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A Conversation with Democritus | Ben Moore | TEDxZurich


imagine I gave you a time machine and

imagine I gave you a time machine and you could choose any dates in the past

you could choose any dates in the past

you could choose any dates in the past or the future where would you go – this

or the future where would you go – this

or the future where would you go – this was a question I was asked and I at

was a question I was asked and I at

was a question I was asked and I at first I thought well given what we’ve

first I thought well given what we’ve

first I thought well given what we’ve learned in the last 400 years just

learned in the last 400 years just

learned in the last 400 years just imagine what’s possible in the future

imagine what’s possible in the future

imagine what’s possible in the future 400 years from now or ten thousand years

400 years from now or ten thousand years

400 years from now or ten thousand years from now let’s go there and see what

from now let’s go there and see what

from now let’s go there and see what it’s like and on second thoughts you

it’s like and on second thoughts you

it’s like and on second thoughts you might get there to the future and you

might get there to the future and you

might get there to the future and you find that humans have been assimilated

find that humans have been assimilated

find that humans have been assimilated by robots which well maybe that’s not so

by robots which well maybe that’s not so

by robots which well maybe that’s not so much fun after all or even worse you get

much fun after all or even worse you get

much fun after all or even worse you get to the future and we’ve really messed

to the future and we’ve really messed

to the future and we’ve really messed things up and there’s no life at all so

things up and there’s no life at all so

things up and there’s no life at all so I’ll play it safe with my time machine

I’ll play it safe with my time machine

I’ll play it safe with my time machine I’ll go back two and a half thousand

I’ll go back two and a half thousand

I’ll go back two and a half thousand years I’ll go back to have a

years I’ll go back to have a

years I’ll go back to have a conversation with Democritus Democritus

conversation with Democritus Democritus

conversation with Democritus Democritus was a philosopher many historians of

was a philosopher many historians of

was a philosopher many historians of science say he was the first real

science say he was the first real

science say he was the first real scientist

scientist

scientist he made the remarkable advance that the

he made the remarkable advance that the

he made the remarkable advance that the world could be understood with logic

world could be understood with logic

world could be understood with logic thought and experiment rather than just

thought and experiment rather than just

thought and experiment rather than just appealing to the gods and magic only

appealing to the gods and magic only

appealing to the gods and magic only fragments of his writings remain but I

fragments of his writings remain but I

fragments of his writings remain but I would like to tell you about four topics

would like to tell you about four topics

would like to tell you about four topics he wrote about I would like to go back

he wrote about I would like to go back

he wrote about I would like to go back and show Democritus what we’ve learned

and show Democritus what we’ve learned

and show Democritus what we’ve learned about his predictions and tell him what

about his predictions and tell him what

about his predictions and tell him what we’ve learned from science he looked at

we’ve learned from science he looked at

we’ve learned from science he looked at the matter around him and he studied it

the matter around him and he studied it

the matter around him and he studied it and he speculated that everything was

and he speculated that everything was

and he speculated that everything was made of particles so small you can’t see

made of particles so small you can’t see

made of particles so small you can’t see them

them

them he called him a tan

he called him a tan

he called him a tan now I can’t show democritus a picture of

now I can’t show democritus a picture of

now I can’t show democritus a picture of an atom a photograph of an atom but at

an atom a photograph of an atom but at

an atom a photograph of an atom but at first I would show him the PhD thesis of

first I would show him the PhD thesis of

first I would show him the PhD thesis of Albert Einstein he graduated from the

Albert Einstein he graduated from the

Albert Einstein he graduated from the University of Zurich in 1905 that’s the

University of Zurich in 1905 that’s the

University of Zurich in 1905 that’s the cover of his thesis and you might think

cover of his thesis and you might think

cover of his thesis and you might think it would be for the discovery is about

it would be for the discovery is about

it would be for the discovery is about space and time and relativity but no

space and time and relativity but no

space and time and relativity but no it’s 17 short pages beautiful pages of

it’s 17 short pages beautiful pages of

it’s 17 short pages beautiful pages of physics and mathematics

physics and mathematics

physics and mathematics that describe how to measure the sizes

that describe how to measure the sizes

that describe how to measure the sizes of molecules his theory was applied on

of molecules his theory was applied on

of molecules his theory was applied on the image there you see some jittering

the image there you see some jittering

the image there you see some jittering particles that’s Brownian motion those

particles that’s Brownian motion those

particles that’s Brownian motion those are very small specks of pollen floating

are very small specks of pollen floating

are very small specks of pollen floating on water chittering around because

on water chittering around because

on water chittering around because they’re being bombarded by the molecules

they’re being bombarded by the molecules

they’re being bombarded by the molecules in the water and from the random path

in the water and from the random path

in the water and from the random path they make you could use the work that

they make you could use the work that

they make you could use the work that I’m Stein laid out in his thesis to

I’m Stein laid out in his thesis to

I’m Stein laid out in his thesis to calculate the size of the water

calculate the size of the water

calculate the size of the water molecules and indeed 100 years ago it

molecules and indeed 100 years ago it

molecules and indeed 100 years ago it was shown that the molecules were

