Precalculus with Integrated CalculusXYZ Homework Edition

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11.2 The Circular Functions: Sine and Cosine

In Section 11.1.1, we introduced circular motion and derived a formula which describes the linear velocity of an object moving on a circular path at a constant angular velocity. One of the goals of this section is describe the position of such an object. To that end, consider an angle θ in standard position and let P denote the point where the terminal side of θ intersects the Unit Circle, as diagrammed below.

Coordinate-plane figure.
Figure 11.39
Coordinate-plane figure.
Figure 11.40

By associating the point P with the angle θ , we are assigning a position on the Unit Circle to the angle θ . Since for each angle θ , the terminal side of θ , when graphed in standard position, intersects The Unit Circle only once, the mapping of θ to P is a function.1 Since there is only one way to describe a point using rectangular coordinates,2 the mappings of θ to each of the x and y coordinates of P are also functions. We give these functions names in the following definition.

You may have already seen definitions for the sine and cosine of an (acute) angle in terms of ratios of sides of a right triangle.4 While not incorrect, defining sine and cosine using right triangles limits the angles we can study to acute angles only. Definition 11.2, on the other hand, applies to all angles. Since these functions are defined in terms of points on the Unit Circle, they are called circular functions. Rest assured, Definition 11.2 specializes to Definition B.1 when θ is an acute angle. We will see instances of this fact in the next example.

A few remarks are in order. First, after having re-used some of our work from Section B.2 in a few specific instances, we can reconcile Definition 11.2 with Definition B.1 in the case θ is an acute angle. We situate θ in a right triangle with hypotenuse length 1 , adjacent side length ` x ,' and the opposite side length ` y ' as seen below on the left. Placing the vertex of θ at the origin and the adjacent side of θ along the x -axis as seen below on the right effectively puts θ in standard position with θ 's adjacent side as the initial side of θ and the hypotenuse as the terminal side of θ . Since the hypotenuse of the triangle has length 1 , we know the point P ( x , y ) is on the Unit Circle.5

Coordinate-plane figure.
Figure 11.47
Coordinate-plane figure.
Figure 11.48

Definition B.1 gives cos ( θ ) = x 1 = x and sin ( θ ) = y 1 = y which exactly matches Definition 11.2. Hence, in the case of acute angles, the two definitions agree. In other words, the values of the trigonometric ratios of acute angles are the same as the corresponding circular function values.

A second important take-away from Example 11.2.1 is use of symmetry in number. Indeed, we found the sine and cosine of 5 π 6 using the (acute) angle π 6 `for reference.' Since the Unit Circle is rife with symmetry, we would like to generalize this concept and exploit symmetry whenever possible. To that end, we introduce the notion of reference angle.

In general, for a non-quadrantal angle θ , the reference angle for θ (which we'll usually denote α ) is the acute angle made between the terminal side of θ and the x -axis. If θ is a Quadrant I or IV angle, α is the angle between the terminal side of θ and the positive x -axis:

Coordinate-plane figure.
Figure 11.49
Coordinate-plane figure.
Figure 11.50

Reference angle α for a Quadrant I angle

Reference angle α for a Quadrant IV angle

If θ is a Quadrant II or III angle, α is the angle between the terminal side of θ and the negative x -axis:

Coordinate-plane figure.
Figure 11.51
Coordinate-plane figure.
Figure 11.52

Reference angle α for a Quadrant II angle

Reference angle α for a Quadrant III angle

If we let P denote the point ( cos ( θ ) , sin ( θ ) ) , then P lies on the Unit Circle. Since the Unit Circle possesses symmetry with respect to the x -axis, y -axis and origin, regardless of where the terminal side of θ lies, there is a point Q symmetric with P which determines θ 's reference angle, α . The only difference between the points P and Q are the signs of their coordinates, ± . Hence, we have the following:

In light of Theorem 11.1, it pays to know the sine and cosine values for certain common Quadrant I angles as well as to keep in mind the signs of the coordinates of points in the given quadrants.

