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Jupiter...
Our largest planetary neighbor.
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Jupiter is the king of
the planets for a good reason.
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It's the biggest.
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00:00:08,373 --> 00:00:12,373
It dominated the evolution
of the solar system.
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00:00:12,377 --> 00:00:14,907
Jupiter is a violent
world of radiation and storms
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00:00:14,913 --> 00:00:17,381
on an epic scale.
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00:00:17,382 --> 00:00:19,612
The interior of Jupiter
is kind of hard to imagine.
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There may be a
layer inside Jupiter
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00:00:22,821 --> 00:00:25,151
where you get diamond rain.
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00:00:25,156 --> 00:00:29,493
Today, NASA's Juno mission
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is unraveling
Jupiter's deepest secrets.
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00:00:32,730 --> 00:00:34,730
What forces shape
its mysterious storms
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00:00:34,732 --> 00:00:37,901
and cause volcanic eruptions
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that jet lava deep into space?
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Jupiter actually has
more in common with our sun
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than it does with any of
the other planets
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00:00:44,275 --> 00:00:47,544
in the solar system.
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We venture deep inside
the most extreme planet
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in the solar system
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to reveal its inner secrets
and investigate
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if Jupiter could actually
be the sun's secret twin.
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Have you ever dreamed about
traveling out of this world?
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My name is Mike Massimino,
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and I turned that fantasy
into a reality
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when I space-walked to repair
the Hubble space telescope.
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Great job, Mike.
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Now as we expand our knowledge
of our solar system
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from Mercury
to the cosmic unknowns,
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I want to take you
on a personal journey to...
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Captions by vitac...
www.Vitac.Com
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captions paid for by
discovery communications
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welcome to "the planets."
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I'm Mike Massimino.
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Of all the planets
in our solar system,
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Jupiter is hands-down
the biggest and the baddest.
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It's a beast of a world full
of radiation and violent storms.
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It's got so much power,
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it's basically its own
mini-solar system.
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And thanks to the new amazing
high-resolution images
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from NASA's Juno mission,
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more of Jupiter's secrets
are being revealed.
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Jupiter...
The fifth planet from the sun
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and the largest
in the solar system.
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Made almost entirely
of hydrogen and helium,
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Jupiter stretches more than
85,000 miles across.
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It's unfathomably big.
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You know, you can fit
1,000 earths inside.
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Now scientists
have launched a mission
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to study Jupiter
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in more detail than ever before.
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The Juno spacecraft
that launched in 2011
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reached Jupiter's orbit in 2016,
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where it is capturing close-up
images and collecting data.
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And these newest findings
from Juno show a unique
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and extraordinarily
complex world.
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Jupiter has 67 known moons
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and probably a giant
number of ones
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that are not yet known.
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It's like a miniature
solar system all of its own.
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It's a whole environment,
a whole ecosystem.
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The conditions on
and around Jupiter are extreme.
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It doesn't behave like
an ordinary planet.
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Formed at the beginning
of the solar system
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from the same stuff as the sun,
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Jupiter is an enigma.
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Is it hiding a secret history?
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Could Jupiter be
a star in disguise?
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Spread across 50 square miles
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of baking sand
in the scorching Mojave desert,
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these giant telescopes
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listen for radio signals
in outer space.
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NASA's Steve Levin
is on the front line,
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unlocking the secrets
of Jupiter.
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We've known about Jupiter
for thousands of years,
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00:03:53,498 --> 00:03:54,664
and we've studied it
with telescopes
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for hundreds of years.
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In fact, Jupiter was one
of the very first objects
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in the sky that was studied
with telescopes.
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But when we started
using radio telescopes,
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we learned a lot
of surprises about Jupiter.
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These telescopes observe space
by looking at radio waves
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rather than visible light.
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And the radio waves
that come from Jupiter
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aren't what scientists expect
to see from a planet.
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One of the surprises was this
enormous bright radio source
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that turned out to be Jupiter.
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Jupiter gives off
a huge radio signal
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far too bright for its size.
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Scientists think these signals
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are created by
small, charged particles
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interacting with
a magnetic field.
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Most planets have
a magnetic field,
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but Jupiter's is far larger
than any other.
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In fact, the Juno
spacecraft proved
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that Jupiter's magnetic field
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is 10 times stronger
than that of the earth.
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So what is causing
Jupiter's huge magnetic field?
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Scientists believe
the answer might lie
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within alien chemistry
deep within the planet.
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More than 300 million miles
from earth,
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Jupiter is an unimaginably
different world.
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It's a planet that astronomers
call a "gas giant."
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It's made almost
entirely from hydrogen,
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the same material
that forms stars like the sun.
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But beneath its cloudy surface,
a darkness looms.
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Scientists believe a thick,
black liquid swirls below,
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where intense pressures
and temperatures
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transform hydrogen into
a strange new substance.
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The secret of Jupiter's
giant magnetic field
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may lie within this abyss.
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Scientists in Edinburgh
are conducting
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a remarkable experiment
to find out.
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So, we call Jupiter a gas giant,
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but beneath the clouds
of Jupiter,
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the planet's not really
made of gas.
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It's made of something
much, much stranger.
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Scientists know that Jupiter
is 90% hydrogen.
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Let's go.
Things work fast
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when they work here.
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This equipment
can recreate some of the
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incredibly high pressures
found inside Jupiter,
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to find out
what happens to a gas
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00:06:32,757 --> 00:06:35,926
under the extreme conditions
deep inside the planet.
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In the bottom of the ocean,
the pressure from all the water
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that's on top of you
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is about 1,000 times
earth's atmospheric pressure.
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And in the center of the earth,
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it's about a million times.
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But in the center of Jupiter,
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it's almost a billion times
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the pressure of earth's
atmosphere.
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Stewart is going to expose a gas
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more commonly found on earth
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00:06:56,614 --> 00:06:59,950
to the pressures found
deep within Jupiter.
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He uses oxygen because
it's easier to control
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00:07:02,220 --> 00:07:04,150
in the lab,
yet reacts to pressure
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00:07:04,155 --> 00:07:07,085
in the same way as hydrogen.
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00:07:07,091 --> 00:07:08,591
Oxygen is
very similar to hydrogen,
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00:07:08,593 --> 00:07:11,962
and so, they have
similar properties
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00:07:11,963 --> 00:07:15,932
when you put them under pressure
inside a planet.
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At low pressures, light can
easily pass through the sample.
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If I put my hand
behind the sample,
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the light goes away.
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00:07:22,473 --> 00:07:25,273
So, we're seeing light, now,
coming through oxygen,
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and we're able to see
right through it.
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00:07:27,411 --> 00:07:30,480
And of course, oxygen,
like hydrogen,
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when you squeeze on it,
it starts to change.
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Stewart begins
to squeeze the gas.
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00:07:35,720 --> 00:07:37,920
Under extreme pressures,
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00:07:37,922 --> 00:07:42,692
the structure
of oxygen transforms.
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00:07:42,693 --> 00:07:45,362
- 62, 63.
- There it goes.
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00:07:45,363 --> 00:07:48,999
The oxygen has now
just turned solid,
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and crystals are starting
to form in the system.
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The oxygen becomes opaque.
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It's beginning to change
its structure.
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We're starting to
see, the oxygen's beginning
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to turn a little bit darker
and a little more orange,
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00:08:03,681 --> 00:08:05,849
and there it goes.
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00:08:05,850 --> 00:08:09,350
We've turned, now,
our oxygen sample
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00:08:09,353 --> 00:08:10,853
into a totally black
substance here.
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We were trying to shine
light through it,
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and it's being totally
absorbed inside the oxygen.
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Stewart believes his experiments
prove that the pressure
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within Jupiter
transforms hydrogen gas
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into a new, different state.
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But this isn't enough to explain
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Jupiter's enormous
magnetic field.
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An even stranger force
must be at work.
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Deeper inside the planet,
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the conditions intensify.
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Beneath the dark hydrogen,
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scientists think there's
an even more bizarre layer...
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An ocean of liquid,
metallic hydrogen,
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an exotic state of hydrogen
that doesn't exist on earth.
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12,000 miles deep, this metallic
ocean transforms the planet
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into an enormous dynamo.
