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🎯⭐ INTERACTIVE LESSON

Center of Mass

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Center of Mass - Complete Interactive Lesson

Part 1: COM Definition (Discrete)

Center of Mass — Definition (Discrete Systems)

Part 1 of 7

The center of mass (COM) is the mass-weighted average position of a system. For a collection of NN discrete particles:

r⃗cm=∑i=1Nmir⃗i∑i=1Nmi=1M∑i=1Nmir⃗i\vec{r}_{\text{cm}} = \frac{\sum_{i=1}^{N} m_i \vec{r}_i}{\sum_{i=1}^{N} m_i} = \frac{1}{M}\sum_{i=1}^{N} m_i \vec{r}_i

In component form:

xcm=∑mixiM,ycm=∑miyiM,zcm=∑miziMx_{\text{cm}} = \frac{\sum m_i x_i}{M}, \quad y_{\text{cm}} = \frac{\sum m_i y_i}{M}, \quad z_{\text{cm}} = \frac{\sum m_i z_i}{M}

where M=∑miM = \sum m_i is the total mass.

Key Properties

  • The COM is a unique point for any mass distribution
  • It does not need to lie within the physical body (e.g., a ring)
  • For a uniform-density symmetric object, COM lies at the geometric center

Two-Dimensional Systems

For particles in the xyxy-plane, compute each component separately.

Worked Example

Three masses:

  • m1=2m_1 = 2 kg at (0,0)(0, 0)
  • m2=3m_2 = 3 kg at (4,0)(4, 0)
  • m3=5m_3 = 5 kg at (2,3)(2, 3)

Solution:

xcm=2(0)+3(4)+5(2)2+3+5=0+12+1010=2.2 mx_{\text{cm}} = \frac{2(0) + 3(4) + 5(2)}{2+3+5} = \frac{0+12+10}{10} = 2.2 \text{ m}

ycm=2(0)+3(0)+5(3)10=1510=1.5 my_{\text{cm}} = \frac{2(0) + 3(0) + 5(3)}{10} = \frac{15}{10} = 1.5 \text{ m}

So r⃗cm=(2.2,1.5)\vec{r}_{\text{cm}} = (2.2, 1.5) m.

Using Symmetry

If a mass distribution has a line of symmetry, the COM lies on that line. If it has two perpendicular lines of symmetry, the COM is at their intersection.

Negative Mass Trick

To find the COM of an object with a hole, treat it as:

r⃗cm=Mfullr⃗full−Mholer⃗holeMfull−Mhole\vec{r}_{\text{cm}} = \frac{M_{\text{full}}\vec{r}_{\text{full}} - M_{\text{hole}}\vec{r}_{\text{hole}}}{M_{\text{full}} - M_{\text{hole}}}

This is equivalent to adding a "negative mass" at the hole's position.

Example: Disk with Off-Center Hole

A uniform disk of mass MM and radius RR has a circular hole of radius R/2R/2 cut from it, centered at x=R/2x = R/2 from the disk center.

Let σ\sigma be surface mass density. Mfull=σπR2M_{\text{full}} = \sigma \pi R^2, Mhole=σπ(R/2)2=M/4M_{\text{hole}} = \sigma \pi (R/2)^2 = M/4.

xcm=M(0)−(M/4)(R/2)M−M/4=−MR/83M/4=−R6x_{\text{cm}} = \frac{M(0) - (M/4)(R/2)}{M - M/4} = \frac{-MR/8}{3M/4} = -\frac{R}{6}

The COM shifts away from the hole.

Summary

ConceptFormula
COM (1D)xcm=∑mixiMx_{\text{cm}} = \frac{\sum m_i x_i}{M}
COM (vector)r⃗cm=∑mir⃗iM\vec{r}_{\text{cm}} = \frac{\sum m_i \vec{r}_i}{M}
SymmetryCOM lies on axes of symmetry
Negative mass trickSubtract hole contribution

Next: Part 2 — Center of mass for continuous mass distributions using integration.

