Sean Carroll's Mindscape: Science, Society, Philosophy, Culture, Arts, and Ideas - 259 | Adam Frank on What Aliens Might Be Like
Episode Date: December 11, 2023It wasn't that long ago that topics like the nature of consciousness, or the foundations of quantum mechanics, or prospects for extraterrestrial life were considered fringey and disreputable by much o...f the scientific community. In all these cases, the tide of opinion is gradually changing. Life on other worlds, in particular, has seen a remarkable growth in interest -- how life could start on other worlds, how we can detect it in the solar system and on exoplanets, and even thoughts about advanced alien civilizations. I talk with astrophysicist Adam Frank about some of those thoughts. We also give the inside scoop on what professional scientists think about UFOs. Blog post with transcript: https://www.preposterousuniverse.com/podcast/2023/12/11/259-adam-frank-on-what-aliens-might-be-like/ Support Mindscape on Patreon. Adam Frank received a Ph.D. in physics from the University of Washington. He is currently the Helen F. and Fred H. Gowen Professor in the Department of Physics and Astronomy and Distinguished Scientist at the Laboratory for Laser Energetics at the University of Rochester. Among his awards are the National Honors Society Best Book in Science award, and the Carl Sagan Medal from the American Astronomical Society. His new book is The Little Book of Aliens. Web Site U Rochester web page Wikipedia Amazon author page
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Hey, everyone, it's Cal Penn.
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audiobook club on the IHeart Radio app or wherever you get your podcasts. Hello everyone and
welcome to the Mindscape podcast. I'm your host, Sean Carroll. As a working scientist, one of the
things that I've had to do over the years is apply for grant money. And for theoretical
physicists, this is a funny thing because you're supposed to say not only what you're interested in,
the topic you're going to be working on, but what achievements you will have, what progress you
will make. This is very difficult to do as a theoretical physicist. You don't know what's going to
happen before you do it. As an experimenter, you can at least say what experiment you will build
and when you will turn it on, what you hope to see, but of course, experimenters also don't know
exactly what they're going to see. This is not only for theoretical physicists. There are kinds of
experiments or observations where you can say what you're going to do.
But the outcome is so unpredictable that it's actually kind of hard to wrap your brain around what would happen under different circumstances.
One of those examples is the search for extraterrestrial life.
I'm one who believes that it is plausible that we will find life elsewhere in the universe, and also we are not ready for that.
Science fiction authors have thought about the discovery of alien life for a long time, mostly, I have to say, mostly in unrealistic ways. And I don't blame them. You know, they want to tell good stories. So they very often have structures of intelligence and technology and civilizations amongst the aliens that might be a little bit higher or a little bit lower than ours, but are at least recognizable.
right, a galactic empire. As soon as you say the words galactic empire, you kind of know what you have in
mind. It's not a coincidence that Star Wars is basically a Western or basically some kind of
samurai film, right? Now, there's more sophisticated science fiction than Star Wars, but still,
it's just hard as human beings to wrap ourselves, wrap our brains around the idea of what would
an alien civilization be like that is a billion years more advanced than we all.
are. And that's very possible that that's what we find, either a billion years more advanced or
a billion years less advanced in terms of evolutionary timescale, in which case it's little tiny
organisms that we can't really have a conversation with. And I don't really think that we as a
species have thought this through because it's easy to dismiss it as kind of science fictiony,
right? Science fiction authors have talked about looking for and finding alien life for a long time,
so we associate it with science fiction, not with serious science. This is a point made by today's guest, Adam Frank.
Adam is an astrophysicist at the University of Rochester. He has a new book out called simply the Little Book of Aliens.
And he explains in the podcast how not too long ago the entire field of astrobiology was just
considered fringy. It was just considered too speculative. You couldn't get any money to do it,
et cetera. And this is even if you just thought about how do we do the chemistry and the geology
and the so forth to allow life to exist on other environments. What you would think, I hope, now,
is a very straightforward scientific question that we've already talked about on the podcast.
But there is also the possibility that we find not only unicellular life somewhere out there in the universe, but intelligent life.
And it's hard to remove the connotations or associations with UFO conspiracy theorists and things like that.
But we should because it's an important thing that could actually happen to us.
Of course, maybe it won't.
There's the famous Fermi paradox that says there should.
have been aliens that we could easily detect already, but there hasn't been. So it's very possible
that there just aren't any technologically advanced civilizations out there in the world,
but we should keep an open mind about this. I think it's also very plausible that there will be.
So that's what we're talking about in today's podcast. We're going to talk about what kinds of aliens
there could be, how you would go look for them, trying to separate the seriousness from the less
serious ways of talking about this. And best of all, we will let you in on how real,
working scientists think about UFOs and associated controversies.
So with that, let's go.
Adam Frank, welcome to the Minescape Podcast.
Sean, it's great to be here.
So you've written a book about aliens, a little book because I guess we haven't discovered
them yet.
I'm hoping that after we discover them, the big book will be forthcoming.
Well, the book was little because what I really wanted was to give, I wanted to write a book
that was accessible as possible to as broad and old.
audience as possible.
There's some obvious reasons, so lots of people will buy it.
But more than that, right now, the question of life in the universe is one that gets so
much attention, both because of the scientific advances, but more because of what the hype
that sort of goes around with UFOs and UAPs.
And I wanted people to have a fun, fast entry into everything that's happening, both in
that subject, I took on that subject.
But more importantly, what's happening with things like the James Webb Space Telescope,
what's happening at the frontiers of astrobiology, because that's really the exciting part.
We may be the last generation that doesn't know the answer to the question, are we alone?
Yeah, I mean, that's the nice thing about the subject, right, is that you're talking about real science.
Maybe it's not the nice thing, but a thing is that there's real science as well as a little bit of sensationalism,
and we'll get into that.
Right.
Let me just start by orienting ourselves here.
Like, what kind of aliens are we talking about here?
Not in the UFO sense, but there are extraterrestrial life forms.
There could be extraterrestrial life forms that are just single-celled organisms.
There could be ones that are at least comparable to our technological level.
Or there could be ones that are post-human in some sense and almost unimaginable to us, right?
Do you personally have a target in mind when you think about aliens?
All of them.
I think all of them should be considered as part of the search.
Because the amazing thing now is we have the capacity to find all of them.
Right.
You know, when people, when we talk about aliens, exactly, there's this sense of like,
oh, unless it's an alien civilization, no one's interested, right?
If we found evidence of a microbial biosphere, it wouldn't be interesting.
And I reject that entirely, I think for, you know, deep philosophical, historical and scientific reasons,
the discovery of any kind of light, anywhere, would be, other than Earth, would be the greatest
scientific discovery in the history of humanity.
So the important thing is we have the capacity to find biospheres, which is the signatures of just microbial or forests or, you know,
things that don't build civilizations.
We have the capacity now through techno signatures to find technospheres, evidence of a technology,
of civilizations producing technology.
And then, you know, when we get to the truly high scales, yeah, those things should also be,
that's a little bit more in the realm of traditional setting.
But yeah, we have the capacity to find those as well.
So I think what really people need to understand is we didn't have these capacities like even 10 years ago.
And now suddenly the telescopes and the detectors have gotten to the point to be.
able to find these bio and techno signatures.
And NASA's all in.
The whole scientific community is all in, which was not true, again, even 10, 20, 30 years ago.
So, sorry, what about, say more about that transition about being all in that wasn't there 10 or 20 years ago.
Well, you know, I have a whole section in the book of our chapter in the book about the giggle factor, as we call it.
We in the business call it.
Because even when I was a graduate student, way back in the 80s and early 90s.
in the early 90s.
You know, SETI, there was only SETI,
like their astrobiology was not a thing.
The Viking landers had pretty much
kind of closed the door on life on Mars
because of those experiments that were done.
And there was only SETI,
and SETI was still kind of marginal.
It was very marginalized, right?
We had one professor at the University of Washington
where I was a PhD student,
who was into it, Woody Sullivan.
