1 00:00:00,000 --> 00:00:00,760 2 00:00:00,760 --> 00:00:02,455 Let's draw a bunch of parabolic mirrors. 3 00:00:02,455 --> 00:00:04,080 And what I want to do in this video is, 4 00:00:04,080 --> 00:00:06,630 do a bunch of examples of objects 5 00:00:06,630 --> 00:00:08,140 in front of parabolic mirrors. 6 00:00:08,140 --> 00:00:10,800 And think about what the images of those objects 7 00:00:10,800 --> 00:00:14,530 will be based on how far those objects are. 8 00:00:14,530 --> 00:00:17,010 And besides just giving us a better understanding 9 00:00:17,010 --> 00:00:21,240 of parabolic mirrors, this will also, it 'll hopefully also 10 00:00:21,240 --> 00:00:23,940 give us a sense of how do we manipulate or how can we 11 00:00:23,940 --> 00:00:25,640 conceptualize these light rays? 12 00:00:25,640 --> 00:00:27,550 Which will be a pretty useful tool 13 00:00:27,550 --> 00:00:30,570 when we tackle other types of reflective or refractive 14 00:00:30,570 --> 00:00:32,509 devices like lenses. 15 00:00:32,509 --> 00:00:33,990 So that's a parabolic mirror. 16 00:00:33,990 --> 00:00:37,180 I've drawn its principal axis right over here. 17 00:00:37,180 --> 00:00:39,763 And let me just copy and paste this just so that I-- actually, 18 00:00:39,763 --> 00:00:41,180 let me draw the focal point, too. 19 00:00:41,180 --> 00:00:43,560 So this is the focus right over here. 20 00:00:43,560 --> 00:00:46,260 So let me just draw the focus right over there. 21 00:00:46,260 --> 00:00:47,950 And this is the center of curvature. 22 00:00:47,950 --> 00:00:51,450 It's twice the distance from this point as the focus. 23 00:00:51,450 --> 00:00:54,580 So that is the-- let me make it as close as possible. 24 00:00:54,580 --> 00:00:57,899 So that is the center of curvature right over there. 25 00:00:57,899 --> 00:00:59,190 And let me copy and paste this. 26 00:00:59,190 --> 00:01:01,050 So we can reuse this later on in the video. 27 00:01:01,050 --> 00:01:02,760 I don't have to keep drawing it. 28 00:01:02,760 --> 00:01:04,739 So copy it. 29 00:01:04,739 --> 00:01:06,017 So I've copied that. 30 00:01:06,017 --> 00:01:07,600 Now, let's put an object-- and I think 31 00:01:07,600 --> 00:01:08,920 we did this in the last video. 32 00:01:08,920 --> 00:01:12,660 Let's put an object beyond the center of curvature. 33 00:01:12,660 --> 00:01:13,950 So let's put an object here. 34 00:01:13,950 --> 00:01:17,510 And the convention is to use an upward pointing arrow. 35 00:01:17,510 --> 00:01:18,560 This isn't a light ray. 36 00:01:18,560 --> 00:01:19,910 It's used to show an object. 37 00:01:19,910 --> 00:01:22,290 And we use the tip of the arrow to really show 38 00:01:22,290 --> 00:01:23,450 the top of the object. 39 00:01:23,450 --> 00:01:26,737 And that's usually where we trace our light rays from. 40 00:01:26,737 --> 00:01:28,070 But it doesn't have to be there. 41 00:01:28,070 --> 00:01:28,710 We could do the middle. 42 00:01:28,710 --> 00:01:29,740 You could do the bottom. 43 00:01:29,740 --> 00:01:31,760 And you could figure out what the image of the object's 44 00:01:31,760 --> 00:01:32,390 going to be. 45 00:01:32,390 --> 00:01:33,630 So let's do that. 46 00:01:33,630 --> 00:01:36,040 And when you're dealing with parabolic mirrors, 47 00:01:36,040 --> 00:01:39,490 it's easiest to have to show just two light rays. 48 00:01:39,490 --> 00:01:41,851 One that goes parallel to the principal axis. 49 00:01:41,851 --> 00:01:43,350 And one that goes through the focus. 50 00:01:43,350 --> 00:01:45,850 Because you know what's going to happen to each of those 51 00:01:45,850 --> 00:01:46,600 when they reflect. 52 00:01:46,600 --> 00:01:48,550 And you don't have to do any math there. 