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Space Sciences
Orbital Mechanics
1619
Intermediate

Kepler's Third Law

T2=4π2GMa3T^2 = \frac{4\pi^2}{GM} a^3

Orbital period squared is proportional to semi-major axis cubed.

By Johannes Kepler

Space Sciences
Kepler's Third Law
1619 · Johannes Kepler
Human Reviewed
84%

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Why it matters: Enabled Newton to discover universal gravitation; foundation of spaceflight.

Discoverers: Johannes Kepler (1619)

What does it mean?

Orbital period squared is proportional to semi-major axis cubed.

Why should I care?

Enabled Newton to discover universal gravitation; foundation of spaceflight.

Equation Compass

Variables & Units

SymbolNameUnitMeaning
TTPeriodsOrbital period
aaSemi-major axismOrbit size
MMCentral masskgMass being orbited

Worked Example

Earth year from a = 1 AU and M = solar mass.

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Kepler's Third Law

T2=4π2GMa3T^2 = \frac{4\pi^2}{GM} a^3

Real-world impact

Satellite constellations

Elliptical orbits place Starlink, GPS, and Webb at precise altitudes.

Photo: Unsplash — satellite orbit

Orbital period squared is proportional to semi-major axis cubed.

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