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In which John Green, Hank Green, and Emily Graslie teach you about, well, everything. Big History is the history of everything. We’re going to start with the Big Bang, take you right through all of history (recorded and otherwise), and even talk a little bit about the future. It is going to be awesome. In the awe-inspiring sense of the word awesome. In this episode, we walk you through the start of everything: The Big Bang. We’ll look at how the universe unfolded at its very beginning, and how everything in the universe that we know today came into being. So that’s kind of a big deal, right?
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Transcript Provided by YouTube:
00:00
Hi. I’m John Green and this is Crash Course Big History, in which we’ll be looking at
00:04
the history of, like, everything. I’m talking about 13.8 billion years, from the big bang to now.
00:11
I mean, in this series, we are literally going to attempt to tell you the story of
00:15
what Douglas Adams famously called “life, the universe, and everything.”
00:19
Mr Green! Mr Green! That’s not history. That’s science, and science is for nerds!
00:24
Oh, me from the past! Things would be so much easier for you if you would just accept that
00:29
you are, in fact, a nerd! And that’s okay! I mean, look at this picture, dude!
00:34
Anyway, academics often describe history as like, all the stuff that’s happened since
00:37
we started writing things down, but they only start there because that’s where we have the best information.
00:43
And yeah, I think that the advent of writing was a huge deal, obviously, but as a start
00:48
date for history, it’s totally arbitrary! It’s just a line we drew in the sand and said “okay, history begins now!”
00:56
In Big History, we’re gonna start history when it really starts – at least, we think
01:00
– at the creation of the universe, and we’re gonna end that story where it ends – please
01:05
let that be after I die! Well, I guess it will definitely be after I die, just – I want it to be a while after I die!
01:12
So we’re even gonna terrify traditional historians by using physics to make some predictions
01:16
about the future, and we’re gonna end many trillions and trillions of years from now,
01:21
when the universe itself, spoiler alert: dies. At least, in a manner of speaking.
01:26
[Theme Music]
01:35
Hey! I’m not John. If you’re thinking we look a little bit the same, that’s because we’re brothers.
01:39
I’m Hank. Anyway, if you wanna learn the 13.8 billion year history of the universe in the same amount
01:45
of time that we usually cover the 238 years of American history, you’re not gonna get the same resolution.
01:50
Of course, knowing the names and dates of American history is important, but we just can’t do that in Big History.
01:56
There are much broader historical questions in the story of the universe that can only
02:01
be explored by zooming out to the ultimate scale. As you zoom out, you see a lot more
02:05
of the picture. The details get a little fuzzy, but we quickly realize that history is everything.
02:11
Cosmology, geology, biology, social sciences, literature, physics… Everything!
02:17
You might think that such a scale would be filled with way too much detail, but the amount
02:21
of detail an answer requires, depends on the nature of the question. Some questions can
02:25
only be explored by zooming out. That is what Big History does.
02:29
Speaking of zoomed out, this is Earthrise, one of the most famous photographs of all
02:35
time. William Anders, an Apollo astronaut, took it in 1968. From the surface of another
02:40
world, we see our planet as a little ball in space. No borders, no people, no buildings.
02:46
Just oceans and clouds and continents being shined upon by the sun.
02:50
That sheer expansion of scale gives me perspective. It lets me imagine all the complexity of life
02:55
on Earth, from the gasoline engine that powered my trip to the studio, to political instability
02:59
in Nepal as part of a thriving, living, teeming mass of life floating in the emptiness of space.
03:05
So what that photograph does for physical space, Big History aims to do for everything.
03:10
I mean, we wanna contextualize all of existence. We wanna outline the most powerful and important breakthroughs,
03:16
the tremendous scale of existence, and how we know what we know, and why we’re sure we know it.
03:21
All right, let’s go to the Thought Bubble. So the universe is big. Like, really big. And it’s also old.
03:27
Like, 13.8 billion years old, which is enough years that there is no way to actually comprehend it.
03:33
So let’s just compress that age to 13 years, small enough that our puny brains can handle it.
03:39
On that timescale, the universe would have begun 13 years ago, in 2001. George W Bush
03:44
had just been sworn in as president, most Americans on the internet were connecting to it with dial-up modems.
03:49
Right, so the first stars and galaxies would have formed 12 years ago, but seven and a
03:53
half more years would pass until the Earth formed, about 4.5 years ago. Move a little
03:59
bit up to four years ago – that’s when the first single celled life formed on Earth.
04:03
Then leap forward nearly three and a half more years before the first multi-cellular
04:06
organisms in the Cambrian explosion…
04:09
What I’m trying to explain is that all complex life on Earth is a fairly recent development.
04:13
Like, on this scale, the dinosaurs went extinct about three weeks ago —
04:17
roughly the last time I changed my Facebook status.
04:19
Humans and chimpanzees split from their last shared ancestor about three days ago!
04:24
The first homo sapiens emerged fifty minutes ago, roughly the last time I checked my email.
