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A

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very

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useful

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approximation

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for

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many

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physical

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applications,

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especially

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for

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simple

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harmonic

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motion

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and

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pendulums

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in

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particular.

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It

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states

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that

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Excerpt

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when

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the

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angle

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is

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small,

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and

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expressed

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in

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radians

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,

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then

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we

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may

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approximate

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sin(

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θ) by θ.

At the same time, we may approximate cos(θ) by 1 and tan(θ) by θ.

This follows because the sine function may be expressed as the infinite Taylor series:

Latex
* by {*}θ{*}.{excerpt} At the same time, we may approximate *cos(θ)* by *1* and *tan(θ)* by {*}θ{*}. 

This follows because the sine function may be expressed as the infinite *Taylor series*:
\\
{latex}\begin{large} \[ sin( \theta ) = x - \frac{x^{3}}{3!} + \frac{x^{5}}{5!} - \frac{x^{7}}{7!} + ... \]\end{large}{latex}
\\
If the angle is small enough, then we can 


If the angle is small enough, then we can ignore all but the first term, giving


Latex
ignore all but the first term, giving
\\
{latex}\begin{large} \[ sin( \theta ) \approx x\theta \]\end{large}


This gives us our criterion for "small enough", because it is clear that this will be the case when x is much greater than x3/3!, or in other words 6 >> x2.

Similarly, the Taylor series for cos(θ) is


Latex
\begin{large} \[ cos( \theta ) = 1 - \frac{x^{2}}{2!} + \frac{x^{4}}{4!} - \frac{x^{6}}{6!} + ... \]\end{large}


so that in the small angle approximation we have

Latex
\begin{large} \[ cos( \theta ) \approx 1 \]\end{large}


Finally, the expansion for the tangent is

Latex
\begin{large} \[ tan( \theta ) = \theta + \frac{x^{3}}{3} + \frac{2x^{5}}{15} + \frac{17x^{7}}{217} + ... \]\end{large}


So that for small angles

Latex
\begin{large} \[ tan( \theta ) \approx \theta \]\end{large}{latex}
\\
This gives us our criterion for "small enough", because it is clear that this will be the case when *x* is much greater than {*}x^3^/3!{*}, or in other words *6 >> x^2^*.