Orbital Eccentricity

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A measure of the shape of a celestial body's orbit, expressed as a unitless number.

Description (Specifications)[edit]

The orbital eccentricity of a planet is expressed as a number notated as e, standing for eccentricity.

  • A value of e=0 is a perfectly circular orbit.
  • A value of e=1 a parabolic orbit.
  • If e has a value of greater than one it represents a hyperbolic trajectory.

Worlds[edit]

Diagram of a world with an eccentric orbit around a star:

Diagram Elliptical Orbit Basic Plain.png

Stars[edit]

Diagrams of stars with eccentric orbits around a barycenter, a common center of mass:

Diagram Large Small Binary Stars Orbits 06.png

Diagram Binary Stars Orbits 01.png

History & Background (Dossier)[edit]

A perfectly circular orbit is indicated by an eccentricity of zero. Increasingly elliptical orbits have values between zero (0) and one (1). Parabolic orbits are indicated by a value of one, while values above 1 represent hyperbolic orbits, typically associated with celestial objects that are not bound to a star.

See the references below for further definition and application.

See also[edit]

Star systems

References & Contributors (Sources)[edit]

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