Lesson 6 of 195 minutes

Circular Motion and Gravitation

Start with the lesson question, connect the representations, and test the model with evidence.

circular motionradial accelerationcentripetal forcegravitationorbitsapparent weight

Learning objectives

  • Construct system and free-body diagrams.
  • Apply Newton's laws to connected and accelerated systems.
  • Design an investigation that tests a force model.
Lesson flowHook, model, explanationShow guidance

Inspect the opening phenomenon

Predict what changes, then name the evidence.

Apply in the lab

Name the evidence before reading the answer.

Read only what helps

Then use the lab and recall check.

More when needed

Transcript and resources stay available below.

Course progress

AP Physics 1 — Algebra-Based · Force and Translational Dynamics · Lesson 6

Circular Motion and Gravitation

In progress

Decision challenge

Observe the phenomenon. Then connect the representations.

Use the opening example to make a prediction, identify evidence, and explain which model supports it.

Constant Speed, Nonzero Acceleration | AP Physics 1

Predict the direction of acceleration for an object moving at constant speed around a circle.

Calculate speed and radial acceleration, then identify which real interaction supplies the inward net force.

Before

Predict the direction of acceleration for an object moving at constant speed around a circle.

During

Pause after radius and period appear and calculate the speed before the result is shown.

After

Name the real interaction that supplies the inward net force in one circular-motion example.

Reference drawerTranscript, source notes, scripts, and package status stay tucked away until you need them.7 files

Lesson reading

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5 min

Video script

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Transcript fallback

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courses/ap-physics-1/modules/02-force-and-translational-dynamics/lessons/02-circular-motion-and-gravitation/video-transcript.md

Test Radial Force Versus Speed

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1 hr 20 min

Mastery check

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7 questions / 15 min

Book section:courses/ap-physics-1/modules/02-force-and-translational-dynamics/lessons/02-circular-motion-and-gravitation/book-section.md
Transcript for accessibility and fallback

# Accessible transcript: Constant Speed, Nonzero Acceleration Constant speed does not mean zero acceleration. In uniform circular motion, the velocity arrow keeps turning, so acceleration points toward the center. At radius point eight meters and period two seconds, speed is two pi r over T: two point five one meters per second. Radial acceleration is v squared over r: seven point nine meters per second squared inward. Quick check: is centripetal force a new force to add? Pause. No. It is the inward net force supplied by real interactions like tension, friction, or gravity. Learn free at EduQuest AI. ## Visual description A marker travels around a circle with tangent velocity arrows and inward acceleration arrows. A numerical radius-and-period example calculates speed and radial acceleration, followed by real-force icons for tension, friction, and gravity.

Reading lab

Core explanation

Connect the lesson's words, diagrams, graphs, evidence, and equations.

Driving question

How can an object accelerate continuously while its speed remains constant, and what interaction keeps an orbit curved?

Before learning: direction prediction

A ball moves counterclockwise around a circle at constant speed. At the rightmost point, draw its velocity and acceleration vectors. Then list the actual forces that might produce the acceleration.

Hook: constant speed can still mean acceleration

In uniform circular motion, velocity changes direction every instant. Acceleration points toward the circle's center even when speed is constant.

Circular kinematics

For radius rr and speed vv,

ar=v2r=ω2r.a_r=\frac{v^2}{r}=\omega^2r.

With period TT,

v=2πrT,ar=4π2rT2.v=\frac{2\pi r}{T},\qquad a_r=\frac{4\pi^2r}{T^2}.

Velocity is tangent to the path; radial acceleration points inward and is perpendicular to velocity in uniform circular motion.

Velocity tangent and acceleration inward at four points on a circle

Worked example: rotating platform

A marker moves in a circle of radius 0.80 m0.80\text{ m} with period 2.0 s2.0\text{ s}:

v=2π(0.80)2.0=2.51 m/s,v=\frac{2\pi(0.80)}{2.0}=2.51\text{ m/s}, ar=v2r=7.90 m/s2.a_r=\frac{v^2}{r}=7.90\text{ m/s}^2.

“Centripetal force” is the inward net force

Newton's second law radially is

Fr=mv2r.\sum F_r=m\frac{v^2}{r}.

Do not add a new force labeled “centripetal” to a free-body diagram. Tension, gravity, friction, normal force, or a combination supplies the inward net force.

Free-body diagrams for a level turn and vertical-circle bottom

Level curve

For a car turning on a flat road without slipping, static friction points toward the center:

fs=mv2r.f_s=m\frac{v^2}{r}.

Since fsμsmgf_s\le\mu_smg, the ideal maximum speed is vmax=μsgrv_{max}=\sqrt{\mu_sgr}.

Vertical circle

At the bottom of a vertical circle, inward is upward:

FNmg=mv2r.F_N-mg=m\frac{v^2}{r}.

At the top, inward is downward. Radial signs must follow the local inward direction.

Universal gravitation

Two pointlike or spherically symmetric masses attract with magnitude

Fg=Gm1m2r2.F_g=G\frac{m_1m_2}{r^2}.

rr is center-to-center separation. The gravitational field due to mass MM is

g=GMr2.g=\frac{GM}{r^2}.

