All chapters Unit 2 · Integral & Vector Calculus

Triple integrals: Cartesian, cylindrical, spherical

Chapter 12 of 15
The hook

One ball, three coordinate systems

A CT scanner does not photograph your insides — it reconstructs them. It fires X-rays through your body from every angle, measures how much each ray is absorbed, and from those shadows rebuilds the density at every point. The total mass it recovers is one number: TδdV\displaystyle\iiint_T \delta\,dV, the density δ\delta summed over the solid region TT. That triple integral is the machine this chapter builds — and the first lesson is that the coordinate system you choose can turn a page of algebra into three lines.

Here is the cleanest possible demonstration. The volume of a ball of radius aa is 43πa3\tfrac{4}{3}\pi a^3 — the formula everyone memorises and almost no one can derive. Watch it fall out of spherical coordinates, then watch Cartesian drown in square roots.

ρ spherical · 3 lines dV = ρ² sin φ dρ dφ dθ Cartesian · a page z from −√(a²−x²−y²) to +√(a²−x²−y²)
Same solid. Left: spherical coordinates slice it into onion shells of constant ρ\rho — three clean integrals. Right: Cartesian coordinates chop it into slabs whose every limit is a nested square root ±a2x2y2\pm\sqrt{a^2-x^2-y^2} — a page of work for the same number.

In spherical coordinates the ball is just 0ρa0 \le \rho \le a, 0ϕπ0 \le \phi \le \pi, 0θ2π0 \le \theta \le 2\pi, the volume element is dV=ρ2sinϕdρdϕdθdV = \rho^2\sin\phi\,d\rho\,d\phi\,d\theta, and the whole computation is:

02π ⁣ ⁣0π ⁣ ⁣0aρ2sinϕdρdϕdθ=2π2a33=43πa3.\int_0^{2\pi}\!\!\int_0^{\pi}\!\!\int_0^{a}\rho^2\sin\phi\,d\rho\,d\phi\,d\theta = 2\pi\cdot 2\cdot \frac{a^3}{3} = \frac{4}{3}\pi a^3.

In Cartesian coordinates the very same volume is

aa ⁣a2x2a2x2 ⁣a2x2y2a2x2y21dzdydx,\int_{-a}^{a}\!\int_{-\sqrt{a^2-x^2}}^{\sqrt{a^2-x^2}}\! \int_{-\sqrt{a^2-x^2-y^2}}^{\sqrt{a^2-x^2-y^2}} 1\,dz\,dy\,dx,

which is correct, doable, and miserable — three trigonometric substitutions deep. The mathematics is identical; only the coordinates differ. Choosing the coordinate system is the skill this chapter trains.

Why this matters

Single integrals measure along a line, double integrals over a flat region. The triple integral is how you total anything spread through a three-dimensional body: its volume, its mass, its centre of mass, the heat stored in it, the dose a tumour absorbs. Every one of those is T(something)dV\iiint_T (\text{something})\,dV. The hard part is almost never the calculus — it is setting up the limits, and picking the coordinate system in which the limits are simple. Get that habit and the integrals do themselves.

The method that always works

The 3-D ritual, and Cartesian triple integrals

Chapter 10 gave you a ritual for double integrals: sketch → describe the region → read off the limits → integrate. Triple integrals extend it by exactly one move. Here is the full ritual, and you never skip it:

The 3-D ritual
  1. Sketch the solid TT (roughly — you are not drawing for an art class).
  2. Shadow. Project TT straight down onto a coordinate plane (usually xyxy). That silhouette is a 2-D region — and it supplies the outer double integral's limits.
  3. Slice. Over each point of the shadow, run a vertical line up through the solid. It enters through a floor surface and leaves through a roof surface — those two surfaces are the inner zz-limits.
  4. Limits, then integrate from the inside out: zz first (floor to roof), then the shadow's double integral.

One honest sentence before you panic about "seeing" a solid in your head: nobody pictures a 3-D region whole. Every competent person projects it to a flat shadow and slices it — that is what the ritual is. "I can't visualise in 3-D" names a thing literally no one does; it is not a deficit, it is the universal condition, and shadow-and-slice is the workaround everyone uses.

