1 00:00:08,240 --> 00:00:11,600 Speaker 1: Hey, or hey, I have a question about stars, and 2 00:00:11,640 --> 00:00:14,880 Speaker 1: you're asking me. Is it about cartoon stars? Close? Actually 3 00:00:14,920 --> 00:00:18,080 Speaker 1: it's about Hollywood stars, all right? Yeah, I live next 4 00:00:18,120 --> 00:00:19,840 Speaker 1: to Hollywood, so I might be able to answer it. 5 00:00:19,880 --> 00:00:22,279 Speaker 1: What's the question, all right? How many stars can you 6 00:00:22,360 --> 00:00:26,759 Speaker 1: have in a single family, like media stars. Let's see, 7 00:00:26,800 --> 00:00:29,960 Speaker 1: there's the two athlete brothers. I think there are three 8 00:00:30,000 --> 00:00:34,640 Speaker 1: hemps Worth brothers, and there are four Baldwin brothers. What 9 00:00:34,720 --> 00:00:38,520 Speaker 1: about the Jackson five? That just might be the peak 10 00:00:38,680 --> 00:00:41,760 Speaker 1: of stardom in a family. Any denser with stars and 11 00:00:41,760 --> 00:00:47,839 Speaker 1: it might collapse into what a Paparassi black hole? That 12 00:00:47,920 --> 00:01:05,959 Speaker 1: sounds dense and dangerous. Hi am or him and cartoonists 13 00:01:05,959 --> 00:01:08,840 Speaker 1: and the creator of PhD comics. Hi, I'm Daniel. I'm 14 00:01:08,840 --> 00:01:11,679 Speaker 1: a particle physicist, and I was really disappointed the first 15 00:01:11,680 --> 00:01:14,760 Speaker 1: time I saw the walk of stars in Hollywood. Really 16 00:01:15,080 --> 00:01:19,080 Speaker 1: why it wasn't shiny enough for there were to those 17 00:01:19,120 --> 00:01:21,920 Speaker 1: chewing gum and cigarettes all over the place. Yeah, it 18 00:01:21,959 --> 00:01:25,240 Speaker 1: wasn't nearly as glamorous as I expected. And also I 19 00:01:25,240 --> 00:01:27,800 Speaker 1: didn't recognize the names of anybody I saw, So I 20 00:01:28,040 --> 00:01:30,280 Speaker 1: who are all these people? You mean? You're physicists and 21 00:01:30,280 --> 00:01:34,840 Speaker 1: you didn't know police making the movies or radio stars. Yeah, 22 00:01:34,880 --> 00:01:36,440 Speaker 1: it's always it's kind of weird to have your star 23 00:01:36,520 --> 00:01:38,880 Speaker 1: because it just makes people walk all over it all 24 00:01:38,880 --> 00:01:41,720 Speaker 1: the time. Put out their cigarette on your star on 25 00:01:41,760 --> 00:01:43,720 Speaker 1: the Walk of Fame. Think if they give you a 26 00:01:43,760 --> 00:01:45,640 Speaker 1: Nobel Prize and then they put the metal on the 27 00:01:45,680 --> 00:01:49,720 Speaker 1: floor in a busy intersection. Exactly. They don't pave the 28 00:01:49,760 --> 00:01:52,960 Speaker 1: streets with busts and Nobel Prize winners, right, but maybe 29 00:01:53,000 --> 00:01:55,960 Speaker 1: they should. They should. They need some more humility, for sure. 30 00:01:55,960 --> 00:01:57,960 Speaker 1: Would you take a Hollywood start they offered you one 31 00:01:58,200 --> 00:02:00,960 Speaker 1: for what? Maybe for a podcast? Sky's the limit for 32 00:02:01,040 --> 00:02:03,559 Speaker 1: this podcast. I would do anything for this podcast, even 33 00:02:03,600 --> 00:02:08,680 Speaker 1: except a Hollywood Walk of Fame star, But welcome to 34 00:02:08,760 --> 00:02:12,320 Speaker 1: that podcast. Daniel and Jorge explain the Universe aprilucent of 35 00:02:12,360 --> 00:02:15,320 Speaker 1: I Heart Radio, in which the universe is the star 36 00:02:15,480 --> 00:02:18,799 Speaker 1: and it's full of stars and we don't understand those stars, 37 00:02:18,840 --> 00:02:22,280 Speaker 1: but we'd like to, and so we apply our curiosity 38 00:02:22,320 --> 00:02:24,959 Speaker 1: and we serve on the waves of your curiosity to 39 00:02:25,000 --> 00:02:28,680 Speaker 1: ask the biggest, deepest questions about the universe, not just 40 00:02:28,800 --> 00:02:31,280 Speaker 1: about stars, about about where they come from and where 41 00:02:31,320 --> 00:02:33,840 Speaker 1: they end up, how they all work, and what it 42 00:02:33,960 --> 00:02:36,960 Speaker 1: all means. We don't shy away from anything in this podcast. 43 00:02:37,040 --> 00:02:39,040 Speaker 1: We ask all of it and we break it all 44 00:02:39,080 --> 00:02:41,320 Speaker 1: down to you in a way we hope makes sense 45 00:02:41,360 --> 00:02:43,600 Speaker 1: and maybe even makes you laugh. Yeah, because it is 46 00:02:43,600 --> 00:02:46,880 Speaker 1: a pretty famous universe. Although Daniel I thought we were 47 00:02:46,919 --> 00:02:49,280 Speaker 1: the stars of the podcast. Where are we the supporting 48 00:02:49,320 --> 00:02:53,359 Speaker 1: actors or the extras or are we like the catering service? Yes, 49 00:02:53,440 --> 00:02:56,040 Speaker 1: we are the service staff, the stars of the podcast. 50 00:02:56,040 --> 00:03:00,799 Speaker 1: Are you the listeners? Oh? Could save there? Yeah, we 51 00:03:00,919 --> 00:03:03,680 Speaker 1: like to talk about the amazing universe out there and 52 00:03:03,720 --> 00:03:06,240 Speaker 1: all of the famous stuff in it, especially the stars, 53 00:03:06,360 --> 00:03:08,200 Speaker 1: because I feel like the stars are the stars of 54 00:03:08,200 --> 00:03:11,600 Speaker 1: the universe. I'm just grateful that stars exist, that matter 55 00:03:11,720 --> 00:03:15,520 Speaker 1: forms these incredible clumbs that glow so brightly. Imagine if 56 00:03:15,560 --> 00:03:18,120 Speaker 1: most of the universe was dark, it wasn't glowing, it 57 00:03:18,160 --> 00:03:20,280 Speaker 1: would be so much harder to figure out what was 58 00:03:20,320 --> 00:03:23,440 Speaker 1: going on. So I'm grateful to these like lighthouses in 59 00:03:23,480 --> 00:03:26,480 Speaker 1: the universe that tell us what's going on and illuminated 60 00:03:26,520 --> 00:03:29,000 Speaker 1: for us. Like literally, Yeah, that's why. I mean, they're 61 00:03:29,040 --> 00:03:31,880 Speaker 1: like the stars of the universe, Like you know, they're 62 00:03:31,919 --> 00:03:34,120 Speaker 1: the main attraction. That's why people go to the universe. 63 00:03:34,560 --> 00:03:36,360 Speaker 1: That's why they stream it, that's why they down the 64 00:03:36,440 --> 00:03:39,120 Speaker 1: bootleg versions of it. That's right, And that's why people 65 00:03:39,160 --> 00:03:41,880 Speaker 1: like summer more than winter, right, because the Sun is 66 00:03:41,920 --> 00:03:46,080 Speaker 1: the star over closer to the star of our solar system. Yeah, exactly, 67 00:03:46,240 --> 00:03:48,880 Speaker 1: we feel closer to it, and we literally feel it's warmth. 68 00:03:48,920 --> 00:03:51,200 Speaker 1: I mean, it's incredible that this star, which is a 69 00:03:51,240 --> 00:03:54,800 Speaker 1: burning ball of plasma nine three million miles away, you 70 00:03:54,800 --> 00:03:57,640 Speaker 1: can still feel the heat of that with your bare hands. 71 00:03:58,080 --> 00:03:59,960 Speaker 1: You know, Like, have you ever been near a bond 72 00:04:00,080 --> 00:04:02,720 Speaker 1: fire that's so hot you can stand near it, take 73 00:04:02,760 --> 00:04:05,120 Speaker 1: a few steps back and it just dissipates. Right, Well, now, 74 00:04:05,160 --> 00:04:08,080 Speaker 1: imagine a bonfire so hot you can still feel its 75 00:04:08,120 --> 00:04:12,000 Speaker 1: heat ninety three million miles away. That's our star. It's 76 00:04:12,040 --> 00:04:14,480 Speaker 1: just it's mind boggling. Yeah, our star is it pretty 77 00:04:14,520 --> 00:04:17,839 Speaker 1: hot here. It's blowing up all the time. It should 78 00:04:17,880 --> 00:04:21,039 Speaker 1: get a star on the Walk of Fame. It's pretty famous. 79 00:04:21,320 --> 00:04:23,600 Speaker 1: It's the biggest star out there. We I like it, 80 00:04:23,720 --> 00:04:25,880 Speaker 1: you know, I mean I can't look at it directly, 81 00:04:26,160 --> 00:04:28,680 Speaker 1: but till its pressence half a half of the time. 82 00:04:28,760 --> 00:04:31,360 Speaker 1: It's been in a lot of movies, right, It's IMDb 83 00:04:31,480 --> 00:04:36,239 Speaker 1: page is amazing as a long list of credits. Yes, 84 00:04:36,440 --> 00:04:39,560 Speaker 1: every living human being, an animal, and plant and insect 85 00:04:40,480 --> 00:04:42,720 Speaker 1: is credited to our son exactly. It should at least 86 00:04:42,760 --> 00:04:45,919 Speaker 1: get acknowledgements in like every paper. Scientists should be acknowledging 87 00:04:45,920 --> 00:04:48,000 Speaker 1: it and thank you to the Sun for providing all 88 00:04:48,000 --> 00:04:50,800 Speaker 1: the energy we use. I'm gonna do that next time. Seriously, 89 00:04:50,880 --> 00:04:53,920 Speaker 1: it should get a Hollywood star on the Walk of Fame. 90 00:04:54,760 --> 00:04:57,080 Speaker 1: But it is pretty unique in our solar system. It 91 00:04:57,279 --> 00:05:00,360 Speaker 1: is basically the main thing in our solar system us right, 92 00:05:00,440 --> 00:05:02,880 Speaker 1: and our solar system, for the longest time, was the 93 00:05:02,920 --> 00:05:06,000 Speaker 1: only way we had to learn about this basic unit 94 00:05:06,040 --> 00:05:09,559 Speaker 1: of the universe, how solar systems and planetary systems work. 95 00:05:10,000 --> 00:05:11,840 Speaker 1: So for a long time we thought this was it, 96 00:05:11,920 --> 00:05:14,320 Speaker 1: that this was the way it happened, and we imagine 97 00:05:14,320 --> 00:05:17,279 Speaker 1: that maybe every other solar system looked like this. But 98 00:05:17,360 --> 00:05:19,440 Speaker 1: the more we look out in the universe, the more 99 00:05:19,480 --> 00:05:23,080 Speaker 1: we discover that things out there are weird, or that 100 00:05:23,200 --> 00:05:26,360 Speaker 1: we are weird, that we are unusual compared to what's 101 00:05:26,400 --> 00:05:29,400 Speaker 1: out there in the universe. So you gotta ask basic, 102 00:05:29,640 --> 00:05:32,880 Speaker 1: simple questions about how the universe works, because you might 103 00:05:32,960 --> 00:05:35,599 Speaker 1: be surprised by the answers. Yeah, well, I think we're 104 00:05:35,640 --> 00:05:39,080 Speaker 1: definitely weird that regardless of our son. What we do 105 00:05:39,120 --> 00:05:40,560 Speaker 1: you mean that you mean me? And you do you 106 00:05:40,560 --> 00:05:43,719 Speaker 1: mean the whole human race? You mean podcast listeners? I 107 00:05:43,720 --> 00:05:47,480 Speaker 1: mean like the royal We like the royal family, especially us, 108 00:05:47,640 --> 00:05:50,400 Speaker 1: the kings of this podcast. Do we have a dual 109 00:05:50,520 --> 00:05:52,480 Speaker 1: king monarchy in this podcast or is one of those 110 00:05:53,000 --> 00:05:58,400 Speaker 1: we're cokings. I think we're cokings. That's why we do 111 00:05:58,440 --> 00:06:02,040 Speaker 1: in this podcast. We coke up on the universe. We 112 00:06:02,200 --> 00:06:04,719 Speaker 1: sniff up the deliciousness of the universe. Oh man, I 113 00:06:04,720 --> 00:06:09,280 Speaker 1: was thinking coca cola, but dark the universe is my drug. Man, 114 00:06:09,480 --> 00:06:12,520 Speaker 1: the universe. It does get you high. But anyways, it 115 00:06:12,600 --> 00:06:15,800 Speaker 1: is a pretty special star. And I wonder, Daniel, when 116 00:06:15,920 --> 00:06:18,040 Speaker 1: you mentioned like other stars in other parts of the universe. 