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Triple Integral Calculator – Spherical, Cylindrical & Polar Coordinates

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Triple Integral Calculator

Convert between Cartesian, cylindrical, and spherical coordinates. Compute volume integrals for 3D shapes using the correct triple integral formula. A complete triple integral solver and integration limits reference for students and researchers.

🧮 Open Wolfram Alpha Triple Integral Solver →
📍 3D Coordinate System Converter

Enter Cartesian coordinates (x, y, z) to convert to Spherical and Cylindrical.

Volume Integral Calculator

Select a 3D shape, enter its dimensions, and see the triple integral formula, step-by-step evaluation, and volume in multiple units.

𝒥 Jacobian Calculator for Coordinate Transformations

The Jacobian determinant must be included when setting up triple integrals in curvilinear coordinates. Select a coordinate system to see the full Jacobian matrix, determinant calculation, and volume element.

Triple Integral Limits Visualizer

Select a 3D region and coordinate system to see the correct integration limits displayed as a properly formatted nested triple integral ∫∫∫.

What is a Triple Integral?

A triple integral extends the concept of integration to three-dimensional regions in space. Written as ∫∫∫E f(x, y, z) dV, it sums the value of a function f over every infinitesimal volume element dV within a 3D region E. By Fubini's theorem, this triple integral equals three successive single integrals — computed from the inside out — making it a practical triple integral solver for real-world problems.

Physically, triple integrals compute mass (when f is density), total electric charge, probability over a 3D distribution, and — most importantly — volume (when f = 1, so ∫∫∫E 1 dV = volume of E). This page functions as a complete multiple integral calculator and multiple integral solver for common academic problems.

General iterated form:

ba g2(x)g1(x) h2(x,y)h1(x,y) f(x, y, z) dz dy dx

Six orders of integration are possible for Cartesian coordinates (dz dy dx, dz dx dy, dy dz dx, dy dx dz, dx dz dy, dx dy dz). The choice affects the limits but not the final result.

Triple Integrals in Cylindrical Coordinates

Use cylindrical coordinates when the integration region has circular symmetry around the z-axis — such as cylinders, cones, and paraboloids. In cylindrical coordinates, x = r cos θ, y = r sin θ, z = z. The volume element becomes dV = r dr dθ dz, where r is the Jacobian — never forget to include it.

The transformed triple integral is: ∫∫∫E f(x,y,z) dV = ∫∫∫ f(r cos θ, r sin θ, z) r dr dθ dz. This polar coordinates integral calculator approach makes cylindrical and cone problems tractable.

Worked Example: Volume of a Cylinder (radius 2, height 5)

V = 0 20 50 r dz dr dθ

  1. Inner: ∫50 r dz = 5r
  2. Middle: ∫20 5r dr = [5r²/2]20 = 10
  3. Outer: ∫0 10 dθ = 20π ≈ 62.83
  4. V = 20π ≈ 62.83 units³ (matches πR²h = π(4)(5) = 20π ✓)

Triple Integrals in Spherical Coordinates

Use spherical coordinates for regions with spherical symmetry — spheres, hemispheres, spherical shells, and cones with apex at the origin. The relations are x = ρ sin φ cos θ, y = ρ sin φ sin θ, z = ρ cos φ. The volume element is dV = ρ² sin φ dρ dφ dθ — this ρ² sin φ factor is the Jacobian.

The spherical integral: ∫∫∫E f dV = 0π0R0 f(ρ,φ,θ) ρ² sin φ dρ dφ dθ.

Worked Example 1: Volume of Sphere radius R

  1. Inner: ∫R0 ρ² dρ = R³/3
  2. Middle: ∫π0 sin φ dφ = [−cos φ]π0 = 2
  3. Outer: ∫0 dθ = 2π
  4. Product: (R³/3)(2)(2π) = 4πR³/3 ✓

Worked Example 2: Volume of Upper Hemisphere radius 3

  1. φ limit changes from 0 to π/2 (upper half only)
  2. Inner: ∫30 ρ² dρ = 27/3 = 9
  3. Middle: ∫π/20 sin φ dφ = [−cos φ]π/20 = 1
  4. Outer: ∫0 dθ = 2π
  5. Product: (9)(1)(2π) = 18π ≈ 56.55 units³

How to Set Up Triple Integral Limits

Setting up limits correctly is the key challenge in solving triple integrals. Follow this systematic approach:

  1. Identify the region — sketch a diagram of the 3D solid.
  2. Choose coordinates — Cartesian for boxes, cylindrical for cylinders/cones, spherical for spheres.
  3. Outermost limits — must be constants (e.g., 0 to 2π for θ).
  4. Middle limits — may be functions of the outermost variable only.
  5. Innermost limits — may depend on both outer variables.

