.
588
00:34:22,080 --> 00:34:26,680
With these cyclones surrounded by
eight stormy vortices in the North,
589
00:34:26,760 --> 00:34:28,760
and five in the South.
590
00:34:31,720 --> 00:34:35,240
There are these weird cyclones,
gigantic swirls,
591
00:34:35,320 --> 00:34:38,760
vortices of gas
swirling around Jupiter's poles
592
00:34:38,840 --> 00:34:41,160
and they're clearly forming
patterns.
593
00:34:42,200 --> 00:34:44,240
It's hard to get a sense of scale
here.
594
00:34:44,320 --> 00:34:47,720
The North Polar central cyclone,
that one right at the pole,
595
00:34:47,800 --> 00:34:50,200
that's 2,500 miles across.
596
00:34:50,280 --> 00:34:53,600
That is almost as big as the
Continental United States.
597
00:34:53,680 --> 00:34:55,880
What is going on there?
598
00:34:55,960 --> 00:34:58,280
This is nothing like what we see on
Earth.
599
00:35:01,200 --> 00:35:03,200
On Earth our weather is
600
00:35:03,280 --> 00:35:05,360
driven by heat from the sun.
601
00:35:05,440 --> 00:35:07,840
It hits our planet at the equator
602
00:35:07,920 --> 00:35:10,680
and flows across the surface.
603
00:35:10,760 --> 00:35:14,400
Powerful cyclones form over tropical
waters
604
00:35:14,480 --> 00:35:16,920
and move around the planet.
605
00:35:17,000 --> 00:35:20,880
But the polar regions receive less
energy from the sun,
606
00:35:20,960 --> 00:35:23,640
so cyclones can't form at the poles.
607
00:35:24,640 --> 00:35:28,200
We see that if you're at the
equator, it's warmer, it's stormier.
608
00:35:28,280 --> 00:35:31,960
If you're at the poles, where the
sun is slightly harder to see,
609
00:35:32,040 --> 00:35:34,480
that activity goes away.
610
00:35:34,560 --> 00:35:38,520
But the weather on Jupiter couldn't
be more different.
611
00:35:38,600 --> 00:35:40,760
We see lightning and convective
thunderstorms
612
00:35:40,840 --> 00:35:43,080
at the poles of Jupiter
but not at the equator.
613
00:35:43,160 --> 00:35:45,840
That's sort of the opposite of what
we see on the Earth.
614
00:35:45,920 --> 00:35:48,680
Question is, what's driving
Jupiter's storms?
615
00:35:50,880 --> 00:35:54,680
Jupiter is five times further from
the sun than the Earth
616
00:35:54,760 --> 00:35:57,960
and receives only a fraction of the
sun's energy.
617
00:35:58,040 --> 00:36:01,160
And unlike Earth,
Jupiter's polar regions
618
00:36:01,240 --> 00:36:03,640
seem to be where the action is.
619
00:36:03,720 --> 00:36:07,200
Something is driving the planet's
weird weather
620
00:36:07,280 --> 00:36:11,240
and Juno's scans of the giant
planet's thermo emissions
621
00:36:11,320 --> 00:36:14,400
suggest it could be Jupiter itself.
622
00:36:14,480 --> 00:36:19,000
You can actually see the internal
heat of Jupiter coming right up
through.
623
00:36:19,080 --> 00:36:23,360
And so, Jupiter will look very
bright in areas where we can see
that heat.
624
00:36:24,680 --> 00:36:29,720
Juno detects searing heat beneath
Jupiter's cloud bands.
625
00:36:29,800 --> 00:36:31,800
Jupiter has so much material.
626
00:36:31,880 --> 00:36:34,440
So much mass, so much gravity
that the interior
627
00:36:34,520 --> 00:36:37,160
is incredibly dense and
very, very hot.
628
00:36:37,240 --> 00:36:40,160
At the core it's probably many
thousands of degrees hotter
629
00:36:40,240 --> 00:36:42,240
than the surface of the sun.
630
00:36:43,280 --> 00:36:46,760
This fiery inferno buried in
Jupiter's dark heart
631
00:36:46,840 --> 00:36:48,880
is a relic from its birth,
632
00:36:48,960 --> 00:36:50,960
billions of years ago.