θ ( degrees ) θ ( radians ) cos ( θ ) sin ( θ ) 0 0 1 0 30 π 6 3 2 1 2 45 π 4 2 2 2 2 60 π 3 1 2 3 2 90 π 2 0 1

Coordinate-plane figure.
Figure 11.53

A couple of remarks are in order. First off, the reader may have noticed that when expressed in radian measure, the reference angle for a non-quadrantal angle is easy to spot. Reduced fraction multiples of π with a denominator of 6 have π 6 as a reference angle, those with a denominator of 4 have π 4 as their reference angle, and those with a denominator of 3 have π 3 as their reference angle.7

Also note in number above, the angles π 3 and 7 π 3 are coterminal. As a result, have the same values for sine and cosine. It turns out that we can characterize coterminal angles in this manner, as stated below.

Recall the phraseology `if and only if' means there are two things to argue in Theorem 11.2: first, if α and β are co-terminal, then cos ( α ) = cos ( β ) and sin ( α ) = sin ( β ) . This is immediate since coterminal share terminal sides, and, in particular, the (unique) point on the Unit Circle shared by said terminal side. Second, we need to argue that if cos ( α ) = cos ( β ) and sin ( α ) = sin ( β ) , then α and β are coterminal.

To prove this second claim, note that when an angle is drawn in standard position, the terminal side of the angle is the ray that starts at the origin and is completely determined by any other point on the terminal side. If cos ( α ) = cos ( β ) and sin ( α ) = sin ( β ) , then their terminal sides share a point on the Unit Circle, namely ( cos ( α ) , sin ( α ) ) = ( cos ( β ) , sin ( β ) ) . Hence, α and β are coterminal.

The Reference Angle Theorem in conjunction with the table of sine and cosine values on Page Section 11.2 can be used to generate the figure on the next page. We recommend committing it to memory.

Figure: Important Points on the Unit Circle
Figure 11.58 Important Points on the Unit Circle

Our next example uses The Reference Angle Theorem in a slightly more sophisticated context.

A couple of remarks about Example 11.2.3 are in order. First, we note the right triangle we used to find sin ( α ) is a scaled 5-12-13 triangle. Recognizing this Pythagorean Triple9 may have simplified our workflow. Along the same lines, since, the Unit Circle, by definition, is described by the equation x 2 + y 2 = 1 , we could substitute x = 5 13 in order to find y . We leave it to the reader to show we get the exact same answer regardless of the approach used.

Our next example turns the tables and makes good use of the Unit Circle values given on Section 11.2 as well as Theorem 11.2 in a different way: instead of giving information about the angle and asking for sine or cosine values, we are given sine or cosine values and asked to produce the corresponding angles. In other words, we solve some rudimentary equations involving sine and cosine.10

One of the key items to take from Example 11.2.4 is that, in general, solutions to trigonometric equations consist of infinitely many answers. To get a feel for these answers, the reader is encouraged to follow our mantra from Chapter 10 - that is, `When in doubt, write it out!' This is especially important when checking answers to the exercises.

For example, another Quadrant IV solution to sin ( θ ) = 1 2 is θ = π 6 . Hence, the family of Quadrant IV answers to number above could just have easily been written θ = π 6 + 2 π k for integers k . While on the surface, this family may look different than the stated solution of θ = 11 π 6 + 2 π k for integers k , we leave it to the reader to show they represent the same list of angles.

It is also worth noting that when asked to solve equations in algebra, we are usually looking for real number solutions. Thanks to the identifications made on page Section 11.1, we are able to regard the inputs to the sine and cosine functions as real numbers by identifying any real number t with an oriented angle θ measuring θ = t radians. That is, for each real number t , we associate an oriented arc t units in length with initial point ( 1 , 0 ) and endpoint P ( cos ( t ) , sin ( t ) ) .

Coordinate-plane figure.
Figure 11.75
Coordinate-plane figure.
Figure 11.76

In practice this means in expressions like ` cos ( π ) ' and ` sin ( 2 ) ,' the inputs can be thought of as either angles in radian measure or real numbers, whichever is more convenient.

Suppose, as in the Exercises, we are asked to find all real number solutions to the equation such as sin ( t ) = 1 2 . The discussion above allows us to find the real number solutions to this equation by thinking in angles. Indeed, we would solve this equation in the exact way we solved sin ( θ ) = 1 2 in Example 11.2.4 number. Our solution is only cosmetically different in that the variable used is t rather than θ : t = 7 π 6 + 2 π k or t = 11 π 6 + 2 π k for integers, k .

