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Support your local PBS station.

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NARRATOR:
Across the solar system,

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spectacular storms are raging.

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JAMES DOTTIN:
What we've learned about
weather on other planets

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has rewritten the rulebook
on what we thought was possible.

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NARRATOR:
From corrosive clouds...

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GEORGE DRANSFIELD:
If you were to go skydiving
through the clouds of Venus,

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there wouldn't be
a lot of you left at the end.

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NARRATOR:
...to global dust storms.

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DAVID GRINSPOON:
On Mars, the whole atmosphere
basically freaks out,

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and the storm grows to the point

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where it engulfs
the entire planet.

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We don't have anything
like that on Earth.

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NARRATOR:
Storms found
in unexpected places...

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DERRICK PITTS:
It's a moon that
looks like this!

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How do you have these features
on the moon of a planet?

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NARRATOR:
...and made
of bizarre materials.

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SHANNON MACKENZIE:
Buckets and buckets of rain

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are falling on the surface,
and yet,

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it's not water
raining out of the atmosphere,

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but liquid methane.

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NARRATOR:
Extra-terrestrial weather

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makes exploration challenging.

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ABIGAIL FRAEMAN:
Seeing the skies get
darker and darker and darker,

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we started to realize that,

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"Oh, this is actually,
this is a really bad one."

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NARRATOR:
But can teach us so much.

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PETER GAO:
It opens up the possibilities
of, "What is weather?"

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NARRATOR:
What drives these exotic storms
raging across the solar system?

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And how do they shape
a planet's destiny?

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"Solar System: Storm Worlds."

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Right now, on "NOVA."

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♪

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NARRATOR:
It's midsummer.

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♪

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A storm is brewing.

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♪

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It unleashes torrents of rain...

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...forming floods that drain
into rushing rivers...

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♪

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...and giant lakes.

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♪

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This is the only world
in our solar system

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where rainstorms
pummel the surface.

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♪

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The only world other than Earth.

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Here, more than 800 million
miles from the sun...

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...orbits the largest
of Saturn's moons.

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In some ways,
Titan is more similar to Earth

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than any other place
in the solar system.

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But upon closer inspection,

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you will find that it's
actually exceptionally alien.

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The surface temperature of Titan

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is around
- 300 degrees Fahrenheit.

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NARRATOR:
Far too cold for liquid water.

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DOTTIN:
What's fascinating is that

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the rain that's falling
out of the sky on Titan

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and filling up the lakes

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is usually found on Earth
as a flammable gas.

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NARRATOR:
Methane.

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Titan is a world shaped
by alien storms,

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and it is not alone.

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MACKENZIE:
It's pretty mind-blowing

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that as we look elsewhere
in the solar system,

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we see these weather patterns

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that look very familiar to us,

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and yet there are
also these wild extremes.

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♪

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DRANSFIELD:
Some of the storms
we're seeing

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are like supersized versions

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of the storms
that we see here on Earth.

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♪

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NARRATOR:
And the more we explore,

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the more weird and wonderful
weather we're finding.

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GRINSPOON:
Pretty much every planet
with weather

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has some oddity to it
that's surprised us.

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NARRATOR:
So what creates the wild
diversity in weather

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across the solar system?

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GAO:
We're so used to dealing with
our specific brand of weather.

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But there's just
so much more out there,

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if you look
at these stormy worlds.

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♪

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♪

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ALEJANDRO SOTO:
When I hear the word
"weather,"

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I get a memory

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of when I was a kid,
standing out in a field...

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♪

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...when the wind would pick up,
the sky would darken a bit,

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and you knew
it was about to rain.

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[wind gusting]

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And yet it would also be
the best.

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NARRATOR:
From towering thunderstorms

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to howling blizzards

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to choking dust storms,

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our atmosphere
is a restless place.

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But what causes all this chaos?

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JEN GUPTA:
Earth, like all the planets,

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is essentially a big ball
floating in space

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being heated by the sun.

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It's pretty simple, really.

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But because of the shape
of a planet,

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its spherical geometry,

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it's actually really hard
to heat the planet evenly.

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For a start,

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there's always a side
of the Earth

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in darkness,
the night side of the planet.

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DOTTIN:
And some parts,

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like the Equator,

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receive more sunlight

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than others, like the poles,

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and that creates
an energy imbalance.

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But because the Earth is
surrounded by this atmosphere,

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this envelope of gas
that's free to move around,

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it can carry the heat from
the hot places to the cold

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in an attempt to equalize
this imbalance.

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LEIGH FLETCHER:
And without that conveyor belt
of energy motion,

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we wouldn't have

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the incredible diversity ofweather

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that we can see around us today.

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♪

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NARRATOR:
Wind, rain, and lightning
are all side effects

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as our atmosphere balances
hot and cold.

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♪

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And what applies here
applies elsewhere, too.

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CLARA SOUSA-SILVA:
In our solar system, wherever
there's an atmosphere,

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there's weather, no matter how
different

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an atmosphere from Earth's.

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FRAEMAN:
Some are thicker,
some are thinner,

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sometimes they're made
of different things.

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And all of these combine

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to give these crazy cool weathersystems

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that are all so different

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across the solar system.

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♪

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NARRATOR:
To see this alien weather
in action

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across our vast solar system,

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we head away
from our shared star...

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♪

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...passing a planet so small
and close to the sun

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that it has no atmosphere,

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to encounter a planet

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smothered by one.

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PITTS:
Venus looks so beautiful
in the evening sky.

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Brilliant, clear, white,

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just stunningly lovely to see,

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yet it's such a horribly nasty
environment.

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NARRATOR:
Looking down from orbit,

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we can't actually see
Venus's surface at all.

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Instead, all we see are endless,
thick, churning clouds

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that completely conceal
the rest of the planet.

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♪

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GRINSPOON:
Historically, we thought,
"Oh, Venus has clouds.

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"They're probably made out
of water.

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It might be sort of nice there."

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[laughing]: But then,

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when we started to actually get
data from spacecraft,

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we discovered,
no, they're not water.

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In fact, they're battery acid.

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♪

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SOUSA-SILVA:
The clouds on Venus are

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made up of extremely
concentrated sulfuric acid,

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one of the most corrosive
substances we know of.

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If you were to go skydiving

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through the clouds of Venus,

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there wouldn't be a lot of you
left at the end.

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NARRATOR:
But if we could
withstand the acid

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and took the plunge down
through Venus's clouds...

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...we'd reach a landscape
that is eerily calm...

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...but with air pressure
more than 90 times greater

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than at Earth's surface.

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GAO:
Even though we don't realize it,

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air has weight.

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It's being pulled down bygravity,

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just like the rest of us.

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And so, on Venus, where the
atmosphere

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is so thick and so massive,

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all that air
is being pulled down,

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and if we're
on the bottom of it,

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then we'll feel
all that pressure.

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SOUSA-SILVA:
If you find yourself
on the surface of Venus,

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you would almost immediately
be crushed.

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But if somehow you survived

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and tried to go for a stroll,
it would be exhausting.

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The atmosphere is so thick,

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it would be like
walking through molasses.

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NARRATOR:
The surface of Venus

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is comparable to the bottom
of Earth's oceans,

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but with a key difference.

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At about 900 degrees Fahrenheit,

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this is the hottest planetary
surface in the solar system.

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And again, Venus's extreme
atmosphere is responsible.

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SOUSA-SILVA:
Carbon dioxide
and other molecules

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are able to absorb
and radiate heat,

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and so, in large enough
quantities,

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they can act like
a planetary blanket

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that traps
that heat in a planet.

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That's what we call
the greenhouse effect.

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NARRATOR:
And Venus's incredibly
dense atmosphere

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is 96.5% carbon dioxide.

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♪

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Even 0.04% CO2 in our atmosphere

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is enough to initiate
a climate crisis

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in our world right now.

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So you can imagine
how bad it is on Venus.

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NARRATOR:
Venus's extreme
greenhouse effect

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means it's even hotter
than Mercury.

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Which is why what
we would find there

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is so extraordinary.

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♪

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What look like
snow-capped mountains

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towering over
the scalding surface.

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For generations,
we could only guess

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at what lay beneath
Venus's clouds.

