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Proud to be part of LJMU,
in partnership with the Faulkes Telescope Project

 

Many years ago, a mathematician named Johannes Kepler created a set of rules explaining planets' movement in our Solar System. Thanks to later discoveries about gravity by Isaac Newton, we can now apply Kepler's Laws to determine properties of our Solar System, such as the mass of the Sun.

Use this activity to discover more about Kepler's 3 Laws of planetary motion and calculate the mass of the biggest object in our Solar System, the Sun.

By the end of this activity you will:

  • Know the fundamental principles of Kepler’s Laws.
  • Know the properties of an ellipse.
  • Be able to use Kepler’s 3rd Law to find the mass of the Sun.

To complete this resource you will need: 

IT Equipment

  • OPTIONAL - Spreadsheet software (e.g. MS Excel) - if you are new to spreadsheet software, use this MS Help Sheet
Files Needed
Worksheet (289.95 KB)
Answer sheet (632.36 KB)
The picture shows a cartoon portrait of Johannes Kepler in front of an artist's impression of the Solar System.
Credit The Schools' Observatory

 

Approx Duration
30 - 60 mins

 

Have a go

  1. Watch the 3 videos on Kepler’s Laws.
  2. Make notes as you watch the videos.
  3. Use the Planetary Data Sheet and Fact Sheet to complete the Worksheet (you can use graph paper to complete Task 1, or you can choose to use a spreadsheet application like MS Excel or Google Sheets)
  4. Use the Answer sheet to check your work