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(dramatic orchestral music)
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- [Narrator] Venus.
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At the surface, it's air
is 95% carbon dioxide.
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The atmospheric pressure is
like being 900 meters deep
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in Earth's oceans.
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It's hotter than anywhere
else in the solar system,
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except the sun.
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And yet, visionary
engineers and scientists
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are now unveiling daring new strategies
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to explore its tortured landscapes,
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to sail it's turbulent, upper-level winds,
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to imagine altering its very climate.
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(intense instrumental music)
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They are taking the first steps
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towards settling the
second planet from the sun.
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- [Mission Control]
Ignition sequence started.
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All engines are started.
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We have a liftoff. We have a liftoff.
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(indistinct chatter)
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(rocket rumbling)
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- [Narrator] The early 1970s.
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The Space Age was at its peak.
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The Apollo astronauts
were exploring the moon.
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- [Astronaut] Those
rocks have been waiting
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four and a half billion years
for us to come grab 'em.
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- [Narrator] Robotic spacecraft
had visited Venus ...
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(thunder rumbling)
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Mars ...
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Mercury ...
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and Jupiter, with new missions
on the drawing boards.
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And yet, in those heady days,
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America and Europe faced a
series of daunting challenges.
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The ongoing Cold War ...
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unchecked industrial pollution ...
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race and class conflict ...
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a sudden fuel shortage.
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Many thought that only
strict Earth preservation
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and laws limiting industry
could save civilization.
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(gentle woodwind music)
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Meanwhile, a small cadre
of scientists, philosophers
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and writers sought answers
in farsighted engineering ...
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decentralized information systems ...
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which later became the internet
and cellular networks ...
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molecular biology ...
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which led to gene sequencing
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and the promise of nanotechnology ...
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and human expansion into space.
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They envisioned moon bases ...
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cities on Mars ...
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grand orbital habitats.
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The so-called space colonies would pioneer
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a whole new way of living.
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(feverish string music)
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Future residents in space
would be free to live
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by whatever social contracts they chose.
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Huge structures assembled
by astronauts and robots,
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they would draw upon
resources on the moon ...
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- [Astronaut] Stand by for pitch
over. Oh, are we coming in.
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- [Narrator] Materials from asteroids ...
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and on the free energy of the sun.
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These plans consistently
overlooked one planet ...
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Venus.
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Hellishly hot and enveloped
in a crushing atmosphere,
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how could anyone ever live there?
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To some visionary thinkers,
Venus held a unique promise,
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one that led to one of the most innovative
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mission ideas on the books.
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(building orchestral music)
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A spacecraft carrying astronauts
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is bound inward toward the sun.
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It slips into low orbit around Venus,
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docking with an uncrewed
sister ship sent months before.
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One will de-orbit,
protected by an arrow shell,
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as it bleeds speed into heat.
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(booming)
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A parachute further slows the vehicle.
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But it isn't heading for a landing.
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Instead of continuing to the surface,
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it deploys and inflating envelope,
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an airship up to 130 meters in length.
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The High-Altitude Venus
Operational Concept, HAVOC.
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Its crew sales for about 30 Earth days,
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navigating in the fast wins,
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suspended beneath an inflated
envelope of helium gas.
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Circling the planet, they deploy probes
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to learn about its atmosphere and geology.
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They send out a fleet of
small robotic balloons
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to dip down into the
hostile, lower atmosphere.
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(dramatic orchestral music)
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Their studies complete, the crew ascends
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to their transport ship in orbit.
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Then, kicked off by a powerful rocket,
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they escape Venus's
nearly Earth-level gravity
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and make the 100-day
journey back to Earth.
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HAVOC-style missions would set the stage
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for a longterm plan to
permanently settle Venus.
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(atmospheric music)
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Though the landscape of Venus
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is a hot, high-pressure death trap,
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the upper atmosphere
could offer safe harbor.
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- In the clouds of Venus,
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which is 50 kilometers
up from the surface,
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there is a realm where
it's very much Earth-like
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in terms of the conditions,
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except for the clouds themselves
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are made out of
concentrated sulfuric acid.
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- Of course, you still have no
atmosphere with oxygen in it.
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You still have the sulfur oxides
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that give you sulfuric acid.
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So you don't want to go
outside without any protection.
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But in terms of temperature and pressure,
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it's very, very Earth-like.
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- So you can imagine sending humans there
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and some kind of a balloon platform
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or some other floating platform
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to explore the clouds of Venus,
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and you wouldn't need a pressure suit,
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and you wouldn't have to worry
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about the thermal environment;
it would be quite pleasant.
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You would just need some thin protection
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from the acid clouds,
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and you would need a breathing apparatus,
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since it's mostly carbon dioxide.
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But in terms of the environment,
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say compared to the surface of Mars,
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the clouds of Venus would
be a much easier place
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to send human beings.
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- [Narrator] Let's take a slice
of the planet's atmosphere.
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From the sweltering ground
to the vacuum of space,
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200 kilometers tall.
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On the surface, you'd feel as squeezed
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as diving, nearly a kilometer underwater
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and being big twice as
hot as in a pizza oven,
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But, rise up 50 kilometers,
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and you'll enjoy Earth-normal pressure
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and springtime temperatures.
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This moderate zone,
high in the atmosphere,
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has plenty of light, but
not too much radiation.
