Episode Transcript
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0:00
What exactly does figuring
0:02
out if aliens exist have to do with
0:04
the end of the world. Well,
0:07
it turns out that the odd emptiness
0:09
that we find in the universe can give
0:11
us clues about what may have gone
0:13
on or didn't go on before
0:16
we humans came along. Did
0:18
something bad happen? And
0:20
if so, might it happen to us
0:22
two? Looking around
0:25
for signs of whether we're the only intelligent
0:27
life to have ever evolved can
0:29
help answer those questions. And
0:32
when you look at it, the universe does
0:34
seem amazingly large for
0:37
Earth to be the only planet with life
0:39
on it. Consider it
0:41
like this. Let's say
0:44
that you're a photon, a tiny
0:46
packet of light, and one
0:48
day you had the wherewithal this set out
0:50
to travel across the universe. You
0:53
would find that, perhaps to your great surprise,
0:55
such a trip would take you around fifty
0:58
billion years. Yes, you, light,
1:01
which can travel at the speed of light, would
1:04
take fifty billion years to cross from
1:06
one side of the universe to the other. At
1:08
least that's how long it would appear to take you to
1:10
as humans. And this is
1:13
just the observable universe. The amount
1:15
of the universe that light like you has had time
1:17
to travel across since the Big Bang. Within
1:20
that vast space, there are anywhere
1:22
from one billion to two trillion
1:24
galaxies by our current causes,
1:26
at least of which our own Milky
1:28
Way is on the larger side of the spectrum.
1:31
There are larger but there are also a lot of
1:33
smaller ones too. Within
1:35
these billions or trillions of galaxies
1:37
are billions and billions and billions
1:40
of stars, and probably exponentially
1:43
more planets. The total number
1:45
of planets and stars in our universe, the
1:47
total number of places for life to exist,
1:50
is mind bogglingly large. And
1:53
so you packet of light or wavelength,
1:56
depending on your mood, might think
1:58
to yourself, as you traveled across the verse
2:00
and saw that the Earth is the only
2:02
planet that is home to intelligent life.
2:05
Out of the attend to the who knows what power
2:07
planets that could host life, You
2:09
might think to yourself, in your little photon
2:12
voice, what waste
2:16
are we alone in the universe? And
2:18
if we are alone, why? These
2:20
are the questions at the heart of the Fermi paradox,
2:23
and they continue to nag at us. The
2:25
answer is plainly obvious if you look at
2:27
it, but it depends on how you look
2:29
at it. With the Fermi paradox,
2:32
the same thing can look very different to any
2:34
two people. And it's not just the
2:36
paradox itself. Even the evidence
2:39
is equally ambiguous. It's
2:41
all like one big contradem words
2:43
that have two meanings that are the opposite
2:45
of one another, like how weather
2:48
can mean both to wear away and to withstand
2:50
something. The size of our empty universe
2:53
can mean that we are both alone or
2:56
one of many. Another
2:58
example of this ambiguity is the very
3:00
presence of life on Earth, something
3:03
that people who believe that we're not alone in the universe
3:06
point to. His evidence is that life
3:08
here on Earth seems to have emerged the first
3:10
chance that it had. The famous
3:12
astronomer and science writer Carl Sagan
3:15
was one of those people. He was an optimist
3:18
when it came to the family paradox. He
3:20
believed that life was out there, we just
3:23
hadn't found it yet. Sagan
3:25
pointed to evidence from the fossil record that here
3:27
on Earth life began as early as
3:30
five hundred million years after the Earth form.
3:32
It was almost like it was waiting to emerge,
3:35
and since it emerged quickly here on Earth,
3:38
it stands to reason that life should emerge
3:40
wherever it gets the chance, anywhere in our
3:43
universe. When you take
3:45
into account the idea that there are perhaps three
3:47
hundred billion stars in the Milky Way alone,
3:50
even if some small fraction of those
3:52
have habitable planets that could host life,
3:55
then we should expect to encounter it sometime
3:57
soon as we spread out to explore
3:59
the country side around planet Earth. But
4:02
there's a problem with basing our view of the
4:04
rest of the universe on our own existence.
4:08
The idea that we can gain insight into
4:10
our universe from our existence is called the
4:12
anthropic principle, and it's
4:14
vulnerable to a logical fallacy called
4:16
selection bias. Being
4:18
the only intelligent life in the universe, we're
4:21
the only data point in our data set,
4:23
and so we tend to skew the results
4:26
a little bit. It's hard to resist
4:28
the temptation of cherry picking the data
4:30
when there's only one cherry. Yes,
4:33
of course, life can arise. Our
4:35
very existence proves that fact. But
4:37
what it does not prove is that the emergence
4:40
of intelligent life or any life,
4:42
really is easy or inevitable.
4:45
What if, instead, life emerging
4:47
in our universe is really, really
4:50
really hard. Perhaps
4:52
the existence of living, breathing, intelligent
4:55
things here on Earth doesn't show the emergence
4:57
of life is inevitable. Perhaps as
5:00
shows that it was the singularly most unlikely
5:02
event in the history of our entire
5:04
universe. If
5:11
you could crack open a strand of your DNA
5:14
and read the pairs of adenine, guanine,
5:17
cite of scene and dimin the
5:19
ones and zeros of your genetic code, you
5:21
would find a history of life on
5:24
Earth written into it. Not
5:26
only does your DNA contain the blueprints
5:28
for making a full version of you, but
5:30
if you look at it correctly, it also
5:33
bears the marks of those who have come before you.
