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11.2 Evaluation of double integrals in polar form

11.2 Evaluation of double integrals in polar form

Written by the Fiveable Content Team • Last updated August 2025
Written by the Fiveable Content Team • Last updated August 2025
Calculus IV
Unit & Topic Study Guides

Double Integrals in Polar Coordinates

Conversion from Cartesian to Polar Coordinates

A double integral in Cartesian coordinates f(x,y)dA\iint f(x,y)\, dA can be rewritten in polar coordinates using the substitutions x=rcosθx = r\cos\theta and y=rsinθy = r\sin\theta. The function f(x,y)f(x,y) becomes f(rcosθ,rsinθ)f(r\cos\theta,\, r\sin\theta), and the area element transforms as well.

The key piece of the conversion is the Jacobian determinant, which equals rr. This factor accounts for the fact that the area element in polar coordinates is not a simple rectangle. Instead, it's a small "wedge" whose size depends on how far you are from the origin. The Cartesian area element dA=dxdydA = dx\,dy becomes:

dA=rdrdθdA = r\,dr\,d\theta

So the full converted integral is:

f(rcosθ,rsinθ)  rdrdθ\iint f(r\cos\theta,\, r\sin\theta)\; r\,dr\,d\theta

That extra rr is easy to forget, and leaving it out is one of the most common mistakes on exams.

Benefits and Applications of Polar Coordinates

Polar coordinates simplify double integrals when the region of integration has circular, annular, or rotational symmetry. If you're integrating over a disk, a ring, or a sector, polar coordinates will almost always produce cleaner limits than Cartesian.

Certain functions are also much easier to handle in polar form. For example, ex2y2e^{-x^2 - y^2} looks difficult in Cartesian coordinates, but in polar form it becomes er2e^{-r^2}, which is straightforward to integrate with respect to rr. Functions involving x2+y2x^2 + y^2 generally benefit from the substitution x2+y2=r2x^2 + y^2 = r^2.

These techniques appear frequently in physics and engineering, particularly when modeling electromagnetic fields, gravitational potentials, fluid flow, and other systems with radial symmetry.

Conversion from Cartesian to Polar Coordinates, Multiple Integrals | Boundless Calculus

Evaluating Polar Double Integrals

Setting Up the Integration Limits

Before computing anything, sketch the region of integration in the rθr\theta-plane. This step prevents most limit-setting errors.

  1. Identify the angular limits. Determine the range of θ\theta that sweeps across the entire region. For a full disk, 0θ2π0 \leq \theta \leq 2\pi. For a quarter-disk in the first quadrant, 0θπ/20 \leq \theta \leq \pi/2.
  2. Identify the radial limits. For each angle θ\theta, determine where rr starts (the inner boundary) and where it ends (the outer boundary). These limits can be constants (e.g., 1r31 \leq r \leq 3 for an annular region) or functions of θ\theta (e.g., 0r2cosθ0 \leq r \leq 2\cos\theta for a circle offset from the origin).
  3. Write the integral. The standard setup with rr as the inner integral is:

θ1θ2r1(θ)r2(θ)f(rcosθ,rsinθ)  rdrdθ\int_{\theta_1}^{\theta_2}\int_{r_1(\theta)}^{r_2(\theta)} f(r\cos\theta,\, r\sin\theta)\; r\,dr\,d\theta

The radial limits can depend on θ\theta, but the angular limits should be constants.

Conversion from Cartesian to Polar Coordinates, Double Integrals in Polar Coordinates · Calculus

Evaluating the Radial and Angular Integrals

Work from the inside out. Here's a concrete example: evaluate 0π/402r2drdθ\int_0^{\pi/4}\int_0^2 r^2\,dr\,d\theta.

Step 1: Evaluate the inner (radial) integral. Treat θ\theta as a constant and integrate with respect to rr:

02r2dr=13r302=83\int_0^2 r^2\,dr = \frac{1}{3}r^3\Big|_0^2 = \frac{8}{3}

Step 2: Evaluate the outer (angular) integral. Substitute the result from Step 1 and integrate with respect to θ\theta:

0π/483dθ=83θ0π/4=83π4=2π3\int_0^{\pi/4} \frac{8}{3}\,d\theta = \frac{8}{3}\,\theta\Big|_0^{\pi/4} = \frac{8}{3}\cdot\frac{\pi}{4} = \frac{2\pi}{3}

When the radial limits depend on θ\theta, the result of the inner integral will be a function of θ\theta rather than a constant, so the outer integral requires more work.

Interpreting the Area Element

The polar area element dA=rdrdθdA = r\,dr\,d\theta represents a small curved patch, not a true rectangle. Its radial width is drdr, and its arc length is rdθr\,d\theta. The product of these gives the area of the patch.

Notice that as rr increases, the patch gets larger even if drdr and dθd\theta stay the same. This is why the factor of rr appears: regions farther from the origin contribute more area per unit of drdθdr\,d\theta. Near the origin (small rr), the patches are tiny; far from the origin (large rr), they're much bigger.

To find the total area of a polar region (without any additional function), you integrate just the area element:

A=rdrdθA = \iint r\,dr\,d\theta

This is equivalent to setting f=1f = 1 in the double integral.