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It's an ideal location
for a research station.
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(intriguing electronic music)
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Imagine frequent flights into
the stormy clouds of Venus.
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(thunder rumbling)
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The airships would be
spun from carbon fiber
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harvested from the atmosphere itself,
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their electric motors powered by the sun.
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Ahead, a permanent floating
station, a cloud city awaits.
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- I have been thinking of this idea
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that you could float habitats
in the atmosphere of Venus.
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And the habit has could be very large,
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they could be kilometers in scale.
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And the interesting thing
is, if you did this,
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you wouldn't even need to
have hydrogen or helium
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to make them float, because
the atmosphere of Venus
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is mostly carbon dioxide.
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Oxygen and nitrogen,
ordinary, breathable air
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would float in the atmosphere of Venus.
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And inside their giant bubbles,
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you can walk around on the inside,
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because the air that's holding you up
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is also the air that you can breathe.
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The lifting gas is your environment.
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- [Narrator] The interior
ecosystem can be lush
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with plenty of room to breathe
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and plenty of acreage for growing food.
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This home in the clouds can
be nearly self-sustaining.
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Looking up through the
transparent domed rooftop,
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you watch vessels come and go.
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Suspended beneath the
habitat, the logistics hub
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to house its core services
and computer systems.
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The docking ports are
staggered across two levels
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to accommodate the wide girths
of several airships at once.
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(propellor buffeting)
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(soft orchestral music)
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Expeditions set of off,
launching instruments as they go.
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They'll diverge onto different courses,
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running survey transects
above the surface of Venus.
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- There are some experiments
that you could only do
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if you actually go and float
around in the atmosphere.
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And what you could do is
answer a lot of the mysteries
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that remain about the
atmosphere and the clouds.
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There's a lot we don't
know about what the clouds
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are made out of, what kind of
chemistry is going on there.
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There are gases we call the rare gases:
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neon, argon, krypton, xenon.
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Or the noble gases, and
they're called the noble gases
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because they don't react with other gases.
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On the periodic table, they're the column
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all the way on the right,
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and they don't react with anything.
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And because of that, they tend to record
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longterm aspects of a planet's history,
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because they haven't been
perturbed by chemistry.
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And in addition, there are
mysteries of the radiation,
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the way solar energy is
absorbed and deposited
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in the clouds and in the atmosphere
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that we would really like to understand,
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both to understand Venus,
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and also just to round
out our understanding
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of the way climate works on planets,
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which of course is very
important to us here on Earth,
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struggling with climate change.
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There are measurements we would love to do
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within the atmosphere of Venus
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that could tell us more about the origins
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and evolution of that planet.
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- [Narrator] The tough balloons
will last for many months,
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their sensors alert for
low-frequency, infrasonic waves.
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- Is Venus volcanically active?
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Does Venus have plate recycling today?
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Those are geophysics questions
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that could be answered through seismology,
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which we can do from balloon,
potentially, by measuring.
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This is wonderful, taking
advantage of the fact
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that the Venus' atmosphere is so thick
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that sound waves from earthquakes
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will propagate up through the atmosphere
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and can be measured from
balloon or from orbit.
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It's astounding.
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- [Narrator] Each science buoy
makes a trip around the globe
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in about four Earth days.
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As they spread out, they
form a global network,
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performing standoff
seismology, meteorology,
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atmospheric chemistry,
and surface observations.
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But if these balloon probes
can collect all these data,
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why send people all the way to Venus?
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- Humans can do things
that robots can never do.
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That's just a fact.
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We can think on the fly, we have hands.
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The difficulty of putting
hands on another planet,
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it's extraordinary.
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And link them to a mind.
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So, we could ...
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with humans in the Venus
clouds or in orbit at Venus,
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make observations, it would
be a telescopic observations,
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measurements of chemistry,
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00:14:54,620 --> 00:14:58,260
or set up an observatory at
Venus to study the Venus clouds
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and changes that we
might expect to be coming
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from volcanic and seismic
activity at Venus.
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00:15:04,610 --> 00:15:09,610
So it's the Lando Calrissian
model, right? (laughing)
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The cloud society at Venus.
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We would get more data
by having people there.
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- Human beings are marvelously versatile,
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but human explorers are a
lot harder to keep alive
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in the atmosphere of Venus.
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They need oxygen, they
need food, they need sleep.
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So I'd love to see human explorers
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go to the atmosphere of Venus.
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I'd love to see human explorers
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that could operate via tele-robotics
250
00:15:43,900 --> 00:15:46,160
some of our high-temperature systems
251
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on the surface of Venus,
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so that the humans would
be in the atmosphere,
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but they're controlling by virtual reality
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a system that's on the surface of Venus.
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I thought it would be a
pretty advanced mission.
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That's not something that we're
quite ready to do quite yet.
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(driving electronic music)
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- [Narrator] Success of such missions
259
00:16:07,840 --> 00:16:10,050
will depend on the people who fly them.
260
00:16:11,140 --> 00:16:14,460
No matter how comfortable the
cloud community dwellings,
261
00:16:14,460 --> 00:16:17,920
scientists and engineers
may only agree to work there
262
00:16:17,920 --> 00:16:20,720
if there is a guarantee
of return to Earth.
