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Konstantin Batygin: Planet 9 and the Edge of Our Solar System | Lex Fridman Podcast #201


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The following is a conversation with Konstantin Batygin, Planetary Astrophysicist at Caltech,
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interested in, among other things, the search for the distant, the mysterious Planet 9,
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in the outer regions of our solar system. Quick mention of our sponsors, Squarespace,
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Literati, Onnit, and Ni. Check them out in the description to support the podcast.
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As a side note, let me say that our little sun is orbited by not just a few planets in the
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planetary region, but trillions of objects in the Kuiper Belt and the Oort Cloud that extends
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over three light years out. This to me is amazing, since Proxima Centauri, the closest star to our
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sun, is only 4.2 light years away, and all of it is mostly covered in darkness. When I get a chance
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to go out swimming in the ocean, far from the shore, I'm sometimes overcome by the terrifying
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and the exciting feeling of not knowing what's there in the deep darkness. That's how I feel
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about the edge of our solar system. One day, I hope humans will travel there, or at the very
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least, AI systems that carry the flame of human consciousness. This is the Lux Friedman podcast,
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and here's my conversation with Konstantin Batygin.
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What is Planet Nine? Planet Nine is an object that we believe lives in the solar system beyond
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the orbit of Neptune. It orbits the sun with a period of about 10,000 years, and is about five
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earth masses. So that's a hypothesized object. There's some evidence for this kind of object.
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There's a bunch of different explanations. Can you give an overview of the planets in our solar
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system? How many are there? What do we know and not know about them at a high level?
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All right. That sounds like a good plan. So look, the solar system basically is comprised of two
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parts, the inner and the outer solar system. The inner solar system has the planets Mercury, Venus,
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Earth, and Mars. Now, Mercury is about 40% of the orbital separation of where the Earth is.
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It's closer to the sun. Venus is about 70% than Mars is about 160% further away from the sun than
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is the Earth. These planets that we, one of them we occupy, are pretty small. They're
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to leading order, sort of heavily overgrown asteroids, if you will. This becomes evident
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when you move out further in the solar system and encounter Jupiter, which is 316 earth masses,
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right? 10 times the size. Saturn is another huge one, 90 earth masses at about 10 times
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the separation from the sun as is the Earth. And then you have Uranus and Neptune at 20 and 30,
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respectively. For a long time, that is where the kind of massive part of the solar system ended.
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But what we've learned in the last 30 years is that beyond Neptune, there's this expansive field
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of icy debris, a second icy asteroid belt in the solar system. A lot of people have heard
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of the asteroid belt, which lives between Mars and Jupiter, right? That's a pretty common thing
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that people like to imagine and draw on lunchboxes and stuff. But beyond Neptune, there's a much
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more massive and much more radially expansive field of debris. Pluto, by the way, it belongs to that
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second icy asteroid belt, which we call the Kuiper belt. It's just a big object within that
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population of bodies. Pluto, the planet. Pluto, the dwarf planet, the former planet, you know.
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Why is Pluto not a planet anymore? I mean, it's tiny. We used to...
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For size matters when it comes to planets. 100%. It's actually a fascinating story.
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When Pluto was discovered in 1930, the reason it was discovered in the first place is because
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astronomers at the time were looking for a seven Earth mass planet somewhere beyond Neptune.
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It was hypothesized that such an object exists. When they found something, they interpreted that
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as a seven Earth mass planet and immediately revised its mass downwards because they couldn't
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resolve the object with the telescope. It looked like just a point mass star rather than a physical
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disk. They said, well, maybe it's not seven. Maybe it's one. Then over the next 40 years,
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Pluto's mass kept getting revised downwards, downwards, downwards until it was realized
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that it's 500 times less massive than the Earth. Pluto's surface area is almost perfectly equal
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to the surface area of Russia, actually. Russia is big, but it's not a planet.
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Well, actually, we can touch more on that. That's another discussion. In some sense,
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earlier in the century, Pluto represented our ignorance about the edges of the solar system.
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Perhaps Planet Nine is the thing that represents our ignorance about now the modern
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set of ignorances about the edges of our solar system. That's a good way to put it.
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By the way, just imagining this belt of debris at the edge of our solar system is incredible.
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Can you talk about it a little bit? What is the Kuiper belt and what is the Oort cloud?
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Yeah. Okay. Look, the simple way to think about it is that if you imagine Neptune's orbit like
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a circle, maybe a factor of one and a half, 1.3 times bigger on a radius of 1.3 times bigger,
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you've got a whole collection of icy objects. Most of these objects are sort of the size of
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Austin, maybe a little bit smaller. If you then zoom out and explore the orbits of the most
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long period, the Kuiper belt object, these are the things that have the biggest orbits
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and take the longest time to go around the sun, then what you find is that beyond a critical
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orbit size, beyond a critical orbit period, which is about 4,000 years, you start to see
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weird structure. All the orbits sort of point into one direction. All the orbits are kind of
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tilted in the same way by about 20 degrees with respect to sun. This is particularly pronounced
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in orbits that are not heavily affected by Neptune. There you start to see this weird dichotomy
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where there are objects which are stable, which Neptune does not mess with gravitationally,
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and unstable objects. The unstable objects are basically all over the place because they're
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being kicked around by Neptune. The stable orbits show this remarkable pattern of clustering.
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We, back I guess five years ago, interpreted this pattern of clustering as a gravitational
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one way sign, the existence of a planet in a distant planet, something that is shepherding
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and confining these orbits together. Of course, you have to have some skepticism when you're
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talking about these things. You have to ask the question of, okay, how statistically significant
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is this clustering? There are many authors that have indeed called that into question. We have
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done our own analyses. Basically, just like with all statistics where there's multiple ways to
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do the exercise, you can either ask the question of, if I have a telescope that has surveyed this
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part of the sky, what are the chances that I would discover this clustering? That basically tells you
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that you have zero confidence. That does not give you a confident answer one way or another.
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Another way to do the statistics, which is what we prefer to do, is to say we have a whole night
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sky of discoveries in the Kuiper Belt. If we have some object over there, which has
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right ascension and declination, which is a way to say it's there on the sky, and it has
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some brightness, that means somebody looked over there and was able to discover an object
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of that brightness or brighter. Through that analysis, you can construct a whole map on the sky
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of where all of the surveys that have ever been done have collectively looked. If you do the
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exercise this way, the false alarm probability of the clustering on which the Planet 9 hypothesis
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is built is about 0.4%. Wow. Okay. So there's a million questions here. One, when you say bright
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objects, why are they bright? Are we talking about actual objects within the Kuiper Belt or the stuff
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we see through the Kuiper Belt? This is the actual stuff we see in the Kuiper Belt. The way you go
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about discovering Kuiper Belt objects is pretty easy. I mean, it's easy in theory, hard in practice.
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All you do is you take snapshots of the sky, choose that direction and take the high exposure
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snapshot, then you wait a night and you do it again, and then you wait another night and you
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do it again. Objects that are just random stars in the galaxy don't move on the sky,
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whereas objects in the solar system will slowly move. This is no different than if you're driving
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down the freeway, it looks like trees are going by you faster than the clouds. This is parallax.
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That's it. It's just they're reflecting light off of the sun and it's going back and hitting this.
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There's a little bit of a glimmer from the different objects that you can see
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based on the reflection from the sun. So there's actual light, but it's not darkness.
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That's right. These are just big icicles, basically, that are just reflecting sunlight
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back at you. It's then easy to understand why it's so hard to discover them because light has to
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travel to something like 40 times the distance between the earth and the sun and then get
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reflected back. Was it like an hour travel? Yeah, that's right. That's something like that,
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because the earth to the sun is eight minutes, I believe. Yeah, in that order of magnitude.
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So that's interesting. So you have to account for all of that, and then there's this huge amount of
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data pixels that are coming from the pictures, and you have to integrate all of that together
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to paint a high estimate of the different objects. Can you track them? Can you be like,
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that's Bob? Yes, exactly. In fact, one of them is named Joe Biden. This is not even a joke.
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Okay, is there a Trump one or no? No, actually, I don't know. I haven't checked for that, but
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the way it works is if you discover one, you right away get a license plate for it.
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Okay, so the first four numbers is the first year that this object has appeared in the data set,
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if you will. And then there's this code that follows it, which basically tells you where in
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the sky it is. So one of the really interesting Kuiper Belt objects, which is very much part of
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the Planet Nine story is called VP113, because Joe Biden was vice president at the time, got
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nicknamed Biden. VP113, got nicknamed Biden. Beautiful. What's the fingerprint for any particular
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object? Like how do you know it's the same one? Or you just kind of like, yeah, from night to night,
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you take a picture, how do you know it's the same object? Yeah, so the way you know is it appears
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in almost exactly the same part of the sky except for moves. And this is why actually you need at
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least three nights, because oftentimes asteroids, which are much closer to the earth, will appear
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to move only slightly, but then on the third night will move away. So the third night is really there
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to detect acceleration. Now, the thing that I didn't really realize until I started observing
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together with my partner in crime and all this, Mike Brown, is just the fact that for the first
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year when you make these detections, the only thing you really know with confidence is where
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it is on the night sky and how far away it is. Okay, that's it. You don't know anything about
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the orbit. Because over three days, the object just moves so little, right? That whole motion on
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the sky is entirely coming from motion of the earth, right? So the earth is kind of the car,
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the object is the tree, and you see it move. So then to get some confident information about
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what its orbit looks like, you have to come back a year later, and then measure it again.
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Oh, it just needs to do three nights and come back a year later and do another three nights.
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Yeah. So you get the velocity, the acceleration from the three nights, and then you have the
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maybe the additional information. Because an orbit is basically described by six
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parameters. So you at least need six independent points, but in reality, you need many more
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observations to really pin down the orbit well. And from that, you're able to construct for that
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one particular object, an orbit, and then there's, of course, like how many objects are there?
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There's like fourish thousand now. But in the future, that could be like millions?
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Oh, sure. Oh, sure. So in fact, these things are hard to predict, but there's a new observatory
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called the Vera Rubin Observatory, which is coming online maybe next year. I mean, with COVID,
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these things are a little bit more uncertain, but they've actually been making great progress
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with construction. And so that telescope is just going to scan the night sky every day
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automatically. And just it's such an efficient survey that it might increase the census of
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the distant Kuiper Belt, the things that I'm interested in by a factor of 100. I mean, that
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would be that would be really cool. And yeah, that's an incredible... I mean, they might just find
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Planet 9. I mean, that's almost like literally pictures, like visually. I mean, sure. Yeah.
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The first detection you make, all you know is where it is in the sky and how far away it is.
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If something is, you know, 500 times away from the sun, as far away from the sun as the earth,
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you know that's Planet 9. That's when the story concludes. And then you can study it.
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Now you can study it. Yeah. By the way, I'm going to use that as like, I don't know,
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a pickup line or a dating strategy, like see the person for three days and then don't see them
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at all and then see them again in a year to determine the orbit. And over time, you figure out
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if sort of from a cosmic perspective, this whole thing works out. Yeah. I have no dating
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advice to give. I was going to use this as a metaphor to somehow map it onto the human
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condition. Okay. You mentioned the Kuiper Belt. What's the orb cloud? If you look at the Neptune
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orbit as one, then the Kuiper Belt is like 1.3 out there. Yeah. And then we get farther and
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farther into the darkness. What? So, okay, you've got the main Kuiper Belt, which is about,
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say, 1.3, 1.5. Then you have something called the scattered disk, which is kind of an extension
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of the Kuiper Belt. It's a bunch of these long, very elliptical orbits that hug the orbit of Neptune
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but come out very far. So, that, the scattered disk with the current senses, like some of the
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longest orbits we know of, have a semi major axis, so half the orbit length, roughly speaking,
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of about 1,000, 1,000 times the distance between the Earth and the Sun. Wow. Now, if you keep moving
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out, okay, eventually, once you're at sort of 10,000 to 100,000, roughly, that's where the
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orb cloud is. Now, the orb cloud is a distinct population of icy bodies and is distinct from
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the Kuiper Belt. In fact, it's so expansive that it ends roughly halfway between us and the next
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star. Its edge is just dictated by, to what extent, does the solar gravity reach? Solar
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gravity reaches that far. Yeah. So, it has to, wow. Yeah. In fact, imagining this is a little bit
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overwhelming. So, there's a giant, like, vast, icy rock thingy. It's like a sphere. It's like,
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you know, it's almost spherical structure that encircles the Sun and all the long period comets
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come from the orb cloud. They come the way that they appear. I mean, for already, I don't know,
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hundreds of years, we've been detecting that occasionally, like, a comet will come in and
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it seemingly comes out of nowhere. Yeah. The reason these long period comets appear,
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they're on very, very long time scales, right? These orb cloud objects that are sitting, you know,
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30,000 times as far away from the Sun as is the Earth actually interact with the gravity of the
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galaxy that tied, effectively, the tide that the galaxy exerts upon them and their orbits
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slowly change in a long gate to the point where once they, their closest approach to the Sun,
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starts to reach a critical distance where ice starts to sublimate, then we discover them as
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comets because then ice comes off of them. They look beautiful on the night sky, etc. But they're
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all coming from, you know, really, really far away. So, are any of them coming our way from
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collisions? Like, how many collisions are there? Or is there a bunch of space for them to move
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around? Yeah, it's completely collisionless. Out there, the physical radii of objects are so small
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compared to the distance between them, right? It's just, it is truly a collisionless environment.
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I don't know. I think that probably in the age of the solar system,
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there have literally been zero collisions in the word cloud. Wow. When you, like, draw a picture
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of the solar system, everything's really close together. So, everything, I guess, here's spaced
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far apart. Do rogue planets like flying every once in a while and join? Not rogue planets,
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but rogue objects from out there. Oh, sure. Oh, sure. Yeah. Join the party? Yeah, absolutely.
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We've seen a couple of them in the last three or so years, maybe four years now. One, the first one
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was the one called Ua Moa Moa. It's been all over the news. The second one was Comet Borisov,
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discovered by a guy named Borisov. Yeah, so the way you know they're coming from elsewhere is,
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unlike solar system objects, which travel on elliptical paths around the sun, these guys travel
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on hyperbolic paths. So, they come in, say hello, and then they're gone. And the fact that they
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exist is totally, like, not surprising, right? The Neptune is constantly ejecting
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Kuiper belt objects into interstellar space. Our solar system itself is sort of leaking icy debris
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and ejecting it. So, presumably, every planetary systems around other stars do exactly the same
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thing. Let me ask you about the millions of objects that are part of the Kuiper belt and
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the part of the ORE cloud. Do you think some of them have primitive life? It kind of makes you sad
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if there's a primitive life there and they're just kind of like lonely out there in space.
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How many of them do you think have life, like bacterial life? Probably an negligible amount.
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Zero, you know, like zero with like a plus on top, right? Zero plus plus. Yeah.
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So, you know, if you and I took a little trip to the interstellar medium, I think we would develop
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cancer and die real fast, right? It's rough. Yeah, it's a pretty hostile radiation environment.
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You don't actually have to go to the interstellar medium. You just have to leave the Earth's
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magnetic field too, and then you're not doing so well suddenly. So, you know, this idea of,
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you know, life kind of traveling between places, it's not entirely implausible, but you really
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have to twist, I think, a lot of parameters. One of the problems we have is we don't actually
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know how life originates, right? So, it's kind of a second order question of survival in the
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interstellar medium and how resilient it is because we think you require water,
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but, and that's certainly the case for the Earth, but, you know, we really don't know for sure.
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That said, I will argue that the question of like, are there aliens out there is a very
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boring question because the answer is, of course, there are. I mean, like, we know that
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there are planets around almost every star. Of course, there are other life forms. Life is
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not some specific thing that happened on the Earth, and that's it, right? That's a statistical
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impossibility. Yeah, but the difficult question is, before even the fact that we don't know how
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life originates, I don't think we even know what life is, like, definitionally. Like,
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formalizing a kind of picture of, in terms of the mechanism we would use to search for life out
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there, or even when we're on a planet to say, is this life? Is this rock that just moved from
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where it was yesterday, life, or maybe not even rock, something else? I got to tell you, I want
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to know what life is, okay, and I want you to show me. I think there's a song to basically accompany
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every single thing we talk about today, and probably half of them are love songs, and somehow
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we'll integrate George Michael into the whole thing. Okay, so your intuition is there's life
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everywhere in our universe. Do you think there's intelligent life out there?