The Cartesian triple integral, by shadow and slice
TfdV=shadow ⁣[floor(x,y)roof(x,y)f(x,y,z)dz]dA.\iiint_T f\,dV = \iint_{\text{shadow}}\!\left[\int_{\text{floor}(x,y)}^{\text{roof}(x,y)} f(x,y,z)\,dz\right]dA.
Worked example · WE-1 · pure setup, the tetrahedron

Find the volume of the tetrahedron TT: x,y,z0x, y, z \ge 0 and x+y+z1x + y + z \le 1.

Shadow. Set z=0z = 0: the solid's footprint on the xyxy-plane is the triangle 0x10 \le x \le 1, 0y1x0 \le y \le 1 - x. Slice. Above a point (x,y)(x, y) of that triangle, zz runs from the floor z=0z = 0 up to the roof z=1xyz = 1 - x - y (the slanted plane). So

V=01 ⁣ ⁣01x ⁣ ⁣01xy1dzdydx=01 ⁣ ⁣01x(1xy)dydx=01(1x)22dx=16.V = \int_0^1\!\!\int_0^{1-x}\!\!\int_0^{1-x-y} 1\,dz\,dy\,dx = \int_0^1\!\!\int_0^{1-x}(1-x-y)\,dy\,dx = \int_0^1 \frac{(1-x)^2}{2}\,dx = \frac{1}{6}.

The whole skill was the setup; the integration was three easy steps. Notice the structure of the limits — outer constant, each inner limit depending only on the variables further out. That nesting is the single most-tested correctness check in the chapter.

Worked example · WE-2 · the integrand rides along

Over the same tetrahedron, evaluate TxdV\displaystyle\iiint_T x\,dV (think of xx as a density that grows away from the yzyz-plane).

TxdV=01 ⁣ ⁣01x ⁣ ⁣01xyxdzdydx=01x(1x)22dx=124.\iiint_T x\,dV = \int_0^1\!\!\int_0^{1-x}\!\!\int_0^{1-x-y} x\,dz\,dy\,dx = \int_0^1 x\,\frac{(1-x)^2}{2}\,dx = \frac{1}{24}.

The point worth carrying: the integrand changed nothing about the limits. Volume, mass, a moment — same region, same shadow, same slice; only the function inside changes. Set the region up once and every quantity over it is within reach.

When there is an axis of symmetry

Cylindrical coordinates: polar, with a z-axis

Cylindrical coordinates are nothing new — they are Chapter 10's polar coordinates with the zz-axis carried along unchanged:

x=rcosθ,y=rsinθ,z=z,dV=rdrdθdz.x = r\cos\theta, \qquad y = r\sin\theta, \qquad z = z, \qquad \boxed{\,dV = r\,dr\,d\theta\,dz\,}.

That rr in the volume element is exactly the polar rr you were told in Chapter 10 never to drop — and Chapter 11 named it for what it is: the Jacobian of the polar map. Same factor, same reason, now with a height. (We do not re-derive it here; that was Chapter 11's whole job.)

When to reach for cylindrical

Three tells, any one of which is enough: an axis of rotational symmetry; a circular (or annular) shadow in the xyxy-plane; or an integrand built from x2+y2x^2 + y^2 (which becomes a clean r2r^2). When you see a cylinder, a cone, a paraboloid, or "rotated about the zz-axis," reach for rdrdθdzr\,dr\,d\theta\,dz.

Worked example · WE-3 · the load-bearing r

Find the volume of the solid above the paraboloid z=x2+y2z = x^2 + y^2 and below the plane z=4z = 4.

Shadow. The two surfaces meet where x2+y2=4x^2 + y^2 = 4, so the footprint is the disk r2r \le 2. Slice. Above a point at radius rr, the solid runs from the floor z=r2z = r^2 (the paraboloid, since x2+y2=r2x^2+y^2 = r^2) up to the roof z=4z = 4. With dV=rdrdθdzdV = r\,dr\,d\theta\,dz:

V=02π ⁣ ⁣02 ⁣ ⁣r24rdzdrdθ=02π ⁣ ⁣02r(4r2)drdθ=2π[2r2r44]02=2π4=8π.V = \int_0^{2\pi}\!\!\int_0^{2}\!\!\int_{r^2}^{4} r\,dz\,dr\,d\theta = \int_0^{2\pi}\!\!\int_0^{2} r(4 - r^2)\,dr\,d\theta = 2\pi\Big[2r^2 - \tfrac{r^4}{4}\Big]_0^2 = 2\pi\cdot 4 = 8\pi.

