AP Physics 1  ·  Unit 2: Forces & Translational Dynamics  ·  Lesson 2.9

Deep Dive: Circular Motion

🔬 Deep Dive
The unit finale — everything you have learned about forces converges here.
2.9.A.1Concept

Why Circular Motion Is Accelerated Motion

Acceleration means any change in velocity — and velocity is a vector, so it changes if either its size or its direction changes. An object moving in a circle at a perfectly constant speed is still accelerating, because its direction is changing every instant. This is the single idea that unlocks the whole topic.

centerrv (tangent)a_cVelocity is always tangent to the circle.Acceleration always points toward the center — perpendicular to v.

At every point, the velocity vector is tangent to the circle (it points in the direction of motion). Because that direction is continuously turning, the velocity is continuously changing — so there must be an acceleration, and therefore a net force, causing it.

🔑Constant speed does not mean constant velocity. In uniform circular motion, speed is constant but velocity is not — the direction changes constantly, which is why there is acceleration.
2.9.A.2ConceptMath

Centripetal Acceleration

The acceleration in circular motion always points toward the center of the circle — perpendicular to the velocity. We call it centripetal acceleration ("center-seeking"). Its magnitude is:

a_c = v² / r

where v is the object's speed and r is the radius of the circular path. Notice speed is squared: doubling the speed makes the centripetal acceleration four times larger, while doubling the radius only halves it.

ExampleWorked Example — Car Rounding a Curve

A car travels at 20 m/s around a curve of radius 50 m. Find its centripetal acceleration.

2.9.A.3ConceptMath

Centripetal Force

By Newton's Second Law, an acceleration toward the center requires a net force toward the center. Combining ΣF = ma with a_c = v²/r gives the centripetal force equation:

ΣF_c = m·v² / r

This is not a new force. "Centripetal force" is just the name for the net inward force — whatever real force happens to point toward the center. It is the left side of Newton's Second Law applied to the radial direction.

Watch velocity (green) stay tangent and centripetal force (amber) always point inward. Change speed, radius, and mass — notice speed matters most because it enters the formula as v².

Speed (v)8 m/s
Radius (r)5 m
Mass (m)2 kg
a_c = v²/r
12.80 m/s²
F_c = mv²/r
25.6 N
T = 2πr/v
3.93 s
f = 1/T
0.255 Hz

Try doubling speed — force quadruples. Then double radius — force only halves. Speed dominates because it's squared.

⚠️Never add a separate "centripetal force" to a free-body diagram. The centripetal force is always provided by a real force already on your diagram — tension, gravity, normal force, or friction. Drawing it as an extra arrow double-counts the force.
2.9.A.4Concept

What Provides the Centripetal Force

In every circular-motion problem, your first job is to ask: which real force is pointing toward the center? That force (or the net of several) is what equals mv²/r.

Ball on a string
Tension
Car on a flat curve
Static friction
Satellite in orbit
Gravity
Loop-the-loop (top)
Gravity + Normal force
ExampleGuided Example — Ball on a String

A 0.5 kg ball is whirled in a horizontal circle of radius 1.2 m at 6 m/s. Find the tension in the string (ignore gravity for the horizontal case).

Step 1Identify the centripetal source
The only inward force is the string tension, so T = ΣF_c = mv²/r.
2.9.A.5Concept⚠ Watch Out

Vertical Loops & Minimum Speed

In a vertical circle — a roller-coaster loop, a bucket of water swung overhead — gravity is always down, but "toward the center" changes direction as you go around. At the very top, both gravity and the normal force point downward, toward the center, so they add together:

F_N + mg = m·v² / r

The minimum speed at the top happens when the track can barely touch the object — the normal force drops to zero (F_N = 0). Then gravity alone provides the centripetal force:

v_min = √(g·r)
ExampleWorked Example — Minimum Speed at the Top of a Loop

A roller coaster loop has a radius of 8 m. What is the minimum speed a cart needs at the top to maintain contact with the track? Use g = 10 m/s².

⚠️Centrifugal force is not real in an inertial frame. The outward "push" you feel on a loop or a turn is your own inertia trying to carry you in a straight line while a real inward force bends your path. Never place a centrifugal force on a free-body diagram.
2.9.B.1ConceptMath

Period, Frequency & Circular Orbits

The period T is the time for one complete lap. Since the object covers the circumference 2πr in one period at speed v:

T = 2πr / v

Frequency f is the number of laps per second, and it is simply the reciprocal of the period: f = 1/T (measured in hertz).

f = 1 / T

A circular orbit is the ultimate example: a satellite is in constant free fall, and gravity is the centripetal force that keeps it curving around the Earth. Setting gravity equal to mv²/r is how you find orbital speeds — a direct bridge to later gravitation topics.

🔑The circular-motion toolkit: (1) speed is constant but velocity is not, (2) acceleration points to the center with a_c = v²/r, (3) the net inward force is mv²/r and is provided by a real force, (4) at the top of a loop v_min = √(gr), and (5) T = 2πr/v with f = 1/T. This lesson pulls together free-body diagrams, Newton's laws, gravity, and friction — the whole unit at once.
ExampleGuided Example — Orbital Speed and Period

A satellite orbits Earth at a radius of 8.0 × 10⁶ m where g ≈ 6.2 m/s² at that altitude. Find its orbital speed and period.

Step 1Set gravity equal to centripetal force
For a circular orbit, gravity provides all the centripetal force: mg = mv²/r. The satellite's mass cancels from both sides → g = v²/r → v = √(gr)
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