Glossary of Orbital Mechanics Terms

Key terms used throughout this site. Links point to pages with more detailed treatment.

TermDefinition
AphelionThe point in an orbit farthest from the Sun. See First Law.
PerihelionThe point in an orbit closest to the Sun.
Apoapsis / PeriapsisGeneral terms for farthest/closest point in an orbit around any body (not just the Sun).
Angular momentumMeasure of rotational motion; conserved in orbital motion. See Angular Momentum.
Astronomical Unit (AU)The average Earth-Sun distance, about 149.6 million km.
Conic sectionA curve formed by slicing a cone: circle, ellipse, parabola, or hyperbola.
Eccentricity (e)A measure of how elongated an ellipse is. e=0 is a circle; 0<e<1 is an ellipse.
EllipseA closed oval curve with two foci. See Ellipse Geometry.
EpochA specific moment in time used as a reference point for orbital elements.
Focus (pl. foci)One of two special points inside an ellipse. The Sun sits at one focus of each planet's orbit.
Gravitational constant (G)The constant in Newton's gravity law, approximately 6.674 × 10−11 N·m²/kg².
Hohmann transferAn efficient orbital maneuver using two engine burns. See Spacecraft Navigation.
InclinationThe angle between an orbit's plane and a reference plane (e.g., the ecliptic).
Kepler's LawsThree laws of planetary motion. See Overview.
Orbital period (T)The time for one complete orbit.
PerturbationA small deviation from a Keplerian orbit caused by external forces. See Perturbations.
Semi-major axis (a)Half the longest diameter of an ellipse; the "average orbital radius."
Semi-minor axis (b)Half the shortest diameter of an ellipse.
Synodic periodThe time between successive alignments of a planet and the Sun as seen from Earth. See Mars Mission Planning.

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