1 00:00:08,520 --> 00:00:11,240 Speaker 1: Hey, Kelly, do you ever wish that our night sky 2 00:00:11,560 --> 00:00:14,960 Speaker 1: was I don't know, a little bit more dramatic, more dramatic. 3 00:00:15,360 --> 00:00:19,639 Speaker 1: We've got a huge moon, planets, stars, and all of 4 00:00:19,680 --> 00:00:22,079 Speaker 1: the Milky Way. You've got pretty high standards for the 5 00:00:22,160 --> 00:00:24,200 Speaker 1: night sky. What did you have in mind? I don't know. 6 00:00:24,320 --> 00:00:26,960 Speaker 1: Sometimes I think it's boring to have just that one 7 00:00:27,240 --> 00:00:30,080 Speaker 1: huge moon. It seems like it might be more exciting 8 00:00:30,120 --> 00:00:33,080 Speaker 1: to have lots of little moons up there. Okay, all right, 9 00:00:33,159 --> 00:00:36,440 Speaker 1: that's true. It's kind of like having an only child. Yeah, 10 00:00:36,479 --> 00:00:39,720 Speaker 1: and not just an only child, like a single mega child. 11 00:00:40,479 --> 00:00:44,000 Speaker 1: You want drama. What's more dramatic than the Earth's mega 12 00:00:44,120 --> 00:00:46,800 Speaker 1: child hovering above you in the sky. Yeah, I guess 13 00:00:46,800 --> 00:00:48,880 Speaker 1: I wanted drama. But now I'm worried that the idea 14 00:00:48,880 --> 00:00:51,720 Speaker 1: of a mega child is going to give me nightmares. Yeah, 15 00:00:51,760 --> 00:01:09,600 Speaker 1: me too. I like my two little ones. Hi. I'm Daniel. 16 00:01:09,680 --> 00:01:12,240 Speaker 1: I'm a particle physicist, and I'm very happy to have 17 00:01:12,319 --> 00:01:16,120 Speaker 1: too normal sized children instead of one mega child. And 18 00:01:16,200 --> 00:01:18,920 Speaker 1: I'm Kelly. I'm a parasitologist, and I also have two 19 00:01:18,959 --> 00:01:21,280 Speaker 1: normal sized children, and that works well for me. You 20 00:01:21,360 --> 00:01:24,240 Speaker 1: having considered the concept of like combining them together into 21 00:01:24,280 --> 00:01:27,080 Speaker 1: one child unification of the children. You know, Zach likes 22 00:01:27,120 --> 00:01:29,720 Speaker 1: to joke that they stack when he stacks them. They 23 00:01:29,760 --> 00:01:31,760 Speaker 1: don't seem very happy about it, and so you know, 24 00:01:31,800 --> 00:01:34,080 Speaker 1: I haven't thought too hard about trying to combine them. 25 00:01:34,080 --> 00:01:35,800 Speaker 1: I don't think they'd be big fans of that. I'm 26 00:01:35,800 --> 00:01:38,320 Speaker 1: pretty sure my kids wouldn't be into that either. Well, 27 00:01:38,360 --> 00:01:41,960 Speaker 1: Welcome to the podcast Daniel and Jorge explain the universe 28 00:01:42,040 --> 00:01:44,720 Speaker 1: and which we ask the hard questions of the universe. 29 00:01:44,760 --> 00:01:47,720 Speaker 1: We talked about the crazy stuff that's out there deep 30 00:01:47,800 --> 00:01:50,000 Speaker 1: in the cosmos, and we talked about the tiny little 31 00:01:50,040 --> 00:01:53,160 Speaker 1: particles that are wriggling around inside my children, your children, 32 00:01:53,400 --> 00:01:56,960 Speaker 1: and everybody's children. We try to explore the entire universe 33 00:01:57,000 --> 00:01:59,720 Speaker 1: and explain all of it to you. Normally we have 34 00:01:59,800 --> 00:02:02,360 Speaker 1: my friend and co host Jorge him here on the podcast, 35 00:02:02,480 --> 00:02:05,800 Speaker 1: but he's unavailable today, so we have our wonderful, hilarious 36 00:02:05,840 --> 00:02:08,920 Speaker 1: guest host, Kelly Weener Smith. Hello, I'm excited to be back. 37 00:02:09,000 --> 00:02:11,160 Speaker 1: Thanks very much for joining us and for talking to 38 00:02:11,240 --> 00:02:14,880 Speaker 1: us about crazy stuff in the universe. So on the podcast, 39 00:02:14,960 --> 00:02:18,480 Speaker 1: we sometimes like to dig into stuff that's really complicated, 40 00:02:18,800 --> 00:02:21,280 Speaker 1: like how does quantum field theory work, and what is 41 00:02:21,320 --> 00:02:23,680 Speaker 1: the real charge of the electron? Or what is it 42 00:02:23,760 --> 00:02:26,760 Speaker 1: like to go inside a black hole? These are deep 43 00:02:26,800 --> 00:02:29,160 Speaker 1: and complicated questions about the universe that we try to 44 00:02:29,160 --> 00:02:32,160 Speaker 1: take apart and explain to you. But sometimes we also 45 00:02:32,200 --> 00:02:35,440 Speaker 1: like to dive into simpler seeming in questions, questions that 46 00:02:35,760 --> 00:02:38,320 Speaker 1: might seem like they have an obvious answer but then 47 00:02:38,400 --> 00:02:41,640 Speaker 1: have some interesting little wrinkles. It's good to have diversity, yeah, 48 00:02:41,639 --> 00:02:44,119 Speaker 1: because questions are at the heart of science, and they're 49 00:02:44,160 --> 00:02:46,800 Speaker 1: not just the questions that scientists ask when they're doing 50 00:02:46,840 --> 00:02:49,320 Speaker 1: their research, but we're also interested in the questions that 51 00:02:49,440 --> 00:02:53,040 Speaker 1: everybody asks. And sometimes the best questions are the questions 52 00:02:53,080 --> 00:02:56,960 Speaker 1: that children ask, the most obvious questions which sometimes have 53 00:02:57,040 --> 00:02:59,359 Speaker 1: a tricky answer. And I remember looking up at the 54 00:02:59,480 --> 00:03:02,840 Speaker 1: night sky with my kids, who are now twelve and fourteen, 55 00:03:02,960 --> 00:03:07,520 Speaker 1: but earlier asked very simple, basic, fun questions about the universe, 56 00:03:07,600 --> 00:03:11,160 Speaker 1: like why do we only have one moon? Or do 57 00:03:11,480 --> 00:03:14,480 Speaker 1: we only have one moon? Kelly, what kind of questions 58 00:03:14,480 --> 00:03:16,360 Speaker 1: do your kids ask when they look at the night sky? 59 00:03:16,639 --> 00:03:18,959 Speaker 1: I was just trying to think of a good example 60 00:03:19,120 --> 00:03:22,320 Speaker 1: of Like, my daughter is seven, and she's always asking 61 00:03:22,320 --> 00:03:24,560 Speaker 1: me questions that I don't know the answer to some 62 00:03:24,680 --> 00:03:27,560 Speaker 1: of them super fundamental, which makes me think, how is 63 00:03:27,600 --> 00:03:30,120 Speaker 1: it that I'm walking around not knowing the answer to 64 00:03:30,160 --> 00:03:32,560 Speaker 1: all of these fundamental things, but yet I still managed 65 00:03:32,600 --> 00:03:35,440 Speaker 1: to survive. But no good example is coming to mind 66 00:03:35,520 --> 00:03:37,480 Speaker 1: right now. But we've got one of those apps on 67 00:03:37,480 --> 00:03:39,120 Speaker 1: our phone where you can sort of point it at 68 00:03:39,200 --> 00:03:40,960 Speaker 1: whatever in the night sky and it tells you what 69 00:03:41,000 --> 00:03:42,600 Speaker 1: it is. And we spend a lot of time sitting 70 00:03:42,640 --> 00:03:44,880 Speaker 1: on our car at night looking up at stuff, and 71 00:03:44,920 --> 00:03:46,840 Speaker 1: it's a lot of fun. She asked lots of questions, 72 00:03:46,880 --> 00:03:48,800 Speaker 1: but nothing's coming to mind right now that I did 73 00:03:48,800 --> 00:03:50,840 Speaker 1: not know the answer to. What's your favorite question your 74 00:03:50,880 --> 00:03:52,960 Speaker 1: kids have asked you? One of my favorite questions my 75 00:03:53,080 --> 00:03:56,080 Speaker 1: kids have asked me are questions like where are we 76 00:03:56,200 --> 00:03:59,080 Speaker 1: in the universe. You know, they're just getting used to 77 00:03:59,120 --> 00:04:01,440 Speaker 1: the idea of like our houses in the neighborhood, and 78 00:04:01,480 --> 00:04:03,680 Speaker 1: the neighborhood is in the city, and that city is 79 00:04:03,720 --> 00:04:06,480 Speaker 1: in a state somewhere we have like a location and address, 80 00:04:07,000 --> 00:04:09,200 Speaker 1: and so they wanted to know, like, where are we 81 00:04:09,320 --> 00:04:13,520 Speaker 1: in the universe? What's our like universe address? And of course, 82 00:04:13,520 --> 00:04:16,800 Speaker 1: you know, the hardcore physics answer is that every place 83 00:04:16,839 --> 00:04:19,480 Speaker 1: in the universe is the same, and physics doesn't care 84 00:04:19,520 --> 00:04:22,680 Speaker 1: about location and translationally and variant and stuff. But that 85 00:04:22,720 --> 00:04:25,760 Speaker 1: answer is not very satisfying for a four year old. Yeah, 86 00:04:25,800 --> 00:04:27,400 Speaker 1: that's why it's a bummer to have a physicist for 87 00:04:27,440 --> 00:04:31,920 Speaker 1: a dad. But instead I try to describe to them, 88 00:04:31,960 --> 00:04:34,039 Speaker 1: you know, what the galaxy looks like, and how the 89 00:04:34,040 --> 00:04:36,440 Speaker 1: galaxy fits in with other galaxies, and what we know 90 00:04:36,520 --> 00:04:39,279 Speaker 1: about sort of our cosmic neighborhood. And the thing I 91 00:04:39,360 --> 00:04:42,479 Speaker 1: love about their questions is that they are both easy 92 00:04:42,640 --> 00:04:46,520 Speaker 1: and hard. They're like easy to ask but sometimes hard 93 00:04:46,600 --> 00:04:49,360 Speaker 1: to answer. And they're the obvious questions, as you said, 94 00:04:49,360 --> 00:04:51,760 Speaker 1: that you don't always think about when you're walking around 95 00:04:51,760 --> 00:04:53,839 Speaker 1: the world. But that's why I think that children really 96 00:04:53,880 --> 00:04:57,599 Speaker 1: are sometimes the most natural scientists, because they don't just 97 00:04:57,720 --> 00:04:59,960 Speaker 1: accept things as they are. They ask questions about the 98 00:05:00,000 --> 00:05:01,840 Speaker 1: and say why is it this way or is it 99 00:05:01,880 --> 00:05:04,560 Speaker 1: that way? After all? Totally, And what I love about 100 00:05:04,600 --> 00:05:06,960 Speaker 1: Ada is that she'll tell me that I'm wrong. I 101 00:05:07,000 --> 00:05:09,360 Speaker 1: wish I had that confidence. So you know, not only 102 00:05:09,400 --> 00:05:11,880 Speaker 1: do they ask good questions, but they still have the 103 00:05:11,920 --> 00:05:14,560 Speaker 1: confidence of children to be like, no, I don't think so. 104 00:05:14,760 --> 00:05:16,840 Speaker 1: And so today in the podcast, we'll be talking about 105 00:05:16,839 --> 00:05:19,960 Speaker 1: a question which seems to have an obvious answer. So 106 00:05:20,000 --> 00:05:27,919 Speaker 1: on today's program will be answering the question how many 107 00:05:28,040 --> 00:05:31,359 Speaker 1: moons does the Earth have? So, Kelly, tell me what 108 00:05:31,440 --> 00:05:32,719 Speaker 1: you thought when you saw that we would be talking 109 00:05:32,720 --> 00:05:35,360 Speaker 1: about this today. So you sent me a list of 110 00:05:35,360 --> 00:05:38,039 Speaker 1: topics we could talk about, And when I read this one, 111 00:05:38,400 --> 00:05:42,120 Speaker 1: I thought, well, the answer seems obvious. The answer is one. 112 00:05:42,680 --> 00:05:45,560 Speaker 1: And if the answer seems obvious, then either Daniel needs 113 00:05:45,600 --> 00:05:48,560 Speaker 1: to be fired because he's not asking good questions anymore, 114 00:05:49,160 --> 00:05:53,120 Speaker 1: or there's something fundamental that I'm missing, and it's probably 115 00:05:53,160 --> 00:05:56,000 Speaker 1: the second. And so I suggested that we talked about 116 00:05:56,000 --> 00:05:57,760 Speaker 1: this one because I figured this was a question that 117 00:05:57,800 --> 00:06:00,360 Speaker 1: would teach me something new. Awesome. This is a fun 118 00:06:00,480 --> 00:06:02,640 Speaker 1: question to dig into. We get to hear about like 119 00:06:02,720 --> 00:06:05,360 Speaker 1: what exactly is a moon, what counts as a moon, 120 00:06:05,720 --> 00:06:08,159 Speaker 1: even a little bit about the etymology of the word 121 00:06:08,240 --> 00:06:10,760 Speaker 1: moon and when it came into use, and what else 122 00:06:10,839 --> 00:06:13,440 Speaker 1: is out there orbiting around the Earth and could you 123 00:06:13,560 --> 00:06:16,440 Speaker 1: call it a moon? So, as usual, before I dug 124 00:06:16,480 --> 00:06:18,760 Speaker 1: into this, I wanted to know what everybody else out 125 00:06:18,880 --> 00:06:21,320 Speaker 1: there thought. Sometimes I used to walk around the campus 126 00:06:21,320 --> 00:06:24,240 Speaker 1: if you see Irvine and ask students there these questions 127 00:06:24,279 --> 00:06:27,440 Speaker 1: to see what the general level of knowledge was or confusion. 128 00:06:27,520 --> 00:06:30,359 Speaker 1: These days, of course, because the pandemic, I'm sending emails 129 00:06:30,360 --> 00:06:34,159 Speaker 1: out into the Internet asking listeners to speculate baselessly without 130 00:06:34,200 --> 00:06:37,479 Speaker 1: the chance to do any research on these difficult physics questions. 131 00:06:37,600 --> 00:06:39,840 Speaker 1: Did you actually stop students on the campus and ask 132 00:06:39,920 --> 00:06:42,200 Speaker 1: them how many moons does they are? Have? No, I 133 00:06:42,200 --> 00:06:45,080 Speaker 1: haven't because this question is too recent, But I wonder 134 00:06:45,160 --> 00:06:47,560 Speaker 1: what they would say. I've noticed that our listeners tend 135 00:06:47,560 --> 00:06:50,200 Speaker 1: to give better informed answers than the random you see 136 00:06:50,200 --> 00:06:53,440 Speaker 1: Irvine student. Nothing against you see Irvine. Of course, our 137 00:06:53,480 --> 00:06:56,080 Speaker 1: listeners may just be like a subset of the universe 138 00:06:56,080 --> 00:06:59,360 Speaker 1: that's more interested in understanding the universe. But I hope 139 00:06:59,400 --> 00:07:01,279 Speaker 1: one day to get back to campus and getting to 140 00:07:01,320 --> 00:07:03,560 Speaker 1: ask the students those questions. It was fun to sort 141 00:07:03,560 --> 00:07:05,960 Speaker 1: of see their faces when I asked them these questions. 