1 00:00:01,560 --> 00:00:04,760 Speaker 1: Welcome to Stuff from the Science Lab from how stuff 2 00:00:04,760 --> 00:00:16,200 Speaker 1: works dot com. You guys, welcome to the podcast. This 3 00:00:16,320 --> 00:00:18,040 Speaker 1: is Alison. I don't know if the science editor at 4 00:00:18,040 --> 00:00:20,279 Speaker 1: how stuff works dot com. And there is Robert Lamb, 5 00:00:20,320 --> 00:00:23,400 Speaker 1: science writer and how stuff works dot com. So, Alison, 6 00:00:23,480 --> 00:00:27,320 Speaker 1: have you seen the movie Phantasm? I've not seen it. 7 00:00:27,320 --> 00:00:29,560 Speaker 1: It's a nineteen seventies flick, right, yeah, harror flick. You 8 00:00:29,800 --> 00:00:32,560 Speaker 1: haven't seen it. I have not, but you've mentioned it before, right, Well, okay, 9 00:00:32,560 --> 00:00:34,960 Speaker 1: it's awesome. It's um. I mean it's it's horrible, but 10 00:00:34,960 --> 00:00:39,199 Speaker 1: it's awesome. It's um. The basic plot line here is 11 00:00:39,440 --> 00:00:44,040 Speaker 1: you have a mortuary where some funny things are happening. 12 00:00:44,080 --> 00:00:48,480 Speaker 1: There silver balls flying around, stabbing people in the head. Uh. 13 00:00:48,520 --> 00:00:50,840 Speaker 1: And there are these dwarves running around in these little 14 00:00:51,280 --> 00:00:54,000 Speaker 1: like I think they're yellow, little yellow robes, okay, like 15 00:00:54,120 --> 00:00:58,600 Speaker 1: evil dwarves. Right, And you come to find out that 16 00:00:58,680 --> 00:01:01,840 Speaker 1: all of this basically has to do with gravity. There's 17 00:01:01,840 --> 00:01:04,040 Speaker 1: a really tall man, like a scary old man. It's 18 00:01:04,040 --> 00:01:06,919 Speaker 1: really tall, Okay. And it turns out he's from another 19 00:01:06,959 --> 00:01:13,360 Speaker 1: planet where the gravity is more intense, like a larger world. Okay, 20 00:01:13,440 --> 00:01:16,800 Speaker 1: so that's why he's taller when he comes to this world, okay, 21 00:01:17,040 --> 00:01:20,360 Speaker 1: and the deal with the dwarves, he's taking corpses and 22 00:01:20,480 --> 00:01:24,560 Speaker 1: smushing them down, making a more compact and bringing him 23 00:01:24,560 --> 00:01:26,600 Speaker 1: back to life a zombies and then sending them to 24 00:01:26,720 --> 00:01:30,960 Speaker 1: this other world to be like slaves. All right, So 25 00:01:31,120 --> 00:01:34,160 Speaker 1: dwarves are being used as as as zombies. Dwarves are 26 00:01:34,200 --> 00:01:36,880 Speaker 1: being used as slave labor on another world where there's 27 00:01:36,959 --> 00:01:40,880 Speaker 1: more gravity. And so this all occurs thanks to gravity. Yes, 28 00:01:40,959 --> 00:01:43,200 Speaker 1: like it Like for me anyway, as as a kid. 29 00:01:43,319 --> 00:01:45,680 Speaker 1: You know, it's like, you know, gravity is, They're great, 30 00:01:45,720 --> 00:01:48,080 Speaker 1: but I never think about it. But then somebody comes 31 00:01:48,080 --> 00:01:51,040 Speaker 1: along and shows me how gravity is affect you know, 32 00:01:51,880 --> 00:01:55,080 Speaker 1: zombie dwarves and uh and it it really you know, 33 00:01:55,160 --> 00:01:58,480 Speaker 1: unders it really resonated with me and underlining how amazing 34 00:01:58,480 --> 00:02:02,640 Speaker 1: gravity is. I mean, um, like I said, we take 35 00:02:02,640 --> 00:02:05,960 Speaker 1: it for granted because it's everywhere, because every pretty much 36 00:02:06,000 --> 00:02:10,040 Speaker 1: every physical act on the planet um involves gravity in 37 00:02:10,120 --> 00:02:14,120 Speaker 1: somewhere and within another. So that's what we're going to 38 00:02:14,200 --> 00:02:16,359 Speaker 1: talk about the day. We're gonna We're gonna basically talk 39 00:02:16,360 --> 00:02:21,360 Speaker 1: about four examples um of technologies that utilize gravity in 40 00:02:21,400 --> 00:02:26,120 Speaker 1: a way that highlight just how amazing it is. But 41 00:02:26,200 --> 00:02:27,840 Speaker 1: of course to do that, we need to talk briefly 42 00:02:27,880 --> 00:02:31,200 Speaker 1: about about gravity itself. Now, we have an excellent article 43 00:02:31,440 --> 00:02:35,920 Speaker 1: on how Stuff Works dot Com about this um and 44 00:02:36,120 --> 00:02:39,080 Speaker 1: I recommend checking that out if you want more details. 