Multivariable Calculus • Multiple Integrals

Triple Integrals: Cylindrical — Triple integrals in cylindrical coordinates

Unlock the power of cylindrical coordinates to evaluate triple integrals over regions with circular symmetry.

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Inside this lesson 10 sections 5 questions 9 figures

SECTION 1

Historical Context & Motivation

Long before anyone wrote down a triple integral, mathematicians and scientists wrestled with measuring volumes and masses of objects that were not simple boxes or spheres. In the real world, many shapes—pipes, cans, volcanoes, whirlpools—have a natural circular symmetry around some central axis. Trying to describe these shapes using plain Cartesian coordinates (the familiar x, y, z grid) often produces ugly, complicated algebra. The development of cylindrical coordinates gave mathematicians an elegant shortcut: wrap a polar coordinate system around the vertical axis, and suddenly circular regions become simple to describe.

1600s • Cartesian Coordinates Established

René Descartes and Pierre de Fermat independently developed the rectangular coordinate system, allowing geometry problems to be expressed as algebra. This laid the foundation for all coordinate-based calculus.

1690s • Newton & Leibniz Formalize Calculus

Isaac Newton and Gottfried Wilhelm Leibniz independently created the framework of integration and differentiation. Single integrals could now compute areas and accumulated quantities systematically.

1700s • Euler & Polar Coordinates

Leonhard Euler popularized polar coordinates (r, θ) for two-dimensional problems, making it far easier to handle curves and regions with circular symmetry. This naturally extended into three dimensions as cylindrical coordinates.

1800s • Multiple Integrals Formalized

Mathematicians like Augustin-Louis Cauchy and Bernhard Riemann rigorously defined double and triple integrals, including the rules for changing variables between coordinate systems—the Jacobian determinant.

Modern • Engineering & Physics Applications

Today, cylindrical-coordinate triple integrals are essential in electromagnetism, fluid dynamics, and structural engineering wherever cylindrical symmetry appears—from MRI machines to rocket nozzles.

The central question this lesson addresses is: how do we set up and evaluate a triple integral when the region of integration has circular symmetry? By the end, you will be able to convert a Cartesian triple integral into cylindrical form, identify the correct limits of integration, and compute volumes, masses, and other quantities with confidence.

SECTION 2

Core Principles & Definitions

Before diving into integrals, you need to understand what cylindrical coordinates actually are. Think of them as a mashup of two systems you already know: polar coordinates in the horizontal plane and the ordinary vertical z-axis from Cartesian coordinates. Instead of locating a point with (x, y, z), you use (r, θ, z), where r is the distance from the z-axis, θ (theta) is the angle measured from the positive x-axis, and z is the height.

1

Cylindrical Coordinates (r, θ, z)

A point in 3D space is described by its radial distance r from the z-axis, its angle θ in the xy-plane, and its height z. Conversion: x = r cos θ, y = r sin θ, z = z.
2

The Jacobian Factor: r

When you switch from Cartesian to cylindrical coordinates, the volume element changes from dx dy dz to r dr dθ dz. The extra factor of r comes from the Jacobian determinant of the coordinate transformation.
3

When to Use Cylindrical Coordinates

Use cylindrical coordinates whenever the region of integration has circular symmetry around a vertical axis—cylinders, cones, paraboloids, or any region described by x² + y² = r².
4

Limits of Integration

You must determine bounds for each variable: θ typically ranges from 0 to 2π for full rotation, r from 0 outward to the boundary, and z between two surfaces.
✦

KEY TAKEAWAY

Imagine you are slicing a cake. In Cartesian coordinates, you would cut it into tiny rectangular boxes—awkward for a round cake. In cylindrical coordinates, you cut thin wedge-shaped slices that fan out from the center. Each wedge is wider on the outside than the inside, which is exactly why you multiply by r—it accounts for the fact that outer wedges sweep through more area than inner ones.

SECTION 3

Visual Explanation: The Cylindrical Coordinate System

xzyrθP(r, θ, z)zCylindrical Coordinate SystemA point P is located by (r, θ, z)r = radial distance from z-axisθ = angle from positive x-axisz = height above xy-plane
The diagram shows a 3D coordinate system with the three cylindrical coordinates labeled. The radial distance r (purple) extends from the z-axis to the projection of point P in the xy-plane, the angle θ (cyan) sweeps from the positive x-axis, and the height z (green) lifts the point vertically to its final position P(r, θ, z).

Notice that the r and θ components are exactly the same as polar coordinates—they describe where the point sits in the horizontal xy-plane. The z coordinate then lifts the point up (or down) to its true three-dimensional position. This is why cylindrical coordinates are sometimes described as polar coordinates plus height. Any time you see a region bounded by expressions like x² + y² ≤ a², you can immediately replace that with r ≤ a—a single, clean inequality instead of a messy sum of squares.