53 00:01:48,550 --> 00:01:50,960 So let's have the parallel ray. 54 00:01:50,960 --> 00:01:51,970 That's the parallel ray. 55 00:01:51,970 --> 00:01:56,280 When it reflects-- the parallel incident ray, when it reflects, 56 00:01:56,280 --> 00:02:00,180 it will go through the focus. 57 00:02:00,180 --> 00:02:01,840 And then, let's have an incident ray 58 00:02:01,840 --> 00:02:03,200 that goes through the focus. 59 00:02:03,200 --> 00:02:05,990 60 00:02:05,990 --> 00:02:07,805 And when it reflects, it will be parallel. 61 00:02:07,805 --> 00:02:10,310 62 00:02:10,310 --> 00:02:13,060 And this is the example we actually saw in the last video. 63 00:02:13,060 --> 00:02:14,670 And so whatever light is being emitted 64 00:02:14,670 --> 00:02:17,020 from this point over here in that direction, 65 00:02:17,020 --> 00:02:19,830 it will come back and converge again at this point. 66 00:02:19,830 --> 00:02:22,720 And we could actually do it at every point along the-- 67 00:02:22,720 --> 00:02:24,019 we could do it halfway. 68 00:02:24,019 --> 00:02:26,310 This halfway point of the arrow, just to make it clear. 69 00:02:26,310 --> 00:02:28,640 This halfway point of the arrow, same thing. 70 00:02:28,640 --> 00:02:30,700 You have a parallel. 71 00:02:30,700 --> 00:02:34,280 Something parallel will go, will reflect a parallel incident 72 00:02:34,280 --> 00:02:36,319 ray will reflect through the focus. 73 00:02:36,319 --> 00:02:38,360 And I'll just do it for this one right over here. 74 00:02:38,360 --> 00:02:40,191 It will reflect through the focus. 75 00:02:40,191 --> 00:02:41,690 And then, if you have something that 76 00:02:41,690 --> 00:02:44,360 goes through the focus, an incident ray that 77 00:02:44,360 --> 00:02:48,840 goes through a focus, it will reflect parallel. 78 00:02:48,840 --> 00:02:51,760 So this point will correspond to this point over here. 79 00:02:51,760 --> 00:02:55,480 I think that makes it clearer, that this image, the image 80 00:02:55,480 --> 00:02:57,000 of this object when it's reflected 81 00:02:57,000 --> 00:03:02,660 by this parabolic mirror will look just like that. 82 00:03:02,660 --> 00:03:05,830 So it will actually form a real image. 83 00:03:05,830 --> 00:03:09,109 It'll form a real image that is smaller 84 00:03:09,109 --> 00:03:10,150 than this original image. 85 00:03:10,150 --> 00:03:12,260 It's not so clear, the way I did it over here. 86 00:03:12,260 --> 00:03:14,949 But you could push this even further back out. 87 00:03:14,949 --> 00:03:16,490 And it'll be clear that this is going 88 00:03:16,490 --> 00:03:19,580 to be a smaller real image than that right over there. 89 00:03:19,580 --> 00:03:21,560 Now, let's do a couple more examples. 90 00:03:21,560 --> 00:03:23,860 So let me just paste my drawing. 91 00:03:23,860 --> 00:03:25,170 So I don't have to redraw it. 92 00:03:25,170 --> 00:03:26,194 Let's see what happens. 93 00:03:26,194 --> 00:03:26,860 Let me write it. 94 00:03:26,860 --> 00:03:30,070 So here the image, just so we can keep track of things. 95 00:03:30,070 --> 00:03:39,580 Here, the image is real and smaller than the actual object 96 00:03:39,580 --> 00:03:44,110 when the actual object is beyond the center of curvature. 97 00:03:44,110 --> 00:03:47,547 And actually, let me make it a little bit clearer by drawing. 98 00:03:47,547 --> 00:03:49,880 Let me do another example like that where I do something 99 00:03:49,880 --> 00:03:52,900 big way out here just to make it clear. 100 00:03:52,900 --> 00:04:00,420 So once again, we go parallel, reflect through the focus. 101 00:04:00,420 --> 00:04:03,090 And then, we can go through the focus. 