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As it spins, it creates
a magnetic field
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that extends nearly
4 million miles around Jupiter,
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the biggest planetary structure
in the solar system.
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Scientists now believe
metallic hydrogen
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powers Jupiter's magnetic field.
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But in the lab,
it's proving difficult to make.
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00:09:30,368 --> 00:09:33,068
The only possible explanation
for that magnetic field
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00:09:33,070 --> 00:09:35,438
is the existence
of a metallic state of hydrogen
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00:09:35,439 --> 00:09:38,375
deep within Jupiter.
And so, it's really...
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Experiments are trying
to catch up to nature.
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The pressure inside Jupiter
is unrivaled
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by the other planets
in our solar system.
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Only the sun creates
a greater force.
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00:09:50,955 --> 00:09:54,555
Jupiter is so big,
so massive that,
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00:09:54,558 --> 00:09:55,988
we know, as you descend
into the interior of Jupiter,
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00:09:55,993 --> 00:09:58,393
you will reach pressures
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00:09:58,396 --> 00:09:59,826
where an element like hydrogen
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00:09:59,830 --> 00:10:03,330
doesn't just liquify.
195
00:10:03,334 --> 00:10:06,302
It actually begins to behave
like a metal.
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00:10:06,303 --> 00:10:09,033
Now, the reason
a metal is shiny is that,
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00:10:09,039 --> 00:10:11,469
metal atoms
actually share electrons.
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00:10:11,475 --> 00:10:12,775
And with the hydrogen
compressed so close together,
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00:10:12,777 --> 00:10:14,777
the same thing happens,
200
00:10:14,779 --> 00:10:17,079
and you get metallic hydrogen.
201
00:10:17,081 --> 00:10:18,748
This metallic hydrogen
is something
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00:10:18,749 --> 00:10:21,649
that is very difficult to make.
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00:10:21,652 --> 00:10:24,952
But because Jupiter
is so powerful, it's so cool,
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00:10:24,955 --> 00:10:28,691
and it has such awesome gravity,
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00:10:28,692 --> 00:10:32,962
it can create metallic hydrogen.
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00:10:36,333 --> 00:10:40,033
Jupiter's magnetic field
reaches out deep into space.
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00:10:40,037 --> 00:10:41,767
When tiny charged particles
come into contact with it,
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00:10:41,772 --> 00:10:45,208
they produce radio waves
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00:10:45,209 --> 00:10:48,509
that telescopes
can detect on earth.
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00:10:48,512 --> 00:10:50,480
Scientists observing Jupiter
in ultraviolet light
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00:10:50,481 --> 00:10:53,611
can see
an extraordinary phenomena
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00:10:53,617 --> 00:10:56,017
caused by the magnetic field...
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00:10:56,020 --> 00:10:58,750
Huge auroras,
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00:10:58,756 --> 00:11:00,186
the brightest and biggest
in the solar system.
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00:11:00,191 --> 00:11:01,658
The auroras here on earth,
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00:11:01,659 --> 00:11:04,089
our northern
and Southern lights,
217
00:11:04,094 --> 00:11:05,994
are caused by the interaction
of our magnetic field
218
00:11:05,996 --> 00:11:08,565
with particles from the sun.
219
00:11:08,566 --> 00:11:10,996
Well, Jupiter's magnetic field
is so extreme,
220
00:11:11,001 --> 00:11:14,637
it actually generates auroras
all by itself.
221
00:11:14,638 --> 00:11:18,408
But the unparalleled
brightness of Jupiter's auroras
222
00:11:18,409 --> 00:11:22,549
can't be explained
by its magnetic field alone.
223
00:11:28,157 --> 00:11:30,487
What awesome power
is fueling Jupiter's auroras?
224
00:11:30,493 --> 00:11:31,893
When I first travelled to
the Hubble space telescope
225
00:11:31,894 --> 00:11:35,530
as an astronaut,
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00:11:35,531 --> 00:11:38,800
I was mesmerized by how bright
the colors in space were.
227
00:11:38,801 --> 00:11:41,801
The sun's light was the
whitest white I had ever seen.
228
00:11:41,804 --> 00:11:43,572
I can only imagine how bright
the massive auroras around
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00:11:43,573 --> 00:11:46,942
Jupiter look from space.
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00:11:46,943 --> 00:11:50,613
But what's causing this majestic
light show around Jupiter?
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00:11:52,815 --> 00:11:55,183
NASA's Juno spacecraft
is on the mission to find out.
232
00:11:55,184 --> 00:11:58,120
Jupiter behaves more like a star
233
00:11:58,121 --> 00:12:02,557
than an ordinary planet,
like earth.
234
00:12:02,558 --> 00:12:05,427
It's made from the same stuff
as the sun,
235
00:12:05,428 --> 00:12:10,598
and supercharged auroras suggest
236
00:12:10,600 --> 00:12:15,100
that extremely powerful
radiation surrounds Jupiter.
237
00:12:15,104 --> 00:12:17,234
This makes getting near
to the planet very difficult.
238
00:12:17,240 --> 00:12:18,707
Trying to get
anywhere close to Jupiter
239
00:12:18,708 --> 00:12:21,338
is really, really hard
240
00:12:21,344 --> 00:12:22,874
because of the intense radiation
of the magnetic field.
241
00:12:22,879 --> 00:12:25,409
So, when you send a spacecraft,
242
00:12:25,415 --> 00:12:27,783
you understand it's not gonna
live for very long.
243
00:12:27,784 --> 00:12:31,784
We've not been to Jupiter
that many times,
244
00:12:33,156 --> 00:12:35,386
which is one reason NASA's
Juno mission is so exciting.
245
00:12:35,391 --> 00:12:38,221
The Juno spacecraft
has been sent
246
00:12:38,227 --> 00:12:40,627
right into the heart
of Jupiter's auroras
247
00:12:40,630 --> 00:12:42,097
to discover the secrets
behind the radiation
248
00:12:42,098 --> 00:12:44,298
that causes them.
249
00:12:44,300 --> 00:12:48,537
Launched in 2011,
250
00:12:48,538 --> 00:12:51,468
Juno traveled at more than
124,000 miles per hour,
251
00:12:51,474 --> 00:12:53,674
to reach Jupiter in 2016.
252
00:12:53,676 --> 00:12:57,946
It's currently
orbiting the planet,
253
00:12:57,947 --> 00:13:01,516
and will circle it 37 times
during its mission.
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00:13:01,517 --> 00:13:03,985
While in orbit, Juno is sending
back images of Jupiter
255
00:13:03,986 --> 00:13:08,023
like we've never seen before.
256
00:13:08,024 --> 00:13:12,194
This first-ever infrared image
of Jupiter's Southern lights
257
00:13:12,195 --> 00:13:16,731
shows off its
incredible auroras.
258
00:13:16,732 --> 00:13:19,568
This is NASA's jet propulsion
laboratory in California.
259
00:13:19,569 --> 00:13:21,036
It's the nerve center
for the Juno mission.
260
00:13:21,037 --> 00:13:23,637
The data's looking amazing.
261
00:13:23,639 --> 00:13:26,308
All the scientists
are incredibly excited.
262
00:13:26,309 --> 00:13:29,109
Heidi Becker is studying
the radiation environment
263
00:13:29,111 --> 00:13:30,911
around Jupiter using Juno.
264
00:13:30,913 --> 00:13:33,181
When Juno went through
the really nasty
265
00:13:33,182 --> 00:13:38,482
radiation environment
for the first time,
266
00:13:38,488 --> 00:13:41,988
it's kind of an
edge-of-your-seat-type moment.
267
00:13:41,991 --> 00:13:44,159
Heidi measures the strength
of radiation around Jupiter
268
00:13:44,160 --> 00:13:47,429
by looking at
photographs of stars
269
00:13:47,430 --> 00:13:49,660
taken by the Juno spacecraft.
270
00:13:49,665 --> 00:13:51,365
This is a regular,
271
00:13:51,367 --> 00:13:55,067
radiation-free image
272
00:13:55,071 --> 00:13:57,939
collected by Juno's
star tracker.
273
00:13:57,940 --> 00:14:01,376
The stars appear
like points of light,
274
00:14:01,377 --> 00:14:04,746
like you're used to when you
look up at the stars at night.