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But, thanks to radar images

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beamed back by
NASA's Magellan orbiter,

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we now have detailed maps
of the planet's surface.

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So, here we have an image
taken by Magellan,

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and what we're looking at

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is actually Maxwell Montes.

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Maxwell Montes here

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is the highest region on Venus.

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And what you'll notice
is that around this image,

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the surface looks dark.

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But in the center,
where Maxwell Montes is,

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it's much brighter--
it almost looks white.

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We weren't expecting

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to have such
radar-bright regions

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on the highlands,
in the mountaintops of Venus.

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♪

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GUPTA:
When you see those radar images
of Maxwell Montes,

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it's hard not to imagine
snow-capped mountains.

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♪

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NARRATOR:
But given the conditions
on Venus,

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snow as we know it
is impossible.

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♪

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In places, it's so hot,

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the ground actually glows,

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like metal
coming out of a forge.

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GRINSPOON:
On Earth, you can imagine

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waiting till nighttime
to cool off.

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That wouldn't work on Venus.

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There's no relief at night
on Venus from the temperature.

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And in fact, if you go
from the equator to the pole,

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it doesn't get any cooler,
for the same reason--

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that thick atmosphere
is very efficient

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at redistributing the heat.

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NARRATOR:
It is a world where there
is no place for snow to hide.

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00:13:54,523 --> 00:13:56,007
But there's one way
to cool off on Venus,

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and that's to go up a mountain.

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♪

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NARRATOR:
A phenomenon that we here
on Earth can also relate to.

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♪

254
00:14:18,685 --> 00:14:21,170
PORT:
Everyone knows
when you go up a mountain,

255
00:14:21,170 --> 00:14:24,173
you should always pack a jacket.

256
00:14:24,173 --> 00:14:25,968
And the reason for that
is because it's much colder.

257
00:14:25,968 --> 00:14:27,245
But why is it colder?

258
00:14:27,245 --> 00:14:29,765
Well, when you go up a mountain,
there's less air,

259
00:14:29,765 --> 00:14:31,525
and that means
there's less pressure.

260
00:14:31,525 --> 00:14:34,183
♪

261
00:14:34,183 --> 00:14:36,841
NARRATOR:
And as the pressure decreases,

262
00:14:36,841 --> 00:14:39,430
so does the temperature.

263
00:14:41,570 --> 00:14:43,503
PORT:
So, as we go up in elevation,

264
00:14:43,503 --> 00:14:45,056
we cross a threshold

265
00:14:45,056 --> 00:14:47,507
where the temperature
drops low enough

266
00:14:47,507 --> 00:14:51,028
that water can be a solid.

267
00:14:51,028 --> 00:14:54,824
And this is what we call
the snow line.

268
00:14:56,654 --> 00:14:58,759
NARRATOR:
Venus's snow line suggests

269
00:14:58,759 --> 00:15:01,452
something may be freezing
up there.

270
00:15:01,452 --> 00:15:04,213
But even its highest peaks

271
00:15:04,213 --> 00:15:07,837
are far too hot
for that something to be water.

272
00:15:07,837 --> 00:15:10,944
And that points us
to substances

273
00:15:10,944 --> 00:15:15,707
that solidify
at much higher temperatures.

274
00:15:15,707 --> 00:15:17,399
PORT:
So, instead of water,

275
00:15:17,399 --> 00:15:20,505
it actually could be
something like this.

276
00:15:20,505 --> 00:15:22,852
So this is a piece of galena,

277
00:15:22,852 --> 00:15:24,716
also known as a lead sulfide.

278
00:15:24,716 --> 00:15:26,442
On Earth,
it's present as a solid,

279
00:15:26,442 --> 00:15:28,030
as you can see here.

280
00:15:28,030 --> 00:15:29,411
But on Venus,

281
00:15:29,411 --> 00:15:32,690
it may only be a solid
in the highlands.

282
00:15:32,690 --> 00:15:35,072
NARRATOR:
Deep in Venus's lowlands,

283
00:15:35,072 --> 00:15:38,144
like valleys,

284
00:15:38,144 --> 00:15:41,181
it's hot enough for compounds
like lead sulfide

285
00:15:41,181 --> 00:15:44,391
to vaporize,

286
00:15:44,391 --> 00:15:47,498
drift on the wind,

287
00:15:47,498 --> 00:15:49,396
and, as the winds flow up

288
00:15:49,396 --> 00:15:51,571
into the mountains of
Maxwell Montes...

289
00:15:55,678 --> 00:15:59,199
...the temperature drops
just enough for the compounds

290
00:15:59,199 --> 00:16:02,444
to freeze out of the air.

291
00:16:06,068 --> 00:16:10,762
At 820 degrees Fahrenheit,

292
00:16:10,762 --> 00:16:13,834
Venus's atmosphere
may coat its mountaintops

293
00:16:13,834 --> 00:16:15,284
not in snow,

294
00:16:15,284 --> 00:16:19,012
but in a metallic frost.

295
00:16:27,745 --> 00:16:29,540
PORT:
We still don't know for sure

296
00:16:29,540 --> 00:16:32,025
if metal frost can explain
the bright regions

297
00:16:32,025 --> 00:16:34,027
that we're seeing
on the mountaintops.

298
00:16:34,027 --> 00:16:36,236
There's still a lot
that we don't know about Venus,

299
00:16:36,236 --> 00:16:38,273
and that's because
we haven't even sent a lander

300
00:16:38,273 --> 00:16:40,171
to the surface of Venus
since the 1980s.

301
00:16:40,171 --> 00:16:42,035
But it's amazing to think

302
00:16:42,035 --> 00:16:44,037
that something like this
could be condensing

303
00:16:44,037 --> 00:16:46,108
on the mountaintops of Venus.

304
00:16:50,043 --> 00:16:53,322
When we think of the possibility
of metallic frost on Venus,

305
00:16:53,322 --> 00:16:56,774
it sounds crazy, but that's
only crazy for us Earthlings.

306
00:16:56,774 --> 00:16:59,087
If you have
a different atmosphere,

307
00:16:59,087 --> 00:17:03,229
you get different weather,
different phenomena playing out.

308
00:17:03,229 --> 00:17:07,267
♪

309
00:17:09,649 --> 00:17:13,032
NARRATOR:
Leaving this crushing world
behind...

310
00:17:16,414 --> 00:17:18,382
...we head out in search
of an atmosphere

311
00:17:18,382 --> 00:17:23,214
that could almost be
Venus's opposite.

312
00:17:25,734 --> 00:17:29,600
To reach it,
we bypass our own planet.

313
00:17:36,745 --> 00:17:40,128
Passing two potato-shaped moons

314
00:17:40,128 --> 00:17:43,614
orbiting our other
next-door neighbor,

315
00:17:43,614 --> 00:17:46,065
we encounter an atmosphere

316
00:17:46,065 --> 00:17:49,896
more than 10,000 times thinner
than Venus's.

317
00:17:54,659 --> 00:17:57,524
With little in the way
of cloud cover,

318
00:17:57,524 --> 00:18:02,219
we don't need radar to get
a look at the Martian surface.

319
00:18:04,600 --> 00:18:07,224
Yet, images sent back
by our orbiters

320
00:18:07,224 --> 00:18:11,883
suggest rain may have once
fallen here.

321
00:18:14,196 --> 00:18:17,717
These pictures show
that Mars is covered in features

322
00:18:17,717 --> 00:18:22,687
which appear to have been
created by flowing water.

323
00:18:22,687 --> 00:18:24,482
DOTTIN:
With such a thin atmosphere,

324
00:18:24,482 --> 00:18:26,105
it's really difficult

325
00:18:26,105 --> 00:18:28,210
to retain heat, and certainly

326
00:18:28,210 --> 00:18:29,591
not enough heat to have

327
00:18:29,591 --> 00:18:31,110
liquid water on the surface.

328
00:18:32,732 --> 00:18:36,805
NARRATOR:
So if Mars was once home
to lakes and rivers,

329
00:18:36,805 --> 00:18:40,291
it must have had a much thicker
atmosphere in the past.