263
00:16:21,756 --> 00:16:24,506
(rocket roaring)
264
00:16:33,023 --> 00:16:36,613
(curious electronic music)
265
00:16:43,840 --> 00:16:46,660
Habitats in the clouds require energy.
266
00:16:47,890 --> 00:16:50,660
One way to get it is to troll for power:
267
00:16:52,750 --> 00:16:57,290
extend a strong cable from the
cold altitude of the dwelling
268
00:16:58,380 --> 00:17:01,220
down into the hot depths
of the atmosphere.
269
00:17:03,010 --> 00:17:05,200
But don't let it touch the ground.
270
00:17:07,570 --> 00:17:10,060
The difference in temperature
between the cable's top
271
00:17:10,060 --> 00:17:13,240
and bottom can generate electricity,
272
00:17:13,240 --> 00:17:16,340
employing what's known
as the Seebeck Effect.
273
00:17:19,070 --> 00:17:21,880
It's an electro thermodynamic device
274
00:17:21,880 --> 00:17:23,920
that needs no moving parts.
275
00:17:23,919 --> 00:17:26,499
(soft orchestral music)
276
00:17:26,500 --> 00:17:29,360
But there may be an even simpler solution,
277
00:17:29,360 --> 00:17:32,320
one that puts no drag
on the floating station.
278
00:17:33,990 --> 00:17:35,950
- As you get higher and higher,
279
00:17:35,950 --> 00:17:38,570
as you get above the
thickest of the cloud decks
280
00:17:38,570 --> 00:17:41,330
at about 50 kilometers above the surface,
281
00:17:41,330 --> 00:17:44,550
once you get above the cloud
decks, it gets very sunny.
282
00:17:44,550 --> 00:17:46,940
It's actually sunnier than the Earth.
283
00:17:46,940 --> 00:17:51,180
It's not ferociously hot,
because there's still some amount
284
00:17:51,180 --> 00:17:54,150
of the high cloud that diffuses
the light a little bit,
285
00:17:54,150 --> 00:17:56,050
but there's plenty of solar energy.
286
00:17:56,050 --> 00:17:59,770
So I picture the habitats that could float
287
00:17:59,770 --> 00:18:03,000
in the area above the
thick clouds of Venus,
288
00:18:03,000 --> 00:18:04,830
probably as being solar powered.
289
00:18:04,830 --> 00:18:07,830
There's plenty of sunlight,
the temperature is nice.
290
00:18:07,830 --> 00:18:11,810
Why not pop out your solar
panels and run on the sun?
291
00:18:11,810 --> 00:18:13,260
It should work.
292
00:18:13,255 --> 00:18:14,875
(bright orchestral music)
293
00:18:14,880 --> 00:18:17,700
- [Narrator] Solar power on
Earth depends on batteries
294
00:18:17,700 --> 00:18:19,690
to store the energy after sunset.
295
00:18:21,470 --> 00:18:24,500
But nighttime on Venus is much longer.
296
00:18:26,030 --> 00:18:29,750
- The surface of Venus rotates
very slow and backwards,
297
00:18:29,750 --> 00:18:31,640
so if you were on the surface,
298
00:18:31,640 --> 00:18:34,890
the day-night cycle would
be hundreds of days.
299
00:18:34,890 --> 00:18:37,400
But once you get above the surface,
300
00:18:37,400 --> 00:18:40,250
what happens is the clouds
301
00:18:40,250 --> 00:18:42,290
whip around the planet very quickly.
302
00:18:43,280 --> 00:18:47,930
So there's a phenomenon called
atmospheric superrotation.
303
00:18:47,930 --> 00:18:50,500
That means that the
atmosphere actually rotates
304
00:18:50,500 --> 00:18:51,770
faster than the planet.
305
00:18:52,810 --> 00:18:56,950
So at the Earth-like level,
at about 50 to 60 kilometers,
306
00:18:56,950 --> 00:19:01,070
it takes about four days for
the winds to circle the planet.
307
00:19:01,070 --> 00:19:04,980
So if you were floating in
a balloon or in a habitat
308
00:19:04,980 --> 00:19:07,850
that was just stationary
and following the winds,
309
00:19:07,850 --> 00:19:12,070
you'd see about two
Earth days of sunlight,
310
00:19:12,070 --> 00:19:15,460
and then you'd have about
two Earth days of nighttime.
311
00:19:15,460 --> 00:19:18,130
So when you're talking
about power for the habitat,
312
00:19:18,130 --> 00:19:21,410
of course, you would
have to provide for power
313
00:19:21,410 --> 00:19:23,640
for the nighttime, and your nighttime's
314
00:19:23,640 --> 00:19:27,550
going to be about two Earth
days, but that's not impossible.
315
00:19:27,550 --> 00:19:30,600
You could imagine being
solar-powered during the day
316
00:19:30,600 --> 00:19:32,740
and then having enough energy storage
317
00:19:32,740 --> 00:19:35,510
to keep on living and working
318
00:19:35,510 --> 00:19:36,820
and doing whatever you're doing
319
00:19:36,820 --> 00:19:39,220
for your human habitats
during the nighttime.
320
00:19:44,164 --> 00:19:46,584
(soft music)
321
00:19:48,160 --> 00:19:50,170
- [Narrator] Like the
International Space Station,
322
00:19:50,170 --> 00:19:52,540
a modest-sized floating field station
323
00:19:52,540 --> 00:19:54,870
could support a small group of researchers
324
00:19:54,870 --> 00:19:57,100
for deployments lasting several months.