142 00:07:06,040 --> 00:07:08,240 Speaker 1: I bet you have a reputation as being one of 143 00:07:08,240 --> 00:07:11,400 Speaker 1: the like super weird professors. Well, you know, I don't 144 00:07:11,520 --> 00:07:13,680 Speaker 1: dress very fancy, so maybe they just think I'm some 145 00:07:13,840 --> 00:07:17,560 Speaker 1: random homeless person asking them hard physical questions. Every college 146 00:07:17,600 --> 00:07:21,600 Speaker 1: has homeless person or physics professor, it can be hard 147 00:07:21,640 --> 00:07:23,920 Speaker 1: to tell the difference, physics professor, you can't tell the 148 00:07:23,960 --> 00:07:28,440 Speaker 1: difference between Yeah, anyway, Thank you to everybody who volunteered 149 00:07:28,440 --> 00:07:30,720 Speaker 1: to answer these questions. If you'd like to participate for 150 00:07:30,800 --> 00:07:33,440 Speaker 1: a future episode of the podcast, please write to me 151 00:07:33,720 --> 00:07:36,960 Speaker 1: two questions at Daniel and Jorge dot com. Here's what 152 00:07:37,040 --> 00:07:40,320 Speaker 1: some of our listeners had to say. The obvious answer 153 00:07:40,360 --> 00:07:43,120 Speaker 1: that pops into my head immediately would be one. So 154 00:07:43,200 --> 00:07:46,800 Speaker 1: I'm pretty sure that answer is wrong. Well, we have 155 00:07:47,080 --> 00:07:53,520 Speaker 1: just our celebrity moon, the moon, and I don't know, 156 00:07:54,040 --> 00:07:59,080 Speaker 1: maybe we might have caught up some small objects there, 157 00:08:00,160 --> 00:08:05,800 Speaker 1: probably a Deslo car elon musk scent, who knows. I 158 00:08:05,840 --> 00:08:10,280 Speaker 1: don't know exactly. I'm one sure that the Earth has 159 00:08:10,360 --> 00:08:14,640 Speaker 1: two moons, the classic moon that we see in the 160 00:08:14,720 --> 00:08:18,240 Speaker 1: sky and Keith Moon. I would say the Earth has 161 00:08:18,320 --> 00:08:21,040 Speaker 1: one moon. I don't know if you would consider satellites 162 00:08:21,120 --> 00:08:23,320 Speaker 1: or a space station a moon because the orbit the Earth, 163 00:08:24,800 --> 00:08:27,280 Speaker 1: but I would probably just consider one moon. Well, I 164 00:08:27,320 --> 00:08:32,280 Speaker 1: guess this depends on your definition of moon the natural moons. 165 00:08:32,360 --> 00:08:36,199 Speaker 1: It has the one large natural moon, and I believe 166 00:08:36,280 --> 00:08:39,440 Speaker 1: they've discovered a couple of asteroids that have been captured 167 00:08:39,720 --> 00:08:44,480 Speaker 1: in loose enough for bits that they're probably temporary. If 168 00:08:44,480 --> 00:08:49,319 Speaker 1: you're going to call any artificial uh satellite a moon, 169 00:08:50,760 --> 00:08:54,400 Speaker 1: which they've been called artificial moons, then that number goes 170 00:08:54,440 --> 00:08:58,600 Speaker 1: into the millions, depending on how small a particle you 171 00:08:58,640 --> 00:09:03,080 Speaker 1: want to count. There's nuts and bolts and pieces of 172 00:09:03,200 --> 00:09:09,200 Speaker 1: rocket and larger things that satellites, fragments of satellites that 173 00:09:09,240 --> 00:09:13,360 Speaker 1: have collided with each other, so uh, a whole lot 174 00:09:13,440 --> 00:09:15,480 Speaker 1: of them, all right, Kelly, So what do you think 175 00:09:15,480 --> 00:09:18,160 Speaker 1: about our listeners responses here? I thought there were some 176 00:09:18,280 --> 00:09:21,640 Speaker 1: very insightful responses, you know. One of them was essentially 177 00:09:21,640 --> 00:09:25,600 Speaker 1: asking questions about maybe how do we define moons. I 178 00:09:25,640 --> 00:09:28,760 Speaker 1: thought somebody had a clever thought that the Tesla car 179 00:09:28,960 --> 00:09:31,360 Speaker 1: might now be sort of orbiting, although I think of 180 00:09:31,400 --> 00:09:35,479 Speaker 1: the Tesla car was shot Mars word instead of moonword. 181 00:09:35,640 --> 00:09:37,400 Speaker 1: But it was clear that people sort of thought through 182 00:09:37,440 --> 00:09:39,680 Speaker 1: their answers, and yeah, they had some clever answers. What 183 00:09:39,720 --> 00:09:42,080 Speaker 1: do you think? Yeah, I was impressed as well. In 184 00:09:42,120 --> 00:09:43,720 Speaker 1: the end, of course, it's going to come down to 185 00:09:43,760 --> 00:09:45,679 Speaker 1: the definition. I hope that we end up with the 186 00:09:45,720 --> 00:09:48,800 Speaker 1: definition of moon that doesn't allow Elon Musk to have 187 00:09:48,960 --> 00:09:52,520 Speaker 1: created his own personal moon. That would seems sort of unsatisfying. 188 00:09:52,640 --> 00:09:55,000 Speaker 1: That would be too much power for one person. The 189 00:09:55,080 --> 00:09:59,000 Speaker 1: dude's already a billionaire and owns three like really valuable 190 00:09:59,000 --> 00:10:02,480 Speaker 1: companies like it, doesn't need to create astronomical objects on 191 00:10:02,520 --> 00:10:04,560 Speaker 1: top of all of it. Although he wants to create 192 00:10:04,640 --> 00:10:07,559 Speaker 1: a Mars colony, which is maybe even more powerful than 193 00:10:08,000 --> 00:10:10,240 Speaker 1: creating a moon. So I guess we'll have to see 194 00:10:10,240 --> 00:10:11,800 Speaker 1: what the future holds. Do you think that's because he 195 00:10:11,840 --> 00:10:14,440 Speaker 1: wants to be dictator of Mars? I like joking about 196 00:10:14,480 --> 00:10:19,559 Speaker 1: that with Zack. Yes, he claims he wants a representative 197 00:10:19,640 --> 00:10:22,959 Speaker 1: not a direct democracy, So we'll see what happens when 198 00:10:22,960 --> 00:10:24,720 Speaker 1: the time comes. Well, if he gets to pick who 199 00:10:24,800 --> 00:10:26,400 Speaker 1: goes to Mars, and they're probably going to elect him 200 00:10:26,440 --> 00:10:29,160 Speaker 1: president anyway. But let's get back to the topic. We're 201 00:10:29,160 --> 00:10:31,920 Speaker 1: not talking about Elon Musk's plan to colonize Mars. We're 202 00:10:31,920 --> 00:10:34,600 Speaker 1: talking about moons and how many moons the Earth has 203 00:10:34,760 --> 00:10:38,440 Speaker 1: and what exactly is a moon? So let's dig into 204 00:10:38,480 --> 00:10:42,560 Speaker 1: that first and talk about what qualifies as a moon. So, 205 00:10:42,640 --> 00:10:45,040 Speaker 1: without doing any research, Kelly, what would you use to 206 00:10:45,120 --> 00:10:47,960 Speaker 1: define a moon? So I would have guessed that a 207 00:10:48,000 --> 00:10:53,240 Speaker 1: moon is a big thing that isn't bigger than the 208 00:10:53,280 --> 00:10:56,120 Speaker 1: planet that it orbits. So a big thing that orbits 209 00:10:56,160 --> 00:10:59,480 Speaker 1: around a planet, and it has to be big, but 210 00:10:59,520 --> 00:11:02,439 Speaker 1: it can't be bigger than the thing that it's orbiting around. 211 00:11:02,840 --> 00:11:05,280 Speaker 1: That's how I would have defined it. But but probably 212 00:11:05,320 --> 00:11:08,360 Speaker 1: that's wrong. And then your definition would it have to 213 00:11:08,360 --> 00:11:10,440 Speaker 1: be natural or could be manned? Me that? Could we 214 00:11:10,480 --> 00:11:14,680 Speaker 1: build an artificial moon? Oh h no, No, I've always 215 00:11:14,679 --> 00:11:18,199 Speaker 1: thought of it as being natural. Yeah, what about you? Well, 216 00:11:18,200 --> 00:11:20,120 Speaker 1: I really wasn't sure because it seems like in lots 217 00:11:20,160 --> 00:11:23,080 Speaker 1: of directions there are arbitrary distinctions you have to make. 218 00:11:23,240 --> 00:11:25,680 Speaker 1: And that's the problem often in astronomy is that the 219 00:11:25,720 --> 00:11:29,160 Speaker 1: categories between things get blurred, and you always find something 220 00:11:29,280 --> 00:11:31,840 Speaker 1: right on the edge between the different categories, and in 221 00:11:31,880 --> 00:11:33,240 Speaker 1: the end, you know, we're just we're looking at the 222 00:11:33,280 --> 00:11:35,800 Speaker 1: universe and we're trying to categorize it to understand is 223 00:11:35,800 --> 00:11:37,720 Speaker 1: that we can talk about it together. Doesn't mean that 224 00:11:37,760 --> 00:11:41,360 Speaker 1: those categories actually reflect something deep and true about the universe. 225 00:11:41,360 --> 00:11:44,640 Speaker 1: There's sometimes just the words we've used to describe stuff, 226 00:11:44,960 --> 00:11:46,760 Speaker 1: and so as we see more stuff out there in 227 00:11:46,760 --> 00:11:49,439 Speaker 1: the universe, we're gonna find things that break those categories. 228 00:11:49,520 --> 00:11:51,400 Speaker 1: But the definition that I found for moon is that 229 00:11:51,440 --> 00:11:54,480 Speaker 1: it has to be a quote natural body, right, So 230 00:11:54,520 --> 00:11:57,520 Speaker 1: it needs to be a natural body that's orbiting a planet. 231 00:11:57,840 --> 00:12:00,440 Speaker 1: And to me already this is problem that like a 232 00:12:00,520 --> 00:12:03,840 Speaker 1: natural body means not like a human made satellite. So 233 00:12:03,960 --> 00:12:07,079 Speaker 1: we built a death Star for example, Officially that wouldn't 234 00:12:07,160 --> 00:12:12,400 Speaker 1: qualify as a moon. But what if we just like 235 00:12:12,800 --> 00:12:15,400 Speaker 1: you know, pulled out a huge chunk of Earth and 236 00:12:15,520 --> 00:12:18,040 Speaker 1: threw it out into space and then it went into 237 00:12:18,160 --> 00:12:21,120 Speaker 1: orbit around the Earth. Is that a natural body? It's 238 00:12:21,160 --> 00:12:24,360 Speaker 1: like made of rock, right, It's essentially the same process 239 00:12:24,400 --> 00:12:27,360 Speaker 1: that created our moon as we understand it. But I 240 00:12:27,360 --> 00:12:30,080 Speaker 1: think according to this definition, it wouldn't be a moon 241 00:12:30,280 --> 00:12:32,280 Speaker 1: because you know, it would have been like as the 242 00:12:32,320 --> 00:12:34,920 Speaker 1: result of a human process. It really does seem like 243 00:12:34,960 --> 00:12:36,360 Speaker 1: if you just took a chunk of earth and you 244 00:12:36,480 --> 00:12:39,320 Speaker 1: put it up there, it should count. But I suppose 245 00:12:39,360 --> 00:12:42,240 Speaker 1: satellites are just chunks of Earth that we've we've done 246 00:12:42,240 --> 00:12:45,600 Speaker 1: things too, that we send up into space, and so 247 00:12:46,080 --> 00:12:49,079 Speaker 1: maybe it shouldn't count. Yeah, exactly, That's where I was going. 248 00:12:49,160 --> 00:12:52,040 Speaker 1: What is a satellite other than like an ultra refined 249 00:12:52,160 --> 00:12:55,120 Speaker 1: piece of Earth that you've somehow, you know, manipulated into 250 00:12:55,160 --> 00:12:58,120 Speaker 1: a complex technological object. But in the end, it's a 251 00:12:58,120 --> 00:13:00,920 Speaker 1: piece of the Earth that we've launched into space. And 252 00:13:00,960 --> 00:13:02,760 Speaker 1: you know, for those of you who don't know the 253 00:13:02,880 --> 00:13:05,959 Speaker 1: history of our moon, we think that our moon is 254 00:13:06,000 --> 00:13:09,040 Speaker 1: basically a big chunk of Earth that was vaulted out 255 00:13:09,120 --> 00:13:12,280 Speaker 1: into space when another proto planet hit Earth when it 256 00:13:12,360 --> 00:13:15,240 Speaker 1: was very very young, and this collision led to this 257 00:13:15,480 --> 00:13:18,319 Speaker 1: enormous blab of stuff getting tossed out there, which eventually 258 00:13:18,360 --> 00:13:21,800 Speaker 1: coalesced into the Moon. And when we studied the surface 259 00:13:21,840 --> 00:13:24,400 Speaker 1: of the Moon, we found elements of it which look 260 00:13:24,480 --> 00:13:27,040 Speaker 1: exactly the same as elements of the surface of the Earth, 261 00:13:27,040 --> 00:13:28,800 Speaker 1: which suggests that they really do have sort of a 262 00:13:28,880 --> 00:13:31,840 Speaker 1: common origin. So this definition of a moon being a 263 00:13:31,960 --> 00:13:35,640 Speaker 1: natural body not a human made object is a little tricky, 264 00:13:35,760 --> 00:13:37,640 Speaker 1: and I don't think the definition there is very clear. 265 00:13:37,800 --> 00:13:41,640 Speaker 1: Can I ask a sort of tangential question, of course, So, well, 266 00:13:41,720 --> 00:13:43,880 Speaker 1: Zach and I were reading about the Moon. We came 267 00:13:43,920 --> 00:13:47,160 Speaker 1: across this fact that the Moon is sort of carbon poor, 268 00:13:47,320 --> 00:13:48,960 Speaker 1: like maybe there's some carbon up there, but you're gonna 269 00:13:48,960 --> 00:13:50,679 Speaker 1: have trouble growing plants and stuff because there's not a 270 00:13:50,720 --> 00:13:53,559 Speaker 1: lot of carbon. If the Moon is just a chunk 271 00:13:53,600 --> 00:13:57,640 Speaker 1: of Earth that got expelled, why do we have so 272 00:13:57,720 --> 00:13:59,320 Speaker 1: much carbon and they have so little. Is that the 273 00:13:59,360 --> 00:14:02,320 Speaker 1: result of natal processes that happened after the Moon got 274 00:14:02,360 --> 00:14:05,720 Speaker 1: cut off partly, Yeah, Mostly the Earth and the Moon 275 00:14:05,800 --> 00:14:09,040 Speaker 1: are made up of very similar stuff. It's mostly oxygen 276 00:14:09,160 --> 00:14:12,520 Speaker 1: and silicon and calcium and iron and that kind of stuff. 