Trigonometric Identities

⚡ Key Takeaways

One-line statement: Trigonometric identities are equations involving trigonometric functions that hold true for every value of the variable for which both sides are defined. Key result in words: From a single relationship — the Pythagorean identity sin⁡2θ+cos⁡2θ=1\sin^2\theta + \cos^2\theta = 1 — together with the addition formulas, the entire web of trigonometric identities can be derived. Where it applies: Simplifying expressions, solving trigonometric equations, evaluating integrals, modelling waves and oscillations, and rotating coordinates. Who/when: Rooted in Greek astronomy (Hipparchus, ~150 BCE) and Indian mathematics (Aryabhata, ~500 CE), formalized by Euler in the 18th century.

💡 The Core Insight

A point moving around the unit circle has coordinates (cos⁡θ,sin⁡θ)(\cos\theta, \sin\theta). Because that point always lies on the circle of radius 1, its coordinates obey x2+y2=1x^2 + y^2 = 1 at all times. Almost every trigonometric identity is a consequence of this geometric fact combined with how angles add when rotations are composed. Identities are the algebraic shadow of circular motion.

Formal Statement

DefinitionTrigonometric Functions on the Unit Circle

Let θ\theta be an angle measured counterclockwise from the positive xx-axis. The point where the terminal side of θ\theta meets the unit circle has coordinates (cos⁡θ,sin⁡θ)(\cos\theta, \sin\theta). The six functions are defined as:

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

Derivation hint: read the coordinates directly off the unit circle; tangent is the slope y/xy/x of the terminal ray.

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

Derivation hint: the reciprocal functions are defined as the multiplicative inverses of sine, cosine, and tangent respectively. Here xx and yy are the horizontal and vertical coordinates (dimensionless, since the radius is 1), and θ\theta is the angle (in radians or degrees).

TheoremThe Pythagorean Identity

For every real number θ\theta:

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

Derivation hint: apply the equation of the unit circle x2+y2=1x^2 + y^2 = 1 with x=cos⁡θx=\cos\theta, y=sin⁡θy=\sin\theta. Dividing [3] through by cos⁡2θ\cos^2\theta and by sin⁡2θ\sin^2\theta yields two companions:

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

Derivation hint: divide every term of [3] by cos⁡2θ\cos^2\theta and use tan⁡=sin⁡/cos⁡\tan = \sin/\cos, sec⁡=1/cos⁡\sec = 1/\cos.

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

Derivation hint: divide every term of [3] by sin⁡2θ\sin^2\theta and use cot⁡=cos⁡/sin⁡\cot = \cos/\sin, csc⁡=1/sin⁡\csc = 1/\sin.

TheoremAngle Addition Formulas

For all angles α\alpha and β\beta:

6
sin⁡(α±β)=sin⁡αcos⁡β±cos⁡αsin⁡β\quad \sin(\alpha \pm \beta) = \sin\alpha\cos\beta \pm \cos\alpha\sin\beta

Derivation hint: project a rotated unit vector onto the axes, or expand the real/imaginary parts of ei(α±β)=eiαe±iβe^{i(\alpha\pm\beta)} = e^{i\alpha}e^{\pm i\beta}.

7
cos⁡(α±β)=cos⁡αcos⁡β∓sin⁡αsin⁡β\quad \cos(\alpha \pm \beta) = \cos\alpha\cos\beta \mp \sin\alpha\sin\beta

Derivation hint: same as [6]; note the sign of the sine product reverses relative to the addition sign.

8
tan⁡(α±β)=tan⁡α±tan⁡β1∓tan⁡αtan⁡β\quad \tan(\alpha \pm \beta) = \frac{\tan\alpha \pm \tan\beta}{1 \mp \tan\alpha\tan\beta}

Derivation hint: divide [6] by [7] and then divide numerator and denominator by cos⁡αcos⁡β\cos\alpha\cos\beta.

TheoremDouble-Angle and Half-Angle Formulas

Setting β=α\beta = \alpha in [6] and [7]:

9
sin⁡2α=2sin⁡αcos⁡α\quad \sin 2\alpha = 2\sin\alpha\cos\alpha

Derivation hint: put β=α\beta=\alpha into the sine addition formula [6].

