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SIM-01 · ORBITAL MECHANICS · KEPLERIAN · EQUATORIAL PLANE

Two-Body Orbit Sketch

The conic solved from four Keplerian elements, with Earth at the focus. Start with eccentricity — the view rescales itself so the whole orbit stays in frame.

Model & Assumptions

CONIC FROM ORBITAL ELEMENTSEQ. 1
r(ν) = a(1 − e²) / (1 + e cos ν)
T = 2π √(a³ / μ)
a is the semi-major axis, e the eccentricity, ω the argument of periapsis (rotating the conic in plane), and ν the true anomaly locating the spacecraft on it. μ = 398 600.4418 km³/s².
  • Two-body gravity only — no J2, drag, or third-body perturbations.
  • Planar motion: inclination and RAAN are not drawn, so the conic is shown in its own plane.
  • Geometry is exact for the elements shown; the marker is placed by true anomaly, not propagated in time.
  • Periapsis below the surface is flagged rather than clipped — the conic is still drawn.
SOLVER SOURCEscipk/scipk.github.ioVIEW REPOSITORY →