117 00:06:18,240 --> 00:06:20,880 Speaker 1: I wonder when in human history we realized that our 118 00:06:20,960 --> 00:06:23,560 Speaker 1: sun was a star, just like those little pin points 119 00:06:23,560 --> 00:06:25,159 Speaker 1: you see in the night sky. Like, was that a 120 00:06:25,160 --> 00:06:28,560 Speaker 1: big revelation for people? It was a big revelation, absolutely, 121 00:06:28,920 --> 00:06:30,560 Speaker 1: And you know that kind of revelation is a few 122 00:06:30,640 --> 00:06:33,720 Speaker 1: hundred years old. But there was this moment, like a 123 00:06:33,720 --> 00:06:37,320 Speaker 1: few hundred years ago when Newton and others realized that 124 00:06:37,360 --> 00:06:40,320 Speaker 1: there was probably one set of laws of physics, and 125 00:06:40,320 --> 00:06:43,599 Speaker 1: those laws applied equally to like things here on Earth 126 00:06:43,960 --> 00:06:47,520 Speaker 1: and motion of things in the sky, including the Sun, 127 00:06:47,640 --> 00:06:51,120 Speaker 1: and including all those stars, and so understanding that the 128 00:06:51,160 --> 00:06:54,200 Speaker 1: Sun was a star suggested that all those other pin 129 00:06:54,240 --> 00:06:57,520 Speaker 1: pricks in the sky were also probably solar systems that 130 00:06:57,600 --> 00:07:00,480 Speaker 1: might have planets on them. And you write that realization 131 00:07:00,600 --> 00:07:02,760 Speaker 1: is just a few hundred years old. But what a 132 00:07:02,880 --> 00:07:05,960 Speaker 1: mind blowing idea to realize, you know, that we are 133 00:07:06,040 --> 00:07:09,640 Speaker 1: one of billions and billions and billions. That really must 134 00:07:09,680 --> 00:07:12,119 Speaker 1: shake the whole foundation of what you think it means 135 00:07:12,160 --> 00:07:14,280 Speaker 1: to be human. Makes it a little less unique, like 136 00:07:14,480 --> 00:07:16,680 Speaker 1: less of a star of the universe, to think that, 137 00:07:16,720 --> 00:07:19,360 Speaker 1: you know, there's zillions of suns out there. Yeah, but 138 00:07:19,400 --> 00:07:22,480 Speaker 1: it immediately begs lots of other questions, like what are 139 00:07:22,520 --> 00:07:25,080 Speaker 1: those stars? Like? What are those solar systems? Like? Are 140 00:07:25,120 --> 00:07:28,320 Speaker 1: their planets in life around those solar systems? While it 141 00:07:28,480 --> 00:07:30,800 Speaker 1: suggests that there might be, because we know that our 142 00:07:30,880 --> 00:07:34,280 Speaker 1: sun is not rare or weird or interesting, that it's 143 00:07:34,280 --> 00:07:36,720 Speaker 1: just one of billions, we don't actually know and until 144 00:07:36,880 --> 00:07:40,520 Speaker 1: recently we hadn't seen planets around any other star. Until 145 00:07:40,560 --> 00:07:44,040 Speaker 1: like twenty thirty years ago, we'd never observed a planet 146 00:07:44,040 --> 00:07:46,320 Speaker 1: around a star other than our own. It could have 147 00:07:46,360 --> 00:07:50,360 Speaker 1: been that our Solar system was the only one with planets, right, 148 00:07:50,400 --> 00:07:53,080 Speaker 1: How weird would that have been, right? Yeah, although you 149 00:07:53,120 --> 00:07:55,440 Speaker 1: have to assume that their movies are in a different language. 150 00:07:56,240 --> 00:07:59,600 Speaker 1: So maybe you know there's like a local star. Maybe 151 00:08:00,160 --> 00:08:04,000 Speaker 1: everyone's famous in that in Poland? Isn't that the same throughout? 152 00:08:04,000 --> 00:08:07,320 Speaker 1: I'm world famous in Poland? That's a classic mel Brooks joke. Yeah, 153 00:08:07,320 --> 00:08:10,040 Speaker 1: but we didn't know, like maybe the planetary formation was 154 00:08:10,120 --> 00:08:13,480 Speaker 1: really unusual, and most stars just form as stars, right, 155 00:08:13,520 --> 00:08:15,720 Speaker 1: They gather up all the stuff and that's it. You 156 00:08:15,800 --> 00:08:18,600 Speaker 1: just have stars, and having planets is weird and results 157 00:08:18,600 --> 00:08:21,320 Speaker 1: of some strange fluctuation. Now, of course we know the 158 00:08:21,360 --> 00:08:24,160 Speaker 1: opposite is true, that planets are totally normal, and that 159 00:08:24,280 --> 00:08:27,360 Speaker 1: most solar systems have planets, that their planets everywhere. There's 160 00:08:27,400 --> 00:08:29,920 Speaker 1: billions and trillions of planets out there, right, And I 161 00:08:29,960 --> 00:08:32,200 Speaker 1: think something interesting is that I think by now maybe 162 00:08:32,320 --> 00:08:35,120 Speaker 1: most people know that all stars out there are suns, 163 00:08:35,600 --> 00:08:37,040 Speaker 1: but I think most people assume them. When you look 164 00:08:37,080 --> 00:08:39,880 Speaker 1: at a star in the night sky, it's like one star, 165 00:08:40,200 --> 00:08:42,800 Speaker 1: like one sun that you're looking at, like each pinpoint 166 00:08:42,920 --> 00:08:46,880 Speaker 1: is this this one specific sun that's shining. But that's 167 00:08:46,880 --> 00:08:50,160 Speaker 1: not necessarily true, right, that's right, it's not necessarily true. 168 00:08:50,559 --> 00:08:54,360 Speaker 1: It turns out that sometimes stars formed together, and then 169 00:08:54,400 --> 00:08:58,280 Speaker 1: you can have more than one star in a solar system. 170 00:08:58,320 --> 00:09:01,679 Speaker 1: And if they're really far away, basically every other star is, 171 00:09:01,800 --> 00:09:05,000 Speaker 1: it's not always easy to make them out by I. So, 172 00:09:05,000 --> 00:09:07,120 Speaker 1: so some things that you see in the sky might 173 00:09:07,160 --> 00:09:11,320 Speaker 1: be binary or triinary or even crazier star systems. Yeah, 174 00:09:11,360 --> 00:09:13,480 Speaker 1: but they're so far away they they look like one 175 00:09:13,520 --> 00:09:15,880 Speaker 1: pin point, right, Yeah, unless you have a really powerful 176 00:09:15,880 --> 00:09:19,560 Speaker 1: telescope or use some cool techniques we're gonna talk about today, 177 00:09:19,679 --> 00:09:22,920 Speaker 1: it's pretty hard to tell if it's one star or several. 178 00:09:23,040 --> 00:09:24,960 Speaker 1: And so today on the podcast, we'll be asking the 179 00:09:25,040 --> 00:09:35,440 Speaker 1: question how many stars can a solar system have? Now, Daniel, 180 00:09:35,480 --> 00:09:38,440 Speaker 1: are these like still our stars? Are these like YELP 181 00:09:38,480 --> 00:09:42,040 Speaker 1: review stars? There's no limit on how many stars you 182 00:09:42,040 --> 00:09:43,640 Speaker 1: can give on YELL. I think you can be like, 183 00:09:44,920 --> 00:09:47,680 Speaker 1: I think five is the most? Can you give ten stars? 184 00:09:47,679 --> 00:09:50,040 Speaker 1: And yell? Isn't there some premium subscription version we can 185 00:09:50,040 --> 00:09:52,280 Speaker 1: give as many stars that you want and if not, yelp, 186 00:09:52,360 --> 00:09:55,959 Speaker 1: I totally suggest you offer that to people. Yeah, let 187 00:09:56,000 --> 00:09:58,880 Speaker 1: people be effusive, right, because I would give our solar 188 00:09:58,920 --> 00:10:02,760 Speaker 1: system totally t out of five stars only ten, Daniel, 189 00:10:02,880 --> 00:10:05,520 Speaker 1: Come on, I mean that's double the maximum and being 190 00:10:05,559 --> 00:10:09,520 Speaker 1: generous here, like, like, are you looking at other solar 191 00:10:09,559 --> 00:10:12,800 Speaker 1: systems thinking maybe they have better boba ti or pizza. 192 00:10:13,040 --> 00:10:14,440 Speaker 1: I don't need to have options. I can go to 193 00:10:14,440 --> 00:10:16,960 Speaker 1: a restaurant and I can rate it just on its food. 194 00:10:17,000 --> 00:10:19,120 Speaker 1: I don't need to compare it to the other restaurants 195 00:10:19,120 --> 00:10:21,480 Speaker 1: in town. I can say five out of five would 196 00:10:21,520 --> 00:10:23,439 Speaker 1: have that falafel again, and in the same way, I 197 00:10:23,520 --> 00:10:26,760 Speaker 1: can say ten out of five. I would totally evolve here. Again, 198 00:10:27,600 --> 00:10:29,720 Speaker 1: it seems really unscientific of you, Daniel. I would have 199 00:10:29,920 --> 00:10:33,800 Speaker 1: expected something more systematic, you know, like, are you assuming 200 00:10:33,840 --> 00:10:37,240 Speaker 1: you've tasted every pizza in the universe? Sometimes my belly 201 00:10:37,280 --> 00:10:40,480 Speaker 1: feels like I have. But no, I it's purely subjective. 202 00:10:40,559 --> 00:10:43,160 Speaker 1: I totally agree. I have no scientific system for rating 203 00:10:43,280 --> 00:10:45,920 Speaker 1: solar systems. Well, I would give our solars some I 204 00:10:45,920 --> 00:10:49,560 Speaker 1: guess infinity stars because you know I'm here because of it, 205 00:10:49,679 --> 00:10:53,440 Speaker 1: and that's worth an infinite amount of a value to me. Well, 206 00:10:53,440 --> 00:10:55,200 Speaker 1: I'm glad that you don't forget the little stars that 207 00:10:55,240 --> 00:10:58,240 Speaker 1: helped you along the way. Our star is a little underdog, 208 00:10:58,679 --> 00:11:00,640 Speaker 1: but yeah, it's it's kind of an interesting question. How 209 00:11:00,640 --> 00:11:03,319 Speaker 1: many stars can a solar system have? Like we know 210 00:11:03,520 --> 00:11:06,320 Speaker 1: our solar system has one, and we know that their 211 00:11:06,360 --> 00:11:08,760 Speaker 1: binary star systems out there, but like how many can 212 00:11:08,800 --> 00:11:11,920 Speaker 1: you fit into one place? Like ten twenty? And these 213 00:11:11,920 --> 00:11:14,320 Speaker 1: are my favorite kinds of questions, the one that are 214 00:11:14,400 --> 00:11:16,600 Speaker 1: very simple and just sort of like blow up basic 215 00:11:16,640 --> 00:11:19,960 Speaker 1: assumptions you maybe never thought to ask about. Like people 216 00:11:20,000 --> 00:11:22,520 Speaker 1: are now cool with wondering how many planets could there 217 00:11:22,520 --> 00:11:25,680 Speaker 1: be in imagining solar systems with like twenty planets or 218 00:11:25,720 --> 00:11:28,480 Speaker 1: just two planets or like really big weird planets or 219 00:11:28,520 --> 00:11:31,000 Speaker 1: fluffy planets or something. People are like sort of stretch 220 00:11:31,080 --> 00:11:32,960 Speaker 1: their mind that way. But I think a lot of 221 00:11:32,960 --> 00:11:35,200 Speaker 1: people haven't really bent their minds in the other direction. 222 00:11:35,240 --> 00:11:37,559 Speaker 1: I think most people think of a solar system is 223 00:11:37,640 --> 00:11:40,200 Speaker 1: like a star with stuff around it, And so I 224 00:11:40,240 --> 00:11:43,640 Speaker 1: think it's really good to like remind ourselves that the 225 00:11:43,679 --> 00:11:46,880 Speaker 1: example we see, what we sort of define our existence around, 226 00:11:47,080 --> 00:11:49,960 Speaker 1: isn't necessarily representative. That we've got to keep our minds 227 00:11:50,000 --> 00:11:53,280 Speaker 1: open to other kinds of stellar families. Yeah, and it 228 00:11:53,320 --> 00:11:55,040 Speaker 1: made me think of Star Wars, you know, and that 229 00:11:55,120 --> 00:11:58,160 Speaker 1: famous scene in that first movie where Luke Skywalker is 230 00:11:58,200 --> 00:12:00,280 Speaker 1: looking out into the horizon and he see there are 231 00:12:00,280 --> 00:12:03,320 Speaker 1: two stars in the sky. I know that's crazy and 232 00:12:03,320 --> 00:12:05,520 Speaker 1: it would make for a crazy like pattern of day 233 00:12:05,559 --> 00:12:06,760 Speaker 1: and night. I don't know how you could be a 234 00:12:06,760 --> 00:12:09,480 Speaker 1: farmer on a planet with two sons. You'd have two ships. 