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I think it's entirely plausible. I mean, it's entirely plausible. I think there's intelligent
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life on Earth. So yeah, taking that, like, say, whatever this thing we got on Earth,
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whether it's dolphins or humans, say that's intelligent. Definitely dolphins. I mean,
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have you seen the dolphins? Well, they do some cruel stuff to each other. So if cruelty
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is a definition of intelligence, they're pretty good. And then humans are pretty good on that
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regard. And then there's like, pigs are very intelligent. I got actually a chance to hang
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out with pigs recently. And they're, aside from the fact they were trying to eat me,
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they're very, they love food. They love food, but there's an intelligence to their eyes that was
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kind of like haunts me, because I also love to eat meat. And then to meet the thing, I later ate.
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And that was very intelligent, and almost charismatic with the way it was expressing
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it himself, herself, itself, was quite incredible. So all that to say is, if we have intelligent life
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here on Earth, if we take dolphins, pigs, humans, from the perspective of like planetary science,
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how unique is Earth? Okay, so Earth is not a common outcome of the planet formation process.
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It's probably a something on the order of maybe a 1% effect. And by Earth, I mean,
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not just an Earth mass planet, okay? I mean, the architecture of the solar system
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that allows the Earth to exist in its kind of very temperate way.
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One thing to understand, and this is, this is pretty crucial, right, is that the Earth itself
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formed well after the gas disk that formed the giant planets had already dissipated.
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You see, stars start out with, you know, the star and then a disk of gas and dust that encircles it,
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okay? From this disk of gas and dust, big planets can emerge. And we have over the last two,
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three decades discovered thousands of extra solar planets as an orbit of other stars.
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00:26:43.680
What we see is that many of them are, you know, have these expansive hydrogen helium atmospheres.
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The fact that the Earth doesn't is deeply connected to the fact that Earth took about 100
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million years to form. So we missed that, you know, train, so to speak, to get that hydrogen
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helium atmosphere. That's why, actually, we can see the sky, right? That's why the sky is,
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well, at least in most places, that's why the atmosphere is not completely opaque.
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With that, you know, kind of thinking in mind, I would argue that we're getting the kind of
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emergent pictures that the Earth is, is not, you know, everywhere, right? We, there's sort of the
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sci fi view of things where we go to some other star and we just land on random planets and they're
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all Earth like, that's totally not true. But the even a low probability event, even if you're
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imagine that Earth is a 1 in a million or 1 in a, you know, 1 in 10 million occurrence, there are
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10 to the 12 stars in the galaxy, right? So you just, you always win by, by large numbers.
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That's right, by supply.
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00:27:58.080
They save you. Well, do you've hypothesized that our solar system wants to possess the
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population of short period planets that were destroyed?
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Our solar system wants to possess the population of short period planets that were destroyed by the
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evil Jupiter migrating through the solar nebula. Can you explain?
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If I was to say, what was the kind of, the key outcome of searches for extra solar planets,
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it is that most stars are encircled by short period planets that are, you know, a few
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Earth masses, right? So a few times bigger than the Earth and have orbital periods that kind of
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range from days to weeks.
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00:28:42.000
Now, if you go and ask the solar system, what's in our region, right? In that region,
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00:28:48.400
it's completely empty, right? It's just, it's astonishingly hollow. And I think, you know,
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from the sun is not some special star that decided that it was going to form the solar system.
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So I think, you know, the natural thing to assume is that the same processes of planet
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formation that occurred everywhere else also occurred in the solar system.
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Following this logic, it's not implausible to imagine that the solar system once possessed
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a system of intramercurian, like, you know, compact system of planets. So then we asked ourselves,
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would such a system survive to this day? And the answer is no. At least our calculations
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suggest it's highly unlikely because of the formation of Jupiter. And Jupiter's primordial
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kind of wandering through the solar system would have sent this collisional field of debris that
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would have pushed that system of planets onto the sun.
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00:29:50.880
So was Jupiter, this primordial wandering, what did Jupiter look like? Like, why was it wandering?
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00:29:57.200
It didn't have the orbit it has today?
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00:29:59.920
We're pretty certain that giant planets like Jupiter, when they form, they migrate. The reason
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00:30:04.720
they migrate is, you know, on a detailed level, perhaps difficult to explain, but, you know,
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it's just in a qualitative sense that they form in this fluid disk of gas and dust. So it's kind
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of like, okay, if I plop down a raft somewhere in the ocean, will it stay where you plop it down?
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Or will it kind of get carried around? It's not really a good analogy because it's not like
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Jupiter is being advected by the currents of, you know, gas and dust. But the way it migrates is
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it carves out a hole in the disk and then through by interacting with the disk gravitationally,
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right? It can change its orbit. The fact that the solar system has both Jupiter and Saturn,
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here complicates things a lot, right? Because you have to solve the problem of the evolution of
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the gas disk, the evolution of Jupiter's orbit in the gas disk, plus evolution of Saturn's and
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00:31:05.360
their mutual interaction. The common outcome of solving that problem, though, is pretty easy to
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00:31:14.720
explain. Jupiter forms its orbit shrinks, and then once Saturn forms, its orbit catches up
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00:31:21.600
basically to the orbit of Jupiter, and then both come out. So there's this inward outward pattern
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00:31:26.640
of Jupiter's early motion that happens sort of within the last million years of the lifetime
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00:31:34.080
of the solar system's primordial disk. So while this is happening, if our calculations are correct,
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which I think they are, you can destroy this inner system of few earth mass planets.
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00:31:51.680
And then in the aftermath of all this violence, you form the terrestrial planets.
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00:31:58.480
Where would they come from in that case? So Jupiter clears out the space,
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00:32:02.000
and then there's a few terrestrial planets that come in, and those come in from the
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00:32:08.960
disk somewhere, like one of the larger objects. Yeah, what actually happens in these calculations
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00:32:13.840
is you leave behind a rather mass depleted, like, remnant disk, only a couple earth masses.
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00:32:22.640
Yeah. So then from that remnant population, annulus of material over 100 million years,
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by just collisions, you grow the earth and the moon and everything else.
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00:32:37.040
You said annulus?
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Annulus.
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00:32:38.960
Annulus.
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00:32:39.680
Annulus, yeah.
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00:32:40.480
That's a beautiful word, what does that mean?
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00:32:42.160
Well, it's like a disk that's kind of thin.
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00:32:44.960
It's like a, yeah, it's something that is, you know, a disk that's so thin it's almost
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flirting with being a ring.
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00:32:52.960
Like, I was going to say this reminds me of Lord of the Rings.
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So like this, the word just feels like it belongs in a token level.
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00:32:59.520
Yeah.
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00:32:59.520
Okay. So that's incredible. And so that, in your sense, as you said, like 1%, that's a rare.
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00:33:06.400
The way Jupiter and Saturn danced and cleared out and, you know, cleared out the short period
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00:33:15.920
debris and then changed the gravitational landscape, that's a pretty rare thing to...
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00:33:20.080
It's rare and moreover, like, you don't even have to go to our calculations.
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00:33:24.640
You can just ask the night sky, how many stars have Jupiter and Saturn analogs?
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00:33:30.960
And the answer is Jupiter and Saturn analogs are found around only 10% of sunlight stars.
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00:33:36.240
So they are, they themselves, like you kind of have to score an A minus or better on the test to,
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00:33:41.600
you know, on the planet formation test to become a solar system analog, even in that basic sense.
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00:33:47.920
And moreover, you know, lower mass stars, which are very numerous in the galaxy,
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00:33:55.600
so called M dwarves, think like 0% of them, well, maybe like some negligible fraction
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00:34:02.400
of them have giant planets. Giant planets are a rare, you know, outcome of planet formation.
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00:34:10.320
One of the really big problems that remain unanswered is why.
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00:34:14.160
We don't actually understand why they're so rare. How hard is it to simulate
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00:34:20.400
all of the things they've been talking about, each of the things we've been talking about,
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00:34:23.840
and maybe one day, all of the things we've been talking about and beyond? Meaning,
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00:34:29.440
like from the initial primordial solar system, you know, a bunch of disks with,
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00:34:36.640
I don't know, billions, trillions of objects in them, like simulate that such that you eventually
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00:34:42.480
get a Jupiter and a Saturn, and then eventually you get the Jupiter and the Saturn that clear
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00:34:47.760
out a disk, change the gravitational landscape, then Earth pops up, like that whole thing,
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00:34:52.080
and then be able to do that for every other system in the, every other star in the galaxy,
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00:35:00.080
and then be able to do that for other galaxies as well.
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00:35:06.000
Yeah, so maybe start from the smallest simulation, like what is actually being done today?
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00:35:11.200
I mean, even the smallest simulation is probably super, super difficult. Even just like one object
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00:35:15.520
in the Kuiper ball is probably super difficult to simulate.
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00:35:18.160
I mean, I think it's super easy. I mean, like, it's just not that hard. But, you know, let's,
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00:35:25.920
let's ask the most kind of basic problem. Okay, so the problem of having a star and
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00:35:33.120
something in orbit of it, that you don't need a simulation for, like, you can just write that
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00:35:37.440
down on a piece of paper. This gravity would like, yeah, I guess, I guess it's important to try to,
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00:35:44.960
you know, one way to simulate objects in our solar system is to build the universe from scratch.
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00:35:50.400
Okay, we'll get to building the universe from scratch in a sec. But let me just kind of go
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00:35:55.200
through the hierarchy of what, you know, what we do. Two objects. Two objects, analytically
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00:36:01.120
solvable, like, we can figure it out very easily. If you just, you don't even, I don't think you,
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00:36:06.480
yeah, you don't need to know calculus. It helps to know calculus, but you don't necessarily need
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00:36:11.120
to know calculus. Three objects that are gravitationally interacting, the solution is chaotic.
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00:36:18.480
Doesn't matter how many simulations you do, you, the answer loses meaning after, after some time.
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00:36:25.200
I feel like that is a metaphor for dating as well, but gone.
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00:36:28.000
Now look, yeah, so, so the fact that you go from analytically solvable to unpredictable,
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00:36:38.880
you know, when you were, you know, when your simulation goes from two bodies to three bodies,
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00:36:44.560
should immediately tell you that the exercise of trying to engineer a calculation where you form
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00:36:52.160
this whole entire solar system from scratch and hope to have some predictive answer is, is a futile
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00:36:58.800
one, right? We will never succeed at such a simulation. I just to clarify, you mean like
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00:37:05.040
explicitly having a clear equation that generalizes the whole process enough to be able to make a
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00:37:11.520
prediction? Or do you mean actually like literally simulating the objects as a hopeless pursuit
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00:37:16.880
once it increases beyond three? The simulating them is not a hopeless pursuit, but the outcome
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00:37:22.480
becomes a statistical one. What's actually quite interesting is I think we have all the equations
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00:37:32.000
figured out, right? Like, you know, in order to really understand this, the formation of the
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00:37:38.240
solar system is suffices to know gravity and magnetohydrodynamics. I mean, like the combination of
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00:37:46.640
Maxwell's equations and, you know, Navier Stokes equations for the fluids, you need to know
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00:37:50.960
quantum mechanics to understand the opacities and so on. But we have those equations in hand.
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00:37:58.960
It's not that we don't have that understanding. It's that putting it all together
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00:38:02.800
is A, very, very difficult, and B, if you were to run the same evolution twice, changing, you know,
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00:38:13.360
the initial conditions by some infinitesimal amount, some, you know, minor change in your
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00:38:19.120
calculation to start with, you would get a different answer. This is one, this is part
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00:38:26.000
of the reason why planetary systems are so diverse. You don't have like a, you know, very predictive
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00:38:32.880
path for you start with a disk of this mass and it's around this star. Therefore, you're going
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00:38:39.920
to form the solar system, right? You start with this and therefore you will form this huge outcome,
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00:38:46.000
huge set of outcomes, and some percentage of it will resemble the solar system.
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00:38:50.720
You mentioned quantum mechanics and we're talking about cosmic scale objects. You've talked about
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00:38:58.480
that the evolution of astrophysical disks can be modeled with Schrodinger's equation.
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00:39:03.600
I sure did. Why? It's like, how does quantum mechanics become relevant when you consider
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00:39:13.040
the evolution of objects in the solar system? Yeah. Well, let me take a, take a step back and
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00:39:18.000
just say it like, I remember being, you know, utterly confused by quantum mechanics when I
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00:39:25.200
first learned it. And the Schrodinger equation, which is kind of the parent equation of, of
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00:39:31.200
that whole field, you know, seems to come out of nowhere, right? The way that, the way that I was
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00:39:37.520
sort of explaining, I remember asking, you know, my professor is like, but where does it come from?
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00:39:42.640
He's like, well, it's just like, don't worry about it. And just like calculate the hydrogen,
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00:39:48.400
you know, energy levels, right? So it's like, I could do all the problems. I just
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00:39:52.800
did not have any intuition for, for where this parent, you know, super important equation came
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00:39:58.960
from. Now, down the line, I was, remember, I was preparing for my own lecture and I was trying to
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00:40:04.400
understand how waves travel in self gravitating disks. So, you know, again, there's a very broad
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00:40:15.120
theory that's already developed, but I was looking for some simpler way to explain it really
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00:40:20.400
for the purposes of teaching class. And so I thought, okay, what if I just imagine a disk as an
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00:40:27.200
infinite number of concentric circles, right, that interact with, with each other gravitationally?
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00:40:36.080
That's a problem in some sense that I can solve using methods from like this late 1700s, right?
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00:40:44.480
I can write down Hamiltonian, well, I can write down the energy function basically of their,
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00:40:49.760
their interactions. And what I found is that when you take the continuum limit,
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00:40:57.440
when you go from discrete circles that are talking to each other gravitationally to a
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00:41:02.880
continuum disk, suddenly this gravitational interaction among them, right? The, the governing
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00:41:11.120
equation becomes the Schrodinger equation. I had to think about that for a little bit.
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00:41:15.680
Did you just unify quantum mechanics and gravity? No, this is not the same thing as like, you know,
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00:41:22.480
fusing relativity and quantum mechanics. But it did, it did get me thinking a little bit.
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00:41:29.280
So the fact that waves in astrophysical disks behave just like wave functions of, of particles,
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00:41:37.840
kind of like an interesting analogy, because for me, it's easier to imagine waves traveling through,
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00:41:44.080
you know, astrophysical disks or really just sheets of paper. And the reason this is that
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00:41:51.840
analogy exists is because there's actually nothing quantum about the Schrodinger equation.
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00:41:57.040
The Schrodinger equation is just a wave equation. And all of the interpretation that comes from it
link |
00:42:05.040
is quantum, but the equation itself is not a quantum being.
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00:42:11.120
So you can use it to model waves. It's not turtles, it's waves all the way down. You
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00:42:16.080
could pick which level you picked the wave at. And so it could be at the solar system level
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00:42:20.640
that you can use it. Right. And also it actually provides a pretty neat calculational tool because
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00:42:27.760
it's difficult. So we just talked about simulations, but it's difficult to simulate
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00:42:32.160
the behavior of astrophysical disks on time scales that are in between a few orbits and
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00:42:40.480
their entire evolution. So it's over a time scale of a few orbits. You have, you do a hydrodynamic
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00:42:47.280
simulation, right? You do that. Basically, that's something that you can do on a modern computer,
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00:42:54.320
on a time scale of say a week. When it comes to their evolution over their entire lifetime,
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00:42:59.920
you don't hope to resolve the orbits. You just kind of hope to understand how the system behaves
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00:43:04.320
overall. In between, right, to get access to that, as it turns out, it's pretty, it's pretty cute.
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00:43:11.360
You can use a Schrodinger equation to get the answer rapidly. So it's a calculational tool.
