1 00:00:00,280 --> 00:00:02,840 Speaker 1: Brought to you by the reinvented two thousand twelve camera. 2 00:00:03,160 --> 00:00:06,880 Speaker 1: It's ready. Are you hey there, Text Stuff listeners, This 3 00:00:06,920 --> 00:00:09,200 Speaker 1: is Jonathan Strickland and I have got a request for 4 00:00:09,240 --> 00:00:11,440 Speaker 1: all of you. Now, Chris and I have decided that 5 00:00:11,440 --> 00:00:13,720 Speaker 1: we're going to try and experiment. We're doing our first 6 00:00:13,920 --> 00:00:17,400 Speaker 1: crowd sourced episode of tech Stuff and we want to 7 00:00:17,400 --> 00:00:21,480 Speaker 1: know what your pick is for the worst video game 8 00:00:21,720 --> 00:00:25,600 Speaker 1: of all time. Now, nominations you can. You can make 9 00:00:25,680 --> 00:00:28,479 Speaker 1: one nomination. You nominate one game, and you need to 10 00:00:28,480 --> 00:00:30,639 Speaker 1: tell us the name of the game and the platform 11 00:00:30,760 --> 00:00:32,839 Speaker 1: it was on. And it could be any platform. It 12 00:00:32,840 --> 00:00:37,000 Speaker 1: could be an arcade game, it could be a PC, Mac, Xbox, 13 00:00:37,040 --> 00:00:41,360 Speaker 1: PS three, Nintendo handheld console. It can be web based 14 00:00:41,840 --> 00:00:43,839 Speaker 1: if you like. But just you let us know what 15 00:00:43,840 --> 00:00:45,560 Speaker 1: the platform is so we can make sure we count 16 00:00:45,600 --> 00:00:49,440 Speaker 1: that as the votes. So you can nominate your game 17 00:00:49,600 --> 00:00:53,920 Speaker 1: either through email, which is tech Stuff at how stuff 18 00:00:53,920 --> 00:00:58,320 Speaker 1: works dot com, or you can nominate through Twitter or Facebook. 19 00:00:58,720 --> 00:01:01,560 Speaker 1: And we're gonna put a cut off date on this. 20 00:01:01,680 --> 00:01:03,640 Speaker 1: I want to have the episode go up by the 21 00:01:03,720 --> 00:01:07,720 Speaker 1: end of September of eleven. So let's say you need 22 00:01:07,800 --> 00:01:12,960 Speaker 1: to get your nominations in by September eleven, So if 23 00:01:12,959 --> 00:01:15,880 Speaker 1: you get those nominations into us, we will make sure 24 00:01:15,920 --> 00:01:19,240 Speaker 1: we include those in the process and we will have 25 00:01:19,280 --> 00:01:22,640 Speaker 1: an episode where we give you the worst video games 26 00:01:22,800 --> 00:01:25,800 Speaker 1: of all time based upon the votes of our listeners. 27 00:01:26,040 --> 00:01:30,840 Speaker 1: Thanks a lot. Can't wait to hear from you. Get 28 00:01:30,840 --> 00:01:34,039 Speaker 1: in touch with technology with tech Stuff from how stuff 29 00:01:34,040 --> 00:01:42,640 Speaker 1: works dot com. Hello, everyone, Welcome to tech Stuff. My 30 00:01:42,720 --> 00:01:44,560 Speaker 1: name is Chris Poet and I am an editor at 31 00:01:44,560 --> 00:01:47,760 Speaker 1: how stuff works dot com. Sitting across from me as 32 00:01:47,800 --> 00:01:51,520 Speaker 1: always and for some reason twisting up a rubber dinosaur 33 00:01:51,800 --> 00:01:55,960 Speaker 1: is senior writer Jonathan Strickland, Little Darlin, the smiles returning 34 00:01:56,000 --> 00:01:59,280 Speaker 1: to the faces, Little Darling, it seems like years since 35 00:01:59,320 --> 00:02:02,960 Speaker 1: it's been here. H. That was a nice choice for 36 00:02:03,040 --> 00:02:07,320 Speaker 1: today's topic, which is I think something that everyone will 37 00:02:07,360 --> 00:02:09,840 Speaker 1: find electrifying. Yeah, and in fact, this comes to us 38 00:02:09,840 --> 00:02:20,480 Speaker 1: courtesy of a Google Plus suggestion. This comes from Adam, 39 00:02:20,520 --> 00:02:22,600 Speaker 1: who says this may be a bit simple, but have 40 00:02:22,680 --> 00:02:25,080 Speaker 1: you guys ever done an overview of solar technology and 41 00:02:25,160 --> 00:02:28,239 Speaker 1: solar tech history? Just re listened to your battery podcast 42 00:02:28,280 --> 00:02:33,200 Speaker 1: and it made me wonder more about alternative energy sources. Adam, um, 43 00:02:33,240 --> 00:02:36,120 Speaker 1: your definition of simple and my definition of simple are 44 00:02:36,240 --> 00:02:40,240 Speaker 1: too very different things. But but yeah, we're gonna talk 45 00:02:40,240 --> 00:02:45,040 Speaker 1: about solar power, solar cells also known as photo voltaic cells, 46 00:02:45,639 --> 00:02:49,520 Speaker 1: and uh kind of where it came from. M Yeah, 47 00:02:49,560 --> 00:02:52,400 Speaker 1: they're not they're certainly not new. UM. We have an 48 00:02:52,480 --> 00:02:56,200 Speaker 1: article about how solar cells work on the website UM 49 00:02:56,280 --> 00:02:59,000 Speaker 1: which discusses how they were used in the nineteen fifties 50 00:02:59,400 --> 00:03:02,840 Speaker 1: in space uh space technology. Yeah. In fact, the well, 51 00:03:03,280 --> 00:03:06,960 Speaker 1: to go back even further, the photoelectric effect, which of 52 00:03:07,000 --> 00:03:11,720 Speaker 1: course is the basis of photovoltaic fells, that was first 53 00:03:12,160 --> 00:03:16,800 Speaker 1: discovered by a or at least first observed by a 54 00:03:16,840 --> 00:03:23,320 Speaker 1: French physicist named Edmund Beckerel. It's an eighteen thirty nine. Wow, 55 00:03:23,360 --> 00:03:26,840 Speaker 1: that was some time ago. Yeah. Now, granted he observed 56 00:03:26,880 --> 00:03:32,200 Speaker 1: that certain materials, if if exposed to sunlight, would produce 57 00:03:32,240 --> 00:03:35,360 Speaker 1: a certain amount of electric current, but there wasn't really 58 00:03:35,400 --> 00:03:38,240 Speaker 1: any way of putting that to any use at the time. 59 00:03:38,280 --> 00:03:41,720 Speaker 1: It was just it was an interesting scientific observation and 60 00:03:41,800 --> 00:03:46,360 Speaker 1: that was the the limit of it. Einstein himself began 61 00:03:46,480 --> 00:03:49,400 Speaker 1: to ruminate on this, decided about, you know, to kind 62 00:03:49,400 --> 00:03:52,080 Speaker 1: of think about what is the nature of light, how 63 00:03:52,120 --> 00:03:54,720 Speaker 1: does it interact with the nature of electricity, what's the 64 00:03:54,760 --> 00:03:58,760 Speaker 1: relationship there? Um? And then he actually won a Nobel 65 00:03:58,840 --> 00:04:04,560 Speaker 1: Prize based on his observations. Now, the first module photo 66 00:04:04,640 --> 00:04:07,280 Speaker 1: vote vol take module, because a module is a collection 67 00:04:07,440 --> 00:04:10,880 Speaker 1: of photo voltaic cells. In fact, we can get this 68 00:04:10,920 --> 00:04:13,080 Speaker 1: out of the way and really early on, if you 69 00:04:13,120 --> 00:04:15,520 Speaker 1: want to talk about like the a sense of scale, 70 00:04:16,080 --> 00:04:21,560 Speaker 1: an individual photo voltaic cell, when grouped together with other 71 00:04:21,680 --> 00:04:24,719 Speaker 1: photo voltaic cells, makes a module, and groups of modules 72 00:04:24,760 --> 00:04:28,640 Speaker 1: together make an array. So it's just it's just as 73 00:04:28,839 --> 00:04:31,120 Speaker 1: a question of scale. So array isn't a group of 74 00:04:31,120 --> 00:04:34,000 Speaker 1: modules and modules a group of photo photo voltaic cells. 