235 00:12:09,520 --> 00:12:14,000 Speaker 1: Maybe you have some crazy almanac. You're like, Okay, it's summer, now, 236 00:12:14,000 --> 00:12:16,960 Speaker 1: it's double summer. Now, it's half summer. Now it's sort 237 00:12:17,000 --> 00:12:19,360 Speaker 1: of winter. You know, like if the seasons it would 238 00:12:19,360 --> 00:12:22,000 Speaker 1: just be nuts, right right, Well, let's get into it, Daniel, 239 00:12:22,000 --> 00:12:24,480 Speaker 1: how many stars can a solar system have? And so, 240 00:12:24,520 --> 00:12:26,360 Speaker 1: as usually, we were wondering how many people out there 241 00:12:26,360 --> 00:12:28,760 Speaker 1: have thought about this question or even knew that you 242 00:12:28,800 --> 00:12:31,160 Speaker 1: could have more than one or two stars in a 243 00:12:31,240 --> 00:12:34,160 Speaker 1: solar system. So Daniel went out there into the wild 244 00:12:34,200 --> 00:12:36,760 Speaker 1: for the internet to ask people how many stars can 245 00:12:36,840 --> 00:12:39,480 Speaker 1: a solar system have? So thank you very much to 246 00:12:39,559 --> 00:12:42,480 Speaker 1: everybody who participated. If you are out there and been 247 00:12:42,480 --> 00:12:44,800 Speaker 1: listening to the podcast and never have lent your voice 248 00:12:44,800 --> 00:12:47,520 Speaker 1: to these questions. Please write to us two questions at 249 00:12:47,600 --> 00:12:50,640 Speaker 1: Daniel and Jorge dot com. No pressure, but I think 250 00:12:50,640 --> 00:12:53,360 Speaker 1: you'll love it. Here's what people had to say. I 251 00:12:53,360 --> 00:12:57,680 Speaker 1: hadn't really considered that, but I know that, Um, a 252 00:12:57,760 --> 00:13:02,600 Speaker 1: large number of solar systems. Do you have at least 253 00:13:03,000 --> 00:13:07,080 Speaker 1: two stars? There might be somewhere three, but I'm not 254 00:13:07,160 --> 00:13:13,319 Speaker 1: actually sure the maximum. So yeah, I think a solar 255 00:13:13,360 --> 00:13:16,480 Speaker 1: system can have more than one star. I remember seeing 256 00:13:16,480 --> 00:13:21,240 Speaker 1: something on the television about a binary star system, so 257 00:13:21,280 --> 00:13:24,280 Speaker 1: I think it can have more than one star. I 258 00:13:24,320 --> 00:13:28,480 Speaker 1: think a solar system can have one or two stars. Um, 259 00:13:28,559 --> 00:13:32,040 Speaker 1: we have one star that is our sun, and then 260 00:13:32,440 --> 00:13:37,040 Speaker 1: there are binary systems, which consists of two stars orbiting 261 00:13:37,080 --> 00:13:42,360 Speaker 1: around each other, and I think it is possible for 262 00:13:42,480 --> 00:13:47,040 Speaker 1: there to be like planetary objects orbiting them. You have 263 00:13:47,640 --> 00:13:51,560 Speaker 1: binary stars and triple star systems. Whether there's any limit 264 00:13:51,600 --> 00:13:56,160 Speaker 1: onto it, I doubt it. As long as it's contentionally locked. 265 00:13:56,720 --> 00:13:59,080 Speaker 1: I don't think they se limit. But at some point 266 00:13:59,440 --> 00:14:03,160 Speaker 1: it will stop being a solar system become a galaxy. Well, 267 00:14:04,360 --> 00:14:07,360 Speaker 1: I know that there are binary systems, which would mean 268 00:14:07,440 --> 00:14:12,520 Speaker 1: two stars. I don't see why they couldn't be three stars. 269 00:14:13,760 --> 00:14:17,560 Speaker 1: I in a solar system, and I think I saw 270 00:14:17,600 --> 00:14:22,520 Speaker 1: a science fiction program where they mentioned as seven star 271 00:14:22,680 --> 00:14:26,880 Speaker 1: solar system, but that was science fiction, probably not based 272 00:14:26,920 --> 00:14:31,040 Speaker 1: in fact. But I really don't know what the upper 273 00:14:31,080 --> 00:14:37,080 Speaker 1: limit would be, probably something between three and seven. I'm 274 00:14:37,200 --> 00:14:42,760 Speaker 1: not sure of a physical limit. A solar system can 275 00:14:42,920 --> 00:14:47,000 Speaker 1: certainly have multiple stars. I know binary stars are very common. 276 00:14:48,000 --> 00:14:50,440 Speaker 1: I'm not sure if there's anything to say that you 277 00:14:50,480 --> 00:14:55,840 Speaker 1: couldn't have ten stars or in some amazing orbit around 278 00:14:55,880 --> 00:14:59,640 Speaker 1: each other. I suspect in nurse stellar nursery, whether they're 279 00:14:59,640 --> 00:15:01,840 Speaker 1: all quite compact. You have a lot of stars in 280 00:15:02,080 --> 00:15:06,480 Speaker 1: close proximity that have a gravitational impact on each other. Well, 281 00:15:07,000 --> 00:15:10,640 Speaker 1: a solar system, you can probably have a bunch of 282 00:15:10,640 --> 00:15:13,560 Speaker 1: stars I know are obviously our solar system has one, 283 00:15:13,880 --> 00:15:17,800 Speaker 1: and I know that many of the stars solar systems 284 00:15:17,800 --> 00:15:20,480 Speaker 1: out there have two stars. And I'm sure you can 285 00:15:20,520 --> 00:15:23,080 Speaker 1: have like a trinary system. I feel like I've seen 286 00:15:23,120 --> 00:15:25,400 Speaker 1: a couple of movies with that. I don't know if 287 00:15:25,400 --> 00:15:27,440 Speaker 1: there's a fundamental limit, but I know it gets a 288 00:15:27,440 --> 00:15:30,360 Speaker 1: little harder to get all the equations to balance out 289 00:15:30,760 --> 00:15:32,920 Speaker 1: if you have more and more stars. Things get a 290 00:15:32,960 --> 00:15:35,600 Speaker 1: little chaotic when you have a bunch of things orbiting 291 00:15:35,640 --> 00:15:39,200 Speaker 1: each other. So I'm gonna go with maybe three might 292 00:15:39,200 --> 00:15:42,320 Speaker 1: be sort of like the practical limit, but maybe there's 293 00:15:42,320 --> 00:15:45,320 Speaker 1: some more, all right, A lot of guessing. Most people 294 00:15:45,320 --> 00:15:47,280 Speaker 1: start to like one or two. I guess you don't 295 00:15:47,320 --> 00:15:51,040 Speaker 1: hear about like a three or more than two star system, right, Like, 296 00:15:51,320 --> 00:15:54,040 Speaker 1: I feel like binary star is a common phrase. Yeah, 297 00:15:54,120 --> 00:15:56,040 Speaker 1: people are being conservative here. They're not, like, you know, 298 00:15:56,240 --> 00:15:59,760 Speaker 1: reaching out and imagining solar systems with like fifties stars 299 00:15:59,760 --> 00:16:01,360 Speaker 1: and of and stuff like that. I think it just 300 00:16:01,400 --> 00:16:03,880 Speaker 1: goes to show you that people think of solar systems 301 00:16:04,080 --> 00:16:06,800 Speaker 1: as dominated by a star or maybe two and then 302 00:16:06,840 --> 00:16:08,960 Speaker 1: planets around it. Right. I guess it's hard to wrap 303 00:16:09,040 --> 00:16:10,800 Speaker 1: your head a right, it might just be like chaos, 304 00:16:10,920 --> 00:16:13,200 Speaker 1: like who would win or who would be the dominant star? 305 00:16:13,320 --> 00:16:15,480 Speaker 1: Or why wouldn't they just crash into each other? Yeah, 306 00:16:15,520 --> 00:16:17,400 Speaker 1: you feel like a solar system has to have somebody 307 00:16:17,400 --> 00:16:19,320 Speaker 1: in charge. Well, it could be like a committee run 308 00:16:19,520 --> 00:16:22,680 Speaker 1: solar system, you know, majority rules or you know, I'm 309 00:16:22,720 --> 00:16:25,680 Speaker 1: sure they use the Robert's rule to make decisions about 310 00:16:25,840 --> 00:16:27,680 Speaker 1: orbits and things like that. So you're in favor of 311 00:16:27,680 --> 00:16:31,360 Speaker 1: socialism when it comes to organisms, sellar Sylar semi favorite 312 00:16:31,400 --> 00:16:37,080 Speaker 1: solar socialism. Yes, the s S s S cosmic social 313 00:16:37,120 --> 00:16:43,160 Speaker 1: Society of Socialist Solar Systems and communistic cosmologists. Nice. Nice, 314 00:16:43,760 --> 00:16:46,040 Speaker 1: but then it gets all eaten up by a democratic 315 00:16:46,120 --> 00:16:50,760 Speaker 1: dark matter. Unfortunately, dark matter will totally win the vote, 316 00:16:50,760 --> 00:16:53,600 Speaker 1: actually because it totally would out vote us. Right, we 317 00:16:53,680 --> 00:16:57,480 Speaker 1: do not want there, you go, it's more autocratic, I think, 318 00:16:57,680 --> 00:17:00,680 Speaker 1: astronomically autocratic. Yeah, it's just like an some countries they 319 00:17:00,720 --> 00:17:03,480 Speaker 1: have more animals than people, like Denmark has more pigs 320 00:17:03,560 --> 00:17:05,680 Speaker 1: than people, and so if they give pigs the vote, 321 00:17:05,920 --> 00:17:08,080 Speaker 1: the people will probably get voted out of office. Well, 322 00:17:08,160 --> 00:17:11,520 Speaker 1: let's not make any politician jokes here with pigs. You 323 00:17:11,720 --> 00:17:16,040 Speaker 1: just did, No, I didn't. But I like this person 324 00:17:16,080 --> 00:17:18,760 Speaker 1: who said that they've seen a star system with seven 325 00:17:18,840 --> 00:17:22,560 Speaker 1: stars in science fiction. Yeah. Yeah, that means that authors 326 00:17:22,600 --> 00:17:25,800 Speaker 1: out there have been creative in imagining the in stellar systems. 327 00:17:25,880 --> 00:17:28,960 Speaker 1: So again, kudos to science fiction authors, right, or like 328 00:17:29,000 --> 00:17:31,440 Speaker 1: Avengers movies. I feel like those Avengers movies have like, 329 00:17:31,920 --> 00:17:34,879 Speaker 1: you know, twenty stars in them, and did you give 330 00:17:34,960 --> 00:17:39,000 Speaker 1: them all five stars? On yell IMDb? Daniel? Are you 331 00:17:39,080 --> 00:17:43,359 Speaker 1: reviewing movies on yelled? But Anyways, let's get into Daniel. 332 00:17:43,359 --> 00:17:45,800 Speaker 1: I guess most people seem to know about binary stars, 333 00:17:45,880 --> 00:17:48,159 Speaker 1: and I'm sure that just means that has two stars. 334 00:17:48,320 --> 00:17:51,119 Speaker 1: So let's talk about for binary star system how common 335 00:17:51,160 --> 00:17:53,480 Speaker 1: are they and how can they come to be? Like 336 00:17:53,520 --> 00:17:55,320 Speaker 1: how do you get a star system with two stars 337 00:17:55,359 --> 00:17:57,960 Speaker 1: in it? Yeah, most of them are binary star systems, 338 00:17:58,000 --> 00:18:01,320 Speaker 1: but we'll talk later about solar systems with even more stars. 339 00:18:01,680 --> 00:18:04,160 Speaker 1: But it's not rare at all. So it's a third 340 00:18:04,240 --> 00:18:06,240 Speaker 1: of the stars in the solar system are in a 341 00:18:06,400 --> 00:18:08,560 Speaker 1: binary star system. So like when I look at the 342 00:18:08,680 --> 00:18:11,120 Speaker 1: night sky, a third of the stars that I'm looking 343 00:18:11,160 --> 00:18:14,159 Speaker 1: at are actually two stars. Yeah, exactly. Wow, So if 344 00:18:14,240 --> 00:18:16,639 Speaker 1: I look out and I'm seeing double it's I'm about 345 00:18:16,680 --> 00:18:19,720 Speaker 1: a third, right, Like it's not in my eyesight necessarily, yeah, 346 00:18:19,920 --> 00:18:22,760 Speaker 1: or you know, stop having drinks or whatever, but yeah, exactly. 347 00:18:22,800 --> 00:18:24,960 Speaker 1: There are lots and lots and lots of double star 348 00:18:25,040 --> 00:18:28,240 Speaker 1: systems out there, something we really didn't imagine until recently. 