1.5 Trigonometric Functions

Coming Concepts

  • •

    Convert angle measures between degrees and radians.

  • •

    Recognize the triangular and circular definitions of the basic trigonometric functions.

  • •

    Write the basic trigonometric identities.

  • •

    Identify the graphs and periods of the trigonometric functions.

  • •

    Describe the shift of a sine or cosine graph from the equation of the function.

Trigonometric functions are used to model many phenomena, including sound waves, vibrations of strings, alternating electrical current, and the motion of pendulums. In fact, almost any repetitive, or cyclical, motion can be modeled by some combination of trigonometric functions. In this section, we define the six basic trigonometric functions and look at some of the main identities involving these functions.

1.5.1 Radian Measure

To use trigonometric functions, we first must understand how to measure the angles. Although we can use both radians and degrees, radians are a more natural measurement because they are related directly to the unit circle, a circle with radius 1. The radian measure of an angle is defined as follows. Given an angle θ, let s be the length of the corresponding arc on the unit circle (Figure 1.55). We say the angle corresponding to the arc of length 1 has radian measure 1.

s1θ=s rad
Figure 1.55: The radian measure of an angle θ is the arc length s of the associated arc on the unit circle.

Since an angle of 360∘ corresponds to the circumference of a circle, or an arc of length 2⁢π, we conclude that an angle with a degree measure of 360∘ has a radian measure of 2⁢π. Similarly, we see that 180∘ is equivalent to π radians. Table 1.10 shows the relationship between common degree and radian values.

Table 1.10: Common Angles Expressed in Degrees and Radians
DegreesRadiansDegreesRadians001202⁢π/330π/61353⁢π/445π/41505⁢π/660π/3180π90π/2
Example 1.5.1 (Converting between Radians and Degrees).


  1. (a)

    Express 225∘ using radians.

  2. (b)

    Express 5⁢π/3 rad using degrees.

Solution: Use the fact that 180∘ is equivalent to π radians as a conversion factor: 1=π⁢rad180∘=180∘π⁢rad.

  1. (a)

    225=∘225⋅∘π180∘=5⁢π4 rad

  2. (b)

    5⁢π3 rad = 5⁢π3⋅180∘π=300∘

Checkpoint 1.5.1.

Express 210∘ using radians. Express 11⁢π/6 rad using degrees.

Hint: π radians is equal to 180.∘

1.5.2 The Six Basic Trigonometric Functions

Trigonometric functions allow us to use angle measures, in radians or degrees, to find the coordinates of a point on any circle—not only on a unit circle—or to find an angle given a point on a circle. They also define the relationship among the sides and angles of a triangle.

To define the trigonometric functions, first consider the unit circle centered at the origin and a point P=(x,y) on the unit circle. Let θ be an angle with an initial side that lies along the positive x-axis and with a terminal side that is the line segment O⁢P. An angle in this position is said to be in standard position (Figure 1.56). We can then define the values of the six trigonometric functions for θ in terms of the coordinates x and y.

x-axisy-axisO1P=(x,y)θ
Figure 1.56: The angle θ is in standard position. The values of the trigonometric functions for θ are defined in terms of the coordinates x and y.
Definition.

Let P=(x,y) be a point on the unit circle centered at the origin O. Let θ be an angle with an initial side along the positive x-axis and a terminal side given by the line segment O⁢P. The trigonometric functions are then defined as

sin⁡θ =y csc⁡θ =1y
cos⁡θ =x sec⁡θ =1x
tan⁡θ =yx cot⁡θ =xy

If x=0,sec⁡θ and tan⁡θ are undefined. If y=0, then cot⁡θ and csc⁡θ are undefined.

We can see that for a point P=(x,y) on a circle of radius r with a corresponding angle θ, we can also define cos⁡θ and sin⁡θ this way

cos⁡θ=xr⁢ and ⁢sin⁡θ=yr.

