Destiny In Space Page #2
- Year:
- 1994
- 40 min
- 129 Views
orbiter and the satellite ...
the crew learned that they
could tighten it once again ...
showing that we can
control tethers in space.
Tether's under control.
Unexpected snags
are bound to arise.
But we learn from them
and keep moving forward.
To build more reliable spacecraft,
we need light but tough materials.
To test them, in 1984
with dozens of materials
attached to its surface ...
exposing them to the
wear and tear of space.
Columbia, Houston.
We have a tally-ho on LDEF.
We left it in orbit for six years,
long enough for an interplanetary trip.
Ready to go get it?
and took it back to Earth.
We found a wealth of information
embedded in these panels.
Splatters.
As the microscopes reveal ...
the vacuum of space
is anything but empty.
This pattern, I don't
know what this is.
A continuous bombardment
of micrometeorites ...
pitted the surfaces with craters.
But the most serious hazard
in space is radiation.
As the shuttle hangs suspended
above the Earth's horizon ...
we see only the lights of
its cargo bay in the darkness.
But we can't see the harmful cosmic
radiation that is everywhere here.
High-energy charged particles ...
are streaming out from
the Sun and other stars.
On Earth, we are protected
by the atmosphere ...
and the surrounding
magnetic field.
In space, the radiation can
penetrate the walls of our craft.
A Japanese x-ray satellite reveals
erupting from the Sun.
On interplanetary trips ...
we'll have to retreat to
heavily shielded onboard shelters ...
whenever solar storms are sighted.
Most of the planets are too
hostile for people to visit.
But that doesn't stop us
from exploring them.
Okay, understand. We have a go
for deploy, so we're starting out.
Five, four, three ...
two, one, mark.
- Do we have motion?
- I see motion.
It's stable? It's clear of the ASE.
Where humans cannot safely go ...
we send remotely controlled
robot explorers.
Commanding them from Earth ...
we use their electronic eyes and sensors
to explore the alien landscape.
In 1989, the Galileo spacecraft ...
began a five-year journey to Jupiter ...
the largest planet
in our solar system.
Galileo just kind of dissolves
out into nothingness ...
as it goes into the
darkness of space.
And that's the last we saw of it.
sent back to Earth in 1979 ...
by two robot probes named Voyager.
This was our first opportunity
to marvel at its Great Red Spot ...
three times the size of Earth.
The molecular building
blocks for life ...
may be swirling within Jupiter's
turbulent atmosphere.
If Galileo's probe confirms this ...
we should gain new insights
into the origins of life.
Though it is our nearest planetary
neighbor, Venus was always a mystery.
our view of its surface.
Then we sent a spacecraft
named Magellan to orbit the planet.
through the clouds.
Magellan collected so much data ...
that we can now explore the surface
as if we were actually there.
We begin 60,000 feet up.
To help scientists
recognize its features ...
a computer has exaggerated the
height of the terrain 10 times.
Perhaps these pancake domes ...
were caused by lava pushing through
weak spots in the surface.
These craters, some the
size of Connecticut ...
were made by collisions
with comets and asteroids.
On Earth, ancient craters like these
have been eroded by wind and water.
But there is little
wind and no water here.
Venus swelters beneath a thick
atmosphere of carbon dioxide ...
which acts like a greenhouse:
It allows sunlight to filter in,
but then traps the heat inside.
The surface temperature
is hot enough to melt lead.
In the distance, the great
Gula Mons volcano.
We are now soaring more than
The long, smooth strips
that now and then cross our path ...
are small portions of the surface
that Magellan's radar did not scan.
The Magellan craft has shown us the
fantastic surface of an alien planet ...
where no human could
ever hope to land.
But there is another world in our
solar system that people can visit.
Future generations of explorers
will walk upon Mars.
Do you know what that is?
To prepare the way for them,
we could send a robot like this ...
We might dispatch a whole flock of
these helpers to explore the terrain.
Unlike us, they are almost
immune to radiation ...
and need no air or water.
And they never get homesick.
Robots like this
Russian Mars rover ...
being tested in
Death Valley, California ...
have already been programmed
like negotiating rugged terrain.
help us construct a Mars base.
But operating them
will be a challenge.
At the speed of light,
takes up to 20 minutes to
travel from Earth to Mars.
If there is or ever has been life
somewhere else in the solar system ...
Mars is a good place
to look for traces.
open the Martian plain.
It is as long as the
entire United States.
We are now descending
from 40,000 feet ...
into a part of the valley
known as Candor Chasma.
the Earth's Grand Canyon.
The height of the terrain
has not been exaggerated.
This is how it really looks.
Life as we know it must
Water may have flowed
through these canyons long ago.
Perhaps it nourished life.
Fossil life forms may lie exposed
on the floor of these canyons.
If we find any, it would
that life has existed beyond Earth.
It would mean that life
probably is abundant in our galaxy ...
and awaiting discovery
in the universe beyond.
Today, Mars is a frozen world.
The average temperature here is
lower than at the Earth's South Pole.
But long ago, when water
may have flowed here ...
it must have been warmer.
We don't know
why Mars turned so cold ...
to change once again.
Could future generations
somehow transform Mars ...
into an Earth-like world
To do it, we might imagine some-
how raising the temperature ...
to build up the atmosphere
and melt the ice caps.
This would create
lakes and rivers.
Then we could introduce plants
to fill the air with oxygen.
Animals and people
could now breathe the air.
for us to colonize.
What would life be like on Mars?
Perhaps we could
build farms and cities.
Or perhaps we will leave
Mars as we found it.
Those decisions will be
made by our descendants.
If terraforming is even possible,
it would take thousands of years.
By then, we may have
Though it would take about 100,000 years
to reach them with present technology ...
future generations
may travel faster.
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