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Male narrator: In the beginning,
there was darkness,
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and then, bang,
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00:00:04,504 --> 00:00:07,131
giving birth to an endless
expanding existence
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of time, space, and matter.
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Every day, new discoveries
are unlocking the mysterious,
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the mind-blowing,
the deadly secrets
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of a place we call
The Universe.
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00:00:21,854 --> 00:00:24,439
In the deep nothingness
of space,
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the cosmic silence is broken.
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- Space is actually kind of
a noisy place.
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Narrator. Galaxies, stars,
planets, and moons sing out
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00:00:39,872 --> 00:00:41,582
with strange and alien music.
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[electronic warbling]
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- They sound a little bit like
an alien fax.
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Narrator:
Now the cosmic playlist
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in a top ten countdown,
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00:00:50,049 --> 00:00:53,552
the greatest hits
of the universe...
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in a symphony of alien sounds.
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As the promo line
for Ridley Scott's
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science-fiction film Alien,
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it was designed to send chills
down your spine.
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It's based on
the unsettling idea
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that space is a vacuum,
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and sounds, whether screams,
shouts, or songs,
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can't travel in a vacuum.
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But is that really true?
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- Well, it's kind of narrow
to think that, in space,
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you can't hear anyone scream,
because, in fact, here on Earth,
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there are lots of sounds
we can't hear.
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They're either too high a pitch
or too low a pitch.
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Moreover, space
isn't completely empty.
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And then finally, you know,
what's the definition of space?
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If I'm an astronaut
on the surface of Mars
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and I have a spacesuit on,
am |I in space, or am I not?
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Well, I would think I am.
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- Okay, let's try
right over here.
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Narrator: Back on Earth,
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Bruce Bette
of The Planetary Society
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in Pasadena, California,
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has given a lot of thought
to Mars
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and the subject of sound.
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He's programmed his computer
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with what he calls
the "Mars in at or”
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to demonstrate what his voice
would sound like
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in the cold, carbon-dioxide
atmosphere of Mars...
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without those space suits.
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- The atmosphere of Mars
would actually change your voice
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so it sounded deeper.
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So let's go ahead and simulate
that using the Mars in at or,
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and I will record my voice,
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and then we will shift it
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to what it would sound like
on Mars.
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This is what
I'd sound like on Mars,
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although I'd be wishing
I had some oxygen to breathe.
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Then I go ahead and process it,
put it through the Mars in at or.
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And then we play it back
and see what it sounds like.
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[deep voice] This is
how I would sound on Mars,
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although I'd be wishing I had
some oxygen to breathe.
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Narrator: Of course, if humans
ever do make it to Mars,
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we will not hear their voices
through the atmosphere.
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Instead, we'll get them
via radio waves...
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the way many
of our most important sounds
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already reach us.
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-Yes.
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- We're familiar with thinking
of sound as something
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that comes
through the air to us,
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just like we hear each other
when we're talking,
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but, in fact,
a lot of the sounds that we hear
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are transmitted
through electromagnetic signals.
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For example, your television
actually transmits
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a television signal into sound
that you can hear.
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- Who's our first contestant
tonight?
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Narrator:
Sound in the cosmos
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will never reach us directly
across empty space,
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so radio, light,
or other electromagnetic waves
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are the inevitable carriers,
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bringing us a universe
we can hear...
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in all its variety.
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[cosmic warbling]
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- Space is actually kind of
a noisy place.
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It has many, many sources
of noise
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that we are able to detect
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with special radio telescopes,
for example.
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Narrator:
These alien sounds
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make up
an incredible collection—
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The ultimate playlist.
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We've polled our expert panel
of scientists, astronomers,
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and physicists
to rank the top ten—
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The greatest sounds
from the expanse of space...
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ending with a number one
that will surprise us all.
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And now the countdown starts.
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Coming in at number ten,
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ringing out from a distance
of 13 billion light-years,
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the birth cry of the universe
in a hit called
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"The Audio Afterglow
of the Big Bang."
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[whirring]
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- It's remarkable
that the young universe
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actually made a sound,
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and the reason we know that is
that we can actually witness
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the glowing gases that were
present at that time.
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Narrator: The glow
from these gases
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is known as the cosmic microwave
background radiation,
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or CMBR.
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It is a faint trace
of microwaves
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that stretches
across every point in the sky.
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Discovered by scientists
in the mid-1960s,
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the radiation is the afterglow
of the big bang.
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The famous blotchy satellite map
of the CMBR
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represents the cosmos
in its infancy,
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when it was only
380,000 years old.
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- When we look at the CMBR map,
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we're essentially looking
at a voice print
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of the early universe,
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because those tiny variations
in color
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correspond to variations
in temperature,
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and those correspond
to variations
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in density and pressure.
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Well, pressure waves are just
sound waves.
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So we're seeing
little variations in pressure,
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little sound waves
in the early universe.
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Narrator: To understand
the audio afterglow
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of the big bang,
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we need to know
how the early universe
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varied its pressures
to generate sound waves.
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To find out,
astronomer Mark Whittle
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and organ builder Manuel Rosales
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visit the magnificent pipe organ
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at Claremont United Church
of Christ in California.
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In a way, the 4,000 pipes
in this organ are comparable
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to the voice
of the early universe.
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[organ pipes droning]
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- Manuel, the amazing thing
about the early universe is that
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all its pipes
were sounding together,
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and it would be lovely
if we could just try that
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with this organ.
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So do you think
we could do that now,
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play all the notes at once?
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- Yes, let's pull out
all the stops and try it.
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- Ah, that's where
that phrase comes from.
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- Yes.
- Okay, let's go.
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[cacophonous droning]
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Very powerful, but really
hussy white noise kind of sound,
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but an even more remarkable
thing about the primordial sound
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is that, in fact,
a few particular tones
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were present and were stronger
at any given time.
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[cacophonous droning]
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[whirring]
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Narrator: This is the opening
note of hit number ten,
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"The Audio Afterglow
of the Big Bang."
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A computer sound analyzer
reveals its strong tones
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as distinct columns
on a color-coded graph.
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As hussy as the early
cosmic sound is,
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it differs
from pure white noise...
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which has no organized features
at all on the analyzer.
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[hissing]
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The sound of the audio
afterglow, on the other hand,
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comes through with a vaguely
musical quality.
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[whirring]
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[hissing]
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[whirring]
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[cacophonous droning]
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The pipes of this, or any organ,
are made of wood and metal,
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but the pipes
of the early universe
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were pits of dark matter,
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the mysterious substance
whose existence is known
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only from its gravity.
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- What drives the sound waves
is gravity.
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So, for example,
if there's a region
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00:09:02,249 --> 00:09:04,834
of slightly higher density
of dark matter,
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00:09:04,835 --> 00:09:06,920
there's a gravitational force
pulling in.
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Gas that's surrounding
this region feels that pull,
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and it falls in.
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But it's gas, so it also—
as it falls in, it compresses.
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00:09:15,888 --> 00:09:17,764
That compression acts
like a spring,
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and so it pushes the gas
back out.
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But then it overshoots
until it falls back in again.
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This is how the motion of
the gas falls in, bounces out,
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falls in, bounces out.
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So we have an oscillating
pressure wave, a sound wave.
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00:09:37,493 --> 00:09:39,369
Narrator: The cosmic
background radiation,
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as important as it is,
is just a still picture.
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Its imprint of sound
has the effect
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of no more than one noisy,
barely musical note.
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And even hearing that
is a struggle.
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The pipe organ
helps show us why.
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♩ ♩
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- The sounds of the universe
are way too low for us to hear.
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In fact, what's the lowest note
that this organ plays?
189
00:10:06,647 --> 00:10:08,649
- It is a pipe 32 feet long,
190
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and it can only be played
with one's foot.
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[deep note plays]
192
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- Yeah, that's pretty deep.
193
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32 feet were nothing compared
to the cosmic organ pipes.
194
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They were between 20,000
and 400,000 light-years across.
195
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- Sorry, we don't have
any pipes quite that long.
196
00:10:28,710 --> 00:10:30,461
- No.
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00:10:33,382 --> 00:10:36,968
Narrator: The deep sound
of the early universe is so low,
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we can hear it only after
a massive shift upward.