349 00:18:28,240 --> 00:18:30,600 Speaker 1: It turns out to be really pretty common. So I 350 00:18:30,680 --> 00:18:33,040 Speaker 1: guess maybe a question is how do they form? Like 351 00:18:33,280 --> 00:18:35,879 Speaker 1: why didn't they just form as one star? How did 352 00:18:35,920 --> 00:18:37,639 Speaker 1: they come to have two stars? Right? Well, you have 353 00:18:37,720 --> 00:18:40,280 Speaker 1: to imagine how solar systems form. Right, you have this 354 00:18:40,400 --> 00:18:44,240 Speaker 1: big cloud of gas and dust initial building blocks of 355 00:18:44,320 --> 00:18:47,400 Speaker 1: the solar system. What makes that collapse? Right? What makes 356 00:18:47,440 --> 00:18:50,320 Speaker 1: that collapse into a star? Sometimes you get like a 357 00:18:50,400 --> 00:18:53,119 Speaker 1: shock wave that comes through from like a supernova or 358 00:18:53,160 --> 00:18:55,720 Speaker 1: something that triggers this collapse. But often you have a 359 00:18:55,800 --> 00:18:58,840 Speaker 1: really big cloud that's too big for just one star 360 00:18:59,000 --> 00:19:01,600 Speaker 1: to form. So we call these like stellar nurseries. You 361 00:19:01,640 --> 00:19:04,399 Speaker 1: get like bunches and bunches of stars all forming at 362 00:19:04,440 --> 00:19:07,920 Speaker 1: the same time. And so sometimes those stars formed close 363 00:19:08,080 --> 00:19:10,600 Speaker 1: enough that they start to tug on each other, and 364 00:19:10,680 --> 00:19:12,720 Speaker 1: they pull on each other, and then they become a 365 00:19:12,760 --> 00:19:16,040 Speaker 1: binary star system. So like you could have formed a 366 00:19:16,240 --> 00:19:19,199 Speaker 1: larger star right in the middle, But where the stars 367 00:19:19,240 --> 00:19:21,959 Speaker 1: actually form depends a little bit on like what happens 368 00:19:21,960 --> 00:19:24,080 Speaker 1: to be a little bit denser, because remember this is 369 00:19:24,119 --> 00:19:27,359 Speaker 1: a gravitational process, and so the dense spot pulls on 370 00:19:27,520 --> 00:19:30,760 Speaker 1: other stuff and accumulates. It's a runaway process, and so 371 00:19:30,920 --> 00:19:33,080 Speaker 1: you just happen to have like two spots that are 372 00:19:33,080 --> 00:19:35,200 Speaker 1: a little denser, a little closer to each other. You 373 00:19:35,280 --> 00:19:37,920 Speaker 1: can get stars forming close enough to form a binary 374 00:19:37,960 --> 00:19:40,560 Speaker 1: star system. I guess they each are sort of dominant 375 00:19:40,600 --> 00:19:43,119 Speaker 1: in their little region. But it just so happens that 376 00:19:43,240 --> 00:19:45,520 Speaker 1: the two reunions are sort of close enough together that 377 00:19:45,600 --> 00:19:48,680 Speaker 1: they form a system together. Yeah, and you can imagine 378 00:19:48,680 --> 00:19:52,239 Speaker 1: it's not that different from our Sun and Jupiter. If 379 00:19:52,320 --> 00:19:54,800 Speaker 1: Jupiter was a little bit bigger. You know, it has 380 00:19:54,840 --> 00:19:57,680 Speaker 1: like only one percent of the mass of the Solar system. 381 00:19:57,720 --> 00:20:00,240 Speaker 1: If it had like a little bit more, you could 382 00:20:00,280 --> 00:20:03,239 Speaker 1: call that thing a star. So why didn't Jupiter get 383 00:20:03,320 --> 00:20:04,840 Speaker 1: more mass? Well, you know, if it's been a little 384 00:20:04,880 --> 00:20:07,840 Speaker 1: bit further away, or the dynamics of how things have 385 00:20:07,920 --> 00:20:10,080 Speaker 1: been distributed had been different, you might have had a 386 00:20:10,160 --> 00:20:13,560 Speaker 1: more balanced distribution between the Sun and Jupiter. Interesting, like 387 00:20:13,640 --> 00:20:16,080 Speaker 1: we could have had a binary system. Like if Jupiter 388 00:20:16,240 --> 00:20:19,159 Speaker 1: had turned on or eating more of that infinite pizza, 389 00:20:19,359 --> 00:20:22,240 Speaker 1: we would have like a second star in our sky. Yeah. 390 00:20:22,359 --> 00:20:24,600 Speaker 1: So it's just an example of how out of basically 391 00:20:24,640 --> 00:20:27,359 Speaker 1: a single cloud of stuff, you can have two foulside, right, 392 00:20:27,359 --> 00:20:30,560 Speaker 1: you can have two places where things start to accumulate 393 00:20:30,840 --> 00:20:33,880 Speaker 1: and doesn't always just collapse down to one. So that's 394 00:20:33,880 --> 00:20:35,960 Speaker 1: a good example, and you know a little bit different, 395 00:20:36,000 --> 00:20:37,960 Speaker 1: and yeah, we could have had a binary star system. 396 00:20:38,040 --> 00:20:41,080 Speaker 1: We could have been tattooeding basically right, although it wouldn't 397 00:20:41,080 --> 00:20:43,000 Speaker 1: They wouldn't look that big, right, Like the Sun would 398 00:20:43,000 --> 00:20:45,040 Speaker 1: look really big in our sky, but Jupiter would just 399 00:20:45,119 --> 00:20:47,920 Speaker 1: look like a pinpoint, wouldn't it. Well, Jupiter is much 400 00:20:47,960 --> 00:20:50,920 Speaker 1: further away than the Sun, and so it does look 401 00:20:51,000 --> 00:20:53,320 Speaker 1: a lot less bright for that reason. But it depends, 402 00:20:53,359 --> 00:20:55,520 Speaker 1: you know, on how things work. If Jupiter had been bigger, 403 00:20:55,560 --> 00:20:57,240 Speaker 1: it probably would have ended up in a different spot 404 00:20:57,320 --> 00:20:59,560 Speaker 1: in the Solar system. We had this whole fun podcast 405 00:20:59,600 --> 00:21:02,280 Speaker 1: episode how Jupiter ended up where it is, and it 406 00:21:02,359 --> 00:21:04,639 Speaker 1: sort of drifted towards the center of the Solar system 407 00:21:04,680 --> 00:21:06,960 Speaker 1: and then Saturn wrangled it and pulled it back out. 408 00:21:07,320 --> 00:21:09,399 Speaker 1: But if Jupiter had been bigger, it might have just 409 00:21:09,560 --> 00:21:11,399 Speaker 1: drifted towards the inner part of the Solar system and 410 00:21:11,480 --> 00:21:14,280 Speaker 1: formed a very tight binary spiral with our son, or 411 00:21:14,440 --> 00:21:16,760 Speaker 1: they might have even merged. I guess the question for 412 00:21:16,920 --> 00:21:18,760 Speaker 1: me is that if you have these two big things 413 00:21:18,800 --> 00:21:21,679 Speaker 1: in the Solar system, why don't they just crash into 414 00:21:21,760 --> 00:21:24,840 Speaker 1: each other? I think that's one question, And the other 415 00:21:24,920 --> 00:21:27,639 Speaker 1: question is what is it like to have two stars 416 00:21:27,680 --> 00:21:29,639 Speaker 1: in your Solar system? And so let's get into that 417 00:21:29,800 --> 00:21:34,200 Speaker 1: and maybe more star systems, but more stars in them 418 00:21:34,240 --> 00:21:49,520 Speaker 1: than two. But first, let's take a quick break. We're 419 00:21:49,520 --> 00:21:53,560 Speaker 1: talking about two star systems, systems with multiple stars in them, 420 00:21:53,760 --> 00:21:55,760 Speaker 1: and we started with two. Daniel, what is it like 421 00:21:55,960 --> 00:21:58,199 Speaker 1: to have a two stars in your system? Like, well, 422 00:21:58,280 --> 00:22:00,520 Speaker 1: wouldn't the two stars just crash into each other or 423 00:22:00,640 --> 00:22:04,040 Speaker 1: suck each other up? Well, things can be in stable orbits. Right, 424 00:22:04,080 --> 00:22:06,160 Speaker 1: It's like asking the question why doesn't the Earth get 425 00:22:06,240 --> 00:22:08,800 Speaker 1: sucked into the Sun For the same reason, it has 426 00:22:08,880 --> 00:22:11,520 Speaker 1: the right velocity and the right direction to be in 427 00:22:11,600 --> 00:22:14,080 Speaker 1: a stable orbit. As two objects approach each other, it's 428 00:22:14,119 --> 00:22:17,000 Speaker 1: possible for them to crash and do each other and 429 00:22:17,200 --> 00:22:19,200 Speaker 1: you know, suck each other up. It's also possible for 430 00:22:19,280 --> 00:22:21,000 Speaker 1: them to be in a stable orbit. So if you 431 00:22:21,080 --> 00:22:23,119 Speaker 1: had two stars in a system, you would have the 432 00:22:23,240 --> 00:22:26,360 Speaker 1: two stars circling each other forever kind of right, Yeah, 433 00:22:26,400 --> 00:22:29,760 Speaker 1: they could be stably circling their common center of mass. 434 00:22:30,359 --> 00:22:32,200 Speaker 1: And so instead of thinking about it like as a 435 00:22:32,240 --> 00:22:34,480 Speaker 1: solar system with a star at the center and everything 436 00:22:34,600 --> 00:22:37,439 Speaker 1: moving around it, think about it like two stars at 437 00:22:37,440 --> 00:22:40,640 Speaker 1: the center orbiting some point in between them, and then 438 00:22:40,720 --> 00:22:43,159 Speaker 1: probably there are other things in the solar system and 439 00:22:43,200 --> 00:22:46,480 Speaker 1: they're orbiting that also that common center of mass, the 440 00:22:46,560 --> 00:22:49,399 Speaker 1: point between the two stars. Like if you're a planet, 441 00:22:49,680 --> 00:22:52,520 Speaker 1: you would orbit the center that like the middle point 442 00:22:52,560 --> 00:22:54,760 Speaker 1: between them. Yeah, if your planet, it doesn't matter to 443 00:22:54,800 --> 00:22:57,040 Speaker 1: you if you have two stars orbiting each other, or 444 00:22:57,080 --> 00:22:59,680 Speaker 1: if you replace those two stars with a big star 445 00:23:00,200 --> 00:23:02,040 Speaker 1: right at the center of mass, it looks the same 446 00:23:02,080 --> 00:23:05,159 Speaker 1: to you from a Newtonian dynamics, and so yeah, you 447 00:23:05,200 --> 00:23:07,560 Speaker 1: could just orbit the center of mass of those two stars. 448 00:23:07,840 --> 00:23:09,960 Speaker 1: So if you were far enough away from these two stars, 449 00:23:10,280 --> 00:23:13,280 Speaker 1: like life wouldn't be that different from what we have now, right, Like, 450 00:23:13,400 --> 00:23:16,320 Speaker 1: it's not like we would you know, sometimes see one 451 00:23:16,440 --> 00:23:18,560 Speaker 1: star to the right and another one to the left, 452 00:23:18,720 --> 00:23:20,920 Speaker 1: or sometimes you know, you would only see one star, 453 00:23:21,040 --> 00:23:23,400 Speaker 1: like usually you would probably only see you would see 454 00:23:23,440 --> 00:23:25,080 Speaker 1: the two stars at the same time in the sky. 455 00:23:25,280 --> 00:23:27,520 Speaker 1: That's right. Probably the two stars would be closest to 456 00:23:27,600 --> 00:23:29,560 Speaker 1: each other at the center of the system, and then 457 00:23:29,600 --> 00:23:32,440 Speaker 1: you'll be orbiting both of them. And so like having 458 00:23:32,520 --> 00:23:35,080 Speaker 1: a crazy system like we were talking about before, where 459 00:23:35,119 --> 00:23:38,680 Speaker 1: you like passed between the stars is less likely, And 460 00:23:39,000 --> 00:23:40,639 Speaker 1: if you had a system like that, it wouldn't be 461 00:23:40,760 --> 00:23:44,000 Speaker 1: very stable, Like that's a three body system. Those systems 462 00:23:44,000 --> 00:23:46,960 Speaker 1: are very very chaotic, and so a system like that 463 00:23:47,040 --> 00:23:49,639 Speaker 1: would likely just eject or lose its planets. And so 464 00:23:49,720 --> 00:23:51,600 Speaker 1: it's be very unlikely to have a planet in a 465 00:23:51,680 --> 00:23:54,679 Speaker 1: system where like the planet is passing between the two stars, 466 00:23:54,920 --> 00:23:57,520 Speaker 1: most likely to be doing an orbit around the two 467 00:23:57,560 --> 00:23:59,920 Speaker 1: star system. I see, So instead of seeing like one 468 00:24:00,200 --> 00:24:02,560 Speaker 1: bright circle in the sky, you would just see two 469 00:24:02,600 --> 00:24:05,280 Speaker 1: of them. Yeah, but they mostly be moving together, right, 470 00:24:05,480 --> 00:24:07,879 Speaker 1: but they might change in size relatively chick to each other, right, 471 00:24:07,920 --> 00:24:10,400 Speaker 1: Like as I'm going around, sometimes I'm closer to one 472 00:24:10,520 --> 00:24:13,000 Speaker 1: and sometimes I'm closer to the other one. So maybe 473 00:24:13,000 --> 00:24:15,399 Speaker 1: the weather would be really weird, right, Yeah, And they 474 00:24:15,440 --> 00:24:18,480 Speaker 1: can eclipse each other, right, one can pass in front 475 00:24:18,640 --> 00:24:21,800 Speaker 1: of the other, so you could have a son's sun eclipse, right, 476 00:24:22,160 --> 00:24:24,560 Speaker 1: because they could be different brightnesses and different colors. You 477 00:24:24,760 --> 00:24:26,639 Speaker 1: have like a red star and a yellow star, and 478 00:24:26,720 --> 00:24:29,760 Speaker 1: so like the color in the sky could change as 479 00:24:29,840 --> 00:24:31,760 Speaker 1: they pass in front of each other. That'd be pretty cool. 480 00:24:31,800 --> 00:24:34,520 Speaker 1: Would they change, like with the sky change color? Probably right, 481 00:24:34,600 --> 00:24:36,480 Speaker 1: like the light would get mixed up. Yeah, I'd be 482 00:24:36,480 --> 00:24:39,720 Speaker 1: awesome for artists. You know that golden hour the photographers 483 00:24:39,760 --> 00:24:41,159 Speaker 1: like to use at the beach trying to be like 484 00:24:41,520 --> 00:24:45,080 Speaker 1: lots of different kinds of colored hours cool. Alright, So 485 00:24:45,160 --> 00:24:47,280 Speaker 1: then and and these systems are stable. You say these 486 00:24:47,320 --> 00:24:50,080 Speaker 1: systems are stable. The two body system can be stable. 