1 00:00:00,240 --> 00:00:04,760 Speaker 1: Brought to you by Toyota. Let's go places. Welcome to 2 00:00:05,160 --> 00:00:14,280 Speaker 1: stuff you should know from house stuff Works dot com. Hey, 3 00:00:14,440 --> 00:00:18,119 Speaker 1: welcome to the podcast. I'm Josh Clark. There's Chipper and 4 00:00:18,200 --> 00:00:22,119 Speaker 1: Cheery Chuck. Chucker's Bryant right across from me. How are 5 00:00:22,120 --> 00:00:25,240 Speaker 1: you doing? I'm good man. I'm about to go get 6 00:00:25,280 --> 00:00:29,680 Speaker 1: that jar of moonshine for my cubicle. And we've never 7 00:00:29,720 --> 00:00:31,680 Speaker 1: done a show where we just drank moonshine the whole time. 8 00:00:32,360 --> 00:00:36,360 Speaker 1: I think we should. What better day? I don't think 9 00:00:36,360 --> 00:00:39,120 Speaker 1: it's at my desk at home? Oh? Really, do you 10 00:00:39,159 --> 00:00:41,120 Speaker 1: have beers still? Or there may be some other there? 11 00:00:41,120 --> 00:00:43,159 Speaker 1: I don't know what about. Well, there's a case of 12 00:00:43,159 --> 00:00:47,120 Speaker 1: beer that some other dude sent me, like not it 13 00:00:47,200 --> 00:00:49,440 Speaker 1: wasn't show related, but it's been sitting there for like 14 00:00:49,479 --> 00:00:53,239 Speaker 1: a year. What shiner back? Oh? I got some too, 15 00:00:53,600 --> 00:00:56,960 Speaker 1: And then there's a couple of beers from like England, 16 00:00:57,600 --> 00:00:59,920 Speaker 1: and then there may be some moonshine. So let's just 17 00:01:00,000 --> 00:01:04,000 Speaker 1: get drunk. Okay, So you're feeling good, I'm just getting folks, 18 00:01:04,040 --> 00:01:11,479 Speaker 1: we're gonna do that, is what you're saying. Um, Well, 19 00:01:11,520 --> 00:01:15,560 Speaker 1: my intro is, uh, you've already pood pooed it. Yeah, 20 00:01:15,560 --> 00:01:17,160 Speaker 1: I feel kind of bad about that. Oh, I don't 21 00:01:17,200 --> 00:01:19,800 Speaker 1: feel bad. It's pretty much part for the course, buddy, 22 00:01:20,120 --> 00:01:26,640 Speaker 1: Are you ready, Chuck? Uh? Many many years ago, roughly 23 00:01:26,680 --> 00:01:31,520 Speaker 1: around four eight billion years ago, um, the Earth really 24 00:01:31,520 --> 00:01:34,640 Speaker 1: started to forming together from a bunch of dust and 25 00:01:35,040 --> 00:01:40,400 Speaker 1: rocks and other dust, so says you, because right, because 26 00:01:40,400 --> 00:01:44,000 Speaker 1: the universe was spinning, right, and all these particles were spinning, 27 00:01:44,000 --> 00:01:47,360 Speaker 1: and as they came together, forming an accretion from an 28 00:01:47,360 --> 00:01:51,840 Speaker 1: incretion disk, they formed the Earth and all other planets obviously, right, 29 00:01:52,320 --> 00:01:56,840 Speaker 1: and all of that spin. Thanks to the laws of thermodynamics, 30 00:01:57,320 --> 00:02:02,160 Speaker 1: one of them, uh, continued to spin and actually accumulated, 31 00:02:02,560 --> 00:02:06,279 Speaker 1: and so the Earth just's spinning. That's why it's spinning, 32 00:02:06,320 --> 00:02:08,600 Speaker 1: because it's always been spinning and all of its particles 33 00:02:08,600 --> 00:02:10,800 Speaker 1: that make it up have been spinning. So it's spinning 34 00:02:10,800 --> 00:02:13,720 Speaker 1: because of the conservation of angular momentum. Right. Yeah. In 35 00:02:13,840 --> 00:02:16,240 Speaker 1: Newton's first law of motion, of course, that's what it was. 36 00:02:16,280 --> 00:02:20,080 Speaker 1: Not thermodynamics. There is a law of motion, which is 37 00:02:20,120 --> 00:02:23,840 Speaker 1: what if an object uh, an object in motion will 38 00:02:23,880 --> 00:02:27,119 Speaker 1: remain in that state of motion unless basically someone comes 39 00:02:27,120 --> 00:02:29,359 Speaker 1: along and puts the brakes on it. Right, unless something 40 00:02:29,720 --> 00:02:32,480 Speaker 1: acts upon it, exactly, and in the vacuum of space, 41 00:02:32,880 --> 00:02:35,160 Speaker 1: there's nothing to act upon it to slow the Earth down. 42 00:02:35,160 --> 00:02:37,000 Speaker 1: So it's just gonna keep going. And actually the Earth 43 00:02:37,040 --> 00:02:40,600 Speaker 1: has slowed in its older age. Four million years ago, 44 00:02:40,840 --> 00:02:44,760 Speaker 1: a day uh lasted twenty two hours. Yeah, it's been 45 00:02:44,800 --> 00:02:48,000 Speaker 1: slowing consistently over time, right, Yeah, but it's gonna take 46 00:02:48,040 --> 00:02:51,799 Speaker 1: a while to stop. I think in four hundred million 47 00:02:51,880 --> 00:02:54,960 Speaker 1: years in the future, they think that the day will 48 00:02:55,000 --> 00:02:58,320 Speaker 1: be twenty six hours, so to two years. Slowing by 49 00:02:58,360 --> 00:03:02,320 Speaker 1: two or two hours a day over four million years, 50 00:03:02,320 --> 00:03:05,320 Speaker 1: it's not it's not quick. Well, in four million years, 51 00:03:05,880 --> 00:03:07,760 Speaker 1: is there going to be any Earth? I don't know. 52 00:03:08,320 --> 00:03:10,799 Speaker 1: That's such a good question. What will we look like. 53 00:03:11,000 --> 00:03:13,440 Speaker 1: I don't think it's me It's four million years, that's 54 00:03:13,480 --> 00:03:17,120 Speaker 1: my guess. Um. Okay, so the Earth is slowing. We 55 00:03:17,200 --> 00:03:20,040 Speaker 1: understand why it's spinning. We understand that it is slowing down. 56 00:03:21,000 --> 00:03:23,519 Speaker 1: But what happens if somebody just comes along just stops 57 00:03:23,520 --> 00:03:28,799 Speaker 1: it automatically, like just stopped poop stopped. Well, and by 58 00:03:28,840 --> 00:03:32,040 Speaker 1: the way, Jerry, that wasn't an edit. Yeah, that's our 59 00:03:32,120 --> 00:03:34,840 Speaker 1: signal when we beep, that is a call out to Jerry. 60 00:03:36,240 --> 00:03:39,600 Speaker 1: So we're moving very fast, like faster than the speed 61 00:03:39,640 --> 00:03:42,440 Speaker 1: of sound, even though it didn't feel like it. Um 62 00:03:42,560 --> 00:03:45,520 Speaker 1: So if someone stopped it, those same things that would 63 00:03:45,520 --> 00:03:47,840 Speaker 1: happen if you just stopped your car all of a sudden, 64 00:03:48,320 --> 00:03:50,800 Speaker 1: or a train stopped all of a sudden, would happen 65 00:03:51,160 --> 00:03:53,480 Speaker 1: here on Earth, except it would be much more drastic 66 00:03:53,520 --> 00:03:56,119 Speaker 1: because we're spinning much faster. We're spinning in an easterly 67 00:03:56,160 --> 00:03:58,760 Speaker 1: direction at about a thousand miles an hour along the equator. 68 00:03:59,600 --> 00:04:01,560 Speaker 1: So yeah, if all of a sudden you stop the Earth, 69 00:04:01,600 --> 00:04:04,760 Speaker 1: everything that's unattached to the Earth would keep going eastward 70 00:04:04,960 --> 00:04:08,400 Speaker 1: about a thousand miles an hour, mass, instantly dead, massive flooding, 71 00:04:09,160 --> 00:04:13,600 Speaker 1: you name it, the wind, shock waves, buildings, everything just go. 72 00:04:14,440 --> 00:04:16,520 Speaker 1: And you said something that I find kind of interesting, 73 00:04:16,560 --> 00:04:18,679 Speaker 1: like when I when I when I started to research 74 00:04:18,720 --> 00:04:20,719 Speaker 1: like the Earth's rotation, It's one of those things where 75 00:04:20,720 --> 00:04:23,240 Speaker 1: I just assume I know what I'm talking about, and 76 00:04:23,279 --> 00:04:24,960 Speaker 1: then the more I looked into I was like, oh, yeah, 77 00:04:25,000 --> 00:04:28,040 Speaker 1: there's a lot of little stuff here, like questions like 78 00:04:28,120 --> 00:04:31,120 Speaker 1: why don't we feel the fact that we're moving through 79 00:04:31,200 --> 00:04:34,159 Speaker 1: space at about a thousand miles an hour and well, 80 00:04:34,279 --> 00:04:37,039 Speaker 1: I found the answer because the Earth moves at a 81 00:04:37,080 --> 00:04:41,560 Speaker 1: constant speed, the constant rate of rotation. There's no acceleration 82 00:04:41,640 --> 00:04:45,039 Speaker 1: or deceleration, which we would feel if that happened. Right, 83 00:04:45,200 --> 00:04:47,880 Speaker 1: Why don't we spin off the Earth? Do you know why? 84 00:04:48,080 --> 00:04:52,000 Speaker 1: I do? Okay? Here? Because of gravity and the gravitational 85 00:04:52,040 --> 00:04:54,560 Speaker 1: poll like, we we want to spin off the Earth. 