And he was the,
only one. And, you know, everybody loved Woody, but there was just this general sense,
because he was a great side. He was a radio scientist. But there was always this sort of sense
of, oh, that's marginal on, right? That's something that's not, you know, certainly don't do that
for your career, right? Don't make any choice. And that, I think, held for quite a while. And then
after 1995, we get the first discovery of exoplanets. We get that Martian meteorite, which
looked like it might have had evidence for life, didn't. But that launched like the new era of
astrobiology. And starting from that point, NASA starts putting money into astrobiology. By the first
decade of the new century, there are astrobiology centers. By the time you get to the, you know,
10 years ago, we now have a full census of exoplanets. We now that, know that every planet in the sky
has a family of worlds orbiting it. Every fifth star, sorry, every, I'm sorry, what I meant to say was
Every star in the night sky has a family of planets.
And every fifth star has a planet in the habitable zone, in the right place for life to form.
So, and most importantly, as I'm sure we'll talk more about, this process of atmospheric characterization,
where we figured out a way to look into the atmospheres of these worlds that are 40 light years away and detect their composition and therefore be able to find signatures of microbial life or, you know, signatures of.
of a biosphere or signatures of a technosphere.
That kind of that propelled everything.
That changed everything.
And now the, you know, last year, the astronomy or two years ago, the astronomy decadal
survey was announced where, you know, all of astronomers got together and decided what
the next big project should be.
And the, it's there in the name.
The next big telescope is going to be the habitable world's observatory.
So, you know, the giggle factor is over.
There's still some issues about techno signatures.
versus biosignatures, that's very much my thing right now.
But even that is we find we're overcoming that.
So the scientific community is all in on the search for cosmic life.
There's a weird analogy to the foundations of quantum mechanics in that in both cases,
it was something people talked about for decades.
There was giggles.
There were giggles about it.
It was kind of fringy.
But then what is changing is that technology is forcing us to confront some things.
And suddenly, oh, yeah, okay, now you're allowed to talk about it.
Yeah, I think that's a great analogy, right? Because it was quantum information science and the idea that, oh, quantum computers where you have to swallow the superposition's hole, that suddenly people were like, what's a superposition again? And so I think that's a really nice analogy. It was the technology, the ability to first detect exoplanets. That was a major revolution. And then now once we got really good with the transit method, which is where you find exoplanets by watching the star or the planet,
between you and the star.
And there's a few moments there, or maybe an hour,
where the light passes through the planet's atmosphere.
And you can look at the absorption spectra,
all the fingerprints that come from chemicals in the atmosphere hitting the light.
That's what did it.
And so now suddenly, and we're still on the hairy edge.
Like JWST is just at the edge.
We might, if we're lucky, be able to get a biosignature.
I mean, that would be amazing.
But it's going to be the next telescopes, the 30.
meter class telescopes and then the habitable world's observatory that's really going to put us in theirs.
My impression is that JWST wasn't actually conceptualized as something that was looking for
habitability of exoplanets. It was kind of designed to look at distant galaxies, but then it turns out to
be good for it. So it's kind of not surprising that if you purpose build a telescope, it would be
able to do a much better job. Yeah, that's it. And so it is actually lucky that the JWST has the right
bands, the spectral bands that is looking for, that actually are overlap with many of the
regions we think these bio and techno signatures may live in. So for example, there was just
this really interesting discovery a couple of about a month ago where this entirely new
class of habitable planet, which we call a hysean world, hydrogen ocean world, had its
atmosphere characterized in a way that actually indicated, yeah, this is.
So let me just explain.
A Hecenaean world is it's a sub-Neptune, so it's a planet that's maybe eight times the mass of the Earth pretty big.
And normally you'd think that would look like Neptune or Uranus, you know, which was a world that is maybe has a rocky core.
And then just slushes and ices and then hydrogen healing it.
Not a good place for life.
But they have figured out that there's this possibility of a world that has a pretty thick hydrogen atmosphere.
And hydrogen is a very good greenhouse gas.
So what you could have below it if you have enough water is a liquid ocean, a warm liquid ocean.
So this is, you know, this hydrogen ocean worlds.
And this is an, what's so exciting to me at least, this is an entirely new class of habitable world, right?
We always think, oh, you need an earth and it needs to be in the habitable zone, yada, yada.
And this is an entirely crazily different kind of world.
And the JWST was able to find methane in the atmosphere, characterized methane in the atmosphere,
at like the 5-sigma level, so very strong detection.
And then also CO2, I think at like the 3.5 signal levels.
So that really meant, and those levels were enough to say like, oh, yeah, this is what we
think if there's a liquid ocean down.
Like those levels were fit exactly what the models bring.
So there's an example of the JWST doing atmospheric characterization at a very high level
and getting us information, even if it didn't have an actual biosignature.
There were some, like there was a little indication of, what is it, dimethyl sulfide, which is what plankton fart into the atmosphere.
But that was, nobody really believed that for sure.
Even the authors were like, look, we're just saying we see a little wiggle there.
But it was showing that JWST is there for getting at least certain kinds of exoplanet information that we need.
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It's Cal Penn.
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And I really thought about it.
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I wouldn't get into the actual technological capabilities of us in detail later.
But first, I do want to lay the groundwork about this what we might be able to find in the sense that, like we said, there's primitive life, there's human comparable life, and there's way, way beyond human.
And I think that one thing that people don't seem to quite internalize in this discussion is the chances that any life we would find are at the human-compatible level are only,
almost nil in my view, just because it's very easy for a planet to have been evolving for either a billion more years than us or a billion less years than us.
Yeah. And actually, David Kipping and I and Caleb Sharp did a paper a few years back where David did all the Bayesian kung fu to show that, you know, we called it, I think, contact inequality.
That basically, if you detect somebody, odds are they're older than, you know, for a whole bunch of reasons.
and that was always one of the first places like,
okay, I really got to understand Bayesian statistics.
But it was a very nice paper,
and the result was pretty clear that, as you say,
it just sort of confirms an intuition that odds are
you're not going to find somebody at your level of technology.
You know, in order to, to, if you're going to find them,
they probably have to exist a long time.
Like if they only exist 200 years, good luck,
unless they're very copious, unless there's a lot of civilizations.
So in general, you're going to find somebody much older than you.
So, yeah, and right, we've only had techno signatures.
We've only been a technologically detectable civilization for, you know, a hundred years maybe.
So it's just unlikely that you're going to find someone at our level, which is what makes a lot of the UFO stuff kind of a little bit ridiculous.
Right.
Because this seems to be so close to our technologies.
Well, and if the civilizations don't just blow themselves up, which is certainly one of the options on the table, do we even have sensible?
notions of what they would be, what they would be like, or is that kind of just hopeless to speculate
about? No, actually, we're working on a paper on this right now. The whole idea, so, you know,
in the book I talk about this NASA grant we got. I'm the principal investigator on this.
The first grant NASA has ever given for atmospheric techno signatures. You know, as, you know,
I recount the history in the book because it's important of this, because I said, because of the
giggle factor, there was basically no funding for.
especially from NASA. And NASA tried a couple times to fund, you know, at a very low level, some SETI work.
And Congress, somebody in Congress, why, or three times, stood up and said, we're not going to waste money on these finding little green men and killed it.
So NASA, you know, is a government agency. And they learned like, we don't, we're not going here anymore.
And so it was literally in the call for proposals in these astrobiology programs to like, no, we don't want, they were like, we don't want SETI.
SETI. So when we finally managed to get this grant through, which was like not Radio SETI, but was using, you know, things like the JWST to find out in Spirit Technosignatures, that was a big deal. And one of the things we said was we are also, we're going to look, you know, we're going to make a library of possible techno signatures, but we're also going to try and push the field forward, right? And this has been a problem with SETI is that most of it is in the gray literature, right? There's or, you know, conference proceedings. There's, there's never been a continuous.
coherent, ongoing back and forth between the literature and then the next thing you want to do
because there was never a coherent community. It was just brave souls doing it on their own.