SECTION 4

Mathematical Framework

Coordinate Conversions

To convert between Cartesian and cylindrical coordinates, use the following relationships. These are the same conversions from polar coordinates, with z unchanged.

CARTESIAN TO CYLINDRICAL

r=√(x2+y2),θ=arctan(y/x),z=zr = √(x² + y²), θ = arctan(y / x), z = z

Here r ≥ 0 is the radial distance, and θ is measured in radians from the positive x-axis (0 ≤ θ < 2π).

CYLINDRICAL TO CARTESIAN

x=rcosθ,y=rsinθ,z=zx = r cos θ, y = r sin θ, z = z

Use these to convert the integrand f(x, y, z) into f(r cos θ, r sin θ, z) before integrating.

The Volume Element

The most critical piece of the puzzle is the volume element (also called the differential volume). In Cartesian coordinates the tiny box has volume dV = dx dy dz. When we switch to cylindrical coordinates, the shape of that tiny piece changes—it becomes a small wedge—and the volume becomes:

VOLUME ELEMENT IN CYLINDRICAL COORDINATES

dV=r⋅dr⋅dθ⋅dzdV = r · dr · dθ · dz

The factor of r is the Jacobian of the transformation from (x, y) to (r, θ). Never forget this r factor—it is the most common mistake in cylindrical integration.

General Triple Integral Form

TRIPLE INTEGRAL IN CYLINDRICAL COORDINATES

∫∫∫Ef(x,y,z)dV=∫θ1θ2∫r1(θ)r2(θ)∫z1(r,θ)z2(r,θ)f(rcosθ,rsinθ,z)⋅rdzdrdθ∫∫∫_E f(x, y, z) dV = ∫_{θ₁}^{θ₂} ∫_{r₁(θ)}^{r₂(θ)} ∫_{z₁(r,θ)}^{z₂(r,θ)} f(r cos θ, r sin θ, z) · r dz dr dθ

The integration order shown is dz dr dθ (inside out). The limits for z may depend on r and θ, the limits for r may depend on θ, and the limits for θ are constants.

⚠

Common Mistake Alert

The number-one error students make is forgetting to include the extra r factor when converting dV. Always write dV = r dr dθ dz—even before you start finding limits. Circle it, highlight it, tattoo it on your brain.

SECTION 5

Detailed Breakdown: The Cylindrical Volume Element

To truly understand why the extra r factor appears, it helps to visualize what a tiny piece of volume actually looks like in cylindrical coordinates. Instead of a rectangular box, the infinitesimal volume element is a curved wedge. The following diagram breaks this wedge apart so you can see where every dimension comes from.

Cylindrical Volume Element (dV = r dr dθ dz)A small wedge-shaped piece of space at distance r from the z-axisz-axisdrdzr dθrdθdr = radial thicknessr dθ = arc-length widthdz = vertical heightVolume of wedge ≈ (dr) × (r dθ) × (dz) = r · dr · dθ · dz
This diagram shows the tiny wedge-shaped volume element. Its three dimensions are dr (radial thickness in purple), r dθ (arc-length width in cyan), and dz (vertical height in green). Multiplying these together gives dV = r dr dθ dz.

The key insight is that the arc-length dimension is r dθ, not just dθ. When you are close to the z-axis (small r), the arc is short, so the wedge is small. When you are far from the axis (large r), the same angular increment dθ sweeps through a longer arc, making the wedge bigger. This is precisely why the factor of r appears in the volume element.

Coordinate SystemVolume Element dVShape of Element
Cartesian (x, y, z)dx dy dzRectangular box
Cylindrical (r, θ, z)r dr dθ dzCurved wedge
Spherical (ρ, θ, φ)ρ² sin φ dρ dθ dφSpherical wedge

Comparison of volume elements across coordinate systems

SECTION 6

Worked Example: Volume of a Solid Cylinder

Let's find the volume of the solid region E bounded by the cylinder x² + y² = 4 (radius 2) between the planes z = 0 and z = 3. In Cartesian coordinates this integral would require awkward square-root limits, but in cylindrical coordinates it becomes straightforward.

