Circular Motion & Gravitation — Practice · Grade 12 Science
Chapter: Forces, Rotation & EquilibriumWhat this practice covers
By the end of Circular Motion & Gravitation you should be able to:
- I can calculate centripetal acceleration (a = v²/r) and centripetal force (F = mv²/r) for uniform circular motion.
- I can apply Newton's law of universal gravitation (F = Gm₁m₂/r²) to find the gravitational force between two masses.
- I can explain how gravity supplies the centripetal force that holds a satellite in orbit.
10 questions, numeric, multiple choice and written answer, each with a worked explanation.
Vocabulary used: centripetal acceleration, centripetal force, period (T), Newton's law of universal gravitation, gravitational constant (G).
Problem 1
Answer and explanation
2 m/s²
a = v²/r = 10² ÷ 50 = 100 ÷ 50 = 2 m/s², directed toward the center of the curve.
Problem 2
Answer and explanation
18 N
F = mv²/r = 2 × 6² ÷ 4 = 2 × 36 ÷ 4 = 72 ÷ 4 = 18 N.
Problem 3
- Along the direction of motion (tangent to the circle)
- Outward, away from the center
- Toward the center of the circle
- There is no net force
Answer and explanation
Toward the center of the circle
Uniform circular motion requires a center-seeking (centripetal) net force. The outward feeling is an illusion of the accelerating frame.
Problem 4
- one-half as strong
- twice as strong
- unchanged
- one-quarter as strong
Answer and explanation
one-quarter as strong
Gravitation is an inverse-square law (F ∝ 1/r²). Doubling r multiplies the force by 1/2² = 1/4.
Problem 5
Answer and explanation
Even at constant speed the satellite's direction is always changing, and any change in velocity is acceleration — here it is centripetal acceleration pointing toward Earth's center. The force supplying it is gravity: Earth's gravitational pull provides exactly the mv²/r needed to bend the satellite's path into a circle, so it 'falls around' the planet.
Problem 6
Answer and explanation
6000 N
F = mv²/r = 1,200 × 20² ÷ 80 = 1,200 × 400 ÷ 80 = 1,200 × 5 = 6,000 N, directed toward the center of the curve.
Problem 7
Hints
Centripetal describes net inward force, not an additional mysterious interaction.
Answer and explanation
It quadruples force because F=mv²/r.
Problem 8
Hints
State what the supplied observations or conditions establish, and separate that from any assumption.
Answer and explanation
g=GM/r² decreases with distance from the center; doubling r gives one quarter the field.
Problem 9
Answer and explanation
r=2R, so g is one quarter of its surface value.
For ideal point masses or a spherical source outside its surface, Newtonian gravitation gives F=GMm/r² with center-to-center separation r. A satellite’s altitude h above a spherical Earth is not r; use r=R+h. Doubling center distance reduces force and gravitational acceleration to one quarter. The familiar near-surface g≈9.8 m/s² is an approximation over modest height differences, not the same value at every orbital distance.
r=2R, so g is one quarter of its surface value.
Response criteria
- Interpret labels, structures, axes, units and directions correctly.
- Explain the physical or environmental relationship or mechanism.
- Respect stated assumptions and distinguish observation from inference.
Problem 10
Answer and explanation
ac=16/2=8.0 m/s² and inward net force=0.50×8=4.0 N. Tension equals that net only if the specified geometry and other forces establish it as the sole inward contribution.
ac=16/2=8.0 m/s² and inward net force=0.50×8=4.0 N.
Tension equals that net only if the specified geometry and other forces establish it as the sole inward contribution.
Response criteria
- Use the stated measurements or conditions, with correct units.
- Connect the result to the physical or environmental mechanism or evidence relationship.
- Identify the assumption, model limit or further evidence requested.