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AP Physics C: Mechanics · Framework 2026-27
Unit 2

Force and Translational Dynamics

Translational dynamics begins with a declared system and uses the external-force resultant to determine center-of-mass acceleration.

Exam weight
20–25%
Topics
10

Introduction

Translational dynamics begins with a declared system and uses the external-force resultant to determine center-of-mass acceleration.

A free-body diagram is an interaction ledger, not a picture of motion. Draw only forces exerted on the chosen system, identify their agents, and project those forces onto useful axes before writing Newton’s law.

The force models in this unit have conditions. Dry friction is piecewise, an ideal spring is linear only over a stated range, linear drag is a low-speed model, and inverse-square gravity relies on source geometry. State the model before solving its differential equation.

01
System boundary

separates internal interactions from external forces

02
Newton’s laws

connect interaction vectors to center-of-mass motion

03
Force models

supply gravitational, contact, spring, and drag terms

04
Radial dynamics

projects real forces toward a curved path’s center

Current exam guidance: Aligned to the current 2026–27 AP Physics C: Mechanics framework, with calculus-based modeling, derivations, experimental reasoning, and explicit assumptions.
2.1

Systems and Center of Mass

How can a many-particle system have one translational equation?

Short answer

A mass-weighted position defines the center of mass, and internal force pairs cancel when the particle equations are summed, leaving external force to govern its motion.

Know firstVector components · Definite integrals · Newton’s third-law pairs

The boundary decides which interactions survive

For discrete masses, r⃗cm=M−1∑imir⃗i\vec r_{cm}=M^{-1}\sum_i m_i\vec r_i; for a continuous body, replace the sum with M−1∫r⃗ dmM^{-1}\int\vec r\,dm. The center of mass is a weighted coordinate and need not lie inside material. A system may also change shape, separation, or internal energy while its center-of-mass motion stays simple.

For constant total mass, differentiating twice and summing particle equations gives Ma⃗cm=∑F⃗extM\vec a_{cm}=\sum\vec F_{ext}. Internal third-law pairs cancel in this whole-system sum, although they can rearrange constituents and transfer energy internally. Matter or energy crossing the boundary must be entered explicitly; mass flow requires momentum-flux accounting.

Physics model

The center of mass is a weighted position

Change one mass and see how the system center shifts while the coordinate origin stays fixed.

Left mass
2 kg at −3 m
Right mass
4 kg at +3 m
Center
1 m
left massvariable right masscenter of masscoordinate origin
The center of mass is a weighted positionChange one mass and see how the system center shifts while the coordinate origin stays fixed.center of massorigin
xcm=∑imixi∑imi=1M∫x dmx_{cm}=\frac{\sum_i m_i x_i}{\sum_i m_i}=\frac{1}{M}\int x\,dm
Read this figure without the graphic

Change one mass and see how the system center shifts while the coordinate origin stays fixed.

Current quantityValue
Left mass2 kg at −3 m
Right mass4 kg at +3 m
Center1 m
Model relationxcm=∑imixi∑imi=1M∫x dmx_{cm}=\frac{\sum_i m_i x_i}{\sum_i m_i}=\frac{1}{M}\int x\,dm

Locate a nonuniform rod’s center of mass

  1. Find total mass: M=∫0Lkx dx=kL2/2M=\int_0^Lkx\,dx=kL^2/2.
  2. Compute the first moment: ∫0Lx dm=∫0Lkx2 dx=kL3/3\int_0^Lx\,dm=\int_0^Lkx^2\,dx=kL^3/3.
  3. Divide first moment by total mass.
Result
xcm=2L3x_{cm}=\frac{2L}{3}
Units: The result is a length measured from the low-density end.

Boundary cases

  • A uniform rod would have xcm=L/2x_{cm}=L/2.
  • Changing the origin changes the coordinate but not the physical point.

Because density increases toward the right end, the center of mass lies at two thirds of the rod length.

Choose a center-of-mass model

SystemExpressionKey condition
point massesM−1∑mir⃗iM^{-1}\sum m_i\vec r_iall positions use one frame
continuous bodyM−1∫r⃗ dmM^{-1}\int\vec r\,dmdensity supplies dmdm
constant-mass motionMa⃗cm=∑F⃗extM\vec a_{cm}=\sum\vec F_{ext}no mass crosses boundary

Build the system equation

  1. Draw the boundary and list what crosses it.
  2. Compute total mass and weighted position.
  3. Classify every interaction as internal or external.
  4. Cancel internal pairs only after summing all constituent equations.
  5. Apply the result to center-of-mass motion, not automatically to each part.

Keep these three ideas

  • Center of mass is a mass-weighted coordinate.
  • Internal pairs cancel only in a whole-system sum.
  • External resultant controls constant-mass center-of-mass acceleration.

Keep reading Unit 2: Force and Translational Dynamics

You just read the first topic free. Your free trial opens the rest of this unit, every AP Physics C: Mechanics unit, and all 19 AP courses.

  • 2.1 Systems and Center of MassRead
  • 2.2 Forces and Free-Body Diagrams
  • 2.3 Newton’s Third Law
  • 2.4 Newton’s First Law
  • 2.5 Newton’s Second Law
  • 2.6 Gravitational Force
  • 2.7 Kinetic and Static Friction
  • 2.8 Spring Forces
  • 2.9 Resistive Forces
  • 2.10 Circular Motion
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