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The semi-major axis of the planet's orbit is equal to 4 AU.
Given the following data:
Kepler's third law of planetary motion states that the square of any planetary body's orbital period (T) is directly proportional to the cube of its orbit's semi-major axis (a).
Mathematically, Kepler's third law of planetary motion is given by this formula:
[tex]T^2 =a^3[/tex]
Where:
Substituting the given parameters into the formula, we have;
[tex]8^2 =a^3\\\\a^3=64\\\\a=\sqrt[3]{64}[/tex]
a = 4 AU.
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