277 00:14:12,559 --> 00:14:15,440 Speaker 1: That's because we think that the Moon and the Earth 278 00:14:15,480 --> 00:14:18,360 Speaker 1: are made up of the remnants of a huge collision 279 00:14:18,480 --> 00:14:21,840 Speaker 1: between the proto Earth and a Mars sized planet, like 280 00:14:22,120 --> 00:14:25,480 Speaker 1: fifty million years after the Solar system formed, and the 281 00:14:25,600 --> 00:14:29,440 Speaker 1: remnants of that huge collision coalesced into the Earth and 282 00:14:29,520 --> 00:14:32,000 Speaker 1: into the Moon. But you're right that there is very 283 00:14:32,080 --> 00:14:34,480 Speaker 1: little carbon on the Moon, but there is carbon on 284 00:14:34,520 --> 00:14:38,560 Speaker 1: the Earth's surface, and we're not sure why. One theory 285 00:14:38,680 --> 00:14:42,200 Speaker 1: is that carbon tends to form very volatile compounds, things 286 00:14:42,240 --> 00:14:44,160 Speaker 1: that would end up in an atmosphere if the Moon 287 00:14:44,240 --> 00:14:46,800 Speaker 1: could keep one. So the Earth hangs onto some of 288 00:14:46,840 --> 00:14:49,400 Speaker 1: these things, some of this carbon, because it's big enough 289 00:14:49,440 --> 00:14:51,880 Speaker 1: to keep hold of its atmosphere it has more gravity, 290 00:14:52,040 --> 00:14:54,800 Speaker 1: But the Moon can't. Anything like an atmosphere on the 291 00:14:54,800 --> 00:14:58,200 Speaker 1: Moon just boils away. Interesting okay, thanks. So the definition 292 00:14:58,240 --> 00:14:59,960 Speaker 1: of a moon is that needs to be a natural 293 00:15:00,000 --> 00:15:03,080 Speaker 1: a body in orbit around a planet, and you said 294 00:15:03,120 --> 00:15:06,160 Speaker 1: that it needs to be big. Officially, technically there's no 295 00:15:06,520 --> 00:15:10,440 Speaker 1: minimum size to a moon. A moon could be like huge, 296 00:15:10,560 --> 00:15:13,840 Speaker 1: like our moon, or you know, according to astronomers, it's 297 00:15:13,880 --> 00:15:16,720 Speaker 1: okay to have a moon that's like a kilometer in size. 298 00:15:16,800 --> 00:15:19,320 Speaker 1: I find that very unsatisfying. Like to me, a moon 299 00:15:19,560 --> 00:15:21,640 Speaker 1: is something that you should be able to, like put 300 00:15:21,680 --> 00:15:24,160 Speaker 1: a settlement on one day, and you can't really do 301 00:15:24,240 --> 00:15:28,920 Speaker 1: that with a one kilometer sized quote unquote moon. I 302 00:15:28,920 --> 00:15:31,280 Speaker 1: don't know. I don't want to buy that, but apparently 303 00:15:31,280 --> 00:15:32,720 Speaker 1: it's part of the definition. It would be like the 304 00:15:32,720 --> 00:15:35,640 Speaker 1: little prints right walking around this tiny little planet. But 305 00:15:35,720 --> 00:15:38,920 Speaker 1: I think that comes from our experience, right, just because 306 00:15:38,960 --> 00:15:41,080 Speaker 1: we have this one big moon, we tend to think 307 00:15:41,280 --> 00:15:43,520 Speaker 1: that's what you gotta have in a moon. But as 308 00:15:43,560 --> 00:15:45,640 Speaker 1: well talk about later, so many planets in the Solar 309 00:15:45,680 --> 00:15:47,840 Speaker 1: System don't have a huge moon, to have a lot 310 00:15:47,840 --> 00:15:51,000 Speaker 1: of smaller moons, And so part of the joy of 311 00:15:51,000 --> 00:15:54,320 Speaker 1: astronomy and and of exploring the universe is discovering that 312 00:15:54,440 --> 00:15:57,000 Speaker 1: our corner of the universe is weird, is unusual, is 313 00:15:57,040 --> 00:15:59,320 Speaker 1: not representative, and we've got to sort of like stretch 314 00:15:59,360 --> 00:16:01,720 Speaker 1: our mind then get used to a different way of 315 00:16:01,720 --> 00:16:04,080 Speaker 1: thinking about what a moon is. Yeah, it is really 316 00:16:04,080 --> 00:16:06,960 Speaker 1: hard to wrap your mind around just how different it is. 317 00:16:07,000 --> 00:16:08,880 Speaker 1: And yeah, I'm very earth centric. I guess I would 318 00:16:08,880 --> 00:16:11,360 Speaker 1: like moons to all sort of fits in a nice 319 00:16:11,400 --> 00:16:13,920 Speaker 1: little mold that matches the moon that I have, and 320 00:16:13,960 --> 00:16:15,840 Speaker 1: you touch it on really all the important issues. I 321 00:16:15,840 --> 00:16:17,800 Speaker 1: think that was really tremendous. The other thing you mentioned 322 00:16:18,040 --> 00:16:20,200 Speaker 1: is that it shouldn't be bigger than the planet, right, 323 00:16:20,760 --> 00:16:23,360 Speaker 1: And in the definition of a moon, officially, the upper 324 00:16:23,400 --> 00:16:26,000 Speaker 1: limit on the size of a moon is pretty vague, 325 00:16:26,440 --> 00:16:29,280 Speaker 1: Like what happens when the moon approaches the size of 326 00:16:29,280 --> 00:16:31,600 Speaker 1: the planet. Then you might ask, like, well, which one 327 00:16:31,640 --> 00:16:33,520 Speaker 1: is the planet and which one is the moon? Right? 328 00:16:33,640 --> 00:16:36,960 Speaker 1: Or if they're exactly equal size, could you consider them 329 00:16:37,000 --> 00:16:39,760 Speaker 1: to be like a binary planet system? So where does 330 00:16:40,040 --> 00:16:44,560 Speaker 1: our moon fall relative? And they'll like Earth to Moon 331 00:16:44,800 --> 00:16:47,880 Speaker 1: ratio side, Like, is our moon big for a moon? 332 00:16:48,120 --> 00:16:50,080 Speaker 1: Is it the biggest relative to the size of the 333 00:16:50,120 --> 00:16:52,880 Speaker 1: planet it orbits is? So is our moon weird relative 334 00:16:52,920 --> 00:16:55,280 Speaker 1: to the other moons? Our moon is very weird. Our 335 00:16:55,320 --> 00:16:58,920 Speaker 1: moon is basically that megachild. The diameter of the Moon 336 00:16:59,400 --> 00:17:01,880 Speaker 1: is more than a quarter of the diameter of the Earth, 337 00:17:02,360 --> 00:17:05,119 Speaker 1: and that's the biggest moon to planet ratio in the 338 00:17:05,119 --> 00:17:08,080 Speaker 1: Solar System by like a factor of five. There's no 339 00:17:08,240 --> 00:17:10,480 Speaker 1: other planet out there that has such a big moon 340 00:17:10,600 --> 00:17:13,920 Speaker 1: relative to the planet. Like there are moons of Jupiter 341 00:17:14,240 --> 00:17:16,240 Speaker 1: that are roughly the same size as our moon, but 342 00:17:16,280 --> 00:17:19,040 Speaker 1: of course Jupiter is huge, and so relative to the 343 00:17:19,040 --> 00:17:21,840 Speaker 1: size of Jupiter, those moons are very very small, So 344 00:17:21,880 --> 00:17:24,480 Speaker 1: we have a really weird big moon. You know, it's 345 00:17:24,520 --> 00:17:26,800 Speaker 1: kind of amazing that we've managed to figure out anything, 346 00:17:26,880 --> 00:17:29,159 Speaker 1: which is sort of a phrase that, if I'm remembering correctly, 347 00:17:29,200 --> 00:17:31,600 Speaker 1: I've said in almost every single one of these episodes 348 00:17:31,640 --> 00:17:33,760 Speaker 1: we've done together. But it seems like, you know, our 349 00:17:33,800 --> 00:17:36,479 Speaker 1: Solar System is so weird, and our planet and the 350 00:17:36,480 --> 00:17:39,159 Speaker 1: moon is so weird. It gives us such a weird 351 00:17:39,240 --> 00:17:41,399 Speaker 1: frame of reference. But I know, it's exciting that we 352 00:17:41,440 --> 00:17:44,120 Speaker 1: can still figure stuff out. Yeah, and it's a real 353 00:17:44,280 --> 00:17:47,920 Speaker 1: journey to peel away these preconceptions and understand that things 354 00:17:47,920 --> 00:17:51,280 Speaker 1: we thought were fundamental, things we thought we're obvious or universal, 355 00:17:51,600 --> 00:17:54,200 Speaker 1: are really just unusual. You know. It's just like when 356 00:17:54,240 --> 00:17:56,760 Speaker 1: you go traveling and you discover like, oh, not everybody 357 00:17:56,880 --> 00:17:59,320 Speaker 1: drinks coffee for breakfast. You know, it turns out there 358 00:17:59,320 --> 00:18:01,600 Speaker 1: are other ways to live, and that's the joy of 359 00:18:01,640 --> 00:18:04,440 Speaker 1: exploring the universe, you know, discovering the tea is also 360 00:18:04,480 --> 00:18:08,159 Speaker 1: acceptable at breakfast times. No, no, no, no, no, no, 361 00:18:08,840 --> 00:18:11,240 Speaker 1: that's just wrong. One fact that I really liked while 362 00:18:11,280 --> 00:18:13,200 Speaker 1: I was reading through here was that those like one 363 00:18:13,280 --> 00:18:17,880 Speaker 1: kilometer size moons are sometimes called moonlits. And I thought 364 00:18:17,880 --> 00:18:19,920 Speaker 1: that was super cute. So I asked my seven year 365 00:18:19,960 --> 00:18:21,840 Speaker 1: old today. I was like, how many moons does the 366 00:18:21,840 --> 00:18:25,479 Speaker 1: Earth have? So she, being a very clever kid, was like, well, 367 00:18:25,520 --> 00:18:27,399 Speaker 1: I thought it was one, but you're asking me this, 368 00:18:27,560 --> 00:18:30,720 Speaker 1: so what does that mean? And and so I told 369 00:18:30,720 --> 00:18:32,320 Speaker 1: her like, well, you know you can have these little 370 00:18:32,359 --> 00:18:35,000 Speaker 1: things called moonlits. And she said, well, what does that mean? 371 00:18:35,080 --> 00:18:37,160 Speaker 1: And so I tried to explain that let's means little 372 00:18:37,200 --> 00:18:39,639 Speaker 1: things and she was like, well, when else does it 373 00:18:39,680 --> 00:18:42,840 Speaker 1: mean that? And I had a like, uh, you know, 374 00:18:42,880 --> 00:18:44,720 Speaker 1: like a moment of not being able to figure it out, 375 00:18:44,720 --> 00:18:46,439 Speaker 1: but I came up with piglets and outlets, and I 376 00:18:46,480 --> 00:18:48,480 Speaker 1: was very proud of myself. So anyway, that was a 377 00:18:48,520 --> 00:18:50,680 Speaker 1: fun moment with the seven year old today. Yeah, I 378 00:18:50,720 --> 00:18:53,439 Speaker 1: love those little endings lits and like, it's just like 379 00:18:53,480 --> 00:18:57,280 Speaker 1: the diminutive in Spanish, you know, eto or eno or 380 00:18:57,320 --> 00:18:59,640 Speaker 1: these kind of things in romance languages. So I'm glad 381 00:18:59,640 --> 00:19:01,440 Speaker 1: that we have those in English. Also, you could really 382 00:19:01,480 --> 00:19:04,000 Speaker 1: stick them on anything, you know, like I'm not having dessert, 383 00:19:04,000 --> 00:19:08,840 Speaker 1: I'm having dessert lits. It makes everything cuter, it really does. 384 00:19:09,280 --> 00:19:11,159 Speaker 1: So where are we with the moons? Moons have to 385 00:19:11,200 --> 00:19:14,520 Speaker 1: be a natural body orbiting a planet. No minimum size. 386 00:19:14,760 --> 00:19:17,679 Speaker 1: The oppera limit is kind of vague. One thing I 387 00:19:17,760 --> 00:19:20,760 Speaker 1: read suggested that you could effectively describe an upper limit 388 00:19:20,840 --> 00:19:24,400 Speaker 1: on the moon by requiring that the center of mass 389 00:19:24,440 --> 00:19:28,239 Speaker 1: of the planet and moon together should be inside the 390 00:19:28,280 --> 00:19:30,960 Speaker 1: diameter of the planet. Right, So the center of mass 391 00:19:30,960 --> 00:19:33,719 Speaker 1: of two objects is sort of like the weighted average 392 00:19:34,040 --> 00:19:36,320 Speaker 1: of all of their stuff. If you've got more stuff 393 00:19:36,320 --> 00:19:38,159 Speaker 1: in the planet than in the moon, it's going to 394 00:19:38,200 --> 00:19:41,040 Speaker 1: be closer to the planet mathematically and physically. It's actually 395 00:19:41,160 --> 00:19:43,840 Speaker 1: the location that the two things are orbiting. Right. We 396 00:19:43,960 --> 00:19:46,600 Speaker 1: say that the Moon, for example, orbits the Earth, but 397 00:19:46,680 --> 00:19:49,840 Speaker 1: actually the two things are orbiting each other, or more precisely, 398 00:19:50,040 --> 00:19:53,480 Speaker 1: they're both orbiting the center of mass of the two things. 399 00:19:53,720 --> 00:19:55,680 Speaker 1: And if you have two things that are equal mass, 400 00:19:55,800 --> 00:19:58,280 Speaker 1: then their center of masses right between them. If one 401 00:19:58,280 --> 00:20:00,720 Speaker 1: of them is infinitely massive, then the center of mass 402 00:20:00,800 --> 00:20:03,159 Speaker 1: is at the center of that very massive object. In 403 00:20:03,160 --> 00:20:05,920 Speaker 1: a more realistic scenario, where one thing is very massive 404 00:20:05,960 --> 00:20:07,919 Speaker 1: and one thing is much smaller, you can have the 405 00:20:07,920 --> 00:20:10,640 Speaker 1: center of mass of the system of the two things 406 00:20:11,040 --> 00:20:14,399 Speaker 1: be close to the center of the larger object. And 407 00:20:14,440 --> 00:20:16,919 Speaker 1: so here the definition is like, is the center of 408 00:20:17,000 --> 00:20:20,680 Speaker 1: mass of the two objects underneath the ground within the 409 00:20:20,920 --> 00:20:24,160 Speaker 1: radius of the larger object. That's sort of a cool definition. 