1 00:00:01,020 --> 00:00:02,020 Hi! 2 00:00:02,020 --> 00:00:03,020 I'm Pritish 3 00:00:03,020 --> 00:00:05,500 Today, we will be talking about Trigonometry. 4 00:00:05,500 --> 00:00:09,639 This is the first video on Trigonometry. 5 00:00:09,639 --> 00:00:13,590 I would like to start with "Why do we want to study Trigonometry?" 6 00:00:13,590 --> 00:00:16,990 and "What is Trigonometry?" 7 00:00:16,990 --> 00:00:22,350 You would certainly know that Euclidean geometry is very fundamental to how we think about 8 00:00:22,350 --> 00:00:24,150 nature. 9 00:00:24,150 --> 00:00:29,770 The way we visualize things in Physics, for example, we use Euclidean geometry in the 10 00:00:29,770 --> 00:00:31,090 way we think. 11 00:00:31,090 --> 00:00:39,250 And often, Euclidean geometry requires some amount of innovative thinking to reason about 12 00:00:39,250 --> 00:00:40,590 problems. 13 00:00:40,590 --> 00:00:46,809 And often when you want to talk about Physics, you don't want geometry to be 14 00:00:46,809 --> 00:00:49,010 your bottleneck in thinking about Physics. 15 00:00:49,010 --> 00:00:59,239 So Trigonometry and Coordinate Geometry are two subjects which try to make a more systematic 16 00:00:59,239 --> 00:01:06,740 study of Geometry. 17 00:01:06,740 --> 00:01:08,700 And what is "Trigonometry"? 18 00:01:08,700 --> 00:01:26,110 Trigonometry is about a study of angles in an "algebraic" way. 19 00:01:26,110 --> 00:01:30,299 You would feel more comfortable doing Algebra 20 00:01:30,299 --> 00:01:37,069 Algebra is something you can do in a more mechanical way. 21 00:01:37,069 --> 00:01:43,069 Whereas, Geometry often requires an innovative leap. 22 00:01:43,069 --> 00:01:48,130 Using trigonometry, you'll be able to reason about geometric problems in a more algebraic 23 00:01:48,130 --> 00:01:52,110 way. 24 00:01:52,110 --> 00:01:55,450 Let's start with the very basics of what is an angle. 25 00:01:55,450 --> 00:02:06,169 You know from basic Euclidean geometry, that if you have a circle of radius 'r', 26 00:02:06,169 --> 00:02:15,770 then the perimeter of the circle is equal to 2.\pi.r. 27 00:02:15,770 --> 00:02:20,110 We know this from basic geometry. 28 00:02:20,110 --> 00:02:34,640 A basic reasoning will tell you that length of the arc of half a circle 29 00:02:34,640 --> 00:02:36,110 is \pi.r. 30 00:02:36,110 --> 00:02:51,350 Similarly, if I take a quarter circle, the length of the arc is (\pi/2).r. 31 00:02:51,350 --> 00:03:03,720 In general if I pick out an angle of, say, \alpha degrees (like this could be 60 degrees), 32 00:03:03,720 --> 00:03:26,600 then you can easily reason that the length of an arc with angle \alpha degrees is (\alpha/360).(2.\pi.r). 33 00:03:26,600 --> 00:03:30,990 This is just a basic ratio and proportion argument. 34 00:03:30,990 --> 00:03:45,030 Let me write this as ((2.\pi.\alpha)/360).r. 35 00:03:45,030 --> 00:03:51,190 We are more generally taught since school to think in terms of degrees. 36 00:03:51,190 --> 00:03:54,190 The full circle has 360 degree. 37 00:03:54,190 --> 00:03:57,300 But now when we have to write the length of an arc, 38 00:03:57,300 --> 00:03:59,700 we have to write an annoying expression ((2.\pi.\alpha)/360).r. 39 00:03:59,700 --> 00:04:12,010 It would be much nicer to call this expression ((2.\pi.\alpha)/360) as the "angle" itself. 40 00:04:12,010 --> 00:04:18,459 Instead of \alpha degrees if we could call ((2.\pi.\alpha)/360) as the "angle", then 41 00:04:18,459 --> 00:04:27,490 it would be much nicer. 42 00:04:27,490 --> 00:04:31,360 As there are different ways to measure objects, for example, length, you can measure it in 43 00:04:31,360 --> 00:04:34,080 meters or inches. 44 00:04:34,080 --> 00:04:37,240 similarly this is a different unit for measuring angles. 45 00:04:37,240 --> 00:04:45,529 This is angle in "radians". 46 00:04:45,529 --> 00:04:47,510 Thinking in terms of radians is very important. 47 00:04:47,510 --> 00:04:53,229 My math teacher used to tell me that when you are learning a new language, 48 00:04:53,229 --> 00:04:55,830 for example, if I am trying to speak in English, 49 00:04:55,830 --> 00:04:58,960 if I want to learn it well, I should not think in a different language. 50 00:04:58,960 --> 00:05:02,750 For example, I should not think in Hindi and translate to English every time I am speaking. 51 00:05:02,750 --> 00:05:07,900 You should really start thinking in English, if you want to learn English well. 52 00:05:07,900 --> 00:05:14,550 Similarly here, thinking in terms of radians is often the better thing to do 53 00:05:14,550 --> 00:05:33,639 because now the length of arc with angle \theta radians is simply (r.\theta). 54 00:05:33,639 --> 00:05:38,949 So that's why thinking in terms of radians is often the more natural way to think about 55 00:05:38,949 --> 00:05:42,308 angles. 56 00:05:42,308 --> 00:05:49,719 Just to be more familiar with this conversion, 57 00:05:49,719 --> 00:05:56,830 lets see that 360 degrees is '2 \pi' radians. 