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00:10:41,014 --> 00:10:44,017
[tone zooming higher]
200
00:10:49,273 --> 00:10:51,566
The background radiation
of the universe
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00:10:51,567 --> 00:10:56,067
dates from 380,000 years
after its creation.
202
00:10:56,155 --> 00:10:58,991
But what happened before that?
203
00:10:58,991 --> 00:11:02,995
Is it possible to uncover
the whole song of the universe
204
00:11:02,995 --> 00:11:06,915
from the very instant
of the big bang?
205
00:11:14,631 --> 00:11:18,718
The cosmos is filled with
a symphony of alien sounds,
206
00:11:18,719 --> 00:11:20,887
and we're counting down
the top ten
207
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of the universe's greatest hits.
208
00:11:23,849 --> 00:11:26,351
Number ten on the playlist
sings out
209
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with the earliest tones
of the universe
210
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from "The Audio Afterglow
of the Big Bang."
211
00:11:32,399 --> 00:11:36,694
[whirring]
212
00:11:36,695 --> 00:11:39,364
But our download
of the universe's birth song
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00:11:39,364 --> 00:11:42,033
has some problems.
214
00:11:42,034 --> 00:11:45,537
With the cosmic organ playing
all its pipes at once,
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00:11:45,537 --> 00:11:47,372
what reaches our ears
sounds like
216
00:11:47,372 --> 00:11:50,708
only one complex, noisy note.
217
00:11:50,709 --> 00:11:52,711
[whirring]
218
00:11:52,711 --> 00:11:56,172
It's only one note because it
comes from the pressure waves
219
00:11:56,173 --> 00:11:59,843
we read from the map of
the cosmic background radiation,
220
00:11:59,843 --> 00:12:02,846
which is just a still picture of
the sound in the early universe
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00:12:02,846 --> 00:12:07,346
taken 380,000 years
after its birth.
222
00:12:07,684 --> 00:12:10,103
How then do we run
the clock backwards
223
00:12:10,103 --> 00:12:13,064
and hear the rest of the song?
224
00:12:13,065 --> 00:12:15,400
- Modern cosmology
is sufficiently advanced
225
00:12:15,400 --> 00:12:18,653
that it's possible to create
a computer replication,
226
00:12:18,654 --> 00:12:21,239
a simulation
of the young universe.
227
00:12:21,240 --> 00:12:25,160
It's possible to re-create
within a computer
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00:12:25,160 --> 00:12:27,745
what's going on
and how the sound developed
229
00:12:27,746 --> 00:12:29,247
right from the very,
very beginning
230
00:12:29,248 --> 00:12:33,748
through those
first 400,000 years.
231
00:12:33,752 --> 00:12:36,629
Narrator: They are the same kind
of supercomputer simulations
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that have given us pictures
233
00:12:38,257 --> 00:12:41,385
showing how the early universe
evolved.
234
00:12:45,180 --> 00:12:47,765
The dark-matter pipes
of the early universe
235
00:12:47,766 --> 00:12:51,269
acted like those
in the church organ.
236
00:12:51,270 --> 00:12:55,770
As bigger pipes were played,
deeper notes were sounded.
237
00:12:56,108 --> 00:12:57,943
As the universe expanded,
238
00:12:57,943 --> 00:13:02,364
there was more space
and more time.
239
00:13:02,364 --> 00:13:04,366
More space meant bigger pipes.
240
00:13:04,366 --> 00:13:07,035
So the notes in the song
got lower and lower
241
00:13:07,035 --> 00:13:09,037
as the song played out.
242
00:13:09,037 --> 00:13:11,914
[deep whirring, creaking]
243
00:13:16,295 --> 00:13:17,796
Put it all together,
244
00:13:17,796 --> 00:13:20,340
and the first 400,000 years
of the universe
245
00:13:20,340 --> 00:13:24,344
can be condensed down
to just ten seconds—
246
00:13:24,344 --> 00:13:27,263
A haunting primal scream.
247
00:13:27,264 --> 00:13:30,267
[whirring]
248
00:13:38,525 --> 00:13:40,652
- The gas that's falling in
and out
249
00:13:40,652 --> 00:13:42,737
of these dark-matter regions
250
00:13:42,738 --> 00:13:46,324
is ultimately going to become
the first stars,
251
00:13:46,325 --> 00:13:48,160
the first galaxies,
and ultimately,
252
00:13:48,160 --> 00:13:50,787
it'll be corralled
into the thousands of galaxies
253
00:13:50,787 --> 00:13:54,707
that we see around us today.
254
00:13:54,708 --> 00:13:59,208
So while it's been amusing,
really, and playful
255
00:13:59,671 --> 00:14:02,465
to reproduce these sounds
for us to listen to,
256
00:14:02,466 --> 00:14:06,261
in the big picture, they play
an enormously important role
257
00:14:06,261 --> 00:14:08,429
in crafting the structure
of the universe
258
00:14:08,430 --> 00:14:10,014
that's going to unfold
and the universe
259
00:14:10,015 --> 00:14:12,017
that we find ourselves in today.
260
00:14:12,017 --> 00:14:15,020
[whirring]
261
00:14:19,983 --> 00:14:22,527
Narrator: From the big-band
sound of the big bang,
262
00:14:22,527 --> 00:14:25,488
our countdown
takes a step down in size
263
00:14:25,489 --> 00:14:28,158
to the modest
15-million light-year span
264
00:14:28,158 --> 00:14:31,536
of a galaxy cluster.
265
00:14:31,536 --> 00:14:33,704
Coming in at number nine
on our list
266
00:14:33,705 --> 00:14:36,666
of the universe's
top ten hits
267
00:14:36,666 --> 00:14:39,752
is the "Deep Tone of Perseus."
268
00:14:39,753 --> 00:14:42,756
[deep warbling]
269
00:14:45,884 --> 00:14:48,720
This is low sound
to the extreme,
270
00:14:48,720 --> 00:14:50,847
emanating
from the Perseus cluster,
271
00:14:50,847 --> 00:14:54,016
a grouping
of roughly 1,000 galaxies
272
00:14:54,017 --> 00:14:58,517
250 million light-years
from Earth.
273
00:14:58,605 --> 00:15:00,940
- The central galaxy
in this cluster of galaxies
274
00:15:00,941 --> 00:15:03,985
has a huge super-massive
black hole at its center.
275
00:15:03,985 --> 00:15:08,485
Narrator: The cluster's central
galaxy is called Perseus A,
276
00:15:08,573 --> 00:15:11,867
and its super-massive black hole
gives it what's called
277
00:15:11,868 --> 00:15:14,287
an active galactic nucleus,
278
00:15:14,287 --> 00:15:17,957
which shoots out energy
in the form of gigantic jets,
279
00:15:17,958 --> 00:15:21,544
tearing
into the surrounding space.
280
00:15:21,545 --> 00:15:24,047
- For reasons which we don't
fully understand,
281
00:15:24,047 --> 00:15:26,007
it seems to be coming out.
282
00:15:26,007 --> 00:15:28,676
The energy is being produced
episodically
283
00:15:28,677 --> 00:15:31,888
about every 10 million years or so.
284
00:15:31,888 --> 00:15:36,017
Narrator. Those energy pulses
are actually waves of pressure.
285
00:15:36,017 --> 00:15:39,437
And that's exactly
what sound waves are:
286
00:15:39,438 --> 00:15:41,565
pressure waves.
287
00:15:43,775 --> 00:15:47,195
The wave, as demonstrated
by sports fans,
288
00:15:47,195 --> 00:15:50,615
has an up-and-down motion
that's very familiar to us.
289
00:15:50,615 --> 00:15:53,326
But these UC Berkeley students
will switch gears
290
00:15:53,326 --> 00:15:55,786
and show us how a sound wave
is different.
291
00:15:55,787 --> 00:15:59,624
- Okay, everyone,
lose the pom-poms!
292
00:15:59,624 --> 00:16:02,043
Since sound waves
are pressure waves,
293
00:16:02,043 --> 00:16:04,962
we're gonna build a pressure
wave out of all these students.
294
00:16:04,963 --> 00:16:07,131
Okay, everybody, let's line up.
295
00:16:07,132 --> 00:16:09,134
You go over here
and then shoulder-to-shoulder
296
00:16:09,134 --> 00:16:10,385
just like this.
