Daniel and Kelly’s Extraordinary Universe - Where did the Earth's atmosphere come from?
Episode Date: June 8, 2021Daniel and Jorge explain where the air you breathe came from, and whether there's hope for deep breaths on exoplanets. Learn more about your ad-choices at https://www.iheartpodcastnetwork.comSee omny...studio.com/listener for privacy information.
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Isn't that against school policy?
That seems inappropriate.
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Hey, Daniel, did you see that amazing volcano that erupted in Iceland?
Is that the one in Fagratalsfayat?
Oh, nice. Is that how you say it in Icelandic?
I don't actually speak Icelandic, though I do speak some Danish.
Icelandic is more like Old Norse.
But Iceland, the country, is super awesome and filled with volcanoes.
Yeah, and there's one right now spewing hot lava, like as we speak.
Yeah, it's like the earth is breathing out.
More like burping or vomiting?
The earth got indigestion, I think.
I wonder how you say indigestion in Icelandic.
Maybe it's just a volcano.
Volcano's fiat.
Hi, I'm Jorge. I'm a cartoonist and the creator of PhD comics.
Hi, I'm Daniel. I'm a particle physicist and I'm substantially less gassy than the island of Iceland.
Are you less gassing than the average physicist?
No comment.
Are you all full of gas?
I'm more full of hot air, yeah, exactly.
Well, welcome to our podcast, Daniel and Jorge, Explain the Universe, a production of I-Hard Radio.
In which we blow your mind into tiny little hot pieces of gas by talking about all the crazy stuff that exist in our universe.
We go way, way back to the very beginning of the universe, talk about how all that happened,
how it led to this crazy, beautiful structure that we see today, and what progress is,
we've made in unraveling that structure and understanding the fundamental nature of matter and
space and time. And of course, what the open questions are still. Yeah, we are here burping out
amazing facts about the universe and expelling them out into the atmosphere for all of you to
breathe in to your brains and absorb them and hopefully get nourished with some amazing
bruce about the universe. That's right. We want these hot truths to roll over you like lava flowing
it out of a volcano, but, you know, we hope not to burn you too much.
Things are getting kind of hot, Daniel. I love it. Do you lava it? I love it. And I love it.
And who doesn't love lava? But yeah, it's a pretty big universe. And we are just this small,
tiny little planet floating in the middle of mostly emptiness, careening through space,
ready to be hit by an asteroid perhaps. And this planet has a long and illustrious history.
It hasn't looked the way it currently does for most of its life. We don't think of the solar system
and the galaxy is changing very much, they seem sort of static.
But on a cosmological time scale, things are crazy.
Things are chaotic.
Things are changing all the time.
Yeah, it's easy to think when you look out into the universe and to the stars that things are always the way they are right now.
But no, actually, the universe is very dynamic and it's changing and it's constantly evolving.
Which tells us something important about what is going to be like.
If we want to know what the future Earth is going to be like and whether humans can still live on it,
We better dig into its past and understand how it got to be such a warm and wonderful, cozy place to live.
Yeah, what are we going to be burping in a hundred million years, perhaps, or having indigestion with?
Yeah, so the earth has an amazing history.
And so one part of the earth that's very important to us is its atmosphere.
I count on it every day.
I breathe it in.
It fills me with life every single moment, really, if you think about it.
No, absolutely.
We rely on it every single day.
Well, we couldn't live without it.
It feeds not just us, of course, but all the things that we eat, drink the atmosphere.
It's a very complex, an elaborate system of pumping gases out of plants and into plants and out of the ocean and into the ocean.
It's an amazing and complicated system.
And it's incredible that it works at all, frankly, and that it's even at all stable.
Thank goodness we haven't because without an atmosphere, we wouldn't be here.
We wouldn't just be out of breath and choke to death, but we would also be pretty toasted thanks to all of the radiation coming from space.
That's right.
The atmosphere is here. It keeps us warm and acts like a blanket and also acts like a shield, protecting us from so many rocks and particles and all sorts of stuff coming from space.
So it's a pretty important part of life here on Earth today and hopefully it'll stick around for another billion years or so.
Yeah, and we should appreciate it because it wasn't always here on Earth.
The Earth didn't always have an atmosphere.
There was a time and the history of Earth that we were basically naked, right, out in space.
Nothing to drape over us.
That's right.
If you build a time machine and you want to see the early Earth, don't neglect to bring your
space suit. Because if you go back two, three, four billion years into Earth's history, you're
not going to be able to breathe whatever was on the Earth if there even was anything.
Yeah. And so a big question would be, how did it get this way? How is it that we have?
This beautiful and fresh, well, depending on where you live, fresh air for us to take in and enjoy and
live with. It's a fascinating story that dates way back to the very beginning of the solar system and
involves lots of dramatic pauses like volcanoes and meteors and all sorts of other crazy stuff.
So today on the podcast, we'll be asking the question.
Where did the earth get its atmosphere?
Yeah, where did it get its airs, Daniel?
Its ambiance.
That's right.
It is a very, very fine place to hang out.
It's very airy.
It's very blue and transparent.
I love what you've done with the place, really.
I have to do a lot of burping, apparently.
I'm guessing maybe.
Is that count as interior design
if you're designing an entire planet
or is it still exterior design?
I guess it depends.
Are you like an alien shopping for planets?
Or are you like an earthling
looking around?
I'm imagining the aliens come.
They take over the earth
and they don't really like what we've done
with the place and they want to fix it up a little bit
so they hire some like massive geoengineering firm
to do the equivalent of interior design
but for the whole planet.
I wonder if that'll be like a future career.
like, hey, Mom, I want to be a geo-designer
or a geodecorator.
That's right.
Mars has been using that same shade of red
for like a billion years.
It's time to pick a fresh color.
Yeah.
How about a cyan or a nice mango,
a guava color?
You need always three words
in every name for a shade of paint,
you know, wild mountain raspberry or something.
Right.
That's so you can sell more of them.
To be honest, because if you just sell red and blue,
you're out of business.
Well, if you're covering a whole planet,
I think you're going to sell a lot of gallons
of paint. So yeah, so the Earth didn't always have the atmosphere that we're breathing right now.
