1 00:00:00,010 --> 00:00:04,170 Like we did with parabolic mirrors, what I really want to do in this video 2 00:00:04,210 --> 00:00:09,800 is just for put objects at different distances relative to this convex lens 3 00:00:10,040 --> 00:00:12,920 and just think about what its image will look like 4 00:00:12,920 --> 00:00:16,950 And the whole point of doing that is going through all the different situations but 5 00:00:16,960 --> 00:00:19,990 more is getting practice of how to think about it 6 00:00:19,990 --> 00:00:23,340 So let's first put an object out here 7 00:00:23,510 --> 00:00:28,540 That's more than two focal lengths away from the lens 8 00:00:28,540 --> 00:00:30,720 I'll put the object right here 9 00:00:30,760 --> 00:00:32,670 We'll do our classic arrow 10 00:00:32,770 --> 00:00:37,280 Actually I'll make a point here. When we dealt with parabolic mirrors 11 00:00:37,290 --> 00:00:42,100 we talked about the distance of two focal lengths being our center of curvature 12 00:00:42,180 --> 00:00:45,480 Over here we're just gonna call it 2 focal length, because it's really not 13 00:00:45,480 --> 00:00:47,540 the center of curvature-- 14 00:00:47,550 --> 00:00:51,020 or this distance really isn't the radius of curvature of 15 00:00:51,040 --> 00:00:53,640 each of these curves. So we're just gonna call it 2 focal lengths 16 00:00:53,950 --> 00:00:59,150 So with that said, let's actually try to figure out what the image of this thing would look like 17 00:00:59,150 --> 00:01:02,710 as the light from it gets refracted through this lens 18 00:01:02,710 --> 00:01:06,390 So like always, it's useful to draw one ray 19 00:01:06,490 --> 00:01:10,690 Every point of this object is emitting rays in every direction 20 00:01:10,690 --> 00:01:12,830 because it's diffusely reflecting light 21 00:01:12,850 --> 00:01:15,320 So we can just pick rays that are convenient 22 00:01:15,320 --> 00:01:17,280 So we can go from the tip of the arrow 23 00:01:17,290 --> 00:01:22,360 and go parallel to our principal axis just like that 24 00:01:22,440 --> 00:01:26,470 I'm not gonna show all the internal refraction within this lens right here 25 00:01:26,600 --> 00:01:31,270 But we know that if we enter the lens, parallel to the principal axis 26 00:01:31,270 --> 00:01:41,630 when we get refracted, we will go through the focal point on the other side of the lens 27 00:01:41,990 --> 00:01:45,100 And on the left side of the lens 28 00:01:45,100 --> 00:01:48,340 we'll do another ray that goes through the focal point on the left side 29 00:01:48,340 --> 00:01:59,770 and then comes out parallel 30 00:02:00,190 --> 00:02:04,530 The incident ray goes through the left focal point 31 00:02:04,700 --> 00:02:10,710 and when it gets refracted, it will now be parallel 32 00:02:10,789 --> 00:02:18,790 And so the light that came from that point of the object will reconverge right over here 33 00:02:18,840 --> 00:02:21,530 So if you did this for every point of this object 34 00:02:21,530 --> 00:02:25,310 if you did a point in the middle right over here, it would reconverge right over here 35 00:02:25,350 --> 00:02:30,100 If you did this point right over here, it would reconverge right over there 36 00:02:30,100 --> 00:02:38,170 So the image of this object is going to look like this 37 00:02:38,190 --> 00:02:46,220 So it's going to be a real image. The rays actually converge here. So it's a real inverted image 38 00:02:46,230 --> 00:02:48,980 It was pointing up before. Now it's pointing that down 39 00:02:48,980 --> 00:02:53,370 And in this situation, it's actually going to be smaller than the original 40 00:02:53,490 --> 00:02:57,700 So, real, smaller, inverted image 41 00:02:57,700 --> 00:03:00,270 Let's do a couple of other scenarios 42 00:03:00,390 --> 00:03:05,580 Let me copy and paste this before starting this video to save on time 