Note that we can define the other trigonometric functions in a similar way, by replacing x or y in the original definition with x/r or y/r, (see Figure 1.57). Also note that we can convert the other direction to get

x=r⁢cos⁡θ⁢ and ⁢y=r⁢sin⁡θ

and this holds for all circles.

x-axisy-axisP=(x,y)=(r⁢cos⁡θ,r⁢sin⁡θ)xyθ1r
Figure 1.57: For a point P=(x,y) on a circle of radius r, the coordinates x and y satisfy x=r⁢cos⁡θ and y=r⁢sin⁡θ.

Table 1.11 shows the values of sine and cosine at the major angles in the first quadrant. From this table, we can determine the values of sine and cosine at the corresponding angles in the other quadrants. The values of the other trigonometric functions are calculated easily from the values of sin⁡θ and cos⁡θ.

Table 1.11: Values of sin⁡θ and cos⁡θ at Major Angles θ in the First Quadrant
θsin⁡θcos⁡θ001π61232π42222π33212π210
Example 1.5.2 (Evaluating Trigonometric Functions).


Evaluate each of the following expressions.

  1. (a)

    sin⁡(2⁢π3)

  2. (b)

    cos⁡(−5⁢π6)

  3. (c)

    tan⁡(15⁢π4)

Solution:

  1. (a)

    On the unit circle, the angle θ=2⁢π3 corresponds to the point (−12,32). Therefore, sin⁡(2⁢π3)=y=32.

    xy1P=(−1/2,3/2)θ=2⁢π/3
    Figure 1.58:
  2. (b)

    An angle θ=−5⁢π6 corresponds to a revolution in the negative direction, as shown. Therefore, cos⁡(−5⁢π6)=x=−32.

    xy1P=(−3/2,−1/2)θ=−5⁢π/6
    Figure 1.59:
  3. (c)

    An angle θ=15⁢π4=2⁢π+7⁢π4. Therefore, this angle corresponds to more than one revolution, as shown. Knowing the fact that an angle of 7⁢π4 corresponds to the point (22,−22), we can conclude that tan⁡(15⁢π4)=yx=−1.

    xy1P=(2/2,−2/2)θ=15⁢π4
    Figure 1.60:
Checkpoint 1.5.2.

Evaluate cos⁡(3⁢π/4) and sin⁡(−π/6).

Hint: Look at angles on the unit circle.

As mentioned earlier, the ratios of the side lengths of a right triangle can be expressed in terms of the trigonometric functions evaluated at either of the acute angles of the triangle. Let θ be one of the acute angles. Let A be the length of the adjacent leg, O be the length of the opposite leg, and H be the length of the hypotenuse. By inscribing the triangle into a circle of radius H, as shown in Figure 1.61, we see that A,H, and O satisfy the following relationships with θ:

sin⁡θ=OH csc⁡θ=HO
cos⁡θ=AH sec⁡θ=HA
tan⁡θ=OA cot⁡θ=AO
xyHOAθ
Figure 1.61: By inscribing a right triangle in a circle, we can express the ratios of the side lengths in terms of the trigonometric functions evaluated at θ.
Example 1.5.3 (Constructing a Wooden Ramp).


A wooden ramp is to be built with one end on the ground and the other end at the top of a short staircase. If the top of the staircase is 4 ft from the ground and the angle between the ground and the ramp is to be 10∘, how long does the ramp need to be?

Solution: Let x denote the length of the ramp. In the following image, we see that x needs to satisfy the equation sin(10)∘=4/x. Solving this equation for x, we see that x=4/sin(10)∘≈23.035 ft.

xθ=10∘4 feet
Figure 1.62:
Checkpoint 1.5.3.

A house painter wants to lean a 20-ft ladder against a house. If the angle between the base of the ladder and the ground is to be 60∘, how far from the house should she place the base of the ladder?

Hint: Draw a right triangle with hypotenuse 20.

1.5.3 Trigonometric Identities

A trigonometric identity is an equation involving trigonometric functions that is true for all angles θ for which the functions are defined. We can use the identities to help us solve or simplify equations. The main trigonometric identities are listed next.

Rule 1.5.1 (Trigonometric Identities).

