Transcript of YouTube Video: Life In Our Universe | Crash Course Pods: The Universe #8

Transcript of YouTube Video: Life In Our Universe | Crash Course Pods: The Universe #8

The following is a summary and article by AI based on a transcript of the video "Life In Our Universe | Crash Course Pods: The Universe #8". Due to the limitations of AI, please be careful to distinguish the correctness of the content.

Article By AIVideo Transcript
00:00

I've been excited for this conversation

00:01

Katie because I've mentioned it online a

00:04

few times but I don't know if I've

00:05

talked to you about it I've been having

00:07

the

00:08

depression MH and it's not been fun it's

00:12

been challenging but in this process of

00:16

kind of going through a period

00:18

of of darkness and uh and difficulty I

00:23

have taken an astonishing amount of

00:25

solace in this project that we've been

00:28

doing oh good I've been thinking about

00:32

my

00:33

protons and how complicated they are and

00:36

how of course it's difficult for a

00:38

collection of protons this large to make

00:40

it

00:41

through together sticking together you

00:44

know as as a body must and it's made me

00:47

think a lot about what you're calling

00:49

the astrophysics of

00:52

life right but I realize I don't

00:55

actually know anything about the

00:56

astrophysics of life and so it's had me

00:59

thinking speculatively but I'm excited

01:01

for this conversation because after it

01:03

hopefully I'll be able to think in a

01:04

more grounded way about the fact that

01:07

I'm big bang

01:09

stuff and understand a little bit more

01:12

about the relationship

01:15

between the universe and uh

01:23

me a reality I've faced over and over

01:26

again as I've had these conversations

01:28

with Dr Mack is how insignificant life

01:31

on Earth is in respect to our universe

01:34

not only are we living on a speck of

01:36

dust in a tremendously vast space But

01:39

even the type of matter we're made of is

01:42

an afterthought compared to dark energy

01:44

and dark matter that negligibility or

01:48

sheer smallness can evoke a sense of

01:50

wonder but also a sense of futility so

01:54

life typically does not factor into

01:57

cosmology but what about the inverse how

01:59

does cosmology factor into life well

02:03

here's our

02:06

[Music]