75 00:04:34,120 --> 00:04:36,680 Speaker 1: I'm gonna stumble over that over and over in this episode, 76 00:04:36,720 --> 00:04:38,919 Speaker 1: so I hope you guys are listening at twice speed 77 00:04:38,960 --> 00:04:40,760 Speaker 1: so that the chipmunk is messing up over and over 78 00:04:40,760 --> 00:04:43,200 Speaker 1: and not me. Anyway. The first module was built by 79 00:04:43,240 --> 00:04:47,720 Speaker 1: Bell Laboratories, and that was in nineteen fifty four. And uh, 80 00:04:47,960 --> 00:04:50,640 Speaker 1: at that point they were thinking of it kind of 81 00:04:50,760 --> 00:04:53,520 Speaker 1: they think they called it a solar battery. They didn't 82 00:04:53,560 --> 00:04:55,920 Speaker 1: even call it a solar cell at that point, and 83 00:04:56,360 --> 00:04:59,360 Speaker 1: it was kind of considered to be an interesting idea 84 00:04:59,480 --> 00:05:03,360 Speaker 1: but not at all practical. I think they determined that 85 00:05:03,640 --> 00:05:06,719 Speaker 1: based upon the amount of work and uh it took 86 00:05:06,760 --> 00:05:11,240 Speaker 1: to develop and manufacture that first module. They were getting 87 00:05:11,279 --> 00:05:15,039 Speaker 1: about a watt for every I think it's two fifty 88 00:05:15,040 --> 00:05:19,720 Speaker 1: bucks per what, which is not efficient doesn't even compare 89 00:05:19,800 --> 00:05:24,960 Speaker 1: to other materials at all. Right, So not something that 90 00:05:24,960 --> 00:05:27,640 Speaker 1: they could implement immediately in order to to try and 91 00:05:27,680 --> 00:05:31,240 Speaker 1: generate electricity. And and then later on the fifties and 92 00:05:31,240 --> 00:05:34,600 Speaker 1: then into the sixties, really primarily in the sixties, that's 93 00:05:34,640 --> 00:05:37,840 Speaker 1: when the space industry began to use these solar cells 94 00:05:37,880 --> 00:05:42,640 Speaker 1: in order to get power for vehicles that be traveling 95 00:05:42,680 --> 00:05:47,159 Speaker 1: through space and also satellites that would be placed in 96 00:05:47,320 --> 00:05:48,919 Speaker 1: orbit around the Earth. You know, you have to have 97 00:05:49,040 --> 00:05:55,039 Speaker 1: power going to these satellites somehow, and you know, batteries 98 00:05:55,080 --> 00:05:58,360 Speaker 1: can provide power, but power batteries will die out and 99 00:05:58,400 --> 00:06:01,599 Speaker 1: there's no way of recharging easily when you can't tether 100 00:06:01,760 --> 00:06:08,159 Speaker 1: the device to the Earth. Okay, spot Nick, enough of that. Um. So, 101 00:06:08,160 --> 00:06:11,320 Speaker 1: solar cells were a way to be first for satellites 102 00:06:11,320 --> 00:06:15,640 Speaker 1: to gather power and remain in orbit functioning properly for longer. 103 00:06:16,240 --> 00:06:20,320 Speaker 1: Um Now, why are we even talking about solar power 104 00:06:20,320 --> 00:06:25,000 Speaker 1: in the first place. Well, mainly because it's abundant, and 105 00:06:25,720 --> 00:06:29,960 Speaker 1: one would imagine inexpensive. I mean, you've got about a 106 00:06:30,000 --> 00:06:33,719 Speaker 1: thousand watts of energy per square meter of the planet's surface. Yeah, 107 00:06:33,760 --> 00:06:37,279 Speaker 1: that's a lot of energy. Uh. You know, the Sun 108 00:06:37,520 --> 00:06:40,480 Speaker 1: shoots out lots of lots of energy towards the Earth. 109 00:06:40,520 --> 00:06:43,159 Speaker 1: I mean, really, the Sun shoots out lots of energy everywhere, 110 00:06:43,240 --> 00:06:46,080 Speaker 1: but we on Earth are happy to receive quite a 111 00:06:46,080 --> 00:06:49,880 Speaker 1: bit of it. Uh and we some of it gets 112 00:06:49,880 --> 00:06:52,720 Speaker 1: absorbed in the atmosphere, some of it gets absorbed by 113 00:06:52,720 --> 00:06:55,799 Speaker 1: the surface of the Earth, some of it is converted 114 00:06:55,880 --> 00:07:01,200 Speaker 1: into energy via photosynthesis by the agitation, and then the 115 00:07:01,240 --> 00:07:03,960 Speaker 1: rest of it just kind of gets reflected back off 116 00:07:04,000 --> 00:07:07,880 Speaker 1: into space. So there's all this energy that is not 117 00:07:07,960 --> 00:07:11,160 Speaker 1: being used in any meaningful way at all, and it's 118 00:07:11,240 --> 00:07:15,480 Speaker 1: just it's going away. And uh So the thought is 119 00:07:15,680 --> 00:07:18,840 Speaker 1: using solar cell technology, we could perhaps harness some of 120 00:07:18,840 --> 00:07:22,280 Speaker 1: this energy that otherwise we would just lose um. And 121 00:07:23,320 --> 00:07:29,000 Speaker 1: that's the basis behind the the push for solar energy. Now, 122 00:07:29,440 --> 00:07:32,800 Speaker 1: the engineering challenges that face us as we try to 123 00:07:33,200 --> 00:07:36,400 Speaker 1: actually harness that power are what kind of keep us 124 00:07:36,440 --> 00:07:39,920 Speaker 1: from just adopting it wholesale. That and also, I mean 125 00:07:39,920 --> 00:07:43,440 Speaker 1: there's some practical problems besides the engineering issues. Right, Like, 126 00:07:44,240 --> 00:07:46,560 Speaker 1: if you live in a place where there's not a 127 00:07:46,600 --> 00:07:49,400 Speaker 1: lot of you don't get a lot of sun, then 128 00:07:49,560 --> 00:07:51,680 Speaker 1: solar energy doesn't make a whole lot of sense. It 129 00:07:51,680 --> 00:07:54,920 Speaker 1: would be a lot it would be a heavy investment 130 00:07:55,280 --> 00:07:57,720 Speaker 1: for very little payoff. Um. Now, if you live in 131 00:07:57,720 --> 00:08:00,240 Speaker 1: a place that tends to get sun most of the error, 132 00:08:00,680 --> 00:08:05,840 Speaker 1: than solar cells make a lot more sense. Yeah. The 133 00:08:05,880 --> 00:08:10,320 Speaker 1: basics involve something that we've talked about many times in 134 00:08:10,320 --> 00:08:14,440 Speaker 1: the show. Semiconductors, which is a material that allows some 135 00:08:14,520 --> 00:08:18,720 Speaker 1: electrons to flow, but not all the available electrons to flow, 136 00:08:19,360 --> 00:08:23,640 Speaker 1: permits some flow of electricity, but not there's some control, right. 137 00:08:23,680 --> 00:08:26,640 Speaker 1: It acts somewhat like a conductor and somewhat like an insulator. 