330
00:18:42,673 --> 00:18:44,295
FRAEMAN:
In the early 2000s,

331
00:18:44,295 --> 00:18:46,539
we'd seen that there were hints

332
00:18:46,539 --> 00:18:47,885
that liquid water had once been

333
00:18:47,885 --> 00:18:48,955
on the Martian surface

334
00:18:48,955 --> 00:18:50,232
from our orbiters,

335
00:18:50,232 --> 00:18:51,785
but we didn't have
definitive proof

336
00:18:51,785 --> 00:18:53,546
from the surface.

337
00:18:53,546 --> 00:18:55,996
So the goal of the Mars
Exploration Rover mission

338
00:18:55,996 --> 00:18:58,137
was to follow the water.

339
00:18:58,137 --> 00:19:02,520
MAN:
T minus five, four, three,

340
00:19:02,520 --> 00:19:05,005
two, main engine start,

341
00:19:05,005 --> 00:19:07,560
zero, and liftoff

342
00:19:07,560 --> 00:19:10,183
of the Delta rocket
with Opportunity,

343
00:19:10,183 --> 00:19:11,840
a chance to explore

344
00:19:11,840 --> 00:19:15,844
and unlock the secrets
of our neighboring planet.

345
00:19:15,844 --> 00:19:18,433
FRAEMAN:
I was 16 years old
when Spirit and Opportunity

346
00:19:18,433 --> 00:19:20,193
launched and landed on Mars.

347
00:19:20,193 --> 00:19:22,920
But I had the
amazing opportunity

348
00:19:22,920 --> 00:19:25,888
through an outreach program
to actually go to be at NASA,

349
00:19:25,888 --> 00:19:27,649
at the Jet Propulsion
Laboratory,

350
00:19:27,649 --> 00:19:28,960
when the rovers landed.

351
00:19:28,960 --> 00:19:31,204
MAN:
Getting a bounce to signal.

352
00:19:31,204 --> 00:19:33,241
[cheering]

353
00:19:33,241 --> 00:19:35,450
FRAEMAN:
And I was in the room
with the science team

354
00:19:35,450 --> 00:19:36,865
when Opportunity landed on Mars,

355
00:19:36,865 --> 00:19:40,213
and it was the most
amazing experience.

356
00:19:40,213 --> 00:19:42,008
[cheering and applauding]

357
00:19:42,008 --> 00:19:44,528
NARRATOR:
Two rovers named Spirit
and Opportunity

358
00:19:44,528 --> 00:19:47,047
were sent to opposite sides
of the Red Planet

359
00:19:47,047 --> 00:19:50,085
to search for definitive proof

360
00:19:50,085 --> 00:19:53,226
that Mars's dry landscape

361
00:19:53,226 --> 00:19:54,883
was once a water world.

362
00:19:58,749 --> 00:20:02,235
At first glance,
modern Mars doesn't appear

363
00:20:02,235 --> 00:20:05,721
to be a very dynamic place.

364
00:20:05,721 --> 00:20:07,482
With an average
surface temperature

365
00:20:07,482 --> 00:20:10,416
of about
- 80 degrees Fahrenheit

366
00:20:10,416 --> 00:20:14,005
and an atmosphere just
one percent as thick as Earth's,

367
00:20:14,005 --> 00:20:16,491
it is a freezing desert.

368
00:20:18,803 --> 00:20:23,187
Typically, we think of
Mars as this dead world.

369
00:20:23,187 --> 00:20:26,742
But we do see changes
on the surface over time.

370
00:20:29,538 --> 00:20:33,887
NARRATOR:
Strange, overlapping lines,

371
00:20:33,887 --> 00:20:37,650
often dozens of feet wide,

372
00:20:37,650 --> 00:20:41,274
can stretch for miles.

373
00:20:45,658 --> 00:20:48,661
Unlike many of Mars's features,

374
00:20:48,661 --> 00:20:53,113
these are not relics.

375
00:20:53,113 --> 00:20:57,532
We see them appear
and disappear.

376
00:21:02,675 --> 00:21:05,850
What are these bizarre,
shape-shifting patterns?

377
00:21:05,850 --> 00:21:09,268
♪

378
00:21:13,133 --> 00:21:16,930
In January 2004,
Spirit and Opportunity

379
00:21:16,930 --> 00:21:20,313
began to investigate Mars.

380
00:21:20,313 --> 00:21:25,698
♪

381
00:21:25,698 --> 00:21:30,323
But their mission wasn't
expected to last very long.

382
00:21:30,323 --> 00:21:32,325
GUPTA:
Mars is covered in dust.

383
00:21:32,325 --> 00:21:34,223
It gets everywhere,

384
00:21:34,223 --> 00:21:37,123
including on the solar panels
of Mars rovers.

385
00:21:37,123 --> 00:21:40,678
As the solar panels
got dustier and dustier,

386
00:21:40,678 --> 00:21:42,370
the power levels
that the rover would have

387
00:21:42,370 --> 00:21:44,233
would get lower
and lower and lower,

388
00:21:44,233 --> 00:21:46,546
and eventually,
they would just stop working.

389
00:21:48,237 --> 00:21:50,067
NARRATOR:
The team hoped the rovers

390
00:21:50,067 --> 00:21:51,896
would last
at least three months,

391
00:21:51,896 --> 00:21:55,659
a feat they surpassed.

392
00:21:57,661 --> 00:22:00,353
But, as the months wore on,

393
00:22:00,353 --> 00:22:03,908
the power levels
continued to drop.

394
00:22:05,531 --> 00:22:07,256
What was really exciting

395
00:22:07,256 --> 00:22:08,672
was, at one point
in the mission,

396
00:22:08,672 --> 00:22:10,846
as we were seeing
the power levels

397
00:22:10,846 --> 00:22:13,228
getting lower
and lower and lower,

398
00:22:13,228 --> 00:22:15,886
all of a sudden,
the power levels were

399
00:22:15,886 --> 00:22:17,577
back up high again.

400
00:22:17,577 --> 00:22:22,237
♪

401
00:22:22,237 --> 00:22:25,171
Almost as high as they were
when the rovers had landed.

402
00:22:26,724 --> 00:22:29,934
And you can take a look at
the before and after pictures,

403
00:22:29,934 --> 00:22:32,420
and you can see that
it looks like the solar panels

404
00:22:32,420 --> 00:22:35,802
have just been wiped clean.

405
00:22:35,802 --> 00:22:37,942
You could call up AAA
and send them to Mars

406
00:22:37,942 --> 00:22:39,772
with the rag
to clean everything off.

407
00:22:39,772 --> 00:22:41,463
They couldn't have done
a better job.

408
00:22:44,673 --> 00:22:47,849
NARRATOR:
Finally, a clue
to what might be happening

409
00:22:47,849 --> 00:22:50,921
was spotted by Spirit's Navcam.

410
00:22:56,478 --> 00:23:00,620
♪

411
00:23:00,620 --> 00:23:02,933
In the mid-afternoon sun...

412
00:23:02,933 --> 00:23:04,417
♪

413
00:23:04,417 --> 00:23:06,350
...heating
of the Martian surface

414
00:23:06,350 --> 00:23:10,527
creates towering vortices,

415
00:23:10,527 --> 00:23:14,013
which can grow miles high.

416
00:23:17,775 --> 00:23:20,709
Dust devils.

417
00:23:20,709 --> 00:23:23,298
GUPTA:
I imagine it would be
absolutely terrifying

418
00:23:23,298 --> 00:23:25,887
to be standing
on the surface of Mars

419
00:23:25,887 --> 00:23:28,683
and see one of these dust devils
coming straight at you.

420
00:23:30,719 --> 00:23:32,825
FRAEMAN:
You might think
that there was this

421
00:23:32,825 --> 00:23:36,104
tornado-force wind
coming towards the rover,

422
00:23:36,104 --> 00:23:38,900
and it might pick the rover up
and spin them around

423
00:23:38,900 --> 00:23:40,522
and do all sorts
of horrible things.

424
00:23:40,522 --> 00:23:42,248
But in reality,

425
00:23:42,248 --> 00:23:45,044
the Martian atmosphere
is actually very, very thin,

426
00:23:45,044 --> 00:23:47,667
and so you can have
a dust devil pass over you

427
00:23:47,667 --> 00:23:49,531
and, and you would
barely even notice it.