325
00:19:59,090 --> 00:20:03,100
But, using the same materials
and construction techniques,
326
00:20:03,100 --> 00:20:04,960
there's practically no limit
327
00:20:04,960 --> 00:20:07,730
to how big these
structures could be built.
328
00:20:07,726 --> 00:20:09,306
(impressive brass music)
329
00:20:09,310 --> 00:20:12,390
Many could cluster together
to support a relatively large
330
00:20:12,390 --> 00:20:15,420
group of astronauts over
much longer periods.
331
00:20:16,650 --> 00:20:19,330
- I picture the idea of these habitats
332
00:20:19,330 --> 00:20:23,320
as being the size of
cities, kilometers in scale.
333
00:20:23,320 --> 00:20:25,650
So I sort of love the idea, and of course,
334
00:20:25,650 --> 00:20:29,890
once you put in one city
in the atmosphere of Venus,
335
00:20:29,890 --> 00:20:33,930
why not more, why not 10, why
not a 100, why not 10,000?
336
00:20:33,930 --> 00:20:35,580
There's a lot of Venus out there.
337
00:20:38,500 --> 00:20:41,300
- [Narrator] But how safe
are these structures?
338
00:20:42,720 --> 00:20:45,200
- Well, the nice thing about the balloons
339
00:20:45,200 --> 00:20:48,720
in the atmosphere of Venus,
if they're very, very large,
340
00:20:48,720 --> 00:20:51,290
is that they'd be running
with the inside pressure
341
00:20:51,290 --> 00:20:54,010
about the same as the outside pressure.
342
00:20:54,010 --> 00:20:56,760
So it wouldn't be like a space habitat,
343
00:20:56,760 --> 00:20:59,860
say an O'Neill habitat in Earth orbit,
344
00:20:59,860 --> 00:21:01,350
where if you puncture a hole in it,
345
00:21:01,350 --> 00:21:03,680
you get an explosive decompression
346
00:21:03,680 --> 00:21:05,900
and all of the air rushes out.
347
00:21:05,900 --> 00:21:07,270
You'd have the outside air
348
00:21:07,270 --> 00:21:10,010
is about the same pressure
as the inside air.
349
00:21:10,010 --> 00:21:12,130
There'd be some exchange of gases.
350
00:21:12,130 --> 00:21:15,500
You wouldn't want that, but it
wouldn't burst like a balloon
351
00:21:15,500 --> 00:21:17,580
in a catastrophic failure.
352
00:21:17,580 --> 00:21:18,930
When you have something this big,
353
00:21:18,930 --> 00:21:22,770
it takes a very, very
long time to decompress.
354
00:21:22,770 --> 00:21:24,750
If you pop a balloon that's this big,
355
00:21:24,750 --> 00:21:26,240
it's over in an instant,
356
00:21:26,240 --> 00:21:28,160
but when you put a hole in a balloon
357
00:21:28,160 --> 00:21:30,350
that's hundreds of meters across,
358
00:21:30,350 --> 00:21:32,970
it takes a long time to deflate.
359
00:21:32,970 --> 00:21:35,320
And something that's
thousands of meters across,
360
00:21:35,320 --> 00:21:37,710
a city, would take days and days
361
00:21:37,710 --> 00:21:39,770
to lose very much atmosphere.
362
00:21:39,770 --> 00:21:40,980
Nevertheless, of course,
363
00:21:40,980 --> 00:21:42,620
I think you'd want to work very hard
364
00:21:42,620 --> 00:21:45,300
to make sure that you
don't get those punctures
365
00:21:45,300 --> 00:21:47,650
and you'd make sure that you have multiple
366
00:21:47,650 --> 00:21:50,730
lifting gas areas, so
that even if you did,
367
00:21:50,730 --> 00:21:53,070
for one reason or another, have a failure
368
00:21:53,070 --> 00:21:56,670
that made one part of
the city lose atmosphere,
369
00:21:56,673 --> 00:21:59,923
the rest of it would have enough
lifting gas to hold you up.
370
00:22:03,290 --> 00:22:06,530
- [Narrator] These are
large, complex assemblies.
371
00:22:06,530 --> 00:22:09,080
Fortunately, very little of their mass
372
00:22:09,080 --> 00:22:11,080
would have to be hauled here from Earth.
373
00:22:12,530 --> 00:22:15,110
- A lot of the materials
374
00:22:15,110 --> 00:22:17,190
that you could use to build a habitat,
375
00:22:17,190 --> 00:22:21,130
you might be able to make just
from the atmosphere of Venus.
376
00:22:21,130 --> 00:22:23,920
It turns out that, in modern engineering,
377
00:22:23,920 --> 00:22:27,110
one of the most versatile,
one of the most useful,
378
00:22:27,110 --> 00:22:29,930
materials you can make is carbon fiber.
379
00:22:29,930 --> 00:22:34,000
Carbon fiber is strong. It's lightweight.
380
00:22:34,000 --> 00:22:36,370
You can do a lot with carbon fiber.
381
00:22:36,370 --> 00:22:39,110
But of course, to make a
whole city, you need more
382
00:22:39,110 --> 00:22:42,270
than just the structural
members of carbon fiber.