Reciprocal identities

tan⁡θ=sin⁡θcos⁡θ cot⁡θ=cos⁡θsin⁡θ
csc⁡θ=1sin⁡θ sec⁡θ=1cos⁡θ

Pythagorean identities

sin2⁡θ+cos2⁡θ=11+tan2⁡θ=sec2⁡θ1+cot2⁡θ=csc2⁡θ

Addition and subtraction formulas

sin⁡(α±β)=sin⁡α⁢cos⁡β±cos⁡α⁢sin⁡β
cos⁡(α±β)=cos⁡α⁢cos⁡β∓sin⁡α⁢sin⁡β

Double-angle formulas

sin⁡(2⁢θ)=2⁢sin⁡θ⁢cos⁡θ
cos⁡(2⁢θ)=2⁢cos2⁡θ−1=1−2⁢sin2⁡θ=cos2⁡θ−sin2⁡θ
Example 1.5.4 (Solving Trigonometric Equations).


For each of the following equations, use a trigonometric identity to find all solutions.

  1. (a)

    1+cos⁡(2⁢θ)=cos⁡θ

  2. (b)

    sin⁡(2⁢θ)=tan⁡θ

Solution:

  1. (a)

    Using the double-angle formula for cos⁡(2⁢θ), we see that θ is a solution of

    1+cos⁡(2⁢θ)=cos⁡θ

    if and only if

    1+2⁢cos2⁡θ−1=cos⁡θ,

    which is true if and only if

    2⁢cos2⁡θ−cos⁡θ=0.

    To solve this equation, it is important to note that we need to factor the left-hand side and not divide both sides of the equation by cos⁡θ. The problem with dividing by cos⁡θ is that it is possible that cos⁡θ is zero. In fact, if we did divide both sides of the equation by cos⁡θ, we would miss some of the solutions of the original equation. Factoring the left-hand side of the equation, we see that θ is a solution of this equation if and only if

    cos⁡θ⁢(2⁢cos⁡θ−1)=0.

    Since cos⁡θ=0 when

    θ=π2,π2±π,π2±2⁢π,…,

    and cos⁡θ=1/2 when

    θ=π3,π3±2⁢π,…⁢ or ⁢θ=−π3,−π3±2⁢π,…,

    we conclude that the set of solutions to this equation is

    θ=π2+n⁢π,θ=π3+2⁢n⁢π, and ⁢θ=−π3+2⁢n⁢π,n=0,±1,±2,….
  2. (b)

    Using the double-angle formula for sin⁡(2⁢θ) and the reciprocal identity for tan⁡(θ), the equation can be written as

    2⁢sin⁡θ⁢cos⁡θ=sin⁡θcos⁡θ.

    To solve this equation, we multiply both sides by cos⁡θ to eliminate the denominator, and say that if θ satisfies this equation, then θ satisfies the equation

    2⁢sin⁡θ⁢cos2⁡θ−sin⁡θ=0.

    However, we need to be a little careful here. Even if θ satisfies this new equation, it may not satisfy the original equation because, to satisfy the original equation, we would need to be able to divide both sides of the equation by cos⁡θ. However, if cos⁡θ=0, we cannot divide both sides of the equation by cos⁡θ. Therefore, it is possible that we may arrive at extraneous solutions. So, at the end, it is important to check for extraneous solutions. Returning to the equation, it is important that we factor sin⁡θ out of both terms on the left-hand side instead of dividing both sides of the equation by sin⁡θ. Factoring the left-hand side of the equation, we can rewrite this equation as

    sin⁡θ⁢(2⁢cos2⁡θ−1)=0.

    Therefore, the solutions are given by the angles θ such that sin⁡θ=0 or cos2⁡θ=1/2. The solutions of the first equation are θ=0,±π,±2⁢π,…. The solutions of the second equation are θ=π/4,(π/4)±(π/2),(π/4)±π,…. After checking for extraneous solutions, the set of solutions to the equation is

    θ=n⁢πandθ=π4+n⁢π2,n=0,±1,±2,….
Checkpoint 1.5.4.

Find all solutions to the equation cos⁡(2⁢θ)=sin⁡θ.

Hint: Use the double-angle formula for cosine.

Example 1.5.5 (Proving a Trigonometric Identity).


Prove the trigonometric identity 1+tan2⁡θ=sec2⁡θ.

Solution: We start with the identity

sin2⁡θ+cos2⁡θ=1.