410 00:20:24,320 --> 00:20:25,359 Speaker 1: That is a cool So I have a couple of 411 00:20:25,440 --> 00:20:29,000 Speaker 1: questions to see if I understand. So one, does it 412 00:20:29,040 --> 00:20:32,399 Speaker 1: depend on how far apart the things are or is 413 00:20:32,400 --> 00:20:34,879 Speaker 1: it like you just when you make this comparison, you 414 00:20:34,880 --> 00:20:36,720 Speaker 1: you know, sort of mentally put these things right next 415 00:20:36,760 --> 00:20:38,800 Speaker 1: to each other and then compare the center of mass. 416 00:20:38,920 --> 00:20:41,600 Speaker 1: It definitely depends on how far apart they are, right 417 00:20:41,680 --> 00:20:44,520 Speaker 1: because for example, if they're equally massive, you'd be right 418 00:20:44,560 --> 00:20:47,200 Speaker 1: between them, and that definitely depends on the distance between 419 00:20:47,240 --> 00:20:49,159 Speaker 1: the two objects. Yes, and so that would mean you 420 00:20:49,200 --> 00:20:51,720 Speaker 1: have two planets as opposed to a moon and a 421 00:20:51,760 --> 00:20:55,160 Speaker 1: planet in that definition. And so so you have two 422 00:20:55,160 --> 00:20:58,239 Speaker 1: things that are like one is just a little bit 423 00:20:58,280 --> 00:21:00,760 Speaker 1: smaller than the other, and one is big er, but 424 00:21:00,840 --> 00:21:05,400 Speaker 1: the smaller one is made out of something much more 425 00:21:06,000 --> 00:21:08,480 Speaker 1: massive or dense or I'm not quite sure what word 426 00:21:08,480 --> 00:21:11,480 Speaker 1: I'm looking for here. Could the smaller thing end up 427 00:21:11,520 --> 00:21:14,360 Speaker 1: being the planet that gets orbited by a bigger thing 428 00:21:14,400 --> 00:21:18,480 Speaker 1: because it has more like gravitational pull? Absolutely? Yeah. For example, 429 00:21:18,800 --> 00:21:21,720 Speaker 1: if you had something orbiting a black hole, right, a 430 00:21:21,760 --> 00:21:24,760 Speaker 1: super duper dense object, then the center of mass of 431 00:21:24,760 --> 00:21:27,320 Speaker 1: the system is definitely going to be within the event horizon, 432 00:21:27,440 --> 00:21:29,600 Speaker 1: even if though the black hole could be smaller. Right, 433 00:21:29,600 --> 00:21:31,680 Speaker 1: black holes are very very compact. They don't have to 434 00:21:31,720 --> 00:21:34,760 Speaker 1: be very very large, but they are supermassive. So that's awesome. 435 00:21:34,800 --> 00:21:37,639 Speaker 1: You're really like pushing the boundaries of this definition. But 436 00:21:37,720 --> 00:21:39,399 Speaker 1: I don't know. I guess a black hole could have 437 00:21:39,440 --> 00:21:41,440 Speaker 1: a planet orbiting it. I'm not sure if you would 438 00:21:41,440 --> 00:21:43,360 Speaker 1: call that a planet or a moon, right, if you're 439 00:21:43,440 --> 00:21:46,080 Speaker 1: orbiting a black hole, Yeah, it's trippy, I guess, I, 440 00:21:46,720 --> 00:21:51,080 Speaker 1: as a not physicist, find it sort of unsatisfying that 441 00:21:51,119 --> 00:21:54,080 Speaker 1: if the moon is too far away, it might or 442 00:21:54,119 --> 00:21:56,400 Speaker 1: if something that feels sort of moon like is too 443 00:21:56,400 --> 00:21:59,080 Speaker 1: far away, it wouldn't count as a moon because the 444 00:21:59,119 --> 00:22:02,399 Speaker 1: center of masses is not within the bigger body or something. 445 00:22:02,640 --> 00:22:05,560 Speaker 1: It feels like distance shouldn't matter for the definition, But 446 00:22:05,960 --> 00:22:08,040 Speaker 1: that's a biologist take on it. Well, it definitely has 447 00:22:08,040 --> 00:22:10,560 Speaker 1: to be in orbit. And I think that one problem 448 00:22:10,720 --> 00:22:13,000 Speaker 1: with this whole categorization is that this is like a 449 00:22:13,119 --> 00:22:16,080 Speaker 1: natural hierarchy. I mean, you have the Sun and the 450 00:22:16,119 --> 00:22:19,480 Speaker 1: stuff orbiting around the Sun, and then you call those planets, 451 00:22:19,480 --> 00:22:21,960 Speaker 1: but that's sort of arbitrary because they're orbiting around the Sun. 452 00:22:22,320 --> 00:22:25,119 Speaker 1: And then there's things orbiting around the planets, right, and 453 00:22:25,160 --> 00:22:27,360 Speaker 1: you call those moons. In the end, it's just sort 454 00:22:27,359 --> 00:22:30,440 Speaker 1: of a natural hierarchy of stuff orbiting stuff that's orbiting 455 00:22:30,480 --> 00:22:33,440 Speaker 1: other stuff, and our categorization of it is you're really 456 00:22:33,440 --> 00:22:35,760 Speaker 1: going to try to draw lines there where they really 457 00:22:35,800 --> 00:22:39,560 Speaker 1: aren't lines. Yeah, but that's like a fundamental problem with science. 458 00:22:39,600 --> 00:22:43,119 Speaker 1: You know, in biology, we categorize things, and constantly nature 459 00:22:43,200 --> 00:22:45,480 Speaker 1: does not care how we categorize it. She moves away 460 00:22:45,480 --> 00:22:47,639 Speaker 1: outside of our categories. Yeah, I guess it's tough just 461 00:22:47,680 --> 00:22:50,560 Speaker 1: finding a definition that is useful I guess in biology 462 00:22:50,760 --> 00:22:52,800 Speaker 1: there was a huge revolution a couple hundred years ago, 463 00:22:52,880 --> 00:22:55,280 Speaker 1: right because you guys had been categorizing stuff based on 464 00:22:55,480 --> 00:22:58,600 Speaker 1: how it looked and what it did, and then discovered 465 00:22:58,760 --> 00:23:01,840 Speaker 1: the genetic relation ships between everything, and that there was 466 00:23:01,920 --> 00:23:05,159 Speaker 1: actually a real, true organization to all these animals that 467 00:23:05,280 --> 00:23:08,439 Speaker 1: didn't necessarily respect how they looked or how we observe 468 00:23:08,560 --> 00:23:10,479 Speaker 1: them well. And then it turns out that, you know, 469 00:23:10,560 --> 00:23:13,359 Speaker 1: how do you define species? That's actually a pretty difficult question. 470 00:23:13,440 --> 00:23:15,720 Speaker 1: The tree of life doesn't just branch, it sort of comes, 471 00:23:15,800 --> 00:23:19,399 Speaker 1: the branches come back together and you get horizontal gene transfer. 472 00:23:19,440 --> 00:23:22,480 Speaker 1: And how do you categorize species of bacteria when they're 473 00:23:22,480 --> 00:23:25,600 Speaker 1: swapping jeans all the time, and it gets complicated fast. Well, 474 00:23:25,600 --> 00:23:28,280 Speaker 1: in physics, it's interesting they think about how these words 475 00:23:28,320 --> 00:23:30,920 Speaker 1: were used for a long time. People use the word 476 00:23:31,040 --> 00:23:34,520 Speaker 1: satellite to also refer to moons, and this is before 477 00:23:34,560 --> 00:23:38,520 Speaker 1: we had things in space like GPS and telecommunications, satellites 478 00:23:38,560 --> 00:23:41,440 Speaker 1: and you know, laser weapons and all that kind of stuff. Now, 479 00:23:41,440 --> 00:23:43,879 Speaker 1: when you say satellite, you think of something people build, 480 00:23:43,920 --> 00:23:47,200 Speaker 1: maybe electronics and launched into space. But before spot Nick, 481 00:23:47,240 --> 00:23:51,680 Speaker 1: before ninety seven, astronomers used the word satellite to talk 482 00:23:51,680 --> 00:23:55,720 Speaker 1: about anything orbiting another object, and so they didn't really 483 00:23:55,800 --> 00:24:00,320 Speaker 1: use the word moon scientifically. They referred to Luna, for example, 484 00:24:00,480 --> 00:24:04,119 Speaker 1: as Earth satellite. Then when they launched sput Nick, they realized, 485 00:24:04,119 --> 00:24:05,760 Speaker 1: whole on a second, what are we going to call that? 486 00:24:06,000 --> 00:24:08,679 Speaker 1: And so they started to use the word artificial satellite. 487 00:24:08,680 --> 00:24:10,679 Speaker 1: But that was a little bit too cumbersome, and so 488 00:24:10,800 --> 00:24:14,040 Speaker 1: now we just say satellite when we mean artificial satellite. 489 00:24:14,280 --> 00:24:17,439 Speaker 1: And then moon, which was a word mostly used like 490 00:24:17,520 --> 00:24:20,680 Speaker 1: in science fiction and a sort of popular culture, became 491 00:24:20,800 --> 00:24:23,639 Speaker 1: a more official scientific word. I think that's sort of 492 00:24:23,640 --> 00:24:26,879 Speaker 1: cool that the scientists adopted a word from sort of 493 00:24:26,920 --> 00:24:29,800 Speaker 1: common usage. That's totally fascinating. And I've been reading about 494 00:24:29,880 --> 00:24:32,040 Speaker 1: the space race and I didn't know this history of 495 00:24:32,040 --> 00:24:34,880 Speaker 1: the word satellite. And when I saw that they named 496 00:24:34,880 --> 00:24:37,239 Speaker 1: spot Nick an artificial satellite, I was like, well, that's 497 00:24:37,280 --> 00:24:39,760 Speaker 1: sort of clunk. Why not just call it satellite? But 498 00:24:39,840 --> 00:24:42,639 Speaker 1: it makes sense now. A lot of the fathers of 499 00:24:42,720 --> 00:24:46,480 Speaker 1: rocket science or whatever. We're really into sci fi. I 500 00:24:46,480 --> 00:24:49,200 Speaker 1: think almost all of the fathers of rocket science claimed 501 00:24:49,200 --> 00:24:51,879 Speaker 1: that they were inspired by Jules Verns. What is it 502 00:24:51,920 --> 00:24:54,000 Speaker 1: called to the moon? I wonder if the fact that 503 00:24:54,040 --> 00:24:56,560 Speaker 1: they were all super into sci fi sort of helped 504 00:24:56,880 --> 00:24:59,480 Speaker 1: get the word moon into the scientific literature. Yeah it 505 00:24:59,480 --> 00:25:01,600 Speaker 1: makes me one or what else? Like will in the 506 00:25:01,720 --> 00:25:04,159 Speaker 1: future be part of science. You know, things that we 507 00:25:04,200 --> 00:25:06,080 Speaker 1: say but you wouldn't hear a scientists say, you know, 508 00:25:06,119 --> 00:25:09,119 Speaker 1: like a shooting star is our word for a meteor, 509 00:25:09,240 --> 00:25:11,000 Speaker 1: but you never see that in the science paper. But 510 00:25:11,040 --> 00:25:13,720 Speaker 1: maybe someday in the future, you know, the language will 511 00:25:13,920 --> 00:25:18,719 Speaker 1: transmogrify itself into official scientific physics speaker could be. All right, 512 00:25:18,840 --> 00:25:21,040 Speaker 1: So we have our definition of a moon. It has 513 00:25:21,080 --> 00:25:25,040 Speaker 1: to be a natural body, right, not something engineered by 514 00:25:25,160 --> 00:25:28,919 Speaker 1: humanity or elon Musk. Has to orbit a planet. But 515 00:25:29,080 --> 00:25:32,639 Speaker 1: there's really no minimum size to it, though there seems 516 00:25:32,640 --> 00:25:34,680 Speaker 1: to be some sort of sense of an upper limit 517 00:25:34,720 --> 00:25:37,560 Speaker 1: that you shouldn't have your moon being larger than your planet. 518 00:25:37,640 --> 00:25:40,199 Speaker 1: All right, So, now that we have our definition, or 519 00:25:40,200 --> 00:25:41,960 Speaker 1: at least a definition we're gonna work with for the 520 00:25:42,000 --> 00:25:44,359 Speaker 1: rest of this episode, let's take a break before we 521 00:25:44,400 --> 00:25:59,600 Speaker 1: move back to figuring out exactly how many moons Earth has. 522 00:25:59,600 --> 00:26:03,439 Speaker 1: So we have a definition. Now, how many moons do 523 00:26:03,520 --> 00:26:06,760 Speaker 1: we have, Daniel, So let's count them first. Of course, 524 00:26:06,920 --> 00:26:09,439 Speaker 1: we have the number one candidate. The classic moon, the 525 00:26:09,480 --> 00:26:13,000 Speaker 1: one you're familiar with, the one we all grew up loving. Right, 526 00:26:13,320 --> 00:26:16,000 Speaker 1: this is the moon we call the moon, which is 527 00:26:16,119 --> 00:26:18,240 Speaker 1: sort of a silly name, right, calling the moon the moon. 528 00:26:18,280 --> 00:26:20,760 Speaker 1: It reminds me actually, when I was a kid, we 529 00:26:20,800 --> 00:26:22,960 Speaker 1: had a cat and nobody could agree on what to 530 00:26:23,000 --> 00:26:25,600 Speaker 1: call the cat, so we just called it the cat, 531 00:26:26,240 --> 00:26:29,240 Speaker 1: and that just became its name. And for a while 532 00:26:29,240 --> 00:26:31,600 Speaker 1: I felt sad for like, oh, poor cat doesn't get 533 00:26:31,600 --> 00:26:34,639 Speaker 1: a name, But he didn't care. It got fed, it 534 00:26:34,720 --> 00:26:37,240 Speaker 1: got pet it doesn't need a name. I think it's 535 00:26:37,280 --> 00:26:40,320 Speaker 1: good that you became more creative that you got I 536 00:26:40,320 --> 00:26:43,520 Speaker 1: can't tell if calling it the moon is very egocentric, 537 00:26:43,600 --> 00:26:45,960 Speaker 1: like that is our moon, so it is the moon, 538 00:26:46,280 --> 00:26:49,240 Speaker 1: or if it just represents a lack of creativity. Hard 539 00:26:49,280 --> 00:26:52,000 Speaker 1: to say. Well, as we were saying earlier, it's really weird, 540 00:26:52,160 --> 00:26:54,480 Speaker 1: Like it's huge. It's more than a quarter of the 541 00:26:54,520 --> 00:26:57,320 Speaker 1: diameter of the Earth in the Solar System. The next 542 00:26:57,440 --> 00:26:59,919 Speaker 1: largest moon relative to his planet is one of the 543 00:27:00,000 --> 00:27:02,199 Speaker 1: moons of Neptune, which is almost six percent of the 544 00:27:02,240 --> 00:27:05,480 Speaker 1: diameter of Neptune. So that's a pretty big gap. Like 545 00:27:05,880 --> 00:27:09,160 Speaker 1: mostly moons are small compared to their planet. The moon 546 00:27:09,320 --> 00:27:11,399 Speaker 1: is really a very weird and Or and I did 547 00:27:11,400 --> 00:27:13,880 Speaker 1: a whole episode about how the Earth got its moon 548 00:27:13,920 --> 00:27:16,800 Speaker 1: and the various theories and how people are testing those, 549 00:27:16,800 --> 00:27:18,600 Speaker 1: and so if you're interested in the details of the 550 00:27:18,720 --> 00:27:22,359 Speaker 1: history of the moon, then good check out that episode. 