Daniel and Kelly’s Extraordinary Universe - Could we see moons around exoplanets?

Episode Date: October 24, 2023

Daniel and Jorge are over the moon about the possibility of spotting alien moons.See omnystudio.com/listener for privacy information....

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Starting point is 00:02:07 have resources available for you at loveyourmind today.org. Hey, Daniel, do you ever worry about the ethics of using a telescope? What do you mean? What are the ethical questions about looking through a telescope? I mean, like, what you're looking at? Well, I'm not pointing them at my neighbor, if that's what you mean. Not your next door neighbor. What about your next galaxy neighbor?
Starting point is 00:02:35 Are you asking if we have the right to look at distant objects in the sky? Yeah, you know, like what if there are aliens there on a planet or a moon? And we're like spying on them. Well, I hope they're not offended if we catch them sunbathing, or I guess star bathing? Aren't all-stars suns? But yeah, don't you think aliens have a right to privacy? I don't know. Maybe they're alien celebrities.
Starting point is 00:02:56 so they're like starbathing stars. Wait, are you saying celebrities can't have privacy either? Are you secretly a stalker? No, I'm saying astronomers are just interstellar paparazzi. Well, uh, sounds like they need to draw their curtains more. Well, I just hope you don't get the rest of us punched in the face. Hi, I'm Jorge McCartunist and the author of Oliver's Great Big Universe. Hi, I'm Daniel. I'm a particle physicist and a professor at UC Irvine,
Starting point is 00:03:36 and if it gets the aliens to come, I want them to punch us in the face. Us in the face? How about just you in the face? I mean, please don't volunteer my face for your science. I was volunteering humanity's collective face. Some of us are sensitive in the face. It might be worth a puncher, too, to learn. we're not alone in the universe? Can we pick where they're going to punch us?
Starting point is 00:03:59 You know, like when you're playing as kids? You mean in the Daniel part of the face rather than the Jorge part of the face? Definitely the Daniel part. But anyways, welcome to our podcast, Daniel and Jorge, explain the universe, a production of iHeartRadio. In which we try to teach you all about the mysteries of the universe rather than punching you in the face with them. We think that is possible to gently absorb all of the crazy intricacies of how the universe
Starting point is 00:04:25 works from its tiny little particles to its mysterious swirling black holes without getting bruised basically anywhere on your body. We seek to serve up the mysteries of the universe in a gentle and comfortable manner. That's right. We bring you the one-two punch of science and bad dad jokes to talk about all the amazing things that are happening in the universe, all the peaceful things, and also all of the combative things. And the mysteries that we love to dig into are the ones that tell us about our context in the universe. Is where we are in the universe, weird and unusual or are there many such backyards with many such podcasts giving all the same dad jokes? Yeah, that is maybe one of the biggest questions in the universe is are we alone in the
Starting point is 00:05:07 universe or are we one of many, many alien civilizations out there in space? And are we the only ones making dad jokes? And how many of them are spying on us while we're sunbathing in our backyards? Well, I guess, you know, technically in an infinite universe, that there's probably a planet it out there where dad jokes are like the epitome of intelligence and literature. Are you saying that's not our universe? Are you saying that's not our planet? That is definitely not our planet. I think there's a reason they're called dad jokes, not just jokes. But maybe there's an alien species out there where, you know, it's like the height of wit, you know. Right. Well, we should try to sell our books on that planet then because we have a lot of readers.
Starting point is 00:05:47 Yeah, it would be intergalactic bestsellers, not just international bestsellers. But we're not just interested in whether our books will sell to alien species. We're interested in whether there are aliens out there, whether life exists in other parts of the galaxy. And part of that question is asking whether our whole setup is unusual. Are there stars with planets around them? Do those planets have similar conditions to the planets here? Is there something weird and strange about the solar system or is it very common? Yeah. Is the planet Earth a rare gem that exists out there in the cosmos?
Starting point is 00:06:20 or is it sort of like a, you know, cheap Chatsky that you can find anywhere? And just a few decades ago, we didn't know the answers to basic questions like, are there planets around other stars? Fortunately, as we develop new and more powerful eyeballs, we've been able to discover those planets. And now we are pushing further. We are asking deeper and more subtle questions about the nature of those planets, their atmospheres, their surfaces, even what's in orbit around them.
Starting point is 00:06:46 So today on the podcast, we'll be tackling the question. Could we see moons around exoplanets? Now, Daniel, I imagine these are like moons, like the orbiting celestial bodies and not like aliens mooning. Or maybe alien death stars, right? We don't care. We just want to discover them. Wait, wait, wait, wait. I think maybe we should draw a line.
Starting point is 00:07:11 If there are alien death stars, maybe we don't want to meet them. Maybe these are not the aliens we're looking for. I think we'd rather know they're there than live in. ignorance, wouldn't we? If we know they're there, then they know we're here. We could just use that Jedi mind trick. That's right. Make them forget and dazzle them with our dad jokes.
Starting point is 00:07:28 And they'll be like, what, what? And then they won't want to associate with us and then problem self. These aren't the jokes you're looking for. That's right. Or maybe they'll want to annihilate us right away. But we are curious about the environments of these planets. Having moons affects life on Earth and tells us a lot about the history of that solar system. And just in general, we want to know, like, our solar system.
Starting point is 00:07:50 is pretty Mooney, are other solar systems Mooney as well. Mooney and wonderful, because I think as you said earlier, up until a few years ago, a few decades ago, we didn't even have confirmation. There were other planets out there, right? We just imagine or assume there were, but we had not actually seen any. Yeah, it could have been that we were one of very, very few perhaps singular solar systems that had planets around it. It could have been that the reason that there's life here around our sun is that it was the
Starting point is 00:08:18 only one with a rocky habitable person. Now, of course, we know the opposite is true. We know there are planets all over the galaxy. We've seen a few thousand of them, and we estimate that there are zillions of them, that they're almost literally everywhere in the galaxy. That's a real change in the way we see our whole context in the universe. Yeah, because I imagine even, like, jumping from our sun to the stars in the sky was kind of a big leap for humanity too, right? Like, you can look at our sun and it looks circular, at least if you see a projection of it or through a filter,
Starting point is 00:08:48 you can see that it's a giant ball, but the stars in the sky just look like little pinpoints. And so it must have been a pretty big leap to think, you know, those pinpoints are actually stars. It is a pretty big leap. And to understand how big a leap it is, to understand how far away they are is pretty tricky. I mean, even the Greeks knew that the other stars were likely suns, but they thought they were much, much closer than they actually are. The Greeks couldn't understand how far away these stars actually were. So, yeah, it really expands your whole mental picture of the universe. to understand that our sun is one of many of those stars and that therefore there are lots and lots
Starting point is 00:09:24 of places where life might exist in the universe. Yeah, and those stars out there are really far away. That's why they look like pinpoint. And so basically until recently, it was almost impossible to really see a planet on them, right? It was very tricky. And for a long time, people thought it might be impossible. But astronomers are very clever and very hardworking. And now we have lots of tricks to discover planets around other stars.