5:36
You'll find your parents genes, of course, and their
5:38
parents. But as you go further back
5:40
in time, you'll also find the contributions
5:42
of all of the animals in bacteria that
5:44
ever reproduced along the last several
5:47
billion years to form a connected
5:49
chain of life that eventually led
5:51
to you. But you'll
5:53
find that you run into a wall the further you
5:55
go back. There's a point beyond
5:58
which we can no longer read the taves
6:00
of our DNA. It ends
6:02
right before we get to the emergence of life
6:04
here on Earth the very beginning. That
6:06
is to say, no one is sure how
6:09
life began as
6:12
it stands now, the general consensus
6:14
among sciences the concept of a biogenesis,
6:18
that life emerged from nothing nothing
6:20
living anyway, let's
6:22
go back to the early Earth. About five
6:25
million years after it formed, the
6:27
surfaces just begun to cool enough that
6:30
solid clay ground has begun to form,
6:32
and with the cooling off, the muggy atmosphere
6:34
cooled as well, condensing in the rain
6:37
that began to collect in pools which would
6:39
become the peatree dishes where life
6:41
took its first steps. But
6:43
to get from here to life, something
6:46
extremely unlikely had to happen.
6:49
Plain old, lifeless molecules had
6:52
to spontaneously arrange themselves
6:54
into new forms that became the
6:56
building blocks of life. At
6:58
this point, there was nothing but raw materials
7:01
on Earth, and we have to get from here to
7:03
living organisms. That
7:05
means that not only do you have a functioning organism,
7:08
it has to carry with it the encoded instructions
7:10
to make a copy of itself, and some way
7:13
to read those instructions and actually make that copy.
7:16
It's like the idea of putting some plastic
7:18
pellets and metal shavings into a bucket
7:20
and expecting an autonomous three D printer
7:23
to form from it, or
7:25
more to the point, it would be like
7:27
the idea of rotting meat growing maggots.
7:31
For a long time, humans thought
7:33
that this kind of thing spontaneous generation,
7:35
was how some life arose. Prior
7:38
to when science took up the mantle of explaining
7:40
our universe, people relied on their
7:42
everyday observations to explain occurrence
7:45
is like maggots growing on rotting meat, seeming
7:47
to appear out of nowhere. It
7:49
seemed just as likely as anything that maggots
7:51
could spontaneously generate, or
7:54
baby mice from grain, which was another
7:56
common folk belief. But eventually
7:59
scientists figured out a way to disprove this idea,
8:01
which really gained support when we realized
8:04
that tiny, unseen life lived around
8:06
us everywhere and that it had a hand
8:08
in a lot of the things that we saw. Germ
8:11
theory was developed and the concept
8:13
of spontaneous generation was abandoned.
8:16
That is until the nineteen fifties,
8:19
when researchers started working hard on figuring
8:21
out how life on Earth might have come
8:23
about. Spontaneous generation
8:26
made an unexpected comeback. A
8:29
biogenesis holds that quadrillions
8:32
upon quintillions of simple molecules
8:34
present in Earth's early atmosphere and
8:36
oceans randomly configured themselves
8:39
into a mind bending number of different combinations.
8:42
Some of these abominably large number
8:44
of combinations happen to create useful complex
8:47
molecules like amino acids, which
8:49
are the precursors for proteins. Now,
8:52
it's one thing to form simple molecules
8:55
to randomly combined to form more complex
8:57
molecules, but there is still the issue
8:59
of replication. Ship If those
9:01
molecules don't make a younger copy of themselves,
9:04
that innovative chemical chain is broken
9:06
and the new molecule loses the chance to
9:08
continue to evolve in a new and even more
9:10
complex things. And
9:12
this is the point where science is currently stuck.
9:15
Somehow, they say, some of those molecules
9:18
managed to form a stable string of
9:20
nuclear times, probably r N,
9:22
a ribonucleic acid which
9:25
is capable of doing two very important
9:27
things. It can encode information
9:29
in its nuclear tide chain, and it
9:32
can also transcribe those nuclear tides
9:34
to produce proteins. And once you
9:36
have proteins, you can do all sorts
9:38
of things that supports life. Back
9:41
in two organic
9:43
chemists Stanley Miller and Herald Urray
9:45
saw it to show that this was possible by recreating
9:48
the conditions of earlier Earth. In a flask. They
9:51
simulated a primitive ocean and built
9:53
an atmosphere out of the gases thought back
9:55
in the fifties to have been present on Earth soon
9:57
after it formed. They mimicked
9:59
why in storms with the flickering electrical
10:01
current, and when Miller inspected the
10:03
broth that resulted, he found
10:06
that nineteen amino acids and amans,
10:08
the precursors to proteins, had assembled
10:10
spontaneously. It
10:12
seems that Miller had shown that when the conditions
10:15
were right, the foundations for life would
10:17
arise. But
10:19
lately the idea that a biogenesis
10:21
just happened randomly is falling out
10:24
of favor. Instead, some
10:26
scientists have begun to suspect that there
10:28
is some set of organizing principles
10:30
that serves as a driving force for life
10:33
to emerge. Just like how
10:35
gravity will draw a ball downhill, or
10:37
how magnets will always repel or attract
10:40
one another when they're close together, there
10:42
is some fundamental governing force of nature
10:45
that causes life to assemble along
10:47
predictable lines. We just
10:49
haven't figured out what that force or those lines
10:52
are yet. This is
10:54
a pretty surprising idea if you think of
10:56
it. One of the laws of the universe,
10:59
the second law of therm mom dynamics, is
11:01
that things tend towards disorder, not
11:04
order. The idea that, when presented
11:06
with the right conditions, dead molecules
11:08
in the universe will organize themselves
11:10
into something living and breathing runs
11:13
totally counter to that, and
11:15
this new view also includes evolutionary
11:17
biology as one stretch of these
11:19
organizing principles of life. So
11:22
the idea is that molecules arrange themselves
11:25
into self replicating, metabolizing
11:27
parts that form increasingly complex
11:29
beings that eventually include you and
11:32
me, which makes you wonder
11:34
what the end point is. To
11:53
some people, the idea that life arose
11:55
from simple dead molecules that just happened
11:57
to randomly assemble themselves in the
12:00
living things is just too
12:02
unlikely to accept, And
12:04
even if we do accept that this is precisely
12:07
how life arose on Earth, the
12:09
idea that it could ever happen again anywhere
12:11
else is too improbable.