Volume of a Cylinder Using Cylindrical Coordinates

  1. 1

    Step 1 — Convert the Region to Cylindrical Coordinates

    The cylinder x² + y² = 4 becomes simply r = 2 in cylindrical coordinates. The solid fills the full circle around the z-axis, so θ goes from 0 to 2π. The height z goes from 0 to 3. Therefore: 0 ≤ θ ≤ 2π, 0 ≤ r ≤ 2, 0 ≤ z ≤ 3.
    Limits: θ ∈ [0, 2π], r ∈ [0, 2], z ∈ [0, 3]
  2. 2

    Step 2 — Write the Integral with dV = r dz dr dθ

    Since we want volume, the integrand f = 1. Including the Jacobian factor r, the integral is: V = ∫₀²π ∫₀² ∫₀³ r dz dr dθ.
    V = ∫₀²π ∫₀² ∫₀³ r dz dr dθ
  3. 3

    Step 3 — Integrate with Respect to z (Innermost)

    The integrand r does not depend on z, so integrating r with respect to z from 0 to 3 gives r × (3 − 0) = 3r.
    ∫₀³ r dz = 3r
  4. 4

    Step 4 — Integrate with Respect to r (Middle)

    Now integrate 3r with respect to r from 0 to 2. Using the power rule: ∫₀² 3r dr = 3 × (r²/2) evaluated from 0 to 2 = 3 × (4/2) = 3 × 2 = 6.
    ∫₀² 3r dr = 6
  5. 5

    Step 5 — Integrate with Respect to θ (Outermost)

    Finally, integrate 6 with respect to θ from 0 to 2π: ∫₀²π 6 dθ = 6 × (2π − 0) = 12π.
    V = 12π ≈ 37.70 cubic units
  6. 6

    Step 6 — Verify

    The formula for the volume of a cylinder is V = πr²h = π(2²)(3) = 12π. Our integral matches perfectly, confirming the answer.
    ✓ Confirmed: V = 12π

SECTION 7

Strengths, Limitations & When to Choose Cylindrical

Cylindrical coordinates are not always the best choice. The table below compares them to Cartesian and spherical coordinates, so you can make a quick decision when facing a triple integral.

FeatureCartesianCylindricalSpherical
Best forRectangular boxes, planesCylinders, cones, paraboloidsSpheres, hemispheres
Volume elementdx dy dzr dr dθ dzρ² sin φ dρ dθ dφ
Symmetry exploitedNone (flat faces)Circular cross-sectionsSpherical symmetry
Ease of limitsEasy for boxes; messy for curvesEasy when x² + y² appearsEasy when x² + y² + z² appears
Common pitfallSquare-root limitsForgetting the r factorForgetting ρ² sin φ factor

Comparison of coordinate systems for triple integrals

🧭

DECISION RULE

Here is a quick heuristic: look at the region and the integrand. If you see x² + y² in the boundary equations or the function, cylindrical coordinates will likely simplify the problem. If you see x² + y² + z², spherical is probably better. If the region is a plain box with flat faces, stick with Cartesian. Choosing the right coordinate system is like choosing the right tool: a wrench works great on bolts, but you would not use it to hammer a nail.

SECTION 8

Connection to Advanced Theory

The cylindrical triple integral is not an isolated technique—it connects to several deeper ideas in mathematics and physics. Understanding these connections will help you see the bigger picture as you continue into more advanced courses.

This LessonAdvanced Extension
Volume element dV = r dr dθ dzGeneral change-of-variables formula using the Jacobian determinant for any coordinate transformation
Computing volume: ∫∫∫ dVComputing mass, center of mass, and moments of inertia: ∫∫∫ ρ(r,θ,z) · r dz dr dθ
Cylindrical symmetry (r, θ, z)Spherical coordinates (ρ, θ, φ) for full 3D radial symmetry; generalized curvilinear coordinates
Evaluating definite triple integralsGauss's Divergence Theorem and Stokes' Theorem in vector calculus, which convert volume integrals to surface integrals

How this lesson connects to more advanced mathematics

In physics, the cylindrical coordinate triple integral appears constantly. Electric fields around wires, fluid flow through pipes, and heat distribution in cylindrical rods are all modeled with these integrals. In engineering, computing the moment of inertia of a cylindrical shaft requires exactly the technique you learned today, with the integrand changed from 1 (for volume) to r² times a density function. Mastering this coordinate system now will pay dividends across many future courses.

SECTION 9

Practice Problems

Question 1: CONCEPTUAL

When converting a triple integral from Cartesian to cylindrical coordinates, why must you include an extra factor of r in the volume element? Explain the geometric reasoning in your own words.
Show answer
The factor of r appears because the volume element in cylindrical coordinates is a curved wedge, not a rectangular box. The width of the wedge in the angular direction is the arc length r dθ, which depends on how far the element is from the z-axis. Farther out (larger r), the same angular increment dθ sweeps through more space. Multiplying by r accounts for this stretching, ensuring that we correctly measure the volume of each small piece. Without this factor, the integral would undercount volume far from the axis and overcount volume near it.