297
00:16:10,385 --> 00:16:13,262
Stretch out over there
a little bit, no gaps.
298
00:16:13,263 --> 00:16:15,640
You're gonna be students
colliding with each other
299
00:16:15,640 --> 00:16:19,810
like molecules colliding
in a sound wave.
300
00:16:19,811 --> 00:16:21,771
That's looking a lot better.
301
00:16:21,771 --> 00:16:23,481
Do you feel like a bunch
of molecules?
302
00:16:23,482 --> 00:16:24,649
All: Yeah!
303
00:16:24,649 --> 00:16:26,651
- Okay, okay,
this is looking good.
304
00:16:26,651 --> 00:16:28,569
We have a bass drum
at each end of the line.
305
00:16:28,570 --> 00:16:30,029
You'll see why in a minute.
306
00:16:30,030 --> 00:16:32,657
We'll get things going
with this drummer over here.
307
00:16:32,657 --> 00:16:36,160
He's gonna hit the drum,
and watch what happens.
308
00:16:36,161 --> 00:16:37,579
Bang!
309
00:16:37,579 --> 00:16:40,331
In this case, the pressure is
a good healthy shove,
310
00:16:40,332 --> 00:16:42,125
and it moves
from student to student
311
00:16:42,125 --> 00:16:43,793
all the way down the line.
312
00:16:43,793 --> 00:16:46,754
At the end, the last student
applies his pressure
313
00:16:46,755 --> 00:16:48,757
to the second drum
by banging on it.
314
00:16:48,757 --> 00:16:51,384
Bang!
315
00:16:51,384 --> 00:16:53,386
This second drum is like
our eardrum.
316
00:16:53,386 --> 00:16:57,139
When pressure from a sound wave
in the air hits our eardrums,
317
00:16:57,140 --> 00:16:58,349
we hear the sound.
318
00:16:58,350 --> 00:17:01,019
This is just how sound travels
through the air,
319
00:17:01,019 --> 00:17:03,896
except instead of having
students shoving each other,
320
00:17:03,897 --> 00:17:06,190
there are air molecules
shoving each other.
321
00:17:06,191 --> 00:17:10,236
A sound needs a medium
to travel through.
322
00:17:10,237 --> 00:17:12,489
It can't travel
through a vacuum.
323
00:17:12,489 --> 00:17:14,908
So, in fact, to get
from point A to point B,
324
00:17:14,908 --> 00:17:17,535
you need air molecules
hitting each other.
325
00:17:17,536 --> 00:17:20,205
That's how it works.
326
00:17:23,208 --> 00:17:25,210
Narrator: So how do
those pressure waves
327
00:17:25,210 --> 00:17:27,795
from number nine's
"Deep Tones of Perseus"
328
00:17:27,796 --> 00:17:29,714
travel through
what's essentially
329
00:17:29,714 --> 00:17:34,135
the vacuum
of intergalactic space?
330
00:17:34,135 --> 00:17:37,638
Astrophysicist Richard Pogge
of Ohio State University
331
00:17:37,639 --> 00:17:40,391
gives us a sense
of the emptiness in deep space
332
00:17:40,392 --> 00:17:44,892
at his school's
football stadium.
333
00:17:44,980 --> 00:17:46,898
- While it's true
that sound waves can't travel
334
00:17:46,898 --> 00:17:49,525
through the vacuum of space,
space is not a complete vacuum.
335
00:17:49,526 --> 00:17:51,945
I'm here at Ohio Stadium,
home of the Buckeyes.
336
00:17:51,945 --> 00:17:54,197
It's very empty today.
I'm the only one here.
337
00:17:54,197 --> 00:17:55,573
And I can't think
of a better place
338
00:17:55,574 --> 00:17:58,201
to illustrate
the vacuum of space.
339
00:17:58,201 --> 00:18:00,286
Narrator: The empty stadium
can be a stand-in
340
00:18:00,287 --> 00:18:01,997
for the vacuum of space
341
00:18:01,997 --> 00:18:06,497
if we compare it with what
it looks like on game day.
342
00:18:06,751 --> 00:18:09,670
[crowd cheering]
343
00:18:09,671 --> 00:18:13,216
With more than 102,000 people
in its seats,
344
00:18:13,216 --> 00:18:16,636
Ohio Stadium would be like
the atmosphere on Earth
345
00:18:16,636 --> 00:18:20,806
jam-packed with air molecules.
346
00:18:20,807 --> 00:18:23,267
- So how much do we have to
clear out this stadium
347
00:18:23,268 --> 00:18:25,061
to equal the vacuum of space?
348
00:18:25,061 --> 00:18:27,146
Believe it or not,
you have to clear out everybody,
349
00:18:27,147 --> 00:18:30,441
including me,
and then even I'm too much.
350
00:18:30,442 --> 00:18:33,027
Narrator: No more than
a single cell from Pogge's body
351
00:18:33,028 --> 00:18:34,779
could remain in Ohio Stadium
352
00:18:34,779 --> 00:18:39,279
to come close to the vacuum
of deep space.
353
00:18:39,284 --> 00:18:42,161
With what seems like almost
nothing in the expanse
354
00:18:42,162 --> 00:18:45,415
between galaxies
of the Perseus cluster,
355
00:18:45,415 --> 00:18:49,915
the existence of sound waves
seems all the more incredible.
356
00:18:50,670 --> 00:18:52,838
- How do you propagate
a sound wave through empty space
357
00:18:52,839 --> 00:18:54,173
when it's mostly empty?
358
00:18:54,174 --> 00:18:56,384
Let's use the example of me
running down the field.
359
00:18:56,384 --> 00:18:58,886
I have to run a long ways
before I encounter somebody,
360
00:18:58,887 --> 00:19:00,305
but I still encounter somebody,
361
00:19:00,305 --> 00:19:02,974
and I can pass energy
along to them.
362
00:19:02,974 --> 00:19:05,184
The same is true of atoms
in interstellar space.
363
00:19:05,185 --> 00:19:08,146
It has to travel a long ways,
maybe 300 light-years,
364
00:19:08,146 --> 00:19:09,772
before it encounters
another particle,
365
00:19:09,773 --> 00:19:11,775
but when it encounters it,
it passes the energy,
366
00:19:11,775 --> 00:19:15,737
and the wave moves along.
367
00:19:15,737 --> 00:19:18,114
Narrator: The colliding
particles in the Perseus cluster
368
00:19:18,114 --> 00:19:21,700
also emit faint X-rays
whose traces,
369
00:19:21,701 --> 00:19:24,078
imaged by the Chandra
space telescope,
370
00:19:24,079 --> 00:19:26,331
tell us the waves are there.
371
00:19:26,331 --> 00:19:28,207
But these waves are huge,
372
00:19:28,208 --> 00:19:30,043
and the notes they produce
are lower
373
00:19:30,043 --> 00:19:34,543
than anything any human
has ever experienced.
374
00:19:35,674 --> 00:19:40,174
- The pitch is about 57 octaves
below our hearing,
375
00:19:40,178 --> 00:19:42,305
below the middle
of a piano range,
376
00:19:42,305 --> 00:19:45,182
and that actually qualifies this
for the Guinness Book of Records
377
00:19:45,183 --> 00:19:48,186
as the deepest pitch
known to man.
378
00:19:48,186 --> 00:19:50,354
[deep pulsing]
379
00:19:50,355 --> 00:19:53,024
Narrator: The extreme deep note
emanating from Perseus
380
00:19:53,024 --> 00:19:55,359
is so far below
our hearing range
381
00:19:55,360 --> 00:19:57,820
that it can only be
approximated.
382
00:19:57,821 --> 00:20:00,198
It's been said
the galaxy cluster is playing
383
00:20:00,198 --> 00:20:02,366
an awesomely low B-flat,
384
00:20:02,367 --> 00:20:05,620
and scientists calculate
it'll be playing constantly
385
00:20:05,620 --> 00:20:09,123
for 2 1/2 billion years.
386
00:20:12,711 --> 00:20:14,879
Number nine's
"Deep Tone of Perseus"
387
00:20:14,879 --> 00:20:17,923
drones on,
as the countdown advances.
388
00:20:17,924 --> 00:20:21,218
A secret number one waits
at the end of the line,
389
00:20:21,219 --> 00:20:22,720
but first...
