Nova (1974–…): Season 40, Episode 6 - Earth from Space - full transcript
EARTH FROM SPACE is a groundbreaking two-hour special that reveals a spectacular new space-based vision of our planet.
NARRATOR:
Our planet: Earth.
You may think you know it well.
But a startling new picture
is emerging
of a world shaped by forces
more dynamic and intertwined
than we ever imagined,
raising possibilities
that defy common sense.
How can sandstorms
in the Sahara Desert
transform the Amazon rainforest
over 5,000 miles away?
In the frigid ocean
beneath Antarctica,
how can a vast
undersea waterfall
500 times bigger
than Niagara Falls
lead to a gigantic
feeding frenzy near the equator?
And how can warm water streaming
past the coast of Africa
trigger a weather catastrophe
half a world away
in the southern United States?
Scientists have begun to find
surprising answers
to these and other
profound questions
thanks to a network
of satellites
orbiting high above the earth.
Ever watchful,
their senses extend far beyond
what our eyes can see.
EMILY SHUCKBURGH: It's really the
last bastion of human discovery.
We're discovering new things
every day.
NARRATOR: What are these hidden forces
that rule our world?
How are the oceans,
the continents, the atmosphere
and even the sun
bound together,
and how do they affect
all living things?
For the first time,
we can understand
how earth, fire, wind and water
join together
to create the dynamic
environments
that shape life
in all its forms.
WALEED ABDALATI:
Their interaction
is what has created
the environment, the diversity,
the kind of life
we see on earth today.
NARRATOR:
With astonishing images
created from a wealth of new
information from satellites,
this is our planet
as never seen before.
"Earth from Space,"
right now on NOVA.
♪ NOVA 40x11 ♪
Earth From Space
Original Air Date on February 13, 2013
== sync, corrected by elderman ==
Major funding for NOVA is
provided by the following:
NARRATOR: Since humans first ventured
into space,
some of the greatest gifts
of exploration
have been the new views
of our home.
Who can forget the iconic
"earthrise" images
of the Apollo era?
And now from the International
Space Station,
we have these spectacular
vistas.
The blue marble is finally
revealing its secrets.
It's a planet alive with
activity and constant change,
its surface transformed
by humans
yet still ruled by powerful
natural forces
that we are only beginning
to understand.
ABDALATI: It's just spectacular
when you view it from space.
It's teeming with diversity,
with beauty.
Amazing colors, you know,
the blues and the greens
and the whites.
PIERS SELLERS:
You see the world
as one huge system
all linked through
the atmosphere and the oceans,
rolling its way
around the sun.
NARRATOR: So what is it that shapes
Earth's dynamic face?
What are the essential
ingredients,
and how do they combine to
generate and sustain all life?
How do the natural forces
that surround us work together
to create an engine
powerful enough
to nourish and drive life
forward in all its diversity?
Our best hope for answers
may come from above.
Orbiting over our heads
are 120 satellites
keeping watch from space.
Most operate at altitudes
ranging from a few hundred miles
above the surface of the planet
to as high as 25,000 miles.
Each one of these
Earth-observing satellites
reveals a different piece
of the puzzle.
Each carries an array of
exquisitely sensitive detectors,
designed to reveal
what would otherwise
be hidden from our view.
The satellites are
absolutely amazing
because not only can we see
visible things from space,
but also we can see things that
aren't visible to the human eye.
So satellites are enabling us
to turn what are
invisible processes
into visible things we can see
and then understand.
NARRATOR: To see how our world works,
in this program
we have taken information
provided by satellites,
combined it with
computer models,
and rendered the results
in these scientifically
accurate graphics.
With the invisible
now revealed,
we can see Earth as
an endlessly changing system.
These images will show
in great detail
how sunlight, moisture,
land and atmosphere interact
in unexpected ways,
with seemingly local events
often triggered by forces
far away in space and time.
And with these new insights,
for the first time,
scientists can begin
to understand
the intimate relationship
between the planet
and all the living things
it supports.
ABDALATI:
It's really the thrill,
because it matters so much,
of piecing together the story
of what the earth is doing,
how it's changing,
why it's changing
and how ultimately
that affects humans.
NARRATOR:
The first piece of the puzzle
is in understanding
the massive influence the sun,
from 93 million miles away,
has on our planet.
The world's continuously bathed
in a flow of energy
from the sun.
That warms the earth.
Everything that you can see
that lives and breathes
and moves on the earth
is pushed by the sun.
NARRATOR:
Now an electronic eye in space
can measure the impact
of the sun's energy
all around the earth.
One of NASA's newest satellites,
named for a meteorologist,
polar-orbiting Suomi,
launched in 2011,
provides the view.
The spacecraft is the size
of a small school bus.
It orbits 500 miles up, circling
the planet 14 times a day.
On board, it carries
five separate sensors
that enable it to see things
invisible to human eyes.
The light that we can see
is confined to a narrow band
of electromagnetic radiation,
just a tiny portion of what
the satellite can pick up.
Electromagnetic radiation
spans a spectrum
that goes far beyond the
familiar colors of the rainbow.
ABDALATI: If you were to consider
the full spectrum to be a line
that stretched from New York
City to Los Angeles,
the piece that our eyes
could see
would be about
the size of a dime.
There is so much other
information out there
available to us,
and that's in large part
what these satellites do.
NARRATOR: One of this satellite's
key instruments is called CERES,
an acronym for Clouds and
Earth's Radiant Energy System.
It detects a broad range
of the spectrum,
including the very short and
very long wavelengths of light
in the ultraviolet and infrared
that we can't see.
This is a CERES-eye view
of the planet.
Anything that emits heat
gives off infrared radiation,
so the CERES data shows
the earth in shades of heat,
accurate to a fraction
of a degree.
It reveals how the planet
as a whole reacts to sunlight,
both absorbing and reflecting
the radiation
coming from our local star.
At the poles, the sun strikes
at an oblique angle,
and what little light there is
gets reflected back out to space
by the ice and clouds.
These are the primary reasons
why the poles remain cool.
At the equator,
it's a very different story.
Not only does the planet receive
more direct sunlight here,
the lack of ice means that
less of the sun's energy
is reflected back into space.
And at the equator,
the sun's concentrated energy
fuels a heat engine
that can trigger weather events
around the world.
Perhaps the best place to see
the impact of the sun's heat
is an area in the Atlantic
just north of the equator
and west of Africa:
the coastal waters
of the Cape Verde islands.
Here, the sea provides a living.
The local fishermen keep
a careful eye on the weather.
They know that storms
can bring a good catch.
Turbulent weather stirs up
nutrients from the deep,
attracting great shoals of fish.
It's the hottest time
of the year,
and the sun beats down
relentlessly.
By late afternoon,
the huge inflow of heat energy
has led to the buildup
of large cloud formations.
Sometimes, these formations
develop into massive storms.
It's a process that satellites
are revealing in fine detail.
Circling above the fishermen is
a NASA satellite called Aqua--
Latin for "water."
It orbits the poles.
One of its key tasks is to
monitor the complex interaction
between sunlight and water.
JEFFREY HALVERSON: Aqua satellite
is one of NASA's flagship satellites.
Its primary function is to study
the hydrologic cycle on Earth:
vapor in the atmosphere,
liquid ocean,
the temperature of that ocean
and the ice.
NARRATOR:
One of Aqua's instruments
looks down at the sea
around Cape Verde,
again in infrared,
sensing heat.
Highlighted here in yellow,
over one million
square miles of ocean
reaches a critical temperature:
80 degrees.
At this temperature,
the sea is evaporating fast,
producing an invisible gas:
water vapor.
SHUCKBURGH: By looking at the infrared,
the Aqua satellite
is able to measure the amount
of water vapor evaporating
from the surface of the ocean.
NARRATOR:
Aqua shows that this area
is producing millions of tons
of water vapor every hour.
Based on that data,
it's possible to create an image
of what the vapor
might look like
if these fishermen
could actually see it
in the air around them.
Water vapor is much lighter
than air,
and vast columns rise upward,
directly from the surface
of the sea.
The water vapor carries with it
heat, the energy of the sun.
HALVERSON: Well, water vapor is like
invisible energy.
It's like molecules
escaping the ocean,
taking heat energy with them,
and they're like little
mobile solar collectors
that are zipping
around the atmosphere.
NARRATOR: Half a mile up,
as the air cools,
the water vapor condenses
back into liquid water--
tiny droplets
that form vast clouds.
The vapor releases
the sun's energy,
the heat it received earlier.
The result is a storm.
HALVERSON: Molecules condense
in the atmosphere
and become liquid again,
and when that happens,
that heat is given off
into the atmosphere
and it warms the atmosphere,
and that's the heat
that powers storm systems.
NARRATOR: In the worst storms, the heat
captured by the water vapor
is equivalent to up to 200 times
the global production of
electricity at any given moment.
The process of evaporation
results in something
we don't need special
instruments to see.
The rising heat drives
the clouds up to ten miles high.
As the clouds rise upward,
the earth's rotation
causes them to spin.
The thunderclouds merge
into a vast vortex.
This is the birth
of a hurricane.
(loud winds blowing)
It is 2005, the busiest
hurricane season on record.
On August 27,
a meteorological satellite
is tracking
a category three hurricane
that started in the Bahamas.
Its name is Hurricane Katrina.
Throughout the region,
there is one question
on everyone's mind:
will the hurricane hit land,
or will it blow itself out?
The answer may come from
a NASA satellite called TRMM,
the Tropical Rainfall
Measuring Mission.
TRMM is equipped with a radar
and imager
that operate in the microwave
range of the spectrum.
These are higher in energy
and shorter in wavelength
than other radio waves.
The instruments
bounce microwaves
off raindrops in the clouds,
allowing scientists to build
a three-dimensional model
of the internal structure
of a hurricane.
HALVERSON: We can actually look
at microwave energy
which is generated
within the clouds
and coming from
the ocean's surface.
It's almost as if the clouds
are now invisible to us;
we can see right through them
like taking a CAT scan
to look inside those clouds.
NARRATOR: This satellite is
a powerful tool,
and now its sensors reveal
something ominous.
Huge, vertical columns
of warm water vapor
burst up from near the center
of the storm.
Almost like hurricanes
within hurricanes,
these climbing vortices deliver
added infusions of energy
into the heart of the storm,
fueling its growth even more.
These new sources of energy
are called hot towers.
HALVERSON: If they occur in the right place
at the right time,
near the very center
of the system,
they can be like
a giant spark plug
that gets that
whole engine running
at very, very high speed.
NARRATOR: The hot towers draw more and
more water vapor off the ocean.
This triggers a feedback loop
that leads to
a runaway reaction.
In just 24 hours,
Hurricane Katrina grows
into a category five monster.
(loud winds blowing)
(screaming)
NARRATOR: All this violence
is a direct result
of the power of the sun
on the ocean.
Ferocious winds blow
for two days straight,
reaching 175 miles an hour,
twisting steel like paper
and ripping apart homes
and buildings.
Over three trillion gallons
of rain a day
and a massive tidal surge
from the Gulf of Mexico
combine to inundate whole areas
of the Gulf Coast.
Katrina leaves its mark
across 90,000 square miles.
Over a million people
are displaced.
Katrina becomes the standard
by which future hurricanes
will be assessed.
But even this extreme hurricane
is just a tiny brushstroke
in a much bigger picture:
a picture of how the sun drives
water around the entire planet
with radically different effects
in different places,
all under the watchful gaze
of our eyes in space.
Take just a single day in July.
In New York, commuters swelter
in 95 degree heat.
Searing winds pump hot air
into the region from the south,
creating oppressive,
humid conditions.
7,000 miles away,
in Mumbai, India,
commuters here struggle
to cope with torrential rain.
The deluge comes so fast
that the streets
are flooded in hours.
Meanwhile, in Chile,
the desert of the Atacama
is almost totally dry.
There are places here
where rainfall
has never been recorded.
Such diverse environments,
thousands of miles apart,
appear totally unrelated.
But by pulling back
for a wider view,
we can see that they are in fact
intimately connected.
Orbiting 22,000 miles
from Earth's surface
is a chain of five
weather-tracking spacecraft,
including this one:
NASA's GOES East.
GOES is an acronym
for Geostationary Operational
Environmental Satellite.
Each moves in a fixed position
relative to the earth,
called a geostationary orbit.
They always look down
on the same parts of the planet.
The combined data
from these five satellites
gives scientists a unique
perspective on the earth.
SHUCKBURGH:
By having several of them
located at different positions
around the equator,
we're able to get a view
of the whole earth
24 hours a day.
NARRATOR: By observing the entire earth,
these satellites reveal
how energy moves
throughout the globe,
beginning with the impact
of the sun on water.
The process is the same
everywhere,
but the outcome will be very
different in different places.
Converted from
the numerical data,
these five circles
graphically depict
what the satellites
actually sense.
They reveal the total picture
of water vapor produced on earth
in a single frame.
Seen here in fast forward,
one second is equal to a day.
It shows how water vapor
produced at the equator
continuously transports the
sun's energy towards the poles.
Local landscapes and topography
affect the vapor's impact,
with results unique
to each region.
In India at the end of July,
the warm water vapor is drawn
from over the ocean
by the difference in temperature
between land and sea.
Rising to high altitude,
the vapor cools over the land
and condenses back into water.
We call the result
the Asian Monsoon.
Nearly a trillion tons of rain
falls out of the sky,
transforming parched land
into fertile plains.
The monsoon eventually moves
to the east, reaching China,
where it floods the paddies
that are ideal for growing rice.
This process helps provide food
for three billion people,
almost half the world's
population.
Meanwhile, on the other side
of the world in South America,
westbound winds
drive water vapor
across the high peaks
of the Andes.
The altitude strips the air
of its moisture,
which falls as snow
on the mountains,
creating on the far side
in central Chile
the arid desert of the Atacama.
That same July day
in the eastern United States,
hot, moist air surges north
straight from
the Gulf of Mexico.
With no natural barrier
in the way,
more than 100 million Americans,
from Memphis to New York,
swelter in the summer heat.
