Thursday, August 20, 2026

Circular Motion and Gravitation UPCAT Reviewer: Lesson and Practice

TEACHER ABI UPCAT MATHEMATICS

Circular Motion and Gravitation

Identify inward force and tangential motion, calculate circular quantities, and reason about gravity, weight, satellites, and orbital changes.

5-10 minute lesson27 original questionsAdaptive practiceSaves progress
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Circular Motion and Gravitation

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Velocity is tangent; acceleration and net force are inward

An object moving in a circle continually changes velocity direction even when its speed is constant. The required acceleration points toward the center.

ac = rFc = mv²r

“Centripetal force” is not an extra kind of force. It is the name for the net inward force, which may be supplied by tension, friction, gravity, a normal force, or a combination.

Fgravity = Gm₁m₂weight = mg

Velocity is tangent

If the inward force disappears, the object initially follows the tangent.

Force is inward

Centrifugal force is not an additional outward force in an inertial-frame force diagram.

Speed has a squared effect

At fixed m and r, doubling v requires four times Fc.

Gravity follows an inverse square

Doubling center-to-center separation reduces force to one-fourth.

Orbit is continuous free fall

Tangential speed carries the satellite forward while gravity curves its path.

DO IT FAST

At any point, draw TANGENT and INWARD

TANGENT: Direction of instantaneous velocity.

INWARD: Direction of centripetal acceleration and net force.

Then identify which real force supplies the inward result. For comparisons, use proportional reasoning before substituting numbers.

Why it works

Most circular-motion mistakes come from pointing velocity inward, inventing an outward force, or ignoring the squared speed and inverse-square distance relationships.

WORKED EXAMPLES

Five forms you should recognize

1. Force and direction

Problem: A 2 kg object moves at 4 ms in a radius of 2 m.

Fc = 2(4²)÷2 = 16 N inward

Its velocity remains tangent to the circle.

2. String breaks

Problem: A stone travels in a circle and its string breaks.

Conclusion: Tension disappears, so the stone initially follows the tangent at the release point—not a radial line outward.

3. Gravitational comparison

Problem: Center-to-center distance doubles.

Fnew = Fold÷2² = Fold÷4
4. Mass versus weight

Problem: A 60 kg person stands where g = 1.6 m.

weight = 60(1.6) = 96 N

Mass remains 60 kg.

5. Satellite orbit

Problem: Why does a satellite not fall straight down?

It is falling under gravity, but its tangential speed carries it forward so the surface curves away as its path curves inward.

COMMON TRAPS

Check before you commit

  • Pointing circular velocity toward the center
  • Adding a separate centripetal force to the real inward forces
  • Assuming constant speed means zero acceleration
  • Measuring gravitational separation surface-to-surface
  • Changing mass when only location changes
  • Claiming gravity is absent in orbit
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Core Practice

Use mixed forms with less scaffolding.

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Apply the competency in unfamiliar representations.

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QUICK ANSWERS

Circular Motion and Gravitation FAQ

What supplies centripetal force?

It depends on the situation: tension, friction, gravity, a normal force, or a combination can provide the net inward force.

Why do astronauts feel weightless if gravity acts?

They and their spacecraft share free fall, so the supporting normal force is nearly absent.

Do heavier satellites orbit faster?

Not at the same circular-orbit radius around the same central body; satellite mass cancels from the orbital-speed relation.

RELATED COMPETENCIES

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