390
00:20:22,721 --> 00:20:24,889
[high-pitched squeal]
391
00:20:24,889 --> 00:20:27,016
A strange, high-pitched squeal
392
00:20:27,016 --> 00:20:29,560
hints at what comes in
at number eight...
393
00:20:29,561 --> 00:20:33,064
sounds from space and their link
to signals from...
394
00:20:33,064 --> 00:20:35,232
extraterrestrials.
395
00:20:40,405 --> 00:20:42,073
Starting with the big bang,
396
00:20:42,073 --> 00:20:43,574
we've been tracking the top ten
397
00:20:43,575 --> 00:20:46,369
of the universe's
greatest hits—
398
00:20:46,369 --> 00:20:50,869
The best of the alien sounds
from space.
399
00:20:51,416 --> 00:20:54,669
Jumping to number eight
on the countdown,
400
00:20:54,669 --> 00:20:58,547
we find a sudden wide variety
of different sounds—
401
00:20:58,548 --> 00:21:03,048
Clicks, whines, and screeches—
402
00:21:03,803 --> 00:21:05,888
All coming from strange stars
403
00:21:05,889 --> 00:21:10,389
singing out from everywhere
we look in the galaxy.
404
00:21:10,602 --> 00:21:13,187
They're cosmic squeals
with a rhythm section
405
00:21:13,188 --> 00:21:17,192
in the "Beat of the Pulsars."
406
00:21:17,192 --> 00:21:19,652
Every pulsar has
a different sound,
407
00:21:19,652 --> 00:21:21,236
but they are all related,
408
00:21:21,237 --> 00:21:23,197
because they're repeating blips,
409
00:21:23,198 --> 00:21:26,409
beating out regular rhythms.
410
00:21:26,409 --> 00:21:28,369
The different sounds come
from beats
411
00:21:28,369 --> 00:21:30,579
sounding out
at different speeds.
412
00:21:30,580 --> 00:21:34,709
[buzzing]
413
00:21:34,709 --> 00:21:38,963
The first pulsars to be detected
emitted radio waves so regular
414
00:21:38,963 --> 00:21:43,463
that astronomers first thought
they were signals from aliens.
415
00:21:43,468 --> 00:21:47,805
But the truth about them was
quickly discovered.
416
00:21:47,806 --> 00:21:50,600
- A pulsar is a rapidly rotating
neutron star.
417
00:21:50,600 --> 00:21:52,101
That's a very dense star.
418
00:21:52,101 --> 00:21:54,937
And it's got two beams of
radiation coming out the poles.
419
00:21:54,938 --> 00:21:59,438
As those beams rotate
and intersect our line of sight,
420
00:21:59,484 --> 00:22:01,527
we see a series of pulses.
421
00:22:01,528 --> 00:22:04,822
[clicking]
422
00:22:04,823 --> 00:22:07,951
We can think of pulsars being
associated with sound,
423
00:22:07,951 --> 00:22:09,661
because they were
first discovered
424
00:22:09,661 --> 00:22:11,537
with radio telescopes.
425
00:22:11,538 --> 00:22:16,038
There was a series of beeps
that radio telescopes detected.
426
00:22:16,668 --> 00:22:19,629
For a slowly rotating pulsar,
427
00:22:19,629 --> 00:22:22,506
you might have a series of beats
like a metronome—
428
00:22:22,507 --> 00:22:25,051
Beep, beep, beep, beep.
429
00:22:25,051 --> 00:22:29,551
[metronomic clicking]
430
00:22:29,597 --> 00:22:31,974
Or you might hear
a beep-beep, beep-beep,
431
00:22:31,975 --> 00:22:33,059
beep-beep, beep-beep.
432
00:22:33,059 --> 00:22:36,270
[rapid clicking]
433
00:22:36,271 --> 00:22:38,106
[buzzing]
434
00:22:38,106 --> 00:22:39,816
Now, for a rapidly
rotating pulsar,
435
00:22:39,816 --> 00:22:41,526
the beeps blur together,
so you got...
436
00:22:41,526 --> 00:22:42,985
[trilling tongue]
Like that.
437
00:22:42,986 --> 00:22:47,486
[buzzing]
438
00:22:47,615 --> 00:22:49,033
[high-pitched buzzing]
439
00:22:49,033 --> 00:22:50,993
And for a very rapidly
rotating pulsar,
440
00:22:50,994 --> 00:22:52,662
it's just a continuous sound
441
00:22:52,662 --> 00:22:54,914
that registers like a note
in your ears.
442
00:22:54,914 --> 00:22:57,917
[high-pitched buzzing]
443
00:23:00,128 --> 00:23:02,880
Narrator: Pulsars form
from the collapse
444
00:23:02,881 --> 00:23:04,549
of very massive stars
445
00:23:04,549 --> 00:23:09,049
after they explode
as supernovas.
446
00:23:10,179 --> 00:23:12,264
But how long
does it actually take
447
00:23:12,265 --> 00:23:15,017
for a massive star to collapse?
448
00:23:15,018 --> 00:23:19,518
That's what Sherman D.
of Tampa, Florida, wanted to...
449
00:23:20,565 --> 00:23:23,568
when he texted
his question to us.
450
00:23:23,568 --> 00:23:26,320
- Sherman, the visible effects
of a supernova can last
451
00:23:26,321 --> 00:23:28,698
for months or years
or even centuries
452
00:23:28,698 --> 00:23:30,700
if you're looking
at the supernova remnant—
453
00:23:30,700 --> 00:23:32,868
The expanding gases.
454
00:23:32,869 --> 00:23:34,912
But although
it may seem incredible,
455
00:23:34,913 --> 00:23:37,665
the collapse of the core
of a massive star
456
00:23:37,665 --> 00:23:39,833
can take just a second or two,
457
00:23:39,834 --> 00:23:43,546
and that's what initiates
the supernova explosion.
458
00:23:46,257 --> 00:23:49,760
Narrator: Our own Sun isn't
massive enough to go supernova,
459
00:23:49,761 --> 00:23:52,221
but it is a giant ball
of hydrogen
460
00:23:52,221 --> 00:23:55,724
330,000 times more massive
than the Earth
461
00:23:55,725 --> 00:23:58,060
and burning by nuclear fusion.
462
00:23:58,061 --> 00:24:00,772
So our home star
can hardly keep quiet,
463
00:24:00,772 --> 00:24:03,483
as our next hit proves.
464
00:24:03,483 --> 00:24:07,983
This hot combo chimes in at
number seven on the countdown.
465
00:24:08,613 --> 00:24:13,113
Here it is,
the "Song of the Sun."
466
00:24:13,743 --> 00:24:14,994
- The Sun makes sounds,
467
00:24:14,994 --> 00:24:16,495
but they're not really
sunny sounds.
468
00:24:16,496 --> 00:24:17,914
They're not happy sounds.
469
00:24:17,914 --> 00:24:22,414
They're kind of low, ominous
roars that gurgle along.
470
00:24:22,543 --> 00:24:27,043
[low humming]
471
00:24:27,465 --> 00:24:30,134
The Sun makes sounds because
there are a bunch of gases
472
00:24:30,134 --> 00:24:33,262
going up and down through
a process called convection.
473
00:24:33,262 --> 00:24:34,805
So they're sending
pressure waves
474
00:24:34,806 --> 00:24:37,642
through the ball of gas
that is the Sun,
475
00:24:37,642 --> 00:24:39,644
and it kind of rings
like a bell.
476
00:24:39,644 --> 00:24:44,144
[low humming]
477
00:24:44,232 --> 00:24:46,734
Narrator: Unlike a bell,
the Sun rings
478
00:24:46,734 --> 00:24:50,279
with 10 million different tones
at once.
479
00:24:50,279 --> 00:24:52,322
We detect them
from the tiny bulges
480
00:24:52,323 --> 00:24:56,823
from the pressure waves
on the Sun's surface.
481
00:24:57,620 --> 00:25:01,457
Solar satellites measure
the height of the bulges
482
00:25:01,457 --> 00:25:03,750
with exquisite accuracy.
483
00:25:03,751 --> 00:25:08,251
Apart from sound,
they also produce science.