This graphic,
based on information
provided by satellites,
depicts the interaction between
the atmosphere and the oceans
as they connect in a global
pattern of circulation
that results in our
local weather.
SHUCKBURGH:
The satellite data shows that
it's all one
interconnected system,
but that in different parts
of the world,
different processes
are happening.
We can see the monsoons
and their effect.
We can see the effects
on deserts
in a different part
of the world.
And that together shows us
how water vapor is connecting
with life on earth.
NARRATOR: But this vast cycle
of sunlight, water and land
is just one pattern among many
on this planet we call home.
A cycle with even
greater consequences
for the long-term climate
involves extreme cold.
To see how that works, we have
to turn the earth upside down
and look at it from below.
Antarctica remains the earth's
last great wilderness,
a vast frozen continent
plunged in darkness
for almost six months
of each year.
In winter,
temperatures can drop
below minus 110 degrees
Fahrenheit,
and an incessant
100-mile-an-hour gale blows.
It's hard to believe
that anything life-giving
could start here
in this bleak place.
But that's exactly
what happens.
Antarctica's ice
plays a vital part
in maintaining global climate,
sustaining life even in lush,
warm jungles
thousands of miles away.
ABDALATI: Antarctica is a fundamental
element of the climate system.
And while it may sit silently
and majestically
at the edge of the planet
for very few to see,
things go on there
that spread out
all over the world,
that affect the world
as a whole.
NARRATOR: It's a paradox that such a bleak
and barren place
is so critical
to life on our planet.
On average, it's 43 degrees
colder than the North Pole.
Why should Antarctica
be so much colder,
and how does that affect
the rest of the world?
The detectors on NASA's
polar-orbiting satellite Suomi
provide part of the answer.
The instruments sense
in the infrared and ultraviolet
parts of the spectrum.
They show that the poles receive
little of the sun's energy
and reflect most of it
back out into space.
That's one reason why the poles
stay cold.
But there's another factor that
makes Antarctica colder still.
This image has been
pieced together
from 17 different satellites
that sense the infrared,
or heat.
The continental mass
of Antarctica
lies beneath this swirling
maelstrom of cloud.
A computer model of the data
shows what happens
as the warm moist air
arriving from the tropics
collides with the cold air
over the South Pole.
The result is
a massive storm system.
And just like a hurricane,
it rotates as a result
of the spin of the earth.
Only this is much larger
than a hurricane,
4,000 miles in diameter.
Where that cold air and warm air
meet high up in the atmosphere,
the air starts to rotate
around Antarctica.
The winds can be up
in the atmosphere
as much as 200 miles an hour.
NARRATOR: This circulation pattern
is called the polar jet,
a ceaseless circle
of wind and storms.
The relentless clockwise wind,
seen here in yellow,
drives the seawater below,
shown in light blue.
DAVID ADAMEC: Those strong winds are sending
a jet around in the ocean,
and it's driving
an ocean circulation
that is felt almost all the way
to the bottom of the ocean,
two and a half miles deep.
NARRATOR: The Southern Ocean
rings the continent
with no land to interrupt
a vast body of moving water.
This is the Antarctic
Circumpolar Current.
And these are
the "Screaming Sixties,"
the roughest, most dangerous
seas on the planet.
Here, storms rage almost
every day of the year,
whipping hundreds of trillions
of gallons of water
into a ceaseless frenzy.
Now the infrared instrument
on the Aqua satellite
which senses atmospheric
temperature
puts the pieces
of this puzzle together.
The winds of the polar jet
and the water
of the circumpolar current
together form an impenetrable
barrier around Antarctica,
isolating it from the rest
of the planet
and depriving it of warmth.
That is why the whole region
remains exceptionally cold
all year round.
ABDALATI: What's incredible about
what the satellites tell us
is that the movement of air
and actually the movement
of ocean current
around the perimeter
of Antarctica
isolates the continent
from the rest of the world.
NARRATOR: So why is this relentless cold
so important to the planet
way beyond Antarctica?
The answer lies in a remarkable
property of water:
what happens when it freezes.
The Aqua satellite reveals
the start of the process.
It sweeps the surface
with its microwave scanner,
looking through the clouds
to detect the distinct
signature of ice.
SHUCKBURGH: The microwave instruments
on the satellite
enable us to see through
the clouds
to the sea ice around Antarctica
throughout the year.
What's particularly incredible
about that is
we're able to take measurements
of the sea ice
in places where as scientists,
as humans, we can't even go.
NARRATOR: This satellite gives us
an accurate picture
of the extent of sea ice
around Antarctica
over the course of a year.
Seen here in summer,
Antarctica is nearly
one and a half times the size
of the United States,
covered in ice.
But in winter,
it grows even more.
Over five and a half million
square miles of ice form
around the continent.
It grows to the size
of all of Africa.
This vast ice formation
has a profound effect
on life across the planet.
How can its impact
extend so far?
One of the best places
to understand the power of ice
is the huge bay
along the northwestern coast
of Antarctica: the Weddell Sea.
Here, a constant gale blows
and cools the seawater
to freezing temperatures.
Once the upper layer of ocean
falls below 29 degrees
Fahrenheit,
a critical threshold is crossed.
The surface of the ocean
begins to freeze.
(crackling)
At a microscopic level,
tiny crystals start to grow,
knitting themselves together.
As the crystals bond,
they expel salt into the water.
The salt forms brine that drips
down long, narrow tubes
and holes in the ice
as it forms.
The brine is denser than regular
seawater and it sinks downwards.
As winter's grip tightens,
the formation of ice
speeds up and spreads.
Soon, large slicks appear
on the surface
and thicken into a solid mass.
What started as
a microscopic process
can soon be seen from space.
Each year, more than
200 billion tons of ice form
in the Weddell Sea alone,
releasing tens of trillions
of tons of dense brine
into the ocean.
The fate of all this brine
is a mystery.
The crucial question is
where does it all go?
A satellite called Jason,
jointly operated by NASA
and the French space agency,
is providing new answers.
Jason bounces radar signals
off the surface of the ocean
to measure its height.
The instrument also reveals
the shape of the sea floor
far below.
We can make very accurate maps
of submarine bathymetry.
But we don't do that directly;
we do that by measuring the
surface of the sea from space,
very, very accurately
and over time.
NARRATOR:
Jason's radar is so precise
that it can detect
minute changes
in the level of the sea surface
produced by the peaks and
valleys of the terrain below.
The data makes it possible
to map the ocean floor.
ADAMEC: You have a satellite that's
up there, 500 miles up in space,
and it's returning an accuracy
of a little less
than half an inch.
What that means is, you know,
I've stuck this instrument
in Washington, D.C., say,
and I'm looking at a crowd
of people in Boston
and I can tell you
whether or not their toes
are over the curb or not.
That's what this satellite
is doing.
NARRATOR:
The satellite data
allows scientists to make
a three-dimensional map
of the ocean floor
beneath the Weddell Sea.
It reveals a vast chasm,
two miles deep,
off Antarctica's
continental shelf.
As the brine descends
into the ocean,
it eventually falls over
this precipice.
Other sensors attached
to the sea floor
track the flow of the brine
as it sinks.
SHUCKBURGH: What we're really
excited about is that
we're able to take that data
that shows us what the bottom
of the ocean looks like
and combine it with data
from sensors under the water.
And that enables us
to look at the dense water
and where it goes.
NARRATOR: Combining data from satellites
and undersea instruments,
scientists can reconstruct
what is happening
hidden beneath the ice.
What they learn is astounding.
One trillion gallons
of salty brine
plunge down through
the Weddell Sea every hour,
a torrent equivalent to the
volume of 500 Niagara Falls.
The brine spreads out
towards the edge
of the Antarctic
continental shelf
and then falls into the chasm
revealed by Jason.
A vast submarine waterfall
plummets downward.
The cold, dense brine
falls slowly, silently,
into the abyss,
two miles down
to the ocean floor below.
It will not resurface
for hundreds of years.
What happens to the brine next
is still being investigated.
But computer models
combined with satellite data
are helping scientists
to figure out where it goes.
This animation shows the
undersea current in action.
The purple area is the brine.
The outflow from Antarctica
drives the salty water
towards the equator,
along the sea floor.
ADAMEC: All the water in the bottom
of every ocean around the globe
has its start within six miles
of the Antarctic continent.
It creates the coldest, densest
water that's on the planet.
NARRATOR:
The cold, salty liquid
becomes part of a worldwide
circulation system,
stirring and cooling
all the world's oceans.
Leaving Antarctica,
it has embarked on a journey
that could take 1,000 years
to complete.
As it migrates
towards the equator,
the cold bottom current mixes
with fresher and warmer water
and slowly rises.
It then joins
other ocean currents
and eventually returns south,
where it cools once more.
Finally, returning
to Antarctica,
the seawater freezes
and releases its salt again,
completing the cycle.
It's an endless loop that is
critical to the whole planet.
ABDALATI: The importance of dense water
in Antarctica is that
it really forms the basis
of global ocean circulation.
The temperature
and the salt combine
to cause sinking and rising
in different parts,
which sets up
this conveyor belt,
this interaction of
all of the ocean water.
NARRATOR: In the Arctic, frigid winter
winds cause the ocean to freeze.
The North Atlantic currents
cool and sink to the bottom,
then head south again.
All over the world, slow-moving
currents of seawater like this
regulate the average
temperatures of the oceans
to within one degree.
This stability has
a profound effect on life
all across the world.
This NASA simulation shows
the surface of the entire ocean,
a web of currents
in constant motion.
But satellites show us that
the oceans don't work alone.
The currents affect the air,
the atmosphere,
that sits above them.
The ocean and atmosphere
are intimately connected.
For instance,
the Gulf Stream
takes warm water
from the Gulf of Mexico
north to the eastern
United States and Europe,
generating warm air.
On the other side
of the world,
another current
called the Kuroshio
carries heat from China
north to Japan.
ocean currents distributing heat
around the planet.
The climate we live in
is a result of ocean
circulation patterns.
The reason in the United States
that North Carolina
and South Carolina are warm
is because there is
the Gulf Stream.
And the reason there's
a Gulf Stream
really takes root in Antarctica.
NARRATOR: As a major engine driving
the world's ocean currents,
Antarctica helps protect
Earth's climate
from wild swings
in temperature.
The constant,
dependable circulation
of the oceans around the globe
and the relatively stable
temperatures it produces
have made Earth
a hospitable planet.
Long-term stability provided
time for life to flourish
and complex animals
and plants to evolve.
And this is how a process
that began with Antarctic ice
continues to sustain our world.
ABDALATI: When you put it all together,
you get a story
of how ocean circulation affects
climate and weather
and what that means today,
tomorrow
and 20 years out
into the future.
(rumbling)
NARRATOR: But ocean currents
and the atmosphere
are not the only players.
Beneath the sea floor,
forces inside the earth
are a crucial source
for the basic materials
that nurture life.
This hidden mechanism
is driven by ceaseless,
often violent activity.
Two recent examples:
A magnitude nine earthquake
strikes Japan in 2011.
An entire section
of the country
moves eight feet
towards North America.
A year earlier, 2,500 miles to
the south in Papua New Guinea,
the volcano Rabaul erupts.
It fires a vast plume of ash
high into the atmosphere.
These are catastrophic,
hugely destructive events
with an enormous cost
in human lives.
But the natural forces
behind these disasters
also provide the materials
we and other living organisms
need to survive.
And satellites help show us
how this happens.
Canada's RADARSAT is
one of several satellites
that use highly sensitive radar
to map the earth's surface
in three dimensions.
Bouncing radio waves off
the terrain below,
these satellites continually
sweep the surface of the globe.
They can measure the height
of the earth's surface every day
to an accuracy of less
than a quarter of an inch.
When the data is plotted
over time,
we can see in fine detail
how the earth's crust
is constantly moving.
This is the surface
of the crater
atop Mount St. Helens
in Washington state.
Animation reveals how it swells
over the course of three weeks,
driven by a surge of molten
magma beneath the crater.
Satellites can actually see
the crustal plates moving now.
We can see bulges and dips
where the magma is moving around
underneath the crust.
NARRATOR: This animation shows the
swelling of Mount Etna in Italy
as magma accumulates beneath it
over nine years.
When the volcano erupts,
the land sinks back.
SELLERS:
So we're getting a picture now
of what the world looks like
under the crust
and how that affects
the other dynamic processes
of the so-called solid earth.
NARRATOR: Every day, dozens of volcanoes
around the world are erupting,
while 4,000 earthquakes
shake the ground.
Our earth is dynamic,
constantly ejecting gases
and magma from its depths.
And some of this activity
has a vital impact on life.
The secret to understanding how
lies deep beneath
the ocean's surface.
Here, a crucial chemical
reaction takes place
between molten rock
and deep ocean water.
The Jason satellite's
sea surface-mapping radar
reveals a chain
of active volcanoes
a mile and a half down, at the
bottom of the Pacific Ocean.
This is where
that critical interaction
between molten rock
and freezing water takes place.
This footage was taken with
a remotely operated submarine,
also called Jason.
Lava and superheated gases
spill out of cracks
in the ocean floor,
known as hydrothermal vents.
Jason reveals what happens
when cold ocean water
penetrates into the cracks.
A magma chamber below
heats the water
to up to 750 degrees
Fahrenheit.
In the pressure-cooker
environment inside the cracks,
the dense salty water actually
dissolves the solid rock.
Complex chemical reactions
take place,
producing minerals
containing sulfur and iron.
These are nutrients that living
organisms need to survive.
The seawater, now loaded with
minerals from inside the earth,
streams out of the
hydrothermal vents.
These nutrients feed
a thriving ecosystem
that includes shrimp and exotic
creatures like tubeworms.
The deep ocean currents carry
the leftover nutrients away.
Over thousands of years, they
circulate through the oceans,
ultimately rising to the surface
and contributing to an amazing
explosion of life.
And we can see this activity
with NASA's Aqua satellite,
which is equipped
with instruments
that observe the earth
in many wavelengths
of the electromagnetic spectrum.