Watch the rr. Drop it from the element — integrate (4r2)(4 - r^2) alone — and you get 32π333.5\tfrac{32\pi}{3} \approx 33.5 instead of 8π25.18\pi \approx 25.1: a wrong answer that looks perfectly reasonable. There is no sign it is wrong except that you skipped the Jacobian. This exact slip returns, dressed up, in the gauntlet.

End of sitting 1 — you can now run the shadow-and-slice ritual in Cartesian and in cylindrical coordinates, and you know the cylindrical rr is the polar Jacobian, never optional. After the break: spherical coordinates and their famous sinϕ\sin\phi; then the Coordinate Lab to drill the one decision that matters — which system — and the exam-shaped practice set.

When everything radiates from the origin

Spherical coordinates, and the sinϕ\sin\phi everyone drops

Spherical coordinates pin a point by its distance from the origin and two angles:

Spherical coordinates (φ measured from the +z-axis)
x=ρsinϕcosθ,y=ρsinϕsinθ,z=ρcosϕ,dV=ρ2sinϕdρdϕdθ.x = \rho\sin\phi\cos\theta, \quad y = \rho\sin\phi\sin\theta, \quad z = \rho\cos\phi, \qquad \boxed{\,dV = \rho^2\sin\phi\,d\rho\,d\phi\,d\theta\,}.
  • ρ0\rho \ge 0 is the straight-line distance from the origin (00 \to \infty).
  • ϕ\phi is the angle down from the +z+z-axis (the colatitude), 0π0 \to \pi: ϕ=0\phi = 0 points straight up, ϕ=π\phi = \pi straight down, ϕ=π2\phi = \tfrac{\pi}{2} is the equator.
  • θ\theta is the same azimuth as before, going around, 02π0 \to 2\pi. Note r=ρsinϕr = \rho\sin\phi ties spherical back to cylindrical.
Notation convention — check the angle names

In this chapter, θ\theta is the azimuth in the xyxy-plane with 0θ2π0\le\theta\le2\pi, while ϕ\phi is measured down from the positive zz-axis with 0ϕπ0\le\phi\le\pi. Some books interchange the names θ\theta and ϕ\phi. That is only a relabelling: keep the stated ranges and attach sin(polar angle)\sin(\text{polar angle}) to the angle measured from the zz-axis.

The headline mark-loser: the dropped sinϕ\sin\phi

Why is the element ρ2sinϕ\rho^2\sin\phi and not just ρ2\rho^2? Picture the little box cut out by nudging each coordinate: its sides are dρd\rho (outward), ρdϕ\rho\,d\phi (north–south), and ρsinϕdθ\rho\sin\phi\,d\theta (east–west). That last side is short near the poles and longest at the equator, because the circles of constant latitude shrink to a point at the poles — and sinϕ\sin\phi is exactly that shrink factor. Multiply the three sides: dρρdϕρsinϕdθ=ρ2sinϕdρdϕdθd\rho \cdot \rho\,d\phi \cdot \rho\sin\phi\,d\theta = \rho^2\sin\phi\,d\rho\,d\phi\,d\theta. Forget the sinϕ\sin\phi and you are pretending the Earth's longitude lines stay equally far apart all the way to the pole. This is the three-dimensional cousin of Chapter 11's dropped rr, and the single most common lost mark in the chapter.

When to reach for spherical

Reach for it when the geometry radiates from the origin: spheres, balls, cones with their apex at the origin, regions between two concentric spheres, or an integrand built from x2+y2+z2x^2 + y^2 + z^2 (which becomes a clean ρ2\rho^2). If the boundary is "ρ=\rho = constant," spherical makes the outer limit a single number.

Worked example · WE-4 · the sin φ does visible work

Evaluate B(x2+y2+z2)dV\displaystyle\iiint_B (x^2 + y^2 + z^2)\,dV over the unit ball BB: ρ1\rho \le 1.