484
00:25:09,173 --> 00:25:12,259
- So using these sounds from
the Sun that we can observe,
485
00:25:12,260 --> 00:25:15,054
we can actually tell
very detailed things
486
00:25:15,054 --> 00:25:17,514
about the interior structure
of our star.
487
00:25:17,515 --> 00:25:20,684
For example, one of the amazing
things that we can tell
488
00:25:20,685 --> 00:25:24,021
is when there's a sun spot group
on the other side of the star,
489
00:25:24,022 --> 00:25:25,982
even before it comes
around the limb
490
00:25:25,982 --> 00:25:30,482
and we're able to see it
with our optical telescopes.
491
00:25:31,529 --> 00:25:33,989
Narrator: The Sun may be
the biggest source for sound
492
00:25:33,990 --> 00:25:35,658
in the solar system.
493
00:25:35,658 --> 00:25:39,286
But next in line is Jupiter.
494
00:25:39,287 --> 00:25:43,416
So coming in at number six
in the top ten is a medley
495
00:25:43,416 --> 00:25:47,086
of strange electronic
"Jazz from Jupiter."
496
00:25:47,086 --> 00:25:51,586
[whistling static]
497
00:25:52,050 --> 00:25:54,093
"Jazz from Jupiter" comes to us
498
00:25:54,093 --> 00:25:57,429
courtesy of the two legendary
Voyager spacecraft,
499
00:25:57,430 --> 00:26:01,930
now on their epic journey
to the edge of the solar system.
500
00:26:03,061 --> 00:26:04,687
- The two Voyager spacecraft
501
00:26:04,687 --> 00:26:06,397
are headed
for interstellar space.
502
00:26:06,397 --> 00:26:07,815
They're on the very outer edges
503
00:26:07,815 --> 00:26:10,067
of the bubble the Sun creates
around itself.
504
00:26:10,068 --> 00:26:13,946
Today Voyager 1 is 118 times
as far from the Sun
505
00:26:13,946 --> 00:26:15,280
as the Earth is,
506
00:26:15,281 --> 00:26:19,781
almost four times as far
from the Sun as Neptune is.
507
00:26:20,912 --> 00:26:23,372
Narrator: Project scientist
Ed Stone has been heading
508
00:26:23,372 --> 00:26:25,624
the Voyager mission
since its two spacecraft
509
00:26:25,625 --> 00:26:27,918
made their grand tour
of the outer planets
510
00:26:27,919 --> 00:26:30,379
beginning in 1979.
511
00:26:34,092 --> 00:26:36,177
On their approach to Jupiter,
512
00:26:36,177 --> 00:26:38,262
the first thing
each one encountered
513
00:26:38,262 --> 00:26:41,515
was the giant planet's
bow shock,
514
00:26:41,516 --> 00:26:45,770
producing a wind-like sound
from the electronic data.
515
00:26:45,770 --> 00:26:50,270
[wind rushing]
516
00:26:50,608 --> 00:26:52,610
- There's a wind blowing
outward from the Sun
517
00:26:52,610 --> 00:26:54,069
at about a million miles
per hour.
518
00:26:54,070 --> 00:26:55,488
It is supersonic.
519
00:26:55,488 --> 00:26:58,824
As that wind approaches contact
with a magnetic field
520
00:26:58,825 --> 00:27:02,453
around, say, Jupiter,
it has to go subsonic.
521
00:27:02,453 --> 00:27:04,830
There is a sonic shock
which forms
522
00:27:04,831 --> 00:27:07,625
in front of the magnetic field
of Jupiter.
523
00:27:07,625 --> 00:27:09,043
That's called the bow shock.
524
00:27:09,043 --> 00:27:11,170
It's very much like
a sonic shock
525
00:27:11,170 --> 00:27:12,880
in front
of a supersonic aircraft.
526
00:27:12,880 --> 00:27:16,592
[wind rushing]
527
00:27:16,592 --> 00:27:18,510
Narrator: More intriguing
than the bow shock
528
00:27:18,511 --> 00:27:20,429
is the Jovian chorus,
529
00:27:20,429 --> 00:27:22,806
sounding something like
the chorus of birds
530
00:27:22,807 --> 00:27:24,183
chirping at dawn.
531
00:27:24,183 --> 00:27:27,186
[high-pitched chirping]
532
00:27:30,731 --> 00:27:33,817
Both it and the bow shock
come from radio waves
533
00:27:33,818 --> 00:27:37,029
generated by
fast-moving charged particles
534
00:27:37,029 --> 00:27:40,198
within the bubble
of Jupiter's magnetic field.
535
00:27:40,199 --> 00:27:43,160
[wind rushing]
536
00:27:43,161 --> 00:27:45,746
[high-pitched chirping]
537
00:27:45,746 --> 00:27:48,957
Now, the scramble toward
the mysterious number one
538
00:27:48,958 --> 00:27:52,378
in the top ten
swings to the moons of Jupiter
539
00:27:52,378 --> 00:27:54,463
and the rings of Saturn,
540
00:27:54,463 --> 00:27:56,715
where the noises
from electric loops,
541
00:27:56,716 --> 00:27:59,593
glowing gases,
and streams of wind
542
00:27:59,594 --> 00:28:02,555
vie for distinction
as the spookiest sounds
543
00:28:02,555 --> 00:28:04,473
in the solar system.
544
00:28:04,473 --> 00:28:07,017
[eerie buzzing]
545
00:28:10,062 --> 00:28:11,563
The top ten countdown
546
00:28:11,564 --> 00:28:13,399
in the alien sounds
of the universe
547
00:28:13,399 --> 00:28:15,359
has reached Jupiter,
548
00:28:15,359 --> 00:28:19,859
sending out its own brand
of space music.
549
00:28:20,239 --> 00:28:22,366
But the next hit is no solo.
550
00:28:22,366 --> 00:28:25,702
Jupiter has a backup group.
551
00:28:25,703 --> 00:28:29,206
They're the Jovian moons
circling the giant planet.
552
00:28:29,207 --> 00:28:32,168
And now they have
their own album.
553
00:28:32,168 --> 00:28:35,129
It places at number five
in the top ten,
554
00:28:35,129 --> 00:28:39,629
and the tune is called
"Moons Over Jupiter."
555
00:28:40,051 --> 00:28:42,887
[electronic warbling]
556
00:28:42,887 --> 00:28:45,556
The lead singer
is the moon Ganymede,
557
00:28:45,556 --> 00:28:48,100
recorded by
the Galileo spacecraft,
558
00:28:48,100 --> 00:28:52,562
arriving at Jupiter
in late 1995.
559
00:28:52,563 --> 00:28:54,815
- The sounds that Galileo
sent back
560
00:28:54,815 --> 00:28:56,399
from Jupiter's moon Ganymede—
561
00:28:56,400 --> 00:28:58,652
By the way, the largest moon
in the solar system—
562
00:28:58,653 --> 00:29:00,112
Are very intriguing.
563
00:29:00,112 --> 00:29:02,989
They sound a little bit like
an alien fax.
564
00:29:02,990 --> 00:29:04,074
[electronic warbling]
565
00:29:04,075 --> 00:29:06,035
In fact, when I played
that sound clip
566
00:29:06,035 --> 00:29:07,536
in my office yesterday,
567
00:29:07,536 --> 00:29:10,038
people came around the corners
to see what was going on,
568
00:29:10,039 --> 00:29:12,291
if I was receiving
some alien transmission.
569
00:29:12,291 --> 00:29:15,669
[electronic warbling]
570
00:29:15,670 --> 00:29:17,254
Narrator:
As with Voyager,
571
00:29:17,255 --> 00:29:21,755
Galileo's sounds came
from ionized gas, or plasma.
572
00:29:22,927 --> 00:29:26,931
Atoms in a plasma are split
apart into negative electrons
573
00:29:26,931 --> 00:29:29,516
and positive atomic nuclei,
574
00:29:29,517 --> 00:29:34,017
in other words,
charged particles.
575
00:29:34,230 --> 00:29:35,856
Two slender antennas
576
00:29:35,856 --> 00:29:38,483
on the spacecraft's
plasma wave instrument
577
00:29:38,484 --> 00:29:39,776
picked up the radio waves
578
00:29:39,777 --> 00:29:41,528
that the charged particles
produced
579
00:29:41,529 --> 00:29:44,782
as they were set in motion
by a magnetic field.
