Trigonometric Identities and Equations

⚡ Key Takeaways

Trigonometric identities are equations relating trig functions that hold for all valid inputs; trig equations ask for the specific inputs that make a relation true. Master the Pythagorean, sum/difference, double/half-angle identities and you can simplify any expression and solve any standard trig equation. Used everywhere: physics waves, engineering, navigation, computer graphics. Foundational work spans Hipparchus (c. 150 BC) through Euler (1748).

💡 The Core Insight

Sine and cosine are the coordinates of a point moving around the unit circle. Because the circle has radius 1, the Pythagorean theorem instantly gives sin⁡2+cos⁡2=1\sin^2+\cos^2=1. Because rotating by angle AA then by angle BB is the same as rotating by A+BA+B, the sum formulas follow. Every identity is a geometric or algebraic consequence of these two facts. An identity is a structural truth; an equation is a question about location.

Formal Statement

DefinitionUnit-Circle Definitions

For an angle θ\theta measured counterclockwise from the positive xx-axis, let P=(x,y)P=(x,y) be the point where the terminal ray meets the unit circle x2+y2=1x^2+y^2=1. Then:

1
cos⁡θ=x,sin⁡θ=y,tan⁡θ=yx=sin⁡θcos⁡θ\quad \cos\theta = x,\qquad \sin\theta = y,\qquad \tan\theta = \frac{y}{x}=\frac{\sin\theta}{\cos\theta}

Derivation hint: These are definitions, but note tan⁡\tan is the slope of the terminal ray, undefined when x=cos⁡θ=0x=\cos\theta=0. The reciprocal functions are:

2
csc⁡θ=1sin⁡θ,sec⁡θ=1cos⁡θ,cot⁡θ=1tan⁡θ=cos⁡θsin⁡θ\quad \csc\theta=\frac{1}{\sin\theta},\qquad \sec\theta=\frac{1}{\cos\theta},\qquad \cot\theta=\frac{1}{\tan\theta}=\frac{\cos\theta}{\sin\theta}

Derivation hint: Each is the multiplicative inverse of a primary function; domains exclude points where the denominator vanishes. Here θ\theta is a real number (radians) or angle measure; x,yx,y are real coordinates with x2+y2=1x^2+y^2=1.

TheoremThe Pythagorean Identities

For all θ\theta where the functions are defined:

3
sin⁡2θ+cos⁡2θ=1\quad \sin^2\theta + \cos^2\theta = 1

Derivation hint: Apply x2+y2=1x^2+y^2=1 with x=cos⁡θx=\cos\theta, y=sin⁡θy=\sin\theta.

4
1+tan⁡2θ=sec⁡2θ\quad 1 + \tan^2\theta = \sec^2\theta

Derivation hint: Divide [3] by cos⁡2θ\cos^2\theta.

5
1+cot⁡2θ=csc⁡2θ\quad 1 + \cot^2\theta = \csc^2\theta

Derivation hint: Divide [3] by sin⁡2θ\sin^2\theta.

TheoremSum and Difference Identities

For all angles A,BA,B:

6
cos⁡(A−B)=cos⁡Acos⁡B+sin⁡Asin⁡B\quad \cos(A-B) = \cos A\cos B + \sin A\sin B

Derivation hint: Compute the squared distance between unit-circle points at angles AA and BB two ways (law of cosines vs. coordinate distance).

7
cos⁡(A+B)=cos⁡Acos⁡B−sin⁡Asin⁡B\quad \cos(A+B) = \cos A\cos B - \sin A\sin B

Derivation hint: Replace BB with −B-B in [6], using cos⁡(−B)=cos⁡B\cos(-B)=\cos B, sin⁡(−B)=−sin⁡B\sin(-B)=-\sin B.

8
sin⁡(A±B)=sin⁡Acos⁡B±cos⁡Asin⁡B\quad \sin(A\pm B) = \sin A\cos B \pm \cos A\sin B

Derivation hint: Use the cofunction relation sin⁡ϕ=cos⁡(π2−ϕ)\sin\phi=\cos(\tfrac{\pi}{2}-\phi) and apply [6]/[7].

9
tan⁡(A±B)=tan⁡A±tan⁡B1∓tan⁡Atan⁡B\quad \tan(A\pm B) = \frac{\tan A \pm \tan B}{1 \mp \tan A\tan B}

Derivation hint: Divide [8] by [7] and simplify by dividing numerator and denominator by cos⁡Acos⁡B\cos A\cos B.

TheoremDouble- and Half-Angle Identities
10
sin⁡2θ=2sin⁡θcos⁡θ\quad \sin 2\theta = 2\sin\theta\cos\theta

Derivation hint: Set A=B=θA=B=\theta in [8] with the plus sign.