45 00:02:39,160 --> 00:02:45,359 Speaker 1: But basically, two schools of thought. There's there's Newton Newton's 46 00:02:45,440 --> 00:02:48,760 Speaker 1: uh a theory of universal gravitation from back in the 47 00:02:49,040 --> 00:02:53,400 Speaker 1: sixt eighties, and this is the idea. The gravity is 48 00:02:53,440 --> 00:02:56,600 Speaker 1: a predictable force that acts on all matter in the universe, 49 00:02:56,760 --> 00:03:01,160 Speaker 1: and it's a function of both mass and distance. Right. Basically, 50 00:03:01,200 --> 00:03:04,240 Speaker 1: each particle of matter attracts every other particle of matter, 51 00:03:04,880 --> 00:03:09,400 Speaker 1: all right. Whether we're talking about a great or a 52 00:03:09,520 --> 00:03:13,600 Speaker 1: massive sign. Okay, whether we're talking about a spaceship or 53 00:03:13,639 --> 00:03:17,040 Speaker 1: I don't know, a dog, everything has gravity, all right. 54 00:03:17,240 --> 00:03:18,800 Speaker 1: And if ever, and if the only two things you 55 00:03:18,840 --> 00:03:21,040 Speaker 1: had in the universe were a dog and a spaceship, 56 00:03:21,520 --> 00:03:24,760 Speaker 1: they would each have a great gravitational pull and it 57 00:03:24,840 --> 00:03:29,520 Speaker 1: would be drawn to each other. Okay, um, go ahead. 58 00:03:29,760 --> 00:03:32,600 Speaker 1: And then along comes Einstein. Yes, along comes Einstein, and 59 00:03:32,639 --> 00:03:37,320 Speaker 1: he says, fooie to this whole dog and spaceship business. 60 00:03:37,480 --> 00:03:39,800 Speaker 1: And he says that, he says that gravity isn't even 61 00:03:39,840 --> 00:03:44,000 Speaker 1: a force, all right, he's a he's seeing it more 62 00:03:44,200 --> 00:03:47,960 Speaker 1: as a distortion in the shape of space time, all right, 63 00:03:48,440 --> 00:03:53,480 Speaker 1: as the you know, a distortion in the fourth dimension. 64 00:03:54,320 --> 00:03:58,000 Speaker 1: And in Einstein's footsteps. You have some more modern theories 65 00:03:58,040 --> 00:04:02,120 Speaker 1: as well, okay, that are less even even less proven. 66 00:04:02,360 --> 00:04:05,080 Speaker 1: There's the idea that UM that gravity is due to 67 00:04:05,240 --> 00:04:09,200 Speaker 1: little particles called gravitons that that cause objects to be 68 00:04:09,200 --> 00:04:11,960 Speaker 1: attracted to one another. And there's another theory that there's 69 00:04:12,000 --> 00:04:16,719 Speaker 1: gravitational radiation UM, which which is supposedly the ideas that 70 00:04:16,880 --> 00:04:20,320 Speaker 1: gravitational radiation is generated when an object is accelerated by 71 00:04:20,360 --> 00:04:24,279 Speaker 1: the external force. Basically, the idea here is that gravity 72 00:04:24,320 --> 00:04:30,159 Speaker 1: is is awesome and every day it's mysterious. Um. Basically, 73 00:04:30,160 --> 00:04:32,640 Speaker 1: the idea here that it is that as every day 74 00:04:32,680 --> 00:04:34,800 Speaker 1: as gravity is, there's a lot we don't know. There's 75 00:04:34,800 --> 00:04:36,520 Speaker 1: a lot we don't know about it. It's still kind 76 00:04:36,560 --> 00:04:39,279 Speaker 1: of a mystery in many ways. All right. So with that, 77 00:04:39,360 --> 00:04:41,600 Speaker 1: let's kick off with four cool things that gravity can 78 00:04:41,640 --> 00:04:43,360 Speaker 1: do for you. Yeah, what do you got? What can 79 00:04:43,400 --> 00:04:46,080 Speaker 1: gravity do for you? Well, if you listen to our 80 00:04:46,160 --> 00:04:50,479 Speaker 1: Fighting Asteroids podcast, we touched on this briefly but gravity 81 00:04:50,680 --> 00:04:54,080 Speaker 1: can actually I could save the Earth from being destroyed 82 00:04:54,080 --> 00:04:57,120 Speaker 1: by some crazy space rock and always good. Yeah, I 83 00:04:57,160 --> 00:05:01,239 Speaker 1: like this. Um, So this thing called a gravity tractor, 84 00:05:01,320 --> 00:05:03,800 Speaker 1: and I'm not talking about the the grateful dead cover 85 00:05:03,880 --> 00:05:07,120 Speaker 1: band that seems to be located in upstate New York 86 00:05:07,120 --> 00:05:11,440 Speaker 1: of the same name. This gravity tractor, actually, um might 87 00:05:11,480 --> 00:05:14,039 Speaker 1: have a might have a chance of being built. According 88 00:05:14,040 --> 00:05:17,000 Speaker 1: to the BBC, there's this British company by the name 89 00:05:17,040 --> 00:05:20,240 Speaker 1: of E. A. D. S Astrium that they finally started 90 00:05:20,279 --> 00:05:23,719 Speaker 1: taking concrete steps to make the graph tractor reality. So 91 00:05:23,839 --> 00:05:26,000 Speaker 1: it's the graph tractor gonna do it well. It's a 92 00:05:26,120 --> 00:05:31,200 Speaker 1: robotic spacecraft weighing roughly ten tons or so, and it 93 00:05:31,240 --> 00:05:34,159 Speaker 1: has a has a particularly daunting task. Once it's launched 94 00:05:34,160 --> 00:05:37,360 Speaker 1: into space, it has to get within forty eight m 95 00:05:37,560 --> 00:05:41,200 Speaker 1: so roughly a hundred fifty feet of the space rocking question. 