551 00:27:22,440 --> 00:27:24,560 Speaker 1: But it's interesting that, you know, in the sort of 552 00:27:24,560 --> 00:27:27,760 Speaker 1: the history of astronomy I was reading about this, people 553 00:27:27,800 --> 00:27:32,080 Speaker 1: didn't really think about the Moon as a moon until 554 00:27:32,200 --> 00:27:35,879 Speaker 1: they discovered Jupiter's moons. Like people were looking up in 555 00:27:35,960 --> 00:27:38,239 Speaker 1: the sky and they saw, of course stars and they 556 00:27:38,280 --> 00:27:40,479 Speaker 1: saw the moon, but they just thought of it as 557 00:27:40,520 --> 00:27:46,000 Speaker 1: like another celestial object. They were wrong. And then you know, 558 00:27:46,040 --> 00:27:49,240 Speaker 1: when Galileo and other folks saw the moons of Jupiter 559 00:27:49,240 --> 00:27:50,960 Speaker 1: and they're like, hey, look at that, there are things 560 00:27:51,119 --> 00:27:53,560 Speaker 1: orbiting Jupiter. That's when it clicked in the place and 561 00:27:53,560 --> 00:27:56,360 Speaker 1: they're like, wait a second, what Jupiter's got over there 562 00:27:56,440 --> 00:27:59,159 Speaker 1: is the same thing that we've got over here. And 563 00:27:59,200 --> 00:28:01,000 Speaker 1: that's when they really eyes that this was a whole 564 00:28:01,000 --> 00:28:04,400 Speaker 1: new kind of thing in space. That's so interesting. That's 565 00:28:04,440 --> 00:28:06,400 Speaker 1: why it's so important to you know, to learn more 566 00:28:06,400 --> 00:28:08,320 Speaker 1: and to step outside your comfort zone because there's so 567 00:28:08,320 --> 00:28:10,560 Speaker 1: many things that become obvious when you see how other 568 00:28:10,680 --> 00:28:13,320 Speaker 1: things are done, and the moon is actually considered a 569 00:28:13,359 --> 00:28:16,200 Speaker 1: planet for a while, though the definition of a planet 570 00:28:16,200 --> 00:28:18,879 Speaker 1: has also changed. Back then, a planet was just like 571 00:28:19,160 --> 00:28:23,439 Speaker 1: another astronomical object. People didn't really understand the relationship between 572 00:28:23,440 --> 00:28:25,520 Speaker 1: the planets and the stars and all this kind of stuff. 573 00:28:25,760 --> 00:28:28,240 Speaker 1: So if you go back to very early astronomy, what 574 00:28:28,440 --> 00:28:31,560 Speaker 1: these words mean is totally different from what they mean today. 575 00:28:31,880 --> 00:28:34,600 Speaker 1: So it's pretty tricky to read, like you know, early 576 00:28:34,680 --> 00:28:38,080 Speaker 1: astronomical texts. That sounds super confusing. So it makes me wonder. 577 00:28:38,200 --> 00:28:40,880 Speaker 1: So if you can be changing what the definition of 578 00:28:40,920 --> 00:28:44,000 Speaker 1: a planet is, can you have things that are not 579 00:28:44,120 --> 00:28:48,880 Speaker 1: planets that have moons? You can definitely have things that 580 00:28:48,960 --> 00:28:52,479 Speaker 1: are not planets that have stuff orbiting them, and we 581 00:28:52,520 --> 00:28:55,120 Speaker 1: will talk about that later in the episode. There are 582 00:28:55,160 --> 00:28:57,760 Speaker 1: things in the Solar System orbiting other things that are 583 00:28:57,760 --> 00:29:00,800 Speaker 1: not planets, for sure. Sorry I got excited. It is 584 00:29:00,880 --> 00:29:03,640 Speaker 1: very cool. And for example, you know, just as a teaser, 585 00:29:03,800 --> 00:29:08,200 Speaker 1: Pluto no longer considered a planet, but it does have 586 00:29:08,360 --> 00:29:11,560 Speaker 1: things orbiting it, right, Pluto has something which you would 587 00:29:11,560 --> 00:29:15,560 Speaker 1: call a moon, Sharon, which is half the diameter of Pluto. 588 00:29:15,720 --> 00:29:18,000 Speaker 1: So that's pretty fuzzy, like which one is a planet, 589 00:29:18,000 --> 00:29:19,920 Speaker 1: which one is the moon. Pluto is only twice as 590 00:29:20,000 --> 00:29:23,840 Speaker 1: big as its moon. So if Sharon or Charon, however 591 00:29:23,880 --> 00:29:25,880 Speaker 1: you say, it ends up being called the moon, that 592 00:29:25,960 --> 00:29:29,400 Speaker 1: makes our moon a little bit less exciting. Yeah, Or 593 00:29:29,440 --> 00:29:32,240 Speaker 1: if Pluto gets repromoted back into it being a planet, 594 00:29:32,520 --> 00:29:35,200 Speaker 1: then Sharon would be the largest moon relative to a 595 00:29:35,240 --> 00:29:38,240 Speaker 1: planet in the Solar System. But because Pluto's no longer 596 00:29:38,400 --> 00:29:43,560 Speaker 1: technically a planet, Sharon loses that distinction. Sharon shure, Sharon, Alright, 597 00:29:43,600 --> 00:29:46,040 Speaker 1: so everybody knows about the moon. That's not what people 598 00:29:46,040 --> 00:29:48,960 Speaker 1: want to hear about. Are there other things orbiting the 599 00:29:48,960 --> 00:29:52,360 Speaker 1: Earth that could also be considered moons and so at? 600 00:29:52,360 --> 00:29:55,120 Speaker 1: In fact, there are, but they're sort of on the 601 00:29:55,200 --> 00:29:58,400 Speaker 1: border line of whether you would really technically call them 602 00:29:58,440 --> 00:30:00,360 Speaker 1: a moon. One of my favorites, they say, the object 603 00:30:00,360 --> 00:30:02,160 Speaker 1: which I won't even try to pronounce. You're gonna have 604 00:30:02,200 --> 00:30:03,720 Speaker 1: to look it up, but it goes by the name 605 00:30:03,800 --> 00:30:07,520 Speaker 1: of the space being, and it's this object like five 606 00:30:07,680 --> 00:30:12,120 Speaker 1: kilometers in diameter that's orbiting the Sun in the vicinity 607 00:30:12,200 --> 00:30:13,960 Speaker 1: of the Earth. But it seems like we've got to 608 00:30:13,960 --> 00:30:16,800 Speaker 1: try to pronounce it, right, So I'm gonna try crew 609 00:30:16,840 --> 00:30:20,280 Speaker 1: with me, Crew with crew with me. That sounds about right. 610 00:30:20,600 --> 00:30:22,280 Speaker 1: If I had no idea how to pronounce it, I 611 00:30:22,280 --> 00:30:24,120 Speaker 1: would guess that was correct. And I have no idea 612 00:30:24,120 --> 00:30:27,120 Speaker 1: how to pronounce it, so I guess that's correct. I 613 00:30:27,160 --> 00:30:29,320 Speaker 1: don't even know what the like, you know, origin of that, 614 00:30:29,360 --> 00:30:31,800 Speaker 1: what language that comes from. It looks Irish to me, 615 00:30:31,880 --> 00:30:34,440 Speaker 1: and I have I have no reason. I don't actually 616 00:30:34,440 --> 00:30:36,600 Speaker 1: know anything about the Irish language. So mean, maybe I 617 00:30:36,640 --> 00:30:39,480 Speaker 1: should stop. Maybe it's Gaelic for space being. Somebody out 618 00:30:39,480 --> 00:30:41,480 Speaker 1: there who speaks Gaelic let us know how to say 619 00:30:41,600 --> 00:30:45,120 Speaker 1: space being in Gaelic. So this is a fun object 620 00:30:45,240 --> 00:30:49,600 Speaker 1: because it's in orbit technically around the Sun, but it's 621 00:30:49,840 --> 00:30:52,640 Speaker 1: ring resonance with the Earth. This is something maybe people 622 00:30:52,640 --> 00:30:55,440 Speaker 1: haven't realized that, like things that are orbiting the Sun 623 00:30:55,480 --> 00:30:58,920 Speaker 1: are also interacting with each other. Right, our orbit around 624 00:30:58,960 --> 00:31:01,160 Speaker 1: the Sun is mostly a big lips and it's dominated 625 00:31:01,160 --> 00:31:03,240 Speaker 1: by the Sun. The shape of that lips is mostly 626 00:31:03,240 --> 00:31:07,040 Speaker 1: controlled by the gravitational power of the Sun. But there 627 00:31:07,040 --> 00:31:09,880 Speaker 1: are other things also orbiting with us, and they tug 628 00:31:09,920 --> 00:31:12,360 Speaker 1: on us, they pull on us, and they can change 629 00:31:12,400 --> 00:31:15,440 Speaker 1: our orbit. And sometimes you get two objects and what 630 00:31:15,480 --> 00:31:17,960 Speaker 1: you call a resonance, which means that they are very 631 00:31:18,000 --> 00:31:20,920 Speaker 1: regularly tugging on each other in a systematic way that 632 00:31:21,040 --> 00:31:23,560 Speaker 1: changes both of their orbits and makes it stable, so that, 633 00:31:23,600 --> 00:31:26,680 Speaker 1: for example, they will like meet two or four times 634 00:31:26,840 --> 00:31:29,480 Speaker 1: while going around the Sun, depending on their relative speed, 635 00:31:29,640 --> 00:31:32,120 Speaker 1: and nudge each other in just the right way. So, 636 00:31:32,160 --> 00:31:35,240 Speaker 1: for example, Saturday and Jupiter are both really really powerful 637 00:31:35,480 --> 00:31:37,920 Speaker 1: and they're in an orbital residence with each other. So 638 00:31:38,040 --> 00:31:40,440 Speaker 1: this is an object that's moving around the Sun, but 639 00:31:40,480 --> 00:31:44,480 Speaker 1: it's in resonance with the Earth, so it's strongly influenced 640 00:31:44,480 --> 00:31:47,400 Speaker 1: by the Earth's gravity. But does it does it orbit 641 00:31:47,440 --> 00:31:49,560 Speaker 1: in the same shape the Moon duns? So how is 642 00:31:49,600 --> 00:31:53,040 Speaker 1: an orbit and a resonance different? So this thing moves 643 00:31:53,120 --> 00:31:55,840 Speaker 1: around the Sun, you know, but so does the Moon. 644 00:31:56,000 --> 00:31:58,240 Speaker 1: Right if you tracked the moon. The Moon goes around 645 00:31:58,240 --> 00:32:00,680 Speaker 1: the Sun. The Earth goes around the Sun one but 646 00:32:00,800 --> 00:32:04,320 Speaker 1: the Moon is gravitationally mostly bound to the Earth. This 647 00:32:04,360 --> 00:32:08,959 Speaker 1: thing is primarily mostly bound to the Sun, but because 648 00:32:09,000 --> 00:32:11,760 Speaker 1: of the influence of the Earth, if you look at 649 00:32:11,800 --> 00:32:13,960 Speaker 1: its orbit from the Earth, it looks like it makes 650 00:32:14,000 --> 00:32:18,120 Speaker 1: a bean shaped motion around the Earth. Like if you 651 00:32:18,160 --> 00:32:20,320 Speaker 1: put the Earth, if you're sending of your reference frame 652 00:32:20,360 --> 00:32:22,680 Speaker 1: and you plot where the space being is and you 653 00:32:22,800 --> 00:32:25,200 Speaker 1: like take data points from day to day and imagine 654 00:32:25,200 --> 00:32:28,000 Speaker 1: where it is. It makes a bean shape all the 655 00:32:28,000 --> 00:32:30,240 Speaker 1: way around the Earth. So does that mean it doesn't 656 00:32:30,320 --> 00:32:33,280 Speaker 1: quite fit the definition? Because like do orbits need to 657 00:32:33,320 --> 00:32:37,200 Speaker 1: be elliptical and not not being shaped? It means that 658 00:32:37,240 --> 00:32:40,080 Speaker 1: there's not really a clear distinction. We have a three 659 00:32:40,120 --> 00:32:42,640 Speaker 1: body system. We have the Sun, we have the Earth, 660 00:32:42,760 --> 00:32:45,240 Speaker 1: and we have the space being, and they're all tugging 661 00:32:45,280 --> 00:32:48,040 Speaker 1: on each other. And so to ask the question like 662 00:32:48,440 --> 00:32:51,280 Speaker 1: what is the space being orbiting? Is it orbiting the Earth? 663 00:32:51,360 --> 00:32:54,160 Speaker 1: Is it orbiting just the Sun, doesn't have a clear 664 00:32:54,240 --> 00:32:57,400 Speaker 1: precise answer unless you define an arbitrary distinction. But there 665 00:32:57,520 --> 00:33:00,800 Speaker 1: is no natural distinction between these two scenarios. Is like 666 00:33:00,840 --> 00:33:03,840 Speaker 1: a smooth continuum of being like the Moon where you're 667 00:33:03,920 --> 00:33:07,560 Speaker 1: very clearly disorbiting the Earth and being like Mercury, where 668 00:33:07,600 --> 00:33:11,240 Speaker 1: you're very clearly disorbiting the Sun. And then these quasi 669 00:33:11,440 --> 00:33:14,920 Speaker 1: satellites of Earth that are very clearly affected by Earth 670 00:33:14,960 --> 00:33:17,640 Speaker 1: and sort of moving around Earth as they move around 671 00:33:17,640 --> 00:33:20,240 Speaker 1: the Sun. And that's what the space bean is. It's 672 00:33:20,280 --> 00:33:23,960 Speaker 1: a quasi satellite of the Earth. All right, So two things. One, 673 00:33:24,480 --> 00:33:26,479 Speaker 1: every time you say space being I'm going to continue 674 00:33:26,480 --> 00:33:28,560 Speaker 1: to chuckle. I don't think I'm gonna stop doing that, 675 00:33:28,640 --> 00:33:31,920 Speaker 1: because it's just funny and cute and too you know, 676 00:33:31,920 --> 00:33:34,320 Speaker 1: I feel like it would be really nice in science 677 00:33:34,360 --> 00:33:37,880 Speaker 1: classes if like, how hard it is to do these 678 00:33:37,880 --> 00:33:41,040 Speaker 1: definitions and how so few things fit into these definitions 679 00:33:41,120 --> 00:33:42,760 Speaker 1: was sort of made more clear, and maybe they do 680 00:33:42,840 --> 00:33:45,280 Speaker 1: that in school today. It constantly blows my mind how 681 00:33:45,360 --> 00:33:48,480 Speaker 1: much I think that we have the world bend nicely. 682 00:33:49,120 --> 00:33:52,320 Speaker 1: But everything breaks the bins. Everything breaks the bins because 683 00:33:52,360 --> 00:33:55,640 Speaker 1: the world is continuous, right, and it's huge, and so 684 00:33:55,680 --> 00:33:58,160 Speaker 1: there's always going to be an example of something in between. 685 00:33:58,200 --> 00:34:02,000 Speaker 1: These crisp distinctions are are our artificial way to try 686 00:34:02,000 --> 00:34:04,640 Speaker 1: to impose order on the universe. And back when we 687 00:34:04,680 --> 00:34:08,280 Speaker 1: hadn't seen so many things, those gaps might have seen meaningful. 