Starting point is 00:09:47 And so now people are pushing into what many people believe is impossible, understanding the atmospheres, the surfaces, and maybe even the orbiting bodies of those planets. I wonder what did, well, I'm sure we'll get into it, but what's the driving question here to know whether an exoplanet has a moon? Like, do you think maybe the moon is the one that's habitable or you're just trying to study other moons? I think all of those things, moons might be the most common place for life in the universe.
Starting point is 00:10:14 It might be that moons around big planets are. are the best place for life to evolve. And the humanity is very, very weird for developing directly on the surface of a planet. On the other hand, moons also tell you a lot about the history of the solar system, how it formed, how it came to be, which tells you a lot about where you expect to find planets that might have life on them. So it's as much about understanding the detailed history of other solar systems and thinking about where we might find life.
Starting point is 00:10:42 Well, as usual, we were wondering how many of you out there had thought about this question and wondered if we could see moons in other planets. Thanks very much to everybody who offers their unprepared insights. We really enjoy this segment of the podcast, and we want to hear from you. Please don't be shy. Write to us to questions at danielandhorpe.com. So think about it for a second.
Starting point is 00:11:01 Do you think we could ever see moons around exoplanets? Here's what people had to say. Just finished listening to the podcast with the exoplanet researcher. And do I think we could see them? No. But we do have confirmed. existence of moons around exoplanets. I believe that number is currently at two. I think we will definitely be able to see moons around exoplanets. James Webb will be able to
Starting point is 00:11:26 analyze the atmospheres of exoplanets and it might even be strong enough to see moons. And if not James Webb, there's probably going to be another set of eyeballs in the future that will be able to do it. I think that in order to be able to detect moons of exoplanets, we would need very sensitive telescope and other instruments, capable of measuring the lightest, faintest of changes in the light emitted from other stars. My best guess in terms of finding exoplanet moons would be to measure the gravity between that planet, that exoplanet and its star, and see if we can account for any extra gravity, that would be from a moon or maybe some sort of nudge or tug on that moon.
Starting point is 00:12:09 I think this depends on your definition of what it means to see a moon. It seems like it would be nearly impossible to imagine directly imaging any, especially given that we haven't directly imaged an exoplanet yet. But if we had a sufficiently large planet around a star with a big enough percentage of its star's mass, and if it in turn had a moon that was a significant percentage of its mass, then I would imagine that they could probably detect the combined wobble of the interaction between those three. All right. A lot of optimism here, I feel. Everyone's like, sure, yeah, eventually, sort of in one way or another. Yeah, there's this bubbling sense that eventually we could figure out basically any problem, that in our future lies more and more powerful techniques and telescopes and smarter people that could extract this kind of information from the universe. I love that.
Starting point is 00:12:56 It's so inspiring to hear people's optimism. Yeah, yeah. And I think by smarter people, you mean the engineers, right? I mean, my students and my students' students. And the engineers that actually do it for them, right? I think that's what you're saying, right? I don't know. We just submit the work order and it comes back.
Starting point is 00:13:11 You know, who knows who doesn't. Yada, yada, yada, you got a telescope. That's right. We toy anonymously. That's what happens to all smarter people. No, of course, the field of astronomer is filled with people who analyze the data and people who build the devices and people who plan for the next generation of devices. It's a whole ecosystem of smart people from physicists to planetary scientists to engineers to computer scientists, all sorts of people all working together. Well, this is a pretty big question, or I guess a small question, is how do you see the moon around a planet,
Starting point is 00:13:41 orbiting a star that is light years or at least millions of miles away, it's a pretty tough question. It is a pretty tough question. And it's going to require us to get even better at seeing those planets. All the techniques we have for seeing moons are basically like super powerful versions of the ways that we see planets. All right. Well, let's break it down for people. Daniel, first of all, what is an exoplanet and what do we know about them? So an exoplanet is very simply just a planet around another star. So the planets are the planets around our sun. An exoplanet is a planet around, for example, Alpha Centauri, or any other star that's
Starting point is 00:14:18 not our sun. Exo just meaning like outside the solar system. I see. Like an outer planet. Well, I guess not because an outer planet could be the planets in our solar system. Like anything outside of our solar system that's a planet is an exoplanet. Yeah. A planet around another star would be an exoplanet.
Starting point is 00:14:36 And they have to be far away because the nearest. star is several light years away, which is really, really far. It's very far compared to the distance between the planets. And so an exoplanet is going to be very, very different from any planet in our solar system just in terms of like where it is. And we hadn't actually seen one or confirmed there were any planets around any other stars until basically like 30 years ago, right? Yeah. It's incredible if you make a plot of like the number of planets we've seen over time dating back like thousands of years until fairly recently we'd only ever seen like six. Right? And then Uranus and Neptune are discovered in the last few hundred years. And then Pluto and then
Starting point is 00:15:14 unpluto. So we're back down to eight. And then it wasn't until the 1990s, only 30 years ago that we finally saw one outside of our solar system. Until then, we only speculated. We only imagined. We'd had calculations. We had speculations, but we had no actual data until about 30 years ago when we developed these techniques to see the planets or to deduce their existence around other stars. Yeah, because one of the listeners who replied earlier said the word C is a little bit tricky, right? We didn't actually see planets and other stars. We sort of like figure out they were there, but we didn't actually see them. Yeah, exactly.
Starting point is 00:15:50 And so we have these really cool techniques to deduce that they exist. And, you know, you can argue philosophically about what did it mean to see something. But we didn't see exoplanets directly until much more recently. The first discoveries came from just observing the impact of those planets on the stars, course we can see. Which is kind of crazy to think, right? Because like what possible impact in the Earth have on the Sun? The Sun is like a million times heavier than the Earth, right? Or more. It's all about making these things more sensitive and getting down to the details. Like mostly you're right. The Earth has basically no impact on the Sun. But if you analyze the Sun super duper closely,
Starting point is 00:16:28 then yeah, the Earth does have a little bit of an impact on the Sun. The same way that, for example, the other planets have an impact on the Earth. Mostly the Earth's orbit around the Sun is, just a story of two bodies, the Earth and the Sun orbiting their combined center of mass. But if you get super duper precise about it, then you have to take into account like the effect of Jupiter and Saturn on the orbit of the Earth. So all of these little complications can actually reveal the rich structure of the solar system if you study them with enough precision. It's pretty mind-boggling to think.