was shown that the molecules were

was shown that the molecules were smaller than the wavelength of light so

smaller than the wavelength of light so

smaller than the wavelength of light so you can’t actually shine a light onto

you can’t actually shine a light onto

you can’t actually shine a light onto them to take a photograph but I could

them to take a photograph but I could

them to take a photograph but I could show

show

show Democritus this this is the first image

Democritus this this is the first image

Democritus this this is the first image of a molecule that was made actually in

of a molecule that was made actually in

of a molecule that was made actually in 2009 by researchers at IBM Zurich they

2009 by researchers at IBM Zurich they

2009 by researchers at IBM Zurich they used what is called an atomic force

used what is called an atomic force

used what is called an atomic force microscope which is like a mechanical

microscope which is like a mechanical

microscope which is like a mechanical very fine slither of material that is

very fine slither of material that is

very fine slither of material that is pushed across the molecule with a laser

pushed across the molecule with a laser

pushed across the molecule with a laser and it has little sensors piezoelectric

and it has little sensors piezoelectric

and it has little sensors piezoelectric sensors on it and they can move this

sensors on it and they can move this

sensors on it and they can move this around the molecule in three dimensions

around the molecule in three dimensions

around the molecule in three dimensions picking up its charge field and from

picking up its charge field and from

picking up its charge field and from that you can make the image on the top

that you can make the image on the top

that you can make the image on the top there which correspond exactly to those

there which correspond exactly to those

there which correspond exactly to those total diagrams you learn about in

total diagrams you learn about in

total diagrams you learn about in chemistry quite beautiful but what’s at

chemistry quite beautiful but what’s at

chemistry quite beautiful but what’s at the center of those connecting places

the center of those connecting places

the center of those connecting places they’re the atoms well that I could also

they’re the atoms well that I could also

they’re the atoms well that I could also show to Democritus because just a few

show to Democritus because just a few

show to Democritus because just a few years ago researchers in the Netherlands

years ago researchers in the Netherlands

years ago researchers in the Netherlands and Germany they built a quantum

and Germany they built a quantum

and Germany they built a quantum microscope this was the first picture of

microscope this was the first picture of

microscope this was the first picture of an Assam hydrogen atom that was made in

an Assam hydrogen atom that was made in

an Assam hydrogen atom that was made in 2013 quantum microscope

2013 quantum microscope

2013 quantum microscope pretty complicated thing but what you’re

pretty complicated thing but what you’re

pretty complicated thing but what you’re looking at here is is a picture made up

looking at here is is a picture made up

looking at here is is a picture made up by ejecting the electrons out of the

by ejecting the electrons out of the

by ejecting the electrons out of the hydrogen atom looking at where they fall

hydrogen atom looking at where they fall

hydrogen atom looking at where they fall onto a detector and reconstructing how

onto a detector and reconstructing how

onto a detector and reconstructing how where they came from and what you’re

where they came from and what you’re

where they came from and what you’re seeing there is really the wave function

seeing there is really the wave function

seeing there is really the wave function the probability function of where the

the probability function of where the

the probability function of where the electrons can be found quite different

electrons can be found quite different

electrons can be found quite different to those sort of planetary orbit type

to those sort of planetary orbit type

to those sort of planetary orbit type pictures that I was taught in school at

pictures that I was taught in school at

pictures that I was taught in school at least now Democritus

least now Democritus

least now Democritus might wonder where all of these atoms

might wonder where all of these atoms

might wonder where all of these atoms came from and prior to this year I

came from and prior to this year I

came from and prior to this year I wouldn’t have been able to answer that

wouldn’t have been able to answer that

wouldn’t have been able to answer that question but there was a remarkable

question but there was a remarkable

question but there was a remarkable event that took place some months ago

event that took place some months ago

event that took place some months ago for one-minute fabric of space vibrated

for one-minute fabric of space vibrated

for one-minute fabric of space vibrated stretched and expanded it was picked up

stretched and expanded it was picked up

stretched and expanded it was picked up by gravitational wave detectors in

by gravitational wave detectors in

by gravitational wave detectors in Europe and America a rough location

Europe and America a rough location

Europe and America a rough location could be identified after this source

could be identified after this source

could be identified after this source that was disturbing space time and

that was disturbing space time and

that was disturbing space time and astronomers all around the world focused

astronomers all around the world focused

astronomers all around the world focused the telescope’s into that region and

the telescope’s into that region and

the telescope’s into that region and they saw an explosion of light decaying

they saw an explosion of light decaying

they saw an explosion of light decaying away from some cosmic event that had

away from some cosmic event that had

away from some cosmic event that had occurred that blue dot there is shining

occurred that blue dot there is shining

occurred that blue dot there is shining with the light of a billion stars what

with the light of a billion stars what

with the light of a billion stars what it comes from is a merger between two

it comes from is a merger between two

it comes from is a merger between two neutron stars this is an artist’s

neutron stars this is an artist’s

neutron stars this is an artist’s representations neutron stars are what’s

representations neutron stars are what’s

representations neutron stars are what’s left over when a giant star collapses at