11
cos⁡2θ=cos⁡2θ−sin⁡2θ=1−2sin⁡2θ=2cos⁡2θ−1\quad \cos 2\theta = \cos^2\theta - \sin^2\theta = 1-2\sin^2\theta = 2\cos^2\theta - 1

Derivation hint: Set A=B=θA=B=\theta in [7]; obtain alternate forms using [3].

12
sin⁡2θ=1−cos⁡2θ2,cos⁡2θ=1+cos⁡2θ2\quad \sin^2\theta = \frac{1-\cos 2\theta}{2},\qquad \cos^2\theta = \frac{1+\cos 2\theta}{2}

Derivation hint: Solve the second and third forms of [11] for sin⁡2\sin^2 and cos⁡2\cos^2 (the power-reduction formulas).

13
sin⁡θ2=±1−cos⁡θ2,cos⁡θ2=±1+cos⁡θ2\quad \sin\frac{\theta}{2} = \pm\sqrt{\frac{1-\cos\theta}{2}},\qquad \cos\frac{\theta}{2} = \pm\sqrt{\frac{1+\cos\theta}{2}}

Derivation hint: Replace θ\theta with θ/2\theta/2 in [12] and take square roots; sign depends on the quadrant of θ/2\theta/2.

Why It Holds / Derivation

ProofDeriving the Difference Formula for Cosine — Equation 6

We prove cos⁡(A−B)=cos⁡Acos⁡B+sin⁡Asin⁡B\cos(A-B)=\cos A\cos B+\sin A\sin B using the unit circle and the distance formula. 1. Place two points on the unit circle: P=(cos⁡A,sin⁡A)P=(\cos A,\sin A) at angle AA, and Q=(cos⁡B,sin⁡B)Q=(\cos B,\sin B) at angle BB. 2. The angle between OPOP and OQOQ is A−BA-B. Compute the squared distance PQ2PQ^2 directly:

14
PQ2=(cos⁡A−cos⁡B)2+(sin⁡A−sin⁡B)2\quad PQ^2=(\cos A-\cos B)^2+(\sin A-\sin B)^2

Derivation hint: Distance formula between PP and QQ. 3. Expand: PQ2=cos⁡2A−2cos⁡Acos⁡B+cos⁡2B+sin⁡2A−2sin⁡Asin⁡B+sin⁡2BPQ^2=\cos^2A-2\cos A\cos B+\cos^2B+\sin^2A-2\sin A\sin B+\sin^2B. Group using [3] twice:

15
PQ2=2−2(cos⁡Acos⁡B+sin⁡Asin⁡B)\quad PQ^2 = 2 - 2(\cos A\cos B+\sin A\sin B)

Derivation hint: cos⁡2A+sin⁡2A=1\cos^2A+\sin^2A=1 and cos⁡2B+sin⁡2B=1\cos^2B+\sin^2B=1. 4. Now compute PQ2PQ^2 using the law of cosines in triangle OPQOPQ where ∣OP∣=∣OQ∣=1|OP|=|OQ|=1 and the included angle is A−BA-B:

16
PQ2=12+12−2(1)(1)cos⁡(A−B)=2−2cos⁡(A−B)\quad PQ^2 = 1^2+1^2-2(1)(1)\cos(A-B)=2-2\cos(A-B)

Derivation hint: Law of cosines c2=a2+b2−2abcos⁡Cc^2=a^2+b^2-2ab\cos C. 5. Equate [15] and [16]: 2−2(cos⁡Acos⁡B+sin⁡Asin⁡B)=2−2cos⁡(A−B)2-2(\cos A\cos B+\sin A\sin B)=2-2\cos(A-B). Cancel and divide by −2-2:

17
cos⁡(A−B)=cos⁡Acos⁡B+sin⁡Asin⁡B■\quad \cos(A-B)=\cos A\cos B+\sin A\sin B \qquad\blacksquare

Derivation hint: Subtract 2 from both sides, divide by −2-2. Every other sum/difference and multiple-angle identity follows algebraically from this one and [3].

∎
mathematician · Leonhard Euler | 1707–1783

Euler unified trigonometry with the exponential function through his celebrated formula eiθ=cos⁡θ+isin⁡θe^{i\theta}=\cos\theta+i\sin\theta. From this single relation, all trig identities become consequences of the exponential law ei(A+B)=eiAeiBe^{i(A+B)}=e^{iA}e^{iB}. Multiplying out the right side and matching real and imaginary parts instantly reproduces the sum formulas [7] and [8]. Euler's 1748 Introductio in analysin infinitorum standardized the modern function-based view of trigonometry — treating sin⁡\sin and cos⁡\cos as functions of a real variable rather than ratios in a particular triangle, which is exactly how we use them today.