102 00:04:03,090 --> 00:04:06,882 We go through the focus and then reflect out like that. 103 00:04:06,882 --> 00:04:08,590 And there you see, now, it's much clearer 104 00:04:08,590 --> 00:04:12,010 that the image is going to be much smaller. 105 00:04:12,010 --> 00:04:16,190 And, of course, inverted relative to the actual object. 106 00:04:16,190 --> 00:04:18,490 Now, let's do this again. 107 00:04:18,490 --> 00:04:20,470 But this time, let's place the object 108 00:04:20,470 --> 00:04:22,890 at the center of curvature. 109 00:04:22,890 --> 00:04:29,090 So let's place the object right over here. 110 00:04:29,090 --> 00:04:32,010 So right at that distance that twice the distance 111 00:04:32,010 --> 00:04:35,820 from the vertex of the parabola to the focus. 112 00:04:35,820 --> 00:04:38,150 So we do a parallel line. 113 00:04:38,150 --> 00:04:39,990 These lines are the hardest thing to do. 114 00:04:39,990 --> 00:04:43,957 So parallel incident ray, parallel to the principal axis. 115 00:04:43,957 --> 00:04:45,540 This is the principal axis right here. 116 00:04:45,540 --> 00:04:49,820 Principal axis-- that's what this line is right over here. 117 00:04:49,820 --> 00:04:52,900 It's kind of the line of symmetry of the parabola. 118 00:04:52,900 --> 00:04:55,300 When it reflects, it will reflect through the focus. 119 00:04:55,300 --> 00:04:58,050 120 00:04:58,050 --> 00:05:00,330 And then, let's take another ray that goes, 121 00:05:00,330 --> 00:05:02,847 the incident ray goes through the focus. 122 00:05:02,847 --> 00:05:04,805 And when it reflects, it will reflect parallel. 123 00:05:04,805 --> 00:05:07,440 124 00:05:07,440 --> 00:05:11,140 And my drawing isn't the neatest drawing on the planet. 125 00:05:11,140 --> 00:05:14,540 And actually, let me draw it a little bit better than that. 126 00:05:14,540 --> 00:05:15,850 Well, that's pretty good. 127 00:05:15,850 --> 00:05:16,800 Let me just. 128 00:05:16,800 --> 00:05:19,620 So that's the incident ray that was parallel. 129 00:05:19,620 --> 00:05:23,860 And then, an incident ray that goes through-- 130 00:05:23,860 --> 00:05:26,375 let me-- I'm having trouble drawing these. 131 00:05:26,375 --> 00:05:28,570 An incident ray that goes through the focus 132 00:05:28,570 --> 00:05:32,120 will then come out and reflect right over there. 133 00:05:32,120 --> 00:05:33,340 And they'll converge. 134 00:05:33,340 --> 00:05:36,200 And the way I've drawn it, my drawing isn't ideal. 135 00:05:36,200 --> 00:05:39,219 But the way, but the reality is, is 136 00:05:39,219 --> 00:05:41,260 that they'll converge so that the image will just 137 00:05:41,260 --> 00:05:44,420 be in an inverted same size version as this thing up here. 138 00:05:44,420 --> 00:05:45,700 Because it's symmetric. 139 00:05:45,700 --> 00:05:47,900 Let me see if I can redraw this whole thing, 140 00:05:47,900 --> 00:05:50,020 so it comes out neater. 141 00:05:50,020 --> 00:05:51,770 So far, that looks good. 142 00:05:51,770 --> 00:05:57,450 So then, you want to reflect like that. 143 00:05:57,450 --> 00:05:59,360 You got-- you're coming through the focus. 144 00:05:59,360 --> 00:06:01,910 And then, you have another ray that goes through the focus. 145 00:06:01,910 --> 00:06:03,451 This whole thing should be symmetric. 146 00:06:03,451 --> 00:06:06,190 And then, when it reflects, it comes back out like that. 147 00:06:06,190 --> 00:06:07,800 So that makes a little bit clearer. 148 00:06:07,800 --> 00:06:09,270 So this is the object. 149 00:06:09,270 --> 00:06:11,690 And now, its image is just an inverted version 150 00:06:11,690 --> 00:06:12,430 of this object. 151 00:06:12,430 --> 00:06:17,370 The image comes into focus, or the rays 152 00:06:17,370 --> 00:06:21,670 converge at the same distance from the actual mirror 153 00:06:21,670 --> 00:06:23,470 as the actual object. 