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00:43:17.280
That's fascinating. By the way, astrophysical disks, how, what are they, how broad is this
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00:43:22.960
definition? Okay. So astrophysical disks span a huge, huge amount of ranges. They start maybe
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00:43:31.920
at the smallest scale. They start with actually Kuiper Belt objects. Some Kuiper Belt objects
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00:43:36.800
have rings. So that's maybe the smallest example of an astrophysical disk. We've got this little
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00:43:43.440
potato shaped asteroid, you know, which is, you know, sort of the size of LA or something. And
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00:43:49.200
around it is, are some rings of icy matter. That object is a small astrophysical disk. Then you
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00:43:57.120
have Saturn, the rings of Saturn. You have the next set of scale. You have the solar system
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00:44:02.320
itself when it was forming. You have a disk. Then you have black hole disks. You have galaxies.
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00:44:09.440
Discs are super common in the universe. The reason is that stuff rotates, right? I mean,
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00:44:15.760
gravity works. Yeah. So, and those rings could be the material that composes those rings could be,
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00:44:23.920
it could be gas, it could be solid, it could be anything. That's right. So the disk that made
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00:44:31.680
from which the planets emerged was predominantly hydrogen and helium gas. On the other hand,
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00:44:36.560
the rings of Saturn are made up of, you know, icicle, ice, little like
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00:44:42.960
ice cubes this big, about a centimeter across. That sounds refreshing. So that's incredible.
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00:44:49.120
Hydrogen and helium gas. So in the beginning, it was just hydrogen and helium around the sun.
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00:44:55.760
How does that lead to the first formations of solid objects in terms of simulation?
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00:45:01.760
Okay. Here's the story. So you're like, have you ever been to the desert?
link |
00:45:07.680
Yes. I've been to the Death Valley and actually it was terrifying just as a total tangent,
link |
00:45:12.080
I'm distracting you. But I was driving through it and I was really surprised because it was
link |
00:45:17.600
at first hot. And then as it was getting into the evening, there's this huge thunderstorm,
link |
00:45:23.200
like it was raining and it got freezing cold. I was like, what the hell? It was the apocalypse.
link |
00:45:28.160
Yes. I feel like just sit there listening to Bruce Springsteen, I remember, and just thinking,
link |
00:45:33.280
I'm probably going to die. And I was okay with it because Bruce Springsteen was on the radio.
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00:45:37.600
Look, when you've got the boss, you know, you're ready to meet the boss. Yeah. So look, I mean,
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00:45:43.920
it's a good line. It's true. Yeah. By the way, to continue on this tangent,
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00:45:50.640
I absolutely love the Southwest for this reason. During the pandemic, I drove from LA to New Mexico
link |
00:46:01.280
a bunch of times. The madness of weather. Yeah. The chaos of weather, the fact that it will be
link |
00:46:07.680
blazing hot one minute and then it's just like, we'll decide to have a little thunderstorm,
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00:46:13.120
maybe we'll decide to go back momentarily to like a thousand degrees and then go back to the
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00:46:17.920
thunderstorm. It's amazing. That, by the way, is chaos theory in action, right? But let's get back
link |
00:46:25.360
to talking about the desert. So in the desert, tumbleweeds have a tendency to roll because the
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00:46:31.760
wind rolls them. And if you're careful, you'll occasionally see this family of tumbleweeds where
link |
00:46:38.160
like there's like a big one and then a bunch of little ones that kind of hide in its wake, right?
link |
00:46:44.480
And they're all rolling together and almost look like, you know, a family of ducks crossing a street
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00:46:49.440
or something. Or for example, you know, if you watch Tour de France, right, you've got a whole
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00:46:56.720
bunch of cyclists and they're like cycling, you know, within 10 centimeters of each other. They're
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00:47:01.840
not BFFs, right? They're not trying to ride together. They are riding together to minimize the
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00:47:09.600
collective, you know, air resistance, if you will, that they experience. Turns out solids
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00:47:17.280
in the protoplanetary disk do just this. There's an instability wherein solid particles, right,
link |
00:47:26.640
things that are a centimeter across will start to hide behind one another and form these clouds.
link |
00:47:33.680
Why? Because cumulatively, that minimizes the solid component of this aerodynamic interaction
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00:47:42.080
with the gas. Now these clouds, because they're kind of a favorable energetic condition for the
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00:47:49.120
dust to live in, they grow, grow, grow, grow, grow until they become so massive that they collapse
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00:47:54.880
under their own weight. That's how the first building blocks of planets form. That's how the
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00:48:00.320
big asteroids got there. That's incredible. So is that simulatable or is it not useful to simulate?
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00:48:06.800
No, no, that's simulatable. And people do these types of calculations. It's really cool. That's
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00:48:13.600
actually, that's one of the many fields of planet formation theory that is really, really active.
link |
00:48:19.520
Right now, people are trying to understand all kinds of aspects of that process. Because of
link |
00:48:24.080
course, I've explained it as if there's one thing that happens, turns out it's a beautifully rich
link |
00:48:33.200
dynamic. But qualitatively, formation of the first building blocks actually follows the same
link |
00:48:39.680
sequence as formation of stars. Stars are just clouds of gas, hydrogen helium gas that sit in
link |
00:48:48.080
space and slowly cool. And at some point, they contract to a point where their gravity overtakes
link |
00:48:57.280
the thermal pressure support, if you will. And they collapse under their own weight,
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00:49:01.680
and you get a little baby solar system. That's amazing. So do you think one day
link |
00:49:05.280
it'll be possible to simulate the full history that took our solar system to what it is today?
link |
00:49:13.360
Yes, and it will be useless. So you don't think your story, many of the ideas that you have about
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00:49:21.520
Jupiter clear in the space, like retelling that story in high resolution is not that important?
link |
00:49:26.640
I actually think it's important. But at every stage, you have to design your experiments,
link |
00:49:35.680
your numerical computer experiments so that they test some specific aspect of that evolution. I
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00:49:44.560
am not a proponent of doing huge simulations because even if we forget the information theory
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00:49:53.760
aspect of not being able to simulate in full detail the universe, because if you do, then
link |
00:50:01.440
you have made an actual universe. It's not the simulation. Simulation is, in some sense,
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a compression of information. So therefore, you must lose detail. But that point aside,
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if we are able to simulate the entire history of the solar system in excruciating detail,
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I mean, it'll be cool, but it's not going to be any different from observing it, right? Because
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theoretical understanding, which is what ultimately I'm interested in, comes from taking
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complex things and reducing them down to something that, you know, some mechanism
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00:50:45.360
that you can actually quantify. That's the fun part of astrophysics, just kind of
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simulating things in extreme detail. We'll make cool visualizations, but that doesn't get you to
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any better understanding than you had before you did the simulation.
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00:51:04.880
If you ask very specific questions, then you'll be able to create very highly compressed,
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nice, beautiful theories about how things evolve. And then you can use those to then
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generalize to other solar systems, to other stars and other galaxies and say something
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generalizable about the entire universe. How difficult would it be to simulate
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00:51:28.240
our solar system such that we would not know the difference? Meaning, if we are living in a
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simulation, is there a nice, think of it as a video game, is there a nice compressible way of
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doing that? Or just kind of like you intuited with a three body situation, is just a giant mess
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that you cannot create a video game that will seem realistic without actually building your
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scratch? I'm speculating, but one of the, yeah, I know you have a deep understanding of this,
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but for me, I'm just going to speculate that for at least in the types of simulations that we can
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do today, inevitably, you run into the problem of resolution. It doesn't matter what you're
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doing, it is discrete. Now, the way you would go about asking, what we're observing, is that a
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simulation or is that some real continuous thing? You zoom in and try and find the grid scale, if
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you will. Yeah, I mean, it's a really interesting question and because the solar system itself
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and really the double pendulum is chaotic, pendulum sitting on another pendulum
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00:53:03.040
moves unpredictably once you let them go. You really don't need to inject any randomness
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00:53:10.480
into a simulation for it to give you stochastic and unpredictable answers. Weather is a great
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00:53:17.120
example of this. Weather has a typical weather systems have a lapen of time of a few days,
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and there's a fundamental reason why the forecast always sucks two weeks in advance.
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00:53:31.920
It's not that we don't know the equations that govern the atmosphere, we know them well. Their
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solutions are meaningless though after a few days. The zooming in thing is very interesting. I think
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about this a lot, whether there'll be a time soon where we would want to stay in video game worlds,
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whether it's virtual reality or just playing video games. I think that time came in the 90s
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and it's been that time. Well, it's not just came, it's accelerated. I just recently saw
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that WoW and Fortnite were played 140 billion hours and those are just video games and that's
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00:54:13.600
increasing very, very quickly, especially with the people coming up now and being born now and
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00:54:18.400
become teenagers and so on. Let's have a thought experiment where it's just you and a video game
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00:54:24.400
character inside a room. Where you remove the simulation, they need to simulate a lot of objects.
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If it's just you and that character, how far do you need to simulate in terms of zooming in
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for it to be very real to you, as real as reality? First of all, you mentioned zooming in,
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which is fascinating because we have these tools of science that allow us to zoom in in all kinds
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of ways in the world around us, but our cognitive abilities like our perception system as humans
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is very limited in terms of zooming in. So we might be very easily fooled.
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Some of the video games on the PS4 look pretty real to me. I think you would really have to
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interrogate. I think even with what we have today, Ace Combat 7 is a great example. The way that the
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clouds are rendered, it looks just like when you're flying on a real airplane, the kind of
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transparency. I think that our perception is limited enough already to not be able to tell
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00:55:42.240
some of the differences. There's a game called Skyroom. It's an Elder Scrolls world playing
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game. I played it for quite a bit. I think I played it very different than others. There'll be
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long searches of time where I would just walk around and look at nature in the game. It's
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incredible. Oh, sure. It's just like the graphics is like, wow, I want to stay there. It was better.
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I went hiking recently. It was as good as hiking. So look, I know what you mean. Not to go on a
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huge video game tangent, but the third Witcher game was astonishingly beautiful, especially
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like playing on a good hardware machine. This is pretty legit. That said,
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I don't resonate with the I want to stay here. One of the things that I love to do
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00:56:43.120
is to go to my boxing gym and box with the guy. There's nothing quite like that physical
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experience. That's fascinating. That might be simply an artifact of the year you were born.
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Maybe. Because if you're born today, it almost seems like stupid to go to a gym.
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00:57:06.160
You go to a gym to box with the guy. Why not box with Mike Tyson? When you yourself,
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in his prime, when you yourself are also an incredible boxer in the video game world.
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00:57:15.920
For me, there's a multitude of reasons why I don't want to box with Mike Tyson.
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00:57:21.040
No, I enjoy tea and I want to have an ear. No, but your skills in this meat space,
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in this physical realm is very limited and takes a lot of work. You're a musician.
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00:57:35.520
You're an incredible scientist. You only have so much time in the day, but in the video game
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00:57:41.200
world, you can expand your capabilities and all kinds of dimensions that you can never have
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possibly have time in the physical world. It doesn't make sense to be existing,
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00:57:53.120
to be working your ass off in the physical world when you can just be super successful
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in the video game world. But I still, you enjoy sucking at stuff?
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Yeah, I really struggle to get better. I sure do. I think these days with music,
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music is a great example. We just started practicing live with my band again after
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00:58:18.080
not playing for a year. It was terrible. It was just a lot of the nuance, a lot of the detail
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00:58:26.800
is just that detail that takes years of collective practice to develop. It's just lost, but it was
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just an incredible amount of fun, way more fun than all the studio sitting around and playing
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00:58:42.320
that I did throughout the entire year. There's something intangible or maybe tangible about
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being in person. I sure hope you're wrong. That's not something that will get lost,
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because I think there's such a large part of the human condition is to hang out. If we were doing
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00:59:06.800
this interview on Zoom, I'd already be bored out of my mind. Exactly. I mean, there's something
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to that. I'm almost playing devil's advocate, but at the same time, I'm sure people talk about
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00:59:23.040
the same way at the beginning of the 20th century about horses, where they are much more efficient.
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00:59:30.000
They're much easier to maintain than cars. It doesn't make sense to have all the ways that cars
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00:59:36.480
break down. There's not enough infrastructure in terms of roads for cars. It doesn't make any
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00:59:41.200
sense. Horses and nature, you could do the nature where you should be living more natural life.
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Those are real. You don't want machines in your life that are going to pollute your mind
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and the minds of young people, but then eventually just cars took over. In that same way, it just
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seems... Going back to horses. You can play Red Dead Redemption. Redemption. You can ride
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01:00:08.080
horses in the video game world. Let me return us back to Planet Nine. Always a good place to
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01:00:14.640
come back to. Now that we did a big historical overview of our solar system, what is Planet
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01:00:20.240
Nine? Planet Nine is a hypothetical object that orbits the solar system at an orbital period
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01:00:30.320
of about 10,000 years. An orbit which is slightly tilted with respect to the plane of the solar
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01:00:37.680
system, slightly eccentric. The object itself, we think, is five times more massive than the earth.
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01:00:46.240
We have never seen Planet Nine in a telescope, but we have gravitational evidence for it.
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01:00:53.600
This is where all the stuff we've been talking about, this clustering ideas, maybe you can speak
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01:00:58.560
to the approximate location that we suspect. Also, the question I wanted to ask is,
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01:01:04.960
what are we supposed to be imagining here? Because you said there are certain objects in
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01:01:09.040
the Kuiper Belt that have a direction to them that they're all flocking in some way. That's
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01:01:16.480
the sense that there's some gravitational object, not changing their orbit, but confining them.
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01:01:24.000
Grouping their orbits together. What would happen if Planet Nine were not there? Is these orbits
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01:01:29.760
that roughly share a common orientation, they would just disperse. They would just become
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01:01:36.480
as a mutally symmetric point everywhere. Planet Nine's gravity makes it such that these objects
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01:01:44.800
stay in a state that's basically anti aligned with respect to the orbit of Planet Nine
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01:01:52.880
and sort of hang out there and kind of oscillate on timescale of about a billion years.
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01:01:58.320
That's one of the lines of evidence for the existence of Planet Nine. There are others.
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01:02:03.920
That's the one that's easiest to maybe visualize just because it's fun to think about orbits that
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01:02:08.160
all point into the same direction. But I should emphasize that, for example, the existence of
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01:02:16.320
objects, again, Kuiper Belt objects that are heavily out of the plane of the solar system,
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01:02:21.520
things that are tilted by, say, 90 degrees, that's not, we don't expect that as an outcome
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01:02:28.640
of planet formation. Indeed, planet formation simulations have never produced such objects
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01:02:35.440
without some extrinsic gravitational force. Planet Nine, on the other hand, generates them very
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01:02:40.960
readily. So that provides kind of an alternative population of small bodies in the solar system
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01:02:49.440
that also get produced by Planet Nine through an independent kind of gravitational effect.
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01:02:53.920
So there are basically five different things that Planet Nine does individually that are
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01:03:03.200
like kind of maybe a one sigma effect where you'd say, yeah, okay, if that's all it was,
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01:03:09.200
maybe it's not no reason to jump up and down. But because it's a multitude of these puzzles
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01:03:16.080
that all are explained by one hypothesis, that's really the magnetism, the attraction of the
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01:03:23.040
Planet Nine model. So can you just clarify? So most orbit, most planets in the solar system orbit
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01:03:33.280
and approximately the same, so it's flat. Yeah, it's like one degree. The difference between
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01:03:39.440
them is about one degree. But nevertheless, if we looked at our solar system, it would look,
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01:03:45.440
and I could see every single object, it would look like a sphere.
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01:03:48.080
The inner part where the planets are would look like flat. The Kuiper belt and the Asteroid belt
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01:03:58.000
have a larger... It gets fatter and fatter and fatter and becomes a sphere.
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01:04:03.520
That's right. And if you look at the very outside, it's polluted by this
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01:04:08.640
quasi spheroidal thing. Nobody's, of course, ever seen the Oort cloud. We've only seen
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01:04:15.200
comments that come from the Oort cloud. So the Oort cloud, which is this population of
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01:04:21.920
distant debris, its existence is also inferred. You could say alternatively, there is a big
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01:04:30.480
cosmic creature that occasionally is sitting at 20,000 AU and occasionally throws an icy
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01:04:36.640
rock towards the sun like that. Spaghetti monster, I think it's called.
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01:04:39.680
Okay. So it's a mystery in many ways, but you can infer a bunch of things about it.
