An object's orbital period is the time it takes to complete one full trip around the body it orbits.
An object's orbital period is the time it takes to complete one full trip around the body it orbits. Kepler's Third Law connects that period to the size of the orbit (semi-major axis) and the mass being orbited.
The Moon orbits Earth (M = 5.97×10²⁴ kg) at a = 3.84×10⁸ m. T = 2π√((3.84×10⁸)³ / (6.674×10⁻¹¹ × 5.97×10²⁴)) ≈ 2,373,000 s ≈ 27.5 days — matching the Moon's real orbital period.
Using Kepler's Third Law relating period squared to the semi-major axis cubed.
No — for small orbiting bodies, it depends almost entirely on distance and the central body's mass.
They're much farther away, and period increases with distance per Kepler's law.