275
00:14:04,747 --> 00:14:07,347
The stars are constant points
of light in the photograph,
276
00:14:07,350 --> 00:14:10,480
but when radiation particles
hit the camera,
277
00:14:10,486 --> 00:14:12,216
they appear, suddenly,
as additional white spots
278
00:14:12,221 --> 00:14:15,991
and streaks of light.
279
00:14:15,992 --> 00:14:17,792
So, each of these frames
is another level of radiation.
280
00:14:17,793 --> 00:14:19,893
And all of these
squiggles and holes
281
00:14:19,896 --> 00:14:22,296
that are being added
to this star field,
282
00:14:22,298 --> 00:14:24,165
that's the radiation signature.
283
00:14:24,166 --> 00:14:26,935
These are
the radiation particles
284
00:14:26,936 --> 00:14:30,036
that create Jupiter's auroras.
285
00:14:30,039 --> 00:14:32,207
The particles are kind of like
machine-gun fire,
286
00:14:32,208 --> 00:14:34,976
creating bullet holes
in an image.
287
00:14:34,977 --> 00:14:36,677
And so, we can count
those individual bullet holes,
288
00:14:36,679 --> 00:14:38,146
and that's what
helps me understand
289
00:14:38,147 --> 00:14:43,447
the radiation environment.
290
00:14:43,452 --> 00:14:46,388
So, one person's noise is
another person's music or data.
291
00:14:46,389 --> 00:14:48,419
This data from Juno
allows scientists
292
00:14:48,424 --> 00:14:51,393
to map the planet's radiation.
293
00:14:51,394 --> 00:14:54,794
The radiation fields
of Jupiter are so intense,
294
00:14:54,797 --> 00:14:57,766
we know they're going to
eventually fry our spacecraft.
295
00:14:57,767 --> 00:15:00,997
Juno has on the order
of about a 2-year lifetime.
296
00:15:01,003 --> 00:15:05,203
We understand that.
297
00:15:05,207 --> 00:15:07,075
This intense radiation
lights up Jupiter's auroras,
298
00:15:07,076 --> 00:15:12,576
but where does it come from?
299
00:15:12,582 --> 00:15:16,051
What's feeding Jupiter's
magnetic field with radiation?
300
00:15:16,052 --> 00:15:18,682
Scientists looking for evidence
have spotted clues
301
00:15:18,688 --> 00:15:21,218
in a mysterious bright spot
302
00:15:24,093 --> 00:15:25,523
tracing a path
across the lights.
303
00:15:25,528 --> 00:15:28,258
They now think that lo,
304
00:15:28,264 --> 00:15:31,600
one of the 67 moons
that orbit Jupiter,
305
00:15:31,601 --> 00:15:34,069
holds the key
to the planet's auroras.
306
00:15:34,070 --> 00:15:35,800
There's this very intense
magnetic interaction
307
00:15:35,805 --> 00:15:38,035
between Jupiter and its moons,
308
00:15:38,040 --> 00:15:41,240
and you can actually see this
in the Aurora.
309
00:15:41,243 --> 00:15:42,643
And you see a glowing spot
moving around in the auroras.
310
00:15:42,645 --> 00:15:45,675
And one of the most
dramatic ones,
311
00:15:45,681 --> 00:15:50,151
the most dramatic footprints
to see, is that of lo.
312
00:15:50,152 --> 00:15:53,752
Io orbits
at 217,000 miles from Jupiter,
313
00:15:53,756 --> 00:15:57,125
held in place by the planet's
massive gravity.
314
00:15:57,126 --> 00:15:59,856
It's nothing like the moon
that orbits earth.
315
00:15:59,862 --> 00:16:02,530
When we sent
our first spacecraft,
316
00:16:02,531 --> 00:16:04,461
we saw, amazingly,
317
00:16:04,467 --> 00:16:06,597
volcanoes going off.
318
00:16:06,602 --> 00:16:11,372
Could these remote volcanoes
319
00:16:15,811 --> 00:16:19,011
be the source of Jupiter's
supercharged auroras?
320
00:16:19,014 --> 00:16:21,944
On my second mission
on space shuttle Atlantis,
321
00:16:21,950 --> 00:16:23,950
we brought a replica
of Galileo's telescope
322
00:16:23,952 --> 00:16:28,122
just like the one
that he used to discover
323
00:16:28,123 --> 00:16:30,323
Jupiter's four largest moons,
including lo.
324
00:16:30,325 --> 00:16:33,094
In Galileo's wildest dreams,
325
00:16:33,095 --> 00:16:35,425
he probably never would've
theorized that volcanoes
326
00:16:35,430 --> 00:16:37,430
on lo would be playing a role in
327
00:16:37,432 --> 00:16:39,600
Jupiter's stunning auroras.
328
00:16:39,601 --> 00:16:41,371
But that's just what
some scientists
329
00:16:43,038 --> 00:16:46,138
are on the hunt to prove.
330
00:16:46,141 --> 00:16:49,009
Scientists at
Syracuse university in New York
331
00:16:49,010 --> 00:16:52,010
are investigating
if volcanoes on lo
332
00:16:52,013 --> 00:16:54,243
are the cause of
Jupiter's magnificent auroras
333
00:16:54,249 --> 00:16:56,517
by making their own volcano.
334
00:16:56,518 --> 00:16:59,148
I've poured lava
over 1,000 times,
335
00:16:59,154 --> 00:17:01,454
and probably have seen more lava
336
00:17:01,456 --> 00:17:05,456
than a lot of volcanologists.
337
00:17:05,460 --> 00:17:08,290
Professor Bob Wysocki
runs the lava project.
338
00:17:08,296 --> 00:17:11,832
He uses his homemade
furnace to replicate
339
00:17:11,833 --> 00:17:14,263
the geological conditions
on other worlds.
340
00:17:14,269 --> 00:17:17,669
Tonight, he's gearing up
to investigate
341
00:17:17,672 --> 00:17:20,508
how volcanic activity on one
of Jupiter's moons
342
00:17:20,509 --> 00:17:23,239
might fuel the planet's
deadly radiation
343
00:17:23,245 --> 00:17:26,445
and light up its auroras.
344
00:17:26,448 --> 00:17:30,684
Bob heats basalt rock
until it melts.
345
00:17:30,685 --> 00:17:32,785
The furnace burns
at 2,300 degrees Fahrenheit.
346
00:17:32,787 --> 00:17:35,317
It takes an immense amount
of energy
347
00:17:35,323 --> 00:17:37,923
to melt even a small amount
of rock.
348
00:17:37,926 --> 00:17:40,256
So, where does lo get the energy
349
00:17:40,262 --> 00:17:44,832
to fuel its volcanoes?
350
00:17:44,833 --> 00:17:46,133
All signs point to lo's immense
immense and malevolent neighbor,
351
00:17:46,134 --> 00:17:49,970
Jupiter.
352
00:17:49,971 --> 00:17:52,301
The planet traps lo
in a gravitational tug-of-war
353
00:17:52,307 --> 00:17:56,076
with other orbiting moons.
354
00:17:56,077 --> 00:17:59,677
Inside lo, the relentless push
and pull from Jupiter
355
00:17:59,681 --> 00:18:03,251
heats up the interior
to melting point,
356
00:18:05,420 --> 00:18:06,750
creating smoldering currents
beneath the surface.
357
00:18:06,755 --> 00:18:10,325
As the pressure builds,
358
00:18:12,827 --> 00:18:15,327
the lava finally erupts
through the moon's crust.
359
00:18:15,330 --> 00:18:18,199
It shoots scorching
fountains of lava
360
00:18:18,200 --> 00:18:21,700
up to half-a-mile high
361
00:18:25,373 --> 00:18:27,741
and floods the frozen surface
with molten rock.
362
00:18:27,742 --> 00:18:31,212
- Okay, Jeff, you ready to go?
- Yeah.
363
00:18:31,213 --> 00:18:33,213
In Syracuse, Bob is ready
to pour the lava.
364
00:18:33,215 --> 00:18:35,945
We are just that one step below
365
00:18:35,951 --> 00:18:40,187
what comes out of a volcano
366
00:18:40,188 --> 00:18:41,988
and making and replicating
what happens in nature.