633
00:36:51,040 --> 00:36:53,760
The violent collisions
that formed the planet
634
00:36:53,840 --> 00:36:56,320
leave its core seething hot,
635
00:36:56,400 --> 00:36:58,720
a heat that remains to this day,
636
00:36:58,800 --> 00:37:02,760
buried under thousands of miles of
insulating gas.
637
00:37:02,840 --> 00:37:05,480
As the heat slowly leaks outwards,
638
00:37:05,560 --> 00:37:08,040
Jupiter's fast rotating atmosphere
639
00:37:08,120 --> 00:37:12,920
gets churned up into vicious cyclones
and thunderstorms.
640
00:37:13,000 --> 00:37:15,480
That's what's really driving most of
the weather.
641
00:37:15,560 --> 00:37:17,840
It's not the sun,
it's Jupiter itself.
642
00:37:19,840 --> 00:37:22,560
And as Juno soars above the planet,
643
00:37:22,640 --> 00:37:25,200
it reveals another weather mystery.
644
00:37:25,280 --> 00:37:28,320
The craft detects bursts of
radio waves,
645
00:37:28,400 --> 00:37:31,720
spiking up to four times a second,
646
00:37:31,800 --> 00:37:35,920
a tell-tale sign of ferocious
lightning strikes.
647
00:37:38,440 --> 00:37:41,760
Clouds are moving around
in the atmosphere, building up
electric charge
648
00:37:41,840 --> 00:37:44,120
and causing bolts of lightning
to form.
649
00:37:44,200 --> 00:37:47,800
And we've actually seen this with
the Juno spacecraft.
650
00:37:47,880 --> 00:37:50,200
These are mega-storms,
651
00:37:50,280 --> 00:37:52,520
orders of magnitude bigger than here
on Earth.
652
00:37:56,840 --> 00:38:00,600
And Juno finds that there's more
to these thunderclouds
653
00:38:00,680 --> 00:38:03,120
than just flashes of light,
654
00:38:03,200 --> 00:38:06,440
giant icy hail stones of water
and ammonia,
655
00:38:06,520 --> 00:38:11,520
that chemical which gives Jupiter's
clouds their orange colour.
656
00:38:15,120 --> 00:38:18,080
High up in Jupiter's atmosphere,
the ammonia
657
00:38:18,160 --> 00:38:20,440
is mixing with the water
658
00:38:20,520 --> 00:38:25,280
and it becomes a liquid ball that
starts to collect ice around it
659
00:38:25,360 --> 00:38:27,600
and it will fall like hail does,
660
00:38:27,680 --> 00:38:29,800
deep into Jupiter's atmosphere.
661
00:38:31,280 --> 00:38:33,840
On Earth
hail falls to the ground.
662
00:38:33,920 --> 00:38:36,520
But on Jupiter, there is no ground.
663
00:38:38,160 --> 00:38:41,280
It gets lifted in the atmosphere
because of an updraft
664
00:38:41,360 --> 00:38:43,400
and then more ice
and it builds bigger
665
00:38:43,480 --> 00:38:46,120
and then it falls down and then
it gets carried back up.
666
00:38:46,200 --> 00:38:49,760
So hail's often many layers
being built.
667
00:38:51,720 --> 00:38:55,000
These icy balls grow layer by layer
668
00:38:55,080 --> 00:38:57,440
as they soar up and down the
atmosphere.
669
00:38:57,520 --> 00:39:00,120
If they formed in storms here on
Earth,
670
00:39:00,200 --> 00:39:02,200
they'd cause some serious damage.
671
00:39:03,840 --> 00:39:06,240
So if you were buzzing around
Jupiter
672
00:39:06,320 --> 00:39:09,000
and you were near where
these storms were,
673
00:39:09,080 --> 00:39:12,040
you might get hit by hail coming up
or going down.
674
00:39:13,040 --> 00:39:15,040
This is one of the most
675
00:39:15,120 --> 00:39:19,320
violent energetic atmospheres in the
entire solar system.
676
00:39:21,280 --> 00:39:25,000
Juno is revealing Jupiter's hidden
secrets.