487 00:24:50,440 --> 00:24:53,200 Speaker 1: Three body system is very complicated, and we're gonna have 488 00:24:53,200 --> 00:24:55,880 Speaker 1: a old podcast episode about that very soon. The three 489 00:24:55,960 --> 00:24:58,800 Speaker 1: body problem is famously difficult to solve. But a two 490 00:24:59,000 --> 00:25:00,920 Speaker 1: star system can be stable, and then you can have 491 00:25:00,960 --> 00:25:03,879 Speaker 1: a planet orbiting around that two star system. That's the 492 00:25:04,000 --> 00:25:07,000 Speaker 1: key to stability is to really take a three body 493 00:25:07,119 --> 00:25:09,840 Speaker 1: system and make it into effectively two body by putting 494 00:25:09,880 --> 00:25:11,720 Speaker 1: two of them close to each other, so you can 495 00:25:11,920 --> 00:25:14,160 Speaker 1: sort of treat them as one. Right, And you're saying 496 00:25:14,359 --> 00:25:17,200 Speaker 1: those are more stable, which means that they're you know, 497 00:25:17,359 --> 00:25:19,960 Speaker 1: more likely like the ones that are chaotic probably crash 498 00:25:20,040 --> 00:25:22,639 Speaker 1: into each other or something else happened. Yeah, exactly. And 499 00:25:22,720 --> 00:25:25,840 Speaker 1: there may have been a lot of triinary star systems formed. 500 00:25:25,920 --> 00:25:28,840 Speaker 1: We have three stars all forming together, but that's a 501 00:25:29,000 --> 00:25:31,800 Speaker 1: very unstable situation. And so that's why we have a 502 00:25:31,840 --> 00:25:35,440 Speaker 1: lot more binary star systems than triinary star systems because 503 00:25:35,520 --> 00:25:38,159 Speaker 1: probably when there were three, two of them got together 504 00:25:38,320 --> 00:25:41,359 Speaker 1: and ejected the third. Kind of like human relationships a 505 00:25:41,400 --> 00:25:43,960 Speaker 1: little bit kind of like the Hemsworth Brothers. You know, 506 00:25:46,720 --> 00:25:48,960 Speaker 1: I don't think they've injected anyway. Well, I guess the 507 00:25:49,080 --> 00:25:51,720 Speaker 1: third one is not as famous. Yeah, exactly. But you 508 00:25:51,840 --> 00:25:53,560 Speaker 1: kind of blew my mind when you said about a 509 00:25:53,640 --> 00:25:56,520 Speaker 1: third of stars out there are binary systems. And I 510 00:25:56,560 --> 00:25:58,159 Speaker 1: guess maybe a question is like, how do we know, 511 00:25:58,520 --> 00:26:00,520 Speaker 1: Like in the nice sky, they just look like pinpoints. 512 00:26:00,600 --> 00:26:03,520 Speaker 1: How do we know that there are two in each 513 00:26:03,560 --> 00:26:05,760 Speaker 1: of those pinpoints? So we can study these things and 514 00:26:05,840 --> 00:26:08,560 Speaker 1: we can tell sometimes when they're binary star systems. There's 515 00:26:08,600 --> 00:26:11,399 Speaker 1: two ways to do it. One is just visually, like 516 00:26:11,560 --> 00:26:14,760 Speaker 1: you get a really powerful telescope. You can actually see 517 00:26:15,280 --> 00:26:17,879 Speaker 1: that a star is not spherical in your telescope. You 518 00:26:17,920 --> 00:26:19,240 Speaker 1: don't even have to be able to see like the 519 00:26:19,359 --> 00:26:21,880 Speaker 1: gap between them. You can just tell that it looks 520 00:26:21,920 --> 00:26:24,200 Speaker 1: more like a peanut, or it's all along, or that 521 00:26:24,280 --> 00:26:26,440 Speaker 1: its shape seems to be changing in a way that's 522 00:26:26,480 --> 00:26:29,680 Speaker 1: consistent with two stars near each other. Oh, I see 523 00:26:29,760 --> 00:26:31,639 Speaker 1: like as they rotate it maybe it looks like a 524 00:26:31,680 --> 00:26:34,720 Speaker 1: blob kind of changing shape. It looks like a blob. 525 00:26:34,760 --> 00:26:37,320 Speaker 1: So that's number one. That's the easiest way. That was 526 00:26:37,400 --> 00:26:39,399 Speaker 1: the first way we've ever done it. The second is 527 00:26:39,440 --> 00:26:42,320 Speaker 1: that we can use Doppler effects. So you have two 528 00:26:42,440 --> 00:26:44,879 Speaker 1: stars orbiting each other. Now, so now they have a 529 00:26:45,000 --> 00:26:47,919 Speaker 1: velocity relative to each other. And so the same way 530 00:26:47,960 --> 00:26:50,520 Speaker 1: that we measure the velocity of a star relative to 531 00:26:50,600 --> 00:26:53,560 Speaker 1: the Earth by looking at how it shifts the wavelength 532 00:26:53,640 --> 00:26:55,880 Speaker 1: of the light that's getting to us, because if it's 533 00:26:55,920 --> 00:26:59,200 Speaker 1: moving away from us, it stretches out the wavelength. That 534 00:26:59,240 --> 00:27:02,320 Speaker 1: makes the wavelengths longer and redder. That's called red shift. 535 00:27:02,480 --> 00:27:04,479 Speaker 1: But if two stars are orbiting each other, then their 536 00:27:04,560 --> 00:27:07,480 Speaker 1: velocity relative to the Earth is constantly changing. They're like 537 00:27:07,640 --> 00:27:10,280 Speaker 1: faster slow or faster slower, faster, slower, And so we 538 00:27:10,359 --> 00:27:13,880 Speaker 1: can measure this changing red shift, and we can deduce 539 00:27:14,320 --> 00:27:17,040 Speaker 1: that a star that looks just like one actually has 540 00:27:17,119 --> 00:27:19,399 Speaker 1: this pattern of two stars moving back and forth. We 541 00:27:19,480 --> 00:27:22,240 Speaker 1: can tell which light is coming from which star based 542 00:27:22,280 --> 00:27:24,880 Speaker 1: on the red shift pattern I see, because I guess 543 00:27:24,920 --> 00:27:27,040 Speaker 1: if if it's only one star in that system, that 544 00:27:27,400 --> 00:27:30,960 Speaker 1: star is not really jiggling, right, it's probably just sitting 545 00:27:31,320 --> 00:27:34,520 Speaker 1: pretty solidly in the center of its system, not wriggling 546 00:27:34,600 --> 00:27:38,040 Speaker 1: around or moving around something close by. That's right, unless 547 00:27:38,119 --> 00:27:40,399 Speaker 1: there's a big planet there. And so now we have 548 00:27:40,520 --> 00:27:43,440 Speaker 1: like really really sensitive techniques to measure the lights from 549 00:27:43,480 --> 00:27:46,399 Speaker 1: these stars to see if there are planets tugging on 550 00:27:46,520 --> 00:27:49,399 Speaker 1: those stars. And so in the same way we detect 551 00:27:49,520 --> 00:27:52,600 Speaker 1: exo planets by seeing that they're tugging on the stars 552 00:27:52,680 --> 00:27:55,280 Speaker 1: and causing these weird Doppler patterns in the stars, you 553 00:27:55,400 --> 00:27:58,920 Speaker 1: can see exo stars, right. You can see that this 554 00:27:59,080 --> 00:28:01,720 Speaker 1: star is not just one, but it's actually two based 555 00:28:01,840 --> 00:28:05,120 Speaker 1: on the light that comes from It's exactly the same technique. Wow, 556 00:28:05,280 --> 00:28:07,359 Speaker 1: So I guess we've been able to see them now 557 00:28:07,400 --> 00:28:09,320 Speaker 1: for a while, and we actually know a lot about 558 00:28:09,359 --> 00:28:11,720 Speaker 1: these binary systems, right, That's right. And there's a third 559 00:28:11,800 --> 00:28:14,840 Speaker 1: way that we see these binary systems, and that's also 560 00:28:15,040 --> 00:28:18,480 Speaker 1: borrowed from exoplanets, and that's this eclipse technique that we 561 00:28:18,560 --> 00:28:21,000 Speaker 1: were talking about. Having two stars line up in front 562 00:28:21,040 --> 00:28:22,840 Speaker 1: of each other in the same way that we see 563 00:28:22,960 --> 00:28:26,120 Speaker 1: exo planets by seeing like how they eclipse their star. 564 00:28:26,400 --> 00:28:28,280 Speaker 1: In that case, the planet is passing in front of 565 00:28:28,359 --> 00:28:30,560 Speaker 1: the stars, so it dims the light just a little bit. 566 00:28:30,680 --> 00:28:33,080 Speaker 1: But we are really precise telescopes to measure that if 567 00:28:33,280 --> 00:28:35,600 Speaker 1: one of the stars is brighter than the other, then 568 00:28:35,680 --> 00:28:37,720 Speaker 1: as it passes in front of the other star, it 569 00:28:37,800 --> 00:28:40,320 Speaker 1: can eclipse it, it will change how much light we 570 00:28:40,440 --> 00:28:42,760 Speaker 1: are seeing. You get a regular pattern of that, you 571 00:28:42,840 --> 00:28:45,120 Speaker 1: can deduce it. It's a binary star system. So a 572 00:28:45,200 --> 00:28:48,160 Speaker 1: lot of these techniques really come from sort of extrapolating 573 00:28:48,200 --> 00:28:51,880 Speaker 1: from exoplanet techniques, and I imagine if they're very different stars, 574 00:28:52,200 --> 00:28:54,400 Speaker 1: then you could even tell it to apart, right, because 575 00:28:54,840 --> 00:28:58,080 Speaker 1: stars have kind of like a fingerprint depending on their material, 576 00:28:58,120 --> 00:29:00,840 Speaker 1: and so you can be have like a very unique nature. Exactly. 577 00:29:00,880 --> 00:29:03,040 Speaker 1: They have a fingerprint just as you said, based on 578 00:29:03,160 --> 00:29:06,760 Speaker 1: what they're burning, because different elements have different quantum levels 579 00:29:06,800 --> 00:29:10,160 Speaker 1: and so they give off photons at different energies. And 580 00:29:10,280 --> 00:29:12,800 Speaker 1: that's also we rely on that for the Doppler pattern. Right. 581 00:29:12,800 --> 00:29:14,640 Speaker 1: You might ask, like, how do you know if the 582 00:29:14,760 --> 00:29:16,560 Speaker 1: light from a star is red shifted or not. You 583 00:29:16,600 --> 00:29:19,000 Speaker 1: can't tell what it's like over there. What you can 584 00:29:19,200 --> 00:29:22,840 Speaker 1: because you know exactly what energy level hydrogen gives off 585 00:29:22,840 --> 00:29:25,080 Speaker 1: when it's hot, and we know that energy level, so 586 00:29:25,200 --> 00:29:27,720 Speaker 1: we can compare what we measure to what we see. 587 00:29:28,360 --> 00:29:30,440 Speaker 1: And so you're right, if one star is heavier, has 588 00:29:30,480 --> 00:29:32,280 Speaker 1: more metals than it, it's going to glow with a 589 00:29:32,360 --> 00:29:35,720 Speaker 1: different set of spikes in the spectrum, and as one 590 00:29:35,760 --> 00:29:37,520 Speaker 1: passes in front of the other, you'll see like the 591 00:29:37,600 --> 00:29:40,640 Speaker 1: color that light literally change as they eclipse each other. 