Compute the arc length of an Archimedean spiral segment using numerical integration. Perfect for calculus, physics, and design applications.
An Archimedean spiral (also known as arithmetic spiral) is defined in polar coordinates by the equation r(θ) = a + bθ, where a is the initial radius (at θ=0) and b controls the spacing between turns. This spiral is characterized by constant separation between successive turnings.
Arc Length in Polar Coordinates
For a curve given in polar form r = f(θ) from θ = α to β, the total arc length is:
L = ∫αβ √( r² + (dr/dθ)² ) dθ
For the Archimedean spiral, dr/dθ = b, so the integrand simplifies to:
L = ∫αβ √( (a + bθ)² + b² ) dθ
The indefinite integral can be evaluated using trigonometric substitution or integration by parts. The result is:
Therefore, the definite length from θ₁ to θ₂ is:
Note: For a = 0, the formula simplifies to L = ½ [ θ √(θ²+1) + ln( θ + √(θ²+1) ) ] evaluated between limits.
Take the classic spiral r = θ (a=0, b=1) from θ=0 to θ=2π. Then:
This matches the numerical result from the calculator (21.256) within 0.0025, confirming the accuracy.
The parameter b determines the radial increase per radian: after one full turn (2π radians), the radius increases by 2πb. The initial radius a shifts the entire spiral outward. For a given θ range, larger b produces longer spirals because the radius grows faster.
Numerical Integration
When an analytical antiderivative is complex or unavailable, numerical methods like Simpson's rule (used here) provide accurate approximations. The adaptive Simpson algorithm refines the step size in regions where the function changes rapidly, ensuring high precision with minimal computation.
| Parameter | Effect |
|---|---|
| a (initial radius) | Shifts the spiral outward; distance from origin at θ=0. |
| b (growth rate) | Controls spacing between turns: constant radial increment per radian = b. |
| θ range | Determines number of turns and total arc length. |