The integrand is x2+y2+z2=ρ2x^2 + y^2 + z^2 = \rho^2, and dV=ρ2sinϕdρdϕdθdV = \rho^2\sin\phi\,d\rho\,d\phi\, d\theta, so the whole thing is ρ2ρ2sinϕ=ρ4sinϕ\rho^2 \cdot \rho^2\sin\phi = \rho^4\sin\phi:

02π ⁣ ⁣0π ⁣ ⁣01ρ4sinϕdρdϕdθ=02π ⁣dθ2π0π ⁣sinϕdϕ201 ⁣ρ4dρ1/5=2π215=4π5.\int_0^{2\pi}\!\!\int_0^{\pi}\!\!\int_0^{1}\rho^4\sin\phi\,d\rho\,d\phi\,d\theta = \underbrace{\int_0^{2\pi}\!d\theta}_{2\pi}\cdot \underbrace{\int_0^{\pi}\!\sin\phi\,d\phi}_{2}\cdot \underbrace{\int_0^{1}\!\rho^4\,d\rho}_{1/5} = 2\pi\cdot 2\cdot\tfrac15 = \frac{4\pi}{5}.

The 0πsinϕdϕ=2\int_0^\pi \sin\phi\,d\phi = 2 is unmissable here. Drop the sinϕ\sin\phi and you would compute 2ππ15=2π253.952\pi\cdot\pi\cdot\tfrac15 = \tfrac{2\pi^2}{5} \approx 3.95 instead of 4π52.51\tfrac{4\pi}{5}\approx 2.51 — wrong, and again with nothing to flag it but the missing factor.

Worked example · WE-5 · application: the centroid of a hemisphere

Where is the centre of mass of a uniform solid hemisphere of radius aa (z0z \ge 0, ρa\rho \le a)? By symmetry xˉ=yˉ=0\bar x = \bar y = 0; only zˉ\bar z is in question. We need the volume and the zz-moment.

Volume (a hemisphere, ϕ\phi only 0π20 \to \tfrac{\pi}{2}):

V=02π ⁣ ⁣0π/2 ⁣ ⁣0aρ2sinϕdρdϕdθ=2π1a33=23πa3.V = \int_0^{2\pi}\!\!\int_0^{\pi/2}\!\!\int_0^{a}\rho^2\sin\phi\,d\rho\,d\phi\,d\theta = 2\pi\cdot 1\cdot\frac{a^3}{3} = \frac{2}{3}\pi a^3.

zz-moment (with z=ρcosϕz = \rho\cos\phi, the integrand is ρcosϕρ2sinϕ=ρ3cosϕsinϕ\rho\cos\phi\cdot\rho^2\sin\phi = \rho^3\cos\phi\sin\phi):

zdV=02π ⁣ ⁣0π/2 ⁣ ⁣0aρ3cosϕsinϕdρdϕdθ=2π120π/2cosϕsinϕdϕa44=πa44.\iiint z\,dV = \int_0^{2\pi}\!\!\int_0^{\pi/2}\!\!\int_0^{a}\rho^3\cos\phi\sin\phi\, d\rho\,d\phi\,d\theta = 2\pi\cdot\underbrace{\tfrac12}_{\int_0^{\pi/2}\cos\phi\sin\phi\,d\phi}\cdot \frac{a^4}{4} = \frac{\pi a^4}{4}.

So

zˉ=zdVV=πa4/423πa3=3a8.\bar z = \frac{\iiint z\,dV}{V} = \frac{\pi a^4/4}{\tfrac23\pi a^3} = \frac{3a}{8}.

The centre of mass sits at 3a8\tfrac{3a}{8} up the axis — not halfway, because there is more material near the flat base than near the dome. 3a8\tfrac{3a}{8} is a classic, memorable result, and a favourite exam number.

Interactive playground

The Coordinate Lab

The skill this chapter trains is a decision: which coordinate system, and therefore which volume element. So commit to both before the Lab tells you anything. Pick a solid, choose a coordinate system, choose its volume element dVdV — and only then does the Lab reveal whether your system was the clean one and whether your element was right. A wrong element that names the exact factor you dropped is the whole point; recognising the right setup after being shown it is not the same skill as choosing it.

The Coordinate Lab
Solid:
the solid
Step 1 · commit a coordinate system
Step 2 · commit the volume element dV

Two of the five element chips are booby-traps — the dropped rr and the dropped sinϕ\sin\phi. They are never the right element, in any system. The set-up integral and its value appear only when both your commitments are correct.

