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Explain How Planets and Satellites Stay in Orbit

In this worksheet, students will explore the fact that the Earth orbits around the Sun, and what stops the Earth and the other planets from moving away from each other.

'Explain How Planets and Satellites Stay in Orbit' worksheet

Key stage:  KS 3

Year:  Year 9 Science worksheets

Curriculum topic:   Physics: Motion and Forces

Curriculum subtopic:   Forces

Popular topics:   Space worksheets, Physics worksheets

Difficulty level:  

Worksheet Overview

You may have seen the hammer throw in athletics events. When the athlete swirls their hammer, the cord between the athlete's hands and the hammer stop it from moving away from the athlete - until they let go of course! The hammer will then fly away in a straight line.

 

Hammer thrower

A hammer thrower in action

 

This is similar to how the Earth travels in orbit around the Sun, with one difference - there is no cord holding the Earth in orbit; instead, it is the force of gravity.

 

Gravity stops the Earth and all the other planets and moons from just drifting through space in a straight line. Essentially, it keeps them in orbit.

 

Solar system
The planets in orbit around the Sun

 

As can be seen in the diagram of the Solar System above, the planets closer to the Sun have a more curved orbit because the force of gravity from the Sun gets stronger the closer you get to it.

 

The force of gravity is also responsible for keeping the moon orbiting around the Earth. Without the Earth's gravity, the moon would just drift away into space.

 

Earth and moon
The Moon orbiting the Earth

 

The force of gravity can also keep our artificial satellites in orbit around the Earth without the need for power because gravity from the Earth holds them in position. Similar to how the planets orbit around the Sun, satellites that are closer to the Earth orbit faster and on a more curved path than those that are further from the Earth.

 

Satellite in orbit

A satellite orbiting the Earth 

 

Let's try some questions on this now.

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