02:11

conversation I should say you know

02:13

before we start that my usual area of

02:17

research does not touch life in any way

02:21

but there are some very clear things

02:26

that we can say as astrophysicists

02:30

about the relationship between the

02:32

cosmos and humans and like what we are

02:36

made of and how life works I mean so I

02:38

think that one of the things that we've

02:40

talked about before but I think is is

02:42

good to reiterate is what you just

02:45

mentioned that we are big bang stuff I

02:47

mean if you think about like what we are

02:48

made of by mass if you just kind of add

02:51

up all of our our molecules and atoms

02:55

and stuff by mass we're mostly oxygen

02:58

and then car carbon and then hydrogen

03:02

nitrogen phosphorus calcium but if you

03:05

count by the number of particles that we

03:07

have in us like the number of atoms by

03:09

number we are we are vastly more

03:12

hydrogen so we're something like 63%

03:15

hydrogen wow you know the hydrogen

03:17

nuclei the protons those do come just

03:20

right from The Big Bang and may or may

03:22

not have ever been inside a star that's

03:25

just the Big Bang made a bunch of

03:27

protons and those protons became us most

03:31

of what we are made of is that stuff

03:34

that came from The Big Bang and has not

03:36

become another kind of atom so it's not

03:40

even like a processed hydrogen it's a

03:43

raw

03:44

unfiltered organic hydrogen Straight

03:47

From the

03:48

Source yes exactly yeah so some of the

03:51

hydrogen has been through stars but a

03:53

lot of it is just it was in space it was

03:57

part of the cloud of gas that the Milky

04:00

Way formed out of and the cloud of gas

04:02

that the solar system formed out of and

04:04

became us right became the stuff that we

04:07

are made of those those protons those

04:09

hydrogen nuclei now the rest of the

04:13

atoms in our body the oxygen the carbon

04:15

the Hy the nitrogen the calcium the

04:17

phosphor sulfur all of that kind of

04:18

stuff that was formed inside Stars so in

04:22

order to make us we needed to get

04:24

together not just the protons but a

04:27

bunch of these heavier elements that can

04:30

make structures can make you know solid

04:33

materials that kind of stuff so the Big

04:35

Bang made hydrogen helium a little tiny

04:40

bit of lithium maybe a little little

04:43

tiny bit of

04:44

burum but was mostly hydrogen and

04:49

everything else gets formed in stars or

04:52

through some other process involving

04:55

Stars involving cosmic rays that kind of

04:58

thing so if if you look at like the

05:00

other stuff we're made of so carbon was

05:03

mostly made in low mass stars at the end

05:06

of their lives so like stars like the

05:08

sun when they die they create this you

05:11

know sort of big nebula blow off their

05:14

outer layers and there's processes that

05:16

happen inside and that makes some carbon

05:18

and then also massive stars when they

05:20

explode that creates some heavier

05:21

elements carbon is one of the things

05:24

that's made in that nitrogen is kind of

05:26

similar oxygen is mainly made in the

05:29

explosions of massive stars and then you

05:31

know calcium phosphorus sulfur those are

05:34

all kind of similarly mostly in these

05:37

these massive star explosions sometimes

05:40

in exploding white dwarfs so stars are

05:43

creating everything else that were made

05:45

of there are some elements that are

05:47

mostly made when cosmic rays slam into

05:50

other particles and break them apart and

05:52

so you get like burum and Boron and a

05:55

little bit of lithium some of those are

05:57

made from like cosmic rays like cracking

05:59

open other atoms like doing fion but for

06:02

the most part you look at most of the

06:04

periodic table and it's massive stars or

06:09

end of life processes of stars and the

06:11

reason for that is that you need a lot

06:13

of energy to create heavy elements and I

06:15

think we've talked about this to some

06:17

degree where you know with like a a star

06:22

like our sun fuses hydrogen into helium

06:24

in its core uh that's pretty much all

06:27

the Sun is going to do at some point

06:29

it's going to run out of hydrogen in the

06:30

core it's going to Puff out it's going

06:31

to make a few heavier elements in the

06:33

sort of end of life process but mostly

06:36

it's just going to do hydrogen into

06:37

helium but more massive stars have

06:39

processes going on in their cores that

06:41

can fuse heavier elements they've got

06:43

way more temperature higher temperatures

06:45

more pressure and they can squish

06:48

together all these elements when it gets

06:49

to iron you can't fuse iron and still

06:53

get energy out and so then things get

06:55

more complicated and that things heavier

06:57

than iron you really need like super NOA

07:00

or some kind of much more complicated

07:03

process to get those heavier elements

07:05

you know you can make some amount of

07:06

heavier elements inside the core of the

07:08

star and then most of the stuff that's

07:11

made is really in the Supernova

07:12

explosions and we can look like

07:15

literally just look at the periodic

07:16

table and that will tell us how massive

07:20

an element is and like where it fits in

07:23

that realm right not really well sort of

07:26

yeah I mean you can look at the periodic

07:27

table and see the masses of the elements

07:29

yeah there's a little bit of a some

07:32

subtleties to how those Fusion events

07:35

happen and I don't doubt that man I mean

07:36

the subtleties involved in just like

07:38

what a proton weighs uh has has thrown

07:41

me for an absolute Loop so but in

07:44

general you know if something's heavier

07:46

than iron or not heavier than iron yeah

07:49

but the I mean but the thing is like so

07:51

when I first started learning about

07:52

Stellar Fusion like about you know Stars

07:55

making heavier elements I thought like

07:58

uh you know you you kind of of you kind

08:00

of first learn about like massive stars

08:03

burning carbon and nitrogen and oxygen

08:05

and and they make sort of shells of

08:07

heavier elements in the core and and and

08:10

I kind of thought okay so that's how it

08:12

happens you create these shells of these

08:14

different elements and then those of the

08:16

element that that gets kind of blown out

08:17

into the universe and that's how the

08:20

that's how the um right so like when the

08:22

star explodes that gets spread out and

08:26

that's how we get all the iron and

08:28

oxygen that we need yeah but like a lot

08:31

of it's actually formed like during the

08:34

Supernova so oh like a lot of the carbon

08:38

that's formed in the core of stars kind

08:40

of stays there in the remnant depending

08:44

on what kind of star it is but you know

08:46

the the Supernova itself is is not just

08:49

something that spreads the elements but

08:51

it's also part of what makes the

08:52

elements so you get you dump so much

08:55

energy into all this material so quickly

08:57

a lot of that creat creates a lot of

09:00

these heavier elements so it's it's a

09:02

mix between some of the stuff is just

09:04

formed in the star and you know and gets

09:07

disperse but but in a lot of cases it's

09:09

it's really that those explosions that

09:11

have to happen to create most of like

09:14

the periodic table okay and to create a

09:16

lot of that um a lot of the stuff that

09:18

that's coming out so there's there's

09:20

some interesting subtleties that I was

09:22

kind of reading about um last night and

09:25

I got I got a little bit fixated on

09:28

carbon and I I wasn't sure how much we

09:30

wanted to talk about carbon specifically

09:34

I love talking about carbon because you

09:36

know one of my obsessions is uh biomass

09:39

Global biomass like what is life on

09:42

Earth actually made out of and the way

09:45

they determine that is by number of

09:47

carbon atoms right yeah yeah so carbon

09:51

is a super useful atom for life for for

09:55

creating anything any kind of

09:56

complicated molecules there's a lot of

09:59

it it's very abundant in the universe

10:01

and it it has the ability to form these

10:03

four bonds right so it has four veence

10:06

electrons which means that there's kind

10:07

of four places you can kind of attach to

10:09

a carbon atom and that means that you

10:12

can create really complex chains really

10:14

complex structures with that carbon very

10:17

stable bonds and you can also form

10:19

really strong double or even triple

10:21

bonds with carbon because of the way

10:23

that the electrons are set up and so it

10:25

makes a really great basis for something

10:28

as complicated as life and all life is

10:31

is kind of based on carbon as far as we

10:34

are aware there's in science fiction

10:36

people talk about like Silicon based

10:37

life because you can have sort of

10:39

similar things going on but in in

10:40

practice everything we've seen is is

10:43

carbon based so the carbon is forming

10:45

kind of the backbone of the stuff that

10:48

life is made of there was this this

10:50

weird bit of History around people

10:52

trying to understand how nuclear fusion

10:56

in Stars Works where they ran into this

10:59

problem with carbon which is that like

11:01

it's it's reasonably straightforward to

11:05

create you know helium out of hydrogen

11:08

there's a kind of chain of processes

11:09

that happens but the energetics kind of

11:11

works out in a in a way that makes some

11:13

sense creating carbon in a star is kind

11:16

of complicated in a way that like for a

11:20

long time scientists kind of couldn't

11:22

figure out how that could even happen so

11:24

what you need to do to do that is you

11:26

first fuse together two helium nuclei

11:29

helium four so that's helium with two

11:32

neutrons and two protons in the nucleus

11:34

you fuse the helium four together to

11:36

make burum burum 8 and then somehow you

11:41

need to get another helium to combine

11:43

with the burum to make carbon 12 okay so

11:48

so brillium has has four protons then

11:52

you know add two more you can get um you

11:54

got to do something complicated you can

11:56

get carbon 12 out of that in principle

12:00

but in practice that burum is really

12:03

unstable and just decays very

12:06

quickly and if you throw the helium into

12:10

the brillium that's also really unstable

12:13

and decays really quickly and so you end

12:15

up with this situation where it just

12:18

doesn't seem like there should be enough

12:20

time to create a lot of stable carbon

12:24

right so we're living in a universe that

12:26

has more stable carbon than we would

12:28

anticipate

12:29

based on carb getting made that way yeah

12:32

yeah and there was there was a lot of

12:35

lot of discussion of like can you even

12:36

get all of those elements to fuse do you

12:39

need um do you need like ridiculously

12:42

high temperatures so the first

12:43

calculations needed like billions of

12:45

degrees of temperature to get this

12:47

Fusion to even happen in the first place

12:49

there was some revised calculations they

12:51

they had to figure out Quantum tunneling

12:53

because before they knew about Quantum

12:55

tunneling they couldn't even figure out

12:57

how to get any of these Fusion events to

12:59

happen because these nuclei would be

13:01

positively charged they would repel each

13:02

other and they wouldn't get close enough

13:04

for the strong nuclear force to take

13:05

over for them to actually fuse so they

13:07

had to figure out Quantum tunnel and get

13:09

them to actually fuse but they knew

13:10

these Decay times were really really

13:12

fast and so there was this effort to

13:15

like figure out how carbon ever happens

13:18

and uh Fred Hoy who is a famous

13:20

astronomer and he was what he was an

13:22

interesting figure because he also was

13:24

like super opposed to the idea of the

13:26

big bang and he thought that there must

13:28

be a steady safe universe and I think

13:29

this was sometime around like the 20s or

13:32

30s or I don't know exactly the dates

13:33