138 00:08:27,440 --> 00:08:31,200 Speaker 1: And uh and and it's the relationship between the semiconductor 139 00:08:31,280 --> 00:08:35,840 Speaker 1: and photons, which are the particles that we can you know, 140 00:08:36,400 --> 00:08:39,680 Speaker 1: units of light energy really because you talk about how 141 00:08:39,800 --> 00:08:41,440 Speaker 1: light can be both a wave and a particle, but 142 00:08:41,520 --> 00:08:44,559 Speaker 1: really talk about a photon having a certain amount of 143 00:08:44,640 --> 00:08:49,600 Speaker 1: energy um. And the energy has to be enough to 144 00:08:49,679 --> 00:08:52,600 Speaker 1: cause the semiconductor to conduct electricity. And I guess we 145 00:08:52,600 --> 00:08:56,600 Speaker 1: can get into how that works and the basis behind that, 146 00:08:57,120 --> 00:08:59,960 Speaker 1: and uh really comes down to things like a selah 147 00:09:00,040 --> 00:09:05,200 Speaker 1: common crystals. Yeah, yeah, well it's possible. I should say 148 00:09:05,360 --> 00:09:10,080 Speaker 1: upfront that it's not always silicon. That's true, silicon being 149 00:09:10,200 --> 00:09:14,679 Speaker 1: the predominant material it's used. I think for the purposes 150 00:09:14,720 --> 00:09:17,559 Speaker 1: of of this early part of the discussion, I think 151 00:09:17,559 --> 00:09:20,400 Speaker 1: we should think of the solar cells that you see 152 00:09:21,040 --> 00:09:24,280 Speaker 1: mounted on roofs and different places, because those are the 153 00:09:24,280 --> 00:09:26,560 Speaker 1: ones with which most of us are familiar. So, yeah, 154 00:09:26,760 --> 00:09:30,280 Speaker 1: the dominant semiconductor used in that as silicon. Right, So 155 00:09:30,480 --> 00:09:33,080 Speaker 1: in order to understand how the solar cells work, we're 156 00:09:33,080 --> 00:09:35,320 Speaker 1: gon we're gonna have to take a little a little 157 00:09:35,400 --> 00:09:39,439 Speaker 1: chemistry lesson here and learn more about silicon itself. So, 158 00:09:39,600 --> 00:09:43,880 Speaker 1: silicon is an atom that has fourteen electrons. Yea. There 159 00:09:43,880 --> 00:09:47,600 Speaker 1: are three different shells um and the first two are 160 00:09:47,760 --> 00:09:51,360 Speaker 1: are full. There are two and eight electrons, but uh 161 00:09:51,480 --> 00:09:55,480 Speaker 1: the outer shell has room for eight, but generally only 162 00:09:55,480 --> 00:10:00,560 Speaker 1: has four. So, uh, you know the shells case you 163 00:10:00,679 --> 00:10:04,640 Speaker 1: don't remember, the shells are essentially they represent a general 164 00:10:04,760 --> 00:10:09,040 Speaker 1: space around the nucleus of the atom where electrons are 165 00:10:09,480 --> 00:10:13,640 Speaker 1: capable of existing. And because electrons are negatively charged and 166 00:10:13,640 --> 00:10:22,079 Speaker 1: and like charge, Uh, what's the word thank you? It 167 00:10:22,280 --> 00:10:26,160 Speaker 1: just escaped repulse to repelled? Yes, that those those sometimes 168 00:10:26,160 --> 00:10:28,840 Speaker 1: they away from thank you. Yeah. I was like, I 169 00:10:28,880 --> 00:10:31,240 Speaker 1: think they don't like each other. And I was like, 170 00:10:31,400 --> 00:10:34,840 Speaker 1: that's probably not quite as sophisticated as our listeners expect, 171 00:10:34,920 --> 00:10:40,200 Speaker 1: well they expected from me. You're so so like like 172 00:10:40,360 --> 00:10:44,640 Speaker 1: charges repel one another, Thank you, Mr Palette. Without you, 173 00:10:44,760 --> 00:10:47,400 Speaker 1: I would have just been sitting here quiet and Matt 174 00:10:47,400 --> 00:10:50,360 Speaker 1: would have been snickering in the other room. Space is 175 00:10:50,400 --> 00:10:52,480 Speaker 1: getting really read. It was really entertining, you know, it 176 00:10:52,600 --> 00:10:56,040 Speaker 1: happens sometimes my brain just gives out on me. So, yes, 177 00:10:56,160 --> 00:11:00,600 Speaker 1: light getting back to it like charge repels like so, so, 178 00:11:00,960 --> 00:11:04,199 Speaker 1: these electron shells represent a space where electrons are capable 179 00:11:04,200 --> 00:11:07,200 Speaker 1: of existing, and you can't have more electrons in that 180 00:11:07,280 --> 00:11:11,840 Speaker 1: space because the negative charges would push push the electrons out. 181 00:11:12,400 --> 00:11:14,840 Speaker 1: So then the second shell, that's the one where you 182 00:11:14,840 --> 00:11:17,560 Speaker 1: can have up to eight electrons there, and then the 183 00:11:17,600 --> 00:11:20,040 Speaker 1: third shell, up to eight can exist there, but only 184 00:11:20,160 --> 00:11:23,480 Speaker 1: four are there in a in a silicon atom, So 185 00:11:24,080 --> 00:11:27,960 Speaker 1: if you you know, there's room for more electrons there. 186 00:11:28,200 --> 00:11:31,440 Speaker 1: In a way, I hesitate to use the word want 187 00:11:31,679 --> 00:11:35,360 Speaker 1: because it's just sentience. But it's it's these atoms are not, 188 00:11:35,440 --> 00:11:38,080 Speaker 1: as far as we know, sentient in any way, tend 189 00:11:38,200 --> 00:11:44,040 Speaker 1: to Yeah, they there is a a there's a tendency 190 00:11:44,160 --> 00:11:47,640 Speaker 1: for these atoms to require more electrons in that final 191 00:11:47,679 --> 00:11:51,360 Speaker 1: shell to have a full outer shell. Right, that's that's 192 00:11:51,400 --> 00:11:54,560 Speaker 1: the goal of these atoms, as if there were like 193 00:11:54,600 --> 00:11:57,880 Speaker 1: some sort of conscious goal. So, so when you get 194 00:11:57,920 --> 00:12:01,440 Speaker 1: a whole lot of silicon atoms together, they tend to 195 00:12:01,840 --> 00:12:06,959 Speaker 1: bond together, um because they begin to share electrons in 196 00:12:07,000 --> 00:12:09,280 Speaker 1: their outer shells, and so they get really really tight. 197 00:12:09,679 --> 00:12:12,640 Speaker 1: So a silicon atom will bond with four other silicon 198 00:12:12,760 --> 00:12:15,360 Speaker 1: atoms to fill up that outer shell. And each of 199 00:12:15,360 --> 00:12:18,000 Speaker 1: those silicon atoms are bonding to up with up to 200 00:12:18,120 --> 00:12:20,320 Speaker 1: four other silicon itoms to fill up their outer shell, 201 00:12:20,320 --> 00:12:23,000 Speaker 1: and this creates a crystalline structure, and they bond with 202 00:12:23,040 --> 00:12:26,679 Speaker 1: four friends and so on and so on. So, yeah, 203 00:12:26,760 --> 00:12:29,480 Speaker 1: you get this crystalline structure. Now, once you have this, 204 00:12:30,559 --> 00:12:34,640 Speaker 1: we're talking right now about a pure silicon crystalline structure, right, 205 00:12:34,760 --> 00:12:37,680 Speaker 1: So when you get all these these outer shells full 206 00:12:37,679 --> 00:12:40,880 Speaker 1: of electrons, there's a problem and that it doesn't really 207 00:12:41,600 --> 00:12:44,920 Speaker 1: conduct electricity at that point because you don't have any 208 00:12:44,960 --> 00:12:49,160 Speaker 1: free electrons, free raining electrons to uh to move through 209 00:12:49,200 --> 00:12:53,320 Speaker 1: that material. So if you introduce electricity, it's hard. It 210 00:12:53,360 --> 00:12:56,280 Speaker 1: takes a lot more energy to break the electrons out 211 00:12:56,280 --> 00:12:59,760 Speaker 1: of those bonds so that they will flow through. If 212 00:12:59,760 --> 00:13:01,040 Speaker 1: you you can do it, but you have to put 213 00:13:01,080 --> 00:13:03,360 Speaker 1: a lot of energy into the system. Yeah. What you're 214 00:13:03,360 --> 00:13:06,120 Speaker 1: looking for here is free carriers, the electrons that are 215 00:13:06,120 --> 00:13:10,160 Speaker 1: wandering around. Um. That will allow you to conduct electricity. 