Question

as the distance from the sun gets greater, the orbital time takes
longer
it remains the same
shorter
rewatch

Explanation:

Step1: Kepler's Third Law

Kepler's third law states that \( T^2\propto r^3 \), where \( T \) is the orbital period and \( r \) is the distance from the sun.

Step2: Analyze the relationship

If \( r \) (distance from the sun) increases, then \( T \) (orbital time) must increase. For example, Mercury (close to the sun) has a short orbital period, while Neptune (far from the sun) has a long orbital period.

Answer:

longer