It used to be a pretty inhospitable place, right?
That's right. It used to be a place where humans or animals could not survive.
Because I guess initially, you know, we formed around a brand new sun and we were just a
bunch of rocks and gas kind of gathered together by gravity, right?
Yeah, everything in the whole solar system, of course, came from the same big cloud of gas and
dust to form the sun and the planets and everything. But the story is a little bit more
complicated. Yeah. So we were wondering, as usual, how many people out there know the story of
our atmosphere and how we got to have the air that we have? So as usual, Daniel went out there
into the wilds of the internet to ask people, where did Earth get its atmosphere? And so as usual,
if you'd like to participate by answering funny questions with no preparation, please write to me
to questions at Daniel and Jorge.com. Trust me, it's fun. Here's what people had to say.
I'm going to guess from rocks during the heavy bombardment period when they hit Earth,
the gases got released into the atmosphere.
But the oxygen in the atmosphere, which is actually a lot higher today, came from, I think it's cyanobacteria.
Those rocks in Australia, the first thing is to photosynthesize and actually caused a huge extinction event.
When the Earth was just formed, it was hot, and I think there were many chemical reactions going on
we have atomic reactions and all.
So maybe because of the reactions,
I think probably they were just hydrogen and helium in the beginning.
But then due to all these reactions,
all the different gases were formed
and maybe that's how we got our atmosphere.
Let's see, we have lots of nitrogen
that prevents everything from blowing up.
Then we have some oxygen and some organ,
and that's about what I know about Earth's atmosphere.
I can't really tell you what it comes from.
I think the atmosphere came from volcanic activity when the earth was young.
And I know that the oxygen came from cyanobacteria producing it when life just got started on Earth.
Well, the proto-earth was very, very hot.
So I would say that the burning and the temperature itself would cause gases to form that would accumulate around the earth being trapped in its.
gravitational field and once the earth cooled the composition of the those gases must have changed
especially when life started to arise and would start to change the atmosphere and take out
carbon dioxide and fill it with oxygen i think they say mars used to have an atmosphere
maybe we stole mars atmosphere here have it on earth now our atmosphere came from all the various
eruptions on the Earth. In other words, the Earth's hot air.
The biggest contributor is alive, different organisms,
recycling various chemicals from the atmosphere. Apart from that,
atmosphere is replenished by absorbing comet trails and volcano emissions.
I'm assuming, like, at the formation of the Earth,
there was a bunch of like dust and rocks and like just surrounding chemicals
and the Earth kind of lumped together, the rocks lumped together,
created kind of some strong gravity and like particles and like air particles were like,
hey, there's some gravity here. I guess let's like stick around, stick to it. And that's what
happened. All right. A lot of pretty detailed answers. People have thoughts on the topic.
Yeah, they have errors. They have a lot of things to say about how we got our atmosphere.
That's pretty cool. Do you think it's out there in the popular culture, kind of the history of
our atmosphere? Yeah, or you know, maybe it's just so immediate. People think about it. They
literally breathe it in and out every day.
So it's not some like weird, abstruse topic that only physicists wake up late at night
thinking about.
It's something everybody thinks about.
And these days with all the discussion of global warming and climate change, it's
something that people really do think about.
What's in the air and how we can influence it.
And I guess it's kind of interesting that nobody was surprised.
Nobody was like, what?
We didn't always have an atmosphere?
Like, people seem to know that it came from somewhere.
Yeah, somebody even suggested we stole it from Mars.
No way.
What?
Is it hot air? Is there air hot?
Exactly. They're going to come looking for it.
Bring it pulled over with a vacuum and suck it all back up.
Sir, do you have a receipt for this atmosphere?
I do. I just lost it 7 billion years ago.
Oops. Who keeps records that long anyway?
Yeah, so it is an interesting story how we got our atmosphere.
And so it's interesting to think that that wasn't always the case.
You know, we were just a little barren rock floating out in space with some gas, right?
Yeah, it's really a fascinating story because the Earth has had different atmosphere.
years through its history.
Like, if you took a time machine back to the very, very early hot earth, you'd experience
something very different from if you went back like three billion years ago or one billion
years ago.
So it's really, it's a fascinating, very, very dynamic story with lots of twists and turns.
Yeah.
And it's not just like a different temperature maybe or slight tweaks in the composition.
It's like a totally different set of gas that was enveloping the earth, right?
Yeah, we have like atmosphere 3.0 these days.
We're not breathing the original atmosphere or even the second.
an atmosphere. We're like on the third version of the atmosphere. It's been upgraded twice already.
Wow. Do you think we got it this time or do you think we're due for an upgrade? I'm pretty happy
with it. I got no notes. Like do we have to schedule the update? You know, can we schedule it for
like a few billion years from now when we're not around? Well, that's the problem is sometimes,
you know, you're happy with your version of your operating system and then it updates itself.
And you're like, no, don't change anything. It was great. Do we have auto update on? Maybe we should
turn that off. Because sometimes things don't work the same, you know? That's the solution to climate change
rather just untick that box on the atmosphere operating system that says, no updates, please.
All right, everybody stopped breathing for about 100 years, and then we'll get a new one.
We're going to reboot, yeah.
All right, well, so you're saying this is not our first atmosphere.
We're in the third version.
So what was the first version of the atmosphere?
So the first version in the atmosphere formed when Earth formed itself.
As we were saying before, everything in the solar system came from the same basic constituents.
You had this huge cloud of hydrogen mostly and a little helium and trace heavier elements.
And that whole thing got sparked into a collapse, which led to the formation of the sun, of course,
which is a huge ball of hydrogen.
And then the planets gathered together and it all basically came out of the same stuff.
And you had planets form because you had like little rocky cores that gathered together
and gradually pulled other stuff along with it.
And so what was Earth's atmosphere when it first formed?
Well, the only gases around really were hydrogen and helium mostly.
So just like Jupiter and the sun and the other gas giants have big atmospheres,
mostly of hydrogen with a little bit of helium.
Earth also had a helium hydrogen envelope around it when it first formed.
Right, because I guess, you know, the whole area in space was covered in hydrogen and helium.