580
00:29:44,782 --> 00:29:48,952
[electronic warbling]
581
00:29:48,953 --> 00:29:52,581
- These sounds that we hear
from Ganymede are the evidence
582
00:29:52,581 --> 00:29:55,083
that Ganymede actually has
a magnetic field,
583
00:29:55,084 --> 00:29:57,044
and you cannot find
that information
584
00:29:57,044 --> 00:29:58,837
without using
the plasma-wave instrument,
585
00:29:58,838 --> 00:30:00,422
as we did on Galileo.
586
00:30:00,423 --> 00:30:02,925
[electronic warbling]
587
00:30:05,094 --> 00:30:07,846
Narrator: A very sudden burst
of alien sound
588
00:30:07,847 --> 00:30:11,475
came from another
of Jupiter's moons.
589
00:30:11,475 --> 00:30:15,770
It happened when Galileo flew
over lo's north pole.
590
00:30:15,771 --> 00:30:20,271
[static thundering]
591
00:30:21,235 --> 00:30:22,778
- My favorite moon
in the solar system
592
00:30:22,778 --> 00:30:24,237
is Jupiter's moon lo.
593
00:30:24,238 --> 00:30:26,156
It looks a lot like a pizza.
594
00:30:26,157 --> 00:30:28,993
This is the most
volcanically active moon
595
00:30:28,993 --> 00:30:30,494
in the entire solar system,
596
00:30:30,494 --> 00:30:32,162
10 or 100 times
more volcanically active
597
00:30:32,163 --> 00:30:33,205
than the Earth.
598
00:30:33,205 --> 00:30:35,957
It literally spews tons
of material
599
00:30:35,958 --> 00:30:37,501
into space every second—
600
00:30:37,501 --> 00:30:39,711
Sulfur and oxygen atoms.
601
00:30:39,712 --> 00:30:42,923
These get ionized
in Jupiter's magnetic field
602
00:30:42,923 --> 00:30:45,300
and actually connect back
to Jupiter,
603
00:30:45,301 --> 00:30:49,763
to the north and south poles,
making a doughnut.
604
00:30:49,764 --> 00:30:52,600
Narrator: The doughnut is called
the lo flux tube,
605
00:30:52,600 --> 00:30:55,894
and the charged particles carry
a monster electric current
606
00:30:55,895 --> 00:30:59,857
between Jupiter
and its volcanic moon.
607
00:30:59,857 --> 00:31:01,900
As Galileo flew through it...
608
00:31:01,901 --> 00:31:03,068
[static thundering]
609
00:31:03,069 --> 00:31:05,780
The sound ended as abruptly
as it started.
610
00:31:05,780 --> 00:31:08,991
[static continues]
611
00:31:08,991 --> 00:31:11,159
[static stops]
612
00:31:15,373 --> 00:31:19,251
With Jupiter and its moons
finishing their acts,
613
00:31:19,251 --> 00:31:21,711
our countdown swings to Saturn,
614
00:31:21,712 --> 00:31:25,465
smaller than Jupiter but right
up there in the top ten.
615
00:31:25,466 --> 00:31:29,511
The ringed planet comes in
at number four on the list.
616
00:31:29,512 --> 00:31:33,557
Listen up for
the "Surreal Sounds of Saturn."
617
00:31:33,557 --> 00:31:35,725
[ghostly buzzing]
618
00:31:35,726 --> 00:31:38,562
They come to us
from the Cassini spacecraft,
619
00:31:38,562 --> 00:31:41,648
which has been delivering
mind-blowing pictures and data
620
00:31:41,649 --> 00:31:46,149
since its arrival
at the ringed planet in 2004.
621
00:31:47,780 --> 00:31:49,990
As on Voyager and Galileo,
622
00:31:49,990 --> 00:31:52,867
Cassini's plasma wave
instrument is our proxy
623
00:31:52,868 --> 00:31:55,537
for human ears in space.
624
00:31:55,538 --> 00:31:57,873
[ghostly buzzing]
625
00:31:57,873 --> 00:31:59,708
- The eerie and bizarre sounds
626
00:31:59,708 --> 00:32:02,794
we hear from Cassini's radio
and plasma-wave instrument
627
00:32:02,795 --> 00:32:05,172
make me think of Halloween.
628
00:32:05,172 --> 00:32:08,216
[ghostly buzzing]
629
00:32:08,217 --> 00:32:10,302
They're due to the aurora
on Saturn,
630
00:32:10,302 --> 00:32:11,928
very similar to Earth's aurora.
631
00:32:11,929 --> 00:32:14,431
[ghostly buzzing]
632
00:32:14,432 --> 00:32:16,767
Your ears could never pick up
these frequencies,
633
00:32:16,767 --> 00:32:19,019
but we move them into a range,
and when we do,
634
00:32:19,019 --> 00:32:21,438
we were surprised to see
how eerie and scary
635
00:32:21,439 --> 00:32:22,606
they actually were.
636
00:32:22,606 --> 00:32:26,568
[ghostly buzzing]
637
00:32:29,530 --> 00:32:31,240
Narrator:
The "Surreal Sounds of Saturn"
638
00:32:31,240 --> 00:32:35,740
isn't the ringed planet's
only song on the countdown.
639
00:32:36,370 --> 00:32:40,123
Turn it over, and we find
number three on the playlist:
640
00:32:40,124 --> 00:32:43,210
"Saturn's Flip Side."
641
00:32:43,210 --> 00:32:45,128
[wind blowing eerily]
642
00:32:45,129 --> 00:32:48,799
Scientists call this hit
a crossover.
643
00:32:48,799 --> 00:32:53,299
This crossover has nothing to do
with mixing musical styles
644
00:32:53,471 --> 00:32:54,889
but describes radio waves
645
00:32:54,889 --> 00:32:57,641
from Saturn's northern
and southern hemispheres,
646
00:32:57,641 --> 00:32:59,893
as they actually crisscross
in frequency
647
00:32:59,894 --> 00:33:04,148
over a period of time.
648
00:33:04,148 --> 00:33:06,483
- We saw something really
strange in our radio data,
649
00:33:06,484 --> 00:33:08,110
in our plasma-wave data—
650
00:33:08,110 --> 00:33:12,489
A couple of crossing frequencies
that apparently suggested
651
00:33:12,490 --> 00:33:14,325
that the northern
and southern hemispheres
652
00:33:14,325 --> 00:33:16,160
were rotating
at different rates.
653
00:33:16,160 --> 00:33:18,996
That's very unfamiliar to us
on a solid Earth,
654
00:33:18,996 --> 00:33:21,748
where the Earth rotates
at one rate.
655
00:33:21,749 --> 00:33:24,001
It actually turns out
we don't think Saturn's rotating
656
00:33:24,001 --> 00:33:25,419
at different rates.
657
00:33:25,419 --> 00:33:28,839
We think that high-altitude
zonal winds are tricking us
658
00:33:28,839 --> 00:33:31,383
and making us think that
there's different rotation
659
00:33:31,383 --> 00:33:33,176
in the northern
and southern hemisphere,
660
00:33:33,177 --> 00:33:34,678
but it's probably not the case.
661
00:33:34,678 --> 00:33:38,682
[electronic whirring]
662
00:33:38,682 --> 00:33:39,891
Narrator: Similar waves,
663
00:33:39,892 --> 00:33:42,853
following the lines of Saturn's
magnetic field,
664
00:33:42,853 --> 00:33:47,274
revealed a surprise
about the ringed planet.
665
00:33:47,274 --> 00:33:49,818
- One of the most bizarre things
that Cassini found
666
00:33:49,818 --> 00:33:52,654
was apparently the Saturn day
was about six minutes longer
667
00:33:52,655 --> 00:33:54,531
than it was back
in the days of Voyager,
668
00:33:54,532 --> 00:33:55,991
mere decades earlier.
669
00:33:55,991 --> 00:33:58,535
The determination of the length
of Saturn's day
670
00:33:58,536 --> 00:34:00,955
is actually not possible
by watching the clouds rotate
671
00:34:00,955 --> 00:34:02,164
around the planet.
672
00:34:02,164 --> 00:34:04,166
We have to use
these radio emissions,
673
00:34:04,166 --> 00:34:05,375
the sounds of space,
674
00:34:05,376 --> 00:34:07,795
to see what the deep interior
is doing.