86 00:04:55,400 --> 00:04:58,880 Speaker 1: That's you know, that's in there. But the force of gravity, 87 00:04:58,960 --> 00:05:00,760 Speaker 1: or the force that wants to spin us off the 88 00:05:00,800 --> 00:05:04,560 Speaker 1: Earth is point three the force of gravity, right, centrifugal 89 00:05:04,680 --> 00:05:07,479 Speaker 1: force weigh much more gravity going on than there is 90 00:05:07,640 --> 00:05:10,200 Speaker 1: uh the other So and I found that if the 91 00:05:10,200 --> 00:05:15,680 Speaker 1: Earth rotated at a rate of eighty minutes, right, it's 92 00:05:15,680 --> 00:05:18,360 Speaker 1: spun around on its axis one full time, So one 93 00:05:18,440 --> 00:05:21,920 Speaker 1: day was eighty minutes long. That would be fast enough 94 00:05:21,960 --> 00:05:23,920 Speaker 1: to overcome the force of gravity, would be thrown off 95 00:05:23,920 --> 00:05:27,039 Speaker 1: into space. But we're not going anywhere because that the 96 00:05:27,080 --> 00:05:29,960 Speaker 1: Earth is never gonna start speeding up like that. That's 97 00:05:30,000 --> 00:05:33,880 Speaker 1: just crazy talk. No, And it's not gonna stop spinning 98 00:05:34,000 --> 00:05:37,560 Speaker 1: either anytime soon. But we can still have fun with 99 00:05:37,560 --> 00:05:42,000 Speaker 1: this topic. So, say that we were existing right now 100 00:05:42,200 --> 00:05:44,120 Speaker 1: as the Earth was really starting to slow down, was 101 00:05:44,200 --> 00:05:47,680 Speaker 1: making its last turn. So it did it gradually like 102 00:05:47,760 --> 00:05:52,880 Speaker 1: Superman style, right, and then, um, the ecosystems were intact. 103 00:05:53,680 --> 00:05:57,039 Speaker 1: Everything was generally intact the moment the Earth stopped spinning 104 00:05:57,680 --> 00:06:00,440 Speaker 1: the day the Earth stood still exactly. Yeah, there would 105 00:06:00,480 --> 00:06:03,120 Speaker 1: be some really interesting things that happened, like a lot 106 00:06:03,160 --> 00:06:06,760 Speaker 1: of are the geography of this planet. I took for 107 00:06:06,800 --> 00:06:09,440 Speaker 1: granted until I read this article, which really opened my eyes. 108 00:06:10,279 --> 00:06:11,920 Speaker 1: So what what what? What are some of the things 109 00:06:11,960 --> 00:06:15,040 Speaker 1: that would happen if they're just stop spinning. Uh? Well, 110 00:06:15,400 --> 00:06:20,120 Speaker 1: seismologists think that it would set off a massive chain 111 00:06:20,200 --> 00:06:25,880 Speaker 1: of super earthquakes because they suspect that UM, the rotation 112 00:06:25,880 --> 00:06:28,240 Speaker 1: the Earth, plays a big role in the movement of 113 00:06:28,240 --> 00:06:32,560 Speaker 1: the tectonic plates. So they seismologists think that you know, 114 00:06:32,839 --> 00:06:37,440 Speaker 1: we would all be dead because of massive, massive earthquakes. Okay, 115 00:06:37,839 --> 00:06:40,360 Speaker 1: we'd probably be dead for a lot more reasons which 116 00:06:40,440 --> 00:06:44,640 Speaker 1: we can explore, but yes, diverse. Yeah, because think about it, 117 00:06:44,680 --> 00:06:48,039 Speaker 1: that that spinning Earth, the centrivigal force of the Earth 118 00:06:48,680 --> 00:06:54,080 Speaker 1: um is so strong that um it it basically keeps 119 00:06:54,080 --> 00:06:57,479 Speaker 1: the oceans in place. It creates a bulge around the equator, 120 00:06:57,560 --> 00:07:01,000 Speaker 1: Like the Earth is not a perfect sphere. Um it's 121 00:07:01,040 --> 00:07:05,080 Speaker 1: bulged at the middle, and it's that's because of its spin, 122 00:07:05,560 --> 00:07:09,400 Speaker 1: and that bulge actually brings the world's oceans towards the equator. 123 00:07:09,880 --> 00:07:12,440 Speaker 1: In the southern hemisphere they moved north. In the northern hemisphere, 124 00:07:12,480 --> 00:07:14,880 Speaker 1: they moved south. But it's being pulled towards the middle 125 00:07:14,960 --> 00:07:17,880 Speaker 1: of the Earth. There's spare tire. So if it stops 126 00:07:17,920 --> 00:07:21,360 Speaker 1: spinning all of a sudden, the world's oceans would go 127 00:07:21,480 --> 00:07:24,280 Speaker 1: towards the poles. Yeah, like quickly. It would be pretty 128 00:07:24,320 --> 00:07:27,720 Speaker 1: cool to see, I guess not if you're at the poles. 129 00:07:27,800 --> 00:07:30,200 Speaker 1: Did you see a map of what it would look like. Yeah, 130 00:07:30,280 --> 00:07:35,160 Speaker 1: like basically a supercontinent in the center on both sides 131 00:07:35,200 --> 00:07:38,000 Speaker 1: of the equator. Yeah, like all the way around the globe, 132 00:07:38,040 --> 00:07:40,360 Speaker 1: and two big oceans, one on top and one on 133 00:07:40,400 --> 00:07:42,360 Speaker 1: the bottom. Yeah, and the one on the top of 134 00:07:42,440 --> 00:07:45,640 Speaker 1: the Arctic would actually be about a thousand meters deeper, 135 00:07:46,080 --> 00:07:48,600 Speaker 1: not because there'd be more water there, but because the 136 00:07:48,600 --> 00:07:52,760 Speaker 1: Antarctic basin is bigger deeper. That makes sense, so the 137 00:07:52,800 --> 