688 00:34:08,480 --> 00:34:10,560 Speaker 1: But as we keep looking at the universe, we find 689 00:34:10,560 --> 00:34:12,960 Speaker 1: stuff that feels in those gaps, and you know, the 690 00:34:13,000 --> 00:34:15,160 Speaker 1: same must be true in biology, right, that's what the 691 00:34:15,239 --> 00:34:17,880 Speaker 1: duck bill platypus is. Right, It's like, hold on a second, 692 00:34:18,239 --> 00:34:20,719 Speaker 1: what do you mean mammals? You know, right, right, it's 693 00:34:20,800 --> 00:34:22,880 Speaker 1: nature's way of being, like, you cannot put me in 694 00:34:22,880 --> 00:34:26,560 Speaker 1: a box. Yeah, so that's the space being. Also, I'm 695 00:34:26,560 --> 00:34:28,239 Speaker 1: saying the space being because it is fun to say, 696 00:34:28,360 --> 00:34:30,320 Speaker 1: and because I'm trying to avoid having to pronounce the 697 00:34:30,360 --> 00:34:32,960 Speaker 1: actual name of the thing. Yeah. No, sure, that makes sense, 698 00:34:33,160 --> 00:34:34,880 Speaker 1: It's okay. So here's what I want to know. So 699 00:34:35,080 --> 00:34:39,120 Speaker 1: we're not taught that the space being is a moon 700 00:34:39,320 --> 00:34:41,480 Speaker 1: in school, or at least I wasn't. So if you 701 00:34:41,520 --> 00:34:44,960 Speaker 1: were to walk into a random astronomer's office at some 702 00:34:45,120 --> 00:34:48,880 Speaker 1: university and ask them does the space being count as 703 00:34:48,920 --> 00:34:51,480 Speaker 1: a moon? Are they gonna like roll their eyes and 704 00:34:51,520 --> 00:34:53,320 Speaker 1: be like not this again. Or are they going to 705 00:34:53,440 --> 00:34:56,480 Speaker 1: be like, oh, that's a really interesting question, Like how 706 00:34:56,480 --> 00:35:01,280 Speaker 1: does the astronomy community do this question? That's a great question. 707 00:35:01,320 --> 00:35:03,080 Speaker 1: I bet that half of them would roll our eyes 708 00:35:03,120 --> 00:35:05,319 Speaker 1: and half of them would be like, you know, I 709 00:35:05,360 --> 00:35:08,600 Speaker 1: was on the committee that decided what a quasi satellite is, 710 00:35:08,640 --> 00:35:10,680 Speaker 1: and I have a very strong opinion about it, because 711 00:35:10,719 --> 00:35:12,920 Speaker 1: you know, they get hotheaded about this stuff, right, And 712 00:35:12,920 --> 00:35:14,960 Speaker 1: you will now sit for three hours while I explain 713 00:35:15,000 --> 00:35:18,600 Speaker 1: the difference to you and you regret asking immediately. Yeah, 714 00:35:18,640 --> 00:35:21,279 Speaker 1: And sometimes I wonder, like what does it matter? You know, 715 00:35:21,360 --> 00:35:23,520 Speaker 1: people argue about whether Pluto is a planet or a 716 00:35:23,600 --> 00:35:26,680 Speaker 1: dwarf planet, like, what are the consequences? Why does anybody 717 00:35:26,719 --> 00:35:29,760 Speaker 1: really care? We're just making these names up. It doesn't 718 00:35:29,840 --> 00:35:32,960 Speaker 1: change what Pluto is. It's not like Pluto shrinks if 719 00:35:32,960 --> 00:35:36,160 Speaker 1: we call it a dwarf planet or grows in importance 720 00:35:36,239 --> 00:35:38,160 Speaker 1: if we call it a real planet. These are just 721 00:35:38,239 --> 00:35:41,600 Speaker 1: our arbitrary categorizations of the universe. So the affect how 722 00:35:41,640 --> 00:35:44,640 Speaker 1: we think and how we talk, but really it's it's inconsequential. 723 00:35:44,719 --> 00:35:46,000 Speaker 1: You know. I can see why it would matter to 724 00:35:46,000 --> 00:35:48,000 Speaker 1: you if you are an astronomer, because maybe it affects 725 00:35:48,000 --> 00:35:50,600 Speaker 1: the way you model things based on how these definitions 726 00:35:50,640 --> 00:35:53,080 Speaker 1: fall out. But I imagine to the lay public it's like, 727 00:35:53,160 --> 00:35:56,920 Speaker 1: what are we paying these people for. That's a good point. 728 00:35:57,320 --> 00:35:59,600 Speaker 1: That's a good point. And so we have this thing 729 00:35:59,640 --> 00:36:02,000 Speaker 1: that said the moons to the quasi satellite, and that's 730 00:36:02,040 --> 00:36:04,040 Speaker 1: just one example. You know, there are lots of these 731 00:36:04,080 --> 00:36:06,800 Speaker 1: things that are sort of loosely bound to the Earth 732 00:36:07,280 --> 00:36:10,120 Speaker 1: orbiting the Sun that can be fairly small, like this 733 00:36:10,200 --> 00:36:12,839 Speaker 1: thing is only five kilometers in diameter. As you get 734 00:36:12,920 --> 00:36:15,640 Speaker 1: smaller and smaller, there are many many more of these things. 735 00:36:15,680 --> 00:36:17,720 Speaker 1: Some of them are more loosely bound to the Earth. 736 00:36:18,040 --> 00:36:19,799 Speaker 1: But you know, if you're gonna call this thing a moon, 737 00:36:19,880 --> 00:36:22,040 Speaker 1: then you've got to call all those other little things 738 00:36:22,120 --> 00:36:25,000 Speaker 1: moons also, So if you're gonna open the door that wide, 739 00:36:25,040 --> 00:36:27,120 Speaker 1: then Earth is going to have a lot of little moons, 740 00:36:27,239 --> 00:36:32,200 Speaker 1: and high school astronomy becomes totally untenable. And unfortunately, it 741 00:36:32,200 --> 00:36:34,040 Speaker 1: doesn't change what it looks like in the sky, right, 742 00:36:34,080 --> 00:36:35,919 Speaker 1: You can't look up in the sky and see this thing. 743 00:36:36,200 --> 00:36:39,480 Speaker 1: The closest it ever comes to Earth is like seven 744 00:36:39,520 --> 00:36:43,000 Speaker 1: and a half million miles away, which is thirty times 745 00:36:43,160 --> 00:36:46,480 Speaker 1: further away from the Earth than our moon is. Plus, 746 00:36:46,520 --> 00:36:48,839 Speaker 1: of course it's super tiny, so you have almost no 747 00:36:48,920 --> 00:36:51,799 Speaker 1: change of spotting this thing. It was difficult for astronomers 748 00:36:51,840 --> 00:36:53,640 Speaker 1: to even see it in the first place. It was 749 00:36:53,640 --> 00:36:55,879 Speaker 1: only discovered in the last twenty years. Is it safe 750 00:36:55,920 --> 00:36:58,200 Speaker 1: to assume that it's center of masses within the Earth 751 00:36:58,320 --> 00:37:00,280 Speaker 1: or the center of mass for the two bodies falls 752 00:37:00,280 --> 00:37:03,719 Speaker 1: within Earth? Absolutely? Yeah, because the Earth totally dominates this 753 00:37:03,760 --> 00:37:05,600 Speaker 1: thing when it comes to mass. This thing is only 754 00:37:05,640 --> 00:37:07,759 Speaker 1: five kilometers in diameter, and it's just a big chunk 755 00:37:07,760 --> 00:37:10,440 Speaker 1: of rock, and so the Earth dwarfs this thing. Okay, 756 00:37:10,440 --> 00:37:12,800 Speaker 1: even though it's super far away, it still works. Okay, 757 00:37:12,920 --> 00:37:15,800 Speaker 1: that's our like best candidates, is there like a second 758 00:37:15,800 --> 00:37:18,319 Speaker 1: best candidate. There's something else which I think is super fun, 759 00:37:18,480 --> 00:37:22,759 Speaker 1: which astronomers and science communicators called a temporary moon for 760 00:37:22,800 --> 00:37:25,680 Speaker 1: a while. And this is a weird object which at 761 00:37:25,719 --> 00:37:28,680 Speaker 1: the end of last year sort of swooped in from 762 00:37:28,680 --> 00:37:32,319 Speaker 1: deep space and orbiting the Earth a couple of times, 763 00:37:32,400 --> 00:37:34,480 Speaker 1: and people are like, oh, what is this thing? It 764 00:37:34,560 --> 00:37:36,520 Speaker 1: was like only forty ft long, and it has this 765 00:37:36,640 --> 00:37:40,160 Speaker 1: strange cylindrical shape, and they spotted it on his telescope 766 00:37:40,400 --> 00:37:42,160 Speaker 1: and they're like, wait a second, what is this thing? 767 00:37:42,600 --> 00:37:45,440 Speaker 1: And it looks like a piece of a rocket. What 768 00:37:45,960 --> 00:37:49,120 Speaker 1: it's space debris. It's space debris. And so it turns 769 00:37:49,160 --> 00:37:51,239 Speaker 1: out this is a long lost piece of an ill 770 00:37:51,360 --> 00:37:55,200 Speaker 1: faded NASA mission. There was this mission in nineteen sixty 771 00:37:55,239 --> 00:37:58,680 Speaker 1: six called Surveyor two. Is a robotic spacecraft that was 772 00:37:58,719 --> 00:38:00,640 Speaker 1: going to go land on the Moon and it was 773 00:38:00,640 --> 00:38:03,680 Speaker 1: going to go explore the Moon, etcetera. But mid course 774 00:38:03,760 --> 00:38:06,279 Speaker 1: there was a failure in the sort of ballistics and 775 00:38:06,320 --> 00:38:09,560 Speaker 1: the trajection and they lost contact with the craft and 776 00:38:09,640 --> 00:38:12,200 Speaker 1: one of the thrusters failed to ignite, and so basically 777 00:38:12,239 --> 00:38:14,279 Speaker 1: they lost this thing. Part of it crashed on the Moon, 778 00:38:14,560 --> 00:38:16,719 Speaker 1: and part of it just like tumbled out into deep 779 00:38:16,719 --> 00:38:19,880 Speaker 1: space sort of lost, they thought forever. And so this 780 00:38:19,920 --> 00:38:23,040 Speaker 1: thing has been like out there in space for you 781 00:38:23,080 --> 00:38:28,040 Speaker 1: know what, seventy years, almost bouncing around, swooshing around, and 782 00:38:28,160 --> 00:38:32,000 Speaker 1: somehow it ended up coming back to Earth. That's crazy, 783 00:38:32,239 --> 00:38:34,319 Speaker 1: first of all, I think it's more like fifty years though, right, 784 00:38:34,360 --> 00:38:37,879 Speaker 1: But like, it's amazing that we have that much resolution 785 00:38:38,200 --> 00:38:40,920 Speaker 1: that we could find it again. It's really incredible. But 786 00:38:41,000 --> 00:38:43,640 Speaker 1: you know, we are monitoring stuff that comes close to Earth, 787 00:38:43,800 --> 00:38:45,680 Speaker 1: and we're looking for stuff that's sort of like tumbling 788 00:38:45,719 --> 00:38:48,200 Speaker 1: towards the Earth. This is a pretty small object though 789 00:38:48,440 --> 00:38:50,960 Speaker 1: that it's also a weird shape. Right. If you're looking 790 00:38:51,000 --> 00:38:52,879 Speaker 1: out in the space and you see this forty ft 791 00:38:52,920 --> 00:38:56,759 Speaker 1: long cylindrical object, my first guess is gonna be like aliens, right, 792 00:38:57,200 --> 00:38:59,480 Speaker 1: And so how disappointed to look at it and then see, 793 00:38:59,520 --> 00:39:03,239 Speaker 1: like you say, written down the side, it's just our 794 00:39:03,320 --> 00:39:07,160 Speaker 1: old trash. But it's fascinating. People have done a study 795 00:39:07,200 --> 00:39:09,360 Speaker 1: to figure out like what happened to it, and it 796 00:39:09,440 --> 00:39:11,759 Speaker 1: turns out that when it tumbled out into space. It 797 00:39:11,800 --> 00:39:15,400 Speaker 1: was very gently pushed further into space by the pressure 798 00:39:15,480 --> 00:39:18,799 Speaker 1: of sunlight. We talked about this on the podcast, that 799 00:39:18,840 --> 00:39:21,879 Speaker 1: you could build a spaceship that sails on light. It's 800 00:39:21,880 --> 00:39:24,600 Speaker 1: called a solar sail. Just have a huge sheet of 801 00:39:24,640 --> 00:39:27,200 Speaker 1: material and the photons from the sun when they hit 802 00:39:27,280 --> 00:39:29,839 Speaker 1: it are going to transfer their momentum to that, just 803 00:39:29,880 --> 00:39:33,640 Speaker 1: like wind on Earth transfers its momentum to a sail 804 00:39:33,719 --> 00:39:37,040 Speaker 1: on a sailboat. And so that's like by design. But here, 805 00:39:37,040 --> 00:39:39,279 Speaker 1: of course, it's just a rocket tumbling in space, was 806 00:39:39,440 --> 00:39:43,440 Speaker 1: very gently, over decades and decades pushed deeper out into space. 807 00:39:43,560 --> 00:39:46,919 Speaker 1: Are you familiar with Project Westward? No? Tell me, Oh 808 00:39:46,920 --> 00:39:48,880 Speaker 1: my gosh. So the idea here was so this was 809 00:39:48,920 --> 00:39:51,480 Speaker 1: like during the Cold War, and the US was worried 810 00:39:51,480 --> 00:39:53,759 Speaker 1: that they would lose their ability to communicate with other 811 00:39:53,880 --> 00:39:57,640 Speaker 1: nations if our undersea cables got cut by the Soviets, 812 00:39:58,239 --> 00:40:00,399 Speaker 1: and so in that case we would have to rely 813 00:40:00,520 --> 00:40:02,920 Speaker 1: on sending radio waves up and we would have to 814 00:40:02,920 --> 00:40:05,239 Speaker 1: hope that they would bounce off the ionosphere. But that's 815 00:40:05,239 --> 00:40:08,600 Speaker 1: sort of a not super reliable way of sending radio communications, 816 00:40:08,719 --> 00:40:10,799 Speaker 1: and so I think it was m i T came 817 00:40:10,880 --> 00:40:13,080 Speaker 1: up with the solution where they were like, well, we 818 00:40:13,160 --> 00:40:17,160 Speaker 1: could be sure that the ionosphere would have stuff that 819 00:40:17,160 --> 00:40:20,120 Speaker 1: would bounce the radio waves back if we put up 820 00:40:20,560 --> 00:40:26,520 Speaker 1: over four hundred million copper needles. That's a great idea, right, 821 00:40:26,640 --> 00:40:29,120 Speaker 1: And so the argument was that you would put these 822 00:40:29,160 --> 00:40:31,680 Speaker 1: needles up and it would give us some information about 823 00:40:31,680 --> 00:40:33,680 Speaker 1: how well this was gonna work. But in about two 824 00:40:33,719 --> 00:40:37,400 Speaker 1: to three years, the combination of gravity and the sun 825 00:40:37,800 --> 00:40:41,719 Speaker 1: pushing these needles back into the atmosphere would clear everything out, 826 00:40:42,280 --> 00:40:44,920 Speaker 1: clear everything out. Does that mean these copper needles come 827 00:40:45,120 --> 00:40:48,000 Speaker 1: raining back down to the service to impale people. Well, 828 00:40:48,280 --> 00:40:50,960 Speaker 1: they do start raining back down towards Earth, but they're 829 00:40:51,000 --> 00:40:53,160 Speaker 1: like literally only a couple of maybe centimeters