04:29
We left Africa 26 minutes ago. The American-Indians reached the Americas 6 minutes ago —
04:35
roughly the last time I checked my Twitter.
04:36
We invented agriculture 5 minutes ago. Ancient Egypt? 3 minutes ago! The Black Death? 24
04:43
seconds ago. The Industrial Revolution – 6 seconds. World War One, 2 seconds. The Cold
04:49
War, th e first man on the moon, your birth, the internet, the Big Mac? All within the last second.
04:55
But in many other ways, complex life and humanity are exceptional. Thanks, Thought Bubble!
04:59
Also exceptional, by the way, the Mongols! [Mongoltage]
05:04
Okay, let’s begin at the beginning! The big bang!
05:07
Hank, wait a second! Woah, woah, woah, woah, woah. I- I don’t understand how we know that
05:10
the big bang is really the beginning. Like, what happened before the big bang?
05:14
Well. Okay. Uh… Theoretical physicists say that space and time are not two different
05:20
things. They are two expressions of one thing – space-time. And space-time was created by
05:26
the big bang, thus time didn’t exist before the big bang, so it doesn’t make much sense
05:31
to ask what happened before it. There was no “then”, then!
05:35
Of course, this, like many ideas in cosmology, doesn’t really make any sense to our puny
05:40
human brains. It’s largely beyond our comprehension, rather like explaining color to a blind person.
05:45
We know that it’s true because the math works and it explains our observations so elegantly,
05:50
but it’s so far outside of how we directly perceive the world, that I don’t think it’s
05:54
something even the most genius physicists are able to imagine.
05:58
But yeah, if you’re gonna do a chronological study of the universe, the creation of time
06:02
is probably a pretty good place to start the story.
06:04
So the big bang wasn’t something that happened inside the universe, nor did it expand into
06:09
some kind of void. It was literally the moment when both time and space were created. The
06:15
thing that was banging was the universe itself. It was expanding from an unimaginably tiny
06:20
point to an unimaginably large universe, unimaginably quickly.
06:25
Unimaginable is basically the subtitle to the story of the big bang, but then again,
06:29
it’s also kind of the subtitle to everything else in big history.
06:32
I mean, I can only do this occasionally, but sometimes you look outside and you’re like,
06:36
“Oh, my goodness! This is nuts! How did we get trees?” Needless to say, we will be talking about that.
06:42
Anyway, the universe is a hard worker, and it got most of the heavy lifting done in those
06:47
first few seconds. For comparison, it takes me about twenty minutes after I wake up for
06:51
me to even get myself into a standing position. But the universe is somewhat more efficient.
06:55
In the barest fraction of the first second, the universe inflated from something many,
07:00
many, many times smaller than an atom to about the size of a grapefruit. Like, think of it
07:05
this way: in much less than a blink of an eye, if it’d originally been the size of a
07:08
tennis ball, it would have inflated to over ninety billion light-years across.
07:12
This inflation theory has been well backed-up by mathematics for a long time now, but it
07:16
has recently received some staggering new support from the BICEP project at the South
07:21
Pole, which sadly has nothing to do with my guns.
07:23
Ten seconds after the big bang, the universe had expanded enough that the normal rules
07:27
of the universe, with atomic forces and gravity and electromagnetism that we know and love
07:32
today, were already in charge. All of the anti-matter created in the big bang had combined
07:37
with matter and annihilated itself, leaving behind only one billionth of the matter created
07:42
in the big bang, and that billionth is everything! And I mean everything. Every grain of sand,
07:48
every blueberry you will ever eat, every star that you will ever see – everything!
07:52
We’ve already tried to understand how big a billion is, but just pause to think about that – everything!
07:58
Everything! Is one billionth of the matter created in the big bang. [Explosion sound]
08:04
The first law of thermodynamics is that matter and energy cannot be created or destroyed.
08:09
Everything we have now, we had then. The matter that makes up your body right now has been
08:14
around since those moments 13.8 billion years ago. It’s simply changed form.
08:20
After just three minutes, the universe was cool enough that the nuclei of atoms started
08:24
forming – just hydrogen and helium back then, the two simplest elements – keep those two
08:28
in mind, however, because it turns out, if you take a bunch of hydrogen and you wait
08:32
like, several billion years, you might just grow yourself some humans!
08:35
Let’s remember: at this time, the universe was still very, very hot. I don’t wanna use
08:39
the word unimaginable too often, but it was unimaginably hot!
08:43
The universe remained like an uber-hot sea dominated by radiation, but then luckily,
08:48
it simmered down to a balmy 5,000 degrees Fahrenheit about 380 thousand years after
08:52
the big bang, allowing matter and radiation to separate.
08:56
And remember, matter is just a more congealed form of energy. I mean, you are a somewhat
09:01
firm bag of energy. In my case, not that firm.
09:04
So anyway, at 5,000 degrees Fahrenheit, radiation was finally able to move freely through the
09:09
universe, and we see that radiation today as the end of the Dark Ages that followed
09:13
the big bang, and the beginning of a brilliant flash that we call Cosmic Background Radiation,
09:19
which is a great name for a band.
