Linked from

The 35 pages that link to Kepler orbit, each with the reason it gives.

• Orbital eccentricityNarrower topic: Its conic-section paths are classified by eccentricity.

• Orbital elementsNarrower topic: Classical orbital elements describe this ideal two-body motion directly.

• Vis-viva equationNarrower topic: The vis-viva relation follows from this two-body orbital model.

• Orbit determinationNarrower topic: Its six classical elements provide a common coordinate system for describing estimated orbits.

• Oort cloudNarrower topic: Orbital mechanics connects a comet's measured path to the scale of its source region.

• Yarkovsky effectNarrower topic: The effect slowly modifies the orbital elements of an otherwise Keplerian path.

• Orbital perturbationNarrower topic: It is the unperturbed orbit against which deviations are measured.

• Specific orbital energyNarrower topic: Its conic shape and size are classified by specific orbital energy.

• Rings of SaturnNarrower topic: Each ring particle follows an orbit around Saturn, modified by nearby particles and moons.

• Orbital maneuverNarrower topic: It provides the baseline orbit that a maneuver changes.

• Poynting–Robertson effectNarrower topic: The effect slowly modifies the nearly Keplerian paths followed by circumstellar dust.

• Circular orbitNarrower topic: Circular orbits are one member of this broader family of gravitational paths.

• Lunar theoryNarrower topic: It supplies the baseline ellipse that lunar theory modifies.

• Polar orbitNarrower topic: Polar inclination is one orientation property within the broader Keplerian orbit description.

• Bi-elliptic transferNarrower topic: Each transfer arc is modeled as a Kepler orbit between impulsive burns.

• Interplanetary dust cloudNarrower topic: Dust particles follow near-Keplerian paths between significant perturbations.