677
00:39:30,600 --> 00:39:34,720
On Earth dazzling auroras
light up the skies
678
00:39:34,800 --> 00:39:37,080
as charged particles from the sun
679
00:39:37,160 --> 00:39:40,040
interact with atoms high in the
atmosphere.
680
00:39:41,320 --> 00:39:43,600
Deep in the outer solar system,
681
00:39:43,680 --> 00:39:45,880
Jupiter's too far from the sun
682
00:39:45,960 --> 00:39:49,000
for strong auroras to form
in this way.
683
00:39:49,080 --> 00:39:52,560
But high above the giant planet's
poles,
684
00:39:52,640 --> 00:39:56,640
Juno spots a seemingly impossible
light show.
685
00:39:58,960 --> 00:40:00,960
The auroras of Jupiter are
686
00:40:01,040 --> 00:40:03,840
tremendously larger than the ones
we find here on Earth.
687
00:40:03,920 --> 00:40:08,200
In fact, the aurora rings at the
poles are bigger than our planet
itself.
688
00:40:08,280 --> 00:40:12,000
Jupiter's auroras emit primarily
ultraviolet and X-ray light.
689
00:40:12,080 --> 00:40:14,480
So you can't see it with the naked
human eye.
690
00:40:14,560 --> 00:40:17,480
But if you could see them and you
were at Jupiter,
691
00:40:17,560 --> 00:40:20,360
that would be an amazing light show.
692
00:40:20,440 --> 00:40:23,160
Because those auroras are strong.
693
00:40:26,000 --> 00:40:28,280
These glowing displays
are evidence of
694
00:40:28,360 --> 00:40:31,480
charged particles slamming into
Jupiter's atmosphere.
695
00:40:33,160 --> 00:40:35,680
But if they're not coming
from the sun...
696
00:40:35,760 --> 00:40:38,160
where are they coming from?
697
00:40:38,240 --> 00:40:40,280
Hunting for an answer
698
00:40:40,360 --> 00:40:43,360
Juno snaps an image of Jupiter's
southern lights
699
00:40:43,440 --> 00:40:46,680
with its ultraviolet imaging
spectrometer.
700
00:40:46,760 --> 00:40:50,440
Inside the aurora
it glimpses something strange.
701
00:40:51,720 --> 00:40:56,200
When Juno studied the lights coming
from the aurora on Jupiter,
702
00:40:56,280 --> 00:40:59,480
it found that they were even
stronger than expected.
703
00:40:59,560 --> 00:41:02,760
And, in fact, when you look at
Jupiter's poles in wavelengths
704
00:41:02,840 --> 00:41:05,600
that our eyes can't see,
for example ultraviolet,
705
00:41:05,680 --> 00:41:07,680
you see a hot spot.
706
00:41:08,800 --> 00:41:11,200
This hot spot marks the point where
707
00:41:11,280 --> 00:41:13,840
huge concentrations of charged
particles
708
00:41:13,920 --> 00:41:15,920
strike Jupiter's atmosphere.
709
00:41:16,000 --> 00:41:18,000
Tracing their trajectory
710
00:41:18,080 --> 00:41:21,920
reveals the culprit of Jupiter's
dazzling light shows,
711
00:41:22,000 --> 00:41:24,840
the volcanoes of Jupiter's powerful
moons.
712
00:41:27,360 --> 00:41:31,880
Jupiter's moon Io has hundreds
of active volcanoes spewing out
materials
713
00:41:31,960 --> 00:41:33,960
way out into space
and many of those get
714
00:41:34,040 --> 00:41:36,840
trapped by the magnetic fired of
Jupiter.
715
00:41:36,920 --> 00:41:38,960
Io's volcanoes
716
00:41:39,040 --> 00:41:41,520
fire out jets of charged particles
717
00:41:41,600 --> 00:41:45,480
which are swept up by the giant
planet's magnetic field.
718
00:41:45,560 --> 00:41:49,360
It's funnelling those particles down
and slamming into specific spots
719
00:41:49,440 --> 00:41:51,920
in Jupiter's atmosphere.
720
00:41:52,000 --> 00:41:54,760
But Io isn't the only moon
responsible for
721
00:41:54,840 --> 00:41:57,360
Jupiter's polar light show.
