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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(

...

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}


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


Latex
{latex}

\\

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

\\

{latex}\begin{large} \[ sin( \theta ) \approx \theta \]\end{large}{latex}

\\

This gives us our criterion for "small 


This gives us our criterion for "small enough",

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because

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it

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is

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clear

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that

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this

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will

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be

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the

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case

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when

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x

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is

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much

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greater

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than

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x

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3

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/3!

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,

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or

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in

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other

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words

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6

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>>

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x

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2

...

.

Similarly,

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the

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Taylor

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series

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for

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cos(

...

θ) is


Latex
* 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
{latex}

\\
so that in the small angle approximation we have 
\\
{latex}\begin{large} \[ cos( \theta ) \approx 1 \]\end{large}{latex}

\\


Finally,

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the

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expansion

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for

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the

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tangent is

Latex
* 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
{latex}
\\
So that for small angles 
\\
{latex}\begin{large} \[ tan( \theta ) \approx \theta \]\end{large}{latex}
\\