43 00:03:05,980 --> 00:03:12,910 Let's do a situation now where the object is at the 2 focal distances. I guess we can call that 44 00:03:13,480 --> 00:03:20,430 Let's put the object right over here 45 00:03:20,890 --> 00:03:22,850 We can do the exact same thing 46 00:03:22,850 --> 00:03:26,470 You might want to do it on paper on your own to get some practice doing it 47 00:03:26,480 --> 00:03:31,960 We'll do one ray that's parallel 48 00:03:31,980 --> 00:03:36,560 When it gets refracted, it will go through the focal point on the other side 49 00:03:36,580 --> 00:03:40,750 And then we'll do another ray that goes through the focal point on the left side 50 00:03:40,750 --> 00:03:45,110 and then it will become parallel 51 00:03:45,130 --> 00:03:48,080 And they can reconverge or they converge right over there 52 00:03:48,090 --> 00:03:53,340 So you can see that this is actually a parallelogram 53 00:03:53,350 --> 00:03:58,490 This distance right there is going to be the same thing as that distance over here 54 00:03:58,490 --> 00:04:01,690 It is actually--I don't want to say symmetry. You can't flip it over 55 00:04:01,690 --> 00:04:05,190 But this is a--and this distance right over here is going to be the same 56 00:04:05,190 --> 00:04:08,080 thing as this distance over here. I won't go into all the geometry 57 00:04:08,090 --> 00:04:17,210 Anyway, this would be an inverted image of exactly the same size at the exact same distance 58 00:04:17,260 --> 00:04:19,780 Actually I didn't talk about distance in this one over here 59 00:04:19,800 --> 00:04:24,340 Over here, it's a real image; it's smaller and it's also going to be closer in 60 00:04:24,340 --> 00:04:27,150 than this one was. It's gonna be closer to lens 61 00:04:27,160 --> 00:04:33,090 But here the image is going to be the same size as the original object 62 00:04:33,220 --> 00:04:37,620 It's going to be inverted, but it's going to be at the same distance from the lens 63 00:04:37,620 --> 00:04:41,470 just on the other side. Once again this is a real image 64 00:04:41,830 --> 00:04:43,920 Let's do another one 65 00:04:45,610 --> 00:04:47,810 Copy and paste 66 00:04:48,080 --> 00:04:52,480 So let's stick something between one focal length and two focal lengths 67 00:04:53,230 --> 00:05:03,020 So what's put my object right over there 68 00:05:03,040 --> 00:05:06,600 So once again, let's go parallel 69 00:05:06,620 --> 00:05:16,460 then we will refract through the focus on the other side 70 00:05:16,480 --> 00:05:19,250 And then let's go through the focus on the left side 71 00:05:19,870 --> 00:05:25,330 And then we will refract and go parallel 72 00:05:25,370 --> 00:05:30,830 So here, we will have--remember, I could use any point. Here I just used the tip 73 00:05:30,850 --> 00:05:34,250 because I know the base will converge over there 74 00:05:34,250 --> 00:05:38,410 If I took 2 points, it would go converge right back there 75 00:05:38,560 --> 00:05:40,760 And then if I did with a point right here 76 00:05:40,770 --> 00:05:43,360 and I did that same exercise, it would go right over there 77 00:05:43,360 --> 00:05:47,150 And so the whole image would show up over here 78 00:05:47,150 --> 00:05:50,580 So here, it's real; it's inverted; and it's larger 79 00:05:50,770 --> 00:05:57,220 and it is now further away from the lens than the object on the other side 80 00:05:57,220 --> 00:06:00,020 This is really kind of the reverse of the first example 81 00:06:00,030 --> 00:06:04,210 The first example, the object was larger and more than two focal lengths away 82 00:06:04,210 --> 00:06:06,250 and the image was in this range 83 00:06:06,250 --> 00:06:09,870 Now the object is here and now the image's on the other side. So they're kind of-- 84 00:06:10,040 --> 00:06:13,790 that's really just the other side of that first examples 85 00:06:13,820 --> 