So to get back to your question, one of the things we're doing right now is to try and
systematize futures, right? We're actually taking methods from what's called future studies,
which has been applied to climate change and trying to apply these two techno signatures. What,
if anything can you say might be generic about the evolution of civilizations and it's been an
interesting project to because you've got to map out the spaces right you're never going to be able to
predict futures you're going to be able to predict like the fans of trajectories like the wide
range of trajectories and so i think if you focus on things like energy use you know trying to focus
on the physical aspects not the sociological aspects then you can sort of map out
questions like do they have interstellar travel do they have faster than light
travel, do they have, you know, and so you can at least begin to get a sense of what those,
what those parameters look like. And the nice thing, of course, because the second law of
thermodynamics is your friend, right? No matter what happens, I doubt the second law of thermodynamics
is going to be overcome. So therefore, that is going to leave imprints on your planet and on your,
solar system. So I think that's a very, using the second law of thermodynamics, which is what
the Dyson spheres are all about, is a good way of saying, of guiding your intuition about what
these civilizations and what the imprints will leave.
Let's not imagine that everyone here knows what a Dyson sphere is or the second law of thermodynamics.
So how do those things help us look for life elsewhere?
Yeah.
Okay.
So what is a civilization?
It's really just a mechanism for harvesting energy and putting it to work.
And, you know, like human beings 300,000 years ago, basically every day, every human being had one human
being's worth of power, right?
You know, there's horsepower and there's human beings.
But as we progressed working together,
we were slowly able to harvest more energy
so that right now, I had to do this calculation once,
each of us has the equivalent in our house,
just our house alone,
of about between 50 and 100 human beings at work for us,
just from the power coming through the outlet.
So the very famous second law of thermodynamics
tells us that if you want to use energy to do work,
you're going to create waste of some version.
You know, could be waste, could be just heat, you know, random motions of atoms.
But you can generalize that to mean, you're just going to create.
There's going to be noise.
There's going to be, you know, there's just going to be a consequence of trying to harvest that energy and use it for work.
So one of the, so this is a great thing to think about for alien civilizations because they,
civilizations are going to be harvesting energy.
It's the very definition in the definition.
So a long time ago, back in 1960, Freeman Dyson, very smart physicist,
realized that one way, one thing you can consider that might be universal in the trajectory
of civilizations would be to harvest as much energy as possible from your solar system,
and that means your star.
You would try and surround the entire star with solar collectors, get all that energy,
and do whatever you want to do with it, whatever you're interested in doing it.
So the idea was to build a Dyson sphere, a sphere around the star that had solar
collectors inside. Now he knew immediately that was on gravitationally unstable. So really these days
we think about Dyson swarms, you know, just these giant planet-sized machines that are solar
panels that are orbiting the star. Now, the thing about that is, is if you do that, you're collecting
energy, you're going to, some bike by the action of collecting and harvesting that energy, you are going
to create waste heat. You're going to warm up, basically. And you should be visible in the infrared.
The whole thing should be glowing, this giant machine should be glowing in the infrared.
And he proposed that in that paper, the first paper, he said, this is what you should look for.
And people have been doing that.
People have been, you know, there's been a few studies, Jason Wright in particular recently,
looking for Dyson's.
And you can extend this idea to almost anything.
One of the things that we've proposed is that in a civil planet that has civilization, you would see in the chemical networks in the atmospheres.
you'd see evidence of the non-equilibrium processes and their dissipation that are going on.
And you would be able to look for that in the atmosphere as an indication that there was something going on in that planet that was beyond just not having any life or beyond having just a biosphere.
There's a cascade upward in sense of how much dissipation happens because of your use of energy.
Okay, wait a minute. I want to get back to that.
But first, I need to harp on Dyson's thing because I don't believe it.
I don't think it's right.
I think it makes a pretty simple error.
As long as you have a source of energy that is hotter than your environment, then there's useful work you can extract from it.
So if you're at all a smart technological civilization, you should cascade the heat that you're emitting back out in the universe all the way down to the temperature of the microwave background.
So I don't think that Dyson spheres should be visible at all.
Well, so you want to have a cascade of machines, but each machine is going to have some level of dissipation that, I mean, I'm not sure that you can harvest all of the dissipated energy. I mean, I think at some point you're going to have, you're right? I mean, you're not going to be able to get away with this. I could figure it out.
I think, you know, it's interesting. I think I recall papers, I recall a paper I think that was discussing about these sort of cascades of machines. But ultimately, right, you can't harvest at all, right? I mean, some of it is going to have to be dissipation.
Yeah, you have to harvest, you can't lower your temperature below that of your environment.
Right, right, right.
Which I think is three degrees, Calvin.
Yeah, all right.
So that was one thing.
But now the, and I do want to get back to the super civilizations, but now you're, I want to hear more about this analogous thing, which I take it to be with just the existence of life, not necessarily with technology.
And I completely agree that, you know, primitive life obeys the second law and is not even very optimized.
to turn its energy into waste heat.
So what exactly is the signature that you're looking for?
The life, so everybody should take a deep breath, right?
All that oxygen in the atmosphere is a consequence of this invention about two and a half billion years ago of a new form of photosynthesis, right?
Which was completely changed the planet, right?
So photosynthesis was actually not a very efficient affair before this happened.
It required there to be, it was extracting iron ions.
That's what it used as a, you know, you get in a photon, you'd move some iron in the ocean around, you know, some molecules around ions.
And then you'd be able to make a sugar.
Once photosynthesis, once life figured out, oh, I can use water as the substrate.
right? That changed everything because water's everywhere. Now you're done with your rate limiting step.
And so you break apart water molecule, use the hydrogen as part of the molecular machinery to make the sugar and you burp out the oxygen.
So that was an enormous change in the planet's history, right? That the introduction of oxygen into the whole geosphere changed.
and it eventually put the oxygen into the atmosphere, the 21% that we have now.
And it's that continuous flux of oxygen into the atmosphere is a driver of non-equilibrium chemistry, right?
I mean, if that oxygen went away, for whatever reasons, very quickly, they don't know the exact time,
but certainly within a million years or so, all the oxygen gets bound up with rocks again,
and it's gone.
You're back to the previous nitrogen CO2 dominated.
So it's both, so the presence of certain chemicals, the flux of those chemicals, means that your atmospheric state is non-equilibrium.
It's life that's driving it in there.
And then even more to the point, this is some really fascinating work that's going on now.
People like Sarah Walker and others and Sarah Seeger, you know, have been trying this idea of looking for agnostic biosignatures, things that don't have anything to do what's happened on Earth.
And one of the interesting ways to do this is looking at the, again, the network property, right?
If you, of the, that you see in the chemical network and the atmosphere.
The network properties of who's reacting with whom in a system where life is pushing those chemicals into the atmosphere is going to look very different.
And they've shown, there's a great paper by Kim et al a few years ago, will look very different than a random network.
And so by looking at, you know, who's connected to who the, you know, the greenness, the greenness,
the degree centrality, all of these network topology characteristics,
you can really see differences between biology building the network
and just random or just pure geophysics.
Yeah, actually, I'm very sympathetic to that
because anyone, every time people talk about CO2 or methane or oxygen or whatever,
I'm like, okay, maybe here on Earth there was a certain way that was made,
but come on, these molecules are so simple that maybe there's a different chemical process going on.
we don't know about. But if you have like some very complex carbohydrates, hydrocarbon,
I just invented a new word, a carbohydrate. Hydrocarbons are things that life naturally makes
or even very, very complicated molecules at all. That sounds like a promising place to look.
But maybe those are harder to look for? I don't know. Well, they will require bigger telescopes
that have longer, you know, where we can, you know, the whole point of a big telescope is it's a light
bucket. The bigger your bucket, the more light you gather, the more light you gather, the faster
you can look for a spectral feature. So it is true that that, but again, we're just starting
down this road. So this idea of agnostic biosignatures is something that really only in the last
five, ten years, people have really begun and there's been funding for. And so network properties
of one of them looking at, again, this idea of dissipation trying to calculate the, you know,
how far away from you are, how far are you from the equilibrium state of the atmosphere?
You know, using that metric, the distance as a measure of how much life, you know, dumb life or smart life is pushing you away.
But I really love what is interesting, and we're working on this as well, the whole idea of information architecture, right?
Using information theoretic measures of how come.
This is what assembly theory is about.
That's one of the things why, you know, people, why those guys were interested in assembly theory.
But there's others of seeing like, just how, how do you make?
how complex this molecule is or atom is, and how much does that allow you to say,
okay, this could only be produced by life or this could only be produced by technology.
