Orbital Mechanics (Astrodynamics)

Keplerian Two-Body Problem (The Baseline Model)

The two-body model treats a spacecraft as a point mass under a central gravitational field. It is the foundation for orbit geometry, orbital periods, and energy relationships. In simple terms: it describes the “ideal orbit” before reality adds complexity.

  • Conics: circular/elliptic (bound), parabolic/hyperbolic (escape and flyby).
  • Energy: specific orbital energy determines orbit size.
  • Mean motion: links semi-major axis to orbital period.

Orbital Elements (A Compact Orbit Description)

Orbits are commonly parameterized by a small set of elements (size, shape, orientation, and location). In simple terms: orbital elements are a “coordinate system” for orbits.

  • Semi-major axis (a) and eccentricity (e): size and shape.
  • Inclination (i), RAAN (Ω), argument of periapsis (ω): orientation.
  • True/mean anomaly: where the spacecraft is along the orbit.

Perturbations (Where Reality Deviates)

Real trajectories are influenced by non-ideal forces. For LEO satellites, drag and Earth’s oblateness (J2) often dominate. In simple terms: perturbations slowly “push” the orbit away from the ideal shape.

  • Atmospheric drag: decays semi-major axis; depends on density and solar activity.
  • J2 effects: nodal regression and periapsis precession.
  • Third-body gravity: Sun/Moon effects, critical for cislunar missions.
  • Solar radiation pressure: meaningful for high area-to-mass spacecraft.

Maneuvering (Trajectory Control)

Maneuvers change orbital energy and geometry. Basic building blocks include plane changes, Hohmann transfers, and phasing maneuvers. In simple terms: a small velocity change (Δv) can reshape the entire orbit.

  • Impulsive vs. low-thrust: short burns vs. long-duration thrusting with optimization.
  • Δv budget: a key driver of propulsion sizing and mission feasibility.
  • Trajectory optimization: compute-efficient planning for complex missions.

Modern Focus (What Is Getting Important Now)

  • Cislunar logistics: transfers, staging, and sustained operations around the Moon.
  • Debris management: conjunction screening and maneuver planning at scale.
  • Active removal: rendezvous + capture + deorbit; example: ELSA-M concept for end-of-life services.

Resources

  • MIT OCW — astrodynamics course material.
  • CelesTrak — orbit data and references.