1 00:00:00,090 --> 00:00:02,490 The following content is provided under a Creative 2 00:00:02,490 --> 00:00:04,030 Commons license. 3 00:00:04,030 --> 00:00:06,330 Your support will help MIT OpenCourseWare 4 00:00:06,330 --> 00:00:10,720 continue to offer high quality educational resources for free. 5 00:00:10,720 --> 00:00:13,320 To make a donation or view additional materials 6 00:00:13,320 --> 00:00:17,280 from hundreds of MIT courses, visit MIT OpenCourseWare 7 00:00:17,280 --> 00:00:19,338 at ocw.mit.edu. 8 00:00:21,242 --> 00:00:22,950 PROFESSOR: Because there was a point when 9 00:00:22,950 --> 00:00:25,140 you could start to read. 10 00:00:25,140 --> 00:00:29,110 Behind that point, you couldn't read it anymore, 11 00:00:29,110 --> 00:00:30,960 and in front of that point you could. 12 00:00:30,960 --> 00:00:33,300 So when you were at a large distance-- 13 00:00:33,300 --> 00:00:36,136 when the text was at a large distance from your eyes, 14 00:00:36,136 --> 00:00:37,260 what do the text look like? 15 00:00:37,260 --> 00:00:39,390 I saw a couple of different explanations. 16 00:00:39,390 --> 00:00:41,070 So what did the text look like when 17 00:00:41,070 --> 00:00:44,170 you were a large distance away? 18 00:00:44,170 --> 00:00:45,510 What did it look like? 19 00:00:45,510 --> 00:00:48,750 Black lines. 20 00:00:48,750 --> 00:00:51,120 Anyone else have another description they want to use? 21 00:00:51,120 --> 00:00:52,800 Black lines. 22 00:00:52,800 --> 00:00:53,620 Blurry. 23 00:00:53,620 --> 00:00:55,770 I like that. 24 00:00:55,770 --> 00:00:59,070 What did you say? 25 00:00:59,070 --> 00:00:59,911 Chinese characters? 26 00:00:59,911 --> 00:01:01,410 It looked like a different language. 27 00:01:01,410 --> 00:01:02,610 You couldn't read it. 28 00:01:02,610 --> 00:01:05,459 You could tell that there was some difference between them, 29 00:01:05,459 --> 00:01:06,225 right? 30 00:01:06,225 --> 00:01:07,933 Like, you could tell that there was maybe 31 00:01:07,933 --> 00:01:12,110 a vertical line or something, but you couldn't recognize it. 32 00:01:12,110 --> 00:01:14,280 You couldn't decide what it was. 33 00:01:14,280 --> 00:01:15,000 OK, I like that. 34 00:01:15,000 --> 00:01:16,875 So maybe it looked like a different alphabet. 35 00:01:19,610 --> 00:01:25,400 Different alphabet, nice. 36 00:01:25,400 --> 00:01:25,900 I like that. 37 00:01:25,900 --> 00:01:27,480 That's good. 38 00:01:27,480 --> 00:01:31,770 What about when you were a small distance away, 39 00:01:31,770 --> 00:01:34,530 what did it look like? 40 00:01:34,530 --> 00:01:42,040 Actual words, real writing, you could read it. 41 00:01:47,030 --> 00:01:50,090 You can see details about those letters, 42 00:01:50,090 --> 00:01:51,657 and we're going to call that-- 43 00:01:51,657 --> 00:01:53,490 we're going to say that you can see details, 44 00:01:53,490 --> 00:01:56,030 but I really like Juan's different alphabet there. 45 00:01:56,030 --> 00:01:58,250 Because you can see that it's not 46 00:01:58,250 --> 00:02:00,330 a Chinese character, or a Cyrillic character, 47 00:02:00,330 --> 00:02:02,780 or a different alphabet that you're not used to. 48 00:02:02,780 --> 00:02:06,560 But you could read the characters. 49 00:02:10,022 --> 00:02:11,980 Now just because you are standing farther back, 50 00:02:11,980 --> 00:02:14,110 does that mean the letters weren't actually 51 00:02:14,110 --> 00:02:16,870 there like they changed into some other mysterious language? 52 00:02:19,390 --> 00:02:21,370 No, they're still there. 53 00:02:21,370 --> 00:02:24,250 You just can't read the characters. 54 00:02:24,250 --> 00:02:27,110 You can't see detail. 55 00:02:27,110 --> 00:02:28,360 You could read the characters. 56 00:02:28,360 --> 00:02:31,930 You can see details. 57 00:02:31,930 --> 00:02:37,150 Here, you cannot see details. 58 00:02:41,970 --> 00:02:44,100 How would you say the angular size 59 00:02:44,100 --> 00:02:49,590 of that text would compare when you are a large distance away 60 00:02:49,590 --> 00:02:51,960 versus when you're a small distance away? 61 00:02:51,960 --> 00:02:56,490 In your camera-- when you have these two cameras here, 62 00:02:56,490 --> 00:03:00,930 you take an image, and that gets transferred back to your brain. 