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โž—Calculus II Unit 2 Review

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2.6 Moments and Centers of Mass

2.6 Moments and Centers of Mass

Written by the Fiveable Content Team โ€ข Last updated August 2025
Written by the Fiveable Content Team โ€ข Last updated August 2025
โž—Calculus II
Unit & Topic Study Guides

Moments and Centers of Mass

The center of mass is the single point where you could balance an object perfectly. Calculating it requires integrating mass distributions across a shape, and it connects integration techniques you've already learned to real physical problems like balance, rotation, and structural design.

In Calc II, you'll mostly work with one-dimensional distributions (rods, wires) and two-dimensional regions (thin plates). Symmetry often cuts the work in half, and Pappus's theorem gives you a clever shortcut for volumes of revolution.

Center of Mass for Linear Distributions

The center of mass is the point where an object's total mass can be thought of as concentrated. For a system of discrete particles along a line, you find it with a weighted average:

xห‰=โˆ‘i=1nmixiโˆ‘i=1nmi\bar{x} = \frac{\sum_{i=1}^{n} m_i x_i}{\sum_{i=1}^{n} m_i}

Here mim_i is the mass of particle ii and xix_i is its position. The numerator is called the first moment of the system. The denominator is the total mass.

For continuous objects like a rod or wire, mass isn't concentrated at points. Instead, you describe it with a linear density function ฮป(x)\lambda(x), which gives mass per unit length at position xx. A rod with varying thickness, for instance, has higher ฮป(x)\lambda(x) where it's thicker.

The continuous version of the center of mass formula is:

xห‰=โˆซabxโ€‰ฮป(x)โ€‰dxโˆซabฮป(x)โ€‰dx\bar{x} = \frac{\int_a^b x \, \lambda(x) \, dx}{\int_a^b \lambda(x) \, dx}

  • The denominator โˆซabฮป(x)โ€‰dx\int_a^b \lambda(x) \, dx gives the total mass MM.
  • The numerator โˆซabxโ€‰ฮป(x)โ€‰dx\int_a^b x \, \lambda(x) \, dx gives the moment about the origin M0M_0, which measures how the mass is distributed relative to x=0x = 0.

Example: Suppose a rod extends from x=0x = 0 to x=4x = 4 with linear density ฮป(x)=3x\lambda(x) = 3x. The total mass is โˆซ043xโ€‰dx=24\int_0^4 3x \, dx = 24. The moment is โˆซ04xโ‹…3xโ€‰dx=โˆซ043x2โ€‰dx=64\int_0^4 x \cdot 3x \, dx = \int_0^4 3x^2 \, dx = 64. So xห‰=6424=83โ‰ˆ2.67\bar{x} = \frac{64}{24} = \frac{8}{3} \approx 2.67. The center of mass is shifted toward the heavier end, which makes sense since the density increases with xx.

Center of mass for linear distributions, Calculating Centers of Mass and Moments of Inertia ยท Calculus

Center of Mass for Thin Plates

A thin plate (or lamina) is a flat, two-dimensional object with negligible thickness. Its mass distribution is described by a surface density (or area density) ฯƒ(x,y)\sigma(x, y), which gives mass per unit area.

The center of mass (xห‰,yห‰)(\bar{x}, \bar{y}) for a plate occupying region RR is:

xห‰=โˆฌRxโ€‰ฯƒ(x,y)โ€‰dAโˆฌRฯƒ(x,y)โ€‰dA,yห‰=โˆฌRyโ€‰ฯƒ(x,y)โ€‰dAโˆฌRฯƒ(x,y)โ€‰dA\bar{x} = \frac{\iint_R x \, \sigma(x, y) \, dA}{\iint_R \sigma(x, y) \, dA}, \qquad \bar{y} = \frac{\iint_R y \, \sigma(x, y) \, dA}{\iint_R \sigma(x, y) \, dA}

When the plate has constant (uniform) density, ฯƒ\sigma cancels out of the fraction, and the formulas simplify to:

xห‰=โˆฌRxโ€‰dAโˆฌRdA,yห‰=โˆฌRyโ€‰dAโˆฌRdA\bar{x} = \frac{\iint_R x \, dA}{\iint_R dA}, \qquad \bar{y} = \frac{\iint_R y \, dA}{\iint_R dA}

The denominator is just the area of RR. In this uniform case, the center of mass is called the centroid since it depends only on geometry, not mass.