but it was early on he was trying to

13:35

figure out how this how carbon could be

13:37

made and he figured out there there had

13:39

to be some kind of like resonance state

13:41

so some kind of excited state of a

13:44

carbon nucleus that would allow it to

13:47

more favorably like form from the burum

13:50

and the helium and then that state could

13:53

Decay into the ground state of carbon 12

13:55

that is kind of stable right and so he

13:57

just predicted there had to be this had

13:59

to exist and he wrote down what the

14:00

energy of it had to be and he's like

14:03

this has to be there or else you know

14:05

Carbon can't happen in any reasonable

14:08

amount and then uh subsequently he

14:12

convinced some experimentalists to do

14:14

some experiments and try and find this

14:16

excited state of carbon and they found

14:17

it and it was there it was where it had

14:19

to be because if it hadn't been there

14:21

you know we wouldn't have carbon and and

14:23

oil was like we have to have carbon

14:24

there has to be this state and so he

14:26

predicted it turns out there is this

14:27

excited state one and something like

14:29

2,000 times that excited state will

14:31

Decay to carbon instead of everything

14:34

just decaying into helium nuclei again

14:37

and that's enough to allow carbon to be

14:41

formed at reasonable levels in Stars

14:43

there's just so many things that had to

14:46

go right yeah it gets weirder too like

14:50

you talked about fine-tuning in the past

14:52

but like this feels like and I know that

14:55

like we're biased because we live in the

14:57

universe that that ended up happening

14:59

right and so like that's going to bias

15:03

us but it is so weird that we needed

15:05

that to happen one out of every 2,000

15:07

times so there could be carbon so there

15:09

could be us and it's one of these things

15:11

like when you look this stuff up because

15:13

I was reading about this to to you know

15:16

prepare to to talk about it because I've

15:18

only only kind of read about it a little

15:20

bit in the past and a lot of the sources

15:23

you find for it are like well this

15:25

proves God yeah yeah yeah I definitely

15:29

call people telling me over the years

15:32

that the universe's bias toward carbon

15:35

is the best indication of a

15:38

God yeah I mean you know and I don't I

15:42

don't think that's a particularly

15:44

compelling argument but it is it is a

15:46

fascinating process and and it gets even

15:48

more interesting because once you have

15:51

carbon 12 you need to make oxygen and

15:54

you do that by throwing another helium

15:56

nucleus at Carbon 12 and if there were a

16:00

resonance in that state also then every

16:03

all the carbon 12 would just turn into

16:05

oxygen and then you wouldn't have carbon

16:07

again and so hoil predicted okay so now

16:10

there can't be an oxygen resonance State

16:12

and there isn't wow turns out and and I

16:15

was reading up on this and some people

16:17

calculated that if you had like a0 5%

16:20

change in the strength of the nucleon

16:22

interactions then Stars would either all

16:25

make carbon or all make oxygen but not

16:27

the other one wow

16:30

and so and so either way if it if it

16:32

went this way or that way there's no us

16:37

yeah yeah yeah and so it's this kind of

16:39

wild I don't know if it's a coincidence

16:42

or just something that because we see it

16:44

it has to have existed right you know

16:47

but there's this kind of interesting set

16:50

of circumstances where it's just not as

16:52

straightforward as you might think to

16:54

form all of the elements that we need to

16:56

form in order for like us to exist but

16:59

and I know that you don't like it when I

17:00

apply scientific reasoning to real life

17:03

um

17:05

but isn't that also true for humans

17:09

right like for individual human lives

17:10

like it's very easy for me to say like

17:13

oh if Sarah hadn't taken that Boxing

17:15

class we would have never met and we

17:17

would have never had kids and our so our

17:19

kids wouldn't exist well well that's

17:22

true right but like if Sarah hadn't

17:24

taken that Boxing class something else

17:26

might have happened right right so in in

17:28

science we call the anthropic principle

17:30

like this idea that like It's tricky to

17:33

assign probabilities to things and so on

17:36

when not having that observation would

17:38

mean you cannot do that observation you

17:39

know what I mean like so often the

17:41

anthropic principle is applied to like

17:43

you know we live on the surface of a

17:44

planet we don't live in the middle of

17:46

the Sun and that's not because there's

17:49

more space on the surface of the planet

17:50

than in the middle of the sun it's just

17:52

because if we lived in the middle of the

17:53

sun we wouldn't be living and we

17:55

wouldn't be able to say that we live in

17:57

the middle of the sun we just wouldn't

17:58

exist right so the fact that we live on

18:00

the surface of Planet means we can talk

18:02

about living on the surface of a planet

18:03

and so that's a kind of anthropic

18:06

argument for the fact that we live here

18:08

or we live in the habitable zone of our

18:10

solar system right we live in a part of

18:12

our solar system where liquid water is

18:14

possible if we lived on you know the

18:17

surface of Neptune or something liquid

18:20

water is impossible we wouldn't be

18:22

living we wouldn't be there to talk

18:23

about it stuff like that and yet it is

18:26

also true that if it's astonishing that

18:29

Sarah took that Boxing class like what

18:32

you know like and it's astonishing that

18:34

we ended up existing like the fact that

18:37

anything exists at all my main

18:40

conclusion from seven and a half

18:42

episodes of learning from you is the

18:44

fact that anything exists at all is a

18:46

real mind blower yes yeah yeah no I'd

18:50

agree I'd agree with that and I guess

18:53

the thing that I'm constantly finding

18:55

out is just all of the kind of the nice

18:58

little stories we have about you know

19:00

this happened then this happened then

19:01

this happened it's all just so much more

19:03

complicated than that if you really dig

19:05

into it and and the the things that feel

19:08

like inevitabilities are kind of not you

19:11

know like life is kind of not an

19:13

inevitability of chemistry in some sense

19:17

right or Nuclear Physics I mean in the

19:19

sense that like Nuclear Physics might

19:22

have happened differently in a way that

19:23

was not going to ever set up the

19:25

conditions for chemistry in life right

19:28

and and you know it's it's nice that it

19:30

came out this way because existence is

19:33

cool but it's also not something that is

19:37

like you know it was it was written into

19:40

the laws of physics that we were going

19:41

to be here and talking about you know

19:44

the

19:44

universe so you don't think that there's

19:46

necessarily anything inherent to the

19:49

laws of physics that

19:52

made life or us inevitable given the

19:56

constant of nature that we observe you

19:58

can draw a straight line in some sense

20:02

from The Big Bang to us right because

20:05

you do get to this point where it's like

20:07

okay big bang makes hydrogen hydrogen

20:09

and helium and then helium hydrogen

20:11

makes stars and stars make more helium

20:13

and make all these other elements and

20:15

because the nuclear interactions are

20:17

what they are it's it's possible to

20:19

create these heavier elements and those

20:20

are going to collect into rocky planets

20:22

and then those rocky planets are

20:24

sometimes going to have life because of

20:26

a sort of process of chemistry to

20:29

biology that happens so in that sense

20:33

yeah I mean I don't know if it's

20:35

inevitable but it's there's a clear

20:38

through line there's a clear story that

20:40

goes there but at some point I guess one

20:44

wonders if the constant of nature as

20:47

they are were inevitable right and and

20:51

that goes that that comes into questions

20:53

about like kind of about Multiverse

20:56

ideas about this idea that maybe there

20:58

are regions of the universe where the

21:00

laws of physics are different which

21:01

could be the case you know when when

21:03

people talk about multiverses usually in

21:06

fiction what they mean is like the many

21:07

worlds interpretation of quantum

21:09

mechanics this idea that every time a

21:10

Quantum event happens the universe

21:12

splits into two where it went different

21:14

ways that's what people use for like

21:17

fictional parallel universe stories

21:19

stuff like that great for fiction great

21:21

for fiction but in physics a lot of what

21:23

we mean when we talk about Multiverse is

21:26

is just the idea that there could be

21:27

different regions of a larger space that

21:30

includes our observable universe but

21:32

beyond that as well in which laws of

21:34

physics might be different you know the

21:36

circumstances the environment might be

21:38

different and different things could

21:39

happen so there could be regions of this

21:42

larger Multiverse where the nuclear

21:45

interactions are slightly different and

21:47

chemistry can't happen or maybe it

21:49

happens very very differently I don't

21:51

know so that could be another anthropic

21:53

bias that we happen to be in this

21:56

situation yeah and that's how ropic

21:59

principle comes up most often in physics

22:01

is this idea of you know I mean

22:04

essentially we don't know why the Conant

22:08

of nature are what they are in a lot of

22:11

cases like the biggest one that people

22:13

complain about is the value of the

22:15

cosmological constant so the strength of

22:17

dark energy essentially we don't know

22:20

why dark energy is here but not zero

22:24

right or not large like the cosmological

22:26

constant is kind of small in some sense

22:28

that makes sense if you're talking about

22:30

the the value of this number and so you

22:32

know we get this acceleration but not

22:34

until the universe has existed for many

22:36

billions of years and you know it

22:38

doesn't prevent the existence of

22:41

galaxies and and things it just after

22:43

they've existed for a long time then at

22:45

some point they're going to not form

22:47

anymore you know so there's this weird

22:48

middle place where the cosmological

22:50

constant is small but not zero and

22:52

people use anthropics to argue that that

22:54

makes sense because a lot of predictions

22:57

from first principles depend depending

22:58

on what your sort of starting

23:00

assumptions are might lead you to a

23:02

cosmological constant that's either zero

23:03

or very large and a universe with a very

23:07

large cosmological constant is not going

23:09

to have planets it's not going to have

23:12

galaxies like it's it's going to be

23:14

accelerating too fast too quickly for

23:16

structure to form a cosmological

23:18

constant of zero is not a problem really

23:21

for the formation of structures so

23:23

arguing that it should be small but not

23:25

zero is a little bit tricky but people

23:27

use anthropic arguments to argue that it

23:29

should be small or zero and the fact

23:31

that it's small is maybe just because of

23:34

you know Chance in This bigger space But

23:37

It's tricky to make those arguments

23:39

because you can't really Place

23:41

probabilities on where we end up in this

23:43

larger space with different values in a

23:45

way that is consistent you have to put

23:48

in a whole lot of assumptions and the

23:49

anthropic principle can kind of help

23:51

with that but it can't push you to exact

23:53

numbers in certain ways and so then you

23:56

have to do something more complicated so

23:58

that that's how it usually comes up is

23:59

something to do with dark energy or or

24:02

maybe even dark matter but yeah it could

24:04

apply to this you know Carbon thing as

24:07

well right like right we wouldn't be

24:10

here if if the carbon resonance weren't

24:12

there right so yeah but it is and we are

24:17

yeah so it's an interesting question

24:21

[Music]

