Syllabus Edition

First teaching 2023

First exams 2025

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Circular Orbits in Gravitational Fields (CIE A Level Physics)

Revision Note

Leander

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Leander

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Circular orbits in gravitational fields

  • For objects in a circular orbit in a gravitational field the gravitational force is related to the centripetal acceleration it causes
  • Planets travel around the Sun in orbits that are (approximately) circular and within the Sun's gravitational field
    • Objects in a circular orbit travel at a constant speed
  • The orbit is a circular path, therefore the direction in which the object is travelling will be constantly changing
    • A change in direction causes a change in velocity
  • Acceleration is the rate of change of velocity, therefore if an object is constantly changing direction then its velocity is constantly changing, so an object in orbit is accelerating
  • A resultant force is needed to cause an acceleration
  • This resultant centripetal force is due to the gravitational force FG created by the object being orbitted 
  • The resultant force must act at right angles to the instantaneous velocity of the object to create a circular orbit
    • This is always towards the centre of the orbit
    • The instantaneous velocity of the object is the velocity at a given time

Gravitational force and instantaneous velocity

Motion in an orbit, downloadable IGCSE & GCSE Physics revision notes

The direction of the instantaneous velocity and the gravitational force at different points of the Earth’s orbit around the sun

Worked example

A binary star system consists of two stars orbiting about a fixed point B. The star of mass M1 has a circular orbit of radius R1 and mass M2 has a radius of R2. Both have a linear speed v and an angular speed ⍵ about B.Worked example - circular orbits in g fields, downloadable AS & A Level Physics revision notes

State the following formula, in terms of G, M2, R1 and R2

(a) The angular speed ⍵ of M1

(b) The time period T for each star in terms of angular speed ⍵

Answer:

(a) 

Step 1: Equating the centripetal force of mass M1 to the gravitational force between M1 and M2

M subscript 1 R subscript 1 omega squared space equals space vertical line fraction numerator G M subscript 1 M subscript 2 over denominator open parentheses R subscript 1 plus space R subscript 2 close parentheses squared end fraction

Step 2: M1 cancels on both sides

R subscript 1 omega squared space equals fraction numerator space G M subscript 2 over denominator open parentheses R subscript 1 plus space R subscript 2 close parentheses squared end fraction

Step 3: Rearrange for angular velocity ⍵

omega squared space equals fraction numerator space G M subscript 2 over denominator R subscript 1 open parentheses R subscript 1 plus space R subscript 2 close parentheses squared end fraction

Step 4: Square root both sides

omega space equals space square root of fraction numerator G M subscript 2 over denominator R subscript 1 open parentheses R subscript 1 plus R subscript 2 close parentheses squared end fraction end root

(b) 

Step 1: Angular speed equation with time period T

omega space equals fraction numerator space 2 straight pi over denominator T end fraction

Step 2: Rearrange for T

T space equals fraction numerator space 2 straight pi over denominator straight omega end fraction

Step 3: Substitute in ⍵

T space equals space 2 straight pi space divided by space square root of fraction numerator G M subscript 2 over denominator R subscript 1 open parentheses R subscript 1 plus R subscript 2 close parentheses squared end fraction end root space equals space 2 straight pi space square root of fraction numerator straight R subscript 1 open parentheses straight R subscript 1 plus straight R subscript 2 close parentheses squared over denominator GM subscript 2 end fraction end root

Examiner Tip

Many of the calculations in the Gravitation questions depend on the equations for Circular motion. Be sure to revisit these and understand how to use them!

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Leander

Author: Leander

Expertise: Physics

Leander graduated with First-class honours in Science and Education from Sheffield Hallam University. She won the prestigious Lord Robert Winston Solomon Lipson Prize in recognition of her dedication to science and teaching excellence. After teaching and tutoring both science and maths students, Leander now brings this passion for helping young people reach their potential to her work at SME.