Right, which probably can only be produced by life.
Right, exactly.
So speaking of which, I mean, let's finish up the advanced civilization business.
There's an obvious problem working in the background here.
We've gone 25 minutes in the podcast without mentioning it.
But where are all these advanced civilizations?
Didn't Professor Fermi point out a paradox in this way of thinking?
Yes, the infamous Fermi paradox.
What I like about the Fermi paradox is that it's the first, you know, it was 1950, right?
And so in the book, you know, I sort of go through this history.
The decade of the 50s is amazing because you start with Fermi.
Then you have the Miller-Uray experiment, which was this first experiment that showed like,
it may not be that hard to get life started.
And then you end with Drake doing his first seti search.
So the Fermi paradox is the idea that look, if the stars, if intelligent life is common,
and if intelligent life can travel, figures out how to travel at even a tenth of the speed of light,
then basically the whole universe should be filled or the whole galaxy should be filled with intelligent life.
They should have been able to hop from one star system to the next and settled and built up, you know,
civilization and moved on to it.
So that is what we call the direct Fermi paradox.
Why aren't they here now?
So, of course, if you're into UFOs, the answer is clear.
They are here now.
But if you're not into UFOs, there is an entire sort of, you know, cottage industry of people coming up with answers to that.
Well, we're a zoo.
We're being held, you know, nobody's, they're not contacting us because they want to leave us alone and watch us.
But I actually think, and we did a whole series of papers on this, I think there's an easier answer.
to this, which is the debate about the Fermi paradox was how fast does that civilization front move, right?
You know, is does it take, in the original calculation that Hart did of the Fermi paradox,
1975, Hart showed it takes about 600,000 years if you're moving at like 0.1c, which is very short
compared to the age of the galaxy, hence the Fermi paradigm. And then Sagan and others said,
oh, no, no, it's going to stall out because of resource issues. We did a simulation. We did
we made a little galaxy turning around and we did a really nice simulation of Jonathan Carroll,
my postdoc, former postdoc, ran this.
And what we found is, yes, the front travels very fast.
You know, you colonize your galaxy very quickly.
But if you add the fact that civilizations don't last forever, right?
I mean, you know, civilizations die.
If you allow the civilizations to die, now you have to ask, what is the steady state occupation?
of the galaxy.
And what you find is you can end up with,
depending on the parameters of your space travel,
you can end up with pockets that are un-colonized
or settled for millions of years.
And those pockets, it's possible that we just live in one of those pockets.
And maybe we were visited a billion years ago,
and maybe there was a civilization that was set up for, you know, 10,000 years,
which is a lot longer than we've lasted.
But all evidence of that is gone.
the paper I did with Gavin Schmidt, the one on the Silorian hypothesis, where we showed that if there was a civilization here 100 million years ago, there's no way to know. There's no fossils. There's no. The only way you can find is to look at, look for isotopic anomalies. So in that sense, I'm not so bothered. I can't let you quite get away with that so quickly. I want to hear more about this. So if, I mean, how big of a civilization are you saying could have been here 100 million years ago, the size of our current civilization? Easily. Yeah, easily. We're not going to.
to leave. So the equivalent of Manhattan would just be erased from the earth in 100 million years.
It is ground down. Yeah. In that paper, as Gavin, you know, pointed out, that the Earth's surface
gets pretty well restructured, you know, after a few million years, certainly by 10 million years,
anything that was on the surface is gone, because a lot of the surface is gone, right? It's been
subducted and come back up. So there's not a whole lot of pristine, there's almost no pristine surface
from even, you know, 100 million years ago. So we're,
And then fossils.
Everyone's like, well, there'll be fossils.
The fossil record is so incomplete.
Very few things get fossilized.
So if you had a civilization that was worldwide and that lasted 10,000 years, that is still so short that nothing would be, you wouldn't find anything now, you know, 100 million years later.
So that's a pretty remarkable fact.
That's why we wrote that paper is just not that we were saying there was a civilization, but just like the interesting scientific question of like,
could you tell? And the answer is
probably not.
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So two things
come to mind immediately, but I can also
come up with objections to them. One is
that the chemical and atmospheric
signatures would have been pretty
enormous. And the other thing is wouldn't have had a big effect on, not by leaving fossils,
but by affecting other life forms, effects on the biosphere that would show up in the fossil record.
Yeah. Well, the first one, the atmospheric record, it's really where you're going to have to
look for the record for it. And this is what we did in the paper. It was in, I can never pronounce
this, stratigraphy, stratigraphy, in the strata. We're going to look for isotopic anomalies because
the temperature went up or the temperature went down or you know or plastics or and as we showed
you know 10,000 years is probably too short to really pick out that you need there are signals
there are definitely signals of interesting things happening but in they're very long you know
stretched across long times and in you can find better explanations like you know climate change
or you know a massive volcanic but also as we pointed out in the paper no one's ever
actually done the kind of high resolution
studies.
I just can't pronounce stratigraphygriography
of the kind
that you need. So that in that sense
that's where you're right. That's where
you'd have to look up to now
with what we have. You can't say there's
anything. But as we, that's the end
of the paper like hey, maybe people should look at this
more carefully. And your second point,
forgot what was your second point?
Causing mass extinctions or new
fauna to show up or something like that?
Yeah, that's an
interesting point. We did not consider that in the paper. My guess would be, but it's only a guess,
is that unless you lived for a very long time, you probably wouldn't be able to catch that level
of something so short. I'm not sure about that, though. I mean, we are right. People would say we're
driving a mass extinction. Will our mass extinction really show up or not? I don't know. So that's a
possibility, and we'd have to look to see if that were true. Okay, good. Here's my other crazy
possibility. So what if civilizations last a little bit longer?
than you assumed in your paper.
And so, but they're rare.
So it's not surprising that we don't have one here in the galaxy.
We haven't been taken over.
But 1% of the galaxies that we can see in the field have been taken over by advanced civilizations.
Is there any way we would know that and have we looked?
People, so that idea of galactic engineering comes from the idea of the Kardasheff scale,
which we can very quickly go over.
In this golden era of SETI, right after 1960,
Cardishchev was a Russian physicist who proposed that there were three levels of civilizations
as a good way of characterizing them based on their energy use.
Type 1 harvested all the energy falling on their planet.
Type 2 harvested all the energy coming from their star, a la a Dyson sphere.
And type 3 harvested all the energy of all the stars in their galaxy.
Maybe even moving the stars around to clump them.
together. Sure. So no one, I mean, people have not really looked for this. And the problem,
the reason why people have not really looked for this is that, again, there's never been any
money for this, right? You know, like you, you know, to do a search like this, you need telescope
time and you need graduate students. And there's been never any funding for this. So maybe here
and there people have like tried this or that, but never been a coherent study of this. And
hopefully now that things are changing, you'll, there will be the ability some funding to look for
those kinds of like really galactic engineering or even planetary engineer. Here's an interesting
exo or a tariff, sorry, techno signature that Jill Tarter came up with. If you found, if you looked
at a solar system and saw three planets or four planets that all had the exact same climate,
that would be a really good indication that those worlds, at least some of those worlds had been
terraform. That's a good one. Yeah. That's a real, I thought that was a really clever one. So, you know,
this idea of solar system scale engineering or galactic.
engineering, that's a great place. That's a really good place to look, which, you know, once we have
a true program in techno signatures, we can do that. But I think that the data has already
been collected for the galaxies. We have galaxy surveys with Spectra. I'll take us one grad student
to take this up as a project and scan through the data from, I don't know, Sloan or something
like that. Well, you have to know what, you'd have to figure out what exactly are you looking for.
I mean, because, you know, it's very, this is always the dilemma. How do you determine what's a natural
signal and what's not a natural signal. I mean, so what nobody has done right now is articulated
what explicitly would be the signature of that kind of engineering. So with the Dyson sphere,
we say like, oh, look, you need infrared. You need to have very bright infrared sources. And there's
been a couple of studies of those, but not much. So, you know, the first job is to figure out
what the techno or biosignature is and then go look for it. And, you know, you're not going to get
telescope time unless you, or even archival time.
time, right, to go look through all this unless you know what you're looking for.