154 00:06:23,470 --> 00:06:26,110 And it's going to be the same size, just inverted. 155 00:06:26,110 --> 00:06:35,800 So that's-- so here the image is real and the same size 156 00:06:35,800 --> 00:06:37,010 as the object. 157 00:06:37,010 --> 00:06:39,300 Let's do a couple more of these. 158 00:06:39,300 --> 00:06:41,000 I think you get the hang of it. 159 00:06:41,000 --> 00:06:42,000 And you might want to try them out. 160 00:06:42,000 --> 00:06:43,374 You might want to pause the video 161 00:06:43,374 --> 00:06:46,380 and try it on paper because really nothing beats practice. 162 00:06:46,380 --> 00:06:51,720 So let's stick our object between the center of curvature 163 00:06:51,720 --> 00:06:53,966 and the focus and the focal point. 164 00:06:53,966 --> 00:06:55,340 So if we put our object there, we 165 00:06:55,340 --> 00:06:59,000 could have a light ray that goes parallel to the principal axis. 166 00:06:59,000 --> 00:07:02,020 And then, it will reflect out through the focus. 167 00:07:02,020 --> 00:07:04,810 And then, you could have another point. 168 00:07:04,810 --> 00:07:06,675 It goes through another ray. 169 00:07:06,675 --> 00:07:08,010 It goes through the focus. 170 00:07:08,010 --> 00:07:09,540 And then, it reflects. 171 00:07:09,540 --> 00:07:11,140 And then, it will reflect out. 172 00:07:11,140 --> 00:07:16,340 173 00:07:16,340 --> 00:07:17,980 And let me draw it better than that. 174 00:07:17,980 --> 00:07:20,580 Actually, this is-- I should probably 175 00:07:20,580 --> 00:07:23,470 have used a more precise tool when I did all of this. 176 00:07:23,470 --> 00:07:27,060 So let me draw it right over here. 177 00:07:27,060 --> 00:07:29,070 So I have the parallel one. 178 00:07:29,070 --> 00:07:31,360 And then, it goes through the focus 179 00:07:31,360 --> 00:07:34,936 just like that when it gets reflected. 180 00:07:34,936 --> 00:07:36,810 I really should have had a line tool for this 181 00:07:36,810 --> 00:07:38,690 to have neater drawings. 182 00:07:38,690 --> 00:07:42,840 And then, a ray that goes through the focus 183 00:07:42,840 --> 00:07:45,300 will be reflected out parallel. 184 00:07:45,300 --> 00:07:47,150 It would be reflected out parallel. 185 00:07:47,150 --> 00:07:50,820 And at least for the light that comes from that tip, 186 00:07:50,820 --> 00:07:53,120 they will re-converge at that tip. 187 00:07:53,120 --> 00:07:56,070 And if you did it for every point on this arrow, 188 00:07:56,070 --> 00:07:57,720 the image would be an inverted arrow 189 00:07:57,720 --> 00:07:59,510 that is bigger than the original. 190 00:07:59,510 --> 00:08:00,620 And it is beyond. 191 00:08:00,620 --> 00:08:03,530 It's almost the opposite of the first example that we showed. 192 00:08:03,530 --> 00:08:06,560 And so now the image is bigger than the original. 193 00:08:06,560 --> 00:08:10,140 So the image is real. 194 00:08:10,140 --> 00:08:11,820 And it is bigger. 195 00:08:11,820 --> 00:08:17,260 And the image will, where it converges 196 00:08:17,260 --> 00:08:20,494 is going to be beyond the center of curvature. 197 00:08:20,494 --> 00:08:21,410 And you could imagine. 198 00:08:21,410 --> 00:08:23,126 If this was the object right here, 199 00:08:23,126 --> 00:08:24,750 then this would be the image over here. 200 00:08:24,750 --> 00:08:26,500 If you just trace the lines backwards. 201 00:08:26,500 --> 00:08:29,470 So there's a symmetry here between this example 202 00:08:29,470 --> 00:08:31,600 and the first one we did up here. 203 00:08:31,600 --> 00:08:33,070 Now, let's just do a couple more. 204 00:08:33,070 --> 00:08:36,580 Let's imagine if the object is actually at the focal point. 205 00:08:36,580 --> 00:08:38,679 It's actually at the focus. 