Region 1: Rectangular Box (0≤x≤2, 0≤y≤3, 0≤z≤4)

20 30 40 dz dy dx = 24

Region 2: Sphere of Radius R (Spherical)

0 π0 R0 ρ² sin φ dρ dφ dθ = 4πR³/3

Region 3: Cylinder Radius R, Height h (Cylindrical)

0 R0 h0 r dz dr dθ = πR²h

Region 4: Cone Height h, Base Radius R (Cylindrical)

0 h0 Rz/h0 r dr dz dθ = πR²h/3

Region 5: Between Spheres radius a and b

0 π0 ba ρ² sin φ dρ dφ dθ

Region 6: Upper Hemisphere Radius R

0 π/20 R0 ρ² sin φ dρ dφ dθ = 2πR³/3

Triple Integral Formulas — Reference Table

This reference table shows the triple integral, coordinate system, and exact formula for common 3D shapes. Color-coded: Cartesian Cylindrical Spherical.

Shape System Triple Integral ∫∫∫ Result
Sphere (R) Spherical 0π0R0 ρ²sinφ dρdφdθ 4πR³/3
Hemisphere (R) Spherical 0π/20R0 ρ²sinφ dρdφdθ 2πR³/3
Cylinder (R, h) Cylindrical 0R0h0 r dz dr dθ πR²h
Cone (R, h) Cylindrical 0h0Rz/h0 r dr dz dθ πR²h/3
Box (a, b, c) Cartesian a0b0c0 dz dy dx abc
Ellipsoid (a,b,c) Spherical Scaled sphere transformation 4πabc/3
Sph. Shell (r,R) Spherical 0π0Rr ρ²sinφ dρdφdθ 4π(R³−r³)/3
Paraboloid (R, h) Cylindrical 0R0hr²/R²0 r dz dr dθ πR²h/2

Worked Examples

1. Triple Integral Over a Sphere in Spherical Coordinates

Evaluate the volume of a sphere of radius 2 using spherical coordinates. The triple integral ∫∫∫ ρ² sin φ dρdφdθ with ρ ∈ [0,2], φ ∈ [0,π], θ ∈ [0,2π] gives (R³/3)(2)(2π) = (8/3)(2)(2π) = 32π/3 ≈ 33.51.

2. Triple Integral in Cylindrical Coordinates for a Cylinder

For a cylinder of radius 3 and height 4: ∫03040 r dz dr dθ. Inner: 4r. Middle: ∫30 4r dr = [2r²]30 = 18. Outer: 18 × 2π = 36π ≈ 113.10. Confirms πR²h = π(9)(4) = 36π ✓.

3. Convert Cartesian to Spherical Coordinates Integral

Replace x² + y² + z² with ρ². Replace dx dy dz with ρ² sin φ dρdφdθ. For a ball of radius R: ∫∫∫ (x²+y²+z²) dV = ∫∫∫ ρ² · ρ² sin φ dρdφdθ = (R&sup5;/5)(2)(2π) = 4πR&sup5;/5.

4. Volume of a Cone Using a Triple Integral

Cone with apex at origin, base radius R, height h. Cylindrical: ∫0h0Rz/h0 r dr dz dθ. Innermost: [r²/2]Rz/h0 = R²z²/(2h²). Middle: ∫h0 R²z²/(2h²) dz = R²h/6. Outer: ×2π = πR²h/3 ✓.

5. Triple Integral Over a Rectangular Box

Box [0,3]×[0,4]×[0,5]: ∫304050 dz dy dx. Inner: 5. Middle: ∫40 5 dy = 20. Outer: ∫30 20 dx = 60. Volume = 60 = l × w × h = 3 × 4 × 5 = 60 ✓.

6. Double Integral in Polar Coordinates

Area of disk radius 3: ∫030 r dr dθ. Inner: [r²/2]30 = 9/2. Outer: (9/2)(2π) = 9π ≈ 28.27 = π(3)² ✓. The Jacobian r in the double polar integral ensures correct area measurement.

7. Jacobian for Spherical Coordinate Transformation

Compute det[∂(x,y,z)/∂(ρ,φ,θ)]. The 3×3 matrix of partial derivatives evaluates to det = ρ² sin φ, confirming dV = ρ² sin φ dρdφdθ. At ρ=2, φ=π/4: Jacobian = 4 sin(45°) = 4/√2 ≈ 2.828.

8. Changing Order of Integration

For ∫101xy0 f dz dy dx, the region is 0≤x≤y≤1, 0≤z≤y. To switch to dz dx dy: ∫10y0y0 f dz dx dy. Always re-examine which variable bounds which by reading the region from the diagram.