10
cos⁡2α=cos⁡2α−sin⁡2α=2cos⁡2α−1=1−2sin⁡2α\quad \cos 2\alpha = \cos^2\alpha - \sin^2\alpha = 2\cos^2\alpha - 1 = 1 - 2\sin^2\alpha

Derivation hint: put β=α\beta=\alpha into [7], then substitute sin⁡2α=1−cos⁡2α\sin^2\alpha = 1-\cos^2\alpha (or vice versa) using [3].

11
sin⁡2α=1−cos⁡2α2,cos⁡2α=1+cos⁡2α2\quad \sin^2\alpha = \frac{1-\cos 2\alpha}{2},\qquad \cos^2\alpha = \frac{1+\cos 2\alpha}{2}

Derivation hint: solve the two right-hand forms of [10] for sin⁡2α\sin^2\alpha and cos⁡2α\cos^2\alpha.

12
tan⁡α2=1−cos⁡αsin⁡α=sin⁡α1+cos⁡α\quad \tan\frac{\alpha}{2} = \frac{1-\cos\alpha}{\sin\alpha} = \frac{\sin\alpha}{1+\cos\alpha}

Derivation hint: replace α\alpha by α/2\alpha/2 in [11], take the ratio, and rationalize.

Why It Holds / Derivation

ProofDeriving the Cosine Addition Formula from Rotation

We prove cos⁡(α−β)=cos⁡αcos⁡β+sin⁡αsin⁡β\cos(\alpha - \beta) = \cos\alpha\cos\beta + \sin\alpha\sin\beta, from which all of [6]–[8] follow. 1. Place two points on the unit circle: P=(cos⁡α,sin⁡α)P = (\cos\alpha, \sin\alpha) and Q=(cos⁡β,sin⁡β)Q = (\cos\beta, \sin\beta). 2. The squared distance between them, by the distance formula, is

13
PQ2=(cos⁡α−cos⁡β)2+(sin⁡α−sin⁡β)2\quad PQ^2 = (\cos\alpha - \cos\beta)^2 + (\sin\alpha - \sin\beta)^2

Derivation hint: apply d2=(Δx)2+(Δy)2d^2 = (\Delta x)^2 + (\Delta y)^2 to the two unit-circle points. 3. Expanding and using [3] twice (once for each angle):

14
PQ2=2−2(cos⁡αcos⁡β+sin⁡αsin⁡β)\quad PQ^2 = 2 - 2(\cos\alpha\cos\beta + \sin\alpha\sin\beta)

Derivation hint: expand the squares, group cos⁡2+sin⁡2=1\cos^2+\sin^2 = 1 for each angle, collect the cross terms. 4. Now rotate the whole picture so QQ sits at angle 00, i.e. at (1,0)(1,0), and PP sits at angle (α−β)(\alpha - \beta). The distance is unchanged by rotation, so

15
PQ2=(cos⁡(α−β)−1)2+(sin⁡(α−β)−0)2=2−2cos⁡(α−β)\quad PQ^2 = (\cos(\alpha-\beta) - 1)^2 + (\sin(\alpha-\beta) - 0)^2 = 2 - 2\cos(\alpha-\beta)

Derivation hint: same distance formula applied to (cos⁡(α−β),sin⁡(α−β))(\cos(\alpha-\beta),\sin(\alpha-\beta)) and (1,0)(1,0); use [3]. 5. Equating [14] and [15] and cancelling the common 22:

16
cos⁡(α−β)=cos⁡αcos⁡β+sin⁡αsin⁡β■\quad \cos(\alpha-\beta) = \cos\alpha\cos\beta + \sin\alpha\sin\beta\qquad \blacksquare

Derivation hint: set the two expressions for PQ2PQ^2 equal and divide by −2-2. Replacing β\beta with −β-\beta (and using the even/odd properties below) gives the ++ version; the sine formulas follow from sin⁡θ=cos⁡(π2−θ)\sin\theta = \cos(\tfrac{\pi}{2}-\theta).