58 00:05:56,830 --> 00:06:04,939 The perimeter of the entire circle is '2.\pi.r' and '2\pi' is the angle of the entire circle. 59 00:06:04,939 --> 00:06:16,000 Similarly, 180 degrees is \pi. 90 degrees is \pi/2 and so on. 60 00:06:16,000 --> 00:06:20,520 So we just saw how to measure angles in degrees and radians 61 00:06:20,520 --> 00:06:27,250 and we said that radians is the more natural unit to think about angles. 62 00:06:27,250 --> 00:06:33,069 So that now the length of the arc with angle of \theta radians is just r.\theta. 63 00:06:33,069 --> 00:06:36,558 In the rest of the video, we will talk about trigonometric ratios, 64 00:06:36,558 --> 00:06:40,680 we'll define what they are and we'll talk about some trigonometric identities. 65 00:06:40,680 --> 00:06:46,999 These are the algebraic tools which will help us reason about angles in a more algebraic 66 00:06:46,999 --> 00:06:52,159 way. 67 00:06:52,159 --> 00:06:54,189 Let's look at an angle \theta. 68 00:06:54,189 --> 00:07:00,520 Whenever we write \theta as an angle, it is assumed that it is in radians, 69 00:07:00,520 --> 00:07:03,889 as we know that radians is the more natural unit to think about angles. 70 00:07:03,889 --> 00:07:09,539 Let's say the radius is 'r', 71 00:07:09,539 --> 00:07:19,190 and we just saw that the length of the arc is r.\theta. 72 00:07:19,190 --> 00:07:23,240 Now there are other interesting parameters that you would want to know about the angle. 73 00:07:23,240 --> 00:07:30,960 For example, if we drop a perpendicular from the top vertex, 74 00:07:30,960 --> 00:07:39,210 what is the height of this line segment? 75 00:07:39,210 --> 00:07:47,129 Let's call the vertices as A, B and C. 76 00:07:47,129 --> 00:07:55,249 This side BC is "opposite" to the angle. 77 00:07:55,249 --> 00:08:04,110 The side AC is the side that is "adjacent" to the angle. 78 00:08:04,110 --> 00:08:17,789 And the side AB is the "hypotenuse". 79 00:08:17,789 --> 00:08:25,149 So we would like to know the height of the line segment BC is. 80 00:08:25,149 --> 00:08:28,180 One thing that you know from similarity of triangles is that 81 00:08:28,180 --> 00:08:39,000 suppose I have two triangles like this. 82 00:08:39,000 --> 00:08:47,100 You know from similarity of triangles that BC/AB = DE/AD. 83 00:08:47,100 --> 00:08:57,430 (Note that angles BCA and DEA are right angles.) 84 00:08:57,430 --> 00:09:01,070 These are two triangles which have all three angles the same, 85 00:09:01,070 --> 00:09:10,130 and therefore they are "similar" and hence the ratio of sides are equal. 86 00:09:10,130 --> 00:09:14,970 Because of similarity of triangles, this ratio is purely a property of the angle, 87 00:09:14,970 --> 00:09:20,020 and is not related to any of the sides. 88 00:09:20,020 --> 00:09:34,190 This ratio is defined as the "sine" of the angle. 89 00:09:34,190 --> 00:09:47,420 To remember it more easily, let's call sin(\theta) as opposite/hypotenuse. 90 00:09:47,420 --> 00:10:06,990 Now we can see that since the hypotenuse is 'r', the length of the opposite side is now 91 00:10:06,990 --> 00:10:10,970 'r.(sin \theta)'. 92 00:10:10,970 --> 00:10:19,130 Similarly, now we can define the ratio of the adjacent/hypotenuse. 93 00:10:19,130 --> 00:10:30,840 So that is defined as cos \theta. 94 00:10:30,840 --> 00:10:43,750 Again, since the hypotenuse is 'r', the adjacent side is of length r.(cos \theta). 95 00:10:43,750 --> 00:10:55,180 In terms of this ratio, this will be AC/AB = AE/AD. 96 00:10:55,180 --> 00:11:05,030 And by similarity of triangles, this is just a 97 00:11:05,030 --> 00:11:06,171 property of the angle, 98 00:11:06,171 --> 00:11:09,560 and does not depend on the sides of the triangle. 99 00:11:09,560 --> 00:11:21,900 Now, we'll see our first trigonometric identity. 100 00:11:21,900 --> 00:11:37,910 From Pythagoras' theorem, we know that for any right angled triangle, 101 00:11:37,910 --> 00:11:41,510 the sum of squares of the two sides is equal to the square of the hypotenuse. 102 00:11:41,510 --> 00:11:54,220 So let's write down here : (opp)^2 + (adj)^2 = (hyp)^2. 103 00:11:54,220 --> 00:11:58,930 This is what Pythagoras' theorem tells us. 104 00:11:58,930 --> 00:12:13,730 If we divide by (hyp)^2 throughout, we get that (opp/hyp)^2 + (adj/hyp)^2 = 1. 105 00:12:13,730 --> 00:12:19,760 Now, if you look at our definitions of sin \theta and cos \theta, 106 00:12:19,760 --> 00:12:31,430 this tells us that, (sin \theta)^2 + (cos \theta)^2 = 1. 107 00:12:31,430 --> 00:12:36,130 A usual convention to write (sin \theta)^2 is that 108 00:12:36,130 --> 00:12:38,380 you don't write the brackets all the time. 109 00:12:38,380 --> 00:12:51,870 So what we do is, write it as sin^2(\theta) and cos^2(\theta). 110 00:12:51,870 --> 00:12:57,560 So as to not confuse with, for example, sin(\theta^2). 111 00:12:57,560 --> 00:13:03,820 This would mean sin(\theta^2), whereas this is (sin \theta)^2