Semi-major axis
Definition: Half the longest diameter of an ellipse; for an orbit it sets the orbit's characteristic size and energy.
Why it matters and connects: Kepler's third law relates semi-major axis to period, making it measurable through repeated positions or timing.
Boundary or common confusion: It is not the instantaneous star–planet distance except for a circular orbit.
\(P^2=a^3\)
Orbital period
Definition: The time required for a body to complete one orbit relative to a specified reference direction.
Why it matters and connects: Period ratios reveal resonances, and period combined with semi-major axis tests the central mass through Keplerian dynamics.
Boundary or common confusion: Sidereal and synodic periods differ; the relevant definition must match the observation.
\(P^2=\frac{4\pi^2}{GM}a^3\)
Mean-motion resonance
Definition: A configuration in which two orbital periods are close to a ratio of small integers, causing gravitational kicks to repeat at preferred phases.
Why it matters and connects: Repeated geometry can protect or destabilize orbits, structure rings and asteroid populations, and maintain moon eccentricities.
Boundary or common confusion: A near-integer period ratio alone does not prove resonant locking; the resonant angle must librate rather than circulate.
\(P_2/P_1\approx p/q\)
Perturbation
Definition: A deviation from ideal two-body motion caused by additional masses, nonspherical gravity, drag, radiation, or relativity.
Why it matters and connects: Small accumulated perturbations reveal unseen masses, shape orbital architecture, and must be modeled for spacecraft navigation.
Boundary or common confusion: A perturbation is not necessarily negligible; weak forces acting repeatedly can dominate long-term evolution.
Tidal force
Definition: The differential gravitational acceleration across an extended body.
Why it matters and connects: Tides distort worlds, exchange spin and orbital angular momentum, and can dissipate orbital energy as interior heat.
Boundary or common confusion: Tidal force is a gradient in gravity, not simply strong gravity; dissipation depends on material response and orbital state.
\(\Delta g\propto GM R/r^3\)
Hill sphere
Definition: The region around an orbiting body where its gravity can dominate satellite motion against the tidal influence of the central object.
Why it matters and connects: It provides a first estimate of where moons or rings can remain bound and how planet mass and orbital distance affect satellite systems.
Boundary or common confusion: Stable satellite orbits occupy only part of the Hill sphere and are altered by eccentricity, inclination, and other perturbers.
\(r_H\approx a(m/3M)^{1/3}\)