Inverse-square gravitational field at two radii

Doubling distance from the center reduces field magnitude to one-fourth.

Circular orbits

For a small satellite in a circular orbit around mass MM, gravity supplies radial net force:

GMmr2=mv2r.G\frac{Mm}{r^2}=m\frac{v^2}{r}.

Thus

v=GMr,T=2πr3GM.v=\sqrt{\frac{GM}{r}},\qquad T=2\pi\sqrt{\frac{r^3}{GM}}.

Satellite mass cancels. Higher circular orbits have lower speed but longer period.

Worked comparison

If orbital radius becomes four times larger around the same central mass, speed becomes one-half and period becomes 43/2=84^{3/2}=8 times larger.

Apparent weight and weightlessness

Scale reading is usually a normal force, not gravitational force. In orbit, astronauts and spacecraft are both freely falling; gravity is not zero. Their apparent weight is near zero because support force is near zero.

During learning: radial audit

  1. Mark the circle center and local inward direction.
  2. Draw only real external forces.
  3. Resolve the inward components and write Fr=mv2/r\sum F_r=mv^2/r.
  4. Keep tangential and radial equations separate.
  5. For gravity use center-to-center radius and state spherical/point-mass assumptions.

Misconception clinic

“Constant speed means no acceleration.” Direction change produces radial acceleration.

“Centripetal force is an extra force.” It names the inward net force requirement.

“Circular motion needs an outward force.” In an inertial frame, the net force is inward.

“Astronauts float because gravity is absent.” They float because spacecraft and occupants fall together.

“Higher orbit means faster satellite.” Higher circular orbit means lower speed and longer period.

After learning: retrieval and transfer

  1. How are velocity and acceleration oriented in uniform circular motion?
  2. What real force turns a car on a flat road?
  3. Why must center-to-center distance be used in gravitation?
  4. How do circular orbital speed and period change with radius?
  5. Why does an orbiting scale read nearly zero?

AP-style evidence routine

  1. Define object/system, center, radius, and instant.
  2. Draw a free-body diagram with real forces only.
  3. Choose inward-positive radial and tangential axes.
  4. Apply Newton's second law by direction.
  5. State gravity/orbit assumptions.
  6. Check dimensions, limits, directions, and physical contact constraints.

Key takeaway

Circular motion requires inward acceleration supplied by real interactions. Gravity can provide that inward net force, producing continuous free fall around a central body.

Further learning and alignment

Practice labTest Radial Force Versus SpeedOpen this when you are ready to apply the model, collect evidence, and check your explanation.1 hr 20 min

Lab: Test Radial Force Versus Speed

Objective

For fixed mass and radius, does inward force vary with speed squared as Fr=mv2/rF_r=mv^2/r?

Safety

Teacher supervision is required. Use a commercial centripetal-force apparatus or a securely enclosed horizontal rotating system. Wear eye protection if required, inspect all connections, keep the rotation zone clear, use low masses/speeds, and never rotate objects overhead or toward people. Stop for vibration, fraying, looseness, or unstable motion.

Materials

  • approved enclosed centripetal-force apparatus;
  • low-mass rotating object;
  • force sensor or calibrated spring;
  • radius scale;
  • timer/photogate/video;
  • protective boundary.

Low-cost alternative: use teacher-provided prerecorded data from a safe apparatus rather than an open hand-spun setup.

Simulation alternative: approved circular-motion simulation with exported raw data and stated idealizations.

Steps

  1. Inspect apparatus and obtain teacher approval.
  2. Measure rotating mass and radius with uncertainty.
  3. Keep mass and radius fixed.
  4. Collect at least six safe steady-speed conditions.
  5. Measure period over multiple revolutions and calculate v=2πr/Tv=2\pi r/T.
  6. Record inward force and repeat each condition three times.
  7. Preserve raw times, force readings, and anomalies.
  8. Plot FrF_r versus v2v^2.

Expected Result

FrF_r should be linear in v2v^2 with slope near m/rm/r and intercept consistent with zero within uncertainty.

Analysis

  • Fit slope/intercept and compare slope to measured m/rm/r.
  • Propagate or bound period, radius, mass, and force uncertainty.
  • Discuss sensor zero, drag, changing radius, nonhorizontal motion, bearing friction, and speed variation.
  • Distinguish inward net force from any one sensor reading if other radial forces act.

Reflection Questions

  1. Why plot force versus v2v^2 rather than vv?
  2. Which real force did the apparatus use inward?
  3. How would doubling radius at fixed speed affect required force?
  4. What evidence showed speed was steady?

Claim-evidence-reasoning conclusion

Claim whether evidence supports Frv2F_r\propto v^2. Cite fit, uncertainty, and residual pattern, then connect evidence to radial Newton's second law.

Accessibility

Offer safety, measurement, timing, data, graphing, uncertainty, and narration roles. Use high-contrast/tactile markers and screen-reader tables. Learners may analyze shared or simulated data without operating rotation equipment.

Extension Challenge

Use the fitted model to predict force at one new approved speed, test once, and compare within uncertainty.