🛰️ SATELLITE TOOLKIT (STK) — ORBITAL MECHANICS COURSE
AGI Systems Tool Kit (STK) scenario files for 16 orbital mechanics lessons. Download a lesson's ZIP, unzip it, then open the .sc or .wsp file in STK. Requires ANSYS STK (free academic license available).
L01SIZE
Orbital size and the semi-major axis — the fundamental parameter that defines how large an orbit is and sets the orbital period via Kepler's Third Law.
Eccentricity and orbital shape — from circular LEO to highly elliptical transfer orbits; how the shape of the ellipse affects ground track and coverage.
Inclination angle — how the orbital plane tilts relative to the equator, determining which latitudes are accessible and how the ground track sweeps the globe.
Right Ascension of the Ascending Node — the angle that rotates the orbital plane around Earth's polar axis, placing ground tracks at the desired longitudes.
Argument of perigee — locates the low point of the orbit within the orbital plane; critical for HEO missions that need apogee dwell over specific regions.
True anomaly — the satellite's current angular position in its orbit, tying real-time position to the Keplerian elements and enabling access window prediction.
Low Earth Orbit (160–2,000 km) — rapid passes, short contact windows, and global coverage with large constellations; the home of ISS, Starlink, and most imaging satellites.
Medium Earth Orbit (2,000–35,786 km) — the realm of GPS, Galileo, and GLONASS; longer orbital periods and wider footprints than LEO but below the GEO belt.
Highly Elliptical Orbit — the Molniya and Tundra families that park apogee over high latitudes for hours, providing persistent coverage where GEO satellites can't reach.
Sun-synchronous orbit — a near-polar orbit where RAAN precesses to match Earth's solar year, keeping the same local solar time for consistent lighting in imagery.
Rocket launch mechanics — modeling ascent trajectories, parking orbits, and insertion burns in STK to simulate how payloads reach their target orbital slots.