Yeah, no, I do not agree. I think this is a very doable project. You got a million galaxy
spectra. You ask a machine learning model to say, is there some fraction of these that look
weird in a universally common way? And then you go back and look at those galaxies and ask
if there's anything weird looking about them. Well, you could do that. I mean, I'm not sure if
anybody has done, I mean, certainly people have done various kinds of anomaly searches for other
kinds of things. Like, for example, the moon, we have enough data about the moon to look for
anybody left something from a billion years ago. But again, like, you know, so people have done,
like, have done test projects with that. Like, you can find, you can give like 50 square miles
around the lunar lander and machine learning will find it immediately. Be like, that's different.
But I still think with the galaxies, it must be an interesting question to look at the
galaxy, you still got to figure out, you know, you know, just finding, you could, yeah, you can find
weird things and so you'd have a big giant box of weird things but you know
sorting out the weird from the alien weird is yeah you got in I think you're going to have
to know what you're looking for so I'd be interested to see if anybody's tried I'm sure
people have done this just for looking for quasars right looking for odd quasars or such but
but if you know if you haven't created that category is like no these are the things I want
you to have been because they might be aliens I don't know if anybody's ever done that
well I guess that's what they would do it is that is that what what
For all the things that AI and machine learning are overhyped about,
I think one of the things that they're pretty good at is, you know,
not making presumptions that humans make.
So if you just asked it, like, is there a systematic way that some fraction of galaxies are weird?
I'm not saying it's alien.
Like, maybe you make some other epochal astrophysical discovery, right?
But just ask it that.
And then if it says, yes, these 3% of galaxies are really weird,
then go back and look at them.
And then, you know, rather than presuming what the signature would be.
Yeah. I'd have to say, I mean, it feels like somebody, for reasons that have nothing to do with aliens, people must have done that, right?
Exactly. You know, it's interesting. One, when we, Tabi star or Bajoyan star, that star that people thought maybe we'd found a Dyson swarm around was sort of exactly that. There was a pipeline from the Kepler data that was, you know, identified transits automatically. And then it would spit out the ones that were like, I don't know what this is. This one doesn't make any sense to me. Right. And then there was a citizen.
science project that actually identified
Bejoian stars being like,
wow, these don't look anything like a planet.
And that is where, you know,
for, I mean, there were many possibilities.
Alien megastructures was at the bottom of the list.
But for a while, people were like, whoa, this is the kind of thing
we'd expect if it was alien.
So that was an example of doing exactly what you think.
There's a machine learning algorithm for these transits.
And then it spits out the ones that like,
this doesn't look like anything I understand.
But you know, one thing I want to emphasize is from my perspective,
I'm not a huge fan when it comes to techno signatures of like the galactic engineering or the because that assumes a level of technology and a level of organization and a level of cosmic coherence to a civilization that I'm not sure is possible because if the speed of light is really a boundary then you know it may be very hard to have galactic civilizations right if it takes unless you're very long lived right unless you're your species very long lived you should be you're you're you're
super technologically advanced.
Why should you have not conquered debt?
That's a whole other time.
Not sure about God.
I mean, right, this gets into us right.
Sure, or if they're machines, right?
If they are, you know, if they're fully silicon, right?
And I talk about that in the book.
That's a real.
How long is the biological era?
How long until we are replaced by our robot master?
But I still, you know, there's that, that running in that direction still makes less sense to me.
Then let's just look at the planets, right?
planets, you know, let's just, it's, let's just eavesdrop on the planets that we can,
because we couldn't do that before, right?
And we could just look at these planets and look to see whether, again, yeah, anomalies,
whether there's anything happening on the planets that is weird.
And we couldn't do that before.
So looking at that scale of galactic engineering, which is just, we just don't know,
whereas we at least have one example of a species of, you know, life forming on a planet,
that species becoming intelligent and changing the planet,
at least, you know, we have the existence proof for that one.
So that, and we couldn't do that before,
and so that's the one I'm most excited about.
So what are we doing to look for life elsewhere?
I mean, obviously we're probably doing something very different
to look for intelligent life than to look for microbial life,
but we have this image of Jody Foster sitting at a radio telescope wearing earphones.
Probably we have other techniques rather than that by now.
that's the main emphasis for me that I'm trying to get people to understand is that that is what I call classic seti and it's great idea but we've moved that now becomes just a subset of this much larger array of possibilities which was just never possible before one of the thing about the classic setty that Frank Drake did is you kind of needed a beacon you needed somebody sending a message at you focusing their their radio energy because if not if you were doing it you
into the all-sky, you'd need something that was so bright it was a star, right?
So that assumed there was this whole sort of assumption that like, yeah, they want to contact
you, they're interested in contact, whereas now what's possible with JWST, etc., is that I call
the metabolic techno signatures.
It's just the civilization or the biosphere just going about its business.
We don't have to really care whether they're trying to contact us.
They're just doing what they're doing.
And we're like detectives on a stakeout with our, you know, in our car,
with our cold cups of coffee and our crappy donuts.
And we're just watching the planet or the stellar system.
We're just looking for them going about their business.
And that wasn't possible before.
And now it is.
So when it comes to life, we can look for these biosignatures, things like oxygen or, you know,
the network properties of the chemicals that we talked about before.
When it comes to techno signatures, we can look for, we actually have the capacity.
We just wrote a paper on this.
We could find chlorofluorocarbons.
in a planet 40, at our level, at our level, Earth's level of chloroformicarbacarbons,
which are people don't know. That's the chemical we banned because it was destroying the ozone.
Yeah. But it's absolutely not natural. There's no way we know to produce CFCs naturally.
And we showed in a paper that the James Webb Space Telescope, with a couple of assumptions,
and about a few hundred hours of observing time, could detect chloroflorocarbons. At our level,
certainly at five or ten times our level
in a planet that was 40 light years away.
So we can detect atmospheric,
either pollutants, I'm putting that in quotes,
because you may put chloro-fluor carbons in your atmosphere on purpose.
If you want to terraform Mars,
CFCs are a great idea.
They're very good greenhound.
There's been a paper that's shown
you can detect city lights, artificial illumination.
There was a paper that showed you could look for
if you were deploying solar panels on a large scale.
There is an imprint in the reflected light,
the reflectivity changes.
We call that the ultraviolet edge.
And that would be detectable, just like plants, actually, there's a red edge,
the reflectance of Earth already.
You can see it.
All the plants, all the chlorophyll puts a reflectance edge in the red.
Sorry, sorry.
Say what is it doing?
They're absorbing red or they're reflecting red?
What exactly is that?
AR, it is a change in, because of what it's absorbing in, more in the blue green,
it adds a change in the reflectance of light at the red light.
So you see climb at the red.
Okay.
More red.
Gotcha.
Yeah.
Because you're absorbing the blue green.
So that is a, that's already.
We've shown that Earth has that.
Somebody from, you know, somebody looking at Earth.
Somebody looking at Earth for the last two billion years could tell Earth was an inhabited planet.
Right.
That's what's incredible.
So, yeah, all these things are now possible.
And that's really what the book is about in the next 10, 20, 30 years.
we're going to have data. I don't know what's going to say, but we're going to have data relevant to this, rather than yelling at each other about our opinions, man, which is pretty much with the last 2,500 years of it.
Hey, it's also what podcasts do. I don't want you to be badmouthing, yelling at each other's with our opinions. But so which of these are going on? Are these programs or are they just like individual investigators proposing to NASA to collect some data? No, it's all in. So NASA is funding astroids.
biology in a big way. And again, this, the decadal survey really shows, right? The decadal survey said,
look, the next $12 billion telescope you build is going to be about life. It's going to be
tuned to find life. And that is just the tip of the iceberg of showing that NASA is all in
in terms of its funding. There's a number of different programs that speak to habitability,
to biosignatures, to exobiology. Our grant is in the exobiology program. But there's lots and
lots of others that NASA
is funding. Everything from doing
developing more powerful methods of
atmosphere characterization
to studying the
cycles or the
evolution of atmospheres. That's another project
I'm involved in. Many
of the planets we're going to be looking at are going to be
close to their stars, what are called
M dwarf planets. These are
the planets we're going to look for are orbiting
the most abundant type of star
which is not the sun. The sun is not the
most abundant star. It's a
redder, smaller mass, star, and the habitable zone for those are very close to the star.