00:07:56,600 Speaker 1: water would be shallower by comparison. But yeah, I was 138 00:07:56,600 --> 00:08:00,760 Speaker 1: looking so like Chicago would be just under the north 139 00:08:01,000 --> 00:08:06,880 Speaker 1: shore of the Northern Hemisphere's ocean. Um and from that 140 00:08:06,920 --> 00:08:10,200 Speaker 1: point down the United States would be largely intact. All 141 00:08:10,240 --> 00:08:14,080 Speaker 1: the way into the Caribbean South it would just be land. 142 00:08:14,480 --> 00:08:19,120 Speaker 1: It's pretty neat, good looking map. I love freaky weird maps. Yeah, 143 00:08:19,440 --> 00:08:22,560 Speaker 1: like the early maps. Those were a little weird. There's 144 00:08:22,600 --> 00:08:28,200 Speaker 1: a blog called um unusual Maps, I think maps. I 145 00:08:28,200 --> 00:08:30,160 Speaker 1: can't remember what's called, but it's just like this blog 146 00:08:30,200 --> 00:08:33,480 Speaker 1: about strange maps. It's pretty neat. I used to collect maps, 147 00:08:33,800 --> 00:08:35,959 Speaker 1: Oh yeah, yeah, I mean I didn't have a ton. 148 00:08:36,000 --> 00:08:39,720 Speaker 1: I had like fifteen or sixteen like cool map posters. 149 00:08:40,320 --> 00:08:41,640 Speaker 1: Nice to still have a few of them, but I 150 00:08:41,720 --> 00:08:43,160 Speaker 1: think they went the way of the Dodo in my 151 00:08:43,200 --> 00:08:46,600 Speaker 1: house where they like scholastic foldouts. No, like you know, 152 00:08:46,920 --> 00:08:51,280 Speaker 1: some were like you know, civil War map or the 153 00:08:51,320 --> 00:08:54,720 Speaker 1: Earth at this point map, or you know, just very 154 00:08:54,840 --> 00:08:56,480 Speaker 1: none of them. We're just straight up. I think I 155 00:08:56,480 --> 00:08:59,600 Speaker 1: had one straight up map. Um, so what else would 156 00:08:59,600 --> 00:09:03,640 Speaker 1: happen once that? What happened is the uh? And Robert 157 00:09:03,720 --> 00:09:07,720 Speaker 1: Lamb wrote this, didn't he No, Jonathan at a berry? 158 00:09:07,840 --> 00:09:11,240 Speaker 1: That's right, at a berry at a berry. Good job. 159 00:09:11,760 --> 00:09:13,800 Speaker 1: He says that it will take a whole year to 160 00:09:13,880 --> 00:09:16,719 Speaker 1: pull off what the Earth does in a day, so 161 00:09:18,520 --> 00:09:22,360 Speaker 1: one part of the world would be a blazing, scorching desert, 162 00:09:22,679 --> 00:09:24,480 Speaker 1: and then one part of the Earth would be a barren, 163 00:09:24,840 --> 00:09:28,240 Speaker 1: frozen wasteland half a year, half half the year. And 164 00:09:28,400 --> 00:09:32,439 Speaker 1: that's because the since the Earth rotates on its access 165 00:09:32,440 --> 00:09:37,120 Speaker 1: in about twenty four hours a little under, I think, um, 166 00:09:37,160 --> 00:09:39,640 Speaker 1: if it stopped doing that, it would still move around 167 00:09:39,679 --> 00:09:41,560 Speaker 1: the Sun, it just wouldn't spin on its axis. So 168 00:09:42,000 --> 00:09:44,360 Speaker 1: I figured this out. If you're having trouble visualizing it, 169 00:09:44,400 --> 00:09:47,559 Speaker 1: like I did, put your thumb in front of your 170 00:09:47,600 --> 00:09:49,760 Speaker 1: face out a little bit so that your thumbnail is 171 00:09:49,760 --> 00:09:52,200 Speaker 1: facing you, and then pretend that the Sun is in 172 00:09:52,240 --> 00:09:55,040 Speaker 1: between you and your thumb, and your thumb is the Earth, 173 00:09:55,679 --> 00:09:58,240 Speaker 1: and you just rotated around so that your thumbnails facing 174 00:09:58,280 --> 00:10:00,679 Speaker 1: you all the time. But it's going around the Sun, 175 00:10:00,920 --> 00:10:04,280 Speaker 1: and you'll see that at any given point, right, it's 176 00:10:05,240 --> 00:10:07,880 Speaker 1: the this part of the Earth is facing a different 177 00:10:07,920 --> 00:10:10,280 Speaker 1: part of the sun the thumbnail. So there would be seasons, 178 00:10:10,280 --> 00:10:14,199 Speaker 1: but there'd be four seasons, and they would be very different. 