Starting point is 00:16:58 I mean, the Sun is so big and the Earth is just this tiny little marble next to it, like that it would have an effect on the whole thing. I can see maybe pulling a little bit more on the part of the sun that's closest to the Earth, maybe some of that plasma, but to think that it could move the entire sun is pretty hard to believe. Yeah, well, imagine instead you had two objects that had the same mass, right? Like two stars, the same mass. And they're orbiting each other.
Starting point is 00:17:22 Clearly, they have an effect on each other. What they're orbiting is actually a point right in between them. Now, as you shrink one of those things down and grow the other one, so it becomes asymmetric, the point they're orbiting moves towards the center of the center of the. the heavier one. If one of them was infinitely massive or the other one was massless, then they would both be orbiting a point at the center of the biggest object. But if the earth is not massless, if it actually does have some mass, then it's pulling that center of mass a little bit away from the center of the sun. And if you measure the motion of the sun very precisely,
Starting point is 00:17:53 you can detect that. And that's why these things are so hard. That's why it took so long to see these things is that it requires really precise measurements now of the motion of stars in other solar systems. Yeah, it's pretty mind-blowing, but I guess maybe one thing that helped was that we didn't start looking for Earth-sized planets, right? We started looking for Jupiter-sized planets. Well, we started looking for anything we could see, and we didn't know what was out there, right? We had speculation about what kind of planets might exist in other solar systems, but we didn't really know what we could find. You're right, though, that the first techniques we developed were more powerful for Jupiter-sized planets. The bigger the planet and the closer it was to the star,
Starting point is 00:18:31 the easier it was for us to find them. Like those were the first planets found, right? They were basically a giant gas planets. Yeah, they call them hot Jupiters because they're the size of Jupiter and they're very close to the star. The closer they are of the star, the faster the orbit,
Starting point is 00:18:47 the easier it is to find them because they tug on the star. And so one of these techniques is called the radial velocity method. You look at the light from the star and you see if it's shifted in frequency. If a star is moving away from you, it's redshifted.
Starting point is 00:19:00 If a star is moving towards you, it's blue shifted. If a star is getting wiggled by a planet that's orbiting it, then it's going to get redshifted and blue shifted, redshifted, and blue shifted, it's going to wiggle a little bit in its frequencies. And that's what they look for. But that's more powerful for big planets and planets that are close to their stars. But then we develop other ways to look at planets, really quick. What are some of these other ways that we can see exoplanets? So another way is the transit method, which is basically an eclipse. As the planet passes in front of the star, it dims it a little bit. It blocks some of the light.
Starting point is 00:19:31 And so again, if you're just measuring the light from the star, roughly, you're never going to notice this. If you make very precise measurements of the light from the star, you can see these dips and you can see the patterns. If the planet goes around many, many times, you'll see the same pattern over and over again. Unfortunately, this one is also best at seeing big planets that eclipse the light more and close by planets that block more light from their sun and go around many times so we can see many transits. Yeah, like if the moon didn't reflect any light and you can. and see it in the night sky, you could still maybe every once in a while know it's there because it would block the light from the sun. You'd see an eclipse. Exactly. And there are techniques that will let you see planets that are further from the sun. And these are actually the direct
Starting point is 00:20:12 imaging ones. We can look at a solar system and we can block the light from the sun called the coronagraph, a little thing that prevents the light from the star from getting into the telescope and only look at the stuff around it. And now we have powerful enough telescopes that you can actually see dots around those stars. So these are direct images of light from the telescope. And those planets. And those are most powerful at seeing planets that are far away from the star. Because the further they are from the star, the easier it is to tell them apart from the blinding light from the star itself. Yeah, it's like you basically put your thumb. Like if you look up at the sky, you put your thumb over the star and then you see there are any other twinkles around it,
Starting point is 00:20:49 right? Exactly. And so we have like a few pixels of light from these planets. Of course, the planets themselves are not glowing. It's all reflected light from their star. But, you know, it bounced off the planet first. So it's just like looking at the, the planet. The same way the Earth is illuminated by our sun. And that's the closest we have of an actual picture of another planet, right? Like I've seen the plots. They're a bit old, right? And now we've had these photos for 15 years or something like that. Yeah, they're getting better and better, but they're not great. I mean, they're pretty fuzzy. If you took pictures of your kids like this, none of your relatives would be very impressed with your photography.
Starting point is 00:21:20 It's like a few pixels here and there. Yeah. Although my kids nowadays avoid getting their picture taken, as I think most kids do. And so they're kind of a big blur anyways. And then what's the last kind of method we use to detect these exoplanets? The last technique is called microlensing. And that's essentially using the planet as a lens to distort light from some other star. If there's light from another star behind the solar system that's passing through that solar system, then it can get bent around the planet. Because the planet, of course, is massive and it changes the shape of space.
Starting point is 00:21:57 And so it can act like a giant lens. This is sort of similar to the way we can see dark matter. in the sky by seeing its gravitational lensing. So here it's called microlensing because it's a smaller amount of lensing as the light passes around the planet. Yeah, you're seeing how it bends the light coming at you. And so those are the different ways that we can see exoplanets. But now the big question is, are there moons around these exoplanets out there in the universe?
Starting point is 00:22:20 What is it like on those moons? Could we ever see them? And how are we going to see them? So let's dig into that. But first, let's take a quick break. Smokey the bear Then you know why Smokey tells you when he sees you passing through Remember please be careful it's the least that you can do
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Starting point is 00:25:21 and maybe the push to make your next pivot. Listen to these women and more on She Pivots, Now on the IHeartRadio app, Apple Podcasts, or wherever you get your podcasts. All right, we're talking about finding exo moons. Do you call them exo moons if it's a moon around an exoplanet? Yeah, we call them exo moons, unless you have a better name for them. It shouldn't it be like exo-exo moons? because it's like a different body out on an exoplanet?
Starting point is 00:25:58 There are exo moons around exoplanets. There are two exos there. But I think exo just means in another solar system. Well, what do you call the moons around Jupiter? Moons. Indo moons? Yeah, there you go. Indo moons.