Dividing both sides of this equation by cos2⁡θ, we obtain

sin2⁡θcos2⁡θ+1=1cos2⁡θ.

Since sin⁡θ/cos⁡θ=tan⁡θ and 1/cos⁡θ=sec⁡θ, we conclude that

tan2⁡θ+1=sec2⁡θ.
Checkpoint 1.5.5.

Prove the trigonometric identity 1+cot2⁡θ=csc2⁡θ.

Hint: Divide both sides of the identity sin2⁡θ+cos2⁡θ=1 by sin2⁡θ.

1.5.4 Graphs and Periods of the Trigonometric Functions

We have seen that as we travel around the unit circle, the values of the trigonometric functions repeat. We can see this pattern in the graphs of the functions. Let P=(x,y) be a point on the unit circle and let θ be the corresponding angle . Since the angle θ and θ+2⁢π correspond to the same point P, the values of the trigonometric functions at θ and at θ+2⁢π are the same. Consequently, the trigonometric functions are periodic functions The period of a function f is defined to be the smallest positive value p such that f⁢(x+p)=f⁢(x) for all values x in the domain of f. The sine, cosine, secant, and cosecant functions have a period of 2⁢π. Since the tangent and cotangent functions repeat on an interval of length π, their period is π (Figure 1.63).

−2⁢π−3⁢π2−π−π2π2π3⁢π22⁢π−0.20.2sin⁡(x) −2⁢π−3⁢π2−π−π2π2π3⁢π22⁢π0.960.981cos⁡(x)
−2⁢π−3⁢π2−π−π2π2π3⁢π22⁢π−22csc⁡(x) −2⁢π−3⁢π2−π−π2π2π3⁢π22⁢π−22sec⁡(x)
−2⁢π−3⁢π2−π−π2π2π3⁢π22⁢π−22tan⁡(x) −2⁢π−3⁢π2−π−π2π2π3⁢π22⁢π−22cot⁡(x)
Figure 1.63: The six trigonometric functions are periodic.

Just as with algebraic functions, we can apply transformations to trigonometric functions. In particular, consider the following function:

f⁢(x)=A⁢cos⁡(B⁢(x−α))+C. (1.10)

In Figure 1.64, the constant α causes a horizontal or phase shift. The factor B changes the period. This transformed sine function will have a period 2⁢π/|B|. The factor A results in a vertical stretch by a factor of |A|. We say |A| is the “amplitude of f.” The constant C causes a vertical shift.

x-axisy-axis vertical shift C−ACC+A amplitude =A period = 2⁢π/|B| horizontal shift (not unique)
Figure 1.64: A graph of a general cosine function.

Notice in Figure 1.63 that the graph of y=cos⁡x is the graph of y=sin⁡x shifted to the left π/2 units. Therefore, we can write cos⁡x=sin⁡(x+π/2). Similarly, we can view the graph of y=sin⁡x as the graph of y=cos⁡x shifted right π/2 units, and state that sin⁡x=cos⁡(x−π/2).

A shifted sine curve arises naturally when graphing the number of hours of daylight in a given location as a function of the day of the year. For example, suppose a city reports that June 21 is the longest day of the year with 15.7 hours and December 21 is the shortest day of the year with 8.3 hours. It can be shown that the function

h⁢(t)=3.7⁢sin⁡(2⁢π365⁢(t−80.5))+12

is a model for the number of hours of daylight h as a function of day of the year t (Figure 1.65).

06012018024030036005101520h⁢(t)=3.7⁢sin⁡(2⁢π365⁢(t−80.5))+12Day of the yearNumber of daylight hours
Figure 1.65: The hours of daylight as a function of day of the year can be modeled by a shifted sine curve.
Example 1.5.6 (Sketching the Graph of a Transformed Sine Curve).


Sketch a graph of f⁢(x)=3⁢sin⁡(2⁢(x−π4))+1.

Solution: This graph is a phase shift of y=sin⁡(x) to the right by π/4 units, followed by a horizontal compression by a factor of 2, a vertical stretch by a factor of 3, and then a vertical shift by 1 unit. The period of f is π.