216 00:13:10,480 --> 00:13:13,080 Speaker 1: You know, if there are a lot of them. Um. 217 00:13:13,160 --> 00:13:16,800 Speaker 1: So what you have to do next is really dope. Yeah, yeah, 218 00:13:17,040 --> 00:13:19,360 Speaker 1: you have to dope the silicon. Now that means that 219 00:13:19,400 --> 00:13:24,520 Speaker 1: you are introducing impurities or other elder ingredients if you will, 220 00:13:24,600 --> 00:13:27,320 Speaker 1: into the silicon crystal. So you know when you think 221 00:13:27,320 --> 00:13:30,160 Speaker 1: about impurities and usually that has a negative connotation to it, 222 00:13:30,200 --> 00:13:32,760 Speaker 1: but in this case, it's something that's really necessary you 223 00:13:32,800 --> 00:13:36,600 Speaker 1: can put there. Now, there are two different routes to go, right. 224 00:13:36,679 --> 00:13:39,240 Speaker 1: You can put in atoms into You can introduce atoms 225 00:13:39,280 --> 00:13:43,120 Speaker 1: into this mixture that have more electrons in their elder 226 00:13:43,200 --> 00:13:47,840 Speaker 1: shell than silicon does. Now, that's going to introduce extra 227 00:13:47,920 --> 00:13:51,679 Speaker 1: electrons into this crystall instructures. Some electrons that are not 228 00:13:51,880 --> 00:13:54,679 Speaker 1: bonded with other atoms. So that's where you've got these 229 00:13:54,679 --> 00:13:57,720 Speaker 1: free carriers, and then it doesn't take as much energy 230 00:13:57,880 --> 00:14:00,439 Speaker 1: when you introduce energy into the system to break those 231 00:14:00,440 --> 00:14:05,680 Speaker 1: electrons free from the structure. UM, it's still requires energy 232 00:14:05,720 --> 00:14:09,840 Speaker 1: because they're the those electrons are still attracted to the um, 233 00:14:09,880 --> 00:14:14,319 Speaker 1: the positively charged nucleus, but it doesn't take as much 234 00:14:14,360 --> 00:14:17,720 Speaker 1: as if all the atoms were bonded to one another 235 00:14:18,160 --> 00:14:22,240 Speaker 1: with no free electrons. Yeah, if you used, for example, 236 00:14:22,280 --> 00:14:26,680 Speaker 1: phosphorus and uh introduced that to pure silicon, first of all, 237 00:14:26,840 --> 00:14:29,400 Speaker 1: they would really hit it off at the party. Yes. 238 00:14:30,880 --> 00:14:32,880 Speaker 1: Oh wait, I'm thinking of introducing in a totally different 239 00:14:32,880 --> 00:14:37,840 Speaker 1: way anyway. So if you dope some pure silicon with 240 00:14:38,360 --> 00:14:42,920 Speaker 1: with phosphorus um, you would add you would essentially be 241 00:14:43,000 --> 00:14:46,160 Speaker 1: adding free electrons or source of free electrons, let's say that, 242 00:14:46,480 --> 00:14:50,800 Speaker 1: and that would create an end type uh semiconductor and 243 00:14:51,040 --> 00:14:53,960 Speaker 1: meaning negative because again, electrons have a negative charge, so 244 00:14:54,040 --> 00:14:56,640 Speaker 1: you've actually got more of a negative charge than a 245 00:14:56,720 --> 00:15:00,120 Speaker 1: positive charge because you have these extra electrons. Uh. Now, now, 246 00:15:00,240 --> 00:15:03,400 Speaker 1: if you were to introduce a material that had fewer 247 00:15:03,920 --> 00:15:06,680 Speaker 1: electrons in its outer shell than silicon, you would end 248 00:15:06,800 --> 00:15:12,280 Speaker 1: up with spaces for electrons where no electrons exist. That 249 00:15:12,320 --> 00:15:15,720 Speaker 1: would be a P type of silicon, yes, because you 250 00:15:15,720 --> 00:15:18,640 Speaker 1: would have a space for electrons, but there would be 251 00:15:18,680 --> 00:15:21,400 Speaker 1: no electron to fill that space. Now, if you were 252 00:15:21,440 --> 00:15:24,400 Speaker 1: to take these two types of silicon, the N type 253 00:15:24,400 --> 00:15:27,360 Speaker 1: and the P type and put them together, then the 254 00:15:27,720 --> 00:15:30,760 Speaker 1: like the extra electrons from the N type want to 255 00:15:30,920 --> 00:15:33,960 Speaker 1: go and again want being just they tend to go 256 00:15:34,200 --> 00:15:37,640 Speaker 1: to the P type because there's a positive hole there 257 00:15:38,160 --> 00:15:40,800 Speaker 1: and you have the negative charged electrons in the N type. 258 00:15:41,040 --> 00:15:46,000 Speaker 1: So there's this immedia desire to transfer or tendency to transfer. 259 00:15:46,200 --> 00:15:51,320 Speaker 1: Chris is just laughing because I'm adding anthropomorphiz sizing electrons. Look, 260 00:15:51,760 --> 00:15:56,040 Speaker 1: some of my best friends are free carriers. Okay, hey, 261 00:15:56,120 --> 00:16:00,880 Speaker 1: let's go to the P type. Oh, man, is too early. 262 00:16:01,600 --> 00:16:03,280 Speaker 1: I didn't want to see the animated version of this. 263 00:16:03,560 --> 00:16:06,040 Speaker 1: Little know, the electrons with little faces drawn on a 264 00:16:06,120 --> 00:16:09,680 Speaker 1: big smile. Hey, so you got a hole there? I 265 00:16:09,680 --> 00:16:13,560 Speaker 1: can feel that. So the uh yeah, there's this tendency 266 00:16:13,640 --> 00:16:16,120 Speaker 1: for the electrons to move across. Well, this creates this 267 00:16:16,160 --> 00:16:19,000 Speaker 1: actually can create a barrier that acts like a diode. 268 00:16:19,280 --> 00:16:22,080 Speaker 1: And if you've listened to our Basic Electronics podcast, you 269 00:16:22,120 --> 00:16:26,320 Speaker 1: know that a diode is this channel that allows electricity 270 00:16:26,320 --> 00:16:28,880 Speaker 1: to flow one way but not back in the other 271 00:16:28,920 --> 00:16:34,560 Speaker 1: directions one way street exactly. And in this case, interestingly enough, 272 00:16:35,000 --> 00:16:38,360 Speaker 1: it will allow electrons to transfer from the PA side 273 00:16:38,400 --> 00:16:43,000 Speaker 1: to the inside, but not the other way around. Oh yeah, 274 00:16:43,160 --> 00:16:45,960 Speaker 1: so because that's not what they normally want to do, right. 275 00:16:46,560 --> 00:16:50,880 Speaker 1: So now this is where we finally get into introducing 276 00:16:50,920 --> 00:16:54,360 Speaker 1: photons into this system. All right, So you've got this, 277 00:16:54,440 --> 00:16:57,080 Speaker 1: You've got the system here where you've got this barrier 278 00:16:57,160 --> 00:16:59,920 Speaker 1: between the N type selicon and the B type cell 279 00:17:00,080 --> 00:17:03,920 Speaker 1: con and you've got the potential for electrons to move 280 00:17:04,000 --> 00:17:08,560 Speaker 1: across this barrier if you introduce energy into the system, 281 00:17:08,600 --> 00:17:12,560 Speaker 1: and the photons are that energy. So when a photon 282 00:17:13,280 --> 00:17:16,800 Speaker 1: of a proper amount of energy strikes the silicon, UH, 283 00:17:16,920 --> 00:17:20,400 Speaker 1: it can create enough energy for the electrons to transfer 284 00:17:20,440 --> 00:17:23,639 Speaker 1: across this barrier. Now, once the electrons cross cross that 285 00:17:23,680 --> 00:17:26,280 Speaker 1: barrier from the P type to the ND type UH, 286 00:17:26,320 --> 00:17:29,800 Speaker 1: they are now in a negatively charged environment, so that 287 00:17:29,960 --> 00:17:32,760 Speaker 1: the tendency is for these electrons to try and get 288 00:17:32,800 --> 00:17:35,560 Speaker 1: back to the positively charged environment, but they can't pass 289 00:17:35,640 --> 00:17:40,280 Speaker 1: that barrier. So if you were to create a pathway 290 00:17:40,320 --> 00:17:43,240 Speaker 1: from the negative side to the positive side. The electrons 291 00:17:43,280 --> 00:17:46,439 Speaker 1: would follow that pathway and do whatever it was you 292 00:17:46,480 --> 00:17:48,560 Speaker 1: wanted them to do if it meant they could get 293 00:17:48,600 --> 00:17:51,160 Speaker 1: to the positive side on the other end. So it's other. 