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.
00:00 | I've been excited for this conversation |
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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 |
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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 |
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01:01:56 | h |
01:01:58 | [Music] |