And most of it went into the sun, but I imagine some of it sort of hung out around the little rocky planets that were forming.
Yeah, but not for very long.
So what happens is these things are forming and they're collapsing and there's sort of a race,
like the sun is gobbling up a huge amount of this stuff and the gas giants are out there,
they're gobbling up a lot of it.
And here in the inner solar system, it turned out to be pretty hard to hold on to any gas
because you're competing with the sun that's slurping up all of the hydrogen as much as it can
and you don't have the gravity that like Jupiter has because the inner part of the solar
system is warmer so there's no like rock ice to help you build a planet rapidly to grab
some of that helium and that hydrogen.
So out in the outer part of the solar system where Jupiter,
was you had rocks formed together, but also with ice that let them see these larger planets
that could hold onto their hydrogen.
But here in the inner solar system, Earth was just sort of like too small to really hang
on to its hydrogen.
So it was a very short-lived atmosphere.
I guess maybe like, you know, lighter elements like hydrogen and helium, they get more
easily sucked in by the sun and other planets than the rocks that we have, right?
That's kind of what happens is that, you know, it's so light that it can just leave and get
sucked in by the sun.
whereas the rocks, it's harder for the sun to have pulled this in.
That's exactly right.
And there was also an opposite effect because once the sun started burning,
it was producing a solar wind, which is a huge amount of radiation,
that then blew off the rest of our atmosphere.
We had no magnetic field yet to protect ourselves from these things.
Magnetic field is formed when layers inside the earth are like mixing and blending and spinning,
but the earth was too young to have like differentiated
and have these nicely divided layers that could produce a magnetic field.
And so the solar radiation also blew off any gas that we did manage to grab.
So initially we had a little bit of gas around our kind of brand new Earth,
but then it quickly either left or it got blown away.
Yeah.
So this first atmosphere was very, very short-lived.
I'm not even really sure you could say it was like settled down before it got slurped up by the sun
and then blown off by the solar radiation.
Yeah, I feel like there's a lot of gas and wind in this story.
This is getting a little, you know, gastric here, not just cosmic.
Take a tumms, but there was a lot of stuff going on.
Like the early solar system was a very chaotic place.
And it could have gone in lots of directions.
You know, you could have a planet here or a planet there.
The reason we have a planet exactly here depends on a lot of very small chaotic factors
that depended just on like the distribution of the initial stuff.
But a little bit more clumpy over there, you would have gotten a different set of planets.
All right.
So then we had a little bit of hydrogen and helium, but then that quickly went away.
And so what was our second atmosphere?
So then the earth was barren, right?
We had just a ball of rock with really no atmosphere to speak of.
So they have this period here where the earth is like naked.
There's just no atmosphere protecting the surface of the earth from basically space.
And, you know, interestingly, I talked to some geologists, and they don't see the earth as naked in that sense.
Like, for them, the atmosphere is part of the crust.
It's just like a different kind of crust.
You know, they don't think of it as like the crust ends at the surface and then you have atmosphere.
the atmosphere is just sort of like part of the crust because there's like constant interchange between the atmosphere and the surface and it's just like you know another layer of the earth sure I guess to a geologist they want it all they want it all
they're like the air that's part of my grant proposal as well it's part of geology of course everything's geology humans we're also geology we are part of geology absolutely yeah we are part of the crust and that's where this outer gas layer of the crust that we call atmosphere came from when it was replenished it was replaced it was
planished from inside the earth because volcanoes like the one in Iceland and the other ones
around the earth outgast like internal processes inside the earth led to these explosions and
eruptions which can produce enormous quantities of gas meaning like was all this gas formed inside
of the earth or it just got trapped as the earth was sort of forming and all those rocks
actual rocks were coming together yeah it's all in there and it's all mixed together you know
you have carbon you have sulfur you have oxygen these are all the
elemental ingredients of the solar system which are then compressed and mixed together there's a lot
of chemistry going on so these elements all mixed together in the way that's like energetically most
favorable but then yeah they get spewed up from underneath the earth and you know these rocks have
gases dissolved in them sometimes and then those can come out when there's less pressure or i guess
maybe as things were sort of churning and coming up from the surface then the gas was able to
escape the rock exactly large gas bubbles exactly can make their
way up through the crust and then emitted by the volcanoes. I mean, that's why volcanic eruptions
happen, right? We talked about this in a recent episode on most massive volcanoes in the solar
system. When you have lava that has like a lot of silica dissolved into it, then it becomes like
very sticky and it can absorb a lot of gas. And then a gas builds up the pressure and then it erupts
and the gas can be freed. Right. And so that's how we got things like water, water vapor and CO2
and hydrogen up in the atmosphere in that second atmosphere? Yeah. So the second atmosphere is mostly
as you say water vapor, carbon dioxide, sulfur dioxide, and then a huge amount of just nitrogen.
And very importantly, there was no free oxygen, no like O2 molecules were floating around in the
atmosphere. So this second atmosphere is not something we can breathe at all. It would be totally
toxic. You took a time machine back to this volcanic period of the earth and you took a deep breath
as you stepped out. You would die pretty quickly. Great. Not a great place to visit.
No, exactly. But bring your space suit, you know, no big deal. Pack some oxygen.
Yeah, just pack oxygen for 50 years.
And there's one other source of sort of basic ingredients for our atmosphere in those early days.
It didn't just come from inside the Earth.
There were some deposits from outside the Earth because during this period of chaos in the early solar system,
there was a lot of stuff moving around.
The planets were switching positions and passing through the asteroid belt and passing through the asteroid belt in the other direction,
which led to a lot of bombardment of the Earth.
by really big rocks.
This is called the late heavy bombardment.
And some of those rocks have water, they have ice,
they have other things frozen into them,
which then evaporated when they hit the earth.
Interesting.
So those rocks had other sort of gaseous elements,
and then when they hit the earth,
they made it into our atmosphere.
Yeah, just like we talk about how comets
probably replenished the earth's water
in the very same way, right?
Earth had water when it formed,
but then it boil off because we lost our atmosphere
and it's very hot surface.
And we had a whole episode about how comets replenished the Earth's water.