What to notice
  • The solid's symmetry chooses the system. Origin-centred and round → spherical; an axis with circular cross-sections → cylindrical; flat faces at right angles → Cartesian.
  • A correct element in the wrong system still "works" — and is a nightmare. You can integrate the ball in Cartesian with dxdydzdx\,dy\,dz; the Lab grants it is correct, then points at the three clean lines spherical would have given.
  • The traps are the marks you lose. Choosing cylindrical and "drdθdzdr\, d\theta\,dz" drops the rr; choosing spherical and "ρ2dρdϕdθ\rho^2\,d\rho\,d\phi\,d\theta" drops the sinϕ\sin\phi. Neither is ever the volume element.

Retrieval gauntlet

Commit to an answer before reading the feedback. These interleave Cartesian, cylindrical and spherical on purpose — knowing which system a solid wants is half the skill.

Quiz 1 · Cartesian setup — which integral is the tetrahedron?

Which iterated integral correctly gives the volume of the tetrahedron x,y,z0x, y, z \ge 0, x+y+z1x + y + z \le 1?

Quiz 2 · cylindrical, and the r

The solid above the paraboloid z=x2+y2z = x^2 + y^2 and below z=4z = 4 has volume:

Quiz 3 · spherical, and the sin φ

The "ice-cream" solid inside the sphere ρ=1\rho = 1 and inside the cone ϕπ3\phi \le \tfrac{\pi}{3} has volume:

Predict the next step. You have the ice-cream wedge sketched and you know the element is ρ2sinϕ\rho^2\sin\phi. Before revealing: what are the three limits, and which integral produces the 12\tfrac12?

Limits. Inside the sphere ρ=1\rho = 1: 0ρ10 \le \rho \le 1. Inside the cone measured from the axis: 0ϕπ30 \le \phi \le \tfrac{\pi}{3}. All the way around: 0θ2π0 \le \theta \le 2\pi. So

V=02π ⁣ ⁣0π/3 ⁣ ⁣01ρ2sinϕdρdϕdθ=2π[cosϕ]0π/313=2π(112)13=π3.V = \int_0^{2\pi}\!\!\int_0^{\pi/3}\!\!\int_0^{1}\rho^2\sin\phi\,d\rho\,d\phi\,d\theta = 2\pi\cdot\Big[-\cos\phi\Big]_0^{\pi/3}\cdot\frac13 = 2\pi\cdot\big(1 - \tfrac12\big)\cdot\frac13 = \frac{\pi}{3}.

The 12\tfrac12 is the ϕ\phi-integral: 0π/3sinϕdϕ=1cosπ3=112=12\int_0^{\pi/3}\sin\phi\,d\phi = 1 - \cos\tfrac{\pi}{3} = 1 - \tfrac12 = \tfrac12. Use sin\sin of the angle instead of this, and you land on the 3π3\tfrac{\sqrt3\,\pi}{3} distractor.

Quiz 4 · choose the system — do not integrate

Match each solid to the coordinate system with the cleanest limits:  (i) the ball x2+y2+z29x^2+y^2+z^2 \le 9;  (ii) the cylinder x2+y21, 0z5x^2+y^2 \le 1,\ 0 \le z \le 5;  (iii) the box 0x2, 0y3, 0z10 \le x \le 2,\ 0 \le y \le 3,\ 0 \le z \le 1.

Quiz 5 · spherical, integrand and element both convert

Converting Bx2+y2+z2dV\displaystyle\iiint_B \sqrt{x^2+y^2+z^2}\,dV over the unit ball BB to spherical coordinates and evaluating gives:

Predict the next step. The trap in Q5 is the power of ρ\rho. Before revealing: what does x2+y2+z2\sqrt{x^2+y^2+z^2} become, and what power of ρ\rho does the integrand carry once you include the element?

Integrand. x2+y2+z2=ρ2=ρ\sqrt{x^2+y^2+z^2} = \sqrt{\rho^2} = \rho — the first power. Multiply by the element ρ2sinϕ\rho^2\sin\phi: the integrand is ρρ2sinϕ=ρ3sinϕ\rho\cdot\rho^2\sin\phi = \rho^3\sin\phi. Then

02π ⁣ ⁣0π ⁣ ⁣01ρ3sinϕdρdϕdθ=2π214=π.\int_0^{2\pi}\!\!\int_0^{\pi}\!\!\int_0^{1}\rho^3\sin\phi\,d\rho\,d\phi\,d\theta = 2\pi\cdot 2\cdot\frac14 = \pi.

