Mechanics of particles and systems Orbital mechanics Concept
Kepler orbit
Summary
A Kepler orbit is the path of a body that moves under the inverse-square gravity of a single point mass and feels no other force. It is a conic section with the attracting centre at a focus: an ellipse, a parabola or a hyperbola. In the degenerate case it is a radial line. It is the exact solution of the two-body problem and the starting point of all orbit calculations. See the definition.
Where this leads
23 pages build on this one.
- Orbital perturbation
- Gravity assist
- Tests of general relativity
- Hohmann transfer orbit
- Transit light curve
- Equation of time
- Lense–Thirring precession
- Bi-elliptic transfer
- Planetary migration
- Poynting–Robertson effect
- Osculating orbit
- Orbital resonance
- Clohessy–Wiltshire equations
- Shakura–Sunyaev alpha disk model
- Lambert's problem
- Roche limit
- Orbital elements
- Vis-viva equation
- Patched conic approximation
- Perihelion precession of Mercury
- Tidal locking
- Roche lobe
- Yarkovsky effect
Further reading
About this page
| Tag | BXFSBB8Q46 |
|---|---|
| URI | m2://BXFSBB8Q46 |
| Kind | concept |
| Writing | W0 stub |
| MSC | 70F05, 70F15 |
| Same as | |
| Changed | 3 November 2026 |
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Used by
- Orbital perturbation
- Gravity assist
- Transit light curve
- Equation of time
- Lense–Thirring precession
- Bi-elliptic transfer
- Planetary migration
- Poynting–Robertson effect
- Osculating orbit
- Orbital resonance
- Clohessy–Wiltshire equations
- Shakura–Sunyaev alpha disk model
- Lambert's problem
- Roche limit
- Orbital elements
- Vis-viva equation
- Patched conic approximation
- Perihelion precession of Mercury
- Tidal locking
- Roche lobe
- Yarkovsky effect