Building Intuition

🧠 Intuition

Think of cos⁡θ\cos\theta and sin⁡θ\sin\theta as the shadow of a rotating clock hand of length 1: the horizontal shadow is the cosine, the vertical shadow is the sine. As the hand sweeps, the two shadows trade size, but the Pythagorean identity [3] guarantees the combined shadow always reconstructs a full unit length — the hand never stretches. The sum formulas answer: "If I know the shadows at angle AA and at angle BB, what are the shadows at A+BA+B?" The answer isn't simple addition — shadows interfere. Equation [7] says the new horizontal shadow is the product of the two horizontal shadows minus the product of the two vertical ones. That minus sign is the fingerprint of rotation, the same minus that appears in complex multiplication. For equations, switch viewpoints. Solving sin⁡θ=0.5\sin\theta=0.5 isn't simplifying — it's asking "where on the circle is the height exactly 0.50.5?" There are two such points per revolution and infinitely many revolutions, hence infinitely many solutions, which is why every trig equation answer carries a "+2πn+2\pi n" tail.

Figure
The unit circle showing cosine and sine as coordinates of point P at angle θ
θ P=(cos θ, sin θ) cos θ sin θ x y (0,0)

Worked Examples

ExampleProving an Identity by Simplification

Given: Prove the identity sin⁡θ1+cos⁡θ+1+cos⁡θsin⁡θ=2csc⁡θ\dfrac{\sin\theta}{1+\cos\theta} + \dfrac{1+\cos\theta}{\sin\theta} = 2\csc\theta.

Steps: 1. Combine the left side over a common denominator sin⁡θ(1+cos⁡θ)\sin\theta(1+\cos\theta):

18
LHS=sin⁡2θ+(1+cos⁡θ)2sin⁡θ(1+cos⁡θ)\quad \text{LHS}=\frac{\sin^2\theta + (1+\cos\theta)^2}{\sin\theta(1+\cos\theta)}

2. Expand the numerator: sin⁡2θ+1+2cos⁡θ+cos⁡2θ\sin^2\theta + 1 + 2\cos\theta + \cos^2\theta. 3. Apply [3], sin⁡2θ+cos⁡2θ=1\sin^2\theta+\cos^2\theta=1, so the numerator becomes 1+1+2cos⁡θ=2+2cos⁡θ=2(1+cos⁡θ)1 + 1 + 2\cos\theta = 2 + 2\cos\theta = 2(1+\cos\theta). 4. Substitute back:

19
LHS=2(1+cos⁡θ)sin⁡θ(1+cos⁡θ)=2sin⁡θ\quad \text{LHS}=\frac{2(1+\cos\theta)}{\sin\theta(1+\cos\theta)} = \frac{2}{\sin\theta}

5. By definition [2], 2sin⁡θ=2csc⁡θ\dfrac{2}{\sin\theta}=2\csc\theta.

sin⁡θ1+cos⁡θ+1+cos⁡θsin⁡θ=2csc⁡θ✓\boxed{\dfrac{\sin\theta}{1+\cos\theta}+\dfrac{1+\cos\theta}{\sin\theta}=2\csc\theta \quad\checkmark}
ExampleSolving a Trigonometric Equation

Given: Solve 2cos⁡2θ+cos⁡θ−1=02\cos^2\theta + \cos\theta - 1 = 0 for 0≤θ<2π0 \le \theta < 2\pi.

Steps: 1. Let u=cos⁡θu=\cos\theta. The equation becomes the quadratic 2u2+u−1=02u^2+u-1=0. 2. Factor: (2u−1)(u+1)=0(2u-1)(u+1)=0, so u=12u=\tfrac{1}{2} or u=−1u=-1. 3. Case cos⁡θ=12\cos\theta=\tfrac{1}{2}: On [0,2π)[0,2\pi) the cosine equals 12\tfrac12 at θ=π3\theta=\tfrac{\pi}{3} (1st quadrant) and θ=5π3\theta=\tfrac{5\pi}{3} (4th quadrant). 4. Case cos⁡θ=−1\cos\theta=-1: This occurs only at θ=π\theta=\pi. 5. Collect all solutions in the interval:

θ=π3, π, 5π3\boxed{\theta = \frac{\pi}{3},\ \pi,\ \frac{5\pi}{3}}

(If all real solutions were wanted, add +2πn+2\pi n, n∈Zn\in\mathbb{Z}, to each.)