−3⁢π/2−π−π/2π/2π3⁢π/22⁢π−224f⁢(x)=3⁢sin⁡(2⁢(x−π4))+1xy
Figure 1.66:
Checkpoint 1.5.6.

Describe the relationship between the graph of f⁢(x)=3⁢sin⁡(4⁢x)−5 and the graph of y=sin⁡(x).

Hint: The graph of f can be sketched using the graph of y=sin⁡(x) and a sequence of three transformations.

1.5.5 Inverse Trigonometric Functions

The six basic trigonometric functions are periodic, and therefore they are not one-to-one. However, if we restrict the domain of a trigonometric function to an interval where it is one-to-one, we can define its inverse. Consider the sine function (Figure 1.63). The sine function is one-to-one on an infinite number of intervals, but the standard convention is to restrict the domain to the interval [−π/2,π/2]. By doing so, we define the inverse sine function on the domain [−1,1] such that for any x in the interval [−1,1], the inverse sine function tells us which angle θ in the interval [−p⁢i/2,π/2] satisfies sin⁡θ=x. Similarly, we can restrict the domains of the other trigonometric functions to define inverse trigonometric functions, which are functions that tell us which angle in a certain interval has a specified trigonometric value.

Definition.

The inverse sine function, denoted sin−1 or arcsin, and the inverse cosine function, denoted cos−1 or arccos, are defined on the domain D={x∣−1≤x≤1} as follows:

sin−1⁡(x)=y⁢ if and only if⁢sin⁡(y)=x⁢ and −π2≤y≤π2; (1.11)
cos−1⁡(x)=y⁢ if and only if⁢cos⁡(y)=x⁢ and ⁢0≤y≤π.

The inverse tangent function, denoted tan−1 or arctan, and inverse cotangent function, denoted cot−1 or arccot, are defined on the domain D={x∣−∞<x<∞} as follows:

tan−1⁡(x)=y⁢ if and only if⁢tan⁡(y)=x⁢ and −π2<y<π2; (1.12)
cot−1⁡(x)=y⁢ if and only if⁢cot⁡(y)=x⁢ and ⁢0<y<π.

The inverse cosecant function, denoted csc−1 or arccsc, and inverse secant function, denoted sec−1 or arcsec, are defined on the domain D={x∣|x|≥1} as follows:

csc−1⁡(x)=y⁢ if and only if⁢csc⁡(y)=x⁢ and −π2≤y≤π2,y≠0; (1.13)
sec−1⁡(x)=y⁢ if and only if⁢sec⁡(y)=x⁢ and ⁢0≤y≤π,y≠π/2.

To graph the inverse trigonometric functions, we use the graphs of the trigonometric functions restricted to the domains defined earlier and reflect the graphs about the line y=x (Figure 1.67).

−11−π/2π/2sin−1⁡(x)
−11π/2πcos−1⁡(x)
−11−π/2π/2tan−1⁡(x)
−11π/2πcot−1⁡(x)
−11−π/2π/2csc−1⁡(x)
−11π/2πsec−1⁡(x)
Figure 1.67: The graph of each of the inverse trigonometric functions is a reflection about the line y=x of the corresponding restricted trigonometric function.
External Resource.

Go to the following site for more comparisons of functions and their inverses.

When evaluating an inverse trigonometric function, the output is an angle. For example, to evaluate cos−1⁡(1/2), we need to find an angle θ such that cos⁡θ=1/2. Clearly, many angles have this property. However, given the definition of cos−1, we need the angle θ that not only solves this equation, but also lies in the interval [0,π]. We conclude that cos−1⁡(1/2)=π/3.

We now consider a composition of a trigonometric function and its inverse. For example, consider the two expressions sin⁡(sin−1⁡(2/2)) and sin−1⁡(sin⁡(π)). For the first one, we simplify as follows:

sin⁡(sin−1⁡(2/2))=sin⁡(π/4)=22.

For the second one, we have

sin−1⁡(sin⁡(π))=sin−1⁡(0)=0.