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01:04:46.880
By the way, both terrifying and exciting that there's this vast darkness all around us that's
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01:04:51.520
full of objects that they're just throwing. It's actually astonishing that we have only
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01:05:00.240
explored a small fraction of the solar system. That really kind of baffles me because,
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01:05:07.760
remember, as a student studying physics, you do the problem where you put the earth around the sun,
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01:05:15.280
you solve that and it's one line of math and you say, okay, well, that surely was figured out by
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01:05:21.520
Newton. So all the interesting stuff is not in the solar system, but that, it's just plainly not
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01:05:30.160
true. There are mysteries in the solar system that are remarkable that we are only now starting to
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01:05:38.160
just kind of scratch the surface of. And some of those objects probably have some information
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01:05:42.960
about the history of our solar system. Absolutely. Like a great example is small
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01:05:48.960
meteorites. Small meteorites are melted. They're differentiated, meaning some of the
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01:05:55.280
iron sinks to corn. You say, well, how can that be? Because they're so small that they wouldn't
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01:06:01.440
have melted just from the heat of their accretion. Turns out the fact that the solar nebula, the
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01:06:07.920
disk that made the planets was polluted by aluminum 26 isn't itself a remarkable thing. It means
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01:06:14.880
the solar system did not form an isolation. It formed in a giant cloud of thousands of other
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01:06:21.360
stars that were also forming, some of which were undergoing, going through a supernova
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01:06:27.280
explosion, some of, and releasing these unstable isotopes that, of which we now see kind of the
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01:06:35.680
traces of. It's so cool. Do you think it's possible that life from other solar systems was injected
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01:06:43.360
and that was what was the origin of life on Earth? Yeah, the panspermy idea. That's seen as a low
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01:06:51.760
probability event by people who studied the origin of life, but that's because then they would be
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01:06:56.720
out of a job. Well, I don't think they'd be out of the job because you just then say you have to
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01:07:01.760
figure out how life started there. But then you have to go there. We can study life on Earth much
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01:07:07.280
easier. We could study it in the lab much easier because we can replicate conditions that are
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01:07:12.880
from an early Earth much easier from a chemistry perspective, from a biology perspective.
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01:07:19.520
You can intuit a bunch of stuff. You can look at different parts of Earth. To an extent,
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01:07:24.400
I mean, the early Earth was completely unlike the current Earth. There was no oxygen.
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01:07:31.120
One of my colleagues at Caltech, Joe Kirschnick, is certain, something like 100% certainty that
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01:07:41.600
life started on Mars and came to Earth on Martian media rights. This is not a problem that I like
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01:07:51.840
to kind of think about too much, like the origin of life. It's a fascinating problem, but it's
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01:07:58.960
not physics and I just don't love it. It's the same reason you don't love, I thought you're a
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01:08:05.520
musician. Music is not physics either, so why are you so into it? 100% physics. In all seriousness,
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01:08:15.680
though, there are a few things that I really, really enjoy. I genuinely enjoy physics. I genuinely
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01:08:23.840
enjoy music. I genuinely enjoy martial arts and I genuinely enjoy my family. I should have said that
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01:08:32.160
all in a reverse order or something, but I like to focus on these things and not worry too much
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01:08:38.080
about everything else. You know what I mean? Yes. Just because, like you said earlier,
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01:08:43.440
there's a time constraint. You can't do it all. There's many mysteries all around us and they're
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01:08:50.800
all beautiful in different ways. To me, that thing I love is artificial intelligence. Perhaps I love
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01:08:58.160
it because eventually I'm trying to suck up to our future overlords. The question of, you said
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01:09:05.040
there's a lot of kind of little pieces of evidence for this thing that's Planet 9. If we were to try
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01:09:12.080
to collect more evidence or be certain, like a paper that says, like you drop it, clear, we're
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01:09:20.560
done, what does that require? Does that require ascending probes out or do you think we can do
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01:09:26.240
it from telescopes here on Earth? What are the different ideas for conclusive evidence for Planet
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01:09:31.280
9? The moment Planet 9 gets imaged from a telescope on Earth, it's done. I mean, it's just there.
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01:09:37.760
Can you clarify, because you mentioned that before, from an image, would you be able to tell?
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01:09:42.800
Yes. From an image, the moment you see something, something that is reflecting sunlight back at you
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01:09:52.160
and you know that it's hundreds of times as far away from the sun as the Earth, you're done.
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01:10:02.240
So basically, if you have a really far away thing that's big, five times the size of Earth,
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01:10:09.760
that means that is Planet 9. Could there be multiple objects like that? I guess...
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01:10:16.080
In principle, yeah. I mean, there's no law of physics that doesn't allow you to have multiple
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01:10:22.160
objects. There's also no evidence at present for there being multiple objects.
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01:10:25.680
I wonder if it's possible, just like we're finding exoplanets where they're given the
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01:10:30.960
size of the ore cloud, there's basically, it's rare and rare, but they're sprinkled, Planet 9,
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01:10:36.960
10, 11, 12, some... Got 13. Yeah, it goes after that. I can just keep counting. So just something
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01:10:46.000
about the dynamic system, it becomes lower and lower probability event, but they gather up,
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01:10:53.520
would they become larger and larger maybe, something like that. I wonder, I wonder if
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01:10:58.480
discovering Planet 9 will just be almost like a springboard, it's like, well, what's beyond that?
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01:11:05.360
It's entirely plausible. The ore cloud itself probably holds about five Earth masses or seven
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01:11:11.360
Earth masses of material. So it's not nothing. And it all ultimately comes down to,
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01:11:22.640
at what point will the observational surveys sample enough of the solar system to
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01:11:28.720
reveal interesting things? There's a great analogy here with Neptune and the story of
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01:11:36.720
how Neptune was discovered. Neptune was not discovered by looking at the sky. It was discovered
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01:11:42.880
by, it was discovered mathematically. So yeah, the orbit of Uranus, when Uranus was found,
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01:11:50.400
this was 1781, it's the kind of tracking, both the tracking of the orbit of Uranus as well as
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01:12:00.800
the reconstruction of the orbit of Uranus immediately revealed that it was not following
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01:12:07.440
the orbit that it was supposed to. The predicted orbit deviated away from where it actually was.
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01:12:13.200
So in the mid 1800s, a French mathematician by the name of Orban Le Verrier did a
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01:12:23.600
beautifully sophisticated calculation which said, if this is due to gravity of a more distant planet,
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01:12:31.120
then that planet is there. And then they found it. But the point is, the understanding of where to
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01:12:38.720
look for Neptune came entirely out of celestial mechanics. This case with Planet 9 is a little
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01:12:45.920
bit different because what we can do, I think relatively well, is predict the orbit and mass
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01:12:51.200
of Planet 9. We cannot tell you where it is on its orbit. The reason is we haven't seen
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01:12:56.480
the Kuiper Belt objects complete an orbit, their own orbit even once because it takes 4,000 years.
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01:13:04.400
But I plan to live on as an AI being and I'll be tracking those orbits.
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01:13:12.640
So it takes 4,000 or 5,000 years. I mean, it doesn't have to be AI. It could be longevity.
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01:13:17.040
There's a lot of really exciting genetic engineering research. So you'll just be a
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01:13:20.800
brain waiting for the orbit to complete for the basic Kuiper Belt objects.
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01:13:27.600
That's right. That's kind of the worst reason to want to live a long time. Can the brain smoke
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01:13:35.680
a cigarette? Can you just light one up while you're waiting?
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01:13:43.680
But you're making me actually realize that the one way to explore the galaxy is by just sitting
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01:13:52.560
here on Earth and waiting. So if we can just get really good at waiting, it's like a Moa Moa or
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01:13:58.320
these interstellar objects that fly in, you can just wait for them to come to you. Same with
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01:14:02.960
the aliens. You can wait for them to come to you. If you get really good at waiting,
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01:14:07.920
then that's one way to do the exploration because eventually the thing will come to you.
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01:14:12.320
Maybe the intelligent alien civilizations get much better at waiting and so they all decide
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01:14:19.920
to give them theoretically to start waiting. It's just a bunch of ancient intelligent civilizations
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01:14:25.360
of aliens all throughout the universe just sitting there waiting for each other.
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01:14:29.200
Look, you can't just be good at waiting. You got to know how to chill. You can't just sit around
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01:14:35.360
and do nothing. You got to know how to chill. I honestly think that as we progress, if the aliens
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01:14:42.240
are anything like us, we enjoy loving things we do. It's very possible that we just figure out
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01:14:49.600
mechanisms here on Earth to enjoy our life and we just stay here forever that exploration becomes
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01:14:58.080
less and less of an interesting thing to do. So you basically, yes, wait and chill. You get
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01:15:03.600
really optimally good at chilling and thereby exploring is not that interesting. So in terms
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01:15:10.720
of 4,000 years, it would be nothing for scientists. We'll be chilling and just all kinds of scientific
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01:15:15.520
explorations will become possible because we'll just be here on Earth.
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01:15:19.840
So chill. So chill.
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01:15:21.680
So chill. You have a paper out recently because you already mentioned some of these ideas,
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01:15:25.600
but I'd love it if you could dig into it a little bit. Of course.
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01:15:28.480
The injection of inner or cloud objects into the distant Kuiper Belt by Planet 9.
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01:15:34.800
What is this idea of Planet 9 injecting objects into the Kuiper Belt?
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01:15:40.720
Okay. Let me take a brief step back and say, when we do calculations of Planet 9, when we do the
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01:15:48.080
simulations, as far as our simulations are concerned, sort of the Neptune, like kind of the
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01:15:58.320
transneptunian solar system is entirely sourced from the inside. Namely, the Kuiper Belt gets
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01:16:06.240
scattered by Neptune and then Planet 9 does things to it and aligns the orbits and so on.
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01:16:11.760
Then we calculate what happens on the lifetime of the solar system. Yeah, yeah, yeah.
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01:16:18.240
During the pandemic, one of the kind of questions we asked ourselves, and this is indeed something
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01:16:23.040
we, Mike and I, Mike Brown, who's a partner in crime on this, and I do regularly, is we say,
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01:16:31.760
how can we, A, disprove ourselves and B, how can we improve our simulations? What's missing?
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01:16:40.640
One idea that maybe should have been obvious in retrospect is that all of our simulations
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01:16:46.720
treated the solar system as some isolated creature, but the solar system did not form an
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01:16:52.240
isolation. It formed in this cluster of stars. During that phase of forming together with thousands
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01:16:59.680
of other stars, we believe the solar system formed this almost spherical population of icy debris
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01:17:07.920
that sits maybe at a few thousand times the separation between the Earth and the Sun,
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01:17:17.280
maybe even a little bit closer. If Planet 9 is not there, that population is completely dormant,
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01:17:24.560
and these objects just slowly orbit the Sun, nothing interesting happens to them ever.
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01:17:32.480
But when we realize that if Planet 9 is there, Planet 9 can actually grab some of those objects
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01:17:37.680
and gravitationally reinject them into the distant solar system. So we thought, okay,
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01:17:43.440
let's look into this with numerical experiments. Do our simulations, does this process work? And if
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01:17:49.280
it works, what are its consequences? So it turns out indeed, not only does Planet 9 inject
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01:17:58.400
these distant inner or cloud objects into the Kuiper belt, they follow roughly the same pathway
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01:18:06.640
as the objects that are being scattered out. So there's this kind of two way river of
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01:18:14.160
material, some of it is coming out by Neptune scattering, some of it is moving in. And if you
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01:18:21.360
work through the numbers, you kind of, at the end of the day, that it has an effect on the best fit
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01:18:28.240
orbit for Planet 9 itself. So if you realize that the data set that we're observing is not entirely
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01:18:34.800
composed of things that came out of the solar system, but also things that got re injected back in,
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01:18:39.840
then turns out the best fit Planet 9 is slightly more eccentric. That's kind of getting into the
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01:18:44.240
weeds. The point here is that the existence of Planet 9 itself provides this natural bridge
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01:18:52.880
that connects an otherwise dormant population of icy debris of the solar system with things that
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01:18:58.000
we're starting to directly observe. So it can flow back, so it's not just the river flowing one way,
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01:19:02.160
it's maybe a smaller stream go back and backwash. You want to incorporate that into the simulations
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01:19:09.040
into your understanding of those distant objects when you're trying to make sense of the various
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01:19:13.760
observations and so on. Exactly. That's fascinating. I got to ask you, some people think that many
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01:19:21.760
of the observations that you're describing could be described by a primordial black hole. First,
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01:19:28.720
what is a primordial black hole and what do you think about this idea? Yeah. So primordial black
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01:19:33.760
hole is a black hole which is made not through the usual pathway of making a black hole,
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01:19:41.680
which is that you have a star, which is more massive than 1.4 or so solar masses. Basically,
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01:19:50.240
when it runs out of fuel, runs out of its nuclear fusion fuel, it can't hold itself up anymore and
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01:19:58.320
just the whole thing collapses on itself. You create a simple way to think about it is you
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01:20:08.160
create an object with zero radius that has mass but zero radius, singularity. Now, such black
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01:20:18.160
holes exist all over the place. In the galaxy, there's in fact a really big one at the center
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01:20:23.200
of the galaxy. That one's always looking at you when you're not looking. It's always talking
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01:20:31.040
about you. And when you turn off the lights, it wakes up. That's right. So such black holes
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01:20:38.800
are all over the place. When they merge, we get to see incredible gravitational waves that they
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01:20:44.160
emit, etc. One plausible scenario, however, is that when the universe was forming, basically
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01:20:50.720
during the Big Bang, you created a whole spectrum of black holes, some with masses of 5 Earth masses,
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01:20:59.920
some with masses of 10 Earth masses, like the entire mass spectrum size, some the mass of
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01:21:07.520
asteroids. Now, on the smaller end, over the lifetime of the universe, the small ones kind of
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01:21:14.240
evaporate. And they're not there anymore. At least this is what the calculations tell us. But 5
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01:21:21.680
Earth masses is big enough to not have evaporated. So one idea is that Planet 9 is not a planet,
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01:21:29.600
and instead it is a 5 Earth mass black hole. And that's why it's hard to find. Now,
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01:21:37.040
can we right away from our calculations say that's definitely true or that's not true? Absolutely
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01:21:45.280
not. In fact, our calculations tell you nothing other than the orbit and the mass. And that means
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01:21:55.120
the black hole, I mean, it could be a 5 Earth mass cup. It could be a 5 Earth mass hedgehog
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01:22:01.920
or a black hole, or really anything that's 5 Earth masses will do, because the gravity of a
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01:22:07.440
black hole is no different than the gravity of a planet. If the Sun became a black hole tomorrow,
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01:22:14.480
it would be dark, but the Earth would keep orbiting it. This notion that, oh, black holes suck
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01:22:20.960
everything in, that's like a sci fi notion. It's just mass. What would be the difference between
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01:22:26.800
a black hole and a planet in terms of observationally? Observationally, the difference would be that you
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01:22:34.320
will never find the black hole. The truth is, I never looked into this very carefully,
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01:22:43.520
but there are some constraints that you can get just statistically to say, okay, if the Sun
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01:22:50.640
has a binary companion, which is a 5 Earth mass black hole, then that means such black holes would
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01:22:58.000
be extremely common, and you can sort of look for lensing events, and then you say, okay,
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01:23:03.360
maybe that's not so likely. But that said, I want to emphasize that there's a limit to what
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01:23:09.840
our calculations can tell you. That's the orbit and the mass.
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01:23:13.920
So I think there's a bunch, like Ed Whitten, I think wishes it's a black hole, because I think
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01:23:21.200
one exciting thing about black holes in our solar system is that we can go there and we can maybe
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01:23:27.600
study the singularity somehow, because that allows us to understand some fundamental things about
link |
01:23:32.000
physics. If it's a planet, it's a planet nine, we may not, and we go there, we may not discover
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01:23:39.920
anything profoundly new. The interesting thing, perhaps you can correct me about, planet nine
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01:23:46.320
is like the big picture of it, the whole big story of the Kuiper Belt and all those kinds of things.
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01:23:52.000
It's not that planet nine would be somehow fundamentally different from, I don't know, Neptune
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01:24:00.080
in terms of the kind of things we can learn from it. So I think that there's kind of a hope that
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01:24:05.600
it's a black hole because it's an entirely new kind of object. Maybe you can correct me.
