Gravitational Field Strength (Cambridge (CIE) IGCSE Physics)

Revision Note

Lindsay Gilmour

Written by: Lindsay Gilmour

Reviewed by: Caroline Carroll

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Gravitational field strength of a planet

Gravitational field strength and mass

  • The relationship between gravitational field strength and mass is:

The greater the mass of a planet, the greater the strength of the gravitational field at its surface

  • The value of g (gravitational field strength) varies from planet to planet depending on their mass and radius

Gravitational field strength of bodies in the Solar System

Gravitational field strength diagram, downloadable IGCSE & GCSE Physics revision notes

The strength of the gravitational field at the surface of a planet depends on its mass and radius

Gravitational field strength and distance

  • The relationship between gravitational field strength and distance is:

As the distance from a planet increases, the strength of the gravitational field decreases

  • At the surface of a planet, the value of g (gravitational field strength) is constant, but it decreases with distance from the planet

Examiner Tips and Tricks

You do not need to remember the value of g on different planets for your exam, and the value of g for Earth is given on the front page of the exam paper.

Gravitational attraction of the Sun

  • Orbital motion is a result of the gravitational force of attraction acting between two bodies

  • This gravitational force

    • always acts towards the centre of the larger body

    • causes the orbiting body to move in a circular path

  • The Sun contains most of the mass (>99%) of the Solar System

  • Therefore, for objects orbiting around the Sun

    • the Sun's gravitational attraction keeps them in orbit

    • the force is directed from the orbiting object to the centre of the Sun

Orbital motion of the Earth around the Sun

6-1-5-motion-in-an-orbit

The Sun's gravitational force of attraction keeps the Earth in orbit around the Sun

Orbital motion of planets

Extended tier only

  • As the distance from the Sun increases:

    • the Sun's gravitational field strength decreases

    • the orbital speed of a planet decreases

  • For an object to maintain a circular orbit, it must have a centripetal force

    • For planets orbiting the Sun, this force is the Sun's gravitational attraction

  • Therefore, the centripetal force on a planet depends on

    • the strength of the Sun's gravitational field

    • the distance of the planet from the Sun

  • The further away a planet is from the Sun, the weaker the strength of the Sun's gravitational attraction and the weaker the centripetal force

  • The centripetal force on a planet is proportional to its orbital speed

  • Therefore, the further a planet is from the Sun:

    • the smaller its orbital speed

    • the longer its orbital period

Orbital speed and distance

Orbit of planets around the Sun, downloadable IGCSE & GCSE Physics revision notes

The closest planets to the Sun have the fastest orbital speeds, and the furthest have the slowest

  • This trend in orbital speed and distance can be seen in the data of the planets in the Solar System:

Orbital radius, speed and period data

Planet

Orbital radius (million km)

Orbital speed (km/s)

Orbital period (days or years)

Mercury

57.9

47.9

88 days

Venus

108.2

35.0

225 days

Earth

149.6

29.8

365 days

Mars

227.9

24.1

687 days

Jupiter

778.6

13.1

11.9 years

Saturn

1433.5

9.7

29.5 years

Uranus

2872.5

6.8

 75 years

Neptune

4495.1

5.4

165 years

Examiner Tips and Tricks

Be careful with your wording in this topic when talking about gravity. It is important to refer to the force of gravity as 'gravitational attraction', ' strength of the Sun's gravitational field' or 'the force due to gravity'. Avoid terms such as 'the Sun's gravity' or even more vague, 'the force from the Sun'. 

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Lindsay Gilmour

Author: Lindsay Gilmour

Expertise: Physics

Lindsay graduated with First Class Honours from the University of Greenwich and earned her Science Communication MSc at Imperial College London. Now with many years’ experience as a Head of Physics and Examiner for A Level and IGCSE Physics (and Biology!), her love of communicating, educating and Physics has brought her to Save My Exams where she hopes to help as many students as possible on their next steps.

Caroline Carroll

Author: Caroline Carroll

Expertise: Physics Subject Lead

Caroline graduated from the University of Nottingham with a degree in Chemistry and Molecular Physics. She spent several years working as an Industrial Chemist in the automotive industry before retraining to teach. Caroline has over 12 years of experience teaching GCSE and A-level chemistry and physics. She is passionate about creating high-quality resources to help students achieve their full potential.