383
00:22:42,270 --> 00:22:45,020
So I expect that, if
we were making a city,
384
00:22:45,020 --> 00:22:47,510
or 10 cities, or 1,000 cities,
385
00:22:47,510 --> 00:22:50,140
we're probably going to have
to go down to the surface
386
00:22:50,140 --> 00:22:51,910
and grab up materials.
387
00:22:51,910 --> 00:22:55,130
So, you will be mining
the surface of Venus
388
00:22:55,130 --> 00:22:56,850
to bring up other materials
389
00:22:56,850 --> 00:23:00,080
like the silicon and the silicate rocks
390
00:23:00,080 --> 00:23:01,870
and the lesser materials.
391
00:23:01,870 --> 00:23:04,810
There's a lot you can get
out of the atmosphere,
392
00:23:04,810 --> 00:23:06,710
but not everything of course.
393
00:23:06,710 --> 00:23:10,310
What you want to avoid
doing as much as possible
394
00:23:10,310 --> 00:23:11,890
is you want to try to avoid
395
00:23:11,890 --> 00:23:14,340
bringing things all the way from Earth,
396
00:23:14,340 --> 00:23:16,300
because the key to living
in the solar system
397
00:23:16,300 --> 00:23:20,610
is learning to use the materials
that you can find on-hand.
398
00:23:20,610 --> 00:23:23,540
Bringing things up from
Earth as a camping trip,
399
00:23:23,540 --> 00:23:25,700
but we don't want to just go camping.
400
00:23:25,700 --> 00:23:27,960
We want to live in the solar system.
401
00:23:27,957 --> 00:23:31,367
(light orchestral music)
402
00:23:34,430 --> 00:23:35,850
- [Narrator] What began with a few
403
00:23:35,850 --> 00:23:37,820
science outposts and airships
404
00:23:38,960 --> 00:23:42,840
could expand into a far
flung, interconnected network
405
00:23:42,840 --> 00:23:45,000
of communities beyond Earth.
406
00:23:48,744 --> 00:23:52,454
(gentle percussive music)
407
00:23:52,450 --> 00:23:56,060
The old romantic vision of
self-sustaining space settlements
408
00:23:56,060 --> 00:23:58,330
could come alive in the orbit of Venus.
409
00:23:59,430 --> 00:24:02,040
Habitats many kilometers in size
410
00:24:02,040 --> 00:24:04,020
can be constructed from materials
411
00:24:04,020 --> 00:24:07,210
mined from the atmosphere or asteroids,
412
00:24:07,210 --> 00:24:11,280
and they'd be powered by free
energy from the nearby sun.
413
00:24:12,290 --> 00:24:15,680
These utopian structures could rotate
414
00:24:15,680 --> 00:24:18,640
to provide comfortable
gravity and pleasant weather.
415
00:24:20,420 --> 00:24:22,920
Large ships could dock there,
416
00:24:22,920 --> 00:24:26,570
bringing cargo to be distributed
down the gravity well
417
00:24:26,570 --> 00:24:29,220
to the floating towns
in Venus's atmosphere.
418
00:24:30,640 --> 00:24:33,470
But the builders of such a
city will have to wrestle
419
00:24:33,470 --> 00:24:36,460
with one inevitable design constraint:
420
00:24:36,460 --> 00:24:38,960
most of the mass must be allocated
421
00:24:38,960 --> 00:24:42,030
to sheltering the
residents from radiation.
422
00:24:43,470 --> 00:24:46,910
- If we had a colony at the
launch points, for example,
423
00:24:46,913 --> 00:24:48,653
we'd probably have to shield them
424
00:24:48,650 --> 00:24:52,450
with many meters of regolith, of dirt.
425
00:24:52,450 --> 00:24:55,200
Well, that's okay. We can
mind dirt from the moon.
426
00:24:55,200 --> 00:24:56,770
The moon's got plenty of dirt.
427
00:24:56,770 --> 00:24:59,070
But that's a lot of
stuff you have to bring
428
00:24:59,070 --> 00:25:02,480
for no other purpose than hiding away
429
00:25:02,480 --> 00:25:04,880
from the particles
coming away from the sun,
430
00:25:04,880 --> 00:25:08,100
galactic cosmic rays
coming in from outer space.
431
00:25:09,710 --> 00:25:11,620
- [Narrator] On the other
hand, the cloud dwellers
432
00:25:11,620 --> 00:25:13,830
would be safely tucked
into the atmosphere.
433
00:25:15,050 --> 00:25:19,060
- Venus does not have a magnetic
field to deflect particles,
434
00:25:19,060 --> 00:25:21,950
but it still does have an atmosphere.
435
00:25:21,950 --> 00:25:24,780
So at the level of the
middle cloud deck of Venus
436
00:25:24,780 --> 00:25:26,410
and a little bit above,
437
00:25:26,410 --> 00:25:29,070
we're still talking
about a lot of atmosphere
438
00:25:29,070 --> 00:25:30,750
between you and space.
439
00:25:30,750 --> 00:25:33,790
So the good thing is that
we have enough atmosphere
440
00:25:33,790 --> 00:25:36,770
to attenuate the worst of the radiation.
441
00:25:36,770 --> 00:25:39,080
We're not getting the protons
442
00:25:39,080 --> 00:25:42,490
from the solar flare
coronal mass ejections
443
00:25:42,490 --> 00:25:44,650
that would be very, very dangerous,
444
00:25:44,650 --> 00:25:47,810
maybe very deadly for
an unprotected human.
