CIE A Level Physics

Topic Questions

Syllabus Edition

First teaching 2020

Last exams 2024

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13.1 Universal Gravitation

1a2 marks

Planets create large gravitational fields. 

State what is meant by a gravitational field.

1b
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1 mark

The Earth has a larger gravitational field strength than the moon. 

State what is meant by gravitational field strength.

1c
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4 marks

Saturn has a gravitational field strength of 10.5 N kg–1 on its surface and a radius of 58 000 km. 

(i)
State the acceleration due to gravity of an object on Saturn.
[1]
(ii)
Calculate the mass of Saturn.
[3]
1d
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2 marks

Fig 1.1 represents Saturn as an isolated uniform sphere. 

Sketch the lines to represent the gravitational field outside the sphere.

13-1-1d-e-saturn-field-lines

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2a
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2 marks

State Newton's law of gravitation.

2b
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2 marks

Newton's law of gravitation assumes the masses are point masses. 

The planets in our Solar System and the Sun are not point masses. 

Explain why the law still applies to the planets in our Solar System.

2c
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1 mark

Explain why g is approximately constant for small changes in height near the Earth’s surface.

2d
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3 marks

The gravitational force between the Earth and the Sun is 3.52 × 1022 N.  

Calculate the radius of the Earth's orbit around the Sun. 

   Mass of Earth = 6.0 × 1024 kg

   Mass of Sun = 2.0 × 1030 kg

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3a
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3 marks

Explain what is meant by a geostationary orbit.

3b
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2 marks

A satellite of mass m is in a circular orbit around a planet of mass with linear speed v

Show that M is given by the expression:

            M space equals space fraction numerator v squared r space over denominator G end fraction

3c
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2 marks

Show that the mass M can also be written in terms of the time period of the satellite T as

            M space equals space fraction numerator 4 pi squared r cubed space over denominator T squared G end fraction

3d
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4 marks

Calculate the radius of a geostationary orbit around Earth. 

Mass of Earth = 6.0 × 1024 kg

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1a
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2 marks

Explain how the force(s) on a satellite can result in the satellite being in a circular orbit around a planet.

1b
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4 marks

The Earth and the Moon may be considered to be uniform spheres that are isolated in space. The Earth has mass M, radius R and mean density ρ. 

The Moon, mass m, is in a circular orbit about the Earth with radius nR, as illustrated in Fig. 1.1.

 

q1b-paper-4-specimen-2022-cie-ial-physics

Fig. 1.1

The Moon makes one complete orbit of the Earth in time T.

Show that the mean density ρ of the Earth is given by the expression

rho equals fraction numerator 3 pi n cubed over denominator G T squared end fraction

where G is the gravitational constant.

1c
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3 marks

The radius R of the Earth is 6.38 × 106 m and the distance between the centre of the Earth and the centre of the Moon is 3.84 × 108 m.

The period T of the orbit of the Moon about the Earth is 27.3 days.

Use the expression in (b) to calculate ρ.



ρ = ................................... kg m–3 

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2a
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2 marks

Mars may be considered to be a uniform sphere of radius 3400 km with its mass M concentrated at its centre. A stone of mass 3.67 kg rests on top of Olympus Mons, the largest volcano on Mars, which is 25 km high.

The gravitational force on the stone is 13.3 N.

Mars spins on its axis with a period of 1 day and 37 mins. 

Calculate M.

2b
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3 marks

Determine the force required to maintain the stone in its circular path.

2c
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2 marks

Derive the equation

         g space equals fraction numerator space G M over denominator r squared end fraction

where G is Newton's gravitational constant, is the mass and r is the distance from the mass for the gravitational field strength due to a point mass.

2d
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2 marks

Olympus Mons is an active volcano.

Calculate the acceleration due to gravity of the stone if it was thrown upwards to twice the height of Olympus Mons.
 
a = ..................................... m s–2

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3a
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5 marks

Explain 

(i)
What is meant by a geostationary orbit.                        
                                                [3] 
(ii)
Why it is preferable to have a satellite in this orbit for TV and telephone signals
                                           [2]
3b
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4 marks

A satellite of mass m is in orbit around a planet. 

The mass of the planet may be considered to be concentrated at its centre.

Show that the time period T of the orbit of the satellite is given by the expression

T squared space equals space open parentheses fraction numerator 4 pi squared R cubed over denominator G M end fraction close parentheses

 

where R is the radius of the orbit of the satellite and G is the gravitational constant. 

Explain your working.

3c
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2 marks

The radius of a geostationary orbit around Earth is 4.2 × 107 m.

 Calculate the mass of the Earth.

3d
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3 marks

The radius of the Earth is 6400 km.

Determine the ratio

fraction numerator gravitational space field space strength space of space satellite space on space the space Earth apostrophe straight s space surface over denominator gravitational space field space strength space of space the space satellite space at space the space geostationary space orbit end fraction

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