12:14
That virtually proves that we humans
12:16
are alone in the universe. One
12:19
issue people raise is time. They
12:22
say that Earth just simply hasn't been around
12:24
long enough for all of that random
12:26
chemical trial and error to have taken
12:28
place. The idea that life
12:31
organizes along some unknown universal
12:33
principles definitely addresses that idea
12:35
of time, and so does pant spermia.
12:38
Pant Spermia is a concept from astrobiology,
12:41
and it says that the seeds of life are
12:44
all over the universe in abundance everywhere.
12:46
They can be found on board asteroids
12:48
and other celestial objects, and
12:50
that these seeds of life are constantly bombarding
12:53
planets all over the universe.
12:56
If the conditions on the planet happen to be right,
12:59
well, then those sea needs of life will germinate
13:01
and grow into something new and living.
13:04
This certainly addresses the issue of time.
13:07
Life could have evolved elsewhere in the universe,
13:09
which is billions of years older than Earth, and
13:12
then spread to our planet aboard an asteroid.
13:15
We've recently found that some chemical
13:18
precursors to life can be found on celestial
13:20
objects like asteroids, and that they're
13:22
able to survive re entry into an atmosphere,
13:24
which can get pretty hot. This is
13:27
important because it's widely accepted that
13:29
an atmosphere is a precondition for life
13:31
to emerge. If you
13:33
take pants bermia, and you take the recent view
13:35
that life follows some organizing principles
13:38
as immutable as the laws of physics, then
13:40
you arrive at a conclusion that Earth
13:43
is just another place that happened to have the
13:45
right conditions when a rock bearing
13:47
the precursors to life landed around
13:49
four billion years ago. In
13:52
this view, then of course life
13:54
is abundant in the universe. But
13:57
then we find ourselves right back to where we
13:59
started. Where is everybody?
14:02
Perhaps the best answer to that comes not
14:04
from an astrobiologist or an astronomer,
14:07
but from an economist named Robin
14:09
Hansen, who proposed that
14:12
there must be something, some incredibly
14:14
difficult step between the point where
14:16
dead matter forms life and the point
14:18
where intelligent life becomes a galactically
14:21
colonizing civilization that
14:23
no species has ever been able
14:25
to overcome. He calls
14:27
it the great filter. Every
14:30
piece of matter in the universe is the sort of thing that could
14:32
have started that process, started
14:34
life, and then advanced life, etcetera. But
14:38
so far nothing out there has done
14:40
that. So the great filter is whatever is
14:42
in the way, whatever makes
14:45
it hard for any one piece of ordinary
14:47
dead matter to produce expanding, lasting
14:49
life. There's surely a countless
14:52
number of steps along the path from dead
14:54
matter to the emergence of a galactically
14:56
visible civilization. But the
14:58
Great Filter high Path says, supposes
15:00
that a handful of them are really, really
15:03
hard, and that one of them in particular
15:06
must be so hard that is thus
15:08
far prevented any life from reaching
15:10
galactic proportions.
15:13
This is Oxford University philosopher
15:15
Toby ord if there
15:17
were a hundred pieces you needed to get into the
15:19
right order in order to create something that
15:22
obeyed natural selection and and was
15:25
it the basic level needed
15:27
to actually bootstrap up towards
15:29
complex life, then there are a hundred
15:31
factorial ways you could arrange
15:34
those pieces. That's that's more than uh
15:36
tends to the power of a hundred different possibilities.
15:39
And then it just turns out you need an incredibly
15:41
rare event to get there. The Great
15:43
Filter offers two possible solutions
15:45
to the question posed by the Fermi paradox.
15:48
Whereas everybody everybody
15:50
never existed, or everybody
15:53
is dead, if the
15:55
Great Filter is in our past, it says
15:57
pretty strongly that we are the first and
16:00
only intelligent life that exists
16:02
in the universe. If that's
16:04
true, then by the Great Filter, there
16:07
is something, some step, some
16:09
right of passage you could call it, that
16:12
has prevented every other life from
16:14
reaching the point that we're at. And
16:17
if that's the case, then we are the only
16:19
life to have made it through the Great Filter.