445
00:25:47,810 --> 00:25:52,020
We get the 10 tons of
atmosphere per square meter
446
00:25:52,020 --> 00:25:54,620
shielding us from the radiation.
447
00:25:54,620 --> 00:25:56,400
Another reason that the clouds of Venus
448
00:25:56,400 --> 00:25:58,600
are a nice place to colonize.
449
00:25:58,597 --> 00:26:01,597
(atmospheric music)
450
00:26:04,800 --> 00:26:07,890
- [Narrator] Venus has nearly
the same gravity as Earth.
451
00:26:09,120 --> 00:26:13,420
While it has much more land
area, it has no oceans.
452
00:26:16,220 --> 00:26:20,130
What would it take to make
the entire planet livable,
453
00:26:20,130 --> 00:26:21,790
to terraform it?
454
00:26:23,320 --> 00:26:26,490
We would have to re-water the whole world.
455
00:26:30,977 --> 00:26:34,667
(atmospheric electronic music)
456
00:26:34,670 --> 00:26:38,290
In the early solar system,
the second planet, Venus,
457
00:26:38,290 --> 00:26:41,270
may have been the most hospitable of all,
458
00:26:41,270 --> 00:26:43,240
but as the sun brightened,
459
00:26:43,240 --> 00:26:45,850
Venus struggled to hold on to its oceans.
460
00:26:48,360 --> 00:26:52,480
Carbon dioxide and methane
from volcanoes trapped heat,
461
00:26:53,760 --> 00:26:55,820
evaporating the seas.
462
00:26:55,822 --> 00:26:58,462
(steam hissing)
463
00:26:58,459 --> 00:27:01,129
(uncanny music)
464
00:27:02,930 --> 00:27:06,800
Atmospheric water vapor
became a greenhouse gas,
465
00:27:06,800 --> 00:27:10,870
holding even more energy from
the sun and the planet below.
466
00:27:12,880 --> 00:27:14,440
- Four and a half billion years ago,
467
00:27:14,440 --> 00:27:17,270
Earth's atmosphere was also CO2-rich.
468
00:27:17,270 --> 00:27:22,270
That is, the original atmosphere
of the terrestrial planets.
469
00:27:22,420 --> 00:27:26,020
Venus has a very thick carbon
dioxide atmosphere today.
470
00:27:26,020 --> 00:27:31,020
And we would, too, if you took
all of the carbonate rocks,
471
00:27:31,770 --> 00:27:34,820
the rocks that hold carbon,
took all the limestone on Earth,
472
00:27:34,820 --> 00:27:39,040
took Florida, evaporated
it back into the sky.
473
00:27:39,040 --> 00:27:40,920
All that carbon dioxide
474
00:27:40,920 --> 00:27:43,860
would be about the equivalent
of the carbon dioxide
475
00:27:43,860 --> 00:27:46,190
that's in the Venus atmosphere right now.
476
00:27:50,490 --> 00:27:53,200
- Venus is really off
the scale in a sense.
477
00:27:53,200 --> 00:27:55,480
For us to load our atmosphere
478
00:27:55,480 --> 00:27:58,630
with the amount of CO2
that's in Venus's atmosphere
479
00:27:58,630 --> 00:28:01,840
would require us to free
up all the carbonate rocks
480
00:28:01,840 --> 00:28:04,250
on our world and get all that carbon
481
00:28:04,250 --> 00:28:05,240
into the atmosphere.
482
00:28:05,240 --> 00:28:07,710
And that would take hundreds and hundreds
483
00:28:07,710 --> 00:28:08,760
of millions of years.
484
00:28:11,390 --> 00:28:12,950
- [Narrator] Space visionaries today
485
00:28:12,950 --> 00:28:15,620
are looking to advanced technologies
486
00:28:15,620 --> 00:28:18,730
to send Venus back in a
more Earth-like direction.
487
00:28:20,000 --> 00:28:21,690
- You would have to,
obviously, do something
488
00:28:21,690 --> 00:28:24,720
about the very, very
strong greenhouse effect.
489
00:28:24,720 --> 00:28:27,780
Maybe you would do that
by putting aerosols
490
00:28:27,780 --> 00:28:28,720
into the atmosphere,
491
00:28:28,720 --> 00:28:30,900
filling the atmosphere with dust
492
00:28:30,900 --> 00:28:33,270
long enough to collapse that greenhouse
493
00:28:33,270 --> 00:28:37,110
and get that CO2 to
condense out on the surface.
494
00:28:37,110 --> 00:28:39,890
And then you'd have to find
some way to keep it condensed,
495
00:28:39,890 --> 00:28:42,550
maybe with, now we're getting
science fictional here,
496
00:28:42,550 --> 00:28:44,410
but maybe with orbiting
mirrors or something
497
00:28:44,410 --> 00:28:46,440
to cut down on that solar radiation.
498
00:28:49,210 --> 00:28:51,210
- [Narrator] British scientist Paul Birch
499
00:28:51,210 --> 00:28:54,580
proposed transporting
trillions of tons of hydrogen
500
00:28:54,580 --> 00:28:56,540
from gas planets such as Jupiter.