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01:24:11.680
Yeah. I mean, of course here, my own biases creep in because I'm interested in planets around
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01:24:18.320
other stars. And I would say, I would disagree that we wouldn't find things that would be truly
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01:24:27.680
fundamentally new, because as it turns out, the galaxy is really good at making
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01:24:34.320
five or three earth mass objects. The most common type of planet that we see, that we
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01:24:43.440
discover orbiting around other stars is a few earth masses. In the solar system,
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01:24:48.240
there's no analog for that. We go from one earth mass object, which is this one,
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01:24:53.040
to skipping to Neptune and Uranus, which themselves are actually relatively poorly
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01:24:58.480
understood, especially Uranus from the interior structure point of view. If planet nine is a
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01:25:04.800
planet, going there will give us the closest window and to understanding what other planets look like.
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01:25:11.760
And I will, I'll say this, that planets kind of in terms of their complexity on some logarithmic
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01:25:20.640
scale fall somewhere between a star and an insect. And the insect is way more complicated than a star.
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01:25:31.360
All kinds of physical processes and really biochemical processes that occur inside of an
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01:25:37.360
insect that just make a star look like somebody is like playing with the spring or something.
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01:25:44.480
So, I think it would be arguably more interesting to go to planet nine if it's a planet,
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01:25:57.760
because black holes are simple. They're basically macroscopic particles.
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01:26:05.600
Just like the style you mentioned, in terms of complexity. So, it's possible that planet nine
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01:26:09.840
is supposed to be like homogeneous is like super, like heterogeneous is a bunch of cool
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01:26:15.360
stuff going on that could give us intuition. I never thought about that, that it's just
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01:26:20.000
basically earth number two in terms of size and gives us, starts giving us intuition that
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01:26:26.640
could be generalizable to earth like planets elsewhere in the galaxy.
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01:26:31.280
I mean, yeah, Pluto is also in the sense like, you know, Pluto is a tiny, tiny thing, right?
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01:26:36.880
Just like, you would imagine it's just a tiny ball of ice like who cares. But the New Horizons
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01:26:42.320
images of Pluto reveal so much remarkable structure, right? They reveal glaciers flowing,
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01:26:49.120
and these are glaciers not made out of water ice, but, you know, CO ice. It turns out at those
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01:26:54.880
temperatures, right, of like 40 or so Kelvin, water ice looks like metal, right? Just doesn't
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01:27:01.920
flow at all. But then ice made up of carbon monoxide starts to flow. I mean, there's just
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01:27:07.840
like all kinds of really cool phenomena that you otherwise just wouldn't really even imagine
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01:27:15.840
that occur. So, yeah, I mean, there's a reason why I like planets.
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01:27:21.280
Well, let me ask you, I find, as I read the idea that Ed Whitton was thinking about this
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01:27:28.720
kind of stuff, fascinating. So, he's a mathematical physicist who's very interested in string theory,
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01:27:35.840
won the field's medal for his work in mathematics. So, I read that he proposed a fleet of probes
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01:27:44.560
accelerated by radiation pressure that could discover a planet nine primordial black holes
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01:27:49.840
location. What do you think about this idea of sending a bunch of probes out there?
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01:27:55.280
Yeah, look, the way the idea is a cool one, right? You go and you say, you know, launch them
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01:28:04.720
basically isotropically, you track where they go. And if I understand the idea correctly,
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01:28:11.360
you basically measure the deflection and you say, okay, that must be something
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01:28:18.000
there since the probe trajectories are being altered.
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01:28:21.600
Also, the measurement, the basic sensory mechanism is the, it's not like you have
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01:28:26.000
sensors on the probes, it's more like you're, because you're very precisely able to capture,
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01:28:31.600
to measure the trajectory of the probes, you can then infer the gravitational
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01:28:35.120
fields and I think, I think that's the basic idea. You know, back a few years ago, we had
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01:28:42.560
conversations like these with, you know, engineers from JPL, they more or less convinced me that
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01:28:50.880
this is much more difficult than it seems because you don't, at that level of precision,
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01:28:57.280
right? Things like solar flares matter, right? Solar flares, right, are completely
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01:29:03.200
chaotic. You can't predict which, where a solar flare will happen. That will drive
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01:29:08.240
radiation pressure gradients. You don't know where every single asteroid is. So like,
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01:29:12.880
actually doing that problem, I think it's possible, but it's, it's not a trivial matter, right?
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01:29:20.880
Well, I wonder, not just about Planet Nine, I wonder if that's kind of the future of doing
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01:29:27.840
science in our solar system is to just launch a huge number of probes. So like a whole order of
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01:29:34.320
magnitude, many orders of magnitude, larger numbers of probes and then start to infer a bunch
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01:29:40.640
of different stuff, not just gravity, but everything else. So in this regard, I actually
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01:29:46.080
think there is a huge revolution that's to some extent already started, right? The standard kind
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01:29:52.880
of like timescale for a NASA mission is that you like propose it and it launches, I don't know,
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01:29:59.200
like 150 years after you propose, I'm over exaggerating, but you know, it's just like some
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01:30:05.280
huge development cycle and it gets delayed 55 times. Like that is not going away, right?
link |
01:30:15.680
The really cutting edge things, you have to do it this way because you don't know what you're
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01:30:20.400
building, so to speak. But the CubeSat kind of world is starting to, you know, provide an avenue
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01:30:29.520
for like launching something that costs a few million dollars and has a turnaround timescale
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01:30:36.800
of like a couple of years. You can imagine doing PhD theses where you design the mission,
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01:30:42.960
the mission goes to where you're going and you do the science all within a time span of five,
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01:30:48.240
six years. That has not been fully executed on yet, but I absolutely think that's on the horizon
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01:30:55.920
and we're not talking a decade, I think we're talking like this decade. Yeah, and the companies
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01:31:01.280
are accelerating all this with Blue Origin and SpaceX. There's a bunch of more CubeSat oriented
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01:31:09.600
companies that are pushing this forward. Let me ask you on that topic, what do you think about
link |
01:31:16.800
either one? Elon Musk with SpaceX going to Mars, I think he wants SpaceX to be the first
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01:31:23.680
to put a first human on Mars. And then Jeff Bezos got to give him props, wants to be the first to
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01:31:33.120
fly his own rocket out into space. You know, wasn't there a guy who like built his rocket out of
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01:31:41.200
garbage? Yeah. This was like a couple years ago and somewhere in the desert he launched himself.
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01:31:47.440
I'm not tracking this closely, but I think I am familiar with folks who built their own rocket
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01:31:52.720
to try to prove the Earth is flat. Yes, that's the guy. He was also like he also jumped some limousine.
link |
01:32:00.400
Truly revolutionary mind. You have to
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01:32:04.000
greater men than either you or I. So look, it's been astonishing to watch how really over the
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01:32:13.360
last decade the commercial sector took over this industry that traditionally has really
link |
01:32:23.280
been like a government thing to do. Motivated primarily by the competition between nations
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01:32:30.960
like the Cold War. And now it's motivated more and more by the natural forces of capitalism.
link |
01:32:38.640
Yes, that's right. So, okay, here I have many ideas about I think on the one hand, right,
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01:32:45.360
like what SpaceX has been able to do, for example, phenomenal. If that brings down the price of
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01:32:54.320
SpaceX within that turnaround timescale for space exploration, which I think it inevitably will,
link |
01:33:01.600
that's a huge boost to the human condition. The same time, right, if we're talking
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01:33:08.400
astronomy, there also it comes at a huge cost. And the Starlink satellites is a great example
link |
01:33:15.600
of that cost. At one point, in fact, I was just camping in the Mojave with a friend of mine,
link |
01:33:23.520
and they saw this string of satellites just kind of appear and then disappear into nowhere. So that
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01:33:33.040
is beginning to interfere with earth based observations. So I think there's tremendous
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01:33:39.840
potential there. It's also important to be responsible about how it's executed.
link |
01:33:44.800
Now, with Mars and the whole idea of exploring Mars, I don't have like strong opinions on whether
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01:33:53.520
a manned mission is required or not required. But I do think the thing to keep in mind is that
link |
01:34:06.400
I'm not signed on, if you will, to the idea that Mars is some kind of a safe haven that we can
link |
01:34:13.840
escape to. Mars sucks. Living on Mars, if you want to live on Mars, you can have that experience
link |
01:34:25.600
by going to the Mojave desert and camping, and it's just not a great...
link |
01:34:31.920
It's interesting, but there's something captivating about that kind of mission of us
link |
01:34:35.920
striving out into space, and by making Mars in some way habitable for at least months at a time,
link |
01:34:46.000
I think would lead to engineering breakthroughs that would make life in many ways much better
link |
01:34:51.760
on earth. It will come up with ideas we totally don't expect yet, both on the robotic side,
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01:34:57.840
on the food engineering side, maybe we'll switch from... There'll be huge breakthroughs in insect
link |
01:35:07.120
farming as exciting as I find that idea to be. In the ways we consume protein, maybe
link |
01:35:15.680
it'll revolutionize, we do factory farming, which is full of cruelty and torture of animals,
link |
01:35:21.840
we'll revolutionize that completely because of our... We shouldn't need to go to Mars to
link |
01:35:27.760
revolutionize life here on earth, but at the same time, I shouldn't need a deadline to get
link |
01:35:32.720
shit done, but I do need it. In the same way, I think we need Mars. There's something about
link |
01:35:38.000
the human spirit that loves that longing for exploration. I agree with that thesis. Going
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01:35:43.120
to the moon and that whole endeavor has captivated the imagination of so many, and it has led to
link |
01:35:56.160
incredible ideas, really, and probably in nonlinear ways, not like, okay, we went to the moon,
link |
01:36:03.120
therefore, some person here has thought of this. In that similar sense, I think space exploration
link |
01:36:10.320
is... There's some real magnetism about it, and it's on a genetic level. We have this
link |
01:36:18.720
need to keep exploring when we're done with a certain frontier, we move on to the next frontier.
link |
01:36:26.240
All that I'm saying is that I'm not moving to Mars to live there permanently ever, and I think
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01:36:33.120
that... I'm glad you noted the degradation of the earth. I think that is a true leading order
link |
01:36:43.520
challenge of our time. Yeah, a great engineer. That's a bunch of engineering problems. I'm
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01:36:48.320
most interested in this space because as I've read extensively, it's apparently very difficult to
link |
01:36:54.080
have sex in space, and so I just want that problem to be solved because I think once we solve the
link |
01:36:59.760
sex in space problem, we'll revolutionize sex here on earth, thereby increasing the fun on earth,
link |
01:37:05.600
and the consequences of that can only be good. I mean, you've got a clear plan, right, and it
link |
01:37:13.120
sounds like... I'm submitting proposals to NASA as we speak. That's right. I keep getting rejected.
link |
01:37:19.520
I don't know why. Okay. You need better diagrams. Better pictures. I should have thought of that.
link |
01:37:26.400
You a while ago mentioned that there's certain aspects in the history of the solar system and
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01:37:31.760
earth that resulted... It could have resulted in an opaque atmosphere, but it didn't. We can see the
link |
01:37:39.760
stars. Somebody mentioned to me a little bit ago... It's almost like a philosophical question for you.
link |
01:37:48.240
Do you think the human society would develop as it did or at all if we couldn't see the stars?
link |
01:37:59.280
It would be drastically different. If it ever did develop... So I think some of the early
link |
01:38:06.960
developments of like... Fire. First of all, that atmosphere would be so hot because if you have
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01:38:15.440
an opaque atmosphere, the temperature at the bottom is huge. So we would be very different
link |
01:38:24.320
beings to start with. We'd have very different... It could be cloudy in certain kinds of ways
link |
01:38:27.920
that you could still get. Okay. Think about like a greenhouse, right? A greenhouse is cloudy,
link |
01:38:34.560
effectively, but it's super hot. Yeah, it's hard to avoid having an atmosphere. If you have an
link |
01:38:41.760
opaque atmosphere, it's hard to... Venus is a great example. Venus is... I don't remember exactly how
link |
01:38:48.720
many degrees, but it's hundreds in Celsius. It's not 100, it's hundreds. Even though it's only a
link |
01:38:56.240
little bit closer to the sun, that temperature is entirely coming from the fact that the atmosphere
link |
01:39:00.880
is thick. So it's just a sauna of sorts. Yeah, you go there, you feel refreshed after you come back.
link |
01:39:07.520
But if you stay there, I mean, so, okay, take that as an assumption. This is a philosophical
link |
01:39:13.920
question, not a biological one. So you have a life that develops under these extremely hot
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01:39:18.480
conditions. Yeah, so let's see. So much of the early evolution of mankind was driven by exploration.
link |
01:39:26.800
Yeah. Right. And the kind of interest in stars originated in part as a tool to guide that exploration.
link |
01:39:37.280
Right? I mean, that in itself, I think would be a huge differential in the way that we
link |
01:39:46.240
are of our evolution on this planet. Yeah, I mean, stars, that's brilliant. So even in that aspect,
link |
01:39:52.800
but even in further aspects, astronomy just shows up in basically every single development
link |
01:40:00.720
in the history of science up until the 20th century, it shows up. So I wonder without that,
link |
01:40:08.480
if we would even get calculus. Yeah, look, that's a great point. Newton in part developed calculus
link |
01:40:16.960
because he was interested in understanding, explaining Kepler's laws, right? In general,
link |
01:40:23.360
that whole mechanistic understanding of the night sky, right, replacing a religious understanding
link |
01:40:29.760
where you interpret, you know, this is, you know, this whatever fire god writing his,
link |
01:40:35.360
you know, little chariot across the sky as opposed to, you know, this is some mechanistic set of
link |
01:40:42.000
laws that transformed humanity and arguably put us on the course that we're on today, right?
link |
01:40:50.320
The entirety of the last 400 years and the development of kind of our technological world
link |
01:40:57.040
that we live in today was sparked by that, right? Abandoning an effectively, you know,
link |
01:41:05.520
a non secular view of the natural world and kind of saying, okay, this can be understood. And if it
link |
01:41:13.760
can be understood, it can be utilized, we can create our own variants of this. Absolutely,
link |
01:41:19.600
we would be a very, very different species without astronomy. This I think extends
link |
01:41:26.400
beyond just astronomy, right? There are questions like why do we need to spend money on X, right?
link |
01:41:34.880
Where X can be anything like paleontology, right? The meeting patterns of penguins.
link |
01:41:42.320
Yeah, that's like, that's right. I think, you know, there's a tremendous under appreciation
link |
01:41:51.040
for the usefulness of useless knowledge, right? I mean, I didn't come up with this. This was a
link |
01:41:59.360
little book by the guy who started the Institute for Advanced Studies. But, you know, it's so true,
link |
01:42:08.800
so much of the electronics that are on this table, right, work on Maxwell's equations. Maxwell
link |
01:42:15.040
wasn't sitting around in the 1800s saying, you know, I hope one day, you know,
link |
01:42:19.600
we'll make, you know, a couple of mics. So, you know, a couple, you know, a couple guys can, you
link |
01:42:28.160
know, have this conversation, right? That wasn't at no point was that the motivation. And yet,
link |
01:42:35.760
you know, it gave us the world that we have today. And the answer is, if you are a purely
link |
01:42:42.320
pragmatic person, if you don't care at all about kind of the human condition, none of this,
link |
01:42:46.640
the answer is, you can tax it, right? Like the useless things have created
link |
01:42:56.640
way more capital than useful things. And the sad thing, I mean, first of all, it's really important
link |
01:43:03.680
to think about and it's brilliant in the following context. And like Neil deGrasse Tyson is this
link |
01:43:10.960
book about the role of military based funding in the development of science. And then so much of
link |
01:43:20.080
technological breakthroughs in the 20th century had to do with humans working on different military
link |
01:43:27.440
things. And then the outcome of that had nothing to do with military. It had some military application,
link |
01:43:32.480
but their impact was much, much bigger than military.