Two separate ρ\rho's are in play: one from the integrand (ρ1\rho^1) and two from the element (ρ2\rho^2). Lose track of either — call the root ρ2\rho^2, or drop the element's ρ2\rho^2 — and you land on a wrong-but-plausible 4π5\tfrac{4\pi}{5} or 2π2\pi.

Exam translator

What the exam will actually ask

Exam shapes

In standard Indian engineering-math exams, and likely in MCC201A unless your class notes differ, triple integrals wear four costumes — each one you have now seen worked:

  • "Evaluate TfdV\iiint_T f\,dV over ⟨solid⟩" → run the ritual: sketch, shadow, slice (WE-1, WE-2).
  • "Find the volume / mass / centroid" → volume 1dV\iiint 1\,dV; mass δdV\iiint \delta\,dV; centroid zˉ=zδdVmass\bar z = \dfrac{\iiint z\,\delta\,dV}{\text{mass}} (WE-5).
  • "Evaluate using cylindrical / spherical coordinates" → match the element. The dropped rr and dropped sinϕ\sin\phi are the classic lost marks (WE-3, WE-4).
  • "Change to a convenient coordinate system" → the question is the decision: the system whose symmetry matches the solid (Beat 1 thesis, Q4).

Worked solutions are complete; nothing points off this page. Do them as listed — interleaved on purpose — not blocked by method. Two of them, PR5 and PR7, open with a faded bridge: part of the work is set out, the key step left for you to predict.

PR1 · Cartesian · a tetrahedron

Shape · coordinate-plane tetrahedron ⇒ Cartesian shadow + slice

PR1. Find the volume of the tetrahedron bounded by the coordinate planes and the plane x+2y+z=4x + 2y + z = 4.

Shadow. Set z=0z = 0: the footprint is x+2y4x + 2y \le 4, x,y0x, y \ge 0, so 0x40 \le x \le 4, 0y4x20 \le y \le \tfrac{4-x}{2}. Slice. zz from 00 to the roof z=4x2yz = 4 - x - 2y:

V=04 ⁣ ⁣0(4x)/2 ⁣ ⁣04x2ydzdydx=04(4x)24dx=163.V = \int_0^4\!\!\int_0^{(4-x)/2}\!\!\int_0^{4-x-2y} dz\,dy\,dx = \int_0^4 \frac{(4-x)^2}{4}\,dx = \frac{16}{3}.

Quick check: the plane has intercepts 4,2,44, 2, 4, and the coordinate-plane tetrahedron of intercepts a,b,ca, b, c has volume abc6=4246=163\tfrac{abc}{6} = \tfrac{4\cdot 2\cdot 4}{6} = \tfrac{16}{3}. ✓

PR2 · cylindrical · under a paraboloid

Shape · circular shadow + axis symmetry ⇒ cylindrical; dV = r dr dθ dz

PR2. Find the volume of the solid under z=9x2y2z = 9 - x^2 - y^2 and above z=0z = 0.

Shadow. The paraboloid meets z=0z = 0 where x2+y2=9x^2 + y^2 = 9, the disk r3r \le 3. Slice. zz from 00 to 9r29 - r^2; keep the rr:

V=02π ⁣ ⁣03 ⁣ ⁣09r2rdzdrdθ=2π03r(9r2)dr=2π[9r22r44]03=2π814=81π2.V = \int_0^{2\pi}\!\!\int_0^{3}\!\!\int_0^{9-r^2} r\,dz\,dr\,d\theta = 2\pi\int_0^3 r(9 - r^2)\,dr = 2\pi\Big[\tfrac{9r^2}{2} - \tfrac{r^4}{4}\Big]_0^3 = 2\pi\cdot\frac{81}{4} = \frac{81\pi}{2}.

PR3 · spherical · a spherical cap inside a cone

Shape · sphere + cone from the origin ⇒ spherical; dV = ρ² sin φ dρ dφ dθ

PR3. Find the volume of the solid inside the sphere ρ=2\rho = 2 and above the cone ϕπ4\phi \le \tfrac{\pi}{4}.