501
00:28:59,170 --> 00:29:04,010
The idea is to convert atmospheric
CO2 into oceans of water,
502
00:29:04,010 --> 00:29:05,810
plus mountains of graphite.
503
00:29:10,210 --> 00:29:14,130
Birch also suggested shielding
Venus from the sun's heat
504
00:29:14,130 --> 00:29:16,250
with enormous, thin panels ...
505
00:29:18,290 --> 00:29:22,220
to cool the atmosphere,
shrink its volume ...
506
00:29:23,210 --> 00:29:24,900
and lower its pressure.
507
00:29:24,896 --> 00:29:27,556
(uncanny music)
508
00:29:29,820 --> 00:29:33,700
These giant screens would
convert solar energy
509
00:29:33,700 --> 00:29:36,560
to power other terraforming operations ...
510
00:29:38,430 --> 00:29:41,650
like capturing carbon and
sealing it underground.
511
00:29:46,520 --> 00:29:48,700
Nobel Prize winner Paul Crutzen
512
00:29:48,700 --> 00:29:51,950
proposed injecting sulfur
dioxide into the air
513
00:29:51,950 --> 00:29:55,350
to simulate the dark smoke
of gargantuan volcanoes
514
00:29:55,350 --> 00:29:58,090
to cool the surface and
tame the greenhouse.
515
00:30:01,900 --> 00:30:03,690
David Grinspoon and Mark Bullock
516
00:30:03,690 --> 00:30:07,170
suggest that exposing
native calcium and magnesium
517
00:30:07,166 --> 00:30:10,156
could pull carbon down
into carbonate rocks.
518
00:30:10,158 --> 00:30:12,828
(uncanny music)
519
00:30:18,387 --> 00:30:21,567
But where to find a whole
planet's worth of water?
520
00:30:23,800 --> 00:30:27,090
- Fortunately, I suppose,
if this was your goal,
521
00:30:27,090 --> 00:30:30,230
there's a lot of stray icy
objects in the solar system,
522
00:30:30,230 --> 00:30:32,690
the whole outer solar
system, the Kuiper Belt,
523
00:30:32,690 --> 00:30:36,380
is loaded with icy objects and
would not miss a few of them.
524
00:30:36,380 --> 00:30:39,160
There are literally trillions
of icy objects out there.
525
00:30:39,160 --> 00:30:41,650
So if you're imagining some far future
526
00:30:41,650 --> 00:30:43,610
where somebody's got the technical prowess
527
00:30:43,610 --> 00:30:45,430
and the will to do this,
528
00:30:45,430 --> 00:30:47,640
I would take some of
these large, icy objects,
529
00:30:47,640 --> 00:30:50,020
some large number of them
and crash them into Venus,
530
00:30:50,020 --> 00:30:54,120
which would both raise the
dust to collapse the greenhouse
531
00:30:54,120 --> 00:30:58,840
and would return Venus to
a more watery condition.
532
00:30:58,840 --> 00:31:01,370
This is not a near-term
project. (chuckles)
533
00:31:01,373 --> 00:31:04,713
(frenetic string music)
534
00:31:06,250 --> 00:31:08,730
- [Narrator] To put icy
objects on a collision course
535
00:31:08,730 --> 00:31:12,330
with Venus takes delicate
orbital mechanics,
536
00:31:13,360 --> 00:31:17,010
a slow-motion ballet of many small robots
537
00:31:17,010 --> 00:31:20,110
with the collective power
to move mega mountains.
538
00:31:28,480 --> 00:31:30,610
The swarm distributes itself
539
00:31:30,610 --> 00:31:34,020
according to the unique gravity
map of the chosen object.
540
00:31:40,510 --> 00:31:43,560
Choreographed clusters of thruster firings
541
00:31:43,560 --> 00:31:46,470
nudge each massive ice world inbound
542
00:31:46,470 --> 00:31:48,550
onto its own safe trajectory.
543
00:31:57,900 --> 00:32:01,160
The bots may process
their captured objects,
544
00:32:01,160 --> 00:32:04,140
separating out water and extracting metals
545
00:32:04,140 --> 00:32:06,960
during their long journey
to the inner solar system.
546
00:32:08,820 --> 00:32:12,350
The icy bodies may change
shape as materials are mined.
547
00:32:14,600 --> 00:32:16,420
These intelligent machines
548
00:32:16,420 --> 00:32:19,010
might also make clones of themselves
549
00:32:19,010 --> 00:32:22,320
to scale up the operation
and get it done faster.
550
00:32:25,978 --> 00:32:28,148
(booming)
551
00:32:29,480 --> 00:32:31,910
When the processed icy asteroids arrive,
552
00:32:31,910 --> 00:32:35,660
they'll be delicately
maneuvered into impact speeds
553
00:32:35,660 --> 00:32:37,520
that preserve the most water.
554
00:32:39,050 --> 00:32:41,300
(rumbling)
555
00:32:44,060 --> 00:32:47,270
Dust from the crashes
should cut down sunlight,
556
00:32:47,270 --> 00:32:48,370
cooling it quicker.
557
00:32:51,150 --> 00:32:55,970
But smack the planet too hard,
and you may unleash hell.
558
00:32:58,690 --> 00:33:01,220
Count on Venus to fight back.
