Science / kepler

Kepler's Third Law

🛰️ Orbital mechanics
Kepler's Third Law
PIA12235 - The Moon, orbiting on Kepler's schedule for 4.5 billion years. NASA.

Question

Is there a pattern in how long orbits take?

Johannes Kepler noticed in 1609 that the planets' orbital periods are not random: the square of the period equals a constant times the cube of the average distance (T² proportional to a³). The astonishing part is that it applies to EVERYTHING - the planets, the Moon, the ISS, your phone's GPS satellites. The same rule, no matter what is orbiting.

The math

T²/a³ = 4π²/(GM). Check it: the Moon takes 423.5 times longer to orbit than the ISS (27.3 days vs 92.9 minutes), so it must orbit 423.5 to the power 2/3 = 56.4 times farther out: 6,791 km × 56.4 = 383,000 km - the Moon's actual distance (384,400 km). From timing alone.

Why it matters

You can weigh the Earth without ever touching it: measure the Moon's orbit and GM falls out of the equation. That is how we know Earth's mass to five significant figures - pure arithmetic on a clock and a distance.

Sources

  1. Wikipedia - Kepler's laws of planetary motion [1]