428
00:23:49,531 --> 00:23:51,706
But even though a Martian
dust devil

429
00:23:51,706 --> 00:23:53,432
might not be able to
pick you up,

430
00:23:53,432 --> 00:23:55,537
it can certainly pick dust up.

431
00:23:57,677 --> 00:23:59,403
NARRATOR:
It's thought that

432
00:23:59,403 --> 00:24:02,855
as these whirlwinds
traveled over the rovers,

433
00:24:02,855 --> 00:24:05,374
they sucked dust
off the solar panels,

434
00:24:05,374 --> 00:24:08,308
like a vacuum.

435
00:24:08,308 --> 00:24:12,623
So a mission expected
to last just a few months

436
00:24:12,623 --> 00:24:15,454
was extended again,

437
00:24:15,454 --> 00:24:19,665
and again,

438
00:24:19,665 --> 00:24:22,012
and again.

439
00:24:23,738 --> 00:24:25,636
But the cleaning power
of the dust devils

440
00:24:25,636 --> 00:24:28,397
doesn't just work on rovers.

441
00:24:28,397 --> 00:24:32,436
[wind roaring]

442
00:24:32,436 --> 00:24:36,267
♪

443
00:24:36,267 --> 00:24:38,684
As they travel,

444
00:24:38,684 --> 00:24:39,995
these huge vortices

445
00:24:39,995 --> 00:24:43,171
suck up dust
from Mars's surface,

446
00:24:43,171 --> 00:24:47,037
exposing the darker bedrock
beneath.

447
00:24:49,660 --> 00:24:53,008
Leaving trails so large,

448
00:24:53,008 --> 00:24:56,184
we can see them clearly
from space.

449
00:24:56,184 --> 00:24:59,636
♪

450
00:24:59,636 --> 00:25:03,156
There are no Martians
creating the lines.

451
00:25:05,400 --> 00:25:10,405
The culprit is
the Martian atmosphere.

452
00:25:12,649 --> 00:25:16,445
Dust devils
might create the tracks,

453
00:25:16,445 --> 00:25:21,209
but something else
wipes them away.

454
00:25:21,209 --> 00:25:23,694
♪

455
00:25:23,694 --> 00:25:25,489
Just like Earth,

456
00:25:25,489 --> 00:25:29,735
Mars has a tilt
that gives it seasons.

457
00:25:29,735 --> 00:25:33,739
Summer in one hemisphere
means winter in the other.

458
00:25:37,743 --> 00:25:40,021
And with no oceans
or thick atmosphere

459
00:25:40,021 --> 00:25:42,541
to help spread heat
around the globe,

460
00:25:42,541 --> 00:25:45,923
an extreme temperature
difference.

461
00:25:48,374 --> 00:25:51,757
So here, dust helps
drive the action.

462
00:25:53,206 --> 00:25:57,625
♪

463
00:25:57,625 --> 00:26:01,145
As summer arrives
in the southern hemisphere,

464
00:26:01,145 --> 00:26:04,217
warmer temperatures
drive stronger winds,

465
00:26:04,217 --> 00:26:07,600
which kick dust up into the air.

466
00:26:09,326 --> 00:26:13,572
The dust absorbs sunlight
and heats the air around it...

467
00:26:16,644 --> 00:26:18,266
...further strengthening
the winds,

468
00:26:18,266 --> 00:26:22,822
which lift even more dust...

469
00:26:27,758 --> 00:26:32,280
...until a storm forms...

470
00:26:34,834 --> 00:26:39,908
...wiping away
dust devil trails.

471
00:26:39,908 --> 00:26:44,188
And these storms can combine
and grow so large...

472
00:26:47,951 --> 00:26:52,438
...that they engulf
the entire planet,

473
00:26:52,438 --> 00:26:56,649
sometimes blocking more than
99% of the incoming sunlight

474
00:26:56,649 --> 00:26:59,997
from reaching the surface...

475
00:27:01,758 --> 00:27:06,072
...and the solar panels
of Mars rovers.

476
00:27:08,799 --> 00:27:14,011
In May 2018, with Opportunity
still active on the surface,

477
00:27:14,011 --> 00:27:17,497
a storm began to build.

478
00:27:17,497 --> 00:27:18,913
FRAEMAN:
It only took a couple of days

479
00:27:18,913 --> 00:27:22,571
of seeing the skies get
darker and darker and darker

480
00:27:22,571 --> 00:27:24,263
before we started
to realize that,

481
00:27:24,263 --> 00:27:26,817
"Oh, this is actually,
this is a really bad one."

482
00:27:26,817 --> 00:27:29,130
Um, and by the end of the week,

483
00:27:29,130 --> 00:27:31,857
we knew that this was
the worst dust storm

484
00:27:31,857 --> 00:27:33,790
that we were ever gonna
have to survive.

485
00:27:33,790 --> 00:27:37,103
We knew we were probably gonna
lose communication with Oppy.

486
00:27:37,103 --> 00:27:40,279
So we let her go dark

487
00:27:40,279 --> 00:27:44,214
and we just waited and waited.

488
00:27:44,214 --> 00:27:47,631
NARRATOR:
Mars's low gravity means
the dust in the air

489
00:27:47,631 --> 00:27:51,704
can remain there for months.

490
00:27:51,704 --> 00:27:54,500
♪

491
00:27:54,500 --> 00:27:56,640
Eventually,
with so little sunlight

492
00:27:56,640 --> 00:27:59,781
reaching the Martian surface,

493
00:27:59,781 --> 00:28:02,404
the temperature differences
which fueled the storm

494
00:28:02,404 --> 00:28:05,235
are dampened,

495
00:28:05,235 --> 00:28:07,962
cutting off
its own energy supply,

496
00:28:07,962 --> 00:28:12,691
and the dust finally settles.

497
00:28:12,691 --> 00:28:15,694
But by the end of 2018,

498
00:28:15,694 --> 00:28:19,111
even after the Martian skies
had cleared,

499
00:28:19,111 --> 00:28:22,701
there was no signal
from Opportunity.

500
00:28:22,701 --> 00:28:24,633
And with winter looming,

501
00:28:24,633 --> 00:28:27,050
it was unlikely
the rover's electronics

502
00:28:27,050 --> 00:28:29,017
would survive the cold.

503
00:28:30,985 --> 00:28:33,608
♪

504
00:28:33,608 --> 00:28:35,990
On February 13, 2019,

505
00:28:35,990 --> 00:28:40,649
NASA declared
its mission complete.

506
00:28:40,649 --> 00:28:42,582
FRAEMAN:
I know it sounds weird,

507
00:28:42,582 --> 00:28:44,653
'cause it's a robot...
[laughs]

508
00:28:44,653 --> 00:28:46,345
...but it's sort of
the same feeling you have

509
00:28:46,345 --> 00:28:48,105
when you might lose a loved one

510
00:28:48,105 --> 00:28:50,383
who's lived a very full life.

511
00:28:50,383 --> 00:28:53,352
I was a high school student
when they landed.

512
00:28:53,352 --> 00:28:55,492
By the time
Opportunity's mission ended,

513
00:28:55,492 --> 00:28:58,460
I had gone to college,
I had gotten a Ph.D.,

514
00:28:58,460 --> 00:28:59,910
I had done a post-doc,

515
00:28:59,910 --> 00:29:02,223
and then I had been hired
by NASA

516
00:29:02,223 --> 00:29:05,640
to work on this very same
Opportunity rover

517
00:29:05,640 --> 00:29:07,815
that had inspired me when
I was a high school student.

518
00:29:10,231 --> 00:29:14,269
NARRATOR:
Sent to Mars to hunt
for ancient evidence of water,

519
00:29:14,269 --> 00:29:19,723
Opportunity not only succeeded,
but exceeded expectations,

520
00:29:19,723 --> 00:29:24,107
lasting over 14 years
thanks to the Martian weather.

521
00:29:27,144 --> 00:29:32,460
♪

522
00:29:32,460 --> 00:29:34,255
Despite their differences,

523
00:29:34,255 --> 00:29:40,192
Venus and Mars have
one thing in common.