Question 2: BASIC CALCULATION

Evaluate the triple integral ∫₀²π ∫₀¹ ∫₀⁴ r dz dr dθ. What geometric solid does this integral represent?
Show answer
Working inside out: First, ∫₀⁴ r dz = 4r (since r is constant with respect to z). Second, ∫₀¹ 4r dr = 4 × (r²/2) from 0 to 1 = 4 × (1/2) = 2. Third, ∫₀²π 2 dθ = 2 × 2π = 4π. The answer is 4π. This integral computes the volume of a cylinder of radius 1 and height 4 centered on the z-axis. You can verify: V = πr²h = π(1)²(4) = 4π. ✓

Question 3: INTERMEDIATE

Use cylindrical coordinates to find the volume of the solid bounded below by the plane z = 0, above by the paraboloid z = 4 − r², and within the cylinder r = 2. Set up and evaluate the triple integral.
Show answer
The paraboloid z = 4 − r² equals 0 when r = 2, which aligns with the cylinder boundary. The limits are θ ∈ [0, 2π], r ∈ [0, 2], z ∈ [0, 4 − r²]. The integral is V = ∫₀²π ∫₀² ∫₀^(4−r²) r dz dr dθ. Inner integral: ∫₀^(4−r²) r dz = r(4 − r²). Middle integral: ∫₀² (4r − r³) dr = [2r² − r⁴/4] from 0 to 2 = (8 − 4) = 4. Outer integral: ∫₀²π 4 dθ = 8π. The volume is 8π ≈ 25.13 cubic units.

Question 4: APPLIED

A cylindrical water tank has radius 3 meters and height 5 meters. The density of sediment-laden water varies with height as ρ(z) = 1000 + 50z kg/m³ (denser at the top due to mixing). Use a triple integral in cylindrical coordinates to find the total mass of water in the tank.
Show answer
The mass is M = ∫∫∫ ρ dV = ∫₀²π ∫₀³ ∫₀⁵ (1000 + 50z) · r dz dr dθ. Inner integral: ∫₀⁵ (1000r + 50rz) dz = r[1000z + 25z²] from 0 to 5 = r(5000 + 625) = 5625r. Middle integral: ∫₀³ 5625r dr = 5625 × (r²/2) from 0 to 3 = 5625 × 4.5 = 25312.5. Outer integral: ∫₀²π 25312.5 dθ = 25312.5 × 2π = 50625π ≈ 159,043 kg. The total mass is 50625π kilograms, or roughly 159,043 kg.

Question 5: CRITICAL THINKING

Consider the region E inside the sphere x² + y² + z² = 9 and outside the cylinder x² + y² = 1. Set up (but do not fully evaluate) the triple integral in cylindrical coordinates that gives the volume of E. Explain how you determined the limits for z, and discuss whether cylindrical or spherical coordinates would be more efficient for this problem.
Show answer
In cylindrical coordinates, the sphere x² + y² + z² = 9 becomes r² + z² = 9, so z ranges from −√(9 − r²) to √(9 − r²). The cylinder x² + y² = 1 becomes r = 1. The volume integral is V = ∫₀²π ∫₁³ ∫_{−√(9−r²)}^{√(9−r²)} r dz dr dθ. The z-limits were found by solving r² + z² = 9 for z. The r-limits run from 1 (outside the cylinder) to 3 (the sphere's radius in the xy-plane). While this integral is doable in cylindrical coordinates, it requires evaluating ∫ r√(9 − r²) dr (a substitution). Spherical coordinates would make the sphere's boundary simpler (ρ = 3), but the cylinder's boundary becomes the more complex equation ρ sin φ = 1. Neither coordinate system is dramatically easier here—this is a problem where you must weigh the trade-offs. In practice, cylindrical is slightly more straightforward because the r-integral, while involving a square root, is a standard substitution.

SUMMARY

Lesson Summary

Summary

Cylindrical coordinates (r, θ, z) combine polar coordinates in the xy-plane with the standard vertical z-axis. They are the ideal choice for evaluating triple integrals over regions with circular symmetry—cylinders, cones, and paraboloids. The conversion rules are x = r cos θ, y = r sin θ, and z = z. The critical step when setting up the integral is replacing the Cartesian volume element dx dy dz with the cylindrical volume element dV = r dr dθ dz, where the extra factor of r is the Jacobian of the coordinate change.

To evaluate a triple integral in cylindrical form, work from the inside out: integrate with respect to z first (whose limits may depend on r and θ), then r (whose limits may depend on θ), and finally θ (whose limits are constants, often 0 to 2π). Mastering this technique opens the door to computing volumes, masses, centers of mass, and moments of inertia for rotationally symmetric objects—a skill that appears throughout physics and engineering.

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