In the same way, asteroids and other things probably also replenished part of our atmosphere.
Cool.
All right, well, let's get into how we actually got breathable oxygen in our atmosphere
and how we know all of these things.
How do we know the history of our atmosphere?
But first, let's take a quick break.
December 29th, 1975, LaGuardia Airport.
The holiday rush, parents hauling luggage, kids gripping their new Christmas toys.
Then, at 6.33 p.m., everything changed.
There's been a bombing at the TWA terminal.
Apparently, the explosion actually impelled metal glass.
The injured were being loaded into ambulances, just a chaotic, chaotic scene.
In its wake, a new kind of enemy emerged, and it was,
here to stay. Terrorism.
Law and order criminal justice system is back. In season two, we're turning our focus
to a threat that hides in plain sight. That's harder to predict and even harder to stop.
Listen to the new season of Law and Order Criminal Justice System on the IHeart Radio app,
Apple Podcasts, or wherever you get your podcasts.
My boyfriend's professor is way too far.
friendly, and now I'm seriously suspicious.
Oh, wait a minute, Sam, maybe her boyfriend's just looking for extra credit.
Well, Dakota, it's back to school week on the OK Storytime podcast, so we'll find out soon.
This person writes, my boyfriend has been hanging out with his young professor a lot.
He doesn't think it's a problem, but I don't trust her.
Now, he's insisting we get to know each other, but I just want her gone.
Now, hold up.
Isn't that against school policy?
That sounds totally inappropriate.
Well, according to this person, this is her boyfriend's former professor, and they're the same age.
And it's even more likely that they're cheating.
He insists there's nothing between them.
I mean, do you believe him?
Well, he's certainly trying to get this person to believe him
because he now wants them both to meet.
So, do we find out if this person's boyfriend really cheated with his professor or not?
To hear the explosive finale, listen to the OK Storytime podcast
on the Iheart radio app, Apple Podcasts, or wherever you get your podcast.
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to get caught. And I just looked at my computer screen. I was just like, ah, gotcha.
On America's Crime Lab, we'll learn about victims and survivors,
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Listen to America's Crime Lab on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts.
Hey, sis, what if I could promise you you never had to listen to a condescending finance, bro,
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How in just a few months, you can have this much credit card debt and it weighs on you.
It's really easy to just like stick your head in the sand.
It's nice and dark in the sand.
Even if it's scary, it's not going to go away just because you're avoiding it.
And in fact, it may get even worse.
For more judgment-free money advice, listen to Brown Ambition on the Iheart Radio app, Apple Podcast, or wherever you get your podcast.
talking about the history of air, basically, right?
Where did air come from?
And why is it so fresh to breathe?
Yeah, exactly.
It's something that's all around us,
but it's something that we rely on.
So we better understand why it's here
and whether it's going away.
Yeah.
Do you think air is offended when we sneeze or like cough?
Like, you know, get it out of my body.
No, I think it's probably grateful.
It's like, ooh, that's much more interesting.
Yeah, who wants to be inside of a wet, warm human?
Yuck.
All right.
Well, we had one atmosphere, but then it was blown away
by the sun and cosmic rays.
And then we had got a second atmosphere
that was burped up from the rock
inside of the core of the earth.
And this atmosphere had a lot of oxygen,
but it just wasn't free oxygen.
Like it was inside of CO2 and H2 or S.O2,
but it was not something that we could use.
Like if we breathe at that,
you wouldn't be able to get that oxygen.
Yeah, your lungs can't use that, right?
Even though there's oxygen in CO2,
if you step into a room that's pure CO2,
you're going to fall unconscious pretty quickly.
Yeah, not good.
All right.
So then that's our second atmosphere.
How did we get breathable oxygen then?
Breathable oxygen came from life, right?
This was terraformed by tiny, tiny little microbes.
But the first oxygen that was produced on Earth wasn't actually from those microbes.
The very first came from ultraviolet light that hit the Earth's atmosphere.
When UV photons, these are just really high energy particles from the sun, hit H2O molecules of water,
they can break it up and you can get.
yet ozone formed in the atmosphere.
An ozone is just a form of oxygen.
It's an O3 molecule.
And it forms in the upper atmosphere
and it helps to actually shield us from ultraviolet light.
So ozone, again, not something you can breathe,
but it's oxygen in the atmosphere,
which then shielded us from UV,
which helped life, I think, evolve a little bit.
Interesting.
So like you just have water molecules, H2Os there.
And then when it gets hit by this light,
it just breaks up and I guess breaks up.
But then the oxygen doesn't go into O2, it goes straight into O3.
Yeah, in these chemical processes, you always get a mixture of everything.
But primarily, this is how ozone is formed.
And you also get some other stuff forming.
You know, you get a little bit of O2.
But that's only responsible for like 1% of the oxygen in the atmosphere.
That's certainly not enough for us to breathe.
All right, but it did sort of form enough O2 then that you kind of had a shield around Earth
so that you could, you know, evolve little organism that did make.
02. Well, it made 03, which is ozone, which is primarily the shield. But exactly, it provides
a shield to protect us from UV and that can protect the DNA of delicate little critters as
they're evolving on the Earth. All right. So then that's how we got most of our oxygen then is
through bacteria and things like that. Yeah. So bacteria have been around for quite a while
churning away in the oceans of the Earth. And at some point, they evolved the ability to do
photosynthesis, right? To take sunlight and to combine the energy.
from sunlight with CO2 and water and to produce oxygen.
And when this happens, they're essentially producing fuel for themselves.
And so this is a really cool little thing that they evolved.
It's called cyanobacteria that first evolved this ability to basically drink energy from the sun.
And this started about 2.7 billion years ago.
And that's a very efficient way to turn CO2 and H2O into oxygen.
I guess maybe that, you know, in the primordial soup, you know, the Earth,
was, you know, inhospitable, but there were little tiny things that could grow in this
environment in the oceans. And then that started churning out O2. But that wasn't very
beneficial for them, right? No, it actually poisons them. Cyanobacteria are killed by the
presence of O2. And so if they make too much of it, they kill themselves off. And again,
they don't need O2. It's like a byproduct. It's a waste product for them. But they wanted the CO2,
right? Plants breathe CO2 and produce oxygen. Animals like us breathe O2 and
produce CO2 and cyanobacteria. They're not plants. They're like the precursors of photosynthesis
in plants. So they made a lot of oxygen, but that's not quite the oxygen we breathe today, right?
