Triple integrals in cylindrical coordinates are one of the most powerful tools you'll use in Calc III, and they show up constantly on exams—especially when you're dealing with regions that have circular symmetry. Think cylinders, cones, paraboloids, or any solid where the cross-section perpendicular to one axis is a circle. The moment you see phrases like "bounded by the cylinder x2+y2=4" or "region inside a cone," your brain should immediately jump to cylindrical coordinates. This isn't just about making integrals easier; it's about recognizing when and why a coordinate system matches the geometry of your problem.
You're being tested on three interconnected skills: coordinate conversion, setting up appropriate bounds, and correctly applying the Jacobian. The conceptual heart of this topic is understanding that changing coordinate systems requires adjusting your volume element—and forgetting that extra r in dV=rdrdθdz is one of the most common exam mistakes. Don't just memorize the formulas below—know why each piece exists and when each technique applies.
The Coordinate System Foundation
Before you can integrate, you need to fluently move between Cartesian and cylindrical representations. These conversions form the backbone of every problem you'll encounter.
Definition of Cylindrical Coordinates (r,θ,z)
r measures radial distance—the horizontal distance from the z-axis to the point's projection in the xy-plane
θ measures angular position—the angle from the positive x-axis, measured counterclockwise in the xy-plane
z remains unchanged—identical to Cartesian z, representing vertical height above or below the xy-plane
Conversion Formulas
Cartesian to cylindrical:r=x2+y2, θ=arctan(y/x) (adjust for quadrant), z=z
Cylindrical to Cartesian:x=rcosθ, y=rsinθ, z=z—these substitutions transform your integrand
Recognize common surfaces:x2+y2=a2 becomes simply r=a, which is why cylindrical coordinates excel for circular regions
Visualization of the System
Points live on concentric cylinders—each value of r defines a cylinder of that radius centered on the z-axis
Angular slices like pizza—θ sweeps around the z-axis, dividing space into wedge-shaped regions
Vertical stacking unchanged—the z-coordinate works exactly as in Cartesian, making cylinders and cones natural to describe
Compare: Cylindrical vs. Spherical coordinates—both handle circular symmetry, but cylindrical keeps z linear while spherical uses two angles. Use cylindrical when your region has a vertical axis of symmetry (cylinders, cones); use spherical for radial symmetry from a point (spheres, hemispheres).
The Jacobian and Volume Element
This is where students lose the most points. The volume element isn't just drdθdz—there's a critical factor that accounts for how space "stretches" in curvilinear coordinates.
Volume Element: dV=rdrdθdz
The factor r is non-negotiable—it compensates for the fact that arc length at radius r is rdθ, not just dθ
Geometric interpretation: small volume elements farther from the z-axis are larger, so r scales the contribution appropriately
Forgetting r is the #1 error—always write dV=rdrdθdz explicitly when setting up your integral
Jacobian for Cylindrical Coordinates
The Jacobian determinant equals r—this comes from computing ∂(r,θ,z)∂(x,y,z) and taking the absolute value
Connects to the change of variables theorem—the Jacobian ensures area/volume is preserved when transforming coordinate systems
Appears automatically in dV—when you write rdrdθdz, you've already incorporated the Jacobian
Compare: The Jacobian r in cylindrical vs. ρ2sinϕ in spherical—both arise from the same principle (measuring how coordinates stretch space), but spherical has two angular variables contributing. If an FRQ asks you to justify your volume element, cite the Jacobian.
Setting Up the Integral
The art of triple integrals lies in correctly identifying bounds and choosing an efficient integration order. This is where geometric reasoning meets computational strategy.
Setting Up Triple Integrals in Cylindrical Coordinates
Replace all Cartesian expressions—substitute x=rcosθ, y=rsinθ, and x2+y2=r2 throughout your integrand
Include the Jacobian factor r—your integral takes the form ∭f(r,θ,z)⋅rdrdθdz
Simplify before integrating—expressions like x2+y2 become simply r, often dramatically reducing complexity
Determining Integration Limits
θ bounds reflect angular extent—full rotation is 0 to 2π; half-space or wedge regions use smaller intervals
r bounds define radial reach—typically 0 to a constant or 0 to a function of θ for more complex regions
z bounds capture vertical extent—often functions of r (and sometimes θ), describing top and bottom surfaces
Order of Integration
dzdrdθ is most common—integrate vertically first when z-bounds depend on r, as with cones or paraboloids
Symmetry can eliminate variables—if the integrand is independent of θ, that integral often just contributes a factor of 2π
Switch order strategically—if one order creates difficult bounds or integrands, try another; the region determines what's possible
Compare: Integrating a cone vs. a cylinder—for a cone like z=r, your z-bounds depend on r (making dz first natural), while a cylinder r=2 has constant r-bounds regardless of z. Recognizing this distinction speeds up setup significantly.
Techniques and Applications
Knowing how to evaluate and when to apply cylindrical integrals separates competent students from excellent ones.
Techniques for Evaluating Triple Integrals
Exploit symmetry ruthlessly—odd functions integrated over symmetric intervals vanish; even functions can double half-integrals
Factor separable integrands—if f(r,θ,z)=g(r)⋅h(θ)⋅k(z), compute three single integrals and multiply
Sketch the region first—a quick drawing prevents bound errors and reveals simplifications you might otherwise miss
Applications: Volume, Mass, and Center of Mass
Volume calculation: set f=1 and compute ∭rdrdθdz—the integral directly gives volume
Mass with variable density: if ρ(r,θ,z) gives density, then M=∭ρ⋅rdrdθdz
Center of mass coordinates: compute xˉ=M1∭x⋅ρ⋅rdV and similarly for yˉ, zˉ—convert x and y to cylindrical form
Compare: Finding volume vs. finding mass—both use the same integral structure, but mass requires incorporating a density function ρ(r,θ,z). On FRQs, check whether density is constant (simplifying to volume × density) or variable (requiring full integration).
Quick Reference Table
Concept
Key Formula or Fact
Coordinate conversion (to cylindrical)
r=x2+y2, θ=arctan(y/x), z=z
Coordinate conversion (to Cartesian)
x=rcosθ, y=rsinθ, z=z
Volume element
dV=rdrdθdz
Jacobian determinant
J=r
Full rotation bounds
θ∈[0,2π]
Typical r bounds
r∈[0,R] or r∈[0,f(θ)]
Volume integral
V=∭rdrdθdz
Mass integral
M=∭ρ(r,θ,z)⋅rdrdθdz
Self-Check Questions
Why does the volume element in cylindrical coordinates include a factor of r, and what would go wrong if you omitted it?
Compare setting up bounds for a solid cylinder x2+y2≤4, 0≤z≤3 versus a cone z=x2+y2 below z=2. How do the z-bounds differ in structure?
Given the integral ∭(x2+y2)dV over a cylindrical region, what does the integrand become in cylindrical coordinates, and why does this simplify evaluation?
If a density function is ρ=z, explain how you would set up the integral for the mass of the solid bounded by r=1 and 0≤z≤4.
When would you choose drdzdθ as your integration order instead of the more common dzdrdθ? Give a geometric scenario where this makes sense.