592 00:29:40,640 --> 00:29:42,680 Speaker 1: It's pretty cool. Yeah, it's pretty cool because I guess 593 00:29:42,680 --> 00:29:44,680 Speaker 1: when you look at the sky, I mean, everything just 594 00:29:44,720 --> 00:29:47,960 Speaker 1: looks like white pinpoints, but there's a ton of information, 595 00:29:48,120 --> 00:29:49,880 Speaker 1: like if you look at the different frequencies. Right. Yeah, 596 00:29:49,920 --> 00:29:53,200 Speaker 1: it's another great example of how much information about incredible 597 00:29:53,280 --> 00:29:56,360 Speaker 1: mind blowing stuff is out there, like literally washing over 598 00:29:56,480 --> 00:29:59,840 Speaker 1: us every day, that we're mostly ignoring. I wouldn't say mostly, 599 00:29:59,840 --> 00:30:05,440 Speaker 1: I largely. Except for a few scientists paying attention to 600 00:30:05,480 --> 00:30:07,440 Speaker 1: a few corners in the universe, most of what the 601 00:30:07,520 --> 00:30:09,920 Speaker 1: universe is telling us and gets ignored. Yeah, it's not. 602 00:30:11,200 --> 00:30:13,520 Speaker 1: But we have done this with lots and lots of stars, 603 00:30:13,680 --> 00:30:15,920 Speaker 1: Like we have looked out there and we have identified 604 00:30:16,000 --> 00:30:20,400 Speaker 1: more than a hundred thousand binary stars just looking here 605 00:30:20,440 --> 00:30:23,040 Speaker 1: from Earth. Right. Yeah, but you're saying that even though 606 00:30:23,040 --> 00:30:27,440 Speaker 1: they're more stable binary system, that they're still not super stable, 607 00:30:27,520 --> 00:30:30,880 Speaker 1: meaning that they are less likely to have planets. Yeah, 608 00:30:30,920 --> 00:30:33,800 Speaker 1: because you had a third body now becomes chaotic, right, 609 00:30:33,880 --> 00:30:36,920 Speaker 1: A two body system very stable, happy to orbit around 610 00:30:36,960 --> 00:30:39,600 Speaker 1: each other for the rest of time at a third body, 611 00:30:39,680 --> 00:30:43,080 Speaker 1: like a planet, and it gets complicated because as those 612 00:30:43,160 --> 00:30:45,840 Speaker 1: two stars orbit each other, sometimes one gets a little 613 00:30:45,880 --> 00:30:48,320 Speaker 1: closer to the planet and one gets a little further away, 614 00:30:48,360 --> 00:30:50,600 Speaker 1: and that adjust the orbit of the planet. It can 615 00:30:50,680 --> 00:30:53,600 Speaker 1: knock it off. Its orbit and orbits are a little 616 00:30:53,640 --> 00:30:56,040 Speaker 1: bit fragile. You get a push in the wrong moment 617 00:30:56,080 --> 00:30:59,000 Speaker 1: in the wrong direction and boom you're rocketing out into 618 00:30:59,040 --> 00:31:02,480 Speaker 1: space or your arashing into the Sun. And so these 619 00:31:02,560 --> 00:31:05,280 Speaker 1: systems are not as likely to have planets as single 620 00:31:05,360 --> 00:31:09,240 Speaker 1: star systems like ours. But our Solar system is pretty stable. 621 00:31:09,320 --> 00:31:10,960 Speaker 1: But we have like a ton of objects in it. 622 00:31:11,440 --> 00:31:13,800 Speaker 1: Why isn't it chaotic? We do have a ton of objects, 623 00:31:13,840 --> 00:31:16,360 Speaker 1: but mostly they're very small and very far from each other, 624 00:31:16,640 --> 00:31:18,760 Speaker 1: like the two biggest objects in the Solar System, the 625 00:31:18,840 --> 00:31:23,040 Speaker 1: Sun and Jupiter. The Sun dominates the gravity by huge amount. 626 00:31:23,080 --> 00:31:27,400 Speaker 1: It's like twenty five thousand times more powerful gravitationally than Jupiter. 627 00:31:27,600 --> 00:31:29,920 Speaker 1: So it's almost like we have a two body system. 628 00:31:30,000 --> 00:31:32,640 Speaker 1: We can mostly ignore Jupiter, and the other planets are 629 00:31:32,680 --> 00:31:35,000 Speaker 1: so small that they don't really affect us. If they 630 00:31:35,040 --> 00:31:37,200 Speaker 1: were closer, like they were in the early part of 631 00:31:37,240 --> 00:31:39,280 Speaker 1: the Solar System, you would have a lot more chaos, 632 00:31:39,400 --> 00:31:41,880 Speaker 1: and we had a lot more chaos. Well we're looking 633 00:31:41,960 --> 00:31:44,320 Speaker 1: at is sort of like the stable remnant of four 634 00:31:44,440 --> 00:31:47,440 Speaker 1: billion years of craziness. Well, I think it's also interesting 635 00:31:47,480 --> 00:31:49,760 Speaker 1: you were telling me that you can also have like 636 00:31:49,840 --> 00:31:53,360 Speaker 1: a star and a black hole system, Like you could 637 00:31:53,400 --> 00:31:55,400 Speaker 1: have a solar system with a star and a black 638 00:31:55,440 --> 00:31:58,840 Speaker 1: hole in it, exactly because sometimes stars become black holes. 639 00:31:58,960 --> 00:32:01,600 Speaker 1: So what happens if you have two stars and one 640 00:32:01,640 --> 00:32:03,640 Speaker 1: of them is big enough to collapse eventually into a 641 00:32:03,640 --> 00:32:05,360 Speaker 1: black hole and the other one isn't, then you get 642 00:32:05,400 --> 00:32:08,840 Speaker 1: a star orbiting a black hole. And that's super cool. 643 00:32:08,920 --> 00:32:12,080 Speaker 1: And that's actually the first way that we discovered black holes. 644 00:32:12,520 --> 00:32:16,360 Speaker 1: We saw this star orbiting something nothing, nothing that we 645 00:32:16,400 --> 00:32:19,400 Speaker 1: could see at least, and that was great evidence of 646 00:32:19,480 --> 00:32:21,600 Speaker 1: the existence of a black hole. So we did a 647 00:32:21,640 --> 00:32:25,000 Speaker 1: whole fun podcast episode about Sickness X one this discovery 648 00:32:25,000 --> 00:32:27,000 Speaker 1: of a black hole. It's pretty nice because the star 649 00:32:27,240 --> 00:32:29,520 Speaker 1: that you can see tells you a lot about how 650 00:32:29,640 --> 00:32:32,640 Speaker 1: much mass is there. From its orbital radius and its velocity, 651 00:32:33,040 --> 00:32:35,200 Speaker 1: you can deduce its mass and the mass of the 652 00:32:35,240 --> 00:32:37,640 Speaker 1: black hole. So it's pretty cool, right, And you can 653 00:32:37,720 --> 00:32:42,400 Speaker 1: even have like planets orbiting this binary star black hole system. 654 00:32:42,560 --> 00:32:44,760 Speaker 1: Like you could maybe be on a planet and look 655 00:32:44,840 --> 00:32:46,640 Speaker 1: up at the sky and there be a sun and 656 00:32:46,720 --> 00:32:49,040 Speaker 1: a black circle right and a black hole and you're 657 00:32:49,040 --> 00:32:50,760 Speaker 1: in the night sky, Like you could have an anti 658 00:32:50,880 --> 00:32:55,120 Speaker 1: sunset where the black hole, you know, it's below the horizon. Yeah, 659 00:32:55,200 --> 00:32:57,160 Speaker 1: what would that be like? That would be an awesome eclipse, 660 00:32:57,400 --> 00:33:00,040 Speaker 1: a black hole passing in front of the star. That 661 00:33:00,120 --> 00:33:02,280 Speaker 1: would be pretty super cool to see. It would also 662 00:33:02,320 --> 00:33:04,160 Speaker 1: make me feel a little nervous, you know, to be 663 00:33:04,280 --> 00:33:07,520 Speaker 1: that close to a black hole. It's a nerve wrecking 664 00:33:07,640 --> 00:33:09,920 Speaker 1: enough to be close to it a giant exploding star, 665 00:33:10,120 --> 00:33:14,520 Speaker 1: but now now you're orbiting also a black hole. Yeah, exactly. 666 00:33:14,800 --> 00:33:17,080 Speaker 1: That would be pretty crazy. And sometimes a binary star 667 00:33:17,160 --> 00:33:20,040 Speaker 1: system is a little fuzzy, like sometimes the two stars 668 00:33:20,120 --> 00:33:22,240 Speaker 1: can help each other out, or like they can steal 669 00:33:22,400 --> 00:33:25,560 Speaker 1: material from each other. For example, of this famous kind 670 00:33:25,640 --> 00:33:29,480 Speaker 1: of supernova type one, a supernova comes from a binary 671 00:33:29,560 --> 00:33:33,000 Speaker 1: star system. It only happens under very special conditions. When 672 00:33:33,040 --> 00:33:35,800 Speaker 1: you have one star that becomes a white dwarf, which 673 00:33:35,840 --> 00:33:38,320 Speaker 1: means that it's blown out most of its fuel and 674 00:33:38,440 --> 00:33:40,720 Speaker 1: what's left is just like a hot mass of stuff. 675 00:33:40,720 --> 00:33:43,560 Speaker 1: It's not fusing anymore. It's just like glowing because it's 676 00:33:43,600 --> 00:33:46,480 Speaker 1: hot like hot metal does. And it's not massive enough 677 00:33:46,520 --> 00:33:48,920 Speaker 1: to collapse into a black hole or go supernova, So 678 00:33:49,040 --> 00:33:52,000 Speaker 1: otherwise it would just sit there forever, cooling for trillions 679 00:33:52,040 --> 00:33:54,880 Speaker 1: of years. But if it's got a partner near it, 680 00:33:54,960 --> 00:33:58,120 Speaker 1: like a really big star orbiting right around it, it's 681 00:33:58,160 --> 00:34:00,840 Speaker 1: gravity can suck in some of the mater curial from 682 00:34:00,880 --> 00:34:03,959 Speaker 1: that other star and that can trigger a supernova. Now 683 00:34:04,080 --> 00:34:07,240 Speaker 1: it has enough gravity to collapse, and Type one A 684 00:34:07,280 --> 00:34:09,560 Speaker 1: supernova is the one that tell us about dark energy 685 00:34:09,600 --> 00:34:12,279 Speaker 1: and expansion of the universe. Those are the conditions needed 686 00:34:12,320 --> 00:34:14,920 Speaker 1: for a type one A supernova. Every single one is 687 00:34:15,000 --> 00:34:18,400 Speaker 1: exactly that scenario. Really, all of the type one and 688 00:34:18,440 --> 00:34:20,160 Speaker 1: those are the ones we used to like map out 689 00:34:20,160 --> 00:34:22,840 Speaker 1: the universe, right, those are really important for us. Yeah, exactly, 690 00:34:23,040 --> 00:34:25,600 Speaker 1: a star that goes supernova by itself, that's called a 691 00:34:25,640 --> 00:34:28,520 Speaker 1: type two supernova. So Type one A are these very 692 00:34:28,600 --> 00:34:31,359 Speaker 1: special conditions from a binary star system with a white 693 00:34:31,400 --> 00:34:34,840 Speaker 1: dwarf that gobbles energy and mass from its partner to 694 00:34:34,960 --> 00:34:37,720 Speaker 1: trigger the supernova. So we wouldn't have those without binary 695 00:34:37,760 --> 00:34:40,280 Speaker 1: star systems, so we wouldn't have learned so much about 696 00:34:40,320 --> 00:34:43,920 Speaker 1: the universe. Interesting. So that's a binary system that's not stable, right, 697 00:34:43,920 --> 00:34:46,560 Speaker 1: because one of them is getting sucked into the other. Yeah, exactly. 