And it's possible that you just, you know, there's so much crap coming off to star because
of solar flares that maybe the atmospheres don't last. So, you know, you got no atmosphere
or no habitability. So that's a whole program. So NASA across a wide range of fronts is funding
astrobiology as one of its major programs now. It's one of their principal programs.
And there is this opposite thing we can try to do, which is to draw attention to ourselves, right?
To beam signals out to the world or to send probes out there with record players on them.
Are we still doing that? And is that a good idea?
I am not a fan of many of messaging estuary territorial intelligence. I have watched too much science fiction.
Exactly.
to think that's a good idea.
I just really,
the main problem with it
is that who gets to do it?
The idea that some astronomer
with access to a radio telescope
beams a powerful signal
to some distant star system
just seems like,
of course we should consider the possibility
that's a bad idea, right?
We may decide,
okay, we're wrong,
but you have to consider the possibility.
And so I think there really needs
to be some kind of international
body that debates this, makes it a public debate, and so we can decide whether we want to do this.
Hey, everyone, it's Cal Penn. I'm the host of Earsay, the Audible and I Heart Audio Book Club. This week on the podcast, I'm sitting down with Ray Porter, the narrator of Andy Weir's
audiobook Project Hail Mary, massive sci-fi adventure about survival and science. And what happens when you wake up alone, very far
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People will say like, oh my God, I cried at the end.
It's like, yeah, dude, me too.
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Yeah, I'm also of the opinion that maybe they would help us, maybe they would hurt us.
Let's see first if we can figure some stuff out for ourselves before we draw our attention
to this vastly more powerful intergalactic force that may be for good or for evil.
Okay. Well, how optimistic are you about this? I mean, it's certainly possible that the solution of the Fermi paradox is that life happens on one planet in 10 to the 100, and therefore it's just us. Do we have any way of competently estimating how likely we're going to succeed here?
The best we can do, I think, is the word. I'm going to quote my own work here. But Woody Sullivan and I, a bunch of years back, did this page?
where we said, look, there's the Drake equation, right? The Drake equation, the time-honored
equation, which allows you to, like, plug in values that you've made up and try and answer how many
civilizations there are in the galaxy. And Woody and I asked, look, we've got this exoplanet data.
What can we use it for, right? How can, it's got to tell us something about the question about
civilization. And so what we're able to do is, you know, it's always with science. It's the question
you can answer, not the question
you want to answer. Oh, yeah. And so
what we were able to do was we were able
to manipulate the Drake equation and
answer this question. How
bad does the
per planet odds
for forming
a civilization have to be
to make us the only ones
in the universe, right? The only time it's
ever happened to the observable universe. And that
answer turns out to be 10 to the minus
22, right? Now you can say, well, what does that mean? Like, we don't
have, you know, is 10 to the minus 22 big or is it small? And for this, then you look at the
literature, right? Because people have been trying to theoretically calculate or estimate in one
way or the other how, what the odds of what this per planet probability should be. And then
that's where you break up into pessimists and optimists. I talk about that in the book, right? And so
in general, the pessimists were like 10 to the minus 15, right? And even the most pessimistic of all pessimists.
which was this calculation that was done
and all suddenly my brain's going to go blank on the author
but where they said absolutely
and it was a really interesting calculation that they did
kind of based on the anthropic principle
but they said look
it's 10 to the minus 20
we get 10 to the minus 20
for the probability of forming a civilization per planet
and that's so small that
you know there can never be any civilizations around
our number was 10 to the
minus 22, which would mean that there's 100 civilizations before us. I mean, even if we can't
observe them, it means it's happened. So the only thing I think that's useful about what we did is it
we called it the pessimism line. It showed the difference between really what you mean by pessimism.
And 10 to the minus 22 is small enough because what it is means that there's been 10 to the 22
experiments, right? Every habitable zone planet is an experiment in life and civilizations.
And in order for us to be the only ones, it means every one of those experiments fail. And I think
then it sort of falls to the pessimist to say, well, what is it? It happened with us, but what
happened, why, what are the filters that keep it from happening anywhere else? So that's kind of my,
that's what I would say, where I'm at with that. So I completely understand where the number
10 minus 21 or 10 minus 22 comes from. That's the reciprocal of the number of planets that might
be profitable. So that, that's fine. But I've no idea of how people are estimating the probability
that a planet forms life in the first place. Forget about intelligent life.
for civilizations. Like, where are we getting that from? Well, some people do combinatorics. They say,
okay, how long do you have to wait for a DNA to, you know, form by bouncing around? Other people
looked at the number of species that formed and their durations. I think that's what went into the,
because he was actually asking about intelligence. Other people will use the kind of a Bayesian analysis
of when did life appear on Earth, which is pretty quickly, right? So, you know, with the planets
It's 4.5 billion years old. By 3.8 billion years, we've got the zircons. I love that.
The little zircons. Whatever that. That's such a great word. That indicate that there may have
already been life on Earth. So people have various methods. And of course, you're absolutely right.
If you're going to say it all seems like, you know, magic and smoke and mirrors, it is.
I mean, it's very hard to do this ab initio. But people have tried various ways. And so there is
a literature. There is a literature of people trying very clearly to do this. And one of our points in
this was that like even the most pessimistic of pessimists actually turns out to be an optimist
based on the number we got. That's just very surprising to me. Like no one has said maybe the
probability is 10 to the minus 40 of life forming. We seem to know so little about it. Yeah. There's only
one. And that was the combinatorics argument. But people, you know, the problem with that was it was
shown very quickly that you don't need to assemble DNA from scratch. So that argument was sort of
went by the wayside in people. Yeah. But the fact that,
Life started fairly early on Earth is essentially meaningless to me because you have to
conditionalize on the fact that life already exists.
We already know that.
So it's not telling me very much.
So I'm not saying that the number is small.
I'm just saying, is there any principled reason to estimate that number big or small?
I mean, how advanced are we in coming up with theories for how life formed?
Yeah.
There I would say we're still, I mean, especially in terms of being able to get a number.
that you'd like, I think we don't have it yet.
I mean, our pro, we've made enormous progress
in understanding the evolution of life
on Earth and the possible routes
for abiogenesis.
But still, being able to use that to get,
there's a huge literature on this of people arguing back and forth,
but I don't think there's anything of the kind
you want. And in some sense, that's why
all of these estimations, you know,
we just got to go look, you know? We just got to go look
and the beautiful thing is we find one
other example of
even microbial life.
And all bets are off, right?
What is your personal feeling about right here in the solar system?
Are you optimistic about finding something?
Yeah, I am.
I am.
Just because, God, I was just looking at this yesterday for this project we're involved in on looking at planetary,
the interaction between planetary interiors and their atmospheres.
And the moons, all those moons out there are like, there's so much water.
So we are seeing so many subsurface oceans on these moons.
So the moons around the gas giants and the ice giants were just formed with lots and lots of water.
And it turns out that they have significant oceans hiding beneath either layers of ice.
Like Europa has a, I think like a 10 mile or 6 mile thick layer of ice, which is sitting on top of a 60 mile deep ocean.
There's more water on the moon of Europa, which is about Earth the size of Earth's moon.
than on Earth, all of Earth's oceans.
And it is just one of a handful,
beyond the order of five, ten moons,
all of which out there,
all of which have significant subsurface oceans.
So I think there's a lot of possibilities out there.
And the next, you know,
if we manage to make it through everything we're going through right now,
the future, there's a lot of interesting possibilities
of what could be living,
what might have started in those oceans.
Is Europa your favorite target?
Europe is my favorite target,
because it's so cool. But I mean, that's probably just my bias because I'm old enough to remember
when Europa was discovered to be an ocean moon. Yeah. But Encelis, which is orbiting Saturn, is a really
interesting one because there you're getting the geysers. You're getting the water sprayed out into
space and you can fly things through that water. That's how we discovered the water was brine. Very
salty, very good for getting life started. So I love Europa because it's so cool, but I think probably
is, you know, once we start getting out into the outer solar system, we may find other ones that are better, the search.