One tool is called MODIS.
MODIS is pretty much the crown
jewel of the Aqua satellite.
It's an enormous scanner.
So it basically covers
the whole world every day.
NARRATOR: MODIS scans the ocean
in the infrared
and the visible portions
of the spectrum.
It can detect extremely subtle
changes in the temperature
and color of the water.
So what we have in space
is an instrument
that looks at very, very small
parts of the spectrum,
and we measure how much light
comes back
in each part of the spectrum.
NARRATOR: Looking down at the west coast
of South America,
MODIS detects an upwelling
of cold water
150 miles west of Peru.
Then it detects a particular
shade of green.
This identifies the source
as chlorophyll,
a sign of plant life.
It's clear that the satellite
has spotted a massive bloom
of tiny organisms
called phytoplankton.
Just below the surface, these
phytoplankton are absorbing
the rich soup of minerals that
have come from the deep ocean.
And with light from the Sun,
and carbon from the carbon
dioxide in the air,
they multiply by the billions.
As MODIS shows, the plankton
multiply so quickly
that in just 24 hours,
500 square miles of ocean
have turned to this
distinctive green color.
GENE FELDMAN:
They replicate very, very fast.
So you can have a plankton bloom
that doubles over the course
of a day
and can cover hundreds or
thousands of kilometers
of the ocean surface.
NARRATOR: It's the minerals from beneath
the earth's crust
that have helped fuel this
vast explosion of plankton--
over 800 thousand tons of living
material.
And that's only the beginning.
This plankton is the base of
the food chain for marine life.
The bloom triggers one of
the largest feeding frenzies
on earth.
Trillions of anchovies
and sardines
feast on the tiny organisms.
They, in turn,
attract larger predators
to one of the densest
concentrations
of marine life anywhere.
Sharks converge.
And even birds, flying above,
dive down to join the feast.
And up above, humans are here,
too, taking advantage
of one of the world's most
productive fishing grounds.
The satellite data reveals
similar upwellings
all around the world, delivering
nutrients, seen here in pink,
into the surface waters.
Each upwelling triggers
a plankton bloom.
FELDMAN: Phytoplankton provide
that key link
between this energy out here,
the raw materials
that this planet holds
and the food engine
that allows life to flourish.
NARRATOR: These vast green ribbons
of plankton
can cover as much as a fifth
of the world's ocean surfaces,
about 45 billion tons of biomass
every year.
The plankton are one link
in a chain of life
that begins deep beneath
the seafloor.
The most important plant life
on this planet
are these microscopic
little green plants
that float in the ocean.
NARRATOR:
Plankton may be key to life,
but they themselves
don't live long.
MODIS shows how,
in just 72 hours,
a bloom can rapidly weaken
and fade.
All the plankton
that have not been eaten
die and sink into the abyss.
They take their precious
minerals with them
all the way back
to the ocean floor.
Here they will remain
for millennia,
a thick carpeting of tiny
carcasses half a mile deep.
Some of the minerals may
ultimately be recycled.
Some may emerge through
hydrothermal vents again,
millions of years from now.
But some plankton,
through yet another
extraordinary chain of events,
will deliver their precious
cargo of nutrients
not just to life in the ocean,
but also to life on land.
Half a world away from the coast
of Peru, where plankton bloom,
lies the Sahara Desert
in North Africa.
The Sahara is enormous--
it makes up a tenth
of the African continent.
It's one of the driest
and dustiest places on earth.
Surprisingly, the remains
of ancient plankton are here,
hidden in this arid landscape.
It is May,
the hottest month of all.
Camel herders travel through
one of the most exposed regions
of the Sahara:
the Bodele Depression.
Six thousand years ago,
this was covered by the world's
largest freshwater lake.
The floor of the lake is covered
with the ancient remains
of plankton-- called diatomite--
laid down in a much earlier age,
when an ocean covered
the region.
With its eye on the earth
from 400 miles above,
NASA's Landsat 7 is one of the
latest generation of satellites
studying the composition of
rocks that make up our planet.
It sweeps the Bodele, producing
these high resolution pictures
in multiple wavelengths
of visible light.
The white expanse
is the diatomite
on the bed of the lake.
The size of the lake is over
a thousand kilometers long
and 600 kilometers wide.
But with a satellite image,
we can see the whole extent
of the basin on a series
of images
and visualize that on a computer
in a matter of minutes.
NARRATOR:
The satellite image analysis
shows over 24,000 square miles
of sediment,
all of it diatomite.
We can map where the diatomite
sediment is
on the floor of the lake.
NARRATOR:The diatomite from the plankton
is a rich source of phosphorous,
an element needed by all living
things to produce energy.
But for this nutrient to
re-enter the chain of life,
it must first embark
on a long journey
that can be seen from space.
The journey begins here on the
ancient lakebed in the Sahara.
The wind sweeps up a few flakes
of diatomite into the air.
The flakes fracture
into a fine powder
and are carried off by the wind.
A dust storm builds.
22,000 miles above, the European
weather satellite Meteosat 8
looks down from its
geostationary orbit.
It records a daily pulse of dust
rising off the Bodele
Depression.
Here it's visible
as a whitish dust cloud
lifting from the desert
with clockwork regularity
at noon each day.
BRISTOW: Although the individual
particles of dust are minute--
they're hundredths or
thousandths of a millimeter
in diameter-- there are such
vast clouds of this dust
that you can see it
on satellite images.
NARRATOR: The dust cloud is over
a hundred stories high
and 200 miles wide.
From here it will head west
on an epic journey.
Seen from space,
the dust is blown across Africa.
At the Atlantic coast, it's
drawn up high into the sky.
This simulation,
based on satellite data,
shows how prevailing winds carry
the dust cloud west and south
3,000 miles across the Atlantic.
As much as 7,000 tons of dust
are airborne at any one time.
The destination is set
by the winds:
South America and the Amazon.
We're taking literally thousands
of tons of this dust,
which is containing phosphate,
and exporting that
from the Bodele.
The wind is carrying it out
across the Atlantic
to fertilize the Amazon.
NARRATOR: Here in these clouds
high above the rainforest,
what was once living plankton
reaches the end of its journey.
The minerals in the dust,
which include energy-giving
phosphorous,
dissolve into water droplets
and fall to the Amazon in rain.
BRISTOW: Areas like the Amazon jungle,
although they appear very rich,
the soils are actually very
depleted, they've been leached.
And one of the things that
they're short on is phosphate.
NARRATOR:
Rain falls incessantly
throughout the Amazon's
wet season,
delivering thousands of tons of
phosphate into the forest below.
It passes into the soil
and the roots of the trees,
nourishing the rain forest.
The effect of all this
natural fertilizer
can be seen clearly from orbit.
Terra is the twin
of the Aqua satellite.
It circles the earth
every 99 minutes,
monitoring how fast vegetation
is growing.
SELLERS: We can see all the green
vegetation on earth--
wall to wall, every day--
and it tells you almost
everything you want to know
about the state of life
on earth.
NARRATOR:
With its color scanner,
Terra can see the effect of
the Sahara dust on the Amazon
at the end of the rainy season.
It observes an increase
in the distinctive green color
of chlorophyll.
Like the plankton blooms
in the ocean,
the forest is kicking
into overdrive...
watered by rain
and nourished by the minerals
borne across the Atlantic
by the dust cloud.
For every leaf that exists now,
three more will grow in a week.
It's the culmination
of a chain of events
that began far back in time
and halfway around the world.
SELLERS: Ancient sediments laid down
by other organisms
millions of years ago
get eroded, make dust,
the winds bring them
across the Atlantic,
fertilize the tropical forest
in the Amazon.
NARRATOR: The migration of Bodele dust
to the Amazon
is just one of many ways
that vital minerals spread
to living habitats
all over the world.
Every landscape has
its own story
and its own way of entering
the chain of life.
BRISTOW: The exchange of nutrients
from the land
is going on
all over the globe every day.
NARRATOR: And in certain areas,
this is what accounts
for the special productivity
of the soil.
The Great Plains of North
America are rich in minerals
eroded from the Rocky Mountains.
These are vital ingredients
for growing wheat and corn.
In Bangladesh, the Ganges delta
is rich in iron
washed down from the Himalayas
in river sediments,
ideal for growing rice.
The hidden transport of minerals
creates fertile soils
that enable plants to thrive.
These minerals are the basis
of the food chain
for all life on land,
including us.
SELLERS:
All of this reminds you
how interconnected
the earth system is...
...that no living thing lives
in isolation from processes
that may happen a long way away
in both space and time
from itself.
NARRATOR: Satellites provide a vivid
new perspective on the links
between land, sea,
air and life.
This new perspective
helps us see
how the natural forces
of our planet fit together,
and that includes the atmosphere
and something as basic
as the air we breathe.
Less than a quarter
of the air around us
is comprised of oxygen, but that
oxygen is essential to life.
It's what all animals need
to burn fuel in their bodies.
Oxygen is vital to metabolism.
It provides the energy
that allows even the most active
creatures to survive and thrive
and to master
their environments.
Scientists believe
that the abundance of oxygen
in the atmosphere was essential
for the evolution of large,
intelligent mammals like us.
The human brain alone uses about
20% of the oxygen we breathe.
But where does
all this oxygen come from?
Satellites can help us answer
that question.
NASA's Aura satellite
is one of several spacecraft
that are helping scientists
study the earth's atmosphere.
Along with ground instruments,
it can analyze the atmosphere
and pinpoint its composition.
It builds a picture
of the nitrogen,
oxygen and carbon dioxide
that together make up 99%
of the air we breathe.
This computer
visualization shows
how the earth's atmosphere
changes over 24 hours.
During the day, oxygen--
seen here in blue--
rises all over the planet.
At night, carbon dioxide--
shown in orange--
is on the rise.
And the oxygen we need
is given to us by plants.
Before plants, there was
no oxygen in the atmosphere.
So plants did all the hard work
of allowing the atmospheric
concentration
to build up over time, allowing
all other life to develop.
They made the place habitable
for us.
NARRATOR: Plants breathe in carbon dioxide
and expel oxygen.
They produce so much
that the vast Amazon rainforest
is often called the lungs
of the earth.
But the real picture
is more complex.
The verdant wilderness
of plants and animals
is one of the oldest,
most abundant living systems
on earth.
Over two million square miles
of lush rainforest
teem with half the world's
living species.
SELLERS:
The Amazon is
the largest natural preserve
of life on the continents
that's left in the world.
Thousands of miles
of almost virgin forest,
thousands of species
that have been there
for an awfully long time.
NARRATOR: So dense is the Amazon jungle
that it has a dramatic impact
on the air above it.
It starts in the trillions
of leaves far below.
We can use animation to show
what this invisible process,
known as photosynthesis,
might look like.
During the day, the leaf takes
up carbon dioxide from the air,
seen here in orange.
It converts the carbon
into sugar for energy and growth
and releases oxygen,
seen in blue.
Each one of these trees
will release
hundreds of thousands of cubic
meters of oxygen
in the course of its life.
And as for the Amazon
as a whole,
a fifth of the world's oxygen
is produced here.
But there's a surprising twist:
we will breathe
almost none of it.
Satellite data and ground
measurements reveal
that almost all the oxygen the
Amazon produces during the day
remains there and is reabsorbed
into the forest at night.
SELLERS: With the advantage
of the satellites,
we can now see that the Amazon
basically uses
all its own oxygen
and uses all its own
carbon dioxide.
It is, as far as we can tell,
almost a closed system
in itself-- almost.
NARRATOR: But the Amazon still plays
a vital part
in generating the oxygen
that we breathe.
What satellites
now make clear is
producing the oxygen that
benefits us takes an extra step.
The process begins with rain,
which falls up to 250 days
a year in the Amazon.
The soil of the rainforest
is continually washed
into the Amazon river system,
taking with it nutrients
and organic material.
An average of two million tons
of this sediment
is released every 24 hours.
The sediment flows eastward,
traveling 4,000 miles
into the Amazon delta.
Here, microscopic plankton
near the surface thrive
on the nutrients and
their population explodes.
As they spread further
out to sea,
some of these tiny organisms
act like plants,
absorbing carbon dioxide
and releasing oxygen.
Again the Aqua satellite shows
us how a giant plankton bloom
grows to cover 25,000
square miles.
This vast area translates into a
huge boom in oxygen production,
made available
to the entire planet.
FELDMAN: When plankton grow,
they release oxygen.
That oxygen ultimately finds
its way into the atmosphere.
NARRATOR:
The massive scale of this impact
is revealed when the satellite
data is visualized.
This animation shows the oxygen
produced by plankton blooms,
seen here in bright blue.
The Amazon plankton bloom
releases billions of gallons
of oxygen into the atmosphere
every day.
Within a few days
the plankton die,
leaving most of the oxygen
they produced in the air
as they sink to the bottom
of the ocean.
Similar explosions
of microscopic life
happen all over the world.
Plankton's major role
in replenishing oxygen
in the atmosphere is something
we've only fully grasped
with the help of satellites.
FELDMAN:
Satellites gave us
that very first global picture,
global assessment of what
the ocean's plants were doing.
NARRATOR: And what plankton are doing is
providing life-giving oxygen
for us.
FELDMAN: Plankton in the ocean are
responsible for over half
of the oxygen that we breathe,
and it's what most creatures on
this planet rely on to survive.
NARRATOR: Microscopic organisms
as well as rainforests
are the lungs of the earth.
So what other secrets of life
can satellites--
our eyes in space-- reveal?
It turns out that another
surprising way life is sustained
is through a violent force:
lightning.
From orbit, the whole earth
buzzes with electricity.
Astronauts are often amazed
by the intensity
of the electrical storms raging
far beneath them.
SELLERS: You can see
a thousand miles' worth
of lightning flashes left and
right as you're looking down,
and they seem to set each other
off like fireworks,
bang, bang, bang, bang, bang.
It's really quite amazing.
NARRATOR: But to understand lightning's
global impact,
we need more than just
observation.
NASA's TRMM satellite carries
a high-speed camera
that can detect individual
lightning bolts.