∎
DefinitionEven–Odd (Symmetry) Identities

Reflecting the angle through the xx-axis sends θ→−θ\theta \to -\theta, flipping the sign of yy but not xx:

17
cos⁡(−θ)=cos⁡θ,sin⁡(−θ)=−sin⁡θ,tan⁡(−θ)=−tan⁡θ\quad \cos(-\theta) = \cos\theta,\qquad \sin(-\theta) = -\sin\theta,\qquad \tan(-\theta) = -\tan\theta

Derivation hint: the point at −θ-\theta has the same xx-coordinate but the negated yy-coordinate. Cosine is even; sine and tangent are odd.

mathematician · Leonhard Euler | 1707–1783

Euler did more than anyone to turn trigonometry from a table-bound art into algebra. His formula eiθ=cos⁡θ+isin⁡θe^{i\theta} = \cos\theta + i\sin\theta (1748) reduces every identity above to ordinary rules for exponents: the addition formulas become eiαeiβ=ei(α+β)e^{i\alpha}e^{i\beta} = e^{i(\alpha+\beta)}, and the Pythagorean identity becomes ∣eiθ∣2=1|e^{i\theta}|^2 = 1. He also standardized the notation sin⁡\sin, cos⁡\cos, tan⁡\tan and treated the trig functions as analytic functions of a real (and complex) variable rather than as chords or half-chords of circles.

Building Intuition

🧠 Intuition

Picture a clock hand of length 1 sweeping around. Its tip's shadow on the floor is cos⁡θ\cos\theta and its shadow on the wall is sin⁡θ\sin\theta. As it turns, those two shadows trade lengths back and forth, but the hand's length never changes — and that unchanging length, squared, is exactly cos⁡2θ+sin⁡2θ=1\cos^2\theta + \sin^2\theta = 1. The addition formulas just describe what happens to the shadows when you turn the hand by an extra angle: turning by α\alpha then β\beta is the same as turning once by α+β\alpha+\beta, so the shadow lengths must combine in a fixed bookkeeping way. Identities feel mysterious as algebra but are obvious as geometry — they are conservation laws for the spinning hand.

Figure
The unit circle: sine and cosine as coordinates of a rotating point
θ cos θ sin θ (cos θ, sin θ) x y O

Worked Examples

ExampleSimplifying an expression

Given: Simplify sin⁡2x1−cos⁡x\dfrac{\sin^2 x}{1 - \cos x}.

Steps: 1. Replace sin⁡2x\sin^2 x using the Pythagorean identity [3]: sin⁡2x=1−cos⁡2x\sin^2 x = 1 - \cos^2 x. 2. Factor the numerator as a difference of squares: 1−cos⁡2x=(1−cos⁡x)(1+cos⁡x)1 - \cos^2 x = (1-\cos x)(1+\cos x). 3. The expression becomes (1−cos⁡x)(1+cos⁡x)1−cos⁡x\dfrac{(1-\cos x)(1+\cos x)}{1-\cos x}. 4. Cancel the common factor (1−cos⁡x)(1-\cos x), valid when cos⁡x≠1\cos x \neq 1.

18
sin⁡2x1−cos⁡x= 1+cos⁡x (cos⁡x≠1)\quad \frac{\sin^2 x}{1-\cos x} = \boxed{\,1 + \cos x\,}\qquad (\cos x \neq 1)

Derivation hint: rewrite sin⁡2\sin^2 via [3], factor, then cancel.

ExampleComputing an exact value with the addition formula

Given: Find the exact value of cos⁡75∘\cos 75^\circ.

Steps: 1. Write 75∘=45∘+30∘75^\circ = 45^\circ + 30^\circ. 2. Apply the cosine addition formula [7]:

cos⁡75∘=cos⁡45∘cos⁡30∘−sin⁡45∘sin⁡30∘\cos 75^\circ = \cos 45^\circ\cos 30^\circ - \sin 45^\circ\sin 30^\circ

3. Substitute known values: cos⁡45∘=sin⁡45∘=22\cos 45^\circ = \sin 45^\circ = \tfrac{\sqrt 2}{2}, cos⁡30∘=32\cos 30^\circ = \tfrac{\sqrt 3}{2}, sin⁡30∘=12\sin 30^\circ = \tfrac12. 4. Compute:

cos⁡75∘=22⋅32−22⋅12=64−24\cos 75^\circ = \frac{\sqrt 2}{2}\cdot\frac{\sqrt 3}{2} - \frac{\sqrt 2}{2}\cdot\frac12 = \frac{\sqrt 6}{4} - \frac{\sqrt 2}{4}
19
cos⁡75∘=6−24≈0.2588\quad \cos 75^\circ = \boxed{\dfrac{\sqrt 6 - \sqrt 2}{4} \approx 0.2588}

Derivation hint: split 75° into known special angles and apply [7].

