For small angles, the trigonometric functions sine, cosine, and tangent can be calculated with reasonable accuracy by the following simple approximations:
\begin{align} \sin\theta& ≈ \tan\theta ≈ \theta,\\[5mu] \cos\theta& ≈ 1-\tfrac12\theta2 ≈ 1, \end{align}
provided the angle is measured in radians. Angles measured in degrees must first be converted to radians by multiplying them by .
These approximations have a wide range of uses in branches of physics and engineering, including mechanics, electromagnetism, optics, cartography, astronomy, and computer science. One reason for this is that they can greatly simplify differential equations that do not need to be answered with absolute precision.
There are a number of ways to demonstrate the validity of the small-angle approximations. The most direct method is to truncate the Maclaurin series for each of the trigonometric functions. Depending on the order of the approximation,
style\cos\theta
1
The accuracy of the approximations can be seen below in Figure 1 and Figure 2. As the measure of the angle approaches zero, the difference between the approximation and the original function also approaches 0.
The red section on the right,, is the difference between the lengths of the hypotenuse,, and the adjacent side, . As is shown, and are almost the same length, meaning is close to 1 and helps trim the red away.
The opposite leg,, is approximately equal to the length of the blue arc, . Gathering facts from geometry,, from trigonometry, and, and from the picture, and leads to:
Simplifying leaves,
Using the squeeze theorem, we can prove that which is a formal restatement of the approximation
\sin(\theta) ≈ \theta
A more careful application of the squeeze theorem proves that from which we conclude that
\tan(\theta) ≈ \theta
\cos2A\equiv1-2\sin2A
\theta=2A
The Taylor series expansions of trigonometric functions sine, cosine, and tangent near zero are:[2]
where is the angle in radians. For very small angles, higher powers of become extremely small, for instance if, then, just one ten-thousandth of . Thus for many purposes it suffices to drop the cubic and higher terms and approximate the sine and tangent of a small angle using the radian measure of the angle,, and drop the quadratic term and approximate the cosine as .
If additional precision is needed the quadratic and cubic terms can also be included,,, and.
One may also use dual numbers, defined as numbers in the form
a+b\varepsilon
a,b\inR
\varepsilon
\varepsilon2=0
\varepsilon\ne0
\cos(\theta\varepsilon)=1
\sin(\theta\varepsilon)=\theta\varepsilon
Near zero, the relative error of the approximations,, and is quadratic in : for each order of magnitude smaller the angle is, the relative error of these approximations shrinks by two orders of magnitude. The approximation has relative error which is quartic in : for each order of magnitude smaller the angle is, the relative error shrinks by four orders of magnitude.
Figure 3 shows the relative errors of the small angle approximations. The angles at which the relative error exceeds 1% are as follows:
The angle addition and subtraction theorems reduce to the following when one of the angles is small (β ≈ 0):
cos(α + β) | ≈ cos(α) − β sin(α), | |
cos(α − β) | ≈ cos(α) + β sin(α), | |
sin(α + β) | ≈ sin(α) + β cos(α), | |
sin(α − β) | ≈ sin(α) − β cos(α). |
In astronomy, the angular size or angle subtended by the image of a distant object is often only a few arcseconds (denoted by the symbol ″), so it is well suited to the small angle approximation. The linear size is related to the angular size and the distance from the observer by the simple formula:
D=X
d | |
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where is measured in arcseconds.
The quantity is approximately equal to the number of arcseconds in a circle, divided by, or, the number of arcseconds in 1 radian.
The exact formula is
D=d\tan\left(X
2\pi | |
1296000{'' |
and the above approximation follows when is replaced by .
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.
In optics, the small-angle approximations form the basis of the paraxial approximation.
The sine and tangent small-angle approximations are used in relation to the double-slit experiment or a diffraction grating to develop simplified equations like the following, where is the distance of a fringe from the center of maximum light intensity, is the order of the fringe, is the distance between the slits and projection screen, and is the distance between the slits: [3]
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)where the values for sin(0.75) and cos(0.75) are obtained from trigonometric table. The result is accurate to the four digits given.
. Mary L. Boas. Mathematical Methods in the Physical Sciences. 2006. Wiley. 26. 978-0-471-19826-0.