long, like 830 00:40:53,200 --> 00:40:55,560 Speaker 1: maybe two centimeters or something. These aren't huge, and that's 831 00:40:55,560 --> 00:40:58,759 Speaker 1: why they needed four million of them. That sounds like 832 00:40:58,800 --> 00:41:02,200 Speaker 1: approximately the size is of a bullet. You're talking about 833 00:41:02,400 --> 00:41:05,120 Speaker 1: space bullets raining down on the Earth. But that would 834 00:41:05,120 --> 00:41:08,480 Speaker 1: definitely burn up before it hits Earth, right, right, Yes, 835 00:41:08,560 --> 00:41:11,520 Speaker 1: of course I think so. Yeah, so our atmosphere is 836 00:41:11,520 --> 00:41:14,480 Speaker 1: like a bulletproof vest. Yes, thank you atmosphere. But so 837 00:41:14,560 --> 00:41:16,280 Speaker 1: the first one that they shot up there, it didn't 838 00:41:16,320 --> 00:41:18,160 Speaker 1: deploy the right way, so a bunch of these needles 839 00:41:18,160 --> 00:41:20,839 Speaker 1: clumped instead of spreading nicely, and so some of these 840 00:41:20,920 --> 00:41:24,640 Speaker 1: clumps fifty years later are still tracked as space debris 841 00:41:25,000 --> 00:41:27,759 Speaker 1: because the clumps didn't de orbit the way that they 842 00:41:27,760 --> 00:41:29,480 Speaker 1: thought they would. And then they did a second shot, 843 00:41:29,520 --> 00:41:32,080 Speaker 1: and the second shot dispersed and they were able to confirm, yes, 844 00:41:32,120 --> 00:41:35,399 Speaker 1: the radio waves bounced back more when we have supplemented 845 00:41:35,400 --> 00:41:37,719 Speaker 1: the ionosphere with all of these needles. But then we 846 00:41:37,760 --> 00:41:39,839 Speaker 1: had to go to the United Nations and promise we 847 00:41:39,840 --> 00:41:42,680 Speaker 1: were going to stop messing up the space environment and 848 00:41:42,719 --> 00:41:45,160 Speaker 1: that we were going to consult people from here on out. 849 00:41:45,480 --> 00:41:47,640 Speaker 1: And one of the articles of the Outer Space Treaty 850 00:41:47,680 --> 00:41:50,960 Speaker 1: actually requires people to do consultations. And that was motivated 851 00:41:51,000 --> 00:41:54,399 Speaker 1: by Project Westward, because what the heck is the US doing? 852 00:41:54,600 --> 00:41:58,240 Speaker 1: So anyway, tangent related to the Sun pushing things back 853 00:41:58,320 --> 00:42:01,440 Speaker 1: into orbits or sorry, back into the atmosphere. Yeah, and 854 00:42:01,440 --> 00:42:04,040 Speaker 1: we have a whole fun podcast episode about space junk 855 00:42:04,360 --> 00:42:07,320 Speaker 1: and how dangerous it is and that's all smashing into itself. 856 00:42:07,360 --> 00:42:09,480 Speaker 1: And if we don't get this stuff under control, all 857 00:42:09,520 --> 00:42:11,920 Speaker 1: of space might be useless to us. We might be 858 00:42:12,239 --> 00:42:14,960 Speaker 1: trapped down here on Earth because we'd be surrounded by 859 00:42:14,960 --> 00:42:17,800 Speaker 1: our own garbage. So check out that episode if you're interested. 860 00:42:17,920 --> 00:42:21,200 Speaker 1: But this is one particularly interesting object, and it came 861 00:42:21,320 --> 00:42:25,400 Speaker 1: in November twenty and made a few large loops around 862 00:42:25,400 --> 00:42:27,000 Speaker 1: the Earth. And so that's why they called this sort 863 00:42:27,040 --> 00:42:29,960 Speaker 1: of like a temporary moon, because even though it was 864 00:42:30,040 --> 00:42:32,920 Speaker 1: lost in deep space, somehow it ended up close enough 865 00:42:32,960 --> 00:42:35,600 Speaker 1: for the Earth to grab it again and loop around. 866 00:42:35,800 --> 00:42:38,360 Speaker 1: But it wasn't a stable orbit, which is really fascinating. 867 00:42:38,440 --> 00:42:40,120 Speaker 1: It was like stable enough to loop around a few 868 00:42:40,160 --> 00:42:42,920 Speaker 1: times and then get tossed back out into space. So 869 00:42:43,000 --> 00:42:46,880 Speaker 1: in March continued his journey and is now back into 870 00:42:46,920 --> 00:42:49,840 Speaker 1: deep space somewhere. WHOA. So, so was this like a 871 00:42:49,920 --> 00:42:53,080 Speaker 1: sycom angle for getting people interested in this, because it 872 00:42:53,080 --> 00:42:56,719 Speaker 1: seems like because it was artificial, it shouldn't count as 873 00:42:56,719 --> 00:42:59,280 Speaker 1: a moon at all, not a temporary moon. It shouldn't 874 00:42:59,280 --> 00:43:01,719 Speaker 1: be a moon. Or do different people use different definitions 875 00:43:01,719 --> 00:43:03,400 Speaker 1: than the one that we settled upon at the beginning 876 00:43:03,440 --> 00:43:05,840 Speaker 1: of the episode, Yeah, exactly. I think this was just 877 00:43:05,880 --> 00:43:09,640 Speaker 1: a clickbait moon, not really by any definition. If you're 878 00:43:09,640 --> 00:43:12,400 Speaker 1: going to require that moons be natural, may not be 879 00:43:13,000 --> 00:43:16,040 Speaker 1: manufactured by humanity. Then this is definitely not a mood. 880 00:43:16,239 --> 00:43:18,360 Speaker 1: But it's cool that we capture something from deep space 881 00:43:18,400 --> 00:43:21,040 Speaker 1: and it orbited us a little while before going back 882 00:43:21,160 --> 00:43:24,479 Speaker 1: out into the dark deep emptiness. Yeah, no, that's super cool. 883 00:43:24,600 --> 00:43:26,640 Speaker 1: All right, So let's take our second break before we 884 00:43:26,680 --> 00:43:29,440 Speaker 1: start to talk a bit more about moons on planets 885 00:43:29,440 --> 00:43:44,000 Speaker 1: other than our own. Okay, so we've talked a bit. 886 00:43:44,040 --> 00:43:47,560 Speaker 1: How about how Earth has one for sure moon and 887 00:43:47,600 --> 00:43:52,359 Speaker 1: a couple maybe moons, quasi moons, quasi moons. Right, tell 888 00:43:52,360 --> 00:43:54,160 Speaker 1: me a bit more about what else is typical in 889 00:43:54,200 --> 00:43:56,560 Speaker 1: the Solar System. How many moons do the other planets have. 890 00:43:56,760 --> 00:43:59,640 Speaker 1: It's really interesting because the Earth, as we were saying, 891 00:43:59,840 --> 00:44:03,720 Speaker 1: is really weird, Like having a really big moon is weird. Also, 892 00:44:04,040 --> 00:44:07,400 Speaker 1: having just one moon is weird. So the eight planets 893 00:44:07,400 --> 00:44:09,399 Speaker 1: in the Solar System, of course, the Earth has one moon. 894 00:44:09,640 --> 00:44:13,200 Speaker 1: Two of the planets have no moons, Mercury and Venus, 895 00:44:13,800 --> 00:44:17,560 Speaker 1: and the other five planets have two hundred and four 896 00:44:17,640 --> 00:44:21,400 Speaker 1: moons in between them. So that's really fascinating and you 897 00:44:21,440 --> 00:44:24,319 Speaker 1: might wonder like, well, why do Mercury and Venus have 898 00:44:24,400 --> 00:44:28,080 Speaker 1: no moons? And the reason is that they're so close 899 00:44:28,120 --> 00:44:31,160 Speaker 1: to the Sun. The Sun is this like really terrible 900 00:44:31,400 --> 00:44:35,960 Speaker 1: overwhelming gravitational force and it tugs on things. We talked 901 00:44:35,960 --> 00:44:39,040 Speaker 1: to the program before about tidal forces. The closer you 902 00:44:39,080 --> 00:44:41,200 Speaker 1: are to the Sun, the more it tugs on you. 903 00:44:41,600 --> 00:44:43,680 Speaker 1: So if you're an object, it's not just like a point. 904 00:44:43,800 --> 00:44:45,799 Speaker 1: If you have like an extent to you, and the 905 00:44:45,840 --> 00:44:48,120 Speaker 1: Sun is going to tug harder on the bit that's 906 00:44:48,120 --> 00:44:51,080 Speaker 1: closer and not as hard on the bid that's further away, 907 00:44:51,280 --> 00:44:53,279 Speaker 1: and that's an effective force on you. So the Sun is, 908 00:44:53,320 --> 00:44:56,440 Speaker 1: for example, squeezing mercury and venus all the time. It's 909 00:44:56,480 --> 00:44:58,799 Speaker 1: pulling on them, and that makes it very hard for 910 00:44:58,840 --> 00:45:02,520 Speaker 1: them to have any in a stable orbit around them. Basically, 911 00:45:02,520 --> 00:45:04,360 Speaker 1: if they have a moon, the Sun is going to 912 00:45:04,440 --> 00:45:07,040 Speaker 1: steal it when it swoops around the planet on the 913 00:45:07,040 --> 00:45:09,400 Speaker 1: close side. So here I'm finding that I want to 914 00:45:09,440 --> 00:45:11,759 Speaker 1: ask you if that means in other Solar systems, the 915 00:45:12,000 --> 00:45:14,040 Speaker 1: close planets don't have moons. But I'm jumping if I 916 00:45:14,080 --> 00:45:16,239 Speaker 1: do that, aren't I We don't know the answer to 917 00:45:16,239 --> 00:45:18,440 Speaker 1: that question yet. We'll talk about that in a minute, 918 00:45:18,600 --> 00:45:21,080 Speaker 1: but yeah, it's a fascinating question. We know that in 919 00:45:21,239 --> 00:45:24,600 Speaker 1: our Solar system, the innermost planets Mercury and Venus have 920 00:45:24,760 --> 00:45:27,279 Speaker 1: no moons, and you know, that might be part of 921 00:45:27,320 --> 00:45:30,359 Speaker 1: the answer of why the Earth only has one moon 922 00:45:30,440 --> 00:45:32,440 Speaker 1: and it's a really big one. It might be that 923 00:45:32,600 --> 00:45:35,839 Speaker 1: anything else the Sun is basically going to steal, and 924 00:45:35,880 --> 00:45:38,200 Speaker 1: that we're only capable of having like either really big 925 00:45:38,200 --> 00:45:41,440 Speaker 1: moons or quasi moons that were sort of sharing with 926 00:45:41,560 --> 00:45:45,360 Speaker 1: the Sun. That might be the partial answer to that question. Interesting, 927 00:45:45,360 --> 00:45:47,560 Speaker 1: So we have the Sun to thank for the space being. Yeah, 928 00:45:47,719 --> 00:45:49,719 Speaker 1: the Sun is toasting our space being for us. But 929 00:45:49,760 --> 00:45:52,000 Speaker 1: then further out in the Solar system, there are lots 930 00:45:52,000 --> 00:45:55,120 Speaker 1: and lots of moons. You know, the other five planets 931 00:45:55,120 --> 00:45:58,320 Speaker 1: with moons have two hundred and four of these things combined, 932 00:45:58,760 --> 00:46:00,960 Speaker 1: you know, in Jupiter and sat And have like dozens 933 00:46:00,960 --> 00:46:04,320 Speaker 1: of them. And you know, Saturn has this crazy ring system, 934 00:46:04,360 --> 00:46:07,600 Speaker 1: and inside those rings are rocks that are big enough 935 00:46:07,640 --> 00:46:11,319 Speaker 1: to be considered moons. Sometimes they're called you know, moonlits, 936 00:46:11,400 --> 00:46:14,760 Speaker 1: sometimes are called minor moons. But there are all sorts 937 00:46:14,760 --> 00:46:16,960 Speaker 1: of things, and so the deeper you go out into 938 00:46:17,000 --> 00:46:19,799 Speaker 1: our Solar system, the more you find these objects that 939 00:46:19,840 --> 00:46:22,239 Speaker 1: have moons and lots and lots of moons. To do 940 00:46:22,360 --> 00:46:25,480 Speaker 1: any of the moons have moons. I wish they did 941 00:46:25,520 --> 00:46:27,200 Speaker 1: have moons. And what would you call that anyway? Would 942 00:46:27,320 --> 00:46:33,480 Speaker 1: that be like a moon moon or squared? That's a 943 00:46:33,480 --> 00:46:36,720 Speaker 1: great question. And so far we haven't found any moons 944 00:46:36,760 --> 00:46:40,400 Speaker 1: that have moons. And the reason is similar to why 945 00:46:40,400 --> 00:46:43,319 Speaker 1: Mercury doesn't have moons. If you're a moon, then you're 946 00:46:43,360 --> 00:46:45,640 Speaker 1: near a big planet, and that means that there are 947 00:46:45,640 --> 00:46:48,720 Speaker 1: tidal forces, and so it's pretty hard to hold onto 948 00:46:48,760 --> 00:46:50,960 Speaker 1: something and not have it gets slurred up and just 949 00:46:51,040 --> 00:46:54,719 Speaker 1: become another moon of the planet you're orbiting. So if 950 00:46:54,760 --> 00:46:57,359 Speaker 1: you're Io and you're orbiting Jupiter, right, Jupiter is an 951 00:46:57,480 --> 00:47:01,440 Speaker 1: enormous gravitational pull. The reason that Io is like hot inside, 952 00:47:01,480 --> 00:47:04,720 Speaker 1: it's because of Jupiter's tidal forces, and so anything orbiting 953 00:47:04,760 --> 00:47:07,040 Speaker 1: Io is just going to get pulled away. It's very 954 00:47:07,160 --> 00:47:10,560 Speaker 1: very hard to have a stable orbit. Although there's this 955 00:47:10,760 --> 00:47:14,239 Speaker 1: really crazy moon of Saturn. This moon is called Rhea, 956 00:47:14,680 --> 00:47:18,040 Speaker 1: and recently they've spotted some stuff in orbit around Rhea, 957 00:47:18,239 --> 00:47:21,760 Speaker 1: maybe sort of like these very small particles. It almost 958 00:47:21,760 --> 00:47:25,960 Speaker 1: looks like this moon of Saturn has its own ring system. 