675
00:34:07,795 --> 00:34:10,005
And that's where we found
this mystery.
676
00:34:12,841 --> 00:34:16,052
Narrator: It's virtually
impossible to slow down a planet
677
00:34:16,053 --> 00:34:20,223
the size of Saturn that much
in such a short time.
678
00:34:20,224 --> 00:34:23,393
So scientists now realize
the radio emissions
679
00:34:23,394 --> 00:34:27,022
probably don't give
an accurate picture.
680
00:34:27,022 --> 00:34:30,108
And by sophisticated mapping
of Saturn's winds,
681
00:34:30,109 --> 00:34:32,736
they now have a better take
on Saturn's day,
682
00:34:32,736 --> 00:34:37,236
which happens to be 10 hours,
34 minutes, and 13 seconds long.
683
00:34:38,450 --> 00:34:41,578
[electronic whirring]
684
00:34:41,579 --> 00:34:44,623
Now we're closing in
on the surface of Titan,
685
00:34:44,623 --> 00:34:46,333
Saturn's biggest moon,
686
00:34:46,333 --> 00:34:49,669
as it swings
into the Alien Sounds Countdown.
687
00:34:49,670 --> 00:34:54,170
Hit number two rings out
as "Totally Titan."
688
00:34:54,174 --> 00:34:56,843
And it opens with
an otherworldly hiss
689
00:34:56,844 --> 00:34:59,513
from an actual microphone
on the Huygens lander,
690
00:34:59,513 --> 00:35:01,139
separated from Cassini
691
00:35:01,140 --> 00:35:03,809
and parachuting through
Titan's methane atmosphere,
692
00:35:03,809 --> 00:35:08,104
nearly a billion miles away
from Earth.
693
00:35:08,105 --> 00:35:10,148
- If you're parachuting,
you're going to hear...
694
00:35:10,149 --> 00:35:11,692
[imitates wind rushing]
695
00:35:11,692 --> 00:35:14,861
That's exactly what we hear
in these Huygens sounds.
696
00:35:14,862 --> 00:35:18,365
[wind rushing]
697
00:35:18,365 --> 00:35:20,825
Narrator: The sound was
transmitted as the lander headed
698
00:35:20,826 --> 00:35:25,326
toward Titan's surface in 2005.
699
00:35:26,332 --> 00:35:29,626
- The acoustic sensor on Huygens
was essentially a microphone,
700
00:35:29,627 --> 00:35:33,172
but it only sampled
every couple seconds.
701
00:35:33,172 --> 00:35:35,924
It would take a little sound—
tiny, tiny sound bite
702
00:35:35,924 --> 00:35:38,718
and then nothing and then
a tiny, tiny sound bite.
703
00:35:38,719 --> 00:35:42,097
It wasn't planned
to turn that into sounds
704
00:35:42,097 --> 00:35:43,973
that the public could hear.
705
00:35:43,974 --> 00:35:48,061
[wind rushing]
706
00:35:48,062 --> 00:35:50,397
Narrator: But unlike
the other sounds from Saturn,
707
00:35:50,397 --> 00:35:53,483
these were not converted
from radio waves.
708
00:35:53,484 --> 00:35:57,984
They began as true sound waves
in Titan's methane atmosphere,
709
00:35:58,614 --> 00:36:00,824
and The Planetary Society
stepped in
710
00:36:00,824 --> 00:36:03,660
to convert the staccato sampling
of the microphone
711
00:36:03,661 --> 00:36:08,040
into something audible
to human ears.
712
00:36:08,040 --> 00:36:11,126
- In the end, what you hear
is mostly wind noise
713
00:36:11,126 --> 00:36:14,087
as the parachute's descending
through the atmosphere.
714
00:36:14,088 --> 00:36:16,924
And then things get much,
much quieter on the surface.
715
00:36:16,924 --> 00:36:18,008
It goes from...
716
00:36:18,008 --> 00:36:20,343
[imitates wind rushing]
717
00:36:20,344 --> 00:36:21,595
To suddenly being...
718
00:36:21,595 --> 00:36:23,221
[imitates air hissing]
719
00:36:23,222 --> 00:36:26,350
[wind rushing]
720
00:36:26,350 --> 00:36:30,850
But what's really profound is,
we're hearing sounds
721
00:36:31,188 --> 00:36:33,231
taken by
an actual acoustic sensor
722
00:36:33,232 --> 00:36:35,025
from a billion miles away.
723
00:36:35,025 --> 00:36:39,195
First time we've ever heard
sounds from another planet
724
00:36:39,196 --> 00:36:43,696
or moon around another planet.
725
00:36:43,826 --> 00:36:46,537
Narrator: But the rushing wind
wasn't the only sound
726
00:36:46,537 --> 00:36:48,121
coming from Huygens.
727
00:36:48,122 --> 00:36:50,457
As data streamed in
from the lander
728
00:36:50,457 --> 00:36:52,584
on the way to Titan's surface,
729
00:36:52,584 --> 00:36:54,794
white-knuckled engineers
in Mission Control
730
00:36:54,795 --> 00:36:57,047
held their breath,
731
00:36:57,047 --> 00:37:01,547
hoping the intrepid spacecraft
would make its landing safely.
732
00:37:02,177 --> 00:37:04,179
The final chapter in the story
733
00:37:04,179 --> 00:37:06,973
is told in
an incredible music video
734
00:37:06,974 --> 00:37:10,477
guaranteed to keep you
on the edge of your seat.
735
00:37:20,070 --> 00:37:21,404
We've been counting down
736
00:37:21,405 --> 00:37:24,116
the top ten alien sounds
of the universe,
737
00:37:24,116 --> 00:37:28,161
and we've almost reached
number one.
738
00:37:28,162 --> 00:37:32,499
But first we're shifting
into high gear...
739
00:37:32,499 --> 00:37:35,460
as number two runs
with an astronomical riff
740
00:37:35,461 --> 00:37:36,837
from the Huygens space probe
741
00:37:36,837 --> 00:37:39,756
visiting
Saturn's largest moon...
742
00:37:39,757 --> 00:37:41,842
Titan.
743
00:37:41,842 --> 00:37:46,342
It's the only alien sound that
comes with its own music video.
744
00:37:47,765 --> 00:37:49,349
Look and listen.
745
00:37:49,349 --> 00:37:53,269
Cut two on number two—
it's "Totally Titan."
746
00:37:56,440 --> 00:38:00,026
- Here we have what's called
the bells and whistles movie
747
00:38:00,027 --> 00:38:01,737
from Cassini-Huygens,
748
00:38:01,737 --> 00:38:03,405
and it's showing the descent,
749
00:38:03,405 --> 00:38:07,200
and it's a great example
of using sound
750
00:38:07,201 --> 00:38:10,120
to convey all sorts
of different kinds of data.
751
00:38:10,120 --> 00:38:12,997
[warbling and squealing]
752
00:38:12,998 --> 00:38:14,457
Narrator:
Just as a Geiger counter
753
00:38:14,458 --> 00:38:17,794
announces radioactivity
using audible clicks,
754
00:38:17,795 --> 00:38:19,963
the instruments
on the Huygens lander
755
00:38:19,963 --> 00:38:21,422
were given their own sounds
756
00:38:21,423 --> 00:38:24,134
to register the measurements
they were taking.
757
00:38:24,134 --> 00:38:28,634
[warbling and chiming]
758
00:38:28,889 --> 00:38:31,683
- Those chimes you hear—
each one of those means
759
00:38:31,683 --> 00:38:33,768
that an instrument
was taking a picture
760
00:38:33,769 --> 00:38:35,187
or some other kind of data.
761
00:38:35,187 --> 00:38:37,397
Different instruments are
a different chime.
762
00:38:37,397 --> 00:38:40,942
We also are hearing a kind of
a hum in the background.
763
00:38:40,943 --> 00:38:44,488
That's the signal strength
to the Cassini spacecraft.
764
00:38:44,488 --> 00:38:46,406
We've got a ticking that occurs
765
00:38:46,406 --> 00:38:49,242
that has to do with the spinning
and rotation of the spacecraft.
766
00:38:49,243 --> 00:38:53,455
Every time it rotates once,
they have the tick.