left over when a giant star collapses at

left over when a giant star collapses at the end of its life and its core

the end of its life and its core

the end of its life and its core condenses into a very dense state of

condenses into a very dense state of

condenses into a very dense state of neutrons now what’s this all got to do

neutrons now what’s this all got to do

neutrons now what’s this all got to do with atoms well it was found that these

with atoms well it was found that these

with atoms well it was found that these mergers between dead stars this is where

mergers between dead stars this is where

mergers between dead stars this is where the heavier elements are actually

the heavier elements are actually

the heavier elements are actually created before this observation we were

created before this observation we were

created before this observation we were missing part of the puzzle as to where

missing part of the puzzle as to where

missing part of the puzzle as to where atoms came from and now we have a

atoms came from and now we have a

atoms came from and now we have a complete picture we can look at the

complete picture we can look at the

complete picture we can look at the periodic table of atoms and say where

periodic table of atoms and say where

periodic table of atoms and say where everything came from this is it here so

everything came from this is it here so

everything came from this is it here so the hydrogen in your bodies about 20% of

the hydrogen in your bodies about 20% of

the hydrogen in your bodies about 20% of you originates in the Big Bang 13.8

you originates in the Big Bang 13.8

you originates in the Big Bang 13.8 billion years ago that’s how old most of

billion years ago that’s how old most of

billion years ago that’s how old most of you are there’s no other source of

you are there’s no other source of

you are there’s no other source of hydrogen since then

hydrogen since then

hydrogen since then the oxygen in your bodies was made in

the oxygen in your bodies was made in

the oxygen in your bodies was made in exploding supernova massive stars at the

exploding supernova massive stars at the

exploding supernova massive stars at the end of their lives and then some of the

end of their lives and then some of the

end of their lives and then some of the trace elements that

trace elements that

trace elements that would be dead without like iodine

would be dead without like iodine

would be dead without like iodine there’s only a few grams in in our

there’s only a few grams in in our

there’s only a few grams in in our bodies but we can’t live without it

bodies but we can’t live without it

bodies but we can’t live without it that was all made in the exploding

that was all made in the exploding

that was all made in the exploding neutron stars quite a story quite an

neutron stars quite a story quite an

neutron stars quite a story quite an accomplishment of science to figure out

accomplishment of science to figure out

accomplishment of science to figure out the origin of all these elements the

the origin of all these elements the

the origin of all these elements the next thing

next thing

next thing Democritus talked about was the night

Democritus talked about was the night

Democritus talked about was the night sky he speculated that the stars that

sky he speculated that the stars that

sky he speculated that the stars that glowed were actually distant Suns like

glowed were actually distant Suns like

glowed were actually distant Suns like our Sun he couldn’t prove that because

our Sun he couldn’t prove that because

our Sun he couldn’t prove that because there were no telescopes at this time so

there were no telescopes at this time so

there were no telescopes at this time so I’d like to go back and show him a

I’d like to go back and show him a

I’d like to go back and show him a telescope I would like to show him one

telescope I would like to show him one

telescope I would like to show him one of the most beautiful images ever taken

of the most beautiful images ever taken

of the most beautiful images ever taken this is by the Hubble Space Telescope so

this is by the Hubble Space Telescope so

this is by the Hubble Space Telescope so I will just step out the way because you

I will just step out the way because you

I will just step out the way because you can just watch this and I’ll comment

can just watch this and I’ll comment

can just watch this and I’ll comment over a little bit of it I can’t show

over a little bit of it I can’t show

over a little bit of it I can’t show Democritus our own galaxy cuz we’re in

Democritus our own galaxy cuz we’re in

Democritus our own galaxy cuz we’re in the middle of it but I can show him

the middle of it but I can show him

the middle of it but I can show him Andromeda which is our nearest neighbor

Andromeda which is our nearest neighbor

Andromeda which is our nearest neighbor it contains hundreds of billion stars

it contains hundreds of billion stars

it contains hundreds of billion stars like our own Milky Way this image is a

like our own Milky Way this image is a

like our own Milky Way this image is a composite of many pointings of the

composite of many pointings of the

composite of many pointings of the hubble space telescope to show the whole

hubble space telescope to show the whole

hubble space telescope to show the whole image you would need 600 of these

image you would need 600 of these

image you would need 600 of these screens

screens

screens to what you’re seeing are close to a

to what you’re seeing are close to a

to what you’re seeing are close to a billion stars and I at least are not

billion stars and I at least are not

billion stars and I at least are not used to seeing a billion things from

used to seeing a billion things from

used to seeing a billion things from here by scanning over this image you can

here by scanning over this image you can

here by scanning over this image you can get a sense scale of a single galaxy

get a sense scale of a single galaxy

get a sense scale of a single galaxy [Music]

[Music]

[Music] one of the next

one of the next

one of the next predictions that Democritus made was

predictions that Democritus made was

predictions that Democritus made was that there should be planets out there

that there should be planets out there

that there should be planets out there in space like the earth and that is one

in space like the earth and that is one

in space like the earth and that is one of the most remarkable accomplishments

of the most remarkable accomplishments

of the most remarkable accomplishments that we’ve actually made in astronomy in

that we’ve actually made in astronomy in

that we’ve actually made in astronomy in the last century I think is the

the last century I think is the

the last century I think is the discovery that nearly all of the stars

discovery that nearly all of the stars

discovery that nearly all of the stars we see in the night sky have their own

we see in the night sky have their own

we see in the night sky have their own planets orbiting them get back in a

planets orbiting them get back in a

planets orbiting them get back in a minute to describe how we’ve understood

minute to describe how we’ve understood

minute to describe how we’ve understood that

that

that [Music]

[Music]

[Music] this song I actually broke is from my

this song I actually broke is from my

this song I actually broke is from my last album I wrote it for my wife I hope

last album I wrote it for my wife I hope

last album I wrote it for my wife I hope you like it

you like it

you like it [Music]