96 00:05:41,400 --> 00:05:43,360 Speaker 1: And once it gets within that range, it has to 97 00:05:43,520 --> 00:05:45,520 Speaker 1: pull the rock toward it, and the two of them 98 00:05:45,520 --> 00:05:48,359 Speaker 1: march happily off on a path that's not kind of 99 00:05:48,600 --> 00:05:52,040 Speaker 1: coincide with the Earth and now in theory though it 100 00:05:52,080 --> 00:05:54,719 Speaker 1: could also if you had a New York area jam 101 00:05:54,760 --> 00:05:58,600 Speaker 1: band floating in space. It could also use its immense 102 00:05:58,600 --> 00:06:01,360 Speaker 1: gravity to to pull them aside as well. Right right, 103 00:06:01,400 --> 00:06:03,960 Speaker 1: and I think if you pull the string cheese incident 104 00:06:04,080 --> 00:06:06,240 Speaker 1: on there, I mean it could just do crazy winners 105 00:06:06,480 --> 00:06:09,080 Speaker 1: with a space rocks headed our way. Um. And the 106 00:06:09,200 --> 00:06:11,599 Speaker 1: other chicky thing about the tractors, it's gonna we have 107 00:06:11,640 --> 00:06:14,359 Speaker 1: to launched. The other chicky thing about the tractors that 108 00:06:14,440 --> 00:06:16,160 Speaker 1: has to be launched fifteen years ahead of time. So 109 00:06:16,839 --> 00:06:19,520 Speaker 1: we're kind of we're kind of stuck. This is what 110 00:06:19,520 --> 00:06:22,279 Speaker 1: we're relying on right now. So gravity, it can it 111 00:06:22,320 --> 00:06:25,080 Speaker 1: can save you from a space rock someday. Perhaps what 112 00:06:25,120 --> 00:06:27,720 Speaker 1: else can it do out in space? Well, gravity can 113 00:06:27,800 --> 00:06:31,560 Speaker 1: also help you fire a spaceship to some distant corner 114 00:06:31,760 --> 00:06:34,159 Speaker 1: of the Solar System. I like the way that sounds. Yeah, 115 00:06:34,279 --> 00:06:37,479 Speaker 1: this is something we call gravity assist. Sometimes you see 116 00:06:37,480 --> 00:06:40,120 Speaker 1: it referred to as a gravity slingshot, but that's a 117 00:06:40,120 --> 00:06:43,320 Speaker 1: little misleading. Um, so just think of it. It's gravity assist, 118 00:06:44,160 --> 00:06:46,800 Speaker 1: all right. And to understand that, you need to think 119 00:06:46,800 --> 00:06:50,400 Speaker 1: of the Solar System in terms of the Sun's gravity. Well, okay, 120 00:06:52,160 --> 00:06:54,680 Speaker 1: imagine a bathtub, all right, It's filled with water and 121 00:06:54,680 --> 00:06:57,440 Speaker 1: it has a little boat in it. Okay, you pull 122 00:06:57,560 --> 00:07:01,200 Speaker 1: the drain, the water begins to to to go to 123 00:07:01,200 --> 00:07:04,080 Speaker 1: to leave the bathtub in the form of a whirlpool. 124 00:07:04,279 --> 00:07:06,520 Speaker 1: The little boat is going to be pulled towards the whirlpool, 125 00:07:07,000 --> 00:07:09,520 Speaker 1: all right. In the scenario, the Sun is the whirlpool. 126 00:07:09,640 --> 00:07:12,160 Speaker 1: It's the object of the most mass and if it 127 00:07:12,200 --> 00:07:15,880 Speaker 1: has the most gravitational pool and spacecraft, right, and it's 128 00:07:15,920 --> 00:07:18,720 Speaker 1: gonna if it's if the little toy boat is moving 129 00:07:18,760 --> 00:07:21,320 Speaker 1: towards the world pool, it's gonna go faster to move 130 00:07:21,360 --> 00:07:23,120 Speaker 1: away from the world pool. It has to work harder 131 00:07:23,880 --> 00:07:27,720 Speaker 1: and it's going slower. Okay, that's basically the gravity well. 132 00:07:28,080 --> 00:07:32,520 Speaker 1: So if we want to send something farther out into 133 00:07:32,520 --> 00:07:36,360 Speaker 1: the gravity well, out to one of the outer planets, um, 134 00:07:36,440 --> 00:07:39,080 Speaker 1: we need to we need a little help, all right, 135 00:07:39,640 --> 00:07:42,840 Speaker 1: and and it and it uh, it's more effective if 136 00:07:42,840 --> 00:07:45,080 Speaker 1: we don't have to depend on say, you know, thrusters 137 00:07:45,120 --> 00:07:48,360 Speaker 1: and rockets to do all of the work and take 138 00:07:48,400 --> 00:07:51,360 Speaker 1: a take advantage of inherent force. Right. So that's where 139 00:07:51,360 --> 00:07:53,160 Speaker 1: the gravity assist comes in. And this is a fly 140 00:07:53,240 --> 00:07:56,920 Speaker 1: by technique where we can add or subtract momentum to 141 00:07:57,040 --> 00:08:00,400 Speaker 1: increase or discrete decrease the energy of a spacecraft. Orbit, 142 00:08:00,640 --> 00:08:03,840 Speaker 1: so we've used it. Yes, UM. Take, for for example, 143 00:08:03,920 --> 00:08:09,880 Speaker 1: Voyager two launched in um, we flew it by Jupiter. 