That's right. The oxygen that was made by cyanobacteria originally didn't stick around to the atmosphere
because oxygen is super duper reactive. It doesn't usually just hang out. Like if it can react with
anything around it, it will. So you have this fresh earth covered in rocks and these rocks are very
reactive with oxygen. Like, imagine a bunch of iron out there and you combine it with oxygen.
What do you get? You get rust. And so basically, most of the oxygen produced by the earth in
the first few hundred million years was then breathed in by the rocks on the earth. They
like sucked it all up. Wow. Like the earth was, you know, shiny and nice looking. And then suddenly
these bacteria breathed oxygen and everything rusted. Yeah. It was like hundreds of millions of
years where the earth was getting like weatherized by all the oxygen that was being produced.
And you know how you talk about like free radicals, et cetera, in your body, maybe causing damage
and causing cancer? That's all because of oxygen. Oxygen is very reactive. It's like a crazy
thing. It's going to touch and break things near it. And so that's what happened when cyanobacteria
started pumping O2 into the atmosphere is that it's starting to get absorbed by all these rocks and
break them down and weatherize them. And as you say, rust the entire planet. I guess that's a process
that had to happen, you know what I mean?
Like, you can't just have like a shiny, brand new, rust-free earth and also have oxygen.
Like, if you're going to put oxygen in the atmosphere, you have to first, you know, rust everything before you can breathe it.
Yeah, everything is going to drink up that oxygen.
So if you want enough floating around in the atmosphere for other things like animals to breathe,
then you've got to sort of like fill up all the reservoirs out there that are just going to gobble the oxygen so that there's enough to float around.
It's sort of like electrons in a semiconductor.
You've got to fill up all the lower energy.
levels so you can have some floating around in the conduction band and conduct electricity.
Right, right.
That was the first analogy I was going to go with for that.
I think these cyanobacteria are super amazing.
And I love how plants basically co-opted them.
Because, you know, the cyanobacteria, they evolved photosynthesis.
And now when we look inside plants, we see these little objects inside a plant cell that can do
the same thing, these chloroplasts.
But those things are basically cyanobacteria.
They got co-opted by the plants.
The plants like ate them and said, okay, come do that work for me now.
So the cyanobacteria should get all the credit for evolving this incredible ability.
The plants just took it over.
They're like the managers.
Yeah.
Or you could look at it the other way, right?
You could say that cyanobacteria, you know, kind of form plants around themselves, kind of, to do all their hard work.
They just have to sit back and get a can.
Exactly.
Yeah.
You can look at anything two ways, I guess.
All right.
to then we had to wait until everything was rusted before we got our third atmosphere.
Yeah, it wasn't until everything was rusted that the oxygen being produced by cyanobacteria
and then later also by plants could just sort of hang out in the atmosphere,
that those levels could climb to the point where like animals could breathe them.
And so now we're up to the atmosphere that we have today, which is, you know, still mostly nitrogen.
It's like 78% nitrogen, but a good 21% of our atmosphere is O2.
Wow. And it was all made by bacteria and plants, basically, right? Like before, like, you know,
we didn't get that. We made that. Yeah, it was made by living creatures and it took a long,
long time, right? So if you're imagining, like, let's go to Mars and produce enough oxygen for
the atmosphere for us to walk around and breathe, like it takes a long time. Even when you got,
like, gillions of tiny little machines pumping out oxygen, it took millions and millions of years.
Yeah. It took like 400 million years, actually, to be precise.
And in a way, they sort of ruined the planet for themselves a little bit, right?
Or do you think they were co-evolving as they were changing the atmosphere?
They're definitely co-evolving, and cyanobacteria are still with us.
They still produce half of the oxygen that we have on the Earth.
Currently, like, half of it is made by plants and half of it is made by cyanobacteria.
So they're still around in the oceans.
Yeah, and so that's how we got our atmosphere.
And it's not, I mean, it's a lot, obviously, because we have a lot to breathe.
But in terms of the scale of the Earth, it's a really small sliver or a small coating of
air that we have on the planet.
Yeah, the whole Earth, of course, is, you know, 6,000 kilometers in radius.
The atmosphere, what we consider at least the atmosphere is, you know, just like 30 or 50
kilometers high.
So it's a very, very thin veneer.
It's like a, you know, very thin coating of water on a billiard ball.
Yeah, because like what the Earth is, what, like 10,000 kilometers in radius or something
like that?
6,400.
6,400 kilometers in radius, but only the last 30 kilometers are atmosphere.
Yeah, and where exactly you say the atmosphere ends depends really just on where you want to say it ends.
Some people say it's up to 100 kilometers because, you know, it falls off very smoothly as you go out into space.
But 97% of the mass of the atmosphere, like most of the stuff in the atmosphere, is within the first 30 kilometers.
Do geologists also claim space as geology as well?
They're like, you know, just keep going.
Their atmosphere is geology, space is geology, galaxies are geology.
When they say we are one with the universe, they mean it literally.
Like the universe is just all part of the earth.
We are one, and that one is geology.
You got below the surface and above the surface, and it's just two parts to the whole universe.
No, it's all one big surface to a geologist.
But it's actually quite interesting.
There are lots of like really fascinating layers to the atmosphere.
Like you might imagine, as you go higher up, the air gets thinner and thinner and colder and colder until you got out into space and it's like super freezing.
But actually the temperature like varies and it gets hotter and colder and hotter and colder as you go up.
Really? Depending on like the composition or did you just get like pockets of stuff?
Yeah, depending on the composition, there are all these fascinating layers.
Like as you go up, you know, you go above like Mount Everest, for example, things get colder and colder and thinner and thinner.
But then when you get to like this ozone layer, things turn around and start to get hotter.
As you go past the stratosphere, things actually start to get hotter and hotter and hotter, not quite back up to like surface levels.