The inverse function is supposed to “undo” the original function, so why isn’t sin−1⁡(sin⁡(π))=π? Recalling our definition of inverse functions, a function f and its inverse f−1 satisfy the conditions f⁢(f−1⁢(y))=y for all y in the domain of f−1 and f−1⁢(f⁢(x))=x for all x in the domain of f, so what happened here? The issue is that the inverse sine function, sin−1, is the inverse of the restricted sine function defined on the domain [−π/2,π/2]. Therefore, for x in the interval [−π/2,π/2], it is true that sin−1⁡(sin⁡x)=x. However, for values of x outside this interval, the equation does not hold, even though sin−1⁡(sin⁡x) is defined for all real numbers x.

What about sin⁡(sin−1⁡y)? Does that have a similar issue? The answer is n⁢o. Since the domain of sin−1 is the interval [−1,1], we conclude that sin⁡(sin−1⁡y)=y if −1≤y≤1 and the expression is not defined for other values of y. To summarize,

sin⁡(sin−1⁡y)=y⁢ if −1≤y≤1

and

sin−1⁡(sin⁡x)=x⁢ if −π2≤x≤π2.

Similarly, for the cosine function,

cos⁡(cos−1⁡y)=y⁢ if −1≤y≤1

and

cos−1⁡(cos⁡x)=x⁢ if ⁢0≤x≤π.

Similar properties hold for the other trigonometric functions and their inverses.

Example 1.5.7 (Evaluating Expressions Involving Inverse Trigonometric Functions).


Evaluate each of the following expressions.

  1. (a)

    sin−1(−3/2

  2. (b)

    tan⁡(tan−1⁡(−1/3))

  3. (c)

    cos−1⁡(cos⁡(5⁢π/4))

  4. (d)

    sin−1⁡(cos⁡(2⁢π/3))

Solution:

  1. (a)

    Evaluating sin−1⁡(−3/2) is equivalent to finding the angle θ such that sin⁡θ=−3/2 and −π/2≤θ≤π/2. The angle θ=−π/3 satisfies these two conditions. Therefore, sin−1⁡(−3/2)=−π/3.

  2. (b)

    First we use the fact that tan−1⁡(−1/3)=−π/6. Then tan⁡(π/6)=−1/3. Therefore, tan⁡(tan−1⁡(−1/3))=−1/3.

  3. (c)

    To evaluate cos−1⁡(cos⁡(5⁢π/4)), first use the fact that cos⁡(5⁢π/4)=−2/2. Then we need to find the angle θ such that cos⁡(θ)=−2/2 and 0≤θ≤π. Since 3⁢π/4 satisfies both these conditions, we have cos⁡(cos−1⁡(5⁢π/4))=cos⁡(cos−1⁡(−2/2))=3⁢π/4.

  4. (d)

    Since cos⁡(2⁢π/3)=−1/2, we need to evaluate sin−1⁡(−1/2). That is, we need to find the angle θ such that sin⁡(θ)=−1/2 and −π/2≤θ≤π/2. Since −π/6 satisfies both these conditions, we can conclude that sin−1⁡(cos⁡(2⁢π/3))=sin−1⁡(−1/2)=−π/6.

Key Concepts

  • •

    Radian measure is defined such that the angle associated with the arc of length 1 on the unit circle has radian measure 1. An angle with a degree measure of 180∘ has a radian measure of π rad.

  • •

    For acute angles θ, the values of the trigonometric functions are defined as ratios of two sides of a right triangle in which one of the acute angles is θ.

  • •

    For a general angle θ, let (x,y) be a point on a circle of radius r corresponding to this angle θ. The trigonometric functions can be written as ratios involving x,y, and r.

  • •

    The trigonometric functions are periodic. The sine, cosine, secant, and cosecant functions have period 2⁢π. The tangent and cotangent functions have period π.

Key Equations

  • •

    Generalized sine function

    f⁢(x)=A⁢sin⁡(B⁢(x−α))+C

Glossary

periodic function

a function is periodic if it has a repeating pattern as the values of x move from left to right

radians

for a circular arc of length s on a circle of radius 1, the radian measure of the associated angle θ is s

trigonometric functions

functions of an angle defined as ratios of the lengths of the sides of a right triangle

trigonometric identity

an equation involving trigonometric functions that is true for all angles θ for which the functions in the equation are defined