16:23
That means that we can be optimistic about our future.
16:27
We made it through that right of passage that has
16:29
kept every other attempt at life from evolving.
16:32
It means our big, vast universe isn't
16:34
wasted on us. It's just waiting
16:36
there for us to use it, and
16:38
guilt free too. Since no one else
16:41
is around to use it, we have a
16:43
responsibility to put it to use.
16:45
You could even say. But
16:47
there's another possibility to the Great
16:49
Filter too. It may also
16:51
lie just ahead in our future.
16:55
Maybe intelligent life is a dime a dozen
16:57
in the universe. But the reason we don't
16:59
see other civilizations is
17:01
because they've all died off. And
17:04
if all of those intelligent civilizations
17:07
all died before any
17:09
any of them could make it off
17:11
of their home planet and spread throughout the universe,
17:15
the Great Filter is a big red flag
17:17
for us. It
17:19
tells us that we should expect to meet the same
17:21
fate that every other intelligent
17:24
life has. The Great Filter
17:26
will spell the end of the world for
17:28
us too. To
17:30
answer the question of whether we face imminent
17:32
doom or not, we have to look at the
17:35
evolution of life, and to
17:37
do that we have no choice but to
17:39
turn to the one place where we know life
17:41
evolved. At the risk of
17:43
falling victim to the selection bias, we
17:45
have to look to Earth for clues. We've
17:49
already talked about how utterly improbable
17:51
the origin of life appears to have been, but
17:54
it's probably best to start looking even
17:56
further back than that. If
18:01
life emerged on Earth, that means that the conditions
18:03
were right for life on Earth. That's
18:05
the one day to point we have ipso fact,
18:08
though, so the best way to find out
18:10
what conditions life requires is
18:12
to look at the conditions of our planet. And
18:15
it turns out that Earth has
18:17
some spectacularly peculiar characteristics
18:20
that make it ripe for life. So
18:22
peculiar, in fact, that a pair
18:24
of researchers named Peter Ward and Donald
18:27
Brownlee rolled all of them up into
18:29
what they call the rare Earth hypothesis. It's
18:31
just what it sounds like when you add up
18:34
all of its peculiarities. Earth
18:36
is not like other planets. First,
18:39
Earth happened to form around the right kind of star.
18:42
Our son is a main sequence star, which
18:45
means it produces light and heat by
18:47
fusing hydrogen into helium.
18:49
Main Sequence stars aren't rare. They
18:51
make up about nine of stars.
18:53
But our Son also happened to be of the right size
18:56
too. It's not so large that it
18:58
will use up its fuel in just a few billion
19:00
years. That means that the Sun's
19:02
slow, steady burn would go on long enough
19:05
to give life time to develop. The
19:07
Sun also isn't too small to support life
19:09
either. It is you could say,
19:12
just right for life. Our
19:14
Sun has also placed in a really great spot in our
19:17
galaxy. We happen to be located
19:19
out in the country, in a bit of a backwater
19:21
when it comes to the Milky Way, about
19:23
twenty eight thousand light years from the galactic
19:26
center, in a galaxy that's one thousand
19:28
light years across. For decades,
19:31
study presumed that the center of the galaxy
19:33
would be the most happening spot. That's
19:35
where the most stars tend to be, and more
19:37
stars would be more potentially habitable
19:40
planets. Civilizations
19:42
that arose in the center might even be in contact
19:44
with one another, forming something of a galactic
19:46
urban area. But recently
19:49
it's become clear that the galactic center
19:51
might not be so flourishing. After all. There
19:54
are more stars, sure, but more
19:56
stars also means that there are more collapsing
19:58
stars, which release bursts of
20:00
energy that can burn away the atmosphere of any
20:02
planets in the vicinity, So
20:05
the galactic center might actually be less
20:07
of a bustling urban area and more
20:09
like sterile and dead. Our
20:12
Sun is pretty far away from the galactic center,
20:14
way out past the suburbs where nothing
20:17
much happens. In other words, that's
20:19
good for life on Earth because it means that
20:21
it cuts down on the number of sterilization
20:23
events as life developed over Earth's
20:25
history, giving it a good chance of
20:27
succeeding. And Earth
20:30
just so happens to be located within the
20:32
Sun's goldilocks zone that I mentioned in the last
20:34
episode. If it was a little nearer
20:36
the Sun and about one and a half million kilometers
20:39
closer, it would be too hot to support
20:41
life, and much further away
20:43
Earth would be too cold for it.
20:46
It also turns out that where Earth is positioned
20:48
in the Solar System is hugely
20:50
important to giving life a fighting chance.
20:53
Earth is the third rock from the Sun, with
20:56
five others between us and the rest of the galaxy.
20:59
Six if the math that suggests there's a
21:01
planet nine out there turns out to be correct,
21:04
or if you continue to count hapless Pluto,
21:07
the Sun and the planets in our Solar System
21:09
formed from a massive cloud of cosmic
21:11
dust, that same stuff that might have
21:13
blown up so many alien pilots traveling
21:16
between the stars. We still
21:18
aren't quite sure exactly how the planets
21:20
formed. One model astoundingly
21:22
suggested that they could have formed in as little
21:24
as a thousand years, but
21:26
the birth of the Solar System was likely a
21:28
free for all grab of the elements that
21:30
make up the planets today. Initially,
21:33
astronomers presumed that the planets formed
21:36
in their current arrangement, but lately
21:38
it's become clear that that probably wasn't
21:40
the case. The planets may have actually
21:42
moved around and migrated from one
21:44
spot to another in the early life of the Solar
21:47
System before settling into the arrangement
21:49
that we see them in today. If
21:52
that's correct, then we were astoundingly
21:54
lucky that Jupiter ended up where it didn't.