I always I’ve been looking at these

I always I’ve been looking at these images for 30 years as an astrophysicist

images for 30 years as an astrophysicist

images for 30 years as an astrophysicist I always it always makes you feel so

I always it always makes you feel so

I always it always makes you feel so small and insignificance

small and insignificance

small and insignificance but also it fills me with this or about

but also it fills me with this or about

but also it fills me with this or about how amazing that universe actually is

how amazing that universe actually is

how amazing that universe actually is we’ve learnt so much but there’s still

we’ve learnt so much but there’s still

we’ve learnt so much but there’s still an awful long way to go to really

an awful long way to go to really

an awful long way to go to really understand some of the complicated

understand some of the complicated

understand some of the complicated things like why there is something and

things like why there is something and

things like why there is something and not nothing so each of these little

not nothing so each of these little

not nothing so each of these little pixels contains a star something like

pixels contains a star something like

pixels contains a star something like the Sun some smallest and larger we’re

the Sun some smallest and larger we’re

the Sun some smallest and larger we’re scanning through to the center of

scanning through to the center of

scanning through to the center of Andromeda and then the end of the movie

Andromeda and then the end of the movie

Andromeda and then the end of the movie will zoom out

so how how did Democritus come up with

so how how did Democritus come up with the idea that there are planets orbiting

the idea that there are planets orbiting

the idea that there are planets orbiting these stars I would like to ask him that

these stars I would like to ask him that

these stars I would like to ask him that it’s quite a remarkable prediction he

it’s quite a remarkable prediction he

it’s quite a remarkable prediction he made and as I mentioned we’ve learned

made and as I mentioned we’ve learned

made and as I mentioned we’ve learned that most stars out there in our galaxy

that most stars out there in our galaxy

that most stars out there in our galaxy have their own worlds orbiting them how

have their own worlds orbiting them how

have their own worlds orbiting them how do we know that with one technique is

do we know that with one technique is

do we know that with one technique is quite simple and it’s the most commonly

quite simple and it’s the most commonly

quite simple and it’s the most commonly used technique to find planets around

used technique to find planets around

used technique to find planets around other worlds and here’s a little example

other worlds and here’s a little example

other worlds and here’s a little example of how we do that if the alignment is

of how we do that if the alignment is

of how we do that if the alignment is just right that planet will orbit in

just right that planet will orbit in

just right that planet will orbit in front of the star this is an example of

front of the star this is an example of

front of the star this is an example of Venus transiting the Sun and our

Venus transiting the Sun and our

Venus transiting the Sun and our telescopes are not powerful enough to

telescopes are not powerful enough to

telescopes are not powerful enough to see the planets themselves they’re too

see the planets themselves they’re too

see the planets themselves they’re too small and too faint but the planet has a

small and too faint but the planet has a

small and too faint but the planet has a small size and it blocks out some of the