524
00:29:40,192 --> 00:29:43,574
Their weather is powered
by solar energy.

525
00:29:47,268 --> 00:29:49,201
But beyond the asteroid belt...

526
00:29:52,514 --> 00:29:57,243
...ruled by
the dwarf planet Ceres,

527
00:29:57,243 --> 00:30:00,419
the sun's influence wanes.

528
00:30:02,593 --> 00:30:06,218
And yet,
the next planet we encounter

529
00:30:06,218 --> 00:30:07,978
is a storm world...

530
00:30:10,187 --> 00:30:13,225
...on the grandest scale.

531
00:30:23,752 --> 00:30:26,928
PITTS:
If you were just arriving
at Jupiter in a spacecraft,

532
00:30:26,928 --> 00:30:29,275
you would be stunned by what you
see.

533
00:30:29,275 --> 00:30:30,898
First of all, there's the size.

534
00:30:32,140 --> 00:30:37,905
You can fit 1,300 planet Earths
inside Jupiter.

535
00:30:37,905 --> 00:30:39,285
In fact, you could fit all of
the planets

536
00:30:39,285 --> 00:30:41,046
in the solar system insideJupiter

537
00:30:41,046 --> 00:30:42,599
and still have room to spare.

538
00:30:45,498 --> 00:30:49,917
NARRATOR:
Jupiter is a gas giant

539
00:30:49,917 --> 00:30:53,852
on which storms can grow bigger
than Earth itself.

540
00:30:56,993 --> 00:31:00,962
Since 2016,
NASA's Juno spacecraft

541
00:31:00,962 --> 00:31:05,449
has been exploring
this gargantuan planet

542
00:31:05,449 --> 00:31:08,901
and found its weather
is anything but subtle.

543
00:31:08,901 --> 00:31:14,079
[thunder rumbling]

544
00:31:14,079 --> 00:31:17,634
Jupiter's thunderstorms
can produce lightning bolts

545
00:31:17,634 --> 00:31:21,569
ten times more energetic
than anything recorded on Earth.

546
00:31:21,569 --> 00:31:24,261
[thunder rumbling,
lightning crackling]

547
00:31:24,261 --> 00:31:28,645
Most of the flashes lie beneath
thick ammonia ice clouds.

548
00:31:31,027 --> 00:31:34,651
But the most powerful storms
break free,

549
00:31:34,651 --> 00:31:38,551
soaring to the edge of space.

550
00:31:38,551 --> 00:31:42,038
[thunder booming,
lightning crackling]

551
00:31:42,038 --> 00:31:46,732
The scale of Jupiter's storms
may be hard to comprehend.

552
00:31:48,630 --> 00:31:50,770
But Juno found
that the frequency

553
00:31:50,770 --> 00:31:53,704
of its lightning strikes
is remarkably similar

554
00:31:53,704 --> 00:31:57,363
to Earth's thunderclouds.

555
00:32:00,746 --> 00:32:03,024
DRANSFIELD:
It's odd that lightning
is such a common occurrence

556
00:32:03,024 --> 00:32:04,025
here on Earth,

557
00:32:04,025 --> 00:32:05,371
but it's taken us centuries

558
00:32:05,371 --> 00:32:07,615
to really understand how itworks.

559
00:32:07,615 --> 00:32:10,859
[thunder claps,
lightning crackles]

560
00:32:10,859 --> 00:32:12,827
NARRATOR:
The substance responsible

561
00:32:12,827 --> 00:32:18,177
for our planet's thunderstorms
is water.

562
00:32:18,177 --> 00:32:19,316
The way that lightning getsformed

563
00:32:19,316 --> 00:32:21,353
is that it relies on collisions

564
00:32:21,353 --> 00:32:25,288
between icy particles and watery
droplets.

565
00:32:25,288 --> 00:32:29,395
And as the watery droplets
are moving upwards and colliding

566
00:32:29,395 --> 00:32:31,501
with the icy particles
that are falling downwards,

567
00:32:31,501 --> 00:32:36,678
they're exchanging charge
with each other.

568
00:32:36,678 --> 00:32:39,267
So you get a separation
of charge

569
00:32:39,267 --> 00:32:41,960
from the top of a cloud
to the bottom of the cloud.

570
00:32:43,375 --> 00:32:45,101
And as that separation of charge

571
00:32:45,101 --> 00:32:47,241
becomes bigger
and bigger and bigger,

572
00:32:47,241 --> 00:32:49,588
eventually, the atmosphere
can't cope anymore.

573
00:32:49,588 --> 00:32:51,210
PITTS:
And when that occurs,

574
00:32:51,210 --> 00:32:53,661
now a flow of electricity
can happen.

575
00:32:53,661 --> 00:32:58,217
[lightning crackling]

576
00:32:58,217 --> 00:33:02,221
NARRATOR:
A single bolt of lightning
is so powerful,

577
00:33:02,221 --> 00:33:05,121
it can heat the surrounding air

578
00:33:05,121 --> 00:33:08,883
to temperatures greater
than the surface of the sun.

579
00:33:08,883 --> 00:33:13,992
♪

580
00:33:17,996 --> 00:33:23,242
So how can clouds
produce so much energy?

581
00:33:23,242 --> 00:33:26,314
HEIDI BECKER:
For all of our history,
lightning has been

582
00:33:26,314 --> 00:33:29,007
something
that humans have feared.

583
00:33:29,007 --> 00:33:33,011
But what's driving it
really is the water cycle.

584
00:33:33,011 --> 00:33:35,151
The sun heats the water,

585
00:33:35,151 --> 00:33:37,808
it evaporates,
becomes water vapor,

586
00:33:37,808 --> 00:33:39,810
rises up into the atmosphere,

587
00:33:39,810 --> 00:33:42,261
cools, and eventually becomes

588
00:33:42,261 --> 00:33:44,298
water droplets in clouds.

589
00:33:44,298 --> 00:33:46,610
And intuitively, as humans,

590
00:33:46,610 --> 00:33:49,234
we actually understand
what's happening very well.

591
00:33:49,234 --> 00:33:51,960
We wet our hand,

592
00:33:51,960 --> 00:33:53,755
and it feels cold because

593
00:33:53,755 --> 00:33:57,069
the water is stealing energy
from our hand,

594
00:33:57,069 --> 00:33:59,071
breaking up the
water molecules,

595
00:33:59,071 --> 00:34:00,417
turning them into
water vapor

596
00:34:00,417 --> 00:34:01,418
so that they can

597
00:34:01,418 --> 00:34:02,695
rise up intothe sky.

598
00:34:04,249 --> 00:34:07,252
NARRATOR:
Water evaporation
requires energy,

599
00:34:07,252 --> 00:34:12,291
whether it's from
our body heat or the sun.

600
00:34:12,291 --> 00:34:17,365
As water turns from a liquid
to a gas, it stores this energy.

601
00:34:18,815 --> 00:34:23,026
And when it turns back into
a liquid, in the form of clouds,

602
00:34:23,026 --> 00:34:27,755
it releases this energy
back into the atmosphere.

603
00:34:27,755 --> 00:34:29,584
What's kind of incredible
to believe

604
00:34:29,584 --> 00:34:33,278
is that a, a small little
cumulus cloud that you might see

605
00:34:33,278 --> 00:34:36,281
floating in the sky, looking
so graceful and peaceful,

606
00:34:36,281 --> 00:34:38,179
is actually the result

607
00:34:38,179 --> 00:34:40,837
of an enormous amount of energy
being released.

608
00:34:40,837 --> 00:34:44,461
It's the same
as hundreds of tons of TNT.

609
00:34:46,187 --> 00:34:48,155
NARRATOR:
And for an average thunderstorm,

610
00:34:48,155 --> 00:34:52,297
the energy released is
equivalent to a nuclear blast.

611
00:34:54,402 --> 00:34:57,716
It's this huge release of heat

612
00:34:57,716 --> 00:35:01,133
that makes thunderclouds
so turbulent,

613
00:35:01,133 --> 00:35:04,240
causing
the countless icy collisions...

614
00:35:04,240 --> 00:35:06,656
[thunder rumbling,
lightning crackling]

615
00:35:09,141 --> 00:35:11,592
...which power
Earth's lightning.