294 00:17:51,200 --> 00:17:53,439 Speaker 1: In other words, it's like a really exclusive party and 295 00:17:53,440 --> 00:17:55,040 Speaker 1: you're like, Okay, you can come into the party, but 296 00:17:55,119 --> 00:17:59,320 Speaker 1: you gotta carry my stuff into the room with you. 297 00:17:59,600 --> 00:18:02,280 Speaker 1: And people want to get the party, You're like that totally. 298 00:18:02,359 --> 00:18:04,479 Speaker 1: The party is worth it. I will carry your stuff. 299 00:18:04,920 --> 00:18:07,360 Speaker 1: That's kind of the the analogy I'm going with here. 300 00:18:07,440 --> 00:18:09,560 Speaker 1: There's a party I want to go to tonight. Did 301 00:18:09,560 --> 00:18:13,320 Speaker 1: I mention that anyway? So, so do you do you 302 00:18:13,359 --> 00:18:17,120 Speaker 1: have to power somebody's computer to do it? No? Fortunately not. 303 00:18:17,359 --> 00:18:21,080 Speaker 1: So the electrons will do work along this pathway. And 304 00:18:21,080 --> 00:18:23,880 Speaker 1: that's just a basic circuit, right, it's a and it's 305 00:18:23,920 --> 00:18:27,160 Speaker 1: it allows current to flow. So photon hits the silicon 306 00:18:27,600 --> 00:18:29,480 Speaker 1: uh and as long as the photon has enough energy 307 00:18:29,520 --> 00:18:32,680 Speaker 1: to break that bond, the electron goes across the barrier, 308 00:18:33,080 --> 00:18:34,720 Speaker 1: wants to get back to the pea side, will go 309 00:18:34,840 --> 00:18:37,600 Speaker 1: through this pathway to get back to the peace side, 310 00:18:37,600 --> 00:18:39,600 Speaker 1: and along the way will do work. So that work 311 00:18:39,680 --> 00:18:43,280 Speaker 1: might be lighting a light bulb. That's the basic example 312 00:18:43,320 --> 00:18:48,600 Speaker 1: that you see in most uh sure drawings. So that's 313 00:18:48,680 --> 00:18:52,040 Speaker 1: that's the basic principle. Now we gotta address a couple 314 00:18:52,080 --> 00:18:55,600 Speaker 1: of other minor points to actually play a big role 315 00:18:55,680 --> 00:18:58,639 Speaker 1: in in y solar cells work and why they aren't 316 00:18:58,680 --> 00:19:02,359 Speaker 1: as um why we don't see them everywhere right now, Yeah, 317 00:19:02,520 --> 00:19:05,520 Speaker 1: you mean, like, um, the fact that, well there are 318 00:19:05,560 --> 00:19:10,440 Speaker 1: other components to the solar cells to sure how light 319 00:19:10,520 --> 00:19:14,320 Speaker 1: bounces off stuff like silicon. Right, Silicon tends to be 320 00:19:14,400 --> 00:19:16,720 Speaker 1: very shiny, which means that some photons when they strike 321 00:19:16,800 --> 00:19:18,760 Speaker 1: the surface are just going to reflect off and not 322 00:19:18,800 --> 00:19:21,560 Speaker 1: get absorbed at all, which is a problem. If you're 323 00:19:21,560 --> 00:19:25,120 Speaker 1: not absorbing the energy, then you cannot, um, you don't 324 00:19:25,119 --> 00:19:27,320 Speaker 1: have enough energy for the electrons to break free by 325 00:19:27,320 --> 00:19:30,080 Speaker 1: the way, that that we call that the band gap energy, 326 00:19:30,200 --> 00:19:33,720 Speaker 1: to to break free of that that final electron shell. 327 00:19:34,119 --> 00:19:37,240 Speaker 1: So one problem is that not all photons have the 328 00:19:37,280 --> 00:19:40,760 Speaker 1: same amount of energy because light comes in a variety 329 00:19:40,920 --> 00:19:45,080 Speaker 1: of forms. You know, we talked about the spectrum of light. 330 00:19:45,160 --> 00:19:47,000 Speaker 1: So you know, you can see light like visible light 331 00:19:47,119 --> 00:19:50,080 Speaker 1: and has a pretty wide spectrum, but even beyond that 332 00:19:50,320 --> 00:19:54,879 Speaker 1: is an even wider spectrum infrared light, ultraviolet light, and 333 00:19:54,880 --> 00:19:56,800 Speaker 1: then you know of course all the different colors. Well, 334 00:19:56,840 --> 00:20:01,399 Speaker 1: each of those types of of light have a different 335 00:20:01,400 --> 00:20:04,600 Speaker 1: amount of energy, and if the energy is not sufficient 336 00:20:05,040 --> 00:20:08,840 Speaker 1: to UH to overcome the band gap energy, the electron 337 00:20:08,880 --> 00:20:12,840 Speaker 1: is not going anywhere. So if the energy is more 338 00:20:13,200 --> 00:20:16,480 Speaker 1: than what the band gap needs, that electron will move, 339 00:20:16,520 --> 00:20:20,000 Speaker 1: but some of that energy is wasted. Like for example, 340 00:20:20,040 --> 00:20:21,840 Speaker 1: if I need if I can lift a hundred and 341 00:20:21,880 --> 00:20:25,800 Speaker 1: ten pounds and there's a weight in front of me 342 00:20:25,840 --> 00:20:28,000 Speaker 1: that's a hundred pounds, I can lift that up. But 343 00:20:28,040 --> 00:20:30,000 Speaker 1: if there are two weights that are a hundred pounds, 344 00:20:30,080 --> 00:20:31,879 Speaker 1: I'm still only gonna be able to lift one up. 345 00:20:31,880 --> 00:20:34,399 Speaker 1: Even though I'm capable of lifting over a hundred pounds, 346 00:20:34,440 --> 00:20:38,440 Speaker 1: I'm not capable of lifting two hundred pounds. So if 347 00:20:38,480 --> 00:20:41,320 Speaker 1: you get a photon that actually has say twice as 348 00:20:41,400 --> 00:20:43,680 Speaker 1: much energy as the band gap energy, then you could 349 00:20:43,720 --> 00:20:50,520 Speaker 1: actually move to electrons per photon UM. So that's another problem. 