767
00:38:53,455 --> 00:38:55,039
Narrator:
Though it's just an assembly
768
00:38:55,040 --> 00:38:56,833
of pure scientific information,
769
00:38:56,834 --> 00:38:59,545
the video seems to preserve
what must have been
770
00:38:59,545 --> 00:39:03,549
those last moments
of high tension...
771
00:39:03,549 --> 00:39:06,343
when the scientists
in Mission Control wondered,
772
00:39:06,343 --> 00:39:09,304
"Will the tiny spacecraft
land safely,
773
00:39:09,304 --> 00:39:11,306
or will it crash?"
774
00:39:11,306 --> 00:39:14,726
[warbling and squealing]
775
00:39:14,726 --> 00:39:18,938
- So here we go,
and almost down...
776
00:39:18,939 --> 00:39:21,691
and then...
777
00:39:21,692 --> 00:39:25,779
and we're landed.
778
00:39:25,779 --> 00:39:28,239
Narrator:
Mission accomplished...
779
00:39:28,240 --> 00:39:32,118
with sound a billion miles away.
780
00:39:35,622 --> 00:39:37,540
"Totally Titan"
has been a thrill
781
00:39:37,541 --> 00:39:39,334
at number two on the countdown,
782
00:39:39,334 --> 00:39:43,834
but now we spin the platter
on the mysterious number one...
783
00:39:44,464 --> 00:39:46,048
[cosmic whistling]
784
00:39:46,049 --> 00:39:50,011
A song that comes from a place
totally unlike anything else
785
00:39:50,012 --> 00:39:53,765
in the universe
we've ever encountered.
786
00:39:53,765 --> 00:39:56,392
While some remind us
of the strange signals
787
00:39:56,393 --> 00:39:58,311
from Jupiter and Saturn,
788
00:39:58,312 --> 00:40:00,397
there are also sounds
in this song
789
00:40:00,397 --> 00:40:03,149
that are completely different
from anything we've measured
790
00:40:03,150 --> 00:40:07,650
or detected anywhere else
in the cosmos...
791
00:40:09,615 --> 00:40:11,575
because number one
on the countdown
792
00:40:11,575 --> 00:40:14,494
has sounds alien
to the entire universe,
793
00:40:14,494 --> 00:40:17,622
except for the place
where they originate.
794
00:40:17,623 --> 00:40:20,417
Number one in the universe's
greatest hits
795
00:40:20,417 --> 00:40:23,503
resounds with echoes
of a singular place.
796
00:40:23,503 --> 00:40:27,673
"The Echoes of Earth."
797
00:40:38,977 --> 00:40:42,855
- Here on Earth, we're used to
thinking of the alien sounds
798
00:40:42,856 --> 00:40:45,525
as being everything that comes
from beyond our planet,
799
00:40:45,525 --> 00:40:49,320
and that might be examples
of plasma waves
800
00:40:49,321 --> 00:40:53,116
and pressure moving through
astrophysical media or objects.
801
00:40:53,116 --> 00:40:57,328
But, really, if you think about
observing our Earth from afar,
802
00:40:57,329 --> 00:40:59,205
the aliens are us.
803
00:40:59,206 --> 00:41:00,665
And our sounds are unique,
804
00:41:00,666 --> 00:41:03,335
because they come
from living organisms,
805
00:41:03,335 --> 00:41:04,961
whether it be human language...
806
00:41:04,962 --> 00:41:07,130
[indistinct chatter]
807
00:41:07,130 --> 00:41:08,214
Or bird songs.
808
00:41:08,215 --> 00:41:11,426
[bird trilling]
809
00:41:13,553 --> 00:41:16,264
Narrator: An alien probe
exploring Earth space
810
00:41:16,264 --> 00:41:19,016
would certainly pick up the
Jupiter- or Saturn-like sounds
811
00:41:19,017 --> 00:41:23,517
of charged particles propelled
by Earth's magnetic field.
812
00:41:24,856 --> 00:41:27,191
But our planet,
unlike the others,
813
00:41:27,192 --> 00:41:29,777
also emits radio waves,
814
00:41:29,778 --> 00:41:34,115
broadcast into the cosmos
by human beings.
815
00:41:34,116 --> 00:41:37,828
[warbling and beeping]
816
00:41:37,828 --> 00:41:40,914
[static whirring]
817
00:41:40,914 --> 00:41:44,667
- Good evening, this is
Professor Reginald A. Fessenden,
818
00:41:44,668 --> 00:41:48,463
speaking to you
from Brant Rock, Massachusetts.
819
00:41:48,463 --> 00:41:51,883
Narrator: In 1906,
at Brant Rock, Massachusetts,
820
00:41:51,883 --> 00:41:54,760
Reginald Fessenden made
the first radio broadcast
821
00:41:54,761 --> 00:41:57,722
of speech and music.
822
00:41:57,723 --> 00:42:00,726
Fessenden was the inventor
of AM radio,
823
00:42:00,726 --> 00:42:05,226
transmitting his first signals
on Christmas Eve.
824
00:42:05,689 --> 00:42:10,189
It was picked up by sailors
hundreds of miles out at sea
825
00:42:10,360 --> 00:42:14,860
and has been traveling
through space ever since.
826
00:42:14,906 --> 00:42:16,616
- Ever since the beginning
of radio,
827
00:42:16,616 --> 00:42:19,243
we've really been broadcasting
out into space.
828
00:42:19,244 --> 00:42:21,496
And we've been sending out
these signals,
829
00:42:21,496 --> 00:42:23,789
in the hopes that somebody
will intercept them.
830
00:42:23,790 --> 00:42:25,917
Of course,
space is a very large place,
831
00:42:25,917 --> 00:42:27,710
and, therefore,
it's hard to know
832
00:42:27,711 --> 00:42:29,546
who would have gotten them
and when,
833
00:42:29,546 --> 00:42:34,046
but there they are on their way
out to who knows where.
834
00:42:35,719 --> 00:42:38,930
- Hello from the children
of Planet Earth.
835
00:42:38,930 --> 00:42:40,723
[woman speaking Japanese]
836
00:42:40,724 --> 00:42:43,184
Narrator. Earthly sounds are
also traveling through space,
837
00:42:43,185 --> 00:42:47,685
not by radio, but aboard the two
Voyager space probes...
838
00:42:47,856 --> 00:42:51,234
on a slow but steady course
to the stars.
839
00:42:51,234 --> 00:42:54,195
- Bonjour, tout le monde.
840
00:42:54,196 --> 00:42:57,407
- One of the examples
of how important sound is
841
00:42:57,407 --> 00:43:00,618
to us here on Earth is that
when we launched Voyager,
842
00:43:00,619 --> 00:43:03,413
we actually included
a golden record
843
00:43:03,413 --> 00:43:05,331
of sounds from our Earth.
844
00:43:05,332 --> 00:43:08,209
And this was to represent
not only human sound
845
00:43:08,210 --> 00:43:10,295
but also sounds
of the many creatures
846
00:43:10,295 --> 00:43:12,171
that live here on Earth with us.
847
00:43:12,172 --> 00:43:14,174
So it's really
a sound fingerprint
848
00:43:14,174 --> 00:43:16,342
of life on our planet.
849
00:43:16,343 --> 00:43:18,887
[dog barking]
850
00:43:21,223 --> 00:43:22,599
Narrator:
As we take our own place
851
00:43:22,599 --> 00:43:26,269
among the top ten hits
in our playlist,
852
00:43:26,269 --> 00:43:29,272
we realize they only scratch
the surface
853
00:43:29,272 --> 00:43:33,025
of the cosmic voices
calling out in the void.
854
00:43:33,026 --> 00:43:35,486
From creation
to the present day,
855
00:43:35,487 --> 00:43:39,157
space has produced
a broad catalog of sounds
856
00:43:39,157 --> 00:43:42,785
to accompany
its brilliant sights.
857
00:43:42,786 --> 00:43:45,663
As strange as
these many sounds seem,
858
00:43:45,664 --> 00:43:49,125
we've learned that they carry
important messages,
859
00:43:49,126 --> 00:43:51,962
helping to solve mysteries
of nature
860
00:43:51,962 --> 00:43:56,462
and our ultimate understanding
of the universe.
67138
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