367
00:18:41,990 --> 00:18:43,620
Well, we're doing
an experiment today
368
00:18:43,625 --> 00:18:46,725
to try to better understand
369
00:18:46,728 --> 00:18:49,728
what happens
when ice meets lava.
370
00:18:49,731 --> 00:18:54,201
Geologist Jeff Karson
is joining Bob
371
00:18:54,202 --> 00:18:56,870
to see what happens
when volcanoes erupt on lo.
372
00:18:56,871 --> 00:19:02,409
Io is extremely cold.
373
00:19:02,410 --> 00:19:05,140
Its surface is made from sulfur
dioxide that is frozen solid.
374
00:19:05,146 --> 00:19:09,146
Bob monitors the furnace,
while Jeff examines
375
00:19:09,150 --> 00:19:12,219
how lava interacts with the ice.
376
00:19:12,220 --> 00:19:15,289
The physics that govern
the way the lava flows form,
377
00:19:15,290 --> 00:19:18,020
the way they cool,
the shapes they take on,
378
00:19:18,026 --> 00:19:21,695
these are all the same
on other planetary objects,
379
00:19:21,696 --> 00:19:23,996
but the same basic
physics applies.
380
00:19:23,999 --> 00:19:26,229
Scientists believe
that the hot lava
381
00:19:26,234 --> 00:19:27,901
pouring out of lo's volcanoes
382
00:19:27,902 --> 00:19:31,072
onto its icy surface
383
00:19:33,575 --> 00:19:35,975
has a direct effect
on Jupiter's radiation.
384
00:19:35,977 --> 00:19:37,444
Moving onto the ice,
385
00:19:37,445 --> 00:19:39,775
a bunch of bubbles
are starting to form.
386
00:19:39,781 --> 00:19:42,349
You see a completely
different style
387
00:19:42,350 --> 00:19:43,550
of behavior of the lava here.
388
00:19:43,551 --> 00:19:47,151
I'm gonna step back, actually,
389
00:19:47,155 --> 00:19:48,585
'cause I can feel the heat
so intensely here.
390
00:19:48,590 --> 00:19:51,358
But those bubbles are forming
391
00:19:51,359 --> 00:19:53,389
because water vapor
is being produced,
392
00:19:53,395 --> 00:19:55,325
boiling the water in the ice.
393
00:19:55,330 --> 00:19:58,830
The vapor is escaping
through the lava
394
00:19:58,833 --> 00:20:00,233
and blowing these
beautiful bubbles.
395
00:20:00,235 --> 00:20:02,765
It's a really good analog
396
00:20:02,771 --> 00:20:05,839
for what could be happening
on other planetary objects,
397
00:20:05,840 --> 00:20:08,440
like on lo.
398
00:20:08,443 --> 00:20:12,313
The hot lava
causes the frozen ice
399
00:20:12,314 --> 00:20:13,714
to instantly vaporize
into clouds of steam.
400
00:20:13,715 --> 00:20:17,051
On a place like lo,
401
00:20:17,052 --> 00:20:19,482
it would be sulfur
that's being vaporized,
402
00:20:19,487 --> 00:20:22,387
and sulfur dioxide
making bubbles
403
00:20:22,390 --> 00:20:26,560
and being released
into the atmosphere.
404
00:20:26,561 --> 00:20:27,728
Scientists now think
that vaporized sulfur dioxide
405
00:20:27,729 --> 00:20:32,566
is the key ingredient
406
00:20:32,567 --> 00:20:36,967
to explain Jupiter's
extraordinary auroras.
407
00:20:36,971 --> 00:20:42,209
Io's volcanoes vaporize
the toxic sulfur dioxide.
408
00:20:42,210 --> 00:20:47,047
They blast it into
a nearly 50-mile umbrella plume.
409
00:20:47,048 --> 00:20:49,416
One ton every second flies
into orbit around Jupiter.
410
00:20:49,417 --> 00:20:52,217
The sulfur dioxide supercharges
411
00:20:52,220 --> 00:20:54,820
the deadly radiation belt
around the planet
412
00:20:54,823 --> 00:20:57,453
with a lethal particle storm.
413
00:20:57,459 --> 00:20:59,389
Jupiter's magnetic field
then captures
414
00:20:59,394 --> 00:21:01,894
the sulfur dioxide particles
415
00:21:01,896 --> 00:21:04,996
and accelerates them
to the poles of the planet
416
00:21:04,999 --> 00:21:07,067
at almost the speed of light.
417
00:21:07,068 --> 00:21:10,738
They strike Jupiter's atmosphere
418
00:21:10,739 --> 00:21:13,439
and create the spectacular
Aurora patterns,
419
00:21:13,441 --> 00:21:16,410
over 100 times more energetic
420
00:21:16,411 --> 00:21:18,911
than the northern lights
on earth.
421
00:21:18,913 --> 00:21:22,013
And now, thanks to Juno imagery,
422
00:21:22,016 --> 00:21:26,253
scientists have confirmed
that lo's volcanoes
423
00:21:26,254 --> 00:21:28,384
are indeed contributing
to this massive light show.
424
00:21:28,390 --> 00:21:33,660
These eruptions
on Jupiter's moon
425
00:21:33,661 --> 00:21:37,561
help generate a lethal radiation
engulfing the whole planet.
426
00:21:37,565 --> 00:21:41,535
But it's not just radiation
that makes Jupiter so extreme.
427
00:21:41,536 --> 00:21:43,904
Deadly storms rage
on the surface.
428
00:21:43,905 --> 00:21:46,373
Today, Juno is sending
back photos
429
00:21:46,374 --> 00:21:49,174
of unimaginable weather systems,
430
00:21:49,177 --> 00:21:53,113
enormously more powerful
than even the most
431
00:21:53,114 --> 00:21:56,014
terrifying hurricanes on earth.
432
00:21:56,017 --> 00:21:58,185
The weather on
Jupiter is pretty darn extreme.
433
00:21:58,186 --> 00:22:00,116
There are these belts
that have winds
434
00:22:00,121 --> 00:22:02,221
that are zooming around
very quickly,
435
00:22:02,223 --> 00:22:04,023
and then in one direction in one
436
00:22:04,025 --> 00:22:06,193
and then the other direction
in the other.
437
00:22:06,194 --> 00:22:07,794
Among all the swirling bands,
438
00:22:07,796 --> 00:22:10,796
there's an enigma,
439
00:22:10,799 --> 00:22:14,769
one feature that
doesn't seem to change...
440
00:22:20,471 --> 00:22:23,640
Jupiter's famous great red spot.
441
00:22:23,641 --> 00:22:26,071
When I space-walked
for the first time in 2002
442
00:22:26,076 --> 00:22:28,506
to help repair
the Hubble space telescope,
443
00:22:28,512 --> 00:22:30,342
I just couldn't believe
how incredible the earth
444
00:22:30,347 --> 00:22:33,647
looked from outer space.
445
00:22:33,651 --> 00:22:36,481
One of the coolest sights
were the lightning storms.
446
00:22:36,487 --> 00:22:38,955
But the storms on earth
are nothing compared to
447
00:22:38,956 --> 00:22:42,156
the ferocious ones on Jupiter.
448
00:22:42,159 --> 00:22:44,089
And as scientists find out more
about these storms,
449
00:22:44,094 --> 00:22:48,264
they're unlocking the secrets
450
00:22:48,265 --> 00:22:53,265
to the planet's
mysterious red spot.
451
00:22:53,270 --> 00:22:55,438
Jupiter... more than 1,000 times
larger than the earth.
452
00:22:55,439 --> 00:22:57,839
It's the biggest
and baddest planet
453
00:22:57,841 --> 00:23:00,641
in the solar system.
454
00:23:00,644 --> 00:23:04,580
It's so deadly, it seems
to have more in common
455
00:23:04,581 --> 00:23:06,881
with the sun
than a planet like earth.
456
00:23:06,884 --> 00:23:09,384
Jupiter has single storms
457
00:23:09,386 --> 00:23:11,716
that are larger
than its neighboring planets.
458
00:23:11,722 --> 00:23:14,290
They rage for centuries
and create
459
00:23:14,291 --> 00:23:16,091
its unmistakable appearance.