959 00:47:26,239 --> 00:47:29,279 Speaker 1: What I know, isn't that cool? I never thought about 960 00:47:29,280 --> 00:47:32,280 Speaker 1: like a moon with rings around. It is pretty cool. 961 00:47:32,600 --> 00:47:35,320 Speaker 1: That's awesome. So so how if it can't have moons, 962 00:47:35,360 --> 00:47:38,239 Speaker 1: how does it manage to maintain its rings? Well, the 963 00:47:38,280 --> 00:47:41,120 Speaker 1: reason you sometimes have rings instead of moons are because 964 00:47:41,160 --> 00:47:44,040 Speaker 1: of tidal forces. Basically, rings are moons that have been 965 00:47:44,080 --> 00:47:47,160 Speaker 1: torn apart by tidal forces. And so it might be 966 00:47:47,200 --> 00:47:49,160 Speaker 1: that there was an object there and then it got 967 00:47:49,160 --> 00:47:51,759 Speaker 1: sort of shredded by tidal forces, and what we're seeing 968 00:47:51,840 --> 00:47:54,560 Speaker 1: is something transient that these rings might not last for 969 00:47:54,719 --> 00:47:56,600 Speaker 1: very long. You know, by very long we mean on 970 00:47:56,719 --> 00:47:59,040 Speaker 1: astrophysical time scale. So they might be there a million 971 00:47:59,120 --> 00:48:01,360 Speaker 1: years or so. But if you leave the Solar system 972 00:48:01,360 --> 00:48:03,560 Speaker 1: and come back and five million, you might find that 973 00:48:03,600 --> 00:48:06,680 Speaker 1: they're not there anymore. Okay, so let's move out of 974 00:48:06,680 --> 00:48:08,799 Speaker 1: our solar system. What does this look like in other 975 00:48:08,840 --> 00:48:12,040 Speaker 1: solar system? So, for example, do the mercury and venus 976 00:48:12,080 --> 00:48:16,319 Speaker 1: equivalents and other solar systems lack moons like we see 977 00:48:16,360 --> 00:48:18,680 Speaker 1: in our solar system. It's such a good question and 978 00:48:18,719 --> 00:48:21,360 Speaker 1: one we just don't know the answer to yet because 979 00:48:21,640 --> 00:48:24,960 Speaker 1: we have never seen a moon in another solar system, 980 00:48:25,280 --> 00:48:28,040 Speaker 1: Like every moon that any human has ever seen has 981 00:48:28,160 --> 00:48:31,440 Speaker 1: only ever been in our solar system. Isn't that like 982 00:48:31,640 --> 00:48:34,960 Speaker 1: crazy and slightly frustrating. It's both of those things, And 983 00:48:35,000 --> 00:48:37,240 Speaker 1: it reveals to me, like just how often I assume 984 00:48:37,280 --> 00:48:39,440 Speaker 1: that science has figured out so many things that are 985 00:48:39,520 --> 00:48:42,400 Speaker 1: much harder than I apparently understand. So why do we 986 00:48:42,440 --> 00:48:44,360 Speaker 1: know that all these other solar systems have planets but 987 00:48:44,400 --> 00:48:46,560 Speaker 1: we don't know that they have moons? Well, moons are 988 00:48:46,680 --> 00:48:48,840 Speaker 1: much smaller, and they're just harder to see them planets. 989 00:48:49,200 --> 00:48:51,040 Speaker 1: You know, we now sort of take it for granted 990 00:48:51,040 --> 00:48:53,839 Speaker 1: that we can see planets around other stars, But that's 991 00:48:53,880 --> 00:48:57,040 Speaker 1: pretty recent. It was like that we started to be 992 00:48:57,040 --> 00:48:59,840 Speaker 1: able to really do this and spot planets and other soldiers. 993 00:49:00,400 --> 00:49:03,200 Speaker 1: Until then, we had never seen a planet around a 994 00:49:03,280 --> 00:49:07,160 Speaker 1: star that wasn't our star. We didn't know until then, if, 995 00:49:07,200 --> 00:49:10,400 Speaker 1: for example, our star was the only one that had planets, 996 00:49:10,440 --> 00:49:13,759 Speaker 1: we could have been like the weirdest star in the universe. Now, 997 00:49:13,800 --> 00:49:15,880 Speaker 1: of course, we know, because we've looked and we've seen 998 00:49:16,040 --> 00:49:17,919 Speaker 1: that lots and lots and lots of stars have lots 999 00:49:17,920 --> 00:49:19,920 Speaker 1: and lots of planets. We're also learning, of course, that 1000 00:49:19,920 --> 00:49:22,360 Speaker 1: our Solar system is weird in all sorts of interesting ways. 1001 00:49:22,520 --> 00:49:25,319 Speaker 1: But the problem is that the techniques we used to 1002 00:49:25,320 --> 00:49:28,640 Speaker 1: see those planets are better when the planets are large 1003 00:49:28,719 --> 00:49:31,120 Speaker 1: and when they're close to the Sun, and that makes 1004 00:49:31,160 --> 00:49:33,600 Speaker 1: it pretty hard to see moons, which tend to be 1005 00:49:33,719 --> 00:49:36,680 Speaker 1: small and further from the star. We haven't found any 1006 00:49:36,719 --> 00:49:39,800 Speaker 1: instances of a moon that's like huge or one of 1007 00:49:39,840 --> 00:49:41,840 Speaker 1: those instances where it's hard to determine which one is 1008 00:49:41,880 --> 00:49:43,680 Speaker 1: the planet and which one is the moon because they're 1009 00:49:43,680 --> 00:49:46,640 Speaker 1: both pretty big, and so there's no big things that 1010 00:49:46,680 --> 00:49:50,000 Speaker 1: break this rule. We haven't confirmed any moons and other 1011 00:49:50,000 --> 00:49:52,799 Speaker 1: solar systems are you're looking for the duck built platypus 1012 00:49:52,840 --> 00:49:55,719 Speaker 1: of moons out there somewhere No so far zero. There 1013 00:49:55,719 --> 00:49:59,080 Speaker 1: have been some candidates. People have some really clever ideas 1014 00:49:59,120 --> 00:50:02,319 Speaker 1: for how you might see moons around planets in other 1015 00:50:02,400 --> 00:50:05,480 Speaker 1: solar systems. Like one way that we see the planet 1016 00:50:05,800 --> 00:50:07,839 Speaker 1: is that the planet passes in front of the star 1017 00:50:08,320 --> 00:50:10,480 Speaker 1: makes like a little eclipse, it like dims the star 1018 00:50:10,600 --> 00:50:12,839 Speaker 1: a little bit. And if it does that several times, 1019 00:50:12,880 --> 00:50:14,520 Speaker 1: you can see a pattern, so you can get a 1020 00:50:14,560 --> 00:50:16,560 Speaker 1: sense for like, oh, this is really something that's passing 1021 00:50:16,600 --> 00:50:18,439 Speaker 1: in front of the star. It must be a planet. Now, 1022 00:50:18,480 --> 00:50:21,320 Speaker 1: if there's a moon around that planet and it's orbiting 1023 00:50:21,360 --> 00:50:24,120 Speaker 1: that planet. As it passes around the planet, it might 1024 00:50:24,400 --> 00:50:27,200 Speaker 1: add to that eclipse a little bit and then pass 1025 00:50:27,280 --> 00:50:29,680 Speaker 1: behind the planet and dip again. And so if you 1026 00:50:29,680 --> 00:50:33,280 Speaker 1: have really refined measurements, you might see these like wiggles 1027 00:50:33,320 --> 00:50:36,800 Speaker 1: on the wiggles that tell you that there's something going 1028 00:50:36,840 --> 00:50:40,040 Speaker 1: around that planet. And there are some cases where people 1029 00:50:40,080 --> 00:50:41,480 Speaker 1: look at the data and they're like, yeah, I think 1030 00:50:41,560 --> 00:50:44,120 Speaker 1: those are wiggles and wiggles, but other people analyze the 1031 00:50:44,160 --> 00:50:46,560 Speaker 1: same data and they're like, no, there's no evidence for that. 1032 00:50:46,719 --> 00:50:48,799 Speaker 1: So we're really at the edge of being able to 1033 00:50:48,840 --> 00:50:52,840 Speaker 1: detect XO moons. We haven't seen any yet. Well that's exciting, Like, 1034 00:50:52,880 --> 00:50:55,879 Speaker 1: hopefully in our lifetime we figure out how to do that. Well, yeah, 1035 00:50:55,960 --> 00:50:58,160 Speaker 1: hopefully in our lifetime. I mean, we're on the edge 1036 00:50:58,160 --> 00:51:00,280 Speaker 1: of learning so much about these other solars to times, 1037 00:51:00,280 --> 00:51:03,240 Speaker 1: like figuring out what's any atmosphere of those planets, seeing 1038 00:51:03,239 --> 00:51:05,680 Speaker 1: what moons there are. There was also a lot of excitement. 1039 00:51:05,680 --> 00:51:07,560 Speaker 1: I don't know if you remember about this one particular 1040 00:51:07,640 --> 00:51:11,560 Speaker 1: star called Tabby Star, which dimmed really weirdly all of 1041 00:51:11,600 --> 00:51:13,879 Speaker 1: a sudden, and people thought like, wait a second, what's 1042 00:51:13,880 --> 00:51:17,400 Speaker 1: blocking this star? Is this evidence of like an alien megastructure. 1043 00:51:17,640 --> 00:51:20,359 Speaker 1: Is somebody out there building a dison spear around this star, 1044 00:51:20,600 --> 00:51:22,600 Speaker 1: which was really fun and you know inspired, I'm sure 1045 00:51:22,600 --> 00:51:25,279 Speaker 1: a lot of science fiction novels. But it turns out 1046 00:51:25,320 --> 00:51:27,720 Speaker 1: that it was just like a big cloud of dust 1047 00:51:27,800 --> 00:51:30,880 Speaker 1: and debris. But it might be that, like, you know, 1048 00:51:30,960 --> 00:51:33,400 Speaker 1: there was a planet out there and it had a moon, 1049 00:51:33,640 --> 00:51:36,759 Speaker 1: and that moon got like tidally disrupted and torn up 1050 00:51:36,960 --> 00:51:39,360 Speaker 1: and ended up being this big cloud of stuff that 1051 00:51:39,440 --> 00:51:42,120 Speaker 1: partially blocked the star. So that might have been like, 1052 00:51:42,440 --> 00:51:45,840 Speaker 1: you know, evidence of the destruction of an excellent moon. WHOA, 1053 00:51:46,160 --> 00:51:48,919 Speaker 1: that's pretty cool. That's pretty cool. Yeah, But I'm looking 1054 00:51:48,960 --> 00:51:51,359 Speaker 1: forward to scientists figuring that out and so we can 1055 00:51:51,400 --> 00:51:54,440 Speaker 1: get a sense for like how unusual is it to 1056 00:51:54,560 --> 00:51:57,839 Speaker 1: have just like one big moon, How unusual is it 1057 00:51:57,880 --> 00:52:00,719 Speaker 1: to have inner planets with no moons? How weird is 1058 00:52:00,719 --> 00:52:03,360 Speaker 1: it to have huge gas giants with like a dozen moons. 1059 00:52:03,760 --> 00:52:06,160 Speaker 1: We ask these basic questions because we just don't know 1060 00:52:06,200 --> 00:52:08,040 Speaker 1: the answers, and really the only way to figure it 1061 00:52:08,040 --> 00:52:10,440 Speaker 1: out is to go out there and explore the universe 1062 00:52:10,520 --> 00:52:12,920 Speaker 1: and to like actually look with our eyeballs and our 1063 00:52:12,960 --> 00:52:15,759 Speaker 1: telescopes and get the answers. It's a cool time to 1064 00:52:15,800 --> 00:52:18,640 Speaker 1: be alive. It is a cool time to be alive. So, Kelly, 1065 00:52:18,640 --> 00:52:20,080 Speaker 1: what are you going to go back and tell your 1066 00:52:20,120 --> 00:52:23,279 Speaker 1: seven year old about how many moons the Earth has? Well, 1067 00:52:23,480 --> 00:52:25,640 Speaker 1: I think she's going to be super excited. She We've 1068 00:52:25,640 --> 00:52:28,080 Speaker 1: been talking to her about Apollo and the space race, 1069 00:52:28,080 --> 00:52:29,920 Speaker 1: and I think she'll be super excited to hear that 1070 00:52:30,000 --> 00:52:32,359 Speaker 1: one of those you know, boosters came back around again 1071 00:52:32,400 --> 00:52:34,600 Speaker 1: and is still floating in deep space. So I'll tell 1072 00:52:34,600 --> 00:52:37,160 Speaker 1: her about that, and I definitely think she's going to 1073 00:52:37,280 --> 00:52:40,759 Speaker 1: love that there's something called a space being or something 1074 00:52:40,800 --> 00:52:42,480 Speaker 1: we referred to as a space being because we can't 1075 00:52:42,480 --> 00:52:44,719 Speaker 1: pronounce its real name. I think she's going to get 1076 00:52:44,760 --> 00:52:46,880 Speaker 1: a total kick out of that information. What about you, 1077 00:52:46,920 --> 00:52:48,920 Speaker 1: what are you gonna tell your kids? Yeah, my kids 1078 00:52:48,960 --> 00:52:51,600 Speaker 1: also will tell them that there's weird stuff floating out there, 1079 00:52:52,000 --> 00:52:54,280 Speaker 1: and that in the end, it's all just sort of arbitrary. 1080 00:52:54,400 --> 00:52:56,320 Speaker 1: What we call a moon and what we call a 1081 00:52:56,400 --> 00:53:00,279 Speaker 1: quasi satellite is really just an arbitrary distinction, but that 1082 00:53:00,480 --> 00:53:03,480 Speaker 1: their questions are valuable questions, and that these really simple, 1083 00:53:03,560 --> 00:53:06,560 Speaker 1: basic questions about the universe are sometimes the most interesting, 1084 00:53:06,840 --> 00:53:10,400 Speaker 1: the hardest to answer and reveal something about you know, 1085 00:53:10,440 --> 00:53:12,879 Speaker 1: what we've thought about our place in the universe, what 1086 00:53:12,920 --> 00:53:15,080 Speaker 1: we think is natural, what we think is normal, what 1087 00:53:15,120 --> 00:53:18,600 Speaker 1: we think is typical, and it probably is really unusual. 1088 00:53:18,680 --> 00:53:22,040 Speaker 1: And that's somewhere out there there's an alien kid looking 1089 00:53:22,120 --> 00:53:24,560 Speaker 1: up at the sky and asking the alien mom, like, 1090 00:53:24,800 --> 00:53:27,080 Speaker 1: why do we have five moons? You know, it's just 1091 00:53:27,160 --> 00:53:29,760 Speaker 1: every planet to have five moons. I love that idea 1092 00:53:29,840 --> 00:53:32,640 Speaker 1: that we're all asking the same questions, but just very 1093 00:53:32,719 --> 00:53:35,560 Speaker 1: much separated. All right, So thank you very much everybody 1094 00:53:35,600 --> 00:53:38,680 Speaker 1: for going on this curiosity journey with us and listening 1095 00:53:38,680 --> 00:53:41,600 Speaker 1: to us talk about the number of moons around the Earth. 1096 00:53:41,840 --> 00:53:43,719 Speaker 1: If you have stuff you'd like to hear us talk about, 1097 00:53:43,760 --> 00:53:46,840 Speaker 1: please send them to us two questions at Daniel and 1098 00:53:47,000 --> 00:53:49,680 Speaker 1: Jorge dot com. Thanks again, Kelly for joining us today 1099 00:53:49,680 --> 00:53:51,680 Speaker 1: and thanks to all of you for tuning in. Thanks 1100 00:53:51,680 --> 00:54:00,960 Speaker 1: for having me. It was a lot of fun. Thanks 1101 00:54:00,960 --> 00:54:03,560 Speaker 1: for listening, and remember that Daniel and Jorge explained. The 1102 00:54:03,680 --> 00:54:06,759 Speaker 1: Universe is a production of I Heart Radio or more 1103 00:54:06,840 --> 00:54:10,200 Speaker 1: podcast from my Heart Radio visit the I Heart Radio app, 1104 00:54:10,480 --> 00:54:13,960 Speaker 1: Apple Podcasts, or wherever you listen to your favorite shows.