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- Orbit_equation abstract "In astrodynamics an orbit equation defines the path of orbiting body around central body relative to , without specifying position as a function of time. Under standard assumptions, a body moving under the influence of a force, directed to a central body, with a magnitude inversely proportional to the square of the distance (such as gravity), has an orbit that is a conic section (i.e. circular orbit, elliptic orbit, parabolic trajectory, hyperbolic trajectory, or radial trajectory) with the central body located at one of the two foci, or the focus (Kepler's first law).If the conic section intersects the central body, then the actual trajectory can only be the part above the surface, but for that part the orbit equation and many related formulas still apply, as long as it is a freefall (situation of weightlessness).".
- Orbit_equation wikiPageID "997464".
- Orbit_equation wikiPageRevisionID "582813421".
- Orbit_equation hasPhotoCollection Orbit_equation.
- Orbit_equation subject Category:Orbits.
- Orbit_equation comment "In astrodynamics an orbit equation defines the path of orbiting body around central body relative to , without specifying position as a function of time. Under standard assumptions, a body moving under the influence of a force, directed to a central body, with a magnitude inversely proportional to the square of the distance (such as gravity), has an orbit that is a conic section (i.e.".
- Orbit_equation label "Equazione dell'orbita".
- Orbit_equation label "Orbit equation".
- Orbit_equation sameAs Equazione_dell'orbita.
- Orbit_equation sameAs m.03xw2_.
- Orbit_equation sameAs Q7100057.
- Orbit_equation sameAs Q7100057.
- Orbit_equation wasDerivedFrom Orbit_equation?oldid=582813421.
- Orbit_equation isPrimaryTopicOf Orbit_equation.