From this information it's
possible to build a picture
showing the distribution of
lightning all across the globe.
Astonishingly, 40 strikes occur
every second.
That's more than three million
strikes a day.
So how is all this lightning
created?
And what is the effect
of all this energy
streaking through
the earth's atmosphere?
Each day, the combined force
of sunlight and water vapor
creates 40,000 thunderclouds.
The rising columns of moist air
generate powerful updrafts
that turn water vapor
into ice particles
inside the clouds.
As ice and water droplets smash
into each other at great speed,
vast charges of static
electricity build up.
An average thundercloud contains
enough energy
to power a city the size
of Denver for ten hours.
Eventually the charge builds
to a point
where air molecules
are torn apart
and a lightning bolt is born.
A bolt is no thicker
than a human thumb,
yet it's five times
the temperature
of the surface of the sun.
As it burns through
the atmosphere,
the electricity breaks apart
the molecules of nitrogen
contained in the air.
ADAMEC:
A lightning stroke,
it actually splits the nitrogen
into single nitrogen molecules.
Nitrogen doesn't like that.
It's desperately looking
for something
to connect back to with and it
often does it with oxygen.
NARRATOR: When oxygen bonds
with nitrogen,
it creates a vital nutrient
called nitrate.
Satellites show the extent
of nitrate--
simulated here in yellow--
produced by the more than three
million lightning bolts
that strike every day.
This creates about 13,000 tons
of nitrate.
It dissolves in water droplets
in the clouds
and falls to the ground in rain.
Most people are familiar
with nitrates
because they're fertilizers.
So when it rains
in a thunderstorm,
in a way you're getting a free
fertilizing,
because the water will have
nitrates in it.
NARRATOR: Nitrate is absorbed
through the roots of plants
and enters the food chain.
When we eat these plants, the
nitrates become available to us.
And so this vital nutrient
enters the cells
of every living organism
on earth,
where it is critical for
building the structure of plants
and helps make proteins and DNA
in our bodies as well.
It is essential for the survival
of all living things.
But nitrate production
is not the only way
in which lightning
promotes life on earth.
In the Canadian Yukon,
a massive wildfire devastates
over ten square miles of forest
in less than a week.
Such blazes often start with
a random bolt of electricity
from the sky.
In distant Siberia, over 1,500
square miles of forest
burn to the ground,
sparked by a lightning bolt.
These flames may seem
purely destructive,
but thanks in part
to satellites,
we see that they can
also be life-giving.
The Terra satellite can detect
the location of every fire
on earth by looking at its heat
signature in infrared.
SELLERS: Terra basically gives us a map
of all the fires
in all the forests and
grasslands of the world
every day.
NARRATOR: This sped-up visualization
of Terra's data
shows a year's worth of fire
all around the world.
The vast swaths of orange are
actually thousands of tiny dots.
Each one represents
a half square mile of land
where a fire has burned,
over 19 million square miles
in total.
The Terra data also reveal
fire's role in renewing life.
SELLERS:
The observations have shown us
how important fire is
as an element of change.
NARRATOR: The benefits of change
can be witnessed
in the forests
of northern Canada.
This is a vibrant forest,
but it has its share of dead
and diseased trees.
Locked inside them are
ingredients that are essential
for new life: elements like
carbon, sulfur and phosphorous.
Yet in a cold environment
like this,
trees take decades to decompose
and return these elements
back to the soil.
Fire can shorten the cycle
to a matter of hours.
The pine tree
is highly flammable.
It's full of sap and resins
that burn easily.
The oxygen in the atmosphere
fuels the flames.
ADAMEC:
When you're looking at fire,
you're looking at
a rapid oxidation.
That's what fire is.
NARRATOR:
Within a matter of hours,
what may have started as a spark
from a single lightning bolt
turns acres of forest to flames.
The nutrients these trees
have stored for so long
end up in the ash.
Fires also consume
the dead animals
whose bodies litter the forest,
returning the nutrients they
contain back to the soil.
The smoke climbs into the sky,
and the ultimate impact
of this nutrient-rich ash
can eventually be seen
from space.
With its infrared sensor,
Terra can pick out the heat
given off by the leaves
of healthy new vegetation
that grows after fire.
A pulse of new growth
follows every blaze.
Huge areas of forest get burned
down quite regularly
and they're followed almost
immediately by rapid regrowths.
NARRATOR:
In forests all over the world,
the data from Aqua and Terra
show that within months,
large areas devastated
by fire are rejuvenated.
From a global perspective,
wildfires are essential
to the cycle of life.
Fire's like a great blender
for all the materials
in the earth system, so when you
get dead living material,
particularly in the forests,
fire will rip through there
and decompose that stuff
very quickly into its basic
minerals and compounds
that new life can use
almost immediately.
NARRATOR: Fire is such an intrinsic part
of nature
that many plants have evolved
to make active use of it.
The pine tree drops its seeds in
the ashen aftermath of a blaze
to make the most
of the nutrients
that have been released.
Wildfires are essential
to maintaining the health
of many of the world's
ecosystems.
It's a mechanism by which
habitats that are no longer
productive regenerate.
We can now follow this process
over decades.
SELLERS: When you look 30 years
of satellite data,
you see this continuous, dynamic
rearrangement of the biosphere.
The nutrients that that tree
has pulled up from the soil
are being dropped back down
again on the soil
to feed the next generation.
The effect of all this is
to allow the biosphere
to turn over far more quickly
and efficiently.
NARRATOR: By looking at the world
from orbit,
we see our home planet anew.
We discover countless hidden
connections, all linked to life.
The circulation of weather
and ocean currents
affects the ebb and flow of ice
at the poles.
Originating
in the earth's crust,
erupting magma interacts
with cold ocean water,
producing nutrients that rise
to the surface
and nourish aquatic life.
Eventually, airborne in dust,
nutrients travel
around the planet,
finally enabling tiny plankton
to fill the air with oxygen.
That allows complex animals
like us to survive.
Oxygen also allows fire to burn,
which, in turn, accelerates
the pace of death and rebirth
in the forest.
Above all, life's major driver
is the energy we receive
from the sun.
As the earth rotates
over 24 hours,
the planet responds to the
incredible power of the sun,
our local star.
Each day more than
a million terawatts--
over 7,000 times our global
energy consumption--
strike earth.
This triggers a wave of activity
around the globe.
At dawn, plants on land
and plankton at sea
begin to photosynthesize
and grow.
At the same time,
sunlight drives wind and weather
around the globe.
We are also a part
of this cycle,
as our bodies respond
to the daily inflow of energy
from above.
Our skin cells use sunlight
to create essential vitamins.
Even the flight paths of planes
reveal our intimate relationship
with the rhythms
of day and night.
Aircraft travel west in
the morning to extend the day
and east in the evening
to reduce the night.
But while the sun nurtures
all life on earth,
it also has the power
to destroy.
And with the help of a very
different kind of satellite,
we are coming to understand just
how great a threat it can pose.
Orbiting 22,000 miles
above the earth
is the Solar Dynamics
Observatory.
This satellite looks not at
the earth, but away from it.
Its task is to observe the
radiation released by the sun--
what scientists call
space weather.
We have this wonderful
new satellite
that is up in space, looking
at the sun 24 hours a day
and is providing unprecedented
images of the sun
and where space weather is born.
NARRATOR: These striking images
are produced
by the SDO's ultraviolet sensor,
detecting light frequencies
beyond the blue end
of the visible spectrum.
The sun emits constant light,
heat and other forms
of radiation,
along with occasional dangerous
bursts of charged particles.
GILBERT:
Most people don't realize
that the earth is exposed
to charged particles
that are constantly coming away
from the sun
at about a million miles
an hour.
NARRATOR: Sometimes a massive pulse
of those charged particles
erupts from the sun's surface.
It's called
a coronal mass ejection
and it contains billions of tons
of charged particles
superheated to tens of millions
of degrees
and blasted out at millions
of miles per hour.
It has the potential to wreak
havoc on our planet.
This supercomputer visualization
shows what happens
when a coronal mass ejection
occurs.
The explosion is equivalent
to 14 million Hiroshima bombs.
It sends a cloud of charged
particles millions of miles wide
racing towards earth.
Without some kind of protection,
these enormous blasts would
strip away the atmosphere,
destroy our fragile ecosystems
and scorch the earth.
Over time, repeated coronal mass
ejections would even cause
the oceans to dry up,
leaving behind a planet
as barren and bleak as Mars.
Fortunately the earth has
an invisible shield,
a magnetic field that satellites
are now enabling us
to better understand.
Orbiting between 40,000 and
120,000 miles above the earth,
NASA has a network of satellites
called THEMIS.
Each is equipped with highly
sensitive instruments
that can detect the strength
of magnetic fields.
GILBERT:
THEMIS is a series
of probes that are aligned along
the earth's magnetosphere
and they detect variations
in the magnetic fields.
NARRATOR: This computer model,
using THEMIS data,
shows how an invisible
magnetic force field
called the magnetosphere
protects the earth.
It's generated by the rotation
of the earth's core.
GILBERT: THEMIS allows us to build
a overall picture
of the structure
of the magnetosphere
and how it operates.
NARRATOR: THEMIS reveals how
the magnetic field
is constantly blasted
by the sun.
The wave of charged particles
called the solar wind
distorts the magnetosphere into
a gigantic teardrop shape,
120,000 miles across.
As wave after wave
of solar particles
strike the outer magnetosphere,
most are deflected.
But when a coronal mass ejection
arrives,
it tears open the magnetosphere,
allowing a vast number
of charged particles
to breach the magnetic field's
first layer.
The particles are free to rush
in towards the planet.
But the earth has a second line
of defense.
Inner magnetic fields steer
the radiation
down towards the poles.
GILBERT: This process is extremely
energetic.
Particles get accelerated
and then they travel down
along the magnetic field lines
towards the polar regions.
NARRATOR:
The radiation streams downward,
encircling both
the North and South poles,
and triggers something we can
see with our own eyes,
one of nature's true wonders:
the Northern and Southern
lights, or the aurora.
As the radiation strikes
the upper atmosphere
at extreme speed, it excites
the air molecules.
This makes them glow.
The oxygen in the air radiates
red and green.
The nitrogen, red and blue.
These charged particles
that originated from the sun
get trapped and then
interact directly
with the earth's atmosphere,
causing these beautiful colors.
So when we're looking
at the aurora,
basically we're looking
at the fact
that the sun and the earth
are intimately connected.
NARRATOR:
The aurora is a vivid reminder
of how potentially lethal energy
from the sun is dissipated
in the upper atmosphere.
The earth's magnetic field has
shielded the planet
from the sun's deadly radiation
for billions of years,
enabling life to take hold
and flourish.
Satellites are revealing
one final piece
of this incredible puzzle--
the role that humanity plays.
Our human footprint
has grown so large
that we have become a major
global force in our own right.
Our impact is the consequence
of a system
that has created
and sustained life
for three and a half billion
years.
Our success as a species
has resulted
in rapid population growth.
And today our presence
can be seen
across 80% of the landmass.
Now we, in turn, are affecting
the many natural cycles
that govern our planet.
Looking for signs of pollution,
the environmental satellite
Aura's infrared sensor reveals
the atmosphere's chemical
fingerprint
and shows us how we are
affecting the entire globe.
We already manufacture more
than twice the nitrate produced
by lightning, much of it used
for fertilizer and explosives.
Our factories release
more sulfur
than all the earth's volcanoes.
Our industry and transportation
produce more carbon dioxide
than the Amazon rainforest
captures.
Our cities generate dust,
trigger electrical storms
and affect rainfall.
And these are just a few
of our impacts
on earth's natural cycles.
Our earth is changing.
We're on a path to somewhere
and our ability to understand
that path is crucial
to success in the future.
And satellites help us answer
some of the most fundamental
questions
needed to understand
how our planet behaves.
NARRATOR:
But there is one key difference
between the impact
of nature and our own.
Unlike volcanoes,
the motion of ocean currents,
or the oxygen produced by
forests and plankton blooms,
we make conscious decisions
about what we do.
And here satellites
are crucial once more.
The information they provide
can help us meet
the challenges of the future.
SELLERS: The real power of satellite
observations
is they represent
objective truth.
They tell us about what
the world actually is doing,
not what we would like it
to be doing,
not what we might fear it
to be doing,
but what it's actually doing.
And it's that that allows us
to see change,
real change, for what it is.
NARRATOR: Satellites are telling us that
the oceans are slowly warming.
In the past 30 years,
the average temperature
of the ocean's surface has risen
by half a degree.
Models suggest this extra heat
could be increasing the
intensity of hurricanes
and violent storms
all around the world.
Satellite data shows
that in Antarctica,
ice shelves that took many
thousands of years to form
are collapsing year after year.
And in the Arctic, sea ice is
diminishing at an alarming rate.
Many factors play a part
in these dramatic changes,
but most scientists agree
that human activity through
our release of greenhouse gases
is the main driving force.
All around the globe, satellites
are recording change,
but there is a problem.
Just as we are able to capture
and measure these changes,
many of the current fleet
of satellites
are coming to the end
of their lives.
Satellites need fuel
to stay in their orbits.
When their time is up,
they must either use the last of
their fuel to boost themselves
far away from the earth
or descend and burn up
on reentry.
It's predicted that the number
of NASA's earth-observing
satellite systems will go
from 20 down to fewer than ten
within the next decade.
The constant stream
of information
from these vital instruments
in space will fade.
If we fail to replace
these satellites,
we could lose our ability to
track the web of connections
that is fundamental to life.
ADAMEC: The complex interactions would
be absolutely invisible to us
without a larger view
of the earth.
It's the consistency and the
amount of data that they provide
that allows us to understand
the processes that are going on
in the earth that are important
to maintaining life
as we know it.
NARRATOR:
Little more than half a century
after the birth
of satellite technology,
we are still only beginning
to realize its possibilities.
Our planet harbors mysteries
beneath its white clouds,
blue oceans
and verdant landscapes.
And they can only be solved
with the help
of these eyes in the sky looking
down at earth from space.