144 00:08:10,040 --> 00:08:12,560 Speaker 1: Will first, just you know, to see Jupiter, that was 145 00:08:12,760 --> 00:08:16,119 Speaker 1: one of its mission objectives. But also um, by flying 146 00:08:16,200 --> 00:08:20,080 Speaker 1: flying by Jupiter, this provided traject trajectory boost to shoot 147 00:08:20,080 --> 00:08:23,720 Speaker 1: it towards Saturn. Now again go back and going back 148 00:08:23,720 --> 00:08:25,920 Speaker 1: to the spaceship and the dog. You know, both both 149 00:08:25,920 --> 00:08:29,720 Speaker 1: the spaceship and the dog have mass and therefore have 150 00:08:29,960 --> 00:08:34,240 Speaker 1: their own gravitational pool. Right, So Voyager two has its 151 00:08:34,240 --> 00:08:38,000 Speaker 1: own gravitational pool, as does Jupiter. All right. So when 152 00:08:38,000 --> 00:08:41,520 Speaker 1: the spacecraft actually tugs on Jupiter as it goes past, 153 00:08:41,679 --> 00:08:45,679 Speaker 1: all right, and actually decreases the planet's orbital momentum by 154 00:08:45,679 --> 00:08:50,560 Speaker 1: a tiny amount, very tiny amount. In return, the spacecraft 155 00:08:50,600 --> 00:08:55,240 Speaker 1: acquires momentum from Jupiter. Except as we're talking, a significant 156 00:08:55,240 --> 00:08:58,520 Speaker 1: amount of momentum, and uh, and it it shoots it 157 00:08:58,559 --> 00:09:01,480 Speaker 1: off in this new trajectory. Okay. Uh. One of the 158 00:09:01,720 --> 00:09:05,160 Speaker 1: more useful analogies, uh that that you find for this 159 00:09:05,360 --> 00:09:10,480 Speaker 1: is imagine a kid standing next to um a train track, okay, 160 00:09:10,840 --> 00:09:13,240 Speaker 1: and he has a softball in his hand. The softball 161 00:09:13,320 --> 00:09:16,920 Speaker 1: is a spacecraft, all right, And then hurtling down the 162 00:09:17,960 --> 00:09:22,360 Speaker 1: train track is a locomotive, al right. The locomotive is Jupiter. 163 00:09:22,840 --> 00:09:26,160 Speaker 1: If you were to throw the softball and hit the 164 00:09:26,240 --> 00:09:30,680 Speaker 1: front of the coming train, then the softball would would 165 00:09:30,760 --> 00:09:33,679 Speaker 1: veer off into another direction with the momentum of the train. 166 00:09:36,040 --> 00:09:38,480 Speaker 1: So it's it's very useful for for shooting off any 167 00:09:38,520 --> 00:09:42,400 Speaker 1: number of probes UH into into the surrounding Solar system 168 00:09:42,440 --> 00:09:45,280 Speaker 1: and uh A lot of people have even looked at 169 00:09:45,559 --> 00:09:49,720 Speaker 1: considered possibilities of using it for the future use of 170 00:09:49,760 --> 00:09:53,720 Speaker 1: man space spacecraft being able to like use the the 171 00:09:53,840 --> 00:09:57,080 Speaker 1: Sun's gravity to shoot an aircraft off to a not 172 00:09:57,160 --> 00:10:02,480 Speaker 1: an aircraft, of using the Sun's gravitational poole to um 173 00:10:02,640 --> 00:10:06,480 Speaker 1: to shoot a spaceship off towards another system. Have you've 174 00:10:06,480 --> 00:10:09,440 Speaker 1: seen Star Trek or any number of science fiction properties, 175 00:10:09,480 --> 00:10:12,640 Speaker 1: then you've you've you've heard examples of this, So I'd 176 00:10:12,640 --> 00:10:14,840 Speaker 1: say that's a cool thing. Gravity shooting you to a 177 00:10:14,880 --> 00:10:18,000 Speaker 1: distant corner of the galaxy. On a more earthly level, 178 00:10:18,080 --> 00:10:21,040 Speaker 1: gravity can perhaps let your home someday. And this is 179 00:10:21,080 --> 00:10:23,240 Speaker 1: an idea that's been around for quite a while. Back 180 00:10:23,280 --> 00:10:25,000 Speaker 1: in the nineteen seventies, there are a bunch of fellows 181 00:10:25,040 --> 00:10:27,480 Speaker 1: at the Lawrence Livermore lab who thought we should try 182 00:10:27,480 --> 00:10:31,120 Speaker 1: to harness the energy potential of gravity courtesy of black hole. 183 00:10:31,720 --> 00:10:34,000 Speaker 1: So this is what they had in mind. You guys, 184 00:10:34,000 --> 00:10:36,880 Speaker 1: remember that a black hole forms when this big old 185 00:10:36,880 --> 00:10:40,160 Speaker 1: star is dying and it's collapsing inward, and the end 186 00:10:40,200 --> 00:10:44,480 Speaker 1: result is this tiny object that's just unspeakably dense. So 187 00:10:44,600 --> 00:10:47,120 Speaker 1: the gravitational force of a black hole is large, so 188 00:10:47,200 --> 00:10:49,560 Speaker 1: large that not even light can escape it. I know 189 00:10:49,640 --> 00:10:52,000 Speaker 1: you guys know this, but let's just reiterate it. So 190 00:10:52,160 --> 00:10:55,400 Speaker 1: the idea was, according to these scientists, was well, let's 191 00:10:55,440 --> 00:10:59,360 Speaker 1: locate a black hole, well, get it to orbit the Earth. 