698 00:34:46,560 --> 00:34:48,600 Speaker 1: And then when it goes supernova, you can like blow 699 00:34:48,719 --> 00:34:50,960 Speaker 1: up the other star like that goes totally crazy. You 700 00:34:51,000 --> 00:34:54,400 Speaker 1: wouldn't want to be a planet on that system. You 701 00:34:54,440 --> 00:34:56,759 Speaker 1: wouldn't want to be a star in that family. Like 702 00:34:56,880 --> 00:34:59,160 Speaker 1: when one of the hands with brothers blows up, sorry 703 00:34:59,440 --> 00:35:01,680 Speaker 1: giving a ra in public and people ful filled it 704 00:35:01,760 --> 00:35:03,440 Speaker 1: with the cell phone, then it's all over for the 705 00:35:03,480 --> 00:35:05,920 Speaker 1: whole family. I just meant their career blows up, you know, 706 00:35:06,000 --> 00:35:07,759 Speaker 1: like one of them becomes Thor and the other ones, 707 00:35:07,880 --> 00:35:11,680 Speaker 1: you know, whatever they're doing, they're not Thor, they're not Thor. 708 00:35:11,760 --> 00:35:14,239 Speaker 1: I think that's how their parents now call them. This 709 00:35:14,360 --> 00:35:16,879 Speaker 1: is my son Thor, which is my other son, not Thor. 710 00:35:17,719 --> 00:35:20,040 Speaker 1: And this is my other son Awsome, not Thor. Hey, 711 00:35:20,080 --> 00:35:22,280 Speaker 1: if one of my siblings was a god on screen, 712 00:35:22,400 --> 00:35:24,920 Speaker 1: and then yes, I would define myself. Is not that one? 713 00:35:26,400 --> 00:35:31,359 Speaker 1: If one of your siblings, I see, well, I'm sure 714 00:35:31,360 --> 00:35:34,080 Speaker 1: they're happy not to be you as well. Everybody in 715 00:35:34,120 --> 00:35:36,320 Speaker 1: the universe except for me is happy to not be me, 716 00:35:36,640 --> 00:35:38,920 Speaker 1: all right, Well, let's get into more than just two 717 00:35:38,960 --> 00:35:41,359 Speaker 1: stars in a solar sism. You can you have three 718 00:35:41,520 --> 00:35:44,160 Speaker 1: or four or five or maybe even more than that. 719 00:35:45,200 --> 00:36:00,120 Speaker 1: But first, let's take another quick break. All right, we're 720 00:36:00,160 --> 00:36:03,920 Speaker 1: talking about multi star systems, solar systems with more than 721 00:36:04,280 --> 00:36:07,839 Speaker 1: one or two stars, Daniel, Are those common in the universe? Also? 722 00:36:07,920 --> 00:36:10,520 Speaker 1: Can you have a solar system with three stars or 723 00:36:10,640 --> 00:36:13,319 Speaker 1: four stars? Yeah, it turns out it's not that rare. 724 00:36:13,480 --> 00:36:17,000 Speaker 1: Like the most common systems are single and double systems 725 00:36:17,040 --> 00:36:19,440 Speaker 1: for the reasons we talked about. But you can actually 726 00:36:19,560 --> 00:36:23,200 Speaker 1: build a stable system out of more than two stars. 727 00:36:23,280 --> 00:36:26,040 Speaker 1: You can have a third star, and the trick is 728 00:36:26,120 --> 00:36:28,080 Speaker 1: to have two of them be like really close to 729 00:36:28,120 --> 00:36:30,520 Speaker 1: each other and the other one be a little further away. 730 00:36:30,600 --> 00:36:33,600 Speaker 1: So like a triple star system, you have two stars 731 00:36:33,680 --> 00:36:35,600 Speaker 1: like the center, and then instead of a planet, you 732 00:36:35,640 --> 00:36:37,759 Speaker 1: have like another star out there and it's sort of 733 00:36:37,800 --> 00:36:41,000 Speaker 1: a wide orbit around the two stars. But hey, you've 734 00:36:41,000 --> 00:36:44,319 Speaker 1: got three stars in orbit around their common center of mass. 735 00:36:44,400 --> 00:36:46,759 Speaker 1: So that's a triple system. And why not, right, I mean, 736 00:36:46,800 --> 00:36:51,440 Speaker 1: they're consensing cosmological objects, you know, to each their own 737 00:36:51,600 --> 00:36:53,839 Speaker 1: that's right. I believe in polly star systems or whatever 738 00:36:53,880 --> 00:36:57,439 Speaker 1: you thought it, Polly physics. There you go. We're open 739 00:36:57,480 --> 00:36:59,319 Speaker 1: minded here on the podcast. I think what you mean 740 00:36:59,480 --> 00:37:01,759 Speaker 1: is like haveing a system kind of like ours, where 741 00:37:01,800 --> 00:37:04,000 Speaker 1: there's a big there's something in the middle that's big 742 00:37:04,080 --> 00:37:06,600 Speaker 1: and happening, and then there's maybe like a third one 743 00:37:06,719 --> 00:37:10,719 Speaker 1: like Jupiter way out there where it's not really disrupting 744 00:37:10,840 --> 00:37:13,760 Speaker 1: as much the two star system in the middle. Yeah, exactly, 745 00:37:13,840 --> 00:37:16,840 Speaker 1: take our star and split it into two tightly orbiting 746 00:37:16,880 --> 00:37:20,160 Speaker 1: each other, and then graduate Jupiter into a star. And 747 00:37:20,239 --> 00:37:22,640 Speaker 1: that's a good mental picture for what a trinary star 748 00:37:22,760 --> 00:37:25,480 Speaker 1: system might look like. It's not like three stars are 749 00:37:25,560 --> 00:37:28,520 Speaker 1: like all whizzing around each other in close quarters in 750 00:37:28,680 --> 00:37:31,800 Speaker 1: some crazy like dance. Yeah, it's really more like a 751 00:37:31,880 --> 00:37:34,760 Speaker 1: binary system with an orbiting third partner. It's like a couple, 752 00:37:34,840 --> 00:37:38,359 Speaker 1: but then there's someone in the preference checking them out. 753 00:37:38,480 --> 00:37:41,520 Speaker 1: There's a close friend, a camry couple, a close friends 754 00:37:42,160 --> 00:37:45,320 Speaker 1: Uncle George, we'll just call him uncle George, exactly. And 755 00:37:45,440 --> 00:37:48,800 Speaker 1: that's the recipe for building these more complex star systems 756 00:37:48,920 --> 00:37:51,560 Speaker 1: and having them be stable. For example, if you want 757 00:37:51,719 --> 00:37:55,239 Speaker 1: a quadruple star system, and there is one, it's called 758 00:37:55,320 --> 00:38:00,360 Speaker 1: Alpha Jeminorum. This is basically two binary star systems orbiting 759 00:38:00,440 --> 00:38:02,920 Speaker 1: each other. So you have like a tight pair and 760 00:38:03,040 --> 00:38:06,160 Speaker 1: another tight pair and they're orbiting each other. Like how 761 00:38:06,239 --> 00:38:08,520 Speaker 1: far away are we talking about? Like are they really 762 00:38:08,560 --> 00:38:11,399 Speaker 1: far away or are they like you know, spinning around 763 00:38:11,440 --> 00:38:13,760 Speaker 1: pretty fast around each other. Yes, So the two closer 764 00:38:13,840 --> 00:38:16,560 Speaker 1: ones have periods that are really small. So like the 765 00:38:16,640 --> 00:38:19,640 Speaker 1: pairs orbit each other in like days, right, so they're 766 00:38:19,719 --> 00:38:22,279 Speaker 1: really whizzing around each other. But then there's a much 767 00:38:22,360 --> 00:38:26,120 Speaker 1: bigger separation between the pairs, and that's typical. That's how 768 00:38:26,200 --> 00:38:29,520 Speaker 1: you become stable. And so the pairs of pairs orbit 769 00:38:29,560 --> 00:38:31,920 Speaker 1: each other, you know, more like in a period of years, 770 00:38:32,040 --> 00:38:34,320 Speaker 1: and in other star systems it can be hundreds or 771 00:38:34,440 --> 00:38:37,200 Speaker 1: thousands of years for the larger set. I mean, it's 772 00:38:37,280 --> 00:38:40,040 Speaker 1: it's not like our solar system. It's more like you know, 773 00:38:40,600 --> 00:38:43,120 Speaker 1: like a Meani galaxy almost, yes, sort of. But they 774 00:38:43,160 --> 00:38:46,160 Speaker 1: are definitely orbiting each other. They are gravitationally bound to 775 00:38:46,360 --> 00:38:48,880 Speaker 1: each other, you know, the way like the Orc cloud 776 00:38:49,120 --> 00:38:52,200 Speaker 1: is really really far out there, but it's still gravitationally 777 00:38:52,280 --> 00:38:54,560 Speaker 1: bound to our Sun, and so it's part of our 778 00:38:54,640 --> 00:38:57,240 Speaker 1: solar system. I see. So that's a system we actually 779 00:38:57,280 --> 00:38:59,160 Speaker 1: know about what we can see it. It's two couples 780 00:38:59,200 --> 00:39:02,280 Speaker 1: swinging around. Yeah, and it's really awesome because we originally 781 00:39:02,320 --> 00:39:04,839 Speaker 1: thought it was a binary system because you can see 782 00:39:05,239 --> 00:39:07,960 Speaker 1: the two stars visually, right, So you can see the 783 00:39:08,000 --> 00:39:09,719 Speaker 1: two stars, and then when you look at each one, 784 00:39:09,800 --> 00:39:11,719 Speaker 1: you can tell, oh my gosh, each one turns out 785 00:39:11,760 --> 00:39:14,040 Speaker 1: to also be a binary. But you can only tell 786 00:39:14,400 --> 00:39:17,600 Speaker 1: based on these spectroscopic measurements, the measuring of light and 787 00:39:17,640 --> 00:39:20,239 Speaker 1: seeing the Doppler shift. Well, that must have been a 788 00:39:20,440 --> 00:39:23,120 Speaker 1: weird revelation, right, yeah, and one at a time, right, 789 00:39:23,120 --> 00:39:25,520 Speaker 1: you're like, oh my gosh, this binary star system turns 790 00:39:25,520 --> 00:39:27,680 Speaker 1: out to be triinary. Let's check out the other one 791 00:39:27,760 --> 00:39:31,360 Speaker 1: that's binary. And then it turns into an eight solar 792 00:39:31,719 --> 00:39:35,120 Speaker 1: sun system. And yeah, you never know, you never know. Well, 793 00:39:35,280 --> 00:39:37,840 Speaker 1: what about more than four stars? So that's a pretty 794 00:39:37,880 --> 00:39:40,319 Speaker 1: high number. Can you have more than four stars? You can. 795 00:39:40,600 --> 00:39:44,400 Speaker 1: There's a system of five stars. This is the Glease system. 796 00:39:44,640 --> 00:39:46,640 Speaker 1: This is organized in sort of a crazy way, like 797 00:39:46,760 --> 00:39:49,320 Speaker 1: a set of hangars where one hangar hangs off the 798 00:39:49,440 --> 00:39:50,880 Speaker 1: edge of the other one hangs out the edge of 799 00:39:50,920 --> 00:39:54,080 Speaker 1: the other one. You have like a binary star system. 800 00:39:54,200 --> 00:39:57,040 Speaker 1: But then it turns out that one of them looks 801 00:39:57,120 --> 00:39:59,800 Speaker 1: like a binary star, right, so you have instead of 802 00:40:00,000 --> 00:40:02,200 Speaker 1: a binary star system, now you have a trinary. Then 803 00:40:02,200 --> 00:40:04,719 Speaker 1: you zoom in on one of those in the binary, 804 00:40:04,800 --> 00:40:07,879 Speaker 1: and turns out that's a binary. And then you zoom 805 00:40:07,880 --> 00:40:09,560 Speaker 1: in on one of those in that binary, and that 806 00:40:09,800 --> 00:40:13,759 Speaker 1: turns out to be a binary. Yes, like a nested yeah. 807 00:40:14,040 --> 00:40:16,239 Speaker 1: And really that's the only way to be stable is 808 00:40:16,320 --> 00:40:19,640 Speaker 1: to have these things be separated into like effectively two 809 00:40:19,760 --> 00:40:22,200 Speaker 1: body systems, but where one of the bodies turns out 810 00:40:22,280 --> 00:40:24,759 Speaker 1: to have complicated like inner motion. So this one is 811 00:40:24,800 --> 00:40:26,880 Speaker 1: like a four level hierarchy, and this is called the 812 00:40:26,960 --> 00:40:29,960 Speaker 1: Glease system g L I E S E. You need 813 00:40:30,080 --> 00:40:32,360 Speaker 1: like a hierarchy, But is that hierarchy due to the 814 00:40:32,600 --> 00:40:35,800 Speaker 1: size like each as you go down a level, the 815 00:40:35,920 --> 00:40:38,279 Speaker 1: sun's get smaller. Are they all the same size? It 816 00:40:38,400 --> 00:40:42,200 Speaker 1: just happened to like be trapped in this hierarchical orbits. 817 00:40:42,400 --> 00:40:44,359 Speaker 1: They don't have to be smaller. They can be large, 818 00:40:44,360 --> 00:40:45,960 Speaker 1: and they can even be larger, but then you just 819 00:40:46,040 --> 00:40:47,759 Speaker 1: need the orbits to be a little bit bigger so 820 00:40:47,880 --> 00:40:50,600 Speaker 1: that effectively it looks like a single star system from 821 00:40:50,680 --> 00:40:53,160 Speaker 1: the distance of the other star. Right, you just need 822 00:40:53,239 --> 00:40:56,080 Speaker 1: to be to be small enough then to be close enough, 823 00:40:56,360 --> 00:40:58,200 Speaker 1: or for you to be far enough away that you 824 00:40:58,239 --> 00:41:01,160 Speaker 1: can mostly treat a binary system like a single star 825 00:41:01,360 --> 00:41:02,920 Speaker 1: for it to be stable. I wonder what it's like 826 00:41:03,040 --> 00:41:04,680 Speaker 1: to be a planet in that system. Is it just 827 00:41:04,760 --> 00:41:09,680 Speaker 1: like a constant disco ball, you know, it's experienced day 828 00:41:09,719 --> 00:41:13,000 Speaker 1: and night like light flashing in and out. Well, some 829 00:41:13,120 --> 00:41:14,680 Speaker 1: of the stars are going to be so distant that 830 00:41:14,760 --> 00:41:17,919 Speaker 1: they're just gonna look like moons, right, or they're gonna 831 00:41:17,960 --> 00:41:19,640 Speaker 1: look like other things. Well, I give this one a 832 00:41:19,719 --> 00:41:23,080 Speaker 1: five star rating for sure for having five stars. But wait, 833 00:41:23,440 --> 00:41:26,000 Speaker 1: there's more. Yeah, is it possible to have more? Yeah, 834 00:41:26,080 --> 00:41:29,240 Speaker 1: we have found star systems with more than five stars. 