350 00:20:50,600 --> 00:20:53,800 Speaker 1: So how do we get past the reflective problem? Well, 351 00:20:54,040 --> 00:20:56,880 Speaker 1: usually they get around it by putting on some kind 352 00:20:56,880 --> 00:21:00,959 Speaker 1: of material that is an anti reflective property, um, just 353 00:21:01,000 --> 00:21:05,640 Speaker 1: to keep the photons from bouncing away UM. And that 354 00:21:05,640 --> 00:21:07,199 Speaker 1: that's one thing they have to do. They also have 355 00:21:07,280 --> 00:21:10,080 Speaker 1: to put a cover plate on it, you know, glass, 356 00:21:10,200 --> 00:21:14,840 Speaker 1: essentially to keep the solar cell from being damaged. Because 357 00:21:15,040 --> 00:21:17,520 Speaker 1: again we were talking about the solar cells that you 358 00:21:17,560 --> 00:21:21,600 Speaker 1: see the arrays that you see in on rooftops and 359 00:21:21,960 --> 00:21:24,639 Speaker 1: um and for in some instances on the side of 360 00:21:24,640 --> 00:21:26,000 Speaker 1: the I see a lot of them on the side 361 00:21:26,000 --> 00:21:30,560 Speaker 1: of the road where they have some kind of equipment there, um, 362 00:21:30,600 --> 00:21:32,560 Speaker 1: you know, a sign or something that they want to 363 00:21:32,680 --> 00:21:36,680 Speaker 1: use to uh, you know, to provide messages to people 364 00:21:36,680 --> 00:21:38,919 Speaker 1: who are traveling on the roadway. They'll have a giant 365 00:21:39,119 --> 00:21:41,159 Speaker 1: or not a giant, but a large solar panel out 366 00:21:41,200 --> 00:21:43,720 Speaker 1: there to help power the sign. Um. You know, that's 367 00:21:43,720 --> 00:21:46,040 Speaker 1: sitting out there all the time, so you know, you 368 00:21:46,040 --> 00:21:48,240 Speaker 1: don't want it to be damaged by the rain or 369 00:21:48,760 --> 00:21:51,560 Speaker 1: or anything. Um, So you know, you have to have 370 00:21:51,600 --> 00:21:54,560 Speaker 1: these other things that are they're going on. But unfortunately, 371 00:21:55,440 --> 00:21:59,360 Speaker 1: these uh, these solar cells are not particularly efficient. Yeah, 372 00:21:59,400 --> 00:22:02,919 Speaker 1: there's actually there's several reasons why efficiency is a problem. 373 00:22:03,000 --> 00:22:04,840 Speaker 1: One of those is, you know, I mentioned the whole 374 00:22:04,880 --> 00:22:10,200 Speaker 1: band gap energy problem. Whereas one temptation would be to 375 00:22:10,240 --> 00:22:12,639 Speaker 1: build a solar cell that be able to gather as 376 00:22:12,640 --> 00:22:15,119 Speaker 1: many photons as possible. In other words, aim for the 377 00:22:15,160 --> 00:22:18,760 Speaker 1: lowest common denominator, like create material that's going to have 378 00:22:18,880 --> 00:22:24,000 Speaker 1: the lowest band gap energy, so that even weak photons 379 00:22:24,880 --> 00:22:28,080 Speaker 1: would be able to make electrons flow. Well, here's the 380 00:22:28,119 --> 00:22:32,400 Speaker 1: problem with that. Current is that would be the number 381 00:22:32,400 --> 00:22:35,520 Speaker 1: of electrons that move through a system. Right, But there's 382 00:22:35,520 --> 00:22:39,520 Speaker 1: another element called voltage, and and voltage is more like 383 00:22:40,040 --> 00:22:41,760 Speaker 1: if you want to think of it in terms of plumbing, 384 00:22:41,800 --> 00:22:44,800 Speaker 1: voltage would be the pressure and current would be the 385 00:22:44,800 --> 00:22:50,280 Speaker 1: amount of water um. So voltage and current together, When 386 00:22:50,320 --> 00:22:52,760 Speaker 1: you combine the two together, you get power. That's the 387 00:22:52,800 --> 00:22:56,280 Speaker 1: product of current and voltage. So you mustapply the two 388 00:22:56,280 --> 00:22:59,200 Speaker 1: and you get power. So the power from any system 389 00:22:59,240 --> 00:23:01,200 Speaker 1: is going to be dependent upon the current and the voltage. 390 00:23:01,240 --> 00:23:05,040 Speaker 1: If you use material that has a low band gap energy, 391 00:23:05,800 --> 00:23:09,440 Speaker 1: you get a lower voltage in that system, so you've 392 00:23:09,480 --> 00:23:12,320 Speaker 1: actually decreased the voltage. So the current increases, but the 393 00:23:12,359 --> 00:23:17,359 Speaker 1: voltage decreases, so the product does not necessarily become enough 394 00:23:17,400 --> 00:23:20,400 Speaker 1: for it to be a good return on investment. So, 395 00:23:20,720 --> 00:23:23,360 Speaker 1: in other words, you could create something that creates has 396 00:23:23,400 --> 00:23:26,320 Speaker 1: more current but a lower voltage, the power is less. 397 00:23:26,560 --> 00:23:28,640 Speaker 1: It does it doesn't do as much work as say, 398 00:23:28,880 --> 00:23:31,520 Speaker 1: materials that have a higher band gap energy, even though 399 00:23:31,600 --> 00:23:34,600 Speaker 1: you've even though you are discounting more photons in that 400 00:23:34,720 --> 00:23:37,359 Speaker 1: in that other system, the photons that are hitting are 401 00:23:37,400 --> 00:23:42,080 Speaker 1: producing more energy. UM. So that's one issue. Although you 402 00:23:42,119 --> 00:23:44,960 Speaker 1: can kind of work around that in a way. You 403 00:23:45,000 --> 00:23:50,320 Speaker 1: can create a multi junction cell. And a multijunction cell 404 00:23:50,960 --> 00:23:53,159 Speaker 1: is uh. You can think of that as layers of 405 00:23:53,200 --> 00:23:56,880 Speaker 1: cells on top of one another, and one layer has 406 00:23:56,960 --> 00:23:59,520 Speaker 1: a certain band gap energy, and then the next one 407 00:23:59,600 --> 00:24:02,119 Speaker 1: has a different band gap energy, and the next one 408 00:24:02,160 --> 00:24:05,040 Speaker 1: has yet another band gap energy. In order to capture 409 00:24:05,040 --> 00:24:07,520 Speaker 1: as many of these photons as possible, and that will 410 00:24:07,560 --> 00:24:09,280 Speaker 1: help a little bit. So that's one way you can 411 00:24:09,320 --> 00:24:10,840 Speaker 1: do it. It's a very expensive thing to do, but 412 00:24:10,960 --> 00:24:13,119 Speaker 1: NASA has been doing it for years. That's that's what 413 00:24:13,240 --> 00:24:17,080 Speaker 1: NASA solar cells tend to be, our multi junction cells 414 00:24:17,119 --> 00:24:19,640 Speaker 1: because you know, you want to you want the satellites 415 00:24:19,680 --> 00:24:23,119 Speaker 1: to last a really long time so um, and you 416 00:24:23,160 --> 00:24:26,280 Speaker 1: want them to be very efficient. But that's one problem 417 00:24:26,280 --> 00:24:30,840 Speaker 1: with efficiency. Another is just the design of the solar 418 00:24:30,840 --> 00:24:33,800 Speaker 1: cells themselves. In order for these electrons to hit a 419 00:24:33,840 --> 00:24:36,199 Speaker 1: pathway a circuit, you know, they have to they have, 420 00:24:36,280 --> 00:24:40,440 Speaker 1: you have to create that pathway for them, and that 421 00:24:40,520 --> 00:24:43,480 Speaker 1: raises some challenges. Where do you put how do you 422 00:24:43,480 --> 00:24:46,760 Speaker 1: create this pathway the top of the solar cell. It's 423 00:24:46,760 --> 00:24:48,879 Speaker 1: hard to make a conductive layer, right, because I mean 424 00:24:49,000 --> 00:24:52,080 Speaker 1: usually we tend to use metal. Metal is a good conductor. 