We will study the sine and cosine functions in greater detail in Section 11.3. Until then, keep in mind that any properties of the sine and cosine functions developed in the following sections which regard them as functions of angles in radian measure apply equally well if the inputs are regarded as real numbers.

Beyond the Unit Circle

In Definition 11.2, we define the sine and cosine functions using the Unit Circle, x 2 + y 2 = 1 . It turns out that we can use any circle centered at the origin to determine the sine and cosine values of angles. To show this, we essentially recycle the same similarity arguments used in Section B.2 to show the trigonometric ratios described in Definition B.1 are independent of the choice of right triangle used.12

Consider for the moment the acute angle θ drawn below in standard position. Let Q ( x , y ) be the point on the terminal side of θ which lies on the circle x 2 + y 2 = r 2 , and let P ( x , y ) be the point on the terminal side of θ which lies on the Unit Circle. Now consider dropping perpendiculars from P and Q to create two right triangles, Δ O P A and Δ O Q B . These triangles are similar,13 thus it follows that x x = r 1 = r , so x = r x and, similarly, we find y = r y . Since, by definition, x = cos ( θ ) and y = sin ( θ ) , we get the coordinates of Q to be x = r cos ( θ ) and y = r sin ( θ ) . By reflecting these points through the x -axis, y -axis and origin, we obtain the result for all non-quadrantal angles θ , and we leave it to the reader to verify these formulas hold for the quadrantal angles as well.

Coordinate-plane figure.
Figure 11.77
Coordinate-plane figure.
Figure 11.78

Not only can we describe the coordinates of Q in terms of cos ( θ ) and sin ( θ ) but since the radius of the circle is r = x 2 + y 2 , we can also express cos ( θ ) and sin ( θ ) in terms of the coordinates of Q . These results are summarized in the following theorem.

Note that in the case of the Unit Circle we have r = x 2 + y 2 = 1 , so Theorem 11.3 reduces to our definitions of cos ( θ ) and sin ( θ ) in Definition 11.2. Our next example makes good use of Theorem 11.3.

Theorem 11.3 gives us what we need to `circle back' to the question posed at the the beginning of the section: how to describe the position of an object traveling in a circular path of radius r with constant angular velocity ω . Suppose that at time t , the object has swept out an angle measuring θ radians. If we assume that the object is at the point ( r , 0 ) when t = 0 , the angle θ is in standard position. By definition, ω = θ t which we rewrite as θ = ω t . According to Theorem 11.3, the location of the object Q ( x , y ) on the circle is found using the equations x = r cos ( θ ) = r cos ( ω t ) and y = r sin ( θ ) = r sin ( ω t ) . Hence, at time t , the object is at the point ( r cos ( ω t ) , r sin ( ω t ) ) , as seen in the diagram below.

Coordinate-plane figure.
Figure 11.83

Equations for Circular Motion

We have just argued the following.

Exercises

In Exercises -, find the exact value of the cosine and sine of the given angle.

  1. θ = 0
  2. θ = π 4
  3. θ = π 3
  4. θ = π 2
  5. θ = 2 π 3
  6. θ = 3 π 4
  7. θ = π
  8. θ = 7 π 6
  9. θ = 5 π 4
  10. θ = 4 π 3
  11. θ = 3 π 2
  12. θ = 5 π 3
  13. θ = 7 π 4
  14. θ = 23 π 6
  15. θ = 13 π 2
  16. θ = 43 π 6
  17. θ = 3 π 4
  18. θ = π 6
  19. θ = 10 π 3
  20. θ = 117 π

In Exercises -, find all of the angles which satisfy the given equation.

  1. sin ( θ ) = 1 2
  2. cos ( θ ) = 3 2
  3. sin ( θ ) = 0
  4. cos ( θ ) = 2 2
  5. sin ( θ ) = 3 2
  6. cos ( θ ) = 1
  7. sin ( θ ) = 1
  8. cos ( θ ) = 3 2
  9. cos ( θ ) = 1.001

In Exercises -, solve the equation for t . (See the remarks on page Section 11.2.)

  1. cos ( t ) = 0
  2. sin ( t ) = 2 2
  3. cos ( t ) = 3
  4. sin ( t ) = 1 2
  5. cos ( t ) = 1 2
  6. sin ( t ) = 2
  7. cos ( t ) = 1
  8. sin ( t ) = 1
  9. cos ( t ) = 2 2

In Exercises -, let θ be the angle in standard position whose terminal side contains the given point then compute cos ( θ ) and sin ( θ ) .

