WJEC A-Level Physics 1420QS
Basic Physics
Kinematics
Dynamics
Energy Concepts
Solids Under Stress
Using Radiation to Investigate Stars
Particles and Nuclear Structure
Conduction of Electricity
Resistance
D.C. Circuits
The Nature of Waves
Wave Properties
Refraction of Light
Photons
Lasers
Circular Motion
Vibrations
Kinetic Theory
Thermal Physics
Nuclear Decay
Nuclear Energy
Capacitance
Electrostatic and Gravitational Fields of Force
Orbits and the Wider Universe
Magnetic Fields
Electromagnetic Induction
Option A: Alternating CurrentsOption A
Option B: Medical PhysicsOption B
Option C: The Physics of SportsOption C
Option D: Energy and the EnvironmentOption D
Mathematical Requirements (Appendix C)
Orbits and the Wider Universe
Newton's law of gravitation applied to orbits
- 3 things to know
- A2 Unit 4 Section A
Overview
Recall questions on Newton's law of gravitation applied to orbits.
What you need to know
Answer each one before you reveal it.
Write the equation obtained by setting the gravitational force equal to the centripetal force for a circular orbit.
Give the equation relating the orbital period to the speed and the radius.
Questions from this subtopic
Each one with the model answer underneath.
- 1
What provides the centripetal force that holds a planet in orbit around the Sun?
Model answer
The gravitational attraction between the planet and the Sun.
- 2
Write the equation obtained by setting the gravitational force equal to the centripetal force for a circular orbit.
Model answer
GMm/r² = mv²/r, where M is the central mass, m the orbiting mass, v the orbital speed and r the orbital radius.
- 3
Rearrange that to give the orbital speed, and define every symbol.
Model answer
Cancelling m and one factor of r gives v = √(GM/r), where v is in m s⁻¹, G the gravitational constant, M the central mass in kilograms and r the orbital radius in metres.
- 4
Why does the mass of the orbiting body not affect its orbital speed?
Model answer
It appears on both sides of the equation and cancels, so every object at the same radius must travel at the same speed.
- 5
How does orbital speed change as the orbital radius increases?
Model answer
It falls in proportion to one over the square root of the radius, so a more distant planet moves more slowly.
- 6
Calculate the orbital speed of a satellite 7.2 × 10⁶ m from the Earth's centre, taking M as 6.0 × 10²⁴ kg.
Model answer
v = √(GM/r) = √(6.67 × 10⁻¹¹ × 6.0 × 10²⁴ ÷ 7.2 × 10⁶) = √(5.56 × 10⁷), which is 7.5 × 10³ m s⁻¹.
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