460
00:23:16,093 --> 00:23:18,093
If you were to go to Jupiter,
you'd be in for
461
00:23:18,095 --> 00:23:20,225
some very serious weather.
462
00:23:20,230 --> 00:23:22,660
But, hey, maybe the kitesurfing
would be good,
463
00:23:22,666 --> 00:23:26,302
or the parachuting,
because you have to deal with
464
00:23:26,303 --> 00:23:31,773
some serious winds
and some serious storms.
465
00:23:31,775 --> 00:23:35,645
In 2017, the Juno mission sent
back photos of Jupiter's poles,
466
00:23:35,646 --> 00:23:38,046
which were covered
in dense, massive storms.
467
00:23:38,048 --> 00:23:40,616
The Southern pole
boasts cyclones
468
00:23:40,617 --> 00:23:43,786
that are 600 miles in diameter,
469
00:23:43,787 --> 00:23:46,187
the size of Texas.
470
00:23:46,190 --> 00:23:50,827
And close to Jupiter's
northern pole,
471
00:23:50,828 --> 00:23:53,896
this anti-cyclonic storm
is 3,700 miles long,
472
00:23:53,897 --> 00:23:56,065
bigger than the entire U.S.
473
00:23:56,066 --> 00:23:58,696
But even this storm
doesn't compare
474
00:23:58,702 --> 00:24:00,202
to Jupiter's great red spot.
475
00:24:00,204 --> 00:24:03,034
The great red spot
476
00:24:03,040 --> 00:24:06,109
is this gigantic swirling storm
477
00:24:06,110 --> 00:24:08,810
that has lasted
for hundreds of years.
478
00:24:08,812 --> 00:24:11,481
You know, storms on earth
don't last that long.
479
00:24:11,482 --> 00:24:14,612
Jupiter's great red
spot is one of the biggest
480
00:24:14,618 --> 00:24:17,987
and oldest storms
in the solar system.
481
00:24:17,988 --> 00:24:20,618
The Juno cam captured the
closest-ever photos of the spot
482
00:24:20,624 --> 00:24:25,194
on July 10, 2017,
483
00:24:25,195 --> 00:24:28,795
recording storm clouds moving
at over 350 miles per hour.
484
00:24:30,134 --> 00:24:33,664
But the mystery remains.
What keeps it spinning?
485
00:24:33,670 --> 00:24:38,670
Scientists at UCLA's spinlab
in California
486
00:24:38,675 --> 00:24:41,175
are trying to understand
Jupiter's extreme weather.
487
00:24:41,178 --> 00:24:42,908
It would be impossible for us
to get to Jupiter and survive,
488
00:24:42,913 --> 00:24:45,543
so we have the next best thing.
Here at spinlab,
489
00:24:45,549 --> 00:24:48,017
we do simulations
of Jupiter in the lab.
490
00:24:48,018 --> 00:24:50,418
Juan Lora has a surprising tool
491
00:24:50,420 --> 00:24:52,450
to understand Jupiter's
atmosphere...
492
00:24:52,456 --> 00:24:53,886
A tank of water.
493
00:24:53,891 --> 00:24:56,991
With this setup here,
494
00:24:56,994 --> 00:24:59,024
we are simulating a planetary
atmosphere in the lab.
495
00:24:59,029 --> 00:25:01,529
I know it doesn't look much
like a planet,
496
00:25:01,532 --> 00:25:04,332
but imagine just looking down
at the center of the table,
497
00:25:04,334 --> 00:25:05,764
and that represents the polar
region of the planet.
498
00:25:05,769 --> 00:25:08,599
The table will spin.
499
00:25:08,605 --> 00:25:12,805
So, as you head out
to the edges of the table,
500
00:25:12,810 --> 00:25:15,110
that represents lower latitudes
on the planet.
501
00:25:15,112 --> 00:25:19,081
Jupiter is the fastest
spinning planet
502
00:25:19,082 --> 00:25:23,482
in the solar system.
503
00:25:23,487 --> 00:25:25,587
A day on Jupiter
lasts only 10 hours.
504
00:25:25,589 --> 00:25:27,256
The fluid in the table
is now spinning
505
00:25:27,257 --> 00:25:28,757
like a planetary atmosphere
would be.
506
00:25:28,759 --> 00:25:30,389
So, now, we're gonna
add some dye,
507
00:25:30,394 --> 00:25:33,763
and let's see what happens.
508
00:25:33,764 --> 00:25:35,694
The colored fluids represent
different cloud systems.
509
00:25:35,699 --> 00:25:37,867
This experiment
should reveal clues
510
00:25:37,868 --> 00:25:40,268
about how they interact.
511
00:25:40,270 --> 00:25:42,338
Adding any sort of
turbulence to a rotating fluid
512
00:25:42,339 --> 00:25:46,909
will create some
interesting dynamics.
513
00:25:46,910 --> 00:25:49,278
Juan stirs the water
to create turbulence.
514
00:25:49,279 --> 00:25:51,609
Turbulence occurs
in Jupiter's atmosphere
515
00:25:51,615 --> 00:25:53,315
when gasses of different
temperatures and speeds
516
00:25:53,317 --> 00:25:55,284
come together.
517
00:25:55,285 --> 00:25:57,285
Once you get turbulence,
and you disturb a fluid
518
00:25:57,287 --> 00:26:00,223
that is rotating quickly,
519
00:26:00,224 --> 00:26:02,924
like this tank and like Jupiter,
then you get these vortices.
520
00:26:02,926 --> 00:26:06,426
And the vortices
are very stable,
521
00:26:06,430 --> 00:26:08,830
and they like to interact
with each other sometimes.
522
00:26:08,832 --> 00:26:10,399
This is like the red spot.
523
00:26:10,400 --> 00:26:12,430
As soon as it was formed,
524
00:26:12,436 --> 00:26:14,303
it is able to be maintained
525
00:26:14,304 --> 00:26:17,704
by the rotation of Jupiter.
526
00:26:17,708 --> 00:26:20,038
Jupiter's rotation
energizes the great red spot
527
00:26:20,043 --> 00:26:23,213
and keeps it spinning.
528
00:26:24,748 --> 00:26:28,885
But how did it get so large
in the first place?
529
00:26:28,886 --> 00:26:34,086
The great red spot
is larger than whole planets.
530
00:26:34,091 --> 00:26:37,731
Winds whip around it at over 400
miles per hour to form a cyclone
531
00:26:39,863 --> 00:26:42,899
that rises nearly 5 miles
above the clouds.
532
00:26:42,900 --> 00:26:46,500
The striking red color
is believed to be the gas
533
00:26:46,503 --> 00:26:49,103
reacting with the sun's rays.
534
00:26:49,106 --> 00:26:53,242
Behind the sunburnt surface,
535
00:26:53,243 --> 00:26:55,511
these twisting clouds
remain gray inside.
536
00:26:55,512 --> 00:26:58,681
As smaller storms approach,
537
00:26:58,682 --> 00:26:59,882
they are ruthlessly cannibalized
by the giant.
538
00:26:59,883 --> 00:27:04,353
Their energy and spin
539
00:27:04,354 --> 00:27:08,324
add to the great red spot's
size and power.
540
00:27:08,325 --> 00:27:13,125
Is this superstorm
destined to rage forever?
541
00:27:13,130 --> 00:27:14,297
Today, scientists can see
something strange is happening.
542
00:27:14,298 --> 00:27:15,498
Jupiter's great red spot
543
00:27:15,499 --> 00:27:18,067
has been changing
over the past 20 years.
544
00:27:18,068 --> 00:27:19,468
So, here, an image taken
in 1995,
545
00:27:19,469 --> 00:27:21,569
where you can see that
the great red spot
546
00:27:21,571 --> 00:27:24,740
is quite large
and oval-shaped.
547
00:27:24,741 --> 00:27:26,809
If you compare this image
to one taken in 2009,
548
00:27:26,810 --> 00:27:28,678
the spot has become
more circular,
549
00:27:28,679 --> 00:27:30,979
and it's also smaller in size.
550
00:27:30,981 --> 00:27:33,211
And then, from 2014,
shows, again,
551
00:27:34,952 --> 00:27:39,488
a further shrinkage of the spot.