192 00:10:59,480 --> 00:11:01,960 Speaker 1: That's now that that's the point I think where you 193 00:11:02,040 --> 00:11:04,640 Speaker 1: just you cancel this plan like that just sounds like 194 00:11:04,679 --> 00:11:07,640 Speaker 1: the worst idea ever. Hey, let me just okay, it 195 00:11:07,640 --> 00:11:10,400 Speaker 1: gets better, Okay, Okay. So you're gonna get the said 196 00:11:10,400 --> 00:11:12,080 Speaker 1: black hole to orbit the Earth with the help of 197 00:11:12,080 --> 00:11:14,959 Speaker 1: a spaceship, and once it's in permanent orbit, just you know, 198 00:11:15,040 --> 00:11:18,360 Speaker 1: kind of hanging out like black hole does, you're gonna 199 00:11:18,520 --> 00:11:21,800 Speaker 1: tap the power of said black hole by firing matter 200 00:11:21,840 --> 00:11:24,120 Speaker 1: into it. Okay. So the whole plan is we're going 201 00:11:24,200 --> 00:11:27,520 Speaker 1: to go and find the most destructive force in the universe. 202 00:11:27,720 --> 00:11:30,520 Speaker 1: We're going to bring it home and then we're going 203 00:11:30,559 --> 00:11:33,800 Speaker 1: to feed it. Yes, yes, and then wait, it gets better. 204 00:11:34,120 --> 00:11:37,400 Speaker 1: So you know that things get really tiny, as are 205 00:11:37,440 --> 00:11:39,800 Speaker 1: you know, hurtling towards their on their death spiral towards 206 00:11:39,800 --> 00:11:43,320 Speaker 1: a black hole. Well, all that getting tiny business generates 207 00:11:43,360 --> 00:11:46,360 Speaker 1: an amounse amount of energy, and they thought that this 208 00:11:46,400 --> 00:11:49,320 Speaker 1: amount of energy could in fact be enough to start 209 00:11:49,320 --> 00:11:53,960 Speaker 1: a fusion reaction. So this one, this idea of a 210 00:11:53,960 --> 00:11:57,120 Speaker 1: black hole gravity thing, actually never came to fruition. I 211 00:11:57,120 --> 00:12:00,280 Speaker 1: think probably the the first point of business was moving 212 00:12:00,360 --> 00:12:03,040 Speaker 1: the black hole, or actually maybe even locating black hole 213 00:12:03,080 --> 00:12:04,719 Speaker 1: and then moving black hole. So a couple of a 214 00:12:04,760 --> 00:12:07,439 Speaker 1: couple of a couple of holes in this plan. Yes, 215 00:12:09,920 --> 00:12:13,000 Speaker 1: the latest incarnation of gravity power is a lamp. It's 216 00:12:13,040 --> 00:12:18,640 Speaker 1: a little bit simpler and a black hole. No no, no, no, um. 217 00:12:19,040 --> 00:12:21,960 Speaker 1: Let me explain. It's conceived of by this grad student 218 00:12:21,960 --> 00:12:24,920 Speaker 1: at Virginia Tech, and I think he entered his invention 219 00:12:24,920 --> 00:12:27,400 Speaker 1: in some sort of TEO thousand in a green Tech award. 220 00:12:28,200 --> 00:12:30,280 Speaker 1: And it's a guy by the name of claymont. Well. 221 00:12:30,360 --> 00:12:34,480 Speaker 1: Clay calls his lamp the gravity So conceptually, here's how 222 00:12:34,640 --> 00:12:38,439 Speaker 1: Clay's gravity powered lamp works. If you picture kind of 223 00:12:38,480 --> 00:12:43,040 Speaker 1: a cylinder shaped floor lamp, maybe about five feet tall. Um, 224 00:12:43,240 --> 00:12:45,440 Speaker 1: Now imagine that there are these like five ten pound 225 00:12:45,440 --> 00:12:48,920 Speaker 1: brass swats sitting there at the top. And for those 226 00:12:48,960 --> 00:12:50,640 Speaker 1: of you guys who don't know what one is, there's 227 00:12:50,640 --> 00:12:54,280 Speaker 1: a ball screw in in the in the floor lamp. 228 00:12:54,320 --> 00:12:56,160 Speaker 1: And what is the what is ball screw? I had 229 00:12:56,200 --> 00:12:58,719 Speaker 1: no idea before I started doing this podcast. Well, it's 230 00:12:58,720 --> 00:13:02,240 Speaker 1: a it's a linear screw and um, something rotates downward 231 00:13:02,320 --> 00:13:05,200 Speaker 1: on it. So it's kind of like falling on the 232 00:13:05,200 --> 00:13:08,160 Speaker 1: ball screw. It's moving downward on the ball screw. And 233 00:13:08,200 --> 00:13:10,520 Speaker 1: as these brass weades moved downward on the ball screw, 234 00:13:10,920 --> 00:13:16,439 Speaker 1: the screw rotates, and that rotational motion is able to 235 00:13:16,480 --> 00:13:20,120 Speaker 1: spin a generator and convert the motion into electricity. So 236 00:13:20,200 --> 00:13:21,880 Speaker 1: if you can't quite picture, you can always check out 237 00:13:21,880 --> 00:13:24,400 Speaker 1: the illustration. We have a good one on our how 238 00:13:24,400 --> 00:13:28,520 Speaker 1: gravity powered lamps were an article. So anyway, this electricity 239 00:13:28,520 --> 00:13:32,280 Speaker 1: powers ten led bulbs which light up and whaila you 240 00:13:32,320 --> 00:13:34,439 Speaker 1: have light. And do you think, well, how long is 241 00:13:34,480 --> 00:13:37,000 Speaker 1: that going to take? Because gravity can happen relatively fast right, 242 00:13:37,760 --> 00:13:40,280 Speaker 1: falling objects might be down to the bottom and lamp, 243 00:13:40,280 --> 00:13:43,280 Speaker 1: but actually it takes four hours, so that would be 244 00:13:43,400 --> 00:13:45,400 Speaker 1: a good amount of light. Would it would work faster 245 00:13:45,520 --> 00:13:50,679 Speaker 1: on the the phantasm planet with the dwarves? Sure would, Surewood. 