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*small-angle approximation*

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small-angle approximation

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*x*â†’ 0}})The

**small-angle approximation**is a useful simplification of the basic trigonometric functions which is approximately true in the limit where the angle approaches zero. They are truncations of the Taylor series for the basic trigonometric functions to a second-order approximation. This truncation gives:

begin{align}

sin theta &approx theta cos theta &approx 1 - frac{theta^2}{2} tan theta &approx theta, end{align}where {{mvar|Î¸}} is the angle in radians.The small angle approximation is useful in many areas of engineering and physics, including mechanics, electromagnetics, optics (where it forms the basis of the paraxial approximation), cartography, astronomy, computer science, and so on.## Justifications

### Graphic

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.File:Small_angle_compair_odd.svg|**Figure 1.**A comparison of the basic odd trigonometric functions to {{math|Î¸}}. It is seen that as the angle approaches 0 the approximations become better.File:Small_angle_compare_even.svg|

**Figure 2.**A comparison of {{math|cos

*Î¸*}} to {{math|1 âˆ’ {{sfrac|

*Î¸*2|2}}}}. It is seen that as the angle approaches 0 the approximation becomes better.

### Geometric

(File:Small angle triangle.svg|600px)

The red section on the right, {{math|d}}, is the difference between the lengths of the hypotenuse, {{mvar|H}}, and the adjacent side, {{mvar|A}}. As is shown, {{mvar|H}} and {{mvar|A}} are almost the same length, meaning {{math|cos *Î¸*}} is close to 1 and {{math|{{sfrac|

*Î¸*2|2}}}} helps trim the red away.

cos{theta} approx 1 - frac{theta^2}{2}

The opposite leg, {{mvar|O}}, is approximately equal to the length of the blue arc, {{mvar|s}}. Gathering facts from geometry, {{math|*s*{{=}}

*AÎ¸*}}, from trigonometry, {{math|sin

*Î¸*{{=}} {{sfrac|

*O*|

*H*}}}} and {{math|tan

*Î¸*{{=}} {{sfrac|

*O*|

*A*}}}}, and from the picture, {{math|

*O*â‰ˆ

*s*}} and {{math|

*H*â‰ˆ

*A*}} leads to:

sin theta = frac{O}{H}approxfrac{O}{A} = tan theta = frac{O}{A} approx frac{s}{A} = frac{Atheta}{A} = theta.

Simplifying leaves,
sin theta approx tan theta approx theta.

### Calculus

sin theta approx theta , tan theta approx theta , {{math|cos*Î¸*â‰ˆ 1 âˆ’ {{sfrac|

*Î¸*2|2}}}}can also be expressed this way, considering the fact that Î¸ tends to zero{{math|{{sfrac|

*sin (Î¸)*|Î¸}}â‰ˆ1}} , {{math|{{sfrac|

*tan (Î¸)*|Î¸}}â‰ˆ1}} , cos theta approx 1. In fact, an approximation can also be synonymous with the word "limit" and Î¸ in radians, being too small, tends to zero. It can be proved using Squeeze Theorem that in terms of limit calculus,

### Algebraic

(File:Small-angle approximation for sine function.svg|thumb|300px|The small-angle approximation for the sine function.)The Maclaurin expansion (the Taylor expansion about 0) of the relevant trigonometric function isBOOK, Mary L. Boas, Boas, Mary L., Mathematical Methods in the Physical Sciences, 2006, Wiley, 26, 978-0-471-19826-0,
begin{align} sin theta &= sum^{infin}_{n=0} frac{(-1)^n}{(2n+1)!} theta^{2n+1}

&= theta - frac{theta^3}{3!} + frac{theta^5}{5!} - frac{theta^7}{7!} + cdots end{align}where {{mvar|Î¸}} is the angle in radians. In clearer terms,
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 {{val|0.000001}}, or {{sfrac|{{val|10000}}}} the first term. One can thus safely approximate:
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,
tan theta approx sin theta approx theta,

## Error of the approximations

File:Small angle compare error.svg|thumb|upright=2|**Figure 3.**A graph of the relative errorrelative errorFigure 3 shows the relative errors of the small angle approximations. The angles at which the relative error exceeds 1% are as follows:

- {{math|tan
*Î¸*â‰ˆ*Î¸*}} at about 0.176 radians (10Â°). - {{math|sin
*Î¸*â‰ˆ*Î¸*}} at about 0.244 radians (14Â°). - {{math|cos
*Î¸*â‰ˆ 1 âˆ’ {{sfrac|*Î¸*2|2}}}} at about 0.664 radians (38Â°).

## Specific uses

### Astronomy

In astronomy, the 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. The linear size ({{mvar|D}}) is related to the angular size ({{mvar|X}}) and the distance from the observer ({{mvar|d}}) by the simple formula
D = X frac{d}{206,265}

where {{mvar|X}} is measured in arcseconds.The number {{val|206265}} is approximately equal to the number of arcseconds in a circle ({{val|1296000}}), divided by {{math|2Ï€}}.The exact formula is
D = d tan left( X frac{2pi}{1,296,000} right)

and the above approximation follows when {{math|tan *X*}} is replaced by {{mvar|X}}.

### Motion of a pendulum

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.### Structural mechanics

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.### Piloting

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.### Interpolation

Small-angle formulas may be used for interpolating between trigonometric table values. When Î² â‰ˆ 0, then sin(Î²) â‰ˆ Î², cos(Î²) â‰ˆ 1, and the angle sum and difference identities reduce to: cos(Î± + Î²) â‰ˆ cos(Î±) - Î²sin(Î±), cos(Î± - Î²) â‰ˆ cos(Î±) + Î²sin(Î±),sin(Î± + Î²) â‰ˆ sin(Î±) + Î²cos(Î±),sin(Î± - Î²) â‰ˆ sin(Î±) - Î²cos(Î±).Example: sin(0.755)
sin(0.755) = sin(0.75 + 0.005)

â‰ˆ sin(0.75) + (0.005)cos(0.75) [sin(0.75) and cos(0.75) values from trigonometric table]

â‰ˆ (0.6816) + (0.005)(0.7317)

â‰ˆ 0.6853.

â‰ˆ sin(0.75) + (0.005)cos(0.75) [sin(0.75) and cos(0.75) values from trigonometric table]

â‰ˆ (0.6816) + (0.005)(0.7317)

â‰ˆ 0.6853.

## See also

- Skinny triangle
- Infinitesimal oscillations of a pendulum
- Versine and haversine
- Exsecant and excosecant

## References

{{reflist}}**- content above as imported from Wikipedia**

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