Common Misconceptions

⚠️ Common mistake

The function notation is not distributive. In general

20
sin⁡(α+β)≠sin⁡α+sin⁡β\quad \sin(\alpha + \beta) \neq \sin\alpha + \sin\beta

Derivation hint: test α=β=90∘\alpha=\beta=90^\circ: left side =sin⁡180∘=0=\sin 180^\circ = 0, right side =1+1=2= 1+1 = 2. Also be careful: sin⁡2θ\sin^2\theta means (sin⁡θ)2(\sin\theta)^2, while sin⁡−1θ\sin^{-1}\theta means the inverse (arcsine), not 1/sin⁡θ=csc⁡θ1/\sin\theta = \csc\theta. And every identity carries hidden domain restrictions — cancellations like the one in [18] are only valid where the cancelled factor is nonzero.

Counterexample

Students often "prove" an identity by manipulating both sides until they reach 0=00=0, then declare victory. But this can validate a false statement if a step is reversible only conditionally. For instance, squaring is not reversible: from the false equation sin⁡x=−sin⁡x\sin x = -\sin x one can square to get the true sin⁡2x=sin⁡2x\sin^2 x = \sin^2 x. The squaring step introduced solutions that were not in the original. Rule: to prove an identity, transform one side into the other using only equivalences; never assume the thing you are trying to prove.

Connections

connection

Trigonometric identities sit at a crossroads of several fields. They are the algebraic backbone of Solving Trigonometric Equations, where rewriting an expression into a single function often unlocks the solution. They power Trigonometric Integration, where formulas like [11] convert un-integrable powers into linear combinations of cosines. They are equivalent statements about Complex Numbers via Euler's formula, turning trigonometry into the arithmetic of points on the unit circle in the complex plane. They generalize the Pythagorean Theorem (set θ\theta to recover a2+b2=c2a^2+b^2=c^2 in a right triangle), and they underlie Fourier Series, where every periodic signal is built from sines and cosines that must be combined using these very identities.

Real-World Applications

🔬 Where this appears

Historical Development

⏳ History
- ~150 BCE — Hipparchus of Nicaea compiles the first known table of chords, the direct ancestor of the sine function, for astronomical prediction.
- ~150 CE — Ptolemy in the Almagest states "Ptolemy's theorem," which is geometrically equivalent to the sine and cosine addition formulas.
- ~500 CE — Aryabhata (India) tabulates the jya (half-chord), introducing what would become the sine; the word "sine" descends from a mistranslation of this term.
- ~10th century — Abu al-Wafa al-Buzjani (Persia) derives the double-angle and addition formulas in essentially modern form and introduces the tangent.
- 1464 — Regiomontanus writes De triangulis omnimodis, the first European treatise treating trigonometry as an independent subject.
- 1614–1620 — John Napier & Henry Briggs publish logarithms, making the product-to-sum identities a practical computing shortcut for centuries.
- 1748 — Leonhard Euler publishes Introductio in analysin infinitorum, giving eiθ=cos⁡θ+isin⁡θe^{i\theta}=\cos\theta+i\sin\theta and modern functional notation, unifying all identities.
- 1822 — Joseph Fourier shows arbitrary periodic functions decompose into sines and cosines, vastly extending the relevance of the identities.

Subtleties & Limits

open-problem

Identities are clean over the real numbers, but extending them raises genuine subtleties. When trig functions are continued to complex arguments, sin⁡z\sin z and cos⁡z\cos z become unbounded (e.g. cos⁡(iy)=cosh⁡y→∞\cos(iy) = \cosh y \to \infty), yet the addition formulas [6]–[7] still hold formally — a reminder that "identity" depends on domain. The inverse functions are not single-valued: arcsin⁡\arcsin requires a branch choice, and "solving" sin⁡x=c\sin x = c yields infinitely many solutions, so an "identity" in inverse functions like arcsin⁡(sin⁡x)=x\arcsin(\sin x) = x holds only on a restricted interval. At the research frontier, questions about which sums of trig values are rational or algebraic (Niven's theorem and its generalizations) remain delicate, and the transcendence of values like cos⁡(1)\cos(1) connects to deep open problems in number theory.

See Also

The Unit Circle · Solving Trigonometric Equations · Complex Numbers · Fourier Series · Law of Sines and Cosines · Trigonometric Integration · Radian Measure