In many Calc II problems, you won't set up full double integrals. Instead, for a region between curves f(x)f(x) and g(x)g(x) (where f(x)โ‰ฅg(x)f(x) \geq g(x)) from x=ax = a to x=bx = b with uniform density, you can use:

  • Total area: A=โˆซab[f(x)โˆ’g(x)]โ€‰dxA = \int_a^b [f(x) - g(x)] \, dx
  • Moment about the y-axis: My=โˆซabx[f(x)โˆ’g(x)]โ€‰dxM_y = \int_a^b x[f(x) - g(x)] \, dx
  • Moment about the x-axis: Mx=โˆซab12[f(x)2โˆ’g(x)2]โ€‰dxM_x = \int_a^b \frac{1}{2}[f(x)^2 - g(x)^2] \, dx

Then xห‰=My/A\bar{x} = M_y / A and yห‰=Mx/A\bar{y} = M_x / A. The MxM_x formula comes from the fact that the average height of a thin vertical strip between the two curves is 12[f(x)+g(x)]\frac{1}{2}[f(x) + g(x)].

Center of mass for linear distributions, Moments and Centers of Mass ยท Calculus

Symmetry in Centroid Location

Symmetry is your best friend for these problems because it can eliminate half the computation.

  • If a region is symmetric about the y-axis, then xห‰=0\bar{x} = 0.
  • If a region is symmetric about the x-axis, then yห‰=0\bar{y} = 0.
  • If a region is symmetric about both axes (or the origin), both coordinates are 0.

How to use symmetry in practice:

  1. Sketch the region and look for lines of symmetry.
  2. For each axis of symmetry, set the corresponding centroid coordinate to the value on that axis. (If symmetric about x=0x = 0, then xห‰=0\bar{x} = 0.)
  3. Only compute the integral for the remaining coordinate(s).

For example, the region between y=x2y = x^2 and y=1y = 1 is symmetric about the y-axis, so xห‰=0\bar{x} = 0 immediately. You only need to calculate yห‰\bar{y}.

Pappus's Theorem for Revolution Solids

Pappus's theorem provides an elegant connection between centroids and volumes of revolution: the volume of a solid formed by rotating a plane region about an external axis equals the area of the region times the distance its centroid travels.

V=2ฯ€dห‰โ‹…AV = 2\pi \bar{d} \cdot A

Here dห‰\bar{d} is the distance from the centroid to the axis of rotation, and AA is the area of the region. The quantity 2ฯ€dห‰2\pi \bar{d} is the circumference of the circle traced by the centroid.

Steps to apply Pappus's theorem:

  1. Identify the plane region and the axis of rotation. (The axis must not pass through the region.)
  2. Find the area AA of the region using geometry or integration.
  3. Find the centroid of the region, then determine dห‰\bar{d}, the perpendicular distance from the centroid to the axis of rotation.
  4. Compute V=2ฯ€dห‰โ‹…AV = 2\pi \bar{d} \cdot A.

Example: A semicircular region of radius rr has area A=12ฯ€r2A = \frac{1}{2}\pi r^2 and its centroid sits at distance dห‰=4r3ฯ€\bar{d} = \frac{4r}{3\pi} from the diameter. Rotating about the diameter gives:

V=2ฯ€โ‹…4r3ฯ€โ‹…12ฯ€r2=43ฯ€r3V = 2\pi \cdot \frac{4r}{3\pi} \cdot \frac{1}{2}\pi r^2 = \frac{4}{3}\pi r^3

That's the volume of a sphere, which confirms the theorem works.

Pappus's theorem also works in reverse: if you know the volume of a solid of revolution and the area of the generating region, you can solve for the centroid location.

Moments of Inertia (Second Moments)

While the center of mass uses first moments (โˆซxโ€‰dm\int x \, dm), moments of inertia use second moments (โˆซx2โ€‰dm\int x^2 \, dm). The moment of inertia measures how mass is distributed relative to an axis and determines an object's resistance to rotational acceleration.

  • Moment of inertia about the y-axis: Iy=โˆซabx2โ€‰ฮป(x)โ€‰dxI_y = \int_a^b x^2 \, \lambda(x) \, dx (for a linear distribution)
  • Moment of inertia about the x-axis: Ix=โˆฌRy2โ€‰ฯƒ(x,y)โ€‰dAI_x = \iint_R y^2 \, \sigma(x,y) \, dA (for a thin plate)

Moment of inertia is to rotation what mass is to linear motion. A larger moment of inertia means the object is harder to spin. This concept connects the integration techniques from this unit to rotational dynamics in physics, where torque, angular momentum, and rotational equilibrium all depend on how mass is distributed relative to an axis.

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