But, you know, getting kind of warm before they turn around again and then get colder as you go up through the mesosphere.
And then it turns around again and it actually gets hotter and hotter as you go into space.
Right.
Yeah, because I guess those are the layers that are absorbing a lot of the sunlight.
Is that what's happening?
They are absorbing a lot of the sunlight and they are evaporating, right?
What's going to be leaving the earth?
What's going to be making it out there to the higher levels are the faster moving particles.
And so the earth is sort of like differentiating.
We are losing our atmosphere constantly.
We had a whole podcast about that.
And primarily we lose the hotter atoms, the faster moving ones.
So while it's not very dense up there, there's not a lot of heat.
You have faster moving particles, which are the ones that are escaping.
And so technically it is hotter.
Yeah, the hot ones are always the first ones to leave, for sure.
And there's also sort of like radioactive elements out there in our atmosphere too, right?
Like some pretty not safe stuff out there.
Yeah, absolutely.
1% of our atmosphere is actually argon.
You know, you've got like 78% nitrogen, 21% oxygen, and then 1% argon, which is sort of weird.
It's this radiogenic argon 40, which comes from the decay of potassium 40.
And it's really interesting actually because mostly what you have out there in the universe,
like made by stars, is argon 36, which is, you know, a different isotope of argon that's made in the fusion inside stars.
But here on earth, most of the argon in our atmosphere is argon 40.
which comes from this radioactive decay.
And it took people a long time to figure out that that's where it came from and how it worked.
And it was a fun puzzle that was solved a few decades ago.
And there's also some pretty interesting elements like Krypton and neon and methane in our atmosphere.
It's not just like nitrogen and air and oxygen.
Yeah, remember that everything in our solar system came from those same basic soup of ingredients.
Inside the sun, of course, you have fusion making new heavy elements.
But outside of the sun, everything is just a mixture of the same elements that went in.
right? We have no fusion happening on Earth. All the elemental like Krypton or neon or hydrogen or
oxygen or all the other weird stuff that we have came from fusion inside some star somewhere else.
Our solar system is a population one solar system, which is the third generation in our universe.
So all of these atoms of oxygen and other stuff were formed inside a star billions of years ago,
which then blew up and led to the formation of this dust cloud, which eventually became our solar system.
That means we're all a little bit
Kryptonian, right?
A little bit, yeah.
All of these things that we're made of
that we're breathing,
that we're relying on,
all came from somewhere else.
We're fused inside a star somewhere.
And so that's how we got our atmosphere
through a lot of burping by the earth
and surviving some winds
and a lot of bacteria making it.
And that's how we got the air that we have today.
And thank goodness because it smells pretty good.
It could have smelled that, right?
I guess we're lucky that the earth smells good.
It probably did smell pretty bad for long periods.
you know, they're probably some pretty stinky times when Earth is young.
Yeah, the stinker scene, I think it's called.
You know, teenagers, they never smell very.
Yeah, to introduce them to deodorant and then things pick up from there.
All right, let's get into how we know this interesting history of our atmosphere
and what it could mean for the future of Earth and people breathing in it.
But first, let's take another quick break.
December 29th, 1975, LaGuardia Airport.
The holiday rush, parents hauling luggage, kids gripping their new Christmas toys.
Then, at 6.33 p.m., everything changed.
There's been a bombing at the TWA terminal.
Apparently, the explosion actually impelled metal, glass.
The injured were being loaded into ambulances, just to chaos.
chaotic, chaotic scene.
In its wake, a new kind of enemy emerged, and it was here to stay.
Terrorism.
Law and Order Criminal Justice System is back.
In Season 2, we're turning our focus to a threat that hides in plain sight.
That's harder to predict and even harder to stop.
Listen to the new season of Law and Order Criminal Justice System on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts.
My boyfriend's professor is way too friendly, and now I'm seriously suspicious.
Oh, wait a minute, Sam.
Maybe her boyfriend's just looking for extra credit.
Well, Dakota, it's back to school week on the OK Storytime podcast, so we'll find out soon.
This person writes, my boyfriend has been hanging out with his young professor a lot.
He doesn't think it's a problem, but I don't trust her.
Now, he's insisting we get to know each other, but I just want her gone.
Now, hold up.
Isn't that against school policy?
That sounds totally inappropriate.
Well, according to this person, this is true.
her boyfriend's former professor, and they're the same age.
And it's even more likely that they're cheating.
He insists there's nothing between them.
I mean, do you believe him?
Well, he's certainly trying to get this person to believe him because he now wants them
both to meet.
So, do we find out if this person's boyfriend really cheated with his professor or not?
To hear the explosive finale, listen to the OK Storytime podcast on the IHeart Radio app,
Apple Podcasts, or wherever you get your podcast.
A foot washed up a shoe with some bones in it.
They had no idea who it was.
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Using new scientific tools, they're finding clues in evidence so tiny you might just miss it.
He never thought he was going to get caught.
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I was just like, ah, gotcha.
On America's Crime Lab, we'll learn about victims and survivors,
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Your entire identity has been fabricated.
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All right, we're talking about the history of our atmosphere and we're kind of in our third atmosphere is what you're saying.
Like we, you know, we're not in our starter home.
We're not in our second home.
We're like in our vacation home almost.
We've been working on this for a while.
We're living the dream right now.
Breathing the dream.
We are.
We are.
And I love hearing those kinds of stories when you look around and you don't really know what the history of the earth is.
And then you discover through various like really subtle clues and awesome detect.
of work that things have changed,
that the Earth used to be really, really
different. Because, you know, your naive assumption
is like, I don't know, the Earth formed and had its
atmosphere has always been like this. That's the
simplest story and science always prefers a
simplest story. But it's super fun
when you discover that the story is more complicated
than it has twists and turns.
But you can't just like tell that story. You've got
to find the clues. You've got to discover that
story. Yeah, because that's a big question.
It's like, how do we know all these details?
I feel like that was a very detailed story
of how we got our atmosphere. But
there was nobody around really to sort of measure the oxygen or to see what was happening.
So how do we know all of these things?
Yeah, we have to look for clues in the geological record.