22:02
Jupiter is a gas giant made up
22:04
largely of hydrogen and helium with a metal
22:06
and ice core. It's like a Sun that
22:08
never started burning because it lacked the
22:10
mass needed for gravity to kick start
22:13
fusion. But Jupiter is
22:15
massive, truly, you could
22:17
fit around within it.
22:20
It's the most massive planet in our Solar
22:22
System, and because of its mass
22:25
and its position between Earth and the chaos
22:27
of the interstellar space outside of
22:29
our Solar System, Jupiter acts
22:31
as a huge defensive guard for our
22:33
planet. When asteroids or comets
22:36
or other flotsam and jetsam bent on destruction
22:38
in oer our Solar System, Jupiter's
22:41
extraordinary gravitational pull draws
22:43
them into its orbit and slingshots
22:45
them out back into space. Without
22:48
Jupiter to run interference for Earth, it
22:50
would have a steady diet of life ending
22:52
bombardments from space. So
22:55
thanks Jupiter. This
22:58
is astronomer Donald brown Lee. He's
23:00
one of the guys who came up with the rare Earth hypothesis.
23:03
Jupers are actually pretty
23:05
rare uh planets
23:09
and um uh so uh
23:12
in terms of rare Earth. You know whether
23:14
it was juper is good or bad. Typical
23:16
planet as systems probably don't have jupers.
23:19
Our moon, too, seems to have played a number
23:21
of factors and fostering life on
23:23
Earth. Our moon's pretty
23:26
unusual itself as far
23:28
as moons go. It's enormous. It's
23:30
about one point to percent the mass of the
23:32
Earth and doesn't sound like much. But
23:34
other planets moons like Phobos and Demos,
23:36
which or a bit Mars, are closer to
23:38
asteroids in size. Our moon
23:41
more resembles a small planet, and
23:43
because it's so big, it has some very
23:45
peculiar effects on Earth. For
23:47
one, it stabilizes our planet. The
23:50
Earth doesn't sit upright as it spins around
23:52
on its axis. It's tilted actually
23:55
at about a twenty three degree angle.
23:58
Because of this tilt, we have seas which
24:00
create predictable variations in the temperature
24:03
of regions on Earth over the course of
24:05
the year. So when you think
24:07
about the difference between winter and summer,
24:09
you get a good idea how much variation a
24:12
tilt can create. And add
24:14
more of an angle to the tilt and the Earth
24:16
and the temperature variations would become more
24:18
severe. Since during winter or hemisphere
24:21
would be further away than it is now from the
24:23
Sun and much closer in the summer.
24:26
And if you added in some wobble, like if
24:28
the tilt of the Earth wasn't stable and fluctuated,
24:31
all of these wild swings and temperature
24:33
could make it very difficult for life to take
24:35
hold. The Moon's mass
24:38
actually exerts gravity over Earth and keeps
24:40
it stable, not wobbling or tilting
24:42
more than it does, and allowing for a
24:44
nice, gradual, predictable
24:46
and not two varying seasonal temperature
24:49
shifts that we even have
24:51
a moon appears to be a fluke itself. The
24:54
current view is that the Moon was calved off
24:56
from Earth following a head on collision in
24:58
the Earth's early history with a planetoid
25:01
about the size of Mars called Thea, which
25:03
the Earth likely absorbed. This
25:05
giant impact hypothesis explains
25:08
a lot. The Moon is unusually
25:10
large and unusually close to us
25:12
because it was created of a mixture of Earth and
25:14
that fateful planetoid. Because
25:17
the Moon is so close to Earth, it's tidally
25:19
locked and orbit around us. It doesn't
25:22
spin on its axis, which is why we
25:24
always see the same side of the Moon as
25:26
it orbits us. This is an important
25:28
feature because it also creates the tide
25:31
you're on Earth. As
25:33
the Moon orbits Earth, it pulls the oceans
25:36
toward it, stretching them out on the
25:38
ends and narrowing them in the middle. We
25:41
hear on our planet experience this as low
25:43
tide or high tide, depending on where you are.
25:46
And it was in these tidal pools of young
25:48
Earth's oceans where some people think
25:50
life began. When
25:55
those ancient tides came in, they deposited
25:58
a flood of molecules into the tidle pools,
26:01
and as they withdrew and the water evaporated
26:03
in the sun, the increasing concentration
26:05
of salt could have provided just the right
26:08
laboratory conditions where those earliest
26:10
chemicals could combine. Without
26:12
a moon as large and as close as ours is,
26:15
these tides could not have existed on Earth,
26:17
and those early proteins would have lacked that
26:19
kind of natural peatrie dish.
26:22
So the moon itself is a collection
26:24
of exquisite coincidences that supported
26:26
life on Earth. But perhaps the
26:28
most peculiar aspect of Earth is
26:31
that it has massive plates that make up the
26:33
crust, which slide along a molten
26:35
bed underneath that. It, in
26:37
other words, features plate tectonics.
