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Mathematics · Ch 3 — Trigonometric Functions

Trigonometric Equations and Principal Solutions

3.1.1

Trigonometric Equations and Principal Solutions

A solution of a trigonometric equation is any value of the angle that makes the equation true when substituted in. For example, θ=π6\theta=\dfrac{\pi}{6} satisfies sin⁡θ=12\sin\theta=\dfrac12 because sin⁡π6=12\sin\dfrac{\pi}{6}=\dfrac12; so does θ=5π6\theta=\dfrac{5\pi}{6}, because sin⁡5π6=12\sin\dfrac{5\pi}{6}=\dfrac12 as well. In fact the same equation is also satisfied by θ=5π6+2π=17π6\theta=\dfrac{5\pi}{6}+2\pi=\dfrac{17\pi}{6}, by θ=π6−2π=−11π6\theta=\dfrac{\pi}{6}-2\pi=-\dfrac{11\pi}{6}, and so on forever, purely because sine has period 2π2\pi. Likewise θ=π4\theta=\dfrac{\pi}{4} satisfies cos⁡θ=12\cos\theta=\dfrac{1}{\sqrt2}, and θ=7π4\theta=\dfrac{7\pi}{4} satisfies cos⁡θ=12\cos\theta=\dfrac{1}{\sqrt2} too (since cos⁡7π4=cos⁡(2π−π4)=cos⁡π4\cos\dfrac{7\pi}{4}=\cos\left(2\pi-\dfrac{\pi}{4}\right)=\cos\dfrac{\pi}{4}).

Because of this periodicity a trigonometric equation can have infinitely many solutions, so mathematicians agree to first describe only the solutions that lie in one standard window, [0,2π)[0,2\pi) — one full period, starting from 00 and not including 2π2\pi itself.

Definition (Principal Solution). A solution α\alpha of a trigonometric equation is called a principal solution if 0≤α<2π0\le\alpha<2\pi.

For example, both π6\dfrac{\pi}{6} and 5π6\dfrac{5\pi}{6} lie in [0,2π)[0,2\pi), so both are principal solutions of sin⁡θ=12\sin\theta=\dfrac12. But 13π6\dfrac{13\pi}{6}, although it does satisfy sin⁡θ=12\sin\theta=\dfrac12 (because 13π6=2π+π6\dfrac{13\pi}{6}=2\pi+\dfrac{\pi}{6}), is not a principal solution, since 13π6∉[0,2π)\dfrac{13\pi}{6}\notin[0,2\pi).

A function's value can also fix how many principal solutions an equation has: θ=0\theta=0 is the only principal solution of sin⁡θ=0\sin\theta=0 in [0,2π)[0,2\pi) (note 2π2\pi itself is excluded by the strict upper bound), while cos⁡θ=−1\cos\theta=-1 has exactly one principal solution, θ=π\theta=\pi, because cosine only touches −1-1 once per period.

Worked Example 1 — Find the principal solutions of sin⁡θ=12\sin\theta=\dfrac12. Since sin⁡π4\sin\dfrac{\pi}{4}... (correction — using the standard angle) sin⁡π6=12\sin\dfrac{\pi}{6}=\dfrac12 and 0≤π6<2π0\le\dfrac{\pi}{6}<2\pi, so π6\dfrac{\pi}{6} is one principal solution. Using the allied-angle identity sin⁡θ=sin⁡(π−θ)\sin\theta=\sin(\pi-\theta), we also get sin⁡(π−π6)=sin⁡π6=12\sin\left(\pi-\dfrac{\pi}{6}\right)=\sin\dfrac{\pi}{6}=\dfrac12, i.e. sin⁡5π6=12\sin\dfrac{5\pi}{6}=\dfrac12, and 5π6\dfrac{5\pi}{6} also lies in [0,2π)[0,2\pi). So the two principal solutions are π6\dfrac{\pi}{6} and 5π6\dfrac{5\pi}{6}.

Worked Example 2 — Find the principal solutions of cos⁡θ=12\cos\theta=\dfrac12. cos⁡π3=12\cos\dfrac{\pi}{3}=\dfrac12 and π3∈[0,2π)\dfrac{\pi}{3}\in[0,2\pi), so π3\dfrac{\pi}{3} is one principal solution. Using cos⁡θ=cos⁡(2π−θ)\cos\theta=\cos(2\pi-\theta): cos⁡(2π−π3)=cos⁡π3=12\cos\left(2\pi-\dfrac{\pi}{3}\right)=\cos\dfrac{\pi}{3}=\dfrac12, i.e. cos⁡5π3=12\cos\dfrac{5\pi}{3}=\dfrac12, and 5π3∈[0,2π)\dfrac{5\pi}{3}\in[0,2\pi). So the principal solutions are π3\dfrac{\pi}{3} and 5π3\dfrac{5\pi}{3}. …