And so the rock record, like rocks that were formed 500 million years ago or a billion years ago or 2 billion years ago,
how they formed and which kinds of rocks formed tell us about what atmosphere there was around.
Because some kind of rocks can only form in the presence of oxygen.
And other kind of rocks can only form if there's no oxygen.
So as you look at the rock layers, you can look like back in time and get a sense for like what was going on.
Right? Because I guess the rocks are sort of changing, right? They're turning. They're flipping over. They sort of build up as they're growing, right? So then that's where you get the record.
Yeah. If you drive through the desert, for example, and you see canons, et cetera. You can see these stripes in the rocks, right? Where do those stripes come from?
Those are layers of rocks that have been laid down over millions and billions of years. As you say, the surface is like,
active. Stuff is coming out from underneath and then creating new layers which get laid down
and then pushed down. And sometimes those layers then break and get pushed back up to the
surface and revealed. And so we can see that history. That's why like dinosaurs are buried in
the earth because we're constantly laying down new layers of rock on top of the old ones.
And so that's super cool because it's basically like a snapshot of what was going on on the planet
back in the day. And if you can look at those rocks and see patterns in them, then you can get a clue
as to like what was going on in the atmosphere
because all those rocks as we were saying before
interacted with the atmosphere.
That leaves an imprint on the rock basically
like if there was a lot of oxygen or not
or other kinds of gases
then the rocks look different.
Yeah, and one of the most important clues
are these formations called
banded iron. And these are really
beautiful. You should Google them and check them out because
they're basically these rocks with these thick
red stripes in them, this
oxidized iron stripes. And that
tells us a lot about when this
oxygenation event happened when the cyanobacteria started pumping oxygen into the atmosphere
because it started to bind with the iron that was out there and get weatherized and make these
layers and layers of basically rust inside the earth's atmosphere. So you can look back at these
first earliest layers of rust and pinpoint when oxygen started to be produced. That makes me think of
like a heavy metal band or something. Bandit iron. First rust. Yeah, there you go. Red rust.
It's super cool because it's sort of like rings on a tree because you can see these bands.
It's not just like, oh, oxygen turned on, started to be produced and then everything after that is just rusted iron.
You have these bands where it's like rusted iron and then rusted iron and then none and then run and then turned on and off and on and off.
You can be like, oh, look, the earth just burped here or it just passed wind.
Yeah, what happens is that this oxygen that these bacteria produce is actually poisonous to them, right?
cyanobacteria do not like a lot of oxygen. So they produced a bunch of oxygen and some cases
there was like a lot of iron around in the water to grab that oxygen and then sink back down to
the ocean floor and form a band. But sometimes the cyanobacteria would produce too much oxygen.
It couldn't all get like breathed in by this iron and then they would poison themselves and like
kill themselves off and then they wouldn't be producing as much anymore. And so there wouldn't be
as much iron deposited. But then the conditions were favorable again for a cyanobacteria.
which would then grow back
and produce a huge amount of oxygen
which would they create another band
and sort of this sort of cycle effect
where they overproduce and kill themselves
and then grow back.
That's kind of what's happening to us right now.
I mean, we are creating so much CO2.
Every time we breathe out, we create CO2
and so we didn't have all these other processes
to replenishes the O2.
We would be basically poisoning ourselves, right?
Breathing ourselves out of a planet.
Yeah, we could have a sort of similar effect
where we have like human civilization builds up
and then poisons itself with CO2
and then you have like a calm period on the earth for a million years while you have like small bands of humanity surviving rebuilding civilization to poison ourselves again.
I can see your brain just writing the sci-fi novel there.
I think I've read that one.
But I guess maybe a question is like how do we correlate that to time?
Like we can see these bands in the rock, but how do we know that band took place or was formed, you know, 300 million years ago or six billion years ago?
How do we get that calibration of the rings in the tree?
Oh yeah, great question. It's like, how do we know the age of any rock? You know, and I remember thinking about this as a kid wondering like, what does it even mean the age of a rock? You know, because like lava is lava. Rock can melt or flow. It's like asking how old water is. But when you talk about the age of a rock, you're not talking about like when the chemical elements or even the elements inside the rock were formed because that happened inside a star billions of years ago. We're talking about like when this crystal was created because rocks are a solid formation.
of these elements, right?
It's like cool together to form a solid object.
So you can measure that age of the rock,
which is when did this thing become a solid object?
How long ago was this thing fluid?
When did it transition to becoming solid?
And you can measure that because when that happens,
it captures things inside of it,
these crazy little crystals.
And those crystals, some of them are radioactive
and they like decay very slowly over time.
You can measure how many of those are and calibrate them.
And that's what you do to measure the age of rocks.
I see.
Like when the rock forms, they capture like a ticking clock almost inside of them.
It's sort of similar to carbon dating, which we can use to age like things that were once alive,
you know, because they have certain ratios of carbon in them.
But here we're talking about things that are much, much older.
So we use these radiometric dating methods based on the natural radioactive decay of things like potassium and carbon to date these ancient, ancient events.
Nowadays, they just use Tinder for dating different rocks.
That's a terrible joke.
I apologize for that.
So yeah, so that's how we know then how the history of our atmosphere.
Yeah, because we can look at this record.
And so that's one piece of evidence is these banded iron formations.
And you know, this has a big influence on like our civilization.
Because Detroit, for example, is in a location where there used to be an ocean with huge colonies of cyanobacteria
depositing lots of bands of iron.
And so like that's why a huge fraction of the steel deposits available.
on Earth are like near Detroit.
And that's why we have a car industry near Detroit
because of this cyanobacteria.
So I love these like connections from the ancient times
back to like, you know, modern civilization.
And even politics, they always talk about the rust belt, right?
Yeah, exactly.
It should be talking about the cyanobacteria belt, really.
Yeah, nobody wants to be in that political group.
For sure.
But this also lines up with other pieces of evidence.