link |
01:43:36.560
The splitting of the atom is kind of a canonical example of this. We all know the tragedy that,
link |
01:43:43.120
you know, arises from splitting of the atom. And yet, you know, so much, I mean,
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01:43:50.320
the atom itself does not care for what purpose it is being split. So,
link |
01:43:55.200
So I wonder if we took the same amount of funding as we used for war and poured it into
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01:44:00.800
like totally seemingly useless things like the mating patterns of penguins, we would get the
link |
01:44:07.280
internet anyway. I think so. I think so. And, you know, perhaps more of the internet would have
link |
01:44:15.200
penguins, you know? So we're both joking. But in some sense, like, I wonder, it's not the
link |
01:44:22.480
penguins, because penguins is more about sort of biology, but all useless kind of tinkering and all
link |
01:44:28.240
kinds of, in all kinds of avenues. And also because military applications are often
link |
01:44:37.760
burdened by the secrecy required. So it's often like so much, the openness is lacking. And if we
link |
01:44:46.160
learned anything from the last few decades is that when there's openness in science,
link |
01:44:51.040
that accelerates the development of science. That's right. That's true. The openness of science
link |
01:44:56.480
truly, you know, it benefits everybody. The notion that if, you know, I share my science with you,
link |
01:45:04.640
then you're going to catch up and like know the same thing. That is a short sighted view point,
link |
01:45:10.480
because if you catch up and you open, you know, you discover something that puts me in a position
link |
01:45:18.480
to do the next step, right? So I absolutely agree with all of this. I mean, the kind of question
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01:45:28.800
of like military funding versus non military funding is obviously a complicated one. But
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01:45:34.720
at the end of the day, I think we have to get over the notion as a society that we are going to,
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01:45:43.360
you know, pay for this and then we will get that, right? That's true if you're buying like,
link |
01:45:50.800
I don't know, toilet paper or something, right? It's just not true in the intellectual pursuit.
link |
01:45:55.440
That's not how it works. And sometimes it'll fail, right? Like sometimes like a huge fraction of what
link |
01:46:02.800
I do, right? I come up with an idea. I think, oh, it's great. And then I work it out. It's totally
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01:46:07.600
not great, right? It fails immediately. Failure is not a sign that the initial pursuit was worthless.
link |
01:46:14.880
So failure is just part of this kind of this whole exploration thing. And we should fund more
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01:46:19.520
and more of this exploration, the variety of the exploration. I think it was Linus Pauling or somebody
link |
01:46:25.120
from, you know, that generation of scientists, you know, a good way to have good ideas is to have
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01:46:32.080
a lot of ideas. So that's, I think that's true. If you are conservative in your thinking, if you
link |
01:46:39.840
worry about proposing something that's going to fail and oh, what if, you know, like, I, there's no
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01:46:47.040
science police that's going to come and arrest you for proposing the wrong thing. And, you know,
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01:46:52.800
it's also just like, why would you, why would you do science if you're afraid of, you know,
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01:46:59.280
you know, taking that step? It would be so much better to propose things that are plausible,
link |
01:47:05.520
that are interesting, and then for a fraction of them to be wrong, then to just kind of, you know,
link |
01:47:10.480
make incremental progress all your life, right? Speaking of wild ideas, let me ask you about
link |
01:47:16.800
the thing we mentioned previously, which is this interstellar object a more and more.
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01:47:22.640
Could it be space junk from a distant alien civilization?
link |
01:47:26.160
You can't immediately discount that by saying absolutely it cannot. Anything can be space
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01:47:34.720
junk. I mean, from that point of view, can any of the Kuiper Belt objects we see be space junk?
link |
01:47:40.800
Anything on the night sky can in principle be space junk.
link |
01:47:44.640
And Kuiper Belt would catch interstellar objects potentially and like,
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01:47:48.960
force them into an orbit if they're like small enough?
link |
01:47:51.840
Not the Kuiper Belt itself, but you can imagine like Jupiter family comments
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01:47:55.760
being captured, you know, so you can actually capture things. It's even easier to do this very
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01:48:02.720
early in the solar system. Like early in the solar system's life, while it's still in a cluster of
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01:48:07.200
stars, it's unavoidable that you capture debris, whether it be natural debris or unnatural debris,
link |
01:48:15.840
or just debris of some kind from other stars. That it's like a daycare center, right? Like
link |
01:48:22.480
everybody passes their infections on to other kids. Yeah. You know, one more,
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01:48:27.600
one more. There's been a lot of discussion about it. There's been a lot of interest in this over,
link |
01:48:33.520
is it aliens or is it not? But let's like, if you just kind of look at the facts,
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01:48:37.680
like what we know about it is it's kind of like a weird shape and it also accelerated,
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01:48:43.840
you know, right? Like that's the two, those are the two interesting things about it.
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01:48:50.560
There are puzzles about it and perhaps the most daring resolution to this puzzle is that
link |
01:49:02.160
it's not, you know, aliens or it's not like a rock, it's actually a piece of hydrogen ice.
link |
01:49:08.560
So this is a friend of mine, you know, Daryl Seligman, Greg Laughlin came up with this idea
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01:49:15.520
that in giant molecular clouds that are just clouds of hydrogen helium gas that live in,
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01:49:24.720
live throughout the galaxy at their cores, you can condense ice to become the hydrogen,
link |
01:49:31.440
you know, icebergs, if you will. And then that explains many of the aspects of,
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01:49:37.920
in fact, I think that explains all of the more mystery how it becomes elongated because basically
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01:49:46.320
the hydrogen ice sublimates and kind of like a bar of soap that, you know, slowly kind of elongates
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01:49:53.200
as you, as you strip away the surface layers, how it was able to accelerate because of a jet
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01:50:01.760
that is produced from, you know, the hydrogen coming off of it, but you can't see it because
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01:50:05.600
it's hydrogen gas, like all of this stuff kind of falls together nicely. I'm intrigued by that
link |
01:50:13.680
idea truly because it's like, if that's true, that's a new type of astrophysical object.
link |
01:50:21.040
And it would be produced by what's the monster that produced it initially, that kind of object.
link |
01:50:27.120
So this is giant molecular, molecular clouds, they're everywhere. I mean, they are,
link |
01:50:30.960
the fact that they exist is not... Are they rogue clouds or are they part of like an
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01:50:36.800
oar cloud? No, no, no, they're rogue clouds. They're just floating about. Yeah. So if you go,
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01:50:41.600
like, a lot of people imagine the galaxy as being a, you know, a bunch of stars, right? And
link |
01:50:48.720
they're just orbiting, right? But the truth is, if you fly between stars, you run into clouds.
link |
01:50:55.040
They don't have any large object that creates orbits, they're just floating about.
link |
01:50:59.200
Just floating? But why are they floating together? Are they just float together for time and not?
link |
01:51:03.840
Well, so these are the, these eventually become the nurseries of stars. So as they, as they cool,
link |
01:51:10.480
they contract and, you know, then collapse into stars or into groups of stars. But some of them,
link |
01:51:17.520
the starless molecular clouds, according to the calculations that Daryl and Greg did, can
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01:51:26.160
then, can create these like icicles of hydrogen ice. I wonder why they would be flying so fast,
link |
01:51:33.840
because they seem to be moving pretty fast at a quick pace.
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01:51:36.160
You mean, one more?
link |
01:51:36.960
One more, yeah.
link |
01:51:38.160
That's just because of their acceleration due to, due to the sun. If you stop, I mean, it's like,
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01:51:44.560
take something really far away, let it go, and the sun is here. By the time it comes close to the
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01:51:49.600
sun, right, it's moving pretty fast. So that's an attractive explanation, I think, not so much,
link |
01:51:56.640
because it's cool, but it makes a clear prediction, right, of when Verrubin Observatory comes online
link |
01:52:05.040
next year or so, we will discover many, many more of these objects, right? And they have,
link |
01:52:12.800
so I like, I like theories that are falsifiable and not just testable, but falsifiable. It's
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01:52:19.360
good to have a falsifiable theory where you can say, that's not true. Aliens is one that's
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01:52:26.480
fundamentally difficult to say, no, that's not aliens.
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01:52:29.920
Well, the interesting thing to me, if you look at one alien civilization,
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01:52:35.280
and then we look at the things it produces, in terms of if we were to try to detect the alien
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01:52:40.160
civilization, there is like, say there's 10 billion aliens, there would probably be
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01:52:52.560
trillions of dumb drone type things produced by the aliens, and then be many, many, many
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01:53:00.480
more orders of magnitude of junk. So like, if you were to look for an alien civilization,
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01:53:06.640
in my mind, you would be looking for the junk. That's the more efficient thing to look for.
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01:53:12.080
So I'm not saying Amua Amua has any characteristics of space junk, but it kind of opened my eyes,
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01:53:18.880
to the idea that we shouldn't necessarily be looking to the queen of the ant colony. We
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01:53:25.440
should be looking at, I don't know, I don't know, like the traces of alien life that doesn't
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01:53:31.760
look intelligent in any way, may not even look like life. It could be just garbage. We should be
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01:53:36.560
looking for garbage. Just generically. Garbage that's producible by unnatural forces. I mean,
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01:53:47.200
for me, at least that was kind of interesting, because if you have a successful alien civilization
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01:53:52.880
that we would be producing many more orders of magnitude of junk, and that would be easier
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01:53:57.120
potentially to detect. Well, so you have to produce the junk, but you have to also launch it.
link |
01:54:02.080
So this is the, this is where let's, let's imagine, disposal. Yeah. But let's imagine we are a
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01:54:09.680
successful civilization that, you know, has made it to space. We clearly have, right? And yes,
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01:54:15.920
we're in the infancy of that pursuit. But, you know, we've launched, I don't know how many satellites.
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01:54:23.520
Probably if you count GPS satellites, it must be at least thousands.
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01:54:28.720
It's certainly thousands. I don't know if it's over 10,000, but it's on that order.
link |
01:54:32.320
But it's on that, like a large order of magnitude. How many of the things that we've launched
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01:54:37.680
will ever leave the solar system? I think two.
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01:54:41.040
Two so far. Well, maybe the Voyager, the Voyager 1, Voyager 2. I don't know if the Pioneer.
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01:54:46.640
So maybe three, like. Oh, there's also a Tesla Roadster out there.
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01:54:51.440
That one, it will never leave the solar system. It'll just, I think that one will
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01:54:55.360
eventually collide with Mars. That can be SpaceX's first Mars.
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01:55:02.240
But look, so there is an energetic cost to interstellar travel, which is really hard to
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01:55:08.560
overcome. And when we think about, you know, generically, what do we look for in an alien
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01:55:14.240
civilization? Oftentimes, we tend to imagine that the thing you look for is the thing that we're
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01:55:19.680
doing right now, right? So I think that, you know, if I look at the future, right, and for a while,
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01:55:27.520
like, okay, if aliens are out there, they must be broadcasting in radio, right? That radio,
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01:55:35.440
you know, the amount that we broadcast in radio has diminished tremendously in the last 50 years.
link |
01:55:42.800
But we're doing a lot more computation, right? What are the signs of computation? Like,
link |
01:55:49.280
that's a good, that's an interesting question to ask, right? Where, I don't know, I think
link |
01:55:54.800
something on the order of a few percent of the entire electrical grid last year went to mining
link |
01:56:01.280
Bitcoin, right? Well, there could be a lot of, in the future, different consequences of the
link |
01:56:08.960
computation, which I mean, I'm biased, but it could be robotics. It could be artificial intelligence.
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01:56:14.560
So we may be looking for intelligent looking objects, like that's what I meant by probes,
link |
01:56:22.320
like things that move in kind of artificial ways.
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01:56:25.200
But the emergence of AI is not an if, right? It's happening right in front of our eyes.
link |
01:56:33.360
And the energetic costs associated with that are becoming, you know, a tangible problem.
link |
01:56:39.600
So I think, you know, if you imagine kind of extrapolating that into the future, right,
link |
01:56:45.440
what are the, you know, what becomes the bottleneck, right? The bottleneck might be
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01:56:53.120
powering, you know, powering the AI, broadly speaking, not one AI, but powering that entire
link |
01:56:58.960
AI ecosystem, right? So I don't know. I think, you know, space junk is kind of,
link |
01:57:05.760
it's an interesting idea, but it's heavily influenced by like sci fi of 1950s, where by 2020,
link |
01:57:13.760
we're all like, flying to the moon. And so we produce a lot of space junk. I'm not
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01:57:21.040
sure if that's the pathway that alien civilizations take. I've also never seen an alien civilization.
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01:57:27.840
That's true. But if your theory of chill turns out to be true, and then we don't,
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01:57:35.440
you know, we don't necessarily explore, we seize the exploration phase of like alien civilizations
link |
01:57:41.360
quickly sees the exploration phase of their efforts, then perhaps they'll just be chilling
link |
01:57:50.240
in a particular space, expanding slowly, but then using up a lot of resources and then have to
link |
01:57:56.400
have a lot of garbage disposal that sends stuff out. And the other, you know, the other idea was
link |
01:58:02.480
that it could be a relay that you'll almost have like these GPS like markers, these sent throughout,
link |
01:58:10.400
which I think is kind of interesting. It's similar to this probe idea of sending
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01:58:17.440
a large number of probes out to measure gravitational,
link |
01:58:23.520
to measure basically, yeah, the gravitational field, essentially. I mean, a lot of people
link |
01:58:28.960
at Caltech or in MIT are trying to measure gravitational fields. And there's, there's a
link |
01:58:34.640
lot of ideas of sending stuff out there that accurately measures those gravitational fields
link |
01:58:42.880
to have a greater understanding of the early universe. But then you might realize that
link |
01:58:48.880
communication through gravitation through gravity is actually much more effective than
link |
01:58:53.600
than radio waves, for example, something like that. And then you send out, I mean, okay, if you're
link |
01:58:59.440
an alien civilization that's able to have gigantic masses, like basically, we're getting there as a
link |
01:59:08.160
civilization. No, we're not not even close. Well, I mean, I mean, like be able to sort of
link |
01:59:16.720
play with black holes, that kind of thing. So we're talking about a whole another different
link |
01:59:20.720
order of magnitude of masses, then it may be very effective to send signals via gravitational waves.
link |
01:59:26.880
I actually, my sense is that all of these things are genuinely difficult to predict.
link |
01:59:33.680
And I don't mean like to kind of shy away. I just, I really mean, if you think, if you take
link |
01:59:40.560
imagination of what the future looked like from 500 years ago, right, it's just,
link |
01:59:47.040
it is so hard to conceive of the impossible. So it's almost like, it's almost limiting to try and
link |
01:59:56.960
imagine things that are an order of magnitude, or two orders of magnitude ahead in terms of
link |
02:00:02.960
progress, just because you mentioned cars before, if you were to ask people what they wanted in
link |
02:00:11.120
1870, it's faster buggies. So I think the whole kind of alien conversation inevitably gets limited
link |
02:00:22.880
by our entire kind of collective astrophysical lack of imagination.
link |
02:00:29.360
So to push back a little bit, I find that it's really interesting to talk about these wild ideas
link |
02:00:37.520
about the future, whether it's aliens, whether it's AI, with brilliant people like yourself,
link |
02:00:43.840
who are focused on very particular tools of science we have today to solve very particular
link |
02:00:48.960
like rigorous scientific questions. And it's almost like putting on this wild dreamy hat,
link |
02:00:54.160
like some percent of the time and say, like, what are like, what would alien civilizations
link |
02:00:58.640
look like? What would alien trash look like? Well, what would our own civilization that
link |
02:01:04.720
sends out trillions of AI systems out there, like how 9000, but 10,000 out there, what would
link |
02:01:11.040
that look like? And you're right, any one prediction is probably going to be horrendously
link |
02:01:16.080
wrong, but there's something about creating these kind of wild predictions that kind of opens up.
link |
02:01:22.960
No, there's a huge magnetism to it, right? And some of it,
link |
02:01:26.480
you know, I mean, some of the Jules Verne novels did a phenomenal job predicting the
link |
02:01:36.400
future, right? That actually was a great example of what you're talking about,
link |
02:01:40.960
like allowing your imagination to run free. I mean, I just hope, I just hope there's dragons.
link |
02:01:48.880
That's, I love dragons. Yeah, dragons are the best.
link |
02:01:52.560
But see, the cool thing about science fiction and these kinds of conversation,
link |
02:01:58.480
it doesn't just predict the future, I think. Some of these things will create the future.