179 00:10:14,640 --> 00:10:17,719 Speaker 1: The line demarcating them would be really different. And when 180 00:10:17,760 --> 00:10:21,720 Speaker 1: you went from winter to summer, eventually you would have 181 00:10:22,200 --> 00:10:25,480 Speaker 1: nothing but sunlight and then nothing but dark, depending on 182 00:10:25,920 --> 00:10:31,200 Speaker 1: the temperature swing would be huge. So what that means is, um, 183 00:10:31,440 --> 00:10:35,360 Speaker 1: we'd probably have a really difficult time propagating with with 184 00:10:35,440 --> 00:10:38,480 Speaker 1: husbandry in general. And you don't mean sex, you're talking 185 00:10:38,480 --> 00:10:41,079 Speaker 1: with plants and animals. I'm not sure what you mean. 186 00:10:41,080 --> 00:10:45,640 Speaker 1: They're propagating with husbandry sounded like a euphemism. No, just 187 00:10:45,800 --> 00:10:48,480 Speaker 1: farming and animals. All that would be more difficult, if 188 00:10:48,559 --> 00:10:53,040 Speaker 1: not impossible, Um to grow crops, you know, for or 189 00:10:53,240 --> 00:10:55,240 Speaker 1: you know, maybe you grow them during the sunny parts 190 00:10:55,280 --> 00:10:57,480 Speaker 1: of the year. What you can grow and then store. 191 00:10:58,040 --> 00:11:00,439 Speaker 1: But we'd be in bad shape. I think we've very 192 00:11:00,440 --> 00:11:03,440 Speaker 1: bad as far as that goes. But botanically speaking, we 193 00:11:03,520 --> 00:11:06,720 Speaker 1: are a pretty uh, pretty quick witted species, so we 194 00:11:06,760 --> 00:11:10,400 Speaker 1: could possibly overcome it technologically maybe you know, I'll bet 195 00:11:10,400 --> 00:11:13,440 Speaker 1: we'd have a really good sunglasses. Yeah, yeah, that's true 196 00:11:13,520 --> 00:11:18,760 Speaker 1: and coats. Um what else would happen anything? Uh, Well, 197 00:11:18,840 --> 00:11:21,840 Speaker 1: the magnetic field, well gravity, I got something on gravity here. 198 00:11:21,880 --> 00:11:23,920 Speaker 1: Gravity would be changed, which is not in the article, 199 00:11:24,679 --> 00:11:28,680 Speaker 1: but um, it would change significantly if it stopped spinning 200 00:11:28,720 --> 00:11:32,160 Speaker 1: because uh, centrogal force of course, what you're talking about 201 00:11:32,600 --> 00:11:35,880 Speaker 1: contributes to that gravitational field, and it wouldn't exist any longer, 202 00:11:36,200 --> 00:11:39,959 Speaker 1: so the gravitational fiel would be strongest at the poles 203 00:11:40,000 --> 00:11:42,160 Speaker 1: instead of at the equator, and who knows what that 204 00:11:42,160 --> 00:11:46,840 Speaker 1: would do. You'd just be a lot heavier at the poles, 205 00:11:46,920 --> 00:11:49,959 Speaker 1: right you think, maybe, Okay, we'd also lose a very 206 00:11:49,960 --> 00:11:54,760 Speaker 1: interesting thing called the Coriolis effect. Yeah, my favorite, which 207 00:11:54,800 --> 00:11:57,760 Speaker 1: you know, um, supposedly with the Coriolis effect, if you're 208 00:11:57,800 --> 00:12:00,880 Speaker 1: in the Northern Hemisphere, if you flush the toilet, the 209 00:12:00,920 --> 00:12:03,360 Speaker 1: water goes down the drain clockwise and in the Northern 210 00:12:03,440 --> 00:12:06,280 Speaker 1: Hemisphere county clockwise. That it's not true. It's all plumbing, 211 00:12:06,280 --> 00:12:09,040 Speaker 1: it's all the design of the drain, the Coriolis effected. 212 00:12:09,320 --> 00:12:10,920 Speaker 1: There has nothing to do with what part of the 213 00:12:10,920 --> 00:12:12,560 Speaker 1: Earth you're in. It's no, it has nothing to do 214 00:12:12,600 --> 00:12:16,960 Speaker 1: with like the drain, the supposedly the Coreolis effect, the 215 00:12:17,040 --> 00:12:20,520 Speaker 1: fact that the Earth is spinning faster at the equator 216 00:12:20,559 --> 00:12:23,960 Speaker 1: than it is at the poles. Uh. It has long 217 00:12:24,000 --> 00:12:27,200 Speaker 1: been tapped as a reason for whirlpooles. They're saying, No, 218 00:12:27,320 --> 00:12:30,040 Speaker 1: that's probably if it's if you're talking about a drain, 219 00:12:30,080 --> 00:12:31,760 Speaker 1: it's the angle of the drain, it's the design of 220 00:12:31,800 --> 00:12:33,760 Speaker 1: the drain, it's the water rushing in when you flush 221 00:12:33,840 --> 00:12:36,600 Speaker 1: the toilet has nothing. That's an old wives tale. But 222 00:12:36,679 --> 00:12:41,480 Speaker 1: there's a coreal Coreoles effect. It's just not quite as interesting. Basically, 223 00:12:41,480 --> 00:12:44,440 Speaker 1: it says that if you leave the north pole and 224 00:12:44,480 --> 00:12:47,520 Speaker 1: fly toward the equator towards a certain market the equator, 225 00:12:47,720 --> 00:12:49,719 Speaker 1: if you're going a straight line, you're gonna miss your 226 00:12:49,720 --> 00:12:53,160 Speaker 1: mark because there are spinning and it's spinning faster at 227 00:12:53,160 --> 00:12:55,800 Speaker 1: the equator than it is at the pole Coreoli. It's 228 00:12:55,800 --> 00:13:01,320 Speaker 1: a curve like a Yeah, you have to basically correct longitudinally, 229 00:13:01,800 --> 00:13:05,520 Speaker 1: okay um to hit your target. Like you just can't 230 00:13:05,559 --> 00:13:07,040 Speaker 1: find a straight line from the north pole of the 231 00:13:07,080 --> 00:13:08,880 Speaker 1: equator if you're trying to get to a certain spot. 232 00:13:09,880 --> 00:13:14,320 Speaker 1: That's the Coriolis effect. Nice, I guess unless I'm missing something. 233 00:13:14,400 --> 00:13:16,760 Speaker 1: It seems kind of basic. Uh yeah, that's kind of 234 00:13:16,760 --> 00:13:19,319 Speaker 1: basic once you wrap your head around it. Uh. There 235 00:13:19,360 --> 00:13:21,400 Speaker 1: are some things that are slowing the earth down. Like 236 00:13:21,440 --> 00:13:25,040 Speaker 1: you said, the days are longer now than they used 237 00:13:25,080 --> 00:13:29,160 Speaker 1: to be. Uh, yes, they used to be what twenty 238 00:13:29,160 --> 00:13:32,840 Speaker 1: two hours you said fion years ago? Yeah, okay, um, 239 00:13:32,960 --> 00:13:35,640 Speaker 1: so we are slowing down. There is uh tidal friction 240 00:13:36,360 --> 00:13:41,000 Speaker 1: and the tide drags two point three milliseconds on each 241 00:13:41,800 --> 00:13:45,800 Speaker 1: century every hundred years. So that's pretty slow, right, But 242 00:13:45,840 --> 00:13:48,440 Speaker 1: it adds up over time, surely, of course it does. 243 00:13:48,679 --> 00:13:51,720 Speaker 1: Um weather can affect it. Two wins can actually slow 244 00:13:51,760 --> 00:13:56,319 Speaker 1: it down. Earthquakes can redistribute the mass and actually speed up. 245 00:13:56,880 --> 00:13:59,560 Speaker 1: Didn't it speed up in the earthquake in Japan? Yeah? 246 00:13:59,640 --> 00:14:03,160 Speaker 1: I think by um one point eight microseconds that the 247 00:14:03,200 --> 00:14:07,400 Speaker 1: Earth's day, it's solar day, was accelerated because that earthquake 248 00:14:07,520 --> 00:14:11,440 Speaker 1: was so massive. Nothing we could notice. What about magnetic 249 00:14:11,679 --> 00:14:13,720 Speaker 1: field though, That's okay, so what I don't fully get. 250 00:14:13,960 --> 00:14:17,200 Speaker 1: So with the magnetic field there, we're not quite sure 251 00:14:17,240 --> 00:14:19,680 Speaker 1: why Earth or how Earth has a magnetic field. But 252 00:14:19,880 --> 00:14:23,680 Speaker 1: the prevailing theory is that because of this coreolis effect 253 00:14:24,000 --> 00:14:27,920 Speaker 1: in the center of the earth, um whirlpools are created 254 00:14:29,040 --> 00:14:31,960 Speaker 1: of molten iron, and as this molten iron kind of 255 00:14:31,960 --> 00:14:34,760 Speaker 1: moves around informs these world pools that actually generates an 256 00:14:34,800 --> 00:14:38,240 Speaker 1: electrical field, an electrical current, which in turn generates a 257 00:14:38,280 --> 00:14:41,560 Speaker 1: magnetic field. So we have this magnetic field. We think 258 00:14:41,600 --> 00:14:44,160 Speaker 1: that's how we have it. But we also have long 259 00:14:44,200 --> 00:14:47,520 Speaker 1: suspected that the magnetic field protects the Earth from solar winds, 260 00:14:47,560 --> 00:14:51,560 Speaker 1: which are positively charged ions from the Sun that travel 261 00:14:51,600 --> 00:14:53,760 Speaker 1: about a million miles an hour off of the Sun 262 00:14:53,800 --> 00:14:57,360 Speaker 1: toward us, and they're about a million degrees celsius. And 263 00:14:57,400 --> 00:14:59,920 Speaker 1: we long thought that it protected our atmosphere from be 264 00:15:00,200 --> 00:15:03,480 Speaker 1: stripped of the ions that we need. Then we started 265 00:15:03,520 --> 00:15:06,480 Speaker 1: looking at other planets and um that don't have any 266 00:15:06,520 --> 00:15:08,200 Speaker 1: magnetic field, because I think it's just the Earth and 267 00:15:08,240 --> 00:15:09,840 Speaker 1: the Sun in our solar system are the only ones 268 00:15:09,840 --> 00:15:13,080 Speaker 1: with magnetic fields. UM. And we found that they lose 269 00:15:13,120 --> 00:15:16,560 Speaker 1: ions at about the same rate that our atmosphere loses ions. 270 00:15:16,600 --> 00:15:18,680 Speaker 1: So we don't know what the magnetic field is doing. 271 00:15:18,960 --> 00:15:21,480 Speaker 1: But I did come across this one interesting fact. We 272 00:15:21,520 --> 00:15:25,040 Speaker 1: lose about a ton of atmosphere a day, really yep, 273 00:15:25,160 --> 00:15:28,920 Speaker 1: and and mostly in the form of water vapor. So 274 00:15:29,240 --> 00:15:32,720 Speaker 1: the Earth is drying out very slowly. Wow. Ye boys, 275 00:15:32,760 --> 00:15:36,560 Speaker 1: So we're slowing down, We're drying out, and in four 276 00:15:36,920 --> 00:15:40,280 Speaker 1: million years will all be toasted. Yeah. That's pretty much 277 00:15:40,360 --> 00:15:42,200 Speaker 1: the long and short of this. And what what We 278 00:15:42,240 --> 00:15:44,680 Speaker 1: did a podcast on what would the Earth look like 279 00:15:44,760 --> 00:15:48,280 Speaker 1: in different inter roles in the future, and I think 280 00:15:48,280 --> 00:15:52,120 Speaker 1: we eventually landed on ultimately destruction and if we're even 281 00:15:52,160 --> 00:15:54,560 Speaker 1: here any longer. Yeah, exactly. We'll use the Earth up. 282 00:15:55,000 --> 00:15:57,720 Speaker 1: It's probably where we landed. Yeah, I think you're right. Well, 283 00:15:57,760 --> 00:16:02,320 Speaker 1: good going, Chuck. Let's hear for Chuck everybody. UM, do 284 00:16:02,360 --> 00:16:04,240 Speaker 1: you have anything else? I do not, sir. If you 285 00:16:04,240 --> 00:16:06,520 Speaker 1: want to learn more about the Earth standing still, go 286 00:16:06,640 --> 00:16:09,040 Speaker 1: to how stuff works dot com and type in earth 287 00:16:09,680 --> 00:16:13,320 Speaker 1: um and it will bring up some pretty cool articles 288 00:16:13,440 --> 00:16:18,600 Speaker 1: and probably an entire channel. There's Earth science just fascinates me. Yeah, 289 00:16:18,680 --> 00:16:21,440 Speaker 1: me too, I said, search bars somewhere in there, which 290 00:16:21,440 --> 00:16:25,440 Speaker 1: means it's time for a listener mail. Uh. You know 291 00:16:25,520 --> 00:16:27,280 Speaker 1: you called out for how we helped you in your 292 00:16:27,280 --> 00:16:32,840 Speaker 1: life emails. We got one from Rachel in Portland, Portland. Um, 293 00:16:32,920 --> 00:16:35,560 Speaker 1: you guys, Uh, you guys have helped me through some 294 00:16:35,880 --> 00:16:38,800 Speaker 1: of the toughest times in my life. I've shortened the 295 00:16:38,840 --> 00:16:41,280 Speaker 1: beginning and August I moved from a small town in 296 00:16:41,280 --> 00:16:44,720 Speaker 1: Mississippi to attend the University of Portland in Oregon. The 297 00:16:45,320 --> 00:16:47,880 Speaker 1: transition was rough, Needless to say, I did not handle 298 00:16:47,920 --> 00:16:51,760 Speaker 1: it well. I started smoking again, I had trouble focusing 299 00:16:51,800 --> 00:16:54,360 Speaker 1: on in attending classes, and I could tell that I 300 00:16:54,400 --> 00:16:57,720 Speaker 1: wasn't settling well or making friends. On top of all that, 301 00:16:57,800 --> 00:17:00,600 Speaker 1: my three year relationship with my high school sweetheart fell 302 00:17:00,600 --> 00:17:03,400 Speaker 1: apart because at the distance and stress of us both 303 00:17:03,400 --> 00:17:07,080 Speaker 1: beginning university. I began to relapse into depression, something I've 304 00:17:07,080 --> 00:17:10,000 Speaker 1: struggled with off and on for five years. Found myself 305 00:17:10,040 --> 00:17:12,480 Speaker 1: unable to listen to music, even because every song I 306 00:17:12,600 --> 00:17:17,359 Speaker 1: heard made me so sad, A one of those heartbreak 307 00:17:17,440 --> 00:17:19,320 Speaker 1: dates when you just sit around and like listen to 308 00:17:19,320 --> 00:17:23,240 Speaker 1: the radio and cry. I downloaded your podcast to listen 309 00:17:23,240 --> 00:17:25,200 Speaker 1: to as I walked to and front classes, and while 310 00:17:25,240 --> 00:17:27,840 Speaker 1: I did homework. Didn't notice at first, but every time 311 00:17:27,880 --> 00:17:30,359 Speaker 1: your podcast was on it made me laugh. I'd feel 312 00:17:30,359 --> 00:17:32,600 Speaker 1: a little bit better. About halfway through the semester, I 313 00:17:32,640 --> 00:17:35,280 Speaker 1: found the courage to seek help and visit the campus 314 00:17:35,600 --> 00:17:39,399 Speaker 1: health center for therapy and antidepressants. I am now my 315 00:17:39,440 --> 00:17:41,960 Speaker 1: second semester of college with a three point nine for 316 00:17:42,119 --> 00:17:44,720 Speaker 1: g p A. I have a few great friends, and 317 00:17:44,720 --> 00:17:47,960 Speaker 1: I'm even dating someone new. I love my school and 318 00:17:48,000 --> 00:17:50,760 Speaker 1: I love the city of Portland. I feel as if 319 00:17:50,800 --> 00:17:54,280 Speaker 1: your podcast servan integral part of helping me make the 320 00:17:54,320 --> 00:17:56,840 Speaker 1: transition from home to here. I've learned and laugh with y'all, 321 00:17:56,880 --> 00:18:01,119 Speaker 1: and now and then a southern draw will sneak into 322 00:18:01,160 --> 00:18:03,440 Speaker 1: one of your voices and make me nostalgic with this out. 323 00:18:04,040 --> 00:18:05,600 Speaker 1: It may sound silly, but I feel I'll come to 324 00:18:05,600 --> 00:18:07,439 Speaker 1: know you guys. I really want to thank you for 325 00:18:07,480 --> 00:18:11,400 Speaker 1: helping me through such a hard time. Rachel eighteen in Portland. 326 00:18:11,720 --> 00:18:15,760 Speaker 1: Thanks Rachel, it's awesome. I'm glad to hear you're doing better. Yeah. 327 00:18:15,920 --> 00:18:19,000 Speaker 1: I had a rough first few weeks of college. I 328 00:18:19,000 --> 00:18:22,000 Speaker 1: think a lot of people do. And uh, I think 329 00:18:22,119 --> 00:18:25,840 Speaker 1: my advice is to just stick it out and before 330 00:18:25,880 --> 00:18:28,439 Speaker 1: you know it, you're gonna be loving it. I remember 331 00:18:28,520 --> 00:18:31,320 Speaker 1: my parents telling me that when I went off the camp, 332 00:18:31,680 --> 00:18:35,280 Speaker 1: oh yeah, even like camp. I did not like camp. 333 00:18:35,760 --> 00:18:37,880 Speaker 1: Did you like going off the college? Yeah, that's fine, 334 00:18:37,960 --> 00:18:40,879 Speaker 1: you're probably ready with that. Yeah, I was. I freaked 335 00:18:40,880 --> 00:18:43,119 Speaker 1: out because I at the last minute, I tried to 336 00:18:43,200 --> 00:18:45,320 Speaker 1: change to go to Georgia Tech because my brother was there, 337 00:18:45,680 --> 00:18:47,240 Speaker 1: and I was basically scared. I was like, I just 338 00:18:47,240 --> 00:18:49,800 Speaker 1: want to go to school with my brother, and uh 339 00:18:49,880 --> 00:18:52,240 Speaker 1: it didn't Uh it was too late to get the 340 00:18:52,240 --> 00:18:53,639 Speaker 1: application in and so I was like, all right, I 341 00:18:53,640 --> 00:18:56,920 Speaker 1: guess I'm going to Georgia by myself. And uh it 342 00:18:57,119 --> 00:18:59,800 Speaker 1: ended up being the greatest thing ever. But I'm glad 343 00:19:00,000 --> 00:19:01,960 Speaker 1: stuck it out, you know the rest of the story. Yeah, 344 00:19:02,000 --> 00:19:04,280 Speaker 1: it is true. I mean, like, you know, just hanging 345 00:19:04,320 --> 00:19:06,760 Speaker 1: in there and being brave, even when it feels like 346 00:19:06,840 --> 00:19:10,040 Speaker 1: that's the worst thing to do. Often it's it's often 347 00:19:10,040 --> 00:19:11,920 Speaker 1: the best thing to do. And six years later and 348 00:19:12,000 --> 00:19:14,200 Speaker 1: I had a college diploma and a lot of friends 349 00:19:14,200 --> 00:19:18,399 Speaker 1: for life. It's good, chuckers. Uh, let's see. If you 350 00:19:18,440 --> 00:19:21,880 Speaker 1: have a great story about solar wind or how we've 351 00:19:21,920 --> 00:19:24,720 Speaker 1: helped you or call ite or whatever we want to 352 00:19:24,720 --> 00:19:27,560 Speaker 1: hear about it, you can find us on Twitter right 353 00:19:28,200 --> 00:19:31,040 Speaker 1: s y SK podcast. I feel like a lot of 354 00:19:31,080 --> 00:19:34,719 Speaker 1: you aren't getting that s y SK podcast. It's a 355 00:19:34,720 --> 00:19:37,600 Speaker 1: great Twitter feed. Yeah, Josh is the Twitter master. We 356 00:19:37,640 --> 00:19:41,440 Speaker 1: have a great Facebook page that Chuck helms Facebook dot 357 00:19:41,480 --> 00:19:44,879 Speaker 1: com slash stuff. You should know. People love that. You 358 00:19:44,880 --> 00:19:48,240 Speaker 1: can send us an email, which is fine. Uh. That's 359 00:19:48,280 --> 00:19:51,879 Speaker 1: Stuff Podcast at Discovery dot com and everybody, seriously, stop 360 00:19:51,880 --> 00:19:54,600 Speaker 1: what you're doing right now. Go to the home of 361 00:19:54,680 --> 00:19:58,120 Speaker 1: Josh and Chuck on the web. It's our very own website. 362 00:19:58,160 --> 00:20:06,520 Speaker 1: It's fun. It's called stuff. You should oh dot com 363 00:20:06,560 --> 00:20:08,960 Speaker 1: for more on this and thousands of other topics. Because 364 00:20:09,000 --> 00:20:18,199 Speaker 1: it how stuff works. Dot com m brought to you 365 00:20:18,240 --> 00:20:20,520 Speaker 1: by Toyota. Let's Go Places