00:06:18,850 Let's do a couple more 86 00:06:18,870 --> 00:06:27,070 So let's put the object at the focal point and see what would happen 87 00:06:27,090 --> 00:06:31,310 And sometimes people memorize this type of things for physics exams 88 00:06:31,330 --> 00:06:35,310 You don't need to. All you have to do is remember just think about 2 rays 89 00:06:35,310 --> 00:06:38,830 usually from the tip of the arrow that gives you a sense what the image will look like 90 00:06:38,950 --> 00:06:42,380 and you do one parallel and one that goes through the focal point 91 00:06:42,410 --> 00:06:43,800 Well, with that said 92 00:06:43,800 --> 00:06:47,340 we're gonna do something slightly different when something is sitting at the focal point 93 00:06:48,080 --> 00:06:50,910 When something is sitting at the focal point 94 00:06:50,930 --> 00:06:54,130 one is we can do the parallel 95 00:06:54,440 --> 00:06:58,660 It will be refracted through the focal point on the other side 96 00:06:58,990 --> 00:07:04,920 And then instead of doing a ray that goes through the focal point on this side 97 00:07:04,920 --> 00:07:08,130 because actually you can't. You're sitting on the focal point right there 98 00:07:08,230 --> 00:07:13,610 Let's do a ray that does not get refracted. We did a similar thing with the parabolic mirrors 99 00:07:13,620 --> 00:07:19,920 What I want do is a ray that'll go right to the center of the lens 100 00:07:19,920 --> 00:07:22,450 where it won't get refracted 101 00:07:22,860 --> 00:07:28,260 It's just go straight through the center of the lens 102 00:07:28,710 --> 00:07:35,440 So what you have here is, both of these rays that were diverging from this point from this tip 103 00:07:35,440 --> 00:07:37,100 they don't reconverge anywhere 104 00:07:37,120 --> 00:07:39,690 And they don't even look like they're diverging from another point 105 00:07:39,690 --> 00:07:43,050 if someone's eyeball is right over here 106 00:07:43,410 --> 00:07:47,010 They're just going to see these as 2 parallel rays of light 107 00:07:47,010 --> 00:07:50,820 So no image will form. Not a real image or virtual image 108 00:07:50,840 --> 00:07:56,920 So we can say no image is going to form 109 00:07:57,990 --> 00:08:08,290 Now the last case is, let's put the object less than one focal distance away 110 00:08:09,140 --> 00:08:16,880 Let's put the object right over here. And think about what happens 111 00:08:16,900 --> 00:08:19,520 Once again, the light ray from this tip 112 00:08:19,520 --> 00:08:24,390 where to go parallel. It will be refracted through the focal point on the other side 113 00:08:24,810 --> 00:08:26,720 And then let's do another light ray, going 114 00:08:26,720 --> 00:08:30,590 in a direction as if it were coming the direction of the focal point on this side 115 00:08:30,610 --> 00:08:32,270 So it comes from that direction 116 00:08:32,289 --> 00:08:34,229 The light ray would go like that 117 00:08:34,590 --> 00:08:39,790 And then it would come out on the other side parallel 118 00:08:40,000 --> 00:08:43,300 So clearly, these two light rays are not converging 119 00:08:43,309 --> 00:08:45,560 So no real image's going to form 120 00:08:45,690 --> 00:08:51,390 But they do look like they're diverging from some point 121 00:08:51,720 --> 00:08:59,350 Continue these lines. They both look like they're coming from a point right over there 122 00:08:59,350 --> 00:09:04,020 So what's going to happen? If someone's eyes are processing these light rays 123 00:09:04,100 --> 00:09:06,880 they're gonna see the tip of this arrow all the way up here 124 00:09:06,880 --> 00:09:11,200 They're gonna see the base of this arrow down here 125 00:09:11,580 --> 00:09:29,700 And essentially, they're going to see a magnified virtual image of the actual arrow 126 00:09:29,810 --> 00:00:00,000 Anyway, hopefully you found that interesting