616
00:35:15,527 --> 00:35:18,426
Several missions to Jupiter
have detected water

617
00:35:18,426 --> 00:35:20,877
in its atmosphere.

618
00:35:22,396 --> 00:35:25,709
But the planet receives just
four percent of the sunlight

619
00:35:25,709 --> 00:35:29,127
that reaches Earth,

620
00:35:29,127 --> 00:35:33,510
too little energy to account for
its ferocious lightning storms.

621
00:35:35,547 --> 00:35:39,067
♪

622
00:35:39,067 --> 00:35:43,210
But looking at the planet
in infrared

623
00:35:43,210 --> 00:35:46,454
reveals a different source
of energy.

624
00:35:46,454 --> 00:35:49,250
Jupiter is radiating heat,

625
00:35:49,250 --> 00:35:53,668
almost twice the energy
it receives from the sun.

626
00:35:56,361 --> 00:35:59,536
FLETCHER:
So, Jupiter itself
is slowly cooling,

627
00:35:59,536 --> 00:36:02,574
and has been over the entire age
of the solar system.

628
00:36:02,574 --> 00:36:07,130
And as it's cooling, the entire
gas giant is slowly shrinking.

629
00:36:07,130 --> 00:36:10,409
And as it shrinks,
it's relinquishing that energy

630
00:36:10,409 --> 00:36:13,723
that was left over
from when Jupiter was born.

631
00:36:13,723 --> 00:36:15,173
That's enough to power

632
00:36:15,173 --> 00:36:17,209
the gargantuan storms
that we see.

633
00:36:17,209 --> 00:36:21,282
[crackling]

634
00:36:21,282 --> 00:36:23,802
NARRATOR:
This internal heat means water.

635
00:36:23,802 --> 00:36:29,014
The chemical powering
Earth's storms

636
00:36:29,014 --> 00:36:32,190
also powers storms on Jupiter.

637
00:36:34,985 --> 00:36:38,161
In vapor form, water rises,

638
00:36:38,161 --> 00:36:41,578
carrying heat energy
from deep inside the planet...

639
00:36:44,236 --> 00:36:49,345
...until it reaches a place
under the ammonia ice clouds...

640
00:36:51,001 --> 00:36:52,520
[thunder crashes]

641
00:36:52,520 --> 00:36:53,797
...where it's cool enough

642
00:36:53,797 --> 00:36:56,490
to condense into
liquid water droplets

643
00:36:56,490 --> 00:36:59,562
and ice crystals.

644
00:37:01,322 --> 00:37:04,808
The energy released
by this condensing water

645
00:37:04,808 --> 00:37:08,467
powers the growth
of violent thunderstorms.

646
00:37:12,230 --> 00:37:15,094
But because Jupiter
has so much internal heat

647
00:37:15,094 --> 00:37:18,166
that's trying to escape,

648
00:37:18,166 --> 00:37:22,654
in some places, enough energy is
released by condensing water...

649
00:37:24,483 --> 00:37:29,247
...that ice crystals are swept
up into the ice clouds above.

650
00:37:34,493 --> 00:37:39,636
Here, ammonia acts
as an antifreeze...

651
00:37:41,328 --> 00:37:43,433
...allowing thunderclouds
to grow

652
00:37:43,433 --> 00:37:47,472
to more than 35 miles tall

653
00:37:47,472 --> 00:37:51,924
and lightning to strike
at minus 150 degrees Fahrenheit.

654
00:37:53,616 --> 00:38:00,864
♪

655
00:38:00,864 --> 00:38:03,902
Jupiter and Earth
may be worlds apart,

656
00:38:03,902 --> 00:38:07,319
but both play host
to lightning storms

657
00:38:07,319 --> 00:38:12,082
which are driven by water.

658
00:38:14,568 --> 00:38:16,155
I just find it wicked cool
that on a planet

659
00:38:16,155 --> 00:38:17,674
as different as Jupiter,

660
00:38:17,674 --> 00:38:20,643
the weather is being formed
in much the same way

661
00:38:20,643 --> 00:38:21,816
as it is here on Earth.

662
00:38:26,787 --> 00:38:30,480
NARRATOR:
However, there is one more place
in the solar system

663
00:38:30,480 --> 00:38:35,382
with even more
Earth-like weather.

664
00:38:35,382 --> 00:38:37,867
PITTS:
But what's really interesting
and exciting is,

665
00:38:37,867 --> 00:38:40,352
the liquid that's being shiftedaround

666
00:38:40,352 --> 00:38:41,664
isn't water.

667
00:38:43,390 --> 00:38:46,876
NARRATOR:
To find it, we travel
400 million miles farther

668
00:38:46,876 --> 00:38:49,361
from the sun

669
00:38:49,361 --> 00:38:54,608
and encounter another gas giant.

670
00:38:54,608 --> 00:38:57,404
But this isn't our destination.

671
00:38:57,404 --> 00:39:00,648
♪

672
00:39:00,648 --> 00:39:06,136
Saturn is orbited by
an amazing variety of moons,

673
00:39:06,136 --> 00:39:10,417
so many that it can be hard
to keep track of them all.

674
00:39:14,006 --> 00:39:15,905
Iapetus, Rhea,

675
00:39:15,905 --> 00:39:17,527
Enceladus...

676
00:39:17,527 --> 00:39:20,634
GAO:
Tethys, Mimas, Epimethys.

677
00:39:20,634 --> 00:39:25,639
Helene, Prometheus, uh, Calypso.

678
00:39:25,639 --> 00:39:27,468
Shoot, there's that
really funny one.

679
00:39:27,468 --> 00:39:28,573
Phoebe.

680
00:39:28,573 --> 00:39:30,437
There's Pan,
which is really cool

681
00:39:30,437 --> 00:39:32,059
because it looks like a ravioli.

682
00:39:32,059 --> 00:39:34,372
GRINSPOON [laughing]:
I didn't cram for this.

683
00:39:34,372 --> 00:39:35,787
Did I mention Mimas?

684
00:39:35,787 --> 00:39:37,409
GRINSPOON:
What's the little,
really weird...

685
00:39:37,409 --> 00:39:38,617
Hyperion.

686
00:39:38,617 --> 00:39:40,412
Uh...
[chuckles]

687
00:39:40,412 --> 00:39:41,586
Um...

688
00:39:41,586 --> 00:39:43,553
Um, uh, let's see.

689
00:39:43,553 --> 00:39:46,245
And a bunch more.
[laughs]

690
00:39:47,246 --> 00:39:50,077
NARRATOR:
But one is special.

691
00:39:50,077 --> 00:39:53,874
More than 20 times the mass
of all the others combined.

692
00:39:56,221 --> 00:40:00,570
It's the only moon in the solar
system with a thick atmosphere.

693
00:40:10,269 --> 00:40:14,998
In November 1980,
NASA's Voyager 1 spacecraft

694
00:40:14,998 --> 00:40:17,760
revealed Saturn
and its many moons

695
00:40:17,760 --> 00:40:21,315
in greater detail
than ever before.

696
00:40:21,315 --> 00:40:24,732
PITTS:
When the Voyager 1 spacecraft
flew by Titan,

697
00:40:24,732 --> 00:40:26,527
we could see
that it had an atmosphere,

698
00:40:26,527 --> 00:40:28,011
and a thick atmosphere,

699
00:40:28,011 --> 00:40:32,499
but this was only
a tantalizing view.

700
00:40:32,499 --> 00:40:34,466
SOTO:
The images from Voyager of Titan

701
00:40:34,466 --> 00:40:37,745
were exciting but also,
in a way,

702
00:40:37,745 --> 00:40:39,298
infuriating, right?

703
00:40:39,298 --> 00:40:43,371
It confirmed everything that
we had thought about Titan,

704
00:40:43,371 --> 00:40:45,615
but it didn't allow us
to see down to the surface.

705
00:40:45,615 --> 00:40:48,031
With Voyager, we could do some
remote sensing

706
00:40:48,031 --> 00:40:52,208
and start to tell that
the surface was, was very cold,

707
00:40:52,208 --> 00:40:54,175
but in
the right temperature range

708
00:40:54,175 --> 00:40:57,040
so that you might actually have
liquid methane on the surface.