246 00:13:51,320 --> 00:13:54,439 Speaker 1: It's also worth noting here that the hour glass is 247 00:13:54,480 --> 00:13:58,720 Speaker 1: actually a gravity powered timetelling device. Yeah, and it seems 248 00:13:58,720 --> 00:14:02,160 Speaker 1: like a little bit of a simple concept than the 249 00:14:02,160 --> 00:14:06,319 Speaker 1: The gravity powered lamp also cuckoo clocks, but are also 250 00:14:06,400 --> 00:14:11,520 Speaker 1: worth considering that they're actually powered by black holes. So anyway, 251 00:14:11,559 --> 00:14:13,719 Speaker 1: the thing with Poort Clay's lamp is that the d 252 00:14:13,880 --> 00:14:16,400 Speaker 1: technology isn't quite where it needs to be, and the 253 00:14:16,480 --> 00:14:18,559 Speaker 1: LEDs aren't as efficient as they need to be, and 254 00:14:18,640 --> 00:14:21,800 Speaker 1: so that means the weights would have to be much heavier. 255 00:14:21,840 --> 00:14:24,560 Speaker 1: And that's about where we are with the gravity powered lamp. 256 00:14:24,640 --> 00:14:28,000 Speaker 1: So you cannot buy one at your local lamp star. 257 00:14:28,280 --> 00:14:31,280 Speaker 1: It sounds promising, though, I like the idea of gravity 258 00:14:31,280 --> 00:14:35,400 Speaker 1: powered electronics. Well, I'll tell you another thing that gravity 259 00:14:35,440 --> 00:14:40,080 Speaker 1: can do for us. What gravity can help us understand 260 00:14:40,080 --> 00:14:43,400 Speaker 1: what's going on underneath the Earth surface. And how many 261 00:14:43,480 --> 00:14:45,960 Speaker 1: do that? Well, think of it this way. Imagine an 262 00:14:46,000 --> 00:14:50,080 Speaker 1: appetizer sampler platter. All right, you know it's it's covered 263 00:14:50,120 --> 00:14:54,640 Speaker 1: with fried cheese sticks, hush puppies. What are the what's 264 00:14:54,680 --> 00:14:57,520 Speaker 1: the meat on the stick called? Oh, chicken settee? Chicken 265 00:14:57,560 --> 00:15:01,560 Speaker 1: sette all right, all of idea of different foods. Now, 266 00:15:02,080 --> 00:15:05,760 Speaker 1: something late and fluffy too, right? Yeah? Like, well, hush 267 00:15:05,800 --> 00:15:09,360 Speaker 1: puppies are lighting fluffy? Right? Well, what's something light and 268 00:15:09,360 --> 00:15:13,240 Speaker 1: fluffy do you get as an appetizer? Um, we'll see. 269 00:15:13,240 --> 00:15:15,680 Speaker 1: I think that's the thing. Most appetizers, they're so hideously 270 00:15:15,800 --> 00:15:19,240 Speaker 1: unhealthy that you get them in small portions first, right, okay, 271 00:15:19,240 --> 00:15:23,240 Speaker 1: So imagine something light and fluffy appetizer, but hush puppy. 272 00:15:23,640 --> 00:15:26,440 Speaker 1: So so you have all these different items on the plate, right, 273 00:15:26,880 --> 00:15:31,880 Speaker 1: and all of them have different densities, okay, which means 274 00:15:32,720 --> 00:15:36,400 Speaker 1: and all of them have gravitational pools, all right, And 275 00:15:37,000 --> 00:15:40,880 Speaker 1: the more dense the appetizer item, the more gravitational pool 276 00:15:40,920 --> 00:15:45,520 Speaker 1: it has. Okay, Okay, all right, Well, our planet is 277 00:15:45,560 --> 00:15:49,480 Speaker 1: basically an appetizer platter when it comes to gravity. All right, 278 00:15:51,120 --> 00:15:55,720 Speaker 1: there are our planet has is covered with varying densities 279 00:15:55,760 --> 00:15:59,600 Speaker 1: of rock. Um, you have you have water that's cold, 280 00:15:59,640 --> 00:16:01,720 Speaker 1: you have water that's hot, and of course there's different 281 00:16:01,720 --> 00:16:04,000 Speaker 1: tensity there. Um. You know, you look under the Earth, 282 00:16:04,000 --> 00:16:06,800 Speaker 1: they're gonna be they're gonna be empty caverns, they're going 283 00:16:06,880 --> 00:16:10,080 Speaker 1: to be uh, you know, blocks of solid bedrock. There's 284 00:16:10,120 --> 00:16:13,200 Speaker 1: going to be you know, liquid magma. So gravity is 285 00:16:13,200 --> 00:16:15,120 Speaker 1: gonna vary according to where are you on there. That's 286 00:16:15,120 --> 00:16:17,640 Speaker 1: interesting because I guess I just think of it as 287 