Linked from

The 75 pages that link to Kepler's laws of planetary motion, each with the reason it gives.

• Radial velocity methodNarrower topic: The method’s orbital interpretation relies on the same period, shape, and distance relations.

• Orbital periodNarrower topic: The period relation belongs to this broader description of orbital motion.

• Milankovitch cyclesNarrower topic: They provide the orbital geometry underlying eccentricity and seasonal timing.

• Hohmann transfer orbitNarrower topic: They provide the orbital framework for estimating transfer time and motion.

• Lunar librationNarrower topic: The Moon’s variable orbital speed follows the same orbital geometry that drives longitudinal libration.

• Orbital rendezvousNarrower topic: They explain why an object in a lower orbit can catch one in a higher orbit.

• Tidal accelerationNarrower topic: They describe orbital motion at a given moment, while tidal acceleration changes the orbit over time.

• Circular orbitNarrower topic: Circular motion is a special case of the orbital patterns these laws describe.

• Sidereal yearNarrower topic: They provide the framework for understanding Earth’s orbital period.

• Exoplanet detectionNarrower topic: They connect a planet’s measured period to the scale and shape of its orbit.

• Space rendezvousNarrower topic: They explain why spacecraft in different orbits move at different speeds and return to positions predictably.

• Kepler's equationNarrower topic: Kepler's equation is the computational form of the timing problem behind the area law.

• Kepler's second lawNarrower topic: The equal-area rule is the second of the three laws.

• Gliese 581dNarrower topic: These orbital rules connect the proposed signal’s period to Gliese 581d’s inferred orbit.