559
00:33:01,220 --> 00:33:04,320
With a thicker crust
and no plate tectonics,
560
00:33:04,320 --> 00:33:07,860
Venus doesn't vent its internal
heat as easily as Earth.
561
00:33:08,820 --> 00:33:10,050
It builds up.
562
00:33:13,810 --> 00:33:18,210
This world has erupted and
repaved its entire surface
563
00:33:18,210 --> 00:33:20,860
at least once in its history
564
00:33:20,862 --> 00:33:23,362
(tense music)
565
00:33:30,470 --> 00:33:33,050
(gentle music)
566
00:33:34,690 --> 00:33:37,110
To remodel an entire planet
567
00:33:37,110 --> 00:33:39,470
seems like the ultimate act of hubris,
568
00:33:40,890 --> 00:33:42,620
but we're already doing it.
569
00:33:45,000 --> 00:33:47,760
- Could we ever terraform
Venus and go live on it?
570
00:33:47,760 --> 00:33:49,420
Well, our more immediate task
571
00:33:49,420 --> 00:33:52,780
is to avoid veneraforming Earth right now.
572
00:33:52,780 --> 00:33:54,610
That is, to not turn Earth into Venus
573
00:33:54,610 --> 00:33:56,960
by increasing the greenhouse effect.
574
00:33:56,960 --> 00:33:59,180
So I don't advocate immediately going
575
00:33:59,180 --> 00:34:01,810
and trying to live on Venus or Mars
576
00:34:01,810 --> 00:34:04,260
and trying to terraform them
577
00:34:04,262 --> 00:34:06,232
to escape from our problems here.
578
00:34:06,230 --> 00:34:08,850
However, the mental exercise of imagining
579
00:34:08,850 --> 00:34:11,420
how we would terraform another planet,
580
00:34:11,420 --> 00:34:13,550
I think, is very valuable for our task
581
00:34:13,550 --> 00:34:17,110
of learning how to manage
ourselves on Earth better,
582
00:34:17,110 --> 00:34:18,980
because it forces us to ask,
583
00:34:18,980 --> 00:34:22,440
how would we interact
constructively with the planet?
584
00:34:22,440 --> 00:34:25,780
How would we intentionally
alter a planet's climate
585
00:34:25,780 --> 00:34:27,410
and manage a planet's climate
586
00:34:27,410 --> 00:34:30,550
as opposed to unintentionally
and inadvertently
587
00:34:30,550 --> 00:34:32,630
messing with a planet's climate
588
00:34:32,630 --> 00:34:34,590
as we've been doing here on Earth?
589
00:34:35,860 --> 00:34:40,160
- I think actually learning
to live in the solar system
590
00:34:40,160 --> 00:34:44,020
is going to teach us ways
to help us live on Earth.
591
00:34:44,020 --> 00:34:46,820
What we call pollution on the Earth,
592
00:34:46,820 --> 00:34:49,910
on the moon we'd call
that valuable resources.
593
00:34:49,910 --> 00:34:51,770
That's gonna help us live on Earth,
594
00:34:51,770 --> 00:34:55,510
just understanding that an
ecosystem is a closed cycle.
595
00:34:55,510 --> 00:34:57,990
There is no such thing as waste.
596
00:34:57,990 --> 00:35:00,940
All of the waste has to
be recycled and come back.
597
00:35:04,700 --> 00:35:06,370
- [Narrator] On the other hand,
598
00:35:06,370 --> 00:35:09,420
learning the techniques
to better manage Earth
599
00:35:09,420 --> 00:35:11,050
might just give us the tools
600
00:35:11,050 --> 00:35:15,220
to tackle living on or
around other worlds.
601
00:35:17,090 --> 00:35:22,090
It might take decades,
centuries, millennia ...
602
00:35:23,080 --> 00:35:25,890
but our distant descendants
may well be born
603
00:35:25,890 --> 00:35:29,700
into a solar system with more
than one place to call home.
604
00:35:33,460 --> 00:35:36,520
Some may be in the clouds of atmospheres.
605
00:35:36,515 --> 00:35:39,425
(soft piano music)
606
00:35:43,950 --> 00:35:45,650
Some may orbit freely.
607
00:35:53,690 --> 00:35:56,950
Still others might live
on the surfaces of worlds.
608
00:36:00,224 --> 00:36:02,854
- I think we should move
out into the solar system,
609
00:36:02,850 --> 00:36:05,910
and I really want to go everywhere.
610
00:36:05,910 --> 00:36:10,910
I want to put human beings
at the poles of Mercury.
611
00:36:11,000 --> 00:36:13,350
I want to go to Venus.
I want to go to Mars.
612
00:36:13,350 --> 00:36:15,340
I think we should go into
the outer solar system
613
00:36:15,340 --> 00:36:18,490
and start looking at some of the resources
614
00:36:18,490 --> 00:36:19,710
of the Kuiper belt.
615
00:36:20,580 --> 00:36:23,150
I think human beings can, and we should,
616
00:36:23,150 --> 00:36:24,780
settle the whole solar system,
617
00:36:32,540 --> 00:36:35,190
- [Narrator] As it was when
the planets first formed,
618
00:36:37,470 --> 00:36:42,010
Earth's twin made
beckoned us to its shores.
619
00:36:43,243 --> 00:36:46,913
(building orchestral music)
620
00:36:55,352 --> 00:36:59,352
(intriguing instrumental music)
47078
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