small size and it blocks out some of the

small size and it blocks out some of the Starlight and in the graph you can see

Starlight and in the graph you can see

Starlight and in the graph you can see the intensity of light and the Sun drops

the intensity of light and the Sun drops

the intensity of light and the Sun drops by a tenth of a percent so by looking

by a tenth of a percent so by looking

by a tenth of a percent so by looking for these dips in starlight we can find

for these dips in starlight we can find

for these dips in starlight we can find planets orbiting of the Worlds and by

planets orbiting of the Worlds and by

planets orbiting of the Worlds and by the amount that the light dips we can

the amount that the light dips we can

the amount that the light dips we can figure out how big the planet is that’s

figure out how big the planet is that’s

figure out how big the planet is that’s blocking the star lines putting all the

blocking the star lines putting all the

blocking the star lines putting all the few thousand planets together that have

few thousand planets together that have

few thousand planets together that have been discovered so far onto one plot it

been discovered so far onto one plot it

been discovered so far onto one plot it looks like this this is a an orrery

looks like this this is a an orrery

looks like this this is a an orrery these are all real planetary systems

these are all real planetary systems

these are all real planetary systems observed around stars in our galaxy the

observed around stars in our galaxy the

observed around stars in our galaxy the diversity was quite shocking to

diversity was quite shocking to

diversity was quite shocking to astronomers because there’s so much

astronomers because there’s so much

astronomers because there’s so much variety in the number of configurations

variety in the number of configurations

variety in the number of configurations of solar systems out there there are

of solar systems out there there are

of solar systems out there there are some were like our own with planets

some were like our own with planets

some were like our own with planets orbiting at the same distance from their

orbiting at the same distance from their

orbiting at the same distance from their stars others were quite different you

stars others were quite different you

stars others were quite different you had all the planets orbiting within the

had all the planets orbiting within the

had all the planets orbiting within the distance of Mercury there are planets

distance of Mercury there are planets

distance of Mercury there are planets orbiting binary stars there are planets

orbiting binary stars there are planets

orbiting binary stars there are planets of all shapes and sizes it’s quite

of all shapes and sizes it’s quite

of all shapes and sizes it’s quite remarkable even the nearest star Proxima

remarkable even the nearest star Proxima

remarkable even the nearest star Proxima be in the Alpha Centauri triple star

be in the Alpha Centauri triple star

be in the Alpha Centauri triple star system that has its own world orbiting

system that has its own world orbiting

system that has its own world orbiting it and just this last week we’ve heard

it and just this last week we’ve heard

it and just this last week we’ve heard about Rosslyn 128 which has a earth-like

about Rosslyn 128 which has a earth-like

about Rosslyn 128 which has a earth-like planet in the habitable

planet in the habitable

planet in the habitable eleven light-years away Democritus was

eleven light-years away Democritus was

eleven light-years away Democritus was right in those three statements so far

right in those three statements so far

right in those three statements so far the last statement that survives that he

the last statement that survives that he

the last statement that survives that he made was that many of these worlds out

made was that many of these worlds out

made was that many of these worlds out there would be dead and barren and empty

there would be dead and barren and empty

there would be dead and barren and empty but many will be filled with life in the

but many will be filled with life in the

but many will be filled with life in the next ten years we will be able to see if