== sync, corrected by elderman ==
This NOVA program is available
on DVD and Blu-ray.
NOVA is also available
for download on iTunes.
Our planet: Earth.
You may think you know it well.
But a startling new picture
is emerging
of a world shaped by forces
more dynamic and intertwined
than we ever imagined,
raising possibilities
that defy common sense.
How can sandstorms
in the Sahara Desert
transform the Amazon rainforest
over 5,000 miles away?
In the frigid ocean
beneath Antarctica,
how can a vast
undersea waterfall
500 times bigger
than Niagara Falls
lead to a gigantic
feeding frenzy near the equator?
And how can warm water streaming
past the coast of Africa
trigger a weather catastrophe
half a world away
in the southern United States?
Scientists have begun to find
surprising answers
to these and other
profound questions
thanks to a network
of satellites
orbiting high above the earth.
Ever watchful,
their senses extend far beyond
what our eyes can see.
EMILY SHUCKBURGH: It's really the
last bastion of human discovery.
We're discovering new things
every day.
NARRATOR: What are these hidden forces
that rule our world?
How are the oceans,
the continents, the atmosphere
and even the sun
bound together,
and how do they affect
all living things?
For the first time,
we can understand
how earth, fire, wind and water
join together
to create the dynamic
environments
that shape life
in all its forms.
WALEED ABDALATI:
Their interaction
is what has created
the environment, the diversity,
the kind of life
we see on earth today.
NARRATOR:
With astonishing images
created from a wealth of new
information from satellites,
this is our planet
as never seen before.
"Earth from Space,"
right now on NOVA.
♪ NOVA 40x11 ♪
Earth From Space
Original Air Date on February 13, 2013
== sync, corrected by elderman ==
Major funding for NOVA is
provided by the following:
NARRATOR: Since humans first ventured
into space,
some of the greatest gifts
of exploration
have been the new views
of our home.
Who can forget the iconic
"earthrise" images
of the Apollo era?
And now from the International
Space Station,
we have these spectacular
vistas.
The blue marble is finally
revealing its secrets.
It's a planet alive with
activity and constant change,
its surface transformed
by humans
yet still ruled by powerful
natural forces
that we are only beginning
to understand.
ABDALATI: It's just spectacular
when you view it from space.
It's teeming with diversity,
with beauty.
Amazing colors, you know,
the blues and the greens
and the whites.
PIERS SELLERS:
You see the world
as one huge system
all linked through
the atmosphere and the oceans,
rolling its way
around the sun.
NARRATOR: So what is it that shapes
Earth's dynamic face?
What are the essential
ingredients,
and how do they combine to
generate and sustain all life?
How do the natural forces
that surround us work together
to create an engine
powerful enough
to nourish and drive life
forward in all its diversity?
Our best hope for answers
may come from above.
Orbiting over our heads
are 120 satellites
keeping watch from space.
Most operate at altitudes
ranging from a few hundred miles
above the surface of the planet
to as high as 25,000 miles.
Each one of these
Earth-observing satellites
reveals a different piece
of the puzzle.
Each carries an array of
exquisitely sensitive detectors,
designed to reveal
what would otherwise
be hidden from our view.
The satellites are
absolutely amazing
because not only can we see
visible things from space,
but also we can see things that
aren't visible to the human eye.
So satellites are enabling us
to turn what are
invisible processes
into visible things we can see
and then understand.
NARRATOR: To see how our world works,
in this program
we have taken information
provided by satellites,
combined it with
computer models,
and rendered the results
in these scientifically
accurate graphics.
With the invisible
now revealed,
we can see Earth as
an endlessly changing system.
These images will show
in great detail
how sunlight, moisture,
land and atmosphere interact
in unexpected ways,
with seemingly local events
often triggered by forces
far away in space and time.
And with these new insights,
for the first time,
scientists can begin
to understand
the intimate relationship
between the planet
and all the living things
it supports.
ABDALATI:
It's really the thrill,
because it matters so much,
of piecing together the story
of what the earth is doing,
how it's changing,
why it's changing
and how ultimately
that affects humans.
NARRATOR:
The first piece of the puzzle
is in understanding
the massive influence the sun,
from 93 million miles away,
has on our planet.
The world's continuously bathed
in a flow of energy
from the sun.
That warms the earth.
Everything that you can see
that lives and breathes
and moves on the earth
is pushed by the sun.
NARRATOR:
Now an electronic eye in space
can measure the impact
of the sun's energy
all around the earth.
One of NASA's newest satellites,
named for a meteorologist,
polar-orbiting Suomi,
launched in 2011,
provides the view.
The spacecraft is the size
of a small school bus.
It orbits 500 miles up, circling
the planet 14 times a day.
On board, it carries
five separate sensors
that enable it to see things
invisible to human eyes.
The light that we can see
is confined to a narrow band
of electromagnetic radiation,
just a tiny portion of what
the satellite can pick up.
Electromagnetic radiation
spans a spectrum
that goes far beyond the
familiar colors of the rainbow.
ABDALATI: If you were to consider
the full spectrum to be a line
that stretched from New York
City to Los Angeles,
the piece that our eyes
could see
would be about
the size of a dime.
There is so much other
information out there
available to us,
and that's in large part
what these satellites do.
NARRATOR: One of this satellite's
key instruments is called CERES,
an acronym for Clouds and
Earth's Radiant Energy System.
It detects a broad range
of the spectrum,
including the very short and
very long wavelengths of light
in the ultraviolet and infrared
that we can't see.
This is a CERES-eye view
of the planet.
Anything that emits heat
gives off infrared radiation,
so the CERES data shows
the earth in shades of heat,
accurate to a fraction
of a degree.
It reveals how the planet
as a whole reacts to sunlight,
both absorbing and reflecting
the radiation
coming from our local star.
At the poles, the sun strikes
at an oblique angle,
and what little light there is
gets reflected back out to space
by the ice and clouds.
These are the primary reasons
why the poles remain cool.
At the equator,
it's a very different story.
Not only does the planet receive
more direct sunlight here,
the lack of ice means that
less of the sun's energy
is reflected back into space.
And at the equator,
the sun's concentrated energy
fuels a heat engine
that can trigger weather events
around the world.
Perhaps the best place to see
the impact of the sun's heat
is an area in the Atlantic
just north of the equator
and west of Africa:
the coastal waters
of the Cape Verde islands.
Here, the sea provides a living.
The local fishermen keep
a careful eye on the weather.
They know that storms
can bring a good catch.
Turbulent weather stirs up
nutrients from the deep,
attracting great shoals of fish.
It's the hottest time
of the year,
and the sun beats down
relentlessly.
By late afternoon,
the huge inflow of heat energy
has led to the buildup
of large cloud formations.
Sometimes, these formations
develop into massive storms.
It's a process that satellites
are revealing in fine detail.
Circling above the fishermen is
a NASA satellite called Aqua--
Latin for "water."
It orbits the poles.
One of its key tasks is to
monitor the complex interaction
between sunlight and water.
JEFFREY HALVERSON: Aqua satellite
is one of NASA's flagship satellites.
Its primary function is to study
the hydrologic cycle on Earth:
vapor in the atmosphere,
liquid ocean,
the temperature of that ocean
and the ice.
NARRATOR:
One of Aqua's instruments
looks down at the sea
around Cape Verde,
again in infrared,
sensing heat.
Highlighted here in yellow,
over one million
square miles of ocean
reaches a critical temperature:
80 degrees.
At this temperature,
the sea is evaporating fast,
producing an invisible gas:
water vapor.
SHUCKBURGH: By looking at the infrared,
the Aqua satellite
is able to measure the amount
of water vapor evaporating
from the surface of the ocean.
NARRATOR:
Aqua shows that this area
is producing millions of tons
of water vapor every hour.
Based on that data,
it's possible to create an image
of what the vapor
might look like
if these fishermen
could actually see it
in the air around them.
Water vapor is much lighter
than air,
and vast columns rise upward,
directly from the surface
of the sea.
The water vapor carries with it
heat, the energy of the sun.
HALVERSON: Well, water vapor is like
invisible energy.
It's like molecules
escaping the ocean,
taking heat energy with them,
and they're like little
mobile solar collectors
that are zipping
around the atmosphere.
NARRATOR: Half a mile up,
as the air cools,
the water vapor condenses
back into liquid water--
tiny droplets
that form vast clouds.
The vapor releases
the sun's energy,
the heat it received earlier.
The result is a storm.
HALVERSON: Molecules condense
in the atmosphere
and become liquid again,
and when that happens,
that heat is given off
into the atmosphere
and it warms the atmosphere,
and that's the heat
that powers storm systems.
NARRATOR: In the worst storms, the heat
captured by the water vapor
is equivalent to up to 200 times
the global production of
electricity at any given moment.
The process of evaporation
results in something
we don't need special
instruments to see.
The rising heat drives
the clouds up to ten miles high.
As the clouds rise upward,
the earth's rotation
causes them to spin.
The thunderclouds merge
into a vast vortex.
This is the birth
of a hurricane.
(loud winds blowing)
It is 2005, the busiest
hurricane season on record.
On August 27,
a meteorological satellite
is tracking
a category three hurricane
that started in the Bahamas.
Its name is Hurricane Katrina.
Throughout the region,
there is one question
on everyone's mind:
will the hurricane hit land,
or will it blow itself out?
The answer may come from
a NASA satellite called TRMM,
the Tropical Rainfall
Measuring Mission.
TRMM is equipped with a radar
and imager
that operate in the microwave
range of the spectrum.
These are higher in energy
and shorter in wavelength
than other radio waves.
The instruments
bounce microwaves
off raindrops in the clouds,
allowing scientists to build
a three-dimensional model
of the internal structure
of a hurricane.
HALVERSON: We can actually look
at microwave energy
which is generated
within the clouds
and coming from
the ocean's surface.
It's almost as if the clouds
are now invisible to us;
we can see right through them
like taking a CAT scan
to look inside those clouds.
NARRATOR: This satellite is
a powerful tool,
and now its sensors reveal
something ominous.
Huge, vertical columns
of warm water vapor
burst up from near the center
of the storm.
Almost like hurricanes
within hurricanes,
these climbing vortices deliver
added infusions of energy
into the heart of the storm,
fueling its growth even more.
These new sources of energy
are called hot towers.
HALVERSON: If they occur in the right place
at the right time,
near the very center
of the system,
they can be like
a giant spark plug
that gets that
whole engine running
at very, very high speed.
NARRATOR: The hot towers draw more and
more water vapor off the ocean.
This triggers a feedback loop
that leads to
a runaway reaction.
In just 24 hours,
Hurricane Katrina grows
into a category five monster.
(loud winds blowing)
(screaming)
NARRATOR: All this violence
is a direct result
of the power of the sun
on the ocean.
Ferocious winds blow
for two days straight,
reaching 175 miles an hour,
twisting steel like paper
and ripping apart homes
and buildings.
Over three trillion gallons
of rain a day
and a massive tidal surge
from the Gulf of Mexico
combine to inundate whole areas
of the Gulf Coast.
Katrina leaves its mark
across 90,000 square miles.
Over a million people
are displaced.
Katrina becomes the standard
by which future hurricanes
will be assessed.
But even this extreme hurricane
is just a tiny brushstroke
in a much bigger picture:
a picture of how the sun drives
water around the entire planet
with radically different effects
in different places,
all under the watchful gaze
of our eyes in space.
Take just a single day in July.
In New York, commuters swelter
in 95 degree heat.
Searing winds pump hot air
into the region from the south,
creating oppressive,
humid conditions.
7,000 miles away,
in Mumbai, India,
commuters here struggle
to cope with torrential rain.
The deluge comes so fast
that the streets
are flooded in hours.
Meanwhile, in Chile,
the desert of the Atacama
is almost totally dry.
There are places here
where rainfall
has never been recorded.
Such diverse environments,
thousands of miles apart,
appear totally unrelated.
But by pulling back
for a wider view,
we can see that they are in fact
intimately connected.
Orbiting 22,000 miles
from Earth's surface
is a chain of five
weather-tracking spacecraft,
including this one:
NASA's GOES East.
GOES is an acronym
for Geostationary Operational
Environmental Satellite.
Each moves in a fixed position
relative to the earth,
called a geostationary orbit.
They always look down
on the same parts of the planet.
The combined data
from these five satellites
gives scientists a unique
perspective on the earth.
SHUCKBURGH:
By having several of them
located at different positions
around the equator,
we're able to get a view
of the whole earth
24 hours a day.
NARRATOR: By observing the entire earth,
these satellites reveal
how energy moves
throughout the globe,
beginning with the impact
of the sun on water.
The process is the same
everywhere,
but the outcome will be very
different in different places.
Converted from
the numerical data,
these five circles
graphically depict
what the satellites
actually sense.
They reveal the total picture
of water vapor produced on earth
in a single frame.
Seen here in fast forward,
one second is equal to a day.
It shows how water vapor
produced at the equator
continuously transports the
sun's energy towards the poles.
Local landscapes and topography
affect the vapor's impact,
with results unique
to each region.
In India at the end of July,
the warm water vapor is drawn
from over the ocean
by the difference in temperature
between land and sea.
Rising to high altitude,
the vapor cools over the land
and condenses back into water.
We call the result
the Asian Monsoon.
Nearly a trillion tons of rain
falls out of the sky,
transforming parched land
into fertile plains.
The monsoon eventually moves
to the east, reaching China,
where it floods the paddies
that are ideal for growing rice.
This process helps provide food
for three billion people,
almost half the world's
population.
Meanwhile, on the other side
of the world in South America,
westbound winds
drive water vapor
across the high peaks
of the Andes.
The altitude strips the air
of its moisture,
which falls as snow
on the mountains,
creating on the far side
in central Chile
the arid desert of the Atacama.
That same July day
in the eastern United States,
hot, moist air surges north
straight from
the Gulf of Mexico.
With no natural barrier
in the way,
more than 100 million Americans,
from Memphis to New York,
swelter in the summer heat.