206 00:08:38,679 --> 00:08:40,190 So let's draw an object there. 207 00:08:40,190 --> 00:08:42,049 Let's think about what would happen. 208 00:08:42,049 --> 00:08:47,640 So if we're at the focus, a ray that comes out parallel 209 00:08:47,640 --> 00:08:53,370 will go through the focal point and come out just like that. 210 00:08:53,370 --> 00:08:56,940 And then, here we're going to-- you can't-- we can't have a ray 211 00:08:56,940 --> 00:08:57,820 that just goes. 212 00:08:57,820 --> 00:09:00,760 Well, actually we could have a ray that goes through. 213 00:09:00,760 --> 00:09:04,141 Well, that-- you can't go into the object. 214 00:09:04,141 --> 00:09:05,890 So here, I'll do a slightly different ray. 215 00:09:05,890 --> 00:09:10,100 I'll do a ray that intersects the parabolic mirror 216 00:09:10,100 --> 00:09:10,859 right over there. 217 00:09:10,859 --> 00:09:12,400 And the reason why I want to do there 218 00:09:12,400 --> 00:09:14,290 is because there the parabolic mirror 219 00:09:14,290 --> 00:09:17,070 is essentially flat and essentially vertical. 220 00:09:17,070 --> 00:09:18,770 So you can imagine that the incident 221 00:09:18,770 --> 00:09:21,411 ray is going to be the same thing as the reflected ray. 222 00:09:21,411 --> 00:09:23,410 So you could draw a ray that comes in like that. 223 00:09:23,410 --> 00:09:25,520 So this is a departure from what we did before. 224 00:09:25,520 --> 00:09:28,120 And then the reflected ray will come out like that. 225 00:09:28,120 --> 00:09:29,930 So what happens when an object is 226 00:09:29,930 --> 00:09:35,200 at the focal point is that all of the light that's coming off 227 00:09:35,200 --> 00:09:41,120 of this object in any direction will all be made, 228 00:09:41,120 --> 00:09:43,330 it will all be made parallel. 229 00:09:43,330 --> 00:09:44,990 And so it won't converge. 230 00:09:44,990 --> 00:09:46,070 So it won't converge. 231 00:09:46,070 --> 00:09:47,920 So it won't be able to form a real image. 232 00:09:47,920 --> 00:09:49,790 And it's not, it doesn't look like it's 233 00:09:49,790 --> 00:09:53,300 diverging from some point in the mirror. 234 00:09:53,300 --> 00:09:55,600 So it won't even form a virtual image. 235 00:09:55,600 --> 00:10:00,060 So here, there will actually be no image 236 00:10:00,060 --> 00:10:02,780 when the object is actually at the focal point. 237 00:10:02,780 --> 00:10:05,510 And then, the last case, as you can imagine, 238 00:10:05,510 --> 00:10:08,410 is if an object is closer than the focal point. 239 00:10:08,410 --> 00:10:09,980 So let's draw that. 240 00:10:09,980 --> 00:10:13,770 So let's put an object at the focal point. 241 00:10:13,770 --> 00:10:15,840 So right over here. 242 00:10:15,840 --> 00:10:20,060 And here, just for the sake of argument, one I can draw. 243 00:10:20,060 --> 00:10:22,040 I can always draw a parallel. 244 00:10:22,040 --> 00:10:24,200 And anything that, any light that goes parallel 245 00:10:24,200 --> 00:10:26,930 will then look to come out in a direction that 246 00:10:26,930 --> 00:10:28,750 would go through the focal point. 247 00:10:28,750 --> 00:10:30,470 So it would go through the focal point. 248 00:10:30,470 --> 00:10:32,320 It would come out in that direction. 249 00:10:32,320 --> 00:10:34,070 Although the object itself is blocking. 250 00:10:34,070 --> 00:10:36,100 But it would look to go in that direction. 251 00:10:36,100 --> 00:10:38,130 It would be reflected in that direction. 252 00:10:38,130 --> 00:10:40,120 And then, you could imagine a ray of light 253 00:10:40,120 --> 00:10:42,240 that would have been coming from the focal point, 254 00:10:42,240 --> 00:10:44,890 or would have been coming from the same direction. 