26:39
It thought that this is a major
26:42
reason why the Earth has actually
26:44
had an amazingly stable
26:47
climate for most of you know, temperatures
26:49
for for most of its uh
26:51
age. So it's drastically different
26:54
than Venus or or
26:56
Mars, which are famously unstable
26:59
over tri lage uh time scope.
27:01
So so we really owe a lot uh
27:03
to this. We don't really know why I played
27:06
tectonics works on
27:08
our on Earth. It doesn't work on Mars, it
27:10
doesn't work on vines, it doesn't work on mercury,
27:12
doesn't work on any Yeah, I
27:14
mean they're there, are you know, movements
27:16
of rocks rolled to each other, but not I played tectonics
27:18
of the type that we that
27:21
we have here, So so we think it's really important.
27:23
As far as we know, Earth is the only planet
27:25
to feature plate tectonics, which
27:27
actually is a massive thermostat for the planet.
27:31
When oceanic plates slide underneath
27:33
the lighter continental plates, massive
27:35
amounts of the oceanic crusts is
27:38
crushed and absorbed into magma.
27:40
The rock in those oceanic plates contains
27:43
huge stores of carbon dioxide, so
27:45
when volcanoes release magma from
27:47
beneath the crust, it also contains some of
27:49
that CEO two, which travels as
27:51
a gas up into the atmosphere and
27:54
there it hangs around and it absorbs
27:56
sunlight, which in term warms the atmosphere
27:59
and eventually the planet below. And
28:01
when the planet warms, more of the oceans
28:03
evaporate, warming the atmosphere even
28:06
more. When you have a warm, wet
28:08
atmosphere, you have lots of
28:10
rain that rain brings
28:13
dissolves c O two back down to Earth.
28:15
Rocks on Earth are an excellent store of carbon,
28:18
and when CO two rich, rain falls
28:20
on them as the knock on effect of weathering
28:23
them, meaning the wearing down
28:25
definition, not the opposite one. All
28:27
of that carbon in the rocks and rain makes
28:30
its way to the sea, where it dissolves
28:32
and eventually sinks to the ocean's bottom.
28:35
As more carbon is removed from the atmosphere
28:37
and stored, the planet begins to cool
28:39
again. Over time, the carbon
28:41
at the bottom of the ocean forms new oceanic
28:44
plate crusts, and eventually it
28:46
will find itself along an ocean ridge where
28:49
it collides with the continental plate and
28:51
the whole process begins again, and the
28:53
Earth starts to warm once more. This
28:57
unique property of Earth has kept the planet's
28:59
climate stable more or less constantly
29:02
for more than four billion years, which
29:04
has allowed life on Earth to grow and
29:07
flourish.
29:14
When you take all of these details together,
29:16
a weird picture of Earth emerges. It's
29:19
almost freakishly perfect for life.
29:22
That's so many different variables, each
29:24
at just the right temperature, just the
29:26
right location, heat time, whatever
29:29
would come together to form a stable
29:31
whole seems to make Earth a
29:34
staggeringly improbable place.
29:36
You couldn't ask for a better place for life to emerge.
29:39
And maybe that's the point. Maybe
29:42
the seeds of life are commonplace in the universe,
29:44
but Earth is unique. We
29:47
simply don't know. We still
29:49
know so little about space, our galaxy,
29:52
and the universe that we can't say if
29:54
Earth is freakishly unique or one of
29:56
many. And as we get better at
29:58
deducing the existence of habit of planets
30:00
with our space telescopes, they seem
30:02
to pop out of the cosmos like a magic
30:05
eye poster does when you lose focus in
30:07
just the right way. Maybe planets
30:09
that can sustain life are more abundantly the
30:11
universe than we realize perhaps
30:13
assembling those seeds into life is
30:15
where the filter lies. The farther
30:18
back we look in time, the less we understand.
30:21
So if you're going to look for something that
30:23
might be really hard, harder than it seems,
30:26
farther back in time is the plausible place to
30:28
look, because that's where we don't understand things.
30:32
Uh, And the very first step from
30:34
completely dead matter to some proto
30:36
life that has to be the
30:38
earliest step on the one we have the
30:41
least knowledge of, and more plausibly it's
30:43
the hardest step. Or perhaps
30:45
not. Perhaps right now the universe is teeming
30:47
with primitive life. Perhaps the great
30:49
filter lies somewhere after that. There
30:52
were, after all, some enormous steps
30:54
to get from the emergence of life here on Earth
30:57
in the moment we're sharing between us right
31:00
now, m
31:14
back on the early Earth, tucked away just
31:16
so, in a solar system, tucked away
31:18
just so, in the galaxy with its
31:21
volcanoes chugging away at producing a warm
31:23
atmosphere and its oceans producing a
31:25
warm liquid medium for molecules
31:28
to organize into life. At some point,
31:30
one particular moment in Earth's history,
31:33
all of those separate components came
31:36
together to form a full fledged
31:38
living cell. As
31:40
far as we can tell, this moment happened around
31:42
three point eight billion years ago. At
31:45
first, these simple, single celled organisms
31:48
were nothing more than gooey bags,
31:50
with the parts for replicating themselves and
31:52
the parts for converting food into energy
31:55
all slashing together inside of the cell.