This graphic,
based on information
provided by satellites,
depicts the interaction between
the atmosphere and the oceans
as they connect in a global
pattern of circulation
that results in our
local weather.
SHUCKBURGH:
The satellite data shows that
it's all one
interconnected system,
but that in different parts
of the world,
different processes
are happening.
We can see the monsoons
and their effect.
We can see the effects
on deserts
in a different part
of the world.
And that together shows us
how water vapor is connecting
with life on earth.
NARRATOR: But this vast cycle
of sunlight, water and land
is just one pattern among many
on this planet we call home.
A cycle with even
greater consequences
for the long-term climate
involves extreme cold.
To see how that works, we have
to turn the earth upside down
and look at it from below.
Antarctica remains the earth's
last great wilderness,
a vast frozen continent
plunged in darkness
for almost six months
of each year.
In winter,
temperatures can drop
below minus 110 degrees
Fahrenheit,
and an incessant
100-mile-an-hour gale blows.
It's hard to believe
that anything life-giving
could start here
in this bleak place.
But that's exactly
what happens.
Antarctica's ice
plays a vital part
in maintaining global climate,
sustaining life even in lush,
warm jungles
thousands of miles away.
ABDALATI: Antarctica is a fundamental
element of the climate system.
And while it may sit silently
and majestically
at the edge of the planet
for very few to see,
things go on there
that spread out
all over the world,
that affect the world
as a whole.
NARRATOR: It's a paradox that such a bleak
and barren place
is so critical
to life on our planet.
On average, it's 43 degrees
colder than the North Pole.
Why should Antarctica
be so much colder,
and how does that affect
the rest of the world?
The detectors on NASA's
polar-orbiting satellite Suomi
provide part of the answer.
The instruments sense
in the infrared and ultraviolet
parts of the spectrum.
They show that the poles receive
little of the sun's energy
and reflect most of it
back out into space.
That's one reason why the poles
stay cold.
But there's another factor that
makes Antarctica colder still.
This image has been
pieced together
from 17 different satellites
that sense the infrared,
or heat.
The continental mass
of Antarctica
lies beneath this swirling
maelstrom of cloud.
A computer model of the data
shows what happens
as the warm moist air
arriving from the tropics
collides with the cold air
over the South Pole.
The result is
a massive storm system.
And just like a hurricane,
it rotates as a result
of the spin of the earth.
Only this is much larger
than a hurricane,
4,000 miles in diameter.
Where that cold air and warm air
meet high up in the atmosphere,
the air starts to rotate
around Antarctica.
The winds can be up
in the atmosphere
as much as 200 miles an hour.
NARRATOR: This circulation pattern
is called the polar jet,
a ceaseless circle
of wind and storms.
The relentless clockwise wind,
seen here in yellow,
drives the seawater below,
shown in light blue.
DAVID ADAMEC: Those strong winds are sending
a jet around in the ocean,
and it's driving
an ocean circulation
that is felt almost all the way
to the bottom of the ocean,
two and a half miles deep.
NARRATOR: The Southern Ocean
rings the continent
with no land to interrupt
a vast body of moving water.
This is the Antarctic
Circumpolar Current.
And these are
the "Screaming Sixties,"
the roughest, most dangerous
seas on the planet.
Here, storms rage almost
every day of the year,
whipping hundreds of trillions
of gallons of water
into a ceaseless frenzy.
Now the infrared instrument
on the Aqua satellite
which senses atmospheric
temperature
puts the pieces
of this puzzle together.
The winds of the polar jet
and the water
of the circumpolar current
together form an impenetrable
barrier around Antarctica,
isolating it from the rest
of the planet
and depriving it of warmth.
That is why the whole region
remains exceptionally cold
all year round.
ABDALATI: What's incredible about
what the satellites tell us
is that the movement of air
and actually the movement
of ocean current
around the perimeter
of Antarctica
isolates the continent
from the rest of the world.
NARRATOR: So why is this relentless cold
so important to the planet
way beyond Antarctica?
The answer lies in a remarkable
property of water:
what happens when it freezes.
The Aqua satellite reveals
the start of the process.
It sweeps the surface
with its microwave scanner,
looking through the clouds
to detect the distinct
signature of ice.
SHUCKBURGH: The microwave instruments
on the satellite
enable us to see through
the clouds
to the sea ice around Antarctica
throughout the year.
What's particularly incredible
about that is
we're able to take measurements
of the sea ice
in places where as scientists,
as humans, we can't even go.
NARRATOR: This satellite gives us
an accurate picture
of the extent of sea ice
around Antarctica
over the course of a year.
Seen here in summer,
Antarctica is nearly
one and a half times the size
of the United States,
covered in ice.
But in winter,
it grows even more.
Over five and a half million
square miles of ice form
around the continent.
It grows to the size
of all of Africa.
This vast ice formation
has a profound effect
on life across the planet.
How can its impact
extend so far?
One of the best places
to understand the power of ice
is the huge bay
along the northwestern coast
of Antarctica: the Weddell Sea.
Here, a constant gale blows
and cools the seawater
to freezing temperatures.
Once the upper layer of ocean
falls below 29 degrees
Fahrenheit,
a critical threshold is crossed.
The surface of the ocean
begins to freeze.
(crackling)
At a microscopic level,
tiny crystals start to grow,
knitting themselves together.
As the crystals bond,
they expel salt into the water.
The salt forms brine that drips
down long, narrow tubes
and holes in the ice
as it forms.
The brine is denser than regular
seawater and it sinks downwards.
As winter's grip tightens,
the formation of ice
speeds up and spreads.
Soon, large slicks appear
on the surface
and thicken into a solid mass.
What started as
a microscopic process
can soon be seen from space.
Each year, more than
200 billion tons of ice form
in the Weddell Sea alone,
releasing tens of trillions
of tons of dense brine
into the ocean.
The fate of all this brine
is a mystery.
The crucial question is
where does it all go?
A satellite called Jason,
jointly operated by NASA
and the French space agency,
is providing new answers.
Jason bounces radar signals
off the surface of the ocean
to measure its height.
The instrument also reveals
the shape of the sea floor
far below.
We can make very accurate maps
of submarine bathymetry.
But we don't do that directly;
we do that by measuring the
surface of the sea from space,
very, very accurately
and over time.
NARRATOR:
Jason's radar is so precise
that it can detect
minute changes
in the level of the sea surface
produced by the peaks and
valleys of the terrain below.
The data makes it possible
to map the ocean floor.
ADAMEC: You have a satellite that's
up there, 500 miles up in space,
and it's returning an accuracy
of a little less
than half an inch.
What that means is, you know,
I've stuck this instrument
in Washington, D.C., say,
and I'm looking at a crowd
of people in Boston
and I can tell you
whether or not their toes
are over the curb or not.
That's what this satellite
is doing.
NARRATOR:
The satellite data
allows scientists to make
a three-dimensional map
of the ocean floor
beneath the Weddell Sea.
It reveals a vast chasm,
two miles deep,
off Antarctica's
continental shelf.
As the brine descends
into the ocean,
it eventually falls over
this precipice.
Other sensors attached
to the sea floor
track the flow of the brine
as it sinks.
SHUCKBURGH: What we're really
excited about is that
we're able to take that data
that shows us what the bottom
of the ocean looks like
and combine it with data
from sensors under the water.
And that enables us
to look at the dense water
and where it goes.
NARRATOR: Combining data from satellites
and undersea instruments,
scientists can reconstruct
what is happening
hidden beneath the ice.
What they learn is astounding.
One trillion gallons
of salty brine
plunge down through
the Weddell Sea every hour,
a torrent equivalent to the
volume of 500 Niagara Falls.
The brine spreads out
towards the edge
of the Antarctic
continental shelf
and then falls into the chasm
revealed by Jason.
A vast submarine waterfall
plummets downward.
The cold, dense brine
falls slowly, silently,
into the abyss,
two miles down
to the ocean floor below.
It will not resurface
for hundreds of years.
What happens to the brine next
is still being investigated.
But computer models
combined with satellite data
are helping scientists
to figure out where it goes.
This animation shows the
undersea current in action.
The purple area is the brine.
The outflow from Antarctica
drives the salty water
towards the equator,
along the sea floor.
ADAMEC: All the water in the bottom
of every ocean around the globe
has its start within six miles
of the Antarctic continent.
It creates the coldest, densest
water that's on the planet.
NARRATOR:
The cold, salty liquid
becomes part of a worldwide
circulation system,
stirring and cooling
all the world's oceans.
Leaving Antarctica,
it has embarked on a journey
that could take 1,000 years
to complete.
As it migrates
towards the equator,
the cold bottom current mixes
with fresher and warmer water
and slowly rises.
It then joins
other ocean currents
and eventually returns south,
where it cools once more.
Finally, returning
to Antarctica,
the seawater freezes
and releases its salt again,
completing the cycle.
It's an endless loop that is
critical to the whole planet.
ABDALATI: The importance of dense water
in Antarctica is that
it really forms the basis
of global ocean circulation.
The temperature
and the salt combine
to cause sinking and rising
in different parts,
which sets up
this conveyor belt,
this interaction of
all of the ocean water.
NARRATOR: In the Arctic, frigid winter
winds cause the ocean to freeze.
The North Atlantic currents
cool and sink to the bottom,
then head south again.
All over the world, slow-moving
currents of seawater like this
regulate the average
temperatures of the oceans
to within one degree.
This stability has
a profound effect on life
all across the world.
This NASA simulation shows
the surface of the entire ocean,
a web of currents
in constant motion.
But satellites show us that
the oceans don't work alone.
The currents affect the air,
the atmosphere,
that sits above them.
The ocean and atmosphere
are intimately connected.
For instance,
the Gulf Stream
takes warm water
from the Gulf of Mexico
north to the eastern
United States and Europe,
generating warm air.
On the other side
of the world,
another current
called the Kuroshio
carries heat from China
north to Japan.
ocean currents distributing heat
around the planet.
The climate we live in
is a result of ocean
circulation patterns.
The reason in the United States
that North Carolina
and South Carolina are warm
is because there is
the Gulf Stream.
And the reason there's
a Gulf Stream
really takes root in Antarctica.
NARRATOR: As a major engine driving
the world's ocean currents,
Antarctica helps protect
Earth's climate
from wild swings
in temperature.
The constant,
dependable circulation
of the oceans around the globe
and the relatively stable
temperatures it produces
have made Earth
a hospitable planet.
Long-term stability provided
time for life to flourish
and complex animals
and plants to evolve.
And this is how a process
that began with Antarctic ice
continues to sustain our world.
ABDALATI: When you put it all together,
you get a story
of how ocean circulation affects
climate and weather
and what that means today,
tomorrow
and 20 years out
into the future.
(rumbling)
NARRATOR: But ocean currents
and the atmosphere
are not the only players.
Beneath the sea floor,
forces inside the earth
are a crucial source
for the basic materials
that nurture life.
This hidden mechanism
is driven by ceaseless,
often violent activity.
Two recent examples:
A magnitude nine earthquake
strikes Japan in 2011.
An entire section
of the country
moves eight feet
towards North America.
A year earlier, 2,500 miles to
the south in Papua New Guinea,
the volcano Rabaul erupts.
It fires a vast plume of ash
high into the atmosphere.
These are catastrophic,
hugely destructive events
with an enormous cost
in human lives.
But the natural forces
behind these disasters
also provide the materials
we and other living organisms
need to survive.
And satellites help show us
how this happens.
Canada's RADARSAT is
one of several satellites
that use highly sensitive radar
to map the earth's surface
in three dimensions.
Bouncing radio waves off
the terrain below,
these satellites continually
sweep the surface of the globe.
They can measure the height
of the earth's surface every day
to an accuracy of less
than a quarter of an inch.
When the data is plotted
over time,
we can see in fine detail
how the earth's crust
is constantly moving.
This is the surface
of the crater
atop Mount St. Helens
in Washington state.
Animation reveals how it swells
over the course of three weeks,
driven by a surge of molten
magma beneath the crater.
Satellites can actually see
the crustal plates moving now.
We can see bulges and dips
where the magma is moving around
underneath the crust.
NARRATOR: This animation shows the
swelling of Mount Etna in Italy
as magma accumulates beneath it
over nine years.
When the volcano erupts,
the land sinks back.
SELLERS:
So we're getting a picture now
of what the world looks like
under the crust
and how that affects
the other dynamic processes
of the so-called solid earth.
NARRATOR: Every day, dozens of volcanoes
around the world are erupting,
while 4,000 earthquakes
shake the ground.
Our earth is dynamic,
constantly ejecting gases
and magma from its depths.
And some of this activity
has a vital impact on life.
The secret to understanding how
lies deep beneath
the ocean's surface.
Here, a crucial chemical
reaction takes place
between molten rock
and deep ocean water.
The Jason satellite's
sea surface-mapping radar
reveals a chain
of active volcanoes
a mile and a half down, at the
bottom of the Pacific Ocean.
This is where
that critical interaction
between molten rock
and freezing water takes place.
This footage was taken with
a remotely operated submarine,
also called Jason.
Lava and superheated gases
spill out of cracks
in the ocean floor,
known as hydrothermal vents.
Jason reveals what happens
when cold ocean water
penetrates into the cracks.
A magma chamber below
heats the water
to up to 750 degrees
Fahrenheit.
In the pressure-cooker
environment inside the cracks,
the dense salty water actually
dissolves the solid rock.
Complex chemical reactions
take place,
producing minerals
containing sulfur and iron.
These are nutrients that living
organisms need to survive.
The seawater, now loaded with
minerals from inside the earth,
streams out of the
hydrothermal vents.
These nutrients feed
a thriving ecosystem
that includes shrimp and exotic
creatures like tubeworms.
The deep ocean currents carry
the leftover nutrients away.
Over thousands of years, they
circulate through the oceans,
ultimately rising to the surface
and contributing to an amazing
explosion of life.
And we can see this activity
with NASA's Aqua satellite,
which is equipped
with instruments
that observe the earth
in many wavelengths
of the electromagnetic spectrum.
One tool is called MODIS.