835 00:41:29,440 --> 00:41:32,080 Speaker 1: There's one we saw recently which is a crazy six 836 00:41:32,440 --> 00:41:36,000 Speaker 1: star system. This one has like three pairs of binaries, 837 00:41:36,160 --> 00:41:38,279 Speaker 1: So you have like three of these little guys and 838 00:41:38,360 --> 00:41:42,879 Speaker 1: that's organized into a triinary system. Whoa, So it's three 839 00:41:43,000 --> 00:41:46,440 Speaker 1: binary stars. But is it hierarchical? Like is do you 840 00:41:46,520 --> 00:41:48,920 Speaker 1: have like a binary star and then the binary system 841 00:41:49,000 --> 00:41:50,880 Speaker 1: orbiting that one, and then you have a binary system 842 00:41:50,920 --> 00:41:53,520 Speaker 1: orbiting the other one? You have two binary systems where 843 00:41:53,560 --> 00:41:55,239 Speaker 1: they have like a larger one and a smaller one 844 00:41:55,560 --> 00:41:57,840 Speaker 1: and then those two are organized into a binary and 845 00:41:57,920 --> 00:42:01,520 Speaker 1: then that quad star system is in a binary relationship 846 00:42:01,680 --> 00:42:05,640 Speaker 1: with another binary star system. So it's definitely hierarchical. It's 847 00:42:05,680 --> 00:42:09,239 Speaker 1: like a Sementi swinging party in space. Yeah, and I 848 00:42:09,280 --> 00:42:11,399 Speaker 1: don't know if they have any planets. We haven't seen any, 849 00:42:11,520 --> 00:42:14,480 Speaker 1: but it's pretty crazy. Why wouldn't they have planets? Well, 850 00:42:14,520 --> 00:42:17,000 Speaker 1: it's just so chaotic, right, there's so much gravity all 851 00:42:17,040 --> 00:42:18,840 Speaker 1: the time that would be pretty hard to find a 852 00:42:18,920 --> 00:42:21,719 Speaker 1: stable orbit. Like, it's amazing that even these found a 853 00:42:21,760 --> 00:42:24,759 Speaker 1: stable orbit, right, I guess how did they find that orbit? 854 00:42:24,920 --> 00:42:27,000 Speaker 1: Did they? Do you think they were born, you know, 855 00:42:27,160 --> 00:42:29,279 Speaker 1: near each other and that's just what they settled into. 856 00:42:29,400 --> 00:42:31,680 Speaker 1: Or do you think they you know, one of them 857 00:42:31,760 --> 00:42:34,479 Speaker 1: was cruising by and God pulled in. It's actually really 858 00:42:34,600 --> 00:42:39,000 Speaker 1: hard to capture another object like Gravitationally, it's actually impossible 859 00:42:39,080 --> 00:42:42,560 Speaker 1: to capture an object that's passing by because of conservation 860 00:42:42,640 --> 00:42:45,879 Speaker 1: of energy. If it's coming by and it's not in orbit, 861 00:42:46,000 --> 00:42:48,440 Speaker 1: that means it's not a hyperbolic trajectory. And if it 862 00:42:48,520 --> 00:42:51,840 Speaker 1: unless it loses energy somehow, it's just gonna whizz around 863 00:42:51,880 --> 00:42:54,040 Speaker 1: you and shoot out into space. So to capture an 864 00:42:54,080 --> 00:42:57,240 Speaker 1: object you need like something else to give away energy 865 00:42:57,440 --> 00:43:00,319 Speaker 1: or collide with it or something. So much more likely 866 00:43:00,440 --> 00:43:02,840 Speaker 1: is that this formed this way, that it came together 867 00:43:02,960 --> 00:43:05,920 Speaker 1: this way gravitationally from the initial collapse in cloud. It 868 00:43:06,000 --> 00:43:09,200 Speaker 1: just happened to form six points there that gobble up 869 00:43:09,200 --> 00:43:11,759 Speaker 1: a lot of the mass and then coalesced into this 870 00:43:11,960 --> 00:43:14,600 Speaker 1: stable system. And then these are pretty rare, right, Like 871 00:43:14,840 --> 00:43:17,000 Speaker 1: we only know of one. Yeah, this is really rare. 872 00:43:17,040 --> 00:43:19,839 Speaker 1: There's very few systems like this, and this particular one 873 00:43:20,040 --> 00:43:23,400 Speaker 1: is super weird because not only does it have like 874 00:43:23,640 --> 00:43:26,759 Speaker 1: six stars in it, but they are eclipsing. So these 875 00:43:26,800 --> 00:43:30,320 Speaker 1: stars are all eclipsing binaries, which means that all of 876 00:43:30,400 --> 00:43:34,040 Speaker 1: them orbit each other in just the right plane so 877 00:43:34,160 --> 00:43:36,279 Speaker 1: that they block the light from each other on its 878 00:43:36,320 --> 00:43:39,240 Speaker 1: way to Earth. So it's like, not only is it weird, 879 00:43:39,320 --> 00:43:41,960 Speaker 1: but they all happen to be arranged exactly the right 880 00:43:42,040 --> 00:43:44,759 Speaker 1: way to eclipse each other's light from the point of 881 00:43:44,800 --> 00:43:46,719 Speaker 1: view of Earth, like they're on the same level and 882 00:43:46,760 --> 00:43:49,399 Speaker 1: this level just happens to be like in our eyeline. Yeah, 883 00:43:49,800 --> 00:43:51,759 Speaker 1: And so this was discovered by a test, which is 884 00:43:51,840 --> 00:43:55,640 Speaker 1: this awesome telescope that looks for exoplanets via this transit 885 00:43:55,719 --> 00:43:58,080 Speaker 1: method of dimming of the light of a star to 886 00:43:58,120 --> 00:44:00,160 Speaker 1: see something passing in front of it. And so we 887 00:44:00,239 --> 00:44:04,680 Speaker 1: detected all of these crazy activities in this one solar system. Wow, 888 00:44:04,920 --> 00:44:08,040 Speaker 1: it was like blinking like crazy, like randomly. Yeah. And 889 00:44:08,440 --> 00:44:11,000 Speaker 1: just like in the other hierarchies, like the closer the 890 00:44:11,080 --> 00:44:15,080 Speaker 1: little binaries orbit each other sometimes days or years, but 891 00:44:15,200 --> 00:44:18,680 Speaker 1: the furthest pair, like the quad system that's orbiting around 892 00:44:18,719 --> 00:44:22,120 Speaker 1: the other binary system, they orbit every two thousand years. 893 00:44:22,480 --> 00:44:25,200 Speaker 1: This was really like a quad couple that's much closer 894 00:44:25,440 --> 00:44:27,719 Speaker 1: and then a binary system that's a little further away, 895 00:44:27,800 --> 00:44:30,480 Speaker 1: but they are tied together. Wow. Well that's kind of romantic. 896 00:44:30,520 --> 00:44:32,800 Speaker 1: They've been together for two thousand years. That's something to 897 00:44:32,880 --> 00:44:34,920 Speaker 1: aspire to. But now I'm afraid to ask, Daniel, can 898 00:44:34,960 --> 00:44:37,440 Speaker 1: you have a solar system with more than six stars? 899 00:44:37,840 --> 00:44:40,320 Speaker 1: You know you can? And we have found one. The 900 00:44:40,480 --> 00:44:44,239 Speaker 1: craziest star system we've ever seen has seven stars in it. 901 00:44:44,920 --> 00:44:48,160 Speaker 1: And this is a star system called New Scorpii, which 902 00:44:48,200 --> 00:44:51,160 Speaker 1: is pretty awesome name. It's five light years away and 903 00:44:51,200 --> 00:44:54,200 Speaker 1: it has seven stars. It's like, geez, get greedy much? 904 00:44:54,520 --> 00:44:59,160 Speaker 1: They just like the party. I guess we're just jealous, right, 905 00:44:59,160 --> 00:45:00,719 Speaker 1: I'm like, man, they're having a lot more fun over 906 00:45:00,800 --> 00:45:03,959 Speaker 1: there than we are. I think with each start there's 907 00:45:04,000 --> 00:45:07,319 Speaker 1: just more drama. You know, that's soap operated in your life. 908 00:45:07,400 --> 00:45:09,919 Speaker 1: Some people can't live without it. But this seven star 909 00:45:10,000 --> 00:45:13,600 Speaker 1: system is sort of organized into two systems. One of 910 00:45:13,640 --> 00:45:15,759 Speaker 1: them has four stars and the other one has three, 911 00:45:16,120 --> 00:45:19,080 Speaker 1: and those two systems orbit each other. But it's really cool, 912 00:45:19,239 --> 00:45:21,719 Speaker 1: hierarchic goal. It's hard to describe over the radio, so 913 00:45:21,800 --> 00:45:24,160 Speaker 1: I suggest you google it. But it's pretty cool system 914 00:45:24,360 --> 00:45:26,919 Speaker 1: like two clusters that are kind of far away enough 915 00:45:27,040 --> 00:45:30,080 Speaker 1: from each other that they don't destabilize each other, but 916 00:45:30,120 --> 00:45:32,000 Speaker 1: they're orbiting around each other, and each one of those 917 00:45:32,040 --> 00:45:36,520 Speaker 1: clusters has another two separate clusters within them. Yeah, exactly. 918 00:45:36,880 --> 00:45:39,279 Speaker 1: It's pretty crazy. And so you know, life on that 919 00:45:39,400 --> 00:45:42,719 Speaker 1: planet with like seven sunrises and seven sunsets every day, 920 00:45:43,239 --> 00:45:46,600 Speaker 1: that sounds pretty exciting. Imagine having seven parents, that's gonna 921 00:45:46,640 --> 00:45:49,840 Speaker 1: be pretty confusing. Like how do you make decisions. I 922 00:45:49,880 --> 00:45:53,319 Speaker 1: guess you pull all your parents and the majority wins. Well, 923 00:45:53,400 --> 00:45:57,040 Speaker 1: mommy said I could have dessert, which mommy mom said 924 00:45:57,360 --> 00:45:59,680 Speaker 1: that I can have a treat. The majority of my 925 00:45:59,760 --> 00:46:03,120 Speaker 1: mom said I never treat, all right, well, I give 926 00:46:03,200 --> 00:46:06,040 Speaker 1: the universe, you're right, a lot of stars for being 927 00:46:06,239 --> 00:46:08,680 Speaker 1: so awesome and unpredictable. I mean, who would have thought 928 00:46:08,760 --> 00:46:11,479 Speaker 1: you could have seven stars in one system. It's pretty cool, 929 00:46:11,800 --> 00:46:14,399 Speaker 1: and it's just an example of how the universe does 930 00:46:14,480 --> 00:46:17,279 Speaker 1: stuff that you didn't expect. It does exactly what you 931 00:46:17,440 --> 00:46:20,799 Speaker 1: didn't anticipate, and that everything we thought we've learned about 932 00:46:20,840 --> 00:46:23,560 Speaker 1: the universe from last thousand years, assumptions that were at 933 00:46:23,600 --> 00:46:27,040 Speaker 1: the bedrock of our understanding, should be questioned because they 934 00:46:27,120 --> 00:46:29,600 Speaker 1: could be wrong and things could be very different out 935 00:46:29,640 --> 00:46:31,719 Speaker 1: there in other corners of the universe. I'm starting to 936 00:46:31,800 --> 00:46:33,919 Speaker 1: question YELP reviews. Maybe they should go up to seven 937 00:46:33,960 --> 00:46:37,840 Speaker 1: stars because the universe has said in the bar, the 938 00:46:37,920 --> 00:46:40,040 Speaker 1: stars bar. All right, well, we hope you enjoyed that, 939 00:46:40,160 --> 00:46:42,600 Speaker 1: And speaking of stars, give us a good rating on 940 00:46:42,880 --> 00:46:46,280 Speaker 1: iTunes or Spotify or or wherever you're listening to this podcast, 941 00:46:46,520 --> 00:46:49,200 Speaker 1: and tell your friends thanks for joining us. See you 942 00:46:49,320 --> 00:46:59,400 Speaker 1: next time. Thanks for listening, and remember that Daniel and 943 00:46:59,480 --> 00:47:01,840 Speaker 1: joor Hicks Blame the Universe is a production of I 944 00:47:02,120 --> 00:47:05,520 Speaker 1: Heart Radio or more podcast from my Heart Radio. Visit 945 00:47:05,560 --> 00:47:09,040 Speaker 1: the I Heart Radio app, Apple Podcasts, or wherever you 946 00:47:09,160 --> 00:47:11,640 Speaker 1: listen to your favorite shows h