Finding Life Beyond Earth Page #10
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- 2011
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with Earth-like qualities.
So much for theory.
The question is:
Do such planets actually exist?
Geoff Marcy is one astronomer
trying to directly answer
that question.
He's a planet hunter, scanning
the heavens for signs of planets
that may have already formed
around other stars
thousands of light years away
from our solar system.
It is actually quite a challenge
to find planets
around other stars,
and the reason is very simple--
planets don't shine.
Planets are essentially dark.
NARRATOR:
By using advanced telescopes,
dedicated planet hunters
like Geoff
have found ways to overcome
this challenge.
If you watch a star,
it ought to have the same
brightness all the time, 24/7.
But if there's a planet orbiting
that star,
when the planet crosses in front
of the star,
the planet will block a little
of the starlight
and you'll see the star dim,
a tiny amount,
every time the planet
crosses in front,
over and over in a repeated way.
And, marvelously, you can learn
the size of the planet,
because the bigger
the planet is,
the more light
from the star it blocks.
And so we learn an enormous
amount of information
about these planets
just by watching stars dim.
NARRATOR:
Not surprisingly, most of the
planets astronomers have found
this way are giant ones
that block a lot of star light.
By also observing
the gravitational pull
they have on their stars,
Geoff calculates that most
of these giant planets
are made of gas and are unlikely
to be habitable.
But the holy grail is to find
far smaller, rocky worlds,
like Earth, where the conditions
for life could exist.
MARCY:
The challenge of finding
Earth-sized planets is enormous.
When an Earth crosses
in front of a star,
it blocks only one one hundredth
of one percent
of the light from the star.
NARRATOR:
The Kepler space telescope
is designed to detect
this subtle dimming.
Its mission:
to focus on onetiny spot of space
and scrutinize 1 50,000 stars
for signs of planets
the size of Earth.
Sensitive enough to detect
minute dips in a star's light,
Kepler is already producing
mountains of data,
and thousands of new planet
candidates are being discovered.
MARCY:
Kepler has now already
discovered
a few planets that have
a diameter and a mass
that indicates clearly
the planet is rocky.
And so we now have for the first
time in human history
definite planets out there
among the stars
that remind us of home.
NARRATOR:
These first rocky planets
are too close to their stars
to sustain life.
But the sheer number
of smaller planets being found
is transforming our view
of solar systems beyond our own.
MARCY:
We've learned that nature
makes some large planets,
the size of Jupiter and Saturn,
but nature makes even more
of the smaller planets
the size of Neptune,
and even more of the planets
the size of the Earth.
The number of planets
is sort of like
the rocks and pebbles
you see on a beach.
There are a few big boulders;
there are many more rocks;
and there are an uncountable
number of grains of sand
that represent the Earth-sized
planets we see in the cosmos.
NARRATOR:
Geoff believes
it's only a matter of time
before we find
a habitable planet.
I suspect that this scene we see
here is one that's reproduced
billions of times over
among the Earth-like planets,
the habitable planets,
in our Milky Way galaxy.
NARRATOR:
But even if we find a world
just the right size
and in just the right place,
could we detect life from a
distance of trillions of miles?
The James Webb space telescope
may be able to do just that.
Due to go into orbit
later this decade,
this new telescope is three
times more powerful than Hubble.
It will be able to analyze
starlight
passing through the atmospheres
of the closest Earth-like
worlds,
looking for the telltale signs
of life itself.
good that if you find a planet
with oxygen, methane,
carbon dioxide, nitrogen,
like our own Earth,
there's probably plant life
on that planet
that is producing the oxygen.
NARRATOR:
As telescopes see farther
and spacecraft voyage closer
to distant worlds,
new discoveries are transforming
what we thought we knew
about our solar system
and our galaxy.
GREEN:
I am constantly awestruck
by the data that's coming in
our current fleet of missions.
Science fiction didn't tell us
in any way, shape or form
what we're finding out now.
SQUYRES:
Years from now, people are
gonna look back on this
exploration in the solar system.
You can only go someplace for
the first time once, right?
And we're doing that now.
NARRATOR:
Scientists are finding
organic molecules,
the raw ingredients
that life needs to take hold,
in our solar system and beyond.
GLAVIN:
I think we'd be naive to think
that this chemistry
and life here on earth
is the only place that it's
happening in the universe.
I mean the fact is that
we've got billions of galaxies,
you know, trillions
of star-forming environments
that probably have
the same chemistry going on.
NARRATOR:
The right conditions
that make a world habitable
could be more widespread
than ever imagined.
All of this leads us to think
that life should be an easy
start on another world.
NARRATOR:
And the same forces of nature
that forged life here
could be playing out elsewhere
in our galaxy.
A lovely exercise for everyone
to do
is to look up
into the night sky,
look at the twinkling lights
by and large all have planets.
And that's just our galaxy.
There are hundreds of billions
of galaxies out there
like our Milky Way,
and so the number of planets
in our universe
is a truly uncountable number.
NARRATOR:
So the race is now on
to see if life actually exists
beyond Earth.
Will life first be discovered
on a moon such as Enceladus?
Will it be found
by an advanced telescope?
Or will it be found at all?
Whatever the answer,
many believe this is a turning
point in history,
when we at last have the
technology and the know how
to find out if there is life
beyond Earth.
The exploration continues
on NOVA's website,
where you can watch any part
of this program again,
take a tour
of the solar system,
find out how we can detect
distant planets
where life might be possible,
and dig deeper into space and
flight with expert interviews,
interactives, video clips
and more.
Follow NOVA on Facebook and
Twitter, and find us online
at pbs.org.
Major funding for NOVA
is provided by:
And...
And the Corporation
for Public Broadcasting
and by PBS viewers like you.
Additional funding is provided
by Millicent Bell, through:
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