Small-angle approximation

The accuracy of the approximations can be seen below in Figure 1 and Figure 2. As the angle approaches zero, it is clear that the gap between the approximation and the original function quickly vanishes.

• 
  Figure 1. A comparison of the basic odd trigonometric functions to θ. It is seen that as the angle approaches 0 the approximations become better.
• 
  Figure 2. A comparison of cos θ to 1 − θ²/2. It is seen that as the angle approaches 0 the approximation becomes better.

The red section on the right, d, is the difference between the lengths of the hypotenuse, H, and the adjacent side, A. As is shown, H and A are almost the same length, meaning cos θ is close to 1 and θ²/2 helps trim the red away.

${\displaystyle \cos {\theta }\approx 1-{\frac {\theta ^{2}}{2}}}$

The opposite leg, O, is approximately equal to the length of the blue arc, s. Gathering facts from geometry, s = Aθ, from trigonometry, sin θ = O/H and tan θ = O/A, and from the picture, O ≈ s and H ≈ A leads to:

${\displaystyle \sin \theta ={\frac {O}{H}}\approx {\frac {O}{A}}=\tan \theta ={\frac {O}{A}}\approx {\frac {s}{A}}={\frac {A\theta }{A}}=\theta .}$

Simplifying leaves,

${\displaystyle \sin \theta \approx \tan \theta \approx \theta .}$

Using the squeeze theorem,[3] we can prove that ${\displaystyle \lim _{\theta \to 0}{\frac {\sin(\theta )}{\theta }}=1,}$ which is a formal restatement of the approximation ${\displaystyle \sin(\theta )\approx \theta }$ for small values of θ.

A more careful application of the squeeze theorem proves that ${\displaystyle \lim _{\theta \to 0}{\frac {\tan(\theta )}{\theta }}=1,}$ from which we conclude that ${\displaystyle \tan(\theta )\approx \theta }$ for small values of θ.

Finally, using L'Hôpital's rule tells us that ${\displaystyle \lim _{\theta \to 0}{\frac {\cos(\theta )-1}{\theta ^{2}}}=\lim _{\theta \to 0}{\frac {-\sin(\theta )}{2\theta }}=-{\frac {1}{2}},}$ which rearranges algebraically to give ${\displaystyle \cos(\theta )\approx 1-{\frac {\theta ^{2}}{2}}}$ for small values of θ.

The small-angle approximation for the sine function.

The Maclaurin expansion (the Taylor expansion about 0) of the relevant trigonometric function is[4]

${\displaystyle {\begin{aligned}\sin \theta &=\sum _{n=0}^{\infty }{\frac {(-1)^{n}}{(2n+1)!}}\theta ^{2n+1}\\&=\theta -{\frac {\theta ^{3}}{3!}}+{\frac {\theta ^{5}}{5!}}-{\frac {\theta ^{7}}{7!}}+\cdots \end{aligned}}}$

where θ is the angle in radians. In clearer terms,

${\displaystyle \sin \theta =\theta -{\frac {\theta ^{3}}{6}}+{\frac {\theta ^{5}}{120}}-{\frac {\theta ^{7}}{5040}}+\cdots }$

It is readily seen that the second most significant (third-order) term falls off as the cube of the first term; thus, even for a not-so-small argument such as 0.01, the value of the second most significant term is on the order of 0.000001, or 1/10000 the first term. One can thus safely approximate:

${\displaystyle \sin \theta \approx \theta }$

By extension, since the cosine of a small angle is very nearly 1, and the tangent is given by the sine divided by the cosine,

${\displaystyle \tan \theta \approx \sin \theta \approx \theta }$,

In astronomy, the angular size or angle subtended by the image of a distant object is often only a few arcseconds, so it is well suited to the small angle approximation.[5] The linear size (D) is related to the angular size (X) and the distance from the observer (d) by the simple formula:

${\displaystyle D=X{\frac {d}{206\,265}}}$

where X is measured in arcseconds.

The number 206265 is approximately equal to the number of arcseconds in a circle (1296000), divided by 2π.

The exact formula is

${\displaystyle D=d\tan \left(X{\frac {2\pi }{1\,296\,000}}\right)}$

and the above approximation follows when tan X is replaced by X.

The second-order cosine approximation is especially useful in calculating the potential energy of a pendulum, which can then be applied with a Lagrangian to find the indirect (energy) equation of motion.

When calculating the period of a simple pendulum, the small-angle approximation for sine is used to allow the resulting differential equation to be solved easily by comparison with the differential equation describing simple harmonic motion.

The small-angle approximation also appears in structural mechanics, especially in stability and bifurcation analyses (mainly of axially-loaded columns ready to undergo buckling). This leads to significant simplifications, though at a cost in accuracy and insight into the true behavior.

The 1 in 60 rule used in air navigation has its basis in the small-angle approximation, plus the fact that one radian is approximately 60 degrees.

The formulas for addition and subtraction involving a small angle may be used for interpolating between trigonometric table values:

Example: sin(0.755)

sin(0.755)	= sin(0.75 + 0.005)
	≈ sin(0.75) + (0.005)cos(0.75)
	≈ (0.6816) + (0.005)(0.7317)	[Obtained sin(0.75) and cos(0.75) values from trigonometric table]
	≈ 0.6853.