31:58
They spread by dividing into exact
32:00
replicas of themselves. But over
32:02
time, over a very very long time,
32:05
some new versions of these simple cells began
32:07
to appear, and they had new specializations.
32:11
Their interiors became compartmentalized,
32:13
no longer slashing together, which
32:15
meant that the processes they carried out, like
32:18
converting that food to energy, became
32:20
vastly more efficient. So
32:23
processes like photosynthesis were
32:25
able to develop. And after they did,
32:27
the oxygen that this early cellular
32:29
life excreted as waste started
32:32
to settle into the atmosphere, creating
32:34
an entirely new one that would eventually
32:37
support the rise of new types of life.
32:39
Then comes the invention of sex, a
32:42
new type of reproduction where two entirely
32:44
distinct individuals combined to form a
32:46
new third version of themselves. And
32:49
it's about here that natural selection
32:51
cracks its knuckles and comes aboard
32:54
as the driving force of evolution here
32:56
on Earth. When natural
32:58
selection is presented with new options
33:00
rather than rough copies of the same thing, new
33:03
adaptations emerge much more quickly,
33:06
which kicks evolution into hyper
33:08
drive. The simple celled
33:10
organisms that made up life on Earth got
33:13
better at being living things, and
33:16
then for a long time nothing
33:19
much changed. It seems
33:21
as if life had reached the stasis,
33:23
maxed out, come upon some invisible
33:26
wall, and take into coasting.
33:28
Rather than progressing toward ever more complexity,
33:32
Earth seemed content with its fast
33:34
seas teeming with specialized, extremely
33:37
well adapted, single celled organisms.
33:40
After that first three hundred million years
33:42
of ceaseless innovation, life
33:44
on earths stayed the same for the next three
33:47
billion years. But
33:49
around five hundred million years ago something
33:52
huge happened. Life suddenly
33:54
developed new ambitions, and
33:56
it exploded into new, extremely
33:58
complicated and sophisticated forms.
34:01
And in geological terms, it happened
34:04
overnight. Basically go from
34:06
nothing to everything. This is Dr
34:09
Phoebe Cohen. She's a paleontologist
34:11
at Williams College in Massachusetts.
34:14
So the vast majority of
34:16
the history of life on Earth is that
34:19
of microscopic organisms.
34:22
Before the Cambrian almost
34:24
all life was microscopic or
34:27
at least very very small, and
34:29
ecosystems were dominated by things
34:32
like amiba and bacteria.
34:34
And after the Cambrian ecosystems
34:37
are dominated by animals, um
34:39
and so it's a really, really huge shift in
34:42
the biological evolution
34:44
of our planet. This sudden surge
34:47
in complexity is called the Cambrian Explosion.
34:50
We aren't quite sure why it happened. It's
34:52
possible it was triggered when the widespread
34:54
glaciation that covered Earth just before
34:56
it began to melt. Or perhaps
34:59
it was the oxygen and levels in the atmosphere
35:01
released by photosynthesis slowly
35:03
displacing the Earth's atmosphere of carbon
35:05
dioxide, ammonia, and methane. We
35:08
need lots of oxygen to power the conversion
35:10
of food to energy, and perhaps
35:12
the Cambrian explosion was triggered when
35:14
atmospheric oxygen reached a critical
35:17
threshold that could support more complex
35:19
life. So if you go into low oxygen
35:21
areas of the ocean today, there's plenty of animals
35:23
living with almost no oxygen, but they're not doing
35:26
anything. They're very boring. They kind of just lay there
35:29
because they don't have enough oxygen to do anything
35:31
exciting. So one idea
35:33
is that oxygen did reach some sort of threshold
35:36
around the Cambrian that enabled organisms
35:38
to start doing fun things like chasing
35:41
after each other and ripping each other apart, and
35:44
that that played a big role in changing
35:46
sort of the structure of ecosystems that lead
35:48
to a huge diversification um
35:51
within the animal claid. Whatever
35:54
the reason, half a billion years ago,
35:56
most of the complex body plans that are
35:58
still around on Earth to day suddenly
36:01
arrived. It's as if those
36:03
organizing principles of life entered
36:05
a new phase. Within
36:08
just thirty million years, plants
36:10
made their debut on land, and just
36:12
forty million years after that, animals
36:14
followed them out of the water. It's
36:17
astounding to think of, but within
36:19
a span of just seventy million
36:21
years, life on Earth went from
36:23
nothing but single celled aquatic
36:25
organisms to animals
36:27
that lived and moved and walked around on land.
36:31
Because life had remained so simple for
36:33
so long before it, the Cambrian explosion
36:36
makes an excellent candidate for the Great
36:38
Filter. It could be so
36:40
unlikely that it universally denies
36:43
intelligent life from forming evolutionarily
36:46
speaking, there's never been a more important
36:48
event in the history of Earth. Following
36:51
the emergence of life, twenty
36:53
of the thirty six body plans that
36:55
exist on Earth today, the plans
36:58
that give shape to squid and the ish,
37:00
and humans and worms, all suddenly
37:02
appeared on Earth, and those
37:04
new body plans led to a riot
37:07
of evolution. The dinosaurs
37:09
rose and fell, and small mammals
37:11
emerged from their burrows and climbed the trees.
37:14
Tree dwelling apes found their way out of the
37:16
savannah and started walking upright,
37:19
becoming the first contours of humans.