next ten years we will be able to see if

next ten years we will be able to see if Democritus was right or not we can’t

Democritus was right or not we can’t

Democritus was right or not we can’t obviously go there today because we

obviously go there today because we

obviously go there today because we don’t have the technology but we can

don’t have the technology but we can

don’t have the technology but we can observe life on the surfaces of these

observe life on the surfaces of these

observe life on the surfaces of these worlds by looking for bio signatures bio

worlds by looking for bio signatures bio

worlds by looking for bio signatures bio signatures are molecules that wouldn’t

signatures are molecules that wouldn’t

signatures are molecules that wouldn’t be present in the atmospheres of worlds

be present in the atmospheres of worlds

be present in the atmospheres of worlds if those worlds didn’t have life here’s

if those worlds didn’t have life here’s

if those worlds didn’t have life here’s an example we have Venus the Earth and

an example we have Venus the Earth and

an example we have Venus the Earth and Mars and those graphs show the sunlight

Mars and those graphs show the sunlight

Mars and those graphs show the sunlight that’s passed through the atmospheres of

that’s passed through the atmospheres of

that’s passed through the atmospheres of these planets and some of the molecules

these planets and some of the molecules

these planets and some of the molecules in the atmosphere have blocked the

in the atmosphere have blocked the

in the atmosphere have blocked the sunlight and you get those dips so you

sunlight and you get those dips so you

sunlight and you get those dips so you see all these worlds have carbon dioxide

see all these worlds have carbon dioxide

see all these worlds have carbon dioxide but only the earth has ozone they’re

but only the earth has ozone they’re

but only the earth has ozone they’re very prominent which comes from free

very prominent which comes from free

very prominent which comes from free oxygen and water too so oxygen is a bio

oxygen and water too so oxygen is a bio

oxygen and water too so oxygen is a bio signature of life it’s produced by

signature of life it’s produced by

signature of life it’s produced by living things if there was no life on

living things if there was no life on

living things if there was no life on earth there would be no oxygen in its

earth there would be no oxygen in its

earth there would be no oxygen in its atmosphere at the moment our telescopes

atmosphere at the moment our telescopes

atmosphere at the moment our telescopes are just not big enough to detect these

are just not big enough to detect these

are just not big enough to detect these bio signatures in other worlds but

bio signatures in other worlds but

bio signatures in other worlds but coming online we have these remarkable

coming online we have these remarkable

coming online we have these remarkable instruments and they’re going to look at

instruments and they’re going to look at

instruments and they’re going to look at this effect when the planets class in

this effect when the planets class in

this effect when the planets class in front of their stars some of the

front of their stars some of the

front of their stars some of the Starlight will pass through their

Starlight will pass through their

Starlight will pass through their atmospheres they will measure the

atmospheres they will measure the

atmospheres they will measure the spectrum and search for those chemicals

spectrum and search for those chemicals

spectrum and search for those chemicals that would indicate life these are the

that would indicate life these are the

that would indicate life these are the instruments that are coming online we

instruments that are coming online we

instruments that are coming online we have the next generation Space Telescope

have the next generation Space Telescope

have the next generation Space Telescope the James Webb telescope with its six

the James Webb telescope with its six

the James Webb telescope with its six meter gold-plated mirror that’s going to

meter gold-plated mirror that’s going to

meter gold-plated mirror that’s going to be launched in just two years and then

be launched in just two years and then

be launched in just two years and then we have this remarkable telescope from