09:21
Physicists call it the fingerprint of the universe and it’s one of the most important
09:25
pieces of historical evidence we have for the big bang, because CBR is everywhere.
09:30
Tune your radio to a frequency that doesn’t have a station – a portion of the static you
09:35
hear is actually that cosmic background radiation being picked up by your radio. So you can
09:40
literally hear the universe in its infancy!
09:43
Sometimes it can be tricky to know what’s true, especially when we’re talking about
09:47
stuff that happened so far in the distant past. That is why we created science, that
09:52
elegant system for sorting out the facts from the fertilizer.
09:56
So just using your limited human senses, you might come to the same conclusion as 19th
09:59
century scientists, that the universe is static, eternal and infinite… But then, using our
10:06
minds, if the universe is infinite and contains infinite stars and it has always existed,
10:10
then the night sky, and the day-time sky for that matter, would literally be filled with
10:15
stars – so much that day and night would be indistinguishable! This is clearly not the
10:20
case, so something must be amiss.
10:22
The universe must either be not static, not infinite or not eternal. So which is it? You
10:27
know how when an ambulance drives towards you, the sound-waves are compressed and the
10:30
siren sounds higher pitched, and as it speeds away, the waves are stretched out and the
10:33
pitch is lower? It’s the Doppler effect.
10:35
Well, here’s another name you’ve heard. Edwin Hubble. He realized that light does the same
10:40
thing. Galaxies and stars moving away from us have their light stretched out, making
10:45
it more red, and stars moving toward us have their light compressed, making it more blue.
10:49
Combined with the work of Henrietta Leavitt, which allowed us to accurately estimate how
10:53
far away stars are, Hubble was able to determine that stars, on the whole, are flying away from each other.
10:59
He discovered that the most remote objects in the sky were all red-shifted and were actually
11:03
other galaxies beyond the milky way, moving away from us. From here, he built upon the
11:08
work of Belgian Catholic priest Georges Lemaitre, who hypothesized that the universe began at
11:13
a single point. Big bang cosmologists wanted proof though. They knew that the amount of
11:18
radiation released by the big bang would be massive, and they wanted to see it.
11:22
It wasn’t until the 1960s that it was found accidentally, by two guys working on an antenna
11:28
at Bell Laboratories in New Jersey. They were trying to eliminate all the background noise
11:32
from an extremely sensitive radio antenna, but they found this faint hum coming from every direction.
11:37
They tried everything they could to get rid of it, including murdering the pigeons that
11:41
kept pooping on the antenna – kinda sad, but those pigeons – they gave their lives for
11:46
one of the most profound discoveries in modern science. A conversation with a local radio
11:50
astronomer lead them to show their findings to an astronomer at Princeton, who confirmed
11:54
the existence of what had been predicted for years.
11:57
The final piece of that big bang puzzle is that we can see it. Light has a speed. When
12:02
we look at the sun, we’re seeing the light that left it eight minutes ago, but if we
12:06
look at something that’s 13.8 billion light-years away, we’re seeing the stuff that happened
12:10
13.8 billion years ago! That radiation has been traveling since the very beginning of the universe.
12:16
Not only can we tell very clearly that there was just nothing there before that, we can
12:21
now study that radiation to learn the sequence of events of the big bang. We can also see
12:25
that the chemical composition of the early universe is what we’d expect to see – a lot
12:29
of hydrogen, a lot of helium and a tiny pinch of lithium. The rest of the periodic table
12:34
had to wait for the fiery furnaces and the bellies of stars to be created.
12:39
But more on that, next episode!
12:40
As far as we’ve come in the past century in crafting a history of the universe, there
12:44
are still many things cosmologists have yet to discover. For instance, the universe behaves
12:49
as if there’s a bunch of matter in it that we can’t see or detect. Galaxies’ gravitation
12:54
is affected by this matter, but it’s otherwise completely invisible to us. Physicists call
12:58
it dark matter, but we have no idea what it is! But as in any historical endeavor, new
13:03
discoveries will alter the story in future years, so expect the big histories of ten
13:08
or twenty years from now to look very different from today’s.
13:11
But this isn’t discouraging, because like, knowing everything would be boring!
13:15
There’s a lot left to discover, and at the current pace of scientific inquiry, many of those
13:20
amazing discoveries will await us in our lifetime! Or at least in your lifetime.
13:24
Whether it be World War Two or the life of Abe Lincoln, all histories ultimately start
13:29
with the big bang. Yeah, it would be silly to start your typical World War Two textbook
13:33
with the big bang, but it would be about a hundred trillion, trillion times more ridiculous
13:37
to say the big bang – the mother of all historical events – was not history.
13:42
And that’s why big history reaches into the lives of every person on this tiny speck of
13:47
dust we call home, regardless of nation, class or creed, and forms our common story.
13:53
See you next time!
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This post was previously published on YouTube.
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Photo credit: Screenshot from video.