552
00:27:39,489 --> 00:27:45,695
These NASA photos show just
how much the spot has changed
553
00:27:45,696 --> 00:27:50,132
from 1994 to
the newest image in 2017.
554
00:27:50,133 --> 00:27:51,463
The great red spot feeds
on other storms to survive.
555
00:27:51,468 --> 00:27:54,236
It consumes them,
556
00:27:54,237 --> 00:27:57,137
absorbing their energy
to keep spinning.
557
00:27:57,140 --> 00:27:59,640
And if it's not fed,
it'll starve.
558
00:27:59,643 --> 00:28:02,043
It's possible that,
in the past 20 years,
559
00:28:02,045 --> 00:28:03,375
fewer of those vortices
have come into contact
560
00:28:03,380 --> 00:28:06,449
with the great red spot.
561
00:28:06,450 --> 00:28:09,780
Scientists also think
that some smaller storms
562
00:28:09,786 --> 00:28:12,786
could actually damage
the great red spot.
563
00:28:12,789 --> 00:28:15,989
Another possibility
is that it's eating,
564
00:28:15,993 --> 00:28:17,259
if you will, vortices that are
spinning more slowly
565
00:28:17,260 --> 00:28:19,330
than it is spinning,
566
00:28:21,198 --> 00:28:25,698
and therefore, there's
a net loss of spin.
567
00:28:25,702 --> 00:28:29,102
Storms that move more slowly or
spin in the opposite direction
568
00:28:30,440 --> 00:28:33,270
could be putting the brakes
on the great red spot.
569
00:28:33,276 --> 00:28:35,244
Its extraordinary longevity
could simply be
570
00:28:35,245 --> 00:28:37,513
an exceptional streak of luck
571
00:28:37,514 --> 00:28:39,782
that's only now running out.
572
00:28:39,783 --> 00:28:41,583
The fact that it's changing,
and so quickly,
573
00:28:41,585 --> 00:28:43,815
and so dramatically,
after being stable
574
00:28:43,820 --> 00:28:46,150
for so long,
does suggest that, maybe,
575
00:28:46,156 --> 00:28:48,786
something is taking place.
576
00:28:48,792 --> 00:28:51,092
Maybe it will shrink
till the point we can't see it.
577
00:28:51,094 --> 00:28:54,330
We don't know.
We have to keep watching.
578
00:28:54,331 --> 00:28:57,600
Only time will tell
if Jupiter's most famous feature
579
00:28:57,601 --> 00:28:59,301
will survive another 100 years.
580
00:28:59,302 --> 00:29:04,240
The extreme physics on Jupiter
581
00:29:04,241 --> 00:29:06,371
creates unparalleled weather
systems visible from space,
582
00:29:06,376 --> 00:29:10,046
and scientists are just
beginning to understand
583
00:29:10,047 --> 00:29:13,647
the conditions inside
the planet's clouds.
584
00:29:13,650 --> 00:29:14,880
What they're finding
is extraordinary.
585
00:29:14,885 --> 00:29:16,585
One of the big surprises
586
00:29:16,586 --> 00:29:20,856
when we got to Jupiter
with a spacecraft,
587
00:29:20,857 --> 00:29:23,357
was to see that there was
lightning on the dark side.
588
00:29:23,360 --> 00:29:28,397
These images
taken by NASA spacecraft
589
00:29:28,398 --> 00:29:31,667
are evidence of lightning
strikes in Jupiter's atmosphere.
590
00:29:31,668 --> 00:29:36,638
They could trigger an
astonishing chemical reaction
591
00:29:36,640 --> 00:29:39,809
deep inside Jupiter's
colorful clouds.
592
00:29:39,810 --> 00:29:44,547
A thick fog of gas
surrounds Jupiter.
593
00:29:44,548 --> 00:29:47,378
Friction in the clouds generates
super bolts of lightning.
594
00:29:47,384 --> 00:29:49,114
These strikes are many times
more powerful
595
00:29:51,888 --> 00:29:55,324
than lightning on earth.
596
00:29:55,325 --> 00:29:59,195
62 miles beneath the surface,
597
00:29:59,196 --> 00:30:02,096
the clouds harbor methane,
as well as hydrogen.
598
00:30:02,099 --> 00:30:03,899
When the superheated
electric shock
599
00:30:03,900 --> 00:30:05,700
rips through the atmosphere,
600
00:30:05,702 --> 00:30:08,402
the conditions are perfect
601
00:30:08,405 --> 00:30:11,435
for an extraordinary
chemical reaction
602
00:30:17,104 --> 00:30:20,973
unlike anything else
in the solar system.
603
00:30:20,974 --> 00:30:24,644
There's no question
that 85,000 miles across,
604
00:30:24,645 --> 00:30:28,145
Jupiter is the king of all
planets in the solar system.
605
00:30:28,148 --> 00:30:32,748
And the amazing forces at play
on this hostile planet
606
00:30:32,753 --> 00:30:34,783
can create millions
of jewels fit for a crown.
607
00:30:34,788 --> 00:30:37,288
Jupiter's
lightning bolts are stronger
608
00:30:37,291 --> 00:30:39,358
than anything
we've witnessed on earth,
609
00:30:39,359 --> 00:30:42,559
and the resulting
chemical reaction
610
00:30:42,563 --> 00:30:46,093
unleashes a shower
of unimaginable riches.
611
00:30:46,099 --> 00:30:48,468
The lightning transforms
the elements into diamonds.
612
00:30:48,469 --> 00:30:50,499
Jupiter keeps its bling
on the inside,
613
00:30:50,504 --> 00:30:52,034
because it may be
raining diamonds.
614
00:30:52,039 --> 00:30:54,769
Now, think about this.
615
00:30:54,775 --> 00:30:57,243
Jupiter has incredibly
strong winds,
616
00:30:57,244 --> 00:31:01,080
and diamonds are really hard.
617
00:31:01,081 --> 00:31:03,349
So, talk about a hail storm.
618
00:31:03,350 --> 00:31:04,850
Scientists at Cardiff university
619
00:31:04,852 --> 00:31:10,322
are trying to understand
620
00:31:10,324 --> 00:31:13,024
how diamonds might be created
out of thin air on Jupiter.
621
00:31:13,026 --> 00:31:16,996
Professor Oliver Williams
simulates Jupiter's
622
00:31:16,997 --> 00:31:20,166
lightning-charged atmosphere
in the lab.
623
00:31:20,167 --> 00:31:21,797
I'm using an airtight chamber
that I've sucked all the air out
624
00:31:21,802 --> 00:31:25,302
to make a vacuum.
625
00:31:25,305 --> 00:31:27,705
I'm flowing in 99% hydrogen
and 1% methane,
626
00:31:27,708 --> 00:31:30,877
and this is like
the atmosphere of Jupiter.
627
00:31:30,878 --> 00:31:34,308
But the experiment
really begins when Oliver adds
628
00:31:34,314 --> 00:31:37,014
the final ingredient...
Lightning.
629
00:31:37,017 --> 00:31:38,347
I'm gonna break this gas down
using high-power microwaves.
630
00:31:38,352 --> 00:31:40,782
This is very like lightning,
631
00:31:40,787 --> 00:31:42,826
where the high electric field
is breaking down the air
632
00:31:44,825 --> 00:31:47,393
and making these
lightning bolts.
633
00:31:47,394 --> 00:31:51,464
Microwaves,
like lightning on Jupiter,
634
00:31:51,465 --> 00:31:55,101
break down hydrogen
and methane gas.
635
00:31:55,102 --> 00:31:57,902
It glows purple
as the atoms break apart.
636
00:31:57,905 --> 00:32:01,105
So, diamond is fundamentally
made out of carbon.
637
00:32:01,108 --> 00:32:04,038
Methane is actually carbon
with four hydrogen atoms,
638
00:32:04,044 --> 00:32:07,680
and we're able to strip
these hydrogen away.
639
00:32:07,681 --> 00:32:11,381
The microwaves release
carbon atoms from methane gas.
640
00:32:11,385 --> 00:32:13,152
The atoms join together
to form a diamond.
641
00:32:13,153 --> 00:32:16,923
Inside this chamber,
642
00:32:16,924 --> 00:32:19,792
a slice of diamond literally
grows out of thin air.