00:16:17,680 --> 00:16:20,400 Speaker 1: such a constant uniform Yeah. Yeah, we think of it 288 00:16:20,480 --> 00:16:24,720 Speaker 1: more as uh, you know, a pizza with a pizza's 289 00:16:24,720 --> 00:16:28,240 Speaker 1: worth of you know, of a uniform gravitational pool. But 290 00:16:28,720 --> 00:16:31,960 Speaker 1: like if you go up to Hudson Bay in Canada, Um, 291 00:16:32,200 --> 00:16:34,960 Speaker 1: the gravity is actually less there. And I need to 292 00:16:35,000 --> 00:16:38,359 Speaker 1: stress that it's not not less in the sense that 293 00:16:38,360 --> 00:16:41,480 Speaker 1: that you can go to, uh to Hudson Bay and 294 00:16:41,600 --> 00:16:43,800 Speaker 1: uh and feel like you lost weight. It's right, You're 295 00:16:43,800 --> 00:16:45,240 Speaker 1: not gonna be able to fit in your skinny jeans, 296 00:16:45,240 --> 00:16:49,320 Speaker 1: are right. The Earth's gravity is still pretty uniform, um, 297 00:16:49,400 --> 00:16:54,240 Speaker 1: all all across the globe, but it varies um to 298 00:16:54,360 --> 00:16:57,560 Speaker 1: it to a slight degree um wherever you go. All right, 299 00:16:58,680 --> 00:17:00,720 Speaker 1: So um, you know, most people say, well, what does 300 00:17:00,840 --> 00:17:04,119 Speaker 1: what does that matter? Right? It matters when you start 301 00:17:04,440 --> 00:17:09,400 Speaker 1: looking into fluid dynamics, alright. The ocean, for instance, Um, 302 00:17:09,480 --> 00:17:12,800 Speaker 1: you have it dictates the flow of hot and cold water, 303 00:17:13,160 --> 00:17:16,000 Speaker 1: all right. I think of it as a topography, okay, 304 00:17:16,160 --> 00:17:18,639 Speaker 1: Like if you have a hill next to a plane, 305 00:17:19,200 --> 00:17:21,360 Speaker 1: you know water is gonna flow down that hill. All right. 306 00:17:21,760 --> 00:17:23,800 Speaker 1: Well you have the same kind of topography going on 307 00:17:24,000 --> 00:17:27,880 Speaker 1: across the planet, except in terms of gravity, with fluids 308 00:17:27,960 --> 00:17:33,240 Speaker 1: drawn towards the areas of higher gravity. Okay. So we're 309 00:17:33,320 --> 00:17:36,920 Speaker 1: very interested in finding out exactly what this uh, this 310 00:17:37,200 --> 00:17:40,280 Speaker 1: secret topography looks like. We in fact, we've launched to 311 00:17:40,760 --> 00:17:45,520 Speaker 1: um Um orbiting a spacecraft. There's a European Space Agencies 312 00:17:45,920 --> 00:17:49,919 Speaker 1: Gravity Field and Steady State Ocean Circulation Explore and this 313 00:17:50,000 --> 00:17:53,440 Speaker 1: is up there right now, um, yes, called GHOS. See 314 00:17:54,000 --> 00:17:56,320 Speaker 1: that one went up in two thousand nine. And then 315 00:17:56,359 --> 00:18:00,320 Speaker 1: there's NASA's Gravity Recovery and Climate experiment that's called Race 316 00:18:00,720 --> 00:18:03,480 Speaker 1: and Grace went up in two thousand two. All right, ghost. 317 00:18:03,520 --> 00:18:07,080 Speaker 1: These mission has been to take a picture of what 318 00:18:07,920 --> 00:18:10,719 Speaker 1: this uh, the secret topography of gravity, which we call 319 00:18:10,800 --> 00:18:13,240 Speaker 1: the geode, to take a picture of what that looks 320 00:18:13,280 --> 00:18:16,199 Speaker 1: like right at nay moment of time, Like what are 321 00:18:16,200 --> 00:18:19,200 Speaker 1: the highs, what are the lows? Uh? Grace has been 322 00:18:19,359 --> 00:18:24,000 Speaker 1: looking at how the geo changes, because it's always changing too. 323 00:18:24,119 --> 00:18:26,040 Speaker 1: It's not like like you can you know, you'll be 324 00:18:26,040 --> 00:18:27,520 Speaker 1: able to go here, and oh, the gravity is always 325 00:18:27,520 --> 00:18:30,080 Speaker 1: going to be this, especially when it comes to the ocean. 326 00:18:30,160 --> 00:18:32,520 Speaker 1: And why do we care if the geo changes? Because 327 00:18:32,560 --> 00:18:35,720 Speaker 1: the more we understand how the ocean transports heat and water, 328 00:18:35,880 --> 00:18:38,359 Speaker 1: the more we understand how the ocean moves, And the 329 00:18:38,359 --> 00:18:40,119 Speaker 1: more we understand how the ocean moves, the more we 330 00:18:40,200 --> 00:18:43,520 Speaker 1: understand how the atmosphere moves. See, it's all a part 331 00:18:43,560 --> 00:18:47,280 Speaker 1: of Earth's outer layer of fluid, all right, and that 332 00:18:47,359 --> 00:18:50,800 Speaker 1: is where our weather takes place. UM and uh and 333 00:18:50,920 --> 00:18:54,399 Speaker 1: you know everything from from fierce hurricanes, two patterns of 334 00:18:54,480 --> 00:18:58,800 Speaker 1: drought and uh floods and what have you? All right, UM, 335 00:18:58,840 --> 00:19:01,560 Speaker 1: so it helps us a better understanding of global climate. 