How much credence should we put on truly wacky forms of life? Like, I'm sure you've read Dragon's Egg by Robert Forward, where there was life on the surface of a neutron star, or the black cloud by Hoyle, where it was some giant molecular cloud.
Like, how open-minded should we be about the forms life could take?
I'm not wild about those, especially, you know, in doing this work, I've had to look at a lot of the evolutionary biology literature.
You know, and one problem with the black cloud is how did it evolve?
Like, how did you get the processes of Darwinian evolution to work for these interstellar clouds?
So I tend to think, and it's maybe my bias, but I think it's much better, especially because we can now.
We don't need to think about, you know, new life on neutron stars.
We have finally the possibility of going out and looking for the kind of life we understand.
which is made out of molecular modules, right?
Our understanding of life is that it is principally driven by molecular shenanigans.
You know, you need these modules that can build bigger things, that can then take on different
purposes and that can hold energy, sorry, old information, have these gorgeous information
architectures associated.
And I just think that right now, because we can do it, that's where we should be spending
our time.
That's more likely.
And we finally can do it.
and there is a rich literature,
rich understanding of evolution
in a very generic sense
that we can apply.
Okay, but don't come to me
when the giant interstellar cloud
gets mad at us for not taking it seriously.
Dissing it, yeah.
It's wrath.
Okay.
All right, good.
So we've gone this long
without seriously confronting the whole UFO mess.
Every six months, there's a UFO report,
and I go on the internet and say,
yeah, it's not really UFO.
It's not aliens.
always get like, well, oh, but there's going to be a report coming out in the next six months that
will reveal everything and you will be ashamed. And so far, it has not happened to me. I mean,
I don't know what your experience here is. Pretty much the same thing. I wanted in the book to
cover UFOs. About a third of the book is about UFOs and UAPs because I wanted people to understand
how to separate the wheat from the chafe, right? So the history of UFOs is one of, you know, people
seeing things. I'll never tell somebody they didn't see something. I wasn't there, right? But science is
about public knowledge and science has very high standards of evidence for good reason. It's why the
cell phone works. It's why your knee replacement surgery doesn't kill you. And so a claim to that,
you know, that something is related to life somewhere else in the universe is a huge claim. And you're
going to have to do a lot better than fuzzy photographs and personal stories, no matter how
compelling those personal stories are. So as I always like to say, there is nothing right now
that would link any, there's no evidence that would link any UFO, UAP to the something
beyond Earth technology. We should do the search. I am all for, you know, the NASA panel. I think,
you know, people are so interested in this. I think we should do a full, open, transparent search,
and we'll see what happens.
And also, I'm glad the pilots have been able to come through.
You know, I've talked at length with Ryan Graves, the pilot for, you know, one of the Navy pilots.
And what I like about him, he's like very agnostic.
He's like, look, I saw this.
It was behaving in ways that no jet, I've been around a lot of jets, that no jet ever, you know, moved.
But, you know, I need you guys to tell me what it is.
He's not saying it's aliens.
And he recognizes the fact that just seeing something is not proof, right?
You need, and this I have, so I have a whole chapter where I go through like, what would you need?
Okay, if you really wanted to do a scientific search, what would you need?
You'd need to build your own instruments so you understand them.
You'd need a rational search strategy.
And then you'd need some way to harvest all this data and comb through it.
So as you said, the problem with UFOs and UAPs is that the history of it is full of conspiracy theories and oakses,
where everybody's always telling us next year, you know, where the data is going to be released.
It never happens.
And so people need to really understand.
They need to a healthy doth of skepticism.
As I'd like to say, you should think about UFOs and the claims made about them as if you had just got into Times Square and some guy says, hey, man, I've got a $100 Rolex.
Do you want to buy it?
Is it really a Rolex?
Probably not.
I've seen it with my own eyes.
And what would you say about the idea that from the aliens point of view, you know, talk to us about the plausibility?
of extraterrestrial advanced civilizations coming to visit us
and being susceptible to having fuzzy photographs of themselves taken
or crashing in Nevada.
Yeah, well, this is the real problem with it.
It's like, look, this is what I want people to understand
who are interested in UFOs.
Because, listen, people who really are interested in UFOs,
for whatever reason, I think, cool, look, I'm interested in aliens.
I love aliens, right?
But, you know, if you don't want to just believe,
if you want to know, then you've got a kind of a,
sink the science through, right?
You don't want to, you know, I can write a science fiction story.
You can write a science fiction story.
That's not what we're interested in.
So the idea, let's first of all take the whole idea that you saw lights in the sky, right?
Because apparently the aliens don't want to land on the White House lawn and be like,
yo, we're here.
So that means they're trying to hide.
And therefore, they suck at it.
Because, like, what?
You can't turn the lights off?
Like, you know, there's a, you know, there's a cloaking device.
that just doesn't seem to work.
Or they've got a bunch of, you know, 13-year-olds flying these things
who've stolen it from their parents.
So there's just that sort of coherent part of the argument.
It just doesn't make sense that they don't want to be revealed,
but they keep showing themselves.
And then there's the blurry photographs.
Photography has gotten obviously a lot better since 1947 with our first.
That's the first real UFO sighting that catches on.
And yet it's always blurry photographs.
It's always blurry photographs.
And remember the Chinese spy balloon, right?
Oh, yeah.
There was a picture, I think it's a selfie that the pilot,
you know, one of the U2 pilots is taking.
And he's holding the camera over his head and you can see his helmet.
And then you see the Chinese spy balloon and you can see the rivets on the solar panels
below the payload.
And it's like, come on, why aren't there thousands of pictures like this?
So there's just, and then there's the crashes, obviously the crashes,
like the thing's able to get through interstellar space.
and it crashes, you know, once it gets your,
because it got hit by lightning.
That was part of the story in the Roth.
I mean, they're sending us there at 1987 Dodge Omnis, right?
Yeah.
So it's just, I don't, again, I don't want to make fun of, you know, people.
But I just think you have to sort of like,
you have to ask for a coherent, consistent,
scientifically integrated story.
And these are the kind of things that tell you that this just doesn't make much sense.
I mean, that's a good line you're selling us, Adam,
but it's exactly what an agent of the deep.
state would be telling us if they wanted to hide the truth. So I have to maintain my skepticism so
far. Somebody said that to me on Twitter one time and I was like, well, if I am, where's the check
from the deep state? Because, you know, I got more Mets paraphernalia to buy. And then he said,
hey, everybody, you can see this is why this guy isn't trustworthy. And I said, you know what?
That's what my kid said when I hid their Halloween candy in 2002. This guy's not trustworthy.
But it does. I mean, maybe this is a good place to wrap up because it's,
It takes us back to the beginning where you mentioned the almost tension between the science
of this and the science fiction of it, right?
I mean, it goes in both ways.
There are enthusiasts who are very invested in the existence and discovery of alien life,
whether it's microbes or civilizations.
And then there's a reaction against that that maybe makes it hard to take it seriously.
How do we balance those two very natural human impulses?
Yeah, I think, you know, the whole point, this is the beauty of science, right?
Science teaches you how to change your mind, right?
I'm open.
I'm literally doing a calculation now with some friends where we're looking at how long would the lunar lander be visible.
How long on the moon before this process called gardening, which is micrometeorite's just eroding?
That's how the regal it ended up being such so fine.
Because look, I'm willing to consider that somebody came through a billion years ago and, you know, left their lunch pail.
or whatever, or a monolith, who knows.
So, you know, the, I'm willing to consider the possibility.
If the data for the UAPs, let's say we do a UAP study and we do see things making right-hand
turns at Mach 500, you know, if the data's good, I'll be like, okay, here we go, right?
So the beauty of science is it shows you how to change your mind with honor, right?
And I think that's what separates.
I've met a lot of people in the UFO community and UAP community.
and there are those who are totally abbat.
They're like, look, this is what I believe or I'm interested in, I think it could be.
But the data will, if the data shows me something different, that's where I'll go.
And what I found is there's also people not like this.
I was just on the Tamron Hall show and the whole thing was about UFOs.
And I would talk to some of the people behind the before we went on.