37:22
And it's about here that we arrive
37:24
at another step in the long span
37:26
between the emergence of life on Earth and
37:29
us, the evolution
37:31
of intelligent life. Humans
37:36
tend to think of intelligence is what differentiates
37:38
us from other life on Earth, but
37:41
instead we seem more like the current
37:43
endpoint in an evolution of intelligence.
37:49
Signs of intelligence, in some form or fashion
37:51
are all around us. In two
37:53
thousand eight, Japanese researchers
37:56
showed that slime mold, a unicellular
37:58
organism, can learn a schedule
38:00
of electric shocks when they
38:02
shocked the mold at regular intervals,
38:05
and yes, they shocked mold. The
38:07
mold learned to anticipate the next shock
38:09
and recoil from it before it was delivered.
38:12
The Moosta plants have shown that they can learn
38:14
to differentiate between being dropped and being
38:17
touched. Where initially the plants
38:19
responded to both experiences in the same
38:21
way by curling their leaves, after
38:24
being dropped several times, they learned to keep
38:26
their leaves unfurled, and they retain
38:28
this learned behavior even after they haven't
38:30
been dropped or touched for months. The
38:34
use of tools, which we imagine is quintessentially
38:36
human, isn't unique to us either.
38:39
Chimpanzees use tools to make gathering
38:42
food easier, like sticks to draw
38:44
termites from their mountains by the fistful, and
38:46
rocks to bash open hard shelled nuts
38:49
to get to the meat inside. But
38:51
at some point we drew away from
38:53
the rest of life. In the development
38:55
of our intelligence, we became
38:57
the first animals to use tools
38:59
to make other tools. This
39:02
is the birth of technology. No
39:04
longer were we relegated to using
39:06
only what was found in nature. We
39:08
learned to use nature to fashion new tools
39:10
to better suit our needs. We
39:13
made spearheads and axes, out of stone
39:16
and learned to hunt large animals. Meat
39:18
is more energy dense than plants, and
39:20
we learned to cook food about eight hundred thousand
39:23
years ago. When we did, we unlocked
39:25
a tremendous amount of nutrients and energy that
39:27
hadn't been available to us before. We
39:30
developed language, which allowed us
39:32
to better coordinate ourselves and hunt together
39:35
and interact with one another more effectively.
39:38
We learned to make clothes to keep us warm
39:40
as we spread out beyond the subtropical
39:42
climate we evolved in. We learned
39:44
to make boats to carry us to new places.
39:47
We learned to make ceramics to store our food.
39:49
We learned to grow crops, which led to cities
39:51
in the foundation of the modern era. And
39:54
there was another quirk of that chance collision
39:56
between the planetoid THEA, and Earth, which
39:58
produced the Moon. It also produced
40:01
massive deposits of minerals and metals
40:03
near the surface that humans could easily get
40:05
to. Over time, we
40:07
abandon those stone tools in favor
40:10
of more reliable metal ones, and
40:12
eventually we put all of those millions
40:14
of years of accumulated intelligence
40:16
and technology into ships that broke
40:19
the bonds of Earth and launched the
40:21
first of our species into space. Within
40:24
the astronomically short period of about
40:26
a hundred thousand years, humans
40:29
left the wild and went to space.
40:32
But perhaps as unlikely as the emergence
40:34
of human intelligence may seem, it
40:36
may simply be the expected outcome of
40:38
those organizing principles of life. There
40:41
are two options before us. Then, either
40:43
we humans are unique in our universe and utterly
40:46
alone, or we are not. And
40:49
if there is other life elsewhere, then that
40:51
means that the great filter, the hardest
40:53
step, lies not in our past, but
40:55
in our future. It means
40:57
that the challenge that lies ahead of us is more
41:00
difficult, more improbable to overcome
41:02
than dead molecules organizing themselves
41:05
into living cells or apes
41:07
learning to build ships to the moon, And
41:10
rather than having millions of years to try
41:12
and fail before succeeding, we will
41:14
have one shot to get it right.
41:17
If the great filter lies in our future, then
41:19
it appears that we are entering it right
41:21
now, now here in the
41:24
twenty one century, four point three
41:26
billion years after life emerged on Earth.
41:28
We are entering the evolutionary step that
41:31
no life in the universe has ever managed
41:33
to survive. Carl Sagan had
41:35
this this great phrase about
41:38
humanity has grown powerful before
41:40
it's grown wise um and our power
41:43
through technology has been increasing
41:45
exponentially, but our wisdom
41:47
has been maybe it's been increasing
41:50
a little bit, but suddenly not exponentially,
41:53
and it's it's getting these two
41:55
things have got out of check with each other. We've got an unsustainable
41:58
level of risk. The technology
42:00
that got us to this point is taking a new shape,
42:03
one that we haven't encountered before, and
42:05
it is presenting new risks to the survival
42:07
of our species and indeed life
42:10
on Earth. You right
42:12
now are living in what maybe
42:15
the beginning of the most dangerous period
42:17
in the history of the human race.
42:32
On the next episode of The End of the World
42:34
with Josh Clark, if
42:36
we are the only intelligent life, humans
42:38
could have a bright, long future ahead of
42:41
us, a triple less civilization
42:43
based on super intelligence,
42:46
super happiness, and super longevity.
42:48
But between us and that bright future lay
42:51
existential risks, and they're like
42:53
nothing we've ever encountered before.
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