255 00:10:44,890 --> 00:10:47,510 So you could imagine coming from the same direction 256 00:10:47,510 --> 00:10:50,000 as the focal point would be reflected 257 00:10:50,000 --> 00:10:51,730 parallel, in a parallel direction 258 00:10:51,730 --> 00:10:52,815 to the principal axis. 259 00:10:52,815 --> 00:10:56,060 260 00:10:56,060 --> 00:10:58,710 Now, these two light rays are not converging. 261 00:10:58,710 --> 00:11:00,400 But they look like they're diverging 262 00:11:00,400 --> 00:11:03,932 from some point behind the mirror. 263 00:11:03,932 --> 00:11:05,390 They'll look like they're diverging 264 00:11:05,390 --> 00:11:07,070 from some point behind the mirror. 265 00:11:07,070 --> 00:11:09,930 So in this case, we are forming a virtual image. 266 00:11:09,930 --> 00:11:15,352 267 00:11:15,352 --> 00:11:16,810 And the virtual image will actually 268 00:11:16,810 --> 00:11:18,510 look something like this. 269 00:11:18,510 --> 00:11:24,162 And so it'll be larger than the original virtual image. 270 00:11:24,162 --> 00:11:25,370 So it's kind of a magnifying. 271 00:11:25,370 --> 00:11:26,995 If you were to go to-- what are called? 272 00:11:26,995 --> 00:11:30,717 --a fun house at the circus or the amusement park, whatever. 273 00:11:30,717 --> 00:11:33,050 And if you were to get close enough to parabolas mirror, 274 00:11:33,050 --> 00:11:37,960 it would show a magnified version of you. 275 00:11:37,960 --> 00:11:39,067 A virtual version of you. 276 00:11:39,067 --> 00:11:41,150 And actually, let me draw that a little bit bigger 277 00:11:41,150 --> 00:11:42,750 just because it might not be clear. 278 00:11:42,750 --> 00:11:44,120 So let me draw. 279 00:11:44,120 --> 00:11:48,570 So if this is the mirror, that is the focal point. 280 00:11:48,570 --> 00:11:51,450 This right here is the principal axis. 281 00:11:51,450 --> 00:11:55,670 This is maybe you, maybe whatever object. 282 00:11:55,670 --> 00:11:57,600 You could draw a ray that goes parallel. 283 00:11:57,600 --> 00:12:00,130 It will reflect in the direction of the focal point. 284 00:12:00,130 --> 00:12:02,180 So it'll reflect out like that. 285 00:12:02,180 --> 00:12:04,397 It'll be blocked by the object, though. 286 00:12:04,397 --> 00:12:05,980 And then, something that looks like it 287 00:12:05,980 --> 00:12:07,521 would have come from the focal point, 288 00:12:07,521 --> 00:12:09,450 from the same direction as the focal point 289 00:12:09,450 --> 00:12:12,920 would then be reflected parallel to the principal axis. 290 00:12:12,920 --> 00:12:16,080 So these two rays, once again, there are diverging. 291 00:12:16,080 --> 00:12:19,390 But they look like, to the human brain, to the human eye, 292 00:12:19,390 --> 00:12:22,380 they look like they came from that point over there. 293 00:12:22,380 --> 00:12:24,690 And so this would correspond to that point 294 00:12:24,690 --> 00:12:26,070 on the virtual image. 295 00:12:26,070 --> 00:12:28,499 296 00:12:28,499 --> 00:12:30,290 So hopefully, that gives you some practice. 297 00:12:30,290 --> 00:12:32,040 But the most important thing, it gives you 298 00:12:32,040 --> 00:12:34,220 some practice dealing with these arbitrary rays 299 00:12:34,220 --> 00:12:36,986 that we're showing emanating from the tip of this arrow. 300 00:12:36,986 --> 00:12:38,610 And we could do it for the whole arrow. 301 00:12:38,610 --> 00:12:41,235 But the reason why we're picking these rays in these directions 302 00:12:41,235 --> 00:12:42,760 is that they're easy to work with. 303 00:12:42,760 --> 00:12:45,027 They go through the focus, they'll come out parallel. 304 00:12:45,027 --> 00:12:46,610 If the incident ray is parallel, it'll 305 00:12:46,610 --> 00:00:00,000 come out through the focus.