link |
02:02:05.440
Planting the idea. The humans are amazing, like fake it till you make it.
link |
02:02:12.320
Humans are really good at taking an idea that seems impossible at the time. And for
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02:02:18.880
any one individual human, that idea is like planting a seed that eventually materializes
link |
02:02:25.920
itself. It's weird. It's weird how science fiction can create science fiction.
link |
02:02:30.400
And drive some of these. It drives the science.
link |
02:02:32.320
Yeah, I agree with you. And I think in this regard, I'm like a sucker for sci fi.
link |
02:02:40.880
It's all I listen to now when I run. And some of it is completely implausible,
link |
02:02:49.840
right? And it's like, I don't care. It's both entertaining and it's just like
link |
02:03:00.000
its imagination. You know about The Black Clouds book? I think it's by Fred Hoyle.
link |
02:03:05.280
This has great connections with a lot of the advancements that are happening in NLP right now
link |
02:03:13.440
with transformer models and so on. But it's just Black Cloud shows up in the solar system.
link |
02:03:19.920
And then people try to send, and then it learns to talk back at you. So anyway,
link |
02:03:26.560
we don't have to talk at all about it, but it's just something worth checking out.
link |
02:03:30.880
With that on the alien front with The Black Cloud, to me, and the exact on the NLP front,
link |
02:03:36.400
and also just explainability of AI, it's fascinating. Just a very question. Stephen
link |
02:03:41.520
Wolfram looked at this with the movie Arrival. It's like, what would be the common language
link |
02:03:46.000
that we would discover? The reason that's really interesting to me is we have aliens here on Earth.
link |
02:03:51.200
Japanese. Japanese is the obvious answer. Japanese. Yeah, that would be the common.
link |
02:03:56.240
And maybe it would be music, actually. That's more likely. It wouldn't be language. It would be
link |
02:04:02.160
art that they would communicate. But I do believe that we have,
link |
02:04:07.200
I'm with Stephen Wolfram on this a little bit, that to me, computation, like programs we write,
link |
02:04:15.680
that they're kind of intelligent creatures. And I feel like we haven't found the common
link |
02:04:19.600
language to talk with them. Like our little creations that are artificial are not born
link |
02:04:27.120
with whatever that innate thing that produces language with us. And coming up with mechanisms
link |
02:04:33.760
for communicating with them is an effort that feels like it will produce some incredible
link |
02:04:41.840
discoveries. You can even think of, if you think that math has discovered, mathematics in itself
link |
02:04:47.520
is a kind of... Oh yeah, it's an innate construction of the world we live in. I think we are
link |
02:04:57.200
part of the way there because pre 1950, computers were human beings that would carry out arithmetic.
link |
02:05:08.800
And I think it was Ulam who worked in Los Alamos at the time, like towards the end of
link |
02:05:16.640
the Second World War, wrote something about how in the future computers will not be
link |
02:05:25.200
just arithmetic tool, but will be truly an interactive thing with which you could do
link |
02:05:33.200
experiments. At the time, the notion of doing an experiment, not like in the lab with some
link |
02:05:38.640
beakers, but an experiment on a computer designing a miracle experiment was a new one.
link |
02:05:50.160
70% of what I do is I write code, terrible code to be clear, but I write code that creates
link |
02:06:00.880
an experiment which is a simulation. So in that sense, I think we're beginning to interact with
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02:06:07.600
the computer in a way that you're saying, not as just a fancy calculator, not as just a call
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02:06:14.800
and request type of thing, but something that can generate insights that are otherwise completely
link |
02:06:25.120
unattainable. They're unattainable by doing analytical mathematics. Yeah, and there's with
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02:06:31.280
AlphaFol2, we're now starting to crack open biology, so being able to simulate at first
link |
02:06:38.480
trivial biological systems and hopefully down the line complex biological systems,
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02:06:43.040
my hope is to be able to simulate psychological, like sociological systems like humans. A large
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02:06:51.840
part of my work at MIT was on autonomous vehicles, and the fascinating thing to me was about
link |
02:06:57.840
pedestrians, human pedestrians interacting with autonomous vehicles and simulating those systems
link |
02:07:03.760
without murdering humans will be very useful, but nevertheless is exceptionally difficult.
link |
02:07:09.600
When is my Mustang going to drive itself? I'm not even joking. It turns out it's much more
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02:07:19.760
difficult than we imagined, and I suppose that's the kind of the progress of science
link |
02:07:27.440
is just like going to Mars. It's probably going to turn out to be way more difficult than we
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02:07:34.480
imagined. Sending out probes to investigate planet nine at the edge of our solar system
link |
02:07:39.360
might turn out to be way more difficult than we imagined, but we do it anyway, and we figured
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02:07:43.440
out in the end. Mars is great. Sending humans to Mars is way more complicated than sending
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02:07:50.400
humans to the moon. You'd think just naively, but if they're in space, who cares? If you go there,
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02:07:57.200
why don't you go there? Life support is an extremely expensive thing.
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02:08:05.120
There's a bunch of extra challenges, but I disagree with you. I would be one of the
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02:08:08.800
early people to go. I used to think not. I used to think I'd be one of the first maybe million
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02:08:13.520
to go once you have a little bit of a society. I think I'm upgrading myself to the first like
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02:08:18.240
$10,000. That's right, front of the cabin. Not completely front, but it would be interesting
link |
02:08:24.960
to die. I'm okay with death sucks, but I like the idea of dying on Mars. Of all the places to die,
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02:08:35.840
I've got to say in this regard, I don't want to die on Mars. I don't. No, no, I would much rather
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02:08:42.320
die on Earth. Death is fundamentally boring. Death is a very boring experience. I've never
link |
02:08:51.440
died before, so I don't know from first hand experience. As far as you know. It could be a
link |
02:08:55.840
reincarnation, all those kinds of things. You mean where would you die if you had to choose?
link |
02:09:02.320
Oh, man. Okay. There's a question of who I'd want to die with. I'd prefer not to die alone,
link |
02:09:15.120
but surrounded by family would be preferable, where I think northern New Mexico, and I'm not
link |
02:09:24.640
even joking. This is not a random place. Would that be your favorite place on Earth?
link |
02:09:29.840
Not necessarily, favorite place on Earth to reside indefinitely, but it is one of the most
link |
02:09:40.160
beautiful places I've ever been to. There's something attractive about going.
link |
02:09:49.760
Returning to nature in a beautiful place. Let me ask you about another aspect of your life
link |
02:09:57.360
that is full of beauty. Music. Okay. You're a musician. The absurd question I have to ask,
link |
02:10:05.200
what is the greatest song of all time? Objectively speaking. The greatest song of all time.
link |
02:10:10.800
I suppose that could change moment to moment, day to day, but if you were forced to answer for
link |
02:10:16.160
this particular moment in your life, that's something that pops to mind. This could be
link |
02:10:20.800
both philosophically, this could be technically as a musician, like what you enjoy, maybe lyrics.
link |
02:10:25.360
Like for me, lyrics is very important, so I would probably, my choice would be lyrics based.
link |
02:10:32.480
I don't want to answer in terms of just technical prowess. I think technical prowess is impressive.
link |
02:10:42.400
It's impressive what can be done. I wouldn't place that into the category of the greatest
link |
02:10:47.280
music ever written. Some classical music that's written is undeniably beautiful, but I don't
link |
02:10:55.520
want to consider that category of music either just because, so if I was to limit the scope of
link |
02:11:06.000
this philosophical discussion to the kind of music that I listen to, probably What's My Age Again
link |
02:11:14.560
by Blink One and Two, it's just, it's a solid one. It's got, you know.
link |
02:11:21.440
Said nobody ever. That's a good song. I don't even know if you're joking.
link |
02:11:26.080
No, no, I am joking. It's a good one, but it's, yeah, I mean.
link |
02:11:29.920
Oh, I think the back is a close second.
link |
02:11:34.960
What's my age again? Oh, yeah.
link |
02:11:37.840
No, I mean, it would probably, you know, songwriting wise, I think the Beatles came pretty close to.
link |
02:11:44.960
Would they influential to you? Absolutely.
link |
02:11:46.560
I was like the Beatles.
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02:11:47.600
Yeah. Love the Beatles. I love the Beatles.
link |
02:11:50.960
Would it be yesterday?
link |
02:11:53.600
Yeah.
link |
02:11:53.920
Like, I think Strawberry Fields Forever is one of, you know what one of my favorite Beatles songs is?
link |
02:12:00.000
It's, you know, In My Life, right? That song. It's hard to imagine how whatever a 24 year old
link |
02:12:07.680
wrote that. It is one of the most introspective pieces of music ever. You know, I'm a huge Pink Floyd
link |
02:12:16.480
fan. And so I think, you know, if you were to, you can sort of look at the entire dark side of the
link |
02:12:22.400
moon album and as, you know, getting pretty close up there to the pinnacle of what, you know, can be
link |
02:12:29.680
created. So, you know, Time's a great song. Yeah. It's a great song.
link |
02:12:34.720
Just the entirety of just the instruments, the lyrics, the feeling created by a song,
link |
02:12:42.080
like Pink Floyd can create feelings, the entire experience. I mean, you have that with the wall
link |
02:12:49.120
of just transporting you into another place. Songs don't, not many songs could do that as well.
link |
02:12:57.920
Not many artists can do that as well as Pink Floyd did.
link |
02:13:00.400
There are a lot of bands that you can kind of say, oh yeah, like if you take Blink 182, right?
link |
02:13:07.120
If you have no idea, like if you are listening to sort of that type of pop punk for the first time,
link |
02:13:14.160
it's difficult to differentiate between Blink 182 and like some 41 and the
link |
02:13:19.600
thousand of other like lesser known bands that all sounded, they all had that sparkling production
link |
02:13:25.760
feel. They all kind of sounded the same, right? With Pink Floyd, it's hard to find another band
link |
02:13:35.360
that you're like, well, is this one Pink Floyd? Like you know when you're listening to Pink Floyd,
link |
02:13:41.440
when you're listening to. The uniqueness, that's fascinating. You know, in the calculation
link |
02:13:47.440
of the greatest song in the greatest band of all time, you could probably, you could probably
link |
02:13:53.120
actually quantify this like scientifically, is like how unique, if you play different songs,
link |
02:13:59.840
how well are people able to recognize whether it's this band or not? And that, you know,
link |
02:14:04.160
that's probably a huge component to greatness. Like if the world would miss it if it was gone.
link |
02:14:10.400
Yes, yes. But there's also the human story, things like I would say Output Johnny Cash's
link |
02:14:17.040
cover of Hurt is one of the greatest songs of all time. And that has less to do with the song.
link |
02:14:24.400
But your interaction with it?
link |
02:14:25.920
The interaction with it, but also the human, the full story of the human. So like it's not just
link |
02:14:30.880
if I just heard the song and be like, okay, that, but if it's the full story of it, also the video
link |
02:14:37.520
component for that particular song. So like that, you can't discount the full experience of it.
link |
02:14:43.920
Absolutely. You know, I have no confusion about not about being, you know, anywhere,
link |
02:14:51.200
you know, in that link. But I just like, I sometimes think about, you know, music that is
link |
02:14:57.360
being produced today feels oftentimes feels like, like kind of clothes, like clothes that you buy
link |
02:15:06.000
at like H&M and you wear it three times before they rip and you throw away. So like, so much of it
link |
02:15:14.400
is, it's not bad. It's just kind of forgettable, right? Like the fact that we're talking about Pink
link |
02:15:20.880
Floyd in 2021 is in itself an interesting question. Why are we talking about Pink Floyd?
link |
02:15:27.920
And it's, there's something unforgettable about them and unforgettable about the art that they
link |
02:15:33.200
created. That could be the markets that like, so Spotify has created this kind of market where
link |
02:15:40.000
the incentives for creating music that last is much lower because there's so much more music.
link |
02:15:46.240
You just want something that shines bright for a short amount of time, makes a lot of money and
link |
02:15:51.120
moves on. And I mean, the same thing you see with the news and all those kinds of things. We're
link |
02:15:54.880
just living in a shorter and shorter, shorter like time scale in terms of our attention spans.
link |
02:16:01.600
And that nevertheless, when we look at the long arc of history of music, perhaps there will be
link |
02:16:07.360
some songs from today that will last as much as Pink Floyd. We're just unable to see it.
link |
02:16:13.120
Yeah. Just the collected works of Nickelback. Exactly. You never know. You never know. Justin
link |
02:16:18.880
Bieber, it could be a contender. I've recently started listening to Justin Bieber just to
link |
02:16:23.360
understand what people are talking about. And I'll just keep my comments to myself on that one.
link |
02:16:27.840
It's too good to explain. The words cannot capture the greatness that is the Bebes.
link |
02:16:35.520
You as a musician, so you write your music, you play guitar, you sing. Maybe can you give
link |
02:16:45.600
an overview of the role music has played in your life? You're one of the, you're a world class
link |
02:16:51.120
scientist. And so it's kind of fascinating to see somebody in your position who is also a great
link |
02:17:00.720
musician and still loves playing music. Yeah. Well, I wouldn't call myself a great musician.
link |
02:17:07.120
One of the best of all time. That's right. We were saying offline confidence is like the most
link |
02:17:14.640
essential thing about being a rock star. Exactly. The confidence and kind of like moodiness, right?
link |
02:17:21.520
Yeah. Look, I mean, music plays an absolutely essential role in everything I do because I lose,
link |
02:17:30.960
if I stop playing for one reason or another, say I'm traveling, I notably lose creativity in
link |
02:17:38.640
every other aspect of my life, right? There's something, I don't view playing music as a
link |
02:17:47.360
separate endeavor from doing science or doing whatever. It's all part of that same creative
link |
02:17:53.760
thing, which is distinct from, I don't know, pressing a button or like. So it's not a break
link |
02:18:03.520
from science. It's a part of your science. It's absolutely, it's a part of, I would say,
link |
02:18:10.000
it's a thing that enables the science, right? The science would suck even more than it does
link |
02:18:16.800
already without the music. And that means like the creating of the writing of the music or is it
link |
02:18:22.320
just even playing other people's stuff? Is it the whole of it? Yeah. It's definitely both.
link |
02:18:27.600
Yeah. And also just, I love to play guitar. I love to sing. My wife tolerates my
link |
02:18:40.400
screeching singing and even kind of likes it. Yeah. So people should check out your stuff.
link |
02:18:46.560
You have a great voice. So I love your stuff. Is there something you're super busy?
link |
02:18:52.080
Is there something you can say about practicing for musicians, for guitar, for you're also in a
link |
02:19:00.080
band? So like that whole, how you can manage that? Is there some tricks or some hacks to
link |
02:19:07.360
being a lifelong musician while being like super busy? So I would say, you know,
link |
02:19:13.760
the way that I optimize my life is I try to do the thing that I'm passionate about
link |
02:19:21.520
in a moment and put that at the top of the priority list. There are moments when, you know,
link |
02:19:27.760
you just, you feel inspired to play music. And if you're in the middle of something,
link |
02:19:31.600
if you can avoid, if that can be put on hold, just do it, right? There are times when you
link |
02:19:36.640
get inspired about something scientific, you know, I do my best to drop everything, go into that,
link |
02:19:45.040
you know, mode of, or that isolated mode and execute upon that. So it's a chaotic, you know,
link |
02:19:53.440
I think I have a pretty chaotic lifestyle where I'm always doing kind of multiple things and
link |
02:19:59.040
jumping between what I'm doing. But at the end of the day, it's not like, you know, those moments
link |
02:20:10.560
of inspiration are actually kind of rare, right? Like most of the time, all of us are just doing
link |
02:20:18.640
kind of doing the stuff that needs to get done. If you do the disservice to yourself of saying,
link |
02:20:26.320
oh, I'm inspired to, you know, do this calculation, figure this out. But I've got to answer email
link |
02:20:32.720
or just like do something, something silly. You know, that is a, that is nothing more than the
link |
02:20:40.240
service. And also, like I have some social media presence, but I mostly stay off of, you know,
link |
02:20:48.080
social media to, you know, just frankly, because like, I don't kind of, I don't enjoy the mental
link |
02:20:55.440
cycles that it. Yeah, it robs you of that. Yeah, those, those precious moments that could be filled
link |
02:21:03.760
with inspiration in your, in your other pursuits. But there's something to maybe you and I are
link |
02:21:10.400
different in this, like I tried to play at least 10 minutes of guitar every day, almost on the
link |
02:21:17.520
technical side, like keeping that base of basic competence going. And I mean, the same way like
link |
02:21:28.640
writers will get in front of a paper, no matter what, that kind of thing. It just feels like that
link |
02:21:35.040
for my life has been essential to the daily ritual of it. Otherwise, days turn into weeks,
link |
02:21:42.000
weeks turn into months and you haven't played guitar for months. No, no, I understand. For me,
link |
02:21:48.160
I think it's, it's been like, if we have a gig coming up, we'll definitely. You need deadlines.