MODIS is pretty much the crown
jewel of the Aqua satellite.
It's an enormous scanner.
So it basically covers
the whole world every day.
NARRATOR: MODIS scans the ocean
in the infrared
and the visible portions
of the spectrum.
It can detect extremely subtle
changes in the temperature
and color of the water.
So what we have in space
is an instrument
that looks at very, very small
parts of the spectrum,
and we measure how much light
comes back
in each part of the spectrum.
NARRATOR: Looking down at the west coast
of South America,
MODIS detects an upwelling
of cold water
150 miles west of Peru.
Then it detects a particular
shade of green.
This identifies the source
as chlorophyll,
a sign of plant life.
It's clear that the satellite
has spotted a massive bloom
of tiny organisms
called phytoplankton.
Just below the surface, these
phytoplankton are absorbing
the rich soup of minerals that
have come from the deep ocean.
And with light from the Sun,
and carbon from the carbon
dioxide in the air,
they multiply by the billions.
As MODIS shows, the plankton
multiply so quickly
that in just 24 hours,
500 square miles of ocean
have turned to this
distinctive green color.
GENE FELDMAN:
They replicate very, very fast.
So you can have a plankton bloom
that doubles over the course
of a day
and can cover hundreds or
thousands of kilometers
of the ocean surface.
NARRATOR: It's the minerals from beneath
the earth's crust
that have helped fuel this
vast explosion of plankton--
over 800 thousand tons of living
material.
And that's only the beginning.
This plankton is the base of
the food chain for marine life.
The bloom triggers one of
the largest feeding frenzies
on earth.
Trillions of anchovies
and sardines
feast on the tiny organisms.
They, in turn,
attract larger predators
to one of the densest
concentrations
of marine life anywhere.
Sharks converge.
And even birds, flying above,
dive down to join the feast.
And up above, humans are here,
too, taking advantage
of one of the world's most
productive fishing grounds.
The satellite data reveals
similar upwellings
all around the world, delivering
nutrients, seen here in pink,
into the surface waters.
Each upwelling triggers
a plankton bloom.
FELDMAN: Phytoplankton provide
that key link
between this energy out here,
the raw materials
that this planet holds
and the food engine
that allows life to flourish.
NARRATOR: These vast green ribbons
of plankton
can cover as much as a fifth
of the world's ocean surfaces,
about 45 billion tons of biomass
every year.
The plankton are one link
in a chain of life
that begins deep beneath
the seafloor.
The most important plant life
on this planet
are these microscopic
little green plants
that float in the ocean.
NARRATOR:
Plankton may be key to life,
but they themselves
don't live long.
MODIS shows how,
in just 72 hours,
a bloom can rapidly weaken
and fade.
All the plankton
that have not been eaten
die and sink into the abyss.
They take their precious
minerals with them
all the way back
to the ocean floor.
Here they will remain
for millennia,
a thick carpeting of tiny
carcasses half a mile deep.
Some of the minerals may
ultimately be recycled.
Some may emerge through
hydrothermal vents again,
millions of years from now.
But some plankton,
through yet another
extraordinary chain of events,
will deliver their precious
cargo of nutrients
not just to life in the ocean,
but also to life on land.
Half a world away from the coast
of Peru, where plankton bloom,
lies the Sahara Desert
in North Africa.
The Sahara is enormous--
it makes up a tenth
of the African continent.
It's one of the driest
and dustiest places on earth.
Surprisingly, the remains
of ancient plankton are here,
hidden in this arid landscape.
It is May,
the hottest month of all.
Camel herders travel through
one of the most exposed regions
of the Sahara:
the Bodele Depression.
Six thousand years ago,
this was covered by the world's
largest freshwater lake.
The floor of the lake is covered
with the ancient remains
of plankton-- called diatomite--
laid down in a much earlier age,
when an ocean covered
the region.
With its eye on the earth
from 400 miles above,
NASA's Landsat 7 is one of the
latest generation of satellites
studying the composition of
rocks that make up our planet.
It sweeps the Bodele, producing
these high resolution pictures
in multiple wavelengths
of visible light.
The white expanse
is the diatomite
on the bed of the lake.
The size of the lake is over
a thousand kilometers long
and 600 kilometers wide.
But with a satellite image,
we can see the whole extent
of the basin on a series
of images
and visualize that on a computer
in a matter of minutes.
NARRATOR:
The satellite image analysis
shows over 24,000 square miles
of sediment,
all of it diatomite.
We can map where the diatomite
sediment is
on the floor of the lake.
NARRATOR:The diatomite from the plankton
is a rich source of phosphorous,
an element needed by all living
things to produce energy.
But for this nutrient to
re-enter the chain of life,
it must first embark
on a long journey
that can be seen from space.
The journey begins here on the
ancient lakebed in the Sahara.
The wind sweeps up a few flakes
of diatomite into the air.
The flakes fracture
into a fine powder
and are carried off by the wind.
A dust storm builds.
22,000 miles above, the European
weather satellite Meteosat 8
looks down from its
geostationary orbit.
It records a daily pulse of dust
rising off the Bodele
Depression.
Here it's visible
as a whitish dust cloud
lifting from the desert
with clockwork regularity
at noon each day.
BRISTOW: Although the individual
particles of dust are minute--
they're hundredths or
thousandths of a millimeter
in diameter-- there are such
vast clouds of this dust
that you can see it
on satellite images.
NARRATOR: The dust cloud is over
a hundred stories high
and 200 miles wide.
From here it will head west
on an epic journey.
Seen from space,
the dust is blown across Africa.
At the Atlantic coast, it's
drawn up high into the sky.
This simulation,
based on satellite data,
shows how prevailing winds carry
the dust cloud west and south
3,000 miles across the Atlantic.
As much as 7,000 tons of dust
are airborne at any one time.
The destination is set
by the winds:
South America and the Amazon.
We're taking literally thousands
of tons of this dust,
which is containing phosphate,
and exporting that
from the Bodele.
The wind is carrying it out
across the Atlantic
to fertilize the Amazon.
NARRATOR: Here in these clouds
high above the rainforest,
what was once living plankton
reaches the end of its journey.
The minerals in the dust,
which include energy-giving
phosphorous,
dissolve into water droplets
and fall to the Amazon in rain.
BRISTOW: Areas like the Amazon jungle,
although they appear very rich,
the soils are actually very
depleted, they've been leached.
And one of the things that
they're short on is phosphate.
NARRATOR:
Rain falls incessantly
throughout the Amazon's
wet season,
delivering thousands of tons of
phosphate into the forest below.
It passes into the soil
and the roots of the trees,
nourishing the rain forest.
The effect of all this
natural fertilizer
can be seen clearly from orbit.
Terra is the twin
of the Aqua satellite.
It circles the earth
every 99 minutes,
monitoring how fast vegetation
is growing.
SELLERS: We can see all the green
vegetation on earth--
wall to wall, every day--
and it tells you almost
everything you want to know
about the state of life
on earth.
NARRATOR:
With its color scanner,
Terra can see the effect of
the Sahara dust on the Amazon
at the end of the rainy season.
It observes an increase
in the distinctive green color
of chlorophyll.
Like the plankton blooms
in the ocean,
the forest is kicking
into overdrive...
watered by rain
and nourished by the minerals
borne across the Atlantic
by the dust cloud.
For every leaf that exists now,
three more will grow in a week.
It's the culmination
of a chain of events
that began far back in time
and halfway around the world.
SELLERS: Ancient sediments laid down
by other organisms
millions of years ago
get eroded, make dust,
the winds bring them
across the Atlantic,
fertilize the tropical forest
in the Amazon.
NARRATOR: The migration of Bodele dust
to the Amazon
is just one of many ways
that vital minerals spread
to living habitats
all over the world.
Every landscape has
its own story
and its own way of entering
the chain of life.
BRISTOW: The exchange of nutrients
from the land
is going on
all over the globe every day.
NARRATOR: And in certain areas,
this is what accounts
for the special productivity
of the soil.
The Great Plains of North
America are rich in minerals
eroded from the Rocky Mountains.
These are vital ingredients
for growing wheat and corn.
In Bangladesh, the Ganges delta
is rich in iron
washed down from the Himalayas
in river sediments,
ideal for growing rice.
The hidden transport of minerals
creates fertile soils
that enable plants to thrive.
These minerals are the basis
of the food chain
for all life on land,
including us.
SELLERS:
All of this reminds you
how interconnected
the earth system is...
...that no living thing lives
in isolation from processes
that may happen a long way away
in both space and time
from itself.
NARRATOR: Satellites provide a vivid
new perspective on the links
between land, sea,
air and life.
This new perspective
helps us see
how the natural forces
of our planet fit together,
and that includes the atmosphere
and something as basic
as the air we breathe.
Less than a quarter
of the air around us
is comprised of oxygen, but that
oxygen is essential to life.
It's what all animals need
to burn fuel in their bodies.
Oxygen is vital to metabolism.
It provides the energy
that allows even the most active
creatures to survive and thrive
and to master
their environments.
Scientists believe
that the abundance of oxygen
in the atmosphere was essential
for the evolution of large,
intelligent mammals like us.
The human brain alone uses about
20% of the oxygen we breathe.
But where does
all this oxygen come from?
Satellites can help us answer
that question.
NASA's Aura satellite
is one of several spacecraft
that are helping scientists
study the earth's atmosphere.
Along with ground instruments,
it can analyze the atmosphere
and pinpoint its composition.
It builds a picture
of the nitrogen,
oxygen and carbon dioxide
that together make up 99%
of the air we breathe.
This computer
visualization shows
how the earth's atmosphere
changes over 24 hours.
During the day, oxygen--
seen here in blue--
rises all over the planet.
At night, carbon dioxide--
shown in orange--
is on the rise.
And the oxygen we need
is given to us by plants.
Before plants, there was
no oxygen in the atmosphere.
So plants did all the hard work
of allowing the atmospheric
concentration
to build up over time, allowing
all other life to develop.
They made the place habitable
for us.
NARRATOR: Plants breathe in carbon dioxide
and expel oxygen.
They produce so much
that the vast Amazon rainforest
is often called the lungs
of the earth.
But the real picture
is more complex.
The verdant wilderness
of plants and animals
is one of the oldest,
most abundant living systems
on earth.
Over two million square miles
of lush rainforest
teem with half the world's
living species.
SELLERS:
The Amazon is
the largest natural preserve
of life on the continents
that's left in the world.
Thousands of miles
of almost virgin forest,
thousands of species
that have been there
for an awfully long time.
NARRATOR: So dense is the Amazon jungle
that it has a dramatic impact
on the air above it.
It starts in the trillions
of leaves far below.
We can use animation to show
what this invisible process,
known as photosynthesis,
might look like.
During the day, the leaf takes
up carbon dioxide from the air,
seen here in orange.
It converts the carbon
into sugar for energy and growth
and releases oxygen,
seen in blue.
Each one of these trees
will release
hundreds of thousands of cubic
meters of oxygen
in the course of its life.
And as for the Amazon
as a whole,
a fifth of the world's oxygen
is produced here.
But there's a surprising twist:
we will breathe
almost none of it.
Satellite data and ground
measurements reveal
that almost all the oxygen the
Amazon produces during the day
remains there and is reabsorbed
into the forest at night.
SELLERS: With the advantage
of the satellites,
we can now see that the Amazon
basically uses
all its own oxygen
and uses all its own
carbon dioxide.
It is, as far as we can tell,
almost a closed system
in itself-- almost.
NARRATOR: But the Amazon still plays
a vital part
in generating the oxygen
that we breathe.
What satellites
now make clear is
producing the oxygen that
benefits us takes an extra step.
The process begins with rain,
which falls up to 250 days
a year in the Amazon.
The soil of the rainforest
is continually washed
into the Amazon river system,
taking with it nutrients
and organic material.
An average of two million tons
of this sediment
is released every 24 hours.
The sediment flows eastward,
traveling 4,000 miles
into the Amazon delta.
Here, microscopic plankton
near the surface thrive
on the nutrients and
their population explodes.
As they spread further
out to sea,
some of these tiny organisms
act like plants,
absorbing carbon dioxide
and releasing oxygen.
Again the Aqua satellite shows
us how a giant plankton bloom
grows to cover 25,000
square miles.
This vast area translates into a
huge boom in oxygen production,
made available
to the entire planet.
FELDMAN: When plankton grow,
they release oxygen.
That oxygen ultimately finds
its way into the atmosphere.
NARRATOR:
The massive scale of this impact
is revealed when the satellite
data is visualized.
This animation shows the oxygen
produced by plankton blooms,
seen here in bright blue.
The Amazon plankton bloom
releases billions of gallons
of oxygen into the atmosphere
every day.
Within a few days
the plankton die,
leaving most of the oxygen
they produced in the air
as they sink to the bottom
of the ocean.
Similar explosions
of microscopic life
happen all over the world.
Plankton's major role
in replenishing oxygen
in the atmosphere is something
we've only fully grasped
with the help of satellites.
FELDMAN:
Satellites gave us
that very first global picture,
global assessment of what
the ocean's plants were doing.
NARRATOR: And what plankton are doing is
providing life-giving oxygen
for us.
FELDMAN: Plankton in the ocean are
responsible for over half
of the oxygen that we breathe,
and it's what most creatures on
this planet rely on to survive.
NARRATOR: Microscopic organisms
as well as rainforests
are the lungs of the earth.
So what other secrets of life
can satellites--
our eyes in space-- reveal?
It turns out that another
surprising way life is sustained
is through a violent force:
lightning.
From orbit, the whole earth
buzzes with electricity.
Astronauts are often amazed
by the intensity
of the electrical storms raging
far beneath them.
SELLERS: You can see
a thousand miles' worth
of lightning flashes left and
right as you're looking down,
and they seem to set each other
off like fireworks,
bang, bang, bang, bang, bang.
It's really quite amazing.
NARRATOR: But to understand lightning's
global impact,
we need more than just
observation.
NASA's TRMM satellite carries
a high-speed camera
that can detect individual
lightning bolts.
From this information it's
possible to build a picture
showing the distribution of
lightning all across the globe.
