The orbital period is the time required to complete one orbit. It is related to mean motion by T=2π/n.
Ancestors (8)
- Mean motion
- Orbital element
- Kepler orbit
- Celestial mechanics
- Classical mechanics
- Branches of physics
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Incoming links (57)
- Accretion-disk stream-impact hot spot
- Cataclysmic-variable period bounce
- Comet energy diffusion
- Cross-sectional-area current
- Doppler spectroscopy
- Empty and full loss-cone capture rates
- Exoplanet
- Facing geometry of synchronous rotation
- Falling bodies and lunar motion as tests of gravity
- Gas-driven contraction of a planetesimal binary
- Gravitational mass degeneracy
- Isotropic stellar mass loss
- Kepler's laws of planetary motion
- Kepler's third law
- Light curve
- Lunar phase
- Methods of detecting exoplanets
- Nova-induced binary detachment
- Orbit averaging
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- Phase folding of a light curve
- Phase-mixed radial probability of a Kepler orbit
- Planet-stationary orbit
- Planet-synchronous orbit
- Poynting–Robertson decay of a circumplanetary orbit
- Sidereal month
- Spin-orbit resonance
- Stellar radial-velocity semi-amplitude
- Synchronous rotation
- Tidal locking
- Virial theorem on a Kepler ellipse
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