643
00:32:19,793 --> 00:32:21,693
So, what we've done is,
we've broken down these gasses
644
00:32:21,695 --> 00:32:23,695
that you do see
in places like Jupiter.
645
00:32:23,697 --> 00:32:27,066
And from this chemistry,
we've grown a crystalline form
646
00:32:27,067 --> 00:32:30,667
of carbon, which is diamond.
647
00:32:30,671 --> 00:32:33,201
Experiments like this
suggest diamonds form like hail
648
00:32:33,206 --> 00:32:36,106
in Jupiter's lightning storms.
649
00:32:36,109 --> 00:32:38,539
But something even
more extraordinary happens
650
00:32:38,545 --> 00:32:41,581
as they fall.
651
00:32:41,582 --> 00:32:42,882
As the diamonds are zapped
into existence,
652
00:32:42,883 --> 00:32:47,820
they begin to descend
653
00:32:47,821 --> 00:32:50,121
through the atmosphere
as diamond hail stones.
654
00:32:50,123 --> 00:32:53,823
They plummet thousands of miles
655
00:32:53,827 --> 00:32:58,364
through Jupiter's atmosphere,
towards the core,
656
00:32:58,365 --> 00:33:01,901
racing into higher and higher
pressures and temperatures.
657
00:33:01,902 --> 00:33:07,172
When they hit 14,400 degrees,
658
00:33:07,174 --> 00:33:08,404
they melt, creating a shower
of liquid diamond raindrops.
659
00:33:08,408 --> 00:33:12,244
But what comes next
660
00:33:12,245 --> 00:33:14,245
is an even more bizarre
theoretical possibility.
661
00:33:14,247 --> 00:33:17,917
Diamond rain could lead
662
00:33:17,918 --> 00:33:22,188
to a sparkling diamond ocean
far below.
663
00:33:24,157 --> 00:33:26,157
Jupiter's world may be
stranger than science fiction.
664
00:33:28,857 --> 00:33:30,011
The extreme physics on Jupiter
665
00:33:32,092 --> 00:33:33,939
creates weather totally unlike
anything on earth.
666
00:33:34,768 --> 00:33:36,345
The tremendous forces
forge a unique world
667
00:33:38,238 --> 00:33:39,008
in our solar system.
668
00:33:41,508 --> 00:33:43,047
In fact, Jupiter behaves
more like a star
669
00:33:46,108 --> 00:33:53,109
than a mere planet.
670
00:33:56,239 --> 00:33:58,047
Could Jupiter actually be
the sun's secret twin?
671
00:33:59,045 --> 00:34:00,661
Jupiter and earth
are almost nothing alike.
672
00:34:02,418 --> 00:34:04,111
In fact, Jupiter doesn't
share many qualities
673
00:34:06,518 --> 00:34:08,172
with any of the planets
in our solar system.
674
00:34:10,392 --> 00:34:12,431
What if Jupiter wasn't supposed
to be a planet at all?
675
00:34:14,830 --> 00:34:16,292
What if it's really
a star in disguise?
676
00:34:18,230 --> 00:34:20,230
Images captured from NASA's
Juno mission in 2017 show
677
00:34:21,834 --> 00:34:23,219
that Jupiter is a planet
of extremes.
678
00:34:25,237 --> 00:34:27,084
It dwarfs every other planet
in the solar system.
679
00:34:27,441 --> 00:34:28,604
So, was Jupiter meant
to be a star?
680
00:34:28,611 --> 00:34:30,342
Just as the sun is made
primarily of hydrogen,
681
00:34:30,411 --> 00:34:30,950
so is Jupiter.
682
00:34:32,081 --> 00:34:33,197
And so, it looks like a star,
683
00:34:34,411 --> 00:34:35,642
only it's one
that's not burning.
684
00:34:36,346 --> 00:34:37,346
Jupiter is really massive,
685
00:34:38,982 --> 00:34:40,213
and it's held onto its hydrogen.
686
00:34:40,888 --> 00:34:42,658
So, that's kind of unusual
in the solar system,
687
00:34:44,790 --> 00:34:46,175
is to have a planet
made of hydrogen.
688
00:34:46,623 --> 00:34:48,692
Scientists are beginning
to understand how Jupiter formed
689
00:34:48,699 --> 00:34:52,768
by investigating what happened
690
00:34:54,298 --> 00:34:55,298
in the early solar system.
691
00:34:57,743 --> 00:35:00,409
They're hunting for clues
692
00:35:02,709 --> 00:35:04,440
by observing the birth
of other distant stars.
693
00:35:06,711 --> 00:35:07,942
Deep in the deserts
of California
694
00:35:10,885 --> 00:35:12,385
sits the Owens valley
radio observatory.
695
00:35:13,686 --> 00:35:15,686
These dishes make up
the Carma radio telescope array.
696
00:35:18,928 --> 00:35:20,313
This location
is absolutely gorgeous.
697
00:35:22,358 --> 00:35:23,857
Astronomer John Tobin scans
the skies for newborn stars.
698
00:35:23,864 --> 00:35:25,826
Rather than building one
really big radio telescope,
699
00:35:26,135 --> 00:35:27,289
which is very difficult to do,
700
00:35:27,435 --> 00:35:28,666
they built a lot
of small dishes.
701
00:35:29,236 --> 00:35:30,429
Then they linked them together.
702
00:35:30,768 --> 00:35:32,115
And the further apart
you move them,
703
00:35:32,773 --> 00:35:33,927
the higher resolution you get,
704
00:35:35,705 --> 00:35:37,359
which means it acts
like a bigger telescope,
705
00:35:38,881 --> 00:35:39,974
and you can see finer detail.
706
00:35:39,981 --> 00:35:41,174
John is looking for protostars,
707
00:35:41,882 --> 00:35:42,459
brand-new stars
708
00:35:45,521 --> 00:35:46,637
that are only just condensing
709
00:35:48,051 --> 00:35:49,398
from a vast cloud
of gas and debris.
710
00:35:50,787 --> 00:35:51,941
A protostar is a newborn star,
711
00:35:52,593 --> 00:35:54,055
so it's still
in the process of forming
712
00:35:54,163 --> 00:35:55,125
and building up its mass.
713
00:35:56,031 --> 00:35:57,031
And in interstellar space,
714
00:36:00,731 --> 00:36:01,962
there are clouds
of gas and dust,
715
00:36:04,536 --> 00:36:06,190
and at the center,
a protostar will be born.
716
00:36:07,270 --> 00:36:09,347
Jupiter was formed from
the same clouds of hydrogen gas
717
00:36:10,376 --> 00:36:11,415
and dust that formed stars.
718
00:36:13,549 --> 00:36:14,973
Could it have formed
like a protostar?
719
00:36:16,349 --> 00:36:18,388
John is finding evidence
thousands of light-years away
720
00:36:18,752 --> 00:36:20,099
that explains
how star systems form.
721
00:36:20,784 --> 00:36:21,746
This image is showing you
722
00:36:23,589 --> 00:36:24,820
that the black and the contours,
723
00:36:25,661 --> 00:36:27,085
they're the intensity
of the radiation
724
00:36:27,630 --> 00:36:28,991
that we're detecting
from this protostar.
725
00:36:28,998 --> 00:36:30,191
There's not just one protostar,
726
00:36:31,728 --> 00:36:32,767
but there's two protostars.
727
00:36:34,803 --> 00:36:36,573
So, these two peaks
that you see here and here,
728
00:36:38,703 --> 00:36:40,088
those are the two
forming protostars.
729
00:36:42,144 --> 00:36:43,305
It's a solar system
very different from our own.
730
00:36:43,312 --> 00:36:44,851
And my first reaction
to this was, "wow."
731
00:36:46,977 --> 00:36:48,093
I couldn't believe the detail
732
00:36:49,551 --> 00:36:51,051
that we were seeing
towards this object.
733
00:36:52,151 --> 00:36:54,190
Because previously, we knew
there was one thing there,
734
00:36:55,084 --> 00:36:56,313
but then we found out
that there looks like
735
00:36:56,320 --> 00:36:57,818
there's at least two objects
around this protostar.
736
00:36:57,825 --> 00:36:58,902
And so, that was unexpected.