Part 2: COM (Continuous Bodies)

Center of Mass — Continuous Bodies via Integration

Part 2 of 7

For a continuous mass distribution, sums become integrals:

r⃗cm=1M∫r⃗ dm\vec{r}_{\text{cm}} = \frac{1}{M}\int \vec{r}\,dm

The key is expressing dmdm in terms of geometry:

GeometryMass element
1D (rod, wire)dm=λ(x) dxdm = \lambda(x)\,dx
2D (plate, disk)dm=σ(x,y) dAdm = \sigma(x,y)\,dA
3D (solid)dm=ρ(x,y,z) dVdm = \rho(x,y,z)\,dV

where λ\lambda, σ\sigma, ρ\rho are linear, surface, and volume mass densities.

Non-Uniform Density

Worked Example: Rod with λ(x)=αx\lambda(x) = \alpha x

A rod extends from x=0x = 0 to x=Lx = L with linear density λ(x)=αx\lambda(x) = \alpha x.

Step 1: Find total mass

M=∫0Lαx dx=αL22M = \int_0^L \alpha x\,dx = \alpha \frac{L^2}{2}

Step 2: Find xcmx_{\text{cm}}

xcm=1M∫0Lx⋅αx dx=1αL2/2⋅αL33=2L3x_{\text{cm}} = \frac{1}{M}\int_0^L x \cdot \alpha x\,dx = \frac{1}{\alpha L^2/2}\cdot \alpha \frac{L^3}{3} = \frac{2L}{3}

The COM is shifted toward the denser (heavier) end, which makes physical sense.

Two-Dimensional Bodies

Semicircular Wire (Uniform)

A uniform semicircular wire of radius RR and mass MM lies in the upper half-plane.

By symmetry, xcm=0x_{\text{cm}} = 0. For ycmy_{\text{cm}}, parameterize with angle θ\theta:

dm=λR dθ,y=Rsin⁡θdm = \lambda R\,d\theta, \quad y = R\sin\theta

ycm=1M∫0πRsin⁡θ⋅λR dθ=λR2M[−cos⁡θ]0π=λR2⋅2λπR=2Rπy_{\text{cm}} = \frac{1}{M}\int_0^{\pi} R\sin\theta \cdot \lambda R\,d\theta = \frac{\lambda R^2}{M}[-\cos\theta]_0^{\pi} = \frac{\lambda R^2 \cdot 2}{\lambda \pi R} = \frac{2R}{\pi}

Semicircular Disk (Uniform)

For a solid semicircular disk, use area element dA=r dr dθdA = r\,dr\,d\theta:

ycm=1M∫0π∫0R(rsin⁡θ)σ⋅r dr dθ=4R3πy_{\text{cm}} = \frac{1}{M}\int_0^{\pi}\int_0^R (r\sin\theta)\sigma \cdot r\,dr\,d\theta = \frac{4R}{3\pi}

Shapeycmy_{\text{cm}}
Semicircular wire2R/π2R/\pi
Semicircular disk4R/(3π)4R/(3\pi)
Hemisphere shellR/2R/2
Solid hemisphere3R/83R/8

Summary

MethodExpression
Generalr⃗cm=1M∫r⃗ dm\vec{r}_{\text{cm}} = \frac{1}{M}\int \vec{r}\,dm
1D rodxcm=∫x λ(x) dx∫λ(x) dxx_{\text{cm}} = \frac{\int x\,\lambda(x)\,dx}{\int \lambda(x)\,dx}
2D plateUse dm=σ dAdm = \sigma\,dA with appropriate coordinates
Key resultsSemicircle wire 2R/π2R/\pi; hemisphere 3R/83R/8

Next: Part 3 — COM velocity and momentum.

Part 3: COM Velocity & Momentum

COM Velocity and Momentum

Part 3 of 7

Differentiating the COM position gives the COM velocity:

v⃗cm=dr⃗cmdt=1M∑imiv⃗i=p⃗totalM\vec{v}_{\text{cm}} = \frac{d\vec{r}_{\text{cm}}}{dt} = \frac{1}{M}\sum_{i} m_i \vec{v}_i = \frac{\vec{p}_{\text{total}}}{M}

Therefore the total momentum of the system equals:

p⃗total=Mv⃗cm\vec{p}_{\text{total}} = M\vec{v}_{\text{cm}}

This is a profound result: the total momentum of a system is the same as if all the mass were concentrated at the COM moving with v⃗cm\vec{v}_{\text{cm}}.

