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Physics worksheet featuring step-by-step examples of Kepler's Third Law applied to planets in our solar system and exoplanets.

Worksheet with Kepler's 3rd Law problems calculating orbital periods for Neptune, Mars, Venus, Pluto, and an exoplanet mass.

Worksheet with Kepler's 3rd Law problems calculating orbital periods for Neptune, Mars, Venus, Pluto, and an exoplanet mass.

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Show Answer Key & Explanations Step-by-step solution for: Worksheet – Keplers 3rd Law - Physics @ CSU Stanislaus
Final Answer:
a) 28650
b) 169 years

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Explanation:
We’re using Kepler’s Third Law, which says:
P² = a³,
where:
- P is the orbital period in Earth years,
- a is the average distance from the Sun in astronomical units (AU).

For Neptune:
- Given: a = 30.6 AU
- So, a³ = 30.6 × 30.6 × 30.6
Let’s compute step by step:
30.6 × 30.6 = 936.36
936.36 × 30.6 ≈ 28,650 (rounded — that’s a³)
So P² = 28,650
Then P = √28,650 ≈ 169 years.

That’s why:
a) P² = a³ = 30.6³ ≈ 28,650
b) P = √28,650 ≈ 169 years
Parent Tip: Review the logic above to help your child master the concept of kepler s third law worksheet.
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