709
00:40:57,040 --> 00:40:59,180
And so we, we just knew that we
had to go back

710
00:40:59,180 --> 00:41:02,839
and, and learn more.

711
00:41:02,839 --> 00:41:08,155
MAN:
Five, four, three, two, one,

712
00:41:08,155 --> 00:41:11,296
and liftoff of
the Cassini spacecraft

713
00:41:11,296 --> 00:41:14,506
on a billion-mile trek
to Saturn.

714
00:41:14,506 --> 00:41:16,888
NARRATOR:
The legendary
Cassini-Huygens mission

715
00:41:16,888 --> 00:41:20,443
took almost seven years
to reach Saturn

716
00:41:20,443 --> 00:41:22,514
and spent over a decade

717
00:41:22,514 --> 00:41:26,035
exploring the planet
and its moons.

718
00:41:26,035 --> 00:41:29,417
And on December 25, 2004,

719
00:41:29,417 --> 00:41:33,111
nearly a quarter of a century
after Voyager 1's flyby...

720
00:41:34,975 --> 00:41:40,187
...the Huygens probe
detached from Cassini

721
00:41:40,187 --> 00:41:44,087
in a bid to become the first
probe ever to land on a body

722
00:41:44,087 --> 00:41:47,090
in the outer solar system.

723
00:41:47,090 --> 00:41:49,403
♪

724
00:41:49,403 --> 00:41:51,543
You know, there was
so much anticipation

725
00:41:51,543 --> 00:41:53,649
of what that surface
might be like.

726
00:41:53,649 --> 00:41:56,790
But I think in none
of our wildest dreams

727
00:41:56,790 --> 00:42:00,518
was the surface of Titan
as interesting and beautiful

728
00:42:00,518 --> 00:42:04,073
and exotic and exciting
as it turns out to actually be.

729
00:42:12,737 --> 00:42:16,844
NARRATOR:
During its two-and-a-half-hour
descent to Titan,

730
00:42:16,844 --> 00:42:20,917
Huygens captured images
of intricate ridges,

731
00:42:20,917 --> 00:42:23,644
deep gullies,

732
00:42:23,644 --> 00:42:27,924
and, perhaps most strikingly,
river channels.

733
00:42:31,894 --> 00:42:35,345
GRINSPOON:
It was truly like a dream,
but there they are.

734
00:42:35,345 --> 00:42:36,450
These are real pictures coming

735
00:42:36,450 --> 00:42:38,486
from our first-ever descent
to Titan.

736
00:42:38,486 --> 00:42:41,559
And, uh, it's unmistakable
what we're seeing.

737
00:42:41,559 --> 00:42:43,561
And I'll, I'll just
never forget that moment.

738
00:42:44,907 --> 00:42:46,356
PITTS:
It's a moon!

739
00:42:46,356 --> 00:42:48,911
It's a moon
that looks like this!

740
00:42:48,911 --> 00:42:51,430
Not a planet.

741
00:42:51,430 --> 00:42:55,642
How do you, how do you have
these fluvial erosional features

742
00:42:55,642 --> 00:42:57,678
on the moon of a planet?

743
00:42:57,678 --> 00:43:00,508
♪

744
00:43:00,508 --> 00:43:06,204
NARRATOR:
The team had designed
Huygens to float,

745
00:43:06,204 --> 00:43:11,692
but it landed in what appeared
to be an empty riverbed.

746
00:43:11,692 --> 00:43:16,179
And the river channels it imaged
during its descent were dry.

747
00:43:18,803 --> 00:43:21,012
The probe continued
to transmit data

748
00:43:21,012 --> 00:43:24,015
from Titan's surface
for more than an hour

749
00:43:24,015 --> 00:43:29,020
before its breathtaking mission
came to an end.

750
00:43:29,020 --> 00:43:33,403
But Cassini continued to explore
the surface from afar.

751
00:43:35,889 --> 00:43:40,652
♪

752
00:43:40,652 --> 00:43:44,656
It saw a landscape
of rolling dune fields,

753
00:43:44,656 --> 00:43:48,349
vast plains,

754
00:43:48,349 --> 00:43:52,043
and more dried-up rivers.

755
00:43:52,043 --> 00:43:54,977
It seemed Titan
was a desert world.

756
00:43:57,945 --> 00:44:03,641
But in 2006, after
many months of searching...

757
00:44:06,264 --> 00:44:08,680
...Cassini's radar instrument
found

758
00:44:08,680 --> 00:44:14,306
what everyone
had been waiting for:

759
00:44:14,306 --> 00:44:18,172
lakes and seas of liquid methane
at the north pole.

760
00:44:20,140 --> 00:44:23,868
Titan's equatorial region
may be a desert,

761
00:44:23,868 --> 00:44:29,977
but Cassini had proved that
its poles were anything but.

762
00:44:29,977 --> 00:44:31,358
FLETCHER:
So that difference we could see

763
00:44:31,358 --> 00:44:33,084
between the deserts

764
00:44:33,084 --> 00:44:34,741
down around the equatorialregion

765
00:44:34,741 --> 00:44:36,087
and the seas that were present

766
00:44:36,087 --> 00:44:37,709
up at high latitudes

767
00:44:37,709 --> 00:44:39,366
had us scratching our heads.

768
00:44:40,988 --> 00:44:42,714
NARRATOR:
What could be carving channels

769
00:44:42,714 --> 00:44:48,030
over a thousand miles away
from the poles?

770
00:44:55,002 --> 00:44:57,591
MACKENZIE:
We think about deserts
as dry places,

771
00:44:57,591 --> 00:45:00,732
and most of the time they are,
but they're carved,

772
00:45:00,732 --> 00:45:04,563
they're shaped, they're defined
by these seasonal rainstorms

773
00:45:04,563 --> 00:45:07,118
that may happen
only once or twice a year.

774
00:45:08,326 --> 00:45:12,986
The question is, could something
similar be happening on Titan?

775
00:45:12,986 --> 00:45:14,781
Saturn happens to be tilted

776
00:45:14,781 --> 00:45:17,369
at about the same angle that the
Earth is.

777
00:45:17,369 --> 00:45:18,923
So as it's going around the sun,

778
00:45:18,923 --> 00:45:22,581
it experiences seasons much
like we do here on the Earth.

779
00:45:22,581 --> 00:45:25,067
But it takes Saturn and Titan
a lot longer

780
00:45:25,067 --> 00:45:27,138
to go around the sun than we do.

781
00:45:27,138 --> 00:45:29,865
It takes 29-and-a-half years.

782
00:45:29,865 --> 00:45:32,695
Titan shares the same orbital
plane as Saturn.

783
00:45:32,695 --> 00:45:34,939
And so it also experiences
seasons

784
00:45:34,939 --> 00:45:37,562
as it's going around the sun.

785
00:45:37,562 --> 00:45:39,633
If we take the southern
hemisphere, for example,

786
00:45:39,633 --> 00:45:42,256
there are seven years of summer

787
00:45:42,256 --> 00:45:44,776
where the southern hemisphere
is pointed

788
00:45:44,776 --> 00:45:47,537
towards the sun and receiving
more energy.

789
00:45:47,537 --> 00:45:49,091
That extra bit of energy,

790
00:45:49,091 --> 00:45:51,265
even though it's only a 100th

791
00:45:51,265 --> 00:45:53,371
of what we experience here
on the Earth,

792
00:45:53,371 --> 00:45:56,754
is enough to pump the atmosphere
full of methane,

793
00:45:56,754 --> 00:45:58,031
thanks to evaporation

794
00:45:58,031 --> 00:45:59,964
from the lakes in the
south pole.

795
00:45:59,964 --> 00:46:04,658
♪

796
00:46:04,658 --> 00:46:07,972
NARRATOR:
Cassini saw this happening.

797
00:46:07,972 --> 00:46:11,596
It flew by Titan during
the southern summer...

798
00:46:14,392 --> 00:46:20,363
...and saw methane clouds
swirling around the south pole.

799
00:46:21,502 --> 00:46:24,540
But the clouds
didn't stay there.