425 00:24:52,160 --> 00:24:55,480 Speaker 1: Most metals are good conductors. Yeah, and the series resistance 426 00:24:56,320 --> 00:24:59,480 Speaker 1: of silicon is so high that it causes a lot 427 00:24:59,480 --> 00:25:01,959 Speaker 1: of loss. Mean, if you're using something like copper, right, 428 00:25:01,960 --> 00:25:04,040 Speaker 1: it would do great. Yeah, but copper doesn't have that 429 00:25:04,040 --> 00:25:09,159 Speaker 1: photovoltaic quality. There's the problem. So if you're using metal 430 00:25:09,200 --> 00:25:12,720 Speaker 1: to conduct the electricity, to act as the circuit, to 431 00:25:12,760 --> 00:25:18,280 Speaker 1: act as the pathway for these electrons, um, the question is, well, 432 00:25:18,520 --> 00:25:20,880 Speaker 1: you can't really, you can't encase it in metal because 433 00:25:20,880 --> 00:25:23,120 Speaker 1: if you did, then no photons would get through. There 434 00:25:23,119 --> 00:25:25,439 Speaker 1: has to be at least one side open. You know, 435 00:25:25,520 --> 00:25:29,320 Speaker 1: you can create some conductive material that is, uh, you can, 436 00:25:29,400 --> 00:25:32,560 Speaker 1: you can weave through the glass. But there's also a 437 00:25:32,600 --> 00:25:36,640 Speaker 1: concern that you know, photons are these tiny, tiny, tiny particles, 438 00:25:37,200 --> 00:25:41,040 Speaker 1: and even the thinnest metal material that might make up 439 00:25:41,080 --> 00:25:45,040 Speaker 1: a grid in a solar module, for example, will block 440 00:25:45,240 --> 00:25:50,240 Speaker 1: some electron photons. Rather which means that you're losing efficiency 441 00:25:50,320 --> 00:25:53,800 Speaker 1: that way. So that's that's one of the reasons why 442 00:25:53,840 --> 00:25:57,000 Speaker 1: solar panels can have problems with efficiency is that just 443 00:25:57,160 --> 00:26:00,960 Speaker 1: based on the design itself, in order to conduct those 444 00:26:00,960 --> 00:26:07,080 Speaker 1: electrons and provide electricity, you're blocking off some of the photons. 445 00:26:07,280 --> 00:26:09,560 Speaker 1: So you're never going to get a hundred percent efficiency 446 00:26:09,600 --> 00:26:13,160 Speaker 1: because just based on the technology itself, it's blocking its 447 00:26:13,200 --> 00:26:21,720 Speaker 1: own source of power. That's frustrating. Photons just shake. Yeah, 448 00:26:22,240 --> 00:26:26,480 Speaker 1: So they've been working on trying other types of materials, uh, 449 00:26:26,640 --> 00:26:30,000 Speaker 1: stuff like a morphous silicon, cadmium tell your ide and 450 00:26:30,119 --> 00:26:34,920 Speaker 1: copper iridium, gallium decelenide. Had some of that the other day. 451 00:26:34,960 --> 00:26:39,400 Speaker 1: It was delish, But yeah, I mean these are using 452 00:26:39,440 --> 00:26:42,680 Speaker 1: these materials, uh, you know, they've they've been trying to 453 00:26:42,760 --> 00:26:46,760 Speaker 1: find some advantages. One of those is that with some 454 00:26:46,800 --> 00:26:50,040 Speaker 1: of those materials you can create a thinner material, a 455 00:26:50,040 --> 00:26:53,240 Speaker 1: thinner panel or thinnel thinner cell, and they call them 456 00:26:53,240 --> 00:26:57,560 Speaker 1: thin film solar cells. And basically, yeah, these are very 457 00:26:57,600 --> 00:27:00,800 Speaker 1: neat because, um, a lot of the again the arrays 458 00:27:00,800 --> 00:27:05,040 Speaker 1: that we had in our initial example are pretty solid. 459 00:27:05,520 --> 00:27:09,080 Speaker 1: They don't they don't bend, and the thin film solar cells. Yes, 460 00:27:09,080 --> 00:27:12,919 Speaker 1: they do break, but um. Actually a couple of companies 461 00:27:12,920 --> 00:27:17,720 Speaker 1: have found ways to print thin film solar cells by 462 00:27:17,800 --> 00:27:22,920 Speaker 1: spraying and and ink made with these materials onto foil UM, 463 00:27:22,960 --> 00:27:25,879 Speaker 1: which is really cool because uh, it enables it to 464 00:27:25,920 --> 00:27:29,239 Speaker 1: be somewhat flexible, and you can use it in places, uh, 465 00:27:29,359 --> 00:27:32,040 Speaker 1: these types of solar cells in ways that you wouldn't 466 00:27:32,119 --> 00:27:35,679 Speaker 1: be able to otherwise. UM. Really you could see something 467 00:27:35,800 --> 00:27:40,880 Speaker 1: like this on a handheld calculator because those solar cells, 468 00:27:41,160 --> 00:27:44,360 Speaker 1: you know, the little itty bitty ones um, are thinner 469 00:27:44,720 --> 00:27:47,480 Speaker 1: than the ones that you see on on rooftops and 470 00:27:47,520 --> 00:27:51,200 Speaker 1: in different places like that. UM. The thing is they 471 00:27:52,760 --> 00:27:58,680 Speaker 1: they're about fifty efficient at maximum UM, which is more 472 00:27:58,760 --> 00:28:03,399 Speaker 1: likely to be more like fifty efficient UM, which is 473 00:28:03,440 --> 00:28:07,440 Speaker 1: of course also south of the efficiency that they strive 474 00:28:07,520 --> 00:28:10,960 Speaker 1: for with the uh, the silicon based wafer cells, the 475 00:28:11,040 --> 00:28:15,520 Speaker 1: hard cells. So you know, it's it's they're getting to 476 00:28:15,640 --> 00:28:18,239 Speaker 1: be more of a reality. This is something that's been 477 00:28:18,240 --> 00:28:22,080 Speaker 1: in development for several years now, UM, and they're you're 478 00:28:22,080 --> 00:28:25,320 Speaker 1: seeing them in more places. But they also have their drawbacks, 479 00:28:25,920 --> 00:28:27,919 Speaker 1: you know, and you know there are other drawbacks with 480 00:28:27,960 --> 00:28:30,520 Speaker 1: solar panels as well. The efficiency is a big one, 481 00:28:30,600 --> 00:28:35,720 Speaker 1: because the less efficient a solar array is, the more 482 00:28:36,280 --> 00:28:38,360 Speaker 1: cells you're going to need in order to generate the 483 00:28:38,360 --> 00:28:43,080 Speaker 1: electricity you want. Right you and in general big areas 484 00:28:43,120 --> 00:28:45,480 Speaker 1: to get a lot of sun. That's that's your prime 485 00:28:46,280 --> 00:28:51,080 Speaker 1: target for any sort of solar power facility. Um, you know, 486 00:28:51,120 --> 00:28:55,360 Speaker 1: it's it's one thing to put solar cells over the 487 00:28:55,400 --> 00:28:58,440 Speaker 1: roof of your house, is very difficult to generate enough 488 00:28:58,440 --> 00:29:03,440 Speaker 1: power to actually uh be completely subsist just on on 489 00:29:03,480 --> 00:29:06,120 Speaker 1: solar power. For one thing, if you're if it's if 490 00:29:06,160 --> 00:29:08,320 Speaker 1: you're using the power as soon as it's generated, then 491 00:29:08,320 --> 00:29:10,080 Speaker 1: you're only going to be able to use power during 492 00:29:10,080 --> 00:29:12,440 Speaker 1: the day and on a sunny day at that, right, 493 00:29:12,480 --> 00:29:14,760 Speaker 1: So you're gonna have to have batteries, some sort of 494 00:29:14,800 --> 00:29:18,760 Speaker 1: storage medium in order to h to store power and 495 00:29:18,840 --> 00:29:21,800 Speaker 1: use it later. And just frankly, I don't think there 496 00:29:21,840 --> 00:29:25,120 Speaker 1: are that many houses that are have enough efficient solar 497 00:29:25,160 --> 00:29:30,040 Speaker 1: panels to just rely on solar energy and battery backup. Now, 498 00:29:30,120 --> 00:29:34,000 Speaker 1: there are some and in fact, I've I've heard stories 499 00:29:34,040 --> 00:29:36,840 Speaker 1: about people who are still connected to the electricity grid 500 00:29:36,880 --> 00:29:41,760 Speaker 1: who are using solar power predominantly in their houses and um, 501 00:29:41,880 --> 00:29:44,719 Speaker 1: and in some cases if they generate more electricity than 502 00:29:44,760 --> 00:29:49,200 Speaker 1: they are consuming, they can