AP Precalculus ›  Unit 3  ·  30–35% of the AP Exam

Unit 3 Trigonometric and Polar Functions

Everything here starts with a circle. Follow a point around the unit circle to build sine, cosine, and tangent, use them to model anything that repeats, and then switch to the polar coordinate system, where angles and radii replace left-right and up-down.

📝 30–35% of AP Exam🕐 35–50 Class Periods📺 15 Episodes🧮 Radian Mode
EP.3.1

Periodic Phenomena

Tides, clocks, and traffic all repeat. A relationship is periodic when outputs show a repeating pattern over equal-length input intervals, and the period is the length of one full cycle.

PeriodOne cycle determines allGraphing from a description
🕐 2 class daysOpen lesson →
EP.3.2

Sine, Cosine, and Tangent

Put an angle in standard position on the unit circle and measure it in radians. The sine, cosine, and tangent come straight from the point where the angle's terminal ray meets the circle.

Standard positionRadian measuretan θ = sin θ / cos θ
🕐 2–3 class daysOpen lesson →
EP.3.3

Sine and Cosine Function Values

On a circle of radius r, the point at angle θ is (r cos θ, r sin θ). Use isosceles right and equilateral triangles to find exact values at multiples of π/4 and π/6.

(r cos θ, r sin θ)Multiples of π/4Multiples of π/6
🕐 2–3 class daysOpen lesson →
EP.3.4

Sine and Cosine Function Graphs

Unwrap the unit circle and the sine and cosine graphs appear. Both oscillate between −1 and 1, tracking the vertical and horizontal displacement of a point as it travels around the circle.

f(θ) = sin θg(θ) = cos θOscillates between −1 and 1
🕐 2–3 class daysOpen lesson →
EP.3.5

Sinusoidal Functions

Sine and cosine are the parent sinusoidal functions. Describe them with period, frequency, amplitude, and midline, and recognize that sine is odd while cosine is even.

AmplitudePeriod & frequencyMidline
🕐 2–3 class daysOpen lesson →
EP.3.6

Sinusoidal Function Transformations

In a·sin(b(θ + c)) + d, each constant does one job. Read amplitude, period, phase shift, and vertical shift straight off the equation, and build the function from them.

a sin(b(θ + c)) + dPhase shift −cPeriod 2π/|b|
🕐 2–3 class daysOpen lesson →
EP.3.7

Sinusoidal Function Context and Data Modeling

Model a periodic situation. Maxima and minima give you the amplitude and vertical shift, the spacing between peaks gives the period, and a known point gives the phase shift. Or use sinusoidal regression.

Estimating a, b, c, dSinusoidal regressionContextual domain
🕐 2–3 class daysOpen lesson →
EP.3.8

The Tangent Function

Tangent is the slope of the terminal ray. It has period π, vertical asymptotes wherever cosine is zero, and its transformations work a little differently than sine and cosine.

Period πAsymptotes at π/2 + πkTransforming tan θ
🕐 2 class daysOpen lesson →
EP.3.9

Inverse Trigonometric Functions

Arcsine, arccosine, and arctangent turn a trig value back into an angle. Because trig functions are periodic, each is only invertible after you restrict its domain.

arcsin, arccos, arctanRestricted domainsOutput is an angle
🕐 2–3 class daysOpen lesson →
EP.3.10

Trigonometric Equations and Inequalities

Use inverse trig functions to solve equations and inequalities, then account for periodicity to find every solution. In a context, the domain often limits the answers.

Infinitely many solutionsDomain restrictionsTrig inequalities
🕐 3–4 class daysOpen lesson →
EP.3.11

The Secant, Cosecant, and Cotangent Functions

The reciprocal functions secant, cosecant, and cotangent each have vertical asymptotes where their parent function is zero. Learn their graphs, ranges, and domains.

sec θ = 1/cos θcsc θ = 1/sin θcot θ = cos θ / sin θ
🕐 2 class daysOpen lesson →
EP.3.12

Equivalent Representations of Trigonometric Functions

Rewrite trig expressions using the Pythagorean identity and the sine and cosine sum identities, and use those forms to solve equations and verify other identities.

sin²θ + cos²θ = 1Sum identitiesDouble-angle identities
🕐 3–4 class daysOpen lesson →
EP.3.13

Trigonometry and Polar Coordinates

Locate a point with a radius and an angle instead of left-right and up-down. Convert between polar and rectangular coordinates, and see complex numbers as points in a plane.

(r, θ)x = r cos θ, y = r sin θComplex plane
🕐 2–3 class daysOpen lesson →
EP.3.14

Polar Function Graphs

In r = f(θ), the input is an angle and the output is a signed radius. Graph polar functions on a restricted domain and compare them with their rectangular graphs.

r = f(θ)Signed radiusRestricting θ
🕐 2–3 class daysOpen lesson →
EP.3.15

Rates of Change in Polar Functions

Is a point moving toward the origin or away from it? Use the sign of r and whether it's increasing or decreasing to find out, and use average rate of change to describe how the radius changes per radian.

Toward / away from originRelative extrema of rRate of change of r
🕐 2–3 class daysOpen lesson →
✅ Progress Checks in AP Classroom
Part 1 covers Topics 3.1–3.7 (21 multiple-choice, 2 free-response). Part 2 covers Topics 3.8–3.15 (24 multiple-choice, 2 free-response). Complete each one after you finish its topics, then review the rationales for anything you missed.