63 00:03:00,930 --> 00:03:03,700 When you're far from the text, what 64 00:03:03,700 --> 00:03:08,310 is the angular size of that text? 65 00:03:08,310 --> 00:03:09,570 It's what? 66 00:03:09,570 --> 00:03:10,980 It's smaller, right? 67 00:03:10,980 --> 00:03:13,020 So let's do this. 68 00:03:13,020 --> 00:03:16,485 We have small angular size. 69 00:03:21,460 --> 00:03:24,750 What about when you're close? 70 00:03:24,750 --> 00:03:25,470 It gets large. 71 00:03:25,470 --> 00:03:28,650 You get a large angular size. 72 00:03:32,290 --> 00:03:34,660 And you can get closer, and closer, and closer, 73 00:03:34,660 --> 00:03:36,550 and closer until each of those letters 74 00:03:36,550 --> 00:03:39,070 actually looks pretty big, so the angular size 75 00:03:39,070 --> 00:03:43,180 of those letters is big, and you can easily see the details. 76 00:03:43,180 --> 00:03:48,550 So there was some point in between where you could first, 77 00:03:48,550 --> 00:03:51,760 as you got closer, start to see details. 78 00:03:51,760 --> 00:03:54,100 You could first start to read the characters. 79 00:03:54,100 --> 00:03:57,340 You could first tell that they were words in writing. 80 00:03:57,340 --> 00:04:08,500 And we call that the smallest angular size, you 81 00:04:08,500 --> 00:04:10,950 or your detector-- 82 00:04:10,950 --> 00:04:16,230 your detector-- can resolve. 83 00:04:20,589 --> 00:04:24,160 So when astronomers talk about resolving things, 84 00:04:24,160 --> 00:04:28,010 that means they're talking about seeing details. 85 00:04:28,010 --> 00:04:31,780 So for each of your eyes, there is a smallest angular 86 00:04:31,780 --> 00:04:34,750 size that your detector can resolve, 87 00:04:34,750 --> 00:04:37,390 and for people, that size-- we're 88 00:04:37,390 --> 00:04:38,800 actually going to calculate this, 89 00:04:38,800 --> 00:04:41,260 but we're running out of time a little bit today. 90 00:04:41,260 --> 00:04:44,910 So for a person, your smallest angular size-- 91 00:04:44,910 --> 00:04:47,720 I'm just going to write this down over here-- 92 00:04:47,720 --> 00:04:49,810 for a person, the smallest angular size 93 00:04:49,810 --> 00:04:55,000 is equal to about 3 times 10 to the minus 4 radians. 94 00:04:58,550 --> 00:05:00,950 All right, that doesn't mean a whole lot. 95 00:05:00,950 --> 00:05:03,520 What that means is when you're about a meter or so away, 96 00:05:03,520 --> 00:05:08,650 you can read text that's a couple of millimeters tall. 97 00:05:08,650 --> 00:05:11,980 For different telescopes, they can actually 98 00:05:11,980 --> 00:05:15,760 resolve details that are much smaller than that 99 00:05:15,760 --> 00:05:18,660 in terms of angular size. 100 00:05:18,660 --> 00:05:31,970 For the micro observatory telescopes, 101 00:05:31,970 --> 00:05:37,130 we've got an angular size of about 7 times 10 102 00:05:37,130 --> 00:05:41,150 to the minus 5 radians. 103 00:05:41,150 --> 00:05:44,090 And for the Chandra X-ray telescope, 104 00:05:44,090 --> 00:05:50,390 the one that we're going to use, we 105 00:05:50,390 --> 00:05:53,390 are going to see that it's resolution, or the smallest 106 00:05:53,390 --> 00:05:58,460 angle that it can see details, is 5 times 10 107 00:05:58,460 --> 00:06:01,650 to the minus 6 radians. 108 00:06:04,340 --> 00:06:06,980 Which one of these detectors has the smallest angle 109 00:06:06,980 --> 00:06:07,860 that it can see? 110 00:06:11,270 --> 00:06:13,685 Which one of these numbers is the smallest? 111 00:06:17,210 --> 00:06:17,900 OK. 112 00:06:17,900 --> 00:06:26,240 Because remember this is 0.0003 radians, so 3 times 10 113 00:06:26,240 --> 00:06:27,990 to the minus 4. 114 00:06:27,990 --> 00:06:32,930 We move the decimal point over one, two, three, four places, 115 00:06:32,930 --> 00:06:35,660 and we get 0.0003. 116 00:06:35,660 --> 00:06:45,530 This one is 0.00007, so smaller, and this one is 5-- 117 00:06:45,530 --> 00:06:48,320 or I'm sorry. 118 00:06:48,320 --> 00:06:56,700 0.000005 radians, so this number is smaller. 119 00:06:56,700 --> 00:06:59,990 So if you guys can only see this, 120 00:06:59,990 --> 00:07:03,860 that means that other telescopes could be farther away, 121 00:07:03,860 --> 00:07:05,380 and they could still see details. 122 00:07:05,380 --> 00:07:09,340 Or they can see smaller details than we can see.