Limits. 0ρ20 \le \rho \le 2, 0ϕπ40 \le \phi \le \tfrac{\pi}{4}, 0θ2π0 \le \theta \le 2\pi:

V=02π ⁣ ⁣0π/4 ⁣ ⁣02ρ2sinϕdρdϕdθ=2π(1cosπ4)83=8π(22)34.907.V = \int_0^{2\pi}\!\!\int_0^{\pi/4}\!\!\int_0^{2}\rho^2\sin\phi\,d\rho\,d\phi\,d\theta = 2\pi\cdot\Big(1 - \cos\tfrac{\pi}{4}\Big)\cdot\frac{8}{3} = \frac{8\pi\,(2 - \sqrt2)}{3} \approx 4.907.

The ϕ\phi-integral 0π/4sinϕdϕ=122\int_0^{\pi/4}\sin\phi\,d\phi = 1 - \tfrac{\sqrt2}{2} is where the 2\sqrt2 enters — and where the sinϕ\sin\phi earns its keep.

PR4 · decision-only · name the system

Shape · no integration — choose the system and say why in one line

PR4. For each, name the coordinate system and a one-line reason — do not integrate. (a) (x2+y2)dV\iiint (x^2+y^2)\,dV over a finite cylinder; (b) dV\iiint dV over the region between two concentric spheres; (c) fdV\iiint f\,dV over a rectangular brick.

(a) Cylindrical. The integrand x2+y2=r2x^2 + y^2 = r^2 and the circular cross-section both point at rdrdθdzr\,dr\,d\theta\,dz.

(b) Spherical. Both boundaries are "ρ=\rho = constant," so the ρ\rho-limits are just the inner and outer radii — spherical turns the shell into a rectangle.

(c) Cartesian. Six flat faces at right angles ⇒ six constant limits. Anything fancier only drags in roots.

PR5 · faded bridge · cylindrical mass

Shape · cylinder + density ⇒ cylindrical; mass = ∭ δ dV

PR5. Find the mass of the cylinder r1r \le 1, 0z20 \le z \le 2 with density δ=z\delta = z (denser toward the top).

Bridge: mass is TδdV\iiint_T \delta\,dV with δ=z\delta = z and dV=rdrdθdzdV = r\,dr\,d\theta\,dz, so the integrand is zrz\,r. Before revealing, predict the next step: what are the three limits, and which factor is the Jacobian you must keep?

Set up. 0r10 \le r \le 1, 0θ2π0 \le \theta \le 2\pi, 0z20 \le z \le 2; integrand zz, element rdrdθdzr\,dr\,d\theta\,dz:

m=02π ⁣ ⁣01 ⁣ ⁣02zrdzdrdθ=2π1201rdr202zdz=2π.m = \int_0^{2\pi}\!\!\int_0^{1}\!\!\int_0^{2} z\,r\,dz\,dr\,d\theta = 2\pi\cdot\underbrace{\tfrac12}_{\int_0^1 r\,dr}\cdot \underbrace{2}_{\int_0^2 z\,dz} = 2\pi.

The rr here is the Jacobian, not part of the density — keep both straight: density is zz, the rr comes from dVdV.

PR6 · spherical mass

Shape · half-ball + radial density ⇒ spherical; mass = ∭ δ dV

PR6. Find the mass of the upper half-ball z0z \ge 0, ρ1\rho \le 1 with density δ=ρ\delta = \rho (proportional to distance from the centre).

Set up. Half-ball ⇒ ϕ\phi from 00 to π2\tfrac{\pi}{2}. Integrand δ=ρ\delta = \rho times element ρ2sinϕ\rho^2\sin\phi gives ρ3sinϕ\rho^3\sin\phi:

m=02π ⁣ ⁣0π/2 ⁣ ⁣01ρ3sinϕdρdϕdθ=2π10π/2sinϕdϕ1401ρ3dρ=π2.m = \int_0^{2\pi}\!\!\int_0^{\pi/2}\!\!\int_0^{1}\rho^3\sin\phi\,d\rho\,d\phi\,d\theta = 2\pi\cdot\underbrace{1}_{\int_0^{\pi/2}\sin\phi\,d\phi}\cdot \underbrace{\tfrac14}_{\int_0^1\rho^3\,d\rho} = \frac{\pi}{2}.