Starting point is 00:26:15 No, just moons. And Jupiter is a great example because something we notice in our solar system is there are kind of a lot of moons, right? we have 226 moons in our solar system and something we wonder is like is that weird are we kind of moony or are we moon poor compared to other solar systems like what's a typical number of moons to have we just don't even know and we have a whole episode about how like moons form right how you get a moon yeah exactly it's really fascinating the number of ways that you can get a moon they can form with a planet you can capture them it can be the result of a collision the point is that it tells you a lot about the history of the solar system It's like a record of what happened here before you showed up. Right. Like our solar system, we've talked about before, it was a pretty chaotic place. And so it kind of makes sense that there was just a lot of debris out there floating, flying around. And so not all of it was going to get into planets.
Starting point is 00:27:08 And so it makes sense we have the smaller bodies out there orbiting the bigger bodies. Yeah, although we have an incredible range of sort of size of those bodies. Like our moon is huge. It's like more than 1% the mass of the Earth, which is very, very unusual. More typical size is like one 10,000th the mass of the planet. But then there's also like Sharon, which is one eighth the mass of Pluto, even though Pluto not officially a planet anymore. But we have this incredible variation in the sizes of the moons. And in their origin and their composition, it's really an incredible diversity. Or I guess in the relative size,
Starting point is 00:27:43 right? Because some of the moons around Jupiter, aren't they almost the same size as our moon? Yeah, exactly. We're talking about the relative sizes. And some of the moons around Jupiter are huge, absolutely and potential places for life to exist, which is one of the things that makes us wonder whether moons around exoplanets might also be habitable. All right, well, we talked about how we can see other planets and other stars in the universe. And I guess as astronomers were like,
Starting point is 00:28:06 okay, we've seen those. Now it's increased the difficulty. Exactly. It's fine things orbiting not just around other stars, but around the things that are orbiting around other stars. And this is the game in science, right? People have come along and done the simplest thing. All right, now let's come along and do the next harder thing.
Starting point is 00:28:22 And then the next generation is like, well, that was easy. Now let's do the next harder thing. And so I love how we're always making progress. We're always pushing the boundaries here. But are we done though? I feel like I'm still waiting for that, you know, actual picture of another planet in another solar system, you know, like a photograph photograph. Yeah, no, we're never done. Right.
Starting point is 00:28:40 We're always pushing, but we're pushing in lots of directions simultaneously. People are working on that photograph. One idea that's being worked on, which we talked about in the podcast, is like using the sun itself as a gravitational lens. You put a camera out deep in the solar system. You can use the sun to gather a huge amount of light from a distant solar system. And the sun will focus all that light on the camera you have out like near Neptune, treating the sun like this huge lens and making a solar system sized camera. That could give you a picture of the surface of exoplanets. Wait, what? Like our sun?
Starting point is 00:29:13 Yeah, our sun. You have the sun acting like a gravitational lens gathering light and then focusing it on a camera. you put way deep in the solar system and you can take a picture of something super far away with a lens effectively the size of the sun. Whoa. Pretty cool. Let's do it. Pick or it didn't happen. It's pretty tricky project
Starting point is 00:29:33 because you have to get a camera like pretty far out in the solar system and that could take decades and then moving it takes a long time. But it definitely can be done. And someday we will see the surface of exoplanets. And then you've got to get the aliens to stay still and smile for the camera. And it takes, you know, a thousand years. is just to say cheese.
Starting point is 00:29:50 Yeah, then they have to sign that waiver, you know, so you can publish the picture. There you go. You seem really concerned about the aliens here. Hey, man, I'm just looking out for them. I just don't want them to come and punch us in the face over something silly, like legal forms. You don't want them to punch you in the face when you take a picture of them in the bathroom. I have no idea when they're in the bathroom. Like, what are you doing over there?
Starting point is 00:30:14 Is that what you call the bathroom? I don't know. I'm just taking pictures. Oh, I see. You're going to claim ignorance. Look, I just want to say there's a lot of moon jokes I'm not making around here. Thankfully, thankfully. All right.
Starting point is 00:30:25 Well, then, how can we see these X-A-Moons? We basically use the same methods we use to detect other planets, or are we trying some different things? Both. The bread and butter is to take the same methods and make them super-duper-sensitive. The transit method is one of the most sensitive methods for finding these planets if everything is lined up. And you can also use it to discover the moons in a couple of ways, because the moon will affect how the planet blots out the light from the star.
Starting point is 00:30:52 Number one, it can affect when it happens. Like the moon is tugging on the planet the same way the planet is tugging on the star, which makes when the planet gets in front of the sun and blocks its light, change a little bit as the moon is orbiting the planet. It's like yanking on the planet a little bit. So it changes the timing in these transits. Right. Like I guess like our moon, the moon here is making the earth.
Starting point is 00:31:17 wiggle a little bit. And so the idea is that another planet and another solar system, if it has a moon, a big enough moon, it's making that planet wiggle. And so when it moves in front of its star, it's going to block the light in a wiggly fashion. Exactly. And if you count enough of these transits, you can start to notice these patterns. And then you can fit it to a model. You can say like, well, can I explain why this transit was a little bit later and that transit was a little bit earlier by assuming that there's a moon there pulling on it? Is it all consistent? You don't just like look for noise and say well I don't know it was noisy maybe there was a moon you have a specific description of what that moon might look like and how it would affect the planet right like
Starting point is 00:31:56 if you notice that the wiggling is regular then you know there's something going on like it can't just be like random wiggling exactly and there's a second way which is that the moon itself can also contribute to blocking the light not just when the planet blocks it but the moon could also have its own little moony eclipse right because if the moon is lined up at the same time as the planet, you can add a little bit of eclipsiness to the planet. It effectively makes the planet's shadow a little bit bigger. If you have a model for how that moon is orbiting the planet and when the planet is going around the sun, you can predict exactly when the moon's going to be in the right position to add to the eclipse. But wouldn't it always block the light from the sun? Like, you know,
Starting point is 00:32:36 it's pretty small compared to that planet and the planet is small compared to the sun. Wouldn't it always be sort of in sight or in view? It might also always be in view, but it doesn't always have to contribute to the amount of eclipse, like let's say they're all lined up if you see like moon and then planet and then star. If the moon is already in the shadow of the planet, then it's not contributing to the decrease in the light. Only when the moon is sort of offset a little bit from the planet. So it's like adds a little shoulder to the planet. Is it going to increase the amount of light that's being blocked? And that's the kind of thing they look for. They look for these transit dips with like a little wiggle on the down edge or wiggle on the
Starting point is 00:33:14 up edge when the moon is peeking around the side of the planet. Basically have to have moon rise or moon set along the planet for it to contribute to the transit dip. Wow. But now we're talking about like a super duper tiny dip in the light, right? Like our moon would blog very little of our giant sun. Yeah, exactly. We're talking about really sensitive measurements.
Starting point is 00:33:33 And until recently, people thought this is impossible. You know, you need very, very accurate understanding of the light and very precise measurements of the intensity of the light coming from these things. things. So it wasn't until like 2007, more than decade after exoplanet discoveries, the people really started working on this in detail, like taking the idea seriously. And one of the biggest challenges is that most of these techniques that we've used to find exoplanets are good at finding planets close to the star, like we talked about. Hot Jupiter's, right? Really big planets, really close to their stars. But those planets are unlikely to have moons. And so that
Starting point is 00:34:11 makes it very challenging to find any of these moons. Why are they unlikely to have moons? For the same reason that Mercury and Venus don't have moons in our solar system, right? All the other planets have them and Mercury and Venus don't. It's because of the tidal forces from the sun. As you get close to the sun, the tidal forces, the difference in gravity from one side to the other side of a planet, for example, get very, very intense. And that will just disrupt the orbit of a moon. In order to have a moon orbiting a planet, you basically need the sun to leave it a little bit alone. You need to plan it to be able to dominate the gravitational experience of that moon so the moon can be trapped in an orbit. But if the sun is really, really
Starting point is 00:34:48 close by, then the sun's tidal forces make a moon's orbit impossible. Like they'll tend to pull the moon towards the sun and then eventually that moon will either fly off into space or fall into the sun. Exactly. Essentially, it's like a three-body system, which we've talked about before, is this fundamentally chaotic. The only arrangement for a three-body system to be stable is if two of those bodies are pretty close together and pretty far from the third body, which is like if you have a distant plan with the moon orbiting it. That planet gets too close to the sun, you now have a three body problem and you're going to lose your moon.
Starting point is 00:35:20 So you're saying that's kind of a problem because our exoplanet detection methods depend on being close to the sun, but those planets might not have any moons. Exactly. So the kind of planets we're good at finding are the kind of planets we expect to not have very many moons. On the other hand, there's lots of planets out there and we can sometimes see planets a little further from their star and maybe one of those hot jupiters will have a big enough moon that's orbiting close enough to it to be stable so there's not no hope but it's pretty tricky but i thought the
Starting point is 00:35:49 transit method the one where we're looking for eclipses and distant stars those don't depend on the closeness of this planet they do indirectly depend on the closeness of the planet what you want is a short period because you want to see many transits if your planet is really far from your star and orbits like once every 80 years, then you're most ever going to see one transit. And it's pretty hard to be sure that what you're looking at is a planet if you only see one eclipse. If you see it regularly and it happens every four days and you can really study it in detail and you can convince yourself that you're seeing a planet, not for example like a star
Starting point is 00:36:22 spot, something on the surface of the star that's dimmer and darker and decreasing the intensity of the light. The period of the orbit makes a big difference. Yeah, exactly. Because you want more examples. Right, right. Yeah, like some of the planets in our solar system take like 200 years, right, to go around the sun? Exactly. And so if you're an alien graduate student and you're trying to discover Pluto in our solar system, then you're going to be a student for a long, long time.
Starting point is 00:36:47 Yeah, it's going to take even longer to get that PhD. Thousands of years. I hope you guys live long out there. So then what about direct imaging, like taking a direct photograph? Is that better for planets that are far away from the star? Yeah, that's possible. We're sort of just on the cutting edge of being able to do that. even for planets. And so we're pushing those limits and we're developing new technologies and there's a whole new generation of space-based telescopes that are going to be super awesome at doing direct
Starting point is 00:37:15 imaging of those planets. And so as that gets better, it'll start to be possible to potentially see moons around those planets. But you know, as we said, like currently planets are basically one or two pixels. So resolving a moon around those planets would be really challenging with a couple of exceptions. If those moons have ways to like really make themselves known, then we might be able to see them. So like, for example, if you look at Jupiter here in our solar system with a regular telescope in your backyard, you can actually see the moons of Jupiter, right? You see little
Starting point is 00:37:46 points around a bigger circle of the planet. The idea is that if you point a bit powerful enough telescope at these distant planets, you could see maybe the dot front of the planet, but also maybe little dots around it, that might be the moons. Yeah, you might, especially if those moons are weird in some way. Like if those moons are super volcanic and they're shooting out really hot gases, you might be able to spot that. Or if the moons are super duper hot, like they're squeezed by their planet with tidal forces so that internally they're very high temperature, then they might glow at a different temperature than their planet and be easier to see them. And so there's some weird kind of moons that you might be able to direct image before regular normal humps of rock. But I think
Starting point is 00:38:30 we're going to have to wait for our direct imaging technology to improve significantly before we can expect to see pixels from exo moons. Interesting. I wonder if you can do like a eclipse method on a planet that's far away. You know what I mean? Like if you're looking at the light from a reflected from a planet and you see a dip itself, I wonder if that could be a sign that there's a moon there. Yeah, that's a cool idea.
Starting point is 00:38:52 And you're right, the reflected life from that planet should dip when the moon passes in front of it. Again, we're still at the cutting edge of even seeing. pixels from those planets. And so there you'd need like to study those pixels over time and to look for dips and to understand every other possible source of dips because that planet's light is already going to be variable as the planet goes around the stars. You're going to have to understand that and then variations on that. But yeah, that's a cool idea. Thanks. I'll take the Nobel Prize. We have it on record. All right. Well, these seem like long shot sort of sounds like from what you're saying that we're not super close to being able to do this. But have we? Have we found any
Starting point is 00:39:30 moons out there and other planets? Have there been any discoveries? So we are right on the edge of being able to do this, which means that we have like a couple of candidates that are disputed. There are some people who think these probably are exo moons and other people who think they're probably not. You know, the evidence is like really right on the edge and people split over the statistical analysis of these things.
Starting point is 00:39:50 But it's fun because we have a couple of things to dig into and to talk about. All right. Let's do it. What are these candidates for possible exo moons? So there was one discovered in 2018. This was the first exo moon candidate. And it's around planet Kepler 1625B. Kepler 1625 is the star.