Common Misconceptions

⚠️ Common mistake

An identity is not an equation to "solve." When asked to prove an identity, you may not move terms across the equals sign as if solving — that assumes the very thing you're proving. Instead, transform one side until it equals the other, or transform each side independently to a common third expression.

sin⁡2θ\sin^2\theta means (sin⁡θ)2(\sin\theta)^2, not sin⁡(θ2)\sin(\theta^2). The exponent applies to the function value. Also sin⁡−1θ\sin^{-1}\theta denotes the inverse function (arcsine), not 1/sin⁡θ=csc⁡θ1/\sin\theta=\csc\theta. This notational clash is a frequent source of error.

Never cancel a function across a sum. sin⁡(A+B)≠sin⁡A+sin⁡B\sin(A+B)\ne \sin A+\sin B. The sum formula [8] is the correct expansion.

Counterexample

A student claims sin⁡2θ=sin⁡θ\sqrt{\sin^2\theta}=\sin\theta. Test θ=3π2\theta=\tfrac{3\pi}{2}: here sin⁡θ=−1\sin\theta=-1, so sin⁡2θ=1\sin^2\theta=1 and 1=1≠−1\sqrt{1}=1\ne -1. The square root returns the non-negative root, so correctly sin⁡2θ=∣sin⁡θ∣\sqrt{\sin^2\theta}=|\sin\theta|. This same trap explains the ±\pm sign in the half-angle formulas [13] — the sign must be chosen according to the quadrant, not assumed positive.

Connections

connection

Trig identities sit at a busy crossroads. They are the algebraic engine behind Trigonometric Functions and depend directly on the geometry of The Unit Circle. In analysis, the power-reduction forms [12] are essential for integration — every integral of sin⁡2\sin^2 or cos⁡2\cos^2 in Integral Calculus is computed by replacing them with cos⁡2θ\cos 2\theta terms. The deepest link is to Complex Numbers via Euler's formula, which turns all of trigonometry into exponential algebra. The sum-to-product forms underpin Fourier Series, where any periodic signal decomposes into sines and cosines, and the double-angle relations connect to Rotation Matrices in Linear Algebra.

Real-World Applications

🔬 Where this appears

Historical Development

⏳ History
- c. 150 BC — Hipparchus of Nicaea compiles the first known table of chords, the ancestor of the sine table, to predict astronomical positions.
- c. 100 AD — Ptolemy states what is now equivalent to the sum and difference identities as "Ptolemy's theorem" on cyclic quadrilaterals in the Almagest.
- c. 500 AD — Aryabhata introduces the half-chord (the true sine), tabulating values and an early version of the half-angle relation in India.
- c. 1000 AD — Abu al-Wafa of Baghdad establishes the modern sine, tangent, secant relations and proves the double-angle and addition formulas geometrically.
- 1464 — Regiomontanus writes De triangulis omnimodis, the first European text treating trigonometry as a discipline independent of astronomy.
- 1593 — François Viète derives multiple-angle formulas and uses them to solve high-degree polynomial equations.
- 1722 — Abraham de Moivre publishes the formula (cos⁡θ+isin⁡θ)n=cos⁡nθ+isin⁡nθ(\cos\theta+i\sin\theta)^n=\cos n\theta+i\sin n\theta, linking powers to multiple angles.
- 1748 — Leonhard Euler unifies trigonometry with the exponential function via eiθ=cos⁡θ+isin⁡θe^{i\theta}=\cos\theta+i\sin\theta in the Introductio, recasting all identities as exponential algebra.
- 1822 — Joseph Fourier shows arbitrary periodic functions decompose into sines and cosines, making trig identities central to modern physics and engineering.

Subtleties & Limits

open-problem

The "subtleties" here are domain and inverse-function issues rather than unsolved research problems. The chief one: trig equations have infinitely many solutions because sin⁡\sin and cos⁡\cos are periodic, so any complete answer requires the general form θ0+2πn\theta_0 + 2\pi n. Restricting to a principal interval (as in the inverse functions arcsin⁡,arccos⁡,arctan⁡\arcsin,\arccos,\arctan) discards solutions, and students must consciously reintroduce them. A deeper subtlety: identities derived by squaring both sides may introduce extraneous solutions that satisfy the squared equation but not the original — every solution must be checked back in the unsquared form. Likewise, dividing by a trig function silently assumes it is nonzero and may lose solutions where that function equals zero. Finally, the half-angle sign ambiguity in [13] has no universal resolution; it can only be settled by knowing the quadrant of the half-angle, which is information outside the identity itself.

See Also

The Unit Circle · Trigonometric Functions · Inverse Trigonometric Functions · Complex Numbers · Law of Cosines · Fourier Series · Rotation Matrices · Radian Measure