24:24

yeah so every element we are made of

24:27

either comes from The Big Bang itself or

24:30

was made by stars from their core or as

24:33

a result of them exploding that adds a

24:36

bit more of a wow factor to the periodic

24:38

table for me and it turns out it's very

24:41

difficult for stars to create a stable

24:43

version of carbon that element essential

24:46

to Life as We Know It physicists had to

24:48

discover Quantum tunneling the ability

24:50

of some particles to Tunnel through

24:52

barriers and an excited state of carbon

24:55

to prove it was even possible and for us

24:58

to exist they also had to determine that

25:00

oxygen didn't have an excited state add

25:04

that to the fact that we live in a part

25:05

of the universe that allows liquid water

25:07

to exist and that we have just enough

25:10

dark energy to allow planets to form and

25:13

life can seem inevitable but the

25:15

existence of the building blocks of life

25:17

was not inevitable and knowing what we

25:20

know it might even have been

25:26

improbable so I want to ask if I can

25:29

take you forward to the rocky planets

25:33

these rocky planets are

25:35

forming I don't really understand how

25:37

but I trust you that they formed we can

25:39

just kind of walk through how we got

25:41

here great from the beginning of the

25:43

solar system so the solar

25:45

system has been around for something

25:48

like 4 and a half billion years maybe

25:51

just a little bit longer than that so

25:53

the sun formed somewhere around maybe

25:55

4.6 billion years ago so the universe is

25:58

13.8 billion years old it took a while

26:01

for the sun to form and you know it's

26:03

not surprising really that we weren't

26:06

formed way way earlier

26:09

because you need a certain number of

26:11

generations of stars to create enough

26:13

heavy elements to create rocky planets

26:16

and life and depending on where what

26:19

kind of environment you're in in the

26:21

universe that can take a while I mean if

26:23

you were in an environment where there

26:24

are lots of stars forming very very

26:26

quickly like in a really Rich center of

26:29

a galaxy cluster or something like that

26:31

then those time scales can be very short

26:33

cuz massive stars don't live very long

26:35

you can in in some handful of millions

26:38

of years you can have a a situation

26:40

where stars are forming and and you're

26:41

creating a lot of heavy elements in the

26:43

part of the universe that we're in it

26:45

took about three generations of stars

26:47

before like our star is about a third

26:49

generation Star as far as we know so a

26:53

couple of generations of stars did their

26:55

Supernova created their elements

26:58

polluted the interstellar medium we call

27:01

it pollution that's that's a great line

27:03

polluting the interstellar medium yeah

27:05

yeah or

27:08

enrichment sometimes we say enrichment

27:10

we're being nice about it enriching

27:12

feels better than polluting yeah I'm

27:14

quite fond of the idea that we're sort

27:16

of living in some kind of Galactic

27:18

suburb and so things just happen a

27:19

little later here you know like the way

27:21

that a little further out from the city

27:23

people might find out about the hot new

27:25

band a few months after the folk

27:29

yeah yeah and you know there's there's

27:31

arguments about a galactic habitable

27:34

zone this idea that if you live too far

27:37

out or too far in in a galaxy things are

27:40

not as suitable for life so too far out

27:42

you just don't have enough heavy

27:43

elements like there aren't enough

27:45

generations of stars you don't have

27:46

enough enrichment too far in you have to

27:49

deal with like there's a super massive

27:50

black hole there's a lot of radiation

27:52

there's you know maybe Stars forming

27:54

very very quickly going Supernova a lot

27:56

and it's just dangerous

27:58

it's just a dangerous place to be

28:00

because you're you're you're going to

28:02

get zapped by something before life can

28:04

really develop and and that's that's a

28:06

very poorly defined kind of region of

28:09

the of the Galaxy but like we're inside

28:12

a region where it seems like that's a

28:14

reasonable place to live it's a you know

28:17

it's a decent kind of neighborhood for

28:19

you know it's it's not too boring it's

28:21

not too scary right so we live in a

28:24

decent not too boring not too scary

28:26

region of our gy Galaxy and as a result

28:30

this third generation star was able to

28:32

form about 4.6 billion years ago yeah

28:35

yeah and so what happened was the you

28:38

know you had a big cloud of gas and dust

28:40

and and it coalesced and created a a

28:43

disc of material and the sun formed in

28:46

the center where it was really dense

28:48

there was a lot of material there and

28:49

then this the disc first it was like a

28:52

protocell cloud and then it was the star

28:54

and then there's this protoplanetary

28:56

disc and it's just a disc of like gas

28:57

and dust and you know little bits of

28:59

metals or whatever material from that

29:02

protostellar cloud and that slowly

29:05

coalesces into planets so planets sort

29:07

of form in these edes in this uh these

29:09

little knots in this disc and for a long

29:13

time there's you know collisions between

29:16

these protoplanets and you know

29:18

everything's really chaotic but

29:20

eventually the gas and dust in this disc

29:22

gets kind of you know hoovered up by the

29:24

forming planets and you you end up with

29:26

a stable set of of planets going around

29:29

okay and we still don't have a very good

29:31

understanding of that whole process it's

29:33

a complicated process you know you get

29:36

lots of different kinds of solar systems

29:38

that form some with really massive

29:40

planets really close in called hot

29:42

Jupiters those seem to be pretty common

29:44

in the universe we're not entirely sure

29:46

how that goes we don't entirely know why

29:48

the planets are distributed the way they

29:50

are in our solar system and there are

29:51

some tricky bits you know going from

29:53

certain scales where it seems

29:55

complicated to get the material to stick

29:57

together at those scales and not like

29:59

bounce off and so Planet formation is a

30:01

complicated science but eventually you

30:03

end up with you know we have this this

30:05

sort of hot protoplanet like sort of

30:08

molten because everything's kind of been

30:10

crashing together that's the the young

30:12

Earth and then it gets crashed into by

30:14

something about the size of Mars and

30:16

that creates a you know blob of material

30:18

that sort of shoots out and and becomes

30:20

probably some kind of ring and then

30:21

turns into the moon that's the story

30:23

that we think is happening there and so

30:25

then we have the Earth and the moon and

30:28

over time the Earth cools and at some

30:31

point in this process you know it it

30:33

sort of develops water maybe the water

30:35

was kind of already there maybe comets

30:37

came in and brought in water it's a

30:39

little bit unclear it seems like

30:40

probably the water was already there and

30:42

then it kind of was able to collect on

30:43

the surface and the Moon is kind of

30:47

possibly helpful for life and we're not

30:49

really sure of the details of that but

30:51

it it sort of stabilizes the seasons a

30:54

bit so having a large Moon might be

30:56

helpful for life but at this stage it

30:58

doesn't really matter cuz at this stage

30:59

it's just you know there's water there's

31:01

Rock Earth is still kind of warm and we

31:04

think that probably life began like near

31:07

a hydrothermal vent under the ocean most

31:10

likely that seems like a good place

31:12

right like that seems like a good place

31:13

for chemistry to happen it's warm it's

31:16

wet yeah what you really need for life

31:18

as far as we understand it is some kind

31:21

of source of nutrients so you need

31:22

chemicals that can react with each other

31:25

you need energy and specifically you

31:27

need need a gradient of energy there

31:29

needs to be a way to move energy from

31:31

one place to another right so you can't

31:33

just be in a in a uniformly hot space or

31:36

something it has to be possible to you

31:38

know move the energy so you know maybe

31:40

sunlight is a source of energy coming

31:43

from outside and you can do something

31:44

with that or something like a