737
00:37:00,396 --> 00:37:02,050
We didn't know that
we were gonna find that,
738
00:37:05,734 --> 00:37:06,965
and so that was
a surprise to us.
739
00:37:09,604 --> 00:37:11,643
Could Jupiter have once stood
toe-to-toe with the sun?
740
00:37:14,205 --> 00:37:16,205
From the outside, each young
star system looks alike,
741
00:37:18,847 --> 00:37:20,709
starting life as a spiraling
disc of dust and gas.
742
00:37:20,716 --> 00:37:22,447
But what evolves inside
can be very different.
743
00:37:22,985 --> 00:37:24,178
Deep in the middle of the disc,
744
00:37:26,585 --> 00:37:28,009
turbulence can cause
the central cloud
745
00:37:29,588 --> 00:37:33,562
to split into two
and collapse into not one,
746
00:37:37,900 --> 00:37:39,247
but two shining stars
in the center.
747
00:37:39,830 --> 00:37:41,600
The stars orbit each other
in a hypnotic dance.
748
00:37:43,772 --> 00:37:44,734
Born from the same cloud,
749
00:37:48,042 --> 00:37:50,779
this solar system
has twin stars.
750
00:37:56,418 --> 00:37:58,457
Any dust and gas left over
will go on to form planets.
751
00:37:58,987 --> 00:38:01,026
In our solar system, the sun
is the only shining star.
752
00:38:03,926 --> 00:38:05,273
But another massive ball
of hydrogen
753
00:38:08,564 --> 00:38:09,911
quietly orbits from afar...
Jupiter.
754
00:38:10,794 --> 00:38:12,948
Could this planet be the sun's
double that didn't ignite?
755
00:38:13,869 --> 00:38:15,254
Scientists believe
that solar systems
756
00:38:16,839 --> 00:38:18,032
with twin suns are very common.
757
00:38:20,639 --> 00:38:22,832
Well, since that first result
using these telescopes here,
758
00:38:24,242 --> 00:38:25,939
we've been carrying out a much
larger survey of protostars,
759
00:38:25,946 --> 00:38:27,641
in order to see just how many
star systems form with two
760
00:38:27,648 --> 00:38:28,533
or three or more stars.
761
00:38:31,649 --> 00:38:33,534
And we're finding that
a surprisingly large number
762
00:38:35,053 --> 00:38:36,746
of star systems form
with more than one star.
763
00:38:37,657 --> 00:38:39,619
John wants to try to
discover the precise conditions
764
00:38:40,396 --> 00:38:41,858
that create these binary
solar systems,
765
00:38:44,833 --> 00:38:46,064
where two stars
orbit each other.
766
00:38:47,533 --> 00:38:49,259
We've been putting together
a compendium of images
767
00:38:49,266 --> 00:38:50,843
of young star systems
in order to find out
768
00:38:52,741 --> 00:38:54,011
which ones are binary
or multiple.
769
00:38:55,271 --> 00:38:56,656
So, this one is
a single-star system.
770
00:38:57,307 --> 00:38:58,307
This one here is a double.
771
00:38:59,982 --> 00:39:01,059
As many as half of all stars
772
00:39:03,419 --> 00:39:04,766
in the universe
have a partner star,
773
00:39:04,987 --> 00:39:06,718
both formed from a single
disc of gas and dust
774
00:39:07,156 --> 00:39:07,849
that breaks apart.
775
00:39:09,856 --> 00:39:11,818
The system we were looking at
is located right here,
776
00:39:11,858 --> 00:39:14,243
where the clouds of gas are kind
of stretched out and extended.
777
00:39:15,197 --> 00:39:16,813
There might be
multiple centers of collapse
778
00:39:18,297 --> 00:39:20,297
that can lead to the formation
of more than one star.
779
00:39:20,769 --> 00:39:22,462
A cloud of gas and dust
that is stretched out
780
00:39:22,869 --> 00:39:24,369
will likely collapse
into multiple stars
781
00:39:24,740 --> 00:39:25,702
very close to each other.
782
00:39:27,640 --> 00:39:28,717
John thinks our solar system
783
00:39:29,973 --> 00:39:31,320
must have formed
in a different way.
784
00:39:32,178 --> 00:39:33,409
So, we think
our own solar system
785
00:39:36,018 --> 00:39:37,711
may have looked something
more like this one,
786
00:39:38,618 --> 00:39:40,580
where you have just one star
surrounded by its disc,
787
00:39:41,990 --> 00:39:43,414
and then the disc itself
is lower mass
788
00:39:44,460 --> 00:39:46,460
and is not going to fragment
into more than one star.
789
00:39:46,790 --> 00:39:48,483
Scientists believe
the type of hydrogen cloud
790
00:39:51,465 --> 00:39:52,735
that gave rise
to our solar system
791
00:39:54,497 --> 00:39:56,113
cut short Jupiter's quest
to become a star.
792
00:40:00,542 --> 00:40:02,389
In its race to grow up,
the sun got a head start,
793
00:40:05,842 --> 00:40:08,073
sucking up 99% of all the matter
in the young solar system.
794
00:40:10,648 --> 00:40:12,418
When it reached
27 million degrees, it ignited.
795
00:40:13,322 --> 00:40:15,361
Meanwhile, the same cloud
was condensing into Jupiter,
796
00:40:16,422 --> 00:40:17,961
rapidly snowballing
to collect two-thirds
797
00:40:18,325 --> 00:40:19,402
of all the matter left over.
798
00:40:21,657 --> 00:40:23,004
But there was not enough
matter left
799
00:40:24,700 --> 00:40:26,200
for Jupiter to get big enough
to ignite,
800
00:40:27,269 --> 00:40:28,193
so it became a gas giant
801
00:40:30,806 --> 00:40:32,399
more than double the mass
of all other planets
802
00:40:32,406 --> 00:40:33,522
in the solar system combined.
803
00:40:36,245 --> 00:40:36,899
No normal planet,
804
00:40:37,412 --> 00:40:38,836
Jupiter is the star's
younger sibling.
805
00:40:39,812 --> 00:40:40,928
It would make sense to think,
806
00:40:43,185 --> 00:40:44,762
"well, where is
the sun's binary partner?"
807
00:40:45,085 --> 00:40:46,662
And immediately,
the mind goes to Jupiter.
808
00:40:47,256 --> 00:40:48,564
If Jupiter
had gathered enough mass
809
00:40:50,726 --> 00:40:51,573
to ignite into a star,
810
00:40:54,026 --> 00:40:55,552
it's unlikely that the earth
would have ever been formed.
811
00:40:55,559 --> 00:40:57,367
The solar system would be
a very different place
812
00:41:01,336 --> 00:41:01,913
with twin suns.
813
00:41:02,936 --> 00:41:04,898
Instead, Jupiter became
the most extraordinary world
814
00:41:05,107 --> 00:41:05,877
in the solar system.
815
00:41:08,337 --> 00:41:09,684
Everything about Jupiter
is extreme.
816
00:41:11,380 --> 00:41:13,111
Its mass is more than
300 times that of earth.
817
00:41:13,310 --> 00:41:15,195
You could fit 1,000 earths
inside this one planet.
818
00:41:15,284 --> 00:41:16,592
It has a magnetic
field so intense,
819
00:41:18,654 --> 00:41:20,039
it would kill you
with the radiation.
820
00:41:22,791 --> 00:41:24,330
Its winds blow
at over 400 miles an hour.
821
00:41:25,121 --> 00:41:26,814
I mean, can you imagine
a more extreme place?
822
00:41:27,757 --> 00:41:28,719
To me, Jupiter is perhaps
823
00:41:30,332 --> 00:41:31,893
the most fascinating object
in our solar system.
824
00:41:31,900 --> 00:41:33,054
It's certainly the most alien.
825
00:41:34,700 --> 00:41:35,393
It is an enormous,
826
00:41:40,342 --> 00:41:41,419
strange ball of swirling gas
827
00:41:43,272 --> 00:41:45,119
surrounded by its own
miniature planetary system.
828
00:41:46,108 --> 00:41:47,916
Formed at the very beginning
of the solar system
829
00:41:50,714 --> 00:41:51,984
from the same material
as the sun,
61844
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