Again, we look into the record to see what could happen
with oxygen and what could happen without oxygen.
oxygen and there are other minerals like pyrite this thing called fools gold which can only form
when there's no oxygen in the atmosphere if there's oxygen around then the elements that would
otherwise make pyrite tend to make other things instead and so you can see like oh pyrite was
only created until about a certain date several billion years ago so that's another clue and i
imagine also there's a lot of it is sort of theoretical kind of based on models of how the earth
formed right for example we can only go back so much with these methods like when you're talking
about before, like, you know, our early, our first atmosphere getting blown away by the solar
wind. That's, you know, we don't have evidence for that. But, you know, from what we know,
how the planets get formed, that's probably what happened. Yeah. And we know the solar wind exists.
We can measure the solar wind. And so we can model what would happen if we didn't have a magnetic field.
So, yeah, there's a lot of things we can do to validate those models. But absolutely, there's modeling
going on all over the place in all of these studies. And, you know, we try to make assumptions.
and when they were trying to find ways to check them
and to validate those assumptions, absolutely.
Another thing we do is we think about like
how life could have evolved.
A lot of the basic chemical building blocks of life
couldn't have formed if we had oxygen in the atmosphere.
So life produced oxygen,
but in lots of cases, it's inhibited by the presence of oxygen.
The kind of life that me and you are,
this aerobic kind of life that relies on oxygen,
is fairly late showing up in the evolutionary record.
And so if we had had oxygen,
oxygen, like outgassed by those volcanoes, we might not have formed life.
Right.
Because the earliest life, like our ancestors were anaerobic, right?
They didn't like oxygen.
Yeah.
They're poisoned by oxygen.
And not just the life itself, but like the chemical building blocks, a lot of those amino acids
that they needed to like bump together in a weird way in the primordial soup.
Those couldn't have formed if there was oxygen.
Because oxygen is just like so excited.
It bonds to everything.
It prevents other things from happening.
So if we'd had oxygen around, we couldn't have made those building blocks and maybe life itself wouldn't have started.
So it's a good thing we didn't have oxygen then, but it's a good thing that we have it now.
Yes, exactly.
And it's like such a delicate balance, right?
We needed oxygen to not be around and then we needed these other life to exist for a while and then to produce a bunch of oxygen so that we could evolve.
It's a crazy story.
Right.
But I guess it's all one constant evolution, right?
You can't just ask, like, we wouldn't be here if we didn't have oxygen, but maybe some other
anaerobic beings would be here having a podcast, right?
Breathing out less hot air than we are.
Yeah, at least less smelly air, maybe.
Yeah, absolutely.
It's just that our particular path relied on all of these things happen in a particular order.
Absolutely, if things had been different, you know, you could have evolved life in lots of other
different ways.
Well, I guess I'm glad that it worked out this way.
And it's good to know these things also because, not just because maybe we want to change.
other planets, but we may also want to find other planets like ours that have an atmosphere.
And so knowing these things might help us find, or maybe our second or fourth home,
our retirement home maybe for humanity.
Yeah, we are just now able to probe the atmospheres of planets around other stars by
seeing how light passes through them as they block their stars.
And understanding how a planet forms its atmosphere and how that atmosphere evolves is really
crucial to answering the question like, is there one out there we could land on? Because there might
be a planet out there in a habitable zone, meaning it's like warm enough to melt water on the
surface, but there might not be an atmosphere. And that's not terribly useful because it can take
millions and millions of years, even if you like plant cyanobacteria in the water on an alien
planet to produce enough oxygen. So it's a really interesting question. Like, how long does this
take? Is it unusual on Earth? Could it happen faster on other planets? Is it already? Is it already?
happening on other planets out there right now with primitive life producing oxygen.
It's a really interesting and deep question and one that might be really important for the
future of humanity.
Yeah, you don't want to like pack up all your things, move halfway across the galaxy, and
then when you get there, it's melt.
That wouldn't be good.
And also for our neighbors, you know, Elon Musk talks a lot about moving to Mars and making
it a second home for humanity, but it's going to take a long time before you can walk on
the surface of Mars and like take a deep breath and survive, not to mention even enjoy it.
all right well it kind of makes you grateful for the air that we have because you know this is kind of
the only thing we have to breathe and the only place in our solar system and maybe in our galaxy
that we know of right now where we could comfortably walk around outside and breathe the air
I'm very grateful I'm full of it you're full of hot air and cold air and all the airs
I'm putting them all on at the same time and burping them and doing other contributions to the air
all at the same time and speaking Icelandic very badly into a microphone for other
people to hear. All right, well, that's the history of our atmosphere, and we hope you enjoyed
that. Thanks for joining us. See you next time.
Thanks for listening, and remember that Daniel and Jorge Explain the Universe is a production
of IHeart Radio. For more podcasts from IHeart Radio, visit the IHeartRadio app, Apple Podcasts,
or wherever you listen to your favorite shows.
December 29th, 1975, LaGuardia Airport.
The holiday rush, parents hauling luggage, kids gripping their new Christmas toys.
Then, everything changed.
There's been a bombing at the TWA terminal.
Just a chaotic, chaotic scene.
In its wake, a new kind of enemy emerged, terrorism.
Listen to the new season of Law and Order Criminal Justice System
on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts.
My boyfriend's professor is way too friendly, and now I'm seriously suspicious.
Wait a minute, Sam. Maybe her boyfriend's just looking for extra credit.
Well, Dakota, luckily, it's back to school week on the OK Storytime podcast, so we'll find out soon.
This person writes, my boyfriend's been hanging out with his young professor.
a lot. He doesn't think it's a problem, but I don't trust her. Now he's insisting we get to know
each other, but I just want her gone. Hold up. Isn't that against school policy? That seems
inappropriate. Maybe find out how it ends by listening to the OK Storytime podcast and the IHeart
Radio app, Apple Podcasts, or wherever you get your podcasts. I'm Dr. Scott Barry Kaufman,
host of the psychology podcast. Here's a clip from an upcoming conversation about how to be a better
you. When you think about emotion regulation, you're not going to choose.
an adaptive strategy which is more effortful to use unless you think there's a good outcome.
Avoidance is easier. Ignoring is easier. Denials easier. Complex problem solving takes effort.
Listen to the psychology podcast on the IHeart Radio app, Apple Podcasts, or wherever you get your
podcasts. This is an IHeart podcast.