31:46

hydrothermal vent where you have the hot

31:49

hydrothermal vent and the cooler ocean

31:51

and you can extract energy from that and

31:53

then you need a liquid and probably

31:55

water it seems like I mean all all life

31:58

on Earth involves water in some way

32:00

that's the liquid that life on Earth

32:03

uses there's speculation that maybe you

32:05

can use other liquids as the thing that

32:08

allows the chemicals to move around you

32:10

know people talk about the possibility

32:12

of life in like the methane ocean on

32:15

Titan possibly I mean it's unclear it's

32:18

unclear if you can use other liquids but

32:20

water seems to be the one that I mean

32:22

it's the one everything on Earth uses

32:24

and it's it's how we Define a habitable

32:28

zone when we talk about a habitable zone

32:29

of a solar system is there's kind of a

32:32

distance from the center of the solar

32:34

system where you're close enough to the

32:36

star that it's possible for water to

32:38

exist as liquid but not so far that it's

32:40

all ice right so you don't want it to be

32:42

either steam or ice you want it to be

32:44

able to be liquid on the surface of the

32:46

planet and that's all IL defined because

32:48

you could also have you know a really

32:50

thick atmosphere that would make it so

32:52

that everything is too hot for liquid

32:54

water like on Venus so Venus is

32:56

nominally in the habitable zone of our

32:58

solar system but it's too hot for Life

33:01

Life as We Know It Anyways too hot for

33:03

liquid water and then Mars is nominally

33:06

also in the habital zone but it's got

33:09

basically no atmosphere and so so it

33:11

doesn't have enough atmosphere to have

33:13

liquid water yeah it's it's a little bit

33:15

too cold I mean there are times of the

33:17

year in places in on Mars when it can be

33:19

above freezing on the surface above Z

33:22

Celsius but the um because the

33:24

atmosphere is so thin you can't have

33:25

liquid water MH the ice will sulate but

33:28

that's it so you don't just need to be

33:30

in the habitable zone you also need to

33:32

have the right amount of atmosphere so

33:34

that you can have liquid water yeah yeah

33:37

and that probably took time to develop

33:39

on Earth I would imagine yeah so so at

33:41

some point we had liquid water so we had

33:43

this hydrothermal vent and probably what

33:46

happened at that place is that you had a

33:49

bunch of chemicals and you got this

33:52

chemistry kind of happening and then

33:54

that chemistry sort of by chance created

33:58

some stuff that's like the ingredients

34:00

of RNA so we think it's probably started

34:03

with RNA and then there was this sort of

34:05

what they call molecular natural

34:07

selection which is just kind of like

34:09

lots of sort of interactions between

34:10

molecules that are kind of random but

34:12

then some are like a little bit more

34:14

likely to happen and then that turns

34:16

into biology and actual natural

34:18

selection you get these first RNA cells

34:20

and then those evolve into DNA and and

34:22

that whole process is very complicated

34:24

but there's a kind of logical

34:27

progression that that scientists have

34:28

worked out where you can go from very

34:30

simple sets of organic molecules like

34:34

amino acids and things and through a lot

34:37

of time um I mean we're talking probably

34:40

a billion years or something maybe half

34:43

a billion years I don't know somewhere

34:44

around there to go from these simple

34:47

chemicals to life but if you have a

34:50

whole lot of these chemicals a lot of

34:52

water and a lot of time just from the

34:54

bouncing around from the energy

34:56

injection from the thermal events is

34:58

going to kind of happen and and we've

35:00

done lab experiments where you can make

35:02

the components of RNA from molecules

35:05

that we get just from like Interstellar

35:08

dust or like things that we see out

35:10

there in space so we we see amino acids

35:12

on comets Interstellar dusts meteors

35:15

this stuff just kind of exists out there

35:16

the the sort of building blocks of the

35:19

kinds of chemicals that we think formed

35:21

the first life and then through these

35:23

interactions near this energy source and

35:26

just lots of time and r events we think

35:28

that that can eventually turn into

35:31

something that becomes single cell life

35:34

and so over

35:35

this half billion years or whatever that

35:38

occurs and then we have single cell life

35:40

and then natural selection kicks in in a

35:43

more formal way where the life wants to

35:46

hang around and the only only the life

35:48

that wants to hang around ends up

35:50

hanging around um a different version of

35:53

the anthropic principle perhaps um well

35:56

I mean you end up with you know the

35:58

natural selection in the form of like

36:00

the things that are most adapted to the

36:04

environment progress and the other

36:06

things don't yeah yeah right I don't

36:08

mean to imply that these um single-

36:10

celled organisms were making conscious

36:11

choices about whether to be here um or

36:15

indeed that any of us are right I'm not

36:18

I'm not convinced of that so then we

36:20

have this very very long period yes

36:24

where life is is single cell that's

36:26

about a billion I think yeah before the

36:29

first not single celled right so we had

36:31

single only single- celled organisms for

36:34

longer than we didn't have life on Earth

36:36

that's wild yeah and depending on how

36:39

long you think this all happened I mean

36:41

the earliest fossils are from like half

36:44

a billion years after the formation of

36:46

the earth as far as we know but like it

36:48

could have been much much faster than

36:49

that it could have been like some number

36:51

of millions of years uh we don't know

36:53

exactly but um it could have been

36:56

reasonably quick that the first life

36:58

formed out of this chemistry and then it

37:00

just took a long time for these single

37:02

cells to turn into anything that

37:03

persists enough that we have a a solid

37:06

record of it so when you talk about it

37:09

that way when you talk about it as

37:11

chemistry it doesn't actually seem that

37:12

different from astrophysics like it

37:14

doesn't seem totally separate for me

37:17

that there's a chemistry process that

37:20

leads

37:21

to hydrogen becoming helium or that that

37:26

leads to these massive Supernova

37:28

creating stable carbon and then there's

37:31

a chemistry process that allows amino

37:35

acids to become RNA and then there's a

37:38

chemistry process that allows is just

37:40

everything chemistry well I mean I I

37:43

would call the the earlier bits of that

37:45

sort of nuclear physics rather than

37:46

chemistry but it's all just kind of the

37:48

rearrangement of of matter yeah right

37:51

like through physical processes yeah

37:54

which makes me think about how

37:55

everything is just the rearrangement of

37:56

matter like yeah writing a novel is just

37:59

the rearrangement of matter or making

38:01

making a painting is just the

38:03

rearrangement of matter right you're

38:04

just rearranging paint and canvas into a

38:07

representation of something yeah and

38:09

you're messing around with like

38:11

information content and entropy in in

38:14

complicated ways yeah that's so true

38:18

you're messing around with entropy when

38:19

you're writing a novel maybe that's the

38:21

problem I'm

38:23

having need to accept that I'm

38:25

just just I'm trying to do something

38:28

that's

38:29

fundamentally against what the universe

38:31

wants to do I'm trying to I'm trying to

38:34

make a story that makes sense and the

38:35

universe is like I'm trying to have a

38:36

little more

38:38

disorder that tension is is causing me a

38:41

lot of problems right now Dr Mack I mean

38:43

you'll be comforted to know that it at

38:45

all moments you are actually increasing

38:46

the entropy of the universe because

38:48

you're putting so much Blood Sweat and

38:49

Tears into trying that to to make that

38:52

process of order that it it it is the

38:54

total amount of entropy is still going

38:55

up sure yeah have no of course there's

38:58

no way that I can yeah and even in even

39:01

in that work that I'm doing I'm

39:02

increasing entropy yeah yeah always cool

39:07

yeah that isn't that comforting Just for

39:09

future

39:10

reference I'm

39:11

[Laughter]