COM Acceleration

a⃗cm=dv⃗cmdt=1M∑mia⃗i=F⃗extM\vec{a}_{\text{cm}} = \frac{d\vec{v}_{\text{cm}}}{dt} = \frac{1}{M}\sum m_i \vec{a}_i = \frac{\vec{F}_{\text{ext}}}{M}

Internal forces cancel in pairs (Newton's third law), so only external forces determine COM motion.

Explosions and Internal Forces

When a body explodes or breaks apart, no external forces act during the explosion. Therefore:

v⃗cm, before=v⃗cm, after\vec{v}_{\text{cm, before}} = \vec{v}_{\text{cm, after}}

Worked Example

A 10 kg projectile moving at 2020 m/s horizontally explodes into two pieces. A 4 kg piece comes to rest. Find the velocity of the 6 kg piece.

Solution:

pbefore=10×20=200 kg⋅m/sp_{\text{before}} = 10 \times 20 = 200 \text{ kg}\cdot\text{m/s}

pafter=4(0)+6v2=200p_{\text{after}} = 4(0) + 6v_2 = 200

v2=2006=1003≈33.3 m/sv_2 = \frac{200}{6} = \frac{100}{3} \approx 33.3 \text{ m/s}

The COM continues at vcm=20v_{\text{cm}} = 20 m/s throughout.

Recoil Problems

A classic application: a person standing on a frictionless surface throws an object.

Worked Example

A 60 kg person on a frictionless frozen lake throws a 5 kg ball at 1010 m/s (relative to ground). Both start at rest.

0=60vp+5(10)  ⟹  vp=−5060=−56≈−0.83 m/s0 = 60 v_p + 5(10) \implies v_p = -\frac{50}{60} = -\frac{5}{6} \approx -0.83 \text{ m/s}

The person recoils in the opposite direction.

Continuous Mass Loss

If mass is ejected continuously (foreshadowing rockets), the momentum equation becomes differential:

dp⃗=v⃗ dmd\vec{p} = \vec{v}\,dm

This leads to the variable-mass equation we'll study in Topic 8.

Summary

ConceptKey Equation
COM velocityv⃗cm=∑miv⃗iM\vec{v}_{\text{cm}} = \frac{\sum m_i \vec{v}_i}{M}
Total momentump⃗total=Mv⃗cm\vec{p}_{\text{total}} = M\vec{v}_{\text{cm}}
No external forcesv⃗cm=const\vec{v}_{\text{cm}} = \text{const}
ExplosionsCOM velocity unchanged
Recoil∑p⃗i=0\sum \vec{p}_i = 0 if starting from rest

Next: Part 4 — The center of mass reference frame.

Part 4: COM Reference Frame

COM Reference Frame

Part 4 of 7

The center-of-mass frame (also called the zero-momentum frame) is the reference frame in which the total momentum is zero:

p⃗total ′=∑miv⃗i ′=0\vec{p}_{\text{total}}^{\,\prime} = \sum m_i \vec{v}_i^{\,\prime} = 0

To transform from the lab frame to the COM frame, subtract v⃗cm\vec{v}_{\text{cm}}:

v⃗i ′=v⃗i−v⃗cm\vec{v}_i^{\,\prime} = \vec{v}_i - \vec{v}_{\text{cm}}

Why Use the COM Frame?

  • Total momentum is always zero — simplifies collision analysis
  • Kinetic energy splits into COM motion + internal motion
  • Elastic collisions are symmetric in the COM frame

Kinetic Energy Decomposition

The total KE in the lab frame separates as:

Ktotal=12Mvcm2⏟Kcm+∑12mivi′2⏟KintK_{\text{total}} = \underbrace{\frac{1}{2}M v_{\text{cm}}^2}_{K_{\text{cm}}} + \underbrace{\sum \frac{1}{2}m_i v_i'^2}_{K_{\text{int}}}

where vi′=∣v⃗i−v⃗cm∣v_i' = |\vec{v}_i - \vec{v}_{\text{cm}}|.