Starting point is 00:40:11 B means the planet. And then the moon is called Kepler 1625B dash I. Why I? Was there an A, B, C, D, E, F, G, H moon? Or are they just going for like an iPhone reference here? No, I think it's Roman numerals. Like the first one's going to be I, the second one's going to be I-I, the third one. one would be i i i this kind of thing uh i see all right yeah switching it up exactly and so here's this
Starting point is 00:40:36 two separate independent pieces of evidence that suggests that there might be a moon here what we're looking at is a jupiter size planet around the star right but it's like earth distance from the sun but it's like a huge planet that's what we think is there that's what we think is there that's the planet that we're pretty sure is there that's kepler 1625b it's mass but maybe uh not necessarily it has to be a gas giant, does it? We know something about its mass because we know it's orbit. And so we know roughly its volume and we know roughly its mass. And so we can tell something about the density.
Starting point is 00:41:08 And these planets of this size are almost always gas giants. All right. So that's what we think is there. And so it's sort of an unusual planet already because it's a cool Jupiter. We talked earlier about how lots of the planets we've discovered are hot Jupiters, big planets very close to their star, like within the orbit of Mercury. But this is a farther out orbit which makes it a cool. Jupiter. And the first thing they noticed is this transit timing variation, that the planet is
Starting point is 00:41:33 blocking the light from the star behind it, but it's not in a regular fashion. There are wiggles there in exactly the way you would expect if there was a moon. I see. So it's not like going around its sun in a regular way. It has a little wiggle to its orbit. Exactly. It has a little wiggle to its orbit, which can be explained very nicely by the presence of a moon. Like they do all the statistical calculations. They have two models like with and without the moon. And the one with the moon better explains the data like much, much better explains the data than the model without the moon. Although could it be something else as well? It could be something else, right? It could be that there are other planets in this solar system and those planets are tugging on it.
Starting point is 00:42:14 And that would be much more complicated because you could have multiple planets like several Jupiter-sized planets that are yanking on it. It's very difficult to model. And that's one reason why this is not a smoking gun discovery because there are other ways that you could get this kind of signature. What they did to follow up is they looked at some Hubble data. They looked at Hubble data pointed at this star to see if they could see an impact of the moon on the transit itself, not just the timing, but like could we see wiggles in the dip, right? Are there like shoulders in this transit that indicate that we're seeing like a moon rise as the planet is blocking the light from the star? Like is the moon from this cool Jupiter also blocking the light from the
Starting point is 00:42:53 star sometimes? Yeah, exactly. And we only have, unfortunately, one really clear transit because this comes from Hubble and Hubble is not a planet finding telescope. It's busy doing lots of things. It's not always looking at one star. So they have only like 40 hours of data from this star with Hubble, but they did see a clear transit and there is a dip there that looks like a Neptune size moon around this Jupiter size planet. Wow, that would be a huge moon, wouldn't it? Yeah, literally. That would be huge. It's more like a sister planet almost. Yeah, although technically, if it's orbiting a planet, then it's a moon. What if they're both planets?
Starting point is 00:43:31 Yeah, this gets into a really murky territory of where you define things to be binary planets and where one of them is a moon. They have this definition where if the center of mass is inside the surface of one of them, then one of them is a planet and the other one is a moon. In this case, that Jupiter is so much bigger than the Neptune that the Neptune qualifies as a moon. You only have one data point. Why don't we get more? I think that people are excited about that.
Starting point is 00:43:56 and are working on it. But you know, Hubble time is very, very precious. And there's lots of good things to use Hubble for. In the meantime, people have been like analyzing this and reanalyzing this and other groups have analyzed this data. And not everybody agrees with the interpretation that the first paper came up with. Some people look at the transit data and they say, no, there's no dip there from a moon. It doesn't look like there's any shoulder there. Another group analyzed it and said they do agree with the shoulder, but they disagree with the uncertainties and the other measurements. And the point is that the data is fuzzy. It's not crisp and clear. It's not obvious. It requires like heavy duty statistical techniques to extract this information. And so we just
Starting point is 00:44:33 really can't be 100% confident. Wow. So they published this paper with just one like data point? Well, they have one example of the transit, but they also have the transit timing, right? So those are two independent streams of information. One is the timing of the transits and the other is like the actual photometric, like looking at the dip in the light. Seeing the moon itself. actually eclipse. They have lots more of examples of the moon tugging on the Jupiter and changing its transits, but only one example of the moon itself blocking the light. And they sort of match together, I guess, right? They do match together according to one group and their analysis and they don't match together according to another group. Sounds like they need more data. We definitely
Starting point is 00:45:14 need more data. We need more telescopes and more eyeballs. It's so frustrating when our knowledge of the universe is just limited by like how many eyeballs we've built. Because There's nothing stopping us from building more. It's just money. It's just money. It's just money. We can just print more. Come on.
Starting point is 00:45:31 Daniel doesn't need his money. Let's do it. Print some more money. Make some more telescopes. Done. Let's do it. Hey, a lot of engineers will be put to work building the Daniel funded telescope.
Starting point is 00:45:42 Yeah, I'm sure. I'm sure. Do it. Okay, I will print my own money and I'll see if engineers out there will accept it as payment. 100,000 Daniel bucks. Well, no, well, I mean, if you commit fraud that way,
Starting point is 00:45:53 Who's going to believe your scientific findings? Yeah, exactly. And that's why there's no Daniel Space Telescope. All right. Well, what's another discovery we've made in this attempt to find other moons? So there's a second potential discovery. This one's Kepler 1708b-I. And this was a really cool strategy to look specifically for planets that have long periods
Starting point is 00:46:18 that are further away from their stars because they're rarer, at least in our catalog at least, they're rare and the kind of things we can see, but they are more likely to have moons, we think. Because that's kind of the trend in our solar system, right? Like we have one moon, Mars is two in the inner solar system, but in the outer solar system, like Jupiter and Saturn have dozens of moons. Yeah, exactly. Because the further you get away from your star,
Starting point is 00:46:41 then the more freedom you have to, like, dominate your gravitational environment, capture moons or retain moons or all that kind of stuff. So they thought, well, let's focus on cool giants, these planets that are further away. And in the whole catalog of exoplanets we've ever discovered, they're only like 70 that qualify is these cool giants. I see. If they're not cool, they're not included in the study.
Starting point is 00:47:03 You're not invited to the party. Only cool giants. Hot giants is a totally different party with a totally different vibe. Here it's more of a hipster, you know, scene. Yeah, we're listening to jazz around here. So sit down, have a drink, chill out. I'm not sure jazz is considered cool. by the kids these days.