39:14

[Music]

39:21

sorry this podcast has experienced a

39:24

lovely reception from the public but we

39:26

did get a one star review from someone

39:28

who wondered is this guy really that

39:31

anxious yeah Anonymous reviewer I am

39:34

really that anxious and in a universe of

39:37

ever increasing disorder where

39:39

everything that comes together will in

39:41

time fall apart I have to confess a

39:43

measure of confusion as to your lack of

39:45

anxiety but of course while there's

39:47

nothing to be done about entropy there

39:49

are ways we can have at least some peace

39:51

of mind including life insurance which

39:54

can help those you will inevitably leave

39:56

behind

39:58

and with policy genius you can find life

39:59

insurance policies that start at just

40:01

$292 per year for $1 million of coverage

40:05

some options offer same day approval and

40:07

avoid unnecessary medical exams policy

40:10

genius lets you compare quotes from

40:11

America's Top insurers in just a few

40:13

clicks to find your lowest price and

40:15

policy genius gives you unbiased advice

40:17

from a licensed expert support team

40:19

which is why they have thousands of

40:21

festar reviews on Google and trust pilot

40:23

so don't put off life insurance make it

40:25

easy with policy genius

40:27

head to policygenius.com crashcourse or

40:30

click the link in the description to get

40:32

your free life insurance quotes and see

40:34

how much you could save that's

40:36

policygenius.com

40:50

[Music]

40:54

crashcourse so a few generations of

40:56

stars formed super noi that spread their

40:58

elements across the interstellar medium

41:00

polluting or enriching it depending on

41:03

how you look at it and those elements

41:05

coales to form our solar system from

41:08

there the process was actually quite

41:10

linear Nuclear Physics led to the

41:12

formation of RNA which led to the

41:14

formation of DNA which led to the

41:16

formation of unicellular life likely

41:19

near a hydrothermal vent beneath the

41:21

surface of the ocean that whole process

41:23

can seem very orderly given that all

41:26

creation cre

41:27

disorder in the grand scheme of

41:33

things I don't know if if this is more

41:35

or less comforting to you

41:38

but it seems like if this process

41:42

happened on Earth and it happened

41:43

probably pretty

41:44

quickly then it's very likely to have

41:47

happened in other places right it has to

41:49

have right because like

41:52

otherwise the idea that Earth is alone

41:54

in this just seems kind of absurd

41:57

yeah I hear arguments you know where

41:59

it's like well we just don't know either

42:01

way but like like we we have a pretty

42:04

good idea of how this chemistry stuff

42:07

happens in an environment like the early

42:09

Earth and we know of something like

42:13

5,000 planets around other stars that

42:15

exist those planets exist and and maybe

42:18

only you know a few dozen are what we

42:21

would call habitable in the sense of

42:23

being like at the right distance from

42:24

their star and we don't know anything

42:26

about their atmospheres so maybe they're

42:27

all like Venus we don't know or maybe

42:29

they're all like Mars but like some of

42:32

them must have some kind of environment

42:36

that's not horribly dissimilar to that

42:39

of the early Earth and and even like in

42:41

our own solar system there are several

42:43

places where we think this kind of life

42:46

might have happened I mean we don't have

42:48

another planet in the habitable zone

42:50

right now that seems to have liquid

42:53

water on the surface but Mars probably

42:55

had liquid water billions of years ago

42:58

a few billion years ago it seems to have

43:00

had liquid water we have really good

43:01

evidence of that in fact that a few

43:03

billion years ago Mars did have liquid

43:07

water we see evidence of you know River

43:10

beds stuff like that and and there's an

43:13

active search for you know signs of past

43:16

life on Mars it may or may not exist we

43:18

don't know but it certainly had

43:21

conditions that were pretty similar to

43:22

Earth in a lot of ways in its early

43:25

history and un fortunately something

43:28

happened where it kind of lost its

43:31

atmosphere possibly because the magnetic

43:33

field failed because the planet might

43:36

have cooled down too quickly or

43:37

something like that and the atmosphere

43:39

was blown off by the Sun so it did have

43:41

a thick atmosphere that was suitable for

43:43

liquid water it doesn't anymore but at

43:45

some time it did right and then the

43:48

other interesting thing about our solar

43:49

system is we have several other

43:51

candidates for where life could

43:53

currently exist and they're not anywhere

43:55

near the habitable zone because the

43:57

habitable zone is this narrowly defined

44:00

like could you have liquid water on the

44:01

surface of a rocky planet but what you

44:03

really need for life is chemistry an

44:06

energy source and water right and if you

44:09

go out to the outer solar system some of

44:12

the moons of Jupiter and Saturn have

44:16

chemistry we've seen evidence of the

44:18

right kind of mix of chemicals in those

44:20

moons they seem to have liquid water

44:23

under the surface one way or another and

44:26

they have the energy source of the tidal

44:28

heating of being in orbit around a gas

44:32

giant so they're constantly being like

44:35

pulled and stretched by the gravity of

44:37

the planet they're orbiting so we've got

44:39

around Jupiter we've got Europa gamine

44:41

and Kalisto all seem to have the

44:44

possibility of subsurface oceans Europa

44:47

is a particularly exciting one because

44:49

we have evidence that there's like salty

44:51

water under the icy surface it's like

44:53

100 km of ice and then we think there's

44:55

like salty water underneath that

44:57

and there's some likelihood we think of

44:59

hydrothermal vents under the surface of

45:02

Europa I mean anything could be under

45:04

the surface of Europe I mean there could

45:06

be fish like like we have no idea but it

45:09

seems like it has the right conditions

45:11

right and then Saturn we got Enceladus

45:14

which also has very clear evidence of

45:17

undersurface water well there's there's

45:19

like a spray coming out of of Enceladus

45:22

we can see like venting liquid you know

45:26

coming out of Enceladus so we think that

45:28

there's hydrothermal vents probably

45:29

under enceladus's surface as well and

45:31

this giant ocean that's spraying

45:33

material out into the universe right and

45:36

then Titan is an interesting one too

45:38

because Titan also seems to have

45:41

probably a subsurface liquid water ocean

45:43

we're not certain about that but it

45:44

looks like it probably has that but also

45:46

it has like a whole like hydrosphere

45:49

like it's got It's got liquid on the

45:51

surface it's just not liquid water it's

45:52

liquid methane so Titan has this really

45:55

thick atmosphere like methane

45:58

clouds and there's liquid methane oceans

46:02

and and and rivers and and ponds and

46:05

like lakes on the

46:07

surface and then the rocks and things

46:10

are solid water ice so you have all

46:12

these like Boulders of solid water ice

46:14

and mountains of solid water ice and

46:16

then you have these lakes and it really

46:18

is liquid methane and I mean we don't

46:21

know if anything can live in liquid

46:24

methane but it's it's liquid it's got

46:26

complex organic chemicals probably maybe

46:30

there's something living in those oceans

46:32

we don't know so it's not just

46:37

that life we presume would be common

46:41

because it wasn't that hard to make it

46:43

here it was hard to make complex life

46:45

but it wasn't that that hard obviously

46:47

we've done it we've done a bunch of it

46:48

right like we've got a lot of different

46:49

life on Earth it does seem like if

46:52

correct me if I'm wrong that we only

46:54

made eukaryotic cells once so that seems

46:56

to have been a big jump that seems to

46:58

have been kind of challenging but we did

47:00

it of course you don't have to have a

47:02

eukariotic cell to have life and there

47:03

may be other ways of developing life and

47:05

everything and what this makes me

47:07

think and I'm interested to see if I'm

47:11

on the wrong track here because I

47:12

probably am is that it may be in fact

47:16

that life is sort of inevitable if you

47:20

have these elements of of water or some

47:24

kind of liquid that works and you have

47:27

the potential for chemistry and you have

47:29

this ability to do energy transfer like

47:33

it could be that it just happens almost

47:35

every time it it could be yeah we we

47:37

really don't know I mean it seems

47:39

logical that when all the ingredients

47:42

are together probably it'll happen but

47:45

yeah we really don't know and there's

47:46

been lots of efforts over the years to

47:49

try to quantify our uncertainty in that

47:53

and the one that's most famous is What's

47:55

called the Drake equation so Frank Drake

47:57

who who passed away only just very

47:59

recently I think within the last year

48:01

was this famous astronomer who who just

48:03

wrote down an equation to like quantify

48:07

how many specifically how many

48:09

technological civilizations are there

48:11

out there in the galaxy we can talk to

48:13

okay so this is a very specific question

48:15

this isn't how much life is there this

48:16

is can we talk to them on the radio

48:19

right how many how many people can we

48:20

talk to on the radio this equation I

48:22

should say is not meant to be like you

48:25

write down the solution to this equation

48:28

and it gives you a number and you trust

48:29

that number this equation is really

48:31

about like how to talk about what we

48:34

don't understand understanding the

48:36

variables even if we don't understand

48:38

the numbers yeah yeah so the the

48:40

equation is really about like let's

48:43

write down what we need to know to

48:45

answer this question what's write down

48:47

what are the big uncertainties right and

48:48

so the there are lots of different ways

48:50

to write down this equation one way you

48:52

can do it is you can say okay the the

48:53

number of technological civilizations we

48:56

can talk to okay that's going to be

48:57

equal to First you need to know the

48:59

number of stars right then you need to

49:02

know what fraction of those stars have

49:04

planets which we think I mean we know

49:06

there's a large number of stars there's

49:07

like 400 billion in our galaxy right

49:10

okay uh we think that

49:12

probably quite a lot of them most stars

49:14

probably have planets that number is

49:16

somewhere close to one okay um wow in

49:20

terms of stars that have planets then

49:23

then you want to know the number of

49:25

habitable zone planets per Star right

49:29

and that number is pretty uncertain but

49:32

it's also probably not that far from one

49:34

really maybe like a tenth somewhere in

49:37

that range like on average it's such an

49:40

astrophysicist thing to say it's not

49:42

that far from one it's probably like

49:44

0.1 yeah or maybe like 01 if you're

49:47

really pessimistic right but

49:49

like which is pretty close to one it's

49:52

pretty close to one to you guys it's

49:53

it's within a it's within a couple

49:55

orders of magnitude right like as a

49:57

cosmologist that's basically one

49:59

Whatever Right Round Up round down you

50:01

get it's it's somewhere around one

50:03

between

50:04

1% and

50:06

90% yeah these are all very very

50:09

uncertain numbers okay sure of course

50:12

okay but you need that yeah so somewhere

50:13

around there and then but then then it

50:15

gets to the point where we just have no

50:17

idea right okay so then the fraction

50:20

that have life okay that's the next

50:22

number in this in this equation so the

50:25

textbook that I that I taught my inro to

50:27

astronomy class from a couple years ago

50:31

says that for that number the

50:33

pessimistic estimate is 01 the

50:35

optimistic estimate is one we don't

50:38

actually have any idea right like we

50:41

have no idea right of course because

50:42

we've never seen a second example of it

50:45

yeah and we have no idea how inevitable

50:47

any of those steps were that we looked

50:49

at okay so then let's say that's

50:51

fraction of that have life maybe it's

50:53

close to one we don't know and then the

50:56

next one is the fraction of those

50:58

planets with life in which some species

51:00

evolves to intelligence okay so there's

51:02

the fraction that has life and then the

51:03

fraction that have intelligence out of

51:05

the ones that have life okay and again

51:10

no idea the textbook also puts it

51:12

between 01 and one but like we don't

51:15

know and and that's that's a funny thing

51:17

too because like I mean depending on how

51:19

you define

51:21

intelligence that kind of seems to have

51:23

happened once on earth right

51:27

like and and I I think about this a lot

51:29

because you know you look at a place

51:31

like like New Zealand right New Zealand

51:34

kind of broke off from other places

51:36

pretty early on when when there were a

51:37

whole bunch of birds right like

51:40

everything was kind of dinosaurs and

51:41

birds and New Zealand's like native

51:45

ecology the native species were just

51:47

Birds right like they have like birds

51:50

filled all the niches and two Atara yeah

51:52

yeah and the and the and the couple of

51:54

reptiles right so Birds filled all the

51:56

nichas but they never turned into like

51:59

talking birds like I mean talking in the

52:02

sense of like I mean they can say some

52:03

of them can say some words right but

52:05

like but they never figured out like

52:06

what's keeping the Stars apart yeah or

52:08

or got anywhere close to that yeah they

52:10

didn't turn into what we would normally

52:12

call a sort of technologically

52:15

intelligent species right right and they

52:17

had there was time there was lots of

52:19

time uh but it was the mammals that went

52:22

that direction the birds didn't yeah

52:25

right and so it really only has happened

52:27

once and then when you consider the fact

52:29

that our species which is overwhelmingly

52:31

the most technologically sophisticated

52:33

species in in the history of life on

52:35

Earth is about 250,000 years old maybe

52:38

300,000 years old brand new you know

52:41

younger than elephant younger than Bears

52:43

younger than giraffes like just brand

52:46

new and and and we don't you know we

52:49

don't know we know how old we are but

52:52

you know to get to the unknown unknowns

52:54

we have no idea how long we'll be here

52:57

we have no idea like what the end of the

52:58

temporal range is yeah and that's

53:01

another thing that comes into this

53:03

equation it's written in different ways

53:05

in this uh case it's like the fraction

53:09

of existence during which intelligent

53:11

life survives right yeah okay so it's

53:14

you can write it in terms of like the

53:16

number of years that that intelligent

53:18

life sticks around before destroying

53:21

itself or being destroyed by something

53:23

that number can vary a lot

53:26

no no joke it can yeah

53:30

so that's right so so then it's like

53:34

maybe it takes a really long time for

53:36

intelligence of the sort of like

53:38

technological intelligence to develop

53:40

and and maybe we don't have that much

53:42

time where we can exist without

53:45

something terrible happening either by

53:47

our own hand or something else we don't

53:50

seem to have any stars nearby that could

53:52

go

53:53

supernova anytime soon in an

53:56

astronomical sense but like it could

53:59

have been the case that we could have

54:00

evolved on a planet that was you know

54:03

next to a big uh massive star that was

54:06

going to go supernova and totally

54:07

sterilize the surface of the world right

54:10

like that could happen quite a lot we

54:12

don't we don't know so that's one of

54:14

those things that that is also a big

54:15

unknown in this equation is like how

54:18

long do we persist and and I should say

54:20

like I feel bad talking about

54:22

intelligent life and not including like

54:24

the Dolphins and the octopi but like

54:26

there octopuses I guess is the correct

54:28

plural anyway but we're talking

54:30

specifically about like people we can

54:31

talk to yeah and we might get better at

54:33

talking to dolphins or talking to whales

54:35

or talking to octopuses over time but in

54:39

terms of the current

54:41

technology there is a different level

54:43

now it's possible that octopuses tried

54:45

it all out for us you know like 50

54:48

million years ago and they were like

54:49

this is not good no y'all don't want to

54:51

do this and they like just went back to

54:53

living happily in the ocean and and

54:55

doing their thing we don't know but like

54:57

yeah I think we have to acknowledge that

55:00

humans are a little different from other

55:02

yes animals currently yeah and we don't

55:05

know how often stuff like this happens

55:08

and we also don't yeah to your point we

55:09

don't know how long it lasts because

55:11

it's very weird and it does feel a

55:12

little fragile because it's never

55:14

happened before so far as we can tell

55:17

and because we're becoming much more

55:19

powerful very quickly you know like

55:21

we've only been in the atomic age for

55:24

one human lifetime

55:27

so are we going to be in the atomic age

55:29

for five human lifetimes or 5,000 human

55:31

lifetimes I have no idea yeah and I and

55:34

I think it's it's probably not that easy

55:36

to do something that would wipe out all

55:39

human life on earth like I could even

55:41

easily imagine humans doing something to

55:44

ourselves that basically wipes out

55:45

technological civilization our ability

55:48

to talk to their planets right we could

55:49

slow ourselves down a lot you know we

55:52

could definitely slow ourselves down and

55:54

it's kind of hard for me to imagine

55:57

us I don't know maybe we do maybe maybe

56:00

I need to be a little more optimistic I

56:02

was about to say it's hard to imagine us

56:03

not screwing that up but maybe that's

56:06

just the darkness talking the truth is

56:08

that we've shown an astonishing capacity

56:10

so far for adapting to new um new worlds

56:15

like that's always been our gift right

56:17

is the two gifts I think we have are

56:19

that we can adapt to new spaces and that

56:21

we collaborate better than almost any

56:22

other species I guess ants but like we

56:26

we have a mix of an ability to

56:27

collaborate and an ability to reason

56:29

that's pretty cool yeah and and you know

56:32

depending on who you ask human

56:35

biological evolution may or may not be

56:37

significant anymore but we've we've

56:40

found ways to get around that by using

56:42

our big brains to change our

56:44

environments to suit us better instead

56:46

of changing us to suit our environments

56:48

better and and we have a lot of tools in

56:50

that direction well and it's just

56:52

astonishing to me that we've left our

56:53

atmosphere that took so much work that

56:56

you know that that's so hard I think if

57:01

you pitch that idea to humans 500 years

57:03

ago they would have been like that

57:04

sounds very very difficult yeah it is it

57:07

is amazing what we've done like the

57:10

thing that I find so amazing is just how

57:12

much we know right that we've been able

57:16

to understand the evolution of the

57:19

Universe from basically the beginning to

57:21

now and not just that we know it but

57:23

that we're able to share it and pass it

57:26

on that we have these technologies that

57:29

allow us to communicate that knowledge I

57:31

think about that a lot in terms of you

57:34

know why the Scientific Revolution

57:35

happened when and where it did was

57:38

partly because of like medical journals

57:40

and scientific journals and the ability

57:42

to share information really widely

57:46

across time and

57:47

space and then the miracle of being able

57:50

to learn from the dead being able to

57:52

hear from them directly you know Drake

57:55

isn't with us but but the equation is I

57:58

love that yeah yeah and there's

58:01

something lovely as well about the fact

58:04

that I mean I guess there's like

58:06

evolutionary pressure that we like to

58:08

solve puzzles right that that that's

58:11

there's evolutionary pressure for for

58:12

that making us happy to better

58:15

understand things but I think it's also

58:17

lovely that that we like to talk about

58:19

them too right that we like to teach

58:22

that we like to share information that

58:24

we like to that that it can be enough of

58:26

a reward just to have the joy of sharing

58:29

something cool and not necessarily be

58:32

personally benefiting from that like you

58:35

see that in in the scientific Community

58:37

all the time yeah the light in

58:39

somebody's eye when you help them

58:41

understand something is I mean maybe

58:43

there's an evolutionary pressure to do

58:45

that but I don't I don't think that's

58:47

ultimately why we do it and and even

58:49

where where there is no um you know

58:51

there's no profit incentive the narrow

58:53

incentives don't make sense with

58:55

something like Wikipedia or with uh

58:58

teaching college where a lot of times

59:01

the uh the the the profit incentives

59:03

don't make a ton of sense but there's

59:05

still there's still joy in it there's

59:07

still meaning in it and it doesn't have

59:09

to be grounded in those incentives it

59:11

can be grounded in something else like

59:12

something like love H yeah love for

59:17

other people love for the subject love

59:20

for the um for the joy of learning and

59:22

the joy of sharing it like that that

59:25

that there can be something there yeah

59:27

and it and it's on all sides you know

59:30

it's it's a it's a joy to learn it's a

59:32

joy to teach it's a joy to just share

59:36

enthusiasm and excitement and and be

59:41

part of all of us gaining a better

59:44

understanding of the universe that we

59:45

live in and and you know sort of

59:47

expanding our perspectives and our

59:49

Horizons that is is a wonderful

59:52

thing you've made me feel better good

59:56

I'm very glad I'm glad we got there I'm

59:59

glad we settled on that that's so

01:00:02

true we're not so bad after all we're

01:00:05

all right we're all right we might make

01:00:13

[Music]

01:00:16

it so in a strange sense our existence

01:00:20

wasn't inevitable until it was given

01:00:23

everything we learned in today's episode

01:00:26

it's not hard to see how life got

01:00:27

started and yet the fact that we exist

01:00:30

is still pretty astonishing to me after

01:00:34

all other planets and moons may be

01:00:36

habitable but there is no other us at

01:00:39

least as far as we know in one sense the

01:00:42

only thing that could have happened

01:00:43

happened but I also feel an unavoidable

01:00:46

sense of gratitude that matter

01:00:48

rearranged the way it did in a way that

01:00:51

formed beings who in Dr Max's words can

01:00:54

experience the joy of sharing something

01:00:57

cool in the next episode our journey

01:00:59

will finally lead us to now Katie will

01:01:02

give us a snapshot of the Universe from

01:01:04

our present day vantage point and I'll

01:01:06

ask some questions I've been patiently

01:01:08

holding back for eight long

01:01:15

[Music]

01:01:16

episodes the show is hosted by me John

01:01:18

Green and Dr Katie Mack this episode was

01:01:21

produced by Hannah West edited by lonus

01:01:23

Oben housee with music and mixed by

01:01:25

Joseph tuna n medish special thanks to

01:01:27

the perimeter Institute for theoretical

01:01:29

physics our associate script editor is

01:01:31

Annie fillenworth our editorial

01:01:33

directors are dror Darcy Shapiro and

01:01:35

Megan moery and our executive producers

01:01:37

are Heather di Diego and Seth Radley

01:01:40

this show is a production of complexly

01:01:43

if you want to help keep crash course

01:01:44

free for everyone forever you can join

01:01:46

our community on patreon at

01:01:48

patreon.com/crashcourse

01:01:56

h

01:01:58

[Music]