  1. P ( 7 , 24 )
  2. Q ( 3 , 4 )
  3. R ( 5 , 9 )
  4. T ( 2 , 11 )

In Exercises -, use the results developed throughout the section to find the requested value.

  1. If sin ( θ ) = 7 25 with θ in Quadrant IV, what is cos ( θ ) ?
  2. If cos ( θ ) = 4 9 with θ in Quadrant I, what is sin ( θ ) ?
  3. If sin ( θ ) = 5 13 with θ in Quadrant II, what is cos ( θ ) ?
  4. If cos ( θ ) = 2 11 with θ in Quadrant III, what is sin ( θ ) ?
  5. If sin ( θ ) = 2 3 with θ in Quadrant III, what is cos ( θ ) ?
  6. If cos ( θ ) = 28 53 with θ in Quadrant IV, what is sin ( θ ) ?
  7. If sin ( θ ) = 2 5 5 and π 2 < θ < π , what is cos ( θ ) ?
  8. If cos ( θ ) = 10 10 and 2 π < θ < 5 π 2 , what is sin ( θ ) ?
  9. If sin ( θ ) = 0.42 and π < θ < 3 π 2 , what is cos ( θ ) ?
  10. If cos ( θ ) = 0.98 and π 2 < θ < π , what is sin ( θ ) ?

In Exercises -, use your calculator to approximate the given value to three decimal places. Make sure your calculator is in the proper angle measurement mode!

  1. sin ( 78.95 )
  2. cos ( 2.01 )
  3. sin ( 392.994 )
  4. cos ( 207 )
  5. sin ( π )
  6. cos ( e )

In Exercises -, write the given function as a nontrivial decomposition of functions as directed.

  1. For f ( t ) = 3 t + sin ( 2 t ) , find functions g and h so that f = g + h .
  2. For f ( θ ) = 3 cos ( θ ) sin ( 4 θ ) , find functions g and h so that f = g h .
  3. For f ( t ) = e 0.1 t sin ( 3 t ) , find functions g and h so that f = g h .
  4. For r ( t ) = sin ( t ) t , find functions f and g so r = f g .
  5. For r ( θ ) = 3 cos ( θ ) , find functions f and g so r = g f .
  6. For each function S ( t ) listed below, compute the average rate of change over the indicated interval.16 What trends do you notice? Be sure your calculator is in radian mode!

    S ( t ) [ 0.1 , 0.1 ] [ 0.01 , 0.01 ] [ 0.001 , 0.001 ] sin ( t ) sin ( 2 t ) sin ( 3 t ) sin ( 4 t )

In Exercises -, find the equations of motion for the given scenario. Assume that the center of the motion is the origin, the motion is counter-clockwise and that t = 0 corresponds to a position along the positive x -axis. (See Equation 11.3 and Example 11.1.3.)

  1. A point on the edge of the spinning yo-yo in Exercise from Section 11.1.

    Recall: The diameter of the yo-yo is 2.25 inches and it spins at 4500 revolutions per minute.

  2. The yo-yo in exercise from Section 11.1.

    Recall: The radius of the circle is 28 inches and it completes one revolution in 3 seconds.

  3. A point on the edge of the hard drive in Exercise from Section 11.1.

    Recall: The diameter of the hard disk is 2.5 inches and it spins at 7200 revolutions per minute.

  4. A passenger on the Big Wheel in Exercise from Section 11.1.

    Recall: The diameter is 128 feet and completes 2 revolutions in 2 minutes, 7 seconds.