link |
02:21:53.840
Yeah, that's right. No, like we will, we will sharpen up definitely, you know, especially
link |
02:22:02.080
coming up to a gig. And it's like, you know, we're not trying to make money with this. This is like
link |
02:22:07.200
just for the, for that satisfaction of doing something and doing something well, right?
link |
02:22:15.040
But overall, I would say most, I play guitar most days, most days. And, you know, when I
link |
02:22:24.560
put kids to sleep, I play guitar, you know, with them and we like, just make up random songs about,
link |
02:22:31.680
you know, about our cat or something, you know, like we just do kind of random stuff.
link |
02:22:38.720
But, you know, music is always involved in that process.
link |
02:22:42.000
Keeping it fun. You have Russian roots?
link |
02:22:44.320
I sure do.
link |
02:22:45.360
Were you born in Russia?
link |
02:22:46.400
I was.
link |
02:22:47.120
Yeah.
link |
02:22:47.680
When did you come here?
link |
02:22:49.120
So, I came to the US in very, the very end of 99, but so I was like almost 14 years old.
link |
02:22:59.520
But along the way, we spent six years in Japan. So, like we moved from Russia to Japan in 94.
link |
02:23:07.760
And then to the US in 99. So, like elementary school.
link |
02:23:12.000
Oh, interesting.
link |
02:23:12.640
School in Japan.
link |
02:23:13.520
So, elementary school in Japan.
link |
02:23:16.160
Yeah.
link |
02:23:17.680
So, that's interesting. Do you still speak Russian?
link |
02:23:20.560
Sure.
link |
02:23:21.360
Okay.
link |
02:23:21.680
Okay. Maybe I'll, let me ask you in Russian, what do you remember about Russia?
link |
02:23:31.440
It'd be interesting to hear you speak Russian.
link |
02:23:33.440
Well, in general, I remember, I mean, I was eight when we left. And, of course, I remember everything in the first year, including the transition from 1991 to 1992, this turbulent period, and, of course, 1993.
link |
02:23:58.000
I mean, I still remember very well how, at some point, Pepsi Cola appeared first, and then Coca Cola appeared, and then, I remember, I was, I don't know, six years old, and then I thought, how can it be that Coca Cola stole the product and did the same thing?
link |
02:24:18.560
So, for people who don't speak Russian, Constantine was talking about basically his first in 1992 interaction with capitalism, which is Pepsi, and at first he discovered Pepsi, and then he discovered Coke, and he was confused how such theft could occur.
link |
02:24:48.480
Yeah, like an intellectual property theft. And remember, Pepsi arrived to the Soviet Union first, and there was some, there's some complicated story, which I don't quite understand the details of, for a while, Pepsi, like, commanded submarines or something.
link |
02:25:05.920
Yeah, Pepsi had like a fleet of Soviet submarines that it was.
link |
02:25:10.000
It was sponsoring tanks and this fessing, and I remember, there's certain things that trickled in, like McDonald's, I remember that was a big deal, certain aspects of the West.
link |
02:25:20.560
Absolutely, so, I mean, we went to McDonald's, and we stood, I mean, this is absurd, right, from kind of looking at it from today's perspective, but we stood in line for like six hours to get into this McDonald's, and, you know, I remember inside, it was just like,
link |
02:25:39.280
a billion people, and I'm just taking a bite out of that Big Mac, and I'm like, wow.
link |
02:25:46.640
What was it, an incredible experience for you? So, like, what is the taste of the West, like, did you enjoy it?
link |
02:25:53.280
I enjoyed the fact that, I mean, this is like, this is getting into the weeds, but I really enjoyed the fact that the top of the bun had those seeds, you know, like, and I remember how on the commercials, like, the Big Mac would kind of bounce.
link |
02:26:09.200
And I was like, the seeds, how do they inject the seeds into the bread, like, amazing, right? So, I think it was, uh, artistry.
link |
02:26:18.480
Yeah, you enjoyed the artistry of the culinary experience.
link |
02:26:21.280
Exactly, it was the, you know, it was the food art, that is the Big Mac.
link |
02:26:25.840
Actually, I still don't know the answer to that, how do they get the sesame seeds on the bun?
link |
02:26:28.800
It's better to not know the answer.
link |
02:26:31.360
You just wander the mystery of it all, yeah, I remember it being exceptionally delicious, but I'm with you, I don't know, you didn't,
link |
02:26:39.120
I mentioned how transformative Pepsi was, but to me, basically sugar based stuff, like Pepsi was, or Coke, I don't remember which one we partook in, but that was an incredible experience.
link |
02:26:50.880
Yeah, yeah, yeah, yeah, no, absolutely. And, you know, I think it's, you know, it was an important and formative period.
link |
02:27:03.200
I sometimes, I guess, rely on that a little bit, you know, in my daily life, because I remember, like, the early 90s were real rough, you know, like, my parents were kind of on the, on the bottom of the spectrum in terms of, you know, in terms of financial well being.
link |
02:27:26.400
So, kind of like, just when I run into trouble, not like, you know, money trouble, just any kind of trouble these days, it just kind of is not particularly meaningful when you compare it to that, that turbulent time of the early 90s.
link |
02:27:45.360
And the other thing is, I think there's, there's like an advantage to, to being, you know, an immigrant, which is that you get, you go through the mental exercise of changing your environment completely early in your life, right?
link |
02:28:00.640
You go, it's by no means, you know, pleasant in the moment, right? But, like, going into Japanese elementary school, right? Like, I didn't go to some, like, private, you know, thing. I just went to a regular, like, Japanese public elementary school, and that was the non Japanese person in my class.
link |
02:28:22.640
So, just like the learning Japanese and just kind of. So, that's a super humbling experience in many ways was when you, like, made fun of all that kind of stuff. Oh, yeah. Being the outsider.
link |
02:28:32.960
Oh, absolutely. But, you know, you kind of do, you kind of do that. And then you kind of, then you're just kind of are okay with, with stuff, you know what I mean?
link |
02:28:44.240
And so, like, doing that again in middle school in the US, it was arguably easy because it was like, yeah, well, I've already done this before. So, I think it kind of prepares you mentally a little bit for, for switching up for whatever, you know, changes that will come up for the rest of, of your life.
link |
02:29:02.240
So, I wouldn't trade that, that experience really for anything. It's a huge aspect of, of who I am. And I'm sure you can relate to a lot of this.
link |
02:29:14.800
Yes. Is there advice from your life that you can give to young people today, high school, college, you know, about their career, or maybe about life in general?
link |
02:29:26.720
I'm not like a career coach by life coach, right? Like, I'm definitely not a life coach. I don't have it all figured out. But I think there's a, there's a perpetual cycle of, you know, thinking that there is a, there's kind of like a template for success, right?
link |
02:29:48.640
Maybe there is, but in my experience, I haven't seen it, right? You know, I would say people in high school, right? So much of their focus is on getting straight A's, filling their CV with this and this and this.
link |
02:30:07.520
So that, it looks impressive, right? That, that is not, I think, a good way to optimize your life, right? Do the thing that fills your life with passion. Do the thing that fills your life with, with interest and, you know, do that perpetually, right?
link |
02:30:28.160
A straight A student, you know, is really impressive, but also, you know, somewhat boring, right? So, so I, I think, you know, injection of more of that kind of interest into, into the lives of young people would go a long way in, in just both upping their level of happiness and then just kind of ensuring that looking forward,
link |
02:30:55.120
they are not suffering from a, you know, perpetual condition of, oh, I have to satisfy these like, you know, check boxes to, to do well, right?
link |
02:31:04.800
Because you can lose yourself in that whole process for the rest of your life. But it's nice if it's possible, like Max Tecmark was exceptionally good at this at MIT, figure out how you can spend a small part of your percent of your efforts, such that your CV looks really impressive.
link |
02:31:21.520
Yeah, absolutely. There's no, like, without a doubt, like, that's, that's a baseline that you need to have.
link |
02:31:29.280
And then spend, so like, spend most of your time doing like amazing things you're passionate about, but such that it kind of like Planet Nine produces objects that, that feed your CV, like, slowly over time.
link |
02:31:45.280
So getting good grades in high school, maybe doing extracurricular activities or, or in terms of like, you know, for programmers that's producing code that you can show up on GitHub, like leaving traces, like, throughout your efforts such that your CV looks impressive to the rest of the world.
link |
02:32:02.720
In fact, I mean, this is somewhat along the lines of what I'm talking about. See, like, getting like good grades is important, but grades are not a tangible, like, product.
link |
02:32:14.160
Like, you cannot show your A and have your A live a separate life from you. Code very much does, right? Music very much takes on, you know, provided somebody else listens to it, right? Provide, like, takes on a life of its own.
link |
02:32:32.800
That's kind of what I mean, right? Doing, doing stuff that, that can then get separated from, from you is, is exceptionally attractive, right? It's like a, it's like a fun, and it's, and it's also very impressive to others.
link |
02:32:50.000
I think we're moving to a world where grades mean less and less, like certifications mean less and less. If you look at, especially again, in the computing fields, getting a degree, finishing your, currently just get it, finishing your degree, whether it's Bachelors or Masters of PhD is less important than the things you've actually put out into the world.
link |
02:33:10.320
Right, right. And that's a fascinating kind of, that's great that in that sense, the meritocracy in its richest, most beautiful form is, is starting to win out.
link |
02:33:20.720
Yeah, it's weird because like, you know, my understanding, and I'm not like, I don't know the history of science well enough to, to speak very confidently about this, but, you know, the advisor of my advisor of my advisor from undergrad, like, didn't have a PhD.
link |
02:33:39.440
Right, so I think it was a more common thing back in the day, even in the academic sector, to, you know, not have, you know, Faraday, like Faraday didn't know algebra, right, and drew diagrams about, you know, magnetic fields, like his Faraday's law was derived entirely from intuition.
link |
02:34:03.600
So, it is interesting to, to how the world of academia has evolved into a, you got to do this and then get PhD, then you have to postdoc once and twice and maybe thrice and then, like, you, you move on.
link |
02:34:18.640
So, you know, it does, I do wonder, you know, if we're, you know, if there's a better approach.
link |
02:34:25.440
I think we're heading there, but it's a fascinating historical perspective, like that we might have just tried this whole thing out for a while,
link |
02:34:32.720
where we put a lot more emphasis on grades and certificates and degrees and all those kinds of things.
link |
02:34:38.000
I think the difference historically is, like, we can actually, using the internet, show off the, show off ourselves and our creations better and better and more effectively,
link |
02:34:50.160
whether that's code or producing videos or all those kinds of things.
link |
02:34:53.840
That's right.
link |
02:34:54.640
It can become a certified drone pilot.
link |
02:34:56.320
Of all the things you want to pick, yeah, for sure.
link |
02:34:59.760
Or you could just fly and make YouTube videos against hundreds of thousands of views with your drone and never getting a certificate.
link |
02:35:06.080
That's probably illegal.
link |
02:35:07.600
Don't do it.
link |
02:35:08.480
What do you think is the meaning of this whole thing?
link |
02:35:11.200
So, you look at planets, they seem to orbit stuff without, without asking the why question.
link |
02:35:19.680
And for some reason, life emerged on earth such that it led to big brains that can ask the big why question.
link |
02:35:26.560
Do you think there's an answer to it?
link |
02:35:31.920
I'm not sure what the question is.
link |
02:35:33.280
Like, what do you think?
link |
02:35:34.080
Meaning of life?
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02:35:34.800
The meaning of life.
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02:35:37.040
It's 42.
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02:35:37.680
It's 42.
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02:35:38.640
Yeah.
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02:35:39.120
But, you know, aside from that, it's, you know, why, I think there is a big question.
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02:35:47.280
Why, I think if the question you're asking is like, why we do all this, right?
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02:35:54.640
Why we do all this.
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02:35:58.000
It's part of the human condition, right?
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02:36:00.400
Human beings are fundamentally, I feel like, non, like sort of stochastic and fundamentally interested in, in
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02:36:11.920
kind of expanding our own understanding of the world around us.
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02:36:19.200
And creating stuff to enable that understanding.
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02:36:22.800
So, we're like stochastic, fundamentally stochastic.
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02:36:25.200
So, like, there's just a bunch of randomness that really doesn't seem like it has a good explanation.
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02:36:30.160
And yet, there's a kind of direction to our being that we just keep wanting to create and to understand.
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02:36:35.600
That's right.
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02:36:36.240
So, we're, you know, that claim to be anti science, right?
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02:36:42.240
And yet, in their anti science, you know, discussion, like, well, like, if you're so, you know, scientific,
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02:36:51.360
then how, why don't you explain to me how, I don't know, this works.
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02:36:55.200
And like, it always, there's that fundamental seed of curiosity and interest that is common to all of us.
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02:37:03.760
Is absolutely what makes us human, right?
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02:37:07.200
And, and I'm in a privileged position of being able to, you know, to have that be my job, right?
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02:37:16.960
I think as, you know, as time evolves forward, you know, and the kind of economy changes,
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02:37:25.680
I mean, we're already starting to see, you know, a shift towards that type of, you know,
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02:37:30.400
creative, you know, enterprise as being, as merging, taking over a bigger and bigger chunk of the sector.
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02:37:38.880
It's not yet, I think, the dominant portion of the economy by any account.
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02:37:44.960
But if we compare this to like, you know, the time when the dominant thing you would do would be to,
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02:37:52.640
you know, go to a factory and do the same exact thing, right?
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02:37:57.120
I think, you know, there is a tide there and things are sort of headed in that direction.
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02:38:02.400
Yeah, life's becoming more and more fun.
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02:38:04.320
I can't wait, honestly, what happens next.
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02:38:06.640
You can't wait to just chill.
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02:38:08.080
Just chill.
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02:38:08.880
The terminal point of this is just chill and wait for those Kuiper Belt objects to complete one orbit.
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02:38:14.720
I'm going to credit you with this idea.
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02:38:17.120
I do hope that we definitively discover a proof that there is a Planet Nine out there in the next
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02:38:24.240
few years so you can sit back with a cigar, a cigarette, or vodka, or wine and just say,
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02:38:30.400
I told you so.
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02:38:31.840
That's already happening.
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02:38:33.680
I'm going to do that later today.
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02:38:36.320
As I mentioned, confidence is essential to being a rock star.
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02:38:40.320
I really appreciate you explaining so many fascinating things to me today.
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02:38:44.960
I really appreciate the work that you do out there.
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02:38:47.680
And I really appreciate you talking with me today.
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02:38:50.800
Thanks, Constantine.
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02:38:50.800
It was a pleasure.
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02:38:51.840
Thanks for having me on.
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02:38:52.800
Thanks for listening to this conversation with Constantine Batigan.
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02:38:56.800
And thank you to Squarespace, Literati, Onit, and NI.
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02:39:02.400
Check them out in the description to support this podcast.
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02:39:06.000
And now let me leave you with some words from Douglas Adams in the Hitchhiker's Guide to the
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02:39:10.240
Galaxy.
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02:39:12.000
Far out in the uncharted backwaters of the unfashionable end of the western spiral arm of the
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02:39:18.640
galaxy lies a small, unregarded yellow sun.
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02:39:23.680
Orbiting this at a distance of roughly 92 million miles is an utterly insignificant
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02:39:29.920
little blue green planet whose ape descendant life forms are so amazingly primitive that
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02:39:36.480
they still think digital watches are a pretty neat idea.
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02:39:41.600
Thank you for listening.
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02:39:42.640
I hope to see you next time.