Astonishingly, 40 strikes occur
every second.
That's more than three million
strikes a day.
So how is all this lightning
created?
And what is the effect
of all this energy
streaking through
the earth's atmosphere?
Each day, the combined force
of sunlight and water vapor
creates 40,000 thunderclouds.
The rising columns of moist air
generate powerful updrafts
that turn water vapor
into ice particles
inside the clouds.
As ice and water droplets smash
into each other at great speed,
vast charges of static
electricity build up.
An average thundercloud contains
enough energy
to power a city the size
of Denver for ten hours.
Eventually the charge builds
to a point
where air molecules
are torn apart
and a lightning bolt is born.
A bolt is no thicker
than a human thumb,
yet it's five times
the temperature
of the surface of the sun.
As it burns through
the atmosphere,
the electricity breaks apart
the molecules of nitrogen
contained in the air.
ADAMEC:
A lightning stroke,
it actually splits the nitrogen
into single nitrogen molecules.
Nitrogen doesn't like that.
It's desperately looking
for something
to connect back to with and it
often does it with oxygen.
NARRATOR: When oxygen bonds
with nitrogen,
it creates a vital nutrient
called nitrate.
Satellites show the extent
of nitrate--
simulated here in yellow--
produced by the more than three
million lightning bolts
that strike every day.
This creates about 13,000 tons
of nitrate.
It dissolves in water droplets
in the clouds
and falls to the ground in rain.
Most people are familiar
with nitrates
because they're fertilizers.
So when it rains
in a thunderstorm,
in a way you're getting a free
fertilizing,
because the water will have
nitrates in it.
NARRATOR: Nitrate is absorbed
through the roots of plants
and enters the food chain.
When we eat these plants, the
nitrates become available to us.
And so this vital nutrient
enters the cells
of every living organism
on earth,
where it is critical for
building the structure of plants
and helps make proteins and DNA
in our bodies as well.
It is essential for the survival
of all living things.
But nitrate production
is not the only way
in which lightning
promotes life on earth.
In the Canadian Yukon,
a massive wildfire devastates
over ten square miles of forest
in less than a week.
Such blazes often start with
a random bolt of electricity
from the sky.
In distant Siberia, over 1,500
square miles of forest
burn to the ground,
sparked by a lightning bolt.
These flames may seem
purely destructive,
but thanks in part
to satellites,
we see that they can
also be life-giving.
The Terra satellite can detect
the location of every fire
on earth by looking at its heat
signature in infrared.
SELLERS: Terra basically gives us a map
of all the fires
in all the forests and
grasslands of the world
every day.
NARRATOR: This sped-up visualization
of Terra's data
shows a year's worth of fire
all around the world.
The vast swaths of orange are
actually thousands of tiny dots.
Each one represents
a half square mile of land
where a fire has burned,
over 19 million square miles
in total.
The Terra data also reveal
fire's role in renewing life.
SELLERS:
The observations have shown us
how important fire is
as an element of change.
NARRATOR: The benefits of change
can be witnessed
in the forests
of northern Canada.
This is a vibrant forest,
but it has its share of dead
and diseased trees.
Locked inside them are
ingredients that are essential
for new life: elements like
carbon, sulfur and phosphorous.
Yet in a cold environment
like this,
trees take decades to decompose
and return these elements
back to the soil.
Fire can shorten the cycle
to a matter of hours.
The pine tree
is highly flammable.
It's full of sap and resins
that burn easily.
The oxygen in the atmosphere
fuels the flames.
ADAMEC:
When you're looking at fire,
you're looking at
a rapid oxidation.
That's what fire is.
NARRATOR:
Within a matter of hours,
what may have started as a spark
from a single lightning bolt
turns acres of forest to flames.
The nutrients these trees
have stored for so long
end up in the ash.
Fires also consume
the dead animals
whose bodies litter the forest,
returning the nutrients they
contain back to the soil.
The smoke climbs into the sky,
and the ultimate impact
of this nutrient-rich ash
can eventually be seen
from space.
With its infrared sensor,
Terra can pick out the heat
given off by the leaves
of healthy new vegetation
that grows after fire.
A pulse of new growth
follows every blaze.
Huge areas of forest get burned
down quite regularly
and they're followed almost
immediately by rapid regrowths.
NARRATOR:
In forests all over the world,
the data from Aqua and Terra
show that within months,
large areas devastated
by fire are rejuvenated.
From a global perspective,
wildfires are essential
to the cycle of life.
Fire's like a great blender
for all the materials
in the earth system, so when you
get dead living material,
particularly in the forests,
fire will rip through there
and decompose that stuff
very quickly into its basic
minerals and compounds
that new life can use
almost immediately.
NARRATOR: Fire is such an intrinsic part
of nature
that many plants have evolved
to make active use of it.
The pine tree drops its seeds in
the ashen aftermath of a blaze
to make the most
of the nutrients
that have been released.
Wildfires are essential
to maintaining the health
of many of the world's
ecosystems.
It's a mechanism by which
habitats that are no longer
productive regenerate.
We can now follow this process
over decades.
SELLERS: When you look 30 years
of satellite data,
you see this continuous, dynamic
rearrangement of the biosphere.
The nutrients that that tree
has pulled up from the soil
are being dropped back down
again on the soil
to feed the next generation.
The effect of all this is
to allow the biosphere
to turn over far more quickly
and efficiently.
NARRATOR: By looking at the world
from orbit,
we see our home planet anew.
We discover countless hidden
connections, all linked to life.
The circulation of weather
and ocean currents
affects the ebb and flow of ice
at the poles.
Originating
in the earth's crust,
erupting magma interacts
with cold ocean water,
producing nutrients that rise
to the surface
and nourish aquatic life.
Eventually, airborne in dust,
nutrients travel
around the planet,
finally enabling tiny plankton
to fill the air with oxygen.
That allows complex animals
like us to survive.
Oxygen also allows fire to burn,
which, in turn, accelerates
the pace of death and rebirth
in the forest.
Above all, life's major driver
is the energy we receive
from the sun.
As the earth rotates
over 24 hours,
the planet responds to the
incredible power of the sun,
our local star.
Each day more than
a million terawatts--
over 7,000 times our global
energy consumption--
strike earth.
This triggers a wave of activity
around the globe.
At dawn, plants on land
and plankton at sea
begin to photosynthesize
and grow.
At the same time,
sunlight drives wind and weather
around the globe.
We are also a part
of this cycle,
as our bodies respond
to the daily inflow of energy
from above.
Our skin cells use sunlight
to create essential vitamins.
Even the flight paths of planes
reveal our intimate relationship
with the rhythms
of day and night.
Aircraft travel west in
the morning to extend the day
and east in the evening
to reduce the night.
But while the sun nurtures
all life on earth,
it also has the power
to destroy.
And with the help of a very
different kind of satellite,
we are coming to understand just
how great a threat it can pose.
Orbiting 22,000 miles
above the earth
is the Solar Dynamics
Observatory.
This satellite looks not at
the earth, but away from it.
Its task is to observe the
radiation released by the sun--
what scientists call
space weather.
We have this wonderful
new satellite
that is up in space, looking
at the sun 24 hours a day
and is providing unprecedented
images of the sun
and where space weather is born.
NARRATOR: These striking images
are produced
by the SDO's ultraviolet sensor,
detecting light frequencies
beyond the blue end
of the visible spectrum.
The sun emits constant light,
heat and other forms
of radiation,
along with occasional dangerous
bursts of charged particles.
GILBERT:
Most people don't realize
that the earth is exposed
to charged particles
that are constantly coming away
from the sun
at about a million miles
an hour.
NARRATOR: Sometimes a massive pulse
of those charged particles
erupts from the sun's surface.
It's called
a coronal mass ejection
and it contains billions of tons
of charged particles
superheated to tens of millions
of degrees
and blasted out at millions
of miles per hour.
It has the potential to wreak
havoc on our planet.
This supercomputer visualization
shows what happens
when a coronal mass ejection
occurs.
The explosion is equivalent
to 14 million Hiroshima bombs.
It sends a cloud of charged
particles millions of miles wide
racing towards earth.
Without some kind of protection,
these enormous blasts would
strip away the atmosphere,
destroy our fragile ecosystems
and scorch the earth.
Over time, repeated coronal mass
ejections would even cause
the oceans to dry up,
leaving behind a planet
as barren and bleak as Mars.
Fortunately the earth has
an invisible shield,
a magnetic field that satellites
are now enabling us
to better understand.
Orbiting between 40,000 and
120,000 miles above the earth,
NASA has a network of satellites
called THEMIS.
Each is equipped with highly
sensitive instruments
that can detect the strength
of magnetic fields.
GILBERT:
THEMIS is a series
of probes that are aligned along
the earth's magnetosphere
and they detect variations
in the magnetic fields.
NARRATOR: This computer model,
using THEMIS data,
shows how an invisible
magnetic force field
called the magnetosphere
protects the earth.
It's generated by the rotation
of the earth's core.
GILBERT: THEMIS allows us to build
a overall picture
of the structure
of the magnetosphere
and how it operates.
NARRATOR: THEMIS reveals how
the magnetic field
is constantly blasted
by the sun.
The wave of charged particles
called the solar wind
distorts the magnetosphere into
a gigantic teardrop shape,
120,000 miles across.
As wave after wave
of solar particles
strike the outer magnetosphere,
most are deflected.
But when a coronal mass ejection
arrives,
it tears open the magnetosphere,
allowing a vast number
of charged particles
to breach the magnetic field's
first layer.
The particles are free to rush
in towards the planet.
But the earth has a second line
of defense.
Inner magnetic fields steer
the radiation
down towards the poles.
GILBERT: This process is extremely
energetic.
Particles get accelerated
and then they travel down
along the magnetic field lines
towards the polar regions.
NARRATOR:
The radiation streams downward,
encircling both
the North and South poles,
and triggers something we can
see with our own eyes,
one of nature's true wonders:
the Northern and Southern
lights, or the aurora.
As the radiation strikes
the upper atmosphere
at extreme speed, it excites
the air molecules.
This makes them glow.
The oxygen in the air radiates
red and green.
The nitrogen, red and blue.
These charged particles
that originated from the sun
get trapped and then
interact directly
with the earth's atmosphere,
causing these beautiful colors.
So when we're looking
at the aurora,
basically we're looking
at the fact
that the sun and the earth
are intimately connected.
NARRATOR:
The aurora is a vivid reminder
of how potentially lethal energy
from the sun is dissipated
in the upper atmosphere.
The earth's magnetic field has
shielded the planet
from the sun's deadly radiation
for billions of years,
enabling life to take hold
and flourish.
Satellites are revealing
one final piece
of this incredible puzzle--
the role that humanity plays.
Our human footprint
has grown so large
that we have become a major
global force in our own right.
Our impact is the consequence
of a system
that has created
and sustained life
for three and a half billion
years.
Our success as a species
has resulted
in rapid population growth.
And today our presence
can be seen
across 80% of the landmass.
Now we, in turn, are affecting
the many natural cycles
that govern our planet.
Looking for signs of pollution,
the environmental satellite
Aura's infrared sensor reveals
the atmosphere's chemical
fingerprint
and shows us how we are
affecting the entire globe.
We already manufacture more
than twice the nitrate produced
by lightning, much of it used
for fertilizer and explosives.
Our factories release
more sulfur
than all the earth's volcanoes.
Our industry and transportation
produce more carbon dioxide
than the Amazon rainforest
captures.
Our cities generate dust,
trigger electrical storms
and affect rainfall.
And these are just a few
of our impacts
on earth's natural cycles.
Our earth is changing.
We're on a path to somewhere
and our ability to understand
that path is crucial
to success in the future.
And satellites help us answer
some of the most fundamental
questions
needed to understand
how our planet behaves.
NARRATOR:
But there is one key difference
between the impact
of nature and our own.
Unlike volcanoes,
the motion of ocean currents,
or the oxygen produced by
forests and plankton blooms,
we make conscious decisions
about what we do.
And here satellites
are crucial once more.
The information they provide
can help us meet
the challenges of the future.
SELLERS: The real power of satellite
observations
is they represent
objective truth.
They tell us about what
the world actually is doing,
not what we would like it
to be doing,
not what we might fear it
to be doing,
but what it's actually doing.
And it's that that allows us
to see change,
real change, for what it is.
NARRATOR: Satellites are telling us that
the oceans are slowly warming.
In the past 30 years,
the average temperature
of the ocean's surface has risen
by half a degree.
Models suggest this extra heat
could be increasing the
intensity of hurricanes
and violent storms
all around the world.
Satellite data shows
that in Antarctica,
ice shelves that took many
thousands of years to form
are collapsing year after year.
And in the Arctic, sea ice is
diminishing at an alarming rate.
Many factors play a part
in these dramatic changes,
but most scientists agree
that human activity through
our release of greenhouse gases
is the main driving force.
All around the globe, satellites
are recording change,
but there is a problem.
Just as we are able to capture
and measure these changes,
many of the current fleet
of satellites
are coming to the end
of their lives.
Satellites need fuel
to stay in their orbits.
When their time is up,
they must either use the last of
their fuel to boost themselves
far away from the earth
or descend and burn up
on reentry.
It's predicted that the number
of NASA's earth-observing
satellite systems will go
from 20 down to fewer than ten
within the next decade.
The constant stream
of information
from these vital instruments
in space will fade.
If we fail to replace
these satellites,
we could lose our ability to
track the web of connections
that is fundamental to life.
ADAMEC: The complex interactions would
be absolutely invisible to us
without a larger view
of the earth.
It's the consistency and the
amount of data that they provide
that allows us to understand
the processes that are going on
in the earth that are important
to maintaining life
as we know it.
NARRATOR:
Little more than half a century
after the birth
of satellite technology,
we are still only beginning
to realize its possibilities.
Our planet harbors mysteries
beneath its white clouds,
blue oceans
and verdant landscapes.
And they can only be solved
with the help
of these eyes in the sky looking
down at earth from space.
== sync, corrected by elderman ==
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