Interpretation

  • KcmK_{\text{cm}}: energy of the system's bulk motion
  • KintK_{\text{int}}: energy of internal (relative) motion
  • In a perfectly inelastic collision, Kint→0K_{\text{int}} \to 0 (all internal KE is lost)

Worked Example

A 2 kg ball at 66 m/s collides with a 4 kg ball at rest.

vcm=2(6)+4(0)6=2 m/sv_{\text{cm}} = \frac{2(6) + 4(0)}{6} = 2 \text{ m/s}

Kcm=12(6)(2)2=12 JK_{\text{cm}} = \frac{1}{2}(6)(2)^2 = 12 \text{ J}

Kint=12(2)(6−2)2+12(4)(0−2)2=16+8=24 JK_{\text{int}} = \frac{1}{2}(2)(6-2)^2 + \frac{1}{2}(4)(0-2)^2 = 16 + 8 = 24 \text{ J}

Ktotal=12+24=36 J=12(2)(6)2✓K_{\text{total}} = 12 + 24 = 36 \text{ J} = \frac{1}{2}(2)(6)^2 \checkmark

Elastic Collisions in the COM Frame

In the COM frame, an elastic collision is beautifully simple: each particle reverses its velocity.

v1′after=−v1′before,v2′after=−v2′beforev_1'^{\text{after}} = -v_1'^{\text{before}}, \quad v_2'^{\text{after}} = -v_2'^{\text{before}}

Transforming back to the lab frame:

v1after=v1′after+vcm=−v1′+vcmv_1^{\text{after}} = v_1'^{\text{after}} + v_{\text{cm}} = -v_1' + v_{\text{cm}}

This gives the familiar results:

v1after=m1−m2m1+m2v1+2m2m1+m2v2v_1^{\text{after}} = \frac{m_1 - m_2}{m_1 + m_2}v_1 + \frac{2m_2}{m_1+m_2}v_2

v2after=2m1m1+m2v1+m2−m1m1+m2v2v_2^{\text{after}} = \frac{2m_1}{m_1+m_2}v_1 + \frac{m_2 - m_1}{m_1+m_2}v_2

Summary

ConceptKey Result
COM frame transformv⃗i′=v⃗i−v⃗cm\vec{v}_i' = \vec{v}_i - \vec{v}_{\text{cm}}
Zero momentum∑miv⃗i′=0\sum m_i \vec{v}_i' = 0 always
KE decompositionK=Kcm+KintK = K_{\text{cm}} + K_{\text{int}}
Elastic (COM frame)Velocities reverse
Perfectly inelasticAll KintK_{\text{int}} is lost
Reduced massμ=m1m2/(m1+m2)\mu = m_1 m_2/(m_1+m_2)

Next: Part 5 — COM motion under external forces.

Part 5: COM Under External Forces

COM Motion Under External Forces

Part 5 of 7

Newton's second law for the center of mass:

F⃗ext=Ma⃗cm=Mdv⃗cmdt=dp⃗totaldt\vec{F}_{\text{ext}} = M\vec{a}_{\text{cm}} = M\frac{d\vec{v}_{\text{cm}}}{dt} = \frac{d\vec{p}_{\text{total}}}{dt}

This is the most powerful consequence of the COM concept:

No matter how complex the internal interactions, the COM moves as if it were a single point particle of mass MM subject to the net external force.

Applications

  • A wrench tossed in the air: the COM follows a parabola even though the wrench rotates
  • A firework in flight: the COM continues on the parabolic trajectory after explosion
  • A binary star system: the COM follows the gravitational trajectory of the total mass

Projectile Breakup

Worked Example

A projectile is launched at 45°45° with speed v0v_0. At the top of its trajectory, it breaks into two equal pieces. One piece falls straight down. Where does the other piece land?

Solution:

Step 1: Range of intact projectile: R=v02sin⁡(90°)/g=v02/gR = v_0^2 \sin(90°)/g = v_0^2/g

Step 2: At the peak, the projectile is at x=R/2x = R/2, y=R/4y = R/4, with velocity (v0/2,0)(v_0/\sqrt{2}, 0).

Step 3: The COM must continue the original parabolic path and land at x=Rx = R.

Step 4: Piece 1 (m/2m/2) falls straight down from x=R/2x = R/2. By COM condition at landing time:

R=(m/2)(R/2)+(m/2)(x2)mR = \frac{(m/2)(R/2) + (m/2)(x_2)}{m}

x2=2R−R/2=3R2=3v022gx_2 = 2R - R/2 = \frac{3R}{2} = \frac{3v_0^2}{2g}

The second piece lands at 3R/23R/2 from the launch point — 50% farther than the original range.