Starting point is 00:47:22 Oh, all right. Thanks for filling me in. All right, well, let's dig into this cool giant moon, what we know about it, and what it tells us about how solar systems form. But first, let's take another quick break. Smokey the Barre. Then you know why Smokey tells you
Starting point is 00:47:43 when he sees you passing through. Remember, please be careful. It's the least that you can do. With matches, don't play with fire. After 80 years of learning his wildfire prevention tips, Smokey Bear lives within us all. Learn more at smokybear.com, and remember, Only you can prevent wildfires.
Starting point is 00:48:05 Brought to you by the USDA Forest Service, your state forester and the ad council. I'm Simone Boys, host of the Brightside podcast, and on this week's episode, I'm talking to Olympian, World Cup champion, and podcast host, Ashlyn Harris. My worth is not wrapped up in, How many things I've won, because what I came to realize is I valued winning so much that once it was over, I got the blues, and I was like, this is it.
Starting point is 00:48:32 For me, it's the pursuit of greatness. It's the journey. It's the people. It's the failures. It's the heartache. Listen to The Bright Side on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. Have you ever wished for a chance? change but weren't sure how to make it? Maybe you felt stuck in a job, a place, or even a relationship. I'm Emily Tish Sussman, and on she pivots, I dive into the inspiring pivots of women who have taken big leaps in their lives and careers. I'm Gretchen Whitmer, Jody Sweeten. Monica Patton. Elaine Welteroth. I'm Jessica Voss. And that's when I was like, I got to go.
Starting point is 00:49:11 I don't know how, but that kicked off the pivot of how to make the transition. Learn how to get comfortable pivoting because your life is going to be full of them. Every episode gets real. about the why behind these changes and gives you the inspiration and maybe the push to make your next pivot. Listen to these women and more on She Pivots, now on the IHeartRadio app, Apple Podcasts, or wherever you get your podcasts.
Starting point is 00:49:37 Hello, Puzzlers. Let's start with a quick puzzle. The answer is, Ken Jennings' appearance on The Puzzler with A.J. Jacobs. The question is, what is the most entertaining listening experience in podcast land.
Starting point is 00:49:54 Jeopardy truthers who say that you were given all the answers believe in... I guess they would be conspiracy theorists. That's right. Are there Jeopardy truthers? Are there people who say
Starting point is 00:50:05 that it was rigged? Yeah, ever since I was first on, people are like, they gave you the answers, right? And then there's the other ones which are like, they gave you the answers and you still blew it. Don't miss Jeopardy legend
Starting point is 00:50:18 Ken Jennings on our special game show week of the Puzzler podcast. The Puzzler is the best place to get your daily word puzzle fix. Listen on the IHeart radio app, Apple Podcasts, or wherever you get your podcasts. All right.
Starting point is 00:50:45 We're talking about cool giants, not the, you know, plain old giants. Not the lame giants, but the cool giants. And seeing if they have any moons in them. That's right. The moons have to be cool, too? Some of these moons could be hot, right? They could be volcanic.
Starting point is 00:51:03 They could have all sorts of stuff going on inside, even if the planet itself is pretty cool. That would be cool. All right, so we've been talking about finding moons and other planets outside of our solar system in distant stars, and there are many different ways to do it that are getting better and better every day. And so we have a couple of candidates.
Starting point is 00:51:20 of things that might be moons, exo moons out there. And one of them is this one called 1708 B.I. That's right. And this one was just discovered last year, 2022. And they looked again at the transits. They're looking for like shoulders. When this planet is going around the star, are there moments when it's blocking more light than you expect,
Starting point is 00:51:41 which could be explained by having a moon orbiting that planet and like rising past the limb of the planet or coming around the back and blocking the light? and so they were looking for these little shoulders and it's really pretty cool they do see some they see these little shoulders inside this transit blip and I think by shoulder you mean like
Starting point is 00:52:00 if the planet didn't have a moon when it stopped making an eclipse with the star behind it the light from the star would just drop off or at least drop off relatively quickly but if it has a little moon maybe trailing behind it then the light from the star would go down mostly
Starting point is 00:52:15 but not all the way but then a little bit of a shadow would remain and then the shadow would go away And that's the kind of thing you're looking for, right? There's a moment after which the planet is no longer blocking the star, but the moon might be blocking it a tiny little bit all by itself, which extends this transit dip. Or maybe the moon isn't like in front of the planet.
Starting point is 00:52:34 And so then first the moon gets out of view of the star, and then the planet drops out of the eclipse. And so you see this little shoulder in the light from the star. Exactly. And so they see this shoulder and they can explain it using, again, a Neptune-sized moon. This planet has a Mars-like orbit, so it's even further from its star than the previous one. And the planet itself is huge.
Starting point is 00:52:56 It's five times the mass of Jupiter. So it's a really big planet with a Neptune-sized moon candidate. And the only explanation we have for these shoulders is an exo-moon. There's no other explanation other than like just random noise. You know, maybe it's just fluctuations in the data. And they've done a statistical calculation, and that seems unlikely to like one part in a hundred or so. So it's not like smoking gun evidence again,
Starting point is 00:53:22 but it's a pretty nice signature of what could be a Neptune-sized exomeun. And we have more than one data point here in this case? Yeah, we have more than one shoulder. They've seen several transits of Kepler 1708. Oh, and it always has this little shoulder? Or would you expect it to sometimes have a shoulder, sometimes not have a shoulder because the moon is kind of going around the planet, right?
Starting point is 00:53:43 Exactly. So you expect the shoulder to vary, and they see it vary, and just the way you would. expect for a moon, right? It has the right wiggles at the right time. Like if you assume this moon, this Neptune size moon is going around every month and you see it in a monthly
Starting point is 00:54:00 way in the orbit of the planet around the star. Exactly. And in this case they're able to calculate the orbit of the moon around the planet. It has a period of several days. And so they factor that into their model. They have this mathematical model that says, here's the star, here's the planet, here's the moon going around it.
Starting point is 00:54:16 When should we expect to see dips from just the planet from the planet plus the moon from just the moon they can use that to predict very precisely the light curve they expect to see and it all lines up i mean in reality they've done it in reverse they said what mathematical model of that solar system would explain the dips that we see and the cool thing is that they can explain it and they can only explain it with a model that includes a moon pretty cool can they tell like how far away this moon is from its planet from the like the shoulders width or the size of the shoulder? That must be how they're estimating that it's Neptune size.
Starting point is 00:54:52 Or is it from how the light dips? It's definitely from how the light dips. The period comes from when those dips happen. So yeah, you can estimate the volume of that moon and the period of that moon. Cool. Well, was that a big deal when they discovered this or is this still something they're confirming? This is definitely something they're confirming. Nobody's like 100% sure that this is an exo moon.
Starting point is 00:55:15 It's like in the candidate stage. And they're planning to observe more with Hubble and with James Webb and with other devices. The next transit of this planet in the star was in March of this year. And so I hope that they got some data and they're analyzing it now. Yeah, as we speak, might be confirming this right now. And as more data comes in from more cool giants or more exoplanets, we're going to see more and more hints of exo moons until eventually this goes from like, maybe tentative discovery to like we are drowning in exo moons they're everywhere you know people who
Starting point is 00:55:49 get their PhD on like a single tentative discovery are going to be amazed when 10 years later people are doing their PhDs with thousands of candidates oh man I guess that's how it went with exoplanets right like people for work for a long time just to find one exoplanet and then as the technology and the techniques got better and now they're finding them by the thousands yeah exactly now people are doing like statistical analysis you know distributions of planet sizes They're looking at trends in these planets to try to understand what it means about how solar systems form. And so right now, we're at this very exciting moment. We're on the cusp of being able to see these exo moons.
Starting point is 00:56:24 And we know that as technology improves in the future, we're going to be able to ask and answer really interesting questions. Like how common is it to have hundreds of moons in a solar system or to have moons whose relative size is so big compared to the planet like ours is? I guess that's the big goal, right? is to compare other solar systems to ours. It's like our most solar systems out there like ours? Or is ours weird? And if it's weird, why is it weird, right? Yeah.
Starting point is 00:56:50 And is that weirdness crucial for life? Or maybe it hindered life here in our solar system and made it less likely, right? Maybe life is really, really common in the universe. And we were late to get started because we have a weird moon or not enough moons or too many moons or something. What we know is that there are going to be surprises. Like when we started discovering exoplanets, we were surprised by what we found. models of how the solar system formed have been completely upended by our discoveries about
Starting point is 00:57:16 exoplanets and exo moons i'm sure will also have lots of surprises yeah like it was a big surprise how many exoplanets there are out there right especially the ones that are like earth yeah exactly how many hot jupiters there were and the diversity of moons in just our solar system is crazy right we have moons that were formed with planets we have moons that were captured moons made out of weird stuff moons that might have come from collisions There are probably a whole other ways to make moons we haven't even thought of because they don't exist in our solar system. The diversity of exo moons is going to be really, really wild.
Starting point is 00:57:49 There's going to be some weird stuff out there. And moons have a big impact on life itself, right? Like think about how much of life on Earth is sort of sync to the lunar calendar. Yes, some people speculate that having such a big moon with its dramatic tides could have had a big impact on the formation of life here on Earth. People think that like in the brackish water between the freshwater and the salt water, that the sloshing around, the mixing up of all those chemicals in the primordial soup might have really helped life form.
Starting point is 00:58:18 And so having the moon there with its big dramatic tides could have been a big boost to the formation of life. It might be that it's crucial to have such a big moon. That'd be really fascinating, right? If we found life in other solar systems and in every case they had a weirdly big moon. Whoa. We might have the moon to thank for being here. Exactly.
Starting point is 00:58:37 Or it might be that mostly life is on moons, right? that maybe moons are a better place to have life than actually the surface of the planet. You know, we think that, for example, under the ice in Europa or inside Io or on Ganymi, there might still be life in our solar system. So it might be even in our solar system that is rare for life to start on a planet compared to moons. Yeah. It might be that life is over the moon about having a moon. And that joke.
Starting point is 00:59:08 Exactly. And people have really fun theories about how. life can evolve on these moons using like the planetary magnetic field as a shield from cosmic rays and being close to the star but avoiding being tightly locked to the star as all sorts of reasons why life could form on a moon and because there are so many more moons than planets we think that means even more places for life to start right right although aren't moons harder to have an atmosphere because they're smaller are smaller so it's harder to have an atmosphere but you can have life within those moons, right? You could have underwater oceans. Most life in the universe might be under
Starting point is 00:59:45 ice crusts. Whoa. They might be cooler than us or most certainly they are cooler than us, at least us here on the podcast. They might have no concept of the universe, right? If you form in a dark ocean, you can't even access the sky, right? You'd have to somehow drill a hole in that ice and climb out before you even know that the rest of the universe is there. What a crazy mind shift that would have to be. Well, there might be like how we thought about the Earth and the universe before, right? We thought there was a ceiling, basically. They might actually have a ceiling.
Starting point is 01:00:17 They might literally have a ceiling, exactly. Well, hopefully they'll blow the roof off of that bit of science there. We're always in awe of everything we discover and always surprised by what the universe has in store for us. Yeah, because I guess scientists are always aiming higher. They're always getting more and more ambitious. In other words, they're always shooting for the moon. All right, well, we hope you enjoyed that.
Starting point is 01:00:39 But thanks for joining us. See you next time. Thanks for listening. And remember that Daniel and Jorge Explain the Universe is a production of IHeartRadio. For more podcasts from IHeartRadio, visit the IHeartRadio app, Apple Podcasts, or wherever you listen to your favorite shows.
Starting point is 01:01:09 Every case that is a cold case that has DNA right now in a backlog will be identified in our lifetime. On the new podcast, America's Crime Lab, every case has a story to tell, and the DNA holds the truth. He never thought he was going to get caught, and I just looked at my computer screen. I was just like, ah, gotcha. This technology is already solving so many cases. Listen to America's Crime Lab on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. I'm Dr. Scott Barry Kaufman, host of the Psychology Podcast. Here's a clip from an upcoming conversation about how to be a better you. When you think about emotion regulation, you're not going to choose an adaptive strategy
Starting point is 01:01:58 which is more effortful to use unless you think there's a good outcome. Avoidance is easier. Ignoring is easier. Denials is easier. Complex problem solving. effort. Listen to the psychology podcast on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. Get fired up, y'all. Season two of Good Game with Sarah Spain is underway. We just welcomed one of my favorite people, an incomparable soccer icon, Megan Rapino, to the show, and we had a blast. Take a listen. Sue and I were like riding the lime bikes the other day and we're like, we're like, people write bikes because it's fun. We got more incredible guests like Megan in store, plus news of the day and more.
Starting point is 01:02:40 So make sure you listen to Good Game with Sarah Spain on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. Brought to you by Novartis, founding partner of IHeart Women's Sports Network. This is an IHeart podcast.

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