  5. Consider the numbers: 0 , 1 , 2 , 3 , 4 . Take the square root of each of these numbers, then divide each by 2 . The resulting numbers should look hauntingly familiar. (See the values in the table on Section 11.2.)
  6. On page Section 11.2, we see that the sine and cosine functions of angles can be considered functions of real numbers. With help from your classmates, discuss the domains and ranges of f ( t ) = sin ( t ) and g ( t ) = cos ( t ) . Write your answers using interval notation.
  7. Another way to establish Theorem 11.3 is to use transformations. Re-read the discussion following Theorem 8.4 in Chapter 8 and transform the Unit Circle, x 2 + y 2 = 1 , to x 2 + y 2 = r 2 using horizontal and vertical stretches. Show if the coordinates on the Unit Circle are ( cos ( θ ) , sin ( θ ) ) , then the corresponding coordinates on x 2 + y 2 = r 2 are ( r cos ( θ ) , r sin ( θ ) ) .
  8. In the scenario of Equation 11.3, we assumed that at t = 0 , the object was at the point ( r , 0 ) . If this is not the case, we can adjust the equations of motion by introducing a `time delay.' If t 0 > 0 is the first time the object passes through the point ( r , 0 ) , show, with the help of your classmates, the equations of motion are x = r cos ( ω ( t t 0 ) ) and y = r sin ( ω ( t t 0 ) ) .

Answers

  1. cos ( 0 ) = 1 , sin ( 0 ) = 0
  2. cos ( π 4 ) = 2 2 , sin ( π 4 ) = 2 2
  3. cos ( π 3 ) = 1 2 , sin ( π 3 ) = 3 2
  4. cos ( π 2 ) = 0 , sin ( π 2 ) = 1
  5. cos ( 2 π 3 ) = 1 2 , sin ( 2 π 3 ) = 3 2
  6. cos ( 3 π 4 ) = 2 2 , sin ( 3 π 4 ) = 2 2
  7. cos ( π ) = 1 , sin ( π ) = 0
  8. cos ( 7 π 6 ) = 3 2 , sin ( 7 π 6 ) = 1 2
  9. cos ( 5 π 4 ) = 2 2 , sin ( 5 π 4 ) = 2 2
  10. cos ( 4 π 3 ) = 1 2 , sin ( 4 π 3 ) = 3 2
  11. cos ( 3 π 2 ) = 0 , sin ( 3 π 2 ) = 1
  12. cos ( 5 π 3 ) = 1 2 , sin ( 5 π 3 ) = 3 2
  13. cos ( 7 π 4 ) = 2 2 , sin ( 7 π 4 ) = 2 2
  14. cos ( 23 π 6 ) = 3 2 , sin ( 23 π 6 ) = 1 2
  15. cos ( 13 π 2 ) = 0 , sin ( 13 π 2 ) = 1
  16. cos ( 43 π 6 ) = 3 2 , sin ( 43 π 6 ) = 1 2
  17. cos ( 3 π 4 ) = 2 2 , sin ( 3 π 4 ) = 2 2
  18. cos ( π 6 ) = 3 2 , sin ( π 6 ) = 1 2
  19. cos ( 10 π 3 ) = 1 2 , sin ( 10 π 3 ) = 3 2
  20. cos ( 117 π ) = 1 , sin ( 117 π ) = 0
  21. sin ( θ ) = 1 2 when θ = π 6 + 2 π k or θ = 5 π 6 + 2 π k for any integer k .
  22. cos ( θ ) = 3 2 when θ = 5 π 6 + 2 π k or θ = 7 π 6 + 2 π k for any integer k .
  23. sin ( θ ) = 0 when θ = π k for any integer k .
  24. cos ( θ ) = 2 2 when θ = π 4 + 2 π k or θ = 7 π 4 + 2 π k for any integer k .
  25. sin ( θ ) = 3 2 when θ = π 3 + 2 π k or θ = 2 π 3 + 2 π k for any integer k .
  26. cos ( θ ) = 1 when θ = ( 2 k + 1 ) π for any integer k .
  27. sin ( θ ) = 1 when θ = 3 π 2 + 2 π k for any integer k .
  28. cos ( θ ) = 3 2 when θ = π 6 + 2 π k or θ = 11 π 6 + 2 π k for any integer k .
  29. cos ( θ ) = 1.001 never happens
  30. cos ( t ) = 0 when t = π 2 + π k for any integer k .
  31. sin ( t ) = 2 2 when t = 5 π 4 + 2 π k or t = 7 π 4 + 2 π k for any integer k .
  32. cos ( t ) = 3 never happens.
  33. sin ( t ) = 1 2 when t = 7 π 6 + 2 π k or t = 11 π 6 + 2 π k for any integer k .
  34. cos ( t ) = 1 2 when t = π 3 + 2 π k or t = 5 π 3 + 2 π k for any integer k .
  35. sin ( t ) = 2 never happens
  36. cos ( t ) = 1 when t = 2 π k for any integer k .
  37. sin ( t ) = 1 when t = π 2 + 2 π k for any integer k .
  38. cos ( t ) = 2 2 when t = 3 π 4 + 2 π k or t = 5 π 4 + 2 π k for any integer k .
  39. cos ( θ ) = 7 25 , sin ( θ ) = 24 25
  40. cos ( θ ) = 3 5 , sin ( θ ) = 4 5
  41. cos ( θ ) = 5 106 106 , sin ( θ ) = 9 106 106
  42. cos ( θ ) = 2 5 25 , sin ( θ ) = 11 5 25
  43. If sin ( θ ) = 7 25 with θ in Quadrant IV, then cos ( θ ) = 24 25 .
  44. If cos ( θ ) = 4 9 with θ in Quadrant I, then sin ( θ ) = 65 9 .
  45. If sin ( θ ) = 5 13 with θ in Quadrant II, then cos ( θ ) = 12 13 .
  46. If cos ( θ ) = 2 11 with θ in Quadrant III, then sin ( θ ) = 117 11 .
  47. If sin ( θ ) = 2 3 with θ in Quadrant III, then cos ( θ ) = 5 3 .
  48. If cos ( θ ) = 28 53 with θ in Quadrant IV, then sin ( θ ) = 45 53 .
  49. If sin ( θ ) = 2 5 5 and π 2 < θ < π , then cos ( θ ) = 5 5 .
  50. If cos ( θ ) = 10 10 and 2 π < θ < 5 π 2 , then sin ( θ ) = 3 10 10 .
  51. If sin ( θ ) = 0.42 and π < θ < 3 π 2 , then cos ( θ ) = 0.8236 0.9075 .
  52. If cos ( θ ) = 0.98 and π 2 < θ < π , then sin ( θ ) = 0.0396 0.1990 .
  53. sin ( 78.95 ) 0.981
  54. cos ( 2.01 ) 0.425
  55. sin ( 392.994 ) 0.291
  56. cos ( 207 ) 0.891
  57. sin ( π ) 0.055
  58. cos ( e ) 0.912
  59. One solution is g ( t ) = 3 t and h ( t ) = sin ( 2 t ) .
  60. One solution is g ( θ ) = 3 cos ( θ ) and h ( θ ) = sin ( 4 θ ) .
  61. One solution is g ( t ) = e 0.1 t and h ( t ) = sin ( 3 t ) .
  62. One solution is f ( t ) = sin ( t ) and g ( t ) = t .
  63. One solution is f ( θ ) = 3 cos ( θ ) and g ( θ ) = θ .
  64. As we zoom in towards 0 , the average rate of change of sin ( k t ) approaches k .