actually feed energy back into 503 00:29:49,240 --> 00:29:52,520 Speaker 1: the grid and their power company will compensate them for 504 00:29:52,560 --> 00:29:56,160 Speaker 1: that much. Is a nice benefit, especially because these solar 505 00:29:56,280 --> 00:29:59,560 Speaker 1: arrays can be very expensive to install, right And usually 506 00:29:59,560 --> 00:30:02,560 Speaker 1: that only I mean, if you are in the right 507 00:30:02,680 --> 00:30:04,880 Speaker 1: area and you've got the right kind of solar cells, 508 00:30:04,920 --> 00:30:07,520 Speaker 1: then you may actually make enough where you're making money 509 00:30:07,560 --> 00:30:10,840 Speaker 1: from the power company. But more often it's a reduction 510 00:30:10,920 --> 00:30:13,040 Speaker 1: in your power bill. Like, first of all, your power 511 00:30:13,040 --> 00:30:14,720 Speaker 1: bill is not gonna be that high anyway, because you're 512 00:30:14,720 --> 00:30:18,240 Speaker 1: mostly relying on the solar cells and the power company 513 00:30:18,320 --> 00:30:22,760 Speaker 1: is providing whatever amount left over you require. But then 514 00:30:22,760 --> 00:30:26,000 Speaker 1: occasionally you produce more than what you need, uh, so 515 00:30:26,040 --> 00:30:28,240 Speaker 1: your bill will just be lower at the end. Yeah, 516 00:30:28,320 --> 00:30:31,240 Speaker 1: it's not like your you can recoup your investment overnight 517 00:30:31,480 --> 00:30:34,560 Speaker 1: or over sunny day, right especially. Yeah, and if you 518 00:30:34,600 --> 00:30:38,000 Speaker 1: happen to have a stretch of time where it's just 519 00:30:38,200 --> 00:30:41,080 Speaker 1: overcast day after day after day, then that those are 520 00:30:41,120 --> 00:30:43,920 Speaker 1: days when you're not really gonna be producing that much power. Um. 521 00:30:44,040 --> 00:30:46,760 Speaker 1: Not to say that it isn't worthwhile, no, but it 522 00:30:47,000 --> 00:30:49,600 Speaker 1: you know, don't expect you know, to make it back 523 00:30:49,680 --> 00:30:55,880 Speaker 1: up immediately. And another difficulty is that some depending on 524 00:30:55,920 --> 00:30:58,040 Speaker 1: the materials that are going into those solar panels, they 525 00:30:58,040 --> 00:31:02,520 Speaker 1: may or may not be either rare earth metals, which 526 00:31:02,680 --> 00:31:05,040 Speaker 1: there there's a whole host of problems. We if you've 527 00:31:05,040 --> 00:31:09,280 Speaker 1: heard O our podcast on rare earth materials, then you 528 00:31:09,320 --> 00:31:11,600 Speaker 1: know you know that that has its own host of 529 00:31:11,720 --> 00:31:15,600 Speaker 1: issues as well. Uh. There's also the possibility of depending 530 00:31:15,600 --> 00:31:17,959 Speaker 1: on again on the material in the solar cell, there 531 00:31:18,000 --> 00:31:21,040 Speaker 1: may be very toxic material in there, or material that 532 00:31:21,080 --> 00:31:24,440 Speaker 1: may not it'sself be toxic, but the manufacturing process of 533 00:31:24,480 --> 00:31:29,920 Speaker 1: that material itself produces toxic toxic materials. So there is 534 00:31:30,000 --> 00:31:34,600 Speaker 1: the potential for solar power to do environmental harm indirectly. 535 00:31:35,000 --> 00:31:39,640 Speaker 1: You know, the actual production of electricity isn't environmentally destructive, 536 00:31:39,960 --> 00:31:44,600 Speaker 1: but the process of building those solar panels itself maybe. 537 00:31:45,200 --> 00:31:47,520 Speaker 1: So you have to look at the big picture and 538 00:31:47,560 --> 00:31:51,160 Speaker 1: the full impact of the system. You can't just look 539 00:31:51,200 --> 00:31:53,200 Speaker 1: at Hey, you know, I'm getting energy from the sun. 540 00:31:53,320 --> 00:31:57,440 Speaker 1: I'm not burning any fossil fuels. Uh, this is clean energy. 541 00:31:57,680 --> 00:32:00,880 Speaker 1: Everything's hunky dorry. You have to look beyond that in 542 00:32:01,000 --> 00:32:05,280 Speaker 1: order to really consider the impact of the system. Yeah, 543 00:32:05,360 --> 00:32:08,240 Speaker 1: which you know that mean eventually get to a point 544 00:32:08,280 --> 00:32:09,960 Speaker 1: where you're looking at it from such a big picture 545 00:32:10,080 --> 00:32:15,400 Speaker 1: that you're thinking there's no solutions out there. Goodnight kids. Well, 546 00:32:15,440 --> 00:32:17,800 Speaker 1: I think, uh, well, we've sort of talked about it 547 00:32:17,840 --> 00:32:21,280 Speaker 1: another podcast to like the bloom Box and other other things. 548 00:32:21,280 --> 00:32:23,800 Speaker 1: But yeah, I mean it's it's one of those things 549 00:32:23,800 --> 00:32:26,480 Speaker 1: where in the long run, I think it's a it's 550 00:32:26,480 --> 00:32:29,200 Speaker 1: gonna end up being a combination of solutions, you know, 551 00:32:29,320 --> 00:32:33,360 Speaker 1: to get off of fossil fuels, rather than just a single, uh, 552 00:32:33,520 --> 00:32:36,280 Speaker 1: you know, single one. I think it will probably involve 553 00:32:36,320 --> 00:32:39,280 Speaker 1: jackostile terriers on a treadmill. It might, and it might 554 00:32:39,400 --> 00:32:41,560 Speaker 1: very well, because as far as I can tell, they 555 00:32:41,560 --> 00:32:45,360 Speaker 1: have an inexhaustible supply of energy. Yeah, especially if you 556 00:32:45,480 --> 00:32:47,720 Speaker 1: if you, you know, have a treat at the end 557 00:32:47,760 --> 00:32:52,880 Speaker 1: of the the little conveyor belt, they'll just run, run, run, anyway, 558 00:32:53,120 --> 00:32:55,400 Speaker 1: that's neither here nor there. Well, that was a great 559 00:32:55,440 --> 00:32:59,480 Speaker 1: discussion about solar panel technology. I hope that answered your question, Adam. Uh, 560 00:32:59,600 --> 00:33:03,800 Speaker 1: it was a fun things topic to cover and uh, well, 561 00:33:04,240 --> 00:33:06,640 Speaker 1: if you guys have suggestions for topics that you would 562 00:33:06,680 --> 00:33:09,360 Speaker 1: like us to talk about, feel free to let us know. 563 00:33:09,680 --> 00:33:12,960 Speaker 1: You can contact us on Twitter or Facebook. Our handle 564 00:33:13,040 --> 00:33:16,760 Speaker 1: at both of those is text Stuff hs W. Or 565 00:33:16,840 --> 00:33:19,080 Speaker 1: you can send us an email and that address is 566 00:33:19,360 --> 00:33:22,760 Speaker 1: text Stuff at how stuff Works dot com and Chris 567 00:33:22,800 --> 00:33:27,240 Speaker 1: and I will talk to you again really soon. Be 568 00:33:27,360 --> 00:33:29,960 Speaker 1: sure to check out our new video podcast, Stuff from 569 00:33:30,000 --> 00:33:32,840 Speaker 1: the Future. Join how Stuff Work staff as we explore 570 00:33:32,880 --> 00:33:37,440 Speaker 1: the most promising and perplexing possibilities of tomorrow. The How 571 00:33:37,480 --> 00:33:41,240 Speaker 1: Stuff Works iPhone app has arrived. Download it today on iTunes, 572 00:33:45,800 --> 00:33:48,400 Speaker 1: brought to you by the reinvented two thousand twelve camera. 573 00:33:48,720 --> 00:33:49,880 Speaker 1: It's ready, are you