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Learning objective

Define orbital speed using the formula 2 r π v = T, where r represents the orbit's radius and T is the orbital period, and be able to recall and apply this equation.

Read the explanation, check the common trap, then practise with flashcards and questions.

Exam focus

  • Read the explanation.
  • Check key terms.
  • Practise with linked questions.
Cambridge IGCSE Combined ScienceSpace physicsSupplement contentPractical objective

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Quick explanation

Define orbital speed using the formula 2 r π v = T, where r represents the orbit's radius and T is the orbital period, and be able to recall and apply this equation

  • This point belongs to Stars and the Universe, especially Stars and the Universe outcomes.
  • You need to be able to define orbital speed using the formula 2 r π v = T, where r represents the orbit's radius and T is the orbital period, and be able to recall and apply this equation.
  • The key ideas to know are Define and Calculate.
  • Use the linked flashcards and practice questions to check recall, then practise applying the idea in an exam-style answer.

Key concepts

DefineCalculate

Why it matters

This objective helps connect Stars and the Universe outcomes to exam-style questions, flashcards, and revision notes for Stars and the Universe.

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Practice Questions7 linked questions

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Paper 6 structured question: Stars and the Universe

Paper 6Alternative to PracticalPractical1 marks

Method

Method for Measuring Orbital Speed

In this experiment, you will measure the time taken for a satellite to complete one orbit at different radii. Record the radius and the time taken for each orbit.

Radius (m)Time (s)
1060
20120
30180
  1. a

    State the independent variable in this experiment.

    Aim for approximately 1 distinct marking point.

    [1]
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