    S ( t ) [ 0.1 , 0.1 ] [ 0.01 , 0.01 ] [ 0.001 , 0.001 ] sin ( t ) 0.9983 1 1 sin ( 2 t ) 1.9867 1.9999 2 sin ( 3 t ) 2.9552 2.9995 3 sin ( 4 t ) 3.8942 3.9989 4

  65. r = 1.125 inches, ω = 9000 π radians minute , x = 1.125 cos ( 9000 π t ) , y = 1.125 sin ( 9000 π t ) . Here x and y are measured in inches and t is measured in minutes.
  66. r = 28 inches, ω = 2 π 3 radians second , x = 28 cos ( 2 π 3 t ) , y = 28 sin ( 2 π 3 t ) . Here x and y are measured in inches and t is measured in seconds.
  67. r = 1.25 inches, ω = 14400 π radians minute , x = 1.25 cos ( 14400 π t ) , y = 1.25 sin ( 14400 π t ) . Here x and y are measured in inches and t is measured in minutes.
  68. r = 64 feet, ω = 4 π 127 radians second , x = 64 cos ( 4 π 127 t ) , y = 64 sin ( 4 π 127 t ) . Here x and y are measured in feet and t is measured in seconds

Adapted from Precalculus, Preliminary 4th Edition (integrated calculus), by Carl Stitz and Jeff Zeager (stitz-zeager.com), licensed under CC BY-NC-SA 3.0. Changes were made: reformatted as an accessible XYZ web edition. License: CC-BY-NC-SA-3.0.

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