9. Volume Between Two Spheres

Spherical shell between radii 1 and 3: ∫0π031 ρ² sin φ dρdφdθ. Inner: [ρ³/3]31 = 27/3 − 1/3 = 26/3. Middle: 2. Outer: 2π. Product: 4π(26/3) ≈ 109.0 = 4π(27−1)/3 = 4π(26)/3 ✓.

10. Triple Integral for a Hemisphere

Upper hemisphere radius R: φ from 0 to π/2 only. ∫0π/20R0 ρ² sin φ dρdφdθ. Inner: R³/3. Middle: ∫π/20 sin φ = 1. Outer: 2π. Volume = 2πR³/3 = half of 4πR³/3 ✓.

Frequently Asked Questions

What is a triple integral used for?
Triple integrals compute quantities over 3D regions: volume (∫∫∫ 1 dV), mass (∫∫∫ ρ(x,y,z) dV), electric charge, moments of inertia, and probability. When the integrand f = 1, the triple integral gives the exact volume of the region E.
How do you evaluate a triple integral?
By Fubini's theorem, evaluate three successive single integrals from the inside out. Compute the innermost integral (treating outer variables as constants), substitute the result, compute the middle integral, then the outermost. The limits of inner integrals may depend on outer variables; the outermost limits must be constants.
When should I use spherical coordinates for a triple integral?
Use spherical coordinates when the region is a sphere, hemisphere, spherical shell, or cone with apex at the origin. The Jacobian ρ² sin(φ) must be included: dV = ρ² sin φ dρdφdθ. This spherical integral calculator approach simplifies limits dramatically for these symmetric regions.
When should I use cylindrical coordinates?
Use cylindrical coordinates for regions with circular symmetry around the z-axis: cylinders, paraboloids, cones. The Jacobian is r: dV = r dr dθ dz. This is essentially the triple polar integral calculator approach extending 2D polar to 3D.
What is the Jacobian in a triple integral?
The Jacobian is the determinant of the matrix of partial derivatives when changing coordinate systems. It scales volume correctly under the transformation. Cylindrical: J = r. Spherical: J = ρ² sin(φ). Forgetting the Jacobian is the most common error in setting up triple integrals in non-Cartesian coordinates.
What is the volume element in spherical coordinates?
dV = ρ² sin(φ) dρ dφ dθ. Here ρ is the radial distance from the origin (0 to R), φ is the polar angle from the z-axis (0 to π), and θ is the azimuthal angle in the xy-plane (0 to 2π). The factor ρ² sin(φ) is the Jacobian of the spherical transformation.
How do I set limits for a triple integral over a sphere?
In spherical coordinates: ρ from 0 to R, φ from 0 to π, θ from 0 to 2π. The integral is ∫0π0R0 ρ² sin φ dρdφdθ = 4πR³/3. For a hemisphere, change φ upper limit to π/2.
What is the difference between a double and triple integral?
A double integral ∫∫D f(x,y) dA integrates over a 2D region, computing area or volume under a surface. A triple integral ∫∫∫E f(x,y,z) dV integrates over a 3D solid, computing volume, mass, or other 3D quantities. Triple integrals require three nested integrations and three sets of limits.
How do I convert a triple integral from Cartesian to cylindrical?
Substitute x = r cos θ, y = r sin θ, keep z unchanged. Replace dx dy dz with r dr dθ dz (multiply by the Jacobian r). Convert limits: x² + y² ≤ R² becomes r ≤ R. Full form: ∫∫∫ f(r cos θ, r sin θ, z) · r dr dθ dz.
What does dV equal in spherical coordinates?
dV = ρ² sin(φ) dρ dφ dθ. This is equivalent to three infinitesimal arc lengths multiplied: × ρ × ρ sin(φ). The factor ρ² sin(φ) ensures volumes are measured correctly in the curved spherical coordinate system.

Related Calculators

📍 Coordinate Systems
C
Cartesian: (x, y, z) — boxes, rectangular regions.
Y
Cylindrical: (r, θ, z) — cylinders, cones, circular symmetry.
S
Spherical: (ρ, φ, θ) — spheres, hemispheres, full 3D symmetry.
𝒥 Jacobian Quick Ref
2D
Polar: dA = r dr dθ
Jacobian = r
Y
Cylindrical: dV = r dr dθ dz
Jacobian = r
S
Spherical: dV = ρ² sin φ dρdφdθ
Jacobian = ρ² sin φ
📐 Volume Formulas
Sphere 4πR³/3
Hemisphere 2πR³/3
Cylinder πR²h
Cone πR²h/3
Torus 2π²Rr²
Ellipsoid 4πabc/3
💡 Key Symbol Reference
∫∫∫
Triple integral over region E
ρ
Radial distance (spherical)
φ
Polar angle from z-axis (0 to π)
θ
Azimuthal angle (0 to 2π)
r
Radial distance (cylindrical)
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