722
00:41:57,440 --> 00:41:59,680
If we go further out,
Europa,
723
00:41:59,760 --> 00:42:02,400
Ganymede, Callisto,
those are more icy,
724
00:42:02,480 --> 00:42:05,240
don't necessarily have volcanoes.
725
00:42:05,320 --> 00:42:09,160
These icy moons twist up Jupiter's
magnetic field.
726
00:42:10,160 --> 00:42:12,200
Some of these moons have magnetic
fields
727
00:42:12,280 --> 00:42:14,400
that interact with Jupiter's
magnetic field.
728
00:42:14,480 --> 00:42:18,200
And that actually intensifies the
aurora display on Jupiter.
729
00:42:19,680 --> 00:42:22,200
Jupiter's moons work together to
energise
730
00:42:22,280 --> 00:42:25,880
the greatest northern lights in the
solar system.
731
00:42:25,960 --> 00:42:28,320
But in these beautiful displays
732
00:42:28,400 --> 00:42:32,120
is a stark reminder of the danger
Juno faces.
733
00:42:32,200 --> 00:42:35,600
When you look at these pictures of
the aurora on Jupiter and you think,
734
00:42:35,680 --> 00:42:38,440
"That's beautiful. Wouldn't it be
great to see in person?"
735
00:42:38,520 --> 00:42:42,360
The answer is, "No. No, it wouldn't.
Because they would kill you."
736
00:42:42,440 --> 00:42:44,480
What's causing these displays
737
00:42:44,560 --> 00:42:48,560
are subatomic particles accelerated
to tremendously high speeds
738
00:42:48,640 --> 00:42:51,000
by the magnetic fields involved.
739
00:42:52,080 --> 00:42:54,920
The radiation around Jupiter is
lethal.
740
00:42:56,600 --> 00:42:58,600
The lifetime of the Juno mission is
741
00:42:58,680 --> 00:43:02,160
very limited by the extreme
conditions it has to survive in.
742
00:43:02,240 --> 00:43:04,600
We think that in the future
all of the instruments
743
00:43:04,680 --> 00:43:07,120
will be so radiated
they won't really work any more.
744
00:43:09,320 --> 00:43:11,800
When Juno's titanium armour fails,
745
00:43:11,880 --> 00:43:15,840
Jupiter's deadly radiation will
damage the craft beyond repair.
746
00:43:18,120 --> 00:43:20,880
So the team plans to go out
with a bang,
747
00:43:20,960 --> 00:43:24,000
thrusting Juno into Jupiter's
atmosphere
748
00:43:24,080 --> 00:43:26,080
where the craft will be torn apart.
749
00:43:27,640 --> 00:43:30,960
Eventually it will be drawn down
into Jupiter's depths
750
00:43:31,040 --> 00:43:33,080
and become a part of the planet
itself.
751
00:43:34,320 --> 00:43:37,920
Before then, Juno has many more
mysteries to unlock.
752
00:43:39,280 --> 00:43:42,280
We'll answer some questions and
we'll raise some more,
753
00:43:42,360 --> 00:43:45,880
that's what I expect,
and we'll get some fantastic images.
754
00:43:47,520 --> 00:43:50,240
Every single thing has turned out to
be a surprise.
755
00:43:50,320 --> 00:43:53,240
There're so many things that Juno
has opened our eyes to
756
00:43:53,320 --> 00:43:56,400
that I can't imagine having not
sent it.
757
00:43:56,480 --> 00:43:58,480
So we're in for at least a year more
758
00:43:58,560 --> 00:44:01,640
of the most profound surprises about
Jupiter.
759
00:44:01,720 --> 00:44:04,680
What we're learning,
what we're unlocking,
760
00:44:04,760 --> 00:44:08,240
not just about Jupiter,
but the formation of the
solar system
761
00:44:08,320 --> 00:44:11,320
and the potential formation of life
itself here on Earth...
762
00:44:11,680 --> 00:44:12,680
It's mind-blowing.
763
00:44:12,760 --> 00:44:14,760
subtitles by Deluxe
64152
Can't find what you're looking for?
Get subtitles in any language from opensubtitles.com, and translate them here.