And some of them, I brought them and they were like, yeah, look, if the data goes that way.
And there was one person in particular unnamed who I said, well, listen, if we were able to show that those things,
those pictures you were showing are natural phenomena, what would you
do. And they were like, oh, no, no, no, I know that they were ill. Right? So it's like, okay, now it's a
religion, right? Right. Right. So the point about science fiction is important, though, because I still,
a lot of my ideas come from good science fiction, a lot of things I'm interested in to pursue.
Kim Stanley Robinson, there's a couple ideas he had that drove me to research projects.
So I think there's a very important interchange between science fiction and this field,
particularly when it comes to civilizations.
And it's that scientists are not the best
at asking some of the questions you need to,
especially about civilizations, right?
We're not trained in sociology or anthropology or there's a way in which you need
our imaginations to be lifted out of the kind of way we think of things.
Scientists think of things.
And so I've always wanted to have like a conference
where we asked some of the best science fiction writers.
We put a bunch of scientists posed questions to them
and have them tell us stories, you know, that are focused.
that we might be able to, might be able to drive us.
So I think there is a very important interchange between science fiction and this field
and thinking about aliens.
But the point is to not get lost, right?
Is to understand when something is just a science fiction story,
untethered to reality.
And when, when, because of course with science,
what we need is we need constrained imagination, right?
We have our imaginations, let our imaginations go,
but it's got to be constrained by the laws of physics and biology and evolution.
even if we're going to extrapolate.
So I think that's the balance we have to find.
Well, I do, I completely agree with you that the little nudge to the imagination that science fiction can give us is wonderfully valuable and we should cherish it.
At the same time, I worry a little bit.
You know, I just had Zach and Kelly Wienersmith on the show talking about the challenges we would face if we wanted to colonize Mars or the moon or something like that.
I'm thinking also of just how people think about the future of AI or interstellar travel.
And there's this idea that science fiction authors do the best they can, but they're telling stories.
And they can sometimes give us the wrong impression about how easy certain things are.
Right.
I mean, no one predicted the Internet very effectively.
They may have mentioned the possibility of computers and being connected, but no one, as far
as I know, a hundred years ago was correctly predicting what the world would look like now.
So on the one hand, I want to caution against taking science fiction too seriously, but on the other
hand, is there a way that scientists can loosen up a bit and put their brains to work
in thinking more carefully about the future? Because I feel like we're in this dichotomy between
either thinking in science fictiony terms or like scientists saying, if I can't build an experiment
that tests it in the next five years that I'm not interested.
Yeah, that's a great question.
I think there is that space.
And I think that's one of the things that makes techno signatures,
this field that I'm in so interesting.
And again, I want to recognize, like,
while biosignatures is a very well-established field in astrobiology,
techno-signatures is new.
I think there's like, R-Grant and one other.
Because NASA is still a little bit hesitant, like, you know,
aliens, alien civilizations, is that really, you know?
But so I think the really fascinating thing about technology,
Signatures is this attempt to systematize futures, right?
To ask, to use that constrained imagination, to really loosen up, to have some tools at our disposal, but also loosen up.
And that really requires discussions with it's got to be interdisciplinary.
Like the really exciting thing about techno signatures in SETI, you know, I don't really use the word SETI anymore because I think carries a different kind of connotation.
But is techno signatures is that you've got to talk to biologists.
You've got to talk to anthropologists.
You know, what is technology?
How do we even define technology?
One of the things, there is a, there was a document that was done called the indigenous critique of SETI.
And it was a bunch of indigenous scholars looking at the history of SETI and saying like,
here's a bunch of stuff you guys haven't thought of.
You know, because SETI was basically, was a, you know, it was a group of men, basically,
you know, all sort of coming from the similar background.
and they were doing great work, but of course they were limited, right?
If you're going to think about the wide possibility of civilizations,
probably having just one kind of human being from one socioeconomic group is probably not the best thing.
And so I really love, even though I didn't necessarily agree with everything in the indigenous critique,
I found it really opened my mind, right?
It allowed me to consider other things.
And that's kind of what we have to do.
It can't just be scientists in dialogue with or can't be just physicists and astronomers alone.
We've got to be in dialogue with other scientists.
the humanities and see how we can constrain, but still expand.
That's good.
And so I should just stop it there because that was such an eloquent statement, but I have one
more question for you.
It's a softball.
Don't worry.
Because I don't want people to, you know, we're talking about this pretty dispassionately,
but I think you're making the case pretty effectively that this is a prospect.
It might not happen within our lifetimes, but it could that we could actually detect, even
forgetting about civilizations.
We could detect life on another planet in a kind of somewhat realistic way.
And you said, you know, at the beginning that this would be a big deal.
Let's just sit and marinate in how big a deal it would be.
It would be a hugely big deal.
Yeah, yeah.
And I think it would be a hugely big deal for two reasons.
Let's take life, just like, you know, dumb life, if we even found microbes.
The amazing thing, look, we're both theoretical physicists, right?
And, you know, black holes are awesome, stars are awesome, comets are awesome.
But life is weird, right?
Life is a physical system that, you know, goes beyond itself.
It creates, it innovates.
It does stuff that no other system that we know of can do.
And as if we, as for right now, it seems like we're an accident.
As far as we know, we're an accident.
It's the only time it's happened in the entire universe, you know, which would be really weird.
So to find just one example that has happened somewhere else would sort of blow the doors off that.
And I think we'd recognize that this incredible creative capacity is something the universe does.
It didn't just happen here once by mistake.
It's part of the universe.
This creative, ongoing, you know, expansion of possibilities that is evolution is something that could be happening all over the universe.
And then who knows how far it goes, right?
You know, especially once you get to intelligence or you don't even need to have the kind of intelligence we have.
The idea of liquid brains.
Like, who knows what life, you know, how life engages with the rest of the physical world.
So that's number one.
We would become part of this community of life.
And that would reorder, I think, everything about the way we think of ourselves in the future.
Part two is if we found a civilization, it would tell us something very important.
We all know, well, not we all know, but the people who are paying attention as far as I'm concerned,
know that, like, we face a lot of challenges.
There's some existential challenges to human civilization.
not to human beings.
I don't think we're ever going to go extinct or not any time soon.
But like this global civilization we all depend on, from climate change to nuclear war to possibly maybe AI, you know, it's not clear we're going to be here in 200 years in this form.
And so finding one other example of a technological civilization would show like, okay, somebody made it, right?
It is possible to do this.
Because right now, we don't know whether or not sustainable long-term civilizations are even a thing the universe does, right?
Maybe like there are no sustainable long-term civilization.
So finding one would show us like, okay, somebody made it.
And that would be like an existence proof.
And I think it would give us hope.
So to close this up, I will say, when people say, oh, but it's not going to be that.
It's not going to matter that much.
It's you're going to find life 40 light years away.
Who cares?
And I like to bring up the Copernican revolution.
Right.
Because in 1400, everybody went to all the smart people went to bed going like, oh, look, you know, tomorrow the sun's going to rise over the horizon.
Because the earth's the center of the universe and the sun goes over.
around the earth. Two hundred years later, all educated people were like, oh, look, the horizon,
tomorrow morning, the horizon's going to roll down and the sun's going to appear to, and that simple
nothing changed, right? But that simple astronomical fact was implicated in the Renaissance,
was implicated in the Enlightenment, was even implicated in the Protestant Reformation, right? It
became a building block in this profound transformation and how human beings understood each other. And I
think the discovery of life, no matter what kind it is, will be the Copernican Revolution
times a thousand. It'll just rewire how we understand ourselves. That's a good science
fiction plot. We discovered the existence of intelligent life elsewhere. We don't even get to talk
to it, but it changes our civilization here in a dramatic way. Right. It leads to that,
along with maybe other things that are happening to us, because we are facing, like, we have a
problem with the biosphere. It's clear the biosphere is about to get rid of us, right? And so maybe
the discovery of life elsewhere sort of
we need this new understanding of our place
on the planet and maybe that would
be part of it, you know? Sometimes
shaking things up is a good thing. So Adam Frank,
thanks for your contributions to doing exactly that
and thanks for being on the Mindscape podcast. Thank you, Sean.
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