PR7 · faded bridge · a second moment

Shape · z² over the ball ⇒ spherical; z = ρ cos φ

PR7. Evaluate Bz2dV\displaystyle\iiint_B z^2\,dV over the unit ball ρ1\rho \le 1.

Bridge: in spherical, z=ρcosϕz = \rho\cos\phi, so z2=ρ2cos2ϕz^2 = \rho^2\cos^2\phi; times the element ρ2sinϕ\rho^2\sin\phi the integrand is ρ4cos2ϕsinϕ\rho^4\cos^2\phi\sin\phi. Before revealing, predict the next step: what is 0πcos2ϕsinϕdϕ\int_0^{\pi}\cos^2\phi\sin\phi\,d\phi?

The ϕ\phi-integral is a u=cosϕu = \cos\phi substitution: 0πcos2ϕsinϕdϕ=[cos3ϕ3]0π=13+13=23\int_0^{\pi}\cos^2\phi\sin\phi\,d\phi = \big[-\tfrac{\cos^3\phi}{3}\big]_0^{\pi} = \tfrac13 + \tfrac13 = \tfrac23. Then

Bz2dV=02π ⁣ ⁣0π ⁣ ⁣01ρ4cos2ϕsinϕdρdϕdθ=2π2315=4π15.\iiint_B z^2\,dV = \int_0^{2\pi}\!\!\int_0^{\pi}\!\!\int_0^{1}\rho^4\cos^2\phi\sin\phi\,d\rho\,d\phi\,d\theta = 2\pi\cdot\frac23\cdot\frac15 = \frac{4\pi}{15}.
Pre-flight checklist — run it before you integrate
1. Sketch drawn? Shadow and slice identified, limits read off them?\textbf{1.}\ \text{Sketch drawn? Shadow and slice identified, limits read off them?} 2. Outer limits constant? Each inner limit depends only on variables further out?\textbf{2.}\ \text{Outer limits constant? Each inner limit depends only on variables further out?} 3. Cylindrical: is the r present in dV=rdrdθdz?\textbf{3.}\ \text{Cylindrical: is the } r \text{ present in } dV = r\,dr\,d\theta\,dz? 4. Spherical: is the sinϕ present in dV=ρ2sinϕdρdϕdθ?\textbf{4.}\ \text{Spherical: is the } \sin\phi \text{ present in } dV = \rho^2\sin\phi\,d\rho\,d\phi\,d\theta? 5. Did the coordinate system match the solid’s symmetry — or did you fight it?\textbf{5.}\ \text{Did the coordinate system match the solid's symmetry — or did you fight it?}

Three things to carry out of this chapter

  1. The ritual is shadow then slice. Project the solid to a flat shadow for the outer limits, slice from floor to roof for the inner limit. Nobody pictures the whole solid; everybody projects and slices.
  2. The coordinate system is a decision, and it is the skill. Origin-radial → spherical; an axis with circular cross-sections → cylindrical; flat right-angled faces → Cartesian. Match the symmetry to the surface that becomes a constant.
  3. Never drop the Jacobian. dV=rdrdθdzdV = r\,dr\,d\theta\,dz (cylindrical) and dV=ρ2sinϕdρdϕdθdV = \rho^2\sin\phi\,d\rho\,d\phi\,d\theta (spherical). The dropped rr and the dropped sinϕ\sin\phi are the marks the chapter is engineered to make you stop losing.
The anchor, one more time

Back to the CT scanner. Reconstructing a body's total mass from its density is exactly TδdV\iiint_T \delta\,dV — and a real scanner does it in whichever coordinates make the patient simplest, slice by slice. You have just learned the three systems it chooses between, and the one habit (keep the Jacobian) that separates a right answer from a plausible wrong one. Re-do PR5 and PR7 from a blank page tomorrow — not re-read, re-do. Keeping the rr and the sinϕ\sin\phi is muscle memory, built with the pencil.

What's next. Chapter 13 leaves volumes behind for line integrals — adding up a force along a path — and Green's theorem, which trades a boundary walk for an area integral. The "total something over a region" idea continues; the region just becomes a curve and the area it encloses.

Same material, another voice

If a different explanation would help, these map one-to-one onto this chapter — free, from MIT OpenCourseWare: