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Where Did Water Come From?

12:05EnglishBy PBS EonsTranscribed Jul 15, 2026
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0:00

4.5 billion years ago earth was off to a

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rocky start we just collided with

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another early planet the size of mars a

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cataclysmic event that melted both

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planets and spun off a sizable chunk of

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lava that cooled into our moon this

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impact set the stage for the haitian eon

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named of course for hades the greek god

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of the underworld it was a name that

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matched earth's generally hellish vibes

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at that point since our planet was so

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hot that our atmosphere actually

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contained vaporized gaseous rock we're

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talking temperatures around 2 000

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degrees celsius but as the earth and the

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moon began to cool something new formed

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on earth's surface liquid water which

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seems standard after all 71 of the earth

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is covered in our estimated 366

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trillion gallons of water except we

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shouldn't have that water we formed too

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close to the sun mercury venus and mars

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are all super low on water so where did

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ours come from and why do we have so

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much of it well it's complicated and

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still debated but we think our water

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came from a few unlikely sources

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space dust and even the sun

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water itself isn't actually that

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uncommon in our solar system it's just

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further out for example jupiter's moon

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europa is a quarter of the earth's size

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but has twice as much water as we do and

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that has to do with the fact that europa

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formed farther away from the sun because

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in the beginning of our solar system we

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were all star stuff our solar system is

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formed from a nebula the dusty remains

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of an exploded star as that star dust

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collided and collapsed it formed our sun

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and the gravity of that young sun made

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all the rest of the dust spin around it

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in a flat plate like cloud called a

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protoplanetary disk but our early sun

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was hot and soon that disk of dust began

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to differentiate solar and magnetic

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winds blasted light gases away from the

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sun leaving mostly heavier elements like

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iron and silica behind which is why

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earth is a rocky planet that's what was

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in our section of the disk lots of iron

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and lots of silica we also had some of

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the ingredients for water but not all

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water is made of hydrogen and oxygen and

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oxygen is pretty heavy so we have a lot

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of it in fact though it only makes up

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about 21 of our atmosphere oxygen binds

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so readily to silica and iron that it's

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the most common element on our planet

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but oxygen is only part of what you need

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for water and hydrogen is really light

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so it got blown out towards jupiter

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saturn and other planets which now have

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a lot of water ice so if it didn't form

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here to start with where did we get that

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missing ingredient where did our

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hydrogen come from and when did it get

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here the easy answer is we got pelted

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with it water ice and hydrogen hang out

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in the outer solar system but sometimes

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they come inwards in the form of space

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pebbles aka asteroids and meteorites and

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there is a specific type of meteorite

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called a chondrite that is full of water

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but i don't mean full of water like a

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gusher you can't crack open a meteorite

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like a coconut and sip star water from

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it as much as i would like to as much as

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we would like to do instead the solo

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hydrogen and the complete h2o water

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molecules have become part of the

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chemical structure of the minerals that

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make up chondrites these include

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minerals like serpentine chlorite and

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smektite which hold on to their water

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tight this is actually how most of

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earth's water is stored today while we

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have a bunch of liquid water we estimate

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that earth's rocks hold maybe 18 times

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the amount of water that our oceans have

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so how do you get that water out of

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these minerals well the easiest way is

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to melt it which isn't always going to

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happen just by flinging those

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water-bearing minerals at the earth

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after all we have solid chondrite

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meteorites that hit our planet and

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didn't melt but that's because they hit

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today if they'd hit earth in the haitian

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that would have been a much different

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story back in the beginning of the

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haitian anything that hit the surface

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would have just melted straight into our

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magma oceans there hydrogen met oxygen

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and the resulting water superheated into

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gas lighter than magma the water vapor

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would bubble up and out into our

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atmosphere but this process was a race

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against the clock because our magma

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surface was cooling and once a solid lid

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of rock formed no more water could

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escape the oldest traces of rocks we

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found date to about 4.4 billion years

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old so that's probably when the lid of

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solid rock formed but those rocks have

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signs of something surprising they were

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exposed to a liquid ocean yep as soon as

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the earth cooled enough to put a cap on

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the magma we had an ocean that said it

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was probably a little different than the

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oceans we see today earth's atmosphere

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in the early hayden was full of carbon

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dioxide and was very thick potentially

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as thick as

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215 bars of pressure which is 215 times

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what it is now with all that pressure

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and heat earth's surface was

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weird today water turns to gas when it

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reaches 100 degrees celsius but if you

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change the pressure you can change when

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water turns to gas you can even do this

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by walking up a mountain at the top of

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mount everest where air pressure is a

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third of what we see at sea level water

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turns to gas at only 68 degrees celsius

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and in the haitian the much thicker

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atmosphere meant that the reverse was

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happening it was so thick that even when

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the surface was 230 degrees celsius

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water didn't boil so our first ocean was

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super heated fortunately for us that

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superheated ocean didn't last by the end

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of the haitian four billion years ago

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the surface of the earth was very

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similar to what it's like today a rocky

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crust an ocean of liquid but not

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superheated water and an atmosphere of

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about the same pressure as today so from

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meteorites to magma to air to

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superheated oceans that should be the

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story of earth's water but there's one

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really big problem with this story turns

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out the chemical composition of the

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water and the hydrogen and chondrite

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meteorites doesn't actually match the

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chemical composition of most of the

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water on earth the water that is in our

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rocks when we say chemical composition

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what we mean is isotopes or types of

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hydrogen there are two really important

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isotopes of hydrogen the regular brand

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with one proton and one electron and

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what's known as deuterium with a proton

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and neutron the addition of a neutron

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makes deuterium heavier than regular

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hydrogen most of the deuterium in our

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solar system was actually formed in the

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big bang and it's a huge component of

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chondrite meteorites they're heavy with

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this old type of hydrogen the oceans are

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pretty heavy too but our modern oceans

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aren't actually a great representation

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of our early water for one they're not

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230 degrees celsius and for another

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they've been sitting on our surface for

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4.4 billion years so we know they've

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undergone some changes strangely if we

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want to understand what our liquid water

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looked like 4.4 billion years ago we

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actually have to look at the water

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that's contained within our rocks when

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earth's magma oceans cooled enough to

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form a seal of hard rock not all the

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water in the magma escaped into the

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atmosphere a lot of it was trapped below

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the surface in a layer of earth known as

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the mantle over time pieces of the

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mantle have been shoved to the surface

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through plate tectonics and we've been

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able to look at the hydrogen the rocks

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of the mantle contain and it's a lot

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lighter than the hydrogen we see in the

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oceans which is part of why the source

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of earth's water is still somewhat

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debated how could we have such light

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water in our rocks when chondrites have

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such heavy water this problem has

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spurred a lot of research in the last

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decade scientists did find a special

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meteorite called an instatite that has

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lighter hydrogen but most of them think

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there's not enough of these meteorites

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to make up the difference then in 2021

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scientists reported on some interesting

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samples that were collected from an

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asteroid and maybe came up with the

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answer they found that the samples had a

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uniquely high level of light hydrogen

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but to confirm their growing suspicions

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of where that hydrogen came from they

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had to replicate the process so they

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measured the hydrogen and water content

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of olivine crystals before and after

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they exposed them to the equivalent of

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solar wind when they looked at them

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afterwards they found that just like the

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asteroid samples they had a crust of

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accumulated water built with light

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hydrogen so where did this light water

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come from well it's literally light

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water because it came from the sun solar

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winds from our sun shoot out a lot of

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particles including protons when those

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protons hit dust in their path they can

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sometimes steal an electron and a proton

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plus an electron is light hydrogen slam

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that light hydrogen into a rock with

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some oxygen in it and boom you've made

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light water or more realistically slap

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that hydrogen ion into some localized

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space dust or a meteorite when that

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falls to earth it carries down light

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water into our magma ocean which is then

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trapped in our mantle over time so the

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story of water on earth is

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complicated during the haitian we

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accumulated light water and stored it in

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the rocks that became our mantle but

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meteorites continued to rain down and

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our oceans eventually became full of

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much heavier water so the water that you

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drink today has had quite a journey to

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get here and it isn't all from the same

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source it came from space as a

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combination of meteorites and sunburnt

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dust it melted into our magma then

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bubbled out and rained down into

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superheated puddles eventually it cooled

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enough to let life form so while the

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story of where earth's water came from

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is incredibly complex what it ultimately

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means is that your existence boils down

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to space dust and sky pebbles

10:07

wednesday october 12th is national

10:09

fossil day and we've made it an annual

10:11

tradition to do something fun on the

10:13

eons channel to celebrate this year it's

10:15

a four hour live stream michelle cali

10:18

and i will be here on youtube playing

10:20

paleontology games answering your

10:22

questions and hanging out with special

10:23

guests we are so grateful for the

10:25

wonderful community that has grown

10:27

around this channel and we want to give

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you an inside look at who makes eons and

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how it gets made it's a real team effort

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from our writers and editors to our

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producers and our patrons so we hope

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you'll join us then for what we're

10:38

calling eons live an epic live stream i

10:42

would pronounce that epoch but an epoch

10:44

live stream doesn't make sense when you

10:46

say it like that

10:48

hope to see you there so now that you

10:49

know about the origins of our water be

10:51

sure to check out the search for the

10:53

earliest life to find out what might

10:54

have been the first earthling and we're

10:57

star struck by this month's eontologists

11:00

annie and eric higgins chase r shambo

11:02

colton jake hart john davidson ing alex

11:05

tamai and melanie lamb carnival by

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becoming an ianite at patreon.com eons

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you can get fun perks like submitting a

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joke for us to read like this one from

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derek helling what do you call two

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machyrotis's wearing sleeveless jackets

11:19

best friends

11:21

i guess anybody could be best friends

11:23

wearing sleeveless jackets versus little

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saber-tooth things but whatever fun

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thanks for your joke

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and as always thank you for joining me

11:33

in the atom low studio subscribe at

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youtube.com eons for more adventures in

11:37

deep time

11:42

[Music]

11:46

anything that hit the surface would have

11:47

just melted straight into our oceans

11:50

made of magma

11:54

ah

11:56

[Music]

12:00

laser beams on their heads

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