COM of an Atwood Machine

Consider an Atwood machine with masses m1>m2m_1 > m_2, connected by a massless string over a frictionless pulley.

The acceleration: a=(m1−m2)gm1+m2a = \frac{(m_1 - m_2)g}{m_1 + m_2}

COM acceleration: Mass m1m_1 accelerates down, m2m_2 accelerates up, both with magnitude aa.

acm=m1a↓+m2a↑m1+m2=m1(−a)+m2(a)m1+m2a_{\text{cm}} = \frac{m_1 a_{\downarrow} + m_2 a_{\uparrow}}{m_1 + m_2} = \frac{m_1(-a) + m_2(a)}{m_1+m_2}

Wait — actually m1m_1 goes down (−a-a) and m2m_2 goes up (+a+a)... but the net external force is (m1−m2)g(m_1 - m_2)g downward while the string/pulley system is internal.

acm=(m1−m2)g−0m1+m2a_{\text{cm}} = \frac{(m_1 - m_2)g - 0}{m_1 + m_2}

Actually: the constraint forces (tension, normal from pulley) contribute externally via the pulley support. The COM accelerates downward at:

acm=(m1−m2)2g(m1+m2)2a_{\text{cm}} = \frac{(m_1 - m_2)^2 g}{(m_1+m_2)^2}

Summary

ScenarioCOM Behavior
Only gravitya⃗cm=g⃗\vec{a}_{\text{cm}} = \vec{g} (parabolic path)
No external forcesv⃗cm=const\vec{v}_{\text{cm}} = \text{const}
Breakup/explosionCOM continues original trajectory
Person on boatCOM stays fixed; boat shifts

Next: Part 6 — Problem-solving workshop.

Part 6: Problem-Solving Workshop

Center of Mass — Problem-Solving Workshop

Part 6 of 7

Strategy Guide

StepAction
1Identify the system and all masses
2Choose coordinates (use symmetry!)
3Determine if the problem is discrete or continuous
4For F⃗ext=0\vec{F}_{\text{ext}} = 0: use v⃗cm=const\vec{v}_{\text{cm}} = \text{const}
5For integration: choose dmdm wisely (λdx\lambda dx, σdA\sigma dA, ρdV\rho dV)
6Check: does the COM position make physical sense?

Problem 1: Two-Dimensional Integration

Find the COM of a quarter-disk of radius RR and uniform surface density σ\sigma in the first quadrant.

Solution:

By symmetry, xcm=ycmx_{\text{cm}} = y_{\text{cm}}.

M=σ⋅πR24M = \sigma \cdot \frac{\pi R^2}{4}

Using polar coordinates with x=rcos⁡θx = r\cos\theta:

xcm=σM∫0π/2∫0R(rcos⁡θ) r dr dθx_{\text{cm}} = \frac{\sigma}{M}\int_0^{\pi/2}\int_0^R (r\cos\theta)\,r\,dr\,d\theta

=σM⋅R33⋅[sin⁡θ]0π/2=σR3/3σπR2/4=4R3π= \frac{\sigma}{M} \cdot \frac{R^3}{3} \cdot [\sin\theta]_0^{\pi/2} = \frac{\sigma R^3/3}{\sigma \pi R^2/4} = \frac{4R}{3\pi}

r⃗cm=(4R3π,4R3π)\vec{r}_{\text{cm}} = \left(\frac{4R}{3\pi}, \frac{4R}{3\pi}\right)

Problem 2: Collision + COM

A 3 kg block moving at 44 m/s to the right collides elastically with a 1 kg block at rest.

In the COM frame:

vcm=3(4)+1(0)4=3 m/sv_{\text{cm}} = \frac{3(4) + 1(0)}{4} = 3 \text{ m/s}

COM frame velocities:

  • v1′=4−3=1v_1' = 4 - 3 = 1 m/s (right)
  • v2′=0−3=−3v_2' = 0 - 3 = -3 m/s (left)

Check: 3(1)+1(−3)=03(1) + 1(-3) = 0 ✓

After elastic collision (reverse in COM frame):

  • v1′after=−1v_1'^{\text{after}} = -1 m/s
  • v2′after=+3v_2'^{\text{after}} = +3 m/s

Back to lab frame:

  • v1after=−1+3=2v_1^{\text{after}} = -1 + 3 = 2 m/s
  • v2after=3+3=6v_2^{\text{after}} = 3 + 3 = 6 m/s

Verify: 3(2)+1(6)=12=3(4)+1(0)3(2) + 1(6) = 12 = 3(4) + 1(0) ✓ and KE is conserved ✓

Workshop Takeaways

Problem TypeKey Technique
Non-uniform rodxcm=∫xλ(x)dx∫λ(x)dxx_{\text{cm}} = \frac{\int x\lambda(x)dx}{\int \lambda(x)dx}
2D shapesUse polar coords for circular regions
CollisionsTransform to COM frame, reverse, transform back
Missing pieceNegative-mass subtraction
Solids of revolutionUse disk/shell slicing

Next: Part 7 — Comprehensive review & applications.

Part 7: Review & Applications

Center of Mass — Review & Applications

Part 7 of 7 — Comprehensive Assessment

Formula Reference

FormulaExpression
Discrete COMr⃗cm=∑mir⃗iM\vec{r}_{\text{cm}} = \frac{\sum m_i \vec{r}_i}{M}
Continuous COMr⃗cm=1M∫r⃗ dm\vec{r}_{\text{cm}} = \frac{1}{M}\int \vec{r}\,dm
COM velocityv⃗cm=p⃗totalM\vec{v}_{\text{cm}} = \frac{\vec{p}_{\text{total}}}{M}
Newton's 2nd (system)F⃗ext=Ma⃗cm\vec{F}_{\text{ext}} = M\vec{a}_{\text{cm}}
KE decompositionK=12Mvcm2+KintK = \frac{1}{2}Mv_{\text{cm}}^2 + K_{\text{int}}
Reduced massμ=m1m2m1+m2\mu = \frac{m_1 m_2}{m_1+m_2}

Key COM Positions

ShapeCOM
Uniform rodL/2L/2 from end
Solid coneh/4h/4 from base
Semicircle wire2R/π2R/\pi from center
Solid hemisphere3R/83R/8 from base

AP-Style Free Response

A uniform solid disk of mass MM and radius RR has a hole of radius R/3R/3 drilled through it. The hole is centered at distance R/3R/3 from the disk's center. Find the COM of the remaining piece.

Solution:

Let the disk center be at the origin and the hole center at x=R/3x = R/3.

Area of full disk: πR2\pi R^2. Area of hole: π(R/3)2=πR2/9\pi(R/3)^2 = \pi R^2/9.

Mass of full disk: Mfull=M⋅πR2πR2−πR2/9=M⋅98M_{\text{full}} = M \cdot \frac{\pi R^2}{\pi R^2 - \pi R^2/9} = M \cdot \frac{9}{8}

Mass of hole: Mhole=M8⋅98M_{\text{hole}} = \frac{M}{8} \cdot \frac{9}{8}... Let me redo this more carefully.

Let σ=M/(πR2−πR2/9)=M/(8πR2/9)=9M/(8πR2)\sigma = M/(\pi R^2 - \pi R^2/9) = M/(8\pi R^2/9) = 9M/(8\pi R^2)

Mfull=σπR2=9M/8M_{\text{full}} = \sigma \pi R^2 = 9M/8

Mhole=σπR2/9=M/8M_{\text{hole}} = \sigma \pi R^2/9 = M/8

xcm=Mfull(0)−Mhole(R/3)Mfull−Mhole=−(M/8)(R/3)9M/8−M/8=−MR/24M=−R24x_{\text{cm}} = \frac{M_{\text{full}}(0) - M_{\text{hole}}(R/3)}{M_{\text{full}} - M_{\text{hole}}} = \frac{-(M/8)(R/3)}{9M/8 - M/8} = \frac{-MR/24}{M} = -\frac{R}{24}

The COM shifts R/24R/24 away from the hole.

🎉 Topic Complete — Center of Mass

You've mastered:

PartTopicStatus
1Discrete COM definition✅
2Continuous bodies (integration)✅
3COM velocity & momentum✅
4COM reference frame✅
5COM motion under external forces✅
6Problem-solving workshop✅
7Review & applications✅

Key Insight: The center of mass reduces complex multi-body problems to single-particle dynamics. Master the COM frame and you'll cut through collision and explosion problems with ease.