336 00:19:02,320 --> 00:19:05,800 Speaker 1: On a more specific note, UM scientists think it will 337 00:19:05,800 --> 00:19:09,040 Speaker 1: be able to look, uh, look at changes in in gravity, 338 00:19:09,200 --> 00:19:13,880 Speaker 1: changes in density too, to determined shifts and water mass 339 00:19:13,960 --> 00:19:17,399 Speaker 1: caused by droughts or floods. And it will also also 340 00:19:17,760 --> 00:19:21,960 Speaker 1: allow us to better understand plate tectonics, UH, seismic activity. 341 00:19:22,119 --> 00:19:26,080 Speaker 1: You know, what's what's happening underneath underneath the soil um 342 00:19:26,080 --> 00:19:28,440 Speaker 1: in the crust to you know, the leads to two 343 00:19:28,520 --> 00:19:32,040 Speaker 1: two earthquakes and uh another phenomena and uh and just 344 00:19:32,119 --> 00:19:37,639 Speaker 1: the geological geophysical processes that underlie the the Earth. Sorry, 345 00:19:37,640 --> 00:19:39,520 Speaker 1: but it's pretty it's pretty I'm getting a little long 346 00:19:39,520 --> 00:19:41,919 Speaker 1: winded here, but it's pretty pretty, pretty awesome, and that's 347 00:19:41,920 --> 00:19:44,919 Speaker 1: why we're looking into it. So I hope you've inspired 348 00:19:44,920 --> 00:19:47,800 Speaker 1: some reverence for gravity and you besides the kind of 349 00:19:47,840 --> 00:19:49,639 Speaker 1: gravity that trips you up and makes you fall flat 350 00:19:49,680 --> 00:19:53,120 Speaker 1: on your face and gravity is pretty cool. Um. So 351 00:19:53,160 --> 00:19:55,160 Speaker 1: now we would like to take a moment to imagine 352 00:19:55,200 --> 00:19:59,919 Speaker 1: a world without gravity. Oh, we were going to talk 353 00:20:00,080 --> 00:20:02,080 Speaker 1: about it or just imagine it, because I was just 354 00:20:02,119 --> 00:20:05,520 Speaker 1: going to picture it. Yeah. One thing that's really gonna 355 00:20:05,520 --> 00:20:08,440 Speaker 1: suck is that all the atmosphere is going to drift 356 00:20:08,480 --> 00:20:12,720 Speaker 1: off into space and we're not gonna be able to breathe. Yeah. Also, 357 00:20:12,880 --> 00:20:14,359 Speaker 1: I don't think I don't think our hair is gonna 358 00:20:14,359 --> 00:20:17,320 Speaker 1: look right. I mean, how do you style your hair 359 00:20:17,359 --> 00:20:20,520 Speaker 1: for that? That's true? I mean what kind of products 360 00:20:20,600 --> 00:20:25,639 Speaker 1: could could combat that effect? Um? I think that it 361 00:20:25,640 --> 00:20:28,840 Speaker 1: would suck if the the oceans boiled away and just 362 00:20:28,920 --> 00:20:32,879 Speaker 1: kind of float it off into the void um. On 363 00:20:32,960 --> 00:20:35,240 Speaker 1: a more mundane level, I think eating would kind of 364 00:20:35,359 --> 00:20:39,679 Speaker 1: pose a number of challenges. Only the astronauts. They'd be 365 00:20:39,720 --> 00:20:42,640 Speaker 1: sitting there, happy as you please, eating their dinner out 366 00:20:42,640 --> 00:20:45,000 Speaker 1: of their bags. Everybody else would just be in full 367 00:20:45,000 --> 00:20:48,160 Speaker 1: freak out mode. Yeah, like trying to run after their 368 00:20:48,200 --> 00:20:53,200 Speaker 1: hamburger which had floated off into bun Yeah, and the 369 00:20:53,280 --> 00:20:55,960 Speaker 1: chop bits of onion and I'm sorry, catch ups. Just 370 00:20:56,000 --> 00:20:59,680 Speaker 1: a globular thing floating out there. Yeah, yeah, that would 371 00:20:59,680 --> 00:21:02,240 Speaker 1: be bad. So that would be a world without gravity, 372 00:21:02,280 --> 00:21:05,040 Speaker 1: and we hope that we may never encounter it. So 373 00:21:05,080 --> 00:21:06,880 Speaker 1: if you want to tell us why you think gravity 374 00:21:06,920 --> 00:21:09,360 Speaker 1: is cool or maybe not so cool, send us an 375 00:21:09,359 --> 00:21:12,240 Speaker 1: email at science stuff at how stuff works dot com, 376 00:21:12,400 --> 00:21:15,400 Speaker 1: or go read about gravity where we're at site. Yeah, 377 00:21:15,400 --> 00:21:17,119 Speaker 1: and when you got to check out the blogs where 378 00:21:17,680 --> 00:21:21,840 Speaker 1: we handle any number of scientific specs, including zombies from 379 00:21:21,840 --> 00:21:32,600 Speaker 1: time to time. Thanks for listening, guys. For more on 380 00:21:32,640 --> 00:21:35,119 Speaker 1: this and thousands of other topics, is that how stuff 381 00:21:35,119 --> 00:21:38,679 Speaker 1: works dot com. Want more how stuff works, check out 382 00:21:38,720 --> 00:21:40,920 Speaker 1: our blogs on the house stuff works dot com home 383 00:21:40,960 --> 00:21:47,720 Speaker 1: page