800
00:46:28,268 --> 00:46:31,443
MACKENZIE:
In 2010, there was a giant cloud

801
00:46:31,443 --> 00:46:34,999
that formed over the equatorial
region in the shape of an arrow.

802
00:46:34,999 --> 00:46:37,104
And as it moved across
the surface of Titan,

803
00:46:37,104 --> 00:46:40,625
we saw that land
that was bright before

804
00:46:40,625 --> 00:46:43,835
darkened, uh,
after the cloud passed over.

805
00:46:43,835 --> 00:46:45,457
And the area that darkened

806
00:46:45,457 --> 00:46:49,461
is equivalent to about
Utah and Arizona put together.

807
00:46:49,461 --> 00:46:51,498
So how did that happen?

808
00:46:51,498 --> 00:46:52,879
What is responsible for that?

809
00:46:52,879 --> 00:46:54,570
Well, we think
the best explanation

810
00:46:54,570 --> 00:46:57,642
is a giant rainstorm.

811
00:46:57,642 --> 00:47:03,234
♪

812
00:47:03,234 --> 00:47:09,067
NARRATOR:
In Titan's deserts,
autumn brings change to the air.

813
00:47:09,067 --> 00:47:11,898
Monsoons arrive
from the south...

814
00:47:16,212 --> 00:47:20,872
...unleashing torrents
of methane rain.

815
00:47:20,872 --> 00:47:25,704
But because of Titan's low
gravity and dense atmosphere,

816
00:47:25,704 --> 00:47:29,847
the raindrops fall about
six times slower than on Earth.

817
00:47:33,954 --> 00:47:37,855
These storms dump enough liquid
methane onto the surface...

818
00:47:40,961 --> 00:47:43,308
...to create flash floods...

819
00:47:46,622 --> 00:47:49,659
...which drain
into dry riverbeds...

820
00:47:53,940 --> 00:47:56,701
...carving into the landscape...

821
00:48:06,918 --> 00:48:12,544
...before spilling out
onto vast floodplains.

822
00:48:17,929 --> 00:48:20,173
MACKENZIE:
So, thanks to Cassini, we know

823
00:48:20,173 --> 00:48:22,382
that massive floods
are happening on Titan.

824
00:48:22,382 --> 00:48:24,487
And just a few months later,

825
00:48:24,487 --> 00:48:28,043
which is only, like,
five Titan days, that same land

826
00:48:28,043 --> 00:48:31,080
reverted to what it looked
like before, it brightened.

827
00:48:31,080 --> 00:48:32,564
And the clouds themselves

828
00:48:32,564 --> 00:48:36,120
that were responsible for
that rain had already moved on.

829
00:48:36,120 --> 00:48:41,884
♪

830
00:48:41,884 --> 00:48:47,579
NARRATOR:
In 2022, five years after
the Cassini mission ended,

831
00:48:47,579 --> 00:48:49,857
the James Webb Space Telescope

832
00:48:49,857 --> 00:48:55,622
turned its infrared gaze
towards Saturn's largest moon.

833
00:48:56,692 --> 00:49:00,489
By now it was late summer
in Titan's northern hemisphere,

834
00:49:00,489 --> 00:49:06,253
and the telescope spotted
something remarkable:

835
00:49:06,253 --> 00:49:10,292
huge clouds over the north pole.

836
00:49:10,292 --> 00:49:15,814
The traveling storms
had reached their destination.

837
00:49:16,850 --> 00:49:19,853
It is now believed
Titan's storm belt

838
00:49:19,853 --> 00:49:24,996
goes on an epic
29-and-a-half-year journey

839
00:49:24,996 --> 00:49:30,105
from one pole to the other
and back again.

840
00:49:30,105 --> 00:49:32,210
Slow-motion seasons

841
00:49:32,210 --> 00:49:36,732
unleashing massive,
slow-motion storms,

842
00:49:36,732 --> 00:49:41,944
creating seasonal rivers
of methane,

843
00:49:41,944 --> 00:49:46,535
in a desert
on one of Saturn's moons.

844
00:49:46,535 --> 00:49:49,987
♪

845
00:49:55,509 --> 00:49:58,857
MACKENZIE:
It's pretty incredible
to be standing here

846
00:49:58,857 --> 00:50:01,791
in a desert landscape
on the Earth

847
00:50:01,791 --> 00:50:04,415
and think about
how similar that is

848
00:50:04,415 --> 00:50:06,865
to a landscape
a billion miles away

849
00:50:06,865 --> 00:50:08,902
elsewhere in the solar system,

850
00:50:08,902 --> 00:50:12,457
the same processes,
the same desert monsoon systems

851
00:50:12,457 --> 00:50:14,390
we think are at work on Titan,

852
00:50:14,390 --> 00:50:18,153
creating vistas much like
this one that we see here.

853
00:50:18,153 --> 00:50:21,397
And yet the compounds,
the materials

854
00:50:21,397 --> 00:50:24,538
that are involved in that
process are totally different,

855
00:50:24,538 --> 00:50:26,540
and the temperature's
totally different,

856
00:50:26,540 --> 00:50:28,439
and the timescales
are totally different.

857
00:50:28,439 --> 00:50:31,476
And they're leading
to a phenomenal landscape

858
00:50:31,476 --> 00:50:34,479
like the one that we see here.

859
00:50:34,479 --> 00:50:36,861
♪

860
00:50:43,178 --> 00:50:46,077
SOUSA-SILVA:
On all these worlds,
all this complexity,

861
00:50:46,077 --> 00:50:47,596
all these storms

862
00:50:47,596 --> 00:50:50,254
ultimately come from one
fundamental law of nature.

863
00:50:50,254 --> 00:50:52,911
FLETCHER:
That need to move energy

864
00:50:52,911 --> 00:50:55,673
from where it's plentiful
to where it's scarce.

865
00:51:01,230 --> 00:51:03,474
DOTTIN:
What makes these worlds
so different

866
00:51:03,474 --> 00:51:05,200
are the unique conditions

867
00:51:05,200 --> 00:51:07,029
that are found
in their atmospheres.

868
00:51:07,029 --> 00:51:08,962
[thunder rumbling]

869
00:51:08,962 --> 00:51:11,344
GUPTA:
Because that determines
the chemistry

870
00:51:11,344 --> 00:51:14,692
that drives their storms
and shapes their surfaces.

871
00:51:14,692 --> 00:51:17,729
[thunder rumbling]

872
00:51:17,729 --> 00:51:20,042
GRINSPOON:
You know, it's a pretty
amazing time to be alive

873
00:51:20,042 --> 00:51:22,493
in, in that we have the ability

874
00:51:22,493 --> 00:51:26,013
to be monitoring weather
on other planets.

875
00:51:26,013 --> 00:51:28,533
And yet I feel like
we're in our early stages

876
00:51:28,533 --> 00:51:31,018
of understanding weather
beyond Earth.

877
00:51:32,572 --> 00:51:34,505
DRANSFIELD:
There are hundreds
of billions of stars

878
00:51:34,505 --> 00:51:36,093
out there in the galaxy.

879
00:51:36,093 --> 00:51:40,269
And we now know that planets
around stars is the norm.

880
00:51:40,269 --> 00:51:43,030
GAO:
So that's potentially
billions and billions

881
00:51:43,030 --> 00:51:44,687
of planets orbiting out there,

882
00:51:44,687 --> 00:51:46,448
all each with their own
weather systems and storms.

883
00:51:47,690 --> 00:51:49,382
FRAEMAN:
And I think there are things
that are happening

884
00:51:49,382 --> 00:51:52,523
on these planets that we haven't
even begun to imagine,

885
00:51:52,523 --> 00:51:54,249
because they're gonna be
so different

886
00:51:54,249 --> 00:51:56,147
from anything else
that we've been able

887
00:51:56,147 --> 00:51:59,150
to experience
in our own solar system.

888
00:52:00,324 --> 00:52:02,395
GAO:
And so that
just makes me think of,

889
00:52:02,395 --> 00:52:04,638
what possibilities exist
out there?

890
00:52:05,639 --> 00:52:09,298
What have we not thought of?

891
00:52:09,298 --> 00:52:13,333
♪

