Equations · equation
Kepler's Third Law
Celestial Mechanics · 1619
- Equation
- T² = 4π²a³ / GM
- Field
- Celestial Mechanics
- Named After
- Johannes Kepler
- Symbols
- T orbital period · a semi-major axis of the orbit · G gravitational constant · M mass of the central body
- Year
- 1619
Significance
Orbital period squared scales with orbit size cubed — the harmony that let Newton reverse-engineer the inverse-square law, and how we weigh stars, planets, and black holes today.
Referenced by
constant
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instrument
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