we have this remarkable telescope from

we have this remarkable telescope from the European Southern Observatory with

the European Southern Observatory with

the European Southern Observatory with its 40 meter mirror those

its 40 meter mirror those

its 40 meter mirror those carved to scale in front of the

carved to scale in front of the

carved to scale in front of the observatory though with these telescopes

observatory though with these telescopes

observatory though with these telescopes we can find if there is oxygen in the

we can find if there is oxygen in the

we can find if there is oxygen in the atmospheres of these are the worlds

atmospheres of these are the worlds

atmospheres of these are the worlds we’ve already actually detected water on

we’ve already actually detected water on

we’ve already actually detected water on some planets but oxygen is harder and

some planets but oxygen is harder and

some planets but oxygen is harder and there are other molecules we can look

there are other molecules we can look

there are other molecules we can look for such as nitrous oxide from decaying

for such as nitrous oxide from decaying

for such as nitrous oxide from decaying plants Missal chloride from fires

plants Missal chloride from fires

plants Missal chloride from fires because only once living things can burn

because only once living things can burn

because only once living things can burn so that would be a strong indicator of

so that would be a strong indicator of

so that would be a strong indicator of life or maybe life is sort of like

life or maybe life is sort of like

life or maybe life is sort of like ourselves and happily pollutes its

ourselves and happily pollutes its

ourselves and happily pollutes its atmosphere and we can detect the

atmosphere and we can detect the

atmosphere and we can detect the chlorofluorocarbons in their worlds so

chlorofluorocarbons in their worlds so

chlorofluorocarbons in their worlds so Democritus I think would be quite

Democritus I think would be quite

Democritus I think would be quite impressed by our discoveries he might

impressed by our discoveries he might

impressed by our discoveries he might also ask the same question as many of us

also ask the same question as many of us

also ask the same question as many of us given all of these worlds out there how

given all of these worlds out there how

given all of these worlds out there how comes life hasn’t already visited us and

comes life hasn’t already visited us and

comes life hasn’t already visited us and I I would be able to show him a picture

I I would be able to show him a picture

I I would be able to show him a picture of a UFO because the CIA just

of a UFO because the CIA just

of a UFO because the CIA just Declassified its database of UFOs and

Declassified its database of UFOs and

Declassified its database of UFOs and there are thousands of terrible images

there are thousands of terrible images

there are thousands of terrible images like this from the sixties and

like this from the sixties and

like this from the sixties and unfortunately that’s the best I have to

unfortunately that’s the best I have to

unfortunately that’s the best I have to show to Democritus even though today we

show to Democritus even though today we

show to Democritus even though today we have a billion high-resolution

have a billion high-resolution

have a billion high-resolution smartphone cameras around the world

smartphone cameras around the world

smartphone cameras around the world still no one good picture of a UFO or an

still no one good picture of a UFO or an

still no one good picture of a UFO or an alien and you know this is this is known

alien and you know this is this is known

alien and you know this is this is known as the Fermi paradox and I think I’ve

as the Fermi paradox and I think I’ve

as the Fermi paradox and I think I’ve uncovered the answer to that why

uncovered the answer to that why

uncovered the answer to that why intelligent life is leaving it alone

intelligent life is leaving it alone

intelligent life is leaving it alone and we haven’t seen it yet and I will

and we haven’t seen it yet and I will

and we haven’t seen it yet and I will leave you with the last image

thank you very much

thank you very much [Applause]

”

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